HomeEssential information & links to all sections of the website. |
Program OverviewProgram summary.Gives the big picture. |
Scientific ProgramAll activities scheduled at the meeting. |
ShowcaseExhibitors’ recent innovations & industry advancements. |
Speaker(s): Masahiro (Masa) WATANABE, Professor, Atmosphere and Ocean Research Institute (AORI) Deputy Director, UTokyo Center for Climate Solutions (UTCCS) The University of Tokyo
Value of Climate Models in Attributing and Projecting Large-Scale Climate ChangesSpeaker(s): Min-Seop AHN, Assistant Research Scientist Global Modeling and Assimilation Office (GMAO), NASA Goddard Space Flight Center (GSFC) Earth System Science Interdisciplinary Center (ESSIC), University of Maryland
Madden-Julian Oscillation: Physical Mechanism and Model SimulationSpeaker(s): Forrest HOFFMAN, Oak Ridge National Laboratory
Systematic Assessment of Terrestrial and Marine Biogeochemistry in Earth System ModelsSpeaker(s): Satish C.B. MYNENI, Princeton University
Rises in Sea Levels and Changes in the Coastal Biogeochemical ProcessesSpeaker(s): Axel TIMMERMANN, Director and Professor IBS Center for Climate Physics (ICCP), Pusan National University
Past Climate Impacts on Human EvolutionSpeaker(s): William McKINNON, Professor Department of Earth, Environmental, and Planetary Sciences, and McDonnell Center for the Space Sciences Washington University in St. Louis
Exploration of Kuiper Belt in the 21st Century, What Have We Learned and What is to Come?Speaker(s): Eiichi NAKAKITA, Director and Professor, Disaster Prevention Research Institute Deputy Executive Director, Kyoto University
Early Detection of Baby-Rain-Cell Aloft in a Severe Storm and Risk Projection for Urban Flash Flood -Advanced Utilization of Weather Radar-Speaker(s): Soohyun YANG, Assistant Professor Department of Civil and Environmental Engineering Seoul National University
The Role of River Networks in the Renaissance Era of HydrologySpeaker(s): Shunichi KOSHIMURA, Deputy Director, Professor, International Research Institute of Disaster Science, Tohoku University Co-founder & CTO, RTi-cast, Inc.
Catastrophic Tsunami Disaster – Its Impact, Disaster Response, and MitigationSpeaker(s): Daran ZHENG, Nanjing Institute of Geology and Palaeontology (NIGPAS) Chinese Academy of Sciences
The Spatiotemporal Evolution of The Early Cretaceous Jehol Biota in East AsiaSpeaker(s): Philippe LOGNONNÉ, Professor in Geophysics, University Paris Cité Planetary Seismologist, Institut de physique du globe de Paris
Planetary Seismology on Mars, The Moon and BeyondSpeaker(s): Honglei LIN, Associate Research Professor Institute of Geology and Geophysics, Chinese Academy of Sciences
From Apollo to Chang’e-5, What Have We Learned About the Water on The Moon?Speaker(s): Jongchul CHAE, Professor in Astronomy Program Department of Physics and Astronomy Seoul National University
Toward Understanding the Habitability of an Exoplanet Orbiting a Magnetically-active Star from Our Current Understanding of the Sun-Earth Connection in the HeliosphereSpeaker(s): Shan WANG, Assistant Professor Peking University
An Introduction of Magnetic Reconnection: Particle Dynamics and WavesSpeaker(s): Jing ZHANG, Advisor to the President Faculty of Science University of Toyama
Understanding the Water and Nutrient Transport Between Land and Ocean: Toward the Healthy, Productive, and Sustainable Asian Marginal SeasSpeaker(s): Changming DONG, Dean, School of Marine Sciences, Nanjing University of Information Science and Technology
AI Applications in OceanographySpeaker(s): J. Bruce H. SHYU, Professor Department of Geosciences National Taiwan University
Upper-Plate Structures Along Major Convergent Plate Boundaries: Structural Characteristics and Earthquake and Tsunami HazardsSpeaker(s): Shengji WEI, Principal Investigator, Earth Observatory of Singapore (EOS) Associate Professor & Associate Chair, Asian School of the Environment (ASE) Nanyang Technological University
Recent Earthquake Rupture Imaging and New Insights to Fundamental Earthquake PhysicsSpeaker(s): Jian LIN, Director and Professor Advanced Institute for Ocean Research, Southern University of Science and Technology (SUSTech)
Critical Roles of International Geoscience Cooperation in Addressing Pressing Global IssuesSpeaker(s): Chih-Pei CHANG, Distinguished Chair Professor, National Taiwan University Distinguished Professor Emeritus, Naval Postgraduate School
Maritime Continent Monsoon: Topographic Effects and Mesoscale – Large Scale Interactions| Convener: |
Eunsang Cho, Texas State University Hyunglok Kim, Gwangju Institute of Science and Technology |
| Speakers: |
Ana P. Barros, University of Illinois at Urbana-Champaign
John Bolten, Hydrological Sciences Laboratory, NASA Goddard Space Flight Center Venkataraman Lakshmi, University of Virginia Zong-Liang Yang, Department of Earth and Planetary Sciences, University of Texas |
| Session Description: | Remote sensing and modeling have transformed hydrologic science and applications. Spaceborne missions are dedicated to interlinked global hydrologic processes. Furthermore, computational techniques are accelerating analyses of these data and integrating them into the modeling. However, there are existing gaps and challenges the hydrologic community faces such as data uncertainties, limited model physics, and inequitable data availability across the world. How will the hydrologic community use these resources to better understand the world's water resources and to overcome related challenges facing society, particularly in Asia and Oceania. In this invited talk session, we will discuss the benefits, challenges, and opportunities of remote sensing for advancing hydrologic research, integrating multidisciplinary and multisensor data, and employing data assimilation and AI/machine learning. |
| Convener: | Beth Dingley, European Space Agency |
| Speakers: |
Tomiki Miyakawa, The University of Tokyo
Douglas Rao, North Carolina State University |
| Session Description: |
The World Climate Research Programme’s (WCRP) Coupled Model Intercomparison Project (CMIP) has coordinated international climate model experimentation, to develop a better understanding of past, present, and future climate change. Over four decades, CMIP has grown in scope and complexity, targeting climate science addressing the WCRP objectives and serving IPCC Assessments. CMIP6, the latest phase, yielded more than 25 PB of data, with contributions from 131 models, from 48 institutions, representing 26 countries. Work has commenced on future CMIP7 planning. The project aims to meet the growing community needs, enabling climate science and providing actionable climate information to aid policymakers. To facilitate next steps, the two panels that oversee the project, the CMIP and Working Group on Coupled Modelling (WGCM) Infrastructure (WIP) Panels have established seven Task Teams to guide CMIP7 scope and design and facilitate coordinated infrastructure development. These aim to increase CMIP’s scientific and social relevance, widen participation, improve data accessibility, and reduce the carbon footprint. We invite our growing community to attend. We will describe ongoing planning, highlight engagement, and feedback opportunities, and invite attendee feedback and participation. The town hall will be presented by members of the CMIP Panel, Fresh Eyes on CMIP group, and CMIP7 Task Teams. |
| Convener: | Beth Dingley, European Space Agency |
| Speakers: |
Douglas Rao, North Carolina State University Froila Palmeiro, Centro Euro-Mediterraneo sui Cambiamenti Climatici Evgenia Galytska, Bremen University Alistair Duffey, University College London Nebiyu Tekesa, Arba Minch University Gen Tolhurst, The Bureau of Meteorology Beth Dingley, European Space Agency |
| Associated Sections: | AS, HS, IG, OS (Not Limited To) |
| Description: |
The Coupled Model Intercomparison Project (CMIP) is an international climate modelling project, designed to better understand past, present, and future changes in the climate. More than 50 modelling centres around the world participated in CMIP6, which has already generated in excess of 14 PB of unique data. From its inception, there has been a focused effort to make the model intercomparison data available to scientists beyond the climate modelling community. With more data access platforms and analysis tools being created every year to support the use of CMIP data, it can be difficult to know where to begin. Primarily led by members of the new Early Career Scientists group, Fresh Eyes on CMIP, this workshop will provide an overview of ways to access CMIP data and present some useful analysis tools and methods to help with using it. The key topics across the session will cover:
|
| Convener: | Weile WANG, NASA Ames Research Center |
| Instructors: |
Weile WANG, NASA Ames Research Center Hugo Kyo LEE, NASA Jet Propulsion Laboratory Koji DAIRAKU, University of Tsukuba Dong-Hyun CHA, Ulsan National Institute of Science and Technology Tsengdar LEE, NASA Headquarters |
| Associated Sections: | AS, HS, IG, OS (Not Limited To) |
| Description: |
The goals of this workshop are:
|
In the era of the escalating climate crisis, the significance of climate technology to mitigate and adapt to these changes is on the rise. There is a growing need for the research and development of various technologies particularly those grounded in the expertise of Geoscience, and the widespread adoption of climate tech based on these innovations. In this session, we will firstly introduce the overall concept and current status of climate technology, followed by a leading climate tech company to share their insights into the commercialization process of the technologies and discuss the future of the climate tech industry. Lastly, we intend to explore avenues for collaboration by discussing the vision and activities of the Chung Mong-Gu Foundation, which fosters and supports the climate tech industry.
| Convener: | Lili Lei, Nanjing University |
| Instructors: |
Jeffrey Anderson, U.S. Geological Survey Soyoung Ha, National Center for Atmospheric Research |
| Associated Sections: | AS, HS, OS (Not Limited To) |
| Description: | This workshop is designed to be a short course that provides a practical introduction to ensemble filters from theories to tools along with realistic applications. There will be two main lectures, one is for “Introduction to Ensemble Data Assimilation” and the other is for “Introduction to the Data Assimilation Research Testbed (DART) and its Applications for the Model for Prediction Across Scales (MPAS)”. Basic ensemble filter algorithms will be covered along with an overview of extensions required for successful application in large earth system models. Various flavors of ensemble filters can be tested through the Data Assimilation Research Testbed (DART), a community software facility for ensemble filter data assimilation. DART can produce high-quality weather predictions but can also be used to build a comprehensive forecast system for any prediction model and observations. DART has been applied to NWP at scales ranging from sub-kilometer to global, but also to space weather, oceans, sea ice, terrestrial systems, hydrologic models, and many other earth system applications. This workshop is open for all participants to AOGS who have interests. Attendees will leave with a solid foundation that will allow them to explore using DART for existing models and observations, especially the Model for Prediction Across Scales (MPAS) for global and regional applications. They will also have a basic understanding of what would be required to develop DART assimilation capabilities for new models or observations. |
Disasters occur or are mitigated based on the relative magnitude between the ‘hazard’ factor to drive them and the ‘societal capacity’ factors to withstand them. Non-stationarity in climate, which began to be detected in the late 20th century, have now become widespread to the point that they are noticeable by the general public. In other words, climate change is increasingly recognized as a major driver of extraordinary disasters worldwide, and it has become the focus of numerous studies in almost every country. However, there is relatively less public interest in the societal capacity required to cope with disasters. Vulnerability, especially concerning ‘aging’ social infrastructure, is undoubtedly crucial especially in developed nations with a long history of urban development. In summary, we are confronting to a combined difficulty with two major challenges, the ‘changing climate’ and the ‘aging infrastructure’. Taking South Korea as an example, the first multipurpose dam, Soyanggang Dam, celebrated its 50th anniversary in 2023, and from now on, a multitude of social infrastructure will age beyond 50 years in the coming years. This session is designed to re-evaluate the issue of aging social infrastructures in the context of climate change and to discuss forward-looking scientific and technological alternatives and policy directions to address it.
Speaker(s): Prof Sang-Mook LEE ,
Marine Geoscientist
Seoul National University
Abstract
Scientific developments are considered the primary source of the economic prosperity of a country. This faith in science appears stronger among economists and policymakers than those involved in day-to-day activities. However, science policy is often confused with a policy for science. The former is dictated by national interest and ideology, including long-term plans for the country. Because it is so crucial, whether to let scientists formulate the science policy of a nation is a long-standing issue in many countries. Policymakers and politicians generally provide the overall picture with some help from scientists. A common approach adopted by developing countries is the so-called ‘mid-level entry strategy.’ The idea is to dispense basic science to developed countries and focus on those areas that may bring immense profits. And when the time comes, and technology matures, bet heavily on those specific areas and jump ahead of the flock to reap the benefit. However, many consider DARPA (Defense Advanced Research Projects Agency) the most successful research and development (R&D) institution in the US. It is said that the accomplishment of the agency was possible because they started with basic science and moved up to applied and practical research. Doing so dominated the entire value chain, and the know-how was then disseminated to the public. Such observation leads one to conclude that, contrary to the myth of mid-level entry strategy, the real big reward for R&D of a country comes from starting at the fundamental level. On the other hand, because scientific and technological development is not straightforward, some examples may point to the contrary. detected polar stratospheric jets associated with polar fronts. Other heating mechanisms proposed in the literature, such as Joule heating, polar haze heated by sunlight, etc., seem only the secondary mechanisms that follow atmospheric ionization caused by the energetic particle bombardment.
Session Chair(s): Ramesh KRIPALANI, Retired Senior Scientist, Indian Institute of Tropical Meteorology
AS04-A025
| Invited
Multidecadal Variability of Northern Hemisphere Summer Monsoon Forced by the SST Inter-hemispheric Dipole
Jianping LI1#+, Jiaqing XUE2, Bingchao WANG2,3, Yongkui YU2, Cheng SUN4, Jiangyu MAO5
1Ocean University of China, 2Nanjing University of Information Science & Technology, 3Guiyang Meteorological Bureau, 4Beijing Normal University, 5Chinese Academy of Sciences
The sea surface temperature inter-hemispheric dipole (SSTID) is an important variability mode of global SST anomalies, characterized by an anti-phase variation of SST between the two hemispheres. In this study, the decadal variability of the Northern Hemisphere summer monsoon (NHSM) is found to be strongly regulated by the SSTID, with positive (negative) phases of the SSTID corresponding to the strengthening (weakening) of NHSM. Both observation and SST-forced atmospheric model simulations suggest that the SSTID related thermal forcing modulates the NHSM by causing planetary-scale atmospheric circulation adjustments. Positive SSTID events lead to coherent increase (decrease) of surface air temperature over the entire Northern (Southern) Hemisphere, increasing the inter-hemispheric thermal contrast (ITC). As sea level pressure changes are just opposite to air temperature, the increase of ITC enhances the inter-hemispheric pressure gradient (Southern Hemisphere minus Northern Hemisphere), leading to the strengthening of summer monsoonal circulation and the increase of monsoon rainfall in the Northern Hemisphere.
AS04-A023
| Invited
Moist Baroclinic Instability of the East Asian Summer Monsoon
Tim LI1#+, Guang YANG2
1University of Hawaiʻi at Mānoa, 2North Carolina State University
A unique feature of the East Asian summer monsoon is dominated eastward-propagating synoptic-scale disturbances along a subtropical Meiyu front. The synoptic disturbances are strongly coupled with moisture and precipitation, and cannot be explained by traditional dry baroclinic instability theory. In this study, a new theoretical framework is developed, and it extends a traditional 2-level baroclinic model by considering a moisture tendency equation and feedbacks among perturbation moisture, precipitation and circulation. An eigenvalue analysis shows that the most unstable mode has a preferred zonal wavelength of 3400 km, an eastward phase speed of 10 m/s and a westward tilted vertical structure, all of which are in good agreement with observations. Both horizontal and vertical advection processes contribute to low-level moistening. Sensitivity tests show that the instability and the scale selection arise primarily from the moistening and condensational heating processes, while the modest background vertical shear provides an additional energy source for the perturbation growth. The new moist baroclinic instability theory explains well the observed characteristics of the development of synoptic-scale disturbances along the subtropical Meiyu front.
AS04-A005
| Invited
Dynamical Processes of ENSO’s Impact on Southeast Asian Summer Monsoon and Their Future Changes
Song YANG1#+, Shuheng LIN1, Buwen DONG2
1Sun Yat-sen University, 2University of Reading
The dynamical response of Southeast Asian summer monsoon (SEASM) to ENSO shows a large spread among CMIP6 models, and only some models can capture the observed features of ENSO’s impact on the monsoon. The problem of the bad-performance models is that the ENSO-related warm SST anomalies extend too far westward in the western equatorial Pacific (WEP) and are overly persistent, caused by a weak negative shortwave radiation feedback due to a low sensitivity of precipitation to local SST changes related to the cold bias in climatological SST. On the other hand, from the mature winter to the decaying summer of El Niño, the El Niño-related anomalous eastward current does not reverse to westward current because of the weak El Niño discharge process, attributed to the weak westerly wind anomalies associated with El Niño. The prolonged anomalous eastward current thus also contributes to the slow decay of WEP SST anomalies via inducing excessively persistent warm zonal advection in the WEP. For a warmer climate, CMIP6 models projects an enhanced response of the SEASM to ENSO, attributed to weakened warm SST anomalies in WEP during El Niño decaying summer. The El Niño related WEP SST anomalies decay rapidly and eventually dissipate from El Niño mature winter to the following summer, intensifying the anomalous anticyclonic circulation over the western North Pacific by enhancing the zonal gradient of SST anomalies between the tropical Indian Ocean and the WEP. The fast decay of WEP SST anomalies is mainly determined by increased latent heat flux from oceans to the atmosphere due to strengthened surface wind, caused by the eastward shifts of ENSO-induced anomalous Walker circulation and associated precipitation anomalies that are resulted from the El Niño-like change in background SST in the equatorial Pacific under global warming.
AS04-A066
Asian-Australian Summer Monsoons Linkage to ENSO Strengthened by Global Warming
Chenxi XU1#+, S. Y. Simon WANG2, Krishna BORHARA2, Brendan M. BUCKLEY3, Ning TAN1, Yaru ZHAO1, Wenling AN1, Masaki SANO4, Takeshi NAKATSUKA4, Zhengtang GUO1
1Chinese Academy of Sciences, 2Utah State University, 3Columbia University, 4Nagoya University
The El Niño-Southern Oscillation (ENSO) used to affect the Asian summer monsoon (ASM) and Australian summer monsoon (AusSM) precipitation in different ways but global warming may have changed it. This study built robust annual ASM (AusSM) precipitation reconstructions during 1588–2013 (1588–1999) to examine the ENSO-monsoon relationship and how it has changed. During the period of 1588–1850 when natural climate variability was dominant, the ENSO-monsoon and inter-monsoon relationship was weak and non-stationary. Since 1850, however, both the inter-monsoon and ENSO-monsoon relationships saw an enhancement and this trend has been persistent to the present day, suggesting the influence of anthropogenic climate warming. Further analysis of climate model projections found that global warming can strengthen the ENSO-monsoon association that, subsequently, acts to synchronize the ASM and AusSM variations.
AS04-A035
Robust Changes in Global Subtropical Circulation Under Greenhouse Warming
Shijie ZHOU#+, Ping HUANG
Chinese Academy of Sciences
The lower tropospheric subtropical circulation (SC) is characterized by monsoons and subtropical highs, playing an important role in global teleconnections and climate variability. The SC changes in a warmer climate are influenced by complex and region-specific mechanisms, resulting in uneven projections worldwide. Here, we present a method to quantify the overall intensity change in global SC, revealing a robust weakening across CMIP6 models. The weakening is primarily caused by global-mean surface warming, and partly counteracted by the direct CO2 effect. The direct CO2 effect is apparent in the transient response but is eventually dominated by the surface warming effect in a slow response. The distinct response timescales to global-mean warming and direct CO2 radiative forcing can well explain the time-varying SC changes in other CO2 emission scenarios. The declined SC implies a contracted monsoon range and drying at its boundary with arid regions under CO2-induced global warming.
AS04-A006
| Invited
Constraining the Global Mean Surface Temperature During 1850-1880 with New Statistical Physical Model
Qingxiang LI#+
Sun Yat-sen University
As IPCC ARs stated, global warming is estimated based on the global average temperature of pre-industrialization (represented by the average throughout 1850 to 1900 with relatively sparse observations). Given the impossibility of massive increasing observation data in the early stages, accurately constraining this baseline has become an unresolved issue. Based on a data-driven research paradigm, we developed a new statistical physical model to quantify the contribution of external forcings to global warming as a “deterministic trend” of the surface temperature series (instead of as non-stationary processes that yield a stochastic trend) and by which constrained the reconstruction of the early time series (1850-1880). The results suggest that the latest AR6 still slightly underestimates the rate of global warming since pre-industrialization, as the existing dataset slightly overestimates surface temperature anomalies over this baseline period. Our study provides a new perspective on the attribution and historical reconstruction of global warming since industrialization. These insights should also help humanity develop future climate change adaptation and mitigation strategies.
AS04-A071
PDO and AMO Modulation of the ENSO–Asian Summer Monsoon Teleconnection During the Last Millennium
Na WANG1#+, Sylvia DEE1, Jun HU2, Nathan STEIGER3, Kaustubh THIRUMALAI4
1Rice University, 2Xiamen University, 3Hebrew University of Jerusalem, 4The University of Arizona
Observations show that the teleconnection between the El Niño-Southern Oscillation (ENSO) and the Asian summer monsoon (ASM) is non-stationary. However, the underlying mechanisms are poorly understood due to the inadequate availability of reliable, long-term observations. This study uses two state-of-the-art data assimilation-based reconstructions of last millennium climate to examine changes in the ENSO–ASM teleconnection; we investigate how modes of (multi-)decadal climate variability (namely, the Pacific Decadal Oscillation, PDO, and the Atlantic Multidecadal Oscillation, AMO) modulate the ENSO–ASM relationship. Our analyses reveal that the PDO exerts a more pronounced impact on the ASM variability than the AMO. By comparing different linear regression models, we find that including the PDO in addition to ENSO cycles can improve the prediction of the ASM, especially for the Indian summer monsoon. In particular, the dry (wet) anomalies caused by El Niño (La Niña) in India will be enhanced during the positive (negative) PDO phases due to a compounding effect. However, composite differences in the ENSO–ASM relationship between positive and negative phases of the PDO and AMO are not statistically significant. A significant influence of the PDO/AMO on the ENSO–ASM relationship occurred only over a limited period within the last millennium. By leveraging the long-term paleoclimate reconstructions, our findings underscore the non-stationary nature of the PDO and AMO in modulating the ENSO–ASM relationship.
AS04-A058
Active and Inactive Lightning Frequency Cases During the Quasi-stationary Band-shaped Precipitation Systems in 2023
Hisayuki KUBOTA1#+, Yukihiro TAKAHASHI1, Mitsuteru SATO1, Yoshihisa YAMANOUCHI2, Akiyoshi FUKAYA2
1Hokkaido University, 2IHI Corporation
Recently heavy rainfall events are increasing in Japan. Especially during the Baiu-Meiyu rainfall season, heavy rainfall associated with quasi-stationary band-shaped precipitation systems frequently occurred. It was found that lightning frequencies were active during the heavy rainfall observed in July 2017. On the other hand, lightning frequencies were inactive during the heavy rainfall observed in the following year in July 2018. It was analyzed that convective systems were different between the two cases and that leads the difference of lightning activities. In this study 25 lightning and weather observation systems were deployed over the Southeast Asia, western north Pacific islands and Japan to monitor the lightning activities over these regions. During July 10, 2023, heavy rainfall was observed over northern Kyushu Island in Japan and rainfall amount reached 266 mm within 12 hours. Lightning was very active during the heavy rainfall. Another heavy rainfall was observed over Shikoku Island in Japan during August 9 to 10, 2023 and rainfall amount reached 638 mm within 24 hours. On the other hand, lightning activities were very weak during this case. We analyzed the difference of environmental conditions between the two cases. During the heavy rainfall in northern Kyushu case, west-southwesterly low-level wind provided moisture into the convective clouds. The origin of the moisture can be traced back to China continent. Rich amount of aerosol may lead to create more graupel in the clouds for favorable conditions for lightnings. However, heavy rainfall in Shikoku Island case, south-southeasterly low-level wind was dominant which was blown from the open ocean over the Pacific Ocean. Poor amount of aerosol moisture may suppress creating graupel in the clouds for lightning. It is similar to our previous study that we observed less lightning activity in the tropical cyclone generated far from southeast Asian islands.
AS04-A002
Atmospheric Rivers Over East Asia During Early Boreal Summer: Role of Indo-western Pacific Ocean Capacitor
Zesheng CHEN1+, Yan DU1#, Renguang WU2, Zhiping WEN3
1Chinese Academy of Sciences, 2Zhejiang University, 3Fudan University
Atmospheric Rivers (ARs), corridors of intensive water vapor transport, have received much attention recently due to their potential large economic and societal impacts. However, a comprehensive understanding of the interannual variability of ARs over East Asia is still lacking. This study examines the frequency of AR occurrence over East Asia based on the EAR5 reanalysis. It is shown that the frequency of AR occurrence over East Asia displays obvious seasonality, with its peak in early boreal summer. ARs contribute to up to 50% of total precipitation and largely modulate the interannual variability of precipitation in East Asia during early boreal summer. The interannual variability of ARs over East Asia during early boreal summer is largely controlled by the Indo-western Pacific Ocean Capacitor (IPOC) effect, which is mainly triggered by El Niño-Southern Oscillation and sometimes by Indian Ocean dipole. During early boreal summer, a higher frequency of AR occurrence over East Asia is associated with anomalous anticyclonic circulation (AAC) over the Indo-western Pacific region. The AAC, the atmospheric signal of the IPOC mode, indicates an enhanced East Asian summer monsoon and a northwestward shift of the western North Pacific subtropical high, favoring the AR occurrence over East Asia. This study illustrates that a strong positive Indian Ocean dipole event could impact AR activity over East Asia in the following summer by triggering the IPOC effect. The IPOC-related signals 2-4 months ahead could be useful to predict the AR occurrence over East Asia during early boreal summer.
Session Chair(s): Defeng ZHAO, Fudan University, Weigang WANG, Institute of Chemistry Chinese Academy of Science, Zhe WANG, The Hong Kong University of Science and Technology, Cheng WU, Gothenburg University
AS58-A006
Important Roles of Oxygenated Volatile Organic Compounds in Photochemical Pollution in Hong Kong
Zhe WANG#+
The Hong Kong University of Science and Technology
Oxygenated volatile organic compounds (OVOCs) are crucial reactive pollutants with profound implications for air quality and human health. They play critical roles in tropospheric photochemistry and oxidation capacity, significantly influencing radical cycling and O3 formation. Despite their increasing recognition, the lack of precise quantification hampers a full understanding. We present an integrated study of OVOCs employing both real-time online measurement and the cartridge-based analytical method in the coastal atmosphere of Hong Kong. Using PTR-ToF-MS, we measured 83 VOC species, where OVOCs constituted the majority (77.4%) of concentrations, contributing significantly (>50%) to photochemical OH reactivity and ozone formation potential (OFP). The newly developed analytical method based on UHPLC-MS/MS identified and quantified 47 carbonyl compounds, which play a substantial role in peroxyl radical and ozone formation. Furthermore, previously unmeasured long-chain carbonyls (C≥5) and di-carbonyls, absent in conventional methods, displayed noteworthy abundance and photochemical reactivity, enhancing the O3 formation rate by up to 30%. This comprehensive study underscores the importance of OVOCs, especially carbonyl compounds, in photochemical pollution, providing insights for effective photochemical pollution control. The developed methodologies enrich our understanding of OVOC chemical composition and reactivity, augmenting our grasp of their significance in atmospheric chemistry and air quality.
AS58-A007
Characteristics and Origins of C1–C5 Alkyl Nitrates Observed at a Coastal Site in Hong Kong
Hao SUN#+, Dasa GU
The Hong Kong University of Science and Technology
Alkyl nitrates (RONO2) constitute a vital subclass of total reactive nitrogen (NOy) within the Earth's atmosphere. These compounds play a pivotal role in atmospheric chemistry, exerting a substantial influence on air quality. The concentration of alkyl nitrates exhibits considerable variability across diverse regions of human habitation. Characterizing the variations in alkyl nitrate concentrations poses a significant challenge, essential for evaluating the intensity of photochemical reactions and discerning contributions from various sources. Hereby, we present the alkyl nitrate measurement results via canister sample collection and GC-MSD/ECD analysis at a coastal site in Hong Kong during 2021. An analysis of the source apportionment of eight C1-C5 alkyl nitrate species, employing anthropogenic and marine tracers, indicates that the predominant contributors to alkyl nitrates in Hong Kong are associated with secondary formation. Moreover, heightened contributions from biomass combustion were observed during the autumn and winter seasons. Notably, marine emissions exert a significant influence on methyl nitrate levels, particularly in the summer. Our study underscores the noteworthy impact of inland biomass burning on photochemical pollutants in Hong Kong. Consequently, recognizing the regional interdependence, cross-regional cooperation in governance within the Greater Bay Area is imperative for a more comprehensive management strategy addressing secondary photochemical pollution.
AS58-A014
Molecular Chemical Composition and Sources of Organic Aerosol in Shanghai Based on Online Analysis
Shuhui XUE+, Defeng ZHAO#, Hao LUO, Zhuosi WANG, Hongru SHEN, Ying ZHANG, Lin WANG, Shanshan WANG, Jianmin CHEN, Chengyu NIE, Zhen SONG
Fudan University
Organic aerosols (OA) account for a large portion of atmospheric aerosols, which have played a significant role in climate change and human health. The typical sources of POA (Primary OA) like biomass burning, cooking and transportation had been obtained by different measurement techniques. The specific sources of SOA (Secondary OA) are still unclear due to limited highly sensitive and quickly responsive measurement techniques, which have been proven challenging. Source apportionment is key to understand the formation and air pollution control for policy makers. However, the detailed sources of OA in megacities are currently unclear due to lack of information of chemical composition of OA at molecular level. Particularly, specific precursors and formation processes of SOA in megacities remain largely unclear. The newly developed high-resolution online measurement technology like extractive electrospray ionization time-of-flight mass spectrometer (EESI-TOF-MS) can provide specific information of OA at molecular level. In this study, we measured chemical composition of OA at molecular level using EESI-TOF-MS at Shanghai in February to March, 2022 and investigated the sources of OA. More than 1000 organic species were detected. Twelve sources (factors) are determined on mass spectra by bin-PMF (Positive Matrix Factorization), of which seven factors are identified as POA and five factors as SOA. POA sources are identified its source based characteristic tracers and time series. SOA sources are identified by linking to their precursors and processes based detailed mass spectra, their time series, and concomitant measurement of physiochemical parameters and gas-phase species. We found that both POA and SOA contribute significantly to OA in winter at urban Shanghai. Online molecular composition in this study reveals under-appreciated sources and processes of OA in megacities. These information enables better understanding of OA sources and more effective air pollution control strategy.
AS58-A022
| Invited
Direct Determination, Characteristics, and Origins of Fine Particulate Amines at a Coastal Mountain Site in Northern China
Xinfeng WANG#+, Mingxuan LIU, Zhiyi LIU, Yueru JIANG, Min LI, Yujiao ZHU, Likun XUE, Wenxing WANG
Shandong University
Amines are important nitrogenous compounds in the atmosphere, they affect new particle formation, aerosol properties, climate change and human health. Due to the relatively high volatility, strong polarity, and low ambient concentrations, they are subjected to great difficulty in the accurate determination. In this study, a derivatization- free determination method based on HPLC-MS was developed to determine the amines in fine particle samples collected at coastal Mt. Lao in the spring of 2021. The samples were pre-treated with a non-derivatization method and separated with a hydrophilic interaction column. 16 amines were identified and quantified with the limits of detection from 0.59 to 75.46 ng mL−1 and the recovery rates ranging from 59% to 92%. The average concentration of amines at the sampling site was around 60 ng m−3. Dimethylamine was the most abundant specie with mean fraction of 27% among the quantified amines, followed by diethylamine and ethanolamine. Meanwhile, amines exhibited higher concentrations during the daytime than nighttime at the mountain site. Most amines primarily came from terrestrial activities, while TMA was mainly from marine sources. Seven source factors were identified by PMF model, including agricultural emissions, industrial production, biomass burning, coal combustion, marine emissions, traffic emissions and crustal dusts. Notably, high contributions from agricultural source and biomass burning were observed at this coastal mountain site.
AS58-A021
Identification of Simple and Complex Nitro-aromatic Compounds Derived from Lignin Pyrolysis in PM2.5 in Urban Guangzhou Using UPLC-Orbitrap MS
Yuhuang CHENG#+, Jian Zhen YU
The Hong Kong University of Science and Technology
Lignin is a polyphenolic polymer commonly found in the supportive tissue of plants. When biomass burns, lignin can release various phenolic compounds into the atmosphere. These lignin-derived phenols can be easily nitrated due to the strong electron-donating effect of the hydroxyl group and methoxy group on their benzene ring. The resulting nitrated products are nitro-aromatic compounds (NACs), which are important components of brown carbon. While simple NACs have been identified, including 4-nitrophenol (4NP), 4-nitrocatechol (4NC), 2-methyl-4-nitrophenol (2M4NP), 3-methyl-4-nitrophenol (3M4NP), and 5-nitrosalicylic acid (5NSA), lignin-derived NACs with more and larger substituent groups on the benzene ring have received little attention. In this study, we applied a high-resolution UPLC-Orbitrap mass spectrometer (MS) system to analyze NACs in 58 ambient PM2.5 samples collected at an urban site in Guangzhou in 2013. The outstanding resolution of Orbitrap MS enabled us to identify NACs with 30 different molecular weights and more than 300 individual NACs, taking isomers into consideration. Among the simple NACs with authentic standards or quantification surrogates, the four most abundant ones were 5NSA, 4NC, 3NSA, and 4NP, with average concentrations ranging from 4.4 to 14.2 ng m-3. In addition, we classified a group of complex lignin-derived NACs, which included hydroxypropyl-dinitrophenol, dimethoxy-nitrophenol, hydroxyethyl-dinitrophenol, hydroxyethyl-nitrophenol, ethyl-nitrocatechol, and nitrovanillic acid. These compounds contain multiple substituent groups (e.g. methoxy group, hydroxypropyl group, and hydroxyethyl group) originating from lignin. We observed a strong correlation (R2 ranges from 0.50 to 0.98) between most of these complex NACs and the simple NACs throughout the entire sampling year, indicating the simple NACs likely originated from the burning of lignin. Furthermore, we detected other untargeted NACs, such as trinitrophenol and nitrobenzenetriol, in our samples.
AS58-A019
Global Model Underestimation of Ozone Production Tied to Unknown Sources of Reactive Nitrogen and Reactive Carbon in the Tibetan Plateau
Jianshu WANG1+, Chunxiang YE1#, Haoqi WANG2, Shaojie SONG2
1Peking University, 2Nankai University
Tropospheric ozone (O3) plays a crucial role in air quality, climate change, and human health. The large span of tropospheric O3 photochemistry across various global chemical transport models hinders our ability to evaluate tropospheric O3 distribution and its environmental impacts. An in-depth understanding of O3 photochemistry relies on observational constraints on the O3 chemical budget, especially in pristine environments or free troposphere. Here we present a detailed O3 chemical budget observation at a remote site over the Tibetan Plateau. Surprisingly high production rate of peroxy radicals was observed, which was mainly attributed to oxidation reactions of oxygenated volatile organic compounds (OVOCs). Radical chain propagation rates were promoted by elevated nitrogen oxides (NOx) and further facilitated O3 production. Neither OVOCs nor NOx could be explained by their local chemical production, suggesting missing sources of them. A global chemical transport model, GEOS-Chem, underestimated both OVOCs and NOx and hence underestimated the O3 production rate by 60%. The global model also underestimated photolysis frequencies and water vapor and therefore underestimated the O3 destruction rate by 20%. Our findings indicate a need for additional observations on the fate of reactive carbon and reactive nitrogen, to improve the model's ability to predict tropospheric O3.
AS58-A009
Photocatalytic Oxidation of Nitrogen Dioxide on Titanium Dioxide : Evidence to a Novel Heterogeneous Source for Dinitrogen Pentoxide
Yuan LIU1+, Biwu CHU2#
1University of Chinese Academy of Sciences, 2Research Center for Eco-Environmental Sciences, Chinese Academy of Sciences
N2O5 serves as a pivotal intermediate in the atmospheric nitrogen cycle. Utilizing a flow tube reactor, we have unveiled a previously undocumented source of N2O5 during the photocatalytic oxidation of NO2 on the TiO2 surface. The release rate of N2O5 from TiO2 was found to be contingent on initial NO2 concentration, relative humidity, O2/N2 ratio, and irradiation intensity. Both experimental evidence and quantum chemical calculations concur that NO2 can react with surface hydroxyl groups and electron holes generated on TiO2, subsequently combining with another NO2 molecule to form N2O5. This N2O5 physiosorbs on TiO2, exhibiting a low adsorption energy of -0.13 eV. Box model simulations suggest that this newfound source of N2O5 emitted from TiO2 could elevate daytime N2O5 concentrations by up to 20% in urban areas where abundant TiO2-containing materials and high NOx concentrations are co-present. Our research not only presents a novel chemical mechanism for N2O5 formation but also holds significant implications for air quality in urban settings.
AS58-A005
Nitrogen Shares in Future Global Air Pollution and the Scope of Feasible Interventions
Yixin GUO1#+, Lin ZHANG2, Wilfried WINIWARTER3, Jinfeng CHANG4
1The Hong Kong University of Science and Technology, 2Peking University, 3International Institute for Applied Systems Analysis, 4Zhejiang University
Reactive nitrogen emissions from energy and food production (Nr; nitrogen oxides, NOx, and ammonia, NH3) contribute substantially to global PM2.5 and O3 air pollution, damaging human, ecosystem and vegetation health. To illustrate the role of Nr controls in near-term air quality management, we quantify how the shares of Nr in global PM2.5 pollution evolve from the present to the year 2050. We use the GEOS-Chem atmospheric chemistry transport model and future emission scenarios under various climate-socioeconomic pathways. We find that the phase-out of anthropogenic NH3 emissions remains necessary for achieving the WHO target for PM2.5 and that this is more effective than phasing out NOx. For more moderate Nr control levels of 25% and 50%, NH3 controls become less effective than NOx controls in many locations. This is because climate mitigation policies enable clean energy transitions thus reductions of NOx and SO2 emissions, the chemical regime shifts towards a NH3-saturated regime. The later NH3 is addressed, the more ambitious reduction level is required for effectiveness to emerge. To illustrate the technological and policy feasibility of Nr controls, we assess achievable Nr (NH3 and NOx) emission mitigation potentials and evaluate consequent reductions in global air pollution, and human and ecosystem health impacts. We construct an integrated modeling framework that combines future N intervention scenarios, integrated assessment models and the GEOS-Chem model. We find that, through improving crop nitrogen use efficiency and exploiting abatement technologies for industrial, transport and power sectors, global NH3 and NOx emissions can be reduced by 40% and 52%, respectively, of 2015 levels by 2050, generating a wide array of consequent benefits for air, yields, ecosystems and human health. Without nitrogen interventions, environmental/health objectives examined will deteriorate by 2050 compared to 2015. Nr interventions remain a key strategy for improving global environmental health that should not be overlooked.
Session Chair(s): Venugopal VURUPUTUR, Indian Institute of Science, Bangalore, Sridhara NAYAK, Japan Meteorological Corporation
AS11-A005
Exploring the Asian Australian Monsoon Rainfall Extremes via Moisture Transport Patterns with Insights from Explainable Machine Learning
Jia Xin GUO+, Wei-Ting CHEN#
National Taiwan University
The Asian Australian Monsoon (AAM) region, characterized by abundant precipitation and hydrological extremes, necessitates in-depth explorations of crucial synoptic environmental factors influencing extreme rainfall events. Building on previous research highlighting moisture content and low-level dynamic flow, we developed a data-driven framework using Variational Autoencoder (VAE), an unsupervised and explainable machine learning model, to dissect prominent moisture transport patterns and explore their linkage to extreme precipitation emergences. The vertically-integrated water vapor transport (IVT) from ECMWF Reanalysis v5 (ERA5) is adopted as the primary indicator of moisture environment. Through VAE, daily fields of IVT spanning from 2001 to 2019 are encoded into two-dimensional vectors on a continuous latent space and classified into different regimes. Each latent dimension captures the seasonal progression and synoptic to sub-seasonal variability, respectively, of the large-scale moisture transport pattern. The heat maps of extreme rainfall occurrence derived from Integrated Multi-satellitE Retrievals of Global Precipitation Measurement (IMERG) 0.5-hourly data reveal distinctive patterns across various moisture transport regimes. This hints a potential correspondence between distinct extreme rainfall distributions and specific moisture transport configurations in the AAM region. Detailed investigations into each moisture transport regime, employing composite analyses of synoptic fields and tropical variability indices, elucidate the modulation of moisture transport and the possible mechanisms in influencing extreme rainfall emergence. The current VAE model serves as a foundational step in interpreting the primary factors driving variations in moisture transport patterns and offers the opportunity for estimating future changes in extreme convective systems' hotspots using the “storyline approach”, given the higher confidence in synoptic flow modeling in General Circulation Models. Results and discussions based on CMIP6 models will also be presented to provide valuable insights to the broader scientific discourse on extreme rainfall events in the AAM region.
AS11-A008
Glo3DHydroClimEventSet(v1.0): A Global‐scale Event Set of Hydroclimatic Extremes Detected with the 3D DBSCAN‐based Workflow (1951–2022)
Zhenchen LIU#+, Wen ZHOU
Fudan University
The emergency of global‐scale hydroclimatic extremes (i.e., meteorological droughts, extreme precipitations, heat waves and cold surges) and associated compound events has recently drawn much attention. A global‐scale unified and comprehensive event set with accurate information on spatiotemporal evolutions is necessary for better mechanism understanding and reliable predictions in sequential studies. Accordingly, this manuscript describes the first‐generation global event‐based database of hydroclimatic extremes produced with the newly proposed 3D (longitude–latitude–time) DBSCAN‐based workflow of event detection. The short name of this database is Glo3DHydroClimEventSet(v1.0) , which is obtained from the FigsharePlus webpage ( https://doi.org/10.25452/figshare.plus.23564517 ). The 1951–2022 ERA5‐based multiscale and multi‐threshold daily running datasets of precipitation and near‐surface air temperature are calculated and employed as the input data. A comprehensive event set of hydroclimate extremes is the output of the 3D DBSCAN‐based workflow. From perspectives of spatiotemporal evolutions, this event‐based database is also measured and attached with metric information. For case‐based validation, some recently reported hydroclimatic extremes (e.g., the 2020 summertime flood‐inducing Yangtze River extreme precipitation event) are employed and accurately detected in the Glo3DHydroClimEventSet(v1.0) database. Meanwhile, global‐scale spatiotemporal distributions are preliminarily analysed. For example, global‐scale event counts of extreme heatwaves displayed an increasing tendency since 2005, with a rapid increase after 2010. To sum up, this Glo3DHydroClimEventSet(v1.0) database may facilitate new scientific achievements concerning event‐based hydroclimatic extremes, especially in communities of atmosphere, hydrology, natural hazards and associated socioeconomics. The DOI-based paper linkage is https://doi.org/10.1002/joc.8289.
AS11-A009
Typical Synoptic Patterns Responsible for Summer Regional Hourly Extreme Precipitation Events Over the Middle and Lower Yangtze River Basin, China
Jingwen ZENG#+, Anning HUANG, Danqing HUANG
Nanjing University
Based on the hourly rainfall gauge data and ERA5 reanalysis for the period 1980–2020, typical synoptic patterns responsible for summer regional hourly extreme precipitation events (RHEPE) over the middle and lower Yangtze River basin have been objectively identified using a circulation clustering method. It is found that the Meiyu front with different locations and intensities imbedded in the East Asian summer monsoon, and landfalling typhoons are the leading contributors. As the dominant synoptic pattern, the Meiyu front pattern is associated with ∼92% of the total RHEPE occurrence and can be categorized into a southerly strong-Meiyu type and a northerly weak-Meiyu type. The RHEPE occurrence shows a predominant morning peak associated with the southerly strong-Meiyu type and a secondary late afternoon peak related to the northerly weak-Meiyu type, in which the Meiyu front is pushed northward by the strengthened western North Pacific subtropical high accompanied by accelerated low-level southwesterly flow
AS11-A021
Interannual Variability and Drivers of Extreme Precipitation Over the Yangtze River Basin
Yucong LIN#+
Ca' Foscari University of Venice
Utilizing ERA5 reanalysis data, we carried out a series of analyses to investigate the spatiotemporal characteristics of extreme precipitation over the Yangtze River Basin (YRB) and the major drivers influencing the interannual variability of summer extreme precipitation during 1950-2021. The results indicate that anomalous anticyclones/cyclones over the western North Pacific (WNP) and El Niño/La Niña like sea surface temperature (SST) patterns in the preceding winter are associated with increased/decreased summer extreme precipitation over the YRB. Furthermore, the El Niño and Southern Oscillation (ENSO), the Indian Ocean Dipole (IOD), and the anomalous Indian Ocean Basin Warming (IOBW), which occur in boreal autumn/winter, are shown to have delayed effects on the YRB's extreme precipitation in the subsequent summer. Both ENSO and IOD have the capability to generate anomalous anticyclones/cyclones over the Western North Pacific (WNPAC/WNPC), which in turn can enhance or diminish water vapor transport, leading to an increase or decrease in summer extreme precipitation over the YRB. However, the impact of negative ENSO-IOD forcings is generally weaker than that of positive forcings. The persistence of the abnormal tropospheric WNPAC/WNPC is primarily driven by local thermodynamic forcing and feedback from the IOBW. It is noteworthy that only strong ENSO events can trigger the anomalous IOBW, resulting in more pronounced responses in summer extremes. Notably, the negative ENSO-IOD phases yield non-linear outcomes, thus offering less robustness for the predictability of summer extremes over the YRB. This study provides valuable insights into the interannual variability of summer extreme precipitation in the YRB, highlighting the key predictors and physical mechanisms responsible for these variations. Keywords: Yangtze River Basin; extreme precipitation; ENSO; IOD; Indian Ocean Basin Warming; WNPAC.
AS11-A025
The Spatiotemporal Distribution and Evolution of Short-term Intense Precipitation in China
Shoujuan SHU#+
Zhejiang University
Based on meteorological observation from stations over the past thirteen years, China was divided into seven regions: Central China, East China, Southwest China, Southeast China, North China, Northeast China, and Western China. A study was conducted on the spatial and temporal distribution characteristics and their evolution of short-duration intense precipitation in China. The results found that the occurrence of short-duration intense precipitation in China is seasonal, mainly occurring in spring and summer, and primarily concentrated from May to September. Among them, the southern regions have the highest frequency in summer, followed by East China and Central China, then the eastern coastal areas of North China and the southern coastal areas of Northeast China, with the Western region having a very low frequency. In terms of daily occurrence of short-duration intense precipitation, it occurs mostly in the early morning in the Southwest and Central China; while in the downstream Southeast and East China, it mainly occurs in the afternoon, with the highest frequency in coastal areas. In the plains of Northeast China, it also occurs mainly in the afternoon, but with a frequency far less than that of the Southeast and Southwest regions. In the plains of North China, there is no significant difference in the daily time period of occurrence, with occurrences in the early morning, afternoon, and evening. In terms of average intensity of short-duration intense precipitation, the Southeast and North China regions are more intense than other regions. The early morning short-duration intense precipitation in the Southwest and Central China has an eastward transmission characteristic, showing that after the convective cell is generated, it moves eastward, and intensifies in the afternoon upon reaching East and South China. Over the thirteen years, the occurrence of short-duration intense precipitation has shown different evolutionary characteristics in different regions.
AS11-A030
Impact of Aeolus Wind Data Assimilation on a Heavy Rain Forecast
Izumi OKABE#+, Kozo OKAMOTO
Japan Meteorological Agency
As the first satellite mission to give wind profile information on a global scale, Aeolus was launched in 2018, and its horizontal line of sight wind data has been available from the European Space Agency (ESA) Earth Online Portal since May 2020. The significant positive impact of this data on numerical weather prediction has been reported in many researches (Rennie et al., 2021; George et al., 2021). We presented about the assimilation impact on JMA’s global data assimilation and forecasting system and the impact on typhoon forecasting in AOGS 2021 and 2022 (Okabe and Okamoto 2024, accepted). We have started investigating the assimilation impact on heavy rain forecasts using both global and regional data assimilation systems. The configuration of the control experiments (CNTLs) in these assimilation experiments mirrored the operational global system as of December 2019 and the operational regional system as of April 2020 of the Japan Meteorological Agency. The test experiments (TESTs) were the same as CNTLs except the use of Aeolus data. The target event is the heavy rainfall incident that struck Kumamoto and Kagoshima prefectures on the southern Japanese island of Kyushu, on July 4th, during the heavy rain events of July 2020 in the middle of the Baiu season (the East Asian rainy season). As a result of flooding and landslides, more than seventy people were confirmed dead, and approximately 15,000 buildings were destroyed, damaged or flooded. In the TEST of the global experiments, the positional error in heavy rain forecasts has been slightly improved. The investigation into the assimilation impact in the regional experiments is ongoing. The detailed results will be shown in the presentation.
AS11-A043
Evaluation of WRF Land Surface Model Accuracy in Sub-seasonal to Seasonal Rainfall Prediction Skill Across Thailand
Kritanai TORSRI1#+, Chakrit CHOTAMONSAK2, Duangnapha LAPYAI2, Kevalin INLAUNG2, Punnathorn THANADOLMETHPHORN2, Rati SAWANGWATTANAPHAIBUN 1, Pattarapoom PEANGTA1, Apiwat FAIKRUA1, Jakrapop AKARANEE1
1Ministry of Higher Education, Science, Research and Innovation, 2Chiang Mai University
This study assesses the WRF model's accuracy in predicting sub-seasonal to seasonal rainfall in Thailand, specifically focusing on the performance using Noah and Noah-MP land surface models. The research aims to contribute insights into the WRF model's efficacy for sub-seasonal to seasonal rainfall prediction, improving understanding and reliability for the region. The analysis utilizes weekly summer rainfall data with a fine 5 km resolution nested domain driven by CFS Reanalysis data. The study centers on a selected 2021 summer monsoon event marked by a strong Madden-Julian Oscillation. Evaluation of model predictions for six sub-regions reveals increased rainfall in Weeks 2 and 9, generally aligning with observations. Discrepancies exist, particularly in the model's overestimation in the east and south but accurate predictions in the southwest. Probability Distribution Function plots highlight divergent rainfall patterns. Noah-MP outperforms Noah, suggesting its suitability for refining the model to enhance rainfall predictions in Thailand.
AS11-A035
Can a 12 KM Global Model Simulate the Observed Cloud Microphysical and Extreme Rainfall Relationship of Indian Summer Monsoon?
Tanmoy GOSWAMI#+, Parthasarathi MUKHOPADHYAY, R. Phani Murali KRISHNA
Indian Institute of Tropical Meteorology
The increase in the frequency of extreme precipitation in different parts of the world is well documented and a cause for concern in terms of global climate change. Although clouds are the only source of precipitation, there is a lack of knowledge about the type of clouds involved in extreme precipitation events. Observations by MODIS and IMD show that over the central Indian region (19oN-26oN, 75oE-85oE), about 60% of the extreme precipitation comes from deep convective clouds (DCC), which have a cloud top pressure (CTP) of less than 440 hPa and an optical cloud thickness (COT) of over 23. It was also observed that cloud water liquid (CWL) and COT show the highest correlation with extreme precipitation and also show the highest contrast between extreme and non-extreme precipitation events. Simulations (hindcast) of a global 12KM model are also analysed for extreme precipitation events. It is found that the model underestimates the threshold for extreme precipitation (99th percentile climatology) with increase of lead time. Simulations of the associated cloud optical parameters also deteriorate with increasing lead time. The model tends to overestimate the convection and cloud water liquid during an extreme precipitation event. The model also fails to capture the observed relationship between the frequency of extreme precipitation and the frequency of deep convective clouds and shows no correlation between them at all lead times.
Session Chair(s): Jooil KIM, Scripps Institution of Oceanography, UC San Diego
AS31-A018
Evaluating the Carbon Absorption Capacity of Urban Forests by GPP Quantification based on Multi-scale Observations
Jangho LEE#+, Sujong JEONG
Seoul National University
Vegetation in urban areas, referred to as ‘urban forests’, is recognized as a localized carbon sink for removing a considerable amount of atmospheric CO2 and the areas of them are changing as urbanization accelerates. Thus, quantifying the carbon uptake of vegetation in urban areas is necessary for improving GHG inventories in cities. Given that the carbon sequestration of urban forests is calculated based on coarse spatiotemporal resolution statistics, the carbon absorption capacity of urban forests is often inadequately quantified and easily overlooked. However, there are limited studies estimating GPP in urban forests due to substantial variation in environmental factors directly related to photosynthesis in cities and the difficulties of obtaining data that can isolate the influence of vegetation. Therefore, we deployed hyperspectral devices (FloX, JB Hyperspectral Devices) to observe Solar-induced chlorophyll fluorescence (SIF) and Eddy covariance system instruments to measure CO2 fluxes together in two urban forests (Changgyeongung and Namsan Park) in Seoul to explore the carbon uptake capacity of urban forests. We primarily analyzed seasonal trends in Net Ecosystem Exchange (NEE) using CO2 flux data to examine whether or not urban forests are carbon sinks. By comparing canopy-level SIF with satellites SIF on the same date, along with the CO2 flux, we found ground-observed SIF can represent the dynamic plant physiological responses. Subsequently, we attempted to quantify GPP at these multi-scale observation sites by partitioning NEE and Soil Canopy Observation of Photosynthesis and Energy fluxes (SCOPE) model simulation. This study holds significance in utilizing diverse scale observational data to help us understand the physiological function and responses of urban forests and improve GHG inventories within cities. Additionally, it introduces the first multi-scale observation site that simultaneously measures CO2 flux and SIF in the same urban forests, emphasizing the need for high spatiotemporal resolution data through the ground-based observation network.
AS31-A035
Practical Application of AICAN (Asian Initiative for Clean Air Networks) Against Episodes of Wildfires, Fireworks, and High PM
Chan Ryul PARK#+, Hong-Duck SOU, Daun RYU, Jinsuk JEONG
National Institute of Forest Science
Tree and forests can have a potential to abate the fine dust through the adsorption and deposition under the tree canopy against episodes of wildfire, fireworks and high PM in a city. During high PM episodes in Winter and Spring, most peoples do hesitate to take a field activity of walking, trekking, and climbing in hilly and mountainous landscapes dominated by 63.5% of forests in Korea. Thus, National Institute of Forest Science (NIFoS) has been established Asian Initial for Clean Air Networks (AiCAN) across the Korean Peninsula (44 locations, 132 points) to measure TSP, PM10, PM2.5, PM1.0 and meteorological factors (wind velocity, relative humidity, and temperature) with the equipment of GRIMM EDM 365 from 2019 to 2022. All observation data was monitored in ten minutes interval and the maintenance process of equipment was followed by the legislation of Korean Government. We analyzed the annual amount of PM reduction by forests comparing with the observation point between forests and urban by the analysis of AiCAN dataset. The PM reduction in the forest was the highest in spring and winter when high PM concentrations were observed, and the annual PM10 and PM2.5 were reduced by 32.9kg/ha and 22.7kg/ha in 2021, 26.4kg/ha and 19.3kg/ha in 2022, 29.2kg/ha and 18.9kg/ha in 2023. In consideration of theoretical value was estimated as 46kg/ha, the observation values were distributed at the range of theoretical values. This abatement could be attributed to the effects on absorption, adsorption, blocking, and deposition of fine dusts under tree canopy of forests. NIFoS will utilize this platform to understand the interaction between forests and aerosol not only for predictable and controlled Events of high PM episodes, yellow dusts, heat waves, and typhoon, also un-predictable and un-controlled events of wildfires and fireworks.
AS31-A026
Enhancing Methane Inventory Accuracy in Urban Waste Sector: A Case Study in Seoul
Donghee KIM#+, Sujong JEONG, Dong Yeong CHANG1,1
Seoul National University
Methane (CH4) is important greenhouse gas with a high Global Warming Potential (GWP) that significantly contributing to climate change. In urban, methane emissions are mainly come from the energy and waste sectors. This study aims to enhancing our understanding of methane emissions from the waste sector, especially solid waste disposal, as a major contributor to total urban methane emissions. Landfills, a key source in the waste sector, substantially contribute to methane emissions through the decomposition of organic waste. The emissions are influenced by weather conditions, but existing methane inventories inadequately consider this variability. In this study, we introduce an improved methane inventory methodology that includes meteorological conditions, offering a more comprehensive representation of methane emissions. In the context of Seoul, we present spatiotemporally high-resolution methane inventories derived from the waste sector. The results show a significant increase in methane emissions during the spring and summer seasons, emphasizing the seasonal variability associated with waste decomposition processes. This detailed understanding is crucial for effective urban methane management. The implementation of our methodology holds significance in improving the accuracy of methane emission estimates from the waste sector. By integrating weather conditions into the methane inventory, this study contributes to a more improved understanding of methane emissions in urban area. This enhanced methodology can support the development of more effective waste management policies and strategies to mitigate methane emissions, addressing climate change in urban environments.
AS31-A020
Significant Methane Emissions from Urban Manholes
Jaewon JOO+, Sujong JEONG#, Jaewon SHIN, Dong Yeong CHANG1,1
Seoul National University
Sewer networks are one of the major sources of greenhouse gas (GHG) emissions in urban areas. However, they are currently missing in South Korea's national GHG inventory. Here, we measured atmospheric methane emissions from urban sewer networks in old residential and commercial areas of Seoul (Gwanak district) using a GHG monitoring platform consisting of the electric vehicle and GHG monitoring instruments such as methane (CH4), and ethane (C2H6). The results of this research showed significant CH4 emissions of about 573 [395-831] CH4 t y-1 from sewers through the manholes and rain gutters. The CH4 emissions in the study area are primarily due to microbial activity within the sewer networks, as suggested by the majority of C2:C1 ratios being below 0.005. This is because more than 90% of the sewer network in Seoul is a gravity drain type of combined sewer network, resulting in the generation of CH4 emissions from the microbial activity. Thus, manholes and rain gutters, which are directly connected to the combined sewer networks are major sources of atmospheric methane emissions in Seoul. The results of this study suggest that proper treatment of sewer networks especially manholes and rain gutters are required to mitigate the one of the significant methane emissions in urban areas of South Korea. This work was supported by Korea Environmental Industry & Technology Institute (KEITI) through "Project for developing an observation-based GHG emissions geospatial information map", funded by Korea Ministry of Environment (MOE)(RS-2023-00232066).
AS31-A008
Eddy Covariance Measurements of Methane Flux in Urban Beijing
Yibo HUANGFU1#+, Bin YUAN1, Xianjun HE1, Ziyang LIU1, Thomas KARL2, Martin GRAUS2, Marcus STRIEDNIG2, Xiaodong CHEN3, Hongjuan LI3, Min SHAO1
1Jinan University, 2University of Innsbruck, 3Ausao Ecological Instrument Co., Ltd.
Methane was recognized as one of the most important greenhouse gases after carbon dioxide. Accurate estimation of methane emission is the key to establishing a reasonable and effective reduction target and strategy for achieving the goal of limiting global warming to 1.5 ℃ within reach. Using the eddy covariance technique, methane flux was measured at a meteorological tower in Beijing, China in the summertime to increase the understanding of methane emission in urban regions. The footprint climatology (90% contour lines) demonstrates that the measured flux can represent the summer emission characteristics of ~70 km2 of surrounding areas categorized as the typical urban landscape in the megacity of Beijing. The quality assurance and quality control results show more than 50% of the flux data can be labeled with high quality. Compared with the methane flux measured in other cities, the methane flux measured in Beijing, 152.6 ± 107.9 nmol/m2/s, was relatively large. There was no significant diurnal pattern and no clear correlation between methane flux and temperature/solar radiation can be found, which suggests that the biogenic source might not be the dominant source of methane within the footprint area. Constant background emission due to natural gas leakage was likely the main contributor.
AS31-A030
Carbontracker-CH4: NOAA’s Atmospheric Assimilation System for Estimating Methane Emissions Consistent with Measurements of Methane and Its Isotopes
Youmi OH1#, Lori BRUHWILER1, Xin LAN1, Sourish BASU2, Sylvia MICHEL3, John B. MILLER1+, Arlyn ANDREWS1
1NOAA Global Monitoring Laboratory, 2NASA Goddard Space Flight Center, 3University of Colorado Boulder
Atmospheric methane (CH4) is currently more than 160% above pre-industrial levels, and the 2020-2022 growth was the fastest since systematic measurements started in the 1980s. This rapid increase is a challenge for reaching the climate mitigation goals of the Global Methane Pledge from COP26, which requires steep cuts in CH4 emissions by 2030. Slowing or reversing the accelerating growth in atmospheric CH4 will require an improved understanding of the anthropogenic and natural CH4 budget, which is currently underconstrained. We have improved our understanding of the global CH4 budget via precise measurements of 13C:12C (δ13C-CH4), a tracer capable of separating fossil and microbial emissions. When atmospheric CH4 increased rapidly after 2006, δ13C-CH4 decreased after increasing for the last 200 years, indicating that the CH4 rise has been dominated by microbial sources such as wetlands and agriculture, not fossil fuels. To provide quantitative estimates of global CH4 emissions that are consistent with observed patterns of atmospheric CH4 and δ13C-CH4, we updated CarbonTracker-CH4 by jointly assimilating atmospheric measurements of CH4 and δ13C-CH4, optimizing source-specific fluxes at a grid-scale, and extending our estimation from 1997 to 2021.Our inversion shows that the global CH4 emission has increased more than 100 Tg yr-1 since 2000 and reached ~650 Tg yr-1 in 2021, and the large long-term increase was from Asia and North America regions. We find that the dual-tracer inversion of CH4 and δ13C-CH4 attributes the growth in atmospheric CH4 in 2020-2021 to a large increase in microbial sources and a slight decrease in fossil sources. The large increase in emissions was mostly from the tropical and Eurasian regions. In contrast, the inversion that uses CH4 data only does not match atmospheric δ13C-CH4 and simulates an increase in fossil sources in 2020-2021. All our results are publicly available at https://gml.noaa.gov/ccgg/carbontracker-ch4/.
AS31-A021
Characteristics and Origins of CH4, CO2 and CO Observed at a Coastal Site in Hong Kong
Wai Ming CHAN1+, Dasa GU1#, Ka Fung LEUNG1, Yuchen MAI1, Sin Ka MAK1, Hao SUN1, Xin LI1, Xiangyunong CAO1, Tsz Ching TSE1, Zhenxing LIANG1, Zijie XU1, Donald BLAKE2
1The Hong Kong University of Science and Technology, 2University of California, Irvine
The industrial revolution escalated greenhouse gas (GHG) emissions, driving climate change to a critical juncture that necessitates immediate action. Monitoring essential GHGs like CO2 and CH4 is imperative for comprehending their impact on the climate system. East Asia, with high energy consumption and robust industrial activity, is a significant GHG emitter, emphasizing the need for meticulous monitoring. While CO is not a direct GHG, it reacts with atmospheric OH radicals, affecting the lifetime of CH4 and influencing radiative forcing and the global climate. CO is an important trace gas of combustion processes and industrial activities, providing insights into the sources of CH4 and CO2. Thus, monitoring CH4, CO, and CO2 enhances our understanding of climate change and, to a lesser extent, improves air quality, yielding dual benefits. To investigate the characteristics of CH4, CO2, and CO, we established a sampling and instrumental analysis system at the Hong Kong University of Science and Technology. Observation results revealed pronounced seasonality, with higher concentrations in the cold season and lower concentrations in the warm season for all three gases. Non-parametric wind regression and the HYSPLIT back trajectory model indicated that continental air masses carried more concentrated gases, while oceanic air masses contributed to local air dilution. Fluctuations around the background level showed a strong correlation between CH4 and CO, while CO2 exhibited a lower correlation with the other two. This suggested distinct sources in Hong Kong compared to typical Chinese cities, where CO2 and CO exhibited a higher correlation usually. Further analysis utilizing the Potential Source Contribution Function (PSCF) identified Central and East China, as well as northern Guangdong, as major source regions for CH4 and CO, with Central China being the dominant source region for CO2. These findings provide valuable insights for developing effective carbon neutrality policies in Hong Kong and China.
AS31-A013
Comprehensive Monitoring of Urban Greenhouse Gases and Air Quality Using Observations from Ground to Space: The Seoul-Tokyo EM27/SUN Campaign
Hayoung PARK1#+, Sujong JEONG1, Jin-Soo PARK2, Matthias FREY3, Hiroshi TANIMOTO3, Isamu MORINO3, Hirofumi OHYAMA3, Astrid MUELLER3
1Seoul National University, 2National Institute of Environmental Research, 3National Institute for Environmental Studies
Seoul and Tokyo, as major global contributors to greenhouse gas emissions and air pollutants, are focal points for emission reduction initiatives with significant implications for global climate change mitigation. In the winter of February 2022 and 2023, Seoul National University Climate Lab and the National Institute for Environmental Studies (NIES) conducted an extensive observational campaign in both cities using portable ground-based FTIR spectrometers, EM27/SUN, offering a comprehensive analysis of column-averaged dry air mole fractions of CO2, CH4, and CO (XCO2, XCH4, XCO). In addition, we incorporated integrated observations of CO2, CH4, and CO concentrations using ground-aircraft-satellite measurements intensively carried out in Seoul to monitor greenhouse gases and air quality in a megacity. We analyze the spatial distributions and variations of greenhouse gases and air pollutants within the urban area of Seoul, as well as assess the emission characteristics using a combination of the Column-Stochastic Time-Inverted Lagrangian Transport model (X-STILT) and ratio analysis. This study presents results from the two-year campaign, offering a comparative analysis of greenhouse gas concentrations in Seoul, South Korea and Tokyo, Japan. Overall, this research aims to monitor the current atmospheric conditions in the two major cities, as well as to analyze the three-dimensional structure of greenhouse gases and air pollutants in Seoul.
Session Chair(s): Lakshmi Kumar T. V., Jawaharlal Nehru University
AS04-A063
| Invited
Causes of 2022 Pakistan Flooding and Its Linkage with China and Europe Heatwaves
Huang-Hsiung HSU1#+, Chi-Cherng HONG2, An-Yi HUANG 3, Wan-Ling TSENG4
1Academia Sinica, 2University of Taipei, 3Oregon State University, 4National Taiwan University
In boreal summer of 2022, Pakistan experienced extremely high rainfall, resulting in severe flooding and displacing over 30 million people. At the same time, heatwaves persisted over central China and Europe. The coexistence of these extreme events suggests a possible linkage. Our analysis indicated that the record rainfall was mainly induced by compounding factors. These included (1) La Niña-induced strong anomalous easterlies over the northern Indian subcontinent, (2) intense southerlies from the Arabian Sea with an upward trend in recent decades, (3) an interaction between extratropical and tropical systems, specifically the northerly flow downstream of the Europe blocking and the southerly monsoon flow from the Arabian Sea. Wave activity flux and regression analyses unveiled a distinct stationary Rossby wave-like pattern connecting the flooding in Pakistan and heatwaves in Europe and China. This pattern, an emerging teleconnection pattern in recent decade, exhibited substantial differences from the reported teleconnection patterns. We also noted the positive feedback of the excessive Pakistan rainfall could further enhance the largescale background flow and the heavy rainfall itself. The 2022 Pakistan flood event was an intensified manifestation of the 2010 Pakistan flood event, which was also caused by compounding factors, but occurred in a more pronounced upward trend in the both tropics and extratropics.
AS04-A026
Moisture Dynamic Processes Driving the Westward Propagation of Quasi-biweekly Oscillation in Asian Tropical Summer Monsoon Rainfall
Weizhen CHEN1+, Song YANG1, Wei WEI1#, Yuhao CAI1, Zeming WU2
1Sun Yat-sen University, 2Zhejiang University
The quasi-biweekly oscillation (QBWO) is an important component of tropical monsoon variations. The QBWO rainfall demonstrates a westward propagation chain from the western North Pacific to the Arabian Sea. Specifically, a delay of about 2 days is observed in the rainfall increase over the Bay of Bengal following an increase over the South China Sea. The mechanisms for the development of QBWO rainfall in the Asian tropical monsoon region is revealed by a moisture budget analysis. Positive specific humidity anomalies are primarily induced by the leading horizontal moisture advection at the lower level. The interaction between QBWO anticyclones circulation anomalies and mean moisture gradient facilitates the increase of moisture in the Asian tropical monsoon region, thereby instigating the westward extension of QBWO. Furthermore, the mean zonal cross-equatorial flow also contributes to the moisture transportation dynamics. The westward propagation chain revealed may benefit the subseasonal rainfall prediction in the Asian tropical monsoon region.
AS04-A068
Middle East Warming in Spring Enhances Summer Rainfall Over Pakistan
Lei ZHOU1#+, Baosheng LI2, Jianhuang QIN3, Tianjun ZHOU4, Dake CHEN5, Shugui HOU1, Raghu MURTUGUDDE6
1Shanghai Jiao Tong University, 2Sun Yat-Sen University, 3Hohai University, 4Chinese Academy of Sciences, 5Ministry of Natural Resources, 6University of Maryland
The South Asian summer monsoon is one of the most spectacular monsoon systems in the world. It affects the production and lives of billions of people. Climate change is reshaping the spatial distribution of summer monsoon rainfall. This study has found that rainfall over Pakistan and northwestern India during the summer monsoon has increased by 46% from 1979 to 2022 and is increasing at a rate of 0.4-0.6 mm/day per decade. The enhancement of summer rainfall on the edge of the South Asian monsoon is mainly caused by the rapid warming in spring over the Middle East. The Middle East is one of the most significant regions in terms of global warming, which is found to be 0.5 K per decade during spring. The spring Middle East warming can trigger a decrease in sea level pressure in the region and result in the enhancement of the cross-equatorial winds, which in turn leads to the emergence of low-level jet (LLJ) winds in spring. This process persists until the onset of the summer monsoon, when the LLJ is further strengthens and shifts northward. Since LLJ transport boatloads of moisture into the subcontinent, the northward shift of the LLJ results in the excess supply of moisture to Pakistan and northwestern India. This new research implies that arid and semi-arid countries and regions such as Pakistan and northwestern India, which are on the edge of the monsoon, are now exposed to frequent heavy rainfall events. This will lead to more disasters like the 2022 Pakistan Floods with unacceptably high loss of life and property.
AS04-A018
The Synergistic Effect of the Preceding Winter Mid-latitude North Atlantic and Summer Tropical Eastern Indian Ocean SST on Extreme Heat Events in Northern China
Hao WANG1+, Jianping LI1#, Fei ZHENG2
1Ocean University of China, 2Sun Yat-sen University
Summer extreme heat events happen frequently in northern China (NC) during recent decades, which have serious impacts on the society and ecosystem. The present study reveals that there is a synergistic effect of the preceding winter positive mid-latitude North Atlantic SST anomaly (pMNA SSTA) and summer negative tropical eastern Indian Ocean SST anomaly (nTEI SSTA) on strengthening the summer extreme heat events in NC. The extreme heat events are stronger and more frequent when the two factors cooccur, and the probability of a strengthened extreme heat events is higher, which indicates a synergistic effect of the two factors. The preceding winter pMNA SSTA and summer nTEI SSTA exert their synergistic effect through a series of atmospheric and snow cover bridges. The preceding winter pMNA SSTA could lead to an anomalous anticyclone over central Asia via the eastward propagating Rossby wave, which decreases snowfall and the subsequent snow cover there. The negative snow cover anomaly may persist into spring and induce a local anomalous anticyclone in summer via the snow-hydrological effect, which is accompanied by an atmospheric teleconnection featured with an anomalous cyclone over West Siberia and an anomalous anticyclone over NC. The summer nTEI SSTA can also induce the anomalous anticyclone there via the Rossby wave propagation. Thus, the two factors exhibit evident synergistic effect on the atmospheric circulation anomaly over NC. The anomalous anticyclone corresponds to the increased atmosphere thickness, which favors the increase of air temperature in NC and the strengthening of extreme heat events. Therefore, the preceding winter pMNA SSTA and summer nTEI SSTA have significant synergistic effect on strengthening the summer extreme heat events in NC.
AS04-A017
The Quadrupole Precipitation Pattern Over Eastern China and its Associated Atmospheric Circulations and Ocean Conditions
Yuting LIU+, Danqing HUANG#
Nanjing University
The purpose of this study is to understand the regime shifts of the East Asian summer monsoon precipitation in different warming periods. We revealed a new precipitation pattern over eastern China as a “+ - + -” precipitation pattern from south to north. The circumglobal teleconnection, the negative phase of the interdecadal Pacific oscillation, the warming over the high-latitude North Atlantic, and the warming over Northern Hemisphere can be used to explain the quadrupole precipitation pattern. These findings could highlight the role of jet streams linking the quadrupole pattern to the teleconnections, dominant decadal ocean variabilities and the warming over Northern Hemisphere.
AS04-A083
Intensification of the East Asian Summer Monsoon Lifecycle: Dynamics of Consecutive Compound Wet and Hot Extremes
Suyeon MOON1+, Hyungjun KIM2,1#
1The University of Tokyo, 2Korea Advanced Institute of Science and Technology
Serving as the lifeblood, summer monsoon precipitation fuels agriculture, industry, and daily life in East Asia (EA). Yet, its dark side emerges when severe events batter densely populated regions, causing havoc and disaster. In recent years, South Korea, China, and Japan have all faced the wrath of extreme precipitation events. We zoom into the role of stationary front-induced precipitation, a key character that shapes more than 40% of EA’s summer rainfall narrative. Sifting through observations from 1958 to 2015, we have found a 19.8% surge in the intensity of frontal rainfall. With the Large Ensemble simulations, we have untangled the role of anthropogenic greenhouse gas forcing impact, revealing it as the primary cause behind the amplified EA summer frontal rainfall. Behind this intensification, two culprits emerge: the amplified western North Pacific subtropical high (WNPSH) and increased water vapor convergence. In addition to the enhanced frontal rainfall, the hot extremes have become more severe in the subsequent season. The westward and northward expansion of WNPSH evokes the hot extremes over EA. Our findings suggest that human-induced global warming is radically reshaping the EA summer wet and hot extremes, by sharing a key regional climate mechanism. This transformation is likely to continue, potentially redefining the future of summer extremes in EA.
AS04-A089
Monsoon Onset Mechanism and Its Reproducibility in Global Climate Models
Yoshiyuki KAJIKAWA1#+, Tsuyoshi YAMAURA2
1Kobe University, 2RIKEN Advanced Institute for Computational Science
Monsoon onset signifies the commencement of the rainy season and the reversal of wind circulation over the Asian monsoon area. The factors of the monsoon onset include the thermal condition and arrival of disturbances (e.g. tropical cyclones, Intraseasonal variability). While the prediction of the monsoon onset timing remains a challenging issue, the Cloud system resolving global climate model (CRGCM), which has the advantage of reproducing the tropical disturbance, shows the potential to extend the predictability of the onset timing. Here, we analyze the historical experiment of the Global climate model (MIROC) and CRGCM (NICAM) with prescribed observed SST, especially focusing on the monsoon onset. The results show less reproducibility interannual variability. Of interest is the significant negative interannual correlation between seasonal mean Indian summer monsoon (ISM) strength and the ISM onset timing (summer monsoon tends to be stronger following the early onset) in the GCM and CRGCM while the observational data does not show such significant interannual relation. The ISM system in the model might be mainly driven by the thermal condition in longer persistency. We will discuss the effects of less intraseasonal activity in the model and advance the comprehensive understanding of the combinational effects of different time scale variations such as thermal conditions and disturbances.
AS04-A030
Weather Types and Rainfall Variability During Northeast Monsoon Over Malaysia Associated with ENSO
New XIA YAN#+, Liew JUNENG, Fredolin TANGANG
Universiti Kebangsaan Malaysia
Extreme precipitation often dominant around Malaysia during the Northeast Monsoon. However how the extreme precipitation is associated to different monsoonal synoptic circulation is not fully understood. Based on the weather types classification method, this study examines the dominant large-scale patterns related extreme precipitation in Malaysia during Northeast Monsoon season. Daily weather types (WTs) during Northeast Monsoon season (November to February) over Malaysia region (3°S-10°N, 100°–120°E) has been analyzed using 850hPa winds from the Fifth Generation of the European Centre for Medium-Range Weather Forecasts (ECMWF) Reanalysis Data (ERA5) from 1981-2020 by using k-means clustering. Ten WTs were obtained to analyzed in terms of circulation patterns, frequency of occurrence, typical progression and precipitation characteristics and relation to El-Nino Southern Oscillation (ENSO). The resulting WTs represent and include the main synoptic circulation patterns related to the Cold Surge and Borneo Vortex. Cold surge patterns are predominant in January and February while weakening cold surges show significantly reduced frequency during November and December. Three out of ten clusters show Borneo Vortex occurring in different locations over the South China Sea. Most of the WTs remain on the same type during transition and persistence not exceeding 6 days. Clusters that exhibit Borneo Vortex occurrence typically produce heavy rainfall near east coast of Peninsular Malaysia while weakening cold surge shows significant heavy rainfall near south of Borneo. Lastly, the extend to which the El-Nino-Southern Oscillation modulates the probability of occurrence of each of the ten WTs is then discussed.
AS04-A016
Exploring a New Aspect of Multi-phase Rotated Empirical Orthogonal Function for Capturing Spatiotemporal Variations in Temperature
Kamana MISHRA#+, Sarita AZAD
Indian Institute of Technology Mandi
The Northwest Himalayan (NWH) region has experienced substantial impacts from climate change, necessitating a thorough examination of its dynamic spatiotemporal patterns through suitable statistical methods. To capture systematic trends and elucidate localized characteristics, we employed Rotated Empirical Orthogonal Functions (REOFs) on mean temperature data spanning from 1981 to 2021. Utilizing REOF analysis, we subdivided the NWH region into snow and non-snow cover areas, enhancing the precision of data representation. Particularly in the western parts of Uttarakhand (U.K.) and Himachal Pradesh (H.P.), the second REOF mode of mean temperature exhibited noteworthy fluctuations, explaining 38.7% of the overall variance. However, the associated principal component (PC) failed to accurately depict the data patterns in these regions. In response, we introduced Multi-phase REOF analysis for the first time, aiming to identify PCs that faithfully represent the original data and offer insights into specific temporal variations. Additionally, we explored potential factors contributing to these variances in the specified NWH locations. The deduced physical properties and identified temperature zones from this analysis can enhance climate change modeling in the area.
Session Chair(s): Xiquan DONG, The University of Arizona, Chuanfeng ZHAO, Peking University
AS66-A015
Ice-over-water Multilayer Cloud Properties and Identification in an Artificial Neural Network Approach
Sunny SUN-MACK1,2#+, Patrick MINNIS2, William L. SMITH JR.2, Yan CHEN1, Gang HONG1,2
1Analytical Mechanics Associates, Inc, 2NASA Langley Research Center
Clouds are a crucial component of the atmospheric energy system, particularly the radiative balance within, above, and below the troposphere. The vertical distribution of cloud mass and phase determines layer heating rates, the loss of radiation to space, and the amount of radiative heating at the surface. Thus, it is important to know how clouds are distributed both vertically and horizontally at all times of day. Satellite remote sensing is the only approach available to monitor clouds day and night around the globe. In this paper several artificial neural network (ANN) algorithms, employing several Aqua MODIS infrared channels, profiles of relative humidity and temperature from GMAO numerical weather analyses, and the retrieved total cloud visible optical depth, are trained to detect multilayer ice-over-water cloud systems and to retrieve some of their properties as identified by a year of 2008 Aqua MODIS data matched with CloudSat and CALIPSO (CC) cloud profiles. The CC lidar and radar profiles provide the vertical structure that serves as output truth for the multilayer algorithm. The neural networks were trained using one year (2008) of cloud top height data from the CC dataset, with correlation around 0.94 (0.95) and MAE as low as 0.82 (0.81) km for nonpolar regions during the day (night). Applying the trained ANN to independent year 2009 MODIS data resulted in a combined ML and single layer hit rate of 86.4% (85.1%) for nonpolar regions during the day (night). Since the ANN is trained using near-nadir MODIS pixels, infrared radiance corrections were developed as a function of view zenith angle from MODIS and applied to off-nadir pixels when processing MODIS swath data. The multilayer amount derived with the ANN is relatively invariant with increasing view zenith angle compared to the multilayer amount without the corrections.
AS66-A005
Characteristics of Mesoscale Convective Systems Associated Warm Sector Rainfalls for the Hong Kong Region
Shiwei YU1+, Hui SU1#, P.W. CHAN2
1The Hong Kong University of Science and Technology, 2Hong Kong Observatory
Mesoscale convective systems (MCSs) are known to induce heavy rainfall and pose significant weather hazards in tropical and extratropical regions. As a subset of MCSs, warm sector rainfalls (WSRs) refer to heavy rainfalls within a weakly forced synoptic environment under the impact of monsoonal airflows. They are often formed in the southern coast of the East Asian monsoon region (e.g. southern China) during the pre-summer season (April-June). Despite extensive studies on the mechanisms of MCS rainfall and the considerable improvement in predictive skills, accurately forecasting MCS-associated WSRs remains challenging. Hong Kong, as a subtropical coastal city in southern China, frequently experiences MCS-associated WSR events. In order to gain a better understanding these events, we analyzed 214 MCSs and 9 WSRs that occurred in the Hong Kong region between April and June from 2005 to 2023. Firstly, we examined the water vapor conditions around Hong Kong using the global navigation satellite system (GNSS) technique. Our findings revealed that during WSRs, the water vapor hovered at a higher level of 62 mm for approximately 36 hours, in contrast to the gradually increasing pattern observed in the other MCSs. Additionally, we investigated three factors - moisture, lift, and instability – related to MCSs using the European Centre for Medium-Range Weather Forecasts reanalysis dataset (ERA5). Our analysis indicated that low moisture deficit lasted for 36/48 hours before the initial/maximum precipitation of WSRs. Furthermore, a stronger convergence in the low atmosphere was observed 36/48 hours before the initial/maximum precipitation of WSRs, compared to the 0/12-hour signal found in other MCSs. In terms of instability, we observed a rapid reduction preceding the maximum precipitation of the MCSs, while the decline shows a smoothing pattern with a small magnitude for the initial time reference. Interestingly, the instability did not display significant fluctuations during WRSs.
AS66-A001
Amplified Interhemispheric Rainfall Contrast in Boreal Summer Due to Reduction in Anthropogenic Emissions Under COVID-19 Green Economic-recovery Scenarios
Xiaochao YU1, Hua ZHANG1#+, Bing XIE1, Piers M. FORSTER2
1China Meteorological Administration, 2University of Leeds
Our study looks at the precipitation responses to two possible future emission-mitigation pathways, pushed by the continuing Coronavirus Disease 2019 pandemic (Covid-19) and achieving carbon neutrality in the mid-21st century. We find that simultaneous-reduction in well-mixed greenhouse gases (WMGHGs) and aerosol emissions results in enhanced interhemispheric precipitation contrast in 2040s by amplifying interhemispheric thermal contrast and strengthening meridional overturning circulation at tropics. Reduced aerosol emissions induce generally-increased precipitation in the Northern Hemisphere (NH) and an amplified intertropical rainfall contrast, while reduced WMGHG emissions dominates decrease in precipitation in the areas away from aerosol emission sources. Further, the above precipitation contrast will be enhanced under stronger emission-mitigation pathways, mainly attributed to larger precipitation increases in the NH caused by reduced aerosols. More aggressive WMGHG mitigation policies are required to offset the NH warming driven by aerosols, to avoid the risk of regional drying or wetting driven by the asymmetry in interhemispheric energy budgets.
AS66-A012
Urban Effect on Air Pollution and Precipitation
Zhining TAO1#+, Mian CHIN2
1Morgan State University, 2NASA Goddard Space Flight Center
More than 50% of the global population live in urban areas that contribute to 0.5% of the world’s total land. The resulting concentrated economic and social activities make urban a unique micro-environment that affects air quality and precipitation. Usually, it is more polluted in urban space than its surrounding areas with elevated aerosol levels. The microphysical and radiative effects of aerosols (AMR) would impact cloud and precipitation developments. The direction and magnitude of such urban effect on local precipitation and storms remains an open scientific question. In this study, a fully coupled regional chemistry transport model – the NASA Unified Weather Research & Forecasting (NU-WRF) model – has been applied to the Houston metropolitan area to untangle the complex interactions among urban landscape, aerosols, and precipitation. The simulation results have been evaluated against the measurements of local meteorology and air quality. A series of sensitivity experiments have been conducted to quantify the effect of urban land vs. anthropogenic aerosols on local precipitation onset and intensity. The results show that the urban effects greatly enhanced convection right before rainfall starts via AMR interactions. With the same storm system, aerosols can either suppress or intensify precipitation depending on the underlying land use.
AS66-A003
Effect of Vertical CCNC Explosion on Hail and the Uncertainty Evaluation Compared with Initial Meteorological Condition
Xiaofei LI#+
Northwest University
The uncertainty of the cloud condensation nuclei concentration (CCNC) effect on hail precipitation due to perturbed initial meteorological conditions (IC) has been evaluated using an ensemble data from an idealized hailstorm by the high-resolution Weather Research and Forecasting (WRF) simulation. Varied CCNC from clean to polluted condition in six concentrations with uneven intervals resulted in a curve pattern that increasing firstly and then decreasing with single peak for hail precipitation rate. Vertical sensitive simulations showed that CCN at 750-800 hpa plays a dominant role in the change of hail rate, while the total precipitation is dominated by 700-800 hpa height CCNC. However, we found some tiny perturbed ICs from ECMWF, including thermodynamic (TQ, potential temperature and mixed water vapor ratio) and kinematic condition (UV, U wind speed and V wind speed), can even change the curve style with multiple peaks, indicating a potential large uncertainty for CCNC effect on hail in an uncertain IC. Although the meteorological perturbations produce large uncertainties in both hail and total precipitation, varying CCNC by an order of magnitude causes even larger uncertainties than the meteorological perturbations. Changing CCNC modifies the predictability of hail precipitation, with higher predictability in moderately polluted environments compared with very clean and polluted environments. Perturbing the initial meteorological conditions does not qualitatively change how aerosols affect hail and total precipitation.
AS66-A023
Determination of Cirrus Occurrence and Distribution Characteristics Over the Tibetan Plateau Based on the Swop Campaign
Dan LI1+, Jiali LUO2#, Zhen YANG2
1Chinese Academy of Sciences, 2Lanzhou University
Balloon sounding with the Compact Optical Backscatter Aerosol Detector (COBALD) and Frost Point hygrometers (FPs) provides in situ data for a better understanding of the vertical distribution of cirrus clouds. In this study, eight summer balloon-borne measurements in Kunming (2012, 2014, 2015, and 2017) and Lhasa (2013, 2016, 2018, and 2020) over the Tibetan Plateau were used to show the distribution characteristics of cirrus clouds. Differences of cirrus occurrence were compared by different indices: the backscatter ratio (BSR) at a 455 nm/940 nm wavelength (BSR455 > 1.2/BSR940 > 2), the color index (CI > 7), and the relative humidity with respect to ice (RHice > 70%). Analysis of the profiles indicated that BSR455 > 1.2 was the optimal criterion to identify the cirrus layer and depict the distribution of the CI and RHice within cirrus clouds. The results showed that the median CI (RHice) within the cirrus clouds at both sites was mostly in the 18–20 (90%–110%) range at pressures below 120 hPa. Furthermore, the balloon-borne measurements combined with Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) measurements indicated a high frequency of cirrus occurrence near the tropopause in Kunming and Lhasa. The top height of cirrus occurrence at both sites was above the cold point tropopause and the lapse rate tropopause. Both Kunming and Lhasa had the highest frequency of thin cirrus clouds in the 0–0.4 km vertical cirrus thickness range.
AS66-A025
Analysis of Global Light Rain System from GPM/DPR Observation and Its Seasonal Variations
Seoeun CHOI1#+, Sang-Moo LEE1, Jihoon RYU2, Euijong KANG1
1Seoul National University, 2Korea Institute of Atmospheric Prediction Systems
Atmospheric cloud system and the associated precipitation is responsible for variations in how moisture is released and how heat is distributed in Earth's atmosphere. The global distributions of clouds significantly impact on local weather patterns as well as overall climate system. While light rain may not boast high intensity compared to heavy rain, it accounts for significant fraction of rain occurrence and light rain system has recognized as one of the most important atmospheric phenomena to understand global hydrological cycle. The launch of Global Precipitation Measurement (GPM) Dual-frequency Precipitation Radar (DPR) has enabled a nearly-global (65oS–65oN) detection of the horizontal and vertical structures of clouds, enabling to understand global precipitation distributions. This research aims to analyze drop size distribution (DSD) characteristics and cloud echo-top height (CETH) defined as the top height of DPR echo from the ground altitude to avoid land elevation interference of light rain using GPM/DPR measurement from 2019 to 2021. In this study, a Gaussian mixture model (GMM) clustering was employed to categorize the light rain system globally. The parameters utilized for the classification in this study are mass-weighted mean diameter (Dm), and normalized intercept parameter (log10Nw) at the clutter-free bottom level, and CETH from GPM/DPR-retrieved products. By using both of microphysical and macrophysical properties of clouds, global light rain was clustered as the following three types: (1) oceanic shallow, (2) oceanic moderate, and (3) continental types. Additionally, to classify prevailing types across different seasons, GMM clustering was conducted seasonally, following the same method. On a global scale, distinct rainfall characteristics are notably disparate between summer and winter, with uniquely classification into two types: oceanic and continental in winter. Henceforth, the DSD parameters will be examined and predominant regions will also be discussed for a comprehensive understanding of the variations in rainfall patterns across seasons.
AS66-A028
A Modeling Study of Aerosol Effect on a Summer Nocturnal Convective Precipitation Event in Beijing
Yue ZHOU1#+, Chuanfeng ZHAO2, Yue SUN1
1Beijing Normal University, 2Peking University
Using the Weather Research and Forecasting Model with Chemistry (WRF-Chem) model, this study investigates the potential contributions of aerosol direct effect (ADE) and aerosol indirect effect (AIE) on a nocturnal convective precipitation event occurred on 9-10 September 2019 in Beijing. It shows that the ADE and AIE both contribute to the spatial distribution of rainfall in urban areas. The ADE plays a more important role to the changes of heavy precipitation. The ADE causes a slight decrease in precipitation before 13:00 (UTC, hereafter) on 9 September (precipitation I), while increases precipitation during 13:00-21:00 (Precipitation II). The AIE has a weak effect on precipitation before 18:00 on 9 September, while decreases precipitation after 18:00. Further simulation analyses show that the ADE suppresses convection and precipitation by inducing greater surface shortwave radiative cooling and stability during Precipitation I, which reduces the convective energy (CAPE) losses and then increases the later CAPE. The ADE-induced CAPE increase makes the updraft stronger, increasing the cloud fraction and transporting more cloud water into the upper troposphere. This, in turn, causes greater latent heat release from freezing and then stronger convection, resulting in higher rain rate during Precipitation II. During 12:00-18:00, the AIE causes a decrease in CAPE, which weakens the updraft. The AIE decreases the snow mixing ratio above 700 hPa except at 15:00-16:00 on 9 September, which can decrease the release of latent heat from freezing, contributing to the decrease in precipitation after 18:00. Due to the greater stability before 10:00 and longer time required for the updraft to overcome this stability, the ADE necessitates 2-3 hours to adjust the simulated rainfall time series in the study area.
Session Chair(s): Kenneth JUCKS, NASA Headquarters, Ja-Ho KOO, Yonsei University
AS79-A002
| Invited
The Silk Road Teleconnection Along the Summer Subtropical Asian Jet: Dynamics and Changes Under Global Warming
Yu KOSAKA#+, Yuta UCHIDA
The University of Tokyo
The Silk Road teleconnection is a waveguide teleconnection along the summer subtropical Asian jet along the northern periphery of the Asian summer monsoon anticyclone, also known as the Tibetan/South Asian high. The teleconnection induces undulation of the monsoon anticyclone. It often causes extreme weather events in East Asia such as heat waves and heavy rains. Our analysis of the energetics of the interannual Silk Road teleconnections shows that the baroclinic energy conversion associated with meridional heat transport in the mid- to lower troposphere is key to its maintenance. In a large ensemble AGCM simulation dataset d4PDF and CMIP6 simulations, we find the teleconnection significantly weakens under global warming. This is because baroclinic energy conversion becomes less efficient under reduced linkage with the mid- to lower tropospheric circulation anomalies due to the uplift of the jet axis and enhanced tropospheric stratification. Besides, the southward shift of the Asian jet associated with global warming prevents wave packet injection from the North Atlantic subpolar jet.
AS79-A016
Intraseasonal Variability of the Asian Summer Monsoon Anticyclone
Joowan KIM#+, Hyeong-Gyu KIM, Dahuin CHONG
Kongju National University
The variability and related dynamical mechanisms of the Asian Summer Monsoon Anticyclone (ASMA) were examined on intraseasonal time scale. The intraseasonal behavior of the ASMA is largely related to the convective activity over Indian and East Asian regions reflecting its developing mechanisms. In addition, generation and propagation of Rossby waves over the Eurasian continent also significantly affect the behavior of the ASMA. Particularly, the Rossby wave patten frequently observed over the Eurasian jet (a.k.a. Silk Road Pattern, SRP) significantly influences the intraseasonal variability of the ASMA. The SRP's eastward propagation along the Eurasian jet and dynamical coupling with lower troposphere plays a crucial role in the dynamic variability within the monsoon anticyclone, leading to notable variations in surface weather and chemical transport in the upper troposphere and lower stratosphere across East Asia.
AS79-A009
| Invited
Characterizing Intraseasonal and Interannual Variability in the Composition of the Asian Summer Monsoon Anticyclone Using Aura Microwave Limb Sounder Measurements
Michelle SANTEE1#+, Gloria MANNEY2, Luis MILLAN1, Nathaniel. J LIVESEY1
1California Institute of Technology, 2NorthWest Research Associates
The Aura Microwave Limb Sounder (MLS), launched in July 2004, makes simultaneous co-located measurements of trace gases and cloud ice water content (a proxy for deep convection) in the upper troposphere / lower stratosphere (UTLS) on a daily basis. With its dense spatial and temporal sampling, extensive measurement suite, and insensitivity to aerosol and all but the thickest clouds, Aura MLS is well suited to characterizing UTLS composition in the region of the Asian summer monsoon (ASM) and quantifying the considerable spatial and seasonal variations therein. In addition, the 19-year MLS data record is invaluable for assessing interannual variability in the impact of the ASM on the UTLS. In this talk we will examine MLS measurements of cloud ice and both tropospheric (CO, CH3Cl, CH3CN, HCN) and stratospheric (O3, HNO3, HCl) tracers, along with meteorological reanalyses, to place the 2017 and 2022 ASM seasons observed in detail by the StratoClim and ACCLIP field campaigns, respectively, into the spatial and temporal context of other monsoons in the last two decades. We will also briefly look at the 2024 ASM season that will just be getting underway.
AS79-A007
| Invited
The 2022 Asian Summer Monsoon Chemical and Climate Impacts Project (ACCLIP)
Paul A. NEWMAN1#+, Laura L. PAN2, Elliot ATLAS3, Bill RANDEL2, Troy THORNBERRY4, Brian TOON5
1NASA Goddard Space Flight Center, 2National Center for Atmospheric Research, 3University of Miami, 4NOAA Chemical Sciences Laboratory, 5University of Colorado at Boulder
The Asian summer monsoon Chemical and Climate Impact Project (ACCLIP) used the NASA WB-57f research aircraft, the NSF/NCAR Gulfstream V (GV) research aircraft, the Korean NARA King Air, and a broad set of balloon launches to investigate atmospheric processes that influence ozone depletion and climate in the Korea/Japan region. The NASA WB-57 and NSF GV were flown from Osan Air Base, Republic of Korea during the July-August 2022 period. The circulation of the summertime northern hemisphere upper troposphere – lower stratosphere (UTLS) is dominated by the Asian summer monsoon anticyclone (ASMA or oftentimes called the Tibetan anticyclone). This anticyclonic summer flow develops in response to the southern Asia monsoon and is broadly centered on Tibet. ACCLIP was designed to examine how the ASMA circulation and transport influences the UTLS chemical and aerosol behavior, including links to surface emissions. This presentation will provide background on the ASMA and discuss its wider importance. We will highlight observed dynamical and transport aspects during the summer of 2022, including comparisons to climatological behavior. The ACCLIP mission focused on sampling the ASMA’s eastern flank and outflow into the Pacific Ocean, including mapping the vertical and horizontal structure of UTLS circulation and composition.
AS79-A001
A Transport Overview for ACCLIP (2022) Airborne Observations: From Deep Convection to the Lower Stratosphere
Warren SMITH1#+, Laura L. PAN1, Rei UEYAMA2, Shawn HONOMICHL1, Teresa CAMPOS1, Silvia VICIANI3, Francesco D'AMATO3, Giovanni BIANCHINI3, Marco BARUCCI3
1National Center for Atmospheric Research, 2NASA Ames Research Center, 3National Research Council - National Institute for Optics
The Asian summer monsoon (ASM) has long been known as a weather system, but only recently has its role in atmospheric composition come to be explored in detail. During boreal summer, an anticyclone forms in the upper troposphere and lower stratosphere (UTLS) over Asia which is associated with a pronounced enhancement of chemical and aerosol species lofted from the boundary layer (BL) by ASM deep convection. Transport from the ASM UTLS anticyclone to the global atmosphere was the target of a recent airborne field campaign: The Asian Summer Monsoon Chemical and Climate Impact Project (ACCLIP, 2022). In this work, we overview the transport characteristics contributing to ACCLIP airborne sampling with the aid of Lagrangian trajectory modeling. Specifically, we use backward trajectories to connect airborne sampling to deep convection over Asia, and forward trajectories to connect airborne sampling to the stratosphere. Airborne measurements of the tropospheric tracer carbon monoxide (CO) from ACCLIP are used to link model results with the observed UTLS environment. This analysis provides valuable context for the ACCLIP observations, as well as new insight into the role of ASM transport in impacting global atmospheric composition. We show that ACCLIP sampling had convective contributions from both the East and South Asian summer monsoons, with East Asian convection contributing preferentially higher pollutant concentrations. We also show the majority of sampled air masses in the upper troposphere reached the tropopause within the subsequent week.
AS79-A005
The Unique Tropopause Structure Over the Asian Summer Monsoon and Its Role in UTLS Transport
Laura L. PAN1#+, Shawn HONOMICHL1, Warren SMITH1, Troy THORNBERRY2, Glenn DISKIN3, Rei UEYAMA4, Paul BUI4, Jonathan DEAN-DAY4, Silvia VICIANI5, Francesco D'AMATO5
1National Center for Atmospheric Research, 2NOAA Chemical Sciences Laboratory, 3NASA Langley Research Center, 4NASA Ames Research Center, 5National Research Council - National Institute for Optics
The Asian summer monsoon (ASM) anticyclone is known as the region with the highest tropopause during the season, ranging from 380-400 K potential temperature on average, in contrast to the tropical tropopause at ~375 K. The ASM anticyclone, therefore, appears to be a large continental-scale convection-driven tropospheric "bubble" over the subtropical background stratosphere. The east-west oscillation of the anticyclone at the top of the convection creates a unique mixing zone of stratospheric and tropospheric air near the eastern edge of the anticyclone, where the ACCLIP campaign conducted research flights. Using the WB-57 measurements of temperature, ozone, water vapor, carbon monoxide, together with the large-scale tropopause analysis, we characterize the mixing zone and its implication on the transport of convectively lofted Asian boundary layer air into the UTLS of greater northern hemisphere.
AS79-A006
UT/LS Ozone Variability and Its Impact on Satellite-based Total Ozone Retrievals in East Asia
Chiyoung KIM+, Sang Seo PARK#
Ulsan National Institute of Science and Technology
In the East Asian region, particularly during the winter and spring seasons, the occurrence of secondary ozone peaks in the Upper Troposphere/Lower Stratosphere (UT/LS) at approximately 14 km altitude coincides with active stratosphere-to-troposphere exchange (STE). The significance of these phenomena lies in their contribution to the spatiotemporal variability of total ozone levels, a critical parameter for understanding atmospheric composition and dynamics. The variability in UT/LS ozone emerges as a crucial factor influencing the overall spatiotemporal variation in total ozone. This emphasizes the need to address and account for the complexities arising from vertical ozone distribution when interpreting satellite-retrieved total ozone data. The study focuses on a comprehensive analysis utilizing data from two distinct satellites: the Infrared Atmospheric Sounding Interferometer (IASI), which relies on infrared (IR) channels, and the TROPOspheric Monitoring Instrument (TROPOMI), employing ultraviolet (UV) channels. For the 5-year dataset, we examine the contribution of uncertainties resulting from changes in ozone vertical distribution, with a specific emphasis on UT/LS ozone variability, to the retrieval accuracy of total ozone levels. By comparing the datasets obtained from these two satellite instruments, each utilizing different spectral regions, we aim to enhance our understanding of the challenges associated with satellite-based total ozone retrievals.
AS79-A021
Improving Chemical Boundary Conditions of a Regional Chemistry-transport Model for UTLS Ozone Simulation
Taehee KIM1#+, Kyung-Hwan KWAK1, Heon-Seok DO1, Ja-Ho KOO2, Sang Seo PARK3, Jae-Heung PARK4
1Kangwon National University, 2Yonsei University, 3Ulsan National Institute of Science and Technology, 4Seoul National University
The upper troposphere-lower stratosphere (UTLS) ozone distribution is primarily determined by the complex interactions between the troposphere and stratosphere. To fully understand the dynamic and physiochemical processes in the atmospheric layers, comprehensive data representing UTLS ozone variations are essential. To fill this knowledge gap, researchers from the National Center for Atmospheric Research and the National Aeronautics and Space Administration in the United States have collaborated with researchers in Korea and conducted the ACCLIP (Asian Summer Month Chemical and Climate Impact Project) campaign. This study performs numerical simulations for the ACCLIP campaign periods using the Weather Research and Forecasting (WRF) model coupled with the Community Multiscale Air Quality (CMAQ) model. The faithful chemical boundary conditions are vitally important in order to O3 simulations in the UTLS. In our simulation, we employ the Whole Atmosphere Community Climate Model, characterized by 6-hour time steps. This model is selected from a range of global models due to its ability to capture the complex dynamics of the atmosphere across diverse altitudes and regions. Ozonesonde observations were made 38 and 11 times in the Anmyeondo and Osan, respectively, in August 2022. The study aims to assess the feasibility of simulating ozone concentrations in the middle and upper troposphere (3-10 km altitude) using the WRF-CMAQ modeling system by incorporating proper chemical boundary conditions. To simulate ozone distribution in the UTLS, the model top of WRF was extended from 50 hPa to 10 hPa. The number of vertical grids increased. The simulation results were evaluated and showed the reliability of ozone simulations concerning tropospheric altitude. In addition to validation, the principal dynamics and chemical processes influencing UTLS ozone variability were investigated. This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (RS-2023-00219830).
Session Chair(s): Lin DU, Shandong University
AS10-A002
| Invited
Chemical and Optical Characterization and Sources of Atmospheric Organic Aerosols in Coastal Areas
Caiqing YAN1#+, Haibiao CHEN2, Qingpeng MENG1, Yanjun YANG1, Ruiyu LI1, Xiang DING3
1Shandong University, 2Environment Research Institute, 3Chinese Academy of Sciences
Located in the junction of land and ocean, coastal areas can be affected by land-based and marine emissions. And atmospheric organic aerosols in coastal cities may have significant regional characteristics. In this study, atmospheric fine particulate matter (PM2.5) were collected across different seasons at a coastal rural site in Qingdao, China using a high-volume particle sampler, to investigate the chemical and optical characterization of PM2.5-bound organic fractions (especially water-soluble organic carbon, WSOC) in the coastal suburbs of under the influences of different weather scenarios and air masses. Major PM2.5 species, molecular composition of water-soluble organic fractions, and primary and secondary organic tracers were analyzed using different types of chromatographs and mass spectrometers. Furthermore, absorption and 3D fluorescence spectra were obtained by advanced spectral analysis instruments. The results showed that, compared to marine air masses influenced samples, WSOC affected by continental air masses exhibited higher light absorption coefficients and generally had a higher degree of aromaticity and unsaturation, as well as contained more molecular formulas of WSOC, especially enriched with sulfur-containing compounds. In contrast, relatively more abundant halogen-containing compounds and higher ship emissions source contributions were identified in the marine air masses influenced samples. Furthermore, the isoprene-sourced SOA contribution from marine emissions was also identified in this study. More detailed discussions will be presented in this talk.
AS10-A004
Formation and Transformation of Sea Spray Aerosols: Insights from Laboratory Studies
Lin DU#+
Shandong University
Sea spray aerosol (SSA) represents a major source of aerosol particle populations and significantly impacts the Earth’s radiation budget, cloud formation, and microphysics. It is thus crucial to investigate SSA formation and its atmospheric transformation. Here sea spray aerosol generators were first built and used to study the effects of different organic matters on the production efficiency, size, and morphology of SSA. The molecular weight and concentration of the polymer would affect the production efficiency of SSA. Combining with the measurement of surface tension, we found no clear relationship between surface tension and the yield of SSA, due to the properties of the substances themselves. In addition, the key chemical processes such as the interaction between surface-active molecules, water-soluble organic compounds, and biological macromolecular enzymes at the gas-liquid interface were studied through combination of a Langmuir model and infrared reflection–absorption spectroscopy (IRRAS). We found that the adsorption of glucose and trehalose on the fatty acid monolayer led to the expansion of the mean molecular area. Saccharide–lipid interactions increased with increasing complexity of the saccharide in the order of glucose < trehalose. In a seawater solution, the effects of dissolved saccharides on the ordering and organization of fatty acid chains were muted. The enhancement of the carbonyl band to the low wavenumber region implied that soluble saccharides can form new hydrogen bonds with fatty acid molecules by displacing large amounts of water near the polar headgroups of fatty acids. Our studies provide sufficient insights into formation and transformation of SSA, which would be helpful for improving the accuracy of aerosol emission model parameters.
AS10-A009
The Critical Role of Dimethylamine in the Rapid Particles Formation of Marine Areas
Xiuhui ZHANG#+, Haotian ZU
Beijing Institute of Technology
Recent experiment (He et al, 2021, Science) revealed a vital nucleation process of iodic acid (HIO3) and iodous acid (HIO2) under the marine boundary layer conditions. However, HIO3-HIO2 nucleation cannot effectively derive the observed rapid new particle formation (NPF) in broad marine regions. Dimethylamine (DMA) is a promising basic precursor to enhance nucleation considering its strong ability to stabilize acidic clusters and the wide distribution in marine atmosphere, while its role in HIO3-HIO2 nucleation remains unrevealed. Hence, a method combining quantum chemical calculations and Atmospheric Cluster Dynamics Code (ACDC) simulations was utilized to study the HIO3-HIO2-DMA nucleation process. We found that DMA can compete with HIO2 to accept the proton from HIO3 as a basic precursor in the most stable configurations of HIO3-HIO2-DMA clusters. DMA can significantly enhance the cluster formation rates of HIO3-HIO2 kinetically for more than 103-fold in regions with abundant amine and scarce iodine based on combined factors of high nucleation ability and high concentration of DMA. Furthermore, the iodine oxoacids nucleation enhanced by DMA may explain the sources of rapid NPF events under different conditions corresponding to multiple ocean regions, which can provide important inspirations to understand the frequent and intensive NPF events in broad marine regions.
AS10-A007
Formation Mechanism of Sea Spray Aerosols
Xiaofei WANG#+
Fudan University
Bubble bursting on water surfaces is believed to be a main mechanism to produce submicron drops, including sea spray aerosols, which play a critical role in forming cloud and transferring various biological and chemical substances from water to the air. Over the past century, drops production mechanisms from bubble bursting have been extensively studied. They usually involve the centrifugal fragmentation of liquid ligaments from the bubble cap during film rupture, the flapping of the cap film, and the disintegration of Worthington jets after cavity collapse. Here, we show that a major fraction of previously identified as “bubble bursting” submicron drops are in fact generated via a new underwater mechanism, which are not from bursting process at the water surface. This finding may reshapes our understanding of sea spray aerosol production.
AS10-A011
Factors Controlling Inorganic Sulfate and Organosulfate Formation from the Reaction of Sulfur Dioxide with Organic Peroxides
Narcisse TSONA TCHINDA#+, Lin DU, Xiaofan LV
Shandong University
As important reservoirs for alkoxy radicals and organic peroxy radicals (ROx), organic peroxides are well-known determinant tracers in ROx chemistry. To evaluate the contribution of these peroxides in chemical processes and aerosol formation, we used quantum chemical modeling to examine the pH effect on the degradation of two selected organic peroxides (methyl hydroperoxide (MHP) and benzoyl peroxide (BZP)) by reaction with dissolved SO2 (S(IV)). Results showed that due to the presence of the hydroperoxyl group in its structure, MHP preferably forms inorganic sulfate and methyl sulfate in the pH range 1.81 – 6.97, while forming methyl sulfate, exclusively, at pH > 6.97, unlike BZP that exclusively forms benzoyl sulfate in the pH range investigated. The kinetics of these reactions, explored over the ranges pH 1 – 10 and 240 – 340K, indicate that the effective rate constants of the transformation of both organic peroxides exhibit positive pH and temperature dependencies in the pH and temperature ranges investigated. Over this pH range, BZP is more effectively degraded than MHP, with estimated atmospheric lifetimes in the ranges 5.02×10-19 s – 8.25×10-3 s for BZP and 1.34×10-5 s – 5.05×1010 s for MHP, at 298.15 K. The high reactivity of BZP relative to MHP can be attributed to the activation effect of the benzyl ring on the peroxyl function. Besides the pH effect, this study highlights the role of different substituents on the -O-O- function in altering the kinetics of organic peroxides degradation, and would serve as a ground to evaluate the pH effect in more kinetic analysis of different sources of particulate sulfate. This study further indicates that the aqueous-phase degradation of organic peroxides can adequately drive the change in the chemical composition of dissolved organic matters, both in terms of organic and inorganic sulfate mass fractions.
AS10-A013
Anthropogenic-biogenic Interactions During Biogenic Volatile Organic Compounds Oxidation in the Presence of SO2
Li XU#+
Uniersity of Science and Technology of China
Mixing of anthropogenic pollutants and biogenic volatile organic compounds impacts the formation of secondary organic aerosols (SOA) to an elusive extent. SO2 is one prevalent anthropogenic pollutant whose role on biogenic SOA formation remains unclear, especially under atmospheric complex pollution conditions. The present study explores factors including relative humidity (RH), NOx and NH3 that may influence the role of SO2 on biogenic SOA formation. Results showed that with a constant SO2 concentration, the increase in RH transformed SO2 sinks from stabilized Criegee intermediates to peroxides in aerosol particles. The associated changes in particle acidity and liquid water content may collectively first lead to decreased and then increased SOA yield with increasing RH. The reaction between peroxides and SO2 under high RH is responsible for the formation of organosulfates, especially highly oxidized organosulfates. When NO2 and SO2 coexisted, aerosol yields were higher than with either pollutant alone. Such a synergistic effect of SO2 and NO2 on aerosol formation is mainly because that the nucleation of sulfuric acid could further promote the gas-particle partition of products from NO3· oxidation and particle-phase reactions, In the coexistence of SO2 and NH3, NH3 weakened the enhancement effect of SO2 on SOA yields. The neutralization of aerosol acidity by NH3 may be the main reason for the antagonistic effect between NH3 and SO2. Our research highlight that it is necessary to comprehensively consider RH and the concentration levels of NOx and NH3 when evaluating effects of SO2-involved anthropogenic-biogenic interactions on SOA formation from the oxidation of biogenic volatile organic compounds.
AS10-A012
Interfacial Oxidation Processing of Riverine and Marine Surface Microlayers: An Impact on VOCs and SOA in the Atmosphere
Yiqun WANG#+, Sasho GLIGOROVSKI
Chinese Academy of Sciences
Ozone (O3) and sulfur dioxide(SO2) oxidation chemistry on the organic film and water surface microlayer (SML) generates volatile organic compounds (VOCs) to the atmosphere. To shed light on the proposed significance of this chemistry, we investigated the formation of VOCs through heterogeneous chemistry of O3 (100 ppb) and SO2(30 ppb)with authentic SML collected from 10 sites in the South China Sea using a reactor coupled to proton transfer reaction−time of flight−mass spectrometry (PTR−TOF−MS) and a high-resolution quadrupole Orbitrap mass spectrometer(SESI-Orbitrap-MS), subsequently identified by off-line techniques. On the basis of the semiquantitative data of the identified compounds, we estimated the production rates of the key saturated and unsaturated ketones and aldehydes, which correspond to the experimental conditions applied in this study. These results provide a significant update to our understanding of abiotic formation of VOCs in the marine atmosphere, which should be considered in future model studies to properly evaluate the VOC contribution of ozone heterogeneous chemistry with the SML.
AS10-A006
Role of Sea Spray Aerosol at the Air-sea Interface in Transporting Aromatic Acids to the Atmosphere
Yaru SONG+, Lin DU#
Shandong University
Aromatic acids are ubiquitous in seawater and can be transported to the atmosphere via sea spray aerosol (SSA). Despite their importance in affecting the global radiative balance, the contribution of marine aromatic acids and their transport mechanisms through SSA remain unclear. Herein, the distribution of particle size and number concentration of SSA produced in seawater containing nine different aromatic acids (i.e., benzoic acids, benzenedicarboxylic acids, hydroxybenzoic acids, vanillic acid, and syringic acid) was studied using a custom-made SSA simulation chamber; moreover, enrichment of aromatic acids in SSA and their emission flux to the atmosphere were analyzed. Transmission electron microscopy (TEM) images clearly revealed that aromatic acids can be transferred to the nascent SSA. Interestingly, the morphology associated with benzene dicarboxylic acids-coated particles showed that aromatic acids can promote the growth of other surfaces of sea salt, thus making the sea salt core spherical. Aromatic acids showed a significant enrichment behavior at the air-sea interface, which clearly indicated that SSA represent a source of aromatic acids in the atmosphere. Vanillic acid had the largest global emission flux through SSA (962 tons yr-1), even though its concentration in seawater was lower. The calculated results indicated that the global annual flux of aromatic acids was not only affected by the concentration in seawater, but also by their enrichment factor (EF). These data are critical for further quantifying the contribution of organic acids to the atmosphere via SSA, which may provide an estimate of the potential influence of the atmospheric feedbacks to the ocean carbon cycle.
AS10-A005
Governance of Marine Emissions and Terrestrial Air Masses: Influence on the Composition and Properties of Carbonaceous Aerosols Over the Eastern China Marginal Seas
Kuanyun HU+, Lin DU#
Shandong University
Marine aerosols contribute significantly to atmospheric aerosols, playing substantial roles in influencing the regional and global environment and climate. Marine aerosols over the Eastern China Marginal Seas (ECMS: Bohai Sea-BS, Yellow Sea-YS and East China Sea-ECS) are co-controlled by productive seawater and populated land, but the composition and variation of marine aerosols remain poorly understood. In this study, marine aerosol samples were collected in spring of 2023 covering the entire ECMS to explore the spatial variation and the optical properties of carbonaceous species. Due to significant terrestrial transport, the concentration of TSP and carbonaceous species shows a spatial variation of high in the north and low in the south at latitude. Utilizing satellite data and backward trajectory analysis, the elevated solubility of organic carbon (OC) in southern YS may possibly be influenced by long-range transport and atmospheric aging of terrestrial biomass combustion and marine bioactive gases. Terrestrial transport increases aerosol light absorption, while marine sources and solar radiation weaken it. Humic-like substances are the predominant fluorescent chromophores, and marine sources can regulate the abundance of protein-like substances. The elevated simple forcing efficiency (SFE) and relative radiative forcing (RRF) in the near ultraviolet and visible light range indicate considerably warming effect attributed to terrestrial pollutants. The current results suggest that emphasis should be placed on the effect of terrestrial source transport in BS, while in the relatively open YS and ECS, more attention should be paid to the contribution of marine sources to marginal sea aerosols.
AS10-A008
Experimental Evidences for Droplets Formation Through Film Flapping During Bubble Bursting
Xiaofei WANG#, Xinghua JIANG+
Fudan University
Tiny water drops produced from bubble bursting play a critical role in forming cloud, scattering sunlight, and transporting pathogens from water to the air. Bubbles burst by nucleating a hole at their cap foot and may produce jets, or film drops. The latter originate from the fragmentation of liquid ligaments formed by the centripetal destabilization of opening hole rim. They constitute a major fraction of the aerosols produced from bubbles with cap radius of curvature (R) > ~ 0.4 × capillary length(a). However, our present understanding of the corresponding mechanisms does not explain the production of most submicron film drops, which represent the main number fraction of sea spray aerosols. In this study, we report observations showing that bursting bubbles with R < ~0.4a are actually mainly responsible for submicron film drops production, through a mechanism involving the flapping shear instability of the cap with the outer environment. With this newly proposed pathway, the complex relations between bubble size and number of drops produced per bubble can be better explained, providing a fundamental framework for understanding production flux of aerosols and the transfer of substances mediated by bubble bursting through the air-water interface and the sensitivity of the process to the nature of the environment.
Session Chair(s): Noel KEENLYSIDE, University of Bergen
AS33-A002
| Invited
Conundrums of Earth System Predictability
Chidong ZHANG#+
NOAA Pacific Marine Environmental Laboratory
This presentation discusses several conundrums in the current studies of Earth system predictability. This presentation focuses on the potential predictability including its source and limit, instead of the actual predictability (prediction skills). Boundary conditions as the source of climate predictability at the early stage of climate prediction using atmosphere-only models disappear in fully coupled Earth system models (except at the top of the atmosphere). Slowly evolving phenomena, such as the MJO, ENSO, and AMOC, have been cited as the sources of predictability from intraseasonal to decadal timescales. But most of these slowly evolving phenomena are now the targets of prediction and their sources of predictability remain ambiguous. Restrictively speaking, initial conditions are the only sources of predictability for a fully coupled Earth system. If sources of weather predictability come from signals of perturbations in initial conditions, sources of climate predictability come from signals of the mean state in initial conditions, then sources of S2S predictability would be a combination of signals of both perturbations and the mean state in initial conditions. Finally, it is argued that a predictable phenomenon must have a constant feature, which can take various non-static and spatially/temporally varying forms.
AS33-A023
Developing a Global Coupled Configuration at the Met Office for Implementation at All Timescales and Ready for Future HPC Infrastructures
Charline MARZIN#+
Met Office
The Met Office along with its partners has recently released a Global Coupled configuration GC5 which will be the baseline for upcoming upgrades to the NWP, seasonal and climate modelling systems. As well as improving most aspects of atmosphere and ocean parametrisation, the development of this configuration made use of an extensive and innovative seamless testing framework to test and improve the model using data assimilation, ensemble, coupled and climate change tests. The configuration provides significant improvements to the southern Ocean, tropical rainfall and several key modes of variability and performance metrics. Additional work to understand the impact of latest development on climate sensitivity and the use of perturbed parameter ensembles will be presented. This configuration is also forming the baseline for the next generation modelling system that will enable better scalability on future infrastructures and preliminary results will be presented.
AS33-A016
Supermodelling to Improve Climate Prediction
Noel KEENLYSIDE1#+, Francine SCHEVENHOVEN1, Ping-Gin CHIU1, Tarkeshwar SINGH2, Francois COUNILLON2, Mao-Lin SHEN1, Gregory DUANE1,3
1University of Bergen, 2Nansen Environmental and Remote Sensing Center, 3University of Colorado
Climate models are plagued by long-standing biases that degrade predictions. While increasing resolution of global climate models to km scales promises to reduce biases, there is little evidence so far of improvements with currently available computing power. Supermodelling is an alternative approach that has demonstrated reductions in long-standing biases, such as the double ITCZ and tropical SST biases, at a fraction of the computational cost of km scale models. A supermodel is a combination of models that interact during their simulations to mitigate errors before they develop into large-scale biases. Here I will present recent results from a supermodel based on three Earth System Models (NorESM, CESM, MPIESM) trained using observed SST. The models were combined using ocean data assimilation with monthly frequency. The simulation of tropical climate is markedly improved in the supermodel compared to that of the respective standalone models. Seasonal predictions performed with this model are underway and first results will be shown. In addition, I will summarize work on combining atmospheric models that promises to lead to even greater improvements in simulating global climate.
AS33-A001
A Multi-year Climate Prediction System Based on CESM2
Yong-Yub KIM1#+, June-Yi LEE2, Axel TIMMERMANN2, Yoshimitsu CHIKAMOTO3, Sun-Seon LEE2, Eun Young KWON1, Wonsun PARK2, Nahid A. HASAN3, Ingo BETHKE4, Filippa FRANSNER4, Alexia KARWAT2, Abhinav R. SUBRAHMANIAN1
1IBS Center for Climate Physics, 2Pusan National University, 3Utah State University, 4Bjerknes Centre for Climate Research
Here we present a new seasonal-to-multiyear earth system prediction system which is based on the Community Earth System Model version 2 (CESM2) in 1° horizontal resolution. A 20- member ensemble of temperature and salinity anomaly assimilation runs serves as the initial condition for 5-year forecasts. Initialized on January 1st of every year, the CESM2 predictions the exhibit only weak climate drift and coupling shocks, allowing us to identify sources of multiyear predictability. To differentiate the effects of external forcing and natural climate variability on longer-term predictability, we analyze anomalies calculated relative to the 50-member ensemble mean of the CESM2 large ensemble. In this presentation we will quantify extent to which marine biogeochemical variables are constrained by physical conditions. This analysis provides crucial insights into error growth of phytoplankton and the resulting limitations for multiyear predictability.
AS33-A014
Potential Predictability of Forage, Pelagics and Demersals Biomass
Hyung-Gyu LIM1#+, Colleen PETRIK2
1Korea Institute of Ocean Science and Technology, 2University of California San Diego
With the emergence of predictive skills of climate variability, we currently stand at the horizon of being able to forecast marine ecosystems. However, the assessment of the capacity to predict high trophic levels of marine ecosystems has been rarely investigated. Here, we investigate predictability of fish biomass integrated by spatially explicit mechanistic model of fish with three functional types. We also evaluate the bottom-up biophysical drivers of fish that are predicted by decadal prediction outcomes from an Earth system model, initialized through forced ocean-sea ice simulations. We found that temperature drivers have longer predictability ~8 years while biological drivers have predictabilities within 1-2 years. The fish biomasses have skillful predictability within 2 years globally, extended more years regionally. These findings build upon prior research in evaluating the predictability of bottom-up drivers on fish, potentially illuminating a path towards operating forecast systems of living marine resources.
AS33-A019
Exceptional Multi-year Prediction Skill of the Kuroshio Extension in the CESM High-resolution Decadal Prediction System
Who KIM1#+, Stephen YEAGER1, Gokhan DANABASOGLU1, Ping CHANG2
1National Center for Atmospheric Research, 2Texas A&M University
The Kuroshio Extension (KE) has far-reaching influences on climate as well as on local marine ecosystems. Thus, skillful multi-year to decadal prediction of the KE state and understanding sources of skill are valuable. Retrospective forecasts using the high-resolution Community Earth System Model (CESM) show exceptional skill in predicting KE variability up to lead year 4, substantially higher than the skill found in a similarly configured low-resolution CESM. The higher skill is attained because the high-resolution system can more realistically simulate the westward Rossby wave propagation of initialized ocean anomalies in the central North Pacific and their expression within the sharp KE front, and does not suffer from spurious variability near Japan present in the low- resolution CESM that interferes with the incoming wave propagation. These results argue for the use of high-resolution models for future studies that aim to predict changes in western boundary current systems and associated biological fields.
AS33-A018
Estimating Seasonal to Multi-year Predictability of Statistics of Climate Extremes Using the CESM2-based Climate Prediction System
Alexia KARWAT1#+, June-Yi LEE1, Christian FRANZKE1, Yong-Yub KIM2
1Pusan National University, 2IBS Center for Climate Physics
Climate extremes, such as heat waves, heavy precipitation, intense storms, droughts, and wildfires, have become more frequent and severe in recent years as a consequence of human-induced climate change. Estimating the predictability and improving prediction of the frequency, duration, and intensity of these extremes on seasonal to multi-year timescales are crucial for proactive planning and adaptation. However, climate prediction at regional scales remains challenging due to the complexity of the climate system and limitations in model accuracy. Here we use a large ensemble of simulations, assimilations, and reforecasts using Community Earth System Model version 2 (CESM2) to assess the predictability of statistics of climate extremes with lead times of up to 5 years. We show that the frequency and duration of heat waves during local summer in specific regions are predictable up to several months to years. Sources of long-term predictability include not only external forcings but also modes of climate variability across time scales such as El Niño and Southern Oscillation, Pacific Decadal Variability, and Atlantic Multidecadal Variability. This study implies opportunities to deepen our scientific understanding of sources for long-term prediction of statistics of climate extremes and the potential for the associated disaster management.
AS33-A004
Future North Atlantic Warming Hole Modulates Interhemispheric Temperature Change
In-Hong PARK#+, Sang-Wook YEH
Hanyang University
Accurately projecting the impact of the North Atlantic subpolar cooling region despite global warming, known as 'warming hole', on global climate is critical but uncertain due to its complex mechanisms. Here, we use the latest multi-model simulations (CMIP6) to investigate the impact of changes in the warming hole on future climate change. We find that changes in the warming hole play an important role in creating an asymmetry in temperature and precipitation patterns between the hemispheres: the weaker the warming hole (corresponding to strong warming in the North Atlantic subpolar region), the greater non-radiative fluxes (sensible and latent heat flux) transported to the atmosphere, leading to greater warming in the Northern Hemisphere than the Southern Hemisphere. This difference in warming leads to an energy imbalance between the hemispheres, resulting in a northward shift of the Inter-Tropical Convergence Zone (ITCZ). These changes have a significant impact on the distribution of precipitation, contributing to the precipitation imbalance between the two hemispheres. Our findings highlight that a better understanding of the warming hole is important for accurate projections of future global climate, especially hemispheric temperature and precipitation patterns.
AS33-A003
Changing Footprint of the Pacific Decadal Oscillation on Global Land Surface Air Temperature
Zhenzhong ZENG1#+, Alan ZIEGLER2, Deliang CHEN3, Philippe CIAIS4, Laurent LI5, Shijing LIANG1, Dashan WANG1, Rongrong XU1, Lili LIANG1
1Southern University of Science and Technology, 2Kasetsart University, 3University of Gothenburg, 4Institut Pierre Simon Laplace, 5Laboratoire de Météorologie Dynamique
Decadal-scale periods of global warming slowdown and acceleration are associated with varying phases of the Pacific Decadal Oscillation (PDO). However, the footprint of the PDO on land temperature has not been determined and how this footprint has changed over time remains unknown. Here we use an observational dataset of global land temperature since 1901 to search the footprint of the PDO and its influence on the variability of climate warming rates. We find that a warming acceleration associated with the transition of PDO from negative to positive phase has remained high and has been expanding in area since the early 20th century. Meanwhile, the warming slowdown associated with the reverse transition appears to be shrinking worldwide. This configuration implies that in the coming decade with a likely occurrence of an ascending transition of the PDO, a period of faster anthropogenic global warming could be anticipated.
Session Chair(s): Wei-Ting CHEN, National Taiwan University, Shih-Hao SU, Chinese Culture University
AS52-A001
Cold Fog Amongst Complex Terrain (CFACT)
Zhaoxia PU#+
University of Utah
Fog frequently forms in high-elevation complex terrain as over water bodies but is less understood and difficult to predict. Cold fog forms via various thermodynamic, dynamic, and microphysical processes when the air temperature is less than 0°C. It occurs frequently during the cold season in the western United States yet is challenging to detect using standard observations and very difficult to predict. The Cold Fog Amongst Complex Terrain (CFACT) project goals are to 1) investigate the lifecycle of cold-fog events over complex terrain with the latest observation technology, 2) improve microphysical parameterizations and visibility algorithms used in numerical weather prediction (NWP) models, and 3) develop data assimilation and analysis methods for current and next-generation (e.g., sub-kilometer scale) NWP models. The CFACT field campaign took place in Heber Valley, Utah, during January and February 2022, with support from NSF’s Lower Atmospheric Observing Facilities (managed by NCAR’s Earth Observing Laboratory), the University of Utah, and Ontario Technical University. A network of ground-based and aerial in situ instruments and remote sensing platforms were used to obtain comprehensive measurements of thermodynamic profiles, cloud microphysics, aerosol properties, and environmental dynamics. Nine intensive observation periods (IOPs) explored various mountainous weather and cold-fog conditions. Field observations, NWP forecasts, and large-eddy simulations provided unprecedented data sources to help understand the mechanisms associated with cold-fog weather and to identify and mitigate numerical model deficiencies in simulating winter weather over mountainous terrain. This presentation summarizes the CFACT field campaign, its observations, and recent progress in science data analysis, fog process studies, numerical simulations, and model validation. [References: Pu, Z., E. Pardyjak, S. Hoch, I. Gultepe, A. G. Hallar, A. Perelet, R. Beal, G. Carrillo-Cardenas, X. Li, M. Garcia, S. Oncley, W. Brown, J. Anderson, J. Witte, A. Vakhtin, 2023: Cold Fog Amongst Complex Terrain. Bulletin of the American Meteorological Society. 104, E2030-E2052. https://doi.org/10.1175/BAMS-D-22-0030.1].
AS52-A002
Effects of In-land Breeze Induced by Neighboring Land Type Patches on Vertical Energy Transport in Large Eddy Simulations of VVM
Wei-Ting CHEN#+, Tzu-Han HSU, Chien-Ming WU, Po-Yen CHEN
National Taiwan University
Boundary layer turbulence, crucial for vertical energy and moisture transport, can be influenced by coherent horizontal flows driven by diurnal heating difference in land surfaces. This study employs Large Eddy Simulations of the vector vorticity equation cloud-resolving model (VVM) coupled with the Noah Land Surface Model to explore these processes. Three land type configurations are examined: a combination of half grassland and half urban land (HALF), entire grassland (GRASS), and entire urban land (URBAN). All experiments adopt a 12.8 12.8 km2 horizontal domain with 100 m grid spacing and 20 m vertical resolution. The initial condition reflects a stable, windless environment with convective available potential energy close to zero, sourced from a 06 LST radiosonde observation over the western plain of Taiwan during springtime. As the simulated solar insolation varies from 06 to 14LST, the developed circulation features a near-surface horizontal flow from grassland to urban reaching 2 m/s at noon and a weaker but thicker upper-layer return flow from urban to grassland. The urban patch exhibits an overall updraft with the maximum of 0.3 m/s. Both urban and the grass regions in HALF exhibit weaker vertical turbulent kinetic energy compared to URBAN and GRASS. The boundary layer over the grassland patch in HALF is more stable, with a significant transition zone at the boundary layer top. In HALF, the latent heat flux is predominantly contributed by the grassland patch, exceeding that in GRASS by 9% at noon. The column water vapor (CWV) over the grassland patch in HALF remains constant over time, while the CWV over the urban patch increases. As the induced circulation crossing different land types in HALF potentially plays a dominant role in energy transport, future investigations will focus on its influence on local stability, entrainment at boundary layer top and local surface fluxes.
AS52-A012
Numerical Simulation of Water Vapor Changes in Yilan Under Cold High-pressure Conditions
Pei-Di JENG+, Jou-Ping HOU#
National Defense University
To understand the difference in the amount of water vapor transported to Yilan under the influence of the northeast monsoon, this study used the WRF model (Weather Research and Forecasting Model, WRF) to simulate water vapor transported by different types of cold high pressure with the highest spatial resolution of 500 m. Calculate the total amount of water vapor and water vapor flux in the Lanyang Plain, and analyze the potential precipitation trend in this area. The research results found that on November 26, 2021, and October 25, 2022, the cold high pressure was at a higher latitude (40 。 N), and the low-level water vapor content in the Yilan was higher; on December 6, 2023, and December 7, 2023, the cold high pressure was at a lower latitude (30 。 N), and the low-level moisture is lower. Such a result may be related to the strength of the cold air mass, the path and time of the cold air mass passing through the ocean, and the physical mechanism of cold air mass transformation in the ocean boundary layer.
AS52-A003
Examining the Long-term Variations in the Winter Rainfall Features in Yilan, Taiwan and the Future Projections Under Climate Change Scenarios
Chin-Hsiang WU, Shih-Hao SU#+
Chinese Culture University
The northeast Taiwan region, particularly Yilan, exhibits distinct spatial rainfall patterns during wintertime northeasterly conditions. These patterns are intricately connected to the interaction between large-scale background flow and complex topography. Kabasawa (1950) initially described the characteristic winter rainfall in Yilan, noting a decrease in precipitation from the coast towards the southwestern mountainous region. Su et al. (2022) further developed a conceptual model during the YESR2020 campaign, elucidating the interplay between local circulation and rainfall patterns influenced by northeasterly winds and complex terrain. This model contrasts with Kabasawa's (1950) findings, revealing a decline in rainfall distribution from the southwestern mountains towards the plains. Spatial rainfall characteristics are intricately linked to variations in large-scale background wind features and moisture flux distribution. Over the past 40 years, an analysis of Yi-Lan's rainfall unveiled terrain-locked precipitation patterns, emphasizing the ERA5 reanalysis data to assess long-term changes in wind features and moisture distributions. Notably, rainfall hotspots were identified on the windward side of prevailing northeasterlies in the mountainous region, decreasing towards the plains. Average rainfall exhibited an upward trend, particularly pronounced in the southern mountain region. High-resolution cloud model experiments illustrated that alterations in large-scale background wind features influence local circulation patterns over terrain, impacting convective initiation locations. This characteristic pattern was consistently observed through cluster analysis of historical rainfall data. The southern mountains experienced higher moisture flux and more easterly wind directions during precipitation hotspots. In essence, understanding the relationship between background winds and rainfall aids in projecting future changes in precipitation characteristics in Yilan under climate change scenarios.
AS52-A005
UAV-assisted Exploration in Topographic-induced Wind and Rainfall During YESR in Yilan, Taiwan
Hou Lun LAO1#+, Sheng-Hsiang WANG1, Shih-Hao SU2, Hung-Chi KUO3
1National Central University, 2Chinese Culture University, 3National Taiwan University
During the winter Northeast Monsoon season, northern Taiwan experiences recurrent episodes of heavy rainfall. Especially in the southern Yilan, due to the unique interaction between its distinctive topography and the Northeast Monsoon, resulting in prolonged and intense rainfall. Notably, this region broke Taiwan's annual rainfall record in 2022. However, the intricacies of the interaction between the Northeast Monsoon and local topography lack clarity, primarily due to a dearth of vertical observational data. To bridge this knowledge gap, the Yilan Experiment of Severe Rainfall was executed in both 2021 and 2022 (YESR2021, YESR2022), providing comprehensive three-dimensional datasets. Utilizing two decades of meteorological station and reanalysis data, this study classifies wind directions in the Yilan region under varying environmental wind conditions. Results indicate a prevailing westward surface wind component during periods dominated by the Northeast Monsoon, with a maximum of 76.5% occurring at ambient wind directions between 50-70 degrees. This aligns with the periods of maximum rainfall duration and intensity. Moreover, the maximum frequency of intense rainfall in the plains and coastal mountain areas occurs under different angles of the environmental wind, indicating distinct mechanisms for heavy rainfall in these regions. Additionally, this study is going to incorporate high-temporal and spatial resolution unmanned aerial vehicle (UAV) vertical observations from YESR2021 and YESR2022. The aim is to calculate moist Froude number and moist static energy, providing insights into the convection location and intensity. By integrating stability analysis with ground station results, a comprehensive exploration of the favorable conditions for rainfall in the Yilan will be conducted.
AS52-A009
Performance Assessment of PBL Structures Based on Observation and Model Study
Fang-Yi CHENG#+, Hong ZHAO
National Central University
Due to the advances in the atmospheric boundary layer observation technique, many high spatial- and temporal-resolution instruments are deployed to investigate turbulence structures. This study conducts observation and model simulation to investigate the planetary boundary layer structures. The radial wind profiler, Doppler wind lidar, microwave radiometer profiler, and radiosonde were used to study the PBL mean and turbulent fields. We performed high-resolution WRF simulations with various types of PBL schemes to assess the impact of the PBL parameterizations on the meteorological fields. When model resolution approaches the scales of the most energy-containing turbulence, the gray-zone problem occurs. This study characterized the turbulence kinetic energy based on the observation and model simulation and assessed the model performance against the observation data. Details will be discussed during the conference.
AS52-A006
Dispersion Simulations for an Oil Burn Experiment in Alaska
Fong NGAN1,2#+, Mark COHEN1, Hyun-Cheol KIM3, Brian GULLETT4, Johanna AURELL4, Josip ADAMS5, Victoria SCHOLL5, Chris OWEN4, Karen STONE6
1National Oceanic and Atmospheric Administration, 2University of of Maryland, 3NOAA Air Resources Laboratory, 4U.S. Environmental Protection Agency, 5U.S. Geological Survey, 6U.S. Department of Interior
An oil burn experiment was conducted at the University of Alaska Fairbanks’ Poker Flat Research Range on a subset of a 1 ha artificial pond during August 2-3, 2022. The downwind PM 2.5 concentrations were measured with unmanned aircraft systems (UAS) flown by the U.S. Geological Survey carrying the U.S. Environmental Protection Agency’s (EPA) “Kolibri” sampler. The near-field wind velocity, temperature, and relative humidity were collected using radiosonde. In this study, we used the Weather Research and Forecasting (WRF) model to provide meteorological fields in a sub-kilometer spatial resolution for running NOAA’s dispersion model, HYSPLIT, to simulate the transport and dispersion of one of the oil burn experiments. One of the sources of uncertainty in dispersion modeling is the accuracy of the meteorological input used to drive the model. Potential errors in the simulated wind fields may cause the modeled plume to move in the wrong direction, while the uncertainty of stability and turbulent parameters may result in an inaccurate mixing in the dispersion simulation. We assimilated the radiosonde data in WRF simulations through observational nudging to improve the meteorological fields that later were used to drive HYSPLIT dispersion modeling. There were seven burns in this experiment. Burn 3 was conducted on August 3, 2022, starting at 1711 UTC. The observational nudging with the wind profiles collected by the radiosonde successfully reduced the bias in wind speed and direction prediction. The nudged simulation still underpredicted the wind speed, but its variation along with altitude was much improved by the observational nudging using the radiosonde data. We compared the transport pattern from HYSPLIT results driven by two sets of WRF meteorological data (non-nudged and nudged). When using the WRF wind fields corrected by the wind measurements, the modeled plume moved in a direction more consistent with the UAS measurement.
Session Chair(s): Sridhara NAYAK, Japan Meteorological Corporation, Zhenchen LIU, Fudan University, Kritanai TORSRI, Ministry of Higher Education, Science, Research and Innovation
AS11-A042
| Invited
Interhemispherical Footprint on Indian Monsoon Floods
Venugopal VURUPUTUR1#+, Rajat JOSHI2, Pritam Jyoti BORAH1
1Indian Institute of Science, Bangalore, 2Princeton University
The seasonal extremes of Indian Summer Monsoon Rainfall (ISMR) - floods and droughts – are often thought to be triggered by external forcing such as the El Niño Southern Oscillation. Specifically, La Niña (El Niño) conditions are believed to modulate monsoon circulation leading to seasonally anomalous excess (deficit) rain over India. However, historical records suggest that nearly 40-50 % of these seasonal extremes (floods or droughts) over India have occurred when the equatorial Pacific sea surface temperatures were near neutral. Here, we focus specifically on monsoon floods and highlight the differences in rainfall evolution during (i) flood and normal rainfall years, and (ii) floods associated with La Niña and No La Niña conditions. Our analysis suggests that floods appear to be mainly because of increased rainfall either at the beginning and/or end of the season. In particular, we show that during Non La Niña floods, there is a near-doubling of rainfall during late-August/early-September. More importantly, we show using reanalysis that this abrupt increase in rainfall accumulation can be related to an interplay between atmospheric conditions in the northern and southern midlatitudes. Specifically, our analysis suggests that a wave train curving in from northern mid-latitudes towards equator, coupled with a blocking high centred around (60N, 15E) and an anomalously strong low level jet, in late August may have led to the observed heavy rain over India. Equally importantly, a large pressure gradient between India and Madagascar over a 20-day period in late-August appears to be a critical driver for strengthening of the low-level jet.
AS11-A055
Arctic Sea-ice Decline Causes Extreme Tropical Precipitation Events Under Greenhouse Warming
Sandeep NARAYANSETTI#+, Swapna P, Krishnan RAGHAVAN
Indian Institute of Tropical Meteorology
Arctic sea-ice decline has been accelerating under greenhouse warming. We investigate the tropical precipitation extreme events response to declining Arctic sea-ice using observations and climate model simulations. Idealized warming experiments in which Arctic becomes ice free under greenhouse warming show robust response on the tropical precipitation extreme events. We find enhancement of mean tropical precipitation and increasing propensity of extreme precipitation events over South Asian region. The enhanced Arctic sea-ice melt increases the mid-latitude waviness transcending energy further southwards into the tropics. This in addition to northward shift of intertropical convergence zone enhances tropical precipitation. The enhanced energy in the tropics along with the anomalous mid-latitude intrusions provide a conducive environment for moisture convergence and intense summer monsoon precipitation events over South Asia. Our findings suggest that the intense precipitation events over the South Asian Summer monsoon region are projected to increase as the Arctic continues to warm more quickly than the rest of the planet under greenhouse warming.
AS11-A057
Simulation of Heavy Rainfall Event on August 28, 2023 in West Sumatra Using 3DVar and 4DVar Weather Radar Data Assimilation
Jaka PASKI1#+, Donaldi PERMANA2, Junshi ITO1
1Tohoku University, 2Indonesian Agency for Meteorology, Climatology and Geophysics
On August 28 2023, heavy rainfall of 102 mm/day occurred over West Sumatra in Indonesia and caused flooding and landslides in the vicinity. To improve the NWP simulation of this rainfall event, weather radar data assimilation is one way to improve the initial atmospheric data conditions. This research aims to investigate the effect of Doppler weather radar data assimilation on the Weather Research Forecasting (WRF) numerical model and compare between three-dimensional and four-dimensional variations data assimilation methods (3DVar and 4DVar). Three simulations were conducted using the WRF model, i.e. without data assimilation, with 3DVar and 4DVar data assimilation. The simulation was then compared with surface rainfall observation data and Quantitative Precipitation Estimation (QPE) from Doppler weather radar data. The results indicate improvements in the numerical model using assimilated data.
AS11-A054
Climatology of Convectively Coupled Equatorial Waves Using 20 Years of High-resolution IITM GFS Model Hindcast Simulations
Himabindu HANUMANTHU+, Parthasarathi MUKHOPADHYAY#
Indian Institute of Tropical Meteorology
Fundamental modes of tropical variability consist of convectively coupled equatorial waves (CCEWs). The understanding and simulations of CCEWs remained a significant issue in weather and climate modelling. Using 20 years of IITM GFS T1534 (~12.5 km resolution) hindcast data from 2000 to 2019, the climatology of CCEWs and the Madden-Julian Oscillation (MJO) in particular are analyzed for the first time in the present study. We evaluated the high resolution 12km GFS model prediction of tropical variability with respect to observations like IMERG rainfall and NOAA OLR data. The results shows that the features are well simulated up to day 3 forecast. However, there are certain biases noted in the simulation of tropical waves which need further improvement. The main characteristics of the climatological equatorial rainfall through it’s space–time spectra are accurately portrayed, and the model's performance is assessed by analyzing the rainfall's diurnal phase. These long-term results can serve as benchmarks to enhance the model physics for predicting such wave patterns and further improvement.
AS11-A050
Development of UAV-mounted Image Disdrometer for Observing Raindrop Particle Size Distribution at High Altitude
Gaiya TANAKA#+, Makoto NAKAYOSHI, Shiho ONOMURA
Tokyo University of Science
In recent years, accurate monitoring of precipitation has become increasingly important in Japan, as heavy rainfall disasters have been becoming more frequent due to global warming. As a current rainfall monitoring system, tipping bucket rain gauges are widely used throughout Japan, but the spatial resolution are too large to capture rainfall pattern precisely. Therefore, there is a rising demand for weather radar that can observe precipitation intensity at a finer spatial resolution. Presently, Multi-Parameter Radar (MP Radar) is used as a radar-based rainfall observation system. This radar can estimate real-time raindrop particle size distribution and utilize them for rainfall intensity calculations. However, the accuracy of the estimated raindrop particle size distribution has not been sufficiently validated. In this study, we aim to validate the accuracy of the raindrop particle size distribution estimated by the MP Radar. To achieve this, we modified the Image Disdrometer developed by Onomura et al. (2019) to create an instrument capable of measuring raindrop size distributions at high altitudes. Specifically, we miniaturized the conventional Image Disdrometer to less than 1/4 of its original size and mounted it on a drone. Before conducting actual observations by flying the drone over a target region of MP Rader, we hovered it at a few meters above the ground to verify the accuracy of the raindrop particle size distribution observed by a conventional laser disdrometer and the UAV-mounted observation instrument. The results of this observation will be presented at AOGS2024.
Session Chair(s): Chaerin PARK, Seoul National University
AS31-A002
| Invited
Watching the Earth Breathe: Observations of Carbon Dioxide and Solar-induced Fluorescence with OCO-2 and OCO-3
Thomas KUROSU#+, Abhishek CHATTERJEE, Vivienne PAYNE
California Institute of Technology
The Orbiting Carbon Observatory-2 and the Orbiting Carbon Observatory-3 are NASA's first two missions designed specifically for the space-based measurement of carbon dioxide. OCO-2 was launched in 2014 and, as part of NASA’s “A Train”, has been making continuous global measurements of dry-air column CO2 (XCO2) and solar-induced fluorescence (SIF) from a sun-synchronous, low-earth orbit with a fixed 1336h equator crossing time. In 2019 OCO-3, the spare instrument copy of OCO-2, was installed on the International Space Station (ISS). Like OCO-2, OCO-3 also measures XCO2 and SIF but does so at all times between dawn and dusk, without a fixed repeat cycle and limited to ±52º latitude due to the inclined orbit of the ISS. Both instruments perform observations in nadir, ocean glint, and target geometry, with an extra mode added to OCO-3 that is dedicated to map urban areas. This presentation will give an overview of the two missions, highlight some of the challenges of CO2 monitoring from space, and provide a summary of the contributions OCO-2&3 observations have made to advance our understanding of carbon cycle science on global and local scales.
AS31-A017
| Invited
Urban Fossil Fuel-CO2 Emissions, and the Role of the Biosphere, Based on Measurements of Atmospheric Radiocarbon
John B. MILLER1#+, Scott J. LEHMAN2, Charles MILLER3, Brian MCDONALD4
1NOAA Global Monitoring Laboratory, 2University of Colorado, Boulder, 3California Institute of Technology, 4NOAA Chemical Sciences Laboratory
Despite inventory-based, or “bottom-up”, estimates of fossil fuel-CO2 (CO2ff) emissions likely being accurate to within 10% at annual, national scales for most developed countries, uncertainties can be much larger at urban scales. Top-down approaches can also provide additional information such as the seasonality of emissions and can be closer to real time than most bottom-up approaches. We will present CO2ff emissions estimates based on atmospheric radiocarbon (14C) and CO2 measurements for the U.S., with a focus on Los Angeles. Whether from ground-based in situ sensors, or via ground-based or satellite remote sensing, measurements of CO2 concentrations alone are not sufficient to determine fossil emissions. This is because terrestrial ecosystem CO2 exchange can influence, and even dominate, spatio-temporal gradients of CO2, confounding the interpretation of CO2. The rarest isotope of C, 14C, is completely absent from fossil fuels allowing us to use precise measurements of atmospheric CO2 and its 14C:C ratio to separate the fossil and biospheric contributions to observed gradients. We will present estimates of CO2ff emissions for Los Angeles for 2015, August 2021 and summer 2023 based on regular monitoring and intensive measurement campaigns. These top-down results will be compared to bottom-up emissions estimates from Vulcan and the GRAAPES emissions data products. We will also present a summary of results from other urban areas in the United States and elsewhere highlighting the significance of the urban biosphere. Finally, we will demonstrate the application of measurements of nitrogen oxides and carbon monoxide to improve the spatial and temporal disaggregation of total CO2 into its fossil and biospheric fractions.
AS31-A014
| Invited
CarbonWatch-Urban: Granular CO2 Emissions Information for Every Town and City in New Zealand
Jocelyn TURNBULL1#+, Sara MIKALOFF FLETCHER2, Gordon BRAILSFORD2, Sally GRAY2, Rowena MOSS2, Stijn NAUS2, Lucy HUTYRA3, Kevin GURNEY4
1GNS Science, 2National Institute of Water and Atmospheric Research, 3Boston University, 4Northern Arizona University
Urban areas are responsible for the vast majority of fossil fuel CO2 emissions, thus mitigation actions are often taken at the city level. Detailed information about urban emissions and offsetting potential is needed to guide mitigation actions and to evaluate the efficacy of these actions. CarbonWatch-Urban is a multi-tiered approach to provide fine-scale CO2 emissions and sink information for all of New Zealand’s urban areas. First, we have established a high resolution (street segments and buildings, hourly) bottom-up inventory of Auckland's fossil fuel CO2 emissions from a variety of data sources and optimised the UrbanVPRM land surface model to estimate the biogenic CO2 budget of the Auckland region. We use in situ and flask observations of CO2, 14CO2, CO, COS and black carbon to separate and quantify the various components of Auckland’s CO2 flux, and an atmospheric inversion framework to rigorously validate and improve the bottom-up flux estimates. Yet the majority of New Zealand’s urban CO2 emissions are from smaller towns and cities, and simply extending the Auckland observation framework across the country is not feasible due to topography, urban form and cost constraints. Therefore use Auckland experience to expand the bottom-up flux modelling framework nationally, applying the improvements identified in Auckland. We use a less rigorous but realistic campaign-style flask observations system from a range of towns and cities spanning New Zealand’s climate, topography and urban from to validate and improve the flux models and provide the best estimates of New Zealand’s urban emissions, with granular information in space and time.
AS31-A006
Characterizing Tokyo’s Methane Sources from Vehicle-based Measurements
Taku UMEZAWA1,2#, Yukio TERAO1+, Masahito UEYAMA3
1National Institute for Environmental Studies, 2Tohoku University, 3Osaka Metropolitan University
Cities are the major source of greenhouse gases and thus target for emission reduction. Recent reports on atmospheric measurements of methane and its fluxes in urban areas suggest that substantial emissions occur in many cities, and emission inventories are highly uncertain for urban sources such as energy and waste sectors. Tokyo is Japan’s and world’s largest megacity and urgently needs investigation of accurate greenhouse gas emissions to support mitigation actions. We developed a vehicle-based mobile measurement system with a mid-infrared absorption spectrometer for methane and ethane (MIRA ULTRA, Aeris Technologies). Ethane helps us identify leakage of natural gas since its representative methane/ethane composition is known. In September–October 2023, we conducted 3-week mobile measurements in Tokyo and surrounding areas with total driving distance of about 2400 km. About 1000 points with high methane elevations were identified, and ethane/methane enhancement ratio calculated for individual points were used to group them into biogenic, fossil fuel and combustion sources. The ethane-methane classification indicated that major contributions to Tokyo’s methane emissions come from biogenic and fossil fuel sources, while combustion sources are relatively minor. Strong biogenic methane peaks were found around landfill sites and wastewater treatment plants, and fossil fuel peaks were found frequently in residential and industry areas. Presentation will include discussion on emission magnitudes.
AS31-A001
On the Large Variation in Atmospheric CO2 Concentration at Shangdianzi GAW Station During Two Dust Storm Events in March 2021
Xiaolan LI1#+, Weijun QUAN2, Xiao-Ming HU3
1China Meteorological Administration, 2Environmental meteorology Forecast Center of Beijing-Tianjin-Hebei, 3The University of Oklahoma
Dust storms have large impacts on air quality and meteorological elements; however, their relationships with atmospheric greenhouse gases (e.g., CO2) and radiation components remain uncertain. In this study, the co-variation of dust and CO2 concentrations and its possible influencing mechanism are examined using observations at the Shangdianzi (SDZ) regional Global Atmosphere Watch (GAW) station along with simulations of the Vegetation Photosynthesis and Respiration Model coupled with the Weather Research and Forecasting model (WRF-VPRM), during two dust storm events on March 15 and 28, 2021. During these events, hourly CO2 concentrations decreased by 40–50 ppm at SDZ while dust concentrations increased to 1240.6 and 712.4 µg m−3. The elevated dust increased diffusive shortwave irradiance by 50–60% and decreased direct shortwave irradiance by ~60% along with clouds. The dust events were attributed to the passages of two cold front systems over northern China. At SDZ, during the frontal passages, wind speed increased by 3–6 m s−1 and relative humidity decreased by 50–60%. The CO2 variations associated with the frontal systems were captured by the WRF-VPRM despite the overestimated surface CO2 level at SDZ. Biogenic CO2 flux plays an indistinctive role on the large CO2 variation at SDZ as it is weak during the non-growing season. The cold fronts pushed polluted air southeastward over the North China Plain and replaced it with low-CO2 air from Northwest China, leading to the declines in CO2. These findings demonstrate that meso-scale synoptic conditions significantly affect the regional transport and dispersion of CO2, which can influence the prediction of terrestrial carbon balance on a regional scale.
AS31-A009
Atmospheric CO2 Concentrations and Contributions from Biogenic and Anthropogenic Sources in the Pearl River Delta Region of China
Boru MAI#+
China Meteorological Administration
The dynamics of atmospheric CO2 concentrations in urban agglomerations have been a topic of interest in research on global climate change, yet there remain significant uncertainties within the estimates of CO2 contributions from biogenic and anthropogenic sources. In this study, the Weather Research and Forecasting model coupled with the Vegetation Photosynthetic Respiration Model (WRF-VPRM) was implemented with local VPRM parameters to simulate the atmospheric CO2 concentration in the Pearl River Delta (PRD) region of China during 2019–2021. The results show that (1) WRF-VPRM accurately simulates the distribution of the atmospheric CO2 concentration in the PRD region from 27-km grids to 4-km grids, with the hourly average bias of 4-km grids being −1.27 ppm. The accuracy of CO2 simulations is significantly impacted by solar radiation, while ocean winds increase the CO2 simulation bias in coastal areas. The increase in motor carbon emissions during evening rush hours also affects the CO2 simulation accuracy in urban areas. (2) In spring, summer, autumn, and winter, the average CO2 concentrations in the PRD region were 431.56±3.01 ppm, 427.55±3.51 ppm, 426.20±3.89 ppm, and 434.27±3.82 ppm, respectively. Anthropogenic emissions were the main factor, accounting for 20.59% of the total CO2 concentration in the region; by contrast, the contribution from vegetation emissions was only 1.57%. (3) High CO2 concentration centers (CO2 exceed 436 ppm) occur throughout the year at the border of Yunfu and Zhaoqing, northeast Qingyuan, and southern Huizhou. CO2 concentrations were below 426 ppm in the region around the Pearl River Estuary in summer and fall.
Session Chair(s): Jianping LI, Ocean University of China, Huang-Hsiung HSU, Academia Sinica
AS04-A027
| Invited
Changing Characteristics of Extreme Precipitation and Temperature Across Northeast India and Bangladesh
Rajib MAITY#+, Subharthi SARKAR, Ashesh Rudra PAUL
Indian Institute of Technology Kharagpur
Northeast part of India including West Bengal (henceforth referred as NEI) and Bangladesh is facing the impacts of changing climate. A recent study revealed some interesting and crucial findings using a multi-model multi-scenario analysis on the complexity of future precipitation and temperature dynamics across NEI, including Bangladesh (Paul and Maity, 2023). Under the SSP585 scenario, the Simple Daily Intensity Index (SDII) is projected to increase by 2.4 mm/day over the last three decades of the present century (2071-2100) compared to the base value of 14.4 mm/day over 1981-2014. The analysis also reports significant changes with respect to Consecutive Dry Days (CDD), Consecutive Wet Days (CWD), Number of Summer Days Index (SU) and Warm Spell Days Index (WSDI). The maximum and minimum temperatures are expected to increase by 4.0˚C and 5.5˚C, respectively, with a higher rate of rise in minimum temperature, leading to a decrease in the Diurnal Temperature Range (DTR) by up to 1.5˚C. Other studies involving the entire Indian mainland established the most of the NEI as ‘Climate change Hotspots’ (Sarkar and Maity, 2024), with particularly pronounced exposure in multi-attributed precipitation and temperature characteristics over future than rest of the country. Further analysis including two crucial socioeconomic factors, namely, population density and Human Development Index (HDI) reveals most part of NEI to be ‘vulnerable’ to changing climate as well (Sarkar and Maity, 2024). We expect these findings to be helpful in climate-informed planning and management of multiple sectors such as, water resources, agriculture, infrastructure etc. across NEI and Bangladesh.
AS04-A004
Exploring Temperature Sensitivity and Changes in Snow Persistency in High-mountain Asia
Manuel Tobias BLAU1,2#+, Pratik KAD3,4, Jenny V. TURTON5, Kyung-Ja HA2
1IBS Center for Climate Physics, 2Pusan National University, 3NORCE Norwegian Research Center, 4Bjerknes Centre of Climate Research, 5Arctic Frontiers AS
Snow-covered regions span over large portions of the Northern Hemisphere and polar regions. Also, alpine regions in high mountain ranges are often covered by snow. The snow cover of High-Mountain Asia (HMA) from the Hindu Kush Himalayan is undergoing an unprecedented and mostly irreversible state due to global warming. These changes pose a significant threat to two billion people and are exacerbating the risk of species extinction. Recent results indicate an overall decline in snow cover over the HMA. Our preliminary findings highlight the declining trend of snow persistence. Using current reanalysis data, satellite observations, and state-of-the-are climate simulations for the climate model intercomparison project phase 6 (CMIP6), we derived a significant decline in mountain snow persistence and its sensitivity to temperature changes. In our analysis, we identified global warming as the predominant factor contributing to the loss of snow, as opposed to regional warming. We investigated the stochastic link between the variability of the South Asian monsoon circulation and the snow cover in the HMA region. The results indicate a strong sensitivity of snow persistency and depth to regional and global warming and to the changes in accumulation rates determined by the differing strength of the monsoon systems. Further, we highlight the dependence of the results on the spatial resolution of the dataset.
AS04-A008
Impact of Tibetan Plateau Spring Snow on the Summer Heat Wave Frequency Over the Indochina Peninsula
Xiaojing JIA#+
Zhejiang University
In this work, we investigated the impact of the interannual variation in Tibetan Plateau snow cover (TPSC) on the summer heat wave frequency (HWF) over the Indochina Peninsula (ICP) (HWF_ICP) for 1981-2020. This study shows that the spring TPSC variation over the central TP is positively correlated with the summer HWF_ICP and can explain up to 30% of the summer HWF_ICP variance. Analysis of the apparent heat source shows that more-than-normal spring snow cover over the central TP has a cooling effect on the above atmosphere, which induces negative geopotential height anomalies in the upper troposphere. The anomalous spring TPSC and its cooling effect can persist until summer. In summer, the TPSC-associated low anomalies propagate eastward to the East Asia-Japan Sea area. The anomalous westerly winds along the south flank of these low anomalies strengthen the climatological westerly jet. Changes in the westerlies are accompanied by anomalous ascending and descending air motion north and south of 30°N over the coast of East Asia and the western Pacific. The anomalous descending air motion south of 30°N causes an enhanced subtropical high, less cloud cover, and more downward solar radiation, which are favorable conditions for a greater occurrence of heat waves over the ICP. The results of current study may provide useful information for improving the seasonal forecast skill of the summer HWF_ICP variation.
AS04-A061
The Influence of Snow Cover Over the Tibetan Plateau on Surrounding and Remote Regions' Climate
Zhibiao WANG1#+, Renguang WU2
1Chinese Academy of Sciences, 2Zhejiang University
The influence of winter-spring eastern Tibetan Plateau snow anomalies on the East Asian summer monsoon has been the focus of previous studies. The present study documents the impacts of boreal summer western and southern Tibetan Plateau snow cover anomalies on summer rainfall over East Asia and the relationship between the eastern Tibetan Plateau snow cover and the North American air temperature in spring. Analysis shows that more snow cover in the western and southern Tibetan Plateau induces anomalous cooling in the overlying atmospheric column. The induced atmospheric circulation changes are different corresponding to more snow cover in the western and southern Tibetan Plateau. The atmospheric circulation changes accompanying the western Plateau snow cover anomalies are more obvious over the midlatitude Asia, whereas those corresponding to the southern Plateau snow cover anomalies are more prominent over the tropics. As such, the western and southern Tibetan Plateau snow cover anomalies influence the East Asian summer circulation and precipitation through different pathways. Moreover, a stable relationship is identified between the eastern Tibetan Plateau snow cover and the North American SAT in spring before the mid-2000s. Positive snow-cover anomalies over the eastern Tibetan Plateau induce cooling in the local atmospheric column. The atmospheric cooling stimulates a large-scale atmospheric wave pattern at the upper level that extends northeastward from the eastern Tibetan Plateau via northeast Asia and the North Pacific to North America. An anomalous high forms over North America, accompanied by anomalous descent. In the northwestern part, the horizontal advection by anomalous southerly winds along the west flank of anomalous anticyclone induces SAT increase. In the central part, the enhanced surface sensible heat flux following anomalous descent-induced downward shortwave radiation increase leads to SAT increase.
AS04-A052
The East-asian Spring to Summer Monsoon Weather Calendar Constructed by Self-organizing Maps of Atmospheric Low-level Winds and Applied to Taiwan Meiyu and Tropical Cyclone Analysis
Sheng-Fong HUANG#+, Mong-Ming LU
National Taiwan University
East Asian monsoon (EAM) exists substantial changes during April-July. As part of the EAM, the first distinct rainy period in Taiwan known as Meiyu occurs from pentad 27 (May 11-15) to pentad 36 (June 25-29). It makes up about one third of the annual total rainfall. The Meiyu is sensitive to a narrow rainband oriented in southwest-northeast direction from northeast Vietnam through Taiwan to Okinawa. In this study we aim to document the relationship between Taiwan Meiyu and the progression of the daily weather types and tropical cyclones (TC) in the EAM region (0°-37.5°N, 90°E-140°E). The progression is characterized by a monsoon weather calendar built on the wind patterns of 44 years (1979-2022) of April-July daily 850-hPa winds using the self-organizing map (SOM) method. The daily wind patterns are classified into 9 units of a 3×3 SOM. The occurrence frequency of each unit on the pentad basis suggests that the period of April-July can be separated to late spring (pentad 19-24), transition (pentad 25-33), and early summer (pentad 34-42) monsoon evolution stages. The monsoon weather calendar reveals the relationship between Taiwan Meiyu, TC and EAM. After separating the years to the groups with and without TCs, we found that over the SCS and the southern Philippine Sea the westerly flow is stronger and rainfall amount is larger during the years with TCs, whereas stronger northeasterly wind and less rainfall are observed over Taiwan. The results suggest that the monsoon weather calendar can be useful for identifying the unusual years of which the progression of the daily weather types is distinctly different from others and the extreme/rare events are more likely to occur.
AS04-A045
Spatial Heterogeneity of Summer Rainfall Trends Over the Tibetan Plateau Contributed by Different Rainfall Intensities
Meirong WANG1#+, Jun WANG2, Xiuping YAO3
1Nanjing University of Information Science & Technology, 2Nanjing University, 3China Meteorological Administration Training Centre
Recent years have witnessed contrasting trends in summer total rainfall (STR) over the Tibetan Plateau (TP), with an increase in the northern and a decrease in the southern TP. This study identifies four significant centers of rainfall trends: eastern TP (“region A”), Qiangtang Plateau (“B”), Qaidam Basin (“C”), and the northern foothills of the Himalayas (“D”). Heavy rainfall dominates STR trends in regions A and D, accounting for 55.6% and 52.0%, respectively. In region B, moderate and light rainfall contribute almost equally, accounting for 37.3% and 44.8% of the STR trend, respectively. Region C is primarily influenced by light rainfall, explaining 71.2% of the STR trend. Notably, the contributions of different rainfall intensities to STR in each region vary annually, with region A experiencing more heavy rainfall, region B having moderate dominance but less light rainfall, and region C and D showing reduced and increased light rainfall contributions, respectively. Mechanistically, the strengthening of the upper-level westerly jet and the South Asian High, coupled with changes in moisture transport and convective available potential energy, collectively cause variations in rainfall intensity, characterizing the spatial heterogeneity in STR in the TP.
AS04-A065
Monsoon Break Over the South China Sea During Summer: Statistical Features and Associated Atmospheric Anomalies
Minghao BI1+, Ke XU2#, Riyu LU1
1Chinese Academy of Sciences, 2Institute of Atmospheric Physics, Chinese Academy of Sciences
This study identifies break events of the South China Sea (SCS) summer monsoon (SCSSM) based on 42 years of data from 1979 to 2020, and investigates their statistical characteristics and associated atmospheric anomalies. A total of 214 break events are identified by examining the convection evolution during each monsoon season. It is found that most events occur between June and September and show a roughly even distribution. Short-lived events (3–7 days) are more frequent, accounting for about two thirds of total events, with the residual one third for long-lived events (8–24 days). The SCSSM break is featured by drastic variations in various atmospheric variables. Particularly, the convection and precipitation change from anomalous enhancement in adjoining periods to a substantial suppression during the break, with the differences being more than 60 W m−2 for outgoing longwave radiation (OLR) and 10 mm d−1 for precipitation. This convection/precipitation suppression is accompanied by an anomalous anticyclone in the lower troposphere, corresponding to a remarkable westward retreat of the monsoon trough from the Philippine Sea to the Indochina Peninsula, which reduces the transportation of water vapor into the SCS. Besides, the pseudo-equivalent potential temperature declines sharply, mainly attributable to the local specific humidity reduction caused by downward dry advection. Furthermore, it is found that the suppressed convection and anomalous anticyclone responsible for the monsoon break form near the equatorial western Pacific and then propagate northwestward to the SCS.
AS04-A024
Characteristics of the Precipitating System Caused Nocturnal Rainfall Over the Southern Meghalaya Plateau, Northeast India
Fumie MURATA1#+, Toru TERAO2, Hiambok J. SYIEMLIEH3, Laitpharlang CAJEE3, Shyam Sundar KUNDU4
1Kochi University, 2Kagawa University, 3North-Eastern Hill University, 4North Eastern Space Applications Centre
Diurnal variation of precipitation is distinct over the tropical region. In the Indian monsoon region, nocturnal rainfall is dominant over the upslope area of the Himalayas and Megalayas, where climatologically heavy rainfalls occur. There are several studies which investigated the mechanism of the nocturnal rainfall from observations and numerical modeling. However, investigations using in-situ weather radars have not been conducted. This study conducts a case study of a nocturnal rainfall on 20-22 July 2019, using the ISRO Cherrapunji Doppler radar, which was continuously operated in every 15 min. The radar reflectivity was corrected by the GPM DPR and in-situ disdrometer. The analysis period was in an active spell, and southwesterly wind was dominant. The convective activity became active in the south of the plateau in the nighttime and a small rainband with less than several tens kilometers was formed, approached toward the plateau.
Session Chair(s): Xiquan DONG, The University of Arizona, Chuanfeng ZHAO, Peking University
AS66-A022
| Invited
Libera and Continuity of the Earth Radiation Budget Climate Data Record
Peter PILEWSKIE1#+, Maria HAKUBA2
1University of Colorado Boulder, 2Jet Propulsion Laboratory
The Libera Mission, named for the daughter of Ceres in Roman mythology, will provide continuity of the Clouds and the Earth’s Radiant Energy System (CERES) Earth radiation budget (ERB) observations from space. Libera’s attributes enable a seamless extension of the ERB climate data record. Libera will acquire integrated radiance over the CERES FM6-heritage broad spectral bands in the shortwave (0.3 to 5 μm), longwave (5 to 50 μm) and total (0.3 to beyond 100 μm) and adds a split-shortwave band (0.7 to 5 μm) to provide deeper insight into shortwave energy deposition. The Libera science objectives associated with continuity and extension of the ERB data record are to identify and quantify processes responsible for ERB variability on various times scales. Key to our understanding of outgoing shortwave radiation is the radiative effects of clouds aerosols. Libera’s stewardship of the ERB record begins in the latter part of this decade, at an important juncture in the monitoring of climate change trends. The Libera split-shortwave channel will provide additional information to help quantify shortwave cloud and aerosol effects. This talk will examine our latest understanding of radiative perturbations due to clouds and aerosols and the expected contributions and advances from the Libera mission.
AS66-A019
Global Clear-sky Downwelling Shortwave Flux Using CCCma and MODTRAN6 Radiative Transfer Models
Baike XI1#+, Xiquan DONG1, Xiang ZHONG1, Jordann BRENDECKE1, Jiangnan LI2, Howard BARKER2
1The University of Arizona, 2Environment and Climate Change Canada
Challenges persist in providing accurate estimates of Earth’s surface shortwave (SW) radiation budget at the global scale. This is partly because Radiation Transfer Models (RTMs) are needed to determine surface fluxes. In this study, clear-sky total, direct, and diffuse SW fluxes at the surface were calculated by two RTMs: the computationally taxing high-spectral resolution MODTRAN6.0.2.5 (M6.0); and a computationally efficient low-spectral resolution correlated k-distribution (CKD) (Li and Barker 2005). Both RTMs used the same inputs, which includes profiles of state variables, aerosol properties, and surface albedos. The computed SW fluxes from these RTMs were compared to the NASA CERES SYN1deg product that was computed by NASA Langley’s modified broadband Fu-Liou RTM, which is widely used to study Earth’s radiation budget. Initial comparisons between three surface SW fluxes are encouraging: global annual means are 246.5 for M6.0, 245.4 for CKD, and 242.3 Wm-2 for SYN1. While regional differences can be large, most are less than CERES’s estimated uncertainty for monthly-mean surface SW irradiance of ~6 W m-2. Sensitivities of clear-sky SW/μ0 fluxes, where μ0 is cosine of solar zenith angle, to precipitable water vapor (i.e., clear-sky water vapor radiative kernel) are about -0.7 W m-2/(kg m-2) over oceans from both M6.0 and CERES SYN1 products (Zhong et al. 2024). To quantitatively estimate their SW flux uncertainties, surface observations from seven sites in different climatic regions (polar regions, oceans, lands, desert) were used (see Brendecke et al. 2024). Computed SW fluxes from M6.0 and CKD are summarized in Table 1 (without aerosol), and three RTMs calculations with aerosols against the surface observations are listed in Table 2. Mean difference between two RTMs in Table 1 is 0.6 Wm-2, whereas their differences in Table 2 are 1.9 and 3.8 Wm-2 compared to surface observations.
AS66-A008
Aerosol-cloud-radiation Interactions in Determining Multi-decadal Trends of Solar Radiation Reaching the Surface
Mian CHIN1#+, Huisheng BIAN2, Martin WILD3, Donifan BARAHONA1, Hongbin YU1, Yun QIAN4, Anton DARMENOV1, Paul STACKHOUSE, JR.5, Norman LOEB5, Rachel PINKER6, Yuanchong ZHANG7
1NASA Goddard Space Flight Center, 2University of Maryland, Baltimore County, 3ETH Zurich, 4Pacific Northwest National Laboratory, 5NASA Langley Research Center, 6University of Maryland, College Park, 7Columbia University
Incoming solar radiation drives the Earth’s climate system. Long-term surface observations of solar radiation reaching the surface have shown decreasing or increasing trends in different regions of the world in the past several decades, indicating the change of atmospheric components that reflect and/or absorb the solar radiation. This study investigates the roles of aerosols and clouds play in determining the multi-decadal surface radiation trends through a series of model simulations with the NASA GEOS model and analysis of ground-based observations and satellite-derived data products. We will 1) assess the effects of climate variability on trends of cloud cover and aerosol amount, 2) estimate the effects of aerosols on cloud variations and trends through aerosol-cloud-radiation interactions, and 3) identify the roles of aerosol, cloud, and climate change in multi-decadal trends of solar radiation reaching the surface in different regions of the world.
AS66-A013
Impacts of Atmospheric Environment on Arctic Surface Radiation Balance by Changing Cloud Properties
Chuanfeng ZHAO1#+, Yan XIA2, Haotian ZHANG2
1Peking University, 2Beijing Normal University
Atmospheric environmental variables including the aerosols, the stratospheric ozone and large scale atmospheric circulations, can modify the surface radiation balance and then affect Arctic climate by changing cloud properties. Using observation data, we found that aerosols from mid-latitude via long-range transport can change the cloud properties by decreasing cloud droplet effective radius and increasing cloud liquid water path, particularly in winter. Correspondingly, aerosols from mid-latitude enhance cloud thermal emissivity, contributing to Arctic warming by 8-10 W/m2 in winter. Using reanalysis meteorology data, we further found that depletion of stratospheric ozone has a significant contribution to the Siberian warming occurred in Spring 2020. A good correlation is found between the surface warming in Siberian region and stratospheric ozone depletion. Further analysis shows that the depletion of ozone depletion increases the upper troposphere air instability, resulting in a significant increase of upper level clouds, further causing surface warming. Also using reanalysis data, we found the significance of North Atlantic Oscillation (NAO) on the surface radiation balance over Greenland ice sheet (GrIS) by modulating the spatial distribution of clouds. It shows that the spatial and temporal variations in clouds in different phases over the GrIS are closely related to the NAO, and the response of clouds to changes in the atmospheric circulation field during the NAO varies in different regions of the GrIS. Shortly, this study provides the potential warming contribution in the Arctic by modulating cloud properties from three environmental factors, aerosols, depletion of stratospheric ozone, and NAO.
AS66-A018
Distinctive Aerosol-cloud-precipitation Interactions in Marine Boundary Layer Clouds from the ACE-ENA and SOCRATES Aircraft Field Campaigns
Xiquan DONG#+, Baike XI, Xiaojian ZHENG
The University of Arizona
The aerosol-cloud-precipitating interaction within the cloud-topped Marine Boundary Layer (MBL), are being examined using aircraft in-situ measurements from Aerosol and Cloud Experiments in the Eastern North Atlantic (ACE-ENA) and Southern Ocean Clouds Radiation Aerosol Transport Experimental Study (SOCRATES) field campaigns. SOCRATES clouds have a larger number of smaller cloud droplets compared to ACE-ENA summertime and wintertime clouds. The ACE-ENA clouds, especially in wintertime, exhibit pronounced drizzle formation and growth, attributed to the strong in-cloud turbulence that enhances the collision-coalescence process. Furthermore, the Aerosol-Cloud Interaction (ACI) indices from the two aircraft field campaigns suggest distinct sensitivities. The aerosols during ACE-ENA winter are more likely to be activated into cloud droplets due to more larger aerosols and strong vertical turbulence. The enriched aerosol loading during SOCRATES generally leads to smaller cloud droplets competing for available water vapor and exhibiting a stronger ACI. The ACI calculated near the cloud base was noticeably larger than the layer-mean and near-cloud-top, owing to the closer connection between the cloud layer and sub-cloud aerosols. Notably, the sensitivities of cloud base precipitating rates to cloud-droplet number concentrations are more pronounced during the ACE-ENA than during the SOCRATES campaigns. The in-cloud drizzle evolutions significantly alter sub-cloud cloud condensation nuclei (CCN) budgets through the coalescence-scavenging effect, and in turn, impact the ACI assessments. The results of this study can enhance the understanding and aid in future model simulation and assessment of the aerosol-cloud interaction. From this talk, we want to tentatively answer the following three questions: What are the characteristics of MBL aerosol and clouds properties, and their similarities and differences over these regions? What are the cloud microphysical responses to the sub- and above-cloud aerosols/CCN (ACIs) To what extent the drizzle drops influence the sub-cloud aerosols/CCN (ACPIs)?.
AS66-A020
Variation of Cloud Properties with Dust and Anthropogenic Aerosols in Northwestern Pacific
Keying LI1+, Tianyi FAN1#, Chuanfeng ZHAO2, Xin YANG1
1Beijing Normal University, 2Peking University
Dust and anthropogenic aerosols from East Asia are transported to the Northwestern Pacific (NWP) by westerlies and active extratropical cyclones, modifying clouds of different types and affecting the energy budget of Earth. These aerosols have diverse effects on cloud properties and radiation forcing due to their distinct optical and hygroscopicity properties. In this study, we investigate the variation in the cloud properties of different cloud types with dust and anthropogenic aerosols under specific weather patterns. We classify the clouds into regimes based on the "K-means" clustering algorithm utilizing the Himawari-8 satellite cloud products. Weather patterns are classified by the principal component analysis in T-mode (T-PCA) to identify the meteorological factors that favor the formation of the prevailing cloud regime under the weather systems. Events dominated by the two types of aerosols are identified based on the largest dust and anthropogenic AOD anomalies, respectively. Our analysis suggests that the sensitivities of cloud properties to AOD depend on aerosol types. Considering the influence of meteorology on the cloud processes, the relative contribution of aerosols and meteorological factors are assessed using multiple linear regression. This study helps to improve our understanding of the variation of clouds with different types of aerosols in NWP.
Session Chair(s): Joowan KIM, Kongju National University
AS79-A008
Sub-seasonal Variability of Asian Summer Monsoon Transport of Aerosols and CO to the UTLS in the Context of Recent Aircraft Observations in the Asia
Mian CHIN1#+, Huisheng BIAN2, Gao CHEN3, Peter COLARCO4, Paul A. NEWMAN1
1NASA Goddard Space Flight Center, 2University of Maryland, Baltimore County, 3NASA Langley Research Center, 4National Aeronautics and Space Administration
We present our study on the sub-seasonal variability of UTLS aerosols and CO that is a result of the variability induced by the sub-seasonal variability of the Asian summer monsoon (ASM) dynamics. We use the NASA global model GEOS simulations that incorporates emissions from anthropogenic, biomass burning, volcanic, and other natural sources to simulate CO, aerosols and related gases with model experiments separating source types (anthropogenic, biomass burning, volcanic) and source regions (East Asia, South Asia). Using the model results that are evaluated with observations from recent aircraft measurements (StratoClim, summer 2017 and ACCLIP, summer 2022) in the UTLS over the Asian summer monsoon regions, we will discuss (1) the sub-seasonal variability of transport pathways of surface-generated pollutants to reach UTLS, and (2) sub-seasonal variability of aerosol composition that is determined by the variability of source type and source regions, and (3) similarities and differences of ASM dynamics between two summers of 2017 (StratoClim) and 2022 (ACCLIP) in the context of ASM interannual variability.
AS79-A004
Aerosol Size Distribution in the Troposphere Over the Tibetan Plateau
Dan LI#+, Janchun BIAN, Zhixuan BAI
Chinese Academy of Sciences
The Tibetan plateau around by the Taklimakan and Gobi deserts in the West and North, through have limited human activities. The aerosol vertical distribution play a key role in radiative balance. In-situ measurements are needed to investigate the size distribution of the particles in the troposphere. Aerosol size (0.13-3μm) distributions and concentration were measured by balloon-borne sensors (POPS) launched Kunming (25.01°N, 102.65°E) since 2015. However, balloons payload with POPS were launched systematically every tow month from June 2020 to November 2023 in Lhasa (29.66°N, 91.14°E) or Golmud (36.48°N, 94.93°E) or Lijiang (100.22°E, 26.85°N) over the Tibetan Plateau. In total, 36 profiles will give a vertical distribution of particles from surface to the lower stratosphere (25 km) around the Tibetan Plateau. Concentration decreased for all particle sizes above the boundary layer where smallest particles increased in the Asian tropopause aerosol layer (ATAL) around the tropopause. Furthermore, volcano and dust storm have significant impact on aerosol size distribution around the tropopause.
AS79-A011
Possible Effects of Siberian Wildfire on Variation in Vertical Distribution of Hydrocarbons Over East-Asian UTLS During Asian Summer Monsoon
Donghee LEE1+, Ja-Ho KOO1#, Laura L. PAN2, Patrick SHEESE3, Kaley WALKER3
1Yonsei University, 2National Center for Atmospheric Research, 3University of Toronto
As many reported, the strength of Asian Summer Monsoon Anticyclone (ASMA) has increased recently. ASMA is one of the pivotal pathways of surface chemical species into upper troposphere and lower stratosphere (UTLS) over Northern Hemisphere. Also, the previous research on the linkage between intensity of ASMA and Siberian wildfire activity has been presented. Therefore, we examined the long-term variation of hydrocarbons in East Asian UTLS related to Siberian wildfire during Asian summer monsoon period. For this purpose, we used Atmospheric Chemistry Experiments (ACE)-FTS v4.1/4.2 to investigate vertical profiles of hydrocarbons (HCN, CO, C2H2, C2H6 etc.) in East Asia, and Moderate Resolution Imaging Spectroradiometer (MODIS) MOD14/MYD14 and MCD64A1 to analyze wildfire activity (Fire Count (FC) and Burned Area (BA)) in Siberia. As a result, we found the enhancement of hydrocarbons in summer (June to August) over UTLS (8-13km altitude). In addition, Siberian wildfire occurred mainly in the summer season. These enhancements of hydrocarbons in north China show the highest correlations with FC and BA in Siberia (R = ~ 0.5 to 0.6), meaning that Siberian wildfire might affect variability of hydrocarbons composition in UTLS. Additionally, we found that activity of Siberian wildfire has increased in conjunction with expanded ASMA area recently, investigated from Modern-Era Retrospective analysis for Research and Application version 2 (MERRA-2). As the ASMA expanded, we confirmed higher geopotential height, warmer temperature, arid weather in Siberia near surface. Furthermore, interesting point is that hydrocarbon concentration in UTLS has increased when ASMA intensified. However, we need to carefully evaluate increased hydrocarbon concentration related to expanded ASMA since the pattern of enhanced hydrocarbon concentration by latitude is different. This work was supported by Korea Environment Industry & Technology Institute (KEITI) through "Climate Change R&D Project for New Climate Regime", funded by Korea Ministry of Environment (MOE) (2022003560006).
AS79-A014
Vertical Ozone Profile Pattern in August, South Korea Based on the Ozonesonde Measurement
Ja-Ho KOO1#+, Joowan KIM2, Hyungyu KANG2, Sangjun KIM1, Seonggyun NA1, Sang Seo PARK3, Jin-Soo PARK4
1Yonsei University, 2Kongju National University, 3Ulsan National Institute of Science and Technology, 4National Institute of Environmental Research
In this study, we show preliminary results about the comparison of summertime (August) ozonesonde measurements from 2021 to 2023. Ozonesonde measurements were performed in both western (Anmyeon, Seosan, and Osan) and eastern (Pohang) region of Korean peninsula. First, we found that the annual variation of tropopause height. Ozone tropopause heights are higher in 2022 compared to those in 2021 and 2023. Interestingly, surface ozone at Anmyeon is lower and tropospheric convection is more intensified in 2022, implying that the tropospheric stability affects the extent of stratospheric intrusion to the troposphere, which seems associated with the enhancement of surface ozone. If we compare the ozone vertical profile between western and eastern region (i.e.,, Anmyeon vs. Pohang), free-tropospheric ozone level is higher but near-surface ozone level is lower in the east of Korean peninsula, indicating that the effect of stratospheric ozone intrusion is not much significant to the enhancement of near-surface ozone. For understanding this discrepancy, we need to consider the different pattern of air pollutant emission between the west and east of Korean peninsula; A number of power plants and industrial complex are located near the Anmyeon and Seosan). Based on these results so far, we can conclude that the intrusion of stratospheric ozone-rich air mass should be considered for assessing the high level of near-surface ozone in the region where the large emission and chemical processes of precursors happen. Additional further analyses are still necessary for better understanding.
AS79-A013
Analysis of Ozone Intrusion Events and Comparison with Chemical Reanalyses Using Daily Ozonesonde Measurements
Hyungyu KANG1#+, Subin OH2, Sanghyun AN1, Joowan KIM1, Ja-Ho KOO3, Sang Seo PARK4
1Kongju National University, 2National Institute of Meteorological Research, 3Yonsei University, 4Ulsan National Institute of Science and Technology
In order to understand the impact of the summer monsoon on ozone distribution over East Asia, 24 daily ozonesonde measurements were conducted at the Anmyeon site (36.54°E, 126.25°N), South Korea in August 2021. Electrochemical Concentration Cell (ECC) type ozonesonde was used for the ozone profiling from August 5 to 31, and it revealed an average Total Column Ozone (TCO) of 300 DU, consistent with regional climatology. Notably, TCO increased by approximately 17%, reaching 351 DU from August 17 to 19. This ozone concentration increase in the upper troposphere and lower stratosphere (UTLS) was linked to a Stratosphere-Troposphere Exchange (STE) event over the Korean Peninsula. The elevated ozone concentrations in the UTLS were examined through mid-tropospheric ozone observations, indicating a connection to the eastward expansion of the Asia summer monsoon anticyclone and subsequent anticyclonic wave breaking. Horizontal transportation also played a role in mid-tropospheric ozone concentration increases. Analysis of potential vorticity from reanalysis data revealed a coherent vertical structure with the intruded high ozone signature. Ozone data from chemistry reanalyses (MERRA-2 and CAMS) were compared to the ozonesonde measurements to assure their data quality. While TCO and stratospheric ozone are similar among the three datasets, the lower troposphere and surface values show significant spreads, revealing their uncertainty.
AS79-A003
Source Identification of High NOx Events Observed During ACCLIP
Shawn HONOMICHL1#+, Laura L. PAN1, David EDWARDS1, Sara MARTINEZ-ALONSO1, Warren SMITH1, Allessandro FRANCHIN1, Eleanor WAXMAN2, Andrew ROLLINS2
1National Center for Atmospheric Research, 2National Oceanic and Atmospheric Administration
Lightning is one of the leading sources of upper tropospheric (UT) active nitrogen (NOx) which is an important catalyst for the production of ozone and destruction of methane in the UT. Tropospheric ozone is an important greenhouse gas and radiative forcing calculations are particularly sensitive to changes in ozone concentrations in the cold UT. Lightning NOx has a significant impact on the tropospheric ozone budget and global climate, and understanding its sources is of interest. Currently, a large range exists in estimated global emission rates of lightning NOx (2-8 Tg/yr) from models and more needs to be done to reduce this uncertainty. The Asian Summer Monsoon (ASM) has been identified as a strong source region for UT NOx. During the ACCLIP field campaign, there were numerous instances where pockets of high NO2/NO concentrations were observed in the UT by instruments on the NCAR GV and NASA WB-57 research aircraft. Since deep convection in the ASM also pumps up NOx from boundary layer sources, separating the contributions from pollution and lightning are challenging. To tackle this issue, we explore an analysis of multiple datasets, taking advantage of the high spatial and temporal resolution GEMS satellite NO2 data. With the assistance of a Lagrangian trajectory model, we examine the relationship of high NOx data from airborne in situ measurements with the GEMS high NO2 hot spots and lightning data from the Earth Networks Global Lightning network. This exploratory study aims to identify and distinguish lightning and pollution sources for high NOx measurements and provide insight for general source identification.
AS79-A018
Monsoon Dynamics In Southern Luzon, Philippines: Raindrop Size Distribution and Soil Erosion Insights
Jefferson RAPISURA1#+, Decibel FAUSTINO-ESLAVA1, Wei-Yu CHANG2, Gabriel Angelo MAMARIL1, Bianca Maria Laureanna PEDREZUELA1, Maria Regina REGALADO1, Earvin Jon GUEVARRA1, Jenielyn PADRONES1, Loucel CUI1, Juan Miguel GUOTANA1, Rosemarie Laila AREGLADO1, Carla DIMALANTA3, Ben Jong-Dao JOU4
1University of the Philippines Los Baños, 2National Central University, 3University of the Philippines Diliman, 4National Taiwan University
This study investigates raindrop size distribution (RSD) characteristics during the Northeast Monsoon (NEM) and Southwest Monsoon (SWM) seasons in Southern Luzon, Philippines, from 2018-2023, using an OTT Parsivel disdrometer installed at the University of the Philippines Los Baños - National Agromet Station (UPLB-NAS) in Los Baños, Laguna (14.1647°N, 121.2501°E). The research reveals that smaller raindrops dominate in the NEM, while larger drops prevail in the SWM. Both monsoons exhibit predominantly stratiform rainfall, with convective rains in both SWM and NEM, displaying continental-like characteristics. Intensity-based analysis indicates a concentration of smaller drops during NEM and a higher occurrence of small drops in SWM during torrential events (> 30mm/hr). Larger drops (>3mm) are notably present in SWM across all intensity categories. Simultaneously, the study explores soil erosion processes during NEM and SWM, considering the region's susceptibility to heavy rainfall and erosion. Using the same disdrometer, the research established a relationship between rainfall intensity (R) and kinetic energy (KE). Kinetic energy expenditure (KEexp) and kinetic energy content (KEcon) expressions are introduced, exploring their relationships with R through linear, power, exponential, and logarithmic models. This integrated approach advances understanding of both precipitation dynamics and soil erosion during NEM and SWM in Southern Luzon. The implications extend to the development of accurate erosion prediction models and sustainable land management practices, enhancing the resilience of the region during these critical monsoon periods.
Session Chair(s): Jungho HWANG, Yonsei University, Fangxia SHEN, Beihang University
AS19-A003
| Invited
Inhalable Particle-bound Marine Biotoxins in a Coastal Atmosphere: Concentration Levels, Influencing Factors and Health Risks
Yan WU#+
Shandong University
Marine biotoxins can be aerosolized into the atmospheric environment and cause negative health effects through respiratory exposure and other pathways. Characterizing marine biotoxins (MBs) composition in coastal aerosol particles has become essential to tracking sources of atmospheric contaminants and assessing human inhalable exposure risks to air particles. Here, coastal aerosol particles were collected over an almost 3-year period for the analysis of eight representative MBs, including brevetoxin (BTX), okadaic acid (OA), pectenotoxin-2 (PTX-2), domoic acid (DA), tetrodotoxin (TTX), saxitoxin (STX), ciguatoxin (CTX) and ω-Conotoxin. Our data showed that the levels of inhalable airborne marine biotoxins (AMBs) varied greatly among the subcategories and over time. Both in daytime and nighttime, a predominance of coarse-mode AMB particles was found for all the target AMBs. Based on the experimental data, we speculate that an ambient AMB might have multiple sources/production pathways, which include air-sea aerosol production and direct generation and release from toxigenic microalgae/bacteria suspended in surface seawater or air, and different sources may make different contribution. Regardless of the subcategory, the highest deposition efficiency of an individual AMB was found in the head airway region, followed by the alveolar and tracheobronchial regions. This study provides new information about inhalable MBs in the coastal atmosphere.
AS19-A008
| Invited
Influence of Aerosol Acidity on Biological Components
Guangjie ZHENG#+
Tsinghua University
Aerosol Acidity largely regulates the atmospheric multiphase chemistry. In addition, recent studies have suggested the potential role of acidity on the biological components of particulate matter. Here, we investigated into this issue by simultaneous measurements of the chemical and biological components in Beijing, a megacity in China. Based on these measurements, the aerosol acidity can be estimated, and its potential influence on the biological components are investigated.
AS19-A002
| Invited
The Exometabolome of Culturable Microorganisms from an Urban Atmosphere
Wei HU#+, Rui JIN, Pingqing FU
Tianjin University
Atmospheric microorganisms are important components of bioaerosols and potentially impact terrestrial ecosystems and climate. The survival and metabolic activities of atmospheric microbes in suitable settlements may affect cloud chemistry and characteristics and functions of microbiomes in surface ecosystems. Therefore, the metabolic processes and characterization of metabolites occurring in atmospheric viable microorganisms settled suitable habitats remain highly explorable. This study used ultra-high resolution Fourier transform ion cyclotron resonance mass spectrometry (ESI-) to characterize the exo-metabolites of typical bacterial and fungal strains isolated from atmospheric particles at the molecular level, and the molecules were annotated using the KEGG database to investigate their metabolic processes. Microbial culture results showed that Proteobacteria, Firmicutes, and Actinobacteria dominated the culturable bacteria, while fungi were dominated by Ascomycota, with Aspergillus and Penicillium being the predominant genera. The molecular compositions of exo-metabolites from bacteria and fungi were characterized by distinct differences, with bacteria having a higher molecular diversity than fungi. Bacterial exo-metabolites were mainly composed of CHON and CHONS compounds, which accounted for over 90% of all detected compounds. While, fungal exo-metabolites were dominated by CHO and CHON compounds. Pantoea vagans produced more unsaturated hydrocarbons compounds containing amino or amide groups. The exo-metabolites (CHO compounds) of Talaromyces sp. were mainly CRAM-like compounds. The metabolite formulas were annotated and enriched using the KEGG database, revealing significant differences in central metabolic pathways between the different bacteria and fungi. Lipid metabolism was predominant in Pantoea vagans and Bacillus subtilis, while carbohydrate metabolism was the main pathway in Pseudomonas baetica and Bacillus toyonensis. The methane metabolism and lysine biosynthesis were the primary pathways in Aspergillus, and Talaromyces sp. specialized in aflatoxin biosynthesis. This study further illustrates that atmospheric microorganisms could have intense metabolic activities and provides a basis for evaluating their impacts on cloud chemistry and surface ecosystems after deposition.
AS19-A004
Dynamic Changes of Bacterial Aerosols in Haze and Sandstorm Events: Implications for Atmospheric Processes and Public Health
Fangxia SHEN#+, Jiahui MA, Yinghan TENG
Beihang University
The adverse health effects of air pollutants are closely related to their components. Bioaerosols, as an integral part of particles, play a crucial role. However, the dynamics of bioaerosols during pollution processes are not well understood. In this study, we investigated the dynamics of bacterial aerosols over a one-week period. During the sampling period, haze and sandstorm events occurred sequentially, with a transition period in between. We applied 16S rDNA and 16S rRNA sequencing techniques to explore the total bacterial community and the active bacteria, respectively. A distinct profile of bacterial aerosols was observed during the haze and the sandstorm event. The highest bacterial diversity was observed in the sandstorm samples, while the lowest was observed in the haze samples. Furthermore, the bacterial aerosols during the haze showed the greatest difference from those during the transition period when compared to the sandstorm samples. The total bacterial profile, as revealed by 16S rRNA sequencing results, was found to be distinct from the active bacterial communities in the sandstorm samples. Similarly, the underlying ecological drivers shaping the bacterial community structures showed different patterns. We found that the selective forces played a role in shaping the active bacterial communities in the sandstorm samples, as well as the total bacteria in the haze samples. A common feature during the haze and sandstorm episodes was the long residence time of bacteria in the air, indicating that the prolonged residence can lead to changes in the structure of airborne bacterial communities. Furthermore, the results indicate that several pathogens or opportunistic pathogens were more prevalent in the active bacterial communities of the sandstorm samples and the total bacteria in the haze samples, suggesting an increased health risk for humans, animals and even plants.
AS19-A001
Airborne Microbes in Five Important Regions of Chinese Traditional Distilled Liquor (Baijiu) Brewing: Regional and Seasonal Variations
Xue QIAO#+
Sichuan University
Baijiu is one of the six primary distilled spirits in the world. It is produced through the solid-state fermentation of grains in the open environment, so high-quality Baijiu brewing largely depends on terrior. Environmental microbes are one of the most important factors affecting the quality, quantity, and flavors of Baijiu. As atmosphere is a pool and transport pathway for microbes from the ambient environment to Baijiu brewing ecosystems, we explored the functional microbes of Baijiu brewing in five important regions. The regions fell into two topographical types, namely, plain and river-valley. In total, 41 functional microbes were identified rich (relative abundance >0.1%) in at least one of the regions, such as the fungi of Aspergillus, Candida, Cladosporium, Debaryomyces, Penicillium, Pichia, Rhizopus, Saccharomyces, and Wickerhamomyces) and the bacteria of Acetobacter, Bacillus, Clostridium, Enterobacter, Lactobacillus, Methanosarcina, Methanobacterium, Methanobrevibacter, and Pseudomonas. However, some functional bacteria (e.g., Clostridia, Gluconacetobacter, and Weissella) and fungi (e.g., Dekkera, Eurotium, Issatchenkia, Mucor, and Phoma) were not rich or were not detected in the atmosphere. Airborne microbiomes and the Phylogenetic Diversity (PD) index were significantly different between the main brewing season (winter) and the summer break in each region, except for the fungi in one region. In winter, airborne microbiomes were significantly different among almost all the regions. The relative abundance of bacterial fermentation function in each region increased from summer to winter. The relative abundances of fungal yeast function were higher in winter for the plain regions but were higher in summer for the river-valley regions. In sum, our results suggested that: (1) atmosphere was one but not the sole important source of functional microbes for Baijiu brewing and (2) microbiomes in different regions might be quite different but they could share some major functions related to Baijiu brewing.
AS19-A006
Metagenomic and Machine Learning Meta-analyses Characterize the Airborne Resistome Features and Their Hosts in China Mega-cites
Dong WU#+
East China Normal University
Urban ambient air contains a cocktail of antibiotic resistance genes (ARGs) emitted from various anthropogenic sites. However, what largely unknown is whether the airborne ARGs exhibit site-specificity or their pathogenic hosts persistently exist in the air. Here, by retrieving 1.2Tb metagenomic sequences (n = 136), we examined the airborne ARGs from hospitals, municipal wastewater treatment plants (WWTPs) and landfills, public transit centers, and urban sites located in seven China’s megacities. As validated by the multiple machine learning-based classification and optimization, ARGs’ site-specificity was found to be the most apparent in the hospital air, with featured resistances to clinical-used rifamycin and (glyco)peptides, whereas the more environmentally prevalent ARGs (e.g. resistance to sulfonamide and tetracycline) were identified being more specific to the non-clinical ambient air settings. Nearly all metagenome-assembled genomes (MAGs) that possessed the site-featured resistances were identified as pathogenic taxa, which occupied the upper-representative niches in all the neutrally distributed airborne microbial community (P < 0.01, m = 0.22 – 0.50, R2 = 0.41 – 0.86). These niche-favored putative-resistant pathogens highlighted the enduring antibiotic resistance hazards in the studied urban air. These findings are critical, albeit the least appreciated till our study, to gauge the airborne dimension of resistomes’ feature and fate in urban atmospheric environments.
AS19-A005
Release of Inhalable Particles and Viable Microbes to the Air During Packaging Peeling: Emission Profiles and Mechanisms
Yan WU#+
Shandong University
Packaging is necessary for preserving and delivering products and has significant impacts on human health and the environment. Particle matter (PM) may be released from packages and transferred to the air during a typical peeling process, but little is known about this package-to-air migration route of particles. Here, we investigated the emission profiles of total and biological particles, and the horizontal and vertical dispersion abilities and community structure of viable microbes released from packaging to the air by peeling. The results revealed that a lot of inhalable particles and viable microbes were released from package to the air in different migration directions, and this migration can be regulated by several factors including package material, effective peeling area, peeling speed and angles, as well as the characteristics of the migrant itself. Dispersal of package-borne viable microbes provides direct evidence that viable microbes, including pathogens, can survive the aerosolization caused by peeling and be transferred to air over different distances while remaining alive. Based on the experimental data and visual proof in movies, we speculate that nonbiological particles are package fibers fractured and released to air by the external peeling force exerted on the package and that microbe dispersal is attributed to surface-borne microbe suspension by vibration caused by the peeling force. This investigation provides new information that aerosolized particles can deliver package-borne substances and viable microbes from packaging to the ambient environment, motivating further studies to characterize the health effects of such aerosolized particles and the geographic migration of microbes via packaging.
AS19-A007
Microbial Ecology of Indoor Environments: The Significance of Shoe Dust in Shaping Indoor Microbiota
Fangxia SHEN#+, Mengzhen WANG, Chenji LI, Haidan LI
Beihang University
The role of indoor microbial exposure in human health has received increasing attention, given that individuals spend a significant portion of their time indoors. However, the factors influencing the microbial dynamics within inhabited environments are not yet comprehensively understood. This study aimed to investigate the bacterial dynamics in both the air and floor dust within occupied environments. Residences, dormitory and office environments were chosen. And the sampling was performed over a month during which window openings were infrequent. We employed amplicon sequencing techniques to characterize the indoor bacterial and fungal communities. Our findings revealed a diverse microbial community present in both the indoor air and floor dust samples. Specifically, the bacterial communities in the air exhibited greater similarity compared to those in the floor dust, whereas the fungal communities showed less discrepancy. Analysis using the Sloan Neutral Model (SNM) indicated that stochastic processes significantly influenced the structure of both the airborne and floor-borne bacterial communities. Furthermore, we investigated the microorganisms associated with the dust on the soles of shoes and compared them to the indoor microbiome. Interestingly, we observed a high degree of similarity between the shoe-related microorganisms and those found in the floor dust. This suggests that shoe-associated microorganisms could potentially be used to “re-wild” the indoor microbiota.
Session Chair(s): Jiwoo LEE, Lawrence Livermore National Laboratory, Yun-Young LEE, APEC Climate Center
AS39-A007
| Invited
Novel Approaches to Multi-resolution Evaluation of Climate Models: Hierarchical and Topological Data Analysis
Hugo LEE1#+, Alexander GOODMAN2, Jae Won CHOI3
1Jet Propulsion Laboratory, California Institute of Technology, 2California Institute of Technology, 3The University of Texas at Dallas
Earth System Models (ESMs) exhibit varying spatial resolutions, distinct from satellite observations. We aim to determine the optimal spatial resolution for new simulations that enhance our understanding of regional climate change. Traditional upscaling, by averaging high-resolution data onto coarser grids, loses critical details. Our novel toolkit for climate model evaluation counters this by integrating Hierarchical and Topological Data Analysis (HDA and TDA) into the Jet Propulsion Laboratory's system, enabling multi-resolution analysis. The multi-resolution evaluation separately characterizes spatial features of key climate model variables at coarse and fine scales, examining their resolution-dependent performance. We leverage HDA based on the Hierarchical Equal Area isoLatitude Pixelization (HEALPix) to evaluate temperature and humidity from climate models against state-of-the-art level 3 (L3) products from AIRS and CrIS. Unlike standard latitude-longitude representations, HEALPix grids consist of hierarchical and equal-area cells that can be efficiently upscaled. We have pioneered a prototype HDA for Earth science datasets, enabling dynamic spatial resolution changes and analysis of spatial variability at multiple scales, showcasing the value of high-resolution data. Topology, the study of shapes, and the emerging field of TDA, lie at the intersection of algebraic topology, machine learning, and statistics. Topological data can reveal latent structures and play a crucial role in understanding spatiotemporal patterns in datasets. Currently, no quantitative metric measures spatial pattern differences in Earth science datasets across spatial resolutions. We developed topological descriptors that summarize the spatial structures of climate models and satellite observations into persistence diagrams (PDs). Our TDA-based measure allows for systematic evaluation of multi-resolution data without the need for regridding. TDA's greatest advantage is its ability to quantitatively compare shape properties, which are invariant under continuous transformations, thus offering a significant step forward in climate model evaluation.
AS39-A010
NIMS/KMA Plans for Climate Change Projection Production and Utilization on CMIP7
ChuYong CHUNG1#+, Young-Hwa BYUN1, Hyun Min SUNG1, Jin-Uk KIM2, Sungbo SHIM1
1National Institute of Meteorological Sciences, 2Korea Meteorological Administration
The NIMS/KMA has been actively contributing to the CMIP program since CMIP3. NIMS participated in CMIP6 by utilizing the UKESM developed by the UK Met Office to generate future climate change scenarios for four distinct Shared Socio-economic Pathways. NIMS also employed the KMA Advanced Community Earth (K-ACE) model, a modified version of HadGEM2-AO developed through in-house research, to analyze global climate projections. Five different regional climate models were used for the regional climate simulations: HadGEM3-RA, RegCM4, CCLM, GRIMs, and WRF, organized under the CORDEX-EA program. Furthermore, for the South Korean area, NIMS produced 1km resolution climate change scenario data using the statistical downscaling technique, PRIDE. These projections played a pivotal role in contributing to the preparation of the Sixth Assessment Report by the IPCC and provided crucial foundational data for national climate change adaptation efforts. Currently, NIMS has initiated preparations for CMIP7 participation. In this program, K-ACE will be employed for producing global climate projections, having undergone improvements such as coupling with an ocean-biogeochemistry model, TOPAZ, and modifications to the cloud-aerosol process, among other enhancements. NIMS plans to use a reduced number of RCMs compared to the CMIP6 phase but intends to increase the ensemble members by combining physical processes. Currently under consideration as RCM candidates are WRF and WRF-ROMS. To comprehend the impact of climate change on local-scale heavy rain, a Convection Permitting Model can be employed. For the South Korean region, our objective is to produce more high-resolution, detailed climate scenarios through sensitivity experiments and reliability verification studies. This presentation aims to introduce KMA's Earth System Models, aligning with recent trends and developments outlined in CMIP7, and presenting the overall plans for the generation and utilization of global-regional-local climate projections in line with CMIP7.
AS39-A004
A Close Connection Between the Double-ITCZ Biases in Atmospheric and Coupled Climate Models at Monthly Time Scale
Baijun TIAN1,2#+, Ji-Won KIM1, Michael ZHAO3
1California Institute of Technology, 2University of California, Los Angeles, 3Rutgers University
The double-intertropical convergence zone (ITCZ) bias (DIB) is one of the most prominent and long-standing tropical precipitation biases in coupled global climate models and its root causes are still unclear. Here, we examine the relative contribution of the DIB in atmospheric models and the tropical sea surface temperature (SST) bias in coupled models to the DIB in coupled models at monthly instead of annual time scale using 59 paired atmospheric and coupled models from Coupled Model Intercomparison Project Phases 5/6. We find the DIBs in atmospheric and coupled models are positively correlated at each month although with no correlation at annual mean. In contrast, the high correlation between the DIB and tropical SST bias in coupled models at annual mean becomes much weaker at each month. These changes are particularly large during boreal winter (December-April) and summer (July-September). Our results suggest that both the DIB in atmospheric models and the tropical SST bias in coupled models play an important role in producing the DIB in coupled models.
AS39-A008
Evaluation of Seasonal-to-multiyear ENSO Prediction Skill in Multiple Decadal Prediction Systems
Jung CHOI#+, Seok-Woo SON
Seoul National University
Near-term climate predictions that incorporate seasonal-to-decadal time scales have recently received much attention from policymakers, stakeholders, and the climate science community in the context of climate risk management. The primary source of seasonal-to-multiyear prediction skill is the low-frequency variability of sea surface temperature, such as the El Niño–Southern Oscillation (ENSO). This study assesses the seasonal-to-multiyear prediction skill of ENSO using large ensembles of the Coupled Model Intercomparison Project phases 5 and 6 retrospective decadal predictions. By taking advantage of large ensemble sizes, the relative importance of the ensemble size versus the multi-model ensemble average in predicting multi-year ENSO index is evaluated. The results show that a multi-model ensemble reforecast successfully predicts ENSO over a year in advance. While its seasonal prediction skill in the following spring and summer is achieved by multi-model ensemble averaging of relatively smaller ensemble members, the multi-year prediction of winter ENSO needs a larger ensemble size. The methodology used in this study, which verifies the impact of the ensemble size and multi-model ensemble average, could be applied to any climate prediction studies and would improve our understanding of climate prediction. (Reference: Choi, J. and S.-W. Son, 2022, Seasonal-to-decadal prediction of El Niño–Southern Oscillation and Pacific Decadal Oscillation, npj Climate and Atmospheric Science 5:29; https://doi.org/10.1038/s41612-022-00251-9).
AS39-A005
Changes in Importance of Teleconnection Patterns Associated with Heat Wave in East Asia Under CMIP6 CDR-reversibility
Ji-Seon OH1+, Maeng-Ki KIM1#, Young-Hwa BYUN2, Hyun Min SUNG2
1Kongju National University, 2National Institute of Meteorological Sciences
In this study, we analyzed changes in teleconnection patterns associated with heat wave in East Asia using 1pctCO2 (ramp-up, 1%/yr increase) and 1pctCO2-cdr (ramp-down, 1%/yr decrease) simulations of the CMIP6 CDR-reversibility. To examine changes in teleconnection patterns associated with heat wave, Empirical Orthogonal Function (EOF) analysis was performed for the 250hPa geopotential height shifted by one year for every 30 years during the total period to show mode changes over time. The first mode represented a trend, showing consistent spatial patterns of increased and decreased geopotential height in response to change in CO2 concentration. The second mode exhibits a pattern similar to Circumglobal Teleconnection (CGT), gradually transitioning to a sub-mode during the ramp-up period with a weakening pattern. The pattern recovers during the ramp-down, but it remains in the sub-mode. The fourth mode is similar to the Arctic-Siberian Plain (ASP) pattern, which is responsible for the high-latitude East Asian heat wave pattern and is mainly in the sub-mode during the ramp-up but becomes the main mode after the transition to the ramp-down. These results suggest that the main mode of the teleconnection patterns that affect heat wave in East Asia may change as CO2 concentrations increase and decrease. [This work was funded by the Korea Meteorological Administration Research and Development Program under Grant (KMI2022-01311)].
AS39-A006
Consistent Inter-model Spread of Extratropical Westerly Jet Meridional Positions in CMIP6 Models Between the Northern and Southern Hemispheres in Boreal Winter
Li TANG#+, Riyu LU
Chinese Academy of Sciences
This study investigates the inter-model spread of extratropical westerly jets between 52 Coupled Model Intercomparison Project phase 6 (CMIP6) models in boreal winter. The results show that there is a substantial spread in latitude of upper-tropospheric westerly jet between models, characterized by large inter-model standard deviations to the poleward and equatorward of jet axis, although the multi-model ensemble mean (MME) of the models performs well in simulating meridional position of westerly jets. Furthermore, we detect the consistency of inter-model jet position spread between the northern and southern hemispheres, based on the inter-model empirical orthogonal function (EOF) decomposition and correlation of regional-averaged zonal winds. Specifically, the models that simulate the westerly jets poleward/equatorward than MME position in one hemisphere tend to also simulate the jets poleward/equatorward in the other hemisphere. Accordingly, we define a global jet spread index to depict the concurrence of jet shift in the two hemispheres. The results of regression analyses based on this index indicate that the models positioning the jets poleward than MME tend to simulate a wider Hadley Cell, a poleward-shifted Ferrel Cell in the southern hemisphere, and a wider intertropical convergence zone (ITCZ). Finally, the inter-model spread of ITCZ width is mainly determined by the spread of convective precipitations between the models, implying that different convection parameterization schemes may play a crucial role in inducing the inter-model spread of extratropical westerly jets and the concurrence of meridional jet shift in the two hemispheres.
AS39-A003
Intermodel Spread of the Southern Hemisphere Hadley Circulation Expansion in CMIP6
Ije HUR1#+, Changhyun YOO1, Sang-Wook YEH2, Young-Ha KIM3
1Ewha Womans University, 2Hanyang University, 3Seoul National University
The Hadley Circulation (HC) is a large-scale overturning circulation in the tropics that plays an important role in the Earth's energy and water cycles. Both observations and climate models show that the HC has been expanding poleward in recent decades, and this expansion is accelerating in future projections of the Coupled Model Intercomparison Project Phase 6 (CMIP6) models. However, the CMIP6 models differ widely in their projections of how much the HC will continue to expand, especially in the Southern Hemisphere (SH). In this study, we investigate the mechanisms by which the inter-model spread in SH HC expansion takes place. We use of the 22 CMIP6 model simulations with the historical and Shared Socio-economic Pathway (SSP) 5-8.5 scenarios. The HC is defined as the zonal mean mass streamfunction, and its edge is defined by the latitude where the sign of the streamfucntion at 500 hPa changes to positive in the subtropics. The intermodel spread in the HC trends is investigated by using the intermodel empirical orthogonal function (EOF) of the mass streamfunction trend patterns. We find that the first leading EOF (EOF1), which shows an anomaly at the HC edge, explains the 49.7% of the variance between the trend patterns and shows a significant correlation of 0.87 with the change of the HC extent. In the simulations with a relatively large HC expansion, the mean wind and temperature fields show an enhanced poleward jet shift and an increase in static stability in the subtropics. The difference in the mean fields results in intermodel spread and the eddy field. Analysis using the Eliassen-Kuo equation suggests that the meridional eddy heat flux dominantly explains the intermodel spread, while the eddy momentum flux contribution is about the half of the eddy heat flux.
AS39-A002
Introduction to the PCMDI Metrics Package (PMP), a Tool for Collective Earth System Model Evaluation
Jiwoo LEE1#+, Ana ORDONEZ1, Paul ULLRICH1, Peter GLECKLER1, Yann PLANTON2, Min-Seop AHN3, Bo DONG1, Kristin CHANG1
1Lawrence Livermore National Laboratory, 2Monash University, 3NASA Goddard Space Flight Center
The PCMDI Metrics Package (PMP) is an open-source Python-based framework that enables objective "quick-look" comparisons and benchmarking of Earth System Models (ESMs). The PMP’s connection to the Observations for Model Intercomparisons Project (obs4MIPs) enables considerations of multiple available observation-based reference datasets. The PMP has been used for routine and systematic evaluation of thousands of simulations from Coupled Model Intercomparison Projects (CMIPs), with atmospheric focus. Its results have been produced in the context of all model simulations contributed to CMIP6 and earlier CMIP phases, and we are making progress in preparing more seamless application of the tool and the result database for the next generation of CMIP (i.e., CMIP7) with particular attention to higher resolution simulations and regional-focused evaluations. The PMP offers capabilities for modeling groups to easily evaluate simulations and track changes during the development cycle, in the context of the range of structural errors in the multi-model ensemble. The latest version of PMP, version 3, emphasizes statistics of large- to global-scale annual cycles, tropical and extratropical modes of variability including ENSO and MJO, regional monsoons, cloud feedback, extremes, and high frequency characteristics of simulated precipitation. We are working toward implementing more metrics with extending scope of the realm, such as stratosphere (e.g, QBO), atmospheric dynamics (e.g. blockings), and high-latitude area (e.g, sea-ice). The PMP is prototyping the evaluation of higher resolution simulations such as from the HighResMIPs and cloud-resolving E3SM experiments. This presentation will introduce the PMP and discuss its future plan.
AS07-A012
The Interactions of Multiple Local Circulations and Their Impacts on Air Quality
Yuxi LIU+, Ning ZHANG#
Nanjing University, China
Impacts of local circulations and their interactions on ozone in Suzhou on 5 June 2019 are investigated using surface observations and three-dimensional air quality simulations. It is found that cities on the southeastern shore of Lake Taihu, such as Suzhou, Jiaxing, and Huzhou, have higher ozone concentrations compared with other cities in the Yangtze River Delta, although their emission levels are relatively low. Local circulations and their interactions are found to be the primary causes of the episode. The coupling of lake-land breeze circulation (LLBC), sea breeze circulation (SBC), and urban heat island circulation (UHIC) in regions on the southeastern shore of Lake Taihu such as Suzhou and Jiaxing create wind convergence zones, influencing the spatiotemporal distribution of ozone in the boundary layer. During the daytime, the LLBC plays a dominant role in maintaining the wind convergence zone. It transports pollutants to the surrounding regions of Lake Taihu, resulting in reduced pollution concentrations over the lake and worsen air quality in surrounding areas. The UHIC decouples with SBC at noon, leading to a stronger SBC, thus contributing to a reduction in pollution in upwind regions but hinders downwind diffusion. The UHIC enhances the convergence zones of secondary circulations, making it easier for the accumulation of ozone pollutants in areas between Lake Taihu and lakeside cities.
AS07-A015
Changes in Air Pollution and Health Risks in the United States
Guzailinuer YASEN#+, Qi LIU, Weidong GUO
Nanjing University, China
The health effects of air pollution have become more important and apparent in recent years. Exposure to air pollutants is associated with increased mortality hospitalization rates. However, it should be noted that the health effects of air pollution may vary in different regions. Here we focus on the health risks of air pollution in specific areas and the underlying attribution analysis. Considering that Day-to-day (DTD) temperature variability is an important characteristic of air temperature, which significantly affects human health, we examined the long-term trends of DTD over the past 26 years in the United States, and its association with changing air pollution. By using the observed data and The Coupled Model Intercomparison Project Phase 6 (CMIP6) multi-model simulations, We demonstrate that the positive trend of the DTD index in US can be attributed to the anthropogenic aerosols, while the negative trend of which can be attributed to the natural forcing and greenhouse gas forcing. The observed DTD enhancement over 1997-2022 is dominated by the effect of anthropogenic aerosols, while natural forcing and GHGs partially counteract the effect of anthropogenic aerosols. Based on climate modeling experiments, we demonstrate that the reduced aerosol emissions in US can contribute to the enhanced trend of DTD in USA, Which may indicate that the effect of improved air pollution on health risks in US is not entirely positive.
AS08-A009
NOx and ClNO2 Fluxes in Urban Beijing
Xiaoxiao ZHANG1+, Bin YUAN1#, Yibo HUANGFU1, Xianjun HE1, Thomas KARL2, Martin GRAUS2, Marcus STRIEDNIG2
1Jinan University, China, 2University of Innsbruck, Austria
We employed a modified the Cavity Attenuated Phase Shift NO2 monitor and Chemical Ionization Mass Spectrometer, coupled with the eddy covariance method, to quantify NOx and ClNO2 fluxes in urban Beijing. We assessed the temporal and spatial emission characteristics of NOx, and evaluating the anthropogenic NOx emission inventory. Through ClNO2 flux measurements, we also analyzed the impact of deposition on ClNO2 concentration and yield. Our findings highlight NOx flux exhibiting spatial and temporal heterogeneity in urban Beijing. Comparison results indicate that the current emission inventory overstates NOx emission in the city of Beijing. For ClNO2, our study reveals a significant influence of deposition on its concentration and yield.
AS08-A018
Characteristics and Source Contributions to Aerosol Aminiums Over China Coastal Area and Seas
Ying CHEN#+
Fudan University, China
Atmospheric amines are gaining more and more attention in the field of atmospheric chemistry owing to their important roles in new particle formation and growth. In this study, aerosol aminiums over a coastal city (Shanghai) and the Yellow and East China seas (YECS) were characterised. The concentrations of ammonium, dimethylaminium (DMAH) and trimethylaminium plus diethylaminium (TMDEAH) over Shanghai were all found to be higher in the winter of 2018 than in the summer of 2019, suggesting their non-negligible terrestrial contributions. DMAH and TMDEAH concentrations over the YECS in summer were closely correlated and linked to surface phytoplankton biomass, implying that marine biogenic sources might be a predominant contributor to aminiums at this time. Aminiums over Shanghai generally showed a bimodal distribution with a main peak in droplet mode and a secondary peak in condensation mode, suggesting the notable contribution of aqueous-phase or heterogeneous reaction to the formation of aminiums. In contrast, aminiums over the YECS often showed a unimodal distribution, which may be caused by the competition between amines and NH3 for reaction with acidic compounds. We estimated the contributions of marine biogenic sources, 73.6% to DMAH and 80.1% to TMDEAH over the YECS, using methanesulfonate/non-sea-salt SO42– as an indicator. Our results suggest that marine biogenic emission of amines from China’s marginal seas may have a potential impact on coastal cities, and this source should be considered in modelling new particle formation and air quality in coastal areas.
AS08-A026
A Detailed Analysis of Ammonia Emission Estimates from Fertilizer Application in the Indian Agricultural Context
Thirunagari BABY KEERTHI1+, Sri Harsha KOTA1#, Rajesh KUMAR2
1Indian Institute of Technology Delhi, India, 2University Corporation for Atmospheric Research, United States
Atmospheric ammonia emissions are deleterious due to their role in multifaceted environmental pollution. It has been demonstrated that volatile ammonia (NH3), through interacting with sulphur dioxide and nitrogen oxide gaseous emissions, contributes to the formation of airborne fine particulate matter contributing to air quality degradation, reduced visibility, and regional haze. Further, NH3 released by nitrogen (N) fertilizer applications (FA) worldwide leads to substantial economic loss in the agriculture sector. India, after China, stands as the world's second-largest producer and consumer of synthetic N-fertilizer. Despite the significance of NH3 in the global nitrogen (N) cycle, notable inaccuracies and uncertainties persist in India regarding its atmospheric emissions. Current assessments of emissions from fertilizer applications rely on 'fixed' emission factors, introducing limitations and uncertainties in the estimation process. This study aimed to enhance the accuracy of NH3 emission estimations by correcting the fixed emission factor with different modification factors (MFs). These MFs are functions of crucial influencing variables, including fertilizer type, soil pH, application method (basal and top dressing), application rate, and temperature. In 2018-19, the overall NH3 emissions in India reached approximately 3.15 tera-grams (Tg). The considered fertilizer types encompass Urea (2959 Giga-grams (Gg)), DAP (Di-ammonium phosphate (112.6 Gg), AS (15.30 Gg), and NPK (65.96 Gg). Considering all fertilizer types, the agroclimatic regions of India characterized by the highest NH3 emissions are the ‘Trans Gangetic Plain Region (525.61 Gg)’ followed by the ‘Upper Gangetic Plain Region (466.83 Gg)’. The total NH3 emissions were found to peak during the monsoon season (Jul-Sep; 1217.35 Gg) followed by winter (Dec-Mar; 926.36 Gg). The current study addresses the exigency to minimize NH3 emissions from FA and helps in implementing various stringent mitigation strategies and regulatory actions for sustainable environmental management.
AS08-A027
Inter-annual Variation of Nitrate in Beijing Across Seasons from 2015 to 2019: The Trends and Drivers
Wenxing FU+, Momei QIN#, Jianlin HU
Nanjing University of Information Science & Technology, China
Nitrate has become an increasingly important component of fine particulate matter (PM2.5) in some major cities in China. It didn’t decrease as rapidly as the precursor nitrogen oxides (NOx) did (or even increased), which has attracted wide interest. However, previous research mainly focused on elevated nitrate in cold seasons, leaving seasonal disparities in the trends of nitrate unclear. Here we investigated the interannual trends in nitrate at an urban site in Beijing for all seasons over 2015-2019 and explored the drivers by assembling in-situ measurements, machine learning, and chemical transport model (CTM) simulations. The results show that nitrate would increase in all seasons with the impacts of meteorology removed (i.e., de-weathered), at rates ranging from 1.1% per year in winter to 9.8% per year in summer. Such emission-induced increases in nitrate were inhibited by meteorology in the fall and winter, as a result of decreased humidity, while enhanced in the spring and summer. In addition, the de-weathered nitrate concentrations increased nonlinearly with NO2, with steeper slopes of nitrate to the precursor in 2018-2019 than in 2015-2017, reflecting a higher nitrogen oxidation ratio (NOR) in more recent years. The reduced NOx emissions in spring, fall, and winter increased nocturnal NO3 radicals, which could facilitate the heterogeneous formation of nitrate at night and promote NOR. In summer, NOR increased as well, but this might primarily be related to increased daytime OH radicals and enhanced NO2+OH nitrate production. This study highlighted the distinct impacts of emission changes and meteorology on nitrate in four seasons, and the necessity for season-specific nitrate control strategies.
AS08-A028
Simulating the Sources of Nitrous Acid and the Impacts on Secondary Pollutants in the Fall: A Case Study in the Yangtze River Delta
Xun LI+, Momei QIN#, Jianlin HU, Jingyi LI, Xiaodong XIE
Nanjing University of Information Science & Technology, China
Nitrous acid (HONO) is a significant primary source of OH radicals in the troposphere. Thus it affects the oxidizing capacity of the atmosphere and the formation of ozone (O3) and fine particulate matter (PM2.5). However, the abundance of HONO is always not constrained in the chemical transport models (CTMs), indicating the sources have not been well recognized. In this study, we updated the parameterizations of HONO formation, particularly considering the impacts of light intensity and relative humidity on heterogeneous reactions of NO2 on ground and aerosol surfaces, and added new sources (photolysis of nitrate, the heterogenous formation of HONO on soot, etc.) in the air quality model CMAQv5.3.2. We conducted simulations and investigated major sources of HONO at a rural site in the Yangtze River Delta region in the fall of 2020. The improved HONO chemistry case led to a substantial increase in HONO and reduced the gap between the simulation and observation (NMB from -0.83% to -0.40%). A sensitivity test indicated that negative biases of modeled NO2 (most likely due to emissions) explained the remaining model-observation discrepancies. Overall, the main formation pathway of HONO at the site was the heterogeneous reaction on ground surfaces, accounting for approximately 90% of HONO formation at night and ~80% during the daytime. Meanwhile, we found a 2× increase in the daytime average OH concentration and a 1.8× increase of HO2 with improved HONO simulation, resulting in enhanced nitrate, sulfate, ammonium, and SOA by factors of 1.3, 0.3, 0.8, and 1.1, respectively. This study emphasized the role of HONO chemistry in the formation of secondary pollutants, and future work needs constraint of radicals in the CTMs as well.
AS08-A029
The Impact of Domestic Volatile Chemical Products on Air Quality in Megacities in YRD, China
Yongliang SHE#+, Jianlin HU, Momei QIN
Nanjing University of Information Science & Technology, China
Volatile chemical products (VCPs) have been considered one of the major sources of reactive organic carbon (ROC, including volatile organic compounds (VOCs), and semi/intermediate volatile organic compounds (S/IVOCs)) in megacities. Among VCPs, emissions from domestic volatile chemical products (DVCPs, for instance, personal care products, cleaning products, and insecticides) and the associated impacts are not well understood, particularly in China. In this study, we compiled an emission inventory for DVCPs and explored the impacts of DVCP emissions on the atmospheric environment over the Yangtze River Delta (YRD) using an air quality model. The newly estimated emissions from DVCPs are four times higher than those in the traditional inventory and accounted for 10% of total residential emissions in the YRD. The simulation with updated DVCP emissions compared well with measurements in terms of DVCP tracers (e.g., siloxanes, isopropanol) in urban Shanghai. With improved gas-phase chemistry for oxygenated VOCs as well as parameterization for secondary organic aerosol (SOA) from compounds that had been overlooked earlier, DVCPs contributed to the daily maximum 1-hour O3 and SOA by up to ~3 ppb and ~1 μg/m3 in November of 2019. The impacts were higher in the urban center of Shanghai and under unfavorable meteorological conditions (e.g., stagnation). This study revealed that DVCP emissions are sources that cannot be overlooked in urban centers. Considering the dynamic nature of DVCP emissions, which evolve alongside changes in formulas and our lifestyle, they need more attention in the future.
AS08-A038
Characteristics of Ozone Formation Using BOXMOX Model at the Incheon Skyscraper During the Ozone Alert Period in 2023
Ilkwon NAM1,2+, Jiyoung KIM1, Jeong-Min PARK1, Beomsuk KIM3, Gangwoong LEE2, Yongjoo CHOI2#
1National Institute of Environmental Research, Korea, South, 2Hankuk University of Foreign Studies, Korea, South, 3POSCO International, Korea, South
Since the residential type in urban areas have moved to the high-altitude along with increasing the number of the tall buildings, the public demand for information about atmospheric pollutants at those levels including ozone also have increased. As the first air quality monitoring station (AQM) at high altitude, the AQM at the top of POSCO Tower Songdo (37.39 °N, 126.64 °E, 305m a.s.l.) has been measured since December 2022. Because POSCO Tower Songdo is located in the upwind region of the Seoul Metropolitan Area (SMA) along with industrial complexes and large point source nearby, it is suitable location for identifying the effects from both local emission and long-range transport of ozone and precursors. During ozone alert periods (from May to June 2023), gaseous pollutants (O3, NOx, SO2, CO) and non-methane VOCs (NMVOCs) were measured using Air Quality Monitoring System (AQMS, T series, Teledyne API.) and Selected Ion Flow Tube Mass Spectrometer (SIFT-MS, Voice 200, Syft Tech.), respectively. Also, the nitrogen oxides (HONO and HNO3) were obtained by Monitor for AeRosols and Gases in ambient Air (MARGA, 2060, Metrohm) We analyzed ozone formation characteristics at high altitude in SMA using the BOX Modeling eXtensions (BOXMOX) model by conducting the sensitivity test. We believed that these results could be scientific evidence for formulating ozone management policies.
AS08-A039
Updating the EDGAR Emission Inventory with the Developed In-house Emission Inventory Prepared from the Ground-based Surveys and Analysing Its Impact Using WRF-Chem
Arpit KATIYAR1#, Sri KOTA1, Krunesh GARG2+
1Indian Institute of Technology Delhi, India, 2Punjab Pollution Control Board, India
This study emphasizes on the initial crucial step towards mitigating the particulate matter (PM2.5) by scientifically quantifying and pinpointing its sources. The need for the accurate emission inventories is of paramount importance, and among the diverse methods available, ground-based activity data stands out for its high precision. However, preparing such emission inventories poses challenges as it is very resource and time intensive. This study focusses on the preparation of a detailed emission inventory for PM2.5, with a resolution of 300m × 300m, using ground-based activity data for eight non-attainment cities in Punjab, India (Jalandhar, Amritsar, Patiala, Mandi Gobindgarh, Khanna, Naya Nangal, Dera Bassi, and Dera Baba Nanak). Furthermore, using this in-house emission inventory, Emissions Database for Global Atmospheric Research (EDGAR) which is a widely acclaimed database, is updated and WRF-Chem simulations are performed, the results of which are also a part of this study. The findings of this study reveal Jalandhar is the highest contributor to PM2.5 emissions, estimated 4296 tons/year, respectively, while Dera Baba Nanak emerges as the least contributor with total PM2.5 emissions of 92 tons/year. The primary sources identified across all cities are predominantly vehicular, road dust, industrial, and domestic emissions, making them the top four contributors. Another important insight from this study is the identification of the hotspots within each city from the gridded total emission maps. The results of this study hold critical importance for policymakers, providing a basis for informed decisions and targeted actions to reduce emissions and protect public health. Ultimately, the study emphasizes the importance of thorough emission quantification and source identification in developing effective strategies for reducing particulate matter.
AS08-A040
Reconciling Missing OH Reactivity in the 3-D Chemical Transport Model
Hyeonmin KIM1+, Rokjin J. PARK1#, Saewung KIM2, Do-Hyeon PARK1, Sang-Woo KIM1, Hyeong-Ahn KWON3, Jinkyul CHOI4
1Seoul National University, Korea, South, 2University of California, United States, 3University of Suwon, Korea, South, 4University of Colorado at Boulder, United States
The OH reactivity (OHR), the reciprocal of the OH lifetime, indicates the total amount of reactive trace gases loading in the atmosphere. We examine the characteristics of OHR and the environment in South Korea during the Korea-United States Air Quality (KORUS-AQ) campaign by using the comprehensive NASA DC-8 airborne measurements. The data present that anthropogenic emissions control OHR in South Korea with significant contributions of CO, OVOCs, NOX, and hydrocarbons showing the increase of observed total OHR (tOHR) near and downwind regions of the primary emission sources. However, we found that a 3-D chemical transport model (CTM), GEOS-Chem, underestimates the concentrations of CO and OVOCs compared with observations, thus causing significant OHR underestimation. To reconcile the discrepancy between observed and simulated OHR (missing OHR), we examine the model's processes, such as emission inventories and chemistry schemes. We first adopt the observationally constrained VOC emission inventory based on the preceding studies using airborne and satellite observations. The adopted emission inventories lead to the increase of simulated OVOCs (~16%), aromatics (~23%), and O3 (~4%). Second, we update tropospheric chlorine chemistry to the model, resulting in the increases of simulated NOX (~12%), O3 (~2%), OH (~5%), and HO2 (~2%). Furthermore, we quantify the impact of CO underestimation in the model on the NOX-O3-HOX cycle and simulated OHR. As a result, we reconcile some parts of the missing OHR from ~52% to ~40%, but OVOCs and O3 underestimation in the model still need to be figured out.
AS08-A042
Impact of Aerosol Liquid Water Content on the Heterogeneous Formation of Particulate Nitrate During High-PM2.5 Events
Yongmi PARK+, Subin HAN, Youn-Suk SON, Wonsik CHOI#
Pukyong National University, Korea, South
Secondary inorganic aerosols, including sulfates, nitrates, and ammonium, are known as the primary constituents of fine particulate matter (PM2.5). Recently, the proportion of sulfates has diminished while that of nitrates has increased with the reduction in sulfur emissions due to stricter regulations. To investigate the impacts of nitrates on PM2.5 concentration growth for pollution periods, we conducted field intensives at the Yongdang Campus of Pukyong National University, located in the coastal area of Busan, from January 2021 to June 2022. The measurement site is adjacent to a port and a small industrial complex. Measured components included water-soluble inorganic ions (PILS-IC, Metrohm Eco IC 883, Metrohm) and precursor gases (NO, NO2, NH3, O3; TEI instruments). The aqueous liquid water content (ALWC) and pH were calculated using the ISORROPIA II thermodynamic equilibrium model. First, we found that nitrates played a significant role in the accumulation of high PM2.5 concentrations, regardless of the season. This study attempted to elucidate the nitrate formation mechanism that contributed to the growth of PM2.5 concentrations under highly polluted conditions. We further analyzed temporal variations and correlations among the concentrations of inorganic particles, excess ammonium, humidity, ALWC, and Ox (NO2+O3) to support the nitrate formation processes we propose here. The tentatively proposed nitrate formation process that increases PM2.5 concentrations in this coastal site is as follows. Initially, the ALWC increased through the sea breeze system due to increasing specific humidity in the daytime, in turn, increasing relative humidity at night. Then, N2O5 reacted with the surface of aerosol H2O to form HNO3 (aq) at night, leading to the formation of nitrates. Thus, the heterogeneous formation increased the concentration of nitrates at night, which subsequently led to an increase in the PM2.5 levels.
AS08-A043
Ozone Pollution in Urban Coastal Environments: Surface Ozone Concentration Gradient and Advection Rate During Sea Breeze Periods
Subin HAN+, Yongmi PARK, Wonsik CHOI#
Pukyong National University, Korea, South
In urban coastal environments, mesoscale atmospheric circulation can potentially influence air quality by affecting the chemical processes of air pollutants. In this study, we measured air pollutant concentrations (NO2, NO, and O3) in Incheon and Ulsan, developed urban coastal areas in South Korea. Based on highly spatially resolved observations, we investigated the spatiotemporal variations of pollutants affected by local emission environments. Additionally, we examined the effects of sea breeze on surface ozone concentrations and the associated chemical processes. To verify emission environments in Incheon and Ulsan, we referred to land cover maps. Incheon is primarily traffic-oriented due to its proximity to cargo terminals, ports, and an airport, while Ulsan features extensive industrial areas along the coastline. We installed air quality sensors in representative areas for each microenvironment and conducted measurements for two weeks. We found that the variation of the air pollutant concentrations varied depending on the emission environments. Notably, an inverse correlation was observed in the NOx and O3 changes during the diurnal pattern on weekdays, and this variation was more distinct in traffic and industrial areas. These variations of NOx and O3 concentration were also evident during sea breeze periods. Measured O3 near the coast was relatively high during sea breeze periods. However, in the industrial areas with high NOx emissions, O3 concentrations showed a decreasing gradient. This suggests that NOx emissions from inland areas contributed to the reduction in O3 concentrations. Based on the O3 concentration gradient, we evaluated the impact of sea breeze on O3 concentrations through quantifying O3 advection rates, and examined approaches to the chemical budget of O3 concentrations.
AS08-A045
Estimation of Major Emission Sources of Carbonaceous Aerosols in Industrial Area Nearby Seoul Metropolitan Area in Korea
Seora WOO1#+, Yongjoo CHOI1, Jong Sung PARK2, Pilho KIM2
1Hankuk University of Foreign Studies, Korea, South, 2National Institute of Environmental Research, Korea, South
Although carbonaceous aerosols are higher health risk to humans than PM2.5, there are still uncertainty in Physicochemical properties, transportation, and spatiotemporal distribution. This study used one year semi-continuous PM2.5 chemical composition from the Gyeonggi Air Quality Research Center in Ansan, Korea (37.31°N, 126.80°E) to identify the major sources of carbonaceous aerosols in PM2.5. Because Ansan is a representative industrial and urban mixture area nearby Seoul Metropolitan Area, it is suitable to monitoring the various type of PM2.5 characteristics. Carbonaceous aerosols were analyzed using sunset OCEC analyzer based on NOISH (National Institute for Occupational Safety and Health) thermal optical transmittance (TOT) analysis protocol. Then, we classified the concentrations of organic carbon (OC; from OC1 to OC4) and elemental carbon (EC; from EC1 to EC6) detected depending on the analysis temperatures (310 °C to 870 °C). Additionally, the hourly-based 12 heavy metal components (Si, Ti, V, Mn, Fe, Ni, Cu, Zn, As, Se, Br, Pb) in PM2.5 was also measured using XRF (X-Ray Fluorescence spectrometer) and the major emission sources of carbonaceous aerosols will be identified using statistical approaches (such as principal component analysis (PCA) and/or a receptor model). Therefore, we believe that this research will be helpful to formulating effective regulation policies for the carbonaceous aerosols by estimating the contribution of emission sources, quantitatively.
AS08-A049
Source Apportionment of PM2.5 in an Industrial Area Nearby Seoul in Korea During 2020 Using Positive Matrix Factorization (PMF) Model
Pilho KIM1+, Jong Sung PARK1#, Su-Hyun SHIN1, Changhyeok KIM1, Jeong-Min PARK1, Yongjoo CHOI2
1National Institute of Environmental Research, Korea, South, 2Hankuk University of Foreign Studies, Korea, South
To improve air quality, it is important to establish effective reduction and regulation policies for major pollutants by estimating their contributions and impacts on human health. For these purposes, comprehensive semi-continuous PM2.5 measurements from the Gyeonggi Air Quality Research Center in Ansan, Gyeonggi-do (37.3202 ºN, 126.8283 ºE, 13 m above sea level), which is located in industrial and urban mixture areas, has been conducted since 2020 to identify characteristics of complicated industrial areas. We selected hourly-based chemical species of PM2.5 from January 1 to December 31 in 2020, including inorganic ions from an ambient ion monitor (9000D AIM), trace elements from an online x-ray fluorescence spectrometer (XRF Xact 625i), and carbonaceous aerosol (organic and elemental carbon) from thermal optical transmittance analyzer (Semi-continuous OCEC Analyzer) based on a modified NOISH (National Institute for Occupational Safety and Health) Method. To estimate the contributions of sources, the Positive Matrix Factorization (PMF) receptor model was applied to PM2.5 chemical speciation data which passed the strict QA/QC criteria. The highest source contribution was ammonium nitrate as 39.6% and followed by ammonium sulfate (21.3%), Gasoline (10.9%), Diesel (9.8%), Roadway emission (7.7%), Industry (3.8%), Coal Combustion (2.6%), Oil Combustion (1.8%), Soil (1.4%), and Nonferrous metal (1.0%). Additionally, conditional probability function (CPF) analysis was performed to understand the influence of local emissions. Most emission sources were located in the west direction where an industrial area and a highway are located. However, the diesel emission source was highly contributed from the east direction, where Ansan Bus Terminal and major commercial facilities are located. We believe the evidence of local contributions will be useful in formulating policies that improve the air quality in industrial/urban mixed areas in Gyeonggi Province, Korea.
AS08-A051
Simultaneous Measurements of Nocturnal NO3 Radical and N2O5 in the Wintertime in Seoul During the ASIA-AQ Campaign
Chisung YUN1+, Yongjoo CHOI1, Jeonghwan KIM1, Jiseon LEE1, Taekyung YI2, Changdong YUN2, Hyunmin LEE2, Meehye LEE2, Gangwoong LEE1#
1Hankuk University of Foreign Studies, Korea, South, 2Korea University, Korea, South
NO3 radical was found to play a critical role as a dominant oxidant in the nocturnal atmospheric chemistry, especially in the absence of the OH radical. It mainly oxidizes volatile organic compounds (VOCs) and NOx in an urban air mass during the night. Furthermore, N2O5, produced by the reaction with NO3 radical and NO2 in thermal equilibrium, contributes to the formation of nighttime secondary organic aerosol and the subsequent increase in daytime ozone production through a series of heterogeneous reaction. The chemistry of these reactive nitrogen oxides is significantly influenced not only by its source and sink mechanisms but also by complex weather conditions, including local and region circulations. Therefore, it is necessary to continuously monitor the chemical processes of NO3 radical and N2O5 for all seasons. We performed to measure NO3 radical in the summertime using a home-made Long-Path Differential Optical Absorption Spectroscopy (LP-DOAS) in Seoul. Currently, we also successfully developed Incoherent Broadband Cavity-Enhanced Absorption Spectroscopy (IBB-CEAS) to observe N2O5. This study aims to simultaneously measure and characterize the NO3 radical and N2O5 in the wintertime at Korea University in Seoul during the Asia-AQ campaign. Subsequent analysis will be conducted to assess the wintertime temporal variations and chemical mechanisms based on the production and loss of NO3 radical and N2O5 in Seoul with the simultaneous measurements of key trace gases, particulate pollutants and meteorological parameters. The detailed data analysis will be presented during the conference.
AS13-A005
The Shear-relative Variation of Inflow Angle and Its Relationship to Tropical Cyclone Intensification
Jie MING1#+, Jun ZHANG2, Rogers ROBERT3
1Nanjing University, China, 2University of Miami, United States, 3NOAA's Atlantic Oceanographic and Meteorological Laboratory, United States
Characterizing inflow structure is important to better represent tropical cyclone impacts in numerical models. While much research has considered the impact of storm translation on the distribution of inflow angle, comparatively less research has examined its distribution relative to the environmental wind shear. This study analyzes data from 3655 dropsondes in 44 storms to investigate the radial and shear-relative distribution of surface inflow angle. Emphasis is placed on its relationship with intensity change. The results show that the radial variation in the inflow angle is small and not significantly dependent on the shear magnitude or intensity change rate. In contrast, the azimuthal distribution of the inflow angle shows a significant asymmetry, with the amplitude of the asymmetry increasing with shear magnitude. The maximum inflow angle is located in the downshear side. The degree of asymmetry is larger in the outer core than in the eyewall. Intensifying storms have a smaller degree of asymmetry than steady-state storms under moderate shear.
AS13-A014
Statistical Seasonal Forecasting of Tropical Cyclone Landfalls on Taiwan Island
Ziqing CHEN+, Kelvin T. F. CHAN#
Sun Yat-sen University, China
Forecasting tropical cyclone (TC) activities has been a topic of great interest and research. Taiwan island is one of the key regions that is highly exposed to TCs in the western North Pacific. Here we utilize the mainstream reanalysis datasets in 1979–2013 and propose an effective statistical seasonal forecasting model, namely the Sun Yat-sen University (SYSU) Model, for predicting the number of TC landfalls on Taiwan island based on the environmental factors in the preseason. The comprehensive predictor sampling and multiple linear regression shows that the 850-hPa meridional wind over west of the Antarctic Peninsula in January, the 300-hPa specific humidity at the open ocean southwest of Australia in January, the 300-hPa relative vorticity at the west of the Sea of Okhotsk in March and the sea surface temperature in April at the South Indian Ocean are the most significant predictors. The correlation coefficient between the modeled results and observations reaches 0.87. The model is validated by the leave-one-out cross validation and recent 9-year observations (2014–2022). The prediction of the SYSU Model exhibits a 98% hit rate in 1979–2022 (43 out of 44), suggesting an operational potential in the seasonal forecasting of TCs landfall on Taiwan island.
AS13-A015
Distinct Future Changes of ENSO-induced Tropical Cyclone Activities Between Atmosphere-only and Coupled Models in the CMIP6
Fang WANG1+, Zhao JIUWEI1#, Zhang LEYING2
1Nanjing University of Information Science & Technology, China, 2Nanjing Forestry University, China
This study utilizes the HighResMIP-CMIP6 data to investigate future changes in tropical cyclone (TC) activity, including TC genesis frequency (TCGF) and track density (TCTD), in response to El Niño-Southern Oscillation (ENSO). The TC activity changes from uncoupled (atmosphere-only) and coupled runs are very diverse, indicating large uncertainty for future projections. Full-coupled models projected an El Niño-like Sea surface temperature (SST) warming over the equatorial Pacific, while uncoupled (atmosphere-only) models reveal a La Niña-like warming pattern. This SST difference further induced diverse atmospheric circulation anomalies, eventually contributing to distinct TCGF and TCTD changes during ENSO phases for future projections. Further detailed analysis reveals that the El Niño-like or La Niña-like warming patterns are two extreme cases. It shows a strong variance of simulated SST across different models. The accurate projection and simulation of central Pacific SSTs and Eastern Pacific SSTs is the key to reducing the diverse behaviors of TC activity among these models. We detected three crucial regions, that is the central Pacific, the subtropical eastern North Pacific, and the equatorial eastern Pacific, that could modulate TC activity in response to ENSO in numerical models. These results help to further improve the accuracy of models to simulate future TC changes.
AS13-A029
Assessment of an Experimental Version of fvGFS for TC Genesis Forecasting Ability in the Western North Pacific
Shu-Jeng LIN1#+, Huang-Hsiung HSU2
1Chinese Culture University, Taiwan, 2Academia Sinica, Taiwan
We evaluated the ability of the fvGFS with a 13-km resolution in simulating tropical cyclone genesis (TCG) by conducting hindcast experiments for 42 TCG events over 2018–19 in the western North Pacific (WNP). We observed an improved hit rate with a lead time of between 5 and 4 days; however, from 4- to 3-day lead time, no consistent improvement in the temporal and spatial errors of TCG was obtained. More “Fail” cases occurred when and where a low-level easterly background flow prevailed: from mid-August to September 2018 and after October 2019 and mainly in the eastern WNP. In “Hit” cases, 850-hPa streamfunction and divergence, 200-hPa divergence, and genesis potential index (GPI) provided favorable TCG conditions. However, the Hit–Fail case differences in other suggested factors (vertical wind shear, 700-hPa moisture, and SST) were nonsignificant. By contrast, the reanalysis used for validation showed only significant difference in 850-hPa streamfunction. We stratified the background flow of TCG into four types. The monsoon trough type (82%) provided the most favorable environmental conditions for successful hindcasts, followed by the subtropical high (45%), easterly (17%), and others (0%) types. These results indicated that fvGFS is more capable of enhancing monsoon trough circulation and provides a much better environment for TCG development but is less skillful in other types of background flow that provides weaker large-scale forcing. The results suggest that the most advanced high-resolution weather forecast models such as the fvGFS warrant further improvement to properly simulate the subtle circulation features (e.g., mesoscale convection system) that might provide seeds for TCG.
AS13-A030
Evaluation of the Possibility of a Korean Typhoon Impact-based Forecast Using a Regional Multi-hazard Risk Index
Hana NA1,2#+, Woo-Sik JUNG1
1Inje University, Korea, South, 2Inje University, Korea, South
Typhoons affecting the Korean Peninsula are getting stronger and dying down (WMO, 2021; IPCC, 2021; Na and Jung, 2021). The National Oceanic and Atmospheric Administration (NOAA) and the National Weather Service (NWS) have established disaster prevention and changed the national management policy stance by providing information on risks in advance about the effects of extreme weather disasters, responding to them, and taking action in advance. A paradigm shift was attempted by declaring the Weather-Ready Nation (WRN), a national strategy to minimize damage, as a strategic plan for the next 10 years in 2011. Starting with the declaration of paradigm shift of WRN, various countries around the world (Britain, France, Japan, China, etc.) have conceptualized the words READY and PREPARE in relation to tropical cyclones such as typhoons and hurricanes, establishing disaster prevention. In addition, with the help of the World Meteorological Organization, several developing countries in East Asia (Philippines, Vietnam, Thailand, etc.), which are heavily affected by typhoons, are also actively introducing impact forecasts (Katie et al., 2016; Nguten et al., 2021; Nofal et al., 2021; Thuc et al., 2022; Do and Kuleshov, 2022).This study aims to evaluate the possibility of typhoon impact prediction in Korea by utilizing the risk index calculated by the Typhoon-Ready System, which was developed to establish the basis for typhoon impact prediction in Korea. The possibility and validity of the risk index were analyzed through the analysis of representative typhoon cases applying the complex weather disaster risk index based on impact prediction, and in particular, the possibility of typhoon impact prediction in Korea was evaluated through the risk level proposal for regional-specific risk indices, which are the core of impact prediction. This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No.RS-2023-00212688).
AS13-A032
Evaluation of the Genesis Potential Indices in the CMIP6 Models with Bias Correction Methods and Projecting Future Tropical Cyclone Potential
Erandani Lakshani WIDANA ARACHCHIGE1,2#+, Wen ZHOU3, Ralf TOUMI2, Xuan WANG4, Oluwafemi Ebenezer ADEYERI4, Dushantha Sandaruwan Jayarathana WIJENDRA NAIDHELAGE 4,5
1Nanyang Technological University, Singapore, 2Imperial College London, United Kingdom, 3Fudan University, China, 4City University of Hong Kong, Hong Kong SAR, 5University of Exeter, United Kingdom
Genesis Potential Indices (GPIs) indicate the potential of the Tropical cyclone (TC) occurrence in response to large-scale environmental conditions. Recent studies use simulated GPIs from the Coupled Model Intercomparison Project Phase 6 (CMIP6) to investigate the physical explanation of projected global TC changes. In this work, we first evaluate the ability of CMIP6 historical simulations (1979-2003) to capture long-term variations in GPIs (dynamic GPI and Emanuel GPI) compared to the GPIs from observational data sets. The presence of inherent biases in the models prevents both the GPI simulations and the individual terms of GPIs from adequately reproducing the observed variation. Thus, bias correction was conducted via direct approach using univariate (quantile delta mapping; QDM) and multivariate (N-dimensional probability density function transform; MBCn) methods and component-wise with QDM on CMIP6 simulated GPIs in historical and future projections (2075-2099) under high emission (SSP5-8.5) scenario. Overall model evaluation on all BC methods in historical GPI simulations under the direct bias correction exhibits a slightly better performance than the component-wise approach. Even though we observed no significant difference between the future changes from GPIs from bias-corrected CMIP6 and the raw models, we observed substantial model uncertainty reduction in the corrected models, emphasizing the improved reliability of the models for future projections. This study provides a comprehensive assessment of bias correction techniques used in CMIP6 models for GPI simulation, along with the projected potential for TC formation.
AS13-A033
Straight-moving Tropical Cyclones Over the Western North Pacific Trigger the Wave Trains Over the North Pacific During Winter
Shuaiqiong MA#+, Bo PANG, Riyu LU
Chinese Academy of Sciences, China
This study investigates the large-scale circulation anomalies induced by straight-moving tropical cyclones (TCs) over the western North Pacific (WNP) during winter. Corresponding to the straight-moving TCs, a quasi-stationary wave train is excited as alternative geopotential height anomalies in the upper troposphere stretching from East Asia to the North Pacific. Specifically, the anomalous anticyclones are initially formed over East Asia to the north of TCs and then lead to the subsequent anomalies in the downstream areas. Further analysis reveals that the upper-level anticyclonic anomalies are excited by negative Rossby wave sources, which are mainly attributed to the poleward vorticity advection by anomalous divergence relevant to TCs. In addition, the diagnosis indicates that the generation of wave source is caused by the product of the TC-induced divergent flows and the prominent meridional vorticity gradient in association with East Asian upper-tropospheric westerly jet. The above processes differ from the recurving TCs in summer and autumn, which undergo extratropical transition when they move northward into the mid latitude. These findings imply that the tropical disturbances over the WNP, such as straight-moving TCs, can remotely affect weather over the extratropics, and thus have implications for improving the weather forecast over the extratropics through improving tropical disturbance forecast.
AS13-A034
Examinations on Global Changes in the Total and Spatial Extent of Tropical Cyclone Precipitation Relating to Rapid Intensification
Yaxin LIU#+
Sun Yat-sen University, China
Moderate tropical cyclone precipitation (TCP) is of great significance to regional water resource supply, while extreme TCP could bring significant adverse impacts to ecosystems and society, especially when tropical cyclones intensify rapidly, leaving no time to take prevention actions. Whether rapid intensification (RI) of tropical cyclones (TCs) affect TCP in both land and ocean remains unknown. Here we classified TCs which have undergone increases in the maximum sustained wind speed (MSW) by at least 30 knots within 24-h into RI category. We analyzed TCP totals provided by daily precipitation from Precipitation Estimation from Remotely Sensed Information using Artificial Neural Networks-Climate Data Record (PERSIANN-CDR) and spatial extent from 1983 to 2019 in the four categories based on regions (land and ocean) and RI-experiencing characteristics (with- and without-RI). TCP totals and spatial extent was identified by the restricted moving neighborhood method and semi-variogram framework. The results show that TCP totals on the ocean are larger than those on the land, since RI-experiencing TCP are higher than TCP without RI experiencing, although RI processes tend to increase TCP totals in the extremely high percentiles more significantly on land than ocean. The four regions of the Northeast Pacific Ocean (EP), South Pacific Ocean (SP), Northwest Pacific Ocean (WP), and North Atlantic Ocean (NA) show increases in regional mean and extreme TCP totals. The highest increase in the extreme TCP totals (0.37 mm day−1 year−1) over the NA region occurs in the RI_ocean category, which is 2.6 times the average positive enhancement trend across all basins. The increasing rate of the extreme TCP totals over the WP region is higher in track points with RI-experiencing than without RI-experiencing. The category of RI_land over the regions of NA, EP and SP shows a significant increase in the regional mean TCP spatial extent.
AS13-A036
Atmospheric and Oceanic Responses to Super Typhoon Mangkhut in the South China Sea: A Coupled CROCO-WRF Simulation
Mingyu LI#+, Chaoxia YUAN, Zhao JIUWEI
Nanjing University of Information Science & Technology, China
The South China Sea (SCS) is the largest marginal sea in the Northwest Pacific Ocean, and it encounters frequent typhoons. The atmosphere and ocean will create significant thermal and dynamic responses during the intense disturbance caused by typhoons. However, these responses have not been thoroughly investigated owing to the complicated marine environment. According to the satellite data, the SCS Basin was observed to have a strong SST response to Typhoon Mangkhut, resulting in widespread SST cooling. A coupled model was used to investigate the atmospheric and oceanic responses to Typhoon Mangkhut. Best-track data, satellite SST, and ARGO measurements show that the coupled WRF-CROCO simulation displays better track, intensity, SST, temperature, and salinity profiles than those of the WRF-only simulation. Results show that the typhoon induced rightward intensifications in wind speed, ocean current, and SST. The following are some remarkable atmosphere and ocean responses: (1) the SST below the inner-core region is cooled by 1°C, resulting in a 37%–44% decrease in wet enthalpy, and the central pressure is increased by ~9 hPa. Therefore, the changes in SST below the inner-core region of the SCS Basin have a significant impact on air-sea fluxes under high-wind conditions. (2) the ocean boundary layer analysis shows that near-inertial oscillations on the right side of the typhoon track and a strong inertial current up to ~2.28 m/s in the upper ocean were observed, which resonated with the local wind and flow field on the right side and induced strong SST cooling. (3) a decrease in SST decreased the moist static energy of the typhoon boundary layer, thereby weakening the typhoon’s intensity. The difference in equivalent potential temperature and sea surface pressure have a good correlation, indicating that the influence of moist static energy on typhoon intensity cannot be overlooked.
AS13-A041
Features of Boundary Layer During Tropical Cyclone Landfall Observed at the Boseong Tall Tower
Jinhui JU1+, Doosun PARK1#, Young-Hee LEE1, Ki-Hoon KIM2, Hyeon-Ju GIM3, Taewon PARK4, Sora IN5
1Kyungpook National University, Korea, South, 2Korea Meteorological Administration, Korea, South, 3Korea Institute of Atmospheric Prediction Systems, Korea, South, 4Chonnam National University, Korea, South, 5National Institute Meteorological Sciences, Korea, South
This study examines the characteristics of PBL for landfalling TC cases using data from the Boseong Tall Tower. The Boseong Tall Tower, the second highest multi-level meteorological tower in Asia, provides vertical profiles of the lower planetary boundary layer (PBL), enabling investigation of the characteristics of the lower PBL over land. It is particularly useful when a tropical cyclone (TC) makes landfall, as observations with sonde over land can be difficult. Previous studies have suggested that the track, intensity and structure of a TC are influenced by turbulent processes in the Planetary Boundary Layer (PBL), and the parameterization of the TC boundary layer used in the ocean may not match well with land. Therefore, it is important to understand the characteristics of the PBL over land, especially when TCs make landfall, for better TC prediction and prevention. Based on our analysis, it appears that the log layer may not accurately represent the depth of the surface layer when assuming a near-neutral surface layer. This suggests that alternative assumptions may be necessary. In contrast to previous studies, our findings indicate that the fitted surface frictional speed (u*s) slightly increases with wind speed, while the fitted roughness length (z0) decreases with mean wind speed. These suggest that stronger surface wind speeds result in a wider range of wind speeds, which may be influenced by ocean surface features due to the proximity of the Boseong Tall Tower to the coastline. Additionally, we compare the vertical eddy diffusivity (Km) as measured by observation and the parameterization used in the numerical model. [Funding. This study was supported by the Korea Meteorological Administration Research and Development Program (KMI2022-01312)].
AS13-A047
Enhancing Prediction of Precipitation and Winds During Typhoon Approaches
Minyeong KIM#+, Seonghee WON, Hyun-Soo LEE
Korea Meteorological Administration, Korea, South
A prediction system for wind and precipitation during typhoons affecting the Korean Peninsula was developed based on the characteristics of wind and precipitation areas along the track of past typhoons, and to improve the accuracy, sensitivity experiments were conducted based on the selection criteria for similar past typhoons. As a result of Typhoon KHANUN by selecting similar typhoon cases in the past, the wind prediction was good result, but precipitation prediction was relatively inaccurate. To improve the observation-based typhoon prediction system, we conducted a prediction experiment using an ensemble numerical model. Among the predicted ensemble members, we selected those whose typhoon centers were within 50 km of the official typhoon information and then averaged the precipitation/wind forecast fields. The wind prediction results showed over estimated, while precipitation prediction showed significant improvement in accuracy compared to observations.
AS13-A048
Improvement in Typhoon BAVI Simulation Through Air-sea Coupling with Realistic Sea Water Salinity
Woojin CHO1#+, Dong-Hyun CHA1, Minho KWON2, Jiseok HONG2
1Ulsan National Institute of Science and Technology, Korea, South, 2Korea Institute of Ocean Science and Technology, Korea, South
The decrease in sea surface temperature (SST) with latitude is one of the factors that weakens the intensity of typhoons moving towards mid-latitude. Atmosphere-only models (i.e., WRF) with high horizontal resolution which use prescribed SST for low boundary conditions sometimes overestimate the intensity of decaying typhoons in mid-latitude. The air-sea interaction reduces this overestimate of typhoon intensity by producing realistic SST cooling below the typhoon. However, excessive SST cooling in coupled models often occurs and this can decrease the typhoon intensity. In this case, ocean vertical structure may be associated. We investigate the effect of air-sea interaction and the vertical structure of ocean below typhoon BAVI in 2020 by comparing 3-km high-resolution WRF and WRF-ROMS coupled model. For the WRF-ROMS experiment, 3D ocean data is necessary, and the HYCOM analysis data is usually used. However, the salinity of HYCOM in East China Sea has a large uncertainty because HYCOM does not fully reflect the Changjiang river freshwater. So we conducted WRF-ROMS simulation with Changjiang river discharge to create realistic salinity input for typhoon BAVI simulation. As a result, WRF with prescribed HYCOM SST overestimates the intensity of typhoon BAVI, but WRF-ROMS with HYCOM salinity underestimates the typhoon intensity. WRF-ROMS with realistic salinity shows the salinity in East China Sea is lower than normal due to high Changjiang river discharge, and the freshwater inflow makes ocean stratification in East China Sea. Ocean stratification makes a barrier layer and reduces the vertical mixing and SST cooling under typhoon BAVI, increasing typhoon intensity.
AS13-A051
Understanding the Characteristics of Recurving Tropical Cyclones in the Western North Pacific
Md Afjal HOSSAIN1+, Il-Ju MOON1#, Md. Jalal UDDIN1, Vineet Kumar SINGH2
1Jeju National University, Korea, South, 2Indian Institute of Tropical Meteorology, India
Tropical cyclones (TCs) in the western North Pacific (WNP) follow two distinct tracks: some move in a west-northwest direction, while others recurve in a north-northeast direction. Recurving TCs possess a major disaster risk for the densely populated coastline of Korean Peninsula and Japan. While there have been studies on recurving TCs in the WNP, the statistical characteristics of the recurving TCs and whether their features are changing due to climate change have not been thoroughly investigated to date. Apart from that, there are discrepancies in extracting the recurving TCs in this basin. Therefore, this study proposes a new methodology comprising a set of criteria to realistically extract recurving TCs in this basin. TCs extracted based on proposed new criteria, we investigate statistical characteristics such as the seasonal distribution and trend, recurving location (latitude and longitude), the number of occurrences, lifetime maximum intensity (LMI) and recurving time nexus, translation speed, and the recurving angle of recurving TCs during the period 1981–2021 among others. Moreover, we further examine the reasons of varying frequencies of recurving TCs in different years. Results suggest that position and strength of WNP subtropical high (WNPSH) plays a pivotal role in recurving TCs varying frequencies in WNP. Finally, we investigate whether recurving TCs characteristics change over time. These findings will contribute to understanding the characteristics of recurving TCs in the WNP, especially in the face of climate change.
AS13-A078
Westerlies Controlling of the Water Vapor Transport to the Tibet Plateau by the Tropical Cyclones in the Bay of Bengal
Xiaoli ZHOU#+
Fudan University, China
This study investigates the water vapor transport to the Tibetan Plateau (TP) induced by Bay of Bengal (BOB) tropical cyclones (TCs) in May during 1979-2019. The water vapor around the BOB TCs can be transported to the south of the TP by the southerlies at the upper troposphere east of the TC center. Whether the water vapor can cross the southern boundary of the Tibetan Plateau (SBTP) may rely on the different configurations of BOB TCs and long-wave trough and ridge. We found that the water vapor may (may not) cross SBTP if the TC’s wind field converges with the westerlies in front of the trough (ridge). The physical mechanism is explored according to the momentum equation. When the TC moves northward around the SBTP, its wind field could interact with the trough (Type-T TC) and ridge (Type-R TC) in the westerlies. In the area close to the trough line (ridge line), the meridional acceleration is positive (negative), hence meridional component of velocity increases (decreases). Therefore, it is more favorable for the water vapor transported northward if a Type-T TC enters the westerlies from the area close to the trough line than the ridge line. The simulation of the BOB TC cases configuration using WRF model confirms the importance of the relative position between the Type-T TC and the SBTP to the water vapor transport over the SBTP. For the Type-T TC, the meridional moisture budget over the SBTP is positively correlated with the TC intensity and negatively correlated with the distance between the TC center and the SBTP. However, for the Type-R TC, the meridional moisture budget is not related to the TC intensity and the distance. The configuration of TC and long-wave trough or ridge may be predictable through the intraseasonal oscillation activity in the eastern BOB and the southern Arabian Sea. May and October to December are the bimodal phases of BOB TC frequency, which decreases month by month from October to December and is relatively low in May. However, the contribution rate of MMBa is the highest in May. Seasonal variation in the meridional position of the westerlies is the key factor affecting the contribution rate. The relatively south position of the westerlies in November and December results in the lower contribution rate of MMBa.
AS15-A002
Utilizing Satellite Remote Sensing and Meteorological Data to Evaluate Potential Wind Power Generation Sites Along the Coast and Offshore of Taiwan
Chih-Yen WANG#+, Po-Chun HSU
National Central University, Taiwan
This study evaluates potential sites for wind power generation in the Taiwan Strait and inland areas of Taiwan, employing data from multiple satellites, reanalysis, and meteorological stations. The calculation of wind energy is based on transforming these wind speed data to the elevation of wind turbines, considering blade surface area and other coefficients for potential electrical energy estimation. In offshore areas, water depth determines the suitability of fixed or floating wind turbines, with depths exceeding 60 meters being suitable for floating turbines, and shallower waters being appropriate for fixed ones. Inland Taiwan's wind patterns are influenced by topography and buildings. Due to the stability of the wind, coastal areas emerge as prime locations for wind turbine installation. The spatiotemporal characteristics of wind at each potential site are the primary considerations in this assessment. Wind speeds in the Taiwan Strait range from 4 m/s to 15m/s, typically higher in winter. According to the Meteorological Information Based Green Energy Operations Center in Taiwan, the effective wind speed range for turbines is 3 m/s to 25 m/s, which means that wind turbines can operate throughout the year in the Taiwan Strait. Additionally, climatic-scale variations in wind speed are also considered. From 2012 to 2023, an annual increase of approximately 0.15m/s was observed in February, April, May, October, and December in the Taiwan Strait. Comprehensive assessments indicate that the central offshore areas of the Taiwan Strait exhibit higher wind energy potential, with water depths conducive to fixed wind turbines.
AS15-A007
Development of Long-term Climate Data Algorithm Based on GEMS Data
Ha Jeong JEON1+, Sang Seo PARK1#, Jeong Ah YU2
1Ulsan National Institute of Science and Technology, Korea, South, 2National Institute of Environmental Research, Korea, South
The demand for long-term climate analysis is increasing with the flow of global climate change. Accordingly, the need for Level 3(L3) data from satellite observation has also increased in climate studies. In particular, the Geostationary Environmental Monitoring Spectrometer (GEMS) mounted on geostationary satellites is highly evaluated in East Asia, and it is time to develop a L3 algorithm tailored to the model grid to effectively utilize GEMS for climate analysis. Therefore, this study developed a long-term climate analysis data production algorithm based on GEMS data. Data for January 1, 2022, were estimated using GEMS AOD, NO2, and total O3 data. To consider the homogeneity of data, all data that produce L3 data was collected by using only Full Mode Scan. Data quality correction was performed by applying Cloud Fraction and Final Algorithm Flag. In addition, we used the area weighted average calculation method to achieve stable production. In this data production, the most used spatial resolution, 0.25° X 0.25°, was adopted, and using this data, the combination with other satellites for long-term data production will be conducted.
AS15-A008
Cloud Top Characteristics of Vortices Generated on the Tibetan Plateau with Different Paths Revealed by FY-4
Bo LI1#+, Yang GAO2
1National Satellite Meteorological Cener, China Meteorological Administration, China, 2China Meteorological Administration, China
The Tibetan Plateau Vortexes (TPV) can trigger mesoscale convective systems (MCSs) under appropriate conditions. These MCSs not only contribute most of the precipitation in the plateau area, but also move eastward along with TPV under appropriate conditions, triggering a series of mesoscale convective activities along the way. These precipitation events are often intense and long-lasting, often causing serious flooding disasters. However, due to the lack of observation data and complex terrain over plateau areas, the study of weather systems in plateau areas has always been a challenge. This work utilizes Fengyun-4 meteorological satellite and reanalysis data to study the cloud top structure characteristics of plateau vortices with different movement paths. A comparative analysis was conducted on the differences in cloud top height, cloud top temperature, cloud top brightness temperature, and brightness temperature difference of different satellite channels among three paths of plateau vortices: Colonel in situ, moving eastward but not descending to the plateau, and moving eastward beyond the plateau. The influence of these variables on the movement path of plateau vortices was also discussed.
AS15-A012
Emission Estimation Using TROPOMI Satellite in East Asia
Jun-Yu LU#+, Fang-Yi CHENG
National Central University, Taiwan
The conventional emission estimation for air quality simulation was based on the bottom-up method, which relies on the accuracy of the emission inventory. During Taiwan's winter and spring seasons, the northeasterly monsoonal wind prevails, which transports the air pollutants from East Asia to Taiwan. However, the updates of emissions in East Asia is slow, making it challenging to promptly capture changes in emission sources. This leads to forecasting bias during transboundary pollution events. Recently, more real-time and high-resolution satellite data have been used to constrain the bottom-up estimated emissions. This study aims to use TROPOMI satellite data to update the bottom-up estimated emissions in East Asia. This correction intends to address the issue of underestimated transboundary air pollutants in Taiwan. Through a mass balance adjustment of emissions derived from satellite and model-retrieved NO2 column densities, the adjusted NOx emissions are higher than the bottom-up estimated emissions, which furthermore enhances the model performance of the transboundary pollution event.
AS15-A020
Detection of Methane Gas Emissions in the Suncheon Area, North Korea Using Sentinel-2 Satellite Data
Minju KIM+, Jeongwoo PARK, Chang-Uk HYUN#
Dong-A University, Korea, South
As extreme weather events such as heatwaves and wildfires increasingly occur worldwide due to climate change, efforts are underway to reduce greenhouse gas emissions. Among various greenhouse gases, methane significantly impacts climate change, with a global warming potential approximately 82.5 times that of CO2 over a 20-year period. Reducing methane gas emissions, which have a relatively potent warming effect, is essential for mitigating climate change, and continuous monitoring is crucial for identifying and managing sources and amounts of emissions. Satellites can periodically observe the same areas, enabling continuous monitoring of methane emissions, and their global coverage allows for the detection of methane gas in extensive or inaccessible areas. The Sentinel-2 satellite, with its short revisit cycles and high-resolution imagery across various spectral bands, is useful for methane gas detection. Previous research has conducted methane detection studies on well-known methane emission sources using the shortwave infrared (SWIR) bands of various satellites. In this study, we utilized the Google Earth Engine (GEE), which allows for rapid analysis of satellite data in a web browser, to leverage the short revisit cycles and broad spectral band coverage of the Sentinel-2 satellite. We detected and monitored methane plumes from the 2.8 Jikdong Coal Mine located in Suncheon, South Pyongan Province, North Korea. The results of this study are expected to provide important data for the establishment of environmental policies and strategies for climate change mitigation. Furthermore, it demonstrates the practicality of remote sensing technology in methane emission monitoring and highlights the potential use of Sentinel-2 satellite data in climate change studies.
AS15-A024
Fusion of Total Precipitable Water Using GK2A/AMI, NWP and Radiosonde Over East Asia
Seunghee LEE#+, Hyejin MOON, Jae-Young BYON, Myoung-Hee LEE
Korea Meteorological Administration, Korea, South
Total Precipitable Water(TPW), a column of water vapor content in the atmosphere, is an important meteorological factor and play a critical role in the occurrence of precipitation and atmospheric river. The current TPW algorithm operational at NMSC calculates TPW based on AMI Aerosol Profile(AAP) in for clear-sky areas, and uses values calculated from numerical weather prediction (NWP) for cloudy-sky regions. The validation results for this algorithm with radiosonde show an RMSE 6.9mm and a bias of 0.377mm. To fuse the distribution of TPW in all sky conditions, this study proposes a retrieval algorithm based on the light gradient boosting machine (LGBM) model using GK2A/AMI data, Radiosonde, ERA5, and three NWP models data. Through statistical verification, with a root mean square error (RMSE) of 6.697~7.056mm, a bias of -0.929~0.377, and a Pearson's R of 0.942~0.946. We utilize the previously generated NWP prediction field to retrieve TPW in real-time. Detailed introduction of new TPW will be presented in the conference. This research was supported by the “Technical development on high-impact weather detection and prediction using meteorological satellite data”(KMA2020-00121) of “Technical Development on Weather Forecast Support and Convergence Service using Meteorological Satellites” project funded by the National Meteorological Satellite Center, Korea Meteorological Administration.
AS15-A025
Analysis on the Effects of Slant Path Simulation for the All-sky Data Assimilation Using a 1DVAR System
Dabin YEOM1+, Ji-Soo KIM2, Tae-Myung KIM1, Hyung-Wook CHUN3, Myoung Hwan AHN1#
1Ewha Womans University, Korea, South, 2Seoul National University, Korea, South, 3Korea Meteorological Administration, Korea, South
The theoretically calculated radiance (B) in the process of utilizing satellite data into numerical weather prediction models plays an important role in various processes. For example, the difference between observed data O and calculated B is used to understand the error characteristics of the observed data or to determine whether clouds are present in the observed data. Therefore, accurately calculating B is one of the most basic processes for the use of satellite data. To achieve this, various efforts are being made, such as improving the accuracy of radiative transfer models as well as accurately inputting surface characteristics. In this study, we focus on using temperature and humidity profiles along the slant path considering the direction in which satellite data is obtained, rather than the vertical path for the input of the radiative transfer model. Previous studies on clear-sky conditions have shown that applying a slant path result in a noticeable deviation when the viewing angle is far from nadir and in regions with high variability in atmospheric temperature and humidity. This study extends this to investigate the effect of the slant path radiative transfer model in the presence of clouds. When the horizontal range of clouds is not extensive, the presence of clouds varies depending on the chosen path. Furthermore, application of the slant path explicitly considers the parallax effect of clouds in the simulation process, allowing for a more accurate calculation of B values. Taking all these factors into account, we aim to analyze the impact of slant path simulations on vertical temperature and humidity retrieval by analyzing the results of 1DVAR models for all-sky cases.
AS15-A026
Global Trends in Occurrence Frequency of Extremely Heavy Precipitation During 2001–2020 Derived from Various Satellite-based Precipitation Estimation Products
Hamin KOO+, Hyunho LEE#
Kongju National University, Korea, South
Heavy precipitation events are of great importance as large amounts of rainfall concentrated in a short duration can generate severe natural disasters, which then cause widespread damage to human societies. Many previous studies have shown an increasing trend in the atmospheric water vapor due to global warming, readily indicated by the Clausius-Clapeyron relation. However, most of studies on the occurrence frequency of heavy precipitation are generally conducted on regional or national scales.In this study, we use three satellite-based precipitation estimation products—Integrated Multi-satellitE Retrievals for GPM (IMERG), Global Satellite Mapping of Precipitation (GSMaP), and Global Precipitation Climatology Project (GPCP)—and one rain gauge-based precipitation product, NOAA Climate Precipitation Center (CPC), and examine the global trend in occurrence frequency of heavy precipitation from 2001 to 2020. Using the number of days when the daily precipitation amount exceeds the 95th percentile of precipitation amount (FP95) and utilizing the Mann-Kendall test, Sen’s slope estimator, linear regression, and innovative trend analysis, we find that the trends of FP95 from the various analysis methods are generally comparable but highly vary depending on the precipitation products. The trends of FP95 in the lands from IMERG and GPCP are generally similar with those from CPC. However, the trends in the oceans are noticeably inconsistent across all the products. The FP95 from GSMaP increases significantly both in the lands and in the oceans except for some regions, but those from GPCP are decreasing on most of the oceans. Because satellite-based precipitation estimation products derive the amount of precipitation indirectly from atmospheric elements such as water vapor, liquid water path, and cloud top temperature, trends in the atmospheric parameters provided by a polar orbiting satellite are also analyzed to explain the discrepancies in trends of FP95 across the precipitation products.
AS15-A028
Use of Retrieved Thermodynamic Variables from the Satellite Observation for the Understanding and Predicting Convective Precipitation
Jinyeong KIM+, Jin LEE, Junha LEE, Suna CHO, Myoung Hwan AHN#
Ewha Womans University, Korea, South
Heavy rains occurring in a short time can cause significant damage, but it is difficult to accurately predict or observe its occurrence and dissipation. In this study, we investigated the possibility of understanding the development of convective precipitation clouds using thermodynamic variables (such as lifting convective level (LCL), level of free convection (LFC), stability index, etc.) with a 10-minute interval and 2 km spatial resolution produced by GK-2A. The accuracy of these variables produced by GK-2A is estimated by comparing with the collocated radiosonde data. In case of stability indices, the weighted linear regression coefficients for KI, LI, SSI, and TTI all showed values above 0.7, and the errors were randomly distributed without bias. The error for SSI and LI were larger at night than during the day, and the overall pattern of differences between satellite and radiosonde products was similar across stations. Furthermore, an analysis of 21 significant outlier cases that occurred during the comparison revealed that all outlier cases corresponded to one or more of the following: nighttime near-surface PBL, near-surface inversion layer, or instability in temperature and humidity profiles in the radiosonde data. LCL deviation ranged widely from -120 to 70, and RMSE varied between 30 and 130 based on initial ascent altitudes. Using 962.25 hPa as a reference, the deviation was -3.24, with an RMSE of 31.77, indicating the highest accuracy. Derived temperature and humidity profiles from GK-2A align closely with radiosonde data under suitable ascent altitudes. In selected convective cases, the LCL decreased by approximately 70.94 hPa (0.23 hPa/min) in the 6 hours before convective cloud formation, confirming a link between higher vertical convection altitudes and a heightened potential for strong convection. We also plan to present additional analysis on the relation of LFC and CAPE to the convective precipitation.
AS15-A031
Study on U-Net-based Deep Learning Model for Detecting Convective Initiation Probability Using GK2A/AMI Satellite Data
JinYoung KIM#+, Eunha SOHN, Myoung-Hee LEE
Korea Meteorological Administration, Korea, South
Convective clouds, accompanied by heavy rainfall and thunderstorms, can lead to substantial damages. Hence, the detection of Convective Initiation (CI) plays a crucial role in weather monitoring and prediction. While radar observations mainly detect precipitation particles in the mature stage of convective clouds, satellite data can identify convection cells before the formation of precipitation particles. Satellite data also offers the advantage of covering a wide area with high temporal resolution. In this study, we aimed to predict convective initiation by adopting the U-Net-based LightningCast model, originally developed for lightning prediction by NOAA/CIMSS, as our foundational model. Since the GEO-KOMPSAT-2A (GK2A) satellite lacks a lightning detection sensor like Geostationary Lightning Mapper (GLM), we employed ground-based radar reflectivity as ground truth. After aligning radar echoes with the GK2A Korean Peninsula area, we selected radar reflectivity that exceeded 35dBZ at least once within 60 minutes as our target data. We utilized observation data from GK2A Advanced Meteorological Imager (AMI) during the summer as input and conducted a study to identify the optimal channel combination through sensitivity testing. This research was supported by the “Technical development on high-impact weather detection and prediction using meteorological satellite data”(KMA2020-00121) of “Technical Development on Weather Forecast Support and Convergence Service using Meteorological Satellites” project funded by the National Meteorological Satellite Center, Korea Meteorological Administration.
AS15-A032
Prediction of Low-level Wind Fields Using ConvLSTM Model with GK2A and SCADA
Junghae HEUR#+, Yong-Sang CHOI
Ewha Womans University, Korea, South
Prediction of wind vectors in the low troposphere is beneficial in many application fields. Conventionally, Supervisory Control and Data Acquisition (SCADA) has been used for the low-level (1000 hPa) wind estimation. On the other hand, a recent study has developed the algorithm that can predict clear-sky high-level (500-750 hPa) wind vectors a few minutes to hours ahead using the Korean geostationary satellite (GK2A) water vapor channels only. Here we find the correlation between the two level wind fields from the GK2A and SCADA by using Convolutional Long Short-Term Memory (ConvLSTM) model. Then this model is applied to predict low-level wind fields for the entire Korean Peninsula. Our results show that our low-level wind fields have higher accuracy than those from the numerical weather prediction. Also shown is a potential that GK2A high-level wind can be used to predict low-level wind where the observations are unavailable. We expect that this study can serve to improve weather and wind power prediction.
AS15-A036
Quantitative and Qualitative Assessment of Geo-KOMPSAT-2A(GK-2A) Rapid-Scan Atmospheric Motion Vectors
Soobong LEE1#+, Kwang-Deuk AHN2, Inchul SHIN1
1Korea Meteorological Administration, Korea, South, 2National Institute of Meteorological Research, Korea, South
The Rapid-Scan Atmospheric Motion Vector (RS-AMV) provides satellite-based three-dimensional wind information, and it can be useful information for initializing numerical weather prediction(NWP) model through data assimilation. In addition, It can be useful for a forecaster to be tracking the convection cell and analyzing wind information around the typhoon. Advanced Meteorological Imagery (AMI) on board the GEO-KOMSAT-2A(GK-2A) can capture the imagery of East Asia every two minutes. With this advantage, the RS-AMV can be generated with better spatio-temporal resolution than AMV. RS-AMV is derived as following steps: 1) target selection via optimal method using largest standard deviation in specific area, 2) height assignment based on cross-correlation with Cloud Top Pressure (CTP) product, 3) calculate displacement between the similar pixels in earlier or later image, 4) assign quality information on each vectors in RS-AMV via comparison with surrounding pixels. In this study, the quantitative and qualitative evaluations were performed using in-situ observation and analysis fields from NWP model. As the results of the quality assessment, we found that the major issues of RS-AMV are height assignment and wind speed. Additionally, the cause of the problem and which parts of the algorithm caused the problem were presented. This study was carried out with the support of the Korea Meteorological Administration R&D program[Meteorological satellite forecast support and convergence service technology development] (KMA2020-00121).
AS15-A037
Research on Satellite Water Vapor Data Based Synoptic Meteorological Phenomena Analysis Methods
Ok Hee KIM#+
Korea Meteorological Administration, Korea, South
Water vapor imagery is a suitable satellite data to track upper atmospheric flow. It is useful for analyzing synoptic meteorological phenomena as tracking cyclonic flows, vorticities, dry areas and wet areas that appear in water vapor images, and identifying the location of troughs/ridges by utilizing the strengthening and weakening tendencies of dry areas and anticyclonic air flows. Synoptic meteorological phenomena can be analyzed extensively using water vapor image. Infrared and visible images are useful for analyzing clouds distributed in the upper, middle, and lower layers of the atmosphere. In water vapor images, upper-level waves and darkening-related troughs, which are precursor stages of low pressure system that cannot be seen in clouds that appear in visible and infrared images, can be identified through air flow analysis. In this study, we specifically showed some methods to analyze troughs through the tendency of dry areas to strengthen or weaken using water vapor imagery. Through this study, we found that the troughs are located right in front of the maximum brightness temperature area of the dry zone and the ridges are located in the area where the wet region begins to gradually dry in the water vapor image, and where the clouds begin to dissipate in the infrared and visible images.
AS15-A038
Atmospheric Temperature and Humidity Profiles from FY4B-GIIRS Measurements: Physical Algorithm AAP vs. ANN-based Algorithm
Kyungsoo LEE1+, Sang-Moo LEE1#, Jaeeon KIM1, Junhyung HEO2, Byung-il LEE2, Hoyeon SHI3
1Seoul National University, Korea, South, 2Korea Meteorological Administration, Korea, South, 3Danish Meteorological Institute, Denmark
Hyperspectral infrared (IR) sounder measures radiances at CO2 and H2O bands with high spectral resolution, and these measurements can be used to retrieve atmospheric temperature/ humidity profiles which are important in short-term weather forecasts. GIIRS (Geostationary Interferometric Infrared Sounder) of FY-4B is the first hyperspectral IR sounder in the geostationary orbit, and measures wide area with high temporal resolution. GIIRS-measured radiances contain vertical information on atmospheric CO2 and H2O, allowing to estimate atmospheric temperature/humidity from space. Of course, development of relevant retrieval algorithm is necessary. Improving weather forecasting capabilities, the Korean National Meteorological Satellite Center developed a physical algorithm so-called AAP (Advanced Meteorological Imager (AMI) Atmospheric Profile) for the retrieval of atmospheric thermodynamical properties. The AAP algorithm is based on the 1D-Var scheme and was originally developed for GEO-KOMPSAT-2A AMI sensor. In this research, sensitivity tests were conducted to find the best set of GIIRS channels and observation/background error covariances. Then obtained results were used for adapting the original AAP algorithm for GIIRS sensor. It was found that the modified AAP algorithm performs well with 36 GIIRS channels. Results indicate that the rms error of the modified AAP algorithm compared with ERA5 atmospheric profile is reduced when the observation error is prescribed as larger value. In addition, artificial intelligence algorithm was also developed for temperature/humidity retrievals by training GIIRS-measured radiances with collocated ERA5 atmospheric temperature/humidity profiles. ANN, CNN, ResNet, and U-Net methods were used, and results were compared for that purpose. GIIRS-measured TBs were directly related to ERA5 profiles without any first guess profile. The test results show that the algorithm based on ResNet yields the highest performance compared to the other algorithms. However, it is noted that these neural network algorithms perform not better than the physical algorithm in terms of rms errors.
AS15-A040
Regional Characteristics of Aerosol Optical Depth from GOCI-II Over East Asia
Joonhee KIM1+, Sang-Moo LEE1#, Hyeong-Ahn KWON2
1Seoul National University, Korea, South, 2University of Suwon, Korea, South
Geostationary Ocean Color Imager – II (GOCI-II) onboard GEO-KOMPSAT-2B has operated since 19 February 2020 and has monitored aerosol optical depth (AOD) over East Asia. Although GOCI-II has provided invaluable AOD datasets such as hourly measurements, biases of GOCI-II AOD are not sufficiently analyzed to exploit GOCI-II AOD data in a data assimilation system for air quality forecast. This study aims to analyze the characteristics of GOCI-II AOD data in terms of bias and root mean square (RMS) error from December 2021 to January 2023, by comparing GOCI-II data with aerosol optical properties derived from the AErosol RObotic NETwork (AERONET) data. To make comparable datasets between GOCI-II and AERONET, GOCI-II AODs were averaged within a square grid box centered on each AERONET site having size of xo. The sensitivity test was conducted by increasing the grid box size x from 0.1˚ to 1.0˚ with the increment of 0.1˚. The bias of GOCI-II AOD to AERONET AOD depends on the selected grid box size in most AERONET sites, showing smaller biases as grid box size decreases, possibly due to data representativeness. It is expected that there will be certain threshold at which bias will not decrease further. In addition, bias of GOCI-II AOD according to the aerosol type was examined. Here, aerosol types were classified into 6 categories: dust, non-absorbing coarse, mixture, high-absorbing fine, moderating-observing fine, and non-absorbing fine. AOD over the eastern China showed higher value compared to neighboring countries during the study period. The characteristics of GOCI-II AOD identified by this study will be utilized to improve a design of pre-processing process of satellite-derived AOD for data assimilation.
AS15-A041
Comparison of AMV Calculated Using Optical Flow Method and GK2A Rapid-Scan-AMV
Ji-Hoon JEONG#+, Inchul SHIN
Korea Meteorological Administration, Korea, South
Atmospheric Motion Vector (AMV) is a satellite product that tracks atmospheric current by monitoring the movement of clouds and water vapor in three sequential satellite images. It is valuable for enhancing the precision of forecast and analysis fields in numerical model data assimilation. Additionally, it's crucial for understanding wind structures in typhoons. The National Meteorological Satellite Center (NMSC) from Korea Meteorological Administration (KMA) is currently producing Rapid-Scan (RS)-AMV, which has an improved spatiotemporal resolution than AMV, using the rapid-scan data from Geo-Kompsat-2A (GK2A). This output features a height assignment technique that utilizes Cloud Top Pressure (CTP) to obtain local wind information with less reliance on numerical weather prediction (NWP) models. In this study, we focused on increasing the vector count by computing vectors through optical flow. We analyzed atmospheric current using these vectors and validated the accuracy of the optical flow AMV by comparing them with RS-AMV. Optical flow is a technique that calculates the movement of pixels between two image frames as vectors. we used the Farnebäck algorithm, which calculates this movement for all pixel values in the image. Height assignment using GK2A Cloud Top Pressure (CTP) was applied to the optical flow AMV. The optical flow AMV calculated in this way was verified qualitatively and quantitatively through case analysis and observation data such as radiosonde and wind profiler.
AS15-A043
Improvement of GK-2A Atmospheric Vertical Information with PCA
Junhyung HEO#+, Byung-il LEE, Myoung-Hee LEE
Korea Meteorological Administration, Korea, South
The GK-2A AAP (Geo-Kompsat-2A AMI Atmospheric Profile) and other 1D-Var atmospheric profile retrieval algorithms have common limitations related to ill-posed problems due to a lack of observed information, leading to unstable retrieved profiles or reliance on initial guess profiles. In our study, we addressed these challenges by employing Empirical Orthogonal Functions (EOFs) and Principal Components (PCs) for temperature and humidity profiles to mitigate the ill-posed equation problem through variable reduction. The number of components of vertical profile was reduced using main EOFs and PCs. Furthermore, we modified the GK-2A AAP based on Principal Component Analysis (PCA-AAP) to achieve optimized atmospheric vertical information. The temperature and humidity profiles were calculated using PCA-AAP, with the Unified Model (UM) and GK-2A radiance serving as inputs, mirroring the approach employed in GK-2A AAP. Validation of the PCA-AAP retrieved profiles was conducted using radiosonde data in August 2022. The accuracy of PCA-AAP was found to be nearly comparable to that of both the initial guess and GK-2A AAP. Notably, PCA-AAP successfully avoided retrieving inaccurate profiles observed in GK-2A AAP, attributed to the stabilizing effect of main EOFs. The results demonstrate that the PCA technique complements the GK-2A AAP algorithm, providing stable and continuous vertical profiles. Consequently, we plan to enhance the accuracy of EOFs by incorporating global radiosonde data and model analysis data. This improvement is anticipated to contribute significantly to supporting very short-range forecasting and nowcasting more effectively. This research was supported by the “Technical development for utilizing meteorological satellite data for numerical weather predication”(KMA2020-00122) of “Technical Development on Weather Forecast Support and Convergence Service using Meteorological Satellites” project funded by the National Meteorological Satellite Center, Korea Meteorological Administration.
AS15-A053
Using Machine Learning to Convert Satellite Images Into Radar Reflectivity for Rainfall Intensity
Po Che HUANG1+, Chuan-Ming LIU1#, Lawrence Jing-Yueh LIU2,3
1National Taipei University of Technology, Taiwan, 2University of Illinois Urbana-Champaign, United States, 3National Central University, Taiwan
Extreme weather often causes major disasters, such as the flash flood brought by intense rainfall. To assess rainfall position and intensity, we usually use satellite images and radar reflectivity as a reference. Radar reflectivity provides high-resolution information of rainfall structure, but the range that radar can detect is limited based on the location and range of each radar site. In remote areas or places such as the Pacific Ocean, the radar data cannot cover. In contrast, satellite images offer a broader range of coverage, providing information in a global scale. Therefore, we propose a machine learning framework to train models that combines radar reflectivity and satellite image data. Firstly, the visible light and infrared data are obtained from the Himawari-9 satellite in Taiwan area from July to December, 2023. Then, the radar reflectivity is provided by the Taiwan Central Weather Administration (CWA) in Taiwan area as labels. In this study, the U-net model captures the features of satellite images to predict rainfall intensity and generate radar reflectivity. The reason we choose U-net is because of its excellent performance in image segmentation. Hence, it is an optimal choice to identify the edges of cloud layers and predict rainfall intensity. This research not only aims to extend the detection range of radars, providing more comprehensive weather information, but also helps observe the formation and causes of typhoons and other severe rainfall events. This efficient framework can contribute to monitor various extreme weather conditions and provide real-time warnings, thereby reducing the losses caused by disasters.
AS23-A001
| Invited
Characteristics of Land Atmospheric Interaction as a Result of Plant Response in the East Asia and Its Impact on the Extreme Climate Events
Ji-Hye YEO1+, Daeha KIM2, Yeonghwa KO1, Kyung-Ja HA1#
1Pusan National University, Korea, South, 2Jeonbuk National University, Korea, South
In recent times, global temperatures have been rising due to global warming, with East Asia being one of the regions experiencing the highest rate of increase. Furthermore, under high CO2 emission scenarios, the increasing evaporative demand in the East Asia region is projected to rise more rapidly than land surface evaporation. This land-atmosphere moisture difference exhibits high vapor pressure deficits, which can lead to extreme temperatures and droughts. The estimation of potential evapotranspiration, a key indicator of evaporative demand, remains unclear in the available reanalysis or model data, as they do not account for plant responses to CO2. We only focused on stomatal changes in response to CO2 changes, and the results showed an increase in surface resistance with increased CO2, the effect of which was largely offset by vapor pressure deficits, which affects the increase in potential evapotranspiration. In particular, in the case of drought, when plant responses are not considered, potential evapotranspiration tends to overestimate drought in East Asia by approximately 17% compared to scenarios that take vegetation into account. We examined the characteristics of land-atmosphere interactions in East Asia based on land types using a land-atmosphere coupling matrix. Specifically focusing on the characteristics of land-atmosphere coupling and its changes with and without considering plant responses, we analyzed the resulting changes in extreme climate events such as heatwaves and droughts.
AS23-A006
The Forecast Skill of the Summer Precipitation Over Tibetan Plateau Improved by the Adoption of a 3D Sub-grid Terrain Solar Radiative Effect Scheme in a Convection-permitting Model
Anning HUANG#+
Nanjing University, China
We have successfully incorporated a 3-dimensional sub-grid terrain solar radiative effect (3D STSRE) parameterization scheme into a convection-permitting Weather Research and Forecasting model (WRF_CPM) in this study. Impacts of 3D STSRE scheme on the ability of WRF_CPM in forecasting the precipitation in summer over the Tibetan Plateau (TP) and nearby regions with complex terrain have been systematically addressed by conducting experiments without and with the 3D STSRE scheme. Results show that the application of 3D STSRE scheme can obviously mitigate the overestimation of surface solar radiation (SSR) and rainfall over TP and nearby regions, especially over the areas with much more rugged terrain (i.e., southern TP) in the WRF_CPM without 3D STSRE scheme. Further mechanism analyses indicate that the decreased surface heating induced by the reduction of SSR reduces the intensity of the thermal-low pressure over the TP, which leads to the diminished strength of southwesterly winds and thereafter the weaker convergence of moisture flux over the southern TP. Moreover, the weakened surface thermal forcing makes the local atmosphere more stable, suppressing the vertical water vapor transport and local convection. These effects greatly alleviate the overestimation of precipitation over the southern TP produced by the WRF_CPM without the 3D STSRE scheme.
AS23-A007
Changes in the Spatiotemporal Distribution of the Timing and Duration of the Soil Freeze–thaw Status from 1979 to 2018 Over the Tibetan Plateau
Xin LAI#+, Siyuan YAO
Chengdu University of Information Technology, China
Changes in the soil freeze–thaw status will inevitably affect the thermal conditions and properties of the Tibetan Plateau (TP), thereby affecting its upper atmosphere, and further afield in East Asia and even globally. In this study, using the soil temperature simulated by the Community Land Model Version 5.0, the timing and duration of the soil freeze–thaw status were divided into freeze start-date, freeze end-date, and freeze duration. Results showed: (1) The model effectively reproduces seasonal multi-layer soil temperature changes, showing strong correlation with observations. (2) There is a clear trend of delayed freezing, advanced thawing, and shortened freeze duration from northwest to southeast over the TP. From 1979 to 2018, the freeze start-date was delayed by 7.3 days (1.9 days/decade), the freeze end-date advanced by 6.4 days (1.7 days/decade), and the freeze duration shortened by 13.7 days (3.6 days/decade). The timing and duration of the soil freeze–thaw status vary across different regions of the TP. The freeze start-date in all areas of the TP has been delayed in the past 39 years. Except for the sub-cold zone and arid regions of the TP, the freeze end-date has occurred earlier and the freeze duration has shortened, with the most significant changes in the sub-cold zone and humid regions. (3) The timing and duration of the soil freeze–thaw status are significantly correlated with surface air temperature, elevation, and latitude. The strongest correlation is with surface air temperature, followed by altitude and latitude. The western TP shows a stronger correlation than the eastern TP. The rate of change in the soil freeze–thaw status increases with altitude to 3000 m above sea level, while this rate decreases with elevation above 3000 m. The greatest rate of change is observed at 29°N.
AS23-A008
Biophysical Impact of Greening Vegetation on Near-surface Air Temperature Under Hot Extremes
Yipeng CAO+, Weidong GUO#, Jun GE
Nanjing University, China
Satellite data shows increasing leaf area of vegetation since 2000, which may exert biophysical effects on near-surface air temperature (SAT). However, such effects remain largely unknown because prior studies either focus on land surface temperature, which differs from SAT, or rely on simulations, which are limited by model uncertainties. As a widely used metric in climate and extremes research, SAT is more relevant to human health and terrestrial ecosystem functions. Therefore, it is necessary to explore impacts of greening on SAT and extremes based on observations. Here, we investigate the greening effects on SAT and subsequent extremes over 2001–2022 based on an enhanced global dataset for the land component of the fifth generation of European ReAnalysis (ERA5-land). We find that greening can cause cooling effects on the mean SAT and more pronounced cooling effects on SAT extremes in Europe, East Asia and Central North America, where evident greening was observed since 21st century. An attribution analysis suggests that the main driving factor for the additional cooling effect of greening in hot extremes is the enhanced evapotranspiration. Moreover, the biophysical effects of vegetation on high temperatures vary with climate conditions and vegetation types. Our study reveals a considerable climate benefit of greening on SAT, which may have implications for climate mitigation in different regions around world.
AS23-A010
Research on Estimation/prediction of Surface Solar Irradiance Based on Machine Learning
Dongyu JIA#+
Lanzhou City University, China
This study used radiation observation data and remote sensing data to explore the different factors affecting radiation estimation and prediction based on machine learning algorithms. The results indicate that: (1) The estimation of radiation is influenced by weather condition levels and pollution levels, where the estimation of global solar radiation is linearly related to the weather condition level, while the diffuse solar radiation shows a non-linear relationship. In heavily polluted weather, the use of machine learning for solar radiation estimation performs poorly. (2) In all prediction scenarios, the feature selection (FS) of the Random Forest (RF) model is higher than that of the Support Vector Regression (SVR) model, and this performance advantage becomes more pronounced when the lead time exceeds 90 minutes. (3) Remote sensing data can assist in improving radiation prediction. Full-channel input of FY-4A remote sensing data can provide better prediction results, but considering time and computational cost, the optimal three-channel model is a better choice.
AS23-A012
Can Climate Models Accurately Capture the Sub-seasonal Dynamics of Tibetan Plateau Snow Cover?
Xin MIAO#+, Weidong GUO
Nanjing University, China
The snow cover on the Tibetan Plateau (TP) undergoes sub-seasonal changes, which exert a substantial influence on weather and climate in the surrounding and downstream regions. However, current climate models struggle to accurately capture the rapid changes of TP snow cover. Our research indicates that, most global climate models in phase 6 of the Coupled Model Intercomparison Project (CMIP6) largely overestimate the snow amount over the TP, along with notable biases in the rapid fluctuations of TP snow cover. Similarly, these biases are also present in regional climate simulations. Through in-depth analysis, we identify snowfall and snowmelt as primary contributors to the observed rapid changes in TP snow cover. The simulated biases in rapid snow changes over the TP result from the excessive snowfall and albedo bias in both global and regional climate simulations. Our findings reveal the potential sources of simulated biases in rapid snow changes over the TP and offer a promising perspective for improving the accuracy of TP regional and global climate simulations.
AS23-A013
Interdecadal Response of Eurasia Snow Cover to Northern Hemisphere Sea Surface Temperature
Xianru LI+, Zhigang WEI#
Beijing Normal University, China
Based on reanalysis data from ERA5_Land, MEERA2, HadISST, NCEP-NCAR reanalysisⅠ and other datasets, the response characteristics between interdecadal Eurasia snow cover in winter and spring and sea surface temperature in Northern Hemisphere (NHSST) in winter are investigated. Barnett and Preisendorfer canonical correlation analysis (BP-CCA) and regression analysis are used in this paper. Main conclusions are as follows: In the past 40 years, except for Equatorial East Pacific region, the NHSST has increased. And except for eastern Siberia, the snow cover basically decreased. The interdecadal influence of winter NHSST on Eurasia snow cover lasts until spring after removing the linear trend. In the first mode of BP-CCA, winter and spring snow cover increase in Europe and decrease in central Eurasia when the North Atlantic and Northwest Pacific Sea temperatures rise (AMO+, PDO-) in winter. At this time, the height field and surface temperature decrease, water vapor and precipitation increase, trough deepens in Europe, and then snow cover increases in winter and spring. In central Eurasia, the variations are revised. In the second mode of BP-CCA, there is a significant reverse change between snow cover over Eurasia and Northeast Pacific SST with a quasi-16a period, and the North Atlantic SST is a tripole type. When the SST increases in the Northeast Pacific Ocean and the mid-latitude Atlantic Ocean in winter, the trough and ridge in Eurasia all weaken, surface temperature increase, and then winter snow cover decrease. In spring, the water vapor flux and precipitation decreased significantly, and snow cover decreased.
AS23-A015
Preference of Afternoon Precipitation Over Dry Soil in the North China Plain During Warm Seasons
Sixuan LI1+, Jianping GUO2, Zhanqing LI3,1#, Xuanze ZHANG4, Tianning SU3, Jing WEI3
1Beijing Normal University, China, 2Chinese Academy of Meteorological Sciences, China, 3University of Maryland, United States, 4Chinese Academy of Sciences, China
The influence of soil moisture on atmospheric precipitation has been extensively studied, but few of these studies have considered the role of land-atmosphere coupling in afternoon precipitation events at a sub-daily timescale. Here, using in-situ observations and reanalysis datasets, we investigated the effect of the soil moisture anomaly (SMA) on warm seasons’ afternoon precipitation in the North China Plain (NCP), which is identified as a strong land-atmosphere coupling region. Afternoon precipitation events (APE) were separated from all precipitation events in the NCP during the warm seasons of 2010 to 2019. It follows from a comparative analysis that APE is more likely to be initiated on drier soil, which has little dependence on the thresholds used for identifying APE. However, no affirmative relationship is found between precipitation amount in the first hour of APE (APE1hour) and the soil moisture. Further analyses indicate that larger amounts of APE1hour result from higher convective available potential energy (CAPE), higher moist static energy (MSE), or weaker vertical shear of horizontal wind. When considering the joint effects of SMA and atmospheric variables, APE tend to occur on drier (wetter) soil with lower (higher) lower-tropospheric stability, CAPE, or MSE. This study highlights the significant roles of land-atmosphere interactions on local atmospheric precipitation, especially the joint roles of soil moisture and atmospheric variables on precipitation.
AS23-A016
Biophysical Factors Control the Interannual Variability of Evapotranspiration in an Alpine Meadow on the Eastern Tibetan Plateau
Shaoying WANG1#+, Yu ZHANG2, Xianhong MENG1, Lunyu SHANG1, Zhaoguo LI1
1Chinese Academy of Sciences, China, 2Chengdu University of Information Technology, China
Evapotranspiration (ET) is a key parameter regulating land–atmosphere interaction processes and the water cycle. The seasonal and interannual variability of ET and its environmental controls over an alpine meadow in a subfrigid humid zone of the Tibetan Plateau (TP) are reported on. Direct measurements were made using the eddy covariance method over a 10-year period with a significant increase in growing season length (GSL). The results showed that annual ET for the alpine meadow site was 492 ± 66 mm in comparison with 635 ± 88 mm of precipitation (P), with a ratio of ET/P ranging from 0.63 (2017) to 1.04 (2010). The path analysis and Priestley–Taylor coefficient (ET/ETeq) revealed that the daily ET experienced energy-limited and water-limited seasons within the year. During the water-limited non-growing season, the daily surface conductance (Gs) and ET/ETeq increased positively with soil water content (SWC). During the energy-limited growing season, the 16-day average ET, ET/ETeq, and Gs scaled positively with the normalized difference vegetation index (NDVI). ET/ETeq increased nonlinearly with an increase in Gs, but was insensitive to increases in Gs greater than the threshold Gs*. The mean Gs and Gs* were strongly regulated by the maximum NDVI. The maximum NDVI, Gs*, and annual mean Gs explained 46%, 80%, and 68%, respectively, of interannual variation in annual ET. Thus, we concluded that biophysical factors, rather than P and GSL, mainly controlled the interannual variability in annual ET. These findings are critical for understanding the response mechanism of ET to the changing biotic and abiotic conditions in the TP.
AS23-A018
Simulation of Regional Soil Moisture at High Spatiotemporal Resolution Using WRF-Hydro
Chin-Chi YEH#+, Chia-Jeng CHEN
National Chung Hsing University, Taiwan
Soil moisture is one of the critical variables in the hydro-climate system; however, the gauge-based measurement poses a great challenge in its spatial coverage. To obtain more comprehensive soil moisture data over Taiwan, this study aims to leverage the Weather Research Forecasting model-Hydrological modeling system (WRF-Hydro). To ensure a more reliable regional simulation, the default soil texture, soil hydraulic parameters, and land use/cover data in WRF-Hydro are replaced with locally curated data to better reflect the actual surface characteristics of Taiwan. The Taiwan Hydraulic Digital Elevation Model (HyDEM) is used to configure catchment characteristics in the pre-processing of WRF-Hydro. Gauge- or radar-based precipitation is used as the meteorological forcing to drive WRF-Hydro. Simulated soil moisture will be compared and validated with gauge- and satellite-based data in Taiwan. We believe that the outcome of this work will provide more effective soil moisture information for ensuing hydro-climatic modeling and disaster monitoring.
AS27-A006
Aerosol as a Potential Factor to Control the Increasing Torrential Rain Events in Urban Areas Over the Last Decades
Seoung Soo LEE#+
Earth System Science Interdisciplinary Center, United States
This study examines the role played by aerosol in torrential rain that occurred in the Seoul area, which is a conurbation area where urbanization has been rapid in the last few decades, using cloud-system-resolving model (CSRM) simulations. The model results show that the spatial variability in aerosol concentrations causes the inhomogeneity of the spatial distribution of evaporative cooling and the intensity of associated outflow around the surface. This inhomogeneity generates a strong convergence field in which torrential rain forms. With the increases in the variability in aerosol concentrations, the occurrence of torrential rain increases. This study finds that the effects of the increases in the variability play a much more important role in the increases in torrential rain than the much-studied effects of the increases in aerosol loading. Results in this study demonstrate that for a better understanding of extreme weather events such as torrential rain in urban areas, not only changing aerosol loading but also changing aerosol spatial distribution since industrialization should be considered in aerosol–precipitation interactions.
AS27-A007
Impacts of an Aerosol Layer on a Mid-latitude Continental System of Warm Cumulus Clouds: How Do These Impacts Depend on the Vertical Location of the Aerosol Layer?
ChangHoon JUNG1#, Seoung Soo LEE2+, Junshik UM3
1Kyungin Women's University, Korea, South, 2Earth System Science Interdisciplinary Center, United States, 3Pusan National University, Korea, South
Effects of an aerosol layer on warm cumulus clouds in the Korean Peninsula when the layer is above or around the cloud tops in the free atmosphere are compared to those effects when the layer is around or below the cloud bases in the planetary boundary layer (PBL). For this, simulations are performed using the large-eddy simulation framework. When the aerosol layer is in the PBL, aerosols absorb solar radiation and radiatively heat up air enough to induce greater instability, stronger updrafts and more cloud mass than when the layer is in the free atmosphere. Interestingly, even though the aerosol layer in the PBL intercepts more solar radiation reaching the surface, resulting in reduced surface heat fluxes, instability, updraft intensity, and cloud mass, the overall effect still leads to more cloud mass. Hence, there is a variation of cloud mass with the location of the aerosol layer, which arises from an interplay between aerosol-induced changes in the surface fluxes and those in radiative heating of air. Even without impacts of aerosols on radiation, there is still more cloud mass when the aerosol layer is in the PBL, because aerosol-induced changes in droplet nucleation induces aerosol-induced invigoration of updrafts. However, the variation of cloud mass is much smaller when there is only aerosol impacts on droplet nucleation than when aerosol impacts on both of radiation and nucleation are present. Hence, aerosol impacts on nucleation and those on radiation work together to amplify the variation of cloud mass with the altitude of the aerosol layer. This study reveals that this variation of cloud mass also reduces as aerosol concentrations in the layer decrease. Furthermore, the transportation of aerosols by updrafts reduces aerosol concentrations in the PBL.
AS27-A009
Physical Properties of Clouds Embedded in the Cold-air Outbreaks Over the Yellow Sea Depending on Air Pollution
Subin JEON+, Hyunho LEE#
Kongju National University, Korea, South
In middle and high latitudes, marine stratocumulus clouds often form after cold fronts pass, with cold air flowing from the continents during winter. Because these stratocumulus clouds persist over a relatively broad region and a relatively long duration compared to clouds associated with typical low-pressure systems, they can produce significant cloud radiative forcing, which is negative owing to their low altitudes and large cloud water contents. As they move downwind, they usually experience transition to cumulus clouds with lower cloud fraction. While increasing sea surface temperature has been recognized as the main factor to control the transition, some recent studies have pointed out that precipitation, which can be modulated by aerosols, is also important to the transition. In this study, we present the physical properties of boundary-layer clouds embedded in the cold-air outbreaks over the Yellow Sea occurred from 2013 to 2023. We identify the entire cases seen on the MODIS observations during the period, a total of 119 cases. The cloud fraction peaks at the middle of the cloud trajectories and then decreases as the clouds move downwind. The cloud top temperature generally increases along the trajectories although the cloud top height is also increasing, while the cloud water path remains relatively unchanged as the clouds move downwind. Beyond analyzing the mean properties of the entire cold-air outbreak stratocumulus clouds, we select some cases and categorize them as either ‘clean’ or ‘polluted’ based on the average carbon monoxide concentration over the upwind region of the trajectories. We then illustrate the effects of pollution on the cloud evolution by comparing the properties of the two cloud groups. Additionally, we conduct a series of numerical simulations and examine in detail how aerosols influence the cloud evolution and the transition to cumulus clouds.
AS27-A010
The Spatiotemporal Characteristics of Precipitation and Particulate Matter, and the Impacts of Wet Removal Based on Long-term Surface Measurements in Korea
Junshik UM1#+, Suji HAN1, Seoung Soo LEE2, ChangHoon JUNG3
1Pusan National University, Korea, South, 2Earth System Science Interdisciplinary Center, United States, 3Kyungin Women's University, Korea, South
Precipitation is an important process that contributes to the energy budget of the earth by modulating the water cycle and also assists in controlling the concentration of atmospheric pollutants by scavenging particulate matter (PM) (i.e., wet removal). Previous studies attempted to quantify the impact of wet removal mechanisms on PM concentrations, however, they performed the research based on short-term measurements, limited sites, or a few precipitation event cases. Thus, this study showed the spatiotemporal characteristics of precipitation and the concentration of PM (i.e., PM2.5 and PM10) in six regions (i.e., Seoul, Busan, Daejeon, Daegu, Gwangju, and Jeju) individually, and quantified the impact of the wet removal on the concentration of PM by precipitation events based on long-term measurements in six regions in Korea. Precipitation and PM10 surface measurements in six regions were used for 22 years (2001-2022), while PM2.5 surface measurements were only available for 8 years (2015-2022). All measurements were made with a one-hour resolution. The spatiotemporal variabilities (i.e., yearly, seasonal, and monthly averages) of precipitation and the concentration of PM were calculated in each region. The precipitation events were identified when the threshold time interval (i.e., 2 hours) was presented within the hourly precipitation data. Based on the duration, average intensity, and accumulated amount of precipitation events, the characteristics of precipitation events were analyzed. The variation in the concentration of PM during the precipitation events and the rate of wet removal were quantified as functions of the characteristics of precipitation events (i.e. duration, average intensity, and accumulated amount of precipitation events) for each of the six regions. The spatiotemporal characteristics of the regional wet removal effects that occurred by precipitation events were calculated, and the influence of the precipitation properties on the wet removal effects was evaluated.
AS53-A003
Ensemble Coupling of the Atmospheric Model NICAM
Takashi ARAKAWA1#+, Hisashi YASHIRO2, Kengo NAKAJIMA1
1The University of Tokyo, Japan, 2National Institute for Environmental Studies, Japan
Meteorological phenomena are highly nonlinear, and small differences in initial values can significantly affect the results. Therefore, ensemble calculations are a commonly used computational technique in weather/climate simulations to reduce the inevitable uncertainty inherent in individual simulations and to quantitatively evaluate the degree of uncertainty. However, obtaining an average value with sufficient accuracy requires a large number of ensembles, which in turn requires significant computational resources. For example, in the case of the atmospheric model NICAM with a resolution of 3.5 km and 1024 ensembles, 131072 nodes were used, but with this number of nodes, it was not possible to calculate 1024 ensembles at once, and a method of repeating 4 cycles of 256-member ensemble calculations per cycle was employed. Therefore, in our study, we coupled a low-resolution ensemble with single high-resolution computation. This method can replace high-resolution large-scale ensembles with fewer computational resources. Furthermore, we can expect to obtain more accurate results by coupling low-resolution calculations, which excel in reproducing large-scale fields, with high-resolution calculations, which excel in reproducing detailed fields. A general-purpose coupler, h3-Open-UTIL/MP, was applied to this study. Two execution modes are possible on this coupler: many-to-one coupling, where multiple ensemble runs are coupled to a single model, and many-to-many coupling, where multiple coupled models are executed as an ensemble. In this study, the later mode was applied. We coupled low resolution NICAM ensemble and high resolution NICAM single model, on the Wisteria/BDEC-01 of the University of Tokyo. For the calculations, optimization of the single model and variable resource allocation were applied to minimize computational resources (node-time) as much as possible. In this presentation, the details of the ensemble coupling will be explained and the computational performance will be discussed.
AS53-A005
Parallelized Remapping Algorithms for KM-scale Global Weather and Climate Simulations with Icosahedral Grid System
Chihiro KODAMA1#+, Hisashi YASHIRO2, Takashi ARAKAWA3, Daisuke TAKASUKA3, Shuhei MATSUGISHI3, Hirofumi TOMITA4
1Japan Agency for Marine-Earth Science and Technology, Japan, 2National Institute for Environmental Studies, Japan, 3The University of Tokyo, Japan, 4RIKEN Advanced Institute for Computational Science, Japan
Speeding up the post-processes in addition to the weather and climate simulation itself is important for speeding up the overall workflow. There are a wide variety of post-processes, but one typical post-process required for many models is remapping from model native grids to latitude-longitude grids. Here, we developed a series of parallelized remapping algorithms for NICAM, a global weather and climate model with an icosahedral grid system, and demonstrated their performance with global 14-0.87-km mesh model data on the supercomputer Fugaku. The original remapping tool in NICAM supports parallelization only in reading and interpolating data. In our proposed algorithms, the process of data writing is parallelized by separating output files or using the MPI-IO library, both of which enable us to remap 0.87-km mesh data with 670 million horizontal grid points and 94 vertical levels. The benchmark with 14-km mesh data shows that the developed algorithms significantly outperform the original algorithm in terms of elapsed time (by 7.4-8.7 times) and memory usage (by 2.8-5.0 times). Among the proposed algorithms, the separation of output files, along with reduced MPI communication size, leads to a better performance in the elapsed time and its scalability, and the use of the MPI-IO library leads to a better performance in memory usage. The remapping year per wall-clock day, assuming a six-hourly output interval, is up to 0.56 with 3.5-km mesh data, demonstrating the feasibility of handling global cloud-resolving climate simulation data in a practical time. This study demonstrates the importance of IO performance, including MPI-IO, in accelerating weather and climate research on future supercomputers.
AS53-A013
Kilometer-scale Global Weather Forecasting Using the Korean Integrated Model: A Case Study of Extreme Heavy Rainfall in the Korean Peninsula
Ilseok NOH#+, Heeje CHO, Junghan KIM, Woo-Jin LEE
Korea Institute of Atmospheric Prediction Systems, Korea, South
The Korean Integrated Model (KIM) is a global weather forecast model independently developed by the Korea Institute of Atmospheric Prediction Systems (KIAPS). Comprising a spectral element-based dynamical core and a scale-aware physics package on cubed-sphere grids, KIM is currently deployed by the Korea Meteorological Administration (KMA) in a 12 km resolution, with data assimilation for weather forecasting. However, acknowledging the challenges in accurately simulating precipitation systems, particularly sudden and intense heavy rains around the Korean Peninsula, there is a growing need for a higher resolution model. In this study, we attempted to simulate KIM with a 3-4 km horizontal resolution, strategically avoiding cumulus parameterization specifically for cases of extreme heavy rainfall. The primary aim was to assess the possibility of positioning KIM as a Global Cloud-Resolving Model (GCRMs). As a result, KIM demonstrating a stable 10-day simulation of extreme rainfall case and more realistic compared to the 8 km simulation.
AS59-A005
Retrieval of AOD Over Shallow and Turbid Coastal Waters from Himawari-8
Zibo YOU+, Yi WANG#
China University of Geosciences, China
Himawari-8, as a geostationary satellite, carries Advanced Himawari Imager which can perform full-disk observations every 10 minutes. Due to coastal water being turbid, shallow, and mixed with the land, the aerosol retrieval product cannot accurately retrieve the Aerosol Optical Depth (AOD) over shallow and turbid coastal waters. To fill the gap in this area, we developed a coastal water retrieval algorithm with a spatial resolution of 2 km. The land mask is first performed by normalized difference water index (NDWI), and then the cloud mask is performed by a spatial variation test based on 2.3 μm and some traditional reflectance and bright temperature threshold tests. After that, the water pixels are classified into open ocean pixels and coastal pixels by power-law fitting algorithm and Elevation and Topography at 1 arc minute (ETOPO1) bathymetry. After performing gas correction, the AOD and aerosol properties were retrieved using the Dark-Target algorithm for the open ocean pixels. For the coastal pixels, the AOD was retrieved using the 2.3 μm top of atmosphere reflectance and the aerosol properties of the nearest open ocean pixel. This algorithm can improve the accuracy and coverage of the coastal AOD.
AS59-A009
Observation of the Background Levels of Atmospheric Aerosols and Greenhouse Gases Around Taiwan
Charles CHOU#+, Chih-Chung CHANG, Mao-Chang LIANG
Academia Sinica, Taiwan
Since the industrial revolution, human beings have produced a large amount of air pollutants. Air pollution results in changes in the atmospheric composition, which in turn alters the energy budget of the Earth system and, consequently, causes the present-day climate crisis. The main climate active substances in the air pollutants include the greenhouse gases and atmospheric aerosols. The greenhouse gases absorb IR radiation and cause warming of the atmosphere, whereas aerosols could cause warming or cooling effects, depending on the microphysical and optical properties. The eastern Asia is among the most polluted regions in the world. Along the course of energy transition and air pollution mitigation, monitoring data provide the crucial evidence to evaluate the status of environmental changes. This study has been conducting observation of atmospheric aerosols (PM10) and major greenhouse gases (CO2, CH4, N2O) at three remote sites (Penghu, Green Island, Cape Fuguei) around Taiwan. The preliminary results of observation for 2018 – 2019 showed that, in terms of annual mean level, the background mixing ratios of CO2, CH4, and N2O were 418 ppmv, 1.95ppmv, and 334.3 ppbv, respectively. Moreover, according to the observation data from the Penghu, Green Island and Cape Fuguei research stations, we estimated the background level of atmospheric aerosols (annual mean of PM10) was 30.6 ugm-3.
AS59-A014
Application of GEMS AOD Data on Satellite- and Model-based Monitoring of Haze from Forest Fires in Southeast Asia
Efthymia PAVLIDOU1#+, Zhong Yi CHIA2, Chee-Kiat TEO2, Boon Ning CHEW2
1Meteorological Service Singapore, Singapore, 2Centre for Climate Research Singapore, Singapore
At the Meteorological Service of Singapore, Himawari geostationary data are used for transboundary haze monitoring and retrieval of Aerosol Layer Height with the application of different Random Forest architectures and Sentinel-5p/TROPOMI training data. The Numerical Atmospheric-dispersion Modelling Environment (NAME) is used for dispersal modelling and forecasting of forest fire emissions, and for further derivation of AOD. We evaluate performance of the system in recent haze incidents using the GEMS AOD product as reference. GEMS is the first satellite sensor dedicated to atmospheric monitoring in geostationary orbit, providing hourly AOD and Aerosol Layer Height information. The aim of this study is to explore the potential of GEMS to support operational, high frequency haze monitoring and validation of dispersion model outputs, specifically in the challenging environment of Southeast Asia.
AS59-A017
Long-term Trend Analysis of Asian Aerosol Optical Depth Based on Ground-based Observational Data
Yujin CHAI1#+, Jhoon KIM1,2, Yeseul CHO1
1Yonsei University, Korea, South, 2Korean Academy of Science and Technology (KAST), Korea, South
Aerosols are closely associated with air quality, climate change, and public health. Moreover, aerosol concentrations exhibit significant regional variations and considerable temporal fluctuations. Therefore, studying the long-term changes in aerosol concentration and analyzing the trends are essential for air quality improvement and climate change research. In this study, we present the long-term trends of Aerosol Optical Depths (AODs) across Asia and compare the trends of Fine-mode Aerosol Optical Depths (FAODs) and Coarse-mode Aerosol Optical Depths (CAODs). AOD represents the attenuation of solar radiation due to aerosols in the entire atmosphere, serving as an indicator of aerosol quantity. The Aerosol Robotic Network (AERONET) is a ground-based observational network providing information on aerosol optical properties worldwide. AERONET holds long-term data and offers continuous observations through daily measurements. For this reason, we analyzed the long-term trends of AOD using AERONET data. To examine changes in aerosol quantity attributed to anthropogenic sources and yellow dust, we presented trends in Coarse-mode Aerosol Optical Depths (CAODs) and Fine-mode Aerosol Optical Depths (FAODs), categorizing aerosols based on size. By comparing CAODs and FAODs, common trends were identified in trend analysis across countries or sub-regions. Through this analysis, it becomes evident that aerosol concentrations vary significantly regionally. However, it is apparent that factors such as each country's local environment and air quality policies exert substantial influence on aerosol trends.
AS59-A028
Surface Reflectance and Aerosol Type Optimization for GOCI-II Aerosol Retrieval
Jeewoo LEE1#+, Jhoon KIM1,2, Seoyoung LEE1
1Yonsei University, Korea, South, 2Korean Academy of Science and Technology (KAST), Korea, South
Since its launch in 2020, the GOCI-II (Geostationary Ocean Color Imager-II) onboard the GEO-KOMPSAT-2B (GK-2B) satellite has provided aerosol products using the Yonsei aerosol retrieval (YAER) algorithm (Lee et al., 2023). The GOCI-II YAER algorithm retrieves aerosol optical depth (AOD) at 550 nm using an inversion algorithm with a precalculated look-up table (LUT) over UV to near-IR wavelengths. The surface reflectance database is collected using the Cox and Munk method (Cox and Munk, 1954) and the minimum reflectance technique (Hsu et al., 2004) over ocean and land, respectively. When calculating the minimum reflectance, the minimum value of Lambertian Equivalent Reflectance (LER) of each wavelength is designated as the surface reflectance at each pixel. The 550 nm AOD is the weighted average of AOD of two aerosol types that minimize the standard deviation among the six pre-assumed types. In this study, we improved the performance of the GOCI-II YAER algorithm by optimizing the surface reflectance calculation method and tuning the aerosol type selection phase. First, the spectral AOD of the YAER algorithm was validated to the AOD from the AErosol RObotic NETwork (AERONET) to test the stability of the minimum reflectance. The wavelength on which its AOD showed the highest consistency with AERONET was used as the standard of the minimum reflectance to fix the surface reflectance of all other wavelengths. Second, aerosol type selection phase was tuned to take more aerosol optical information during the selection. As a result, the updated product showed improved validation statistics when compared to AERONET AOD in terms of % within expected error (EE), the correlation coefficient, and the root mean squared error (RMSE). The improved GOCI-II AOD can help mitigate the air quality issues and expand our knowledge of diurnal variations of aerosols over Northeast Asia.
AS59-A030
Change of Slant Column Densities of NO2 According to the Spatial Resolution of Airborne Remote Sensing in Urban Areas During KORUS-AQ and SIJAQ Campaign
Seungjae LEE#+, Sang Seo PARK
Ulsan National Institute of Science and Technology, Korea, South
There are remaining uncertainties from satellite remote sensing retrieval of nitrogen dioxide (NO2), one of important pollutants for understanding urban air quality study. In this research, we analyze the impact for spatial resolution of observation pixels on retrieved differential slant column density (dSCD), regarded as one of uncertainty factor. Airborne measurement data which offers a higher resolution remote sensing data compared to satellites and useful for evaluating spatial variability were collected from KORUS-AQ and SIJAQ campaign. Comparing dSCD maps among different spatial resolutions, we confirm that some point sources and structures of NO2 density distribution were diluted and smoothed at a low resolution. Also, we confirm increase of standard deviation values that shows deviation of information on pixels over 2 km spatial resolution. In future, we can study the impact of spatial resolution on other trace gases that has different spatiotemporal variability. Furthermore, we can advance the understanding of satellite data according to spatial resolution.
AS59-A033
Quantifying NOx Lifetimes and Emissions in Seoul, South Korea, Using Geostationary Satellite Observations
Sojeong LEE1+, Ja-Ho KOO1#, Hyeji CHA1, Jeong Ah YU2
1Yonsei University, Korea, South, 2National Institute of Environmental Research, Korea, South
This study aims to quantify NOx lifetimes and emissions in Seoul, South Korea, using data from Geostationary Environment Monitoring Spectrometer (GEMS) tropospheric NO2 observations in 2022 along with ECMWF wind field data. NOx lifetimes are determined by analyzing systematic difference obtained through fitting NO2 line density to a model function, considering wind directions and wind speed. The results indicate that, with a fitting interval of 100×100km2, the calculated lifetimes ranged from 14.14 to 50.19 minute in spring, 16.23 to 53.61 minute in summer, 19.32 to 62.89 minute in autumn and 24.2 to 62.02 minute in winter (R2>0.8). When the fitting interval is 100×200km2, lifetime ranged from 34.05 to 82.61 minute in spring, 33.81 to 80.28 minute in summer, 30.13 to 94.07 minute in autumn and 61.11 to 94.89 minute in winter (R2>0.8). The quantified NOx emissions for 2022 were determined based on the lifetime fitting results, ranging from 210.66 Gg to 714.93 Gg with a 100×100km2 lifetime fitting interval and from 174.33 Gg to 390.88 Gg with 100×200km2 lifetime fitting interval. To verify these results, we used Clean Air Policy Support System (CAPSS) emissions inventory data. The mean of NOx emissions for 2016-2020 within the fitting interval area was 203.7±21.22 Gg. In conclusion, adopting a 100×200km2 fitting interval provided better visibility of the movement of the NO2 plume, resulting in longer calculated lifetimes. The study acknowledges the high uncertainty in lifetime fitting results during winter and emphasizes the careful interpretation of winter emission results. Future studies are proposed to compare NOx lifetimes and emissions in other East Asian regions for verification. This work was supported by Korea Environment Industry & Technology Institute (KEITI) through "Climate Change R&D Project for New Climate Regime", funded by Korea Ministry of Environment (MOE) (2022003560006).
AS59-A034
Trans-pacific Transport of Asian Pollutants in CMIP6 Related to the Western Pacific Pattern
Taegyung LEE1+, Ja-Ho KOO1#, Sungbo SHIM2
1Yonsei University, Korea, South, 2National Institute of Meteorological Sciences, Korea, South
Trans-Pacific transport is important because it not only affects air quality in East Asia but also in North America. In April, trans-Pacific transport is associated with the Western Pacific pattern (WP). When the WP is positive phase, favorable atmospheric circulation for trans-Pacific transport is formed over the North pacific, leading to an increase of the Aerosol Index (AI) over the North America. Climate change leads to extreme weather phenomena. WP is no exception. Changes in the WP due to climate change are expected to impact trans-Pacific transport as well. Coupled Model Intercomparison Project phase 6 (CMIP6) makes possible to examine the changes associated with climate change and thus predicting the changes in air quality. In this analysis, we investigated whether CMIP6 simulated the spatiotemporal pattern of Aerosol Optical Depth (AOD) according to WP and examined the tendencies of the WP phase under different Shared Socioeconomic Pathways (SSPs). CMIP6 effectively simulated the changes in atmospheric circulation and the AOD associated with the variations in the WP phase. When comparing the four SSPs (SSP1-2.6, SSP2-4.5, SSP3-7.0, SSP5-8.5), the frequency and intensity of positive WP phase were highest in the highest CO2 emission scenario, SSP5-8.5. This suggests that the higher carbon emission, the more frequent and intense trans-Pacific transport. Further investigation is needed to understand the underlying reasons for increased frequency and intensity of positive WP phase in high carbon emission. Additionally, the analysis should be conducted using more model data. This work was supported by Korea Environment Industry & Technology Institute (KEITI) through "Climate Change R&D Project for New Climate Regime", funded by Korea Ministry of Environment (MOE) (2022003560006).
AS59-A035
Analyzing PM2.5 Nighttime Peaks in South Korea
Juhee LEE1, Seonggyun NA1+, Jinkyu HONG1, Jeongwoo KIM1, Sang-Woo KIM2, Soojin PARK2, Ja-Ho KOO1#
1Yonsei University, Korea, South, 2Seoul National University, Korea, South
PM2.5 denotes aerosol particles in the air with aerodynamic diameter of less than 2.5μm. PM2.5 contributes to social and economic challenges and negatively affects human health. Research into the temporal and spatial variability of PM2.5 is crucial for its effective management. The Ministry of Environment has operated a ground-based observation network, AirKorea, since the early 2000s to continuously monitor air pollutants, including PM2.5 and its precursors (NO2, SO2, etc.). This study analyzed diurnal variations in PM2.5 concentrations in South Korea using data from AirKorea observation network from 2016 to 2021. In South Korea, PM2.5 levels typically begin to rise at 8 a.m. during rush hour, peak around 10 a.m., and then decrease after noon as radiation levels increase. A subsequent increase is observed starting around 6 p.m. during the evening rush hour, with another peak occurring at night. Many previous studies have indicated that the morning peak in PM2.5 is influenced by increased anthropogenic emissions, and the afternoon decrease is affected by an increase in Planetary Boundary Layer (PBL) height. However, research specifically investigating the nighttime peak is limited. In this study, to determine the cause of the PM2.5 nighttime peak in South Korea, we analyzed the differences in meteorological conditions (PBL height, wind speed, relative humidity) and air pollutants (PM10, NO2, SO2) on days with the PM2.5 nighttime peak compared to days without it. Additionally, we used PM2.5 compositional data to compare the concentrations of its constituents on days with the nighttime peak to those on days without such peaks in Seoul, Ulsan, Jeju, Gwangju, and Daejeon. This work was supported by Korea Environment Industry & Technology Institute (KEITI) through "Climate Change R&D Project for New Climate Regime", funded by Korea Ministry of Environment (MOE) (2022003560006).
AS59-A036
High-resolution Direct Aerosol Radiative Forcing Calculation Using GEMS AOD and Aerosol Type in South Korea
Juhee LEE1+, Dayeong LEE1, Yeseul CHO1, Sang Seo PARK2, Jeong Ah YU3, Ja-Ho KOO1#
1Yonsei University, Korea, South, 2Ulsan National Institute of Science and Technology, Korea, South, 3National Institute of Environmental Research, Korea, South
This study explores the key energy source between the Earth and the atmosphere, solar radiation, which directly and indirectly influences the weather. Changes in the Earth's system impact radiative equilibrium, and the concept of radiative forcing (RF) was introduced to quantify these effects. RF is influenced by specific atmospheric components such as trace gases, with significant impacts primarily attributed to changes in clouds and aerosols. To understand direct aerosol radiative forcing (DARF) caused by aerosols, we developed an algorithm considering aerosol optical depth (AOD) and aerosol types using the Geostationary Environment Monitoring Spectrometer (GEMS) on the GK-2B (Geostationary Korea Multi-Purpose Satellite-2B) satellite. GEMS AOD algorithm version 2.0 and the libRadtran version 2.0.4 radiative transfer model were employed as input data. Aerosol types were classified as Black Carbon, dust, and non-absorbing aerosol, and the OPAC model was used for DARF calculations based on aerosol types. Surface (SFC), top of atmosphere (TOA), and atmospheric (ATM) DARF spatial distributions were examined in major Korean cities. To obtain city-specific DARF time series from November 2021 to April 2023, city boundaries were defined, and the average AOD values of all GEMS pixels within each boundary were used as input data. For validation purposes, a comparison with Aerosol Robotic Network (AERONET) inversion data for RF was also conducted. This study aims to enhance understanding of air pollution issues in South Korea and the variation characteristics of DARF in different regions throughout the day. This work was supported by Korea Environment Industry & Technology Institute (KEITI) through "Climate Change R&D Project for New Climate Regime", funded by Korea Ministry of Environment (MOE) (2022003560006).
AS59-A050
Constraining the Diurnal Variation of Tropospheric Oxidation Capacity Using GEMS Products
Sang-Ik OH+, Rokjin J. PARK#
Seoul National University, Korea, South
The hydroxyl radical (OH) is a pivotal oxidant in the troposphere, playing a crucial role in determining the lifetime of critical pollutants such as carbon monoxide (CO) and methane (CH4). The primary generation of tropospheric OH occurs through the photolysis of ozone (O3) in the presence of water vapor (H2O), making tropospheric OH's abundance and oxidative capability heavily dependent on diurnal patterns. Yet, due to its ephemeral lifetime of approximately one second and its scant concentration in the troposphere, direct measurement of tropospheric column OH (TCOH) and its diurnal fluctuation remains unattainable through global satellite monitoring. Efforts have been made to use satellite observations as a proxy to study OH variability on temporal scales longer than a day, often in conjunction with chemistry transport or machine learning models. With the launch of the Geostationary Environment Monitoring Spectrometer (GEMS) in February 2020, which provides hourly measurements of atmospheric pollutants like O3, nitrogen dioxide (NO2), and formaldehyde (HCHO) over Asia, our understanding of these pollutants' diurnal variations has significantly advanced. This study introduces a method for approximating the diurnal variation of TCOH by employing satellite data on OH precursors, including the hourly-changing observations from GEMS. Utilizing training data from satellite observations and TCOH values from chemical composition reanalysis fields, the supervised machine learning model adeptly predicts the diurnal variation of TCOH when provided with inputs of OH precursors. The findings also indicate a promising avenue for integrating this approach into high-resolution CH4 modeling for East Asia.
AS59-A051
Sensitivity of GEMS Formaldehyde Vertical Columns to Multiple Factors
Gitaek LEE1+, Rokjin J. PARK1#, Hyeong-Ahn KWON2, Eunjo HA1, Dongwon LEE3, Hyunkee HONG3, Francois HENDRICK4, Corinne VIGOUROUX4, Gaia PINARDI4, Isabelle DE SMEDT4, Michel Van ROOZENDAEL4, Pucai WANG5
1Seoul National University, Korea, South, 2University of Suwon, Korea, South, 3National Institute of Environmental Research, Korea, South, 4Royal Belgian Institute for Space Aeronomy, Belgium, 5Chinese Academy of Sciences, China
Volatile organic compounds (VOCs) are precursors to surface ozone and secondary organic aerosols. In East Asia, simulations from chemical transport models often miss significant VOCs due to uncertain emission sources. Formaldehyde (HCHO), a byproduct of VOC oxidation, can act as an indicator to provide observational constraints on VOC emissions. The Geostationary Environment Monitoring Spectrometer (GEMS) commenced hourly monitoring of HCHO vertical column densities (VCDs) over East Asia starting in August 2020. This study assesses the updated operational GEMS HCHO retrieval algorithm (version 3) by comparing it with TROPOMI and ground-based observations (FTIR, MAX-DOAS) throughout its three years of operation. We introduce several enhancements to the retrieval algorithm, particularly regarding background corrections and the input parameters that influence air mass factor (AMF) calculations. We observe that utilizing hourly background surface reflectance from GEMS, rather than OMI Lambertian equivalent reflectivity, results in 20–30% lower AMFs over land areas in East Asia. The revised GEMS HCHO data generally align with the spatial distributions observed by TROPOMI HCHO (r=0.67–0.88), despite slightly underestimating VCDs (NMB=-28% to -17%) across the scanning domain. Additionally, we explore factors affecting AMF sensitivity using HCHO vertical profiles obtained from airborne measurements during the KORUS-AQ campaign. We note that certain geometric conditions, particularly in the early morning (7–8 KST) and afternoon (15–16 KST), significantly impact the AMF, potentially increasing reliance on model accuracy in VCD calculations. Our findings underscore the necessity of precise model simulations in calculating HCHO AMF.
AS59-A056
NO2 Tropospheric Vertical Column Density from MAX-DOAS Observation in Seoul and Yongin, Korea During the ASIA-AQ Campaign
Giyeol LEE1#+, Yongjoo CHOI1, Yugo KANAYA2, Meehye LEE3, Junsu GIL3
1Hankuk University of Foreign Studies, Korea, South, 2Japan Agency for Marine-Earth Science and Technology, Japan, 3Korea University, Korea, South
Nitrogen dioxide (NO2) is a gaseous atmospheric pollutant that contributes as catalysts to the formation of ozone in the troposphere and plays a significant role in atmospheric chemistry. The ground-based Multi-Axis Differential Optical Absorption Spectroscopy (MAX-DOAS) have been employed to investigate tropospheric trace gases (including NO2) and aerosols at a fixed location with high temporal resolution and accuracy. The continuous measurements of ground-based MAX-DOAS are advantageous in effectively observing the high temporal variations of NO2 Tropospheric Vertical Column Density (NO2 TropoVCD). Aiming to obtain the reliable NO2 TropoVCD in Seoul Metropolitan Area (SMA), two MAX-DOAS have been operated in Seoul (37.59°N, 127.03°E, 80 m) and Yongin (37.34°N, 127.27°E, 167 m), downwind of Seoul, since October 2023 and October 2021, respectively. During Airborne and Satellite Investigation of Asian Air Quality (ASIA-AQ) campaign, the purposes of this study are summarized as follows: (1) validation of NO2 TropoVCD from Geostationary Environmental Monitoring Spectrometer (GEMS) using the MAX-DOAS, (2) comparison of the differences in MAX-DOAS NO2 TropoVCD between two sites, (3) assessment of NO2 advection from Seoul to Yongin using the NO2 vertical profile. We believe these results will contribute to improving the accuracy of GEMS NO2 products and the understanding of NO2 behavior in SMA.
AS59-A067
Retrieval of the SO2 Slant Column Density and Mixing Ratio Using UV-VIS MAX-DOAS Instrument
Gyeong PARK+, Hanlim LEE#
Pukyong National University, Korea, South
In this study, we developed a ground-based sulfur dioxide (SO2) Slant Column Density (SCD) retrieval algorithm based on Differential Optical Absorption Spectrometer (DOAS) from hyperspectral measurements to monitor industrial stack plumes. Our algorithm has an advantage of a capability to continuously and remotely monitor industrial SO2 plumes rather than in-situ SO2 measurements. Also, it has a valuable advantage that we know uncertainty of instruments we use and experimental situation we have approximately. And we calculated the optical path length using the observation geometry for mixing ratio retrieval. In a industrial stack plume observation situation, the optical path length that considers the distance between the instrument and the stack and the plume thickness together can increase the accuracy of the mixing ratio retrieval. The experimental data to test this algorithm of SCD and mixing ratio was obtained in Haman, South Korea in August, 2022 and Gimhae, South Korea in November 2023. Since most in-situ measurements has a product in the unit of mixing ratio, it has a valuable advantage of being able to confirm the accuracy of observation through comparison of the retrieved mixing ratio and in-situ.
AS60-A008
Mesospheric Tides Comparisons at Low Latitudes Observed by Two Collocated Meteor Radars
Jian LI+, Wen YI#, Xianghui XUE
University of Science and Technology of China, China
Accurate knowledge of mesospheric winds and waves is essential for studying the dynamics and climate in the mesosphere and lower thermosphere (MLT) region. In this study, we conducted a comparative analysis of the mesosphere tidal results obtained from these two adjacent meteor radars at low latitudes in Kunming, China from November 2013 to December 2014 were analyzed and compared. These two radars operate at different frequencies of 37.5 MHz and 53.1 MHz, respectively. However, an overall good agreement was observed between the two radars in terms of horizontal winds and tide observations. The results showed that the dominant tidal waves of the zonal and meridional winds are diurnal and semidiurnal tides. Moreover, we conducted a statistical comparison of tide amplitudes and phases observed by both radars, revealing a high degree of correlation between the tidal parameters. Additionally, the variances and covariances of tidal amplitudes and phases were found to be quite similar for the two radars. Thus, mesospheric tides at low latitudes observed by two collocated meteor radars with different frequents exhibit strong consistency.
AS60-A009
Roles of Atmospheric Wave Forcing in Momentum Budget of Climatological and Disrupted Quasi-biennial Oscillations in MERRA-2 Reanalysis
Hoijin UH+, Wonseok LEE, Byeong-Gwon SONG, In-Sun SONG#
Yonsei University, Korea, South
Various mean-flow oscillations in the equatorial middle atmosphere can be generated by interaction between the zonally averaged mean flow and numerous atmospheric wave modes. Quasi-biennial oscillation (QBO) is one of the most well-known examples in the wave-mean interaction in the tropical lower stratosphere. However, the QBO can be modulated by momentum forcing due not only to equatorial waves but also to horizontally propagating Rossby waves that originate from the extratropical region. In the northern winters of 2015/2016 and 2019/2020, the downward progression of westerly QBO phase was interrupted by localized and intensified easterlies, mainly due to exceptionally large wave momentum forcing due to extratropical Rossby waves. In this study, global wave modes represented by Hough and vertical structure functions are obtained from MERRA-2 reanalysis data by decomposing global winds and temperature into components associated with Kelvin, Rossby-gravity, inertia-gravity, and Rossby waves. Then, resolved wave momentum forcing (Eliassen-Palm (EP) flux divergence) due to each wave mode is estimated. To compute EP flux and its divergence, methods of obtaining temperature perturbations and vertical wind velocity induced by each wave mode have been developed. Comparison of EP flux divergence for climatological QBO indicates that dominant eastward (westward) wave momentum forcing is due to Kelvin waves (Rossby waves). The QBO momentum budget in terms of zonal wind tendency due to advection, the resolved wave momentum forcing due to each wave mode, analysis increments, the parameterized gravity wave drag, and the residual tendency will be discussed together with wave momentum budget in the disrupted QBO periods.
AS60-A014
Preliminary Results of Mesospheric Temperature Mapper in the Mesosphere Lower Thermosphere at King Sejong Station, Antarctica
Ji Eun KIM#+, Jeong-Han KIM, Geonhwa JEE, Changsup LEE
Korea Polar Research Institute, Korea, South
Many researches over the past decades have been shown that OH airglow known as the peak emission altitude of about 87km is very useful to study not only the propagation and dissipation of atmospheric gravity waves but also the mesospheric temperature variation with time. Recently, KOPRI (Korea Polar Research Institute) has started to operate Mesospheric Temperature Mapper (MTM) at King Sejong Station, Antarctica (62.2S, 58.8W) since its installation on Jan. 2023, in order to study the small-scale gravity wave activities and temperature variation near mesopause region. MTM instrument provides two dimensional OH airglow intensity and rotational temperature every 30s with a high spatial resolution of ~0.5km.In this study, we introduce the KSS MTM instrument and present some preliminary results which compare the temperatures obtained from MTM for 26 clear nights during 2023 austral winter season with the temperatures from co-located KSS Meteor Radar and Aura/MLS satellite.
AS65-A003
Assessment of Dynamical Downscaling Performance Over CORDEX East Asia Using MPAS-A Global Variable Resolution Model
Yiyuan CHENG+, Jianping TANG#
Nanjing University, China
This study presents regional climate simulations for East Asia and China using the Model for Prediction Across Scale-Atmosphere (MPAS-Atmosphere) driven by ERA-Interim reanalysis. In a 29-year simulation (1988-2016), MPAS-A with a global variable resolution (VR) configuration (92-25km mesh refinement over East Asia) is evaluated for precipitation, near-surface air temperature, and circulation against observed climate using combined observational datasets. Large-scale deviations, such as the northward displacement of rain belts, excessively triggered precipitation on the ocean, and stationary surface air temperature biases, are identified. These deviations are attributed to simulated circulation, moisture transports. Focusing on the summer monsoon with the highest uncertainty in East Asian climate, comparative experiments are conducted using a similar 92-25km grid under global variable resolution settings (MPAS-VR) and limited-area settings (MPAS-RCM) for simulations from April to August during 1998-2017. Constrained by the “reanalysis-based” lateral boundary conditions (LBCs), MPAS-RCM could well capture the evolution of large-scale fields and becomes a proper reference for evaluating MPAS-VR. MPAS-VR reproduced the conclusions of the previous 29-year simulation. MPAS-RCM, benefiting from a more realistic water vapor transport, alleviates the wet bias and presents better daily variations and rain belts’ evolution. However, MPAS-RCM did not exhibit a clear advantage in the distribution of climate indices related to extreme events over land. Additionally, its performance in terms of climatology and interannual variability of the surface temperature are insufficient compared to MPAS-VR. With the same dynamic core and model physics, those climate features are similarly resolved by the two simulations. the study underscores the robustness and potential of the VR approach, particularly regarding extreme rainfall and heat wave.
AS65-A008
WRF Gray‑zone Dynamical Downscaling Over China: Model Performance and Added Value
Shuangshuang WANG+, Shuyu WANG#
Nanjing University, China
This study presents an in-depth evaluation of the Weather Research and Forecasting (WRF) model's performance in the context of gray-zone (9 km) dynamical downscaling over China, emphasizing the added value it brings to regional climate modeling. The term "gray-zone" refers to scales where traditional parameterization schemes are neither fully effective nor entirely redundant, a common challenge in atmospheric modeling. Our work bridges this gap, focusing on the transitional scale phenomena. The research utilized the advanced WRF model, incorporating recent updates in its physics and dynamics schemes, to conduct high-resolution simulations over China. The study period spanned multiple years to capture a comprehensive range of meteorological conditions, including extreme climate events. Our evaluation criteria involved a comparative analysis of the WRF model outputs against observational datasets and ERA5 reanalysis to assess its performance and added value. Key findings demonstrate that the WRF model, when applied in the gray-zone, significantly enhances the representation of mesoscale meteorological features compared to ERA5. This improvement was particularly notable in complex terrain areas, where the model accurately captured local near-surface air temperature patterns and precipitation distributions. Furthermore, the model showed a marked improvement in simulating extreme climate events, such as heavy rainfall and heatwaves, which are critical for regional climate impact assessments. The added value of the WRF gray-zone downscaling is evident in its ability to provide more accurate and detailed climate information at a regional scale. This is particularly beneficial for China, where diverse topography and climatic conditions pose a challenge for conventional models. The significant advancements and potential of gray-zone dynamical downscaling using the WRF model over China facilitate better decision-making in sectors like agriculture, water resource management, and urban planning, where precise climate data is crucial.
AS65-A009
Will the Arid and Semi-arid Regions of Northwest China Become Wetter Under Stabilized 1.5°C and 2.0°C Warming Futures?
Mi ZHANG#+, Shuyu WANG
Nanjing University, China
Future dry-wet changes of Northwest China and their mechanisms remain controversial. Therefore, this work projected seasonal and annual dry-wet conditions in the arid and semi-arid regions by analyzing the variation of water availability, which is defined as precipitation minus evaporation, based on the downscaled future regional climate change under 1.5/2.0°C stable warming scenarios (1.5s/2.0s) using Weather Research and Forecasting (WRF) model. The results showed that, the water availability in arid increased by 1.09 and 1.24 mm/month under future warming scenarios of 1.5s and 2.0s, respectively, while in semi-arid, the increase was lower than in arid and even decreased in summer. The results of changes in moisture transport suggested that the stronger increase in water availability in arid may be related to the inflow of moisture from arid and the outflow from semi-arid in summer. The moisture budget analysis further demonstrated that, the increase of water availability in arid was mainly due to the enhanced contribution of the thermodynamic term caused by warming, which further increased by 8% with an additional warming of 0.5°C. Whereas the decrease in summer semi-arid was from a negative contribution of the non-linear term, which may be related to reduced moisture transport due to changes in the East Asian summer monsoon.
AS65-A010
Dynamic Downscaling Simulation and Projection of Precipitation Extremes Over China Under a Shared Socioeconomic Pathway Scenario
Neng LUO1#+, Ruiqiang DING1, Yan GUO1, Jin FENG2
1Beijing Normal University, China, 2China Meteorological Administration, China
In this study, Weather Research and Forecasting (WRF) based dynamic downscaling simulation was performed over China at a horizontal resolution of 25 km. To reduce the systematic large-scale biases from lateral boundary conditions, a dynamic blending (DB) technique was introduced in downscaling, and its performance was compared with downscaling without DB (NO_DB) as well as the driving global climate model (GCM, i.e., HadGEM3). In the present-day simulation for verification, added values were found in DB, relative to the GCM and NO_DB, in simulating the precipitation extremes, especially over southeastern China. Possible causes responsible for this improvement were further analyzed. In the GCM, excessive moisture and atmospheric heating in the upper troposphere in conjunction with abnormally strong deep convection resulted in excessive extreme precipitation over southeastern China, while in NO_DB, insufficient moisture and atmospheric heating in the whole troposphere in conjunction with abnormally weak convection suppressed extreme precipitation there. In comparison, DB showed a closer representation of observations in terms of vertical velocity and vertical profiles of atmospheric moisture and heating, accounting for the improved simulation of extreme precipitation. In the future projection under the SSP5-8.5 scenario, both the GCM and DB predicted that extreme precipitation would increase in most parts of China; however, DB indicated a larger increase over southeastern China relative to the GCM. Stronger moisture flux convergence over southeastern China in DB accounted for this larger increase, and in addition, the thermodynamic effect associated with more precipitable water dominated the stronger moisture flux convergence.
AS65-A011
Assessing the Performance and Added Value of High-resolution 5KM RegCM4 Simulations Over Peninsular Malaysia
Abdul Azim AMIRUDIN1#+, Liew JUNENG2, Fredolin TANGANG3,4, Ester SALIMUN1, Jing Xiang CHUNG5
1National University of Malaysia, Malaysia, 2Universiti Kebangsaan Malaysia, Malaysia, 3Universiti Brunei Darussalam, Brunei Darussalam, 4Ramkhamhaeng University, Thailand, 5Universiti Malaysia Terengganu, Malaysia
High-resolution climate simulations has gained importance in recent climate change impact studies. This approach allows for the investigation of the "gray zone," denoting resolution higher than 10 km where model exhibit uncertainties. Therefore, our objective is to determine the added value high-resolution model simulations over the Peninsular Malaysia based on high resolution simulations using RegCM4 driven by the Fifth Generation of the European Centre for Medium-Range Weather Forecasts (ECMWF) Reanalysis (ERA5). Two one-way nested domains were employed. The first domain covers the entire Southeast Asia and was configured at 25km grid resolution. The second domain covers the entire Peninsular Malaysia and was configured at 5km grid resolution. Given the complex resolution of Peninsular Malaysia there is potential for significant advantages in adopting high-resolution simulations. Climate Hazards Group InfraRed Precipitation with Station (CHIRPS) and Climate Hazards Group Infrared Temperature with Stations (CHIRTS) data were used as references data for precipitation and temperature respectively. The analysis covers the period 1990 to 2014 and extreme climate indices were calculated using Expert Team on Climate Change Detection and Indices (ETCCDI). Extreme precipitation used were RX1day, RX5day, CWD, CDD, R95Pptot, R99ptot and SDII. Fo temperature, it is TNN, TXN, TXX, TXN, TN90P, TN10P, TX10P and TX90P. The 5km resolution model shows remarkable improvements in simulating rainfall distribution and characteristics during the DJF season in the Northeastern part of Peninsular Malaysia. High-resolution 5km models demonstrate better capabilities in simulating extreme wet indices. Additionally, the high resolution simulations also improve the rainfall diurnal cycles over Peninsular Malaysia. The 5km resolution model also shows enhancements in simulating extreme temperatures, especially over the high-altitude regions. These findings show the relevancy of the high resolution model in simulating climate extremes. Moreover, it highlights the need of high resolution simulation in studying the climate over a complex topography in Peninsular Malaysia.
AS65-A014
Projected Changes in Mean Temperature, Precipitation and Extreme Snowfall Events Over the Tibetan Plateau Based on a Set of RegCM4 Simulations
Yuanhai FU, Xianbing TANG+, Xuejie GAO#
Chinese Academy of Sciences, China
Tibetan Plateau (TP, with the height > 3000 m) is a region with complex topographical features and a large diversity of climate both in space and time. Future climate change over TP and the surrounding areas is investigated based on the ensemble of a set of the 21st century climate change projections using a regional climate model, RegCM4. The model is driven by five different GCMs at a grid spacing of 25 km. Results show the RegCM4 greatly improves the temperature and precipitation simulations by providing finer scale spatial details of them over the region. The topographic effects are well reproduced by RegCM4 but not the GCMs. General warming and increase in precipitation are found in both GCM and RegCM4 simulation, but with substantial differences in both the spatial distribution and magnitude of the changes. For temperature, RegCM4 projected a more pronounced warming in DJF over TP compared to its surrounding areas. The increase of precipitation is more pronounced and over the basins in DJF for RegCM4. For the extreme indices of snowfall, RegCM4 generally reproduces the spatial distributions although with overestimation in the amount. General decreases in SNOWTOT and S1mm, with greater magnitude over the eastern part are projected. Both S10mm and Sx5day show decrease over the eastern part but increase over the central and western parts. Notably, S10mm shows a marked increase (more than double) with high cross-simulation agreement over the central TP. Significant increases in all four indices are found over the Tarim and Qaidam basins, and northwestern China north of the TP. The projected changes show topographic dependence over the TP in the latitudinal direction, and tend to decrease/increase in low-/high-altitude areas.
AS65-A017
Future Projection of Extreme Temperature Over the Korean Peninsula Under Global Warming Levels, Using RCMs in CORDEX-EA Phase 2
Do-Hyun KIM1#+, Jin-Uk KIM2, Tae-Jun KIM1, Young-Hwa BYUN1, ChuYong CHUNG1
1National Institute of Meteorological Sciences, Korea, South, 2Korea Meteorological Administration, Korea, South
This study presents future projection of extreme temperature over the Korean Peninsula (KP) under the global warming levels (GWLs) of 2.0℃ and 1.5℃. For projection, bias-corrected large ensemble of the Regional Climate Model in CORDEX-East Asia Phase 2 is used. Under GWL of 2.0℃ (1.5℃), extreme minimum and maximum temperature intensity indices (TNn and TXx) would increase by 2.61℃ (1.91℃) and 2.38℃ (1.58℃) compared to present period. Extreme temperature frequency indices (TN10p and TX90p) would decrease 17.7 days (14.0 days) and increase 30.9 days (20.1 days). In addition, extreme cold and warm events occurring once every 20 years during present period are expected to change a reoccurrence of 28.9 years (22.6 years) and 5.9 years (7.2 years). Meanwhile, there are several noteworthy points in the projection. The extreme temperature over the KP would increase over the northern KP than the southern KP, which is more distinct in TNn than TXx. The spatial pattern in TX90p is similar from that of TXx but the pattern in TN10p is different from that of TNn. In other words, a smaller increase in TN10p is expected over the inland KP.
AS65-A020
Investigating the Evolving Feedback Mechanisms Influencing Water Availability in Africa from the Past to Future Prospects
Ngoc Kim Hong NGUYEN#+, Koji DAIRAKU, Fumiya AOKI
University of Tsukuba, Japan
This study comprehensively examines the evolving feedback mechanisms shaping water availability in Africa, particularly emphasizing the critical need for adaptive measures in response to severe drought events. Drawing from an extensive dataset that incorporates satellite-based information, observational data, CORDEX AF44 RCP8.5, and CMIP6 SSP585 scenario, the research employs advanced indices, including the Standardized Precipitation-Evapotranspiration Index (SPEI). Methodologically, the investigation analyzes drought trends spanning 1983-2005 and projects into the future (2051-2100). Noteworthy findings reveal a conspicuous reduction in drought severity anticipated from the 2070s-2080s afterward, underscoring the necessity of addressing evolving drought conditions. The study highlights the intricate nexus between water availability and soil moisture; it even recorded a positive sensitivity coefficient, emphasizing the pivotal role of considering soil moisture feedback and moisture convergence in estimating water availability. Mean flow convergence is a substantial contributor, constituting approximately 55% of the overall moisture convergence across the African continent. These nuanced insights advocate for a holistic understanding of evolving feedback mechanisms, emphasizing the necessity for proactive measures to mitigate climate-induced water scarcity. This research has significant implications for informing effective water resource management and adaptive strategies, especially in the context of prolonged drought episodes in Africa.
AS65-A021
Sensitivity of East Asian Summer Precipitation in 2022 to Boundary Layer and Convection Schemes
Junseo PARK+, Eunji KIM, Haeun JO, Tae Ho MUN, Dong-Hyun CHA#
Ulsan National Institute of Science and Technology, Korea, South
In East Asia, about half of the annual precipitation occurs during the summer, with the East Asian Summer Monsoon (EASM) region being affected by various temporal scale variability factors, making its prediction challenging. Therefore, understanding the characteristics of the East Asian summer precipitation and improving simulation performance through optimal experimental design are essential meteorological tasks. In particular, summer precipitation in East Asia, mainly convective, requires consideration of heat, moisture, and momentum exchanges between the land, ocean, and atmosphere, and mixing processes in the boundary layer triggered by the complex topography of East Asia. Hence, elements such as the Cumulus Parameterization Scheme (CPS) and the Planetary Boundary Layer (PBL) scheme significantly impact the simulation of these processes. The 2022 East Asian summer precipitation was similar to the normal year, but the Korean Peninsula recorded the highest hourly rainfall since observation by the Korea Meteorological Administration (KMA) began, showing a different pattern from the normal year. This study examined the differences in the simulation of summer precipitation in the East Asian region in 2022 using the Weather Research and Forecasting (WRF) model based on PBL schemes and CPS combinations. The PBL scheme is vital in describing the interactions between convection and horizontal flow within the boundary layer. Among various PBL schemes, this study employed the nonlocal Yonsei University (YSU) scheme and the combined local and nonlocal closure Asymmetric Convective Model version 2 (ACM2) to compare the simulation performance and precipitation characteristics according to different physical schemes. We also investigated the impacts on weather prediction through differences in the vertical structure and large-scale environmental field.
AS65-A027
Performance Evaluation and Future Projection of East Asian Climate Using SSP Scenario-based CORDEX-East Asia Multi-RCMs
Jinuk KIM1#+, Chu Yong CHUNG2, Tae-Jun KIM1, Do-Hyun KIM1, Young-Hwa BYUN1
1National Institute of Meteorological Sciences, Korea, South, 2National Meteorological Satellite Center, Korea, South
In this study, the performance of five RCMs and their ensemble mean for present-day climate simulations are evaluated. RCMs have relatively high performance for climatology patterns for Korea peninsular, East China and Japan, while relatively low performance is observed for the Tibetan plateau and India. Future climate changes under four SSP scenarios are analyzed for late 21st century (2081 ~ 2100) compared to present day (1995 ~ 2014). East Asia is expected to experience temperature increases of 2.4℃ to 6.2℃ and precipitation increases of 6.7% to 12.6%, with stronger changes in higher-emission scenarios. Among the five RCMs, HadGEM3-RA projects the largest increase in temperature while GRIMs is characterized by the strongest increase in precipitation. In line with mean warming rates, warm extreme days (TX90p) are projected to increase by 35.7 ~ 93.3 days and cold extreme days (TN10p) are projected to decrease by 23.4~35.2 days. The results of this study can be used as a reference for future detailed analyses of East Asian climate changes and its impacts as well as for assessing the importance of carbon neutrality.
AS65-A030
Deep Learning Statistical Downscaling of Compound Heatwave and Drought Drivers During the Passage of the West Africa Monsoon Flow
Eromosele Precious EBIENDELE#+, Koji DAIRAKU
University of Tsukuba, Japan
In the climate scientific community, there has been a recent emergence of deep learning as a new approach for downscaling large-scale atmospheric fields to a regional scale. Our study focuses on the added value of integrating a coupled-monsoon-trained deep learning architecture in downscaling the drivers of Compound heatwave and drought (temperature and precipitation) during the passage of the West African monsoon flow. In our study, we design three deep learning frameworks (CNN, UNET, and UNET++) following the perfect prognosis approach with a primary target of exploring each model's transferability ability in warm and cold conditions. Our study's findings highlight the significant contribution in terms of the added value of deep learning coupled-monsoon architecture to high-elevation regions, particularly in the central Sahel region. Conclusively, by implementing this approach, we intend to improve the accuracy of climatic information for present and future compound events risk over the West Africa region.
AS65-A032
Analyzing the Interplay of Soil Moisture, Precipitation, and Evapotranspiration and Drought Conditions in Anticipation of Water Availability Challenges Across the African Continent
Ngoc Kim Hong NGUYEN#+, Koji DAIRAKU, Fumiya AOKI
University of Tsukuba, Japan
In forthcoming scenarios, the African continent is expected to face significant challenges in water availability due to soil dryness and low air aridity index, with higher vapor pressure deficits (VPD). This study examines the complex interaction relationship between soil moisture (SM), precipitation (P), and evapotranspiration (E), and how they relate to drought. Specifically, the focus is on understanding changes in SM, VPD seasonal dynamics, and drought conditions using the Standardized Precipitation-Evapotranspiration Index (SPEI). Using various data sources such as observations, satellite-based data, reanalysis data, CORDEX RCMs under the Africa 44 domain, and CMIP6 GCMs, we analyze historical 1981-2005 and future climate scenarios 2051-2100. Positive feedbacks in the SM-(P-E) relationship show a positive varying coefficient, except for an unusually high level observed in satellite data. According to the SPEI with a 1-month interval, a shift from wet to dry conditions is projected around 2085. Future conditions under RCP8.5 suggest less severe "Extreme" and "Very" dry periods compared to the past, while the study recorded GCMs indicate a higher intensity and frequency of drought than RCMs. Additionally, VPD is notably active in the Sahel and Southern Africa, with future projections anticipating a stronger relationship between SM and VPD in summer compared to winter. These findings underscore the pressing need for proactive water resource management strategies in the face of anticipated challenges, emphasizing the importance of understanding the intricate dynamics between land-atmosphere interaction for effective drought mitigation and adaptation efforts.
AS65-A033
Impact of Climate Model Biases on Assessing Cooling Demand in Japan
Saurabh KELKAR#, Koji DAIRAKU+
University of Tsukuba, Japan
As temperatures rise, businesses and households will need more energy to keep cool, increasing the cooling demand. Several studies used climate model simulations to show that climate change will likely increase cooling demand in many parts of the world. Climate models are the primary source of long-term climate information and are known to have biases. However, these biases are not explicitly discussed while investigating the cooling demand. The present study addresses how climate model biases and bias adjustment of heat stress may play a role in assessing cooling demand. Cooling degree days are calculated as a proxy for temperature and human discomfort to excess heat to investigate the cooling demand. Estimation is performed using climate information from an ensemble of general circulation models (MRI-CGCM3, MIROC5, CCSM4), reanalysis data (JRA25), and regional climate models (NHRCM, NRAMS, WRF) forced by general circulation models and reanalysis before and after the bias adjustment. Results are validated using cooling degree days based on observed temperature data from NARO. Reduction in temporal deviations for cooling degree days based on forcing data and corresponding regional climate models is noticed after the bias adjustment, indicating its effectiveness. Detrended cooling degree days suggest that changes in fluctuations after bias adjustment may be attributed to reduced temperature biases. The change is more prominent in cooling degree days determined from forcing data, indicating that the biases in coarser resolution data may significantly impact estimating cooling demand more than in regional climate simulations. These findings show how model biases and bias adjustments may affect the representation of cooling demand, highlighting the need to consider such uncertainties in future studies.
AS72-A006
Fingerprint-based Attribution and Constrained Projection of Global Risk of Daily Compound Hot Extremes
Liangwei LI1+, Xihui GU1#, Louise J. SLATER2, Xueying LI3, Lunche WANG1, Dongdong KONG1, Xiang ZHANG4
1China University of Geosciences, China, 2University of Oxford, United Kingdom, 3Helmholtz Centre for Environmental Research – UFZ, Germany, 4China University of Geosciences (Wuhan), China
Compound hot extremes (CHEs)—the concurrence of daytime and nighttime heat—have been increasing under anthropogenic warming, causing serious damage to human society and ecosystems. However, the anthropogenic fingerprint in past and future changes in daily CHEs and the corresponding fingerprint-constrained population exposure remain unclear. Here, using a fingerprint-based detection and attribution method, we quantify contributions of different external forcings to the historical increase in CHEs by defining three daily-scale metrics: the probability ratio (PR) of CHEs, and the proportion of CHEs in the number of extreme hot days/nights (PTday/PTnight). All three metrics have increased significantly by 98.04%, 139.67%, and 141.91% globally from 1950 to 2014, especially in Europe and North America. We find it is very likely (>90%) for human to leave fingerprints in increasing daily CHEs. The increases in PR, PTday, and PTnight that are attributable to greenhouse gas emissions are 113.62%, 144.88%, and 145.26%, respectively. By the end of the 21st century under a high-emission scenario, our fingerprint-constrained projections indicate that these metrics would increase to approximately 131.23, 0.41, and 0.43, respectively, which is a significant reduction in magnitude and uncertainty, relative to the raw projections. In some regions such as the mid and high-latitudes, almost all daytime or nighttime extreme-heat events would become CHEs. We further find that CHEs disproportionately affect densely populated areas in fingerprint-constrained projections of population exposure. Our results indicate that adaptive measures are required to alleviate the increasing proportion of CHEs and the disproportionate population exposure in densely populated areas.
AS72-A009
Modulations of Madden-Julian Oscillation and Quasi-biweekly Oscillation on Early Summer Tropical Cyclone Genesis Over Bay of Bengal and South China Sea
Weizhen CHEN1+, Chang-Hoi HO2#, Song YANG1, Zeming WU3, Hongjing CHEN1
1Sun Yat-sen University, China, 2Seoul National University, Korea, South, 3Zhejiang University, China
The Madden-Julian oscillation (MJO) and the quasi-biweekly oscillation (QBWO) are prominent components of the intraseasonal oscillations over the tropical Indo-Pacific Ocean. This study examines the tropical cyclone (TC) genesis over the Bay of Bengal (BOB) and the South China Sea (SCS) on an intraseasonal scale in May−June during 1979−2021. Results show that the convection associated with the two types of intraseasonal oscillations simultaneously modulates TC genesis in both ocean basins. As the MJO/QBWO convection propagated, TCs form alternately over the two basins, with a significant increase (decrease) in TC genesis frequency in the convective (non-convective) MJO/QBWO phase. Based on the anomalous genesis potential index associated with the MJO/QBWO, an assessment of the influence of various factors on TC genesis is further assessed. Middle-level relative humidity and lower-level relative vorticity play key roles in the MJO/QBWO modulation on TC genesis. The MJO primarily enhances large-scale cross-equatorial moisture transport, resulting in significant moisture convergence, while the QBWO generally strengthens the monsoon trough and induces the retreat of the western North Pacific subtropical high, increasing the regional lower-level relative vorticity. The potential intensity and vertical wind shear make small or negative contributions. This study provides insights into the neighboring basin TC relationship at intraseasonal scales, which has a potential to improve the short-term prediction of regional TC activity.
AS72-A013
Synergies Between Urban Heat Island and Compound Heat Extremes in Chinese Megacities of Different Climate Zones
Xinyi JIANG#+
Nanjing University, China
Under global climate warming and local anthropogenic influence, urban areas are threatened by increasingly serious heat extremes across the globe, posing a great threat to human health and the survival of city residents. Using global climate reanalysis and local daily air temperature datasets since the 1960s, we disentangle the synergies between urban heat island (UHI) and compound heat extremes in Chinese megacities of different climate zones. We find that the heat extremes in China have nearly tripled in frequency, intensity, and duration since this century. The nighttime- and compound-heat extremes remarkably amplified in cities, and account for 76.3% of extreme heat events in the past decade. After classifying the weather stations into urban and non-urban types with LULC maps and quantifying the urban impacts of amplified heat extremes in four metropolitan areas of China, we find the BTH region seems to be the most vulnerable region suffering from urbanization-accelerated heat extremes, with a relative contribution of the frequency, intensity, and duration by nearly 55.3%, 51.7%, 55.4%, respectively. Overall, urbanization has a positive contribution to the frequency, duration, and intensity of high temperatures in the BTH, YRD, and SCB regions. The PRD does not clearly match, possibly due to the strong influence of land-sea circulation and the geographical location near the equator. Urbanization-accelerated heat extremes are more pronounced in temperature climate zones, which may be attributed to the stronger UHI intensity resulting from lower wind speed and less evapotranspiration.
AS72-A021
Roles of Intra-seasonal Oscillations in the Sub-seasonal Prediction of the 2010 Long-lasting Compound Heatwave Over Southern China
Kaiqi WANG+, Tuantuan ZHANG#, Song YANG, Wenshi LIN
Sun Yat-sen University, China
Sub-seasonal prediction of regional compound heatwaves and their predictability sources remain unclear. In this study, the underlying mechanisms associated with a long-lasting compound heatwave occurred from 1-18 July 2010 over southern China, and the major sources of its sub-seasonal prediction skill are identified. The result shows that both the development and decay of this compound heatwave are mainly dominated by atmospheric processes (i.e., adiabatic heating associated with anticyclonic circulation), whereas the land-atmosphere coupling processes play an important role in sustaining the heatwave. Further analysis indicates that the tropical intra-seasonal oscillation with periods of 30-90 days and 10-30 days produce anticyclonic circulation over southern China and facilitate the occurrence and maintenance of the heatwave during its entire and second half periods, respectively. The National Centers for Environmental Prediction (NCEP) Climate Forecast System version 2 (CFSv2) shows a low skill in predicting the 2010 compound heatwave over southern China when the lead time is longer than 2-pentad leads, which is mainly attributed to the model’s bias in representing the intensity and phase of intra-seasonal oscillations.
AS72-A025
The Responses of Tree Radial Growth to the Summer Heatwaves in China Over the Past Four Decades
Shuhan NONG+, Peng ZHANG#
Nanjing University, China
The frequency and intensity of summer heatwaves have been increasing in China over the past few decades. Long-term records of such extreme events can be used to put the recent changes in a long-term context. That is essential to understanding the drivers of the long-term variations and changes of the high-temperature extremes. However, the observational records of the heatwave events are short, and cannot cover the long time period, especially before the industrial era. The tree-ring proxy has the potential to infer the variability of summer heatwaves over the past time, and has been successfully extend the variation of the frequency of the summer heatwaves over inner East Asia. Here we quantify the relationships between the variability of the radial growth of trees and the variabilities of the frequency, intensity and duration of the heatwaves over China on various timescales based on the publicly-available tree-ring width data in China, and the heatwave features calculated based on the ERA5 dataset. The results show overall increasing trends in the frequency, intensity and duration of the summer heatwaves over all the tree-ring sites in China for the past few decades. In contrast, the trees over the different sites exhibit distinct trends in their radical growth, with some showing increasing trends and some showing radical declines in the growths over the recent two decades. The statistical analysis shows that the correlation between the tree-ring growth and the heatwave frequency in summer changes from negative to positive with the increase in the elevations of the tree-ring sites. Despite an overall positive response, tree-ring growths show negative responses to the heatwave frequency in some high-elevation sites. Further results will show the spatial pattern and reasons of the response diversity of the tree-ring growth to the summer heatwaves in China over the past decades.
AS75-A014
Effect of Meteorological Data Assimilation on Regional Particulate Matter Forecasts Over the Korean Peninsula Using WRF-Chem and 3DVAR
Yunjae CHO#+, Hyun Mee KIM
Yonsei University, Korea, South
Meteorological data assimilation (DA) combined with the online coupled chemistry meteorology model (CCMM) can improve the air quality forecasts, as it helps reduce the uncertainties of meteorological initial conditions while considering the interaction between meteorology and air quality. In this study, the effects of meteorological DA on weather and particulate matter (PM) forecasts of the online CCMM are examined. Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) and WRFDA three-dimensional variational (3DVAR) system are used. The nesting domains of the model represent East Asia (outer domain) and the Korean Peninsula (inner domain), respectively. The two high PM concentration cases were selected, and four experiments with different DA domains were conducted for each case. When the meteorological DA was performed in the outer domain, the forecast errors (root-mean-squared error (RMSE) and bias) of meteorological variables were the smallest, while the errors were the largest in the experiment without DA. In addition, when the meteorological observations were assimilated in the outer domain, the forecast errors of PM concentration were the smallest. The effect of the meteorological DA on the PM forecast error reduction lasted approximately 58-66 hours. The synoptic meteorological forecasts were improved by performing meteorological DA in the outer domain. The improved forecasts in the outer domain enhanced the meteorological initial and boundary conditions of the inner domain, which consequently led to the improvement of the meteorological and PM forecasts in the inner domain. Acknowledgements: This work was supported by a grant from a National Research Foundation of Korea (NRF) grant funded by the South Korean government (Ministry of Science and ICT) (Grant 2021R1A2C1012572) and Yonsei Signature Research Cluster Program of 2023 (2023-22-0009).
AS75-A015
Anthropogenically and Meteorologically Modulated Ozone Trends Over China and Its Implications for Crop Yield and Human Health Since China’s Clean Air Actions
Dan YAN#+
Nanjing University, China
China has experienced increasingly serious ozone (O3) pollution in recent years, posing a great threat to agricultural ecosystem and human health. Here, we analyzed ozone trends across China using multi-source observations combined with multi-model calculations. Ozone increases steadily in China between 2013−2022, with a fast increase rate of 4.4 μg m−3 yr−1 in Phase I of Action Plan and a much smaller 0.6 μg m−3 yr−1 in Phase II. Results highlight that the deteriorative O3 pollution in Phase I and early Phase II is dominated by the nonlinear O3-emission response. Persistent decline in O3 precursors has shifted its chemical regime in urban areas and began to show a positive influence on ozone mitigation in recent years. Meteorological influence on O3 variations is minor until 2019 (~10%), but it greatly accelerates or relieves the O3 pollution after then, showing comparable contribution to emissions. Strong connections between surface O3 levels and SSC synoptic weather patterns are identified, with the dry tropical (DT) weather pattern featured by dry and hot air masses as the main contributor to 35.3% of the high ozone occurrences and partly explaining the observed ozone trends in recent decade (e.g., +9.7% ozone increase per tripling of the DT frequency). Using the agricultural statistical data and empirical algorithms, it is estimated that the annual yields of winter wheat, single-cropping rice, double-cropping early rice and late rice are reduced by 9.0−17.0%, 6.0−8.2%, 4.8−9.4% and 3.9−7.0%, respectively, in China during 2014–2022 due to the ozone exposure. Epidemiological model predicts totally 0.8−3.0 thousand yr−1 more deaths across China with altered anthropogenic emissions since clean air actions, and additional health burdens by −1.5~0.3 thousand yr−1 from perturbated meteorology. This study calls for stringent emission control and climate adaptation strategies to attain the ozone pollution mitigation in China.
AS75-A016
The Underlying Mechanisms of PM2.5 and O3 Synergistic Pollution in East China
Yawei QU#+
Jinling Institute of Technology, China
The rapid development of Chinese cities is accompanied by air pollution. Although the implementation of air pollution control strategies in recent years has alleviated PM2.5 pollution, O3 pollution and the synergistic pollution of PM2.5 and O3 have become more serious. To understand the underlying chemical interaction mechanisms between PM2.5 and O3, we applied the modified Weather Research and Forecasting model with Chemistry (WRF-Chem) to study the effects of aerosol-photolysis feedback and heterogeneous reactions on the two pollutants and revealed the contribution of different mechanisms in different seasons and regions in Yangtze River Delta (YRD) in eastern China. We found that, through the aerosol-photolysis feedback, PM2.5 decreased the surface photolysis rates JNO2 and JO1D, resulting in a decrease in O3 concentration in the VOC-sensitive area and a slight increase in the NOx-sensitive area. The heterogeneous reactions reduced O3 concentration in the YRD in spring, autumn and winter by consuming HxOy. While in summer, the heterogeneous absorption of NOx decreased O3 in the NOx-sensitive areas and increased O3 in the VOC-sensitive areas. Heterogeneous reactions also promoted the secondary formation of fine sulfate and nitrate aerosols, especially in winter. Through the combined effect of two chemical processes, PM2.5 can lead to a decrease in O3 concentration of -3.3 ppb (-7.6%), -2.2 ppb (-4.0%), -2.9 ppb (-6.3%), and -5.9 ppb (-18.7%), in spring, summer, autumn and winter in YRD. Therefore, if the PM2.5 concentration decreases, the weakening effect of PM2.5 on the ozone concentration will be reduced, resulting in the aggravation of ozone pollution. This study is important for understanding the synergistic pollution mechanism and provides a scientific basis for the coordinated control of urban air pollution.
AS75-A018
Impacts of Large-scale Land-sea Interactions on O3 Pollution in China's Coastal Cities
Songci ZHENG1+, Fei JIANG1#, Shuzhuang FENG1, Yang SHEN1, Huan LIU2, Hai GUO3, Xiaopu LYU3, Zhe CAI4, Mengwei JIA1, Chenxi LOU1, Chuanyou YING5, Xiaoyuan WANG6, Qian LIU1
1Nanjing University, China, 2Tsinghua University, China, 3The Hong Kong Polytechnic University, Hong Kong SAR, 4Nanjing Climblue Technology Co. Ltd., China, 5Fuzhou Research Academy of Environmental Sciences, China, 6Zhejiang Province Environmental Monitoring Center, China
Land-sea atmosphere interactions (LSAIs) are important processes affecting ozone (O3) pollution in coastal areas. While the effects of small-scale LSAIs, such as sea-land breezes, have been widely studied, the impact of large-scale LSAIs on O3 pollution is not yet fully understood. Here we investigated an O3 episode to illuminate the role of large-scale LSAIs in O3 pollution in the southeastern coastal, Bohai-Yellow Seas and adjacent regions through observations and model simulations. The results are presented below. 1) O3 pollution in southeastern coastal cities and the northern Bohai Sea’s coastal regions was mainly caused by transport from over the eastern China seas (ECS), the Bohai-Yellow Seas, respectively. 2) Affected by the Mongolian High, the study regions initially experienced a typical unimodal O3 diurnal variation. Precursors emitted from Beijing-Tianjin-Hebei, Northeast China (NEC) and Japan-Korea were transported to ECS, and precursors from Beijing-Tianjin-Hebei, Shandong, and NEC were transported to the Bohai-Yellow Seas. Photochemical reactions produced O3 in marine air masses, causing higher O3 levels over the sea than in coastal regions. As the Mongolian High shifted eastward and expanded, northeasterly winds transported O3-rich marine air masses from over ECS to the southeastern coastal regions, and southerly winds transported them from over the Bohai-Yellow Seas to their coastal region, which prolonged pollution and weakened diurnal variations. 3) In the southeastern coastal, Japan-Korea contributed the most, with an average of about 5 ppb and a peak of up to 30 ppb. The contributions of Beijing-Tianjin-Hebei and NEC were comparable, with an average of about 2 ppb and hourly peaks of 19 and 10 ppb, respectively. In the northern Bohai Sea, Shandong’s emission contributed significantly in both phases (27.5% and 26.1%, respectively), and emissions from the Korean Peninsula and marine shipping had a notable impact on O3 during the second phase (10.7% and 13.7%, respectively).
AS75-A023
Seasonal and Multi-scale Difference of the Relationship Between Built-up Land Landscape Pattern and PM2.5 Concentration Distribution in Nanjing
Cheng YUAN1#+, Jiachen MENG1, Wenchao HAN2
1Nanjing University of Information Science & Technology, China, 2Chinese Research Academy of Environmental Sciences, China
The urban landscape pattern, which can affect the air pollutants distribution in urban areas, was significantly changed due to the expansion of built-up land. Deeply understanding of the mechanisms by which urban landscape patterns influence the PM2.5 concentration distribution is fundamental for urban pollution control. However, the relationship between the built-up land landscape pattern and PM2.5 concentration distribution is still unclear at different grid scales in different seasons. In this study, four landscape metrics were calculated to quantify the distribution characteristics of built-up land in Nanjing, and the impact of built-up land landscape patterns on PM2.5 concentration distribution at different grid scales in different seasons was further analyzed. Results showed that the dominant landscape pattern metrics affecting PM2.5 concentration in different areas of Nanjing was closely related to the topography: in the main urban areas with flat terrain, the aggregation, shape, and proportion of built-up land significantly affected PM2.5 concentration, while the influence of the shape and proportion of built-up land was more noticeable in the hilly southwest suburbs. The effect of built-up land landscape pattern on PM2.5 concentration in winter was more significant than that in summer in general, and the relatively greater seasonal differences in this effect can be seen in the aggregation and proportion of built-up land. With the grid increasing, the correlation between the built-up land landscape pattern and the PM2.5 concentration distribution increased in the main urban areas but mostly decreased in the southwest suburbs, indicating that the PM2.5 concentration distribution in the main urban areas was mostly contributed by the spatial transmission of pollutants, while the PM2.5 concentration distribution in the southwest suburbs was mostly dominated by local emissions. We suggest that the planning of flexible urban strategies with respect of PM2.5 pollution control in different areas should be implemented considering the influence of topography.
AS75-A024
Relationship Between Arctic Oscillation and PM2.5 Concentrations in Seoul: An Analysis Using ERA5 Data and WRF Model Assessments
Junseo PARK1+, Woojin CHO1, Tae Ho MUN1, Hongjun CHOI1, Dong-Hyun CHA1#, Sung Chul HONG2, Min-Hyeok CHOI2, Jae-Bum LEE2
1Ulsan National Institute of Science and Technology, Korea, South, 2National Institute of Environmental Research, Korea, South
Monitoring and predicting fine particulate matter (PM2.5) concentrations is crucial for public health, especially in urban areas where air pollution is a significant risk. Understanding factors influencing PM2.5 variabilities – such as synoptic-field changes, interannual and seasonal variability, and climatic indices – is vital for effective air quality management and public health protection in densely populated and industrially advanced regions like East Asia. The Arctic Oscillation (AO) significantly influences regional weather patterns, potentially affecting air quality in urban areas like Seoul, Korea. This study investigates the relationship between PM2.5 concentrations in Seoul and the AO using ECMWF Reanalysis v5 (ERA5) and the Weather Research and Forecasting (WRF) model. From 2015 to 2023, we analyzed daily average PM2.5 concentrations from 48 air quality stations in Seoul, focusing on November to April, which typically experience numerous high concentration events. A regression analysis was conducted to understand the impact of AO phases on Seoul's air quality. This analysis identified that PM2.5 concentrations correlate with various weather variables, showing different patterns during positive and negative AO phases. These correlations uncovered the influence of the AO on air quality. Moreover, accurate forecasting of high PM2.5 concentration events is vital for public health and environmental management. Thus, we also evaluated the WRF model's performance in forecasting weather variables during high pollution events to enhance predictive accuracy and preparedness. This research found the impact of the AO on Seoul's air quality, verifying the interaction between synoptic-scale weather variables and urban-scale air pollution. Consequently, forecasting local-scale PM2.5 concentrations in East Asia must consider dealing with climate indices, particularly the AO phase.
AS75-A025
PM2.5 Contribution of Precursor Emissions in the East and West Regions of Gangwon Province, South Korea
Dongwon CHOI#+, Taehee KIM, Kyung-Hwan KWAK
Kangwon National University, Korea, South
Particulate matter (PM2.5) is generated not only by primary emission sources but also by secondary processes from precursors in the atmosphere. For this reason, the Ministry of Environment has recently implemented measures to reduce precursor emissions from power plants and on-road mobile sources nationwide. Despite the intensive efforts, the PM2.5 concentration remains steady both in the east and west regions of Gangwon province. To establish effective PM2.5 reduction measures in the Gangwon province, it is necessary to identify not only its emission sources in the regions but also the PM2.5 contribution of precursors. In addition, the Yeongseo (west) and Yeongdong (east) regions have different emission source characteristics in Gangwon province. This study aims to evaluate the PM2.5 contribution to air pollutants emitted from the Yeongseo and Yeongdong regions, separately in February 2023. We utilized the CMAQ-BFM(Brute Force Method) to calculate the PM2.5 contribution of air pollutants. PM10, PM2.5, SO2, NOX, NH3, and VOCs are chosen for emitted air pollutants in the contribution analysis. The simulation results of PM2.5 concentration were verified using data from urban air quality monitoring stations in the study area. Results showed that emission contribution from the Yeongseo region was approximately 20%, while that from Yeongdong region was approximately 10%. We estimate the contribution of each air pollutant for each region individually. Acknowledgment" "This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE)."
AS75-A028
Influences of External Inflow and Atmospheric Stagnation on PM2.5 Episodes in South Korea
Jimin KIM#+, Dongwon CHOI, Yeon-Uk KIM, Ha-Yoon JEONG, Kyung-Hwan KWAK
Kangwon National University, Korea, South
Fine particulate matter (PM2.5) episodes in Korea were primarily known to be originated from the inflow of pollutants from upwind countries and regions or occur due to atmospheric stagnation. To effectively manage such high PM2.5 concentrations, this study classified the occurrence types of high-concentration PM2.5 cases by utilizing an atmospheric recirculation factor (RF) and the concentrations of PM2.5 components (SO42-, NO3-, NH4+). Additionally, we quantitatively analyzed the dominance of inter-regional influence through time-lag correlation analysis. The target regions included Seoul, Ansan, Seosan, Daejeon, Gwangju, Ulsan, and Jeju, where the atmospheric environment research institutes operated by the national institute of environmental research are located. The study period is from January to December in 2021. Hourly concentration data of PM2.5 and its composition components, along with local meteorological forecasting model (LDAPS) data from the Korea Meteorological Administration, were analyzed. Four types of high-concentration cases were identified: inflow from abroad, stagnation after inflow, inflow from other regions, and atmospheric stagnation. As a result, the frequencies of inflow from abroad and atmospheric stagnation after inflow were high in the western coastal and metropolitan regions. Additionally, it was confirmed that sulfate and nitrate components are suitable indicators for foreign inflow and atmospheric stagnation, respectively. This work was supported by “the FRIEND (Fine Particle Research Initiative in East Asia Considering National Differences) Project through the National Research Foundation of Korea (NRF) funded by the Ministry of Science and ICT (2023M3G1A1090663).” and "This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE) (C10168180002)."
AS77-A005
Convective Cloud Detection and Tracking Using the Himawari-8 Data
Yikun YANG1#+, Chuanfeng ZHAO1, Yue SUN2
1Peking University, China, 2Beijing Normal University, China
As one of the precursors of severe storms, convective clouds are a special type of clouds that play a critical role in the global hydrological cycle and radiative energy budget at a local or global scale. Due to complex physical and dynamic processes and large spatiotemporal variability, convective clouds especially for the small spatial scales contribute to significant uncertainties in existing weather and climate models' simulations. Convective cloud detection and tracking is one of the crucial tasks to understand their development and evolution characteristics. Based on the Himawari-8 data with higher spatial and temporal resolutions, a convective cloud detection and tracking algorithm was constructed by combining machine learning, region-growing, area-overlapping, and Kalman filter algorithms. First, a complicated and strict spatiotemporal matching strategy between the Himawari-8 AHI data and CloudSat cloud profile radar was established, such as parallax correction model was constructed to minimize the impact of parallax. In addition, to expand the sample volume of convective clouds, region-growing algorithm is further used. Then, a convective cloud detection model suitable for both day and night time was constructed based on the XGBoost machine learning model. The convective cloud detection results are extensively evaluated by comparisons with cloud property products of JAXA AHI, traditional threshold algorithm, and CloudSat data. In addition, to achieve tracking of large-scale, small-scale, and fast-moving convective clouds, the automatic tracking of convective clouds algorithm is achieved by comprehensively using the area overlapping and Kalman filter algorithms. Validation results indicate that the algorithm developed can detect convective clouds of different scales with high accuracy, and the results show good continuity during day-to-night transitions.
AS86-A001
Some New Attempts of Decadal Increment Method in Decadal Climate Prediction
Yanyan HUANG#+
Nanjing University of Information Science & Technology, China
Effective Decadal/near‐term climate prediction can provide key climate information one or several decades in advance for policymakers and stakeholders, it has recently developed a high profile in the scientific community and beyond. However, current decadal climate prediction skill is far from successful. Our studies provide a new decadal increment method, which can skillfully predict the decadal variabilities of east Asian summer monsoon,summer precipitation over North China, extreme precipitation over South China and Pacific Decadal Oscillation. There are three steps in the increment method. First, the decadal variability (DV) of predictand is obtained by applying a 5‐year running mean. Second, the 3‐year decadal increment (DI) of the DV (DV at the current year minus the DV at the 3 years before, DI_DV) is predicted by a statistical forecast model with the leading several years of predictors in DI form. Third, the predicted DI_DV is added to the observed DV at 3 years ago to obtain the final DV prediction. This decadal increment method provides a promising and valuable approach to decadal climate prediction.
AS86-A002
Asymmetry of Winter Precipitation Event Predictions in South China
Shixin ZHEN+, Zhaolu HOU#, Jianping LI, Yina DIAO, Yazhou ZHANG
Ocean University of China, China
Winter precipitation anomalies in South China (SC) frequently result in severe disasters. However, the evaluation of prediction performance and distinctions between positive precipitation anomaly events (PPA, wet condition) and negative precipitation anomaly events (NPA, dry condition) in current operational models remains incomplete. This study employed the Climate Forecast System version 2 (CFSv2) to assess winter precipitation prediction accuracy in SC from 1983 to 2021. Differences in predicting PPA and NPA events and the underlying physical mechanisms were explored. The results indicate that CFSv2 can effectively predict interannual variations in winter precipitation in SC, as there is a significant time correlation coefficient of 0.68 (0.62) between observations and predictions, with a lead time of 0 (3) months. The model revealed an intriguing asymmetry in prediction skills: PPA outperformed NPA in both deterministic and probabilistic prediction. The higher predictability of PPA, as indicated by the perfect model correlation and signal-to-noise ratio, contributed to its superior prediction performance when compared to NPA. Physically, tropical signals from the ENSO and extratropical signals from the Arctic Sea ice anomaly, were found to play pivotal roles in this asymmetric feature. ENSO significantly impacts PPA events, whereas NPA events are influenced by a complex interplay of factors involving ENSO and Arctic Sea ice, leading to low NPA predictability. The capability of the model to replicate Arctic Sea ice signals is limited, but it successfully predicts ENSO signals and reproduces their related circulation responses. This study highlights the asymmetrical features of precipitation prediction, aiding in prediction models improvement.
AS86-A007
The CMA-GEPS Extreme Forecast Index for Temperature and Verification on the Extreme High Temperature Forecasts for the Summer of 2022
Fei PENG#+
CMA Earth System Modeling and Prediction Centre, China
In order to improve the ability of the CMA global ensemble prediction system (CMA-GEPS) to forecast extreme weather, aiming at the difficulty of reasonably calculating model climate due to small samples of historical forecasts from CMA-GEPS together with the lack of the re-forecast dataset, a method to build the model climate required by extreme forecast index (EFI) was investigated via using the insufficient samples of deterministic forecasts through extending the forecast samples in both time and space. By employing the operational forecast data of CMA-GEPS and the ERA5 reanalysis dataset, the forecast ability of CMA-GEPS for extreme high temperature in four representative regions at home and abroad for the summer of 2022 was evaluated. Results from the relative operating characteristic curve showed that CMA-GEPS EFI had the ability to discriminate extreme high temperature within the short- and medium-range forecast lead times of 1-10 days. Taking the maximum TS score as the criterion, the critical thresholds of EFI for issuing warning signals of extreme high temperature was determined. The forecast ability of EFI was decreased with the increase of forecast lead times, and different performance was exhibited in different regions: the forecast ability of extreme high temperature in the middle and lower reaches of the Yangtze River in China was higher than that in North China for all lead times; the forecast ability of EFI in western Europe was better than that in central Europe for the 1-7-d lead times, meanwhile the EFI forecast ability in central Europe for the 8-10-d lead times was better. Evaluation results from the economic value model revealed that risk decisions based on the EFI forecast information owned certain economic value. A case study further demonstrated that the CMA-GEPS EFI could provide early warnings for extreme high temperature in the medium forecast range.
AS86-A015
Impact of the Stochastically Perturbed Parameterization Tendencies Scheme in the Korean Integrated Model
Ja-Young HONG#+, Taehyoun SHIM, Shin-Woo KIM, Kyung-Hee SEOL
Korea Institute of Atmospheric Prediction Systems, Korea, South
The Korea Institute for Atmospheric Prediction Systems (KIAPS) was established in 2011 with a mission to develop a global atmosphere-only numerical weather prediction system for operational use at the Korea Meteorological Administration (KMA). This system was completed on schedule, and made operational at KMA in April 2020, immediately giving a world-class performance. The system is based on a new atmospheric model called the "Korean Integrated Model" (KIM), which is based on a cubed-sphere grid and uses the spectral element method within its dynamical core. Deterministic data assimilation (DA) is based on a hybrid-4DEnVar algorithm, and forecast uncertainties are modelled by a 50-member Ensemble Prediction System (EPS). The EPS is based on a local ensemble transform Kalman filter (LETKF) DA algorithm, and further schemes are included to account for deficiencies and uncertainties in the DA process and the forecast model. In this presentation, we examine the sensitivity to stochastically perturbed physical tendencies (SPPT), which aims to account for uncertainties in the forecast model and test a three-scale pattern, which consists of a linear combination of three independent random patterns, each describing a different correlation scale. To reduce computational costs, the sensitivity tests were carried out within a low-resolution framework, and we analyzed the effect of the schemes on the ensemble mean error and spread in temperature, geopotential height, and specific humidity in extended medium-range forecasts. In regions where the control experiment, including only initial perturbations, did not adequately reflect the ensemble spread, it is anticipated that the SPPT approach will result in increased forecast skill.
AS86-A016
Decadal Variations Afro-Asian Monsoon Rainfall: Roles of Atlantic Multidecadal Variability and Interdecadal Pacific Variability
Zichen TANG+, Song YANG#
Sun Yat-sen University, China
The Afro-Asian monsoon is a major component of the global monsoon system, with a large-scale rainbelt covering Africa, South Asia, and East Asia. Previous studies have demonstrated that the Afro-Asian summer monsoon (AfroASM) rainfall exhibits prominent decadal variability. By investigating observations and ensemble simulations, this study reveals that the decadal variation of the rainfall in the Sahel and eastern China is mainly caused by the interdecadal Pacific variability (IPV) and the Atlantic multidecadal variability (AMV), with positive (negative) phase of the AMV contributing to intensified (weakened) AfroASM rainfall, and the IPV corresponds to opposite impacts. The AMV and IPV influence AfroASM rainfall by modifying the tropical easterly jet (TEJ). Positive AMV favors a stronger TEJ, but positive IPV leads to a weaker TEJ, vice versa for their negative phases. The AMV elicits more contribution in the exit region of the TEJ, while the IPV contributes more in its entrance region, which concurs that the rainfall in the Sahel receives a larger impact from the AMV, and the IPV influences eastern China rainfall more strongly.
AS91-A003
Impacts of Urbanization on the Triggering Environment of an Tornado Event in Yangtze River Delta, China
Rumo WANG1+, Tianyi FAN1#, Zhaniqng LI2
1Beijing Normal University, China, 2University of Maryland, United States
Extensive observational and modeling studies demonstrate the influence of urbanization on the intensity of convective storms and extreme precipitation. Nevertheless, the impact of urbanization on the tornado triggering environment is relatively lacking at present. Here we examine the impact of anthropogenic aerosol emission and land surface changes on the triggering environment of an EF3 supercell tornado on 14th May, 2021 in Yangtze River Delta, a rapidly urbanized region in China. The event is simulated by Weather Research and Forecasting Model coupled with Chemistry (WRF-Chem) with an updated land use category. Significant Tornado Parameter (STP) is used to assess the tornado-triggering environment based on evaluation of convective available potential energy, wind shear, storm relative helicity, and lifting condensation level. Sensitivity tests show that anthropogenic aerosols due to urbanization enhances tornado-triggering environment, with the increase of storm relative helicity (SRH1) dominates the enhancement. Meanwhile, condensation of aerosol releases more latent heat, changes the airflow, and leads to the increase of SRH1. Moreover, change of land surface alters the sensible and latent heat fluxes, thus affecting the dynamical and thermodynamical conditions. Together, changes of aerosol and land surface due to urbanization influence the environment that are conducive to tornado formation.
AS91-A004
Urban Representation Based on Local Climate Zones (LCZs) for the Community Earth System Model (CESM)
Yuan SUN1#+, Zhonghua ZHENG1, Keith OLESON2, Cenlin HE3, Lei ZHAO4, Ning ZHANG5
1The University of Manchester, United Kingdom, 2National Center for Atmospheric Research, United States, 3NSF National Center for Atmospheric Research, United States, 4University of Illinois Urbana-Champaign, United States, 5Nanjing University, China
Urban areas worldwide are increasingly threatened by climate-driven risks. In response to the need for urban climate adaptation, an explicit urban representation in global climate models contributes to realistically simulating urban heat and water fluxes across regions. This study attempts to enhance representation of urban surface heterogeneity within the Community Earth System Model (CESM), by developing a new scheme to represent urban areas based on local climate zones (LCZs). In CESM's land component, the Community Land Model (CLM), we incorporated the urban LCZ scheme as an option alongside its default scheme. The CESM-LCZ scheme increases the subgrid-level urban land use types to 10 LCZs, with each LCZ represented by a unique set of urban canopy parameters (UCPs). The modified model is verified by present-day simulations and applied for future urban climate projections. We envision that the global-scale simulations of urban climates will provide scientific support for broader communities, enabling them to conduct assessments of LCZ-related impacts and inform urban planning decisions.
AS91-A005
Enhancing Extreme Rainfall Monitoring in the Philippines Using Average Recurrence Interval and Regional Frequency Analysis Approach
Danica LOQUELOQUE1#+, Julie Mae DADO2, Faye Abigail CRUZ2, Emilio GOZO2, Jose Ramon VILLARIN2, Sherdon Niño UY2
1Tohoku University, Japan, 2Manila Observatory, Philippines
Hydrometeorological disasters caused by extreme precipitation pose significant hazards in the Philippines, underscoring the urgent need for a robust monitoring system to safeguard human lives and assets in the country. This study proposes a tool for identifying potential extreme rainfall events using average recurrence interval (ARI). To enhance the reliability of ARI statistics beyond historical records, we employed Regional Frequency Analysis (RFA) across the Philippines, utilizing TRMM 3B42 rainfall data. Following the methodology outlined by Hosking and Wallis (1997), rainfall data were first pooled into homogeneous regions before estimating precipitation quantiles for different ARIs. Our findings reveal that RFA produced a lower Root Mean Square Error (RMSE) compared to traditional frequency analysis, signifying the reliable implementation of resulting ARI statistics for monitoring applications. To illustrate, three past cases of extreme rainfall events that vary in intensity and impact were examined. The equivalent ARI maps of these events captured areas that experienced flooding and landslides associated with the extreme rainfall event. Expanding our analysis, we applied ARI thresholds for extreme rainfall detection to our experimental WRF forecasts, comparing the outcomes with results based on monthly climatological rainfall thresholds. This comparative evaluation demonstrated the added value of ARI thresholds in detecting rainfall amounts surpassing monthly climatological levels, providing crucial insights into extreme weather monitoring. Lastly, recognizing the importance of medium-term rainfall events lasting up to a week, initial assessments exploring the physical and statistical properties of medium-term events revealed a seasonal pattern in different regions, particularly demonstrating improved homogeneity in areas affected by tropical cyclone disturbances, while variability remains over Mindanao and the Eastern Philippines during the northwest monsoon season. Despite these regional nuances, there is potential in using ARI for effective extreme weather monitoring applications, emphasizing its relevance across diverse temporal scales and geographical contexts.
AS91-A006
Social-economic Transitions and Vulnerability to Extreme Temperature Events from 1960 to 2020 in Chinese Cities
Yang XIE1, Ziqiao ZHOU2+, Qinghua SUN3, Mengdan ZHAO1, Jinlu PU1, Qiutong LI1, Yue SUN3, Hancheng DAI4#, Tiantian LI3
1Beihang University, China, 2City University of Hong Kong, Hong Kong SAR, 3Chinese Center for Disease Control and Prevention, China, 4Peking University, China
Climate change leads to more frequent and intense extreme temperature events, causing a significant number of excess deaths in cities in China. Using an epidemiological approach, we analyze all-cause deaths related to heatwaves and cold spells in 2,852 Chinese counties from 1960 to 2020. Economic losses associated with these events are determined through the value of statistical life. Findings reveal that cold-related cumulative excess deaths (1,133 thousand) are approximately 2.5 times higher than heat-related deaths, despite an increase in heat-related fatalities in recent decades. Monetized mortality due to heat-related events is estimated at 1,284 billion CNY, while cold-related economic loss is 1,510 billion CNY. Notably, cities located in colder regions experience more heat-related excess deaths, and vice versa. Economic development does not significantly reduce mortality risks to heatwaves across China. This study provides insights into the spatial-temporal heterogeneity of heatwaves and cold spells mortality, essential for policymakers ensuring long-term climate adaptation and sustainability.
AS91-A009
Impacts of Block-scale Urban Morphology on Strong Wind Induced by Typhoon "Muifa" (2212): A Case Study in Shanghai
Dahu YANG+, Ning ZHANG#
Nanjing University, China
Studying on the impacts of block-scale urban morphology on strong wind holds significant implications for predicting local severe winds, which have the potential to trigger safety and economic hazards. In this study, the strong wind induced by typhoon "Muifa" (2212) in Shanghai, China, was simulated using the Weather Research and Forecasting (WRF) model coupled with Parallelized Large-eddy simulation Model for Urban applications (PALM-4U). The findings were as follows: (1) Frontal area fraction (λf), building area fraction (λp), building surface to plan area ratio (λb) and height-to-width ratio (hw) showed a significant correlation with the strong wind indices (gust factor (GF) and relative wind speed (RS)). (2) The impacts of block-scale urban morphological indices on the average strong wind indices can be mainly categorized into two stages: acceleration and stabilization, and the transitional zone correspond to λf (0.07-0.09), λp (0.35-0.45), λb (1.3-1.6) and hw (2.2-2.4), respectively. (3) The accelerating effects of the urban morphological indices on the extreme features of the strong wind indices were manifested as the shifting and broadening of the probability density functions. In extreme cases, the average values would be significantly surpassed by the extreme values during the stabilization phase. The strong wind indices with 1% probability of occurrence can result in differences reaching λf (GF: 0.83, RS: 1.12), λp (GF: 1.03, RS: 1.34), λb (GF: 0.81, RS: 1.17) and hw (GF: 0.92, RS: 1.16), respectively.
AS91-A021
Assessment of Changes in Extreme Precipitation Indexes Affecting Flood Risk in Ulaanbaatar City, Mongolia
Baljinnyam NYAMJANTSAN#+, Dulamsuren DASHKHUU , Gantulga ONOLBAATAR
Information and Research Institute of Meteorology, Hydrology and Environment, Mongolia
In this study, four extreme precipitation indices with the highest impact on Ulaanbaatar's flood risk were chosen, and their changes over the last 60 years of climate data have been investigated. In addition, Future trends in maximum daily precipitation indices( RX1day), which are used as parameters for flood risk estimation, were estimated as well using regional ECAM5 and HadGEM2 model data. According to the findings, the number of consecutive rainy days increased from 1975 to 1994 and then decreased beginning in 1995. Throughout 1966 and 2022, observed daily maximum precipitation (RX1day) and extreme precipitation (R95p) indices rose by 2 mm and 7 mm, respectively. However, there was not a clear pattern in the number of days with precipitation greater than 20 mm (R20) across the years. However, there was no discernible trend in the number of days with precipitation of more than 20 mm (R20) over the years.
AS91-A024
Contrasting Interactions of Urban Heat Islands with Dry/Moist Heat Waves and Their Implications for Urban Heat Stress
Dong-Hwi KIM1#+, Kyeongjoo PARK1, Jong-Jin BAIK1, Han-Gyul JIN2, Beom-Soon HAN3
1Seoul National University, Korea, South, 2Pusan National University, Korea, South, 3Inha University, Korea, South
The interactions between urban heat islands (UHIs) and heat waves have been studied in many cities around the world because of their scientific interest as well as their influences on urban heat stress. However, few studies examined how these interactions vary with the characteristics of heat waves. Using observation data in Daegu, South Korea for 2001–2022, this study reveals that the interactions between UHIs and heat waves are contrasting under two distinct heat wave types (dry heat waves and moist heat waves). Dry (Moist) heat waves are defined as heat waves with daily mean relative humidity lower (higher) than its 10th (90th) percentile. Dry heat waves exhibit significantly higher temperature, lower cloud fraction, and lower soil moisture than those under moist heat waves. The mean UHI intensity, which is defined as the mean urban-rural difference in daily minimum 2-m temperature, under dry heat waves is significantly stronger than that under non-heat waves by 1.07 °C, but that under moist heat waves is weaker by 0.24 °C. This indicates that the interactions between UHIs and heat waves are primarily synergistic (negative) under dry (moist) heat waves. Interestingly, the temperature-humidity index, humidex index, and discomfort index in the urban area are not significantly different between dry and moist heat waves during the nighttime. This implies that heat waves that synergistically interact with UHIs do not necessarily lead to higher urban heat stress than those that negatively interact with UHIs. Therefore, monitoring changes in humidity under heat waves is indispensable for assessing extreme urban heat stress as well as interactions between UHIs and heat waves.
Session Chair(s): Xiaokang CHEN, University of Science and Technology of China, Zhe JIANG, Tianjin University
AS12-A001
Evaluating the Spatiotemporal PM10-2.5 Characteristics with High-resolution Predictions Based on an Ensemble Machine Learning Method in China, 2013-2020
Su SHI+, Weidong WANG, Renjie CHEN, Haidong KAN, Xia MENG#
Fudan University
There are limited studies investigating the health implications of coarse particulate matter (PM10-2.5). Accurate exposure assessment is important for conducting PM10-2.5–related epidemiological studies. In this study, we aimed to develop an ensemble machine learning method to estimate PM10-2.5 concentrations in mainland China during 2013–2020. The study was conducted in two stages. In the first stage, we developed two methods: indirect method refers to developing models for PM2.5 and PM10 separately and subsequently calculating PM10-2.5 as the difference between PM2.5 and PM10, which was commonly used in previous studies; and the direct method refers to establishing a direct model between PM10-2.5 measurements and relevant predictors, which few studies have done so. In the second stage, we integrated predictions from the indirect and direct methods with the generalized additive model. Internal cross validation (CV) and external CV were performed to validate the model performance. Overall, the indirect method performed better in internal CV with higher R2 and lower RMSE (R2=0.91; RMSE=10.02 μg/m3), while the direct method performed better in external CV (R2=0.62; RMSE=18.48 μg/m3). Predicting accuracy was improved in ensemble model regarding both internal CV (R2=0.95; RMSE=7.17 μg/m3) and external CV (R2=0.63; RMSE=18.30 μg/m3), comparing to indirect and direct methods. The predictions produced by the ensemble model captured the spatiotemporal pattern of PM10-2.5, even in sand and dust storms seasons. Our study provides an ensemble machine learning strategy with advantages of both indirect and direct methods for estimating PM10-2.5 concentrations, which holds significant potential to support future epidemiological studies and address knowledge gaps in health effects of studies.
AS12-A003
Advancing Gas-phase Chemical Solver in WRF-Chem: A Deep Learning Approach with Multi-head Self-attention Mechanism
Zihan XIA#+, Chun ZHAO, Qiuyan DU, Zining YANG, Mingshuai ZHANG, Liang QIAO
University of Science and Technology of China
Atmospheric gas-phase chemistry simulation is crucial for assessing environmental impact, crop growth, and human health. However, numerical models' computational cost has led to simplifications or even the omission of crucial chemistry. Previous attempts to use artificial intelligence (AI) algorithms have faced the curse of dimensionality and error propagation issues. Here, we present MHSA-CSolver, a novel approach that uses Multi-Head Self-Attention to replace the SAPRC-99 mechanism's numerical solver in WRF-Chem. It marks the first successful effort that an entire complex mechanism has been successfully replaced with a single AI solver and seamlessly coupled into a numerical model, enabling fast, accurate, and stable simulations without the need for separate solvers for each species as previously required. When we compared it with other AI solvers based on Multi-Layer Perceptron and Residual Neural Network architectures, our analysis revealed significant deviations in the simulation of ETOH, C2H2, and C3H6 using all AI solvers, which could be attributed to incomplete input variables we use neglecting key intermediate species involved in their reactions. Remarkably, MHSA-CSolver outperformed other AI solvers, delivering high simulation accuracy (mean R2 of 0.99, mean RMSE of 5.20 ppb, mean NMB of 1.88%, excluding ETOH, C2H2, and C3H6 from calculations) while maintaining fast simulation speed (14.3 seconds to predict concentrations of 74 chemical species across 675,000 grid cells on a single CPU). Moreover, we observed that adjusting the learning rate significantly enhanced the model's performance. Furthermore, upon coupling MHSA-CSolver into WRF-Chem, we achieved a remarkable speed improvement with a simulation time of 15.62 seconds, which is ~10.2 times faster than the original SAPRC-99 mechanism (158.93 seconds). The hybrid model successfully reproduced the spatial distribution and temporal sequence of various chemical species, particularly those challenging to simulate in previous works, such as NOx and HNO3.
AS12-A008
A Machine Learning Approach to Unraveling the Complex Relationship Between Air Pollution and Weather
Chiao-Wei CHANG+, Chien-Ming WU#
National Taiwan University
The air pollution weather (APW) in Taiwan can be recognized as a specific weather type that involves intricate interactions between the weather systems across multiple scales. In this study, we are developing a data-driven framework that maps the evolution of synoptic weather to local air pollution episodes and identifies the air pollution weather in Taiwan. A volume-to-point (VTP)-based autoencoder model is established with ERA5 reanalysis from 2006-2010 as the training dataset. The VTP-based autoencoder model can identify subtle differences in synoptic weather patterns. Within the latent spaces, the autoencoder model effectively distinguishes 19 distinct types of synoptic weather patterns in boreal winter, each displaying distinct configurations of mean sea level pressure (MSLP) and geopotential height on 500 hPa (z500). Among these synoptic weather patterns, we first identify seven types that are highly correlated with APW based on the statistical analysis of air pollution index (API) in Taiwan over each synoptic weather type. For instance, W1, W2, W12, W15 and W16 are exhibiting different propagation patterns of Rossby Wave and the Siberian-Mongolian High pressure (SMH) and the air pollution dispersion in Taiwan is regulated by the propagation of the edge of SMH. W6 is characterized with deep troughs favoring the extratropical cyclogenesis and the cold fronts that passes through Taiwan, the air pollution typically occurs in the intermittence between cold fronts. W14 manifests that the pattern that the major high- and low-pressure systems stay distant from Taiwan, and the continued weak-synoptic condition favors the air pollution. This framework can also be applied on future climate projection. The mitigation of synoptic weather patterns under various future climate scenario leads to the changes in climate distribution of APW in Taiwan. This framework can serve as quantified diagnosis tool but also a potential downscaling method.
AS12-A010
Deep Learning-derived Anthropogenic and Meteorological Drivers of Surface Ozone Change in China
Min WANG1+, Xiaokang CHEN1, Tailong HE2, Zhe JIANG3#, Jane LIU4, Hong LIAO5, Dylan JONES4, Yanan SHEN1
1University of Science and Technology of China, 2University of Washington, 3Tianjin University, 4University of Toronto, 5Nanjing University of Information Science & Technology
Urban air pollution continues to pose a significant health threat, despite regulations to control emissions. Here we present a comparative analysis of the anthropogenic and meteorological drivers of surface ozone (O3) change in China by integrating deep learning (DL) and chemical transport model (CTM) methods. The DL method suggests volatile organic compound (VOC)-limited regimes in urban areas over northern inland China in contrast to strong nitrogen oxides (NOx)-limited regimes in GEOS-Chem simulations. Sensitivity analysis indicates that the inconsistent O3 responses are partially caused by the inaccurate representation of O3 precursor concentrations at the locations of urban air quality stations in the simulations. The DL method exhibits possible weakened anthropogenic contributions to surface O3 rise in the North China Plain, for example, 1.53 and 0.54 ppb/y in 2015-2019 and 2019-2021, respectively. Similarly, GEOS-Chem simulations suggest an accelerated decrease in surface O3 concentrations driven by the decline in nitrogen dioxide (NO2) concentrations. Furthermore, both DL and GEOS-Chem models suggest the reverse of meteorological contributions to the observed O3 change in the North China Plain in 2019-2021, which is mainly resulted from the reversed changes in meteorological variables in surface air temperature and relative humidity. This work highlights the importance of DL as a supplement to CTM-based analysis. The derived O3 drivers are helpful for making effective regulatory policies to control O3 pollution in China.
Session Chair(s): Sandeep NARAYANSETTI, Indian Institute of Tropical Meteorology, Zhenchen LIU, Fudan University, Sridhara NAYAK, Japan Meteorological Corporation
AS11-A024
Local Land-climate Dynamics Worsen Climate Extremes and Heighten the Risk of Heat Stress for Humans
Oluwafemi Ebenezer ADEYERI1,2#+, Wen ZHOU3, Christopher NDEHEDEHE2, Kazeem ISHOLA4, Patrick LAUX5, Xuan WANG1
1City University of Hong Kong, 2Griffith University, 3Fudan University, 4Maynooth University, 5Karlsruhe Institute of Technology
Heatwave dynamics exhibit unique spatial heterogeneity, posing cascading environmental and societal challenges. Employing bias-adjusted climate models, we unveil these complexities by investigating heatwave dynamics, population exposure, and compound hydrometeorological extremes across 50 global regions within historical (1979-2014) and future epochs (2025-2060 and 2065-2100) under Shared Socio-economic Pathways (SSPs) 245 and 585. Our analysis reveals intricate couplings between heatwave occurrence and interlinked hydrometeorological extremes, including droughts and synergistic dry-hot events, regulated by large-scale atmospheric and terrestrial processes. Each region presents a unique climatological fingerprint, emphasizing the imperative for region-specific assessments over generalized approaches. For instance, robust lower-tropospheric moisture advection from the Atlantic Ocean into West and Central Africa, amplified by monsoonal winds, co-occurs with a Saharan monsoon trough and a weak Mediterranean ridge, mitigating heatwave frequency in these regions. Moreover, vertically integrated moisture flux convergence emerges as the dominant driver modulating heatwave frequency in the South American Monsoon zone, accounting for 41% of its variability. Relative humidity at 700 hPa and zonal winds at 1000 hPa also play significant roles, contributing 32% and 27%, respectively. Future projections depict a quadrupling of both heatwave frequency and compound events, exacerbating thermal stress and amplifying regional vulnerability. Population exposure to heatwaves is projected to escalate, exceeding fourfold and tenfold in the near- and far-future, respectively. Notably, South America and Europe exhibit substantial climate-driven exposure across all scenarios, underlining the urgency of regionally tailored adaptation and mitigation strategies in a warming planet.
AS11-A048
| Invited
Extremes in the Himalayas: Causes and Consequences on the Changing Climate
Netrananda SAHU#+
University of Delhi
Impact of climate change on hydrological regime in the Himalayan region is become a significant issue in Indian context. In the Himalayas, the hydrological processes keep on continuously disrupted due to decreasing rainfall, increasing temperature, reduced snow cover depth, population pressure, hydropower generation, dam construction, transportation development, road construction, intensive agricultural activities, and many others. Climate change has accelerated the melting of Himalayan glaciers, with profound impacts on the planetary health realms of the Himalayan region and that now threaten hundreds of millions of people. Rapid temperature rise in the Himalayas amplifies glacial retreat. Rising temperatures linked to increasing landslides in the Himalayas. Changing precipitation patterns in the Himalayas have a lot of implications for water resources and ecosystems. Accelerated biodiversity loss in the Himalayas due to climate change and habitat fragmentation. Rapid shifting of habitats in the Himalayas have implications for alpine flora and fauna, mounting threats to endangered species in the Himalayas. Altered species distributions provided evidence about the climate-induced disruptions. Himalayan ecosystems act as crucial carbon sinks, storing vast amounts of carbon. A call for urgent conservation efforts is necessary to preserve the pristine Himalayan environment.
AS11-A061
Compound Long-duration Dry and Hot Events in China: Characteristics, Drivers, and Projections
Yi YANG+, Jianping TANG#
Nanjing University
Compound dry and hot events can cause aggregated damage compared with isolated hazards, especially those with a long duration. Based on observations during 1961-2014, the spatiotemporal characteristics of compound long-duration dry and hot (LDDH) events in China during the summer season are investigated on both a grid basis and a 3D event basis. Grid-scale LDDH events mainly occur in eastern China, especially over northeastern areas. From a 3D perspective, 146 spatiotemporal LDDH (SLDDH) events are detected and grouped into nine spatial patterns. Over time, there is a significant increase in the frequency and spatial extent of SLDDH. Consistent with the grid-scale LDDH events, hotspots of SLDDH events mainly occur in northern China, such as Northeast, North China and Qinghai clusters, which are accompanied by high occurrence frequency and large affected areas greater than 300,000 km2. We then investigate the associated large-scale atmospheric circulation patterns and the physical processes causing their precipitation and temperature anomalies. Moisture budget diagnosis shows that precipitation deficits during the SLDDH events are produced primarily by the suppressed vertical moisture advection associated with the dynamical contribution of anomalous subsidence. In most regions, adiabatic warming due to abnormal subsidence plays a dominant role in determining the near-surface high temperatures during the long-lasting warm and dry periods. The future changes in LDDH events are analyzed using fourteen GCMs from CMIP5 downscaled by four statistical downscaling methods (BCSD, BCCI, BCCAQ, and CDF-t). The downscaling methods can efficiently improve the accuracy over the driving GCMs in terms of spatial variability, bias, and inter-annual variability of LDDH characteristics. In the mid-21st century (2041-2070), the number of SLDDH events under RCP4.5 and RCP8.5 is 2.5 and 3 times that of the present-day level, respectively. A substantial increase in spatially contiguous regions simultaneously experiencing LDDH events is seen by mid-century under both scenarios.
AS11-A063
| Invited
Analysis of Heat and Compound Humid and Dry Heat Extremes in Southeast Asia Under Climate Change
Jianjun YU1#+, Aurel MOISE1, Sandeep SAHANY1, Muhammad Eeqmal HASSIM1,2, Venkatraman PRASANNA1, Gerald LIM2, Chen CHEN1, Fei LUO1, Xin Rong CHUA1, Pavan Harika RAAVI1, Anupam KUMAR1
1Centre for Climate Research Singapore, 2Meteorological Service Singapore
Heat stress poses a growing challenge to the world, particularly in Southeast Asia (SEA), where the projected increase of population, urbanization, and economic expansion expose the region to escalating heat extremes. The compounding effects of humid- and dry-heat extremes amplify the social and environmental impacts in SEA countries. Despite these challenges, a comprehensive assessment of future changes in and exposures to these climate extremes in SEA is lacking. This study utilizes recent high-resolution regional climate change projections dynamically downscaling from CMIP6 from the Centre for Climate Research Singapore. Our primary objective is to assess the projected changes in return periods for the occurrence of heatwaves and the co-occurrence of humid- and dry-heatwaves under three emission scenarios (SSP1-2.6, SSP2-4.5, and SSP5-8.5). Results are analyzed using an ensemble mean of regional climate projections weighted by a skill score for simulating extremes. Comparative analyses with global climate projections are undertaken to contextualize the findings. Our findings indicate a consistent increase in the frequency of heat and compound heat extremes across all scenarios in SEA, with a sustained longer duration. Furthermore, we evaluate the exposure of population in SEA countries and megacities to these heightened heat extremes. The implications on climate change adaptation policies in SEA are discussed, emphasizing the urgent need for proactive measures to mitigate the adverse heat impacts.
AS11-A041
The Impact of Yellow Sea SST Warming on Tropical Night in Seoul Metropolitan Area
TaeHun KANG1#+, Donghyuck YOON2, Young Hyun KIM1, Dong-Hyun CHA1
1Ulsan National Institute of Science and Technology, 2Princeton University
Tropical night events in Seoul metropolitan area were classified into two types: pure-TN (no heatwave before tropical night) and HWTN (tropical night following heatwave). The Sea Surface Temperature (SST) in the Yellow Sea (YS), which has significantly increased over the past 30-year, demonstrated a high correlation with the frequency of tropical nights in Seoul. To investigate the impact of YS SST warming on tropical night in Seoul, the numerical experiment was conducted using the Weather Research and Forecasting (WRF) model. Two experiments were performed for 2013 and 2018, when pure-TN and HWTN were most prevalent; a control experiment (CTL) and a Cooling SST experiment (CSST) which reduced the SST anomaly (2013:1.3K, 2018:2.7K) for the YS area (34.5-38 N, 121-127 E). The impact of YS SST warming was examined by comparing the two experiments (CTL-CSST). The difference in dawntime temperature in Seoul between CTL and CSST was more pronounced in 2013 (0.48K) than in 2018 (0.37K) despite YS SST being lower in 2013 than in 2018. As of 2013 case, the longwave radiation and temperature advection, key synoptic factors for pure-TN, had opposite effects on dawntime temperature in Seoul. In CTL, less low-level cloud cover was simulated, leading to a decrease in net longwave radiation compared to CSST, which induced a cooling effect on temperature in Seoul. Meanwhile, the cold advection in CTL from the Yellow Sea to Seoul was weaker than in CSST, which could be interpreted as temperature advection played a role in preventing the cooling in Seoul in YS SST warming. This result indicated that YS SST warming influenced the increase in dawntime temperature in Seoul through decreasing cold temperature advection, particularly under pure-TN-like synoptic conditions. Furthermore, it suggests that the YS SST warming could be a key factor in the increased pure-TN in Seoul.
AS11-A011
Discovery of a Global Cold Nights Pattern Over Land in Boreal Winter: Circum-Hemisphere Teleconnection of Extreme Cold Events
Ning WANG+, Jianping LI#
Ocean University of China
This study discovers a global teleconnection pattern of cold nights (TN10p) in boreal winter by teleconnection method, which is termed as the Circum–Hemisphere Teleconnection of extreme cold events (CHTe), and investigates its spatial-temporal characteristics and possible causes. The CHTe exhibits five identified centers of action, namely the Southeastern North America, Baffin Bay Coast, Northern Europe, Middle East–North Africa, and Eastern Siberia. The CHTe index depicts that the CHTe displays significant interannual (~3a) and decadal (~10a) variabilities. Besides, the CHTe differs from the known atmospheric teleconnection patterns of the Northern Hemisphere in boreal winter in terms of temporal variability, occurrence year, spatial structure, the TN10p effects and removing the signals. During the CHTe events in boreal winter, the five regions of the CHTe are characterized by significant anomalous geopotential height at the mid-upper levels. This atmospheric circulation may influence the local surface air temperatures by modulating expansion or compression of atmospheric column, further impacting the local TN10p over these regions.
Session Chair(s): Yukio TERAO, National Institute for Environmental Studies
AS31-A024
Inventory System Accounting for Anthropogenic Carbon (ISAAC) for South Korea
Yeonsoo KIM1,2+, Sujong JEONG1#, Myeong-Gyun KIM3, Hyo-Jong SONG3
1Seoul National University, 2Climate Tech Center, 3Myongji University
Quantifying carbon emissions in high resolution is essential for understanding diverse emission characteristics across regions and, based on this understanding, supporting the establishment of carbon-neutral strategies for policymakers. In this study, we introduce ISAAC, the Inventory System Accounting for Anthropogenic Carbon, which estimates bottom-up carbon emissions from the Energy, Industrial Process and Product Use, and Waste sectors at a 1km2 per hour resolution for the years 2020-2022, starting with Seoul and with plans for nationwide coverage. In that, we categorized carbon emission sources into point, line, or area types and developed sector-specific algorithms to disaggregate activity data into these elementary resolutions on an hourly basis. Carbon emissions were calculated using the methodology of the highest applicable tier and then converted into a gridded format to integrate emissions for the entire sector. For uncertainty assessment, uncertainties associated with spatial and temporal allocations were taken into account. The estimated carbon emissions were observed to be greater than those reported by the Seoul Metropolitan Government but smaller than the ones in the Open-Data Inventory for Anthropogenic Carbon Dioxide (ODIAC) dataset. The findings of this study contribute to both political and scientific significance, serving as a basis for developing effective policies to mitigate carbon emissions and providing foundational data for research on understanding urban-scale climate change.
AS31-A004
Spatiotemporal Pattern of FFCO2 Emissions in Cities Around the Greater Bay Area
Jing ZHAO1#+, Guoqing LI1, Qunqun ZHAO2, Tuo WANG1, Tengfei YANG3
1Chinese Academy of Sciences, 2Shandong University of Science and Technology, 3National Earth Observation Data Center
Global fossil fuel CO2 (FFCO2) emissions accounted for more than 77% of the carbon emissions and cities alone account for more than 70% of the global FFCO2 emissions. Mitigation actions at the city level remain a challenge as the urban comprehensive greenhouse gas monitoring system is still under construction, and single monitoring data cannot achieve high-precision estimation and verification of urban carbon emissions. This study, using four high-resolution global-scale FFCO2 emission inventories (ODIAC 2022, EDGAR 8.0, PKU-CO2-v2, GRACED), established the connection between the global and regional scales by quantitatively analyzing the significant differences and variabilities, which are integrated into the constructed Kalman filter fusion algorithm to form FFCO2 emissions that present the best scale of the region. We selected the Greater Bay Area (GBA) as the study area. Sentinel-2 10m Annual Land Use Land Cover data assisted in generating the Urban-Rural Divide of the GBA. Nighttime light (NTL), Gross Domestic Product (GDP), and population density (POP) data were utilized to analyze emission factors from fossil fuel use. Before data reconstruction, FFCO2 emission data shows 140% at the average difference of grid cells in the region, greater than 130% at half of the grids, and greater than 80% at more than three-quarters of the grids. And the coefficient of variation (CV) reaches 16.3%. The reconstructed 3 km data reduce the uncertainty from ±15%-20% to ±10%. The analysis of the FFCO2 emission pattern, urban emission transfer paths, and the factors affecting urban and rural emissions in the GBA will provide a scientific basis for the optimal layout of energy and resources in the GBA and is of great significance to low-carbon transformation and high-quality development and the construction of a “Beautiful Bay Area”.
AS31-A016
Atmospheric Inverse Estimates of Carbon Emissions from Seoul Using Ground and Space Measurements
Sojung SIM#+, Sujong JEONG
Seoul National University
It is crucial to prioritize climate actions with accurate carbon emission estimates to achieve net-zero carbon emissions by 2050. However, the uncertainty of carbon emission estimates at urban scales is substantial due to limited access to activity data and outdated emission factors. The Bayesian inverse method, coupled with atmospheric CO2 measurements, can be employed as an independent verification method to enhance the accuracy of emission estimates. In this study, we verify Seoul’s CO2 emissions using the Bayesian inverse model and ground- and space-based measurements. We develop a Bayesian inverse modeling framework with input data, including anthropogenic CO2 emissions, biogenic CO2 fluxes, atmospheric CO2 measurement, a Lagrangian transport model, and error covariances of both prior emissions and observations. We validate existing CO2 emissions by estimating their optimal values and quantifying uncertainties through sensitivity tests. Finally, we assess the utility of this inverse modeling framework for science-based carbon neutrality policies by examining the contributions of anthropogenic and biogenic activities to CO2 concentration, as well as the spatiotemporal changes in CO2 emissions due to COVID-19. The abundance of ground and space observations over Seoul can sufficiently constrain urban CO2 emissions and support mitigation policies.
AS31-A023
Urban CO2 Flux Characteristics Segmentation Based on Land-use Type Accounting for Footprint
Geun Jae CHOI#+, Sujong JEONG
Seoul National University
The diversity of land types in urban areas introduces challenges in accurately identifying emission sources and sink areas in CO2 fluxes. This study addresses two fundamental questions: How do land-use type characteristics differ within footprint areas? And how can we better characterize the sources and sinks of urban CO2 fluxes within these footprint areas? Our overarching objective is to examine the spatiotemporal characteristics of urban CO2 fluxes, account for the varied land cover types within flux footprint areas, and propose an approach. This approach aims to provide insights into the challenges associated with emission source and sink identification in urban settings. For this study, we utilized approximately four years (2017–2020) of CO2 flux data from the National Institute of Meteorological Sciences, which were observed at five sites (Gajwa, Yongin, Nowon, Sungnam, and Tukseom). To directly characterize the influence of land-use types on flux, we rely on the footprint model proposed by Kljun et al. (2015). Each footprint was calculated for each CO2 flux recorded every 30 minutes. The footprint was polygonized and overlaid with the land-use type map, and the results were expressed as ratios within the footprint range. As a result of the study, YIN's forest ratio per unit footprint and CO2 flux in August were not correlated (r = 0.01), but vegetation effects were reflected (r = -0.43) when the effect of the built-up area was minimized. This suggests that detailed observation of land cover to transport air is necessary based on the footprint analysis. Our overarching objective is to contribute to policy decision-making for climate change mitigation in urban environments. This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Project for developing an observation-based GHG emissions geospatial information map, funded by Korea Ministry of Environment(MOE) (RS-2023-00232066).
AS31-A032
Real-time City-scale CO2 Fluxes Estimated from Background and Urban Greenhouse Gas Monitoring Data
Kyung-Hwan KWAK1#+, Yeon-Uk KIM1, Sooyeon KIM1, Yongchan KIM1, Jea-Chul KIM2
1Kangwon National University, 2AirTech Inc.
Actual emission amounts of greenhouse gases such as carbon dioxide (i.e., CO2) are fundamental to cope with the net-zero emission agenda worldwide. The greenhouse gas emission has been estimated using bottom-up approaches statistically, which is relatively uncertain and time-consuming. Recently, many observation-based methodologies have been proposed (i.e., top-down approaches) to estimate the greenhouse gas emission accurately in near-real-time. However, the observation-based ones have too low spatial resolutions to identify the exact location of emission sources or too small spatial coverage to guarantee the representative emission amounts at a city scale. This study aims to develop an observation-based methodologies for estimating city-scale CO2 fluxes based on two vertically located monitoring sites, which is known as a flux-gradient method. Chuncheon, a mid-size city situated in a basin, is an optimal place for assuming negligible horizontal fluxes of greenhouse gases below an altitude of 300 m, compared to its vertical fluxes geographically. We installed two greenhouse gas monitoring towers at the center of city and at the top of hill located at the boarder of city. By applying a proper atmospheric diffusivity between two altitudes, the net CO2 flux has been continuously monitored at a city scale. We will present the CO2 footprint at the background monitoring site for evaluating the suitability of city-scale CO2 flux estimation and daily/weekly/monthly variations of CO2 flux from the Chuncheon city. This work was supported by Korea Environment Industry & Technology Institute (KEITI) through "Project for developing an observation-based GHG emissions geospatial information map" funded by Korea Ministry of Environment (MOE) (RS-2023-00232066) and "Particulate Matter Management Specialized Graduate Program" through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE)".
AS31-A022
CANIFFER Project: Intensive Greenhouse Gas Monitoring at the Daesan Petrochemical Complex in South Korea
Jaewon JOO+, Sujong JEONG#, Dong Yeong CHANG1,1, Jonghyuk LEE, Yu-Ri LEE, Jaemin HONG, Hayoung PARK, Hyuckjae LEE, Jaewon SHIN, Jueun KIM, Jaehyun LIM
Seoul National University
To achieve carbon neutrality, it's crucial to proactively monitor and mitigate greenhouse gas (GHG) emissions in the industrial sector. The CANIFFER (CArbon sNIFFER) project conducts an intensive GHG monitoring campaign from January 6-14, 2024 (9 days) at the Daesan Petrochemical Industrial Complex, a major industrial hub in South Korea. This campaign aims to assess the current status of GHG emissions by monitoring carbon dioxide (CO2) and methane (CH4) concentrations in the atmosphere of the Daesan Petrochemical Industrial Complex using ground-based spectrometers (EM27/SUN), mobile, in-situ, aircraft, and satellite measurements, as well as GHG modeling methods. This campaign is the first to conduct GHG monitoring research on a large-scale petrochemical industrial complex in South Korea at a time when discussions on quantification and verification of GHG emissions through observations are actively underway. The results of the CANIFFER project will be presented at the AOGS 2024 21st Annual Meeting. This work was supported by Korea Environmental Industry & Technology Institute (KEITI) through "Project for developing an observation-based GHG emissions geospatial information map", funded by Korea Ministry of Environment (MOE)(RS-2023-00232066).
Session Chair(s): Song YANG, Sun Yat-sen University, Hirokazu ENDO, Meteorological Research Institute
AS04-A003
Rainfall Changes Over India in the Deep Future
Sahil SHARMA1,2#+, Kyung-Ja HA2, Eui-Seok CHUNG3, Keith RODGERS2, Sun-Seon LEE1
1IBS Center for Climate Physics, 2Pusan National University, 3Korea Polar Research Institute
Future rainfall changes in India are of paramount importance for crop production and water management, but to date longer-term changes have not been evaluated beyond the year 2100. Here, we leverage a 10-member extension of the CESM2-LE under relatively strong emissions to identify projected rainfall changes and their underlying drivers out to 2500. Our main finding is that after 2100 there are substantial changes in the large-scale atmospheric circulation patterns that are distinct from mechanisms identified for 21st century changes. In particular, we test the hypothesis that under substantial thermal perturbations to the climate system, after 2100 changes in atmospheric stability caused by tropospheric land-sea thermal contrast over India induce a northward shift of large-scale monsoon circulation, which, in turn, results in the northward shift of moisture transport and ultimately leading to increased summer monsoon rainfall over India. These changes reflect local expression of large-scale climate dynamical changes and provide more broader understanding of the underlying mechanism of long-term rainfall changes over India.
AS04-A022
Characteristics and Mechanisms of the Interannual Variability of the Northwest–southeast Shift of the Tropical Easterly Jet’s Core in July
Shihua LIU#+, Sihua HUANG, Zhiping WEN, Yanke TAN, Xiaodan CHEN, Yuanyuan GUO
Fudan University
Previous studies have pointed out that the tropical easterly jet (TEJ) core varies longitudinally or latitudinally. Whether there is a linkage between longitudinal and latitudinal variations of the TEJ core remains unclear. We found that, on the interannual time scale, the northward (southward) movement of the TEJ core is typically accompanied by a westward (eastward) shift, characterized by a noticeable northwest–southeast (NW–SE) displacement. This NW–SE shift is most evident in July. A locational index is defined to capture this shift by the difference of area-averaged 200-hPa zonal winds between the western Arabian Sea (AS) and the southern tip of the Indian Peninsula. Observations and numerical simulations demonstrated that the northwestward- shift (southeastward-shift) TEJ core is caused by the joint and individual influences from the enhanced (suppressed) convective activities over the eastern AS and suppressed (enhanced) convective activities over the northern Bay of Bengal–South China Sea (BOB–SCS). Enhanced (suppressed) convective activities over the eastern AS can induce upper-tropospheric divergence (convergence) and anticyclonic (cyclonic) circulations to the northwest of the convection, leading to anomalous easterly (westerly) over the western AS. The suppressed (enhanced) convective activities over the northern BOB–SCS can further facilitate the northwestward (southeastward) shift through inducing anomalous cyclonic (anticyclonic) circulation centering at the BOB and the associated anomalous westerly (easterly) over the southern tip of the Indian Peninsula. The NW–SE shift of the TEJ core may have an implication for the change in the area of the intense rainfall in South Asia.
AS04-A036
A Predictable Prospect of the South Asian Summer Monsoon
Xingwen JIANG1#+, Tuantuan ZHANG2, Song YANG2, Junwen CHEN3, Zhenning LI4
1Institute of Plateau Meteorology, China Meteorological Administration, 2Sun Yat-sen University, 3Shenzhen Wiselec Technology Co. Ltd., 4The Hong Kong University of Science and Technology
Prediction of the South Asian summer monsoon (SASM) has remained a challenge for both scientific research and operational climate prediction for decades. By identifying two dominant modes of the SASM, here we show that the unsatisfactory prediction may be due to the fact that the existing SASM indices are mostly related to the less predictable second mode. The first mode, in fact, is highly predictable. It is physically linked to the variation of the Indian monsoon trough coupled with large rainfall anomalies over core monsoon zone and the northern Bay of Bengal. An index is constructed as a physical proxy of this first mode, which can be well predicted one season in advance, with an overall skill of 0.698 for 1979–2020. This result suggests a predictable prospect of the SASM, and we recommend the new index for real-time monitoring and prediction of the SASM.
AS04-A038
Examining Scaling Patterns of Extreme Precipitation in High-resolution Global Climate Model: Implications for Future Indian Summer Monsoon
Stella JES VARGHESE1#+, Sajani SURENDRAN2, Kavirajan RAJENDRAN2, Subimal GHOSH3, Akio KITOH4, Karumuri ASHOK5
1Atria University, 2CSIR Fourth Paradigm Institute, 3Indian Institute of Technology Bombay, 4Meteorological Research Institute, 5University of Hyderabad
The increase in the atmospheric water-holding capacity with temperature, as explained by the Clausius-Clapeyron (CC) relationship, elucidates shifts in extreme rainfall intensities under warmer atmospheric conditions. Our investigation focuses on the attributes of extreme rainfall events (EREs) during the Indian summer monsoon season concerning thermodynamic variations and precipitation scaling across the Indian subcontinent and its homogeneous rainfall zones. We use data from both present-day climate simulations and future climate change projection experiments of a high-resolution global climate model. Noteworthy transformations are observed, particularly for very extreme rainfall events (vEREs), indicating their susceptibility to high temperatures. In the future, modified radiative forcing is anticipated to warm the upper atmosphere, introducing stability and counteracting the impact of increased humidity on precipitation intensity. Our analysis further suggests that the interaction of increased moisture content, circulation patterns, and the prevalence of convective clouds will contribute to future changes in EREs.
AS04-A067
Robust Increase in South Asian Monsoon Rainfall Under Global Warming are Driven by Southern Ocean Heat Uptake and Eurasia Cloud Changes
Yong-Jhih CHEN1#, Yen-Ting HWANG1, Jian LU2+
1National Taiwan University, 2Pacific Northwest National Laboratory
South Asian Monsoon (SAM) circulation projections under global warming are known to be highly uncertain among CMIP models, which largely contributes to the uncertainty in SAM rainfall responses. Here, we found that the long-standing uncertainty in SAM circulation changes in CMIP6 models’ future projections arises from two robust and compensating mechanism: a weakening of circulation due to thermodynamic control, and a northward shift of meridional overturning circulation. The thermodynamic weakening cancels out some of the projected increase in SAM rainfall expected from the wet-get-wetter mechanism, and the northward circulation shift explains more than half of the multi-model mean SAM rainfall anomaly. From an energetic perspective, the robustness in the regional northward circulation shift (and thus the increasing SAM rainfall) arises from the interhemispheric asymmetry in atmospheric energy budget originated from extra-tropics: the positive cloud feedback over the extra-tropical Eurasia Continent and the anomalous heat uptake in the Southern Ocean. Our partially-coupled CESM1 simulations supports that the land-sea contrast is not only controlled by the differences in heat capacity between land and ocean, as suggested by previous literature, but is also modulated by extra-tropical processes. When suppressing Eurasia Continent cloud feedback and Southern Ocean heat uptake in 4xCO2 simulation, the anomalous land-sea temperature contrast is reduced from 2.1K in the standard 4xCO2 simulation to 1.6K and the rainfall is reduced in most regions over South Asia. The study highlight that the energetic perspective is a powerful tool to understand monsoon variations. It allows a quantitative attribution of the shift in regional precipitation as the energy budget can be linearly decomposed; moreover, it links the potential root causes of circulation changes and their uncertainty to the TOA and surface fluxes that are tied to model physics and parameterizations, which is valuable for climate model developments.
AS04-A072
Response of Hydrological Cycle to the Climate Forcing Agents – Insights from the CMIP6 GCMs’ Simulations
Lakshmi Kumar T. V.1#+, Bharath JAISANKAR2, Koteswararao KUNDETI3,4, Humberto BARBOSA5, Rao V.B.6
1Jawaharlal Nehru University, 2SRM Institute of Science and Technology, 3National Center of Meteorology, 4National Center of Meteorology, 5Universidade Federal da Alagoes, 6National Institute for Space Research
Over a past few decades, the global hydrological cycle has been significantly impacted by factors such as Greenhouse Gases (GHGs), Anthropogenic Aerosols (AA), Land Use and Land Cover changes (LULC), and climate variability. Notably, the trends in monsoon precipitation in the northern hemisphere are closely tied to the presence of GHGs and AA. This study aims to comprehensively analyze the regional precipitation trends. The investigation is carried out by exploring the relationship between downward solar radiation and evapotranspiration using simulations from the CMIP6 General Circulation Models. The study covers historical data as well as separate experiments only involving GHGs, AA, and Natural Forcings spanning from 1850 to 2014. Analysis of regional trends in downward solar radiation highlights significant reductions in India and Eastern China, particularly from 1960s onwards. The trend analysis of evapotranspiration and precipitation over south and east Asia from the 1950s to 2010s showed a drying trend in Eastern China, while India had an increase in annual total evapotranspiration and rainfall in the same period. These opposing responses in these two regions are due to, more so than the greenhouse gas effect AA emissions having considerable control over Eastern China’s precipitation. In contrast, the greenhouse effect has strong controls on the Indian land region’s hydrological cycle exceeding the forcing brought on by the AA emissions. The models are categorized using a hierarchical tree clustering technique to analyze the model's internal uncertainty, revealing that certain models exhibit energy-limited biases. These biases lead to heightened evapotranspiration responses to insolation changes. These tendencies might be responsible for inducing aridity in the studied areas, consequently leading to an increase in simulated climate extremes.
Session Chair(s): Malte STUECKER, University of Hawaii at Manoa
AS61-A040
| Invited
A Pattern-aware Feedback Framework for Regional Climate Feedback and Projection
Jian LU1#+, Parvathi KOOLOTH1, Yi HUANG2, Derek DESANTIS3
1Pacific Northwest National Laboratory, 2McGill University, 3Los Alamos National Laboratory
We devise a pattern-aware feedback framework for the forced climate response using a suite of Green’s function-based solar radiation perturbation experiments to overcome the caveat of the existing climate feedback literature that disregards the co-variation between circulation and the radiative processes. By considering the energy balance at the top-of-atmosphere, a linear response function (LRF) for important climate variables and feedback quantities such as moist static energy, sea surface temperature, albedo, cloud optical depth, lapse rate etc., is learned from the experiment data. The learned LRF decodes the efficiency of the energy diffusion in both the ocean and atmosphere, and the pattern-aware feedbacks from the radiatively active processes. The LRF can then be decomposed into forcing-response mode pairs which are in turn used to construct a reduced-order model (ROM) describing the dominant dynamics of climate responses. These mode pairs capture the nonlocal effects in the climate response and feedback. An intriguing outcome of our approach is that the most excitable mode of the LRF captures the polar amplified response of the climate system and this mode is explainable in the data-learned, pattern-aware feedback framework. The ROM can be used for predicting the response for a given forcing and predicting the forcing from a given responses, with important bearings on geoengineering.
AS61-A003
| Invited
Impact of Intensified Tropical Rainfall on the Future Equatorial Warming Pattern
Hyuna KIM1#+, Axel TIMMERMANN2, Sun-Seon LEE2, Fabian SCHLOESSER3
1IBS Center for Climate Physics, 2Pusan National University, 3International Pacific Research Center
One of the most striking and robust features of future climate change projections in the tropics is the massive increase in precipitation simulated over the equatorial Pacific. Reaching levels of more than 20% per degree of global warming, the precipitation enhancement will inevitably reduce ocean stratification, which may lead to changes in upper ocean dynamics and temperatures. In our study we document, using a series of freshwater perturbation experiments with the Community Earth System model (CESM), that future equatorial rainfall intensification and its effect on ocean salinity play a fundamental role in establishing the enhanced eastern Pacific warming pattern, and in reducing the Pacific Walker circulation. The rainfall forcing and the corresponding shift in stratification and thermocline slope also explain the subsurface cold wedge, that has been seen in greenhouse warming simulations since the late 1990s and that had remained unexplained. Our results demonstrate that anomalous freshwater forcing does not only play a crucial role in high-latitude North Atlantic ocean dynamics but also as a key mechanism that shapes future climate change in the tropics.
AS61-A008
Influences from Outside of the Tropics Explain Recent Walker Circulation Strengthening
Masahiro WATANABE1#+, Yu KOSAKA1, Masaki TODA1, Ayumu MIYAMOTO2
1The University of Tokyo, 2University of California San Diego
The Walker circulation and associated tropical sea surface temperature (SST) distribution have a significant impact on global climate. However, climate models under historical forcing fail to capture the observed enhancement of the Pacific Walker circulation since around 1980 when observational uncertainty is small. Although a number of hypotheses have been proposed for this discrepancy, quantitative discussions and clues for model improvement are still lacking. Here, using climate model pacemaker simulations, we show that the Pacific Walker circulation strengthening since 1980 can be well explained by remote influence from extratropical SST changes. This equatorward influence occurs mostly through the atmosphere and thermal air-sea coupling. Influence from the Southeastern Pacific, which cools the eastern tropical Pacific, is crucial for the Walker circulation strengthening. We further show that current generation climate models have biases in Southeastern Pacific SST changes, which could have caused the failure in reproducing the Walker circulation trend.
AS61-A020
Historical Changes in Wind-driven Ocean Circulation Drive Pattern of Pacific Warming
Shineng HU1#+, Shuo FU2, Xiao-Tong ZHENG2, Kay MCMONIGAL3, Sarah LARSON4, Yiqun TIAN1
1Duke University, 2Ocean University of China, 3University of Alaska Fairbanks, 4North Carolina State University
The tropical Pacific warming pattern since the 1950s exhibits two warming centers in the western Pacific (WP) and eastern Pacific (EP), encompassing an equatorial central Pacific (CP) cooling and a hemispheric asymmetry in the subtropical EP. The underlying mechanisms of this warming pattern remain debated. Here, we conduct ocean heat decompositions of two coupled model large ensembles to unfold the role of wind-driven ocean circulation. When wind changes are suppressed, historical radiative forcing induces a subtropical northeastern Pacific warming, thus causing a hemispheric asymmetry that extends toward the tropical WP. The tropical EP warming is instead induced by the cross-equatorial winds associated with the hemispheric asymmetry, and its driving mechanism is southward warm Ekman advection due to the off-equatorial westerly wind anomalies around 5°N, not vertical thermocline adjustment. Climate models fail to capture the observed CP cooling, suggesting an urgent need to better simulate equatorial oceanic processes and thermal structures.
AS61-A039
The Role of Ocean Dynamics in Shaping the El Nino-like Response in Tropical Pacific
Fukai LIU1#+, Yiyong LUO1, Qiuxian LI1, Jian LU2
1Ocean University of China, 2Pacific Northwest National Laboratory
The relative roles of the oceanic and atmospheric processes in the pattern formation of the equatorial Pacific sea surface temperature (SST) response to global warming is investigated using a set of climate model experiments embedded with a novel partial coupling technique. The modeling results show that the SST response experiences a transition from a La Niña- like warming pattern at the initial stage to an El Niño-like warming pattern at the quasi-equilibrium stage. By decomposing anomalous equatorial Pacific SST into atmosphere thermally forced passive component and ocean dynamically induced active component, it is found that the SST warming pattern at both stages is entirely induced by its active component. Specifically, the meridional and vertical ocean circulation changes play a dominant role in forming the La Niña-like SST warming pat- tern at the initial stage, and the zonal and meridional ocean circulation changes are responsible for the formation of the El Niño-like SST warming pattern at the quasi-equilibrium stage. In contrast, the passive SST at both stages is characterized by a zonally uniform warming along the equator, which can be explained by a balance between the total effect of the heat transport divergence associated with the mean ocean circulation and the effect of the passive surface heat flux change. In addition, this study finds that it is the slowdown of the Pacific subtropical cells during the transition period that controls the evolution of the equatorial SST warming pattern by changing the meridional and vertical ocean heat transports.
AS61-A028
The Dominant Role of Cloud-radiation Feedback in the Projected Diversified Tropical Pacific SST Warming Pattern
Jun YING#+
Ministry of Natural Resources
The tropical Pacific SST warming (TPSW) pattern in response to global warming projected by almost all CMIP6 models displays a more consistent El Niño-like warming with a weakened zonal SST gradient compared with that by CMIP5 models. However, the magnitude of such warming varies among models, leading to uncertainties in the model projections of future climate change around the Pacific basin and beyond. Here, we find that the first two EOF modes of inter-model uncertainty in the TPSW pattern, explaining more than four fifths of the total inter-model variance, are both tied to different cloud–radiation feedbacks. The EOF1 mode that captures the inter-model difference in the magnitude of the El Niño-like warming as well as the largest inter-model variance in the far eastern equatorial Pacific, could be driven by different cloud–radiation feedbacks in the east. The EOF2 mode, that mainly represents the inter-model spread in the magnitude of the SST warming in the western equatorial Pacific, is primarily associated with different cloud–radiation feedbacks over the central equatorial Pacific which are further modified by changes in ocean dynamics and surface wind speed through a dynamical air–sea coupled process. Considering in isolation the robust common biases of weak negative cloud–radiation feedback over the central equatorial Pacific in models, the projected SST warming in the western equatorial Pacific would be smaller than the multi-model ensemble mean and the zonal SST gradient even more weakened than expected, implying potentially more severe climate extremes under global warming.
AS61-A038
Contrasting the Evolution of the Tropical Pacific SST Responses to Time-invariant Extratropical Forcings in the Two Hemispheres
Hung-Yi TSENG+, Yen-Ting HWANG#
National Taiwan University
This study aims to compare the influences of the northern and southern extratropics on the recent trend in tropical Pacific Sea Surface Temperature (SST) patterns, examining the SST responses in the tropical Pacific to extratropical energy flux imposed on either hemisphere using a fully coupled model CESM1.2. The response of the tropical Pacific SST depends on the hemisphere subjected to forcing. Initially, over the first three years, the two cases exhibit opposite responses in the equatorial Pacific region: Through coupled dynamics, the weakened cross-equatorial southerly trades warm the equatorial central Pacific in the northern-perturbed case while the strengthened southerly trades cool the equatorial region in the southern-perturbed case. Meanwhile, in the northern-perturbed case, the southward spread of the warmed SST in the Northern Hemisphere is blocked by the Intertropical Convergence Zone and fails to influence the equator. Within a decade, both scenarios demonstrate pronounced warming in the eastern equatorial Pacific, highlighting the role of the weakened Subtropical Cell and Equatorial Undercurrent in the development of cold tongue warming. Notably, despite less intense SST warming in the forced region, the southern-perturbed case shows earlier equatorial warming with a more substantial warming trend. Our results have implications for interpreting recent and projected near-future responses of tropical Pacific SST. For instance, the initial response implies that both the recent warming in the Northern Hemisphere's extratropics and the cooling trend over the Southern Ocean may have contributed to the equatorial cooling observed in the past two decades. Looking forward, as the Southern Ocean begins to warm and the slower teleconnection responses become more pronounced, a warming trend in the equatorial Pacific is anticipated. These findings suggest possible methods for reconciling discrepancies between models and observations using a mechanism-based diagnostic approach. However, the associated timescales require further exploration through more realistic experimental setups.
Session Chair(s): Guangxing LIN, Chinese Academy of Sciences, Yang GAO, Ocean University of China
AS38-A003
| Invited
Direct and Indirect Radiative Effects of Anthropogenic Dust on Climate
Xiaohong LIU1#+, Yang SHI2, Chenglai WU3, Zheng LU1, Zachary FRUITS1, Kai ZHANG4, Po-Lun MA4
1Texas A&M University, 2Massachusetts Institute of Technology, 3Chinese Academy of Sciences, 4Pacific Northwest National Laboratory
Dust can affect global climate by scattering and absorbing shortwave and longwave radiation. Dust particles can also modify mixed-phase and ice cloud properties by acting as ice nucleating particles (INPs). Dust is usually recognized as natural aerosol in the Earth system. However, it has been recognized that dust emissions are also related to anthropogenic activities and observations of dust deposition show a large increase in the industrial era. The anthropogenic dust (AD) emissions are not represented in almost all the global climate models and its direct and indirect radiative effects remains unassessed. In this study, we develop a new and physically based method to parameterize AD emission in the DOE’s Energy Exascale Earth System Model version 1 (E3SMv1). This method relates AD emission to the crop land use fraction in the E3SMv1 land component and further constrain the emission by soil moisture content. Our new parameterization produces an annual averaged AD emission of 584 Tg yr-1 in present-day (PD), which contributes to 13.5% of total dust emission. We find that due to the cropland use fraction change, the AD emission increases by 361 Tg yr-1 from pre-industrial (PI) to PD, which induces a net direct radiative forcing of AD of -0.028 W m-2. We further quantify the contribution of AD to global total dust INP population is by using soil dust ice nucleation parameterizations. The indirect radiative effects of AD through aerosol-cloud interactions are estimated.
AS38-A005
Arctic Amplification Induced Decline in West and South Asia Dust Warrants Stronger Anti-desertification Towards Carbon Neutrality
Fan WANG1#+, Yangyang XU2, Meng GAO1
1Hong Kong Baptist University, 2Texas A&M University
Dust loading in West and South Asia has been a major environmental issue due to its negative effects on air quality, food security, energy supply and public health, as well as on regional and global weather and climate. Yet a robust understanding of its recent changes and future projection remains unclear. On the basis of several high-quality satellite retrieval products, we consistently detect a decreasing trend of dust loading in West and South Asia over the last two decades. In contrast to previous studies emphasizing the role of local land use changes, here we attribute the regional dust decline to the continuous intensification of Arctic amplification driven by anthropogenic global warming. Arctic amplification results in anomalous mid-latitude atmospheric circulation, particularly a deepened trough stretching from West Siberia to Northeast India, which inhibits both dust emissions and their downstream transports. Single forcing ensemble model simulations further support the dominant role of greenhouse gases (GHGs) induced Arctic amplification in modulating dust loading over West and South Asia. Future projections under different emission scenarios imply potential adverse effects of carbon neutrality in leading to higher regional dust loading, and thus highlight the importance of stronger anti-desertification counter-actions such as reforestation and irrigation management.
AS38-A007
Modeling Nitrate Aerosols Over East Asia Using Variable-resolution CESM2-MOSAIC
Weiyi WANG1+, Xiaohong LIU2#, Guangxing LIN1, Chenglai WU1
1Chinese Academy of Sciences, 2Texas A&M University
To better represent aerosol properties and effects, we implement the Model for Simulating Aerosol Interactions and Chemistry (MOSAIC) in a variable-resolution Community Earth System Model (VR-CESM) with the highest horizontal resolution at ~0.125° to simulate nitrate aerosols over East Asia. The model captures fine-scale spatial distributions and local maximum values of precursor gases (e.g., SO2, HNO3, and NH3) and aerosols over North China and Sichuan Basin, but tends to underestimate nitrate, sulfate, and ammonium aerosol concentrations at the surface (>30%) compared to in situ observations in China. Over North China, the simulated mass fraction of nitrate burden in coarse mode (~50%) is larger than the previous study’ results. This is associated with a higher bias in dust emission over northwestern China as the model resolution increases and may contribute to a lower bias in nitrate concentrations. Over eastern China, the regional budget analysis of nitrate aerosol shows that its local formation rate is 5.03 Tg/year through gas-aerosol exchange (-10.76 Tg/year) and aqueous chemistry (15.79 Tg/year), which is balanced by the wet and dry deposition (3.95 Tg/year) and transport across boundaries (1.12 Tg/year), with average burden of 0.018 Tg and lifetime of ~1.3 day. Taking account of complex chemical processes and higher resolution, the model simulates detailed spatial patterns of aerosol optical depth (AOD) compared to satellite retrievals of AOD. The reduced low bias in AOD over eastern China (~10%) results from the representation of nitrate aerosol that induces an increase in AOD over North China, Guanzhong Plain, and Sichuan Basin despite uncertainties of dust simulation. These results imply that including complex physical and chemical processes in a high-resolution model is a promising method to study the impact of anthropogenic aerosol emissions over East Asia on air quality and climate change.
AS38-A009
Long-term Observational Analysis of Aerosol Effects on Precipitation in a Heavily Polluted Region
Mengjiao JIANG1,2+, Aili ZOU3, Shuhui LIU4, Guy BRASSEUR2#
1Chengdu University of Information Technology, 2Max Planck Institute for Meteorology, 3Nanjing University of Information of Science & Technology, 4China Meteorological Administration
With the presence of surrounding mountains, high population density and economic development, the Sichuan region experiences significant air pollution emissions. This research focuses on the influence of aerosols on precipitation in the Sichuan region using long-term observations. The analysis is based on various data sources, including hourly precipitation records from the National Meteorological Information Center of the China Meteorological Administration (CMA), MERRA-2 reanalysis data courtesy of the United States National Aeronautics and Space Administration (NASA), Fifth Generation Atmospheric Reanalysis (ERA5) from the European Centre for Medium-Range Numerical Prediction (ECMWF), and hourly Feng Yun Satellite (FY) FY-4A data provided by the National Satellite Meteorological Center of the China Meteorological Administration. The average 24-hour rainfall in the Sichuan region shows a trend of increasing and then decreasing with the increase of the AOD value. However, the turning points are different for clean and polluted regions in Sichuan. The role of aerosols on precipitation is not monolithic. Further analysis is done using satellite and reanalysis data to show the combination of microphysical effects and radiative effects for different rain intensities.
AS38-A013
The Worldwide COVID-19 Lockdown Impacts on Global Secondary Inorganic Aerosols and Radiative Budget
Takashi SEKIYA1#+, Kazuyuki MIYAZAKI2, Henk ESKES3, Kevin BOWMAN2, Kengo SUDO4, Yugo KANAYA1, Masayuki TAKIGAWA1
1Japan Agency for Marine-Earth Science and Technology, 2California Institute of Technology, 3Royal Dutch Meteorological Institute, 4Nagoya University
Air pollutants, including aerosols and tropospheric ozone, significantly affect the Earth’s radiative budget. Global lockdown measures to prevent the spread of the coronavirus disease 2019 (COVID-19) provide a unique opportunity to study the impact of rapid changes in anthropogenic emissions on air pollutants and climate change. While the COVID-19 lockdown impacts on both trace gases and total particulate pollutants have been widely investigated, secondary aerosol formation from trace gases remains unclear. To that end, we quantify the COVID-19 lockdown impacts on NOx and SO2 emissions, sulfate-nitrate-ammonium aerosols, and climate change using multi-constituent satellite data assimilation and model simulations. We find that anthropogenic emissions over East Asia, Europe, and North America were reduced by 19 to 25% for NOx and 14 to 20% for SO2 during April 2020. These emission reductions led to 8 to 21% decreases in sulfate-nitrate-ammonium aerosols over eastern China, Europe, and the eastern United States, corresponding to >34% of the observed aerosol optical depth declines and a global aerosol radiative forcing of +0.14 W m-2 relative to business-as-usual scenario for 2020. These results point to the critical importance of secondary aerosol pollutants in quantifying climate impacts of future mitigation measures. References: Sekiya, T. et al. (2023), The worldwide COVID-19 lockdown impacts on global secondary inorganic aerosols and radiative budget, Sci. Adv., 9, eadh2688, doi:10.1126/sciadv.adh2688.
AS38-A002
Enhanced Synoptic Systems and Air Pollution Due to Radiative Forcing of 2023 Canadian Fire Smoke
Aoxing ZHANG1#+, Tzung-May FU1, Yongqiang LIU2, Pak Wah CHAN3
1Southern University of Science and Technology, 2US Forest Service, 3Fudan University
The impact of wildfires on urban pollution is notably severe. In North America, wildfires often occur in conjunction with high-low-pressure systems, yet the knowledge of interactions between fires and these synoptic structures are limited. In this study, we conducted WRF-Chem simulations based on the Canadian Quebec Fire in June 2023, which had severe air quality impacts on the northeastern United States, to explore the interactions between extratropical cyclones and wildfires. We discovered a self-enhancement mechanism in wildfire transport: fire aerosol-radiation feedback increased air uplift on the fire side of the cyclone by 22%±11%, and the resultant increase in wind speeds led to a 28%±8% increase in ground-level PM2.5 concentrations in the severely polluted areas of the Northeastern United States. This study highlights the need to consider the assessment of wildfire-extratropical cyclone interactions in future climate scenarios, especially regarding their impact on global radiative balance and air quality.
Session Chair(s):
AS89-A013
| Invited
A Review on Oil Gas Methane Emission Measurements: Technologies, Key Findings and Challenges
Donglai XIE#+
Environmental Defense Fund
Methane emissions are a challenge to the global oil and gas industry and to the role and reputation of natural gas in a decarbonizing world. Today, the oil and gas industry has a methane-emissions data problem. The majority of emissions data is derived from desktop calculations informed by engineering equations and emission factors, not real-world measurements. This has significant consequences. Around the world, research reveals that methane-emission inventories consistently underestimate, and in some cases overestimate, actual emissions. Improving the accuracy of emission data is necessary to instill confidence that progress is being made. Advances in methane detection and quantification technology can support robust methane measurements across varying spatial and temporal scales. Over the last decade, various technologies have been developed to detect and quantify methane emissions from the oil and gas sector. These technologies cover source-level emission elements, underground pipelines, medium-scale sites/facilities, and larger-scale basins/continents in their application scenarios. The technology platforms encompass handheld devices; ground-based systems (tower and stationary continuous monitors); vehicle-based systems; airborne systems (drones, helicopters, and fixed-wing planes); and satellites in space. Various technologies and their key features have been reviewed. Key measurement findings for methane emissions from the oil and gas industry have been summarized, covering oil and gas elements (pneumatic devices, flares, storage tanks), operations (liquid unloading, completion flowback), upstream facilities (well pads, offshore platforms, abandoned wells, gathering/processing facilities, and oil sands processing), midstream facilities (pipes, compressor stations, underground storage), downstream systems (pipelines, facilities), and end-uses (domestic, industrial, and transportation). Key challenges for measuring oil and gas methane emissions are discussed, focusing on the temporal intermittency of large oil and gas production regions.
AS89-A019
Tracing China's Methane Growth Using GONGGA-CH4
Min ZHAO#+
Institute of Tibetan Plateau Research
The unprecedented surge in global methane levels has raised global concerns in recent years, casting a spotlight on China as a pivotal emitter. China has taken several actions in recent years to curb the methane emissions, but their effects remain unclear. Here, we developed the Global ObservatioN-based system for monitoring Greenhouse GAses for methane (GONGGA-CH4) and assimilate GOSAT XCH4 observations to assess changes in China's methane emissions. We find the growth in China's methane emissions (0.1±0.3 Tg CH4 yr-2) during 2016-2021 slowed down compared to the preceding years (2011-2015) (0.9±0.5 Tg CH4 yr-2), in contrast to the concurrent acceleration of global methane emissions. As a result, the contribution of China to the global methane emissions dropped significantly. Notably, the slowing down of China’s methane emission is mainly attributable to a reduction in biogenic emissions from wetlands and agriculture, due to a decline in wetland areas and the transition from double-season to single-season rice cropping, while fossil fuel emissions is still increasing. Our results suggest that GONGGA-CH4 provides the opportunity to track China’s methane emission in a quasi-near-real-time manner, providing insights in the implementation of methane-related policies that align with its ambitious climate objectives.
AS89-A017
Quantifying CH4 Emissions from Coal Mine Aggregation Areas in Shanxi, China Using TROPOMI Observations and the Wind-assigned Anomaly Method
Qiansi TU#+
Tongji University
China stands out as a major contributor to anthropogenic methane (CH4) emissions, with coal mine methane (CMM) playing a crucial role. To control and reduce CH4 emissions, China has made a dedicated commitment and formulated an ambitious mitigation plan. To verify the progress made, the consistent acquisition of independent CH4 emission data is required. This paper aims to implement a wind-assigned anomaly method for the precise determination of regional-scale CMM emissions within the coal-rich Shanxi province. We use the TROPOspheric Monitoring Instrument (TROPOMI) CH4 observations from May 2018 to May 2023, coupled with ERA5 wind and a bottom-up inventory dataset based on the IPCC Tier 2 approach covering three regions of Shanxi. The derived emission strengths range from 0.412 Tg yr-1 to 1.176 Tg yr-1, with an average uncertainty of 22%. Our estimates provide a comprehensive characterization of the regions within the Shanxi province, contribute to the validation of emission inventories, and provide additional insights into CMM emissions mitigation.
AS89-A009
| Invited
Unraveling Long-term Trends of Black Carbon Over China: Insights from MODIS Satellite and Implications for Potential Causes
Ying LI1,2#+, Yiwen LIU1, Haoxiang XU1, Fangwen BAO1
1Southern University of Science and Technology, 2Southern Marine Science and Engineering Guangdong Laboratory
Black carbon (BC) is a significant air pollutant with detrimental impacts on human health, climate, and the environment. Understanding its long-term trends is crucial for effective mitigation strategies. This study utilizes MODIS satellite data to estimate the long-term trends of BC over China, investigating potential causes and implications. The analysis reveals a comprehensive assessment of BC concentrations from 2000 to 2020. The results indicate a noticeable increase in BC levels during the early years, followed by a gradual decline in recent times. The spatial distribution of BC concentrations exhibits regional variations, with higher levels observed in densely populated and industrialized areas. To identify potential causes, various factors influencing BC emissions and transport patterns are examined. The study focuses on anthropogenic activities such as industrial emissions, residential energy consumption, and transportation. Additionally, meteorological conditions and atmospheric circulation patterns are considered as they can affect BC dispersion and accumulation. The implications of the observed long-term trends in BC are significant. The reduction in BC levels can be attributed to the implementation of emission control measures, stricter environmental regulations, and increased awareness of air pollution issues. These findings highlight the effectiveness of such measures and emphasize the importance of continued efforts. Moreover, the study underscores the need for continued monitoring and analysis of BC concentrations to evaluate the impact of ongoing mitigation strategies. It also emphasizes the importance of international collaboration in addressing transboundary air pollution, as BC emissions can have far-reaching effects beyond national borders. In conclusion, this study provides valuable insights into the long-term trends of BC over China based on MODIS satellite data. The observed decline in BC levels reflects the effectiveness of emission control measures, while regional variations underscore the significance of local factors. The findings emphasize the importance of sustained efforts to mitigate primary emissions, and air quality monitoring.
AS89-A003
Estimation the Characteristics of Rapidly Changed Strong Emissions Based on NO2 and CO Column Loading and Top-down Approach
Shuo WANG+, Jason COHEN#, Luoyao GUAN
China University of Mining and Technology
In the past few decades, air pollution has been attracting increasing attention, especially in developed and developing countries. Carbon monoxide (CO) and nitrogen dioxide (NO2) are common air pollutants, typically emitted from forest wildfires, fossil fuel combustion, and urban anthropogenic sources simultaneously. There is significant uncertainty in the classification, positioning, and estimation of emission sources in the current emission inventories, and the mixing state of air pollutants is closely related to the characteristics of emission sources. This work constructs daily to weekly constrained emission inventory of NOx and CO source regions globally, which are not previously identified in existing inventories are emphasized. First, the measurements of from 2006 to 2015 of NO2 and CO are analyzed using the Singular Value Decomposition method to pick out subregions undergoing maximal joint changes. These regions are separated into their different major source types based on the magnitudes, uncertainties, temporal variability, and other physical attributes: urban anthropogenic, biomass burning, and long-range transport, etc. Second, the variance-maximization approach and existing inventories (EDGAR, FINN, MEIC) were applied compute the emissions based on a model-free, mass conserving equation, which includes first order physics, chemistry, dynamics and in-situ processing. The results show there are more than 15 subregions all over the world where NO2 or CO or both emissions have been distinguished, with a significant co-emitted source from regions previously thought to have zero emissions. In addition, in each emission type, the intensity and time distribution of the ratio of NO2 to NO emissions are also different, depending on the source type and conditions, in-situ processing of NO2 and CO, as well as the surrounding environmental conditions. The new weighted NOx and CO emission inventories compare better with independent measurements and provide a next generation scheme which is rapid, of increased reliability.
AS89-A001
Hourly Surface NO2 Estimation with Uncertainty Quantification Using GEMS
Qin HE+, Kai QIN#, Jason COHEN
China University of Mining and Technology
Nitrogen dioxide (NO2), a crucial air pollutant, exhibits significant spatiotemporal variability. This study enhances estimating hourly 0.05° health-related near-surface NO2 concentrations from the Geostationary Environment Monitoring Spectrometer (GEMS), the first geostationary sensor to provide hourly daytime NO2 measurements over Asia. While machine learning (ML) has been explored for NO2 estimates, these efforts were limited by polar-orbiting satellite measurements, which yield only daily or instantaneous results. Moreover, challenges remain in assessing the extrapolation ability of ML models across new geographic space without prior training and quantifying the uncertainties in converting satellite-derived NO2 columns to near-surface concentrations. To address these issues, a cross-validation strategy optimizing the match between training and prediction locations is used for overall accuracy estimation, and a machine learning model is developed to concurrently derive the predictive uncertainty along with the NO2 concentrations for each point. The resulting model, trained with GEMS NO2 columns with land use, meteorological, and topographical inputs, captured up to 84% of hourly NO2 variation, achieving a root mean square error of 2.9 ppb and a mean absolute error of 2.1 ppb. Subsequent analysis of the spatial, seasonal, and diurnal variations of NO2 concentrations, derived from the ML model, offers detailed insights. Despite higher observational density in urban areas, the uncertainty remains higher due to spatial and temporal variability, indicating a need for enhanced observations to match the predictability in more remote regions. The explicit quantification aids decision-making and underscores the necessity of cautious interpretation in data-driven atmospheric predictions.
Session Chair(s): Jian-Feng GU, Nanjing University, Kosuke ITO, Kyoto University
AS30-A012
| Invited
A Comparison Between the Only Two Tornado Outbreak Events in China: Tropical Cyclone vs. Extratropical Cyclone Environments
Jingyi WEN1, Zhiyong MENG2#+, Lanqiang BAI3, Ruilin ZHOU 4
1Peking University, 2Department of Atmospheric and Oceanic Sciences, School of Physics, and China Meteorological Administration Tornado Key Laboratory, Peking University, 3Guangdong Meteorological Service, 4Peking University Chongqing Research Institute of Big Data
This study documents the features of tornadoes, their parent storms and the environments of the only two tornado outbreak events in China. The two events were associated with tropical cyclone (TC) YAGI on 12 August 2018, with 11 tornadoes, and with an extratropical cyclone (EC) on 11 July 2021 (EC 711), with 13 tornadoes. Possibly associated with the moister environment, most tornadoes in TC YAGI were spawned from discrete mini-supercells, while a majority of tornadoes in EC 711 were produced from supercells imbedded in QLCSs or cloud clusters. In both events, the high-tornado-density area was better collocated with K index rather than MLCAPE, and with entraining rather than non-entraining parameters possibly due to more moisture. EC 711 had a larger displacement between maximum entraining CAPE and vertical wind shear than TC YAGI, with the maximum entraining CAPE better collocated with the high-tornado-density area than vertical wind shear. Relative to TC YAGI, EC 711 had stronger entraining CAPE, 0-1-km storm relative helicity, 0-6-km vertical wind shear, and composite parameters such as entraining significant tornado parameter, which caused its generally stronger tornado vortex signatures (TVSs) and mesocyclones with a larger diameter and longer lifespan. No significant differences were found in composite parameter of these two events from U.S. statistics. Although obvious dry air intrusions were observed in both events, no apparent impact was observed on the potential of tornado outbreak in EC 711. In TC YAGI, however, the dry air intrusion may have helped tornado outbreak due to cloudiness erosion and thus increase in surface temperature and low-level lapse rate.
AS30-A006
| Invited
Tropical Cyclone Structure and Size: A Theoretical Exploration
Yanluan LIN1#+, Danyang WANG2
1Tsinghua University, 2Purdue University
As an important feature of tropical cyclone (TC), TC structure and size not only impact its flooding area, but also influence its intensity change and movement. First, physical processes influencing TC structure is investigated and it is found that irreversible processes strongly regulate TC structure. Next, a TC potential size model is introduced. The model provides an upper limit of TC outer radius based solely on TC environmental conditions. Finally, factors regulating the lower limit of TC maximum wind radius are discussed.
AS30-A009
Vortex Intensification Mechanisms Within a Numerically Simulated Real Tornado: Analysis of Buoyancy and Dynamic Forces
Wei HUANG1+, Ming XUE2#
1Nanjing University, 2The University of Oklahoma
The intensification of near-ground vertical vortex to reach tornado intensity is usually associated with rapid vertical acceleration and intense vertical stretching near surface. However, the primary cause of such vertical acceleration is still unclear. A successful numerical simulation of an EF4 supercell tornado case of Funing, China on 23 June 2016 is analyzed to understand the tornado vortex intensification mechanism. The vertical acceleration is divided into two parts: effective buoyancy force and dynamic vertical perturbation pressure gradient force (VPPGF). The dynamic VPPGF is further decomposed into the splat and split components by solving the pressure diagnostic equation to separately assess their contributions to the updraft acceleration. The results indicate that the dominant term for enhancing near-surface updraft is dynamic VPPGF, while effective buoyancy plays a weakly positive role in tornado intensification. In the initial stage of intensification, the positive dynamic VPPGF is dominated by the spin term associated with primarily vertical vorticity. The maximum vertical vorticity associated with the mesocyclone and the induced minimum perturbation pressure are located aloft, leading to an upward spin component of dynamic VPPGF that enhances updrafts and further intensifies the tornado vortex. When the ground-level vortex intensifies, the maximum vertical vorticity and the corresponding minimum perturbation pressure are found at the ground. The dynamic VPPGF induced by spin term now directs downward. At this time, the term responsible for maintaining strong vertical acceleration and stretching is now the splat component of VPPGF. This component is maximum near the ground, resulting in upward VPPGF. Horizontal convergence and deformation are primarily responsible for splat term. Trajectory analyses of parcels entering the tornado center further substantiate the above findings, indicating the very important role played by the splat component of dynamic VPPGF at the maintenance stage of tornadoes. This important process has not been identified in previous studies.
AS30-A004
Vortex Alignment During the Rapid Intensification of the Simulated Typhoon Rammasun (2014) in Moderate Vertical Shear
Yecheng FENG+, Liguang WU#
Fudan University
Tropical cyclone (TC) intensification under sheared environmental conditions has garnered significant attention in recent studies. The alignment of TC vortices in the vertical is recognized as a critical factor in the rapid intensification process. However, the mechanisms responsible for vortex alignment remain elusive. In this study, we utilize the high-resolution simulation of Super Typhoon Rammasun (2014) to investigate the evolution of vertical tilt, with a specific focus on the role of asymmetric convection. Our results reveal a structural transition from a misaligned vortex before the onset of rapid intensification to an aligned structure afterward. It is found that the diabatic heating, driven by the asymmetric convection, plays a pivotal role in counteracting the steering effect and offsetting the vertical tilt. We also demonstrate that asymmetric convection in the upshear quadrant significantly enhancing the reduction of vertical tilt. Our findings highlight the importance of the direct effect of diabatic heating on the tilt reduction of the simulated TC.
AS30-A001
Cloud-radiation Feedback Facilitates the Secondary Eyewall Formation of Tropical Cyclones
Yi-Fan WANG#+
Nanjing Innovation Institute for Atmospheric Sciences, Chinese Academy of Meteorological Sciences
Recent studies show that the formation of outer rainbans (ORBs) is essence to secondary eyewall formation (SEF) of tropical cyclones. This study reveals that cloud-radiation feedback (CRF) facilitates SEF of tropical cyclones by promoting the formation of ORBs and their stratiform sectors. In detail, CRF engenders an upper-level anomalous radiative warming in the outer-core region, which induces a secondary circulation that accelerates the release of microphysical heating above the freezing level. The enhanced upper-level latent heating further promotes the outer-core convection and the top-down development of the ORBs. Moreover, CRF promotes a broader stratiform precipitation area and stronger stratiform heating profiles of the ORBs, which forces convective updrafts at the radially inward edge of the stratiform precipitation area and eventually leads to SEF. On the contrary, when the anomalous radiative warming is removed, the organization of ORBs and the development of stratiform precipitation are suppressed due to the absence of the radiation-induced upper-level secondary circulation, thus inhibiting SEF.
AS30-A003
Rapid Perturbation Growth for Binary Tropical Cyclones
Kosuke ITO1#+, Johnny CHAN2,3, Munehiko YAMAGUCHI4
1Kyoto University, 2Asia-Pacific Typhoon Collaborative Research Center, 3City University of Hong Kong, 4Japan Meteorological Agency
It has been known that the track forecast errors of tropical cyclones (TCs) tend to be large when two TCs coexist within 1500 km. To elucidate the possible mechanism, singular vector (SV) analysis was conducted for the interaction of binary TC–like vortices on an f-plane in a nondivergent barotropic model framework. Compared with the SVs for a single vortex, the singular values for binary vortices are larger regardless of the separation distance. Sensitivity experiments show that the singular value can become relatively small with a surrounding basic negative vorticity in contrast to the case for a single TC-like vortex. The initial SV with the largest singular value (1st-ISV) becomes the evolved SV (1st-ESV) that corresponds to the displacement of dual vortices. The vorticity perturbation had a different sign between the center of binary vortices and the outer region in 1st-ISV and tilted against the wind shear in the outer region. The perturbation rapidly developed to the dipole structure about each TC center in a few hours. The dipole continued to grow as far as the necessity condition of barotropic instability was satisfied along the line between the centers of two vortices. In contrast, the time evolution of the perturbation energy almost ceased with the surrounding outer negative perturbation after 2 days. This is because the surrounding outer negative vorticity served to dispatch dual vortices in the basic field, and thus the necessity condition of barotropic instability was not satisfied after about one day. This work suggests that the TC structure and the coexistence of binary TCs can be relevant to the large track forecast errors.
AS30-A002
Tropical Cyclogenesis Bias Over the Central North Pacific in CMIP6 Simulations
Yi-Peng GUO1#+, Zhe-Min TAN1, Zhao JIUWEI2, Xiangbo FENG3, Xu CHEN4, Yi PENG1
1Nanjing University, 2Nanjing University of Information Science & Technology, 3University of Reading, 4The University of Tokyo
Current coupled climate models contain large biases in simulating tropical cyclogenesis, reducing the confidence in tropical cyclone (TC) projection. In this study, we investigated the influence of sea surface temperature (SST) biases on TC genesis in the Coupled Model Intercomparison Project Phase 6 simulations from 1979 to 2014. Positive TC genesis biases were found over the tropical Central North Pacific (CNP) in most of climate models, including the high-resolution models. Compared to coupled models, TC genesis density (TCGD) simulations over CNP in uncoupled models forced by observational SST improved obviously. A warm SST bias over the tropical CNP in the coupled models is the main cause of TC genesis biases. The SST bias-induced diabatic heating leads to an anomalous Gill-type atmospheric circulation response, which contributes to a series of favorable environmental conditions for TC formation over the CNP. Numerical experiments were also performed with HiRAM to demonstrate the influence of SST biases on the TCGD simulation, further confirmed our conclusion. The current results highlight the importance of improving TC simulation in state-of-the-art climate models by reducing SST simulation bias.
Session Chair(s): Kouji ADACHI, Meteorological Research Institute, Weijun LI, Zhejiang University
AS55-A018
Physical States of Aerosol Particles Revealed by Transmission Electron Microscopy
Kouji ADACHI#+
Meteorological Research Institute
Transmission electron microscopy (TEM) is an analytical technique that uses an electron beam to measure small objects, including aerosol particles. In addition to viewing nanoscale materials, TEM can measure the chemical and physical states of the target materials. TEM has been used to measure mixing states, physical and chemical properties, and images of aerosol particles collected around the world. This study focuses specifically on aerosol samples from biomass burning and the Arctic. Biomass burning has a significant impact on global climate. The Arctic region is strongly influenced by global climate change and vice versa. Examples include tarball formation in biomass burning smoke (an increase in the viscosity of organic aerosol particles in smoke) and aerosol mixing states of cloud residual samples in Arctic mixed phase clouds. Implications of the aerosol physical states for climate are discussed.
AS55-A017
| Invited
Liquid-liquid Phase Separation Reduces Radiative Absorption by Aged Black Carbon Aerosols
Weijun LI1#+, Jian ZHANG2,1
1Zhejiang University, 2Yantai University
Black carbon aerosols absorb radiation and their absorptive strength is influenced by particle mixing structures and coating compositions. Liquid-liquid phase separation can move black carbon to organic particle coatings which affects absorptive capacity, but it is unclear which conditions favour this redistribution. Here we combine field observations, laboratory experiments, and transmission electron microscopy to demonstrate that liquid-liquid phase separation redistributes black carbon from inorganic particle cores to organic coatings under a wide range of relative humidity. We find that the ratio of organic coating thickness to black carbon size influences the redistribution. When the ratio is lower than 0.12, over 90% of black carbon is inside inorganic salt cores. However, when the ratio exceeds 0.24, most black carbon is redistributed to organic coatings, due to a change in its affinity for inorganic and organic phases. Using an optical calculation model, we estimate that black carbon redistribution reduces the absorption enhancement effect by 28-34%. We suggest that climate models assuming a core-shell particle structure probably overestimate radiative absorption of black carbon aerosols by approximately 18%.
AS55-A003
Vertical Spatiotemporal Characteristics of New Particle Formation and Ultrafine Particle Evolution at Shenzhen Tower
Hao WU#+
Tsinghua University
New particle formation (NPF) can contribute exceed 60% when activated as cloud condensation nuclei (CCN) at the global scale, understanding the underlying mechanisms and factors is vital for the accurate assessment of particle impacts. Ultrafine particle (UFP) is pervasively distributed in the global atmosphere, their size smaller than 100 nm engender the wildly disparate from the surface to the free troposphere. However, measurements of NPF vertical distributions are rather limited, hindering our advanced understanding of the roles of UFP in the atmospheric boundary layer physical processes. The Shenzhen Meteorological Tower with a height of 356 m is the tallest meteorological in Asia, located in the Shiyan Meteorological Observatory (113.91°E, 22.66°N) near the Shenzhen airport (10 km to the west). The Tower provides 7 vertically distributed observation platforms (at 5, 40, 70, 120, 220, 335, and 350 m). On the ground the SMPS system consisted of a long DMA with a model 3772 CPC, the Nano-SMPS system consisted of a nano-DMA with a model 3776 ultrafine CPC was installed on the tower (350 m). The measurement cycle for the SMPS and Nano-SMPS was 5 min. The time series illustrated UFP at 350 m (14000 cm-3) was higher compared with the ground level (6500 cm-3). Nucleation/Aiken and UFP concentration reach the peak at 8:00 pm (3400/4200/7800 cm-3, respectively), but UFP on the tower exceeds 15000 cm-3 in the night. Vertical difference on polluted days attributed to nocturnal reactions dominated the formation of UFP due to the turbulence transport, our results suggest vertical mixing serves to spread the freshly nucleated particles and NPF precursors from the surface level to the levels higher up in the mixed layer. NPF comparison (GR: 8.29@Ground and 11.14@ Tower nm h-1) indicates that NPF happens faster on the upper layer, the event has 1 h lag on the tower. according to the back-trajectory results, air mass from the southeast origin in Pacific has transported the clean air to tower and ground successively, the CS level has reduced sharply from 0.02 to 0.01 s-1 when the air mass trajectory arrived at tower sites. Vertical spatiotemporal characteristics of new particle formation on tower providing us a unique chance to research the difference and air mass transport impact on the vertical NPF events.
AS55-A010
Enhanced Radiative Properties by Black Carbon in Response to Particle Mixing Structure
Yuanyuan WANG#+, Weijun LI
Zhejiang University
Absorption by black carbon (BC) in the atmosphere strongly affects radiative balance and global climate. The large discrepancies in observed and modeled BC absorption enhancements raise a hot debate. Through applying a new 3D shape model based on electron microscope observations, we propose a new framework that estimates BC absorption enhancement through accounting for mixing structure diversity in individual particles. Our results reveal that the diverse range of mixing structures in individual particles in ambient air leads to complex absorption enhancement that could hardly be predicted by the empirical approximation. The bulk absorption enhancements based on diverse mixing structures provide an explanation for the globally disparate results from laboratory and field observations. The new framework linking microphysical structures to bulk BC optical properties can be used to improve assessment of climate impact.
AS55-A008
Spatial Contrast in Abundance and Mixing State of Black Carbon Particles in Arctic Marine Air
Xiaomi TENG1#+, Weijun LI1, Zongbo SHI2
1Zhejiang University, 2University of Birmingham
Black carbon (BC) contributes to the amplified Arctic warming. There is a geographic bias in Arctic BC studies with lack of observational constraints over sea surface. Here, shipborne observations during May-June 2022 at western Greenland Arctic establish a strong spatiality in both mass concentrations (16.1 ng·m−3 to 61.5 ng·m−3), individual abundance (7 to 31% by number fraction in 80 nm-2 um), mixing state (49 to 86% internally mixed soot) and sources (12 to 19% contribution from biomass burning) of BC, as we classified four BC-involved spatial regions: remote ice-melting sea (IS), typical open sea (OS), coastal urban-influenced air (UA), and ship-influenced events (SE). Spatial discrepancy suggests that soot particles underwent ageing process from coast to IS, and should be typically considered in regional climate models. Additionally, domestic BC particles from incomplete fossil fuel burning should be paid attention due to the growing human activities in Arctic under the global warming.
Session Chair(s): Shu-Chih YANG, National Central University, George Zhizhao LIU, The Hong Kong Polytechnic University
AS18-A007
Assimilating Dense Ground-based GNSS ZTD Observations for Improving Very Short-term Precipitation Prediction in Taiwan
Shu-Chih YANG1#+, Yi-Pin CHANG1, Ta-Kang YEH2
1National Central University, 2National Taipei University
A convective-scale ensemble data assimilation (EDA) system has been developed in Taiwan to improve very short-term heavy rainfall prediction. This system assimilates the GNSS-ZTD observation from 118 ground-based GNSS stations maintained by the Central Weather Administration (CWA). The ZTD data are available every 30 minutes and thus provide fast moisture information, which can capture the precursor of convection initialization. Results with multiple afternoon thunderstorm events show that assimilating the GNSS-ZTD data provides effective moisture adjustment. Incorporating the surface 10-meter wind further exploits the benefit of ZTD assimilation in very short-term precipitation prediction. Nevertheless, the moisture correction is still limited in the data void region. In addition to the CWA-operated GNSS ZTD stations, more than 400 non-CWA GNSS stations are deployed in Taiwan for purposes like geodesy. This provides a very dense GNSS-ZTD observation network in Taiwan. Most importantly, some non-CWA GNSS-ZTD observations are available over the coast of northwestern Taiwan and around the Taipei Basin. A preliminary investigation of a severe afternoon thunderstorm on 22 July 2019 in the Taipei Basin shows that these data indicate high moisture content 30 minutes before the convection initialization. These data are expected to compensate for the limitation of assimilating the CWA GNSS ZTD, particularly in improving the moisture transport from the upstream. More results on rapid-update data assimilation and very short-term precipitation prediction will be discussed in the presentation.
AS18-A011
GNSS Atmospheric Sounding – The Road Ahead
Kefei ZHANG1#+, Suqin WU1, Longjiang LI1, Dongsheng ZHAO1, Peng SUN1, Haobo LI2, Minghao ZHANG1, Yumeng HAO1, Tong ZHU1
1China University of Mining and Technology, 2RMIT University
As one of the most important sources of atmospheric information, water vapor is very valuable for the studies of extreme weather events and climatic phenomena. The GNSS, demonstrated to be a very effective technique for sounding atmosphere, has experienced unprecedented developments over the past decade due to the rapid deployment of wide-spread space- and ground-based infrastructures. This significant development and the long-term accumulation of GNSS data, has offered a strong data support and new opportunity to advance our understanding of climate change and extreme weather events. This, coupled with the fifth resurgence of artificial intelligence (AI), significant new development of space science and technology and network of satellite networks etc. world frontier advancements, has empowered us enormous new capability and capacity and heralded new horizons of possibilities. All these are expected to help us in the deepening the understanding the atmospheric dynamic process, and mining the detailed information of the formation, evolution, development and dissolution of extreme weather events and complicated atmospheric process. This contribution presents a summary of our 20-year relevant research in the area that involves a full spatial domain of ground-, air- and space-based systems and a comprehensive technological domain of GNSS/geodesy, remote sensing, meteorology and atmosphere. First, the background, current status and recent international frontier developments of the GNSS tropospheric sounding technique are summarized. Then, the theory, technical features and major advancement of the GNSS-derived atmospheric products in the applications of climate analyses and extreme weather forecasting are presented. Finally, the challenges, opportunities and future prospectives in terms of the technique and its innovative applications of national and international significance are provided.
AS18-A014
Tomography Algorithm Used the Gaussian Horizontal Restriction and Sounding Vertical Restriction in the Troposphere Using GNSS
Rong WAN#, Zhikang FU, Zhikang FU, Yang HU+
China Meteorological Administration
GNSS meteorology theory makes GNSS detection of atmospheric water vapor as possible. The motivation of this paper is to obtain the 3D water vapor density products by the grounded GNSS net by tomography method. To solve the lack rank equations,Gaussian horizontal restriction and sounding vertical restriction are used in the tomography algorithm. Not only the wet refraction but the regional water vapor density can be retrieved by the constraint-based tomography algorithm. Water vapor density average deviation is -0.63g/m3, the standard deviation 1.22 g/m3, and the sounding correlation coefficient 0.98. With the introduction of low-level water vapor observations, the three-dimensional water vapor density accuracy has been improved in the whole region, including the lower layer and edge.
AS18-A004
Assimilating FY-4A PWV Retrievals to Improve the WRF Forecasting Performance of Typhoon Haikui
Dengxin HE, George Zhizhao LIU#+
The Hong Kong Polytechnic University
Water vapor is one of the most essential components of the atmosphere and plays an important role in the formation and development of severe weather. This study aims to investigate the impact of assimilating water vapor data retrieved from the FengYun-4A (FY-4A) satellite on the precipitation forecast associated with Typhoon Haikui in the year 2023. By assimilating water vapor data derived from the FY-4A satellite into the numerical weather model, the research focuses on the specific analysis of Typhoon Haikui, examining the effects of assimilating FY-4A satellite-retrieved water vapor data on the precipitation distribution and intensity caused by the typhoon. Various assimilation schemes are conducted to evaluate the effectiveness of assimilating water vapor data by comparing their impacts on Typhoon Haikui's precipitation forecast results, which shows that assimilating FY4A satellite water vapor data holds promising potential to improve the accuracy of forecasting precipitation associated with Typhoon Haikui. This study conducts further analyses to better understand the specific mechanisms behind the role of assimilating FY-4A water vapor data in enhancing precipitation forecasting accuracy related to typhoons and improves the forecast performance by applying the FY-4A satellite-retrieved water vapor data into the WRF model.
AS18-A003
ESTGN: A Multi-factor Driven Graph Network for GNSS Reflectometry Global Ocean Wind Speed Estimation
Zhuo WANG#+, Cuixian LU, Yuxin ZHENG, Yini TAN, Jiafeng LI, Chengbo LIU
Wuhan University
Ocean surface winds play a crucial role in shaping Earth’s weather and climate. In recent years, the Cyclone Global Navigation Satellite System (CYGNSS) mission, launched in 2016, has demonstrated its capability as a reliable remote sensing constellation for retrieving ocean wind speed. This study introduces a novel ensemble spatial-temporal graph network, ESTGN, designed to retrieve ocean wind speed using multiple CYGNSS observations. Initially, the Graph Attention Network (GAT) algorithm is employed to aggregate and extract spatiotemporal features from the Delay Doppler Map (DDM) around the Specular Point (SP). Subsequently, these extracted features are input into Transformer networks to formulate the wind speed forecasting model. The performance of our approach over conventional retrieval algorithms and other deep learning-based methods are evaluated against the fifth generation European Centre for Medium-Range Weather Forecasts (ECMWF) reanalysis (ERA5) products. Additionally, error analysis is conducted to demonstrate the model's robustness at both spatial and temporal scales. The study demonstrates the effectiveness and feasibility of the spatiotemporal deep graph attention neural network in efficiently processing GNSS reflectometry observations and achieving accurate global-scale ocean wind speed retrieval.
AS18-A006
The Spatio-temporal Characteristics of Columnar Water Vapor During Tropical Cyclones Using GNSS Radio Occultation and Altimetry Satellite Data
Jiaqi SHI1+, Min LI1#, Wenwen LI1, Minghao ZHANG2, Kefei ZHANG2
1Wuhan University, 2China University of Mining and Technology
Tropical cyclones (TCs), predominantly occurring in tropical subtropical marine regions, represent complex severe convective weather systems and is typically accompanied by heavy rainfalls. Due to climate change, the Northwestern Pacific region, a hotspot for TCs, has experienced increases in both frequency and intensity of TCs recently. This has exacerbated rainfall-induced flooding disasters, posing significant threats to human life and property in coastal areas. Given close correlation between rainfall and atmospheric water vapor, accurate observation of water vapor dynamics during TCs is crucial. Global navigation satellite system (GNSS) radio occultation (RO) technology provides substantial of atmospheric sounding data globally in all-weather conditions, while Altimetry satellites also contribute crucial water vapor information in ocean regions; they can jointly contribute significantly to a comprehensive analysis of water vapor variations during TCs. By integrating datasets from COSMIC-2, Spire, METOP, FY-3 and Jason-3 observations, we analyzed atmospheric parameters and columnar water vapor (CWV) during 39 TCs in the Northwestern Pacific region from 2019 to 2023, with a focus on tracking parameter variations along TC paths and their correlation with wind speed and distance from the TC's eye. A CWV increase of about 26% was observed within 0.5–10 km altitude during TCs, while a wave-like structure in specific humidity and water vapor pressure profiles was indicated relative to distance from the TC’s eye. For altitudes below 10 km, specific humidity and water vapor pressure revealed a decrease with the distance from the TC’s eye increasing, and their average decline rate were 0.29 g·kg-1·(100km)-1 and 0.26 hPa·(100km)-1, respectively, whereas atmospheric pressure exhibited an increment rate of 1.39 hPa·(100km)-1. This study confirms the effectiveness of RO and altimetry satellite data in monitoring atmospheric parameters and CWV, and could contribute to the understanding of atmospheric conditions during TCs.
Session Chair(s): Sridhara NAYAK, Japan Meteorological Corporation
AS11-A001
Tropical Cyclone Response to Recent Warming in Arabian Sea
Sidha Sankalpa MOHARANA#+, Debadatta SWAIN
Indian Institute of Technology Bhubaneswar
Tropical cyclones (TCs) are extreme weather events associated with severe winds and torrential rains in the coastal regions. They are synoptic-scale low-pressure systems fueled by the latent heat arising from warm ocean waters. Hence, an enhanced TC activity is being observed over all the basins under the influence of global warming. The enhancement is observed either in TC genesis or intensification tendencies. North Indian Ocean experiences the third highest number of TCs every year in the northern hemisphere, distributed over two basins, i.e., Bay of Bengal and Arabian Sea (AS). AS experiences much lesser number of TCs than the Bay. However, TCs in the AS are currently on an increasing trend. Concurrently, the basin has anomalously warmed during recent times too. The current study explores the impact of AS warming on TCs in the basin during the 1991-2020 period. Sea surface temperature (SST), 700m ocean heat content (OHC) and tropical cyclone heat potential (TCHP) have been analyzed to investigate the extent of warming in the basin during 1991-2020. Trends in SST, TCHP and OHC were calculated to be 0.1°C, 3 kJ/cm2, and 4×108 J/m2 per decade, respectively. A change-point analysis was carried out to identify significant changes in the timeseries of SST, TCHP and OHC, as well as the yearly counts of TCs in the basin. The analysis resulted in a coinciding change-point of SST and TCHP in 1998, and that of OHC in 2011. Interestingly, two change-points were identified in the timeseries of TC counts, in 1998 and 2011. The inferences were significant at 95% confidence level. The mechanism of interactions between AS warming and cyclogenesis is being investigated, which is expected to result in a better understanding of the coupling between the atmosphere and the ocean in the current climate change scenario.
AS11-A019
Influence of COVID-19 Prevention and Control Measures on Source-specific Health Risk of PM2.5-bound Metals in Shenzhen
Runhua WANG1#+, Xing PENG2, Xiaofeng HUANG1, Lingyan HE1
1Peking University, 2Peking University Shenzhen Graduate School
The COVID-19 lockdown was a typical occurrence of extreme emission reduction, which presented an opportunity to study the influence of control measures on the health risk of PM2.5. Observations were conducted from 2018-2021 using offline sampling instruments to investigate the concentration of PM2.5 and 21 associated metals before (January, 2018- December, 2019) and during (January, 2020- December, 2021) the COVID-19 lockdown in Shenzhen. Source apportionment of PM2.5-bound metals were conducted, and health risks of individual metals and different sources were assessed. The results showed that the atmospheric PM2.5 concentration decreased by 24% during the control period compared with that before the control in Shenzhen. The main sources of PM2.5-bound metals identified by the positive matrix factorization (PMF) model were vehicle sources, industrial sources, ship sources and dust sources. The emissions from vehicle sources, industrial sources, and ship sources decreased significantly, while dust sources increased during the control period. Combining methods for source apportionment and health risk assessment, we found that the total carcinogenic risk (CR) of five hazardous metals (Cd, Cr, Ni, Co, and Pb) showed a clear decreasing trend. However, the total CR (1.5 × 10−6) in 2021 still exceeded the widely acceptable risk level (i.e., 1×10-6), with the primary contributor of industrial emissions (59%). This study suggested that attentions should be paid not only on PM2.5 mass but also PM2.5-bound compounds especially heavy metals and metalloids to reduce health risks in the future. In summary, the impact of reduced emissions from the epidemic on health risks is relatively small, not as significant as the concentration of particulate matter. Vehicle and industrial sources should be continuously controlled, and regional combined prevention and control should be strengthened in the future in Shenzhen.
AS11-A038
Comparisons of Upper Wind Speed and Cloud Altitude Estimated Using Microcontroller-based Cloud Image Velocimetry
Shogo TOSHIMA+, Makoto NAKAYOSHI#
Tokyo University of Science
Wind speed in the upper atmosphere is crucial for comprehending the mechanisms of meteorological phenomena and improving the accuracy of weather forecasts. The traditional methods, such as Doppler lidar, radiosondes, and tracking the movement of cloud or water vapor patterns with satellite images, have limitations in evaluating atmospheric motion. To address this, we are developing a new method called Cloud Image Velocimetry (hereinafter referred to as CIV). CIV utilizes multiple cameras deployed on the ground, capturing sequential cloud images at certain time interval. Subsequently, we reconstruct 3D cloud coordinates using stereo vision theory and calculate the advection speed of clouds based on the temporal changes in these coordinates. In this research, we focused on improving the accuracy of time synchronization in CIV. Standard commercial cameras, used in previous studies, have inaccurate real-time clocks, leading to difficulties in achieving precise synchronization between the cameras. When multiple cameras are out of sync, the accurate wind velocity cannot be obtained. To address this, we developed a dedicated CIV camera system using the Spresense microcontroller board developed by SONY. The Spresense is equipped with an onboard GPS module, enabling reliable time synchronization between the cameras. Additionally, we enhanced the camera system by replacing the lens with a wide-angle variant and modifying the image sensor to cover a broader observational area. We compared the difference in the number of wind speed calculations between the newly constructed camera and previously used time-lapse cameras. The newly constructed camera exhibited an increase in the number of wind speed calculations by CIV, confirming the camera upgrade. Furthermore, we compared the altitude of clouds base estimated with CIV and a ceilometer. We will present these details at the 2024 AOGS.
AS11-A059
Characteristics of the Summer Western North Pacific High from Satellite Data
Jieun WIE1#+, Jae-Young BYON2, Byung-Kwon MOON1
1Jeonbuk National University, 2Korea Meteorological Administration
The East Asian Summer Monsoon is intricately linked to the behavior of the Western North Pacific High, yet understanding its activation has been a challenge. This study aimed to analyze the characteristics of the summer Western North Pacific High through the utilization of satellite data. The investigation spanned the summer seasons from 2020 to 2023, corresponding to the available satellite data. Initially, the data across this period were transformed into daily averages to compute anomalies. The primary mode delineates the unimodal patterns and intensity fluctuations of the Western North Pacific High, which are linked with the East Asian Summer Monsoon and associated with the Bonin High. The second mode illustrates the northward shift of rain bands concurrent with the development of the Western Pacific Subtropical High. The third mode captures variations in high-pressure systems due to the propagation of a wave-train originating from the North Atlantic. Notably, the first mode derived from GK-2A data did not align with the results from ERA5 and NCEP2 datasets. This study posits the potential utility of GK-2A data in diagnosing changes in the East Asian Summer Monsoon and Western North Pacific High. Acknowledgement: This research was supported by “The Technical Development on Weather Forecast Support and Convergence Service using Meteorological Satellites” of the NMSC/KMA (KMA2020-00121) and the National Research Foundation of Korea (NRF) grant funded by the Government of Korea (MSIT) (No. 2022R1A2C 1008858).
AS11-A062
Different ENSO Teleconnections Over East Asia in Early and Late Winter: Role of Precipitation Anomalies in the Tropical Indian Ocean and Far Western Pacific
Tianjiao MA1+, Wen CHEN1#, Shangfeng CHEN2, Chaim GARFINKEL3, Shuoyi DING4, Lei SONG2, Zhibo LI5, Yulian TANG2, Jingliang HUANGFU2, Hainan GONG2
1Yunnan University, 2Chinese Academy of Sciences, 3Hebrew University of Jerusalem, 4Fudan University, 5Peking University
This study aims to better understand the ENSO impacts on climate anomalies over East Asia in early winter (November–December) and late winter (January–February). In particular, the possible mechanisms during early winter are investigated. The results show that ENSO is associated with a Rossby wave train emanating from the tropical Indian Ocean toward East Asia (denoted as tIO-EA) in early winter. This tIO–EA wave train in El Niño (La Niña) is closely related to a weakening (strengthening) of the East Asian trough, and thereby a weakened (strengthened) East Asian winter monsoon and warm (cold) temperature anomalies over northeastern China and Japan. By using partial regression analysis and numerical experiments, we identify that the formation of tIO–EA wave train is related to precipitation anomaly in the tropical eastern Indian Ocean/ western Pacific (denoted as eIO/wP). In addition, the ENSO-induced North Atlantic anomalies may also contribute to formation of the tIO-EA wave train in conjunction with the eIO/wP precipitation. The response of eIO/wP precipitation to ENSO is stronger in early winter than in late winter. This can be attributed to the stronger anomalous Walker circulation over the Indian Ocean, which in turn is caused by higher climatological SST and stronger mean precipitation state in the Indian Ocean during early winter.
Session Chair(s): Shupeng ZHU, Zhejiang University
AS01-A003
| Invited
The Complexation of Atmospheric Brown Carbon Surrogates on the Generation of Hydroxyl Radical from Transition Metals in Simulated Lung Fluid
Yan LYU1,2#+, Haonan WU1, Xiaobing PANG1, Jiade WANG1, Meirong ZHAO1, Jinyuan CHEN1, Kai QIN2
1Zhejiang University of Technology, 2China University of Mining and Technology
Atmospheric particulate matter (PM) poses great adverse effects through the production of reactive oxygen species (ROS). Various components in PM are acknowledged to induce ROS formation, while the interactions among chemicals remain to be elucidated. Here, we systematically investigate the influence of Brown carbon (BrC) surrogates (e.g., imidazoles, nitrocatechols and humic acid) on hydroxyl radical (•OH) generation from transition metals (TMs) in simulated lung fluid. Present results show that BrC has an antagonism (interaction factor: 20–90 %) with Cu2+ in •OH generation upon the interaction with glutathione, in which the concentrations of BrC and TMs influence the extent of antagonism. Rapid •OH generation in glutathione is observed for Fe2+, while •OH formation is very little for Fe3+. The compositions of antioxidants (e.g., glutathione, ascorbate, urate), resembling the upper and lower respiratory tract, respond differently to BrC and TMs (Cu2+, Fe2+ and Fe3+) in •OH generation and the degree of antagonism. The complexation equilibrium constants and site numbers between Cu2+ and humic acid were further analyzed using fluorescence quenching experiments. Possible complexation products among TMs, 4-nitrocatechol and glutathione were also identified using quadropule-time-of-flight mass spectrometry. The results suggest atmospheric BrC widely participate in complexation with TMs which influence •OH formation in the human lung fluid, and complexation should be considered in evaluating ROS formation mediated by ambient PM.
AS01-A004
| Invited
Environmental Persistent Free Radicals in Atmospheric Particles
Huibin GUO#+
Xiamen University of Technology
Air pollution is one of the most common global environmental issues. Environmental persistent free radicals (EPFRs), as a new type of pollutant that has received much attention in recent years, are widely present in atmospheric particles and may increase human health risks. Compared to traditional PM2.5 and PM10, there is less research on EPFRs. However, the EPFRs in atmospheric particles have universality and complexity, and their impact on atmospheric particulate pollutants may be very serious. Therefore, this paper investigates the pollution characteristics and generation mechanism of EPFRs in atmospheric particles with different particle size distributions, providing new data and ideas for analyzing atmospheric pollution. The study found that the concentration of EPFRs in atmospheric particles ranged from 1.60 × 1013 spins/m3 to 24.48 × 1013 spins/m3, and the EPFRs concentration were lower in PM2.1-10 than in PM<2.1. The results present that g factor range observed in the spectra was 2.0031-2.0038. These EPFRs are considered to correspond to the g-factors of carbon-centred radicals with adjacent oxygen atoms. The concentration of EPFRs was positively correlated with the concentrations of Cu, Fe, Mn, Pb and V through ICP-MS metal analysis experiments, meaning that the presence of metals promoted the formation of EPFRs. This study also discuss reactive oxygen species (ROS), mainly ·OH radicals, which were formed by redox cycle of the EPFRs. This study quantified the health effects of EPFRs in the ET, TB, and P regions of the human lungs. Using cigarettes as a reference, the EPFRs deposition observed in the respiratory system under the same conditions was equal to smoking 29 cigarettes (extrathoracic: 13, tracheobronchial: 8, pulmonary: 8) per person per day. EPFRs with PM<2.1 are more likely to deposit in the alveolar region.
AS01-A020
Unexpected Deterioration of O3 Pollution in the South Coast Air Basin of California: The Role of Meteorology and Emissions
Shupeng ZHU1#+, Kai WU2, Mac Kinnon MICHAEL2, Scott SAMUELSEN2
1Zhejiang University, 2University of California, Irvine
Tropospheric ozone (O3) pollution has long been a prominent environmental threat due to its adverse impacts on vulnerable populations and ecosystems. In recent years, an unexpected increase in O3 levels over the South Coast Air Basin (SoCAB) of California has been observed despite reduced precursor emissions and the driving factors behind this abnormal condition remain unclear. In this work, we combine ambient measurements, satellite data, and air quality modeling to investigate O3 and precursor emission trends and explore the impacts of meteorological variability and emission changes on O3 over the SoCAB from 2012 to 2020. Changes in O3 trends are characterized by declining O3 in 2012-2015, and increasing O3 afterwards with the most extreme O3 exceedances in 2020. Basin-wide increases of MDA8 O3 concentrations over warm season are depicted between 2012 and 2020, with the most significant enhancements (5-10 ppb) observed in San Bernardino County. Persistent heatwaves and weak ventilation on consecutive days are closely correlated with O3 exceedances (r2 above 0.6) over inland SoCAB. While decreasing trends in NOx (-4.1%/yr) and VOC emissions (-1.8%/yr) inferred from emission inventory and satellites during 2012-2020 result in a slow transition for O3 sensitivity from VOCs-limited to NOx-limited, model simulations performed with fixed meteorology indicate that unfavorable meteorological conditions could largely offset regulation benefits, with meteorology anomaly-induced monthly O3 changes reaching 20 ppb (May 2020) and the deterioration of O3 pollution in 2016, 2017, and 2020 is largely attributed to unfavorable meteorological conditions. Nevertheless, anthropogenic emission changes may act as the dominant factor in governing O3 variations across the SoCAB when net effects of meteorology are neutral (typically 2018). This work provides a comprehensive assessment of O3 pollution and contributes valuable insights into understanding the long-term changes of O3 and precursors in guiding future regulation efforts in the SoCAB.
AS01-A016
High-level HONO Exacerbates Double High Pollution of O3 and PM2.5 in China
Chao LIU+, Bingqing LU, Yongyan JI, Xiang LI#
Fudan University
Double high pollution (DHP) of ozone (O3) and fine particulate matter (PM2.5) has been frequently observed in China in recent years. Numerous studies have speculated that DHP was related to nitrous acid (HONO), but the chemical mechanism involved remains unclear. The field observation results of DHP in Shanghai reveal that the high concentration of HONO produced by the nitrogen dioxide (NO2) heterogeneous reactions under high temperature and high humidity conditions promotes the increase of PM2.5 and O3 concentrations. The box model combined with field observations to reconstruct pollution events shows that HONO photolysis produces abundant hydroxyl (OH) radicals that rapidly oxidize volatile organic compounds (VOCs), which accelerates the ROx (OH, hydroperoxyl (HO2), and organic peroxy (RO2) radicals) cycle and results in the accumulation of O3. The elevated O3 accompanied by high concentrations of HONO produces particulate nitrate (pNO3) by promoting the NO2 + OH reaction. This process strengthens the chemical coupling between O3 and PM2.5, which can exacerbate the DHP of O3 and PM2.5. The sensitivity analysis of pNO3/O3-NOx-VOCs found that under nitrogen oxides (NOx = NO + NO2) reduction, the coordinated control of pNO3 and O3 should be achieved through positive emission reduction of alkanes and oxygenated VOCs (OVOCs). Therefore, the research will help design reasonable PM2.5 and O3 control strategies under high HONO concentration, and alleviate the current pressure on air pollution.
AS01-A013
Influence of the Large Topography of the Tibetan Plateau on the Downstream Transport of Ozone
Yancheng ZHU+, Chenyu XIAO, Rongxiang TIAN#, Zhan JIN
Zhejiang University
Ozone pollution poses a significant threat to human health. This study, using ERA5 reanalyzed ozone data from 1979-2021, investigates the high ozone concentrations in the Sichuan Basin, downstream of the Tibetan Plateau's large topography, compared to surrounding areas. Statistical and diagnostic analyses were conducted to explore the spatiotemporal distribution of ozone in the Sichuan Basin and its impact on high ozone value areas (HOVAs) in the downstream region. The results show that: 1. Ozone distribution shows seasonality, with higher concentrations in the lower and middle troposphere during spring and lower in winter, while the upper layer peaks in winter and spring and dips in summer; 2. HOVAs are consistently present in the lower troposphere of the basin throughout the year, more pronounced in summer, and in the middle layer on the southeastern side in winter; 3. Horizontally, ozone converges towards the basin but flows out at 600hPa, especially in winter, while vertically, it accumulates around 600hPa in winter and transports upward in summer; 4. From 1979 to 2021, ozone levels in both HOVAs of the basin have generally increased, with the fastest rise on the southern side. This study's findings are crucial for addressing ozone pollution in the downstream area of the Tibetan Plateau.
AS01-A017
Research on the Mechanism of Surface Ozone Increase Inducing Nitrate Pollution in Typical Cities in the Yangtze River Delta
Yongyan JI+, Zekun ZHANG, Bingqing LU, Xiang LI#
Fudan University
With China's rapid economic growth, issues of atmospheric ozone (O3) and particulate nitrate (NO3−) pollution are increasingly prominent. Their formation processes exhibit complex coupling with atmospheric nitrogen oxides (NOx) and volatile organic compounds (VOCs). Despite sustained NOx reduction in the Yangtze River Delta (YRD), O3 and NO3− concentrations are slowly increasing, presenting new challenges for pollution control. Observations during the Shanghai COVID-19 lockdown revealed that, as NOx decreased, O3 from VOC photochemical reactions increased. The accelerated cycling of OH-HO2-RO2 free radicals promoted O3 generation, outweighing the reduction from VOCs. This explains the increase in O3 despite stable VOC emissions from 2014 to 2020 while NOx decreased. Simulations suggest aggressive VOC reduction (especially alkenes and aromatics) under NOx reduction will curb surface O3. OH-HO2-RO2 free radicals play a crucial role. In eastern China, winter NO3− concentrations in recent years have risen annually, becoming a major PM2.5 component. Driving factors for NO3− increase are unclear, hindering policy formulation. Simulations using 2019 Shanghai winter data indicate that promoting NOx gas-phase and heterogeneous conversion accelerates winter O3 growth, explaining synchronous O3 and NO3− increase. NOx and VOC co-control simulations suggest O3-targeted strategies effectively alleviate YRD winter NO3− pollution, with OH-HO2-RO2 free radicals influencing NO3− formation. Observations during the COVID-19 lockdown and modeling reveal key factors driving O3 and NO3− growth, offering valuable insights for regional pollution control. The study underscores the crucial role of OH-HO2-RO2 free radicals in atmospheric chemistry.
Session Chair(s): Hirokazu ENDO, Meteorological Research Institute, Song YANG, Sun Yat-sen University
AS04-A069
Recent Advances in Understanding Multi-scale Climate Variability of the East Asian Summer Monsoon
Wen CHEN#+
Yunnan University
Studies of the multi-scale climate variability of the Asian monsoon are essential to an advanced understanding of the physical processes of the global climate system. In this talk, the progress achieved in the East Asian summer monsoon (EASM) is reviewed, with a focus on the past several years. The achievements are summarized into the following two topics: (1) the onset and withdrawal of the South China Sea summer monsoon (SCSSM); (2) the climate variations over the EASM transitional zone. The northernmost position of the EASM exhibits significant spatial fluctuations from year to year, thus forming a southwest–northeast-oriented belt between the arid and humid climate zone—the monsoon transitional zone (MTZ). Specifically, new results are highlighted, including the linkage between ENSO and the SCSSM onset has become much weaker and insignificant in recent years; the interannual variability of summer MTZ precipitation is under the combined impacts of oceanic forcings and internal atmospheric teleconnection patterns at mid-high latitudes; and an interdecadal decrease in summer precipitation amount in the MTZ was observed in the late 1990s due to a Silk-Road pattern-like wave train triggered by the combined impacts of the Atlantic Multidecadal Oscillation-like SST warming over the North Atlantic and positive-to-negative phase shift of the Pacific Decadal Oscillation (PDO). Finally, some further discussion on future research directions regarding our understanding of the EASM variability will be given.
AS04-A073
Exploring the Role of the Tibetan Plateau Lakes for Weather Patterns: Initial Research and Observational Evidence
Weiqiang MA#+, Yaoming MA, Weiyao MA
Chinese Academy of Sciences
The Tibetan Plateau, known as the “Roof of the World,” hosts numerous lakes that play a pivotal role in triggering and modulating regional and even global weather patterns. This study focuses on the observational evidence of these lakes on the Tibetan Plateau acting as catalysts for weather phenomena. Lake observations are selected based on typical lakes with a hundred-kilometer scale under the synergistic effect of westerlies and monsoons. Such as Bamu Co, Laang Co and Longmu Co. Extensive field measurements and remote sensing data have been analyzed to unravel the complex interactions between the lakes on the Tibetan Plateau and the surrounding atmosphere. The findings reveal that these lakes, through processes such as lake-effect precipitation, thermal regulation, and evaporation, significantly influence the formation and evolution of weather systems in the region. The lake-effect precipitation, for instance, has been observed to generate localized heavy rainfall and snowfall events downwind of the lakes. The thermal regulation effect of the lakes mitigates extreme temperature variations, while the evaporation from the lakes contributes to the water vapor supply in the atmosphere, thereby affecting cloud formation and precipitation. Furthermore, the study highlights the potential impact of changing lake dynamics, such as fluctuations in lake levels and temperatures, on the regional climate. These observations underscore the importance of incorporating the influences of Tibetan Plateau lakes into weather forecasting and climate modeling. In conclusion, this research provides substantial observational evidence that the lakes on the Tibetan Plateau act as crucial triggers for weather patterns, offering valuable insights for understanding and predicting the complex and dynamic meteorological processes in the region and beyond.
AS04-A014
Increased Population Exposure to Heat and Wet Extremes Moving from Chinese to Global 1.5 or 2.0 °C Warming
Peihua QIN#+
Chinese Academy of Sciences
The Paris Agreement proposed two global warming levels relative to the preindustrial period, with the ideal objective of 1.5 °C warming and an upper boundary of 2.0 °C. However, the years when the temperature will first reach 1.5 or 2.0 °C vary in different regions. Therefore, climate extremes and their population exposure are still not clear at regional or global warming levels. This study investigated climate extremes in China at different Chinese and global warming with 16 CMIP6 models under the middle SSP245 scenario. In China, the year when 1.5 °C warming is projected to occur is 2020 and 2035 for 2.0 °C warming. These values are more than 10 years earlier than the corresponding global warming levels of 2030 and 2049. Population exposure to percentile-based heat extremes at global 1.5 °C warming is projected to greatly increase relative to those when 1.5 °C warming occurs in China due to increases in climate extremes, and exposure to absolute heat extreme indices is projected to decrease from Chinese to global 2.0 °C warming under the joint impacts of increases in extremes and population decreases. Furthermore, from Chinese to global 1.5 °C warming, about 344 million people will experience increased exposure to heat, wet and dry extremes, and around 468 and 371 million people will be affected by increased exposure to heat–wet and heat–dry extremes, respectively. Thus, a more adaptive strategy should be proposed to cope with the future possible natural hazards caused by heat–wet and heat–dry extremes.
AS04-A032
Negative Circumglobal Teleconnection Enhances East China Precipitation Related to Quasi-biweekly East Asia-Pacific Teleconnection
Jing CHEN#+, Zhiping WEN, Xiaodan CHEN
Fudan University
The East-Asia Pacific (EAP) teleconnection is the most prominent pattern of East Asian summer monsoon. Its seesaw-like anomaly centers between Philippines and East Japan closely related to the weather and climate over East China, and are considered to be an important source of East China precipitation forecasts (or even extreme events). This study investigates the East China precipitation anomaly related to quasi-biweekly (QBW) EAP teleconnections and its modulation by the upstream circumglobal teleconnection (CGT) from Eurasia on the intraseasonal timescale. The results show that, during the evolution of the QBW EAP events, the precipitation anomalies over East China are characterized by a southeast-northwest oscillation. Remarkably, when the wet (negative) phase of QBW EAP is preceded by negative CGT, the QBW EAP-related precipitation exhibits enhanced, extended, and prolonged precipitation anomalies and an increased likelihood of extreme precipitation events over East China, although positive CGT typically precedes wet-phase QBW EAP. The cause of such enhanced precipitation is analyzed through moist static energy (MSE) diagnosis. The preceding negative CGT constitutes a low-pressure structure through the entire troposphere over East China and then trigger a rapid recharge (accumulation) of MSE by constraining low-level convection; Once the intense rainfall outbreaks, the pronounced warm advection related to the decaying negative CGT maintains the MSE recharge, prolonging and extending the precipitation anomalies. Our findings show that the configuration of wet-phase QBW EAP and negative CGT in advance is a significant indicator of heavy precipitation over East China and may have important implications for extended-range weather forecasting.
AS04-A033
The Interannual Variation of the Quasi-biweekly East Asian-Pacific Teleconnection in Boreal Summer
Yifeng HUANG+, Zhiping WEN#, Xiaodan CHEN
Fudan University
Based on observations and reanalysis datasets, this paper investigates the interannual variation of the quasi-biweekly East Asian-Pacific teleconnection(QBW-EAP) during the boreal summer between 1979 and 2020. It is found that there are stronger opposite centers with Rossby wave activity located at the northeast of the Philippines and the east of Japan in strong years, whereas the dipole in the weak years is relatively weaker. As the key factor triggering QBW-EAP, the quasi-biweekly convective activities over the tropical western Pacific also shows distinct variations. Stronger quasi-biweekly convection spreads northwestward from the western equatorial Pacific, while weaker quasi-biweekly convection in weak years propagates westward from the western North Pacific(WNP). The difference of quasi-biweekly convective activities associated with QBW-EAP are modified by the sea surface temperate(SST) in the tropical Pacific. During the summer of strong(weak) years, the negative(positive) SST anomalies in preceding winter in the equatorial central-eastern Pacific have transformed to positive(negative), and negative(positive) SST anomalies appear around the WNP, leading to favorable(unfavorable) dynamical conditions including low-level cyclonic(anticyclonic) circulation, ascending(descending) motion, and easterly(westerly) vertical shear in the WNP, thus regulating quasi-biweekly convective activities over the WNP. Correspondingly, the QBW-EAP also shows an interannual variation in intensity. This study implies that the preceding SST in the tropical Pacific is an effective predictor for summer QBW-EAP.
AS04-A041
The Physically Based Seasonal Predictions of Month-by-month Major Modes of the East Asia Summer Monsoon
Ying YANG#+, Zhiwei ZHU
Nanjing University of Information Science & Technology
East Asia summer monsoon (EASM) has distinct month-by-month variations during boreal summer, characterized by northward propagating rainband from south China to Yangtze River basin and eastward propagating western North Pacific anticyclone (WNPAC). Insignificant correlation coefficients occur between the EASM major mode in July (AC_7) and that in June (AC_6) and August (AC_8). Different precursors contribute to the month-by-month distinct EASM variations in summer. EASM major mode in June (AC_6) is related to April-May mean north Atlantic warming (NAW) and cooling tendency of sea surface temperature over western Pacific from February to April. NAW enhances/suppresses convection over Indian Ocean/tropical Pacific, both favoring AC_6 based on Gill model response, while the cooling tendency indicates the slow decay of El Niño (ESD) and enhances AC_6 through the “Indian ocean capacitor effect”. For AC_7, the cooling tendency of SST over tropical Pacific from April to June, representing the fast decay of El Niño (EFD), results in local negative precipitation in July, which modulates AC_7 through the wind-evaporation-sea surface temperature (WES) feedback. The precursors of AC_8 include the June-July mean Atlantic warming (TAW) and the slowly melting of sea ice concentration over Bering Strait (BSSM) from April to May. The mechanism of TAW influencing AC_8 is similar to that of NAW on AC_6. BSSM increases the temperature gradient over tropic and polar, leading to the enhancement of the westerly jet and maintenance of anticyclone over western Pacific, of which the east northerly enlarges AC_8 through the WES feedback. Based on above-mentioned predictors, the month-by-month physics-based empirical (P-E) models of EASM are established and show impressive skills both in the training period and independent forecast compared with results of 0-month lead dynamical model. In summer mean predictions, with initial conditions of May, the P-E models still outperform dynamical models.
AS04-A042
Understanding the Microphysical Characteristics of Extreme Weather Events Using Polarimetric Radar: A Case in Seoul, Korea on August 8, 2022
Hee-Ae KIM1+, Chang-Hoi HO2#, Junho HO3, Guifu ZHANG3, Kyung-Ja HA4, Eun-Kyoung SEO5
1Seoul National University, 2Ewha Womans University, 3The University of Oklahoma, 4Pusan National University, 5Kongju National University
On August 8, 2022, an unprecedented amount of heavy rainfall and lightning occurred in the Seoul metropolitan area, Korea, caused by a stationary frontal system. This extreme weather event was driven by small-scale forcing, highlighting the need for accurate simulation and prediction through observational studies. In the present study, the microphysical characteristics over the heavy rain and lightning areas were investigated using polarimetric radar observations. The focus was on analyzing the differences in radar signatures as a function of lightning activity and rain rate. Lightning activity was closely related to the presence of graupel and ice crystals, especially at altitudes above –10°C, where the presence of graupel is one of the main precursors of lightning. This was indicated by high radar reflectivity > 40 dBZ at altitudes and low differential reflectivity ≤ 0 dB above the melting layer. The radar variables also varied with the rain rate. As the rain rate increased, both the maximum radar reflectivity and the 15 dBZ echo height also increased. Analysis of the radar-based drop size distribution variables indicates the presence of larger and more concentrated raindrops during heavy rainfall. In particular, the proportion of larger particles > 3 mm increased significantly in areas where the rain rate exceeded 60 mm hr–1. This study enhances our understanding of the microphysical processes that occur during heavy rain and lightning events, and highlights the importance of polarimetric radar data in forecasting extreme weather conditions.
AS04-A048
The Intraseasonal Fluctuation of Indian Summer Monsoon Rainfall and Its Relation with Monsoon Intraseasonal Oscillation (MISO) and Madden Julian Oscillation (MJO)
Avijit DEY1#+, Rajib CHATTOPADHYAY1, Susmitha JOSEPH1, Manpreet KAUR1, Raju MANDAL1, R. Phani Murali KRISHNA1, Ak SAHAI1, D. R. PATTANAIK2
1Indian Institute of Tropical Meteorology, 2India Meteorological Department
The intra-seasonal fluctuations of Indian summer monsoon rainfall (ISMR) are mainly controlled by northward propagating Monsoon Intra-seasonal Oscillation (MISO) and eastward propagating Madden Julian Oscillation (MJO). In the current study, we examine the relationship between the intra-seasonal fluctuations (active and break spells) of ISMR with the phase propagation and amplitude of MISO and MJO. We notice that active spells generally occur during MISO phase 2-5 (MJO phase 3-6), and break spells mainly occur during MISO phase 6-8 (MJO phase 6-8 and 1). The association of active/break spells with MISO phases is more prominent than with MJO phases. We show the phase composite of unfiltered and regression based reconstructed rainfall for eight MISO and MJO phases, and the same is consistent with the earlier findings. We notice that the reconstructed field shows a systematic and well-organized northward propagation compared to the unfiltered field. Phase composite also indicates that there is a lead-lag relationship between MISO and MJO phases. MISO phase composite shows more robust northward propagation than the MJO phase composite. MISO reconstructed rainfall explained more percentage variance than MJO reconstructed rainfall with reference to 20-90 days filtered rainfall. It is found that long active (> 7 days) predominantly occurs when either MISO or MJO, or both of them are active, and the associated signal is somewhere in between phase 2-5. A long break occurs when either one or both of them are feeble, or even though associated signals are strong, they are primarily located in phases 1, 6, 7 and 8.
AS04-A051
Distinct Pathways of Atlantic Niño’s Influence on Indian Summer Monsoon
Yaqi JIN1, Lei ZHANG2#+
1South China Sea Institute of Oceanology, 2Chinese Academy of Sciences
Variability of the Indian summer monsoon (ISM) profoundly affects the large population of South Asia, exerting substantial socioeconomic impacts. However, its prediction remains challenging, partly due to our incomplete understanding of its physical drivers. As the dominant interannual climate variability mode in the tropical Atlantic, Atlantic Niño can weaken the ISM through atmospheric teleconnection. Furthermore, a recent study has identified two types of Atlantic Niño with warming centered in the central and eastern basins, respectively. Combining observational analysis and numerical experiments, we investigate their distinct influences on the ISM. Results show that the eastern Atlantic Niño excites extratropical Rossby waves, causing a west–east rainfall dipole anomaly over North India. In contrast, the central Atlantic Niño primarily induces easterly wind anomalies over the tropical Indian Ocean, predominantly affecting India rainfall south of 25˚N. These distinct tropical and extra-tropical pathways suggest that it is imperative to differentiate between the two Atlantic Niño types to enhance the ISM prediction.
AS04-A096
Interdecadal Change of the Oceanic Drivers in Interannual Variation of Northern Hemisphere Land Monsoon Rainfall
Yeyan JIANG#+, Zhiwei ZHU, Juan LI
Nanjing University of Information Science & Technology
Understanding predictability sources of the interannual monsoon rainfall is of vital importance for disaster prevention and mitigation as well as sustainable economic development. In the present study, the oceanic drivers of the interannual monsoon variability are investigated. Using observations from 1971 to 2020, it is shown that the interannual variation of the Northern Hemisphere land monsoon rainfall (NHLMR) is significantly connected with (i) an east–west thermal contrast in the tropical Pacific (TP), (ii) a warm sea surface temperature (SST) in tropical Atlantic (TA) and (iii) a cold SST in tropical Indian ocean (TIO). However, the TIO forcing is highly coupled with TP index. The NHLMR-TP relationship remains stable and robust over the past five decades, while the NHLMR-TA relationship undergoes a rapid enhancement around 1990s. The decadal warming of TIO and TA, which are attributed to the phase transition of Atlantic Multidecadal Oscillation (AMO), could enhance the NHLMR-TA relationship by modulating the pan-tropical Walker circulation. The AMIP-type numerical experiments forced by observed monthly SST also validate the mechanism here.
Session Chair(s): Min-Hui LO, National Taiwan University
AS63-A010
| Invited
Would Wetting a Dry Inland Area Increase Total Precipitation?
Dongryeol RYU1#+, Zhiyuan YANG1, Min-Hui LO2, Sugata NARSEY3, Murray PEEL1, Kaighin MCCOLL4
1The University of Melbourne, 2National Taiwan University, 3Bureau of Meteorology, 4Harvard University
Previous modelling and observational studies have reported positive feedback of soil moisture to local-to-regional precipitation modulated by land-atmosphere interactions and resulting rainfall recycling. However, the impact of soil moisture on total precipitation over spatial and temporal scales that are relevant to practical hydroclimatic and socio-economic concerns needs to be further investigated. In this work, we examine the effect of soil moisture on total precipitation at seasonal and annual time scales via extreme experimental scenarios that assume a large inland lake established in the arid part of Australia. The Community Earth System Model (CESM) with numerical water tracer is used to investigate the complex land-atmosphere interactions triggered by the wetter land surface and to quantify the contribution of recycled soil moisture to total precipitation. The hypothetical lake size is increased from 8 times the size of existing Kati Thanda-Lake Eyre (9500 km2) in South Australia to that of the entire Lake Eyre Basin (>2,350,000 km2). Our experiment shows that, although the soil moisture recycling increases with the inland lake at all sizes, statistically significant increase in total precipitation is observed only when the lake is increased to cover the whole Lake Eyre Basin. Relatively small change in total precipitation is associated with the influence of modified surface energy budget on advective rainfall process via complex land-atmosphere interactions. This also implies subsequent increase or decrease of precipitation in remote regions depending on atmospheric circulation patterns. Results from this study suggest that the instant positive soil moisture-precipitation feedback can be completely offset by the changes in large-scale advective processes, thus more comprehensive analysis of soil moisture-precipitation feedback is required across time and space.
AS63-A015
Climatology of Surface Parameters for the City of Turin (Italy) Using UTOPIA Land Surface Model
Claudio CASSARDO1#+, Valentina ANDREOLI1, Davide BERTONI1, Seon Ki PARK2, Sujeong LIM2, Massimiliano MANFRIN1
1University of Turin, 2Ewha Womans University
While there are several series of daily observations of temperature, precipitation and few other parameters available in many locations in the world, sometimes lasting more than a century, there are much less series of other variables related to the surface atmospheric layer or underground soil, such as sensible and latent heat fluxes, soil heat flux, soil temperature and moisture in the root layer and below it. This work aims to propose a method to evaluate such parameters at a climatic time scale using a trusted land surface model, taking the variables from the outputs of the simulation and creating a database. In this work, the selected model is the UTOPIA (University of TOrino land surface Process Interaction model in Atmosphere). This technique can be applied in general to each site in which hourly observations of the seven parameters needed for the simulation are available (temperature, humidity, pressure, the two components of the horizontal wind velocity, precipitation and solar radiation or cloudiness). In a preliminary phase, the database will be created on the period 1992-2023, on which we have the availability of hourly measurements carried out at the Department of Physics of the Turin University. In a second phase, we plan to develop a methodology to derive hourly observations from the existing series of data gathered in the city of Turin, using peculiar methods to interpolate or extrapolate the missing observations of required inputs and to downscale hourly observations from daily observations. This methodology could be tested using the existing data in the recent climate period.
AS63-A006
Understanding the Biophysical Effects of Afforestation/deforestation Based on the Land Use Model Intercomparison Project
Jun GE1#+, Weidong GUO1, Xin HUANG1, Qi LIU1, Beilei ZAN2, Bo QIU1, Yipeng CAO1
1Nanjing University, 2Nanjing University of Information Science & Technology
Deforestation/afforestation can influence local and regional climate via changes in land surface properties (e.g., albedo and roughness) and land–atmosphere energy and water exchanges. This is mostly called the biophysical process or pathway through which deforestation/afforestation influences climate. Earth system models are powerful tools for resolving the biophysical effects of deforestation/afforestation on climate. The Land Use Model Intercomparison Project (LUMIP), as one of the CMIP6-endoresd MIPs, is designed to advance the understanding of the impacts of land use and land cover changes on climate. The LUMIP provides an unprecedented opportunity to address the challenging issues related to the biophysical effects of deforestation/afforestation. Using simulations from the LUMIP and other CMIP6 MIPS, we show that large-scale deforestation over the northern mid- and high-latitudes can enhance daily temperature variability, leading to more frequent sharp warming and cooling events. We also find that changes in atmospheric aerosol concentrations can modulate the local effect of afforestation on surface temperature. Furthermore, we evaluate the LUMIP models’ performance in simulating the biophysical effects of deforestation on temperature and precipitation and explore the mechanisms for the intermodel uncertainty. These results are expected to provide new insights into the biophysical effects of deforestation/afforestation.
AS63-A011
Impact of East Asian Forest Cover Change on Future Carbon Sequestration
Jin-Soo KIM1#+, Hyo-Jeong KIM2
1Korea Advanced Institute of Science and Technology, 2City University of Hong Kong
Most countries worldwide have declared carbon neutrality goals as net zero emissions to arrest global warming and relevant socio-economical losses. Carbon emissions should be reduced to balance natural carbon sequestration to achieve carbon neutrality. Nature-based climate solutions (NBCSs)—mostly carbon sequestration in the terrestrial ecosystem—largely mitigated fossil carbon dioxide emissions during the past decade. While forests in East Asia have an essential role in carbon sequestration, optimal forest management and restoration (FMR) practices to maximize carbon sequestration have not yet been investigated for East Asia. To find locations for optimal FMR practices, we analyzed an Earth system model results with and without land use land cover change (LULCC) scenarios under future greenhouse gas warming conditions. We found that less precipitation and sunshine in southern China due to increased aerosols lead to less carbon uptake by terrestrial ecosystems under the Shared Socioeconomic Pathways (SSP) 3-7.0 scenario. On the other hand, Korea and Japan generally lose carbon sequestration due to reduced tree cover, which has a more substantial impact than in other East Asian regions. However, some areas in China show increased carbon sequestration due to the afforestation, which might have maximized cost-effective FMR practices, especially in eastern Sichuan, Chongqing, and northern Guizhou. This finding can support appropriate FMR in East Asia with the optimized cost-to-benefit of NBCSs and planning actual practice for the carbon neutrality agenda.
AS63-A007
Improvements in the Land and Crop Modeling Over Flooded Rice Fields by Incorporating the Shallow Paddy Water
Xiaoyu XU1#+, Hiroyuki KUSAKA2, Atsushi MARUYAMA3
1Nanjing University of Aeronautics and Astronautics, 2University of Tsukuba, 3National Agriculture and Food Research Organization
Flooded rice paddies are important for modifying land surface energy and water budgets, especially in Asian countries. This study incorporated shallow paddy water into the Noah with Multi-Parameterization (Noah-MP) model to enhance its performance in capturing the distinct features of small Bowen ratios over flooded rice fields. The paddy surface water was parameterized as one integrated layer along with the top soil layer, and meteorological measurements from two crop sites in Japan, that is, SAITO (early rice) and SAGA (late rice), were employed for model evaluation at the field scale. The simulation results show that the model performance was significantly improved by combining the incorporation of paddy water and the calibration of rice crop parameters, particularly at SAGA. Compared with the reference run using the original version of Noah-MP for SAGA, the underestimation in latent heat and the overestimation in sensible heat during daytime were decreased by ∼74 Wm−2 (∼67%) and ∼92 Wm−2 (∼55%), respectively. Approximately 60%–70% of this improvement was contributed by using calibrated rice crop parameters, while the rest of 30%–40% was from further incorporating paddy water. The decreased ground surface resistance owing to the presence of paddy water was crucial for capturing the features of small Bowen ratios. The observed water depth might help mitigate the underestimation of latent heat nonlinearly. This work may benefit the study of land-atmosphere interactions and local and regional weather and climate in Asia with the widely used coupled Weather Research and Forecasting/Noah-MP model.
AS63-A018
Impact of Urban Growth and Global Warming on Heat Stress in Urban Agglomerations of Southeastern China
Han LIAO1,2+, Zixuan ZHOU1, Pak Him KAM1, Eun-Soon IM1#
1The Hong Kong University of Science and Technology, 2The Hong Kong University of Science and Technology
Southeastern China is a representative region with growing concern due to anthropogenic warming, particularly along the heavily populated eastern coast, characterized by rapid urban development. Previous studies have projected the severity of future heat stress in urban areas, but the majority of long-term climate projections assume static urban land-use properties. In this study, we aim to better represent the transient nature of urban growth by incorporating varying urban density and urban extent, which vary according to the SSP scenarios, into the non-hydrostatic RegCM4 whose performances are optimized over the target regions. While urban land areas continue to extend, it is projected that the trend of increasing urban population will decline in the second half of the 21st century. Consequently, urban density is expected to peak around 2040-2050 and gradually decrease until the end of the century, although this change pattern is not regionally uniform. Our analysis focuses on examining the relative contribution of temperature and humidity to human heat stress along the urban growth in the Yangtze River Delta and the Pearl River Delta, which are home to some of the largest urban agglomerations in China. [Acknowledgements]This research was supported by the Theme-based Research Scheme, T31-603/21-N, which was funded by the Research Grants Council (RGC) of Hong Kong.
Session Chair(s): Jingyu WANG, Nanyang Technological University, Yang GAO, Ocean University of China
AS38-A019
| Invited
Interactions Between Ozone Pollution and Climate Change in China
Hong LIAO#+, Yang YANG, Pinya WANG
Nanjing University of Information Science & Technology
China is suffering from serious ozone pollution issues. High concentrations of ozone not only threaten human health and crop yields, but also make an important contribution to global warming. Clarifying the characteristics of ozone variations and their effects on weather and climate is the scientific basis for the control of air pollution, climate change mitigation, and health effects assessment of ozone.
AS38-A017
Reducing Long-standing Ozone Overestimation Based on a High-resolution Earth System Model
Yang GAO#+, Wenbin KOU, Wenxuan CHENG, Xiuwen GUO, Shaoqing ZHANG
Ocean University of China
Ozone concentrations play vital roles in affecting human health, and reasonably simulating ozone concentration is key to assess its subsequent impact. However, most global models suffer biases of ozone overestimate. In this study, through optimizing an Earth system model at high-resolution of 25 km atmosphere, we achieve improved simulations of ozone concentrations. Specifically, we conduct simulations in summer during 2015-2019 at both high and low (100 km) grid spacings, showing an enhanced capability by substantially reducing traditionally ozone underestimates. The optimized high-resolution Earth system model is expected to be quite useful in better predicting future air quality under a warming climate.
AS38-A016
Interannual Variations in O3 Pollution with a Dipole Structure Over Eastern China Associated with Springtime Thermal Forcing Over the Tibetan Plateau
Qingjian YANG+, Tianliang ZHAO#
Nanjing University of Information Science & Technology
The Tibetan Plateau (TP) is essential in modulating climate change in downstream Eastern China (EC). As a meteorology-sensitive pollutant, changes in O3 in connection with the TP have received limited attention. In this study, using climate analysis of the CHAP O3 product and ERA5 reanalysis data of meteorology for 1980–2020, the effect of springtime TP thermal forcing on the warm season (April–September) O3 pollution over EC was investigated. The strong TP thermal effect significantly modulates the interannual variations in O3 pollution with a dipole pattern over EC, inducing more O3 pollution in northern EC regions and alleviating O3 pollution in the southern regions. In northern (southern) EC, strong TP thermal forcing triggers a significant anomalous high (low) pressure center accompanied by anticyclonic (cyclonic) anomalies, resulting in decreased (increased) total cloud cover, increased (reduced) surface downward solar radiation and air temperature, which are conducive to the anomalous increase (decrease) in surface O3 concentrations. Moreover, the key sources of springtime thermal forcing over the TP influence the major O3 pollution regions over southern and northern EC with a inverse pattern, depending on their locations and orientations to the large topography of the TP. This research reveals an important driving factor for the dipole interannual variation in O3 pollution over EC, providing a new prospect for the effect of the TP on atmospheric environmental change.
AS38-A012
| Invited
Investigating the Interaction Between Transboundary Haze and Planetary Boundary Layer in Singapore
Steve YIM#+, Tao HUANG, Tingting FANG, C.Y. LEONG, Lujia FENG
Nanyang Technological University
Transboundary air pollution is one of the critical environmental problems in Southeast Asia; nevertheless the interaction between transboundary haze and local planetary boundary layer (PBL) remains unclear due to lack of sufficient observations and sophisticated simulations. This study applied LiDAR observation and model simulation to comprehensively evaluate the interaction between transboundary haze and local PBL during a recent transboundary haze episode in Singapore in October 2023. Results show that upper-level southeasterly wind, especially the nocturnal low-level jet, created favorable conditions for aerosol transport when fire hotspot numbers increased in Indonesia. The rapid diurnal increase in PBL height facilitated the entrainment of upper-level haze into the PBL, interacting with ground-level aerosols through turbulent mixing. Model simulations further show the significant contributions of fire emissions to the transboundary haze episode in maritime Southeast Asia. The impacts extended towards the southern region of Peninsular Malaysia, driven by the persistent prevailing southeasterly winds.
AS38-A001
Anomalous Ozone Pollution in the Pearl River Delta, China in 2019: The Impact of El Niño-southern Oscillation
Run LIU1,2#+, Yanxing WU1
1Jinan University, 2Guangdong-Hongkong-Macau Joint Laboratory of Collaborative Innovation for Environmental Quality
Surface ozone (O3) pollution in the Pearl River Delta (PRD), especially persistent O3 pollution episodes lasting three days or longer (OPE3), showed an anomalous peak during the autumn of 2019 (bulge-2019). Our study indicates a strong correlation between the occurrence of OPE3 and low-cloud days, with low-cloud days explaining 55% of the interannual variability of OPE3 in the autumn of 2015-2021. Notably, as much as 74% of the bulge-2019 is related to low-cloud days. However, establishing a direct causal link remains challenging. In autumn 2019, an anomalous cyclone occurred in the western North Pacific, with anomalous northerly winds on its northwestern flank, leading to anomalous downdraft over South China. This pattern was characterized by stagnant, low relative humidity, intensified solar radiation, and low cloud cover conditions that were conducive to the photochemical formation and accumulation of O3. Further analysis of the relationship between low-cloud days and El Niño–Southern Oscillation shows that eastern Pacific El Niño events are associated with fewer low-cloud days in the PRD in autumn, whereas central Pacific (CP) El Niño events result in more low-cloud days. In 2019, with a background of CP El Niño, there was a possibility of an increased frequency of autumn low-cloud days, which might have partially raised the likelihood of the occurrence of bulge-2019.
AS38-A014
Global Warming Causes More Frequent Extreme Precipitation by High-resolution Simulations
Xiuwen GUO#+, Yang GAO
Ocean University of China
Extreme precipitation events have become increasingly frequent, resulting in significant human and economic losses. While global warming's impact on precipitation intensity is extensively studied, low-resolution climate models lack the capability to simulate extreme precipitation events, leading to limited confidence in future projections for disaster planning. Using a high-resolution Earth System Model, we find the extreme precipitation over the west coast of northern hemisphere has been substantially improved compared to low-resolution multi-model ensemble. Under a fossil fuel intensive scenario, these events are projected to occur more frequently with stronger intensity, emphasizing the crucial role of greenhouse gas mitigation in managing the risks associated with intensifying extreme precipitation.
Session Chair(s): Mansing WONG, The Hong Kong Polytechnic University, Kai QIN, China University of Mining and Technology, Jason COHEN, China University of Mining and Technology
AS89-A010
| Invited
Assessing Local and Transboundary Air Pollution and Sectoral Contributions in Southeast Asia
Steve YIM#+
Nanyang Technological University
Southeast Asia is categorized as a typical region with a complex mixture of pollutants from long-term human activities and short natural events such as biomass burning and volcanic eruptions. The consequential fine particulate matter (PM2.5) and ozone (O3) concentration exposure can induce severe health outcomes. Air pollution in this region is largely affected by local and transboundary air pollution. Despite the seriousness of air pollution in the two regions, the understanding about the contributions of local emission sources and transboundary air pollution to air quality remains unclear. This study apportions the contribution of sectoral emissions and transboundary air pollution to PM2.5 and O3 in the regions in different seasons and air pollution episodes. The resultant health impacts are also estimated.
AS89-A012
Cooperative Estimation of Satellite-based Multiple Air Pollutants Using a Knowledge-informed Deep Learning Model
Xinyu YU#+
The Hong Kong Polytechnic University
Air pollution is a persistent global issue that has significant impacts on human health and ecosystems worldwide, thus it is crucial to obtain accurate and reliable air pollutant concentration estimations. Satellite-based observations have tremendous potential for the retrieval of air pollutants, like fine particulate matter (PM2.5), ozone (O3) and nitrogen dioxide (NO2), while these air pollutants were commonly estimated separately in previous studies, resulting in the shared information between different air pollutants being ignored. In this study, we proposed a knowledge-informed deep learning model to realize cooperative estimations of multiple air pollutants with full coverage and 2-km resolution based on Himawari-8 data in the Guangdong-Hong Kong-Macao Greater Bay Area. Specifically, the multi-head attention mechanism was employed to extract the temporal variation patterns of PM2.5, O3 and NO2 on the basis of previous observations, which was then used as prior knowledge and incorporated with the deep forest model. Additionally, meteorological variables, geographical factors and socio-demographic data were also involved as auxiliary data to enhance the estimation accuracy. Cross-validation results based on the measurements from the ground-based air pollution monitoring stations show that the proposed cooperative estimation model can achieve comparable accuracy as compared to the independent estimation results (with an R2 of over 0.7), but in a more efficient way. In this study, we highlight a promising model for the cooperative estimation of multiple air pollutants, and it is of great potential to be applied in other regions.
AS89-A002
Retrieval Algorithm of Absorbing Aerosols Based on UV Radiance Spectrum in East China
Ding LI+, Kai QIN#
China University of Mining and Technology
Quantitative absorbing aerosols play a pivotal role in mitigating air pollution, enhancing trace gas assessment precision, and facilitating accurate calculations of solar radiation. Ultraviolet spectroscopy (UV) is highly sensitive to retrieving absorbing properties of aerosols than visible bands, hourly UV spectrum datasets from geostationary satellites such as GEMS provide great assistance for the dynamic change tracking of absorbing aerosols. This study focuses on refining the algorithm's accuracy in East China, where a complex atmospheric background poses unique challenges. The approach begins with a comprehensive analysis of the limitations and uncertainties inherent in prior knowledge based on long-term active/passive remote sensing observations from ground-based measurements and satellites. Then the integration of machine learning techniques and radiative transfer models builds a robust prior knowledge system and retrieval algorithm. The subsequent evaluation of results will be conducted under different aerosol mixing models for daily situations and occasional extreme pollution events. This study's evolution provides a theoretical foundation for generating high-precision remote sensing datasets at hourly intervals and kilometer-scale resolutions, and also serve as a robust framework supporting China's active engagement in international climate negotiations.
AS89-A004
Multi-band AOD Inversion of MODIS Based on Deep Learning
Yu SUN#+, Lin SUN
Shandong University of Science and Technology
Multi-band aerosol optical depth(AOD) inversion is important for determining the spatial distribution of aerosol types and the content of fine mode aerosols in the air. The multi-spectral satellite sensors such as MODIS with visible and near-infrared wavelength provide feasibility for the inversion of multi-band AOD. However, owing to the insufficient ability to mine useful information, current inversion methods suffer from the "ill-posed" problem, which limits the application of multi-band high-precision AOD. This study proposed a deep learning multi-band AOD inversion algorithm for MODIS supported by long time series AERONET site data, with four wavelength bands(870nm, 675nm, 500nm, and 440nm) AOD inverted. Independent experimental data were used to verify the results of the new model. The results showed that the inversion results of the four bands achieved a high accuracy, with R>0.90, RMSE<0.12, and EE>75%, and had high a stability in different regions.
AS89-A018
TROPOMI Data Analyzed Within a Mass Conservation Strategy Improves New Source Identification and Reduces Uncertainty of NOx Emissions Over China
Lingxiao LU+, Kai QIN, Jason COHEN#
China University of Mining and Technology
Current methods of extracting emissions from satellite profiles rely on a fixed combination of localized models. This work applies a model-free analytical approach to quantify evolving and emerging NOx emission sources with high spatial and daily temporal resolution, by assimilating tropospheric NO2 column data from TROPOMI in a mass-conserving manner. The results herein are presented over three rapidly changing regions in China. These regions are selected in a more comprehensive and uniform way, based on the observations and climate zones themselves, and do not follow arbitrary or political boundaries, including Wuhan city, Shandong and Anhui provinces which are rapidly urbanizing and not frequently addressed in the global literature. A few scientific points are explained in detail. First, the day-to-day and grid-by-grid emissions are found to be 1.96±0.27 µg/m2/s which is similar to MEIC 1.94 µg/m2/s on grids which are larger than 0.3 µg/m2/s, while the results are 1.22±0.63 µg/m2/s higher on grids which are below 0.3 µg/m2/s. Second, through source attribution based on combustion temperature thermodynamics, atmospheric transport, and in-situ chemistry, this work successfully distinguishes five distinct industrial source types. Third, emissions of industrial sources adjacent to the Yangtze River are found to be 160.5±68.9 Kton/yr, which is 163% higher than the a priori, consistent with missing light and medium industry located along the river. Fourth, this work demonstrates which land pixels have an uncertainty larger than or smaller than the day-to-day variability, providing quantitative information for placement of future monitoring stations. It is hoped that these findings will support popularization of this new approach to top-down emissions estimates, raise the importance of constraining emissions uncertainties, more precisely reflect anthropogenic changes, and constrain misidentified emissions.
Session Chair(s): Song GUO, Peking University
AS20-A024
| Invited
Establishing a Functionality-reactivity Relation for Secondary Organic Aerosol Formation from Aromatics
Renyi ZHANG#+, Yixin LI
Texas A&M University
Aromatic hydrocarbons (e.g., benzene, toluene, xylenes, trimethylbenzenes and polycyclic aromatic hydrocarbons) account for 20-30% of the total VOCs in the urban atmosphere and represent as major anthropogenic SOA precursor. Aromatic oxidation occurs via multiple pathways and steps to produce various condensable oxidize organics (COOs), which engage in gas-to-particle conversion to lead to SOA and brown carbon formation. The chemical complexity of VOC oxidation and its subsequent gas-to-particle conversion poses enormous challenges in investigating the SOA formation and properties. This presentation provides an overview of the latest progress in understanding the roles of aromatic oxidation in SOA formation, focusing on multi-generation production of various COO species and their roles in SOA formation. We elucidate the linkage between organic functionality and multiphase reactivity for COOs to provide the critical impetus in predicting COO production and SOA formation based on fundamental chemical mechanisms. Current challenges and future research direction are identified, highlighting the functionality-reactivity relation for explicit representation of SOA formation in predictive atmospheric models.
AS20-A003
| Invited
Research Progress of SOA Formation from Anthropogenic VOCs Under Complex Pollution Condition
Tianzeng CHEN+, Hong HE#
Chinese Academy of Sciences
Although the air quality in China has been greatly improved in recent years, the air pollution remains severe. The annual mean PM2.5 concentrations have not met the second grade of the National Ambient Air Quality Standards in China and are still much higher than the guideline value of the World Health Organization. Thus, the PM2.5 concentration needs to be further reduced. Secondary organic aerosol (SOA) is an important component of PM2.5 and has an important impact on air quality, global climate change, and human health. Therefore, understanding the formation mechanism of SOA is an important basis to control SOA and further reduce PM2.5. As an important precursor of SOA, volatile organic compounds (VOCs) can be oxidized by oxidants such as OH, NO3, Cl, and O3 to generate low volatile organic compounds and further to form SOA through gas-particle partitioning, homogeneous nucleation, aqueous phase reaction, and heterogeneous reaction processes. The formation of SOA can be affected by many factors. The observed SOA concentration is always underestimated by air quality models because a comprehensive understanding of the complexity of SOA chemical composition and formation mechanisms is still lacking, especially that under the highly complex air pollution conditions in China. Therefore, the formation mechanism and influencing factors of SOA under highly complex air pollution conditions have become an important concern in the field of atmospheric sciences. Recently, much laboratory work has focused on the formation of SOA under complex conditions. The research progress of SOA formation from different anthropogenic VOCs are reviewed here, and the methods used and the impact of different influencing factors on SOA formation are introduced. Finally, the key scientific issues that exist in the research of the SOA mechanism at present are put forward, and the future research direction is projected.
AS20-A032
Influence of Secondary Organic Components on the Hygroscopicity of Atmospheric New Particles
Chenxi LI#+, Jumabubi YISHAKE
Shanghai Jiao Tong University
The formation and growth of new particles are important sources of atmospheric particulate pollution and cloud condensation nuclei. Air humidity can influence the water content of new particles in the atmosphere and affect their growth rate. However, due to the high diffusivity of particles below 20 nm, they experience high transport losses in instruments, leading to a scarcity of field observation of their hygroscopicity in this size range. Additionally, limited laboratory investigations have mainly focused on measuring the hygroscopicity of single-component particles (such as (NH4)2SO4 and NaCl). This study generates internally mixed organic-inorganic particles similar in composition to atmospheric new particle and characterizes their hygroscopicity using a nano-differential mobility analyzer system (nano-HTDMA). We tested several combinations of inorganic and organic components: different inorganic components were generated with an electrospray particle generator ((NH4)2SO4), a tube furnace (NaCl) or through acid-base reactions (H2SO4+NH3), while the organic components were produced by oxidizing representative VOCs including -pinene and 1,3,5-trimethylbenzene by O3 or OH in a flow tube reactor. We characterized the hygroscopic growth of these mixed particles in the RH range of 20-90%. The presence of the organic components suppresses particle hygroscopic growth compared to pure inorganic particles. Additionally, the mixed particles show size dependent decrease of deliquescence relative humidity (DRH) compared to the pure inorganic particles. For instance, 9.6 nm particles composed of 50% NaCl and 50% alpha-pinene oxidation products has a DRH of 70%, in contrast to 80% of 9.6 nm NaCl particles. However, 18.6 nm mixed particles have a DRH of ~75%, compared to 79% of 18.6 NaCl particles. This lowering of DRH indicates that hygroscopicity growth of new particles needs to be considered during new particle formation events at moderately humid conditions.
AS20-A017
The Effects of Biogenic Precursors on the Secondary Organic Aerosol Formation from Typical Polycyclic Aromatic Hydrocarbons
Ying YU1+, Song GUO1#, Rui TAN1, Shenrong LOU2, Wenfei ZHU2
1Peking University, 2University of Shanghai for Science and Technology
The mixing of precursors has been demonstrated to alter the secondary organic aerosol (SOA) yield and composition. Here, we measure the SOA yield and composition from photo-oxidation of two polycyclic aromatic hydrocarbons (naphthalene, 2-methylnaphthalene), two terpenes (isoprene, alpha-pinene), and their binary mixtures, representative anthropogenic and biogenic precursors, under both low and high NOx condition in an environmental smog chamber. The SOA composition is measured by the Filter Inlet for Gases and Aerosols coupled to a high-resolution time-of-flight chemical ionization mass spectrometer (FIGAERO-CIMS). Our results show that the SOA yield of naphthalene and 2-methylnaphthalene under high NOx is lower than that under low NOx, consistent with previous studies. The suppression of SOA formation is observed in the mixture. This might be resulted from the difference of particle volatility between individual precursor system and mixed system, indicating different oxidation process between them. Our study provides new insights into SOA formation from mixed anthropogenic and biogenic precursor systems.
AS20-A014
Interaction Between Marine and Terrestrial Biogenic Volatile Organic Compounds: Non-linear Effect on Secondary Organic Aerosol Formation
Xiaowen CHEN+, Lin DU, Kun LI#
Shandong University
Biogenic volatile organic compounds (BVOCs) are the largest source of secondary organic aerosols (SOA) globally. However, the complex interactions between marine and terrestrial BVOCs remain unclear, inhibiting our in-depth understanding of the SOA formation in the coastal areas and its environmental impacts. Here, we performed smog chamber experiments with mixed α-pinene (a typical monoterpene) and dimethyl sulfide (DMS, a typical marine emission BVOC) to investigate their possible interactions and subsequent SOA formation. It is found that DMS has a non-linear effect on SOA generation: the mass concentration and yield of SOA show an increasing and then decreasing trend with the increase of the initial concentration of DMS. The increasing trend can be attributed to OH regeneration together with acid-catalyzed heterogeneous reactions by the oxidation of DMS, while the decreasing trend is explained by the high OH reactivity that inhibits the formation of low volatility products. The results from infrared spectra and mass spectra together reveal the contribution of sulfur-containing molecules in the mixed system. Moreover, the mass spectra results indicate that acidic products generated by DMS photooxidation enhance the O:C ratio, while organosulfates are produced to contribute to the formation of mixed SOA. In addition, the trends in relative abundance of highly oxygenated organic molecules (HOMs) with C8-C10 multiple functional groups in different mixed systems agree well with the turning point of the SOA yield. The findings of this study have significant implications for understanding binary or more complex systems in the atmosphere in the coastal areas.
AS20-A011
Sulfur Dioxide Enhances Aerosol Formation from Anthropogenic Volatile Organic Compound Ozonolysis by Producing Sulfur-containing Compounds
Zhaomin YANG+, Lin DU#
Shandong University
Sulfur dioxide (SO2) can affect aerosol formation in the atmosphere, but the underlying mechanisms remain unclear. Here, we investigate aerosol formation and composition from the ozonolysis of cyclooctene with and without SO2 addition in a smog chamber. Liquid chromatography equipped with high-resolution tandem mass spectrometry measurements indicates that monomer carboxylic acids and corresponding dimers with acid anhydride and aldol structures are important components in particles formed in the absence of SO2. A 9.4–12.6 times increase in particle maximum number concentration is observed in the presence of 14–192 ppb SO2. This increase is largely attributed to sulfuric acid (H2SO4) formation from the reactions of stabilized Criegee intermediates with SO2. In addition, a number of organosulfates (OSs) are detected in the presence of SO2, which are likely products formed from the heterogeneous reactions of oxygenated species with H2SO4. The molecular structures of OSs are also identified based on tandem mass spectrometry analysis. It should be noted that some of these OSs have been found in previous field studies but were classified as compounds from unknown sources or of unknown structures. The observed OSs are less volatile than their precursors and are therefore more effective contributors to particle formation and growth, partially leading to the increase in particle volume concentration under SO2-presence conditions. Our results provide an in-depth molecular-level insight into how SO2 alters particle formation and composition.
AS20-A007
Molecular Fingerprints and Health Risks of Smoke from Home-use Incense Burning
Kai SONG+, Song GUO#, Qiqi ZHOU, Zichao WAN, Kun HU
Peking University
The burning of incense for home use is a widespread practice that has been shown to have significant negative impacts on human health and air quality. However, there is a lack of understanding regarding its emission profiles and associated health risks. To address this knowledge gap, we utilized a state-of-the-art thermal-desorption comprehensive two-dimensional gas chromatography–mass spectrometer (TD-GC × GC-MS) to (semi-)quantify the emission factors (EFs) of 317 volatile compounds and thoroughly investigate the organic profiles of smoke from incense burning across a full-volatility range. Results showed that toluene (70.8±35.7 µg g−1) is the most abundant compound in smoke from incensing burning, followed by benzene, furfural, and phenol. Phenol, toluene, furfural, 2-furanmethanol, benzene, and benzyl alcohol are the main contributors to ozone and secondary organic aerosol (SOA) estimation. Intermediate volatility organic compounds (IVOCs) accounted for 19.2 % of the total EFs but 40.0 % of the estimated SOA. Additionally, a novel pixel-based method, combined with aroma analysis, revealed that furfural can act as a key tracer of incense burning and is responsible for the distinctive aroma of incense smoke. High-bioaccumulation-potential (BAP) assessment using pixel-based partition coefficient estimation revealed that acenaphthylene, dibenzofuran, and phthalate esters (PAEs) are chemicals of high-risk concern and warrant further control. Our results highlight the critical importance of investigating home-use incense burning and provide new insights into the health impacts of smoke from incense burning using novel approaches.
AS20-A029
Effect of Secondary Organic Aerosol Formation Pathways on Human Health
Lu QI1#+, KaYuan CHEUNG1, Yufang HAO1, Tianqu CUI1, Robin MODINI1, Imad HADDAD1, Andre PREVOT1, Andre PREVOT1, Jay SLOWIK1, Kun LI2, Jay SLOWIK1, Junji CAO3
1Paul Scherrer Institute, 2Shandong University, 3Chinese Academy of Sciences
Atmospheric aerosols are among the largest global environmental risks to public health and responsible for considerable uncertainty in the climate system. Much of this uncertainty is due to secondary organic aerosol (SOA), which consists of thousands of multifunctional, oxygenated species that are difficult to measure in situ. In consequence, source apportionment studies typically treat SOA as a single bulk quantity (or as a linear combination of non-source-specific vectors), and the effects of specific SOA sources and on human health and climate effect remain poorly constrained. Here we utilize extractive electrospray ionization coupled to time-of-flight and orbitrap mass spectrometers (EESI-TOF and EESI-Orbitrap) to elucidate wintertime SOA sources and formation pathways in Beijing, China. High-RH conditions with widespread cloud formation are typical of severe haze events in Beijing, yielding high aerosol liquid water content (LWC) and thereby favoring aqueous-phase reactions. We identify two factors related to aqueous SOA production, one of which (AqSOA) is characterized by small, highly oxygenated molecules and depends mainly on LWC. The second aqueous factor (AqSOA_AMN) is related to both LWC and NH3+/NH4+, and shows enhancements from N-containing molecules consistent with imidazoles, which are known to be formed from aqueous reactions of glyoxal in the presence of NH4+- containing seed. The AqSOA_AMN factor also exhibits far higher oxidative potential (OP) on a per mass basis than either AqSOA, or aged biomass burning. Further, during pollution events conducive to its formation, AqSOA_AMN has considerable effects on both the SOA-derived and total OP. This highlights the implications of different SOA pathways, including NH3/NH4+- mediated aqueous chemistry, for human health. More generally, we demonstrate that the SOA contributions to oxidation potential (OP) are both considerable and strongly source-dependent and highlight the shortcomings of treating SOA as a bulk or non-source-specific quantity.
Session Chair(s): Xiangrui KONG, University of Gothenburg
AS55-A020
Intense Chemical Reactivity on Aerosol Particle Surfaces
Xiangrui KONG#+
University of Gothenburg
Gas-particle interfaces are known for their chemical activity, particularly when they interact with reversibly adsorbed water, which exists in equilibrium with water vapor. This interaction is crucial as it can facilitate thermodynamic reactions that are typically unlikely, such as spontaneous reactions on salt surfaces when they are solvated by adsorbed water. Salts, particularly chloride salts like NaCl, are widely found on Earth and other planets and exhibit unique properties and chemical reactivities. However, our comprehensive understanding of these properties is still evolving. NaCl, in particular, plays a significant role in Earth's climate. Due to its high hygroscopicity, it contributes to aerosol growth and, consequently, cloud formation. In its dry, crystalline form, NaCl is generally inert, except at its surface, where it can react with nitrogen oxides. This reactivity becomes especially relevant considering that the NaCl surface begins to bind with water at relatively low humidity levels. This study investigates the chemical interactions at gas-particle interfaces, focusing on how NaCl surfaces react with SO2. The study uses a blend of experimental techniques and theoretical models, including a comparison with NH4Cl to assess the impact of different cations. The findings reveal that NaCl surfaces rapidly transform into Na2SO4 and release a new chlorine component when exposed to SO2 in low-humidity conditions. In contrast, NH4Cl surfaces show limited SO2 absorption and minimal change. Further analysis through depth profiling demonstrates the altered layers and specific elemental ratios at the surfaces of the crystals. The study identifies that the chlorine species detected are expelled from the NaCl crystal structure. This conclusion is supported by detailed atomistic density functional theory calculations. Additionally, molecular dynamics simulations bring to light the dynamic and chemically active environment of the NaCl surface, influenced significantly by an intense interfacial electric field and the presence of water layers, even in trace amounts.
AS55-A019
The Roles of Aerosol Liquid Water in Haze Formation
Zhijun WU#+
Peking University
Aerosol liquid water (ALW) plays important roles in haze formation. ALW can serve the reaction vessels in multiphase chemistry and modify the aerosol phase state. Thus, ALW plays profound roles in secondary aerosol formation. The hygroscopic aerosols can take up water and grow in size, thereby, change the aerosol optical properties. In this talk, the roles of aerosol liquid water in haze formation will be summized and the future studies will be pointed out.
AS55-A011
Phase State and Viscosity of Secondary Organic Aerosols and Their Effects on IEPOX-SOA Particle Formation Simulated Over China
Ying LI1#+, Zhiqiang ZHANG2, Yele SUN2
1Dalian University of Technology, 2Chinese Academy of Sciences
Secondary organic aerosols (SOA) can exist in liquid, semi-solid or amorphous solid states, which are rarely accounted for in current chemical transport models (CTMs). Missing the information of SOA phase state and viscosities in CTMs impedes accurate representations of SOA formation and evolution, thus affecting the predictions of aerosol effects on air quality and climate. We have previously developed a method to estimate the glass transition temperature (Tg) of an organic compound based on volatility. In this study, we apply this method to predict the phase state and viscosities of SOA particles over China in summer of 2018 using the Weather Research and Forecasting model coupled to Chemistry (WRF-Chem). This is the first time that spatial distributions of the SOA phase state over China are investigated by a regional CTM. Simulations show that Tg values of dry SOA range from ~290 K to 320 K, with higher values in the northwestern China where SOA particles have low volatilities. Considering the water uptake by SOA particles, the SOA viscosity also shows a prominent geospatial gradient that highly viscous or solid SOA particles are mainly found in the northwestern China. Isoprene epoxydiol secondary organic aerosols (IEPOX-SOA) are key components of sub-micrometer biogenic SOA particles. Based on the predicted viscosity of SOA particles which is a function of chemical composition, ambient temperature and relative humidity, we further simulate the effects of particle phase state on the reactive uptake of IEPOX, which has implications in properly representing the particle phase state involved multiphase chemistry in CTMs.
AS55-A005
The Global Impact of Organic Aerosol Volatility on Aerosol Microphysics
Chloe Yuchao GAO1#+, Susanne BAUER2, Kostas TSIGARIDIS3
1Fudan University, 2NASA Goddard Institute for Space Studies, 3Columbia University
We present MATRIX-VBS, a new aerosol scheme that simulates organic partitioning in an aerosol microphysics model, as part of the NASA GISS ModelE Earth System Model. MATRIX-VBS builds on its predecessor aerosol microphysics model MATRIX (Bauer et al., 2008) and was developed in the box model framework (Gao et al., 2017). The scheme features the inclusion of organic partitioning between the gas and particle phases and the photochemical aging process using the volatility-basis set (Donahue et al., 2006). To assess and evaluate the performance of the new model, we compared its mass concentration, number concentration, activated number concentration, and aerosol optical depth (AOD), to the original scheme MATRIX, as well as against data from the NASA Atmospheric Tomography Mission (ATom) aircraft campaign, the Aerosol Robotic Network (AERONET) ground measurement stations, and satellite retrievals from MODerate resolution Imaging Spectroradiometer (MODIS) and Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO). Results from MATRIX-VBS show that organics are transported further away from their source, and their mass concentration increases aloft and decreases at the surface as compared to those in MATRIX. The mass concentration of organics at the surface agrees well with measurements, and there are discrepancies for vertical profiles aloft. In the new scheme, there is an increased number of particles and fewer activated ones in most regions. The difference in AOD between the two models could be attributed to smaller particles in the new model and the difference in aerosol compositions. The new scheme presents advanced and more comprehensive capability in simulating aerosol processes.
AS55-A012
Evidence of Surface Tension Lowering of Atmospheric Aerosols by Organics from Field Observation in an Urban Atmosphere: Relating to Particle Size and Chemical Composition
Tianyi FAN1+, Fang ZHANG2#, Jingye REN3, Zhanqing LI4, Chenxi LIU1, Yuying WANG5, Xiaoai JIN6, Jieyao LIU1, Yele SUN7
1Beijing Normal University, 2Harbin Institute of Technology, 3Xi’an Institute for Innovative Earth Environment Research, 4University of Maryland, 5Nanjing University of Information Science & Technology, 6Zhejiang A&F University, 7Chinese Academy of Sciences
The surface-active organics lower the aerosol surface tension, leading to enhanced cloud condensation nuclei (CCN) activity and potentially exerting impacts on the climate. Quantification of surface tension is mainly limited to laboratory experiments or modeling work for particles with selected size and known chemical composition, while inferred values from ambient aerosol population is deficient. In this study, we alternatively derive surface tension by combining field measurements at an urban site in northern China with the κ-Köhler theory. The results present new evidence that organics remarkably lower the surface tension of aerosols in polluted atmosphere. We show particles sized around 40 nm are with an averaged surface tension of 53.8 mN m-1, while particles with growing size up to 100 nm show surface tension approaching that of the pure water. By linking field results to the dependence curve of surface tension with the organic mass, we find the decrease of surface tension with increasing organic mass resembles the behavior of dicarboxylic acids, which are water-soluble organic compounds commonly found in urban aerosols. This suggests that these species may play a critical role in depressing the surface tension and altering the CCN activity. The study further reveals that neglect of surface tension lowering effect would result in lowered ultrafine CCN (diameter < 100 nm) concentration by 6.8% to 42.1% at a typical range of supersaturations in clouds, demonstrating the significant impact of surface tension on the CCN concentration of urban aerosols. This work can provide a framework of utilizing field measurements to infer surface tension as observational constrains for CCN parameterization in climate models, and thus to improve the estimation of aerosol climate effect.
AS55-A001
Phase State of PM2.5 in Northeast Asia During 2023 Autumn
Daeun KIM1+, Kyounghee KO1, Changjoon SEONG1, Zhijun WU2, Jiyi LEE3, Kwangyul LEE4, Jun-Young AHN4, Kyoung-Soon JANG5, Changhyuk KIM6, Natsagdorj AMGALAN7, Mijung SONG1#
1Jeonbuk National University, 2Peking University, 3Ewha Womans University, 4National Institute of Environmental Research, 5Korea Basic Science Institute, 6Pusan National University, 7National University of Mongolia
Recent research indicates that phase states (liquid, semi-solid, solid) of aerosols are key factors in the generation of high-concentration particulate matter (PM). Therefore, understanding phase state of aerosol is essential in assessing their effects on air quality and public health. Despite the acknowledged significance, studies focusing on phase state of ambient fine particulate matter (PM2.5) are exceedingly uncommon. To investigate phase state in ambient aerosols, this study was conducted using PM2.5 filters collected simultaneously from September to October 2023 in four sites of Northeast Asia: Seoul, Seosan, Beijing, and Ulaanbaatar. The filters were chosen for the analysis from dates when PM2.5 concentrations exceeding 15 μg/m3, aligning by the World Health Organization's (WHO) standards for high-concentration PM2.5. Moreover, by using an extraction method that combines methanol and water, this research aims to assess the influence of PM2.5 components on phase state. To determine phase state of PM2.5, optical microscopy and poke-and-flow method were used. This study revealed that ambient PM2.5 can exhibit various phases state influenced by multiple factors, and this understanding allows for predictions about their impact on climate change and human health. The results will be presented.
AS55-A014
Particle Phase State and Aerosol Liquid Water Greatly Impact Secondary Aerosol Formation: Insights Into Phase Transition and Role in Haze Events
Xiangxinyue MENG1+, Zhijun WU1#, Jingchuan CHEN1, Qiu YANTING1, Taomou ZONG1, Mijung SONG2, Jiyi LEE3, Min HU1
1Peking University, 2Jeonbuk National University, 3Ewha Womans University
Particles, as crucial reaction vessels in atmospheric chemical processes, undergo dynamic changes in their phase state due to variations in relative humidity (RH) and chemical composition. These changes affect the mass transfer of reactive gaseous molecules between the gas and particle phases, subsequently influencing the secondary formation of aerosols. This study focuses on the haze events during the winter of 2020 in Beijing. It explores the relationship between the phase state of particulate matter and aerosol liquid water (ALW), as well as their role in the formation of secondary aerosols. Our findings reveal that particles predominantly exist as semi-solid or solid during clean winter days with ambient RH below 30%. However, non-liquid to liquid phase transition occurs when the ALW mass fraction exceeds 15% (dry mass) at transition RH thresholds of 40-60%. During haze episodes, the transformation rates of sulfate and nitrate aerosols rapidly increase through phase transition and increased ALW by 48% and 11%, respectively, resulting in noticeable increases in secondary inorganic aerosols (SIA). The presence of abundant ALW, favored by elevated RH and higher proportion of SIA, facilitates heterogeneous and aqueous processes in liquid particles, leading to a substantial increase in the formation of secondary organic aerosols and elevated aerosol oxidation. Consequently, the overall hygroscopicity parameters exhibit a substantial enhancement with a mean value of 23%. These results highlight phase transition as a key factor initiating the positive feedback loops between ALW and secondary aerosol formation during haze episodes over the North China Plain. Accurate predictions of secondary aerosol formation necessitate explicit consideration of the particle-phase state in chemical transport models.
AS55-A004
The Role of Organic Partitioning in Biomass Burning Aerosol Mixing State Evolution
Yiran SHE1#+, Chloe Yuchao GAO1, Susanne BAUER2, Kostas TSIGARIDIS3, Arthur J. SEDLACEK4, Jianmin CHEN1
1Fudan University, 2NASA Goddard Institute for Space Studies, 3Columbia University, 4Brookhaven National Laboratory
Biomass burning aerosols play a key role in both regional and global atmospheric composition, influencing the Earth’s radiative balance. Recent observations from field campaigns have shed light on the dynamic nature of these aerosols, particularly noting changes in aerosol mixing states due to plume aging over different temporal scales. These insights provided the basis for more advanced modeling of aerosol process and mixing state. Our study employs two aerosol microphysics schemes with different organic aerosol treatments - MATRIX with non-volatile organic aerosols and MATRIX-VBS with semi-volatile organic aerosols - within the NASA GISS ModelE Earth system model, to simulate the evolving mixing states of biomass burning aerosols. We evaluate how well both schemes capture the observed variability in biomass burning aerosol mixing states, drawing from data from wildfire campaigns and experiments, including BBOP_(Biomass Buring Observation Project), ORACLES_(ObseRvations of Aerosols above Clouds and their intEractionS), and LASIC_(Layered Atlantic Smoke Interactions with Clouds). Preliminary findings suggest that MATRIX-VBS, with its inclusion of organic aerosol partitioning, more accurately represents the post-wildfire evolution of black carbon aerosol mixing states compared to MATRIX. This underscores the significant influence of aerosol processes, particularly organic condensation, on the evolution of aerosol mixing states.
AS55-A015
Size-resolved East Asian Dust Ice-nucleating Particles: Impact of Atmospheric Chemical Modification on Ice Nucleation Activity
Jingchuan CHEN1#+, Zhijun WU1, Weijun LI2, Min HU1
1Peking University, 2Zhejiang University
Airborne mineral dust triggers ice formation in clouds and alters cloud microphysical properties by acting as ice-nucleating particles (INPs), potentially influencing weather and climate at regional and global scales. Anthropogenic pollution would modify natural mineral dust during the atmospheric transport process. However, the effects of anthropogenic pollution aging on the ice nucleation activity (INA) of mineral dust remain not well-understood. In this study, we investigated the immersion mode ice nucleation properties and particle chemical characterizations of collected size-resolved Asian dust samples (eight particle size classes ranging from 0.18 to 10.0 μm), and testified the chemical modification of aged dust particles via particle chemistry and morphology analyses including the mass concentrations of particulate matter, the water-soluble ion concentrations, the mental element concentrations, and single-particle morphology. The mass fraction of Ca2+ in element Ca and the mean relative mass proportions of supermicron Ca2+ increased by 67.0% and 3.5-11.2% in aged Asian dust particles, respectively, suggesting the occurrence of heterogeneous reactions. On the other hand, the total INP concentrations and total ice nucleation active site densities were consistent between aged and normal dust particles (0.62-1.18 times) without a statistically significant difference. And the INP concentrations and ice nucleation active site densities of chemically aged supermicron dust (1.0-10.0 μm) in each particle size class were nearly equal to or slightly higher than those of normal Asian dust, which were 0.70-2.45 times and 0.64-4.34 times at -18 ℃, respectively. These results reveal that anthropogenic pollution does not notably change the INP concentrations and does not impair the INA of Asian dust. Our work provides direct observational evidence and clarifies the non-suppression effect of anthropogenic pollution on the INA of East Asian dust, advancing the understanding of the ice nucleation of airborne aged mineral dust.
Session Chair(s): Aneesh SUNDARESAN, IBS Center for Climate Physics, Manuel Tobias BLAU, IBS Center for Climate Physics, Pengfei LIN, Chinese Academy of Sciences
AS54-A017
Timely Event Attribution Using Large Ensemble Simulations
Yukiko IMADA1#+, Hiroaki KAWASE2, Chiharu TAKAHASHI2, Hideo SHIOGAMA3, Tetsuya TAKEMI4
1The University of Tokyo, 2Japan Meteorological Agency, 3National Institute for Environmental Studies, 4Kyoto University
There are many evidences of connections between long-term trends of extreme events and the human influence. However, specific extreme events can not totally be blamed on the past human activity, because extreme events can be happened only due to the natural variability. An attempt to examine whether human influence has largely affected the probability of extreme events by comparing large-ensemble climate model simulations under the “factual” conditions and the “counterfactual” ones that omit the influences of anthropogenic climate drivers is known as “Event Attribution” (EA). Over the past decade, the results of various EA studies have been published. EA is in high demand from society as means of contributing to raising awareness of climate change issues, since EA can make people feel the effects of climate change through actual extreme events. In recent years, there has been an increasing demand from society for rapid publication of EA results despite the time it takes to obtain results because of the large ensemble calculations involved in common EA methods. To meet these demands, we are currently working to achieve timely EA using two different methods. One is predictive EA which incorporate operational seasonal forecasting information to prepare large ensemble calculations prior to the occurrence of an extreme event, and the other is statistical EA utilizing an existing large ensemble database. We will present an overview of the results of each method.
AS54-A004
Detection and Attribution of the Weakening of Global Angular Momentum
Susmit Subhransu SATPATHY1,2#+, Christian FRANZKE2
1IBS Center for Climate Physics, 2Pusan National University
The slowing down of the circulation in a warming climate due to anthropogenic forcings is still not understood. The role of internal variability and anthropogenic forced response in climate models influencing the weakening of global angular momentum has not been examined in detail. Here in this study, we utilise a 100-member ensemble simulation (CESM2-LENS) to detect and attribute the causes of the slowing down of atmospheric circulation. We observe a progressive decrease in angular momentum, projected to continue until the year 2100. The rate of weakening is observed to accelerate within the 1980~2020 period closely resembling the Atlantic Multidecadal Oscillation (AMO) and Pacific Decadal Oscillation (PDO) shift, with the entering of the positive phase of AMO and the negative phase of the PDO during the end of the 20th Century. Using, multivariate linear regression analysis, we provide the combined role of AMO, PDO, and GMST (a proxy for climate change signal) in influencing the angular momentum changes during the 20th and 21st centuries. Further, we use a statistical-based approach applied to the ensemble simulations to extract the indirect response (internal variability) and provide the linkage of the AMO and PDO shift in contributing to the weakening rate. Our results elucidate the potential role of the climate system's internal variability and anthropogenic forcings in modulating the distribution of the global angular momentum.
AS54-A018
The Impact of the Tropical Pacific on Projections of an Ice-free Arctic
Jahfer SHARIF1+, Kyung-Ja HA1#, Eui-Seok CHUNG2, Christian FRANZKE1, Sahil SHARMA3,1
1Pusan National University, 2Korea Polar Research Institute, 3IBS Center for Climate Physics
The observed sea ice concentration (SIC) over the Arctic has reduced substantially in recent decades, with largest retreat during the August-September-October (ASO) season. The ensemble mean of the SIC simulated by the Coupled Model Intercomparison Project Phase 6 (CMIP6) projections reveals that the summertime Arctic will turn ice-free during the second half of this century. However, the Arctic sea-ice projections exhibit large uncertainties among the climate models. Though the role of global warming and internal variabilities has been well studied, the impact of the tropical Pacific on Arctic SIC has yet to receive much attention. Observations show that the man Arctic SIC grows during a weakening of the Aleutian Low, corresponding to cooling in the equatorial Pacific, and vice versa. This study uses 36 models with all the available ensemble members to analyze the fate of Arctic SIC under four different CMIP6 Shared Socioeconomic Pathways (SSP) scenarios. We find that the strength of the Pacific-Arctic teleconnection differs significantly among the models. The study demonstrates that the models in which the impact of El Niño-driven SIC loss is stronger than the La Niña-driven SIC growth tend to turn seasonally ice-free 10–20 years earlier than the ensemble mean. We show how the non-linear impact of ENSO-related SIC changes resulted in a faster SIC decline in models with solid teleconnection. The ENSO-induced SIC loss is more robust than the growth events during the historical and future scenarios. Further, we show that the shift in intensity and variability of ENSO by the end of the 20th century triggers the divergence in simulated Arctic SIC. Our results suggest that climate models must better capture the realistic tropical Pacific-Arctic teleconnection to predict the long-term evolution of the Arctic climate.
AS54-A019
Future Thermal Environment in Japan from Large Ensemble Climate Dataset d4PDF
Ko NAKAJIMA1#+, Yukiko IMADA1, Rui ITO2,3, Kazutaka OKA4
1The University of Tokyo, 2Japan Agency for Marine-Earth Science and Technology, 3Meteorological Research Institute, 4National Institute for Environmental Studies, Japan
Human-induced warming led to a temperature approximately 1°C above pre-industrial levels in 2017, and is projected to rise by 4.8°C from 1985–2005 to 2081–2100 under the highest IPCC greenhouse gas emissions scenario (RCP8.5). Recently, the incidence of heatstroke in Japan has increased due to this climate change. Projection future thermal environment is important for climate change strategies. To evaluate future thermal environment, the large ensemble data set called the Database for Policy Decision making for Future climate change (d4PDF). The historical and 4K warming climates were used as current and future climates, respectively. Wet bulb globe temperature (WBGT) is often used to estimate the thermal environment. The simulated WBGT was bias corrected using the method in Piani et al. (2010). A WBGT of 33°C is regarded as a critical threshold indicating an extremely high risk of heatstroke. When it is predicted to surpass this threshold, a heatstroke caution alert is issued. In the current summer, the probability of the daily maximum WBGT exceeding this threshold is less than 10%. In the future climate, it is forecasted that in almost all areas across Japan, the daily maximum WBGT will exceed this threshold with a frequency of more than 50%. The intraday WBGT variations were also evaluated. Harsh heat conditions was indicated not only during the daytime but also at night. For instance, in Tokyo, the nighttime WBGT exceeds 28°C with a frequency of over 70%. According to the standards set by the Ministry of the Environment, this value corresponds to a level where "intense physical activity should be discontinued." These results suggest that under future climate conditions, conducting outdoor activities as currently will be difficult.
AS54-A003
The Decadal Phase Shift and Forced Response of the Indian Monsoon Rainfall and Its ENSO Teleconnection
Aneesh SUNDARESAN1,2#+, Tamas BODAI1
1IBS Center for Climate Physics, 2Pusan National University
The Indian summer monsoon (ISM) is an integral part of the climate system and exhibits significant variabilities ranging from seasonal to multidecadal time scales. The present study investigates the physical mechanism responsible for the externally forced as well as the decadal changes of the ISM rainfall by analysing the CESM2 and MPI-ESM large ensemble simulation datasets. Also, we delve into the mechanism behind the epochal changes in the ENSO-ISM teleconnection. A composite analysis is performed using 10 ensemble members of both models having excess and drought monsoon rainfall during the 1981-2010 period. The excess monsoon periods are associated with an anomalous ascending motion over the Indian Ocean, meanwhile an anomalous descending motion is observed over the Pacific Ocean. Simultaneously, the SST pattern depicts a negative Pacific decadal oscillation (PDO) like pattern over the Pacific Ocean and a positive Atlantic multi-decadal oscillation (AMO) like pattern over the North Atlantic Ocean. The phase changes of the oceanic decadal oscillations and the associated shift in the Walker cell might be the triggering factor of the ISM decadal variability. The forced response of the ISM rainfall during the 1981-2010 period shows an increase over the Indian region and a northward shift in the rainband over the equatorial Pacific and the Atlantic Ocean. The enhanced ISM rainfall was favoured by the strengthening of monsoon low level jet (LLJ) and a reduced dry wind intrusion through the north-west India, mainly caused by the strong west Asian warming. The epochs with strong ENSO-ISM rainfall teleconnections are associated with an eastward shift in the ascending branch of the Pacific Walker cell and precipitation pattern. Changes in the Walker cell are connected to the weakened east-west SST gradient over the Pacific Ocean.
AS54-A014
Drivers of Future Extratropical Sea Surface Temperature Variability Changes in the North Pacific and Beyond
Jacob GUNNARSON, Malte STUECKER#+, Sen ZHAO
University of Hawaii at Manoa
Future changes to climate variability, beyond specific modes such as the El Niño-Southern Oscillation (ENSO), has so far not been well-characterized. A recent sufficiently large climate model ensemble with 100 members (using the Community Earth System Model version 2: CESM2-LE; Rodgers et al. 2021) now allows us for the first time to achieve robust estimates of how the variance of difference climate variables is projected to change in the future and determine why. Intriguingly, future changes to sea surface temperature (SST) variability are highly spatially heterogenous in CESM2-LE, which has important implications for future marine heatwave statistics. We examined these projected SST variance changes (between 1960-2000 and 2060-2100) in the North Pacific using a local linear stochastic-deterministic model, which allowed us to quantify the effect of changes to three drivers on SST variability: ocean “memory” (the SST damping timescale), ENSO teleconnections, and stochastic noise forcing. The ocean memory declines in most areas, but lengthens in the central North Pacific. This change is primarily due to changes in air-sea feedbacks and ocean damping, with the shallowing mixed layer depth playing a secondary role. An eastward shift of the ENSO teleconnection pattern is primarily responsible for the pattern of SST variance change. The framework developed here allows a quantification of future SST variance changes in most of the global ocean regions.
AS54-A016
Understanding the Changes on the Role of Internal Climate Variability in a Changing Climate
Sae-Yoon OH#+, Sang-Wook YEH
Hanyang University
Previous studies indicate that the role of internal climate variability (ICV) is dominant on the uncertainty of surface temperature projections in the near term future climate, while model bias and scenario uncertainty play a large role in the mid- and long-term future climate. However, there is a still lack of understanding on which ICV is the main factor influencing the uncertainty in surface temperature projections. This study focuses on the changes in the characteristics of ICV in surface temperature projections. Using Large Ensemble climate model simulations, we found that the impact of ICV on surface temperature projection remains consistent in a changing climate. We further found that an ENSO-like surface temperature pattern plays a crucial role in determining the inter-model spread of surface temperature simulated in climate models from the present day climate to the future climate. Furthermore, we investigate how these ICV factors change in the future and their impact on global surface temperature trends.
AS54-A015
Contributions of External Forcing and Internal Variability to the Multidecadal Warming Rate of East Asia in the Present and Future Climate
Dajeong JEONG1#+, Changhyun YOO1, Sang-Wook YEH2
1Ewha Womans University, 2Hanyang University
The multidecadal variation in the warming rate of East Asia results from a combination of external forcing and internal variability. Using the Coupled Model Intercomparison Project Phase 6 (CMIP6) multi-model mean, rescaled to match observed temperatures from 1890–2020, we examine that external forcing contributes approximately −0.2 to 0.1 K decade−1 to the warming rate until the 1980s. However, this rate notably increases to 0.4 K decade−1 in recent decades. Further decomposition of this multidecadal variation in the forced response highlights distinct contributions from greenhouse gases, anthropogenic aerosols, and natural forcing. After isolating the internal variability by excluding the external component, the warming rate attributed by internal variability is ±0.15 K decade−1 in the 20th century, peaking at about −0.21 K decade−1 in recent decades. We investigate that 68% of the variance in internally generated temperature anomalies can be explained by the Indian Ocean Basin Mode (IOBM), the Atlantic Multidecadal Oscillation, and the Interdecadal Pacific Oscillation, with the IOBM playing a predominant role. In future simulation under the Shared Socio-economic Pathway 2-4.5 scenario, the impact of external forcing is projected to triple over the 2020–2100 period. While the influence of internal variability remains relatively stable during this period, the contribution of external forcing becomes more pronounced in driving East Asian warming. These findings enhance our understanding of both external and internal factors that shape trends and variations in the warming rate of East Asia and providing valuable insights for refining future climate projections.
AS54-A001
Quantifying Parametric Uncertainty Effects on Tropical Cloud Fraction and ITCZ Precipitation in an AGCM
Feng XIE1,2#+, Lijuan LI1
1Chinese Academy of Sciences, 2Anhui Meteorological Observatory
This work investigates potential improvements through perturbing nine moist physical parameters, using uniform sampling and Latin hypercube sampling methods, and quantifies the parametric uncertainty and effects of nonlinear interaction between parameters on the tropical cloud fraction and the ITCZ precipitation in GAMIL2 (the Grid-Point Atmospheric Model of the IAP LASG, version 2). Results show that the uncertainty ranges of the tropical total cloud fraction, low-marine-stratus cloud (LSC) and ITCZ precipitation associated with multiple-parameter perturbation are larger than those from any single-parameter perturbation. The total cloud fraction is significantly improved with multiple-parameter perturbation and the LSC also increases notably when using parameter values optimized for the total cloud fraction because of the indirect parametric effect on lower-tropospheric stability. The double ITCZ bias with excessive precipitation over the central and eastern Pacific south of the equator can be substantially reduced by suppressing deep convection intensity via multiple parameter perturbation, thereby highlighting the profound influences of interactions between parameters on ITCZ precipitation. The effects of efficiency of precipitation and evaporation for deep convection are highly dependent on the threshold value for relative humidity for deep convection. The overall nonlinear interaction among all the parameters reduces large values of total cloud fraction but has a strong incremental effect on large values of LSC over the southeast Pacific. The strong overall nonlinear interaction in extreme precipitation simulation tends to exacerbate the double ITCZ bias, which is closely associated with its impact on the intensity of moist processes.
Session Chair(s): Su SHI, Fudan University, Xia MENG, Fudan University
AS12-A011
The Capability of Deep Learning Model to Predict Atmospheric Compositions Across Spatial and Temporal Domains
Weichao HAN1#+, Tailong HE2, Zhe JIANG3, Min WANG1, Dylan JONES4, Kazuyuki MIYAZAKI5, Yanan SHEN1
1University of Science and Technology of China, 2University of Washington, 3Tianjin University, 4University of Toronto, 5California Institute of Technology
Machine learning (ML) techniques have been extensively applied in the field of atmospheric science. It provides an efficient way of integrating data and predicting atmospheric compositions. However, whether ML predictions can be extrapolated to different domains with significant spatial and temporal discrepancies is still unclear. Here we explore the answer to this question by presenting a comparative analysis of surface carbon monoxide (CO) and ozone (O3) predictions by integrating deep learning (DL) and chemical transport model (CTM) methods. The DL model trained with surface CO observations in China in 2015-2018 exhibited good spatial and temporal extrapolation capabilities, i.e., good surface daily CO predictions in China in 2019-2020 and over 10% independent observation stations in China in 2015-2020. The spatial and temporal extrapolation capabilities of DL model are further evaluated by predicting hourly surface O3 concentrations in China, the United States (US) and Europe in 2015-2022 with a DL model trained with surface O3 observations in China and the US in 2015-2018. Compared to baseline O3 simulations using GEOS-Chem (GC) model, our analysis exhibits mean biases of 2.6 and 4.8 µg/m3 with correlation coefficients of 0.94 and 0.93 (DL); and mean biases of 3.7 and 5.4 µg/m3 with correlation coefficients of 0.95 and 0.92 (GC) in Europe in 2015-2018 and 2019-2022, respectively. This analysis indicates the potential of DL to make reliable atmospheric composition predictions over spatial and temporal domains where a wealth of local observations for training is not available.
AS12-A013
Unified Model of Forecasting Ozone
Zhenze LIU#+
Nanjing University of Information Science & Technology
The chemical transport models face challenges in simulating the concentrations of surface ozone accurately in all conditions when meteorology and chemical environment are changing. The capability of capturing the principle physical and chemical processes is clearly limited. We propose a unified framework based on deep learning to provide a more accurate prediction of surface ozone. The model is tailored to individual observation sites in China, forming a specific graph that would reflect the interaction between spatial and temporal connection in physics and chemistry. This mitigates the uncertainty associated with model resolution and emissions. We show that the model achieves the State-of-the-Art (SOTA) performance in simulating MDA8 ozone among current process-based and other deep learning models. The model structure is also flexible to be applied to other places where observations are available such as Europe and North America. This work underscores great benefits that can be gained through implementing more measurement sites to enhance the density of the model graph.
AS12-A014
Projecting Global O3 Concentrations to 2100 Under Different Climate Change Scenarios Using Deep Learning
Xingcheng LU1#+, Wanying CHEN2
1The Chinese University of Hong Kong, 2The Hong Kong University of Science and Technology
Ozone (O3) poses significant threats to human health and the environment, emphasizing the vital need to comprehend the impact of climate mitigation on future maximum 8-hour average ozone (O3-8h) trends. This study generates a novel dataset of global-scale, spatially explicit O3-8h concentrations spanning from 2021 to 2100, with a spatial resolution of 0.5°×0.5°. This dataset was created by leveraging deep learning techniques, reanalysis data, emissions data, and bias-corrected CMIP6 future climate scenario data. The model robustness was confirmed through a 5-fold validation, showcasing a correlation coefficient (R2) of 0.78. Our results shed light on the future O3-8h concentrations under different climate change scenarios. Under the SSP1-2.6 scenario, a substantial 38.5% reduction is projected in global O3-8h concentration by 2100, driven by significant emission reductions. In the SSP2-4.5 scenario, most regions will experience a decline in O3-8h from the 2030s, ultimately reducing by 16.8%. Conversely, SSP3-7.0 and SSP5-8.5 present different outcomes, with O3-8h continuing to rise in most regions until the 2070s. Notably, in SSP3-7.0, surface ozone pollution worsens through 2100, particularly impacting East Asia and the Middle East. In SSP5-8.5, despite reductions in precursor emissions (NOx and CO), O3-8h continues to rise until the 2070s due to escalating methane emissions. Ultimately, O3-8h is expected to decrease by 9.3% by 2100. These findings underscore the importance of understanding the drivers behind climate change and advocating for appropriate climate mitigation measures as an urgent priority.
AS12-A015
Is Machine Learning a Winner in Seasonal Prediction of Extreme High Temperature Days in Western North America?
Hui TAN+, Zhiwei ZHU#
Nanjing University of Information Science & Technology
Extreme high temperature events lead to catastrophic consequences on public health, the economy and crop losses over North America. Recently, machine learning (ML) methods have achieved significant success in weather forecast, but could ML also perform effective seasonal prediction of extreme high temperature days (EHDs) over North America? Here we explore the spatiotemporal characteristics of the leading modes of EHDs over western North America (WNA). The ML seasonal prediction models are established using multiple boundary layer precursors associated with the leading modes. Although the ML models exhibit almost perfect prediction skills during the training period, the performance of the independent prediction is not satisfactory. By revealing the physical processes of precursors on the leading modes, we finally identify six physically meaningful predictors and establish the statistical seasonal prediction models. The physics-based models show better prediction performance than the ML models and also could independently predict the EHDs over WNA in 2021.
AS12-A012
| Invited
Application of Deep Learning in Regional Air Quality Management
Shuxiao WANG#, Zhaoxin DONG+
Tsinghua University
Addressing rapidly changing air pollution problems require precise spatiotemporal cognition of basic knowledge such as air pollutants emissions, concentrations and their linkage in China and other developing countries. However, traditional research methods are inadequate to improve the effective temporal and spatial air pollution control strategy timely due to the limited observation sites and high computational. Here we employed several advanced data-driven machine learning methods to investigate the real-time emissions and quantify its impact on air pollutants concentrations. By employed a back-propagation algorithm and a neural-network-based comprehensive chemical transport model, we modified original annual emission inventories and reduced the simulation errors to observation data. The mean absolute error for the NO2, SO2, O3 and PM2.5 concentrations decreased significantly (by 10% to 20 %). Besides, combined with a physically informed variational autoencoder, we achieved the real-time inference of air pollutant emissions by satellite data, which improved the normalized mean biases of NO2 from -0.8 to -0.4 and increased R2 from 0.4 to 0.7. Furthermore, convolutional neural network was utilized to quantify the real-time response of PM2.5 and O3 to emissions and meteorological factors. The deep-learning-based response surface model reduced 90% computational cost whereas promoted spatiotemporal portability. Additionally, dominate meteorological factors and the O3 nonlinearity were identified by deep learning-based air quality simulator. These technique gives more fast and precise knowledge in emissions and concentrations and allows the government to take effective countermeasures ahead to address the heavy pollution period. The application of machine learning promotes the accuracy and timeliness of information for emissions and transformation of air pollutants, which may be continually improved with further efforts in both environmental scientific research and computational technologies.
AS12-A016
Neural Operator Learning for Modeling Carbon Monoxide in India
Sanchit BEDI#+, Sri Harsha KOTA, N.M. Anoop KRISHNAN
Indian Institute of Technology Delhi
Air pollution remains a challenging problem of the modern world. To effectively manage air pollution, air quality modeling is used by the researchers and government to understand the current and future trends, make policy decisions for emissions, and ambient concentrations. Neural Networks, such as Feed Forward Neural Networks (FNNs), Convolutional Neural Networks (CNNs), Long Short Term Memory (LSTM), their combinations and various architectures have been tried in the past to model air pollutants and their concentrations. These architectures are essentially learning the mapping between input and output vectors in finite dimensional spaces, and this sometimes limit their ability to extrapolate to new data and discretization. Recently, neural operators are being developed to learn the mapping between the input and output functions in infinite dimensional spaces. Operator learning involves learning the operator that transforms the input function to generate the output function, without explicitly specifying the operator. In this work, we have applied Neural Operator learning to learn the PDEs that govern the advection and diffusion of Carbon Monoxide over the Indian subcontinent. We have used WRF-Chem simulated data for Carbon Monoxide concentrations over India for the years 2016 and 2017 spanning over different seasons and tested on the data for 2018 for quantifying the effectiveness of the operator learning.
AS12-A017
GAN-based Prediction of Atmospheric Motion Vectors
Byoungjoon NA1#+, Sangyoung SON2
1Kumoh National Institute of Technology, 2Korea University
To better predict storm surge levels and resultant innundations, accurate predictions of wind fields are essential. This study first employed generative adversarial network (GAN) and a deep multi-scale frame prediction method to predict satellite images which were then processed to estimate atmospheric motion vector (AMV) fields loosely based on particle image velocimetry (PIV). Sequences of satellite images of the past 68 tropical cyclones around South Korea were used to train and test GAN. The GAN-derived AMVs were validated with the wind fields derived from numerical weather prediction and radiosonde observations. Through comparison with the radiosonde observations, the root-mean-square error and the wind speed bias of the GAN-derived AMVs were comparable to, and even smaller than those of the NWP-derived wind fields. The current approach may enhance the accuracy in predicting short-term wind velocity fields, which in turn may provide more realistic inputs in storm surge modeling.
Session Chair(s): Jun LI, National Satellite Meteorological Center
AS15-A009
Impact of Bias Correction Scheme with a New Bias Correction Predictor for FY-4A AGRI All-sky Data Assimilation on Typhoon Forecast
Bingying SHI+, Chun YANG#, Jinzhong MIN
Nanjing University of Information Science & Technology
The all-sky assimilation module for Advanced Geosynchronous Radiation Imager (AGRI) onboard the Chinese new generation of geostationary meteorological satellites Fengyun-4A (FY-4A) is constructed in Weather Research and Forecasting Model Data Assimilation (WRFDA) model with Radiative Transfer for the TIROS Operational Vertical Sounder (RTTOV). Based on the characteristics of bias distribution, the cloud effect average is selected as a new bias correction (BC) predictor to remove cloud-related biases in all-sky conditions. The impact of the modified BC scheme and AGRI all-sky assimilation on typhoon Lekima (2019) forecast is evaluated through a set of cycle assimilation experiments with WRFDA 3DVAR component. The result shows that, compared with other BC schemes, the modified BC scheme can effectively reduce the mean standard deviation, root mean square error and absolute mean of observation departure in all-sky conditions. Substantial error reductions in model variables, such as wind, temperature and humidity, are also produced. Meanwhile, compared with clear-sky radiances assimilation, the number of assimilated observations in all-sky assimilation is around 5 times higher. This leads to better analysis fields in all-sky assimilation experiment and further improves track forecast of Lekima by adjusting the subtropical anticyclone and steering flow.
AS15-A018
The First-year On-orbit Bias Characteristics of GIIRS Sounder Onboard FY-4B Satellite
Wei WANG#+, Min MIN
Sun Yat-sen University
China's latest geostationary satellite FY-4B, is equipped with the Geostationary Interferometric Infrared Sounder (GIIRS). This study delves into the first-year bias characteristics of the FY-4B/GIIRS instrument, leveraging observed clear-sky data and utilizing the Radiative Transfer for TOVS (RTTOV) model to simulate infrared (IR) temperature. The results reveal that biases in the long-wave infrared (LWIR) channels are significantly lower than those in the mid-wave infrared (MWIR) channels, indicating the superior performance in the LWIR channels. But across wavenumber from 2228.125cm⁻¹ to 2200 cm⁻¹ channels, the absolute bias increasing rapidly, suggesting diminished sensitivity in the MWIR channel. Furthermore, the annual and diurnal fluctuations of bias are subtle in most channels, except for a slight change exhibiting in the wavenumber less than 850 cm⁻¹ channels, with a coefficient nearing 0.0028. Finally, the correlation coefficient between bias and temperature consistently remains below 0.7, emphasizing the commendable temperature stability of the FY-4B/GIIRS instrument.
AS15-A039
All-sky Microwave Imager Radiance Assimilation in the Korean Integrated Model
Han-Byeol JEONG1,2#+, Sihye LEE1, In-Hyuk KWON1, Adam CLAYTON1, Myoung Hwan AHN2
1Korea Institute of Atmospheric Prediction Systems, 2Ewha Womans University
Satellite microwave imager observations provide extensive information on atmospheric humidity, cloud and precipitation in the lower level atmosphere. The microwave imager all-sky radiances assimilation contributes to improving the forecast accuracy of wind, humidity, and mass variables in the cloud and precipitation areas. Recently, KIAPS have developed an Advanced Microwave Scanning Radiometer 2 (AMSR2) all-sky radiance assimilation system for the Korean Integrated Model (KIM). In the observation pre-processing system, components have been added to support the all-sky approach: Superobbing, radiative transfer model calculations that consider KIM hydrometeors, additional quality control processes, and estimation of observation error based on cloud amount. KIM cycling experiments have been conducted to examine the impact of AMSR2 cloudy pixels. Short-range forecast field verification against MHS, AMSU-A, and AMV observations shows improvements in temperature, humidity, and mass variables in the middle and lower troposphere. In particular, humidity and wind speed O-B statistics improved significantly by up to 2% in the Tropics, where many cloudy pixels are additionally assimilated. A specific question is how much the forecast scores are improved for the extreme event case in the East Asia region. The corresponding results and discussions will be presented in this study.
AS15-A044
Assimilating Satellite-measured Sea Ice Properties Into CICE5 with DART System
Inchae CHUNG1, Sang-Moo LEE1#+, Jeong-Gil LEE2, Young-Chan NOH3, Joo-Hong KIM3, Euijong KANG1, Yonghan CHOI3, Ji-Soo KIM1
1Seoul National University, 2Korea Institute of Science and Technology, 3Korea Polar Research Institute
The variability of Arctic sea ice is important to predict weather and climate in the mid-latitude of the northern hemisphere as well as in Arctic areas. It is important to note that sea ice is one of the most sensitive geophysical parameters to global warming. However, most of sea ice models overestimate sea ice area and thickness in winter and underestimate those in summer, hampering the accurate seasonal/weather forecasts. Therefore, it is necessary to assimilate satellite-based sea ice properties into the sea ice model for better prediction of sea ice properties and the associated other geophysical parameters within the coupled model system. In this study, the satellite-derived sea ice concentration (SIC) and sea ice thickness (SIT) over the Arctic were assimilated by using the DART system into the Community Ice CodE version 5 (CICE5) model. In this study, three SIC data assimilation experiments are conducted: (i) exp1 without data assimilation (ii) exp2 with SIC data assimilation prescribing fixed observation error, and (iii) exp3 with SIC data assimilation prescribing regionally varying observation error. The results showed that the climatological bias in SIC simulation is the most stable for the exp3, inferring that the prescribing regionally varying observation error can improve sea ice simulation with data assimilation. In addition to this, summer SIT was also assimilated into the CICE5 model by implementing the Ensemble Optimal Interpolation (EnOI). The results showed a remarkable improvement in summer sea ice prediction.
AS15-A013
Impacts of Assimilating FY-4A/GIIRS 3D Wind Fields on Typhoon Forecasts
Yan-An LIU1#+, Zhengyan ZHANG1, Jun LI2, Zhenglong LI3, Jiong SHU1
1East China Normal University, 2National Satellite Meteorological Center, 3University of Wisconsin-Madison
The high temporal and spatial resolution atmospheric dynamic profiles retrieved from FY-4A Geostationary Interferometric Infrared Sounder (GIIRS) can provide crucial information on the thermodynamic structure evolution for typhoon monitoring and forecasting. This study investigates the impact of assimilating atmospheric 3D wind fields from the FY-4A/GIIRS on typhoon forecasts, taking Typhoon Lekima (2019) as a case. The results reveal that compared to temperature profiles, wind profiles provide more data coverage around the typhoon and their assimilation improved the initial wind field structure and adjusted the steering flow. The assimilation of GIIRS dynamic profiles alone or the combined assimilation of thermodynamic plus dynamic profiles positively impacts typhoon track forecasts, with a maximum improvement of up to 120 km compared to the control experiment around 48-hour forecast. Additionally, wind profile assimilation positively affects wind field and precipitation forecasts, especially for heavy precipitation, where the ETS score increased by over 10%.
AS15-A034
Impact of Slant-path Radiative Transfer in the Assimilation of Passive Microwave Satellite Observations
Ji-Soo KIM1+, Myoung Hwan AHN2#, Hyung-Wook CHUN3
1Seoul National University, 2Ewha Womans University, 3Korea Meteorological Administration
Radiance from satellite observations is a crucial component in the Numerical Weather Prediction system, and ensuring the high quality of these observations is important for accurate forecasting. This necessitates observation quality control, which utilizes observation counterparts simulated from a radiative transfer model. Traditionally, the radiative transfer models have not fully accounted for the satellite viewing geometry, relying on vertical profiles instead of slanted profiles along the line of sight. However, the discrepancy between slant-path and vertical profiles becomes more pronounced with increasing model resolution. This study implemented a slant-path correction to enhance simulation accuracy. The slant-path profiles were applied to simulate the Advanced Technology Microwave Sounder (ATMS) radiances, and their impact on quality control and assimilation processes was evaluated. The variations of temperature and radiance resulting from the slant-path correction consistently aligned with the meridional distribution of temperature and the satellite scan path. The impact was pronounced in the upper atmosphere and the mid to high-latitude regions. Specifically, over the ocean, the standard deviation of observation minus simulated brightness temperature reduced by up to 4-6% at tropopause channels and 2% at stratospheric and tropospheric channels, with a 6% reduction observed over sea ice regions. Over both ocean and sea ice, the reduction was more prominent at scan edges. The overall effect of the slant-path correction is an improvement in radiance simulation accuracy while some channels exhibited a slight increase in the bias of observation minus simulated TB. This underscores the significance of considering satellite viewing geometry in observation operators for NWP systems. This improvement would contribute to enhancing assimilation and forecast results, which will be presented at the conference.
Session Chair(s): Mizuo KAJINO, Japan Meteorological Agency
AS07-A022
Numerical Simulation of Atmospheric Microplastics and Their Toxicity
Mizuo KAJINO1#+, Satoko KAYABA2, Yasuhiro ISHIHARA3, Yoko IWAMOTO3, Tomoaki OKUDA4, Hiroshi OKOCHI5
1Japan Meteorological Agency, 2University of Tsukuba, 3Hiroshima University, 4Keio University, 5Waseda University
Japan Meteorological Agency has developed a numerical model for atmospheric microplastic particles (NHM-Chem-AMPs). The model divides AMPs into three categories (modes) assuming a log-normal distribution for fine particles (SUB: number-equivalent geometric mean dry diameter of 100 nm), coarse particles (COR: 1 μm), and giant particles (GNT: 10 μm) to calculate the spatiotemporal changes in mass concentration and particle size distribution. NHM-Chem-AMPs provides two versions, a source-specific model of all plastic particles (marine-derived, population-based, and agricultural) and a composition-specific model (polyethylene (PE), Polypropylene (PP), polystyrene (PS), and Polyethylene Terephthalate (PET)). The former is an inverse estimation of emissions based on observations, while the latter is a calculation based on emission inventories by composition. Tire wear particles (TWP), which are considered to be a major component of AMPs, are not handled in NHM-Chem-AMPs, but in the regular version of NHM-Chem. Using NHM-Chem and laboratory experiments, spatial distributions of interleukin-8 (IL-8)-based relative inflammation potentials (IP) of PM2.5 from vehicle exhaust and non-exhaust emission sources including TWP are derived. In this study, IP is first defined as multiplying PM2.5 from different emission sectors by supernatant IL-8 concentrations released using PM2.5 samples, normalized to that of particle-free controls. In our estimates, IP from total vehicle emission is approximately one and two orders of magnitude higher than IP from primary exhaust and IP from fresh TWP, respectively. Recently, however, aged TWPs have been reported to be toxic; thus, the aging process of TWPs needs to be considered in the future.
AS07-A027
Impact of BVOCs Emissions and Aerodynamic Effects of Urban Trees on Urban Air Quality: CFD-chemistry Coupled Model Simulations
Yeon-Uk KIM1#+, Kyung-Hwan KWAK1, Ju-Wan WOO2, Sang-Hyun LEE2, Geon KANG3, Jae-Jin KIM3
1Kangwon National University, 2Kongju National University, 3Pukyong National University
The green infrastructure(such as street trees and green roofs) has become increasingly important to improve urban heatwaves and air quality in urban areas. As a part of green infrastructure, trees were mainly planted for the aesthetics of the city and citizens' relaxation. However, the aerodynamic effects of trees can reduce wind speed and BVOCs emissions of trees contribute to activate chemical reactions affecting air quality. This study used a neighbourhood-scale model incorporating the CFD(Computational Fluid Dynamics) model and the SAPRC(The Statewide Air Pollution Research Center) mechanism. This study aimed to evaluate the impact of urban trees on urban NO, NO2 and O3 concentrations and dispersions, considering both the aerodynamic effects of trees and BVOCs emissions. The study focused on the target area in a densely built-up area in Seoul, Republic of Korea, from September 13th to 19th, 2015. NO, NO2, VOCs, etc. emission rates were estimated using the SOME(Source object-based model for emission). Emissions of BVOCs from the trees were estimated using the MEGAN(Model of Emissions of Gases and Aerosols from Nature) model. Simulation scenarios were designed, considering the aerodynamic effects of trees, BVOC emissions from trees, and AVOC (Anthropogenic Volatile Organic Compound) emissions. As a result of the CFD-SAPRC model simulations, the changes in wind speed induced by trees significantly affected the dispersion patterns of atmospheric pollutants. Furthermore, the emission of BVOCs from trees could deteriorate urban air quality in terms of NO, NO2, O3, etc. The findings highlight the importance of considering both the aerodynamic effects of trees and the chemical reactions of BVOCs when planting trees in urban areas. This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (RS-2023-00219830).
AS07-A031
Effects of Cool Roofs on Turbulent Coherent Structures and Ozone Air Quality in Seoul
Beom-Soon HAN1#+, Jong-Jin BAIK2, Kyung-Hwan KWAK3, Seung-Bu PARK4
1Inha University, 2Seoul National University, 3Kangwon National University, 4University of Seoul
The cool-roof strategy is an effective way of mitigating severe urban heat islands, and its impacts on urban flow and air quality deserve in-depth investigations. This study examines the effects of cool roofs on turbulent coherent structures and ozone air quality in Seoul, South Korea using the Weather Research and Forecasting Community Multiscale Air Quality (WRF-CMAQ) model with a 50 m horizontal grid spacing. Cool roofs decrease the daily average air temperature, planetary boundary layer (PBL) height, and wind speed in the urban area of Seoul by 0.80 °C, 230 m, and 0.17 m/s, respectively. Due to the lowered air temperature by cool roofs, the sea breeze and convective structures weaken and eddies at the PBL top appear less frequently. Since high O3 concentration air flows into Seoul by the sea breeze, the weakened sea breeze decreases the daily average O3 concentration near the surface by 3.3 ppb. Air at lower level is transported upward across the PBL top by convective structures and eddies at the PBL top. The transported air at lower level has lower O3 concentration and higher concentrations of O3 precursors than air at upper level. Therefore, the weakened convective structures and less-frequent appearance of eddies at the PBL top by cool roofs weaken the upward transport of O3 precursors at lower level across the PBL top. As a result, the chemical production of O3 and O3 concentration slightly above the PBL top are decreased. An integrated process rate analysis shows that cool roofs weaken the effects of turbulent coherent structures on O3 concentration.
AS07-A007
Characteristics of the Vertical Distribution of Tropospheric Ozone in Pearl River Delta (PRD), China
Xuejiao DENG#+
China Meteorological Administration
Based on the daily ozone sounding data obtained at Yangjiang, Qingyuan and Hong Kong Observatory (HKO) since 2013 and 2019-2023, and the corresponding tropospheric column ozone (TCO) datasets from satellite AURA Ozone Monitoring Instrument and Aura Microwave Limb Sounder (OMI/MLS), the detail vertical distributions of tropospheric ozone and its influencing factors are presented in Pearl River Delta (PRD). On the whole, ozone profiles observed at Yangjiang, Qingyuan are in accordance with that of the HKO in terms of the vertical structures, indicating OMI/MLS product underestimates the TCO level in the Pearl River Delta (PRD) region. Yangjiang ozone profiles show that there are significant variations both in ozone vertical structure and concentration during the observation period. A significant ozone peak permanently occurs in the lower troposphere at 1.1±0.4 km above surface, and the vertical structural difference is mainly reflected in whether there are low ozone strata (below 30 ppbv) near the tropopause and ozone peaks and high ozone stratification in the middle and upper troposphere. The average ozone peak concentrations in the lower, middle and upper troposphere were higher than the average ground-level ozone concentration. Through the analysis of the profile characteristics, weather situation and backward trajectory, it is concluded that the low ozone strata near the tropopause was caused by regional transport of the tropical air mass from tropical cyclone storm area. Potential vorticity (PV) analysis shows that stratosphere-troposphere exchange (STE) is the main reason for the formation of ozone peak and its concentration variation in the middle and upper troposphere. The photochemical reaction is the main factor affecting the ozone concentration in the lower troposphere. Moreover, STE is also an important factor affecting ozone in the lower troposphere, and its contribution to surface ozone is about 10.9 ppbv.
AS07-A008
Temporal and Spatial Characteristics of Turbulent Transportation of PM2.5 in North China Plain
Yan REN1#+, Hongsheng ZHANG2
1Lanzhou University, 2Peking University
Accurate estimation of turbulent fluxes of fine particulate matter (term as PM2.5) concentration not only helps to calculate source emissions, but also helps to improve the parameterization of PM2.5 turbulent diffusion. Relatively few studies on turbulent transportation of PM2.5 have been reported. In this study, an ultrasonic anemometer and a modified high-frequency scattering extinction coefficient instrument were constructed as a system to obtain PM2.5 mass fluxes, that is PMFlux. Then, PMFlux was applied to the observation stations in four cities of North China Plain, Dezhou, Baoding, Renqiu and Tuonan. Turbulent fluctuations and mass flux of PM2.5 in North China Plain were acquired. For instance, average turbulent mass flux of PM2.5 in Dezhou during December 27, 2018-January 7, 2019 was 0.022 μg m-2 s-1, which shows the overall emission source characteristics; PM2.5 mass flux during five polluted cases were -0.015, -0.030, 0.053, 0.023 and 0.075 μg m-2 s-1, indicating that source-sink properties variated. Turbulent transport law of PM2.5 was also discussed. The normalized standard deviation of PM2.5 in different regions follows a -1/3 power relationship with different coefficients related to the underlying surface characteristics. Similar to wind speed and temperature, the turbulence macroscopic and microscopic characteristics of PM2.5 satisfy the Kolomovgov statistical law. This study extends the application range of Monin-Obukhov similarity theory. Based on this, PM2.5 flux-gradient relationships in four cities were proposed. The turbulent diffusion coefficient, KC, of PM2.5 was also calculated. The results revealed that there is obvious daily variation of KC and a good inverse correlation between KC and PM2.5 concentration. We also found that using heat turbulence diffusion coefficient KH as a replace of KC in existing air quality forecasting models don’t conform the reality physical laws.
AS07-A030
Quantifying Oxidative Potential of Particulate Matter by Ascorbic Acid Assay: A Mechanistic Investigation
Yuhuang CHENG#+, Hanzhe CHEN, Jian Zhen YU
The Hong Kong University of Science and Technology
The inhaled ambient fine particulate matter (PM2.5) could release transition metal (TM, e.g., Cu, Fe, and Mn) ions into human lung tissue. These TM ions could contribute to reactive oxidative species (ROS, e.g., ·O2, H2O2, and ·OH) formation in human lung lining fluid due to their excellent catalytical properties. In addition, ambient organics in PM2.5, especially humic-like substances (HULIS), could complex with TM ions as ligands, facilitating electron transfer during TM-induced ROS generation, thus increasing the adverse oxidative potential (OP) to the human body. Many studies have assessed OP of ambient samples and lab-prepared samples in different acellular OP assays. However, few studies have reported detailed mechanisms or chemical kinetic models to clearly explain the catalytical effects of TM during TM-induced OP formation. In this work, we assessed OP of lab-prepared Cu and Fe samples under different conditions in ascorbic acid (AA) assay. By monitoring the reaction system and analyzing the OP dependence on TM concentration, we proposed a TM-AA complex as the major intermediate and a quasi-Michaelis-Menten mechanism for TM-induced AA oxidation in the OP assay. This mechanism could well explain the unusual chemical kinetics and the nonlinear dose-response observed in TM-induced AA depletion. The following ·OH generation process could also be well understood based on this reaction mechanism. Furthermore, we found that ambient HULIS could stabilize the metal-AA complex, inhibiting the direct electron transfer between metal ions and AA. This results in a long-lasting OP effect of ambient PM2.5 water extract compared with lab-prepared single metal solution. Our results provide in-depth chemical understanding of TM-catalyzed OP formation that links TM concentration and OP together, which gives valuable information and reliable reference for OP calculation and modeling based on measured chemical composition of ambient PM2.5.
AS07-A006
Source Apportionment of PM2.5 Using Positive Matrix Factorization (PMF) in Taiwan from 2017 to 2023
Shao En SUN1#+, Charles CHOU1, Chung Te LEE2, Shih-Yu CHANG3, Chien-Cheng JUNG4
1Academia Sinica, 2National Central University, 3Chung Shan Medical University, 4China Medical University
Long-term monitoring of PM2.5 and the chemical composition provided valuable temporal variation information on air pollutants, which can be used to assess the effectiveness of controlling strategies. The Taiwan Environmental Protection Administration (TEPA) has already established an air quality monitoring network with over 70 stations around Taiwan, continuously collecting data on PM2.5 and related air pollutants. However, the chemical compositions of PM2.5 was not included in the monitoring. This study collected PM2.5 samples and analyzed the chemical composition at six TEPA monitoring stations (Hualien, Banqiao, Zhongming, Douliu, Chiayi, and Xiaognag) from 2017 to 2023. The Positive Matrix Factorization (PMF) method was employed for PM2.5 source apportionment, and ten factors were identified, including “Sulfate”, “Nitrate”, “Traffic emissions”, “Biomass burning”, “Chloride Rich”, “Sea salt”, “Dust”, and “Oil combustion”. Additionally, two factors, including most of the heavy metals were combined as the “Industrial emissions” factor. The result showed that most of the factors have decreasing trends in the six-year period. While “Traffic emissions” showed a decreasing trend, the fraction in PM2.5 increased passively due to larger reductions in “Nitrate” and “Sulfate”. The concentration of “Oil combustion” experienced a rapid drop at the beginning of 2020, possibly due to the implementation of the 2020 Global Sulphur Cap by the International Maritime Organization, which mandated the use of low-sulfur oil in shipping, resulting in a reduction of related components such as V. To investigate why “Industrial emissions” did not decrease, this study used PMF with only the metals data from Zhongming station as an example and constrained one of the factors with the emission profile of coal combustion (Taichung Power Plant). In summary, this study compiled seven years of data and analyzed the potential pollution sources to reveal the temporal variation of each source from 2017 to 2023.
AS07-A025
Influence of Inhaled Size-segregated Aerosols on Human Respiratory System in a Highly Polluted Urban Region of Indo-Gangetic Plain
Nisha RANI+, Monika J. KULSHRESTHA#
CSIR-National Physical Laboratory
Mass-size distributions, correlation with meteorological parameters, human inhalation doses, and influence of size-segregated aerosols on human respiratory system were studied in central Delhi during winter and summer of 2022. Size-segregated aerosol samples were collected using an eight-stage Andersen cascade impactor at CSIR-National Physical Laboratory, New Delhi. The impactor segregates aerosols into nine different size ranges, i.e., <0.43, 0.43-0.65, 0.65-1.1, 1.1-2.1, 2.1-3.3, 3.3-4.7, 4.7-5.8, 5.8-9.0 and >9.0 µm which were classified as sub-micron (PM<0.43-1.1), fine (PM1.1-2.1), and coarse (PM2.1->9) fractions. Mass concentrations of sub-micron, fine, and coarse fractions ranged from 30.6-233.8, 11.0-102.1, and 65.7-158.8 µg/m3 during winter and 12.4-48.1, 10.6-23.3, and 70.1-284.1 µg/m3 during summer respectively. The concentrations of sub-micron and fine particles were relatively higher during winter. In winter, low temperature weakens atmospheric convection, and high RH promotes hygroscopic growth of particles, increasing their accumulation in the atmosphere and, hence, mass concentrations. The concentrations of coarse particles were relatively higher during summer. High temperatures during summer favor convective activities, promoting local resuspension of dust and soil particles. Lognormal mass-size distribution showed a bimodal pattern during winter while unimodal during summer. The multiple-path particle dosimetry (MPPD) model was used to quantify total and regional depositions of size-segregated aerosols in human respiratory airways across various age groups. In all age groups, 35-51% of inhaled submicron, 52-68% of inhaled fine, and 86-96% of inhaled coarse particle concentrations were deposited in human respiratory tract. Coarse particles exhibited the highest deposition in the head (nasal and oral cavities) region, while fine and submicron particles in the pulmonary region. Deposited masses of submicron and fine particles were higher during winter, whereas coarse particles were higher during summer for all age groups. Concentration-weighted trajectory analysis for various size ranges showed that local, regional, and long-range particulate matter transport affected the sampling site’s concentration levels.
AS07-A003
Mobile Observations of Air Pollution Characteristics and Source Tracking : The Case of Megacity Chengdu, China
Hancheng HU#+
Chengdu University of Information Technology
Precise pollution control and source tracking have been commonly used due to the development of portable on-line sampling instruments. This study investigated the spatial distribution characteristics of pollution during a local pollution period in the Shuangliu district of Chengdu, China. The persistent particle size distributions and ozone concentrations in the Shuangliu district were recorded using a mobile observation platform. The three-dimensional spatial and temporal changes in the aerosol size distributions and ozone concentrations were obtained by means of a portable optical particle profiler (POPS), a PO3M ozone detector, a hand-held meteorological station, and a Laser wind lidar. The results indicate that during polluted episodes, the daily particle number concentration (PNC) values ranged from 7,967.63 to 16,342.31 #·cm-3, compared to 4,290.87 to 11,039.61 #·cm-3 during clean episodes. The results revealed that human activities and meteorological conditions were the primary causes of local pollution. Regarding regional transport, 80% of the total particle pollution was likely to occur under the influence of northerly winds and came from the industrial emissions and human activities in upwind areas. Indeed, there are certain relationships between the planetary boundary layer height, the vertical wind direction and speed, and between the planetary boundary layer height and the number concentrations of different particle size ranges. According to the backward trajectory analysis, the industrial cities in northeastern Chengdu, Chongqing Province, were identified as the major regional sources of particle emissions in winter. Our results provide a scientific basis for the control of particulate matter and ozone in the Shuangliu district, which enables targeted pollution prevention and control measures by the relevant departments.
Session Chair(s): Tim LI, University of Hawaiʻi at Mānoa, Rajib MAITY, Indian Institute of Technology Kharagpur
AS04-A085
| Invited
Future Changes in Extreme Precipitation and Their Association with Tropical Cyclone Activity Over the Western North Pacific–East Asian Region in 20 Km AGCM Simulations
Hirokazu ENDO#+, Akio KITOH, Ryo MIZUTA
Meteorological Research Institute
Future changes in extreme precipitation over the western North Pacific–East Asian (WNP-EA) region are investigated using a 20 km mesh atmospheric general circulation model (AGCM). Time-slice simulations are performed under low- and high-emission scenarios using different spatial patterns of changes in sea surface temperature. In the WNP-EA region, future changes in the climatological mean of the annual maximum 1 day precipitation total (Rx1d) are characterized by a large meridional variation, where the higher the latitude, the greater the rate of increase in Rx1d, although this pattern is not so clear under the low emission scenario. This feature probably results from a combination of two factors: a greater warming in high latitudes and a decrease in tropical cyclone (TC) frequency in the subtropics. The future changes in Rx1d climatology for the 20 km AGCM show a marked difference in comparison with those of the lower-resolution AGCM and the Coupled Model Intercomparison Project Phase 5 (CMIP5) models. Part of this discrepancy may come from differences in model resolution through representation of TCs, suggesting that coarse-resolution models may have some systematic bias in their future projection through underestimation of the effect of modulation of TC activity in the WNP-EA region.
AS04-A082
Proxy Records from an Indian Lake to Understand Indian Summer Monsoon Variability and Its Impact on Indian Society
Sreya SENGUPTA1#+, Anil GUPTA1, Arun KAUSHIK1, Shilpa PANDEY2, Prasanta SANYAL3, Manoj JAISWAL3, Dhruv SEN SINGH4, Vartika SINGH2, Biswajit PALAR1
1Indian Institute of Technology Kharagpur, 2Birbal Sahni Institute of Palaeosciences, 3Indian Institute of Science Education and Research Kolkata, 4University of Lucknow
Indian Summer Monsoon (ISM) has played a major role in the growth and development of Indian agriculture and economy thereby shaping the history and lives of people residing in the Indian subcontinent. Recently, Indian lakes have provided significant insight into monsoonal variability. Here, we present a multi-proxy record data set of approximately ~ 6000 cal yr BP using a combination of Accelerated Mass Spectrometry (AMS) 14C and Optically Stimulated Luminescence (OSL) dates from a lake named Chandrika, located in the Gomti river flood plain in the Central Ganga Basin. It is an important agricultural hub and is one of the most densely populated regions of India. The combined dataset of End Member Models (EMMs) major and trace element ratios, Total Organic Carbon (TOC) (wt%), δ13Corg(‰) values and pollen data indicates ~5000 cal yr BP to be the beginning of fluvial to lacustrine transition. It was completed at ~4100 cal yr BP with decreasing ISM precipitation in the region due to 4.2 ka arid event. The lake catchment was dominated by C4 type vegetation during this time period. The beginning of the lacustrine phase after 4100 cal yr BP is accompanied by a return of moderate ISM precipitation condition and the presence of cultural pollen taxa such as Cerealia and microcharcoals indicates the beginning of agricultural activities and human settlement in the region during this time period, which continues up to 3000 cal yr BP. The microcharcoals and cultural taxa increase in abundance after 3000 cal yr BP. Thus, our study shows a close human-climate relationship where shifting climatic pattern after 4.2 ka arid event led to a shift in human habits towards agriculture and pastoralism.
AS04-A084
Cross-seasonal Influence Of Western Tropical Indian Ocean Convection On Winter Climate In Southern China: Role Of The Tibetan Plateau
Ruyue GUO#+, Wei WEI
Sun Yat-sen University
Concurrent cold and wet winter condition in southern China (SC) may cause human discomfort and give rise to freezing rain and snow disasters. It has been linked to the robust convection over the western tropical Indian Ocean (WTIO), which can persist from preceding autumn to winter. The cross-seasonal influence of WTIO convection on the winter climate in SC and the role of the Tibetan Plateau (TP) are revealed by using diagnostic analysis and numerical experiments. Result shows that the anomalous WTIO convection in autumn can excite a wave train propagates northeastward from the Arabian Sea (AS) to SC. The westerly anomalies in the northern flank of the anomalous AS anticyclone are conducive to the widespread cooling in the subtropical Euasia, including the TP. The anomalous cyclone over the TP and SC favors more precipitation in situ. Accordingly, the TP snow cover increased significantly since early winter (NDJ) and persist into the following winter and spring via the snow-albedo effect. The thermal effect of the TP snow cover maintains the anomalous cyclone over SC from autumn to winter. The dynamic effect of the TP topography helps to deepen the Indo-Myanmar trough to its south, favoring more water vapor transport from the Bay of Bengal to SC. The effects of TP help to maintain the influence of the WTIO convection from autumn to winter and result in a cold and wet winter in SC. Result of the CESM experiments further verify that the WTIO heating can triger a wave train propagating to the TP and SC, and the thermal effect of TP is partly responsible for the maintenance of the anomalous circulation into winter.
AS04-A040
The Future Projection of Front Frequency and Precipitation Change in East Asia Using CMIP6
Chia-Chi WANG1#+, Fang-Li YEH1, Huang-Hsiung HSU2
1Chinese Culture University, 2Academia Sinica
The precipitation in spring and Mei-yu seasons is a crucial water resource for agriculture, industry, and people’s livelihood. The future precipitation projection after global warming can provide insights into water resource management. However, the simulation and projection of precipitation and the associated weather phenomena are still uncertain. Here, we apply an objective front detection method to analyze front activities in ERA5 and CMIP6 historical simulations and their future changes (SSP5-8.5) at the end of the 21st century. The original front detection method considers the gradient of wet-ball potential temperature. We have modified this method by including the 850hPa relative vorticity in detecting the Mei-yu fronts. The preliminary results indicate that the location of spring fronts (February to April) is projected to shift northward. The precipitation in the South China Sea, Taiwan, and the Ryukyu Islands will decrease. The Mei-yu (May to June) front frequency will decrease over most East Asia, but the total precipitation will increase, leading to more extreme precipitation. The large-scale moisture transport and circulation change will be discussed to understand the front location and precipitation change mechanism.
AS04-A049
Comparisons Between Short- and Long-lived Break Events During the Western North Pacific Summer Monsoon
Ke XU1#+, Riyu LU2
1Institute of Atmospheric Physics, Chinese Academy of Sciences, 2Chinese Academy of Sciences
The break events of the western North Pacific summer monsoon vary significantly in duration, ranging from a few days to more than two weeks. In this study, we classify the monsoon break events into short-lived (≤8 days) and long-lived (>8 days) events, which account for 78% and 22% of the total events during 1979–2020, respectively. The results show that convection suppression is stronger and broader for long-lived events than for short-lived events. In addition, the temporal distributions of the two break categories are distinct: short-lived events present a roughly even distribution from late July to late September, while long-lived events are highly concentrated, with a striking frequency peak around early September. The mechanisms responsible for break events are investigated. Results indicate that both break categories are co-contributed by 10–25-day and 30–60-day oscillations. Short-lived events result from a phase lock of the two oscillations, which explain 54% and 35% of the convection suppression, respectively. By contrast, long-lived events are initiated by both oscillations but maintained only by 30–60-day oscillations. In addition, 30–60-day oscillations reach the peak intensity after the monsoon onset due to seasonal background changes, which is critical for forming the frequency peak of long-lived events around early September. Furthermore, it is found that long-lived events prefer to occur in the developing phase of positive SST anomalies in the tropical central Pacific, when 30–60-day oscillations are abnormally enhanced over the western North Pacific.
AS04-A055
Korean Precipitation Isotopes Track the Zonal Position of Western Pacific Subtropical High
Sayak BASU1#+, Jasper A. WASSENBURG1, Axel TIMMERMANN2, Yan YANG3, Kei YOSHIMURA3
1IBS Center for Climate Physics, 2Pusan National University, 3The University of Tokyo
The drivers of the oxygen isotope composition in precipitation (d18Oprec) at the Western North Pacific (WNP) proximal region are inadequately understood due to the lack of observational records. Consequently, the climatic significance of the isotopic signature retained in the proxy records (such as speleothems) remains unclear. Here we present isotope-enabled climate model simulations (IsoGSM; 1979-2021) to address the key features of interannual d18Oprec variations. The study area receives its dominant fraction of annual moisture during the East Asian Summer Monsoon season (EASM, Jun-Sep), albeit from multiple oceanic sources. Using IsoGSM moisture-tagging experiments, we assess the variations in source-specific moisture contributions and their association with large-scale atmospheric circulation patterns during the EASM. During 18O-enriched years, higher moisture contributions come from the WNP. These years are associated with El-Nino like tropical sea surface temperature patterns that fuels a westward zonal migration of the Western Pacific Subtropical High (WPSH) that acts as a mechanical barrier to moisture supplied from the 18O-depleted Indian monsoon branch. The zonal migration of WPSH is not affecting precipitation amounts over the Korean Peninsula. Our findings highlight the sensitivity of the d18Oprec values to track the zonal positioning of WPSH. Korean speleothems that record the oxygen isotope composition of fossil precipitation can be used to reconstruct the interannual to decadal variability of WPSH east-west migration.
AS04-A088
Drivers and Characteristics of the Indo-western Pacific Ocean Capacitor (IPOC)
Yan DU1#+, Zesheng CHEN1, Shang-Ping XIE2
1Chinese Academy of Sciences, 2University of California San Diego
Coherently coupled ocean-atmosphere variability of the tropical Indo-Pacific Oceans gives rise to the predictability of Asian summer climate. Recent advances in Indo-western Pacific Ocean capacitor (IPOC) theory and the relationship with El Niño-Southern Oscillation (ENSO) are reviewed. The IPOC features tropical Indian Ocean (TIO) warming and an anomalous anticyclonic circulation over the western North Pacific (WNPAAC), the latter driving water vapor transport to East Asia and causing extreme events, e.g., heavy rainfalls from central China to Japan during the boreal summer. IPOC events often occur in post-ENSO summers, but the significant TIO warming could sustain the WNPAAC without a strong El Niño, forced instead by a strong antecedent positive Indian Ocean Dipole (IOD). In latter cases, the Indian Ocean and WNP act as a self-sustaining system, independent of external forcings. El Niño or positive IOD induces the oceanic downwelling Rossby waves and thermocline warming in the southwest TIO, leading to SST warming and a “C-shaped” wind anomaly during winter and early spring. Furthermore, the southwest TIO downwelling Rossby waves reflect as oceanic Kelvin waves on the African coast. In the early summer, the resultant southeast TIO SST warming induces a second “C-shaped” wind anomaly. Both southwest and southeast TIO warming contribute to the WNPAAC. The WNPAAC modulates the water vapor pathways to East Asia in the late spring and summer, which mostly converge over the South China Sea and adjacent regions before flowing further to the north. More water vapor is transported from the western Pacific warm pool and less from the southern hemisphere and the Indian Ocean. The enhanced Asian Summer monsoon and moisture content lead to extreme rainfalls in central China and Japan during the boreal summer.
AS04-A081
What is the Role of Air-sea Interaction on the Intra-seasonal Fluctuation of the Monsoon Trough?
Yutaro NIRASAWA1#+, Tomoki MIYAKAWA1, Daisuke TAKASUKA1, Takao KAWASAKI1, Ryusuke MASUNAGA2
1The University of Tokyo, 2Japan Agency for Marine-Earth Science and Technology
The monsoon trough (MT) over the Western North Pacific (WNP) influences various extreme events, including tropical cyclones, in east/south-east Asia during boreal summer. It fluctuates intra-seasonally due to intra-seasonal variations such as BSISO. Expanding the knowledge of the MT activity is crucial for understanding and predicting weather phenomena in this region. Considering that the WNP is a region where atmospheric forcing is dominant during boreal summer, air-sea interaction may play an important role in the fluctuation of the MT. In the present study, we compared 10-member ensemble numerical experiments with a non-hydrostatic global atmospheric model “NICAM” and its ocean coupled version “NICOCO” for elucidating the role of air-sea interaction. NICOCO successfully simulated an eastward extension and meridional fluctuation of the MT, while NICAM simulated a slower fluctuation and the MT tended to be stationary. In both experiments, latent and sensible heat flux were larger on the southern portion of convections than the northern portion because the cyclonic circulation following convections acted to accelerate (decelerate) the background monsoonal wind on the southern (northern) portion of convections. This heat flux difference induced a meridionally asymmetric structure of sea surface temperature around convections in NICOCO but not in NICAM, which could have impacts on the fluctuation of convections. Our results suggest that coupling the atmosphere with the ocean improves the representation of the intra-seasonal MT fluctuations over the WNP.
AS04-A060
Interdecadal Variation of the Monsoon Trough and Its Relationship with Tropical Cyclone Genesis Over the South China Sea and Philippine Sea Around the Mid-2000s
Xin WANG+, Wen ZHOU#
Fudan University
This study investigates the interdecadal enhancement of the South China Sea–Western North Pacific monsoon trough (MT) and its relationship with tropical cyclone (TC) genesis in the mid-2000s. Analyses reveal pronounced intensification of the MT, increased synoptic-scale wave activity, and more TC genesis over the South China Sea –Philippine Sea after the mid-2000s. Due to the delayed South China Sea summer monsoon (SCSSM) withdrawal, in the three-dimensional circulation structure, the low-level (850-hPa) MT endures for an extended period, accompanied by a typical cyclonic circulation and more potent convergence and upward motion over the southern South China Sea–Philippine Sea. This creates a beneficial background for TC genesis. Meanwhile, alterations in the intensity and position of the mid-level (500-hPa) Western North Pacific subtropical high and the upper-level (200-hPa) South Asian high impact the vertical circulation structures, thus influencing the overall environmental conditions. Increased moisture, cyclonic anomalies, and enhanced low-level (upper-level) convergence (divergence) act constructively for TC genesis. Intensified barotropic and baroclinic eddy kinetic energy conversions strengthen synoptic-scale systems like synoptic-scale waves, also facilitating TC formation. Anomalous sea surface temperature (SST) warming over the Philippine Sea excites a cyclonic anomaly through an equatorial Rossby wave response due to convective heating, maintaining the MT structure. Model simulations also demonstrate that the warming of SST in September has a positive effect on maintaining the MT structure. In summary, warmer Philippine Sea SST leads to delayed SCSSM withdrawal associated with the persistent MT accompanied by advantageous environmental conditions and more active synoptic-scale waves, leading to the interdecadal increase in TC genesis over the South China Sea–Philippine Sea during the SCSSM withdrawal phase since the mid-2000s.
Session Chair(s): Michiya HAYASHI, National Institute for Environmental Studies
AS61-A009
Revisiting ENSO's Inconsistent Influence on the Equatorial Atlantic
Ingo RICHTER1#+, Tomoki TOZUKA2, Yu KOSAKA2, Shoichiro KIDO1, Ping CHANG3, Hiroki TOKINAGA4
1Japan Agency for Marine-Earth Science and Technology, 2The University of Tokyo, 3Texas A&M University, 4Kyushu University
Even though El Niño-Southern Oscillation (ENSO) is well known to have global impacts, its influence on the adjacent equatorial Atlantic basin is inconsistent. This is perhaps best exemplified by the fact that the extreme 1982 and 1997 El Niño events were followed by Atlantic zonal mode (AZM) events of the opposite sign. Potential reasons for this inconsistent influence are the competition of dynamic and thermodynamic effects, and the delayed effect of off-equatorial Rossby waves forced by wind stress curl in the north-equatorial Atlantic. Here we re-examine this problem using pre-industrial control simulations (piControl) from the Coupled Model Intercomparison Phase 6 (CMIP6). The observed correlation between boreal winter (DJF) sea-surface temperature (SST) in the Niño 3.4 region and the following summer (JJA) SSTs in the ATL3 region is close to zero, indicative of the inconsistent relation between the two. Individual models, however, exhibit a wide range of behaviors with correlations ranging from about -0.5 to +0.5. While the influence of ENSO on equatorial Atlantic SST is inconsistent, the influence of ENSO on surface winds over the equatorial Atlantic is rather robust. All models show a negative correlation between DJF Niño 3.4 SST and boreal spring (MAM) surface winds over the western equatorial Atlantic. In addition, we find that SSTs in the South Atlantic are a precursor to AZM events. Based on these relations, we construct a linear regression model that can predict AZM events in JJA based on a few SST indices in DJF. In most climate models, this simple scheme can predict AZM events with a correlation skill above 0.5 during ENSO years. We will discuss to what extent these insights can help in the prediction of real-world AZM events.
AS61-A034
Isolating Tropical Pacific and Atlantic Interactions on Interannual Timescales
Noel KEENLYSIDE1#+, Lina BOLJKA1, Rodrigo CRESPO MIGUEL2, Ping-Gin CHIU1, Belen RODRIGUEZ-FONSECA2, Francisco CAO GARCIA2, Irene POLO2, William CABOS3, Carlos MECHOSO4
1University of Bergen, 2Universidad Complutense de Madrid, 3University of Alcala de Henares, 4University of California, Los Angeles
Observations indicate periods of time when El Niño Southern Oscillation (ENSO) and Atlantic Niño variability synchronize. During these periods, Atlantic Niño (Niña) events tend to proceed Pacific La Niña (El Niño) events by six months. We analyze historical SST observations using a multivariate empirical mode decomposition and show that the interaction between the two basins occurs on quasi-quadrennial (QQ) and quasi-biennial (QB) timescales, associated with previously identified ENSO timescales. The combination of these two modes over time explains the observed cross-correlation between ENSO and the Atlantic Niño. The QQ mode modulates the strength of the relation on multi-decadal timescales, while the QB mode is mainly responsible for changes in the lead-lag timing. These results are further explained by constructing an inter-basin recharge-oscillator model. Fitting the model to historical data reveals the QQ and QB modes as damped modes. The tropical Atlantic is slaved to ENSO in the QQ mode, while tropical Atlantic appears more important in the QB mode. Finally, these relations are investigated using pacemaker experiments performed with the Norwegian Climate Prediction Model. The model shows that tropical Atlantic variability can explain almost 50% of observed SST variability in the central equatorial Pacific, consistent with a two-way interaction between the two basins.
AS61-A025
Revisiting the Connection Between ENSO and the Following Spring North Tropical Atlantic SST Anomalies
Wei CHEN#+
Chinese Academy of Sciences
The north tropical Atlantic (NTA) displays significant sea surface temperature anomalies (SSTA) during the ENSO decaying spring. We find that this is not always true for El Niño with moderate intensity. Nearly half of the moderate El Niño cases are followed by the strong NTA SSTAs, but others are followed by the weak NTA SSTAs, indicating the uncertainty in the connection between the moderate El Niño and the NTA. Further analysis demonstrates that El Niño, which is accompanied by the strong (weak) Aleutian low leads to the strong (weak) NTA SSTAs, suggesting that the role of the Aleutian low must be considered to fully understand the El Niño–NTA connection. Moreover, the decadal variability in the interannual relationship between ENSO and the NTA SSTA are also examined. We identify a largely weakened impact of ENSO on the SSTA concentrated over the northeast tropical Atlantic (NETA) after the mid-1980s, while the impacts on the SSTA over the northwest tropical Atlantic (NWTA) are stable during the whole period. Further analysis indicates that the decadal changes in the ENSO–NETA connection are due to the westward shift in the ENSO-related convection and teleconnections, resulting from the westward shift of Pacific Walker circulation, induced by the intensified zonal SST gradient over the equatorial Pacific after the mid-1980s.
AS61-A027
The Interdecadal Change of the Relationship Between North Indian Ocean SST and Tropical North Atlantic SST
Juan FENG#+
Chinese Academy of Sciences
The summertime North Indian Ocean (NIO) and tropical North Atlantic (TNA) sea surface temperature (SST) anomalies exert important impacts on atmospheric circulation and climate variation. Little attention is paid on the interdecadal change of NIO-TNA SST connection. This study reveals that the NIO-TNA SST relationship experiences an obvious interdecadal change around the early-2000s. The NIO and TNA SST correlation is positive and significant before the early-2000s, while this connection becomes weak and insignificant after that. This interdecadal change is closely associated with the changes in the ENSO intensity. During 1980-2001, strong ENSO forces a sustained SST warming in the southwest Indian Ocean, which further warms the summertime NIO via inducing antisymmetric circulation and reducing the upward surface latent heat flux. Meanwhile, strong ENSO forces a summertime TNA warming via arousing the Pacific North American (PNA) teleconnection. The PNA weakens the TNA trade winds, then reduces the upward surface heat flux and consequently warms the TNA. Thus, NIO and TNA SST connection is established via ENSO events during 1980-2001. In contrast, during 2002-2020, the summertime NIO SST anomaly is still related to ENSO. However, the connection between the TNA SST anomaly and ENSO is interrupted due to the weak ENSO intensity. Such weak ENSO yields a much weaker PNA teleconnection, which is inefficient to generate the TNA warming. Further analysis shows that the TNA warming during 2002-2020 is generated mainly by the negative North Atlantic Oscillation. Therefore, the connection between NIO and TNA SST anomalies collapses under the weak ENSO condition.
AS61-A033
Initiating Tropical Pacific Decadal Variability from Off-equatorial Subsurface Temperature Anomalies
Yu-Heng TSENG1#+, Sieu Cuong SAN2, Ruiqiang DING3
1National Taiwan University, 2National Kaohsiung Marine University, 3Beijing Normal University
We demonstrate the key role of off-equatorial subsurface temperature anomalies in driving the phase transition of Tropical Pacific Decadal Variability (TPDV) using observation and model experiments. During the positive phase of TPDV, anomalous atmospheric responses in the off-equatorial northwestern Pacific induce positive Ekman pumping. The resulting negative subsurface temperature anomaly generated then propagates along the North Equatorial Countercurrent pathway towards the central basin, causing a sign reversal of the equatorial sea-surface temperature anomalies around three years later. Moreover, the positive phase of TPDV possibly changes the state of the Kuroshio Extension through tropical-extratropical interaction, which subsequently projects onto the footprint of the Pacific Meridional Mode, thereby amplifying subsurface-produced disturbance 0-12 months before the cold peak phase. The cold phase is completely established after five years. Similarly, the same dynamic applies to the reversed phase, leading to a preferred decadal oscillation driven by off-equatorial subsurface temperature anomalies and extratropical-tropical ocean-atmosphere interaction.
AS61-A041
Revisiting Dynamics for ENSO Diversity with an Extended Recharge-oscillator Model
Licheng GENG1, Fei-Fei JIN2#+
1University of Hawaii at Manoa, 2University of Hawaii
The El Niño-Southern Oscillation (ENSO) features remarkable inter-event difference in spatial patterns and is dominated by the Eastern Pacific-type and Central Pacific-type ENSO. The fundamental dynamics for such ENSO diversity has been on the frontier of ENSO research but no consensus has been reached yet. In our recent work, we proposed a generalized mechanism for ENSO diversity by understanding how a single ENSO mode leads to the two types of ENSO. More specifically, we unveiled a nonlinear pathway towards ENSO diversity paved by the deterministic routes to chaos and eased by the stochastic forcing. In this study, we aim at revisiting the nonlinear dynamics for ENSO diversity but using a low-order conceptual model. This model is analytically formulated from the Cane-Zebiak-type framework with rigorous derivation. It is in a similar form as the recharge-oscillator (RO) model but with the sea surface temperature anomaly (SSTA) variable replaced by the principal components of the two leading modes of equatorial SSTA. The model-simulated ENSO behavior well reproduces the observations in terms of ENSO diversity, asymmetry, phase locking, etc. Numerical experiments with this model confirm our previous finding that the linear ENSO mode may evolve into two types of ENSO via the period-doubling route to chaos and that the stochastic forcing allows ENSO diversity to be more readily excited. Relative contribution to ENSO diversity from each individual nonlinear process is also investigated via sensitivity experiments.
AS61-A017
Asymmetry Between Positive and Negative Phases of the Pacific Meridional Mode: A Contributor to ENSO Transition Complexity
Hanjie FAN1#+, Chunzai WANG2, Song YANG1
1Sun Yat-sen University, 2Chinese Academy of Sciences
The Pacific Meridional Mode (PMM) plays a critical role in affecting El Niño-Southern Oscillation (ENSO). This study examines the phase asymmetry of PMM events triggered by tropical and extratropical forcings, namely successive and stochastic events, respectively. It is shown that successive events exhibit negative asymmetry due to stronger trigger in the negative phase, while stochastic events display positive asymmetry due to stronger growth in the positive phase. The opposite phase asymmetry of two types of events respectively results in more frequent persistent La Niña events than El Niño events and more frequent episodic El Niño events than La Niña events, which increase ENSO transition complexity. This research provides a comprehensive understanding of PMM asymmetry and reconciles conflicting perspectives from previous studies. Additionally, the newly proposed contribution of positively asymmetric stochastic PMM events to more frequent episodic El Niño events in this study may enhance our comprehension of ENSO transition complexity.
Session Chair(s): Kun LI, Shandong University
AS20-A023
| Invited
Bayesian Inference-based Estimation of Hourly Primary and Secondary Organic Carbon at Suburban Hong Kong: Evolution Characteristics During PM2.5 Episodes
Jianzhen YU#+, Shan WANG, Kezheng LIAO
The Hong Kong University of Science and Technology
Observation-based data of primary and secondary organic carbon in ambient particulate matter (PM) are essential for model evaluation, climate and air quality research, health effects assessment, and mitigation policy development. Since there are no direct measurement tools available to quantify primary organic (POC) and secondary organic carbon (SOC) as separate quantities, their estimation relies on inference approaches using relevant measurable PM constituents. In this study, we measured hourly carbonaceous components and major ions in PM2.5 for a year and a half in suburban Hong Kong from July 2020 to December 2021. We differentiated POC and SOC using a novel Bayesian inference approach, with sulfate identified as the most suitable SOC tracer. The hourly POC and SOC data allowed us to examine temporal characteristics varying from diurnal and weekly patterns to seasonal variations, as well as their evolution characteristics during individual PM2.5 episodes. A total of 65 city-wide PM2.5 episodes were identified throughout the entire studied period, with SOC contributions during individual episodes varying from 10% to 66%. In-depth analysis of city-wide summertime typhoon episodes revealed elevated SOC levels, especially during daytime hours. High temperature and NOx levels were identified as significant factors contributing to episodic SOC formation. Winter haze episodes exhibited high SOC levels, likely due to persistent influences from regional transport originating from the northern region to the sampling site. Enhanced SOC formation was observed with the increase in nocturnal NO3 radical (represented by [NO2][O3]) under conditions of high water content and strong acidity. This suggests that aqueous-phase reactions involving NO3 radical were likely responsible for SOC formation during winter haze episodes.
AS20-A031
| Invited
Modeling Secondary Organic Aerosols in China
Jianlin HU#+
Nanjing University of Information Science & Technology
rganic aerosol accounts for a significant fraction of fine particulate matter in China. Secondary organic aerosol (SOA), which is formed in the atmosphere from gas-to-particle conversion of primary precursor volatile organic compounds (VOCs) contributes importantly to the total observed organic aerosol. To better quantify the impacts of SOA on human health and climate and to design more efficient control strategies for improving air quality in China, improved understanding of SOA is urgently needed, including its precursors, formation processes and physicochemical properties. In this talk, I will present some results our modeling studies on SOA and its important precursors. We will present a comprehensive evaluation of modeled VOCs in China. Then the impacts of oxgenated VOCs on atmospheric oxidation capacity and SOA will be discussed, the SOA formation from naphthalene will also be introduced.
AS20-A027
Modeling the Formation and Aging Process of Secondary Organic Aerosols from Two Typical Megacities of China: Results with New Observational Constraints
Weiwei HU1#+, Bin YUAN2, Wei CHEN1, Zi TAO1
1Chinese Academy of Sciences, 2Jinan University
Secondary organic aerosols can account for 10-90% of total OA in the ambient air, which impacts substantially to human health and climate change. Semi/intermediate-volatile compounds (S/IVOCs) are important precursors of SOA. However, the quantification measurement of S/IVOCs cannot be fully achieved due to their complex structure and thousands of organic species. In this study, a new method was established to estimate the S/IVOCs mass concentration based on the measured volatility distribution from different primary OA. The volatility of OA was measured using thermodenduer coupled with aerosol mass spectrometer (AMS). Then a box model coupled with Volatility Bin Set (VBS) module was used to simulate the SOA formation from S/IVOCs and volatile organic compounds (VOCs) at urban areas of Megacity Guangzhou and Beijing. The effect of oxidation mechanisms, aging rate, and fragmentation on SOA production, as well as phase separation was explored and evaluated with observation data to restrict the model. The optimum simulation shows that S/IVOC oxidation contributes 51~62% to SOA, where the VOCs contribute the rest and was mainly contributed by anthropogenic sources. The detailed fossil and non-fossil contributions from different sources were also simulated. Secondary sources can explain two-third of both fossil and non-fossil carbons in total OA. Finally, the oxidation state of OA was found to be underestimated based on the current parameterization in the box model which shall be further improved. Our study promotes the understanding of S/IVOCs quantification and their contribution to SOA formation in Chinese urban areas.
AS20-A030
Characterization of Organonitrate in PM1 in Urban and Rural PRD: Insights from Non-refractory and Refractory Organics Detected by a Soot Particle Aerosol Mass Spectrometer (SP-AMS)
Shan HUANG#+
Jinan University
Particulate organonitrates (pON) are a key organic constituent of submicron particulate matter as they may contribute significantly to nighttime formation of secondary organic aerosols (SOA) and also act as a temporary reservoir of reactive nitrogen then indirectly affecting ozone production. Atmospheric organonitrates were characterized based on the field campaigns at urban and rural sites in the Pearl River Delta (PRD) region, China, during autumn when the region often suffered complex air pollution of ozone and particulate matters. A soot particle time of flight aerosol mass spectrometer (SP-AMS) was deployed to provide detailed chemical composition of ambient aerosols in high-time and mass resolution. The pON was quantified by positive matrix factorization (PMF) method and validated by intercomparisons with the results from the other method or instrument. The pON showed slightly higher mass concentration in rural site than that in urban site, while the proportions of organonitrates in total nitrates were close to each other at both sites (19% for urban and 17% for rural). The pON at the urban site generally formed at daytime, including photo-oxidation processes (contributing 16% of total pON mass concentration) and regional transport (33%), in the contrary, nighttime formation (29%) was more significant at the rural site for pON. Biomass burning-related emissions acted as an important source of organonitrates at both sites, providing 25% in the urban area and 34% in the rural region. Based on the calculated organonitrate production potential of different volatile organic compounds (VOCs), biogenic VOCs were dominating organonitrate precursors in both sites, while anthropogenic VOCs such as styrene and cresol were important to organonitrate formation especially in rural nighttime. Moreover, nighttime pON showed pronouncedly positive correlation (R = 0.62~0.76) with the atmospheric oxidants Ox (O3+NO2) in the next morning, suggesting pON might contribute to next-day atmospheric oxidation capacity.
AS20-A035
Theoretical Study of the Iodine Oxoacids-driven Nucleation
Fangfang MA1+, Rongjie ZHANG1, Hongbin XIE1#, Xu-Cheng HE2
1Dalian University of Technology, 2University of Helsinki
Iodine oxoacids (HIO3 and HIO2)-driven nucleation has been suggested to efficiently contribute to new particle formation in marine atmospheres. However, the knowledge of which atmospheric vapors can enhance Iodine oxoacids-driven nucleation remains limited, hindering understanding of their contribution to the formation of new particles in the marine atmospheres. Here, we propose the following research ideas: revealing iodine oxoacids-driven nucleation mechanisms - constructing a high-throughput prediction model for predicting the enhancing potential (EP) of precursors - identifying the highest EP precursor. We firstly investigated the formation mechanisms and kinetics of the HIO3-HIO2 system with theoretical methods. The results showed that HIO2 has strong halogen bond (XBs) forming ability and exhibiting a base behavior when interacting with HIO3, resulting in a high nucleation rate of the HIO3-HIO2 system. Based on the understanding of the mechanism, we inferred that many compounds such as organic acids, amines, etc. could interact with iodine oxoacids and enhancing their nucleation via hydrogen bonds (HBs), XBs and acid-base reactions. Therefore, we calculate the formation free energy (ΔG) values of the dimer clusters for selected compounds with HIO3 or HIO2. Combined both the calculated ΔG and atmospheric concentration of considered precursors, the EP of precursors were evaluated and two quantitative structure-activity relationship (QSAR) model were constructed. It was found that sulfur oxoacids (methanesulfonic acid (MSA) and sulfuric acid (SA)) have the highest EP for HIO3-HIO2-driven nucleation. In addition, although atmospheric bases yield high potential to enhance HIO3-induced nucleation, they present almost a negligible role in HIO2-driven nucleation. By further investigating the larger SA/MSA-HIO3-HIO2 clusters, we found that sulfur oxoacids can participant and enhance HIO3-HIO2 driven nucleation in the realistic marine atmosphere. Additionally, HIO3-HIO2 is an efficient enhancer for sulfur oxoacids-driven nucleation in the marine atmosphere.
AS20-A001
Unveiling the Seasonal Dynamics of Brown Carbon Aerosols in the Asian Outflow Region
Chunmao ZHU1#+, Takuma MIYAKAWA1, Fumikazu TAKETANI1, Dhananjay DESHMUKH2, Bhagawati KUNWAR3, Kimitaka KAWAMURA2, Yugo KANAYA1
1Japan Agency for Marine-Earth Science and Technology, 2Chubu University, 3Hokkaido University
Secondary organic aerosols (SOA), formed from the atmospheric transformation of gaseous precursors, significantly impact climate and air quality. Brown carbon (BrC), a light-absorbing fraction of primary organic aerosols and SOA, plays a crucial role in radiative forcing. However, understanding its formation mechanisms under complex, polluted environments remains a challenge. In this study, we investigated the seasonal dynamics and source-specific contributions to BrC formation in the Asian outflow region, focusing on Fukue Island, a gateway from the Asian continent to the North Pacific. We found that BrC levels exhibit distinct seasonal variations, peaking during winter-spring when influenced by air masses carrying emissions from Asian sources. Water-soluble BrC formation shows a strong association with a specific marker for fossil fuel combustion, suggesting its significant influence during these seasons. Biomass burning emissions, as indicated by another marker, contribute to BrC formation, particularly in spring. A distinct fraction of BrC, soluble in methanol, is more prevalent in summer, hinting at potential contributions from additional sources such as local biogenic emissions present in air masses from this period. This study sheds light on the seasonal dynamics and diverse sources of BrC in the Asian outflow region, even under generally clean atmospheric conditions. Our findings highlight the role of both anthropogenic and biogenic precursors, as well as potentially unique formation processes occurring in less polluted environments. This knowledge contributes to a better understanding of the complex factors influencing BrC formation and its implications for regional climate and air quality.
AS20-A022
Evaluation of a New Real-time Source Apportionment System of PM2.5 and Its Implication on Rapid Aging of Vehicle Exhaust
Pei-Ting YAO1+, Xing PENG1, Liming CAO1, Qiao ZHU2, Liwu ZENG1, Ning FENG1, Ling-Yan HE1, Xiaofeng HUANG1#
1Peking University Shenzhen Graduate School, 2Emory University
Accurate identification and rapid analysis of PM2.5 sources and formation mechanisms are essential to mitigate PM2.5 pollution. However, studies were limited in developing a method to apportion sources to the total PM2.5 mass in real-time. In this study, we developed a real-time source apportionment method based on chemical mass balance (CMB) modelling and a mass-closure PM2.5 composition online monitoring system in Shenzhen, China. The novel methods were verified by comparing with other source apportionment methods, including offline filter analysis, aerosol mass spectrometry, and carbon isotopic analysis. The comparison of these methods showed that the new real-time method obtained results generally consistent with the others, and the differences were interpretable and implicative. Secondary organic aerosol (SOA) and vehicle emissions were the major PM2.5 and OA contributors by all methods. Further investigation on the OA sources indicated that vehicle emissions were not only the main source of primary organic aerosol (POA), but also the main contributor to SOA by rapid aging of the exhaust in the atmosphere. Our results demonstrated a great potential of the new real-time source apportionment method for aerosol pollution control and deep understandings on emission sources.
Session Chair(s): Huiling YUAN, Nanjing University
AS86-A010
| Invited
A New Approach to Represent Model Uncertainty in Forecasting Tropical Cyclones: The Orthogonal Nonlinear Forcing Singular Vectors
Wansuo DUAN1#+, Yichi ZHANG2, Stéphane VANNITSEM3, Han ZHANG2
1Institute of Atmospheric Physics, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Royal Meteorological Institute of Belgium
Tropical cyclone (TC) track forecasting has been considerably improved in recent decades, while TC intensity forecasting remain challenging. In this study, orthogonal nonlinear forcing singular vectors (O-NFSVs) for emulating the impact of model uncertainties are used to conduct TC ensemble forecasting experiments with the Weather Research and Forecasting (WRF) model, with a focus on improving TC intensity forecasting skill. The O-NFSVs approach is compared with the traditional stochastic kinetic-energy backscatter (SKEB) and stochastically perturbed parametrization tendency (SPPT) schemes. The results demonstrate that the O-NFSVs ensembles generally provide a better representation of the model uncertainties affecting TC intensification, with much better deterministic and probabilistic skills. These results also extend to the ability to forecast TC track, although the perturbations have not been optimized for that specific purpose. The O-NFSVs are therefore appropriate perturbation structures for describing the uncertainties of the TC intensity and track forecasting and are also favourable for recognizing the rapid intensification process.
AS86-A011
| Invited
The Importance of Data Assimilation Components for Initial Conditions and Subsequent Error Growth
Lili LEI#+
Nanjing University
Despite a specific data assimilation method, data assimilation (DA) in general can be decomposed into components of the prior information, observation forward operator that is given by the observation type, observation error covariances, and background error covariances. In a classic Lorenz model, the influences of the DA components on the initial conditions (ICs) and subsequent forecasts are systematically investigated, which could provide a theoretical basis for the design of DA for different scales of interests. The forecast errors undergo three typical stages: a slow growth stage from 0 h to 5 d, a fast growth stage from 5 d to around 15 d with significantly different error growth rates for ensemble and deterministic forecasts, and a saturation stage after 15 d. Assimilation strategies that provide more accurate ICs can improve the predictability. Cycling assimilation is superior to offline assimilation, and a flow-dependent background error covariance matrix (Pf) provides better analyses than a static background error covariance matrix (B) for instantaneous observations and frequent time-averaged observations; but the opposite is true for infrequent time-averaged observations, since cycling simulation cannot construct informative priors when the model lacks predictive skills and the flow-dependent Pf cannot effectively extract information from low-informative observations as the static B. Instantaneous observations contain more information than time-averaged observations, thus the former is preferred, especially for infrequent observing systems. Moreover, ensemble forecasts have advantages over deterministic forecasts, and the advantages are enlarged with less informative observations and lower predictive-skill model priors.
AS86-A014
Impacts of Precipitation Uncertainty on Hydrological Ensemble Simulations Over the Ganjiang River Basin
Huiling YUAN1#+, Xiao HAN2
1Nanjing University, 2Chongqing Meteorological Observatory
This study evaluates three quantitative precipitation estimates (QPEs) over the Ganjiang River basin, namely the China Gauged-Based Daily Precipitation Analysis (CGDPA) data, the Precipitation Estimation from Remotely Sensed Information using Artificial Neural Networks-Climate Data Record (PERSIANN-CDR) data, and the Asian Precipitation - Highly-Resolved Observational Data Integration Towards Evaluation of Water Resources (APHRODITE). The study also investigates the impacts of precipitation uncertainty on hydrological ensemble streamflow simulations using the three QPEs as precipitation inputs of the Variable Infiltration Capacity (VIC) distributed hydrological model. New hydrological insights for the region: APHRODITE underestimates precipitation compared to CGDPA, while PERSIANN-CDR shows greater spatiotemporal variability. The ensemble mean streamflow demonstrates greater improvement compared to the results obtained from a single parameter set. Among the three QPEs, the simulations forced by CGDPA show the best deterministic and probabilistic verification scores, followed by APHRODITE. PERSIANN-CDR tends to underestimate evaporation and leads to the lowest score of ensemble streamflow simulations, but shows advantages in simulating extremely low streamflow. The study highlights that high-density gauge-based QPEs remain the most accurate source of precipitation inputs for reliable hydrological simulations, while satellite-gauge merged QPEs can provide valuable inputs for hydrological simulations over the basins where meteorological stations are scarce. References: Han, X., H. Yuan*, 2024: Impacts of precipitation uncertainty on hydrological ensemble simulations over the Ganjiang River basin. Journal of Hydrology: Regional Studies, 51, 101617. https://doi.org/10.1016/j.ejrh.2023.101617.
AS86-A013
Comparison of the ENSO-EASM Relationship in Paleoclimate Proxies and CMIP6 Ensemble Models
Sandro F. VEIGA#+, Yesi ZHAO, Huiling YUAN
Nanjing University
In this study, we investigate the connection between the El Nino Southern Oscillation (ENSO) and the East Asian Summer Monsoon (EASM) simulated by an ensemble of climate models from CMIP6 and evaluate these simulations using the relationship between ENSO-EASM given by paleoclimate proxies. We used a dataset with 300 years and the PiControl climate simulations with the same length. The evaluation is performed by comparing the proxy system modeling given by the proxy dataset and the proxy system modeling given by the models. To account for the different capabilities of climate models in simulating the ENSO-EASM relationship, we applied the weighting scheme to an ensemble of models and obtained weighted proxy system modeling for the ensemble. The weighted ensemble proxy system modeling is compared with the observed proxy system modeling to show the uncertainty reduction provided by this sort of methodology.
AS86-A008
Evaluation and Comparison of the Predictability of the CFS and GEFS Operational Systems at NCEP for Sub-seasonal Forecasts
Yanru YANG#+, Jie FENG
Fudan University
Sub-seasonal predictions, ranging from several weeks to a season, play a vital role in facilitating seamless weather and climate forecasting. A major challenge in sub-seasonal predictions is the inherent complexity of forecasting subject to simultaneous influences from multiple sources of uncertainty in initial and boundary conditions. To address these issues, extensive exploration has been made in research and operation. Since 2011, the Climate Forecast System, version 2 (CFSv2) - a fully coupled atmosphere-ocean-land-sea-ice model - has replaced its predecessor at NCEP, covering the sub-seasonal forecasts up to 45 days. Acknowledging the growing significance of sub-seasonal timescale predictions, the Global Ensemble Forecast System (GEFS) has evolved from its original focus on medium-range ensemble forecasts. The latest iteration, GEFS version 12 (GEFSv12), extends its forecast lead time from 16 to 35 days. Also, GEFSv12 updated the SST, however, with the varying SST obtained from CFSv2 (i.e., a “two-tiered” method) to simulate a one-way forcing from ocean. Despite sharing a common objective of enhancing sub-seasonal prediction accuracy, CFSv2 and GEFSv12 exhibit notable distinctions in their atmospheric model configuration and the handling of air-sea coupling. Quantitative evaluations and comparisons of these two systems, particularly concerning their practical limits in sub-seasonal forecast predictability, remain relatively scarce. In this work, we evaluate and compare the temporal mean and spatial distribution of sub-seasonal predictability limit of CFSv2 and GEFS for variables like temperature, zonal wind, and geopotential height at various vertical levels. The first part of our research entails an in-depth analysis of the limits of subseasonal predictability in the tropics and extratropics using 5-day time averaging. This is followed by an examination of the results based on grid-point fields with Gaussian filtering and 5-day time averaging in these two subseasonal forecast systems. Finally, we quantified the impact of bias correction on these evaluations.
AS86-A012
Improving the Forecasting of El Nino Amplitude Based on an Ensemble Forecast Strategy for Westerly Wind Bursts
Chaopeng JI1#+, Mu MU1, Xianghui FANG1, Lingjiang TAO2
1Fudan University, 2Nanjing University of Information Science & Technology
The forecasting of El Niño amplitude remains uncertain, with false alarms or underestimations often occurring. It has been suggested that westerly wind bursts (WWBs) are crucial atmospheric stochastic forcing that affects the development, amplitude, and predictability of El Niño. Effectively capturing the influence of WWBs in El Niño forecasting systems to mitigate El Niño forecast uncertainties continues to be a widely discussed topic. In this work, two El Niño ensemble forecast scenarios incorporating WWBs were devised utilizing an intermediate coupled model capable of simulating the rational features of El Niño–Southern Oscillation and a refined WWBs parameterization scheme. To start with, both the seasonal variations and the dependence on the oceanic background state were considered to improve the parameterization of WWBs. Furthermore, considering the short intrinsic predictability limit of WWBs with respect to the interannual scale of El Niño evolution, a WWBs ensemble forecast strategy was designed to obtain their occurrence probability and the statistical features of their magnitude and central location. With this in mind, an ensemble forecast of El Niño events occurring during 1979-2021 based on WWBs ensemble forecast was established (termed WWBs-based). For comparison, a conventional El Niño ensemble forecast based on initial conditions (ICs) perturbations was also conducted (termed ICs-based). Results indicated that the WWBs-based approach shows better performance in forecasting the El Niño amplitude than the ICs-based one. The present approach suggests indicates an ensemble forecast with proper consideration of the scale interaction between the fast WWBs and interannual variations is more physically consistent.
AS86-A009
Are RMSE and ACC Sufficient to Determine a Good Forecast?
Jie FENG#+
Fudan University
The Root-Mean-Square Error (RMSE) and Anomaly Correlation Coefficient (ACC) are widely utilized in the verification and evaluation of forecast performance globally. Numerous studies have relied on these metrics to assess the efficacy of forecast systems and methodologies. However, this reliance raises a critical question: Are RMSE and ACC sufficient to determine a forecast? Our review of the literature and theoretical analysis leads us to a negative response. Additionally, we introduce a novel composite metric – 'predictive information' – for enhanced forecast verification. An evaluation using operational forecast data reveals that this predictive information metric offers a more comprehensive assessment of forecasting performance compared to the traditional use of RMSE and ACC alone. Further detailed reasoning supporting this conclusion is also provided.
Session Chair(s): Ja-Yeon MOON, IBS Center for Climate Physics, Chihiro KODAMA, Japan Agency for Marine-Earth Science and Technology
AS53-A009
Future Climate Projections from the Global KM-scale Earth System Simulations
Sun-Seon LEE1#+, Ja-Yeon MOON1, Axel TIMMERMANN2, Jan STREFFING3, Tido SEMMLER3, Thomas JUNG3
1IBS Center for Climate Physics, 2Pusan National University, 3Alfred Wegener Institute
Due to large uncertainties of climate projections on regional scales, assessing the future risk of natural disasters, ensuring sustainable energy and water resources, and developing climate change adaption strategies still remains a daunting task. Recent efforts to tackle this issue include km-scale (cloud permitting/storm resolving) coupled climate model simulations which resolve atmosphere and ocean mesoscale processes and their interactions with the large-scale environment and small-scale topographic features. Here, we present the first results from a series of global coupled 9 km-scale greenhouse warming simulations conducted with the AWI Climate Model version 3 (OpenIFS atmosphere model in TCO1279 resolution and 137 levels coupled to FESOM2 ocean model in 4-15 km resolution). By comparing a set of consecutive 10-year time-slice simulations forced by the SSP585 greenhouse gas emission scenario with a transient simulation at lower-resolution version (31 km atmosphere resolution), we identify key differences in weather and climate-related phenomena, including tropical cyclones, ENSO and regional warming patterns that can be attributed to km-scale dynamics in clouds and atmospheric circulation patterns. The findings from our cloud-permitting climate simulations provide valuable insights into the role of small-scale processes in regional and global climate sensitivity.
AS53-A010
Cloud-feedback with Kilometer-scale Global Warming Simulations
Ja-Yeon MOON1#+, Sun-Seon LEE1, Axel TIMMERMANN2, Jan STREFFING3, Tido SEMMLER3, Thomas JUNG3
1IBS Center for Climate Physics, 2Pusan National University, 3Alfred Wegener Institute
Clouds play a crucial role in regulating the Earth's radiation balance. As a result, changes in clouds and their corresponding feedback are likely to have a significant impact on global climate sensitivity. However, the response of clouds to greenhouse warming on both global and regional scales is not yet well understood. We are presenting first results from a kilometer-scale, cloud-permitting greenhouse warming simulation conducted with the coupled OpenIFS-FESOM2 model (AWI-CM3) in ~9 km atmosphere resolution, 137 vertical levels and 4-15 km variable ocean resolution. Our analysis is based on a set of 10-year time-slice simulations that were branched off from a lower-resolution (31 km) SSP585 transient scenario run with relatively high climate sensitivity. We will examine how atmosphere resolution and cloud granularity impact cloud radiative feedback. Additionally, we will present the results of radiative kernel calculations to determine the role of high cloud feedback in polar amplification.
AS53-A011
Accelerated Future Marine Heatwave Intensification in Marine Protected Areas
Eun-Byeol CHO1#+, Axel TIMMERMANN2, Eun Young KWON1
1IBS Center for Climate Physics, 2Pusan National University
Marine Protected Areas (MPAs) are designated zones for the conservation of marine ecosystems; yet they remain exposed to increasing ocean temperature. Particularly, extreme warming events known as Marine Heatwaves (MHWs) can exert detrimental effects on the marine ecosystems in the MPAs. Understanding future changes in MHWs in the MPAs requires high resolution climate modeling which is capable of resolving regional bathymetric features in MPAs, such as coastlines, continental shelfs or islands. In this study, we utilized the SSP585 greenhouse warming simulations conducted with the OpenIFS-FESOM2 coupled model (AWI-CM3, 31 km atmosphere resolution, 4-15 km ocean resolution) to explore future changes in MHWs in the epipelagic to the upper mesopelagic zones (0-300m depth) of the global MPAs. For present-day climate, MHWs in the MPAs show stronger maximum intensity and are more frequent compared to the global averages. Yet the duration of MHWs is shorter in the MPAs, resulting in a lower cumulative intensity. We also find that the warming rates within the MPAs are similar or slightly lower than the averaged warming rate of the global ocean. However, in response to future warming the cumulative intensities of MHWs are projected to increase 20% more in the MPAs than the global ocean. This implies that, MPAs will be more exposed to extreme temperature rise compared to other regions. Our results underscore the importance of mitigating anthropogenic warming for the conservation of MPAs, providing a rationale for urgent actions to reduce such impacts and preserve these critical marine ecosystems.
AS53-A012
| Invited
Coupled Atmosphere-sea-ice-ocean Feedback Accelerates Rapid Sea Ice Decline in Weddell Sea in High-resolution Global Climate Model
Dae-Won KIM1#+, Thomas JUNG2, Navajyoth PUTHIYAVEETTIL1,3, Wonsun PARK3, Tido SEMMLER2, Axel TIMMERMANN3, Martina ZAPPONINI2
1IBS Center for Climate Physics, 2Alfred Wegener Institute, 3Pusan National University
Sea ice extent around the Antarctic exhibits a high level of variability on interannual and longer timescales, characterized by a positive trend since the satellite era and interruptions due to e.g., the emergence of the Maud Rise Polynya in 2016. Given the relatively short period of observational data and the high level of natural variability, it has remained challenging to unequivocally identify the anthropogenic fingerprint in Antarctic sea ice. Moreover, to properly study the Antarctic sea ice and its response to future warming, it is necessary to capture important dynamics, such as polynyas, the Antarctic slope current, and coastal leads. Many models within the CMIP6 model portfolio do not even have the spatial resolution to adequately resolve these features. This implies that their Antarctic projections may not be as trustworthy and robust as those for the Arctic Ocean. In this study we employ the high-resolution OpenIFS-FESOM (AWI-CM3) coupled general circulation (nominally 30 km atmosphere and 4-25 km ocean resolutions) to investigate the Antarctic sea ice response to greenhouse warming, following a SSP5-8.5 greenhouse gas emission scenario. Our simulation exhibits a sudden decline of Antarctic sea ice in the Weddell Sea (WS) which can be explained by a combination of physical processes that involve continued strengthening of westerlies, increased atmosphere-ocean momentum transfer due to sea ice decline, a spin-up of the Weddell-Sea Gyre and slope current and corresponding vertical and horizontal supply of heat into the Weddell Sea. The resulting decrease of sea ice further leads to heat accumulation in austral summer due to the absorption of short-wave radiation, which can further weaken winter sea ice extent and intensify the momentum transfer and associated heat transport into the Weddell Sea gyre. Our study highlights the relevance of positive atmosphere-sea ice-ocean feedbacks in triggering the abrupt decline in Antarctic sea ice.
AS53-A001
Diurnal Cycle Simulation of Precipitation Over Land with the YUNMA Model
Xindong PENG1,2#+, Yifan ZHAO3, Siyuan CHEN4, Xiaohan LI4
1CMA Earth System Modeling and Prediction Centre, 2CMA Earth System Modeling and Prediction Centre, 3Chinese Academy of Meteorological Sciences, 4PIESAT Information Technology Co., Ltd.
A global-reginal-unified atmospheric model, Yin-Yang-grid Unified Model for the Atmosphere (YUNMA), was used to simulate the diurnal cycle of precipitation over land surface with the help of the new simplified Arakawa-Schubert (NSAS) scheme. The YUNMA model was designed for high-performance computing on many-core computer systems, which achieved an actual speedup rate of 90.65% in a 1600-core parallel computing test of the dynamical core. The NSAS was tested firstly with two new diagnostic closures and a convective trigger function to emphasize the cloud work function corresponding to the free tropospheric large-scale forcing in the YUNMA model. The revised trigger function was effective to improve the diurnal cycle of precipitation in comparison with the two closures in one-month simulating test. Consequently, three-month batched real-case simulations were carried out with the 0.25-degree model. Numerical results revealed the improvement of diurnal precipitation variation by using the revised trigger function with an enhanced dynamical constraint on the convective initiation and a suitable threshold of the trigger. By reducing the occurrence of convection during peak solar radiation hours, the revised scheme was demonstrated to be helpful in delaying the appearance of early-afternoon rainfall peaks over most land areas and accentuating the nocturnal peaks that were wrongly concealed by the more substantial afternoon peak. In addition, the revised scheme enhanced the simulation capability of the precipitation probability density function, such as increasing the extremely low- and high-intensity precipitation events and decreasing small and moderate rainfall events, which contributed to the reduction of precipitation bias over mid-latitude and tropical lands.
AS53-A014
| Invited
Impact of Horizontal Resolution on Medium-range Prediction of Korean Integrated Model
Eun-Hee LEE1#+, Jiyoung JUNG1, Sujeong CHO1, Ji-Young HAN1, Raeseol PARK1, Suk-Jin CHOI2, Hyun NAM1, Ja-Rin PARK1, Youngsu LEE1, Junghan KIM1, Heeje CHO1, Ilseok NOH1
1Korea Institute of Atmospheric Prediction Systems, 2Gangneung-Wonju National University
The Korean Integrated Model (KIM) was developed for the operational global predictions at ~10 km resolution in 2019 by the Korea Institute of Atmospheric Prediction Systems (KIAPS) project. The second phase of the KIAPS project, initiated in 2020, has focused on developing a high-resolution KIM targeting a km-scale model. Recently, a semi-operational update has been conducted, reducing the resolution from 12 km to 8 km. In this study, we review the history of horizontal resolution updates of KIM in the KIAPS projects, and evaluate the benefits of resolution increase in terms of prediction performance. The impact of horizontal resolution on medium-range prediction is investigated from 100 km to 8 km, which is conducted on the cold-run testbed without data assimilation. Special focus is given to the performance improvement between 12 km and 8 km, which is further tested on a year-round testbed of semi-real-time operation, including data assimilation. This encompasses the model’s capability to predict high-impact weather events such as typhoons, and heatwaves affecting South Korea. We also discuss the sensitivity of the scale-aware function in physics schemes to horizontal resolution, which might be removed or relaxed for consistent improvement of predictability, with special concerns about the current development strategy toward km-scale prediction. Finally, a current status of the KIAPS project in km-scale NWP development is introduced in this presentation, which includes fixed- and variable-resolution approaches.
AS53-A007
| Invited
Global Simulations of the Atmosphere with Kilometer to a Few Hundred Meters Grid Spacing
Shuhei MATSUGISHI1#+, Tomoki OHNO1, Masaki SATOH1,2
1The University of Tokyo, 2Yokohama National University
We conducted a global atmospheric simulation with a 220m mesh and additional simulations involving various resolutions using a global cloud-resolving model called NICAM (Satoh et al., 2014). We compare the mean states of simulations and the representation of global convective activity among several resolutions. The resolution ranging from kilometers to sub-kilometers is called a gray zone (Honnert et al., 2020) for the turbulence parameterization used in atmospheric models, which is the boundary between Reynolds Averaged Navier-Stokes (RANS) models and Large Eddy Simulation (LES) models. Therefore, we conducted experiments using MYNN (Nakanishi and Nino 2004), a RANS scheme, and Smagorinsky scheme, an LES scheme, respectively and compared them. A global 220m NICAM simulation was performed by using 81920 nodes on Supercomputer Fugaku. We investigate the dependence of the large-scale state on resolution. The zonal mean humidity and precipitation distribution do not change significantly. A decrease in the lower cloud is noticeable for increasing resolution. The distribution of precipitation is noteworthy: very weak rainfall, such as drizzle with less than 1 mm/hr, is reduced. However, when we focus on rainfall distribution over 1 mm/hr, weak rainfall increases with higher resolution, and the weak rainy area expands. Coarse-grained rainfall distribution is smoother in the sub-km model than in the km model. Differences in turbulence schemes significantly affected cloud reproducibility. We discuss where the km-scale model is well resolved and where it is inadequate from our simulations.
AS53-A004
Establishing a Non-hydrostatic Global Atmospheric Modeling System (iAMAS) at 3-KM Horizontal Resolution with Aerosol Feedbacks on the Sunway Supercomputer of China
Chun ZHAO#+, Jiawang FENG, Jun GU
University of Science and Technology of China
During the era of global warming and highly urbanized development, extreme and high impact weather as well as air pollution incidents influence everyday life and might even cause the incalculable loss of life and property. Although, with the vast development of atmospheric model, there still exists substantial numerical forecast biases objectively. To predict accurately extreme weather, severe air pollution, and abrupt climate change, the numerical atmospheric model requires not only to simulate meteorology and atmospheric compositions simultaneously involving many sophisticated physical and chemical processes but also at high spatiotemporal resolution. Global integrated atmospheric simulation at spatial resolutions of a few kilometers remains challenging due to its intensive computational and input/output (I/O) requirement. Through multi-dimension-parallelism structuring, aggressive and finer-grained optimizing, manual vectorizing, and parallelized I/O fragmenting, an integrated Atmospheric Model Across Scales (iAMAS) was established on the new Sunway supercomputer platform to significantly increase the computational efficiency and reduce the I/O cost. The global 3-km atmospheric simulation for meteorology with online integrated aerosol feedbacks with iAMAS was scaled to 39,000,000 processor cores and achieved the speed of 0.82 simulation day per hour (SDPH) with routine I/O, which enabled us to perform 5-day global weather forecast at 3-km horizontal resolution with online natural aerosol impacts. The results demonstrate the promising future that the increasing of spatial resolution to a few kilometers with online integrated aerosol feedbacks may significantly improve the global weather forecast.
AS53-A002
Developing an Explainable Variational Autoencoder (VAE) Framework for Accurate Representation of Local Circulation in Taiwan
Min-Ken HSIEH#+, Chien-Ming WU
National Taiwan University
This study develops an explainable variational autoencoder (VAE) framework to efficiently generate high-fidelity local circulation patterns in Taiwan, ensuring an accurate representation of the physical relationship between generated local circulation and upstream synoptic flow regimes. Large ensemble semi-realistic simulations were conducted using a high-resolution (2 km) model, TaiwanVVM, where critical characteristics of various synoptic flow regimes were carefully selected to focus on the effects of local circulation variations. The VAE was constructed to capture essential representations of local circulation scenarios associated with the lee vortices by training on the ensemble dataset. The VAE's latent space effectively captures the synoptic flow regimes as controlling factors, aligning with the physical understanding of Taiwan's local circulation dynamics. The critical transition of flow regimes under the influence of southeasterly synoptic flow regimes is also well represented in the VAE’s latent space. This indicates that the VAE can learn the nonlinear characteristics of the multiscale interactions involving the lee vortex. The latent space within VAE can serve as a reduced-order model for predicting local circulation using synoptic wind speed and direction. This explainable VAE ensures accurate predictions of the nonlinear characteristics of multiscale interactions between synoptic flows and the local circulation induced by topography, thereby accelerating the assessments under various climate change scenarios.
AS53-A008
Optimization, Translation, and Transformation of an Atmospheric Model to Utilize GPUs: A Case of NICAM
Hisashi YASHIRO1#+, Kazuya YAMAZAKI2, Takashi ARAKAWA2, Shuhei MATSUGISHI2, Shereo INTYISYAR1, Kengo NAKAJIMA2
1National Institute for Environmental Studies, 2The University of Tokyo
About 30% of the machines currently listed in the TOP500 are equipped with accelerators such as GPUs. These accelerators maintain higher energy efficiency than traditional CPUs and offer cost-effective computational resources. To secure more computational resources for weather/climate simulations, utilizing supercomputers equipped with many accelerators is necessary. We present the results of applying several strategies to utilize GPUs to a non-hydrostatic icosahedral atmospheric model (NICAM, Satoh et al., 2014). 1) We performed GPU porting of the full application using the OpenACC directive and evaluated the computational performance. In this directive-based optimization, there were several patterns to avoid deterioration in calculation speed. 2) The main kernels extracted from dycore were rewritten from Fortran to Python. Writing in Python makes it easy to use backend libraries that use GPUs. 3) Data-driven model components were created by learning the calculation results based on the physical model. Such a model can be interpreted as a transformation from conventional algorithms that have reached their speed limit on modern machine architectures to algorithms that are more suitable for calculations on GPUs.
Session Chair(s): Shovan Kumar SAHU, Meteorological Service Singapore
AS12-A029
Validating a Deep Learning Approach for Weekly Rainfall Anomaly Forecasting: A Case Study in Upper Thailand with Diverse Climate Features
Jakrapop AKARANEE+, Kritanai TORSRI#, Apiwat FAIKRUA, Pattarapoom PEANGTA, Rati SAWANGWATTANAPHAIBUN , Nithiwat SINPHATTHAKUL
Ministry of Higher Education, Science, Research and Innovation
Weekly forecasting is essential, offering a more detailed understanding of rainfall patterns and enabling timely responses to risks and opportunities. Although deep learning methods show promise, their application to weekly rainfall anomaly forecasting presents specific challenges. Addressing these challenges involves capturing complex temporal dependencies and designing models capable of understanding and predicting intricate patterns in climate features. This study utilizes daily rainfall data from the Thai Meteorological Department spanning 1982 to 2015, covering 63 stations in upper Thailand, along with 11 renowned climate indexes (features) influencing Thailand’s climate patterns at various time scales including Madden-Jullian Oscillation (MJO), monsoons, Indian Ocean Dipole (IDO), and El Niño-Southern Oscillation (ENSO). Three sets of climate features were devised: SET-01 incorporates all 11 features as a control run, while SET-02 and SET-03 involve distinct features determined through stepwise selection. SET-02 focuses primarily on MJO activities, while SET-03 is similar to SET-02 but includes considerations for Indian summer monsoon influence. A 20-60 day bandpass filtering was employed on the daily rainfall with different window sizes, up to an 84-day window size for data engineering preparation prior to input into a bi-directional long term memory (Bi-LSTM) network. Our result suggest that prediction skill of the model trained with climate features of SET-02 and SET-03 can be extended up to 5 weeks (with a 35-day window size) with the high temporal correlation of 0.95, 0.88, 0.81, 0.68, and 0.52 and with lowest mean absolute error of 0.57, 0.89, 1.12, 1.42, and 1.63 mm for forecasted week-1, 2, 3, 4, and 5, respectively. This finding presents an alternative approach with a potential set of climate drivers for weekly rainfall forecast in Thailand. Such insights may prove beneficial in key sectors, e.g., water resource management at S2S time scale.
AS12-A030
Machine Learning-based Satellite Retrieval for Enhanced Ground-level NH3 Estimation
Saman MALIK#+, Eunjin KANG, Dongjin CHO, Jungho IM
Ulsan National Institute of Science and Technology
Ammonia (NH3) stands as a pivotal alkaline atmospheric pollutant, primarily originating from agricultural and industrial sources, having significant impacts on both environment and human health. The growing global demand for food and industrial products necessitates a comprehensive understanding of NH3 distribution at fine spatial and temporal scales. However, the sparse distribution of current NH3 monitoring sites globally, coupled with substantial data gaps even in established sites, presents a challenge. To address this gap, satellite remote sensing offers a promising solution. However, the significant variance in spatiotemporal scales between satellite and ground-based measurements complicates the task. In this study, we have used Infrared Atmospheric Sounding Interferometer (IASI) NH3 column products in conjunction with ground-based observations collected from the Ammonia Monitoring Network (AMoN). ERA5 reanalysis data was also incorporated to analyze the influence of external factors on NH3 estimation and distribution. XGBoost was used to estimate ground NH3 concentrations over the United States from 2018 to 2022 at 12km which is finest spatial resolution among all study variables. Significantly, our model exhibits better performance, offering improved spatial and temporal resolution. Beyond conventional applications, we investigated the impact of the COVID-19 pandemic on NH3 concentrations, providing insights into the effectiveness and consistency of our retrieval method with theoretical research. The findings highlight the potential of machine learning approaches in addressing data gaps, paving the way for enhanced NH3 estimation in diverse geographical regions. This study serves as a foundational exploration, advocating for the widespread application of machine learning in NH3 estimation globally. By facilitating continuous and fine-scale observation of NH3 trends, our approach contributes to the efficacy of global NH3 emission monitoring initiatives.
AS12-A033
PM2.5 Prediction Model Using Low-cost Air Sensors Via Machine Learning Techniques
Yi Ming LEE1+, Guan-Yu LIN2, Jhih-Yuan YU3, Chuen-Jinn TSAI1#
1National Yang Ming Chiao Tung University, 2Tunghai University, 3Ministry of Environment
Low-cost sensors (LCS) network is widely used to improve the resolution of spatial-temporal distribution of air pollutant concentrations in urban areas. However, studies on air pollution sources contribution to the microenvironment, especially in industrial and mix-used housing areas, still need to be completed. This study investigated the spatial-temporal distribution and source contributions of PM2.5 in the urban area based on 6 months of the LCS network datasets coupled with machine learning techniques. The Artificial Neural Network (ANN) was used to calibrate the measured PM2.5 by the LCS network. The calibrated PM2.5 was shown to agree with PM2.5 measured by the reference instrument with R2 of 0.85, MNE of 30.91%, and RMSE of 3.73 μg/m3, which meet the criteria for hotspot identification and personal exposure study purposes. This study further develops the PM2.5 predicted model based on the ANN techniques using the microenvironment source as the predicted variables. The present model could estimate the PM2.5 contribution from each microenvironment source. The results showed that temples, fried chicken shops, traffic emissions in shopping and residential zones, and industrial activities such as mechanical manufacturing and precision metal machining were the major sources of PM2.5. The machine learning of the ANN coupled with the LCS network presented in this study is a practical framework for PM2.5 hotspots and source identification, aiding decision-makers in reducing atmospheric PM2.5 concentrations and formulating regional air pollution control strategies.
AS12-A018
| Invited
Integrating Physical Atmospheric Chemistry Model, Machine Learning and XAI to Better Understand Wet Deposition Processes Across East Asia
Young-Hee RYU1#+, Seung-Ki MIN2
1Yonsei University, 2Pohang University of Science and Technology
Wet deposition is an important removal process of atmospheric pollutants and thus has great influences on soil environment and ecosystem. Rainfall amounts and atmospheric pollutant concentration determine the degree of wet deposition. The interannual variation in springtime wet deposition across East Asia is, however, weakly correlated either with rain or atmospheric pollutant concentration. Therefore, we unravel how rain and atmospheric pollutant concentrations quantitatively contribute to wet deposition and its variation across East Asia. The Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) is used to simulate 17 spring seasons (2003–2019) air quality over East Asia. The model evaluation against EANET observation data shows reasonable performance in reproducing sulfate, nitrate, and ammonium wet deposition fluxes. Unlike observation data in which limited data (e.g., rainfall and ionic concentrations in the rainwater at ground level) are available only for rain events, the WRF-Chem simulations offer full 3-D pollutant concentrations at a high temporal resolution. Thus, we develop 21 random forest models that predict 3-hourly wet deposition flux for 21 EANET stations; and employ the SHapley Additive exPlanations (SHAP), one of the widely used eXplainable artificial intelligence (XAI) methods. Rain and liquid water path (grouped as rain) is the most influential variable for almost all stations, but the relative role of rain greatly varies across sites. For heavily polluted stations, the contribution of rain is much larger by up to 4 times than that of pollutant concentration. For remote stations, rain and pollutant concentration are equally important. This study sheds light on integrating an atmospheric model, a machine learning model, and an XAI method to better understand how complicated physical processes are influenced by many variables in an atmospheric model.
AS12-A036
Machine Learning Analysis of Transition Metal-driven Degradation of Polycyclic Aromatic Hydrocarbons
Charles ESU1+, Sung-Ok BAEK2, Jong‑Bae HEO3, Cho KUK1#
1Pusan National University, 2Yeungnam University, 3Busan Development Institute
Transition metals are gaining recognition as crucial elements in the formation and aging of organic aerosols, which have significant implications for air quality. Previous laboratory studies have investigated the kinetics and factors influencing the impact of various metals on organic degradation, but these studies were confined to specific conditions. Traditional regression methods used to study the relationship between the concentrations of organics and metals in aerosols have limitations, particularly when both are co-generated. Here, we employed an explainable machine learning approach to derive the true relationship between the concentrations of metals and polycyclic aromatic hydrocarbons (PAHs). This was based on comprehensive field data collected in Korea from 2013 to 2017. Iron (Fe) exhibited the most potent direct association (Pearson correlation coefficient, r = -0.81, p << 0.01), indicating degradation chemistry, followed by Mg and V (r = -0.45 and -0.35, p << 0.01). This is the first time the degradation effect of V on PAHs has been observed. Further analysis revealed strong associations suggesting synergistic effects between Fe and other metals such as manganese (Mn), cobalt (Co), titanium (Ti), and nickel (Ni) (r = -0.95, -0.91, -0.90 and -0.85; p << 0.01). We discussed the direct effect using the Fenton reaction and single electron transfer, and the interaction effect for Fe under Fe redox cycling, formation of mixed metal complex, and sulfate formation. This research paves the way for a deeper understanding of the degradation and subsequent formation of organics in particulate matter.
Session Chair(s): Jun LI, National Satellite Meteorological Center
AS15-A049
| Invited
KMA Current and Future Satellite Program
Sung-Rae CHUNG#+, Jae Gwan KIM, SeHwan KIM, JeongBin PARK, TaeHyoung OH, Dohyeong KIM
Korea Meteorological Administration
The Korea Meteorological Administration (KMA) has been using not only ground observation data but also meteorological satellite observation data for weather forecasts. And the National Meteorological Satellite Center (NMSC) of the KMA has been operating the Korean second geostationary meteorological satellite, GEO-KOMPSAT-2A (GK2A) officially since July 2019. Various products using the GK2A observation data have been utilized for weather forecasting, Numerical Weather Prediction (NWP) data assimilation, climate change monitoring research, and so on. Additionally, the NMSC has developed simulation imagery such as nighttime true color RGB imagery with artificial intelligence (AI) technology. The KMA has been planned to develop the GK2A follow-on satellite to succeed the mission of the currently operating GK2A successfully in 2031. The GK2A follow-on satellite will be named as GK5 and it will have two payloads, one is the meteorological imager which is improved compared to the AMI of the GK2A on channels and spatial resolution. And the other is a set of space weather payloads named as Korean Space wEather Monitor (KSEM)-II will consist of proton detectors, electron detectors, magnetometer, and charging monitor. Moreover, new products and data service using the GK5 mission will be improved with various ways and timely provision such as through Cloud service, Open API, real-time FTP service, and satellite broadcast. In addition, KMA is also considering developing geostationary satellite with a hyperspectral infrared sounder to strengthen the abilities of weather and climate change monitoring and prediction together with GK5’s imager system. Also LEO meteorological satellite program will be informed in the presentation. More details on the KMA’s future satellite program will be shared at the conference.
AS15-A030
| Invited
Impact Studies of Configurable Reflectarray for Electronic Wideband Scanning Radiometry on Hurricane Ian (2022) Forecast
Zhenglong LI1#+, Pei WANG1, William BLACKWELL2
1University of Wisconsin–Madison, 2MIT Lincoln Laboratory
Existing cross-track microwave sounders on low Earth orbiting (LEO) satellites have a uniform data density concerning the viewing angle, with a single angular look for each field of view (FOV). For instance, the Advanced Technology Microwave Sounder (ATMS) has a scan step of 1.1°. However, not all regions require the same data density. Data-sensitive regions, where large gradients of meteorological parameters exist, necessitate higher data density compared to data-insensitive regions. The Configurable Reflectarray for Electronic Wideband Scanning Radiometry (CREWSR) is a future microwave imaging and sounding sensor designed to offer low-power, low-mass, low-cost, high-performance capabilities, and compatibility with Evolved Expendable Launch Vehicle Secondary Payload Adapter (ESPA)-class small satellite systems. CREWSR is specifically designed to provide high-quality microwave sounding radiance measurements, particularly in data-sensitive regions. It introduces features not available in existing microwave sounders, including configurable density and configurable multiple angular looks. This work aims to assess the added value from CREWSR through a hybrid Observing System Simulation Experiment (OSSE) study. CREWSR radiances are simulated using data from the ECMWF Reanalysis v5 (ERA5). The Advanced Technology Microwave Sounder (ATMS) is employed as a proxy for CREWSR, with higher density and multiple angular looks in data-sensitive regions. The hybrid OSSE approach is chosen for its realism, as all measurements are real except for CREWSR. This study focuses on Hurricane Ian (2022) as the case study to illustrate the impacts of assimilating CREWSR data on the forecast of track, minimum sea level pressure, maximum wind speed, and precipitation.
AS15-A003
Are Physics-based and Machine-learning-based Algorithms Using Geostationary Satellite Measurements Able to Retrieve the Diurnal Cycle of Cloud Base Height?
Min MIN#+, Mengyuan WANG
Sun Yat-sen University
In this study, we developed four specific retrieval methods to determine cloud base height (CBH) and its diurnal cycle using observations from the Himawari-8 geostationary meteorological satellite, which is belonged to JMA. These methods consist of two based on physics principles and two employing machine learning (ML) techniques. To verify their accuracies, validations were performed against CloudSat/CALIOP CBH data from 2017, ensuring independent assessments. Results indicate that the ML-based approaches significantly outperform the physics-based ones, showing a correlation coefficient (R) of over 0.91 and an absolute bias of around 0.8 km. However, assessments using CBH data from ground-based lidar in Yunnan province and cloud radar in Beijing present conflicting results (R < 0.60). Both ML-based methods consistently underestimate CBH, failing to capture its diurnal cycle accurately. The strong agreement observed between ML-derived CBH and the spaceborne sensor could be due to their shared training and validation datasets from CloudSat/CALIOP. Conversely, the CBH derived from the optimal physics-based method exhibits good agreement in daily CBH variations with ground-based observations (R ≈ 0.7) during daytime. Thus, findings from ground-based observations suggest that physics-based algorithms are more reliable and adaptable in retrieving CBH from geostationary satellite data, especially in climate research community. Nonetheless, given adequate spaceborne cloud radar data covering the entire day for training, ML methods could potentially provide more accurate CBH outputs under ideal conditions.
AS15-A004
Accurate Nowcasting of Cloud Cover at Solar Photovoltaic Plants
Pan XIA#+, Min MIN
Sun Yat-sen University
Nowcasting the cloud fraction (CF) or cloud cover (CC) to 4 hours and longer is highly required for generating Solar photovoltaic (PV) power. The advanced imagers onboard the new generation geostationary satellite series provide high spatio-temporal resolution of radiance measurement from visible to infrared spectral region, offer great opportunity for CF nowcasting with artificial intelligence technique. Using the advanced recurrent neural networks (NCP_CF), it is demonstrated that high-efficiency, high-quality and adaptable 0-4h cloud fraction nowcasting are achieved from Advanced Himawari Imager (AHI) radiance measurements for PV plants. Validation at three stations indicates that the NCP_CF prediction system achieves an excellent forecast performance within the first 2-hour horizon, with the mean correlation coefficient (R) close to 0.90 between predicted CF and actual CF, and the mean R close to or more than 0.80 between predicted CF and actual solar radiation observations at PV plants. The prediction system has been used in real-time for applications at three PV power plants.
AS15-A005
Effect of Ground-based Data on Retrieval of Temperature and Humidity Profile of Fengyun-4B Hyperspectral Infrared Sounder
Pengyu HUANG1#+, Min MIN1, Jun LI2
1Sun Yat-sen University, 2National Satellite Meteorological Center
The precision of temperature and humidity profiles in the boundary layer obtained from hyperspectral IR measurements is remarkably constrained by the challenge of distinguishing between surface and atmospheric contributions in this layer. To address this issue, this study proposes a novel joint inversion method, which can spatially and temporally collocate surface air temperature and humidity observations (or analysis). Through theoretical analysis, simulated experiments, and real data experiments, the new joint inversion method improved the resolution of boundary layer temperature and humidity by 0.1 km and 0.3 km, respectively, and reduced errors by 0.3 K and 2%.These findings highlight that the integration of hyperspectral IR measurements with surface air observations, available in near real-time, can yield enhanced boundary layer soundings for improved situational awareness in high-impact weather (HIW) forecasting and nowcasting applications.
AS15-A021
Deep Learning for Rainy Cloud Identification: Insights from Himawari Spectral and Cloud Data
Meng-Yue LIN1#+, Chian-Yi LIU2, Yu-Chun CHEN3, Yi-Chiang YU3
1National Central University, 2Academia Sinica, 3National Science and Technology Center for Disaster Reduction
One of the primary challenges in satellite infrared (IR) quantitative precipitation estimates (QPEs) lies in accurately characterizing the nonlinear relationship between cloud properties and rainfall rates. Machine learning models have proven to be effective tools for addressing such nonlinear problems. This research proposes the use of a deep neural network (DNN) method to classify clouds as either rainy or non-rainy based on brightness temperatures (BTs), reflectances (Refs), and cloud microphysical properties derived from the Advanced Himawari Imager (AHI) aboard the Himawari-8/9 satellite. We proposed to include cloud microphysical properties (CPs) with the BTs and Refs as the parameters in the DNN model training process. Additionally, a comprehensive assessment of features from the used parameters is conducted to elucidate their physical properties. Therefore, the QPE models trained by the DNN can be well-explained, and the cloud-to-rain process might be accurately depicted. The results are not only validated by ground-based radar observation, but are also compared to operational satellite derived precipitation products such as Global Satellite Mapping of Precipitation (GSMaP), and Integrated Multi-satellitE Retrievals for GPM (IMERG). The rainy area exhibits similarities with the reference products, and the mean error and root-mean-squared error of rain intensity are comparable to the reference products. These findings suggest that incorporating cloud microphysical properties contributes to enhancing the performance of QPE models. Looking ahead, satellite QPE techniques hold promise for real-time precipitation monitoring in East Asia.
Session Chair(s): Beom-Soon HAN, Inha University
AS07-A024
Machine Learning Approach to Predict Cardiovascular Disease Occurrence Using Climate and Air Pollution Factors
Siwoo LEE, Eunjin KANG+, Dongjin CHO, Jungho IM#
Ulsan National Institute of Science and Technology
Heart disease, including cardiovascular disease (CVD) and acute myocardial infarction (AMI), is the leading cause of death worldwide. With the consideration of ongoing climate change and air pollution, heart-related diseases are anticipated to impose a significant burden on the healthcare system. Consequently, there is an emerging need for patient prediction studies to aid decision-making within the medical system. Despite numerous studies developing machine learning (ML) prediction models using air pollution and meteorological variables defined as risk factors through epidemiological studies and interpreting them, nationwide research on analyzing the influence of risk factors based on urbanization and vulnerability levels is scarce. This study developed ML-based predictive models for daily counts of CVD and AMI patients using risk factors from the past ten years of data, from 2010 to 2019. Individual prediction models based on administrative divisions (si/gun/gu) in South Korea were constructed by training datasets excluding the year 2015, and the dataset from 2015 was utilized for validation purposes. Among prediction models based on Support Vector Regression, Random Forest (RF), Light Gradient Boosting Machine, and Long Short-Term Memory, RF demonstrated superior performance in predicting both CVD and AMI cases, yielding a coefficient of determination values of 0.81 for each and root mean square errors of 4.45 and 2.99, respectively. In interpreting risk factors using built-in feature importance, 7-day cumulative variables showed higher importance than exposure from the previous day. Compared with risk factors, air pollution-based factors observed a higher critical rank over most regions. Conversely, coastal regions mainly exhibited higher importance in meteorological variables than air pollution-based variables. These results are expected to contribute to policy decisions to prevent cardiovascular disease in patients by focusing on specific risk factors in each region.
AS07-A017
Measuring Pollutant Exposure of Virtual Walkers in an Idealised Urban Boundary-layer Flow Using Large-eddy Simulation
Guangdong DUAN1#+, Keith NGAN2, Tetsuya TAKEMI3
1Dalian Maritime University, 2University of Malaya, 3Kyoto University
Pollutant exposure in the urban air quality literature has been typically interpreted from data for fixed locations, which provides an incomplete picture of exposure for pedestrians (or moving receptors). By analysing the large-eddy simulation data for an aligned building array, we demonstrate that the actual exposure can differ significantly from results interpreted from data recorded by the fixed receptors (corresponding to Eulerian estimates). The current study proposes a simple model to parameterise the exposure time for a virtual walker to cross a pollutant cloud during its sweeping downstream across the avenue. The parameterisation, which depends on the centre-of-mass translation and the cloud size, shows satisfactory performance in areas away from the outlet, where a substantial portion of the pollutants is removed from the control domain and a well-defined centre of mass geometrically vanishes. Applying the tracer age diagnostics, the occurrence time of first exposure for the moving receptors is quantified with no particular caution required for the outlet region. The mean tracer age recorded by the virtual walkers is shown to be up to 25%–75% smaller than conventional spatial averages, implying earlier exposure to the pollutants and hence a reference timescale relying on the latter may lead to delayed emergency response. Evacuation route prioritisation based on virtual walker measurements coincides with that indicated by the parameterisation, suggesting the potential usefulness of the model for exposure risk evaluation against atmospheric air pollution incidents.
AS07-A020
Air Pollution and Its Associated Health Risks Before and After COVID-19 in Shaanxi Province, China
Yuxia MA, Bowen CHENG#+
Lanzhou University
Air pollution is a serious environmental problem that damages public health. In the present study, we used the segmentation function to improve the health risk–based air quality index (HAQI) and named it new HAQI (NHAQI). To investigate the spatiotemporal distribution characteristics of air pollutants and the associated health risks in Shaanxi Province before (Period I, 2015–2019) and after (Period II, 2020–2021) COVID-19. The six criteria pollutants were analyzed between January 1, 2015, and December 31, 2021, using the air quality index (AQI), aggregate AQI (AAQI), and NHAQI. The results showed that compared with AAQI and NHAQI, AQI underestimated the combined effects of multiple pollutants. The average concentrations of the six criteria pollutants were lower in Period II than in Period I due to reductions in anthropogenic emissions, with the concentrations of PM2.5 (particulate matter ≤2.5 μm diameter), PM10 (PM ≤ 10 μm diameter) SO2, NO2, O3, and CO decreased by 23.5%, 22.5%, 45.7%, 17.6%, 2.9%, and 41.6%, respectively. In Period II, the excess risk and the number of air pollution–related deaths decreased considerably by 46.5% and 49%, respectively. The cumulative population distribution estimated using the NHAQI revealed that 61% of the total number of individuals in Shaanxi Province were exposed to unhealthy air during Period I, whereas this proportion decreased to 16% during Period II. Although overall air quality exhibited substantial improvements, the associated health risks in winter remained high.
AS07-A005
Ozone Mortality Burden Changes Driven by Population Aging and Regional Inequity in China in 2013-2050
Xiaokang CHEN1#+, Zhe JIANG2, Yuqiang ZHANG3, Drew SHINDELL4, Shuxiao WANG5, Yanan SHEN1
1University of Science and Technology of China, 2Tianjin University, 3Shandong University, 4Duke University, 5Tsinghua University
Air pollution exposure is closely linked to population age and socioeconomic status. Population aging and imbalance in regional economy are thus anticipated to have important implications on ozone (O3)-related health impacts. Here we provide a driver analysis for O3 mortality burden due to respiratory disease in China over 2013-2050 driven by population aging and regional inequity. Unexpectedly, we find that population aging is estimated to result in dramatic rises in annual O3 mortality burden in China; by 55, 101-134 and 304-527 thousand over the periods 2013-2020, 2020-2030 and 2030-2050, respectively. This reflects the exponential rise in baseline mortality rates with increasing age. The aging-induced mortality burden rise in 2030-2050 is surprisingly large, as it is comparable to the net national mortality burden due to O3 exposure in 2030 (365-461 thousand yr-1). The health impacts of O3 pollution, shown as mortality burden per capita, are inequitably distributed, with more severe effects in less developed provinces than their developed counterparts by 23.3%, 53.7% and 25.7% in 2019, 2030 and 2050, respectively. This temporal variation reflects evolving demographic dividend characterized by a larger proportion of younger individuals in developed regions. These findings are critical for targeted improvement of healthcare services to ensure the sustainability of social development.
AS07-A009
Estimating Birthweight Reduction Attributable to Maternal Ozone Exposure in Low- and Middle-income Countries
Mingkun TONG+, Tao XUE#
Peking University
The effect of O3 on birthweight in low- and middle-income countries (LMICs) remains unknown. A multicenter epidemiological study was conducted to evaluate the association between maternal peak-season O3 exposure and birthweight, using 697,148 singleton newborns obtained in 54 LMICs between 2003 and 2019. We estimated the birthweight reduction attributable to peak-season O3 exposure in 123 LMICs based on a nonlinear exposure-response function (ERF). With every 10–part per billion increment in O3 concentration, we found a reduction in birthweight of 19.9 g [95% confidence interval (CI): 14.8 to 24.9 g]. The nonlinear ERF had a monotonic decreasing curve, and no safe O3 exposure threshold was identified. The mean reduction in birthweight reduction attributable to O3 across the 123 LMICs was 43.8 g (95% CI: 30.5 to 54.3 g) in 2019. The reduction in O3-related birthweight was greatest in countries in South Asia, the Middle East, and North Africa. Effective O3 pollution control policies have the potential to substantially improve infant health.
AS07-A021
Spatio-temporal Analysis of Air Quality Over Two Mega Cities in the West Zone of India
Nehul S#+
Savitribai Phule Pune University
With the advent of industrialization in the world's major metropolitan areas, air pollution has steadily increased. Several strict laws are imposed by the authorities to minimize the impact of pollution in urban dwellings. The lockdown restrictions during COVID-19 pandemic resulted in major air quality improvements worldwide. However, episodic improvements in air quality understates explicit picture of air quality. This merits the cause for spatio-temporal analysis of air quality over two most affected metropolitan regions in west India: Pune and Mumbai, in the past decade. We investigated the air quality by collecting hourly primary data of PM10, SPM, SO2, and NOx at three locations in Pune while daily data of PM10, SO2, and NOx was obtained at eleven locations in Mumbai. As the data were copiously available (2010-2020), decadal, inter-intra seasonal analysis was carried out at multi-timescales. This contributed in intensively exploring the variations in 2020 resulting in critical evaluation during the pandemic year. Against the overall deterioration in air quality in the past decade, finer refinement in air quality was witnessed over Pune during the lockdown. At Mumbai, an overall reduction of 59% was observed at all the locations. In both the cities, the pollution behaviour varied on a spatio-temporal scale within the cities. The study, therefore, infers the distinctiveness of pollutant behaviour on a spatial scale within the city rather than overall average for the city. It also recommends strengthening the air monitoring network in urban dwellings to track varied sources and formulate precise urban planning.
Session Chair(s): Ramesh KRIPALANI, Retired Senior Scientist, Indian Institute of Tropical Meteorology
AS04-A077
Regional Features of Sub-seasonal Maximum and Minimum Precipitation During the Summer Monsoon Season in Japan
Jun MATSUMOTO1,2#+, Fumiaki FUJIBE1
1Tokyo Metropolitan University, 2Japan Agency for Marine-Earth Science and Technology
Climate in Japan is characterized by the East Asian monsoon. Its summer monsoon season shows clear sub-seasonal changes. Summer monsoon precipitation in most parts of Japan comprises early summer (Baiu) and autumn (Shūrin) rainy periods with a relatively dry mid-summer. We aimed to determine details on the features of the seasonal and sub-seasonal progress of precipitation during the warm season in Japan. We assessed the timing of maximum and minimum precipitation based on daily records of Japanese dense local Kunai observations and AMeDAS networks collected at 522 stations for 95 years from 1926 to 2020. The maximum precipitation during Baiu has a northward delay, with a transition zone from the end of June to around July 10 at about 37°N, whereas Shūrin has three precipitation peaks corresponding to late August, mid-September, and early October over a wide area of Japan. The timing and intensity of the precipitation maximum varies according to the El Niño-Southern Oscillation (ENSO) phase, but the northward delay of the Baiu peak and multiple Shūrin peaks are found both in El Niño and La Niña years. Toward the past 30 years, the Baiu has lengthened, the mid-summer minimum shifts slightly earlier, and the main peak of Shūrin precipitation has become less distinct. The results are available at https://doi.org/10.4157/geogrevjapanb.95.55.
AS04-A012
The Increased Summer Monsoon Rainfall in Northwest India: Coupling with the Northwestern Arabian Sea Warming and Modulated by the Silk Road Pattern Since 2000
Mahendra NIMMAKANTI1#+, Nagaraju CHILUKOTI1, Chowdary S JASTI2
1National Institute of Technology Rourkela, 2Indian Institute of Tropical Meteorology
This study investigates changes in rainfall patterns over Northwest India (NWI) and the warming of the Northwestern Arabian Sea (NWAS) since 2000. These changes are attributed to the Silk Road Pattern (SRP) phase change in the late 1990s. The SRP positive phase triggers geostrophic deformation over the Tibetan Plateau (TP) by inducing an anomalous circulation pattern along the westerly jet, at 200 hPa. This deformation along the westerly Jet leads to Jet streaks and thermally indirect ageostrophic circulation over TP. In addition, the intensified heating over the TP led to a westward shift of the South Asian High (SAH). Associated with this, the interaction of positive temperature advection and northward ageostrophic wind (Jet entrance) over south-central Asia generates a southward component of ageostrophic wind (Jet Exit), causing upper-level convergence at southeast TP, excites the sinking cold air thereby strengthen the surface pressure below, over TP. This amplifies the anomalous anticyclone effect over there resulting in strong easterly wind anomalies along the monsoon trough at 850 hPa, disrupting the monsoon circulation. These anomalies, combined with a poleward shifting moisture-laden Low-Level Jet (LLJ), contribute to the warming of the NWAS and increased rainfall over NWI. The NWAS has shown significant summer warming over the past two decades. The poleward shift of the LLJ and SRP-induced circulation changes also impact the ocean dynamics. Given the occurrence of severe floods in this region of the Indian subcontinent, these findings have broader implications for predicting and projecting monsoon variability and extremes.
AS04-A062
Boreal Summer Intraseasonal Oscillation Induced Heat and Salt Variations Create Ideal Environments for Marine Heatwaves in the Northern East China Sea and Southern Yellow Sea
Panini DASGUPTA1#+, Sunghyun NAM1, Saranya J.S.1, Roxy Mathew KOLL2
1Seoul National University, 2Indian Institute of Tropical Meteorology
During the summer of 2016, the Northern East China Sea (NECS) and Southern Yellow Sea (SYS) encountered one of the most severe and destructive marine heatwaves (MHWs) recorded, exhibiting a temperature anomaly exceeding 3°C. The development of such events has been linked to the crucial factor of surface mixed layer shoaling. Using satellite and Hybrid Coordinate Ocean Model (HYCOM) reanalysis data from 1994 to 2015, we examined the mechanisms behind surface mixed layer shoaling during the genesis of MHWs in these regions. Our investigation highlights the significant role played by the northward propagating boreal summer intraseasonal oscillation (BSISO) and associated quasi-stationary Rossby waves in creating conducive conditions for the initiation and intensification of MHWs in these areas. Specifically, BSISO phases 5, 6, and 7 contribute to the formation of MHWs by inducing mixed layer shoaling and increasing solar influx, with both factors being equally crucial. This study provides insights into the relative impacts of sea surface wind and density stratifications on mixed layer shoaling, underscoring its global significance as a primary driver of MHWs.
AS04-A095
Improving the Subseasonal Variability of the Indian Summer Monsoon in a Climate Model
Ankur SRIVASTAVA1#+, Suryachandra Rao ANGULURI1, Subimal GHOSH2
1Indian Institute of Tropical Meteorology, 2Indian Institute of Technology Bombay
Many global climate models, including the Climate Forecast System version 2 (CFSv2), have a biased representation of subseasonal modes of variability of the Indian summer monsoon. For instance, they simulate a weaker summer mean monsoon low-pressure systems (LPS) climatology, faster than observed northward propagation of monsoon intraseasonal oscillations (MISOs), and a systematic dry bias over Indian landmass. The Bay of Bengal (BoB), with its shallow mixed layers and unique thermal stratification, significantly modulates the convective activity in this region at subseasonal-to-seasonal timescales through modulation of sea surface temperature. The highly stratified upper ocean in the BoB is due to the enormous freshwater it receives from rains and rivers. A river routing model is coupled to the CFSv2 to account for the riverine freshwater and the improvements in modelling the upper-ocean structure are analysed. Model simulations indicate that inclusion of temporally varying riverine freshwater improves the upper-ocean state in the BoB and the observed mixed-layer temperature gradients in the Bay are simulated reasonably after incorporating the time varying river runoff. This resulted in increased LPS lifetime and track density, and enhanced rainfall over central India. Better representation of the upper-ocean stratification in the model leads to larger post-convection shoaling of mixed layers at intraseasonal timescales, thereby forming thick barrier layers. Enhanced air–sea interactions restricted to the shallow mixed layer are associated with stronger vorticity, specific humidity and low-level convergence to the north of the intraseasonal convection band. This enhanced low-level moisture convergence north of the convection centre results in realistic northward propagation of MISO and aids LPS activity. It is demonstrated that better simulation of the upper-ocean structure in coupled climate models can improve the representation of subseasonal modes of monsoon variability. These results bear important implications for climate modelling and operational forecasting.
AS04-A093
Role of North Tropical Atlantic in Modulating the ENSO-south Asian Summer Monsoon Teleconnections
Ajinkya ASWALE1#+, Sooraj K.P.1, Swapna P1, Terray PASCAL2, Sandeep NARAYANSETTI1
1Indian Institute of Tropical Meteorology, 2Institut Pierre-Simon Laplace/ Sorbonne Université
Recently, the North Tropical Atlantic Sea Surface Temperature (NTA SST) anomalies have received great attention as a prominent contributing factor to El Niño Southern Oscillation (ENSO) variability, thus emerging as a key-driver of the whole ENSO-South Asian Summer Monsoon (ENSO-SASM) system. Against this backdrop, the current study aims to conduct a comprehensive analysis using observations, reanalysis, and long-term numerical simulations from the IITM Earth System Model (IITM-ESM), to have deeper insights on the role of the NTA SST variability on the ENSO-SASM teleconnections. Our results distinctly demonstrate the pronounced biennial nature of the NTA-ENSO-SASM system thus suggesting a crucial role of NTA SSTs in the biennial ENSO-SASM system. The ensembles of short coupled sensitivity experiments, by imposing observed warm (cold) SST anomalies over NTA, further highlight the key role of NTA SSTs in the reversal of the ENSO conditions through their capacitor effect. It further illustrates the nonlinear characteristics of this system as the cold NTA SST perturbations are more influential than warm NTA SSTs. This non-linearity brings up new perspectives on the NTA-ENSO-SASM system as it is further reflected in the asymmetric response in the simulated ENSO-SASM. These results have larger implications in a global warming future scenario, as the climate variability over NTA and ENSO region is projected to intensify in the future.
AS04-A001
Asian Monsoon Variability: A Review of Collaborative Research with Korean Scientists
Ramesh KRIPALANI1,2#+, Jai-Ho OH3, Kyung-Ja HA4
1Retired Senior Scientist, Indian Institute of Tropical Meteorology, 2Pukyong and Pusan National Universities, 3Nano C&W, 4Pusan National University
The first author has been regularly visiting South Korea since 2000. During the sixteen visits up to 2019 the first author has collaborated with scientists at the Pukyong National University, Pusan National University, IBS Center for Climate Physics, APEC Climate Center all situated in Busan; Meteorological Research Institute, Korea Meteorological Administration in Seoul, and Chosun University, Kwangju. Examination of the Asian Monsoon Variability vis-à-vis the Soviet Snow, ENSO, IODM, North Pacific Oscillation, North Pacific Subtropical High, Arctic and Antarctic Oscillations, Southern Annular Mode, Tibetan High, Atlantic SSTs, Greenland Sea-Ice and using Reanalysis and CMIP data sets has resulted in 20 publications in high-impact factor Journals and have generated some new perspectives in South and East Asia teleconnections. Even the impact of COVID-19 Regulations on monsoon variability over South and East Asia gave some interesting results. A few selected results will be presented at the AOGS2024 Meeting to be held in South Korea during June 2024.
Session Chair(s): Jun YING, Ministry of Natural Resources
AS61-A005
Detecting the Impacts of Anthropogenic Greenhouse Gas and Aerosol Forcings on ENSO
Michiya HAYASHI1#+, Hideo SHIOGAMA1, Tomoo OGURA1, Hiroaki TATEBE2, Malte STUECKER3
1National Institute for Environmental Studies, 2Japan Agency for Marine-Earth Science and Technology, 3University of Hawaii at Manoa
The El Niño-Southern Oscillation (ENSO) is the dominant interannual variability signal. It originates from coupled atmosphere-ocean feedbacks in the equatorial Pacific and impacts global climate and socioeconomics. Recent studies showed that sea surface temperature (SST) variability related to ENSO has already increased in the recent past due to anthropogenic global warming and is projected to increase further in the future. However, it remains unclear to what extent and via which mechanisms ENSO is modulated by each type of external forcing. Here, we show the impact of anthropogenic greenhouse gas (GHG), aerosols (AER), and natural (NAT) forcings on ENSO SST amplitude and its feedback processes. An initial-condition large ensemble of MIROC6 (MIROC6-LE) that provides 50 members of the historical/future and single-forcing experiments is analyzed as well as the historical and single-forcing experiments of CMIP6 climate models. In the MIROC6-LE, the ENSO amplitude, as characterized by the Niño-3 SST variance, increases from the preindustrial era to the early 21st century due to enhanced ocean response to the central Pacific zonal wind anomalies. This ENSO amplification is attributed to both the increased GHG and AER forcings while the NAT forcing does not modulate ENSO at centennial timescale. The CMIP6 multi-model ensemble shows robust inter-model correlations between the dynamic feedback change and ENSO amplitude change in each experiment. The results indicate that the ENSO amplitude change does not scale with global warming levels as both the GHG-driven global warming and AER-driven global cooling modulate ENSO amplitude and thus understanding the ENSO response to each forcing individually is critical to reduce uncertainty in projecting ENSO amplitude changes in the future.
AS61-A006
The Global Sea Level Experiences a Decline During La Niña Years
Huazhen LI#+, Andréa S. TASCHETTO
University of New South Wales
The continuous increase in global sea level poses a significant challenge for coastal regions worldwide. On top of human-induced rise in global mean sea level, year-to-year variations can occur due to natural variability, such as the significant sea level drop experienced during the 2010-11 La Niña event. In this study, we investigate a possible connection between global mean sea level and the El Niño Southern Oscillation. Our findings reveal that declines in global mean sea level are consistently linked to a cooling of the sea surface temperatures in the Niño 3.4 region, the signature of a developing La Niña event. Notably, four out of five La Niña events that occurred from 1993 to 2022, when sea level data is available, display similar trends encompassing increased terrestrial precipitation, expanded global land mass, and decreased global sea level. Intriguingly, our analysis reveals a robust negative correlation coefficient of up to -0.74 between terrestrial precipitation and global sea level fluctuations, suggesting that increased land precipitation during the early stages of a La Niña events leads to declines in global mean sea level. Predicting possible sea level variations across various climate scenarios can allow communities to prepare for potential hazards they might encounter.
AS61-A011
Wintertime Arctic Sea Ice Decline Related to Multi-year La Niña Events
Wenxiu ZHONG1+, Qian SHI1#, Qinghua YANG1,2, Jiping LIU1, Song YANG1
1Sun Yat-sen University, 2Southern Marine Science and Engineering Guangdong Laboratory
Arctic sea ice has undergone a significant decline in the Barents–Kara Seas (BKS) since the late 1990s. Previous studies have shown that the decrease in sea ice caused by increased poleward moisture transport is modulated by tropical sea temperature changes (mainly referring to La Niña events). The occurrence of multi-year La Niña (MYLA) events has increased significantly in recent decades, and their impact on Arctic sea ice needs to be further explored. In this study, we investigate the relationship between sea ice variation and different atmospheric diagnostics during MYLA and other La Niña (OTLA) winters, mainly based on composite analysis. The decline in BKS sea ice during MYLA years is significantly stronger than that during OTLA years. It is because the MYLA is conducive to the warm Arctic-cold continent pattern with a barotropic high-pressure blocked over the Ural region. Consequently, more frequent northward atmospheric rivers intrude into the BKS, intensifying long-wave radiation downward to the underlying surface and melting the BKS sea ice. However, in the early OTLA winter, negative North Atlantic Oscillation presents in the North Hemisphere high latitudes, which obstructs the atmospheric rivers to the south of Iceland. We infer that such a different response of BKS sea ice decline to different La Niña events is related to stratospheric processes. The more frequently occurred MYLA events might partly account for substantial Arctic sea ice loss in recent decades.
AS61-A002
Seasonal ITCZ Control on ENSO Responses to Extratropical Volcanic Forcing
Shih-Wei FANG1#+, Roberta D'AGOSTINO2, Myriam KHODRI3, Francesco S. R. PAUSATA4, Davide ZANCHETTIN5, Claudia TIMMRECK6
1National Central University, 2National Research Council, 3Laboratoire d’Océanographie et du Climat, 4University of Quebec in Montreal, 5University Ca’ Foscari of Venice, 6Max-Planck-Institut für Meteorologie
The response of El Nino Southern Oscillation (ENSO) to a strong volcanic eruption is determined by several controls, included the spatial structure of the volcanic forcing. In the case of extratropical eruptions, a mechanism contributing to post-eruption ENSO evolution involves the forced inter-hemispheric energy imbalance and the associated displacement of the Intertropical Convergence Zone (ITCZ). In this study, using 100 members of diverse (in locations and magnitude) idealized volcanic forcing ensembles from the Max Planck Institute Earth System Model (MPI-ESM1-2-LR), we find that the large (>= 10 Tg Sulfur) north and south extra-tropical eruptions lead to strong El Niño-like and weak La Niña-like responses in the winter next year, respectively, which can be attributed to the opposite displacement of summer ITCZ. Due to the seasonal migration of ITCZ, the southward displacement responses to large north extra-tropical eruptions facilitates an El Niño development in summer with westerly anomalies in the equatorial Pacific, while the northward displacement of south extra-tropical eruptions has a mixture of westerly and easterly anomalies, leading to a weak La Niña-like responses. Furthermore, when separating the 100 members based on initial ENSO states, distinct ENSO responses are found and significant differences in ENSO tendency can be found even 5 years after eruptions. This study stresses the importance of seasonal differences in ITCZ displacement when studying extratropical forcing and contributes to explains the inconsistency of ENSO responses to past volcanic events.
AS61-A032
El Niño Phase Transition by Deforestation in the Maritime Continent
Shengbiao WEI#+, Xin WANG, Chunzai WANG, Qiang XIE
Chinese Academy of Sciences
El Niño-Southern Oscillation (ENSO), an irregular alternation between warm El Niño and cold La Niña phases, is the most prominent air-sea interaction phenomenon on Earth and greatly affects global weather and climate. Nevertheless, it remains unclear whether human activity can alter the characteristics of ENSO. We demonstrate, using reanalysis data and coupled general circulation models, that deforestation over the Maritime Continent (MC) favors a rapid transition of El Niño to La Niña. Deforestation over the MC can induce a regional enhancement in precipitation, which in turn leads to strengthening of the easterly trade winds over the western equatorial Pacific owing to the Gill-response. These stronger trade winds, by inducing a shoaled thermocline in the eastern Pacific, are favorable for the development of cold sea surface temperature anomalies in the eastern equatorial Pacific during El Niño decaying years. Our results suggest that El Niño is more likely to be followed by La Niña if MC deforestation continues in the future.
Session Chair(s): Dong-Hyun CHA, Ulsan National Institute of Science and Technology
AS65-A004
| Invited
Very High-resolution Regional Climate Downscaling Over CORDEX East Asia
Jianping TANG#+, Peiqi YANG, Mengnan MA
Nanjing University
Under the framework of Coordinated Regional Downscaling Experiment-East Asia (CORDEX-EA) project, two climate simulations at 12.5 km resolution using RegCM4 and WRF driven by ERA5 reanalysis are conducted from 1980 to 2019. The results indicate that, both models can well reproduce the mean climatology, interannual variability and annual cycle of precipitation and near-surface air temperature (T2m); compared with simulations at 25 km resolution in the second phase of CORDEX-EA, raising spatial resolution to12.5 km can more effectively reduce simulation biases. WRF is superior in simulating the spatial pattern of annual and seasonal mean precipitation, while RegCM4 overestimates (underestimates) summer precipitation over land (ocean). T2m is also well simulated with cold bias over the Tibetan Plateau and warm bias in winter north of 45°N in both models. Moreover, the annual cycles of precipitation and T2m are better reproduced in WRF with reduced wet biases. These demonstrate higher ability of WRF with respect to climatological features and intra-annual variations. However, RegCM4 outperforms WRF in capturing the interannual variability of precipitation and T2m with higher temporal correlation coefficients in most sub-regions. Furthermore, investigation into simulated annual and seasonal mean wind field and specific humidity at 850hPa against ERA5 datasets shows that, the biases of low-level dynamic and thermodynamical conditions may be responsible for wet (dry) biases in summer over the land (ocean) in RegCM4; meanwhile, the surface upward longwave radiation fluxes are closely related to the T2m biases.
AS65-A002
High-resolution Climate Projection Over the Tibetan Plateau Using WRF Forced by Bias-corrected CESM
Mengnan MA1+, Jianping TANG1#, Tinghai OU2, Peifeng ZHOU1
1Nanjing University, 2University of Gothenburg
The Tibetan Plateau (TP) has undergone significantly stronger climate warming during the past years, but it is still challenging for most regional climate models to realistically simulate the present-day climate and promisingly project the future climate over the TP. In this study, high-resolution simulation using the Weather Research and Forecasting model (WRF) driven by bias-corrected CESM is conducted from 1979 to 2100, with the period from 2006 to 2100 under RCP4.5 and RCP8.5 (Representative Concentration Pathways) scenarios. The simulated present-day climate is evaluated firstly and then the future climate is studied. The results show that compared with station observation, WRF successfully captures the spatial pattern of annual mean surface air temperature (T2m) and precipitation over the TP, with the spatial correlation coefficients larger than 0.95 and 0.70, respectively. However, great underestimation of T2m over the southeastern TP is found in the colder seasons, which is related to the underestimation of snow there, and the snow-temperature positive feedback develops. Limited ability of WRF in reducing the dry bias in summer is probably related to the simulated weaker water vapor transport over the southern and eastern TP. For the future changes, substantial warming, general increase in precipitation and decrease in snow are projected under RCP8.5. Stronger and faster warming, together with significant decrease of snow, occurs over the western TP. Projected precipitation tends to consistently decrease over the western TP and along the south flank of TP which is related to the low-level circulation changes. The occurring frequency of non-precipitation and extreme precipitation will increase especially by the end of 21st century, raising the likelihood of drought and flood occurrences.
AS65-A007
Effects of Convective Inhibition on Future Changes in Summertime Dry Spells Over Japan Projected by Convection-permitting Regional Climate Model Simulations
Akihiko MURATA1#+, Masaya NOSAKA1, Hidetaka SASAKI2, Hiroaki KAWASE1
1Japan Meteorological Agency, 2National Institute for Environmental Studies
The effects of convective inhibition (CIN) on future changes in the length of summertime dry spells over a western part of Japan projected by convection-permitting reginal climate simulations are investigated. As an index of dry spells, maximum consecutive dry days is utilized. The regional climate model used is the non-hydrostatic regional climate model (NHRCM) with a grid spacing of 2 km and the period of the future climate is the end of the 21st century, from 2076 to 2096, under the RCP8.5 scenario. The results reveal that the horizontal distribution of changes in the beginning stage of CIN in August with global warming corresponds well to that in maximum consecutive dry days in the same month, indicating that changes in the earlier stage of CIN can affect those in summertime dry spells. In order to examine causes of the relationship between CIN and maximum consecutive dry days, changes in CIN are decomposed into two terms: The difference in virtual temperature at lifting condensation level (LCL) between parcel and environmental values, and the difference in height between convection base, assumed to be 950 hPa, and level of free convection (LFC). A comparison between the two shows the dominance of the former term, which can be further decomposed into several terms. Further analyses reveal that the primary contributor is changes in relative humidity at convection base. Changes in lapse rate between convection base and LCL also contributes in some places. In conclusion, changes in the length of summertime dry spells are mainly affected by those in relative humidity at convection base.
AS65-A023
Long-term Trend of Mesoscale Convective Systems Over East Asia in Regional Climate Simulation with a Convection-permitting Model
Tae Ho MUN+, Haerin PARK, Dong-Hyun CHA#
Ulsan National Institute of Science and Technology
A mesoscale convective system (MCS) is one of the major causes of extreme precipitation events. In East Asia, synoptic-scale forcings such as fronts and tropical cyclones can induce upward motions strong enough to generate MCSs. Also, MCSs may occur in weak synoptic environments. MCSs can result in heavy rainfall in a concentrated area, leading to significant risks and potential damage. MCSs are challenging to predict because their spatio-temporal scale is smaller than the synoptic-scale. Therefore, it is crucial to understand the characteristics of local MCSs and examine long-term trends and variability. In a previous study, we confirmed that the frequency of heavy rainfall caused by MCSs of short duration and high intensity has recently been increasing in Korea. These are weak synoptic environments MCSs, which are relatively small-scale. However, it can be challenging to understand small-scale MCSs (weak synoptic environments MCSs) using global or regional models and reanalysis data. Recent advances in computing resources have led to attempts to investigate the MCS using convection-permitting models (CPMs), which are high-resolution models. However, there has been little research on this topic in East Asia. Therefore, we simulated a CPM to analyze the long-term trends and variability of MCSs in East Asia. This study investigates the recent spatiotemporal variability (e.g., intensity, duration, and variability in the size of precipitation cells) of MCS in East Asia using a CPM.
AS65-A029
Investigation of Added Value in Regional Climate Models for Analysis of East Asian Storm Track in Future Climate Change Scenarios
Ui-Yong BYUN1+, Eun-Chul CHANG1#, Joowan KIM1, Joong-Bae AHN2, Dong-Hyun CHA3, Seung-Ki MIN4, Young-Hwa BYUN5
1Kongju National University, 2Pusan National University, 3Ulsan National Institute of Science and Technology, 4Pohang University of Science and Technology, 5National Institute of Meteorological Sciences
In the mid-latitudes, synoptic-scale phenomena such as high and low-pressure systems are responsible for the variability in regional-scale weather patterns. To understand this variability, the activity of storm tracks in extra-tropical regions has been analyzed based on observations dating back to the mid-nineteenth century. Initially, research in this area involved direct counts of cyclone movements. Subsequently, a time filtering method based on grid analysis has been adopted to isolate disturbances within a period range of 2 to 7 days. This bandpass filtering approach offers the advantage of enabling the examination of storm track distribution and variability, both spatially and vertically. The comparison of storm track activity between Regional Climate Models (RCMs) and the Global Climate Models (GCMs) used for their input effectively demonstrates the added value (AV) of RCMs. AV is evident in the more detailed representation of storm tracks, highlighting the importance of RCMs in understanding and predicting regional weather phenomena. In this study, we investigate storm track activity in the East Asia region using dynamical downscaling results from the CORDEX (COordinated Regional climate Downscaling EXperiment) East Asia projects. We assess the reproducibility of various RCM data and examine temporal changes in storm track activity. Our analysis extends beyond the historical period to explore variations in storm track intensity under future climate change scenarios. Through this investigation, we aim to confirm the role and AV from RCMs.
AS65-A028
Added Value of Dynamical Downscaling in Sub-seasonal Tropical Cyclone Forecast
Taehyung KIM1+, Dong-Hyun CHA1#, Sang-Min LEE2, Johan LEE2
1Ulsan National Institute of Science and Technology, 2National Institute of Meteorological Sciences
Tropical Cyclones (TCs), a significant natural phenomenon causing substantial socio-economic harm, occur approximately 25 times each year in the western North Pacific (WNP), directly or indirectly impacting Korea with about 3 to 4 TCs annually. Even with a relatively small number of TCs, the potential damage can be extraordinarily extensive. To proactively prepare for and respond to TCs, the focus is on enhancing the predictability of sub-seasonal to seasonal (S2S) forecasts spanning two weeks to two months. Consequently, identifying the causes of sub-seasonal forecasting errors in the Korea Meteorological Administration’s Global Seasonal Forecast System ver.6 (GloSea6) is essential to minimize damage from TCs through proactive measures. GloSea6 underestimated TC activity and intensity in the WNP from June to September. During periods of low performance in sub-seasonal TC simulations, there was a characteristic inability to reproduce Madden-Julian Oscillation (MJO) activities in the WNP and/or variability of the western North Pacific Subtropical High. To improve the forecast skill of sub-seasonal TC forecast, the GloSea6 was subjected to dynamical downscaling using the Weather Research and Forecasting Model (WRF). As for the experiment period, August 2016, when MJO was active in the WNP for a long time and WNPSH was strengthened, was selected. As a result, the added value was produced in which the TC frequency and intensity error were improved. In the GloSea6, the WNPSH rapidly weakened while weakly simulating a zonal Rossby wave from the north of India, but it is shown that the predictability of sub-seasonal TC was improved by realistically simulating the Rossby wave through dynamical downscaling. In addition, we are going to analyze other reasons for the improved TC predictability by dynamical downscaling.
AS65-A036
Added Value of Dynamical Downscaling Over South Asia for Wind Speed
Muhammad Abid KHAN#+, Koji DAIRAKU, Saurabh KELKAR
University of Tsukuba
Due to the advancement in computational capabilities, high-resolution simulations from regional climate models have gained a great deal of attention in recent years. Two distinct regional climate models RCA4 and REMO2009 are examined in this study for their improved effectiveness in simulating wind speed. Our research focuses on evaluating the performance of these models in the South Asian region, which is driven by MPI's Earth System Model. A simulation was conducted based on data collected from the CORDEX-SA, covering 1973-2005. A newly devised tool that facilitates an immediate comparison of probability density functions (PDFs) for m/s is the distribution added value (DAV) metric to quantify the enhanced effectiveness. Observational data are compared to models with high-resolution regional resolutions, for complete probability density functions and upper-tail probability density functions (P95), computed the DAV over annual and seasonal intervals. We observe significant enhancements in the RCA4 model as shown by DAV values that range from 8.4 - 11.5% for the complete PDF and from 4.7 - 12.1% for P95. REMO2009, however, demonstrates adverse values for DAV, indicating limited progress in replicating wind speed patterns. There is a variation in the values between the complete PDF and the P95 ranging from -9.9 to -10.8% and -13.5 to -17.9%, respectively. The ensemble mean indicates DAV values ranging from -2.4% to -2.1% and 0.6% to 1.8% for the complete PDF and P95, respectively. Results suggest that RCA4 appears to exhibit enhanced performance in replicating wind speed characteristics across South Asia, specifically in extreme weather conditions. Consequently, REMO2009 demonstrates limited improvement in the accuracy of representing wind speed patterns, whereas the ensemble mean shows moderate improvement. Overall, our study illustrates the benefit of downscaling m/s at high resolution, indicated by RCA4's favorable DAV. South Asia's climate model and impact assessment are enriched by these findings.
Session Chair(s): Hyunho LEE, Kongju National University, Junshik UM, Pusan National University
AS27-A004
Role of Autoconversion in Simulating the Active Break Spell of Indian Summer Monsoon
Ushnanshu DUTTA1#+, Anupam HAZRA2, Jen-Ping CHEN1
1National Taiwan University, 2Indian Institute of Tropical Meteorology
Simulation of the monsoon intraseasonal oscillations (MISOs) of the Indian summer monsoon, has been a real challenge for the state-of-the-art global coupled climate models. Now, the active-break spell is the building block of MISO and is of much importance to the farmers of the Indian subcontinent for proper planning of crop harvesting. Reliable seasonal forecasting also depends on the extent of realistic simulation of active break spell which determines the seasonal mean ISM. From a series of six sensitivity experiments, we have identified a particular combination of convective autoconversion coefficient and microphysical autoconversion coefficient which is more realistic to simulate ISM mean features, among a series of six sensitivity experiments. The improved bifurcation of convective and stratiform rain leads to the improved vertical profile of diabetic heating. Therefore, the autoconversion can modify dynamics (wind pattern) and temperature through changes in heating which in turn improves the mean ISM characteristics. In this study, we have shown how that combination also performs better in simulating the active break spell of ISM than the control. The proper combination of autoconversion coefficients impacts the conversion of cloud condensate to convective precipitation. At upper levels, this further controls the detrainment of moisture which in turn affects the cloudiness in the mid to upper troposphere. It also effectively controls the convection and hence impacts the active and break spell of monsoon. Therefore, the results presented here demonstrate a road map for the improvement of MISO by realistically simulating the physical processes associated with an accurate combination of autoconversion rates in a coupled climate model.
AS27-A011
Aerosol-induced Convection Over the Ocean and Midnight Shift of Precipitation Over Land of the Maritime Continent
Jinho CHOI1#+, Seoung Soo LEE2, Kyong-Hwan SEO1
1Pusan National University, 2Earth System Science Interdisciplinary Center
The aerosol effects on precipitation and circulation associated with the Madden-Julian oscillation over the Maritime Continent (MC) is investigated using cloud-resolving model. Simulations are performed for the period from December 1st to 4th, 2011 when the MJO-envelope is located over the MC. In simulations with aerosol radiative effects, as the aerosol number concentration increases, precipitation over the sea gets more, while that over the land gets less because of aerosol acting as a radiation absorber. Convection and precipitation over the land are weakened by inducing greater radiative forcings and stability. Therefore, vertical velocity over the land (sea) decreases (increases) by inducing low-level wind divergence (convergence). This results in the successful MJO-envelope that propagates across the MC through more precipitation with more fully developing convection over the sea. The difference in moist static energy (MSE) shows that as the aerosol number concentration increases, less MSE is consumed over the land with higher aerosol concentration than with the lower aerosol concentration during daytime due to the stable environment. This enables more MSE to be stored and to be released during nighttime over the land with the higher aerosol concentration. This induces stronger updrafts and more precipitation over the land that over the sea during nighttime. In general, precipitation over the land (sea) peaks at 17 (02) Local Standard Time (LST). Due to aerosol radiative effects, the peak-phase of diurnal cycle of precipitation over land moves from late-afternoon (17 LST) to midnight (23 LST). This suggests that the MJO-envelope might be able to propagate through the MC if diurnal cycle of precipitation for land becomes similar to that for sea due to aerosol radiative effects.
AS27-A003
Examination of Aerosol Impacts on Convective Clouds and Precipitation in Two Metropolitan Areas in East Asia; How Varying Depths of Convective Clouds Between the Areas Diversify Those Aerosol Effects?
Seoung Soo LEE#+
Earth System Science Interdisciplinary Center
This study examines the role played by aerosols which act as cloud condensation nuclei (CCN) in the development of clouds and precipitation in two metropolitan areas in East Asia that have experienced substantial increases in aerosol concentrations over the last decades. These two areas are the Seoul and Beijing areas and the examination was done by performing simulations using the Advanced Research Weather Research and Forecasting model as a cloud system resolving model. The CCN are advected from the continent to the Seoul area and this increases aerosol concentrations in the Seoul area. These increased CCN concentrations induce the enhancement of condensation that in turn induces the enhancement of deposition. These two types of enhancement work together to increase cloud mass and precipitation amount in a system of less deep convective clouds as compared to those in the Beijing area. In a system of deeper clouds in the Beijing area, increasing CCN concentrations also enhance condensation but reduce deposition. The reduced deposition offsets the enhanced condensation, leading to negligible CCN-induced changes in cloud mass and precipitation amount. Also, in the system, there is a competition for convective energy among clouds with different condensation and updrafts. This competition results in different responses to increasing CCN concentrations among different types of precipitation, which are light, medium and heavy precipitation in the Beijing area. The CCN-induced changes in freezing play a negligible role in CCN-precipitation interactions as compared to the role played by CCN-induced changes in condensation and deposition in both areas.
AS27-A005
Advecting Cloud-borne Aerosols in E3SM
Guangxing LIN#+
Chinese Academy of Sciences
Cloud-borne aerosols (aerosols that are attached to clouds) are formed by aerosol activation, aqueous-phase chemistry in clouds, or coagulation of aerosols with cloud droplets. The representation of cloud-borne aerosols is important for simulating aerosol-cloud interactions. However, most of the current GCMs including E3SM neglect the large-scale transport of cloud-borne aerosols in the model for the sake of saving computational time, which could result in biases in aerosol and cloud simulations. As the grid spacing of GCMs is reduced, the importance of cloud-borne-aerosol transport is expected to become more significant. Therefore, the objective of this study is to investigate the impact of neglected large-scale transport of cloud-borne aerosols in the GCM and to explore how the impact changes with the resolution of GCMs. First, we perform a pair of control simulations with/without considering cloud-borne aerosol advection at ne30 (approximately 1 degree) resolution, and we find that on a global basis, including the cloud-borne aerosol advection increases the cloud-borne aerosol burden approximately by 20%, but decreases the accumulation-mode aerosol number and cloud-droplet number by about 3% and 1.8%, respectively. On the other hand, the regional differences in aerosol and CDNC numbers can be over 30% (e.g., over East Asia, Europe, and Southern Ocean). For the aerosol-radiative forcing, however, the impact of cloud-borne aerosol advection is limited. Furthermore, we run additional set of sensitivity simulations with/without considering cloud-borne aerosol advection at ne120 (approximately 0.25 degree) resolution and compared them to the control simulations. When the resolution is changed to ne120, the impact of cloud-borne-aerosol advection on the aerosol burden is changed little on a global basis, while the regional differences, particularly over the outflow regions are noticeable.
AS27-A012
Cloud Seeding Effects on Orographic Clouds Using Spectral Bin Microphysics Scheme of the WRF Model
Kyoung Ock CHOI1#, Seoung Soo LEE2+, Seong Soo YUM3, Joo Wan CHA4
1Seoul National University, 2Earth System Science Interdisciplinary Center, 3Yonsei University, 4National Institute of Meteorological Sciences
Due to the limitation of field experiments of cloud seeding, numerical models are known as a great tool to investigate seeding effects on clouds. In this study, we developed cloud seeding processes in the spectral bin microphysics scheme of the WRF model, and we simulated an airborne AgI seeding case over the mountainous region of the Korean Peninsula. For the process-level understanding of the effect of cloud seeding, the budget analysis method is employed. Hydrometeor mass changes during each microphysical process and time step are calculated in the spectral bin microphysics scheme. The budget analysis results reveal that the most influential microphysical processes that control cloud seeding impacts on precipitation rate are collision-coalescence among cloud drops and snow melting. However, AgI seeding caused a decrease in precipitation, which is contrary to the object of cloud seeding. Therefore, to find an optimal seeding method for the case, more simulations with different seeding particle masses and types and seeding times and heights were conducted. Among the simulations, a seeding simulation releasing seeding particles 2 hours earlier than the AgI simulation is the only simulation that enhances precipitation. Although seeding methods differ, important microphysical processes on the precipitation are identical to the original seeding case. However, for the simulated case, 2 hours earlier seeding seems to enable to influence precipitation more efficiently because seeding particle-induced ice crystals could contribute to the developing stage of the clouds.
Session Chair(s): Xiaowen LI, Morgan State University, Chien-Ming WU, National Taiwan University
AS37-A001
Evaluation and Improvement of Numerical Models Using the Observation of Falling Speeds of Hydrometeors by the EarthCARE Satellite
Masaki SATOH1,2#+, Woosub ROH1, Shuhei MATSUGISHI1
1The University of Tokyo, 2Yokohama National University
The EarthCARE satellite, scheduled for launch in May 2024, will enable the world's first observations of Doppler velocities from space using radar. This groundbreaking capability allows for the observational understanding of global snow and raindrop falling velocities. In numerical climate and weather forecasting models, falling velocities of snow and raindrops have traditionally relied on empirical formulas based on fragmented observations, lacking comprehensive validation through global observations. These falling velocities have frequently been used as tuning parameters for numerical models. The falling velocity of upper-level clouds directly impacts radiation balance through variations in cloud amount. In contrast, the raindrop velocity influences the formation of cold pools and the organization of convective clouds. After obtaining Doppler velocity observations from the EarthCARE satellite, reliance on these falling velocities as tuning parameters becomes obsolete, introducing observational constraints. Conversely, altering these falling velocities from traditional prescribed values in numerical models leads to deviations in model climatology and equilibrium states from observations, necessitating refinement of other processes, which require the resolution of new compensatory errors. This presentation analyzes the characteristics of Doppler velocities using the global non-hydrostatic model NICAM and discusses the impact of snow and raindrops falling velocities. Specifically, utilizing the EarthCARE-like simulated data based on a global 220m mesh NICAM simulation, we aim to comprehend the global view of falling velocity characteristics and gain insights to analyze the EarthCARE satellite observational data. References: Roh, W., Satoh, M., Hashino, T., Matsugishi, S., Nasuno, T., Kubota, T. (2023) Introduction to EarthCARE synthetic data using a global storm-resolving simulation. Atmos. Meas. Tech., 16, 3331–3344, https://doi.org/10.5194/amt-16-3331-2023Satoh, M. and Matsugishi, S. (2023) Toward global large eddy simulations. Gekkan Kaiyo, , Vol. 55, No. 4, 172-179, https://doi.org/10.15083/0002007328 (in Japanese).
AS37-A003
Understanding of the Doppler Velocity from a Cloud Radar to Study Cloud and Precipitation Before the Launch of the EarthCARE
Woosub ROH1#+, Masaki SATOH1,2
1The University of Tokyo, 2Yokohama National University
The ground remote sensing observation data are relatively concentrated in a metropolitan area because of disaster prevention. The ULTra-sIte for Measuring Atmosphere of Tokyo metropolitan Environment (ULTIMATE, Satoh et al. 2022) project is proposed to use these intensive observation data in the Tokyo area together with satellite observations to evaluate and improve the cloud microphysics schemes of a numerical model and to validate the EarthCARE satellite. The merits of the project are related to several active sensors to detect the vertical distribution of clouds and precipitation, and the detailed information about clouds and precipitation in the specific region. Before the launch of the satellite, it is necessary to evaluate a numerical model using the ground observations with a similar setting to the EarthCARE cloud radar. This study presents evaluation results for cloud microphysics in the global non-hydrostatic model NICAM using ground observations including the 94 GHz cloud radar using the Joint Simulator (Hoshino et al. 2013). We interpret observed and simulated Doppler velocity to understand clouds and precipitation. We extend the evaluation with EarthCARE-like simulations. We also discuss how the EarthCARE can be used to evaluate a global storm resolution model.
AS37-A002
Simulating Moisture Transport Over the Tibetan Plateau in Summer of 2015 Across Convection-parameterized to Convection-permitting Scales with a Global Variable-resolution Model (MPAS-A v7.0)
Gudongze LI+, Chun ZHAO#, Mingyue XU, Jiawang FENG, Lei ZHONG, Rui LI, Yun-Fei FU
University of Science and Technology of China
Moisture transport in summer induces annual precipitation peak over the Tibetan Plateau (TP) thus being one crucial sustentation of water cycle between the TP and its surrounding areas. Accurately simulating moisture transport over the TP is uncertain for current numerical models with one important factor being horizontal resolution. In this study, in order to investigate the difference in moisture transport at resolutions from convection-parameterized to convection-permitting scales, three experiments are conducted for summer of 2015 using a global variable-resolution model (MPAS-A v7.0), including one with a globally quasi-uniform resolution of 60 km (U60km) and two with regional refinements over the TP at resolutions of 16 km (V16km) and 4 km (V4km), respectively. The differences in moisture transport among three simulations are significantly influenced by the changes in wind fields through the Himalayas and eastern TP in two layers, 700~600 and 600~400 hPa, which is largely modulated by their difference in large-scale circulations particularly monsoon depression. At convection-parameterized scale (from 60 km to 16 km), the monsoon depression is slightly stronger and shifts northward along with the mid-latitude westerlies, which is due to the combination of the sensitivity of convection scheme to integrating timestep and different extents of resolved dynamical processes at different resolutions. With horizontal resolution increasing to convection-permitting scale (from 16 km to 4 km), the resolved moist convection along with its associated less latent heat leads to weaker monsoon depression over the south of TP, which is much larger than the resolution induced difference at convection-parameterized scale.
AS37-A008
Precipitation Diurnal Cycle in the Global Convection-permitting Models
Fengfei SONG#+, Jinyan SONG
Ocean University of China
Accurately representing the precipitation diurnal cycle has long been a challenge for global climate models (GCMs). We systematically evaluate the precipitation diurnal cycle in the DYAMOND global convection-permitting models (CPMs) and compare it with the CMIP6 HighResMIP models. Purely increasing the model resolution doesn’t help much in the precipitation diurnal cycle by comparing the high- and low-resolution models in the HighResMIP project. In contrast, the CPMs can better capture the timing of precipitation diurnal cycle, with peak in late afternoon similar to the observation, although the amplitude is slightly overestimated. The better simulated precipitation diurnal cycle in the CPMs is closely related to the simulation of mesoscale convective systems (MCSs), as MCSs contribute about half of the total precipitation. The observed life cycle of MCSs, including initiation and mature stages, is well captured in the MCSs, thus producing a realistic diurnal cycle of MCS precipitation.
AS37-A004
The Characteristics of Convection Lifecycle and the Large-scale Circulation in Global Cloud-resolving Models of DYAMOND Summer Phase
Shao-Yu TSENG+, Wei-Ting CHEN#, Chien-Ming WU
National Taiwan University
In contrast to General Circulation Models, Global Cloud-Resolving Models (GCRMs) resolve convective systems, enabling their direct influence on the large-scale circulation. This provides a valuable opportunity to investigate the influence of convection on the large-scale circulation. This study evaluates the performance of convection lifecycles and large-scale circulation simulated by the GCRMs of the Atmospheric general circulation Modeled On Non-hydrostatic Domains (DYAMOND) summer phase by comparing them with the high-resolution satellite precipitation observations (IMERG) and ERA5 reanalysis. Additionally, we compare these results with the Central Weather Bureau Global Forecast System (CWBGFS), which utilizes gray zone resolution (~15km) with unified parameterization. The comparison focuses on the last 30 days within the simulation periods, and the model outputs were regrided to the same temporal (1 hourly) and spatial (15 km) resolutions. By employing the iterative rain cell tracking method, we track convective core systems (CCSs), which were defined as the spatially contiguous rainfall pixels exceeding 1 mm/hr, to assess the convective processes. Observational data features the increasing number of CCS mergers with longer lifespan, serving as a key metric for evaluating the convective behavior within the GCRMs. Moreover, our assessment extends to the large-scale circulation in moisture spaces, revealing distinct and diverse behaviors among the models. These evaluations yield valuable insights into GCRMs' ability to accurately represent the multi-scale convective dynamics and their impacts on large-scale circulations in the tropical regions.
AS37-A005
Characteristics of Convective Cell Lifecycle Simulated by a Cloud-resolving Model
Xiaowen LI#+, Md Rafsan JANI, Md RAHMAN, Chaz PADILLA
Morgan State University
Atmospheric convection is the key to global circulation dynamics and hydrological cycle. Due to its small-scale and turbulent nature, convection requires parameterization in global climate simulations. The convection parameterization schemes in Global Climate Models (GCMs) generally assume that the convective adjustment occurs within one model time step, therefore bypassing the natural lifecycle of convective cells. However, when GCM time steps approach one hour, this assumption becomes questionable. In this paper, we use high-resolution, cloud-resolving model simulations to study convection lifecycle characteristics. The Goddard Cumulus Ensemble (GCE) model is used to simulate convective cells’ lifecycles using two strategies: 1. single cell simulations forced by initial temperature/humidity perturbations. The simulations end when the single cell dies. 2. Organized convective systems near Darwin, Australia constrained by the large-scale forcing. Three-dimensional image segmentation using the U-Net Machine Learning algorithm are used to identify individual convective cells in the second type of simulations. In addition to presenting characteristics of the simulated convective cells and their mean behavior, we also study how often cells merge and split, and how these events affect convection lifecycle.
AS37-A006
Effects of Lower Troposphere Vertical Mixing on Simulated Clouds and Precipitation Over the Amazon During the Wet Season
Xiao-Ming HU1#+, Ming XUE1, Hector Mayol NOVOA2, Yongjie HUANG1
1The University of Oklahoma, 2Universidad Nacional de San Agustín de Arequipa
Planetary boundary layer (PBL) schemes parameterize unresolved turbulent mixing within the PBL and free troposphere (FT). Previous studies reported that precipitation simulation over the Amazon in South America is quite sensitive to PBL schemes and the exact relationship between the turbulent mixing and precipitation processes is, however, not disentangled. In this study, regional climate simulations over the Amazon in January-February 2019 are examined at process level to understand the precipitation sensitivity to PBL scheme. The focus is on two PBL schemes, the Yonsei University (YSU) scheme, and the asymmetric convective model v2 (ACM2) scheme, which show the largest difference in the simulated precipitation. During daytime, while the FT clouds simulated by YSU dissipate, clouds simulated by ACM2 maintain because of enhanced moisture supply due to the enhanced vertical moisture relay transport process: 1) vertical mixing within PBL transports surface moisture to the PBL top, and 2) FT mixing feeds the moisture into the FT cloud deck. Due to the thick cloud deck over Amazon simulated by ACM2, surface radiative heating is reduced and consequently the convective available potential energy (CAPE) is reduced. As a result, precipitation is weaker from ACM2. Two key parameters dictating the vertical mixing are identified, p, an exponent determining boundary layer mixing and lambda, a scale dictating FT mixing. Sensitivity simulations with altered p, lambda, and other treatments within YSU and ACM2 confirm the precipitation sensitivity. The FT mixing in the presence of clouds appears most critical to explain the sensitivity between YSU and ACM2.
AS37-A007
Analysis and Simulations of a Heavy Rainfall Event Associated with the Passage of a Shallow Front Over Northern Taiwan on 2 June 2017
Chuan-Chi TU1+, Yi-Leng CHEN2,1, Pay-Liam LIN1#, Mu-Qun HUANG1
1National Central University, 2University of Hawaii at Manoa
From 0200 to 1000 LST 2 June 2017, the shallow, east–west-oriented mei-yu front (<1 km) cannot move over the Yang-Ming Mountains (with peaks ∼1120 m) when it first arrives. The postfrontal cold air at the surface is deflected by the Yang-Ming Mountains and moves through the Keelung River and Tamsui River valleys into the Taipei basin. The shallow northerly winds are anchored along the northern side of the Yang-Ming Mountains for 8 h. In addition, the southwesterly barrier jet with maximum winds in the 900–950-hPa layer brings in abundant moisture and converges with the northwesterly flow in the southwestern flank of the mei-yu frontal cyclone. Therefore, torrential rain (>600 mm) occurs over the northern side of the Yang-Ming Mountains. From 1100 to 1200 LST, with the gradual deepening of the postfrontal cold air, the front finally passes over the Yang-Ming Mountains and arrives at the Taipei basin, which results in an east–west-oriented rainband with the rainfall maxima over the northwestern coast and Taipei basin. From 1300 to 1400 LST, the frontal rainband continues to move southward with rainfall over the northwestern slopes of the Snow Mountains. In the prefrontal southwesterly flow, the orographic lifting of the moisture-laden low-level winds results in heavy rainfall on the southwestern slopes of the Snow Mountains and the Central Mountain Range. With the terrain of the Yang-Ming Mountains removed in the high-resolution model, the mei-yu front moves quickly southward without a rainfall maximum over the northern tip of Taiwan.
AS01-A014
Hydroxyl-initiated Oxidation of (E)-β-farnesene: A New Mechanistic Understanding of HOMs Formation
Juan DANG#+, Zhang SHIBO, Hongjin WU
Shandong University, China
As one of the acyclic sesquiterpenes (SQTs), (E)-β-farnesene plays an important role in SOA formation through atmospheric oxidation to form highly oxidized multifunctional molecules (HOMs). In this study, we comprehensively explore the mechanism of oxidation of (E)-β-farnesene with OH radical by quantum chemical calculations. The OH addition reactions with lower free barriers are more dominant than H-atom abstraction reactions. The first-generation products involving acetone, (E)-4-methyl-8-methylenedeca-4,9-dienal, 4-methylenehex-5-enal, 6-methylhept-5-en-2-one, formaldehyde, (E)-7,11-dimethyldodeca-1,6,10-trien-3-one and (E)-6,10-dimethyl-2-methyleneundeca-5,9-dienal are produced from the subsequent reactions of the OH-(E)-β-farnesene adducts with NO and HO2. The second-generation products, including 4-oxopentanal, 4-methylenehex-5-enal, (E)-4-methyl-8-oxodeca-4,9-dienal, formaldehyde and (E)-4-methyl-8-methylenenon-4-enedial. HOMs formation via the autoxidation mechanism is limited by the H-shift. Our proposed mechanism, involving multiple H abstractions by OH radical and subsequent reactions with O2 and HO2, is a more thermodynamically favorable pathway for HOMs formation. The complicated oxidation mechanisms and products of sesquiterpenes (including (E)-β-farnesene) make it difficult to evaluate their contributions to SOA formation in the atmospheric chemical models. We hope the mechanism of (E)-β-farnesene oxidation in the atmosphere from a theoretical perspective would be conducive to clarifying the atmospheric fate of (E)-β-farnesene and even sesquiterpenes.
AS01-A021
Why Did Ozone Concentrations Increase During Shanghai’s Static Management? A Statistical and Radical Chemistry Perspective
Jian ZHU+, Shanshan WANG, Chuanqi GU, Bin ZHOU#
Fudan University, China
In April and May 2022, Shanghai implemented city-wide static management measures to control the Omicron variant, resembling a large-scale experiment. Despite a 30% reduction in VOCs and 50% in NO2, the 23% increase in average ozone levels surprised researchers. Diurnal patterns showed four distinct ozone variations, with Clusters 3 and 4 experiencing significant increases during static management. Observation-Based Model analysis indicated over 30% increases in OH, HO2, and RO2 concentrations in 2022 compared to 2020 and 2021. Despite HONO photolysis being the main ROx radical primary source, radical cycling dominated overall production. With a substantial NO2 decrease relative to VOCs, the VOCs/NO2 ratio rose from 1.6 in 2020 to 3.0 in 2022, affecting radical cycling. The OH radical propagation/termination ratio increased to 2.10, indicating the different precursor reduction proportions strengthened radical cycling. The unequal reduction in VOCs and NO2 during static management caused the rise in ozone concentration in Shanghai. This work was supported by National Natural Science Foundation of China (22176037, 42075097, 22376030, 42375089, 21976031) and National Key Research and Development Program of China (2022YFC3700101).
AS03-A001
Air Quality Benefits from Synergistic Control of Pollutants and Carbon Emissions in Tangshan, China
Jiaxin DONG1#+, Hongliang ZHANG2
1Fudan University, China, 2University of Shanghai for Science and Technology, China
Tangshan City, a major industrial city in the Beijing-Tianjin-Hebei region in the North China Plain, faces severe air pollution. Air pollutants and CO2 emissions share highly common homology, process characteristics and spatio-temporal consistency of emissions. In alignment with commitment to achieving carbon peaking and carbon neutrality, China has proposed plans to promote efficient coordination in pollutants and carbon reduction. However, there is a lack of research on understanding the benefits of co-emission reduction of CO2 and air pollutants. In this study, we use the Community Multiscale Air Quality (CMAQ) model with Weather Research and Forecasting Model (WRF) to simulate the synergistic scenarios of carbon and pollution reduction in 2030 and 2060, respectively. The scenarios include the baseline scenario, reflecting carbon emission reduction consistent with China's 2020 Nationally Determined Contribution (NDC) Target, the reinforcing scenario, outlining a mitigation strategy in line with the global 1.5-degree climate target and China's enhanced NDC commitments, and the moderate scenario, representing an intensity level between the baseline and reinforcing ones. Biogenic emissions are estimated using the Model of Emissions of Gases and Aerosols from Nature (MEGAN), while anthropogenic emission scenario are based on the Multi-resolution Emission Inventory for China (MEIC). This study would help elaborate on the synergies between environmental governance and carbon mitigation and provide a basis for enforcing integrated coordinated environmental pollution and CO2 emission control measures in Tangshan and across China.
AS03-A002
Responses of PM2.5 and O3 to Changes of Meteorology and Emissions in the Fenwei Plain from 2013 to 2020
Guangwu LIN#+
Fudan University, China
Surpassing other regions in China, the Fenwei Plain (FWP) became the most polluted areas area in China in recent years. Despite the pronounced severity of air pollution in this region, there is a notable scarcity of research on the subject, resulting in an unclear understanding of the factors contributing to changes of air pollution during clean air actions. This study seeks to elucidate the variations in air pollution within the FWP from 2013 to 2020, employing simulation results from the Community Multiscale Air Quality (CMAQ) v5.0.2 model. Meteorological fields are generated using the Weather Research and Forecasting (WRF) model, anthropogenic emissions are sourced from the Multi-resolution Emission Inventory for China (MEIC), and biogenic emissions are modeled using the Model of Emissions of Gases and Aerosols from Nature (MEGAN). Initially, the model's performance will be validated against observations, followed by an investigation into the changes in PM2.5 and O3 from 2013 to 2020. Ultimately, the study aims to assess the contributions of variations in meteorological conditions and emissions to the changes in PM2.5 and O3. This research provides a crucial reference for the prevention and control of air pollution in the FWP.
AS03-A003
Changes in Air Pollutants Sources and Health Effects within the Context of Rapid Urban Expansion
Zhaolei ZHANG1+, Yuqiang ZHANG2, Hongliang ZHANG3#
1Fudan University, China, 2Shandong University, China, 3University of Shanghai for Science and Technology, China
Rapid urbanization and industrialization have resulted in diverse anthropogenic activities and emissions between urban, peri-urban and rural regions, leading to varying levels of exposure to air pollutants and associated health risks. However, endeavors to mitigate air pollution and health benefits displayed considerable heterogeneity across different regions. Therefore, comprehending the changes in air pollutant concentrations and health impacts within the urban expansion context is imperative for promoting environmental equity. This paper uses GDP- and population-weighted methods to distinguish anthropogenic emissions from urban, peri-urban and rural regions in the world, and quantified their contributions to air pollutants and fast atmospheric response using the Community Earth System Model 2 (CESM2) from 1975 to 2015. The study reveals the impact of urbanization on environmental justice between countries at different levels of development in the world.
AS03-A008
Impact of Lightning-induced Nitrogen Oxides Over and Around the Tibetan Plateau on the Tibetan Plateau Ozone Valley
Zhou LIU1+, Fengxia GUO2#, Yuqiang ZHANG1
1Shandong University, China, 2Nanjing University of Information Science & Technology, China
Lightning-induced nitrogen oxides (LNOx) can affect ozone (O3) through photochemical processes. However, the impact of LNOx on the Tibetan Plateau (TP) O3 valley, an area with a lower O3 column compared to surrounding areas, remains controversial. Prior to this study, the impact of monsoonal transport on LNOx and related effects on the TP O3 valley has been overlooked. The objectives of this study are to differentiate between locally generated LNOx and monsoon-transported LNOx over the TP and to evaluate their impacts on tropospheric NOx vertical column density, tropospheric column O3, and O3 at different altitudes. The Weather Research and Forecasting model coupled with Chemistry model was used to replicate LNOx, NOx, and O3 over the TP during July 2010, for which nesting techniques and sensitivity experiments were implemented. The findings emphasize the importance of LNOx as a source of NOx in this region, with nonlocal lightning activity being the primary source. Conversely, the influence of locally generated LNOx on NOx levels over the TP is comparatively minor. Overall, LNOx contributes to an increase in O3 over the TP, but one order lower than the O3 depletion. The impact of LNOx on O3 varies across different altitude ranges; it is broadly “C” shaped, reflecting increase in O3 at near-surface and in upper troposphere–lower stratosphere (UTLS) regions and decrease in the middle troposphere. The increase in surface-level O3 over the TP is mainly caused by monsoon-transported LNOx, while locally generated LNOx also plays a crucial role in O3 formation in the UTLS region.
AS03-A010
An Updated Chemical Transport Model to Track the Sources of the Atmospheric Oxidation Capacity
Hongliang ZHANG1#+, Shengqiang ZHU2, Peng WANG2
1University of Shanghai for Science and Technology, China, 2Fudan University, China
China is confronting severe ozone (O3) pollution although particulate matter reduced significantly, causing damage to public health and ecological systems. O3 was influenced significantly by the atmospheric oxidation capacity (AOC), which was evaluated by the sum of oxidation rates of VOCs via reactions with HOx (OH and HO2) and NO3 radicals. Here, we updated the source-oriented CMAQ model to track the sources of HOx and NO3 radicals in the North China Plain (NCP) and Yangtze River Delta (YRD) in China. Specifically, we evaluated the contributions of different anthropogenic and natural sources to AOC by tracking the chemical reactions of HOx and NO3 radicals. Consequently, it’s significant to find that anthropogenic emissions made an important contribution to AOC in China. In the future, AOC contributed by different sources should be considered when designing O3 control policies.
AS03-A011
Deep Learning Based Emulator for Simulating CMAQ Surface Nitrate
Shuai WANG1#+, Hongliang ZHANG2
1Fudan University, China, 2University of Shanghai for Science and Technology, China
Airborne PM2.5 pollution is a leading risk factor for human health, which has been associated with multiple cardiovascular and respiratory diseases. Nitrate is one of the important toxic component and its fraction in PM2.5 is growing in China. The Community Multiscale Air Quality (CMAQ) model is widely used to estimate PM2.5 and its components. The substantial computational cost of CMAQ, including solving a complex system of partial differential equations (PDEs) for transport and aerosol dynamics, and ordinary differential equations (ODEs) for chemistry, poses a bottleneck to its widespread application. Machine learning-based methods have the potential to capture complex physicochemical processes in the atmosphere, and hence replace CMAQ to accelerate pollutant concentration estimation. This study aims to use a neural network emulator based on graph neural networks (GNNs) in an “encoder-processor-decoder” configuration to simulate the surface nitrate concentration of CMAQ. The model will be applied in winter and summer months of 2019 and evaluated against CMAQ results. Computational efficiency will be compared and possible uncertainties will be identified.
AS03-A022
Quantifying the Benefits of Improved Satellite Remote-sensing Observations for Inverse Modeling of NOx and NMVOC Emissions
Jia JUNG1,2#+, Matthew JOHNSON1, Amir Hossein SOURI3,4, Rajesh KUMAR5
1NASA Ames, United States, 2Bay Area Environmental Research Institute, United States, 3NASA Goddard Space Flight Center, United States, 4Morgan State University, United States, 5University Corporation for Atmospheric Research, United States
This study aims to demonstrate the benefits of using novel high spatiotemporal retrieval products from newer satellites for top-down emission estimates of nitrogen oxides (NOx) and non-methane volatile organic compounds (NMVOCs) for the summer of 2019 over the contiguous United States. Recent satellite retrievals have not only advanced spatiotemporal resolution but also greatly reduced error and uncertainty due to reduced noise in the retrievals compared to spaceborne sensors launched in the past. We applied inverse modeling techniques using tropospheric nitrogen dioxide (NO2) and formaldehyde (HCHO) column retrieval products from the Ozone Monitoring Instrument (OMI) and TROPOspheric Monitoring Instrument (TROPOMI) in conjunction with the Weather Research Forecast and Community Multiscale Air Quality Modeling system (WRF-CMAQ). In order to provide a better representation of background chemical composition and avoid misalignment of emission adjustment, we applied monthly scaling factors for ozone (O3) and CO boundary concentrations in addition to the inclusion of lightning and aviation emissions. Satellite-constrained NOx and NMVOCs posterior emissions showed a mitigated discrepancy between observed and modeled columns. The improvement in the model performance was greater when using TROPOMI, primarily benefiting from reduced errors/biases of the satellite retrievals that enabled us to explore corresponding changes in O3 concentrations and production sensitivity regimes using the ratio of HCHO and NO2.
AS06-A001
Assessment of the Long-term Tropical Cyclone Hazard for Coastal Megacities in China Using Centennial Coupled Seasonal Hindcasts
Xiaoqi ZHANG#+, Gregor C. LECKEBUSCH, Kelvin NG
University of Birmingham, United Kingdom
Coastal cities not only in China suffer from multiple natural hazards, such as strong winds, storm surges, extreme precipitation and flooding, from tropical cyclones (TCs). Due to a limited reliable observation period e.g., only ca. 50 typhoon seasons, robust hazard assessments of TCs are often challenging. Here we investigate the time development of the TC frequency-intensity distribution by use of a centennial multi-member seasonal hindcasts ensemble, the ECMWF CSF-20C data set. Based on this we build time-varying event-sets of physical consistent, but non-realised TCs with damage potential for coastal megacities following the approach from Osinski et al. (2016) and Ng and Leckebusch (2021). In this presentation, we show preliminary results for the long-term TC hazard variability resulting from those physically consistent event sets with special attention to the impact-relevant footprints of pure ensemble events. Additionally, the study will focus on several coastal megacities in China in different decades and thus contributing to the general understanding of the variability of the hazards and their time-varying uncertainty. Further implications and applications, e.g. for storm surge assessments are also discussed.
AS06-A002
Interdecadal Change of Relationship Between North Atlantic Oscillation and Tropical Cyclone Genesis Frequency Over the Northwest Pacific Modulated by the Pacific Decadal Oscillation
Zhen WANG#+, Zhao JIUWEI
Nanjing University of Information Science & Technology, China
The relationship between the spring North Atlantic Oscillation (NAO) and the tropical cyclone frequency over the western North Pacific (WNPTCF) in summer and autumn is investigated by use of observation data. It is found that their linkage appears to have an interdecadal change from weak connection to strong connection and then weak connection. During the period of 1950–1971 and 2011-2021, the NAO was insignificantly correlated to the WNPTCF. However, during the period of 1972-2010, they were significantly correlated with stronger (weaker) NAO corresponding to more (fewer) tropical cyclones in the western North Pacific. The relationship between the NAO and the WNPTCF is modulated by the Pacific Decadal Oscillation (PDO). When PDO is in its positive phase, anomalous upper-level westerlies occur over the tropical North Atlantic, allowing the energy associated with the positive phase of NAO propagates towards lower latitudes, leading to cold sea surface temperature anomalies in the tropical North Atlantic during spring. Subsequently, these cold sea surface temperature anomalies adjust the circulation patterns in the tropical North Atlantic, causing positive sea surface temperature anomalies in the Central Pacific, triggering anomalous low-level cyclonic patterns in the Northwest Pacific region, along with anomalous upper-level anticyclonic patterns, ultimately resulting in an increase in the frequency of typhoons. However, when the PDO is in its negative phase, the connection between the NAO and cold sea surface temperature anomalies weakens, breaking the relationship between the NAO and WNPTCF.
AS06-A010
Integrating Temporal and Geospatial Analysis for Climate Profiling in Mindanao, Philippines (2005-2015)
Alexis VALDERRAMA1#+, Quirino Jr SUGON2,1, Rochelle CORONEL3, Clint BENNETT1, Daniel MCNAMARA1, Rogel Mari SESE3
1Ateneo de Manila University, Philippines, 2Manila Observatory, Philippines, 3Ateneo de Davao University, Philippines
In this research, we examine the analysis of a decade's worth of lightning and rainfall data in Mindanao, Philippines, employing a geospatial aggregation methodology. Our approach hinged on the processing of extensive datasets from the Global Precipitation Measurement (GPM) and the World Wide Lightning Location Network (WWLLN). The core of this method involved segmenting Mindanao into a detailed grid system, where each pixel represented a specific geographic area. For each pixel, we calculated a statistical measure that captures the typical intensity of rainfall and frequency of lightning, meticulously avoiding the influence of extreme weather anomalies. This allowed us to construct a highly accurate geospatial climate profile across different regions of Mindanao. The results shows that for annual, seasonal and diurnal climate maps, there has been substantial temporal variations in weather patterns. This illustrates that while certain months consistently show heightened climatic activity, the same periods in subsequent years may not exhibit the same intensity or distribution of rainfall and lightning. The analysis revealed four distinct climatic zones, each characterized by unique patterns of rainfall and lightning. The first zone was identified by its simultaneous high intensity of rainfall and frequent lightning occurrences, suggesting a climate prone to regular and intense thunderstorms. The second zone, marked by high rainfall but less frequent lightning, indicated a wet climate with fewer thunderstorms. In contrast, the third zone showed an inverse pattern with less frequent rainfall but higher occurrences of lightning, pointing to a drier climate where lightning storms are more common. Lastly, the fourth zone, characterized by both infrequent rainfall and lightning, represented the most stable and mild weather conditions. Geospatial mapping has yielded detailed insights into Mindanao's varied climate, vital for improving weather forecasts and developing disaster strategies for each zone's specific climatic conditions.
AS06-A013
Asymmetric Response of Tropical Cyclone Genesis to Symmetric CO2 Concentration Change
Hyunsuk YOON1+, Jaeyeon LEE2, Hyeong-Seog KIM3, Seok-Woo SON1#, Soon-Il AN4, Jongsoo SHIN5
1Seoul National University, Korea, South, 2Princeton University/ NOAA Geophysical Fluid Dynamics Laboratory, United States, 3Korea Maritime and Ocean University, Korea, South, 4Yonsei University, Korea, South, 5Woods Hole Oceanographic Institution, United States
Tropical cyclones (TCs) cause severe economic losses and casualties, which has led to extensive studies on the response of TCs to large-scale environmental changes under global warming and atmospheric CO2 concentration increase. However, changes in TCs due to CO2 concentration decrease, which is necessary for climate mitigation, have not been established. As such, the present study revisits the TC response to CO2 increase and then investigates the TC response to CO2 decrease using the Community Earth System Model 1.2 (CESM1.2). When the atmospheric CO2 concentration is increased until quadrupled (ramp-up, RU), TC genesis increases over the eastern North Pacific and South Pacific, while it decreases over the southern Indian Ocean. Such changes are not completely reversed by symmetrically reducing the atmospheric CO2 concentration (ramp-down, RD). In the RD, TC genesis decreases over the eastern North Pacific, but increases over the Southern Hemisphere basins. Thus, TC genesis over the South Pacific becomes higher in the late RD than in the early RU, which indicates the asymmetric TC response to symmetric atmospheric CO2 change. To gain insight into this asymmetry in TC genesis response, the large-scale environmental changes associated with TC genesis are further analyzed. It is found that the South Pacific experiences an increase in relative humidity and vertical updraft in both RU and RD, thus becoming more favorable to TC genesis. These atmospheric changes appear to be linked with the intensification and southward shift of the Intertropical Convergence Zone during RU and RD, respectively. Nearly reversible changes in these atmospheric variables, and hence the TC genesis, are observed in the southern Indian Ocean. Meanwhile, low-level vorticity change, due to sea surface temperature change centered in the eastern Pacific, is likely responsible for TC genesis change in the eastern North Pacific.
AS10-A001
Distribution and Biochemical Effects of Carbohydrates in Atmospheric Suspended Particles in East Asia: Analyzing Their Sources by Combining Principal Component Analysis and Positive Matrix Factorization
Hung-Yu CHEN#+, Ting Wen LIU
National Taiwan Ocean University, Taiwan
Carbohydrates are the main source of energy for living organisms. Carbohydrates are released into the atmosphere through natural and man-made emissions and are regarded as organic molecular tracers. Carbohydrates on atmospheric particles may come from biomass burning, dust, fungal spores and pollen, etc. In this study, we collected atmospheric particulate samples from April 2019 to September 2020 on the Matsu Islands, which are located at estuary of Minjiang River. During the sampling period, the concentrations of total mass and the water-soluble organic carbon (WS-OC) were 40.03 ± 7.00 μg m-3 and 69.21 ± 72.44 nmol m-3. respectively. For carbohydrate species, the concentrations of total water-soluble carbohydrate and monosaccharide were 0.15 ± 0.11 nmol m-3 and 0.08 ± 0.10 nmol m-3., respectively. Monosaccharides account for nearly 50% of total sugars, which means that monosaccharides in the atmosphere are more available to organisms. In terms of particle size composition, monosaccharide was mainly distributed in fine particles (particle size < 095 μm), while polysaccharide was mainly distributed in particle size between 3 μm ~7.2 μm and < 0.49 μm. In order to further explore the sources of carbohydrates, Principal Component Analysis (PCA) and Positive Matrix Factorization (PMF) were used in this study. The results show four main aerosol sources in the region: biomass burning, anthropogenic sources, marine sources, and mixed sources, indicating that PCA and PMF provide precise insights into aerosols sources. The main source of carbohydrates is biomass burning, exhibiting a seasonal trend. During the biomass burning frequency in spring, it provides a carbon source for microorganisms, promoting nutrient cycling and plant growth, thereby exerting various effects on biogeochemistry.
AS10-A003
Underestimated Role of Sea Surface Temperature in the Formation of Sea Spray Aerosol and the Enrichment of Organic Matter
Jie HU#+
Shandong University, China
The ambiguity surrounding the correlation between sea spray aerosol (SSA) formation and sea surface temperature (SST) hinders the accurate estimation of the impact of SSA on global climate. Here, we developed a temperature-controlled plunging SSA simulation tank to comprehensively investigate the impact of SST on SSA formation from two perspectives of SSA particle size distribution and organic matter enrichment. Our findings showed that the production of accumulation modal and coarse modal particles decreases as SST decreases from 30 ℃ to 0 ℃, while the production of Aitken modal particles decreases from 30 ℃ to 12 ℃, followed by a significant increase from 12 ℃ to 0 ℃. Enrichment factor (EF) results revealed a tenfold in the surfactant’s EF and a fourfold increase in the algae-derived dissolved organic carbon’s EF at 30 ℃ compared to 0 ℃, indicating that the temperature-dependent nature of organic matter in SSA particles significantly enhances their enrichment ability. Using the experimental results, we predict that SST variations may lead to a disparity of at least 191 ± 46 % regarding the contribution of Aitken-mode submicron sea salt particles to cloud condensation nuclei in polar and equatorial waters. Finally, considering the importance of SST for organic enrichment, our estimation indicates the global flux of DOC emitted via SSA is 25.2 Tg C yr-1.
AS11-A002
Five-year Climatology of Local Convections in the Dabie Mountains
Linlin ZHENG#+
Anhui Meteorological Observatory, China
Local Convection in Dabie Mountains (LCDM) occurs more frequently over the Dabie Mountains and brings severe weather to adjacent areas. In order to understand the characteristics of LCDM, their spatial distribution, the monthly and diurnal variations, and possible mechanisms are investigated. Based on radar composite reflectivity data over the 5-y period of 2014–2018 during warm seasons (April–September), a total of 195 cases of LCDM are identified. The LCDM exhibits maximum frequency on the windward slopes of the Dabie Mountains with a secondary maximum on lee slopes. It is demonstrated that LCDM peaks in July and August, while their diurnal variation exhibits a major peak in the afternoon during 12:00–16:00 local solar time (LST). Most LCDM does not leave the Dabie Mountains (NoOut-Type), accounting for 89.7% overall, and has an average 3.5 h lifespan. In contrast, the lifespans of Out-Types (i.e., LCDMs that move away from the Dabie Mountains) are longer (5.8 h on average), while most Out-Type LCDMs develop on southern slopes (‘South-Type’) and a few are also reinforced on northern slopes (‘North-Type’). The South-Type mainly produces short-duration heavy precipitation, while the ‘North-Type’ predominately generates thunderstorms high winds. It is suggested that LCDM is thermally induced, and that both the ‘South-Type’ and ‘North-Type’ are controlled by southerly wind perturbation. Lifting by upslope wind and heat sources over windward slopes has led to ‘South-Type’ development, while ascent induced by wave-like perturbations on lee slopes has led to ‘North-Type’. These mechanisms should be further investigated in future work by using field experiments and numerical simulations.
AS11-A012
A Comparison of Sensitivity Analysis Based on Data Assimilation Using Atmospheric Research Aircraft Observational Data
Seung-Beom HAN1+, Tae-Young GOO1#, Sueng-Pil JUNG2, Min-Seong KIM1, Deok-Du KANG1, Chulkyu LEE1
1National Institute of Meteorological Sciences, Korea, South, 2National Institute of Meteorological Sciences/Korea Meteorological Administration, Korea, South
The Uncertainty in the initial conditions of the numerical model affected the errors in the numerical weather prediction system. Aircraft are considered one of the best platforms to obtain atmospheric spatial information in observational gaps, especially over the sea. National Institute of Meteorological Sciences (NIMS) has operated an atmospheric research aircraft to fill observational gaps. These Aircraft observational data provide a continuous distribution of meteorological variables and contribute significantly to improving the performance of the numerical predictions. In this study, the effect of data assimilation (DA) on the prediction of typhoons affecting the Korean Peninsula was evaluated using high-resolution numerical modeling with atmospheric research aircraft observational data. This analysis was performed using two sets of simulation experiments: (1) WRF (V.4.1.2) run with DA (i.e., WRF-3DVAR), including atmospheric research aircraft observational data (Dropsonde, AIMMS-20) to improve the prediction of meteorological variables (e.g., temperature, wind components, and relative humidity), and (2) WRF run without DA (i.e., CTL). To reflect the data assimilation technique that improved the initial field more effectively, we used the GDAPS, ERA5, and KIM reanalysis fields provided by UM, ECMWF, and KMA as the initial/boundary conditions of the model. Overall, the results simulated by WRF-3DVAR for typhoon events in the study area are in good agreement with those observed in the CTL run. In particular, the air temperature showed improved results in all experiments with data assimilation (Dropsonde, AIMMS-20, and Dropsonde+AIMMS-20), and the wind speed showed improved simulation results in Dropsonde and Dropsonde+AIMMS-20, with the exception of AIMMS-20.
AS11-A013
Advancing Sea Surface Wind Measurements with Stepped Frequency Microwave Radiometer: A Comprehensive Study of Validation, Calibration, and Sensitivity Analysis
Deok-Du KANG#+, Min-Seong KIM, Seung-Beom HAN, Tae-Young GOO, Chulkyu LEE
National Institute of Meteorological Sciences, Korea, South
The National Institute of Atmospheric Sciences (NIMS) employs its KingAir 350H research aircraft for various missions, including the "Severe Weather" (SW) mission. This mission aims to enhance understanding of severe weather events like heavy rain, snowfall, and typhoons through advanced observations, ultimately improving numerical model accuracy. A key instrument aboard the aircraft is the Stepped Frequency Microwave Radiometer (SFMR). Mounted underneath, this C-band radiometer measures ocean brightness temperature to calculate sea surface wind speed and rain rate. Our study compared wind speeds derived from the SFMR with those obtained from dropsondes deployed along the aircraft's flight path. We also investigated the sensitivity of SFMR wind speed estimates to sea surface temperature and salinity, both serving as initial input data. Between June 2022 and October 2023, 21 SW-mission flights covered the Yellow Sea. SFMR data revealed an average wind speed of 8.7 m/s and a maximum of 22.1 m/s. Sea surface temperature and salinity data from buoys and research stations were interpolated to 0.1˚ intervals for sensitivity analysis. Calibration coefficients derived from a dedicated calibration flight on October 26, 2022, were applied to re-calculate wind speeds, which were then compared with pre-calibration estimates and wind speeds obtained from dropsondes at 30m, 150m, and 500m above the sea surface. Notably, the strongest correlation was observed between SFMR-derived wind speeds and those at 500m. This study demonstrates the potential of NIMS aircraft SFMR data for accurate sea surface wind speed measurements, particularly when employing calibration and considering the influence of lower-level wind patterns. Further research can refine these techniques and enhance our understanding of air-sea interaction.
AS11-A014
Numerical Simulation of the October 2021 Heatwave in South Korea: Influence of Typhoon MINDULLE (2116)
Semin YUN1+, Jieun WIE1, Hak-Sung KIM2, Jae-Hee CHO2, Byung-Kwon MOON1#
1Jeonbuk National University, Korea, South, 2Korea National University of Education, Korea, South
South Korea experienced an unprecedented heatwave in October 2021. Such autumn heatwaves have adverse effects on crop production and lead to increased energy consumption. To prepare for heatwaves, analyzing the impact of meteorological conditions is crucial. Therefore, we conducted numerical experiments to analyze the impact of Typhoon MINDULLE (2116) on the heatwave that occurred in October 2021. Using the Weather Research and Forecasting (WRF) model, we performed the experiment replicating reality (TC) and under similar conditions but eliminating typhoon winds (TC-removed). Each experiment consisted of four ensemble members and ran for 41 days, beginning on September 23. During the heatwave, TC simulated 2-m temperatures up to 1.35°C higher than those of TC-removed. This temperature difference was linked to the typhoon's influence, which enhanced warm air advection from the northwest Pacific. These findings indicate that typhoon variability should be considered when forecasting extreme temperatures on the Korean Peninsula.
※ This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No.2022R1A2C1008858), and by the Korea Environment Industry & Technology Institute (KEITI) through the 'Climate Change R&D Project for New Climate Regime,' funded by the Korea Ministry of Environment (MOE) (2022003560001).
AS11-A015
Impact of Dropsonde Data Assimilation on the Prediction of Typhoon Over the Sea Around the Korean Peninsula Using the WRF-ARW Model
Min-Seong KIM1+, Seung-Beom HAN1, Tae-Young GOO1#, Sueng-Pil JUNG2, Deok-Du KANG1, Chulkyu LEE1
1National Institute of Meteorological Sciences, Korea, South, 2National Institute of Meteorological Sciences/Korea Meteorological Administration, Korea, South
The ocean heat fluxes over the sea are critical for simulating typhoon track and intensity because ocean heat fluxes are the energy source for typhoon maintenance and development. Over sea, where there is less observational data than on land, airborne observation can provide high-quality initial conditions for numerical models and help predict typhoon intensities and tracks. The National Institute of Meteorological Sciences (NIMS) initiated the annual operation of NIMS Atmospheric Research Aircraft (NARA) to investigate the atmospheric horizontal and vertical structure preceding severe weather phenomena such as typhoon, and heavy rainfall with the aim of reducing the uncertainty of atmospheric observations as of January 2018.This study investigates the impact of Dropsonde data assimilation for prediction of the typhoon OMAIS over the sea around Korean peninsula using the Weather Research and Forecasting (WRF) Advanced Research WRF model and its 3-dimensional data assimilation (3DVar) technique. Typhoon OMAIS is the first typhoon to land on the Korean Peninsula in 2021. Six experiments were conducted, three with Dropsonde data assimilation at three different initial conditions (UM GDPS, ECMWF ERA5, KIM) and three without Dropsonde data assimilation at three different initial conditions.
AS11-A017
The Atmospheric Circulation Anomalies Associated with the Formation of Marine Heatwaves in the Northeast Pacific
Cong TANG1+, Riyu LU2#
1Ocean University of China, China, 2Chinese Academy of Sciences, China
Extreme and persistent marine heatwaves (MHWs) occur frequently in the Northeast Pacific, with huge impacts on climate, ecosystem and socio-economic. This study investigates the atmospheric circulations associated with the 33 MHWs since 1951 in observations. The composite results reveal that the MHWs in the Northeast Pacific can be triggered by a couple of anticyclonic and cyclonic anomalies, i.e., the anticyclonic anomaly to the northeast of the MHW region and cyclonic anomaly to the southwest. This atmospheric circulation pattern can be detected as the dominant mode through EOF analysis on 500-hPa geopotential height anomalies over the Northeast Pacific-North America region, following the Pacific–North American teleconnection. These observational results are verified by using the outputs of 34 models in the historical simulation from phase 6 of the Coupled Model Intercomparison Project (CMIP6). Further diagnosis of the heat budget is performed, in attempt to illustrate the processes of MHW formation and maintenance.
AS11-A018
Bundelkhand's Paradox: Two Droughts, One Monsoon
Sarat Chandra CHAMARTHI#+, Venugopal VURUPUTUR, Sekhar MUDDU
Indian Institute of Science, Bangalore, India
Central India is affected by Indian Summer Monsoon (ISM) droughts. On a smaller scale, the Bundelkhand sub-region has experienced a series of droughts that have not coincided with ISM droughts. Analysis of daily rainfall data from the past century reveals two distinct drought types in Bundelkhand: Type-1 and Type-2. Type-1 droughts coincide with large-scale ISM droughts. Their evolution and drivers are well studied. In contrast, Type-2 droughts exhibit a different sub-seasonal evolution compared to Type-1. Their onset is in July, and the seasonal rainfall deficit is confined to Bundelkhand. Interestingly, parts of western India receive excess rainfall during Type-2 droughts. This study focuses on the spatiotemporal evolution and the potential drivers of Type-2 droughts. We observe that changes in large-scale circulation moisture convergence are consistent with the rainfall deficits in Bundelkhand. We also analyse the impacts of Type-2 droughts on the regional soil moisture (SM) and evapotranspiration (ET) patterns. SM deficit in Type-2 droughts prevails throughout the cropping season (June-October), leading to lesser vegetation cover and ET. We discuss the implications of our results in the context of a potential "negative feedback loop": decreasing ET leads to decreased atmospheric moisture, further reducing rainfall.
AS11-A022
Assessment of Observation Impact on Meteorological Forecasts for the 2018 Heat Wave in East Asia Using Observing System Experiments
Dae-hui KIM+, Hyun Mee KIM#
Yonsei University, Korea, South
Heat waves are extreme weather events that cause socioeconomic damage over extensive areas. Heat waves are consistently being observed in many regions of the world. However, in terms of short-range predictions, researches to reduce forecast errors for heat waves are insufficient. In this study, the effects of observations used for data assimilation (DA) on forecast errors for variables associated with heat wave were evaluated using observing system experiments with the Weather Research and Forecasting model and a three-dimensional variational DA. All observations used in DA contributed to reducing forecast errors for the meteorological variables (e.g., geopotential height, temperature, and wind) associated with heat wave. As the forecast time increased, upper atmospheric geopotential heights in East Asia and 2-m temperatures around Korea, Japan, and eastern China were underestimated. Upper atmospheric observations reduced forecast errors more than near-surface observations. Advanced Microwave Sounding Unit-A (AMSU-A) had the greatest impact in reducing underestimation of the 200 and 500 hPa geopotential heights and the second greatest impact in reducing underestimation of the 2-m temperature. Radiosonde observations had the greatest impact in reducing underestimation of the 2-m temperature. When specific observations were not used in DA, the Tibetan high and Northern Pacific high were contracted compared to the analysis from the experiment using all observations for DA, causing the clockwise upper atmospheric wind bias through the geostrophic relationship. Therefore, upper atmospheric observations are important for reducing heat wave simulation errors in East Asia. The results of this study could contribute to design an optimal observing system for heat wave forecasts in East Asia. Acknowledgments: This work was supported by a National Research Foundation of Korea (NRF) grant funded by the South Korean government (Ministry of Science and ICT) (Grant 2021R1A2C1012572) and the Yonsei Signature Research Cluster Program of 2023 (2023-22-0009).
AS11-A028
Anthropogenic Impacts on Summer Wetting Trend in Northwest China in Recent 60 Years
Rui HE#+, Yan GUO
Beijing Normal University, China
In the context of global warming, the phenomenon of warming and wetting occurred in northwest China. By comparing the three indexes of total precipitation, precipitation days and precipitation intensity between CN05.1 data, meteorology station from Meteorology Observation Network (CMA) and CMIP6 data, the results show that the precipitation trend in northwest China is significant, and both GHG forcing and AA forcing have some contribution. The results of water vapor decomposition of different external forcing show that the precipitation increasing in northwest China is mainly caused by the dynamic effects of greenhouse gases and anthropogenic aerosols. Further analysis shows that greenhouse gas emissions lead to the northward shift and westward extension of the Western Pacific subtropical high and the Mongolian high anticyclone anomaly, resulting in the easterlies on the north side of the Western Pacific subtropical high and the easterlies on the south side of the Mongolian High anticyclone, which together enter the northwest of China, thus weakening the westerlies and bringing more water vapor to the northwest of China. The anthropogenic aerosol forcing led to the weakening of the subtropical jet axis, resulting in the formation of anomalous anticyclone and cyclone in Central Asia, which affected the precipitation in northwest China.
AS11-A031
Impact of Warm SST on the August 2022 Heavy Rainfall Event in South Korea
Sujin KIM#+, Seok-Woo SON
Seoul National University, Korea, South
The Seoul metropolitan area in South Korea experienced a record-breaking rainfall on August 8th, 2022. The rainfall intensity reached up to 141.5 mm hr-1, causing significant property damages and life losses. The observations show that most clouds that entered the rainfall region passed over the Yellow Sea where sea surface temperature (SST) was over 1.5 ℃ warmer than climatology. In particular, on the night of August 8th when the heaviest rainfall occurred, small clouds formed over the Gyeonggi Bay and were merged with pre-existing rain clouds over the rainfall region. The present study investigates the possible effect of warm SST in the Yellow Sea and Gyeonggi Bay on the heavy rainfall event by performing a series of the Weather Research and Forecasting (WRF) model experiments. Previous studies have suggested that warm SST around the Korean Peninsula cloud lead to heavy rainfall event in land. However, the model experiments do not support them. When SST is replaced with climatology, colder than the observation, rainfall intensity becomes even stronger inland of the Korean Peninsula. When SST is increased by 1 ℃ and 2 ℃, the similar results are obtained. This results indicate a complicated pathway of SST impact on inland precipitation.
AS11-A032
What Makes Heavy Rainfall Events in South Korea More Catastrophic?
Gyuri KIM1#+, Chanil PARK2, Seok-Woo SON1
1Seoul National University, Korea, South, 2Boston College, United States
In South Korea, about 90% of the heavy rainfall events (HREs) are concentrated between June and September. Given the significant socio-economic impacts, understanding their climatological and dynamic/thermodynamic characteristics is of great importance. Although the developing mechanisms of HREs in South Korea are reasonably well known, the factors that determine the intensity of HREs need further research. The present study separates HREs into two groups: i.e., advisory HREs (aHREs), with 12-h accumulated rainfall between 110 mm and 180 mm and warning HREs (wHREs), with 12-h accumulated rainfall over 180 mm. These two groups are then compared from synoptic and thermodynamic perspectives. The synoptic features show no distinct difference between the two group, such as upper-level jet and baroclinic structure. The vertical motion diagnosed by solving the quasi-geostrophic omega equation is also similar. While dynamic omega is similar or even smaller in wHREs, diabatic omega has a slightly larger fraction. The two HREs differ in moisture transport. The atmospheric river is significantly stronger and better organized in wHREs, indicating that the thermodynamic conditions play a more crucial role in determining the intensity of HREs in South Korea.
AS11-A036
Classification of Heavy Rainfall Types and Detailed Characteristics Analysis in the Korean Peninsula Using Ground Observation Data
Ha-Yeong YU+, Myoung-Seok SUH#, Ji-su PARK, Yu-jeong SONG, Chansoo KIM
Kongju National University, Korea, South
With the growing impact of global warming, changes in the frequency and intensity of concentrated heavy rainfall events have been observed. To gain a detailed understanding of the heavy rainfall events occurring on the Korean Peninsula, cluster analysis was conducted. This study utilizes data collected over the past decade (2013-2022) from approximately 700 Automated Weather Stations(AWS) and Automated Surface Observation System(ASOS) stations to analyze precipitation patterns on the Korean Peninsula. Approximately 400 stations were chosen through a simple QC process, considering the missing rate. A comprehensive dataset was compiled, including variables such as rainfall duration (1/3/12 hours), frequency and intensity, and monsoon months (May-September). These variables were normalized to a median of 0 using the Robust transformation based on their deviation from the median. Three common clustering methods K-Means, Self Organizing Map, and Hierarchical Clustering were utilized, and the number of clusters was determined as six through Explained Cluster Variance (ECV) analysis, with K-Means showing the highest ECV. Cluster-1 displayed lower overall rainfall frequency, peaking in August, and was primarily located inland, excluding Gyeonggi-do areas. Cluster-2 exhibited higher rainfall frequencies in July and August, particularly in the western part of the inland region. Cluster-3 covered the eastern and southern coastal areas, including parts of Jeju, experiencing increasing rainfall frequencies from May/June to September. Cluster-4, located inland, demonstrated concentrated heavy rainfall, especially in August. Cluster-5, covering South and East Jeju along with parts of the southern coast, showed moderate and evenly distributed rainfall frequencies, with a peak in July. Finally, Cluster-6, encompassing Jeju and Geoje, consistently displayed high rainfall frequencies, especially in August and September, recording the highest number of heavy rainfall warnings. In this presentation, we will discuss more detailed characteristics of concentrated heavy rainfall occurrences for each cluster, including daily variations.
AS11-A039
Quantifying Flash Droughts Over China from 1980 to 2017
Kaiqi FU1+, Kaicun WANG2#
1Beijing Normal University, China, 2Peking University, China
Drought can develop rapidly over a short period, the so-called “flash drought”. The widely used standardized precipitation evapotranspiration index (SPEI), with traditional time scales longer than 1 month, cannot easily capture flash drought signals. Here, the SPEI with a 5-day (pentad) time scale was proposed to investigate flash droughts in China from 1980 to 2017. New criteria for flash droughts based on the high-resolution index were also developed. Flash droughts were stronger and longer in western and northern China. The intensity and duration of mild, moderate, and severe flash droughts increased during the study period, while severe flash droughts showed the largest increase. The high-resolution SPEI permits us to examine the process of a drought event, that is, how a mild flash drought develops into a severe flash drought. The contribution of precipitation deficit to the duration of mild flash droughts was 50%. As the intensity of flash droughts increased, the contribution of high temperature and increased net radiation to flash drought duration increased from 50% (mild flash droughts) to 74% (severe flash droughts). When flash droughts occurred, Northwestern China and Southwestern China were dominated by unusually weak water vapor transport, while Northeastern China, Northern China, Southern China, and Middle-Lower Yangtze were mainly dominated by abnormal downward motion. The downward motion was generally accompanied by clear sky conditions with fewer clouds, higher air temperature, and higher surface solar radiation, which accelerated and amplified flash droughts triggered by initial precipitation deficits.
AS11-A040
Improvement of Impact-based Forecast Using Multi Model Ensemble in 2024
Sug-gyoung YUN1#+, Hyun-Cheol SHIN1, Eun-Jung KIM1, Jong Im PARK1, Won Jun CHOI1, Jongchul HA1, Young-Cheol KWON1, KieWoung LEE2
1Korea Meteorological Administration, Korea, South, 2Environmental Prediction Research Inc., Korea, South
The Korea Meteorological Administration(KMA) is producing an impact-based forecast data based on both the deterministic forecast and ensemble forecast for heat waves (HW) and cold waves (CW). Ensemble prediction system for impact-based forecast is Multi-Model ensemble system which integrates Unified Model(global, global ensemble, local, and local ensemble models), ECMWF(global and global ensemble models) and KIM(Korean Integrated Model) global model(Hereafter, impact-based forecast based on the deterministic forecast and Multi-Model ensemble are called `DIMF` and ‘MEPS’, respectively.) MEPS determines the risk level by using the probability of occurrence of abnormal temperatures in Korea. Once maximum feels-like temperature(HW) or lowest temperature(CW) from all 93 Multi-Model Ensemble members were extracted, their probability distribution was determined by using a Generalized Extreme Value (GEV) distribution. The performance of MEPS for HW was compared with DIMF for July and August 2022. Verification was conducted by evaluating how well impact-based forecast level(safe, concern, caution, warning, alarm) was matched to the observed risk level in 175 regions. As a result, the ETS score of MEPS is better than DIMF at ‘caution’ and ‘warning’ level in HW but tend to overestimate HW, and the CW MEPS has slightly lower performance than DIMF. If the GEV distribution is used, definition such as a 2-day-lasting high/low temperature or temperature decrease cannot be reflected. Instead of the GEV, a method of obtaining the probability by the actual number of members satisfying the specific condition among the total number of ensembles was developed, and in this way, the tendency of overestimation of the HW in MEPS was slightly improved. In addition, two MEPS that using GEV and the new method about 2023 July to August are compared and the effect of the addition of the KIM ensemble on the performance is investigated.
AS11-A044
Assessing the Potential of Pin Photodiodes for Assembling Inexpensive and Compact Pyranometers
Kanta SUSAKI#+, Sayaka OUCHI, Makoto NAKAYOSHI
Tokyo University of Science, Japan
Urban solar radiation measurements are crucial for evaluating photovoltaic potential and human thermal sensation. Standard pyranometers are expensive and deploying them in multiple locations across the city is challenging. Urban climatological research demands inexpensive and compact solar radiation sensor. There are commercially available pyranometers using silicon photodiodes which are cheaper and downsized compared with standard ones. However, the wavelength covered by silicon photodiodes is 0.4 to 1.1 μm, which is limited to the narrow band for the entire wavelength range of shortwave radiation (0.29 to 3.0 μm); thus, applying pyranometers with silicon photodiodes to urban area might produce inaccurate data due to the varying spectral reflectance of building materials. Here, we scrutinized several types of pin photodiodes which are even less expensive and smaller than photodiode pyranometers. We assessed the viability of assembling pyranometers by ourselves using pin photodiodes. Pin photodiodes emit an electrical current corresponding to the light intensity. The sensitivity-wavelength range of a standard photodiodes is 0.7 – 1.1 μm, although this can vary among different products. Moreover, the size of the photosensitive areas also differs between various models. In this study, 12-day fixed-point outdoor observations were carried out using four varieties of pin photodiodes with different wavelength ranges and photosensitive areas to select the appropriate sensor type for solar radiation measurement. The results showed that the solar radiation measurement accuracy was superior in pin photodiodes with a larger photosensitive area and a wavelength range extending from ultraviolet to near-infrared. In addition, a mobile observation was performed to evaluate whether PIN photodiode pyranometers can be used in the complex radiant environment with different reflective properties of various building materials. The results showed that reflected solar radiation from vegetation and asphalt was not measured accurately with PIN photodiode pyranometers.
AS11-A053
Kilometer-scale Multi-physics Simulations of Heavy Precipitation Events in Northeast China
Hongyong YU1+, Andreas F. PREIN2, Dan QI3, Kaicun WANG4#
1Beijing Normal University, China, 2National Center for Atmospheric Research, United States, 3China Meteorological Administration, China, 4Peking University, China
Despite the fatal impact of heavy precipitation on people’s lives and the social economy, its accurate estimating remains challenging, especially in the Northeast China with the complex terrain and distribution of land and sea. In this study, we show how this issue can be addressed by kilometer-scale simulations as well as how to reduce computational costs. Three typical heavy precipitation events are simulated at 3 km horizontal resolution, and each event is simulated with 24 combinations of parameterization schemes and the simulations are evaluated with gauge observations and compared to satellite products (IMERG, CMORPH, and GSMaP). For the hourly maximum precipitation, the ensemble mean of simulations outperforms all satellite products in the cold vortex case and the heavy snowfall case, and is second only to the best-performing IMERG in the typhoon case. For average accumulated precipitation, the ensemble mean of simulations outperforms all satellite products in the cold vortex case and the heavy snowfall case, and is second only to the best-performing CMOPRH in the typhoon case. The physical configuration of the Morrison scheme and Mellor-Yamada-Janjic scheme without scale-aware cumulus scheme demonstrates the best overall performance. The microphysics scheme significantly impacts the maximum hourly precipitation, whereas the planetary boundary layer (PBL) scheme has a greater influence on the average accumulated precipitation. Employing a scale-aware cumulus scheme only has a pronounced impact on the average accumulated precipitation of the typhoon case. Additionally, the difference in precipitation changes caused by employing the scale-aware cumulus scheme on the microphysics scheme caused by different PBL schemes can exceed 10%. Conducting 24 simulations can be unnecessary because of similarities among simulations (e.g., patterns of accumulated precipitation). Referring to the estimation of data reconstruction to supplement additional simulations based on perturbing one physics scheme at a time resulting in 7 simulations is a recommended new strategy.
AS11-A056
Sensitivity of Summer Heavy Rainfall Events in Korea to Horizontal Resolutions and Physical Parameterizations Using WRF
Minseo YU#+, Seungyeon LEE, Ji Won YOON, Sujeong LIM, Seon Ki PARK
Ewha Womans University, Korea, South
In this study, we conducted sensitivity tests using the Weather Research and Forecasting (WRF) model for summer heavy rainfall cases in Korea in terms of horizontal resolution and physical parameterization schemes. The model employs one-way nesting with horizontal resolutions of 27 km, 9 km, and 3 km, respectively, over the Korean Peninsula (KP), using the NCEP FNL Operational Model Global Tropospheric Analyses with horizontal resolution of 1.0°x1.0° for the initial and boundary conditions. Two heavy rainfall events, occurred in July 2011 and August 2022 over central South Korea, have been considered. The selected cases occurred when blocking highs were located in the northeast of the KP. Over the KP, warm humid air was supplied to the low-level atmosphere from the North Pacific high (NPH), whereas cold and dry air flew into the mid-level of the troposphere along the trough located in the north of KP — causing strong instability. Low-level jet stream was combined with upper-level jet stream; the southwesterly, which supplied heat and water vapor, was lifted and formed tall convective clouds, resulting in heavy rainfalls. The dataset observed from the Automated Weather Stations (AWS) over KP was used to evaluate the model performance. The outcome presented shows importance of finding the best-performing scheme set and horizontal resolution for predicting extreme precipitation.
AS11-A058
| Invited
Compound Humid-heat Extremes: A Comprehensive Study of Changing Climate Trends in East Asia
Jina PARK#+, Jinho YOON
Gwangju Institute of Science and Technology, Korea, South
An inverse relationship exists between temperature and relative humidity (RH) generally, to be more precise with assumption that total water vapor in the atmosphere doesn’t change. In 2023 summer, however, both temperature and RH were elevated over Korea, deviating from the expected physical relationship. The combination of high temperature and high relative humidity induces many heat-related patients. Thus, this study aims to elucidate the variation in compound heat-humid extremes and to comprehend aspects that temperature alone cannot capture. Analyzing station data from the Korean Meteorological Administration (KMA), the time series of daily maximum temperature (Tmax) in Korea during the summer exhibits a consistent increase from 1973 to 2023. In contrast, the RH initially decreased until 2001 and subsequently began to rise. The period is divided into two periods: P1 (1973-2001) and P2 (2002-2023), identifying Tmax and RH. In P1, shows insignificant increase, while RH significantly decreases. In P2, both Tmax and RH exhibit significant increases, and the increase in RH is predominant in southern part of Korea. Extending this analysis to East Asia using ERA5, Japan, Manchuria region and southern China, and the maritime continent demonstrate similar trend to Korea. Since 2001, the rise in RH has brought the atmosphere close to saturation, leading to increased discomfort for humans and a higher incidence of heat-related diseases.
AS11-A060
Dynamic Pathway Linking Pakistan Flooding to East Asia Heatwaves
Zheng-Hang FU1#+, Wen ZHOU1, Shang-Ping XIE2, Ruhua ZHANG1, Xudong WANG1
1Fudan University, China, 2University of California San Diego, United States
In July–August 2022, Pakistan suffered historic flooding while record-breaking heatwaves swept southern China, causing severe socio-economic impacts. Similar extreme events have frequently coincided between two regions during the past 44 years, but the underlying mechanisms remain unclear. Here we use observations and a suite of model experiments to show that the upper-tropospheric divergent wind induced by convective heating over Pakistan excites a stationary anomalous anti-cyclone over eastern China, which further leads to persistent heatwaves. Atmospheric model ensemble simulation further indicates that this dynamic pathway linking Pakistan flooding and East Asia heatwaves is intrinsic to the climate system, largely independent of global sea surface temperature forcing. This dynamic connection via the upper troposphere westerly waveguide is robust, offering hopes to improve the sub-seasonal prediction of extreme events in East Asia.
AS11-A064
Irreversibility of Extreme Precipitation in East Asia Under Multi-scenario to Carbon Neutrality
Min-Uk LEE1+, Jong-Yeon PARK1#, Han-Kyoung KIM1, Young-Hwa BYUN2, Hyun Min SUNG2, Ji-Sook PARK1, Woojin JEON1
1Jeonbuk National University, Korea, South, 2National Institute of Meteorological Sciences, Korea, South
Extreme precipitation refers to a bipolar climate phenomenon in which a high amount of precipitation occurs in a short period or a drought persists for a long period. In a future climate with increased CO2 concentrations, the characteristics of extreme precipitation can undergo significant variations. This study focuses on East Asia (110°-150°E, 20°-50°N) and employs six indices from the Expert Team on Climate Change Detection and Indices (ETCCDI) to assess the reversibility of extreme precipitation events. The Carbon Dioxide Removal (CDR) experiment, simulated by the National Institute of Meteorological Sciences and the Korea Meteorological Administration (NIMS-KMA) climate model, involves increasing the CO2 concentration by 1% per year from the Pre-Industrial (PI) level and decreasing it from four different carbon-neutral points: A (44 years), B (51 years), C (70 years), and D (140 years) from the initial year. The NIMS-KMA simulation proves most effective among eight models from the Coupled Model Intercomparison Project Phase 6 (CMIP6). Results indicate that extreme precipitation indices respond nonlinearly to CO2 concentration, with intensity and frequency indices showing hysteresis. Reversibility is limited, and delayed carbon neutrality leads to increased irreversibility. Notably, the R99 frequency index exhibits the highest irreversibility, ranging from 10.61% to 29.50% from point A to point D. This suggests that postponing carbon neutrality may strengthen the central Pacific warming pattern, intensify subtropical high pressure in the northwest Pacific, and increase water vapor flow into East Asia.
AS14-A003
A Gridded Greenhouse Gases Emission Inventory Based on Multi-source Open Data
Rui WANG+, Yuzhong ZHANG#, Xinlu WANG, Shuang ZHAO
Westlake University, China
In 2021, Ministry of Ecology and Environment of the People’s Republic of China issued the “Pilot Work Plan for Carbon Monitoring and Evaluation” to implement carbon monitoring and assessment pilots for regions, cities, and key industries. The plan specified the need for inversion research on greenhouse gas (GHG) emissions, with a requirement for a prior inventory. Past studies commonly utilized the Emission Database for Global Atmospheric Research (EDGAR) as the prior inventory. However, numerous studies highlighted location mismatches in EDGAR, particularly for high-emission facilities, leading to significant errors in inversion results at the city scale. Therefore, ensuring an accurate and reliable gridded prior inventory at the city level is crucial for improving GHG inversion. In this study, a gridded emission inventory was developed for the predominant greenhouse gas in the atmosphere, namely carbon dioxide (CO2). The approach involved establishing a relationship between tabular GHG emission inventories and spatial proxy data to compile a gridded emission inventory at the city scale. The key challenge of the study lay in acquiring tabular emission inventories and spatial proxy data, especially the spatial location information and activity data for high-emission point sources, which are mostly confidential in the study area. The China City CO2 Emission Dataset (2020) served as the tabular emission inventory, while proxy data for non-point source emissions were derived from publicly available population data, road networks, land use, etc. Obtaining proxy data for point source emissions involved using web crawler technology. Points of interest extracted from online map APIs served as spatial proxy data, and the associated business registration information obtained through crawling was utilized as numerical weight data. Based on the proxy data, emissions from each sector were spatially allocated to the target grid to compile the gridded CO2 emission inventory.
AS14-A007
Global Power Emissions Database (GPEDv2): Emission Trends for Air Pollutants and CO2 of Global Power Plants During 1990-2020
Xinying QIN#+, Dan TONG, Ruochong XU, Xizhe YAN, Qiang ZHANG
Tsinghua University, China
Globally, the power sector is significant for air quality and climate. The past three decades have witnessed the dramatic expansion of global biomass- and fossil fuel-fired power plants, while the tremendously diverse power infrastructure shapes different air pollutant and CO2 emission characteristics. Here, a new version of the Global Power Emissions Database (GPEDv2) compiles unit-level air pollutant emissions (e.g. SO2, NOx, and PM2.5) during 1990-2020 based on bottom-up compilation approaches. By combining GPEDv2 constructed in this study and the previously developed China coal-fired power Plant Emissions Database (CPED), we find that global CO2 emissions from the power sector increased from 7.1 Gt in 1990 to 13.0 Gt in 2020, driven by the growth of power demand. In contrast to the 87% increase in CO2 emissions, global SO2 emissions of power plants decreased by 56% (from 50.4 Mt to 22.2 Mt), NOx only increased by 5% (from 19.6 Mt to 20.6 Mt), and PM2.5 decreased by 38% (from 3.8 Mt to 2.4 Mt). The disproportionately changes in air pollutant emissions were mainly due to the role of emission controls. With stringent emission control measures deployed in Europe, the United States and China, the predominant air pollutant emission contributor has shifted from Europe and the United States in 1990 (e.g. 65% for SO2) to India, the Middle East and North Africa and the Rest of Asia (excluding China) in 2020 (e.g. 61% for SO2). Our results suggest that developing countries that currently lack effective emission control should strengthen emission standards to substantially reduce air pollutant emissions from power plants.
AS14-A009
Regional Effect as a Probe of Atmospheric Carbon Dioxide Reduction in Southern China
Chengliang ZHANG#+
Jinan University, China
To mitigate climate change, China is striving to reduce its carbon dioxide (CO2) emissions before 2030 and has derived a series of national environmental policies to advocate green development. Analysing the changes in regional atmospheric CO2 concentrations could be more convincing in evaluating the impact of the associated strategies. In this study, a three-year continuous observation campaign of the atmospheric CO2 mole fraction was first conducted at the summit of the Nanling Mountains, southern China in 2015–2017 to probe the timely feedback of the implementation of the green policies of the government. The effects of regional emissions and removals on the CO2 mole fraction were subsequently analysed to explore the primary processes and regional contributions driving the background CO2 concentration. Approximately 86.4% of the observed values were filtered as background events, with average CO2 concentrations of 395.9 ± 6.8 ppm. The curve-fitting CO2 mole fraction showed a slight short-term descending trend (0.6–2.2 p.m. y− 1) that was rarely seen against the backdrop of a continuous rise of the global average over the years. In addition to the possible impacts of the changes in regional-scale CO2 sources and sinks, we inferred that the vigorously enforced sustainable development policies of the Chinese government should be accentuated to reduce CO2 emissions. Although the conclusion relies heavily on a relatively short dataset, this study may globally help the people to reduce carbon emissions.
AS14-A016
First Retrieval of Antarctic Methane Profiles from Gaofen-5/AIUS
Shuanghui LIU1#+, Jian XU2, Xiaoying LI1, Lanlan RAO1
1Chinese Academy of Sciences, China, 2National Space Science Center, Chinese Academy of Sciences, China
Methane (CH4) is the second most important greenhouse gas, following carbon dioxide. The analysis of the distribution of atmospheric methane concentrations on a regional scale has become a focal point of international research. Antarctica is the most vulnerable region of the global ecological environment. Monitoring of methane concentrations above Antarctica will provide a basis for assessing the impact of the greenhouse effect on the global climate. The Atmospheric Infrared Ultra-Spectral Sounder (AIUS) carried on the Gaofen 5 satellite is China’s first infrared occultation detector and is capable of observing ozone and various trace gases over Antarctica. This paper assesses the retrieval algorithm (based on the Optimal Estimation Method) for deriving atmospheric methane profiles over Antarctica in 2019 from the AIUS spectra. The results indicate that the deviation between the April, May, and December 2019 data and the ACE-FTS methane profiles is generally within ± 5% in the 12-60 km altitude range. In August, when the altitude is below 20 km, the retrieval accuracy is within ± 3%, and above 20 km, the accuracy gradually decreases with increasing altitude. The retrieval error of the November data is within ± 3% in the 10-60 km range. The methane concentration in Antarctica shows an obvious seasonal variation. The methane concentration in November and December is higher than in other months, which may be related to the significant release of methane from the melting of the Antarctic ice core during the summer.
AS14-A022
Impacts of Methane and Non-methane Near-term Climate Forcers Mitigation on Arctic and Global Surface Climate Change
Kim YOUN AH#+, Seok-Woo SON
Seoul National University, Korea, South
This study investigates the impacts of near-term climate forcers (NTCFs) mitigation on the near-term (2045-2054) global surface air temperature (SAT) and Arctic sea ice concentration (SIC) changes. Specifically, the impacts of methane and non-methane NTCFs are analyzed by examining five climate models from three Shared Socioeconomic Pathways (SSPs) scenarios: control scenario (SSP3-7.0), low non-methane NTCF emission scenario (SSP3-7.0-lowNTCF), and low all NTCF emission scenario (SSP3-7.0-lowNTCFCH4). The impacts of all NTCF and non-methane NTCF mitigations are defined as the changes in SAT and SIC between the SSP3-7.0-lowNTCFCH4 and SSP3-7.0 scenarios and between the SSP3-7.0-lowNTCF and SSP3-7.0 scenarios, respectively. The methane mitigation is also isolated by the difference between the SSP3-7.0-lowNTCFCH4 and SSP3-7.0-lowNTCF scenarios. Global SAT is projected to increase under the control scenario, which is based on regional rivalry over carbon emission policies, with the warming being the largest in the Arctic. The methane mitigation reduces global warming, while the non-methane NTCF mitigation strengthens global warming. The former is qualitatively stronger than the latter, especially in the Arctic from late fall to early winter (October to January). Consistent with the change in Arctic SAT, Arctic SIC is projected to increase with methane mitigation, but decrease with non-methane NTCF mitigation. These results suggest that air quality control policies, accompanied by methane reduction, are necessary to slow down global warming and preserve Arctic sea ice.
AS14-A023
Physical Processes Influencing the Asian Climate Due to the Black Carbon Emissions Over China and India
Feifei LUO#+
Chengdu University of Information Technology, China
Current and expected future aerosol emission changes are particularly strong in East and South Asia, where high population densities imply high potential climate risk. Hence, there is an urgent need for improved knowledge about the near-term influences of changes in aerosol emissions. Here we have developed a set of Systematic Regional Aerosol Perturbations (SyRAP) using the reduced complexity climate model FORTE 2.0 to explore the effects of aerosol-driven climate change. Results show that the increased Black Carbon(BC) concentrations over China and India lead to decreased local surface Temperature (Ts) and precipitation, with seasonal differences in the spatial distribution. Chinese (Indian) BC emissions also impact on Indian (Chinese) climate in specific seasons. The changes of shortwave radiation (SW) dominate the surface cooling and the lower tropospheric warming due to the absorption of BC. The reductions of column-integrated diabatic cooling lead to the decreased local precipitation, while the changes in atmospheric circulation play an opposite role (weakened EAWM, enhanced EASM and ISM). The horizontal/vertical distributions of air temperature anomalies can induce the changes in cloud cover and atmospheric circulation, which further impact on the radiation flux and precipitation. Additionally, the increased surface albedo in winter is helpful to decrease Ts and precipitation.
AS14-A026
Changes in Factors Affecting Future Air Quality in Korea Under the Carbon Net-zero Scenario
Minju YEO#+, Ja-Ho KOO
Yonsei University, Korea, South
Recently, there has been significant global interest in carbon neutrality. The Intergovernmental Panel on Climate Change (IPCC) Special Report approved in 2018 set a target to limit the temperature increase to 1.5°C or less by 2100, emphasizing the need to achieve carbon neutrality by 2050. However, the World Meteorological Organization (WMO) announced in 2023 that the global average temperature had already increased by 1.4°C compared to pre-industrial levels. During the 28th Conference of the Parties (COP) to the United Nations Framework Convention on Climate Change (UNFCCC) in 2023, the first Global Stocktake (GST) was conducted to assess progress towards the goals of the Paris Agreement, outline future directions, and it concluded that the implementation of the Paris Agreement is insufficient across all sectors and has not reached the specified levels. As a result, there should be increased efforts in climate change mitigation and carbon neutrality. The Republic of Korea (Korea) has announced two carbon neutrality scenarios with a goal of achieving net-zero by 2050 in 2022. The transition from fossil fuel-dominated energy supply to renewable and environmentally friendly energy sources is expected to lead to a reduction in fossil fuel consumption, consequently influencing air quality. Notably, among the factors affecting air quality, such as Total Energy Supply, Carbon Intensity, Control Status, and Local Air Pollutant Emission Effects, a substantial change is anticipated in Carbon Intensity. This study examines the predicted changes in each factor affecting air quality under carbon neutrality scenario in Korea and comprehensively estimates the expected air quality changes, particularly in the concentrations of primary air pollutants such as carbon monoxide and sulfur dioxide.
AS16-A002
Aerosol Morphology and Phase Separation: Observation from Northeast Asia's PM2.5 in Autumn 2023
Daeun KIM1+, Kyounghee KO1, Changjoon SEONG1, Zhijun WU2, Jiyi LEE3, Kwangyul LEE4, Jun-Young AHN4, Kyoung-Soon JANG5, Changhyuk KIM6, Natsagdorj AMGALAN7, Mijung SONG1#
1Jeonbuk National University, Korea, South, 2Peking University, China, 3Ewha Womans University, Korea, South, 4National Institute of Environmental Research, Korea, South, 5Korea Basic Science Institute, Korea, South, 6Pusan National University, Korea, South, 7National University of Mongolia, Mongolia
The morphology and phase separation of aerosol particles play a crucial role in scattering and absorbing solar radiation, significantly impacting atmospheric energy balance and climate processes. Therefore, understanding these characteristics is important for predicting aerosol behavior in atmospheric chemistry and climate change. Although interest in this area is growing, significant gaps remain in studies examining the morphology and phase separation of ambient aerosols. To bridge this gap, fine particulate matter (PM2.5) was collected from four Northeast Asian sites (Seoul, Seosan, Beijing, and Ulaanbaatar) in the autumn of 2023 using a high-volume air sampler. These PM2.5 particles were dissolved in a water and methanol solution, nebulized onto a hydrophobic substrate, and placed in a flow-cell for observation. The particles were analyzed by optical microscopy as the relative humidity (RH) decreased. Interestingly, as the RH decreased, a variety of morphologies and phase separation were observed in the ambient aerosols. It is anticipated that these findings will greatly enhance knowledge about how aerosols behave in the context of atmospheric chemistry and climate change, highlighting the importance of further research. The results will be presented.
AS16-A003
The Temporal-spatial Distribution of PM2.5 in Central Taiwan
Ming-Tung CHUANG#+
Academia Sinica, Taiwan
In order to analyze the physicochemical mechanisms affecting the variation of PM2.5 in urban air, we established the UAPRS (Urban Air Pollution Research Site) in Taichung City, the second largest city in Taiwan. The WRF/CMAQ model was used to simulate the impacts of various emissions on the central region of Taiwan. Taking the high pollution event from November 3 to 6, 2021, which was caused by the prevailing easterly or southeasterly winds being blocked by the Central Mountain Range, which resulted in the formation of a weak wind zone in the central region of Taiwan. The wind speed is often weak near the ground at night and the height of the boundary layer is low, one of the reasons for the accumulation of PM2.5 near the ground in the Dadu Mountain on the west side of Taichung City, and the increase in PM2.5 concentration. The model evaluation shows that the sources of pollution in Taichung City are not only the boundary condition, but also the point, line and surface effects. SO42- is mainly generated from point sources in Taichung City, mainly from Emission, from medium of H2O2, Fe, Mn, and O3; NO3- is also mainly generated from point sources in Taichung City, and HNO3 formed at noontime and ANO3 at others; NH4+ from Taichung area source; OM is more complex, mainly from line emission of Taichung City, and other sources such as area and point emissions of Taichung City, and emissions from Changhua County. The most important mechanism is low volatility/semivolatile oxidized combustion OC, which produced most OC in the midday hours, followed by low volatility/semivolatile POA, which may produce OC in the morning or evening; and EC, which mainly comes from line sources in Taichung City and Changhua County.
AS16-A010
Comparison of Aerosol Acidity Averaging Methods with Different Temporal Resolutions and Recommended Conversion Methods
Xiao TIAN#+
Nankai University, China
Aerosol acidity is a key parameter in aerosol chemistry. It can alter the phase partitioning of semi-volatile species, chemical reaction rate, and trace metal solubility, which further impact human health, climate, and terrestrial and oceanic ecosystems. Aerosol acidity is usually characterized by aerosol pH, which is defined as the negative logarithm of the hydrogen ion activity within aerosol liquid water with a base of 10. It is notable that existing studies typically employ the arithmetic mean of pH to represent the average trend of aerosol pH, in fact, this is inappropriate. In this work, the probability distributions of the aerosol pH and aerosol water content (AWC) in the North China Plain (NCP) for winter 2018, as well as their joint probability distribution, were mapped based on GEOS-Chem simulations. Considering the interdependence between aerosol pH and aerosol water content, we proposed an AWC-based pH averaging approach. The results showed that the pHweighted mean and pHmean during the study period differed by nearly 2 units. Moreover, due to the buffering effect of NH3/NH4+, this difference become significantly stabilized when the relative humidity (RH) surpasses 50%. In addition, comparing the variations between different averaging methods at diverse temporal resolutions (3-hour, daily, weekly, monthly, and 3-month) reveals that insufficient temporal resolution may result in the transient fluctuations in AWC to be smoothed. This, in turn, can lead to an overestimation of aerosol pH and an underestimation of AWC. Consequently, it is advisable to use hourly-resolution datasets as the inputs for thermodynamic modeling, and employing the AWC-weighted method when reporting the average pH throughout the study is recommended.
AS17-A009
A Study on the Possibility for Region-based Lightning Detection Using Geostationary Meteorological Satellite
Seung-Hee LEE+, Myoung-Seok SUH#
Kongju National University, Korea, South
Lightning is a phenomenon caused by the discharge of positive and negative charges within clouds, and cloud-to-ground lightning poses significant risks to human life and property. Therefore, understanding the characteristics of clouds where lightning occurs and detecting the areas of lightning occurrence are important. In this study, we investigated the possibility for region-based lightning detection using data from the high spatiotemporal resolution geostationary meteorological satellite GK2A (GeoKompsat-2A) and ground lightning observation equipment LINET (LIghtning NETwork). To use datas with different spatial and temporal resolutions together, lightning events within 5 minutes before and after the satellite observation time were defined as occurring at the satellite observation time. Spatially, the satellite pixel with the shortest distance was found based on the lightning occurrence point, and the pixel with the lowest brightness temperature of the infrared channel in the 15X15 area based on the pixel was defined as the lightning pixel to match time and space. The study selected 12 cases based on the frequency of lightning occurrences during the summer of 2020-2021 (June to August). Among these, 10 cases were designated as training cases, and 2 as validation cases. Lightning primarily occurs in clouds rising near the tropopause due to deep convection. Therefore, to examine the relationship between lightning and brightness temperature, the study analyzed the brightness temperature and lightning occurrence probability graph for the training cases. The results indicated a higher probability of lightning occurrence when the infrared channel brightness temperature was lower, and the brightness temperature difference was close to 0K. Currently, the plan is to derive a regression equation for calculating the probability of lightning occurrence using the training cases. Subsequently, a region-based approach for lightning detection will be designed based on the characteristics of these lightning pixels, and the performance of the regression equation will be evaluated.
AS17-A011
Research on the Relationship Between the Morphological Characteristics of Lightning Channels and Turbulence Dynamics in Thunderstorms
Yang ZHANG1#+, Yurui LI2, Yijun ZHANG2, Yanfeng FAN1
1Chinese Academy of Meteorological Sciences, China, 2Fudan University, China
Turbulence in thunderstorms affects the charge distribution, which in turn affects the lightning channel morphology. Thus, the lightning channel morphology can reflect the characteristics of turbulence. The current understanding of the correlation between the two is still limited to the relationship between macroscopic thunderstorm dynamic characteristics and lightning activity. In this paper, based on three-dimensional radiation source localization data from the Lightning Mapping Array and radar-based data, our analysis shows that the overall morphology and detailed morphology of the lightning channel correspond to different eddy dissipation rate (EDR) characteristics. Lightning with complex channel morphology occurs in regions with large EDRs. In single lightning events, channels that extend directly within a certain height range without significant bifurcation and turning tend to propagate in the direction of decreasing EDRs, while channel bifurcations and turns usually occur in regions with large radial velocity gradients and large EDRs. This study shows the relationship between channel morphology and thunderstorm dynamics and provides a new method for the direct application of channel-level localization data to understand thunderstorm dynamics characteristics.
AS17-A014
Using Radar Retrieved Winds and Thermodynamic Variables to Improve Short-term Quantitative Precipitation Forecast: Case Studies of Severe Weather Storms
Tzu Jui CHOU#+, Yu-Chieng LIOU
National Central University, Taiwan
This research aims to investigate using radar-retrieved variables to improve short-term rainfall forecasts over mountainous regions. Two advanced and fully developed retrieval algorithms named WInd Synthesis System using Doppler Measurement (WISSDOM) and Terrain Permitting Thermal Retrieval Scheme (TPTRS) are used to retrieve the three-dimensional wind, pressure and temperature fields over complex terrain. In addition, the moisture field is estimated based on the statistical relationship between sounding-observed relative humidity and radar reflectivity. The cases selected for analysis are from IOP#5 of TAHOPE 2022, representing an afternoon thunderstorm case over northern Taiwan, and SoWMEX IOP#8, representing a squall line case over southern Taiwan. Results of retrievals in two cases indicate that strong upward motion is consistent with the convergence. In addition, the regions with positive/negative temperature perturbations also coincide with strong updraft/downdraft in the IOP5 case due to the latent heat release. On the other hand, near the surface, the negative temperature perturbation represents the cold pool and high-pressure structure, respectively. Compared with the observations, the model can well capture significant areas of accumulated rainfall for up to three hours in the IOP5 case and six hours in the IOP8 case. The results also imply that the model spin-up time can be effectively shortened after directly assimilating the retrieved kinematic, thermodynamic, and moisture fields.
AS18-A001
Variations of GNSS-derived PWV Under the Influence of ENSO and Its Responses to Floods and Droughts
Yumeng HAO+, Kefei ZHANG#
China University of Mining and Technology, China
EI Nino-Southern Oscillation (ENSO) is a complex ocean-atmosphere interaction phenomenon leading to extreme weather events worldwide and water vapor plays a vital role in the evolution of ENSO. Recently, the Global Navigation Satellite Systems (GNSSs) have been regarded as a relatively new mechanism for quiring high spatial and temporal resolution water vapor due to its unique features of high accuracy, global coverage and all-weather operation capability. However, GNSS derived precipitable water vapor (PWV) has not been well researched for its potential in the study of ENSO. This research is hence to investigate the correlation between ENSO and GNSS-derived PWV in a global context, in particular the variations of PWV time series in response to ENSO before and during floods and droughts. In this study, composite analysis and singular spectrum analysis (SSA) were used to obtain the non-linear trends of PWV anomalies at 16 GNSS stations close to the sea for Nino and Nina years with moderate and higher intensities. Then, the relationships between these non-linear trends of PWV anomalies and ONI show that the correlations on the western Pacific and the eastern Indian Ocean are significantly negative, on the contrary, the correlations on the eastern Pacific and the western Indian Ocean are positive. These results show well consistent with the variations of precipitation in response to ENSO, which to some extent reflect the drought and flooding in these areas. A case study conducted at the COCO station near Indonesia shows that the non-linear trend of the PWV anomalies depicts the evolution of one severe drought event and one severe flood event occurring in Indonesia. These results suggest that GNSS-derived PWV together with other climatic variables can be used as an indication of the evolution of ENSO events and as a possible indicator of drought and flood occurrence.
AS18-A010
Analysis of Ground-based GNSS Real-time Water Vapor Retrieval Accuracy Based on Different Real-time Products
Wenliang GAO#+, Guigen NIE, Yu GUO
Wuhan University, China
Ground-based global navigation satellite system (GNSS) water vapor monitoring technology is characterized by low cost and high temporal and spatial resolution compared to traditional water vapor detection methods. In GNSS meteorology, real-time water vapor retrieval is required for weather forecasting applications such as extreme precipitation and typhoon tracks. In this study, real-time orbit and clock error products provided by various analysis centers, such as IGS, CNES, etc., are used to obtain tropospheric zenith delay (ZTD) values using the real-time precision point positioning (PPP) technique. The accuracy of the real-time ZTD estimation is analyzed by comparing it with the high-precision ZTDs calculated using the final products. Then we extracted the tropospheric wet delay (ZWD) values from the ZTD to further calculate the atmospheric precipitable water vapor (PWV) values, and compared them with the PWV calculated from the radiosonde data to analyze the accuracy of the water vapor calculated from the different real-time products, as well as their spatial and temporal properties.
AS18-A013
An Investigation Into Real-time Retrieval of Precipitable Water Vapor
Peng SUN+, Kefei ZHANG, Suqin WU#, Minghao ZHANG, Longjiang LI
China University of Mining and Technology, China
Water vapor, an important greenhouse gas in the troposphere, is closely related to weather and climate phenomena that affects daily life of human beings. Accurately determining the water vapor content helps us deepen the understanding of atmospheric dynamic processes. Precipitable water vapor (PWV) is an essential parameter for measuring the content of water vapor, and some researchers have focused on real-time PWV retrieval for time-critical meteorological applications. This contribution focuses on the algorithm, software development, and accuracy evaluation of real-time PWV retrievals based on the Global Navigation Satellite Systems (GNSS) precise point positioning (PPP) technique. First, an enhanced multi-GNSS real-time PPP software was developed to estimate the zenith tropospheric delay (ZTD) over the GNSS station. Second, an improved ZHD lapse-rate model was developed to enhance the accuracy of VMF1/VMF3-predicted ZHD. Third, an investigation into the modeling of the weighted mean temperature was introduced. Finally, the accuracy of real-time GNSS PWV was analyzed.
AS19-A009
Bioaerosol
Rui ZHANG#+
Dalian University of Technology, China
Bioaerosols, are also known as primary particles (PBA), are a subset of atmospheric particles. Bioaerosols are either living or dead airborne particles originating in plants, animals, and microorganisms. Early warning and management are crucial for controlling the spread of bioaerosols. Herein, we developed aptamer (SA)-based electrochemical biosensors for rapid and sensitive detection of bioaerosols. The platform features two components: DNA aptamers for their ability to bind and undergo target-induced assembly on the chip surface and functional materials for their ability to provide a high surface density of aptamer-binding sites and facilitate the electron transfer at the biointerface. The sensors were capable of detecting targets with a detection limit to picomole level. Furthermore, this design allowed the detection of ATP in cultured microorganisms and collected real bioaerosols. Overall, this strategy of interfacing DNA aptamers with composite materials represents a versatile approach for the ubiquitous detection of biochemical targets in bioaerosols.
AS24-A001
Connection Between the Tropical Pacific and Indian Ocean and Temperature Anomaly Across West Antarctic
Ping ZHANG+, Anmin DUAN#
Chinese Academy of Sciences, China
West Antarctic and the Antarctic Peninsula have experienced dramatic warming in austral spring since the 1970s. Using observations and the Community Atmosphere Model version 4 (CAM4), this study explores the physical mechanism by which the tropical Pacific and Indian Ocean temperature anomaly mode (PIM) affects the dipolar surface air temperature (SAT) anomalies across the West Antarctic in austral spring. The positive phase of the PIM, characterized by positive sea surface temperature anomalies (SSTAs) in the tropical central-eastern Pacific and western Indian Ocean and negative SSTAs in the Maritime Continent, can generate two branches of stationary Rossby wave trains propagating from the tropical central Pacific and southeastern Indian Ocean to the West Antarctic, with an anticyclonic anomaly appearing over the Amundsen Sea. The northerlies advect warmer air to the Ross–Amundsen Seas, but southerlies advect colder air to the Antarctic Peninsula–Weddell Sea, resulting in the dipole of SAT anomalies over the West Antarctic. In this process, the role of tropical central-eastern Pacific SSTAs dominate, and it is amplified by the SSTAs around the Maritime Continent. The SSTAs in the western Indian Ocean combined with the SSTAs over the Maritime Continent further contribute to the western pole of the SAT. Only simulation that includes a prescribed PIM forcing can exactly reproduce the observations of the dipolar SAT response across the West Antarctic, indicating the need to treat the tropical Pacific and Indian Oceans as a unified whole.
AS24-A004
Atmospheric Rivers in the Southern Hemisphere and Its Impact on the Interannual Variations of Sea Ice in the Antarctic
Kyu-Myong KIM1#+, Alexa HENNY1,2, Dong WU1, Young-Kwon LIM1,3, Jae LEE1
1NASA Goddard Space Flight Center, United States, 2NASA Postdoctoral Program, United States, 3University of Maryland, Baltimore County, United States
Atmospheric Rivers (AR) accounts for more than 90% of poleward moisture transport across midlatitudes of both hemispheres and has a crucial impact on hydrological cycle and surface mass balance over the Antarctic ice sheets. Here we investigate the interannual variations of atmospheric river and associated poleward moisture transport in austral summer and winter using 43-year MERRA-2 reanalysis data. 3-hourly integrated water vapor transport (IVT) is used to detect AR with latitude dependent thresholds of IVT to better detect AR-like features in the polar regions. In austral summer, first two modes from eigen analysis of sea ice are highly correlated with AR activities and poleward moisture transport in the Weddell Sea and Ross Sea, respectively. In austral winter, AR impact is limited to the sea ice in the Weddell Sea. In addition, ZW3 circulation is highly correlated with sea ices in both regions in austral winter. To better understand the effect of AR on sea ice in different parts of the Antarctic, AR genesis regions are identified and AR propagation from the genesis regions are analyzed. Based on 3-hourly AR statistics, four main AR genesis regions in the southern hemisphere (i.e., southern Africa and southwestern Indian Ocean, southern Pacific Ocean, South America monsoon region, and Australia) are identified. The variations of AR frequency and intensity at each genesis regions and associated patterns of atmospheric circulations and its impact on the poleward moisture transports as well as surface heat and radiation flexes will be discussed.
AS24-A005
Antarctic Boundary Layer Study with CALIPSO and In-situ Measurements
Yuekui YANG1#+, Manisha GANESHAN2, Stephen PALM3
1NASA Goddard Space Flight Center, United States, 2Morgan State University, United States, 3Science Systems and Applications, Inc, United States
Antarctica is experiencing unprecedented regional warming and accelerated loss of mass. Planetary boundary layer processes play a key role in these changes. The Antarctic boundary layer often features a strong surface-based inversion (SBI) due to the semi-permanent net radiation deficit at the surface. The stably stratified atmosphere can affect not only mixing process but also interact with clouds and blowing snow. This paper presents the work on Antarctic boundary layer analysis using co-located data from dropsonde, radiosonde, and the CALIPSO satellite, where the in-situ observations provide high resolution vertical atmosphere profile and CALIPSO provides the cloud and blowing snow information. Results show that 1) the Antarctic boundary layer demonstrates clear regional signatures. Factors such as wind shear, radiative forcing, terrain and air mass influences, play a role in the boundary layer mixing; 2) signals of interaction between cloud and the boundary layer are clearly observed. Increased downwelling longwave radiation during cloudy cases evidently abate radiative cooling losses during all seasons, contributing to surface and boundary layer warming, especially during spring, fall, and winter; 3) blowing snow, which is a common phenomenon over the Antarctic continent, can serve as an indicator of boundary layer mixing. SBI strength plays a role in the blowing snow layer development.
AS24-A011
Impacts of the MJO on the Antarctic Atmospheric Rivers
Jihae KIM+, Myong-In LEE#
Ulsan National Institute of Science and Technology, Korea, South
Atmospheric Rivers (AR) are globally occurring phenomena in which water vapor generated in tropical oceans flows towards continents through jet streams, spanning hundreds to thousands of kilometers. When AR events occur, they transport substantial amounts of water vapor, leading to heavy rainfall and snowfall in inland. In the Antarctic, the occurrence of atmospheric rivers results in the melting of ice shelves, the formation of polynya in the Antarctic sea ice, and localized accumulation of snow on glaciers. Previous studies have indicated that atmospheric rivers frequently occur due to tropical cyclones and are associated with climate modes on various timescales, such as the Southern Annular Mode and Pacific-South American pattern 2 on interannual timescales, and the Pacific Decadal Oscillation on decadal timescales. However, the analysis on the phenomenon related to intraseasonal timescale is rare. Therefore, this study diagnoses the relationship between the Madden-Julian Oscillation (MJO) characteristics and the frequency of atmospheric rivers in the Antarctic. The MJO is the most prominent atmospheric oscillation, accounting for 20-30% of the intraseasonal variability in tropical regions. It has a temporal cycle of 30-70 days and exhibits a slow eastward propagation with a speed of approximately 5 m/s. In this study, MJO phases are categorized into four groups (phases 2-3, phases 4-5, phases 6-7, and phases 8-1). In phases 4-5, the vertically integrated water vapor transport (vIVT) flowing into the Antarctic Peninsula (AP) is large, and the surface temperature is increasing in the eastern part of AP, which can accelerate the melting of glaciers.
AS24-A014
Surface Radiative Effects of Arctic Summer Clouds Observed in the Arctic Ocean
Joo-Hong KIM1#+, Chang-Kyu LIM1, Sang-Woo KIM2
1Korea Polar Research Institute, Korea, South, 2Seoul National University, Korea, South
During the Arctic summer expeditions of the Korea Polar Research Institute IBRV Araon, synthetic ship-borne surface and upper-air observations were carried out by the radiosonde balloons, micro-pulse lidar, and surface automatic weather station. Valuable in-situ observation data were obtained over a variety of surface and synoptic conditions, including upper-air met variables (temperature, humidity, pressure and horizontal winds), backscattered signals from clouds, and surface met variables and downward radiative fluxes. These data with reanalysis are used to study the surface radiative effect of clouds over the Arctic Ocean in late summer. Cloud base heights and cloud base temperatures are estimated from the combination of micro-pulse lidar backscatter signals and radiosonde temperature profiles. Results show the cloud base heights are close to the surface during the cold period, but become higher as the temperatures warm. A positive linear relationship dominates between cloud-controlled downward longwave radiative flux and surface air temperature regardless of the sea ice concentration ranges (high: ≥70%, intermediate: 10-70%, low: <10%), but the presence of the warm and clear period obscures the linear relationship.
AS24-A017
Development of the KOPRI Seasonal Forecasting System with NCAR CAM6
Sang-Yoon JUN1#+, Joo-Hong KIM1, Taewon PARK2, Yonghan CHOI1, Eui-Seok CHUNG1, Min-Hee LEE1, Hye Sun CHOI1, Solji LEE1
1Korea Polar Research Institute, Korea, South, 2Chonnam National University, Korea, South
We developed a seasonal climate forecasting system by utilizing the National Center for Atmospheric Research's (NCAR) Community Atmosphere Model version 6 (CAM6) and incorporating sea surface temperature and sea ice concentration boundary data from the National Centers for Environmental Prediction's (NCEP) Climate Forecast System (CFS) reforecast dataset. In the 4-month winter hindcast spanning from 2000 to 2019, initialized on November 1st each year with 11 ensemble members, it was found an anomaly correlation coefficient (ACC) of 0.2 for the detrended winter (December-January-February) mean surface air temperature (SAT) when compared to reanalysis data in the Arctic region (north of 67°N). The climate feedback response analysis method (CFRAM) indicated that cloud-radiation feedback had the most significant impact on SAT bias in the Arctic. Given the similarity in the relationship between Arctic and East Asia SAT within the hindcast results and observations, this implies that improving the accuracy of Arctic cloud simulation could enhance the SAT prediction skill in both the Arctic and East Asia regions.
AS30-A007
Analysis of Typhoon Characteristics and Factors Influencing Precipitation in Shandong Province, China, in the Past 20 Years
Yi ZHANG#+, Yue GAO
Nanjing University, China
Shandong Province in China, with three sides facing the sea, is the province in the northern region of our country that is most affected by typhoons (TC). The number of typhoons affecting Shandong Province is not as high as those along the southeast coast. However, once they occur, they are often interact with mid-latitude weather systems, causing widespread torrential rainfall. Against the background of global warming, TCs can form at higher latitudes, and there is a trend for the location of their maximum intensity to shift towards the poles. Northern China is more susceptible to the impact of typhoons than before, and the typhoon precipitation in this region needs to be widely concerned. This study selected 43 typhoons that have affected Shandong Province from those generated in the Northwest Pacific since 2000 for statistical analysis. The results indicate that on average, there are 2 typhoons that affect Shandong per year, with a concentration between July and September. Most of the typhoons that affect Shandong Province are transitioning typhoons, and their movement speed during the impact period is relatively fast. The intensity of these typhoons is weakened compared to their maximum intensity during their lifetime. The intensity of precipitation is mainly affected by the typhoon's path, movement speed, and intensity,the transitioning status also plays a role, specifically: the shorter the distance between the typhoon center and Shandong, the slower the movement speed, and the stronger the intensity, the greater the precipitation in Shandong during the impact period. Based on these factors, this study further derived a quantitative estimation formula for extreme precipitation in Shandong Province. Due to the influence of environmental vertical wind shear, heavy rainfall in Shandong caused by typhoons with smaller (larger) path curvature mainly occurs on the left (right) side of the typhoon's movement path.
AS30-A008
Is the Outflow-layer Inertial Stability Crucial to the Energy Cycle and Development of Tropical Cyclones?
Yuanlong LI#+
Nanjing University, China
This study revisits the issue of why tropical cyclones (TCs) develop more rapidly with lower environmental inertial stabilities, using ensemble axisymmetric numerical simulations and energy diagnostics based on the isentropic analysis, with the focus on the relative importance of the outflow-layer and boundary layer inertial stabilities to TC intensification and energy cycle. Results show that although lowering the outflow-layer Coriolis parameter and thus inertial stability can slightly strengthen the outflow, it does not affect the simulated TC development, whereas lowering the boundary layer Coriolis parameter largely enhances the secondary circulation and TC intensification as in the experiment with a reduced Coriolis parameter throughout the model atmosphere. This suggests that TC outflow is more likely a passive result of the convergent inflow in the boundary layer and convective updraft in the eyewall. The boundary layer inertial stability is found to control the convergent inflow in the boundary layer and depth of convection in the eyewall and thus the temperature of the energy sink in the TC heat engine, which determines the efficiency and overall mechanical output of the heat engine and thus TC intensification. It is also shown that the hypothesized isothermal and adiabatic compression legs at the downstream end of the outflow in the classical Carnot cycle are not supported in the thermodynamic cycle of the simulated TCs, implying that the hypothesized classical TC Carnot cycle is not closed. It is the theoretical maximum work of the heat engine, not the energy expenditure following the outflow downstream, that determines the mechanical work used to intensify a TC.
AS30-A010
Relationship Between Tropical Cyclone Size Asymmetry and Anomalous Motion
Xiaodong TANG#+, Huilin LI, Juan FANG
Nanjing University, China
Challenges persist in accurately predicting sharp changes in tropical cyclone (TC) motion over a short period of time, even with the employment of state-of-art forecasting technologies. The precise connection between these sudden changes and specific TC structure remains unclear. Here, we delve into the relationship between TC asymmetry (TCA) of outer-core size and anomalous motion, using best-track data spanning the period from 2001 to 2022. Results indicate that TCs characterized by lower TCA tend to display more pronounced deflections than their normal motion. Furthermore, fast-moving TCs exhibit heightened asymmetry and a propensity to accelerate, whereas slow-moving ones lean towards greater symmetry. In addition, TCs demonstrating substantial angular deviations are more prevalent at lower speeds, while fast-moving ones rarely generate anomalous deflections. These findings provide valuable insights into the potential impact of TCA on anomalous TC motion, which can ultimately be used to enhance the accuracy of TC track forecasting.
AS30-A011
Predictability of the Most Long-lived Tropical Cyclone Freddy (2023) During Its Westward Journey Through the Southern Tropical Indian Ocean
Jian-Feng GU1#+, Masaki SATOH2,3, Lili LEI1, Jianping TANG1, Zhe-Min TAN1, Yuqing WANG4, Jing XU4
1Nanjing University, China, 2The University of Tokyo, Japan, 3Yokohama National University, Japan, 4Chinese Academy of Meteorological Sciences, China
In 2023, Storm Freddy emerged as the most long-lived tropical cyclone (TC) in record, lasting 35 days over the southern tropical Indian Ocean and spanning both weather and sub-seasonal to seasonal time ranges. The primary objective of this study is to understand the factors contributing to the poor predictability of Freddy in forecasts spanning over 2 weeks. This holds significant importance as our understanding about the ability of the numerical models to predict long-lived TCs remains limited. Using over 7,000 global ensemble forecasts from five global Numerical Weather Prediction (NWP) centers and a high-resolution regional model, we identified three key factors contributing to the limited predictability of Freddy: the strength of the Mascarene High, the position of Storm Dingani (2023), and the size of Freddy. In large track-error results of the global forecasts and regional simulations for Freddy, the strength of the Mascarene High was underestimated, Dingani was located further northeast, and Freddy was either too large or too small. These findings were further validated through a high-resolution regional model. Specifically, Freddy's track and intensity most closely matched the observations when these three factors were most closely represented. Our study underscores the pivotal role played by the interaction between TCs and multi-scale systems for long-lived TCs.
AS31-A003
A Net CO2 Flux from Tokyo Evaluated by a Model Simulation and a Tower Observation
Kyohei YAMADA1#+, Yosuke NIWA1, Yukio TERAO1, Yasunori TOHJIMA1, Kazuhiro TSUBOI2, Shohei MURAYAMA3, Kentaro ISHIJIMA4
1National Institute for Environmental Studies, Japan, 2Japan Meteorological Agency, Japan, 3National Institute of Advanced Industrial Science and Technology, Japan, 4Meteorological Research Institute, Japan
Urban population and greenhouse gases emissions have grown in recent years. Although Tokyo, Japan, is one of the largest cities in the world with a population of over 37 million, a quantitative evaluation of carbon dioxide (CO2) emissions from Tokyo is insufficient. We estimated net CO2 fluxes from Tokyo for two years from 2019 to 2020 in combination with a global high-resolution model simulation by the Nonhydrostatic ICosahedral Atmospheric Model (NICAM) and the observation at around 250 m height of Tokyo Skytree (35.71°N, 139.81°E), a freestanding broadcasting tower. Observed atmospheric CO2 variations were well simulated at remote sites around Japan owing to use of flux data from a global inverse analysis. Tagged tracers simulations estimated Tokyo-originated CO2 concentration and showed that variations of CO2 concentration in Tokyo area are strongly influenced by wind; southerly winds caused by the sea breeze transport airmass with high CO2 concentrations from power plants and industrial areas distributed along the bay. By removing CO2 data with low wind condition under southern-wind condition, the correlation coefficient of Tokyo-originated CO2 concentrations between the observation and the model is increased reaches the maximum when CO2 data with wind speed lower than 5.5 m/s are removed. Meanwhile, Radon, which has a constant flux distribution in the model, does not show drastic change of the correlation coefficient under southern wind condition with removing low wind speed, suggesting that the changes of correlation of CO2 with removing low wind is caused by the unrealistic flux distribution in the model. This study corrected a prescribed CO2 flux from Tokyo by observation with the removal of the low wind speed data to 10.5 ± 2.2 kg C m-2 year-1 (82.5 ± 17.3 Tg C year-1 in net emissions from the target area in Tokyo).
AS31-A011
Elevated Thanksgiving CO2 Is Associated with the Meteorological and Short-term Energy Change Over Salt Lake City
Ju-Mee RYOO1,2#+, Inez FUNG3, James EHLERINGER4
1NASA Ames Research Center, United States, 2Bay Area Environmental Research Institute, United States, 3University of California, Berkeley, United States, 4The University of Utah, United States
Long-term and high-frequency atmospheric CO2 measurements at multiple sites in Salt Lake Valley (SLV), Utah, have demonstrated that the annual and monthly patterns of CO2 variability align with a priori estimates of CO2 emissions from various anthropogenic and biological sources. In this study, we investigate whether short-term changes in anthropogenic sources, as captured in the Vulcan emissions dataset for the US, can be detected through atmospheric CO2 observations. Specifically, we focus on the Thanksgiving holiday period, during which traffic and energy usage patterns are expected to differ from other periods in November. We observed that on-road CO2 emissions peak during weekday morning and evening rush hours, but are lower during the Thanksgiving holidays and weekends. The CO2 concentrations also show the double peak, suggesting the dominance of traffic emissions in the CO2 diurnal cycle. Interestingly, atmospheric CO2 concentrations during the Thanksgiving holidays were higher than the other periods of November at all SLV monitoring sites between 2008 and 2013, predominantly due to increased non-onroad emissions. While the temporal patterns of emissions and CO2 mole fractions at the monitoring sites were similar, there were differences in the spatial patterns. The suburban Rose Park and downtown Murray sites exhibited the highest CO2 mole fractions among all observed locations. Vulcan anthropogenic emissions data, however, indicated that the emissions at Murray were relatively lower compared to those at Rose Park. The Murray site is located next to a major Interstate freeway, which runs north-south, whereas the Rose Park site is away from the freeway. The CO2 mole fractions were elevated primarily when southerly winds advected emissions along the freeway. This study highlights the role of local processes in understanding CO2 variations in an urban monitoring network.
AS31-A015
Quantification of Fugitive Methane Emissions from the Seoul Combined Cycle Power Plant (SCCPP)
Hyuckjae LEE1+, Sujong JEONG1#, Jaewon JOO1, Dong Yeong CHANG1,1, Jaewon SHIN1, Yeonsoo KIM1,2, Donghee KIM1
1Seoul National University, Korea, South, 2Climate Tech Center, Korea, South
The quantification of methane emissions from fugitive natural gas leakages presents a challenge, however, it is essential for the effective mitigation of methane emissions. The Korea Carbon Project (KCP) endeavored to quantify the fugitive methane emissions from the Seoul Combined Cycle Power Plant (SCCPP) using mobile measurements over approximately 6 months, from January 12 to July 12, 2023. This approach employed an electric vehicle-based atmospheric GHG monitoring platform, which had instruments for measuring CH4, C2H6, and CO2 mounted on it. Three major emission sources from the SCCPP were identified through the mobile measurement strategies and their sources were determined by ethane to methane ratios and methane to carbon dioxide ratios. The maximum methane enhancements from the three major sources were quantified at 56,039, 3,795, and 1,051 ppb, respectively. To quantify the methane emissions from these sources, the Gaussian Plume Dispersion Model (GPDM) and OTM-33a method were used. The emission rates from three major sources at the SCCPP were 7.66±0.8, 7.97±1.03, and 0.31±0.03 GgCO2eq/yr, respectively. The emission rates obtained from the mobile measurements were compared with the bottom-up approach, based on the 2023 fuel consumption data at the SCCPP. These results revealed that the emissions from the three major sources identified at the SCCPP through mobile measurements constituted 35.41%, 21.16%, and 0.73% of the respective bottom-up based inventory estimations. This study suggests that the discrepancy between actual and known emissions could be reduced through measurement-based estimation of methane emissions.
AS31-A019
Designing Additional CO2 In-situ Surface Observation Networks Over South Korea Using Bayessian Inversion Coupled with Lagrangian Modelling
Samuel Takele KENEA#+
National Institute of Meteorological Sciences, Korea, South
Efforts to enhance greenhouse gas (GHG) emission reduction in East Asia play a pivotal role on both global and regional scales in advancing climate mitigation strategies. This study aimed to better constrain anthropogenic CO2 emission estimates by expanding the network of near-surface in-situ stations for CO2 observations across South Korea. To achieve an optimal CO2 network design, we conducted an Observing System Simulation Experiment (OSSE) coupled with STILT, utilizing meteorological data from the Korean Integrated Model (KIM). Our inversion setup incorporated two CO2 emission datasets with a 0.1o resolution: EDGAR v6 for prior emissions and GRACED for truth emissions. A uniform model-mismatch error of 3 ppm was introduced across sites. The effectiveness of the existing five in-situ stations, termed the base network, in South Korea was evaluated to gauge their ability to constrain CO2 surface flux estimates. However, the findings revealed a reduction in flux uncertainty of only 29.2%, which fell short of the desired uncertainty reduction goal. In this base network, the Lotte World Tower (LWT: 37.5126˚E, 127.1025˚E) in Seoul and the Anmyeondo (AMY: 36.538576˚ N, 126.330071˚ E) site in Taean county stood as major contributors, with estimated reductions of 17.48% and 6.35%, respectively. Consequently, we proposed and developed an extended network, identifying seven candidate sites based on consideration of logistical factors, existing infrastructures, and proximity to the emission source regions. An incremental optimization scheme ranked their contributions, resulting in an additional 25% reduction, bringing the total to 54.13%. However, it is noteworthy that diminishing returns (ranging from 13% to less than 0.1%) were observed with an increase in station count mainly due to the possibility that adding a station earlier in the sequence might render subsequent stations redundant. Despite this, the proposed CO2 network successfully reduced uncertainty in emissions.
AS31-A025
Simulating Urban Microclimate and CO2 Concentration According to Land Surface
Woosuk CHOI#, Chae Min LIM+
Sejong University, Korea, South
The majority of people residing in urban areas is leading to the current rapid urbanization. This urbanization process has resulted in the complex microclimate phenomena unique to cities attributed to the reduction in green areas and the construction of high-rise buildings. Buildings, asphalt, and concrete in cities absorb and release radiation, inducing to heat-related environmental issues. Additionally, atmospheric stagnation between densely packed high-rise buildings, coupled with enhanced social activities due to population growth lead to elevated CO₂ concentrations. Urban environments are changed based on land surface conditions such as adjacent building or green spaces, and more. This study simulates urban environmental changes in Gwangjin-gu district in Seoul using the ENVI-met model, which takes into accounts factors such as buildings, vegetation, land cover, and meteorological conditions. Through four-season simulations, it was confirmed that enlarging green spaces is the most effective method to mitigate the urban heat island and reduce CO₂ concentrations. Our findings offer crucial guidelines for sustainable urban development and climate change mitigation, aiming to contribute to urban planning and environmental policymaking.
AS31-A028
Investigation of Altitude-dependent Variation on Ratios from Aircraft Measurements Over the Yellow Sea in the Western Coast of the Korean Peninsula
Jongbyeok JUN1+, Yongjoo CHOI1#, Beom-Keun SEO2, Yonghwan LEE3, Jeonghwan KIM1, Chisung YUN1, Misun LEE4, Jinyeong SONG4
1Hankuk University of Foreign Studies, Korea, South, 2National Institute of Meteorological Sciences, Korea, South, 3KOTITI Testing & Research Institute, Korea, South, 4Hanseo University, Korea, South
To attain Net Zero by 2050, it is crucial to accurately estimate the emissions of CO and long-lived greenhouse gases (GHGs), such as CO2 and CH4. Traditionally, GHGs monitoring has been conducted by long-term measurements at fixed locations and on global scale using satellite observations to capture trends. Recently, aircrafts have been employed to measure the vertical and spatial distribution of GHGs concentrations from the surface to the upper troposphere. Using GLA331-MCEA1 (OA-ICOS; ABB-LGR) which was equipped on a research aircraft (KingAir-C90GT), we measured CO, CO2, and CH4 concentrations over the Yellow Sea of Korea and nearby large coal-fired power plants in 2022 and 2023. To investigate the characteristics of regional emission sources, we calculated the ratios of ΔCH4/ΔCO2, ΔCH4/ΔCO, where delta (Δ) indicates the subtraction of background concentrations (the 1st percentile of each flight), from the measured values. Subsequently, based on back-trajectories from the HYSPLIT model, we analyzed the regional and altitude differences in ΔCH4/ΔCO2 and ΔCH4/ΔCO, which was divided into administrative districts. The estimated ΔCH4/ΔCO2 and ΔCH4/ΔCO ratios obtained through airborne measurement will be compared with those from bottom-up GHGs emission inventories such as Emissions Database for Global Atmospheric Research (EDGAR v6.0) to validate the accuracy of emission inventories.
AS31-A031
Estimation of Carbon Dioxide Emissions from Roads in Major Metropolises in South Korea
Myeong-Gyun KIM+, Hyo-Jong SONG#
Myongji University, Korea, South
In 2020, greenhouse gas (GHGs) emissions from the transportation sector in South Korea accounted for 14.7% of the total. Among various sectors encompassed within the transportation sector, road transport contributed about 96% to the emissions. Therefore, reducing carbon dioxide (CO2) emissions from the road transport sector is essential for achieving national carbon neutrality. However, the current calculation of CO2 emissions in the road transport sector is conducted only at the national level. To achieve more efficient emission reduction, it is necessary to calculate emissions on a regional and road-specific basis, considering the characteristics of each area and road. Therefore, as the initial phase of this study, a model for estimating CO2 emissions from roads in Seoul was developed. This study aims to estimate CO2 emissions from roads in Incheon, Busan, and Ulsan, using the Seoul model as a reference. To achieve this, the first step involved validating and improving the Seoul model. This process included utilizing feature importance analysis for data classification, addressing sample bias through clustering, and conducting model validation using independent datasets. In the next step, the estimation of road CO2 emissions in Incheon, Busan, and Ulsan was conducted using the Seoul model. Subsequently, model construction specific to each of these cities was carried out. The reason for choosing this approach is to assess the general applicability of the model. In the future, independent data will be acquired and model improvement processes will be undertaken to validate the models for these cities. The result of this study is considered a crucial step in estimating regional and road-specific CO2 emissions on a nationwide scale. Through this, it is anticipated that the findings will contribute to policymaking in the road transport sector and enable efficient reduction of CO2 emissions.
AS31-A033
Estimating CO2 and BC Contributions of Emission Sources in Sihwa Industrial Complex Based on Mobile Monitoring
Yongchan KIM#+, Wonseok KO, Yeon-Uk KIM, Dongwon CHOI, Sooyeon KIM, Jimin KIM, Young-Jin SON, Minseo CHOI, Kyung-Hwan KWAK
Kangwon National University, Korea, South
Industrial complex areas can be large sources of air pollutants and greenhouse gases. It is very important to understand in detail the distribution of pollutants in areas with large emissions. In order to understand the detailed emission characteristics of an industrial complex, it is necessary to identify the contribution of emission sources at a detailed scale. Therefore, this study seeks to estimate the contribution of CO2 and BC emission sources based on machine learning techniques. To calculate contribution, five tree-based algorithmic models were used to select the model with the highest predictive performance. And the contribution of greenhouse gases was calculated using the SHAP (Shapley Additive exPlanations) technique. The input variables for machine learning are CO2, BC, U, V, road separation distance, land cover ratio, latitude, and longitude. The spatial distribution of CO2 (GMP252, 2-second intervals; H41-H6, 1-second intervals) and BC (MA200, 1-second intervals) were measured through mobile measurements based on bicycles and electric vehicles. Measurements were conducted 13 times over 4 days from August 21st to August 24th, 2023, and 20 times over 3 days from December 19th to 21st, 2023. CO2 and BC showed high concentrations mainly on the road, and seasonal differences were founded. The analyzed results showed the distribution of emission sources to CO2 and BC concentrations in industrial complexes and the priority of the emission sources which should be reduced first. Acknowledgements: This work was supported by “Korea Environment Industry & Technology Institute(KEITI) through Project for developing an observation-based GHG emissions geospatial information map, funded by Korea Ministry of Environment(MOE) (RS-2023-00232066).” and "This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE)."
AS31-A034
Estimating Seasonal Net CO2 Fluxes from Industrial and Non-industrial Complexes Based on Drone Observation
Sooyeon KIM#+, Yeon-Uk KIM, Dongwon CHOI, Wonseok KO, Young-Jin SON, Jimin KIM, Yongchan KIM, Minseo CHOI, Yeji JEON, Minjeong HONG, Jihyun LEE, Kyung-Hwan KWAK
Kangwon National University, Korea, South
The increase in CO2 in the atmosphere is the major concern worldwide due to its impacts on global warming. The government has announced the goal of net zero greenhouse gas emissions until the year of 2050. It is necessary to quantitatively understand the spatiotemporal and seasonal variations of CO2 fluxes from the emission sources. In Korea, relevant researches have been utilized the eddy covariance technique by implementing gas analyzer at the top of towers to calculate upward and downward fluxes at a single point. To complement the limited applicability of eddy covariance method, in this study, we used drones to calculate and compare the seasonal CO2 fluxes quantitatively in industrial and non-industrial complexes. The drone observations were conducted in the Sihwa industrial complex in Siheung, Korea, and the Kangwon National University athletic field in Chuncheon, Korea. The drone flights were taken for 3 hours after sunrise and 3 hours before sunset, in winter and summer, from 0m to 250m above ground. The estimation results showed the net CO2 fluxes at the two different sites and seasons, revealing the emission characteristics monitored by drone observations. Acknowledgements: This work was supported by “Korea Environment Industry & Technology Institute(KEITI) through Project for developing an observation-based GHG emissions geospatial information map, funded by Korea Ministry of Environment(MOE) (RS-2023-00232066).” And "This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE) (C10168180002)."
AS31-A036
Characteristics of Column Measurements for Urban CO2 Monitoring Using Ground-based Fourier Transform Spectrometer Measurements and Lagrangian Transport Model
Jueun KIM+, Sujong JEONG#, Hayoung PARK, Jaemin HONG, Jonghyuk LEE, Yu-Ri LEE, Sojung SIM
Seoul National University, Korea, South
Urban CO2 monitoring is crucial for climate change mitigation, as CO2 is a major contributor to climate change and is primarily emitted in densely populated urban areas. Recently with the increase in ground-based Fourier transform spectrometer measurements and satellite data in urban area, the importance of understanding XCO2 (Total Column-averaged dry-air mole fraction of carbon dioxide) data is also growing. However, in South Korea, there is little research on XCO2 using ground-based Fourier transform spectrometer in urban area. In this research, we show the results of XCO2 measurements from EM27/SUN ground-based Fourier transform spectrometer in the period of May 2020 to July 2023 over Seoul, South Korea. XCO2 data exhibited an increasing trend of 2.16 ppm yr-1, and a seasonal amplitude of 7.79 ppm. These results are then compared with the surface in-situ CO2 data (SNUCO2M) measured near the EM27/SUN site. When compared with the trend and variability of surface in-situ CO2, total column CO2 showed smaller increases and variability, implying lower concentrations and changes in the upper atmosphere. This study also calculated and compared the footprints of column CO2 and surface CO2 using X-STILT (X-Stochastic Time-Inverted Lagrangian Transport model) and STILT model. We have discovered that the footprints of column CO2 are significantly larger than those of surface in-situ CO2, indicating that column CO2 is influenced by broader area within urban regions. This work was supported by Korea Environmental Industry & Technology Institute (KEITI) through “Project for developing an observation-based GHG emissions geospatial information map”, funded by Korea Ministry of Environment (MOE)(RS-2023-00232066).
AS32-A001
Contrasting Characteristics of Atmospheric Rivers and Their Impacts on 2016 and 2020 Wildfire Seasons Over the Western United States
Ju-Mee RYOO1,2#+, Taejin PARK1
1NASA Ames Research Center, United States, 2Bay Area Environmental Research Institute, United States
An atmospheric river (AR) is a strong filamentary water vapor transport that plays a critical role in regional hydroclimate systems. While climate conditions can affect wildfire activities, the process by which ARs are associated with wildfire patterns remains unclear. Here, we characterize ARs in 2016 and 2020, and associate them with fire spread and burned areas along with other climate conditions in the western U.S. We found the record-high wildfire activity in 2020 was associated with hotter, drier, and windier conditions, with its peak shifted from July to August, unlike the climatological fire seasonality in the western U.S. It was also linked to satellite-observed low soil moisture during pre- and on fire season but high vegetation greenness, a proxy of fuel load, during the pre-fire season. ARs were more frequent but weaker in the summer, while ARs were less frequent and short-lived in the fall of 2020 than those of 2016. The year 2016 experienced a 'coupled' precipitation-wind pattern (i.e. higher wind accompanying high precipitation). In contrast, precipitation was much lower in 2020 than in 2016, showing a 'decoupled' precipitation-wind pattern, particularly in the spring and fall. Under ARs, the contrasting precipitation-wind patterns in 2020 (dry-windy) and 2016 (wet-windy) were more evident. For example, the surface wind (precipitation) in the AR cases was higher by 9% (34%) than in the non-AR cases in 2020 (both years) (p < 0.01) over land. The daily fire activity records demonstrate that long-lived, successive, and coastal ocean-originated (centered) ARs with high precipitation help suppress fire activity (e.g., September-November 2016), while short-lived or no ARs with strong wind and little precipitation rather yield fire activity (e.g., August and September 2020). This result highlights how ARs can be associated with wildfire activity patterns during the pre-fire and fire seasons in the western U.S.
AS32-A004
Future Projection of East Asian Atmospheric Rivers in High-resolution Climate Models
Yeeun KWON+, Seok-Woo SON#
Seoul National University, Korea, South
East Asian atmospheric rivers (ARs) play a critical role in the hydroclimate as they are closely associated with extreme precipitation. Although it is well known that ARs will become more frequent in a warming climate, the future changes of East Asian ARs and their impacts on precipitation in high-resolution climate models remain unclear. The present study investigates the East Asian ARs in the CMIP6 High Resolution Model Intercomparison Project (HighResMIP) models. The results show a robust increase in AR frequency and associated precipitation in the near future (2040-2050) under the SSP5-8.5 scenario. These increases are dominated by thermodynamic processes with a minor role of dynamic processes. Comparing low- and high-resolution model simulations, it is further found that AR-related precipitation is better captured in the latter. This result suggests that the high-resolution modeling would be beneficial for quantifying the hydrological impacts of East Asian ARs in a warming climate.
AS32-A008
Subseasonal Prediction of East Asian Atmospheric River
Hyein KIM+, Yeeun KWON#, Seung-Yoon BACK, Jaeyoung HWANG, Seok-Woo SON
Seoul National University, Korea, South
Atmospheric rivers (ARs) are closely related to local precipitation which can be both beneficial and destructive. Although several studies have evaluated their predictability, there is a lack of studies on East Asia ARs. This study evaluates the subseasonal prediction skill of East Asian ARs in the European Centre for Medium-Range Weather Forecasts (ECMWF) subseasonal-to-seasonal prediction model for 2001-2020 summer. The model successfully predicts the spatial distribution of AR frequency in East Asia, but underestimates it along the boundary of the western North Pacific subtropical high at lead times of one or two weeks. When the prediction skill is quantified by computing the anomaly correlation coefficient and mean square skill score, weekly AR prediction skill saturates around 2 weeks. Such prediction limit is primarily set by wind field errors with a minor contribution of moisture distribution errors. This result suggests that the improved prediction of atmospheric circulation field can improve the predictability of East Asian summer ARs and the associated precipitation.
AS32-A009
A New Quarter-degree Global Atmospheric Rivers Database Based on ERA5
Bin GUAN1#+, Duane WALISER2
1University of California, Los Angeles, United States, 2California Institute of Technology, United States
Atmospheric rivers (ARs) are narrow, elongated, synoptic jets of water vapor that play important roles in the global water cycle and regional weather/hydrology. The need for characterizing and understanding AR life cycles (i.e., from genesis to termination) and their variations between different regions motivated the continual development of an AR tracking algorithm suitable for global studies, namely, Tracking Atmospheric Rivers Globally as Elongated Targets (tARget). The algorithm identifies AR objects at individual time steps based on thresholding integrated water vapor transport (IVT) and other requirements, and tracks each AR object in time and space. Building on three previous versions of the algorithm, this paper discusses further refinements to the algorithm since the last release in 2019, to better handle ARs in tropical and polar areas where the background climate is different from the midlatitudes, as well as “zonal” ARs (those with weak poleward IVT or even equatorward IVT) which the previous versions of the algorithm are not designed to capture. The further refined algorithm is applied to the ERA5 reanalysis over 1940–current at 6-hour intervals and a 0.25° × 0.25°horizontal resolution. The AR detection result is evaluated based on four analyses: (1) comparison of AR defining characteristics to those of Zhu and Newell (1998); (2) comparison of AR landfall dates in western North America, Britain, and East Antarctica with AR detection methods independently developed in other studies for those regions; (3) comparison of AR durations with ground observations of 91 AR events during 2004–2010 from an AR observatory in northern California; and (4) comparison of AR width and total IVT across the AR width with dropsonde observations of 21 ARs over the northeastern Pacific during 2005–2016.
AS32-A012
Impacts of Climate Change on Atmospheric Rivers Over East Asia
Tae-Jun KIM1#+, Jinwon KIM1,2, Jinuk KIM1, ChuYong CHUNG1, Young-Hwa BYUN1
1National Institute of Meteorological Sciences, Korea, South, 2University of California, Los Angeles, United States
Atmospheric rivers (ARs) are closely associated with extreme precipitation and hydrological events in East Asia to cause significant damages to human society. Therefore, predicting the impact of climate change on ARs is crucial for preventing damages caused by extreme precipitation and ensuring effective operation of water management facilities. Projections of future (2080~2099) changes in ARs and related hydrology under the SSP5-8.5 scenario utilizing the CMIP6 multi-model ensemble indicate that the annual-average integrated vapor transport (IVT) in East Asia in the period 2080~2099 will increase by approximately 32.5% compared to the past period (1995~2014) while the annual-average AR frequency will increase by about 111% of the past period. Examination of the water vapor and moist wind components of IVT reveals that the future increase in IVT is primarily due to increases in water vapor. It is inferred that the IVT increase is largely responsible for the increase the AR occurrence frequencies. The changes in AR due to climate change also affect precipitation to increase the total precipitation in East Asia. Examination of the changes in AR characteristics shows that the frequency of intense AR events will also increase due to the climate change. Specifically, significant increases in the frequency of strong AR events during the East Asian summer monsoon season are projected to occur in the future. Projections regarding the frequency and intensity of AR events vary substantially following regions, highlighting the necessity for more detailed regional analyses to further understand the impacts of the climate change on ARs and related hydrology in East Asia.
AS33-A011
Prediction Skill of Length of Day in Multiple Decadal Prediction Systems
Hyunsuk YOON1+, Jung CHOI1, Seok-Woo SON1#, Adam SCAIFE2,3
1Seoul National University, Korea, South, 2Met Office, United Kingdom, 3University of Exeter, United Kingdom
Length of day (LOD) is one of the Earth rotation parameters whose precise estimation and prediction are critical in applications such as interplanetary spacecraft tracking and navigation. LOD fluctuates on interannual or shorter time scales due to the solid Earth’s interaction with the atmospheric non-tidal phenomena such as El Niño–Southern Oscillation (ENSO) and Quasi-Biennial Oscillation (QBO). A recent study (Scaife et al. 2022) reported that LOD can be predicted more than a year ahead, though its result is based on only a single model. In this study, we examine LOD prediction skills in nine state-of-the-art decadal prediction systems that participated in the Decadal Climate Prediction Project (DCPP). LOD prediction skill remains significant for about a year in multiple prediction systems and multi-model mean (MMM), with a notable rebound at 12–15 lead months. This is consistent with the previous research and suggests that models in general can predict LOD a year ahead. LOD predicted by MMM is highly correlated with a linear combination of ENSO and QBO (r = 0.89) and with ENSO alone (r = 0.88), which is qualitatively consistent with observation (r = 0.55 and 0.46 for ENSO and QBO and ENSO alone, respectively). This indicates that LOD variation is well explained by ENSO and QBO, with ENSO playing a major role and QBO being a minor factor. Prediction skill of LOD at the time of rebound is also highly correlated with that of ENSO and QBO combined (r > 0.8), and with that of ENSO (r = 0.78), which further confirms a stronger link between LOD and ENSO. These results suggest that a skillful ENSO prediction may lead to an accurate prediction of LOD and related extra-tropical climate components up to a year ahead.
AS33-A012
Two Pathways of Northern Hemisphere Surface Temperature Change Under a Net-zero Emission Scenario
Yong-Han LEE#+, Sang-Wook YEH
Hanyang University, Korea, South
Recently, the international community has committed to achieving carbon neutrality by 2050 under the Paris Agreement, which aims to keep global average temperatures from rising more than 1.5°C/2°C above pre-industrial levels. By using Community Earth System Model Version 2 (CESM2), we examined the responses of Northern Hemisphere surface temperature under a net-zero emission scenario among ensemble members. Under a net-zero emission scenario, anthropogenic CO2 emissions are increases linearly based on the SSP5-8.5 scenario, and then gradually reduced at the same rate until anthropogenic CO2 emission reach a net-zero. After a net-zero emission was achieved, two pathways of Northern Hemisphere surface temperature change are observed after a certain period. By comparing with ensemble members with different pathways, we found that there exists a significant difference in North Atlantic Ocean, which could be associated with the changes of Atlantic Meridional Overturning Circulation (AMOC) intensity. Acknowledgements: This study was supported by the NRF grant funded by Korean government (NRF-2018R1A5A1024958).
AS33-A015
CESM2 Pencil Ocean Model Development
Jongsoo SHIN1+, Young-Oh KWON1#, Gokhan DANABASOGLU2, Ivan LIMA1, Yu-Chiao LIANG3, Yu-Heng TSENG3, Yen-Chi WU3
1Woods Hole Oceanographic Institution, United States, 2National Center for Atmospheric Research, United States, 3National Taiwan University, Taiwan
In this study, we use the Community Earth System Model version 2 (CESM2) ocean model hierarchy, in which the identical atmosphere, land, and sea-ice components are coupled with ocean models of varying complexity. In particular, we have developed and evaluated the Pencil Ocean Model (PenOM), a one-dimensional (1-D) ocean columns model with the lateral ocean processes disabled. The PenOM is implemented within the Parallel Ocean Program version 2 (POP2), which is the same model framework used for the full 3-D ocean component of CESM2. The PenOM provides a more realistic 1-D thermodynamic ocean compared to a slab ocean model by including multiple ocean layers and allowing a prognostic mixed layer depth evolution and vertical mixing, while is simpler than the fully 3-D ocean general circulation model. In a set of multi-century preindustrial control simulations using the CESM2 ocean model hierarchy, the internal variability of sea surface temperature (SST) in the absence of externally forced signals is analyzed. The results from the PenOM coupled simulation and the 3-D ocean case are compared to examine the respective roles of 1-D ocean processes (e.g., mixing, interannual mixed layer depth variations, and entrainment) and 3-D ocean dynamics (e.g., wind and buoyancy-driven circulation). The objective of this research is to discern the individual contributions of atmospheric forcing, 1-D ocean processes, and 3-D ocean dynamics to the variability and predictability of SST on interannual-to-decadal time scales. In addition, we aim to assess the impact of ocean dynamics on the atmospheric circulation.
AS33-A017
Estimating Contributions of External Forcings and Ocean Processes to the Long-term Predictability of Atlantic Multidecadal Variability
Abhinav R. SUBRAHMANIAN1#+, June-Yi LEE2, Wonsun PARK2, Yong-Yub KIM1
1IBS Center for Climate Physics, Korea, South, 2Pusan National University, Korea, South
The Atlantic Multidecadal Variability (AMV) with dominant timescales of 55 to 70 years serves as a crucial source of predictability for climate variability and changes in many regions. This influence extends not only to the continents surrounding the North Atlantic but also remotely through global atmospheric teleconnection. Although considerable relevant studies have been conducted, challenges remain in better identifying the origins of its variability and predictability and improving predictions of AMV and its teleconnection at longer leads. This study aims to determine the origins of AMV variability and to assess the predictability and long-lead forecast skills of AMV and its teleconnection by using a multi-year Earth System Prediction system based on Community Earth System Model Version 2 (CESM2). The prediction system consists of 50-member uninitialized simulations, 30-member ocean assimilations, and 30-member 5-year hindcasts initiated from every January 1st from 1960 to 2021. Comparison between the mean of large ensemble simulations and observation indicates that external forcings explain about 30% of the observed nonfiltered AMV variability for the last 62 years. We estimate that the ocean internal processes contribute up to 25% (10%) to AMV predictability at a 1-year (5-year) forecast lead. We also investigate prediction skills for regional temperature and precipitation anomalies associated with AMV variability.
AS33-A020
Exploring Sources of Multi-year Predictability of Terrestrial Ecosystem
June-Yi LEE1#+, Yong-Yub KIM2, Jeong-eun YUN1,1
1Pusan National University, Korea, South, 2IBS Center for Climate Physics, Korea, South
The demand for decision-relevant and evidence-based near-term climate information is increasing. This includes understanding and explaining the variability and changes in ecosystems to support disaster management and adaptation choices. As climate prediction from seasonal to decadal (S2D) expands to encompass Earth system dimensions, including terrestrial and marine ecosystems, it is crucial to deepen our scientific understanding of the long-term predictability sources for ecosystem variability and change. Here we explore to what extent terrestrial ecosystem variables are driven by large-scale - potentially predictable -climate modes of variability and external forcings or whether regional random environmental factors are dominant. To address these issues, we utilize a multi-year prediction system based on Community Earth System Model version 2 (CESM2). The system consists of 50-member uninitialized historical simulations, 20-member ocean assimilations, and 20-member hindcast initiated from every January 1st integrating for 5 years from 1961 to 2021. The key variables assessed are surface temperature, precipitation, soil moisture, wildfire occurrence, and Gross Primary Productivity. Our results suggest that land surface processes and ecosystem variables over many parts of the globe can be potentially predictable 1 to 3 years ahead originating from anthropogenic forced signals and modes of climate variability, particularly El Nino and Southern Oscillation and Atlantic Multi-decadal variability. These global modes of climate variability shift regional temperature and precipitation patterns, leading to changes in soil moisture, wildfire occurrence, and terrestrial productivity.
AS33-A021
Indian Warming Ocean Can Reduce Terrestrial and Agricultural Productivity in North America Under Greenhouse Warming
Young-Min YANG1#+, Jae-Heung PARK2, June-Yi LEE3
1Jeonbuk National University, Korea, South, 2Seoul National University, Korea, South, 3Pusan National University, Korea, South
Over the past few decades, the Indian Ocean has exhibited the most significant warming trends globally, imparting profound regional and global consequences. However, the specific ramifications of this warming, particularly concerning terrestrial and agricultural productivity and their impact on terrestrial carbon sinks, have remained unclear. In this study, we unveil a compelling link between Tropical Indian Ocean (TIO) warming and the reduction of terrestrial and agricultural productivity in North America, with the potential to contribute to the decline of carbon sinks. TIO warming initiates an atmospheric teleconnection process, characterized by the propagation of quasi-stationary waves into the extratropics. This process culminates in a widespread deficit of precipitation and soil moisture over North America. Subsequently, agricultural crop yields and terrestrial productivity, accounting for 10-20% of Gross Primary Productivity (GPP), are significantly impacted, thereby contributing to a positive carbon-climate feedback loop. Through simulations replicating TIO warming, we validate the suppression of terrestrial activities in North America under both historical and projected CO2 forcings. This study underscores the pivotal role played by TIO warming in shaping the global terrestrial ecosystem.
AS33-A022
Improving a Data-driven Weather Prediction Model and an Idealized Approach to Understanding Tropical-extratropical Interaction
Daehyun KANG#+, Seon-Yu KANG, Minjong CHEON, Yo-Hwan CHOI, Yumi CHOI, Jeong-Gil LEE
Korea Institute of Science and Technology, Korea, South
Recent deep learning-based models have shown great potential in predicting and interpreting weather and climate phenomena. For example, the data-driven weather forecast models (e.g., GraphCast and Pangu-Weather) showed better forecast skills of the global atmosphere within a week than the operational numerical weather prediction. However, with their short history, understanding of trained physical processes in the deep learning-based model is not satisfactory. Motivated by the above, this study aims to improve the accuracy and capability of data-driven global climate prediction. This study uses a deep learning-based model trained with daily-mean atmospheric variables in the European Centre for Medium-Range Weather Forecasts (ECMWF) reanalysis (ERA5) at 250-km horizontal resolution for 1979-2015. A method to better structuralize the horizontal structure of the global atmosphere into the deep learning model shows great potential to improve data-driven prediction skills, which exhibit reliable deterministic forecast skills within a week. The inference results also exhibit realistic subseasonal climate variability, such as eastward propagation of the Madden-Julian Oscillation (MJO). Additionally, we propose an idealized model to understand the remote influence of atmospheric perturbation from the pre-trained model. The idealized model experiments forced by El Nino- and MJO-like perturbation exhibit realistic atmospheric teleconnection, indicating that the realistic physical processes are adequately trained in the data-driven method. The results of this study shed light on the necessary processes in the model architecture for state-of-the-art global climate prediction.
AS34-A002
| Invited
Reducing Winter Precipitation Biases Over the Western Tibetan Plateau in the Model for Prediction Across Scales (MPAS) with a Revised Parameterization of Orographic Gravity Wave Drag
Yuzhi JI1+, Xin XU1#, Yuan WANG1, Xu ZHOU2, Kun YANG3, Yixiong LU4, Rongrong ZHANG1, Ben YANG1, Jianping TANG1
1Nanjing University, China, 2Chinese Academy of Sciences, China, 3Tsinghua University, China, 4China Meteorological Administration, China
Climate models often overestimate the precipitation in western Tibetan Plateau (TP) during winter, due to their poor ability in representing the orographic drag of unresolved complex terrain. In this study, the parameterization scheme of orographic gravity wave drag (OGWD) in the Model for Prediction Across Scales (MPAS) is revised to account for the nonhydrostatic effects (NHE) on the surface momentum flux of vertically-propagating orographic gravity waves. The effect of revised OGWD scheme on the simulation of winter precipitation over the TP is examined using parallel numerical experiments with the original and revised schemes, respectively. The results show that the revised scheme can effectively alleviate the precipitation biases in western TP by improving the atmospheric circulation and water vapor transport. The NHE reduces the surface wave momentum flux of orographic gravity waves which results in weaker zonal OGWD in the mid-low troposphere and thus stronger westerlies over the TP, reducing the easterly biases in the experiment with the original OGWD scheme. The weakened zonal OGWD promotes a plateau-scale cyclonic circulation to the north of the TP, which suppresses the northern branch of the bifurcated westerlies detouring the TP. According to quantitative analysis, the water vapor transport into the western TP and surrounding areas by upstream westerlies is notably reduced by the northeasterlies of the cyclonic circulation, which eventually leads to the decrease of precipitation in this region.
AS34-A004
Evaluation of Original and Water Stress-incorporated Modified Weather Research and Forecasting Vegetation Photosynthesis and Respiration Model in Simulating CO2 Flux and Concentration Variability Over the Tibetan Plateau
Lunyu SHANG1#+, Xiao-Ming HU2, Hanlin NIU1, Shaoying WANG1, Xianhong MENG1
1Chinese Academy of Sciences, China, 2The University of Oklahoma, United States
Terrestrial carbon fluxes are crucial to the global carbon cycle. Quantification of terrestrial carbon fluxes over the Tibetan Plateau (TP) has considerable uncertainties due to the unique ecosystem and climate and scarce flux observations. This study evaluated our recent improvement of terrestrial flux parameterization in the weather research and forecasting model coupled with the vegetation photosynthesis and respiration model (WRF-VPRM) in terms of reproducing observed net ecosystem exchange (NEE), gross ecosystem exchange (GEE), and ecosystem respiration (ER) over the TP. The improvement of VPRM relative to the officially released version considers the impact of water stress on terrestrial fluxes, making it superior to the officially released model due to its reductions in bias, root mean square error (RMSE), and ratio of standard deviation (RSD) of NEE to 0.850 µmol·m−2 ·s −1, 0.315 µmol·m−2 ·s −1, and 0.001, respectively. The improved VPRM also affects GEE simulation, increasing its RSD to 0.467 and decreasing its bias and RMSE by 1.175 and 0.324 µmol·m−2 ·s −1, respectively. Furthermore, bias and RMSE for ER were lowered to −0.417 and 0.954 µmol·m−2 ·s −1, with a corresponding increase in RSD by 0.6. The improved WRF-VPRM simulation indicates that eastward winds drive the transfer of lower CO2 concentrations from the eastern to the central and western TP and the influx of low-concentration CO2 inhibits biospheric CO2 uptake. The use of an improved WRF-VPRM in this study helps to reduce errors, improve our understanding of the role of carbon flux cycle over the TP, and ultimately reduce uncertainty in the carbon flux budget.
AS34-A010
A Critical Evaluation of Top-hat Approximation in Convection Parameterization at Different Horizontal Scales
Zhao YAXIN1#+, Xiaocong WANG2, Yimin LIU2, Guoxiong WU2
1University of Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China
The top-hat approximation, which is widely used with bulk entraining plume in the mass-flux type convective parameterization schemes, is verified at different horizontal scales by using large eddy model (LES) and cloud resolving model (CRM) simulations, especially those at the limit of vanishing cloud fraction. Five convection cases consisting of three shallow convection cases: RICO, BOMEX, and ATEX from the Global Energy and Water Cycle Experiment (GEWEX) Cloud System Study (GCSS) programs and two deep convection cases including GATE and KWAJEX are conducted. Due to the fact that convective cloudiness fraction increases with increasing horizontal resolution, the cloudy part of turbulent flux increases, leading to considerable errors manifested in top-hat approximation. These errors, however, are largely compensated by the decrease of error in the environmental part, resulting in the relative error in top-hat approximation not increasing significantly with increasing horizontal resolution. At first glance, this brings encouraging results to the modeling community that top-hat approximation is still valid at high resolutions. Nevertheless, increase of error in the cloudy part poses additional difficulties for turbulence schemes, which often struggle to represent turbulence in cloudy part. A multi-plume based scheme is needed instead of a bulk entraining model in order to partially account for the inhomogeneity in cloudy part. Preliminary tests show that three plumes are sufficient to well parameterize the turbulent flux in the cloudy part.
AS34-A012
Addressing Marine Stratocumulus Biases in Taiwan Earth System Model Version 1 (TaiESM1)
Yi-Hsuan CHEN#+, Danielle MANALAYSAY
Academia Sinica, Taiwan
Marine stratocumulus plays a crucial role in regulating Earth’s radiation budget by exerting a strong negative radiative cooling effect. Many state-of-the-art climate models have struggled to accurately simulate the marine stratocumulus features, leading to substantial shortwave radiation biases at both the surface and the top of the atmosphere. These biases may be attributed to deficiencies in physical parameterizations, though the exact causes need to be identified and addressed by individual models. This study aims to address the marine stratocumulus biases in Taiwan Earth System Model Version 1 (TaiESM1) through a two-fold approach: (1) identifying the sources of these biases, and (2) modifying relevant physical parameterization schemes, such as boundary layer and cloud schemes, to resolve these biases. Specifically, this study will utilize DYCOMS-II and VOCALS-REx field observation data, ERA5 reanalysis, and a hierarchy of TaiESM1 simulations including single-column model simulations, hindcast simulations, and AMIP-type and fully coupled simulations. This hierarchy of simulations enables a comprehensive examination of the physical parameterizations in TaiESM1, facilitating the identification and resolution of marine stratocumulus biases. Furthermore, the proposed methodology can be a valuable framework for other modeling centers seeking to address biases in their models.
AS34-A016
Improved Simulation of Northeast China Cold Vortices by Revising the Orographic Gravity Wave Drag Parameterization in the Weather Research and Forecasting Model
Mingshan LI1+, Xin XU2#, Yuan WANG2
1Jingmen Meteorological Service, China, 2Nanjing University, China
The parameterization of orographic gravity wave drag (OGWD) is essential for the simulation of the atmospheric circulation, especially in regions of complex terrain. Current OGWD schemes assume hydrostatic OGWs, but the parameterized OGWs in fine-resolution models with narrow subgrid-scale orography can be significantly affected by nonhydrostatic effects (NHE). This study revises the OGWD scheme in the Weather Research and Forecasting model by accounting for NHE on the surface wave momentum flux of upward-propagating OGWs. To evaluate the performance of the revised OGWD scheme in short-range forecast, two sets of simulations are conducted for nine Northeast China cold vortices (NECVs) in the warm season of 2011 using the original and revised OGWD schemes, respectively. Results show that the model tends to underestimate the NECV intensity, producing too high geopotential height and too weak horizontal wind. The NECV intensity biases are alleviated when accounting for NHE in the OGWD scheme, especially in the mid-to-lower troposphere. Process analyses reveal that NHE act to reduce the lower-tropospheric OGWD by reducing the surface wave momentum flux of OGWs, which strengthens the NECV in the lower troposphere. The NECV intensifies in the mid-upper troposphere as well, owing to the enhancement of post-trough cold advection caused by the strengthened low-level cyclonic circulation. NHE increase as the model resolution changes from 27 km to 3 km, suggesting greater importance of accounting for NHE in OGWD parameterization in high-resolution models.
AS34-A028
Impacts of Single and Multilayer WRF-urban Canopy Models on a Simulated Heavy Rainfall Event in Davao City, Philippines
Michelle Louise TACDERAN#+, Judiel Marie DEL MAR, Rochelle CORONEL
Ateneo de Davao University, Philippines
On May 3, 2017, an intense rainfall event that resulted in heavy flooding occurred in several areas over Davao City, Philippines. According to Lagare et al. (2023), mesoscale convective systems (MCS), due to weak large-scale forcing and different mechanisms, were observed over Davao City during this date. This paper evaluates the impact of urban canopy models (UCM) on a heavy rainfall event over Davao City using the coupled Weather Research and Forecasting (WRF)-Urban modeling system. The WRF’s default urban surface model (BULK Urban Parameterization), Single-Layer Urban Canopy Model (SLUM), and Multi-layer Building Energy Parameterization (BEP) were used to investigate the impact of urbanization to the formation or movement of the mesoscale convective systems. BULK treats the urban canopy as a single rough surface, SLUM takes into account different surface types such as roofs, walls, and streets, while BEP consider individual building features and urban surfaces as it generates the vertical flow of heat, moisture, and momentum. WRF was initially run with 9-, 3- and 1-km horizontal resolution using the 100-m Copernicus Global Land Service Land Cover that has more Urban Land Surface categories than the 1-km MODIS land cover data. UCM sensitivity runs were performed by downscaling the 1-km WRF run to 500-m grid. The multilayer urban canopy parameterization simulated lower biases than the BULK scheme. Significant differences in rainfall and MCS formation were found between the different urban canopy models. Specifically, MCS1 and MCS2 formations and their merging into MCS3 over downtown Davao were more evident in BEP compared to Bulk. MCS3 over the urban area was not observed in SLUM simulation. The multilayer scheme also weakened wind speed and delays moisture transport over the downtown area. Further analysis will be done to tune the model with different stages of Davao City’s urbanization.
AS38-A006
The Impact of Extreme Meteorological Events on Air Pollution in China
Yiting ZHOU#+
Nanjing University, China
Some extreme meteorological events, such as heat wave, atmospheric stagnation and temperature inversion, may have an important impact on air quality through physical and chemical processes, and have a great impact on regional air quality(Han et al., 2014; Lei et al., 2018; Liao et al., 2018; Steiner et al., 2010). When the temperature inversion occurs, the atmospheric boundary layer is stable, which inhibits the transfer of matter and energy in the boundary layer and is not conducive to the diffusion of pollutants. Atmospheric stagnation tends to have a weak wind speed in the boundary layer and a small precipitation, which are not conducive to the diffusion and washout of pollutants. Heat waves are characterized by persistent high temperatures, which have a significant impact on ozone production. Studies show that heat wave days have a greater impact on ozone and PM2.5 concentrations; atmospheric stagnation has a greater impact on PM2.5, and temperature inversion will slightly increase ozone concentrations but have a greater impact on PM2.5.(Yang, J., & Shao, M., 2021).In general, when heatwaves, atmospheric stagnation or temperature inversions are present alone or in combination, ozone and particulate matter concentrations are usually higher in most areas than when there is no extreme weather. Studies have shown that the frequency of extreme meteorological events in China has been on the rise in the past decade(Ding et al.,2016). Therefore, continuing to study the relationship between extreme meteorological events and the pollution of ozone and particulate matter in different regions of China will be of great help to the prevention and control of air pollution in different regions.
AS38-A008
Arctic/North Atlantic Origin Teleconnection Causes Extreme PM10 Events in South Korea
Jeong-Hun KIM1, Maeng-Ki KIM1#, Seong-Joong KIM2,3, Joo-Hong KIM2, Sang-Wook YEH4, Sang-Hyun LEE1, Youngseok LEE1+
1Kongju National University, Korea, South, 2Korea Polar Research Institute, Korea, South, 3University of Science and Technology, Korea, South, 4Hanyang University, Korea, South
Severe PM10 events in South Korea are caused by stable atmospheric circulation conditions related to high-pressure anomalies in the upper troposphere. However, research on why these atmospheric circulation patterns occur is unknown. In this study, we propose new large-scale teleconnection pathways that cause severe PM10 events during the mid-winter in South Korea. This study investigated extremely high (EH)-PM10 instances in South Korea during mid-winter and examined the corresponding atmospheric teleconnection patterns to identify the factors contributing to EH-PM10 events. K-means clustering analysis revealed that EH-PM10 cases were associated with two large-scale teleconnection patterns originating from the North Atlantic Ocean and the Barents-Kara Sea. Atmospheric variability in two key regions trigger the Rossby wave propagation, causing favorable atmospheric conditions for EH-PM10 events in Korea. These large-scale teleconnections led to a high-pressure anomaly over the Korean Peninsula, reducing atmospheric ventilation and weakening the surface pressure system, causing a rapid increase in PM10 concentration within a few days. Understanding this teleconnection phenomenon may assist in implementing emission reduction measures based on the results of short-term forecasts of severe PM10 events. [This work was supported by a grant from the National Institute of Environment Research (NIER), funded by the Ministry of Environment (MOE) of the Republic of Korea (NIER-2021-03-03-007) and the Korea Polar Research Institute (KOPRI) grant titled “Development and Application of the Earth System Model-based Korea Polar Prediction System (KPOPS-Earth) for the Arctic and Midlatitude High-impact Weather Events” funded by the Ministry of Oceans and Fisheries (KOPRI PE23010)].
AS38-A011
Larger Cloud Liquid Water Enhances Both Aerosol Indirect Forcing and Cloud Radiative Feedback in Two Earth System Models
Xi ZHAO1#, Xiaohong LIU2+
1Tianjin University, China, 2Texas A&M University, United States
Previous studies have noticed that the Coupled Model Intercomparison Project Phase 6 (CMIP6) models with a stronger cooling from aerosol-cloud interactions (ACI) also have an enhanced warming from positive cloud feedback, and these two opposing effects are counter-balanced in simulations of the historical period. However, reasons for this anti-correlation are less explored. In this study, we perturb the cloud ice microphysical processes to obtain cloud liquid of varying amounts in two Earth System Models (ESMs). We find that the model simulations with a larger liquid water path (LWP) tend to have a stronger cooling from ACI and a stronger positive cloud feedback. More liquid clouds in the mean-state present more opportunities for anthropogenic aerosol perturbations and also weaken the negative cloud feedback at middle to high latitudes. This work, from a cloud state perspective, emphasizes the influence of the mean-state LWP on effective radiative forcing due to ACI (ERFACI).
AS38-A018
Enhanced Dust Cooling Effect Estimated from Regionally Dependent Refractive Indices
Hao WANG1+, Xiaohong LIU2#, Chenglai WU1, Guangxing LIN1, Tie DAI1, Daisuke GOTO3, Qing BAO1, Toshihiko TAKEMURA4, Guang-Yu SHI1
1Chinese Academy of Sciences, China, 2Texas A&M University, United States, 3National Institute for Environmental Studies, Japan, 4Kyushu University, Japan
The dust direct radiative effect (DRE) depends sensitively on the particle size distribution (PSD) and complex refractive index (CRI). Although recent studies constrained the PSD in the models, CRI uncertainties are still large. Therefore, whether dust warms or cools the climate system remains unclear. Here, we jointly analyze the dust PSD and CRI to constrain the dust DRE by leveraging measurements of dust CRI globally. We find that employing regionally dependent CRI significantly enhances the scattering of dust in shortwave and reduces its absorption in longwave, which is opposite to that caused by increasing the coarse dust fraction via constraining the PSD. Constraining both PSD and CRI ultimately leads to a net DRE of -0.71 W m-2, a cooling stronger than current model estimates. It is crucial to include PSD and regionally varying CRI more realistically to accurately represent the impact of dust on the climate system.
AS38-A021
Climate Effects of Brown Carbon Aerosol Under the Scenario of Future Wildfires
Lulu XU1#+, Guangxing LIN1, Xiaohong LIU2, Fang LI1
1Chinese Academy of Sciences, China, 2Texas A&M University, United States
Wildfires emit large amounts of black carbon and light-absorbing organic carbon, known as brown carbon, into the atmosphere. These particles perturb Earth’s radiation budget through the absorption of incoming shortwave radiation. Given that wildfires are predicted to increase globally in the coming decades, it is important to quantify these radiative impacts. Compared to black carbon, the atmospheric warming effect exerted by brown carbon remains highly variable and poorly represented in climate models. Recently, observational studies found a type of dark brown carbon (i.e., tar balls) generated from wildfires can contribute more than black carbon (nearly three-quarters) to the short visible light absorption. Those indicate that the climate effects of brown carbon may be larger than ever imagined in the future, while the parameterizations of tar balls from wildfires have not been considered in the climate models. And the climate effects of brown carbon under the scenario of future wildfires have not been explored. In this study, we first added parameterizations of tar balls' light absorption to the Modal Aerosol Module (MAM4) in CAM5.4 to represent the light absorption of brown carbon from wildfires. We then collected multi-type observational data (vertical and surface) from several wildfire events to validate the model simulation. Based on this, we finally estimated the direct radiative effects of tar balls and analyzed their effects on clouds and precipitation under the scenario of future wildfires.
AS38-A022
Observed Evidence That Subsidence Process Stabilizes the Boundary Layer and Increases the Ground Concentration of Secondary Pollutants
Yu SHI#+, Fei HU
Chinese Academy of Sciences, China
Subsidence often occurs on clear nights, which affects the development of the nocturnal boundary layer (NBL) and the processes of material and energy transfer. Subsidence in the boundary layer appears to be rare and short-lived, so it is difficult to be observed. In this paper, data from a large tethered balloon (1900 m3) with instruments for measuring meteorological parameters and air pollutants, a ground-based aerosol lidar, a Doppler wind lidar and some other ground observations are combined to analyze the influence of a subsidence process on the boundary layer structure and downward transport of various pollutants. Pollutants were horizontally transported to the observation site driven by southwest low-level jet. Under the downdraft and turbulent kinetic energy transported towards the surface, the vertical subsidence of the pollutants lasted for nearly 5 hours. During this period, the observation data of the tethered balloon hovering at 500 m shows that the concentration of PM2.5, NO3-, SO42- and NH4+ increased by approximately 17 μg m-3, 11 μg m-3, 2.3 μg m-3 and 5 μg m-3, respectively. The vertical subsidence of pollutants had significant effects on the secondary inorganic aerosol concentrations, but the concentration of organic aerosols was not affected. In addition, the O3 concentration in the lower atmosphere increased by 8 ppb. The downward transport of pollutants obviously lagged behind the downward vertical motions by about one hour. The subsidence process also enhanced the inversion intensity of the lower atmosphere. The inversion layer effectively hindered the diffusion of pollutants, and the concentration of ground PM2.5 increased by 42 μg m-3. Our results show that under the effects of descending movements and the downward vertical flux of turbulent kinetic energy, pollutants could also subsided into the lower layer of the NBL.
AS38-A023
A Non-dimensional Index for Characterizing the Transition of Turbulence Regimes in Stable Atmospheric Boundary Layers
Xin SHAO+, Ning ZHANG#
Nanjing University, China
In stable atmospheric boundary layers, turbulence can be categorized into two regimes: a moderate turbulence regime where turbulence is relatively prompted and a weak turbulence regime where turbulence is suppressed. Monin-Obukhov similarity theory, which is the foundation of the modern micrometeorology, is only valid under the moderate turbulence regime. Therefore, understanding the transition between the two turbulence regimes is crucial for the development of stable atmospheric boundary layer theories and parameterizations. Currently, however, there is no physically based, non-dimensional index for characterizing the transition between the two turbulence regimes. This study aims to bridge this research gap by proposing a new non-dimensional index and determining the transition threshold value theoretically. Using CASES-99 dataset, this study reveals that the transition between the moderate and the weak turbulence regimes is related to the establishment of pancake vortices, the vertical length scale of which is comparable to the buoyancy length scale. In order to obtain a non-dimensional index characterizing this process, a simplified spectral model is established. By incorporating horizontal and vertical length scales of turbulence into the spectral model, this study finds that the transition occurs at a critical horizontal Froude number of 0.28. Furthermore, the critical horizontal Froude number can recover previously used height- and site-dependent mean wind speed thresholds by invoking the stability-corrected logarithmic wind profile. These findings hold significant scientific and practical implications for the representation of stably stratified turbulence in numerical simulations for weather and pollutants dispersion. The identified critical horizontal Froude number can be used to constrain the application range of Monin-Obukhov similarity theory and further improve turbulence parameterizations in stable atmospheric boundary layers.
AS38-A024
How Efficient is a 205 MHZ VHF Radar in Estimating the Atmospheric Boundary Layer Height?
Angel Anita CHRISTY+, M.G. MANOJ#
Cochin University of Science and Technology, India
This study presents a novel approach in measuring the atmospheric boundary layer height (ABLH) by utilizing data from a very high frequency (VHF) radar installed at the Advanced Centre for Atmospheric Radar Research in Cochin University of Science and Technology (CUSAT) in India. To ensure the result accuracy, clear-sky days were identified through a dedicated year-long experimental campaign in 2021 involving simultaneous radar and radiosonde operations. The mixing ratio and associated gradient profiles from radiosonde are employed to estimate the reference ABLH values. The new method combines three parameters, viz., signal-to-noise ratio, wind speed and wind direction - in estimating the boundary layer height from radar datasets. The ABLH is determined as the altitude at which the sum of normalized standard deviations of the three parameters peak and then markedly decrease. The results demonstrate a significant correlation (r=0.91 at a 99% confidence level) between the ABLH derived from this methodology and that estimated from the radiosonde data. In contrast to sparsely available radiosonde profiles, this research provides extensive opportunities to investigate the high temporal variability such as the diurnal cycle of ABLH using radar data. Nevertheless, there are certain hurdles in the estimation of ABLH during rainy/cloudy conditions which is yet to be overcome.
AS40-A002
Macro- and Microphysical Characteristics of Extreme Hourly Precipitation Over the Pearl River Delta on the Monsoon Coast (South China)
Juliao QIU1+, Yali LUO2#, Chong WU1, Yanyu GAO3, Shuting YU4
1Chinese Academy of Meteorological Sciences, China, 2Nanjing University of Information Science & Technology, China, 3China Meteorological Administration, China, 4 Ji'nan Meteorological Bureau, China
In this study, the Extreme Hourly Precipitation Areas (EHPAs) of three extreme levels (i.e., between the 95th and 99th percentiles, between the 99th and 99.9th percentiles, beyond the 99.9th percentile) in the Pearl River Delta over South China are identified; then the Extreme Hourly Precipitation Event (EHPE) and associated Convective Cores (CCs) are tracked, and their macro-and-microphysical characteristics are analyzed using multi-year dual-polarization radar observations. Results show that > 90% of EHPAs are smaller than 10 km2, and 65 – 75% of EHPEs last only one hour. They tend to be more localized and persist longer with increasing hourly-precipitation extremity. The EHPEs overlap with the CCs during 50 – 64% of the EHPEs’ life span. Their occurrence frequencies are nearly quadrupled after the monsoon onset over South China Sea, with a major (secondary) peak at about 1400 LST (0600 LST) in the diurnal variations. The CCs are non-linear shaped with about 65% being meso-γ-scale and embedded within mostly meso-β or α-scale 20dBZ regions. The CCs generally contain active warm-rain processes and about 70% possess moderate-to-intense mixed-phase microphysical processes. The ratios of ice water path to liquid water path are about 0.37, and coalescence dominates (about 68%) the liquid-phase processes. The average size of raindrop is slightly larger than the “maritime-like” regime and the average concentration is much higher than the “continental-like” regime. These CCs’ characteristics mostly resemble those of the convection producing extreme instantaneous precipitation, except for a larger horizontal scale and less evident changes with the hourly-precipitation extremity.
AS40-A010
Aerosol Effect on a Record-breaking Rainfall Event in the Great Bay Area of South China from Simulations with WRF-Chem Coupled with Spectral-bin Microphysics
Zhenghui LI1+, Yali LUO2#, JIwen FAN3, Yuwei ZHANG4
1Chinese Academy of Meteorological Sciences, China, 2Nanjing University of Information Science & Technology, China, 3Argonne National Laboratory, United States, 4Pacific Northwest National Laboratory, United States
How anthropogenic aerosols influence extreme precipitation is an open question. On May 7, 2017, a record-breaking rainfall event hit the capital city Guangzhou in South China with a maximum hourly rainfall of 184.4 mm and a maximum 3-hour rainfall accumulation of 382.6 mm, causing serious societal impacts. The observations of PM2.5 indicate increases of aerosol concentration on May 6, 2017 resulting in polluted conditions under which the rainstorms initiated and developed. To investigate the possible contribution of anthropogenic air pollution to this high-impact rainfall event, this study utilizes the Chemistry version of the Weather Research and Forecasting model (WRF-Chem), coupled with spectral-bin microphysics (SBM) and a multilayer urban model embedded with a building energy model (BEM-BEP). The control experiment (CTRL) with realistic anthropogenic emissions can reproduce the diurnal variations of PM2.5 and its surge to peak amount before the convection initiation as found in the observations. The locations, structures and evolutions of convective storms and associated surface rainfall accumulation are also simulated reasonably well compared with the observations. In contrast, the “clean scenario” experiment (CLEAN) with anthropogenic emissions reduced to 10% of CTRL doesn’t capture the observed spatiotemporal distributions of PM2.5, e.g., the near-ground aerosol number concentration at the moment of convection initiation is only about 1/5 of that in the CTRL. A much smaller amount of maximum rainfall accumulation in CLEAN than CTRL (235 vs. 339 mm) is associated with the weaker convective intensity and shorter duration of the rainstorm during the later stage of the rainfall event. We are making ensemble simulations and in-depth analysis to obtain more robust results about urbanization-induced aerosol impacts on the rainfall.
AS40-A016
Role of the Australian High in Seasonal Phase Locking of the Indian Ocean Dipole
Bo TONG+, Wen ZHOU#
Fudan University, China
This study analyzes the effect of the Australian High (AH) on the seasonal phase locking of Indian Ocean Dipole (IOD) events. The anomalous strong AH associated with the positive phase of the Antarctic Oscillation can cause significant easterly wind anomalies and northward cross-equatorial flow over the western Maritime Continent (MC) by strengthening the Australian winter monsoon during May–August. The AH-associated easterly anomalies and northward cross-equatorial flow can create thermodynamic air-sea feedback and contribute to a significant cooling anomaly in the western MC and the tropical eastern Indian Ocean. Without considering the effect of ENSO, these processes contribute to the occurrence of positive IOD events, which begin in early summer, peak in late summer, and decay rapidly thereafter. The effect of ENSO can extend the peak period of IOD into the boreal autumn of that year. An anomalous weak AH corresponds to the occurrence and seasonal phase locking of negative IOD events. Through combined empirical orthogonal function analysis, we find that the effect of the AH can well explain the seasonal phase locking of 34 IOD events (40 in total), which provides an important theoretical basis for the prediction of IOD events.
AS40-A017
A Frequent Ice-free Arctic is Likely to Occur Before the Mid-21st Century
Zili SHEN#+
Fudan University, China
Although the trend of sea-ice extent under global warming has been studied extensively in recent years, most climate models have failed to capture the recent rapid change in the Arctic environment, which has brought into question the reliability of climate model projections of sea ice and suggested a potential shift in Arctic climate dynamics. Here, based on the results of a time-variant emergent constraint method with a weighting scheme, we show that an ice-free Arctic might occur earlier (by at least 5 ~ 10 years) than previously estimated. In other words, Arctic ice will likely disappear before the 2050 s. The observationally constrained date for an ice-free Arctic in September under fossil-fuel-based development (i.e., Shared Socioeconomic Pathway (SSP) 5–8.5) scenarios yields a central estimate of 2050–2054 with a 66% confidence range (equivalent to the IPCC’s ‘likely’ range) of 2037–2066, while an ice-free Arctic will likely occur for another 20 years and 11 years under ambitious mitigation scenarios (i.e., SSP2-4.5) and SSP3-7.0. An ice-free Arctic is unlikely to occur under the sustainable development scenario (i.e., SSP1-2.6). Looking forward, this time-variant emergent constraint may also help detect tipping points in the climate system. Our findings provide useful information to help policy makers cope with climate change.
AS40-A019
Automatic Identification of Rain Cells Using GPM DPR Observations
Zejian WU#+
Nanjing University, China
To study the natural differences between precipitation events with various intensities, it is necessary to focus on the features of their corresponding rain cells, where a rain cell is usually regarded as a continuous precipitation entity in which the rain rate (or radar reflectivity) is higher than surrounding. Thus, the two-dimensional data, Near Surface precipitation Rate (NSR), provided by the Dual-frequency Precipitation Radar (DPR) onboard the GPM satellite with a horizontal resolution of 5 km, can be used for identifying these rain cells. However, the NSR distribution is usually complex with rain cells often adhesive to each other in a larger precipitation system, bringing difficulties for distinguishing them. Also, the large number of rain cells makes manual identification impractical. Hence, an automatic rain-cell-identification algorithm using NSR is proposed in this study. Firstly, identify the NSR peak pixels, which are the pixels with the local maximum NSR value in an area of continuous precipitation with a minimum NSR value set up. Then, assuming each peak corresponds to a rain cell, the scope of the rain cell is determined by expanding from the peak when following two requirements are met: the NSR value of a pixel is larger than some percentage (e.g., 50%) of the corresponding peak NSR, and the NSR value tends to decrease approximately as the range from the peak increases. Results show that the proposed algorithm is capable of distinguishing adjacent rain cells by reconciling the completeness and separation of these rain cells, which are more reasonable than those from the algorithms simply relying on NSR value thresholds and pixel continuity. Therefore, this proposed method can help further studies on more accurate and reliable precipitation features of rain cells and their connection with larger systems as well as their precipitation mechanisms.
AS40-A020
Applying Machine Learning for Precipitation Forecasting in Uneven Rainfall Regions: A Case Study of Taiwan
Fan-Ming CHIU1+, Chuan-Ming LIU1#, Lawrence Jing-Yueh LIU2,3
1National Taipei University of Technology, Taiwan, 2University of Illinois Urbana-Champaign, United States, 3National Central University, Taiwan
Weather plays a vital role in human society. Having advanced access to meteorological information thus can enhance the ability for decision-making and disaster preparedness. The Numerical Weather Prediction (NWP) model was developed due to the increasing demand for accurately predicting weather changes for the next few hours or days. However, the traditional physical-based model requires extensive computational time and costs, which is not an optimal solution in rapidly changing weather conditions. Recently, there has been an increasing interest in using machine learning models as an alternative to NWP models. Current research mainly focuses on two categories based on the types of datasets used: (1) “Reanalysis data” for predicting various meteorological parameters at different altitudes globally; and (2) “Surface observation data” for predicting specific meteorological parameters at individual stations. Research by NVIDIA, Huawei, and Google has shown that the application of reanalysis data with machine learning techniques in weather forecasting is becoming more efficient and accurate than traditional physical-based models. However, reanalysis data still rely on NWP models for preliminary data processing, resulting in high computational costs. As for surface observation data with machine learning techniques, common research focuses on the prediction of temperature and precipitation. These have shown commendable performance in many regions, but heavy rainfall predictions are still challenging due to the imbalanced non-Gaussian data distribution. Therefore, this study aims to utilize surface observation data to enhance the accuracy of machine learning predictions, especially in forecasting extreme precipitation with highly uneven rainfall distribution in Taiwan.
AS40-A022
Thunderstorm Nowcasting in Southeast Asia Based on Cloud Properties from GK2A, Geostationary Satellite
Gyuyeon KIM#+, Yong-Sang CHOI
Ewha Womans University, Korea, South
Southeast Asia experiences vigorous convection patterns due to solar heating, leading to extreme weather events. Thunderstorms occurring in these areas exhibit a diurnal variation, emphasizing the importance of considering diurnal variation to detect thunderstorms. This study suggests a novel method to detect thunderstorms considering the diurnal variation of convection using the geostationary satellite GEO-KOMPSAT 2A (GK2A). We utilize 10-minute GK2A infrared (IR) brightness temperature (BT) and cloud microphysical parameters (e.g. cloud optical thickness, cloud effective radius) to detect thunderstorms effectively. The storm detection results were validated with Global Precipitation Measurement (GPM) Integrated Multi-Satellite Retrievals (IMERG) IR precipitation variables. As result, the thunderstorm detection was further improved when cloud microphysical parameters were applied with BT. This study proposes an optimized threshold of cloud microphysical parameters over time to minimize the false alarm ratio value also maximize the probability of detection and critical success index value. This study will contribute to reducing damage due to thunderstorms in Southeast Asia.
AS40-A023
Assessment of Detecting Heavy Rainfall-inducing MCS in the Korean Peninsula Using Instability Indices from Rawinsonde Data
Minsu KIM#+, Myoung-Seok SUH
Kongju National University, Korea, South
Recent studies have shown an increase in frequency and intensity of heavy rainfall (Hev_Ran) events on the Korean Peninsula, located East Asia, due to global warming. Additionally, several studies have shown that the atmospheric environment and MCS (Mesoscale Convective Systems) causing Hev_Ran in East Asia differs from those in North America and Europe. Therefore, this study aims to reevaluate the possibility of detecting MCS causing Hev_Ran in Korea using instability indices (Inst_Ind) derived from rawinsonde data. Considering the regional, seasonal, and temporal variations of Hev_Ran events in Korea, this study also conducts investigation on the detection capability by Inst_Ind, region, and time as well as threshold optimization. For the recent ten years during the rainy season, hourly accumulated precipitation data from the AWS and rawinsonde data from 8 stations in Korea were used for this purpose. Due to the differing observation frequencies of the two datasets, this study defines the collocated data as those AWS data within -2h~+2h temporally and 100km spatially based on rawinsonde observations. Comparing the Inst_Ind during climate average (Cli_Ave) and Hev_Ran, significant differences were noted for KI, SWEAT, and TPW with more than 20% differences. However, CAPE, LI, SSI, SRH, and TTI did not show significant differences. POD and FAR were used to reevaluate various Hev_Ran intensity (30, 40, and 50mm/h) detection level of the Inst_Ind. Analysis has indicated usefulness in detecting Hev_Ran using SSI, KI, and TPW showing high POD (0.92~0.98) and FAR (0.91~0.99). However, CAPE, LI, SWEAT, SRH indicated less effectiveness regardless of Hev_Ran intensity, showing low POD (0.32~0.48) and high FAR (0.90~0.98).This presentation will further detail the optimization of thresholds for Inst_Ind and provide detailed presentation of the detection capability of Hev_Ran systems and MCS, segmented by station and time.
AS45-A012
Enhancing Ocean Heat Flux Prediction: Noise Reduction for Accurate Sea Ice Dynamics Forecasting
Ikjun HWANG#+, Woosok MOON
Pukyong National University, Korea, South
This research focuses on the crucial role of sea ice balance in the Earth's climate system, highlighting its significance in global climate change. Among the factors affecting this balance, ocean heat flux is key due to its impact on sea ice dynamics. Ocean heat flux, the transfer of thermal energy between ocean and ice, is essential in sea ice's freezing and melting processes. Our research reveals that increases in ocean heat flux are directly correlated with heightened rates of sea ice melting. This correlation is particularly pronounced in polar regions, where even minor rises in ocean temperatures can significantly disrupt the fragile equilibrium necessary for sea ice formation. Inversely, the study also identifies periods when a decrease in heat flux plays a vital role in the stabilization and augmentation of sea ice. Previous studies have indicated that direct measurement of ocean heat flux is not feasible, and approximations derived from sea ice buoy data are often imprecise due to the presence of noise. Addressing this challenge, our study employs observational data to determine boundary temperatures (at the top and bottom positions of ice). These temperatures are then analyzed using a Fourier series to predict ocean heat flux, effectively eliminating noise components and emphasizing principal wave terms. The methodology encompasses a detailed examination of both temperature variations and changes in sea ice, aiming to establish a comprehensive understanding of the heat transfer mechanisms at play. In conclusion, our findings assert the criticality of sea ice in forecasting and managing the future state of the Earth's climate. The research emphasizes the need for specific and empirically derived values of ocean heat flux, moving away from arbitrary assumptions, to enhance the accuracy of climate predictions and inform effective environmental strategies.
AS45-A020
Delayed Impacts of Arctic Sea-ice Loss on Eurasian Severe Cold Winters
Yeon-Soo JANG1+, Jong-Seong KUG2#, Sang-Yoon JUN3, Seok-Woo SON4, Seung-Ki MIN2
1Korea Institute of Ocean Science and Technology, Korea, South, 2Pohang University of Science and Technology, Korea, South, 3Korea Polar Research Institute, Korea, South, 4Seoul National University, Korea, South
This study suggests a possible mechanism of how the Arctic sea-ice loss can influence the mid-latitude climate in the Eurasian continent. It is shown that the low sea-ice concentration over the Barents-Kara-Laptev Seas in autumn typically leads to cold Eurasian in winters. It is demonstrated that the Arctic-to-midlatitude connection depends on the state of late autumn atmospheric circulation. When the autumn sea-ice reduction is accompanied by anticyclonic circulation over northern Eurasia, Eurasia becomes anomalously cold in the early winter. However, when cyclonic circulation is dominant, Eurasian cold anomalies appear in the late winter. This seasonally-delayed response is further found to be related to the wind-driven sea-ice drift that causes warm anomalies over the Barents-Kara Seas in the following winter. These observational results are confirmed by model simulations, indicating that the recent Eurasian cold winters could be linked to their forced response to the Arctic sea-ice loss.
AS45-A026
From Peak to Plummet: On the Impending Decline of the Warm Arctic-cold Continents Phenomenon
Yungi HONG1+, Jinho YOON1#, S. Y. Simon WANG2, Jee-Hoon JEONG3, Hyungjun KIM4,5, Seok-Woo SON6, Sang-Woo KIM6, Baek Min KIM7
1Gwangju Institute of Science and Technology, Korea, South, 2Utah State University, United States, 3Chonnam National University, Korea, South, 4Korea Advanced Institute of Science and Technology, Korea, South, 5The University of Tokyo, Japan, 6Seoul National University, Korea, South, 7Pukyong National University, Korea, South
This study presents an analysis of the future of the Warm Arctic-Cold Continent (WACC) phenomenon in East Asia and North America. Utilizing large-ensemble datas, we project the WACC events for the upcoming decades, focusing on the evolving geographic boundaries of extreme cold temperatures. Our findings indicate a notable northward shift in these boundaries, underlining global warming's influence on the distribution of cold air. There are two key insights: First, our results align with previous studies, confirming an increase in WACC occurrences up to the 2020s. Second, a significant decrease in WACC events is projected from the 2030s onwards, signaling a major shift in extreme winter weather patterns. These findings necessitate a re-examination of current models and theories regarding extreme winter weather. Importantly, this research highlights the need for updated climate models to enhance future preparedness and response strategies.
AS47-A011
Improving Numerical Prediction of Asian Dust Storms Through an Intelligent Optimization System: Optimization of Physical Parameters in WRF-Chem
Ji Won YOON+, Seon Ki PARK#
Ewha Womans University, Korea, South
Asian Dust Storms (ADSs) have been one of the high-impact atmospheric hazards in South Korea (SK). They originate in dry regions, such as the Gobi Desert and Inner Mongolia, primarily during spring, and are transported to SK along the westerlies, significantly impacting air quality in SK. To deal with the air pollution problem, it is vital to use a numerical model to enhance air quality forecasting skills. In particular, the performance of numerical air quality prediction is highly related to the accurate forecast of the dust storm occurrence at the source and the dust concentration. In this study, we built an intelligent optimization system by coupling the micro-genetic algorithm (μGA) and the WRF-Chem model—the WRF-Chem-μGA system. This system can find optimal parameters related to dust emission in WRF-Chem to improve air quality forecasting. For optimization, we selected the case of the recent ADS, which significantly impacted SK. Overall, the WRF-Chem with the optimized set of parameter values outperforms the non-optimized ones in forecasting the ADS events in SK.
AS47-A013
Diagnosis of the KIAPS DA System: Insights from Virtual Sonde Observation Assimilation
In-Hyuk KWON1#+, Hyerim KIM1, Kyung-Hee SEOL1, Minwoo CHOI1, Hui-Nae KWON1,2, Hyun-Jun HAN1
1Korea Institute of Atmospheric Prediction Systems, Korea, South, 2Ewha Womans University, Korea, South
The Korea Institute of Atmospheric Prediction Systems (KIAPS) has embarked on enhancing its predictive capabilities from very short range (~6 hours) to extended medium range (~30 days), including coupling to various earth system components like the land surface, oceans, and sea ice. The first phase of the KIAPS project delivered the global atmosphere-only NWP system that was made operational at the Korea Meteorological Administration (KMA) in April 2020. The NWP model - named the Korean Integrated Model (KIM) - is a non-hydrostatic model on a cubed-sphere grid that employs the spectral element method for its dynamical core. The global data assimilation (DA) system is based on a hybrid-4DEnVar system for the deterministic analysis, and an LETKF for ensemble perturbation updates, and is already giving good performance. However, some systematic model error is found in the KIM forecast. Notably, a positive temperature bias exists below 500 hPa across most regions, except for high latitudes. Furthermore, while an overall wet bias prevails in this region, a dry bias was identified at 850 hPa. Data assimilation uses various observations to produce analysis fields with reduced errors, but persistent systematic errors remain. There is a question as to how much analysis field error can be corrected at most if data assimilation is perfect. To find an answer to this, assuming the analysis field of ERA5 as a truth, a virtual Sonde observation with a dense global grid was created based on ERA5 and used for data assimilation. Results indicated a substantial reduction in analysis errors across most regions when using virtual Sonde observations, in spite of regional variability. Our presentation will focus on quantifying the maximum error correction achievable through data assimilation. Furthermore, the results of virtual Sonde data assimilation will be compared with the current data assimilation results.
AS47-A017
A Comparison Between Dual Localization, Successive Covariance Localization, and Scale-dependent Localization Using a 1000-member Ensemble Forecast During the Tokyo Olympics and an OSSE Based on the QG Model
Zhe-Hui LIN#+, Shu-Chih YANG
National Central University, Taiwan
The ensemble data assimilation (EDA) is widely applied nowadays for its ability to estimate the flow-dependent error covariance. For EDA, localization methods are commonly applied to mitigate the false correction induced by the sampling error. However, localization shrinks covariance over a specified distance much and could seriously sacrifice the benefits from the flow-dependent error covariance. Consequently, several localization schemes, dual localization (DL), successive covariance localization (SCL), and scale-dependent localization (SDL), are proposed to deal with the sampling error in more elaborate manners with consideration of scale. While DL and SDL perform scale separation to the background ensemble perturbation, SCL distributes observations to different scales. Meanwhile, DL and SCL perform localization to observation error covariance (R localization), and SDL performs localization to background error covariance (B localization). In this study, we compare the three schemes with a main concern on the ability to improve covariance estimation. With a convective-scale 1000-member ensemble forecast during the Tokyo Olympics, we evaluate how accurate these schemes can be with a smaller ensemble and measure the skill by comparing with the 1000-member-one without localization. Not only the Kalman gain and increment are inspected, but we also estimate the equivalent B localization matrix for DL and SCL to get a more concrete picture of how the three schemes refine the noisy ensemble-estimated covariance. An OSSE based on the QG model is further conducted to examine whether the findings result from the offline diagnosis persist, and how they evolve in an online cycling experiment.
AS47-A018
Introduction of Global Error Covariance to Nested Ensemble Variational Assimilation
Saori NAKASHITA#+, Takeshi ENOMOTO
Kyoto University, Japan
Regional atmospheric models require lateral boundary conditions obtained from global circulation models. The regional analysis sometimes suffers from deterioration of the large-scale structure than that of the global analysis due to limitations in the domain size and observations. The large-scale error may cause the displacement error for disturbances such as typhoons or synoptic-scale fronts and degrade the performance of convective-scale DA. Although several scale-dependent blending methods of global and regional analyses have been proposed to alleviate those large-scale errors, these blending methods may hinder the optimality of individual DA. Guidard and Fischer (2008) and Dahlgren and Gustafsson (2012) introduced the augmented information vector with the global analysis into the regional variational assimilation and reported promising results. However, their formulations require several assumptions for the error correlations and ignore the covariance between the global and the regional forecast errors. In this study, we extend their augmented variational formulation to an ensemble variational method to relax those assumptions and take the flow-dependency of the forecast error into account. We test the proposed method in the one-way coupling system using ideal one-dimensional models proposed by Lorenz (2005) and compare the results with those of the separate assimilations and of the previous studies. The effect of the covariance between the two domains will also be discussed.
AS47-A020
Applying Variational Bias Correction to Surface Data with a Convective-scale Data Assimilation System
Yi-Hsuan LIN1,2#+, Yen-Chih SHEN1, Guo-Yuan LIEN3, Shu-Chih YANG2, Yi-Chuan LO4
1Central Weather Administration, Taiwan, 2National Central University, Taiwan, 3RIKEN Advanced Institute for Computational Science, Japan, 4Central Weather Bureau, Taiwan
A dense observation network of surface weather stations has been established in Taiwan, which can provide surface pressure, wind, temperature, and humidity measurements in real-time. These observations carry crucial information about spatial and temporal variations in convective-scale weather systems. However, significant biases exist between near-surface observation and model simulation outputs, posing a major challenge in assimilating surface data effectively. The complex terrain of Taiwan even deteriorates the biases between the observations and the model. Therefore, implementing a bias correction scheme in surface data assimilation in Taiwan becomes a critical issue to consider. This study was inspired by the well-established variational bias correction (VarBC) method commonly used in satellite data assimilation. The VarBC method is extended to the surface data assimilation and implemented in a WRF/WRFDA-based convective-scale data assimilation system at the Central Weather Administration (named CWA-RWRF) to assimilate dense surface observations in Taiwan. Utilizing the statistical relationship between innovations and multiple predictor variables in the bias model of VarBC, adaptive bias correction is achieved during assimilation. The impact of the VarBC on surface data assimilation is investigated with a Meiyu front-related heavy rainfall events characterized by coastal convection over western Taiwan from 6 to 8 June 2022. A set of VarBC models is introduced for assimilating 10-meter wind, 2-meter temperature, and 2-meter humidity observations, while radar observation data are also assimilated as in the usual operation. Results indicate that the use of the VarBC reduces the mean errors in the analysis and forecast fields, with particularly significant improvements in 10-meter wind speed and daytime temperature. The influence of the bias correction on the dynamic and thermodynamic conditions for the rainfall events will be further discussed in the presentation.
AS47-A021
Identification of Observation-sensitive Areas for Improving Numerical Prediction of Asian Dust Storms in South Korea Based on Dust Influx Synoptic Patterns
Seungyeon LEE1#+, Xiaohao QIN2, Seon Ki PARK1
1Ewha Womans University, Korea, South, 2Institute of Atmospheric Physics, Chinese Academy of Sciences, China
In air quality prediction, initial conditions are essential for a coupled atmosphere-chemistry model based on atmospheric and aerosol/chemistry observations. Typically, a greater quantity and higher quality of observations result in more accurate model outcomes. However, forecast errors within a specific region of interest can magnify from observational deficiencies in a particular upstream area, primarily originating from initial errors in that region. Therefore, the primary task is to identify these upstream areas where minor initial errors could escalate into significant forecast errors within the area of interest. Conditional Nonlinear Optimal Perturbation for Initial Conditions (CNOP-I) can serve as a crucial tool for adaptive (targeted) observations. Computing CNOP-I involves multiple energy equations defining various variables such as kinetic energy, dry energy, moist energy, etc. This study comprises of two primary objectives: categorizing synoptic weather patterns through which Asian Dust Storms (ADSs) intrude the Korean Peninsula and identifying sensitive areas for adaptive observations concerning each distinct synoptic pattern. A thorough investigation was conducted on ADS events occurring in South Korea over the past 32 years (1990 to 2021). Through principal component analysis, it was confirmed that key variables like temperature, vertical velocity, divergence, specific humidity, ozone mass mixing ratio, and eastward wind play pivotal roles in the occurrence and movement of ADSs, with robust downdrafts and divergence emerging as crucial factors ultimately leading ADSs to converge on the Korean Peninsula. Utilizing these factors as primary variables, dust influx synoptic patterns are classified using the K-means clustering method to identify sensitive areas for adaptive observations in air quality prediction through CNOP-I. These proposed targeted observation areas related to dust patterns aim to improve air quality prediction by categorizing weather conditions triggering severe ADS occurrences in South Korea and identifying upstream regions for intensified observations through international collaborations.
AS48-A001
Significant Reduction of Unequal Population Exposure to Climate Extremes by Achieving the Carbon Neutrality
Seokgeun OH1+, Jung CHOI1, Min-Jee KANG1, Sujong JEONG1, Seung-Ki MIN2, Sang-Wook YEH3, Yeon-Hee KIM2, Seok-Woo SON1#
1Seoul National University, Korea, South, 2Pohang University of Science and Technology, Korea, South, 3Hanyang University, Korea, South
Climate extremes, such as hot temperature and heavy precipitation events, have devastating effects on human societies. As the planet warms, they have become more intense and more frequent. To avoid irreversible damage from climate extremes, many countries have committed to achieving net-zero anthropogenic carbon emissions, or carbon neutrality, by 2050s. Here, we quantify the impact of carbon neutrality on population exposure to climate extremes using multi-model projections from the Coupled Model Intercomparison Project Phase 6 (CMIP6) based on the Shared Socioeconomic Pathway (SSP)1-1.9 and SSP3-7.0 scenarios. It is found that the increasing exposure of the population to hot-temperature and heavy-precipitation extremes can be substantially reduced by 87–98% in the late 21st century by achieving carbon neutrality. The benefits of carbon neutrality are particularly pronounced in Africa and Asia. The potential benefits of carbon neutrality are also significant in North America, Europe, and Oceania, where a reduction in climate extremes is more than twice as important as population decline in reducing population exposure to climate extremes. These results provide important scientific support for ongoing efforts to achieve net-zero carbon emissions by 2050s to reduce potential climate risk and its inequity across continents.
AS48-A003
Characterization of Urban Heat Island Due to Heat Wave Events During the Warming Phase in Taiwan
Yhen-Jhen YOU#+, Fang-Yi CHENG
National Central University, Taiwan
In recent years, the strengthened subtropical pacific high-pressure system has frequently led to prolonged high temperatures. Due to the influence of heatwave events, certain urban areas consistently exhibit higher temperatures than their rural counterparts—a phenomenon known as the urban heat island effect. Previous studies have focused less on the interaction between large-scale circulation patterns and urban heat island effects. The purpose of this study is to examine impact of the Western North Pacific Subtropical High (WNPSH), the predominant synoptic weather system during summer on heat waves and its subsequent influence on the urban heat island. Utilizing EOF analysis and anomalous analysis, the results indicate that the intensity of the WNPSH system has increased in recent years, particularly for the leading EOF (EOF1). This phenomenon may be attributed to the global warming effect. Thus, we focus on EOF1 and its impact on temperature, humidity, and precipitation in Taiwan. A heatwave event was defined as the maximum daily temperature exceeding the 95th percentile for three consecutive days in the plain area (altitude < 500 m). After identifying the heatwave days, the WRF model coupled with the urban canopy model was used to investigate the impact of heat wave events on the urban heat island problem in Taiwan. EOF1 is regressed with humidity, precipitation, and specific humidity to examine the heat wave effects. The preliminary analysis indicates that the warming phase may be more significant in urban sites than rural ones, especially in coastal sites where higher humidity may cause uncomfortable conditions. Detailed discussion will be illustrated during the meeting.
AS48-A010
Future Extreme Climate Projections for South Korea Under Global Warming Targets (1.5°C, 2.0°C, 3.0°C)
Minhae KIM1#+, Jin-Uk KIM2, Tae-Jun KIM1, ChuYong CHUNG1, Young-Hwa BYUN1
1National Institute of Meteorological Sciences, Korea, South, 2Korea Meteorological Administration, Korea, South
This study aims to predict the future climate of South Korea by utilizing climate change scenario. The focus is on forecasting the country’s future climate under warming targets of 1.5°C, 2.0°C, and 3.0°C. The timing of the warming target attainment points was determined using the global climate model (UKESM1), calculating the years when the global temperature rose by 1.5°C, 2.0°C, and 3.0°C relative to the pre-industrial era(1850-1900). In this study, we utilized high-resolution (1km) gridded observation data(2000-2019) and climate change scenario (2021-2100) using PRIDE model in South Korea. We generated 20 ensemble members based on 5 regional climate models (RCM) and 4 Shared Socioeconomic Pathway (SSP) scenarios for analysis. Using the present period of 2000-2019, the annual mean temperature is projected to increase by +0.7°C, +1.4°C, and +2.6°C during the 1.5°C, 2.0°C, and 3.0°C warming periods, respectively. Precipitation is projected to slightly decrease during the 1.5°C warming target, it is anticipated to significantly increase with further warming. The analysis of future extreme climate conditions due to warming reveals an increase in summer heat extremes and a decrease in winter cold extremes. Extreme precipitation and extreme wind/humidity indices are generally expected to increase with warming. According to the research findings, if additional warming beyond 1.5°C occurs, South Korea could face more severe extreme climate events. Therefore, the results of this study are expected to provide essential information for formulating climate change adaptation and mitigation policies different regions in South Korea.
AS48-A014
Projected Thermal Stress in Korea from 1KM High Resolution Scenarios
JaeHee LEE1#+, Hyun Min SUNG1, Jin-Uk KIM2, Sungbo SHIM1, ChuYong CHUNG1, Young-Hwa BYUN1
1National Institute of Meteorological Sciences, Korea, South, 2Korea Meteorological Administration, Korea, South
One of the various thermal indices, apparent temperature (AT) is widely used by meteorological agencies around the world in a wide range of fields, such as heat health warning systems and worker productivity assessments. In this study, we investigated the characteristics of AT changes in South Korea using a national standard climate change scenarios with a high resolution of 1km based on the Coupled Model Intercomparison Project Phase 6(CMIP6). We analyzed thermal stress and its associated contributions during the climate change period in South Korea and five major cities. In the present-day(PD), high AT occurs in major cities due to high temperatures (TAS) and relative humidity (RH). We find that changes in AT are mainly attributed to changes in TAS, whereas changes in RH play a relatively minor role. Similar annual trends between AT and TAS show that the long-term increase in AT is characterized by an increase in TAS, with RH changes playing a relatively minor role. Our research results demonstrate that significant AT can occur even when TAS is relatively low, primarily due to high humidity. Particularly under future warmer climate conditions, high AT may occur first in the five major cities and then expand to surrounding areas. Under future warmer climate conditions, increased TAS and RH from March to June, traditionally not considered hot seasons, may lead to earlier onset of heat risk and more frequent occurrence of high heat stress events.
AS49-A008
Improving the Prediction of the 3 July 2019 Kaiyuan Tornadic Supercell and Embedded Tornado with Data Assimilation
Haojia LI#+
Nanjing University, China
The 3 July 2019 Kaiyuan City, Liaoning Province, tornadic supercell is simulated with the advanced research version of the Weather Research and Forecasting (WRF-ARW) model using three nested grids with 4.05-km, 1.35-km, and 450-m grid spacings. The radar radial velocity and reflectivity data from eight operational Doppler weather radars in different wavebands together with automatic weather station (AWS) data are assimilated through the ARPS three-dimensional variational data assimilation (3DVAR) and cloud analysis systems on the 450-m grid to generate a more accurate initial condition that includes a well-analyzed supercell and associated low-level mesocyclone. Sensitivity experiments show that the analyses and forecasts of the tornadic supercell of the control experiment assimilating both radar and AWS data are significantly improved relative to the one without special data assimilation. The near-surface vortex intensification is not produced when the radar radial velocity and reflectivity data are assimilated alone without AWS data. One assimilation cycle experiment performs better than multi-cycle ones, due to the additional latent heating added by the cloud analysis in each cycle. The use of a divergence constraint in the 3DVAR plays an important role in establishing the low-level mesocyclone during the assimilation and forecast. A tornado-resolving simulation with further nested grids 150 m, 50 m, and 16 m grid spacings starts from the 450-m control initial condition is conducted. The inner-most grid covers the entire period of the observed tornado outbreak and successfully captures the development of tornadic vortices. The intensity of the simulated tornado on the 16-m grid reaches the enhanced Fujita scale 2 (EF2) intensity. The simulated tornado vortices evolved through one-cell, two-cell, and multi-vortex stages. This study represents the first time a real tornado is successfully simulated through the assimilation of multi-radar and high-density surface station data.
AS49-A010
The KIAPS Weakly-coupled Atmosphere-ocean Data Assimilation System
Jiyoun KIM#+, Hye-yeong JANG, Eunbyeol KO, Adam CLAYTON, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems, Korea, South
It has long been known that coupling between the various Earth system components (the ocean, atmosphere, sea ice, and land) produces improved forecasts on seasonal and longer time scales. KIAPS (Korea Institute of Atmospheric Prediction Systems) is now developing a coupled atmosphere-land-ocean-sea ice model aimed at extended-range forecasts, using NEMO (Nucleus for European Modelling of the Ocean) as the ocean model. Also, we are developing a weakly-coupled atmosphere-ocean data assimilation (WCDA) system to provide more balanced initial conditions for this new coupled model. The atmospheric model is based on the KIM (Korean Integrated Model) v4.0 and the atmospheric data assimilation (DA) system uses the “KVAR” variational DA software to run 3DVAR-FGAT analyses within a 6-hour DA cycle. The ocean system is based on KMA’s “GODAPS” system (Global Ocean Data Assimilation and Prediction System), which uses the NEMO ocean model. The ocean DA system uses the NEMOVAR software to run 3DVAR-FGAT analyses, with KIM surface forcing. To match the atmospheric DA cycles, we changed the ocean DA cycles from 24-hours to 6-hours. And we upgraded the NEMO version used by the coupled model. We developed the WCDA system which coupled the ocean DA system to the KIM atmospheric DA system. And we also produced the uncoupled DA system for control experiments. Here, we will introduce our progress for the new WCDA system for the KIM coupled model and present preliminary results.
AS49-A011
Development of Global Ocean data Assimilation System for Use in a Weakly-coupled Data Assimilation System
Eunbyeol KO#+, Adam CLAYTON, Hye-yeong JANG, Jiyoun KIM, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems, Korea, South
The Korea Institute for Atmospheric Prediction Systems (KIAPS) is developing a coupled earth system NWP system aimed at improving the performance of extended-medium-range forecasts. The system will be based on a new coupled model which combines the existing “Korean Integrated Model” (KIM) atmosphere model with models for other earth system components, including the NEMO (Nucleus for European Modelling of the Ocean) ocean model and the SI3 (Sea Ice Modelling Integrated Initiative) sea ice model. To provide the ocean data assimilation component, we are adapting the KMA GODAPS (Global Ocean Data Assimilation and Prediction System), which consists of the NEMO ocean model, the CICE (Community Ice CodE) sea ice model, and the NEMOVAR (NEMO VARiational) data assimilation (DA) system, and obtains surface forcing from KMA UM (Unified Model) forecasts. As part of this work, we have added support for use of KIM rather than KMA UM surface forcing, and we have reduced the cycling period and window length from 24 hours to 6 hours, to match the atmospheric DA cycling system. In this study, we will summarize the configuration of the ocean DA system, and then discuss the impact of changing surface forcing and shortening the cycling period on key analysis and forecast metrics.
AS49-A012
Development of a Global Ocean Data Assimilation System for the NEMO-SI3 Model
Hye-yeong JANG#+, Eunbyeol KO, Jiyoun KIM, Adam CLAYTON, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems, Korea, South
KIAPS (Korea Institute of Atmospheric Prediction Systems) has developed a global ocean data assimilation system base on KMA (Korea Meteological Administration) GODAPS (Global Ocean Data Assimilation and Prediction System). The ocean data assimilation (DA) system is based on NEMOVAR, and uses a 3-Dimension Variational data assimilation – First Guess at Appropriate Time DA method. The assimilated observations include SST observations from satellite and moored buoys, temperature profiles collected by Argo floats, and satellite observations of sea-level anomaly and sea ice concentration. Our actual first goal is to develop a weakly-coupled DA system that combines Korean Integrated Model (KIM)’s existing atmosphere/land DA system with a separate DA system for the NEMO (Nucleus for European Modelling of the Ocean) model that has been chosen for use within the KIM coupled model. In order to make the system suitable for weakly-coupled DA with KIM, we tried to change ocean and sea-ice model from NEMO-CICE (Community Ice CodE) to NEMO-SI3 (Sea Ice Modelling Integrated Initiative) based on the ocean DA system with 6-horly DA window. We will present studies of updated ocean-sea ice model aimed at assessing the impact of the changes on ocean analysis performance.
AS49-A013
Development of 3-hourly Update Global NWP Cycle System
Wonho KIM#+, Adam CLAYTON, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems, Korea, South
KMA (Korea Meteorological Administration) operational global NWP system is based on a 6-hour analysis cycle, with 6-hour data assimilation windows. Early-observation-cutoff analyses are used to initialise the main forecasts, and late-observation-cutoff analyses used to generate background forecasts for the next analysis update. In this system, the most up-to-date forecasts can be sometimes be based on observational data that is at least 6 hours old. By producing analyses and forecasts more frequently, we can reduce this time gap, and potentially improve the quality of the most up-to-date forecast products at certain times of day. In this study, we evaluate two methods of producing 3-hourly rather than 6-hourly analyses: 1. Simply adding extra analyses and forecasts to the current system, without changing the underlying data assimilation cycle. 2. Switching to a 3-hour cycle based only on early-observation-cutoff analyses, but keeping the analysis window lengths at 6 hours. The latter method requires us to overlap the data assimilation windows, but observations are still assimilated only once. Apart from more frequent forecast delivery, this new cycling strategy can benefit from producing smaller analysis increments, and therefore reducing linearization errors in the analysis steps. On the other hand, removing the late-observation-cutoff analyses reduces the number of observations available for assimilation. After introducing our experiment configurations, and the impacts on observation usage, we present results from extended NWP experiments designed to answer the following questions: 1. What is the impact of moving to the 3-hourly cycling system on forecast performance. 2. What is the impact of using fewer observations. 3. What is the impact on gravity-wave noise.
AS49-A014
Development of the Prototype of Observing System Simulation Experiment (OSSE) System Using Korea Integrated Model (KIM) : Verification of Analysis in Terms of Observation Effect
Hyun-Jun HAN#+, Jeon-Ho KANG, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems, Korea, South
One of most advantageous thing of OSSE is that researcher can verify the result of NWP with respect to the truth (called as nature run (NR)). Furthermore, observation can be simulated for any proposed (for example, making new type of sensor, applying realistic forward operator and method, specifying the locations, and error characteristics of the observation). To use such advantage of OSSE, we developed the prototype of global OSSE system used Korea Integrated Model (KIM). In this study, we will introduce the theoretical background of OSSE, forecast system of KIM, and the contents considered for development of the OSSE system used KIM, briefly. To verify the OSSE system used KIM, we performed the denial experiments for synoptic observation (aircraft) and satellite observation (MHS), not only in OSSE but also in OSE. Because of the absence of wind and temperature observation of aircraft in aircraft denial experiment, the performance decrease of KIM analysis against IFS reanalysis were mainly shown at 250 hPa (which is a cruising altitude of aircraft) of the u, v, and T variable. In MHS denial experiment, the performance decrease of T and q variable were appear in KIM analysis. The reaction of analysis due to the observation denial in both OSSE and OSE weren't in the same perfectly, but the result from OSE and OSSE system was similar, we evaluated the OSSE system used KIM is well made enough to analyze the effect of observation. The reaction of analysis due to the observation denial in both OSSE and OSE weren't in the same perfectly, but the result from OSE and OSSE system was similar, we evaluated the OSSE system used KIM is well made enough to analyze the effect of observation.
AS49-A015
Study on Extending the Use of Microwave Satellite Data Over the Land
Hyeyoung KIM#+, Jeon-Ho KANG
Korea Institute of Atmospheric Prediction Systems, Korea, South
The ATMS data have, until now, only been assimilated over sea in Korea Integrate Model(KIM). To extend the coverage of the ATMS over land and sea-ice, we firstly assimilated only the high peaking, non-sensitive surface, channels (ch8~15 over land and ch22~23 over sea-ice). To extend the use of ATMS high peaking channel over land, bias correction and observation error covariance were adjusted. As a result, the analysis field error of stratosphere was reduced especially and the forecast skill improved (GPH NH: 0.48~2.65%, Asia: 1.35~ 2.35%). In order to assimilate more surface-sensitive microwave observation, the contribution of the atmosphere must be separated by removing the effect of surface radiance from the observed brightness temperature. Compared to the ocean, the land skin temperature has higher uncertainties, and surface emissivity is larger at around 0.8-0.95 with higher heterogeneities due to the complex surface condition, making it harder to model. So, estimating the land emissivity/surface temperature directly from satellite is tested. Using the radiation transfer equation and observation, the observation-dependent surface emissivity estimation method was introduced. Preprocessing was performed to remove the edge area and scattered data that cause errors in emissivity retrieval, and remove the data that differed significantly from the emissivity climate value. It was diagnosed that the model surface temperature is about 3K higher than the value calculated based on ATMS observation, which cause 20% difference in the observation increment of channel 6. It is necessary to use a more appropriate surface temperature for microwave surface radiance and correct the resulting bias. The number of observation available on land increased by 200% when an observation-dependent emissivity is applied compared to the default emissivity model. It will be tested to support a more reliable assimilation of the surface-sensitive channels over land.
AS49-A018
Evaluation of the KIAPS LETKF-based Radar Reflectivity DA System
Dayoung CHOI#+, Adam CLAYTON, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems, Korea, South
The renewed KIAPS (Korea Institute of Atmospheric Prediction Systems) aims at developing a unified framework for seamless prediction from very short range (~6 hours) to extended medium range (~30 days), including coupling to various Earth system components, such as the land surface, oceans, and sea ice. For very short range forecasts, KIAPS is developing at the high-resolution (1-5km) model targeting storm-scale high-impact weather over East Asia, centered on the Korean peninsula. We have been developing a convective-scale DA system based on Local Ensemble Transform Kalman Filter (LETKF) that can respond to high-density observations such as radar, with increased horizontal resolution of the model. In order to assimilate from meso-scale observations to synoptic-scale observations, we have completed the development of LETKF-based radar reflectivity DA system for a “testbed” system based on a high-resolution, limited-area version of WRF and a testbed background ingestion system in KIM Package for Observation Processing (KPOP). The LETKF-based convective-scale DA system has been extended to assimilate conventional observations (Sonde, Surface, Aircraft, etc.) provided by KPOP in addition to radar reflectivity observations. Also, we have established the basic framework called the regional ensemble analysis system that is consist of testbed, KPOP, LETKF-based convective DA system. In order to get reasonable ensemble analysis fields through LETKF-based convective-scale DA system and tune radar DA techniques, we need to investigate the analysis performance of radar reflectivity DA added conventional observations. So, we will perform cycle experiments for the assimilation of radar reflectivity adding Sonde, Aircraft, and Surface observations using the regional ensemble analysis system. In this presentation, we will introduce results for the evaluation of LETKF-based radar reflectivity DA on observation-space statistics and the characteristics of ensemble analysis fields. And then, we will proceed with tuning the LETKF-based radar reflectivity method depending on the evaluated analysis performance.
AS49-A019
An Impact Study on a Deep Learning-based Aircraft Temperature Bias Correction in the Korean Integrated Model
Hui-Nae KWON1,2#+, Hyeon-Ju JEON1, Jeon-Ho KANG1, In-Hyuk KWON1, Seon Ki PARK2
1Korea Institute of Atmospheric Prediction Systems, Korea, South, 2Ewha Womans University, Korea, South
The aircraft-based observation bias exists in temperature data due to various factors such as the aircraft type, flight phases, and equipment sensors. Nonetheless, the observation used in the numerical weather prediction (NWP) models is one of the important conventional data. Although the static bias correction (BC) based on the linear regression was applied to the Korean Integrated Model (KIM) Package for Observation Processing (KPOP) system which is being operated in practice, there were limitations of a spatial discontinuity and a dependency on the calculation period of BC coefficients. To reduce these constraints and consider the spatial and temporal characteristics and correlations of each observation at the same time, a bias estimation model was devised based on a Multi-layer Perceptron (MLP) applied an attention method in this study. The attention method makes an estimated bias concentrate on the correlation of more related observation variables. After the predicted bias was removed in the pre-processed procedure, the statistics value improved about 40% and the number of observations available in the data assimilation (DA) system increased about 3.5% in a given test period. As results of DA cycle tests, the error of analysis fields against IFS data was reduced over the North Pacific and North Atlantic Ocean at 250hPa, where most observations exist. Meanwhile, the error increased over North America and Europe area. It results from the different characteristics of model background error according to those regions. In future research, we will take into account way to further reflect regional error characteristics into this BC model.
AS52-A004
Machine Learning Approaches for Boundary Layer Observations with a Low-cost Mini-radiosonde System
Min-Lun WU1, Chiao-Wei CHANG2, Shih-Hao SU1#+
1Chinese Culture University, Taiwan, 2National Taiwan University, Taiwan
This study presents a machine learning (ML) based calibration process and instrument error correction experiment for the novel low-cost mini-radiosonde system, Storm Tracker (ST). To address temperature and moisture errors caused by solar radiation heating. We adopted the Generalized Linear Model (GLM) and Gradient Boosting Model (GBM) as the kernel for ML model development. We used the co-launch radiosonde data from ST and Vaisala-RS41 (VS) between 2018 and 2022 as training inputs to develop a two-stage calibration approach. The data calibration system can correct the observed temperature with the ML model and then calibrate the moisture with the corrected temperature as input. In the data calibration workflow, we also designed a suitable experimental platform based on ST's characteristics to test the instrument's measurement error. It can calibrate the instrument's error as the standard reference for each ST instrument. The results show that the measurement error of ST is a normal distribution. About 70% of the ST instrumental errors can be reduced to within the limitation of instrument accuracy after statistical error correction. The remaining 30% of the instruments still retain the characteristics of random errors, which can be corrected through our ML models. The linear calibration model (GLM) and the non-linear calibration model (GBM) have been compared. Results show that GLM exhibits good calibrating capability for observing the planetary boundary layer (1000-700 hPa). On the other hand, GBM, with a more complex structure, maintains even better calibrating performance statistically. It can reduce the overestimation of convective available potential energy (CAPE) and column water vapor (CWV) amount for PBL observations. Furthermore, this study's systematic data correction process has been made accessible through a dedicated website. This user-friendly platform allows for the seamless application of the correction process, providing a convenient tool for real-time ground-based data correction.
AS52-A008
Spatial Characteristics of Remote Rainfall Events Caused by Typhoons' Outer Circulation and Northeasterly Monsoon
Wen-Wei TSENG1+, Li-Huan HSU2, Shih-Hao SU1#, Jung-Lien CHU2
1Chinese Culture University, Taiwan, 2National Science and Technology Center for Disaster Reduction, Taiwan
This study analyzes remote rainfall events in northeastern Taiwan from September to February over the period of 1980-2020. These events are triggered by the interaction between typhoons and the northeasterly monsoon flow. When background northeasterly winds exceed 7 m/s, a “remote rainfall-prone area” can be defined north of the Philippines, spanning the northern South China Sea to the north Philippine Sea. The confluence of typhoon outer circulations and strong monsoon winds creates a convergence zone, enhancing rainfall in northeast Taiwan by an average of 80–220 mm per day. With typhoons positioned over the rainfall-prone area, the probability of daily maximum rainfall exceeding 200 mm rises above 20%, particularly in the region between 20°N–22°N and 116°E–124°E, northward to Luzon Island. Here, the probability can top 45%. The zone of highest risk for extreme remote rainfall events lies between 20°N–22°N and 118°E–120°E, with over 90% probability when the key convergence zone aligns. Although this convergence zone does not necessarily coincide with significant baroclinic forcing, the abundant moisture supplied from the typhoons remains conducive to heavy rainfall events.
AS52-A010
Analysis of the Variability of Cold-air Damming and Barrier Wind with Snowfall in the Yeongdong Region of Korea
Ji Yun KIM1#+, Han JINHEON1, Kim TAE YEON1, Byung-Gon KIM1, Byunghwan LIM2
1Gangneung-Wonju National University, Korea, South, 2National Institute of Meteorological Sciences, Korea, South
The Yeongdong region experiences various mesoscale phenomena due to the complex topography of the Taebaek Mountains, particularly during winter. Predominant mesoscale features such as Cold-Air Damming (CAD) and barrier winds significantly impact snowfall characteristics, posing challenges for accurate snowfall forecasting. We aim to improve snowfall forecast by classifying Strong Snow (SS) and Strong CAD (SC) cases under similar weather conditions (850hPa temperature below -10℃) using rawinsonde data. Through analysis of observations and LDAPS data, the main factors contributing to snowfall differences between SS and SC cases are investigated. We introduce the Froude number (Fr) to quantify snowfall variability induced by Barrier wind and CAD. In SS1 and SS2 cases, strong northerly to northeasterly flow up to 2km was observed in rawinsonde data. LDAPS revealed a dome-shaped structure over the East Sea with a temperature gradient of 0.5-1K. Snowfall occurred when northeasterly flow penetrated inland deeply. In contrast, SC1 and SC2 cases exhibited a strong inversion layer, with lower-level northwesterly flow thicker up to 1km than the northeasterly layer. LDAPS indicated a strong CAD with a temperature gradient exceeding 2K, inhibiting snowfall by preventing snow clouds from penetrating inland. During the SC3 case on February 14, 2023, the northwesterly barrier wind was poorly represented in the LDAPS simulation. Strong barrier wind (approximately 10 ms-1) inhibited the inland penetration of snow clouds according to rawinsonde, Wind Profiler, and Buoy data. Subsequently, heavy snowfall occurred on February 15 with the inflow of strong northeasterly winds. The investigation of the Froude number confirms the significant influence of barrier wind and CAD on snowfall location and amount. Fr criteria for quantitative differentiation between SS and SC cases at each locations. The investigation of the Froude number would help to quantify the influence of barrier wind and CAD on snowfall location and amount.
AS52-A011
Characteristics of Downslope Windstorms in the Yeongdong Region of Korea
Han JINHEON1#+, Ji Yun KIM1, Kim TAE YEON1, Byung-Gon KIM1, Jung-Hoon KIM2, Ji-Hoon JEONG3, Byunghwan LIM4
1Gangneung-Wonju National University, Korea, South, 2Seoul National University, Korea, South, 3Korea Meteorological Administration, Korea, South, 4National Institute of Meteorological Sciences, Korea, South
Characteristics of downslope windstorm (DW) has been used for the criteria of DW selection mainly based on 1-min average wind and the other meteorological conditions in the Yeongdong region for 2000 - 2020. The criteria is as follows; First, a classification procedure for the downslope windstorm is proposed using surface wind speed (greater than 99 percentile), 1-hour longevity of strong wind (SW), westerly wind direction, low humidity (less than 20 percentile), and leeside warming. The number of DW days satisfying the proposed criteria is 221 (2.9% of total days) for 2000 – 2020. The DW occurrences show distinctive annual variation with its peak in April. Mean wind speed of DW days is 8.2 m s-1 with its duration of 2 hr 30 min and relative humidity of 28 % at Gangneung. Two DW episodes are chosen satisfying the criteria for the intensive analysis. The first episode was 7 May 2021. The sounding shows that the layer of wind speed greater than 25 m s-1 was lowered down to 925 hPa at Gangneung (leeside) relative to 850 hPa at Hoengseong (windward), in the afternoon along with significant warming and drying. The second episode (11 April 2023) was more than 2 times stronger than the first in terms of its intensity and duration except for much more humid condition. The preliminary analysis shows that this kind of strong downslope windstorm was attributable to the partial reflection of mountain wave in the lower troposphere. Froude numbers of Wonju (windward) and Gangneung (downwind) for the both DW events were increased 4 and 5 times greater than those of normal days, respectively. We need to investigate DW mechanisms in terms of gravity wave dynamics and further prerequisite conditions of favorable downslope windstorms to improve DW forecast in the leeside (Yeongdong) of the mountains.
AS54-A005
Bias Correction of Post-process of Multivariate Drought Index Evaluated from the CESM2-LENS
Phynodocle Vecchia RAVINANDRASANA1,2#+, Christian FRANZKE2
1IBS Center for Climate Physics, Korea, South, 2Pusan National University, Korea, South
Efforts to understand extreme events often require reliable climate metrics information. Several studies have focused on correcting the climate model simulation to study the effects of climate change. However, these conventional bias correction methods often fail to distinguish the inter-variable dependence of climate variables output over the climate scenario, even though it is considered relevant for the various impact studies. To counter this, this study evaluated the effectiveness of post-processing bias correction of extreme climate indices rather than the climate models data at a global scale. The Shared Socioeconomic Pathways (SSP3-70) in the ICCP CESM2 large ensemble climate model and ERA5 reanalysis datasets were used in this study. The multi-year drought indices of Standardized Precipitation Evapotranspiration (SPEI) and Quantile Delta Mapping Bias Correction (QDM)-BC method were used. The period between 1979-2014 was used as the calibration period, while 2015-2022 as the evaluation period of the outputs of the SPEI indices over the comparable period (1979–2022). The results show that the QDM-BC post-processing is effective in preserving the distribution of the SPEI as compared to applying the BC to raw climate data. Therefore, this study highly recommends post-processing bias-correction methods on climate extremes in order to preserve the climate change signal and the internal variability in the changing climate of each ensemble member.
AS54-A006
Attributing Greenland Climate Extremes to Anthropogenic Forcing and Natural Variability
Manuel Tobias BLAU1,2#+, Kyung-Ja HA2, Eui-Seok CHUNG3
1IBS Center for Climate Physics, Korea, South, 2Pusan National University, Korea, South, 3Korea Polar Research Institute, Korea, South
Greenland occasionally experiences extreme temperature conditions in terms of temperature and precipitation, which exert a significant impact on the ice sheet covering major parts of the land mass. By employing stochastical methods, we aim to disentangle the role of natural variability and anthropogenic forcings on the development and maintenance of prevailing temperature anomalies over Greenland. Based on current reanalysis datasets and the CESM2 Large Ensemble, we analyze and attribute anomalous warm years to natural variability and anthropogenic forcings. The preliminary results indicate the dominance of blocking-like conditions over Greenland, which coincided with an anomalous anti-cyclonic motion advecting moisture and warm air into the interior of Greenland, destabilizing the atmosphere there. This results in radiative radiative feedback enhancing local warming. Further, analysis of the role of climate variability modes gives implications for the predictability of summer temperature extremes.
AS54-A012
Increasing Global Terrestrial Diurnal Temperature Range for 1980–2021
Xiaowen HUANG1+, Robert DUNN2, Laurent LI3, Tim MCVICAR4, Cesar AZORIN-MOLINA5, Zhenzhong ZENG1#
1Southern University of Science and Technology, China, 2Met Office Hadley Centre, United Kingdom, 3Laboratoire de Météorologie Dynamique, France, 4Commonwealth Scientific and Industrial Research Organisation, Australia, 5Centro de Investigaciones sobre Desertificación, Consejo Superior de Investigaciones Científicas (CIDE, CSIC-UV-Generalitat Valenciana), Spain
The 2021 IPCC report found that most studies show declining trends for the global diurnal temperature range (DTR) since the 1950s, decreasing mainly during 1960–1980. This issue is revisited here using an up-to-date in-situ data set, Hadley Center Integrated Surface Database, constrained by rigorous station selection conditions. The global observed DTR trend was found to reverse during 1980–2021, increasing significantly at a rate of 0.091 ± 0.008°C decade−1. The trend was dominated by a faster rate of increasing daily maximum air temperature. This increasing observed trend in the past four decades was not fully captured in raw CMIP6 models, as models only partially capture the spatial patterns. With global CMIP6 outputs and regionally-available observations, the global land DTR was then estimated, through emergent constraints, to be 0.063 ± 0.012°C decade−1. The study raises concern for risks of increasing DTR globally and provides new insights into global DTR assessment.
AS54-A013
Reconciling Opposite Trends in the Observed and Simulated Equatorial Pacific Zonal Sea Surface Temperature Gradient
Wenrong BAI1+, Hailong LIU2#, Pengfei LIN2, Xichen LI2, Wang FAN2
1Beijing Meteorological Bureau, China, 2Chinese Academy of Sciences, China
The reasons for large discrepancies between observations and simulations, as well as for uncertainties in projections of the equatorial Pacific zonal sea surface temperature (SST) gradient, are controversial. We used CMIP6 models and large ensemble simulations to show that model bias and internal variabilities affected, i.e., strengthened, the SST gradient between 1981 and 2010. The underestimation of strengthened trends in the southeast trade wind belt, the insufficient cooling effect of eastern Pacific upwelling, and the excessive westward extension of the climatological cold tongue in models jointly caused a weaker SST gradient than the recent observations. The phase transformation of the Interdecadal Pacific Oscillation (IPO) could explain ~51% of the observed SST gradient strengthening. After adjusting the random IPO phase to the observed IPO change, the adjusted SST gradient trends were closer to observations. We further constrained the projection of SST gradient change by using climate models’ ability to reproduce the historical SST gradient intensification or the phase of the IPO. These models suggest a weakened SST gradient in the middle of the 21st century.
AS54-A020
Decadal Relationship Between Arctic SAT and AMOC Changes Modulated by the Pacific Variability
Bowen ZHAO1, Pengfei LIN2#, Hailong LIU2, Aixue HU3, Xiaolong CHEN2, Lu YANG2+
1China Meteorological Administration, China, 2Chinese Academy of Sciences, China, 3National Center for Atmospheric Research, United States
The faster warming for Arctic Ocean surface air temperature (SAT) relative to that at lower latitude is connected with various processes, including local radiation feedback, poleward oceanic and atmospheric heat transport. However, we do not fully understand how combinations of different low-frequency internal climate modes influence Arctic amplification on the decadal timescale. Here, the decadal Arctic SAT variation, its connection with the Atlantic Meridional Overturning Circulation (AMOC) and possible underlying mechanisms, are investigated based on several independent observational proxies, pre-industrial experiments, and historical large ensembles of two CMIP6 models. Our study suggests that AMOC and Arctic SAT vary in phase on the decadal timescale, whereas this relationship is weak at the interannual timescale. Further analysis shows that the AMOC accompanied with cross-basin oceanic water/heat transport between Atlantic and Arctic would alter air–sea interface exchange over the melting ice regions, and then amplified poleward atmospheric heat and moisture transports which originated from Pacific Ocean in budget analysis. The resulting enhanced downward longwave radiation finally warms the Arctic SAT. Additionally, the North Pacific Oscillation (NPO) can modulate the relationship between AMOC and Arctic SAT on decadal scale. Specifically, a phase shift in the NPO can contribute 10%–40% of the correlation between AMOC and Arctic SAT. Our study provides potential sources for predicting the Arctic climate and constraining its uncertainty in future projections.
AS55-A002
Exploring the Impact of PM2.5 Phase State on Particle Size Distribution
Changjoon SEONG1#+, Changhyuk KIM2, Zhijun WU3, Jiyi LEE4, Kwangyul LEE5, Jun-Young AHN5, Kyoung-Soon JANG6, Mijung SONG1
1Jeonbuk National University, Korea, South, 2Pusan National University, Korea, South, 3Peking University, China, 4Ewha Womans University, Korea, South, 5National Institute of Environmental Research, Korea, South, 6Korea Basic Science Institute, Korea, South
The phase state and size distribution of particulate matter (PM) are important factors affecting their characteristics. The phase state of PM can affect particle size distribution, however there is limited information about how the phase state of fine PM (PM2.5) in the atmosphere affects its size distribution. In this study, conducted from 2020 to 2022 in Seoul, Seosan, and Beijing, we investigated the impact of the phase state of PM2.5 on its size distribution. PM2.5 filter samples were collected and analyzed using optical observation techniques and the poke and flow method to investigate the phase state of PM2.5. Additionally, during the same periods, the particle number size distributions (PNSD) of PM2.5 and the chemical constituents of the PM2.5 were analyzed. By focusing on the impact of the phase state on the size distribution of PM2.5, this study contributes to our understanding of how phase state and size distribution influence atmospheric pollution. The results will be presented.
AS55-A007
Relationship of Aerosol Optical and Chemical Properties from SPARTAN and AERONET Data in Global Sites
Sujin EOM1+, Jhoon KIM2,3, Seoyoung LEE2, Yeseul CHO2, Sang Seo PARK1#
1Ulsan National Institute of Science and Technology, Korea, South, 2Yonsei University, Korea, South, 3Korean Academy of Science and Technology (KAST), Korea, South
PM2.5 is composed of various chemical substances, and these substances can alter the optical properties of the air. To precisely understand this, we simultaneously analyzed in-situ observations through SPARTAN (Surface Particulate Matter Network) and remote-sensing data through AERONET (Aerosol Robotic Network). SPARTAN sampler provides information on PM mass concentration and chemical composition for each aerosol sample. This study compared SPARTAN and AERONET data from 2016 to 2022 in 11 global observation sites. Focusing on three dominant components—Ammoniated Sulfate, BC, and Fine Soil—found in SPARTAN sampling data, we observed that during periods when Fine Soil mass exceeded BC mass, the wavelength difference of single scattering albedo (SSA) between 870 and 440 nm from AERONET was positive. Conversely, during periods with higher BC mass, this difference was negative. This relationship suggests that the chemical characteristics of aerosols have optically influenced their absorption properties. Therefore, we propose some improvements in existing aerosol type classification algorithms, regarding aerosol chemical states. Furthermore, considering substances with optical absorption and non-absorption characteristics, we calculated the mass ratio of Ammoniated Sulfate to the sum of BC and Fine Soil masses and then analyzed its correlation with SSA at 440 nm. The results, presented for each site, showed relatively strong correlations (R > 0.7).
AS55-A013
Comparing the Surface Tension of Urban Aerosols in Two Megacities Using Field Measurements
Chenxi LIU1#+, Tianyi FAN1, Fang ZHANG2, Yuying WANG3, Jingye REN4, Zhanqing LI5
1Beijing Normal University, China, 2Harbin Institute of Technology, China, 3Nanjing University of Information Science & Technology, China, 4Xi’an Institute for Innovative Earth Environment Research, China, 5University of Maryland, United States
Atmospheric aerosols are enriched with surfactants that reduce the surface tension at the solution/air interface. The reduction of aerosol surface tension leads to enhanced cloud condensation nuclei (CCN) activity, exerting potential impacts on the climate. However, research on surface tension mostly focused on laboratory experiments or modeling work due to limitations in instrumentation and measurement methods. In this study, we alternatively derive the surface tension of aerosols at activation by using hygroscopicity and CCN activity field measurements at two megacities of China based on the κ-Köhler theory. The surface tension calculations for both cities are mostly lower than that of pure water, confirming the reduction of surface tension by the surfactants. Furthermore, the dependence of surface tension to organic mass concentration are calculated in respect to the Szyszkowski-Langmuir equation for various organic species. We find that the dependence in southern city is similar to that of levoglucose which is primarily produced by biomass burning. In contrast, in the northern city the dependence is similar to that of dicarboxylic acids originated from oxidative degradation of anthropogenic (e.g., primary traffic and cooking emissions) and biogenic volatile organic compounds. This work provides the observational constrains of surface tension for urban aerosols, which helps to improve the CCN parameterization in climate models.
AS58-A001
Impacts of Livestock Farming on Emissions and Atmospheric Concentrations of NH3 in Gimje, South Korea: A High-resolution Analysis of Temporal Variations, Spatial Distribution, and Influencing Factors
Jayant NIRMALKAR1+, Joonhyeok CHOI1, Sungjin LEE1, Avinash SHASTRI1, Yeonhoo KIM1, Changhan BAE2, Chul YOO2, Mijung SONG1#
1Jeonbuk National University, Korea, South, 2National Air Emission Inventory and Research Center, Korea, South
Ammonia (NH3), a prominent alkaline gas, contributes a vital role in the production of atmospheric particles by neutralizing acid gases. This process presents challenges to global air quality, human health, and the overall climate. Top of Form The exploration of NH3 emissions and their atmospheric impacts in South Korea's livestock regions is currently insufficient. Therefore, this study seeks to fill research voids by generating high-resolution data on atmospheric NH3, acid gases, PM2.5, and other gas concentrations, along with meteorological variables. The investigation takes place in Gimje, South Korea, spanning from September 22 to October 10, 2023. Real-time NH3 measurements were conducted at both a downwind site (near livestock sites) and an upwind site (farther away) using Los Gatos Research and Cavity Ringdown Spectrometers NH3 analyzers, respectively. Data on PM2.5, various gases (O3, SO2, NO, NO2), and meteorological variables such as wind direction, wind speed, temperature, and relative humidity were measured. An online atmospheric Aerosols and Gases Monitor was utilized to measure acid gases, including HNO3, HONO, and HCl. A strategic 24-hour passive NH3 sampling was implemented at diverse sites, including pig farms, manure treatment plants, cow farms, farmlands, and upwind locations. NH3 concentrations at upwind and downwind sites were statistically similar, indicating widespread livestock emissions in Gimje. Notably, passive sampling at pig farms and manure treatment plants revealed higher NH3 levels due to emissions and volatilization. Diurnal patterns showed increased NH3 during morning livestock activities and nighttime accumulation influenced by lower mixing height, temperature, high humidity, and low wind speed. Afternoons witnessed decreased NH3 concentrations attributed to higher wind speed and temperature, along with reduced humidity. This study emphasizes understanding daily and local NH3 variations for effective pollution control, offering insights crucial for environmental protection and public health in Gimje and beyond.
AS58-A002
Pollution Characteristics of Nitrous Acid and Formaldehyde During the Four Seasons in Shenzhen
Zhen JIANG1+, Lingyan HE2#
1Peking University Shenzhen Graduate School, China, 2Peking University, China
The photolysis of nitrous acid (HONO) and formaldehyde (HCHO) is a critical source of hydroxyl (OH) radicals in the atmosphere, strongly affecting ozone generation. In order to explore the pollution characteristics of nitrous acid (HONO) and formaldehyde (HCHO), long-term observations of HONO and HCHO were conducted in Shenzhen, China from January 2022 to September 2023. The results showed that the average concentration of HONO in Shenzhen during the observation period was highest in winter (0.71 ppbv), followed by autumn (0.64 ppbv), spring (0.59 ppbv) and summer (0.49 ppbv) and the average concentration of HCHO was highest in summer (3.79 ppbv), followed by autumn (2.74 ppbv), winter (2.44 ppbv) and spring (2.13 ppbv). The diurnal variation of HONO showed a similar trend throughout the four seasons, with daytime valleys and nighttime peaks. It was also affected by traffic emissions during the morning and evening peak periods. HCHO showed a more obvious diurnal unimodal characteristics and prominent photochemical generation characteristics. OH radical budget analysis showed that HONO photolysis was the main contributor(60%) to OH radical production in Shenzhen, and it had a significant promoting effect on the early morning photochemical reaction, especially in winter, while HCHO played a more important role in summer and noon. Therefore, by effectively controlling HONO and HCHO, atmospheric oxidation capacity can be reduced, which helps to control O3 pollution.
AS58-A003
Responses of Inorganic Nitrogen to Anthropogenic Emissions and Meteorological Factors in China
Zihan ZHANG#+
Nanjing University, China
Atmospheric nitrogen deposition has attracted more and more attention as a part of acid deposition. Excessive nitrogen deposition not only has a bad influence on ecosystem, but also affect human health. The temporal and spatial distribution of nitrogen deposition flux is influenced by anthropogenic emissions and meteorological conditions. There is a great significance to understand how nitrogen deposition results response to the change of emission conditions and meteorological conditions. We conducted numerical simulations basing on WRF-Chem in China from 2013 to 2019 to study the contribution of anthropogenic emissions and meteorological conditions on nitrogen deposition results. It can be concluded that anthropogenic emission contributes more to nitrogen deposition, while meteorological conditions contribute less, which precipitation is the main meteorological factor affecting nitrogen deposition. Reduced nitrogen deposition has a good consistency with NH3 emission, while oxidized nitrogen deposition has a non-linear relationship with oxidized nitrogen emission. In addition, the contribution of dry and wet deposition to the total nitrogen deposition change is also different in different regions. In the Beijing-Tianjin-Hebei(BTH) region and the Yangtze River Delta(YRD) region, the contribution of dry and wet deposition is similar, while the contribution of wet deposition to the settlement change is larger in the Pearl River Delta region(YRD).
AS58-A008
Interfacial Ozone Oxidation Chemistry at the Water Surface Microlayer as a Source of Light-absorbing and Toxic Compounds in the Ambient Air
Yiqun WANG#, Sasho GLIGOROVSKI+
Chinese Academy of Sciences, China
Water surface microlayer (SML) is ubiquitous in the environment and provides a unique medium for interfacial processing. To investigate the formation of organic compounds including the N-containing organics released in the gas phase, under more realistic conditions, in this study, real-time measurements of volatile organic compounds (VOCs) produced by interfacial oxidation chemistry of gaseous O3 (100 ppb) with an authentic SML by using a novel secondary electrospray ionization ultra-high-resolution quadrupole Orbitrap mass spectrometer (SESI-UHR-MS). We show that ozone oxidation chemistry at the surface microlayers can lead to a large suite of unsaturated and saturated CHO organic compounds in the ambient air of the urban environment. In addition, a large fraction of N-containing organic compounds is produced during this chemistry which can have an impact on human health and the environment. In particular the compounds containing C=N bond are known by their toxicity. We also used Fourier transform ion cyclotron resonance mass spectrometry (FTI-CR MS) for molecular characterization of the organic compounds produced by interfacial oxidation chemistry of gaseous O3 with authentic SML. We show that ozone oxidation chemistry can lead to a large suite of unsaturated and saturated CHO organic compounds including nitrogen (N) containing organic compounds and sulfur(S)-containing organics. The results indicate that the ozone oxidation chemistry at the authentic SML leads to the formation of N-containing compounds ten times more than the N-containing compounds formed by this chemistry on the SML sampled at the upper part of the river at the periphery of the city. We also show that an important number of aromatic compounds with light-absorbing- and toxic- properties are formed which could be discharged into the ocean or atmosphere via gas-water interchange, imposing a great concern on the urban area, in term of human health impact and environmental issues.
AS58-A010
Comparative Analysis in Sensitivity of PM2.5 Mass to Ammonia and Nitrate Availability in Hong Kong and Shanghai Based on Hourly Measurements
Zijing ZHANG1+, Jian Zhen YU1#, Min ZHOU2, Liping QIAO2
1The Hong Kong University of Science and Technology, Hong Kong SAR, 2Shanghai Academy of Environmental Sciences, China
In recent years, fractional contributions of semi-volatile ammonium and nitrate in urban PM2.5 in China have been increasing due to the successful reduction of sulfate. Their contribution to PM2.5 is strongly affected by the gas-particle partitioning ratio, which, in turn, is influenced by physical conditions (i.e., temperature and relative humidity) and chemical composition of PM2.5. Therefore, it is essential to investigate the sensitivity of PM to ammonia and nitrate availability under different atmospheric conditions. We analyzed the concentrations of water-soluble inorganic and gaseous compounds in Hong Kong from 2013 to 2017 and in Shanghai from 2020 to 2022. The ionic PM2.5 compositional data and meteorological parameters were input in ISORROPIA-II to calculate aerosol water content (AWC) and aerosol pH. By examining the datasets by season, we characterized the sensitivity of PM2.5 mass to HNO3 and NH3 availability under different aerosol pH and AWC, following the four-regime plot proposed by Nenes. We further quantified the sensitivity of PM2.5 during winter when PM2.5 levels, as well as the fractional contributions of ammonium and nitrate, were at their highest. Results show that the reduction of water-soluble inorganic compounds was proportional to the reduction of TNO3 (NO3-+HNO3) and sulfate. However, the reduction of TNH3 (NH4++NH3) becomes increasingly efficient as more TNH3 is reduced. During pollution episodes, reducing TNO3 and TNH3 would contribute to lowering PM concentration in Hong Kong. However, in Shanghai, reducing TNH3 by even 30% still would have little effect on PM concentration, so reducing TNO3 would be a more effective approach to improving air quality in Shanghai in the near future. The findings of our study show the importance of controlling TNO3 and TNH3 in Shanghai and Hong Kong and provide valuable insights for other urban aeras to design appropriate policies to improve air quality.
AS58-A018
Measurements and Modelling of Multiphase Nitro-aromatic Compounds at the Summit of Mount Tai in North China
Min LI+, Xinfeng WANG#, Jiazheng LI, Mingxuan LIU, Hongyong LI, Yan WANG, Likun XUE, Wenxing WANG
Shandong University, China
Nitro-aromatic compounds (NACs) in the atmosphere are receiving increasing attention due to their light absorption and biological toxicity. However, there is a scarcity of comprehensive understanding on their distribution characteristics, sources, and formation pathways. In this study, particulate, gaseous, and cloud water samples were simultaneously collected during cloud events at the summit of Mount Tai in northern China in spring, summer, and winter and the contents of 11 major NACs were determined. During cloud events, most NACs were mainly distributed in the particle phase, except dinitrophenols which were mainly distributed in the gas phase in winter. The field-derived effective Henry's law coefficients were several orders of magnitude higher than their theoretical values in pure water. Moreover, the measured concentrations of particulate NACs were substantially greater than the theoretical predictions, especially in spring. The above results indicate that NACs were partly formed via aqueous-phase reactions inside the cloud droplets or on the wet particle surfaces, which changed their distribution patterns. Furthermore, an observationally constrained multiphase chemical box model was developed and employed to elucidate the NACs formation mechanisms in the fine particles. The simulation results indicate the crucial roles of gas-particle partitioning and heterogenous uptake on aerosols. The results highlight the importance of aqueous-phase reactions on the formations of NACs and provides modelling insights on the formation of particulate NACs and the contributions from different sources, addressing the underestimation in traditional models regarding gas-particle partitioning.
AS63-A001
The Maritime Continent’s Rainforests Modulate the Local Interannual Hydroclimate Variability
Min-Hui LO1#+, Ting-Hui LEE1, Chun-Lien CHIANG1, Yan-Ning KUO2
1National Taiwan University, Taiwan, 2Cornell University, United States
The interannual variability of evapotranspiration (ET) in the Maritime Continent (MC) is generally low, despite significant fluctuations in precipitation influenced by the El Niño-Southern Oscillation (ENSO). This study explores the underlying dynamics of this phenomenon, using observations, reanalysis data, and climate model. We decomposed ET into canopy evaporation (CE), canopy transpiration (CT), and soil evaporation (SE) to understand their interactions. Our findings reveal that during El Niño years, reduced precipitation leads to a significant decrease in CE and SE, while CT increases notably due to higher incoming solar radiation. This self-compensating mechanism between CE and CT results in only a slight decrease in ET during El Niño years, thus dampening ET's interannual variation. Conversely, La Niña years show opposite patterns. Furthermore, the MC rainforests have experienced severe deforestation in recent decades. Idealized deforestation simulations in CESM indicate that deforestation leads to a decrease in ET and an increase in precipitation. Notably, deforestation removes the dampening effect of CT, resulting in an amplified interannual variation of ET. This change in ET’s interannual variability due to deforestation also leads to a decreased interannual variation of precipitation. Our detailed investigation reveals that the mean states can modulate deforestation's impacts on precipitation, consequently influencing its interannual variation. Overall, this study underscores the crucial role of forests' CT in regulating the interannual variability of ET and highlights the complex interplay between deforestation, ET, and precipitation in the MC. It emphasizes the significant impacts of deforestation and the critical importance of tropical rainforests in the hydroclimatological cycle.
AS63-A005
An Evaluation of CMIP6 Models in Representing the Biophysical Effects of Deforestation with Satellite-based Observations
Xing LUO#+, Jun GE, Yipeng CAO, Yu LIU, Shiyao WANG, Limei YANG, Weidong GUO
Nanjing University, China
Deforestation can impact surface temperature via biophysical processes. Earth system models (ESMs) are commonly used tools to examine biophysical effects of deforestation, but the model capacity to represent deforestation effects remains unclear. In this study, we comprehensively evaluate the performance of four ESMs of the Coupled Model Intercomparison Project Phase 6 (CMIP6) in representing deforestation effects with a satellite-based benchmark. The results show that the ESMs can basically capture the sign of the temperature response but over- or underestimate the magnitude. Such biases are the consequence of biases in the simulated responses of albedo and sensible and latent heat fluxes. Specifically, the ESMs consistently overestimate the albedo response under snow-covered conditions, for example, in the northern latitudes and in the cold season. The ESMs fail to fully reproduce the observed responses of sensible and latent heat fluxes, and the model bias depends on the model, region and season. The ESMs and observations even disagree on the sign of responses of sensible and latent heat fluxes in some cases. An attribution analysis further shows that biases in the simulated surface temperature response mainly result from biases related to the response of the surface energy partitioning. Biases related to the albedo response only play an important role under snow-covered conditions. Given these model biases, we highlight that when the CMIP6 models are used to investigate deforestation effects, the simulated result should be interpreted with caution. Moreover, the identified model deficiency shown here also has implications for model improvement.
AS63-A009
The Climate Response to Global Forest Area Changes Under Different Warming Scenarios in China
Ying HUANG#+, Anning HUANG, Jie TAN
Nanjing University, China
Human activities have notably affected the Earth’s climate through greenhouse gases (GHG), aerosol, and land use/land cover change (LULCC). To investigate the impact of forest changes on regional climate under different shared socioeconomic pathways (SSPs), changes in surface air temperature and precipitation over China under low and medium/high radiative forcing scenarios from 2021 to 2099 are analyzed using multimodel climate simulations from the Coupled Model Intercomparison Project Phase 6 (CMIP6). Results show that the climate responses to forest changes are more significant under the low radiative forcing scenario. Deforestation would increase the mean, interannual variability, and the trend of surface air temperature under the low radiative forcing scenario, but it would decrease those indices under the medium/high radiative forcing scenario. The changes in temperature show significant spatial heterogeneity. For precipitation, under the low radiative forcing scenario, deforestation would lead to a significant increase in northern China and a significant decrease in southern China, and the effects are persistent in the near term (2021–40), middle term (2041–70), and long term (2071–99). In contrast, under the medium/high radiative forcing scenario, precipitation increases in the near term and long term over most parts of China, but it decreases in the middle term, especially in southern, northern, and northeast China. The magnitude of precipitation response to deforestation remains comparatively small.
AS63-A012
Sensitivity of Land Use/land Cover, and Soil Texture in a Land Surface Model
Sujeong LIM1#+, Seon Ki PARK1, Claudio CASSARDO2, Ji Won YOON1
1Ewha Womans University, Korea, South, 2University of Turin, Italy
Land surface processes and their coupling to the atmosphere are crucial in simulating the regional and global climate. Consequently, it is critical to identify and quantify uncertainty in these land surface model (LSM) processes in order to comprehend the land-atmosphere interactions. The heterogeneous characteristics, such as land use/land cover and soil texture, of the land surface contribute to the uncertainty associated with vegetation and soil parameters in LSM. They can alter the exchange of water and energy fluxes between land and atmosphere and thus impact the meteorological conditions at local and regional scales. In this study, we use the University of Torino land surface Process model for Interaction in the Atmosphere (UTOPIA), a one-dimensional land surface model that represents the interactions at the interface of the atmosphere, vegetation, and soil layers, to examine the sensitivity of land cover and soil texture in LSMs. We will investigate the impact of energy flux partition, soil moisture redistribution, and runoff generation due to land use/land cover and soil texture changes.
AS63-A013
The Impact of Soil Texture on Hydrological Processes in South Korea Based on WRF-Hydro Simulations
Subin KANG1+, Pamela Sofia FABIAN1, Hyun-Han KWON1, Eun-Soon IM2#
1Sejong University, Korea, South, 2The Hong Kong University of Science and Technology, Hong Kong SAR
The accurate estimation of soil texture is crucial as it significantly impacts soil moisture and other hydrological variables. While the Weather Research and Forecasting Hydrological Extension (WRF-Hydro) model is a useful tool for investigating various aspects of hydrological processes and their interactions with the atmosphere, the default soil map provided by USGS and MODIS exhibits potential issues associated with coarse resolution and limited accuracy. To address these limitations, this study conducts a series of sensitivity experiments that consider additional data sources or alternative soil mapping approaches within WRF-Hydro model framework. A comparative analysis is performed by focusing on hydrological variables such as soil moisture and runoff. The study will enhance our understanding of how changes in soil properties influence key hydrological processes and shed light on the impact of diverse soil conditions on the robustness of simulation results. Acknowledgment This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Water Management Program for Drought, funded by Korea Ministry of Environment(MOE)(2022003610003).
AS63-A016
Impacts of Perturbed Land-atmosphere Interactions on Local Hydroclimate
Zhiyuan YANG1#+, Dongryeol RYU1, Min-Hui LO2, Murray PEEL1, Sugata NARSEY3, Kaighin MCCOLL4
1The University of Melbourne, Australia, 2National Taiwan University, Taiwan, 3Bureau of Meteorology, Australia, 4Harvard University, United States
Land-atmosphere coupling serves as an important process that is associated with the variability of hydroclimate from local to regional scales given perturbed land surface conditions. This research was inspired by a potential geo-engineering project, commonly referred to as the Bradfield Scheme, proposed decades ago aiming at introducing a large water expanse into central Australia for the hydroclimatic changes that are favorable toward increased agricultural productivity. Based on idealized simulations by the community earth system model (CESM), we investigate how an inland lake perturbs the land-atmosphere interactions in central Australia and how the local hydroclimate responds to those perturbations. Moreover, the CESM employed in our research enables water isotopes and activates water tracers. We find that the idealized lake would strengthen the precipitation recycling process but fail to cause significant changes in total precipitation (e.g., the precipitation of water vapor originating from the lake region is shown to trivially contribute to total precipitation). The negligible impact on precipitation might be explained by the perturbed land-atmosphere interactions via the changes in the local thermodynamics and dynamics: the lake increases the latent heat flux through changing the surface energy budget, which corresponds to a significantly enhanced moisture flux into the overlying atmosphere; however, it also leads to significant evaporative cooling, creating strong divergence in the lower atmosphere and suppressing precipitation formation. Our research indicates that it is necessary to consider the interactions between land and atmosphere to better understand the underlying mechanisms of (either natural or anthropogenic) land use/land cover changes.
AS63-A017
Analysis of Weather Elements in Downstream City Namyangju Due to Changes in Land Use in Seoul
Soyoung JUNG#+, Seungyeon LEE, Ji Won YOON, Seon Ki PARK
Ewha Womans University, Korea, South
The intensifying concentration of the population in the metropolitan area of South Korea in recent times has led to the urban heat island (UHI) effect, promoting temperature increases in city centers and deteriorating the quality of life. In this study, we examined the impact of changing land use from urban areas to cropland in Seoul for 24 hours from 6 AM on July 26th, 2022, on the weather elements in downstream Namyangju using the WRF model. The results showed a shift in the convergence of winds from the northern part of Seoul towards Namyangju, particularly displaying strong convergence during the night. The temperature decrease in Namyangju was over 1.4℃ higher at night compared to daytime. During the day, temperatures dropped significantly in all directions from Seoul, except for the western part. However, at night, temperatures fell in a limited area to the east. Both Seoul and Namyangju experienced an increase in humidity, attributed to the evaporation of moisture from the cropland in Seoul. This humid atmospheric layer was generated around 1:30 PM and disappeared around 2 AM the following day. This study analyzed temperature changes, wind convergence, and humidity increase in downstream cities when alleviating Seoul's UHI effect. It can serve as crucial research material for predicting downstream city temperatures considering UHI and for planning satellite city constructions to mitigate the concentration of Seoul.
AS63-A019
Convergent Mechanisms and Responses: A Comparative Analysis of Extreme Precipitation in Maritime Continent Under Land Use Changes and Global Warming
Jie HSU1, Chao-An CHEN2, Chia-Wei LAN1, Min-Hui LO1#+, Chun-Lien CHIANG1, Chun-Hung LI1
1National Taiwan University, Taiwan, 2National Science and Technology Center for Disaster Reduction, Taiwan
The Maritime Continent (MC) has experienced severe deforestation in recent decades, leading to atmospheric destabilization. Here, we focus on the changes in extreme precipitation under the land use changes (LUC) and the global warming (GW) in MC. Our results suggested a “wet-get-wetter, dry-get-drier” paradigm for precipitation responses to MC LUC and GW, leading to an increased frequency of both extreme heavy and light precipitation events. However, the mechanisms show different mechanisms between LUC and GW in MC. LUC results in a warmer land surface, inducing an unstable atmospheric environment that affects local convection, manifesting as a negative effect of forest coverage on precipitation changes. As the GW, leading to the capacity of water vapor increases with rising temperatures in the atmosphere, resulting in the enhancement of precipitation. Our research found that LUC and GW cause more potent local effects, resulting in increased (decreased) precipitation in areas that already receive more (less) precipitation. Our study further explores how these two scenarios affect the intensity of extremely heavy and light precipitation in the MC. Atmospheric moisture budget analysis reveals that extreme precipitation events are associated with the dynamic component of vertical moisture advection after LUC or GW.
AS66-A004
The Physical Processes Responsible for the Seasonal Cycle and Climate Feedback of Extratropical Marine Low Cloud
Shuangchen DU#+, Hui SU
The Hong Kong University of Science and Technology, Hong Kong SAR
Marine low clouds are effective at cooling the Earth's surface by reflecting solar radiation. Existing research suggests that the uncertainty surrounding the cloud feedback in subtropical and extratropical regions is crucial to understanding the model spread in Equilibrium Climate Sensitivity (ECS). A recent study by Furtado et al. (2023) discovered that the seasonal patterns of clouds in the mid-latitude oceans of the Northern Hemisphere can provide insights into how clouds may respond to long-term surface warming. Jiang et al. (2023) introduced an additional constraint on ECS based on the seasonal fluctuations of extratropical marine low cloud fraction. Both Jiang et al. (2023) and Furtado et al. (2023) showed a correlation between the seasonal and long-term changes in the extratropical marine low cloud fraction per degree of surface warming. However, the underlying physical mechanisms behind the cloud fraction changes on these two time scales are yet to be fully established. In this study, we examine the contributions of the boundary layer inversion strength versus the extratropical cyclones to the extratropical marine low cloud fraction change on the seasonal and centennial time scales. By investigating these factors, this study aims to enhance our understanding of how the climate system responds to increasing greenhouse gases and improve the accuracy of climate change predictions.
AS66-A006
Tropical High Cloud Cover Trend and High Cloud Feedback in CMIP6 Models
Yanjia WANG#+, Chengxing ZHAI, Hui SU
The Hong Kong University of Science and Technology, Hong Kong SAR
High cloud cover is a crucial factor that regulates the energy balance and plays a significant role in temperature, precipitation, and the overall climate of the tropical region. However, the simulation of high cloud cover in tropical regions is subject to significant uncertainties, which can affect the accuracy of climate models and the prediction of future climate change. The study focuses on the simulation of high cloud cover and high cloud feedback in tropical regions using the Coupled Model Intercomparison Project Phase 6 (CMIP6) models. It is found that from 1984 to 2014, cirrus cloud cover decreases while cirrostratus and deep convection cloud cover increase, with no significant trend in total high cloud cover according to the International Satellite Cloud Climatology Project (ISCCP) data. The study also reveals that the CMIP6 models shows significant discrepancies in the simulating the spatial distribution and temporal variation of high cloud cover. The trend of high cloud cover in tropical regions mainly varies from east to west, with an increase in high cloud cover in the western Pacific and a decrease in the eastern Pacific, and vice versa. The time variation of simulated high clouds is considerably correlated with the sea surface temperature changes from 1980 to 2014. Future research will explore the interactions among large scale circulation, convection, radiation, and high/low cloud feedbacks and SST warming patterns in the models, which can improve our understanding of the complex high cloud feedback in tropical regions and enhance the accuracy of climate models.
AS66-A016
Seasonal Surface Spectral Emissivity Derived from MODIS/VIIRS Data
Yan CHEN1#+, William L. SMITH JR.2, Sunny SUN-MACK1,2, Benjamin SCARINO2, Patrick MINNIS2, Qing TREPTE3, Gang HONG1,2
1Analytical Mechanics Associates, Inc, United States, 2NASA Langley Research Center, United States, 3Science Systems and Applications, Inc., United States
Surface emissivity is essential for many remote-sensing applications including the retrieval of surface skin temperature from satellite-based infrared measurements, the determination of cloud detection thresholds, and the estimation of the surface longwave radiation emission, an important component of the energy budget of the surface-atmosphere interface. The CERES (Clouds and the Earth’s Radiant Energy System) Project is measuring broadband shortwave and longwave radiances and deriving cloud properties from the MODIS on Terra and Aqua and from the VIIRS on NOAA-19 and NOAA-20 orbiters to produce combined global radiation and cloud property data sets. Zhou et al. (IEEE Trans. Geosci. Remote Sens., 49, 2011) used Infrared Atmospheric Sounding Interferometer (IASI) data to create a high spectral resolution surface emissivity atlas for remote sensing and modeling applications. The IASI measures spectral radiances between 3.62 and 15.5 mm. The VIIRS I4 channel width is from 3.55 to 3.93 mm, while MODIS Band 20 is from 3.66 to 3.84 mm. Comparisons of top-of-atmosphere (TOA) radiance calculations with MODIS and VIIRS observations for these bands suggest that the IASI emissivity atlas near 3.7 µm may not be suitable for CERES cloud retrievals. In this paper, the IASI emissivities for the VIIRS and MODIS bands centered near 11mm are used to derive surface skin temperature from nighttime MODIS/VIIRS data. The Goddard Earth Observing System for Instrument Teams (GEOS-IT) numerical weather analyses provide temperature and water vapor profiles fused to correct the observed radiances for atmospheric absorption and emission. Global seasonal emissivity maps are then derived for the VIIRS and MODIS 3.7mm bands that are consistent with the derived skin temperatures and the observed TOA radiances. These seasonal climatology maps will be validated and used in CERES Edition 5 and other CERES-related cloud retrieval algorithms to provide improved clear-sky radiances and derived cloud properties.
AS66-A027
The Influences of Soot and Dust on the Physics Properties and Bidirectional Reflectance of Snowpack
Kun WU1#+, Feng ZHANG2, Jiangnan LI3
1Nanjing University of Information Science & Technology, China, 2Fudan University, China, 3Canadian Centre for Climate Modelling and Analysis, Canada
The optical properties and bidirectional reflectance of the snowpack mixed with different concentrations of soot and dust are discussed in this study. Two mixing rules, Bruggeman and Maxwell-Garnett mixing rules, were considered and compared. It indicates that the extinction coefficient is less changed with the changing of soot and dust concentrations. The single-scattering albedo (asymmetry factor) decreases (increases) with increased concentrations of soot and dust. The optical properties of the snowpack are more sensitive to the change of soot concentration when the soot concentration is over 0.1 ppmw. From the change of optical properties, there is slightly stronger absorption using the Bruggeman mixing rule than using the Maxwell-Garnett mixing rule, while the relative differences between them are small. For semi-infinite snowpack, a reduction of the bidirectional reflection distribution function (BRDF) occurs with increasing concentrations of soot and dust, and the snowpack with heavy dust pollution can cause a larger BRDF reduction than that with heavy soot pollution. This phenomenon is more significant for large snow grain radii. For infinite snowpack, three cases were set to refer to observation. The reduction of BRDF is sharp in the case with a large concentration of dust at the snowpack surface.
AS66-A029
Long-term Trends of Aerosol and Cloud Fraction Over Eastern China Based on Ground-based Observations
Tong YANG+, Xiaoyan MA#, Jianqi ZHAO
Nanjing University of Information Science & Technology, China
We looked into the long-term variability of aerosols and clouds over Eastern China (EC) using MICAPS ground-based data from 1995 to 2019 and MODIS aerosol optical depth (AOD) retrieval from 2003 to 2019. The ground-based observed visibility (VIS) was used to characterize aerosol concentrations. Our study indicate that VIS shows a significant shift over EC in recent decades, as evidenced by falling (P1: 1995–2006)-flat (P2: 2007–2013)-rising (P3: 2014–2019) periods. Correspondingly, a change was observed in cloud fraction (CF) from a strong increase(P1:0.84%/year) to a slow fluctuation(P3:-0.02%/year) during the three periods over the Beijing-Tianjin-Hebei (BTH), but no significant variation over the Yangtze River Delta (YRD) region. In addition, the CF-VIS shows a negative correlation during both P1(BTH:-0.69%/km; YRD:-0.52%/km) and P3(BTH:-0.45%/km; YRD:-0.29%/km) periods while this relationship weakened during P3 (35% weaker in BTH and 44% weaker in YRD). However, it is important to note that this weakening may be influenced by a few factors, such as data processing methods, the location of aerosols relative to the cloud, relative humidity (RH), and large-scale circulation etc. Further studies, including numerical simulations and analysis, are required to determine how much change of cloudiness is attributed to aerosols.
AS73-A006
Influence of Horizontal Convective Rolls and Complex Terrain on the Structure of Multiple Parallel Rainbands
Peiyu WANG1#+, Zhiyong MENG2
1Peking University, China, 2Department of Atmospheric and Oceanic Sciences, School of Physics, and China Meteorological Administration Tornado Key Laboratory, Peking University, China
Multiple parallel rainband (MPRB) is a type of organization of mesoscale convective systems. MPRBs are often accompanied by two different scales of train effects and thus often result in heavy precipitation. Our previous work showed that MPRBs in China have the highest frequency in the Beibu Gulf and its coastal areas and with more than half of them occurring in the mountainous areas along the western coast of the Beibu Gulf. This study tries to understand the formation mechanism of MPRBs in this highest frequency area of coastal Beibu Gulf based on a case study. Result shows that horizontal convective rolls (HCRs) played an important role in the formation of the MPRBs. The HCRs were generated by large vertical wind shear and inflection point instability over coastal area with a low-height mountain orientated almost perpendicular to the orientation of HCRs. Coastal mountains block water vapor from the southern sea and favors the formation of the HCRs and convection initiation. The interaction between the HCRs with the mountainous terrain led to the continuous initiation of convection in the upstream part of HCRs, and formed MPRBs through back-building process. Sensitivity experiments revealed that the height of the coastal terrain apparently affected the structure of MPRBs, but had little effect on the structure of the HCRs. As the height of the mountain range decreases, the MPRB structure keeps weakening or even disappears.
AS73-A013
Formation of Boundary Layer Convergence Lines in the Hetao Area and Its Convection Triggering Effect
Xuefeng MENG#+
Inner Mongolia Meteorological Observatory, China
The results indicated that the BLCL in the Hetao area was formed by the combined influence of surface differences, boundary layer atmospheric circulation and complex terrain. And the BLCL mainly occurred at the border between the Hetao irrigation area and the Kubuqi Desert, and in a smaller arid area along the southeast bank of the Yellow River, with BLCL lengths ranging from 100 to 200 km. BLCL was a shallow system with convection heights of approximately 1000 to 1300 m. The daily variation of BLCL was significant, with a high incidence period from 12:00 to 17:00, accounting for 80%. The probability of BLCL formation in July and August of midsummer was as high as 60%, and 39% of BLCL could trigger convection. The prediction indicators about the formation of BLCL were as follows: (1) The temperature in Hangjinhouqi (53420) in Hetao Irrigation District is 2.5 ℃ lower than that in Habailaigeng (C3183) in Kubuqi Desert,and the relative humidity difference between them is up to 20% .(2) Continuous strong southerly winds was in the Kubuqi Desert and Mu Us Sandy Land areas in Hetao area, with a maximum wind speed of 10 meters above the ground greater than 4 ms − 1.(3) The sea level pressure field is high in the east and low in the west, and a dense isobaric zone was in the Jiziwan of Yellow River with 3-4 isobars. The formation of BLCL is of great significance to the convection triggering in this region, which is manifested in convection triggering, convection strengthening, and convection organization. The generation and convective triggering of BLCL in this specific region are closely related to the distribution characteristics of rapid increase in precipitation from west to east in the Hetao region.
AS73-A014
Distribution Characteristics of Convection Initiation Over a Real-world Sharp Vegetation-contrast Area in North China
Hongjun LIU1#+, Zhiyong MENG2, Lanqiang BAI3, Quxin CUI4
1Institute of Urban Meteorology, China, 2Department of Atmospheric and Oceanic Sciences, School of Physics, and China Meteorological Administration Tornado Key Laboratory, Peking University, China, 3Guangdong Meteorological Service, China, 4Peking University, China
Based on the radar data, this study explored the statistical characteristics of the convection initiations (CIs) during summers from 2012 to 2016 over the Hetao area in North China, where there is a sharp vegetation contrast between irrigation and desert. The durations of the most convections that triggered in the Hetao area are short and the development are weak. The high-incidence areas of CIs are deserts, mountains, and the edge of the Ordos Plateau. The convections over the desert are triggered around noon and last longer time, while the convections over mountains or at the edge of plateaus are mostly initiated at night and last for a shorter time. Some CIs are associated with boundary layer convergence lines (boundaries) caused by non-uniform underlying surfaces. Under different synoptic patterns, the initiation time of boundary-related convections are later than that of nonboundary-related convections, and the durations all longer. When the Hetao area is controlled by a weak high-pressure ridge at 500 hPa and there are southerly winds at low level, the long-duration boundary-related CIs are most likely to be triggered over the Kubuqi Desert.
AS74-A005
Conspicuous Greening Trends Over East Asia in Recent Decades
Min-Seok KIM1+, Jee-Hoon JEONG1#, Hans LINDERHOLM2, Sung-Ho WOO1
1Chonnam National University, Korea, South, 2University of Gothenburg, Sweden
Global warming is rapidly altering the dynamics of terrestrial vegetation, with consequences for regional climate dynamics, biodiversity, agricultural systems, and socio-economic challenges associated with land-use changes. Under the global warming, corresponding global greening trends have been observed in recent decades. Particularly, since the 2000s, vegetation growth has significantly increased in East Asia compared to other regions. To determine whether the recent strong greening trend in East Asia is a result of anthropogenic climate change, or a part of a natural oscillation on longer time scales than the observation period, a combination of satellite observations, tree-ring proxies, and earth system model simulations was used. Tree-ring based reconstruction reveals that the recent significant increase in vegetation in East Asia is a highly unprecedented phenomenon, with levels not observed in the past 200 years. In a warming climate, the enhanced Kuroshio Current and Western North Pacific Subtropical High in winter preceded by the growing season appear to amplify the greening trends in East Asia by inducing favorable warm and wet conditions for vegetation growth. Multiple model simulations from the Coupled Model Intercomparison Project Phase 6 (CMIP6) also depict the recent strong greening trend in East Asia as a manifestation of anthropogenic climate change and project further intensification in the 21st century.
AS74-A007
One-month Forecast for Rice Harvest Date in South Korea
Jina HUR1+, Yongseok KIM1#, Sera JO1, Kyo-Moon SHIM1, Eung-Sup KIM1, Mingu KANG1, Eun-Soon IM2, Subin HA2
1National Institute of Agricultural Sciences, Korea, South, 2The Hong Kong University of Science and Technology, Hong Kong SAR
This study aimed to predict on the rice harvest date in South Korea using one-month temperature forecasts. A global prediction data from the NOAA Climate Forecast System was downscaling using the Weather Research and Forecasting (WRF) model to obtain detailed predictive information. The WRF model utilized a double-nested modeling system, generating 5km gridded information centered on South Korea. Temperature predictive data over 11 years (2012-2022) were employed as input for a phenological model to predict the rice harvest date in advance. The seeding date was assumed to be January 1, and the reference temperature for harvesting was set at 1400°C + 55 days. The maximum and minimum temperature hindcasts tends to underestimate compared to observation. Due to the cold bias of temperature forecast data, the rice harvest date derived from hindcasts tend to be delayed compared to observation. This study highlights the potential of the one-month prediction system in obtaining high-resolution agricultural information. Funding Source: This work was supported by a grant (no. RS-2020-RD009438) from the Rural Development Administration, Republic of Korea. Reference: Hur, J, E-S Im, S Ha, Y-S Kim, E-S Kim, J Lee, S Jo, K-M Shim, M-G Kang, 2023: 1-month Prediction on Rice Harvest Date in South Korea Based on Dynamically Downscaled Temperature, Korean Journal of Agricultural and Forest Meteorology, 25(4), 267~275.
AS74-A009
A Study on Error Correction Techniques in One-month Temperature Forecast Data
Yongseok KIM+, Jina HUR#, Sera JO, Kyo-Moon SHIM, Eung-Sup KIM, Mingu KANG, Seung-Gil HONG
National Institute of Agricultural Sciences, Korea, South
In this study, we analyzed the characteristics of the error in one-month temperature prediction data generated through joint development between the Rural Development Administration and the Hong Kong University of Science and Technology and performed corrections. For this purpose, we colleted hindcast data and weather observation data from 2013 to 2021, and environmental information on latitude, altitude, slope direction, slope, and Land cover index, and analyzed the characteristics of errors. In the case of maximum and minimum temperatures, the higher the elevation, the larger the forecast error. Various machine learning methods were used to correct errors in temperature prediction data, and on average, the RMSE of predicted data corrected with machin learning decreased by 0.475 (maximum temperature) and 0.400 (minimum temperature), respectively, compared to uncorrected predicted data. Through this study, it was found that errors in prediction data are affected by topographical conditions, and that machine learning methods can effectively improve errors by considering various environmental factors. This work was supported by a grant (no. RS-2020-RD009438) from the Rural Development Administration, Republic of Korea. Reference
AS74-A010
Climatic Yield Potential Changes Over Korean Peninsula Using 1-KM High Resolution SSP Scenarios
Sera JO#+, Yongseok KIM, Jina HUR, Kyo-Moon SHIM, Seung-Gil HONG, Mingu KANG, Eung-Sup KIM
National Institute of Agricultural Sciences, Korea, South
The changes in rice climatic yield potential (CYP) across the Korean Peninsula are evaluated based on the new climate change scenario produced by the National Institute of Agricultural Sciences with 18 ensemble members at 1 km resolution under a Shared Socioeconomic Pathway (SSP) and Representative Concentration Pathways (RCP) emission scenarios. To overcome the data availability, we utilize solar radiation for CYP instead of sunshine duration which is relatively uncommon in the climate prediction field. The result show that maximum CYP(CYPmax) decreased, and the optimal heading date is progressively delayed under warmer temperature conditions compared to the current climate. This trend is particularly pronounced in the SSP5-85 scenario, indicating faster warming, except for the northeastern mountainous regions of North Korea. This shows the benefits of lower emission scenarios and pursuing more efforts to limit greenhouse gas emissions. On the other hand, the CYPmax shows a wide range of feasible futures, which shows inherent uncertainties in future climate projections and the risks when analyzing a single model or a small number of model results, highlighting the importance of the ensemble approach. This work was supported by a grant (no. RS-2021-RD009055) from the Rural Development Administration, Republic of Korea.
AS74-A013
Prediction Skill of the Siberian Heatwave and Korean Peninsula Cold Spell in April 2020 Based on Snow Initialization
Joonlee LEE+, Myong-In LEE#, Jihae KIM
Ulsan National Institute of Science and Technology, Korea, South
In April 2020, the 2m temperature over Siberia reached a historically unprecedented heatwave, while the Korean Peninsula experienced a cold spell. This study examines whether the operational model (GloSea6) for KMA accurately predicted the Siberian heatwave and Korean Peninsula cold spell in April 2020. Simultaneously, the impact of snow initialization on the sub-seasonal prediction skill of the model was investigated by prescribing different snow conditions for the Eurasian region. The snow experiments included three conditions: climate-prescribed snow state, snow state produced by the operational model's land surface component (JULES), and assimilated snow state using satellite data. In 2020, similar to the substantial decrease observed in snow amounts, the results generated by the land surface model and assimilation portrayed a dry condition compared to climatic values. In particular, the assimilated snow state exhibited the closest resemblance to the observations. Based on these findings, this study confirms that changes in snow state significantly influence the upper-level wave patterns and temperature variations in the Siberian region. The reduction of snow in the Eurasian region due to future climate change is expected to enhance land-atmosphere interaction in spring, playing a crucial role in the maintenance and strengthening of upper-level stationary waves in the Siberian region.※ This work was funded by the Korea Meteorological Administration Operational System Operation and Development for Climate Prediction Program under Grant KMA2018-00322.
AS74-A015
Evaluating the Predictability of Summer High-temperature Days in South Korea Using 5KM-resolution Long-term Prediction Data
Eung-Sup KIM1#+, Sera JO1, Jina HUR1, Kyo-Moon SHIM1, Yongseok KIM1, Mingu KANG1, Seung-Gil HONG1, Joong-Bae AHN2
1National Institute of Agricultural Sciences, Korea, South, 2Pusan National University, Korea, South
The frequency and intensity of abnormal meteorological and climatic phenomena are increasing due to climate change. According to the abnormal climate report from the Korea Meteorological Administration, the number of high-temperature days in South Korea is showing an increasing trend along with the rise in global mean temperature. This trend especially showing a rapid increase since the 2010s. The increase in temperature and the number of high-temperature days can affect the growth and yield of crops, and can also affect the health of farmers engaged in agriculture. The National Institute of Agricultural Sciences of the Rural Development Administration has established the Pusan National University/Rural Development Administration (PNU/RDA) CGCM-WRF Chain by migrating the PNU CGCM-WRF Chain. The RDA produces 5km-resolution long-term prediction data using PNU/RDA-WRF Chain system to produce and provide weather and climate prediction for use in use agricultural part. Therefore, in this study, we evaluated the predictability of the number of summer high-temperature days in the South Korea over the past 30 years using 5km-resolution long-term prediction data. The correlation between predicted and observed of number of high-temperature days showed a statistically significant at the 99% confidence level, and an accuracy close to 80%.
AS74-A016
A Land-atmosphere Modeling Package (LAMP) Dedicated to Agricultural and Forest Management in South Korea: History So Far and Plans for the Near Future
Seung-Jae LEE1#+, Suhyun KIM1, Seung-Min LEE1, Kyeongsu KIM1, Joo-Yeol BAEK1, Minki HONG2
1National Center for AgroMeteorology, Korea, South, 2Princeton University, United States
In 2014, a Land-Atmosphere Modeling Package for supporting agricultural and forest management was developed at NCAM in South Korea. This modeling package is comprised of two components; one is the Weather Research and Forecasting modeling system (WRF) coupled with Noah-MultiParameterization options (Noah-MP) Land Surface Model (LSM), and the other is offline one-dimensional LSMs including JULES. Recently, the LAMP has been reinforced by adding FDDA, WRF-LES, and chemistry modules. The LAMP was initially started for weather and climate research in the agricultural and forestry sector within the university with government support, but has since expanded its support to local governments, private companies, and air force weather units. It can provide a dynamically and physically scientific tool to be easily applied for high-resolution NWP and making it easy to perform biophysical application and mechanism explanation on small-scale complex terrains. The results are visualized in one, two, and three dimensions using NCL and VAPOR and verified on a regular basis. It has artificial intelligence-based postprocessing methods to increase medium-range predictability. Some example applications using the LAMP are as follows: 1) to understand local wind circulations around observation sites; 2) to characterize agricultural drought in small-scale farmlands based on soil moisture (SM) deficit; 3) to predict snow depth and wetness to reduce the damage to agricultural facilities; 4) to analyze the effects of air temperature reduction by green and cool roofs in Seoul; 5) understand spatiotemporal variations in the atmospheric ventilation index; 6) to simulate rainfall and SM for landslide risk assessment; 7) to compute livestock heat stress in a mechanically ventilated broiler house; and 8) to analyze structure of low level jets near the origin of migratory insect pests. We plan to introduce U. S. National Water Model schemes for the process-level enhancement of terrestrial energy, water, carbon circulation analysis and prediction.
AS83-A004
The Interactions Among Southwesterly Monsoon Flow, Typhoon, Mei-yu Front, Terrain and Heavy Rainfall
Chuan-Chi TU#+, Pay-Liam LIN, Siang-Yu ZHAN, Pei-Chun TSAI, You-Ting LIN
National Central University, Taiwan
We study the IOP2 during Northern Coast Observation, Verification of Dynamics Experiment 2021 (NoCOVID21), and we focused on the details about the interaction between the typhoon (Choi-wan) and the mei-yu front, and the relationship between heavy rainfall over Taiwan and the southwesterly flow. On 3 Jun 2021, the period we defined as the pre-merging period 1, the Choi-wan typhoon and the mei-yu front were farther away with a relative dry region between them, and the two systems kept their characteristics. The atmosphere was warm and moist around the typhoon center, but it was baroclinic across the mei-yu frontal system with large temperature gradient. On 4 Jun, the pre-merging period 2, as the two systems were getting close gradually, the relative dry region was replaced by the moist airmass. The tropical cyclone weakened when its circulation was modified by Taiwan terrain, and the temperature gradient in the frontal region also weakened. On 5 Jun, the merging stage, the tropic cyclone moved to northeast of Taiwan, merging with the mei-yu front and transforming into a strong extratropical cyclone. The extratropical cyclone is characterized by stronger vorticity, circulation, ascent, total precipitable water and rainfall. After 2000 UTC 5 Jun, the extratropical cyclone weakened rapidly. During 5 Jun to 6 Jun, the prefrontal synoptic-related low-level jet (SLLJ) and the marine boundary layer jet (MBLJ) coexisted over southwest of Taiwan, and the MBLJ played an important role on moist transport. The warm and moist LLJs were blocked and lifted by Taiwan terrain, and the upper level divergence was present during 5 Jun to 6 Jun. As a result, the heavy rainfall event occurred over southwestern Taiwan.
AS83-A005
1-9-day Single Deterministic and Probabilistic Forecasts for Extreme Precipitation Events Over Taiwan Using Statistical Post-processing
Joyce JUANG1#+, Hui-Ling CHANG1,2, Chih-Yung Feng FENG3, Han-Fang LIN4, Jing-Shan HONG5, Chuhsing Kate HSIAO6
1Central Weather Administration, Taiwan, 2National Central University, Taiwan, 3Manysplendid Infotech, Ltd., Taiwan, 4Manysplended Infotech Ltd, Taiwan, 5Central Weather Bureau, Taiwan, 6National Taiwan University, Taiwan
Climate change has led to more frequent extreme weather events, posing challenges worldwide and in Taiwan, where advanced weather forecasting is crucial for disaster management and resource planning. For example, during drought, it is vital for authorities to assess the potential for mid-term drought relief within a 10-day period. This necessitates accurate and reliable mid-term precipitation forecasts. And these are urgently needed to address various challenges posed by climate changes, whether in agricultural water resources, water management, urban planning, or disaster risk and insurance planning. Focusing on 1-9-day precipitation forecast, this study developed a post-processing technique to calibrate and downscale the European Centre for Medium-Range Weather Forecasts (ECMWF) single deterministic forecast data (HRES), and generate calibrated probabilistic and single deterministic precipitation forecast. Forecast evaluation shows that generated probabilistic forecasts have superior performance in reliability, discrimination ability, and forecast skill, even for extreme precipitation events. Besides, the post-processed single deterministic forecast displays smaller-scale precipitation characteristic. In other words, more valuable meteorological forecast information can be obtained through the developed post-processing technique.
AS83-A009
A Statistical Post-processing Technique for Probabilistic Forecasts of Consecutive Days of Heat and Cold Events in Taiwan
Yuchen CHIANG1#, Hui-Ling CHANG1,2, Joyce JUANG1+, Pay-Liam LIN2, Chih-Yung Feng FENG3, Kuan-Lun LIU4, Jing-Shan HONG5
1Central Weather Administration, Taiwan, 2National Central University, Taiwan, 3Manysplendid Infotech, Ltd., Taiwan, 4Manysplended Infotech Ltd, Taiwan, 5Central Weather Bureau, Taiwan
In recent years, the increasing frequency of extreme weather events has emphasized the critical need for accurate warnings of heat and cold events, substantially impacting agricultural practices in Taiwan. These events not only disrupt crop growth and development but also markedly influence crop quality and yield. Addressing this challenge, we have developed a statistical post-processing technique that integrates the Bayesian Processor of Output (BPO) and Logistic Regression methods. This approach aims to enhance the quality of extended-range probabilistic forecasts for consecutive days of heat and cold events in the agricultural region. Our evaluation results demonstrate the effectiveness of this methodology in bias correction and downscaling. Calibrated probabilistic forecasts using BPO exhibit better reliability, discrimination, and forecast skill for single-day heat and cold events compared to raw probabilistic forecasts. However, recognizing the interdependence of consecutive heat and cold events, direct multiplication of calibrated forecast probabilities for each consecutive day results in unreliable forecasts. To address this issue, Logistic Regression is applied in conjunction with BPO to adjust forecast probabilities for consecutive days of heat and cold events, leading to a substantial improvement in reliability, particularly for consecutive heat events. This innovative statistical post-processing technique provides a more reliable and skillful prediction for consecutive days of heat and cold events, enabling more effective preparation and mitigation strategies for the agricultural sector in response to changing environmental conditions in Taiwan.
AS83-A021
Raindrop Size Distributions of Seasonal Rainfall Over Taiwan and Their Implications Using Machine Learning Approach
Balaji Kumar SEELA1,2+, Jayalakshmi JANAPATI1, Pay-Liam LIN1#
1National Central University, Taiwan, 2Academia Sinica, Taiwan
The raindrop size distribution (DSD) information is useful to delineate the microphysical characteristics of precipitation and their underlying processes. Furthermore, the RSDs aid in improving the quantitative precipitation estimation (QPE) algorithms and cloud modeling simulations. The RSDs were found to exhibit disparities with geography, season and precipitation type. Here, we used long-terms observations of ground-based disdrometers over north Taiwan to investigate the seasonal and spatial disparities in RSD characteristics. The results demonstrated dominant seasonal variations in the RSDs over the regional differences. Seasonal disparities and underlying microphysical attributes are delineated using remote sensing and re-analysis data sets. The radar reflectivity and rainfall rate (Z-R) relations, which are essential in QPE are established for each season are established. Furthermore, the empirical relations between any two parameters of the Gamma distribution (N(D) =N0Dμ e-ΛD; where D is the raindrop diameter in mm, N(D) is the number distribution function in m−3 mm−1, N0 is the intercept parameter in m−3 mm−1−μ, μ is the shape parameter, Λ is the slope parameter (mm−1) ) are also appraised; which helps in improving the microphysics parameterizations. Apart from the traditional way of estimating the RSD relations, here we machine learning approach to establish the RSD relations.
AS83-A024
Cloud and Rain Microphysical Characteristics of North Indian Ocean Tropical Cyclones During Pre-monsoon, Monsoon, and Post-monsoon Seasons
Surya Pramod JALAKAM1+, Pay-Liam LIN1#, Wei-Yu CHANG1, Balaji Kumar SEELA1,2, Jayalakshmi JANAPATI1
1National Central University, Taiwan, 2Academia Sinica, Taiwan
This study investigates the environmental conditions associated with the frequency of tropical cyclone (TC) occurrences (TCOF) and their impacts on the TC’s rain microphysics over the North Indian Ocean (NIO) throughout the major monsoon stages (pre-monsoon, monsoon, and post-monsoon) from 2014 to 2021. The Arabian Sea (AS) and the Bay of Bengal (BOB) areas are given emphases within the NIO domain. High TCOF is attributed to the combined presence of warm SST and cyclonic wind or positive 850-hPa relative vorticity. During the monsoon season, TCs exhibit limited intensification as a result of a pronounced deep layer wind shear. Using case studies, results show notable differences in the precipitation pattern across the major monsoon stages. Although heightened reflectivity and substantial precipitation are consistently identified within 50km radius from the storm’s center in all monsoon stages, TC Vayu (2019) during monsoon stage stands out with the most intense rainfall and highest reflectivity within the inner band region. This is followed by TC Fani (2019) during pre-monsoon and lastly by TC Kyaar (2019) during post-monsoon. The heightened reflectivity and substantial precipitation observed during the monsoon season are apparently attributed to the abundant presence of relative humidity and cloud liquid water content throughout the monsoon months from June to September.
AS83-A025
An Investigation on Microphysical Characteristics of Heavy Rainfall Events Over Taiwan
Jayalakshmi JANAPATI1+, Balaji Kumar SEELA1,2, Pay-Liam LIN1#
1National Central University, Taiwan, 2Academia Sinica, Taiwan
Heavy to extremely heavy rainfall events are the major source of flash floods, landslides and agricultural damage. An increase in heavy rainfall events, more particularly in between May to September months, over Taiwan necessitate for the detailed investigation. The present study is aimed to investigate the spatial and temporal variations in the heavy rainfall events over Taiwan. Long-term data sets from the ground-based rain gauges, disdrometers, airborne radars (TRMM/GPM DPR) are used to investigate the rainfall and microphysical attributes of heavy rainfall events. The results showed higher occurrence frequency of heavy rainfall events over central Taiwan than the rest of the island. The contour frequency by altitude diagram of rainfall and raindrop size distribution estimates from the GPM DPR data products revealed contrasts in the microphysical features of heavy rainfall events across Taiwan. Apart from this, Modern-Era Retrospective analysis for Research and Applications, Versions2 (MERRA-2), re-analysis. Moderate Resolution imaging spectroradiometer (MODIS) and re-analysis data sets are also used to explore the influence of aerosol-cloud interactions on heavy rainfall events over Taiwan.
AS83-A029
The Feature of the Raindrop Collision Process in Afternoon Thunderstorms Revealed by Drop Size Distribution
Chen-Hau LAN+, Pay-Liam LIN#, Yu-Chieng LIOU
National Central University, Taiwan
The variability of the drop size distribution (DSD) caused by microphysical processes is one of the reasons for poor quantitative precipitation forecasts (QPF) under bulk microphysics schemes. Therefore, it is necessary to understand the actual microphysical process variations in different weather systems. After analyzing the long-term characteristics of DSD, the data in Taiwan indicated that the microphysics processes of afternoon convection in summer exhibit higher variability compared to other weather systems, particularly under warm rain processes. On the other hand, this study attempts to quantitatively analyze the collision effects during the warm rain process using the DSD function. The collision rate (CR) and probability of collision (Prcollision) are effective in categorizing DSD features and predicting collision process fingerprints. In contrast, after comparing with the radar variables, the current bulk microphysics schemes make it difficult to effectively understand the warm rain collision process because of the limitation of the DSD shape. Furthermore, this study performs a synthetic analysis of the observed afternoon convection data during the 2022 TAHOPE/PRECIP experiment to understand the variation of the warm rain collision process under different convection scenarios. The results show that in addition to the collisional aggregation process, the importance of collisional fragmentation on convective evolution has been underestimated.
AS89-A005
Reconstructing High-spatiotemporal Resolution AOD in China With Multi-source Data
Yu SUN#+, Lin SUN
Shandong University of Science and Technology, China
High temporal resolution aerosol optical depth (AOD) observations derived from new-generation geostationary (GEO) satellites possess unique advantages. Unfortunately, the AOD products obtained by GEO satellites are limited to specific region. In this study we use polar orbit satellite data to expand the spatial range of GEO-AOD and propose a multi-source AOD data fusion method based on machine learning. We fully explore the complementary information from multi-source satellite observations and reanalysis data, and generate hourly full-coverage AOD maps in China for an entire day. The verification results indicate fused AOD dataset matches well with the ground AOD measurement. Also, the temporal and spatial AOD variation trends can be reconstructed based on this method, which consistent with the ground air quality monitoring stations observations. The fused dataset substantially enhances the availability of GEO-AOD data, and it has far-reaching significance for the evaluation of air pollution in the near surface regions of China.
AS89-A014
Methane Emissions in Oil and Gas Production Regions in Alberta: A Multiscale Measurement Campaign
Donglai XIE1#+, Hugh LI2
1Environmental Defense Fund, Canada, 2Environmental Defense Fund, United States
Canada imposed new methane regulations on upstream oil and gas sector in 2020 aiming to achieve a 40-45% reduction in methane emissions by 2025, and a 75% reduction by 2030. In 2021 and 2022, Environmental Defense Fund (EDF) conducted multiscale (facility level and regional level) aerial mass balance measurement campaigns in Alberta to assess the actual methane emissions from upstream oil gas sector. In partnership with Scientific Aviation, we completed aerial mass-balance flights around eleven geographically distinct oil and gas production regions within Alberta and compared to the local emission inventories estimated from a model developed by EDF following the same methodologies used by Environment and Climate Change Canada for national inventory reporting. Our analysis revealed that for most regions, measured emissions were ~1.5 to 2 times higher than the inventory. We conducted measurements at 16 upstream O&G facilities in Alberta in 2021, and the measurements revealed that emissions were, on average, 1.7 (SD: 0.6) times higher than the reported emissions for the same year. On a subsequent campaign in 2022, we focused on understudied O&G sectors covering 24 midstream and end-use facilities. These sites were found to be emitting, on average, 4.0 (SD: 1.1) times more CH4 than reported. This work highlights the need for direct measurements to verify modelled inventories and regulation-driven reductions.
AS89-A015
A Comprehensive Approach Towards Improving Regional Methane Emission Estimates Over India
Thara Anna MATHEW#+, Dhanyalekshmi K. PILLAI, Monish Vijay DESHPANDE, Vishnu THILAKAN, Sanjid Backer KANAKKASSERY
Indian Institute of Science Education and Research, Bhopal, India
Considering the higher global warming potential of Methane (CH4) and low residence time in comparison with the other greenhouse gases (GHGs) such as carbon dioxide, the mitigation efforts for minimizing the adverse effect of climate change has recently given increased focus on reducing methane emissions. Accurate estimation of the regional GHG emissions is crucial towards addressing the climate change scenario. In the Indian context, major contributions of methane emissions come from domestic ruminants, fossil fuels, waste, rice agriculture, wetland emissions, etc. In the present study, we use column averaged dry-air mixing ratio of methane (XCH4) from TROPOMI (Tropospheric Monitoring Instrument) on the ESA Copernicus Sentinel-5 Precursor satellite to infer India’s CH4 emissions. We attempt to assess the potential of these retrievals to quantify methane emission hotspots and to improve the emission estimates over the Indian sub-continent. Along with the satellite observations, the Eulerian atmospheric transport model Weather Research Forecast (WRF) coupled with Chemistry (WRF-Chem-GHG) has been used for the forward transport simulations of atmospheric methane. Also, the results from an inversion study by using these satellite observations will be presented.
AS89-A016
Quantifying Per-particle Optical, Physical, and Vertical Properties of Absorbing Aerosols Based on Multiple Surface and Remotely Sensed Measurements Over Coal-dominated Regions
Luoyao GUAN+, Shuo WANG, Jason COHEN#
China University of Mining and Technology, China
The coal energy sector in China, including Shanxi and the Golden Energy Triangle, is marked by numerous coal mines and industries focusing on coal use. Both due to co-emissions as well as over time in the atmosphere in-situ, these particles interact with various low-volatility atmospheric components and form coated structures in which the absorbing aerosol (black carbon and coal dust) forms core, while refractory species (sulfate, nitrate, water, etc.) form shell. This study conducted field observations of surface BC concentration, size distribution, and AOD in coal-mining areas. A Mie model based on a “core-shell” configuration is used with all individual waveband observations, to form a solution space and uncertainty bounds of the per-particle optical information (SSA, ABS, EXT). These values are then used to respectively invert the column number and mass loading. Firstly, fine-mode black carbon aerosols are shown to exhibit a trimodal lognormal fine-mode size distribution, differing from previous studies. These results align with the fact that local sources include a very diverse set of sources including high temperature combustion, low-temperature combustion, coal to chemicals, coal dust, and coal transportation. Secondly, the absorbing aerosol demonstrates strong absorption of solar radiation in the near ultraviolet and blue bands, leading to a situation in which the typical use of aethalometer observations in the typical 880nm band used to obtain BC, yields a significantly low SSA bias. Thirdly, the SSA distribution characteristics of the absorbing aerosols do not entirely conform to the power-law relationship of AAE, resulting in deviations when estimating SSA across all size bins. This finding is consistent with additional bias with respect to many models, which tend to underestimate aerosol mixing and aging. Finally, analyzing the radiative effects and properties from the different radiative bands and size distributions provides detailed information on aerosol physical and optical properties.
Session Chair(s): Jun LI, National Satellite Meteorological Center
AS15-A029
Satellite Data Applications by Combining Imager and Sounder Observations
Likun WANG#+
University of Maryland
It is a common practice for an environmental satellite platform to carry a suite of sensors designed to collect meteorological, oceanographic, climatological, and solar-geophysical observations of the Earth. Among them, a scanning imaging radiometer (collecting visible and infrared imagery) and a hyperspectral infrared sounding instrument (observing infrared spectrum) are often onboard together. In contrast to a state-of-the-art high-spatial-resolution imager instrument, the sounder instrument provides information on the vertical profiles of temperature, water vapor, and critical trace gases of the atmosphere, albeit with coarse spatial resolution. The combination of high spatial resolution measurements from an imager and high spectral resolution measurements from an infrared sounder can take advantage of both spectral and spatial capabilities; hence, it can further improve atmospheric and surface geophysical parameter retrievals and data utilization for numerical weather prediction (NWP) models. Furthermore, owing to its hyperspectral nature and accurate radiometric and spectral calibration, radiance spectra from the IR sounder can be integrated through the spectral response functions (SRF) to simulate imager radiance measurements and thus independently assess spectral and radiometric calibration accuracy of IR channels of the imager. Finally, by taking advantage of high spatial resolution and accurate geolocation of imager measurements, spatially collocated measurements from the imager bands can effectively evaluate the geolocation accuracy of that has a coarse spatial resolution. In this talk, the author presents several applications on satellite data application through data fusion by combing imager and sounder measurements. In addition to previous intercalibration efforts, particularly, in support of data assimilation of NWP models, a recently developed algorithms of Visible Infrared Imaging Radiometer Suite (VIIRS) radiance cluster analysis within Cross-track Infrared Sounder (CrIS) field of view (FOV) to provide sub-pixel scene homogeneity information is presented. By collaborating with the NWP centers, the preliminary data assimilation results will be reported using CrIS-VIIRS Cluster Data.
AS15-A042
Enhancing GK2A Atmospheric Profiles: A Machine Learning Approach with ERA5 Reanalysis Data
Daehyeon HAN#+, Sihun JUNG, Minki CHOO, Juhyun LEE, Jungho IM
Ulsan National Institute of Science and Technology
The atmospheric profile is critical for understanding the status of the atmosphere at various vertical levels, and its accuracy is essential for better weather forecasting. Reanalysis aims to provide accurate profile by assimilating multiple past datasets with its innate time lag. Numerical weather prediction (NWP) models generate three-dimensional atmospheric forecasts from the surface to the top of the atmosphere operationally. To enhance the accuracy of atmospheric profiles from NWP, a radiative transfer model (RTM) is used to reflect current atmospheric conditions from geostationary satellites. The RTM-based approach facilitates real-time corrections to the atmospheric profile, narrowing the gap between NWP and reanalysis data. To further narrow this gap, we propose a machine learning (ML)-based bias correction for atmospheric profiles using data from geostationary satellites and reanalysis. Specifically, we trained a Light Gradient Boosting Machine (LGBM) to update the atmospheric profile product from the Geo-KOMPSAT-2A (GK2A) satellite by simulating the ERA5 reanalysis data. We used brightness temperatures from GK2A's shortwave to infrared channels to capture current atmospheric information. Compared with ERA5 and radiosonde measurements, our model demonstrated improvements over GK2A products in terms of root mean squared error (RMSE) and mean bias. Additionally, we conducted analyses of feature importance and seasonal error patterns. Our findings suggest that ML can enhance RTM-based atmospheric profiles, demonstrating that the synergistic application of additional bias correction methods can be effective.
AS15-A045
Enhancing Land Surface Temperature Imaging Using Reference Based Super-resolution
Lee SUNJU#+, Sewoong AHN, Yeji CHOI, Beomkyu CHOI
SI Analytics
The latest advancements in deep learning for image super-resolution are proving to be valuable for addressing various challenges, including medical imaging, remote sensing, and image enhancement. Traditional single-image super-resolution (SISR) methods often rely on synthetically degraded low-resolution images generated from their high-resolution counterparts, usually through techniques such as bilinear down-sampling. However, these synthesized images may not accurately capture the characteristics of low-resolution images encountered in real-world applications. This issue is particularly critical in the context of weather satellite imaging, as data features such as Land Surface Temperature (LST) inherently lack real-world noise. Therefore, utilizing methods that involve degradation for super-resolution may lead to compromised results. To address this issue, we leverage high-resolution images from a different domain that we can reference. Our dataset utilizes low-resolution images from KOMPSAT2A (GK2A) and reference images from KOMPSAT2B (GK2B) as input images, with LANDSAT images serving as the ground truth. Our model employs Discrete Cosine Transform operations and a Guided Spatial Edge Attention module to transfer the edge areas of the high-resolution reference images to the low-resolution images, allowing us to generate more detailed regions than other methodologies. To validate the model's performance, we compare it with Single Image Super Resolution methodologies, assessing accuracy not only through visual inspection and metrics such as PSNR, SSIM, and MSE but also by comparing accuracy with AWS.
AS15-A054
Merging of SSU Observations with AIRS Toward Extending Stratospheric Temperature Climate Data Records
Likun WANG#+
University of Maryland
Long-term changes in stratospheric temperatures are important for climate trend monitoring and interpreting the radiative effects of anthropogenic emissions of ozone-depleting substances and greenhouse gases. The Stratospheric Sounding Unit (SSU) onboard the historical NOAA Polar Orbiting Environmental Satellite (POES) series was a three-channel infrared radiometer designed to measure temperature profiles in the middle and upper stratospheres. Although the SSU observations were designed primarily for weather monitoring; however, due to continuity, long-term availability, and global coverage, they comprised an indispensable climate data record that had been playing a key role in estimating temperature trends in the middle and upper stratospheres for the period of 1979–2006 (Wang et al. 2012; Zou et al. 2014). On the other hand, since 2002, the hyperspectral infrared sounding measurements including the Atmospheric Infrared Sounder (AIRS), the Infrared Atmospheric Sounding Interferometer (IASI), and the Cross-track Infrared Sounder (CrIS) provides decades of infrared hyperspectral radiance datasets. Moreover, owing to their hyperspectral nature and accurate radiometric and spectral calibration, these datasets provide 3D measurements of stratospheric temperature with high data quality. This study presents recent efforts of merging of the SSU stratospheric temperature data with AIRS. We generated the training datasets of SSU and AIRS from the UMBC 48 profiles for different scan angles using the community radiative transfer model (CRTM). A linear regression model with considering weighting function and instrument noise as constrains is developed to convert AIRS into equivalent SSU based on training datasets. By taking advantages of their overlapped period of SSU and AIRS in 2002-2006, this method will be validated using real observations.
AS15-A055
Understanding Brown Carbon from Wildfires Through the Synergistic Use of DSCOVR EPIC, MISR, and CALIPSO Data Products
Michael GARAY#+, Olga KALASHNIKOVA
California Institute of Technology
Black Carbon (BC), emitted mainly by high-temperature combustion processes, and Brown Carbon (BrC), emitted mainly by smoldering fires or low-temperature biomass combustion, are two of the most important light absorbing substances in atmospheric aerosols. The assessment of the nature and global-scale magnitude of biomass burning (BB) aerosol impacts is currently hindered by an inadequate understanding of the regionally-dependent atmospheric transformations of absorbing aerosol properties that occur during downwind transport of BB plumes and resulting impacts on cloud properties and the radiative balance due, in part, to remote sensing challenges in retrieving spatial information on specific aerosol types. The Earth Polychromatic Imaging Camera (EPIC) sensor aboard the Deep Space Climate Observatory (DSCOVR) spacecraft provides cloud detection, aerosol optical depth (AOD), atmospheric correction, Absorbing AOD (AAOD), the UV-VIS imaginary part of the refractive index, and absorbing aerosol speciation on a 10-km sinusoidal grid through the Multi-Angle Implementation of Atmospheric Correction (MAIAC) algorithm. In this work, we assess the performance of the MAIAC algorithm for EPIC in comparison with near-simultaneous aerosol retrievals from the Multi-angle Imaging SpectroRadiometer (MISR) instrument on the Terra satellite, as well as profiles from the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) instrument on the CALIPSO satellite. We concentrate on major fire events that have taken place during the DSCOVR mission beginning in June 2015, with a focus on North America.
AS15-A014
Detection and Tracking of Shallow and Deep Convection Using the New-generation Geostationary Satellite Over Eastern China
Yahui TANG#+
Beijing Normal University
Convective clouds are common and play a major role in Earth’s water cycle and energy balance. In this study, we construct convective cloud detection and tracking algorithms for the Himawari-8 Level 1 data by texture analysis, clustering, Fourier phase shift, disparity, Hungarian method. By identifying and tracking convective clouds over the course of a year, it was found that most of their lifespans do not exceed one hour. Area, cloud top brightness temperature and cloud optical thickness of convective clouds shows a single-peak type during the life time. In analyzing the characteristics of convective clouds in eastern China, it is found that deep convection occurs mainly in the southern region of China, followed by the central region of North China. The average lifetime of deep convective clouds is about 87 minutes, while the lifetime of deep convective clouds in the central region is slightly shorter, between 60-70 minutes. However, deep convection in the northern region is more often transformed from shallow convective clouds. The transformation time of shallow convective clouds to deep convective clouds is about 48 minutes on average. The average is about 50% of the whole life span. In the area north of the Yangtze River, the transformation time from shallow to deep is between 50-60 minutes, which is slightly longer than 10 minutes relative to the southern area. Overall, this study contributes to our understanding of the physical properties of convective clouds of different intensities during their lifetimes, as well as the spatial and temporal distribution characteristics, and helps us to further investigate the effects of aerosols on convective clouds of different intensities and scales at different lifetimes, which is also conducive to the improvement of weather and climate forecasting.
Session Chair(s): Wonsik CHOI, Pukyong National University
AS08-A036
| Invited
Multiyear Signature of Nitrogen and Carbon Isotope Ratios of PM2.5 in Urban Seoul
Hyomin KIM1, Meehye LEE1#+, Saehee LIM2, Joo-Ae KIM1, Claudia CZIMCZIK3, Xiaomei XU3, Kyungwhan KIM4
1Korea University, 2Chungnam National University, 3University of California, Irvine, 4Korea Institute of Science and Technology
Carbon and nitrogen isotopic ratios were analyzed in PM2.5 samples collected at Korea University Campus from 2018 to 2022. This study focused on radioactive carbon (Δ14C) and stable carbon (δ13C) isotopes in total carbon (TC), as well as stable nitrogen isotope (δ15N) in total nitrogen (TN). Additionally, chemical constituents, including secondary inorganic ions, OC, EC, and water-soluble organic carbon and nitrogen, were investigated. Isotope ratios exhibited clear seasonality, aligning with variations in PM2.5 mass and major chemical composition with frequent occurrence of heavy pollution events during the cold season (October to March). The contribution of non-fossil sources to total carbon exceeded that of fossil fuels, with an average fM (fraction modern) of 0.61±0.09, slightly higher in the warm season than in the cold seasons. In comparison, the δ13C of TC was -24.4±1.0‰ and -25.5±1.0‰ in the cold and warm season, respectively, indicating a more significant influence of coal during the cold season, despite a narrow range of δ13C variations. In the warm season when PM2.5 mass was low, the high fM (0.73 ± 0.14) coupled with low δ13C (–25.9 ± 0.4‰) suggested the contribution of biomass sources through secondary formation. The average δ15N of TN was distinctively higher in the warm season (11.3±3.0‰) than in the cold season (9.3±3.3‰). Notably, δ15N and δ13C exhibited an inverse correlation, with the lowest δ15N associated with the highest PM2.5 mass. The nitrogen and carbon isotope signatures in this study suggest larger contributions from coal-burning sources during the heavy pollution incidents in the cold season.
AS08-A004
| Invited
Interfacial SO2 Oxidation Chemistry at the Sea Surface Microlayer Leads to Enhanced Air Pollution in the Coastal Cities
Sasho GLIGOROVSKI#+
Chinese Academy of Sciences
In the marine boundary layer (MBL), sulfur dioxide (SO2) is oxidized to sulfate, or deposited on ocean surface thereby reacting with the enriched organic material within sea surface microlayer (SML) such as unsaturated fatty acids. Sea surface microlayer (SML) is defined as the most upper layer of the ocean surface water and represents one of the largest active interfaces on earth. In this study, we investigated the interfacial SO2 oxidation chemistry on authentic marine SML sampled from 10 sites on South China Sea. Real-time measurements of the VOCs formation in dark and under light irradiation (300 nm < λ < 700 nm) were performed by utilizing a Secondary Electrospray Ionization High-Resolution Mass Spectrometry (SESI-HRMS) on-line coupled to a reactor. We observed a strong enhancement in VOCs production upon SO2 oxidation chemistry at authentic SML samples under actinic illumination compared to dark conditions. Namely 33 common product compounds were identified in dark, whereas 144 common product compounds were identified in light, among all ten sampling sites. Among all the common product compounds, three CHN compounds with double bond equivalent (DBE) = 2 differing by regular CH2 pattern were detected under light irradiation, and identified as m/z 112.112 [C7H13N]H+, heptanenitrile, m/z 126.128 [C8H15N]H+, octanenitrile and m/z 140.143 [C9H17N]H+, nonanenitrile. Long-chain alkyl cyanides contain C≡N bond in their structure indicating that they are potentially toxic compounds. The resulting data updated new knowledge and constrained the fingerprints of formed VOCs upon the interfacial reaction between SO2 and sea surface microlayer.
AS08-A002
Mercury Isotopic Characterizations During Fog and Non-fog Events at the Marine Boundary Layer
Safrul AMRI+, Ju Hyeon LEE, Seung Hyeon LIM, Eunjin SON, Young Gwang KIM, Hoin LEE, Moonkyoung CHO, Jiwon YOON, Sae Yun KWON#
Pohang University of Science and Technology
Mercury (Hg) is a global atmospheric pollutant due to its long-range transport and biomagnification in ecosystem in the form of methylmercury (MeHg). Fog events play a crucial role in the deposition of atmospheric Hg, accounting for approximately 33% of the MeHg wet deposition and 13% of the total mercury (THg) flux. Hg isotopes are a powerful indicator for discerning sources and biogeochemical processes within the environment. A previous study, which characterized Hg isotopic compositions in fogwaters at the upwelling zone of California, U.S., revealed positive odd MIF signatures, suggesting that photoreduction plays an important role in degrading toxic MeHg to inorganic Hg. Yeongdo Island, situated in South Korea, is characterized by severe summer fog events with a unique blend of urban features, including national geopark and industrial activities (i.e., shipbuilding construction), representing an opportunity to distinguish the relative importance of sources and biogeochemistry of Hg in fogwater. In the summer of 2023, atmospheric water vapors were collected during fog and non-fog events along with precipitation, particulate bound Hg (PBM), total gaseous Hg (Hg0), and seawater. The Hg isotopic compositions of fogwater were also compared between morning and afternoon. Our preliminary results, the median THg concentration in fogwater (1.25±0.74 ng/L) is lower than the water vapor during non-fog events (2.36±0.60 ng/L). Morning fog events (0.94±0.71 ng/L) showed a lower THg concentration than the afternoon (1.56±0.86 ng/L). The higher THg concentration in non-fog vapors and the afternoon fogwater indicate that MeHg photodegradation or Inorganic Hg photoreduction result in the loss of gaseous elemental Hg within the fog. In the upcoming results, the Hg isotopic compositions within fog and non-fog water will provide a deeper understanding of sources and processes, resulting in changes in THg concentration, Hg speciation, and substantial human health impacts via the inhalation of fog.
AS08-A019
High Enrichment of Heavy Metals in Fine Particulate Matter Through Dust Aerosol Generation
Qianqian GAO#+, Xiaofei WANG
Fudan University
Dust is a major source of atmospheric aerosols. Its chemical composition is often assumed to be similar to the parent soil. However, this assumption has not been rigorously verified. Here, we generated dust aerosols from soils to determine if there is particle size-dependent selectivity of heavy metals in the dust generation. Mn, Cd, Pb and other heavy metals were found to be highly enriched in fine (PM2.5) dust aerosols, which can be up to ~6.5-fold. To calculate the contributions of dust to atmospheric heavy metals, regional air quality models usually use the dust chemical profiles from the US EPA’s SPECIATE database, which does not capture the correct size-dependent selectivity of heavy metals in dust aerosols. Our air quality modeling for China demonstrates that the calculated contribution of fine dust aerosols to atmospheric heavy metals, as well as their cancer risks, could have significant errors without using proper dust profiles.
AS08-A022
A Comprehensive Air-sea-land Measurement Campaign of Volatile Organic Compounds (VOCs) During an Ozone Episode in Hong Kong: Utilizing a Novel Helicopter-based Platform
Yuchen MAI1+, Dasa GU1#, Yuxi SUN1, Nirmal Kumar GALI1, Zhi NING1, Donald BLAKE2
1The Hong Kong University of Science and Technology, 2University of California, Irvine
Ground-level ozone has long been recognized as a detrimental pollutant due to its adverse effects on both ecosystems and human health. To address this pollution, reducing the emissions of its precursors, namely nitrogen oxides (NOx) and volatile organic compounds (VOCs), is crucial. However, achieving effective reduction requires a comprehensive understanding of these precursors. In this study, a novel airborne platform, in conjunction with ship and ground sampling, was employed to capture the pollutant profile throughout Hong Kong during an episode day. Through this campaign, we obtained three-dimensional profiles of VOC distribution from both temporal and spatial perspectives. Two campaigns conducted in 2022 were selected to analyze the pollutant distributions in this study. On September 5th, characterized by episodic pollution and prevailing northeast winds, the western region of Hong Kong exhibited higher concentrations (120 ppb) of ozone (O3) than the east region (80 ppb). During the episode, the eastern region, including Tap Mun Island, typically considered a background area, demonstrated relatively low concentration levels (8770 pptv) compared to the western region (12776 pptv). However, it is noteworthy that during non-episode days, the eastern side shared similar concentration levels (5500 pptv) with the western region over water. Regarding the vertical distribution of VOCs, most regions exhibited higher concentrations at lower altitudes (800 ft) compared to higher altitudes (1000-1500 ft), except for the eastern part of Hong Kong. Through further investigation, it was determined that the eastern side had a longer lifetime of pollutants during the episode, while the HYSPLIT analysis revealed that the air mass on the eastern side was mainly influenced by regional transport from Dongguan, whereas the western side was influenced by Huizhou. These findings provide valuable insights into the transportation of air pollutants and contribute to a more comprehensive and dynamic approach in mitigating pollution issues.
AS08-A037
Characteristics of PM2.5 Concentration Variations with a Focus on the Formation of Inorganic Species Based on Multi-seasonal Observations in Korean South Coastal Cities
Wonsik CHOI#+, Yongmi PARK, Myounghwa BYUN, Subin HAN, Youn-Suk SON
Pukyong National University
To understand the mechanism of PM2.5 formation in coastal cities in the southern region of Korea, field intensives were conducted over the four seasons of 2021 – 2022 in Busan, a coastal megacity of South Korea and home to the country’s largest port. During these field intensives, a variety of species were simultaneously measured, including PM2.5, particle size distributions (ranging from 12 nm to 10 mm), inorganic ion components, black carbon, and precursor gases (SOX, NOX, NH3, CO, O3). In this presentation, we present preliminary results and findings from these intensive campaigns. It is known that the increase in fine particle concentrations during spring and summer in the coastal regions of southern Korea (Ulsan and Busan), is influenced by industrial activities and emissions from ships and ports, leading to a rise in sulfate levels. However, this study shows that, since at least 2021, the contribution of nitrates to PM2.5 concentrations has linearly increased, not only in the cold winter but also during warm spring and summer, implying that NOx oxidation has become a more significant contributor to high PM2.5 pollution events in Korean coastal regions. This presentation also discusses the cause of PM2.5 formation, analyzing the evolution of inorganic components, size distributions, and precursor gases during periods of increasing PM2.5 concentrations. These analyses are further supported by thermodynamic model results (ISORROPIA II) and diurnal variations of various factors. These findings highlight the importance of nighttime heterogeneous chemistry involving nitrates in the formation of PM2.5 in Korean coastal regions. The local sea-breeze weather system is expected to contribute to the accumulation of PM2.5 in coastal cities through the formation processes of inorganic species proposed in this study.
Session Chair(s): Chun-Chieh WU, National Taiwan University, Taiga TSUKADA, Colorado State University
AS13-A027
| Invited
Fine-scale Tropical Cyclone Boundary Layer Structure
Karen KOSIBA1#+, Joshua WURMAN2
1University of Alabama Huntsville, 2University of Illinois
The tropical cyclone boundary layer (TCBL) is comprised of coherent structures likely responsible for significant transport of turbulent fluxes throughout the TCBL as well as regions of enhanced damage at the surface. DOW-observed TCBL structures include Tornado Scale Vortices, boundary layer rolls/streaks, and eyewall mesovortices. Results from several tropical cyclones will be discussed in the context of standard tropical cyclone wind models and the relationship between radar winds and derived quantities to anemometry.
DOWs collected data in Category 4 Laura in southwestern Louisiana, including fine-scale, near-surface data in the eyewall. Multiple sets of dual-Doppler analyses were conducted in order to optimize the retrievals of 2D/3D structures. Comparisons between the strength and size of the structures in the eyewall vs. rainbands will be presented. DOWs and an array of surface based instruments, including a prototype, “POLENET”, which attaches existing infrastructure, allowing for a customizable observation level, were deployed in order to correlate observations at radar level with surface observations. Using corrections based on turbulence statistics and roughness lengths, a reduction factor was derived for the radar winds, allowing for comparison between radar level winds and winds observed at 1, 2, and 10 m. Turbulence characteristics, periodicity, and gust factors will be compared to radar-derivations of similar quantities. A new field project, WASHABLE (Winds And Structures in Hurricane Associated Boundary Layers Experiment), is planned for 2024-2025. WASHABLE will deploy DOWs and other instrumentation to expand our understanding of TCBLs, including gust damage relationships and turbulent processes.
AS13-A016
Airborne and Spaceborne Observations of Tropical Cyclones with Microwave Sounders: Retrievals and Assimilations
Mathias SCHREIER#+
California Institute of Technology
Airborne and spaceborne microwave sounders have proven immensely useful for observing tropical cyclones. But both have advantages and disadvantages: While spaceborne observations cover large areas, they often have only one or two overpasses daily; airborne observations, on the other side, can provide longer flight times but cover only a small part of the area. Additionally, precipitation is a big handicap for both when it comes to the retrieval of atmospheric data. We developed a new retrieval algorithm to process data from microwave instruments and make it easier to assimilate atmospheric information. The new algorithm includes a variety of quality checks for easier assimilation. It also includes scattering components and uncertainty estimates and is focused on better use of the data concerning precipitation. The ultimate goal is to optimize the retrieval results for various assimilation methods and provide as much information as possible, especially close to critical areas, like convective cells or centers of tropical cyclones. In this presentation, we will focus on the two types of observations: We will present airborne observations from a microwave sounder and discuss the retrieval data. We will discuss the observation of tropical convection and fully developed tropical cyclones. Additionally, we will discuss the additional information from spaceborne observations for the same phenomena. We will explain how the new retrieval algorithm works on both datasets and how we validated our observations with external information. We will also discuss how we prepared the data for assimilation and how far quality flags and uncertainty values helped to optimize the assimilation processes. Lastly, we will also discuss the impact of the different datasets on the assimilation process. Copyright 2023 California Institute of Technology. Government sponsorship acknowledged
AS13-A060
Analysis and Forecast of Typhoon Chanthu (2021) Using an Ensemble Radar Data Assimilation System: Impact of Model Horizontal Resolution and Assimilation Frequency on Vortex Spindown
Kuan-Jen LIN#+, Shu-Chih YANG
National Central University
Typhoon Chanthu (2021) is a category 5-equivalent super typhoon with a very narrow eye when it is approaching Taiwan. During its northward movement offshore the east coast of Taiwan, it is well-observed by the coastal radar network. Therefore, this study assimilates the high-resolution radar observations using the WRF-local ensemble transform Kalman filter radar assimilation system (WLRAS) to investigate the analysis and prediction of super typhoon Chanthu. Results show that assimilating the radar data greatly improves the analysis of Chanthu. However, significant vortex spindown occurs when the deterministic forecast is initiated. Such results motivate this study to further investigate the causes of the significant vortex spindown. In particular, the impact of model horizontal resolution and assimilation frequency is examined. The original WLRAS uses a triply nested domain with the finest horizontal resolution of 4 km, and the assimilation frequency is 15 minutes. Experimental results show that increasing the model horizontal resolution from 4 km to 1.33 km at the forecast stage can alleviate the spindown issue. Furthermore, the spindown is better resolved when the model resolution is increased earlier at the DA stage. Such results indicate that the high-resolution model is important not only for the forecast but also for the analysis performance. The positive impact of increasing model resolution is attributed to the better-resolved secondary circulation at the eyewall and the stronger warm core structure. Experimental results also show that using either 15-, 30-, and 60-minute assimilation intervals can establish good tangential wind structure within 3 hours, but only the 15-minute rapid update cycle is able to reconstruct the complete typhoon circulation and sustains typhoon intensity after a 12-hour forecast. It reveals that the rapid update cycle is critical for assimilating the dense radar data to obtain an accurate TC analysis and forecast.
AS13-A043
Wind Distribution in the Eye of Tropical Cyclone Revealed by a Novel Atmospheric Motion Vectors Derivation
Taiga TSUKADA1#+, Takeshi HORINOUCHI2, Satoki TSUJINO3
1Colorado State University, 2Hokkaido University, 3Meteorological Research Institute
Observations of wind distribution in the eye of tropical cyclones (TCs) are still limited. In this study, a method to derive atmospheric motion vectors (AMVs) for TCs is developed, where selection from multiple local rotation speeds is made by considering continuity among neighboring grid points. The method is applied to 2.5-min interval image sequences of three TCs, Lan (2017), Haishen (2020), and Nanmadol (2022), observed by Himawari-8 satellite. The results are compared with AMVs derived from research-based 30-sec Himawari-8 special observations conducted for Haishen and Nanmadol, as well as with in-situ observations using dropsondes conducted for Lan and Nanmadol. The AMVs obtained from the 2.5-min interval images in the eye are found to be in good agreement with the dropsonde observations. As asymmetric motions in the obtained AMVs in the eye, transient azimuthal wavenumber-1 features are identified in all three TCs. These features are consistent with algebraically growing wavenumber-1 disturbances, which transport angular momentum inward and accelerate the eye rotation. In the case of Lan, the angular velocity in the eye increased by approximately 1.5 times within 1 hour. This short-term increase is further examined. Visualization of low-level vorticity in the eye and angular momentum budget analysis suggest that angular momentum transport associated with mesovortices have played an important role in the increase of tangential wind and the homogenization of angular velocity in the eye of Lan. A paper related to this presentation has been submitted to JGR-Atmospheres.
AS13-A053
OLR-based Zonally Undulating Strength of the Subtropical High in the Western North Pacific
Sanghyeon YUN+, Rok SEONG, Namyoung KANG#
Kyungpook National University
Subtropical high (STH) is useful measure for understanding extreme weather induced by tropical convections in the East Asia. The semi-permanent STH is controlled by global circulation and dominates the atmospheric patterns of the basin during the boreal summer. The climate of East Asia during the boreal summer varies greatly depending on how STH changes in the region. Previous study has investigated how the western edge of STH expands in response to the variations of environmental conditions (Yun et al. 2023). The edge of STH farther expands during La Niña phase compared to El Niño phase. However, the response of regional STH strength has not been explored yet. It is confirmed that the main convective source in response to the El Niño-Southern Oscillation (ENSO) during June to August is located in the southeastern quadrant (5°N-20°N, 140°E-180°) of the western North Pacific. This study finds that the STH strength in relation to the wave propagation induced by the tropical convection fluctuates apparently in the central northern part (25°N-35°N, 140°E-180°) of the western North Pacific. This geographically asymmetric response of STH to ENSO implies zonally undulating distribution of STH strength during its expansion. Conclusively, La Niña phase is accompanied by weaker strength in the inner region of STH, even though STH experiences westward expansion. In contrast, El Niño phase shows a stronger STH with a shrunken edge to the east. This suggests that the expansion of STH does not necessarily mean an increase in its strength. The importance of this study lies in the fact that the statistical model of OLR effectively illustrates how the ENSO variation and global warming bring the zonally undulating strength of boreal-summer WNPSH.
AS13-A059
A Parametric Model Incorporated with Satellite Wind for Tropical Cyclone Surface Wind Speed Assessment
Yi-Pin CHANG+, Shu-Chih YANG#, Kuan-Jen LIN
National Central University
The surface wind speed (SWS) structure of tropical cyclones (TCs) is essential for assessing their size and intensity, which are critical for disaster prevention. Empirical parametric wind models provide stable products for TC SWS. Although empirical profiles are beneficial for TC initialization and intensity forecast, they can be less representative due to the lack of adjustment from real-time observations. As the quality and coverage of SWS measured by satellites have increased over time, it becomes necessary to complement parametric estimation with satellite data to obtain optimal profiles in real time. This study develops a method to construct the real-time SWS profiles by integrating data from Cyclone Global Navigation Satellite System (CYGNSS) wind, Advanced Scatterometer (ASCAT) wind, and operational initial TC vitals into the parametric wind model. The newly proposed parametric wind model is constructed by quadrants with temporal continuity. Particularly, the methodology handles spatiotemporally inhomogeneous characteristics in different satellite data. The algorithm is applied to the cases during the 2018−2020 Atlantic hurricane seasons, and the results are compared with the Synthetic Aperture Radar (SAR) products and the empirical profiles. Results show that the satellite-incorporated profiles well represent the TC structure and provide continuous and realistic products with TC asymmetry. The application and detailed analysis of satellite-incorporated profiles are further demonstrated with Hurricane Florence (2018).
AS13-A013
Torrential Remote Precipitation of Typhoon Nesat (2022) Over Greater Taipei Area: Dual-polarization Radar Analysis and Ensemble Simulations
Shian-Rong LIAO#+, Chun-Chieh WU
National Taiwan University
Remote precipitation associated with tropical cyclones is more challenging to predict and is often overlooked. Typhoon Nesat (2022) traversed the Bashi Channel, and was associated with a remote precipitation event characterized by three notable differences from previous cases. Firstly, the rainfall hot spot (about 300mm/12-h) was in the Greater Taipei area (GTA) rather than in Yilan. Secondly, cold air associated with the Siberian high had not arrived at the time of the event. Thirdly, there was a secondary moisture transport unconnected with the circulation of Nesat over the offshore area of northern Taiwan. In this study, we not only examined the unique remote precipitation case associated with Nesat, but we also used dual-polarization and dynamics variable data from the Wu-Fan-San radar to analyze the precipitation patterns and temporal distribution for the event. Significant differences appear between the rainband stage (R-stage) and convergence stage (C-stage). Profiles of dBZ, ZDR, KDP, ρhv and hydrometeor identification demonstrate that convection during the R-stage was deeper and contained larger particles than the C-stage. However, high concentrations of small particles at lower altitude and the enhanced convergence observed in the wind field analysis also resulted in significant precipitation during the C-stage. Then, we utilized Weather Research and Forecasting model to conduct ensemble simulations and to explore what roles those different mechanisms from previous researches may have played in causing the event. Results in simulations show that the stronger the northeasterly winds and moisture gradient in the Taiwan Strait, the heavier the rainfall in the GTA. Over the ocean east of northern Taiwan, both the intensity and vertical extent of moisture transport along the edge of the monsoon trough are positively correlated with rainfall in the GTA. And the secondary moisture transport separating from the circulation of Nesat is a distinctive feature compared to previous studies.
Session Chair(s): Francis Chi Yung TAM, The Chinese University of Hong Kong
AS72-A003
| Invited
Future Changes in Summer Monsoon Extremes, Evaporative Demand and Time of Emergence Over Asia in CMIP6 Simulations
Kyung-Ja HA1#+, Ji-Hye YEO1, Suyeon MOON2, Sun-Seon LEE1, Daeha KIM3
1Pusan National University, 2The University of Tokyo, 3Jeonbuk National University
Future greenhouse warming is expected to influence the characteristics of global monsoon systems. In this talk, I will present future changes in summer monsoon extremes, evaporative demand and time of emergence over Asia. Here we used CMIP6 models to determine how the length of the summer rainy season and precipitation extremes over the Asian summer monsoon domain will change in response to greenhouse warming. Over East Asia the models simulate on average the earlier onset and later retreat; whereas over India, the retreat will occur later. The model simulations also show an intensification of extreme rainfall events, as well as an increase of seasonal drought conditions. These results demonstrate the high volatility of the Asian summer monsoon systems and further highlight the need for improved water management strategies in this densely populated part of the world. Understanding the impact of global warming beyond preindustrial conditions on precipitation intensity is crucial for devising effective adaptation and mitigation strategies, particularly in densely populated global land monsoon (GLM) regions. However, the time of emergence (ToE) of extreme summer monsoon precipitation and its dependency on global warming targets has rarely been investigated. Using large ensemble simulations, we reveal that the impacts of anthropogenic forcing on extreme precipitation intensity in GLM regions become evident prior to 2050 accompanied by a sudden expansion of the ToE occurrence area, except for the Northern American monsoon. Furthermore, our study demonstrates that achieving the Paris Agreement goal at 1.5℃ of global warming level can prevent the ToE of extreme precipitation in the Asian and African monsoon regions. This, in turn, has the potential to halve the number of individuals exposed to extreme precipitation. These findings highlight the urgent need for action to mitigate the risk of anthropogenic climate change.
AS72-A004
The Role of Sea Surface Temperature in Shaping the Characteristics of Future Convective Afternoon Rainfall in Taiwan
Wan-Ru HUANG1#+, Yu-Tang CHIEN1, Chao-Tzuen CHENG2, Huang-Hsiung HSU3, Suranjith Bandara KORALEGEDARA1
1National Taiwan Normal University, 2National Science and Technology Center for Disaster Reduction, 3Academia Sinica
Convective afternoon rainfall (CAR) is a significant summer rainfall feature in Taiwan. This study investigates the projected uncertainties in summer CAR in Taiwan, using a dynamical downscaling approach with the Weather Research and Forecasting Model (WRF) and the High-Resolution Atmospheric Model (HiRAM). The projections were driven by four different sea surface temperature (SST) categories derived from CMIP5 model simulations under the RCP8.5 scenario. All projections indicate a reduced frequency but increased intensity of CAR over Taiwan by the end of the 21st century. However, notable differences in the degree of CAR changes were observed among simulations with varying degrees of Pacific SST warming. These variations in potential future changes in CAR frequency and intensity can be attributed to the variations in daytime thermal instability, local inland wind convergence, and moisture flux convergence over Taiwan. Furthermore, this study explored the linkage between local thermodynamic conditions and projected large-scale circulation patterns.
AS72-A024
Evaluation and Projection of Drought Frequency, Intensity and Duration Over Australia
Kevin CHEUNG1#+, Nicholas HEROLD2, Fei JI3, Nidhi NISHANT4
1Nanjing University of Information Science & Technology, 2Applied Climate Science Pty Ltd, 3NSW Department of Planning and Environment, 4University of New South Wales
Drought events, whether driven by meteorological or anthropogenic factors, have wide range and long-term social and economic impacts. However, our knowledge of the major drivers of drought, including the meteorological and the surface hydrological processes, is still limited and thus our ability to forecast the commencement and retreat of drought events is still low. Using two generations of Weather Research and Forecasting (WRF)-based regional climate models (named NSW and Australian Regional Climate Modelling project, iteration NARCliM1.0 and NARCliM1.5) downscaled from CMIP3 and CMIP5 global climate models respectively, three drought indices: the SPI (Standardised Precipitation Index), aSPI (agricultural SPI), and SPEI (Standardised Precipitation-Evapotranspiration or PET Index) are assessed for the Australian region. Evaluation results show that biases in simulated drought frequency vary among models, while consistency is observed in duration and intensity biases. However, simulated drought intensity is too low compared to observed data. Projections for 2060–2079 indicate an overall increase in drought frequency in Australia, but discrepancies exist between NARCliM1.0 and NARCliM1.5, leading to uncertainties. NARCliM1.5 consistently projects greater increases in duration and intensity across most regions compared to NARCliM1.0. Projections for the Australian wheatbelt align between the ensembles, providing higher confidence. Correlation analysis highlights precipitation's impact on drought duration and PET's role in drought intensity for coastal Australia.
AS72-A011
Increase in Ocean-onto-land Droughts and Their Drivers Under Anthropogenic Climate Change
Xihui GU#+, Yansong GUAN
China University of Geosciences
Ocean-onto-land droughts (OTLDs)—i.e., droughts originating over the oceans and migrating onto land—are a recently identified phenomenon with severe natural and human impacts. However, the influence of anthropogenic emissions on past and future changes in OTLDs and their underlying mechanisms remain unclear. Here, using precipitation-minus-evaporation deficits to identify global OTLDs, we find OTLDs have intensified due to anthropogenic climate change during the past 60 years. Under a future high-emissions scenario, the OTLDs would become more frequent (+39.68%), persistent (+54.25%), widespread (+448.92%), and severe (+612.78%) globally. Intensified OTLDs are associated with reduced moisture transport driven by subtropical anticyclones in the northern hemisphere and complex circulation patterns in the southern hemisphere. The reduction in moisture transport during OTLDs is mainly caused by the atmospheric thermodynamic responses to human-induced global warming. Our results underscore the importance of improving understanding of this type of drought and adopting climate mitigation measures.
AS72-A019
IOD Asymmetry in CMIP6- Origins of Biases and Increasing Negative Extremes Under Global Warming
Francis Chi Yung TAM1,2#+, Yiling ZHENG1, Kang XU3, Matthew COLLINS4
1The Chinese University of Hong Kong, 2Shenzhen Research Institute, 3Chinese Academy of Sciences, 4University of Exeter
The Indian Ocean dipole (IOD) is the dominant mode of interannual variability in the tropical Indian Ocean (TIO). Observed IOD events exhibit distinct amplitude asymmetry in relation to negative nonlinear dynamic heating (NDH). Nearly all models in CMIP5 simulate a less-skewed IOD than observed, but 6 out of 20 CMIP6 models can reproduce realistic high skewness. Analysis of less-skewed models indicates that the positive IOD-like biases in the mean state, which can be traced back to their weaker simulations of the preceding Indian summer monsoon, reduce the convective response to positive SSTA in western TIO, resulting in a weaker zonal wind response and weaker nonlinear zonal advection during positive IOD events. Besides, ocean stratification in the eastern TIO influences the IOD skewness: stronger stratification leads to larger mixed-layer temperature response to thermocline changes, contributing to larger anomalous vertical temperature gradient, larger nonlinear vertical advection thus stronger positive IOD skewness. The projections from CMIP6 SSP5-8.5 indicate a notable reduction in IOD asymmetry, which is linked to an increase in extreme negative IOD. Decrease in IOD asymmetry can be attributed to less negative NDH, mainly due to nonlinear zonal advection. Under global warming, enhanced atmospheric stability weakens response of equatorial easterlies to SSTA, leading to reduced nonlinear zonal advection. The amplified positive IOD-like warming pattern is likely to increase the convective response to positive SSTA in eastern TIO. Both factors favor the development of extreme negative IOD. As a consequence regions such as eastern Africa, southern India, and Sri Lanka are projected to experience more severe droughts. These changes underscore the potential risks posed by IOD events in a warming world, emphasizing the importance of understanding IOD changes for improved climate impact prediction and future preparedness.
AS72-A022
Understanding the 2022 Extreme Dragon-boat Rainfall in South China from the Combined Land and Oceanic Forcing
Ziqian WANG#+, Juan XU
Sun Yat-sen University
The most frequent and concentrated rainfall in the pre-flood season in South China usually occurs around the Dragon Boat Festival every year, locally known as ‘Dragon-boat Rainfall (DBR)’. In 2022, a record-breaking DBR attacked South China, causing disastrous flooding. We suggest that this extreme DBR was jointly regulated by the tropical convective forcing and Tibetan Plateau (TP) heating. Distinctly strong low-level southwesterlies and ascending motions over South China were the key atmospheric conditions. And the abnormal low-level southwesterlies were contributed by both the anomalous anticyclone over the western North Pacific and the anomalous westerlies at the southern side of the TP. On the one hand, during the period of 2022 DBR, stronger-than-normal convective forcing over the Maritime Continent induced the low-level anomalous anticyclone over the western North Pacific through triggering the meridional vertical circulation and further promoted the upward motions over South China. On the other hand, positive diabatic heating over the TP forced abnormal warm anticyclone in the mid-upper troposphere, more warm air advected downstream by the background westerlies, intensifying the upward motions over South China. Meanwhile, the TP heating could induce the anomalous low-level westerlies at the southern side of the TP, which further merged into and intensified the southwesterlies over South China and greatly enhanced the moisture transport and convergence there. Therefore, we highlight the strong thermal forcing over the TP, exerting a combined and amplified effect with the convective forcing over the Maritime Continent, dominated the record-breaking DBR in 2022.
AS72-A002
An Energetics Tale of the 2022 Mega-heatwave Over Central-eastern China
Tuantuan ZHANG1#+, Yi DENG2, Junwen CHEN3, Song YANG1, Yongjiu DAI1
1Sun Yat-sen University, 2Georgia Institute of Technology, 3Shenzhen Wiselec Technology Co. Ltd.
It remains a major challenge to attribute heatwave’s lifecycle characteristics quantitatively to interwoven atmospheric and surface actions. By constructing a process-resolving, energetics-based attribution framework, here we quantitatively delineate the lifecycle of the record-breaking 2022 mega-heatwave over central-eastern China from a local energetics perspective. It is found that the cloudlessness-induced radiative heating and atmospheric dynamics dominate the total energy buildup during the developing stage, while the land-atmosphere coupling and atmospheric horizontal advection act most effectively to sustain and terminate the heatwave, respectively. A reduction in anthropogenic aerosols provides a persistent positive contribution during the event, suggesting that pollution mitigation measures may actually increase the amplitudes of future heatwaves. With this framework, initial efforts are made to unravel culprits in a model’s sub-seasonal prediction of this mega-heatwave, demonstrating the framework’s potential for efficiently detecting the origins of climate extremes and quantitatively assessing the impacts of mitigation policies for sustainable development.
Session Chair(s): Tijian WANG, Nanjing University, Min XIE, Nanjing Normal University
AS75-A001
| Invited
The Mutual Interactions Among Ozone, Fine Particulate Matter, and Carbon Dioxide and Their Impact on Summer Monsoon Climate in East Asia
Tijian WANG#+
Nanjing University
Ozone (O3) and fine particulate matter (PM2.5) are the major air pollutants, and CO2 is a critical greenhouse gas in East Asia. They three are active species of radiation. Most importantly, both O3 and PM2.5 can interact with CO2 through the terrestrial ecosystem, thus having effects on the regional climate. To investigate the mutual interactions among O3, PM2.5, and CO2 on the East Asia summer monsoon climate, the coupling regional climate-chemistry-ecology model, RegCM-Chem-YIBs, was improved and applied. Two numerical experiments were performed with and without involving the interactions among the three species. The results showed that the interactions resulted in changes to surface PM2.5, O3, and CO2 of -6~-2 μg/m3, 4~6 μg/m3, and 3~5 ppm, respectively, in northern China. While in southern China, surface PM2.5, O3, and CO2 varied in the range of 2~4 μg/m3, 1~2 μg/m3, and -4~-2. Surface downward shortwave radiation flux (SWF) and longwave radiation flux (LWF) increased in northern China, whereas showed a decreasing trend in southern China. The lower atmosphere was warmed by 1~2 K in north China, enlarging the air temperature gradient between land and sea, inducing easterly and southerly winds at 850hpa in the region. On the contrary, surface cooling exhibited northerly wind anomalies in southern China. The results indicated that the mutual interactions among the three species significantly impact regional climate in East Asia. We argue that future simulations should consider the interactions to better predict air pollution and climate changes in the target region. This study could help to comprehensively understand the climate effects of the mutual interactions among O3, PM2.5, and CO2. The findings provide a scientific reference for the collaborative governance of regional climate and air pollution in East Asia.
AS75-A029
| Invited
Uneven Modifications on the Coastal Atmospheric Sulfur and Cloud Condensation Nuclei Along the Eastern China Seas by Shipping Fuel Transition
Yan ZHANG#+
Fudan University
Marine fuel combustion from shipping releases SO 2 and forms sulfate particles, which may alter low cloud characteristics. A series of strategies were implemented to control the sulfur content of ship fuel oil from 2018 to 2020, offering insights into the effects of the ship fuel oil transition on sulfur-related pollutants and the consequent cloud condensation nuclei (CCN) in the atmosphere. Compared to 2018 in the southeast China waters, shipping SO2 emission decreased by 78% in 2020, resulting in a 76% reduction in ship-related total sulfur concentration, and a decrease of 54% in CCN number concentration under supersaturation 0.2% (CCN0.2) contributed by shipping. The response of CCN0.2 to ship-related sulfate modification is more pronounced in pristine environment than polluted environment, highlighting the uneven changes in coastal CCN along the Eastern China Sea induced by the ship fuel policies. The study provides insights into the variations in coastal atmospheric sulfur-related pollutants and CCN in response to changes in ship fuel oil, prompting the need for further dynamic assessments of the climate effects resulting from potential shifts in ship fuel use in the future.
AS75-A002
| Invited
Land Use and Anthropogenic Heat Modulate Ozone by Meteorology: A Perspective from the Yangtze River Delta Region
Chenchao ZHAN1#+, Min XIE2
1Nanjing University of Information Science & Technology, 2Nanjing Normal University
In the YRD region. O3 pollution episodes are usually in calm conditions characterized by high temperature, low relative humidity, light wind and shallow cloud cover. In this case, land use and AH dictated by human activities significantly modify the urban climate and in turn O3 concentration. Urban expansion can cause an increase in T2 by a maximum of 3 ℃, an increase in PBLH by a maximum of 500 m, a decrease in WS10 by a maximum of 1.5 m/s and an increase in O3 by a maximum of 20 mg/m3. With regard to the sea and lake breezes, the expansion of coastal cities can enhance the sea breeze circulation by ~1 m/s. The expansion of lakeside cities can extend the lifetime of lake breezes from noon to afternoon. Since the offshore flow of the lake breeze transports high O3 from the land to the lake, the onshore flow brings high O3 back to the land. Surface O3 in lakeside cities can increase as much as 30 mg/m3. Compared to land use, the effects of AH are relatively small. The changes mainly appear in and around cities where AH fluxes are large. There are increases in T2, PBLH, WS10 and surface O3 when AH fluxes are taken into account, with increments of approximately 0.2 ℃, 75 m, 0.3 m s-1 and 4 µg m-3, respectively. AH contributes largely to the urban environment, altering meteorological factors, O3 concentration and urban breeze circulation, but its effect on the sea and the lake breezes seems to be limited.
AS75-A003
Relationships of Planetary Boundary Layer Height Variability Over Thailand to ENSO and AOD During Winter Season
Sirapong SOOKTAWEE1#+, Khwanruthai RENUHOM1, Siriwan KAEWKET2, Aduldech PATPAI2, Pramet KAEWMESRI3, Atsamon LIMSAKUL4
1Department of Climate Change and Environment, 2Ministry of Natural Resources and Environment, 3Geo-Informatics and Space Technology Development Agency, 4Environmental Research and Training Center
Climate variability affects various environmental issues. Thailand has been experiencing extreme climate events and air pollution. High concentration of PM2.5, related to aerosol optical depth (AOD), occurs during winter season. Air pollution weather is one of the climate-impact drivers that can enhance severity of atmospheric pollution. Planetary boundary layer height (PBLH) is the height of atmospheric layer where pollutants can be trapped in this layer, and how PBLH variability relates to pollution level in the atmosphere. To investigate the relationships of PBLH variability over Thailand to AOD and ENSO, the EOF and correlation analyses were carried out each month during the winter season (December-February). ERA5 data of 30 years (1991-2020) has been analyzed to present PBLH variability. ENSO indices and VIIRS-AOD data were used to investigate relationships of PBLH to their variations. Leading EOF mode of PBLH for December, January, and February explains 38%, 30%, and 30% of variance, respectively. For the 2nd mode are of 24%, 19%, and 18% for corresponding months, and the 3rd mode are of 7%, 11%, and 14%, respectively. It is worth noting that significant correlations between the 2nd ,3rd, and 2nd modes of December, January, and February to ENSO indices were observed. Relationships of the 2nd ,3rd, and 2nd PCs to AOD show that the increase of PC amplitude is related to increasing of PBLH with reduction of AOD over upper and Northeast regions of Thailand, and vice versa for PC amplitude decreasing. Investigation of this study suggests the ENSO phenomenon correlated to a part of PBLH variability during December-February, and the variation of PBLH over Thailand results in a change of AOD representing PM2.5 level in the atmosphere. Therefore, PBLH variability plays an indirect role in the changing of atmospheric pollution level that required further study to give more understanding in underlying mechanism.
AS75-A022
Atmospheric Circulation Anomalies Related to the Winter PM2.5 Mass Concentration Rapid Decline Cases in Beijing
Yuanliurui REN1+, Wei CHEN2#, Riyu LU2
1Institute of Atmospheric Physics, Chinese Academy of Sciences, 2Chinese Academy of Sciences
In this study, we investigate the atmospheric circulation anomalies related to the PM2.5 mass concentration rapid decline cases in Beijing during winter when the PM2.5 concentration is the greatest. From 2014 to 2021, 66 PM2.5 concentration rapid decline days (RDDs) are identified by considering the 90 % thresholds of the difference of PM2.5 mass concentration between two adjacent days. The composite evolution of PM2.5 mass concentration for rapid decline cases features with a slow increase on the accumulation phase but a rapid decrease on RDDs. The composite evolution of atmospheric circulation anomalies in the lower-troposphere related to these PM2.5 concentration rapid decline cases exhibits a southerly-to-northerly reverse of wind anomalies induced by the eastward shift of cyclonic/anticyclonic geopotential height anomalies from the Kara Sea/East Asia to the Japan Sea/western Pacific. The mid-tropospheric circulation anomalies are characterized by an eastward propagation of the wave-train-like “+−+” pattern, corresponding to the lower-troposphere systems, which together promote the southerly-to-northerly reverse process. Meteorological factors in the planetary boundary layer including temperature, humidity, and boundary layer height also show anomalous warm-to-cold, wet-to-dry, and low-to-high reverse around RDDs, respectively. The results imply that the atmospheric circulation patterns above could be a precursor to the PM2.5 mass concentration rapid decline cases in Beijing.
AS75-A009
Effects of Emission Reductions on Major Anthropogenic Aerosol-radiation-cloud Interactions in East Asia in Winter During 2007-2020
Yaxin HU+, Bingliang ZHUANG#, Yinan ZHOU, Peng GAO, Heng CAO, Shanrong LIANG
Nanjing University
East Asia (EA) has always been a highly concern region for human-induced climate change. In this study, a well-developed regional model RegCM4 is employed to investigate the influences of major anthropogenic aerosol (MAA, including sulfate and primary carbonaceous aerosols) variations from 2007 to 2020 on East Asian climates in winter. Results indicate that high MAA loadings in EA in winter mainly appear in Central to Eastern China. In most area of Asia (5°-55°N, 70°-140°E), the multi-year (2007~2020) mean instantaneous direct and total effective radiative forcing (IDRF and ERF) induced by MAAs are -4.22 and -3.90 W/m2 at the surface in winter, which are 2.29 and 1.96 times of those at the tropopause. In polluted area from southwest to center China (SWCC, 27-33 oN, 102-115 oE), these forcings are much stronger, which causes a dimmer, cooler and drier surface and further stabilizes the lower atmosphere. The multi-year mean sunshine duration, surface air temperature, precipitation, and boundary layer thickness are changed by -20.32 min/day, -0.33 K, -0.08 mm/day, and -12.51 m, respectively in SWCC in winter. Both the aerosol surface IDRF and ERF are weakened by above 30% in SWCC in winter since the Action Plan for Air Pollution Prevention and Control was carried out, which results in less surface dimming and cooling by 9.4 min/day and 0.23 K, respectively. During the most outbreak period in COVID-19 epidemic, the aerosol surface IDRF is weakened by approximately 46.87% compared to that before 2013 in SWCC, which may offset the aerosol cooling effect by 0.28 K.
Session Chair(s): Ning ZHANG, Nanjing University, Dan LI, Boston University
AS91-A013
| Invited
Modelling Extreme Weather and Associated Anthropogenic Influences Over the Urbanized South China Greater Bay Area
Francis Chi Yung TAM1,2#+, Chenxi HU1, Jilong CHEN3, Rui ZHAO4, Chung Shing LAU1, Chi Chiu CHEUNG5, Wei Pang SZE5
1The Chinese University of Hong Kong, 2Shenzhen Research Institute, 3Shenzhen Institute of Meteorological Innovation, 4Fujian Institute of Meteorological Science, 5ClusterTech Limited
We review some recent studies using models to investigate human-induced alterations of extreme weather over East Asiancoastal mega-cities, particularly focusing on the Greater Bay Area (GBA) in South China. Many of these use the pseudo-global warming method and superimpose CMIP climate signals onto historical extreme cases for either attribution purposes or future projections. By running WRF at a convection-resolving resolution for 40 GBA rainfall events, the attribution analysis by Zhao et al. finds an 8-9.5% (12.4%) increase in summertime (non-summer) extreme daily rainfall, attributable to each degree K of surface warming due to human activities. Particularly noteworthy is the super-CC scaling in non-summer seasons, which is linked to intensified low-level wind convergence and updrafts. Chen et al., by simulating 20 tropical cyclones (TC) making landfall within GBA, reported an averaged landfall intensity increase by ~12% in 2075-2099, according to RCP8.5. Hu et al. compared the near future (2030) climate vs urban change impacts on 30 GBA extreme rainfall cases; it is reported that these forcing factors have comparable positive influences, with accumulated urban rainfall enhanced by ~ 13.5% and 9.7%, respectively. Precipitation changes attributable to urban development are primarily concentrated in highly urbanized areas, whereas global warming affects the entire area. We also examine a 2007 GBA heatwave in relation to a nearby TC, and its response to varying urban land cover and climatic conditions. A substantially exacerbated heatwave results from the dual forcing of urbanization and global warming, particularly impacting the daily minimum temperatures. Urbanization considerably bolsters, while climate change undermines sea breezes during the day within the megacity. Finally, we introduce briefly on-going development using a global customizable unstructured model based on NCAR’s Model for Prediction Across Scales - Atmosphere (MPAS-A), called CPAS, and its use on urban climate and extreme research.
AS91-A001
Contribution of Changes in Temperature Mean, Variability and Persistence to Heat Wave Occurrence in Urban Environments
Dan LI1#+, Weilin LIAO2
1Boston University, 2Sun Yat-sen University
While it is well-known that urban temperatures are often higher than temperatures of the rural surroundings (namely, urban and rural temperatures have different mean values, a phenomenon nowadays called the urban heat island effect), it remains unclear whether urban and rural temperatures exhibit any significant differences in terms of variability and persistence. Moreover, whether urban-rural differences in temperature variability and persistence, if exist, contribute to more hot days and heat waves in urban areas has not been investigated. In this study, we aim to address these two questions using a combination of numerical modeling and experimental data, with a focus on the summer season and the daily scale. Our results show that the urban and rural temperatures exhibit large difference in the seasonal mean (as expected) but nearly no difference in the variability, with some difference in the persistence in certain regions. The seasonal mean urban heat island effect (i.e., the higher mean urban temperature) contributes to more heat wave occurrence in urban areas, but such impact is strongly modulated by the summer temperature variability. The urban-rural difference in temperature persistence makes a generally small contribution to the urban-rural difference of heat wave occurrence, with strong regional variabilities. Overall, the urban-rural difference of heat wave occurrence is to a large extent induced by the seasonal mean urban heat island effect.
AS91-A015
Enhancing Urban Air Temperature Forecast with City-scale Graph Neural Networks
Han WANG+, Jiachuan YANG#
The Hong Kong University of Science and Technology
Air temperature (Ta) forecast in urban environments is crucial for human well-being and is thus of great importance for various socio-economic activities. This study proposes a novel deep learning framework that integrates graph neural networks (GNNs) and long short-term memory (LSTM) models to effectively capture the evolution of Ta dynamics within a highly heterogeneous city, Hong Kong. Combining the deep ensemble technique, which fuses models with diverse structures, our framework outperforms traditional LSTM models by over 10% in forecasting Ta for the subsequent six hours during the test year 2021. Notably, the new GNN framework exhibits a remarkable capability in catching rapid, short-term extreme weather variations. Further analysis highlights the importance of incorporating multiple meteorological variables, particularly wind information, to enhance Ta forecast. This study proves the efficacy of GNNs in predicting atmospheric variables at the city scale and paves the way for future advancements in data-driven weather forecasting systems.
AS91-A016
Interaction Between Urban Heat Island and Temporally Compound Heat Waves
Jiachuan YANG#+
The Hong Kong University of Science and Technology
Heat waves (HWs) are extreme climate hazards to human society. Urban areas are the major habitat for human beings today and tend to experience more severe heat stress under HWs than rural areas due to the urban heat island (UHI) effect. Under the changing climate, temporally compound heat waves (CHWs), multiple HWs occurring in sequence with cool breaks between them, will disproportionately increase. Urban heat risk assessment must consider the added vulnerability caused by the compounding of HWs, which remains largely unexplored in the literature. Using ground-based meteorological observations from 1960 to 2017, we investigated the trend of CHWs over China. During the past 50 years, the ratio of CHWs has significantly increased across China. Results reveal consistent increase in the frequency and magnitude of CHWs over urban regions at a continental scale. The intensification of UHI is more evident during CHWs than simple HWs. The findings provide useful guidance for landscape design and planning to create cool cities and neighborhoods.
AS91-A022
Development of Human Heat Balance Model for Heat Stroke Risk Assessment
Makoto NAKAYOSHI#+, Kanta SUSAKI
Tokyo University of Science
The incidence of heatstroke patients has been on the rise in Japan, attributable to global warming and urban heat island effects. The Wet Bulb Globe Temperature (WBGT) is a widely utilized metric in Japan for heat risk assessment and since 2021, a heatstroke risk alert is issued when the WBGT is forecasted to exceed 33°C. While WBGT sensors are cost-effective and monitoring it is straightforward, this method presents significant limitations in assessing heatstroke risk. Heatstroke risk is multifactorial; it is influenced by 5 weather elements, or air temperature, humidity, wind speed, shortwave and longwave radiation, as well as individual human conditions (clothes and activity levels, etc) and attributes (age, sex, and body shape, etc). Unfortunately, WBGT does not account for these variables, leading to a uniform risk assessment across diverse groups, from children to the elderly and from active individuals to those at rest. The human heat balance model, which parameterizes the thermoregulatory functions of the human body, is a promising tool for evaluating individual heatstroke risk. This model integrates both weather and human parameters, offering a more personalized heat risk assessment. Heatstroke is a condition characterized by an abnormal rise in core body temperature; therefore, a model that can accurately predict core body temperature is in high demand. We have developed such a model and validated its accuracy with data obtained from outdoor thermal physiology experiments. Our model outperformed previous models for accurate reproducing both core body and average skin temperature. The details of our model and its performance will be presented at AOGS 2024.
Session Chair(s): Jianping TANG, Nanjing University
AS65-A012
| Invited
Projected Changes in Köppen-Trewartha Climate Zones Under 1.5–4°C Global Warming Targets Over Mid-high Latitudes of Northern Asia Using an Ensemble of RegCM4 Simulations
Xuejie GAO1#+, Jie WU2
1Chinese Academy of Sciences, 2Gannan Normal University
We use an ensemble of a regional climate model (RegCM4) projections to assess future changes in surface air temperature, precipitation and Köppen-Trewartha (K-T) climate types in mid-high latitude Northern Asia (NA) under the 1.5-4°C global warming targets. RegCM4 is driven by five CMIP5 global models over an East Asia domain at a grid spacing of 25 km. Validation of the present day (1986-2005) simulations shows that the ensembles of RegCM4 (ensR) and driving GCMs (ensG) reproduce the major characters of the observed temperature, precipitation and K-T climate zones reasonably well. Greater and more realistic spatial detail is found in RegCM4 compared to the driving GCMs. A general warming and overall increases in precipitation are projected over the region, with these changes being more pronounced at higher warming levels. The projected warming by ensR shows different spatial patterns, and is in general lower, compared to ensG in most months of the year, while the percentage increases of precipitation are maximum during the cold months. The future changes in K-T climate zones are characterized by a substantial expansion of Dc (temperature oceanic) and retreat of Ec (sub-arctic continental) over the region, reaching ~20% under the 4°C warming level. The most significant change in climate types in ensR is found over Japan (~60%), followed by Southern Siberia, Mongolia, and the Korea Peninsula (~40%). The largest change in the K-T climate types is found when increasing from 2°C to 3°C.
AS65-A025
Uncertainty Factors in Mean and Extreme Precipitation Projections Over East Asia
Ana JUZBASIC1#+, Changyong PARK1, Dong-Hyun CHA1, Joong-Bae AHN2, Eun-Chul CHANG3, Seung-Ki MIN4, Youngeun CHOI5, Young-Hwa BYUN6
1Ulsan National Institute of Science and Technology, 2Pusan National University, 3Kongju National University, 4Pohang University of Science and Technology, 5Konkuk University, 6National Institute of Meteorological Sciences
Extreme precipitation events have been increasing worldwide, attributable to global climate change. Because of the potential damage such events can cause to property, human lives, and ecosystems in affected areas, giving policymakers accurate model predictions is of utmost importance. However, all model projections come with some inherent uncertainties. The sources of this uncertainty can be roughly separated into three parts – internal variability of the system, model uncertainty, and scenario uncertainty. The present study used the CORDEX East Asia modeled data from fifteen global climate model (GCM) – regional climate model (RCM) chains to attempt to distinguish the impacts of the different sources of the uncertainty, as well as to compare the differences in uncertainties between mean and extreme event projections in East Asia. The indices used were mean boreal summer precipitation, simple precipitation intensity index (SDII), maximum cumulative 5-day (Rx5d), and maximum daily precipitation (Rx1d). The mean precipitation was not projected to experience significant change regardless of the scenario, but more extreme indices are projected to increase by the end of the century, especially in the RCP8.5/SSP5-8.5 scenario, with Rx1d experiencing the most significant increase. In the near future, internal variability and model uncertainty were the largest contributors to the total uncertainty, with their contribution in the 2030s being similar. By the mid-century, model uncertainty was shown to be the main uncertainty contributor for most indices in most areas of the domain. Additionally, while the scenario uncertainty accounts for a negligible part of variability for the average precipitation, for more extreme precipitation indices, the contribution of the scenario uncertainty is more prominent, reaching over 50% of the total uncertainty of Rx1d in some parts of the domain by the end of the century.
AS65-A018
Impact of Extreme Temperature on Future Photovoltaic Potential Over East Asia
Changyong PARK#+, Ana JUZBASIC, Dong-Hyun CHA
Ulsan National Institute of Science and Technology
East Asia is a highly industrialized region with high CO2 emissions from extensive fossil fuel use. Therefore, to achieve the goal of the Paris Agreement on CO2 reduction, an increase in the production of renewable energy, such as photovoltaic (PV) power, is required in this region. Most renewable energy production is directly affected by weather and climate. This study conducted an impact of extreme temperature on future PV potential (PVpot) over East Asia using the ERA5 datasets, and high-resolution multiple regional climate models participating in the CORDEX-East Asia phase Ⅱ project. According to a previous study (Park et al., 2022), it was suggested that the widespread increase in near-surface air temperature would be a major factor in the future decrease of PVpot in East Asia. Based on the results presented in the previous study, this study sought to determine the impact of extreme temperatures due to differences in warming levels on the future PVpot over East Asia. The results of this study will help to develop policies for efficient future production of renewable energy over East Asia by presenting the projection of future PV power generation on a detailed regional scale.
AS65-A019
Future Projection of Extreme Heat Stress Characteristics in East Asia Based on the SSP Scenarios
Yujin KIM1+, Seung-Ki MIN1#, Yeon-Hee KIM1, Eun-Soon IM2
1Pohang University of Science and Technology, 2The Hong Kong University of Science and Technology
This study examines future changes in the spatiotemporal characteristics of extreme heat stress over East Asia based on the Wet Bulb Globe Temperature (WBGT), using multiple Regional Climate Model (RCM) simulations from the CORDEX East Asia Phase II under Shared Socioeconomic Pathways (SSP) scenarios. The summer mean WBGT in East Asia is projected to increase by 3.2°C (SSP1-2.6) to 7.6°C (SSP5-8.5) compared to the current period (1979-2014) in the late 21st century (2081-2100). While most of the changes in heat stress are explained by temperature increases, changes in relative humidity are found to enhance or alleviate heat stress depending on the region and scenario. Relative humidity decreases over many regions, slightly offsetting the summer mean WBGT increases (up to -6%), while it increases in northeastern and northern China, intensifying WBGT increases (up to +14%). The contribution of humidity to WBGT changes is more pronounced during extreme WBGT days (summer top 5%) and is more evident in low-emission scenarios. To understand extreme heat stress at the regional scale, we analyzed extreme heat stress days (EHDs), defined as days when WBGT exceeds its 95th percentile threshold over more than 10% of the area for each sub-region. According to the high-emission scenario, EHDs in all sub-regions are expected to be ten times more frequent in the late 21st century than at present. The intensity and spatial extent of EHDs are also expected to increase, leading to a significant impact throughout East Asia. Moreover, in the late 21st century, it is predicted that EHDs lasting 80 days or longer will occur in all sub-regions, and most East Asia regions will be affected by severe heat stress throughout the entire summer season.
AS65-A035
SSP-RCP Scenario Based Future Land Use Change Projection Over Ethiopia
Ermias Sisay BRHANE#+, Koji DAIRAKU
University of Tsukuba
Land use land cover (LULC) data are essential for modeling various environmental conditions. Access to high-resolution LULC products at a global and regional scale for public use has been challenging, particularly in developing countries. LULC simulation models are a powerful tool for analyzing the causes and effects of LULC dynamics under different scenarios. Scenario-based simulation can provide valuable information for evaluating the impacts of land strategies under different conditions. In this study, we projected future land use data at a 1-km resolution, comprising six land use types, using the newest integrated scenarios of the Shared Socioeconomic Pathways and the Representative Concentration Pathways (SSPs-RCPs) over Ethiopia. We used the Future Land Use Simulation (FLUS) model to project future land-use dynamics. The development of a future land dataset for Ethiopia can be divided into two parts. Firstly, estimating land use demands for different land use types under different SSP-RCP scenarios extracted from the LUH2 (Land-Use Harmonization 2) datasets. This dataset includes a global projection of multiple land types for successive years. The second part involves conducting a 1 km spatial land simulation using the future land use simulation (FLUS) model under the macro constraints of the demands. Relevant spatial driving factors, such as socioeconomic, distance, and natural factors, are selected. Based on this, a new set of land use projections is produced, with a temporal resolution of 10 years and a spatial resolution of 1km, in eight SSP-RCP scenarios, comprising six land use types in Ethiopia. This dataset demonstrates good performance in comparison to the remotely sensed ESA CCI-LC data. Our land use simulation results indicate satisfactory accuracy with a Kappa value of 0.8, OA of 0.9, and FoM of 0.1. The dataset offers advantages such as fine resolution, current scenarios, and multiple land types.
AS65-A022
Assessing the Impact of Anthropogenic Climate Change on Marine Heatwave Near the Korean Peninsula Using the WRF-ROMS Regional Coupled Model
Young Hyun KIM#+, TaeHun KANG, Woojin CHO, Dong-Hyun CHA
Ulsan National Institute of Science and Technology
According to the Special Report on Ocean and Cryosphere in a Change Climate (SROCC), the frequency of anomalous high sea surface temperatures has more than doubled globally since the 1980s, and the frequency and intensity of marine heatwaves are expected to increase with global warming. Recently, marine heatwaves, lasting from several days to weeks, have become more frequent near the Korean Peninsula. As it is crucial to improve our understanding of the anthropogenic influence on marine heatwaves with ongoing climate change, we aim to investigate the impact of human activities on the occurrence of marine heatwaves near the Korean Peninsula quantitatively. For this purpose, the pseudo-NAT experiment, an approach similar to the pseudo-global warming method, is conducted using the historical (all forcing) and hist-nat (natural forcing only) simulation over the period 1985-2014 from the Coupled Model Intercomparison Project Phase 6 (CMIP6). In the pseudo-NAT experiment, the impact of anthropogenic forcing, the difference between two simulations (historical minus hist-nat), is subtracted from the reanalysis data and that is used as initial and boundary conditions for the Weather Research and Forecasting (WRF) and Regional Ocean Modeling System (ROMS) regional coupled models. The model performance for sea surface temperature has been investigated using a control (CTL) experiment, which is conducted using the Final analysis (FNL) data from the National Centers for Environmental Prediction (NCEP) and HYbrid Coordinate Ocean Model (HYCOM) data as initial and boundary conditions for the WRF and ROMS regional coupled models. Although the WRF-ROMS coupled regional climate model tends to underestimate sea surface temperature, the biases are not significant near the Korean Peninsula, indicating that the models simulate the sea surface temperature well. By comparing the pseudo-NAT and CTL experiments, we confirm that sea surface temperatures with anthropogenic forcing were higher than those without.
Session Chair(s): Kai YANG, Institute of Mountain Hazards and Environment, Chinese Academy of Sciences
AS23-A004
| Invited
Hemispheric Asymmetry of Land-sea Distribution Causes Asynchronous Global Atmospheric Energy Response to Solar Forcing
Yuhui HAN1#+, Zhenning LI2, Ming CAI3, Song YANG1, Xiaoming HU1
1Sun Yat-sen University, 2The Hong Kong University of Science and Technology, 3Florida State University
Largely owing to the presence of oceans, seasonal variations of temperatures do not follow the seasonal variation of solar forcing. Here, we present observational and modeling evidence suggesting a more pronounced temporal misalignment of the annual cycle of global mean atmospheric energy with an approximately 6-month lag compared to eccentricity-driven seasonal solar forcing. Furthermore, despite the stronger eccentricity-driven seasonal solar forcing in the Southern Hemisphere, the seasonal cycle of hemispheric mean atmospheric energy exhibits a greater amplitude in the Northern Hemisphere. Given the distinct heat capacities of land and ocean, we propose a hypothesis attributing this asynchrony to the differing land-ocean distribution between the two hemispheres. To scrutinize this hypothesis, we conduct a fully coupled experiment without land-sea contrast using the Community Earth System Model, eliminating the asynchronous response of global mean atmospheric energy to eccentricity-driven solar forcing. The asynchronous response of global mean atmospheric energy to eccentricity-driven solar forcing is readily reproduced in a simple, idealized 4-box dry radiative-convective climate model, provided it incorporates hemispheric asymmetry in land-sea distribution. This clear demonstration underscores the pivotal role of hemispheric asymmetry in land-sea distribution in shaping the annual cycle of global mean atmospheric energy and serves to further validate our hypothesis.
AS23-A005
| Invited
Warming-and-Wetting Trend Over the China’s Drylands: Observational Evidence and Future Projection
Boyang LI1#+, Dongwei LIU1, Entao YU2, Lixin WANG1
1Inner Mongolia University, 2Chinese Academy of Sciences
A recent significant transition from “warming-and-drying” to “warming-and-wetting” trend over China’s drylands raised widespread attention in the scientific community. Based on observations and model projections, this study indicates the warming and regional wetting trend in China’s drylands is getting stronger. Over the past 60 years, the temperature in China's drylands has increased at a rate of 0.34 °C/10a, much higher than in China (0.29 °C/10a) and globally (0.22 °C/10a). Model projections show stronger warming in the future under both RCP2.6 and RCP8.5 scenarios. Regional increase of precipitation in the past 60 years was found in this study. The wetting trend has been primarily apparent in the western part since the 1980s, particularly in the mountainous areas. In the northeast edge of the Qinghai-Tibet Plateau, the wetting rate exceeded 30 mm/10a. The possible cause of the increase of precipitation in China's drylands may be the higher convective precipitation, also concentrating in mountainous areas. Precipitation will increase slightly in the mid-21st century and then slowly decrease until the end of the 21st century under RCP2.6 scenario. In comparison, under RCP8.5 scenario, it will increase by 15-25% at the end of the 21st century. Considering the decrease of relative humidity in the past decade over most regions in China’s drylands and the decreasing trend presented by CMIP5 and CMIP6 projections, the wetting trend may be weaker in the future. The possible impacts of warming and humidification trends should be given high priority. Though the trend may positively affect the vegetation growth in the short term, in the long run there will be significant challenges in eco-construction and engineering as well as amounts of secondary impacts due to environmental changes.
AS23-A017
| Invited
Characteristics of Ground Surface Heat Flux for Alpine Vegetation in Freeze-thaw Cycles in the Three River Source Region
Siqiong LUO#+, Jingyuan WANG
Chinese Academy of Sciences
Ground surface heat flux is a key component of surface energy flux and serves as a reliable parameter for assessing shallow geothermal energy. Using the observations from four sites and a novel method, we investigated the daily, monthly, and diurnal characteristics of ground surface heat flux across various types of land cover in the Three River Source Region. The contribution of soil heat flux at 5 cm or 7.5 cm to ground surface heat flux was found to be only between 1/2 and 2/3, with the remaining portion being attributed to changes in heat storage of soil and liquid water , heat storage of soil ice and latent heat of ice phase change. The characteristics of ground surface heat flux exhibited significant variations in response to different land-covered vegetation during daily, monthly, and diurnal cycles, as well as two freeze-thaw stages. The alpine marsh-covered soil had the largest annual amplitude in ground surface heat flux on both daily and monthly averages but showed the smallest diurnal amplitude in ground surface heat flux. In the frozen stage, ground surface heat flux played a significant role as a supplement to net radiation in TRSR, particularly in the alpine marsh region where it accounted for approximately −22 % to −80 % of Rn from November to February.
AS23-A024
| Invited
The Leading Modes of Wind Field Variability Over the Western Tibet Plateau and Its Impact on Snow Cover
Jingzhi WANG#+, Xiaofeng LI
Sun Yat-sen University
Snow cover (SC) variability is of great importance to the hydrological cycle centering at the western Tibetan Plateau (TP), as the snow melted water supplies millions of lives in the mid-west and mid-south Asian countries. It is supposed to be modulated significantly by the above atmospheric circulation variability that is the only media brings moisture from above the ocean to high mountains on the western TP. However, the dominate circulation or wind variability over the Western TP and its possible influences on the snow cover is still unclear. This study thereby is conducted to examine the primary modes of the wind fields and its impacts on SC over the western TP. We find the first leading mode of the combined zonal and meridional wind field in annual mean and in most seasons (spring, summer and autumn) over the western TP show high similarity to the Western Tibetan Vortex (WTV), a large-scale atmospheric vortex-like pattern recently recognized over the western TP. The cyclonic (anticyclonic) WTV causes moisture convergence (divergence) and upward (downward) motions over the western TP, resulting in more (less) SC over the western TP in spring season, accounting for up to 30% SC’s variance. In short, the WTV generally represents the first leading mode of the wind field in most seasons over the western TP and significantly modulates the SC above it. This study augments our knowledge of the wind variability and hydrological cycle over the western TP.
AS23-A002
Precipitation Anomaly Over the Tibetan Plateau Affected by Tropical Sea-surface Temperatures and Mid-latitude Atmospheric Circulation in September
Ping ZHANG+, Anmin DUAN#
Chinese Academy of Sciences
Tibetan Plateau (TP) precipitation is affected by anomalous circulation systems in both the tropics and mid-latitudes, due to the TP’s unique geographical location. By using observational, reanalysis, and CMIP6 model datasets, this study reveals the individual and joint effects of the Indian Ocean Dipole (IOD) and Silk Road pattern (SRP) on the interannual variability of TP precipitation in September. In the positive IOD phase, the zonal gradient of the sea-surface temperature anomalies (SSTAs) drives a Gill-type response with an anticyclonic anomaly over the Indian subcontinent and Bay of Bengal. To the north, anomalous westerlies induce a shallow trough, and the associated anomalous southwesterlies transport moisture to the southeastern TP, resulting in surplus precipitation there. Meanwhile, the westerly jet disturbances over the North Atlantic excite an SRP-like pattern, resulting in a baroclinic structure in northern India with the upper (lower) tropospheric anomalous anticyclone (cyclone) over west-central Asia (northern India). The anomalous southwesterlies to the east of the low-level cyclone transport abundant moisture to the southeastern TP, which results in increased precipitation there. The joint effects of IOD and SRP can explain nearly 52% of the TP precipitation anomaly, exceeding the contribution of IOD (19%) and SRP (27%) alone. Our results highlight the necessity of considering the joint effects of drivers in the tropics and mid-latitudes, providing a basis for more accurate simulations and predictions of TP precipitation.
Session Chair(s): Bolei YANG, Nanjing University
AS77-A007
| Invited
Moisture Convection and Tropical Intraseasonal Oscillations
Shuguang WANG#+
Nanjing University
Interaction between convection and circulation is considered pivotal for the emergence and propagation of slow moving tropical intraseasonal modes, including the Madden Julian Oscillation and Boreal Summer Intraseasonal Oscillation. Here, we discuss the crucial role of moisture as the primary driver of the convection-circulation interaction within the framework of moisture mode theory. Sufficiently amount of moisture in the troposphere is imperative for convection. Both the zonal advection of moisture and wind-induced evaporative feedback can be considered dynamically equivalent mechanisms facilitating the progression of intraseasonal modes. These different moist processes are encapsulated into a prognostic equation of moisture. A simple model is further employed to elucidate essential moisture processes governing the dynamics of the tropical intraseasonal modes.
AS77-A001
| Invited
Environmental Conditions Affecting Global Mesoscale Convective System Occurrence
Mark MUETZELFELDT1#+, Robert PLANT1, Hannah CHRISTENSEN2, Zhixiao ZHANG2, Tim WOOLLINGS2, Zhe FENG3, Puxi LI4
1University of Reading, 2University of Oxford, 3Pacific Northwest National Laboratory, 4China Meteorological Administration
The environments of global tracked mesoscale convective systems (MCSs) are assessed over a 20-year period. By assessing the precursor conditions for MCSs and likelihood of MCS occurrence for a given environment, we aim to provide useful information for the assessment and parametrization of MCSs in global atmospheric models. The analysis is performed in two ways, each providing different insights into the environmental conditions that occur before and during MCS occurrence. In the first, environmental conditions up to 24 h before MCS formation, and following MCS track locations after their formation, are investigated at different spatial scales. Different environmental variables are found to show marked increases before MCS initiation, such as CAPE, total column water vapour (TCWV) and mid-level relative humidity, particularly over land. One variable, the vertically integrated moisture flux convergence, shows a robust signal across different regions and even when the diurnal cycle is considered. When the analysis is performed at different spatial scales, a scale break between 200 and 500 km is found, indicating that scales below the break are more important for MCS formation, and providing evidence of a natural length scale for MCS parametrization. In the second analysis, the likelihood of MCS occurrence for a given environmental condition is evaluated, by considering the environments under which different regions (MCS core and shield) occur over the course of all MCS lifetimes. These are compared to regions (non-MCS core and shield) which meet similar criteria but are not part of tracked MCSs. Several environmental variables are found to have useful predictive value for MCS occurrence, including TCWV, relative humidity and equivalent potential temperature. Such relations could be used as triggering conditions for parametrization of MCS effects.
AS77-A002
| Invited
Impact of Global Warming on Mid-latitude Summertime Mesoscale Convective Systems: A Simple Lagrangian Parcel Model Perspective
Qiu YANG1#+, L. Ruby LEUNG2, Zhe FENG2, Xingchao CHEN3
1Peking University, 2Pacific Northwest National Laboratory, 3The Pennsylvania State University
Mesoscale convective systems (MCSs) are the dominant rainfall producer in the U.S. during the warm season, causing natural disasters and severe weather every year. Global climate models have large uncertainty in projecting precipitation changes in the future climate. Here we developed a simple Lagrangian parcel model (includes single- and multi-column models) to investigate the impact of global warming on MCS initiation and growth. The single-column parcel model projects a mean precipitation decrease over the central U.S. and an increase to its east, in agreement with the CMIP5 model projection. It also highlights the crucial role of current climate mean state model bias in influencing future mean precipitation projection. As for convective population, the model captures the decreased occurrence frequency of weak to moderate convection and increased frequency of strong convection due to the increased CAPE and CIN, in agreement with convection-permitting regional simulations. The multi-column parcel model captures readily the cold pool-induced upscale growth feature. It simulates smaller mesoscale clusters over the central U.S. under global warming due to gust front slowdown and subsidence strength enhancement. The model should be a useful tool for investigating the impact of global warming on MCS at mid-latitudes and providing useful guidelines to improve GCM simulations.
AS77-A003
Non-instantaneous Convection-convergence Feedback for Convective Organization in the Tropics
Yan LIU1#+, Zhe-Min TAN1, Zhaohua WU2
1Nanjing University, 2Florida State University
Non-instantaneous Convection-Convergence Feedback (NiCCF) is proposed to explain convective organization in the tropics. Convective response time scale (τ) is defined as the time lag between moisture convergence and convective heating. There are two main phases related to the processes of convective response: shallow convection development and shallow-to-deep convection transition. They are controlled by synoptic-scale boundary layer moisture convergence (M) and lower-tropospheric specific humidity (qm). In the first phase, as qm is small and lags the development of shallow convection, shallow convection occurrence is solely dominated by M (given suitable thermodynamic conditions in the boundary layer). In the second phase, shallow convection further preconditions the atmosphere for shallow-to-deep convection transition by sustaining M and qm through NiCCF, i.e., shallow convection drives large-scale circulation that enhances moisture convergence and upward moisture transport. Additionally, eddy moisture upward transport by shallow convection itself also contributes to an increase of qm. NiCCF is used to explain the propagation and hierarchy structure of super clusters, the diversity of MJO propagation, and convective self-aggregation.
AS77-A004
Microphysical Characteristics of Typhoon Choiwan (2021) Outer Rainbands Derived from Polarimetric Radar Observations at a Research Vessel
Shimin YANG#+, Yu DU
Sun Yat-sen University
Typhoon outer rainbands are important convective systems on the periphery of a typhoon. In the present study, we utilized dual-polarization observations from a C-band ship-borne doppler radar mounted on the Research Vessel Tan Kah Kee to investigate the microphysical characteristics of an outer rainband of Typhoon Choiwan (2021). The observations were conducted during its evolution on the ocean from 0500 UTC to 1300 UTC on June 03, 2021. The eight-hour period is subdivided into three stages: developing, mature and decaying, based on the convection intensity. Distinct microphysical features are identified during each stage. During the mature stage, both ice-phase processes and warm rain processes are active, leading to the coexistence of a small number of exceptionally large drops and high concentrations of smaller drops. The convective cells (CCs) during the mature stage exhibit a raindrop size distribution (DSD) characteristic that falls between “continental-like” (higher raindrop diameter and lower raindrop concentration) and “maritime-like” (lower raindrop diameter and higher raindrop concentration). In the developing and decaying stages, ice-phase processes predominantly govern the growth of raindrops, and both CCs display a “continental-like” DSD characteristic. Furthermore, during the decaying stage, warm rain processes play significant roles in producing raindrops at lower levels. This comprehensive analysis enhances our understanding of the microphysical complexities within Typhoon Choiwan's outer rainbands, providing valuable insights into their evolution and behavior during different stages of convection intensity.
AS77-A008
Moist Halo Region Around Shallow Cumulus Clouds in Large Eddy Simulations
Jian-Feng GU1#+, Robert PLANT2, Chris HOLLOWAY2, Peter CLARK2
1Nanjing University, 2University of Reading
The halo region, immediately outside a cloud, is moister than the air further from the cloud and is distinct from cloud shell in which the downward motions dominate. The moist halo region is critical for the interplay between the cloud and the large-scale environment and also has non-negligible impact on radiation. Previous studies found large uncertainties in estimated halo size and suggested a dependency of halo size on cloud size. However, these used relatively coarse resolution simulations or limited samplings from observations. In this study, the moist buffering halo region of shallow maritime cumulus clouds is systematically investigated using large eddy simulations with various grid resolutions and numerical choices. Auto-correlation analyses of cloud liquid water and relative humidity suggest a converged size of 200-300 m for moist patches outside clouds when model resolution is below 50 m but may overestimate this size due to non-cloudy moist regions. Based on a composite analysis, the structure of the moist halo immediately outside individual clouds is examined. It is found that, regardless of model resolution, the distribution of relative humidity in the halo region does not depend on cloud size, but on the real distance away from the cloud boundary, indicating some size-independent length scales responsible for the halo formation. The relative humidity decays with distance more quickly with finer horizontal resolution, which is possibly related to the model resolution dependency of the cloud spectrum. The halo size near cloud base is larger than that within the cloud layer and this feature is robust across all simulations. Further analyses of backward and forward Lagrangian trajectories originating from the moist halo region reveal the possible role for sub-cloud coherent structures on the cloud-base halo formation. Possible mechanisms explaining cloud halo sizes and associated length scales are discussed.
AS77-A006
Cloud-radiation Feedback Accelerates the Intensification of the Midlevel Vortex for Tropical Cyclogenesis
Bolei YANG1#+, Zhe-Min TAN1, Ji NIE2
1Nanjing University, 2Peking University
Cloud-radiation feedback helps accelerate tropical cyclogenesis, but the mechanism is still under debate. Using idealized numerical simulations in the radiative–convective equilibrium framework, it is revealed that cloud-radiation feedback can bring forward tropical cyclogenesis by accelerating the development of the midlevel vortex. A strong horizontal longwave radiative warming anomaly in the layer between 6 and 11 km altitudes in the vortex region, caused by large concentration of ice-phased particles at high levels, is critical to the development of the midlevel vortex. This longwave radiative warming anomaly induces more upward water vapor flux (mainly in the non-convective region) and then results in more latent heating at upper levels and more sublimation and melting cooling at lower levels. This leads to an increase of the vertical diabatic heating gradient, and then the intensification of the midlevel vortex. A stronger upward water vapor flux also produces more condensates at upper levels and further enhances the horizontal longwave radiative warming anomaly in the upper troposphere, constituting a positive feedback, and then accelerates tropical cyclogenesis.
Session Chair(s): Iain REID, ATRAD Pty Ltd
AS60-A006
Geminids Meteor Shower Observation Based on the Chinese Multistatic Meteor Radars
Maolin LU+, Wen YI#, Jie ZENG, Xianghui XUE, Hailun YE, Tingdi CHEN
University of Science and Technology of China
Geminids meteor shower is one of the most spectacular and reliable annual meteor showers observed from Earth. All-sky meteor radars have become a reliable and widely used tool for observing meteor ablation in the mesosphere and lower thermosphere (MLT) region. Currently, meteor radars mainly operate in single-station observation mode with 6000-20000 meteor echo detection per day. To obtain more abundant and accurate information about the meteors in the MLT region, a multistatic meteor radar system located in central and eastern China was introduced in this study. The radar system consists of two monostatic meteor radars installed in Mengcheng (33.36 °N, 116.49 °E) and Feidong (31.76 °N, 117.55 °E) and a remote receiver installed in Changfeng (31.98 °N, 117.22 °E). Using this radar system, we were able to detect the 2023 Geminids meteor shower at the radiant of R.A.=111°±8°, declination=34°±3° (J2000) with a geocentric velocity of 35.0±2.0 km/s. It was found that there is a clear variation of Geminids meteors among these meteor radars in the early morning.
AS60-A004
Observation of MLT Region Winds, Tides, Temperatures, Relative Densities by the USTC Mengcheng Meteor Radar
Wen YI#+, Xianghui XUE
University of Science and Technology of China
The atmospheric winds, waves, temperatures and densities in the mesosphere and lower thermosphere (MLT) region are essential for studying the dynamics and climate in the middle and upper atmosphere. The University of Science and Technology of China (USTC) meteor radar located at Mengcheng (33.4°N, 116.5°E) has been operating continuously since April 2014. More than 8 years’ observation of mesospheric horizontal winds and tides, temperatures and relative densities are presented in this study. In addition, we present the intercomparison among the meteor radar observations and the Navy Global Environmental Model-High Altitude (NAVGEM-HA) analysis results. The meteor number at northern midlatitudes suffers from diurnal variations in meteor occurrence, with a high count rate in the local morning and a low rate during local afternoon-to-midnight. The meteor count rates show a clear annual variation, with a maximum in September-October and a minimum in February. The horizontal wind in the MLT region has dominant annual variations at midlatitudes, with the eastward wind during summer and the westward wind during winter above 84 km, and the eastward wind during winter and the westward wind during spring below 84 km. The meridional wind shows northward during winter and southward during summer. The diurnal amplitude is dominant, and followed by the semidiurnal tides at midlatitudes. The zonal and meridional diurnal tides show enhancements during the spring (March) with amplitudes that can reach up to 40 m/s and 30 m/s and during autumn (September) with amplitudes that can reach up to 30 m/s and 25 m/s, respectively, basically following the characteristics that are strong during equinox and weak during solstice. Mesopause temperatures and relative densities were estimated by using the ambipolar diffusion coefficient measurements observed by the Mengcheng meteor radar.
AS60-A001
| Invited
Vertical and Horizontal Coverage by Lidar (VAHCOLI): Concept and First Observations of a new Lidar System
Franz-Josef LUEBKEN1#+, Josef HOEFFNER1, Thorben MENSE1, Jan FROH1, Gerd BAUMGARTEN2, Alsu MAUER1, Alexander MUNK3, Michael STROTKAMP3
1Leibniz-Institute of Atmospheric Physics, 2University of Rostock, 3Fraunhofer Institute for Laser Technology
In recent years we have developed a new lidar system called VAHCOLI (Vertical And Horizontal COverage by Lidar) which aims at measuring densities, temperatures, aerosols, and winds with high temporal and spatial resolution covering an entire volume (vertical and horizontal) at regional scales. VAHCOLI applies advanced laser spectroscopy based on a diode-pumped alexandrite ring laser and is installed in a compact housing (appr. 1 qm, 500 kg). The aim is to measure up to an altitude of 100 km and to cover horizontal scales up to several hundred kilometers by deploying several VAHCOLI units each equipped with several fields-of-view. In a first step we performed observations with one unit up to a height of ~25 km where VAHCOLI provides precise winds based on backscatter from tropospheric and stratospheric aerosols. Measurements were performed along five fields of view simultaneously (1 vertical, 4 horizontal) covering a horizontal distance of up to appr. 30 km, including observations of micro-scale wind dynamics. A comparison of our lidar results with data from ECMWF and ADM-Aeolus shows general agreement, but also some differences. In the future the 4D coverage of winds and temperatures by VAHCOLI allows to validate and stimulate models which include small scale dynamics caused by, for example, gravity waves and turbulence.
AS60-A003
| Invited
EPP-climate Link by Reactive Nitrogen Polar Winter Descent Revisited: MIPAS V8 Reprocessing and Future Benefits by the EE11 Candidate Mission CAIRT
Stefan BENDER1#+, Bernd FUNKE1, Manuel LOPEZ PUERTAS[1, Maya GARCIA-COMAS1, Gabriele STILLER2, Thomas VON CLARMANN2, Michael HÖPFNER2, Björn-Martin SINNHUBER2, Miriam SINNHUBER2, Quentin ERRERA3, Gabriele POLI4, Joern UNGERMANN5
1Instituto de Astrofísica de Andalucía (CSIC), 2Karlsruhe Institute of Technology, 3Royal Belgian Institute for Space Aeronomy, 4Italian National Research Council, 5Jülich Research Centre
Polar winter descent of reactive nitrogen (NOy) produced by energetic particle precipitation (EPP) in the mesosphere and lower thermosphere affects polar stratospheric ozone by catalytic reactions. This, in turn, may have implications for regional climate via radiative and dynamical feedbacks. NOy observations taken by the MIPAS/Envisat instrument during 2002--2012 have provided observational constraints on the solar-activity modulated variability of stratospheric EPP-NOy amounts. These constraints have allowed to formulate a chemical upper boundary condition for climate models in the context of solar forcing recommendations for CMIP6. Recently, a reprocessed MIPAS version 8 dataset has been released. Compared to the previous version, we assess what impact the changes in this new data version have on the EPP-NOy quantification, and on the formulation of chemical upper boundary conditions for climate models. The Earth Explorer 11 candidate Changing Atmosphere Infra-Red Tomography (CAIRT) will observe the altitude region from about 5 km to 115 km with an across-track resolution of 30 to 50 km within a 500 km wide field of view. This instrument will provide NOy and dynamical tracer observations from the upper troposphere to the lower thermosphere with unprecedented spatial resolution. Given that neither MIPAS nor any of the current instruments observes the lower thermosphere at this spatial resolution, we will assess the potential of this mission to advance our understanding of the EPP-climate link in the future.
AS60-A012
| Invited
A New Mm-wave Spectrometer for Simultaneous Multi-line Observation at Syowa Station and Its Preliminary Results
Akira MIZUNO1#+, Taku NAKAJIMA1, Hirofumi GOTO1, Tomoo NAGAHAMA1, Ryuho KATAOKA2, Yoshimasa TANAKA2, Rikuto KOIKE2, Mitsumu K. EJIRI2, Yoshihiro TOMIKAWA2,3, Hikaru SUZUKI4, Fuminori TSUCHIYA4, Isao MURATA4, Yasumasa KASABA4
1Nagoya University, 2National Institute of Polar Research, 3Graduate University for Advanced Studies, 4Tohoku University
Among various ground-based remote sensing measurements, microwave spectroscopy is one of the most suitable methods to study the middle atmosphere above the stratosphere because of the following advantages: its high frequency resolution enables to derive the vertical profiles by using the pressure-linewidth relationship, and the altitude range where the pressure broadening exceeds the Doppler linewidth extends higher than those of the infrared spectral lines. However, although the frequency resolution is high, the instantaneous bandwidth is not so wide (a few GHz), making it difficult to observe different molecular species simultaneously with a single spectrometer. The effects of energetic particle precipitation (EPP) on the middle atmosphere, i.e., formation of NOx and HOx and ozone destruction starting with ionization of nitrogen and oxygen molecules, are complicated processes involving ion chemistry, photochemistry, and atmospheric transport. So, for a comprehensive understanding it is important to obtain the information on the temporal changes and correlations of key molecules. We started routine observations in July 2022 at Syowa Station in Antarctica with a newly developed multi-frequency spectrometer that can simultaneously acquire molecular spectra in the 230 GHz, 247 GHz, and 250 GHz bands using an original waveguide-type frequency multiplexer, superconducting mixer receiver, and a 2.5 GHz bandwidth FFT spectrometer. Spectral lines of NO, O3, CO, NO2, and HO2 exist within the frequency bands, and observations are basically made by frequency switching and hot-cold calibration methods. Currently, no significant spectral lines have been detected for HO2 and NO2, but two O3 lines at 249.79 GHz and 249.96 GHz, six hyperfine structure lines of NO around 250.4 GHz and 250.8 GHz, and one CO line at 230.54 GHz have been observed. In the presentation, we will present the instrumental configuration and specification, and preliminary results.
AS60-A010
Secondary Harmonic Generation of Rossby Waves Observed in the Middle Atmosphere
Maosheng HE1#+, Jeffrey FORBES2
1National Space Science Center, Chinese Academy of Sciences, 2University of Colorado Boulder
Rossby waves, also known as planetary waves, are transverse waves propagating zonally in rotating fluids, with the Coriolis force acting as the restoring force. Rossby waves are characterized by long spatiotemporal scales (days to weeks). Their wavelengths are comparable to the scale of the rotating fluid and their periods are longer than the rotational period. Detecting Rossby waves requires continuous and simultaneous monitoring of the rotating fluid from multiple longitude sectors. Moreover, monitoring Rossby waves can be tricky since they are dissipative and transient, making them one of the rare atmospheric phenomena predicted in theory before actual observation. Rossby waves play a crucial role in shaping the weather and climate of Earth's atmospheres, oceans, and plasmas, as well as those of the Sun and other celestial bodies. The nonlinear behavior of Rossby waves helps explain important processes and periodicities in celestial bodies. The lowest-order nonlinearity is the second harmonic generation, where waves interact nonlinearly with themselves, creating new waves with twice the frequency and wavenumber. This behavior, commonly seen in radio communication and nonlinear optics, has been theoretically analyzed and numerically simulated for Rossby waves in the atmosphere but not directly observed. To address this observational challenge, we applied the phase difference technique—a dual-point detection method—on meteor radar data near 95 km altitude from two stations near 54°N latitude, situated in China and Germany. Our analysis discerned a sequence of perturbations in the Earth's middle atmosphere, which could be ascribed to the presence of Rossby waves during the sudden stratospheric warming event in January 2019; notably, two fluctuations with periods of 16 and 8 days and zonal wavenumbers 1 and 2, respectively. The frequency and zonal wavenumber suggests the occurrence of second harmonic generation of a Rossby wave normal mode. See He & Forbes,(2022), https://doi.org/10.1038/s41467-022-35142-3.
AS60-A016
Stratospheric Tropospheric (ST) Radar Observations of Electromagnetic Ion Cyclotron (EMIC) Waves
Jordan JONKER 1, Manuel CERVERA2, David HOLDSWORTH1, David NEUDEGG1, Trevor HARRIS2, Andrew MACKINNON2, Iain REID3,2#+
1Defence Science and Technology Group, 2The University of Adelaide, 3ATRAD Pty Ltd
Recently it has been shown that Stratospheric Tropospheric (ST) wind profiling radars may be simply reconfigured to observe spacecraft in low Earth orbit (LEO) in addition to measuring winds in the ST region. This is of considerable interest to the Space Domain Awareness (SDA) community as the LEO environment is becoming increasing congested and identification and tracking are becoming extremely important. However, as the radio transmissions from these radars traverse the Earth’s ionosphere, they are subject to perturbations due to ionospheric disturbances. These perturbations manifest as variations in the measured Doppler shift measured for the LEO spacecraft. There are many sources of ionospheric disturbances, e.g., those due to atmospheric gravity waves (AGWs) generated in the troposphere which propagate to ionospheric altitudes, small scale plasma instabilities, and electromagnetic ion cyclotron (EMIC) waves. The latter are generated in the magnetosphere and propagate along the geomagnetic field lines as transverse waves into the high-latitude ionosphere. There they mode-convert into compressional waves and propagate equatorward along the magnetic meridian in an ionospheric wave guide centred at the peak electron density of the F2 layer. Ionospheric disturbances have previously been observed by ionospheric sounders, over-the-horizon (OTH) high frequency (HF) radars such as the Super Dual Auroral Radar Network (SuperDARN), incoherent scatter radars (ISRs), global navigation satellite systems (GNSS) and magnetometers. Observation of LEO spacecraft by HF and VHF radar offers a new method for the detection and study of ionospheric disturbances. In this paper we report on observations of ionospheric plasma instabilities and EMIC waves travelling in the ionospheric wave guide from two radars operating at 30 MHz and 55 MHz in the South-Eastern region of Australia.
AS60-A013
The Langfang Dual-frequency Atmospheric Radar System: The First Two-years of Observations
Qingchen XU1#+, Iain REID2,3
1Chinese Academy of Sciences, 2ATRAD Pty Ltd, 3The University of Adelaide
The new dual-frequency atmospheric radar system at the Langfang Observatory in northern China has been in operation for two years. This radar utilizes a novel two-frequency system design that allows interleaved operation of 53.8 MHz for stratosphere and troposphere wind observation, and 35.0 MHz for meteor observation, which optimizes performance for both ST wind retrieval and meteor trail detection. The results of winds and gravity waves (GWs) momentum fluxes in the mesosphere, lower stratosphere and troposphere during the first two-years of observations are presented.
AS60-A011
Small VHF Radar Measurements of Winds and Momentum Flux In the Troposphere, Lower Stratosphere and Mesosphere
Iain REID1,2#+, Bronwyn DOLMAN1,3
1ATRAD Pty Ltd, 2The University of Adelaide, 3University of Adelaide
Radar observations of the troposphere and lower stratosphere made in southern Australia with a VHF ST/Meteor radar are presented. The ST radar was operated using a sub-section of the array and provides an interesting and rare example of a small beam swinging Doppler radar operating in the lower VHF band (55 MHz). Additional sub-arrays were used in Spaced Antenna mode which allows interferometric operation. The radar also operates as a meteor radar and so measurements of mean winds and wave fluxes measured in the Troposphere, Stratosphere, and Mesosphere are available. We have previously presented measurements made using two VHF radars in Germany, one of them which also used a small antenna array, and the present results extend those. Results are presented and discussed in the context of coupling between these regions of the atmosphere and the potential of such small radars for dynamical studies.
Session Chair(s): Myoung Hwan AHN, Ewha Womans University
AS15-A001
Shallow Cumulus Characteristics from Satellite Remote Sensing
Mengqi LIU#+
Chengdu University of Information Technology
Shallow cumulus is one of convective clouds characterized by very weak development, which has a substantial impact on the radiation budget of the Earth-Atmosphere system, weather system evolution, global water cycle, and climate change. Satellite characteristics of shallow cumulus is still associated with larger uncertainties that is partly due to its very fine spatial scale and partly originated from satellite measurements and algorithms. Inner Mongolia grassland is an ideal region for researches of satellite remote sensing shallow cumulus due to the flat terrain, vegetarian stability, and high frequency of shallow cumulus in summer. Therefore, the objective of this program is to quantify satellite-based retrieval of cloud characteristics of shallow cumulus. The ultimately goal is to improve understanding of shallow cumulus from satellite sensors.
AS15-A035
Cloud Feedback to SST Change Over the Tropical Western Pacific: COMS vs MODIS
Yoon-Kyoung LEE+, Yong-Sang CHOI#, Jiwon HWANG
Ewha Womans University
Tropical cloud feedback remains uncertain because the cloud response to temperature varies among numerous observational studies. This study shows that a geostationary view can significantly reduce the uncertainty in estimation of cloud feedback over the tropical western Pacific. The cloud feedback was calculated as the simultaneous relation of daily sea surface temperature (SST) and cloudiness over the tropical western Pacific (TWP) from satellite data: the meteorological imager on the geostationary earth orbit (COMS) versus the MODIS on the low-level earth orbit (MODIS). SST is weighted with the clear-sky fraction data from COMS and MODIS. The regression relation between cloud and SST is strongly negative when using COMS cloud data. This may be due to a larger field-of-view of the COMS over the TWP than that of MODIS. Therefore, to estimate cloud feedback over the TWP in accuracy, such geostationary satellite data are indispensable.
AS15-A050
Seasonal Diurnal Variations of Deep Convective Clouds Over the Philippine Climate Regions
Jason Pajimola PUNAY1+, John Michael Parpan AGUADO1, Ralph Cedric Rodriguez CABATE1, Leonardo Jr. Rivera ESPOSADO1, Aimmiel Renz Ostonal HINA1, Chian-Yi LIU2#
1Bicol University, 2Academia Sinica
This study characterizes the seasonal diurnal variations of deep convective clouds (DCC) over the Philippine climate regions based on the Modified Corona Classification. DCCs during non-tropical cyclone days were identified using infrared brightness temperature threshold of 208 K. Hourly DCC temperature, percentage, and frequency distributions were obtained from 2016 to 2018 during the northeast monsoon season or Amihan (December to February), warm-dry season (March to May), southwest monsoon season or Habagat (June to August), and transition season (September to November). The temperature and percentage distributions of DCC follow a general diurnal pattern in all climate regions and seasons except Type II and during Amihan. Coldest and maximum percentage of DCC occurs in the afternoon (1500-1800 LST), whereas warmest and minimum percentage of DCC happens in the late morning (0900-1200 LST). Although both temperature and percentage displays a general pattern, spatiotemporal maps reveal that coldest DCC (<199 K) does not coincide and are not collocated with areas of high DCC frequency. Reanalysis data were used to further examine the environmental conditions associated with the development of DCC. Warm surface temperature and moisture convergence shows a significant influence on the diurnal development of DCC, while low inhibition, large-scale upward wind, and unstable boundary conditions contribute to deep convective initiation. The findings from this study can improve the understanding of deep convective activity in the Philippines, facilitating more effective disaster risk management associated with deep convective systems.
AS15-A047
Detection and Analysis of Marine Heat Waves in Northeast Asia Using COMS/MI and GK-2A/AMI Sea Surface Temperature Data
Jongho WOO1+, Kyung-soo HAN1#, Eunha SOHN2, Meeja KIM2
1Pukyong National University, 2Korea Meteorological Administration
This study contributes to the broader discourse on the "Application of Satellite Data to Weather, Climate, and Environmental Study," focusing on the detection and analysis of marine heatwaves (MHW) in Northeast Asia. Utilizing high-resolution sea surface temperature (SST) data from the Communication, Ocean, and Meteorological Satellite (COMS)/Meteorological Imager sensor (MI) and GEO-KOMPSAT-2A (GK-2A)/Advanced Meteorological Imager sensor (AMI), the research spans the period from 2012 to 2021.The analysis reveals a discernible surge in both the frequency and intensity of MHW events, particularly post-2018, with the year 2020 marked by prolonged and intense occurrences. Statistical validation, employing Optimal Interpolation Sea Surface Temperature (OISST) data and satellite SST data through T-test assessment, solidly confirms a noteworthy increase in sea surface temperatures. This finding substantiates the assertion that these changes are a direct consequence of climate change rather than random variations. The intricate topography and varied climatic conditions of Northeast Asia add significance to our research, providing critical insights into the localized impacts of global climate dynamics. The identified trends underscore the pressing need for continuous monitoring and more nuanced analyses to inform long-term responses to climate change. This study, by specifically examining MHW events in Northeast Asia, contributes valuable information to the broader goal of advancing remote sensing knowledge and skills for enhanced environmental monitoring, understanding, prediction, and management.
AS15-A046
Characteristics of Cloud Properties and Precipitation from Satellite Observation During the Formation of Tropical Storm Over the Western North Pacific Region
Chian-Yi LIU1#+, Kai-Li ZHU1, Jason Pajimola PUNAY2
1Academia Sinica, 2Bicol University
Several tropical depressions (TDs) form in the Western North Pacific (WNP) region throughout the year. While some of them intensify into tropical storms (TSs), others eventually dissipate. Therefore, the objective of this study is to analyze the characteristics associated with the development of TDs by investigating cloud microphysics and precipitation properties. The analysis is based on data obtained from the geostationary Advanced Himawari Imager (AHI) and Global Precipitation Measurement (GPM) mission. A total of 194 tropical cyclones (TCs) occurring from year of 2015 through 2021 are analyzed in the study. Meanwhile, TCs are classified into two types based on their development scenarios: TD-dissipating and TS-developing cases. Environmental conditions for TC development are investigated by selecting an area extending six times the radius of maximum wind (RMW) from the storm center. Analysis of AHI cloud sciences data reveals significant distinctions between the cases within 48 hours prior to the critical time. Among the three variables examined, TS-developing cases exhibit slightly higher values compared to TD-dissipating cases. Within 24 hours prior to the critical time, TS-developing cases maintain their intensity, while TD-dissipating cases exhibit a decreasing trend. As the critical time approaches, the cloud optical thickness (COT), the cloud effective radius (CER), and the cloud top height (CTH) increase within 6 RMW, indicating thicker cloud layers and larger cloud droplet size throughout the entire region, with stronger updraft. While approaching the critical time, TS-developing cases display more vigorous convective activity with higher COT and CTH near the storm center, along with higher rain rate and wider precipitation range.
AS15-A016
Quantitative Applications of Weather Satellite Data for Nowcasting – Progress and Challenges
Jun LI1#+, Jing ZHENG2, Bo LI3, Min MIN4, Zhenglong LI5, Chian-Yi LIU6, Yunheng XUE7
1National Satellite Meteorological Center, 2China Meteorological Administration, 3National Satellite Meteorological Cener, China Meteorological Administration, 4Sun Yat-sen University, 5University of Wisconsin-Madison, 6Academia Sinica, 7Chengdu University of Information Technology
Monitoring and predicting highly localized weather events over a very short-term period, typically ranging from minutes to a few hours, are very important for decision makers and public action. Nowcasting these events usually relies on radar observations through monitoring and extrapolation. With advanced high-resolution imaging and sounding observations from weather satellites, nowcasting can be enhanced by combining radar, satellite and other data, while quantitative applications of those data for nowcasting are advanced through using machine learning techniques. Those applications include monitoring the location, impact area, intensity, water vapor, atmospheric instability, precipitation, physical properties, optical properties of the severe storm at different stages (pre-convection, initiation, development, and decaying), identification of storm types (wind, snow, hail, etc.), and predicting the occurrence and evolution of the storm. Satellite observations can provide information on the environmental characteristics in the pre-convection stage and are very useful for situational awareness and storm warning. This presentation provides an overview of recent progress on quantitative applications of satellite data in nowcasting and its challenges; future perspectives are also addressed and discussed.
Session Chair(s): Likun XUE, Shandong University
AS08-A025
| Invited
The Size Distributions and Optical Properties of Particulate Organic Nitrates in Urban Air
Ru-Jin HUANG1#+, Wei HUANG2, Chunshui LIN2, Jing DUAN2
1Institute of Earth Environment, Chinese Academy of Sciences, 2Chinese Academy of Sciences
Particulate organic nitrates are ubiquitous in the atmosphere and affect secondary organic aerosol formation and atmospheric radiation balance. The impacts of particulate organic nitrates are regulated by their concentrations, size distributions and optical properties. However, these properties of particulate organic nitrates in ambient air remain poorly understood. Here, the mass size distributions and optical properties of particulate organic nitrates were investigated in urban air of China with a soot particle long-time-of-flight aerosol mass spectrometer and an Aethalometer. The results show a bimodal size distribution of particulate organic nitrates, peaking at ~350 nm in condensation mode (100-400 nm) and ~750 nm in droplet mode (400-2500 nm). The formation processes of particulate organic nitrates in the two size modes were respectively governed by temperature-dependent condensation and aqueous-phase processing. Furthermore, the imaginary part of the refractive index of particulate organic nitrates was calculated by Core-Shell Mie theory and ranged from 0.004 to 0.158 between short visible and ultraviolet wavelengths (370-520 nm). Accordingly, particulate organic nitrates contributed 2-34% to black carbon absorption enhancement throughout the observation period. These results provide a better understanding of the formation of secondary organic aerosol in ambient atmosphere and the impacts of particulate organic nitrates on the atmospheric radiation balance.
AS08-A012
| Invited
Ozone and Fine Particulate Nitrate Formation Across 38 Cities of North China Plain
Likun XUE1#+, Yujiao ZHU1, Jian GAO2, Hong LI2, Yue SUN1, Yingnan ZHANG3, Xuelian ZHONG1, Min ZHAO1, Hengqing SHEN1, Yujie ZHANG2, Shuai WANG4, Guigang TANG4, Wenxing WANG1
1Shandong University, 2Chinese Research Academy of Environmental Sciences, 3The Hong Kong Polytechnic University, 4China National Environmental Monitoring Centre
The North China Plain (NCP), one of the most polluted regions in China, has been suffering from severe ozone (O3) and PM2.5 pollution in the recent decades. In summer 2021, we conducted a large-scale field campaign across 38 cities in the NCP to comprehensively understand the regional distribution and formation mechanisms of O3 and nitrate aerosol. The measurement data were subject to detailed gas phase and multiphase chemical box modelling analyses to diagnose the formation regimes of O3 and nitrate. The results revealed distinct regional distributions of O3, nitrate, and their precursors, e.g., nitrogen oxides (NOx) and volatile organic compounds (VOCs). The O3 formation mechanisms showed a clear regional homogeneity with most cities under VOCs-NOx co-limited regime or VOCs-limited regime. On O3 pollution days, increased sensitivity of O3 formation to NOx was observed, due to the substantial NOx reductions by the pollution control efforts. Light alkenes (C2-C5) and BTEX (benzene, toluene, ethylbenzene and xylenes) are the dominant VOC species that contributed significantly to O3 formation in most cities of the NCP region. The nitrate formation regime and its dependence on the related parameters are also examined, which also showed a regional honogeneity. We also determined the optimal VOCs/NOx reduction ratios for the individual city and the entire region for formulating regional coordinated control strategies for both O3 and nitrate pollution.
AS08-A032
| Invited
The Role of Naphthalene and Its Derivatives in the Formation of Secondary Organic Aerosols in the Yangtze River Delta Region, China
Jingyi LI#+, Fei YE, Kangjia GONG, Haowen ZHANG, Momei QIN, Jianlin HU
Nanjing University of Information Science & Technology
Naphthalene (Nap) and its derivatives, including 1-methylnaphthalene (1-MN) and 2-methylnaphthalene (2-MN), serve as prominent intermediate volatile organic compounds (IVOCs) contributing to the formation of secondary organic carbon (SOC). In this study, the Community Multi-Scale Air Quality (CMAQ) model coupled with detailed emissions and reactions of these compounds was utilized to examine their roles in the formation of SOC and other secondary pollutants in the Yangtze River Delta (YRD) region during summer. Remarkably, significant underestimations of Nap and MN concentrations (by 79% and 85%) were observed at the Taizhou site. To better capture the temporal variations of Nap and MN, their emissions in the YRD region were scaled up by a factor of 5 and 7, respectively, with constraints based on field measurements. After adjusting their emissions, Nap concentrations reached 27 ppt in the YRD, accounting for 4.1% and 9.1% (up to 13.7%) of total aromatics emissions and aromatic-derived SOC, respectively. 1-MN and 2-MN were relatively low, with an average of 3 and 6 ppt in the YRD, and contributed 3.1% of aromatic-derived SOC. The influences of Nap and MN oxidation on ozone and radicals might be trivial on a regional scale but were not negligible when considering daily fluctuations, particularly in Shanghai and Suzhou. This study emphasizes the high SOC formation potentials of Nap and MN, which may pose environmental risks and adverse health.
AS08-A008
A Super Dust Storm Enhanced by Radiative Feedback
Yu CHEN#+, Siyu CHEN
Lanzhou University
As the main dust source area in East Asia, the Gobi Desert (GD) exerts critical impacts on the radiation budget in downstream regions. Dust radiative feedback in the GD on the Mongolian cyclone, however, remains poorly understood. Herein, the dynamic dust source is coupled with the Weather Research and Forecasting model with Chemistry (WRF-Chem) for better dust simulations. Results show that the Mongolian cyclone dominates the dust event in May 2019. Dust radiative feedback results in downward momentum transport and cools northeast of Mongolia by affecting zonal winds and temperature advection. Lower-troposphere cooling and upper-atmosphere warming change the atmospheric vertical structure and enhance baroclinicity. Further, cold air deeply descends into the bottom of the warm air in a wedge shape and promotes the ascension of warm air to enhance the Mongolian cyclone. The strong dust is maintained and continues to cause high dust concentrations in northern China via westerlies. This study explores how dust radiative feedback over the GD can intensify the Mongolian cyclone and provides a scientific reference for related studies.
AS08-A031
The Pivotal Role of Anthropogenic Oxygenated Organic Compounds in New Particle Growth in Urban Beijing
Lizi TANG+, Min HU#, Dongjie SHANG, Zeyu FENG
Peking University
The growth of freshly formed molecular clusters is a decisive process in new particle formation (NPF), which determines the survival of new particles to cloud condensation nuclei sizes, thus the related environment effects. Gas-phase oxygenated organic molecules (OOMs) are thought to be crucial for the growth of newly formed particles. However, the sources of OOMs and their contributions to new particle growth rate are not well understood in urban areas. Herein, gas-phase OOMs were measured on NPF days in the autumn of 2021 in urban Beijing. Our results exhibited a higher oxidation degree of OOMs compared with previous urban observation. This is due to the lower NOx level, which promoted the propagation reactions. By applying a recently developed framework on OOM categorization, 52% and 27% OOMs were attributed to the oxidation of anthropogenic aromatic and aliphatic VOCs. The aerosol dynamic model shows that the condensation of OOMs is the main source to the initial growth of new particles (sub-25 nm), with the contribution of anthropogenic OOMs exceeding 87%, although there are missing contributors to the growth of particles above 15 nm. This study emphasizes the pivotal role of anthropogenic oxygenated organic compounds in new particle growth in urban Beijing, and highlight the importance of controlling anthropogenic precursors for mitigating the environmental impact of NPF.
AS08-A020
Direct Effects of Air Humidity on Dust Aerosol Production: Evidences for the Surprising Role of Electrostatic Forces
Xiewen MA#+, Xiaofei WANG
Fudan University
Dust aerosols are produced by wind erosion, and it is widely accepted that dust aerosols can be produced only if the wind speed exceeds a certain threshold velocity, which is largely controlled by soil moisture content. The relative humidity (RH) in the air could affect soil moisture content, thereby impacting dust production indirectly. However, it is not clear if the RH can directly change dust aerosol production. Here we simulated dust production and show that the RH does play a direct role in affecting the production of dust aerosol in a quite complicated way, which can be explained by a hypothesis that the RH affects both the electrostatic forces and wet-bonding forces between soil particles in opposite directions. The current formula for dust aerosol production flux does not include the direct RH effect, and this study strongly suggests that it could lead to significant errors in estimating dust production.
AS08-A033
Comparison of Tropospheric NO2 Vertical Profile Between Remote Sensing and Airborne In-situ Measurement
Yongjoo CHOI1#+, Yugo KANAYA2, Taehyoung LEE1, Jihee BAN1, Chisung YUN1, Limseok CHANG3, Jun-Young AHN3, Jin-Soo PARK3, Jin-Soo CHOI3, Myungsoo YOO3, Thomas WAGNER4, Van Roozendael MICHEL5
1Hankuk University of Foreign Studies, 2Japan Agency for Marine-Earth Science and Technology, 3National Institute of Environmental Research, 4Max Planck Institute for Chemistry, 5Royal Belgian Institute for Space Aeronomy
The Geostationary Environment Monitoring Spectrometer (GEMS), a geostationary orbit satellite capable of measuring major gaseous pollutants including NO2, was successfully launched in February 2020. It is currently performing its mission, providing hourly information on pollutants in Northeast and Southeast Asia during daytime. One of the key variables determining the accuracy of GEMS NO2 is the a priori vertical distribution provided by the Global Earth Observing System Chemistry-Transport Model (GEOS-CHEM). Validation of NO2 vertical distribution is typically carried out using data from ground-based multi-axis differential optical absorption spectroscopy (MAX-DOAS) observations, but a lack of validation for vertical profiles derived from MAX-DOAS for example by airborne measurements remains a large uncertainty of the retrieval process in remote sensing communities. Therefore, this study validates the accuracy of the vertical distribution of NO2 vertical profiles from MAX-DOAS by airborne measurements conducted at three sites in the Seoul Metropolitan Area, Korea (Yongin, Suwon, and Seoul) during the Satellite Integrated Joint Monitoring of Air Quality (SIJAQ) campaign in 2021 and 2022. This study will improve the accuracy of NO2 vertical profiles from both MAX-DOAS and GEMS products by combining with airborne measurements during the upcoming Airborne and Satellite Investigation of Air Quality (ASIA-AQ) campaigns in 2024.
Session Chair(s): Kosuke ITO, Kyoto University
AS13-A045
Subsequent Tropical Cyclogenesis in the South China Sea Induced by the Pre-existing Tropical Cyclone Over the Western North Pacific: A Case Study
Kelvin T. F. CHAN#, Yue WU, Lifeng XU+
Sun Yat-sen University
Mechanisms of tropical cyclogenesis have been studied for decades. A new one in the South China Sea, namely, PTC-STC is proposed. A subsequent tropical cyclone (STC) in the South China Sea can be induced by a pre-existing tropical cyclone (PTC) over the western North Pacific. The observations, reanalysis, and numerical sensitivity experiments suggest that the terrain of the Philippines (especially Luzon) is geographically essential to the tropical cyclogenesis and development of STC, whereas the intensity and track of PTC are conditionally decisive. If the terrain of the Philippines is replaced by sea, no STC forms. The steep mountain range of Luzon provides static blocking effect that can 1) enhance the upward motion; 2) accumulate warm moist air mass from the westerly and PTC; and 3) constrain the advection of vorticity from the PTC. Meanwhile, the northeasterly from the PTC climbs over the terrains, increases the adiabatic heating, and warms the proximity in the leeside of the mountains. These processes show that the interactions between the PTC and the terrain of the Philippines could provide favorable dynamic and thermodynamic conditions for the tropical cyclogenesis of STC in the low-to-mid troposphere of the South China Sea. Whereas, if the PTC is too strong, it could move into the South China Sea, suppressing the standalone favorable conditions for the tropical cyclogenesis of STC in the South China Sea.
AS13-A017
Can a Pre-existing Tropical Cyclone Generate Another Tropical Cyclone?
Kosuke ITO1#+, Kenji YAMAUCHI2
1Kyoto University, 2University of the Ryukyus
It has been believed that a strong pre-existing tropical cyclone (TC) can contribute to the genesis of another TC to the east or southeast in the western North Pacific through the Rossby wave dispersion (Ritchie and Holland, 1999; Li et al. 2006). However, these TCs are usually observed in the easterly wind where the stationary Rossby wave cannot exist, and a well-coordinated numerical experiment has not been conducted to elucidate the impact of a pre-existing TC. Therefore, we conducted a set of numerical simulations in which a pre-existing TC is removed sufficiently prior to the genesis of a subsequent TC. It turned out that a subsequent TC was generated even without a pre-existing TC in all 10 simulations for a pre-existing TC case according to the genesis environment database of Fudeyasu and Yoshida (2018). Also, the removal of a pre-existing TC hardly affects the intensity of a subsequent TC. This type of a TC is typically located south of a subtropical high, where the horizontal cyclonic shear prevails from west to east widely. Further analysis showed that these TCs were frequently observed in MJO phase 7, El Nino, and positive SST anomaly to the east of the western North Pacific. These are favorable for the genesis of a TC in the broad area of the western North Pacific. In other words, the characteristics are simply explained by the favorable condition in a broader area for the genesis of two TCs in which an eastern TC is generated later because the SST is lower in the east of the western North Pacific, not necessarily relying on the Rossby wave dispersion from a pre-existing TC.
AS13-A002
Why Does Rapid Eyewall Contraction Precede Rapid Intensification in Tropical Cyclones?
Yuanlong LI#+
Nanjing University
Based on the absolute angular momentum (AAM) conservation law, it has long been accepted that tropical cyclone (TC) intensification occurs simultaneously with eyewall contraction. However, some recent studies have found that rapid contraction (RC) of the radius of maximum wind (RMW) could precede rapid intensification (RI) in both observations and simulations, but the understanding of the involved dynamics is incomplete. In this study, the statistical relationship between RC and RI is first revisited based on the extended best track dataset for the North Atlantic and eastern North Pacific during 1999–2019. Results show that, as expected, for more than ∼65% of available TCs, the time of the peak contraction rate precedes the time of the peak intensification rate, on average, by ∼10–15 h. Among those TCs with RC and RI, more than ∼65% involve the onset of RC preceding the onset of RI, on average, by ∼15–25 h. The statistical analysis above suggests that RC tends to precede RI. To understand the corresponding dynamics, theoretical analysis and numerical simulations are further performed. Results show that AAM is not conserved following the RMW, and thus the phenomenon cannot be understood based on the AAM-based dynamics. Both budgets of tangential wind and RMW are shown to provide dynamical insights into the relationship between RI and RC. During the RC stage, due to the weak TC intensity and large RMW, the small curvature of the radial distribution of tangential wind near the RMW favors RC but weak diabatic heating far inside the RMW leads to weak low-level inflow and small radial absolute vorticity flux near the RMW and thus unfavor intensification. As RMW contraction continues and TC intensity increases, the situation is reversed during the RI stage. These findings can help improve our understanding of TC structure and intensity changes.
AS13-A007
Interaction of Cloud Dynamics and Microphysics During Typhoon Rapid Intensification
Zuhang WU1#+, Yun ZHANG1, Yuan WANG1,2
1National University of Defense Technology, 2Nanjing University
The rapid intensification (RI) of tropical cyclones (TCs) becomes more frequent in recent years, but the TC RI forecasts still remain challenging. Better understanding of the physical processes associated with RI of TCs would essentially improve its forecasting capability. The cloud dynamical and microphysical processes, especially their interactions that respond to RI are not well explored. In this study, the cloud macro and micro characteristics associated with RI of a super-typhoon Nanmadol (2022) over the western Pacific are investigated using multiple satellites observations. The storm underwent RI during 15–16 September 2022, and it has wreaked havoc on Japan's most cities as it moved across the Japanese island afterward with a track length of about 1,120 km. It is found inside Nanmadol as well as other typhoons that a few large particles tend to occur in the outer rainbands during RI, due to the interaction of cloud dynamical and microphysical processes. Such unique feature of particle distribution in the outer rainbands could be a potential indicator for RI, and should also be paid attention to in model forecasting of typhoon precipitation.
AS13-A021
The Impacts of Taiwan Terrain on the Rapid Intensification of Typhoon Chanthu (2021)
Wei-Ting FANG1#+, Pao-Liang CHANG2, Ming-Jen YANG3
1Central Weather Administration, 2Central Weather Bureau, 3National Taiwan University
Intensification of Typhoon Chanthu (2021) along the eastern coast of Taiwan was accompanied by pronounced asymmetry in eyewall convection dominated by wavenumber-1 features, as observed by a dense radar network in Taiwan. This study integrates data from multiple radars to analyze the temporal evolution of the inner core structure and kinematic features. The maximum wind speed at 3 km altitude, retrieved from radar observations, exhibited a rapid increase of approximately 18 m s-1 within an 11-hour period during the intensification stage, followed by a significant decrease of approximately 19 m s-1 within 8 hours during the weakening stage, indicative of rapid intensification (RI) and rapid weakening (RW), respectively. Therefore, Chanthu underwent both RI and RW within the 24-hour analyzed period, posing challenges for intensity forecasts. During the intensifying stages, the region of maximum eyewall convection asymmetry underwent a sudden cyclonic rotation from the eastern to the northern semicircle immediately after the initiation of terrain-induced boundary inflow from the south of the typhoon, as observed by surface station data. This abrupt rotation of eyewall asymmetry exhibited better agreement with radar-derived vertical wind shear (VWS) than that derived from global reanalysis data. This finding suggests that the meso-β scale VWS is more representative for tropical cyclones than meso-α scale VWS when the terrain-induced forcing predominates in the environmental conditions. Further examination of the radar-derived VWS indicated that the VWS profile pattern provided a more favorable environment for typhoon intensification. In summary, Chanthu’s RI was influenced by the three factors: 1) terrain-induced boundary inflow from the south of the typhoon, observed by surface station data, 2) low-level flow pointing toward the upshear-left direction, and 3) weak upper-level VWS.
AS13-A028
Diversity of Tropical Cyclones Rapidly Intensification
Ke PENG#+
Nanjing University of Information Science & Technology
The prediction and understanding of rapid intensification (RI) of tropical cyclones (TCs) have always been challenges. The maximum wind speed (Vmax) and the minimum central pressure (Pmin) are two commonly used TC intensity indicators. In most existing works, they only choose a single indicator (mostly Vmax) to investigate the RI process. Whether there is a difference between the RI defined by 24-hour changes of Vmax and 24-hour changes of Pmin, and what the relationship is between RI in Vmax and RI in Pmin are the issues that deserve to be discussed. The study found that rapid changes in Vmax and in Pmin are not always accompanied. RI cases can be divided into three categories: 1) Both the Vmax and the Pmin experienced rapid change (RIpv), 2) only the Vmax strengthened rapidly (RIv), 3) only the Pmin decreased rapidly (RIp). Each type of RI exhibits distinctive TC structures and convective features. At the onset of RIv, the TC intensity is weakest and the TC fullness is smallest. The deep convection is concentrated in the inner-core region. For RIp, the TC intensity is strongest and the TC fullness is the largest. Pmin, as an integral variable, reflects not only the TC intensity but also the TC size. In cases where there is only a rapid change in Vmax (RIv), the TC size expands slowly. In cases where only Pmin deepens rapidly (RIp), the outer circulation expansion is most evident. Thus, RI classified via these two commonly used TC intensity indexes (Vmax and Pmin) could help us further understand the relationship between TC size and TC intensity.
AS13-A038
Evaluating the Role of WISHE in the Rapid Intensification of Tropical Cyclones by Ensemble Simulations
Chieh-Jen CHENG#+, Chun-Chieh WU
National Taiwan University
In the previous work, we examined the role of surface heat fluxes, particularly in relation to the wind-induced surface heat exchange (WISHE) mechanism, in the rapid intensification (RI) of tropical cyclones (TCs). Sensitivity experiments with capped surface fluxes and thus reduced WISHE exhibit delayed RI and weaker peak intensity, while WISHE could affect the evolutions and alter the thermodynamic environment and convective-scale processes of TCs both before and after the onset of RI. Additional ensemble simulations are conducted in this work to further evaluate the role of WISHE in RI. Results of ensemble members show delayed or even no RI and weaker peak intensity when WISHE is capped. The more the WISHE is capped, the weaker intensity of the TC is found, especially the evolution of the minimum sea level pressure. In addition, analyses show that WISHE could determine the intensification rate of both minimum sea level pressure (MSLP) and maximum 10-m wind speed. When the longer period is examined, the larger differences of intensification rate are found among all WISHE-capped experiments. Moreover, when the capped wind speed for calculating the surface heat fluxes is set to a same value and in a same intensification period, the spread of the intensification rate of maximum 10-m wind speed is larger than that of MSLP. Furthermore, based on the RI onset time, the ensemble members are separated into three groups: early, medium, and late group. Results show that earlier RI could be found when vortices are with broader wind field, relatively more axisymmetric low-level wind field and inner-core convection, showing both mass and dynamic field of TCs are also important factor in the RI of TCs. In all, results of ensemble simulations are generally consistent with the previous work, while additional important factors are further pointed out in this study.
AS13-A044
A Numerical Study on the Rapid Intensification and Rapid Weakening of Typhoon Trami (2018)
Jaedeok LEE1#+, Eun-Chul CHANG1, Kosuke ITO2, Chun-Chieh WU3
1Kongju National University, 2Kyoto University, 3National Taiwan University
This study investigated Typhoon Trami (2018) which experienced both rapid intensification (RI) and rapid weakening (RW) events using the Weather Research and Forecasting model version 4.2 with the activation of the three-dimensional Price-Weller-Pinkel ocean model. In general, predicting these extremely intensifying or weakening events remains challenging. For better initial conditions for Trami’s RI and RW, the dynamical initialization with the assimilation of relative humidity is applied by adding more dropsonde data retrieved from the second round of the Tropical Cyclones-Pacific Asian Research Campaign for the Improvement of Intensity Estimations/Forecasts campaign for Trami. Compared to the National Centers for Environmental Prediction global forecast system (GFS) forecast data, the initialized storm shows some improvements in track and intensity forecasts, though the original storm in the GFS forecast data exhibits reasonable track and intensity forecasts. For Trami’s RI, it can be seen that vertical wind shear noticeably decreased and convective bursts significantly increased during the RI period. This dynamically favorable environment may be advantageous for forming robust eye and eyewall structures. Thus, Trami reached a category 5 Saffir-Simpson hurricane wind scale. After that, as Trami turned northward from westward, its translation speed substantially decreased. This slow translation speed contributes to the upwelling development in the rear-right quadrant of Trami, which forms a stable boundary layer. Ultimately, it can cause reduction and asymmetry of surface heat fluxes and convective clouds in Trami’s eyewall area. At the mature stage, one unfavorable factor may in turn affect tropical cyclone intensity and intensification depending on the interaction period. To sum up, Trami’s RI may be associated with a significant decline in vertical wind shear, but for RW, longer interaction with upwelling caused by almost stalled translation speed may be one of the major reasons.
AS13-A066
Rapid Intensification of Typhoon Chanthu (2021) Induced by Topographic Effects of Taiwan
Ya-Shin CHI1#+, Ching-Yuang HUANG1, William SKAMAROCK2
1National Central University, 2National Center for Atmospheric Research
Typhoon Chanthu (2021) underwent short-time rapid intensification (RI) when it moved northward offshore of east Taiwan. During this period, the typhoon environment is characterized by a deep-layer northwesterly vertical wind shear (VWS), as indicated by radar observations in Taiwan. The radial inflow at low levels is enhanced by the recirculating flow of Chanthu around south Taiwan when moving offshore along east Taiwan, against the upshear of VWS to facilitate RI. Simulations with a variable resolution of 60-15-1 km using the Model for Prediction Across Scales (MPAS) have successfully reproduced the RI and indicate an absence of RI as Taiwan terrain is removed in the simulation. To investigate the dynamic mechanism of Chanthu’s RI, the revised Sawyer–Eliassen (SE) equation is solved without the thermal wind balance for the axisymmetric mean vortex to identify the contributions from different nonlinear forcing sources configured in upshear-left (UL), upshear-right (UR), downshear-left (DL), and downshear-right (DR) quadrants of the inner vortex of Chanthu. The SE solutions indicate that diabatic cloud heating from the nonlinear simulations drives most of the secondary circulation, while the vortex spinup is also contributed by asymmetric eddy heat transport, especially in UL and DL quadrants. The asymmetric eddy momentum transport by the recirculating flow plays an important role in spinning up Chanthu, particularly in DR quadrant. In the absence of Taiwan terrain, Chanthu gradually weakens with time as without such asymmetric eddy transport.
AS13-A018
The Global Relationship Between Tropical Easterly Waves and Tropical Cyclone Genesis
Xueqing DU+, Jung-Eun CHU#, Zihao LIN
City University of Hong Kong
Tropical easterly waves (TEWs) are eastward-moving waves that occur within trade winds and play a significant role in the genesis of tropical cyclones (TCs). Previous studies have shown that over 75% of TCs in the North Atlantic (NA) originate from TEWs. Although TEWs and TCs are active in the eastern and western Pacific (EP and WP), studies of the relationship outside of NA have received less attention. This study uses ERA5 reanalysis and IBTrACS data to investigate the relationship between TEWs and TC genesis globally. The global pattern and vertical structure of TEWs are calculated using 2–10-day filtered curvature vorticity (CV) and TD-filtered outgoing longwave radiation (OLR). The findings demonstrate the value of CV as the indicator of TC genesis and reveal that more than 90% of the TCs are generated within the domain of TEWs, and over 70% of TCs are directly associated with TEWs globally. Specifically, 91%, 80%, and 65% of TCs are generated in the presence of cyclonic 850 hPa CV anomalies in the NA, EP, and WP, respectively. Furthermore, the study highlights the manifestation of upper-level anticyclonic CV anomalies during the genesis of TC, in addition to the low-level cyclonic CV anomaly. This study provides a comprehensive global perspective on the distribution of TEWs and their relationship to TC genesis, aiming to enhance our scientific understanding and prediction of TC formation.
Session Chair(s): Tuantuan ZHANG, Sun Yat-sen University
AS72-A001
A Seesawing Teleconnection Between Hydroclimatic Extremes in Southwestern and Northeastern China During the Winter and Early Spring
Kaiqiang DENG1#+, Song YANG1, Ke FAN1, Deliang CHEN2
1Sun Yat-sen University, 2University of Gothenburg
Global climate change has led to more frequent and intense dry and wet extremes, causing considerable socio-economic losses, but whether these extremes in distant regions are linked and what mechanisms are driving their changes remain unclear. Based on the standardized precipitation-evapotranspiration index and ERA5 reanalysis data, this study reveals a seesawing teleconnection between southwestern China (SWC) and northeastern China (NEC) from January to April: when SWC was extremely dry, NEC tended to be anomalously wet, and vice versa. Although the dry-wet teleconnection is most significant on interannual time scales, it also experienced interdecadal changes, with wet SWC and dry NEC in 1979-1998 and 2019-present and dry SWC and wet NEC in 1999-2018. Further investigations suggest that the dry SWC/wet NEC pattern is related to anomalous anticyclones (cyclones) over SWC (NEC), which lead to significant changes in surface temperature and precipitation in the respective regions. The dryness in western (eastern) SWC is mainly influenced by the changes in temperature (precipitation), while the NEC wetness is dominated by the changes in temperature. In addition, observational and modeling studies suggest that the high and low-pressure anomalies over SWC and NEC are caused by zonally and meridionally propagating Rossby wave trains, triggered by the North Atlantic Oscillation and the enhanced Indo-Pacific convection, respectively. These wave trains further lead to the interconnected hydroclimatic extremes in North America, southern Europe, and the Middle East during the JFMA by regulating the atmospheric circulation anomalies over these regions.
AS72-A018
Quantifying the Dynamical and Radiative Processes of the Drastically Weak South Asian Summer Monsoon Circulation in 2015
Wei YU1#+, Lianlian XU1, Song YANG1, Tuantuan ZHANG1, Dake CHEN2, Junwen CHEN3
1Sun Yat-sen University, 2Ministry of Natural Resources, 3Shenzhen Wiselec Technology Co. Ltd.
The South Asian summer monsoon (SASM) circulation in 2015 is the weakest since 2000s, which results in severe drought over broad regions of the Indian peninsula. The 2015 SASM is closely related to the weakened summer meridional thermal contrast between southern Eurasia (SE) and the tropical Indian Ocean (TIO) at the mid–upper troposphere. Based on an updated climate feedback-response analysis method, this study conducts a quantitative attribution analysis of the thermal contrast anomalies associated with the 2015 SASM to multiple dynamical and radiative processes, particular for aerosol process. Result shows that the 2015 weak SASM is mainly attributed to the effect of water vapor (58%), followed by the effects of atmospheric dynamics (18%), clouds (15%), and aerosols (15%), respectively. These positive effects are partially offset by the negative contribution from surface dynamic process (-14%). As the most pronounced factor, the water vapor process weakens the SASM circulation via inducing SE cooling and TIO warming, which is closely linked to the decreased (increased) specific humidity over SE (TIO). Further analysis indicates that the total effect of aerosols is dominated by the changes in black carbon and sea salt. As two important components, the SE cooling and TIO warming separately account for about 51% and 49% to the 2015 SASM. The former is mainly attributed to the cooling effect of clouds, while the latter is mainly induced by the warming effect of atmospheric dynamics. Our result provides a new insight into the 2015 weak SASM from a quantitative perspective.
AS72-A007
Impact of Madden–Julian Oscillation on East Asian Summer Monsoon Forecast for July 2020 in S2S Models
Jieun WIE#+, Jinhee KANG, Byung-Kwon MOON
Jeonbuk National University
The 2020 East Asian summer monsoon season experienced exceptional length and intensity, potentially linked to the Madden–Julian Oscillation (MJO). This study evaluates the MJO's role in the subseasonal-to-seasonal (S2S) model's forecasts for East Asian precipitation. The models generally underestimated cumulative precipitation over the region. However, superior forecasts showcased a distinctive East Asian precipitation band and a well-defined western Pacific subtropical high (WPSH). Notably, the accuracy of East Asian precipitation forecasts correlated more with the location of the WPSH's center than its strength, showing increased precipitation with a southward shift in the center's latitude. Activation of MJO Phases 1–3 intensified the WPSH, shifting its center to lower latitudes. These results suggest that the robust East Asian precipitation in the summer of 2020 was partly influenced by MJO characteristics. Accurate estimation of MJO-WPSH coupling is vital for dependable East Asian precipitation forecasts. Acknowledgments: This work was supported by the Korea Meteorological Administration Research and Development Program under Grant KMI2020-01212 and National Research Foundation of Korea (NRF) grant funded by the Government of Korea (MSIT) (No. 2022R1A2C 1008858).
AS72-A010
Investigating Global Warming Controls on Tropical Cyclone Rainfall Using Convection-resolving Model Experiments
Maiqian XIAO1#+, Francis Chi Yung TAM1,2, Chenxi HU1, Jilong CHEN3, Tsun Ngai CHOW4
1The Chinese University of Hong Kong, 2Shenzhen Research Institute, 3Shenzhen Institute of Meteorological Innovation, 4Department of Mathematics, The Chinese University of Hong Kong
As shown in numerous studies, the impact of tropical cyclones (TC) on coastal regions is expected to become stronger as the climate becomes warmer. However, large uncertainties exist in future projected storm intensity and rain rate under various warming scenarios. In this study, using the Weather and Research Forecasting model (WRF), pseudo-global warming (PGW) experiments for SSP2-45 and SSP5-85 targeted at the end of this century were conducted for 25 historical TCs having great impacts over the Pearl River Delta (PRD) region in South China. It was found that, averaged over all storm cases, the percentage change in extreme rain rate exceeds that given by the Clausius-Clapeyron (CC) relation. Moreover, TC rainfall increments can vary from one case to another, even due to the same PGW forcing. Further inspection revealed that such rainfall response fluctuation which cannot be explained by the CC relation can be attributed to the dynamical component in the moisture flux and its convergence, which in turn is related to changes in TC inflow in the planetary boundary layer when storm intensity increases. In other words, stronger projected TCs will lead to super-CC rainfall anomalies under global warming, with variations of storm response controlling TC rainfall fluctuations on a case-by-case basis. Implications of our results for estimating extreme rainfall in terms of its risks and uncertainties due to future TCs will be discussed.
AS72-A008
Sub-seasonal UK Winter Precipitation Intensifies In-line with Expected Temperature Scaling
James CARRUTHERS1#+, Selma GUERREIRO1, Hayley FOWLER1, Daniel BANNISTER2
1Newcastle University, 2Willis Towers Watson
Interannual to multi-decadal variability in large-scale dynamics such as atmospheric and oceanic circulation results in significant noise and temporary trends in regional climate. Attempting to understand longer term trends as a result of anthropogenic climate change requires disentangling internal variability and climate change signals. One of these climate signals is the Clausius-Clapeyron (CC) scaling in precipitation resulting from temperature increases. In this work, we characterise and constrain variability in sub-seasonal winter rainfall in the UK resulting from synoptic scale-conditions. The UK experiences periods of sustained precipitation in some winters which result in widespread flooding due to extreme accumulation. Using categorised sea-level pressure fields and gridded precipitation between 1900-2020, we simulate ‘expected’ precipitation resulting from North Atlantic synoptic conditions. We find a rising trend since the 1980s in observed monthly accumulation which is not reflected in the simulated precipitation timeseries, indicating that recent wet winters in the UK have been wetter than expected given the synoptic conditions. The rising trend in the residual (observed - simulated) mean monthly precipitation is in line with expected CC scaling rate of ~6-7% per degree warming according to changes in UK annual mean temperature. However, the residual in extreme monthly precipitation has scaled at approximately twice that rate. To better understand differences in changes for average and extreme precipitation accumulation, we explore the influence of dynamical feedbacks which may increase precipitation at higher intensities. We find that residual precipitation is influenced by the persistence of synoptic conditions and exhibits remote teleconnections to sea surface temperature and atmospheric conditions in the tropics and sub-tropics. This work highlights the importance of considering variability in large-scale dynamics when identifying climate change signals and sheds light on influences on sub-seasonal to seasonal winter precipitation in the UK.
AS72-A016
Disentangling the Unprecedented Yangtze River Basin Extreme High Temperatures in Summer 2022: Combined Impacts of the Re-intensified La Niña and Strong Positive NAO
Hongjie HUANG+, Zhiwei ZHU#, Juan LI
Nanjing University of Information Science & Technology
During July and August of 2022, the Yangtze River Basin (YRB) experienced its most extreme high temperature (EHT) event since 1979, resulting in large numbers of human casualties and severe economic losses. This paper reveals the spatial and temporal features of the EHT over the YRB (YRB-EHT) in 2022 and disentangles its extreme nature from a historical perspective. Results showed that: (1) The record-breaking YRB-EHT was directly caused by the adiabatic heating associated with an anomalous barotropic high pressure (or heat dome) and descending motion in the region. The intensified and westward-shifted western North Pacific subtropical high and eastward-extended South Asian high played critical roles in the formation of the heat dome and descending motion anomaly. (2) Convection anomalies over the tropical Atlantic and Pacific induced by the re-intensified La Niña-like Pacific sea surface temperature anomaly pattern, along with the strong positive North Atlantic Oscillation (NAO), were the key contributing factors to the formation of the barotropic high pressure anomaly and YRB-EHT. (3) A physics-based empirical simulation model constructed using the factors of the NAO and tropical convection successfully reproduced the historical year-to-year variation of YRB temperatures, as well as the extreme in 2022, implying that the unprecedented 2022 YRB-EHT had universal dynamic origins. This study highlights the importance of the combined impacts of tropical and extratropical forcings in the record-breaking YRB-EHT in 2022, and thus may provide useful clues for seasonal predictions of summer mean or extreme temperatures in the YRB.
AS72-A023
Paradigm Shift in Compound Warm Events: Dominance of Warm-wet Events in Ice-covered Regions Versus Warm-dry Cases in Non-ice-covered Zones
Xinlu CHEN1, Xiaoming HU1#+, Ran YANG1, Lianlian XU1, Yi DENG2, Ming CAI3
1Sun Yat-sen University, 2Georgia Institute of Technology, 3Florida State University
In regions covered by ice sheets, a paradigm shift characterizes compound warm events, predominantly manifesting as warm-wet events (WWE), in stark contrast to non-ice-covered regions where warm-dry events (WDE) prevail. This shift is primarily attributed to the weakened coupling between the atmosphere and surface, facilitated by the barrier effect of ice cover. This stands in contrast to the robust air-land coupling observed during warm-dry events in non-ice-covered regions. Exploring the mechanisms of WWE and WDE, four representative regions, including Greenland, West Antarctica, Europe, and South China are selected to analyse and compare the key processes of WWE and WDE. Both WWE and WDE are coincided with high-pressure systems, yet their spatial occurrences within dominant system differs. WDE position themselves directly beneath the high-pressure system, while WWE manifest on the poleward side. This spatial disparity highlights the nuanced dynamics of compound events in ice-covered and non-ice-covered regions. Crucially, the causative mechanisms vary for these events. WWE are predominantly triggered by the intrusion of warm and moist air from lower latitudes to high latitudes, while WDE primarily result from the adiabatic warming of localized air, which is controlled by high-pressure system and further enhanced by the decreased soil moisture. This additional distinction adds complexity to our understanding of the mechanisms driving warm-wet and warm-dry compound events in different geographical locations.
AS72-A020
Extremely Strong Western Pacific Subtropical High in May 2021 Following a La Niña Event: Role of the Persistent Convective Forcing Over the Indian Ocean
Minling KE1+, Ziqian WANG1#, Weijuan PAN2, Haolin LUO1, Song YANG1, Ruyue GUO1
1Sun Yat-sen University, 2Guangzhou Meteorological Administration
The variation of the western Pacific subtropical high (WPSH) significantly influences the weather and climate in East Asia. El Niño-Southern Oscillation (ENSO) is considered as one of the most important factors for the abnormal activity of the WPSH. An El Niño event tends to result in an anticyclonic anomaly over the western Pacific in the following spring and summer, leading to a westward-shifted and stronger WPSH. Opposite features can be observed for a La Niña event. Following the typical La Niña event in the winter of 2020/2021, an abnormal cyclonic circulation routinely appeared over the western Pacific in the beginning of 2021, but it was suddenly replaced by an obviously abnormal anticyclone in May. This unanticipated change induced an extremely strong WPSH and posed a challenge for the regional climate prediction. A careful examination of the tropical Indian Ocean revealed a significant abnormal warming process from April to May in 2021, with a peak of positive sea surface temperature anomaly (SSTA) in early May. Consequently, persistent atmospheric convective activity was stimulated by the positive SSTA, accompanied by remarkable and eastward-moving diabatic heating in the tropical Indian Ocean. The convective heating aroused significant easterly anomalies in the form of a Kelvin wave response of the Gill-type mode over the equatorial region from the western Pacific to the eastern Indian Ocean, which induced an abnormal anticyclone through a further positive circulation-convection feedback over the western Pacific. Additional experiments with the LBM model further verify that the persistent convective forcing over the tropical Indian Ocean is responsible for the extremely strong WPSH in May 2021, although during an antecedent La Niña event.
AS72-A012
Comparison on the Modulation Modes on Global Wildfire Activities Driven by Four Types of ENSO from 2001-2020
Fangzhou LI#+
Peking University
ENSO modulates the wildfire activities via interacting with the regional weather conditions, while its dominant meteorological driver varied spatially. In this study, we aim to identify the modulations on global wildfire activities due to four types of ENSO (including the traditional ENSO, such as EP El Niño and EP La Niña, CP El Niño, and CP La Niña) using statistical methods and the latest datasets from 2001-2020. Among the 14 regions suggested by the GFED, the most modulated regions by ENSO are NHSA (Northern Hemisphere South America), EQAS (Equatorial Asia), TENA (Temperate North America), AUST (Australia and New Zealand), and SHSA (Southern Hemisphere South America). It is worth noting that TENA and SHSA regions, located over the east to the Pacific Ocean, share the same modulation mode by ENSO, as enhanced by La Niña while inhibited by El Niño. The other three regions, as NHSA, EQAS, and AUST regions, share the same modulation mode by ENSO, as enhanced by El Niño while inhibited by La Niña.
AS72-A014
Observations of Severe-wind Driven and Other Wildfires with Doppler on Wheels (DOW) Mobile Radars
Karen KOSIBA1#+, Joshua WURMAN2
1University of Alabama Huntsville, 2University of Illinois
Doppler On Wheels (DOW) mobile / targetable truck-borne radars have deployed to collect fine-scale observations in several wildfires, one, recently, causing widespread destruction in an urban area. DOW measurements in wildfires permit the mapping of the windfields, hydrometeors, and airborne particles in the fire plumes, and characterization of the near-fire environment. DOWs can collect windfield and other data below the observing horizon of more distant radars, and at much finer-scale spatial resolution, revealing otherwise unmappable aspects of low-level and small scale structure and evolution. Observations of three wildfires will be discussed: In 2020, two DOWs deployed in the mountains of Colorado and collected dual-Doppler vector wind data primarily in the fire environment. During another fire in 2020, the DOWs were deployed close to wildfires which destroyed many homes. Small-scale vortices and other features are resolvable due to the close proximity of the deployed radars to the wildfires. Dual-Doppler DOW analysis, the first fine-scale dual-Doppler analysis of this type, will be presented. In 2021, a DOW deployed in South Boulder, Colorado in the metropolitan Boulder wildfire / extreme wind event where winds exceeding 45 m/s enhanced fires which destroyed many homes and businesses in the south Boulder area. The evolution of the wind field was mapped.
Session Chair(s): Bingliang ZHUANG, Nanjing University
AS75-A012
| Invited
North China Plain as a Hot Spot of Ozone Pollution Exacerbated by Extreme High Temperatures
Pinya WANG#+
Nanjing University of Information Science & Technology
A large population in China has been exposed to both severe ozone (O3) pollution and extreme heat under global warming. Here, the spatiotemporal characteristics of coupled extremes in surface O3 and heat (OPCs) over China are investigated using surface observations, a process-based chemical transport model (GEOS-Chem), and multi-model simulations from Phase 6 of the Coupled Model Intercomparison Project (CMIP6). North China Plain (NCP; 37–41◦ N; 114–120◦ E) is identified as a hot spot of OPCs, where more than half of the O3 pollution days are accompanied by high temperature extremes. OPCs over NCP exceeded 40 d during 2014–2019, exhibiting an increasing trend. Both O3 concentrations and temperatures are elevated during OPCs compared with O3 pollution days occurring individually (OPIs). Therefore, OPCs impose more severe health impacts to humans than OPIs, but the stronger health effects are mainly driven by the higher temperatures. GEOS-Chem simulations further reveal that enhanced chemical production resulting from hot and stable atmospheric conditions under anomalous weather patterns primarily contributes to the exacerbated O3 levels during OPCs. In the future, CMIP6 projections suggest increased occurrences of OPCs over NCP in the middle of this century, but by the end of this century, OPCs may decrease or increase depending on the pollutant emission scenarios. However, for all future scenarios, extreme high temperatures will play an increasingly important role in modulating O3 pollution in a warming climate.
AS75-A005
| Invited
Impacts of Synoptic Forcing and Cloud Inhibition on Aerosol Radiative Effect and Boundary Layer Structure During Winter Pollution in Sichuan Basin, China
Hua LU#+
Chongqing Institute of Meteorological Sciences
With high aerosol loadings and semi-permanent cloudy weather, Sichuan Basin is an optimal region for studying the influence of synoptic forcing on the interactions between clouds, aerosols, and boundary layer. Through synoptic pattern classification, two predominant pollution 850hPa synoptic patterns characterized with east high west low (EHWL) pressure system and low trough (LT) were identified to be associated with denser liquid cloud, which contributed to obvious cloud radiation interaction(CRI) and aerosol accumulation. Numerical simulation experiments using WRFCHEM showed CRI significantly inhibit aerosol radiation interaction(ARI) under wet and cloudy synoptic forcing. CRI was more pronounced with LT pattern, as a result, CRI inhibition on ARI could cause a 50 % reduction in solar radiation and boundary layer height during the daytime with LT pattern, which obviously surpass that with EHWL pattern. The results revealed non-negligible role of cloud inhibition on ARI under typical pollution synoptic patterns in wet and cloudy regions.
AS75-A008
Inversion of SO2 Emissions Based on Four-dimensional Variational Assimilation and Its Application in the Spring Festival of 2023
He XINYU1#+, Zengliang ZANG1, Li YI1, Hu YIWEN1, Lang LIU2
1National University of Defense Technology, 2Chinese Academy of Sciences
2023年春节期间,许多城市政府放松了对居民燃放烟花爆竹的限制。烟花爆竹含有大量硫粉,快速燃烧时会释放出有毒的空气污染物二氧化硫(SO 2)。因此,SF期间燃放烟花爆竹可能会导致短期内爆发空气污染。在本研究中,我们采用四维变分(4DVar)同化系统,通过 同化每小时的地面观测数据来研究中国SO 2排放的变化。在2022年和2023年的SF期间进行了两组实验,以量化SO 2 排放量的变化。2023年除夕期间,由于烟花爆竹限制放宽,全国除夕夜SO 2 排放量较前一天大幅增加,远高于2022年除夕夜。特别是东北、华北地区中国平原和能源金三角地区由于大量燃放烟花爆竹,是增量排放的主要地区。在除夕达到峰值后,2023年春节期间全国SO 2 排放总量在接下来的两天内迅速下降至大规模烟花燃放活动前的水平。这些发现将有助于地方政府制定SF期间烟花燃放策略。
AS75-A021
Influence of Weather Systems on Synergy of O3 and PM2.5 in China
Lv SHUN#+, Min SHAO, Zihang LIAO
Nanjing Normal University
PM2.5 pollution and O3 pollution continue to threaten air quality and people's health in China. In addition to excessive anthropogenic emissions, adverse weather systems are also important causes of pollution. The study on the co-pollution of PM2.5 and O3 caused by different weather systems and their compounds can provide theoretical basis for the prevention of regional pollution. Based on the monitoring data of China's national Air quality stations and ERA5 reanalysis data, the effects of different weather systems on PM2.5 and O3 co-pollution in the Beijing-Tianjin-Hebei region (BTH), the Yangtze River Delta region (YRD) and the Pearl River Delta region (PRD) of China from May 2014 to July 2022 and the potential mechanisms were analyzed. The results show that there are great differences in the pollution status of different regions under the same weather system under different co-pollution definitions. In the PRD, the frequency of double-high pollution under TH90 standard is higher and is more affected by heat wave. Under the 75/160 (ug/m3) standard, double-high pollution occurs more frequently in the BTH, which is more affected by heat wave and southerly monsoon. In the YRD, the frequencies of double-high pollution under different co-pollution definitions are close, and the influences of the south and north monsoon are greater. The cold wave has a strong effect on the double-high pollution in the BTH, and a small effect on the PRD and the YRD, and the pollution occurs the day before the cold wave in most cases. Through the study of the underlying mechanism, it is found that double-high pollution is easier to occur under the weather conditions of low relative humidity, high temperature and low wind speed. At the same time, it is found that the regional transport of pollutants caused by cold wave will also cause double-high pollution.
AS75-A006
Meteorological Impacts on P-O Pollution Under Diverse Synoptic Weather Patterns in the Yangtze River Delta, China: Synergistic Relationships Between Particulate Matters and Ozone
Yangzhihao ZHAN1#+, Min XIE2
1Nanjing University, 2Nanjing Normal University
The interaction between fine particulate matter (PM2.5) and ozone (O3), known as the P-O relationship, garners considerable global academic interest. We did an innovative investigation by quantitatively assessing the variations in the P-O relationship under various synoptic weather patterns (SWPs). First, by using the sums-of-squares (SS) technique classification method, the SWPs classification was conducted in the Yangtze River Delta (YRD). The results indicate that there are five dominant SWPs in the YRD, including the Aleutian low under SWP1 (occurrence of 45.3 % of the days of the year), an extra-tropical cyclone under SWP2 (21.5%), the western Pacific Subtropical High (WPSH) and tropical cyclone under SWP3 (15.4 %), the WPSH under SWP4 (6.9 %), and a continental high pressure under SWP5 (3.1 %). Second, the effects of meteorology on air pollution under different SWPs in the YRD are studied. High mean PM2.5 concentrations are found under circumstances with higher relative humidity (RH), which are generally associated with the strengthening of the northerly winds introduced by the North China cold high. On the other side, the westward extension of the WPSH leads to hot, dry, and stagnant weather, which is favorable for high levels of O3 pollution. Third, the partial correlation analysis is employed to quantify the separate contribution of meteorology and emissions to the P-O relationship. The meteorological variables can explain only 24% of the PM2.5 variations, but 68% for O3. For SWP2 and SWP3, the photochemical reactions and atmospheric oxidizing capacity are intensified, which can cause a significant rise in O3. For SWP1, SWP4, and SWP5, high PM2.5 pollution increases the absorption of free radicals at the aerosol surface, and secondary inorganic aerosols reduce the radiative effects of aerosols. Reducing PM2.5 and NOX emissions may not necessarily reduce O3 concentrations due to the non-linear relationship between O3 and its precursors.
AS75-A010
Characteristics of Urban Black Carbon Aerosols in the Yangtze River Delta of China Based on Long-term Observations
Yinan ZHOU+, Bingliang ZHUANG#, Peng GAO, Yaxin HU, Heng CAO, Shanrong LIANG
Nanjing University
Black carbon (BC) aerosols are important absorbing components that can impact the regional climate and environment. To better understand the BC effects, long-term variations in BC concentrations and the relationship between BC and other air pollutants are investigated in urban Nanjing of the Yangtze River Delta (YRD) based on near-nine-year observations using a seven-channel aethalometer (AE-31). BC concentrations in YRD city have substantial seasonal and diurnal variations, which are higher in winter (rush hours) and lower in summer (at noon). They have a significant declining trend since 2013 when the Action Plan for Air Pollution Prevention and Control was carried out, which was reduced by at least 45% from 2013 to 2019, and the same applies to heavy pollution episodes. The aerosol absorption coefficient (AAC) has similar temporal variations to BC concentration because BC is the dominant component of absorbing aerosols (>80% at 550 nm). Investigations also indicate that the average contributions of BC from biomass burning (BCbb) and fossil fuel (BCff) to the total BCs concentration could be of equal importance. However, the ratios of BCbb to the total BCs in colder seasons are much higher than those in summer. Nevertheless, both BCbb and BCff might significantly contribute to the high BC loadings in particulate pollution episodes. Further comparisons show that BCs have substantial positive correlations with CO and PM2.5. The relationships between BC and CO imply that the sources of fossil fuel BC aerosols in Nanjing might mainly come from the combustion of industrial coal and gasoline vehicles. An extremely high BC loading or higher BC/PM2.5 ratio always corresponds to a lower O3 concentration, implying that BC might have a substantial influence on O3 formation.
Session Chair(s): Dan LI, Boston University, Ning ZHANG, Nanjing University
AS91-A008
| Invited
Numerical Simulation of Urban Climate in East China with CLM5-LCZs
Ning ZHANG#+
Nanjing University
The urban expansion-induced heat can exacerbate heat stress for urban dwellers, especially during heat waves. The urban parameterization within the Community Land Model version 5 (CLM5) was developed by incorporating the local climate zones (LCZs) framework, named CLM5-LCZs, to simulate the urban climate in eastern China. The results exhibited that daytime and nighttime canopy urban heat island intensity (CUHII) were highest in the Compact Low Rise (LCZ3) and the Compact High Rise (LCZ1) areas respectively, while surface urban heat island intensity (SUHII) peaked in the Large Low Rise (LCZ8) and the Compact High Rise (LCZ1) areas during daytime and nighttime respectively. Urban dwellers were easier exposed to serious heat environment in LCZ3 and LCZ1 areas over the north subtropical climate zone. Contrasts of CUHII and SUHII among different urban classes could exceed 1.7 °C and 5.4°C. The intra-urban heterogeneity may alter the dominant factors controlling SUHII, which were also modulated by local climate and heat wave intensity. Overall, CLM5-LCZs displayed potential of implementing detailed simulations for inter- and intra-city UHIs at a larger scale, and enhancing the capabilities in modelling urban climate and exploring the causes and controls of UHIs.
AS91-A007
Database Construction of Urban Geometric Parameters with Individual Building GIS and Examination of Method of Estimating Building Parameters Using Open DSM Data
Asahi KAWAURA#+, Makoto NAKAYOSHI
Tokyo University of Science
Thermal and aerodynamic properties derived from urban geometry are one of the most important factors in describing specific climates in urban area. In recent years, due to advancements of parameterizations of physical process in the canopy layer, such as single-layer urban canopy model (Kusaka et al., 2001), it has become possible to conduct mesoscale simulations that more accurately account for these properties. Moreover, it is necessary to accurately incorporate aero-thermodynamic parameters such as roughness length, displacement height and sky view factor for high accuracy simulations. The aerodynamic parameters are modeled associated with the building geometry array and calculable by five building morphological parameters, i.e., average building height, maximum building height, standard deviation of building heights, plane area index and frontal area index according to Kanda et al. (2013). Since the calculation of these parameters requires detailed building information, it is common in many previous studies to use aero-thermodynamic parameters based on urban classifications such as Local Climate Zones (Stewart and Oke, 2012). Recently, in major developed countries, high-resolution building GIS has been available as open data. In this study, we constructed the database of urban geometric parameters for the entire Japan and the United States with open building datasets. In addition, we examined the calculation algorithm of urban geometric parameters from open Digital Surface Model (DSM) of ALOS World 3D-30m to expand the database globally for mesoscale to GCM simulation. The algorithm includes the correction of the DSM (hereafter nDSM) based on spatial filtering and the correction of road and forest heights in nDSM using building footprint data of Microsoft Building Footprints. The details of the constructed database and the calculation result of urban geometric parameters by the algorithm will be presented at AOGS2024.
AS91-A010
How Do Urban Heat and Roughness Over a Coastal Megacity Affect Landfalling Tropical Cyclone Intensity? A Case Study Based on TC Victor (1997)
Chenxi HU1#+, Francis Chi Yung TAM1,2, Zhenning LI3, Jilong CHEN4, Yubin LI5, Kevin CHEUNG5, Zong-Liang YANG6, Jung-Eun CHU7, Tsun Ngai CHOW8
1The Chinese University of Hong Kong, 2Shenzhen Research Institute, 3The Hong Kong University of Science and Technology, 4Shenzhen Institute of Meteorological Innovation, 5Nanjing University of Information Science & Technology, 6The University of Texas at Austin, 7City University of Hong Kong, 8Department of Mathematics, The Chinese University of Hong Kong
This study investigates the impacts of urban-induced anthropogenic heat (AH) and surface roughness on Tropical Cyclone (TC) Victor (1997) using the Weather Research and Forecasting (WRF) model. Originating in the South China Sea (SCS) and making landfall over the Greater Bay Area mega-city, TC Victor was characterized by slow movement, loose structure, and a small size. Three parallel experiments were conducted: “Nourban”, where urban areas in the GBA were replaced by cropland, “AH0” (“AH300”) in which the diurnal maximum AH was set to 0 (300W/m2) in city locations. Reduction in both the Power Dissipation Index (PDI) and Integrated Kinetic Energy (IKE) of the storm by urbanization was found during the landfall period. Specifically, a 6.4% in PDI and 4.2% in IKE decrease for AH0 and a more pronounced 27.7% in PDI and 9.2% in IKE decline for AH300 were found compared to Nourban. Lagrangian particle dispersion model further shows that, from 33 to 17 hours pre-landfall, the entrainment of AH-induced hot and arid air into TC secondary circulation led to a diminution of the Convection Available Potential Energy (CAPE) and inertial stability, thereby attenuating the cyclone's development. Further, from 15 hours pre-landfall to 8 hours post-landfall, an intense influx of AH-induced hot and dry air into the TC’s primary circulation, substantially decreased mid-level relative humidity, and further declined the TC intensity. Concurrently, urban surface roughness contributed to a decrease in post-landfall storm intensity through frictional energy dissipation. Moreover, AH decreases rainfall in the TC core but increases it in the southern outer rainbands, while urban surface roughness enhances rainfall in the TC core due to increased frictional convergence. This study underscores the critical role of extreme AH and urban roughness in modulating TC intensity for storms with specific characteristics, emphasizing the need for deeper insights into urban-TC dynamics.
AS91-A014
Impact of Urban Canopy Physics and Detailed Urban Canopy Parameters on High-resolution Simulation Over Two Large Urban Agglomerations in China
Xiangyu AO1#+, Wei HUANG1, Ning ZHANG2
1China Meteorological Administration, 2Nanjing University
Urban physics schemes and urban canopy parameters (UCPs) are vital for fine-scale weather simulations. This study evaluates the impact of different urban canopy schemes and high-resolution UCPs on meteorological fields over two largest urban agglomerations in China against dense automated weather stations for a summer day case with a high-resolution regional operational model. Results show that the single layer urban canopy model (SLUCM) with more realistic building heights mainly has a cool effect which increases the cold bias while decreases the warm bias over the YRD (Yangtze River Delta) and PRD (Pearl River Delta) region, respectively. The simulated 2-m temperature (t2) with the multi-layer urban canopy model (BEP) is slightly better than that of the SLUCM. The SLUCM with optimized building heights significantly reduces overestimation of the 10-m wind speed (ws10). The BEP scheme is obviously superior to SLUCM in ws10 simulation throughout the day over the entire region. The use of gridded UCPs in BEP only has a marginal improvement for t2 and ws10 simulation which may be due to the offset of opposite effect for areas with low and tall buildings. Planetary boundary layer (PBL) scheme has a large impact on the performance of SLUCM over the YRD region: Boulac scheme improves (degrades) the underestimation (overestimation) of nocturnal t2 (ws10) compared to the YSU scheme. This study provides guidance for applying urban canopy schemes into regional operational models and improves understandings of key processes over urban areas.
AS91-A017
A Vehicle-based Observation System Towards Collecting Near-ground Meteorological Big Data
Yuma MATSUDA#+, Shiho ONOMURA, Makoto NAKAYOSHI
Tokyo University of Science
In recent years, the harmful impacts of heat island phenomena and torrential rains are becoming apparent in cities, increasing the demand of the denser ground meteorological data. However, the current fixed observations are operated in the limited number of sites, those are not enough to figure out spatially and temporally various atmospheric fields. Mobile observation is one of the potential methods to overcome the situation of the current near-ground meteorological observation. In previous studies, ordinal meteorological sensors were mounted on vehicles and the comprehensive observation results showed that the method was proven to be viable over the world. However, since those studies installed large stationary sensors in vehicles, the complexity of the setup poses a challenge, requiring substantial efforts and limiting observations to short term. In pursuit of leveraging vehicles for high-density meteorological data acquisition, careful consideration must be given to the installed observation devices in terms of the compactness, security, handiness, and the management of data quality. In this research, we developed a compact monitoring system for vehicle-based meteorological observation, which measures air temperature, humidity, pressure, horizontal wind direction and speed, together with GNSS data and the vehicle travelling data. Those data are transmitted to a cloud server in real time. The system consists of a single-board computer and tiny IoT devices, which are commercially available and low-cost, and make it easy to construct the system. To examine the sensors' appropriate placements on vehicles, the prototype system was installed in a vehicle, and a comparison with stationary observation values was conducted. The results implied that there were some influences of solar heating and heated vehicle’s body, remaining issues in sensor housing. However, during nighttime, the device consistently provided reliable meteorological measurements (nighttime air temperature RMSE = 0.53 ℃). We will present the mobile observation results.
AS91-A018
Land-surface-physics-based Downscaling: A New Approach for Urban Climate Prediction
Lingbo XUE1+, Quang-Van DOAN1#, Hiroyuki KUSAKA1, Cenlin HE2, Fei CHEN3
1University of Tsukuba, 2NSF National Center for Atmospheric Research, 3The Hong Kong University of Science and Technology
The demand for substantial computational resources in dynamical downscaling (D-DS) has hindered extensive exploration of urban climate prediction, especially concerning long-term and high-resolution scenarios. To address this gap, we propose a novel downscaling approach: Land-Surface-Physics-Based Downscaling (LSP-DS). This innovative approach aims to conduct high-resolution, long-term urban-specific simulations with significantly reduced computational requirements. LSP-DS combines the widely used Noah-Multiparameterisation (Noah-MP) land surface model with urban canopy-process physics, forced by rough-resolution reanalysis or numerical modelling data. Our evaluation of LSP-DS focuses on simulating the synergies between the urban heat island (UHI) effect and heat waves (HWs), using the Tokyo area as a case study. The analysis, which combines observational data with a large number of LSP-DS simulations, confirms that the impact of UHI is exacerbated during periods of HWs. To further assess LSP-DS’s performance, we conduct a comparative analysis with conventional direct D-DS over the past decade in the Tokyo and Singapore regions. This comprehensive comparison includes observational and reanalysis data, covering basic meteorological variables, specific extreme weather indicators, and computational resource consumption. Additionally, we provide an assessment and summary of the strengths and weaknesses of LSP-DS, offering guidance to potential users considering this approach for urban climate downscaling.
AS91-A019
Comparison and Validation of Bulk Transfer Coefficient Determination Methods in Urban Canopy Models
Natsuki CHIBA#+, Makoto NAKAYOSHI, Asahi KAWAURA
Tokyo University of Science
In recent years, there has been increasing attention to meteorological phenomena specific to urban areas due to the progression of global warming and urbanization. In the 2000s, the development of urban canopy models that considered the geometric structure of cities advanced. By incorporating these models into the Weather Research and Forecasting (WRF) model, there was an improvement in reproducing urban climate more accurately (Kusaka et al., 2001). In the surface layer, the bulk method is employed for the calculation of heat fluxes. Regarding the modelling the bulk transfer coefficient, generally two approaches were applied in single-layer urban canopy models. Though comprehensive model comparisons were done in Grimmond et al. (2010) in terms of multiple aspects including urban morphology, the impact of the different treatment of bulk transfer modelling have not been clarified. This study aims to address this. In the top-down approach, each urban canopy constituent (roof, wall, ground) is assumed to be directly linked with the above atmosphere and the heat transfers are independent each other; the total sensible heat flux from these components represents the entire sensible heat flux over the urban canopy (Kawai et al., 2005). In the bottom-up approach, it is assumed that the wall and ground surfaces exchange its heat with the urban canyon first then they are transferred to the above atmosphere, while the roof surface exchanges them directly with the above atmosphere. The total sensible heat flux of the entire urban canopy is the sum of those from the roof surface and the urban canyon (Kusaka et al., 2001). This study compares and examines the accuracy of the two methods using data obtained with flux towers in Tokyo (Moriwaki and Kanda, 2011), Vancouver (Christen et al., 2011), and London (Grimmond and Christen, 2012). The results will be presented at AOGS2024.
AS91-A023
Energy Cascading During Extreme and Calm Weather Scenarios Over Urban Atmosphere: Insights from Cube Computational Fluid Dynamics Model
Rakesh Teja KONDURU#+, Rahul BALE
RIKEN Center for Computational Science
In urban environments, the intricate interplay of diverse motion scales, ranging from small-scale turbulent activities near the surface to mesoscale atmospheric circulation patterns, exerts substantial influence over energy transfer and dissipation within the atmosphere. Accurate weather prediction and the development of sustainable urban areas hinge on unravelling these interactions. The urban landscape, marked by high concentrations of buildings, roads, and infrastructure, departs significantly from natural surfaces like forests, resulting in disparities in heat absorption and emission. This divergence disrupts the urban-rural energy equilibrium, leading to distinctive energy cascades over urban regions. Although past research has predominantly explored the impact of urban-scale environmental changes on local weather patterns, there remains a critical knowledge gap regarding energy cascading from the broader mesoscale to the smallest turbulent scale due to alterations in the grid-to-urban scale environment. Our study aims to bridge this gap by utilizing CUBE LES over FUGAKU supercomputer to model complex urban geometries and employing Immersed Boundary Methods (IBM). We will investigate 1-m to 5-m LES simulations under diverse wind conditions, including Calm and Extreme weather (Typhoon) scenarios, as they interact with the urban canopy. Our approach dissects energy scales within urban contexts into distinct spatial and temporal modes, thus deepening our understanding of energy transfer and dissipation mechanisms. Specifically, we seek to identify the fundamental scales of energy transfer, offering insights into scale interactions and enhancing our capacity for severe weather prediction in urban environments.
Session Chair(s): Jason EVANS, University of New South Wales, Dong-Hyun CHA, Ulsan National Institute of Science and Technology
AS65-A015
Including Observational Uncertainty in Climate Model Evaluations
Jason EVANS#+, Hosen IMRAN
University of New South Wales
Model evaluations are performed by comparing a modelled quantity with an observation of the same quantity. The observation is generally considered the “truth” and any deviation from this observed quantity is considered an error. However, we know that all observing systems have uncertainties or errors associated with them. When using gridded observations there are additional uncertainties introduced by the gridding process. Investigation of multiple different gridded observational products for the same quantity reveals a range of equally plausible “truths”. Thus, the model errors identified depend intimately on the choice of observational product used in the evaluation exercise. In acknowledgement of this problem, some previous studies have repeated the evaluation exercise against several observational products and then used the average (or similar) of these results as the overall outcome. Which is a better though, we suggest, an inadequate approach. Here we proposed a method that means models are only considered to be in error when they lie outside the range given by several observational datasets (and their internal uncertainties). In practice, this approach requires the production of a pseudo-observation dataset that is equal to: the maximum observation when the model exceeds all observations; the minimum observation when the model falls below all observations; and the model value when it lies within the observational range and hence it is considered to be indistinguishable from observations. This pseudo-observation data can then be used within traditional statistics to calculate the Observation Range Adjusted (ORA) version of that statistic. This talk demonstrates the technique along with its impact on model evaluation.
AS65-A013
Toward Accurate Future Climate Projections: Multivariate Bias Correction in RCM Boundaries
Youngil KIM#+, Jason EVANS
University of New South Wales
High-resolution hydro-climatological simulations are essential for assessing changes in extreme events. Regional climate models (RCMs) forced with global climate models (GCMs) data are commonly used to provide regional-scale output. However, the inherent systematic biases in GCM-derived input boundary conditions hinder their application for future projections. These biases can be amplified further within the RCM domain, thereby impeding the effective use of climate projections in impact studies, such as the impact of future climate change on water resources and agricultural sectors. Hence, this study undertakes a comprehensive evaluation of multivariate bias correction applied to RCM boundary conditions for future climate projections. This approach, notable for correcting cross-dependence structures among atmospheric variables, has enhanced the simulation accuracy of extreme precipitation and compound events. In this study, the Weather Research and Forecasting model (WRF) with dynamical core (ARW), version 4.2.1, was used for RCM, and a bias-corrected global dataset from the Coupled Model Intercomparison Project Phase 6 (CMIP6) was used to provide the necessary input boundary conditions for the RCM. ERA5 data from the European Centre for Medium-range Weather Forecasts (ECMWF) was also employed as a reference for the bias correction process. The downscaling was performed over the Australasian Coordinated Regional Climate Downscaling Experiment (CORDEX) domain.
AS65-A006
Sensitivity of Summer Precipitation Simulation to the Physical Parameterizations in WRF Over the Tibetan Plateau: A Case Study of 2018
Peifeng ZHOU1#+, Jianping TANG1, Min SHAO2, Mengnan MA1
1Nanjing University, 2Nanjing Normal University
The Tibetan Plateau (TP) holds a pivotal position in regional and global climate, whereas the atmospheric characteristics vary greatly in the simulation with different physical parameterization schemes at the convective gray-zone scale (around 9 km). In this study, 24 sets of experiments were set up with different cumulus parameterization schemes (CPSs), microphysics parameterization schemes (MPSs) and planetary boundary layer parameterization schemes (PBLSs) using the WRF model driven by the ERA5 reanalysis to explore the sensitivity and try to summarize a combination of parameterization schemes suitable for the simulation over the TP. Based on comparisons against in-situ observations, most CPS experiments showed large wet bias and overestimated occurrence of precipitation events, and CTL without CPS and the experiment with Tiedtke CPS show better performance. The influence of MPS and PBLS is less than CPS on the simulation, and Thompson MPS and UW PBLS showed a better performance. Most CPS experiments reach an earlier and more intensive peak compared to the IMERG version 6 satellite precipitation product, except the experiments without CPS, and with Tiedtke or Multi-scale KF, which show closer but weaker peaks. CPS experiments simulate more precipitation associated with water vapor transporting into TP and anomalous cyclonic circulation against the experiment without CPS. Graupel particles and the warm-rain process play a crucial role in the precipitation simulation with different MPSs. Although with less water vapor in the low atmosphere, Lin MPS simulates more precipitation due to more graupel particles and warm-rain processes against CTL with Thompson MPS. PBLSs have a impact on latent heat, then influence evaporation and precipitation. The lower PBL height usually leads to more latent heat and more precipitation. This study will provide experience for promoting a benchmark combination of parameterization schemes and exploring more added value from long-term gray-zone dynamical downscaling simulation over the TP.
AS65-A031
Impact of Planetary Boundary Layer Parameterization Schemes on Systematic Winter Temperature Errors of a Regional Climate Model
Seok-Woo SHIN1+, Minkyu LEE2, Taehyung KIM1, Changyong PARK1, Woojin CHO1, Hongjun CHOI1, Dong-Hyun CHA1#
1Ulsan National Institute of Science and Technology, 2Korea Institute of Energy Research
The dynamical downscaling technique can provide more detailed information on regional scale phenomena over a region of interest in the global data using high-resolution. Regional climate models (RCMs, i.e., WRF) can be a powerful tool for improving our understanding of regional climate dynamical and physical processes. However, systematic temperature errors in RCMs were most prominent in the winter, particularly in Manchuria (MC). Reducing temperature errors is necessary for accurate future projections and air quality forecasts. Although alternative methods such as multi-model ensemble or bias correction are being used, these cold biases have not yet been fully addressed. Meanwhile, the choice of the physical parameterization schemes from region to region influences in the model performance. In particular, the planetary boundary layer (PBL) parameterization schemes play a crucial role in temperature biases related to PBL mixing, which causes the exchange of moisture, heat, and momentum. Therefore, in this study, the sensitivity experiments according to different PBL schemes (YSU, ACM2, MYNN2.5, UW, and MYJ) were conducted to understand those impacts on systematic temperature errors over the MC. The systematic temperature errors and atmospheric fields were analyzed using observation [APHRODITE and the global telecommunications service (GTS) radiosonde data, etc.], reanalysis [ERA5, etc.], and WRF experiments data. As a result, the ACM2 PBL scheme reduced the cold temperature errors in the MC region shown in other PBL schemes. The ACM2 PBL scheme improved the model performance over East Asia in the relationship among the temperature bias, low-level wind, and zonal pressure contrast between the Siberian high and Aleutian low. In the ACM2 PBL scheme run, smaller PBL mixing in the nighttime decreased cold temperature biases by less descending cold air to the surface.
AS65-A037
Policy-relevant Regional Climate Information for Societal Needs
Koji DAIRAKU#+, Saurabh KELKAR, Ermias Sisay BRHANE, Muhammad Abid KHAN, Paul ADIGUN, Eromosele Precious EBIENDELE, Ngoc Kim Hong NGUYEN
University of Tsukuba
To develop reliable regional climate information for climate change adaptation measures, we assess added values of regional multi-ensemble downscaling in collaboration with geoscience researchers, social science and humanities, and officials of local governments in Japan and CORDEX Asia. To investigate uncertainty caused by the structural differences in climate models, multi-model ensemble regional climate scenarios over Japan and CORDEX Asia are developed and investigated for several impact assessments. Development of regional climate scenarios with dynamical and statistical downscaling, and investigation of the added value of regional climate information for heat stress assessment and renewable energy (solar, wind, hydroelectric) assessment are presented. Attempts at downscaling land use and land cover change scenarios and flood assessment with urban greening for climate change adaptation will also be presented. We discuss the current issues of developing policy-relevant regional climate scenarios in collaboration with local stakeholders.
AS65-A024
Limited-area Version of the Korea Integrated Model for Dynamical Downscaling
Heeje CHO#+, Junghan KIM, Ilseok NOH, Woo-Jin LEE
Korea Institute of Atmospheric Prediction Systems
The Korea Integrated Model (KIM) is the operational global numerical weather prediction model employing the spectral element dynamical core. This study introduces a limited-area version of KIM, specifically developed for dynamical downscaling through one-way nesting of low-resolution global simulations. Within the cubed-sphere mesh that constitutes KIM's grid system, the limited-area model operates only on a single face of the cube. To minimize potential inconsistencies with global simulations, the limited-area model utilizes the same model components with the original global KIM, except for adjustments made to accommodate lateral boundary conditions. Various approaches for specifying lateral boundary conditions are examined, considering how the differential operators of the spectral element method require values outside the model domain. The feasibility of the limited-area version of KIM is assessed both as an operational regional forecast model and as a general downscaling tool.
AS65-A026
Evaluating Climate Change in the Arabian Peninsula Using High-resolution Regional Climate Modelling
Hariprasad DASARI1#+, Srinivas DESAMSETTI2, Thang LUONG1, Ibrahim HOTEIT1
1King Abdullah University of Science and Technology, 2Ministry of Earth Sciences
Dynamical downscaling of global climate projections using a high-resolution Regional Climate Model enables a comprehensive examination of the regional climatic patterns and the impact of climate change. Employing the advanced Weather Research and Forecasting model, we downscale the future climate projections of the MPI-ESM1-2-HR model for the CORDEX-domain of the Middle East North Africa region at the recommended resolution of 12-km and the Arabian Peninsula (AP) at 4-km resolution. Such computationally demanding high resolution is needed to resolve the convective nature of perception events over the Peninsula. Our assessment spans both historical (1980-2014) and future (2015-2100) periods, exploring three Shared Socioeconomic Pathways (SSP1-2.6, SSP2-4.5, and SSP5-8.5). Additionally, we supplement this analysis by downscaling ERA5 reanalysis for the historical period. We conduct an analysis of the annual count of rainy and hot days, using various precipitation and temperature thresholds, derived from the 12 and 4-km downscaled projections. Comparisons are made with the parent models output, an in-house high-resolution reanalysis specifically generated for the AP, and satellite data during historical periods. Subsequently, the changes in the annual count of rainy and hot days are further examined across future periods under the aforementioned three SSP scenarios. Results indicate that the downscaling approach effectively captures rainfall and temperature events, during the historical period, surpassing the accuracy of the parent models. Future projections for all SSP scenarios suggest an anticipate increase in normal, heavy, and extreme rainfall events, accompanied by a reduction in moderate rain days across the southwestern to northeastern AP, and a decrease in the northwestern AP. In addition, number of temperature extreme events are projected to increase across all periods and SSPs, with particularly pronounced increases under SSP5-8.5. While both resolutions showed similar patterns of temperature events, the 4-km data provided a detailed distribution of rainfall events.
AS65-A034
Developing CORDEX Southeast Asia Simulations for Use in Vietnam's National Climate Projections
Grace REDMOND1#, Kien TRUONG2+, Erasmo BUONOMO1, Katy RICHARDSON1, Laura BURGIN1, Josh WIGGS1, Hamish STEPTOE1, Kate SALMON1
1Met Office, 2Vietnam Institute of Meteorology, Hydrology and Climate Change
Towards the development of producing 12km Regional Climate Modelling Downscaling Experiments within the CORDEX Southeast Asia framework to inform Vietnam's National Projections, a collaboration between Vietnam Institute of Meteorology Hydrology and Environment (IMHEN) and the UK Met Office. We intend to downscale CMIP6 models using the UK Met Office HadREM3-GA7.05 regional model. We identified suitable CMIP6 models after carrying out a model sub-selection exercise. The output from these model runs will inform Vietnam's national climate projections.
Session Chair(s): Feimin ZHANG, Lanzhou University
AS23-A003
Climatic Effects of Non-growing Season Land Surface Processes Anomalies Over Tibetan Plateau Under the Background of Vegetation Cover Increment
Kai YANG1#+, Qi QI2, Chenghai WANG2
1Institute of Mountain Hazards and Environment, Chinese Academy of Sciences, 2Lanzhou University
The coverage of short vegetation, such as alpine grass over the Tibetan Plateau (TP), has increased in past decades. How changes of non-growing season alpine grass—withered grass stems (WGS) impact on land surface processes and subsequent local and downstream climate still remain unclear. Here, we revealed that an increment in WGS coverage significantly reduce snow depth and snow cover fraction in winter, leading to a decrease in ground albedo. This reduction in albedo results in local ground temperature rising, which accelerates winter snow decline. As a result, WGS coverage increments lead to a shortened persistence of TP winter snow cover (TPWSC) anomalies and weakened surface diabatic heating anomalies in spring. Consequently, the influences of TP thermal forcing on East Asia (EA) atmospheric circulation in summer were altered, resulting in a different pattern of EA summer precipitation (EASP) anomalies. These findings highlight the importance of snow—vegetation feedback in climate changes.
AS23-A009
Temporal Accumulation and Lag Effects of Precipitation on Carbon Fluxes in Terrestrial Ecosystems Across Semi-arid Regions in China
Haixing GONG#+, Guoyin WANG, Tiantao CHENG
Fudan University
Precipitation (PRE) plays a vital role in hydrological processes, ecological vegetation, and land-atmosphere interactions in semi-arid regions. Previous research has mainly focused on the impact of PRE on large-scale regional climate change and ecological evolution. However, there have been few studies on the long-term effects of PRE on carbon fluxes in these regions, especially the time-accumulation and -lag effects. Here, we employed observational data from the Semi-Arid Climate and Environment Observatory of Lanzhou University (SACOL) and integrated multiple data sources, including remote sensing and carbon flux simulation data, to quantitatively assess the lagged response of carbon fluxes to PRE and elucidate the underlying mechanisms from multiple perspectives. Characterization of PRE, soil water content (SWC) and carbon fluxes at SACOL qualitatively reveals the existence of a time-delayed response of carbon fluxes to PRE, both on monthly and finer daily temporal scales. The average lagged response of net ecosystem exchange (NEE) and gross primary productivity (GPP) to accumulated PRE (APRE) is approximately 42 days. When considering time-accumulation and -lag effects, the combined effects of APRE on NEE and GPP increase by 0.37 and 0.58, respectively. Notably, preceding APRE primarily exerts a direct effect on current carbon fluxes, whereas the impact of SWC at a depth of 0.1 m is primarily mediated through the memory effect of preceding APRE, resulting in an indirect effect on carbon fluxes. These findings emphasize the importance of preceding APRE. Significantly, our subsequent study indicates that the delay in NEE and GPP responses to APRE also extends to approximately 40 to 50 days at the regional scale. Our findings emphasize the significant time effects of APRE on carbon fluxes, and considering these effects will contribute to a better understanding of the interplay between PRE and vegetation over semi-arid regions in China.
AS23-A023
Impacts of Regional Uplift of the Tibetan Plateau on Local Summer Precipitation and Moisture Transport
Kai YANG+, Tianliang ZHAO#
Nanjing University of Information Science & Technology
Using the Weather Research and Forecasting (WRF) model, a series of sensitivity experiments were conducted to study the individual and overall effects of the various topographic uplifts of the Tibetan Plateau (TP) on regional climate variability. The presence of the southern slope of the TP facilitates the maintenance and development of the South Asia High (SAH), which produces a positive cyclic response between local precipitation and SAH, so that the northern branch of the South Asian summer monsoon (SASM) maintains the water vapor supply. At the same time, the southern slope of the TP has a positive effect on the mid-latitude tropospheric anomalous cyclone and anticyclone systems which promotes the downstream advancement of the East Asian summer monsoon (EASM) and is favourable for the transfer of water vapor and convective clouds downstream. The role of the TP platform is mainly due to the lifting of moisture generated by its local heating, which promotes the formation of local convective clouds and precipitation while causing adiabatic warming of the troposphere. Water vapor transported from the TP could affect precipitation in central-eastern China (CEC). However, the supply of water vapor in Southern East China (SEC) mainly comes from the southeast coast of China. The Tibetan Plateau sensitive areas (TPSA) have impacts on the water vapor transport path. Removing the TPSA favours an increase in precipitation and convective clouds in SEC. The removal of topographic disturbances promotes the convergence and dispersion of water vapor at mid-latitudes. The mid-latitude dynamical anomaly may form a standoff with the low-latitude dynamical system. This leads to inefficient precipitation and convective generation processes, a weakened monsoon advance over land, and a southward shift in the rainfall belt.
AS23-A011
Tremendous Loss of Wind and Solar Energy Induced by Future Climate Disasters Over the Desertification Region of Boreal China
Feimin ZHANG1#+, Chenghai WANG1, Lin ZHAO2
1Lanzhou University, 2Lanzhou University of Technology
Utilization of wind and solar energy is an important approach to achieve the carbon neutrality target. The desertification region of boreal China has installed and will construct large amount of wind and solar bases. Despite many studies on the projection of future theoretical wind and solar energy, however, influence of future climate disasters on wind and solar energy potentials has not been taken into account, making the technically exploitable potentials over the desertification region of boreal China are not clear. This study investigates the influence of climate disasters on the efficiency loss of wind and solar energy over the desertification region of boreal China under different future climate scenarios. Results illustrate that the annual mean efficiency loss of wind and solar energy in this region caused by future climate disasters would be 15%~23% and 13%~18%, respectively. The maximum and minimum efficiency loss would be located in Qinghai and Mengdong region. Results here illuminate and highlight the urgency of the influence of climate disasters in the policy-making of renewable energy development in the future.
Session Chair(s): Maxime COLIN, Leibniz Centre for Tropical Marine Research, Chien-Ming WU, National Taiwan University
AS57-A008
| Invited
Parameterization of Aerosol Indirect Effects Within Subgrid Convection Scheme
Sungsu PARK#+, Siyun KIM, Chanwoo SONG, Ui-Jin KWON
Seoul National University
The effects of aerosols on global climate through the interactions with cloud and precipitation processes – aerosol indirect effects – has been known to be important in many aspects. Some general circulation models can simulate aerosol indirect effects in association with stratus and stratiform precipitation. However, most GCMs cannot simulate aerosol indirect effects in association with cumulus and convective precipitation. Given the fact that subgrid convection exerts substantial impacts on the simulated global climate, it is important to develop a GCM that can simulate aerosol-cumulus-precipitation interactions. In this talk, we will introduce a new atmospheric GCM that is designed to simulate aerosol indirect effects in both cumulus and stratus - Integrated Moist Physics Parameterizations for the Earth System (IMPrES) - and show various results simulated by IMPrES.
AS57-A010
Solutions of Tropical Convection Under Convective Quasi-equilibrium Constraints
Jia-Yuh YU#+, Dong-Pha DANG
National Central University
Solutions of tropical convection (vertical motion), including both the first (deep) and the second baroclinic (shallow) modes, subject to convective quasi-equilibrium (CQE) constraints are formulated. Under CQE assumption, tropical convection can be decomposed into a product of height-dependent variable and space-dependent variable, with the former constrained by conservation of moist static energy (MSE) or dry static energy (DSE) perturbations, depending on whether the atmospheric column is dominated by ascending or descending motions. We then evaluate the roles of deep and shallow modes of convection in transporting moisture and static energy against observations using the European Centre for Medium-Range Weather Forecasts reanalysis data. The moisture transport by deep mode produces a spatial pattern similar to observations, except for an obvious underestimate of the magnitude over the eastern Pacific convergence zone (EPCZ) and cold tongue areas, where the contribution of shallow mode may account for up to 25% of the total moisture transport. In contrast, the MSE transport by deep mode exhibits a very poor performance, especially over the EPCZ where the observational MSE transport is negative but a positive value is predicted by deep mode. Including the contribution of shallow mode immediately remedies this deficiency, due to a better representation of the bottom-heavy structure of ascending motions over the EPCZ. These improvements apply to almost the entire tropics, although the correlation tends to decrease away from the convergence zones. Since simple atmospheric models often assume a single heating (forcing) profile to represent the effect of cumulus convection, the present study highlights the importance and feasibility of including both deep and shallow modes in a simple atmospheric model, while at the same time maintaining the simple model framework, to more accurately represent the moisture and MSE transports by convection in the tropics.
AS57-A011
Role of Mean States on Atmospheric Responses to Extratropical Thermal Forcing
Yung-Jen CHEN1+, Yen-Ting HWANG1#, John CHIANG2
1National Taiwan University, 2University of California, Berkeley
This study examines the extratropics-to-tropics teleconnection and highlights a strong dependency of the teleconnection on background states. A time invariant extratropical thermal forcing was imposed in the atmospheric model AM2, coupled to an aqua-planet 200m mixed layered ocean, under three distinct idealized control climates: a perpetual equinox-like climate, a perpetual winter-like climate, and a perpetual summer-like climate. The result shows that the perpetual summer-like control case favor the extratropical-to-tropical teleconnection and experience a significant ITCZ shift earlier than the other two cases. We offer two explanations for summer being the optimal season for the teleconnection: (1) The midlatitude eddy response to extratropical surface warming is affected by the warming structure. In summer-like climate, vertical-extending warming significantly suppresses baroclinicity by reducing the meridional temperature gradient, leading to a subtropical eddy momentum flux convergence anomaly and associated Hadley cell adjustment. In winter-like climate, trapped-warming response leads to a more unstable lower troposphere, enhancing wave generation and compensating the effect of decreased meridional temperature gradient. These competing effects result in weak eddy response and inefficient teleconnections.(2) The climatological Hadley cell regime determine the magnitude of Hadley cell responses to anomalous eddy momentum flux. When the Hadley cell is in an eddy-driven regime, usually seen in summer-like climate, the mean circulation is sensitive to eddy momentum flux. The eddy momentum flux response in the summer-like climate could effectively weaken the Hadley cell and lead to the ITCZ shifting. This study unfolds the seasonal dependency of the extratropical-to-tropical teleconnection. While the setting is highly idealized, the study bridges to gaps between our theoretical understanding of the extratropical-to-tropical teleconnection and the time-evolving atmospheric responses in more realistic simulations. It provides a framework to investigate atmospheric circulation responses to various extratropical thermal forcing, e.g. ozone depletion, aerosol emission in historical and future warming scenarios.
AS57-A007
Role of Ocean-atmosphere Interaction in Intraseasonal Variability of Summer Rainfall Over the Indo–Northwest Pacific
Zhen-Qiang ZHOU#+, Yang WANG, Renhe ZHANG, Yanke TAN
Fudan University
The observed negative response of sea surface temperature (SST) to local summer rainfall peaks, when SSTs lag 5-10 days over Indo–Northwest Pacific (Indo-NWP) region, raises questions about the accuracy of atmospheric models in simulating intrasesonal variability. An Atmospheric Model Intercomparison Project simulation forced by daily-varying SSTs (daily-AMIP) derived from a parallel coupled general circulation model (CGCM) run is used to evaluate the impact of high-frequency coupling on intraseasonal variability of summer rainfall over the Indo-NWP region. Compared to CGCM, the daily-AMIP systematically overestimates intraseasonal variability of rainfall over the South China Sea (SCS)-NWP region, consistent with the differences in mean state featuring a cyclonic low-level circulation pattern with enhanced westerlies anchored on the south flank by the monsoon-trade wind confluence. The northward propagation of boreal summer intraseasonal oscillation (BSISO) in daily-AMIP is comparable with CGCM, indicating the random nature of atmospheric internal variability. The amplitude of BSISO in daily-AMIP is larger than CGCM, due to the lack of high-frequency ocean-atmosphere coupling which plays a delayed negative feedback role. In addition, the larger conversion of kinetic energy (CK) in daily-AMIP, resulting from the stronger mean westerly, also energizes BSISO more efficiently than CGCM. Implications for assessing the ability of AMIP to simulate intraseasonal variability over the Indo-Northwest Pacific region are discussed.
AS57-A002
Identifying Cold Pool Scales Over Complex Topography Using TaiwanVVM Simulations
Po-Yen CHEN#+, Chien-Ming WU
National Taiwan University
In this study, our objective is to identify cold pool (CP) scales over Taiwan's complex topography during predominant afternoon thunderstorms environment. For this, we employ a semi-realistic Large-Eddy Simulation (LES), TaiwanVVM, which covers the entire area of Taiwan to capture this phenomenon. Our findings reveal that when buoyancy is defined at a typical environmental scale (around 100 km), the CP's location does not align with the precipitation areas, being mainly concentrated along the mountain ridges. We hypothesize that this discrepancy results from the horizontal scale at which CP buoyancy operates. To assess this scale, systematic analyses are conducted. Utilizing an optimal local environmental scale of approximately 7.7 km, determined by three times the 75th percentile of precipitation object horizontal length, our results indicate a better correlation between CPs and the precipitation areas, both in plain and mountainous regions. The vertical cross-section distinctly illustrates the local convection development due to the interaction between near-surface inflow and CP over complex topography. Moreover, the relatively larger-scale buoyancy field, such as land/sea breeze, can be distinguished from the convective CP scale based on our definition.
AS57-A005
Leveraging Large Eddy Simulation Data and Unet for Subgrid Cold Pool Intensity Prediction
Yi Chang CHEN#+, Chien-Ming WU
National Taiwan University
This study uses Large Eddy Simulation (LES) to simulate high-resolution Cold Pools (CPs), capturing their structures at different resolutions and various convection levels. With this integration, we can obtain a comprehensive range of high-resolution CP structures, particularly the detail of understanding how CPs evolve and interact with their surroundings at different levels of convection. Leveraging the data obtained from LES by the vector vorticity equation cloud-resolving model (VVM), we developed a Unet deep-learning model to predict the high-resolution distribution of CPs based on low-resolution physics variables such as surface wind speed, direction, and precipitation. Our research revealed that the Unet model effectively captures the characteristics of CPs, especially regarding their edges and intensity distribution within sub-grid scales, which is critically linked to developing new convection in the surrounding areas. The results also demonstrate that high-resolution predictions provide enhanced information on horizontal heterogeneity beyond what low-resolution fields offer at various convection levels. Furthermore, we evaluated the performance of the Unet model at various resolutions, assessing its capability to represent sub-grid CPs accurately. This analysis provides helpful information for evaluating cold pool parameterizations in kilometer-scale atmospheric models, where the convection triggered by the effect of the sub-grid CP can be critical. The insights gained from this study enhance our understanding of CP dynamics and are instrumental in developing sub-grid CP parameterizations in the next-generation models.
AS57-A003
Distinguishing Convective-scale Dynamics from Turbulence Through the Nonlocal Effect of Convective Buoyancy
Fu-Sheng KAO+, Chien-Ming WU#
National Taiwan University
This study investigates the cutoff scale at which the non-local circulation generated by the convective buoyancy structure dominates, while the detailed turbulence can be ignored for various types of moist convection in a high-resolution cloud resolving model (CRM). The exploration is based on solving the elliptic equation of vertical acceleration derived from anelastic equation sets. To resolve a spectrum of horizontal scale structures for relatively realistic convection scenarios, we employ a large-eddy simulation (LES) using a vector vorticity equation cloud-resolving model (VVM) with a horizontal resolution of 100 m. A Madden-Julian Oscillation (MJO) transition case from shallow to deep convection over the tropical ocean is used to cover various types of tropical convection. To isolate the convective and turbulent structures, we systematically applied Gaussian convolution at different scales to the buoyancy field. This approach quantitatively filters out high-frequency fluctuations and retains the buoyant thermal structures for both shallow and deep convection. Demonstrating through a deep convective cloud case, our findings reveal that focusing on the buoyancy structure over 2 to 3 km can drive vertical acceleration similar to that of a detailed 100 m resolution. Furthermore, without artificially selecting convective grids, the horizontal scale of cloud liquid water objects can serve as a proxy, presenting the cutoff scale at which a convective cloud can maintain its dynamic structure comparable to the 100 m resolution. The results obtained in this study can serve as a physics-based cutoff scale for simulating the desired convective systems.
AS57-A009
Global Lightning Response to Enhanced Secondary Aerosol Activation: Insights from IMPrES Simulations
Ui-Jin KWON+, Sungsu PARK#, Siyun KIM, Chanwoo SONG
Seoul National University
Aerosol-cloud-precipitation interactions play an important role in setting the frequency and intensity of atmospheric deep convection. Recently, an Integrated Moist Physics Parameterization for the Earth System (IMPrES) was developed, which can comprehensively simulate aerosol-cloud-precipitation interactions in both cumulus and stratus. Under IMPrES simulations, this study analyzes changes in the global distribution of lightning frequency with enhanced secondary aerosol activation, a process where interstitial aerosols entrained in convective updraft plumes undergo activation. Secondary aerosol activation impacts the mass and size of cloud condensate, precipitation rate, convection intensity, and lightning frequency. The lightning frequency is calculated within IMPrES, using the diagnostic lightning parameterizations from several previous studies. Results indicate that enhanced secondary activation is associated with an increase in lightning frequency over most oceans, Eastern Europe, Central and Eastern Asia, India, and Central America, while it tends to decrease over Africa, South and North America, Northern and Western Asia, China, Western Europe, and the North-eastern Atlantic Ocean. More details will be given in the presentation.
Session Chair(s): Yuqiang ZHANG, Shandong University
AS03-A004
| Invited
Simulating Atmospheric Aerosols and Their Climatic Impacts with a Global Variable-resolution Model (iAMAS)
Chun ZHAO#+, Jiawang FENG, Zihan XIA, Chen JIN
University of Science and Technology of China
Aerosol-radiation-cloud interactions and their impacts on meteorological processes and aerosol cycle have been proven to be important. As the two-way interaction between aerosol and meteorological fields are complex, a fully coupled “online” meteorology-chemistry model is a necessary tool to account for these feedbacks in simulating aerosol concentrations and meteorological fields. High-resolution is particularly important in simulating aerosols and their impacts. Traditional modeling method at high resolution relying on limited-area model may introduce some numerical issues and constrain regional feedback to large-scale circulation due to lateral boundary conditions. In this presentation, a global variable-resolution modeling framework of atmospheric aerosols and their climatic feedbacks are introduced. In this model, atmospheric aerosols are simulated simultaneously with meteorological fields, and aerosol-radiation-cloud interactions are included. The model reasonably produces the overall magnitudes and spatial variabilities of global aerosol metrics such as surface mass concentration, deposition, AOD, and radiative forcing compared to observations and previous modeling results. A few experiments with mesh refinements are conducted to demonstrate the impacts of convection-permitting resolution on simulating aerosols and their impacts over Asia.
AS03-A006
Efficiently Modeling Organic Aerosol (OA) Considering Temperature-dependent Evaporation of POA and SOA Formation from VOC, IVOC and SVOC
Ling HUANG1#+, Greg YARWOOD2, Li LI1, Zi'ang WU1, Yangjun WANG1, Gary WILSON2
1Shanghai University, 2Ramboll
Organic aerosols (OA) constitute an important fraction of fine particulate matter (PM2.5) air pollution, yet accurate and efficient OA modeling within chemical transport models (CTM) remains a challenge. Volatility basis set (VBS) schemes for OA have demonstrated improved performance in simulating OA, particularly for secondary organic aerosol (SOA), but their computational complexity impedes application to advanced modeling tasks, such as source apportionment. Conversely, simpler “two-product” schemes are efficient and compatible with source apportionment techniques but tend to underestimate SOA while overestimating primary OA (POA) because treated as non-volatile. We develop an improved two-product framework by (1) treating POA as semi-volatile and (2) adjusting SOA yields from intermediate and semi-volatile organic compounds (IVOC and SVOC, respectively) for atmospheric aging. The former allows temperature-dependent partial evaporation of POA to SVOC which is subsequently oxidized in the gas-phase. For the latter modification, SOA yields are updated to mimic a VBS scheme based on an offline conceptual model. We implemented these concepts within the existing “SOAP2” two-product scheme of the Comprehensive Air Quality Model with extensions (CAMx), to create SOAP3. A series of CTM simulations were conducted with SOAP3 to simulate OA and its components in China during July and November 2018. Results were validated against surface observations and compared to the CAMx SOAP2 and CMAQ AERO7 VBS scheme. While changes in total OA concentrations were minor (-3–16%) between the two two-product schemes, the relative contributions of OA components changed substantially. Compared to SOAP2, SOAP3 substantially reduced POA concentrations (17–44%) and increased SOA concentrations (12–123%)SOAP3, bringing SOAP3 into closer alignment with the CMAQ AERO7 VBS scheme. Our study demonstrates a feasible and readily implemented methodology for improving two-product OA modeling, which is currently employed in many CTMs.
AS03-A005
Impact of Turbulent Mixing Simulated at Multi-scale Resolutions on Urban Pollutant Transport
Zining YANG#+, Chun ZHAO, Qiuyan DU, Gudongze LI, Zihan XIA
University of Science and Technology of China
Coarse-resolution atmospheric models often overlook small-scale physical and chemical processes. Therefore, model resolution has a significant impact on air quality modeling. However, the mechanism of the sub-grid processes that influence atmospheric particulate matter at different scales is unclear, which greatly constrains the accuracy of air quality modeling. Thus, we carry out numerical simulation experiments of atmospheric particulate matter from hundreds of meters to tens of kilometers resolution based on the WRF-Chem model, combined with the Ndown technique for typical pollution cases. The authenticity of the model simulation was verified by comparing the black carbon observation data of March 2019 in the Hefei area with the simulated results. The results show that the surface BC concentration was higher in coarse grids, and the column BC concentration was higher in fine resolution. Differences between the various scale simulations arise primarily during nighttime, with insignificant disparities during the daytime. The boundary layer mixing coefficients diagnosed in the finer resolution model are larger, and the upward vertical wind field simulated by the model reaches a higher altitude as the resolution increases. The high-resolution simulation even resolved turbulent eddies, which may reproduce the overall transport and mixing of atmospheric pollutants. Thus the BC surface concentration is transported higher and farther, leading to a longer lifetime and a higher BC column concentration. Other than the capability of mixing and the vertical wind flux, the dry deposition velocity also controls the formation of BC concentrations. High-resolution simulations of terrain and land use types resolve more spatial details and characteristics. This study will enhance the understanding of the results of multiscale simulations of atmospheric particulate matter characteristics in China and help to improve the accuracy of pollutant simulation, it also provides references for establishing the sub-grid parameterization designed to reduce the uncertainty in simulating the climate.
AS03-A014
Prediction of Vehicle Exhaust Transport in Urban Street Canyons
Yiding ZHOU1, Jue WANG2, Yunge HOU2, Wei MA2, Chun CHEN1, Ruoyu YOU2#+
1The Chinese University of Hong Kong, 2The Hong Kong Polytechnic University
The exhaust emission from transport vehicles significantly contributes to air pollution in urban street canyons. The experimental measurement of roadside exhaust concentration cannot provide a high spatial-temporal resolution, limiting the assessment of direct exposure to vehicle exhaust in street canyons. Correctly predicting vehicle exhaust transport in urban street canyons is crucial for improving urban planning and public health. To address this problem, a numerical simulation method based on computational fluid dynamics (CFD) was developed to predict the vehicle exhaust transport in urban street canyons. A controlled field test was conducted in a realistic scenario to measure the air pollutant distribution surrounding an idling passenger car. The measurement data was used to validate the simulation method. Both the measurement and simulation demonstrate that once emitted, the vehicle exhaust concentration decreases approximately 100 times within 0.3 m and nearly 300 times within 1 m. A case study was conducted in a generic street canyon with 180 m in length and 18 m in width, with idling vehicles stationed at 2-m intervals, simulating a traffic jam or waiting for traffic signals. The simulation shows that the vehicle exhaust distribution is inhomogeneous inside the street canyon. When the approaching wind is perpendicular to the street canyon, the vehicle exhaust accumulates on the leeward side, with higher concentrations observed in lower wind speed areas. At the height of 1.5 m on the pedestrian road, the highest concentration is about two orders of magnitude greater than the lowest one. The transient simulation result further shows that the pedestrian-level concentration reaches the peak value when the emission lasts for over 30 seconds. This suggests the maximum idling time to minimize the impacts on ambient air quality.
AS03-A007
Street Network Design for Alleviating the Residential Exposure to Traffic-related Air Pollution
Xing ZHENG1#+, Jiachuan YANG2, Chi FENG3
1City University of Hong Kong, 2The Hong Kong University of Science and Technology, 3Chongqing Unversity
Air pollution is of significant concern to urban residents. In street network planning, planners need to carefully tackle the trade-off between the residential health risk and the traffic capacity. Yet the relationship between street network planning and traffic pollutant distribution has gained little attention. This study addresses the knowledge gap between street network design and residents’ exposure to traffic pollutants by performing large-eddy simulations. Three street network designs with the same traffic volume have been evaluated: (1) Mini-block with 1-lane roads in high density; (2) Regular-block with 2-lane roads in median density; and (3) Super-block with 4-lane roads in low density. Daily activities of different age groups are considered to examine the vulnerable population in the urban neighborhood, using the personal intake fraction (PIg) that represents the emitted pollutant inhaled averagely by each resident. By changing from Super-block to Mini-block design, the outdoor PIg decreases from 0.632 to 0.477 ppm for the young group and decreases from 0.714 to 0.529 ppm for the adult group, but remains largely unchanged for the elderly group. The Mini-block street network leads to uniform indoor PIg for residents, with a maximum value of 0.251 ppm for the elderly group. For the Regular-block and Super-block cases, residents living in roadside buildings, especially with a long roadside I, tend to bear an unequal level of pollutant burden. With a Super-block design, elderly residents in 25% of the buildings have an indoor PIg up to 0.554 ppm, which is four times larger than the 0.121 ppm intake in other buildings within the superblock. Our results provide insights into the impact of street network design on urban air quality and residential health risks.
AS03-A009
WRF-CMAQ Evaluation in Predicting PM2.5 Concentration During Transboundary Smoke Event in Peninsular Malaysia (PMY)
Nur Nazmi Liyana BINTI MOHD NAPI+, Maggie Chel Gee OOI#
Universiti Kebangsaan Malaysia
Uncontrollable emissions from biomass burning have deteriorated air quality in Peninsular Malaysia and caused severe haze events, which negatively impact human health, society, and the environment. The development of the air quality forecasting model of Weather Research Forecasting - Community Multiscale Air Quality (WRF-CMAQ) will be able to improve the predictability of current continuous air quality monitoring system in Malaysia by covering large areas, sources of emissions, physical and chemical factors, and complex transport pathways. The WRF-CMAQ model, together with fire emissions (FINNv1.5) is deployed with two different settings of weather nudging: without weather nudging (WRF-CMAQwithout_nudging) and grid nudging (WRF-CMAQwith_nudging) in this study to predict the PM2.5 concentration in PMY, especially during transboundary smoke events. Both model outputs were evaluated against the observation data based on the statistical evaluation of correlation coefficient (r), mean fractional bias (MFB), and mean fractional error (MFE). As a result, WRF-CMAQwith_nudging showed that 86% of the evaluated station fulfilled the statistical criteria compared with daily PM2.5 observation data while WRF-CMAQwithout_nudging of about 82% in predicting PM2.5 in this study. Higher accuracy of the WRF-CMAQ model output can improve the spatial coverage prediction of PM2.5 concentration, especially during transboundary events. Hence, higher performance of the prediction model can provide a better understanding of interpreting the output for decision-making to improve the air quality during the re-occurrence of transboundary smoke events in Malaysia.
AS03-A016
WRF-CMAQ-BCG: Accounting for Black Carbon Aging Process in a Two-way Coupled Meteorology - Air Quality Model
Yuzhi JIN#+, Jiandong WANG, Chao LIU
Nanjing University of Information Science & Technology
Black carbon (BC), as a dominant light-absorbing aerosol, exerts significant impacts on the atmospheric environment and global climate. Currently, the uncertainty in numerical simulations of BC primarily arises from the complex aging process. Furthermore, the simulation of BC aging has not been fully incorporated into the Weather Research and Forecasting - Community Multiscale Air Quality (WRF-CMAQ) two-way coupled model. In this study, we developed series modules to account for the BC aging process in WRF-CMAQ model (WRF-CMAQ-BCG). Initially, we introduced two new species, namely "Bare BC" and "Coated BC," to the model to distinguish the aging status of BC. Subsequently, we developed a BC aging module to account for the transformation from Bare BC to Coated BC. Based on the differences in BC aerosol mixing states and hydrophilicity before and after the aging process, wet deposition and aerosol optical calculations were improved. We conducted a simulation using the WRF-CMAQ-BCG model in the United States in June 2010 and validated the results with observational data from the Carbonaceous Aerosols and Radiative Effects Study (CARES) campaign. The model successfully integrates a functionality that distinguishes between internal and external mixing states of BC aerosol. This integration allows for a more accurate assessment of aerosol optical properties.
AS03-A015
Accounting for Mixed Black Carbon Nonsphericity and Heterogeneity Effects for its Optical Property Parameterization
Ganzhen CHEN#+, Chao LIU, Jiandong WANG
Nanjing University of Information Science & Technology
Modeling of atmospheric black carbon (BC) aerosol optical properties exhibits large uncertainties due to their complex mixing state, nonsphericity and heterogeneity. Although various models have been developed based on realistic BC morphologies to represent their optical properties, those models were mostly limited to particle-scale studies and were seldom adopted to large-scale atmospheric or environment models due to BC microphysical property diversities and corresponding optical computational costs. This study develops a multi-dimensional parameterization algorithm for mixed BC optical properties, incorporating influences of the BC mixing state for the individual internal mixture, non-spherical structure for the morphologies of BC and coating, and heterogeneous particle distribution for aerosol ensembles. Our results indicate that the BC morphology has limited influence on aerosol absorption cross section (Cabs), and the differences in Cabs between irregularly coated aggregates and ideal core-shell spherical counterpart are only 3% averagely. However, the relative positions between BC and coating parts may introduce aerosol absorption variations up to 69% as compared with the concentric core-shell results. The optical parameterization is coupled and tested with the Community Atmosphere Model version 6 (CAM6) by the dimension reduction for individual particles and integration for particle ensembles. The influence of BC mixing state (0.0019) and heterogeneity (0.0018) on BC absorption optical depth are approximately three times than that of nonsphericity (0.0006). The global average single scattering co-albedo (1−SSA, i.e., absorption-to-extinction ratio) modeled by CAM6 with our new optical parameterization is reduced from 0.053 to 0.033, much closer to the multi-model mean (0.031) from the sixth phase of the Coupled Model Intercomparison Project. Furthermore, the normalized mean bias of 1−SSA compared to Aerosol Robotic Network observations in regions with rich BC sources are reduced by 20%~80% by adapting our new parameterization.
Session Chair(s): Pay-Liam LIN, National Central University, Eiichi NAKAKITA, Kyoto University
AS83-A034
| Invited
Analysis of Extreme Heavy Rainfall Event on 1-2 June 2017 Over Northern Taiwan Area by Ensemble Simulations
Kaoshen CHUNG1#+, Pei-Jung TSAI1, Ching-Yin KE1, Yu-Chieng LIOU1, Yi-Leng CHEN2,1
1National Central University, 2University of Hawaii at Manoa
This study examines the major characteristic of an extreme rainfall event on 1-2 June 2017 using both observational data and numerical model simulations. A modified k-means clustering method is applied to classify 128-member ensemble simulations into five groups based on rainfall maps. Two of the five groups can be further distinguished as the better simulations through the cluster analysis, offering a comprehensive explanation of the interaction between the mid-to-low-level trough and the front in northern Taiwan. The low-level jet plays a significant role in the extreme rainfall process and highlights the importance of the connection between short-wave troughs and the rainband spatial distributions. In conclusion, this clustering analysis provides useful information of heavy rainfall processes at various scales and helps analyze the dynamic structures of frontal system as well as the performance of model simulations.
AS83-A019
| Invited
Environmental Condition Diagnosis on the Precursors of Soil-sand Disasters
Der-N LIN+, Ben Jong-Dao JOU#
National Taiwan University
From the past soil-sand disaster statistics, it is found once the event occurs, the losses and damages are usually very serious. The main objective of this study is to conduct environment condition diagnostic analysis of historical soil-sand disaster events in a scientific and quantitative ways. It is aimed to identify the key meteorological parameters that are important to the occurrence of soil-land hazards and to test the possible capability of using these findings for warning and preparation for potential soil-sand hazards. It is anticipated the outcomes of this research will effectively support the commander’s determination and to strengthen emergency response for the soil-land disasters. Machine-learning technique will be developed to build a stable and reliable collapse-potential prediction model. The best-possible AI methodology will be applied to identify the collapse-potential precursors. The effective feedback to actual preparation operations and contingency decisions for disaster prevention will be proposed.
AS83-A035
Effects of Turbulence-induced Contingency on Line-shaped Rainbands Using LES
Kosei YAMAGUCHI#+, Yoshiyuki KAWATANI, Eiichi NAKAKITA
Kyoto University
Line-shaped rainbands with self-organization due to back-building phenomena are called line-shaped convective systems, and which stagnate in the same location for a long time, causing flooding and inundation. Predicting their occurrence is extremely difficult because of the mixture of factors derived from necessity, such as topography, and factors derived from contingency, such as natural fluctuations, which are currently expressed by stochastic processes. Therefore, this study aims to understand the outbreak mechanism of line-shaped convective systems using the LES (Large-Eddy Simulation) model developed by Yamaguchi et al. (2016). Moreover, the influence of necessity and contingency, which cannot be evaluated by RANS (Reynolds-Averaged Navier-Stokes equation), is evaluated. First, the SGS(Sub-Grid Scale) model in the LES model was improved to focus on contingency factor. We introduced Bardina model, a kind of scale similarity model that can describe the energy flow from SGS to GS in order to describe the effect of small scale turbulence. As a result, line-shaped rain bands were simulated in both models, with grater rainfall and horizontal convergence when using Bardina model than when using Smagorinsky model. Second, assuming atmospheric micro-turbulence as a contingency, an ensemble experiment was conducted with small noise applied to the flow component while changing the position and timing. The results showed that in an environment with strong horizontal wind convergence constraints, there was no significant change in the location of the onset of line-shaped convective rainstorms, but there was some spread in the rainfall intensity. In addition, the spread was larger when small noise was applied at the timing preceding the onset, suggesting that this may be due to the chaotic nature of the atmosphere.
AS83-A001
Precedent Multifractal Behaviors Against Organization Index of Linear-shaped Convective Systems Using Ensemble Simulation
Akiyuki ONO#+, Kosei YAMAGUCHI, Eiichi NAKAKITA
Kyoto University
Linear-shaped convective systems (LCSs), accompanied by band-shaped areas of heavy rainfall with a length of 50-300 km and a width of 20-50 km, are one of the extreme weather phenomena that can generate record-breaking heavy rainfall in Japan. Early warning information of LCSs considering the meteorological aspects of observation and numerical simulation data is essential in ensuring lead time for flooding controls and evacuation. The current study examines the diagnostic approach of multifractal analysis for LCSs using a cloud-resolving model (CRM) with 500-m horizontal resolution. Multifractal is defined as power laws of 3D spatial scale for water vapor flux (QVF) and turbulence kinetic energy (TKE). The CRM simulation of LCS at Kyoto on 15 July 2012 represented the process that convective clouds organized into a band-shaped cluster. QVF and TKE showed intense multifractality corresponding to convection initiation and resulting in the development of a back-building-like convective cluster. To define the period of the organization of LCS, we estimate the temporal variation of convective mass flux (CMF) which is the total volume of upward moisture flux and fractal dimension of updraft (FDU). When the isolated convective clouds initiated FDU showed a gradual increasing tendency. CMF and FDU increase as merging convective clouds and forming LCS and we defined this period as the organization of LCS. Our analyses revealed multifractal signals on QVF and TKE that appeared about 1-h before LCS was organized. We also conducted the ensemble forecast experiment of the same LCS event to evaluate the robustness of precedent multifractal behavior. The composite analysis for 10 members with larger accumulated rainfall indicated increasing FDU and intense multifractal features on QVF and TKE before the organization of LCSs. Further case studies will exhibit the common behaviors of various LCS events and their regional characteristics.
AS83-A003
3-D Frontogenesis Function Analyses for Meiyu Fronts Affecting Northern Taiwan in the Mesoscale Model
Chuan-Chi TU#+, Pay-Liam LIN
National Central University
3-D frontogenesis function (Miller 1948) is applied to two Meiyu fronts characterized by differences in rainfall intensities and thermal gradients across the fronts (6 June 2022 case versus 2 June 2017 case). The 3-D frontogenesis function includes (1) Differential Heating Terms, (2) Vertical Deformation Terms, (3) Vertical Divergence Term, (4) Stretching Deformation (Confluence) Terms, (5) Shearing Deformation Terms, and (6) Tilting terms. We analyze 3-D frontogenesis function for two Meiyu fronts affecting northern Taiwan in the mesoscale model. Firstly, for the TAHOPE/PRECIP/T-PARC–2022 IOP3 case (6 June), the Meiyu frontal rainband propagates southward and reaches northern Taiwan based on radar reflectivity observations (> 45 dBZ) during 1200–1500 LST 6 June. Consistently, the ENE-WSW 500-m positive frontogenesis band already appears over northern Taiwan at 1200 LST 6 June, indicating the future frontal position in the next few hours (~1500 LST). Terms (1)–(3) are the dominant terms in the 3-D frontogenesis function according to scale analyses. One reason is that vertical velocity as well as vertical thermodynamical structure within the frontal region cannot be neglected in the high-resolution mesoscale model. In contrast, those vertical terms maybe small in the global model. On the other hand, the positive Differential Heating Terms corresponds to the frontal convection zone, where the Vertical Divergence Term shows negative. The 3-D frontogenesis function characteristics are similar for the other Meiyu front (2 June 2017) with much heavier rainfall and smaller thermal gradients in comparison with the TAHOPE IOP3 frontal case.
AS83-A012
Investigation of the Environmental Conditions for the Occurrence of Line-shaped MCSs Associated with Stationary Front Considering Spatio-temporal Characteristics
Kana FUKUDA#+, Yukari NAKA, Eiichi NAKAKITA
Kyoto University
Line-shaped mesoscale convective systems (MCSs) associated with stationary front called Baiu front have caused many heavy rainfall events triggered severe disasters in Japan. Thes phenomena have different spatio-temporal characteristics and can be classified into two types; one is large scale, long duration, and occurs near convergence of Baiu front (type-A), and another is small scale, short duration, and occurs far from more than 100km south of Baiu front (type-B). These differences make a difference of the characteristics of disasters, so the consideration of spatio-temporal characteristics of heavy rainfall events is important for disaster prevention. Then, to ultimately investigate the necessary and sufficient conditions for the occurrence and development of MCSs, past events are extracted from Radar-AMeDAS (Automated Meteorological Data Acquisition System), and we analyze the environmental conditions comprehensively, considering the spatio-temporal characteristics. As a result, the environmental conditions for the occurrence and development of type-A, which occurs under the influence of strong convergence by Baiu front, do not have to be ideal. On the other hand, type-B is important for its self-organized development to have limited and ideal environmental conditions such as strong convective instability, large CAPE (Convective Available Potential Energy), and vertically big change of direction of wind. In the future, we will continue to analyze the relationship between the environmental conditions and physical characteristics such as the area and time of occurrence, which will contribute to deeply understanding the mechanism of the occurrence and development of line-shaped MSCs.
AS83-A022
Observational and Numerical Study on Low Level Jet and Mei-yu Front Precipitation in IOP 3 of TAHOPE/PRECIP 2022
Pay-Liam LIN#+, Chuan-Chi TU, Siang-Yu ZHAN
National Central University
We used ERA5 data to analyze the synoptic weather patterns of TAHOPE IOP 3. The data from weather stations over Taiwan, wind profiler radar at Xinwu station, and radiosondes during the IOP3 were used to analyze the atmospheric thermodynamic structure for the front case. The mei-yu front arrived and stayed over Taiwan during 1200 UTC 6 Jun to 9 Jun. After 1200 UTC 6 Jun, northern Taiwan was occupied by post-frontal cold and dry airmass with wind direction turning to northerly wind. The depth of the post-frontal cold and dry airmass was about 1.5 km. Taiwan was affected by the mei-yu front for about 48 hours, and it resulted in the widespread rainfall on 7 Jun and 8 Jun (especially over western Taiwan costal region). During this period, the low-level wind speed was weak because of the existence of the mei-yu trough, and the synoptic-related low-level jet (SLLJ) was present near 3 km height. On 10 Jun, the southwesterly flow prevailed over the vicinity of the Taiwan with the mei-yu front over north of Taiwan. The low-level jets (LLJs) were present within 1-3 km height on 10 Jun. The low-level winds over post-frontal region turned to the northeasterly wind during 11-12 Jun, resulting in the mei-yu front moving southward and arriving to Taiwan. The post-frontal cold airmass was weaker and shallower with ~1 km depth, and it impacted on Taiwan for about 18 hours. In addition, we simulated the 6 Jun 2022 case, the arrivel of the mei-yu front using numerical model, and we calculated the three-dimensional frontogenesis function to analyze the characteristics of the front.
AS83-A026
Fundamental Research on Heavy Rainfall Control in the Line Shaped Convective System by Introducing Offshore Curtain
Nishimura SHOMA#+, Kosei YAMAGUCHI, Eiichi NAKAKITA
Kyoto University
There is concern that heavy rainfall is becoming more serious as global warming progresses, and it is hoped that heavy rainfall can be mitigated through weather control. Therefore, we would like to consider developing a weather control device as a wind resistor (i.e., Offshore Curtain) by raising a huge kite over the ocean and suspending a huge curtain-like membrane body on the kite. The objective of this study is to investigate whether it is possible to suppress heavy rainfall by manipulating winds to simulate Offshore Curtain through numerical simulations. As the target case, the line shaped convective system case of the 2017 northern Kyushu heavy rainfall was taken up. The meso-scale meteorological model CReSS (Tsuboki and Sakakibara, 2002) was used for the numerical simulation of the heavy rainfall. The wind turbine scheme developed by Uchida et al. (2020) was used to simulate the Offshore Curtain with a size of 1 km x 1 km. The Offshore Curtain was installed on the upstream side of the water vapor inflow path to simulate the suppression of heavy rainfall. The results indicate that the maximum intensity of line shaped convective rainfall can be reduced by up to 40%. In addition, sensitivity experiments were conducted by varying the altitude and horizontal position of the Offshore Curtain, and the rainfall suppression effect varied from -40% to +10%. The lower the altitude, the higher the rainfall suppression effect. The results also suggest that the mechanism of rainfall suppression is the expansion of the weak rainfall area to the leeward side due to the decrease in water vapor uptake and the change in wind velocity field, which mitigates the concentration of heavy rainfall in one location.
AS83-A013
Meteorological Control by Intervention in Wind Speed Field Using LES for the Localized Heavy Rainfall at Toga River, Kobe, Japan, 2008
Taichi NISHIMURA1#+, Kosei YAMAGUCHI1, Takanori UCHIDA2, Eiichi NAKAKITA1
1Kyoto University, 2Renewable Energy Center Research Institute for Applied Mechanics
Localized heavy rainfall (guerrilla heavy rainfall) is not easy to predict due to its small temporal and spatial scales and has recently caused significant damage at urban areas in Japan. Additionally, with the progression of global warming, there is growing concern about the exacerbation of heavy rainfall. Therefore, there is hope that the suppression of heavy rainfall through artificial control of rainfall events with disaster-scale potential. In this study, Toga River heavy rainfall in Kobe, Japan in 2008 was simulated using Large-Eddy Simulation (LES). Furthermore, by manipulating the wind field near the surface, which is a crucial factor in the development of guerrilla heavy rainfall, vortex tubes were weakened. The aim was to evaluate the impact of this weakening on the heavy rainfall. The assumed method for wind field manipulation in this study involves deceleration in the wake region of wind turbines. This was employed to reduce the vertical wind shear that initiates the formation of vortex tubes. The study focused on analyzing the effects of wind speed manipulation on the dynamic and thermodynamic fields. Additionally, by varying the duration, timing, size, and location of wind field manipulation, the sensitivity of these factors was analyzed. As a result, it was demonstrated that wind field manipulation could reduce the maximum rainfall intensity by approximately 27%. The suppression mechanism involves the inhibition of updrafts due to the weakening of vortex tubes, displacement of the position of potential temperature anomalies and airflow convergence caused by updrafts, and a decrease in the intake of water vapor. Furthermore, through spatiotemporal sensitivity experiments for wind field manipulation, we found that the sensitivity of rainfall suppression, particularly concerning the placement of wind turbines, is significant.
AS83-A015
Analysis of Precipitation Systems Causing Short-duration Heavy Rainfall, Focusing on Regional Characteristics
Yuichiro WATANABE#+, Eiichi NAKAKITA
Kyoto University
In Japan, heavy rainfall is brought about by various precipitation systems in diverse regions. Amid concerns over the intensification of heavy rainfall due to global warming, comprehensive understanding of precipitation systems in specific areas is crucial from the perspective of disaster prevention and reduction, especially to prevent river runoff and flooding. This study focuses on specific regions in Japan, aiming to explore the causes of heavy rainfall in each area by conducting an analysis of the spatiotemporal structure and environmental fields of past precipitation systems. For the analysis, data from the Japan Meteorological Agency's AMeDAS accumulated precipitation, national composite radar GPV precipitation intensity, and numerical weather prediction model GPV were used. Several regions where similar linear precipitation bands occurred were selected for analysis. Extraction of heavy rainfall events utilized two thresholds: daily maximum 10-minute precipitation and daily maximum 1-hour precipitation. In the analysis conducted about Kyoto, distinct differences were observed in the precipitation systems obtained with the two thresholds. Precipitation systems obtained from the former threshold were characterized by inflow due to the protrusion of the Pacific-side high-pressure area and locally intense precipitation in an unstable environment. Those obtained from the latter threshold were characterized by the development of a low-pressure area on the Japan Sea side, the meandering of the upper-level jet, and linear precipitation areas originating from Mount Rokko. A similar analysis was conducted about Fukui, but no clear differences were observed. Understanding precipitation systems in Fukui remains a future challenge. Additionally, future efforts will focus on enhancing the understanding of precipitation systems in diverse regions.
Session Chair(s): Zhiyong MENG, Department of Atmospheric and Oceanic Sciences, School of Physics, and China Meteorological Administration Tornado Key Laboratory, Peking University
AS73-A009
| Invited
Unified Master Length-scale for Planetary Boundary Layer Schemes
Bowen ZHOU#+
Nanjing University
Higher-order planetary boundary layer schemes are widely used in mesoscale and global circulation models. They parameterize turbulent processes that are key to convective initiation and organization. These schemes require two separate length scales for turbulent mixing and dissipation respectively. Most schemes assume a single master length scale, legacy of Mellor and Yamada (1974), for both the mixing and the dissipation lengths. Analysis based on recent tall-tower observations and large-eddy simulations reveals drastic differences in the overall profiles of the mixing and the dissipation lengths, which could not be scaled into a single master length. Moreover, the observed dissipation length and the MY length scale even show opposing stability dependence. In this study, we show that the key to a unified master length scale for the representation of both the mixing and the dissipation lengths is through a properly defined turbulence kinetic energy. The resulting master length also exhibits self-similar characteristics that are highly desirable for parameterization purposes.
AS73-A002
| Invited
The Interactions Among the Marine Boundary Layer Jet, Coastal Terrain and Cold Pools and Their Effects on Coastal Convection in South China
Yu DU#+
Sun Yat-sen University
We firstly investigate the interactions among the marine boundary layer jet (MBLJ), coastal terrain, and cold pools through a series of idealized simulations. Their relative heights and strengths are crucial factors to determine the upward motions at their junctions. We further explore their effects on the coastal convection using WRF case simulations and relevant sensitivity experiments. Convection initiation (CI) occurred at the vertex of the coastal concave mountain geometry as a combined result of coastal convergence, orographic lifting, and mesoscale ascent driven by the terminus of a MBLJ. In numerical simulations with the coastline or terrain of South China removed, the coastal CI does not occur or becomes weaker as the MBLJ extends farther north, suggesting that the coastline and terrain play a role in CI. In addition, local small-scale terrain can modulate the detailed location and timing of convection. The convection becomes weaker and moves more slowly when cold pools are weakened through a reduction of rain-evaporation cooling. No convection initiation occurs in the weakest-BLJ run, while rainfall is located to further north with weaker intensity in strongest-BLJ run.
AS73-A015
Desert-oasis Convergence Line and Deep Convection Experiment (DECODE)
Zhiyong MENG1#+, Xuefeng MENG 2, Chenggang WANG3
1Department of Atmospheric and Oceanic Sciences, School of Physics, and China Meteorological Administration Tornado Key Laboratory, Peking University, 2Inner Mongolia Autonomous Region Meteorological Observatory, 3Nanjing University of Information Science & Technology
Convection initiation (CI) has always been a big challenge in weather forecasting worldwide. Boundary layer convergence line is one of the important lifting mechanisms of CI. One major cause of boundary layer convergence line is heterogeneous heating caused by land surface contrast. Along the border of Kubuqi Desert and the Hetao Irrigation District of Inner Mongolia, China, boundary layer convergence lines often occur and deep convections often initiate over the desert side near oasis-desert transition zone. Our statistical analysis showed that about 60 convergence lines form along the desert-oasis border from June to August each year, and 44% of which initiate deep moist convections. These convections sometimes propagate and intensify downstream, causing severe convective disasters. In order to understand the convection initiation, organization, and evolution mechanisms due to vegetation variability across oasis-desert transition zone in Hetao region, DEsert-oasis COnvergence line and Deep convection Experiment (DECODE) was launched from July 5-August 9, 2022 led by the authors of this abstract. About 100 scientists and students from 8 institutes and universities in China participated the experiment. Vertical profiles of Planetary Boundary layer as well as convection and its ambient environment features were observed at two oasis sites and four desert sites. During the experiment, 23 cases of convergence lines with various morphology occurred, and 11 of which initiated convection. In addition to the convergence lines, there also occurred 20 gust fronts, 9 times of horizontal convective rolls, and 1 supercell splitting and 1 tornado. This talk will introduce the background, field campaign and some preliminary analyses of this field experiment.
AS73-A010
Preliminary Study on the Effect of Spot-shaped Clear-air Echoes in the Convection Initiation
Chenggang WANG#+
Nanjing University of Information Science & Technology
The influence of spot-shaped clear-air echoes, commonly observed in desert regions, on convection initiation is preliminarily investigated using weather radar, wind lidar, and boundary layer sounding data during the DECODE observation period in July 2022. These findings suggest that: (1) The appearance of clear-air echoes indicates the occurrence of intense turbulence in the lower atmospheric layers. A stronger echo corresponds to a more pronounced disturbance in the lower layer, which could result in an elevated boundary layer and increased vertical ascent rate, thereby facilitating convection initiation. (2) In summer, Spot-shaped clear-air echoes exhibit distinct diurnal variations with a maximum intensity of 75dBZ. Furthermore, the height of the echo crest ranges between approximately 1-2km. (3) The generation mechanisms for spot-shaped clear-air echoes include dynamic disturbances caused by wind farms, thermal impacts from desert underlying surfaces, and intricate terrain effects. (4) Under various meteorological conditions, four distinct forms of convective system development are initiated by spot-shaped clear-air echoes.
AS73-A007
The Impact of Inhomogeneous Underlying Surfaces on Boundary Layer Jets in the Hetao Region
Liao ZHOU#+
Nanjing University of Information Science & Technology
An investigation on the influence of inhomogeneous underlying surfaces on Boundary Layer jets (BLJs) in the Hetao region was carried out using data from lidar, microwave radiometers, radiosonde balloons during the DECODE observation, and WRF numerical simulations.(1) Changes in atmospheric stability resulting from the inhomogeneous underlying surfaces have a notable impact on BLJs. In the oasis area of Hetao, the intensity of low-level jets is approximately 1.5 m/s lower (10%) compared to the desert region, with the jet axis height approximately 120m higher (50%) than that in the desert. Consequently, the inversion layer in the oasis region demonstrates weaker intensity and higher height.(2) Both terrain and underlying surface attributes affect BLJs by altering the state of the inversion layer. Terrain significantly influences the intensity of BLJs, while underlying surface characteristics have a more pronounced effect on the height of the jets.
AS73-A012
Characteristics of Convection Associated with Boundary Layer Convergence Lines in Warm Season Over Hetao Area
Quxin CUI1#+, Zhiyong MENG2
1Peking University, 2Department of Atmospheric and Oceanic Sciences, School of Physics, and China Meteorological Administration Tornado Key Laboratory, Peking University
Boundary layer convergence line (hereafter referred to as boundary) is one of the most important mechanisms for the convection initiation over Hetao area, where a sharp surface contrast exists between desert and oasis. This work aims to investigate the characteristics of the boundary-associated convective systems. From June to August in the period 2012–2022, 286 convective systems initiated by 213 boundaries were identified and tracked using Thunderstorm Identification Tracking Analysis and Nowcasting based on radar reflectivity observations. Almost all of the boundary associated convective systems were initiated on the arid side of the vegetation contrast. They were tended to move east (24.6%), northeast (21.9%) and southeast (19.3%), and 20% of them developed downstream. The convective systems were usually initiated around 13–14 LST, matured around 15 LST and dissipated around 17 LST. The convective systems were classified into six categories according to their strength and morphology including Weak Line (27.3%), Strong Line (11.9%), Weak Cell (16.4%), Strong Cell (16.4%), Weak Cluster (9.8%), and Strong Cluster (18.2%). The Strong Line and Strong Cluster types were initiated earlier, matured later, lasted longer and had a greater proportion of downstream development. Convective systems in different regions showed different characteristics. There were 179 convective systems initiated by boundaries generated in Kubuqi Desert, with a similar proportion of organizational modes to the population, of which 23% developed downstream. There were 23 convective systems were initiated by boundaries generated in Ulan Buh Desert, with the main organizational mode being Strong Cell. Convective systems (75 cases) associated with boundaries in Lang Mountain were weaker than convection in the other two regions, and the major organizational mode was Weak Line.
AS73-A004
Influences of Desert Afforestation on Boundary Layer Convergence Lines and Related Convection Over Desert-oasis Border
Xuelei WANG1+, Zhiyong MENG2#, Yan YU1
1Peking University, 2Department of Atmospheric and Oceanic Sciences, School of Physics, and China Meteorological Administration Tornado Key Laboratory, Peking University
Inhomogeneous vegetation across desert-oasis has been found to produce boundary layer convergence lines and initiate convections in Hetao area in Inner Mongolia, China. Hetao area has undergone over 30 years of reforestation since 1986. This study aims to understand the impact of the 30-year-reforestation on the behaviors of boundary layer convergence lines and their associated convections. Based on WRF simulation, this study compared the simulated behaviors of boundary layer convergence lines and their associated convections and precipitation using vegetation before and after desert afforestation in the Hetao area. Results showed that desert afforestation decreases the near-surface temperature and increases the near-surface humidity in the afforested desert area. As a result, the formation of near-surface temperature and humidity gradient was retarded and becomes weaker. Consequently, the boundary layer convergence line forms and reaches its maximum length later, and becomes weaker as it forms. The lower near-surface temperature makes CAPE lower and CIN higher in the afforested desert area, causing the convection to reach its maximum intensity later. However, since the near-surface humidity and the vertical transport of water vapor become larger, the convection becomes stronger and dissipates later, which increases the amount and frequency of precipitation over the desert area.
AS73-A005
Differences in the Boundary Layer Convergence Lines at the Border of Oasis/Kubuqi Desert from Oasis/Ulan Buh Desert
Zimeng ZHENG1+, Zhiyong MENG2#
1Peking University, 2Department of Atmospheric and Oceanic Sciences, School of Physics, and China Meteorological Administration Tornado Key Laboratory, Peking University
Boundary layer convergence lines and their associated convection initiation have been found to form frequently at the border of oasis and desert. The characteristics of oasis/desert border may have apparent impact on the behaviors of the boundary layer convergence lines and their associated convection initiation they produced. The Hetao oasis is the largest artificial irrigation oasis in China, which is located in the middle reaches of the Yellow River, bordered on the north by the Lang Mountain, on the south by the Kubuqi Desert, and on the southwest by the Ulan Buh Desert. This study aims to explore the statistical differences in the occurrence and development of the convergence lines at the Border of oasis/Kubuqi from oasis/Ulan Buh Desert and their associated environment features. Significant differences were found in the behaviors of boundary layer convergence lines at the border of oasis/Kubuqi from oasis/Ulan Buh Desert likely due to the apparent different oasis-desert borders. The border between the oasis and the Kubuqi Desert is almost delineated by the Yellow River, making it very clear. However, there exists a surface type transition zone across oasis/Ulan Buh Desert where desert, oasis, and small lakes coexist, which leads to a much weaker temperature gradient. As a result, much less convergence lines occur on the oasis/Ulan Buh Desert side. Many cases form through merging of multiple short convergence lines, and thus being more tortuous, shorter-lived, and triggering less convection compared to their counterparts on the Kubuqi side. The differences in the behaviors of boundary layer convergence lines and their associated convection initiations are also related to their different synoptic patterns.
AS73-A011
A Taiwan Rainband Associated with the Aircraft Crash on 17 November 2020
Che-Yu LIN#+, Cheng-Ku YU
National Taiwan University
Taiwan rainbands (TRs), referring to as convective lines formed near the coast of eastern Taiwan under weakly synoptic weather conditions, are a year-round, well-known mesoscale phenomenon and frequently influence coastal weather. On 17 November 2020, a fighter aircraft took off from the Hualien air force base at ~1805 LST and crashed over coastal water of eastern Taiwan after ~2 minutes later. Radar images indicate the occurrence of a TR during the aviation accident. The objective of this study is to use available surface and radar observations to explore the possible connection of the observed TR to the accident and to document its structure and formation. The synoptic environment accompanying this event was relatively undisturbed and the low-level prevailing winds were mostly easterly. The TR was formed adjacent to the coast of eastern Taiwan at ~1700 LST 17 November and dissipated at ~0700 LST 18 November. The vertical extent of precipitation of the TR was confined to the lowest 2.5 km (MSL), but it was characterized by an obvious convective nature. The strongest radar reflectivities associated with the TR could exceed 50 dBZ. Combination of flight track and radar-observed precipitation information shows that the aircraft flew into the TR, encountered the zone of heavy precipitation (~35 dBZ), and subsequently crashed within a very short period of time (~1 minute). It is thus likely that convective precipitation associated with the TR may represent hazardous weather threatening the aviation safety and operation for this unfortunate event. In addition, the colder nearshore air generated by orographic blocking and contributed partly by the evaporation of former TR’s precipitation was observed to persist and acted as a cold pool to provide a low-level convective forcing leading to the formation of the TR.
AS73-A001
| Invited
Influences of Urbanization on an Afternoon Heavy Rainfall Event Over the Yangtze River Delta Region
Yali LUO1#+, Xiaoling JIANG2, Da-Lin ZHANG3
1Nanjing University of Information Science & Technology, 2National Institute of Natural Hazards, Ministry of Emergency Management of China, 3University of Maryland
This study examines the influences of the UHI effects associated with a city belt over the Yangtze River Delta on generating an afternoon heavy rainfall event over coastal Nantong that is 70–100 km downwind from the city belt. Observational analyses show pronounced urban heat island (UHI) effects along the upstream city belt prior to convection initiation (CI). A series of cloud-permitting model simulations with the finest grid spacing of 1 km are performed to examine the impacts of urbanization on CI and the subsequent heavy rainfall event. Results reveal the generation of warm anomalies and low-level convergence in the planetary boundary layer along the upstream city belt, thereby inducing upward motion for CI. The southwesterly flows of the monsoonal warm-moist air, enhanced by the UHI effects along the city belt, allow the development of convective cells along the belt. Some of the cells merge during their downstream propagation, promoting to the ultimate generation of the distinct heavy rainfall centers in favor of local convective clusters over the 70–100-km downstream coastal city, where atmospheric columns are more moist and potentially unstable under the influences of sea breezes. Sensitivity simulations show small contribution of the downstream city but more influences of urbanization of the upstream city belt to the heavy rainfall event. The above findings not only help explain why more rainfall tends to take place on the downwind side of major cities, but also have important implications to the understanding of the UHI effects on the CI and downstream propagation of convective storms, leading to the eventual generation of heavy rainfall at locations where the regional environment is favorable. These findings have been published in Monthly Weather Review.
Session Chair(s): Yuqing WANG, Chinese Academy of Meteorological Sciences, Kun GAO, Princeton University
AS13-A039
Effect of the Initial Vortex Structure on Intensity Change During the Eyewall Replacement Cycle of Simulated Tropical Cyclones
Yuqing WANG1#+, Xinwei YANG2
1Chinese Academy of Meteorological Sciences, 2University of Chinese Academy of Sciences
This study investigates the effect of the initial tropical cyclone (TC) vortex structure on the intensity change during the eyewall replacement cycle (ERC) of TCs based on two idealized simulations using the Weather Research and Forecasting (WRF) model. Results show that the TC initially with a smaller inner core and weaker outer winds experienced a much more drastic intensity change during the ERC than that initially with a larger inner core and stronger outer winds. It is found that an initially larger TC vortex with stronger outer winds favored the development of more active spiral rainbands outside the outer eyewall, which slowed down the contraction and intensification of the outer eyewall and thus prolonged the duration of the concentric eyewall and slow intensity evolution. In contrast, the initially smaller TC with weaker outer winds corresponded to higher inertial stability in the inner core and weaker inertial stability but stronger filamentation outside the outer eyewall. These led to stronger boundary layer inflow, stronger updraft and convection in the outer eyewall, and suppressed convective activity outside the outer eyewall. These resulted in the rapid intensification of the outer eyewall, and thus rapid weakening followed by a rapid re-intensification of the TC during the ERC. Our findings demonstrate that the realistic initialization of TC structure in numerical models is key to the prediction of TC intensity change during the ERC, and monitoring the activity of spiral rainbands outside the outer eyewall may help improve the short-term intensity forecasts for TCs experiencing ERCs.
AS13-A035
Island-induced Eyewall Replacement in a Landfalling Tropical Cyclone: A Model Study of Super Typhoon Mangkhut (2018)
King Heng LAU1+, Francis Chi Yung TAM2,3#, Chun-Chieh WU4
1Imperial College London, 2The Chinese University of Hong Kong, 3Shenzhen Research Institute, 4National Taiwan University
An unconventional, island-induced eyewall replacement occurred in Super Typhoon Mangkhut (2018) when it crossed Luzon Island. Upon landfall, its original compact eyewall broke down and dissipated rapidly. As Mangkhut exited Luzon and entered the South China Sea, a much larger new eyewall formed at a radius of 150–200 km from the storm center, three times larger than the original one. Unlike the eyewall replacement cycle in intense tropical cyclones, the breakdown of the original eyewall preceded the formation of the new eyewall (NEF) in Mangkhut. This evolution was reproduced reasonably well in a control experiment using the Weather Research and Forecasting Model. Two sensitivity experiments confirmed that the evolution was triggered by Luzon Island, whose terrain is crucial for not only the destruction of the original eyewall but also the NEF. In an axisymmetric framework, it is demonstrated for the first time that the NEF was preceded by the following processes: (1) an increase in the outward forcing of the boundary layer (BL) inflow after landfall due to differential rates of weakening between the radial pressure gradient and the tangential wind, (2) creation of a BL deceleration zone, (3) localized reinforcement of BL inflow deceleration within the NEF region upon re-entry into ocean, following the unbalanced dynamical pathway proposed by Y.-H. Huang et al. (2012), and (4) strengthening of the BL convergence and uplift which initiated and sustained the deep convection of the new eyewall.
AS13-A063
On the Relationship Between the Secondary Eyewall Formation and Compensating Motion
Liang Yi KUO#+, Ching-Yuang HUANG
National Central University
An experiment for secondary eyewall formation (SEF) of Typhoon Hagibis (2019) is conducted using the WRF model. The simulated typhoon rapidly intensifies with the outer eyewall that forms later after the inner eyewall. The compensating sinking motion outside of the inner eyewall strengthens due to the rapidly developing upward motion inside the inner eyewall and the outer rainbands (ORBs) activities. The diabatic heating provided by ORBs is thus locally limited in the sinking motion region, forming a heating gradient pointing outward from the vortex center. The differential heating causes the supergradient force in the boundary layer (BL), which reduces the radial inflow at the inward side leading to radial convergence. Stronger vertical vorticity is generated due to stretching effects, which enhances inertial stability in the vortex and greatly facilitates the convection to migrate counterclockwise without eyewall contraction. On the other hand, BL convergence that induces upward motions provides more diabatic cloud heating as well as stronger compensating sinking motion and thus largely increases the radial heating gradient. The solutions of the Sawyer–Eliassen equation with the nonlinear forcing sources indicate that convective cloud heating associated with both inner eyewall and ORBs is essential for the establishment of SEF.
AS13-A031
Understanding the Mechanisms Leading to the Rapid Eyewall Replacement Cycle in Typhoon Haiyan (2013)
Jun Yu CHEN#+, Chun-Chieh WU
National Taiwan University
Traditional eyewall replacement cycle (ERC) usually weakens the intensity of tropical cyclones (TCs) (Sitkowski et al., 2011), but some TCs that undergoes short-duration ERC often exhibit no significant weakening (Fischer et al., 2020). Previously studies have indicated that initial moat width is positively correlated with ERC duration (Yang et al., 2021). Nevertheless, the detailed mechanisms still require further investigation. To identify the mechanisms that allow the eyewall replacement to be completed in a shorter time period, an ensemble analysis with 40 members by WRF Variational data assimilation (WRF-VAR) was used in this study to simulate the evolution of Typhoon Haiyan (2013), which experienced a short ERC duration and no significant weakening (Lin et al.,2021).The results of the WRF-VAR ensemble indicate a positive correlation between the duration of ERC and the initial moat width, in accordance with the findings of Yang et al. (2021). Subsequently, ensemble members are categorized into two groups, narrow (NG) and wide (WG), selected by the lowest 25% and highest 25% moat width. The analysis shows that there are no significant differences in the initial structural characteristics (e.g., tangential wind and filamentation time) between these two groups. In terms of environmental factors, the WG experiences greater environmental wind shear than the NG prior to the ERC, resulting in a more asymmetric distribution and activity of rainbands. The differences in environmental wind shear may be the cause of the different rainband activity between the two groups and the eventual deviations in moat width when the outer eyewall forms. The results indicate that environmental wind shear can influence the initial moat width, subsequently affects the ERC indirectly. In our future work, we will explore the reasons why a narrow moat accelerates ERC duration in greater details.
AS13-A006
What are the Finger-like Clouds Along the Inner Edge of Hurricane Eyewall?
Kun GAO#+
Princeton University
Regular finger-like cloud features, sometimes referred to as misovortices or helical striations, with alternating updrafts and downdrafts along the inner edge of the hurricane’s eyewall have been frequently captured in LES-type simulations and occasionally observed in radar images. However, many aspects of these features, including their formation mechanism, three-dimensional structure, lifespan and temporal distribution, remain largely unknown. In this study, we conduct high-resolution (~100-m grid spacing) idealized hurricane simulations using the GFDL SHiELD model to investigate these phenomena. Remarkably, we found that these finger-like features can be adequately captured even with a 500-m horizontal grid spacing. These features first manifest when the surface maximum wind of the hurricane reaches about 60 m/s. Once initiated, they persist and propagate azimuthally along with the TC circulation. These features dominate the vertical velocity field in the lower 3 km of the troposphere along the inner edge of the eyewall. A kinetic energy budget analysis suggests they are likely generated by the shear instability caused by the strong azimuthal wind shear. The latent heat release in their updraft cores also can enhance their overturning circulations.
AS13-A040
Impact of Solar Radiation on Low-level and Mid-level Vortices During Tropical Cyclogenesis in Idealized Simulations
Xiaodong TANG#+, Yusheng TENG
Nanjing University
This study investigates how the solar radiation will affect tropical cyclogenesis by examining the evolution of the low-level and mid-level vortices in simulated tropical depressions. Three experiments with distinct solar radiation conditions were conducted: the control experiment with real diurnal radiation, the day-only, and the night-only experiments. It is shown that the daytime radiative conditions were more favorable for mid-level vorticity development, while nighttime conditions were more conducive to low-level vorticity development. The daytime shortwave radiation promoted the formation of stratiform clouds and increased the vertical gradient of diabatic heating at the mid-troposphere, thereby facilitating the development of mid-level vorticity. The vorticity budget analysis showed that the changes in local low-level vorticity are primarily driven by horizontal convergence rather than vertical transport. This implies that the mid-level vorticity is hardly transported to the lower levels. The daytime shortwave radiation suppressed convective development, weakening low-level convergence and limiting low-level vorticity enhancement. These experiments demonstrated that the strong mid-level vorticity caused by solar radiation does not necessarily promote the development of low-level vorticity. Therefore, the acceleration of tropical cyclogenesis by the diurnal radiation cycle is primarily contributed from the low-level vorticity enhancement, which tends to occur at night.
AS13-A004
Effects of Urban Expansion and Anthropogenic Heat Enhancement on Tropical Cyclone Precipitation in the Greater Bay Area of China
Qinglan LI1#+, Lunkai HE2, Yuqing WANG3
1Shenzhen Institutes of Advanced Technology, 2Chinese Academy of Sciences, 3Chinese Academy of Meteorological Sciences
The impact of urban expansion and anthropogenic heat (AH) enhancement on tropical cyclone precipitation (TCP) in the Guangdong–Hong Kong–Macau Greater Bay Area (GBA) of China is investigated by using the Weather Research and Forecasting (WRF) model. Sensitivity experiments are conducted during the landfall periods of two tropical cyclones, Hato (2017) and Mangkhut (2018), by artificially varying the surface AH flux from 0 to 600 W/m2 and the urban land surface from 1985 to 2017, respectively. Results show that the TCP in the GBA's urban region increases with both urban expansion and AH enhancement. However, in the urban downstream region, only AH enhancement causes an increase in TCP, whereas urban expansion has no significant influence on TCP. AH enhancement and urban expansion affect surface temperature, surface sensible heat flux, and surface latent heat flux, leading to changes in atmospheric instability and surface water evaporation, resulting in changes in low-level moisture convergence. The change patterns of the vertically integrated moisture flux divergence between 850 and 910 hPa in the urban and urban downstream regions of the GBA are consistent with those of the TCP changes in this area, indicating that low-level moisture convergence is the key factor determining the TCP changes in the region.
AS13-A012
Tropical Cyclone Fullness and Outer Size Growth
Qiaoyan WU#+
Nanjing University of Information Science and Techonogy
The relationship between the growth of the 34-kt wind radius (R34) of tropical cyclones (TCs) and their fullness using best-track data from 2001 to 2020 was investigated. The storms were categorized into four groups based on a fullness scale: FS1 (fullness ≤ 0.4), FS2 (0.4 < fullness ≤ 0.6), FS3 (0.6 < fullness ≤ 0.8), and FS4 (fullness > 0.8). These groups exhibit unique spatial patterns of very deep convective clouds with infrared brightness temperatures <208 K. The mean R34 growth rates in 24 hr decrease from FS1 to FS4, which is linked to the higher coverage of very deep convection around R34 in storms with lower fullness. This study demonstrates that TC fullness can characterize the spatial distribution of deep convection in storms and serve as a representation of the growth of TC outer region size. These results have implications for understanding the mechanisms behind TC outer size growth.
AS13-A008
Factors Contributing to Tropical Cyclone Size Asymmetry in the Western North Pacific
Lifeng XU+, Kelvin T. F. CHAN#
Sun Yat-sen University
With the advancement in the satellite and reanalysis capability in recent decades, the understanding on the size of tropical cyclone (TC) has been gradually enhanced. However, the asymmetry of TC size receives limited discussion. In this study, we make use of the ERA5 global climatology and the novel definition of tropical cyclone size asymmetry to identify the factors and the corresponding mechanisms resulting in the asymmetric structure of TC size in the western North Pacific. Not only the main factors like TC motion and vertical wind shear, we also perform analysis on potential factors like synoptic flow, relative humidity, etc. In this conference, the comprehensive results will be shown and discussed.
Session Chair(s): Yali LUO, Nanjing University of Information Science & Technology
AS40-A008
How Do Microphysical Characteristics Differ Between Heavier and Lighter Convective Rainfall on the Monsoon Coast (South China)
Yanyu GAO1+, Yali LUO2#, Jiajia HUA1, Chong WU3, Juliao QIU3
1China Meteorological Administration, 2Nanjing University of Information Science & Technology, 3Chinese Academy of Meteorological Sciences
Extreme rainfall can be produced by convective systems with intense or weak convective intensity. However, why convective rainstorms with comparable convective intensities produce quite different rainrates remains elusive. This study investigates microphysical characteristics of Convective Precipitation Features (CPFs) in the Great Bay Area of South China using 5-year dual-polarization radar observations. A CPF is defined as a contiguous strong-echo (>40 dBZ) area of > 11 km2. The CPFs are classified according to their convective intensities (the maximum height of 40-dBZ echo; MaxH40dBZ) as “intense” CPFs (InCPFs; MaxH40dBZ>=9 km), “moderate” CPFs, and “weak” CPFs (WeCPFs; MaxH40dBZ< 6 km). The average of top 5% rainrates in each CPF is used to represent its rainfall intensity (RI). The 50th (53 mm/h) and 90th (117 mm/h) percentiles of the cumulative distribution function of RI are used to further separate each CPF-category into “heavier” rainfall (HR; RI>=117 mm/h), “medium” rainfall (MR; RI of 53–117 mm/h), and “lighter” rainfall (LR; RI<53 mm/h).Both WeCPFs and InCPFs have a wide range of RI from about 1mm/h to 200mm/h. However, the fraction of HR-CPFs increases substantially with increasing RI. Compared to HR- and MR-InCPFs, LR-InCPFs exhibit enhanced mixed-phase microphysical processes, a larger amount of supercooled liquid drops, larger hydrometeor sizes, and smaller horizontal span with higher cloud bases, which favors breakup and evaporation (rather than coalescence) of raindrops. The raindrop size distributions (RSDs) of LR-InCPFs extend from the “maritime” to “continental” regime with a mean concentration much lower than the MR- and HR-InCPFs. Although both size and mass of raindrops in WeCPFs increase downward due to the dominant coalescence in LR-, MR- and HR-WeCPFs, coalescence increases and breakup decreases with higher RI, which can be aided by larger horizontal span of WeCPFs with higher RI and lead to their larger raindrop sizes.
AS40-A005
On the Ensemble Simulation of a Warm-sector Torrential Heavy Rain with a Scale and Structural Perturbing Method
Yuchun ZHAO, Yehong WANG#+
Xiamen Meteorological Bureau
A warm-sector torrential heavy rain event occurred in the coastland area of southeast China and resulted in local floods and serious social impacts on the day of 7 May 2018. The forecasts of mesoscale and globe models available in real operation all gave a miss forecast. The WRF model were used to posteriorly simulate the warm-sector torrential heavy rain event and the results were quite sensitive to the initial fields and the experiment. In order to investigate the possibility of improving the simulation through structurally perturbing initial fields, a convenient and simple method of extracting small-magnitude perturbation with different scales and structures was developed to construct perturbed initial fields. The model initial variables of geopotential height, temperature, horizontal winds, relative humidity and their combinations were perturbed separately to conduct ensemble simulations. The scale and structural perturbations of single or combined variables all had the potentiality to improve the simulation. Model domain-averaged perturbed total energy of ensemble simulations of combined variables grew more quickly and was larger than that of single variable. The energy of ensemble simulations perturbing temperature and relative humidity grew more quickly and was larger than that of perturbing horizontal winds and geopotential height. The energy of ensemble simulations with larger scales perturbations grew faster and was larger than that with smaller scales perturbations. The members with different scale and structural perturbations all had the possibility to get a better simulation than the control experiment. No dependency on or preference to the scale and structure of the perturbations was found in the better simulations. That is, the initial background field played a crucial role in the value and usability of ensemble experiments.
AS40-A027
| Invited
The Predictability and Key Mechanisms of Record-breaking Extreme Rainfall in Northern China and Beijing in Late July 2023
Ming XUE1#+, Ziqi FAN2, Kefeng ZHU3
1The University of Oklahoma, 2Nanjing University, 3Chinese Academy of Meteorological Sciences
From 29 July through 1 August 2023, an extreme precipitation event occurred in northern China, with a maximum accumulated rainfall of more than 1000 mm in Hebei Province and over 700 mm of rainfall in the southwest suburb of Beijing, breaking many records. The extreme precipitation is a result of the reminiscent circulation of super-typhoon Doksuri interacting with the northwestward extending ride of subtropical high and with major mountain ranges in north China. While heavy precipitation was expected from the reminiscent typhoon circulation, the record-breaking precipitation amount was a major challenge to forecast. To understand the predictability of such a recording breaking and inherently rare extreme event, and the key processes responsible for the extreme precipitation, convection-allowing 3 km ensemble forecasts are produced, with different initial conditions and different combinations of physics parameterizations among the members. Most of the ensemble members actually produce maximum accumulated rainfall reaching or exceeding the observed maximum amount. The heaviest precipitation falls along the eastern slope of the Taihang Mountains Range, and the southern slope of the Yanshan Mountains north of Beijing, and alone a convergence zone between the typhoon circulation and the subtropical high ridge. Significant differences exist in the location and amount of maximum precipitation among the forecast members. Somewhat surprisingly, there is a higher sensitivity of the precipitation forecast to PBL scheme than to microphysics scheme. Detailed analyses are carried out to understand how the PBL and microphysics schemes affect the precipitation amount, and how the predicted precipitation depends on the initial condition. Insight is sought on the practical predictability of such extreme precipitation events, and what improvements are needed to improve forecast skills. Objective skill scores of both ensemble consensus forecasts and ensemble probability forecasts will also be calculated to gauge the practical prediction skills of state-of-the-art forecast models.
AS40-A009
Rainfall Forecast Performances and Error Sources for Typhoons Influencing China
Zifeng YU1,2#+
1Shanghai Typhoon Institute/China Meteorological Administration, 2Asia-Pacific Typhoon Collaborative Research Center
By using the object-oriented method of Contiguous Rain Area(CRA), this paper investigates the forecast error components of rainfall and their variation trends for different thresholds and forecast periods for typhoons influencing China in 2019. The correlation between typhoon track errors and displacement errors of rainfall objects is analyzed and the performance improvements of rainfall forecasts calculated with track correction or CRA shifting are compared. Finally forecast errors of rainfall probability distribution around typhoons, radial and asymmetric rainfall distribution are verified and analyzed. The results are as follows: (1) For different forecast periods and rainfall thresholds, the main forecast errors come from displacement error D and pattern error P and rotation error R is minimum. (2) Except for larger rainfall, track error is significantly correlated with displacement error of CRA rainfall object. The improvement of rainfall forecasts made by track error correction is less than that made by CRA shifting correction. (3) The shape of probability density function for rainfall forecasts around typhoon coincides with the observed one. Before and after typhoon making landfall or approaching near coast, the forecasted rainfall intensities in typhoon core area are stronger than the observed ones while they are different out of typhoon core area. (4) Before and after typhoon making landfall or approaching near coast, the forecasted rainfall is closer to typhoon center than the observed one and lagged behind it. The asymmetric structure of the forecasted rainfall is significantly weaker than the observed one especially after typhoon making landfall or approaching near coast.
AS40-A026
Landfalling Tropical Cyclone-induced Rainfall Over Asia in Present and Future
Mincheol MOON1+, Kyung-Ja HA2#, Seung-Ki MIN1
1Pohang University of Science and Technology, 2Pusan National University
The study focused on rainfall features of tropical cyclones (TCs) in the Asia, dividing them into rainfall strength (RS) and area (RA). It found the Western North Pacific (WNP) exhibits higher intensity and larger TC-induced rainfall area than the North Indian Ocean (NIO). In the NIO, RS increased notably, while in the WNP, RA saw a larger rise with increased carbon dioxide (CO2). Examining post-monsoon periods in the NIO revealed increased TC frequency in the Arabian Sea due to favorable conditions like increased LHFLX, weakened zonal circulation, and warming linked to global warming. In the WNP, TC-induced rainfall peaks from July to October; the South China Sea showed strong relationships between environmental factors and RA. However, in East Asia, mid-level humidity didn't significantly impact, but vertical shear played a pivotal role. The analysis stressed the importance of mid-latitude circulation phases in TC tracks, particularly favoring landfall in western East Asia/South China Sea with rising CO2. Recognizing these regional differences is crucial for understanding TC-related rainfall and underscores the need for tailored strategies and policies for managing increased TC frequency and intense rainfall risks in affected regions.
AS40-A006
A Global View on Microphysical Discriminations Between Heavier and Lighter Convective Rainfall
Yali LUO#, Ruizi SHI+
Nanjing University of Information Science & Technology
Microphysical differences between convective clouds producing different rainrates remain elusive. Using long-term records from spaceborne precipitation radars, we investigate the microphysical discriminations between heavier and lighter rainfall over the Earth. The convective precipitation events (CPEs) are classified according to their convective intensity measured using the maximum height of 30-dBZ echo (MaxH30dBZ) into the “intense” CPEs (InCPEs; MaxH30dBZ >9 km), “moderate” CPEs, and “weak” CPEs (WeCPEs; MaxH30dBZ < 5.5 km). Each category is further separated using the maximum near-surface rainrate within each CPE into “heavier” rainfall (HR; >60 mm/h), “medium” rainfall, and “lighter” rainfall (LR; <30 mm/h). The well-recognized convective hotspots on land with a high coincidence of all CPE categories are analyzed. The vertical profiles of maximal radar reflectivity differ between HR and LR mainly below 5 km, highlighting the importance of warm-rain microphysical processes in determining the rainrates. The larger raindrop size and stronger convective updrafts/downdrafts in InCPEs result in a larger fraction of raindrop breakup (30–62%) in the liquid-phase microphysical processes than that in WeCPEs (8–20%). Compared to the LR-InCPEs, the HR-InCPEs exhibit an increased fraction of coalescence plus coalescence-breakup balance (from 29% to 64%) and decrease of breakup processes (from 62% to 30%). In WeCPEs, the dominant coalescence increases from 44% for LR to 61% for HR, while the decreased breakup and evaporation decrease. While the maximum rainrates in InCPEs correspond to relatively large size and low concentration of raindrops than the WeCPEs producing the same category of rainfall, the HR-InCPEs have significantly higher concentration than the LR-InCPEs with a significant portion above the continental regime; the HR-WeCPEs show much higher concentration than the LR-WeCPEs. The higher raindrop concentration and enhanced coalescence for HR result from more humid environment and thicker warm-cloud layers, due to the variations in water vapor channels.
AS40-A001
Analysis of Uncertainties and Associated Convective Processes in Simulations of Extreme Precipitation Over Cities with a Regional Earth System Model: A Case Study
Zhenghui LI1+, Yali LUO2#, Feng CHEN3
1Chinese Academy of Meteorological Sciences, 2Nanjing University of Information Science & Technology, 3Zhejiang Institute of Meteorological Sciences
This study utilizes the Weather Research & Forecasting model coupled with an atmospheric chemistry model, a multi-layer urban canopy model (UCM), and a building energy model to simulate the extreme rainfall event influencing the Guangzhou city in South China on May 7, 2017. By employing small variations in the longwave emissivity of buildings within the UCM, 11 convective-permitting experiments are conducted. The simulated rainfall exhibits non-monotonic dependencies on the longwave emissivity. More extreme rainfall correlates with higher simulation uncertainties. The maximal 18-h and hourly rainfall accumulation vary from a 2-year return period to as high as a 20 or 40-year return period with notable spatial differences. Comparisons between the GOOD and POOR simulations highlight that some minor differences in the near-surface air thermodynamic conditions in urban area could lead to substantial differences in local convection and its impacts on subsequent convective systems. With persistent transportation of warm, moist airflows from the northern South China Sea, formation of a slow-moving mesoscale outflow boundary to the north of the urban agglomeration leads to the development of a quasi-stationary, compactly structured meso-γ-scale rainstorm in the GOOD simulations. The stronger low-level to near-surface convergence and mid-level cyclonic shear within this system substantially enhance low-level updrafts, leading to increased microphysical production and stronger horizontal advection of rainwater within the system. These findings offer some process-based understanding about the uncertainties in simulating urban extreme rainfall and underscore the need to develop ensemble forecasting methods for convection-permitting numerical models that incorporate increasingly complicated representations of anthropogenic influences.
Session Chair(s): Zhaoxia PU, University of Utah, Takeshi ENOMOTO, Kyoto University
AS47-A002
| Invited
Recent Progress in Assimilating Satellite Data for Improved Tropical Cyclone Prediction
Zhaoxia PU#+, Chengfeng FENG
University of Utah
Accurate tropical cyclone prediction is important yet challenging. Innovative satellite observing systems provide essential data sources for improving hurricane research and prediction. This talk will provide an overview of recent progress in satellite data assimilation efforts by the first author's research team, particularly aimed at enhancing tropical cyclone numerical simulation and prediction. The presentation will highlight several new developments, including 1) All-sky assimilation of GOES-R ( NOAA's Geostationary Operational Environmental Satellites) satellite radiances with bias correction and consideration of channel selections; 2) Joint assimilation of data from two NASA-supported smallSats missions, CYGNSS (The Cyclone Global Navigation Satellite System) and TROPICS (The Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats), using various configurations and integrated data assimilation techniques; and 3) Assimilation of ESA Aeolus satellite wind data. The talk will cover the significant impact of these data improvements on accurate numerical simulations of tropical cyclones, as well as the latest advancements in advanced data assimilation methods. Additionally, it will discuss the importance of data quality control and the specification of observational error characteristics. The presentation will also address the challenges and future directions in related fields.
AS47-A015
Adaptive Observation Error Inflation Impact on High-frequency Satellite Data Assimilation: An OSSE with NICAM-LETKF
Rakesh Teja KONDURU#+, Jianyu LIANG, Takemasa MIYOSHI
RIKEN Center for Computational Science
In our research, we explored the complexity of assimilating high-frequency satellite data into the NICAM-LETKF data assimilation system via an Observing Systems Simulation Experiment (OSSE). Three distinct experiments assimilated clear-sky AMSU-A satellite observations at different frequencies: hourly (1H), bi-hourly (2H), three hourly (3H) and six hourly (6H), alongside conventional observation data. Our findings revealed that 1H and 2H assimilations resulted in higher Root Mean Square Error (RMSE) for air temperature compared to 3H and 6H assimilation, indicating an introduction of dynamic imbalances at more frequent assimilation intervals. These imbalances were investigated by computing some representative measures such as the second-time derivative of vertical velocity and found more problematic in 1H and 2H than in 3H and 6H. To mitigate the identified imbalances in 1H and 2H, we adjusted horizontal localization parameters and inflated observation errors. The adjustment of horizontal localization in IH (HLOC) showed a reduction in air temperature RMSE by 5-10% but did not significantly affect the dynamic imbalance. Conversely, inflating observation error standard deviations manually by 60% in the 1H (Rinfl) experiment diminished imbalances by 5-10% and enhanced the global and tropical representation of air temperature, decreasing RMSE by 10-15%. Despite these improvements, manual tuning required for observation error standard deviations proved computationally intensive. To streamline this process, we applied the Adaptive Observation Error Inflation (AOEI) method that adjusts observation error standard deviations online by considering innovations. AOEI not only reduced the imbalance and RMSE effectively in the 1H (AOEI) experiment but also demonstrated superior performance compared to the 3H and 6H assimilation and comparable results to 1H (Rinfl). This approach was consistent in the 2H (AOEI) experiment as well. Consequently, our study concludes that the AOEI method can successfully rectify the imbalances triggered by high-frequency satellite data assimilation in the NICAM-LETKF.
AS47-A014
Thinning and Superobbing Test for Assimilating Satellite Aerosol Observations
Ebony LEE1+, Milija ZUPANSKI2, Seon Ki PARK1#
1Ewha Womans University, 2Colorado State University
Satellite observations offer the advantage of providing relatively high-resolution information on a global scale. Through data assimilation, they improve the initial field in regions where in-situ observations are challenging. However, preprocessing is encouraged before assimilation due to the computational cost and correlated observation errors associated with high-density observations. Thinning and superobbing methods are employed to decrease the quantity of observations, aiming to consist with the model scale and to mitigate the potential influence of horizontal correlations on observation errors. Since the optimal degree of thinning or superobbing varies in space and time, it should be adaptive. Therefore, we test the thinning and superobbing using aerosol optical depth (AOD) retrieved from the Geostationary Environmental Monitoring Spectrometer (GEMS) for the Asian dust storm cases, a high aerosol concentration event occurring in winter and spring over East Asia. The Maximum Likelihood Ensemble Filter (MLEF) and the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) are employed for the assimilation method and regional aerosol simulation model.
AS47-A012
Impact of a Triple-coupled Atmosphere-land-chemistry Data Assimilation System on Predicting Asian Dust Storms
Sujeong LIM1#+, Seon Ki PARK1, Milija ZUPANSKI2, Ebony LEE1
1Ewha Womans University, 2Colorado State University
Asian dust storms (ADSs) occur in the spring and early summer and transport mineral dust particles from the source regions—the Gobi Desert, Inner Mongolia, and Northeast China—over long distances to countries such as South Korea and occasionally to the United States. To improve the ADS prediction, accurate atmospheric and surface conditions as well as aerosol optical depth (AOD) are necessary. For example, soil moisture, representing the wetness conditions over the land surfaces of the source regions, can affect ADSs along with the wind variables. A coupled DA system can provide consistent initial conditions for a coupled prediction model with various components, including atmosphere, land, and chemistry observations. Aiming at developing a triple-coupled DA system, we used a triple-coupled atmosphere-land-chemistry DA system to understand the real environments of ADSs. For this purpose, we implemented the Maximum Likelihood Ensemble Filter (MLEF), a hybrid ensemble-variational data assimilation system, into the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) and conducted a preliminary study on an Asian dust event that occurred in March 2021. As a strongly coupled data assimilation system, MLEF assimilates atmospheric, soil moisture, and AOD observations—the National Centre for Environmental Prediction (NCEP) Prepared Binary Universal Form for the Representation of meteorological data (PrepBUFR), the National Aeronautics and Space Administration’s Soil Moisture Active Passive (SMAP) soil moisture retrievals, and Geostationary Environment Monitoring Spectrometer Level 2 AOD (GEMS AOD)—and simultaneously corrects the atmospheric, land surface, and AOD variables. We anticipate that the triple observations can provide useful information to predict the ADSs through cross-covariance impact.
AS47-A019
Insights from Very Large Ensemble Data Assimilation Experiments with a High Resolution General Circulation Model of the Red Sea
Siva Reddy SANIKOMMU1#+, Naila RABOUDI1, Mohamad EL GHARAMTI2, Peng ZHAN3, Bilel HADRI1, Ibrahim HOTEIT1
1King Abdullah University of Science and Technology, 2National Center for Atmospheric Research, 3Southern University of Science and Technology
Ensemble Kalman Filters (EnKFs), which assimilate observations based on statistics derived from samples of ocean states called ensemble, have become the norm for ocean data assimilation (DA) and forecasting. These schemes are commonly implemented with inflation and localization techniques to increase their ensemble spread and to filter out spurious long-range correlations resulting from the limited-size ensembles imposed by computational burden constraints. Such ad hoc methods were found not necessary in ensemble DA experiments with simplified ocean/atmospheric models and large ensembles. Here, we conduct a series of 1-year-long ensemble experiments with a fully realistic EnKF-DA system in the Red Sea using tens-to-thousands of ensemble members. The system assimilates satellite and in-situ observations and accounts for model uncertainties by integrating a 4km-resolution ocean model with ECMWF atmospheric ensemble fields, perturbed internal physics and initial conditions for forecasting. Our results indicate that accounting for model uncertainties is more beneficial than simply increasing the ensemble size, with the improvements due to large ensemble leveling off at about 250 members. Besides, and in contrast to what is commonly observed with simplified models, the investigated ensemble DA system still required localization even when implemented with thousands of members. These findings are explained by (i) amplified spurious long-range correlations produced by the low-rank nature of the ECMWF atmospheric forcing ensemble, and (ii) non-Gaussianity generated by the perturbed internal physical parameterization schemes. Large ensemble forcing fields and non-Gaussian DA methods might be needed to take full benefits from large ensembles in ocean DA.
AS47-A006
Second Year Progress of PREVENIR: Japan-Argentina Cooperation Project for Heavy Rain and Urban Flood Disaster Prevention
Takemasa MIYOSHI1#+, Yanina SKABAR2, Shigenori OTSUKA1, Arata AMEMIYA1, Juan RUIZ3, Tomoo USHIO4, Hirofumi TOMITA5, Tomoki USHIYAMA6, Masaya KONISHI7
1RIKEN Center for Computational Science, 2National Meteorological Service Argentina, 3University of Buenos Aires, 4Osaka University, 5RIKEN Advanced Institute for Computational Science, 6International Center for Water Hazards and Risk Management, 7Japan Meteorological Agency
This presentation provides recent research highlights of the project PREVENIR, including radar quantitative precipitation estimates (QPE), ensemble nowcasting, data assimilation, numerical weather prediction (NWP), and hydrological model prediction. PREVENIR is an international cooperation project between Argentina and Japan since 2022 for five years under the Science and Technology Research Partnership for Sustainable Development (SATREPS) program jointly funded by the Japan International Cooperation Agency (JICA) and the Japan Science and Technology Agency (JST). The main goal is to develop an impact-based early warning system for heavy rains and urban floods in Argentina. PREVENIR takes advantage of leading research on Big Data Assimilation (BDA) with the Japan’s flagship supercomputer “Fugaku” and its predecessor “K” and develops a total package for disaster prevention, namely, monitoring, QPE, nowcasting, BDA and NWP, hydrological model prediction, warning communications, public education, and capacity building. The total package for disaster prevention will be the first of its kind in Argentina and will provide useful tools and recommendations for the implementation of similar systems in other parts of the world.
AS47-A007
Advancing Forecast Precision: Data-driven Model Generation Via Data Assimilation
Michael GOODLIFF#+, Takemasa MIYOSHI
RIKEN Center for Computational Science
Data-driven models (DDMs) are mathematical or computational models built upon data, where patterns, relationships, or predictions are derived directly from the available information rather than through explicit instructions or rules defined by humans. These models are constructed by analysing large volumes of data to identify patterns, correlations, and trends. In areas such as numerical weather predictions (NWP), these DDMs are becoming increasingly popular with an aim to replace numerical models (or components of) based on real observations. Data assimilation (DA) is a process which combines observations from various sources with numerical models to improve the accuracy of predictions or simulations of a system's behaviour. This presentation focuses on the application of DA methodologies in enhancing the precision and efficiency of DDM generation within computation models characterised by inherent observation error. The aim is to demonstrate the pivotal role that DA techniques can play in refining and optimising the process of DDM generation, thereby augmenting the accuracy and reliability of predictive models despite the presence of observational uncertainties.
AS47-A010
| Invited
Adjoint Models Using Automatic Differentiation
Takeshi ENOMOTO#+
Kyoto University
Adjoint models enable calculation of sensitivity of the cost function to initial conditions or model parameters by performing integration backward in time. The foundation of the variational data assimilation is mathematically rigorous and the procedure to construct an adjoint model has been well-established. However, it is tedious and error prone to write an adjoint by hand. Traditional source-to-source compilers significantly reduce the labour but it still requires human examination. Recent advances in machine learning, which utilize adjoints for backpropagation, have promoted development of frameworks and tools, which typically include automatic differentiation (AD). Graph-based compilers such as JAX and Enzyme trace operators to construct a computational tree for gradient calculation. In this study, we apply JAX and Enzyme to generate adjoints of the three-variable Lorenz-63 model. AD adjoints reproduce exactly the solution of the hand-written code and can be run comparably owing to optimization.
Session Chair(s): Johnny CHAN, Asia-Pacific Typhoon Collaborative Research Center, Munehisa YAMAMOTO, Japan Aerospace Exploration Agency
AS06-A015
| Invited
Increasing Tropical Cyclone Intensity in the Western North Pacific Partly Driven by Warming Tibetan Plateau
Jing XU1#+, Ping ZHAO1, Johnny CHAN2,3, Chi YANG4
1Chinese Academy of Meteorological Sciences, 2Asia-Pacific Typhoon Collaborative Research Center, 3City University of Hong Kong, 4Beijing Normal University
The increase in intense tropical cyclone (TC) activity across the western North Pacific (WNP) has often been attributed to a warming ocean. However, it is essential to recognize that the tropical WNP region already boasts high temperatures, and a marginal increase in oceanic warmth due to global warming does not exert a significant impact on the potential for TCs to intensify. Here we report that the weakened vertical wind shear is the primary driver behind the escalating trend in TC intensity within the summer monsoon trough of the tropical WNP, while local ocean surface and subsurface thermodynamic factors play a minor role. Through observational diagnoses and numerical simulations, we establish that this weakening of the vertical wind shear is very likely due to the increase in temperature of the Tibetan Plateau. With further warming of the Tibetan Plateau under the Representative Concentration Pathway 4.5 scenario, the projected TCs will likely become stronger.
AS06-A017
| Invited
The Relationship Between ENSO and Tropical Cyclone Landfall Intensity; Its Change Under the Surface Warming
Doosun PARK1#+, Eunkyo SEO2, Minkyu LEE3, Dong-Hyun CHA4, Dasol KIM5, Chang-Hoi HO6, Myong-In LEE4, Hyeong-Seog KIM7, Seung-Ki MIN8
1Kyungpook National University, 2Pukyong National University, 3Korea Institute of Energy Research, 4Ulsan National Institute of Science and Technology, 5University of Florida, 6Seoul National University, 7Korea Maritime and Ocean University, 8Pohang University of Science and Technology
The El Nino Southern Oscillation (ENSO) is one of the most influential phenomena actively interacting with the atmosphere to affect weather and climate around the globe. In terms of intensity, the lifetime maximum intensity of TC becomes stronger during El Nino years than La Nina years. However, few studies have examined how intensity at landfall time is related to ENSO. This study shows the relationship of landfall intensity with ENSO and its change under the basin-wide SST warming. According to our analyses, the landfall intensity has no relationship with ENSO under the present SST condition, but if the SST is warmed, the catastrophic TC can hit the East Asian countries during the El Nino. [Funding. This study was supported by the Korea Meteorological Administration Research and Development Program (KMI2022-01312)].
AS06-A009
Probabilistic Analysis of Typhoon Characteristics and Variability Under Global Warming Based on SST Ensemble Simulations by Atmospheric Global Climate Model
Yoshiki MATSUO1#+, Tomoya SHIMURA1, Ryo MIZUTA2, Takuya MIYASHITA1, Nobuhito MORI1
1Kyoto University, 2Meteorological Research Institute
The latest report of the Intergovernmental Panel on Climate Change (IPCC) indicated with high confidence that the ratio of tropical cyclones (typhoons) classified into stronger categories would increase under global warming. However, probabilistic assessments for future changes in typhoon characteristics, which are necessary for coastal protection and adaptation to climate change, have not been conducted. Here, this study probabilistically shows variability and future changes in typhoon intensity, frequency, and typhoon-induced ocean waves. Previously, we developed the slab ocean coupled atmospheric global climate model (MRI-AGCM) by incorporating the ocean cooling induced by strong wind and then improved the model performance of typhoon intensity. Based on the coupled model, we conducted large ensemble simulations of active typhoon season under several representative sea surface temperature (SST) conditions because the variability of typhoon characteristics is considered related with SST spatial patterns. The ensemble simulations were conducted both under historical and future conditions (IPCC-SSP585 scenario). The representative SST conditions were selected to cover the historical SST variability by cluster analysis of 70 years of historical SST data. Based on the ensemble experiment, we quantified the future changes in typhoon characteristics and the natural variability related with SST conditions. Finally, the spectral wave model was forced by the wind of AGCM, and the extreme value distributions of ocean wave heights along the Japanese coast were quantified.
AS06-A014
Distinct Preceding Oceanic Drivers for Interannual Variation of Summer Tropical Cyclone–induced Rainfall in South and East China
Xiaocheng YU1#+, Yue ZHANG2, Wen ZHOU2
1City University of Hong Kong, 2Fudan University
China experiences significant impacts from torrential rainfall associated with tropical cyclones (TCs), particularly in the highly vulnerable regions of South China (SC) and East China (EC). These areas are known for their substantial interannual variation in TC rainfall. This study focuses on delineating the specific TC activities influencing these regions within the western North Pacific (WNP). Our analysis reveals that in SC, positive TC rainfall is primarily linked to a notable increase in TC genesis within the South China Sea (SCS) and the prevalence of westward TC tracks. In EC, rainfall patterns are shaped by a northward extension of both TC genesis and tracks. Further exploration into the modulation effects of preceding sea surface temperature (SST) anomalies in the eastern Indian Ocean (EIO) and the eastern Pacific unveils intriguing findings. Autumn warming in the EIO emerges as a key factor enhancing subsequent summer TC rainfall in SC. Conversely, La Niña events play a crucial role in increasing TC rainfall in EC during the subsequent summer. In summary, this research delves into the distinct atmospheric and oceanic mechanisms governing regional TC rainfall variation in SC and EC. The study underscores the significance of region-specific analyses in comprehending and forecasting TC impacts in China, providing valuable insights for improved disaster preparedness and mitigation strategies.
AS06-A020
Long-term Variability of Rapidly Intensifying Tropical Cyclones Over the Western North Pacific in Fall
Haeun JO1#+, Minkyu LEE2, Dong-Hyun CHA1, Mihye SEO1
1Ulsan National Institute of Science and Technology, 2Korea Institute of Energy Research
Most super typhoons occurring in the Western North Pacific experience the process of rapid strengthening of wind speed within a short period. Although it is hard to explicitly define the rapid intensification (RI) of tropical cyclones, it is generally specified as a period during which the intensification rate is greater than 30 knots (15.4 m/s) within 24 hours. This study delves into the long-term variability of rapidly intensifying tropical cyclones (RI TCs) from 1982 to 2020, occurring in the Western North Pacific. When analyzing the RI TCs by dividing the season into summer (July-August) and fall (September-October), there was a significant tendency for the proportion of RI TCs to increase among all tropical cyclones occurring in the fall. In addition, there was a tendency for the intensity of RI to become stronger in the fall. And, as the density of RI increases in the western part of WNP, the landfall rate in East Asia also showed a very significant tendency to increase, significantly above 10 degrees north latitude. Accordingly, to understand the reasons for the increase of fall RI TCs occurring in WNP, the long-term relationship with the environmental factors was elucidated from two perspectives: 1) Long-term trends of environmental factors and 2) Correlation between environmental factors and RI density. As a result, thermodynamic factors showed an increasing trend in areas of increased RI density. Additionally, the increase in RI density was found to have a moderate to high correlation with changes in thermodynamic variables such as sea surface temperature (SST) and tropical cyclone heat potential (TCHP).
AS06-A016
| Invited
Evaluation of New Version of the Global Satellite Mapping of Precipitation (GSMaP)
Munehisa YAMAMOTO1#+, Masato ITO2, Takuji KUBOTA1
1Japan Aerospace Exploration Agency, 2Remote Sensing Technology Center of Japan
The World Meteorological Organization (WMO) initiated the Space-based Weather and Climate Extremes Monitoring (SWCEM) project, recognizing the need to better utilize and improve the monitoring of weather and climate extremes from space. The Japan Aerospace Exploration Agency (JAXA) has participated in the project as one of the operators of meteorological or Earth observation satellites. The Global Satellite Mapping of Precipitation (GSMaP) product version 05 (algorithm version 8), released in December 2021, provides more than 25 years of hourly precipitation with a resolution of 0.1 degrees since January 1998. GSMaP products provide rainfall estimates not only from passive microwave radiometers and infrared radiometers, but also from rain gauge calibration over land. Some climatology statistics from daily to monthly such as average, extreme rainfall, and drought index are also updated. We investigated the performance of GSMaP to compare some other satellite rainfall products and rain gauges over the whole period. For example, in India, bias and correlation are better than the Integrated Multi-satellite Retrievals for GPM (IMERG). However, an underestimation of rainfall is confirmed along the coastal regions of the Western Ghats. The underestimation is mitigated for the gauge-calibrated products, even in the near real-time product. In this presentation, long-term evaluation results are also presented.
AS06-A012
Water Vapor Transport by an Equivalent-barotropic Cyclonic Anomaly Corresponding to Extreme Austral Late Summer Precipitation in Southeast Australia During 2021
Yue ZHANG#+, Wen ZHOU
Fudan University
Southeast Australia (SEA) experienced a wet February as well as an extremely wet March accompanied by devastating floods during 2021. Regional water vapor balance analysis at different levels indicates the leading role of water vapor inflow through zonal boundaries during February, and the dominant contribution of water vapor input through meridional boundaries during March, providing adequate anomalous moisture for abnormal precipitation. The horizontal distribution of vertically integrated water vapor flux is characterized as an anomalous cyclonic circulation pattern around the Tasman Sea and SEA, responsible for the intensified water vapor transport along northwesterlies from the tropical Indian Ocean and along anomalous onshore easterlies from the Tasman Sea during both months. Partition of the contributions of dynamic and thermodynamic processes to the anomalous atmospheric water vapor flux reveals the dominant role of the anomalous wind field, but the anomalous variation in the moisture field also plays a part in the water vapor convergence for SEA. The presence of upper and lower large-scale atmospheric circulations ascertains that cyclonic water vapor flux is attributed to a dominant equivalent-barotropic cyclone system over SEA. The plausible joint impacts of internal forcing from the positive southern annular mode (SAM) oscillation, and external forcing from La Ni ̃na, are further confirmed by composite analysis; a La Ni ̃na–induced low pressure system dominates the lower level over the Australian continent, and the SAM-caused anomalous cyclonic disturbance propagating from higher latitudes governs the higher level above southern Australia, leading to the important equivalent-barotropic cyclonic circulation just above the region of interest.
AS06-A018
Enhancement of Heat Wave Decision Support System Considering Disaster Management Circumstances
Suran KIM#+
National Disaster Management Research Institute
The research suggests enhanced methods for the decision criteria and systems, structural and unstructured heat waves measures through domestic and international literature and case studies to consider climate and disaster environmental changes. According to the results, it is necessary to develop a heat wave index that considers various variables such as weather conditions, regional characteristics, and the possibility of damage, and improve the response system by determining the level of crisis warnings by considering the developed index and weather warnings together. In addition, since the heat wave situation differs by region, it is needed to prepare detailed criteria for determining the heat wave situation by region and prepare action guidelines suitable for each standard. In addition, various information is needed for efficient decision-making, and it is necessary to upgrade the current heat wave decision-making support system to a platform by collecting and sharing not only weather information but also heat wave-related information such as health damage, livestock death, crop damage, and industrial damage. The research derives measures to improve heat wave measures suitable for domestic conditions through analysis of domestic and foreign heat wave response cases, which is expected to be used to establish a comprehensive plan for extreme heat waves and mid- to long-term heat waves in the future.
AS06-A019
Potential Consequences of Onshore Circulation on Relative Humidity and Heat Health in Parts of Eastern Asia
Robin CLARK#+
Met Office
In subtropical parts of Asia, heat stress often results from a combination of excessive temperature and relative humidity (RH). How these might change, as the world warms in coming decades, is thus of great concern. The two, however, are closely related. Air, warmed by 1°C, for example, can hold 7% more moisture, resulting in a reduced RH which would appear to be beneficial. For parts of Asia, though, onshore winds during the hottest part of the year favour the import of moisture from nearby seas with consequences for the potential RH reduction. My talk will discuss this issue and include resulting projections of future heat health using output from a recent perturbed physics ensemble of Met Office HadGEM3 model simulations.
AS06-A011
Sedimentary Records of Extreme Rainfall in Taiwan Since the Late Holocene
Jianfang HU#+
Chinese Academy of Sciences
Extreme precipitation events present serious risks to human safety and property. It is significant to predict the future patterns and trends of extreme rainfall. The investigation of these events within a geological historical context can provide valuable insights into them. This study reconstructed the history of intense precipitation events in Taiwan over the past 2800 years through a high-resolution analysis of bulk organic carbon (OC) in a sediment core (Core K11) taken from the Southwest Taiwan, northern South China Sea (SCS). Based on the radiocarbon dating (14C) technique, the Fraction modern (Fm) values of OC, representing the proportion of old carbon to modern carbon are obtained. The δ13C and 14C compositions of OC in the Core K11 reveal that the OC is predominantly derived from marine autochthonous production and island-derived petrogenic OC (OCPetro, Blattmann et al., 2018). Taiwan is orogenic, and a high, steep mountain belt has been developed on the island (Dadson et al., 2004). Due to its abundant rainfall, frequent typhoons and earthquakes, together with high relief and erosible rocks, a significant amount of 14C-depleted and δ13C-negative old carbon from bedrocks in Taiwan Island was transported to the northern SCS. A substantial input of old carbon from the bedrocks leads to a decrease in Fm values of the sedimentary OC. The Fm values in the Core K11 decreased during the periods of 16-23 yr BP, 137-164 yr BP, 504-614 yr BP, and 2272-2353 yr BP. Simultaneously, the δ13C showed a negative excursion, indicating a substantial input of old carbon from the Taiwan Island due to intense rainfalls. Hence, the combined application of δ13C and 14C of OC can be used to indicate intense precipitation events in Taiwan Island.
Session Chair(s): Muyin WANG, University of Washington, Seong-Joong KIM, Korea Polar Research Institute
AS45-A015
| Invited
The Influence of the Lower Stratospheric Polar Vortex on Cold Air Outbreaks Under Climate Warming
Edward HANNA1#+, Timo VIHMA2, Jennifer FRANCIS3, Muyin WANG4,5, James OVERLAND5
1University of Lincoln, 2Finnish Meteorological Institute, 3Woodwell Climate Research Center, 4University of Washington, 5NOAA Pacific Marine Environmental Laboratory
The connection between Arctic change and midlatitude weather events is a scientific challenge as events appear local, intermittent, and do not occur every year. This has led to ongoing controversy in the atmospheric community. Here we move beyond previous efforts by hypothesising that movement of the lower stratospheric polar vortex (SPV) to over North American Eurasia provides a mechanism for enhancing regional cold air outbreaks, and explains more Linkage events than when only considering Sudden Stratospheric Warmings (SSW). Based on a recent IASC/WCRP CliC workshop discussion, we identify the following themes as key priorities for further research in this area: Improving weather/climate predictions: improving our ability to predict and understand Arctic-Midlatitude linkages in global climate and Numerical Weather Prediction models for more accurate extreme weather, seasonal to sub-seasonal and climate projections. Stratosphere-troposphere coupling: developing a comprehensive framework for stratosphere-troposphere coupling events beyond just SSW, including asymmetric structures of the SPV, the role of large-scale circulation, and more detailed spatio-temporal analysis of SPV. Impact on extreme weather: investigating the influence of stratospheric forcing and lower atmospheric blocking on extreme weather events, such as temperature and precipitation extremes and identifying precursors in the troposphere. Climate change and Linkages: Examining the impact of climate change on Arctic Amplification and Arctic-Midlatitude linkages, particularly in relation to the Quasi-Biennial Oscillation (QBO) and other tropical drivers (e.g. El Niño Southern Oscillation), and the changing jet stream. Detection and attribution studies of Arctic influence, using AI methods. Model improvements: addressing challenges in numerical models, including their ability to capture Arctic-Midlatitude linkages, blocking, SPV interactions with the jet stream, and the need for better representation of Arctic Amplification in simulations while considering the trade-offs between significance and ensemble size. More non-linear tests and analyses of cross-timescale interaction are needed.
AS45-A010
| Invited
The Weakening of the Stratospheric Polar Vortex as a Consequence to Arctic Sea-ice Loss
Yu-Chiao LIANG1#+, Young-Oh KWON2, Claude FRANKIGNOUL3, Guillaume GASTINEAU3, Karen SMITH4, Lorenzo POLVANI5, Lantao SUN6, Yannick PEINGS7, Clara DESER8, Ruonan ZHANG9, James SCREEN10
1National Taiwan University, 2Woods Hole Oceanographic Institution, 3Sorbonne University, 4University of Toronto Scarborough, 5Columbia University, 6Colorado State University, 7University of California, Irvine, 8National Center for Atmospheric Research, 9Fudan University, 10University of Exeter
This study investigates the stratospheric response to Arctic sea-ice loss and subsequent near-surface impacts by analyzing 200-member coupled experiments using the Whole Atmosphere Community Climate Model version 6 (WACCM6) with preindustrial, present-day, and future sea-ice conditions specified following the protocol of Polar Amplification Model Intercomparison Project. The stratospheric polar vortex weakens significantly in response to the prescribed sea-ice loss, with a larger response to greater ice loss (i.e., future minus preindustrial) than to smaller ice loss (i.e., future minus present-day). Following the weakening of the stratospheric circulation in early boreal winter, the coupled stratosphere-troposphere response to ice loss strengthens in late winter and early spring, projecting onto a negative North Atlantic Oscillation-like pattern in the lower troposphere. To investigate whether the stratospheric response to sea-ice loss and subsequent surface impacts depend on the background oceanic state, ensemble members are initialized by a combination of varying phases of Atlantic Multidecadal Variability (AMV) and Interdecadal Pacific Variability (IPV). Different AMV and IPV states combined, indeed, can modulate the stratosphere-troposphere responses to sea-ice loss, particularly in the North Atlantic sector. Similar experiments with another climate model show that, although strong sea-ice forcing also leads to tighter stratosphere-troposphere coupling than weak sea-ice forcing, the timing of the response differs from that in WACCM6. We also analyzed additional atmosphere-only simulations without atmosphere-ocean coupling, in which the stratosphere-troposphere interaction is substantially weaker, and the largest stratospheric response occurs earlier in November, rather than in December and January. Our findings suggest that Arctic sea-ice loss can affect the stratospheric circulation and subsequent tropospheric variability on seasonal timescales, but modulation by the background oceanic state, model dependence, and atmosphere-ocean coupling need to be taken into account.
AS45-A007
Eurasian Winter Cooling Due to Tropical Western Pacific Convection
Ye-Jun JUN1+, Seok-Woo SON1#, Hera KIM1, Hyo-Seok PARK2, Jinho YOON3
1Seoul National University, 2Hanyang University, 3Gwangju Institute of Science and Technology
Concurrent with global warming, the Eurasian continent has experienced frequent cold winters in recent decades. Although still debatable, such Eurasian winter cooling, which was particularly pronounced over 1987-2006, has been attributed to internal climate variability, the process of which remains elusive. By examining multi-model large ensemble simulations, this study explores the potential sources of internal climate variability responsible for the Eurasian winter cooling trend over 1987–2006. Model simulations show a large ensemble spread in the Eurasian winter surface air temperature trend with an ensemble mean close to zero. A comparison of ensemble members with Eurasian winter cooling to those with warming reveals that the Eurasian winter cooling is accompanied by an anticyclonic sea level pressure (SLP) trend in the sub-Arctic region and a cyclonic SLP trend in the Aleutian region. This dipolar SLP trend is partly associated with enhanced tropical convection over the tropical western Pacific. The linear model simulation shows that the Rossby wave train excited by the tropical heating drives a cyclonic SLP anomaly in the Aleutian region. Its deepening is followed by an anticyclonic SLP anomaly in northern Siberia through mass redistribution. This result suggests that tropical convection has likely acted as a source of internal climate variability driving the Eurasian winter cooling in the recent past.
AS45-A006
Distinguishable Surface Precursors and Responses According to Sudden Stratospheric Warming Types
Hye Sun CHOI1+, Seong-Joong KIM1,2#, Joo-Hong KIM1, Baek Min KIM3
1Korea Polar Research Institute, 2University of Science and Technology, 3Pukyong National University
Sudden stratospheric warming (SSW) is characterized by an extremely weak polar vortex state and the reversal of the circumpolar westerly wind, often leading to cold outbreaks in mid-latitude regions of the Northern Hemisphere. SSW can be categorized according to vortex shapes during the pre- and postwarming periods: traditional “vortex displacement type” is classified as displacement-displacement (DD), while traditional “vortex split type” is classified as either displacement-split (DS) or split-split (SS) types. Unlike the SS type, which showed no clear association with the North Atlantic Oscillation phase before onset, the DS type had a tendency to precede a negative phase of the North Atlantic Oscillation, contrasting with the DD type, which precedes a positive phase. The prolonged negative North Atlantic Oscillation appears to help enhance the planetary wave-2 component, which then causes the stratospheric vortex to weaken and split. Within a subseasonal timescale of 20 days, the frequent occurrence of cold weather in North American was observed following DS type, driven by the development of a downstream trough accompanying the North Pacific ridge.
AS45-A025
Diagnostic Metrics for Evaluating Model Simulations of Arctic-midlatitude Linkages During Boreal Winter
Ha-Rim KIM1+, Baek Min KIM2#, Yong-Sang CHOI1, Jihan SIM2, Minjeong CHO1
1Ewha Womans University, 2Pukyong National University
A distinct midlatitude climate closely linked to the Arctic climate system has recently emerged as a robust testbed for evaluating climate prediction systems. Here, a comprehensive set of diagnostic metrics has been specifically developed to focus on Arctic-midlatitude linkages. The set is comprised of 10 items grouped into three sections: performance, linkages, and processes, encompassing four key variables. These quantitatively intuitive metrics aim to examine the fundamental aspects of the connection between Arctic and midlatitude climates. The diagnosis field includes climatology, teleconnection patterns, major variability modes, and stratosphere-troposphere coupling systems. In this study, three models are used to assess prediction performances, including the National Centers for Environmental Prediction Systems (NCEP CFS), the Global Seasonal Forecasting System version 5 (GloSea5), and new prediction systems developed as part of the Community Earth System Model 2 (CESM2). In evaluating metrics, Japanese 55-year reanalysis (JRA-55) data covering the boreal winter of 2001 to 2016 were used to validate three sub-seasons (October to November, December to January, and February to March) with two statistical methods (anomaly correlation coefficient and normalized root-mean-square error). GloSea5 excels at 6 out of 12 metrics items, especially as it pertains to Arctic Oscillation variability, upper-level circulation pattern, and anomaly thickness relating to boreal-winter temperatures. The NCEP CFS exhibits reasonable performance across all metrics throughout the sub-seasons, except for a deficiency in simulating upper-level circulation patterns. CESM2 reveals clear shortcomings in capturing major teleconnection patterns such as Warm Arctic-Cold Eurasia patterns compared to other models. Nevertheless, CESM2 shows a progressive enhancement of skills across the three sub-seasons. Possible origins that affect models’ performance are also discussed. Diagnostic metrics provide a tool to evaluate the performance of climate prediction systems, as well as to assess past and projected future changes in the boreal winter climate associated with the Arctic-midlatitude linkages.
AS45-A004
Record-breaking Barents Sea Ice Loss Favors to the Unprecedented Summertime Extreme Heatwave in 2021 Over Western North America by Enhancing Rossby Wave Ridge
Fei HUANG#+, Yuying WEI, Zheng CHEN
Ocean University of China
A record-setting extreme heatwave occurred over western North America (WNA) in the summer of 2021, which was associated with an extreme atmospheric Rossby wave ridge (ARR) over WNA and a minimum record event of the preceding winter Barents Sea ice concentration. We identify the remote effect and investigate how the Barents Sea ice loss (BSIL) in the preceding winter relates to the intensity of the ARR and extreme heatwaves in the following June and July (JJ) by analyzing the reanalysis data. Our results suggest that the atmospheric wave activity flux associated with the BSIL transferred wave energy towards the circumglobal teleconnection (CGT)-like wave trains, increasing the wave amplitude and enhancing the ARR over WNA. The anomalous sea ice melting in JJ, originating from the BSIL in the preceding winter through ocean-air-sea ice positive feedback processes, also induces a northward shift of jet stream by meridional temperature gradient change. The weakening of the local jet from the original jet axis area drives anticyclonic anomalies which increases atmospheric subsidence and shortwave radiation. The energy is transferred from the weakened jet to synoptic-scale disturbances via wave-current interaction. The northward jet as a waveguide causes the CGT to shift northward and receive signals from the higher latitude. Both the CGT-like wave trains and the shifted jet streams synergistically contribute to the increase of ARR intensity and the frequency of extreme heatwaves. Overall, the BSIL will serve as an early predictor for properly forecasting the extreme heatwaves over WNA six months in advance, which potentially improves the prediction skills.
AS45-A023
Exploring the Interplay Between Arctic Amplification and Arctic/Barents Oscillation Pattern
Baek-Min KIM1#+, Ho-Young KU1, Namkyu NOH1, Seong-Joong KIM2,3, Woosok MOON1
1Pukyong National University, 2Korea Polar Research Institute, 3University of Science and Technology
This study examines primary atmospheric circulation patterns and their interconnected dynamics over Northern high-latitudes in boreal winter. By applying Empirical Orthogonal Function analysis without detrending and latitude weighting to the surface air temperature anomaly over Northern Hemisphere winter, warm Arctic pattern emerges as a first mode and shows a strongly tendency especially with accelerated warming since 2000s. This pattern explains above 80% of variances of the well-known Arctic Amplification. In the same EOF analysis, the second and third modes align with the Arctic Oscillation (AO) and Barents Oscillation (BO) pattern. These patterns, largely non-trending, can be viewed as the leading internal variabilities of the northern winter. Of particular note is the significant influence of these two modes on the surface temperature variability across the Eurasian continent. When considered collectively, these three modes account for up to 70% of the temperature variability over Central Eurasia. The BO pattern accounts for 30-40% over central Eurasia, and the AO pattern accounts for about 40%, mainly over northern Eurasia. Conversely, the first mode, which could be seen as the spatial pattern of Arctic amplification, explains very little of the temperature variability over Eurasia. This suggests that the inherent spatial layout of Arctic amplification does not directly induce Eurasian temperature variability. However, it is significant to note that this finding does not dismiss the possible significant impact of Arctic amplification on mid-latitude temperature variability. Our study reveals an amplification of internal variabilities since the 2000s, coinciding with the expedited warming of the Arctic, as aptly portrayed in the first mode PC time series. In light of these findings, we propose that the significantly enhanced average Arctic temperature since the 2000s amplifies Northern mid-latitude internal variabilities. This amplification and its implications could be a central point of contention in the ongoing discussions concerning Arctic-midlatitude climate interconnections.
AS45-A016
Contrasting Deep and Shallow Winter Warming Over the Barents–Kara Seas on the Intraseasonal Time Scale
Juncong LI#+
Fudan University
The vertical structure of Arctic warming is of great importance and attracts increasing attention. This study defines two types of Arctic warming events (deep versus shallow) according to their temperature profiles averaged over the Barents–Kara Seas (BKS), and thereupon compares their characteristics and examines their difference in generation through thermodynamic diagnoses. A deep Arctic warming event—characterized by significant bottom-heavy warming extending from the surface into the middle-to-upper troposphere—emanates from the east of Greenland and then moves downstream toward the BKS primarily through zonal temperature advection. The peak day of deep warming event lags that of the precipitation and resultant diabatic heating over southeast Greenland by about four days, suggesting that the middle-to-high tropospheric BKS warming is likely triggered by the enhanced upstream convection at the North Atlantic high latitudes. In contrast, a shallow warming event—manifested by warming confined within the lower troposphere—is preceded by the meridional advection of warm air from inland Eurasia. These anomalous southerlies over Eurasian lands during shallow warming events are related to the eastward extension of the deepened Icelandic low. During deep warming events, the in situ reinforcement of the Icelandic low favors abundant moisture transport interplaying with the southeast Greenland terrain, leading to intense precipitation and latent heat release there. Both deep and shallow warming events are accompanied by Eurasian cooling, but the corresponding cooling of the deep warming event is profoundly stronger. Further, intraseasonal deep Arctic warming events could explain nearly half of the winter-mean change in the warm Arctic–cold Eurasia anomaly.
Session Chair(s): Pay-Liam LIN, National Central University
AS83-A014
| Invited
Climate Change Impact Assessment on Water Related Disasters and Adaptation in Japan
Eiichi NAKAKITA#+
Kyoto University
In recent years, climate related disasters have become more severe. Immediate implementation of adaptation measures is warranted. While scientific research is underway for the better assessment of climate change and its impact, which could be used for formulation of adaptation measures, we must pay attention to the change in and speed of climate risk. There are uncertainties in predictions of climate change and its impacts. However, for ‘no-regret adaptation”, we should apply the precautionary principle, and the lack of scientific evidence or information should not be reasons for inaction. Action without delay is imperative. While bottom-up approaches based on local realities are essential, at national level, it is also necessary to enhance cooperation among relevant government agencies and promote collaboration with both academic and DRR communities. Japanese government have decided razing water-protection standard and the transition to “River Basin Disaster Resilience and Sustainability by All.”
AS83-A007
| Invited
Characteristics and Causes of Taiwan’s Extreme Rainfall in 2022 January and February
Shao-Chin HUANG1, Wan-Ru HUANG2#+, Yi-Chao WU1, Yi-Chiang YU1, Jung-Lien CHU1, Ben Jong-Dao JOU3
1National Science and Technology Center for Disaster Reduction, 2National Taiwan Normal University, 3National Taiwan University
Over the past 40 years (1982–2021), the January and February (JF) rainfall in Taiwan has shown a clear decreasing trend. However, in 2022, the JF rainfall suddenly climbed to the third-highest value ever recorded in Taiwan. This study aims to explore the characteristics and causes of this unique event. Our results show that the significant increase in JF 2022 rainfall is contributed by both an increase in rainfall occurrence frequency and an increase in rainfall intensity. Further analysis shows that most of the JF 2022 rainfall is contributed by the rainy systems propagating from South China or the north of South China Sea to Taiwan but without the frontal structure, which is different from the general concept that JF rainfall is dominated by winter monsoon circulation-induced orographic rainfall and frontal rainfall. As a result, southern Taiwan experienced more than a 130% increase in JF 2022 rainfall compared to the JF climate mean. Possible physical explanations for the increase in JF 2022 rainfall can be attributed to the enhanced winter background circulation, which featured an enhanced regional northeasterly wind at 925 hPa coupled with an enhanced southwesterly wind transporting moisture at 700 hPa covering the domain of (10o-30oN, 100o-120oE). Consequently, an active convection zone extending from the southeastern Bay of Bengal to Taiwan was revealed in JF 2022 to result in the extreme rainfall in Taiwan. Further analysis also indicates that the relationship between the Taiwan JF rainfall and the tropical sea surface temperature has changed since 2002.
AS83-A008
| Invited
Predicting Extreme Wildfire Events: Evaluation of Operational Air Quality Models for the 2023 Quebec Wildfires
Sarah LU1#+, Chin-An LIN2, Rajesh KUMAR3, Shih-Wei WEI3, Stefano ALESSANDRINI 3
1University at Albany, State University of New York, 2University at Albany - State University of New York, 3University Corporation for Atmospheric Research
Wildfires release large amounts of air pollutants, including particulate matter (PM) and trace gases, into the atmosphere, which exerts significant influence on tropospheric chemistry and has detrimental effects on air quality, visibility, climate, and public health. Smoke plumes, once emitted, can be lifted into the free troposphere by fire-induced convection, transported over vast distances, and affect local and regional air quality. In the contiguous United States (CONUS), biomass burning contributes over 25% of the annual primary PM2.5 emissions, peaking in the western states during summer. Observational and numerical studies have shown human-induced climate change leads to an increasing trend of wildfire activity and severity in western boreal North America. Warmer and drier climate is favorable for the occurrence of wildfire activities, which could cause the increase of smoke aerosols. Consequently, the impact of wildfire activities on ambient air quality is expected to become increasingly significant. In 2023, Canada had a record-breaking wildfire season. More land burned in Quebec in June 2023 than in the previous 20 years combined. The smoke plumes caused unhealthy air quality affecting more than 100 million people in eastern North America. Over New York State (NYS), surface monitor network reported PM2.5 concentration exceeding 100 μg/m3, reaching up to 400 μg/m3 at some sites. In this study, we assess several regional and global forecasting systems using observations from surface monitoring network and NYS Mesonet profiler sites. Such assessments are critical for establishing credibility in using operational air quality forecasts for issuing timely air quality warnings to the public so that they can take preventive actions to protect themselves from exposure to smoke. Moreover, the diagnostics yields insights on whether the state-of-the-art models is adequate to capture wildfire-specific air pollution concentrations.
AS83-A011
Statistical Future Projections and Reproducibility Confirmation of Line-shaped Convective System Associated with Stationary Front Using High-resolution d4PDF
Mutsumi OKADA#+, Yukari NAKA, Kana FUKUDA, Eiichi NAKAKITA
Kyoto University
In these days, various water-related disasters caused by heavy rainfall are intensifying due to global warming. In Japan, line-shaped mesoscale convective systems (MCS) with Baiu front also have caused severe disasters, therefore, it’s important to investigate their future changes. Our objective is to evaluate probabilistically the future changes of line-shaped MCS using the 5-km resolution d4PDF. D4PDF stands for ‘database for Policy Decision making for Future climate change’. This dataset was downscale from the outer model with 20-km resolution. This 5-km d4PDF can represent even localized heavy rainfall, and consists of 720-year experiments with four scenarios; past, non-warming past, 2K and 4K warming scenarios. First, in order to investigate the line-shaped MCS, we extracted objectively stationary elliptical heavy rainfall areas from the 3-hour accumulated rainfall distribution of 5-km d4PDF. Then, we checked the spatial distribution of water vapor flux and equivalent potential temperature, which are characterized by the stationary front, and picked up only the line-shaped MCS associated with the stationary front. Next, we confirmed the reproducibility of localized line-shaped MCS in high-resolution d4PDF by comparing it with observational past cases. As a result, it’s confirmed that even 5-km d4PDF can reproduce various patterns of localized line-shaped MCS associated with the stationary front, although the reproducibility is still limited depending on the region and spatial scale. In addition, it’s found that the frequency of line-shaped MCS increases with the progression of warming, even in regions where the occurrence of line-shaped MCS isn’t so frequent in the present climate, such as northern Japan. As a future plan, we would like to evaluate other indicators (e.g., total rainfall, seasonality, and so on) of future changes in line-shaped MCS in order to get meaningful conclusions for disaster prevention planning.
AS83-A018
Examining the “Lower Stability-get-wetter” Mechanism in Tropical Oceanic Precipitation Changes Under Global Warming
Rung-Ying SU1,2#+, Jia-Yuh YU2
1Academia Sinica, 2National Central University
Many studies have investigated how total precipitation across the tropical oceans will respond to global warming. Firstly, the renowned “wet-get-wetter” mechanism emphasizes that the water vapor increase induced by a warmer temperature leads to an increase (or decrease) in precipitation over the climatologically ascending (or descending) regions under global warming. On the other hand, the “warmer-get-wetter” mechanism argues that it is not the water vapor but the spatial pattern of sea surface temperature (SST) warming that determines the change of precipitation. That is, enhanced precipitation only occurs over areas that have the greater SST warming. In this study, we introduce the “gross moisture stratification” (Mq), a variable indirectly linked to atmospheric stability, and propose the “lower stability-get-wetter” mechanism to compare with the earlier mechanisms as well as to explain the change in precipitation over tropical oceans. The simulations in historical and SSP5-8.5 experiments from 24 models in the Coupled Model Intercomparison Project Phase 6 (CMIP6) are examined. The classification of tropical oceans based on the three mechanisms shows that the “warmer-get-wetter” and “lower stability-get-wetter” mechanisms outperform the “wet-get-wetter” mechanism in representing the change in tropical precipitation under global warming. Furthermore, the distribution of change in tropical precipitation exhibits a stronger spatial correlation to the pattern of Mq change than to the pattern of SST change, regardless of seasonal variation. These findings suggest that the “lower stability-get-wetter” mechanism is more appropriate to account for the precipitation changes over the tropical oceans under global warming.
AS83-A030
The Philippine Sea Atmospheric Quasi-biweekly Oscillations and Springtime (March-May) Precipitation Sub-seasonal Variability and Extremes and Their Prediction in the South China Sea and Surrounding Region
Yin-Min CHO#+, Mong-Ming LU
National Taiwan University
Rainfall in the South China Sea (SCS) and surrounding regions can be influenced by multiple-scale weather and climate systems. To enhance the resilience to extreme weather, more researches are needed to investigate the extended-range (5-20 days) rainfall prediction skill in the current state-of-the-art S2S prediction models. The improvement of the extended-range prediction relies on the progress in understanding the large-scale atmospheric intra-seasonal (10-60 days) variability (ISV). The ISV in the Asian-western Pacific monsoon region can be categorized in two time scales: the 30-60-day oscillations such as the MJO and quasi-biweekly oscillations (QBWO) such as the equatorial Rossby waves (ERW). The QBWO is more pronounced than MJO during the months from March to May over the SCS and the surrounding region. In this study, the QBWO over the Philippine Sea is identified in the OLR data during the period from 1991-2023. After separating the 33 years into three categories of strong-QBWO, weak-QBWO, and no-QBWO, we found that the contrast in seasonal rainfall is significantly enhanced especially over the coastal region of South China and the eastern Philippines (4˚-20˚N, 122˚-130˚E). How the QBWO can influence the sub-seasonal rainfall variations and extremes in the Philippines will be discussed. The QBWO related extended-range forecast skill of the sub-seasonal peak rainfall event over the eastern Philippines assessed based on the S2S prediction database (Vitart et al. 2017) will be presented.
AS83-A033
Track Deflection of Typhoon Chanthu (2021) Near Taiwan as Investigated Using a High-resolution Global Model
Ya-Shin CHI1#+, Ching-Yuang HUANG1, William SKAMAROCK2
1National Central University, 2National Center for Atmospheric Research
The global model MPAS with multiple resolution (60-15-1 km) is used to investigate the track deflection of Typhoon Chanthu (2021) near Taiwan. Chanthu exhibited a rightward track deflection as it approached southeast Taiwan and underwent a leftward deflection when moving northward offshore of northeast Taiwan. Numerical experiments are conducted to identify the physical processes for the track deflection. The rightward deflection of the northbound typhoon is induced by the recirculating flow resulting from the effect of Taiwan’s topography. The northward turn of the simulated track toward southeast Taiwan does not occur in the absence of the large-scale MJO flow component. A wavenumber-one potential vorticity (PV) budget analysis indicates that horizontal PV advection dominates the earlier rightward deflection, while the later leftward deflection is mainly in response to stronger asymmetric cloud heating at low levels at the offshore quadrant of the typhoon. A pair of cyclonic and anticyclonic gyres in the wavenumber-one flow difference is induced by Taiwan’s topography. These rotate counterclockwise to drive the track deflection, most often in westbound typhoons. Idealized WRF simulations are also conducted to explore the track deflection under different northbound conditions. The simulations confirm the track deflection mechanism with similar PV dynamics to the real case and illustrate the variabilities of the track deflection for different steering conditions and vortex origins. The rightward deflection of northbound typhoons is essentially determined by a reduced ratio of R/LE where R is the vortex size and LE is the effective length of the mountain range.
Session Chair(s): Bin YUAN, Jinan University, Xiaodong XIE, Nanjing University of Information Science & Technology
AS08-A015
| Invited
Volatile Chemical Products (VCPs) Emissions in China: Emission Characteristics, Emission Estimates and Environmental Impacts
Bin YUAN1#+, Yibo HUANGFU1, Sihang WANG1, Yuanting ZHANG1, Yang YANG1, Yubin CHEN1, Weiwei HU2, Xuemei WANG1
1Jinan University, 2Chinese Academy of Sciences
As an emerging source for organic compounds in the atmosphere, volatile chemical products (VCPs) emissions can strongly affect regional air quality. However, the emission characteristics and strengths of VCPs is not understood well in China. In this presentation, I will introduce recent experimental and modelling activities in our group to characterize organic compounds from the most important VCPs. Using this information, an updated gridded emission inventory of VCPs in China is compiled and emission patterns will be analyzed. In the end, the contributions of VCPs emissions to organic compounds and secondary formation of ozone and organic aerosols will be investigated.
AS08-A034
Seasonal Quantification of the Inter-city Transport of PM2.5 in the Yangtze River Delta Region of China Based on a Source-oriented Chemical Transport Model and the Michaelis-Menten Equation
Jianlin HU#+
Nanjing University of Information Science & Technology
Regional transport plays a crucial role in the pollution of fine particulate matter (PM2.5) over the Yangtze River Delta region (YRD). A practical joint regional emission control strategy requires quantitative assessment of the contribution of regional transport. In this study, the contribution of inter-city transport to PM2.5 among the 41 cities in the YRD region were quantitatively estimated using a source-oriented chemical transport model, and then the relationship between the cumulative contribution of regional transport and the distance was examined using the Michaelis-Menten equation. The results show that the Michaelis-Menten equation is suitable to represent the relationship between the cumulative contribution and transport distance. The coefficient of determination (r2) of the fittings is greater than 0.9 in 71% of the cases in the six subregions and four seasons in YRD. Two key parameters in the Michaelis-Menten equation K1, indicating the maximum contribution of regional transport, and K2, indicating the distance to which the regional transport contribution reach half the maximum contribution, show substantial regional and seasonal variations. The average K1 is 73.6%, with lower values observed in the northern part of the YRD and higher values in central Jiangsu. K2 is larger in northern Jiangsu, as well as central and southern Zhejiang. The local contribution in autumn and winter is lower than that in spring and summer in the northern part of the YRD. Particularly in northern Jiangsu, the local contribution reaches 90.4% in summer but drops to 53.0% in autumn and winter, illustrating significant impacts of regional transport to PM2.5 in autumn and winter in this area. K2 is larger on polluted days, compared to clean days, indicating greater contributions from regional transport to PM2.5 in YRD. The results can serve as a scientific foundation for implementing regional joint prevention and control measures in the YRD region.
AS08-A021
The Historical, Present and Future Impact of Transboundary Pollution on China’s Air Quality and Public Health
Junwei XU1#+, Jintai LIN1, Lulu CHEN1, Ruijing NI2
1Peking University, 2Max Planck Institute
Fine particulate matter (PM2.5) pollution is a severe problem in China. Research on the sources of Chinese PM2.5 pollution has focused on the contributions of China's domestic emissions. However, the impact of foreign anthropogenic emissions has typically been simplified or neglected, partly due to the perception that the short lifetime of PM2.5 (a few days) does not allow long-distance transport. Through a series of studies, we revealed that 8 % of PM2.5 (5 µg m−3) and 19 % of nitrate (2.6 µg m−3) over eastern China in 2015 was contributed by foreign anthropogenic emissions. Yet, only 30 % of such foreign contributions in January were through direct atmospheric transport. The majority (70 %) were through chemical interactions between foreign-transported aerosol precursors and China's domestic emissions of pollutants. We further assessed the extent to which future changes in foreign transboundary pollution would affect the achievability of air quality goals in 2030 and 2060 for China. We found that China and foreign countries need to adopt low-carbon emission pathways coincidently to reduce air pollution and related premature deaths in China effectively. Our research also indicated that foreign emissions had caused an increase of 2-11 ppb in near-surface ozone concentration in China, with more than half of it resulting from chemical reactions during the transport of pollutants from abroad. In another long-term study, we also explored the impact of transboundary pollution transport on PM2.5 and ozone, quantifying the effects of changes in anthropogenic emissions since 1950 on global air quality and public health. We found that transboundary pollution transfer had led to premature deaths of tens of millions of people worldwide. Developed countries have been the major pollution sources for a significant period, providing a scientific basis for building a global environmental cooperation framework based on historical responsibility.
Session Chair(s): Pao-Shin CHU, University of Hawaii
AS13-A064
| Invited
Land-sea Contrast Leading to a Speedup of Landfalling Tropical Cyclones
Johnny CHAN1,2#, Wansuo DUAN3, Quanjia ZHONG4+, Shifei TU5, Jianping LI6, Ruiqiang DING7
1Asia-Pacific Typhoon Collaborative Research Center, 2City University of Hong Kong, 3Institute of Atmospheric Physics, Chinese Academy of Sciences, 4The Hong Kong University of Science and Technology, 5Guangdong Ocean University, 6Ocean University of China, 7Beijing Normal University
Changes in the translation speed of landfalling tropical cyclones (TCs) pose great challenges in disaster preparedness. However, the short-term variations (i.e., hour-to-day timescales) of TCs before landfall have not been systematically investigated, leaving a crucial gap in our understanding. Here we show, based on observations, that globally, a TC approaching landfall tends to accelerate towards the coast, resulting in a mean translation speed increase of approximately 48% during the 60-hour period prior to landfall. A numerical simulation demonstrates that land-sea difference in surface roughness results in an azimuthally asymmetric flow and convection associated with the TC, both of which are enhanced as the TC moves closer to the coast, leading to an increase in the potential vorticity tendency, and thus an acceleration of the TC.
AS13-A037
Interdecadal Change of Tropical Cyclone Translation Speed in South China Sea: Observations, Model Results, and Possible Mechanism
Pao-Shin CHU1#+, Kaiyue SHAN2
1University of Hawaii, 2Tsinghua University
Long-term variations in the translation speed of tropical cyclones (TCs) in the South China Sea (SCS) are studied based on five TC datasets from different institutions. TC translation speed shows an evident rhythm of interdecadal change throughout 1977-2020. This change can be well reproduced by a newly developed trajectory model. The model results indicate that this interdecadal change is primarily due to a corresponding change in the steering flow in the SCS, and such change is closely related to an east-west shift of the subtropical high in the western North Pacific (WNP), which may be driven by the zonal sea surface temperature (SST) gradient between the north Indian Ocean and WNP basins. A new index of the zonal SST gradient is proposed, which is shown to be effective for indicating the interdecadal change in east-west shift of subtropical high, and thus, the TC translation speed in the SCS.
AS13-A061
Deep Learning-based Tropical Cyclone Track Forecasting Using Through Combining of Satellite Observations and Numerical Model Outputs
Juhyun LEE+, Jungho IM#
Ulsan National Institute of Science and Technology
Tropical cyclones (TCs) are severe meteorological events with severe wind and heavy rainfall, which induce high socio-economic damage. Forecasting the track of TCs is therefore one of the most important tasks in the meteorology field. It has been improved with remarkable achievement of improvement in numerical prediction systems. In decades, the error of the task has decreased about 60 %. There are two major contributors to the improvements: the increase in realistic measurements and the advancement of data assimilation techniques. While the numerical model-based forecasts are governed by numerically solved equations, an accurate initial condition is necessary. Here, several observations such as buoys, radar, and satellites played important roles in preparing more precise initial conditions. On the other hand, several unusual atmospheric-ocean events, which cannot be described using existing physics, have been observed because of ongoing climate change. In this study, we proposed the fusion deep learning-based track forecasting model through the fusion of satellite observations and numerical model-based reanalysis data. It consists of two deep learning-based models: 1) image generative model-based pre-trained model and 2) fusion deep learning-based TC track forecasting model. The pre-trained model was conducted to simulate the forecaster’s knowledge of analyzing water vapor flows of satellite observation. The fusion deep learning-based model was constructed with several sets of 2D-CNNs and 3D-CNNs. It showed significant performance compared to the previous studies with a mean distance error of 87.5 km: a latitudinal distance error of 51.7 km and a longitudinal distance error of 59.9 km. It showed better performance compared to the previous deep learning-based approach and comparable performance to the operational forecasts.
AS13-A046
Development of Interpretable Probability Ellipse in Tropical Cyclone Track Forecasts Using Multiple Operational Ensemble Prediction Systems
Seungwoo YOO1+, Chang-Hoi HO2#
1Seoul National University, 2Ewha Womans University
Most tropical cyclone (TC) forecasting centers have implemented a probabilistic circle to represent track uncertainty at a specified lead time. Recent studies suggest that probability ellipses constructed from ensemble prediction systems can convey the anisotropy of track predictability. In this study, a new probability ellipse model is developed to interpret the extent of forward speed and heading uncertainties in ensemble forecasts by selecting an equal proportion of members in the along- and cross-track directions. This method is validated using the 2019–2021 western North Pacific (WNP) TC track forecasts from the ensemble predictions of the European Centre for Medium-Range Weather Forecasts, the United States National Centers for Environmental Prediction, and the Korea Meteorological Administration. When the proportion of ensemble members in the ellipse is set to 70%, more than one-half (50.0%–73.6%) of the forecasts, depending on the lead time, indicate reduced area compared with that of the circle. The mean areas of the probability ellipses are 4.9%, 7.0%, 10.0%, and 11.5% smaller than those of the circle in 48-, 72-, 96-, and 120-h forecasts, respectively. The forward speed shows greater uncertainty than the heading, as evidenced by the along-track radii being larger than the cross-track counterpart in ~60% of the samples, regardless of the lead time. In addition, the regional distribution of the along-track/cross-track ratio in the probability ellipses can explain the dominant direction of the track error in a particular location. The proposed probability ellipse shows potential for application in operational TC track predictions.
AS13-A003
Comparisons Between the Predictability of Tropical Cyclone Track Forecasts in Western North Pacific and Atlantic Basins
Feifan ZHOU#+
Chinese Academy of Sciences
Recent several studies have focused on the predictability of tropical cyclone track forecast. As a response to the question issued by Landsea and Cangialosi (2018) about “the approaching limit of predictability for tropical cyclone track prediction is near or has already been reached”, Zhou and Toth (2020) (short for ZT20) and Yu et al. (2022) (short for Y22) have found that the limit of predictability for tropical cyclone (TC) track prediction has not been reached both in Atlantic (ATL) and Western North Pacific (WNP) regions. However, the predictabilities are different in ATL and WNP regions, as ZT20 found that the 1 day’s improvement can be obtained through 10 years time in ATL, while Y22 found that 2 days’ improvement can be obtained through 15 years time in WNP. Now an interesting question is what causes this difference? To answer this question, this study first checks the predictability of TC tracks in WNP region using the same method as ZT20. Then the error growth rates in both two regions are compared and analyzed. The error growth rate in WNP is found to be higher than that in ATL. This suggests a low predictability of track forecast in WNP. A further investigation about the possible reasons for the different growth rates between ATL and WNP is carried out. The results suggested that TCs in WNP basin have averagely larger size and stronger intensity, which results in a faster growth of error and therefore larger error growth rate. Finally, it is pointed out that because the improvement of forecast skill mainly due to the reduction of initial analysis, although a low predictability is found in WNP region, the improvement of forecast skill in WNP is faster than that in ATL.
AS13-A019
Insight from Global Convection-permitting Model on Forecasting the Typhoon Track
Jun GU1+, Chun ZHAO1#, Jiawang FENG1, Gudongze LI1, Mingyue XU1, Qiuyan DU1, Yubin LI2, Guanghua CHEN3
1University of Science and Technology of China, 2Nanjing University of Information Science & Technology, 3Chinese Academy of Sciences
Successfully forecast track and strength of typhoon would be very important to assess its impact and make mitigation strategy. However, the advance of typhoon track forecasting is very slow if not decelerating in last decades. A few approaches have been applied to improve the skill of numerical weather prediction, with one as increasing model horizontal resolution that could theoretically improve the solving of dynamical equations and reduce the uncertainties from sub-grid physical parameterization. The typhoon In-Fa in 2021 was recognized as one of the top ten weather and climate events in China due to its prolonged duration and severe impact over the continent. Its slow moving speed and complex track make it difficult to be forecasted successfully. Our results show that global convection-permitting forecast can overwhelm the global forecasts at the horizontal resolutions of 15 km and 60 km in terms of the typhoon track. Particularly, the global convection-permitting forecast is also much better than the global forecast with regional refinement at convection-permitting resolution that covers the entire typhoon track, due to better forecasted large-scale circulation in the former one. Multiple global forecasts with regional refinements at different regions reveal that the improvement from global convection-permitting forecast results from its better performance on forecasting subtropical high, cold vortex, neighboring typhoons, and monsoon depression at higher-resolution. Our results imply that it is critical to increase the model resolution to convection-permitting scale covering not only the region with typhoon track but also the regions with the systems interacting with typhoon in order to successfully forecast typhoon track.
AS13-A070
Dynamic Mechanisms on the Track Changes of Typhoon Hinnamnor (2022)
Pin-Hong CHEN#+, Ching-Yuang HUANG
National Central University
This study uses the WRF model to simulate the track evolution of Typhoon Hinnamnor (2022) and explore the dynamic processes associated with the track changes. At the initial stage, the track moves westward as influenced by the steering flow southwest of the subtropical high. Due to interactions with a tropical depression (TD) to the southwest, as a result of Fujiwhara effect, the track of Hinnamnor is shifted southwestward. The TD merges with Hinnamnor at the end, leading to the typhoon's stagnation and intensification. The typhoon circulation is gradually enlarged with stronger flow to the south and east of the vortex, resulting in a noticeable northward component that drives the typhoon northward. This study is divided into two parts to investigate the track evolution. The first part explores the interaction with the TD. Potential vorticity (PV) budget analysis indicates that contributions from diabatic heating increase to counteract the horizontal PV advection, as a primary factor for the typhoon to move southward. After merging, the horizontal PV advection then dominates to drives the typhoon northward. Idealized simulations also confirm the similar mechanism for the track changes in the real case. The second part is aimed to explore the processes involved in typhoon's northward turn that may be related to internal vortex dynamics under the influence of terrain effects. Sensitivity experiments with removal of nearby terrain and different cloud parameterization schemes are conducted to identify their different impacts on the typhoon's northward turn.
Session Chair(s): Jung-Eun CHU, City University of Hong Kong
AS40-A004
| Invited
Preceding Winter Okhotsk Sea Ice as a Precursor to the Following Winter Extreme Precipitation in South China
Jianping LI1#+, Kai JI2, Zhongshi ZHANG2, Ruiqiang DING3, Yurun TIAN4,5, Yongqi GAO4, Jiayu ZHENG4
1Ocean University of China, 2China University of Geosciences, 3Beijing Normal University, 4Chinese Academy of Sciences, 5Hebei Normal University
The winter extreme precipitation over South China (SC) experiences a large year-to-year variability, causing uncertainty in its prediction. Here, we find that the boreal winter sea ice concentration (SIC) in the Okhotsk Sea can serve as a precursor to the following winter's extreme precipitation frequency (EPF) over SC, which has important implications for its prediction. Further analysisreveals that the Okhotsk Sea SIC anomalies help to reinforce North Pacific Oscillation-like atmospheric variability over the North Pacific, which inducesthe development of El Niño-Southern Oscillation (ENSO)-like SST anomalies in the equatorial eastern Pacific. The ENSO may act as a “power amplifier” to boost the impact of the Okhotsk Sea winter SIC anomalies on the following winter EPF over SC via a positive atmosphere–ocean feedback process. Our findings suggest that the Okhotsk Sea SIC may act as a potential precursor for the winter EPF over SC leading by about 1 year, and further improve our understanding of extratropical-tropical interactions and aid predictability of winter extreme precipitation over SC.
AS40-A018
| Invited
Offshore Migration of Summer Monsoon Low-level Jet on a Diurnal Scale
Yu DU#+
Sun Yat-sen University
The low-level jet (LLJ) in the summer monsoon plays a crucial role in affecting nocturnal downstream precipitation in South Asia. This study investigates the diurnal migration of the LLJ over the Bay of Bengal in the summer monsoon, which remains understudied despite the well-documented diurnal offshore propagation of rainfall worldwide. The southwesterly LLJ exhibits maximum strength during the night and morning. The LLJ undergoes a substantial eastward migration of approximately 600 km from the eastern offshore of India at midnight to the center of the Bay of Bengal by afternoon. A linear land-sea breeze model is effective in capturing the diurnal migration with similar speed and phase. Including background wind offshore extends the migration, rather than confining it to the coast. This migration is driven by inertia-gravity waves arising from the diurnal land-sea thermal contrast and is influenced by the westerly upstream wind from the Indian subcontinent. Our results have important implications for understanding diurnal monsoon circulations and their associated precipitation.
AS40-A015
Improving Boreal Summer Precipitation Predictions from the Global NMME Through Res34-Unet
Xuan TONG+, Wen ZHOU#
Fudan University
Global warming and climate change have increased the frequency and intensity of floods and droughts, limiting economic development and threatening human survival. Therefore, accurate global forecasts well in advance of precipitation are essential to facilitate timely adaptation. Current seasonal forecasts are based mainly on numerical models, but raw forecasts suffer from systematic bias and under/overdispersion problems and cannot be directly used in applications. In addition, bias correction methods for global forecasts need to be further developed. Based on a fusion of ResNet34 and Unet, called Res34-Unet, deep learning post-processing is proposed to correct global precipitation forecasts of the North American Multi-Model Ensemble (NMME). Compared with raw global NMME predictions, post-processed precipitation predictions can be improved by up to 45%, which is significant at different latitudes. Feature importance analysis shows that precipitation itself, meridional wind, and sea surface temperature are key factors.
AS40-A014
East Asian Summer Monsoon Precipitation Controlled by the Upstream Westerly Wind
Jun-Hyeok SON1#+, Kyong-Hwan SEO2
1IBS Center for Climate Physics, 2Pusan National University
The seasonal evolution of the EASM rainband and associated stationary circulation pattern is influenced by the mechanical effect of the Tibetan Plateau, and seasonal changes in the westerly wind speeds impinging on the Tibetan Plateau are a key driver of this process. In this study, using interannual variability of the upstream zonal wind speed, the dynamical mechanism for the interannual variations of the EASM precipitation is revealed based on the topographically forced stationary Rossby wave theory. The dynamical mechanism regulating interannual variability in the EASM rainband is essentially the same mechanism that drives the seasonal evolution of the climatological EASM rainband. If the westerly winds impinging on the Tibetan Plateau are stronger (weaker) than average, then the EASM rainband shifts eastward (westward). Large variations in the upstream westerly wind during May induced considerable interannual variation in the zonal location of the rainband (up to a 20–30º shift). The westerly wind speed exhibited less variations in June and July, resulting in a smaller zonal shift of approximately 10º.
AS40-A013
Indian Ocean Dipole and ENSO’s Mechanistic Importance in Modulating the Seasonal Precipitation
Yue ZHANG#+, Wen ZHOU
Fudan University
Eastern China was extremely wet in summer 2020, which is found to be related to the potential delayed effects of the Indian Ocean Dipole (IOD). Additional knowledge is warranted to improve our understanding of detailed mechanisms of such an effect. In this study, we compared physical processes associated with delayed effects of the IOD and El Niño–Southern Oscillation (ENSO) on summer precipitation. Partial correlation and composite analysis reveal that ENSO modulates precipitation mainly over the Yangtze River Valley, whereas IOD benefits precipitation farther north. Both IOD and ENSO can stimulate anticyclonic circulation over the western North Pacific (WNP) in the ensuing summer but with different spatial distributions related to the different sea surface temperature (SST) evolution processes. IOD is similarly followed by warming signals in the Indian Ocean, known as the “capacitor” effect, but the location is closer to Australia than that associated with ENSO. IOD also stimulates significant SST cooling anomalies over the equatorial Pacific during the ensuing summer, jointly contributing to the anomalous anticyclone over WNP. Numerical experiments confirm that combined effects of the Indian Ocean “capacitor” and equatorial Pacific cooling can generate an anomalous anticyclone with wider distribution in the meridional direction over WNP.
Session Chair(s): Yonghwan KWON, Korea Institute of Atmospheric Prediction Systems, Haiqin CHEN, Nanjing University
AS47-A003
| Invited
Multiscale Assimilation of Radar and Aws Data for Typhoon Haikui's Extreme Landfalling Precipitation Forecast
Haiqin CHEN1#+, Kun ZHAO1, Tao SUN2
1Nanjing University, 2National Center for Atmospheric Research
The remnants of Typhoon Haikui together with the southwesterly monsoon caused a record-breaking extreme precipitation event in the Pearl River Delta, leading to four fatalities and dozens of injuries. In recent years, continuous efforts have been made to develop state-of-the-art modeling frameworks and deploy ground-based instruments, especially high-density automatic weather stations (AWS) and radar data, to improve the prediction of landfalling tropical cyclones (TCs).Our study involved assimilating radar data and AWS surface data using a multiscale hybrid ensemble-variational (EnVar) assimilation approach. First, we employed a multistep strategy to assimilate AWS surface data and radar data in different steps. Then, to better represent multiscale uncertainties in the background error covariance (BEC), we explored how to introduce multiscale ensemble BEC in the hybrid EnVar method. Two strategies are designed for generating multiscale ensemble BEC, using multi-resolution ensemble BEC or filtering ensemble BEC into different scales at different assimilation steps of AWS surface data and radar data. Compared to using the same ensemble BEC in all steps, both strategies properly obtained increments at different scales from AWS and radar data, and thus improved forecast skills of heavy rainfall. Filtering ensemble BEC into different scales in different steps demonstrated better performance, with the highest forecast skills of accumulated precipitation and lowest forecast errors of surface variables. Further diagnosis revealed that the improvement of precipitation forecast skill was attributable to the stronger cold pools and gust winds near the surface as well as deeper saturated water vapor layers within the convections. More details will be shown at the conference.
AS47-A005
Scale-dependent Inflation for a Multi-scale Radar Ensemble Data Assimilation System and Its Impact on Short-range Heavy Rainfall Prediction in Taiwan
Lawrence Jing-Yueh LIU1,2#+, Shu-Chih YANG2, Zhe-Hui LIN2
1University of Illinois Urbana-Champaign, 2National Central University
In ensemble data assimilation (EDA), error covariance localization is a necessary strategy to mitigate the sampling error and rank deficiency problems due to the use of a finite ensemble size. For radar EDA, the localization length is chosen as a ten-kilometer scale for all variables to represent the convective-scale signals and prevent spurious correlations at long distances. However, given the multiscale characteristics of heavy rainfall events, a multi-scale radar ensemble data assimilation system is expected to be beneficial in improving heavy rainfall prediction. In this study, a multiscale radar EDA system is established by adopting the successive covariance localization method (SCL) in the Weather Research and Forecasting model Local Ensemble Transform Kalman Filter radar assimilation system (WLRAS-SCL). Assimilating the radial velocity with WLRAS-SCL shows a great impact on predicting a heavy rainfall event on 8 September 2018. Despite its success in short-term precipitation prediction, the SCL technique faces challenges of slightly underestimating the intensity of the small-scale convection, leading to weakened local convection strength within the convection system. Therefore, a Scale-Dependent Inflation method (SDI) is proposed under the WLRAS-SCL framework. This method utilizes the wavelet transformation to separate ensemble perturbations into different scales. Distinct inflation parameters are then assigned to each band of scale. Large weightings are designated for smaller scales and gradually decrease as the scale increases. The primary objective is to mitigate the underestimated local convection strength observed at a smaller scale with the use of SCL. Preliminary results suggested that the SDI method successfully increases the spread at smaller scales, resulting in stronger convections that better agree with observation data. More details about optimizing the use of SDI in multiscale radar data assimilation and its impact on convection development will be provided in the presentation.
AS47-A016
The Mean Diameter Update Approach for Dual-polarimetric Radar Data Assimilation Based on Ensemble Kalman Filter
Bing-Xue ZHUANG1#+, Kaoshen CHUNG2, Wei-Yu CHANG2, Chih-Chien TSAI3
1McGill University, 2National Central University, 3National Science and Technology Center for Disaster Reduction
The mean diameter update (MDU) approach aims to involve the direct relationship between the differential reflectivity (ZDR) and the mean diameter of raindrops in the ensemble-based data assimilation procedure. This approach updates mass-weighted mean diameter (Dm) explicitly to make use of the robust correlation between simulated ZDR and Dm. A series of experiments are conducted to evaluate the impacts on analyses and forecasts and the feasibility with different microphysics parameterization schemes. The results illustrate that the MDU approach can decrease ZDR analysis errors more efficiently, consistent with the further reduction of Dm. Besides, the performance of the quantitative precipitation forecast (QPF) is further improved with the implementation of the MDU approach. In conclusion, the MDU approach involves the feature of ZDR in the ensemble-based data assimilation and enhances the accuracy of analyses and forecasts.
AS47-A001
Observability and Effective Region with Application to Data Assimilation
Wei KANG1#+, Liang XU2
1Naval Postgraduate School, 2Naval Research Laboratory
In this work, we introduce a new definition of observability based on dynamic optimization. The theory is developed with a specific application in mind: limited-area data assimilation. For systems defined by partial differential equations (PDEs), the new definition enables the analysis of observability in a limited area with a significantly reduced computational load. Specifically, the definition of observability leads to a new concept, the so-called effective region. To compute the observability of a given state variable, we show that the computation can be limited to an effective region that is much smaller than the region in which the PDE is defined, resulting matrices involved in the computation substantially smaller than the state space dimension. These concepts are applied to develop a learning-based surrogate data assimilation model in a limited area. Our model employs deep learning techniques, where a neural network is trained using sensor data as inputs and providing the estimated values of the system's states as outputs. Our approach offers numerous benefits. Firstly, computationally intensive tasks, such as generating data and training the neural network, are all performed offline during the design phase of the surrogate data assimilation model. This leads to a significant reduction in online computational burden as the evaluation of the neural network does not require propagating the dynamic model. This is fundamentally different from conventional data assimilation algorithms, such as EnKF or 4D-Var, that require propagating the dynamic model multiple times in every estimation cycle. Secondly, we show that the surrogate data assimilation model is insensitivity to boundary conditions. When generating data for neural network training, the PDE is solved within the effective region without the need to provide accurate boundary conditions around it. This eliminates the requirement for precise lateral conditions, as commonly needed in limited-area models in numerical weather prediction.
AS47-A022
Multivariate Approaches on Deep Learning Based Recovery for Cloudy Cells of Satellite AOD Retrievals
Hae Soo JUNG+, Ji Won YOON, Seon Ki PARK#
Ewha Womans University
Satellite-derived Aerosol Optical Depth (AOD) is valuable for its expansive coverage, particularly exemplified by the Geostationary Environment Monitoring Spectrometer (GEMS) on GK-2B, which excels in providing high-quality aerosol data, especially on well-lit surfaces in the ultraviolet region. However, a notable challenge lies in AOD retrieval in cloudy regions, inherent to satellite-derived AOD. This study explores the potential of deep learning techniques, renowned for adaptability, to address the challenges posed by missing data in satellite-based AOD. While many studies employ multivariate approaches to address missing information, a comprehensive analysis of their impact is lacking. Consequently, this research investigates the influence of multivariate models on satellite-based AOD imputation, comparing them with univariate models. Both models are trained and evaluated on datasets with varying extents of missing information, considering numerical performance assessed by Root Mean Squared Error (RMSE) and visual clarity measured by Structural Similarity Index (SSIM). Sensitivity to the size of missing data is more pronounced in the multivariate model, emphasizing its heightened dependence on training data. In summary, this study highlights the strengths and weaknesses of univariate and multivariate models in filling missing values in satellite-derived AOD. It underscores the significant impact of data distribution during multivariate model training compared to using univariate models, offering valuable insights for researchers addressing missing values in satellite-derived AOD.
AS47-A008
| Invited
Assessing the Impact of Assimilating Both Radar- and Radiometer-based Soil Moisture Retrievals on the Performance of Numerical Weather Prediction Systems
Yonghwan KWON1#+, Sanghee JUN1, Kyung-Hee SEOL1, In-Hyuk KWON1, Eunkyu KIM1, Jeon-Ho KANG1, Hyunglok KIM2
1Korea Institute of Atmospheric Prediction Systems, 2Gwangju Institute of Science and Technology
Accurate estimation of surface soil moisture (SSM) initial conditions have been shown to improve numerical weather prediction skill. Consequently, many operational weather centers employ SSM data assimilation (DA) that integrates satellite-based SSM retrievals into land surface models (LSMs) to generate observation-informed global estimates of SSM. Our recent studies implement the assimilation of SSM data derived from the Advanced SCATterometer (ASCAT) and Soil Moisture Active Passive (SMAP) within a coupled land-atmosphere DA system that is composed of the Korean Integrated Model (KIM) and NASA Land Information System (LIS), and demonstrate the beneficial impact of each SM product on the KIM weather forecasts. In the current study, assimilation of the Soil Moisture and Ocean Salinity (SMOS) SM retrievals is additionally implemented within the KIM-LIS coupled system. The current study aims to evaluate the relative (individual) and combined performance of C-band radar-based (i.e., ASCAT) and L-band radiometer-based (i.e., SMAP and SMOS) SSM products in improving the global SM analysis and atmospheric analysis/forecast. The SSM retrievals from the three microwave satellite systems are separately and simultaneously assimilated into the Noah LSM using an ensemble Kalman filter scheme within the KIM-LIS coupled system. To correct systematic biases between the satellite-based SM retrievals and modeled SM, the cumulative distribution function (CDF) matching method is applied for ASCAT SM data while the anomaly correction method is used for SMAP and SMOS. The global SM analysis obtained from the SM DA is assessed using triple collocation analysis (TCA). Moreover, the atmospheric analysis and forecast of KIM are evaluated by comparing the experimental results against the European Center for Medium-Range Weather Forecasts (ECMWF) Integrated Forecasting System (IFS) analysis and observations from the surface synoptic weather station network (SYNOP).
Session Chair(s): Ramesh KRIPALANI, Retired Senior Scientist, Indian Institute of Tropical Meteorology
AS17-A002
Tornado Intensity, Size, and Vertical Wind Speed Dependence, Radar-based Climatologies, and Near-tornado Thermodynamics
Joshua WURMAN1#+, Karen KOSIBA2
1FARM Univ of Alabama, 2University of Illinois
Our knowledge of tornadogenesis, evolution, and structure has advanced substantially, but many questions/hypotheses remain observationally unconfirmed/untested. These include the size and intensity distribution of tornadoes, the variability wind speeds with height and time, the thermodynamic properties of the air immediately surrounding and being ingested into tornadoes, and how tornado intensity, propagation speed and structure, including variations in wind with height and time, affect human-impacting damage. DOW observations demonstrate that supercell-spawned tornadoes have a characteristic intensity, with peak ground-relative wind speeds above 60 m/s, and a characteristic diameter, near 300 m. These are in stark contrast to damage-based tornado intensity and size statistics. Damage-based intensity estimates were shown to be an average of 2 EF categories low compared to DOW-determined intensities, with extreme cases 4 EF categories different. DOW climatological analysis is being extended to incorporate many more tornadoes, to generalize these results, reduce statistical error, and permit additional tornado metrics to be quantified. DOW observations also reveal that, in contrast to other windstorms, the most intense winds in tornadoes occur very near the surface, perhaps below 10 m AGL. Preliminary observations suggest that there is a distinct and localized change in the near-field thermodynamics during tornado evolution over short time and spatial scales, which suggest changes in storm processes. Preliminary results from the 2024 BEST (Boundary-layer Evolution and Structure of Tornadoes) project, focusing on the thermodynamic and kinematic structure of tornadoes <50-100 m AGL, using proximate DOW radars, PODNet, and Driftersondes will be presented.
AS17-A003
| Invited
Enhancing Conventional Weather Radar Observations of Localized Heavy Precipitations Using AI and a Phased-array Radar
Philippe BARON1#+, Katsuhiro NAKAGAWA1, Shinsuke SATOH1, Tomoo USHIO2, Seiji KAWAMURA1
1National Institute of Information and Communications Technology, 2Osaka University
Localized heavy precipitations (LHP) occur suddenly in summertime and are becoming more frequent in Japan. Understanding and making short-term predictions of them require 4D observations with high spatiotemporal resolutions, typically of few hundred meters and less than 1 minute. The eXtended RAdar Information Network (XRAIN), operated by the Ministry of Land, Infrastructure, Transport and Tourism’s (MLIT), covers most of urban regions in Japan and has been operational for more than 10 years. Therefore, it provides a unique dataset for studying and predicting LHP, as well as assessing their long-term trends. However, XRAIN needs 5 minutes to measure the full 3D storms with a limited number of elevations (~12). This is insufficient to properly capture the 4D rain features when the storms are generated. In this study, we investigate the interpolation of XRAIN data into high-resolution (HR) data using AI and a new Multi-Parameter Phased Array Weather Radar (MP-PAWR) that has been tested in Saitama prefecture (Japan) since 2018. The MP-PAWR is capable of measuring the full 3D rain field surrounding the instrument every 30 seconds with more than 100 elevations. Given a XRAIN sequence of observations, the AI interpolation model produces HR 4D-features with 1 minute and 40 levels up to a height of 10 km. Those HR features are learnt from past MP-PAWR observations. The model, a supervised neural network, is based on an encoder/decoder architecture with Long-Short Term Memory units, in which scalar operations have been replaced by 3D spatial convolutions. We will present the model and its training. Its ability to properly produce HR features that were not measured by XRAIN will be discussed.
AS17-A001
Role of Convective and Circulation Features on Multi-scales in Modulating Tracks of Tropical Cyclones Formed Over the Bay of Bengal
Mohan Murali Krishna GORJA1+, Naresh Krishna VISSA1#, Yesubabu VISWANADHAPALLI2
1National Institute of Technology, Rourkela, 2National Atmospheric Research Laboratory
Large-scale background environment, which can regulate Tropical cyclones (TCs) movement, is modulated by the atmospheric anomalies prevailing on quasi-biweekly (10-20 days;QBWO), intra-seasonal (20-90 days;ISO) and inter-annual (≥91 days) scales. In this regard, many studies noticed the influence of multi-scale atmospheric variability on TCs formation over the North Indian Ocean, including the Arabian Sea and the Bay of Bengal (BoB). However, their influence on the TCs movement needs to be better understood. The current study presents the role of atmospheric variations that prevailed on the various scales, as mentioned above, in determining the movement of TCs formed over the BoB region. Based on the IMD TCs best-track data available from 1982-2020 and global ERA5 reanalysis dataset consisting of single- and multi-level variables, composites of various diagnostic parameters related to the convection and circulation are examined. The identified features from the composite analysis indicated that the atmospheric anomalies on QBWO and ISO scales, in combination with mean climatology, predominantly determine tracks of TCs formed during the pre-monsoon season (March-April-May). In contrast, the mean climatology mean environment (CLM) seems responsible for the observed TCs tracks during the post-monsoon season (October-November-December). More importantly, TCs track-wise diagnosis reveals that QBWO and ISO-induced anomalies jointly provide a guiding effect for TCs moving in northward, north-eastward, and north-westward directions and TCs taking re-curvature. Meanwhile, CLM mainly drives the westward-moving TCs. However, examined anomalies on the inter-annual scale do not exhibit any significant physical linkages with the TCs movement. Further, a case study analysis by performing set of experiments using the Weather Research and Forecasting (WRF-ARW) model initialized with unfiltered and scale-filtered fields also substantiates our previous findings. The findings may provide insights into an improved understanding of TCs movement over the BoB region and help in undergoing research on TCs track prediction at sub-seasonal scales.
AS17-A007
An Algorithm for Tornado Detection Based on Radar Data
Shangdan HUANG1#+, Qiangyu ZENG1, Hao WANG1, Lanqiang BAI2, Jianxin HE1
1Chengdu University of Information Technology, 2Guangdong Meteorological Service
龙卷风是罕见的小规模天气事件,直径从几十米到几公里不等。多普勒天气雷达通常难以探测龙卷风,包括速度模糊、距离折叠和分辨率不足。结合雷达基站数据和双极化参数,提出了用于龙卷风识别和预警的XGBoost算法。该算法根据速度、反射率、光谱宽度、差分反射率和相关系数等特征将雷达数据划分为多个块。该模型的训练、优化和测试表明,龙卷风预警时间可以提前18分钟,提供基于龙卷风生成和发展过程的分类概率。相关的概率值可以帮助预报员做出决策。
AS17-A008
Evaluation of Unprecedented Rain Events Using Equatorially/globally Conditioned Meteorological Analysis Approach
Ashwini RANADE#+
National Institute of Hydrology, Roorkee
Hydro-meteorological extremes are of serious concern globally due to their unusual and unprecedented occurrences in recent global warming period. A new analytical technique, ‘Equatorially/Globally conditioned meteorological analysis (EC/GCMA)’ developed to study the evolution of monsoon and comprehend changes in global atmospheric thermal and circulation during extreme rain events. We understand that monsoon circulation evolves in association with spreading and intensification of equatorial atmospheric thermal condition (warmest-thickest troposphere and lowest pressure), vertical circulation structure (lower tropospheric confluence/convergence and upper tropospheric difluence/divergence), and highest precipitable water. The technique comprises equatorially, globally, and self-conditioned customized thematic global weather charts of mslp (EC-mslp), precipitation water (EC-ppw), level-wise (1000–100 hPa) atmospheric temperature (EC-Tlevel), geopotential height (EC-Zlevel), wind (GC-Wlevel) and as well few numerical values. By combining the equatorially conditioned parameters, the technique classifies the weather systems into four types of global weather regimes (GWRs). Levelwise distribution of the GWRs, streamlines and GC-Wlevel for full depth of the atmosphere provide adequate insight into the 3D structure of the monsoon circulation, area under monsoon condition, seasonal rains and extreme rain events. Few case studies of extremes using EC/GCMA approach provide valuable insight about the phenomenon. Greater warming over east of eastern Tibet and lesser westward produced ‘persistently moderately intense Asia-Pacific monsoon circulation over Indian subcontinent and persistence intense warm-low lower tropospheric convergence-confluence stretched vertically up to 400hPa caused subregional extreme wet spell during July 23–28, 2005 over Mumbai. Combined five factors: cool-low-dry and warm-low-moist regime contrast; squeezing of three different types of flows (deep warm-moist, cool-dry and warm-dry); orographic lifting of moist airs; and pumping of accumulated moist air and intense suction of airs produced unprecedented rains over the Kedarnath range during 16-17 June 2013. We believe this novel approach can replace the conventional routine meteorological charts of atmospheric data.
AS17-A015
Investigations on the Changes in Atmospheric Mean Kinetic Energy During the Life Cycle of a Cyclone
Nishi SRIVASTAVA#+
Birla Institute of Technology
Atmospheric energetics deals with changes in various energy components and how they affect the atmospheric system. The thermal structure of atmosphere gets modified by transfer and redistribution of energy, which generates available potential energy(APE). This APE further transforms into kinetic energy to drive weather and climate, and atmospheric dynamics and play essential roles in Earth's atmospheric system. The mechanical energy components, conversions among them, and generations/dissipations constitute the atmospheric energy cycle, was defined by Lorenz and named the Lorenz energy cycle. In this work, we have evaluated the changes in Mean Kinetic Energy (MKE), one of the essential components of the Lorentz Energy Cycle, owing to a cyclonic activity with a focus over the Indian domain. There is transport of energies between ocean and the atmosphere through various processes. It is essential to quantify the changes that occurred in atmospheric energy in response to oceanic activity. Indian ocean region observes a significant number of depression/ deep depression/ cyclonic and severe cyclonic activities. In the present work, we studied the generation and redistribution of MKE owing to a severe cyclone in the Bay of Bengal region, India, during May 23, named Mocha, formed on 9May23 and dissipated by 15May23. Along with MKE we also investigated variation of omega and relative humidity. In the vertical variation of MKE, we observed high MKE between 200-100 hPa levels before the start and end of the cyclone, but this distribution was disturbed with the development of cyclone and MKE peak shifted in the lower atmosphere during cyclonic activity. MKE values ranged in between 1-1.5 ×105 J m-2. Negative values of omega represent strong upward motions and vertical distribution of omega showed a high negative value corresponding to cyclonic region (~-0.2 Pascal/s) and varied along the path of the cyclone.
AS17-A016
Optimization of Typhoon Track Prediction Based on Ensemble Simulations of HWRF
Chi Jui YANG#+, Chia-Jeng CHEN
National Chung Hsing University
Typhoons pose a significant threat to East and Southeast Asian countries, necessitating the continuous refinement of prediction models. This study delves into the enhancement of typhoon track prediction in the Northwestern Pacific Basin through the application of the Hurricane Weather Research and Forecasting (HWRF) model, version 4.0. To achieve the optimization of typhoon track prediction, diverse ensembles of parameterization schemes within the HWRF framework are leveraged. Various statistical and machine learning techniques are integrated into the generation and selection of diverse ensembles. A systematic approach is adopted to evaluate and compare the performance of different simulation ensembles. Crucial meteorological variables (e.g., atmospheric pressure, wind speed, and sea surface temperature) that show influence over a typhoon’s trajectory are examined, and the most influential components will be identified. Statistical metrics such as typhoon path expect value or Mean Absolute Error of forecasting and Verification Radius are used to assess the accuracy and reliability of the optimized typhoon track prediction.
Session Chair(s): Baek-Min KIM, Pukyong National University
AS45-A013
| Invited
Attribution of Cold-season Arctic Amplification
Eui-Seok CHUNG1#+, Seong-Joong KIM1,2, Kyung-Ja HA3, Sun-Seon LEE4
1Korea Polar Research Institute, 2University of Science and Technology, 3Pusan National University, 4IBS Center for Climate Physics
Both observations and model simulations indicate that the warming response to greenhouse gas forcing is greatest in the Arctic. This phenomenon, commonly referred to as Arctic amplification, is most pronounced in fall and winter, when the sea-ice albedo feedback is not active due to a lack of insolation, which has led numerous studies to emphasize the role of longwave feedback processes and/or poleward energy transport. However, the mechanisms responsible for the seasonal evolution of Arctic amplification remain elusive. In this study, we present modeling evidence that the seasonal evolution of Arctic amplification cannot be linked to a single mechanism. In particular, it is found that cold-season longwave feedback processes are not independent of the sea-ice loss during summer because sea-ice loss-related ocean-to-atmosphere heat fluxes contribute to a surface-intensified warming and moistening in fall and winter. This suggests that Arctic Ocean-mediated seasonal energy transfer links the warm and cold season feedbacks with each other, thereby explaining the seasonal evolution of Arctic amplification, and its peak in the cold season.
AS45-A003
Multi-layered Interactions Underlying Arctic Amplification and Its Impact
Yongkun XIE1#+, Jianping HUANG1, Guoxiong WU2, Yimin LIU2
1Lanzhou University, 2Chinese Academy of Sciences
This presentation will discuss the multi-layered interactions between the atmosphere, ocean, and sea ice to explore the mechanics of Arctic amplification and its effects on mid-latitudes. The main aspects encompass the factors contributing to Arctic amplification from an energy budget perspective, the two-way connections between the Arctic and mid-latitude regions based on a dynamic and thermodynamic coupling perspective, and the general mechanisms by which the Arctic or oceans influence distant land areas from a potential vorticity perspective.
AS45-A018
Internal Variability Amps Up Arctic Amplification
Aodhan SWEENEY1#, Qiang FU1, Stephen PO-CHEDLEY2, Hailong WANG3, Muyin WANG1,4+
1University of Washington, 2Lawrence Livermore National Laboratory, 3Pacific Northwest National Laboratory, 4NOAA Pacific Marine Environmental Laboratory
Since 1980, the Arctic surface has warmed four times faster than the global mean. Enhanced Arctic warming relative to the global average warming is referred to as Arctic Amplification (AA). While AA is a robust feature in climate change simulations, models rarely reproduce the observed magnitude of AA, leading to concerns that models may not accurately capture the response of the Arctic to greenhouse gas emissions. Here, we use CMIP6 data to train a machine learning algorithm to quantify the influence of internal variability in surface air temperature trends over both the Arctic and global domain. Application of this machine learning algorithm to observations reveals that internal variability increases the Arctic warming but slows global warming in recent decades, inflating AA since 1980 by 38% relative to the externally forced AA. Accounting for the role of internal variability reconciles the discrepancy between model simulated and observed AA.
AS45-A008
What Determine the Seasonality of Arctic Amplification
Haijin DAI#+, Jinfeng DING
National University of Defense Technology
In recent decades, Arctic surface temperature increases much faster than that in other regions, which is so called Arctic amplification (AA). A robust feature for AA is that AA reaches its maximum (minimum) in autumn-winter (summer), while it reaches its secondary peak in spring. Based on our previous studies (Dai, 2021, GRL; Dai et al., 2022, JGRA; Dai, 2023, GRL), most of the additional solar radiation induced by sea-ice loss is stored as seasonal heat storage (SHS) in subsurface ocean, which leads to AA minimum in summer. In autumn-winter, SHS is released due to colder surface air and warmer sea surface, which leads to AA maximum without additional solar radiation. In spring, enhanced atmospheric blocking events induce anticyclonic wind anomaly, which allows more warm (cold) air is transported to high (mid) latitude from mid (high) latitude and leads to secondary peak of AA.
AS45-A019
Wintertime Surface Air Temperature Relationship Between the Arctic and Eurasia in the Late Holocene Transient Climate Simulation
Sang-Yoon JUN1#+, Jung CHOI2, Taewook PARK1, Eui-Seok CHUNG1, Seong-Joong KIM1,3
1Korea Polar Research Institute, 2Seoul National University, 3University of Science and Technology
We analyze a wintertime surface air temperature (SAT) relationship between the Arctic and Eurasia in the past 6,000 years using transient climate simulation obtained by the CESM1 model. In this experiment, a long-term trend of SAT resulting from the change of Earth’s orbit from the mid-Holocene to the present is well reproduced. As in the present climate, the SAT dipole pattern over the Arctic–Eurasia region, referred to as the warm Arctic–cold Eurasia, is found as the substantial interannual variability in winter. Here we examine non-stationary SAT relationships between three Arctic regions (Barents–Kara Seas, Sea of Okhotsk, and Scandinavia) and each closely linked Eurasian area by calculating 35-year moving correlation coefficients. Although there is inter-decadal fluctuation, SAT variability in the Sea of Okhotsk is always negatively correlated with Eurasia over the past 6,000 years. In contrast, the negative SAT relationships between the other two Arctic regions and Eurasia sometimes become too weak, or sometimes even positive correlations appear. The results suggest that the large inter-decadal fluctuation of the SAT co-variability over the Arctic–Eurasia region is likely associated with the sea surface temperature change over the North Atlantic and North Pacific.
AS45-A022
Arctic Ocean Amplification in a Warming Climate
Qi SHU#+
Ministry of Natural Resources
Arctic near-surface air temperature warms much faster than the global average, a phenomenon known as Arctic Amplification. The change of the underlying Arctic Ocean could influence climate through its interaction with sea ice, atmosphere and the global ocean, but it is less well understood. Here we show that the upper 2000 m of the Arctic Ocean warms at 2.3 times the global mean rate within this depth range averaged over the twenty-first century in the CMIP6 SSP585 scenario. We call this phenomenon the ‘Arctic Ocean Amplification’. The amplified Arctic Ocean warming can be attributed to a substantial increase in poleward ocean heat transport, which will continue outweighing sea surface heat loss in the future. Arctic Amplification of both the atmosphere and ocean indicates that the Arctic as a whole is one of the Earth’s regions most susceptible to climate change.
AS02-A004
Non-linear Formation of Nitrogen-containing Organic Aerosol from Multi-BVOC Mixtures
Yanchen LI+, Jianhuai YE#
Southern University of Science and Technology, China
At a global scale, biogenic volatile organic compounds (BVOCs) comprise a major fraction of total non-methane VOCs, significant impacting ecosystem functioning and climate change. Literature has consistently demonstrated that the presence of anthropogenic pollutants, such as NOx, can perturb the formation of biogenic secondary organic aerosol (BSOA). During nighttime, BVOCs primarily undergo oxidation by O3 and NO3. The latter pathway leads to the formation of nitrogen-containing organic aerosol (NOA), which plays a vital role in air quality and human health. Current research mainly focuses on NOA formation from individual BVOC precursor. However, in the real atmosphere, multi-reactant oxidation process occurs simultaneously, leading to complex interactions and non-linear effects on NOA formation. The underlying mechanisms of the non-linear formation of NOA from BVOC mixtures remain largely unexplored. This study aims to investigate the formation of NOA resulting from the oxidation of monoterpenes (e.g., limonene) and sesquiterpenes (e.g., longifolene), and elucidate the non-linear formation mechanism, properties, and characteristics of NOA in the multi-precursor system. Three key aspects will be examined: (1) the yields and physicochemical characteristics (e.g., functional groups, volatility, light-absorbing properties) of NOA produced from both individual BVOC system and BVOC mixtures; (2) the interactions between oxidation products and intermediates derived from the oxidation of various BVOCs; (3) the non-linear formation mechanisms of NOA in the presence of BVOC mixtures. This study will provide a comprehensive understanding of NOA formation in the multi-precursor system and their implications for atmospheric chemistry.
AS02-A009
Effects of High-temperature Drought Combined Extreme Weather on Vegetation Feedback and Ozone
Yuting LU#+, Mengmeng LI
Nanjing University, China
Extreme weather becomes more frequent with global warming. The combined extreme weather of high temperature and drought has an impact on air quality and human health, etc. The vegetation-atmosphere feedback during the combined heat wave and drought is also an important natural process affecting the generation of O3. Understanding the trend of heat-drought combined extreme weather and its impact on ozone and BVOC can help mitigate its negative impacts on the environment and human health. Using ERA5 data and major heat wave and drought indicators, the trend of heat wave and heat-drought combined extreme weather in summer in China during 1960-2022 was analyzed. The effects of temperature and soil moisture on isoprene emissions were investigated using Station for Observing Regional Processes of the Earth System (SORPES) observation data. Since the 1960s, the average number of heat wave days, frequency, cumulative intensity and the max duration of heat wave and heat-drought combined extreme weather have been on the rise. The cumulative intensity of heat-drought combined extreme weather is about 1℃ higher than that of heat wave per year. Isoprene emissions increased with increasing temperature, but the relationship between isoprene emissions and soil moisture was complicated. Isoprene emissions increase during mild and moderate droughts; During severe droughts, isoprene emissions decrease. Under the influence of high-temperature drought combined weather, isoprene emissions may increase, which will exacerbate ozone pollution.
AS02-A013
Assessment of the Impact of the Biogenic Emissions Model Using Different Plant Functional Types on Air Quality Modeling in Taiwan
Yi-Ju LEE#+, Fang-Yi CHENG
National Central University, Taiwan
Not only anthropogenic emissions but also biogenic VOC emissions contribute to the concentration of ambient air pollutants. According to the latest “National Forest Resource Survey” from the Forestry and Nature Conservation Agency, Ministry of Agriculture of Taiwan, the total forest area of Taiwan is 2,197,090 hectares, with a forest coverage rate of approximately 60.71%. Therefore, biogenic VOC emissions might play an essential role in air pollutant production in Taiwan. The Model of Emissions of Gases and Aerosols from Nature (MEGAN) provides biogenic emissions by considering the plant functional type (PFT), leaf area index (LAI), and meteorological condition. Since the initial PFT data was from a relatively distant year with a different spatial distribution compared with the observation, this study utilized the land use index to reproduce the PFT dataset and investigated its impact on air quality modeling. WRF version 3.8.1 and CMAQ version 5.2 were conducted to simulate the meteorological field and concentration of air pollutants, respectively, from September 27 to October 10, 2021. The discussion focused on October 5 and 6, when the mountain blocked the synoptic easterly wind, causing the weak wind and severe air pollution in western Taiwan. The simulation with updated PFT data shows lower and higher VOC concentrations (about 20-30 ppbC) compared with the original simulation in western Taiwan's plain region and the central mountain area, respectively. The update of the PFT data is able to improve the overestimation of daytime ozone concentrations in mountainous areas.
AS04-A020
Changes in Land-atmosphere Coupling Increase Compound Drought and Heatwaves Over Northern East Asia
Ye-Won SEO1#+, Kyung-Ja HA2
1IBS Center for Climate Physics, Korea, South, 2Pusan National University, Korea, South
Compound drought and heatwaves (DHW) events have much attention due to their notable impacts on socio-ecological systems. However, studies on the mechanisms of DHW related to land-atmosphere interaction are not still fully understood in regional aspects. Here, we investigate drastic increases in DHW from 1980 to 2019 over northern East Asia, one of the strong land-atmosphere interaction regions. Heatwaves occurring in severely dry conditions have increased after the late 1990s, suggesting that the heatwaves in northern East Asia are highly likely to be compound heatwaves closely related to drought. Moreover, the soil moisture–temperature coupling strength increased in regions with strong increases in DHW through phase transitions of both temperature and heat anomalies that determine the coupling strength. As the soil moisture decreases, the probability density of low evapotranspiration increases through evaporative heat absorption. This leads to increase evaporative stress and eventually amplify DHW since the late 1990s. In particular, seasonal changes in soil moisture and evapotranspiration between spring and summer contributed to the amplification of DHW by enhancing land-atmosphere interaction.
AS04-A037
Long Term Change of Interannual Variation in East Asian Summer Precipitation Since 1999
Jiwon JEONG#+, Jinho YOON
Gwangju Institute of Science and Technology, Korea, South
This study analyzed the long-term change in the interannual variation of the East Asian summer (July-August) precipitation pattern represented by the Meiyu-Baiu-Changma. The July and August GPCP monthly precipitation data from 1979-2022 were divided into six clusters by using Self-Organizing Map (SOM). Two features were noteworthy: First, the temporal distribution of the clusters showed a shift between clusters, indicating a decadal change in precipitation patterns over time. The influence of the Okhotsk Sea air mass and tropical monsoon air mass in the former period, and the North Pacific air mass in the latter period, on the formation of the East Asian summer precipitation pattern was evident. In the latter period, the westward extension and intensification of the WNPSH breaks down the original triple precipitation pattern and affects precipitation in Northeast Asia.
AS04-A044
Trends and Spatio-temporal Variability of Summer Mean and Extreme Precipitation Across South Korea for 1973–2022
Hye-Ryeom KIM1+, Kyung-Ja HA1#, Junghee YUN2, Mincheol MOON3
1Pusan National University, Korea, South, 2Yonsei University, Korea, South, 3Pohang University of Science and Technology, Korea, South
Climate change significantly affects the frequency, intensity, and timing of both mean and extreme precipitation. Extreme precipitation has caused tremendous socio-economic losses and severe impacts on human life, livelihoods, and ecosystems. In South Korea, heavy rainfall events during the boreal summer (June-to-August) have become more frequent and sporadic in recent years. Given the severity of these events, there is an urgent need for investigation into summer extreme rainfall. While previous studies have addressed daily extreme precipitation, there is still a gap in understanding hourly extreme rainfall. Therefore, this study aims to fill that gap by examining trends, spatio-temporal variability, and long-term variations in mean and extreme precipitation over South Korea during the boreal summertime. We utilized daily and hourly observational data and employed various analysis methods. Over the past 50 years (1973–2022), there has been a noticeable increase in maximum hourly precipitation, even though the boreal summer mean precipitation has seen only marginal growth. Regionally, an increase in mean and extreme rainfall occurred in the northern part of the central region and the southern coast of the Korean peninsula. Furthermore, the rise in the intensity and frequency of extreme precipitation, along with an increase in dry days, has contributed significantly to the total summer precipitation in recent years. Our findings provide scientific insights into the progression of extreme summer precipitation events in South Korea.
AS04-A047
Divergent Dynamics and Characteristics of Extreme Precipitation Over Asia
Haeun JEON1, Ji-Hye YEO1+, Hye-Ryeom KIM1, Hyoeun OH2, Kyung-Ja HA1#
1Pusan National University, Korea, South, 2IBS Center for Climate Physcis, Korea, South
Recently, extreme precipitation events in the Asian region have been anticipated to occur more frequently and intensely in the future due to the increase in greenhouse gas concentrations. However, extreme precipitation exhibits different features depending on surface characteristics, and different dynamics. Because most studies on extreme precipitation in the Asian region have been centered around the broad monsoon region, understanding of dynamic-thermodynamic characteristics of extreme precipitation in specific areas is lacking. In this study, we identified specific regions in terms of extreme precipitation quantification to investigate the regional driving factors of extreme precipitation in the Asian monsoon region during the period from 1979 to 2022 (June, July, and August). Through the moisture budget equation, we examined the dynamics, thermodynamic characteristics, and contributions of extreme precipitation. Based on frequency, quantity, and intensity of extreme precipitation, the EASM region was divided into the Yangtze River, Korean Peninsula, and Japan Southern regions, while the SASM region was divided into Indian Central-North, Himalayan Mountains, Bay of Bengal, Indian Northwest, and West Ghat regions. In the dynamic and thermodynamic analysis, extreme precipitation in all specific regions was found to be predominantly influenced by the dynamic convergence term (DY CON). However, unlike the South Asia region where extreme precipitation was mainly dominated by the DY CON, the East Asia region showed high contributions from the thermodynamic term and the convergence of the nonlinear term. Among them, the KP region had the highest contribution of 21% from the thermodynamic advection term, emphasizing regional differences in the characteristics of extreme precipitation. The results imply that understanding the precipitation characteristics of specific regions can contribute to the comprehension of extreme precipitation prediction.
AS04-A050
Role of Inter-basin Coupling Between the Tropical Indian and Pacific Ocean in Wildfire Over Indonesia
Hyeonho LEE+, Kyung-Ja HA#
Pusan National University, Korea, South
In previous studies, it has been demonstrated that the remote forcing associated with climate teleconnections, such as El Niño-Southern Oscillation (ENSO) and the Indian Ocean Dipole (IOD), have a significant impact on wildfires in Indonesia. However, there still exists considerable diversity in wildfire activity among El Niño events, especially with the highest values observed in the major season from August to October. To identify the role of inter-basin coupling, the accelerated termination of IOD and the dominant influence of Indian Basin Wide Mode (IOBM) during the El Niño winter, we categorized cases into four types (i.e., IOD-ENSO-IOBM, (IOD)-ENSO-IOBM, IOD-ENSO-(IOBM), (IOD)-ENSO-(IOBM). The results show that the first (third) type exhibits more vigorous carbon emissions compared to the second (fourth) type. We found a notable difference between the first (second) type, associated with the strong phase of IOBM, and the third (fourth) type, associated with the weak or negative phase of IOBM.
AS04-A053
The Spring to Summer Transition of the East Asian Monsoon and Climatological Intraseasonal Oscillations
Yun-Ting JHU1#+, Mong-Ming LU2
1International Integrated Systems, Inc., Taiwan, 2National Taiwan University, Taiwan
The East Asian monsoon system (EAM) shows strong annual cycle with the wet season in summer and dry in winter. Apart from the annual cycle, the monsoon system exhibits distinct climatological intraseasonal oscillations (CISOs) (Wang and Xu 1997), also known as the fast annual cycle (LinHo and Wang 2002). This study focuses on investigating the relationship between the CISOs, South China Sea (SCS) summer monsoon onset, and extreme rainfall events during the spring to summer transition period (March-June) in the monsoon region of 5°S-35°N, 60°E-150°E. The CISOs are identified based on the harmonic analysis of the OLR data in the 44-year period of 1979-2022. A significant CISO is identified over the SCS as an oscillation with the positive (dry) peak in early May and negative (wet) valley in late May. The timing of the valley point coincides with the dates of the commencement of the SCS summer monsoon. The spring to summer transition of the EAM is further analyzed using the ERA5 daily 850-hPa wind data. We found that the March-July daily wind maps can be classified to five types (weather type, WT). The WT occurrence frequency can well represent the sub-seasonal characteristics of the transition. The ENSO impacts on the EAM can be seen in the interannual variations of the WT frequency. The time windows with high occurrence probability of extreme rainfall events will be presented in the context of multiple-scale climate features such as the CISO, transient ISOs, WTs and ENSO. The implication for the S2S forecasts of the extreme events will be discussed.
AS04-A059
Understanding the East Asian Carbon Cycle Through the Relationship Between High Temperature Events and Vegetation Activity
Minseok SHIN#+, Sang-Wook YEH
Hanyang University, Korea, South
Given the increasing probability of extreme weather events due to climate change and the subsequent increase in the frequency of extreme temperature events, there is a need to understand the relationship between regional extreme temperature events, carbon dioxide concentrations, and vegetation growth in East Asia. In particular, given that East Asia is a region with a large increase in carbon dioxide and a rapid increase in temperature, it is important to understand their interrelationships in the future climate. In this study, we analyzed the effects of springtime anomalies on vegetation-related factors (e.g., GPP, LAI) and carbon dioxide concentrations in East Asia using the TRENDY model and observational data. This study aims to improve our understanding of the East Asian extreme high-temperature phenomenon and its relation to other climate factors, as well as its relationship to vegetation growth and carbon dioxide concentrations.
AS04-A070
Contributing Dynamic and Thermodynamic Factors Behind Unprecedented Summer Rainfalls in Korea During 2022
Hyoeun OH1+, Kyung-Ja HA2#, Jin-Young JEONG3
1IBS Center for Climate Physcis, Korea, South, 2Pusan National University, Korea, South, 3Korea Institute of Ocean Science & Technology, Korea, South
The year 2022 witnessed a range of climate extremes in South Korea, including floods and droughts. Among these, a particularly noteworthy events occurred on August 8, when extreme rainfall, exceeding 380mm/day, led to significant damage in Seoul. Throughout the year, six extreme rainfall events occurred, surpassing one standard deviation of interannual variation from 1982 to 2022. This study focuses on understanding the contributions of dynamic and thermodynamic components in the moisture budget during two persistent extreme rainfall events: June 27-30 and August 8-11. We revealed the distinct roles of winds and moisture contents in these two events. For the June 27-30 event, changes in winds accounted for over 80% of the rainfall, while for the extreme event during August 8-11, both the changes in wind and moisture content played significant roles. South Korea’s rainfall is known to be influenced by the variability of the western North Pacific subtropical high (WNPSH), which, in turn, is impacted by remote forcings including subtropical convections, Pakistan rainfall, and the North Atlantic Oscillation (NAO), through the atmospheric bridge. During June 27-30, two subtropical convections led to the westward expansion of the WNPSH. In contrast, positive NAO and intensified rainfall in Pakistan caused circulation changes that redistributed the thermodynamic characteristics. Owing to these changes, substantial meridional thermal gradients formed, causing zonally elongated rainfall. These findings provide insights into the factors driving extreme rainfall events in South Korea in 2022, highlighting the importance of remote forcings in understanding these events.
AS04-A087
Future Changes in East Asian Summer Monsoon Using CMIP6 Simulations Under 1.5°C, 2°C, and 3°C Global Warming Levels
MinAh SUN#+, Hyun Min SUNG, Jisun KIM, JaeHee LEE, Sungbo SHIM, Young-Hwa BYUN
National Institute of Meteorological Sciences, Korea, South
We examined the characteristics of the East Asian summer monsoon (EASM) in the present-day (PD) and investigated the changes in EASM corresponding to the projection at 1.5, 2.0, and 3.0 °C global warming levels (GWLs) using CMIP6 simulations. The migration of monsoon system is effectively captured by the 30 CMIP6 models, resulting in a pattern correlation coefficient of 0.91, representing improved results compared to previous studies. Separated into P1 (first primary peak; 33-41 pentad) and P2 (from P1 to the withdrawal; 42-50 pentad) during the monsoon period, the frequency and amount of weak to moderate precipitation rates are predominantly higher in P2, while the frequency and amount of moderate to extreme precipitation rates are notably higher in P1. The CMIP6 models project an increase in precipitation, approximately 5.7% °C−1, 4.0% °C−1, and 3.9% °C−1 for the three GWLs, respectively, accompanied by a longer duration due to earlier onset and delayed termination. Under the three GWLs, the projected precipitation frequency decreases below moderate precipitation rates, while it significantly increases above strong precipitation rates. Additionally, the precipitation tendencies in both P1 and P2 are similar to those of the total period, with significant changes being prominent at the 3.0 °C GWL. These precipitation changes are associated with an increase in extreme precipitation amount and influence the future changes in the EASM under a warmer climate.
AS04-A091
Characteristics of the East Asian Summer Monsoon on Extended Medium-range Time Scale Simulated by the Korean Integrated Model
Eun-Hye LEE#+, Eun-Hee LEE, Hye-Jin PARK
Korea Institute of Atmospheric Prediction Systems, Korea, South
Precipitation, a primary phenomenon in East Asia during summer, is mainly caused by the East Asian summer monsoon (EASM) system, which includes zonally elongated Meiyu-Baiu-Changma rain band, as well as extratropical cyclones and typhoons. Sub-seasonal variability of the EASM is closely associated with the large-scale circulation from the tropics to mid-latitude, including the moisture transport derived by the western North Pacific subtropical High (WNPSH) and the East Asian subtropical jet (EASJ). In order to improve the predictability of precipitation, current operational numerical weather prediction models struggle with forecasting from medium to extended medium-range time scales. Korean Integrated Model (KIM), which was developed by the Korean Institute of Atmospheric Prediction System, began operation in 2020 at the Korea Meteorological Administration. In this study, we conduct extended-range hindcast experiments of the KIM to compare with observation. We investigate spatial pattern and systematic errors of the seasonal mean in sub-seasonal simulation of the KIM. Also, we examine how the KIM simulates the EASM over lead time in the sub-seasonal prediction experiment. In other words, we will talk about the extent to which the KIM can reproduce the EASM by simulating the horizontal transport of moisture from the Indian Ocean and Western Pacific and westward extension of the WNSPH, and baroclinity related with the EASJ.
AS04-A094
Interannual Relationship Between Seasonal Mean and Intraseasonal Variability of Australian Summer Monsoon
Mako OKAZAKI#+, Yoshiyuki KAJIKAWA
Kobe University, Japan
It has well been known that the seasonal mean Australian summer monsoon (AUSM) tends to be strong (weak) in La Niña (El Niño) years. Meanwhile, AUSM is also characterized by large intraseasonal variability (ISV). In this study, we examined the interannual variability of AUSM and found the possible impact of the ISV. First, no significant interannual relationship between seasonal mean AUSM and seasonal mean ISV activity (amplitude) was found. However, we found the ISV phase in February effect on the seasonal mean. When the active (inactive) phase of ISV is dominated in February, the monthly mean AUSM in February tends to be largely strong (weak), and this eventually impacts the seasonal mean AUSM. Thus, it is suggested that the phase of ISV in February contributes to the seasonal mean AUSM. Second, we also found the difference in the seasonal evolution of AUSM and ISV activity in austral summer. Climatologically, the AUSM is established in early December and terminates in the middle of March. The ISV activity continues through April after the termination of AUSM in March. The different roles of ISV in each phase of AUSM will be also discussed for a better understanding of AUSM interannual variability.
AS05-A020
Seasonality of MJO Diversity
Seung-Yoon BACK1+, Daehyun KIM1, Seok-Woo SON1#, Daehyun KANG2
1Seoul National University, Korea, South, 2Korea Institute of Science and Technology, Korea, South
Individual Madden-Julian Oscillation (MJO) events have different propagation characteristics, which can be categorized into four types: standing, jumping, slow-, and fast-propagating MJOs. While the relationship between MJO types and El Niño/Southern Oscillation (ENSO)-like anomalous sea surface temperature (SST)/precipitable water (PW) patterns has been well documented in the literature, the role of climatological annual cycles of SST/PW on different MJO types has not been investigated. This study examines the seasonality in frequencies for each MJO type and its relationship with the annual cycle of background conditions. During the extended winter (November-April), fast MJO events are relatively frequent in March-April, while standing and slow MJO events are relatively frequent in November-February. To understand this seasonal difference in frequencies of MJO types, the moisture budget analysis is performed. The positive intraseasonal moisture tendency to the east of enhanced convection is zonally broader in March-April than in November-February. The zonally broader moisture tendency induced the larger zonal scale of the MJO in March-April, which can enhance the faster MJO propagation than in November-February. While the positive moisture tendencies in both seasons are mainly due to the meridional moisture advection, but the difference in tendency between the two seasons is mainly due to the zonal moisture advection. We found that the difference in zonal moisture advection between the two seasons is mainly due to the difference in seasonal moisture distributions. The PW background conditions in November-February show a strong negative moisture gradient over the Pacific, inducing the drying over the Pacific region. In contrast, the negative moisture gradient over the Pacific becomes weaker in March-April, reducing the drying over the Pacific. This study suggests that the difference in zonal moisture gradient between the two seasons, induced by the annual cycle of PW, differs in MJO propagation speed between the two seasons.
AS09-A001
Trends of Source Apportioned PM2.5 in Tianjin Over 2013–2019: Impacts of Clean Air Actions
Jiajia CHEN1+, Qili DAI1, Tianjiao DAI1, Xuehan WANG1, Yinchang FENG1#, Guoliang SHI1, Jianhui WU1, Yufen ZHANG1, Xiaohui BI1, Baoshuang LIU1, Yingze TIAN1, Philip K. HOPKE2,3, Beizhan YAN4, Patrick L. KINNEY5
1Nankai University, China, 2Clarkson University, United States, 3University of Rochester, United States, 4Columbia University, United States, 5Boston University, United States
The study analyzed a long-term PM2.5 speciation dataset in Tianjin, China, using dispersion normalized positive matrix factorization (DN-PMF) to evaluate the impact of specific control policies and measures on source-apportioned PM2.5 in support of China’s Clean Air Actions. Eight sources were resolved, including coal combustion (CC), biomass burning (BB), vehicular emissions, dust, steelmaking and galvanizing emissions, a mixed sulfate-rich factor, and secondary nitrate. After adjusting for meteorological fluctuations, a significant improvement in PM2.5 air quality was observed in Tianjin, with an annual decrease rate of 6.6%. Notably, PM2.5 from coal combustion decreased by 4.1% annually, demonstrating improved control of coal combustion-related emissions and fuel quality. Policies targeting the elimination of winter-heating pollution showed substantial success, as evidenced by reduced heating-related SO2, coal combustion, and sulfate from 2013 to 2019. The two industrial source types exhibited sharp declines after the 2013 mandated controls came into effect to phase out outdated iron/steel production and enforce tighter emission standards for these industries. Biomass burning significantly reduced by 2016 and remained low due to the implementation of a no open field burning policy. However, vehicular emissions and road/soil dust declined during the first phase of the Clean Air Actions but showed positive upward trends afterward, indicating the need for further emission controls. Nitrate concentrations remained constant despite a significant drop in NOX emissions, possibly due to increased ammonia emissions from enhanced vehicular NOX controls. Additionally, port and shipping emissions were evident, implying their impact on coastal air quality. These findings confirm the effectiveness of the Clean Air Actions in reducing primary anthropogenic emissions. However, further emission reductions are necessary to meet global health-based air quality standards. In conclusion, while significant progress has been made in improving air quality in Tianjin, continued efforts are needed to achieve and maintain optimal air quality levels.
AS09-A009
Simulation of Particle Number Concentration in the Present Day and the Preindustrial Period
Xueshun CHEN#+
Chinese Academy of Sciences, China
Quantifying differences in particle number concentration between the pre-industrial period and the present day is crucial to assess climate forcing and environmental effects caused by intensified anthropogenic activities. The lack of vegetation information for the pre-industrial period and the uncertainties in describing particle size distribution associated with primary emission and secondary formation are two leading factors preventing the simulation of particle number concentration. This study calculated the online emissions of biogenic volatile organic compound (BVOC) in the aerosol and atmospheric chemistry model of the Institute of Atmospheric Physics (IAP-AACM) by coupling the model of emissions of gases and aerosols from nature (MEGAN). The vegetation parameters were produced by the IAP Dynamic Global Vegetation Model (IAP-DGVM). The newly developed size-resolved aerosol module in IAP-AACM was adopted to simulate the particle number concentration in the present day and the pre-industrial period. The difference in the global aerosol number concentration between these two periods is presented and the corresponding sources are quantified.
AS12-A004
Improving Spatiotemporal PM2.5 Forecasting Accuracy in Beijing-Tianjin-Hebei of China Base on a Machine Learning Algorithm
Zheng ZHAO1+, Keyi CHEN1, Xiao TANG2#
1Chengdu University of Information Technology, China, 2Institute of Atmospheric Physics, Chinese Academy of Sciences, China
In recent years, fine particulate matter with an aerodynamic diameter less than 2.5 µm (PM2.5) is a major component of severe air pollution as China's economy and society continue to develop, as well as the acceleration of industrialization and urbanization. Accurate prediction of PM2.5 is beneficial to reduce air pollution events and improve people's comfort level of life. Due to lack of sufficient ground-based observations, it is hard to accurately measure air pollution in areas without ground stations. Although currently the air quality numerical models can provide air quality forecast for each model grid, the numerical integration process is affected by various uncertainties, leading to poor prediction performance eventually. In this study, by using NAQPMS model with high spatial resolution forecasting data and satellite data, we build a convolutional long short term memory (Conv-LSTM) algorithm to analyze the predictive performances of the PM2.5 spatiotemporal distribution during a smog event in Beijing-Tianjin-Hebei. The results indicate that this deep learning model can effectively improve the NAQPMS model's short-range PM2.5 prediction (72h) with high spatial resolution.
AS12-A007
Estimation of Global Daily Ground-level PM1 Concentrations and Spatial Exposure Disparities
Shuai WANG1#+, Hongliang ZHANG2
1Fudan University, China, 2University of Shanghai for Science and Technology, China
Exposure to airborne particulate matter (PM) pollution has been associated with multiple cardiovascular and respiratory diseases, which is a leading risk factor for human health. PM1 (PM < 1 μm) has received less attention than the much talked about PM2.5 (PM < 2.5 μm), but it is small enough to penetrate lung tissue into the bloodstream and can carry more heavy metals, chemicals, and volatile organic compounds (VOCs), making it more hazardous when inhaled. There are significant spatial differences in PM concentrations globally due to various reasons including economic activities, emission sources, population density, and geophysical conditions, further leading to disparities in PM pollution exposure. However, the disparities in short- and long-term PM1 exposure at the global scale are not yet clear. Global health risk assessment relies on accurate estimates of PM1 concentrations. However, the sparse amount of PM1 observations is not sufficient to support its exposure assessment. Fortunately, with the development of artificial intelligence, machine learning methods have shown outstanding performance in fusing multi-source data, which has the potential to expand the PM1 record globally and provide an opportunity to explore global disparities in PM1 exposure. In this study, a simple structured robust tree-based model was developed to integrate multi-source data and generate unprecedented global daily 10-km gap-free surface PM1 concentrations. The disparities of short- and long-term PM1 exposure were further quantified in the context of GDP and population distributions. The findings have the potential to inform policy decisions, public health interventions, and environmental management strategies at local, national, and global levels.
AS12-A009
Time Series Forecasting of Dew Point Temperature Using Facebook Prophet Model
Sherin BABU1#+, Binu THOMAS2,3, Tiju JOSEPH MATHEW4
1Assumption College Autonomous, India, 2Marian College Kuttikkanam, India, 3Mahatma Gandhi University, India, 4Christian College, India
The temperature at which water vapour in the air reaches saturation and starts to condense is known as the dew point temperature (DPT). DPT gives the measure of atmospheric moisture. For hydrological and agricultural research applications, precise and accurate DPT estimation is crucial. The effectiveness of Facebook's Prophet model for predicting DPT is examined in this study. Daily DPT readings from the Kottayam station of Kerala, India throughout a 3-year period from January 2017 to December 2019 are used. There is time-related information in the time-series dataset that can be utilized to forecast and evaluate the DPT data. The success of prophet forecasting time-series model is evaluated using the metrics Mean Absolute Error (MAE) and coefficient of determination (R2). The in-sample outcomes of the experiments demonstrate that the Prophet model can accurately forecast dew point temperature values (MAE=1.06, R2=0.60). Along with the use of regression models, Prophet model produces seasonality and trend analysis of the DPT data on a daily, weekly, and annual basis. Weather forecasting, which is crucial for affecting crop growth and boosting agricultural productivity, will benefit from this proposed work.
AS12-A019
Development of a Gap-filled Ground-level PM Estimation Algorithm by Integrating Geostationary Environment Monitoring Spectrometer (GEMS) and Atmospheric Transport Model Data
Eunjin KANG+, Jungho IM#
Ulsan National Institute of Science and Technology, Korea, South
Particulate matter (PM) causes various risks to human health, impacting both physically and psychologically, and has detrimental impacts on ecosystems and climate. Numerous previous studies have been developed to estimate ground-based PM using satellite aerosol products, chemical transport models, and in-situ measurements. However, satellite-derived data suffer from missing values due to clouds, while chemical transport models have limitations in terms of coarse spatial resolution. In this study, we tried to leverage the advantages of both the Geostationary Environment Monitoring Spectrometer (GEMS) Aerosol Optical Depth (AOD) and Community Multiscale Air Quality (CMAQ) AOD as primary variables. Additionally, meteorological reanalysis data and auxiliary variables were utilized to estimate gap-filled PM. We estimated GEMS-derived PM in clear sky conditions and CMAQ-derived PM in cloudy sky conditions, then finally fused two products using a Gaussian process in all-sky conditions. We applied a random forest-based real-time learning model to reflect the rapidly changing atmospheric conditions over East Asia. The overall model performance for PM10 showed comparable accuracy in clear and cloudy conditions, with R2 of 0.82 and RMSE of 28.74 μg/m3 in validation results. When applied to a huge wildfire in Uljin, South Korea, we confirmed the ability to estimate significantly high concentrations across the region without missing values. The developed gap-filled PM product is expected to effectively monitor spatiotemporally continuous PM concentration, including high PM cases.
AS12-A028
High-resolution Satellite Precipitation Using U-net Algorithm
Min-gyeong HWANGBO+, Kyuhee SHIN, Soorok RYU, Gyu Won LEE#
Kyungpook National University, Korea, South
Accurate precipitation prediction is vital for effective management of water-related disasters. Precipitation data derived from the ground radar is commonly utilized due to its proficiency in detecting atmospheric motion and measuring real-time precipitation with high resolution. However, the observation range of the ground radar is limited to local regions, particularly around the land. To obtain precipitation data with finer spatial coverage, including oceans, satellite image becomes a crucial data source. Developing methodologies for quantitatively predicting precipitation from satellite is deemed necessary for monitoring water-related disasters. The use of U-Net for predicting precipitation from geostationary satellites is a deep learning architecture commonly employed for image segmentation tasks. This architecture, known for preserving high-resolution information between input images and output masks, proves valuable in predicting precipitation amounts from geostationary satellites. This study uses a U-Net algorithm for estimating high-resolution satellite precipitation, focusing on selected summer precipitation cases in South Korea during 2019-2020. Constructing the training set involved using dependent variables from Automatic Weather Stations (AWS) grid interpolation data and Hybrid Surface Rainfall (HSR) composite radar precipitation data. Independent variables included simultaneous inputs from Geostationary Korea multi-purpose satellite 2A (GK-2A), utilizing Level-1b data encompassing various channels and Level 2 data such as cloud top height, cloud top temperature, and Brightness Temperature Difference (BTD) values calculated from infrared channels. Both spatial resolutions were set at 1 km, utilizing images with dimensions of 480 (width) × 600 (height). The study compared the performance of the U-Net model using two different dependent variables, revealing that employing the higher-resolution HSR radar composite data allows for the generation of detailed precipitation fields.
ACKNOWLEDGMENT
This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS12-A031
Improving PM2.5 Prediction Performance of CMAQ Through Post-processing Correction Using Artificial Intelligence
Seong-il LEE#+, Hyo-Jong SONG, Youngchae KWON
Myongji University, Korea, South
Air pollution is a big problem all over the world. It is important not only because it reduces the air pollutants that cause, but also because it can be prepared and prevented through accurate predictions. Therefore, research on air pollution is continuously being conducted, but predicting pollutants is difficult because numerous factors are involved. In this study, among various pollutants, a method that can improve PM2.5 prediction performance by utilizing machine learning was studied and compared with previous data. As the data, the result data obtained through CMAQ were used, and the actual observed values were used for comparison. The data of CMAQ used not only PM2.5, but also the data of IPR (Integrated Process Rate), which is the data of the physical mechanism that contributes to the generation of pollutants present in CMAQ. In this study, the research was conducted using the following method. In atmospheric environmental science, machine learning is usually used to predict pollutants, but if the prediction performance is poor, you can change the model structure or use new data to get better results, which requires more time and verification to take advantage of the new data. This study uses a different method than before. This study uses the model's result data as input data, sets the target to Bias (the difference between predicted and observed values), and performs "bias correction" using machine learning and improves the model's performance through "post-processing correction." For performance comparison, scores that divide the grades of PM2.5 and RMSE, IOA, etc. were used, and a total of two models were made and compared with the input data using CMAQ result data and IPR. An analysis was also conducted on what period is used for one data or the results appear differently depending on the region or concentration. These activities have improved performance.
AS12-A032
Estimation of Surface CH4 Concentration from Tropomi Satellite Observations Using Machine Learning
Lee DAGYO1+, Hanlim LEE1#, Wonei CHOI2
1Pukyong National University, Korea, South, 2NASA Goddard Space Flight Center, United States
Methane is the second most important greenhouse gas after carbon dioxide, possessing a global warming potential 21 times greater than that of carbon dioxide. There are also concerns that biogas, a major source of methane, can be a source of fine dust emissions. While satellite observations are extensively used due to their wide spatial coverage and high resolution, the methane concentrations observed from satellites are provided as column amount or column average mixing ratios, making it challenging to directly relate them to surface-level methane concentrations. Methane emissions primarily occur in the lower atmosphere near the surface. In this study, we have developed a surface-level methane concentration estimation model based on machine learning, utilizing satellite data for vertical methane concentrations. "This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE)."
AS12-A035
Estimation of Surface-level Nitrogen Dioxide Concentrations Over Korea from GEMS Observations
Seonyeong PARK1+, Wonei CHOI2, Hanlim LEE1#
1Pukyong National University, Korea, South, 2NASA Goddard Space Flight Center, United States
Nitrogen dioxide (NO2) is an important target for monitoring atmospheric quality. In particular, the surface NO2 concentrations are closely related to human life. This study aims to estimate the diurnal surface NO2 concentrations from the Geostationary Environment Monitoring Spectrometer(GEMS) observations in Korea. The machine learning was used various satellite-based variables, numerical model-based meteorological variables, and auxiliary variable. Random Forest (RF) was evaluated and compared with Multiple Linear Regression (MLR) as a base statistical method. The estimated surface concentrations were validated through cross-validation approaches. The results show that the urban model has great performance in estimating surface NO2 concentrations. The NO2 vertical column density among the GEMS data showed the largest contribution in the model. "This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE)."
AS20-A002
| Invited
Molecular Chemical Characterization of Gas-phase Reactive Organic Carbon (ROC) Emissions from Typical Volatile Chemical Products (VCPs) Manufacturing
Song GUO#+, Daqi LV, Kai SONG, Yuanzheng GONG, Zichao WAN, Kun HU, Sihua LU, Limin ZENG, Shaodong XIE, Min HU
Peking University, China
With the sustained strict control of combustion-related emissions over last decades, volatile chemical products (VCPs) have become an increasingly important anthropogenic source of gas-phase reactive organic carbon (ROC) emissions. In the present work, on-site measurements of gas-phase ROC were performed for typical VCPs manufacturing, including coatings, pesticides, asphalts, consumer products and plastics. Herein, we comprehensively characterized a wide volatility range of organic compounds using a thermal desorption two-dimensional gas chromatography coupled with a quadrupole mass spectrometer (TD-GC×GC-qMS) and a GC coupled with MS and flame ionization detection (GC-MS/FID). In total, 623 species were resolved at the molecular level. Mass fractions of IVOCs ranged from 3.48‰ to 34.97%. Detergents, water-based coatings, asphalts and hair cosmetics possessed high proportions of IVOCs (15.09-34.97%). VOCs dominated OFP, while IVOCs contributed as much as VOCs to SOAP. In terms of chemical components, aromatics were the primary control compounds for the synergistic reduction of O3 and SOA. This work demonstrates that IVOCs from VCPs manufacturing are non-negligible. Our measured source profiles can provide supports for model simulations and parameter estimations, allowing for a more accurate estimate of the impacts of VCPs manufacturing on China's ambient atmosphere.
AS20-A004
| Invited
Intermediate Volatility Compounds Dominate Secondary Organic Aerosol Formation from Biomass Burning Emissions
Kun LI#+
Shandong University, China
Organic gases from biomass burning are a large source of secondary organic aerosol (SOA). Previous smog chamber studies found that the main SOA contributors in biomass burning emissions are volatile organic compounds (VOCs). Intermediate volatility organic compounds (IVOCs), thought to be efficient SOA precursors, are a considerable fraction of biomass emissions, but their contribution to SOA formation has not been directly observed. Here, by deploying a newly-developed oxidation flow reactor to study SOA formation from wood burning, we find that IVOCs can contribute ~70% of the formed SOA, i.e., >2 times more than VOCs. This previously missing SOA fraction is interpreted to be due to the high wall losses of semi-volatile oxidation products of IVOCs in smog chambers. The finding in this study reveals that SOA production from biomass burning is more than 3 times higher compared to previous studies, and highlights the urgent need for more research on the IVOCs from biomass burning and potentially other emission sources. In addition, by applying source apportionment and clustering methods, we are able to track the chemical evolution of SOA molecules. The results provide insights into the multi-generation chemistry when biomass burning emissions are transported in the atmosphere.
AS20-A006
Atmospheric Autoxidation of Typical Volatile Chemical Products
Zihao FU#+, Song GUO, Min HU
Peking University, China
Secondary organic aerosol (SOA), formed in the atmosphere by oxidation of volatile organic compounds (VOCs), affects air quality, climate, and human health. With stricter regulation of atmospheric VOCs originating from vehicles and industries, the use of volatile chemical products (VCPs) and the transformation mechanism of VCPs become increasingly important to quantify air quality. Linalool, a high-production VCP commonly found in cleaning products and disinfectants, is increasingly recognized as an emerging contaminant in both indoor and outdoor air. Understanding the atmospheric transformation mechanism of linalool is crucial for assessing its impact on the atmospheric chemistry and human health. Here, we performed quantum chemical calculations and computational toxicology to investigate the reaction mechanism and toxicity evolution of linalool under the low and high NO/HO2· levels representing the indoor and outdoor environment. Our findings reveal that linalool can undergo the novel mechanisms involving concerted peroxy (RO2·) and alkoxy radicals (RO·) modulated autoxidation, with successive transfer of radical-center in multiple ways, including RO2·-dominated cyclization and H-shift combined with RO·-dominated cyclization, H-shift, and bond scission reactions. This expands the widely known RO2·-dominated H-shift-driven autoxidation and proposes a generalized autoxidation mechanism that leads to the formation of low-volatile SOA precursors. Toxicological analysis shows that over half of transformation products (TPs) exhibited higher carcinogenicity and respiratory toxicity compared to linalool. We also propose time-dependent toxic effects of TPs to assess their long-term indoor and outdoor toxicity. Our results indicates that the strong indoor emission coupled with slow consumption rates, lead to significant health risks under indoor environment. The results highlight complex indoor air chemistry and health concerns regarding persistent toxic products during indoor cleaning which involves use of linalool or other VCPs.
AS20-A012
Characterizing Water Solubility of Fresh and Aged Secondary Organic Aerosol in PM2.5 with the Stable Carbon Isotope Technique
Fenghua WEI+, Xing PENG#, Liming CAO, Mengxue TANG, Ning FENG, Ling-Yan HE, Xiaofeng HUANG
Peking University Shenzhen Graduate School, China
The investigation of the water-soluble characteristics of secondary organic carbon (SOC) is essential for a more comprehensive understanding of its climate effects. However, due to the limitations of the existing source apportionment methods, the water solubility of different types of SOC remains uncertain. This study analyzed stable carbon isotope and mass spectra signatures of total carbon (TC) and water-soluble organic carbon (WSOC) in ambient PM2.5 samples for one year and established stable carbon isotope profiles of fresh and aged SOC. Furthermore, the Bayesian stable isotope mixing (BSIM) model was employed to reveal the water solubility characteristics of fresh and aged SOC in a coastal megacity of China. WSOC was dominated by secondary sources, with fresh and aged SOC contributing 28.1% and 45.2%, respectively. Water-insoluble organic carbon (WIOC) was dominated by primary sources, to which fresh and aged SOC contributed 23.2% and 13.4%. We also found the aging degree of SOC has considerable impacts on its water solubility due to the much higher water solubility of aged SOC (76.5%) than fresh SOC (54.2%). Findings of this study may provide a new perspective for further investigation of the hygroscopicity effects of SOC with different aging degrees on light extinction and climate change.
AS20-A013
Insights on Spatial Inhomogeneity of New Particle Formation Events at Coastal Suburban and Rural Sites in Northern China
Yujiao ZHU1#+, Yanqiu NIE1, He MENG2, Xiaohong YAO3, Likun XUE1, Wenxing WANG1
1Shandong University, China, 2Qingdao Eco-environment Monitoring Center of Shandong Province, China, 3Ocean University of China, China
The atmospheric new particle formation (NPF) events contribute a large amount of global ultrafine particles and cloud condensation nuclei (CCN), thereby reportedly influencing the global climate and the earth’s radiation balance. There is, however, a large inhomogeneity on their occurrence in horizontal and vertical directions, complicating their potential climate impacts. Here, simultaneous measurements of particle number size distributions were conducted to explore the inhomogeneity at both suburban and coastal rural sites in northern China during a summer season in 2020. Five NPF events were observed simultaneous occurred at both sites, in which three NPF events occurring in spatial homogeneity (Scenario 1) and the remaining two NPF events displaying spatial inhomogeneity (Scenario 2). In Scenario 1, the new particle formation rate (FR) narrowly varied between 1.0 cm-3 s-1 to 2.5 cm-3 s-1, with the FRs at both sites were basically consistent. The same was true for the net maximum increase in the nucleation mode particles number concentration (NMINP), with 0.63±0.26×104 cm-3 at ASW site and 0.56±0.17×104 cm-3 at OUC site. However, in Scenario 2, while FR and NMINP at ASW site remained relatively consistent with that in Scenario 1, these two values at OUC site substantial increased by one to two orders of magnitude. The observed ion components, such as SO42-, NO3-, MSA and oxalate can’t support the larger FR and NMINP at OUC site, leaving the roles of HOMs and DMAH+ to be further examined. In contrast, the growth rate (GR) exhibited a higher degree of spatial homogeneity throughout the five NPF events, suggesting the consistent new particle growth throughout the PBL. Our results hypothesize the relative contributions of downward transport and local formation of new particles.
AS20-A015
Contrasting Impacts of Humidity on the Ozonolysis of Monoterpenes: Insights Into the Multi-generation Chemical Mechanism
Shan ZHANG+, Kun LI#
Shandong University, China
Secondary organic aerosol (SOA) formed from the ozonolysis of biogenic monoterpenes is a major source of atmospheric organic aerosol. It has been previously found that relative humidity (RH) can influence the SOA formation from some monoterpenes, yet most studies only observed the increase or decrease in SOA yield without further explanations of molecular-level mechanisms. In this study, we chose two structurally different monoterpenes (limonene with an endocyclic double bond and an exocyclic double bond, Δ3-carene with only an endocyclic double bond) to investigate the effect of RH in a set of oxidation flow reactor experiments. We find contrasting impacts of RH on the SOA formation: limonene SOA yield increases by ~100% as RH increases, while there is a slight decrease in Δ3-carene SOA yield. Although the complex processes in the particle phase may play a role, we primarily attribute it to the water-influenced reactions after ozone attack on the exocyclic double bond of limonene, which leads to the increment of lower volatile organic compounds under high RH condition. However, as Δ3-carene only has an endocyclic double bond, it cannot undergo such reactions. This hypothesis is further supported by the SOA yield enhancement of β-caryophyllene, a sesquiterpene that also has an exocyclic double bond. These results greatly improve our understanding of how water vapor influences the ozonolysis of biogenic organic compounds and subsequent SOA formation processes.
AS20-A016
| Invited
Contribution of Secondary Organic Aerosol Formation to Cloud Condensation Nuclei in the Global Troposphere: A Modeling Perspective
Mingxu LIU#+
Peking University, China
Formation of secondary organic aerosols (SOA) through the atmospheric oxidation of organic vapors has potential to enable particle growth to cloud condensation nuclei (CCN)-relevant sizes. In this work, we constrain a global aerosol model by using aircraft measurements to reveal the global importance of SOA formation in CCN production. Our improved model, with explicit size-resolved aerosol microphysics and parametrizations of semivolatile organic oxidation products, presents a state-of-the-art performance in simulating both particle number concentrations and organic aerosol concentrations dominated (80–95%) by SOA in the remote atmosphere, which have been challenges in previous modeling studies. The SOA formation in concert with aerosol nucleation contributes to more than 50% of CCN concentrations in those pristine environments featuring low background aerosol concentrations. We estimate that the SOA-derived CCN alters the magnitude of cloud radiative forcing by ∼0.1 W m−2. Our findings underscore the necessity for aerosol-climate models to represent controls on CCN concentrations by SOA production.
AS20-A020
Impact of COVID-19 Lockdown on Winter Atmospheric S/IVOCs Pollution Characteristics in Beijing
Zichao WAN+, Kai SONG, Kun HU, Qiqi ZHOU, Song GUO#
Peking University, China
The present study investigates the influence of the COVID-19 lockdown on the characteristics of winter atmospheric Semi-Volatile and Intermediate Volatility Organic Compounds (S/IVOCs) pollution in Beijing. The implementation of lockdown measures during the pandemic resulted in unprecedented changes in human activities and emissions. This research aims to assess the impact of these restrictions on the levels and composition of S/IVOCs in the air and their contribution to Secondary Organic Aerosol (SOA) formation.
AS20-A021
Secondary Organic Aerosol Formation Potential of Emission from Residential Coal Combustion
Zheng CHEN1+, Zichao WAN1, Wenfei ZHU2, Song GUO1#
1Peking University, China, 2University of Shanghai for Science and Technology, China
Residential coal combustion is an important contributor to organic aerosols(OA) in urban and rural areas. However, the chemical characteristic and formation mechanism of secondary organic aerosol(SOA) from residential coal combustion emission still remain indeterminate. In this study, we simulated residential coal combustion processes in the laboratory, and investigated the primary organic aerosols(POA) emissions. An Aerodyne potential aerosol mass reactor(PAM) was used to evaluated the SOA formation. The evolution characteristics of organic aerosols were investigated by High Resolution Time-of-Flight Aerosol Mass Spectrometer(HR-ToF-AMS), and the characteristics of gas precursors was measured by Vocus-Proton Transfer Reaction Mass Spectrometer(Vocus). A direct comparison has been made between the primary emission and secondary formation of residential coal combustion. It will be more conducive to the subsequent study on the contribution of residential coal combustion sources to urban and rural air pollution and the assessment of the health risk of residential coal combustion fume exposure, which provide a reference for the formulation of corresponding control strategies.
AS20-A025
Secondary Organic Aerosol Formation from Daytime and Nighttime Oxidation Chemistry of 2-methylfuran from Biomass Burning
Taekyu JOO1,2#+, Junsu GIL1, David PANDO2, Michelia DAM2, Meehye LEE1, Nga Lee NG2
1Korea University, Korea, South, 2Georgia Institute of Technology, United States
Biomass burning releases a substantial amount of gas-/particle-phase carbon into the atmosphere, and its frequency and intensity are expected to rise with climate change. Recent studies demonstrated that furanoids, which are one of the major compound classes emitted from biomass burning, are reactive to oxidants such as hydroxyl (OH) or nitrate (NO3) radicals and have potentials to form secondary organic aerosol (SOA). Here, we investigated gas-phase oxidation and SOA formation from OH and NO3 oxidation of 2-methylfuran in the presence of NOx. Experiments were performed under dry conditions (RH<5%) with varying initial 2-methylfuran concentrations (91-823ppb) at the Georgia Tech Environmental Chamber facility. We found that SOA yields were moderately higher in NO3 radical experiments (2-4% at 7-50μg/m3) compared to OH radical experiments (1-3% at 8-72μg/m3). Importantly, a substantial amount of SOA was formed after the complete depletion of 2-methylfuran, highlighting the significance of multigenerational chemistry in SOA formation regardless of the type of oxidant. We proposed reaction mechanisms based on the compounds identified using a Filter Inlet for Gases and AEROsols coupled with time-of-flight iodide chemical ionization mass spectrometer (FIGAERO-HR-ToF-I-CIMS). C4H4O3 (hydroxy or carboxylic acid) and C4H3NO5 (organic nitrate) were the major gas species detected in OH and NO3 radical experiments, respectively, and they shared similar formation pathways during peroxy radical reactions (i.e., RO2+NO/NO3/RO2 followed by alkoxy radical decomposition). For particle phase, C4H4O3 and C5H6O3 were the major species identified in OH and NO3 radical experiments, respectively. These compounds exhibited multifunctionalities (carbonyl+carboxylic acid) and presented as oligomers in 2-methylfuran SOA. The comprehensive results from this study can contribute to improving our understanding of furanoids oxidation and subsequent aerosol formation in biomass burning plumes especially when plumes travel over NOx-polluted regions, spanning both daytime and nighttime conditions.
AS20-A026
Seasonal Variation and Environmental Effects of the Ambient Semi-volatile and Intermediate Volatile Organic Compounds (S/IVOCs) in Beijing, China
Kun HU#+, Zichao WAN, Kai SONG, Qiqi ZHOU, Song GUO
Peking University, China
Semi-volatile and intermediate volatile organic compounds (S/IVOCs) are important precursors of secondary organic aerosols (SOA), which is an important component of fine particulate matter (PM2.5). Some previous studies have shown that seasonal variation can make a difference in the concentration level and chemical composition of pollutants. In order to improve the understanding of the characteristics of ambient S/IVOCs of Beijing with seasonal variation, this study used the Tenax TA tube to sample S/IVOCs species for one month in the spring and autumn of 2021, respectively, and quantitatively identified by thermal desorption and comprehensive two-dimensional gas chromatography and mass spectrometry (TD-GC×GC-MS). Nearly 200 species were detected in this study. The results showed that the concentration level and chemical composition of S/IVOCs were significantly different between spring and autumn. The contribution of S/IVOCs to aerosol formation potential (AFP) in two seasons was further compared and the key components were identified. The results of this study are conducive to providing data for air pollution prevention and control in China.
AS20-A033
Assessment and Evaluation of Organic Carbon Concentrations in South Korea, Considering Both Secondary and Primary Sources, Through the Application of Chemical Transport Models and Theoretical Methods
Naser MOHAMMADZADEH+, Myong-In LEE#
Ulsan National Institute of Science and Technology, Korea, South
Organic aerosols, comprising Primary Organic Aerosol (POA) and Secondary Organic Aerosol (SOA), constitute a pivotal element of PM2.5, contributing significantly to air quality degradation. This study employs Positive Matrix Factorization (PMF) to investigate the source apportionment of organic aerosols, differentiating between POA and SOA. The distinction between secondary and primary components is achieved through theoretical methods such as EC-tracer and chemical model simulation fractions. The intricate nature of organic aerosols demands advanced modeling techniques, and in this research, we utilize WRF-Chem (RACM-MADE/VBS) for a comprehensive analysis. The primary goal is to evaluate model simulations concerning the composition of Secondary and Primary Organic Aerosols within PM2.5. This evaluation involves a comparison with observational data collected from ground-based stations in Seoul, South Korea, during the KORUS-AQ 2016 period (May 1st to June 10th). The EC-tracer and model-based-fraction methods yield observation percentages of 62% and 65% for SOA and 38% and 35% for POA, respectively. These results indicate a significant role of the secondary organic portion in Seoul station. From another perspective, model simulations attribute 69% to SOC and 31% to POC, suggesting a slight overestimation of the secondary part and an underestimation of the primary part. Furthermore, this research employs PMF to classify six sources for Seoul stations, namely Soil dust, Motor vehicle, Combustion/Industry, Natural sources, Biomass/field burning. Factor contribution analysis reveals that approximately 25% of Organic Carbon (OC) is derived from secondary sources, while the primary sources contribute to nearly 75%. These findings underscore the importance of accurate source apportionment in air quality studies and emphasize the significance of advanced models, providing valuable insights into PM2.5 composition.
AS20-A034
| Invited
Atmospheric Secondary Pollution Chemistry of Volatile Chemical Products
Hongbin XIE#+, Fangfang MA, Deming XIA
Dalian University of Technology, China
Volatile chemical products (VCPs) have been recognized as an important source of volatile organic compounds emissions to the atmosphere, making VCPs become new precursors leading to secondary pollution in urban atmosphere. Due to the abundance and limited atmospheric transformation mechanisms of VCPs, it is a challenge to identify priority controlled VCPs for the secondary pollution prevention. Herein, quantum chemical calculations and kinetics modeling were employed to investigate the atmospheric transformation mechanism of four types VCPs (i.e., emerging amines, methylsiloxanes, organophosphates and aromatics), and achieved three innovative achievements: (1) A machine learning and big-data driven methods to study the atmospheric transformation mechanisms (i.e., oxidation and clustering) of VCPs was developed. The developed methods increase the efficiency of studying the atmospheric oxidation mechanisms and clustering of VCPs by nearly 10-100-fold. (2) Secondary pollution mechanisms of the selected four types of VCPs were revealed. It was found that these four types of VCPs undergo three novel oxidation mechanisms by employing developed method. More importantly, they can produce low volatile products or highly toxic products (e.g., HCHO, nitrosamines, etc.) via three novel mechanisms. Additionally, we disclosed chemical nature that determines the potential of emerging amines to binary clustering with inorganic acids. Based on the understanding of binary clustering mechanisms, a synergistic clustering mechanism of emerging amines was proposed, which were confirmed by field observation in Beijing. (3) A predictive model for secondary pollution potential of important VCPs was developed and the priority controlled VCPs were identified. Selecting emerging amines as a representative, we developed four high-throughput models to predict the potential of emerging amines to produce carcinogenic nitrosamine and their potential to clustering with inorganic acids. We found that six emerging amines have high potential for atmospheric secondary pollution and should be prioritized for prevention and control.
AS26-A002
Lagged Effect of the PDO on Decadal Variation in Global Land Precipitation
Lili LIANG1#+, Shijing LIANG1, Laurent LI2, Huiling YUAN3, Zhenzhong ZENG1
1Southern University of Science and Technology, China, 2Laboratoire de Météorologie Dynamique, France, 3Nanjing University, China
The Pacific Decadal Oscillation (PDO), as the leading mode of sea surface temperature (SST) in the North Pacific, modulates the global temperature and precipitation. While previous studies have shown a negative relationship between the global precipitation and the PDO, the time-delayed feature of this relationship remains underexplored. Here we investigate the lagged effect of the decadal variations in the PDO on the global land precipitation using cross-correlation at multiple scales. We find that there is a delayed response of precipitation to the PDO, with the regional correlation peaking at a certain delay and gradually decreasing with increasing lag time. We note the asymmetric impacts of the positive and negative PDO phases on precipitation. Seasonal analysis reveals that the PDO is related to land precipitation during the subsequent season relative to the rest of the year, with the highest correlation occurring in the boreal winter. The delay in response is likely due to the constant SST forcing of the PDO to the atmospheric circulation. This study highlights the lag duration of the PDO–precipitation relationship, potentially enriching our understanding of this relationship and enhancing climate predictions on decadal timescales.
AS26-A006
Predictable Patterns of Summertime Surface Air Temperature in Northern Hemisphere and Their Predictability Sources in the SEAS5
Zheng LU+, Yang ZHANG#
Nanjing University, China
Based on 36-yr hindcasts data from the fifth-generation seasonal forecast system of the European Centre for Medium-Range Weather Forecasts (SEAS5), the most predictable patterns of the summertime 2-m air temperature (T2m) in the extratropical Northern Hemisphere are extracted via the maximum signal-to-noise (MSN) empirical orthogonal function (EOF) analysis, and their associated predictability sources are identified by regression and composite analysis of various external forcing fields. The MSN EOF1 is a mono warming pattern in the Northern Hemisphere, which captures the warming trend over the Eurasia and North America, but misses a cold anomaly in the Ural Mountains. The MSN EOF2 features warm anomalies over the western Pacific and cold anomalies over central and eastern Pacific, and eastern North America. The sources of predictability can be traced to the first pattern of the North Pacific Sea Surface Temperature (SST). The MSN EOF3 shows the warm anomalies in northern Eurasia and the cold anomalies in central and eastern Pacific, and its associated predictability is from multiple external forcing factors, including middle-high latitude snow, Eurasia soil temperature, and North Pacific SST. The MSN EOF4 shows the warm anomalies in the mid-eastern Pacific and the cold anomalies in the mid-latitude North America, and a less obvious high-latitude cold anomaly--mid-latitude warm anomaly pattern in the Eurasia. This due to the combined action of land and ocean forcing factors. The MSN EOF5 reflects T2m variability over the Barents Seas, which is plausibly linked to the forcing of the Arctic sea ice. The information on the leading predictable patterns and their sources of predictability is further used to establish a statistical prediction model of seasonal prediction to improve the prediction skill of T2m. The calibrated prediction skill in terms of the anomaly correlation coefficient improves over the Eurasia, implying a possible way to improve the summertime T2m prediction in the SEAS5.
AS26-A007
Implementation and Evaluation of SNICAR Snow Albedo Scheme in Noah-MP (Version 5.0) Land Surface Model
Tzu-Shun LIN1#+, Cenlin HE1, Ronnie ABOLAFIA-ROSENZWEIG1, Fei CHEN2, Wenli WANG3, Michael BARLAGE4, David GOCHIS1
1NSF National Center for Atmospheric Research, United States, 2The Hong Kong University of Science and Technology, Hong Kong SAR, 3Chinese Academy of Sciences, China, 4National Oceanic and Atmospheric Administration/ Environmental Modeling Center, United States
The widely used Noah-Multiparameterization Land Surface Model (Noah-MP LSM) currently adopts snow albedo parameterizations that are semi-physical in nature with nontrivial uncertainties. To improve physical representations of snow albedo processes, a state-of-the-art snowpack radiative transfer scheme, the latest version of the Snow, Ice, and Aerosol Radiative (SNICAR) model, is integrated into Noah-MP in this study. The coupled Noah-MP/SNICAR represents snow grain properties (e.g., shape and size), snow aging, and physics-based snow-aerosol-radiation interaction processes. We compare Noah-MP simulations employing the SNICAR scheme and the default semi-physical Biosphere-Atmosphere Transfer Scheme (BATS) against in-situ albedo observations at three Rocky Mountain field stations. The agreement between simulated and in-situ observed ground snow albedo in the broadband, visible, and near-infrared spectra is enhanced in Noah-MP/SNICAR simulations relative to Noah-MP/BATS simulations. The SNICAR scheme significantly improves the temporal variability of snow albedo (particularly in the near-infrared band) compared to the default semi-physical BATS snow albedo scheme in Noah-MP. Importantly, the Noah-MP/SNICAR model, with constraints of fresh snow grain size from the MODIS snow covered area and grain size (MODSCAG) satellite data, physically represents and quantifies the snow albedo and absorption of shortwave radiation in response to snow grain size, non-spherical (e.g., hexagonal) snow shapes, and light-absorbing particles including dust, organic, and black carbon. The coupling framework of the Noah-MP/SNICAR model provides a means to reduce the bias in simulating snow albedo.
AS26-A015
Advancements in Geo-physical Processes for Snow-covered Lands: A Focus on Noah-MP Within the KIM System
Hyeon-Ju GIM#+
Korea Institute of Atmospheric Prediction Systems, Korea, South
A land surface model (LSM) of Noah, which is so called second generation LSM, was incorporated and optimized within Korea Integrated Model (KIM) system during the initial phase of Korea Institute of Atmospheric Prediction Systems (KIAPS) from 2011 to 2019. Progressing into the ongoing second phase of KIAPS from 2020 to 2026, the third generation LSM, Noah-MultiParameterization (Noah-MP), has been integrated into the KIM system. Despite ongoing optimization efforts within KIM, a critical issue persists—the notable cold bise over snow-covered lands significantly impacts lower tropospheric atmosphere thermal conditions. Consequently, this bias adversely affects the forecasting skill for medium-range and longer-range predictions. This presentation aims to investigate the challenges posed by the cold bise in Noah-MP within the KIM system and propose potential solutions to enhance predictive performance. Acknowledgements: This work was carried out through the R&D project “Development of a Next-Generation Numerical Weather Prediction Model by the Korea Institute of Atmospheric Prediction Systems (KIAPS)”, funded by the Korea Meteorological Administration (KMA2020-02212).
AS29-A011
Distinct Circulation Evolutions of Sudden Stratospheric Warmings Preceded by Cooling and Warming Over the Barents-Kara Seas
Chongyang ZHANG+, Jiankai ZHANG#
Lanzhou University, China
Different tropospheric precursor anomalies of sudden stratospheric warmings (SSWs) may lead to different circulation evolutions. This study found that circulation evolution of SSWs following cooling (CBKS-SSW) and warming (WBKS-SSW) over the Barents-Kara Seas (BKS) are fundamentally different. WBKS-SSWs are typically accompanied by enhanced East Asia trough, enhanced Atlantic ridge and negative tropospheric annular mode anomalies persisting for one month. By contrast, CBKS-SSWs are associated with cooling over northern Eurasia and an absence of sustained tropospheric annular mode anomalies. The dynamic mechanisms are further revealed. WBKS-SSW would suppress (promote) vertical (southeastward) propagation of waves induced by the enhanced BKS wave source, thereby amplifying East Asia trough. Decreased phase speed would promote the westward migration of Ural ridge during WBKS-SSWs, amplifying Atlantic ridge, and the westward migration of Aleutian low during CBKS-SSWs, amplifying northern Eurasia cooling. This study suggests that identifying CBKS-SSWs and WBKS-SSWs is important for the extended-range weather forecasts.
AS29-A012
Impacts of Early-winter Arctic Sea-ice Loss on Wintertime Surface Temperature in China
Xufan XIA+, Jiankai ZHANG#
Lanzhou University, China
Under the background of global warming, Arctic sea-ice loss could be a contributor to extreme cold events in the mid-latitudes over recent decades, especially over East Asia, which has attracted widespread attention. Using both observations and model simulations, we found that sea-ice loss could induce cooling anomalies over Northeast China, North China, Central China, and Northwest China during winter, with significant increases in both the number of extreme cold days and the intensity of extreme low temperatures over these regions. Furthermore, the quantitative analysis of tropospheric processes and stratosphere-troposphere coupling processes indicates that the impact of stratosphere-troposphere coupling on surface cooling over Northeast China associated with BKS sea-ice loss is more important than that over other regions. For the tropospheric processes, the strengthening of the Aleutian low induced by sea-ice loss is favorable for the transport of cold air into China and results in significant cooling, especially in Northeast China. In terms of the stratosphere-troposphere coupling processes, sea-ice loss leads to a displacement of the stratospheric polar vortex toward North China by modulating upward propagating planetary waves.
AS29-A015
Observation of Mesopause Atmospheric Instability of Hainan, China 19.99°N, 110.34°E Based on Na Lidar of Meridian Project
Siyin LIU1+, Zou XU1#, GuoTao YANG2, Dali YANG1, Tiemin ZHANG1, Yi QU1, Hong YANG1, Hanxiao ZHANG1, Hongyan PENG1
1Hainan Normal University, China, 2Chinese Academy of Sciences, China
Atmospheric instability is an important condition leading to meteorological disasters such as typhoons, hurricanes, tornados, heavy rain, and snowstorms, so accurate observation and analysis are critical. Based on the Meridian Project Na Lidar data, atmospheric instability observations were conducted in Hainan, China, the seasonal Ri (Richardson number) distribution and their typical properties are investigated based on 94 accumulated nightly data. The results showed that during this period, Ri values were within 0.5-2, and the seasonal distribution of Ri was similar to that of atmospheric density disturbances and monthly horizontal disturbance wind RMS velocity, with maxima around the summer and winter solstices and minima around the spring and autumn equinoxes, suggesting that the mesosphere atmosphere in Hainan is stable in spring and autumn, while the atmospheric disturbance is relatively strong in summer and winter. It was also found that some Ri values were quite low in November and December, which is evidence that the disturbances of winter in Hainan are still strong. By consulting the single nightly Na density evolution process, selected nights with large disturbances and low Ri values, especially, the atmospheric instability process and the causes of disturbances for detail were analyzed. The gravity wave disturbance activities and potential chemical effects may be the main causes of atmospheric instability processes in Hainan during winter. Meantime, several nights with small disturbances and high Ri values were as controls, during those nights, almost no changes in the sodium layer were seen, which is in line with our theory expectations. These findings will enable us to more accurately understand and predict the development of atmospheric instability, thereby uncovering the natural essence of dynamics and chemical behaviors in the Earth's lower latitude upper atmosphere, and it is of significant value for comprehending and forecasting the occurrence and evolution of meteorological disasters.
AS29-A020
The Predictability of the 2021 SSW Event Controlled by the Zonal-mean State in the Upper Troposphere and Lower Stratosphere
Hyeong-Oh CHO+, Min-Jee KANG, Seok-Woo SON#
Seoul National University, Korea, South
Sudden stratospheric warming (SSW) describes a disruption of the stratospheric polar vortex in the winter hemisphere. It affects not only the stratospheric circulation but also the surface climate for up to two months, serving as an important source of subseasonal-to-seasonal (S2S) predictability in midlatitudes. This study evaluates the predictability of the 2021 SSW and investigates the crucial factors that determine its predictability in the ECMWF and JMA S2S real-time forecasts. In both models, only a subset of the ensemble members predicted the SSW at the lead time of about two weeks before the onset. By comparing the 10 ensembles with successful SSW predictions and those with failed predictions, we found that the ensembles predicting the SSW have relatively stronger wave fluxes from the upper troposphere to the stratosphere than the others. Stronger wave fluxes, particularly those of zonal wavenumber one, are not the result of the tropospheric precursors such as the Ural blocking and Aleutian cyclones but they result from the modulation of the wave propagation by the background state. In particular, the ensembles with failed SSW predictions tend to have a negative potential vorticity gradient in the upper troposphere and lower stratosphere, which limits the upward wave propagation into the stratosphere and provides an unfavorable condition for the SSW. This result suggests that not only the wave sources in the troposphere but also the background state in the upper troposphere and lower stratosphere can modulate the predictability of SSW in S2S prediction models.
AS29-A023
Downward Coupling of 2018 Sudden Stratospheric Warming in SNAPSI Experiments
Dong-Chan HONG+, Seok-Woo SON#
Seoul National University, Korea, South
The downward coupling of the February 2018 Sudden Stratospheric Warming (SSW) is investigated by nudging the zonal mean state of the stratosphere above 90 hPa toward the observation in the subseasonal-to-seasonal prediction models. Experiments with nudging toward the SSW event (NUDGED) simulate the downward propagation of the polar-cap geopotential anomalies and the negative phase of the North Atlantic Oscillation compared to those with nudging toward the climatology (CONTROL). By comparing these two experiments, the downward coupling mechanism of the SSW is investigated. In particular, the tropospheric geopotential anomalies, which can be decomposed into surface pressure and air temperature anomalies, are compared. It is found that the surface pressure change over the Arctic (60-90°N) primarily contributes to the tropospheric geopotential anomaly change, as in the observations. The surface pressure budget analysis further shows that the surface pressure increase over the Arctic primarily results from the poleward mass flux in the stratosphere and near the tropopause. While the poleward mass flux in the stratosphere results from the meridional circulation change due to the easterly winds in the NUDGED experiment, that near the tropopause is mainly driven by the momentum flux and zonal drag changes. This result highlights the importance of mass redistribution in the downward coupling of the SSW.
AS29-A025
Altitude-based Ozone Correlation Analysis in the Antarctic Region Using MERRA-2 Reanalysis Data
Hyeogdo KWEON1+, Ja-Ho KOO1#, Minju PARK1, Taejin CHOI2
1Yonsei University, Korea, South, 2Korea Polar Research Institute, Korea, South
The decrease in ozone concentration due to ozone depletion in the Antarctic stratosphere during the spring season has been a well-established phenomenon, confirmed through numerous studies. This allows increased levels of harmful ultraviolet radiation to reach the Earth's surface, posing potential consequences for human health, ecosystems, and materials. In this study, correlation analysis was conducted by calculating the mean values of ozone concentration data obtained from 8 Antarctic stations and temperature, potential vorticity, zonal and meridional wind speed data provided by MERRA-2 Reanalysis at 6 pressure levels (50, 100, 200, 300, 500, 850hPa). Utilizing altitude-specific ozone data enables a clearer confirmation of the mechanism in which ozone destruction intensifies with decreasing temperatures in the Antarctic stratosphere during the spring, revealing a more distinct positive correlation between ozone and temperature. Such correlation is not well manifested in the upper stratosphere and near the tropopause. The correlation between potential vorticity and ozone influencing the formation of the polar vortex during the Antarctic winter-spring season exhibits a strong negative correlation in the lower stratosphere. In the Dumont d’Urville station corresponding to the southeastern part of Antarctica, these characteristics are not observed, indicating that ozone depletion is skewed towards the northwest of Antarctica. Additionally, using the ozone mixing ratio data from MERRA-2 reanalysis, a distribution of correlation coefficients between ozone and meteorological parameters was created for the latitude range of 90˚S-50˚S over a period of 40 years (1980-2019), categorized by different pressure levels. Subsequently, with the obtained results, the focus turns to exploring spatiotemporal variations in the correlation between ozone and meteorological parameters across the entire Antarctic region. This work was supported by Korea Environment Industry&Technology Institute (KEITI) through "Climate Change R&D Project for New Climate Regime", funded by Korea Ministry of Environment (MOE) (2022003560006).
AS29-A027
Stratosphere-troposphere Exchange in Antarctic Springtime and Its Influence on Tropospheric Ozone
Minju PARK1#+, Sangjun KIM1, Ja-Ho KOO1, Taejin CHOI2
1Yonsei University, Korea, South, 2Korea Polar Research Institute, Korea, South
The Antarctic stratospheric ozone accounts for most of the ozone amount in the atmosphere, and there are seasonal changes according to the occurrence of ozone holes. The stratosphere-troposphere exchange (STE) indicates the result of the inflow of stratospheric ozone down the troposphere. This study calculated the tropopause heights using ozone amount from the ozone sonde data from eight Antarctic bases observed over more than five years and investigated the STE event frequency according to the season. The STE event frequency showed maximum at 55.1% in March, and decreased during the fall-winter period, showing an annual fluctuation at 22.3%, the lowest in August. Regional variations were not significantly different each other. The increase in tropospheric ozone was identified to recognize the STE events. The ozone peak, where increment was the largest, had a monthly average value around 5.8-6.5 km, and showed the lowest amount in August and the highest in March. The amount of ozone transported to the lower layer was 5.9×1017 in July and August and 9.7×1017 in February. Both the ozone peak and ozone flux results showed that the monthly average value changed every year. STE is known to be caused by global scale dynamics such as polar vortex or the Brewer-Dobson circulation. Complex chemistry reactions also are involved in stratospheric ozone's production and depletion. Based on the quantitative results using the high-resolution ozone sonde data, it is necessary to confirm the relationship between the polar climate and the amount of ozone in the future.This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (RS-2023-00219830). This work was supported by Korea Environment Industry&Technology Institute (KEITI) through "Climate Change R&D Project for New Climate Regime", funded by Korea Ministry of Environment (MOE) (2022003560006).
AS29-A035
Comparison of Trends and Distribution of Tropopause Folds in ERA5 and MERRA-2
Kai-Wei CHANG#+, Chia-Hui CHUNG
Chinese Culture University, Taiwan
Stratosphere-tropopause exchange (STE) impacts both stratospheric and tropospheric dynamics, as well as the chemical composition of both regions. As such, STE plays an integral role in the climate system, and improving our understanding of STE will help us address uncertainties in climate change and variability. Tropopause folds (TF) are the dominant mechanisms of STE. Recent research has shown that there exist significant climate trends in TF frequency, but the magnitude and sign of such trends vary with region. In this study, we report the trends and distributions of TF using ERA5 and MERRA-2 reanalyses from 1981-2022. Over East Asia during boreal winter, both reanalyses depict increasing trends over midlatitude East Asia and decreasing trends throughout the Pacific roughly along the latitude of the subtropical jet. In the southern hemisphere, both reanalyses show positive trends of TF occurrence off the west coast of South America, a hotspot of TF. Over the Southern Ocean, however, MERRA-2 suggests the existence of a positive trend while ERA5 does not. This study serves as a basis for understanding TF variations under climate change, and our future work will aim to attribute dynamical explanations to these trends and differences among reanalyses.
AS29-A037
Further Evidence of an Array of Atmospheric Global Free Modes
Takatoshi SAKAZAKI1#+, Michael SCHINDELEGGER2
1Kyoto University, Japan, 2University of Bonn, Germany
The atmosphere has normal mode (free) oscillations spanning a wide range of zonal wavenumbers and frequencies. Previous studies have extensively explored these normal mode oscillations, particularly Rossby modes, in the middle and upper atmosphere, where the amplitudes become large. On the other hand, due to their nearly barotropic nature, these normal mode oscillations distinctly manifest in variations of surface pressure as well. Sakazaki and Hamilton (2020), using surface pressure data from ERA5 reanalysis, demonstrated the existence of a large array of normal mode oscillations as short as 2 hr. One might wonder, however, how well the ERA5 represents realistic normal mode oscillations. That is, certain normal modes observed in ERA5 might be internally generated by the model, independent of realistic signals. In the present study, we use surface pressure data from worldwide meteorological stations and buoys during 1980-2021 to obtain further evidence of normal modes. We will show that at least for modes with a period <6 hr and a zonal wavenumber <5, remarkably similar signals are evident in both ERA5 and station/buoy data.
AS29-A040
Response of Stratospheric Ozone and Temperature to the 11-year Solar Cycle Signal
Yajuan LI1,2#+, Sandip DHOMSE3, Janchun BIAN2, Martyn CHIPPERFIELD3, Wuhu FENG3, Yuan XIA1, Yong YANG2
1Nanjing Xiaozhuang University, China, 2Chinese Academy of Sciences, China, 3University of Leeds, United Kingdom
Solar variability plays an important role in influencing the Earth's climate system. Accurate quantification of the response of stratospheric ozone and temperature to the 11-year solar cycle signal (SCS) is important in understanding global climate change. However, estimates of a realistic solar cycle signal are challenging due to their sensitivity to the quality of the observational datasets, the statistical methodologies as well as the non-linear coupling and complex changes in forcing processes. Here, we use the Microwave Limb Sounder (MLS) ozone profile measurements from 2005-2020 to estimate the 11-year SCS in stratospheric ozone. Additionally, we also analyse output from a chemical transport model (TOMCAT- CTM) simulation (forced with ECMWF ERA5 reanalysis) and the MERRA-2 Stratospheric Composition Reanalysis of Aura Microwave Limb Sounder (M2-SCREAM). We use multivariate linear regression (MLR) models based on ordinary least squares (OLS) and regularised (ridge) approach to estimate the ozone and temperature SCS. The regression coefficients from both OLS and ridge models, including the quasi-biennial oscillation, solar variability, El Niño-Southern Oscillation, Arctic oscillation, Antarctic oscillation, and Eliassen-Palm flux, represent the ozone and temperature variations associated with natural processes. We find that SCS derived using TOMCAT and M2-SCREAM data is consistent with MLS, except that TOMCAT overestimates the SCS in the lower stratosphere. There is an evident seasonal dependence in the ozone and temperature SCS profiles. Both OLS- and ridge-based ozone SCS show a double-peaked structure with primary peak near 5 hPa and secondary peak near 70 hPa. Ridge-based SCS yields smaller coefficients due to correlated explanatory variables. Significant differences between OLS- and ridge-based ozone SCS appear in the tropical mid-stratosphere and extra-tropics of the northern hemisphere, indicating how different settings in SCS using MLR models play a role in the appearance of the solar cycle response.
AS29-A041
PM 2.5 Observations of Outdoor and Indoor Environment at New Delhi, India: Impact of Hadley Cell Circulation During Winter in Northern Hemisphere
Shristy MALIK1#+, S. K. DHAKA2, A. S. RAO1
1Delhi Technological University, India, 2University of Delhi, India
During winter, convergence of air mass (Hadley cell) taking place in the northern India, thus showing a downward motion creating a condition of less dispersion of the pollutants. This is a large-scale downward circulation feature happening in addition to weak wind, low solar radiation, high relative humidity, and lower atmospheric boundary layer. Under these meteorological conditions year long observations of emission of PM2.5 both indoor and outdoor are carried out with a focus on understanding the winter period meteorology and impact of large scale circulation. Measurement is carried using a Compact and Useful PM2.5 Instrument (CUPI) from Nov 2018 to Oct 2019. A high-time resolution data (* 2 min interval) was recorded at New Delhi, India to investigate the difference between outdoor and indoor ambient particulate matter. Year-long observations provide an opportunity to decipher that indoor PM2.5 concentration increases significantly from mid-November 2018 to mid-December 2018. During this high concentration occurrence of PM2.5 , outdoor concentration was higher in the range of 100–200 micro g/m3 than indoor. Indoor pollution was less by 30–50% in comparison to the outdoor environment. Analyses reveal that during a high pollution period, intermittently for a short period, outdoor PM2.5 was less, which coincides with clear weather days suggesting that indoor pollution did not disperse due to a closed environment. Diurnal variation of PM2.5 clearly shows high concentration stays until 12:00 noon in both indoor and outdoor. Diurnal variation of solar radiation showed a consistent increase from 9 am to 2 pm, while relative humidity declined considerably from 10 am to 4 pm (local time); these two factors correspond to less concentration in both indoor and outdoor environments. However, there is no significant difference between outdoor and indoor concentration during summer and monsoon season as upward motion is evident using ERA-5 reanalysis data.
AS35-A006
Changes in the Intraseasonal Variability of East Asian Jet Streams
Yaocun ZHANG#+
Nanjing University, China
The East Asian jet stream is an important component of mid-high latitude circulation systems, and its intraseasonal oscillation plays a crucial role in the formation and development of persistent climate anomalies and extreme events over East Asia-Pacific region. This study examines the changes in the intraseasonal variability (ISV) of the East Asian jet streams using the reanalysis datasets. It is found that the zonal winds over East Asia show notable ISV with a significant period of 10–25 days. The variance of 10–25-day filtered East Asian zonal winds exhibits a significant decrease around 2000, which is mainly contributed by the weakened ISV the East Asian polar-front jet (EAPJ). Further analysis reveals that the EAPJ experienced remarkable ISV changes in both intensity and location. Along with the ISV increase (decrease) of EAPJ intensity (location), the dominant mode of EAPJ intraseasonal variation has changed from its intensity change to position shift since the year 2000. Therefore, The EAPJ plays a major role for the interdecadal transition in ISV of East Asian zonal wind. The ISV changes and mode transition of EAPJ are closely associated with the modulation of lower-level large-scale circulation over Eurasia. The intraseasonal temperature gradient patterns display ISV changes parallel to those of EAPJ around 2000, indicating that the thermal anomalies are effective in leading to corresponding intensity and location variations of EAPJ via thermal wind relationship.
AS35-A009
Unraveling the Impact of External Forcing and Internal Variability on Dust Storm Frequency Reduction in Northwest China
Mengxi QI#+, Ruiqiang DING
Beijing Normal University, China
In this research, we initially examined the key atmospheric circulation pattern influencing the occurrence of dust storms in Northwest China during spring (February-May). We then investigated the drivers impacting atmospheric circulation over the Mongolian Plateau and southern Central Siberia (MPSCS), using NCEP/NCAR reanalysis data and extensive ensemble simulations, and assessed the respective roles of external forces and internal variability. Our results validated a significant inverse correlation between the reduced frequency of spring dust storms in Northwest China post-mid-1980s and heightened geopotential height anomalies over the MPSCS. By scrutinizing five comprehensive ensemble model simulations, we demonstrated that the positive tendencies in atmospheric circulation anomalies over the MPSCS are largely triggered by external forces, accounting for roughly 69.3% of the observed augmentations in the Atmospheric Circulation Index (ACI) trend from 1954 to 2022. Although the North Atlantic Oscillation (NAO) is a leading mode of internal variability associated with geopotential height anomalies over the MPCMS, its contribution is comparatively minor. Our findings underline that the primary cause of the decrease in dust storm frequency in Northwest China since the mid-1980s could be ascribed to global warming-related external forces.
AS35-A014
Influence of the Quasi-Biennial Oscillation on the Spatial Structure of the Wintertime Arctic Oscillation
Cai QINGYU#+
Yunnan University, China
This study reveals that the Quasi-Biennial Oscillation (QBO) has a marked impact on the spatial structure of the Arctic Oscillation (AO) in boreal winter. In particular, the North Pacific center (NPC) of the AO is stronger during the westerly phase of the QBO (WQBO) than the easterly phase of the QBO (EQBO). In other words, the variability associated with the AO over the North Pacific is stronger in WQBO years than EQBO years, even though the overall variability is insensitive to QBO phase. The QBO is suggested to influence the spatial pattern of the winter AO mainly via modulating the intensity of the stratospheric polar vortex, with a stronger stratospheric polar vortex during WQBO than EQBO years. A stronger stratospheric polar vortex can lead to more planetary wave refraction and facilitate the eastward propagation of wave activity flux from the mid-latitude North Pacific to the North Atlantic. Thus an enhanced connection between North Pacific and North Atlantic atmospheric variability is established, and a more prominent NPC of the AO occurs in WQBO years. In addition, the modulation of the AO structure by the QBO and the associated physical process is supported by output from the CNRM-CM6-1 model. Our results indicate that, for seasonal climate prediction in North America based on the AO, WQBO leads to a larger predictable signal while EQBO leads to reduced skill.
AS35-A017
Alternation of the Atmospheric Teleconnections Associated with the Northeast China Spring Rainfall During Recent 60 Years
Zhiwei ZHU#+, Rui LU, Shanshan FU
Nanjing University of Information Science & Technology, China
Northeast China (NEC) is the national grain production base of China, and the local precipitation is vital for agriculture during the springtime. Therefore, understanding the dynamic origins of the NEC spring rainfall (NECSR) variability is of socioeconomic importance. This study investigates the interannual variability of NECSR and reveals an interdecadal shift in the interannual atmospheric teleconnections associated with the NECSR during recent 60 years (1961-2020). The interannual variability of NECSR is mainly modulated by the mid-latitude wave train over Eurasia continent which is associated with the tropical North Atlantic sea surface temperature anomaly (SSTA). This relationship undergone an interdecadal shift during mid-1980s. Before the mid-1980s, the NECSR is related to the Rossby wave train which is coupled with extratropical North Atlantic SSTA, whereas it is linked to a quite different Rossby wave train that coupled with tropical North Atlantic SSTA after then. Both Rossby wave trains could lead to the enhanced NECSR through the anomalous cyclones over East Asia. The weakening of the westerly jet over around North America is mainly responsible for alternation of the atmospheric teleconnections towards NECSR during two epochs.
AS35-A023
Distinct Prediction Skill of the Northern Hemispheric Wintertime Surface Air Temperature Dependent on the QBO Phase
Tian WAN#+
Chinese Academy of Sciences, China
The Quasi-Biennial Oscillation (QBO) is one of the main climate systems in the equatorial stratosphere. Due to its quasi-periodical feature, many studies have investigated its predictability in different forecast systems. However, the predictability of QBO influencing surface climate is still unclear. In this study, the predictability of QBO influencing the boreal winter surface air temperature (SAT) has been verified by using the 36-year hindcasts monthly data from the fifth-generation seasonal forecast system of the European Center for Medium Weather Forecast (SEAS5). The anomaly correlation coefficient (ACC) then becomes to estimate its forecast skill which shows positive over Eurasia in QBO westerly phase (WQBO) while shows significant negative in QBO easterly phase (EQBO). This ACC difference in QBO is linked with the bias between predicted and observed stratospheric polar vortex (SPV), named as predicted error of SPV. During EQBO category, the error is greatly obvious to represent a more strengthened polar vortex than in WQBO, which can further propagate downward to lower troposphere due to enhanced stratosphere-troposphere coupling. As a result, SAT predicted error would correspondingly grow in the Eurasian continent during EQBO. Our study shows that SPV is an important factor in influencing the predictability of QBO modulating surface climate in winter, and can provide potential insight for improving the wintertime SAT forecast in SEAS5.
AS35-A027
Subseasonal to Seasonal Forecast Using Neural Ordinary Differential Equations
Jonghan LEE#+, Woosok MOON
Pukyong National University, Korea, South
This research emphasizes the critical importance of predictions in the face of escalating impacts caused by human-induced greenhouse gas emissions, which contribute significantly to global warming and a subsequent surge in extreme weather phenomena. Since the late 19th century, there has been a substantial rise in Earth's surface temperature, with recent decades experiencing unprecedented warming rates. This change has precipitated a rise in the frequency and intensity of floods, typhoons, and heatwaves, signaling an urgent need for accurate meteorological and climatic predictions. While short-term weather forecasting has benefited from extensive data and research, leading to high predictive accuracy, long-term forecasts, particularly medium-range predictions, lag significantly due to data scarcity. This research aims to bridge this gap by leveraging the advancements in Artificial Intelligence (AI), particularly Deep Learning. We propose a novel approach using Neural Ordinary Differential Equations (Neural ODEs), which represents a transformative step in dynamic systems modeling. Neural ODEs offer a flexible and powerful framework for continuous-time models, which is particularly beneficial for handling sparse or irregularly sampled data prevalent in climate studies. Our methodology utilizes the Empirical Orthogonal Function (EOF) to extract principal component time series from limited climate data. These components serve as inputs for Neural ODEs to predict future climatic conditions. This approach is innovative in its ability to handle non-linearities and temporal dependencies in climatic data, making it highly suitable for medium-range weather forecasting. The potential of Neural ODEs in this context is significant, as they provide a means to accurately predict weather patterns with less data, a common limitation in long-term forecasting. By enhancing the precision of medium-range forecasts, this research contributes to more effective climate change adaptation and mitigation strategies, ultimately aiding in the safeguarding of ecosystems and human societies against the adverse effects of extreme weather conditions.
AS35-A028
Observing the Impact of the Eddy Flux Near the Hadley Cell Edge on the Cell Characteristics During JJA and DJF Seasons in Reanalysis Data
Seungpyo LEE#+, Woosok MOON
Pukyong National University, Korea, South
At the poleward edge of the Hadley Cell, descending air masses lead to the formation of high-pressure systems at the surface, significantly influencing tropical and mid-latitude weather patterns. In subtropical regions, the high-pressure systems maintain continental areas with high temperatures and dry conditions, resulting in the formation of deserts. In mid-latitude regions, the interaction of descending cold air from the polar region to the high-pressure system forms a stationary front, triggering the onset of monsoons. Therefore, the Hadley Cell not only regulates local weather but also contributes to extreme climates and weather phenomena. Recent climate models and reanalysis data indicate that during ongoing global warming, the poleward edge of the Hadley Cell is expanding and the intensity of the Hadley Cell is weakening. This suggests a potential shift of tropical and mid-latitude weather characteristics towards higher latitudes, leading to drastic environmental changes in regions, such as expanded deserts or altered monsoon patterns. Furthermore, the movement of the Hadley Cell may pose challenges in predicting local weather conditions, Eventually, it is impact on the human habitation areas. Therefore, sophisticated understanding of the mechanisms determining the characteristics of the Hadley Cell is crucial. This study aims to investigate the impact of energy flux exchanges between the Hadley Cell and mid-latitude (or equatorial) regions, focusing on the Hadley Cell edge surroundings. We utilize JRA55 reanalysis data and ICOADS observational data from 1979 to 2022 to observe changes in the Hadley Cell induced by global warming, focused on summer (JJA) and winter (DJF). Building upon the zonal symmetric theory of understanding the Hadley Cell, the study predominantly observes changes in Hadley Cell characteristics in accordance with eddy heat flux and eddy momentum flux. This research will ultimately provide deeper insights into the changes in the Hadley Cell induced by global warming.
AS35-A030
Connection of Summer Surface Temperature Anomalies Between the East European Plain–west Siberian Plain and North America on the Interannual Timescale
Chenyu LV+, Riyu LU#, Wei CHEN
Chinese Academy of Sciences, China
This study identifies a significantly positive relationship between summer surface air temperature (SAT) anomalies over two remote regions in the Eurasian continent and North America during the period 1979–2021 on the interannual timescale. The former region includes the East European Plain and the West Siberian Plain, and the latter region includes the central and eastern North America. The regional-averaged summer SAT anomalies show a correlation coefficient of 0.66 between these two regions, which is significant at the 99% confidence level. This intercontinental SAT relationship can be explained by a wave-like pattern of circulation anomalies, which is the leading mode of upper-tropospheric circulation anomalies over the middle and high latitudes of the Northern Hemisphere in summer. Further analysis suggests that the sea surface temperature (SST) anomalies over the Pacific and North Atlantic in the preceding spring, being coupled with the leading mode of atmospheric circulation anomalies over the Pacific–Atlantic sector, persist into summer and affect the SATs in the two remote regions, resulting in the intercontinental SAT connection.
AS35-A031
Enhanced Teleconnection Between Atlantic Multidecadal Variability and the Kuroshio-Oyashio Extension Decadal Variability Under Global Warming
Shujun LI#+, Yiting WANG
Ocean University of China, China
The Atlantic Multidecadal Variability (AMV), an inter-hemisphere alternating natural mode of sea surface temperature in the Atlantic basin, modulates the North Pacific climate variability through atmospheric teleconnections. However, the AMV-related teleconnection is not stationary and is projected to change under global warming, which remains unclear. By analyzing future climate under different emission scenarios simulated by the Coupled Model Intercomparison Project phase 6, we show an enhanced teleconnection between AMV and the decadal variability in the Kuroshio–Oyashio Extension (KOE) under global warming. The increased variability of AMV produce stronger atmospheric remote forcings, leading to expanded anomalous high pressure in the Aleutian Low, which leads to stronger Ekman convergence and increased decadal variability in the KOE region. Our results indicate the remote forcings of AMV may become increasingly important in determining the KOE variability in the future, whereas the weakened Pacific Decadal Oscillation and increased ocean stratification plays a weakening effect.
AS35-A037
Physical Mechanism of the Rapid Increase in Extremely Intense and Long-lived Heatwaves in the Northern Hemisphere Since 1980
Yuqing WANG1+, Wen ZHOU1#, Chunzai WANG2
1Fudan University, China, 2Chinese Academy of Sciences, China
Since 1980, both the intensity and duration of summer heatwaves in the middle and high latitudes of the Northern Hemisphere have significantly increased, leading this region to become a critical area for the significant increase in frequency of extremely intense and long-lived heatwaves. We find that stronger and more persistent high-pressure systems and lower soil moisture before the events are the main drivers of the extremely intense and long-lived heatwaves in the Western Europe and the mid-high latitudes of North America. In Eastern Europe and Siberia, in addition to the above drivers, lower cloud cover before the event is also one of the important drivers for the occurrence of such extreme heatwave events. These factors can change heatwave intensity and duration by influencing surface radiation processes during the event. Using the Self-organizing Maps classification method, we find that the increases in frequency, intensity, and duration of six weather patterns are the main dynamic reasons leading to the increase in extremely intense and long-lived heatwaves after 1980. In addition, the decrease in summer average soil moisture in most region of the middle and high latitudes and the decrease of the summer average cloud cover in Eastern Europe and Siberia are found to be the main thermodynamic reasons leading to the increase in such extreme heatwaves.
AS35-A044
The Impacts of East Siberian Blocking on the Development of the JPCZ
Akira YAMAZAKI1#+, Shin FUKUI2, Shiori SUGIMOTO1
1Japan Agency for Marine-Earth Science and Technology, Japan, 2Japan Meteorological Agency, Japan
Ensemble dynamical downscaling experiments were performed to investigate the influence of East Siberian blocking on a heavy snowfall event that occurred over Fukui City, Japan, in early February 2018 and was associated with the development of the Japan Sea Polar airmass Convergence Zone (JPCZ). The downscaling experiments simulated the enhancement of the East Asian cold air stream and its flow along two routes: the western route, which runs from the Eurasian Continent via the Yellow Sea and the Korean Peninsula; and the northern route, which originates in the Sea of Okhotsk and runs via the northern Japan Sea. As a result, the location and strength of the simulated JPCZ in the downscaling experiments are consistent with those in the Japanese regional reanalysis dataset. For the sensitivity experiments, the blocking that develops over East Siberia just prior to the formation of the JPCZ was removed, and the results indicate that the East Siberian blocking contributes significantly to JPCZ development by enhancing the East Asian cold air stream along the western route. Additional data analyses based on the 20-year reanalysis revealed that East Siberian blocking can enhance both the western and northern routes of the cold air streams.
AS35-A046
The Role of the Meridional Rossby Wave for Extreme Heatwaves Over East Asia
El NOH1+, Joowan KIM1#, Sang-Yoon JUN2
1Kongju National University, Korea, South, 2Korea Polar Research Institute, Korea, South
The North Pacific High is a dominant lower troposphere pressure-system that governs the weather in the East Asian region during the summer, and its western boundary serves as a waveguide for the propagation of Rossby waves from the equatorial to mid-latitudes. The deep convection forcing in the equatorial western Pacific usually creates Rossby waves that propagate northward along this waveguide. This meridional Rossby wave, known as the Pacific-Japan (PJ) pattern, is the dominant teleconnection pattern in the vicinity of East Asia, and it often accompanies extreme weather as Heatwaves. In this study, the circulation and thermodynamic characteristics of the PJ pattern were investigated based on a daily timescale to better understand their relationship with the likelihood of heatwaves in East Asia. According to thermodynamic budget calculations, horizontal heat advection crossing the climatological flow pattern is the key factor for the observed surface air warming. In addition, CMIP6 models also effectively simulate the meridional Rossby waves in the East Asian region, and as a result, they represent the warming phenomena in East Asia. The overall findings of this study provide valuable insights into the development mechanisms of heatwaves on an intraseasonal timescale.
AS36-A002
Development and Application of 1-KM Grid Square Meteorological Data Including Forecast Values
Kaori SASAKI#+
National Agriculture and Food Research Organization, Japan
The Agro-Meteorological Grid Square Data System (AMGSDS) was developed to apply meteorological data to agricultural operations such as planting, cultivation, pesticides, and weeding. The AMGSDS produces and serves daily gridded meteorological data with a spatial resolution of approximately 1-km, using a statistical downscaling method. Observed, forecast, and climatic normal data are seamlessly linked. The dataset covers from 1980 (or 2008) to the next year and is updated every morning based on the latest weather forecasts provided by the Japan Meteorological Agency (JMA). For the past, we use the observed data from The Automated Meteorological Data Acquisition System (AMeDAS). For today and for up to 26 days ahead, we use the forecast data. After 27 days ahead, we use daily climatic normal values. The AMGSDS provides daily data for 14 elements, including daily mean air temperature, daily precipitation, daily mean relative humidity, daily global solar radiation, daily atmospheric radiation, and snow water equivalent. Additionally, the AMGSDS provides hourly data for 3 elements, temperature, relative humidity, and atmospheric radiation. The AMGSDS delivers the data for any spatiotemporal range via the internet on demand, using MS Excel query, programming languages, and mobile apps through the unique deliver system that allows registered users. It will be a powerful tool for the agricultural sector, for example, in decision support systems to reduce weather and climate risks in field crop production.
AS36-A003
Assessing the Potential of Facebook Prophet and Neural Prophet Models in Predicting Equatorial Ionospheric foF2
Sherin BABU1#, Tiju JOSEPH MATHEW2+, Binu THOMAS3,4
1Assumption College Autonomous, India, 2Christian College, India, 3Marian College Kuttikkanam, India, 4Mahatma Gandhi University, India
To understand how ionospheric variation affects high-frequency communication and the global positioning system, accurate prediction of the ionospheric F2 layer critical frequency (foF2) is crucial. This work describes the machine learning based time series forecasting methods namely Facebook Prophet and Neural Prophet, used to forecast daily hourly foF2 values of the ionosphere over the equatorial station Boa Vista, Brazil (2.8° N, 66.7°W). The ionospheric foF2 data obtained from the Digital Ionosonde in Boa Vista during the year 2014 is used to train and test the proposed methods. The performances of the models are evaluated using the mean absolute error (MAE), coefficient of determination (R2), and root mean square error (RMSE) measures. Though both models produce outcomes that are comparable, Neural Prophet offers more accuracy. Neural Prophet's predictions are slightly reliable than Facebook Prophet's.
AS36-A005
Observational Constraints on CMIP6 Models Reveal a Sudden Intensification of Earth's Energy Imbalance Since Late 20th Century
Xuqian LI#+, Qingxiang LI
Sun Yat-sen University, China
Tracking the energy balance of the Earth system is a key method for studying the contribution of human activities to climate change. However, accurately estimating the surface energy balance has long been a challenge, primarily due to uncertainties that dwarf the energy flux changes induced by greenhouse gases and a lack of precise observational data at the surface. We have employed the Bayesian Model Averaging (BMA) method, integrating it with recent developments in surface solar radiation observational data, to refine the ensemble of CMIP6 model outputs. This has resulted in an enhanced estimation of Earth System Energy Imbalance (EEI) changes since the late 19th century. Our findings show that CMIP6 model outputs, constrained by this observational data, reflect changes in energy imbalance consistent with observations in Ocean Heat Content (OHC) and Sea Level Height (SLH), offering a narrower uncertainty range at the 95% confidence level than previous estimates. Observing the EEI series, dominated by changes due to external forcing, we note a relative stability (0.37W/m2) over the past half-century, with a significant intensification (reaching 0.85 W/m2) in the mid to late 1990s, indicating an increased risk of global warming.
AS36-A007
Real-time Measurement of Cloud Heights and Optical Thicknesses for the Efficiency of Solar Panel and Virtual Power Plant by Using LiDAR System
Chih-Wei CHIANG#+
Kun Shan University, Taiwan
At present, the green energy is actively developing intelligent grid. It is expected that through the energy storage system, the renewable energy can be incorporated into the normal power supply and operation with maximum utilization efficiency, which will not only save electricity costs but also reduce carbon emissions. However, the variability and uncertainty of solar energy generation is influenced by solar power cannot accurately assess and predict, when it is integrated into the intelligent grid, it will easily cause voltage fluctuations and affect the stability of the regional power grid. Therefore, the main purpose of this research is attempting to use the advanced LiDAR technology to perform cloud coverage, cloud track, and cloud optical thickness, etc., to evaluate and predict the illuminance of sunlight, instead of the traditional passive illuminance measurement based on automated, intelligent, networked and systematic monitoring to facilitate the intelligent grid system.
AS36-A013
Current Practices and Challenges in Managing Automated Weather Station Data and Networks in Philippine Cities
Erica BAÑARES1#+, Paola Angela BAÑAGA1, Emilio GOZO1, Genevieve Rose LORENZO2, Xzann Garry Vincent TOPACIO3, Alyssa Gewell LLORIN4, Faye Abigail CRUZ1, James Bernard SIMPAS1,5, Sherdon Niño UY1, Francia AVILA1, Jose Ramon VILLARIN1
1Manila Observatory, Philippines, 2University of Arizona, United States, 3Kyushu University, Japan, Japan, 4University of Tsukuba, Japan, 5Ateneo de Manila University, Philippines
Automated weather station (AWS) data is essential in weather and climate monitoring, research, and forecasting, especially in cities. This research provides a comprehensive overview of the Manila Observatory AWS network across four cities in the Philippines: Metro Manila, Cagayan de Oro City, Iloilo City, and Davao City, emphasizing its data management and network operations. The protocols and management system used to regularly monitor and maintain the AWS network, including data collection, archiving and quality control procedures, will be discussed, as well as the challenges and considerations involved in managing the weather station network in urban areas. The data portal through which the weather data can be viewed and disseminated will also be presented. The study emphasizes the importance of AWS networks in providing accurate and timely weather data, which can facilitate broader academic and sector-specific research, enhance well-informed decision-making, and improve the efficiency of disaster response and management. In addition, this study highlights the collaboration between academe/research institutes, private sectors and local government units, showcasing an initiative that offers a sustainable approach for the continuous operation of AWS networks that can be adopted by other cities in developing countries.
AS36-A018
Advancing Accuracy Via Calibration Models: Microsensor Data with AS-LUNG Network Calibrated
Yu Ju LIN1#+, Wei Lun HSU1, Yu-Ting ZENG1, Shih-Chun Candice LUNG2, Chih-Da WU1
1National Cheng Kung University, Taiwan, 2Academia Sinica, Taiwan
In recent years, the precision of air pollution prediction has risen in significance, essential for informed policymaking to elevate environmental standards. However, the growing use of low-cost sensors (LCSs) for air monitoring often lacks essential calibrations. AS-LUNG sensors, acknowledged for their research-grade accuracy, undergo meticulous calibration through correction equations derived from comparative analyses with the high-precision instrument GRIMM 1.109 in controlled laboratory settings. The microsensors collected through Civic IoT Taiwan are also a form of LCSs. The cost-effectiveness of microsensors allows their widespread deployment in densely populated areas. Despite their high numbers, they often lack proper calibration. AS-LUNG sensors, renowned for their research-grade accuracy, undergo meticulous calibration through correction equations derived from comparative analyses with the high-precision instrument GRIMM 1.109 in controlled laboratory settings. This study, centered on Taichung City, harnesses data from over 1,000 microsensors to forecast PM2.5 levels. The microsensor data undergoes rigorous calibration using AS-LUNG, resulting in 2,369,716 hourly data points. This dataset forms a robust basis for refining models and calibrating AS-LUNG sensors, significantly enhancing their accuracy. Post-AS-LUNG model calibration analysis showcases substantial accuracy improvements. Rigorous validation, employing both 10-fold cross-validation and overfitting tests, consistently demonstrates comparable performance to the primary model. Particularly noteworthy is the exceptional performance of the training set, achieving an R2 of 0.87. This pioneering study rectifies the oversight of uncalibrated LCSs in regions lacking monitoring stations, validated through laboratory-calibrated data. The potential replication of similar models in other countries holds promise for bolstering PM2.5 sensor networks, amplifying global environmental monitoring capabilities.
AS36-A028
Analysis of Rainfall-runoff Extremes Using WRF-Hydro Driven by Radar Precipitation
Jian-Jun LIU#+, Chia-Jeng CHEN
National Chung Hsing University, Taiwan
Remotely sensed precipitation data, such as radar precipitation, have been utilized in various hydrologic applications in recent years. In Taiwan, the Quantitative Precipitation Estimation and Segregation Using Multiple Sensors (QPESUMS) data, known for its high spatiotemporal resolution(1 km and 10 min), provides more accurate precipitation estimates, thus demonstrating its importance in improving hydro-meteorological modeling and prediction. This study aims to use the QPESUMS data to drive the Weather Research and Forecasting-Hydrological modeling system (WRF-Hydro) model to simulate the Typhoon Morakot event that influence southern Taiwan. WRF-Hydro, an extension of the hydrological modeling component residing in WRF, has been successfully used for assessing regional hydrological budgets and land-atmospheric interactions. A systematic approach will be adopted to calibrate various parameters in WRF-Hydro driven by the QPESUMS data to enhance simulation accuracy. The more accurate rainfall-runoff simulation shall yield potential improvement in successive flood prediction, which will be an ongoing task based on a two-dimensional flood model.
AS43-A010
S2S Predictability of Sub-summer Western North Pacific Subtropical High
Jung-Eun KIM#+
Ewha Womans University, Korea, South
Recent study has reported that the strong lagged relationship between the late-summer western North Pacific subtropical high (WNPSH) and the previous ENSO has been substantially weakened in the recent decades. Reversely, the WNPSH-ENSO connection during early summer has become pronounced over the decades. It is related to the different evolutions of local and tropical SST anomalies from winter to summer, which depend on the dominant type of the ENSO in the past and recent decades, and the corresponding changes in variabilities and mechanisms of the sub-summer WNPSH. Such change would also influence the S2S predictability of the WNPSH. In this study, we perform the hindcast experiment for the years of 1980-2020 using the atmosphere-only version of the global circulation model. The influence on S2S predictability of the WNPSH due to the change in the WNPSH-ENSO connection will be investigated.
AS43-A013
Does the Madden-Julian Oscillation Contribute to Subseasonal Rainfall Forecasting Skill Over Southeast Asia?
Chen SCHWARTZ#+, Thea TURKINGTON
Centre for Climate Research Singapore, Singapore
The Madden-Julian Oscillation is the dominant source of rainfall variability in the tropics on subseasonal timescales. As such, the MJO plays a significant role in forecasting tropical rainfall on 2-3 weeks timescales, and previous studies have shown an improvement in extreme rainfall prediction skill when an MJO event was present. During boreal winter, certain regions in Southeast Asia (SEA) are greatly affected by intraseasonal rainfall variability associated with the MJO, and improvement of subseasonal prediction skill of MJO-related rainfall could benefit both stakeholders and the vast population in the region. In this work, we first assess the observed over different sub-regions in SEA. Then, the ECMWF extended range model is used to assess whether the MJO actually contributes to forecasting skill of subseasonal rainfall over these sub-regions. Specifically, the forecasting skill of rainfall is examined for the different sub-regions during weeks when MJO phases that are associated with wetter conditions are dominant versus weeks when MJO phases with little to no effect are present.
AS43-A014
Development of the Signal-to-noise Paradox in Subseasonal Forecasting Models: After How Long? Where? Why?
Chaim GARFINKEL1#, Chen SCHWARTZ2+, Amy BUTLER3, Daniela I.V. DOMEISEN4, Judah L. COHEN5, Wen CHEN6, Zachary LAWRENCE3, Jeff KNIGHT7
1Hebrew University of Jerusalem, Israel, 2Centre for Climate Research Singapore, Singapore, 3National Oceanic and Atmospheric Administration, United States, 4ETH Zurich, Switzerland, 5Atmospheric and Environmental Research, United States, 6Yunnan University, China, 7Met Office Hadley Centre, United Kingdom
Subseasonal forecast models are shown to suffer from the same inconsistency found in climate models between the low strength of predictable signals and the relatively high level of agreement they exhibit with observed variability of the atmospheric circulation. That is, subseasonal forecast models show higher correlation with observed variability than with their own simulations, i.e., the signal-to-noise paradox. Also similar to climate models, this paradox is particularly evident in the North Atlantic sector. The paradox is not evident in week 1 or week 2 forecasts, and hence is limited to subseasonal timescales. The paradox appears to be related to overly fast decay of Northern Annular Mode regimes. Three possible causes of this overly fast decay and for the paradox in the Northern Hemisphere are identified: a too-fast decay of polar stratospheric signals, overly weak downward coupling from the stratosphere to the surface (in some models), and overly weak transient synoptic eddy feedbacks. While the paradox is clearly evident in the North Atlantic, things are qualitatively different in the Southern Hemisphere: Southern Annular Mode regimes persist realistically, the stratospheric signal is well maintained, and eddy feedback is, if anything, too strong and zonal.
AS43-A018
Enhancing of Subseasonal to Seasonal Forecast with Integrated Attention Mechanisms in U-Net Models
Uran CHUNG#+, Seongkyu LEE, Soo-Jin SOHN
APEC Climate Center, Korea, South
As the importance of highly accurate sub-seasonal to seasonal forecast data is increasing in the various industries in a climate crisis, this study was carried out a focus on strengthening the U-Net model. We applied Attention and Residual mechanisms to improve the extended U-Net model's accuracy in predicting Sub-seasonal to Seasonal (S2S) climate variables like daily maximum air temperature and daily total precipitation. The different versions of extended U-Net models were constructed incorporating these mechanisms separately and in combination, along with grid search algorithms to optimize hyperparameters of U-Net. The findings indicated in that models applied Attention or Residual mechanisms showed improved accuracy in predicting daily maximum air temperature and daily total precipitation than not applied additional mechanisms, with the Attention-based-on-Residual U-Net performing is the best. However, challenges persisted in improving 1-2 week (e.g., within 10 days) daily maximum temperature and 3-4 week (e.g., after 14 days) precipitation predictions. Future research aims to explore ensemble techniques and specialized approaches from the extended U-Net models.
AS43-A023
Development Status and Predictability of KIM-based Extended-medium Range Prediction System
Taehyoun SHIM#+, Shin-Woo KIM, Ja-Young HONG, Hye-Jin PARK, Kyung-Hee SEOL
Korea Institute of Atmospheric Prediction Systems, Korea, South
This study aims to introduce the development status and present the prediction performance of the Korean numerical weather prediction model (KIM) in relation to the extended medium-range prediction system, which is an important component of the Ensemble Prediction Systems (EPS) that KIAPS will develop in the future. KIM has been developed as the Korea Meteorological Administration’s (KMA) operational numerical weather prediction (NWP) system by the Korea Institute of Atmospheric Prediction Systems (KIAPS). KIM is a newly introduced global atmospheric model system, consisting of a spectral-element non-hydrostatic dynamical core on a cubed sphere grid and an advanced physics parameterization. One of the main goals of KIAPS is to build an ensemble-based forecast system with the coupled modeling system to improve the prediction skill of extended-medium range forecasts up to 30 days (about 4 weeks). Therefore, it is necessary to produce extended-medium range reforecast data to understand climatological characteristics and model bias, and ascertain predictability. To this end, KIAPS is building reforecast system for extended-medium range prediction and producing hindcast data for a specific period. We utilize the KIM-based reforecast system to perform hindcast simulations for the cold season cases for the period of 2001 - 2020 (20 years). The diagnosis and verification of the KIM’s reforecast were compared with the reanalysis data (ERA5). To evaluate the performance of KIM for the extended-medium range, various skill scores such as RMSE, ACC, MSSS, ROC, and CRPS are calculated. These multi-year simulations, such as reforecasts, are expected to contribute to improving the extended-medium range predictability of KIM.
AS43-A025
Estimating the Local Predictability of the January 2021 Sudden Stratospheric Warming Using a Novel Nonlinear Method
Guiping ZHANG1+, Xuan LI2#, Xin ZHOU1
1Chengdu University of Information Technology, China, 2Northwestern Polytechnical University, China
A major sudden stratospheric warming (SSW) occurred in the Northern Hemisphere in January 2021, which caused extreme cold events with record-breaking cold temperatures across East Asia and North America. A better understanding of the SSW predictability for an improved surface seasonal to subseasonal (S2S) forecast is a pressing issue. Here we quantify the local predictability limit of the 2021 SSW event within ERA5 reanalysis data and subseasonal to seasonal (S2S) reforecasts. A novel nonlinear method, Backward Searching for the Initial Condition (BaSIC), is used to estimate the local predictability of the SSW. This method is advanced because the nature of SSW is a chaotic system with intrinsic properties, making it difficult to measure its predictability with traditional linear methods. The local predictability limit of this 2021 SSW event is estimated to be 14 days using BaSIC method. We also trace the sources of forecast errors of this SSW. In the beginning, the overall forecast errors were relatively small, but with the increase of time, errors increased more in the high altitudes over Northern North Atlantic and Northern Eurasia. This indicates that the forecast errors in the 2021 SSW event mainly originate from the high altitude at these places.
AS43-A028
Sub-seasonal Prediction Skill: Is the Mean State a Good Model Evaluation Metric?
Jihun RYU1+, Jinho YOON1#, S. Y. Simon WANG2, Jee-Hoon JEONG3
1Gwangju Institute of Science and Technology, Korea, South, 2Utah State University, United States, 3Chonnam National University, Korea, South
The evaluation of forecast models involves assessing their accuracy in representing observed climate states and predicting future climate variables. Several evaluation methods have been developed, ranging from computationally efficient measures such as the anomaly correlation coefficient to more complex approaches. Although simpler methods may provide limited information, climatology is a commonly used primary evaluation metric due to its simplicity and immediate linkage to model performance. This study focuses on temperature and precipitation, proposing a new metric that integrates climatology and the seasonal cycle for a more accurate assessment of the relationship between mean state performance and predictability on weather and sub-seasonal time scales. This metric shows a strong correlation between temperature and precipitation in various geographical locations, with a more significant effect in tropical areas when considering the seasonal cycle. Temperature also demonstrates higher predictability and a more pronounced relationship compared to precipitation. The relationship discovered serves as an early indicator for predicting the efficacy of S2S models. This offers valuable insights for model development and emphasizes the significance of this integrated metric in enhancing S2S model performance and advancing climate prediction capabilities.
AS46-A008
A Numerical Study of an Afternoon Convection Case in Taiwan Under Weak Synoptic Forcing
Shin-Hau CHEN#+, Chung-Chieh WANG
National Taiwan Normal University, Taiwan
Afternoon convection, a prevalent meteorological phenomenon in Taiwan during the summer. In this research, the Cloud-Resolving Storm Simulator (CReSS) from Nagoya University is employed to investigate a representative case on 18 August 2009, illustrating the typical characteristics of afternoon convection. Both observational data and simulation results reveal that several convergence zones along the mountain ridge in Taiwan, induced by solar heating, play a pivotal role in initiating mountain convection. The sea-breeze (onshore-wind) generated by differential heating between land and sea establishes a transition zone in wind speed, referred to as the sea-breeze front, across the Jianan Plain. The eastward movement and intensification of the sea-breeze front contribute to the initiation of convection over the plain area. The entire convective system comprises numerous meso-γ-scale convective cells, each persisting for approximately an hour. The lifecycle of these cells, encompassing their formation, splitting, and merging, spans up to three hours. This study offers a comprehensive analysis of the mechanisms governing afternoon convection in Taiwan under weak synoptic forcing.
AS46-A012
Optimizing Combination of Different Disdrometer Data for Complete Drop Size Distributions
Sanghun LIM1+, Wonbae BANG1,2, Kyuhee SHIN1, Kwonil KIM3, Viswanathan BRINGI4, Merhala THURAI4, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Center for Atmospheric REmote sensing, Kyungpook National University, Korea, South, 3Stony Brook University, United States, 4Colorado State University, United States
Mesurement of accurate Drop Size Distribution (DSD) is very important because DSD is used to understand microphysical characteristics of rain events such as collision–coalescence, break-up, and evaporation.. However, disdrometer have different advantages and disadvantages. For example, 2D-Video Distrometer (2DVD) Meteorological Particle Spectrometer (MPS) have higher performance for measurement of size and concentration of large (small) raindrops. Against the issue, recent studies have tried to combine DSD between 2DVD and MPS was conducted by fixed critical diameter as reference point. The Critical diameter here refers to a kind of one-point threshold. Meanwhile, the complete DSD have discontinuous issue of number concentration nearby critical diameter. These issues refer to the need to systematize and optimize the way DSD is combined. In this study, we proposed an optimizing combination based on the weighting factor and the variance of DSDs with the undersampling error removed. First of all, the diameter with a small relative deviation of the number concentration of DSD values in the MPS and 2DVD is defined as the critical diameter. the critical diameter of this study means the buffer interval to use the weighting factor nearby the threshold. And then, we removed the error caused by undersampling in the DSD near the critical diameter of the MPS and 2DVD. We compared the rainfall rate and radar reflectivity between the original complete DSD and the new complete DSD as a reference to Pluvio data and Precipitation Occurrence Sensor System (POSS) data. The comparison for summer rainfall events in 2022 in Incheon, South Korea shows the new complete DSD has relatively higher skill scores. In the future, the optimization method will be applied using other disdrometer data, and then verified and generalized. ACKNOWLEDGEMENT: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS46-A016
Thermodynamic and Dynamic Characteristics of Mesoscale Convective Systems Over Seoul Metropolitan Area
Si-Hyeon SON1+, Kyuhee SHIN1, Kwonil KIM2, Jeong-Eun LEE1, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Stony Brook University, United States
The damage caused by heavy rainfall is increasing in South Korea. Particularly, Mesoscale Convective Systems (MCS) have a significant impact on Seoul metropolitan area due to the high density of population and infrastructure. The formation and development of MCS are affected by the thermodynamic and dynamical environment. MCSs passing over the Seoul metropolitan area developed in the distinctive environment due to the complex topography. In this study, we present thermodynamic and dynamical processes of the MCS occurring over the Seoul metropolitan in the summer of four years (2018–2021). We classified the MCS cases into four types: convective cells (CC), mesoscale convective complex (MCC), diagonal squall line (SLD), and parallel squall line (SLD). Korea Local Analysis and Prediction System (KLAPS; reanalysis data) was used to figure out the mechanism of a mesoscale phenomenon. CC was generated by thermal instability and had more than a twofold increase of convective available potential energy (CAPE) (2100 m2 s-2) compared to other types (0~1000 m2 s-2) before the mature stage. MCC showed the smallest value of convective inhibition (CIN) at the mature stage. Total totals index (TTI) significantly changed during MCC and SLD events, and SLP maintained a consistently high total precipitable water (63 mm) throughout the entire stage. In terms of dynamic instability, storm relative helicity (SRH, 0-3km) for SLD (110 m2 s-2) and SLP (125 m2 s-2) was larger than CC (10 m2 s-2) at the mature stage. Wind shear (0-1km, 0-3km, and 0-6km) showed a similar trend, while SLP showed a large value of 0-6km shear before the mature stage. In conclusion, we investigate environmental properties which are conducive to the development of each MCS. ACKNOWLEDGEMENT: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS46-A017
Characteristics of Mesoscale Convective Systems in Korean Peninsula Based on Multi-year Radar Composite
Choeng-Lyong LEE+, Soorok RYU, Gyu Won LEE#
Kyungpook National University, Korea, South
Mesoscale convective systems (MCSs) are organized convective cloud complexes developed by aggregation of several thunderstorms. These cloud systems have spatial scales ranging from a few hundred to a thousand kilometers and a life cycle of several hours, contributing to severe weather events in the Korean peninsula during the warm season. In this study, we investigate the physical properties of the Korean-type MCSs (KMCSs) using three-dimensional datasets from radar networks. The classification of KMCSs was performed using phenomenological elements. Four distinct classes of KMCSs were identified: convective cell (CC), mesoscale convective complex (MCC), parallel squall line (SLP), and diagonal squall line (SLD). The vertical structures of these precipitation types were explored to confirm the physical characteristics using dual-polarization radar observations and feature parameters derived from mean reflectivity and vertical integrated liquid water contents. Furthermore, the generalized microphysical parameters (N0', Dm') derived from polynomial regressions consisting of ZDR and reflectivity were analyzed to demonstrate the microphysical peculiarities. The mean reflectivity (ZDR and KDP) of SLD in the lower atmosphere below 4 km exhibited relatively higher (lower) values compared to other KMCS types, while CC showed opposite tendencies. Additionally, the retrieved microphysical parameters of each type were compared to each other. SLD has a relatively large N0' as compared to CC. The results depict that SLD is composed of small droplets with large number concentrations. Interestingly, Dm' distribution of SLD has two peaks whereas CC has only a peak. We estimate the two peaks are caused by the convective part and stratiform part in the squall line, respectively. Acknowledgment: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS46-A019
Strong Sensitivity of Simulated Supercells to Low-level Moisture: Effects of Near Cloud Base Moisture Flux
Jinlin LI1#+, Ming XUE2
1Nanjing University, China, 2The University of Oklahoma, United States
Idealized numerical simulations using climatological composite sounding from 61 significant tornadoes within China failed to produce sustained storm. An increase in the vertical wind shear showed minimal impact on storm longevity. The simulated storms showed high sensitivity to environmental humidity, however, particularly that at 1-2 kilometers above ground level (AGL). Increasing humidity within this layer led to the formation of long-lived (≥ 2 hours) and more intense supercells, even though the increase did not change the lifting condensation level (LCL) and convective available potential energy (CAPE) of the sounding much. LCL and CAPE are usually considered important environmental parameters and are part of the significant tornado parameter (STP) used in operations. Water vapor entrainment was calculated as moisture fluxes of air across the storm core surface, where the storm surface included the part below cloud base. Results showed that more environmental water vapor was entrained and inflowed into the updraft core near the cloud base of simulated storms when the humidity in the 1-2 km AGL layer increased, and the greater positive buoyancy represented by maximum perturbation potation temperature indicated the more latent heat of water vapor condensation was released within updraft core. Additionally, the time integral of total water vapor entrainment played a pivotal role in determining the evolution of convection. Sustained greater amount of water vapor entrainment led to more intense, sustained convection.
AS46-A021
The Influence of Shear Line in Triggering Heavy Rainfall Events in the Philippines
Sheilla Mae REYES#+, Seungyeon LEE, Seon Ki PARK
Ewha Womans University, Korea, South
Heavy rainfall events (HREs) occur almost throughout the year in the Philippines, constituting one of the most prevalent hazards. While many studies have focused on HREs during the summer monsoon season, there has been relatively limited research on HREs during the winter monsoon season in the country. This study classifies the heavy precipitation spatial patterns and identifies its associated synoptic weather features using the 20-year (2003-2022) daily precipitation dataset obtained from 55 rain gauges from November to February. HREs are classified into six clusters by employing a cluster analysis on the most pertinent principal modes extracted from the principal component analysis. Each cluster exhibits a distinct heavy rainfall spatial pattern, mostly showing more than 50 mm of 24-hour accumulated rainfall in the eastern portion of the country. The results show two conditions for the Shear Line to cause heavy rainfall: (1) a surge of northeasterly winds must prevail with at least near-gale force winds; (2) the Shear Line should interact with different tropical weather systems, such as tropical cyclones, tropical waves, surface troughs, and Borneo vortex. The findings of this study provide valuable insights into weather forecasting by establishing links between the spatial distribution of HREs and synoptic patterns in the Philippines.
AS56-A002
Flash Drought Monitoring Using Diurnal-provided Evaporative Demand Drought Index
Haobo LI#+
RMIT University, Australia
Flash drought, as a relatively new concept, represents a rapidly evolving drought with sudden onset, short-term duration, and great destructiveness. With the warming of the planet in recent decades, the frequent occurrences of flash droughts have resulted in considerable losses to personnel and properties on a global scale. Nowadays, the emerging Evaporative Demand Drought Index (EDDI) has revealed its significant potential and adaptability in the early warning and quantification of flash droughts. In this study, an advanced method for improving the accuracy and temporal resolution of EDDI is proposed. The new set of EDDI estimates is calculated using diurnal-provided potential evapotranspiration values that have been calibrated with weather parameters and Global Navigation Satellite Systems (GNSS) atmospheric products. Then, the monitoring performances of flash droughts resulting from the diurnal-provided EDDIs are evaluated over the period 2010–2021 in Hong Kong. Results showed that the Probability Of Detection (POD) and False Alarm Rate (FAR) were 87.1% and 16.7%, respectively. By comparing with their counterparts obtained from the use of monthly EDDIs, it was found that the improvements made by the new method in the metrics of POD and FAR were 24.6% and 11.2%, respectively. In addition, with the use of diurnal-provided EDDI, the mean lead time for flash drought detection has been prolonged to 37.74 days, offering more time to prevent and mitigate the detrimental effects brought by flash drought events.
AS56-A010
Local Well-posedness of Strong Solution to a Climate Dynamic Model with Phase Transformation of Water Vapor
Jieqiong MA1#+, Ruxu LIAN2, Qingcun ZENG2
1Institute of Atmospheric Physics,Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China
The primitive three-dimensional viscous equations for atmospheric dynamics with the phase transformation of water vapor are studied. According to the actual physical process, we give the heating rate, mass of water, and precipitation rate, which are related to temperature and pressure. In fact, this system strictly obeys the conservation of energy and is used to make better climate predictions. Providing H2 initial data and boundary conditions with physical significance, we prove the local well-posedness of a unique strong solution to the moist atmospheric equations by the contractive mapping principle and the energy method in the H2 framework.
AS61-A004
A Pacific Tropical Decadal Variability Challenge for Climate Models
Yingying ZHAO#+
Laoshan Laboratory, China
Understanding and forecasting Tropical Pacific Decadal-scale Variability (TPDV) strongly rely on climate model simulations. Using a Linear Inverse Modeling (LIM) diagnostic approach, we reveal Coupled Model Intercomparison Project Phase 6 models have significant challenges in reproducing the spatial structure and dominant mechanisms of TPDV. Specifically, while the models' ensemble mean pattern of TPDV resembles that of observations, the spread across models is very large and most models show significant differences from observations. In observations, removing the coupling between extratropics and tropics reduces TPDV by ∼60%–70%, and removing the tropical thermocline variability makes the central tropical Pacific a key center of action for TPDV and El Niño Southern Oscillation variability. These characteristics are only confirmed in a subset of models. Differences between observations and simulations are outside the range of natural internal TPDV noise and pose important questions regarding our ability to model the impacts of natural internal low-frequency variability superimposed on long-term climate change.
AS61-A010
Synchronous Decadal Climate in the Central Tropical Pacific and South Atlantic
Chao LIU1+, Soon-Il AN1#, Soong-Ki KIM1, Malte STUECKER2, Wenjun ZHANG3, Fei-Fei JIN4
1Yonsei University, Korea, South, 2University of Hawaii at Manoa, United States, 3Nanjing University of Information Science & Technology, China, 4University of Hawaii, United States
El Niño/Southern Oscillation (ENSO), the strongest interannual climate variability, strongly influences remote sea surface temperature (SST) in the northern tropical Atlantic, but has only a fragile relationship with SST in the equatorial Atlantic. Here, we reveal a highly synchronous paradigm between Central Pacific (CP) ENSO and tropical South Atlantic SST variability over the past seven decades, but on a decadal timescale. In the boreal spring-summer season, the decade-long warm CP-ENSO-like SSTs actively trigger the cooling of South Atlantic SSTs through teleconnections involving Southern Hemisphere extratropical Rossby waves and equatorial Kelvin waves. The resulting subtropical South Atlantic low-level anticyclonic circulation and northern flank easterlies trigger local ocean-atmosphere feedbacks and strengthen inter-basin teleconnections. A Pacific-driven coupled simulation fairly reproduces the observational features, while a parallel Atlantic-driven simulation shows less feedback to the Pacific. We conclude that the central tropical Pacific is an important source of decadal predictability for tropical Atlantic SST and the surrounding climate.
AS61-A013
Modulation of the Link Between the Hadley Circulation and the Meridional Structure of Tropical SSTs by the Atlantic Multidecadal Oscillation
Ran AN1+, Jianping LI1#, Juan FENG2
1Ocean University of China, China, 2Beijing Normal University, China
This paper investigates the effects of the Atlantic multidecadal oscillation (AMO) on the relationship between the Hadley circulation (HC) and the different meridional structures of the tropical sea surface temperature (SST). The response of the HC to SSTs shows inconsistent variations between the warm and cold phases of the AMO. The response of the HC to SSTs during the cold phase of the AMO is similar to that seen in the long-term and seasonal cycles. However, during the warm AMO phase, the magnitude of this response is significantly reduced. This significant difference in the response is caused mainly by the weakened response amplitude of the equatorially asymmetric HC and SST. The potential mechanisms associated with this suppression are also investigated, and they relate primarily to differences in the SST meridional anomalies within the Indo-Pacific warm pool (IPWP). During the AMO warm phase, the profile of SST anomalies in the IPWP exhibits characteristics similar to an equatorially symmetric distribution, which weakens the equatorially asymmetric component of the tropical SST and then contributes to the suppression of the response ratio. However, the amplitudes of the insignificant negative SST anomalies in the northern and southern IPWP are similar during the cold AMO phase. This distribution of SST anomalies has a minimal impact on the variation of SST gradients. Therefore, the response ratio during the cold AMO phase is comparable to that observed in the long-term and seasonal cycles. Other atmospheric reanalysis data are used to further confirm these results.
AS61-A014
Asymmetric Influences of ENSO Phases on the Predictability of North Pacific Sea Surface Temperature
Zhaolu HOU+, Jianping LI#, Yina DIAO
Ocean University of China, China
The North Pacific sea surface temperature (SST) exerts profound climatic influence. El Niño-Southern Oscillation (ENSO) significantly impacts North Pacific SST, yet the influence from ENSO’s distinct phases on SST predictability remains unclear. Overcoming model limitations, this study assesses SST predictability under diverse ENSO phases using reanalysis. Quantifying predictability limits (PL), results unveil asymmetry: El Niño PL at 5.5 months, La Niña at 8.4 months, and Neutral at 5.9 months. This asymmetry mirrors contemporary multimodal prediction skills. Error growth dynamics reveal La Niña's robust signal strength with slow error growth rate, contrasting El Niño's weaker signal and faster error growth. Neutral exhibits intermediate signal strength and elevated error growth. Physically, predictability signal strength aligns with SST variability, whereas error growth rate correlates with atmospheric-ocean heating anomalies. La Niña, inducing positive heating anomalies, minimizes atmospheric noise impact, resulting in lower error growth. The results are beneficial for improving North Pacific SST predictions.
AS61-A015
Variations in Moist Static Energy Transport Associated with ENSO
Chaeeun HONG#+, Changhyun YOO
Ewha Womans University, Korea, South
Moist static energy (MSE) transport plays a key role in the global atmospheric energy cycle. However, there is a lack of research on the mechanisms by which the MSE transport varies on a year-to-year time scale associated with the leading climate mode, El Niño-Southern Oscillation (ENSO). The MSE consists of the geopotential, sensible, and latent energy, and each transport is decomposed into the transports by the mean meridional circulation and by the eddies. The eddy transport is further divided into the stationary and transient components. We find that an El Niño enhances the northward (southward) MSE transport between 0–15°N (15°N–40°N) by about 0.3 PW (-0.25 PW). At 40°N and poleward, an increased northward MSE transport is observed with a maximum of 0.1 PW near 50 °N. The changes in the tropics and subtropics are primarily due to geopotential energy transport, which is about twice as large as sensible or latent energy transport in the region. The decomposition shows that the strengthened but narrowed Hadley cell during El Niño explains most of the changes in the geopotential energy transport, and the contributions from eddies are at least an order of magnitude smaller than the mean transport. In contrast, in the extratropics, the changes in the MSE transport are attributed to all geopotential, sensible, and latent energy transports. Furthermore, in the extratropics, the eddy transport is found to be as large as the mean transport. We investigate how an ENSO leads to changes in stationary versus transient eddy transports. This study has implications for how the future ENSO will lead to changes in the atmospheric energy cycle.
AS61-A016
The Oceanic Processes Associated with Tropical Pacific Quasi-decadal Variability
Guangliang LI#+, Kewei LYU, Wei ZHUANG, Jianyu HU
Xiamen University, China
The tropical Pacific features not only ENSO variability on interannual timescales (2-7 years) but also decadal-to-multidecadal variability on longer timescales. Particularly, the quasi-decadal SST signal, with a period of ~12 years, exhibits its maximum peak in the Niño4 region. Heat budget analysis based on hindcast simulation from a global ocean model and an ocean reanalysis product indicates that the development of quasi-decadal SST anomalies in the Niño4 region are mainly contributed by the zonal advective feedback (u'Tbar), upwelling feedback (w'Tbar), and thermocline feedback (wbarT'). While the upwelling feedback is linked to the intensity of subtropical cells (STCs) and induces in-phase Niño4 SST anomalies, the phase transition of thermocline feedback and zonal advective feedback lead the Niño4 SST by ~ half year. Taking the development of warming phase as example, subsurface warm anomalies between 100-200 m first appear in the western tropical Pacific and then extend eastward underneath the Niño4 region, which cause deepened thermocline (i.e., thermocline feedback) and higher sea level at Equator. The latter enhances meridional pressure gradient, thus leading to stronger North Equatorial Countercurrent and zonal advective feedback.
AS61-A018
The Role of the Aleutian Low in the Relationship Between Spring Pacific Meridional Mode and Following ENSO
Yuqiong ZHENG#+
Yunnan University, China
The spring Pacific Meridional Mode (PMM) is an important precursor of the El Niño-Southern Oscillation (ENSO). However, recent studies reported that only about half of the spring PMM events were followed by ENSO events. This study examines the role of internal climate variability in modulating the impact of PMM on ENSO using 100-member ensemble simulations of the MPI-ESM. The relationship between spring PMM and following winter ENSO shows a large spread among the 100 members. The variation of spring Aleutian Low (AL) intensity is identified to be an important factor modulating the PMM-ENSO relation. The spring AL affects the PMM-ENSO relation by modifying PMM-generated low-level zonal wind anomalies over the tropical western Pacific. The strengthening of the spring AL is accompanied by westerly wind anomalies over the mid-latitude northwestern Pacific, leading to sea surface temperature (SST) cooling there via an enhancement of upward surface heat flux. This results in increased meridional SST gradient and leads to northerly wind anomalies over the subtropical northwestern Pacific, which turn to surface westerly wind anomalies after reaching the equatorial western Pacific due to the conservation of potential vorticity. Thus, the low-level westerly (easterly) wind anomalies over the tropical western Pacific associated with the positive (negative) spring PMM were strengthened (weakened), which further contribute to an enhanced (a weakened) PMM-ENSO relation. The mechanism for the modulation of the AL on the spring PMM-ENSO relation can be verified by a set of AGCM simulations. This study suggests that the condition of the spring AL should be considered when predicting ENSO on the basis of the PMM.
AS61-A022
Counteracting Impacts of the ENSO and Aleutian Low on the Northeast Asian Winter Surface Air Temperature Anomalies
Xuefeng LIU#+, Zhiwei ZHU
Nanjing University of Information Science & Technology, China
Exploring the mechanisms that modulate Northeast Asia (NEA) winter surface air temperature (NEAWT) holds significant scientific and societal importance. In this study, we investigate the individual and combined impacts of the El Niño-Southern Oscillation (ENSO) and the Aleutian Low (AL) on NEAWT. The significantly positive correlation between El Niño and strengthened AL demonstrates distinct effects on NEAWT. El Niño correlates with positive NEAWT anomalies, while the strengthened AL results in the opposite effect. The impact of El Niño on NEAWT is directly associated with a local anomalous anticyclone, which is the portion of two Rossby wave trains induced by a triple convection pattern over tropical Pacific and Indian Ocean. Conversely, the impact of strengthened AL on NEAWT is directly associated with a local anomalous cyclone, which is the terminal of one Rossby wave train induced by AL. The Indian Ocean warming triggered by El Niño acts to damp the impact of strengthened AL on NEAWT, leading to an anticyclonic anomaly over NEA. The combined impact of ENSO and AL on NEAWT can be understood as a simple combination of the effects of the individual modes. The strengthened AL can intensify (diminish) negative (positive) NEAWT anomalies during La Niña (El Niño), with the weakened AL producing the opposite effect. Further research indicates the Pacific Decadal Oscillation modulates the intensity of AL variations during El Niño/La Niña events.
AS61-A024
The Interaction Between Winter North Pacific Oscillation and ENSO
Masahiro WATANABE1, Wenjun ZHANG2#, Tomoki IWAKIRI1, Suqiong HU2
1The University of Tokyo, Japan, 2Nanjing University of Information Science & Technology, China
The winter North Pacific Oscillation (NPO), the secondary dominant mode of atmospheric variability over the North Pacific, has been recognized as a potential precursor for El Niño-Southern Oscillation (ENSO) development. This work demonstrates that the pre-existing winter NPO signal is primarily excited by sea surface temperature (SST) anomalies in the equatorial western-central Pacific, suggesting that the lagged relationship between ENSO and the NPO involves a tropical-extratropical two-way coupling rather than a purely stochastic forcing of the extratropical atmosphere on ENSO. The winter NPO impacts on the subsequent ENSO evolution are further quantified in our study. We performed an ensemble of “overriding” experiments using the MIROC6 climate model, which reproduces the NPO-ENSO relationship well. In the overriding experiment, surface heat flux and wind stress anomalies over the North Pacific were replaced with those associated with the NPO in the historical runs for five months from November in the preceding year of ENSO. The ENSO events could be reproduced overall without the NPO forcing because of the intrinsic predictability arising from the tropical coupled dynamics. When the positive NPO forcing with varying amplitude is given to the model, the El Niño events are enhanced approximately 22% per standard deviation of the NPO anomaly. The positive SST anomalies in the subtropical eastern North Pacific caused by NPO exhibit an equatorward development, increasing SST in the tropical central Pacific and subsequently affecting the El Niño evolution. However, the La Niña events show a much lower sensitivity (2% per 1std NPO) to the prescribed negative NPO forcing due to asymmetry in the NPO spatial pattern.
AS61-A026
Lessons Learned from the 2023/24 El Niño Development
Ji-Won KIM1#+, Baijun TIAN1,2, Jin-Yi YU3
1California Institute of Technology, United States, 2University of California, Los Angeles, United States, 3University of California, Irvine, United States
The development of the 2023/24 El Niño, following the rare triple-dip La Niña from 2020 to 2023, drew global attention due to its substantial heat accumulation in the western Pacific caused by the prolonged La Niña. Many researchers and news media suggested and reported that the heat buildup of the 2023/24 El Niño had the potential to give rise to another extreme El Niño, similar to the historically strong 1997/98 El Niño. However, its growth rate unexpectedly decelerated after the first half of 2023, particularly in the eastern tropical Pacific regions, leading to its failure to materialize into an extreme event. Armed with these results, this study investigates the spatiotemporal characteristics of the 2023/24 El Niño and identifies two unique points of the event as follows: (1) The 2023/24 El Niño originated as a coastal event during the boreal spring, with its maximum anomalies located in the far-eastern equatorial Pacific near Peru and extending westward. (2) Unlike the oceanic conditions, the atmospheric conditions during the 2023/24 El Niño development were strangely tranquil, lacking noticeable westerly anomalies over the central-eastern equatorial Pacific (which are essential for the growth of El Niño). The reasons behind these unique points and the lessons we can learn from the 2023/24 El Niño development will also be discussed.
AS61-A029
Two Pathways of the Properties of the ENSO Due to the North Atlantic Ocean Under a Net-zero Emission Scenario
SungHyun SONG#+, Sang-Wook YEH
Hanyang University, Korea, South
Achieving carbon neutrality is crucial to mitigate temperature rise, and understanding environmental changes after carbon neutrality is important. In this study, we analyzed the properties of the ENSO during the carbon neutrality period by analyzing the CESM net-zero emission experiment, in which a carbon dioxide emission increases linearly based on the SSP 5-8.5 scenario, and then decrease at the same rate until it reaches a net-zero emission. We focused mainly on a net-zero emission period. We analyzed each of the 8 ensemble members and found that there are two pathways of ENSO properties in which the state of the North Atlantic Ocean differs. We show how the ENSO’s properties are modulated by the North Atlantic Ocean during the carbon neutrality period. This result implies that the inter-basin interactions should be considered to understand the environmental change that is achieved even with a net-zero emission.
AS61-A031
Exploring the Origins of Central-pacific El Niño-like Sea Surface Temperature Anomalies in CMIP6 Simulations
Li-Chiao WANG#, Tzu-Yun LIU+
National Central University, Taiwan
A systematic bias in the extremely westward zonal current has been identified over the equatorial Pacific in the Coupled Model Intercomparison Project 6 (CMIP6) models. This bias tends to diminish the modeled interannual variability of the equatorial zonal current anomalies, with its highest variability concentrated in the western Pacific. An analysis of the mixed-layer heat budget indicates that the simulation of the mean circulation effect is only minimally impacted by the zonal current bias. However, the zonal advective feedback is intricately linked to the biased variability in equatorial zonal current anomalies, with an overestimation (underestimation) observed in the Niño-4 (Niño-3) region. Notably, the magnitude of the zonal advective feedback surpasses that of the thermocline feedback, emerging as the predominant process contributing to the growth of the mixed-layer temperature anomaly tendency in the Niño-4 region. This bias plays a crucial role in producing a more Central-Pacific El Niño-like performance in CMIP6 models.
AS61-A035
Different El Niño Flavors and Associated Atmospheric Teleconnections as Simulated in a Hybrid Coupled Model
Junya HU1#+, Hongna WANG2, Chuan GAO1, Rong-Hua ZHANG2
1Institute of Oceanology, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China
A hybrid coupled model (HCM) has been developed previously, which is composed of an intermediate tropical Pacific Ocean model and a global atmospheric general circulation model (AGCM), denoted as HCMAGCM. In this study, different El Niño flavors, namely the Eastern-Pacific (EP) and Central-Pacific (CP) types, and the associated global atmospheric teleconnections are examined in a 1000-yr control simulation of the HCMAGCM. The HCMAGCM exhibits major different characteristics of EP and CP El Niños in terms of related oceanic and atmospheric variables in the tropical Pacific, including the amplitude and spatial patterns of sea surface temperature (SST), zonal wind stress and precipitation anomalies. An SST budget analysis indicates that the thermocline feedback and zonal advective feedback dominantly contribute to the growth of EP and CP El Niño events, respectively. Corresponding to the shifts in the tropical rainfall and deep convection during EP and CP El Niños, the model also reproduces the differences in the extratropical atmospheric responses during the boreal winter. In particular, the EP El Niño tends to dominantly excite a poleward wave train pattern to the Northern Hemisphere, while the CP El Niño tends to preferably produce a wave train similar to the Pacific North American (PNA) pattern. As a result, there exist different climatic impacts in the North America regions, with a warm-north and cold-south pattern during EP El Niño and a warm-northeast and cold-southwest pattern during CP El Niño, respectively. This modeling result highlights the importance of internal natural processes within the tropical Pacific in the genesis of ENSO diversity, because the active ocean-atmosphere coupling is allowed only in the tropical Pacific within the framework of HCMAGCM.
AS62-A002
Airborne Measurements of Black Carbon, Co, CO2 and Their Source-dependent Characteristics Over the Yellow Sea
Naki YU1+, Min Jae JEONG2, Sangmin OH2, Shanlan LI2, Hee-Jung YOO2, Sumin KIM3,2, Kyung-On BOO4,3, Yongjoo CHOI5, Saehee LIM1#
1Chungnam National University, Korea, South, 2National Institute of Meteorological Sciences, Korea, South, 3Korea Meteorological Administration, Korea, South, 4Numerical Modeling Center, Korea, South, 5Hankuk University of Foreign Studies, Korea, South
Black Carbon (BC) is a particulate matter emitted directly into the atmosphere during the combustion of fossil fuels or the biomass burning. BC strongly absorbs visible light and is highly mobile due to its small size, contributing to regional to global climate change. In this study, we examined airborne measurement data of BC, CO, and CO2 over the Yellow Sea using an aircraft from National Institute of Meteorological Sciences (NIMS) from May 21, 2021 to May 2, 2022. For the 24 flights, the averages of mass concentration (MrBC), mass median diameter (MMD) of rBC particles, fraction of thickly-coated rBC particles (Fthick), shell/rBC core ratio (Rshell/core) were 148.0±202.0 ng m-3, 181 nm, 52±17%, 1.36±0.12, respectively. The averages of MrBC/ΔCO an ΔCO/ΔCO2 were 1.36±0.12, 2.77±1.69 ng m-3 ppbv-1 and 1.78±2.15 ppbv ppbv-1 %, respectively. Airmass trajectories estimated by the Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) model were categorized into Korean Peninsula, China, Mongolia, Russia, Long Range Transport(LRT), Ocean, and the ‘accumulated precipitation along trajectory (APT)’ was also calculated to analyze the mixing state of the black carbon under the influence of wet scavenging. The result showed that among the origins, the averages of MrBC, Fthick, Rshell/core, MrBC/ΔCO, ΔCO/ΔCO2 were the highest in the airmass originating from China, and only the MMD was highest in the airmass from Russia. How the concentration and mixing state of black carbon and MrBC/ΔCO, ΔCO/ΔCO2 changes with APT will analyzed. In addition, specific events such as Asian dust and haze will be analyzed by comparing with aerosol optical depth (AOD). This work was funded by the BK21 FOUR Project and the Korea Meteorological Administration Research and Development Program "Development of Asian dust and haze monitoring and prediction technology" under Grants (KMA 2018-00521).
AS67-A003
Characteristics and Mechanisms of Heavy Rainfall Spatial Distribution and Diurnal Cycle Over an East China Mesoscale Mountain
Churui CHEN1,2#+, Kun ZHAO1, Anning HUANG1, Xingchao CHEN3
1Nanjing University, China, 2Nanjing University, China, 3The Pennsylvania State University, United States
The Dabie Mountain region in East China experiences frequent heavy rainfall every warm season. In this study, we used radar and satellite data to investigate the combined effects of synoptic patterns and topography in determining the spatiotemporal variation of heavy rainfall in the region during the warm seasons of 2008-2020 based on an objective classification method. The results indicate that heavy rainfall is most likely to occur under two typical synoptic patterns (P1 and P2) dominated by a southwesterly monsoon. The diurnal cycle of heavy rainfall under P1 has one significant morning peak, whereas heavy rainfall of P2 reaches its maximum in the morning and lasts for four hours. The morning heavy rainfall peak can be explained by the enhanced moisture transportation due to the inertial oscillation of low-level wind and its interaction with topography. Under P2, the diurnally varied low-level ageostrophic wind south and north of the mountain leads to a low-level convergence over the study region, which facilitates the peak rain intensity in the mornings to remain at high levels before decreasing. Based on the statistical results, a heavy rainfall event caused by a mesoscale convective system (MCS) has been examined by the assimilation of both radar and surface observations into the Variational Doppler Radar Analysis System. The results indicate that the initiation of the MCS resulted from the collisions among three distinct outflow boundaries. The subsequent merge of mesoscale vortexes intensified the newly triggered convection and led to the organization of a south-north-oriented squall line. The study concludes that under the modulation of synoptic patterns, the diurnal cycle and spatial distribution of heavy rainfall is closely related to the scale interactions between the diurnal varying low-level moisture transportation and local terrains in East China.
AS67-A007
Processes of Precipitation Enhancement Over the Da-Tun Mountain During the Influence of Typhoon Meari (2011)
Lin-Wen CHENG#+, Cheng-Ku YU, Syuan-Ping CHEN
National Taiwan University, Taiwan
This study uses dense observational networks of rainfall, Doppler radar data, an upslope model, and theoretical analysis of the seeder-feeder mechanism to investigate the event of intense rainfall over the Da-Tun Mountain (DT) during the influence of Typhoon Meari (2011). The objective is to identify the processes responsible for precipitation enhancement under a typhoon environment. DT is an isolated mountain barrier located adjacent to the northern coast of Taiwan. DT received significant rainfall as Meari was located approximately 300 km northeast of Taiwan and brought strong northerly/northwesterly flow impinging on the mountain. The accumulated rainfall over DT exceeds 260 mm within 10 h period, with maximum precipitation occurring over the northwestern mountain ridge and its leeward slope. During the period of primary interest, the DT region was continuously influenced by the approach and landfall of typhoon background precipitation (including both stratiform and convective precipitation), providing a favorable condition for the operation of the seeder-feeder process. A theoretical equation of the seeder-feeder process was derived and calculated to estimate the low-level precipitation enhancement over DT. In this analysis, feeder clouds are assumed to be generated by upslope lifting so they can be practically estimated from the upslope model. The seeder clouds are approximated by upper-level precipitation at 3 km through the backward trajectory of hydrometers originated in the region of heaviest precipitation over DT. These analyses show that the enhanced precipitation over DT is much better quantified by the theoretical seeder-feeder process than the upslope-lifting-induced precipitation. Furthermore, the theoretical approach provides a better estimate of precipitation enhancement when the typhoon background precipitation is more stratiform in nature. These research findings not only confirm the importance of the seeder-feeder mechanism in enhancing precipitation under a typhoon environment but also imply the complexity of precipitation enhancement processes associated with convective background precipitation.
AS67-A012
Origin of Outer Tropical Cyclone Rainbands
Cheng-Ku YU#+, Che-Yu LIN, Chi Hang PUN
National Taiwan University, Taiwan
Outer tropical cyclone rainbands (TCRs) are a concentrated region of heavy precipitation and hazardous weather within tropical cyclones (TCs). Outer TCRs pose considerable risk to human societies, but their origin is a long-standing, unresolved topic. This study identifies a total of 1029 outer TCRs at their formative stage from 95 TCs by long-term radar observations collected near Taiwan from 2002 to 2019 and aims to provide a robust foundation of the natural diversity of rainband origin. One of the striking findings from the study is that current theories of outer TCRs cannot appropriately explain the observed TCR characteristics and statistics. The results show the dominance of outer origin for the observed outer TCRs, in distinct contrast to theoretical modeling works of outer TCRs, which propose inner-origin scenarios. Large discrepancies between the observed rainband’s propagation characteristics and theoretically predicted propagation velocities of both gravity waves and vortex Rossby waves are found, suggesting that wave disturbances do not have a direct impact on the origin of outer TCRs. Our analysis also suggests that squall-line dynamics are a common, but not the sole, mechanism responsible for outer TCR formation. In particular, the nature of preexisting outer precipitation is found to be an important factor to influence the squall-line and non-squall-line outer TCR initiation.
AS68-A003
Climatological Study of Fog in Japan Using METAR/SPECI Reports
Ryota MISAWA#+, Hirofumi SUGAWARA
National Defense Academy of Japan, Japan
Fog-induced low-visibility significantly affects the operation of various transportation systems, particularly aviation. Fog in and around the airports could impact greatly the safety and efficiency of aircraft takeoffs and landings. Despite the recent developments in forecasting technology, nowcasting remains underway. It is partly because the nowcasting of fog is often based on the experiential knowledges, not on the physical mechanisms of fog formation. To improve the fog nowcasting, more understanding of fog events is needed. This study investigates the characteristics of fog at Japanese airfields using METAR/SPECI report data. In addition to regular hourly observations (METAR), special observations conducted during significant weather events (SPECI), including fog, were utilized. This approach aims to reveal fog events with the higher temporal resolution than the previous studies. We studied fog events at 18 airfields in Japan from 2010 to 2015, focusing on the site-by-site difference of fog types which would be influenced by the local climate and the site terrain. The study used an objective algorithm developed by Tardif and Rasmussen (2007, J.App.Meteorol.Clim.) for investigating fog formation processes. The results revealed that the various types of fog occur at each airfield, although the precipitation fog was relatively major. In some airfields, advection fog or radiation fog was frequently appeared. We found some cases of the cloud base lowering fog, which has not been reported in Japan.
AS68-A007
The Development and Evaluation of Multi-model Diagnostic Ensemble (MMDE)-based In-flight Icing Forecast System
Eun-Tae KIM+, Jung-Hoon KIM#
Seoul National University, Korea, South
In-flight icing deteriorates aircraft performance by deforming fuselages, and affects crucial components of an aircraft such as flight control surfaces, engine inlets, and windshields, thereby posing threats to safe flight operations. In this study, multi-model diagnostic ensemble (MMDE)-based in-flight icing forecast system is developed using two operating global Numerical Weather Prediction (NWP) model outputs used in Korea Meteorological Administration (KMA): Unified Model- and Korean Integrated Model-Global Data Assimilation and Prediction System (UM-GDAPS and KIM-GDAPS). The icing diagnostic indices are composed of early version of NWP model-based categorical algorithms and recently developed fuzzy-logic algorithms, which were (are) used by the global operational aviation weather centers. Outputs from each diagnostic index and MMDE-based icing forecast system are evaluated quantitatively against icing pilot reports collected during 2022 and qualitatively against the in-situ icing observations reported from the KMA/National Institute of Meteorological Science Atmospheric Research Aircraft (NARA) icing cases in Korea. In general, MMDE-based probabilistic forecast showed improved performance skills for detecting both yes- and no-icing observations than that from a single diagnostic. Detailed results will be presented at the conference. Acknowledgement: This research is supported by the Korea Meteorological Administration Research and Development Program under Grants KMA2022-00310 and KMA2022-00410.
AS68-A008
Climatology of Mountain Wave Turbulence in the Recent 44-Years Revealed in ERA5 Data
Yewon SHIN+, Jung-Hoon KIM#
Seoul National University, Korea, South
Mountain wave turbulence (MWT) in Upper Troposphere and Lower Stratosphere (UTLS) is one of the most important sources of aviation turbulence, which poses a threat to the aviation safety and arises from the large-amplitude mountain waves and their subsequent breakings. Occurrence of MWT in UTLS is governed mainly by two parts: 1) Low-level wind speed and static stability projecting to the mountains for the calculation of mountain wave stress (MWS) and 2) Background wind and stability in mid- and upper-levels for the conditions of vertical propagation and breakdown of the mountain waves. Both can be modulated by large-scale atmospheric circulation due to climate change, potentially leading to the changes in MWT. For extending the previous studies on climatology of clear air turbulence (CAT) revealed in the reanalysis data and global response of aviation turbulence to the future climate change, this study examined the climatology of MWT over 44 years (1979-2022) using the ECMWF Reanalysis version 5 (ERA5) data and its interaction with background wind speed and static stability. First, MWT diagnostics were calculated by multiplying surface MWS to CAT diagnostics and using orographic gravity wave drag. Surface MWS showed the seasonal variation near the mountain ranges in both hemispheres. Finally, spatiotemporal distributions and long-term trends of MWT in UTLS were analyzed using the 95th percentiles of various MWT diagnostics. Detailed results of the characteristics and long-term trends of MWT related to background wind speed and static stability will be shown in the conference. Acknowledgment: This research was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00310 and supported by Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education (NRF-2019R1I1A2A01060035).
AS68-A010
Aircraft Icing Detection Algorithm Using Geostationary Satellite Data and Numerical Weather Prediction Model in Korea
Sung-Ho BAEK+, Jung-Hoon KIM#, Eun-Tae KIM
Seoul National University, Korea, South
When an aircraft flies into the cloud with a plenty of large super-cooled water droplets, aircraft icing can occur frequently due to the formation of ice on the aircraft's surfaces. This can pose serious mechanical failures and safety issues, which could lead to a possible accident and damage. Various weather agencies have been used available satellite data and Numerical Weather Prediction (NWP) models to infer such aircraft icing conditions. This study aims to fuse satellite icing products and NWP model-based icing forecast to produce a real-time icing information. We first evaluated two geostationary satellite-based (GK-2A and GOES-R) icing algorithms against the research aircraft-based in situ icing observation data in Korea from February 2018 to August 2022. The results showed that using both satellite algorithms has a higher performance skill than that from the single one. Finally, the icing probability from the GOES-R algorithm and the icy cloud area information from the GK-2A one were combined together for the data fusion with the NWP model-based icing forecast, Korean-Forecast Icing Potential (K-FIP). The K-FIP is a fuzzy-logic algorithm based on the membership functions of temperature, relative humidity, vertical velocity, and cloud mixing ratios for diagnosing 3D icing potential areas. In the selected icing cases along the cross-sections of the CloudSat’s Liquid Water Content, the data-fusion algorithm developed by this study showed a better situational awareness of aircraft icing threat by reducing an overestimation of the diagnosed wide areas of icing potentials solely from the K-FIP. Acknowledgment: This work was funded by the Korea Meteorological Administration’s Research and Development Program “Technical Development on Weather Forecast Support and Convergence Service using Meteorological Satellites” under Grant (KMA2020-00121).
AS68-A012
Multi Model and Diagnostic Ensemble (MMDE)-based Probabilistic Forecast for Deep Convective Area Using KMA’s Operational NWP Models
Yi June PARK+, Jung-Hoon KIM#, Jun Seok PARK
Seoul National University, Korea, South
Deep convection can cause serious weather hazards. So, short- and mid-term forecasts for Deep Convective Area (DCA) are essential for strategic planning of the Air-Traffic Management (ATM). This study developed the Multi Model and Diagnostic Ensemble (MMDE)-based probabilistic forecast system for DCA using the Global Data Assimilation and Prediction System based on the Unified Model and Korean Integrated Models (UM-GDAPS and KIM-GDAPS). Using the radar mosaic data in Korea, the predictand for the DCA was defined as the area where 15 dBZ Echo Top Height (ETH) exceeds the Flight Level (FL) 250 (about z = 7-8 km). Total of 22 predictors derived from the GDAPS outputs consists of the dynamical components including instability, moisture, and lifting, and physical components of cloud and precipitation. For the indices of instability, Area Under the Curve (AUC) of UM-GDAPS was higher than that of KIM-GDAPS. But, moisture and lifting indices showed that the KIM-GDAPS outperformed the UM-GDAPS. For the physical products directly calculated from the NWP model’s physical parameterizations, these showed the AUC of UM-GDAPS is higher than that of KIM-GDAPS highly due to the difference in the cumulus parameterization in the GDAPS. The probability of DCA at a given grid point was calculated as the relative percentage of the number of all ensemble members exceeding each its own threshold that is based on the True Skill Statistics. The reliability diagram comparing with the DCA showed the over-forecasting in all forecast time. But, when comparing with the areas over FL150 of ETH, the lower convective area where ETH exceeds FL150 actually observed at up to 70 % of frequency on average in the 100 % predicted area in forecast fields, which can be eventually very useful for an avoidance guidance of the DCA as the decision support tools in the ATM system in Korea.
AS68-A013
Characteristics of Flight Times and Clear-air Turbulence Encounters Along the Trans-oceanic Flight Routes
Joon Hee KIM+, Jung-Hoon KIM#
Seoul National University, Korea, South
The impact of climate change on upper-level flow has shown that the East Asian jet stream has intensified and shifted poleward at cruising altitudes over the last four decades. In particular, an increase in vertical wind shear at these altitudes has led to more Moderate-Or-Greater (MOG)-level turbulence occurrence. Long-haul transoceanic flights recommended to follow wind optimal routes (WORs) are significantly affected by upper-level winds, which minimizes flight time and consequently reduces fuel consumption. Adoption of such routes to operation is likely to increase further in the future in line with the International Civil Aviation Organization (ICAO)’s Carbon Offsetting and Reduction Scheme for International Aviation (CORSIA). Therefore, examining the changes in WORs due to variations in upper-level flows using historical meteorological data is essential for understanding future projection of aviation operations. In this study, we investigate the relationship between flight times and spatial distribution of the WOR trajectories and changes in upper-level winds by utilizing 40 years of ERA5 reanalysis data (1981-2021). Our results indicate that over the last 40 years during boreal winter (DJF), the east-bound (EB) and west-bound (WB) routes for trans-Pacific flights connecting East Asia and the western United States have also moved northward. This shift has resulted in a shortening (lengthening) of the EB (WB) routes. Flight times have decreased for EB and increased for WB flights. Additionally, we have observed an increase in the potential for MOG-level turbulence along the WORs for many long-haul flight routes. This can lead to higher CO2 emissions, thereby contributing to an acceleration of climate change and potentially creating a positive feedback loop. Acknowledgment: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00310.
AS68-A014
Near-cloud Turbulence Related to the Interaction Between East Asian Jet and Upper-level Outflow of Tropical Cyclone Hagibis
Ju Heon LEE+, Jung-Hoon KIM#
Seoul National University, Korea, South
High potentials of upper-level turbulence in Upper Troposphere and Lower Stratosphere (UTLS) was found over East Asia, which was mainly attributed to the jet dynamics associated shear, convective, and inertial instabilities around the East Asian Jet (EAJ) (e.g., Lee et al., 2023). Those turbulence in UTLS can be modulated by the interaction between EAJ and upper-level outflows of deep convections and Tropical Cyclones (TCs), which is called the Near Cloud Turbulence (NCT). To understand the spatial and temporal distributions of the NCT highly correlated with the EAJ and TC Hagibis in 2019, potentials of NCT throughout the TC life cycle was investigated using the ECMWF Reanalysis version 5 data on model levels (vertical spacing of 8 hPa300 m). Here, the potentials of NCT were examined by magnitudes of turbulence diagnostics such as Potential Vorticity (PV), Vertical Wind Shear (VWS), local Richardson number (Ri), and Brunt-Vӓisӓlӓ frequency (N2) and so on. The results showed that the characteristics of turbulence diagnostics near the outflow of the TC have been changed depending on the distance between the TC and EAJ. After the recurvature stage of the TC, frequencies of various instabilities related to PV, VWS, Ri, and N2 were increased at the southern side of the EAJ. Evolution of turbulence diagnostics around the EAJ in line with the evolution of TC have also been identified, which will be given in more detail at the conference. References: Lee, J. H., Kim, J.-H., Sharman, R. D., Kim, J., & Son, S.-W. (2023). Climatology of Clear-Air Turbulence in upper troposphere and lower stratosphere in the Northern Hemisphere using ERA5 reanalysis data. Journal of Geophysical Research: Atmospheres, 128, e2022JD037679.Acknowledgement: This research was performed by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00410.
AS68-A015
Characteristics of Convectively Induced Turbulence (CIT) Derived from the Radar Data in Korea
Juseob KIM+, Jung-Hoon KIM#
Seoul National University, Korea, South
Convectively Induced Turbulence (CIT) occurs mainly due to the strong variations in vertical velocity within the deep convective clouds. In this study, we estimated an eddy dissipation rate (EDR) from the weather radar data in Korea. EDR is an objective reporting metric of aviation turbulence by the International Civil Aviation Organization. For Numerical Weather Prediction (NWP) model-based turbulence forecast system such as the Graphical Turbulence Guidance (GTG), Lognormal Mapping Technique (LMT) has been used to convert the original values of the NWP model-based turbulence diagnostics to EDR-scale for the prediction of objective intensity of turbulence. Using the LMT, raw value of Spectrum Width (SW) data from the radar observation was converted to the EDR-scale to understand the characteristics of CIT embedded with the convection types in Korea. Following the LMT method suggested by Kim et al. (2021), SW data with reflectivity of ≥ 30 dBZ were collected during 2021. The probability density function (PDF) of the collected SW data was used to construct the best lognormal function fitting to the SW histograms. Finally, three cases representing different types of convective systems such as the squall line, cloud clusters, and isolated thunderstorm were investigated. As a result, spatial and temporal distributions of reflectivity and SW-EDR were found to be dependent upon the type of convective system. Common feature in three case studies was that SW-EDR shows higher values near cloud top areas, while reflectivity was higher near cloud base, which implies that using SW-EDR is more effective way to avoid possible CIT encounter at cruising altitudes than relying solely on reflectivity. Further detailed results will be presented in the conference. Acknowledgement: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00310.
AS68-A016
Comparative Evaluation of Eddy Dissipation Rate Estimation Methods Using Doppler Lidar
SeungWon BAEK1+, Kwonil KIM2, Jung-Hoon KIM3, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Stony Brook University, United States, 3Seoul National University, Korea, South
Turbulence is one of the most significant physical processes in aviation meteorology because of the airplane's safety. However, due to the small spatial and temporal scales and the unpredictable nature of turbulence, detecting its spatiotemporal distribution with conventional observations is limited. Doppler lidar, on the other hand, can provide continuous information about wind fields with high spatiotemporal resolution. Eddy dissipation rate (EDR) is a quantitative measure of turbulence intensity. Various methods have been proposed to estimate EDR using Doppler lidar, but the value depends on the estimation methods and observation strategy. Intercomparison of methods is still needed to ensure estimation accuracy. In this study, we compared the performance of five different EDR estimation methods (power spectrum, second-order structure function, variance, structure function fitting, and velocity azimuth display) using Doppler lidar. The Velocity Azimuth Display (VAD) estimation method was verified using the sonic anemometer at the meteorological tower. EDR estimated from the VAD method showed similar variations and high correlation (CORR > 0.5) with EDR estimated from the sonic anemometer. EDR estimated from the VAD method was affected by elevation angle. The lower the angle, the higher the value of EDR was shown. When comparing by altitude, the 80° elevation angle showed the most similar results to the vertically pointing measurements. All methods from vertically pointing measurements showed almost identical variations and values (CORR > 0.9). The characteristics of each method are presented, considering the instrumental characteristics of Doppler lidar and the scanning strategy. ACKNOWLEDGEMENT: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS68-A019
Evaluation of Different Microphysics Parameterizations on the Prediction of Aircraft Icing
Liping LUO#+
Nanjing University of Aeronautics and Astronautics, China
This study evaluates the aircraft icing potential prediction for a severe aircraft icing event using convection-allowing numerical model with different microphysics schemes. Various microphysics schemes (MP) including the one-moment, two-moment, and three-moment MP schemes (e.g., WSM6, WDM6, Thompson, Morrison, MY, NSSL schemes) are used to simulate the event. The commonly empirical icing algorithms including the IC index, frost point, IP index, CIP are examined based on the simulations. Results show that there exists significant spatiotemporal and temporal variability of the predicted icing conditions among the experiments. Comparisons of aircraft in-situ and satellite observations, and pilot reports of aircraft icing are also made for temperature, cloud liquid water content, cloud type, and median volume diameter. Overall, this work enhances our understanding of cloud microphysics schemes and provides a base for selecting appropriate cloud microphysical solutions for icing weather prediction.
AS70-A010
Enhancing the Accuracy of Scattering Matrix of Non-spherical Particles Across a Broad Size Parameter Range Using Deep Learning
Yue XI+, Lei BI#
Zhejiang University, China
Accurately computing the scattering matrix of non-spherical particles across a complete range of size parameters remains a significant challenge in the field of aerosol remote sensing. Practically, numerically exact methods, such as the Invariant Imbedding T-Matrix Method (IITM), and approximate methods, such as the improved geometric optics method (IGOM), are employed for computations. However, the IGOM’s accuracy degrades for smaller sizes, while the IITM faces computational constraints at large sizes. It is difficult to ensure a smooth transition from the IITM to the IGOM results. To address this issue, we present a deep learning approach that leverages the neural network’s extrapolation and interpolation capabilities. This approach predicts and connects scattering matrix values across transitional size parameter regions. Extensive simulations demonstrate the method’s potential for accurate and real-time computation of the scattering matrix across an entire range of size parameters, offering a promising solution for non-spherical particle scattering computations.
AS70-A014
Potential of Passive Spectral Radiometer Measurements for Mixed Phase Cloud Retrieval
Lijun HU1#+, Chao LIU1, Yao BIN2
1Nanjing University of Information Science & Technology, China, 2Nanjing Joint Institute for Atmospheric Sciences, China
Mixed-phase clouds have significant impacts on the Earth’s water cycle, weather evolution, and radiation balance. However, current passive radiometer measurements can only be used to retrieve the properties of uniform single-layer ice and water clouds, and remote sensing of mixed-phase cloud properties is highly challenging due to the mixture of both water droplets and ice crystals in it. This study uses rigorous radiative transfer and information content analysis to investigate the potential of passive spectral radiometer measurements for mixed-phase cloud retrieval. The optical properties database of mixed-phase cloud is established by considering the ice-water fraction. Analysis suggests that the reflectances in 0.87-, 1.61- and 2.25-μm channels have obvious mixed-phase cloud characteristics. However, preliminary results based on the sensitive tests further indicate that current spectral radiometers are still difficult to infer mixed-phase clouds accurately and it may be necessary to consider more relationships between ice and water properties in the mixture clouds.
AS76-A010
Characteristics of Spatial-temporal Distribution and Storm Morphologies of Tornadoes in Jiangsu Province, China
Fen XU#+
Nanjing Joint Institute for Atmospheric Sciences, China
From 2006 to 2018, spatial- temporal distribution, strength distribution, and storm morphology characteristics of Jiangsu tornadoes are analyzed. There are 41 tornadoes recorded in 27 tornadic days during the 13 year period, with an average annual tornado of 3.2 times. Among them, the most frequent tornado events occurred at EF2 level, accounting for 39%, while the EF4 tornado was only recorded once. Since the 21st century, there has been no record of extreme Tornado Events of EF5 in Jiangsu Province, while the weak tornadoes are likely to be ignored due to the weak disaster. Tornadoes mainly occur in the eastern coastal area, the central coastal area and the western area of the north of the Huaihe River. Compared with the past, the high-risk center of tornado in Central Jiangsu has a trend of moving southward, while the high-risk center in the eastern coastal area shows a feature of northward movement. Most of tornadoes occur in spring and summer, 90% of which are happened in July and August. The beginning of tornadoes is from 10:00 to 20:00 local time, and the peak frequency of tornado genesis in the diurnal variation is between 15:00 and 20:00. About 50% of the tornadoes occur during the Meiyu period, while 27% of them are typhoon tornadoes. More than 50% of tornadoes in Jiangsu are generated in supercell mesocyclone embedded in cluster convective morphology, and about 30% of tornadoes are produced in the QLCSs convective morphology. Contrast to high frequency of tornadoes produced by the discrete cells in the United States, the possibility of tornadoes generated from discrete cells in East China (mainly in Jiangsu Province) is the lowest, and only two tornadoes (less than 5%) were generated in discrete cells in the past 13 years.
AS76-A030
Impact of Vertical Air Motion on Snow Microphysics in Dendritic Growth Layer
Ji-Hye JUNG1+, Kwonil KIM2, Kyuhee SHIN1, Jeong-Eun LEE1, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Stony Brook University, United States
The growth of dendritic particles occurs rapidly in the -15 °C region, where the saturated vapor pressure difference between ice and water maximize. The dendritic growth layer (DGL) plays an important role in the formation and growth of ice particles. However, the microphysics and dynamics in DGL are not fully understood. Ye and Lee (2021) established a hypothesis the generation of new small particles is favorable in the DGL due to the supersaturation associated with updrafts below. Leonie von Terzi et al. (2022) showed the temperature regions where updrafts occurred coincided with that of strongest depositional growth, and that updrafts could potentially be related to latent heat release by enhanced depositional growth. In this study, we analyze the impact of updrafts on snow microphysics in the DGL using the muti-wavelength cloud radar observations (Ka/Ku-band dual-polarization radar and W-band radar) collected during the ICE-POP 2018 (International Collaborative Experiments for Pyeongchang 2018 Olympic & Paralympic winter games). The temperature-axis CFADs of radar variables were constructed to analyze the impact of snow microphysical process on the vertical profiles of radar variables. An increase in reflectivity, a maximum value of differential reflectivity and specific differential phase, and a decrease in the cross-correlation coefficient were found in the region with maximum updraft intensity. We also applied the vertical air velocity estimation and peak finding technique to reveal the snow microphysics related with the updraft. The generation of new ice particles proved to be activated by the updraft in the DGL from the in-detail analysis of the bi-modal Doppler spectra. In conclusion, the characteristic signature of radar variables in the DGL suggest a mechanism for the generation of small particles driven by the presence of an updraft. ACKNOWLEDGEMENT: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS76-A031
The Microphysical Characteristics of Thunderstorm Over Yangtze River Delta, China, During Mei-yu Season
Ji YANG#+
Nanjing Joint Institute for Atmospheric Sciences, China
Using operational polarimetric radar, cloud-to-ground (CG) lightning, and the ERA5 reanalysis data in 2020, this study examined the microphysical characteristics of summer thunderstorm during two active CG lightning periods over Yangtze River Delta in China. The results show that the mei-yu thunderstorm presented the large area and much graupel between 0 to -10 ℃; these were accompanied by large vertical wind shear favoring of thunderstorm organization. Therefore, broad updrafts within the mei-yu thunderstorm were hypothesized, causing lower amounts of dilution and entrainment, facilitating transportation of supercooled liquid water to the mixed-phase region and production of CG lightning. Due to large atmospheric instability, strong updrafts within the post-mei-yu thunderstorm were expected to supply supercooled liquid water for riming process to form more graupel above level of -10 ℃. These provided favorable conditions for thunderstorm electrification, resulting in much more CG lightning during the post-mei-yu period than the mei-yu period.
AS76-A032
Simulation Analysis of Typical Tornadic Supercell and Nontornadic Supercell Processes
Kangyuan SUN#+
Nanjing Joint Institute for Atmospheric Sciences, China
The process of tornado supercells occurred in Funing, Jiangsu Province on June 23, 2016 and the typical non-tornado supercells occurred on April 28, 2015 under the background of of high-altitude cold vortex and surface warm depression were analyzed in detail by using the four-dimensional variational assimilation analysis system simulation, Doppler weather radar, conventional observation and encrypted automatic station data. The results indicate that: (1) The large vorticity region of the tornado supercell is first generated and developed in the middle and upper levels, and then with the weak cold pool outflow and the vertical wind shear in the lower levels continuously strengthening, the large vorticity center is gradually generated in the lower levels and gradually strengthened. Meanwhile, the bottom height and top height of the Mesocyclone are gradually declining. When the vorticity center drops to the ground and the bottom height of the Mesocyclone drops to the lowest level, the tornado is generated. (2) The non-tornado supercell also has generate vorticity centers in the middle and high levels and develops to the lower levels. Under the influence of the strong cold pool near the ground, its vorticity in the lower levels cannot be maintained for a long time or cannot be strengthened or even weakened, thus inhibiting the generation of tornadoes. However, the strong cold pool outflow can also produce gale weather. (3) If the cold pool is too strong, the low-level inflow of the storm will be weakened. When the vertical wind shear of the environment weakens, the supercell will also tend to weaken or even split and dissipate.
AS76-A033
Automatic Center Detection of Tropical Cyclone Using Image Processing Based on Operational Radar Network
Sun Jin MO#+, Ji-Young GU, Seung-Woo LEE
Korea Meteorological Administration, Korea, South
In this study, we propose an algorithm ACTION defined as an automatic center detection of tropical low pressure (TC) using operational radar network-based image processing. Based on the high visibility of weather radar images, the motion vector of TC is calculated from the continuous image change using optical flow to determine the center of rotation as the center of TC. The performance of the algorithm was verified for typhoons affecting the Korean Peninsula (northwestern Pacific typhoon) from 2018 to 2021, and it showed a high detection rate of 80.8% within an error distance of 40 km compared to the best track of KMA (Korea Meteorological Administration). For typhoons with temporally consistent morphological characteristics, the detection rate was 100%. ACTION automatically generates TC central information when TC first enters within the observation radius, even in the absence of uniform radar data. ACTION used opencv, one of the open source libraries. TC central detection is performed in real time and can be applied directly to rapidly generated weather radar images, so it is currently being used by KMA for forecasting. The high-resolution time-resolution TC-centric information calculated through the ACTION is expected to improve the efficiency of TC prediction. Acknowledgement: This research was supported by the grants "Development of analysis technologies for local-scale weather radar network and next generation radar (KMA2021-03221)" and “Development of radar based severe weather monitoring technology (KMA2021-03121)” of the "Development of integrated application technology for Korea weather radar project” funded by the Weather Radar Center, Korea Meteorological Administration.
AS76-A034
Enhancement of Low-level Wind Analysis Using New Terminal Doppler Weather Radar
Youn CHOI#+, Soyeon PARK, Kwang-Ho KIM, Jung SUNG-HWA
Korea Meteorological Administration, Korea, South
The new Terminal Doppler Weather Radar (TDWR) began operating at Incheon International Airport in October 2022. This advanced system has multiple benefits for both aviation operations and meteorological detection. With its high-resolution capabilities, TDWRs can provide precise radar data, accurately detecting small-scale atmospheric phenomena, including rainfall, wind speed, wind direction, and other weather variables, which generate essential information for air traffic management. The Korea Meteorological Administration's Weather Radar Center (WRC) has been using a variational multiple-Doppler radar three-dimensional wind synthesis method called WISSDOM to provide real-time three-dimensional radar wind fields across the Korean Peninsula to KMA forecasters. The WISSDOM wind field is derived from weather radar Doppler velocity and represents three-dimensional wind information based on observations. While the TDWR data is helpful for low-level observations in Gyeonggi Bay, it's essential to have an appropriate observation strategy to combine this data with other radar information efficiently. Additionally, consistency with previously provided TDWR system data, such as the wind shear alarm, must be considered when modifying observation strategies. This research aims to improve wind observation capabilities by modifying observation strategies in the recently upgraded TDWR system. The goal is to enhance the quality of the three-dimensional wind field at low-level heights. We refined our observation strategy and incorporated TDWR data into WISSDOM to achieve this goal. We used the Velocity Azimuth Display (VAD) reconstruction function for Doppler velocity quality control to compare WISSDOM winds with surface wind observations at AWS. Acknowledgements: This research was supported by “Development of radar based severe weather monitoring technology (KMA2021-03121)” of “Development of integrated application technology for Korea weather radar” project funded by the Weather Radar Center, Korea Meteorological Administration.
AS76-A035
Analysis of Mesoscale High Impact Weather Using High-resolution Three-dimensional Wind Fields Derived from Weather Radar Network
Soyeon PARK#+, Kwang-Ho KIM, Jung SUNG-HWA
Korea Meteorological Administration, Korea, South
The frequency of hazardous weather events that exceed our forecasts has been increasing recently. Comprehensive analysis using high-resolution thermodynamic and dynamic instability and vertical shear information is essential to improve understanding and prediction of hazardous weather. The Weather Radar Center (WRC) of the Korea Meteorological Administration (KMA) provides real-time wind fields for the Korean Peninsula using high-resolution 3D wind field products (WISSDOM) derived from the observation of radar radial velocity. This technology allows for quickly providing the dynamic structure of heavy rainfall in 3D, reflecting the dynamic characteristics of precipitation systems in real-time. In this study, we analyzed the structure of complex precipitation systems, such as mesoscale convection cells, using various types of wind information provided by WISSDOM. This included convergence and divergence of upper and lower air currents, vorticity, ascending and descending speeds, and changes in wind systems by layer. Additionally, we calculated vertical wind shear (wind direction and wind speed) and dynamic instability (Storm Relative Helicity, SRH) using WISSDOM wind elements. We used these analyses to understand epidemiological information related to the occurrence and continuation of mesoscale hazardous weather, such as rainy season precipitation systems and mesoscale convective systems. Vertical wind shear and dynamic instability (SRH) calculated based on the radar three-dimensional wind field have been provided to the weather analysis operational system since May 2023 to support forecasting. Through this, it will be possible to analyze the development and continuation of mesoscale convection systems and predict torrential rain-leading signals and areas. Acknowledgements: This research was supported by "Development of radar based severe weather monitoring technology (KMA2021-03121)" of "Development of integrated application technology for Korea weather radar" project funded by the Weather Radar Center, Korea Meteorological Administration.
AS76-A039
Predicting Radar Reflectivity Distributions Based on Machine Learning Models
Weisheng WU1+, Chuan-Ming LIU1#, Lawrence Jing-Yueh LIU2,3
1National Taipei University of Technology, Taiwan, 2University of Illinois Urbana-Champaign, United States, 3National Central University, Taiwan
Weather condition affects our daily life, so prior forecast information can reduce losses caused by disasters worldwide. By investigating meteorological variable trends with machine learning models, the accuracy of meteorological forecasts should be enhanced. In recent years, machine learning methods such as PredRNN, EBGAN, AENN, etc., have been used to predict radar reflectivity distribution. Compared to traditional nowcasting methods, these approaches are indeed much more accurate due to the inclusion of non-linear information. However, machine learning still faces challenges such as amplifying noise, indicating the need for further refinement and improvement. Therefore, we utilize radar reflectivity data with machine learning techniques to provide rainfall intensity information in various regions. The images are treated as sequences and used as inputs for the machine learning model, which then outputs the future radar reflectivity distribution. In this research, a Generative Adversarial Network (GAN) is employed. The Generator takes past one-hour radar reflectivity data to generate data for the next hour, while the Discriminator distinguishes the output of the Generator from ground truth images. The two small models will compete each other. The Generator aims to mislead the Discriminator, while the Discriminator attempts to accurately differentiate between generated and ground truth images. The architecture incorporates Convolutional Long Short-Term Memory (ConvLSTM) to capture both short-term and long-term temporal and spatial features within the sequence of images. The main focus of this research is to enhance the accuracy of rainfall prediction using radar reflectivity distribution with machine learning models, particularly in Taiwan where is often affected by extreme rainfall events such as typhoon or Mei-Yu front.
AS79-A010
The Impact of Asian Summer Monsoon on Transport of Very-short-lived Chlorocarbons to the Stratosphere
Qing LIANG1#+, Paul A. NEWMAN1, Eric FLEMING1,2, Leslie LAIT1,2
1NASA Goddard Space Flight Center, United States, 2Science Systems and Applications, Inc, United States
Stratospheric ozone is catalytically destroyed by chlorine released from ozone-depleting substances (ODS), e.g., chlorofluorocarbons, and halogenated very-short-lived substances (VSLS). In addition to chlorine contributions from continued emissions of Montreal Protocol-regulated long-lived ODSs (from existing banks, production, consumption, and feedstocks), recent research has highlighted concern over rapidly growing emissions of dichloromethane (CH2Cl2) - a chlorinated VSLS (Cl-VSLS). Large emissions come from Asia have developed because of fast economic growth. In this study, we have conducted model simulations with geographically resolved surface emissions of the two most abundant Cl-VSLS, CH2Cl2 and CHCl3, with the NASA GEOS Chemistry Climate Model (GEOSCCM). The simulations cover the 2011-2022 period to understand the transport pathway of Asian Cl-VSLS emissions to the stratosphere and to quantify the contribution of Asian emissions to the stratospheric chlorine budget w.r.t. the global estimate during the 2010s. Our results suggest that the Asian Summer Monsoon plays a dominant role in the troposphere-to-stratosphere transport of Cl-VSLS and is twice as efficient for delivering CH2Cl2 to the stratosphere than the tropics. We will also present GEOSCCM simulated Cl-VSLS impact on stratospheric chlorine and ozone.
AS79-A012
Analysis of Vertical Distribution Patterns of Atmospheric Constituents Over the Korean Peninsula Using Diagonal Snapshot
Jihun KIM1+, Ja-Ho KOO1#, Jin-Soo PARK2, Laura L. PAN3, Paul A. NEWMAN4
1Yonsei University, Korea, South, 2National Institute of Environmental Research, Korea, South, 3National Center for Atmospheric Research, United States, 4NASA Goddard Space Flight Center, United States
Air pollutants have a significant impact on human health. With increasing global awareness of air pollution, research on these constituents has become crucial. Airborne observation has the advantage of informing the vertical distribution of wide-area atmospheric constituents by presenting their similarities and differences. However, Airborne measurement has limitation of data scarcity. Therefore, we additionally used previously unutilized diagonal ascent/descent data from campaigns like the KORUS-AQ (2016), GMAP (2021), SIJAQ (2022), and ACCLIP (2022) to examine the vertical distribution patterns and differences of carbon compounds, nitrogen oxides (NOx), ozone (O3), and volatile organic compounds (VOCs) within the 500m-4000m altitude range over the Korean Peninsula. Notable differences were observed between the KORUS-AQ and SIJAQ campaigns. Although both campaigns were conducted in the late spring to early summer under the same geographical condition, the vertical distributions of O3, NOx, and VOCs during the SIJAQ campaign exhibited greater variability than those in the KORUS campaign. (This study utilized data obtained through aircraft observations from the 2016 KORUS-AQ, 2021 GMAP,2022 SIJAQ, and ACCLIP campaigns. We would like to express our gratitude to all the scientists who contributed to making this observational data available for our research.) This work was supported by Korea Environment Industry & Technology Institute (KEITI) through "Climate Change R&D Project for New Climate Regime", funded by Korea Ministry of Environment (MOE) (2022003560006).
AS79-A015
The Influence of Vertical and Horizontal Advection to the Surface Ozone Change in Summer, South Korea
Ja-Ho KOO1#+, Joowan KIM2, Hyungyu KANG2, Minju PARK1, Sojeong LEE1, Jin-Soo PARK3
1Yonsei University, Korea, South, 2Kongju National University, Korea, South, 3National Institute of Environmental Research, Korea, South
This study examined if the enhancement of summertime surface ozone in South Korea relates to the strength of vertical or horizontal transport of ozone-rich air mass. For this study, we conducted ~50 daily ozonesonde measurements in August 2021 and 2022 and compared to the surface and aircraft ozone measurements for the possible date. When we chose extreme 5 days showing the highest and lowest surface ozone level among all ~ 50 days, we found the interesting contrast: all 5 days of highest (lowest) ozone occurred in August 2021 (2022). The pattern of vertical ozone profile and correlation analyses of ozone between different altitudes indicated that the variation of surface ozone in 2021 is much associated with the strength of stratospheric ozone intrusion in the upper troposphere, implying the potential contribution to the stratospheric ozone to the surface ozone level. In addition, we found an interesting case in 4 to 5 August 2022, showing the quick change of surface ozone level: low in 4 but high in 5 August. We found that this quick change clearly relates to the horizontal transport pattern, converting from southerly to westerly between 4 and 5 August, meaning the large contribution of emission source in 5 August. This work let us know the transport influence (even in vertical scale) should not be neglected in the analysis of recent increasing ozone trend of East Asia.
AS79-A017
Variability of Upper-tropospheric Ozone Over the East Asia from a Perspective of Atmospheric Stationary Waves
Jae-Heung PARK1#+, Ja-Ho KOO2, Sang Seo PARK3, Kyung-Hwan KWAK4, Joowan KIM5, Taegyung LEE2, Uju SHIN2, Jun-Hyeok SON6, Jong-Seong KUG1
1Seoul National University, Korea, South, 2Yonsei University, Korea, South, 3Ulsan National Institute of Science and Technology, Korea, South, 4Kangwon National University, Korea, South, 5Kongju National University, Korea, South, 6IBS Center for Climate Physics, Korea, South
Due to not only adverse influences on the environment and ecosystem but also significant contribution to global warming, it is imperative to gain a comprehensive understanding of variability of tropospheric ozone. By analyzing observational reanalysis datasets since late twentieth century, here we investigated the monthly variability of upper tropospheric ozone (250hPa) from a perspective of atmospheric stationary waves, particularly over East Asia where a stratosphere–troposphere exchange is vigorous. To identify the primary variability modes of upper-tropospheric ozone over East Asia, an empirical orthogonal function (EOF) analysis was employed. It is found that the first three EOF modes collectively account for approximately two-thirds of the total ozone variability over East Asia. The first EOF mode, characterized by a monopole pattern centered from the northeastern China to Sakhalin Island, is associated to a deepening of East Asian trough. Additionally, the second and third EOF modes, featured by meridional and zonal dipoles, are linked to the Western Pacific Oscillation and Eurasia teleconnection. Over the troughs and ridges of those atmospheric stationary waves, upper-tropospheric ozone increases and decreases, respectively. Consequently, our findings underscore the importance of atmospheric stationary waves in understanding the internal fluctuations of ozone in East Asia.
AS81-A006
Investigating Sea Surface Salinity Impacts on Tropical Cyclone Rapid Intensification by Coupled Atmosphere‑wave‑ocean Model Simulations
Huisi MO#+
The Hong Kong University of Science and Technology, Hong Kong SAR
The occurrence of tropical cyclones (TCs) and their subsequent landfall bring about substantial impacts on coastal cities. The prediction of TC impacts remains a challenging task owing to the intricate physical processes responsible TC-induced heavy precipitation, winds, and storm surge. Among the factors influencing TC dynamics, sea surface salinity (SSS) has received limited attention in prior studies, despite its crucial role in ocean density stratification. The significance of SSS lies in its capacity to impact surface fluxes and vertical ocean mixing processes, thereby exerting an indirect but noteworthy influence on the rapid intensification (RI) of TCs. Previous studies indicated that the inclusion of SSS significantly improves the RI detection skill. Nevertheless, the lack of a fully integrated, physically consistent atmosphere-wave-ocean interface with explicit momentum and energy exchanges poses a significant constraint in accurately forecasting the impacts of SSS. Hence, a high-resolution coupled atmosphere–wave–ocean model, namely, the Unified Wave Interface-Coupled Model (UWIN-CM) is employed to stimulate multiscale air–sea interactions, during Super Typhoon Saola and record-breaking rainstorm in Hong Kong. The UWIN-CM couples the Weather Research and Forecasting (WRF) Model, the University of Miami Wave Model (UMWM), and the Hybrid Coordinate Ocean Model (HYCOM) in a single framework that can simulate the physical interactions and exchanges among these three components. To elucidate the physical mechanisms responsible for the SSS effect on RI in South China Sea, this study will compare the coupled UWIN-CM model simulations and in situ measurements to examine the influence of SSS on vertical mixing and TC development, providing a better understanding of TC dynamics and an improvement of TC forecasting capabilities.
Session Chair(s): Kosei YAMAGUCHI, Kyoto University, Pay-Liam LIN, National Central University
AS83-A010
| Invited
Cloud-resolving Ensemble Prediction of the Extreme Rainfall Event on 2 June 2017 in Northern Taiwan
Chung-Chieh WANG#+, Po-Yu HUANG, Shin-Yi HUANG
National Taiwan Normal University
An extreme Mei-yu rainfall event occurred on 2 June 2017 along the northern coast of Taiwan, where a peak amount of 635 mm fell in about 10 hours from 0100-1100 LST. Using ensemble-based sensitivity analysis, an earlier study (Wang et al., 2021) showed that the areal-averaged rainfall in the wider region surrounding northern Taiwan in this event was influenced by frontal moving speed, frontal intensity (contrast), and location and timing of frontal disturbance in experiments using grid sizes of 2.5-5 km, but peak amounts in such runs were no more than 360 mm, suggesting low predictivity for its occurrence. Using 1-km grid size, predictions in a later study (Wang et al., 2023), on the other hand, showed that a peak amount of up to 541 mm can be achieved with a finer grid, but the detailed rainfall pattern and maximum amount are strongly dictated by the presence of a frontal low-pressure disturbance that affected the location and persistence of the surface convergence zone, thus again suggesting high nonlinearity and low predictability. However, in some initial times about 2.5-3 days before the event, the evolutions were more favorable for larger and more concentrated rainfall. In this study, the above extreme rainfall event is further examined, using ensemble forecasts both at 1 km and larger grid sizes, including the experiments carried out in the Taiwan Area Heavy-rainfall Prediction Experiment (TAHPEX). Special attention is given on the predictability of this extreme event and the strategy to produce useful results more effectively with longer lead times for early warning and preparation.
AS83-A020
Implications of Western Pacific Tropical Cyclones’ Raindrop Size Distributions to the Bulk Microphysics Schemes Using Rand Forest Regression Model
Jayalakshmi JANAPATI1+, Balaji Kumar SEELA1,2, Pay-Liam LIN1#
1National Central University, 2Academia Sinica
The widely used two-moment bulk-microphysics (BMPs) schemes explicitly calculate two of the three gamma distribution parameters, often by taking the third parameter to be fixed. However, the fixed value assumption to any of these three parameters results in irregularities with observations. To overcome the limit imposed by fixed parameter values, diagnosed relations between gamma distribution parameters or related variables have been proposed in the literature. In this study, long-terms raindrop size distributions (RSDs) measurements of the Western Pacific tropical cyclones (WP TCs) from the ground-based disdrometers over North Taiwan are used to study the gamma fits of the RSDs. The moments method is adopted to estimate the three (slope, shape and intercept) parameters of the gamma distribution. The gamma parameters are estimated under four scenarios of method of moments (Zero moment to fifth moment). The three gamma parameters estimated under four scenarios are used to estimate the rain integral parameters like rainfall rate, radar reflectivity, total number concentration, and mass-weighted mean diameter. The best moment method scenario is identified by comparing the gamma fitted rain integral parameters with the observed one. The diagnosed relations between any two parameters of the gamma distribution are established and the superior performance of the random forest model over the linear regression model for the WP TCs is also demonstrated in this study.
AS83-A027
Modification of Goddard Cumulus Ensemble to Double-moment Microphysics Scheme: Idealized and Real Case Study
Yu-Jyun LIOU1#+, Kaoshen CHUNG1, Wei-Kuo TAO2, Cheng-Rong YOU1, Li-Hsin CHEN1
1National Central University, 2NASA Goddard Space Flight Center
This study aims to modify Goddard Cumulus Ensemble microphysics (GCE) scheme, which is the widely used microphysics scheme for simulations and forecasts around the world, from single-moment to double-moment scheme. The upgraded scheme predicts the mixing ratios of seven species hydrometeors (water vapor, cloud water, rain water, cloud ice, snow, graupel and hail), and total number concentrations of hydrometeors in warm-rain processes (cloud water and rain water). To examine the performance of GCE double-moment, it was evaluated and compared to different microphysics schemes by: 1) an idealized 3D squall line test; 2) a warm-rain processes dominant real case over Taiwan. For the 3D idealized test, the result of accumulated rainfall is less in GCE double-moment compared to GCE single-moment, but the features of the dynamic, thermodynamic, and rainfall rate are similar as GCE single-moment scheme. In addition, when calculating the total number concentration, GCE double-moment scheme shows the capability to present more diversity of rain droplet sizes in both convective and stratiform regions toward reality, and this is similar as other double-moment schemes. On the other hand, the performance of quantitative precipitation forecast showed that, the GCE double-moment scheme is had better forecast skill compared to the GCE single-moment, especially for the heavy rainfall region.
AS83-A028
Evaluating Different Microphysical Retrieval Methods Using Different Radar Variables and Observation Error Assumptions
Chen-Hau LAN+, Pay-Liam LIN#, Yu-Chieng LIOU, Wei-Yu CHANG
National Central University
Existing algorithms for transforming radar observations into microphysical parameters require information on the drop size distribution (DSD). However, assuming the shape of DSD can lead to significant errors, especially for low moments of microphysical parameters. To reduce DSD model errors, we developed a new algorithm based on variational principles - the Moment-Based Variational (MV) method. The retrieval results of different moments are analyzed using the variational method. Idealized experiments are used to assess the impact of observational errors on different retrieval methods for different observational variables. The results indicate the superiority of the MV method, particularly in lower-order moments, effectively reducing errors under variational approaches. Incorporating different radar observational variables can significantly enhance the MV method retrieval. On the other hand, we used radar observations of different wavelengths from the TAHOPE/PRECIP IOP3 to test the MV method with and compare it with ground-based disdrometers. The MV method exhibits notable improvements in both stratiform and convective precipitation. In summary, this new method transforms polarimetric parameters into model microphysical parameters, which is beneficial to subsequent applications in microphysical scheme adjustments and data assimilation.
AS83-A016
Spatiotemporal Structure of Raindrop Size Distribution in a Convective Precipitation System Simulated by Bin Cloud Microphysics Model
Megumi OKAZAKI1#+, Kosei YAMAGUCHI1, Tomoro YANASE2, Eiichi NAKAKITA1
1Kyoto University, 2RIKEN Cluster for Pioneering Research
The shape of the raindrop size distribution (DSD) changes in time and space due to the influence of environmental fields within the precipitation system and by following various cloud microphysical processes. Previous studies have suggested that the bimodal DSD is formed when the collisional breakup process reaches equilibrium. On the other hand, observation-based studies indicated that convective activity plays an important role in forming the bimodal DSD. However, it is difficult to quantitatively investigate the particle-level variability that constitutes the DSD through observation. Therefore, in this study, we simulated multicellular convection in two dimensions with the bin method to investigate the spatial variation of DSDs during the life cycle of multicellular convection. The bimodal DSD appeared in the region between updraft and downdraft in the mature phase of the multicellular convection. Additionally, the altitude at which the bimodal DSD existed had blowing inflows that entered the precipitation system. The particles constituting the maximum advected to the location where the bimodal DSD appeared because of the inflow. The particles constituting the local maximum fell against the updraft, and their number density increased at this location. On the other hand, the number density decreased because the particles constituting the local minimum were difficult to be advected by the inflow and fell under the influence of the updrafts. We considered that horizontal and vertical size sorting occurred, resulting in bimodal DSDs. It will be necessary to include a breakup process and to check the consistency with observed data from now on.
AS83-A023
Contrasts in the Microphysical Attributes of Polluted and Non-polluted Rainy Days Over Taiwan
Balaji Kumar SEELA1,2+, Jayalakshmi JANAPATI1, Pay-Liam LIN1#
1National Central University, 2Academia Sinica
Air pollution, caused by nature and anthropogenic activities, has a tremendous impact on the Earth’s climate and hydrological cycle. Taiwan, which is located in the East Asian region, is strongly influenced by air pollution. The present work aims to understand the impact of air pollution on precipitation and its microphysical processes during different seasons in Taiwan. In this study, ground-based disdrometers, Global Precipitation Measurement Dual-frequency Precipitation Radar (GPM DPR) and Modern-Era Retrospective analysis for Research and Applications, Versions2 (MERRA-2), re-analysis, and other auxiliary data sets are used to delineate the cloud and rain microphysical attributes between polluted and non-polluted rainy days. The results demonstrated a clear distinction in the RSDs characteristics between the polluted and non-polluted rainy days. The microphysical features of polluted and non-polluted rainy days are examined using the contour frequency by altitude diagrams of rainfall rate, radar reflectivity, and raindrop size distributions. Furthermore, the raindrop size distribution empirical (like Z-R, μ – λ, Dm-R, Nw-R etc.,) that are handy for the quantitative precipitation estimations and cloud modeling simulations are also established for polluted and non-polluted rainy days.
AS83-A032
Study on the Relationship Between Barrier Jets, Topography and Severe Precipitation in Northwestern Taiwan Under Meiyu Frontal Conditions
Jou-Ping HOU1#+, Li-Zhen SU2
1National Defense University, 2Air Force Institute of Techology
Along the northwestern coast of Taiwan, when the Meiyu front passes, the wind speed is often increased due to the influence of topography and merges with the prevailing wind field, resulting in a low-level jet strong wind area, causing severe precipitation. Past studies have found that low-level jets (about 1 km high) under certain conditions, called barrier jets, strongly affect heavy rainfall in northern Taiwan. This study uses the WRF model to simulate the intensity and range of barrier jets with and without topographic conditions in northwestern Taiwan, and then analyzes the main reasons and physical mechanisms that caused severe precipitation in northwestern Taiwan in this case. Research results show that after the Meiyu front touched northern Taiwan in the early morning of June 2, very heavy rain fell in Keelung and the north coast area in just 12 hours. The reason for the heavy precipitation may be related to the intensification of the barrier jet that occurs near the surface when the main body of the front moves toward the Snow Mountains in northern Taiwan. During the movement of the main body of the front over the sea, due to the intensification of the barrier jet, a cyclonic circulation around the jet area, accompanied by the instability of the temperature gradient and the enhancement of the positive potential vortex anomaly area, was the reason for the severe precipitation in this case. Simulations that remove topography show that similar barrier jets cannot appear in northwestern Taiwan, which would significantly change the intensity and range of precipitation.
Session Chair(s): Dipesh RUPAKHETI, Nanjing University of Information Science & Technology, Shovan Kumar SAHU, Meteorological Service Singapore, Hongliang ZHANG, University of Shanghai for Science and Technology
AS08-A048
| Invited
An Operational Air Quality Model for Southeast Asia
Shovan Kumar SAHU1#+, Zhong Yi CHIA2, Boon Ning CHEW2, Chee-Kiat TEO2, Paul AGNEW3, Florent MALAVELLE3, Matthew HORT3
1Meteorological Service Singapore, 2Centre for Climate Research Singapore, 3Met Office
The maritime and continental Southeast Asia experience biomass burning smoke haze incidents recurrently which pose significant impacts on regional environment and public health. Since 2013, Meteorological Service Singapore (MSS) has been developing air quality modeling capabilities in collaboration with the UK Met Office (UKMO) based on Numerical Atmospheric-dispersion Modelling Environment (NAME). The latest iteration of NAME air quality (NAME-AQ) forecast system developed by CCRS/MSS can provide a 48-hour advance air quality forecast for the region and it has been running in real-time since September 2023. This presentation will provide an overview of this system and its performance. The inputs to NAME-AQ model include a high resolution (1 km x 1 km) local emission inventory of Singapore and nearby regions, high-resolution (0.25 km x 0.25 km) landcover and land-use data used for estimating Global Fire Assimilation System (GFAS) biomass burning smoke emissions, Regional Emission Inventory in Asia (REASv3.2) regional anthropogenic emission inventory (0.25° x 0.25°), Copernicus Atmosphere Monitoring Service (CAMS) regional biogenic emissions (0.25° x 0.25°) and Hemispheric Transport of Air Pollution (HTAPv2) regional shipping emissions (0.1° x 0.1°). The European Centre for Medium-Range Weather Forecasts (ECMWF) meteorological forecasts and the CAMS lateral boundary conditions are used to drive the model. Model outputs are now generated for the six criteria pollutants used to determine Singapore’s Pollutant Standard Index (PSI), namely particulate matter (PM10), fine particulate matter (PM2.5), Sulphur dioxide (SO2), Carbon monoxide (CO), Ozone (O3) and Nitrogen dioxide (NO2). The model can capture the concentration peaks due to transboundary smoke haze, as well as local air pollution episodes such as ozone exceedance. Model outputs over Singapore are bias corrected and provided to MSS and ASEAN Specialised Meteorological Centre (ASMC) forecasters who will assess the smoke haze situation and provide the appropriate public advisory.
AS08-A041
| Invited
Commute Exposure to Ultrafine Particles, Black Carbon and Particulate Matters in Nanjing Suburb, China
Dipesh RUPAKHETI1#+, Wenjing ZHANG1, Jingyi LI1, Xiaofang LI1, Yuchen JI1, Maheswar RUPAKHETI2, Jianlin HU1
1Nanjing University of Information Science & Technology, 2Helmholtz Centre Potsdam
This study assessed the exposure of commuters to ultrafine particulate matter (UFP), black carbon (BC), and particulate matter (PM) concentrations in a diverse traffic microenvironment over a 3-km, high-traffic section in suburban Nanjing, China. We evaluated the mean exposure concentration difference between distinct special cases (peak and off-peak hours, weekdays and weekends, severe dust days and holidays) in five traffic microenvironments of subway, bus, taxi, e-bike (electric motorbike) and bicycle. The bicycle commuters were exposed to the highest PM (PM1, PM2.5, PM10) concentration, the bus commuters to the highest BC concentration in the morning peak hours (3.4±3.0 μg/m3), and the bus and taxi commuters to the highest UFP number concentration. The subway (metro) commuter had the lowest mean exposure concentration of PM, BC, and UFP number during the rides. Regarding the total inhaled dose of PM2.5, it was highest to the bicycle commuters (16.25 μg/km) followed by e-bike (1.98 μg/km), bus (1.28 μg/km), taxi (0.69 μg/km), and subway commuters (0.45 μg/km). The exposure levels of PM2.5 (114.6 μg/m3) and BC (1826 ng/m3) on weekdays were higher than those on weekends (170% and 158%, respectively). PM2.5, PM10 and BC concentrations on dust days were significantly higher than those on weekdays and holidays, with the mean exposure concentration of PM10 (1299.2±1285.8 μg/m3) in the evening peak of dust days was 803% and 994% higher than the mean concentrations on weekdays and holidays, respectively.
AS08-A011
Health Impact Estimation of Ground-level Ozone Concentration in Delhi, India: A Four-year Study Using Generalized Linear Model
Pareshbhai Dineshbhai PARMAR1#+, Mina CHANDRA2, Shubham SHARMA1, Sri Harsha KOTA1
1Indian Institute of Technology Delhi, 2Dr. Ram Manohar Lohia Hospital
The ambient concentrations of criteria pollutants across the urban areas of India often exceed the standards. The primary objective of the study is to assess the impact of ground level ozone (O3) exposure on public health in Delhi, India. This was accomplished by examining the association of O3 concentrations with hospital admissions for various respiratory and cardiovascular diseases. The researchers utilized a gridded four-year dataset (2016-2019) containing O3 concentrations (MDA8) obtained from the WRF-Chem model, which was then linked to gridded daily hospital inpatient data of different cardiovascular and respiratory diseases: Bronchial Asthma, Tuberculosis, CAD, COPD, Hypertension, and Diabetes Mellitus. To analyze the associations between O3 concentrations and hospital admissions a Generalized Linear Model (GLM) was used. The results of the study demonstrated that CAD exhibited the highest relative risk (RR: 1.220) associated with O3 exposure, followed by DBM (RR: 1.151), HTN (RR: 1.006), and COPD (RR: 1.019). Furthermore, the disease, age, and gender-specific combined relative risk (CRR) has been calculated. They observed the most significant increase in CRR (3.43%) on the 3rd lag day. Regarding gender-specific effects, the study revealed that male patients displayed slightly higher sensitivity to O3 exposure. Additionally, the study highlighted that patients aged less than or equal to 60 years were notably more susceptible than those over 60 years of age. The greatest disparity between CRR for both age groups was observed on the 3rd lag day (approximately 2.8%). The findings of the study align with existing literature on the age-specific impact of O3 exposure on respiratory health. In summary, this study provides valuable insights into the health risks posed by O3 exposure in Delhi over a four-year period and serves as a valuable reference for future researchers conducting air pollution health risk assessments in urban settings.
AS08-A007
Atmospheric Composition Responses to Anthropogenic Emission Changes
Hongliang ZHANG1#+, Yele SUN2, Hongli WANG3, Peng WANG4
1University of Shanghai for Science and Technology, 2Chinese Academy of Sciences, 3Shanghai Academy of Environmental Sciences, 4Fudan University
Air pollution remains a pressing global issue, prompting nations worldwide to implement various mitigation strategies, often targeting specific pollutants such as particulate matter. While these strategies are crafted with the best intentions, they sometimes yield unwanted effects, including alterations in atmospheric chemical compositions leading to phenomena like ozone increase or unforeseen climate impacts. The DFG-NSFC project titled "Air pollution over China and the unwanted effects of mitigation strategies" aims to understand why ozone is increasing in response to air pollution mitigation strategies. In the project, the established Sino-German collaboration of atmospheric scientists proposed to analyze the key factors that have driven surface ozone concentrations in response to the imposed emission control measures. After three-year hard work, the project is coming to an end and more than 10 papers were published supported by the project. This presentation aims to summarize the outcomes from the Chinese team, including Fudan University, Institute of Atmospheric Physics, Chinese Academy of Sciences, and Shanghai Academy of Environmental Sciences.
AS08-A006
Secondary Pollution and Its Health Effects in Response to Urbanization
Zhaolei ZHANG1+, Hongliang ZHANG2#, Peng WANG1
1Fudan University, 2University of Shanghai for Science and Technology
Rapid urbanization and industrialization have resulted in diverse anthropogenic activities and emissions between urban and non-urban regions, leading to varying levels of exposure to air pollutants and associated health risks. However, endeavors to mitigate air pollution and health benefits displayed considerable heterogeneity across different regions. Therefore, comprehending the changes in air pollutant concentrations and health impacts within the urbanization context is imperative for promoting environmental equity. This paper uses GDP- and population-weighted methods to distinguish anthropogenic emissions from urban and non-urban regions in China, and quantified their contributions to secondary pollutants using the Community Multiscale Air Quality (CMAQ) model in 2010 and 2019. Non-urban anthropogenic emissions are the main contributor to secondary air pollution caused by anthropogenic activities in China. From 2010 to 2019, non-urban anthropogenic emissions of NOx and VOCs decreased by 34% and 25%, respectively. However, urban emissions increased by 37% for NOx and 22% for VOCs in China. These changes led to an increase in O3 concentration sourced both urban and non-urban regions (18% and 105%, respectively). NO2 sourced non-urban and urban anthropogenic emission decrease 18% and increase 65%. The health exposure risk of O3 in non-urban populations and NO2 in urban populations are higher than other residents in China. This study emphasizes the importance of balancing urban and non-urban costs of emissions reduction and health benefits in combating secondary pollution and promoting environmental justice in the rapid urbanization.
AS08-A003
NMVOC Flux in China’s Megacity
Xianjun HE1+, Bin YUAN1#, Yibo HUANGFU1, Xiaoxiao ZHANG1, Thomas KARL2, Martin GRAUS2, Marcus STRIEDNIG2
1Jinan University, 2University of Innsbruck
We conducted urban non-methane volatile organic compound (NMVOC) flux measurements in Beijing, a megacity in China, using the eddy covariance technique with a Proton transfer reaction time of flight-mass spectrometer during the summer of 2021. We analyzed the NMVOC flux dataset by using the positive matrix factorization method to investigate prominent urban NMVOC emission sources. The result emphasizing the importance of vehicle-related emissions for NMVOC emissions was found to be declining, while the demand for eliminating volatile chemical product emissions was increasing. The study also highlighted the unrecognized significance of urban forests in air pollution, with strong temperature dependence observed for biogenic emissions.
Session Chair(s): Ralf TOUMI, Imperial College London, Kun-Hsuan CHOU, Chinese Culture University
AS13-A011
| Invited
IRIS: A Stochastic Global Tropical Cyclone Model
Ralf TOUMI#+, Nathan SPARKS
Imperial College London
Assessing tropical cyclone risk on a global scale given the infrequency of landfalling tropical cyclones (TC) and the short period of reliable observations remains a challenge. Synthetic tropical cyclone datasets can help overcome these problems. Here we present a new global dataset created by IRIS, the ImpeRIal college Storm Model. IRIS is novel because, unlike other synthetic TC models, it only simulates the decay from the point of lifetime maximum intensity. This minimises the bias in the dataset. It takes input from 42 years of observed tropical cyclones and creates a 10,000 year synthetic dataset of wind speed which is then validated against the observations. IRIS captures important statistical characteristics of the observed data. T
AS13-A025
Tropical Cyclone Size Analysis and Forecast by Ensemble Forecast System
Kun-Hsuan CHOU1#+, Chi-Chang LI2
1Chinese Culture University, 2Graduate Institute of Earth Science
Tropical cyclones (TCs) are highly destructive weather systems, and their size is closely related to the extent of the disasters they cause. Therefore, timely monitoring and prediction of changes in the TC wind field structure are crucial. Due to the relative lack of actual observational data around storms, forecasters and researchers have begun considering the use of model data to estimate TC size and structure. This study utilizes two ensemble model datasets, NCEP GFS/EPS and CWA WEPS, to quantitatively calculate the TC size (R34, radius of 34-knot surface wind). The results are compared with MTCSWA, taking into account different data sources such as JTWC Best Track and ASCAT as benchmarks. The findings show that, at the initial time, EPS has a smaller R34 error compared to MTCSWA. In terms of forecast fields, WEPS has smaller errors in the early and mid-period (f00–f84), while GEFS outperforms WEPS in the late period (f90–f108). Overall, WEPS tends to underestimate R34 compared to JTWC; GEFS tends to overestimate on the east side, and MTCSWA generally underestimates on the east side of storms. Additionally, EPS, compared to MTCSWA, captures more trends in asymmetric wind field structure changes but often overestimates the asymmetry, while MTCSWA tends to underestimate. In terms of R34 spread and errors of the ensemble model, from f00 to f48, WEPS has excessive spread, overestimating uncertainty, while GEFS has insufficient spread, underestimating uncertainty. The results of this study, utilizing ensemble model data for an objective analysis of TC size, contribute to understanding the differences between different models or analysis data. It also provides a reference for future related research and forecasting.
AS13-A057
A Geographical Approach for Localized Tropical Cyclone Activity and Risk Factors
Eunhee GIL+, Youngeun KIM, Namyoung KANG#
Kyungpook National University
To minimize the risks from tropical cyclones (TCs), the quantification and regular monitoring of TC activities are strongly needed. While the accumulated cyclone energy (ACE) (Bell et al., 2000) has been widely used for examining the level of basin-wide TC activities, the conventional ACE does not discriminate the regional characteristics of TC risks. By introducing a point-wise version of ACE, this paper proposes a geographical approach to the risk map for TCs. Here, the alternative metric is named the localized ACE (LACE), which interprets the TC risk directly felt by the local residents. Annual LACE measures TC activity by merging the quantities of frequency, intensity, and duration factors, which contribute to the local TC activity in a year. In conjunction with LACE, a concept of LACE potential is also proposed to understand the contributions of the factors to LACE. The LACE potential enables the comparison of the contributions by the factors at a specific location, and the identification of the characteristics of the regional TC risks. To demonstrate the efficacy of the indices, i.e., LACE and LACE potential, this paper provides the response of the local TC activities to El Niño–Southern Oscillation and the Global Mean Sea Surface Temperature in the western North Pacific, and confirms the value of these indices.
AS13-A073
Tropical Depression Aere (2022) and Flooding in Western Japan: The Role of Atmospheric River
Chaehyeon Chelsea NAM1#+, Chanil PARK2, Michael BELL3, Ming-Jen YANG4, Kazuhisa TSUBOKI5,6
1Florida State University, 2Boston College, 3Colorado State University, 4National Taiwan University, 5Nagoya University, 6Yokohama National University
On the morning of July 5, 2022, Tropical Depression (TD) Aere made landfall at Nagasaki, Japan, inducing heavy rainfall. Despite its initial classification as a weak tropical storm with a central sea level pressure of 1,000 hPa and an asymmetric structure, TD Aere's aftermath revealed flash floods across Kyushu island. Our investigation posits that the continuous moisture transport from the atmospheric river played a pivotal role in the flooding, challenging conventional notions about weak tropical storms. TD Aere's elongated structure along the periphery of the western North Pacific High (WNPH) resembled an atmospheric river, with plume-like moisture flux originating from the southwest Warm Pool region. The unusual persistence of convection over Kyushu even after Aere's landfall could be attributed to sustained latent heat support. This ongoing research delves into the intricate interactions among TD Aere, the confluence region between Aere and the WNPH, and the atmospheric river. Leveraging data from the PRECIP/TAHOPE/TPARC-II field campaign, satellite observations, and reanalysis datasets enhances our comprehensive multi-scale analysis. This study aims to unravel the nuanced dynamics contributing to the unexpected impact of TD Aere, shedding light on the broader implications for understanding and predicting extreme weather events.
AS13-A049
Impact of Initial Intensity Error on Simulated Tropical Cyclone Track Over the Western North Pacific
Kyoungmin KIM+, Dong-Hyun CHA#
Ulsan National Institute of Science and Technology
To obtain accurate tropical cyclone (TC) information, high-resolution simulations based on numerical models are necessary. Regional models can simulate TCs at high resolution, and through decades of research and development, they have been consistently improved. However, uncertainties in the global model data used for initial and boundary conditions can lead to errors in TC simulations. In this study, TC simulations were conducted to analyze the impact of error in the initial condition on the performance of its simulation. We targeted TCs for 2006-2018 from June to November. Selected cases were those with TC maintaining at least tropical storm (TS) intensity for three days. The Weather Research and Forecasting (WRF) model was used for conducting TC simulations, and the National Centers for Environmental Prediction (NCEP) Final Operational Global Analysis data were used for initial and boundary conditions. We used the Regional Specialized Meteorological Center (RSMC) Best Track data for verification of simulation results. Analyzing 1128 simulated results over 72 hours, the initial intensities of the selected cases were mostly underestimated compared to RSMC best track. For cases with an initial intensity error of less than -10 m/s, the track position errors (TPEs) of TCs were significantly larger than in other cases. Additional simulations were conducted to correct the initial intensity for cases with initial errors less than -10 m/s and 72-hour TPE exceeding 230.9 km which is the average of 72-hour TPEs. The dynamic initialization (DI) technique was applied to initialize the initial TC intensity similar to the RSMC best track, and the DI results were compared with the prior WRF simulations (CTL). DI showed smaller errors for the TC track compared to CTL, with a 14.6 % improvement in track simulations over 72 hours.
AS13-A050
Evaluation of NCEP Global Forecasting System (GFS) Performance in Predicting Landfalling Tropical Cyclone Rainfall in Korea
Jiwon HWANG1+, Dong-Hyun CHA1#, Minkyu LEE2
1Ulsan National Institute of Science and Technology, 2Korea Institute of Energy Research
It is essential to understand how accurate current forecasting systems are in predicting tropical cyclones (TCs) and associated rainfall to improve mitigation strategies and preparedness. This study examined the impact of storm-related errors on rainfall in landfalling TCs over Korea from 2015 to 2022 by Global Forecast System (GFS) model from the National Centers for Environmental Prediction (NCEP). Most TC track errors were found to be skewed to the left, suggesting that TCs passing over the coast could be located closer to land, increasing average rainfall in the Korean Peninsula. However, even when daily forecasts showed minor errors in track and intensity, TC rainfall still exhibited significant errors in distribution and intensity. These discrepancies can occur when the simulated TCs do not adequately reflect their interaction with the environment. In the GFS model, TCs are characterized by a strong emphasis on storm-centered winds, and this characteristic disrupts the TC-jet interaction and thus weakens the TC outflow. This weakened TC outflow can result in locally weak upper-level winds, reducing vertical wind shear, mid-level updrafts, and upper-level divergence. Thus, these results suggest the sources of error (i.e., storm structure) in mid-latitude TC rainfall forecasts, allowing model developers and forecasters to improve storm precipitation forecasts for this region.
Session Chair(s): Xin XU, Nanjing University
AS34-A006
| Invited
Current Understanding of Gravity Wave Effects in the Atmosphere and Implications to Their Parameterizations
Kaoru SATO#+
The University of Tokyo
Atmospheric gravity waves are one of major atmospheric waves along with Rossby waves. They have been positioned as a difficult phenomenon to study both observationally and numerically due to their small spatio-temporal scales. However, redistribution of momentum by gravity waves is essential to understand the structure, variability, and momentum budget of large-scale phenomena, as it is always incorporated as parameterizations in numerical models for weather and climate prediction. In the past decade, studies using high-resolution observations and high-resolution atmospheric general circulation models that directly capture gravity waves, as well as diagnostic studies using reanalysis data, have greatly advanced our understanding of the global distribution, seasonal variations, dynamical properties, and effects of gravity waves on large-scale fields of the atmosphere. At the same time, problems with parameterizations used in weather and climate prediction models that need great improvement have become elucidated. The role of horizontal propagation of gravity waves, which is not represented in most current parameterizations, and the compensation effect by Rossby waves when the gravity wave forcing represented by the parameterization is excessive will be also discussed.
AS34-A003
| Invited
A Possible Mechanism for the Stratospheric Influence on Tropical Cyclone Intensity: Downward Control by Gravity Waves
Yuan WANG1,2#+, Xu WANG1
1National University of Defense Technology, 2Nanjing University
A possible mechanism for the influence of the stratosphere on the intensity of tropical cyclones (TCs) is found using idealized experiments with adjustment of the damping layer depth of the model. The damping layer set in the lower stratosphere can absorb the stratospheric gravity waves (SGWs) generated by TCs, and the absorbed SGWs can influence the background wind by SGW drag. Therefore, the SGWs can accelerate background wind in the stratospheric circulation after they propagate into the damping layer. The accelerated stratospheric radial wind can promote upwelling under the damping layer, and this upwelling in the tropopause can result in adiabatic cooling. The cooling decreases the temperature around the tropopause and increases the center pressure of the TCs. Therefore, the intensity of the TCs will be weakened by the SGW activity. The above process found in TCs is similar to the stratospheric downward control of the large-scale atmospheric circulation, and it shows the important role of the SGWs in mesoscale systems that results from wave–flow and stratosphere–troposphere interactions. Accurate simulation of the stratosphere is critical for the prediction of TCs.
AS34-A027
Do We Need to Parameterize Mesoscale Surface Turbulent Fluxes for 50KM GCMs?
Min-Seop AHN1,2#+, Andrea MOLOD1
1NASA Goddard Space Flight Center, 2University of Maryland
Air-sea interaction plays a crucial role in the Earth system by exchanging heat, moisture, momentum, aerosols, and gases between the atmosphere and ocean. Recent high-resolution observational and modeling studies have revealed that mesoscale and submesoscale (approximately 1-500km) air-sea interaction is particularly active in ocean eddy-rich regions (e.g., western boundary current regions) and influences the downstream development of synoptic-scale weather systems as well as the local atmosphere and ocean. Despite the growing understanding of the importance of mesoscale and submesoscale air-sea interaction, most state-of-the-art General Circulation Models (GCMs), including Goddard Earth Observing System GCM (GEOS-GCM), do not adequately represent/parameterize the mesoscale/subgrid-scale air-sea interaction. To assess the need for a parameterization of subgrid-scale surface turbulent fluxes in 50km GEOS-GCM, we utilize a high-resolution GEOS-GCM coupled with the Massachusetts Institute of Technology general circulation ocean model (GEOS-MITgcm) simulation (6km for atmosphere and 3km for ocean). The surface turbulent fluxes from GEOS-MITgcm can be decomposed into grid-scale and subgrid-scale fluxes by Reynolds averaging on a larger domain (i.e., 50km). By computing the ratio of subgrid-scale fluxes to the total fluxes on 50km coarsen domains, we assess the importance of a parameterization of mesoscale/subgrid-scale surface turbulent fluxes on 50km domains.
AS34-A001
Extension and Evaluation of University of Washington Moist Turbulence Scheme to Gray-zone Scales
Wei WEI#+
China Meteorological Administration
With the rapid improvement in computational resources, it has become possible to structure numerical weather model simulations to use sub-kilometer grid spacing. Traditional turbulence-mixing closures have become obsolete within the context of the gray zone of turbulence. Here, a new scale-aware algorithm (SA-UW) is developed based on the UW (University of Washington Moist Turbulence) scheme. By dividing both the local and nonlocal vertical turbulence flux into sub-grid and resolved parts, the partition of sub-grid turbulence is tuned by a set of well-acknowledged scale-dependent relationships. Idealized simulations confirm that the newly developed scheme can adequately reproduce sub-grid turbulence transport at gray-zone scales. The inclusion of a nonlocal transport term in the SA-UW scheme is essential, as it vastly improves the distribution and intensity of coherent structures. The SA-UW scheme recovers the conventional UW scheme when grid spacing is larger than the turbulence length scale, thereby evincing the sale-aware capability of the new method. For real-case simulations, the SA-UW scheme can capture the diurnal cycle and provide a more accurate vertical structure of temperature and humidity.
AS34-A017
Understanding of Effects of PBL Schemes on the Prediction of an Extreme Precipitation Event on 30 July 2023 in Northern China
Ziqi FAN1#+, Ming XUE2
1Nanjing University, 2The University of Oklahoma
During 29 July - 1 August 2023, an extreme precipitation event occurred in northern China, with a maximum accumulated rainfall of more than 1000 mm over four days. The sensitivity of predicted rainfall to initialization time and physics parameterizations are investigated through convection-allowing simulations. Thirty-six simulations are conducted using WRF with different initialization times, microphysics, and PBL schemes. Most simulations produce maximum rainfall at or exceeding the observed amount. Among simulations, PBL scheme has the most significant impact on simulated precipitation, including location and maximum amount. YSU and MYNN schemes behave similarly while ACM2 perform quite differently. ACM2 simulation overpredicts precipitation intensity with most of the precipitation being shifted to the northeast. The residual low-level cyclone from a land-falling typhoon in ACM2 moves faster towards the northwest than that in YSU. This influences convergence location between the cyclone and the extratropical high ridge to its northeast, and interaction between the cyclone with the Taihang and Yanshan Mountains. Consequently, the location and intensity of precipitation are affected. Analysis of wind fields and turbulent mixing coefficient profiles in YSU and ACM2 reveals that differences in parameterizations of free tropospheric (FT) momentum mixing coefficients are primary contributors to precipitation differences. Specifically, the turbulent mixing in free troposphere within ACM2 is stronger than that in YSU. This leads to downward transport of higher-level momentum and strengthening of steering-level winds, resulting in cyclone faster northwestern movement, the northwestward positioning of the cyclone circulation, and hence precipitation location and amount differences via the interactions described above. Simulations altering a key parameter and other treatments to FT turbulent mixing within both schemes confirms the key effects of FT turbulent mixing in PBL schemes. This improved understanding of the relationship between parameterized turbulence mixing and predicted extreme precipitation enables us to propose potential solutions for improving extreme precipitation forecasting.
AS34-A019
Mountain-facilitated Downward Transport of Volcano Plumes Exacerbates Air Pollution Over Arequipa, Peru
Xiao-Ming HU1#+, Ming XUE1, Tingting QIAN2, Hector Mayol NOVOA3, Lan GAO1, Jose Luis TICONA JARA4
1The University of Oklahoma, 2Chinese Academy of Meteorological Sciences, 3Universidad Nacional de San Agustín de Arequipa, 4National Service of Meteorology and Hydrology of Peru
Severe air pollution plagues Arequipa Peru due to anthropogenic and natural emissions. Persistent volcano outgassing in the vicinity lead Arequipa ranked among the largest SO2 sources in the world. Since the volcano plumes mostly exist in the free troposphere and stratosphere where horizontal transport acts rather quickly, previous studies mostly focused on global scale impact of volcano plumes. Whether these plumes can be transported to near the surface and affect ambient air quality barely gets research attention. For the first time this study using WRF-Chem simulations to reveal that in the presence of favorable meteorological conditions, the plume from volcano Sabancaya can be transported to Arequipa through a series of advection and dispersion processes: 1), in presence of northerly/northwesterly winds the free troposphere plume from Sabancaya is captured by mountain Chachani and transported downward to Arequipa by nighttime downstream gravity wave. The extent of downward penetration of plume depends on the free troposphere winds and stability. Often the plume is downward transported to above the boundary layer over Arequipa during nighttime. 2), on the following day, convective boundary layer growth further transports the plume above the boundary layer to near the surface through vertical mixing processes, thus exacerbating ambient air pollution over Arequipa. This modeling study discovers a mechanism of how the volcano plumes exacerbate air pollution over Arequipa using SO2 as a tracer. The quantitative contribution of volcano plumes to ambient aerosol pollution needs to be examined using model simulations including aerosol processes and more accurate volcano emissions.
AS34-A009
Investigation of Physical Processes Influencing Fog Dynamics Through WRF Simulations: A Case Study in Delhi's Dense Fog Episode
Anie K. LAL#+, Ravi Kumar KUNCHALA, Manju MOHAN
Indian Institute of Technology Delhi
The remarkable development of the capital city, Delhi, India, has resulted in rapid urbanization, giving rise to urban heat islands and dry islands. In this study, we present a dense radiation fog event from January 2021 using the Weather Research and Forecasting (WRF) model to demonstrate the effects of urbanization on fog due to changes in Land Use Land Cover (LULC). We performed various sensitivity experiments by accounting for the nesting configurations, vertical and spatial resolutions, microphysics, Boundary Layer (PBL) representations, Land Surface Models (LSM), radiation schemes, LULC, and Initial and Boundary Conditions (ICBC), alongside considering fog gravitational settling. The evaluation of 32 parameterization combinations underscores the effectiveness of the WSM7 microphysics, MYNN2.5 PBL, PX-LSM, and CAM-radiation schemes in accurately capturing the dense fog event. Comparing the control run (CNTL) and experimental run (EXP – replacing only the LULC of the study region by modifying the land cover) demonstrates the role of urbanization in the advancement of fog dissipation by 1-2 hours. We primarily attribute near-surface soil moisture as a decisive factor influencing the early lifting and dissipation time of the fog layer by affecting surface fluxes (quantified by Bowen Ratio), turbulent kinetic energy (TKE), and expediting the heating of the boundary layer (<500m from the land surface). Further results reveal that urbanization alters the LWC profile and fog structure, and these changes are more prominent in areas converted from irrigated croplands to urban and built-up areas. The decreasing liquid water path during the dissipation phase in the CNTL run explains the occurrence of 'fog holes' above urban areas in the early morning hours. This phenomenon is expected to grow if urban areas continue to develop in the future.
Session Chair(s): Richard ECKMAN, National Langley Research Center, Jun WANG, The University of Iowa
AS59-A054
Sensitivity of Satellite and Model Tropospheric NO2 Columns to Diurnal Variations in NOx Emissions Over South Korea
Seunghwan SEO1+, Si-Wan KIM1#, Kyoung-Min KIM1, Andreas RICHTER2, Kezia LANGE2, John BURROWS2, Junsung PARK3, Hyunkee HONG4, Hanlim LEE3, Jung Hun WOO5, Jhoon KIM1,6
1Yonsei University, 2University of Bremen, 3Pukyong National University, 4National Institute of Environmental Research, 5Konkuk University, 6Korean Academy of Science and Technology (KAST)
Nitrogen oxides (NOx as sum of NO and NO2) play crucial roles in the production of tropospheric ozone and the formation of nitrate aerosols. Utilizing environmental satellites such as GOME, SCIAMACHY, OMI, and TROPOMI enables spatially continuous observations of NO2, substantially enhancing our understanding of sources, emissions, and atmospheric chemistry. However, these measurements are limited to once per day or even less frequently. After the launch of Geostationary Environmental Monitoring Spectrometer (GEMS) in February 2020, it became possible to obtain hourly measurements of NO2 over Asia from space. For the retrieval of NO2 tropospheric vertical column densities from satellite observations, NO2 vertical profiles from chemical transport models are utilized. In this study, we conducted Weather Research and Forecasting coupled with Chemistry (WRF-Chem) model simulations employing multiple emission inventories with different diurnal NOx emission profiles. Changes in diurnal NOx emission profiles not only influenced temporal patterns but also impacted the absolute amounts of model NO2 columns. We further analyzed and compared the retrieved GEMS NO2 columns with the various WRF-Chem results to investigate the impact of diurnal NOx emission variations on satellite retrievals.
AS59-A053
| Invited
A New Era of Air Quality Monitoring from Space Over North America with TEMPO: Commissioning and Early Nominal Operation Results
Xiong LIU1#+, Kelly CHANCE1, Raid SULEIMAN1, John HOUCK1, John DAVIS1, Gonzalo GONZÁLEZ ABAD1, Caroline NOWLAN1, Huiqun WANG2, Heesung CHONG1, Weizhen HOUCK1, Kevin DAUGHERTY3, Dave FLITTNER3, Christopher CHAN MILLER4, Juseon BAK5, Jim CARR6, Crystal FENN3, David ROSENBAUM3, James SZYKMAN7, Michael NEWCHURCH8, Ronald COHEN9, Aaron NAEGER8,10, Zolal AYAZPOUR1, Christopher BROWN3, Laurel CARPENTER1, Zachary FASNACHT11, Jean FITZMAURICE1, Jeffrey GEDDES12, David HAFFNER11, Jay HERMAN11, Joanna JOINER11, Laura JUDD13,3, K. Emma KNOWLAND14, Nischal MISHRA15, Robert NEECE3, Ewan O'SULLIVAN1, R. Bradley PIERCE16, Wenhan QIN11, Eric ROBACK3, Justin STRICKLAND3, Robert SPURR17, Lukas VALIN7, Alexander VASILKOV18, Eun-Su YANG18
1Center for Astrophysics | Harvard & Smithsonian, 2Smithsonian Astrophysical Observatory, 3NASA Langley Research Center, 4Harvard University, 5Pusan National University, 6Carr Astronautics, 7U.S. Environmental Protection Agency, 8University of Alabama in Huntsville, 9University of California Berkeley, 10National Aeronautics and Space Administration, 11NASA Goddard Space Flight Center, 12Boston University, 13National Center for Atmospheric Research, 14Universities Space Research Association, 15John Hopkins University, 16University of Wisconsin-Madison, 17RT Solutions, 18Science Systems and Applications, Inc.
We present an overview of the initial data products of TEMPO during its commissioning and early nominal operation and preliminary comparison with correlative satellite and ground-based observations. TEMPO is NASA’s first EVI and first host payload. It measures hourly daytime atmospheric pollution over North America from Mexico City to the Canadian oil sands, and from the Atlantic to the Pacific, at high spatiotemporal resolution (~10 km2 at boresight) from the geostationary (GEO) orbit. It uses UV/visible spectroscopy (293-493 nm, 538-741 nm) to measure O3 profiles including lower tropospheric O3 and columns of NO2, H2CO, SO2, C2H2O2, H2O, BrO, IO, as well as clouds aerosols, and UVB. TEMPO provides a tropospheric measurement suite that includes the key elements of tropospheric air pollution chemistry and captures the inherent high variability in the diurnal cycle of emissions and chemistry. The TEMPO instrument was built by Ball in 2018. It was integrated into the host commercial communication satellite Intelsat 40e (IS-40e) by Maxar. IS-40e was successfully launched on April 7 by a SpaceX Falcon 9 rocket on to the GEO orbit at 91°W. The TEMPO Instrument powered up for the first time on orbit in early June to start its commissioning. After a month of dry out and activation, TEMPO first light of solar and earth measurements occurred on July 31-August 2. Nominal operation started on 19 October 2023 after the commissioning phase and the post-launch acceptance review. Science data products are archived and distributed at NASA’s ASDC and will be released to the public in approximately February 2024 for L1b and in April 2024 for L2/3. TEMPO is part of a geostationary constellation to measure air quality along with GEMS (launched in Feb. 2020) over Asia and Sentinel-4 (to launch in 2024) over Europe.
AS59-A026
Diurnal Variations of Atmospheric HCHO According to GEMS: Validation, Intercomparison, and Implications
Weitao FU1+, Lei ZHU1#, Hyeong-Ahn KWON2, Rokjin J. PARK3, Song LIU1, Gitaek LEE3, Xicheng LI1, Yuyang CHEN1, Dongchuan PU1, Juan LI1, Xiaoxing ZUO1, Peng ZHANG1, Yali LI1, Zhuoxian YAN1, Tzung-May FU1, Xin YANG1
1Southern University of Science and Technology, 2University of Suwon, 3Seoul National University
Satellite HCHO observation, the short-lived intermediate oxidation product, is a robust indicator of regional VOC emissions. The launch of the Geostationary Environment Monitoring Spectrometer (GEMS) in 2020 marks a new era of air quality monitoring for the Asia-Pacific with hourly observations. Recently released GEMS HCHO observation offers unprecedented potential, provided that it can capture HCHO diurnal variations. Here we present the first study to evaluate year-round GEMS HCHO observations based on TROPOMI satellite and Pandora ground-based observations. Our study shows that GEMS HCHO is in exceptional agreement with TROPOMI (monthly r = 0.56–0.89 for all collocated regions; less than 20% difference for most areas in China, Korea, and mainland Southeast Asia); furthermore, it captures the diurnal HCHO variations observed by 10 Pandora spectrometers across Asia (r = 0.52–0.94) despite being 33% lower overall, which is common for satellite-ground comparisons and can be attributed to different retrieval sensitivities to the vertical distribution of HCHO. Diurnally, we find that GEMS HCHO does not show strong interannual differences for most regions in different seasons, further demonstrating its stability; HCHO diurnal variations in major urban areas are much stronger than biogenic-dominated areas, reflecting anthropogenic VOC emissions; GEMS also captures the change (2022-2021) of fire emissions estimated from GFED4s inventory in Southeast Asia during January to April. In addition, we also find overall larger weekday-weekend differences in middle-sized cities (e.g., Xi’an), compared to the most densely populated cities (e.g., Shanghai, Seoul). In summary, our study demonstrates the reliability of GEMS in capturing HCHO diurnal variations from biogenic, anthropogenic, and pyrogenic sources.
AS59-A018
Nitrous Acid (HONO) Retrievals from the Geostationary Environment Monitoring Spectrometer (GEMS)
Hyeji CHA1#+, Jhoon KIM1,2, Heesung CHONG3, Gonzalo GONZÁLEZ ABAD3, Dha Hyun AHN1, Sang Seo PARK4, Won-Jin LEE5
1Yonsei University, 2Korean Academy of Science and Technology (KAST), 3Center for Astrophysics | Harvard & Smithsonian, 4Ulsan National Institute of Science and Technology, 5National Institute of Environmental Research
Nitrous acid (HONO) is known to be the significant source of hydroxyl radicals (OH), impacting air quality and climate as a major oxidant in the atmosphere. Many studies have highlighted that the photolysis of HONO can produce substantial amounts of OH throughout the day. Despite the crucial role of HONO in tropospheric chemistry, more research is needed to improve understanding of global HONO budgets. To address this, we developed a prototype HONO retrieval algorithm from the Geostationary Environment Monitoring Spectrometer (GEMS). The retrieval algorithm comprises two major processes, commencing with the spectral fitting of UV spectral range (343-371 nm) using the direct fitting method to obtain the slant columns. Subsequently, the conversion of slant columns into vertical columns is achieved by applying the air mass factor. The last step involves background correction, wherein the slant column amounts of HONO included in the radiance reference spectrum are added to the differential slant columns. Enhancements of HONO resulting from wildfire events in Asia were detected using GEMS. Refining the GEMS HONO retrieval algorithm is expected to enhance our understanding of the diurnal cycle of HONO, along with tropospheric chemistry in Asia.
AS59-A025
Global Long-term (2005-2019) Trends in Formaldehyde Columns According to the OMI Satellite Instrument
Peng ZHANG1+, Lei ZHU1#, Gonzalo GONZÁLEZ ABAD2, Miller CHRISTOPHER2, Song LIU1, Xiaoxing ZUO1, Xicheng LI1, Yuyang CHEN1, Dongchuan PU1, Weitao FU1, Yali LI1, Juan LI1, Zhuoxian YAN1, Xin YANG1, Tzung-May FU1
1Southern University of Science and Technology, 2Center for Astrophysics | Harvard & Smithsonian
Satellite observations of formaldehyde (HCHO) columns provide a reliable proxy of highly reactive volatile organic compounds (VOCs). After correcting for temperature dependence, we find an increasing trend over most of the world from 2005 to 2014 but a decreasing trend in South America and the southwestern United States. From 2010 to 2019, the global HCHO column increased in smaller areas but still decreased in South America. Satellite observations of changes in HCHO columns in the North China Plain (+1.59 ± 0.40% a-1), the Pearl River Delta (+1.96 ± 0.76% a-1), north-central China (+2.74 ± 0.42% a-1), India (+2.10 ± 0.25% a-1), Southeast Asia (+1.96 ± 0.59% a-1), and the southwestern United States (-2.75 ± 0.80% a-1) are consistent with anthropogenic VOCs emission trends from 2005 to 2014. Comparing MODIS land cover data, we found that land cover types caused changes in HCHO columns over Northeast China (+1.56 ± 0.70% a-1), Southern China (+2.22 ± 0.46% a-1), Australia (+2.96 ± 0.90% a-1), South Africa (+1.36 ± 0.52% a-1), and Colombia (-1.80 ± 0.28% a-1) from 2005 to 2014. We also found that variations in HCHO columns in northeastern South America (-1.44 ± 0.28% a-1) and northern Canada (+5.54 ± 1.19% a-1) are mainly driven by wildfire emissions. Over India, the change in HCHO column (+2.00 ± 0.30% a-1) is consistent with the trend of anthropogenic VOCs from 2010-2019. The changes in HCHO columns in northern China (+1.56 ± 0.69% a-1) and eastern South America (-1.25 ± 0.41% a-1) are due to an increase in deciduous broadleaf forests.
AS59-A006
Seasonal and Diurnal Variations in XCO2 Characteristics in China as Observed by OCO-2/3 Satellites: Effects of Land Cover and Local Meteorology
Hengheng ZHAO1#+, Huizheng CHE1, Ke GUI1, Wenrui YAO1, Nanxuan SHANG1, Xutao ZHANG1, Lei LI1, Yu ZHENG1, Zhili WANG1, Hong-Li REN1,2, Hong WANG1, Junying SUN1, Jian LI1, Xiaoye ZHANG1
1Chinese Academy of Meteorological Sciences, 2China University of Geosciences
Monitoring the dynamics of atmospheric CO2 is crucial for enhancing comprehension of the carbon cycle. Using column-averaged dry-air mole fraction of CO2 (XCO2) data collected by the Orbiting Carbon Observatory (OCO)-2 and OCO-3 satellites during 2020–2021, this study explored seasonal and diurnal variations in XCO2 characteristics in typical land cover biomes in China, and investigated their relationships with meteorological drivers. Results showed that XCO2 products retrieved by OCO-2 and OCO-3 have good agreement with Total Carbon Column Observing Network measurements, with average deviations of 0.8 and 1.2 ppm, respectively. The satellite observations revealed XCO2 hotpots located mainly in central and eastern China, and areas of low XCO2 values in western China, with a seasonal curve that was highest (lowest) in spring (summer). The largest seasonal cycle amplitude (∼9 ppm) of XCO2 was observed in forest areas, highlighting its key role in carbon exchange. Additionally, XCO2 was found to have a near-sinusoidal diurnal pattern, characterized by rapid decrease in the early morning as photosynthesis resumed after sunrise, as indicated by the sun-induced chlorophyll fluorescence (SIF), a peak at around midday, and subsequent decrease as SIF increased after mid-afternoon. Urban regions had the highest diurnal cycle amplitude (∼6 ppm) among biomes. Statistical analyses revealed seasonal shift and nonlinear variation in the relationships between XCO2 and meteorological variables, suggesting that CO2 uptake is influenced by favorable humidity conditions. These relationships also provide insight into the sensitivity and adaptability of XCO2 to meteorological factors in diverse ecosystems such as savanna and grassland.
AS59-A062
Analysis of Relationship Between Carbon Dioxide and Nitrogen Dioxide for Urban Areas in East Asia Using GEMS and OCO-3 Data
Jaemin KIM+, Jin-Ah JANG, Sun Ju PARK, Ho-yeon SHIN, Eunyeong KIM, Yun-Gon LEE#
Chungnam National University
Anthropogenic fossil fuel use causes the emission of air pollutants, such as carbon monoxide and nitrogen oxides, along with greenhouse gases. The relationship between greenhouse gas and air pollutant concentrations varies by region, depending on various factors, such as anthropogenic activity patterns, type of fuel, and combustion efficiency. Analysis of the relationship between air pollutants and greenhouse gases over multiple regions can be performed by using satellite-based measurements. Launched in 2019, OCO-3 produces the Snapshot Area Map (SAM) for column-averaged carbon dioxide (XCO2) for several large cities around the world, and this data can be used to identify spatial variations in CO2 concentration due to anthropogenic activities in a relatively wide range of areas (~80 km ⨉ 80 km). Since OCO-3 overpasses at a flexible local time within +/- 5 hours from local noon, efforts for the temporal matching process are inevitable to analyze it together with air pollutant observation data measured from existing low-orbit satellite sensors. Geostationary Environment Monitoring Spectrometer (GEMS), mounted on GEO-KOMPSAT2B launched in 2020, is the world's first geostationary environmental satellite sensor and provides information on air pollutant concentrations by observing East Asia up to 10 times a day. Unlike low-orbit satellites, GEMS has the advantage of being able to be matched in close time with OCO-3 data. This study analyzed the relationship between NO2 and CO2 in various cities in East Asia using GEMS NO2 tropospheric column density data and OCO-3 SAM XCO2 data. The results of the NO2-CO2 relationship analysis for various urban areas are expected to help understand the anthropogenic emission characteristics of each region and further conduct a study on the estimation of CO2 emissions using NO2 data.
Session Chair(s): Shaojie SONG, Nankai University
AS16-A021
Surface Tension Measurement of Deliquesced Aerosol Particles
Masao GEN#+
Chuo University
The surface tension of aerosol particles can potentially affect cloud droplet activation. Hence, direct measurement of the surface tensions of deliquesced aerosol particles is essential but is challenging. Here, we report in situ surface tension measurements based on a novel method that couples a linear quadrupole electrodynamic balance (EDB) with quasi-elastic light scattering (QELS). The EDB-QELS is validated using surface tension measurements of atmospherically relevant inorganic and organic droplets. The surface tension results reasonably agree with the reference values in the range of ∼50–90 mN m–1. We find a significant size dependence for sodium chloride droplets containing surface-active species (sodium dodecyl sulfate) in the size range of ∼5–18 μm. The surface tension increases from ∼55 to 80 mN m–1 with decreased size. Relative humidity (RH)-dependent surface tensions of mixed ammonium sulfate (AS) and polyethylene glycol droplets reveal the onset of liquid–liquid phase separation. Droplets containing water-soluble matter extracted from ambient aerosol samples and 2.3–2.9 M AS exhibit a ∼30% reduction in surface tension in the presence of ∼50 mmol-C L–1 water-soluble organic carbon, compared to pure water (∼72 mN m–1). The approach can offer size-resolved and RH-dependent surface tension measurements of deliquesced aerosol particles.
AS16-A018
| Invited
Emissions of Nitrogen Compounds from an Agricultural Field in the NCP
Yujing MU#+
Chinese Academy of Sciences
Agricultural fields act as an important source for atmospheric nitrogen compounds and play significant roles in regional and global atmospheric environments. Here we show the emission fluxes of N2O, NO, HONO and NH3 from an agricultural filed during a whole year in the North China Plain. The emission fluxes were simultaneously measured by using an open-top chamber method, which could largely counteract the chamber wall effect on reactive nitrogen compounds and cause less interference on the micro-environment of the interface between soil and the atmosphere. All the emission fluxes quickly increased from the field after fertilization with order for appearing their peak emissions as NH3, N2O, HONO and NO. The average emission fluxes of N2O, NO, HONO and NH3 were 182 ng N m-2 s-1, 72 ng N m-2 s-1, 69.8 ng N m-2 s-1 and 246 ng N m-2 s-1 during maize growing period (June-October), and 63.7 ng N m-2 s-1, 15.9 ng N m-2 s-1, 0.5 ng N m-2 s-1, 169 ng N m-2 s-1 during wheat growing period (October-June next year), respectively. The ratios of N2O, NO, HONO and NH3 emissions during the maize period to the wheat period were 2.9, 4.5, 139.6, 1.5, respectively, implying soil temperature plays different roles in their emissions. Compared with the traditional broadcast fertilization, deep soil fertilization could significantly reduce emissions of all the nitrogen compounds and coupling the deep soil fertilization with broadcast nitrification inhibitor could reduce N2O, NO and HONO emissions nearly 100% and NH3 emission of 77.1%. Furthermore, reduction of 30% N-fertilizer for deep soil fertilization in the NCP could reduce N2O emission more than 60% with increasing the maize yield of ~15%. Such control measures are suggested to be advocated for effectively improving the regional air quality in rural areas and mitigating global warming trend.
AS16-A007
Seasonal Variations in the Production of Singlet Oxygen and Organic Triplet Excited Sates in Aqueous Aerosols in Hong Kong, South China
Theodora NAH1#+, Yuting LYU1, Yitao LI1, Yin Hau LAM1, Nadine BORDUAS-DEDEKIND2
1City University of Hong Kong, 2The University of British Columbia
Photooxidants in the atmospheric aqueous phase, such as triplet excited states (3C*) and singlet oxygen (1O2), play important roles in the formation and transformation of secondary organic aerosols (SOA). To elucidate the importance of these aqueous reactions in SOA formation and transformation, it is necessary to quantify the quantum yields and steady-state concentrations of these aqueous photooxidants. However, measurements of aqueous photooxidants in atmospheric samples are still scarce, especially in Asia. In this study, using the chemical probe technique, we show that the illumination of aqueous aerosols in Hong Kong leads to the efficient production of 3C* and 1O2. Experiments were conducted using PM2.5 collected during different seasons in two urban and one semi-rural locations in a year-round study. We observed that 3C* and 1O2 production were the highest in the winter and the lowest in the summer for all three locations. Differences in the locations (urban vs. semi-rural) did not have noticeable effects on 3C* and 1O2 formation. The seasonal trends of 3C* and 1O2 production were found to be due to seasonal variations in the long-range air mass transport. The steady-state concentrations of 1O2 and 3C* correlated with the concentration and absorbance of water-soluble organic carbon in both PM2.5. We also correlated 3C* and 1O2 production to the chemical and optical properties of the PM2.5. Using these correlations, we developed regression models that allow us to predict the quantum yields and steady-state concentrations of 3C* and 1O2 produced based on measurable chemical and optical properties of the PM2.5. This is the first investigation of aqueous photooxidant production in atmospheric aerosols in a South China city, and our findings will help the modeling of aqueous organic aerosol photochemistry in the South China region.
AS16-A011
| Invited
Research on Nitrogen Oxide Reaction Pathways and Driving Factors in the Combined Pollution of Atmospheric Fine Particulate Matter and Ozone
Guoliang SHI#+, Yinchang FENG
Nankai University
Fine particulate matter (PM2.5) and ozone (O3) are two of the most important air pollutants in China. Based on the monitoring data of the Air Quality Research Supersite, this study elucidated the nonlinear relationship between secondary sulfates and their precursor SO2, and determined the main pathways for sulfate generation by establishing an improved solute strength dependent chemical thermodynamic and kinetic model. Further research was conducted on the synergistic effect of atmospheric oxidants and SO2 on the generation of sulfate aerosols. In addition, the chemical cycle of atmospheric nitrogen oxides (NOx) plays an important role in PM2.5 and O3 co-pollution, and its transformation and renoxification are closely related to the generation of particle nitrate and ozone. This study focuses on the chemical cycle process of NOx, to address the scientific issue of the key chemical process of NOx in the formation of PM2.5 and O3. By combining field observation, theoretical analysis and model simulation, the conversion pathways and influencing factors for NOx to generate particle nitrate and ozone, the driving factors' influence on PM2.5 and O3 co-pollution, and the influence of common pollution source emission change on PM2.5 and O3 co-pollution were discussed. Overall, this study emphasizes the effectiveness of using target oxidant control as a new direction for sustainable sulfate mitigation, as China's SO2 concentration is already very low. And the NO2 chemical reaction pathway of secondary nitrate and ozone, as well as the driving factors were revealed. It can improve the emergency regulation ability of atmospheric combined pollution. The influence of common source changes on PM2.5 and O3 concentrations is discussed, which provides theoretical basis for the study of the synergy control of PM2.5 and O3 co-pollution.
AS16-A006
Exploration of the Downward Transport Mechanisms of Biomass Burning Emissions from Indochina at the Low Boundary Layer in East Asia
Chuan-Yao LIN#+
Academia Sinica
Springtime is the biomass burning (BB) season in Indochina. BB emissions are transported to East Asia and Taiwan at elevations of between 2000 and 4000 m and then transported downward to the near-surface layer when weather conditions are favorable. In this study, a numerical model, the Weather Research Forecast with Chemistry (WRF–Chem) model with tracer simulation was employed to explore the downward transport mechanisms and evaluate their potential effects on the planetary boundary layer (PBL) and near-surface layer during the springtime (Feb.-April) in 2018. Ambient backscatter was measured through LiDAR, aerosol optical depth was measured by MODIS and Himawari-8 satellites and by ground observations from the stations of AERONET. The data were applied to identify the transport mechanisms and evaluate the performance of the model. We summarized the downward transport mechanisms surrounding Taiwan, including the thermal effects of mountain downslope circulations (MDC), frontal secondary circulation (FSC) downward transport, and the mixing of MDC and FSC (MMF). Over Taiwan, the contributions of BB emissions for the MDC to the near-surface layer (<500 m), PBL ( <1500 m), and free atmosphere (1500–6000 m) were 0.4%, 4.7%, and >95%, respectively, during springtime in 2018. For the FSC (MMF) mechanisms, the BB contributions to the near-surface layer, PBL, and free atmosphere were 2.5% (3.3%), 15.7% (17.1%), and 84.3% (82.9%), respectively. MMF occurred the most frequently among these three mechanisms and had the largest effect on the near-surface layer and PBL. The downward contributions of BB in different regions, including Taiwan, southern China, and the East China Sea (ECS), were also evaluated.
AS16-A001
Analyzing the Phase State and Chemical Composition of PM2.5 Across Northeast Asia
Changjoon SEONG1+, Daeun KIM1, Rani JEONG1, Qiu YANTING2, Zhijun WU2, Jiyi LEE3, Jun-Young AHN4, Kwangyul LEE4, Kyoung-Soon JANG5, Andreas ZUEND6, Changhyuk KIM7, Natsagdorj AMGALAN8, Mijung SONG1#
1Jeonbuk National University, 2Peking University, 3Ewha Womans University, 4National Institute of Environmental Research, 5Korea Basic Science Institute, 6McGill University, 7Pusan National University, 8National University of Mongolia
The phase state of aerosol particles is a key factor affecting particle size and chemical reactions. Nevertheless, constraints in measurement and analytical techniques result in insufficient information regarding the phase state of atmospheric particulate matter (PM). This study aimed to delve into the correlation between the phase state and chemical attributes of fine PM (PM2.5) using 92 samples collected from Northeast Asia (Beijing, Seoul, Seosan, Ulaanbaatar) during 2020-2022. The analysis showed distinct regional differences in the phase state of PM2.5 in Northeast Asia, which was determined by its chemical composition. Specifically, when primary organic aerosols predominated in the PM2.5 chemical components, a relatively low viscosity was observed. Conversely, when secondary inorganic aerosol components largely constituted the PM2.5 chemical composition, the liquid and (semi)solid phase state was determined based on the (NH4)2SO4:NH4NO3 ratio. Furthermore, liquid phase states of PM2.5 at Northeast Asia were found to be interconnected with aerosol liquid water content (ALWC) in PM2.5. This study suggests a connection between the fundamental physical properties of aerosols and PM2.5 in polluted atmospheres.
AS16-A025
Spontaneous OH Generated in Atmospheric Droplets and Its Role in Processing of Organic Aerosol
Yali JIN+, Hongru SHEN, Hao LUO, Yindong GUO, Zhen SONG, Shuhui XUE, Zhuosi WANG, Defeng ZHAO#
Fudan University
Atmospheric droplets such as cloud water and aerosol liquid water are abundant and ubiquitously distributed in the air, supplying a large quantity of media for chemical reactions. Aqueous phase formation and processing of organic aerosol (OA) have a crucial contribution to concentration and compositions of OA, which is related to air quality, health and climate effects. However, spontaneous generation of hydroxyl radical (OH) in atmospheric droplets reported recently is likely to be very important to aqueous OH budget and OA processing. In this study, we simulate supersaturated and subsaturated systems under atmospherically relevant conditions. We report OH production obtained by using different scavengers, the yield of OH in droplets and the influence of key factors like pH of seed aerosol and ion strength on this spontaneous reaction. Moreover, we investigate the role of spontaneous OH in the processing of OA in atmospheric droplets. This study highlights the contribution of spontaneous OH generation in atmospheric droplets to the formation and processing of OA, which may enable improving simulation of OA budget in numerical models.
Session Chair(s): Takemasa MIYOSHI, RIKEN Center for Computational Science
AS50-A006
An Overview of Japan’s Moonshot Goal 8 R&D Program for Controlling and Modifying the Weather by 2050
Takemasa MIYOSHI1#+, Tetsuo NAKAZAWA2, Takashi SAKAJO3, Kohei TAKATAMA2
1RIKEN Center for Computational Science, 2Japan Science and Technology Agency, 3Kyoto University
Forecast and control are the two sides of a coin. Recent improvements in numerical weather prediction have led to the point where we can start discussing the control of complex, chaotic weather systems. The Japan’s Moonshot Goal 8 research and development (R&D) program or simply MS8 was launched in 2022 to control extreme weather events such as typhoons and torrential rains and to reduce damage from extreme winds and rains, so that we can realize a society safe from such disasters by 2050. As the important first step toward the next 3-decade R&D, MS8 prioritizes numerical simulation experiments to investigate the feasibility of weather control under the constraints of energy and technology within human’s capability in a foreseeable future. Thus far, MS8 achieved promising results to reduce a peak rainfall of heavy downpours, and more results are expected by ongoing efforts. MS8 also accelerates developing basic science and technologies for realizing weather control, such as advanced weather models, computational models of flood damage, and mathematical approaches to intervention optimization techniques for large dimensional systems. In addition, addressing ethical, legal, and social issues (ELSI) is essential and a priority in MS8. This presentation will provide an overview of MS8 with highlighting scientific results.
AS50-A004
Sensitivity of the Rainfall to the Weather Control Practices in the Recent Japanese Heavy Rainfall Events: WRF Model-based Analysis
Yusuke HIRAGA#+, Ryotaro TAHARA
Tohoku University
This study aims to investigate the sensitivity of the rainfall amount to weather modification practices, such as creating a cold pool over the ocean, in order to discuss the possibility of mitigating the heavy rainfall-induced damage. This study first simulated the recent heavy rainfall events induced by zonal moisture transport, including the 2014 Hiroshima localized heavy rainfall event in Japan. The Weather Research and Forecasting (WRF) model with notably high spatiotemporal resolution (~800m spatial resolutions and 80 vertical layers) was used to simulate the 2014 Hiroshima event. This study then represented the considered weather control practices in the simulations by modifying the initial and boundary conditions of the WRF model. For instance, adding the rainwater of 42g/kg over the ocean in the initial condition of the WRF model altered the rainfall amount over the land by up to 50%. The spatial distribution of the rainfall was also significantly changed to be more spread rather than localized. Our model-based analysis suggests the possibility of realistically altering the heavy rainfall pattern over the land, at least for the target event. Further studies are necessary to examine the sensitivity of the rainfall to the magnitude, timing, and location of the weather control practices. It is essential to investigate the effect of weather control practices on the surroundings as well.
AS50-A001
Understanding the Dynamical Changes by an Artificial Cold Pool on Typhoon Hagibis Using the Nonhydrostatic Icosahedral Atmospheric Model (NICAM)
Marguerite LEE1+, Masaki SATOH1,2#
1The University of Tokyo, 2Yokohama National University
Tropical cyclones are highly destructive natural disasters that can be very costly, making them a grave concern to any society. As a part of the Moonshot project of the Typhoon Control Research aiming for a safe and prosperous society, a series of experiments are conducted using the stretched version of the Nonhydrostatic Icosahedral Atmospheric Model (NICAM) with a minimum grid spacing of 1.4km to see the impact an artificial forcing would have on an approaching typhoon. Each experiment has an artificial forcing with a different intensity to induce a cold pool positioned at 27 degrees North Latitude and 138 degrees East longitude in the pathway of typhoon Hagibis. The experiments run for 48 hours before landing in Japan. The intensities provide a constant cooling source of 1K/hr, 2K/hr, 10K/hr and 20K/hr, where each is circular with a radius of 50km. After 6 hours from the initial state when Hagibis approaches Japan, there is some eye distortion where it takes on irregular shapes. All experiments increase sea level pressure between 7 and 14 hours. This change is a sign that there is some weakening occurring. Once the cold pool is in the eye of the typhoon, which occurs from 20 to 24 hours, there is a sharp increase in surface pressure, with the greatest being observed in the 20K/hr and 10K/hr. The results showed changes in the distribution of wind intensities in the eyewall. Although there is no overall reduction in strength, the artificial cold pool has shown some weakening in the approaching typhoon. Improvements are being made to the force, such as changing the location of the cold pool and using evaporative rain to generate the artificial cold pool. This research was supported by JST Moonshot R&D Grant Number JPMJMS2282.
AS50-A002
Influence of Drag Coefficient for Tropical Cyclone Intensification by Numerical Simulations
Hiroaki YOSHIOKA1#+, Hironori FUDEYASU1, Ryuji YOSHIDA1, Junshi ITO2, Takeshi HORINOUCHI3, Kosuke ITO4
1Yokohama National University, 2Tohoku University, 3Hokkaido University, 4Kyoto University
A project ”Moonshot Goal 8” was established to study the possible weakening of typhoon intensity due to artificial interventions supported by Japan Science and Technology Agency. One of our measures is to increase the sea surface drag near typhoons by using obstacles such as large ships. The maximum potential intensity theory suggests that the equilibrium intensity decreases as the surface drag coefficient increases. Still, few numerical studies tested it for real tropical cyclones (TCs). Some studies used fine-resolution simulations (e.g., with a sub-kilometer grid) to agree with the theoretical indication, but the number of cases is limited by calculation resources. Some studies with coarse-resolution models exhibit mixed results. Also, no studies have been conducted to elucidate the effect of surface drag coefficient change in a limited oceanic region. Therefore, we aim to conduct a comprehensive study on how TC would react to surface drag change over limited regions that can be set in various ways. Now, we focused on the intensification of Typhoon Faxai in 2019 and conducted sensitivity experiments by changing the drag coefficient (CD) over the circle area around it. In this study, we ran the Scalable Computing for Advanced Library and Environment (SCALE) at a coarse horizontal resolution of 5 km. The resultant central pressure and maximum 10m wind speed were sensitive to CD, especially for the value. These were reduced almost linearly and weakened by about 60% of the control run (CTL) when CD was set to 3.0 times that in CTL. Additionally, the results of the sensitivity to a radius of changing CD area showed that maximum wind speed during the mature stage has remained unchanged when over 100 km radius area changed. We will conduct further studies until the meeting. JST Moonshot R&D Grant Number JPMJMS2282 supported this research.
AS50-A007
Impact of Sea Surface Evaporation on Developing Tropical Cyclone: Numerical Simulation Study of Typhoon Faxai(2019)
Hiroaki YOSHIOKA#+, Hironori FUDEYASU, Gakuto MOCHIDA, Ryuji YOSHIDA, Yasutomo KIYOHARA
Yokohama National University
A project ”Moonshot Goal 8” was established to study the possible weakening of typhoon intensity due to artificial interventions supported by Japan Science and Technology Agency. We are considering how to reduce the evaporation of water vapor from the sea surface to suppress the intensification of tropical cyclones(TC).Thus, we are developing the surfactant to be sprayed under or around TC. The previous studies suggested that the enthalpy transfer coefficient (CK) is almost constant or increases slightly at high wind speeds. Nevertheless, a limited number of studies have reported on the effects of CK on TC intensity, especially realistic case studies. Therefore, this study aims to investigate the relationships between CK and realistic TC intensification under the numerical simulations to verify the possibility of modification. We focused on the intensification of Typhoon Faxai in 2019, which caused large damage to the Kanto region in Japan. In this study, sensitivity experiments with directly changing water vapor flux from the sea surface around Faxai were conducted by the Scalable Computing for Advanced Library and Environment (SCALE). We tested the control run (CTL) and 5 sensitivity experiments in which water vapor flux decreased by 10% from 90% to 50% around a 200 km radius area moved with the center of Faxai every timesteps. The resultant intensification of Faxai was sensitive. These were reduced almost linearly and weakened by about 10% CTL when set to 50% water vapor flux 200km from the center in CTL. However, it was insensitive to the area of reducing the amount. From 25 km to 150 km radius, the maximum windspeed was reduced linearly over 10% and almost same between 150km and 200km. We will conduct further studies until the meeting.
AS50-A005
Evaluation of Relationship Between Typhoon Activity and Typhoon-related Rainfall Over the Vicinity of Japan Area by Using a Large Ensemble Simulation
Yohei YAMADA#+, Tomoe NASUNO, Masuo NAKANO, Chihiro KODAMA, Misaki HISHINUMA
Japan Agency for Marine-Earth Science and Technology
Typhoons cause tremendous damage to socio-economy every year due to strong wind and heavy rainfall. Their interannual variability (frequency and duration) is affected by natural variabilities such as El Niño. Although previous studies using satellite observations showed a tendency of heavier precipitation around typhoon as their intensity increases, a relationship between typhoon activity and typhoon-related rainfall has not been evaluated systematically to date. This might be associated with insufficient sample number due to a short period of reliable observational data. Our previous studies with an atmospheric general circulation model showed that a variability in the number of typhoons among ensemble members is comparable to the observed interannual variability. This may indicate that interannual variability of typhoon activity is an internal variation of the atmosphere as a first approximation. The variability in ensemble simulation may help us to understand a robust seasonal relationship between typhoon activity and typhoon-related precipitation. In the present study, we evaluated the typhoon activity–rainfall relationship over vicinity of Japan area by using 64-member ensemble simulation with 14 km mesh Nonhydrostatic ICosahedral Atmospheric model. The ensemble simulation was targeted on boreal summers (June–October) in 2009–2019. Typhoon activity was measured by the ACE. Rainfall within a 500-kilometer radius from the center of the typhoon was defined as typhoon-related rainfall. The vicinity of Japan area was defined as the area within a 300 km radius of each meteorological office of Japan Meteorological Agency. The result showed that typhoon-related rainfall decreased as the ACE decreased, and typhoon-related rainfall significantly correlated with the ACE (R=0.88). Although we need to be careful about model bias of NICAM, we were able to confirm a linear relationship between typhoon activity and typhoon-related rainfall.
AS50-A003
Mitigating Typhoon Intensity and Resultant Storm Surges Through Human Intervention: Numerical Experiments of Typhoon Faxai (2019)
Hironori FUDEYASU1#+, Kosuke ITO2, Nobuhito MORI2, Yasutomo KIYOHARA1, Yuji ARAKI3, Takuya MIYASHITA2, Hiroaki YOSHIOKA1
1Yokohama National University, 2Kyoto University, 3Pacific Consultants Co., Ltd.
This study investigates the feasibility of human intervention in mitigating storm surges, specifically focusing on the case of Typhoon Faxai in 2019. Typhoon-induced storm surges significantly threaten coastal areas, especially in enclosed bays like Tokyo Bay, where the effects can be amplified. Our hypothesis posits that strategically placed blocks in narrow bay mouths could effectively reduce the height of significant wave heights of storm surges. We conducted comprehensive numerical simulations focusing on the Typhoon Faxai event to evaluate this hypothesis. Faxai caused extensive damage along the coasts of Tokyo Bay due to severe storm surges and wave heights. The observed peak wave heights were estimated at 3.4 meters in Yokohama and 2.6 meters in Tokyo and Chiba, combined with rapidly developing high waves within the bay and approximately 1.0 m of storm surge. Our experiment (the bay-blocks experiment) involved artificially increasing the friction coefficient by 5-100% over a 5 km-30 km stretch at the entrance of Tokyo Bay. This was compared to a control experiment (CTL), where no alteration in friction coefficient was made. The results of the bay-blocks experiment indicated a notable reduction in sea surface wind speeds, averaging a decrease of -5 m/s compared to the CTL. More importantly, the simulations under the altered wind and pressure conditions demonstrated a decrease in the storm surges by -0.2 m. This reduction has substantial implications for coastal defense strategies, suggesting that human intervention can significantly decrease the impact of typhoon-induced surges. These findings underscore the importance of innovative coastal management strategies in mitigating the effects of natural disasters. The feasibility study provides a foundation for future research on the effectiveness of human interventions in similar coastal environments, offering insights into sustainable and practical solutions for storm surge mitigation.
Session Chair(s): Lei ZHU, Southern University of Science and Technology
AS14-A028
| Invited
Future Emission Pathways in Northeast Asia Under Carbon Neutrality
Jung-Hun WOO1#+, Zbigniew KLIMONT2, Satoru CHATANI3, Young Hwan AHN4, Shinichiro FUJIMORI5, Shaohui ZHANG2, Jia XING6, Younha KIM2, Fei GUO2, Minwoo PARK7, Yisheng SUN8, Youjung JANG7, Jin-Seok KIM7, Minyoung CHOI7, Bomi KIM7
1Seoul National University, 2International Institute for Applied Systems Analysis, 3National Institute for Environmental Studies, 4Sookmyung Women's University, 5Kyoto University, 6George Mason University, 7Konkuk University, 8Tsinghua University
To maintain environmentally sound and sustainable development while at the same time achieving a low-carbon society, it is beneficial to assess effectiveness of air pollution and climate change policies in integrated way. The Air Quality in Northeast Asia(AQNEA) is a research project to study air quality under various future carbon mitigation and air pollution control strategies using multiple Integrated Assessment Models(IAMs) of participating regional and international institutions. Future emissions of six countries – China, South Korea, Japan, North Korea, Mongolia, and Russia – in Northeast Asia were estimated under three future scenarios; baseline, old NDC, and Carbon Neutrality. Based on future scenarios, energy and non-energy activities combining with carbon mitigation policies were projected in multiple energy IAMs, such as MESSAGE, GUIDE. Air pollution control strategies in link with the future energy projections were then applied in multiple air quality IAMs, such as GUIDE, GAINS. In this presentation, harmonized future emissions pathways of GHGs and air pollutants in six countries based on three future scenarios in GAINS framework will be presented on site. Acknowledgements : This research was supported by the FRIEND (Fine Particle Research Initiative in East Asia Considering National Differences) Project through the National Research Foundation of Korea(NRF) funded by the Ministry of Science and ICT(2020M3G1A1114621) and supported by the IIASA Strategic Initiatives Project through the National Research Foundation of Korea (NRF) funded by the Ministry of Science and ICT (NRF-2021K2A9A1A02101523).
AS14-A004
| Invited
Towards Satellite-based 1 KM Resolution Retrieval of NOx Emissions
Jintai LIN#+, Hao KONG, Yuhang ZHANG, Sijie WANG, Wanshan TAN
Peking University
Nitrogen oxides (NOx = NO + NO2) are a major air pollutant which undergoes substantial fine-scale spatiotemporal variations associated with anthropogenic and natural emission sources. Current emission datasets can hardly capture the fine-scale spatial details of NOx emissions. Our previous work has developed a fast, reliable algorithm (PHLET) to retrieve NOx emissions at high spatial resolutions (≤5 km) based on tropospheric NO2 vertical column densities (VCDs) retrieved from satellite instruments. The algorithm derives the lifetimes and emissions of NOx at individual locations by explicitly accounting for the nonlinear chemistry and horizontal transport. Applying the PHLET algorithm to Asia reveals many important emission sources which are missing in current anthropogenic emission inventories and natural emission datasets. In this study, we will discuss the potential of estimating NOx emissions at an unprecedented horizontal resolution of 1 km, by combining satellite NO2 data, physics-based emission inversion and Artificial Intelligence (AI) approach. Such emission data will provide crucial information for future-generation air quality and climate modeling and targeted emission mitigation.
AS14-A030
| Invited
Quantifying Methane Emissions from China's Coal Industry
Kai QIN#+
China University of Mining and Technology
The coal industry is the largest anthropogenic source of methane (CH4) emissions in China. Since 2021, we have carried out co-located observations of in-situ, ground-based and satellite remote sensing using state-of-the-art sensors and platforms in several coal-producing regions. A simple and flexible mass balance approach is applied to these observations to estimate CH4 emissions. This work will introduce an individual coal mine CH4 emission inventory using a mixture of bottom-up and top-down approaches, and a 5-year, grid-by-grid, and day-by-day CH4 emission inventory by merging TROPOMI and eddy covariance observations. Further, we will present a new research strategy by synergizing emerging platforms with high spatial resolution such as PRISMA and GF-5, which can compensate for the coarse resolution of TROPOMI.
AS14-A029
Co-occurrence of Heat and Ozone Extremes in China: Historical Trends and Interactive Health Effects
Meng GAO#+
Hong Kong Baptist University
Climate change and air pollution are two intimately interlinked global concerns. The frequency, intensity, and duration of heat waves are projected to increase globally under future climate change. A growing body of evidence indicates that health risks associated with the joint exposure to heat waves and air pollution can be greater than that due to individual factors. However, the cooccurrences of heat and air pollution extremes in China remain less explored in the observational records. Here we investigate the spatial pattern and temporal trend of frequency, intensity, and duration of cooccurrences of heat and air pollution extremes using China’s nationwide observations of hourly PM2.5 and O3, and the ERA5 reanalysis dataset over 2013–20.
AS14-A002
Revisiting the Quantification of Power Plant CO2 Emissions from Satellite: A Comparative Study Using Three Top-down Approaches
Xiao LU#+, Cheng HE
Sun Yat-sen University
Top-down constraints of CO2 emissions from coal-fired power plants are critical to improving the accuracy of CO2 emission inventory and designing carbon reduction strategies. Different top-down models based on satellite observation have been proposed in previous studies, but discrepancies between these models and the underlying drivers are rarely explored, limiting the confidence of their application to monitor point-source CO2 emissions from satellite. Here, we apply three top-down models to estimate CO2 emissions from individual coal-fired power plants in the United States (US) and China in 2014-2021 from Orbiting Carbon Observatory 2 (OCO-2) satellite observations. The first one applies the Gaussian plume model to optimize emissions by fitting modeled CO2 enhancement to the observation. The second and third methods apply the same inversion framework, but with WRF-Chem and WRF-FLEXPART as forward models, respectively. Results show that the WRF-Chem and WRF-FLEXPART based inversion results are more consistent with the EPA reported emission rates compared to the Gaussian plume model method. This is because application of high-resolution three-dimensional wind fields better captures the shape of observed plumes, compared to the Gaussian plume model which relies on wind field at a single point, and thus the Gaussian plume model has difficulty to optimize emissions under inhomogeneous wind fields or when observations are far away from the power plant. In general, using the WRF-FLEXPART model as the forward model in the inverse analysis shows the best consistency with the EPA’s reports, likely due to its capability to simulate narrow-shape plumes in the absence of numerical diffusion which is inherent in Eulerian model such as WRF-Chem. Our study exposes the capability and limitation of different top-down approaches in quantifying point-source CO2 emissions, advancing their application for better serving increasing constellations of point-source imagers in the future.
AS14-A008
Uncertainty Evaluation of CO2 Emission Dynamic Update Methods in China
Hanwen HU1+, Guannan GENG1, Ruochong XU1, Bo ZHENG1, Qinren SHI2, Qingyang XIAO1, Xiaodong LIU1, Qiang ZHANG1#
1Tsinghua University, 2Laboratoire des Sciences du Climat et l'environnement
Tracking CO2 emissions timely is important for assessment of mitigation effects and supporting policymaking. Most current CO2 emission inventories in China are developed with the statistical yearbook, resulting in an obvious time lag. Few emission inventories have been dynamically updated using various near-real-time data, based on the assumption that changes in activity can approximately represent changes in emissions. However, there still lacks a comprehensive uncertainty evaluation for different update methods. Here, we compare three typical updating methods for CO2 emissions in China: (1) based on the statistical yearbook, which contains detailed provincial data of energy consumption and industrial production; (2) based on the official bulletin information, which includes the year-on-year changes of national fuel consumption with a time delay of one year; (3) based on official monthly statistics, which involve monthly provincial production and transportation turnover with a time lag of one month or two. The first method is recognized as the most accurate, while the latter two are considered as dynamic update methods that require uncertainty assessment through a series of tests. We find that the dynamic update methods generally overestimate CO2 emissions compared with method (1) (-0.08%-2.65%), and the biases increase with the update iteration. Moreover, the biases vary significantly by sector. For example, power sector has the smallest updating biases owing to the high-quality data, while industrial emissions are generally overestimated due to the ignorance of improved efficiency in all the methods. Finally, we design the best-performed dynamic update emission method based on the combination of both bulletin information and official monthly statistics, which redistributes the update results of method (3) using the monthly profile provided by method (2). Our research fills the gap in uncertainty assessment of dynamic update methods for CO2 emissions and provide potential references for improving the accuracy of dynamic CO2 emission inventory.
Session Chair(s): Bin GUAN, University of California, Los Angeles, June-Yi LEE, Pusan National University, Elias MASSOUD, Oak Ridge National Laboratory
AS32-A005
| Invited
Atmospheric Rivers in East Asia Summer as the Continuum of Extratropical and Monsoonal Moisture Plumes
Seok-Woo SON1#+, Chanil PARK2
1Seoul National University, 2Boston College
East Asian atmospheric rivers (ARs) exhibit the most pronounced activity in summer with significant impacts on monsoon rainfall. However, their formation mechanism(s) from a synoptic perspective is yet to be unveiled. In this study, we unravel the inherently complex nature of East Asian summer ARs by applying a multiscale index that quantifies the relative importance of high- (HF) and low-frequency (LF) moisture transports to AR development. It is found that both HF and LF processes contribute to shaping the summertime ARs in East Asia, contrasting to the wintertime ARs which are dominated by HF processes. The categorization of ARs with the multiscale index reveals that HF-dominant ARs are driven by baroclinically-deepening extratropical cyclones, analogous to the widely-accepted definition of canonical ARs. In contrast, LF-dominant ARs result from enhanced monsoon southwesterly between a quasi-stationary cyclone and anticyclone with the latter being the anomalous expansion of the western North Pacific subtropical high, which is reminiscent of the classical monsoon rainband in East Asia. The intermediate ARs, constituting a majority of East Asian summer ARs, exhibit synoptic conditions that combine HF- and LF-dominant ARs with extratropical cyclones traveling along the frontal boundary between a quasi-stationary cyclone and anticyclone. This result indicates that East Asian summer ARs cannot be explained by a single dominant mechanism. Instead, they should be considered as a continuum of extratropical and monsoonal moisture plumes.
AS32-A010
| Invited
Recent East Asian Rainfall Extremes, Moisture Transport & Circulation Clusters
Robin CLARK#+
Met Office
In recent years, many locations in eastern Asia have been impacted by extreme rainfall events with daily totals more like those seen during major storms in the tropics. In this talk, I will present some examples of these events, demonstrating the likely role of atmospheric moisture, funnelled over great distances from sub-tropical latitudes of the Pacific and Indian Oceans into the region where it encounters topography and much colder air from mid and high latitudes. I will also show how the probability of such atmospheric river events varies with circulation clusters in the region and how they might change in coming decades, using data from a new initial condition ensemble of Met Office HadGEM3 climate model simulations.
AS32-A003
Modulation of East Asian Atmospheric Rivers by the Pacific-Japan Teleconnection Pattern
Yeeun KWON1+, Seok-Woo SON1#, Chanil PARK2, Jinwon KIM3,4
1Seoul National University, 2Boston College, 3National Institute of Meteorological Sciences, 4University of California, Los Angeles
Despite growing recognition that atmospheric rivers (ARs) play an important role in summer monsoon rainfall in East Asia, their variability in response to low-frequency climate modes remains less understood. The present study reports the significant control of the Pacific-Japan (PJ) teleconnection pattern on East Asian summer ARs. While Korea and Japan experience more frequent, intense, and persistent ARs during the positive PJ phase, ARs in eastern China are more active during the negative PJ phase. Such AR activity changes are closely related to the PJ modulation of the western North Pacific subtropical high along which anomalous moisture transport organizes on the low-frequency time scale. This finding suggests that the PJ teleconnection pattern is an important source of East Asian summer AR variability and needs to be considered in medium-range forecasts of AR-related hydrological extremes.
AS32-A011
Analyzing Atmospheric Rivers with a Storm-centric Approach
Shakeel ASHARAF1,2#+, Bin GUAN1,2, Duane WALISER2
1University of California, Los Angeles, 2California Institute of Technology
This study introduces the ROTated Atmospheric river coordinaTE (ROTATE) system – a novel storm-centric coordinate system designed specifically for analyzing atmospheric rivers (ARs). It effectively preserves key AR signals in the time mean that may be lost or obscured in simple averaging due to diverse AR orientations and shapes. We used ROTATE to look at crucial characteristics of atmospheric rivers such as how wet the air is, how fast the wind blows, how much water vapor is being transported, and how much rain falls in the northern hemisphere. Composites of key meteorological variables, indicate distinct and clearer patterns of ARs compared to the conventional non-rotated AR centroid-based compositing approach. It is further apparent that the ROTATE system more distinctly delineates the finer details in precipitation distributions for landfalling and oceanic ARs. Overall, the ROTATE system has the potential to serve as a valuable tool for better comparing and understanding the characteristics, processes, and impacts of ARs across different regions.
AS32-A013
The Emergence of Changes in Atmospheric Rivers and the Associated Extreme Rainfall in Response to Greenhouse Warming
June-Yi LEE1#+, Arjun NELLIKKATTIL1, Bin GUAN2,3
1Pusan National University, 2University of California, Los Angeles, 3California Institute of Technology
Atmospheric Rivers (ARs) play a critical role in the global water cycle and the dynamics of extratropical weather patterns. It has been suggested that ARs are projected to become more frequent and more likely to be associated with extreme rainfall events over many parts of the globe in response to greenhouse warming. However, recent changes in ARs and the associated extreme rainfall are not well understood. Here, we investigate recent changes and the emergence of changes in AR frequencies in response to greenhouse warming. To address these issues, we analyze observed data from 1979 to 2020 and large ensemble historical (1850-2014) and SSP3-7.0 (2015-2100) simulations based on Community Earth System Model version 2 (CESM2). The Scalable Feature Extraction and Tracking method recently developed is utilized to detect AR. Our results show increasing trends in AR frequencies particularly over extratropical oceans and land. Analysis of CESM2 large ensemble simulations suggests region-dependent emergence time of AR frequencies and the associated extreme rainfall. We further discuss the key processes for the emergence of AR frequency changes. This study has important implications for future water management and adaptation choices.
Session Chair(s): Panxi DAI, Zhejiang University, Jingyu WANG, Nanyang Technological University
AS48-A002
| Invited
Health and Economic Costs of Future Extreme Heat Risk
Shupeng ZHU1#+, Yida SUN2, Daoping WANG3, Dabo GUAN2
1Zhejiang University, 2Tsinghua University, 3University of Cambridge
Evidence shows an ongoing increase in the frequency and severity of global heatwaves, raising concerns about the future impacts of climate change and the associated socio-economic costs. Here, we develop a disaster footprint analytical framework by integrating climate models, epidemiological and hybrid input-output, and computable general equilibrium global trade models to estimate the mid-century socioeconomic impacts of heat stress. We consider health costs related to heat exposure, the value of heat-induced labor productivity loss, and indirect losses due to economic disruptions cascading through supply chains. We find that the global heatwave days would increase by 104% in 2060 compared to 2022 under SSP585, and the global average annual number of heat-induced deaths would increase to around 1.12 million (0.85 ~ 1.39 million). For economic impacts, we show that the global annual incremental loss increases exponentially from 0.03±0.01 (SSP245) ~ 0.05±0.03 (SSP585) percentage points during 2030 – 2040 to 0.05±0.01 ~ 0.15±0.04 percentage points during 2050 – 2060. By 2060, the expected global economic losses reach a total of 0.6% ~ 4.6% with losses attributed to health loss (37%~45%), labor productivity loss (18%~37%), and indirect loss (12%~43%) under different SSPs. Small and medium-sized developing countries in Southeast Asia and Africa suffer the most from heat risks as well as regional supply chain disruptions.
AS48-A009
| Invited
Stronger Early-spring Dust Outbreaks Across the Northern Hemispheric Mid-latitudes in a Warmer Climate
Ji NIE#+, Yiting WANG, Yan YU
Peking University
Record-breaking dust events in the early-spring of 2021 and 2023 seemingly paused the decreasing trend in East Asian dust activity since the onset of the 21st century. These two recent dust extremes, both associated with abnormally warm and snow-free conditions, pointed to the possibility of regional enhancement in early-spring dust activity under global warming. Here, using satellite measurements, reanalysis data, as well as simulations from a dust emission model and the Coupled Model Intercomparison Project Phase 6 (CMIP6), we show a 10-35% increase in March dust emission across the East Asian, Central Asian, and North American drylands from the 1980s towards the end of the 21st century. This regional enhancement in early-spring dust emission is primarily caused by reduced snow cover in response to warming. In addition to the exposure of bare ground, lower snow cover has been accompanied by stronger surface winds and drier soils, providing a favorable environment for dust emission. Our findings call for adaptation to the anticipated stronger early-spring dust storms across the North Hemispheric mid-latitudes in the upcoming decades.
AS48-A007
The Unprecedented Southeast Asia Heatwave of May 2023
Jingyu WANG1#+, Yang LYU2, Xiefei ZHI2, Xianfeng WANG1, Edward PARK1
1Nanyang Technological University, 2Nanjing University of Information Science & Technology
In May 2023, Southeast Asia experienced an unprecedented heatwave with far-reaching consequences. This study presents a comprehensive overview of the event, including its spatiotemporal evaluation, circulation pattern, driving forces, forecast performance, return period, and the wide-ranging impacts. The heatwave shattered previous temperature records across the region, with maximum temperatures surpassing historical norms by a substantial margin. The study emphasizes the role of tropical waves interaction in amplifying the magnitude of this anomaly. The repercussions of the heatwave were severe, encompassing a high toll on human health, mass mortalities of marine life, diminished agricultural yields, and a significant surge in wildfires. This study underscores the devastating effects of climate change through a vivid portrayal of the unprecedented heatwave in Southeast Asia.
AS48-A016
Different Characteristics of Clouds in Two Types of Heat Waves Over South Korea
Minjeong CHO+, Ha-Rim KIM, Yong-Sang CHOI#
Ewha Womans University
Recent heat waves have been prolonged over South Korea, yet the physical mechanisms influencing their duration remain unclear. This study examined possible causes that led to the extension of summer heat waves over South Korea. 50-year (1973–2022) summer heat waves over South Korea were categorized into two types of events based on their duration: short-term (5−7 days) and long-term (≥16 days) events. Subsequently, we compared the two types of events in terms of the contributions of components of surface energy budget, cloud, and soil moisture using JRA-55 reanalysis data. Both types of heat wave events are mostly caused by increased net shortwave radiation at the surface. This is due to the decrease in clouds attributed to the anticyclonic circulation over South Korea. However, there are different characteristics in short- and long-term events: short-term events showed a fast recovery in clouds at all altitudes, while in long-term events, a slow recovery in lower-level clouds was notable. These continuous fewer clouds at lower levels mainly result in more incoming solar radiation to the surface. This is associated with a conditionally unstable atmospheric field and dry atmosphere, preventing the formation of lower-level clouds. Also, long-term events showed a temporary increase in clouds at 100–200 hPa, contributing to trapping outgoing longwave radiation and eventually leading to surface warming. These findings could contribute to a better understanding of the recent prolonged summer heat waves in South Korea.
AS48-A012
Fuel Availability and Convective Potential Complement Near-surface Weather in Regulating Global Wildfire Activity
Hongxuan SU1#+, Yan YU1, Weidong GUO2, Jiafu MAO3
1Peking University, 2Nanjing University, 3Oak Ridge National Laboratory
Wildfires tend to happen in hot, dry, windy, rainless days – this knowledge about fire weather serves as the basis for both short-term forecast and long-term prediction of global wildfire activity. Yet, wildfires have to occur with fuel and ignition sources, which are underrepresented in fire forecast and prediction practices. By analyzing wildfire activity and vegetation cover from satellite measurements, as well as atmospheric states from reanalysis data, here we show that near-surface weather, represented by the widely analyzed Canadian Forest Fire Weather Index, only partially capture actual wildfire occurrence and intensity across the daily to seasonal time scales. Meanwhile, fuel availability and convective potential provide additional regulation on global wildfires, especially across semi-arid, sparsely vegetated regions. Mechanistically, enhanced convective potential supports lightning ignitions and low-level oxygen convergence, thereby promoting wildfire occurrence and intensity. Based on these findings, we recommend (1) including fuel abundance and convective potential in operational wildfire forecast and (2) revisiting long-term trajectories of wildfires in the context of co-changing atmospheric and terrestrial conditions.
AS48-A008
Future Projection of Extreme Precipitation Over East Asia in HighResMIP Climate Models with Varying Resolutions
Young-Ha KIM+, Seok-Woo SON#, Seokgeun OH
Seoul National University
While climate models are widely used for studying future climate change, they inherently carry uncertainties arising from various factors. The model resolution is one of such factors for extreme precipitation, given that the resolution used in climate modeling is generally too coarse to explicitly resolve precipitation processes. This study examines extreme precipitation over East Asia as simulated and projected by a set of CMIP6 models. To assess its resolution dependence, the models that used varying resolutions in the HighResMIP project are utilized. First, the spatial distribution of extreme precipitation in the historical run is assessed for low-resolution (LR) and high-resolution (HR) models. A large spread is found in the intensity of extreme precipitation among models for both LR and HR sets, while its dependence on the resolution is rather small or moderate. The scaling of the modeled extreme precipitation indicates that both the model spread and the resolution dependence are primarily attributable to the dynamical factor, with minor contributions from the thermal factor. Next, the future projection of extreme precipitation under SSP5-8.5 scenario is evaluated among the models. All the LR and HR models exhibit increasing trends in both the intensity and frequency of extreme precipitation with a weak dependence on the model resolution. Notably, all models show a larger change in the frequency of heavier precipitation. Such change is attributable to the change in the thermal factor in all models. However, the model spread in the extreme-precipitation change is due to both dynamical and thermal factors with comparable contributions.
AS48-A005
Exploring Precipitation Triple Oxygen Isotope Variations: Insights from GISS ModelE2.1 Simulations
Yilin ZHANG1#+, Allegra LEGRANDE2, Nathalie GOODKIN3, Jesse NUSBAUMER4, Shaoneng HE1, Xianfeng WANG1
1Nanyang Technological University, 2NASA Goddard Institute for Space Studies, 3Richard Gilder Graduate School, 4National Center for Atmospheric Research
Precipitation stable isotopes, inducing δ18O, d-excess and 17O-excess, serve as unique tools for understanding the hydrologic cycle and climate change. 17O-excess has been recently recognized as a promising new tracer for understanding water evaporation and condensation history in precipitation processes. However, our understanding of the control mechanisms underlying precipitation 17O-excess remains limited, especially in low-latitude regions crucial to extreme weather dynamics. Isotope-enabled global climate models, specifically GISS ModelE2.1, reasonably reproduce the precipitation δ18O. Higher-order tracers like d-excess and 17O-excess require the model to adequately represent kinetic effects, often through model parameterizations, and simulations of these tracers have thus fallen short. In this study, we evaluated the performance of GISS ModelE2.1 in simulating precipitation triple oxygen isotopes and explored precipitation isotope responses to variations in isotope kinetic fractionation parameters, seawater isotopes, rain evaporation and supersaturation factors. Spatial comparisons suggest that the model slightly underestimates the mean global d-excess and overestimates 17O-excess in polar regions. Monthly time-series comparisons reveal consistent δ18O but notable offsets in d-excess and 17O-excess, with better model performance in higher latitude sites. In addition, the model simulations prove the significant impact of rain evaporation in tropical convection on precipitation d-excess and 17O-excess variations. Moreover, the moisture source vapor isotopes closely resemble the onsite vapor isotopes, suggesting the model simulates minimal influence from upstream convective activities along the transport pathway on precipitation isotopes. This research provides insights into the GISS ModelE2.1’s performance in capturing precipitation triple oxygen isotopes and the mechanisms responsible for the observed variation in precipitation 17O-excess and d-excess. Knowledge of the controls on precipitation triple oxygen isotopes is essential for interpreting paleoclimate records and understanding climate systems within the evolving context of extreme weather events.
Session Chair(s): Joong-Bae AHN, Pusan National University
AS74-A008
A Farmstead-specific Early Warning System for Weather Risk Management in South Korea
Kyo-Moon SHIM#+, Jiwon KIM, Yongseok KIM, Sera JO, Jina HUR, Mingu KANG, Eung-Sup KIM
National Institute of Agricultural Sciences
A farmstead-specific early warning system for weather risk management was built to support climate smart agriculture using farm-level prediction technology of weather and risk information. This system quantifies weather conditions into a ‘weather risk index’ that is customized to crop and its growth stage. When the risk reaches the level causing any damage to the crops, the system is activated and send the corresponding warning messages to the user farmer’s mobile phone. These messages include proper recommendations that farmers can utilize to protect their crops against potential damage. This system has been developed, based on comprehensive technology including the scaling down of weather data to the field level and crop specific risk assessments for operational service. Furthermore, the scientific know-how has been integrated into a web-based warning system (https://agmet.kr). The system is provided to volunteer farmers with direct, one-on-one weather data and risk warnings along with relevant recommendations. It was found that 86.6% of farmers who volunteered for the service were satisfied. As of December 2023, the service was put in operation in 75 cities & counties of South Korea. Now in this area, ca. 18,400 volunteer farmers who raise various crops are participating in this system to receive farm(plot)-specific weather and risk information from the service and in turn, provide feedback and evaluations. This service system will be extended nationwide (155 cities & counties) by 2025. This study was carried out with the support of Research Program for Agricultural Science & Technology Development (Project No. RS-2020-RD009451), National Institute of Agricultural Sciences, Rural Development Administration, Republic of Korea.
AS74-A006
Understanding the Emergent Properties of Catchment-scale Hillslope Aquifers for the Improved Predictability of Soil Moisture and Evapotranspiration in LSM
Minki HONG1#, Seung-Jae LEE2+
1Princeton University, 2National Center for AgroMeteorology
The role of groundwater at the catchment-scale has been increasingly understood as a key process affecting the development of terrestrial water-energy coupled cycles. While the method of streamflow recession analysis, based on the Dupuit-Boussinesq (DB) approximation, has existed as a practical approach to address time-dependent emergent properties of catchment groundwater, the land surface modeling (LSM) community still lacks a proper LSM structure to apply the parameterization scheme for large-scale terrestrial predictions. This study uses a new LSM framework, namely the National Water Model (NWM)-BE3S framework (Hong & Mohanty, 2023), that enables the DB approximation-based depiction of the catchment-scale aquifer to estimate emergent aquifer properties (e.g., hydraulic diffusivity) through streamflow observations. The NWM-BE3S framework integrates the BE3S’s scheme of the soil-groundwater-river continuum (Hong et al., 2020) into the WRF-Hydro NWM configuration. We applied the NWM-BE3S LSM framework to three major basins in Texas (i.e., the Trinity, Brazos, and Colorado River basins). We identified the NWM-BE3S’s predictive performance for soil moisture (SM), and evapotranspiration (ET) was significantly related to the streamflow recession characteristics, which infer aquifer diffusivity. Specifically, as the aquifers exhibit higher non-linearities in their discharge behavior, we found that the flux budget closures of SM and ET are readily done, leading to improved predictability of such water-energy variables. Overall, the research outcomes show the effectiveness of DB-based groundwater hydrology for LSM, implying the importance of catchment-scale conservation of hydraulic continuity. We also plan to implement the new NWM-BE3S into the NCAM Land-Atmosphere Modeling Package (LAMP) for the process-level enhancement of terrestrial water/energy/carbon predictions in Korea.
AS74-A002
Characteristics and Attribution of Surface Evapotranspiration in Typical Ecosystems Under the Background of Climate Change
Tianwei LU+, Yong HAN#, Li DONG, Yurong ZHANG
Sun Yat-sen University
Surface evapotranspiration (ET) is a crucial process in the water cycle, transferring water from terrestrial ecosystems to the atmosphere. However, the pattern of ET variability in typical ecosystems and its main drivers remain unclear in a CO2-enriched climate. This study explored the spatial and temporal heterogeneity and drivers of ET in four types of ecosystems: farmland, forest, grassland, and shrub. The analysis was based on the output data of the CMCC ESM2 model, and focused on the differences between different periods and wetness levels. The Ridge regression method was employed here. As the concentration of CO2 increased, the atmospheric evapotranspiration demand (VPD) also increased. This led to more luxuriant vegetation growth and an overall increasing trend in ET, particularly in shrub ecosystems (7.41 mm decade-1). Our findings indicate that thermal conditions were the primary factor driving ET variability in relatively humid forest and shrub ecosystems, while relative humidity (RH) was the primary factor driving ET variability in relatively arid farm and grass ecosystems. In terms of average contribution over all periods, surface solar radiation (SSRD) contributed 26% and 41% to ET variation in forest and shrub ecosystems, respectively. Meanwhile, RH contributed 49% and 32% to ET variation in farmland and grassland ecosystems, respectively. The main drivers of ET varied across ecosystems and were related to vegetation type and environmental conditions. It is important to note that as the wetness level increased, the contribution of water conditions to ET decreased while the contribution of thermal conditions increased. Correlation analyses revealed that environmental factors moderated the effect of leaf area index (LAI) on ET, as changes in environmental conditions directly affected VPD and ecosystem water sources. The above findings serve as a reference for better comprehension of surface hydrological processes and their connections with ecosystems in the context of climate change.
AS74-A004
Future Change of Suitable Cultivation Area for Major Fruit Trees in South Korea Under RCP 4.5/8.5 Scenarios
Joong-Bae AHN1#+, Eung-Sup KIM2, Kyo-Moon SHIM2, Jina HUR2, Sera JO2, Myoung-Seok SUH3, Dong-Hyun CHA4, Seung-Ki MIN5, Hyun-Suk KANG6
1Pusan National University, 2National Institute of Agricultural Sciences, 3Kongju National University, 4Ulsan National Institute of Science and Technology, 5Pohang University of Science and Technology, 6Numerical Modeling Center/Korea Meteorological Administration
Future change of cultivation area of apple (Malus domestica Borkh.) and mandarin (Citrus unshiu Marc.), which are major fruit crops in South Korea, under the representative concentration pathway (RCP) scenarios is investigated. For the purpose, projected future climate downscaled by five regional climate models with a 12.5 km horizontal resolution is utilized. According to the projection, the cultivation areas of major fruit crops in South Korea are likely to change significantly. That is, the cultivation area of apple (mandarin), which is a major current fruit crop in Type D (C) according to the Köppen–Trewartha climate classification, is projected to be reduced (expanded) as it moves towards higher latitudes and elevations in the future. Apples grown throughout South Korea in the present climate are not expected to be cultivated in the late-21C due to climate change. On the other hand, the cultivation area of mandarins is projected to increase steadily in the future. At present, mandarins are cultivated only in Jeju Island, which is located in the south of the South Korea. However, the cultivation area is expected to increase by 1323% in late-21C under the RCP8.5 scenario compared to the reference period. Moreover, mandarin cultivation is projected to be possible anywhere in South Korea. Nevertheless, in late-21C, excessive increases in temperature that exceeds the appropriate temperature for mandarin in Jeju Island and the southern part of South Korea will eventually decrease the cultivation area of mandarins.
AS74-A012
Study on the Siberian Heatwave and Korean Peninsula Cold Spell in April 2020 Utilizing Regional Replay
Joonlee LEE+, Jihae KIM, Geonhee BAK, Myong-In LEE#
Ulsan National Institute of Science and Technology
In the spring of 2020, Siberia experienced a record-breaking heatwave with unprecedented high average temperatures, while the Korean Peninsula encountered a sudden cold spell due to the southward movement of cold air. This study focuses on the Eurasian teleconnection patterns that developed during the same period, analyzing their occurrence and maintenance mechanisms using global reanalysis data and climate model (GloSea6) experiments. The climate model experiments employed a Regional Replay system, which updates incremental values calculated from the difference between the model’s background and analysis fields for each prognostic variable. The analysis revealed a significant correlation between the high temperatures in the Siberian region (55-75N, 70-110E) and the cold conditions on the Korean Peninsula in April, with the development of large-scale waves in the upper atmosphere of the Eurasian region. The stationary waves showed a strong relationship with North Atlantic sea surface temperature, as confirmed in experiments controlling the entire globe and only the North Atlantic. Even in experiments controlling only the North Atlantic, the simulation of Siberian high temperatures and Korean Peninsula cold conditions suggests a close association with North Atlantic sea surface temperatures. Furthermore, this study proposes that the intensified stationary waves and the enhanced upper atmospheric circulation response in Siberia and East Asia are due to increased land-atmosphere interaction, particularly influenced by reduced snow cover over the Siberia region. Based on the GloSea6 experiment, atmosphere-land interaction experiments confirmed that changes in soil moisture significantly impact temperature variations in the Siberian region. ※ This work was funded by the Korea Meteorological Administration Operational System Operation and Development for Climate Prediction Program under Grant KMA2018-00322.
Session Chair(s): Il-Ju MOON, Jeju National University
AS13-A020
| Invited
Increased Tropical Cyclone Intensification Time in the Western North Pacific Over the Past 56 Years
Liguang WU#+
Fudan University
It has been projected that the influence of anthropogenic climate change on tropical cyclone (TC) intensity could be detected by the end of the century although significant increasing trends in TC intensity metrics have been found based on the currently available historic records. The human influences on TC intensity have been debated for about two decades because of a lack of quantitative assessment of the contributions of large-scale environmental factors and track shifting. As an extension of a previous study, we show that the observed rise in the percentage of intense TCs in the western North Pacific basin over the past 56 years resulted from the combined influence of the track shifting and temporary changes in environmental factors. The influence of environmental factors was primarily owing to the decrease of environmental vertical wind shear and the warming of sea surface temperature. While a small part of the observed rise in the percentage of intense TCs resulted from SST warming, the track shifting increased the TC intensification time by 18.2% (11.3 hours) over the past 56 years, accounting for more than one-third of the observed percentage increase in intense TCs. Since track shifting is also projected in the global warming experiments, this study suggests that anthropogenic climate change may intensify TCs by shifting TC prevailing tracks.
AS13-A067
Feedback of Tropical Cyclones Over the Western North Pacific on La Niña Flavor
Qiuyun WANG+, Jianping LI#
Ocean University of China
The relationship between La Niña and tropical cyclone (TC) activity has not received as much attention as that between El Niño and TCs; in particular, the important role of TCs in affecting La Niña flavor has not been reported. This study reveals a clear feedback of TCs over the western North Pacific (WNP) on La Niña flavor by modulating the Walker circulation and thermocline. When strong WNP accumulated cyclone energy (ACE) occurs three months earlier, the center of sea surface temperature (SST) anomalies shifts to the equatorial eastern Pacific, favoring the development of eastern–Pacific (EP) La Niña. In contrast, weak WNP ACE is associated with central–Pacific (CP) La Niña, and the influence of WNP TCs on the intensity of CP La Niña may be larger than for EP La Niña. More evidence is provided in the predictions of EP and CP La Niña events using the ACE+SST model.
AS13-A071
Pacific Decadal Oscillation Modulates the Relationship Between Pacific Meridional Mode and Tropical Cyclone Genesis in the Western North Pacific
Chao WANG#+
Nanjing University of Information Science & Technology
Pacific Meridional Mode (PMM) is known to be significantly correlated with tropical cyclone (TC) genesis over the western North Pacific (WNP), while the stability of their relationship remains unknown. Here we found that their relationship is nonstationary, which depends on the phase of Pacific Decadal Oscillation (PDO). During the PDO warm phases, the PMM-emanated cyclonic circulation and ascending motion can propagate to the entire WNP due to the enhanced background convection. In contrast, during the PDO cold phases, the PMM-resulted cyclonic circulation and ascending motion are confined to the eastern WNP, while the compensated descending motion prevails in the western WNP. Accordingly, the PMM-induced consistent (inconsistent) changes in large-scale conditions across the western and eastern WNP act to strengthen (weaken) the relationship between the PMM and WNP TC genesis during the PDO warm (cold) phases. The result provides further guidance for improving seasonal prediction of TC genesis.
AS13-A065
Changes in Tropical Cyclone Rainfall with Climate Change
Shifei TU1#+, Jianjun XU1, Johnny CHAN2,3
1Guangdong Ocean University, 2Asia-Pacific Typhoon Collaborative Research Center, 3City University of Hong Kong
Heavy rainfall is one of the major aspects of tropical cyclones (TC) and can cause substantial damages. Here, we show, based on satellite observational rainfall data and numerical model results, that between 1999 and 2018, the rain rate in the outer region of TCs has been increasing, but it has decreased significantly in the inner-core. Globally, the TC rain rate has increased by 8 ± 4% during this period, which is mainly contributed by an increase in rain rate in the TC outer region due to increasing water vapor availability in the atmosphere with rising surface temperature. On the other hand, the rain rate in the inner-core of TCs has decreased by 24 ± 3% during the same period. The decreasing trend in the inner-core rain rate likely results mainly from an increase in atmospheric stability.
AS13-A022
Shifted Relationship Between the Pacific Decadal Oscillation and Western North Pacific Tropical Cyclogenesis Since the 1990s
Cong ZHOU1+, Liguang WU2#
1Shanghai Typhoon Institute of CMA, 2Fudan University
The Pacific Decadal Oscillation (PDO) and Pacific Meridional Mode (PMM) are prominent climate modes in the North Pacific with well-established impacts on tropical cyclone (TC) genesis in the western North Pacific (WNP) basin. While previous research has primarily focused on the roles of the PDO and PMM in regulating TC genesis through the modification of large-scale environmental factors, this study investigates the evolving influence of the PDO on WNP TC genesis since the 1950s. Remarkably, our analysis reveals a shift in the PDO-TC genesis relationship, transitioning from a significant negative correlation to a significant positive correlation since the 1990s. This shift is attributed to variations in the specific large-scale factors through which the PDO affects TC genesis. Furthermore, this study suggests that these changes appear to be linked to the PMM strengthening on the interdecadal timescale in recent decades. The linkage of the PMM strengthening to the PDO-related atmospheric circulation is further confirmed by the results of a 500-year pre-industrial numerical experiment, suggesting that the PMM strengthening may result from natural internal variability. The results underscore the non-stationary relationship between PDO and WNP TC genesis, with the PMM intensity probably influencing their relationship.
AS13-A058
Increasing Frequency of Intense Tropical Cyclones Over the Arabian Sea in a Warmer World
Akash PATHAIKARA MANA1#+, Minkyu LEE2, Seung-Ki MIN1
1Pohang University of Science and Technology, 2Korea Institute of Energy Research
Tropical cyclones are known for their highly destructive nature and cause large economic losses. Our study observed a significantly increasing trend in the number of intense tropical cyclones (INT TCs) over the Arabian Sea (ARB) in the Oct-Nov season from1981-2020. We also noticed that the tropical cyclone heat potential (TCHP) seems to be the key factor behind it by enhancing the integrated heat content of the ocean and associated evaporation. In addition to this, sea surface temperature (SST), moist static energy (MSE) and depth of 26 °C isotherm (D26) also show a strong relation to the power dissipation index (PDI) of INT TCs. To quantify the influence of anthropogenic greenhouse forcing, we analyzed the same climatological variables in different individual forcing simulations from the Coupled Model Intercomparison Project Phase 6 (CMIP6) multiple models. The comparison between observation (OBS), greenhouse gas (GHG), and all-forcings (ALL) along with the pre-industrial control runs (CTL) reveals a faster increase of TCHP in the GHG runs (6 kJ cm-2 decade-1), which is 1.5 times that of OBS. An associated high deepening rate of D26 is also visible in the GHG simulations. The increasing trend of MSE in the ALL runs is also found to be comparable to the OBS, which is majorly contributed by the GHG forcing. The combined impact of the faster-rising TCHP, MSE and SST over the ARB in the GHG runs provides an important monitoring factor, which increases the probability of occurrence of intense TCs over the ARB by the formation of favoring climatological conditions in a warmer world. In future, the analysis will expand to examine the variations in area concerning the threshold values of the aforementioned parameters under different forcings. Our analysis will provide valuable insights into the spatial expansion of INT TCs in a heated globe.
AS13-A075
Poleward Migration of Western North Pacific Tropical Cyclone Activities in the CMIP6-HighResMIP Models Using a New Constrained Detection Method
Zhuoying LI#+, Wen ZHOU
Fudan University
This study intended to investigate the poleward migration of the tropical cyclones(TC) Over the western North Pacific (WNP) using CMIP6-HighResMIP models but found that the formation frequency and latitude differ greatly from the observed data especially in winter and spring when evaluating the model performance. In TRACK algorithm, the formation frequency and latitude outnumber the observed data a lot mainly because some extratropical storms are misidentified as tropical ones. Therefore, this paper put forward a new constrained Detection method based on the monthly 26°isotherm and the location of the westerlies. The error reduced a lot and the new constrained results capture the annual cycle of tropical cyclone formation frequency and latitude fairly well. The TC genesis formation latitude and lifetime maximum intensity latitude(LMI) both have a poleward shift under the SSP5–8.5 scenario and the former is more significant than the latter. In addition, the TC frequency displays significantly reduction. The spatial changes of the dynamics potential genesis index(DPGI) and large-scale environment show that the conditions are more favorable(unfavorable) to TC generation above North(south) of 20°N in the future. In the case of Uneven global warming, the effect of internal variability on TC poleward migration may decrease but still play a dominant role.
AS13-A010
Global Climatology of Rapid Expansion of Tropical Cyclone
Weiling ZHANG+, Kelvin T. F. CHAN#, Lifeng XU
Sun Yat-sen University
Rapid expansion (RE) of tropical cyclone (TC) is a structural evolution that specifies the fast geometric increase in TC size but receives limited attention. In this study, we utilize the 41-yr global climatology of TC outer-core size (effective radius of 34-kt gale-force surface winds, R34EFF) over the period 1979–2019, define RE as the 90th percentile of global expansion samples (i.e. ΔR34EFF > 50 NM per 24 h; 1 NM = 1.852 km), and reveal the global climatology of RE comprehensively. Statistics show that 32% of TCs experienced RE at least once during their lifetime. Chronically, proportion of RE has significantly decreased in the globe, Northern Hemisphere and western North Pacific. Seasonally, RE proportion exhibited two peaks, with one in the early and the other in the late TC season. Distinct spatiotemporal variations of RE are found. In addition, the climatological RE occurrence, RE duration and the associated TC intensity are shown and discussed.
Session Chair(s): Xiao-Ming HU, The University of Oklahoma
AS34-A022
| Invited
Development of a Tibetan Plateau Climate Modelling System with Improved Parameterization Schemes
Kun YANG1#+, Xu ZHOU2, Xin LI2
1Tsinghua University, 2Chinese Academy of Sciences
As the "water tower of Asia", the Tibetan Plateau (TP) is of great interest for its water cycle and related atmospheric processes. The eastern and southern edges of the Tibetan Plateau are generally characterized by steep topography and high precipitation, resulting in large and rapid flood peaks, which can easily lead to floods and mudslides. Responding to these disasters requires high prediction accuracy of numerical meteorological models. In addition, as a region with strong multi-sphere interactions, the TP has experienced warming and wetting of the climate over the last 40 years, with significant changes in all spheres. Therefore, a regional climate system model applicable to the plateau environment is urgently needed to support the understanding of interactions among the spheres and their changes. Current climate models have problems such as wet bias in precipitation throughout the year and cold bias in cold season over the TP. A Tibetan Plateau climate system model (TPCSM) needs to represent typical features of the TP, such as the effects of complex topography, snow, soil, lake processes. Based on observations and field work, we developed and integrated the parameterizations of these processes (orographic turbulent drag, snow fraction and albedo, soil organic matter, thermal roughness length, lake-air interaction, cloud physics etc.) and in WRF4.0. The updated modelling system much reduces the wet bias and cold bias. With the TPCSM, a high-resolution meteorological data for the TP has been development, whose accuracy outperforms that of other main stream data sets for this region.
AS34-A021
| Invited
Relationship Between Vertical Variation of Cloud Microphysical Properties and Thickness of Entrainment Interfacial Layer in Post Stratocumulus Clouds
Seong Soo YUM#+, Inyeob LA
Yonsei University
This study examines the vertical variations of cloud microphysics and their correlation with the thickness of the Entrainment Interfacial Layer (EIL) in stratocumulus clouds, observed from the Physics of Stratocumulus Top (POST) aircraft measurement campaign. From the mixing fraction analysis, we identified EIL between the free atmosphere and cloud top for all fifteen POST flights, and found that EIL thickness significantly influenced the vertical variation of cloud microphysics and thermodynamics. In several flights, a trend towards stronger homogeneous mixing traits with increasing depth from the cloud top was found, indicative of the vertical movement of mixed (i.e., entrainment affected and diluted) parcels. However, in one flight, this trend was limited only to mid-levels of the cloud, with the correlation between virtual potential temperature and liquid water content being strongly negative near the cloud top, suggesting challenges for the descent of mixed parcels. Another important finding is that there was a robust negative correlation between longwave cooling rate near the cloud top and EIL thickness, highlighting differences in radiative cooling rates between mixed and unmixed parcels due to differences in liquid water content between them. These insightful findings will be crucial for enhancing our understanding of the role of EIL in modulating entrainment and the vertical movement of mixed parcels in stratocumulus clouds.
AS34-A018
Prediction of Cloud Microphysics Affected by Entrainment-mixing Using Machine Learning
Chunsong LU1#+, Sinan GAO2
1Nanjing University of Information Science & Technology, 2China Meteorological Administration
Different entrainment-mixing mechanisms between cloud and environment are essential to cloud-related processes; however, accurate representation of entrainment-mixing in weather/climate models still poses a challenge. Machine learning is a promising approach to improve empirical parameterizations of entrainment-mixing mechanisms. In our work, we train an algorithm to understand the impact of entrainment-mixing on microphysics using the simulation data from the Explicit Mixing Parcel Model. Compared with traditional parameterizations, the trained machine learning algorithm achieves more accurate microphysical properties (number concentration and cloud droplet spectral dispersion). The partial dependences of predicted microphysics versus features exhibit strong alignment with physical mechanisms and expectation by interpreting method, overcoming the limitations of the “black box” algorithm. The mechanisms are that the smaller number concentration and larger spectral dispersion correspond to stronger and more inhomogeneous entrainment-mixing. Specifically, number concentration after entrainment-mixing is positively correlated with adiabatic number concentration and liquid water content after entrainment-mixing, and negatively correlated with adiabatic volume mean radius. Spectral dispersion after entrainment-mixing is negatively correlated with liquid water content after entrainment-mixing, turbulent dissipation rate and relative humidity of entrained air. Sensitivity tests suggest number concentration is mainly affected by cloud microphysics and spectral dispersion is primarily influenced by both cloud microphysics and environmental variables; incorporating more features leads to a more effective algorithm. The results have the potential to enhance the representation of entrainment-mixing in weather/climate models.
AS34-A005
Fast and Slow Responses of Atmospheric Energy Budgets to Perturbed Cloud and Convection Processes in an Atmospheric Global Climate Model
Ben YANG1#+, Zhun GUO2, Fengfei SONG3, Yaocun ZHANG1, Tianjun ZHOU2, Yun QIAN4
1Nanjing University, 2Chinese Academy of Sciences, 3Ocean University of China, 4Pacific Northwest National Laboratory
Cloud and convection strongly modulate atmospheric energy budgets, but the latter’s responses often vary across timescales because of complex interactions between fast and slow processes. Here, based on atmospheric model simulations at intermediate state between weather and climate timescales, we investigate how the responses in the global-mean atmospheric energy budgets evolve over time after simultaneously perturbing various cloud-scale processes. We find that the responses in radiative and sensible heat fluxes converge much more rapidly compared to condensation heat associated with precipitation, which is attributed to the compensating feedback effects of precipitation on longwave cooling and shortwave heating. Because of energy conservation, uncertainty in long-term precipitation simulations can be substantially reduced by constraining the fast processes of radiative and sensible heat fluxes. These findings can help economize on computational resources required for model tuning and serve as a crucial link between the convective-scale and equilibrium-state outcomes within the model.
AS34-A026
Does a Scale-aware Convective Parameterization Scheme Improve the Simulation of Heavy Rainfall Events?
Haerin PARK+, Jiwon HWANG, Tae Ho MUN, Dong-Hyun CHA#
Ulsan National Institute of Science and Technology
Precipitation predictability using the non-scale-aware and scale-aware convective parameterization schemes (CPSs) was investigated to assess the necessity of the CPSs within the gray-zone. This study evaluates the performance of the CPS of the Weather Research and Forecasting (WRF) model for 135 heavy precipitation events (HREs) over the Korean Peninsula for 10 years (i.e. 2011-2020). We tested the Kain–Fritsch (KF) scheme (non-scale-aware) and Multi-scale Kain–Fritsch (MSKF) scheme (scale-aware) in the WRF model. The MSKF scheme shows an overall improved performance of precipitation simulation compared to the KF scheme, but the precipitation forecast performance of CPS depends on the characteristics of HREs. When the HREs are characterized by synoptic-scale atmospheric conditions with strong winds and large-scale water vapor transport, the forecast performance of both CPSs is similar because a cloud microphysics scheme can explicitly resolve most of the precipitation. However, in the case of HREs with weak synoptic forcing conditions (e.g., moisture transport and winds) related to the localized and meso-scale HREs, the MSKF scheme can improve overall simulated precipitation by increasing grid-scale precipitation and reducing the overestimation of subgrid-scale precipitation simulated in the KF scheme. Therefore, using the scale-aware CPS in the gray-zone can provide more accurate precipitation forecasts regardless of the environmental condition of the HREs.
AS34-A020
Microphysical Insights Into an Overestimation of Radar Reflectivity in the Simulation of a Snowstorm Case Over Northern China Plain
Xiaoran OUYANG#+, Ying ZHANG
Nanjing University
Accurately modeling the complex microphysical growth processes of ice in the atmosphere poses a significant challenge. This study aims to enhance the simulation of a snowfall event over the Northern China Plain by employing two distinct microphysics schemes—namely, the Thompson and Morrison schemes—within the Advanced Research WRF (Weather Research and Forecasting) model. Both microphysics schemes successfully reproduce the observed event; however, a notable disparity arises in the simulated radar reflectivity between the two schemes. Specifically, the Morrison scheme produces higher radar reflectivity compared to the observational data. Subsequent analysis reveals that this discrepancy may be attributed to an inherent flaw in the collection efficiency of the Morrison scheme, leading to an exaggerated self-aggregation process and larger snow particle sizes. Further sensitivity tests demonstrate that adopting an alternative formula for collection efficiency mitigates this issue, resulting in radar reflectivity values that closely align with observations. This study underscores the critical importance of accurately representing the self-aggregation process and emphasizes the ongoing need for improvement in ice microphysics schemes to enhance the fidelity of snowfall simulations.
AS34-A029
Impact of Moist Thermodynamics Expressions on Climatrogical Temperature Fields Represented in a Global Cloud Resolving Model
Tomoki OHNO#+, Shuhei MATSUGISHI
The University of Tokyo
The phase change of water is one of the main factors driving the Earth's atmospheric general circulation, and the representation of the thermodynamic system of the moist atmosphere is fundamental to general circulation models. The possibility of condensation and freezing of water complicates thermodynamics, and various approximations are used for meteorological and climatological purposes. For example, the latent heat of vaporization is sometimes assumed to be a constant, or the gas constant or specific heat of water vapor is substituted for that of the dry atmosphere. These simplifications are generally done without considering the mutual consistency of the thermodynamic system, and internal inconsistencies have been recognized as one source of error in numerical models. The consistency of thermodynamic systems of the moist air has been considered. Additionally, several studies have addressed the methodologies to guarantee the thermodynamic consistency in numerical models. The impacts of choice of the moist thermodynamics expressions on simulations were examined in several studies. However, the relationship between moist thermodynamics expressions and climatrogical temperature fields represented in general circulation models have not been well discussed yet. This study reports on the impacts of the moist thermodynamics expressions on climatrogical temperature fields represented in a global cloud resolving model. We present how the represented temperature fields were modulated by the change of the moist thermodynamics expressions. We show that, in particular, large differences between simulations with two thermodynamic configurations appear in the tropical upper troposphere. Furthermore, based on the notion that the lapse rates are essentially moist adiabatic in the low-latitude region, we reveal what aspects of the thermodynamic configuration cause differences in the temperature structure through the analyses of moist adiabat.
AS34-A015
Shallow Convection Dataset Simulated by Three Different Large Eddy Models
Xiaocong WANG1#+, Zhao YAXIN2, Yimin LIU1, Guoxiong WU1, Yanjie LIU2
1Chinese Academy of Sciences, 2University of Chinese Academy of Sciences
Shallow convection plays an important role in transporting heat and moisture from the near-surface to higher altitudes, yet its parameterization in numerical models remains a great challenge, partly due to the lack of high-resolution observations. This study describes a large eddy simulation (LES) dataset for four shallow convection cases that differ primarily in inversion strength, which can be used as a surrogate for real data. To reduce the uncertainty in LES modeling, three different large eddy models were used, including SAM (System for Atmospheric Modeling), WRF (Weather Research and Forecasting model), and UCLA-LES. Results show that the different models generally exhibit similar behavior for each shallow convection case, despite some differences in the details of the convective structure. In addition to grid-averaged fields, conditionally sampled variables, such as in-cloud moisture and vertical velocity, are also provided, which are indispensable for calculation of the entrainment/detrainment rate. Considering the essentiality of the entraining/detraining process in the parameterization of cumulus convection, the dataset presented in this study is potentially useful for validation and improvement of the parameterization of shallow convection.
AS34-A014
A Process-oriented Analysis of the Diurnal Cycle of Summer Precipitation Over China in Three Reanalyses
Yanjie LIU1#+, Xiaocong WANG2, Yimin LIU2, Hao MIAO3
1University of Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3China Meteorological Administration
Convective parameterization in numerical models remains an important source of model uncertainty, as evidenced in the deficiency in simulations of the diurnal cycle of precipitation (DCP). To explore the dominant processes in DCP simulation bias, the behaviors of DCP in phase and amplitude over China in three commonly used reanalysis products, including ERA5, JRA-55 and MERRA-2, are compared against GPM (Global Precipitation Measurement) and CMORPH (Climate Prediction Center Morphing Technique). Results show while JRA-55 produces DCP that are closely consistent with observation, ERA5 and MERRA-2 produce precipitation peak 1- to 3-hour earlier than observed. To understand the reasons behind, process-oriented analysis is conducted by investigating apparent heating (Q1), moisture sink (Q2), and the eddy transport of moist static energy (Q1-Qrad-Q2). Only JRA-55 captures the tilting structure of eddy transport associated with convection, whereas ERA5 triggers precipitation too early and develops too fast. MERRA-2 restricts the transport to lower levels, resulting in weak convection activity manifested by small values of cumulus mass flux. Difference of surface conditions and large-scale forcing between different reanalyses in influencing DCP is also investigated. While delayed surface flux may favor reasonable DCP in JRA-55, the large-scale forcing is overall similar between different reanalyses, indicating subgrid-scale schemes other than convection also play an important role in shaping DCP. These imply the need to link DCP with subgrid-scale processes besides convection and to treat physical parameterizations as an integrated system.
Session Chair(s): Jun WANG, The University of Iowa, Binita PATHAK, Dibrugarh University
AS59-A010
| Invited
Atmospheric Aerosol Monitoring Results from GEMS Over Asia
Yeseul CHO1+, Jhoon KIM1,2#, Sujung GO3, Mijin KIM3, Seoyoung LEE3, Minseok KIM1, Won-Jin LEE4, Dongwon LEE4, Omar TORRES3, Sang Seo PARK5, Heesung CHONG6
1Yonsei University, 2Korean Academy of Science and Technology (KAST), 3NASA Goddard Space Flight Center, 4National Institute of Environmental Research, 5Ulsan National Institute of Science and Technology, 6Center for Astrophysics | Harvard & Smithsonian
We present improvements to the GEMS aerosol retrieval algorithm (AERAOD), including spectral binning, surface reflectance estimation, cloud masking, and post-processing, along with validation results. These enhancements aim to provide more accurate and reliable aerosol monitoring results over the Asian region. The adoption of spectral binning in the LUT approach reduces random errors and enhances the stability of satellite measurements. Additionally, we introduce a new high-resolution database for surface reflectance estimation, based on the minimum reflectance method, tailored to the GEMS pixel resolution. Monthly Background Aerosol Optical Depth (BAOD) values are considered to consistently estimate hourly GEMS surface reflectance. Advanced cloud removal techniques have been implemented, significantly improving the effectiveness of cloud detection and enhancing the quality of aerosol retrievals. An innovative post-processing correction method, based on machine learning, is introduced to address artificial diurnal biases in Aerosol Optical Depth (AOD) observations. The performance of GEMS AERAOD products is validated against AERONET and CALIOP data for the period from November 2021 to October 2022. GEMS AOD demonstrates a strong correlation with AERONET AOD (R=0.792) but exhibits bias patterns, including underestimation of high AOD values and overestimation in low AOD conditions. GEMS Single Scattering Albedo (SSA) agrees well with AERONET data within acceptable error ranges, with variations observed among different aerosol types. For GEMS AOD exceeding 0.4, 42.76% (±0.03) and 67.25% (±0.05) of GEMS SSA fall within the specified error bounds, increasing to 56.61% (±0.03) and 85.70% (±0.05) for strong aerosol signals (GEMS AOD > 1.0). Model-enforced post-process correction improves GEMS AOD and SSA performance, reducing the diurnal variation of bias. Validation of GEMS Aerosol Layer Height (ALH) against CALIOP data demonstrates good agreement, with a mean difference of -0.225 km, and 55.29% (71.70%) of data falling within ±1 km (1.5 km).
AS59-A021
| Invited
A Generalized and Unified Aerosol Retrieval Algorithm for Multi-satellite Measurements
Liangfu CHEN1#+, Minghui TAO2, Jinhua TAO1
1Chinese Academy of Sciences, 2China University of Geosciences
The simultaneous retrieval of aerosol optical/microphysical and surface parameters poses a significant challenge due to the limited information available from satellite observations. In this study, we present a robust and flexible aerosol algorithm for satellite measurements, employing the physical-informed deep learning (PDL) method. Unlike the optimized inversion that needs iterative Radiative Transfer (RT) calculations of all the unknowns, the PDL method can model the whole satellite observations with each retrieved aerosol parameter separately with the pre-training of RT simulations. Furthermore, PDL training maximizes the utilization of prior information derived from ground-based aerosol inversions and satellite surface products, and provides an effective constraint to avoid very abnormal values. By applying the PDL algorithm to satellite measurements of multi-spectral, multi-angle, and polarization such as MODIS, MISR, and POLDER-3, the retrieval results have robust high-accuracy compared with AERONET products. With its efficiency in both computation and information utilization, the PDL algorithm, equipped with a flexible framework, stands as a competitive choice for operational aerosol retrieval across diverse satellite measurements.
AS59-A042
Comparison of Aerosol Layer Height Retrievals Among Different Satellite Platforms: GEMS, EPIC, and TROPOMI
Hyerim KIM#+, Xi CHEN, Jun WANG, Gregory CARMICHAEL, Zhendong LU
The University of Iowa
Aerosol Layer Height (ALH) serves as a crucial indicator, revealing the altitude of aerosol layers along the vertical coordinate, essential for evaluating surface air quality and understanding the impact of aerosols on climate. Using passive remote sensing measurements within oxygen (O2) absorption bands, known for their sensitivity to ALH, offers an opportunity to extract global or regional ALH information from satellite observations. In this study, we conduct a comparative analysis of ALH products obtained from O2 absorption measurements across multiple satellite platforms, including the Geostationary Environment Monitoring Spectrometer (GEMS) over Asia, the Earth Polychromatic Imaging Camera (EPIC) in deep space, and the polar-orbiting TROPOspheric Monitoring Instrument (TROPOMI). The validation of these products is carried out using spaceborne lidar measurements from the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP), particularly for typical dust and smoke plumes. Adjustments have been introduced to accommodate inherent variations in the definitions of ALH among different products, ensuring an apple-to-apple comparison. In contrast to CALIOP ALH, both EPIC and TROPOMI ALH show a strong correlation coefficient (R) exceeding 0.7, alongside a slight overestimation by approximately 0.8 km. Conversely, GEMS ALH displays minimal bias (0.1 km) but a slightly lower correlation, with an R value of 0.64. The categorization of GEMS retrievals with Ultraviolet Aerosol Index (UVAI) values equal to or greater than 3 significantly enhances the agreement with CALIOP. GEMS ALH demonstrates a narrower range and lower mean value compared to EPIC and TROPOMI, with further improved correlation when UVAI ≥ 3. Additionally, the diurnal variation of GEMS and EPIC ALH aligns with boundary layer development. We will be able to further validate and compare ALH retrievals from lidar measurements and chemical transport model simulation from the ASIA-AQ field campaign, contributing to a more comprehensive understanding of aerosol vertical distribution.
AS59-A016
Dust Retrieval Algorithms Using Chemical Composition Estimation Obtained from Observational Data
Ehsan PARSA JAVID#+, Sang Seo PARK
Ulsan National Institute of Science and Technology
Dust storms have a considerable impact on atmospheric particle concentrations, particularly during spring, affecting the Korean Peninsula. Satellite monitoring plays a crucial role in rapidly investigating dust storm properties, with thermal infrared observations being especially valuable for discerning particle characteristics. Our study focuses on the atmospheric window band, where dust, rather than gas, predominantly influences top-of-atmosphere (TOA) brightness temperatures. Within the thermal infrared domain, the influence of the refractive index is evident. Using chemical composition data of 14 Asian dust events, we calculate the refractive index specifically for the thermal infrared range. This, along with the determination of Effective Radius (Re) from 2014 to 2023 for dust-laden days at three Korean Peninsula stations, enables the creation of Look-Up Tables (LUTs) to enhance future precision. Notably, our research highlights a significant difference between the radiance calculated by the Radiative Transfer Model (libRadtran) and the currently used practical radiance in the GK-2A satellite. This discrepancy is likely attributed to using ideal meteorological data instead of real-world observations or measurements in satellite retrieval. the reduced imaginary component of the refractive index in Asian dust, critically influencing the single scattering properties of dust aerosols. We emphasize the non-negligible importance of dust single scattering albedo in the infrared realm.
AS59-A038
An Retrieval Algorithm for Aerosol Microphysical and Optical Properties from MODIS Measurement
Minghui TAO1#+, Liangfu CHEN2, Yi WANG1
1China University of Geosciences, 2Chinese Academy of Sciences
The multi-spectral satellite sensors such as MODIS have a large swath, high spatial resolution, and well onboard calibration, enabling aerosol retrievals with daily global coverage. Despite numerous available bands, MODIS aerosol algorithms over land typically only utilize measurements from 2-3 spectral wavelengths to retrieve Aerosol Optical Depth (AOD) based on prescribed aerosol models. To make full use of multi-spectral measurements and prior information, we developed a retrieval algorithm for aerosol microphysical and optical properties based on a physics-informed deep learning (PDL) approach. With physical constraint from radiative transfer simulation, PDL can construct model functions between the whole spectral measurements and each retrieved aerosol parameter separately. AERONET validations in eastern China show that MODIS PDL algorithm can accurately retrieve AOD and fine AOD (R=0.936) at 1 km resolution and has reliable performance in coarse AOD as well as notable sensitivity to aerosol absorption. The flexible and efficient PDL method provides a generalized algorithm for common multi-spectral satellite measurements.
AS59-A024
AOD Data Fusion with Korean Geostationary Satellite Instruments GEMS, AMI, and GOCI-II: Statistical and Deep Neural Network Methods
Minseok KIM1+, Jhoon KIM1,2#, Hyunkwang LIM3, Seoyoung LEE4, Yeseul CHO1, Yun-Gon LEE5, Sujung GO4, Kyung Hwa LEE6
1Yonsei University, 2Korean Academy of Science and Technology (KAST), 3National Institute for Environmental Studies, 4NASA Goddard Space Flight Center, 5Chungnam National University, 6National Institute of Environmental Research
Aerosol optical depth (AOD) data fusion for aerosol datasets obtained from the Geostationary Korea Multi-Purpose Satellite (GEO-KOMPSAT; GK) series was conducted through the application of both statistical and deep neural network (DNN)-based methodologies. The GK mission incorporates the Advanced Meteorological Imager (AMI) on GK-2A, as well as the Geostationary Environment Monitoring Spectrometer (GEMS) and Geostationary Ocean Color Imager-II (GOCI-II) on GK-2B. The statistical fusion approach rectified biases in each aerosol product by assuming a Gaussian error distribution. Utilizing Maximum Likelihood Estimation (MLE) fusion, the technique accounted for pixel-level uncertainties by weighting the root-mean-square error of each AOD product for individual pixels. A DNN-based fusion model was trained to align with Aerosol Robotic Network AOD values through fully connected hidden layers. The results of both statistical and DNN-based fusion generally surpassed the performance of individual GEMS and AMI AOD datasets in East Asia (R = 0.888; RMSE = −0.188; MBE = −0.076; 60.6% within EE for MLE AOD; R = 0.905; RMSE = 0.161; MBE = −0.060; 65.6% within EE for DNN AOD). Particularly, focusing on AOD around the Korean peninsula, encompassing all aerosol products, yielded significantly improved outcomes (R = 0.911; RMSE = 0.113; MBE = −0.047; 73.3% within EE for MLE AOD; R = 0.912; RMSE = 0.102; MBE = −0.028; 78.2% within EE for DNN AOD). The DNN AOD demonstrated effective handling of the rapid increase in uncertainty at higher aerosol loadings. Overall, the fusion AOD, particularly DNN AOD, closely matched with the performance of the Moderate Resolution Imaging Spectroradiometer Dark Target algorithm, exhibiting slightly less variance and a negative bias. Both fusion algorithms stabilized diurnal error variations and provided additional insights into hourly aerosol evolution.
AS59-A007
Reconstruction of Site-scale Dust Optical Depth (DOD) Time Series from 1980 to 2021 in Northern China: Application to the Evaluation of DOD in CMIP6 Historical Simulations
Wenrui YAO1#+, Ke GUI1, Hengheng ZHAO1, Linchang AN2, Nanxuan SHANG1, Xutao ZHANG1, Lei LI1, Yu ZHENG1, Hong WANG1, Zhili WANG1, Junying SUN1, Hong-Li REN1,3, Jian LI1, Huizheng CHE1, Xiaoye ZHANG1
1Chinese Academy of Meteorological Sciences, 2China Meteorological Administration, 3China University of Geosciences
The biases generated by state-of-the-art climate models in simulating dust optical depth (DOD) remain to be detailed. Here a site-scale DOD dataset in March–August over northern China (NC) during 1980–2001 was reconstructed using the empirical relationship between MODIS-retrieved DOD and dust-event frequencies during 2001–2021. Then, through the combined use of MODIS-based and reconstructed DOD, we evaluated the reproducibility of DOD from 13 models participating in phase 6 of the Coupled Model Intercomparison Project (CMIP6) for the historical period (1980–2001 and 2002–2014) and under different Shared Socioeconomic Pathways (SSPs) during 2015–2021. The results demonstrate that CMIP6 models and multi-model ensemble mean (MEM) are capable of capturing the spatial pattern of DOD, but with considerable uncertainty and inter-model variability in magnitude. Regionally-averaged DOD is underestimated by 51.36% during 1980–2001 and overestimated by 30.61% during 2002–2014 in MEM over NC. Simultaneously, the inter-model standard deviations are greater than MEM during 2002–2014, suggesting large discrepancies among individual models. Geographically, models performed significantly better in the Gobi Desert (GD) than in other subregions. Very few models accurately capture the trends in DOD, which can mainly be attributed to the different trends in simulated wind speed (WS), soil moisture, and vegetation cover, and their contributions to dust evolution. Under four SSPs, despite the best correlation between SSP1-2.6-modeled and MODIS DOD over GD, overestimation of DOD is still observed. More models under SSP1-2.6 capture the positive DOD trend, mainly attributable to positive changes in simulated WS over GD.
AS59-A022
Study and Application of Operational Aerosol Product Based on Fengyun Satellite Remote Sensing Data
Yidan SI#+, Lin CHEN, Xingying ZHANG, Na XU
National Satellite Meteorological Center
With the development of Chinese meteorological satellites, the performance of the 3D/MERSI instrument in the domestic Fengyun polar orbit satellite series has basically reached a level comparable to that of MODIS. In the stationary series, AGRI is an advanced radiation imager of FY4B service satellite on the new generation of stationary satellite, which makes domestic and foreign counterparts have higher attention and expectations for its quantitative inversion capability of aerosol, which also forces researchers to strengthen the algorithm research. This study uses the observation data of Fengyun-3D satellite medium resolution imager -II (FY3D/MERSI-II) and FY4B satellite imager (FY4B/AGRI) L1. Firstly, a multi-element remote sensing identification method of cloud, clear sky and haze is proposed. It effectively improves the identification accuracy of clear sky and haze on bright surface. Secondly, based on the characteristics and calibration state of MERSI-II and AGRI instruments, MODIS MXD04_L2 AOD product is used for atmospheric correction, and the influence of surface reflectance relationship between visible and near infrared channel with time, observation angle and surface type is analyzed. The surface reflectance models for MERSI-II and AGRI were reconstructed. Finally, the accuracy of the research results is evaluated by using the same type of products. The results show that the correlation between the FY3D/MERSI-II AOD and MODIS products is ~0.9, and the average deviation is ~0.02. The correlation between AOD and MODIS products retrieved by FY4B/AGRI is ~0.85, and the average deviation is ~0.04. The quantitative capability of Fengyun satellite is preliminarily proved through the algorithm breakthrough in this study. The separation of haze pixels also further improves the detection capability of Fengyun satellites. The FY3D/MERSI-II and FY-4B/AGRI AOD products can provide data support for environmental monitoring, data assimilation, climate change and other fields.
AS59-A060
Spatiotemporal Variations in the Relationship Between AOD and PM in East Asia: Analysis of Meteorological Factors Influencing the Relationship
Kwang Nyun KIM+, Kyungbae CHOI, Hyeon Woo SEO, Jiyun LEE, Yun-Gon LEE#
Chungnam National University
The concentration of particulate matter (PM) poses significant risks to both human health and the atmospheric environment. While ground-based measurements of PM concentrations are possible through in-situ methods, monitoring networks are predominantly situated in urban areas, leading to limited spatial coverage. To overcome this limitation, various studies have endeavored to estimate PM concentrations using satellite-based aerosol optical depth (AOD), which offers a continuous spatial distribution. These efforts rely on the empirical relationship between AOD and PM. However, previous studies often assumed a fixed AOD-PM relationship, overlooking the temporal and spatial variations influenced by meteorological factors. This study explores the spatiotemporal dynamics of the AOD-PM relationship in East Asia, considering various meteorological factors. The association between AOD and PM is variable and occasionally nonlinear due to influences such as planetary boundary layer height (PBLH), relative humidity (RH), wind direction (WD), and wind speed (WS). The AOD-PM relationship fluctuates regionally and seasonally, crucially influenced by meteorological factors. Utilizing AOD, ground-based PM data, and meteorological reanalysis data, we investigate the spatiotemporal characteristics of the AOD-PM relationship and the influencing factors. Results indicate that PBLH, RH, WD, and WS significantly impact the AOD-PM relationship. WD and WS can alter aerosol types, while RH and PBLH are geographically dependent, necessitating consideration in AOD-PM analyses. Notably, AOD-PM correlations are more pronounced in low WS conditions. PBLH and RH exhibit interconnected effects on the AOD-PM relationship, warranting caution when analyzing them separately. These findings contribute to the comprehension of the dynamic AOD-PM relationship, enhancing the precision of PM estimations throughout diverse spatiotemporal ranges.
Session Chair(s): Masao GEN, Chuo University
AS16-A004
| Invited
Enhanced Heterogeneous Decomposition of Inorganic Nitrogen Compounds on Deliquesced Aerosol Particles
Haotian ZHENG1#+, Shuxiao WANG2, Shaojie SONG3, Masao GEN4
1The Hong Kong Polytechnic University, 2Tsinghua University, 3Nankai University, 4Chuo University
The decomposition of nitrogen compounds serves as the basis for atmospheric chemistry and impacts air quality and climate. Recent studies found that the reaction rates of heterogeneous decomposition of nitrogen compounds on aerosol surfaces could reach several orders of magnitudes higher than those in gas phase or dilute water. We integrated laboratory experiments, field observation, and chemical transport model to study two heterogeneous pathways, i.e., photolysis of particulate nitrate and hydrolysis of NO2, and quantified their influence on air quality modeling. The photolysis of particulate nitrate produces HONO, which can oxidize SO2 to sulfate in aerosol water. We find that the significance of this pathway mainly depends on the enhancement effects (by 1–3 orders of magnitude as suggested by the available experimental studies) of nitrate photolysis rate constant () in aerosol liquid water compared to that in the gas phase. Comparisons between model simulations and in-situ observations in Beijing suggest that this pathway can explain about 15% (assuming an enhancement factor (EF) of 10) to 65% (assuming EF = 100) of the model–observation gaps in sulfate concentrations during winter haze. The heterogeneous hydrolysis of NO2 on aerosol water was considered insignificant due to low reaction rate. We find that high ionic strength (I) enhances the reaction rate constants (kI) by more than two orders of magnitude compared to that at infinite dilution (kI=0), yielding log10(kI/kI=0) = 0.058I. Modeling results show that heterogeneous NO2 hydrolysis greatly reduces the negative bias in the simulated concentrations of HONO and nitrate when compared to field observations over the North China Plain and further enhances atmospheric oxidation capacity. Our results suggest that the influence of the heterogeneous decomposition of inorganic nitrogen compounds could be underestimated in previous studies, while more studies are needed to reduce the uncertainties of the enhancement effect.
AS16-A020
| Invited
Understanding the SO2-NO2 Heterogeneous Reaction on the Single Particle Level Using Aerosol Optical Tweezers
Chenxi LI#+, Kaiqi ZHANG
Shanghai Jiao Tong University
Sulfate is one of the major components of atmospheric particulate matter, capable of exerting strong negative impacts on both the atmospheric environment and human health. In recent years, extensive research has been conducted on the mechanisms of sulfate formation. However, significant controversies still exist regarding the primary pathways of sulfate formation under different atmospheric conditions. In this study, we employ a counter-propagating aerosol optical tweezer to stably levitate individual particles in an atmosphere with controlled concentrations of SO2, NO2 and NH3 for extended periods. By collecting and analyzing the Raman scattering signals of the particles, we measure the growth rate and particle composition to reveal the SO2-NO2 heterogenous reaction mechanism and the influencing factors on the reaction rate. We find that due to resonant absorption of the trapping laser and sulfate generation, particle growth occurs in discrete steps (known as thermal locking). Within each step, the particle size slightly decreases, but the salt concentration gradually increases, accompanied by a slight increase in particle temperature compared with the room temperature. A newly developed model shows that the particle temperature and salt concentration variations are about 1K and 1mol/kg, respectively, within each thermally-locked step. The growth rate of particles significantly decreases as particle pH decreases, indicating a strong inhibitory effect of aerosol acidity on the SO2+NO2 reaction, consistent with findings in previous research. By using a multi-layer kinetic model to simulate the particle growth process, we discovered that sulfate generation reactions mainly occur in the vicinity of the particle surface, but at rates lower than those reported in existing literature. One potential cause for such discrepancies may be the different particle sizes used in previous research (nanometer particles) and the current study (micrometer particles).
AS16-A016
Resolving the Kinetics and Physical Property Changes of Atmospheric Organic Aerosol During Photolytic Aging
Bin BAI+, Pengfei LIU#
Georgia Institute of Technology
Organic aerosol (OA) particles represent a substantial fraction of submicron particulate mass in the atmosphere, exerting an important influence on climate. OA undergoes dynamic aging processes over its lifetime in the atmosphere, including photolytic aging directly induced by ultraviolet (UV) light irradiance. Despite its importance, knowledge gaps exist regarding the influence of photolytic aging on OA mass loading and climate-relevant properties such as hygroscopicity, and previous laboratory findings have not been validated with ambient OA. Information about the intermediate stages and time-dependent evolution of OA properties during photolytic aging remain obscure. In this study, we conducted isothermal photolytic aging experiments for both laboratory-generated secondary organic aerosols (SOA) and ambient particles in Atlanta, US, using a high-sensitivity quartz crystal microbalance (QCM-D). Our results reveal that photolytic aging depletes OA mass with lifetimes ranging from 5 to 200 solar hours. This process generates highly volatile vapors and intermediate/semi-volatile moieties, impacting OA composition and partitioning. We also observed diverse changes in OA hygroscopicity, influenced by the initial oxidation state. A thermodynamic volatility model that incorporates photolytic volatility transformation can explain the observed measured mass decay, volatility, and hygroscopicity profiles during photolytic aging within a uniform framework. This study advances our understanding of the complex kinetics, chemical transformations, and physical property changes of OA during photolytic aging, offering insights into OA's atmospheric behavior and climate impact.
AS16-A017
| Invited
Sulfate Formation Driven by Wintertime Fog Processing and a Hydroxymethanesulfonate Complex with Iron: Observations from Single-particle Measurements in Hong Kong
Yang ZHOU 1#+, Yanjing ZHANG1, Rongrong HAN1, Stephen GRIFFITH2, Guanru WU1, Lei LI3, Wenshuai LI1, Mei LI3, Zhen ZHOU3, Wencai WANG1, Lifang SHENG1, Jian Zhen YU4
1Ocean University of China, 2National Taiwan University, 3Jinan University, 4The Hong Kong University of Science and Technology
Fog processing has a significant impact on sulfur chemistry in the atmosphere. This study analyzed three winter fog events in Hong Kong using single-particle aerosol mass spectrometry (SPAMS) and a Monitor for AeRosols and GAses in ambient air (MARGA). Black carbon (BC)-related carbonaceous particles with substantial sulfate amounts comprised the largest particle number fraction (56.7%). Sulfate mass concentration decreased during fog due to the cloud’s effective scavenging, but fog processing notably promoted sulfate formation at the single-particle level (average peak area increases of 31.2%). Hydroxymethanesulfonate (HMS), an important S(IV) compound and fog tracer, was identified accounting for up to 12% by particle number fraction. Although pH showed a positive correlation (r = 0.53–0.69) with HMS particles in each fog scenario, a negative overall correlation (r = -0.51) was observed. Further analysis revealed that the higher aerosol acidity (pH 0.65–3.11), promoted Fe dissolution, leading to 49% of HMS particles being mixed with Fe, which potentially facilitated sulfate formation via the Fenton reaction. Additionally, around 40% of HMS-Fe particles are mixed with oxalate, thereby warranting further attention for their potential to cause more intricate sulfur oxidation processes. This study reveals the initial identification of a high mixed-state of HMS-Fe, which could potentially serve as a crucial avenue for the formation of sulfate on individual particulate matter. Considering the persistent augmentation of aerosol acidity in the Asian region, this phenomenon necessitates further investigation and attention.
AS16-A022
Observational Research of Hydroxymethanesulfonate (HMS) in Beijing and Its Atmospheric Implication
Yunzhi XU1#+, Tao MA2
1Tsinghua University, 2Guangdong University of Technology
Hydroxymethanesulfonate (HMS) is considered to be the most abundant organic aerosol species in North China Plain, which is formed by dissolved SO2 and HCHO in aqueous solution. HMS formation is an important pathway contributing to North China’s haze pollution in autumn and winter, and can explain some of the sulfate overestimation. Previous studies found HMS could come from cloud water, fog water or aerosol water processes. So far, reports on HMS in aerosols focused on humid and cold environments like northern China and near the Arctic areas, while its atmospheric prevalence is unclear and the medium of production is controversial. In the spring of 2021, in March and April, northern China including megacity Beijing witnessed several sandstorm events featured with high particulate levels both in coarse and fine mode. Sandstorm is a kind of typical spring pollution, which have significant impacts on air quality, health, and climate. In this study, we quantified the presence of HMS in sandstorm samples using an optimized ion chromatography method. The average HMS concentration in PM2.5 during the whole campaign was 0.066 ± 0.098 μg m-3 with a maximum value of 0.441 μg m-3. We studied different characteristics and influencing factors of HMS formation during haze and sandstorm episodes. In addition, we studied the distribution and contribution of HMS in different particle sizes during the sandstorm episodes. Our results provide direct observational evidence of heterogeneous HMS formation on the surface of mineral aerosols. HMS is used in this study to illustrate a more complex trend of sandstorm pollution in recent years. Considering that the precursors of HMS, SO2 and HCHO, are mainly from anthropogenic sources and secondary formation in the atmosphere, the presence of HMS in sandstorms indicates that dust particles nowadays are affected by anthropogenic pollution and have become more complex.
AS16-A009
Multiscale Simulations of the Multiphase Chemistry of Hydroxymethylsulfonate (HMS) Aerosols
Haoqi WANG#+
Nankai University
Hydroxymethylsulfonate (HOCH2SO3−, HMS), since its discovery in cloud water in the 1980s, has been recognized as a cloud/fog processing tracer. In earlier years, low levels of HMS were detected in ambient aerosols in Europe and North America, with concentrations below 0.1 μg m–3. Laboratory experiments confirmed the nucleophilic addition of dissolved HSO3− and SO32− and HCHO as the sole source of HMS. The second-order rate constants (k1 and k2), along with the first-order rate constant of HMS decomposition (kd), were also quantified. These chemical mechanisms describing HMS were first incorporated into the cloud chemical box model over the last century. Nevertheless, field measurements in the North China Plain (NCP) found a high HMS concentration at about 2.0 μg m–3, accounting for around 30% of the total sulfur. Laboratory experiments showed that ionic strength significantly increased the rate constant for HMS formation, implying that aqueous aerosols could be a potential medium for HMS formation. In this study, we developed HMS multiphase chemistry in a three-dimensional chemical transport mode GEOS-Chem. The model incorporated the effects of mass transfer processes such as cloud entrainment/detrainment and atmosphere-cloud droplet/aerosol intra/interphase diffusion on reactants and products. Global modeling indicated that high concentrations of HMS typically occur in the lower troposphere, particularly in the Northern Hemisphere, notably Asia, during winter. The nested simulations could match well with the observations in Beijing, in 2015. The high ionic strength of aerosol water greatly facilitated the generation of HMS. That is, aerosol water is also an important medium for HMS generation besides cloud water. The results of the sensitivity experiments indicated that the mutual constraints between emissions, meteorology, and the physicochemical properties of cloud/aerosol liquid water combine to influence the interannual variability of the HMS.
AS16-A005
Long-term Trend Analysis of Visibility and Fine Particulate Matter Characteristics in Central Taiwan
Hong En LAI+, Ta Chih HSIAO#
National Taiwan University
Atmospheric particulate matter (PM) is a primary air pollutant in urban areas. An increase in PM2.5 mass concentration significantly impacts human health and reduces atmospheric visibility. Continuous environmental monitoring is crucial to assess the efficacy of pollution control policies and inform future strategies. However, routine observations of aerosol optical parameters associated with atmospheric visibility and the corresponding high-time-resolution chemical composition of particulate matter are lacking, limiting our understanding of the factors contributing to visibility impairment. Additionally, changes in air quality due to emission reductions can be masked by meteorology, making it highly challenging to determine the impact of control measurements. This study used high-time-resolution instruments to continuously monitor visibility and PM chemical composition from 2017 to 2022 in central Taiwan. Theil-Sen trend analysis was used to determine trends in chemical composition, while a dispersion-normalized approach coupled with seasonal classification based on meteorological conditions was used to mitigate the weather impact on air pollutants. The results show a 35% decrease in extinction coefficient and a 24% decrease in PM2.5, while PM1.0 showed no decrease, especially during visibility degradation. The increasing proportion of PM1.0 in PM2.5 implies a shift from PM1.0-2.5 to PM1.0 dominance in visibility degradation. In addition, the proportion of organic matter in PM2.5 has increased during visibility degradation events in recent years, and the chemical composition has shifted from ammonium nitrate dominance to organic matter dominance when PM1.0 primarily drives pollution, indicating a better understanding of the chemical composition and contribution of PM1.0 is needed. In addition, the long-term trend shows that the contribution of inorganic salts to PM2.5 has decreased in recent years, suggesting that the air pollution control strategy of recent years has achieved some success.
AS16-A014
Dirty Building Surfaces Release Organic Sulfur Compounds Upon Interaction with Sulfur Dioxide and Sunlight Radiation During Day Time
Huifan DENG+, Sasho GLIGOROVSKI#
Chinese Academy of Sciences
Organic sulfur (OS) compounds have been globally identified in ambient secondary organic aerosols (SOA), but their contribution to organic mass remains inadequately quantified, and the current models considerably underestimate ambient SOA formation. OS compounds are surface active and may also play a role in cloud formation. Here, we investigated the reactive uptake of SO2 on urban grime in the dark and under simulated sunlight irradiation at different RHs and applied a kinetic multilayer model of aerosol surface and bulk chemistry. The heterogeneous reaction of sulfur dioxide (SO2) with authentic urban grime under near-ultraviolet sunlight irradiation leads to a large suite of various organic compounds including OS released in the gas phase. Furthermore, we estimated the surface area of urban buildings in the city of Guangzhou on the basis of a building dataset. Calculations indicate that at the core area of Guangzhou, building surface uptake of SO2 is 15 times larger than uptake of SO2 on aerosol surfaces, yielding ~20 ng m−3 of OS that represents an important fraction of the observed OS compounds (60 to 200 ng m−3) in ambient aerosols of Chinese megacities. This chemical pathway occurring during daytime can contribute to the observed fraction of OS compounds in aerosols and improve the understanding of haze formation and urban air pollution.
Session Chair(s): Adam CLAYTON, Korea Institute of Atmospheric Prediction Systems, Soyoung HA, National Center for Atmospheric Research
AS49-A007
| Invited
A Quantile Conserving Ensemble Filtering Framework for Tracer Concentration and Source Estimation and Parameters
Jeffrey ANDERSON#+
NSF National Center for Atmospheric Research
Ensemble filter assimilation algorithms can be described as two steps: 1). Computing increments for an observed variable given an ensemble prior and an observation; 2). Computing increments for state variables given the observation increments. An efficient algorithm that allows the use of arbitrary continuous priors and likelihoods for the first step is described. The key innovation is to select posterior ensemble members with the same quantiles with respect to the continuous posterior distribution as the prior ensemble had with respect to the prior continuous distribution. The second step is a regression in a space to which observed and state variables were independently transformed with a probability integral transform followed by a probit transform; this is a specific form of anamorphosis. This guarantees that the posterior ensembles for state variables have many of the advantages of the observation space quantile conserving posteriors. For example, if state variables are bounded then posterior ensembles will respect those bounds and eliminate most bias near the boundary. Additional challenges arise when applying filters for quantities like rainfall or tracer concentration and source where the appropriate priors can be best represented by mixed PDFs; PDFs that are a sum of continuous and discrete functions. For instance, a source may be exactly zero with finite probability and it may be appropriate to have ensembles that have multiple members that are identical values. An extension of the quantile conserving filter framework that supports ensembles with duplicate values is presented. The new method produces significantly enhanced capabilities for tracer concentration and source estimation in an idealized tracer transport model and in atmospheric GCMs with chemical weather extensions. It is also appropriate for many parameter estimation applications.
AS49-A017
| Invited
KIAPS Data Assimilation for Coupled Earth System
In-Hyuk KWON#+, Adam CLAYTON, Jeon-Ho KANG, Yonghwan KWON, Sanghee JUN, Hye-yeong JANG, Jiyoun KIM, Eunbyeol KO, Dayoung CHOI
Korea Institute of Atmospheric Prediction Systems
The goal of the Korea Institute of Atmospheric Prediction Systems (KIAPS) is to develop a unified framework for accurate weather forecasting from very short range (~6 hours) to extended medium range (~30 days), including coupling to various Earth system components, such as the land surface, oceans, and sea ice. The first phase of the KIAPS project resulted in the global atmospheric NWP system that became operational at the Korea Meteorological Administration (KMA) in April 2020. The NWP model, named the Korean Integrated Model (KIM), is a non-hydrostatic model that uses a cubed-sphere grid and the spectral element method for its dynamical core. The global data assimilation (DA) system of KIM is based on a hybrid-4DEnVar system for the deterministic analysis, and a local ensemble transform Kalman filter (LETKF) for ensemble perturbation updates, and is already giving good performance. Various observation types, including conventional data and satellite radiances, are quality controlled and prepared for assimilation by the KIM Package for Observation Processing (KPOP). Our current development plans include: 1) Developing convective-scale DA to derive initial conditions for short-term severe weather forecasts. A limited area version of LETKF tailored for the reference regional model has been established, emphasizing radar and other high-resolution observations for small-scale analysis; 2) NEMOVAR (Variational data assimilation for NEMO ocean model) is being built for coupled atmosphere-ocean DA, and weakly coupled DA using background fields from the coupled model is tested; and 3) Land surface DA using the existing NASA-LIS has been established for 8-km resolution KIM, and ASCAT is being used to generate soil moisture analysis. Further researches are being conducted on using SMAP and SMOS data for soil moisture DA, and a land surface DA system using LETKF instead of LIS is also being developed.
AS49-A004
Convolutional Neural Network-based Adaptive Localization for an Ensemble Kalman Filter
Lili LEI#+
Nanjing University
Flow-dependent background error covariances estimated from short-term ensemble forecasts suffer from sampling errors due to limited ensemble sizes. Covariance localization is often used to mitigate the sampling errors, especially for high dimensional geophysical applications. Most applied localization methods, empirical or adaptive ones, multiply the Kalman gain or background error covariances by a distance-dependent parameter, which is a simple linear filtering model. Here two localization methods based on convolutional neural networks (CNNs) learning from paired datasets are proposed. The CNN-based localization function (CLF) aims to minimize the sampling error of the estimated Kalman gain, and the CNN-based empirical localization function (CELF) aims to minimize the posterior error of state variables. These two CNN-based localization methods can provide localization functions that are nonlinear, spatially and temporally adaptive, and non-symmetric with respect to displacement, without requiring any prior assumptions for the localization functions. Results using the Lorenz05 model show that CLF and CELF can better capture the structures of the Kalman gain than the best Gaspari and Cohn (GC) localization function and the adaptive reference localization method. For both perfect- and imperfect-model experiments, CLF produces smaller errors of the Kalman gain, prior and posterior than the best GC and reference localization, especially for spatially-averaged observations. Without model error, CELF has smaller prior and posterior errors than the best GC and reference localization for spatially-averaged observations, while with model error, CELF has smaller prior and posterior errors than the best GC and reference localization for single-point observations.
AS49-A020
Towards an End-to-end Data Assimilation System for Atmospheric Composition with Joint Effort for Data Assimilation Integration (JEDI)
Maryam ABDI-OSKOUEI1, Shih-Wei WEI1, Jerome BARRE2, Sarah LU3#+
1University Corporation for Atmospheric Research, 2National Center for Atmospheric Research, 3University at Albany, State University of New York
Joint Effort for Data Assimilation Integration (JEDI) is a unified data assimilation (DA) framework for Earth system prediction and reanalysis developed by the Joint Center for Satellite Data Assimilation (JCSDA). Its primary goals are to streamline research and operational efforts and enhance community collaboration. One major effort that JCSDA is undertaking is the implementation of a robust 4D-Var system for numerical weather prediction but also atmospheric composition applications (such as air quality and anthropogenic emission monitoring). This presentation provides an overview of recent advancements in data assimilation for atmospheric composition applications through the JEDI framework. In specific, we will provide the following update. First, JEDI can cover various data assimilation methodologies ranging from simple 3DVar to 4DEnVar. One example is Prototype NOAA Aerosol ReAnalysis version 1.0 (pNARA v1.0) for the year 2016. In pNARA v1.0, the analysis system is based on 3D-EnVar DA system configuration using elements of the JEDI framework. Second, JCSDA has enlarged the fleet of integrated observations in the atmospheric composition segment, namely TropOMI NO2 and CO, MOPITT CO, MODIS AOD and VIIRS AOD. Furthermore, integration of the TEMPO proxy data is tested. Third, stretched grid DA capability has been implemented and tested in the JEDI system to increase the model resolution within an affordable range of computational cost. We will demonstrate this DA capability with NASA GEOS Composition Forecast (GEOS-CF) model.
AS49-A016
Assimilation of the Microwave Temperature and Humidity Sounders Into the Global Climate Model Using the Ensemble Kalman Filter
Young-Chan NOH1#+, Yonghan CHOI1, Hyo-Jong SONG2, Kevin RAEDER3, Joo-Hong KIM1, Youngchae KWON2
1Korea Polar Research Institute, 2Myongji University, 3National Center for Atmospheric Research
We attempt to assimilate observations from the Advanced Microwave Sounding Unit-A (AMSU-A) and Microwave Humidity Sounder (MHS) on board the low-earth-orbiting satellites. In this study, the data assimilation system consists of the Data Assimilation Research Testbed (DART) and the Community Earth System Model as the global forecast model. DART is based on the ensemble Kalman filter technique, supporting the radiative transfer model that is used to simulate the satellite observations from the model state. In this study, preprocessing modules are developed to assimilate the AMSU-A and MHS data within DART. The preprocessing package mainly consists of the quality control, spatial thinning, and bias correction processes. In the quality control, two sub-processes are included: outlier test and channel selection depending on the cloud condition and surface type. The bias correction process is divided into scan-bias correction and air-mass-bias correction. In addition, the observation error variances are estimated for the AMSU-A and MHS channels, using the assimilation outputs from pre-trial experiments. In the trial experiments, a positive analysis impact is obtained by assimilating the AMSU-A and MHS on top of the DART data assimilation system that already makes use of the conventional measurements. In particular, the analysis errors are significantly reduced in the whole troposphere and lower stratosphere over the Northern and Southern Hemisphere. Overall, this study demonstrates a positive impact on the analysis (called initial condition) when the AMSU-A and MHS observations are assimilated in the DART assimilation system.
AS49-A002
Improving Numerical Simulation of the Record-breaking Dust Event of March 2021 Through Multi-scale Data Assimilation of Aerosol Observations
Shuang MEI#+, Wei YOU, Wei ZHONG, Zengliang ZANG
National University of Defense Technology
Using the Weather Research and Forecasting Chemistry (WRF-Chem) model, this study conducted cycling data assimilation and prediction experiments of the Himawari-8 satellite aerosol optical depth (AOD) product and ground particulate concentration (PM) data during a record-breaking dust event in the Beijing-Tianjin-Hebei region from March 14 to 18, 2021. Three experiments were conducted, comprising a control experiment without assimilation, a traditional three-dimensional variational (3DVAR) experiment, and multi-scale three-dimensional (MS-3DVAR) variational experiment. The results indicate that the control experiment with WRF-Chem model significantly underestimates the intensity and extent of the severe dust event, while the analysis fields and forecasting fields of PM concentration and AOD can be significantly improved in both assimilation experiments. Besides, the MS-3DVAR assimilation approach can utilize multi-scale information in the observational data, thereby yielding better-fitting extreme values and smoother gradients of pollutant concentrations in the initial fields than the 3DVAR assimilation experiment. Compared to the control experiment, the correlation coefficient (CORR) of MS-3DVAR assimilation between the assimilated PM10 analysis fields and observations increased from 0.019 to 0.906. Root mean squared error (RMSE) decreased from 85.080 µg/m3 to 25.295 µg/m3. Independent verification using ground-based Aerosol Robotic Network (AERONET) AOD observations also showed a significant improvement in the simulated AOD value after cycling MS-3DVAR assimilation. And the best assimilation results were obtained at the initial time of forecast and the positive assimilation effect can persist longer than 36 hours.
AS49-A005
Added Value of Three-dimensional Horizontal Winds from Geostationary Interferometric Infrared Sounder for Typhoon Forecast in a Regional NWP Model
Deming MENG1#+, Zhe-Min TAN2, Jun LI3, Zheng MA4, Chen YAODENG1
1Nanjing University of Information Science & Technology, 2Nanjing University, 3National Satellite Meteorological Center, 4Chinese Academy of Sciences
High temporal resolution geostationary hyperspectral infrared sounders can simultaneously profile atmospheric temperature and moisture and track moisture features to provide 3D horizontal winds in clear and partially cloudy scenarios. Thermodynamic information has proven helpful to tropical cyclone (TC) forecasts in numerical weather prediction (NWP) models, but the benefits of dynamic information from geostationary hyperspectral infrared sounders (GeoHIS) are still to be understood. With the re-estimated observation error and multivariate hydrometeor background error covariance, the 3D horizontal winds from the Geostationary Interferometric Infrared Sounder (GIIRS) are synergistically assimilated with hydrometeor information. Then, the impact of the GIIRS-derived 3D horizontal wind assimilation on Typhoon Maria (2018) and Lekima (2019) analysis and forecast are evaluated based on the cycling data assimilation and forecast experiments. Results show that assimilating GIIRS-derived 3D horizontal wind reduces the RMSEs of analysis and forecast for both typhoons, particularly in U and V components. The improved accuracy of large-scale conditions advances typhoons’ track and maximum wind speed forecasts while neutrally improving central sea-level pressure. Furthermore, the additional wind assimilation improves the spatial distribution and intensity of both typhoons’ landfall precipitation prediction. The detailed diagnoses of the Maria case show that a more southerly subtropical high generated by the additional wind assimilation improves the rainfall spatial distribution, and the reasonable water vapor transportation caused by the improved dynamic conditions corrects the precipitation intensity. This work highlights the importance of dynamic information in TC forecasting and emphasizes the need for efficient and high-precision 3D wind measurements to improve NWP models.
AS49-A006
An Equilibrium Between Chaotic Loss and Observational Gain of Information in Forecast-assimilation Cycles
Jie FENG1#+, Zoltan TOTH2
1Fudan University, 2National Oceanic and Atmospheric Administration
Data Assimilation (DA) - Numerical Prediction (NP) systems are designed to monitor the behavior of natural systems. We interpret such systems as shadowing with observations. In this presentation, a general and minimalistic approach is proposed to model the behavior of the coupled Nature - Observing - Data Assimilation - Prediction (NODAP) system. In a General Error Behavior (GEB) model, we select a minimal number of critical parameters to describe the behavior of the analysis equilibrium in the forecast-assimilation cycle. In case of successful shadowing, the amplitude of analysis error between the natural and simulated systems is found to reflect an equilibrium between information gained in the DA step from observing the natural system, and information lost in the NP step of the DA-NP subsystem due to the chaotic expansion of errors. The regime that supports successful long term shadowing is quantitatively studied in the parameter space of observational information accessed by DA, chaotic error growth, the analysis ratio between the assumed observational and background forecast error variances, and the amount of noise added in the DA step.
AS49-A003
Analysis of the Impact of Mass–wind Balance Relationships on Surface Data Assimilation of High Resolution Regional Model
Weiyu DING#+
China Meteorological Administration
With the improvement of model resolution, the recognizable shortwave information of numerical models increases. The mass–wind balance relationships based on geostrophic balance cannot fully meet the needs of data assimilation in low latitude regions and high-resolution convective scale models. This article proposes a mass–wind balance relationships based on the multigrid method, which adds correction without mass-wind constraints on the basis of large-scale mass–wind balance. Single point assimilation experiments and typical case studies were conducted based on the GRAPES (Global Regional Association and PrEducation System) three-dimensional variational system and mesoscale regional model. The experimental results indicate that the new mass–wind balance relationship will significantly increase the analysis increment of several tens of kilometers scale in the lower layer of the model, followed by an increase in analysis increment of about 100 to 200 kilometers scale. The assimilation analysis increment of the new mass–wind balance experiment can describe more increment center positions compared to the control experiment of linear balance constraint, better describing the low-level water vapor convergence, and improving the simulation of initial 0-3 hour precipitation ,0-6 hour 10 meter wind and surface pressure.
Session Chair(s): Huizhong SHEN, Southern University of Science and Technology
AS14-A014
| Invited
Regional Atmospheric and Health Impact Modeling Over the Contiguous U.S.: Linking Energy Use, Emissions, Air Quality, and Health and Economic Impacts
Yang ZHANG#+
Northeastern University
Transition from fossil fuel based energy to clean energy will cause changes in air pollutant emissions, which in turn affect air quality and air pollution induced health outcomes such as mortality and morbidity. In this work, several state-of-science online-coupled models are applied to generate the best possible predictions of surface ozone (O3) and fine particulate matter (PM2.5) concentrations under current emission and climate conditions and their projections under five energy transition scenarios in the U.S. These scenarios include a reference scenario without the clean power plan (refnocpp), a scenario with abundant natural gas (highNG), a scenario with high electric vehicle market share (highEV), a scenario with port electrification (port), and a scenario with intensive building energy efficiency (highEE). The predicted changes in the concentrations of O3 and PM2.5 under these scenarios are then used to drive the Environmental Benefits Mapping and Analysis Program-Community Edition to assess the health and economic impacts of the energy transition scenarios. The skills of individual models and their ensembles are evaluated using available surface network data for simulations under current emission and climate conditions. Compared to individual models and the simple ensemble mean, the weighted ensemble predictions based on the multi-linear regression give the best overall performance for both O3 and PM2.5. Large reduction in mortalities occur for populated urban areas where the changes in emissions are large under all scenarios. Among the scenarios examined, the highEE scenario is projected to lead to the largest reductions in air pollutant emissions, leading to the maximum co-benefit to both air quality and public health. These results provide scientific basis for air pollutant emission control and public health improvement strategies, and inform the relative co-benefit and priority of these future energy transition scenarios.
AS14-A025
| Invited
Agricultural Ammonia Emission Mitigation Potentials and Associated PM2.5 Air Quality and Nitrogen Deposition Benefits in North China
Lin ZHANG1#+, Lu LI1, Yixin GUO2, Zehui LIU1
1Peking University, 2The Hong Kong University of Science and Technology
Ammonia is an important precursor of PM2.5, and it is primarily emitted from agricultural activities. Here we established a framework linking agricultural management technology/measures, an agricultural ammonia emission inventory, and a chemical transport model to assess the mitigation potentials of ammonia emissions in North China. We collected 51 measures of fertilizer application and 53 measures of livestock farming derived from a literature search and then applied them to an updated agricultural ammonia emission inventory at a 3-km resolution in the Beijing-Tianjin-Hebei (BTH) region of North China. The Monte Carlo method was utilized to account for the uncertainties in the management measures. We find that ammonia emissions from livestock farming could be reduced by 79-151 Gg (30%-57%) and from fertilizer application by 58-163Gg (18%-51%) in the BTH region in 2019. We applied two reduction scenarios that could achieve, respectively, the average and maximum ammonia emission reduction, and evaluated the resulting improvements in air quality and nitrogen deposition using the GEOS-Chem High Performance (GCHP) model at a 10-km horizontal resolution in the BTH region. The results show that the baseline of PM2.5 concentration, NHx and NOy deposition in the BTH region in 2019 is 27-61 µg/m3, 8-57 Gg N/month, and 3-51 Gg N/month. Under two ammonia emission reduction scenarios, PM2.5 concentration and NHx deposition would, respectively, reduce 1.4-3.9 µg/m3, 3-14 Gg N/month while NOy deposition would increase 0.5-2 Gg N/month. Our research shows that agricultural ammonia has great emission reduction potential that would benefit the reduction of nitrogen pollution.
AS14-A024
| Invited
Grid-by-grid and Day-by-day Top-down Bottom-up SLCF Emissions from Chinese Energy-related Sources
Jason COHEN#+
China University of Mining and Technology
China is undergoing economic development, movement of people from rural areas into cities, increased energy usage, and increased material and mineral production. At the same time air pollution regulations and energy efficiency have been improving, and new double-carbon policies have been implemented. These factors have led to a wide set of changes of emissions from coal and other fossil sources in terms of magnitude, location, and time. This work uses observations from flux towers, CEMS, upward looking remote sensing, and surface concentration measurements located at and around various coal use sites around China to form a new multi-species emissions dataset. The datasets are used to train flexible, mass-conserving models of simple physics, chemistry, transport, and thermodynamics. These models are used to estimate top-down emissions of NOx, CO, BC, and CH4 using observations from TROPOMI, GF5, and other satellites. Emissions include both day-to-day and grid-to-grid variation, as well as a robust uncertainty range, and are computed on all known energy production and usage grids sources, as well as surrounding grids. The emissions demonstrated attribution of power, steel, coking, aluminum, cement, boilers, rivers, and coalfields. Emissions controls are demonstrated over large-scale averages, and divergence at high geospatial distribution and temporal frequency are explained. A shift from large sources to distributed moderate sources is consistent with flows into tier 3 to 5 cities. While there are decreasing emissions of NOx and BC mass, CO and BC number show consistent increases in some areas and decreases in others. Case studies demonstrate a fundamental connection between CH4 and certain pollutant emissions, a previously unexplored area. Finally, explicit uncertainty analysis concludes 15-20% of all grids have an uncertainty larger than the day-to-day variability, meaning current assessment methods using annual or monthly averages and estimates of small sources may contain bias.
AS14-A021
Improved Estimation of Biomass Burning Emission Based on Multi-source Data
Ying ZHOU#+
Beijing University of Technology
Biomass burning (BB) has an important impact on global, regional and local air quality and human health. Because of the scattered emission and the difficulty in capture, there are some problems in the development of the BB emission inventories, such as lack of key activity data, low spatial-temporal resolution and delayed updates, which limit the research on air pollution and climate change, and restrict the formulation of air quality control policies. (1) Based on the investigation and statistical analysis of key basic information (e.g., proportion of domestic and in-field straw burning, firewood burning quantities), as well as the systematic collection of localized emission factors and component profiles, an elaborate BB emission inventory was developed for China with 1-day temporal resolution and spatial resolution of 1km*1km, which included domestic and in-field burning of crop straw, firewood burning, livestock excrement, forest and grassland fires and 12 kinds of pollutants and GHGs (including detailed species information for PM2.5 and VOCs). (2) By integrating the satellite remote sensing, land use, phenological information, statistical data, and field investigation, emission inventory of open burning for 12 types of crop residues, based on the bottom-up approach, were developed and could be quickly updated. (3) The geostationary and polar-orbiting satellites including the localized satellite are combined for the first time to achieve the near-real-time emission estimation of open burning of crop residue (OBCR) with complete coverage in China. The results provided support for the second national census on pollution source, and air quality assurance for the 2022 Winter Olympics. The results of the OBCR have been incorporated into the Multi-resolution Emission Inventory model for Climate and air pollution (MEIC).
AS14-A012
National Quantification of Methane Emissions Using High-resolution Satellite Data
Lu SHEN1#+, Huiru ZHONG1, Daniel JACOB2, Ritesh GAUTAM3, Mark OMARA3, Jintai LIN1, Tia SCARPELLI4, Alba LORENTE3, Daniel ZAVALA-ARAIZA3, Xiao LU5, Zichong CHEN6
1Peking University, 2Harvard University, 3Environmental Defense Fund, 4University of Edinburgh, 5Sun Yat-sen University, 6Harvard John A. Paulson School of Engineering and Applied Sciences
Methane (CH4) is the second most important anthropogenic greenhouse gas after CO2 and is responsible for 0.6°C global warming since preindustrial times. Reducing methane emissions from fossil fuel exploitation (oil, gas, coal) is an attractive target for climate policy, but current national emission inventories submitted to the United Nations Framework Convention on Climate Change (UNFCCC) are highly uncertain. Here we use high-resolution satellite observations from the TROPOMI instrument to better quantify national emissions worldwide by inverse analysis at up to 50 km resolution. We find global emissions of 62.7 ± 11.5 (2σ) Tg a-1 for oil-gas and 32.7 ± 5.2 Tg a-1 for coal. Eight countries have methane emission intensities from the oil-gas sector exceeding 5% of their gas, and lowering these intensities to the global average level would reduce global oil-gas emissions by 11 Tg a-1 or 18%. We also conduct an ensemble (~40) of high-resolution inversions in China to assess the sensitivity of the results to different bottom-up inventories, satellite data density, and choices of inversion parameters. Our results imply that TROPOMI can provide significant information to assist China’s estimates from the energy sector, and the total coal emission is estimated to be 15 ± 3 Tg a-1 in 2022.
AS14-A010
High-resolution Hybrid Inversion of IASI Ammonia Columns to Constrain US Ammonia Emissions Using the CMAQ Adjoint Model
Yilin CHEN#+
Peking University
Ammonia (NH3) emissions have large impacts on air quality and nitrogen deposition, influencing human health and the well-being of sensitive ecosystems. Large uncertainties exist in the “bottom-up” NH3 emission inventories due to limited source information and a historical lack of measurements, hindering the assessment of NH3-related environmental impacts. The increasing capability of satellites to measure NH3 abundance and the development of modeling tools enable us to better constrain NH3 emission estimates at high spatial resolution. In this study, we constrain the NH3 emission estimates from the widely used 2011 National Emissions Inventory (2011 NEI) in the US using Infrared Atmospheric Sounding Interferometer NH3 column density measurements (IASI-NH3) gridded at a 36 km by 36 km horizontal resolution. With a hybrid inverse modeling approach, we use the Community Multiscale Air Quality Modeling System (CMAQ) and its multiphase adjoint model to optimize NH3 emission estimates in April, July, and October. Our optimized emission estimates suggest that the total NH3 emissions are biased low by 26 % in 2011 NEI in April with overestimation in the Midwest and underestimation in the Southern States. In July and October, the estimates from NEI agree well with the optimized emission estimates, despite a low bias in hotspot regions. Evaluation of the inversion performance using independent observations shows reduced underestimation in simulated ambient NH3 concentration in all 3 months and reduced underestimation in NH4+ wet deposition in April. Implementing the optimized NH3 emission estimates improves the model performance in simulating PM2.5 concentration in the Midwest in April. The model results suggest that the estimated contribution of ammonium nitrate would be biased high in a priori NEI-based assessments. The higher emission estimates in this study also imply a higher ecological impact of nitrogen deposition originating from NH3 emissions.
AS14-A020
Global High-resolution Livestock Ammonia Emission Inventory from 1961 to 2021
Lianming ZHENG+, Huizhong SHEN#
Southern University of Science and Technology
Estimates of global livestock ammonia (NH3) emissions have encountered limitations, lacking details based on rearing stages and systems. In this study, we established a detailed annual bottom-up global high-resolution inventory of livestock NH3 emissions from four stages of manure management, with a spatial resolution of 0.083° × 0.083° for the period from 1961 to 2021. The total livestock NH3 emissions surged from 12.5 to 27.1 Tg (a 117% increase) during this period. In 2021, cattle, chickens, and pigs emerged as the primary emission contributors, making up 52%, 28%, and 14%, respectively, while other livestock types (ducks, sheep, goats, and horses) accounted for only 6%. Concerning livestock rearing stages, field application of solid manure, livestock housing of solid manure, and storage of solid manure are the predominant stages, comprising 43%, 21%, and 15% of total emissions, respectively. At the continental level, Asia, Africa, and the Indian subcontinent emerged as the highest contributors, constituting 26%, 19%, and 19% of total emissions, respectively. From a national perspective, China, India, and the United States stood out as the top emitters, contributing 12%, 11%, and 8% to global emissions, respectively, although their emission growth rates have slowed in recent years. It is particularly noteworthy that India has seen a remarkable increase from 2.0 Tg in 1961 to 3.0 Tg in 2021, warranting attention to its future livestock NH3 emissions. This study improves our understanding of NH3 emissions from livestock production, providing a scientific foundation for stakeholders and policymakers to design region-specific, finely tailored emission reduction strategies in the future.
AS14-A011
Modeling of Fluorinated Greenhouse Gases with the Global Chemistry Transport Model GEOS-CHEM
Yali LI+, Juan LI, Yuyang CHEN, Lei ZHU#, Song LIU, Xicheng LI, Dongchuan PU, Xiaoxing ZUO, Weitao FU, Zhuoxian YAN, Peng ZHANG, Xin YANG, Tzung-May FU, Huizhong SHEN, Jianhuai YE, Chen WANG
Southern University of Science and Technology
Fluorinated gases (F-gases) are growing at the highest relative growth rate among all major greenhouse gases. Previous F-gases modeling studies are configured in the Lagrangian framework, with chemistry being addressed to the minimal level. Here, we add atmospheric chemical and physical processes of 27 F-gases (CFCs, HCFCs, HFCs, PFCs, SF6, NF3, and SO2F2) into the state-of-the-art GEOS-Chem model. The updated model captures most of the observed changes in mixing ratio of F-gases, with significant correlation coefficients (r > 0.55), slight normalized mean biases (NMB < 5.0%), and root mean square errors (RMSE) ranging from 0.01 to 3.03 ppt. Benchmarking shows that the updated model is consistent with the standard version in reproducing atmospheric species, including ozone, OH , CO, NOx, Cl, and ClO, due to the low levels of F-gases. Our work provides a comprehensive Eulerian model for studying F-gases, which could be incorporated into long-term simulations of the greenhouse effect.
AS14-A019
Emission and Influences of Non-road Mobile Sources on Air Quality in China, 2000-2019
Chaoyu WEN+, Jianlei LANG#
Beijing University of Technology
Non-road mobile sources (NRMS) are potential important contributors to air pollution in China. However, their extreme impact on air quality had been seldom studied. In this study, the emission inventory of NRMS in mainland China during 2000–2019 was established. Then, the validated WRF-CAMx-PSAT model was applied to simulate the contribution to the atmospheric PM2.5, NO3-, and NOx. Results showed that emissions increased rapidly since 2000 and reached a peak in 2014–2015, with an annual average change rate (AACR) of 8.7–10.0%; after then, the emissions were relatively stable (AACR, −1.4 to 1.5%). The modeling results indicated that NRMS has become a crucial contributor to the air quality in China: from 2000 to 2019, the contribution to PM2.5, NOx, and NO3- significantly increased by 131.1%, 43.9%, and 61.7%; and for NOx, the contribution ratio in 2019 reached 24.1%. Further analysis showed that the reduction (−0.8% and −0.5%) of the NOx and NO3- contribution ratios was much lower than that (−4.8%) of NOx emissions from 2015 to 2019, implying that the control of NRMS lagged behind the national overall pollution control level. The contribution ratio of agricultural machinery (AM) and construction machinery (CM) to PM2.5, NOx, NO3- in 2019 was 2.6%, 11.3%, 8.3% and 2.5%, 12.6%, 6.8%, respectively. Although the contribution was much lower, the contribution ratio of civil aircraft had the fastest growth (202–447%). Moreover, an interesting phenomenon was that AM and CM had opposite contribution sensitivity characteristics for air pollutants: CM had a higher Contribution Sensitivity Index (CSI) for primary pollutants (e.g., NOx), ~1.1 times that of AM; while AM had a higher CSI for secondary pollutants (e.g., NO3-), ~1.5 times that of CM.
Session Chair(s): Yuekui YANG, NASA Goddard Space Flight Center, Kyu-Myong KIM, NASA Goddard Space Flight Center, Myong-In LEE, Ulsan National Institute of Science and Technology
AS24-A007
| Invited
Investigations of Sea Ice, Cloud and Ocean Processes from Space-based CALIPSO and ICESat-2 Missions
Xiaomei LU#+, Yongxiang HU
NASA Langley Research Center
The seasonal cycles of ocean subsurface biological activity in the Antarctic Ocean are characterized using ICESat-2 measurements and the complex interactions between sea ice melt cycles, ocean biology, water cloud microphysics, and top-of-atmosphere (TOA) cloud albedo are explored. Ocean warming and sea ice melting increase phytoplankton populations in newly opened waters, which in turn leads to increased water cloud droplet number concentrations (Nd) and smaller cloud droplet sizes (Re). The combined effect of increasing Nd and decreasing Re leads to increased cloud albedos that help to offset the albedo decrease incurred from the melting sea ice. These results allow us to assess the effect of ocean biology on sea ice-albedo feedbacks in polar regions. We will present and discuss the science results from space lidars: CALIOP/CALIPSO and ATLAS/ICESat-2. Our results support the continued use of present and future spaceborne lidars to investigate the polar ecosystem response to climate change including interannual, decadal and seasonal changes of sea ice, marine biology activities, cloud and top of atmosphere (TOA) albedos in polar regions and their interactions.
AS24-A006
High Latitude Summertime Atmospheric Circulation Altered by Shrinking Arctic Sea Ice
Doo Young LEE#+, Sang-Wook YEH
Hanyang University
Since the post-2000s (POST), there has been a notable intensification in the decline of summer Arctic sea ice concentration (SIC), accompanied by an accelerated melting rate. Observational analysis strongly suggests that this rapid Arctic SIC decline trend during the POST period is closely associated with the reinforcement of the temperature rise trend observed across most Northern Hemisphere regions. Structural interchanges in the previously dominant Arctic atmosphere are identified as the primary catalyst for this phenomenon. Model experiments conducted to confirm causation prove that the rapid decrease in Arctic SIC, obtained by the Arctic sea surface temperature (SST) nudging regardless of global warming considerations, acts as a key driver for changes in the atmospheric modes. The impact of the altered atmospheric modes during the POST on the trend change in mid-latitude temperatures and extreme heat waves is presented.
AS24-A002
Irreversibility of the Arctic Sea Ice Area to CO₂ Removal
M. Inês CAJADA1#+, Jaeyoung HWANG1, Seok-Woo SON1, Hyo-Seok PARK2, Soon-Il AN3, Jongsoo SHIN4
1Seoul National University, 2Hanyang University, 3Yonsei University, 4Woods Hole Oceanographic Institution
A decrease of Arctic sea ice area (SIA) has been observed in recent decades and is projected to continue in a warming climate. Here, we show that such SIA change is not reversible when atmospheric CO2 concentrations are reduced. Large-ensemble climate model experiments, in which CO2 concentrations are quadrupled and then returned to the initial state, reveal a slow recovery of the Arctic SIA to CO₂ removal, preceded by fast SIA decrease to CO2 increase. While the Arctic SIA is under-recovered in most regions when CO2 concentrations are reduced to the present-day level, the North Atlantic region, in particular the Labrador Sea and Southern Greenland Sea, shows an over-recovery of SIA. The overall under-recovery of Arctic SIA is attributable to increased ocean heat transport and enhanced downward longwave radiation, partly due to more frequent atmospheric rivers in high latitudes in the CO2 removal period compared to the present-day state. In contrast, the over-recovery of North Atlantic SIA is caused by cold sea surface temperature in this region, resulting from a delayed recovery of Atlantic Meridional Overturning Circulation. This result suggests that SIA change to CO2 removal is determined by the opposing effects of atmospheric and oceanic circulations, the former being more important than the latter.
AS24-A009
| Invited
A Novel Perspective on the Factors Driving Future Changes in El Niño Teleconnection
Emilia Kyung JIN#+, Hyun-Ju LEE
Korea Polar Research Institute
Existing climate models consistently project an eastward and poleward shift in the El Niño teleconnection in the future. This study delves into the dynamic processes by examining the wavelength of Rossby waves through spectral analysis, measuring the distance between circulation anomalies, and exploring the dispersion relationship of barotropic Rossby waves. The findings indicate that the wavelength of waves contributing to the teleconnection is anticipated to increase in a warmer climate, accompanied by a rise in the proportion of zonal-wavenumber-2 waves.
Due to changes in the mean state, such as the strengthening of westerlies in high-emission scenarios, the frequencies of waves are altered based on their zonal wavenumbers. This phenomenon is more pronounced in the Southern Hemisphere, where the model spread of the mean state is smaller. Consequently, a notable outcome of this process is a shift in the El Niño's influence towards the high latitudes of both hemispheres. In particular, these changes also lead to changes in the impact of El Niño in Antarctica.
AS24-A008
Impact of Weakened Antarctic Circumpolar Current on the Arctic Climate
Peixi WANG1#+, Yuhui HAN1, Song YANG1, Jun YING2, Zhenning LI3, Xichen LI4, Xiaoming HU1
1Sun Yat-sen University, 2Ministry of Natural Resources, 3The Hong Kong University of Science and Technology, 4Chinese Academy of Sciences
Recent findings show a noteworthy linkage between the Arctic and Antarctic climates. Previous studies have emphasized the impact of the climate change in the northern high-latitudes on that in the southern high-latitudes, but few studies concerned the impact of Southern Ocean circulation on the Arctic climate, especially is seasonality. In this study, we close the Drake Passage (DP) to slow down the Antarctic Circumpolar Circulation (ACC) in the fully coupled Community Earth System Model, to investigate the impact of weakened ACC on the Arctic climate. Two model experiments, DP opened and DP closed experiments, are performed. Relative to the DP opened case, a warmer Antarctic but a colder Arctic appear in the DP closed case resulting from weaker ACC and Atlantic Meridional Overturning Circulation (AMOC). Especially, the changes in surface air temperature in the two poles are largest in winter. Compared to the DP opened case, the anomalous southward heat transport by weakened ACC is largest in winter, contributing to the winter amplification in the Antarctic. However, the seasonal difference in AMOC change is insignificant. To understand the winter amplification in the Arctic, we further analyze local surface heat flux changes in the Arctic. The anomalous downward longwave radiation and sensible and latent heat fluxes are stored in the ocean in summer and released to the atmosphere in the following winter. Although the ocean heat content warms the surface, the upward sensible and latent heat fluxes cool the surface more significantly in winter. This local atmosphere-ocean-ice interaction contributes to the winter amplification in the Arctic. These results shed light on understanding the pole-to-pole linkage.
AS24-A013
Refining the High-latitude Surface Temperature Bias of Climate Model : The Role of Autoconversion Rates in CAM6 Cloud Microphysics
Hyun-Joon SUNG1+, Eun-Hyuk BAEK2, Baek-Min KIM1#
1Pukyong National University, 2Chonnan National University
Despite substantial improvements in estimating the physical processes of global climate models (GCMs), accurately predicting clouds and climatic conditions in northern high-latitude regions remains challenging. This study investigated the impact of autoconversion rates, a critical aspect of cloud microphysics, on the simulation of summer clouds and climate in these high-latitude areas. Using the Community Atmospheric Model version 6 (CAM6), which is known to demonstrate a notable positive bias in cloud liquid and cold bias in northern high-latitude regions, we conducted three sensitivity experiments assessing the effects of varying autoconversion rates within the cloud microphysics scheme. Increasing the autoconversion rate considerably decreased cloud liquid contents and slightly decreased the low-cloud fraction. which contributed to enhanced shortwave radiation during summer and mitigated the cold bias observed in CAM6 over high-latitude regions. Our study underlines the importance of carefully selecting microphysical parameters to improve the accuracy of cloud and climate simulations in GCMs of the northern high latitudes, given the sensitivity of regional air temperatures to these parameters.
AS24-A015
| Invited
Reduced High-latitude Bias in the KIM (Korea Integrated Model): Insights Into Abnormal Arctic Warming Event in January 2016
Baek Min KIM1#+, Jung Hyun PARK1,2, Hyun-Joon SUNG1, Kwang-Hee HAN1, Jihan SIM1, Hyo-Jung LEE1, Hayeon NOH1, Juheon KIM1, Myung-Seo KOO3, Jun-Seong PARK3
1Pukyong National University, 2Korea Polar Research Institute, 3Korea Institute of Atmospheric Prediction Systems
In January 2016, the Arctic experienced a significant warming event, triggered by the arrival of warm, moist air from Storm Frank. This caused a remarkable melting of sea ice in the Barents-Kara Sea. This period of extended warming set new temperature records and influenced extreme cold events in East Asia three weeks later. In our study, we used the advanced KIM coupled model, which combines the atmospheric component of the KIM NWP model with the NEMO-SI3 ocean-sea ice model, to simulate this Arctic event alongside Storm Frank. Initially, the model started with a sea ice concentration similar to actual observations but overestimated the sea ice in the Barents-Kara Sea by more than 30% after five days. We improved the sea ice model's dynamic and thermodynamic processes and conducted extensive sensitivity experiments to reduce this discrepancy. Our research showed that the model was more affected by dynamic processes than thermodynamic ones. Adjusting the sea-ice strength parameters related to thickness and concentration in the ice rheology helped reduce the sea-ice bias by up to 20% in five days. In the early phase of the revised simulation, regions with less sea ice showed a significant rise in surface temperature. This was due to increased downward longwave radiation and turbulent heat flux, indicating a stronger ice-atmosphere interaction. Over longer forecasts, not only did surface temperatures change, but there were also shifts in upper-level atmospheric pressure patterns, leading to a blocking pattern over the Ural Mountains. Our findings highlight the importance of minimizing winter sea ice biases to improve model accuracy and demonstrate the significant impact of ocean-atmosphere interactions in the high latitudes on the performance of predictive models.
AS24-A010
Sub-seasonal Variability of West Antarctic Surface Air Temperature in Austral Summer
Xinlu CHEN+, Xiaoming HU#, Wei WEI, Jiping LIU
Sun Yat-sen University
Increasing surface air temperature (SAT) is an important contributing factor for surface melting events over the west Antarctic ice sheet (WAIS), which not only affects the total mass balance of the Antarctic ice sheet but also weakens the ice shelf stability. Ross ice shelf (RIS), the largest ice shelf over the WAIS, has experienced several massive surface melting events lasting for more than 10 days. To gain more insight into the Antarctic sub-seasonal SAT variability that may lead to such melting events, in this study, the processes associated with 10-30 day SAT variation across the WAIS in austral summer are investigated using the ERA5 reanalysis. SAT anomalies are induced by fluctuations of atmospheric circulation that feature a zonal wavenumber-3 pattern. 10-m landward wind anomalies, regulated by geopotential height anomalies located at the Marie Byrd Land and the Ross Sea, giving rise to synchronous coastal warming by transporting warm moist air. By contrast, inland warming lags behind due to foehn effects triggered by the local topographic barrier. Surface energy budget terms are also examined. Enhanced downward long-wave radiation, associated with increasing air temperature, more cloud and water vapour, plays an essential role in 10-30-day surface warming. In addition, surface melting events over the RIS occur more frequently during 10-30-day near-surface atmospheric warming, demonstrating that sub-seasonal SAT variability might be an important predictor of massive surface melting events.
Session Chair(s): Tetsuo NAKAZAWA, Japan Science and Technology Agency
AS05-A014
Numerical Solutions of a Simple Linear MJO Model on an Equatorial Beta-plane: Comparison with Analytical Solutions and Parameter Sensitivity
Spencer RESSEL1, Daehyun KIM2#+, Peter BLOSSEY1
1University of Washington, 2Seoul National University
Models of the Madden-Julian Oscillation (MJO) exist at varying levels of complexity. Simple linear models attempt to explain the MJO’s near-planetary scale and slow eastward propagation using linearized equations of motion with key physical processes represented by several parameters. These parameters, while often estimated from observational data, are generally taken as constants in the model. Despite this, previous research suggests that many parameters have both spatial-scale and latitude-longitude dependencies. Neglecting these dependencies simplifies the model but complicates the relationship between model-derived MJO-like modes and the observed MJO. This study expands upon the model presented in Ahmed (2021) to examine the sensitivity of the model solution – an MJO-like mode – to model parameters such as convective sensitivity to moisture and temperature anomalies and the coefficients that relate anomalous winds to horizontal moisture gradients. We solve both analytic and numerical representations of a modified Ahmed (2021) model to explore the parameter dependency. We find that simple modifications to the assumed symmetric meridional distribution of mean-state moisture allow the model to capture the asymmetric behavior of the observed MJO about the equator. Additionally, we find that the group velocity, phase speed, and growth rate of the MJO-like mode strongly depend on both the relative magnitudes of convective moisture and temperature sensitivity, as well as the degree to which Weak Temperature Gradient (WTG) balance is assumed.
AS05-A007
Two Types of the Moisture Mode Theories for MJO: Observational Validation
Tim LI1#+, Lu WANG2, Feng HU3
1University of Hawaiʻi at Mānoa, 2Nanjing University of Information Science & Technology, 3Chuzhou University
So far, there are two types of the moisture mode theories for understanding MJO propagation. One emphasizes the zonal asymmetry of boundary-layer perturbation moisture and the other emphasizes the east-west asymmetry of column-integrated moist static energy (MSE) tendency. The two theories were validated with the diagnosis of observational data for the period of 1979-2012, during which 84 eastward-propagating MJO events were identified. The effect of the vertically tilted structure (VTS) of MJO convection on its phase propagation was investigated. It was found that all the MJO events averaged throughout their life cycles exhibited a clear VTS, and the tilting strength was significantly correlated to the phase speed. A normalization method is applied to illustrate clearly the phase evolution of MJO. It is found that the MJO convective centers do not move smoothly, rather jump. Such a discontinuous phase evolution is related to the emerging and developing of new congestus convection to the east of the pre-existing deep convection. While the characteristic length scale of the phase jump depends on a Kelvin wave response, associated time scale represents the establishment of an unstable stratification in the front due to boundary layer moistening. Such a phase evolution characteristic seems supporting the moisture mode theory of the first type that emphasizes the boundary layer moisture asymmetry, because the moisture mode theory of the second type, which emphasizes the MSE tendency asymmetry, might favor more “smooth” phase propagation.
AS05-A009
MJO Diversity in CMIP6 Models
Seung-Yoon BACK+, Daehyun KIM, Seok-Woo SON#
Seoul National University
Recent studies have shown that individual Madden-Julian Oscillation (MJO) events can be categorized into four types based on their propagation characteristics: standing, jumping, slow-, and fast-propagating MJOs. While their structures and impacts in observations are well documented, their representation in state-of-the-art climate models has not been investigated. This study evaluates MJO diversity in 28 Coupled Model Intercomparison Project Phase 6 (CMIP6) models. The model performance for simulating MJO diversity shows a large inter-model spread. To identify the factors that drive MJO diversity in the models, the underlying slow-varying background conditions for each MJO type are investigated using a subset of models whose performance is in the upper quartile (i.e., GOOD models). We find that the horizontal gradient of the background SST and PW anomalies gradually change from the standing to jumping, slow-, and fast-propagating MJO in GOOD models as in observations. These gradual changes in the SST and PW gradient can allow more organized MJO propagation from the standing to fast-propagating MJO by enhancing the Kelvin wave response and the horizontal moisture advection to the east of the MJO convection. Unlike in observations, the impact of the Quasi-Biennial Oscillation (QBO) on MJO diversity is absent in GOOD models. The GOOD models also exhibit weaker cold SST and dry PW mean state biases over the equatorial western Pacific than the other models. These results suggest that MJO diversity in climate models could be improved by better simulating the mean background state and QBO-MJO coupling.
AS05-A017
Global Simulation of the Madden-Julian Oscillation with Stochastic Unified Convection Scheme
Jihoon SHIN1+, Jong-Jin BAIK2#
1Pukyong National University, 2Seoul National University
A new spectral convection scheme, the stochastic unified convection scheme (stochastic UNICON), is implemented in a general circulation model. The global climate simulation using stochastic UNICON is evaluated and compared with UNICON, focusing on the simulation of the Madden–Julian oscillation (MJO). Stochastic UNICON extends the original UNICON by randomly sampling convective updrafts from the joint probability density function constructed at the near-surface, generating a spectrum of convective updrafts in a physically based manner. The performances of UNICON and stochastic UNICON on simulating observed mean climates are comparable, while stochastic UNICON slightly reduces the mean bias of climate variables. For the simulation of intraseasonal variabilities, stochastic UNICON outperforms UNICON in many aspects. Stochastic UNICON improves the simulation of the intensity and propagation patterns of boreal winter MJO, which are too weakly simulated in UNICON. The coherency between MJO-related convection and large-scale circulation is also enhanced, which many climate models underestimate. The improvement of MJO simulation by stochastic UNICON is related to a better representation of the relationship between moisture and convection in the model. The increased frequency of shallow convection in stochastic UNICON leads to stronger moisture convergence that precedes convection activity peak and results in the more robust development of organized convection and more frequent intense precipitation. A precipitation budget analysis reveals that the moisture tendencies due to horizontal advection and convective process are consistently enhanced during MJO developing periods by stochastic UNICON.
AS05-A011
MJO Influence on Subseasonal-to-seasonal Prediction in the Northern Hemisphere Extratropics
Hera KIM1#+, Seok-Woo SON1, Hyemi KIM2, Kyong-Hwan SEO3, Min-Jee KANG1
1Seoul National University, 2Ewha Womans University, 3Pusan National University
The impacts of the Madden-Julian Oscillation (MJO) on the subseasonal-to-seasonal (S2S) prediction in the Northern Hemisphere extratropics are examined using the reforecasts from the S2S project and subseasonal experiment project (SubX). When forecasts are initialized during active MJO, overall extratropical prediction skill becomes significantly higher at 3- to 4-week windows compared to inactive MJO. Such prediction skill improvement is evident in 500-hPa geopotential height over the Pacific-North America and the North Atlantic, and surface temperature over North America, especially when the model is initialized during the MJO phases 6-7 and 8-1. However, the extratropical prediction skill is not modulated by the MJO phases 2-3 and 4-5. This phase dependency is likely set by the arrival time of MJO to the Maritime Continent (MC) barrier that substantially enhances the MJO amplitude error. This result suggests that only MJO phases whose convection lies east of the MC are a source of wintertime S2S predictability in the extratropics.
AS05-A004
Decreasing MJO Predictability by the Indo-Pacific Warm Pool Expansion
Hyemi KIM#+
Ewha Womans University
The Madden-Julian oscillation (MJO) is a dominant mode of tropical intraseasonal variability in which its convective anomalies drive anomalous circulation within the tropics and remotely in the extratropics, thus providing “forecast of opportunity” for global weather/climate events. During the decades, the characteristics of the MJO has changed following by the expansion of the Indo-Pacific warm pool, the largest pool of the warmest ocean temperature on Earth. If the characteristic of MJO has changed by the warm pool expansion, it is likely that its predictability has and will change in the future accordingly. In this study, we will explore the change in MJO predictability by the expansion of the Indo-Pacific warm pool using the CESM2 aqua-planet model experiments. In particular, the aqua-planet perfect-model ensemble forecast experiments show that, by warm pool expansion, the MJO predictability decreases by 5-days, which is mainly caused by disturbed MJO propagation due to the change in moisture distribution.
AS05-A015
Barrier Effect of the Indo-pacific Maritime Continent on Ensemble MJO Prediction
Abhik SANTRA1#, Chidong ZHANG2+, Harry HENDON3
1Monash University, 2NOAA Pacific Marine Environmental Laboratory, 3Bureau of Meteorology
The Madden–Julian oscillation (MJO) is often observed to weaken or sometimes completely decay as its convective anomaly moves from the Indian Ocean over to the Maritime Continent (MC), which is known as the MC barrier effect on the MJO. The MC barrier effect on the Austral summertime MJO is explored in retrospective forecasts from subseasonal-to-seasonal (S2S) prediction models. We select a set of observed MJO events that are blocked by the MC and another set of MJO events that propagate across the MC into the western Pacific. Our analysis indicates that the blocked events are often associated with persistent higher surface pressures over colder sea surface temperatures in the central Pacific, suggesting the large-scale environment plays a role in promoting or inhibiting the MJO propagation across the MC region. Predictive skills of the MJO events continuously propagating across the MC region are greater than those of the blocked MJO events, especially in the ocean-atmosphere coupled models, which is related to the systematic eastward propagating behavior of the MJO convection. We identify the best MJO prediction models and they consistently exhibit greater prediction skills of the continuously propagating MJOs. In contrast, the performance of the all-model ensemble mean is not better than the best models. Realistic eastward propagation in the ocean-atmosphere coupled models suggests air-sea interaction over the western Pacific is critical to improving MJO prediction.
AS05-A006
Maintenance of MJO Convection by Radiative Feedbacks
Wei-Ting HSIAO #, Eric MALONEY+
Colorado State University
The maintenance mechanisms for the Madden-Julian oscillation (MJO) remain an area of active research, and may include a combination of radiative feedbacks, wind-evaporation feedbacks, and moistening produced by lower tropospheric convective heating. This presentation will revisit the importance of radiative feedbacks for supporting MJO convection with a new GPCP precipitation dataset and NASA CERES radiative heating profiles. Prior work by Adames and Kim with the GPCP v1.3 precipitation product and NOAA OLR indicated that radiative feedbacks are strongly supportive of MJO convection as viewed through the vertically integrated moist static energy budget, and provide a strong scale selection mechanism. This presentation uses the newer GPCP v3.2 product to show that while radiative feedbacks still provide a strong scale selection mechanism, the overall strength of radiative feedbacks are weaker than with GPCP1.3. This suggests that the relative role of other feedbacks such as wind-evaporation feedbacks for supporting MJO convection may be more important than once thought. This presentation also uses NASA CERES radiation profiles in a vertically-resolved moisture budget framework that employs the tropical weak temperature gradient assumption to determine the impact of radiative feedbacks on the MJO moisture budget. It is shown that longwave cloud radiative feedbacks onto MJO moisture anomalies are enhanced in the Indian Ocean and southern Maritime Continent region compared to other parts of the tropics, suggesting stronger support for MJO convection there. This finding is consistent with prior work by Mayta and Adames suggesting that the MJO most closely resembles a moisture mode in that region. It is hypothesized that enhanced vertical shear in the Indian Ocean and southern Maritime Continent supports convective organization that fosters greater cloud-radiative feedbacks.
AS05-A001
A New GMS Plane For Madden-Julian Oscillation Analysis
Dong-Pha DANG+, Jia-Yuh YU#
National Central University
A new Gross Moist Stability (GMS) plane under the Convective Quasi-Equilibrium (CQE) assumption is introduced to explore tropical intraseasonal variability using reanalysis datasets over the tropical ocean. The GMS plane combines various parameters, including gross moist stratification, horizontal moisture advection associated with deep convection, gross dry stability, and diabatic sources. Based on the relative position to the critical GMS line, one can determine whether convection is undergoing amplification or decay. This approach offers a visual understanding of the Madden-Julian Oscillation (MJO) and its dynamics across the tropical ocean, effectively illustrating the recharge-discharge energy cycle associated with the MJO and convection intensity. The 2-D plane also highlights the geographical variability in the critical GMS, which acts as a threshold for convection efficiency. It is shown that strong MJO events tend to experience significantly reduced intensity after crossing the Maritime Continent (MC) domain, where the critical GMS is highest, underscoring the geographical and atmospheric circulation factors' influence on the MJO manifested in this 2-D plane. To investigate the MJO diversity, we define the power index derived from the area of the composited recharge-discharge energy cycle. It is shown that the largest power index over the Indian Ocean is associated with the fast MJO, while the lowest value is correlated with non-propagating Intraseasonal Oscillation.
Session Chair(s): Lin WANG, Chinese Academy of Sciences, Yu KOSAKA, The University of Tokyo
AS35-A024
| Invited
North Pacific Blocking in the Present and Future Climate
Seok-Woo SON1#+, Jaeyoung HWANG1, Patrick MARTINEAU 2, Barriopedro DAVID3
1Seoul National University, 2Japan Agency for Marine-Earth Science and Technology, 3Consejo Superior de Investigaciones Científicas-Universidad Complutense de Madrid (CSIC-UCM)
The North Pacific (NP) blocking has a significant influence on cold air outbreaks in East Asia. As it develops and extends westward, a pre-existing cold anomaly over northern Eurasia is pushed southeast. The anomalous meridional flow, associated with blocking-induced circulation anomalies over the North Pacific, further enhances the cold advection. The resulting cold anomaly is then maintained for a while, due to an offset between the temperature advection and the diabatic heating. The NP blocking is projected to decrease in a warming climate. However, even if atmospheric CO2 concentrations are reduced back to the present climate, NP blocking frequency is unlikely to recover. In the CO2 removal climate model experiment, NP blocking is projected to decrease through the middle of CO2 removal. The net result is less frequent NP blocking at the end of CO2 removal compared to the present climate. Such a non-monotonic change of NP blocking is partly explained by the barotropic energy conversion, especially by the eddy interactions with shear deformation. This result suggests that East Asian cold air outbreaks induced by NP blocking may significantly decrease in a warming climate as well as in a CO2 mitigation climate.
AS35-A004
Matching the Weak Temperature Gradient and the Quasi-geostrophic Solutions in a Shallow Water Model
Tsubasa KOHYAMA1#+, Hiroaki MIURA2
1Ochanomizu University, 2The University of Tokyo
The large-scale tropical atmosphere is governed by the weak temperature gradient (WTG) system, in which heating and horizontal divergence are in balance. By contrast, the large-scale midlatitude atmosphere is governed by the quasi-geostrophic (QG) system, in which the Coriolis force and the pressure gradient force are in balance. These atmospheric behaviors are determined by spatially-variant dimensionless numbers, depending on the dominant physical processes such as the rotational effects and typical wind speeds. These regions under the WTG and QG systems should be continuously matched at a certain boundary. Therefore, in this study, we aim to theoretically investigate this matching between the WTG and QG solutions at this tropics-midlatitude (TM) boundary. In particular, here we derive a steady-state analytical solution for a smoothly connected QG and WTG systems in a meridional one-dimensional shallow water model on a frictionless f-plane. In this solution, southerly winds accelerated by heating within the equatorial region are decelerated by radiative cooling in the subtropics. In the midlatitudes, because non-divergent geostrophic winds are dominant, this southerly wind cannot penetrate into the midlatitudes. Therefore, large-scale meridional winds cannot exist at the TM boundary, forming a downward branch of the Hadley circulation. Because the angular momentum originated from the equatorial region cannot be transported into the midlatitudes, a jet stream is generated on the TM boundary. The midlatitude atmospheric state is determined so that the QG solution smoothly matches with the tropical WTG solution, and at the same time, satisfies the boundary condition at the pole. To reproduce the meanderings of the jet stream, the WTG solution near the TM boundary must be further modified by latent heat release from the western boundary currents.
AS35-A002
Long-term Trends of the Atmospheric Circulation and Moist Static Energy Budget in the JRA-55 Reanalysis
Christian FRANZKE#+
Pusan National University
The atmospheric circulation response to global warming is an important problem that is theoretically still not well understood. This is a particular issue since climate model simulations provide uncertain, and at times contradictory, projections of future climate. In particular, it is still unclear how a warmer and moister atmosphere will affect midlatitude eddies and their associated poleward transport of heat and moisture. Here we perform a trend analysis of three main components of the global circulation}the zonal-mean state, eddies, and the net energy input into the atmosphere}and examine how they relate in terms of a moist static energy budget for the JRA-55 reanalysis data. A particular emphasis is made on understanding the contribution of moisture to circulation trends. The observed trends are very different between the hemispheres. In the Southern Hemisphere there is an overall strengthening and during boreal summer, also a poleward shifting, of the jet stream, the eddies, and the meridional diabatic heating gradients. Correspondingly, we find an overall strengthening of the meridional gradients of the net atmospheric energy input. In the Northern Hemisphere, the trend pat- terns are more complex, with the dominant signal being a clear boreal winter Arctic amplification of positive trends in lower-tropospheric temperature and moisture, as well as a significant weakening of both bandpass and low-pass eddy heat and moisture fluxes. Consistently, surface latent and sensible heat fluxes, upward and downward longwave radiation, and longwave cloud radiative fluxes at high latitudes show significant trends. However, radiative fluxes and eddy fluxes are inconsistent, suggesting data assimilation procedures need to be improved.
AS35-A042
Waveguide Teleconnections Along Polar Front Jet. Part 1: Characteristics, Dynamics and Prediction
Peiqiang XU#+, Lin WANG, Wen CHEN
Chinese Academy of Sciences
Waveguide teleconnections are quasi-stationary Rossby wave packets trapped by the atmospheric waveguide. Since their energy dispersion is seriously constrained by the atmospheric waveguide, they can generally propagate into far regions and even become circumglobal, distinguished from the canonical teleconnection pattern that are often oriented in great circle and has limited zonal scale. The amplified activities of waveguide teleconnections can induce violent meandering of the atmospheric jet stream in global and give rise to vigorous energy transfer between extratropics and tropics among the climate system such as atmosphere, ocean, and sea ice. Recently, interests in the waveguide teleconnections have been quickly expanded within climate community for their close connections to many concurrent high-impact extreme weather events in the middle latitudes. In this talk, I will introduce the characteristics, dynamics, and how the waveguide teleconnections can affect the extreme heat events over Eurasia from intraseasonal to interannual timescales. In addition, though they provide alluring predictive potentials for the heat waves on these timescales, I will introduce current challenges confronted by the community to fully use them in practice and possible ways ahead.
AS35-A010
Seasonal and Nonlinear Characteristics of the Kuroshio-Oyashio Extension SST Frontal System’s Impact on Atmospheric Circulation
Dong Wan KIM1#+, Young-Oh KWON1, Claude FRANKIGNOUL2, Clara DESER3, Gokhan DANABASOGLU3, Arnaud CZAJA4, Adam HERRINGTON3, Sunyong KIM1
1Woods Hole Oceanographic Institution, 2Sorbonne University, 3National Center for Atmospheric Research, 4Imperial College London
The role of sea surface temperature (SST) anomalies associated with Kuroshio-Oyashio Extension (KOE) frontal system in the cold season atmospheric circulation variability is investigated using Community Atmospheric Model version 6 (CAM6). In particular, the seasonality and asymmetric characteristics of the response forced by warm and cold SST anomalies are the focus of investigation. In the low resolution (~1deg) simulations, the surface latent heat flux and atmospheric column-mean latent heating response to the KOE SST anomalies show strong seasonal characteristics. The responses are strongest during mid-winter when background atmospheric temperature is coldest of the season, thereby allowing more heat to be transferred from the ocean to the atmosphere. Such an air-sea coupling weakens during early and late winter when background atmospheric temperature is relatively warmer than that of the mid-winter. In addition, the atmospheric response exhibits nonlinear characteristics to the SST forcing such that the latent heating anomalies associated with warm SST forcing are stronger than those associated with cold SST anomalies. Such asymmetric characteristics of the air-sea coupling further impact the downstream large-scale atmospheric circulation response to be asymmetric as well. It is known that the air-sea coupling over the SST frontal system is sensitive to the model’s resolution. Therefore, we also investigate how the seasonality and nonlinearity of the air-sea interaction over the KOE SST frontal system are represented in the variable-resolution CAM simulation in which the North Pacific horizontal resolution is set to be 1/8° while other domains over the globe maintain the 1° resolution. The overall results indicate that even with relatively constant SST anomaly forcing, the atmospheric response can largely vary due to the strong seasonal and nonlinear characteristics of the air-sea coupling.
AS35-A032
Zonal Extension of the Middle East Jet Stream and Its Role in Cross-seasonal Influence of Tropical-mid-latitude Interaction on the East Asian Winter Monsoon
Wei WEI#+, Ruyue GUO
Sun Yat-sen University
The Middle East jet stream (MEJS) is an important upstream upper-level circulation system for the Asian monsoon in winter. It plays a crucial role in connecting the tropics and the mid-higher latitudes and exert impacts on the downstream monsoon regions. Eastward extension of the MEJS indicates a wetter and colder winter in southern China and a later onset of the subsequent Asian summer monsoon. Cross-seasonal interaction between the convection over the western tropical Indian Ocean (WTIO) and the circulation over the North Atlantic, associated with the zonal extension of MEJS, is investigated from preceding autumn to winter by using diagnostic analysis and numerical experiments. Result shows that the intense WTIO convection, which is associated with the eastward extension of MEJS, can excite a cyclonic response over the North Atlantic in autumn (SON). This cyclonic anomaly may be caused by an upstream effect of the tropical heating, or it may be part of a circum-global wave train, which is excited by the WTIO heating and propagates from the Arabian Sea to southern China, then crosses the North Pacific and North America to the North Atlantic. The westerly anomalies in the southern flank of this cyclone intensify the storm track in the North Atlantic. The divergence of EP flux associated with the storm track leads to the development of the negative vorticity to the south and positive vorticity to the north, resulting in a cyclone-anticyclone dipole pattern in the North Atlantic. This NAO-like pattern is formed in early winter (NDJ) and persist into winter (DJF), which is favorable for the eastward extension of the MEJS. The southeastward-propagating wave train from the North Atlantic promotes the persistence of the anomalous anticyclone over the Arabian Sea and the anomalous cyclone over southern China, which sustains the influence of WTIO convection from autumn to winter.
AS35-A020
Atmospheric Meridional Teleconnection Patterns Over the North Pacific in Winter: Energetics and Changes Under Global Warming
Ryo SATOH#+, Yu KOSAKA
The University of Tokyo
The western Pacific (WP) pattern, North Pacific Oscillation (NPO), and the Pacific-North American (PNA) pattern are dominant teleconnection patterns over the wintertime North Pacific, which are characterized by a meridional dipole of height anomalies. Despite many studies, comprehensive understanding of why those patterns are dominant and which processes are important for their maintenance is still insufficient. By using JRA-55 reanalysis and d4PDF large ensemble AGCM simulations, our study systematically extracted 286 meridional teleconnection patterns anchored to various locations over the wintertime North Pacific from monthly mean fields and investigated the energetics for each of the patterns. Specifically, we evaluated energy conversion efficiency, whose reciprocal indicates the time scale for a particular energy conversion process to replenish the total energy associated with a teleconnection pattern. We found that total energy associated with individual patterns is highly correlated with the net efficiency of energy conversion from the climatological mean field and modulated transient eddy activity. This result suggests that net conversion efficiency is the key factor for the dominance of a pattern. In addition, we found baroclinic energy conversion from the climatological mean field is the most efficient process for the maintenance of almost all the patterns, arising from the vertically phase-tilted height anomalies embedded in the baroclinic climatological mean state. We further investigated changes of meridional teleconnection patterns over the wintertime North Pacific under global warming. Comparison between d4PDF historical and +4K experiments reveals that the total energy associated with meridional teleconnection patterns whose node lines are located at 35°N, including the PNA pattern, will increase in the warming climate, while those of patterns with node lines at 45°N, including the WP pattern and NPO, will decrease. We discuss these changes in the light of energetics.
AS35-A029
Comparison of Summertime Drought or Flood Events Over Yangtze River Valley Under Triple-dip La Niña Background During 2020-2022
Shaobo QIAO1#+, Bin WANG2, Shankai TANG3, Fei LIU1, Guolin FENG4, Wenjie DONG1
1Sun Yat-sen University, 2University of Hawaii, 3Lanzhou University, 4National Climate center
Under the triple-dip La Niña background, the Yangtze River Valley suffered from flood or drought events during the past three years of 2020-2022. The summer in 2020 was marked by the longest Meiyu season over the past 60 years, which started on 1 June and ended on 2 August with a duration of 62 days. In summer of 2021, the meiyu rainfall was near normal during June and July, but the Yangtze River Valley rainfall in August exceeded +250 mm. The midsummer in 2022 was marked by high-intensity and long-lasting heatwaves in the Yangtze River valley, with the number of heatwave days setting the highest historical record since 1961. Accordingly, the first question needed to be answered was: whether the La Niña played a role in these events? We found that the strengthening of La Niña in 2020 and 2022 resulted in an enhanced western Pacific subtropical high (WPSH), which is conducive to the super Meiyu in June-July of 2020 and the unprecedented Yangtze River Valley heatwaves in July-August of 2022. On the contrary, the decaying of La Niña has a weak influence on the enhanced WPSH and positive rainfall anomalies in August of 2021. On the other hand, we tended to seek other climate factors beside La Niña that contributed to the differences over the Yangtze River valley in the three years from a subseasonal perspective. We demonstrated that the mid-latitude teleconnection played a crucial role in the 2020 Meiyu onset and withdrawal. The positive rainfall anomalies in August 2021 was significantly promoted by the northward propagation of boreal summer intraseasonal oscillation (BSISO). As for the 2022 Yangtze River Valley heatwaves, the record-breaking Pakistan floods played a leading role.
AS35-A012
Rainfall Variability Near Japan Associated with Meridional Migrations of the Tropics-midlatitude Boundary and the Jet Stream
Mari MUTO1#+, Tsubasa KOHYAMA1, Hiroaki MIURA2
1Ochanomizu University, 2The University of Tokyo
In the tropical and midlatitude atmospheres, large-scale dynamics are governed by different dominant physical processes. The tropics is governed by the weak temperature gradient system where temperature gradient is constrained to be moderate, whereas the midlatitude area is governed by the quasi-geostrophic system where the Coriolis force and pressure gradient force are nearly balanced. Presumably, in order for these two different governing equations to be simultaneously valid in large scales, the boundary between these two regions must be connected by phenomena with small spatial scales. Therefore, in this study, we investigate the atmospheric behavior at the tropics-midlatitude (TM) boundary in the Northern Hemisphere. In particular, we focus on the jet stream and precipitation. The 5800 m height line at the 500 hPa level is defined as the TM boundary. This line serves as a proxy for the northern edge of the tropical region. Next, we focus on the strong wind axis of the westerly jet stream, which moves meridionally at mid-latitudes, because the jet stream can supply vortices with small spatial scales. By measuring the mean latitudinal distance between the jet stream and the boundary, it is shown that the jet stream flows near the TM boundary in most seasons. However, only in seasons when a sea surface temperature (SST) front exists near the TM boundary, the westerly jet stream is trapped above the SST front and temporarily leaves the TM boundary. In particular, focusing on the month of April, the extent to which the jet stream is shifted northward exhibits interannual variability, and when the jet stream takes a northern path, precipitation increases in Japan. Composite analysis shows that the jet stream takes a northern path when the sea surface heat flux, especially the latent heat flux, is anomalously released.
Session Chair(s): Shigeo YODEN, Kyoto University, Hye-Yeong CHUN, Yonsei University
AS29-A031
| Invited
Attempts to Study the Spatiotemporal Evolution of Sudden Stratospheric Warming Events Using Explainable Deep Learning Approaches
Yu-Chiao LIANG1#+, Yi Chang CHEN1, Yi-Jhen ZENG1, Chien-Ming WU1, Jin-De HUANG1, Simon LEE2, Yih WANG1
1National Taiwan University, 2Columbia University
Sudden stratospheric warmings (SSWs) are the most dramatic events in the wintertime stratosphere, and result in substantial disruption to the stratospheric polar vortex, which can be categorized into displacement and splitting types depending on the morphology of the disrupted vortex. Moreover, SSWs are important for subseasonal-to-seasonal weather prediction. Thus, monitoring the genesis and evolution of SSWs is crucial and deserves further advancement. Several statistical methods have been used to study the evolution of SSWs, but the ability of deep learning methods has not yet been explored, mainly due to the scarcity of observed events. To overcome the limited observational sample size, we use historical large-ensemble simulations of the Whole Atmosphere Community Climate Model version 6 to identify thousands of simulated SSWs, and use their spatial patterns to train deep learning models. We start by training neural networks (NNs) with varied complexity to identify SSWs based on the methodology of Charlton and Polvani (2007). Interpretability analysis reveals that NNs learn the geostrophic relationship between wind and geopotential height fields to distinguish SSWs. We next utilize a convolutional NN combined with a variational auto-encoder (VAE) to construct a phase diagram that characterizes the SSW evolution. This approach not only allows us to create a latent space that encapsulates the essential features of the vortex structure during SSWs, but offers new insights into its spatiotemporal evolution mapping onto the phase diagram. The constructed phase diagram depicts a continuous transition of the vortex pattern during SSWs. Notably, the VAE gives a better-reconstructed vortex morphology and more clearly organized vortex regimes for both displacement-type and split-type events than those obtained from principal component analysis. Our results provide an innovative means to characterize SSW evolution and uncover the potential for deep learning techniques to understand the underlying dynamics of extreme stratospheric vortex phenomena.
AS29-A019
Critical Role of the Upper Stratospheric Mean State in the 2021 Sudden Stratospheric Warming
Hyeong-Oh CHO+, Young-Ha KIM, Seok-Woo SON#
Seoul National University
This study investigates the effect of upper-stratospheric preconditioning on the onset of the 2021 Sudden Stratospheric Warming (SSW) by conducting a series of model experiments. The standard experiment fails to predict the 2021 SSW with 16-day lead time. The planetary-scale waves mainly propagate to midlatitudes in the upper stratosphere before the SSW onset, in contrast to the observations where the waves propagate and converge in the polar stratosphere, leading to a rapid weakening of the vortex. The wave convergence in the polar stratosphere results from the poleward migration of the easterly in the upper stratosphere which limits the wave propagation toward midlatitudes but focuses it on the polar region. By nudging the zonal-mean flow above 3 hPa toward the observations, the model successfully predicts the SSW, reproducing the observed feature of wave propagation. The result provides modeling evidence for the critical role of upper-stratospheric preconditioning in the 2021 SSW onset.
AS29-A022
Downward Coupling Mechanism of Sudden Stratospheric Warming: A Mass Flux Perspective
Dong-Chan HONG+, Seok-Woo SON#
Seoul National University
Sudden Stratospheric Warming (SSW) is an important source of subseasonal-to-seasonal predictability due to its significant and long-lasting impacts on surface climate. However, the mechanism of its downward coupling is not yet fully understood. In this study, we investigate the downward coupling mechanism of the SSW in terms of mass redistribution. From the 65-year-long Japanese 55-year Reanalysis (JRA-55), a total of 40 SSW events are identified. Their composite shows a significant increase of tropospheric geopotential and pressure anomalies over the Arctic (60-90°N) after the onset of the SSW, with a prominent surface amplification. The decomposition of tropospheric anomalies into surface pressure and air temperature components reveals that the downward coupling mainly results from surface pressure change. It is further found that the surface pressure change during the SSW is primarily caused by the poleward mass flux near the tropopause, which is mainly driven by the momentum flux change in the upper troposphere and lower stratosphere. This momentum flux change is consistent with the poleward propagation of the planetary-scale wave, which is associated with warm temperature anomaly in the lower stratosphere. This finding provides a new insight into the downward coupling and surface amplification of the SSW.
AS29-A029
Effects of Stratospheric Warming on Ural Blocking Events in Winter
Zhihao LI+, Guokun DAI#, Mu MU
Fudan University
Utilizing the Open Integrated Forecasting System, the responses of Ural blocking (UB) to different stratospheric warming scenarios are investigated. Numerical results show that stratospheric warming with moderate strength in minor patterns prolongs the UB duration and enhances its intensity, while strong stratospheric warming in minor patterns tends to shorten its duration and weaken its intensity, even leading to the collapse of the UB events. Further diagnosis reveals that the planetary wave activity flux propagates downward from the stratosphere to the troposphere after stratospheric warming. Moreover, the convergence of planetary wave activity flux is a key factor for UB enhancement and maintenance. In addition, the weakened meridional temperature gradients, decelerated zonal westerly winds, and a reduced meridional potential vorticity gradient (PVy) result in UB enhancement in response to stratospheric warming with moderate strength. As stratospheric warming strengthens, planetary wave activity flux diverges, westerly winds in the tropospheric mid-latitudes accelerate and the PVy in the Ural sector enlarges, which further weakens UB. Regarding the stratospheric perturbations in major patterns, they have similar influences on UB events, that is, UB enhances with moderate stratospheric warming and weakens with strong warming. However, the strengthened warming would trigger UB re-enhancement, which is closely associated with anomalous activities of tropospheric synoptic-scale waves induced by stratospheric perturbations. These results reveal UB events respond differently to stratospheric warming with various intensities and patterns in the short term, which makes a contribution to understanding stratosphere-troposphere coupling.
AS29-A002
| Invited
Impacts of Stratospheric Polar Vortex on the Wintertime Frontogenesis Over the Northern Hemisphere
Jiankai ZHANG#+
Lanzhou University
The impacts of the Arctic stratospheric polar vortex (SPV) changes on wintertime frontogenesis in the northern middle latitudes are analyzed. Both composite analysis and model simulations reveal that the intensity and frequency of frontogenesis over West Russia, the Mongolian Plateau, the Mediterranean and the southern North Atlantic during weak SPV years are significantly stronger and larger than those during strong SPV years, while the frontogenesis over the northern parts of the North Atlantic and North Pacific Oceans are weaker and less occur during weak SPV years. These features are more noticeable in middle January and February. The contributions of resultant deformation changes to frontogenesis intensity changes over most regions of the middle latitudes are larger than those of horizontal divergence changes, and the contribution of stretching deformation is slightly larger than that of shearing deformation. The changes in frontogenesis intensity are attributed to changes in the tropospheric circulation and temperature gradient associated with the SPV changes. Potential vorticity (PV) anomalies in the upper troposphere and lower stratosphere (UTLS) caused by the weakened and shifted SPV towards Eurasia lead to tropospheric cyclonic flows, favoring more cold-air mass transported towards mid-latitude Eurasia. Meanwhile, more high-PV air towards Eurasia results in steeper tropospheric isentropes during weak SPV years. Consequently, both temperature gradient and frontogenesis over Russia are enhanced. More southward transport of cold-air mass due to the equatorward shift of the polar jet stream induced by the weak SPV enhances the frontogenesis over the southern North Atlantic. Furthermore, the angle between dilatation axis and the isentropes over West Russia, the Mongolian Plateau and the southern North Atlantic is more likely to occur between 0◦ and 45◦, which promotes stronger frontogenesis over these regions during weak SPV years. By contrast, opposite processes occur over the northern North Atlantic, causing weaker frontogenesis there.
AS29-A003
Differences in Response of Stratosphere-troposphere Dynamics to Canonical El Niño and El Niño Modoki in Idealized Modeling
Daria SOBAEVA1,2#+, Yulia ZYULYAEVA3, Sergey GULEV3
1SHIRSHOV INSTITUTE OF OCEANOLOGY OF RUSSIAN ACADEMY OF SCIENCES, 2Moscow Institute of Physics and Technology (National Research University), 3Shirshov Institute of Oceanology
The intensity of the stratospheric polar vortex (SPV) is predicted less than 2 weeks ahead. However, low-frequency components of the climate system, such as large-scale sea surface temperature anomalies (SSTAs) e.g. El Niño–Southern Oscillation (ENSO) and Pacific Decadal Oscillation, extend the period of stratospheric dynamics’ prediction. Since the late 1970s non-canonical phase of El Niño (El Niño Modoki) is observed more frequently. The goal of this work is to analyze the peculiarities of stratosphere-troposphere interaction during the Canonical El Niño (CEN) events and El Niño Modoki (ENM) events in idealized model experiments on Isca platform. In these experiments SSTAs corresponding to ENSO modes were increased compared to the observed values. It is shown that SSTAs in region Nino-3 (CEN) lead to 36% weaker SPV in November–May compared to SPV in the control experiment. Weakening of the vortex with the positive SSTAs anomalies in the middle of equatorial Pacific (ENM) on the background is comparable with one in CEN experiment in amplitude, main differences are observed in late autumn and early spring. It is caused by more intense Rossby waves propagation from tropics to mid-latitudes. Differences also are found in the spatial structure of planetary wave 2 in CEN and ENM experiments. Negative SSTAs, which correspond to La Niña (LN) lead to weakening of the SPV only up to 20% compared to the control values. Analysis of the large-scale structure of the mid-troposphere pressure field show, that both Canonical El Niño and El Niño Modoki lead to amplification of Pacific-North-American mode. During La Niña spatial structure of the pressure anomalies correspond to Northern annular mode amplification. In ENM experiment the highest frequency of sudden stratospheric warmings is observed. Lower frequency is observed in LN experiment, which is twice more than in the control experiment.
AS29-A032
Evaluation of Intensity and Duration of the Arctic Stratospheric Polar Vortex of 44 Years (1979-2022) and Comparison with ICON Model Simulation
Anish KUMAR#+, Khalil KARAMI, Christoph JACOBI
Leipzig University
The stratospheric polar vortex is a seasonal low-pressure system characterized by a strong wind jet and potential vorticity gradient. This study examines the variations of the Arctic stratospheric polar vortex over the period 1979-2022 (44 years) on three isentropic levels (800, 600, 530 K) using ERA5 reanalysis data and a 30-year long time slice control simulation of ICON model. The study includes detailed analysis of vortex area, intensity, location and duration. The ERA5 polar vortex areas (cold season) at 850 K, 600 K, and 530 K are 54.99, 58.32, 52.83 million km2, respectively, and the model indicates 57.92, 45.87, 49.67 million km2, respectively. To ascertain the onset and breakup dates of the vortex, we assess the vortex area to increase 5 million km2, while also examining the wind speed along the vortex edges, which should be at least 28.48, 22.00, and 19.78 m s-1 at 850, 600, and 530 K, respectively. In ERA5, the vortex typically (averaged over 44 years and 3 isentropic levels) starts around November 19th and ends on April 12th, lasting approximately 149 days in ERA5, while in the model, it begins on November 8th, concludes on May 9th, lasting about 182 days. The climatological frequency of stratospheric sudden warming (SSW) in ERA5 is 0.66, slightly lower than the model's frequency of 0.70. Notably, ERA5 doesn't indicate any sudden stratospheric warming (SSW) events in April, whereas the model suggests a 0.10 frequency for April. Conversely, the model lacks SSW events in December, whereas ERA5 shows a 0.10 frequency for that month.
AS29-A005
A Revisit and Comparison of the Quasi-biennial Oscillation (QBO) Disruption Events in 2015/16 and 2019/20
Yue WANG1+, Jian RAO1#, Yixiong LU2, Zefan JU1, Junfeng YANG3, Jing-Jia LUO1
1Nanjing University of Information Science & Technology, 2China Meteorological Administration, 3Chinese Academy of Sciences
As the most dominant variability of the tropical stratospheric zonal winds on the interannual timescale, the quasi-biennial oscillation (QBO) has a significant impact on weather and climate on the hemispheric and even global scales. In contrast to the process of gradual downward propagation of the alternated easterly and westerly winds from the upper to the lower stratosphere, the downward propagation of westerly winds can be abruptly cut off by a rapid development of equatorial easterly winds in the lower stratosphere, which is known as the westerly QBO disruption event. Such an event has been observed twice since the discovery of the QBO in 1953. The QBO disruption has been widely studied in past years, which is hypothesized to be driven by strong extratropical Rossby waves and abrupt strengthening of equatorial waves under a strong westerly background in the tropical lower stratosphere. Various types of waves were active during the two events (2015/16 and 2019/20). During the 2015/16 QBO disruption, the sudden reversal of the QBO winds was attributed to the combination of the westerly QBO phase and a strong Brewer-Dobson circulation. During the 2020 QBO disruption, extratropical waves were enhanced especially in the Southern Hemisphere and propagated equatorward. In addition to the wind disruption, the usual evolution of the stratospheric temperature and trace gases was also disrupted and exhibited anomalously irregular behaviors. Climate models suggest that QBO disruption events might increase with global warming, which pose unprecedented challenges for the QBO prediction and understanding.
AS29-A006
Possible Impact of the QBO-MJO on the Early Summer Precipitation in Eastern China
Zefan JU1+, Jian RAO1#, Yue WANG1, Junfeng YANG2, Qian LU1
1Nanjing University of Information Science & Technology, 2Chinese Academy of Sciences
Using the reanalysis and multiple observations, the possible impact of the Madden–Julian Oscillation (MJO) on early summer (June–July) rainfall in eastern China and its modulation by the Quasi-Biennial Oscillation (QBO) are examined. The composite results show that the suppressed (enhanced) convection anomalies for MJO phases 8–1 (4–5) are more concentrated over the maritime continent and the western Pacific during easterly QBO (EQBO). As a consequence, more significant wet (dry) anomalies develop in South (eastern) China during MJO phases 8–1 (4–5) configured with easterly (westerly) QBO. The enhancement and expansion of the anomalous tropical convection band do not necessarily correspond to enhancement of the extratropical circulation response to MJO phases 8–1 (4–5) configured with westerly (easterly) QBO. The anomalous high (low) over the maritime continent and western Pacific associated with MJO phases 8–1 (4–5) is intensified (deepened) during easterly (westerly) QBO, leading to large southwesterly (northeasterly) anomalies in South China and the coasts, carrying abundant (sparse) moisture. Two anomalous meridional circulation cells are observed for MJO phases 8–1 in the East Asia sector, with downwelling anomalies around 5–20 N, upwelling anomalies around 20–30 N, and another downwelling branch northward of 30 N, which are enhanced during easterly QBO. The anomalous meridional circulation cells are reversed for MJO phases 4–5, which are stronger during westerly QBO with the anomalous downwelling and dry anomalies covering eastern China. The combined impact of MJO phases 8–1 and easterly QBO on the early summer rainfall is noticeable in 1996, 2016, and 2020. The enormous rainfall amount appeared along the Yangtze River in 1996, 2016, and 2020 due to the extended period of MJO phases 8–1 under the background of the easterly QBO.
AS29-A009
QBO Impact on Boreal Winter Surface Climate in the Northern Hemisphere Mid- and High-latitudes
Vinay KUMAR1, Matthew HITCHMAN2, Wenyuan DU2, S. K. DHAKA1, Shigeo YODEN3#+
1University of Delhi, 2University of Wisconsin-Madison, 3Kyoto University
A better understanding of the dynamical coupling between the stratosphere and troposphere could help to improve the prediction of seasonal climate anomalies for a given region of interest. The present study investigates dynamical coupling between the equatorial stratospheric quasi-biennial oscillation (QBO) and the boreal winter surface climate in the Northern Hemisphere mid- and high-latitude regions using 42 years of ERA-5 data from 1979 to 2020. For neutral El Niño Southern Oscillation (ENSO) periods, a QBO westerly (W) phase at 50 to 70hPa favors a higher value of mean sea level pressure in the polar region, with colder conditions and higher snow depth over Eurasia and North America, with the opposite effects during QBO easterly (E) phase. It is observed that planetary wave activity is enhanced in the extratropical upper troposphere and lower stratosphere (UTLS) during QBO W and it is diminished during QBO E. This QBO teleconnection pathway along the UTLS to the high-latitude surface is independent of the traditional “stratospheric pathway” or Holton-Tan (1980) mechanism. Diagnosis of this pathway will provide relevant mechanisms for valuable input to global circulation models of internal sub-seasonal to seasonal variations and can be implemented to improve long-range forecasting at these time scales over Eurasia and North America.
Session Chair(s): Rokjin J. PARK, Seoul National University
AS59-A048
| Invited
Using Geostationary Environment Monitoring Spectrometer (GEMS) Measurements to Investigate the Emission, Transport and Chemistry Processes That Determine Diurnal Variability of Pollutant Distributions Over Asia
David EDWARDS1#+, Duseong JO1, Sara MARTINEZ-ALONSO1, Ivan ORTEGA1, Louisa EMMONS1, Helen WORDEN1, Jhoon KIM2,3
1National Center for Atmospheric Research, 2Yonsei University, 3Korean Academy of Science and Technology (KAST)
Since its launch in 2020, the GEMS instrument has provided four years of geostationary Earth orbit (GEO) hourly, high spatial resolution, shortwave retrievals of atmospheric pollutants over Asia. This has allowed studies of the diurnal variation of trace gas and aerosol concentrations and the consequences for changing air quality and how this depends on emission, transport, and chemistry processes. In this paper, we concentrate on nitrogen dioxide (NO2) measurements and discuss how the relative importance of these processes changes according to different environments and seasons. Including low Earth orbit (LEO) infrared retrievals of carbon monoxide (CO) from MOPITT (morning overpass) and CrIS and TROPOMI (afternoon overpass) also allows helps differentiate combustion sources. We further compare with the NO2 diurnal variability observed by ground-based Pandora sun spectrometer measurements at polluted and less-polluted Asian sites. To help understand the daily differences in diurnal patterns at these regional and local scales, we use the Multi-Scale Infrastructure for Chemistry and Aerosols (MUSICAv0). This uses a global modeling framework with regional grid refinement to resolve chemistry at emission and exposure relevant scales. Finally, we report on the combined use of GEMS, Pandora and MUSICAv0 modeling to assess the expected NO2 distributions for locations of the 2023 ASIA-AQ aircraft field campaign.
AS59-A002
Estimation of NOx Emissions Over China Through Integration of GEOS-Chem Adjoint Model and GEMS NO2 Observations
Yi WANG#+, Lunche WANG, Minghui TAO
China University of Geosciences
Accurate and timely updated NOx emission inventory is significant for simulating and forecasting surface PM2.5 and O3 concentrations. Although NO2 observations from polar-orbit satellite have been widely used to estimate NOx emissions, this estimation is usually conducted at monthly scale due to low temporal resolution (once a day) of the NO2 observations. The new Geostationary Environment Monitoring Spectrometer (GEMS) sensor on board geostationary satellite can provide hourly NO2 observation at daytime, hence provide the potential to constrain NOx emissions at high temporal resolution. In this study, we assimilate GEMS NO2 observations through GEOS-Chem adjoint model to constrain NOx emissions over China at daily and monthly scales. The posterior NOx emissions are to simulate surface NO2 concentrations through GEOS-Chem model, which are further validated with in situ counterpart observations. Results show that no matter daily or monthly posterior NOx emission inventory is used, the simulation is better than that with prior NOx emission inventory used. Additionally, NO2 concentrations from the simulation using daily posterior NOx emission inventory are in better agreement in situ observations than using monthly posterior NOx emission inventory.
AS59-A068
Large Contribution of Soil Emissions to the Atmospheric Nitrogen Budget and Their Impacts on Air Quality and Climate Change in North China
Tong SHA#+
Shaanxi University of Science and Technology
Soil emissions of nitrogen compounds, including NO and HONO, play a significant role in atmospheric nitrogen budget, however HONO has been overlooked in previous research on soil reactive nitrogen (Nr) emissions and their impacts on air quality in China. This study estimates both soil NOx and HONO emissions (SNOx and SHONO) in North China with an updated soil Nr emissions scheme in the WRF-Chem model. The effects of soil Nr emissions on air quality, O3 pollution and climate change are also studied, with a focus on two key regions, Beijing-Tianjin-Hebei (BTH) and Fenwei Plain (FWP) known for high soil Nr and anthropogenic emissions. We find that SNOx is nearly double or triple those of SHONO, the monthly contributions of SNOx (SHONO) account for 37.3% (13.5%) of anthropogenic NOx emissions in the BTH region, and 29.2% (19.2%) in the FWP region during July 2018. Soil Nr emissions have a significant impact on the maximum daily 8-hour (MDA8) O3 and nitrate concentrations, exceeding SNOx or SHONO effects alone. On average, in the BTH region, soil Nr emissions increase MDA8 O3 by 16.9% and nitrate concentrations by 42.4%, and these impacts are 17.2% for MDA8 O3 and 42.7% for nitrate in the FWP region. Additionally, soil Nr emissions contribute to an additional O3 production, ranging from 0 to 24.9% in the BTH region and from 0 to13.8% in the FWP region under different reduction in anthropogenic NOx emissions. Reducing anthropogenic NOx emissions leads to a stronger suppressive effect of soil Nr emissions on O3 mitigation. We also stress that incorporating soil Nr emissions can result in a slower increase rate of air temperature compared to scenarios without soil Nr emissions. We thus highlight the previously underappreciated important role of various soil nitrogen emissions on O3 pollution.
AS59-A044
Evaluating the Performance of WRF-GC V2.0 in Simulating Summertime Surface Ozone Concentrations Over China
Jiajia MO+, Tzung-May FU#, Aoxing ZHANG
Southern University of Science and Technology
Surface ozone is a secondary pollutant that has exceeded allowable levels in many megacities across China. To better understand and forecast ozone concentrations, a series of numerical models are commonly used. The WRF-GC model v2.0 is an online two-way coupling of the Weather Research and Forecasting (WRF) meteorological model (v3.9.1.1) and the GEOS-Chem model (v12.8.0) and includes aerosol-radiation interaction (ARI) and aerosol-cloud interaction (ACI) based on bulk aerosol mass and composition. In this study, we used WRF-GC v2.0 to simulate surface ozone concentrations over China for the summer of 2019 at a horizontal resolution of 27 km and evaluated the model’s performance against surface observations. The model captured the diurnal variation and day-to-day variability of surface ozone in the five megacity clusters where ozone exceedances occurred most frequently, including the Beijing-Tianjin-Hebei (BTH), the Yangtze River Delta (YRD), the Sichuan Basin (SCB), the Fenwei Plains (FWP), and the Pearl River Delta (PRD), with correlation coefficients (R) and normalized mean biases (NMB) ranging from 0.73 to 0.89 and -21% to 48%, respectively. These indicators suggested that WRF-GC’s performance in simulating Chinese surface ozone was at par with other regional air quality models currently in use. WRF-GC showed the best performance in simulating daily maximum 8-hour average (MDA8) ozone over the YRD and PRD areas, with R and NMB ranging from 0.66 to 0.75 and 7% to 22%, respectively. However, the model tended to overestimate surface ozone concentration south of 35°N and underestimate surface ozone in the north, potentially indicating a deficiency in the model’s photochemical mechanism. Further research is needed to understand the factors influencing model performance fully and to continue improving the accuracy of the simulations. This study established a performance benchmark and proved the usability of WRF-GC v2.0 in simulating surface ozone concentrations in China.
AS59-A063
Investigation of Climate Change in Relation to Land Use and Land Cover Changes and Consequent Alteration of Atmospheric Composition Over North-east India
Binita PATHAK1#, Ankita MEDHI2+, Aniket CHAKRABORTY1
1Dibrugarh University, 2University of Delhi
The evidence of changing climate has already been observed across the globe through its spatio-temporal variations. Land Use Land Cover (LULC) change has become one of the most prominent causes for influencing our regional climate. The fragile ecosystem and multiple driving forces in North-Eastern India (NEI) like poor socio-economic conditions, subsistence farming, complex, risk-prone and low productive rainfed agriculture, increasing population pressure and age-old cultural practices of cultivation resulted in rapid LULC change compared to the rest of India. This study aims to investigate the LULC trends and changes over NEI utilizing the LULC generated from LISS III, MODIS and Sentinel 2A satellite sensor imageries for different periods since 1990 to present. In spite of high vegetation and less industrialization, previous studies identify Northeast India as a hotspot for aerosol loading, and trace gases like. The current study aims to link the changes of atmospheric pollutants (CO, O3, CH4, NOx, PM etc.) to the LULC changes using satellite, reanalysis and model simulated data. An increase of 0.098% wetland and 0.033% in total waterbody coverage LULC changes during 1990-2021 is found to alter CH4 emission patterns and magnitudes over the region. Further, the PM emissions are also increasing due to the built up activities in major city like Guwahati. The LULC induced emissions are altering the atmospheric composition over the region and hence contributing to the recent climate change and variability.
AS59-A001
Long-term Measurements of Particle Number Size Distributions in China and Its Applications in Chemical Weather Numerical Model
Xiaojing SHEN#+
Chinese Academy of Meteorological Sciences
Continuous long-term measurements of PNSDs ranging from 3 nm to 10 μm have been conducted at a regional background site, Shangdianzi (SDZ) in the North China Plain (NCP) since 2008, Lin'an Atmosphere Background National Observation and Research Station (LAN) in the Yangtze River Delta (YRD) region since 2013, and urban site in Beijing since 2016. The key findings included: (1) based on the PNSD measurement, new particle formation (NPF) events were identified with the annual frequency of 20-40% in different regions and it showed higher formation rate and growth rate in China; (2) Regional NPF events were observed to occur with the horizontal extent larger than 500 km in NCP region, whereas they were mostly observed around the site within 100–200 km in YRD region; (3) based on the PNSD measurement at LAN from 2013 to 2019, a significant decreasing trend in the Aitken and accumulation mode number concentrations was observed due to the emission control strategies. The PNSDs measurement data were applied to develop a parameterization scheme for aerosol size distribution in initial emission in the GRAPES–CUACE model, which improved the PM2.5 mass concentration simulation result considerably, especially during heavy haze-fog episodes. The PNSD data have also been used in WRF-Chem model to evaluate the contribution of NPF events to the cloud condensation nuclei concentration.
Session Chair(s): Massimo VIENO, UK Centre for Ecology & Hydrology, Yali LUO, Nanjing University of Information Science & Technology, Masaki SATOH, The University of Tokyo
AS36-A006
What Drives the Change of Capacity Factor of Wind Turbine in the United States?
Jiayu XU1#+, Junyu ZOU1, Alan ZIEGLER2, Zhenzhong ZENG1, Jie WU3
1Southern University of Science and Technology, 2Kasetsart University, 3University of Copenhagen
The capacity factor (CF) is a vital parameter used to quantify the performance and efficiency of a wind turbine. An increase in generation efficiency leads to higher wind power production, improving the economics within the growing global wind market. In this research, we use a data-driven statistical method to explore the contributions of the three main drivers of CF change: turbine aging, changes in wind speed, and technological improvements. We find that for the group of old turbines (operated before 2008) with an unchanging technical condition, wind increases contributed ∼10% to the increasing CF on average from 2010 to 2020. For new turbines (built from 2008 to 2020), technological improvements had a strong positive effect on CF from 2015 to 2020, exceeding the effect of wind increases and offsetting the effects of aging. On average, rising wind speeds increased CF by ∼5% per year, while technological improvements increased it by ∼12%. As the installed capacity of wind turbines grew, technological progress became the dominant driver in CF increase. However, poor site selection potentially compromised the positive effect on CF afforded by technology changes early in the decade.
AS36-A009
Global Heat Comfort Conditions Over the Ocean Since 20th Century: Historical Changes and Anthropogenic Contribution
Longshi LIAO#+, Qingxiang LI
Sun Yat-sen University
The changing heat comfort conditions under global warming can have a significant impact on human health and society. Current studies on heat comfort have mainly focused on changes on land, while those over the ocean which pose a potential threat to ocean-based economies and the living conditions of people dependent on the sea remain unclear. This study aims to address this gap by examining historical changes in global human heat comfort conditions over the ocean and separate the contribution of various radiative forcing factors. This study first demonstrates the historical changes of global human heat comfort conditions over the ocean during 1901-2021, based on the heat stress indicator the apparent temperature (APT), commonly defined as a function of the surface air temperature (SAT), relative humidity and near-surface wind speed. As a result, the warming of APT has been 0.011℃/decade faster than SAT. Additionally, we employed the Partial Least Squares Regression method to reasonably separate the specific contributions of each anthropogenic forcing factor on global marine SAT and APT during 1901-2019, with model explained variances up to 92.7% and 88.2%, respectively. Further, the results indicates that the global well-mixed radiative forcing of CO2, the other greenhouse gases (OGHG), stratospheric water vapor (H2O_stra) and the land use have significant positive contributions to global marine SAT and APT warming, while ozone and aerosol acts cooling effects on both. Specifically, global marine SAT and APT warmed about 0.93℃ (1.05℃) from 2000-2019 relative to 1901-1920, respectively, with CO2, land use, H2O_stra and OGHG contributing about 0.82, 0.37, 0.28 and 0.08℃ (0.72, 0.58, 0.46 and 0.20℃) of warming, respectively, while ozone and aerosol cooled the SAT (APT) by about 0.37 and 0.06℃ (0.37 and 0.23℃), with remaining external forcing providing -0.19℃ (-0.31℃).
AS36-A015
Rainfall Estimation Using Interpolation and Linear Regression Method (Case Study Betung District, South Sumatra)
Ratih PRASETYA1#+, Adhi HARMOKO1, Nelly Florida RIAMA2
1University of Indonesia, 2Indonesian Agency for Meteorology, Climatology and Geophysics
This study investigates the importance of predicting rainfall in weather forecasting, focusing on variables like rainfall quantity and rainy-day frequency. Utilizing data processing methods of interpolation and regression techniques, the research fills gaps in observational data and to estimate rainfall. Newton and Lagrange interpolations yield similar results. These methods able to predict rainfall and fill in missing rainy days. Linear regression is also employed to reveal relationships and patterns in monthly rainfall data. Descriptive statistics, including skewness, kurtosis, and boxplots, provide insights into rainfall distribution. The findings indicate an upward trend in rainfall, and projections for January 2023 predict 15 wet days and 318.7 mm of rainfall using regression and interpolation. The methodology involves data from rain gauges, temperature, and humidity that closely related with rainfall. This study enhances understanding of rainfall patterns, variability, and predictions, benefiting meteorological applications in the region.
AS36-A001
Millennial-scale Variability of Greenland Dust Provenance During the Last Glacial Maximum Identified Through Single-particle Analytical Approach
Seokhyun RO1+, Jonghyeon PARK2, Hanjin YOO1, Changhee HAN3, Ahhyung LEE1, Gaheun MUN1, Yeongcheol HAN4, Chul-Un RO1, Sungmin HONG1#
1Inha University, 2Ara Consulting and Technology, 3Korea Water Resources Corporation, 4Korea Polar Research Institute
Dust cycle is an important component of the Earth’s climate system, influencing radiative forcing and balance through a variety of feedback processes. In this context, an extensive understanding of past changes in the atmospheric burden of dust is necessary to improve the model projections of future climate change. Greenland ice core dust records revealed pronounced glacial/interglacial variations in dust concentrations with a 100-fold increase during the Last Glacial Maximum (LGM) compared to the Holocene. However, a discrepancy between the observed and modeled dust fluxes in Greenland during the LGM still exists, possibly due to the changes in potential dust contributors to Greenland. Here, we present the morphological, mineralogical, and geochemical characteristics of insoluble microparticles to constrain the provenance of dust in 11 core sections from the North Greenland Eemian Ice Drilling (NEEM) ice core with ages ranging from ~14.7 to 27.1 ka B.P. This time interval covers cold Greenland Stadials (GS)–2.1a to GS–3 in the LGM. The analyses were performed on insoluble particles in microdroplet samples by scanning electron microscopy with energy dispersive X-ray spectroscopy and Raman microspectroscopy. We found substantially higher kaolinite-to-chlorite (K/C) ratios and chemical index of alteration (CIA) values during GS–2.1 than during GS–3. In addition, carbon contents in particles were distinctly different between GS–2.1 and GS–3. These results propose that the importance source of dust was the Sahara during GS–2.1 and the Gobi Desert and/or European loess during GS–3, highlighting millennial-scale changes in Greenland dust provenance during the LGM. This shift is probably linked to large-scale atmospheric circulation variability in the mid- to high-latitudes of the Northern Hemisphere, which may have been associated with the evolution of continental-scale ice sheets (the Laurentide and Eurasian Ice Sheets) throughout the LGM.
AS36-A022
Ammonium Availability Index of Precipitation at South Asian Sites Under UKRI-GCRF South Asian Nitrogen Hub
U.C. KULSHRESTHA1#+, Chiara DI MARCO2, Eiko NEMITZ2, Sarat NISSANKA3, Zameela AHMED4, Ramesh RAMACHANDRAN 5, Subodh SHARMA 6, Md. Mizanur RAHMAN7, Dendup TSHERING 8, Mark A. SUTTON2
1Jawaharlal Nehru University, 2UK Centre for Ecology & Hydrology, 3University of Paradeniya, 4Maldives National University, 5National Centre for Sustainable Coastal Management, 6Kathmandu University, 7Bangabandhu Sheikh Mujibur Rahman Agricultural University, 8Royal University of Bhutan
Gases such as NH3, NOx and SO2 are emitted from different natural and anthropogenic sources. Partly these gases are deposited or transformed into their corresponding compounds near the sources while a significant fraction is transported to very long distances. NOx and SO2 result in acid formation respectively as HNO3 and H2SO4 which react with available NH3 which is an alkaline gas through a neutralization reaction further forming NH4NO3 and (NH4)2SO4 particles as their salts. These are either removed through dry deposition or through wet deposition process. During wet scavenging, these affect acidity of clouds and precipitation. Thereby, the acidity of precipitation is an indicator of their balance if no other strong anion or cation is present in the rain water. Ammonium Availability Index (AAI) which is a molar ratio expressed as [NH4+]/ 2[nssSO42-] + [NO3-] was calculated in this study for precipitation chemistry network sites viz. DTG, Peradeniya (Sri Lanka), MAP (Maldives), KU, Dhulikhel (Nepal), BSMRAU, Dhaka (Bangladesh) and BRRI, Rangpur (Bangladesh), SC, Kanglung (Bhutan) and NCSCM, Chennai (India). Rain water sample collection was carried out during 2022-23 using a quality protocol at all the sites. The AAI values at BSMRAU and NCSCM sites indicated an insufficient availability of NH4+ to fully neutralize acidity contributed by SO42- and NO3-. At remaining sites, AAI values suggested a complete neutralisation of acidity contributed by nssSO42- and NO3-. The results of this study are highly important for understanding the hot spots of NH3 dominance and local vs long distance sources of NO3- and nssSO42- in south Asia.
AS36-A023
Comparison of Model and Observed Wet Deposition in South Asia
Massimo VIENO1#+, U.C. KULSHRESTHA2, Chiara DI MARCO1, Yuanlin WANG1, Mark A. SUTTON1, Sam TOMLINSON1, Edward CARNELL1, Clare PEARSON1, Eiko NEMITZ1
1UK Centre for Ecology & Hydrology, 2Jawaharlal Nehru University
South Asia atmospheric composition is driven by several processes, such as emissions of primary pollutants, secondary formation, chemical transformations, transport and removal processes. Dry and wet deposition are major processes occurring in the atmosphere affecting air quality and participate to the deposition of reactive nitrogen to ecosystems. An atmospheric chemistry transport model (EMEP MSC-W) is used here to integrate all these processes in South Asia and focus on the wet removal. This work compares the daily observed wet deposition fluxes of oxidized sulphur (SOx), oxidised nitrogen (OXN) and reduced nitrogen (RDN) for a period between January and August 2018 at 5 sites near Delhi. The observed daily wet depositions are intended to capture the rainfall episodes, which are then compared with daily calculated wet deposition. The model better represents the SOx wet deposition, whereas the OXN and RDN is generally overestimated by the model when compared with the observations. Several factors might influence how well the model performs. The emissions inventories used here are derived from the Emission Database for Global Atmospheric Research, with specific emissions for South Asia developed within the South Asia Nitrogen Hub project. Meteorology also plays a key role as precipitation is the main driver of wet removal, however the collected precipitation was relatively well reproduced by the model and did not explain the cause of the discrepancy between model and observed OXN and RDN wet deposition. OXN and RDN have an intrinsic complexity due to chemistry interactions, the emissions sources linked with human and animal activity, and the thermodynamic equilibrium (for example ammonium nitrate). In contrast, SOX is easier to capture due to the relatively simpler chemistry and more stable ammonium sulphate. South Asia also has a large component of mineral dust which react with nitric acid to form coarse nitrate (diameters size >2.5 um).
AS36-A024
An Assessment of Multi-model Simulations of Global Dust Cycles with Remote Sensing Observations
Hongbin YU1#+, Jianyu ZHENG2,1, Mian CHIN1, Michael SCHULZ3, Chamara RAJAPAKSHE1, Huisheng BIAN2, Qian TAN4, Zhibo ZHANG2
1NASA Goddard Space Flight Center, 2University of Maryland, Baltimore County, 3 Norwegian Meteorological Institute, 4Bay Area Environmental Research Institute
Desert dust, one of the most abundant aerosols in the atmosphere, is recognized as an integral component of the Earth system that influences weather and climate via a suite of complex interactions with the energy, water, and carbon cycles. Dust storms also cause detrimental losses of human life and economic activities through degrading air quality, spreading diseases, disrupting transportation, and reducing efficiency of solar power generation. There has been growing attention in the past decades to advancing the research of dust cycle – a chain of processes involving emission, transport, transformation, and removal, and its tight coupling with other components of the system and human dimension. This study uses a suite of remote sensing (AERONET, MODIS, CALIOP, MISR, IASI) and in situ measurements of dust to evaluate 18 major chemical transport models from 15 international institutions participating in the AeroCom Phase III experiment. Major results from this multi-satellite and multi-model analysis include: (1) despite significant progresses over the past decades, the models are still highly diverse in simulating the dust cycle; (2) the simulated dust optical depth (DOD) shows the best agreement with each other and with observations; however, constraining global DOD is far from adequate for assessing the role of dust in the Earth system; (3) the models differ substantially in characterizing dust size distributions, which drives large spread in dust emissions and deposition; and (4) improvements on dust removal parameterizations are needed for both wet and dry processes.
AS36-A025
Wet Deposition of Inorganic and Organic Fractions of Nitrogen Over Different Land-use Sites of Indo-Gangetic Plain
Manisha MISHRA1,2+, Saurabh DHAKAD3, U.C. KULSHRESTHA3#
1Azim Premji University, 2National Yang Ming Chiao Tung University, 3Jawaharlal Nehru University
Indo-Gangetic plain (IGP) is considered as one of the major hotspots of atmospheric nitrogen deposition due to very high population density and emission sources. These depositions of atmospheric reactive nitrogen (Nr) have adverse impacts on the sensitive terrestrial and aquatic ecosystems, crossing their critical loads. Considering limited information on the wet deposition of both inorganic as well as organic forms of Nitrogen (N), molar concentrations of inorganic (NH4+ and NO3-) and organic N in rainwater were monitored at three different land-use sites in Indo-Gangetic Plain (IGP) during the monsoon period (June-September). It has been observed that dissolved organic N (DON) contributed significantly to the total dissolved N (TDN) ranging from 5% to 60% depending on the rain intensity. Dissolved inorganic N (DIN = NH4+ + NO3-) concentration was recorded as high as 221.0 µmol L-1 at urban site to as low as 65.9 µmol L-1 at the rural site. Furthermore, NH4+ contribution to TDN had the order: rural (75%) > urban (70%) > urban megacity (75%) whereas NO3- had contrasting trend (25%, 15% and 8%, respectively). Overall, wet deposition fluxes of atmospheric TDN was observed to be higher at urban sites. This can be attributed to a variety of local N sources such as vehicular emission, microbial emissions, biomass burning, human excreta due to higher population density, and transportation from surrounding areas, as observed from concentration weighted trajectories (CWT) model and cluster analysis. Upwind region of IGP has experienced major influence of air mass transported from agriculturally rich northwest part of India. However, both the downwind sites have experienced by-and-large the influence of south-westerly air-masses originated over the Arabian Sea. This study has found that the DON contributes significantly to TDN and, therefore, its inclusion for nitrogen budget assessment in South Asia is emphasized.
AS36-A026
Wet Deposition of Major Ions in Rainwater at Two Selected Sites in Panipat District, India
Saurabh DHAKAD#+, Ananya SINGH, U.C. KULSHRESTHA
Jawaharlal Nehru University
Fossil fuel combustion is the major source of air pollution which contributes different air pollutants which are removed from the atmosphere via wet and dry deposition processes. The dissolved gases and particulate matter in the atmosphere influence the rainwater chemistry. In the present study, major cations (Na + , NH 4 + , K + , Ca 2+ , Mg 2+ ) and anions (F - , Cl - , NO 3 - , PO 4 3- , SO 4 2- ) in rainwater along with pH and electrical conductivity (EC) were determined. The rainwater samples were collected from two sites having different characteristics in Panipat district of Haryana in North India during Monsoon 2023. The first site, EE has semi-urban characteristics while the second site HVPNL has urban characteristics. Total 21 rain events were collected at the EE site while 14 events were collected at the HVPNL site. The samples were collected by using manual wet collector consisting of a plastic bottle and funnel. In order to protect from any biodegradation, thymol was added to the collected samples. The samples were analysed for major ions by using an ion chromatography (Metrohm, model 881). The average pH of rain water at the EE site was 5.99 and the average pH at HVPNL was 5.90. The average EC value was 35.2 μS/cm at the EE site while the average EC value was 39.2 μS/cm at the HVPNL site. Further, the detailed results will be discussed during the conference.
Session Chair(s): Jian XU, National Space Science Center, Chinese Academy of Sciences, Bingqiang SUN, Fudan University
AS70-A008
Physics-driven Machine Learning Algorithm Facilitates Multilayer Cloud Property Retrievals from Geostationary Passive Imager Measurements
Feng ZHANG1#+, Wenwen LI1, Fuhao YANG2, Bin GUO1, Husi LETU3
1Fudan University, 2Zhejiang Normal University, 3Chinese Academy of Sciences
A physics-driven machine learning (ML) algorithm that integrates radiative transfer model (RTM) simulation and ML techniques has been developed to facilitate multilayer cloud property retrievals from advanced Himawari imager (AHI) measurements based on the geostationary satellite Himawari-8. Theoretical sensitive study revealed that integrating RTM-simulated clear-sky radiances into the retrieval model holds substantial potential to enhance multilayer cloud property retrieval. Thus, a convolutional neural network (CNN) model called CNN_TL was designed for simultaneous retrieval of ice and water properties in multilayer clouds, based on the combined use of visible/near-infrared (VNIR) and thermal infrared (TIR) measurements and RTM-simulated clear-sky radiances as predictors. The CNN_TL model was initially trained using the simulated datasets generated by RTM to gain better model initiation and generalization and further tuned using the standard references from collocated active sensor products through the transfer learning (TL) method. Validation on independent dataset shows CNN_TL-retrieved cloud top heights agreeing well with active sensor products for both overlaying ice and underlying water (RMSEs: 1.219 and 0.863 km), substantially outperforming AHI official products. Additionally, due to separate retrieval of ice and water microphysical properties in multilayer clouds, CNN_TL retrieved overlying ice microphysical properties exhibited a substantial correlation with active sensor products, showing Pearson coefficients above 0.78. Notably, CNN_TL model outperformed the purely ML-based model, demonstrating the advantage of integrating physical RTM simulation and ML techniques through TL method.
AS70-A003
Development of Diffraction Decomposition Order Method for Solving Radiative Transfer Equation
Bingqiang SUN#+, Chenxu GAO, Yijun ZHANG
Fudan University
In radiative transfer process, the distribution of single-scattering energy spans large order of magnitude differences so that the computation of radiative transfer equation is time-consuming. Conventionally, δ-function is used to replace the forward peak of a scattering phase function, such as δ-M and δ-Fit methods. Although computational efficiency is significantly improved in the δ-function truncation methods, computational accuracy is reduced, especially for the transmission in the meridional plane. The diffraction decomposition order (DDO) method is proposed in this study to quickly and accurately solve the radiative transfer equation. Although scattering energy is concentrated on forward direction, the diffraction energy is only limited to small scattering angles. Based on this recognition, the original radiative transfer equation is decomposed into a series of order equations, where the zero-order equation uses δ-function to replace the diffraction peak and the source functions of high order equations are from the differences between the diffraction peak and δ-function. The DDO method keeps not only the computational efficiency of conventional δ-function truncation methods, but also the computational accuracy of the original equation due to the iterative order consideration. The DDO is realized in terms of the successive order of scattering method in this study. In summary, the DDO method can not only be treated as an efficient truncation algorithm, but also be used as an effective radiative transfer method.
AS70-A002
Hyperspectral Remote Sensing of Aerosols from Space
Jian XU1#+, Lanlan RAO2, Zhuo ZHANG2, Gegen TANA2, Chong SHI3, Husi LETU2, Jinghua MAO2, Entao SHI2, Yongmei WANG2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Aerospace Information Research Institute, Chinese Academy of Sciences
Accurate knowledge of aerosols in the lower atmosphere, including their optical properties and vertical distribution, is particularly important for studying the Earth's climatic and weather conditions. The new-generation hyperspectral satellite sensors, such as the Ozone Monitoring Suite (OMS) on board the FengYun-3F (FY-3F) satellite and the Tropospheric Monitoring Instrument (TROPOMI) on board the ESA's Sentinel-5 Precursor (S5P), can provide global observations of atmospheric components. The significant challenge in processing hyperspectral satellite measurements is to enhance the performance of aerosol retrieval algorithms to achieve satisfactory accuracy and efficiency. In principle, the O2-O2 (∼477 nm) and O2 A-bands (∼760 nm) are sensitive to deriving aerosol layer height information, while the near ultraviolet and visible bands are usually used to retrieve aerosol parameters such as ultraviolet index and optical depth. The primary goal of this study is to present the most recent findings on the retrieval of aerosol parameters from the latest satellite hyperspectral measurements.
AS70-A001
Ice Water Path Retrieval from Microwave Humidity Sounder-II Aboard FengYun-3D Satellite
Wenyu WANG1#+, Jian XU1, Husi LETU2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences
The derivation of ice water path (IWP) from microwave radiometer measurements is challenging, which is not easily solved by conventional physics-based methods and the deep learning method is an alternative, efficient, and easy-touse approach that has already been widely used in the area of meteorological element retrieval. There are pros and cons in both methods. Physics-based algorithms have clearer physical mechanisms and processes to analyze the sources of retrieval error, and have been well used in atmospheric temperature, humidity, and atmospheric composition products, but there is a problem of high computational complexity and low accuracy in complex physical processes such as ice clouds. On the contrary, deep learning has the advantage of being computationally fast and relatively more accurate in complex physics problems, but it has the disadvantage of relying heavily on real data and the inability to trace physical processes back to their source, so it is not suitable for all problems. In the face of these difficulties and challenges, This study presents a deep learning framework for global retrieval of IWP using observations from the Microwave Humidity Sounder-II (MWHS-II) aboard the FengYun-3D (FY-3D) satellites. Two deep learning models, Deep Forest (DF21) and Quantile Regression Neural Network (QRNN) are constructed to detect ice cloud flags and retrieve IWP.
AS70-A013
All-day Cloud Water Path Retrieval Study Based on New Generation Geostationary Satellite Infrared Multi-channel Data
Gegen TANA1#+, Jian XU2, Chong SHI3, Lesi WEI1, Jiancheng SHI1
1Chinese Academy of Sciences, 2National Space Science Center, Chinese Academy of Sciences, 3Aerospace Information Research Institute, Chinese Academy of Sciences
The accurate estimation of cloud water path throughout the day is of great significance for the assessment of atmospheric water resources, key parameters of global energy balance and water cycle as well as the study of cloud-radiation-climate effect. However, the current remote sensing algorithms of cloud water mainly take the visible band measurements as input and lack the global scale all day high-precision remote sensing products. Though the cloud water products from passive microwave sensors have advantage of being applied in all-weather situation, the spatial resolution is low. The active microwave sensors have low temporal resolution and spatial coverage, still cannot provide cloud water products with high temporal and spatial resolution. The new generation of geostationary satellites have the characteristics of high spatial-temporal and spectral resolution, which provides important data support for accurately describing the all-day characteristics of clouds. This study plans to use multiple infrared channels from several new generation geostationary meteorological satellites such as FY-4, Himawari-8, GOES-R and Meteosat-8, takes the CloudSat and CALIPSO active radar fusion products as the truth value, and combines machine learning method to build a near global scale all-time cloud detection and phase recognition algorithm. For ice cloud, water cloud and mixed cloud, consider the band configuration characteristics of different satellite sensors, select the optimal channel combination as the input training data, develop the cloud water path retrieval method which is suitable for multiple geostationary satellites. Then, verify the accuracy of the retrieval results in combination with the cloud observation data from ground-based microwave and millimeter wave radiometer observation data.
AS70-A011
Assessing the Super-spheroid Ice Models for Radiative Transfer Simulations and Satellite Retrievals in the Infrared Band
Senyi KONG1#+, Lei BI1, Wei HAN2
1Zhejiang University, 2CMA Earth System Modeling and Prediction Centre, China Meteorological Administration
The accurate representation of microphysical properties of ice particles is essential for radiative transfer simulation in clouds. However, the same microphysical scheme of ice particles is often used in radiative transfer simulations for different regions and atmospheric states. Therefore, due to the inappropriate size and shape assumptions of ice particles, nonnegligible uncertainties could exist, causing bias of simulations as compared to observations. The super-spheroid model offers a flexible framework to represent a range of ice particle shapes, allowing for the optimization of shape parameters to minimize the potential biases in the simulations. This study presents an assessment of super-spheroid ice models for infrared band radiative transfer simulations and satellite retrievals. By adjusting the shape parameters, we aim to achieve minimum bias between simulations and observations and obtain optimal ice particle models for different regions and atmospheric states. We will present representative examples of remote sensing retrieval and data assimilation in numerical weather forecast based on super-spheroid ice models, demonstrating their effectiveness in improving radiative transfer simulations.
AS70-A007
Radiative Heating and Upwelling by Different Types of TTL Clouds Over the Tropical Convective Regions
Siliang LEI#+, Chao LIU
Nanjing University of Information Science & Technology
Tropical tropopause layer (TTL) clouds play important roles in Earth's radiation balance and troposphere-to-stratosphere transport. Examining how different TTL cloud type gives influence on the radiative heating, we classified TTL clouds into three types (i.e., deep convective cloud, optically thick convective anvil cloud, and optically thin cirrus cloud) over the convectively active four tropical regions (i.e., Central Africa and South America continental regions and the Central and Western Pacific oceanic regions), using the combined Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) and CloudSat data. Using the classified cloud data, we first examined characteristics of the macrophysical and microphysical properties of the classified cloud types. Amongst three types of TTL clouds over selected four regions, thin cirrus clouds are most abundant (almost four-fifths), and approximately 7% and 17% of TTL clouds are deep convective cloud and thick convective anvil clouds, respectively. We further examined radiative heating over the TTL altitudes by each cloud type and the associated radiatively-driven upwelling motion. It is revealed that the dominant contribution to the overall radiative heating is from thin cirrus clouds (∼48.4%) because of their abundance. Nevertheless, convective anvil clouds and deep convective clouds are also found to give significant contribution to the radiative heating. Such cloud radiative heating tends to lower the level of zero net radiative heating rate found in the clear sky by ∼400–900 m. The TTL clouds play an important role in the secondary circulation in the TTL by inducing the upwelling motion throughout the TTL, supporting the mechanism that the radiative effect of TTL clouds can enhance the mass flux from the troposphere to the stratosphere.
AS70-A005
Accounting for Particle Nonsphericity and Inhomogeneity in an AI-enabled Aerosol Optical Scheme for Weather and Climate Modeling
Xuan WANG+, Lei BI#
Zhejiang University
Atmospheric aerosols often exhibit nonspherical and inhomogeneous (NSIH) features, which significantly impact their optical properties. However, these features have not been well accounted for in weather or climate models due to the challenge in aerosol optics simulations. To address this gap, we developed a novel AI-enabled aerosol optics approach that incorporates particle nonsphericity and inhomogeneity into aerosol optics simulations. Specifically, we used coated super-spheroid model to represent dust and sea salt aerosols, and developed encapsulated and partially encapsulated fractal model for black carbon aerosols. By using the Invariant Imbedding T-Matrix Method (IITM) method, we have established databases of single-scattering properties of these nonspherical and inhomogeneous aerosols. These databases form the basis for training deep neural networks (DNNs) that can rapidly compute optical properties. The DNNs were then integrated into a newly developed module, referred to as the Nonideal Aerosol Optical Scheme (NAOS), for on-line computation of optical properties. The NAOS module was further on-line coupled with Global/Regional Assimilation and Prediction System with Chinese Unified Atmospheric Chemistry Environment (GRAPES/CUACE). Case studies in East Asia demonstrated the importance for accounting for the NSIH effect, revealing significant impacts on aerosol absorptive optical depth (AAOD), short-wave heating rates and meteorology factors. This work paves the way for more accurate weather and climate predictions, considering the complex nature of atmospheric aerosols.
Session Chair(s): Chung-Chieh WANG, National Taiwan Normal University, Kevin CHEUNG, Nanjing University of Information Science & Technology
AS46-A018
| Invited
Projected Convective Storm Environment in the Australian Region Under Climate Change
Kevin CHEUNG1#+, Fei JI2, Nicholas HEROLD3, Nidhi NISHANT4
1Nanjing University of Information Science & Technology, 2NSW Department of Planning and Environment, 3Applied Climate Science Pty Ltd, 4University of New South Wales
Local thunderstorm has been one of the major meteorological hazards in the Australian region. By nature, these storms have compound impacts, ranging from hail, lightning, flash flood and wind gust, and the impacts always top the list of economic losses. Studies on the climate change impact to local storm face the difficulties of short reliable storm climatology and uncertainties in the numerical modelling with the highest resolution to explicitly resolve convection. In this study we have adopted an approach to examine the ingredients of severe storm development based on regional climate model simulations. The dataset to examine is a major investment in New South Wales (NSW), Australia to perform regional dynamical downscaling for projecting climate change impacts and environmental hazards, which is named the NSW and Australian Regional Climate Modelling (NARCliM) project. The projected convective indices, such as the convective available potential energy (CAPE), to the second half of the twenty-first century based on CMIP3 and CMIP5 scenarios indicate an environment more conducive to thunderstorm development over most of the Australian continent, although the convective inhibition number (CIN) will also increase in many regions. A scheme has been developed to adjust the convective indices and 0–6-km vertical wind shear (VWS) such that the simulated storm days match well with historical records. A measure that combines CAPE and VWS, termed storm severity, further shows that the potential storm days over northern and southeast Australia will increase substantially under climate change.
AS46-A001
Precipitation and Intensity Changes of Intense Typhoon Cases Over Western North Pacific in Future Climate
Yi Ting THEAN1#+, Min-Ru HSIEH2, Chung-Chieh WANG1, Zhe-Wen ZHENG1
1National Taiwan Normal University, 2Academia Sinica
Six of the most intense Western North Pacific typhoons in the 21st century, Megi (2010), Haiyan (2013), Vongfong (2014), Soudelor (2015), Meranti (2016), and Yutu (2018), are reproduced in the Cloud Resolving Storm Simulator (CReSS) at 2.5 km resolution. Their sensitivities between 1981-2000 and 2081-2100 are tested in two Representative Concentration Pathways (RCP), RCP4.5 and RCP8.5. These are averages from 38 Coupled Model Intercomparison Project (CMIP) phase 5 models. There is around 172.5 m (86.6 m) of geopotential height, 2.1 K (1.2 K) atmospheric temperature, 0.9 g kg-1 (0.4 g kg-1) specific humidity, and a 4.0 K (2.1 K) sea surface temperature (SST) increment with a rather anticyclonic circulation in RCP8.5 (RCP4.5). Results show approximately 2.1 mm h-1 (0.8 mm h-1) stronger rainfall rates within 250 km radii and 8.6 hPa (3.6 hPa) weaker central pressure in RCP8.5 (RCP4.5). Generally, the initial geopotential regulates weaker circulation, the initial temperature reduces water vapour saturation, and the decreasing temperature gradients across simulations have inhibited their development. Some typhoons have different sensitivity to wind shear, temperature, water vapour, and SST. For Megi, Haiyan, and Meranti, precipitation has intensified by about 9.1% (7.8%) and 19.7% (16.3%) within 200 km (400 km) radii in RCP4.5 and RCP8.5, respectively. Although increasing background moisture and upward motion have resulted in stronger rainfall, especially at the core, the expanding radius of inner convection would weaken their intensity. Moreover, the risen height of the melting layer would increase the generation height and decrease the quantities of ice phase particles. In water budget analyses, density advection, absolute humidity changing rate, and mainly density convergence are increasing in the future. Furthermore, there is roughly 25.0% (13.1%) more precipitable water and 6.4% (1.8%) more integrated horizontal convergence in RCP8.5 (RCP4.5). Both have substantial contributions to the increasing rainfall.
AS46-A011
Comparative Analysis of Synoptic Environment for Mesoscale Convective Systems Using ERA5 Reanalysis Data
Jeong-Eun LEE+, Gyu Won LEE#
Kyungpook National University
Mesoscale convective systems (MCSs) lead to high-impact weather such as heavy rain, strong winds, and hail. To reduce the significant damage caused by MCSs, it is necessary to improve the forecast accuracy. Much of our understanding of the synoptic setup has focused on the heavy precipitation events in South Korea. Understanding the synoptic patterns that are favorable for the formation and development of MCSs is a good starting point. In this study, we generalize the synoptic conditions according to MCS types through composite analysis using basic and dynamic/thermodynamic variables obtained from European Centre for Medium-Range Weather Forecasts (ECMWF) fifth-generation reanalysis data (ERA5). MCSs were divided into four types, convective cells (CC), mesoscale convective complex (MCC), and parallel/diagonal squall line (PSL/DSL) based on the morphological and movement features of convective storms using radar and satellite images during 2018-2021. The AWS (Automatic Weather Station) reanalysis data was used to determine the reference time for composite analysis. The reference time was defined as the time when the largest 1hour accumulated rainfall occurs within each event. CC is characterized by very weak horizontal pressure gradients because they are mainly developed by orographic lift. MCC developed along with the mesoscale trough deepened by the low pressure over eastern China. The baroclinic structure that induces the upward motion at the east side of an upper-level trough forced the SLD by thermally direct secondary circulation at the entrance of an upper-level jet. SLP is organized on a quasi-stationary frontal zone between a continental low over northeastern China and the North Pacific high. In the future, the observational data will be used to figure out the mesoscale mechanism in more detail. Acknowledgment: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS46-A006
Convective Characteristics and Thermal Dynamic Mechanisms for Coastal Torrential Rainfall Over South China During June 2017
Yun CHEN1#+, Zhilin ZENG2
1China Meteorological Administration, 2Guangdong Meteorological Observatory
Torrential rainfall often occurs at the coast of South China, with background of frontal rain band over northern South China or the Yangtze River basin, but it is difficult to forecast. Based on multiple observation data and ERA5 reanalysis data, we researched coastal torrential rainfall event from 15 to 16 June 2017. We contrasted the precipitation characteristics and ambient atmospheric conditions between frontal rain band and coastal rainfall, and analyzed convection initiation and maintenance mechanisms for the latter. Finally, dynamic effect of the convection maintenance was proposed. The results are as follows. (1) There was considerable discrepancy between frontal and coastal rainfall. The former is presented as stratification cloud and weak convective rainfall caused by cold front. The latter characterized with convective, local, concentrated, and long-lived, which occurred at midnight. (2) Horizontal water vapor advection and vertical water vapor transport within boundary layer accounted for discrepancy between frontal and coastal rainfall. Owing to convective instability in middle and low troposphere associated with warm and moisture transport, rain rate over coastal area is notably higher than those under the east of frontal rain band. (3) Lateral friction and direct block from the Mountains caused vertical vorticity develop in river valley, ultimately triggering updrafts and convection initiation. Horizontal vorticity developed with strengthening of vertical wind shear, while southwesterly jet in boundary layer enhanced at midnight, and horizontal vorticity then partly converted into vertical vorticity, overlying the vertical vorticity originated from lateral friction and direct block. The process above is responsible for the long duration of coastal rainfall as well as dynamic effect of convection maintenance. (4) Rainfall sustaining long duration is also associated with the continuous releasing of convection latent heat. Upward vertical velocity caused by thermal buoyancy related to convection latent heat accounted for 39%-75% of total updraft vertical velocity.
AS46-A020
Characteristics of Elevated Thunderstorms on the Cold Side of Fronts in China During the Period 2017–2021
Xiaogang HUANG#+
National University of Defense Technology
Elevated thunderstorm is a type of severe convection that occurs above a stable boundary layer. Limited by observational data, the elevated thunderstorms in China have not been fully understood. Using the data of cloud-to-ground (CG) lightning strokes and ERA5 from 2017–2021, the elevated thunderstorms on the cold side of fronts (ETCFs) in China are analyzed. In general, ETCFs are mainly located in Hunan and Guizhou provinces. The annual cycle exhibits a peak in spring, and the diurnal cycle exhibits a peak at night. In winter, almost all CG lightning in Hunan and Guizhou is in ETCFs. The lowest frequency of ETCFs is in summer, and most occur in the Northeast China Cold Vortex (NCCV). The spatial distribution of ETCFs is closely related to terrain. ETCFs initiate mostly on the east side of mountains, move from west to east, and dissipate on the west side of the downstream mountains. The main weather pattern of ETCFs in Southwest China is as follows: the cold air near the surface accumulates to form a “cold cushion” due to the blocking of the mountains, and there is a low-level jet above the front and a cyclonic circulation in the middle and lower troposphere. NCCV-related ETCFs are often located in front of warm fronts. With the influence of NCCV and the cold air near the surface, warm and moist air climbs along the fronts, which initiates ETCFs. These results provide some help for further understanding the characteristics of ETCFs in China.
AS46-A007
Comparative Analysis of Lightning Characteristics Between Warm-sector and Frontal Heavy Rainfalls Over South China
Xiaotian WU1#+, Dong ZHENG2, Jie FENG1, Yijun ZHANG1
1Fudan University, 2Chinese Academy of Meteorological Sciences
In early summer (April-June), South China frequently experiences regional heavy rainfall events which have been categorized into frontal heavy rainfall (FR) and warm-sector heavy rainfall (WR) in early studies. It has been recognized that the two types of heavy rainfall present remarkable differences in various aspects, including synoptic-scale forcing, local meso-scale dynamics and thermodynamics, topographic effects, and microphysics. Lightning activity is a reliable indicator of severe convection at very high temporal and spatial frequency and is one of the principal hazards caused by severe convections. Despite its importance, the variation in lightning characteristics between FR and WR periods remains insufficiently explored and understood. This study conducts a comprehensive statistical analysis to discern the differences in lightning activity characteristics between the FR and WR. Utilizing 12 years of cloud-to-ground lightning (CG lightning) observation data, our results exhibit that (1) FR events exhibit a higher flash density compared to WR events, suggesting more intense CG lightning activity within FR scenarios. (2) WR is characterized by a notably higher proportion of positive CG lightning. It also features greater peak current and a higher number of strokes in negative CG lightning compared to FR. (3) FR demonstrates a greater frequency of lightning per unit area of rainfall and a lower volume of precipitation per CG lightning strike. This suggests that frontal storm clouds are more inclined to produce lightning but are less efficient in generating rainfall. Possible reasoning supporting these conclusions are also provided.
AS46-A003
The Key Mesoscale Systems and Mesoscale Vortices of the Henan Extreme Precipitation in 2021
Xiuming WANG1#+, Yongguang ZHENG2, Xiaoding YU2
1China Meteorological Administration Training Center, 2China Meteorological Administration
Based on the Doppler weather radar and surface observations, the key mesoscale systems and features of the rainstorm structure during the period of the extreme precipitation in Henan province on 20 July 2021 are investigated. The results show that a nearly meso-α-scale West Henan Low Vortex (WHLV) near the Songshan Mountain, a surface mesoscale front, a horizontal shear convergence line in the lower troposphere and two strong low-level jets (LLJs) were the main mesoscale systems that triggered the extreme precipitation process. Many mesoscale vortices including meso-β-γ-scale vortices (i.e., meso-vortices) were found within the WHLV. Hourly precipitation over 50 mm was mostly caused by the storms with meso-vortices. In the heaviest precipitation stage of the Zhengzhou Storm (ZZS), a clear meso-vortex above 2 km AGL was identified with the diameter of 15–20 km and the vorticity of 1.0–2.0 × 10−3 s−1, while its lifetime was about 2 h. The low-level ambient airflows converged into the storm from the north, east and south, forming a strong low-level convergence that promoted the development of the storm. Strong convergence and uplift occurred along the east edge of the storm, while the strong easterly LLJ converged with the shallow outflow of the storm. The strongest updraft under 2 km AGL occurred at the northeast end of the storm when a short-lived meso-γ-scale vortex formed at that area. Both the strong low-level convergence and the merge of the convective cells from the east resulted in the eastward propagation of the ZZS.
AS46-A022
| Invited
Experiments of Back-building-type Line-shaped MCS Formed Under Horizontally Homogeneous Environments
Yasutaka WAKAZUKI+, Miteki SATOH#
Ibaraki University
Quasi-stationary back-building type line-shaped convective systems (BB-LSCSs) often cause torrential rainfall, mainly in mid-latitude regions. Generally, the formation of BB-LSCSs is considered to be generated by complicated and combined effects such as topographic effect, wind shear, and vertical instability, and the mechanisms have not been sufficiently clarified. Among the various types of BB-LSCSs, we study the generation mechanisms under horizontally homogeneous atmospheric and surface conditions in this study. Initial bubbles are required for convections to be generated under homogeneous conditions. We developed a novel scheme of initial bubbles named the ALB method (Wakazuki and Satoh 2021), with which unrealistic and strong gravity waves in the formation stage of convection are significantly suppressed. The ALB method consists of cold, moist, and convergent circulation increments below the level of free convection around the center of the initial convection based on physical conservation laws. We performed numerical experiments using the JMA-NHM with a grid spacing of 500m under various atmospheric vertical profiles. Under homogeneous conditions, BB-LSCSs were found to be generated in the trailing part of the preceding deep convective system (PDCS). Different types of vertical temperature gradients, relative humidity at the bottom layer, the depth of the moist layer, and the vertical wind shear from low to mid-level have been tested In the sensitivity experiment to understand the essential generation mechanisms of the LSCSs. Sensitivity experiments showed that developed BB-LSCS is more likely to occur under environments with lower dLFC, deep moist layers, and small vertical wind shear. These facts suggest that the intensification of PDCS largely controlled the generation of LSCSs. In addition, the generation of mesoscale depression due to the condensation heating induces a wide-range convergent flow, and the advection effect is considered essential for the successive generation of the conventions on the up-shear side of the PDCS.
AS46-A009
Understanding Simulated Causes of Damaging Surface Winds in a Derecho-producing Mesoscale Convective System Near the East China Coast Based on Convection-permitting Simulations
Liping LUO1, Ming XUE2, Xin XU3, Lijuan LI4#+
1Nanjing University of Aeronautics and Astronautics, 2The University of Oklahoma, 3Nanjing University, 4Chinese Academy of Sciences
A mesoscale convective system (MCS) occurred over east China coastal provinces and the East China Sea on 30 April 2021, producing damaging surface winds near coastal city Nantong with observed speeds reaching 45 m s-1. A simulation using WRF model at 1.5-km grid spacing generally reproduces the development of convective system and the subsequent organization into an MCS, with an eastward protruding bow segment over the sea. In the simulation, an east-west-oriented high wind swath is generated behind the gust front of the MCS. Descending dry rear-to-front inflows behind the bow and trailing gust front are found to feed the downdrafts in the main precipitation regions. The inflows help establish spreading cold outflows at the sea surface and can enhance the downdrafts through evaporative cooling. Meanwhile, front-to-rear inflows from the south are present, associated with severely rearward-tilting updrafts initially forming over the gust front. Such inflows descend behind (north of) the gust front, significantly enhancing the downdrafts and near-surface winds within the cold pool. Calculated trajectories show that parcels contributing to the simulated strong near-surface winds towards Nantong primarily originate from ahead (south) of the east-west-oriented gust front. Momentum budget analyses reveal that large westward-directed horizontal pressure gradient force within the simulated cold pool and weak sea-surface drag work together to produce rapid flow acceleration towards Nantong. The analyses enrich the understanding of damaging wind characteristics over the East China coast and will be helpful to operational forecasters.
AS46-A002
High-resolution Simulation of Typhoon Hagupit (2008) and Formation Mechanism of Its Rainband
Chung-Chieh WANG1#+, Nan-Chou SU1, Pi-Yu CHUANG1, Wen-Chau LEE2
1National Taiwan Normal University, 2University Corporation for Atmospheric Research
Typhoon Hagupit (2008) moved westward and passed through the Luzon Strait to the south of Taiwan in late September 2008. Using air-borne Doppler radar observations, an earlier study has shown that one of its rainbands to the northeast of the center possessed mixed characteristics of both outer and inner rainbands during this stage. To further study the evolution and formation mechanism of this rainband, cloud-resolving simulation of Hagupit was performed using the Cloud-Resolving Storm Simulation (CReSS) at a horizontal grid size of 1 km. The model results compare quite favorably with observations, and are therefore used for further examination. In the model, repeated rainband formation is seen roughly 300 km to the east of the typhoon center, at the inner side near the end of an older rainband. After initiation, each rainband subsequently grows longer and stronger, and moves downwind with the cyclonic rotation of the typhoon circulation. Using a quasi-Lagrangian framework that moves with the typhoon, the old rainband is reminiscent to a squall line and propagating outward, with precipitation associated with cold pool and divergence at the inner side. This near-surface divergence helps enhance the low-level convergence in the formation area of the new rainband, and thus rainbands form repeatedly there.
Session Chair(s): Haonan CHEN, Colorado State University
AS76-A012
Airborne Phased Array Radar (APAR): The Next Generation of Airborne Polarimetric Doppler Weather Radar
Everette JOSEPH1+, Wen-Chau LEE2#, Krista LAURSEN1
1National Center for Atmospheric Research, 2University Corporation for Atmospheric Research
The National Science Foundation (NSF) of the United States approved the Airborne Phased Array Radar (APAR) Mid-scale Research Infrastructure-2 proposal in 2023 to develop the next generation airborne polarimetric, Doppler weather radar mounted on the NSF/National Center for Atmospheric Research (NCAR) C-130 aircraft. Polarimetric measurements are not available from current airborne tail Doppler radars. The APAR system will consist of four removable C-band active electronically scanned arrays (AESA) strategically placed on the fuselage of the aircraft. Each AESA measures approximately 1.5 x 1.5 m and is composed of 2368 active radiating elements arranged in a total of 37 line replaceable units (LRU). Each LRU is composed of 64 radiating elements that are the building block of the APAR system. The development will take 5 years to be completed in summer 2028. APAR adopts a phased approach as an active risk assessment and mitigation strategy. Both the NSF and the National Oceanic and Atmospheric Administration have funded the APAR project for risk reduction activities in the past 5 years. The APAR Team is actively seeking partners in industry and in the university community. An APAR science and engineering advisory panel has been organized. The authors will update current progress and accomplishments of APAR during the first year of the development, including the activities of the university and private industry partners and the engagement of collaboration with research and operational communities.
AS76-A013
The Airborne Phased Array Radar (APAR) Observing Simulator
Wen-Chau LEE1#+, Bradley KLOTZ2, Jothiram VIVEKANANDAN2
1University Corporation for Atmospheric Research, 2National Center for Atmospheric Research
Development of new observing systems is critical for the advancement of scientific understanding of weather phenomena. These instruments establish a proving ground for future operational transition while also providing tools for the research community. One of the issues with developing new instrumentation is the unknown performance characteristics of the instrument and the subsequent unknowns in uncertainty in measurements. The APAR Observing Simulator (AOS) was developed to understand APAR's measurement capabilities for high-impact weather events. Using Cloud Model 1 (CM1) and Weather Research and Forecasting (WRF) model output to provide various storms of interest and their surrounding environments, simulated NCAR C-130 flights are operated within the model space. Radar moments are determined using the Cloud Resolving Model Radar Simulator (CR-SIM). The output can be examined directly or passed through additional tools to analyze various aspects of the data collected during each flight. This paper will report the recent development of the AOS to better simulate the characteristics of a phased array radar on a moving platform. In addition, the authors will present how AOS will be used as a component in the future APAR data analysis software system.
AS76-A008
Impact of Assimilating C-band Phased-array Radar Data with EnKF on the Forecast of Convection Initiation: A Case Study
Jie MING1, Yinghui LYU1#+, Kun ZHAO1, Hao HUANG1, Xingchao CHEN2, Peng GONG1, Shuguang WANG1
1Nanjing University, 2The Pennsylvania State University
This study used a WRF-based Ensemble Kalman Filter (EnKF) system to assimilate reflectivity (Z) and radial velocity (Vr) data in precipitating and clear-air regions from the Beijing Daxing International Airport C-band phased array radar (C-PAR) to improve the forecasts of a convective initiation (CI) case occurred on June 18, 2020. The results showed that high frequency assimilating the C-PAR Vr in clear-air region is conducive to increase the forecast lead time of CI by significantly improving the initial dynamic and thermodynamic fields, which creates a more accurate pre-CI environment. After assimilating the C-PAR clear-air Vr, the CI case can be accurately predicted with a 20 minutes forecast lead time in the best case scenario. This is the first real case study to demonstrate the benefits of assimilating high spatiotemporal resolution PAR clear-air radial velocity data for the CI process.
AS76-A004
The Flexible Array of Radars and Mesonets (FARM), the Bistatic Adaptable Radar Network (BARN), and the S-band on Wheels (SOW)
Joshua WURMAN1#+, Karen KOSIBA2
1FARM Univ of Alabama, 2University of Illinois
The Flexible Array of Radars and Mesonets (FARM) Facility is an extensive mobile multiple-Doppler radar and in-situ instrumentation network. The FARM comprises four mobile / quickly-deployable radars: two X-band Doppler On Wheels DOW6/DOW7, the Rapid-Scan DOW (RSDOW), the C-band On Wheels (COW), and mini-COW. The FARM includes 3 mobile mesonets (MM) with 3.5-m masts, an array of rugged weather stations (PODNET), weather stations deployed on infrastructure including light/power poles (POLENET), and other instrumentation. The FARM’s integration of radar, in situ, and sounding systems provides robust kinematic, thermodynamic, and microphysical observations. FARM has deployed to >30 projects, obtaining pioneering observations of a myriad of small spatial scale and short temporal scale phenomena including tornadoes, hurricanes, lake-effect snow storms, aircraft-affecting turbulence, convection initiation, microbursts, intense precipitation systems, boundary layer structures and evolution, airborne hazardous substances, coastal storms, wildfires, weather modification, and mountain/alpine weather. Major upgrades and additions to the FARM targeted observing network are proposed. The Bistatic Adaptable Radar Network (BARN), an inexpensive, portable and adaptable, bistatic network employing simplifying technologies, communications networks, and board-based processing. A next-generation long wavelength adaptable/targetable research radar network, comprising an array of truck-borne scanning 10-cm radars, S-band On Wheels (SOW), can provide fine-scale S-band observations of the atmospheric boundary layer, convective, and other precipitating systems, simultaneously measuring dynamically meaningful fine-scale vector wind fields. SOW and BARN will fill critical gaps in current observing systems, providing broadly and inexpensively available long wavelength, dual-polarimetric, near-ground, fine-scale, vector wind observations.
AS76-A005
Doppler Velocity Dealiasing and Noise Filtering Algorithm Based on Iterative Surface Fitting Approach
Wei-Ting FANG1#+, Pao-Liang CHANG2
1Central Weather Administration, 2Central Weather Bureau
Radar Doppler velocity is an essential data for obtaining three-dimensional information about weather systems. However, the automatic and stable recovery of Doppler velocity from dealiasing has been a challenge in real-time scenarios. In this study, an iterative surface fitting dealiasing (ISFD) algorithm designed for weather Doppler radars is proposed. The algorithm employs iterative processes to generate reference fields from Doppler velocity data, utilizing 2D fast Fourier transform (FFT) for dealiasing and noise filtering. Iterations continue until the Doppler velocity data are fully recovered from aliasing. The key innovation of the proposed approach involves the controlled adjustment of the highest-allowed wavenumber of the reference field through a low-pass filter. This adjustment transitions from a low to high wavenumber with each iteration. Initially, a smoothed reference field with a low wavenumber is utilized to dealiase and filter out most of the abnormal data and part of the correct data during the first iteration. Subsequently, the adjusted data are used to generate a new reference field with an increased wavenumber, preserving more correct data for the next iteration. This process repeats until the data reach a stable state. The effectiveness of the ISFD algorithm is evaluated using data from four typhoon cases that impacted Taiwan in 2023. Verification results demonstrate accuracy rates ranging from 97.4% to 100%. This performance underscores the potential operational utility of the ISFD algorithm, providing high-quality Doppler velocity data. Downstream applications, including radar wind retrieval and data assimilation, stand to benefit significantly from the enhanced data provided by the ISFD algorithm.
AS76-A003
A Climatological Study on the Two Types of Bow Echoes Over South China
Ang ZHOU+, Kun ZHAO#, Xin XU
Nanjing University
Classical bow echoes (CBEs) normally develop due to rear-inflow jets, while merger-formation bow echoes (MFBEs) evolve from the merger between linear systems and pre-line convection. MFBEs are rarely documented before and the key processes remain unclear because of the small-scale and fast-evolving merging processes. Using radar observations during 2015-2019, this study examines the characteristics of these two types of bow echoes over South China. Eighteen MFBEs and eleven CBEs are identified, accounting for 62% and 38% of the total twenty-nine bow echoes, respectively. MFBEs commonly occur over coastal regions in the afternoon, where southerly sea breezes provide favorable thermodynamic conditions. About half CBEs develop over mountainous areas in the morning, and northerly winds enhance the local baroclinity and kinematic convergence. A new Merger-Classical (MC) index is proposed to distinguish the environments for the development of two types of bow echoes, disclosing the more favorable near-surface thermal conditions for MFBEs. In addition, more severe weather occurs in metropolitan area near the Pearl River Delta region during MFBEs, in which the accumulated precipitation is about 2.5 times higher than that during CBEs. This study reveals the discrepancies between MFBEs and CBEs over South China, emphasizing the MFBEs account for more than half of the total bow echoes and cause more high-impact weather in the metropolitan area. This study proposes a new perspective on the environment in which bow echo forms by merger process over South China, urging for more research to explore the underlying processes.
AS76-A009
The Development of a Squall Line During IOP3 in TAHOPE 2022
Chiu-Ling LIAO#+, Ming-Jen YANG
National Taiwan University
One of the weather features observed during the Taiwan-Area Heavy rain Observation and Prediction Experiment (TAHOPE) is a mesoscale convective system (MCS) under the influences of Taiwan topography. On 6 June 2022, a squall-line MCS associated with a Mei-Yu front approached northern Taiwan. As it moved close to the coast, the squall line was stagnated and weakened. Radar quantitative precipitation estimation (QPE) by the Central Weather Administration (CWA) showed widespread precipitation exceeding 100 mm/day over the northern Taiwan Strait, but significantly less precipitation on land over northwestern Taiwan. Radiosonde observation at 06 UTC on 6 June revealed a strong southwesterly wind maximum at 2–3 km altitude. Additionally, surface stations recorded a pressure gradient from south to north, indicating the presence of a barrier jet. Using the data from NCAR S-Pol radar in Hsinchu and CWA Shulin radar in New Taipei, and applying the Spline Analysis at Mesoscale Utilizing Radar and Aircraft Instrumentation (SAMURAI) technique, we retrieved three-dimensional wind field indicating strong southwesterly wind in the lower atmosphere. These winds enhanced the low-level convergence ahead of the squall line, causing the stratiform region to develop parallel to the line convection. The mesovortices accompanied by high reflectivity moved along the convective line and contributed to strong rear-to-front flow before the stagnation of squall line. After the deceleration of the convective line, the updraft tilted to the front, and the precipitation-induced evaporation caused the weakening of convection.
Session Chair(s): Jung-Hoon KIM, Seoul National University
AS68-A002
Forecasting Contrail Climate Forcing for Flight Planning and Air Traffic Management Applications
Roger TEOH1#+, Zebediah ENGBERG2, Marc STETTLER1, Thomas DEAN2, Tharun SANKAR3, Marc SHAPIRO2
1Imperial College London, 2Breakthrough Energy, 3Google
Aviation accounts for 3.5% of the global anthropogenic climate forcing, of which approximately half of it can be attributed to contrail cirrus but with large uncertainties1. Contrails form behind an aircraft when conditions in the exhaust satisfy the Schmidt-Appleman criterion, where the initial contrail properties depend on the aircraft characteristics (mass and wingspan), engine soot particle emissions, and ambient conditions. If the atmosphere is ice supersaturated, these contrails can persist, spread, and evolve into contrail cirrus with observed lifetimes of up to 19 h2,3. A recent study4 simulated contrails globally with the trajectory-based contrail cirrus prediction model (CoCiP)5 and estimated that 20% of all flights formed persistent contrails in 2019. Among these flights, 70% of them (17% of all flights) having a net warming effect, while 10% of them (2.7% of all flights) caused 80% of the global annual contrail energy forcing4. One option to mitigate the contrail climate forcing is re-routing flights around regions forecast to form strongly warming contrails, while accounting for the potential for additional fuel consumption, as well as meteorological and contrail model uncertainties in the decision-making process. Here, we developed a 4D contrail forecast model from the trajectory-based CoCiP to identify regions with a high probability of forming strongly warming contrails. The model initialises an infinitesimal flight segment at each grid cell, simulates the persistent contrail segments until its end-of-life, and produces a 4D map of the contrail energy forcing per flight distance. We discuss the technical challenges of developing the contrail forecast model, including the need to: (i) account for different aircraft-engine types and forecast uncertainties, while maintaining computational efficiency; and (ii) validate the model outputs with the trajectory-based CoCiP and satellite observations. These contrail forecasts can be requested via an Application Programming Interface and have been successfully integrated into existing flight planning tools.
AS68-A001
Turbulence Observation and Simulation
Po-Hsiung LIN#+
National Taiwan University
Accurate monitoring and understanding of atmospheric turbulence are crucial for improving flight safety and weather prediction. However, traditional observation methods on EDR such as aircraft observations are not suitable for Taiwan, which are not shated from airliners company to university for research. Therefore, we made a onboard flight set which combination a Mateksys FC H743-WLite flight controller unit (for UAV) and GPS sensor and Mission planner software to record the 50-Hz onboard flight information to get airraft flight status of domestic airlines (UNI ATR74) estimate the atmospheric turbulence on the routes. We present several cases in 2023 during summer thunderstorm and autumn monsoon weathers to estimated the turbilence along the flight route and compared it well to Taiwan Cicial Avisition Administration WRf forecast. This simple solution for turbulence measurement ourselves will move to unmanned aerial vehicles (UAVs) and research jets (such as Taiwan G100 and Japan G400) for typhoon circulation observation with dropsondes.
AS68-A004
Atmospheric Turbulence Retrieved from Global High Vertical-resolution Radiosonde Data
Han-Chang KO1+, Hye-Yeong CHUN1#, Marvin GELLER2, Bruce INGLEBY3
1Yonsei University, 2Stony Brook University, 3ECMWF, Reading
Atmospheric turbulence in the free atmosphere plays a crucial role in mixing air masses, momentum, and energy, while also affecting aircraft operations. Understanding turbulence has remained challenging due to its small-scale and intermittent nature, along with limited high-resolution observational data in the free atmosphere. This study investigates global distributions of atmospheric turbulence utilizing operational high vertical-resolution radiosonde data (HVRRD) for six years from October 2017 to September 2023, based on the Thorpe method. Globally, turbulence is stronger in the troposphere than in the stratosphere. Particularly, a maximum turbulence occurs in 3 to 6 km below the tropopause, followed by a sharp decrease above the tropopause, then turbulence gradually increasing again. Seasonal variations in turbulence are evident, with the troposphere displaying strong turbulence during summer and weak turbulence during winter in both hemispheres, while the stratosphere exhibits strong turbulence during spring. Regional analysis shows turbulence hotspots over the South Pacific and South Africa in the troposphere, while over East Asia and South Africa in the stratosphere. Analysis of a six-year period reveals significant trends of turbulence in various regions, with positive trends in Europe, Siberia, and Antarctica, and negative trends in Alaska, the United States, East Asia, and Southern Africa. In addition, HVRRD provides turbulence information even in regions and high-altitudes where commercial aircraft do not operate, indicating its potential utility not only for current commercial aviation but also for future high-altitude aircraft operations.
AS68-A006
Evaluation of Multi-model and Diagnostic Ensemble (MMDE)-based Probabilistic Turbulence Forecast Using the Two Operational NWP Models of KMA
Dan-Bi LEE1+, Jung-Hoon KIM1#, Hye-Yeong CHUN2
1Seoul National University, 2Yonsei University
The current operational aviation weather centers worldwide mostly provide aviation turbulence prediction information from deterministic turbulence forecasts based on turbulence diagnostics derived from the numerical weather prediction (NWP) model outputs. Considering that the NWP model and turbulence diagnostics have inherent uncertainties, the need for probabilistic turbulence forecasts that take into account such uncertainties and provide confidence for a given forecast products is increasing. In this study, the multi-model and diagnostic ensemble (MMDE)-based probabilistic turbulence forecast is tested using the two operational Global Data Assimilation and Prediction System (GDAPS) outputs of the Korea Meteorological Administration (KMA). Currently, the two GDAPSs are produced separately from the Unified Model (UM) and the Korean Integrated Model (KIM) systems, and the UM- and KIM-based GDAPS data have horizontal resolutions of ~10 km and ~12km, respectively. To derive the MMDE-based probabilistic turbulence forecast, firstly, the UM- and KIM-GDAPS-based probabilistic forecasts are derived separately by considering the GDAPS-based multiple turbulence diagnostics as ensemble members. Then, the MMDE-based probabilistic turbulence forecast is derived by an ensemble mean of the two GDAPS-based probabilistic turbulence forecasts. When comparing the two GDAPS-based probabilistic turbulence forecasts, the predicted turbulence regions are similar in general. But they locally show different turbulence potential regions with different values for severe turbulence. Accordingly, it is expected that the MMDE-based probabilistic turbulence forecast that combines the two GDAPS-based forecasts can provide a better performance skill for detecting severe turbulence. Detailed performance results of the MMDE-based probabilistic turbulence forecast evaluated against available turbulence observations for one year will be presented in the conference. Acknowledgment: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00410, and was supported by Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education (RS-2023-00250021).
AS68-A009
A Climatological Study of Near-cloud Aviation Turbulence Revealed in the Global Reanalysis Data
Soo-Hyun KIM1+, Jung-Hoon KIM2#, Hye-Yeong CHUN3
1NASA Ames Research Center, 2Seoul National University, 3Yonsei University
Moist convection is one of the major sources to generate atmospheric turbulence in the upper troposphere and lower stratosphere (UTLS), directly impacting cruising aircraft. Turbulence associated with convection [near-cloud aviation turbulence (NCT)] can be caused by various generation mechanisms such as shearing and convective instabilities, convectively induced flow deformation, and convective gravity wave (CGW) propagation and its breaking. A recent study by Kim et al. indicates that moderate-or-greater (MOG)-intensity turbulence generated from various sources, including NCT, clear-air turbulence, and mountain wave turbulence, is expected to occur more frequently due to climate change, derived from long-term global climate model data of high-emission scenario and historical condition. In order to ensure a positive long-term trend of NCT at flight levels worldwide using state-of-the-art reanalysis data, this study examines the climatology of upper-level NCT. The analysis is conducted using the European Centre for Medium-range Weather Forecast Reanalysis version 5 (ERA5) data with a horizontal resolution of 0.25° longitude by 0.25° latitude for 44 years (1979-2022). Two indices based on a parameterization scheme of CGW drag (CGWD) of Chun and Baik, which were developed by Kim et al., are calculated: CGWD and eddy dissipation rate derived from CGWD. It is found that NCT diagnostics are concentrated in the tropics and the summertime continents. From probability distribution of NCT diagnostics, the 98th percentile is computed and used as a threshold of MOG-intensity turbulence for calculating occurrence frequencies for 44 years. Also, we analyze NCT trends globally during 1979-2022 in ERA5 reanalysis dataset. Detailed results of climatological analysis of NCT will be presented in the conference. Acknowledgement: This work is funded by the Korean Meteorological Administration Research and Development Program under KMI2022-00410.
AS68-A018
Evaluation of Precipitation Types from Spectral Bin Model Using LDAPS Model Data
Wonbae BANG1,2+, Kwonil KIM3, Jacob CARLIN4,5, Alexander RYZHKOV6,7, Gyu Won LEE1#
1Kyungpook National University, 2Center for Atmospheric REmote sensing, Kyungpook National University, 3Stony Brook University, 4The University of Oklahoma, 5NOAA Oceanic and Atmospheric Research/NOAA National Severe Storms Laboratory, 6NOAA Oceanic and Atmospheric Research, 7NOAA National Severe Storms Laboratory
The surface precipitation type (PT) can be predicted by several ways such as microphysics model and statistics-based method. A recent study showed model-based prediction such as Spectral bin model (SBM) has relatively high accuracy about PT as compared statistics-based methods if good input data is used. Therefore, the performance of SBM should be explored with different input data because input data errors can strongly influence model-based prediction. In this study, we try to utilize LDAPS as input of SBM and evaluate accuracy of LDAPS by comparing with rawinsonde data during ICE-POP 2018 whole period. Also, simulation results from SBM on different input data were compared. PARSIVEL data collected at 5 sites with sounding observation during ICE-POP 2018 period was used to validate the simulated PT of SBM about three types (rain [RA], snow [SN], RASN). The comparison results between LDAPS and rawinsonde show that temperature and wet-bulb temperature (relative humidity) of LDAPS tend to underestimate (overestimate) as compared rawinsonde data below 3 km above ground level known as a critical layer for determination of PT in winter season. SBM with LDAPS data in SN events makes more misprediction as RASN, which implies relatively more melting. In contrast, there are more mispredictions as SN (RASN) in RASN (RA) events in the simulation of SBM with LDAPS data. The results imply the bias of LDAPS data depends on atmospheric environmental condition. In the future, we will explore errors of LDAPS data in various conditions such as precipitation and non-precipitation. Also, we will design a method to reduce errors of LDAPS data. Acknowledgment: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS68-A020
Development of Model Output Statistics for Ceiling and Visibility Prediction at Major Airports in South Korea
Jeonghoe KIM+, Jung-Hoon KIM#
Seoul National University
Low ceiling and reduced visibility are considered as one of the most hazardous weather phenomena in the aviation industry. For safe and efficient aviation operations, meteorological offices regularly issue terminal aerodrome forecasts (TAFs) at every 6-hour at the airport, which include 24-hrs of predictions for various meteorological information such as wind, temperature, visibility, and ceiling. The objective of this study is to develop a model output statistics (MOS) system for the prediction of visibility and ceiling at major airports in South Korea, which can be used as auxiliary information for issuing operational TAFs. Using several years of (1) the Korea Meteorological Administration’s operational and regional numerical weather prediction (NWP) model outputs interpolated to the airport locations and (2) hourly meteorological observations at the airport (i.e., METAR), various statistical models for constructing the MOS system were trained to compute statistical relations between the predictors (NWP model outputs and previous observations) and predictands (observed ceiling and visibility from the measurements at the airports). For the statistical models, both linear (multilinear regression and LASSO) and nonlinear (random forest) models were used to generate regression (continuous values) and classification predictions (nominal values of the categorical expressions) of ceiling and visibility. It was found that the inclusion of the previous observations as the predictors improved the forecast performance skill for the short-term prediction in terms of mean absolute error. With the increase of the projection time to 24-hr forecast, however, forecast performance skill became closer to that of the conventional NWP model outputs by gradually losing its feature importance from previous observations. It was also found that the inclusion of the classification prediction helped improving the short-term forecast skill in terms of balanced accuracy. Acknowledgement: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00310.
AS68-A021
Airport Probability Weather Forecast System by Stochastic Method
Eun-Chul CHANG1#+, Ui-Yong BYUN1, Duho JEONG1, Hye-Yeong CHUN2, Jung-Hoon KIM3
1Kongju National University, 2Yonsei University, 3Seoul National University
In this study, probability weather forecast system for airport support is developed. Air-traffic management requires rapid-updated prediction. The Korea Local Analysis and Prediction System (KLAPS), which is the operating numerical weather prediction model for very-short range forecast, updates initial condition at every 10 minute for 12-hour forecast. The new short-range probability forecast system generates ensemble members by applying stochastic method during model integration which uses KLAPS initial and lateral boundary conditions. Two stochastic methods, stochastically perturbed physics tendencies (SPPT) and stochastic kinetic-energy backscatter scheme (SKEBS), are tested for the forecast system. 20 ensemble members are produced by the system with 20 different set of perturbation fields. Probability prediction is performed for vertical wind shear and visibility. Results from each ensemble member are similar to the control run which is the KLAPS. But, it is shown that some of dispersed members can give information about chances of severe phenomena which can affect air-traffic operation when the control run cannot capture the strong wind shear or low visibility. It is expected that the stochastic method based probability forecast system will provide helpful information for decision makers in operational air-traffic management.
Session Chair(s): Shaojie SONG, Nankai University, Olga KALASHNIKOVA, California Institute of Technology
AS09-A010
| Invited
Characterizing Ammonia Emission Sources in California's Salton Sea Region Using Airborne Thermal IR Imaging, Ground-based Stationary and Mobile Monitoring, and Chemical Transport Modeling
Olga KALASHNIKOVA1#+, Sina HASHEMINASSAB1, Le KUAI1, Yuan WANG2, Chenchong ZHANG2, John H. SEINFELD1, David TRATT3, William PORTER4, Yaning MIAO5
1California Institute of Technology, 2Stanford University, 3The Aerospace Corporation, 4University of California, Riverside, 5California Air Resource Board
Ammonia's role in atmospheric chemistry and air quality is multifaceted and significant. Predominantly emerging from agricultural and industrial activities, as well as from natural sources, it is a key precursor to PM2.5. Ammonia’s interaction with acidic pollutants leads to the formation of ammonium salts, contributing to secondary PM. Nonetheless, ammonia's characterization is fraught with challenges due to its high reactivity and solubility, which hinder accurate measurement and analysis. This complication obscures our understanding of its atmospheric transport and transformation. In California, ammonia emissions are notably high. However, conventional emission inventories often underestimate these emissions, leaving a gap in our understanding of ammonia's true impact on air quality. Particularly, the Salton Sea stands out as a significant emission hotspot, attributable to a combination of agricultural, industrial, dairy, cattle feedlots, and geothermal power plant activities. To characterize the trends, levels, and sources of ammonia in the Salton Sea region, we conducted two comprehensive field campaigns in March and September 2023. These campaigns integrated airborne remote sensing with ground-based stationary and mobile monitoring, coupled with chemical transport modeling. The Aerospace Corporation conducted airborne thermal infrared (TIR) hyperspectral imaging on March 28 and September 25 using the Mako sensor aboard a Twin Otter aircraft. These measurements covered the northwestern and southwestern regions of the Salton Sea, referred to as the Mecca and Imperial regions. To capture variations in emissions throughout the day, the September campaign included airborne measurements conducted both in the morning and in the afternoon. These measurements identified ammonia emission sources down to a few meters, significantly enhancing our understanding of the distribution of individual point sources. Concurrently, mobile ammonia monitoring was conducted in both regions, along with ground-based stationary monitoring of ammonia and other pollutants in Mecca. This presentation will discuss the results gathered during this study and outline the next steps.
AS09-A004
| Invited
Atmospheric Acidity and Its Interaction with Secondary Aerosols
Shaojie SONG#+
Nankai University
Acidity (typically referred to as aerosol acidity and cloud water acidity) is a central component of atmospheric aqueous chemistry. While conventional techniques have proven effective in quantifying cloud pH, their applicability to aerosol water acidity remains limited. Presently, direct methodologies for assessing aerosol pH, although under continuous refinement, are not yet ubiquitously adopted for field measurements. In addressing this gap, thermodynamic equilibrium box models have emerged as pivotal tools, facilitating the estimation of chemical species partitioning across distinct phases—solid, liquid, and gas—and subsequently enabling precise aerosol pH calculations. However, recent discussions underscore substantial discrepancies in aerosol water pH estimates, particularly evident during winter haze episodes in the North China Plain. This study provides an in-depth examination of the computational methods and applicability of the typical thermodynamic models such as ISORROPIA and E-AIM. Notably, reverse (using only aerosol composition as input) calculations, predicated solely on aerosol composition, have exhibited sensitivity to inaccuracies in ion measurements, necessitating cautious interpretation. And aerosol phase state does not have a significant effect on aerosol water pH. Furthermore, multiphase buffering theory elucidates the dynamic pH variability within aerosols, with the NH4+/NH3 (ammonium/ammonia) acid-base pair assuming a predominant buffering role within densely populated continental regions. Concurrently, ongoing research endeavors have sought to delineate the consequential effects of acidity on secondary aerosol, including sulfate, nitrate, and organic sulfur compounds, underscoring the intricate interplay between aerosol composition and environmental factors.
AS09-A007
Spatial and Temporal Variation of Aerosol Optical Depth in Huaihai Economic Zone from 2000 to 2021
Shuhui WU#+, Yong XUE
China University of Mining and Technology
The Huaihai Economic Zone is located in the north-south climate transition zone of China. Notably, as the connection zone between two key regions of air management around the Yangtze River Delta and Beijing-Tianjin-Hebei, it presents significant composite pollution characteristics and becomes a key control area of the Ministry of Ecology and Environment. However, the current studies on the regional level of air pollution in China mainly focus on economically developed regions such as Beijing-Tianjin-Hebei, there are fewer studies on other regions. Aerosol optical depth (AOD) is an important indicator and key parameter for understanding atmospheric physics and regional air quality. Accurate information on the spatio-temporal distribution of AOD and the relationship between AOD and atmospheric pollution is important for promoting inter-regional aerosol transport decompression government decisions. In this study, we investigated the spatio-temporal variation characteristics of AOD in Huaihai Economic Zone during 2000-2021 based on the AOD data from MODIS MCD19A2. A significant regional difference of AOD was presented with the rapid urbanization process and the adjustment of the city's industrial structure, which was mainly manifested as decreasing from the northwest to the southeast. Due to the differences in weather and geography, the distribution of AOD in the four seasons was various. The AOD showed an increasing trend with the development of industrialization until it peaked in 2011. Then, the local community showed a significant downward trend after the active implementation of clean air policies. In terms of seasons, the whole differences in AOD are evident, exhibiting summer > spring > autumn > winter. Higher AOD was observed in winter than in autumn after 2013, and it was controlled in summer. In recent years, the monthly and quarterly differences in AOD have gradually decreased, which implies that the targeted pollution reduction measures have had a good effect.
AS09-A011
| Invited
Understanding Sources of Air Pollution by Combining Machine Learning and Wavelet Analysis
Qili DAI#+, Yuqin SONG, Hao WU
Nankai University
Air quality time series is of significant periodic patterns, which are linked to a variety of emission sources and atmospheric processes. To detect and differentiate these periodic drivers, we proposed a two-step decomposition approach combining a machine learning-based deweathering model and Morlet wavelet analysis. By applying this approach to the seven years measurements of six regulated air pollutants in eight Chinese cities, we identified signals with strong annual cycle, daily cycle, and long-term periodicity in the emission-driven concentrations of primary air pollutants, primarily driven by the recurring winter heating activities, emissions with regular diurnal patterns like traffic, and long-term emission abatement policy, respectively. While local dispersion, large-scale atmospheric circulation, and synoptical weather, were likely responsible for the daily cycle, periodicities around 365 days, and periodicities within a month observed in the meteorologically driven concentrations, respectively. The power of these periodical drivers varied temporally and spatially, implying the heterogeneity of emission rates and region-specific climates. Such a decomposition approach could serve as an effective tool in air quality research and warrants attention for its potential utility in understanding air pollution dynamics.
AS09-A008
Seasonal Characteristics of New Particle Formation in Beijing, China: Frequency, Intensity and Mechanisms
Zeyu FENG+, Lizi TANG, Dongjie SHANG, Min HU#
Peking University
New particle formation (NPF) is an important source of secondary ultrafine particles in atmosphere. Nucleated particles may become activated to form cloud condensation nuclei or drive haze formation through condensation or coagulation growth. However, it is still not clear why NPF could be observed frequently in urban environment of relatively high aerosol loading, and its seasonal characteristics of frequency, intensity and mechanisms need more elucidation. Here we conducted a long- term measurement of particle number concentration distributions (PNSD) down to ~3 nm in urban Beijing during 2022-2023. Short-term measurements of PNSD between ~1-3 nm and concentration of gaseous sulfuric acid (SA) and ammonia (NH3) were also included. During the observation, NPF frequency, formation rate of 3 nm particles (J3) and growth rate of new particles (GR) are ~40%, 4.3 ± 2.7 cm-3 s-1 and 3.4 ± 2.4 nm h-1, respectively. The relative strength of source (e.g., UVB) and sink (e.g., condensational sink, CS) decides whether and when NPF could take place. Additional mechanisms are required to explain the observed J3, apart from SA-NH3-H2O ternary nucleation. Furthermore, J3 and GR exhibit seasonal variation similar to UVB, highest in summer while lowest in winter. This is attributed to the higher concentration of SA and condensational organic matter in summer, which could drive more rapid growth of nucleated particles to the size detection limit (~3 nm) and further. However, NPF frequency exhibits a reverse trend, lowest in summer, due to the lower frequency of clearing air mass. Our results reveal that NPF in summer may have stronger CCN contribution because of the quicker growth of new particles, though its less occurrence compared to other seasons.
AS09-A002
Study on Synergistic Effects of Leading Factors in Secondary Nitrate Gas Formation Pathway
Yuting WEI#+, Guoliang SHI
Nankai University
The control of fine particulate matter (PM2.5) pollution is considered a top priority of environmental protection by many countries and regions around the world. Nitrate is an increasingly important inorganic water-soluble ion in PM2.5, which is formed through the chemical production of gas-phase nitric acid and subsequent partitioning to the aerosol phase during daytime. In ambient environment, these two processes co-exist and it’s necessary to explore the synergistic effects of driving factors on the two processes. Based on online data from long-term continuous observations in northern China, we established a EK&TMA (Empirical Kinetic & Thermodynamic Modelling Approach) map to explore the synergistic effect of the driving factors on the two processes. In addition, as the predominant form of nitrate, the formation of ammonium nitrate (NH4NO3) was discussed. We explored the influence of multiple driving factors on its formation, including meteorological factors, emission sources, and gaseous precursors based on thermodynamic theory, in the ambient environmental atmosphere. Then, the dominant factors during clean periods and haze periods were identified. Our finding demonstrated controlling NO2 is more efficient for particulate nitrate control under weakly acidic environments. And collaborative control of coal source, vehicle source, and dust source is needed to alleviate nitrate pollution. In addition, the emission reduction of ammonia may be more efficient for controlling ammonium nitrate during haze days. The findings of this work provide a deeper understanding of ammonium nitrate formation and inform the design of effective strategies to control particulate matter pollution.
AS09-A005
Establishment of a VOCs Emission Inventory for Multi-year Cyanobacteria in Taihu Lake Under the Influence of Climate Change and Analysis of Driving Factors
Zihang LIAO1#+, Min SHAO1, Yong ZHA1, Chenwu ZHANG2, Lv SHUN1
1Nanjing Normal University, 2Nanjing University
Volatile Organic Compounds (VOCs) are crucial precursors for tropospheric ozone and aerosol formation. Existing research indicates that VOCs released by aquatic algae constitute a significant, yet often overlooked, global source of VOCs. However, relevant studies in this area are scarce. Global climate change has led to alterations in climatic factors affecting algal growth, indirectly impacting the quantity of VOCs released by algae. With advancements in remote sensing technology, it has become possible to explore the spatiotemporal distributions of VOCs released by algae over large water bodies. This study focuses on Taihu Lake, characterized by frequent occurrences of cyanobacterial blooms. Utilizing MODIS satellite imagery from 2001 to 2020, we analyzed the spatiotemporal characteristics of cyanobacterial blooms in Taihu Lake and its subregions. VOCs related source spectra and emission intensities from cyanobacteria in Taihu Lake are collected based on literature review and are used to compile the first inventory of VOCs emissions from blue-green algae blooms in the Taihu Lake. Employing the LightGBM machine learning model and the (SHapley Additive exPlanations) SHAP values, we quantitatively analyzed the major meteorological drivers influencing cyanobacterial blooms in each region. The results indicate a continuous deterioration of cyanobacterial blooms in Taihu Lake in recent years, with released VOCs posing a persistent threat to the atmospheric environment of surrounding cities. The relative impact of meteorological factors varies across regions, but temperature consistently exhibits the highest sensitivity in all areas. This study is poised to provide a scientific basis for further improving air quality in urban areas adjacent to large lakes.
AS09-A003
Quantifying Individual/multiple Air Pollutant Source Impacts and Drivers Under Combined Pollution Conditions
Zhenyu WANG#+, Guoliang SHI
Nankai University
Air pollutions are frequently reported and thus have received increasing public attentions worldwide. Recognizing the sources of pollutants is the key to mitigating air pollution, of which the development of source apportionment technology is an important technical means. However, reactive species such as volatile organic compounds (VOCs) in the atmosphere are susceptible to chemical reactions and are difficult to trace accurately. In addition, there are a wide variety of atmospheric pollutants and complex influencing factors. Therefore, how to quantify the sources of reactive individual pollutant, multi-pollutants and assess the impact effects of multiple factors have become key scientific issues. Our study (1) based on observations and theoretical mechanisms of atmospheric chemistry elucidates the sources of VOCs and their impacts on O3 formation at different chemical reaction stages in cities in southern and northern China through coupled chemical kinetics and receptor model, and successfully revealed the main drivers of photochemically consumed VOCs to promote the formation of O3, (2) Secondly, an ensemble source apportionment technology is proposed for multiple pollutants for the first time through model constraints, and the common sources and effects are quantified, (3) Finally, we investigate the characteristics of the pollution types captured by combined analysis, and apply machine learning algorithms to quantify the effects of drivers on air pollutants and CO2 formation. In summary, this study expands from individual pollutant to multi-pollutant and then explores the influencing factors of pollutants, which not only gradually improves the source apportionment technology, but also provides effective prevention and control suggestions for atmospheric composite pollution.
AS09-A006
Multi-timescale Variation Characteristics of Burning of Crop Residues and Dust Events in Different Regions of China During 2014-2022
Rui LIU1+, Min SHAO2, Qin'geng WANG1#
1Nanjing University, 2Nanjing Normal University
Comprehensive understanding of crucial seasonal factors, including burning of crop residues and dust events, is vital for an Effective and scientific approach to mitigate PM2.5 pollution in the future. Based on hourly observed PM2.5 concentrations and MODIS fire point data from 2014 to 2022, this study conducted a comprehensive analysis of variation characteristics on annual and seasonal scales, with a special focus on differences across major regions. The annual decline rates of burning of crop residues showed an overall downward trend, with notable variations between seasons. Northeast China Region (NEC) was the most affected region by the burning of crop residues and experienced a big drop in the number of fire points in autumn, but a remarkable increase in spring. Similarly, a relatively large number of fire points were also found in North China Region (NC), but there was a slight increase in spring. These findings highlight the necessity to give more attention to the burning in spring, especially for NEC and NC as well. The occurrence of dust storms decreased from 2014 to 2022, but the strong dust events did not decrease. In comparison with the period from 2014 to 2016, dust events between 2020 and 2022 displayed an expanded spatial influence, covering a wider geographical range. The relatively modest decline rate and the expanded spatial influence of dust events during the spring season contributing to the PM2.5 concentrations downwind regions, such as within Northwest China Region (NWC), NC, and NEC. Our findings underscore the significant influence of dust sources on particulate matter and emphasize the need to strengthen control measures for springtime burning of crop residues in the future.
Session Chair(s): Chen SCHWARTZ, Centre for Climate Research Singapore, Kei YOSHIMURA, The University of Tokyo
AS43-A026
| Invited
Introduction to the SNAPSI Project: Quantification of the Stratospheric Contribution to Surface Predictability
Hera KIM1#+, Seok-Woo SON1, Amy BUTLER2, Chaim GARFINKEL3, Peter HITCHCOCK4
1Seoul National University, 2National Oceanic and Atmospheric Administration, 3Hebrew University of Jerusalem, 4Cornell University
This presentation introduces the SNAPSI project, which stands for Stratospheric Nudging And Predictable Surface Impacts (Hitchcock et al. 2022, GMD). The project aims to examine the prediction skills associated with stratosphere-troposphere coupling on subseasonal-to-seasonal (S2S) timescales. Specifically, we investigate the impact of nudging the stratosphere on S2S prediction skill during three recent sudden stratospheric warming (SSW) events using thirteen S2S-prediction models. Although there is dependence on the case, the models demonstrate a significant sensitivity of tropospheric predictability to the stratosphere. For example, the SSW downward impacts are better predicted with stratospheric nudging during the 2018 SSW in the northern hemisphere (NH) and the 2019 SSW in the southern hemisphere. The prediction skills following the 2019 SSW in the NH are marginally affected by the nudging, but this is because the models already captured the SSW anomalies without the nudging. These results suggest that improved prediction of stratospheric mean states may enhance surface predictability with an extended lead time of several weeks. The SNAPSI project also includes working groups focusing on stratosphere-troposphere upward/downward coupling mechanisms, stratospheric impacts on surface extremes and on the tropical convections, and their relation to the QBO.
AS43-A015
Stratospheric Influences on Tropical Convection: Insights from SNAPSI Experiment
Shunsuke NOGUCHI1#+, Members of SNAPSI WG62
1Kyushu University, 2SNAP
Recently, it has been suggested that anomalies in the lower stratosphere, formed in association with sudden stratospheric warming (SSW), impact subsequent tropical convection patterns. If this process is proven to be as robust as the downward influence from the stratosphere to the troposphere in mid-latitudes, there is significant potential for sophisticated forecasting of high-interest phenomena, such as the genesis and intensification of tropical cyclones, on the sub-seasonal to seasonal timescales. However, our understanding of the effects of this downward coupling process in the tropics remains incomplete. This is partly because this coupling manifests through processes, like cumulus convections, which are still represented with uncertainty in current numerical weather prediction models. The SNAPSI (Stratospheric Nudging And Predictable Surface Impacts) project is designed to elucidate the downward influence from the stratosphere through ensemble prediction experiments utilizing nudging (partial circulation constraint) techniques. This initiative aims to compare results from multiple models. Focusing on three SSW events in both hemispheres in recent years, roughly a dozen models have participated in this intercomparison project so far. In addition to several working groups that are already in progress, a new working group has been established to investigate the impact of SSW on tropical convective activities. This presentation will report on the initial results of the analysis being conducted with the goal of capturing the process mentioned above. In all models examined, a general enhancement of convective activity during SSW was confirmed, like the results obtained from the previous nudging experiments conducted with a single model. However, it has been also found that the intensity and pattern of the convective enhancement vary across models. Efforts are currently underway to identify the factors contributing to these differences among the models.
AS43-A012
Evaluating Real-time Subseasonal to Seasonal Tropical Cyclone Prediction
Xiaochun WANG1#+, Frederic VITART 2
1Nanjing University of Information Science & Technology, 2European Center for Medium-Range Weather Forecasts
The real-time WWRP/WCRP Subseasonal to Seasonal (S2S) Prediction Project Phase 2 database was used to evaluate the prediction skill of tropical cyclone from eleven forecasting systems for the North Western Pacific. The variable introduced to evaluate S2S tropical cyclone prediction is daily tropical cyclone probability, which is the occurrence probability of tropical cyclone within 500 km in one day. Using such a definition, the occurrence of tropical cyclone is a dichotomous event. The skill of S2S tropical cyclone prediction can be evaluated using debiased Brier Skill Score, which is the traditional Brier Skill Score with impact of forecast ensemble size removed. Sensitivity tests were conducted to analyze the influence of difference in temporal window and radius in the definition of daily tropical cyclone probability. It is demonstrated that though the daily tropical cyclone probability would vary with a changed radius and temporal window, the debiased Briere Skill Score does not change much since it is related with the ratio of mean error of model forecast and the mean error of a reference climatological forecast. The robustness of the prediction skill indicates the suitability of using the daily tropical cyclone probability and debiased Brier Skill Score to measure tropical cyclone prediction skill at S2S timescale. Compared with the prediction skill of the S2S Prediction Project Phase 1, the real-time S2S tropical cyclone prediction is improved for some forecast systems. Some early results by combining multi-model tropical cyclone forecasts to improve tropical cyclone prediction will also be presented.
AS43-A021
Tropical Cyclone Activities Over the Western North Pacific in Subseasonal Forecast of GloSea6
Eunji KIM+, Taehyung KIM, Dong-Hyun CHA#
Ulsan National Institute of Science and Technology
This study investigated the subseasonal predictability of tropical cyclone (TC) activities based on 24-year (1993-2016) ensemble (21 members) hindcasts of the Global Seasonal Forecast System version 6 (GloSea6) over the western North Pacific (WNP) region from June to September. We analyzed TC activities using three genesis potential index (GPI) developed by Emanuel and Nolan (ENGPI), Murakami et al. (MGPI), and Wang and Murakami (DGPI), respectively, and two tracking algorithms (i.e., TempestExtremes (TE) and direct tracking method of Cha et al. (DT)). Compared to Joint Typhoon Warning Center (JTWC) best track data, these five methods captured TC genesis points well and showed high correlation in TC genesis density correlation map. However, especially in the Philippine Sea, GPIs had a low correlation, while the tracking algorithms had a high correlation in that region. Overall, DGPI had reliable predictability for the TC core region and the mean monthly TC genesis number. In addition, we analyzed TC categories with tracking algorithms and found that GloSea6 did not simulate TCs of category TY (i.e., > 33 m s-1) well. Also, we examined El Niño-Southern Oscillation (ENSO) years and TC peak, low, and normal years.
AS43-A019
Evaluation of Multi-scale Ocean-atmosphere Coupled Modelling System
Yun-Chuan SHAO1#+, Hsi-Hsien TSENG1, Yu-Heng TSENG1, Jian-He CHEN2
1National Taiwan University, 2Central Weather Administration
A novel Multi-scale Ocean and Atmosphere Coupled Modeling System (MUSOACS) has been recently developed to enhance the predictability of extended-range forecasts at the Central Weather Administration in Taiwan. MUSOACS comprises four distinct components, seamlessly integrating global (23km resolution) and regional (5km resolution) ocean-atmosphere coupled models that run concurrently. The regional coupled model is online-driven by the global coupled model. Skill evaluations of the model predictability indicate that the global atmospheric forecast in MUSOACS surpasses the operational atmospheric forecast system at CWA up to 16 days in geopotential height, temperature, and wind vector below 200 hPa height. The predictability of the Madden Julian Oscillation, measured by the RMM index, extends from a 6-day to 20-day lead time. Furthermore, the regional prediction of the 2016/2018 cold surge events in the East Asian notably improves, extending the predictability lead time from 5 to 7 days in the Regional model compartment of MUSOACS. These improvements highlight the superior performance of MUSOACS compared to uncoupled models, attributed to its enhanced simulation of ocean-atmosphere interaction. These finding suggest that MUSOACS holds promising potential to deliver higher-quality extended-range forecast from both global and regional perspectives.
AS43-A011
Hypothesis Testing for Performance Evaluation of Probabilistic Seasonal Rainfall Forecasts
Ke-Sheng CHENG#+
National Taiwan University
Rainfall forecast plays an essential role in natural disaster prevention and mitigation. In contrast to natural disaster prevention and mitigation, for which responsive actions are taken immediately before or after issuing the forecast, tasks like water resources planning and disaster management often need to make decisions several weeks or months in advance. For example, information about seasonal rainfall over the crop-growing season is crucial for irrigation decision-making. Seasonal forecasts are probabilistic in nature. Probabilistic seasonal rainfall forecasting (PSRF) provides a range of plausible forecast results, which allows the forecaster to assess possible outcomes, and estimate the risks and probabilities of those outcomes. Most existing measures for performance assessment of probabilistic forecast systems are either qualitative or cannot make a clear decision about the appropriateness of the forecasts. In this study, we proposed a nonparametric goodness-of-fit test approach based on the Kolmogorov-Smirnov (KS) statistic for the performance evaluation of PSRF. The approach can provide valuable insights into the characteristics (underconfident, overconfident, mean underestimated, mean overestimated) of the PSRF results. We will demonstrate the proposed approach by using PSRF results in northern Taiwan for different seasons.
AS43-A004
Uncertainty in Soil Moisture-precipitation Feedback in Subseasonal Prediction of Rainy Season Development Over Indochina
Mien-Tze KUEH#+, Chuan-Yao LIN
Academia Sinica
The transition to the rainy season in the Indochina Peninsula typically takes place in May, revealing a negative correlation between near-surface temperature and precipitation. This transition signifies the development of the southwest monsoon flow. Skillful subseasonal prediction of the rainy season is crucial to the preparation of the agricultural practices in the region. The real-time forecasts from the ECMWF subseasonal-to-seasonal (S2S) forecasting system provide reasonable week-2 and week-3 predictions of the near-surface temperature tendencies. However, the predictions for the variation in rainfall are unsatisfactory. We find that the local thermodynamic responses in the prediction system may provide hints for the prediction performance. Over the region, the soil moisture increases with the rainfall in the preceding week. The consistency of the relationship between rainfall and preceding soil moisture levels is variable. In contrast to the increase in rainfall corresponding to rising soil moisture levels over plains, such a correlation does not hold true for highlands, where soil moisture increase does not consistently lead to a subsequent rise in rainfall. The surface latent heat flux increases with preceding soil moisture levels over plains, while it shows no sensitivity to soil moisture levels over highlands. The surface sensible heat flux, soil temperature, and near-surface temperature exhibit a negative correlation with preceding soil moisture levels. We speculate that these highlands transition toward an energy-limited regime during the rainy season. A comparison between a dry and hot year and a wet and cool year is ongoing. We will discuss the impact of the distinct monsoon developments on local thermodynamic responses in the conference.
AS43-A006
Application of Sub-seasonal Climate Forecasts for Global Solar Photovoltaic Power Generation
Jung CHOI#+, Seok-Woo SON
Seoul National University
Solar power plants have recently become widespread worldwide for their climate change mitigation benefits. As with other renewable energy sources, solar photovoltaic (PV) energy is highly dependent on weather conditions, and presents a significant challenge compared to conventional fossil fuel-based energy sources. This study discusses the usefulness of sub-seasonal climate forecasts for predicting solar power generation. We evaluate the accuracy of the solar PV potential obtained from atmospheric reanalysis data by comparing it with the observed solar PV power generation in Korea. The same methodology is applied to the global solar PV potential and its forecasts using the UK Met Office seasonal prediction system (GloSea6) for the period of 2016-2022. The results show that the solar PV potential derived from meteorological variables is a reliable metric for estimating solar power generation. Moreover, GloSea6 shows a skillful prediction of solar PV potential for one week in advance. The skill scores vary widely across regions at extended lead times, with some specific regions (e.g., South Asia) maintaining significant skill scores for about 5-8 forecast lead weeks. This result suggests that the current sub-seasonal climate forecasts can provide valuable information to support solar farm management, and highlights the importance of transdisciplinary approach between the solar energy sector and the meteorological research community.
Session Chair(s): Daehyun KIM, Seoul National University
AS05-A018
New Perspectives on Initiation of the Madden-Julian Oscillation Over the Indian Ocean
Xianan JIANG1#+, Junyi XIU2, Renhe ZHANG2
1University of California, Los Angeles, 2Fudan University
Due to significant influences of the Madden-Julian Oscillation (MJO) on global weather and climate extremes, a better understanding of the MJO initiation processes is crucial for improved subseasonal-to-seasonal prediction skill. In this presentation, new perspectives on MJO initiation over the western equatorial Indian Ocean will be discussed. We first demonstrate that initiation of MJO convection over the western Indian Ocean can be triggered by a fast eastward propagating intraseasonal mode, which exhibits widespread signals in both tropics and extratropics with a global wavenumber-1 structure in surface pressure field and a near-constant phase speed of about 10 deg day-1. It is shown that after triggering an enhanced MJO convection over the western Indian Ocean, this fast intraseasonal mode tends to further penetrate suppressed MJO convection near the central Pacific during its eastward propagation. This result suggests that the MJO could be a regional mode confined over the Indo-Pacific region, instead of a globally-navigating mode along the equator. In the second part of this presentation, while the extratropical origin of MJO initiation has been previously proposed based on case studies, we illustrate that MJO initiation over the Indian Ocean can be closely linked to the subseasonal variability of the East Asian Winter Monsoon (EAWM), induced by the quasi-geostrophic anomalous ascending motion associated with a cyclonic Rossby-wave gyre over the northern India Ocean as a part of a circumglobal Rossby wave-train along the subtropical westerly jet. Despite the close association between the MJO activity and the subseasonal variability of EAWM, our analysis suggests a minor role of the MJO for the subseasonal EAWM precipitation, which contradicts many previous studies.
AS05-A010
Diverse MJO Initiation and Propagation: The Crucial Role of Atmospheric Westward-propagating Disturbances
Yuntao WEI1#+, Hong-Li REN2,3, Baoqiang XIANG4,5
1Fudan University, 2Chinese Academy of Meteorological Sciences, 3China University of Geosciences, 4University Corporation for Atmospheric Research, 5NOAA Geophysical Fluid Dynamics Laboratory
Understanding the underlying mechanisms of convective initiation and propagation of Madden-Julian Oscillation (MJO) is important for the subseasonal-to-seasonal prediction. Using the clustering analysis method, we detect a new primary-type MJO onset, in which the preconditioning of WPDs from the central Pacific contributes roughly 60% of the large-scale MJO moisture accumulation over the Indian Ocean. These WPDs can be observed approximately forty days before the MJO onset and thus increase the predictability (~24 days) of primary MJO events by one week, compared to those (~17 days) without WPD precursor signals. This suggests that capturing WPDs in forecasting models might help implement a skillful week 3–4 prediction. In addition, this new type of primary MJO event mostly occurs during boreal summer and a Central Pacific (CP)-type La Nina background. Using global satellite observations and reanalysis data, we unravel that a dual combination of strong/weak WPDs and strong/weak EPDs can shape diverse MJO propagations documented previously using clustering analysis. The dry WPD signals from the CP strengthen the leading suppressed convection over the Western Pacific (WP) and, on the contrary, weaken the moist EPD convection over the Maritime Continent. Thus, when EPD is weak over the WP, the strong (weak) dryness of WPD likely causes a jump-like (stand-like) MJO mode. In contrast, a propagating MJO is supported when EPD becomes strong over the WP, and a further strengthening of the WPD dryness will presumably accelerate MJO; moreover, a weakening of WPD might slow down the MJO speed. These results highlight that the WPDs and their triggering place, i.e., the CP, might serve as key ingredients for better understanding the MJO dynamics and predictability.
AS05-A016
Recent Shift in 2011 of the Winter Madden-Julian Oscillation and Its Associated Changes in Mean State Over Warm Pool
Huang-Hsiung HSU1#+, Wan-Ling TSENG2, Yi-Chi WANG1, Li-Chiang JIANG1, Shu-Hsuan LIN1
1Academia Sinica, 2National Taiwan University
This study detected the regime shift of the wintertime MJO in 2011 and connected the changes in MJO variance to the mean states. Our findings indicated weakened MJO activity over the Indian Ocean and strengthened activity over the western MC, eastern MC, and western Pacific. Over the Indian Ocean, increased descending motion in the mean state suppressed the development of MJO convection and led to the export of moist static energy (MSE) through horizontal advection. Subsequently, the MJO became more active in the MC region due to enhanced import of MSE from both horizontal and vertical advection processes in the western and eastern MC, respectively. Ultimately, the MJO remained more active in the western Pacific due to strong boundary layer convergence and increased moisture. Our study highlighted the role of the mean state in driving the shift in the MJO, with various mechanisms at play. These findings underscore the need for further discussion and investigation into the complex regional characteristics associated with decadal changes in the MJO.
AS05-A012
MJO and High-frequency Convective Activities
Tetsuo NAKAZAWA#+
Japan Science and Technology Agency
The temporal and spatial characteristics of Madden Julian Oscillation (MJO) are not uniform; the MJO signal is sometimes weak, and it is not easy to see its existence. Such characteristic makes us difficult to understand the mechanism of MJO. At the last spring meeting, I first picked up the “top five largest” MJO cases by selecting the large amplitudes of the multivariate MJO index; RMM1 and RMM2, which is similar as the one by Wheeler and Hendon, 2004.One of the final goals of this study is to investigate what determines the amplitude of MJO, but in this presentation, I would like to see one of the MJO activity indexes, by a Space-time Spectral Analysis, using the Maximum Entropy Method (MEM) by Hayashi (1977) and its relationship with high-frequency convective activity, with the period of less than 20 days. One of the previous related studies is done by Nakazawa (1988). We have examined the linkage between the MJO and short-period convective fluctuations, including Kelvin wave, Mixed Rossby gravity (MRG) wave, n=1 Equatorial Rossby(ER) wave, and n=0 eastward intertia gravity(EIG) wave, etc. The result shows that climatologically the equatorial MJO (symmetric along the equator) is strongly linked with Kelvin wave and n=1 ER in April, and the asymmetric MJO in June is linked with MRG and n=0 EIG.
AS05-A013
Causal Relations Between Intraseasonal Oscillations and Tropical Cyclones in Western North Pacific
Chung-Hsiung SUI1#+, Jian-Hung LIAO1, Jau-Ming CHEN2, Hsu-Feng TENG1
1National Taiwan University, 2National Kaohsiung University of Science and Technology
Since intraseasonal oscillations (ISO) in boreal summer (BSISO) exhibit both eastward and northward propagation, the convection-coupled low-level cyclonic and upper-level divergent circulation in BSISO results in a more favorable environment for Tropical Cyclonic (TC) Genesis (TCG). We are interested in TCGs that occur frequently within one to two weeks (referred to as "TCG clustering here) and sporadically at other times. We calculated the TCG number in 10 days during the warm season (July-October) in WNP from 1991 to 2021. The frequency counts of the 0-5 TCG/10days are 58, 98, 82, 50, 31, and 4. By defining 4-5TCG/10days as clustering events, we analyzed the large-scale environment (ENSO, BSISO, and QBWO) associated with the 35 TCG clustering events (TCGc) and 58 events of no TCG (nTCG). TCG clustering events tend to occur in cyclonic low-frequency (LF) phase and BSISO convective phases (phase 6-8) in WNP, and no TCG events tend to occur in anti-cyclonic low-frequency phase and BSISO suppressed phases (phase 2-4) in WNP. Assuming the 323 10-day periods independent, the results are summarize as below: 1) Prob(TCGc) ~10% (35/323), Prob(nTCG) ~18% (58/323); 2) 70% TCGc events (25/35) and 40% nTCG events (25/58) can be attributed to large-scale background; 3) For TCGc, LF+ISO favor TCGc through combined heating and enhanced QBWOs (ISO A). Active QBWOs in return enhance ISO (ISO B); 4) For nTCG, LF+ISO suppress TCG and the TC feedback is weak. The negative influence of large-scale environment is not as effective as the positive influence of large-scale environment on TCGc events. While BSISO may influence TCG clustering that, in return, may also exert up-scale influences on BSISO. To address the feedback issue, we have identified all significant BSISOs to further investigate possible causal relations between TCG and BSISOs.
AS05-A005
Contributions of Air-sea Coupling to Northward-propagating Intraseasonal Convection Over the South China Sea
Yingxia GAO#+
Inner Mongolia University
Northward-propagating convection associated with intraseasonal oscillation (ISO) over the South China Sea (SCS) is closely linked to the evolution of the East China rainy season. In this study, we quantitatively examined the contribution of air-sea coupling to northward propagation of intraseasonal convection over the SCS based on observational diagnosis and model experiments. While oceanic feedback plays a limited role in northward propagation of Indian Ocean and western Pacific ISO, its positive effect on SCS ISO propagation is much larger and nearly comparable with that of atmospheric internal dynamics over the central SCS. Warm intraseasonal sea-surface temperature (SST) anomalies ahead of the convection induce boundary-layer convergence and surface turbulent fluxes, largely favoring growth of moist static energy to the north of the ISO convection. Conversely, weak negative SST anomalies induce divergence and reduced fluxes over the convective center. The underlying SST anomalies strongly promote northward propagation of SCS ISO, but destroy the maintenance of deep convection. We then verified these oceanic feedbacks using atmosphere-only (SPA) and atmosphere–ocean-mixed-layer coupled (SPK) configurations of the Super-Parameterized Community Atmospheric Model (SPCAM3). The SPA simulations produced stronger intraseasonal convection but weaker propagation signals than the SPK simulations, confirming the positive contribution of intraseasonal SST to ISO propagation observed over the SCS.
AS05-A003
Changes in Boreal Summer Intraseasonal Oscillation Under Global Warming in CMIP6 Models
Chaoxia YUAN#+, Zhefang GAO
Nanjing University of Information Science & Technology
Changes in the boreal summer intraseasonal oscillation (BSISO) activities at the end of 21st century under the SSP5-8.5 scenario are assessed here by adopting 17 CMIP6 models and the weak-temperature-gradient assumption. Results show that the intraseasonal variations become more structured. The BSISO precipitation anomaly shows a larger zonal scale and propagates further northward. However, there has no broad agreement among models on the changes in the eastward and northward propagation speeds and the frequency of individual phases. In the western North Pacific (WNP), the BSISO precipitation variance is significantly increased at 4.62% K-1 due to the significantly increased efficiency of vertical moisture transport by per unit BSISO apparent heating. The vertical velocity variance is significantly decreased at -3.51% K-1 in the middle troposphere due to the significantly increased mean-state static stability. Changes in the lower-level zonal wind variance are relatively complex with a significant increase stretching from northwestern to southeastern WNP but the opposite in other regions. This is probably due to the combined impacts of northeastward shift of the BSISO signals and the reduced BSISO vertical velocity variance under global warming. Changes in strong and normal BSISO events in the WNP are also compared. They show same-signed changes in precipitation and large scale circulation anomalies but opposite changes in the vertical velocity anomalies. This is probably because the precipitation anomaly of strong/normal events changes at a rate much larger/smaller than that of the mean-state static stability, causing enhanced/reduced vertical motion.
Session Chair(s): Peiqiang XU, Chinese Academy of Sciences
AS35-A045
| Invited
Relating the Properties of Quasi-stationary Rossby Waves to Jet Latitude and Strength
John METHVEN#+, Thomas FRAME
University of Reading
In recent decades, western Europe has seen a number of extreme seasons. For example, anomalously high precipitation totals for the summers of 2007 and 2012 as well as the exceptionally high temperature of summer 2003 and the coldness of winter 2009/10. One common feature in all these examples is the existence of persistent, near stationary Rossby wave patterns on the tropopause. Here a rigorous framework is used to extract these "slow modes of variability" from data in such a way that each mode has an intrinsic phase speed related only to its spatial structure, in a similar way that a bell rings with a characteristic note. We address how these slow modes of variability relate to the structure of the background state jet that they live on. Idealised experiments using a global primitive equation model are constructed where the only forcing is a weak relaxation to a zonally symmetric balanced background state. The jet is baroclinically unstable, so wave activity is sustained through repeated growth of baroclinic waves and their nonlinear life cycles. Modes of variability in the perturbations are extracted from global data using the empirical normal mode (ENM) technique. This amounts to EOF analysis using pseudomomentum (wave activity) as the norm. For a linear system the ENMs would equal the dynamical normal modes since they are also orthogonal under this norm. Although the system is nonlinear, only a few ENMs dominate the variability and the ratio of pseudoenergy to pseudomomentum yields a unique phase speed for each. It is shown how the properties of the dominant modes depend on the quasi-equilibrium background state jet strength and latitude. In this way seasons with anomalously persistent mid-latitude Rossby wave activity may be related to the interannual variability in the background state zonal flow.
AS35-A038
| Invited
Atlantic Multidecadal Oscillation Modulates the Diversity of the Winter Arctic Oscillation Pattern
Hainan GONG#+
Chinese Academy of Sciences
The nonstationary nature of the winter Arctic Oscillation (AO) pattern, especially for its Pacific center, can lead to significant and sometimes unexpected shifts in the influences of AO on regional weather and climate patterns, particularly in western North America and East Asia. Understanding the drivers and mechanisms behind the AO's spatial nonstationarity is crucial for improving climate predictions and projections associated with AO. Here we present evidence that the Atlantic Multidecadal Oscillation (AMO) plays a critical role in modulating the AO's Pacific center over recent decades. A poleward amplified cooling pattern associated with negative AMO phase enhances the north-south temperature gradient, resulting a strengthened polar jet stream and stratospheric polar vortex (SPV) which induces more planetary waves to reflect from the North Pacific to the North Atlantic. This dynamical process enhances the atmospheric coupling between these two regions, contributing to greater North Pacific variability involved in the AO variability and a more pronounced North Pacific center in the AO pattern. Numerical simulations further support the conclusions. Our findings not only deepen our understanding of the AO's behavior, but also have implications for future projections of AO-related regional climate changes.
AS35-A013
Causality Between the Kuroshio and Gulf Stream SST Variability
Yoko YAMAGAMI1#+, Hiroaki TATEBE1, Tsubasa KOHYAMA2, Shoichiro KIDO1, Satoru OKAJIMA3
1Japan Agency for Marine-Earth Science and Technology, 2Ochanomizu University, 3The University of Tokyo
Low-frequency sea surface temperature (SST) variability in the Kuroshio and Gulf Stream regions has been examined in the context of basin-scale SST phenomena, such as the Pacific Decadal Oscillation and Atlantic Multidecadal Variability, respectively. However, the covariability and causality between Kuroshio and Gulf Stream SSTs remain unclear. Therefore, this study investigates the causality of low-frequency variations in Kuroshio and Gulf Stream SSTs, focusing on the atmospheric circulation anomalies that link SST variability in these two basins. In this study, we conducted idealized model experiments utilizing pre-industrial control of a coupled model, MIROC6, with two different configurations, i.e. non-eddying and eddy-permitting in the ocean model, with pacemaking North Pacific or North Atlantic SST variations. Our analysis reveals that Gulf Stream SST leads to low-frequency Kuroshio SST variations, while the Kuroshio forcing is rather moderate. Consistent with the control experiment, the synchronization of Kuroshio and Gulf Stream SSTs is identified as the leading SVD mode only for the North Atlantic pacemaker with the eddy-permitting model. Furthermore, the mechanisms through which Gulf Stream influences Kuroshio are investigated. Regression analysis indicates that Gulf Stream SST leads to Northern Annular Mode (NAM)-like atmospheric anomalies during winter. Consequently, anticyclonic anomalies in the North Pacific induce oceanic Rossby waves in the Kuroshio Extension. The inability of the non-eddying model to reproduce the causality between Gulf Stream and Kuroshio SSTs can be attributed to the following two factors: (1) a weak NAM-like atmospheric response possibly due to a smaller meridional SST gradient in the North Atlantic compared to the eddy-permitting model and (2) unclear westward oceanic Rossby wave propagations along the Kuroshio Extension jet likely due to the coarse horizontal resolution. The above findings are supported by additional sensitivity experiments that highlight the role of SST in the mid-latitude ocean based on both coupled and atmospheric models.
AS35-A007
Linkages Between Amplified Quasi-stationary Waves and Humid Heat Extremes in Northern Hemisphere Midlatitudes in a Warming World
Jiacan YUAN#+
Fudan University
Humid heat extremes, taking account of both temperature and humidity, have adverse impacts on society, particularly on human health. It has been suggested that quasi- stationary waves (QSWs) with anomalously high amplitudes contribute to the occurrence of near-surface precipitation extremes and temperature extremes in the mid-latitudes of Northern Hemisphere. While little attention is paid to the linkages between amplified QSWs and humid heat extremes. Here we identify amplified QSWs of zonal wavenumbers 5-7 (Wave 5-7) in summer months in a warming climate. These amplified QSWs show clear circum global wave patterns horizontally and nearly barotropic structure vertically. Linking amplified Wave 5-7 to wet-bulb temperature (WBT) extremes, we find that amplified QSWs preferentially induce prominently prolonged WBT extremes in specific regions: north-central North America for amplified Wave 5;western United States, south-central Asia, as well as eastern Asia for amplified Wave 6; western Europe and the Caspian Sea region for amplified Wave 7. Analyses of physical processes indicate that accompanied by the amplification of Wave 5-7, the changes in horizontal temperature advection, adiabatic heating, downward solar radiation, moisture transport and moisture flux convergence, and surface latent heat fluxes largely account for the increase in persistence of WBT extremes.
AS35-A022
Dynamics of the Summertime Waveguide Teleconnection Along the Eurasian Polar Front Jet and Its Change Under Global Warming
Saori SAKAI#+, Yu KOSAKA
The University of Tokyo
The polar front jet (PFJ) over the Eurasian sector is one of the key pathways through which teleconnections affect summer climate in East Asia. In this study, we examine dynamics of this summertime PFJ teleconnection and its changes under global warming by using the ERA5 reanalysis dataset and d4PDF large ensemble AGCM simulations. We extract this teleconnection through an EOF analysis for interannual variability of summer 250 hPa meridional wind anomalies over 50ºN – 80ºN, 0º – 150ºE. EOF1 and EOF2 represent zonally extending wavetrain patterns with orthogonal zonal phases. In ERA5, EOF1 and EOF2 are not well separated, and in d4PDF historical simulations, EOF1 and EOF2 are separated due to the large ensemble size but the fraction of variance is close (23.9% and 21.8%). Therefore we conclude that this teleconnection does not have a dominant zonal phase, unlike the other teleconnection along the subtropical Asian jet. We also found that the PFJ teleconnection arises as internal variability of the atmosphere. The teleconnection affects the development of the Okhotsk high, which brings cool summer to Japan. Through a comparison of d4PDF historical and global warming simulations, we found structural changes in the PFJ teleconnection. For example, the maximum of meridional wind anomalies shifts upperward and poleward due to the tropopause elevation and the change of PFJ axial latitude under global warming. Besides, we found that the teleconnection overall weakens in the troposphere in a warmer climate.
AS35-A011
Extreme Heat Event Over Northwest China Driven by Silk Road Pattern Teleconnection and Its Possible Mechanism
Jie ZHOU1#+, Haipeng YU2
1Lanzhou University, 2Chinese Academy of Sciences
Under the background of global warming, heat wave events have become significantly frequent and have received increasing attention. Northwest China is located in the drylands of central Eurasia, where the climate and ecological environment are more vulnerable to global warming than in other parts of the world. Over the past few decades, the frequency of heat waves in Northwest China has increased significantly, and its causes remain unclear. We found that the heat events in Northwest China were closely related to the Silk Road Pattern teleconnection (SRP), and the strongly positive phase of SRP frequently corresponded to the occurrence of heat waves. Furthermore, the wave source of SRP was determined by the Linear baroclinic model to be located in the North Atlantic Ocean. We then selected an extreme heat event over Northwest China in 2021 as a typical case to discuss the possible mechanism. The regressed circulation fields to daily SRP were highly consistent with the anomalies that occurred during July 9–22, 2021, indicating that the diurnal propagation of SRP modulated the circulation anomaly related to the heat wave event and that diabatic heating influenced by SRP was the primary factor to the thermal low over Northwest China. Diabatic heating was strengthened in the lower troposphere due to the enhancement of downward shortwave radiation and surface sensible heat flux accompanied by strong descending motions and cloud cover reduction by an SRP-guided anticyclone over Northwest China. This study enhances the understanding and certainty regarding large-scale circulation effects on local temperature anomalies in middle latitudes.
AS35-A018
The Diversity of the North Atlantic SST Tripole Pattern and Distinct Climate Influences
Shanshan FU+, Zhiwei ZHU#
Nanjing University of Information Science & Technology
As the dominant mode of spring sea surface temperature(SST) in the North Atlantic on interannual scale, the tripole SST anomalies have a significant affect on surface air temperature(SAT) in Northern Hemisphere. However, different types of the tripole pattern may have the distinct effect. In the present study, three types of tripole pattern are identified according to the SST anomalies intensity of each pole for the period 1961-2020. The climate impacts associated with three types of tripole pattern are marked different from the standard tripole pattern which not distinguishing types. The main processes leading to SAT anomalies vary by region. In years that the tropical pole stronger, there are significant SST and convection anomalies in tropical Indian Ocean and Pacific. The associated circulation anomalies cause the SAT increases in West Africa, Arabian Peninsula, Iranian Plateau and Indo-China Peninsula through anomalous southerly wind and increased shortwave radiation. In years that the mid-latitude pole stronger, the belt barotropic cyclone from Northeast Asia to mid-latitude Pacific is significantly enhanced, leading to the negative SAT anomalies in Northeast Asia. In years that the high-latitude pole stronger, the circulation anomalies are partial to locate at high-latitude. Affected by this, the SAT significantly increases in eastern Caspian Sea, which is contributed by both increased solar radiation and horizontal advection associated with anomalous southerlies. The results reveal the necessity of distinguishing the diversity of the North Atlantic SST tripole pattern in their impacts on climate variability.
Session Chair(s): Takatoshi SAKAZAKI, Kyoto University, S. K. DHAKA, University of Delhi
AS29-A030
| Invited
Obliquely Propagating Gravity Waves: Role in the Quasi-Biennial Oscillation Dynamics
Young-Ha KIM1#+, Georg VOELKER2, Gergely BÖLÖNI3, Günther ZÄNGL3, Ulrich ACHATZ2
1Seoul National University, 2Goethe University Frankfurt, 3Deutscher Wetterdienst
A Lagrangian ray-based parameterization of gravity waves (GWs), Multi-Scale Gravity Wave Model (MS-GWaM), has been developed to represent the transient GW dynamics in a realistic way. MS-GWaM is particularly useful to study 3-dimensional propagation of GWs and its effects in the middle atmosphere. This study investigates obliquely propagating GWs in the tropical stratosphere and their role in the dynamics of the quasi-biennial oscillation (QBO). MS-GWaM is implemented into the ICOsahedral Non-hydrostatic model (ICON) and coupled to the convective source as diagnosed by ICON's cumulus parameterization. A pair of experiments are conducted: one using MS-GWaM in the 3-dimensional framework (3d-Exp), and the other using a 1-dimensional (columnar) variant of MS-GWaM with the steady-state assumption (1d-Exp). The latter follows the usual approach of conventional GW parameterizations. In 3d-Exp, the oblique wave propagation is observed in the tropical stratosphere with large horizontal displacements for GWs that have horizontal wavelengths larger than ~300 km. Especially, a spectrum of GWs that are generated by tropical convection exhibit an equatorward propagation into the shear layer of the QBO. Such equatorward wave propagation is found during a particular phase of the QBO, when the easterly QBO jet is located in the middle stratosphere, but persistently for every QBO cycle throughout the simulation. These waves provide substantial westward-momentum forcing over the equator, significantly contributing to the descent of the easterly QBO phase. The effect of the 3-dimensional wave propagation on the mean flow of the tropical stratosphere is examined by comparing 3d-Exp to 1d-Exp. The result demonstrates that the momentum forcing due to the equatorward propagating GWs in 3d-Exp leads to a much faster and deeper penetration of the easterly QBO phase down to the lower stratosphere, compared to that in 1d-Exp. The implication of the result in QBO modeling is discussed.
AS29-A033
Relative Dynamical Importance of Primary and Secondary Gravity Waves
Alexander S. MEDVEDEV1#+, Gary KLAASSEN2, Erdal YIĞIT3
1Max Planck Institute for Solar System Research, 2York University, 3George Mason University
Gravity waves are generated at all altitudes in the atmosphere, but sources above the lower stratosphere are rarely considered by parameterizations employed in general circulation models. This study assesses the potential impact on the thermosphere produced by small-scale waves originating at different heights. Within the proposed numerical framework, wave sources are represented by wave momentum forcing, whose values are expressed relative to the forcing required to obtain typical wave spectra around the tropopause. Calculations demonstrate that the accumulation of wave momentum steeply drops with height as a consequence of decreasing density, even when the forcing is maintained at a uniform level throughout the middle atmosphere. With increasing altitude, vertically localized sources contribute progressively less. For gravity waves excited near the mesopause to produce an impact comparable with that by waves propagating from below, the forcing must be orders of magnitude stronger than in the troposphere. The estimated forcing of the so-called secondary harmonics by breaking primary waves is much weaker, such that the systematic dynamical effect of secondary waves in the thermosphere is negligible compared to that of the primary waves generated in the troposphere.
AS29-A008
In Situ Generation of Planetary Waves by the Zonally Asymmetric Gravity Wave Drag in the Mesosphere: A Revisit
Ji-Hee YOO+, Hye-Yeong CHUN#, In-Sun SONG
Yonsei University
Based on a general circulation model covering up to the lower thermosphere, called the System for Whole Atmosphere Dynamics Research (SWAD, Song 2023), this study revisits the previous study Holton (1984) who explored the in situ generation of planetary waves (PWs) by the longitudinally varying gravity wave (GW) drag in the mesosphere. To set the GW drag (GWD) as the only PW source while excluding other origins, an aqua planet is configured devoid of the major stationary PW sources. Another important in-situ source, barotropic/baroclinic instability, is restricted throughout the integration by establishing a stable yet realistic boreal winter zonal-mean atmosphere and nudging this state toward the zonal-mean field. This nudging approach efficiently constrains the desired zonal-mean flow, while allowing the wave component to evolve freely. Idealized GWD, shaped sinusoidal in longitude with 100 m/s/day maximum amplitude and zero zonal-mean, is directly introduced at 30–60°N and 50–70 km altitude. Nonzonal GWD generates PWs as a nonconservative source (Z') of the linearized disturbance quasi-geostrophic potential vorticity (q'). While Z' initially amplifies PWs through enhancing q' tendency, steady-state is achieved as the subsequent zonal advection of q' balances Z'. GWD-induced PWs have substantial geopotential height amplitude (500–700 m), slightly less than that of the upward-propagating PWs forced from the troposphere. Characteristics of PWs depend on the GWD configuration: I) PWs have zonal wavenumber (ZWN) equivalent to that of GWD, and II) their amplitude increases in proportion to the GWD asymmetries while III) decreases with ZWN unexpectedly. It arises from the phase difference between Z' and the zonal advection of q' decreasing with ZWN. These PWs deposit positive (negative) forcing of approximately 30 (5–10) m/s/day at their origin (during propagation) and exhibit interhemispheric propagation following westerlies extended into the Southern Hemisphere.
AS29-A021
A Study of Zonal Wavenumber 1 Rossby-gravity Wave Using Long-term Reanalysis Data for the Whole Neutral Atmosphere
Hiroto SEKIDO1#+, Kaoru SATO1, Haruka OKUI1, Dai KOSHIN2, Toshihiko HIROOKA3,4
1The University of Tokyo, 2NSF NCAR HAO, 3Kyushu University, 4Kyushu University
The dynamical characteristics of the zonal wavenumber 1 (s=1) Rossby-gravity wave are examined using recently available reanalysis data for the whole neutral atmosphere over 16 years. An isolated spectral peak that likely corresponds to the s=1 Rossby-gravity mode is detected at heights of and in the two-dimensional (zonal wavenumber-frequency) spectra. The period of the spectral peak is approximately 1.3 days. The s=1 Rossby-gravity wave is properly extracted using a band-pass filter after pre-whitening to remove the diurnal tide. The s=1 Rossby-gravity wave exhibits a characteristic seasonal variation: the amplitudes are largest in the winter hemisphere in the stratosphere and lower mesosphere and are enhanced in both the winter and summer hemispheres in the upper mesosphere. The details are examined in a strong case. The horizontal phase structure at each height is consistent with the normal mode theory. The vertical phase structure is approximately barotropic from the lower stratosphere to the upper mesosphere for 30N and 30S.
AS29-A017
Role of Equatorial Waves and Parameterized Gravity Waves in the QBO Period Change in a Future Climate Simulation
Hyun-Kyu LEE1+, Hye-Yeong CHUN1#, Jadwiga RICHTER2, Isla SIMPSON3, Rolando GARCIA3
1Yonsei University, 2NSF National Center for Atmospheric Research, 3National Center for Atmospheric Research
The role of the parameterized gravity waves and resolved waves in the quasi-biennial oscillation (QBO) period change in a future projection (2015–2100) under the SSP370 is examined using a high-vertical resolution version of the Community Earth System Model 2 (CESM2) and is compared with that in four CESM2 historical simulations (1979–2014). In the future simulation, the peak QBO amplitude is 26.0 m s−1, which is marginally weaker than that in historical simulations from 27.4 to 29.3 m s−1. However, the QBO period is 12 months in the late-future (2065–2100), which is significantly shorter than that in historical simulations from 23.5–30.9 months. The decrease in QBO period in the future is mainly attributed to increased parameterized gravity wave drag (GWD) and resolved wave forcing in the stratosphere. The primary contributor to the shortened QBO period is GWD. The parameterized convective gravity wave momentum flux at the source-level strengthens due to enhanced convective activity in the future simulation, causing strengthening stratospheric GWD. In the future simulation, a key contributor to the strengthening of eastward resolved wave forcing is the increasing Kelvin wave forcing, while changes in wave forcing by other equatorial planetary waves are minor. These increases in both parameterized GWD and Kelvin wave forcing contribute to the speeding up of the QBO period in the future climate.
AS29-A001
Role of the Middle Atmosphere in Climate (ROMIC): Scientific Highlights from a Research Program
Franz-Josef LUEBKEN#+
Leibniz-Institute of Atmospheric Physics
The German Federal Ministry of Education and Research (Bundesministerium für Bildung und Forschung, BMBF) has launched a research initiative in 2013/2014 called ROMIC (Role of the Middle Atmosphere in Climate). The second phase of this project extends until 2024. The aim of ROMIC is to improve our understanding of long term variations in the stratosphere, mesosphere, and lower thermosphere and to investigate their potential role for climate changes in the troposphere. This includes to study coupling mechanisms between various layers and the relative importance of anthropogenic and natural forcing, e. g., by the Sun. Scientists at a total of 13 research institutes in Germany are involved and cover a large range of experimental and theoretical topics relevant for ROMIC. Most projects are linked to international activities and cooperations. Some scientific highlights from the research projects within ROMIC will be presented. In more detail, we will present results from the TIMA project (Trends In the Middle Atmosphere) regarding the future development of noctilucent clouds. In particular, we will address the question, if these clouds will absorb a significant fraction of the solar radiation in a changing climate with increasing greenhouse gases.
AS29-A007
Recent Results from an International Project Called Interhemispheric Coupling Study by Observations and Modelling (ICSOM)
Kaoru SATO1#+, Masashi KOHMA1, Dai KOSHIN2, Haruka OKUI1, Shingo WATANABE3
1The University of Tokyo, 2NSF NCAR HAO, 3Japan Agency for Marine-Earth Science and Technology
Concept of and recent results from an international joint research project, entitled Interhemispheric Coupling Study by Observations and Modelling (ICSOM) are presented. In the late 2000s, an interesting form of interhemispheric coupling (IHC) was discovered: when warming occurs in the winter polar stratosphere, the upper mesosphere in the summer hemisphere also becomes warmer with a time lag of days. This IHC phenomenon is considered to be a coupling through processes in the middle atmosphere (i.e., stratosphere, mesosphere, and lower thermosphere). Several plausible mechanisms have been proposed so far, but they are still controversial. This is mainly because of the difficulty in observing and simulating gravity waves (GWs) at small scales, despite the important role they are known to play in middle atmosphere dynamics. In this project, by networking sparsely but globally distributed radars, mesospheric GWs have been simultaneously observed in seven boreal winters since 2015/16. We have succeeded in capturing five stratospheric sudden warming events and two polar vortex intensification events. This project also includes the development of a new data assimilation system to generate long-term reanalysis data for the whole middle atmosphere, and simulations by a state-of-the-art GW-permitting general circulation model using the reanalysis data as initial values. By analyzing data from these observations, data assimilation, and model simulation, comprehensive studies to investigate the mechanism of IHC are ongoing.
Session Chair(s): Yi WANG, The University of Iowa, Liangfu CHEN, Chinese Academy of Sciences
AS59-A037
| Invited
Monitoring Global PM2.5 and Chemical Composition and Assessing Their Impact on Public Health
Jing WEI1#, Zhanqing LI2,3, Sixuan LI3+
1Peking University, 2University of Maryland, 3Beijing Normal University
Here we employ machine/deep learning and big data techniques to retrieve global and regional (China and US) daily 1 km gapless PM2.5 concentrations, along with their major chemical components. This approach unveils spatiotemporal variability at an exceptionally detailed level, providing insights into air quality monitoring, climate change, and public health studies over the past two decades. Our findings indicate that in 2022, 96%, 82%, and 53% of Earth's populated areas experienced exposure to unhealthy air for at least one day, one week, and one month, respectively. Significantly divergent exposure risks and durations are evident among developed and developing countries, urban and rural areas, and different city zones. Distinct wave-like changes in air quality are observable globally before, during, and after the COVID-19 lockdowns, with corresponding fluctuations in mortality burdens associated with air pollution events. Anthropogenic impacts, both positive (e.g., emission control measures) and negative (pollutant emissions), contribute to these variations. Nature-induced air pollution episodes, such as biomass burning, are also uncovered. Furthermore, our study reveals that wildfire emissions disrupt trends in black carbon and PM2.5 mortality burdens across the US, garnering substantial public attention with coverage from over 60 media outlets, including CBS News, Yahoo News, The Hill, U.S. News, MSN News, and more.
AS59-A012
Sources Apportionment of Atmospheric Visibility in Central Taiwan
Jun Fa YEH+, Ta Chih HSIAO#, Chih Yu CHAN, Chun Chen LU
National Taiwan University
This study conducted long-term aerosol physical, chemical, and optical observations with high-temporal resolution to monitor the visibility variations in Taichung, Taiwan. Since the effect of relative humidity is often included in visual visibility observations, the ambient aerosol light extinction coefficient (bext, amb) was further estimated. Dispersion-normalized Positive Matrix Factorization (DN-PMF) was employed to mitigate meteorological influences for bext, amb source apportionment. Data encompassing particle size distributions (PSDs), gaseous pollutants, and bext, amb were integrated into the DN-PMF to apportion the contributions of atmospheric oxidation capacity (AOC) and bext, amb from different sources, which remains rare in recent studies. First, the results showed that the significant enhancement of secondary inorganic aerosols (SIA), high AOC, and relative humidity (RH) are associated with low visibility and severe PM pollution events. For PSDs, the maximum concentration amplification in the range of 300-1,000 nm confirmed that particles also tend to aggregate within the accumulation mode during event periods, which overlaps the range of visible light wavelength. Secondly, fresh traffic, traffic-related sources, aged traffic/industrial emissions, nitrate-rich secondary aerosols/combustion sources, ozone-related secondary aerosols, and contaminated marine aerosols were resolved in the DN-PMF. The concentration differences between PMF and DN-PMF revealed the corrective impact of DN-PMF on wind-induced concentration under or over-estimation compared to PMF. Finally, the DN-PMF results indicated that traffic and O3-associated secondary sources were the main contributors to AOC. Aged traffic, nitrate-rich secondary sources, and O3-associated secondary sources collectively contributed over 80% of bext, amb, and could correspond to the concentration enhancement in the range of 100-1,000 nm. The results suggest that controlling traffic and secondary sources may be the key to improving PM levels and visibility deterioration.
AS59-A019
Mapping the Seamless Hourly Surface Visibility in China: A Real-time Retrieval Framework Using a Machine-learning-based Stacked Ensemble Model
Xutao ZHANG1#+, Ke GUI1, Zhaoliang ZENG1, Ye FEI2, Lei LI1, Yu ZHENG1, Yue PENG1, Yurun LIU3, Nanxuan SHANG1, Hengheng ZHAO1, Wenrui YAO1, Hong WANG1, Zhili WANG1, Yaqiang WANG1, Huizheng CHE1, Xiaoye ZHANG1
1Chinese Academy of Meteorological Sciences, 2National Meteorological Information Center, 3Chengdu University of Information Technology
Surface visibility (SV), a key indicator of atmospheric transparency, is used widely in the fields of environmental monitoring, transportation, and aviation. However, the sparse distribution and limited number of SV monitoring sites make it difficult to fulfill the urgent need for spatiotemporally seamless fine-scale monitoring. Here, to the best of our knowledge, we developed the first operational real-time SV retrieval (RT-SVR) framework for China that incorporates information from multiple data sources, including Chinese Land Data Assimilation System meteorological data, in situ observations, and other ancillary data. Seamless hourly SV data with 6.25-km spatial resolution are available in real time via the operational RT-SVR model, which was built using a two-layer stacked ensemble approach that combines multiple machine learning algorithms and a deep learning module. Sample-based cross-validation of the RT-SVR model on approximately 41.3 million data pairs revealed strong robustness and high accuracy, with a Pearson correlation coefficient (R) value of 0.95 and a root mean square error (RMSE) of 3.17 km. An additional hindcast-validation experiment, performed with continuous observations obtained over one year (approximately 20.8 million data pairs), demonstrated the powerful generalization capabilities of the RT-SVR model, albeit with slight degradation in performance (R = 0.85, RMSE = 5.28 km). The seamless hourly SV data with real-time update capability enable tracking of the generation, development, and dissipation of various low-SV events (e.g., fog, haze, and dust storms) in China. The developed framework might also prove useful for quantitative retrieval of aerosol-related parameters (e.g., PM2.5, PM10, and aerosol optical depth).
AS59-A031
Elevated Particulate Nitrate and Nitrous Acid Observed Under High Humidity Conditions in Subtropical Urban Areas of East Asia
Hing Cho CHEUNG#+
Academia Sinica
An onsite measurement of the chemical composition of submicron (PM1) particulate matter and nitrous acid (HONO) was conducted at the Urban Air Pollution Research Station (UAPRS), which is located in the urban area of western Taiwan in East Asia during the spring (Mar-Apr) and autumn (Oct-Nov) of 2022. Nitrous acid is a major reservoir of hydroxyl radicals (OHs) during the nighttime and provides an important source of OH for the secondary formation of urban pollutants. In general, the average PM1 was found to be 23.7 mg m-3 during the sampling period while a higher PM1 of 53.8 mg m-3 was depicted during the PM1 episodes. Organic carbon and nitrate components were primary contributors to the chemical composition of PM1 which were 44% and 27%, respectively. However, the nitrate contribution increased to 35% which was the largest contributor to the PM1 episodes. It is noteworthy that a maximum of nitrate was observed in the early morning during PM1 episodes which is likely due to a reaction with OH radicals from the photolysis of HONO. For nitrous acid, the average concentration was 0.78 ppb which was higher in the nighttime. Diurnal variation of the HONO/NO2 ratio is an indicator of changes of vehicle and non-vehicle sources of HONO. A bell-shaped variation of HONO/NO2 was observed during the daytime which indicated that there were non-vehicle sources of HONO in the study region. In addition, higher nitrate and HONO concentrations were found under the high humidity conditions which could imply that the aqueous phase heterogenous formation of the particulate matter was one of the important pathways of haze pollution in the study region.
AS59-A004
Trace Elements in PM2.5 Aerosols in East Asian Outflow in the Spring of 2018: Emission, Transport, and Source Apportionment
Takuma MIYAKAWA1#+, Akinori ITO1, Chunmao ZHU1, Atsushi SHIMIZU2, Erika MATSUMOTO3, Yusuke MIZUNO3, Yugo KANAYA1
1Japan Agency for Marine-Earth Science and Technology, 2National Institute for Environmental Studies, 3HORIBA Ltd.
Trace metals in aerosol particles impact Earth's radiative budget, human health, and ocean biogeochemistry. Semi-continuous measurements of the elemental composition of fine-mode (PM2.5) aerosols were conducted using an automated X-ray fluorescence analyzer on a remote island of Japan during the spring of 2018. Temporal variations in mass concentrations of geochemically important elements for this period, such as Pb, Cu, Si, Fe, and Mn, and their relationships with the emission tracers, carbon monoxide (CO) and black carbon (BC), were reported. A global chemistry transport model (IMPACT) was used to evaluate the source apportionment of these components. Pb and Cu originated mainly from anthropogenic sources (98 % and 93 % on average, respectively) over the East Asian continent. Positive correlations of Pb and Cu with BC and CO and the similarity of their concentration-weighted trajectories indicated that the emission sources of these metals share the region where the large CO (and BC) emission sources are located and that CO can be regarded as a tracer of continental anthropogenic emissions. The air masses with minimized impacts of the wet removal during transport were extracted to elucidate the “top-down” emission ratio of Pb and Cu to CO, which were, for the first time, evaluated as 152.7 and 63.1 µg g−1, respectively, in the springtime East Asian outflow. The analysis of the tagged tracer simulations by the IMPACT model confirmed that BC and Si could be used as tracers for anthropogenic and dust emissions, respectively, during the observation period. The source apportionment of Fe and Mn in PM2.5 aerosols was conducted using Si and BC tracers, which revealed that the anthropogenic contribution was 17 % and 44 % on average, respectively. Based on the air mass origins of Fe and Mn, their anthropogenic fraction varied from 2 % to 29 % and 9 % to 68 %, respectively, during the high-PM2.5-concentration periods.
Session Chair(s): Hyo CHOI, Gangneung-Wonju National University
AS36-A017
Artificial Neural Network Modeling for Real-time Urban Air Pollution
Soo Min CHOI1+, Hyo CHOI2,3#
1Konkuk University, 2Gangneung-Wonju National University, 3Atmospheric and Oceanic Disaster Research Institute
Temporal assessment of urban air pollution associated with their remote inflow was analyzed using a machine learning technique as artificial neural network technique-hyperbolic tangent activation function (ANN-tanh). Using 15 input independent variables (3 hours' earlier PM, gas and meteorological data of the city influenced by 2 days' earlier PM and gas data of a Chinese city, Multilayer perception (MLP) with a back-propagation training algorithm for a feed-forward ANN technique was adopted to predict real-time urban air quality state in 13, 15, and 17 nodes in the hidden layer of the model. Root mean square error (RMSE) with the coefficient of determination (R2) evaluates the performance of the model between the predicted and measured values in 13 (15; 17) nodes in a single hidden layer in three different periods, such as before, during, and after the yellow sand event at the coastal cit. The importance of each independent variable to the dependent variables (PM10, PM2.5, NO2, and O3) in the model was summarized in detail. The closeness of the predicted values to the observed ones, regardless of hidden node numbers, shows a very high Pearson r correlation coefficient. Modeling performance was presented by scatter plots on the four variables and their hourly distributions.
AS36-A019
Source Apportionment and Ozone Formation Potential Analyses of VOCs in Urban Areas of North Texas
Jithin KANAYANKOTTUPOYIL, Kuruvilla JOHN#+
University of North Texas
An evaluation of measured concentrations of Volatile Organic Compounds (VOCs) in North Texas and their critical role in the formation of ozone in urban environments was conducted. A Concentration-Dispersion Normalized Positive Matrix Factorization (CDN-PMF) model was used to apportion sources of VOCs in urban areas close to unconventional shale oil and gas production activities within the Barnett Shale region. Air quality data from three monitoring sites operated by the Texas Commission on Environmental Quality (TCEQ) for an eight-year span from 2015 to 2022 were analyzed. The sites included Dallas Hinton (DAL) in Dallas County, a heavily urbanized area with minimal shale gas activity; Fort Worth Northwest (FWNW) in Tarrant County, a moderately urbanized area with significant shale gas activity; and Denton Airport South (DEN) in Denton County, an exurban region with very high shale gas activity. Source apportionment analysis showed distinct VOC sources at each site. DAL's primary sources were primarily mobile emissions (diesel: 25%, gasoline: 7%, aircraft: 13%) and emissions from oil and gas activities (31%). In FWNW, significant contributors were mobile sources (42%) and oil and gas activities (38%), while DEN was dominated by oil and gas emissions (72%). Considerable yearly variations in source contributions were noted, indicating the impact of unconventional oil and gas development on urban air quality. To understand the impact on ozone, Ozone Formation Potential (OFP) was calculated by organic species. At DAL and FWNW, alkenes were found to be the primary contributors to OFP, whereas in DEN, n-alkanes were predominant. Conditional Bivariate Probability Function (CBPF) analyses were used to characterize the spatio-temporal dynamics of VOC sources, highlighting the short-range transport from emissions-rich regions within the study domain. This study's findings are crucial for developing targeted air quality management strategies in ozone non-attainment areas like Dallas-Fort Worth.
AS36-A020
Advanced Machine Learning Approaches for Ozone Forecasting in Fort Worth, Texas
Jithin KANAYANKOTTUPOYIL, Kuruvilla JOHN#+
University of North Texas
This study presents a comprehensive analysis and forecasting of ozone concentrations at the Fort Worth Northwest (FWNW) site within Texas' Barnett Shale region, characterized by intensive oil and gas activities in close proximity to a major urban area of North Texas. The site has recorded ozone levels above the National Ambient Air Quality Standards (NAAQS) over the past two decades. Ozone forecasting is always challenging due to its nonlinear relationships with physical and chemical characteristics of the atmosphere. The focus of this study is to forecast hourly ozone concentrations using a dataset of observed meteorological variables and measured Total Non-Methane Organic Compounds (TNMOCs) concentrations from publicly available data. Advanced machine learning techniques were employed, involving a Random Forest (RF) model and a deep learning architecture featuring a Recurrent Neural Network (RNN) with Long Short-Term Memory (LSTM) units. The selection of input variables is based on a comprehensive correlation matrix analysis to ensure the relevance of each predictor. The RF model showed excellent training performance with an R2 of 0.97, indicating a strong fit to training data. However, its validation performance dropped to an R2 of 0.81, suggesting decreased accuracy on new data. The LSTM model, conversely, demonstrated more consistent performance, with R2 values of 0.84 on training and 0.85 on validation, indicating better generalization. Both models underwent extensive hyperparameter tuning for enhanced predictive accuracy and reliability. The results show a significant correlation between predicted and actual ozone levels, affirming the efficacy of combining RF and LSTM for environmental forecasting. This study not only contributes to air quality modeling methodologies but also offers vital insights for policy-making and public health in areas impacted by intensive oil and gas activities. It underscores the importance of integrating machine learning for precise and timely air quality forecasting from a sustainable urban development standpoint.
AS36-A021
Estimating the Refractivity Bias of FORMOSAT-7/COSMIC-II GNSS Radio Occultation in the Planetary Boundary Layer
Pham GIA HUAN#+
National Central University
FORMOSAT-7/COSMIC-2 radio occultation (RO) measurements are promising for observing the deep troposphere and providing critical information on the Earth's planetary boundary layer (PBL). However, refractivity retrieved in the low troposphere can have severe bias under certain thermodynamic conditions. This research examines the characteristics of bias in the low troposphere and presents methods for estimating the region-dependent bias using regression models. The results show that the bias has characteristics that vary with land and oceans. With substantial correlation between local spectral width (LSW) and bias, the LSW-based bias estimation model can explain the general pattern of the refractivity bias but with deficiencies in measuring the bias in the ducting regions and certain areas over land. The estimation model involving the relationship with temperature and specific humidity can capture the bias of large amplitude associated with ducting. Finally, a minimum variance estimation that combines the benefits of the individual estimation provides the most accurate estimation of the refractivity bias.
AS36-A029
Assessing the Agricultural Irrigation Effects on Summertime Soil Moisture and Near-surface Meteorology in California's Central Valley
Shu-Hua CHEN1#+, Yang YU1, Chu-Chun HUANG1, Cameron SCHMITT1, Kyaw Tha PAW U1, Kuang-Yu CHANG1, Zhan ZHAO2, Jeremy AVISE2, Chenxia CAI2, Min-Hui LO3
1University of California, Davis, 2California Air Resources Board, 3National Taiwan University
California's Central Valley (CV) is one of the most productive agricultural regions in the world, relying significantly on irrigation. This study explores the impacts of agricultural irrigation on soil moisture and surface meteorology in the CV throughout the 2020 irrigation season. Without the agricultural irrigation effect (WoIR), the Weather Research and Forecasting (WRF) model presents a dry surface soil moisture bias of 0.05 m3/m3 over the CV, compared against the observations from the Soil Moisture Active Passive (SMAP) satellite. After including the irrigation effect (WIR3D), WRF better reproduces the observed surface soil moisture in the CV. A comparison with observations from 35 automatic weather stations across the CV reveals that the mean bias of the simulated 2-m dew point is -1.63 ℃ in WoIR but is 0.04 ℃ in WIR3D. The 2-m temperature change due to irrigation could be cooling or warming over the CV. The complexity of the temperature change arises from the competition between evaporative cooling and greenhouse gas effects induced by irrigation-increased water vapor. Irrigation-increased water vapor also escapes to California's southwestern coast and warms up near-surface temperatures there through the greenhouse gas effect. Compared with planetary boundary layer height (PBLH) derived from Ceilometer aerosol backscatter profiles, the irrigation effect reduces the daytime positive PBLH bias in the model by approximately 800 m (53%), decreasing daily wind speed by 0.5 m/s. In addition, this study also conducts sensitivity experiments to examine the effects of irrigation frequency and irrigation spatial heterogeneity over the CV on PBLH, soil moisture, and near-surface meteorology.
Session Chair(s): Wen-Chau LEE, University Corporation for Atmospheric Research
AS76-A014
Radar Observation of Taipei Heavy Rain and Microburst
Ben Jong-Dao JOU1#+, Chi-Jun JUNG2, Kai-Hsiang YANG3, Yu-Cheng KAO4
1National Taiwan University, 2postdoctor, 3graduate student, 4research scientist
Severe convective storms have become increasingly frequent and intense in the Taipei metropolitan area. Heavy rainfalls and strong surface winds are often observed associated with the occurrence of these severe convective storms. In this presentation, complex thunderstorms in the Taipei Basin produced extreme rain rate leading to an urban flash flood and pronounced downdrafts leading to strong winds near the ground, i.e., the microburst are examined. For the heavy rain case, the storms’ microphysical and dynamic features during the organizing and heavy rain stages, based on observed polarimetric variables of Doppler radars are presented. Shallower isolated cells in the early afternoon characterized by big raindrops produced a rain rate > 10 mm/h, but the rain showers persisted for a short time. The heaviest rainfall, i.e., more than 60 mm within 20 min, occurred when convective cells merged. The columnar features of differential reflectivity (ZDR) and specific differential phase (KDP) became more evident in merged cells, which correlated with the broad distribution of upward motion and mixed-phase hydrometeors. The KDP below the environmental 0oC level increased toward the ground associated with the melted graupel and resulted in subsequent intense rainfalls showing the contribution of the ice-phase process. The related processes are potential for issuing flash flood alert. In Taipei, occurrence frequency of microburst accompanied with the severe afternoon thunderstorms is not clear. According to earlier studies, ~ 30-40% in Denver and 15-20% in Huntsville, Alabama region, severe convective storms are associated with divergent outflow stronger than 10 m/s threshold accompanied with microbursts near the ground. In this presentation, an afternoon thunderstorm associated with microburst in the Taipei basin is also examined. Pronounced descending precipitation cores, flow convergence in the cloud layer, and significant near-ground divergent outflows are major radar signatures obtained.
AS76-A038
Feedback from Polarimetric Radar for the Dynamics and Microphysics Under the Record-breaking Rainfall Environment on 20 July 2021 in Zhengzhou
Yabin GOU1#+, Haonan CHEN2
1Hangzhou Meteorological Observatory, 2Colorado State University
The precipitation microphysics and dynamics around the disastrous waterlogging area in Zhengzhou, China, which collected a record-breaking hourly rainfall of 201.9 mm on 20 July 2021, have been disentangled through the investigation based on disdrometer, gauge and polarimetric radar measurements, including radial velocity, the specific differential phase (KDP), attenuation-corrected reflectivity (ZH) and differential reflectivity (Zdr). The main findings demonstrate that: (i) The microphysical process featured with a coalescence-breakup balance is revealed in the low-level atmospheric layer, which exhibits increasing ZH and KDP but decreasing Zdr, in terms of their timeseries, scattergram, radial height indicator and vertical profiles of ZH, KDP and Zdr. (ii) The advection of large-sized raindrops upon the vertical wind shear (VWS) transition layer was accompanied by a raindrop recirculation process through a reverse advection toward the convergence line below the VWS transition layer. This dynamical process contributed to the highly concentrated liquid water content but decreasing raindrop size toward the surface around the disaster area, which inherently accounts for the vertical evolution tendency of three polarimetric radar variables below the VWS transition layer. (iii) Based on multi-source consistency between radar, disdrometer, and gauge measurements, the physical conversion from KDP to the equivalent radar measurements approximates the microphysical processes across the whole radar coverage to that occurred upon the disdrometer, which effectively mitigates the impacts of spatial variety of microphysical process and then helps to obtain comparable rainfall estimates based on different radar quantitative precipitation estimators.
AS76-A001
Improving Explainability of Deep Learning-based Radar QPE
Haonan CHEN#+
Colorado State University
Deep learning-based approaches have demonstrated great potential for radar-based quantitative precipitation estimation (QPE). In contrast with conventional parametric methods that depend on local raindrop size distributions, such as radar reflectivity (Z) and rainfall rate (R) relationships, a deep learning (DL) model can establish a functional relation between three-dimensional multi-parameter radar observations and surface rain rate measurements. However, the lack of transparency in DL models poses challenges toward understanding the underlying physical mechanisms that drive their outcomes. This obstacle hampers the practical implementation of DL-based QPE models. To address this issue, this research aims to develop a QPE system for polarimetric radar that offers a comprehensible explanation of its functionalities. This system is created by employing a deep neural network consisting of two main modules. The first module is designed to introduce a QPENet that is specifically tailored for polarimetric radar applications. The second module includes a QPESHAP explainability method for elucidating the factors that influence the model precipitation estimates across varying precipitation intensities. In addition, the study offers more accurate visual explanations by visualizing the interactions among the input radar variables. The experimental results showcase the favorable performance of QPENet across different rainfall intensities, with each observable exhibiting distinct effects in light, moderate, and heavy precipitation intensities. The findings derived from the QPESHAP analysis suggest that the DL model effectively captures the fundamental physics associated with precipitation data and radar measurements.
AS76-A011
Improvement of Estimating Orographically Induced Rainfall Intensity Using MP Radar Volume Scanning Observation and Concept of Seeder-Feeder Mechanism
Katsuya SATO1#+, Eiichi NAKAKITA1, Yohei NAKABUCHI2
1Kyoto University, 2East Japan Railway Company
In Japan, the steep terrains make the rain heavier, resulting in a phenomenon called orographic rainfall. One of the causes of this orographic rainfall is the Seeder-Feeder effect. In fact, during Typhoon No. 19 (Hagibis) in 2019, the rainfall observed by radar was a 30% underestimate compared to the rainfall observed on the ground. This is thought to be due to the cedar feeder effect that occurs near the ground. Accurately estimating ground rainfall is very important from a disaster prevention perspective. The purpose of this research is to improve the accuracy of estimating ground rainfall by improving a rainfall model that takes into account orographically rainfall. In this research, we propose a method of estimating the capture rate and ground rainfall intensity with higher accuracy using a polarimetric radar. Here, capture rate is defined as the rate at which raindrops from upper levels collect cloud particles in the lower layers. This kind of real-time estimation can be realized by estimation of raindrop size distribution using a volume scanning polarimetric radar. Also, estimating enhancement of rainfall intensity downwards from the radar observation layer is realized using the concept of the seeder-feeder mechanism. The effectiveness of preventing underestimation of ground rainfall estimation results by considering orographically rainfall due to the Seeder-Feeder effect was reconfirmed. Also, the method of estimating ground rainfall using real-time radar information was able to estimate rainfall with higher accuracy than radar estimated rainfall at higher level rainfall. Furthermore, when real-time radar information from multiple altitudes was used, rainfall could be estimated with higher accuracy than when only radar information from a single altitude was used. The above results demonstrate the effectiveness of the methods of estimating the capture rate using radar information and of estimating enhancement of downwards rainfall intensity is realized using the concept of the seeder-feeder mechanism.
AS76-A016
Improvement of Composite QPE Using Quality Index and Various Composite Methods from Multi-wavelength Radar Measurement
Daehyung LEE1+, Choeng-Lyong LEE1, Geunsu LYU1, Wonbae BANG1,2, Park HONG-MOK1, Alexander RYZHKOV3, Gyu Won LEE1#
1Kyungpook National University, 2Center for Atmospheric REmote sensing, Kyungpook National University, 3NOAA/OAR/National Severe Storms Laboratory
In Korea peninsula, dense radar networks have been established by the 3 agencies: The Korea Meteorological Administration (KMA), the Ministry of Environment (MOE), and the Republic of Korea Air Force (ROKAF) Additionally, several X-band radars were recently installed by KMA and MOE to observe the lower altitude areas and to update radar data rapidly. However, achieving a comprehensive radar composite is quite challenging due to the individual radar characteristics (location, beam width, attenuation, and beam blockage) and various operating strategies caused by agencies with distinct purposes. In the traditional composite methods, each radar data is interpolated to common grid and composited by weighing value. The weighting values usually consider the radar's range and height (nearest, lowest, distance weighted) or fixed to the same value (averaged). These types of composite methods can’t consider each radar characteristics. Therefore, we aim to improve S-band averaged radar composite by using multi-band radar and quality index in this study. The main components of quality indices consist of bandwidth, management status of radar, attenuation, and beam blockage. Additionally, range, height, non-meteorological echo also indirectly considered in quality control processes and composite methods. Hybrid Surface Rainfall (HSR) estimation results (R(ZH), R(ZH,ZDR), R(ZH,KDP), R(ZH,KDP_P) and R(ZH, AH)) using various composited methods (averaged, lowest, distance-weighted, maximum quality index) are compared with rain gauge data to validate the effects of multi-band radar and the quality index. Acknowledgment: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00237740.
AS76-A015
Investigating an Intense Coastal Rainfall Event During TAHOPE/PRECIP-IOP3 Using a Multiscale Radar Ensemble Data Assimilation System
Shu-Chih YANG1#+, Shu-Hua CHEN2, Lawrence Jing-Yueh LIU3,1, Hao-Lun YEH1, Wei-Yu CHANG1, Kaoshen CHUNG1, Pao-Liang CHANG4, Wen-Chau LEE5
1National Central University, 2University of California, Davis, 3University of Illinois Urbana-Champaign, 4Central Weather Bureau, 5University Corporation for Atmospheric Research
A multi-scale radar ensemble data assimilation system has been developed by applying the successive covariance localization (SCL) to the WRF-Radar LETKF assimilation system (WLRAS). The multi-scale WLRAS is applied to study a heavy rainfall event that occurred on 6-7 June 2022 during the IOP3 in the Taiwan-Area Heavy Rain Observation and Prediction Experiment (TAHOPE)/Prediction of Rainfall Extremes Campaign In the Pacific (PRECIP) field campaign. Two experiments were conducted and differed only in using the convective-scale (RDA) or multi-scale corrections (MRDA) in the assimilation of radar radial velocity. The objective of this study is twofold. One is to evaluate the benefit of using multi-scale WLRAS by comparing RDA and MRDA. The other is to understand the mechanisms of the convection development on the western coast of Taiwan as the mei-yu front hovers in northern Taiwan. Compared to RDA, the MRDA experiment exhibits large-area wind corrections, which help reshape and relocate a low-level meso-vortex offshore of western central Taiwan and enhance the frontal intensity offshore of northwestern Taiwan. Consequently, the MRDA improves the very short-term (6h) heavy rainfall prediction over the coast of western Taiwan and better represents the elongated rainband in northern Taiwan during the 3 to 6-h forecast hours. Sensitivity experiments demonstrate the importance of assimilating the radial wind of Chigu and S-Pol radars in establishing the low-level meso-vortex and convergence zones. Although updating the moisture variable with the SCL method positively impacts rainfall prediction, the moisture correction at far distances may be less reliable.
Session Chair(s): Nobuhiro TAKAHASHI, Nagoya University
AS80-A004
Improvement of Precipitation Tracking Algorithm for Global Satellite Mapping of Precipitation
Hitoshi HIROSE1#+, Kento YURA1, Munehisa YAMAMOTO2, Takuji KUBOTA2, Tomoo USHIO1
1Osaka University, 2Japan Aerospace Exploration Agency
Global Satellite Mapping of Precipitation (GSMaP) uses continuous observations from geostationary meteorological satellites (GEOs) to fill gaps in the passive microwave (PMW) satellites observation network. Precipitation is tracked by calculating cloud movement vectors. These cloud movement vectors were previously calculated every hour on a 2.5° grid, but with the improved temporal and spatial resolution of GEOs, they can now be calculated every 10 minutes on a 1.0° grid. The accuracy of the precipitation tracing algorithm in the east-west direction has been dramatically improved by using the high-resolution cloud movement vector. The cloud moving vector tends to be calculated along the direction of upper-level clouds movement. Therefore, it has been reported that the tracking accuracy of middle- or lower-level heavy precipitation is often degraded under a strong vertical wind shear such as in the tropics. Therefore, we tried to introduce the Forecast and Tracking the Evolution of Cloud Clusters technique (ForTraCC; Vila et al. 2008). Since the ForTraCC can track precipitation clusters directly, it is expected to track heavy precipitation from middle- or lower-level clouds without being affected by the movement of upper clouds. Experiments were conducted to correct the cloud moving vector by using the ForTraCC cluster moving vector. As a results, tracking accuracy was improved for middle or lower-level precipitating clouds in the tropics. The research is supported by a grant from the Japan Aerospace Exploration Agency (JAXA), and we would like to express our sincere gratitude for their financial support.
AS80-A002
Initial Validation of Polar Extension of GSMaP PMW-IR Combined Algorithm Using NEXRA Data
Munehisa YAMAMOTO1#+, Takuji KUBOTA1, Shuhei MATSUGISHI2
1Japan Aerospace Exploration Agency, 2The University of Tokyo
The Global Satellite Mapping of Precipitation (GSMaP) provides precipitation estimation by combining observations from multiple microwave radiometers (PMW) onboard low Earth orbit satellites and infrared radiometers (IR) onboard geostationary meteorological satellites. GSMaP product version 05 (algorithm version 8), released in December 2021 has achieved precipitation estimation up to the polar regions only in the PMW observation area. On the other hand, there are still missing areas where the PMW does not pass (c.f., IR only observation) because it is difficult to accurately detect cloud areas at high latitudes due to the radiometric effect at large zenith angle from geostationary Earth orbits. Therefore, it is expected to fill the gap of the missing area to extend the PMW-IR combined algorithm poleward. In this study, the poleward extension of the PMW-IR combined algorithm is developed using the Nonhydrostatic Icosahedral Atmospheric Model-Local Ensemble Transform Kalman Filter (NICAM-LETKF) the Japan Aerospace Exploration Agency (JAXA) Research Analysis (NEXRA) data operating in the JAXA Supercomputer System (JSS3). vertically integrated water vapor and some other outputs are successfully applied to the polar extended PMW-IR combined algorithm on behalf of IR data. In this presentation, the moving vector, Kalman filter noise table, and precipitation distributions are evaluated with those of simulated and observed clouds and precipitation.
AS80-A006
Effects of the Orbit Boost on GPM Dual-frequency Precipitation Radar Observations
Kosuke YAMAMOTO1+, Takuji KUBOTA1#, Takeshi MASAKI2, Kaya KANEMARU3, Nobuhiro TAKAHASHI4, Kinji FURUKAWA1, Tomomi NIO1, Gennosuke KIKUCHI2, Masato ITO2, Tomohiko HIGASHIUWATOKO2
1Japan Aerospace Exploration Agency, 2Remote Sensing Technology Center of Japan, 3National Institute of Information and Communications Technology, 4Nagoya University
The NASA and the JAXA performed orbit boost maneuvers in November 2023 that raised an altitude of the Global Precipitation Measurement (GPM) Core Observatory from 400 km to 435 km to extend its lifetime. Effects of the orbit boost on the spaceborne precipitation radar have been investigated in the Tropical Rainfall Measuring Mission (TRMM) performed in August 2001. This study evaluates effects on DPR observations due to the GPM orbit boost. Spatial resolution at the nadir and swath width is changed at 5.04km×5.04km and 255.8 km at satellite altitude of 407 km to 5.48km×5.48km and 277.9 km at satellite altitude of 442 km, respectively. Distances between adjacent footprints in the cross-track direction between the pre-boost and the post-boost using observation data and they confirmed that changes of the sampling were larger in the cross-track direction (about 5 km to 5.5 km at the nadir). It was found that the DPR coverage tendency was changed by the GPM orbit boost. In pre-boost, DPR achieved 100% coverage in 8 days. On the other hand, with post-boost, the coverage was still 99.9834% after 24 days, slightly less than 100%. This coverage trend is expected to change with satellite maneuvers. The maneuver is expected to change the orbit elements, thereby covering all locations. With analyzing measured radar reflectivity factor at storm top height over the ocean, the sensitivity degradation was found for about 0.8-0.9dB for KuPR, and about 0.7-0.9dB for KaPR.
AS80-A001
Evaluation of Solid Precipitation Products from GPM/DPR
Nobuhiro TAKAHASHI#+
Nagoya University
In the version 07 product of GPM/DPR released in December 2021 newly included several parameters relating to solid precipitation such as flagHail (flagGraupelHail) and MSindex. The former, as the name suggests, detects hail and/or graupel, while the latter detects multiple scattering, which can be used for hail detection since multiple scattering tends to occur when hail appears. In this study, four products relating to the solid precipitation were compared and evaluated including the product named flagHeavyIcePrecpitation (hereafter flagHIP) (which detects large solid precipitation) introduced in the V06 and three products mentioned above. The result showed that contamination of stratiform precipitation appeared in flagGraupelHail and MSindex. Since the flagHIP allows the stratiform precipitation because it targeted large snowflakes as well as hail and graupel, separation of snowflakes type and hail/graupel type was conducted by applying a simple method to convective precipitation. The number of detections were small both for flagHail and MSindex that are less than 0.07 % and 0.04 % of total precipitation pixels, respectively, whereas flagGraupelHail and flaHIP were 10 times larger number. Overlapping area of each product was not large. Multiple scattering appears as a knee structure of DFRm (measured dual frequency ratio) that can be seen in not only MSindex but also flagHail and flagHIP of convective precipitation indicating each algorithm detecting similar types of precipitation even the overlapping pixel numbers were not large. The flagHIP distributed not only tropical region but also mid latitudes indicating the possible detection of graupel from winter shallow convective system which can be seen over Japan sea in winter.
AS80-A003
Development of Spaceborne Ku-band Doppler Precipitation Radar
Nobuhiro TAKAHASHI1#+, Yukari TAKAYABU2, Takuji KUBOTA3, Kaya KANEMARU4, Kazuyuki OKADA3, Kinji FURUKAWA3
1Nagoya University, 2The University of Tokyo, 3Japan Aerospace Exploration Agency, 4National Institute of Information and Communications Technology
The dual-frequency precipitation radar (DPR) on the GPM core observatory has been observing for about 10 years. Regarding the follow-on mission to the GPM/DPR, observations are required to focus on cloud-precipitation processes in order to evaluate global warming, while observations are required to maintain the quality of precipitation map products and to ensure the continuity of radar data assimilation into operational weather forecasts. Since atmospheric dynamics, especially updrafts, play an important role in understanding the cloud and precipitation processes, the mission study was conducted focusing on Doppler velocity observation. We introduced Displaced Phase Center Antenna (DPCA, Durden et al. 2007) to reduce the measurement error caused by satellite speed. Since dual-frequency observations are difficult due to the size of the satellite if we introduce DPCA, Ku-band single-frequency Doppler radar (KuDPR) has been selected. The KuDPR will provide high sensitivity (7.3 dBZ) for Doppler velocity observations in the nadir direction, and the rest of the scan will be similar to that of the DPR. The accuracy of the Doppler velocity is less than 2 m/s including errors due to the vertical motion of the satellite etc. The precipitation estimation algorithm needs to be modified and an algorithm for estimating vertical air motion using Doppler velocity data is required; a single-frequency algorithm has been developed in DPR will be modified by introducing Doppler velocity information which is also affected by the rain drop size distribution. It is expected to develop a method for estimating atmospheric vertical velocity at the same time. The satellite development has started by JAXA as the Precipitation Measuring Mission (PMM). The satellite will be launched in 2029 at an altitude of approximately 430 km and an inclination of 55 degrees to participate in the NASA's Atmosphere Observing System (AOS) mission.
Session Chair(s): Manisha MISHRA, Azim Premji University
AS62-A008
| Invited
Mitigating Methane Emissions from Irrigated Rice Cultivation Using Modified Urea Fertilizer
Arti BHATIA1#+, Ankita PAUL1, Ritu TOMER1, Shikha SHARMA1, Niveta JAIN1, Vinod KUMAR1, Mark A. SUTTON2
1ICAR-Indian Agricultural Research Institute, 2UK Centre for Ecology & Hydrology
Methane (CH4) is a short lived climate pollutant (SLCP), estimated to have a warming potential of 84 times that of carbon dioxide over a 20-year time horizon and rice cultivation is a major source of CH4. Mitigating the emissions of CH4 from rice cultivation is essential for reducing impacts of global warming, especially under the future climate scenario of increasing levels of carbon dioxide and atmospheric temperature. Modified urea fertilizers can mitigate reactive nitrogen emissions, however, studies on the effect of these fertilizers under elevated CO2 and temperature (ECO2T) interaction is lacking. An experiment was conducted in free air temperature and carbon dioxide enrichment (T-FACE) rings growing two rice varieties (Pusa 1509 and PRH 10) with modified urea fertilizer to evaluate the impact on emissions of CH4, nitrous oxide (N2O) and nitrogen use efficiency during 2019. The treatments were urea (UR), Neem oil coated urea (NCU), Limus coated urea (LCU), and no fertilizer (CON) grown under ambient (ambient CO2 and temperature) and ECO2T (1.7oC over ambient and 580ppmCO2). The cumulative seasonal CH4 emitted varied from 31.6 kg ha-1 in LCU to 34.5 kg ha-1 in UR under ambient conditions. NCU and LCU significantly (p<0.05) reduced the CH4 emission and increased rice yield (p<0.05) compared to UR in both the rice varieties. However, the CH4 emission increased under ECO2T interaction by 3.1 % in CON to 8.2% in LCU. The N2O emission varied from 0.37 to 0.43 % of applied N under ambient conditions, and no significant effect of ECO2T was observed on N2O emissions in both the rice varieties. Nitrogen content in rice grain was the significantly(p<0.05) higher with LCU and NCU under ambient, and the harvest N use efficiency was highest with LCU (51.8%) followed by NCU (48%) in PRH 10 variety, but reduced under ECO2T interaction.
AS62-A009
| Invited
Emission Inventory of Short Lived Climate Forcers from Crop Residue Burning
Niveta JAIN1#+, Helen MARY ROSE1, Shivam TOMAR1, Arti BHATIA1, Ulrike DRAGOSITS2, Mark A. SUTTON2
1ICAR-Indian Agricultural Research Institute, 2UK Centre for Ecology & Hydrology
India produces large amount of agricultural residue (~700 million tons per annum) which is used as residential and industrial fuel, cattle fodder and bedding, thatching material, etc. However, due to mechanisation, non-availability of labour and high labour cost, the surplus residue is often burned on field and contributes significantly towards the emission of greenhouse gases, air pollutants, particulates matter and smoke thereby posing threat to human health. Despite its ill effects on the environment and human health burning of crop residue continues to be a prevalent practice. The present study has used the bottom up approach to quantify the emission short-lived climate forcers namely CO, SOx, NOx, NH3, PM2.5, black carbon (BC or EC), non-methane organic compounds (NMOC/NMHC) from on-farm burning of surplus crop residue for last two decades. The emission factors of SLCFs were compiled from peer reviewed literature and only field studies were considered. The primary crop considered for were rice, wheat, cotton, maize, millet, sugarcane, jute, and rapeseed-mustard. Burning of crop residues led to emission of 11.85 Mt of short lived climate forces in 2020. Of the total emission of SLCFs 71% share was of CO, followed by NMOC (15%) and PM2.5 (7.04%). The trend analysis in emission of SLCFs showed the variability of 29.07% in annual emission from 2000 to 2020. The uncertainty in emission of SLCF was also estimated.
AS62-A006
Measurements of Ground Level Ozone at an Urban Site in South Delhi (India)
U.C. KULSHRESTHA#+, Sudesh YADAV
Jawaharlal Nehru University
Ozone (O3) formation in the troposphere is an area of concern as it affects the vegetation, climate, human health and atmospheric composition. Recently, O3 spikes have been reported in Delhi. In this study, synoptic chemical measurements were carried out for ground level O3 during winter season when air pollution levels are seen severe. The study was carried out from October 2022- February 2023 at an urban area in Delhi. The O3 was captured using an assembly consisting of impinger, flow meter and low volume pump operating at a flow rate of 1 litre per minute for 2 hours. The samples were collected three times a day i.e.1100-1300 hrs, 1300-1500 hrs and 1500-1700 hrs. Out of the sampling months, mean O3 was very high during November and February while very low during October month. Out of three sampling intervals, the highest O3 was recorded during 1300-1500 hrs. Moderate O3 levels were recorded during 1500-1700 hrs while the lowest levels were recorded during 1100-1300 hrs. However, in February month during 1500-1700 hrs, the O3 mean was the highest while during 1100-1300 hrs in November month, the O3 levels were the lowest showing an unusual behaviour. O3 variation showed that crop residue burning and plastic waste burning emissions of O3 precursors such as BC and chlorine species had a significant impact. A positive correlation between O3 and temperature indicated that high temperature (intense solar radiation) is responsible for higher rate of O3 formation. Further, the O3 levels were observed directly related to the visibility and inversely related to PM2.5 and PM10 levels.
AS62-A003
An Assessment of Ozone Formation from VOCs Sources and NOx in Western Taiwan Using Machine Learning
Manisha MISHRA1,2+, Pin-Hsin CHEN2, Thi-Thuy-Nghiem NGUYEN2, Thi-Cuc LE2, Guan-Yu LIN3, Chuen-Jinn TSAI2#
1Azim Premji University, 2National Yang Ming Chiao Tung University, 3Tunghai University
The application of statistical models has excellent potential to provide crucial information to mitigate ozone (O3) pollution by capturing its associations with explanatory variables. Considering the large contribution of O3 in degrading the air quality of western Taiwan, three-year (Jan 1, 2019 to Dec 31, 2021) hourly mass concentration data of 54 VOCs, NOX, and O3 from four photochemical assessment and monitoring stations (PAMs), located along the western side: Tucheng (TC), Zhongming (ZM), Taixi (TX) and Xiaogang (XG), were analyzed to identify the effect of anthropogenic/controllable factors on O3 formation and abundance. Owing to the impact of high ambient reactivity of VOCs on the underestimation of sources, photochemical oxidation was assessed to calculate the loss/consumed amount of VOC (VOCcons) which was followed by the source identification. Diurnal and seasonal high O3 concentrations were well corroborated with VOCcons due to rapid photo-oxidation of VOCs during these periods. PMF (positive matrix factorization) results found that VOCs from solvents were the major source at northward (north-TC and central-ZM region) stations whereas VOCs-industrial emissions dominated at southward (southcentral-TX and south-XG, respectively) stations. Furthermore, the machine learning (ML) gradient boost model was applied to evaluate the effect of weather conditions on O3 abundance and major VOC sources contributing to O3 formation. Results clearly showed that meteorological factors favor to reduction of O3 (-46% and -30%) at northward-located stations of western Taiwan but it has a major role in accumulating the O3 (+50% and +13%) in southward-located stations which is mainly transported from the upwind region of south-central Taiwan.
AS62-A005
Laboratory and Field Calibration Study of Low-cost Metal Oxide VOC Sensors Using Regression and Machine Learning Methods
Qiu LIANG-HAN1+, Thi-Cuc LE1, Chuen-Jinn TSAI1#, Jhih-Yuan YU2
1National Yang Ming Chiao Tung University, 2Ministry of Environment
Taiwan have been reported to frequently exceed the 60 ppb threshold limit of maximum 8-hour daily average O3 (O3-MDA8) from the year 2000 to 2022. To investigate the major O3 forming precursors, Taiwan Ministry of Environment (MOE) has deployed a large number of low-cost metal oxide semiconductor (MOS) sensors for real-time measurement of VOCs to trace its complex sources. However, the MOS sensors for atmospheric monitoring significantly affected by meteorological conditions or air pollutants which can cause unstable signal responses. Therefore, this study attempts to evaluate the performance of MOS sensors through long-term (10-12 months) monitoring data in the laboratory and reference VOCs data from air quality monitoring stations (AQMS) using linear regression (LR), multiple linear regression (MLR), and artificial neural network (ANN) to improve the data quality. It was found that the addition of cross-sensitive parameters such as ambient temperature (T), relative humidity (RH), and carbon monoxide (CO), and related parameters such as nitrogen oxides (NOx) for VOC calibration can efficiently improve the data quality and accuracy of the sensors. In the laboratory and field tests, the ANN model has been shown to have best performance when T, RH and CO were added to the VOCs calibration. As compared to R2 (0.44) and MNE (155.64%) of sensor measured manufacturer data, ANN significantly improved the data accuracy with higher R2 (0.72) and MNE (41.36%). On the other hand, the addition of NOx in the model further enhanced the VOCs field calibration with high R2 (0.78) and MNE (33.61%). The ANN calibration model was also successfully utilized for MOS based VOC prediction. This study compares the advantages of various models and parameter options, which can be provided to the regional environmental agencies for calibration to improve the accuracy of VOCs measurement.
AS62-A004
Partitioning of Chlorine and Chloride Aerosols Relating with Ozone, BC, and PM 2.5 Levels at JNU, Delhi (India)
Saurabh DHAKAD+, U.C. KULSHRESTHA#
Jawaharlal Nehru University
Delhi experiences severe air quality deterioration in winters. The role of atmospheric aerosols is well known for affecting human health, visibility, cloud formation, and other atmospheric processes. This also has implications for the economy. However, many background chemical reactions and physical processes are not well understood. In this study, we have attempted to study the relationship between water-soluble gases including chlorine and aerosols including chloride. For this purpose, we measured gases and aerosols on a 12-hour interval period during severe air pollution conditions in winter (November-December 2023). Fine aerosol samples were collected on a Teflon filter (pore size 0.22 microns). Aqueous soluble gases were collected in miliQ water after passing air through a quartz filter. The samples were analyzed using ion chromatography. The pH was measured in aqueous-extracted aliquots of aerosol samples. The average pH of aerosol samples was 5.68. The detailed results will be presented during the conference.
Session Chair(s): Min-Hui LO, National Taiwan University, Seok-Woo SON, Seoul National University
AS43-A016
Improving Global Subseasonal to Seasonal Precipitation Forecasts Using a Support Vector Machine-based Method
Kei YOSHIMURA1#+, Gaohong YIN2, Tamima AMIN1
1The University of Tokyo, 2Jilin University
Subseasonal to seasonal (S2S) precipitation forecasts provide great potential for hydrological forecasting at an extended range (from 2 weeks to 2 months). Current S2S precipitation forecasts are provided by climate models with large biases, and post-processing is required. The study proposed a support vector machine (SVM) regression-based method to improve S2S precipitation forecasts from the European Center for Medium-Range Weather Forecasts (ECMWF) across the globe. Results suggested that the SVM-based method significantly improved ECMWF daily precipitation forecasts in representing the spatiotemporal variation of precipitation with higher consistency and reduced errors when compared to observations. Moreover, the SVM-based method improved the probabilistic skill of ECMWF forecasts, providing higher ranked probability skill score (RPSS) for real-time forecasts. The most significant improvement from the SVM-based method is witnessed in regions with complex terrains where ECMWF yielded the worst skill, such as the Andes mountain range, Congo River Basin, and the Tibet Plateau. However, the SVM-based post-processing method did not alter the characteristics of precipitation forecasts regarding climate zone and lead time. The temperate and continental climate zones yielded relatively higher skill when the lead time is shorter than 2 weeks, while low-latitude regions showed higher predictability when the lead time became longer than 5 weeks, which is attributed to the slow variation of boundary conditions such as the El Niño-Southern Oscillation (ENSO). We are trying to apply the improved precipitation for the hydrological prediction in “Today’s Earth” activity (https://www.eorc.jaxa.jp/water/) and some preliminary results will be shown at the conference.
AS43-A017
Development of a Next Generation Coupled KIM for Weather Forecast and S2S Prediction
Myung-Seo KOO#+, Eunjeong LEE, Mee-Hyun CHO, Hyeon-Ju GIM, Jun-Seong PARK, Jaeyoung SONG, Yong-Jae HAN, Jin-Yun JEONG, Subin KIM
Korea Institute of Atmospheric Prediction Systems
The Korean Integrated Model (KIM) was developed for global weather forecasting at the first Phase (2011–2019) of the Korea Institute of Atmospheric Prediction Systems (KIAPS), and it has become the operational model of the Korea Meteorological Administration (KMA) since April 2020. To improve the predictability beyond 2 weeks, it is necessary to better represent the physical process and interaction between the atmosphere and surface. Therefore, the new KIAPS Phase 2 project (2020–2026) aims to advance the land surface model and to couple the ocean/sea-ice/wave/river-routing models to the operational KIM. At the first stage (2020–2022), ocean (the Nucleus for European Modelling of the Ocean; NEMO) and sea-ice (Sea Ice modelling Integrated Initiative; SI3) models were newly coupled to KIM by means of the own coupler based on Model Coupling Toolkit. The evaluation result showed that the performance of the KIM coupled version is promising on medium-range weather forecast as well as sub-seasonal to seasonal (S2S) simulations when compared to the uncoupled version. The new land surface models, Noah with multiple parameterization (Noah-MP) and community land model (CLM), became optional to explicitly consider the geographical processes within snow and canopy layers. In addition, the river-routing (Catchment-based Macro-scale Floodplain; CaMa-Flood) and wave (Wave Watch III; WW3) models were coupled at a preliminary stage and their sensitivity are being explored. In the conference, the current status and future plan will be presented in detail. Acknowledgements: This work was carried out through the R&D project “Development of a Next-Generation Numerical Weather Prediction Model by the Korea Institute of Atmospheric Prediction Systems (KIAPS)”, funded by the Korea Meteorological Administration (KMA2020-02212).
AS43-A020
Development of Middle Atmosphere Physics Processes for Extended Mid-term Performance
Sunghye BAEK#+
Korea Institute of Atmospheric Prediction Systems
The warm biases above the stratopause profoundly impact atmospheric circulation in the stratosphere and mesosphere, affecting model integration and initial field accuracy. This region, with significantly decreased atmospheric density, undergoes substantial temperature shifts due to minor photochemical reactions. Improving physics processes here is crucial. Our KIM model displays sudden warm biases in forecasts from 50 km to its uppermost layer. The primary factor influencing temperatures beyond the stratosphere is solar UV's interaction with ozone. To address this, we're refining these processes to tackle observed biases, focusing on enhancing ozone physics step by step. This work underscores the need to refine intermediate atmosphere physics to correct warm biases. Doing so is vital for enhancing the precision of mid-term atmospheric predictions.
AS43-A027
Evaluation of the Middle Atmosphere Circulation and Non-orographic Gravity Wave Processes in the Korean Integrated Model
So-Young KIM#+
Korea Institute of Atmospheric Prediction Systems
Proper representation of the middle atmosphere circulation is important to develop the extended medium-range forecast model as the middle atmosphere is dynamically linked to the troposphere. The anomaly in the middle atmosphere propagates to the lower levels and affects the troposphere in the extended medium-range timescale. In this study, the stratosphere and lower mesosphere circulation in the Korean Integrated Model (KIM) has been assessed. In the extended medium-range and seasonal simulations, temperature in the upper stratosphere and mesosphere has cold bias in the summer hemisphere and warm bias in the winter hemisphere, especially in the high latitudes. Those biases are found commonly in different horizontal resolutions and forecast timescales. Consistent with temperature biases, polar night jet and summer hemisphere easterly jet are weaker than in the reanalysis data. Temperature and zonal wind biases suggest that cooling (warming) at the summer (winter) pole by the meridional circulation due to gravity wave drag is overestimated in KIM. In a frontal gravity wave drag parameterization, it was found that generation of frontal gravity waves is excessive at high horizontal resolutions. To prevent this, the frontogenesis threshold for diagnostic of wave generation region was modified to include a dependency on the horizontal resolution. By using modified frontogenesis threshold, which reduces the frontal gravity wave generation overall, zonal wind becomes stronger in the upper stratosphere and mesosphere, leading to warming and cooling in the high latitudes in summer and winter, respectively. This alleviates temperature bias not only in the middle atmosphere but also in the troposphere.
AS43-A024
Characteristics of ENSO-east Asia Teleconnection Modulated by MJO in KIM Subseasonal Prediction
Sae-Rim YEO#+, Eun-Hee LEE, Hye-Jin PARK
Korea Institute of Atmospheric Prediction Systems
This study investigates the El Niño-Southern Oscillation (ENSO)-East Asia teleconnection modulated by Madden-Julian Oscillation (MJO) in subseasonal time scale during boreal winter. In the seasonal time scale, El Niño induces generally warm condition over the East Asia through development of the anticyclonic circulation anomaly over the western North Pacific during winter. However, this relationship can be modulated in subseasonal time scale, which is mainly influenced by MJO. In particular, when El Niño co-occurs with MJO phase 2&3, the enhanced convection over the Indian Ocean leads cyclonic circulation anomalies over the southern east Asia, which is the opposite response to the seasonal mean El Niño’s influence. The similar situations are observed for the La Niña case when the La Niña accompanies MJO phase 6&7. The predictability of these features in Korea Integrated Model (KIM) has been investigated. The KIM shows skillful prediction capability by capturing the ENSO-East Asia teleconnection modulated by the MJO phase within 2 weeks lead time. However, as the forecast lead time increases up to 4 weeks, KIM tends to predict enhanced convection over the Indian Ocean regardless of the MJO phase during El Niño. For La Niña, the eastward propagating features of the MJO become less evident as the forecast lead time increases. The cause of these features has been further investigated through the AMIP simulation of the KIM and comparison with other CMIP6 AMIP models. The results suggest that the models’ characteristic in simulating seasonal mean tropical circulation response to ENSO is closely related to the models’ bias in simulating subseasonal ENSO-East Asia teleconnection. The detailed dynamical rationale for these features will be discussed in this presentation.
AS43-A022
MJO Simulation in the Extended Range Hindcasts of Korean Integrated Model
Hye-Jin PARK#+, Shin-Woo KIM, Taehyoun SHIM, Eun-Hee LEE
Korea Institute of Atmospheric Prediction Systems
The Madden-Julian oscillation (MJO) is the dominant mode of tropical atmospheric variability on sub-seasonal time scales, and is known to affect weather and climate not only in the tropics but also extra-tropics. This study examines the performances of the winter MJO simulations in the extended range hindcast of Korean Integrated Model (KIM), which is the operational global numerical weather prediction model of the Korean Meteorological Administration for the medium-range forecasting. Now the Korean Institute of Atmospheric Prediction System is making various efforts to extend the forecast range from 10 days to 30 days using the KIM. We conducted the ensemble hindcasts experiments with a 50km horizontal resolution and 6 ensemble members (1 control run and 5 perturbed runs). Sea surface temperature and sea ice are prescribed every 00-hour as the ocean boundary condition. The mean bias of MJO related variables over the tropical Indian ocean and Pacific are analyzed and the performance of the MJO simulation is evaluated using the Real-time Multivariate MJO index. Also, we identify the impact of ensemble prediction on the MJO prediction by comparing the prediction skills of MJO between the control run and the ensemble mean. The findings of this study will serve as foundational data contributing to the improvement of MJO prediction.
Session Chair(s): Fei LUO, Centre for Climate Research Singapore
AS81-A010
| Invited
Large-scale Waves and Weather Patterns in Southeast Asia and Link with Predictability of Heavy Precipitation
John METHVEN1#+, Samantha FERRETT1, Gui-Ying YANG1, Emma HOWARD2, Paula GONZALEZ3, Oscar MARTINEZ-ALVARADO1, Thomas FRAME1, Chris HOLLOWAY1, Steve WOOLNOUGH1
1University of Reading, 2Bureau of Meteorology, 3Met Office
High impact weather events with widespread, heavy rainfall in Southeast Asia are commonly associated with the passage of equatorial waves. The occurrence of the waves and their links with rainfall are dependent on larger scale flow regimes, including the MJO, cold surges, the Asian monsoon and ENSO. In this talk the risk of heavy rainfall (a proabilistic forecast) is predicted given numerical ensemble forecasts of the large-scale state combined with the observed statistical relationships between heavy precipitation and the large-scale state. Two contrasting techniques for characterising the large-scale state are used: one based on equatorial wave amplitude and phase, the second based on the identification of patterns of variability over the region and the projection of ensemble forecasts onto those patterns. A two-tiered regime assignment is used. Tier 1 uses clustering to identify pan-Asian scale regimes, which capture ENSO and seasonal variations associated with the monsoon flow. Each regime is partitioned into Southeast Asia regional clusters (tier 2) that capture synoptic patterns of variability and include the signatures of cold surges, phases of the MJO and BSISO and tropical cyclones. The sub-seasonal predictability of the tiered regimes and equatorial waves is assessed separately using UKMO global ensemble forecasts for lead times of up to 5 weeks. There is substantial probabilistic forecast skill with both methods, in many regions outperforming direct prediction of precipitation by models beyond 1-2 days lead time. There is skill in the equatorial region associated with Kelvin waves but this falls rapidly by day 4-5 because the forecast skill of the waves themselves deteriorates. The skill in westward waves extends into week 2 and skill dependent on the weather patterns is substantial in week 3. The extent to which different large-scale components are predictable and yield predictive skill for precipitation with current forecast systems are discussed.
AS81-A011
Characteristics of Extreme Rainfall Events and Associated Flash Floods in Southeast Asia Megacities from V3 Study Projections
Fei LUO1#+, Aurel MOISE1, Sandeep SAHANY1, Muhammad Eeqmal HASSIM1,2, Gerald LIM2, Jianjun YU1, Venkatraman PRASANNA1, Chen CHEN1, Xin Rong CHUA1, Pavan Harika RAAVI1
1Centre for Climate Research Singapore, 2Meteorological Service Singapore
Singapore’s third National Climate Change Study (V3) is the first study to provide high-resolution (both spatial and temporal) climate model projections under different Shared Socio-economic Pathways (SSPs) for both Singapore and neighbouring countries in the South East Asia (SEA) region. Especially for variable rainfall, the high-resolution simulations can go up to 10 minutes and 2 km. This dataset gives us the advantage of examining the variability and amplitude of future heavy rainfall events and their changes compared to the historical period (1995-2014) in great detail. The future SSPs (SSP1-2.6, SSP2-4.5, and SSP5-8.5) are composed of two-time slides of 2040-2059 and 2080-2099 to cover the mid-century and end-century. The future projections extreme value statistics, specifically Generalized Pareto Distribution (GPD) analysis, will be carried out to study the properties of future extreme rainfall events in Southeast Asia megacities. Furthermore, with more extreme rainfall projected in the future, flash floods are also expected to increase in frequency. Flash floods often occur within a short time, generally less than 6 hours, after a rainfall event. The impacts of flash floods arise from traffic disruption, threats to human lives and local ecosystems, and damage to properties and infrastructures. With the V3 study projections, we can fill the gap in our current knowledge of changes in the characteristics of future extreme rainfall events and associated flash floods in Southeast Asia megacities.
AS81-A008
Exploring Dry Spell Characteristics in Southeast Asia Across Different Global Warming Levels: Insights from Convection-permitting Regional Climate Model Simulations in Singapore’s Third National Climate Change Study (V3)
Muhammad Eeqmal HASSIM1,2#+, Sandeep SAHANY1, Aurel MOISE1, Chen CHEN1, Xin Rong CHUA1, Venkatraman PRASANNA1, Pavan Harika RAAVI1, Jianjun YU1, Fei LUO1, Aaron TAN3, Huey Yew CHEONG4, Jerrome NG5
1Centre for Climate Research Singapore, 2Meteorological Service Singapore, 3Yale-NUS College, 4King's College London, 5National University of Singapore
The occurrence of dry extremes in the future can have significant repercussions ranging from water resources management to trans-boundary haze. In this study, we explore the dynamics of dry spells in Southeast Asia, utilising convection-permitting (8-km and 2-km) regional climate model simulations conducted as part of Singapore’s Third National Climate Change Study (V3). By analysing these high-resolution models, we examine variations in dry spell frequency and intensity (duration) under different warming scenarios. The results provide valuable insight for regional climate adaptation efforts in the context of ongoing climate change.
AS81-A005
Strengthened Impact of Late Autumn Arctic Sea Ice on Winter Severe Cold Events in Asia After Late 1990s
Cen WANG+, Hui SU#
The Hong Kong University of Science and Technology
Winter severe cold events (WSCE) frequently plague densely populated areas of Asia, as was the case in January 2008, leading to substantial economic losses and even fatalities. The sea ice concentration anomalies in the northern and southern Arctic (SICN and SICS respectively) are correlated with the occurrence of WSCE in Asia; however, exact time and location of the teleconnections and the strength of the correlations vary. In this study, we focus on the decadal differences in the teleconnections between the Arctic sea ice concentration and the Asian WSCE before and after late 1990s. We find that the impacts of the SICN and SICS on the Asian WSCE occurrence have strengthened after the late 1990s. Specifically, before the late 1990s, the influences of SICS and SICN on the WSCE in Asia were relatively weak, possibly related to the weak intensity of SICS and the limited correlation between SICS and SICN. However, after the late 1990s, the interannual variability of SICS becomes larger and anti-correlated with that of SICN, and their impacts on the Asian WSCE occurrence are in phase, resulting in stronger teleconnection between the Arctic sea ice and Asian WSCE. We further analyzed the physical mechanisms involved in the teleconnections. We find that that SICS and SICN modify atmospheric stability through alterations in surface heat fluxes and surface upward longwave radiation fluxes, and then the magnitudes of westerly winds and the intensity of blocking highs over the northern Eurasian continent, which directly affects the frequency of WSCE in Asia. The decadal differences in the Arctic sea ice influences on the WSCE in Asia may be associated with long-term climate change.
Session Chair(s): Sang-Wook YEH, Hanyang University
AS35-A003
| Invited
Large-scale Atmospheric Circulations and Synoptic Disturbances Associated with Rapid Sea-ice Reduction Events in the Okhotsk Sea
Youichi KAMAE#+, Mone YOKOTA
University of Tsukuba
The Okhotsk Sea (OS), which is located east of Siberia, is characterized by a large fraction of seasonal sea ice cover (between November and June) despite its latitudinal position. The large interannual variability in sea ice concentrations (SIC) in OS attracted much attention from a viewpoint of effects of large-scale atmospheric circulations. Here we investigate association of the large-scale atmospheric circulation including the passage of extratropical cyclones, warm conveyor belts, and atmospheric rivers with the SIC reduction events over the OS on subweekly-to-weekly timescales. We found that the southeasterly wind anomalies over the Sea of Okhotsk, associated with the eastward-moving extratropical cyclones from northern Japan to the North Pacific, contribute to the SIC reduction over the central OS. In addition, during early spring, warm and moist southwesterly winds associated with extratropical cyclones and concurrent enhancement of the Soya Current contribute to the coastal SIC reduction in the southern OS. The warm and moist southwesterly winds exhibit key features of warm conveyor belts and atmospheric rivers. We identified the important contribution of atmospheric rivers to perturbations in cryosphere through the mid-latitude atmosphere-ocean interactions.
AS35-A043
Waveguide Teleconnections Along Polar Front Jet. Part 2: Linkage to the Waveguide Teleconnection Along Subtropical Jet
Peiqiang XU#+, Lin WANG, Wen CHEN
Chinese Academy of Sciences
During boreal summer, there are two prominent waveguides over Eurasia: the subtropical jet and the polar front jet. The variability of large-scale circulation over Eurasia in this season is often featured by intensified waveguide teleconnections along jet streams. Occasionally, we observe the occurrence of double waveguide teleconnections over Eurasia, but there are also cases where only one waveguide is dominant. In this study, our focus is to investigate the coupled relationship between waveguide teleconnections over Eurasia and explore the underlying dynamics that govern this coupling. Observational diagnostics show that the coupling between waveguide teleconnections over Eurasia is not a random occurrence but rather a reflection of the interconnected relationship between dominant internal modes along jet streams. The coupled relation between waveguide teleconnections exhibits significant interdecadal variations. Idealized model experiments indicate it is the location of initial action center, rather than the mean flow difference, plays a dominant role in this coupling. Climate model simulations confirm this hypothesis and further indicates the tripolar SST pattern in North Atlantic and associated jet stream changes above Atlantic are responsible for the location shift of initial action center.
AS35-A025
Troposphere-stratosphere Interaction During Different ENSO and PDO Phases in Idealised Model Experiments
Yulia ZYULYAEVA1#+, Daria SOBAEVA2,3, Sergey GULEV1
1Shirshov Institute of Oceanology, 2SHIRSHOV INSTITUTE OF OCEANOLOGY OF RUSSIAN ACADEMY OF SCIENCES, 3Moscow Institute of Physics and Technology (National Research University)
Large-scale sea surface temperature anomalies (SSTа) such as El Niño Southern Oscillation and Pacific Decadal Oscillation (PDO) affect the spatial structure of the quasi-stationary planetary waves (PW). As storm tracks correspond to a large-scale planetary flow, we find deflection of the main storm tracks in the Northern Hemisphere from their climate mean position during El Niño and La Niña years. On the other hand, extreme states of the stratospheric polar vortex (SPV) can affect the location of the storm tracks over a period from 2 weeks to 2 months. Idealized model experiments were carried out on the Isca platform to determine the differences in the response of tropospheric dynamics to extreme SPV states during the El Niño and La Niña events and different PDO phases. It was shown that it is impossible to state the southward shift of the Atlantic storm track during El Niño years without accounting for the SPV intensity. There is a difference in the region of the tropospheric response. During El Niño events after sudden stratospheric warmings (SSW) the southward shift of the storm track is observed in the western part of the Atlantic-European region, and during La Niña – in the eastern part. We showed that the regions of the southward shift of the Atlantic storm track correspond to the planetary wave crest. In this region tropospheric jet stream has northward tilt before SSW. The intensity of the SPV, expressed as the zonal mean zonal wind, averaged along 600 N at 10 hPa level, has the maximum prognostic potential during La Niña years in combination with the negative PDO phase.
AS35-A026
Mid-latitude Interactions Expand the Hadley Circulation
Woosok MOON#+
Pukyong National University
The Hadley circulation describes a planetary-scale tropical atmospheric flow, which has a major influence on climate. Contemporary theoretical understanding is based upon angular momentum conservation, the basic dynamical constraint governing the state of the flow pattern. However, despite the degree of success in representing the Hadley circulation, the canonical theoretical model does not treat interactions with other regions, particularly the mid-latitudes. Here, we extend the original model of Held & Hou 1980 to include the influence of mid-latitude large-scale atmospheric dynamics, which we treat using the planetary-scale heat equation with a parameterized poleward heat flux driven by synoptic eddies. The energy flux balance within the Hadley cell includes the poleward heat flux at the poleward edge of the cell, which is controlled by the baroclinic instability of the sub-tropical jet. Our theoretical solutions suggest that global warming, which can reduce the baroclinicity of the subtropical jet, may lead to the poleward expansion of the Hadley cell due to the change in energy flux balance within it.
AS35-A015
Strengthened Linkage of Winter Mid-latitudes Climate and Weather Variability to Autumn Regional Arctic Sea Ice Anomalies
Shuoyi DING#+
Fudan University
Reanalysis datasets and sea-ice sensitivity experiments (SC-WACCM) have demonstrated that the autumn sea ice loss in East Siberian-Chukchi-Beaufort (EsCB) Seas favors a colder winter across central-western Eurasia, and even significantly increases the frequency of winter extreme low temperature over western-central China. However, this linkage has been strengthened since the late 1990s, accompanied by an amplified interannual variability of EsCB sea ice. After the late 1990s, due to intensified positive net surface heat flux anomalies during the low sea ice, notably stronger and southward extended Arctic Anticyclonic anomalies will modify the North Atlantic storm track and induce synoptic eddy-mean flow interaction, thereby further amplifying the atmospheric anomalies in turn and contributing to northern Eurasian cooling.
AS35-A021
The Precipitation-recycling Process Enhanced Extreme Precipitation in Xinjiang, China
Jinxia ZHANG#, Shanshan WANG+
Lanzhou University
The amount, frequency and intensity of extreme precipitation over Xinjiang have increased dramatically under the wetting trend in Northwest China, but long-term trends in the precipitation-recycling process remain largely unexplored. Based on dynamic recycling model and MERRA2 reanalysis, we revealed a mean recycling ratio for extreme precipitation in Xinjiang of 42.3% with a growth rate of 2.3% decade−1 during 1982–2019. The increasing trend of extreme precipitation was almost equally attributed to increased recycling precipitation (49%) and external precipitation (51%). The extreme precipitation in Xinjiang exhibited two peak centers, the Tianshan Mountains region (TS) and Kunlun Mountains region (KL), highlighting variations in the water cycle. Specifically, the external cycle predominated the increased extreme precipitation in TS (61%), while the recycling process mainly influenced the increase in KL (67%) due to markedly enhanced evapotranspiration. Moisture source attribution further proved the crucial role of evapotranspiration from Xinjiang and its vicinity in extreme precipitation.
AS35-A008
Influence of the Southern Ocean Dipole on the Inter-model Diversity of Temporal Variability of the Austral Summer Southern Annular Mode in CMIP6 Models
Rui WANG+, Fei ZHENG#, Xiaofeng LI
Sun Yat-sen University
The Southern Annular Mode (SAM) is the predominant mode of climate variability across the Southern Hemisphere (SH) extratropical region. During the late 20th century, the SAM has undergone a remarkable positive trend, particularly pronounced in austral summer (December-January-February, DJF), attributed to ozone depletion in the Antarctic stratosphere. However, state-of-the-art models exhibit noteworthy inter-model spread of the simulated long-term trend of the DJF SAM. This study aims to explore potential sources of the model uncertainty in simulating the DJF SAM trend, using outputs from historical experiments and AMIP experiments from 42 models archived in CMIP6. Corresponding results indicate that the responses of the atmospheric circulation to the dominant mode of SH extratropical sea surface temperature (SST), namely the Southern Ocean Dipole (SOD), play an important role in model performance in reproducing the SAM variability. Models with stronger linkage between the SOD and the SAM tend to simulate a more positive trend as well as a more realistic inter-annual variability of the DJF SAM, the averaged explained variance is over 30% in AMIP experiment. The possible reason for the inter-model uncertainty in depicting the responses of the SAM to the SOD in DJF could be explained by the different sensitivities of atmospheric baroclinicity in middle and high latitudes to the underlying SST anomalies in each model, which may be associated with the internal processes of the climate system.
AS35-A016
Changing Influence of Boreal Summer Indo-pacific Convection on Surface Air Temperature in Canadian Arctic Archipelago Switched by Arctic SST Anomalies
Rui LU1#+, Zhiwei ZHU1, Sang-Wook YEH2
1Nanjing University of Information Science & Technology, 2Hanyang University
The tropical Indo-Pacific convection influences surface air temperatures (SAT) over Canadian Arctic Archipelago (CAA) via inducing poleward propagated Rossby wave train. However, this influence is changing in the past four decades. The changing influence of tropical Indo-Pacific heating on SAT over CAA (CAT) is predominantly attributed to Arctic sea surface temperatures anomalies (SSTA) to the north of the Eurasian continent. The negative Arctic SSTA lead to a weakened East Asia westerly jet by inducing the southeastward propagated Rossby wave. The weakened westerly jet strengthens the meridional gradient of potential vorticity over North Pacific, guiding the Rossby wave propagating northward into CAA and therefore affecting CAT. Conversely, the positive Arctic SSTA impedes the northward propagation of Rossby wave via enhancing the East Asia westerly jet, resulting in a weakened relationship between tropical Indo-Pacific convection and CAT. The present study implies that Arctic thermal condition play a vital role in modulating the tropic-polar connection through switching the waveguide of the Rossby wave train.
Session Chair(s): Hye-Yeong CHUN, Yonsei University, Zeyu CHEN, Chinese Academy of Sciences
AS29-A042
| Invited
Understanding of the Distribution of Pollutants in the Himalayan Region Through Transport and Mountain Meteorology
Narendra SINGH1#, S. K. DHAKA2+
1Aryabhatta Research Institute of Observational Sciences-ARIES, 2University of Delhi
The pristine environment of the Himalayan region is often intruded by the pollutants resulting from biomass burning across foothills, Gangetic plain and also via transboundary pollutants over the year. The transport processes operating over the complex mountainous terrain are quite different from the ones over a flat terrain. Moreover, the logistic difficulty of operating the instruments to make the regular and high resolution measurements over the Himalayan region is very challenging and this limits the availability of ground based real time data. For the first time, a network of 14 stations across a span of about 3000 km, is established to make the high resolution measurement of particulate matter of aerodynamic size less than 2.5µm (PM2.5), with altitude of the sites ranging from about 500-2000 m including the foothill sites as well. These simultaneous measurements are used as the tracers to understanding the dynamics and transport mechanism across the mountain slopes, in addition to providing a real time information on air quality parameter. Apart from a distinct diurnal cycle, pronounced seasonal effect of continental and long range transport are observed. To decipher the processes, two case studies, each of dust storms (PM2.5: 340 μg m−3) and biomass burning (PM2.5: 110 μg m−3), have been carried out that highlight the necessity of continuous PM2.5 measurements to be potentially used for regional climate models and pollution mitigation strategies. Additionally, the lockdown situation is studied for Manora peak Nainital, and the PM2.5 variability over topographically different sites across Himalayas are also investigated. It is observed that the high altitude site is showing relatively better air quality with the annual mean values of PM2.5 in the range of 18 ± 17 μg m−3 and 14 ± 11 μg m−3 from a year to the other during 2018 and 2019 respectively.
AS29-A016
Satellite-based Inventory of Episodes of Stratospheric Penetration of Siberian Wildfires Plumes in the Period 2002 - Present
Alexandra LAENG1#+, Sergey KHAYKIN2
1Karlsruhe Institute of Technology, 2Institut Pierre-Simon Laplace, Université de Versailles Saint-Quentin-en-Yvelines, Sorbonne Université, National Centre for Scientific Research
In recent years, episodes of stratospheric penetration of plumes containing biomass burning products from wildfires became more frequent. An approach to detect and characterize such events from satellite data consists in synergetic use of limb and nadir measurements. It makes use of Absorbing Aerosol Index (AAI) from nadir and vertical profiles of aerosol extinction and biomass burning gases from limb. The approach is applied to detect the episodes of stratospheric penetration of Siberian wildfires plumes in the period from 2002 until present. We present an ongoing inventory of such events, some resulting from PyroCb events, some from other convective lifting mechanisms. It particular, it includes estimations of mass of smoke and gazes injected in the stratosphere by such events, which is a must data for modeling the tropopause-crossing episodes of wildfire smoke plumes. Injected mass estimations are performed from CCI Multi-satellite AAI, MIPAS, MLS, and OMPS NM and LP datasets, using two different methods. The limitations of the approach and its feasibility for OMPS NM combined with CAIRT limb profiler instrument, which is selected for Phase 2 of ESA Earth Explorer 11 mission, are discussed.
AS29-A034
Impact of Extreme Wildfires on Stratospheric Composition from Satellite and Ground-based Observations
Sergey KHAYKIN1#, Alexandra LAENG2+, Florent TENCE1, Sophie GODIN-BEEKMANN1, Qiaoyun HU3, Philippe GOLOUB3, Artem FEOFILOV4, Oceane SOARES1, Tetsu SAKAI5, Isamu MORINO6, Yoshitaka JIN6, Richard QUEREL7, Ben LILEY7
1Institut Pierre-Simon Laplace, Université de Versailles Saint-Quentin-en-Yvelines, Sorbonne Université, National Centre for Scientific Research, 2Karlsruhe Institute of Technology, 3University of Lille, 4Ecole Polytechnique, 5Japan Meteorological Agency, 6National Institute for Environmental Studies, 7National Institute of Water & Atmospheric Research
The severity of wildfires has remarkably increased over the last years in both hemispheres and there is an emerging realization of their effect on climate and ozone layer. Intense wildfires can generate extreme thunderstorms termed Pyrocumulonimbus (PyroCb), that are capable of injecting smoke and other combustion products directly into the stratosphere, where the residence time of aerosols is not limited by cloud scavenging and precipitation. A number of recent studies have put in evidence that the effects of strong PyroCb events on the global stratosphere rival those of moderate volcanic eruptions in terms of magnitude and duration whilst exceeding them in terms of radiative forcing. Here we use global observations by MLS, OMPS, CALIPSO, SAGE III and TROPOMI satellite missions together with ground-based lidar records in France and New Zealand to characterize and quantify the planetary-scale impact of wildfire PyroCb on stratospheric gaseous composition and aerosol optical properties as follows. First, we identify the wildfire events during the last two decades with a measurable stratospheric impact and classify them into four categories ranging from 1 to 4 based on the magnitude and longevity of their stratospheric impact. Then, we quantify the aerosol and gas mass fluxes into the stratosphere for each event. Using a combination of nadir and limb observations along with ERA5 analysis, we explore the spatiotemporal evolution and dynamics of the stratospheric smoke plumes. We show evidence for the geographical and seasonal extension of the tropopause-overshooting PyroCb events. By using long-term ground-based and satellite lidar observations of depolarization, we point out the longevity of fine smoke particles in the stratosphere. Finally, we discuss the impact of the anomalous 2023 Canadian wildfires, which are shown to be responsible for a record-high and persistent season-wide smoke pollution at the commercial aircraft cruising altitudes and the lowermost stratosphere.
AS29-A010
The Impact of Radiation-chemical Coupling in Arctic Stratospheric Ozone Changes on Arctic Stratospheric Polar Vortex
Siyi ZHAO#+, Jiankai ZHANG
Lanzhou University
Impacts of radiation-chemical coupling in Arctic stratospheric ozone variation on the polar vortex during wintertime and early springtime are investigated using a reanalysis dataset and a climate model. Here, we use chemistry–climate numerical experiments to isolate the impacts of radiation-chemical coupling on stratospheric polar vortex. The results reveal there are opposite trends in temperature and ozone between November-December and January-February. From 1980 to 2000, there is an increasing trend in ozone and temperature in the lower stratosphere during November-December, while a decreasing trend is observed in ozone and temperature during January-February. The temperature and ozone trends during 2000-2020 are non-significant. The temperature increase in November-December is related to the wave propagation benefited by the increased refractive index at high latitudes and the strengthened wave number-1 waves activity in the troposphere, and strengthened the residual circulation. This results in a weakened polar vortex and shifted to East of Eurasia continent during November-December. The cooling trend of temperature in January-February is linked to the weakening of planetary wave activity at late December and early January, related to the wave propagation impeded by the decreased refractive index and weakened the downwelling of residual circulation, which leads to a strengthened polar vortex during January-February. The strengthening of the polar vortex in late wintertime and early springtime is primarily induced by the shortwave radiation effect of ozone. This study further reveals that the radiation-chemical effects resulting from ozone variations lead to a slowdown in ozone loss in early winter and a delayed recovery in late winter-early spring, and these effects remain unchanged around the year 2000.
AS29-A039
The Influence of ENSO on the Mid-summer Polar Mesopause
Zeyu CHEN#+
Chinese Academy of Sciences
During mid-summer time, the polar mesopause is characteristic of extremely low temperatures (around 140 K). It is such cold that noctilucent clouds (NLCs) are formed at ~87 km height, and various observational and/or model simulation results with respect to the phenomenon suggest the state of polar mesopause elapses various long-term changes. In this presentation, 22-year satellite observation data from the TIMED/SABER experiment are used to estimate the distribution for global mean temperature and geopotential height for middle atmosphere. Focusing on mid-summer seasons for both northern and southern hemisphere, the state of mesopause, e.g., height position and temperature, are derived, then interannual variabilities are analyzed. Significant difference is seen between the southern and northern hemisphere, in particular in high latitudes 60 degree latitudes poleward. In the southern polar region, variabilities for both height position and temperature are significantly larger than that in the northern hemisphere. Linear Regression Analysis (LRA) is applied to investigate the correlation of the state of polar mesopause and external forcings from the Sun, i.e., the index of solar radio flux f10.7, and that from the Pacific ocean, e.g., the ENSO index MEI.v2. Estimates of correlation coefficient from LRA shows extremely strong correlation of the ENSO signal and the state of southern polar mesopause. Over the period 2002-2023, the correlation coefficient attains > 0.7 with confidence level of 95%. The Northern polar mesopause only show relative strong correlation to the f10.7 index, while impact from the ENSO is substantially weak. The asymmetric correlation to the two external forcings for the mid-summer time polar mesopause in two hemispheres will be presented with detail.
AS29-A038
Climatic Trends in Meteorological Parameters Over Indian Landmass and Isle in Andaman Nicobar and Lakshadweep During 1980-2021
S. K. DHAKA1#+, Shristy MALIK2, A. S. RAO2, Hye-Yeong CHUN3, Narendra SINGH4
1University of Delhi, 2Delhi Technological University, 3Yonsei University, 4Aryabhatta Research Institute of Observational Sciences
An analysis is performed to examine trends in temperature, specific humidity, wind speed over the Indian landmass and in the isles of Lakshadweep (Arabian sea side) and Andaman and Nicobar (Bay of Bengal side) over the last 4 decades (from 1980 to 2021). MERRA data deployed for revealing the large-scale fluctuations and linear trends in these parameters covering 36 stations (30 stations located over landmass and 3 each in the Arabian sea side and in the Bay of Bengal side). Surface temperature (2 m above ground) data showed a linear rise, which is more prominent after 2000, both in the Arabian side and the Bay of Bengal. Over this period, temperature increased ~ 0.7- 0.8 0C on both sides of Indian landmass. About two third stations (24 stations) in the study showed increase in temperature. However, relative humidity data on all island stations exhibited a decrease (prominent during 2000-2021). Quasi-periodic fluctuations in temperature (which is linearly rising) closely relates with the ENSO parameter. Wind speed, in general, showed larger magnitude over Andaman and Nicobar Islands (~ 5.0 m/s yearly averaged) in comparison to Arabian sea (~ 4.0 m/s) and landmass (~ 2.2 m/s). On the other hand, solar cycle (sun spot numbers) and wind speed reflects a weak positive correlation coefficient (< ~ 0.40) but statistically significant while no consequential correlation found between solar cycle and relative humidity. Detailed analysis suggests that relative humidity decreased both over landmass and islands during 2000-2021. Interestingly, surface temperature increased more rapidly between latitudes 7.030N and 12.910N after 2000. Rise in temperature and long period fluctuations (> 2-3 years) in the lower latitudes (< 150N) showed a strong association with ENSO signal suggesting invigorated atmosphere ocean interaction.
Session Chair(s): Richard ECKMAN, National Langley Research Center
AS59-A055
Changes in Tropospheric Composition and Air Quality During the Dzukou Valley Fires in North-east India
Binita PATHAK1#+, Barlin DAS2, Chandrakala BHARALI1, Aniket CHAKRABORTY1, Gayatry KALITA3, Partha SAHU1, Anindita BORAH1, Pradip BHUYAN1
1Dibrugarh University, 2Jorhat Institute of Science and Technology, 3Ministry of Earth Sciences
The North East Indian states (NEI) and adjoining areas, is crucial in terms of atmospheric composition, chemistry and their implications, owing to its geo-climatic environment and complex topography and is conducive for gas-aerosol interactions due to the abundance of solar insolation and reactive precursor gases. The region is mostly vegetated and prone to natural forest fires. In the present study, the Weather Research and Forecasting Model coupled with Chemistry (WRF-Chem, V4.0) is used to simulate such a fire event occurred over Dzukou valley (25°N, 94°E, ~2.4 km amsl) covering an area of ~ 90 km2 during 29th Dec, 2020 -11th Jan, 2021 and the resultant changes in tropospheric composition and air quality in terms of gaseous pollutant concentrations: CO, O3, NO2, CH4 and SO2 and PM10. The model simulations were validated using satellite data, where fire was detected by MODIS and VIIRS-SNPP sensors, and the smoke was detected by Sentinel-2A. The maximum fire radiative power was detected by these sensors on 5th Jan, 2021. The model simulated gaseous pollutant concentrations exhibit sporadic peaks during intense fire days (3rd – 5th, Jan, 2021) with the maximum surface level concentrations of CO being 1.99 ppmv, O3 is 0.06, NO2 is 0.037, SO2 is 0.007 and CH4 is 0.00003 ppmv, which is associated with a percentage increase of ~50%, 25%, 15%, 40% and 15% during the intense fire period. These sporadic peaks are also observed from satellite data. The dispersion of pollutants at higher altitudes results in their reduced concentrations. Nevertheless, the O3 mixing ratio is prominent vertically up to > 2km. The surface level PM10 concentration reaches up to ~200 µg/m3 over the location during 7th-9th, Jan, 2021, after the intense fire period, associated with the secondary aerosols formation and particle growth rate.
AS59-A041
Enhancement of Nighttime Fire Detection and Combustion Efficiency Characterization from Space
Jun WANG#+, Meng ZHOU
The University of Iowa
We present the second-generation FIre Light Detection Algorithm (FILDA-2), which includes advances in fire detection and retrievals of radiative power (FRP), fire visible energy fraction (VEF), and fire modified combustion efficiency (MCE) at nighttime from the holistic use of multiple-spectral radiances measured by the visible infrared imaging radiometer suite (VIIRS) aboard Suomi-NPP (VNP) and National Oceanic and Atmospheric Administration (NOAA)-20/joint polar satellite system (JPSS)-1 (VJ1) satellites. Key enhancements include: 1) a new fast algorithm that maps VIIRS day/night band (DNB) radiances to the pixel footprints of VIIRS moderate (M) and imagery (I) bands; 2) identification of potential fire pixels through the use of the DNB anomalies and I-band thermal anomalies; 3) dynamic thresholds for contextual testing of fire pixels; and 4) pixel-specific estimates of FRP, VEF, and MCE. The MCE derived by FILDA-2 is in good agreement with limited ground-based observations near the fires. The cross-validation of FILDA-2 products from VNP and VJ1 retrievals confirms good consistency in FRP and MCE retrievals globally. FILDA-2 is being implemented by the National Aeronautics and Space Administration (NASA) to generate a new VIIRS data product for fire monitoring, chemical-speciated fire emission estimates, and fire line characterization.
AS59-A013
Quantifying the Spatial Representativeness of Carbon Flux Footprints of a Grassland Ecosystem in the Semi-arid Region
Haixing GONG#+, Guoyin WANG, Tiantao CHENG
Fudan University
Quantifying the single-site representativeness of carbon flux footprints plays a crucial role in land-atmosphere interaction, especially in semi-arid regions with high-frequency turbulence. In this study, we used multi-platform datasets, including observational data derived from the eddy covariance flux monitoring systems of the Semi-Arid Climate and Environment Observatory of Lanzhou University (SACOL) and multivariate satellite remote sensing, to explore the distribution characteristics of carbon flux footprints during 2007-2016, using a Flux Footprint Prediction model. The relative importance of atmospheric boundary layer factors and vegetation factors on the area of carbon flux footprints was quantified by correlation analysis, multiple stepwise regression, and random forest. Physical mechanisms affecting the differences in the spatial distribution of carbon flux footprints were also analyzed. The results show that the carbon flux footprints are usually distributed on the prevailing wind side of the station, whose main contributing source area is the relatively flat grassland at the summit range of SACOL, with a spatial representativeness of 67.4~507.2 m in length and 54,982~105,329 m2 in area. Mechanism studies have shown that the frictional velocity, vegetation Index, atmospheric instability parameters, and wind speed have significant importance on the area of carbon flux footprints due to dynamic and thermal forcing, with frictional velocity being dominant, while wind direction has a major effect on the profile shape. This study provides references for the representativeness of site fluxes for semi-arid regions dominated by grassland ecosystems where observations are often scarce.
AS59-A008
Analyzing Carbon Cycle Anomalies Arising from the 2023 Canadian Wildfire Season Using TROPESS CO Retrieval Data Products
Seungwon LEE#+, Kevin BOWMAN, James MCDUFFIE, David MORONI
California Institute of Technology
In 2023, Canada faced its most severe wildfire season in recorded history, affecting all 13 provinces and territories. Commencing in March, the 2023 Canadian wildfire season escalated in intensity throughout June before gradually subsiding in October, ultimately resulting in a total burned area of 45.7 million acres. The smoke generated by these wildfires extended across North America, traversed the Atlantic, and reached Europe by late June. The NASA TRopospheric Ozone and Precursors from Earth System Sounding (TROPESS) project detected heightened Carbon Monoxide (CO) emissions associated with the 2023 Canadian wildfire season. TROPESS CO data products were generated by extracting the vertical distribution of atmospheric CO state from radiance measurements by the Cross-track Infrared Sounder (CrIS) on the Joint Polar Satellite System-1 (JPSS-1) using an optimal estimation algorithm known as MUlti-SpEctra, MUlti-SpEcies, Multi-SEnsors (MUSES). TROPESS CO data products revealed a significant increase in the column-averaged dry-air mixing ratio of CO from the surface to the top of the atmosphere (XCO) in 2023 compared to the relatively calm season of 2022 in Canada and the Northeastern US. For instance, the Northeastern US and the Eastern Canada region witnessed an average XCO increase of 20.4 ppbv from June 2022 to June 2023. In July 2023, the Western Canada region observed an average XCO increase of 48.4 ppbv compared to July 2022. TROPESS CO products also illustrated the spatial extent of the smoke from the wildfires, covering the entire Northern Hemisphere, and the temporal evolution of the smoke propagating through the polar jet stream. Our discussion will delve into the methodology behind TROPESS CO retrievals and the insights gained from the TROPESS CO retrieval data products regarding carbon cycle anomalies resulting from the 2023 Canadian wildfire season.
AS59-A015
The Multi-year Contribution of Indo-china Peninsula Fire Emissions to Aerosol Radiation Forcing in Southern China During 2013–2019
Jun ZHU#+
Nanjing University of Information Science & Technology
Fire emissions in Southeast Asia transported to southern China every spring (March-May), influencing not only the air quality but also the weather and climate. However, the multi-year variations and magnitude of this impact on aerosol radiation forcing in southern China remain unclear. Here, we quantified the multi-year contributions of fire emissions in Indo-China Peninsula (ICP) region to aerosol radiation forcing in the various southern Chinese provinces during the fire season (March–May) of 2013–2019 combining the GEOS-Chem chemical transport model and the Column Radiation Model (CRM) model simulations. The fire emissions over the ICP region were found to increase the aerosol optical depth (AOD) value by 0.1 (15%) and reduce the single scattering albedo (SSA) in three southern regions of China (YN, GX, and GD from west to east), owing to increases in the proportions of black carbon (BC, 0.4%±0.1%) and organic carbon (OC, 3.0%±0.9%) within the aerosol compositions. The transported smoke aerosols cooled surface but heated the atmosphere in the southern China regions, with the largest mean reduction of -5 Wm-2 (-3%) in surface shortwave radiation forcing and the maximum daily contributions of about -15 Wm-2 (-15%) to the atmosphere radiation forcing in the GX region, followed by the GD and YN regions. The impacts of ICP fire emissions on aerosol optical and radiative parameters declined during 2013–2019, with the highest rate of 0.393±0.478 Wm-2yr-1 in the GX for the shortwave radiation forcing in the atmosphere. Besides, their yearly changes in the contribution were consistent with the annual fire emissions in the ICP region. Such strong radiative perturbations of ICP fire emissions were expected to influence regional meteorology in southern China and should be considered in the climate simulations.
AS59-A045
| Invited
Multi-satellite Multi-species Top-down Emissions Estimation of SLCF Over Energy-rich and Rapidly Changing Asia
Jason COHEN#+
China University of Mining and Technology
Rapid urbanization, industrialization, economic growth, and the movement of millions each year into urbanized has increase energy use and material production, even given technological improvement, environmental regulations, and climate policies. These factors have led to considerable changes in the magnitude, spatial, and temporal distribution of emissions throughout Asia over the past two decades. This work uses day-by-day and grid-by-grid observations of NO2, CO, SSA, AOD, and CH4 from upward-looking sensing platforms, and downward looking satellites (including OMI, TROPOMI, MOPITT, MISR, and others) to compute emissions of BC, CO, NOx, and CH4 in tandem using a flexible, mass-conserving, first-order physics, chemistry, and thermodynamics driven emissions model. Observation campaigns in energy consuming locations throughout China are used to improve a priori emissions estimates at high temporal and spatial frequency, and provide constraints on the emissions modeling system. Emissions are estimated holistically, with both the uncertainty and variability explicitly computed. This method can reliably attribute sources including Power Plants, Iron and Steel, Aluminum, Cement, Coke, Chemicals, Boilers, road and boat transportation. Decreasing emissions are observed at large and well-regulated locations, alongside a shift in from urban and industrial to suburban and rural areas. Targeted species (NOx and Aerosol Mass) generally decrease over large spatial averages (although the geospatial pattern tends to be wrong). Co-emitted species are more complex, with CO and Aerosol Number increasing in some areas and decreasing in others. While year-to-year changes show a small change, specific months or weeks of the year dominate these trends, indicating low-hanging fruit to control emissions has already been used and future improvements will require new approaches. Since high-frequency events dominate total emissions, more and longer field campaigns are urgently needed to represent fat-tail distributions. Finally, impacts of retrieval uncertainty and biases are used to quantify the effects of emissions uncertainties on AMF uncertainties.
Session Chair(s): Cheng-Ku YU, National Taiwan University, Tetsuya TAKEMI, Kyoto University
AS67-A008
Orography-MJO Interaction: Impact on Atmospheric Profiles and Rainfall in West Sumatra's Diverse Topography
Wendi HARJUPA1,2#+, Eiichi NAKAKITA1
1Kyoto University, 2Indonesia National Research and Innovation
Orographic enhancement shapes rainfall in mountains, influenced by phenomena like Madden-Julian Oscillation (MJO). To investigate their correlation, we employed MJO indices, Vertically Integrated Moisture Flux Convergence (VIMFC), Convective Available Potential Energy (CAPE), convective inhibition (CINH), Lifted Condensation Level (LCL), and Level of Free Convection (LFC) extracted from ERA5 reanalysis data spanning 21 years (2001–2022) at five difference locations surrounding the mountains area of west Sumatra, each varying in elevation: the windward side (L1, L2), mountaintop (L3, L4), and leeward side (L5). The elevations strongly influence rainfall, leading to varying rainfall intensities across the 5 locations. Rainfall is higher over the mountaintop, except during the night when it is higher over the windward side. Enhanced rainfall over the mountaintop coincides with lower CINH and higher VIMFC values, while reduced rainfall over the windward side and leeward side occurs when CINH and VIMFC values are higher. MJO strongly influences rainfall and the effects depended on the phase of the MJO. During MJO-3, precipitation increases over all locations. Conversely, during MJO-4, rain tends to decrease, particularly during the day. MJO-3 tends to reduce CAPE, and this reduction is more pronounced during MJO-4. MJO-3 tends to reduce CINH and increase VIMFC, while MJO-4 increases CINH and reduce VIMFC. The reduction (increase) of CINH, and the increase (decrease) of VIMFC during MJO-3 (MJO-4), may explain the increase (decrease) of rainfall. The reduction of CINH is possibly caused by the lowering of the LCL and LFC due to the increase in VIMFC. Hence, VIMFC and CINH play a vital role in MJO-topography interaction, impacting rainfall variability. In summary, both topography and the MJO significantly contribute to variable magnitude, preserving their diurnal cycles. These findings are crucial for understanding the intricate effects of MJO-topography interaction on rainfall patterns.
AS67-A005
Mesoscale and Orographic Influences on the Extreme Rainstorm on July 20, 2021 in Zhengzhou, China
Juanzhen SUN1#+, Rumeng LI2
1National Center for Atmospheric Research, 2Peking University
The extreme rainstorm that on 20 July 2021 in Zhengzhou, China produced 201.9 mm rainfall in one hour, breaking the record of 1-h rainfall accumulation in China. The rainstorm produced 201.9 mm rainfall in one hour, breaking the record of mainland China for 1-h rainfall accumulation in the past 73 years. Using 2-km continuously cycled analyses with 6-min updates that were produced by assimilating observations from radar and dense surface networks with a four-dimensional variational (4DVar) data assimilation system, we illustrate that the modification of environmental easterlies by three mesoscale disturbances played a critical role in the development of the rainstorm. Among the three systems, a meso-beta-scale low pressure system (mesolow) that developed from an inverted trough southwest of Zhengzhou was key to the formation and intensification of the rainstorm. We show that the rainstorm formed via sequential merging of three convective cells, which initiated along the convergence bands in the mesolow. Further, we present evidence to suggest that the mesolow and two terrain-influenced flows near the Taihang mountains north of Zhengzhou, including a barrier jet and a downslope flow, contributed to the local intensification of the rainstorm and the intense 1-h rainfall. The three mesoscale features co-existed near Zhengzhou in the several hours before the extreme one-hour rainfall and enhanced local wind convergence and moisture transport synergistically. Our analysis also indicated that the strong midlevel south/southwesterly winds from the mesolow along with the gravity-current-modified low-level northeasterly barrier jet enhanced the vertical wind shear, which provided favorable local environment supporting the severe rainstorm.
AS67-A004
Distribution Characteristics and Formation Mechanisms of Lightning in the Malacca Strait
Kun-Hsuan CHOU1#+, Kai-Chun WANG1, Shu-Jeng LIN1, Alfred CHEN2
1Chinese Culture University, 2National Cheng Kung University
This study mainly analyzed the lightning distribution characteristics of the Strait of Malacca area in Southeast Asia from 2009 to 2021 and explored the physical mechanisms of lightning formation therein. The lightning data used in this study were obtained from the World Wide Lightning Location Network (WWLLN) developed by University of Washington; the data mainly comprise frequencies of cloud-to-ground lightning. Reanalysis data (ERA5) of the European Centre for Medium-Range Weather Forecasts (ECMWF) were also used as meteorological data for analysis. In addition, variables pertaining to the surface wind field, and convective available potential energy (CAPE) were examined to explore the thermodynamic and dynamic conditions when lightning occurs. Based on 13-year composites, it is shown that lightning activity in this area was higher over the strait than over the land. Both land and sea areas exhibited distinct diurnal cycles. Lightning at sea was prevalent during the night and early morning, whereas lightning over land was prevalent during the late afternoon and evening. Seasonal disparities in lightning occurrences were also noted, with the movement of the Intertropical Convergence Zone influencing the relatively high lightning occurrences in Southeast Asia during Mar–May and Sep–Nov. Furthermore, lightning in the eastern terrestrial area of the strait preceded the western terrestrial area by approximately 1 to 2 h. Additionally, lightning tends to initiate earlier in the more southward parts around the strait. Overall, lightning occurrences strongly correlated with surface airflow convergence, highlighting the diurnal land–sea breeze cycle as the primary mechanism underlying the formation of lightning in the Malacca Strait.
AS67-A011
Impact of Thermally Forced Circulations on the Diurnal Cycle of Summer Precipitation Over the Southeastern Tibetan Plateau
Huiling YUAN1#+, Jingyu WANG2
1Nanjing University, 2China Meteorological Administration
The summer precipitation over the southeastern Tibetan Plateau (SETP) shows remarkable diurnal variations with prominent peaks in the evening. This study investigates how thermally forced circulations regulate the diurnal precipitation over the SETP using surface raingauge observations, and high-resolution reanalysis data during June-August of 2015-2019. The supply of water vapor and the onset of precipitation over the SETP in the afternoon are associated with the upslope winds and upward branch of the mountain-plain solenoids (MPSs) between the SETP and the lowlands (Sichuan Basin and Yunnan-Guizhou Plateau). Despite of the surface cooling, at night, abundant moisture is still transported from the lowlands to the SETP by low-level sustained easterly and strong southerly winds, which are mainly caused by the larger continental-scale thermal circulation combined with the ageostrophic winds of boundary layer inertial oscillations, overwhelming the weak downslope winds of the MPSs off the SETP. Reference: Wang, J., Yuan, H.*, Wang, X., Cui, C., & Wang, X. (2023). Impact of thermally forced circulations on the diurnal cycle of summer precipitation over the southeastern Tibetan Plateau. Geophysical Research Letters, 50, e2022GL100951. https://doi.org/10.1029/2022GL100951.
AS67-A009
Orographically Enhanced Precipitation Associated with Different Background Precipitation of Typhoon Chanthu (2021)
Tsubaki HOSOKAWA#+, Cheng-Ku YU
National Taiwan University
This study aims to document the kinematic and microphysical characteristics of precipitation enhancement over Da-Tun Mountain (DT) of northern Taiwan associated with Typhoon Chanthu (2021), using extensive observations from two ground-based Doppler radars (one of them is the polarimetric radar), dense rain gauge network, and disdrometers. During the analysis period, evolving aspects of orographic enhancement of precipitation corresponding to the two different typhoon background precipitation characteristics (i.e., the outer rainband vs. the weak stratiform) were observed over DT. It was found that the orographic rainfall was more intense during the outer rainband stage, although enhanced precipitation was evident for both stages near the mountain peaks. The dual-Doppler synthesis results indicate a deep layer of upward motions from low to mid levels over DT due to the combination of elevated updrafts associated with the outer rainband and the low-level orographically forced lifting. In contrast, the layer of upward motions during the weak stratiform stage was confined to the lowest levels and was primarily associated with upslope lifting. Analyses of the polarimetric variables show a general increase in drop size and liquid water content with decreasing height, implying collision-coalescence processes. However, the polarimetric characteristics observed over the two stages reveal different hydrometeor sizes of falling collector drops. Relatively larger droplets, which may serve as seeder clouds, were found at 3.5 km MSL within the outer rainband. Measurements from Parsivel disdrometers in DT show wider drop size distributions (DSDs) over mountains compared with the plain region. Furthermore, the noticeable broadening of DSDs was observed during the outer rainband stage due to droplet-size growth over the mountain. Numerous bigger seeder droplets associated with the preexisting convective updrafts within the outer rainband would enhance the accretion of low-level upslope-lifting-generated feeder clouds and contribute to heavier rainfall over DT than the weak stratiform stage.
AS67-A002
Orographic Effects on the Maintenance of Quasi-stationary Convective Band Formed Over the Complex Terrain in the Eastern Part of Shikoku, Japan
Akira NISHII1#+, Taro SHINODA1, Koji SASSA2
1Nagoya University, 2Kochi University
In the eastern part of Shikoku, Japan, characterized by steep micro-scale ridges (approximately 10 km in horizontal scale and 1000 m in height) with various orientations embedded in a larger-scale ridge, a QSCB oriented in a south to north direction occasionally bring heavy rainfall. In this study, we investigate the role of orographic effects on the maintenance of two cases of such QSCBs, Case 1 and Case 2, by using observation and reanalysis data. Case 1 occurred from 12 to 20 JST (UTC+9) on July 3, 2018, and Case 2 happened from 16 to 21 JST on August 15, 2018. Case 1 was divided into Case 1A (from 12 to 15 JST) and Case 1B (from 17 to 20 JST) because the QSCB shifted to 5 km northeast as the low-level wind direction changed from east-southeasterly to south-southeasterly between 15 and 17 JST. Both cases exhibited back-building (BB) characteristics. The starting point of BB in Case 1A was over a micro-scale ridge of 650 m in height oriented in a south-southwest to north-northeast direction (S ridge). While in Case 1B and Case 2, it was at the eastern foot of S ridge. The Froude number at S ridge, Fr=1.76 in Case 1A suggests that upslope lifting maintained the BB in Case 1A, while low-level convergence formed between the flow deflected at upwind of S ridge and the low-level environmental flow was a dominant factor in Case 2, in which Fr=0.70. In Case 1B, despite the high Fr (1.52), the same maintenance mechanism to Case 2 could have contributed. This is because partial flow-splitting can occur even when Fr > 1 especially for the flow relatively parallel to the orientation of a ridge and the complexity of topography may cause the increment of the critical Fr value.
AS67-A010
Moisture Sources and Sinks of Low-level Jets in South China: A Backward and Forward Trace Model Approach
Yuhan LUO#+, Yu DU
Sun Yat-sen University
Low-level jets (LLJs) act as an important carrier of moisture transport, significantly affecting heavy rainfall. In South China, three distinct branches of LLJs coexist, namely the boundary-layer jet in Beibu Gulf (BLJ-BG), the boundary-layer jet in the northern South China Sea (BLJ-SCS), and the synoptic-system-related LLJ in South China (SLLJ-SC). This study employs the Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) with backward and forward trace models to investigate the moisture transport, sources and sinks associated with these LLJs. As the pre-rainy season progresses (from April to June), moisture paths gradually shift from Eurasia and the West Pacific Ocean to the North Indian Ocean. Each LLJ, however, exhibits unique characteristics. The BLJ-BG tends to direct moisture trajectories over the Indochina Peninsula, facilitating the transport of increased moisture from the North Indian Ocean. In contrast, the moisture trajectories of the BLJ-SCS, influenced by the topography of the Indochina Peninsula, tend to circumvent the peninsula, primarily transporting moisture within the local South China Sea. Notably, the BLJ-SCS transports even less moisture from the North Indian Ocean than in periods without the BLJ-SCS. The SLLJ-SC exhibits a pronounced tendency to transport moisture from the northern side. Moisture sinks are closely tied to the terrain for the boundary-layer jets. The BLJ-BG supplies moisture for precipitation in northern Guangxi, and the BLJ-SCS influences central Guangdong precipitation. Additionally, the SLLJ-SC plays a crucial role in transporting moisture to the rain belt in the Yangtze River Basin. This study enhances our understanding of the intricate moisture transport dynamics associated with different LLJs in South China, providing valuable insights for forecasting extreme precipitation events in the region.
AS67-A001
Mechanism of Initiation and Regeneration Convective Cell in Bandung Basin, Indonesia
Irfans Maulana FIRDAUS1#+, Nurjanna Joko TRILAKSONO2, Takeshi YAMAZAKI1
1Tohoku University, 2Institut Teknologi Bandung
The mechanism of convective cell initiation and regeneration in the Bandung Basin (107.35oE-107.95oE; 6.75oS-7.25oS), Indonesia is investigated using a Weather Research and Forecasting (WRF) model. Based on the cumulative distribution function (CDF) and regeneration index (RegI), model simulations were conducted using case studies in February-March 2019. It is found that upslope wind, which is generated by the solar heating, flows to the mountain peak in north and south of the basin, carrying water vapor from the bottom of the basin. Therefore, low-level convergence is formed due to the convergence of winds from the bottom of the basin and from outside the basin. It causes the developing updraft, makes atmosphere unstable, and generates convective initiation (CI). The convective system will be developed in the mountains region, produced precipitation, and formed cold pools on the surface. The cold pool will fall down the slopes and convective activity from the mountains will continue to the bottom of the basin. The convective system’s outflow causes the cold pool to move in the west-east direction. The cold pool will collide with warmer air from the opposite direction, resulting in an updraft at the cold pool leading edge (CPLE), and convection will be re-initiated (convective regeneration) in the Bandung Basin, with the new convective system tending to move eastward.
Session Chair(s): Haobo LI, RMIT University, Xiaoming WANG, Chinese Academy of Sciences
AS56-A009
| Invited
A Dataset of Precipitable Water Vapor Retrieved by the National Ground-based GNSS Network in China During the Period from 1999 to 2022
Hong LIANG#+
China Meteorological Administration
The uncertainty of long-term time series of precipitable water vapor (PWV) derived by radiosondes are greatly concerned due to the moisture heterogeneity related to the changes of the types of humidity sensors. Global Navigation Satellite System (GNSS) provides opportunities to address this issue due to its advantages to estimate PWV under all weather conditions with high accuracy (~1mm), high temporal resolution ( ≤30min), low cost and good potential for homogeneity. The number of ground-based GNSS sites was increasing rapidly from 27 stations in 1999 to more than 1200 stations in 2022 in China. The quality of raw GNSS observations at GNSS sites including pseudo range and phase from GPS were inspected. A simple method to the quality control of raw GNSS observations at GNSS sites were used in order to remove the low quality raw GNSS observations. In order to obtain high-quality ZTD time series, the GNSS observations with quality control in this network were processed using GAMIT packages with the same strategy and reprocessed final orbit products published by IGS. The ZTD was converted into PWV using co-located surface pressure measurements and the weighted averaged atmospheric temperature derived from ERA5 reanalysis. A quality control procedure was implemented to remove the outliers in GNSS ZTD and PWV time series using the time series of the counterpart estimates retrieved from ERA5 reanalysis as references. The error of the PWV dataset was about 0.6~0.8 mm given that the error of ZTD was no more than 4 mm. The annual, summer half-year averaged, and winter half-year averaged PWV over China during the period from 1999 to 2020 shows significant increasing trends with ratios of 0.63, 0.79 and 0.31 mm/10a respectively. This PWV dataset may be beneficial to supporting the researches on the severe weather events and climate change in China.
AS56-A001
| Invited
Spatiotemporal Variations in Atmospheric Water Vapor Over Southwestern China
Minghua WANG1#+, Zhuochen LV1, Weiwei WU2, Chengzhi SUN1
1Nanjing University of Information Science & Technology, 2Institute of Earthquake Forecasting, China Earthquake Administration
The southwestern region of China serves as a corridor for the transportation of water vapor from the Bay of Bengal and the South China Sea to inland China during the summer monsoon. In order to understand the spatiotemporal variations in water vapor over this region, we used the 2011-2022 GNSS data observed at stations located within the region to retrieve hourly precipitable water vapor (PWV). The multiple-year averaged PWV values at these stations range from 11.77 to 33.53 mm, and they show a decrease trend from the southwest to the north of the region. These PWV values are negatively correlated with both station heights and latitudes. Moreover, we observed upward secular trends in PWV variations at all the stations, with an average growth rate of 0.18 mm/year. The PWV time series exhibit significant annual cycles, characterized by amplitudes ranging from 9.75 to 20.94 mm, which are approximately ten times larger than the amplitudes of the semiannual PWV cycles. Generally, PWV values show an increasing trend from January to July, followed by a decline from July to December, with the decline rate exceeding the growth rate. Average diurnal PWV variations reveal predominantly unimodal PWV distributions throughout the day at most stations, except for Station YNRL, where a bimodal PWV distribution was observed. These findings enhance our understanding of the dynamic changes in PWV over southwestern China, providing the basis for effective management of local water resources and disaster mitigation.
AS56-A007
Advanced Zenith Hydrostatic Delay and Weighted Mean Temperature Lapse-rate Models for Vienna Mapping Functions Products
Peng SUN#+, Kefei ZHANG, Suqin WU, Minghao ZHANG, Longjiang LI
China University of Mining and Technology
Zenith hydrostatic delay (ZHD) and weighted mean temperature (Tm) are crucial parameters for converting zenith tropospheric delay (ZTD) to precipitable water vapor (PWV) in GNSS (Global Navigation Satellite Systems) meteorology. These parameters can be obtained from empirical ZHD and Tm models with in-situ atmospheric parameters as inputs. However, most GNSS stations are not mounted with in-situ atmospheric sensors. Fortunately, grid-wise Vienna Mapping Functions (VMF) tropospheric products can be used to interpolate ZHD and Tm over the GNSS stations. Since the VMF products only provide ground surface ZHD and Tm for global grid points, the ZHD and Tm of the four grid points nearest to the GNSS site need to be reduced to the same height of the GNSS site before a horizontal interpolation (e.g., bilinear interpolation or inverse-distance weighted interpolation) is implemented. However, the accuracy of the simple reduction models officially recommended may not be as good as desired in the case that the height of a GNSS site largely differs from that of the four ground surface grid points to be used in the interpolation. In this contribution, a new reduction model for each of the grid points was developed for reducing the grid-wise ZHD and Tm to the target height for the improvement of the interpolation performance. The sample data for the modelling were the 10-year ZHD and Tm profiles over the grid points obtained from ERA5 monthly-mean reanalysis data. Test results showed that the accuracy of the ZHD and Tm interpolated from the VMF products reduced by the new models was significantly better than the ones reduced by traditional methods. It is expected that the new model adds a good value to related fields such as GNSS positioning and GNSS meteorology for better performance.
AS56-A008
Homogenization of Reprocessed Long-term GNSS Precipitable Water Vapor Time Series
Qiuying HUANG1#+, Xiaoming WANG1, Haobo LI2, Chen XIAO1
1Chinese Academy of Sciences, 2RMIT University
Nowadays, the Global Navigation Satellite Systems (GNSS) atmospheric remote sensing technique has emerged as a pivotal tool for the retrieval of atmospheric water vapor contents. Based on the distinct benefits contained in GNSS-derived precipitable water vapor (PWV) time series, including high spatiotemporal resolution, long-term stability and all-weather capability, its feasibility and effectiveness in supporting meteorological applications have been thoroughly confirmed. Nevertheless, GNSS atmospheric products have not been adequately utilized in climate applications, primarily due to the lack of long-term homogeneous GNSS climate records and specifically designed methodologies. In this study, based on our reprocessed long-term PWV time series, we comprehensively investigate the potential temporal shifts within the whole dataset, thereby improving its quality for climate studies. Specifically, the modified Penalized Maximum t test (PMTred), considering the first-order autoregressive noise in the series, is employed to detect potential mean shifts, i.e., change points, in the series representing the difference between GNSS-derived PWV and PWV obtained from the fifth generation European Centre for Medium-Range Weather Forecasts reanalysis (ERA-5) data. The PWV time series from over 200 ground-based GNSS stations, spanning more than 20 years, were tested. It was discovered that some of the detected change points in the sequence were associated with hardware modifications, including changes in receivers, cables, antennas, and radomes. Statistical analysis was also conducted to determine the factors that exerted the most significant impact on the PWV series. Additionally, there are some change points that were not recorded. After the correction of mean shifts in the GNSS data, its consistency has considerably improved in comparison to the ERA-5 data on a global scale.
AS56-A011
Comparing GNSS-PWVs Derived from GNSS Using Different IGS Orbit Products and their Applications in Rainfall Forecasts
Longjiang LI1#+, Kefei ZHANG1, Suqin WU1, Dongsheng ZHAO1, Minghao ZHANG1, Xiaoming WANG2, Haobo LI3, Peng SUN1
1China University of Mining and Technology, 2Chinese Academy of Sciences, 3RMIT University
As one of the most important atmospheric elements, Precipitable Water Vapor (PWV), which can be retrieved from the Global Navigation Satellite Systems (GNSS) measurements, plays a significant role in the study of many weather phenomena. In this research, two types of PWV were derived from GNSS by using two different methods over 66 stations in USA for the period from 2010 to 2020. For the determination of the first type PWV (named PP-PWV), the IGS precision orbit was used to estimate Zenith Total Delay (ZTD) and ECMWF ERA5 was chosen to calculate Zenith Hydrostatic Delay (ZHD) and weighted mean temperature (Tm). For the second type PWV (named RT-PWV), the IGS ultra-fast orbit was used to estimate ZTD, and a global ZHD model and a global Tm model without requirements of any meteorological parameters were used to calculate ZHD and Tm. Then, the two sets of PWV were compared by using PWV derived from sounding data as “ground-truth” references over 10 radiosonde stations. The results showed that the root mean square errors (RMSE) of the PP-PWV ranged from 1.2 mm ~ 3.0 mm, with mean value of 1.7 mm, and the RMSE of RT-PWV ranged from 2.4 mm ~ 4.2 mm, with mean value of 3.1 mm. Finally, based on the two sets of PWV, two rainfall forecast models were constructed and evaluated. The results showed that the two models can achieve good forecast results, and the model based on PP-PWV outperform the one based on RT-PWV.
AS56-A003
Tropospheric Delay Modeling and Application
Weili ZHOU#+, Shuli SONG, Jun JIANG
Chinese Academy of Sciences
Tropospheric delay is one of the major error sources for the high-accuracy geodetic measurement techniques due to the rapid water vapor variation, such as Global Navigation Satellite System (GNSS), Very Long Baseline Interferometry (VLBI) and Satellite Laser Ranging (SLR). To eliminate the tropospheric delay effect on four VLBI stations in China, a prediction model (TRO_P) and a method with 1h update GNSS observations (TRO_G) are proposed for tropospheric zenith delay correction for real-time and 3h latency trajectory determination, respectively. Detailed verification is carried out from zenith delay, different elevation angles, baseline direction and VLBI trajectory determination delay residual. The results using Chang’e-5 observations demonstrate that the mean root mean square (RMS) of residual error of VLBI delay and delay rate for TRO_P are 0.62 ns and 0.75 ps/s at low elevation angles (10deg-28deg), respectively. Moreover, the reduction for the mean RMS of VLBI delay residual using TRO_G is 39.5% meaning from 0.43 to 0.26 ns compared with that using the method with meteorological data (TRO_S) at low elevation angles. The TRO_P and TRO_G methods can be used in any weather conditions. This study can provide a reference for tropospheric delay calibration for trajectory determination of the spacecraft using VLBI or other techniques.
AS56-A012
Effectiveness Evaluation of GNSS Tropospheric Tomography for an Entire Year of 2020 in HK Region
Minghao ZHANG#+, Kefei ZHANG, Suqin WU, Longjiang LI, Peng SUN, Dongsheng ZHAO
China University of Mining and Technology
Global Navigation Satellite Systems (GNSS) tropospheric tomography is a promising technique for obtaining the three-dimensional water vapour density (WVD) field. However, only GNSS tropospheric tomographic results during a period within a year are evaluated for most studies. In this study, the GNSS tropospheric tomographic results in Hong Kong for the entire year of 2020 are evaluated to demonstrate the effectiveness of the GNSS tropospheric tomographic method in any season. The observations of 19 GNSS sites in Hong Kong during the period of 2020 are solved to obtain zenith tropospheric total delays (ZTD) and the range of root mean square error (RMSE) is from 11.5 mm to 15 mm for 19 GNSS sites using ERA5-ZTD as the reference. The pressure and temperature data from VMF1 grid files are used to obtain zenith hydrostatic delay (ZHD) and weight mean temperature (Tm). The perceptible water vapor (PWV) can be obtained based on ZTD, ZHD and Tm, and slant water vapour (SWV) are obtained using VMF1 mapping function. The statistical results show that the range of monthly RMSE is from 1.42/1.38 g/m3 to 2.56/2.55 g/m3 using radiosonde-/ERA5-WVD as the references, respectively. Therefore, the GNSS tropospheric tomographic method has a stable performance in obtaining the three-dimensional WVD field.
Session Chair(s): Daocheng GONG, Jinan University
AS02-A012
Understanding the Trend of Biogenic Secondary Organic Aerosol with CAM6-chem Model
Xinyi DONG#+
Nanjing University
The observed summer surface organic aerosol (OA) concentrations increased slightly in the western United States (WUS), but decreased significantly in the eastern United States (EUS), and the winter OA continued to decline throughout the United States. To understand the drivers influencing the trend of surface OA, we used an improved Community Atmosphere Model version 6 (CAM6) model, which employs tropospheric and stratospheric chemistry and considers the heterogeneous reaction of isoprene epoxydiol-generated secondary organic aerosols (SOAIE) and the rapid photolysis process of monoterpene secondary organic aerosols (MTSOA) to simulate the long-term trend of surface OA between 1988 and 2019. According to the comparative analysis with the observation data of Interagency Monitoring of Protected Visual Environments (IMPROVE), the revised model better reproduces the concentration, spatial distribution, seasonal variation and long-term trend of surface OA. We found that the reduction in summer OA in the EUS region may be attributed to the synergistic effect between SOAIE and MTSOA. As human emissions decrease, primary organic aerosols (POAs) decrease, SOAIE decreases along with sulfates, and MTSOA increases with increased biosource emissions and climate warming. The POA generated by wildfires showed a significant increasing trend (2.9%/year) and a drastic interannual variation (62.8%), which led to a non-significant increase trend of surface OA in the WUS area in summer, while anthropogenic POA dominated the downward trend of OA in winter. Through sensitivity experiments, we found that MTSOA responded linearly to the increase in monoterpene emissions and almost no response to the reduction of NOx emissions, as the MTSOA components from different oxidation pathways offset each other. Therefore, in the context of global warming, the contribution of MTSOA to summer OA is likely to increase day by day. Among them, low volatile high oxygen organic compounds (HOMs) are important components of MTSOA, which have an important contribution to the formation of new particles, which can further affect the formation of cloud condensation nuclei and the radiation balance of the Earth system. By comparing with the field observations, the model can better reproduce the concentration and diurnal cycle characteristics of HOMs-SOA. We further found that HOM-SOA is an important component of MTSOA (36.6%) and SOA (10.7%). This study reveals the important contribution of HOMs-SOA to SOA, and its importance is likely to increase with global warming.
AS02-A010
Organic Nitrates Drive the Production of Urban Secondary Organic Aerosol in Summertime Beijing
Junfeng WANG1+, Xinlei GE1#, Ning ZHANG1, Eleonora ARUFFO2
1Nanjing University of Information Science & Technology, 2University “G. d’Annunzio” of Chieti-Pescara
Secondary organic aerosol (SOA) is of great concern for urban air pollution. Here we use observations from the APHH-Beijing field campaign in summer 2017 to show that nighttime production of organic nitrates (ONs) can play a critical role for SOA the next day. We observe the nighttime build-up to over 40 ppb of products from the oxidation of nitrogen oxide radicals (NOx) and find that they mostly consist of ONs produced by the oxidation of volatile organic compounds (VOCs) by the nitrate radical (NO3). These ONs are mainly in the gas phase at night but can be further oxidized and/or photolyzed the following day to contribute to SOA formation. Anthropogenic alkenes and isoprene are the most important VOCs contributing to nighttime ONs formation. Properly representing this chemistry in models may be complicated by nighttime stratification when NO3 is produced above the surface layer where O3 is not titrated.
AS02-A007
Interactions Between Ozone Pollution, Vegetation and Weather in China
Mengmeng LI#+, Zhipeng JIN, Zihan ZHANG, Yuting LU
Nanjing University
Concurrent heatwave and ozone (O3) extremes have recently emerged as the major environmental crises in China, offsetting the benefits from improved air quality actions. Based on multiple in-situ observations and climate-chemistry coupled modelling, we disentangle the linkage between human activities and climate system in heat-related O3 pollution. We find that intensifying heatwaves accelerate photochemical O3 production by boosting anthropogenic and biogenic emissions, and aggravate O3 accumulation by suppressing dry deposition with water-stressed vegetation, thereby worsening tropospheric O3 pollution by over 40% in China’s urban agglomerations. In turn, ozone is a phytotoxic pollutant that could damage vegetation growth and lead to complicated impacts on air quality. We implement a semi-empirical parameterization regarding the impacts of ozone exposure on photosynthesis rate and stomatal resistance into the Noah-Multi-parameterization (Noah-MP) dynamic vegetation module. The gaseous dry deposition and biogenic emission algorithms are also coupled with Noah-MP to enable the ozone-vegetation coupling. The elevated ozone damages plant photosynthesis, and decreases the national gross primary productivity (−28.85%) and leaf area index (−17.41%). The plant transpiration and surface heat flux, as well as air temperature (e.g., up to +0.16℃ in summer) and other associated meteorological variables are also altered, finally contributing to an increase of surface O3. Otherwise, the suppressed vegetation LAI and biogenic emissions, as well as the lower dry deposition velocity in response to the ozone-vegetation coupling contribute to the remaining ozone changes by −1.07 μg m-3 and 1.18 μg m-3, jointly constituting the complicated ozone-vegetation feedbacks on air quality. Our results highlight the necessity of including the ozone-vegetation coupling in models for reliable prediction of regional climate and air quality.
AS02-A002
Responses of Biogenic Volatile Organic Compound Emissions to Increasing Nitrogen Deposition: a Pilot Study on Eucalyptus Urophylla
Daocheng GONG1#+, Shiwei LIU1, Yujin WANG1, Hao WANG1, Juan HUANG2, Qiao XU1, Boguang WANG1
1Jinan University, 2South China Botanical Garden
Nitrogen (N) is one of the crucial nutrients for plant growth. Currently, the responses of biogenic volatile organic compounds (BVOCs) emission from vegetation leaves to the increasing N deposition remains controversial. Here, we conducted a pilot study on eucalyptus urophylla, which is the most economically important and the widely planted artificial economic forest specie in southern China, a severe N deposition region globally. An intensive in-situ measurement of 17 BVOCs from mature Eucalyptus urophylla in 10-year-old soil N addition plantations were carried out. To simulate current and future N deposition scenarios, three N treatment levels, i.e., 0 (blank control, BC), + 50 (scenario-I, S-I) and + 100 (scenario-II, S-II) kg N·hm-2·yr-1, were employed in the plantations. Results showed that isoprene (37%), α-pinene (39%) and d-limonene (14%) were the main BVOC species under natural condition. The BVOC emission rates can be stimulated up to nearly two-fold under S-I, with the significantly enhanced photosynthetic rate (p < 0.05). While the emission rates were inhibited under the S-II treatment. Our results highlight important insights into the BVOC emissions from artificial economic forest management under current and future N deposition scenarios. It is important to consider and predict the response of BVOC emissions and the ecological functions of vegetation in terrestrial ecosystems to global climate change and atmospheric pollution in the future.
AS02-A011
Vertical Distributions in Isoprene Oxidation Processes and Impacts on Ozone Formation in the Atmospheric Boundary Layer
Xiaobing LI#+, Bin YUAN
Jinan University
Isoprene is a highly reactive volatile organic compound (VOC) from biogenic emissions and is also a vital precursor of ozone globally. The oxidative degradation pathways of isoprene in the atmospheric boundary layer will be changed with height due to substantial vertical changes in concentrations of air pollutants (e.g., NOx and hydrocarbons) and meteorological conditions (e.g., T, RH, and solar radiation). As a result, the vertical changes in isoprene oxidation processes may have important impacts on ozone formation. Unfortunately, the vertical observation information for intermediate oxidation products of isoprene is still very limited by far, affecting the cognition and simulation capacities of ozone pollution. In this study, we utilized the combination of a high-tower platform and online mass spectrometry techniques to make online gradient measurements of isoprene and its key intermediate oxidation products in urban Beijing in the summer of 2021. Constrained by observations, box model simulations were performed to unravel vertical distribution characteristics and key drivers of isoprene oxidation pathways, as well as their influencing mechanisms on ozone formation. We found that isoprene concentrations in daytime sharply declined with height due to chemical removal by OH radicals. The oxidative degradation pathways of isoprene also changed from near the surface to aloft along with the rapid decrease in NO concentration. With the reduced competition for reactions with OH radicals from isoprene, anthropogenic hydrocarbons contributed increasing fractions in ozone formation with increasing height. The results are expected to provide a sufficient understanding of the impacts and contributions of isoprene to ozone formation in the atmospheric boundary layer and provide scientific support for the formulation of ozone pollution control strategies.
AS02-A001
Impacts of Extreme Heat Events on Air Quality in the Northern Hemisphere in Summer 2022
Wenxuan YU1+, Hongliang ZHANG2#, Peng WANG1
1Fudan University, 2University of Shanghai for Science and Technology
Extreme weather events are occurring with increasing frequency and intensity, which not only threaten human health and ecological environment, but also have significant impacts on air quality. The cumulative intensity of extreme heat events in the Northern Hemisphere in 2022 is not seen since at least 1950. This study aims to simulate the impacts of extreme weather events on air quality in the Northern Hemisphere based on the Community Multi-scale Air Quality (CMAQ) v5.0.2 model. The meteorological fields are generated by the Weather Research and Forecasting (WRF) model. The anthropogenic emissions are generated from Emissions Database for Global Atmospheric Research (EDGAR). Biogenic emissions are obtained from the Model of Emissions of Gases and Aerosols from Nature (MEGAN) with the consideration of heat and draught events. The study is intended to investigate the changes in the concentrations of ozone, particulate matter, and other pollutants in response to extreme weather and analyze the cause of air pollution in different countries. Sensitivity experiments will be designed to quantify the impact of extreme heat in 2022 using 2021 as a comparison. This study reveals the response of air quality to extreme weather and provides an important reference for the prevention and control of air pollution during extreme weather.
AS02-A006
The Roles of Sulfur Dioxide on the Optical Properties of Biogenic Secondary Organic Aerosol
Yaying WANG1, Yanchen LI1, Shunyao WANG2, Junfeng WANG3, Qiyuan WANG4, Jianhuai YE1#+
1Southern University of Science and Technology, 2Shanghai University, 3Nanjing University of Information Science & Technology, 4Chinese Academy of Sciences
Ozonolysis of monoterpenes constitutes a significant fraction of atmospheric biogenic secondary organic aerosol (BSOA). Although increased BSOA formation has been observed under sulfate-rich conditions, the underlying mechanisms, as well as the physicochemical properties of the formed BSOA, remain poorly understood. In this study, we investigated the impacts of sulfur dioxide (SO2), an anthropogenic pollutant, on the yields and optical properties of BSOA generated from the ozonolysis of ⍺-pinene, limonene, and β-caryophyllene, in a 50-L quartz flow tube reactor. Enhanced SOA formation was observed through interactions with SO2. Over the course of the experiments, a considerable fraction of SO2 was found to be oxidized by Criegee intermediates and organic peroxides. Light-absorbing components were observed in SOA systems with SO2. The averaged mass absorption coefficient of these components was comparable to those of “brown carbon” in other studies with biogenic precursors. Distinct formation mechanisms of the SO2-mediated BSOA light-absorbing species were observed under dry and humid conditions. And the presence of ammonia further promoted SOA light-absorbing property. Our results highlight that SO2 not only increases SOA formation efficiency but also enhances the potential formation of light-absorbing materials in BSOA, thereby influencing its radiative absorption capacity and impacting global climate.
AS02-A003
Impacts of Extreme High Temperatures on Ozone Formation in Urban Areas
Tianyu HUANG1+, Hongliang ZHANG2#
1Fudan University, 2University of Shanghai for Science and Technology
Ozone pollution has become a pressing issue in Chinese urban areas, posing significant health risks and leading to excess deaths annually. Extreme high temperatures, influenced by climate change, aggravates ozone formation by affecting both natural emissions and photochemical processes. This study utilizes the Community Multi-scale Air Quality (CMAQ) model to examine the influence of extreme high temperatures on ozone formation in urban areas in China. High-temperature periods during the summers of 2022 and 2023 are selected for simulations over key city clusters in priority regions for air pollution control, and results are validated against observations. Sensitivity experiments are also performed to quantify the contributions of high temperatures to ozone concentrations through atmospheric chemical processes and biogenic volatile organic compound (BVOC) emissions, respectively. The research will provide insights into the spatiotemporal distribution and primary formation pathways of ozone during extreme high temperature events.
Session Chair(s): Jayant NIRMALKAR, Jeonbuk National University, Shantanu Kumar PANI, National Central University
AS64-A004
Impacts of Springtime Biomass-burning Aerosols in Northern Peninsular Southeast Asia and the Western North Pacific: An Overview
Shantanu Kumar PANI#+, Neng-Huei (George) LIN
National Central University
Open biomass-burning (BB) occurs almost every year with varying intensities during the dry season (February–April) in northern peninsular Southeast Asia (PSEA; here defined as Myanmar, Laos, Thailand, Vietnam, and Cambodia), in the form of forest fires and agricultural-waste burning, and emits a substantial amount of aerosols and trace gases into the atmosphere. The impact of northern PSEA BB on air quality, atmospheric chemistry, and regional climate was investigated through the integration of in-situ measurements, remote sensing retrievals, and modeling tools over the source region as well as at transboundary locations including the South China Sea and western Pacific region within the framework of the Seven South East Asian Studies (7-SEAS) mission. For instance, severe haze (visibility ≈ 4 km) due to severe BB loadings (the contribution of BB to ambient PM2.5 ≈ 79%) in Chiang Mai, during the spring of 2014, under favorable meteorology can significantly impact the local air quality and public health; moreover, the resulting enhancement in atmospheric heating (as high as 3.6 kelvin per day) could potentially influence the regional radiation budget. Large surface cooling (up to -30.8 W m-2) and atmospheric warming (up to +21.3 W m-2) quantified based on ground-based observations at Lulin Atmospheric Background Station (a high-altitude remote site in the western North Pacific; 2862 m above mean sea level) due to the absorption by BB-induced aerosols, could potentially influence the regional climate.
AS64-A002
Evaluation of the Impact of Springtime Biomass Burning Activities in the Continental Southeast Asia on CO2 and CH4 in the Western Pacific
Chang-Feng OU-YANG1#+, Jia-Lin WANG1, Chia-Ching LIN1, Jia-Yang CHIU1, Wen-Tzu LIU2, Neng-Huei (George) LIN1
1National Central University, 2Chung Yuan Christian University
Carbon dioxide (CO2) and methane (CH4) are the two largest contributors of the well-mixed greenhouse gases (GHGs) in the atmosphere. In every spring, crop residue burning and forest fires contribute to significant emissions of GHGs in Southeast Asia. The emitted GHGs can further enter the Pacific via long-range transport by westerlies. In this study, the measurements of CO2 and CH4 a high-altitude station (Lulin Atmospheric Background Station, LLN, 23.47°N, 120.87°E, 2,862 m ASL) from December 2010 to March 2019 were employed to assess the impact of the springtime biomass burning in the Southeast Asia Peninsula on the two GHGs in the western Pacific. Based on HYSPLIT backward trajectory analysis, the enhancement of CO2 and CH4 were estimated to be approximately 1.5 ppm and 15.1 ppb, respectively, whereas CO was increased by about 22.0 ppb. The potential source areas for LLN as the receptor site in the western Pacific were determined using the concentration weighted trajectory (CWT) algorithm. The CWT patterns of CO2 and CH4 are generally alike. Positive impacts on CO2 and CH4 are revealed along the westerlies passing through the areas covering southern China and Thailand, with few air flows on the western Pacific originated from eastern coastal China. In contrast, a negative contribution on the GHGs from the southern SEA, SCS, and the Pacific was suggested.
AS64-A001
Biomass Burning Effects on Organic Aerosols and PM2.5 Across Northeast Asia
Jayant NIRMALKAR1+, Jiyi LEE2, Kwangyul LEE3, Jun-Young AHN3, Qiu YANTING4, Zhijun WU4, Natsagdorj AMGALAN5, Kyoung-Soon JANG6, Changhyuk KIM7, Mijung SONG1#
1Jeonbuk National University, 2Ewha Womans University, 3National Institute of Environmental Research, 4Peking University, 5National University of Mongolia, 6Korea Basic Science Institute, 7Pusan National University
Biomass burning (BB) emerges as a substantial contributor of toxic organic compounds in PM2.5, exerting a considerable impact on air quality in Northeast Asia. Consequently, accurately quantifying organic carbon from biomass burning (OCBB) is imperative for devising effective mitigation strategies. In the period of March-April 2022, PM2.5 samples collected from Seoul (SL), Seosan (SS), Beijing (BJ), and Ulaanbaatar (UB) underwent analysis for BB markers, such as levoglucosan, mannosan and K+. BB fuel was determined through the analysis of levoglucosan/mannosan and levoglucosan/K+ ratios, while the identification of OCBB involved measuring levoglucosan and optimizing the levoglucosan/OC ratio. The results revealed considerable variations in OCBB contributions among the different sites: SL (27±17%), SS (60±24%), BJ (5±3%), and UB (50±17%). Notably, UB and SS exhibited the highest levels of levoglucosan and OCBB, indicating a pronounced impact of BB in these regions. Through the application of Cluster and Potential Source Contribution Function analyses, it was elucidated that aerosols in UB were affected by local sources and long-range transport (LRT) from northwest (NW) regions. In contrast, SS showed an impact from aged, regional, and LRT aerosols originating from both NW and southern directions.
AS64-A003
Exploring the Impacts of Biomass Burning Aerosols on Monsoon System in East Asia with a Global Variable-resolution Model
Chen JIN#+, Chun ZHAO, Weichen LIU, Jiawang FENG, Jun GU
University of Science and Technology of China
The East Asian monsoon system is a vital component of the global atmospheric circulation, and serves as a primary driver of rainfall in East Asia, playing a crucial role in agricultural production and ecosystems in the region. Biomass burning emission, through aerosol-radiation-cloud interactions, alters the atmospheric temperature, stability, and cloud within the East Asian monsoon system, thereby impacting precipitation patterns and wind field distribution. Numerical simulation of biomass burning and its impacts at regional scale still have large uncertainties, partly due to the relatively coarse horizontal resolution. Limited-area simulations at relatively high-resolution can generally better describe the regional-scale impacts of biomass burning but the impacts can be constrained due to lateral boundary forcing. In this study, a novel modeling framework of biomass burning and its feedbacks with the capability of global variable-resolution simulation is established and utilized. An evaluation of biomass burning aerosols simulated by the model is conducted and the East Asian region is subjected to grid refinement. We employ this model to simulate and analyze the effects of biomass burning and aerosol-boundary-layer-monsoon interactions on monsoon system in East Asia.
Session Chair(s): Qi TANG, Lawrence Livermore National Laboratory, Myung-Seo KOO, Korea Institute of Atmospheric Prediction Systems
AS26-A016
| Invited
Responses of Global Energy and Water Cycles to Key Climate Forcings: Comparative Analysis of LMIP, AMIP, and CMIP in LS3MIP/CMIP6
Hyungjun KIM1,2#+
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo
Atmosphere, ocean, and land are the key components of Earth’s climate system. Their interactions, primarily through the exchange of energy and materials, notably water and carbon, are crucial. Accurate representations of these components and their exchanges within the Earth System Model (ESM) are essential for deepening our understanding of this vast and complex system. The Coupled Model Intercomparison Project (CMIP) plays an important role in providing fundamental climate information, widely utilized by the earth system science community and society at large. As a satellite MIP of CMIP6, the Land Surface, Snow, and Soil-moisture Model Intercomparison Project (LS3MIP) offers a comprehensive assessment of terrestrial processes and diagnoses systematic biases in the land surface models of ESMs. However, the sensitivity of these processes to key climate forcings, specifically the influences of atmosphere and ocean, has not yet been comparatively studied. In this study, we conducted a multi-model-based intercomparison of land-only (LMIP), atmosphere and land-only (AMIP), and fully coupled (CMIP) experiments. This was to assess the distinct effects of the key climate components (i.e., atmosphere, ocean, land) on the performance of ESMs, focusing on the surface energy and water budgets and their global variabilities. In general, the LMIP configuration showed significant performance improvements in major variables including net radiation, evapotranspiration, and runoff for mean bias and temporal variability. In contrast, the differences between AMIP and CMIP for these variables were not substantial. Surprisingly, prescribed sea surface temperature was not effective in reproducing the temporal variability of such variables including precipitation. These findings support that the ocean forcing to terrestrial energy and water cycle is rather weaker than that of the atmosphere in terms of the long-term mean state. Furthermore, they imply that the representation of the atmosphere in state-of-the-art ESMs remains a primary bottleneck toward significant advancements in earth system simulations.
AS26-A001
Tibetan Plateau Soil Temperature are Found to be the First-order Source of Subseasonal-to-seasonal Precipitation Predictability Regionally and Globally: The GEWEX/LS4P Initiative
Yongkang XUE1#+, Aaron BOONE2, Tandong YAO3, Qi TANG4, LS4P TEAM5
1University of California, Los Angeles, 2Meteo France, 3Chinese Academy of Sciences, 4Lawrence Livermore National Laboratory, 5Global Energy and Water Exchanges (GEWEX)
This paper presents a new idea that utilizes information on boreal spring land surface temperature/subsurface temperature (LST/SUBT) anomalies over the Tibetan Plateau (TP) to improve prediction of subsequent summer droughts/floods over several regions over the world, East Asia and North America in particular. The work was performed in the framework of the GEWEX/LS4P Initiative. The LS4P Phase I (LS4P-I) experiment focused on the TP LST/SUBT contribution for subseasonal-to-seasonal (S2S) predictability. The summer 2003, when there was a severe drought/flood over the southern/northern part of the Yangtze River basin, respectively, has been selected as the focus case. More than forty institutions worldwide have participated in this effort, many of which are the major climate/weather centers. Observational evidence of land memory and a statistically significant lag relationship between spring TP LST and summer precipitation were found. With the newly developed LS4P initialization method for TP land temperature, the observed surface temperature anomaly over the TP has been partially produced by the LS4P-I model ensemble mean, and 8 hotspot regions in the world were identified where June precipitation is significantly associated with anomalies of May TP land temperature. Consideration of the TP LST/SUBT effect has produced about 25%-50% of observed precipitation anomalies in most hotspot regions, compatible to the sea surface temperature effect in its hot spot regions. The analysis based on observation reveals an out-of-phase relationship between the TP surface temperature and Rocky Mountains (RM) surface temperature. A TP- RM Circumglobal (TRC) wave train has also been identified. This study suggests that the TP LST/SUBT effect is a first-order source of S2S precipitation predictability, comparable in magnitude to that of the SST effect. With the completion of the LS4P-I, the LS4P-II has been launched and is briefly presented.
AS26-A004
| Invited
Near-global Summer Circulation Response to the Spring Surface Temperature Anomaly in Tibetan Plateau – The GEWEX/LS4P First Phase Experiment
Yang ZHANG+
Nanjing University
Subseasonal to seasonal (S2S) prediction of droughts and floods is one of the major challenges of weather and climate prediction. Recent studies suggest that the springtime land surface temperature/subsurface temperature (LST/SUBT) over the Tibetan Plateau (TP) can be a new source of S2S predictability. The project “Impact of Initialized Land Surface Temperature and Snowpack on Subseasonal to Seasonal Prediction (LS4P)” was initiated to study the impact of springtime LST/SUBT anomalies over high mountain areas on summertime precipitation predictions. The present work explores the simulated global scale response of the atmospheric circulation to the springtime TP land surface cooling by 16 current state-of-the-art Earth System Models (ESMs) participating in the LS4P Phase I (LS4P-I) experiment. The LS4P-I results show, for the first time, that springtime TP surface anomalies can modulate a persistent quasi-barotropic Tibetan Plateau-Rocky Mountain Circumglobal (TRC) wave train from the TP via the northeast Asia and Bering Strait to the western part of the North America, along with the springtime westerly jet from TP across the whole North Pacific basin. The TRC wave train modulated by the TP thermal anomaly play a critical role on the early summer surface air temperature and precipitation anomalies in the regions along the wave train, especially over the northwest North America and the southern Great Plains. The participant models that fail in capturing the TRC wave train greatly under-predict climate anomalies in reference to observations and the successful models. Furthermore, the TP surface temperature anomaly can influence the Southern Hemispheric circulation by generating cross-equator wave trains. More dynamical understanding of the TRC wave train as well as its cross-equator propagation into the Southern Hemisphere will be explored in the newly launched LS4P phase II experiment.
AS26-A003
Improve Climate Model Subseasonal-to-seasonal Precipitation Prediction with Nudging Approach
Qi TANG1#+, Yi QIN2, Yongkang XUE3
1Lawrence Livermore National Laboratory, 2Pacific Northwest National Laboratory, 3University of California, Los Angeles
High fidelity subseasonal-to-seasonal (S2S) precipitation prediction has been highly desired due to its great socioeconomical implications, yet it remains one of the most challenging topics in the weather/climate prediction studies. As part of the Impact of Initialized Land Temperature and Snowpack on Sub-seasonal to Seasonal Prediction (LS4P) project of the Global Energy and Water Exchanges (GEWEX) program, twenty-one climate models follow the LS4P phase I protocol to quantify the impact of the Tibetan Plateau (TP) land surface temperature/subsurface temperature (LST/SUBT) springtime anomalies on the global summertime precipitation. We find that nudging towards reanalysis winds is necessary for climate models to generate atmosphere and land surface initial conditions close to observations. Relative to those initialized with free runs, simulations with the nudged initial conditions can better capture the summer precipitation responses to the imposed TP LST/SUBT spring anomalies at hotspot regions globally. Further analyses show that the enhanced S2S prediction skill is largely attributable to the substantially improved initialization of the Tibetan Plateau-Rocky Mountain Circumglobal (TRC) wave train pattern in the atmosphere. This study highlights the important role that initial condition plays in the S2S prediction and suggests that data assimilation technique (e.g., nudging) should be adopted to initialize climate models for their S2S prediction simulations. In addition, we will discuss the initial results of LS4P phase II using the U.S. Department of Energy, Energy Exascale Earth System Model (E3SM) and its differences from phase I.
AS26-A012
Impacts of Tripolar Snow Anomalies Over the Tibetan Plateau on Northern Hemisphere Atmospheric Circulation in Winter
Wen LUO1+, Qigang WU2#, Yang ZHANG1, Shizuo LIU3
1Nanjing University, 2Fudan University, 3Duke University
Tibetan Plateau (TP) snow cover anomalies show considerable diversity in autumn and winter. The leading EOF mode (EOF1) of anomalous TP snow cover extent (SCE) in autumn-winter is characterized by a uniformly increased or decreased SCE over the whole plateau, which can trigger a wintertime Pacific-North American (PNA)-like atmospheric response as demonstrated in observational and numerical studies. In present study, the EOF2 modes of TP SCE anomaly from autumn to winter show similar zonal tripolar structures with the increased SCE over the northwestern and eastern TP and decreased SCE over the central TP. This TP SCE tripolar pattern exhibits strong co-variability of SCE anomalies in Europe and Lake Baikal. Regression analysis indicates that the above EOF2 mode from autumn to winter is significantly correlated to a high-latitude wave train in winter from the North Atlantic to western Europe, northern Eurasia to northeastern China, and substantial cooling in northeast China and warming in Siberia and the Arctic in winter. Numerical experiments with EOF2-like SCE forcing in TP and synergic SCE changes over Europe and Lake Baikal reproduce the regression pattern of sea level pressure and 500hPa geopotential height on the PC2 time series and confirm the joint effects of snow anomalies over the above three regions. Such TP SCE EOF2 mode–atmosphere relationship may present an additional potential for wintertime predictability.
AS26-A014
Enhancing Long-term Predictive Capabilities: Integrating River Routing Into Earth System Models for Improved Forecasting Mee-Hyun Cho
Mee-Hyun CHO#+
Korea Institute of Atmospheric Prediction Systems
Korea Institute of Atmospheric Prediction Systems (KIAPS) endeavors to advance predictive capabilities beyond the typical two-week horizon by developing a novel integrated model that amalgamates components crucial to the Earth system, specifically oceans, sea ice, and river routing. While rivers constitute pivotal elements within the global hydrological cycle, they have conventionally been neglected in mid-range forecasting. However, their significance increases in long-term predictions concerning the water balance of the Earth system. The river routing model takes land surface model runoff as input and simulates the flow and discharge of rivers, playing a crucial role in exporting freshwater into the oceans. This research coupled the CaMa-Flood model with the Korean Integrated Model (KIM) developed by the KIAPS and analyzes its impact on simulation performance. To evaluate the appropriateness of the integration, the runoff simulated by KIM's surface model is compared with observed runoff and reanalysis data, verifying horizontal distribution and seasonal variations. Additionally, the study examines how freshwater discharge from rivers in the coupled model affects sea surface temperature, salinity, and sea ice distribution in the oceans. Particularly, the impact of the CaMa-Flood integration on polar temperatures in the winter hemisphere and its relevance to climate variability are analyzed. Future endeavors involve refining freshwater discharge into the oceans and evaluating its impact on extreme weather phenomena such as typhoons and polar weather anomalies. Acknowledgements. This work was carried out through the R&D project “Development of a Next-Generation Numerical Weather Prediction Model by the Korea Institute of Atmospheric Prediction Systems (KIAPS)”, funded by the Korea Meteorological Administration (KMA2020-02212).
Session Chair(s): Yiping WU, Central South University of Forestry and Technology, Shuguang LIU, Central South University of Forestry and Technology, Georgii ALEXANDROV, Russian Academy of Sciences
BG06-A012
| Invited
The Exposure of Carbon Stocks in Post-agricultural Ecosystems of the Chinese Loess Plateau and the Central Russian Plain to Climate Change Impacts
Yiping WU1#+, Georgii ALEXANDROV2, Shuguang LIU1, Alexey V. ELISEEV2, Alexander CHERNOKULSKY3
1Central South University of Forestry and Technology, 2Russian Academy of Sciences, 3Obukhov Institute of Atmospheric Physics, Russian Academy of Sciences
Post-agricultural ecosystems of the Chinese Loess Plateau and the Central Russian Plain are the human-induced carbon sinks whose potential is well realized under present climate. To evaluate their potential under changing climate we need a better understanding of their exposure to climate change impacts. The forests that regrew on the croplands abandoned after the collapse of Soviet Union and the forests that were planted in the course of the Grain-for-Green program in China are sequestering carbon from the atmosphere and accumulating it in soil organic matter and tree biomass. How long they could provide such ecosystem service depends on how they would be managed. The optimal management of these forests must take into account the impact of climate change. The impact of climate change on the carbon sequestration potential of post-agricultural ecosystems can be evaluated by use of Earth System Model (ESM) runs, although these ecosystems are not well represented in ESMs. The analysis of ESM runs revealed a substantial uncertainty in the projections of climate change impact on the net ecosystem production in the Chinese Loess Plateau and the Central Russian Plain. Since this uncertainty can be partly attributed to the uncertainty in the projections of precipitation change, the management of the post-agricultural forests should employ an adaptive approach to allow smooth switching between the strategies developed for various scenarios of precipitation change.
BG06-A008
Anomalous Net Biome Exchange Over Amazonian Rainforests Induced by the 2015/16 El Niño: Soil Dryness-shaped Spatial Pattern But Temperature-dominated Total Flux
Jun WANG1#+, Ning ZENG2, Meirong WANG3
1Nanjing University, 2University of Maryland, 3Nanjing University of Information Science & Technology
The magnitude and spatial pattern of anomalous net biome exchange (NBE) induced by the 2015/16 El Niño over Amazonian rainforests remain uncertain. We here investigated them using multi-model posterior NBE products in the Orbiting Carbon Observatory-2 (OCO-2) version 10 modeling intercomparison project (MIP). Results suggest that relative to the annual NBE average in 2017/18, larger anomalous carbon release occurred over the eastern and northern Amazonian rainforests in 2015/16, with a total flux of approximately 0.4 PgC yr–1 after assimilating satellite-observed column CO2 concentrations (XCO2) over land. We further find that this anomalous spatial pattern was predominantly determined by soil dryness, while the total positive NBE anomaly was dominated by higher temperature with its contribution of approximately 68~70%. We believe that atmospheric inversions assimilating more satellite-observed XCO2 in future can provide us more comprehensive understanding how Amazonian rainforests cope with the abiotic stresses induced by El Niño events.
BG06-A009
Coupled Simulation of Atmospheric CO2 in CAS-ESM2.0
Jiawen ZHU#+
Chinese Academy of Sciences
Atmospheric carbon dioxide (CO2) concentration is increasing rapidly since the Industrial Revolution, which has led to unequivocal global warming and crucial environmental change. It is extremely important to investigate interactions among atmospheric CO2, physical climate system and carbon cycle in underlying surface for a better understanding the Earth system. Earth system models are widely used to investigate these interactions by a coupled carbon-climate simulation. The Chinese Academy of Sciences Earth System Model version 2 (CAS-ESM2) has successfully fixed a two-way coupling of atmospheric CO2 with climate and carbon cycle in land and ocean. Using CAS-ESM2, we conducted a coupled carbon-climate simulation by following the CMIP6 proposal of historical emission-driven experiment. This study examines the modeled CO2 by a comparison to observed CO2 in sites Mauna Loa and Barrow, the Greenhouse Gases Observing Satellite (GOSAT) CO2 product. The compared results show that CAS-ESM2 agrees very well with observations in reproducing the increasing trend of annual CO2 during the period 1850−2014 and in capturing the seasonal cycle of CO2 in the two baseline sites, as well as over northern high latitudes. These agreements illustrate a good ability of CAS-ESM2 in simulating carbon-climate interactions, even though uncertainties remain in the processes. This study reports an important stage of the development of CAS-ESM with the carbon and climate coupled, and this coupling will provide significant scientific supports for climate research and China’s goal of carbon neutrality.
BG06-A003
Doubling of Annual Forest Carbon Loss Over the Tropics During the Early 21st Century
Yu FENG1#+, Zhenzhong ZENG2, Ji CHEN3, Chunmiao ZHENG1
1Eastern Institute of Technology, 2Southern University of Science and Technology, 3The University of Hong Kong
Previous estimates of tropical forest carbon loss in the 21st century using satellite data typically focus on its magnitude, whereas regional loss trajectories and associated drivers are rarely reported. Here, we used different high-resolution satellite datasets to show a doubling of gross tropical forest carbon loss (due to forest loss) worldwide from 0.97 ±0.16 Pg C yr-1 in 2001–2005 to 1.99 ±0.13 Pg C yr-1 in 2015–2019. This increase in carbon loss from forest conversion is higher than in bookkeeping models forced by land-use statistical data which show no trend or a slight decline in land-use emissions in the early 21st century. Most (82%) of the forest carbon loss is triggered by large-scale commodity or small-scale agriculture activities, particularly in Africa and Southeast Asia. We find that ~70% of former forest lands converted to agriculture in 2001–2019 remained so in 2020, confirming a dominant role of agriculture in long-term pan-tropical carbon reductions on formerly forested landscapes. The acceleration and high rate of forest carbon loss in the 21st century suggest that existing strategies to reduce forest loss are not successful, and underscore the importance of monitoring deforestation trends following the new pledges made in Glasgow.
BG06-A011
Exploring Riverine Chemical Fluxes and Weathering Processes in Sarawak, Malaysian Borneo
Chris Tsz Long CHEUNG1#+, Ryan MCKENZIE1, Brian BEATY2, Giancarlo DEFRANCESCO1, Dan ASAEL2, Noah PLANAVSKY2, Sharveen RAVICHANDRAN3, Abdulmajid Muhammad ALI3, Ramasamy NAGARAJAN3
1The University of Hong Kong, 2Yale University, 3Curtin University Malaysia
The weathering of silicate minerals on continents regulates atmospheric CO2 over multimillion-year timescales. An important means to study silicate weathering processes is via the study of river chemistry. Southeast Asia features highly favorable conditions for chemical weathering on Earth’s surface; however, river systems in this region remain relatively understudied. Here, we present new elemental, Li isotopic (d7Li), and clay mineralogical data from 24 riverine localities across the state of Sarawak, Malaysian Borneo, sampled during both the wet and dry seasons. Our results exhibit a broad spectrum of d7Lidiss values spanning from 7.6 – 33.7‰. More specifically, for samples located in the western Kuching zone, d7Lidiss values range from 7.6 – 32.5‰ (n = 22) with a mean value of 17.0‰. Conversely, samples located in the eastern Miri and Sibu zones have d7Lidiss values ranging from 20.3 – 33.7‰ (n = 18) with a mean value of 26.9‰. This variation is attributed to differences in topography and weathering regimes, with flat floodplains dominating the Miri and Sibu zones. This would lead to increased soil development and clay formation, therefore driving the heavy d7Lidiss values. This contrasts with the higher topographic relief in the Kuching zone, where soil development would be more limited with greater runoff. Our lithium isotopic data also shows seasonal trends with almost all samples having heavier dissolved values in the dry season. This behaviour reflects a hydrological control on riverine d7Lidiss values with river discharge affecting water-clay residence times and thus Li fractionation. The largest river in Sarawak, the Rajang River, features the heaviest d7Lidiss value at +33.7‰. This is markedly heavier than the currently known global riverine average of +23‰ and notably closer to the global seawater value of +31‰, thus highlighting the potential for Southeast Asian rivers to deliver heavy Li isotopes to the ocean.
BG06-A010
Satellite-based Sun-induced Chlorophyll Fluorescence and Spectral Reflectance Improve the Terrestrial Biospheric CO2 Flux Estimates in India : Special Focus on the Climate Extremes
Aparnna RAVI P#+, Dhanyalekshmi K. PILLAI
Indian Institute of Science Education and Research, Bhopal
Accurate quantification of regional terrestrial fluxes is essential to enhance our understanding of ecosystem carbon sequestration potential, functioning, and the demand for emission reduction. The challenges in this quantification, particularly in regions with substantial observation gaps, prompt an examination of the potential of satellite missions like TROPOMI and OCO-2. These missions provide retrievals of Solar-Induced chlorophyll Fluorescence (SIF) to improve the estimation of terrestrial biosphere CO2 fluxes in India. The study presents enhanced hourly distributions of Gross Primary Productivity (GPP) and Net Ecosystem Exchange (NEE) on a high-resolution grid employing a data-driven approach with the Vegetation Photosynthesis and Respiration Model (VPRM), which is calibrated using the SIF-GPP relationship to improve model performance. The refinement of VPRM's ecosystem respiration by incorporating soil temperature and soil moisture further enhances the model's accuracy. The study concludes that satellite-based SIF data products can potentially inform ecosystem-scale vegetation responses across biomes in India. Simultaneously, the study addresses the observed increasing trend in climate extremes, highlighting the significant influence of drought as a widely observed extreme event on terrestrial ecosystem functioning and the carbon balance. Acknowledging the importance of interannual variability in Indian summer monsoon (ISM) rainfall, which provides 90 percent of the country's annual precipitation, the study aims to identify the impact of drought on terrestrial biosphere carbon processes and the national carbon budget. Employing various meteorological datasets and CO2 flux data from inversion, process-based, and LUE-based models, alongside satellite-derived SIF and eddy covariance flux observations, the comprehensive study quantifies the impact of extreme events on ecosystem behavior and atmosphere-biosphere CO2 exchange fluxes over the Indian region. Preliminary results will be presented and discussed, contributing valuable insights for planning mitigation strategies and policymaking in the context of climate change.
BG06-A019
Evaluation of High-resolution Global Primary Productivity and Evapotranspiration Products Derived from Enhanced BESS Model and GCOM-C SGLI Datasets
Shuai SHAO#+, Kazuhito ICHII, Hase MISAKI
Chiba University
Remoted-sensing-based global carbon flux products derived by terrestrial model has been gaining prominence in recent years for its both vast coverage of in-time land observation and wide consideration of multi atmosphere, vegetation and soil systems and associated fluxes. Breathing Earth System simulator (BESS), a process-based model, has been proved as an advanced diagnostic terrestrial model which considers atmospheric radiative transfer, canopy radiative transfer, photosynthesis, evaporation and soil evaporation. Despite its sophistication, BESS still encounters significant uncertainties, which may be addressed by incorporating high spatiotemporal resolution datasets. This study focuses on enhancing the BESS model using data from the GCOM-C SGLI satellite, launched by JAXA in December 2017. The satellite provides medium spatial resolution (250m to 1km) and operates in multiple spectral bands, aiming to advance the understanding of climate and carbon cycle changes. Our proposed enhancement of the BESS model involves quantifying global gross primary productivity (GPP) and evapotranspiration (ET) using GCOM-C SGLI data with a spatial resolution of 250m and a temporal resolution of 8 days, spanning 2018 to 2022. The study utilizes several SGLI products such as land surface temperature (LST), albedo, leaf area index (LAI), and shortwave radiation (SWR) as model inputs. The expected outputs are to align consistently with existing data from AsiaFlux and FLUXNET sites, based on the performance of our current 5km resolution products. This enhanced product is projected to be available in near-real time on the JAXA website, contributing to the field of global carbon flux estimation.
BG06-A007
Understanding Vegetation Growth Responses to Climate Change and Its Drivers: From Site to Regional Scales
Wenxi TANG1+, Shuguang LIU2#
1Hainan University, 2Central South University of Forestry and Technology
Vegetation growth is affected by past growth rates and climate variability. However, the duration and intensity of this carryover and time-lag effect on ecosystem dynamics relative to that of concurrent environmental drivers remains poorly understood. Insufficient comprehension of time-lag effects from biological and global changes hampers cross-scale biogeochemical model predictions. Here, we show that vegetation growth carryover (VGC) (defined as the effect of current vegetation conditions on subsequent growth) and lagged climatic effects (LCE) (defined as the effect of past climatic conditions) vary significantly between sites and regional scales. We used the vector autoregressive model (VAR) to analyze the VGC and LCE on tree-ring growth and satellite vegetation indicators, predict vegetation responses to future global change, and validate its accuracy. Results showed that at the site scale, vegetation growth in subtropical forests is dominated by the VGC effect. Tree-ring growth is decoupled from canopy condition with a time-lag, and tree ring growth shows species-specific LCE and VGC effects. In 32 major cities of China (regional scale), the strongest and longest LCE on vegetation greenness was due to relative humidity, while the shortest and weakest was due to evapotranspiration. The LCE of precipitation and sunshine duration on vegetation greenness were stronger in the south than in the north. The vegetation greenness predicted by the VAR model was highly consistent with the observed vegetation greenness (root mean squared error, RMSE < 0.08), and the prediction accuracy generally improved by 23.43% compared with the vegetation greenness predicted by the multiple linear regression model. Our study highlights the necessity of considering carryover and time-lag effects when exploring vegetation-climate interaction. The methods developed in this study can be used to reveal the lagged effects on vegetation growth and improve prediction of vegetation dynamics under climate variability.
Session Chair(s): Forrest HOFFMAN, Oak Ridge National Laboratory
BG05-A011
Greening of Human-dominated Ecosystems in India
Taejin PARK1#+, Murali GUMMA2, Weile WANG1, Sunil DUBEY3, Ramakrishna NEMANI1, Pranay PANJALA2
1NASA Ames Research Center, 2International Crop Research Institute for Semi-Arid Tropics, 3Mahalanobis National Crop Forecast Centre
Satellite data show the Earth has been greening and identify croplands in India as one of the most prominent greening hotspots. Though India’s agriculture has been dependent on irrigation enhancement to reduce crop water stress and increase production, the spatiotemporal dynamics of how irrigation influenced the satellite observed greenness remains unclear. Here, we use satellite-derived leaf area data and survey-based agricultural statistics together with results from state-of-the-art Land Surface Models (LSM) to investigate the role of irrigation in the greening of India’s croplands. We find that satellite observations provide multiple lines of evidence showing strong contributions of irrigation to significant greening during dry season and in drier environments. The national statistics support irrigation-driven yield enhancement and increased dry season cropping intensity. These suggest a continuous shift in India’s agriculture toward an irrigation-driven dry season cropping system and confirm the importance of land management in the greening phenomenon. However, the LSMs identify CO2 fertilization as a primary driver of greening whereas land use and management have marginal impacts on the simulated leaf area changes. This finding urges a closer collaboration of the modeling, Earth observation, and land system science communities to improve representation of land management in the Earth system modeling.
BG05-A010
Changes in Leaf and Root Carbon Allocation of Global Vegetation Simulated by the Optimally Integrated Ecosystem Models
Zeyu DUANMU+, Zaichun ZHU#
Peking University
Vegetation carbon allocation, which is sensitive to environmental changes, plays a vital role in regulating the global carbon cycle. However, the response of leaf and root carbon allocation to the dramatically changing environment of global vegetation is still unclear owing to the limited observations. Ecosystem models, although they still suffer from significant uncertainties, are the only available tools that provide valuable insights into the spatiotemporal patterns of global vegetation carbon allocation in response to global environmental changes. In this study, we assessed the performance of seven ecosystem models that participated in TRENDY v8 in simulating global variations in leaf and root carbon. Based on their performance, we developed optimally integrated ecosystem models (OIM) and quantified the changes in the global allocation of root and leaf carbon and the critical drivers from 1982 to 2018. The OIM was generally successful in reproducing the broad shape of root carbon in climate and the spatiotemporal distribution of leaf carbon. The OIM suggested that global vegetation allocated more carbon to roots compared with leaves (root/leaf carbon allocation). Elevated atmospheric CO2 concentrations accounted for the large root/leaf carbon allocation globally, particularly in tropical regions and the northern high latitudes, and the CO2 effects on root/leaf carbon allocation increased with mean annual precipitation. Climate change had similar effects as CO2 concentrations on root/leaf carbon allocation in the northern hemisphere but increased allocation to leaves in tropical regions. Land cover and land use change increased the allocation to leaves. Overall, we tentatively quantified the changes in the carbon allocation to the leaf and root across global terrestrial vegetation under the dramatic global environmental change based on OIM, which could help in-depth understanding of the changes in the functioning of the terrestrial ecosystem and reasonable projection of changes in the future global carbon cycle.
BG05-A002
Benchmarking Soil Moisture and Ecohydrologic Interactions in Earth System Models
Elias MASSOUD1#+, Forrest HOFFMAN1,2, Jiafu MAO1, Yaoping WANG1
1Oak Ridge National Laboratory, 2University of Tennessee, Knoxville
Soil moisture is a key Earth system process, and it helps control the storage and movement of water, carbon, and energy throughout the globe. Earth System Models (ESM) simulate the biogeochemical and hydrological cycles and how soil moisture interacts with other processes. It is important to benchmark how these ecohydrologic processes are represented in ESMs. In this work, we evaluate the ability of models to capture relationships between soil moisture and other processes such as gross primary production, leaf area index, and evapotranspiration. Preliminary results show there is a divergence in how these relationships are represented in the high latitude regions between different models. This effort stems from the United States Department of Energy’s (DOE) RUBISCO project Soil Moisture Working Group (SMWG), which was recently organized to advance the understanding of soil moisture and its interactions with the biogeochemical and hydrological cycles in the Earth system. This presentation will discuss and summarize the activities and results from the ecohydrology benchmarking subtask in the RUBISCO SMWG and will provide details on current progress and future directions.
BG05-A003
Global Gross Primary Production and Transpiration Data Products During 2000-2022 as Simulated by the Vegetation Photosynthesis Model (v3.0), Vegetation Transpiration Model (v2.0), MODIS Images, and ERA5 Climate Data
Xiangming XIAO#+, Li PAN, Baihong PAN, Cheng MENG
The University of Oklahoma
Gross primary production (GPP) and transpiration (T) are closely coupled through individual leaves. To date, substantial progress has been made in estimating GPP and evapotranspiration (ET) at ecosystem and landscape scales, and several global GPP and evapotranspiration datasets from various data-driven models and process-based models are available to the public. However, these global models and their data products still have moderate to large uncertainties. This presentation is composed of three parts. First, we will introduce the Vegetation Photosynthesis Model (v3.0) and Vegetation Transpiration Model (v2.0). VPM estimates daily GPP (g C/m2/day) as a product of the amount of light absorbed by chlorophyll (APARchl) and light use efficiency. The major improvement of VPM v3.0 include (1) leaf traits (broadleaf vs needleleaf) for estimating light absorption, and (2) site-specific optimal air temperature for GPP (Topt-site). VTM estimates daily transpiration (mm H2O/day) as a product of daily GPP and transpiration ratio, which is estimated as an inverse of water use efficiency at the leaf level. Second, we will introduce the results of VPM (v3.0) and VTM (v2.0) simulations over many eddy covariance tower sites as part of our effort for model accuracy and uncertainty evaluation. The comparisons between predicted GPPVPM and TVTM estimates and GPPEC and ETEC from the eddy covariance tower sites are carried out. Third, we will introduce the global GPP and T data products from VPM and VTM simulations with MODIS images and ERA5 climate dataset over the period of 2000-2022. The resultant global GPP and T data products over 2000-2022 could be used for many applications that have significant societal benefits, including ecosystem goods and services, food and water security, and the United Nations Sustainability Development Goals.
BG05-A008
Challenges in Quantifying Global Biogenic Methane Emissions from Land and Freshwater Ecosystems
Qianlai ZHUANG#+
Purdue University
Land and freshwater ecosystems play a significant role in affecting the global methane budget. With future warming, the increase of methane emissions could create large positive feedbacks to the global climate system. We have used observation data of methane fluxes from diverse land and freshwater ecosystems to calibrate and evaluate extant land and freshwater biogeochemistry models of the Terrestrial Ecosystem Model (TEM) and the Arctic Lake Biogeochemistry Model (ALBM) to quantify the global methane emissions for the past few decades and the 21st century in a temporally and spatially explicit manner. Land ecosystems could emit methane from wetlands while uplands could uptake atmospheric methane. TEM simulates that global wetlands emissions are 212 ± 62 and 212 ± 32 Tg CH4 yr−1 due to uncertain parameters and wetland type distribution, respectively, during 2000–2012. After combining the global upland methane consumption of −34 to −46 Tg CH4 yr−1, we estimate that the global net land methane emissions are 149–176 Tg CH4 yr−1 due to uncertain wetland distribution and meteorological input. During 1950–2016, both wetland emissions and upland consumption increased during El Niño events and decreased during La Niña events. For freshwater ecosystems, we find that current emissions are 24.0 ± 8.4 Tg CH4 yr−1 from lakes larger than 0.1 km2. Future projections under the RCP8.5 scenario suggest a 58–86% growth in emissions from lakes. Warming enhanced methane oxidation in lake water can be an effective sink to reduce the net release from global lakes. Additionally, these studies identify the key biogeochemical and physical processes of controlling methane production, consumption, and transport in various hotspot emission regions. Our studies reveal the challenges to better constrain the quantification uncertainty of global biogenic methane emissions across the landscape.
BG05-A009
Enhanced Methane Emissions Linked to Influences of Microbial Activities and Edaphic Factors in Thawing Permafrost of Northern Norway
Jeong-eun YUN1,2+, Inge ALTHUIZEN3, Anja GRESCHKOWIAK4, Hanna LEE4, June-Yi LEE1, Hojeong KANG5#
1Pusan National University, 2Pusan National University, 3Norwegian Research Centre, 4Norwegian University of Science and Technology, 5Yonsei University
Sporadic permafrost is particularly vulnerable to climate warming due to rapid permafrost thaw. This permafrost thaw induces a gradient from palsas to ponds, leading to ecological succession in the landscape through the introduction of vegetation into both environments. Despite rapid landscape changes, the impacts of edaphic factors and vegetation on methane (CH4) flux, which is a significant greenhouse gas, in thawing permafrost are not fully understood. This study aimed to understand the impacts of edaphic factors and plants on CH4 flux and microbial net CH4 production along the thaw gradient during the growing season in northern Norway. We analyzed soil CH4 flux, soil properties, and active microbial abundance and communities through mRNA across the thaw gradient, including palsas, vegetated palsas, thaw slumps, ponds, and vegetated ponds. We observed an increase in CH4 flux along the thaw gradient during the growing season. In palsas, the presence of vegetation acted as a sink, reducing CH4 emissions to -1.17 mg m-2 d-1 compared to 1.7 mg m-2 d-1 in bare palsas. Conversely, the CH4 emissions in vegetated ponds were elevated to 141.9 mg m-2 d-1 compared to 115.75 mg m-2 d-1 in non-vegetated ponds, resulting in a 22.6% increase in CH4 emissions. The ratio of methanogens to methanotrophs, indicating net CH4 production ratio, increased from palsas to ponds. Our results indicate that the elevated net CH4 production ratio in vegetated ponds was driven by increased ammonium concentrations. The high ammonium concentrations in vegetated ponds contributed to enhancing both methanogens and methanotrophs, while simultaneously inhibiting methanotrophs from oxidizing CH4. These findings highlight the potential for increased CH4 emissions in changing landscapes due to permafrost thaw and the introduction of vegetation as a consequence of climate change, underscoring the need for continued monitoring of these vulnerable ecosystems.
Session Chair(s): Zhangcai QIN, Sun Yat-sen University, Umakant MISHRA, University of California Santa Cruz
BG01-A006
| Invited
Integrating Multiscale Data, Artificial Intelligence, and Earth System Model to Predict Environmental Feedback of Microbially-mediated Soil Carbon Dynamics
Yang SONG#+
The University of Arizona
Soil microbial communities are functionally diverse and collaboratively regulate environmental feedback of soil organic matter (SOM) decomposition to changing environments. However, quantifying the environmental feedback of soil microbial communities is still challenging due to the diversity of soil microbial functions and their interaction with the environmental feedback of soil physical and chemical processes. Moreover, it remains unclear to what extent this microbial functional feedback to the changing environment will affect large-scale soil carbon-environment feedback across space and time. To overcome these challenges, we leveraged artificial intelligence (AI) and gene-to-ecosystem data to quantify the responses of diverse microbial functions to changing environments. This quantitative information was then integrated into the Earth system model (ESM) to simulate the microbially-mediated soil decomposition process in response to environmental change. Our study highlighted that the omics-informed functional composition of soil microbial communities can serve as an indicator of integrated environmental regulations on soil carbon dynamics. Environmental regulation on the functional composition of soil microbial communities follows the resource optimization theory. Integrating AI-informed microbial functional dynamics with ESM can mitigate uncertainty in predicting the dynamics of soil carbon emission, especially in nutrient or water-limited environments.
BG01-A002
Predicting Soil Organic Carbon of China in the Future, the Role of Carbon Flux and a 1 KM Global Carbon Fluxes Dataset Using Machine Learning
Wei SHANGGUAN#+, Yongkun ZHANG, Feini HUANG, Xingjie LU, Zhangcai QIN
Sun Yat-sen University
The impact of carbon fluxes on soil organic carbon (SOC) remains underexplored. We employed machine learning to model SOC dynamics, leveraging a space-for-time substitution approach. Our findings project an increase in China's SOC through to the year 2100 across various Shared Socioeconomic Pathways. Sensitivity analyses have identified carbon fluxes as the main drivers for this projected rise, followed by climate change and land use change. Further examination using Explainable Artificial Intelligence has uncovered both spatial and temporal variations in how gross primary production (GPP) influences SOC levels. Notably, GPP's influence on SOC is initially negative at low levels, turning positive once a threshold of approximately 3 gC m-2d-1 is surpassed. Beyond a GPP of about 7 gC m-2d-1, its positive contribution to SOC plateaus. Critical zones for soil carbon sequestration are located around 400 mm annual precipitation line. We develops a new dataset called Global Carbon Fluxes Dataset (GCFD) with the resolution of 1 km. It provides high-resolution spatial and temporal information on gross primary productivity (GPP), terrestrial ecosystem respiration (RECO), and net ecosystem exchange (NEE). The accuracy and spatial details of GCFD are higher compared to other global carbon flux datasets, and it aligns well with remote sensing data on vegetation conditions. The GCFD can serve as a valuable reference for meteorological and ecological analyses, particularly in scenarios that require high-resolution carbon flux maps. GCFD can be accessed at https://dx.doi.org/DOI:10.11888/Terre.tpdc.300009.
BG01-A018
Biochar Converts Rice Paddies Into a Greenhouse Gas Sink
Piljoo KIM#+
Gyeongsang National University
Application of organic material to rice paddies improves soil quality and sequesters atmospheric carbon dioxide (CO2). However, organic amendments also increase methane (CH4) emissions. We compared the impact of organic amendments on net GWP by quantifying greenhouse gas fluxes and soil carbon (C) stock changes in a rice paddy. Most organic amendments increased seasonal CH4 fluxes by 7–30 Mg CO2-eq. ha-1 compared with controls (no organic matter addition). However, the small increases in soil C stock (9–11 Mg CO2-eq. ha-1) were insufficient to reduce the net GWP in these treatments. In contrast, biochar decreased greenhouse gas emissions and increased the soil C stock, leading to a large decrease in net GWP with no effect on rice production. Given that rice paddies account for about 11% of anthropogenic greenhouse gas emissions, the application of biochar could significantly reduce the contribution of flooded rice production to planetary warming.
BG01-A015
Iron Fertilization Effect of Blast Furnace Slag as Soil Amendment on Increasing Soil Carbon Stock Change in Rice Paddy
Lorraine Joule ESTRADA#+, Snowie Jane GALGO, Piljoo KIM
Gyeongsang National University
Blast furnace slag, a byproduct of iron production process hereafter, (silicate fertilizer) contains high amounts of Fe compounds is added to rice paddies to improve soil quality and supply nutrients to the crop. However, the net effect of silicate fertilizer (SF) application on soil organic carbon (SOC) stock change remain unclear. Hypothetically, SF might deplete SOC stock by increasing soil pH and stimulating microbial activity. Conversely, SF can increase SOC stock by improving rice biomass productivity. To evaluate the net effect of SF application on SOC stock change, we estimate the relationship between plant-available silicate (SiO2) and soil organic matter concentrations using national soil survey since it directly influenced by SF. We found a highly positive correlation between the two parameters, suggesting that SF application promotes SOC sequestration. We then compare the effect of SF and lime (CaCO3) addition on the mineralized C loss via flooded incubation test for 30 days. SF application decreased in total C loss, but CaCO3 addition increase this C loss. These findings imply that SF application might increase SOC stock. Finally, we determined the effect of SF on SOC stock changes under field test by analyzing net ecosystem C budget. SF application increased net primary production (NPP) of rice plants by 19–22% over the control and decreased respired C loss by 11–25%. However, around 77% of NPP is removed by rice harvesting, thus the decrease in respired C loss might highly influenced to increase SOC stock. This reduction of respired C loss might be due the interaction between SOC and Fe minerals. Consequently, SF application led to an increased in SOC stock by 0.62–1.07 Mg C ha-1 over the control. Hence, iron slag-based silicate fertilizer can promote C sequestration in soil organic matter while simultaneously improving soil properties and rice productivity.
BG01-A020
A Modeling Approach to Explore Inorganic and Organic Synergies in Enhanced Weathering to Promote Carbon Dioxide Removal
Feng TAO1#+, Benjamin HOULTON2
1Penn State University, 2Cornell University
Scientifically verifiable, durable, and scalable carbon dioxide removal (CDR) technologies are essential to reducing atmospheric CO2 concentrations and avoiding the most dangerous impacts of climate change this century. Within the nature-based solution portfolios, the soil system provides promising CDR and sequestration potential, including in both organic and inorganic forms at time scales that reflect durable removals that exceed 100 years or longer. By applying crushed basic rock (e.g. basalt) dust to cropland with appropriate irrigations, enhanced weathering makes managing soil inorganic carbon (SIC) possible to sequester billions of tons of CO2 over a short period. Meanwhile, the dissolution of cations from rock dust also contributes to a more stabilized soil organic carbon (SOC). Here, we will present a model that couples soil inorganic and organic carbon cycles under applications of rock dust. Our modeling results will assess (1) how the CDR provided by enhanced weathering varies with local environmental and management conditions, (2) synergies between SIC formation and SOC stabilization, (3) the role of cation exchange capacity in regulating CDR by enhanced weathering, and (4) potential CO2 limitation and chemical inhibition in large scale enhanced weathering application. A sophisticated process-based model considering both SIC and SOC dynamics will contribute to a better quantification of carbon sequestration by enhanced weathering at large scales and guide appropriate soil management.
BG01-A022
Soil Carbon Dynamics in Lowland Tropical Forests
Benjamin TURNER#+, Piljoo KIM
Gyeongsang National University
Tropical forest soils contain an enormous reservoir of carbon that is susceptible to perturbations in climate, fertility, and forest productivity. Soil carbon stocks to 1 m depth in tropical forests vary markedly across continental and regional scales but are typically comparable in magnitude to the carbon stored in above ground biomass. However, substantial carbon stocks occur in the subsoils of many tropical forests, yielding substantially more carbon in soils than in vegetation. Despite the perceived stability of this soil carbon, substantial changes occur over the seasonal cycle in tropical monsoon forests due to seasonal variation in root exudation. Long-term experimental nitrogen addition increases carbon sequestration in Asian Ultisols, but addition of nitrogen, phosphorus, or potassium do not alter soil carbon in neotropical Oxisols. However, cations indirectly influence soil carbon stocks via effects on fine roots. Long-term experimental litter manipulation changes the magnitude of soil carbon stocks in neotropical Oxisols, sequestering carbon with litter addition and reducing carbon with litter removal, while also altering its physical and chemical nature. Warming of tropical forest soil causes a substantial loss of carbon via heterotrophic respiration, indicating that tropical forests will be a significant source of atmospheric carbon dioxide in the future. Finally, the dominant type of mycorrhizal fungi influences soil carbon in tropical forests, with a much wider C:N ratio in ectomycorrhiza-dominated forests common in the Asian tropics, compared with forests dominated by arbuscular mycorrhizas typical of the neotropics. Overall, these findings provide important insight into the amounts, forms, and dynamics of carbon in tropical forest soils in a changing world.
BG01-A016
Iron Fertilization and Soil Carbon Sequestration in Rice Paddies
Snowie Jane GALGO#+, Piljoo KIM
Gyeongsang National University
Iron (Fe) fertilization of the ocean mitigates global warming by sequestering carbon dioxide (CO2) in phytoplankton, but the effect of Fe fertilization on carbon (C) sequestration in arable soils remains unknown. Iron is often added to rice paddies as blast furnace slag (BFS), a byproduct of steel manufacturing used as a silicate fertilizer to improve productivity. However, BFS also contains large amounts of Fe oxides, which might promote C sequestration by forming complexes with organic matter. First, to estimate the effect of continuous Fe addition via BFS on soil organic C (SOC) stock, soils were nationally sampled in South Korea. A strong positive correlation between SOC and extractable Fe and available Si concentrations was found, which might presume that the periodic BFS application contributed to an increase in SOC stock. Second, to confirm the effect of Fe addition on SOC stock increase, the effect of BFSs which have different mixing rates of Fe oxides (0-5%, wt wt-1) on the respired C loss was investigated via incubation test. Finally, to verify the effect of Fe addition on SOC stock changes, three different Fe-enhanced silicate fertilizers were applied for rice cultivation, and SOC stock changes were estimated using the net ecosystem C budget. Silicate fertilization significantly increased net primary production (NPP) by 18-20% over the control and this NPP was more highly increased with increasing Fe addition. Silicate fertilizer application highly decreased the respired C loss by 15-30% over the control. As a result, silicate fertilizer application increased around 0.67 Mg C ha-1 of SOC stock over the control during rice cultivation, but this C stock was more highly increased with increasing Fe addition. In conclusion, Fe-enhanced silicate fertilizer might be more effective in improving SOC stock and crop productivity in rice paddies.
BG01-A014
The Higher Soil Carbon Saturation Degree, the Higher Methane Emission in Rice Paddy
So Yeong PARK+, Piljoo KIM#
Gyeongsang National University
Soil organic carbon (SOC) plays a critical role in the global carbon (C) cycle and soil quality. However, soil has its own C saturation degree which was mainly controlled by silt + clay content. Periodic organic amendment application cannot increase SOC stock over its C saturation level but increase the mineralized C loss. Especially in the flooded rice paddy, the applied organic amendments might increase the emission of methane (CH4), which has 27 times higher global warming potential (GWP) than carbon dioxide (CO2), and then significantly worsen global warming. However, organic C protective capacity was not properly evaluated in the flooded rice paddy. First, to characterize the C protective capacity of rice paddy soils, 20 different soils were sampled nationwide in Korean rice paddy during the dried fallow season, and the relationship between silt+clay content and mineral-associated organic C (g C kg-1 soil) was analyzed. The organic C protective capacity of rice paddy was much lower than upland with the relationship, probably due to increased Fe solubility under the flooded soil condition. To investigate the influence of soil C saturation degree on the mineralized C loss, three soils with the same soil forming background but different soil C saturation degrees (74, 77, and 84%) were selected. The same amount of plant biomass was applied before rice transplanting, and then the respired C loss (CO2-C and CH4-C) was annually characterized for two years. Total respired C loss was highly increased with increasing soil C saturation degree. CH4 emission was more highly covered total respired C loss with increasing soil C saturation degree during the flooded rice cropping season and significantly increased the net GWP. Therefore, organic amendments should be carefully managed under the highly C-saturated rice paddy to mitigate global warming, like more recalcitrant organic amendments.
BG01-A017
Effect of Organic Amendments Self-produced Inner Rice Cropping Boundary to Sustain Soil Carbon Stock Under Global Warming Environment
YoungHo SEO#+, Piljoo KIM
Gyeongsang National University
Global warming might accelerate the decomposition of soil organic carbon (SOC) stock, due to more highly increased microbial activity than net primary production (NPP). SOC depletion not only aggravates soil quality but also exacerbates climate change. Therefore, higher amounts and more recalcitrant types of organic amendment applications might be essential under future climate conditions. To investigate the feasibility of organic amendments self-produced inner rice cropping boundary to increase SOC stock under global warming, cover crops during the fallow season and rice during the cropping were cultivated under the present and future climate (2℃ and 200 ppm CO2 elevation over the ambient) conditions. Cover crop biomass and rice straw were incorporated by fresh and biochar (pyrolysis at 400℃ for 2 hours) types. Annual SOC stock changes were estimated using net ecosystem C budget (NECB) which implies the difference between C input and output. Under the present climate condition, no organic amendment (NPK) decreased SOC stock by 0.4 Mg C ha-1 year-1, but fresh biomass application significantly increased SOC stock by 1.5 Mg C ha-1 year-1. In comparison, biochar application slightly increased SOC stock by 0.03 Mg C ha-1 year-1, due to low biochar yield (25-40% of fresh biomass) and low NPP of rice. Global warming more highly decreased annual SOC stock by 0.4-2.6 Mg C ha-1 year-1 over the present under the same amendments. Under global warming, biochar application was more effective than fresh biomass in reducing SOC loss but did not increase SOC stocks. In conclusion, only the utilization of biomass self-produced inner rice cropping boundary may not be enough to increase SOC stock under global warming conditions. Therefore, under future conditions, more application of biochar, a recalcitrant organic amendment, might be essential, via increasing biomass productivity through fertilizer and water management.
Session Chair(s): Zhangcai QIN, Sun Yat-sen University, Piljoo KIM, Gyeongsang National University
BG01-A001
Retrogressive Thaw Slumps Mapping from Remotely Sensed Imagery on Tibetan Plateau Using Deep Learning
Guiyun ZHOU#+
University of Electronic Science and Technology of China
Fine mapping of the retrogressive thaw slumps (RTSs) plays a pivotal role in the study of permafrost degradation and carbon exchange. In this study, we propose a lightweight segmentation network (LerssNet) for automatically mapping the RTSs in the Beiluhe area of the Tibetan Plateau from remotely sensed imagery. LerssNet is constructed on the foundation of an encoder-decoder framework and innovatively incorporates semantic fusion and attention mechanisms in feature propagation. We improve MobileNet as the encoder to support multi-band input, which can capture multi-level semantic features efficiently. The semantic features are spatial group-wise enhanced (SGE) by generating an attention factor and local-global similarity of each pixel location. The self-attention and convolution hybrid module (Acmix) performs feature fusion and dimensionality reduction on the high-level semantic features, which are then concatenated with the low-level features after twice up-sampling. Given the inherent samples normally imbalance in dichotomous segmentation, we employ both statistical and morphological losses for backpropagation and cross-validation. To solve the edge blurring during interpolation, the semantic features are decoded into segmentation results of RTSs using depth-wise separable convolution and dilated convolution alternately. In the experimental phase, approximately 280 RTS polygons are manually delineated from high-resolution Google Earth Images and transformed into binary images. Subsequently, preprocessed 2.5m-resolution Maxar images and ground-truth labels are subdivided into 3380 patches following data augmentation, encompassing training, validation, and test datasets. The LerssNet directly chose training datasets to supervised learning without pretraining, with network hyperparameters automatically updated based on the validation datasets. Tests on the Beiluhe areas demonstrate that the LerssNet is robust, achieving an impressive Mean Intersection over Union(MIoU) of 94.8%. Ablation experiments highlighted the versatility of the training model, yielding a mean pixel accuracy 2.7% higher than that of DeepLab v3+. Furthermore, this methodology exhibits the promise of portability for large-scale applications.
BG01-A005
Mapping Alaskan Soil Carbon Content Using Multi-temporal and Multi-source Remote Sensing Data
Wei PENG+, Yonghong YI#
Tongji University
Soil organic carbon (SOC) is a crucial parameter affecting permafrost changes in the boreal-Arctic region. However, mapping SOC poses great challenges due to limited in-situ measurements and a lack of understanding on the processes controlling SOC distribution. Recently, machine learning (ML) methods utilizing remote sensing data have demonstrated great potential in regional SOC mapping. This study focuses on enhancing the performance of ML models in Alaskan SOC mapping using multi-source and multi-temporal remote sensing data. The models incorporate monthly composite of Sentinel-1 synthetic aperture radar (SAR) backscatter data and the temporal statistics, mitigating data inconsistency. Additional inputs include optical vegetation indices from Sentinel-2 and climate variables from Daymet. After recursive feature elimination, random forest models are trained to map SOC distribution, yielding a reasonable performance (R2=0.35, RMSE=12% g/g*100%). The model shows higher SOC content in the continuous permafrost region such as the North Slope due to slower carbon decomposition and the interior boreal forest region due to more carbon inputs. A 3-dimension (3D) model is also constructed through introducing soil sampling depth as a feature, which can capture vertical SOC variations with an improved performance (R2=0.60, RMSE=9% g/g). To further enhance the model performance, a combination of classification and regression methods in 3D model is employed, including splitting the dataset into different clusters and training individual models for each cluster, resulting in slightly reduced model SOC uncertainty. We also used the feature space resampling to adjust sample distribution, and assigned weights based on their density in the feature space before the training, which demonstrated slightly improved performance. Considering that a single model may not adequately depict the nonlinear relationship between covariates and SOC, other efforts include training different random forest models for different ecoregions to minimize model overfitting.
BG01-A007
Estimating Soil Properties Using Mid-infrared Diffuse Reflectance Spectroscopy
Kyungjin MIN, Jeong Chan LEE#+
Seoul National University
Bio geoscience, Interdisciplinary Geosciences Accurate knowledge of soil properties (chemical, physical, biological) can help us better manage soil and use them as nature-based solutions to climate change. Conventional approaches to assessing soil properties, however, are limited by cost and time, therefore challenging the need for soil monitoring and management. Mid-infrared spectroscopy coupled with Partial Least Squares (PLS) can be a complementary approach for qualitative and quantitative soil property measurements. PLS is divided into PLS1 (single Y variable) and PLS2 (multiple Y variables) based on the number of Y variables. Here, we leveraged 482 soil samples with known soil properties and assessed their mid-infrared spectra. These soils were collected under shallow- and deep-rooted plants at 0-240 cm across the United States. Our goal was to compare the performance of PLS1 and PLS2 models for a given property and to assess the accuracy of their estimations. PLS2 outperformed PLS1 in predicting pH, calcium ion, aluminum ion and sand proportion. Yet, PLS1 was better than PLS2 for other properties. Estimations with an R2 value exceeding 0.80 were achieved in carbon content, nitrogen content, pH, soil texture and calcium ion. As follow-ups, we will build new models by including biological properties such as soil respiration, microbial biomass, and enzyme activities and compare the model performance between the current and new models. Keyword : Soil, Infrared Spectroscopy, Partial Least Square
BG01-A008
Methane Emissions from Wetlands in China and Their Climate Feedbacks in the 21st Century
Tingting LI#+
Chinese Academy of Sciences
Wetlands are large sinks of carbon dioxide (CO2) and sources of methane (CH4). Both fluxes can be altered by wetland management (e.g., restoration), leading to changes in the climate system. Here, we use multiple models to assess CH4 emissions and CO2 sequestration from the wetlands in China and the impacts on climate under three climate scenarios and four wetland management scenarios with various levels of wetland restoration in the 21st century. We find that wetland restoration leads to increased CH4 emissions with a national total of 0.32−11.31 Tg yr−1. These emissions induce an additional radiative forcing of 0.0005−0.0075 W m−2 yr−1 and global annual mean air temperature rise of 0.0003− 0.0053 °C yr−1, across all future climate and management scenarios. However, wetland restoration also resulted in net CO2 sequestration, leading to a combined net greenhouse gas sink in all climate management scenarios, except in the highest restoration level combined with the hottest climate scenario. The highest climate cooling was achieved under medium restoration, with the climate scenario consistent with the Paris agreement target of below 2 °C, with a cumulative global warming potential of −3.2 Pg CO2-eq (2020− 2100). Wetland restoration in the Qinghai−Tibet Plateau offers the greatest cooling effect.
BG01-A010
Asynchronous Flux Variation Complicates Mangrove Blue Carbon Offset by Methane Emission
Xudong ZHU#+
Xiamen University
The climate benefit of mangrove blue carbon can be partially offset by methane emission, but this offset is rarely assessed using multi-year high-frequency observed fluxes. Here, four-year continuous eddy covariance measurements of simultaneous methane and carbon dioxide fluxes were used to examine temporal patterns of methane flux and its blue carbon offset, in a subtropical estuarine mangrove of China. We found both diurnal and seasonal methane fluxes were mainly driven by soil temperature and tidal water level, showing stronger nighttime emission. On average, one-tenth of carbon dioxide uptake was offset by methane emission using the sustained-flux global warming potential metric at a 20-year time horizon, while this offset could vary over an order of magnitude due to asynchronous flux variations across time scales. These results highlight the significant contribution of nighttime emission to mangrove methane budget and confirm the importance of asynchronous flux variations in assessing mangrove’s climate benefit.
BG01-A009
Three Gorges Dam Operations Affect the Carbon Dioxide Budget of a Large Downstream Connected Lake
Xiaosong ZHAO#+
Chinese Academy of Sciences
The effects of dams on carbon dioxide (CO2) fluxes in downstream lakes remain elusive. Here we combined eddy covariance observations and random forest models to examine multi-decadal variations in CO2 fluxes in the Poyang Lake, the largest freshwater lake in China, and quantified the contribution of the Three Gorges Dam (TGD), the world's largest hydraulic project. We found the lake fluctuated between CO2 source and sink in 1961–2016, and tended to be CO2 sink in the post-TGD period (2003–2016) when vegetation expanded early and spatially due to declining water level. TGD can explain approximately 6% of the total differences in annual CO2 fluxes, with major contributions in the impoundment period (up to 22% in middle September to October). The results show a positive side of operational major hydraulic projects on lake carbon sink, and probably caution the negative side of carbon release after dam removal.
BG01-A003
Classification of Indicators on Water and Soil Organic Properties Using Vegetation in Kushiro Mire, Japan
Sawa FUJIWARA+, Katsuaki KOMAI#
Kitami Institute of Technology, Japan
Wetlands are prone to anaerobic conditions due to high flood frequency. Generally, the peat soil in such a wetland contains much organic matter derived from plants. Soil carbon contents in wetlands have been poorly evaluated due to their low accessibility and less observed data. The characteristics of typical vegetation areas in Kushiro mire, the largest wetland in Japan, were examined using observed groundwater level data, NDVI (Normalized Difference Vegetation Index), NDWI (Normalized Difference Water Index), MNDWI (Modified Normalized Difference Water Index), and NDSOC (Normalized Difference Soil Organic Carbon), respectively. NDVI is one of the remote sensing data obtained by satellites and used as an indicator for vegetation activity closely associated with soil organic carbon. NDWI is an indicator used to identify the water's existence. MNDWI is a kind of NDWI but not to be influenced by urban and vegetation areas. NDSOC is an indicator of carbon in soil organic matter, which was proposed in a recent study. At sixty-nine locations vegetated with two different typical plant species (alder and reed), the significant differences in median values for relative groundwater levels, NDVI, NDWI, MNDWI, and NDSOC were statistically evaluated using the Mann-Whitney U test, respectively. The relative groundwater levels were observed in the period from 2018 to 2022. NDVI was obtained from a total of twenty-one Sentinel-2 images in the period from 2017 to 2023. Contrary to previous studies, a significant relationship between relative groundwater level and vegetation was not found. Significant relationships of vegetation species to NDVI, NDWI, MNDWI, and NDSOC were found, respectively.
BG01-A004
Depth-dependent Changes in Soil Chemistry and Carbon Sequestration After 12 Years of Nitrogen Additions in an Agricultural Soil
Hyeju LEE+, Kyungjin MIN#
Seoul National University, Korea, South
Widespread use of nitrogen (N) fertilizer has increased plant growth and associated carbon (C) sequestration in agricultural land. Although enhanced plant growth can influence C inputs into the soil via litter and root exudates, it remains unexplored how these plant responses to N fertilizer affect soil chemistry. In particular, we have a limited understanding of how the chemical and biological changes at surface soils, directly influenced by N fertilization and plant growth, affect the distribution of ions, quantity and persistence of soil organic C in deeper soil layers. Here, we investigate chemical properties from the soils under Miscanthus x giganteus, which has been treated with urea fertilizer at (0, 30, 60, 120, 240 kg N ha-1 yr-1) since 2011. In June 2023, we collected soils along 0-120 cm depth profiles and assessed root biomass, rhizome biomass, soil organic C stock, soil N concentration, and ion concentrations. There were no significant differences in root and rhizome biomass (t ha-1) among N treatment plots. Likewise, soil organic C stock (Mg C ha-1), soil organic C content (%, w/w), and total N content (%, w/w) did not show significant differences among N treatment plots. Instead, depth significantly influenced these properties; root and rhizome biomass, as well as organic C content and total N content decreased along soil depth profiles. Nevertheless, there were notable differences in NO3- (mg L-1) concentrations among N treatment plots. The highest NO3- concentrations were observed where the most fertilizer was applied. As a follow-up, we will investigate microbial biomass C, particulate-, and mineral-associated organic C and assess the degree of soil organic C persistence under N additions. This study will help us understand how deep N inputs in agricultural soils can alter soil organic C chemistry and persistence.
BG01-A011
Woody Biochar Applications Significantly Enhance Net Ecosystem Carbon Budget, Fruit Productivity, and Soil Quality in Red Pepper Cropping System : Two-year Field Experiment
Sohee YOON+, Sang Yoon KIM#
Sunchon National University, Korea, South
Woody biochar (WB) is one of the organic amendments with high soil carbon (C) accumulation and low decomposition potential, considering a low-carbon-emitting material. However, there is a lack of research on net ecosystem carbon budget (NECB) that systematically investigates overall soil organic carbon (SOC) changes, suggesting optimum application rates to improve NECB in red pepper cultivated soils. This study was focused on evaluating NECB, crop growth and productivity, and soil properties in a red pepper cultivated field for two years with woody biochar (WB) application rates (woody biochar at rate of 0, 2.5, 5 and 10 Mg ha-1 under the recommended fertilization as N-P2O5-K2O = 190-112-149 kg ha-1). Our results showed that total C input from fertilizer and WB application over two years was highest at WB10 (11.2 Mg C ha-1), and then followed by WB5 (5.64 Mg C ha-1) > WB2.5 (2.86 Mg C ha-1) > WB0 (0.08 Mg C ha-1). For two years, CO2 emissions increased with increasing WB application levels. CH4 emissions showed negative fluxes in all treatments and were almost negligible in this study. WB application increases cumulative fruit productivity and total biomass productivity. As a result, NECB was highest at WB10 as followed by WB5, WB2.5, WB0, showing a positive value at WB10. To improve NECB, the rational WB application rate was estimated to be 5.3 – 5.8 Mg ha-1 when removing the whole biomass after harvest and 0.2 – 1.7 Mg ha-1 when returning it to the soil, respectively. Increasing WB application levels significantly improved overall soil physicochemical properties such as bulk density and SOC content. In conclusion, optimum level of WB application could be a sustainable organic matter management strategy to improve NECB, fruit productivity, and overall soil quality in red pepper cropping systems.
BG01-A012
Shifting Transplanting Dates Reduces Greenhouse Gas Emissions Without Significant Loss of Productivity in a Paddy Field During Cultivation : A Two-year Field Experiment
Yeomyeong LEE+, Sang Yoon KIM#
Sunchon National University, Korea, South
Shifting rice transplanting dates directly or indirectly affect greenhouse gas (GHG as CH4, CO2 and N2O) emissions in particular CH4 by influencing the rice growth characteristics and flooding days in paddy ecosystems. However, systemic impact has not been evaluated yet. In this study, the field experiment was conducted to investigate the feasibility of shifting transplanting dates and their influencing factors for reducing GHG emissions and maintaining productivity in rice paddy. For the consecutive two years (2022 and 2023), two different rice cultivars (late-maturing and early-maturing) were transplanted at four different dates on May 10 (Time1), May 25 (Time2) as locally recommended transplanting date, June 10 (Time3), and June 25 (Time4). Regardless of rice cultivar, the highest CH4 emissions were observed in the early transplanting (Time1), and significantly decreased by 23.6~86.9% with delaying transplanting dates, irrespective of the investigation years. Our results showed CH4 was contributed to approximately 90% over total GHG emissions, while CO2 and N2O were almost negligible, indicating CH4 as a major contributor to overall global warming impact. Rice productivity progressively improved as the transplanting was delayed, reaching the highest level at Time3, and then slightly decreased at Time4. However, there was no significant loss as compared to the recommended transplanting date (Time2). Correlation analysis revealed significant relationships between CH4 emissions and flooding days, meteorological characteristics (cumulative temperature, sunshine hour etc.), and rice growth and physiological characteristics. In particular, strong positive correlation was observed between total CH4 fluxes and root biomass productivity, which may closely relate to the quantity and quality of root exudate as methanogenic substrates, influencing methanogenic and methanotrophic activities. Conclusively, shifting rice transplanting date could be a promising and innovative strategy and easy way to effectively reduce GHGs emissions without significant productivity loss in paddy field in the era of climate changes.
BG01-A013
Can Rice Ratoon Enhance Carbon Sequestration in Mono-cropping System in Monsoon Climate?
Jasmin MELENDEZ+, Sang Yoon KIM#
Sunchon National University, Korea, South
Incorporation of organic amendments, such as rice straw, has been recommended to enhance soil organic carbon sequestration and maintain soil quality. The addition of organic matter is an important practice to improve rice productivity and increase the input of organic material. However, few studies have been found to explore the potential of rice ratoon in carbon sequestration. In this study, the ratoon of rice (newly emerged shoot and root biomass), and without ratoon rice where investigated at three sampling stages in a 2-week interval after rice were harvested in the field. The chemical properties such as total and labile carbon, nitrogen, and the characteristic of decomposition rate were determined by an incubation experiment after ratoon rice were added in paddy soils. Results have shown that ratoon rice increased the soil carbon input, showing strong potential for enhancing soil carbon. Interestingly, the chemical properties of ratoon root were significantly altered by increasing carbon and nitrogen contents with C/N ratio changes as compared to the control in all sampling stages, which might be affected by green shoot biomass and N translocation. In addition, the timing and fertilization regimes should be investigated to maximize soil C sequestration by enhancing biomass yield of ratoon rice. A long-term study would be required to further investigate the realistic impact of ratoon rice as a new carbon source.
BG01-A019
Effects of Plastic Film Mulching and Stover Recycling on Soil Organic Carbon Stock Changes in Maize Cropping System
Hogyeong CHAE1#+, 2, Piljoo KIM1
1Gyeongsang National University, Korea, South, 2,
Plastic film mulching (PFM) has been popularly utilized to enhance crop pr crop productivity, by controlling weeds and improving soil properties. However, PFM increases not only the net primary production (NPP) as a C input source but also mineralized C loss as a C output source by improving soil temperature and moisture conditions. Moreover, the whole maize aboveground was removed in the present maize cultivation system, and it created a negative net ecosystem C balance (NECB). Therefore, additional organic amendment is essential to increase SOC stock and stover recycling can increase SOC stock. To determine the effects of PFM and stover recycling on SOC stock changes, PFM and no-mulching (NM) were designed as the main treatments. For the sub-treatment, maize aboveground removal (Conventional) and stover recycling were installed. In stover recycling, stover was incorporated as fresh (Fresh) and pyrolyzed (Biochar). PFM improved soil temperature and moisture content by an average of 1.4-1.7℃ and 11-20%, respectively, compared to NM. The improved soil environmental conditions increased grain yield by 34-51%. In conventional treatment, NPP and respired C loss under NM were 6.3 and 6.0 Mg ha-1, respectively. PFM increased both NPP and respired C loss by 12-26 and 26-35% respectively. Compared to conventional treatment, fresh stover recycling increased NPP and respired C loss by 22-27 and 11-23%, respectively. However, Biochar stover recycling decreased NPP by 4.5-5.3 Mg ha-1 and respired C loss by 3.1-3.8 Mg ha-1. Although the stover recycling highly increased NECB compared to conventional treatments by 23 and 47% in fresh and biochar, respectively, all the NECB values showed negative values. Our investigation suggests that pyrolyzed stover recycling was very effective in decreasing the negative impact of PFM on SOC stock but additional organic matter applications such as green manure are recommended to increase SOC stock.
BG02-A001
Modeling Global Carbon Emissions Driven by Land-use Change
Zhangcai QIN#+, Yakun ZHU
Sun Yat-sen University, China
Land-use change (LUC) is one of the major drivers of global anthropogenic carbon emissions. Current estimates of LUC-induced emissions vary widely among models and assessments. Recently, we developed a new bookkeeping model to estimate global emissions by accounting for carbon fluxes associated with all major gross land-use transitions. Here, we show the overall modeling techniques, and the model applications in estimating global and regional LUC-related emissions over the past several decades (1961-2020). LUC has led to about 215 and 142 Pg C of gross carbon emissions and removals, respectively, resulting in an average net emission of 1.2 Pg C annually. Latin America, Southeast Asia, and Sub-Saharan Africa were the top three regions with the highest contributions to net LUC-related emissions. Forest-associated LUC activities (e.g., deforestation, reforestation) dominated carbon fluxes. However, it is still challenging for data and models to identify temporal and spatially explicit LUC-induced emissions hotspots.
BG02-A004
Soil Organic Carbon is a Key Determinant of CH4 Sink in Global Forest Soils
Jaehyun LEE1#+, Hojeong KANG2
1Korea Institue of Science and Technology, Korea, South, 2Yonsei University, Korea, South
Soil organic carbon (SOC) is a primary regulator of the forest–climate feedback. However, its indicative capability for the soil CH4 sink is poorly understood due to the incomplete knowledge of the underlying mechanisms. Therefore, SOC is not explicitly included in the current model estimation of the global forest CH4 sink. Here, using in-situ observations, global meta-analysis, and process-based modeling, we provide evidence to support the notion that SOC constitutes an important variable that governs the forest CH4 sink. We find that a CH4 sink is enhanced with increasing SOC content on regional and global scales. The revised model with SOC function better reproduces the field observation and estimates a 39% larger global forest CH4 sink (24.27 Tg CH4 yr−1) than the model without considering SOC effects (17.46 Tg CH4 yr−1), narrowing the gap between bottom-up and top-down global soil sink estimates. This study highlights the role of SOC in the forest CH4 sink, which shall be factored into future global CH4 budget quantification.
BG02-A007
Measurement, Reporting, and Verification System for Monthly Soil CO2 Flux in South Korea
Jun Ge HYUN+, Ye Lim PARK, Inhye SEO, Minseop JEONG, Yejee OK, Gayoung YOO#
Kyung Hee University, Korea, South
Accurately quantifying soil CO2 flux, a crucial component in the terrestrial ecosystem-atmosphere carbon exchange process, is vital for improving the precision of national greenhouse gas inventories, particularly in the land use sector. However, the lack of continuous, spatially representative data has been a significant barrier to developing reliable soil CO2 flux estimations in South Korea. This study addresses this gap by developing a data-driven model for estimating soil CO2 flux across various land covers in South Korea and constructing a continuous field monitoring system nationally. Utilizing monthly CO2 flux data measured with the chamber method globally (site number = 646), the model was designed to provide a comprehensive perspective on soil CO2 dynamics. To ensure accuracy and applicability, the various machine learning algorithms were compared: multi-linear regression, random forest, artificial neural network, and light gradient boosting machine. In model training process, the leave-one-site-out cross-validation was implemented to enhance model performance and reliability. This method involves systematically excluding data from one site at a time, using it for model validation while employing the remaining data for training. After model development, we further verified its performance with the monthly CO2 flux data from South Korea (site number = 16), including our new observation sites in urban and natural forests. The outcomes of this study are expected to contribute to improving carbon absorption estimation accuracy by land cover type. This enhancement will aid in developing a Tier 3 level national greenhouse gas inventory for South Korea, representing a significant advancement in the country's climate change mitigation efforts. The integration of advanced machine learning techniques with empirical data not only sets a new standard in soil CO2 flux estimation but also serves as a model for other regions striving to enhance their environmental monitoring and policy-making capabilities.
BG02-A012
Spatial and Temporal Evolution of Carbon Fluxes on the Tibetan Plateau and Optimization of Key Model Parameters
Hanlin NIU#+, Xianhong MENG, Lunyu SHANG, Shaoying WANG, Zhaoguo LI, Lin ZHAO, Hao CHEN, Mingshan DENG, Danrui SHENG
Chinese Academy of Sciences, China
This study evaluates the applicability of the Functionally Assembled Terrestrial Ecosystem Simulator (FATES) for modeling vegetation dynamics, specifically in the alpine grasslands of the Tibetan Plateau. FATES, which incorporates plant traits such as height and age, aims to improve the simulation of interspecies competition and coexistence in these ecosystems. A critical aspect of this model is its reliance on vegetation physiological parameters, which are vital for accurately simulating environmental sensitivity and carbon flux processes. The study commenced with an applicability assessment of the original model on the Tibetan Plateau, followed by enhancements to the model's physiological parameters. Calibration was then conducted at three observation sites to tailor the model to local environmental conditions. This was succeeded by a validation process at nine different sites. For the spatial distribution aspect, FLUXCOM and Global land surface satellite (GLASS) data were employed to verify the model's accuracy across these diverse locations. The results indicated a reduction in the deviation and root mean square error of Net Ecosystem Production (NEP), with specific improvements noted from values 0.22 to -0.02 and 1.96 to 1.11 μmol·m⁻2·s⁻1, respectively. Furthermore, there was an enhancement in the correlation coefficient from 0.31 to 0.57. Moreover, the spatial correlations of NEP and Gross Primary Production with FLUXCOM data improved respectively from 0.37 to 0.61, and from 0.78 to 0.82. In the analysis with GLASS, the spatial correlation of Net Primary Production consistently held at 0.77, whereas the correlation for Leaf Area Index decreased from 0.72 to 0.68. These findings suggest that FATES can more reliably simulate the temporal and spatial dynamics of carbon flux in the Tibetan Plateau's alpine grasslands, capturing key aspects of daily and seasonal changes. The model's improved performance contributes to reducing the uncertainty previously associated with simulating carbon flux in this region.
BG04-A003
Sensitivity of Land Surface Temperature to Lengthened Vegetation Growing Season in Boreal Forest
Chang-Eui PARK1#+, Sujong JEONG2
1Korea Institute of Science and Technology, Korea, South, 2Seoul National University, Korea, South
Vegetation phenology are important for shaping seasonal climate over the northern boreal forests. However, the biophysical effects of phenological changes on the land surface temperature (LST) are still unclear. Here, we estimated LST sensitivity to advanced start of growing season (SOS) and delayed end of growing season (EOS) during corresponding green-up and senescence periods over boreal deciduous forests based on experimental set of Community Land Model version 5. Estimated LST sensitivities to advanced SOS and delayed EOS during green-up and senescence periods were −2.1 × 10−2 K day−1 and −2.8 × 10−2 K day−1, respectively, denoting cooling land surface due to phenological changes. Reduced the aerodynamic resistance to SOS and EOS changes and relevant turbulent heat release could explain the higher LST sensitivity to EOS than that to SOS. Hence, the reduced aerodynamic resistance due to phenological shifts could be an important consideration for projecting seasonal climate change.
BG04-A004
Observing Plants Phenology in Tsukuba Botanical Garden Using Satellite Data and Time-lapse Camera
Suzu NAKAMURA1#+, Taiga SASAGAWA2, Ai NAGAHAMA3, Kenlo NASAHARA1
1University of Tsukuba, Japan, 2Chiba University, Japan, 3National Museum of Nature and Science, Japan
Phenology observation using satellite remote sensing has become popular in recent years. Plants phenology is affected by the environment and shows the impact of climate change on plants. The objective of this study is to see such changes by satellite remote sensing. The target area is the Tsukuba Botanical Garden (TBG) in Ibaraki, Japan. TBG is planted with a variety of plants from different climates, which enables to compare plants phenology among many tree species. Planet Scope satellite data is used here as it has high spatial resolution of 3 m, which makes it possible to observe the phenology of a single to several trees. It is known that there is a difference between phenology of a landscape level and of a single tree, and to know the difference, Himawari/AHI data was used as landscape level data, comparison to Planet Scope data. NDVI was calculated from the two satellite data. Also, time-lapse cameras are used as ground verification data. Since December 2022, four time-lapse cameras have been installed at TBG for plant observation. It belongs to Phenological Eyes Network (PEN), a network of long-term automatic ground observation in Japan. The images have high resolution, therefore it is possible to distinguish the leaves and budburst and flowering. Current results are that Planet Scope data shows that the NDVI values for the Japanese larch trees in 2023 were later than those in 2022, and the time-lapse camera images also show that there were more leaves in 2023 than in 2022. Similar analyses are to be conducted for other tree species and also using data from Himawari/AHI.
BG04-A006
The Effect of Urban Heat and Light on Phenological Temperature Sensitivity Over the Greater Seoul Area
Jihyun KIM+, Soyoung SOHN, Yeonjoo KIM#
Yonsei University, Korea, South
Vegetation phenology drives terrestrial ecosystem dynamics and related carbon and water cycles; therefore, it is critical to investigate its sensitivity to temperature under various conditions, which can be provided in urban areas where temperatures are elevated and artificial lights are added. In this study, we analyzed one decade (2012 - 2021) of data on surface temperature, phenology, and land cover from the Moderate Resolution Imaging Spectroradiometer (MODIS), and artificial lights at night (ALAN) data from the Visible Infrared Imaging Radiometer Suite (VIIRS) over the Greater Seoul area in South Korea. We estimated an urbanization index (UI) and the long-term trends of the start of the season and the end of the season (ΔSOS and ΔEOS) and the temperatures (ΔTSOS and ΔTEOS) and in the ALAN (ΔALAN). We then investigated how much of those factors (i.e., ΔT, ΔALAN, and UI) contributed to the ΔSOS and ΔEOS and explored temperature sensitivities of the ΔSOS and ΔEOS under different conditions. We found that 70% of ΔSOS (about 3 days/dec) was primarily attributed to UI, while the ΔEOS (about 4 days/dec) was influenced by ΔALAN and ΔTEOS at similar levels (26% and 31%, respectively). We show that the temperature sensitivity of ΔSOS is higher by 4.5% in the highly urbanized areas, and the temperature sensitivity of ΔEOS is 4.3% higher with increasing lights. Our finding indicates that vegetation phenological response to the increasing temperature would become complicated with the increases of urban-like conditions (i.e., higher levels of CO2 concentration), therefore further studies are required to improve our understanding of terrestrial vegetation response to changing climates. This study is supported by the NRF grants from the MSIT (2020R1C1C1014886, and 2022R1C1C2009543), the KAIA grant from the MOLIT (22CTAP-C163540-02), and the Korea Environment Industry & Technology Institute (KEITI) funded by Korea Ministry of Environment (2022003640002).
BG04-A007
Increasing Sensitivity of Tree Radial Growth to Precipitation
Tiewei LI#+, Bin HE, lanlan GUO
Beijing Normal University, China
The sensitivity of tree growth to precipitation is a key metric for understanding the global vegetation dynamics, but whether the sensitivity has increased or decreased under climate change remains contentious. Here we provide a comprehensive examination of the spatiotemporal changes in the sensitivity of tree growth to precipitation indicated by the radial growth of trees (Spre) over the past century (1901–2012). We found a widespread increase in Spre across most tree-containing biomes in the second half of the 20th century. Both observations and dynamic global vegetation models suggest that the increases in Spre are mainly related to the combined effects of changes in precipitation and atmospheric CO2 concentrations. The increase in Spre in arid biomes was associated with increasing precipitation, whereas the increase in Spre in humid biomes was associated with decreasing precipitation. Elevated CO2 generally increased Spre in arid biomes but decreased Spre in humid biomes. However, this contrasting impact of CO2 was overridden by the changes in precipitation, ultimately leading to a widespread increase in Spre in both arid and humid biomes. The overall decreasing trends in Spre over the past century occurred mainly in the tropical forest biomes, predominantly because increased precipitation is associated with higher water availability. Our study provides new insight into the temporal changes in Spre from the perspective of the radial growth of trees and suggests that tree growth might be increasingly sensitive to precipitation changes with continuing global climate change, potentially affecting the strength of the terrestrial carbon uptake.
BG04-A010
The Expanding Optimal Climatic Space of Global Vegetation Growth During 1982–2020
Jiana CHEN1+, Zaichun ZHU1#, Anping CHEN2, Shi XU1
1Peking University, China, 2Colorado State University, United States
Vegetation plays a crucial role in climate change, serving as both an indicator and regulator. The maximum greenness of vegetation reflects the cumulative impact of environmental factors over time, holding significance for carbon cycling. Vegetation typically reaches maximum greenness under optimal environmental spaces. However, little is known about how the optimal climate space may change under climate change. Here, using nearly four decades (1982–2020) of continuous data on leaf area index and four climate variables, we determined the response curves of optimal climate variables and their changes in geospatial and climatic space. We found the maximum leaf area index (LAImax) increased in > 90.4% of the global vegetated land from 1982–2020. The global optimums for temperature (Topt), radiation (Ropt), vapor pressure deficit (Vopt), and soil moisture (Sopt) increased from 26.5 to 28.2 °C, 178 to 199 W m-2, and 0.6 to 0.9 kPa, 0.40 to 0.37 m3 m-3. Since vegetative growth mainly expanded at the upper temperature limit (0.54 ± 0.37 ℃), upper VPD limit (0.09 ± 0.11 kPa), and lower soil moisture limit (−0.01 ± 0.02 m3 m-3), regions where vegetation maintained optimal climatic conditions could miss the opportunity to increase LAImax. Forests underwent more drastic changes in their ecological niche compared to other vegetation types, except for typical tropical rainforests. The above findings imply that global vegetation has adapted its response to multiple environmental factors over the past decades, and is able to achieve better growth over a wider climatic space. In contrast to previous studies focusing on vegetation movement trajectories in geographic space, our emphasis on changes in climatic space allowed us to gain a more direct understanding of climatic requirements for achieving maximum vegetation growth, offering a theoretical foundation for effective ecosystem management under climate change.
BG04-A011
Advocating a Comprehensive Multi-scale Approach for Unraveling Mechanisms Behind Plant Phenology
Jongho KIM#+, Sujong JEONG
Seoul National University, Korea, South
Plant phenology is commonly observed through visible changes in phenotypes, such as leafing and flowering. Satellite data utilizes variations in greenness to define the start and end of the growing season. While phenology serves as a potent indicator for ecosystem changes, its limitation lies in the variability associated with its definition-target. The diverse interpretations of phenology, influenced by the scale and purpose of the data, hinder its ability to fully represent the complexity of ecosystems. Here, we tried a comprehensive approach for the phenological events in the aspects of different scales, species composition, and physiology. Our approach involved accessing data at various scales to clarify the characteristics and limitation of the data. The primary goal of this approach was to uncover the underlying mechanism of vegetation activity of terrestrial ecosystems attributable to climate changes. Firstly, through a comparative analysis of ground-based and satellite observation data, we examined shrub and earlier leafing species, elucidating the signals of phenology at the landscape scale. Secondly, we investigated the mechanisms governing the structure and function of ecosystems by comparing greenness-based phenology with physiological phenology based on the data such as flux, and satellite-retrieved proxies for photosynthetic activity. Divergent phenological changes were observed depend on the scale of the phenology data. It highlights the necessity for a multi-scale approach, including individual-level assessments, to achieve a precise understanding of landscape-scale dynamics. Notably, variations in the phenology of structure and physiology were noted depending on the site, indicating potential lags between them influenced by plant functional type or climate conditions. These efforts are anticipated to play a crucial role in accurately understanding the role of vegetation in future simulations of carbon absorption due to climate change and in comprehending ecological consequences of phenological mismatches.
BG05-A004
High-resolution Atmospheric CO2 Concentrations Simulated in WRF-Chem Over East Asia from 2009 to 2018
Min-Gyung SEO#+, Hyun Mee KIM
Yonsei University, Korea, South
In this study, high-resolution CO2 concentrations were generated for East Asia to analyze long-term changes in atmospheric CO2 concentrations. Using the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem), atmospheric CO2 concentrations were simulated in East Asia at a resolution of 9 km for a period of 10 years (2009–2018). The annual mean simulated CO2 concentrations in East Asia were 391.027 ppm in 2009 and 412.95 ppm in 2018. The simulated CO2 concentrations exhibited appropriate seasonal variabilities, with lower concentrations during the growing season in the summer and higher concentrations in the winter and spring. The simulated CO2 concentrations were verified using surface CO2 observations, column-averaged CO2 mole fractions (XCO2) from Orbiting Carbon Observatory 2 (OCO-2), and CarbonTracker 2019b (CT2019B) data. Based on surface CO2 observations, the average root-mean-square error (RMSE) of the simulated CO2 concentrations in WRF-Chem was 2.47 ppm, which is smaller than the average RMSE of the CT2019B simulation (5.36 ppm). Based on the OCO-2 XCO2 concentrations, the average RMSE of the simulated XCO2 concentrations in WRF-Chem was 0.37 ppm, which is smaller than the average RMSE of the CT2019B simulation (0.40 ppm). The relationship between the growth rate of simulated CO2 concentrations and Niño 3.4 index revealed that atmospheric CO2 concentrations increased as the uptake of CO2 by vegetation weakened after the occurrence of El Niño events. Therefore, the simulated high-resolution atmospheric CO2 concentrations in East Asia in WRF-Chem over 10 years resembled the observed values and could be highly valuable in understanding the carbon cycle in East Asia. Acknowledgments: This study was supported by a National Research Foundation of Korea (NRF) grant funded by the South Korean government (Ministry of Science and ICT) (Grant 2021R1A2C1012572) and the Yonsei Signature Research Cluster Program of 2023 (2023-22-0009).
BG05-A006
Isolation and Characterisation of Potential Plant Growth-promoting Bacteria
Annelize CHEUNG+, Kung Ming LEUNG, Grace LAI, Simon GRIFFIN#
The ISF Academy, Hong Kong SAR
Global food security will require agricultural intensification, together with fertilisers and crop protectants. But chemical fertilisers (already c. 200 million tonnes globally in 2023) and fungicides, such as azoles, are not only expensive but also cause significant damage to ecosystems and even human health. This project has therefore aimed to isolate and characterise plant growth-promoting bacteria (PGPB) with potential for use as part of a sustainable bio-fertiliser. PGPB may be able to solubilise phosphate, transport trace metals, synthesise plant hormones and protect against pathogens.Raphanus raphanistrum subsp. sativus seeds provided a useful source of plant-associated bacteria, which could be recovered from saline washes. Plant growth-promoting activities were assayed using a variety of functional tests and promising isolates streaked to purity before DNA extraction and sequencing via both Illumina NovaSeq and Oxford Nanopore MinION platforms. The complete genomes of three isolates, AZCO, AZA and AZB, constructed by hybrid assembly, were annotated and analysed using BV-BRC and NCBI BLAST. Microbacterium sp. AZCO (4.11 Mbp, 70.42% G+C) contains genes related to phosphate-solubilisation and IAA synthesis and is able to enhance the growth of Medicago sativa seedlings grown on Pikovskaya’s agar. Bacillus altitudinis AZA (3.68 Mbp, 41.32% G+C) and Bacillus tequilensis AZB (3.96 Mbp, 43.89% G+C) both display antifungal activity towards Aspergillus oryzae, siderophore production, as well as growth on Kraft lignin as the sole source of carbon. AZA also demonstrated cellulase production on CMC agar.
BG05-A013
Investigating the Impact of Model Complexity on the Global Performance of Canopy Radiative Transfer Simulation
Denis GROSHEV1#+, Hyungjun KIM1,2
1Korea Advanced Institute of Science and Technology, Korea, South, 2The University of Tokyo, Japan
This research presents an in-depth intercomparison among several three-dimensional radiative transfer models (RTMs) to evaluate their performance in simulating canopy absorptance and reflectance at different levels of model complexity. The RTMs under examination include simpler models like the flat plate model, intermediate complexity models such as three-layer spherical bush model, SPARTACUS (which segments canopy into 3-layer regions), and more complex ones like FLiES (using Monte-Carlo ray tracing). The simulations are carried out combining remote sensing (e.g., ALOS PALSAR, LandSat) and physically-based information (e.g., solar position). The focus of this study is on the East Asian region, spanning a scale of 0.1° spatial resolution. The methodology involves satellite imagery post-processing, including Savitzky–Golay filter to smooth out noise and Leaf Area Index (LAI) retrieval from NDVI data. The high resolution slope and aspect of terrain, crucial for the proper simulation of surface radiation budget regarding solar geometry, are determined using the MERIT digital elevation model. The relative solar position (i.e, zenith and azimuth angles) at varying time steps is calculated using a NASA algorithm. Forest geometry and density are defined based on the MODIS Land Cover Classification dataset. The comparative analysis of radiative transfer models has yielded fundamental information about the impacts of specific environmental factors, such as forest LAI and soil albedo, on canopy crown absorptance and reflectance. It has also underscored the significance of proper representation of forest geometry, such as tree shape, height, and density distributions, in enhancing the accuracy of large-scale simulations. This study lays the groundwork for a novel approach for estimation of uncertainty in global surface energy balance simulations, which is vital for improved Earth system modeling.
BG06-A001
Warm Early Summer Compensated Reduction in Photosynthesis Caused by 2022 Late Summer Extreme Drought Over the Tibetan Plateau
Xunmei WANG+, Jun WANG#, Ran YAN, Jingye TAN, Weimin JU
Nanjing University, China
The Tibetan Plateau (TP) is ecologically delicate, its vegetation highly sensitive to climate variations. In 2022, China endured an unprecedented compound drought-heatwave, escalating TP’s August temperature to a record high since 2000. This study examined this event’s impact on TP’s photosynthesis using multi-source satellite-based products. We demonstrated persistent high temperatures from April to August 2022, accompanied by shifting soil water. Initially moist from April to June, the soil turned notably dry, hitting its lowest point in August. Consequently, early summer witnessed a substantial enhancement in gross primary productivity (GPP) and near-infrared reflectance of vegetation (NIRv) predominantly due to high temperatures, except for reduction in the eastern and southeastern TP. June recorded the largest positive GPP anomaly since 2000. As summer progressed, severe drought, not high temperatures, dominated, causing obvious negative anomalies in GPP and NIRv, especially in August, concentrated in the central and southwestern TP. Separating the growing season into May-June-July (MJJ) and August-September (AS) revealed a clear contrast. Enhancement in photosynthesis during MJJ compensated the decline in AS, making average positive GPP and weak negative NIRv anomalies in the entire growing season. Specifically, MJJ saw GPP magnitudes of 5.724 TgC mo−1 in FluxSat, 9.491 TgC mo−1 in GOSIF, and 0.004 in NIRv. Conversely, AS experienced a decline: −4.802 TgC mo−1 in FluxSat, −2.837 TgC mo−1 in GOSIF GPP, and −0.006 in NIRv. This delicate balance underscores the intricate interplay between early growth conditions, subsequent environmental stressors, and vegetation's adaptive responses.
BG06-A004
Aboveground Carbon Sequestration of Cunninghamia Lanceolata Forests: Magnitude, Drivers, and Management Option
Chen WANG1+, Shuguang LIU2#, Yu ZHU2
1Hainan University, China, 2Central South University of Forestry and Technology, China
Understanding the spatial variation, temporal changes, and their underlying driving forces of carbon sequestration in various forests is of great importance for understanding the carbon cycle and carbon management options. How carbon density and sequestration in various Cunninghamia lanceolata forests, extensively cultivated for timber production in subtropical China, vary with biodiversity, forest structure, environment, and cultural factors remain poorly explored, presenting a critical knowledge gap for realizing carbon sequestration supply potential through management. Based on a large-scale database of 449 permanent forest inventory plots, we quantified the spatial-temporal heterogeneity of aboveground carbon densities and carbon accumulation rates in Cunninghamia lanceolate forests in Hunan Province, China, and attributed the contributions of stand structure, environmental, and management factors to the heterogeneity using quantile age-sequence analysis, partial least squares path modeling (PLS-PM), and hot-spot analysis. The results showed low values of carbon density and sequestration on average, in comparison with other forests in the same climate zone (i.e., subtropics), with pronounced spatial and temporal variability. Specifically, quantile regression analysis using carbon accumulation rates along an age sequence showed large differences in carbon sequestration rates among underperformed and outperformed forests (0.50 and 1.80 Mg ha−1 yr−1). PLS-PM demonstrated that maximum DBH and stand density were the main crucial drivers of aboveground carbon density from young to mature forests. Furthermore, species diversity and geo-topographic factors were the significant factors causing the large discrepancy in aboveground carbon density change between low- and high-carbon-bearing forests. Hotspot analysis revealed the importance of culture attributes in shaping the geospatial patterns of carbon sequestration. Our work highlighted that retaining large-sized DBH trees and increasing shade-tolerant tree species were important to enhance carbon sequestration in C. lanceolate forests.
BG06-A006
Analysis of Water-energy-food-carbon Nexus of Small Hydropower Basin in Hunan Province, China
Zhenglong WANG+, Shuguang LIU#
Central South University of Forestry and Technology, China
Under the background of water resources shortage and climate change, the water-energy-food-carbon(WEFC) nexus is facing great challenges in Ouyanghai Irrigation Basin(OIB) of Hunan Province, China. Moreover, The impact of the development process of green small hydropower(SHP) on the social-ecosystem is still unknown. In this study, the relationship framework of water, energy, land use and food in OIB was constructed by surveys and material flow methods. Next, by leveraging the principles of physics coupling, exploring the coupling mechanisms and functional relationships among WEF nexus. The results show that: (1) the area of forest and impervious surface in irrigation areas and catchments has increased in the past 30 years, and in irrigation areas has increased from 128.6km2 in 1987 to 175.7km2 in 2020. The area of bare and farmland has declined to varying degrees, so SHP plays an important role in the diversion and irrigation of bare. (2) From 2004 to 2010, there was a correlation between irrigation water volume and crop yield, which r=0.74, P=0.05; From 2011 to 2013, it disappeared; But from 2014 to 2020, it restarted, r=0.76 and p<0.05. The results suggest that the irrigation role played by SHP is highly significant for crop production. The volume of irrigation water provided by SHP could be a direct factor affecting crop yields. (3) From 2004 to 2020, the coupling degree of WEF is mostly greater than 0.8, showing that the system is in a high-level coupling stage. To some extent, there is a complex relationship within it. And the coupling coordination values predominantly fall within the range of 0.7 to 0.9, suggesting that the interactions among the three subsystems are in a phase of transitioning from moderate to high coordination. This study provides the reference for the coordinated development of WEFC nexus in other SHP basins.
BG06-A014
Estimation of Carbon Budget in the Forest Ecosystem of Hunan Province, China, Based on the GEMS Model
Zhaozhen HOU+, Shuguang LIU#
Central South University of Forestry and Technology, China
The accurate estimation of the carbon budget of forest ecosystems is crucial for achieving the Sustainable Development Goals (SDGs). Although there are already many studies on the dynamics of carbon cycle in forest ecosystems, how accurate and whether they can be further improved remains to be seen. The General Ensemble Biochemical Modeling System (GMES) integrates several biogeochemical processes and closely interacts with grid-scale, human-driven factors, such as disturbances and management activities, thereby enhancing the simulation of carbon cycling in a natural, socially coupled system. The GMES is used to simulate the dynamics of ecosystem carbon budget in a typical natural-social coupled system from 1985 to 2021 in Hunan, China, with a spatial resolution of 30 m. Results of the analysis reveal that the forest ecosystem in Hunan Province has an estimated 177.79 Mg C/ha carbon density with a growth rate of 1.39 Mg C/ha/y. The carbon densities of the tree layer and soil layer increased at rates of 0.72 Mg C/ha/y and 0.41 Mg C/ha/y, respectively. The total carbon sequestration of the forest ecosystem is 621.48 Tg C, which successfully offsets 41.28% of apparent carbon emissions since 1997. Changes in land cover and forest management practices are primary factors influencing ecosystem carbon sequestration. A significant increasing trend (P<0.01) was observed in the forest ecosystem carbon sequestration since the natural forest protection project was implemented in 2000. Temperature and precipitation significantly influenced the carbon sequestration of forest ecosystems in Hunan Province, exhibiting a significant positive correlation (r>0.4, P<0.05) in 61.22% and 42.82% of the regions, respectively. This study used the GMES model to reveal the temporal and spatial characteristics of dynamic changes in the forest ecosystem carbon in Hunan Province, providing crucial mechanism information for maximising forest carbon sink.
BG06-A017
Comparison of the Photosynthetic Response of Plants in Urban and Rural Areas
Wei BAI+, Shuguang LIU#
Central South University of Forestry and Technology, China
Rapid urbanization has exacerbated the variability of urban and rural environments, leading to differences in carbon cycling processes between urban and rural areas. The differential vegetation response to environments factors between urban and rural within the processes of carbon water exchange and water utilization is still unclear. Previous studies have utilized artificial control experiments to measure photosynthesis in laboratory settings. However, urban and rural in situ experiments were conducted to compare the effects of urban and rural environmental differences on vegetation growth and to provide a theoretical basis for understanding the environmental adaptation of plant photosynthesis. This study selected Cinnamomum camphora, L. that grow naturally in urban and rural areas for in situ observation. The gas exchange rate of the plants was measured using a LiCor LI-6800 portable gas exchange system (LI-COR Inc.). Among the photosynthetic characteristic indicators, the study found differences between urban and rural plants, including the Rubisco carboxylation (Vcmax), net photosynthetic rate (Pn), stomatal conductance (gs), stomatal limitation (Ls), water use efficiency (WUE), and light energy use efficiency (LUE). The correlation between Vcmax and Pn is stronger in rural areas (r=0.86, p<0.001) than in urban areas (r=0.58, p<0.001), and the two are positively correlated. To achieve the same Pn, plants in rural areas need to have higher stomatal conductance. This study investigates the effect of environmental variations on the photosynthetic properties of plants in urban and rural areas. This study provides detailed measurements of the photosynthetic characteristics of plants in urban and rural environments and lays the foundation for a terrestrial ecosystem model simulation.
BG07-A002
Trace of Water Pollution in the Tokoro River Basin Using Rare Earth Elements
Kanta ITO+, Katsuaki KOMAI#
Kitami Institute of Technology, Japan
The study aimed to investigate the impact of human activities in a watershed and river water pollution on rare earth elements (REEs), elucidating whether REEs could be indicators of anthropogenic contamination at the spatial scale of the watershed. Water samples were collected from 20 locations along the Tokoro River flowing through Kitami City in northern Japan, and the concentrations of 14 REEs at sub-ppb levels were measured. Correlation coefficients between REE concentrations at each location and various factors within the watershed, such as population density, land-use ratio, flow rate, suspended solids concentration, total phosphorus, total nitrogen, and biochemical oxygen demand, were calculated. The significance of these correlations was statistically tested using two different methods. The correlation between the concentrations of light REEs and flow rate, total nitrogen, suspended solids concentration, population density, and land designated for buildings were significantly found among the factors analyzed. Spearman's rank correlation coefficient was more statistically significant than Pearson's correlation. These findings suggest that light REEs have the potential to be indicators of anthropogenic pollution sources, but their non-linearity should be paid attention.
BG07-A008
Source Identification of Methylmercury in Rainwater Using Concentration Weighted Trajectory Analysis
MinJeong KIM+, Mihret Yihalem ABEBE, Jisook YANG, Seunghee HAN#
Gwangju Institute of Science and Technology, Korea, South
This study investigated the sources of methylmercury (MeHg) in wet deposition collected in Gwangju, a suburban area of South Korea. Weekly rainwater samples were collected from January 2017 to December 2021, and MeHg concentrations of rainwater were analyzed. The volume-weighted mean (VWM) concentration of MeHg was determined to be 0.045 ng L-1 and the annual wet deposition flux of MeHg was found to be 0.040 ng m-2. When seasonal variations were considered, the highest VWM concentrations of MeHg found in winter and the highest wet deposition fluxes in summer, as was reported previously. We also noted a positive correlation between PM2.5 and MeHg concentrations, and the correlation factor increased in spring. In the source identification for MeHg in rainwater using concentration weighted trajectory analysis, the air mass inflow from northwest direction was identified as a significant source of MeHg in spring rainwater, indicating importance of Yellow Dust. On the contrary, the air mass inflow from the ocean was identified as a main source of MeHg in summer rainwater, indicating that photodemethylation of dimethylmercury evaded from sea surface significantly contributes to MeHg in summer rainwater. Overall, this study highlights that sources of atmospheric MeHg are diverse and major one is varied by season.
BG07-A010
A Geomicrobiological Perspective to Decipher the Cross Talk Between Nitrogen and Arsenic Biotransformation in Arsenic Impacted Paddy Soil of West Bengal
Shuchishloka CHAKRABORTY+, Rajendra Prasad SAHU, Pinaki SAR#
Indian Institute of Technology Kharagpur, India
Paddy soil is a heterogenous ecosystem that harbours diverse microbial and geochemical landscapes, critical for maintaining ecosystem sustainability and crop yield. Nitrogen (N) is an essential element that supports the ecosystems' productivity. However, a detrimental effect of arsenic (As) on the soil ecosystem is observed due to the increased reliance on As-contaminated groundwater for irrigating the paddy fields. Nevertheless, little is known regarding the undercurrents of major taxa involved in N-As/Fe metabolism, along with other multifaceted interactions. This study aimed to comprehend the N-As crosstalk and multifaceted interactions involved in As biotransformation in paddy soil through a microcosm-based, culture-dependent approach. Characterization of soil parameters depicted the impact of As on soil parameters that maintain soil health and productivity. A significant change in the dominant dissolved N species and As concentration was observed, which was further confirmed by the qPCR analysis of N marker genes, ammonia monooxygenase (amoA), nitrogenase (nifH), nitrite reductase (nirS) and nitrate reductase (narG). Solid and aqueous phase geochemical analyses through X-Ray diffraction, X-photoelectron spectroscopy, and inductively coupled plasma mass spectroscopy signify the role of microbiome in catalyzing considerable alterations in As-bearing mineral phases, resulting in substantial changes in overall geochemistry. The abundance of multifaceted Actinobacteria, Acidobacteria, Sphingomonas, Nitrosomonadaceae, and Nitrososphaeraceae characterized the abundantly present core community and exhibited close interactions among each other that drive the N-As interaction. Functional prediction of the microcosm highlighted major biochemical pathways and plant growth-promoting factors (polyphosphate hydrolysis and auxin biosynthesis). All these major biogeochemical processes were found to be catalyzed by the members of most abundant/core community. This study provides a geomicrobiological insight into diversity, composition, strong biotic interactions and functional potential of microbial communities involved in the biotransformation of N and As in the heterogenous As contaminated paddy soil, summarizing nitrogen as a key player in As mobilization.
BG09-A002
Impacts of Extreme Droughts on Ecosystem Water Use Efficiency Diverge Between Forest and Grassland
Mengtian HUANG#+
Chinese Academy of Meteorological Sciences, China
Ecosystem-scale water use efficiency (WUE), as a quantification of the coupling between carbon and water cycle, determines whether vegetation could survive under severe drought stress. Nevertheless, how extreme droughts affect ecosystem-scale WUE and its difference among regions and biomes are still poorly understood. In this study, using data-oriented gridded products of gross primary productivity (GPP) and evapotranspiration (ET), we assessed the ecosystem WUE change during extreme drought years over China, and further compared drought impacts on WUE between forest and grassland ecosystems. We found a spatial heterogeneity of WUE change in response to extreme droughts across regions. Particularly, grassland WUE was substantially reduced concurrent with suppressed photosynthesis, while most of forest exhibited slightly decreased or even increased WUE under extreme droughts. In addition, we demonstrated that drought characteristics and environmental conditions modulated drought impacts on WUE. Temperature anomalies during droughts and leaf area were found to be the predominant factors driving WUE change for both forest and grassland. With increasing occurrence of compound dry and hot extremes, our results, therefore, would be an insightful supplement to the current understanding of the influence of extreme events on terrestrial ecosystems.
BG09-A004
Response of Air-sea CO2 Flux to Strong ENSO Events in Warm/cold PDO Phase in the Tropical Pacific
Xiaowen WANG1+, Xiujun WANG2,3#, Prabir K. PATRA4,5, Rong-Hua ZHANG6
1Beijing Normal University, China, 2Shanxi Agricultural University, China, 3University of Maryland, United States, 4Japan Agency for Marine-Earth Science and Technology, Japan, 5Tohoku University, Japan, 6Chinese Academy of Sciences, China
The tropical Pacific plays a big role in the global carbon cycle due to its significant CO2 outgassing and large influence on the temporal variability of global ocean-atmosphere CO2 fluxes. There is evidence of strong interannual-to-decadal variability in physical and biogeochemical processes in this region, associated with the El-Nino/Southern-Oscillation (ENSO) and Pacific Decadal Oscillation (PDO), with implications for carbon sources and sinks. However, the understanding is incomplete regarding modulation effects of PDO on the impacts of ENSO events on carbon cycle in the tropical Pacific. Here, we employ a validated basin-scale physical-biogeochemical model to simulate carbon cycle, and evaluate responses of key parameters to the strongest ENSO events over 1980-2020, i.e., 1997-98 El Niño (97EN), 2015-16 El Niño (15EN), 1988-89 La Niña (88LN) and 2007-08 La Niña (07LN). We then analyze and compare the differences in sea surface temperature (SST), dissolved inorganic carbon (DIC), primary productivity (PP), sea minus air pCO2 (ΔpCO2) and CO2 outgassing between the warm and cold ENSO events across the warm and cold PDO phases. Our study shows a significant DIC decrease during 97EN and 15EN, and a significant DIC increase during 88LN and 07LN. However, the anomaly was greater in the central/eastern basin during the warm PDO phase (i.e., 97EN and 88LN), but in western-central section during the cold PDO phase (i.e., 15EN and 07LN), which was also seen in SST anomaly. ΔpCO2 was much lower during 97EN and 15EN than during 88LN and 07LN, with significant differences over 5°S-5°N. Similarly, fCO2 also revealed a much lower level during 97EN and 15EN than during 88LN and 07LN, with larger anomalies in eastern basin during the warm PDO phase than cold PDO phase. We will further investigate the biogeochemical influence of PDO in the tropical Pacific in the future.
BG09-A005
Seasonal and Interannual Variations of Soil Heterotrophic Respiration and Autotrophic Respiration in Inner Mongolia Grassland from 2002 to 2021
Bingyan JIN1#+, Xiujun WANG2,3
1Beijing Normal University, China, 2Shanxi Agricultural University, China, 3University of Maryland, United States
Soil respiration is a key component of the carbon cycle in terrestrial ecosystems, which consists of heterotrophic respiration (HR) and autotrophic respiration (AR). There is evidence of large differences in the seasonal and interannual variability between HR and AR. However, there is a lack of process-based models that simulate HR and AR separately. We calibrated/validated HR and AR models using field data at two typical grassland sites and one desert grassland site in the Inner Mongolia grassland. Then we applied the validated models and satellite data to estimate HR and AR at these sites over 2002-2022. Our results showed a greater season aptitude in HR (2.4-2.9 g C m-2 d-1) than in AR (1.2-1.6 g C m-2 d-1), but a greater interannual variation in AR (NCV: 12-171%) than in HR (NCV: 7-48%). The interannual variability was much stronger in winter than in other seasons for both HR and AR, particularly at the typical grassland sites. The main driving factor of interannual variability was soil temperature for HR, and fine root biomass and gross primary productivity for AR in the Inner Mongolia grassland. This study will contribute to our understanding of key processes regulating carbon cycle in grassland ecosystems.
BG09-A006
Impacts of Nitrogen Fertilization on CO2 Efflux with and Without Organic Amendments in a High-pH Soil
Haolin ZHAO1#, Xiujun WANG2,3+, Minggang XU4
1Beijing Normal University, China, 2Shanxi Agricultural University, China, 3University of Maryland, United States, 4Chinese Academy of Agricultural Sciences, China
Organic amendments and nitrogen (N) fertilization are common practices in agriculture, which have complex influences on the carbon sources and sinks. To evaluate the effects of N-organic carbon combination on CO2 efflux, an over 20-months field incubation experiment with straw/biochar amendments was carried out in a typical soil of North China Plain. We measured CO2 efflux every ~2-4 weeks, and water extractable organic carbon (WEOC) soil microbial biomass carbon (SMBC) in spring, summer and autumn. Our results showed an asymmetric seasonality (slow increasing in spring but rapid decreasing in fall) in the control and biochar treatments, but a symmetric seasonality under straw treatments. For the straw treatments, the increase of CO2 efflux was greater in the first spring than in the second spring. Over the period of 20-months, N fertilization led to a much greater increase in cumulative CO2 efflux with organic amendments (i.e., 7%-13% under biochar and 20% under straw treatment) than without organic amendments (3%). The increase of CO2 efflux under N-straw/biochar combination might be largely attributed to the enhancement in SOC decomposition and break-down of straw/biochar due to the priming effects. The greater increase of CO2 efflux under N-straw treatment was primarily related to the relatively higher content of labile organic carbon in straw. The enhancement of CO2 efflux under N-organic C combination was pronounced mainly in the first year, indicating an early release of CO2 due to decomposition of labile organic carbon in straw/biochar, which was not persistent. Our study highlights that N fertilization with organic amendments can cause changes in various processes of CO2 production in the cropland of north China.
BG09-A009
Decadal Variability of Sea-to-air CO2 Flux in the Tropical Pacific Ocean: Effects of Solubility Pump and Biological Pump
Xiujun WANG1,2#+, Xiaowen WANG3, Rong-Hua ZHANG4
1Shanxi Agricultural University, China, 2University of Maryland, United States, 3Beijing Normal University, China, 4Chinese Academy of Sciences, China
The tropical Pacific plays a big role in the global carbon cycle because of its vast expanse and significant air-sea CO2 flux. There is evidence of large interannual to decadal variability in oceanic physical and biogeochemical processes, which is associated with the El Niño/Southern Oscillation (ENSO) and Pacific Decadal Oscillation (PDO). While numerous studies have demonstrated much greater rates of outgassing during cold ENSO phases, little is known on the impacts of PDO regime shift on sea-to-air CO2 flux in the tropical Pacific. Here, we employ a validated and refined basin-scale physical-biogeochemical model to simulate the carbon cycle in the tropical Pacific over 1980-2022. We then evaluate the differences of sea surface temperature (SST) and dissolved inorganic carbon (DIC), ΔpCO2 and air-sea CO2 flux, together with primary productivity and export production between 1980-1998 (warm PDO phase) and 1999-2022 (cold PDO phase). Our analyses show that cooling occurred in majority of the basin with a significant decrease of SST in the southeast and west parts whereas surface DIC showed a significant increase only in the west warm pool but a modest decrease in northeast section over 1999-2022. The lack of DIC increase in the southeast (where cooling occurred) was attributable to enhanced biological uptake of DIC and export production, resulting from strengthened upwelling during the cold PDO phase. The spatial pattern in change of ΔpCO2 was similar to that of DIC, indicating a dominant role of DIC over decadal timescale. Decadal change in air-sea CO2 flux showed a large similarity in the spatial pattern to that of ΔpCO2, except in the southeast where an increase occurred, which reflected stronger winds over 1999-2022. Our study highlights that there are large differences in responses of solubility pump and biological pump over decadal time scale among different sections of the tropical Pacific Ocean.
BG09-A012
The Great Climate Mitigation Potential of Terrestrial Ecosystem in China
Huan ZHENG+, Bin HE#
Beijing Normal University, China
Limiting climate warming to below 2°C requires more intense mitigation efforts. Alongside the steep reductions in fossil fuel emissions needed, natural climate solutions (NCS) act as an additional first step toward achieving China's emission reduction goals. We first quantified the historical contribution of NCS as 0.34 PgCO2 equivalent (PgCO2e) yr−1 through the implemented national ecological restoration projects as well as positive management measures. Based on successful practices, we then designed 21 pathways to quantify the potential of NCS in increasing terrestrial carbon sinks or reducing greenhouse gas (GHG) emissions in forest, grassland, cropland, and wetland ecosystems. We show that the maximum mitigation potential of NCS between 2020 and 2060 under guaranteed food and fiber security is 1.95 (1.54–2.38) PgCO2e yr−1 (95% CI), which can offset nearly 20% of the annual net emissions. Historically, forest ecosystems have contributed the most to carbon sequestration; however, future projections show cropland ecosystems will account for the largest proportion (47.6%), followed by forest ecosystems. Approximately 47% (0.91 PgCO2e yr−1) of the maximum represents cost-effective mitigation potential that can be realized at ≤100 USD/MgCO2e. Conservation tillage is the most cost-effective option in China, achieving a maximum contribution of 181.60 TgCO2e yr−1. In addition, a series of cropland management measures have contributed 1.14 PgCO2e in the past two decades. Our study highlights the high effectiveness of cropland pathways in reducing carbon emissions and emphasizes the key role of cropland ecosystems in mitigating climate change.
BG12-A001
Patterns and Drivers of CO2 and CH4 Dynamics in the Subtropical Pearl River
Shuai CHEN+, Lishan RAN#
The University of Hong Kong, Hong Kong SAR
The rapid urbanization in China and all over the world has led to significant alterations in riverine carbon cycling, contributing multiple influences on carbon dioxide (CO2) and methane (CH4) dynamics. However, there is a lack of comprehensive studies examining the importance of land use in carbon emissions across entire large river networks. Here we explore the controlling factors of CO2 and CH4 in the subtropical Pearl River, the second-largest river in China in terms of discharge. Our analysis covers 62 streams and rivers spanning 8 Strahler orders of the Pearl River basin. We found land use and aquatic metabolism play significant roles in regulating both gases. Dissolved oxygen, stable isotopes of surface water DIC, the proportion of impervious surface, catchment slope, and river width emerge as major predictors for partial pressure of CO2 (pCO2). For partial pressure of CH4 (pCH4), the major predictors were Chl-a and water temperature. Seasonal variations in pCO2 and pCH4 were strongly influenced by hydrology and climate. These findings highlight the likelihood of significant shifts in riverine carbon emissions as climate change and land use patterns evolve, thereby impacting global carbon cycles profoundly.
BG12-A003
Long-term Acid Deposition Inhibits the Consumption of CO2 by Weathering of Silicic Rock
Qianqian YANG#+
The University of Hong Kong, Hong Kong SAR
Acid deposition inhibits CO2 from participating in chemical weathering, thus reducing the acid buffering capacity (ANC) of the runoff. If these processes are ignored, CO2 consumption would be overestimated. In this study, we examined the role of sulfuric and nitric acids in modulating chemical weathering in a carbonate-deficient watershed (Dinghushan) in south China that once suffered from heavy acid deposition by analyzing hydrochemical composition and δ13C-DIC value of spring and stream water. The results showed that Ca2+ was the dominant cation (41.7%) through the watershed, and the dominant anion changed from NO3- (50.9%) in the upstream to HCO3- (65.6%) in the downstream. The composition of water samples also changed from being controlled by nitric and sulfuric acid weathered silicate rock to controlled by carbonic acid weathered carbonate rocks. The upstream silicate weathering rate is 15.96 t km-2 a-1, of which sulfuric and nitric acid combined contributed to approximately 64%, whereas carbonic acid contributed to the remaining 36%. The associated CO2 consumption rate is only 0.5×105 mol km-2 a-1 due largely to the inhibited CO2 consumption by sulfuric and nitric acids. Continuous reduction in acid deposition in the recent 20 years has resulted in a significant enhancement in the acid buffering capacity in the watershed with NO3- replacing SO42- as the dominant acid-causing ion, although it has not yet completely recovered from the historical acidification. The finding suggested that in acid-sensitive watersheds, the recovery of stream chemistry lags behind the reduction of acidic deposition and continuously inhibited CO2 consumption by rock weathering.
BG12-A005
Spatiotemporal Patterns and Drivers of Carbon Source and Sink from China's Lakes and Reservoirs
Kun SUN#+, Yang GAO
Chinese Academy of Sciences, China
Lakes and reservoirs act as active carbon (C) reactors and regulators, both play an important C balance role in aquatic ecosystems. In China, primary C cycling indicators, including phytoplankton primary productivity (PP) and carbon dioxide (CO2) flux, have been widely studied in various lake systems; However, most relevant studies were focused on individual lakes, there still exists a large knowledge gap on the spatiotemporal patterns and drivers of C source and sink in China’s lakes and reservoirs at a national scale. To evaluate the magnitude of C source and sink from China’s lakes and reservoirs, we developed a bio-optical model-based and machine learning model-based approach to estimate the lake PP and CO2 flux based on national real-time water quality monitoring data. At national scale, the phytoplankton carbon sequestration capacity and CO2 emission flux was estimated at 18.69(± 10.7) Tg C yr−1and 6.78(± 2.5) Tg C yr−1 respectively. If transported and buried C are ignored in the estimates (allowing for the fact that no accurate estimations currently exist), China’s lakes and reservoirs over recent years could be regarded as a large C sink, with a C sequestration capacity of 11.9 Tg C yr-1. Chlorophyll a content, total nitrogen (TN), total phosphorus (TP), and turbidity were determined to be the major drivers of PP; while pH, dissolved oxygen(DO) and air temperature were identified as the general environmental controls of CO2 flux. For the first time, this study clarifies the spatiotemporal patterns and drivers of PP and CO2 flux from China’s lakes and reservoirs, providing a more complete C budget picture of China’s aquatic ecosystems.
BG12-A014
Biogeochemical and Climatic Drivers of CO2 Fluxes from China’s Inland Waters
Yongli ZHOU#+, Shuai CHEN, Boyi LIU, Yuxin LI, Qianqian YANG, Lishan RAN
The University of Hong Kong, Hong Kong SAR
Along the land-to-ocean aquatic continuum, inland waters (rivers, lakes, and reservoirs) are typically sources of atmospheric CO2 due to the extensive remineralization of terrigenous organic carbon that enters the inland waters. Inland waters in China, where some of the world’s largest rivers and half of the world’s reservoirs are located, are currently emitting a total of 98 Tg C of CO2 to the atmosphere annually, about 5% of the global total fluxes. Carbon emissions from inland waters represent an important component of the global carbon budget and regulate global warming, thus it is crucial to understand its biogeochemical and climatic drivers. In this study, we develop a statistical model using machine-learning algorithms for calibrating relationships between the biogeochemical and climatic variables and the partial pressure of CO2 and CO2 fluxes in Chinese inland waters, based on field measurements of water chemistry and remote sensing data. Following this model development, we examine how CO2 fluxes from China’s inland waters in different climatic zones are controlled by individual biogeochemical variables of the upstream terrestrial ecosystems, e.g., net primary production and soil organic carbon, and climatic drivers, e.g., precipitation and temperature.
BG12-A016
Drivers of Fluvial Carbon Cycling in the Upper Changjiang (Yangtze) River, China
Jun ZHONG#+, Si-Liang LI, Sheng XU, Congqiang LIU
Tianjin University, China
Rivers play an important role in global carbon cycling, but there are still large uncertainties concerning riverine carbon sources and fates. Traditionally, dissolved inorganic carbon (DIC) was considered as weathering product and its isotopes (i.e., δ13CDIC and Δ14CDIC) can bring the information of weathering. However, many biogeochemical processes shift the δ13CDIC and Δ14CDIC, masking the weathering information. In addition, the behaviors of DIC in response to short-term climate variabilities are still unclear. Herein, we investigated DIC concentrations, δ13CDIC and Δ14CDIC on spatial and temporal scales in Chinese rivers to uncover the carbon dynamics to short-term climate variabilities and under the controlling factors on carbon biogeochemical processes. Carbon isotopes do not support the theory of weathering in close system, because Δ14CDIC in carbonate-rich catchments also show high values. In contrast, we found that climate variables control the Δ14CDIC on the spatial scale, showing the changing carbon biogeochemical processes under diverse circumstances. In addition, δ13CDIC had negative relationship with changing runoff, and Δ14CDIC showed positive relationship with changing runoff, both of which indicates the influx of biological DIC in the warm and wet season. Overall, we proposed that climate-driven biological carbon activities control the carbon biogeochemical processes, and our study has great implications on understanding global carbon cycle.
BG12-A018
The Impact of Extreme Rainfall on Carbon Emissions from Inland Waters
Yuxin LI#+, Lishan RAN, Yongli ZHOU, Shuai CHEN, Boyi LIU, Qianqian YANG
The University of Hong Kong, Hong Kong SAR
In the face of intensifying global warming, the frequency of extreme weather events, including heavy rainfall, has been on the rise. These events have the potential to significantly impact carbon dynamics in inland water systems, with implications for carbon dioxide (CO2) and methane (CH4) emissions. Assessing the effects of extreme rainfall events on carbon release from inland waters is of utmost importance for a greater understanding of the global carbon cycle. This study aims to tackle this issue by employing machine learning models to simulate carbon emissions from various types of inland water bodies, including lakes, rivers, and reservoirs, based on measured and remote sensing data. By comparing the spatiotemporal patterns of carbon emissions with and without extreme rainfall events, the research can unveil the complex interactions between precipitation patterns and carbon dynamics in aquatic ecosystems. The findings of this study will have important implications for predicting and managing carbon budgets in inland water systems under future climate scenarios.
BG12-A020
A Study of Active Phytoplankton Fluorescence in the Carbon Supersite in the Gdansk Basin of the Baltic Sea
Kristina BOROVKOVA#+, Sergey MOSHAROV
Russian Academy of Sciences, Russian Federation
The Gdansk Basin is one of the most eutrophied areas of the Baltic Sea. The basin is subject to limited water exchange with the North Sea, salinity and temperature barriers between surface and bottom waters, and zones of anoxia. In this area, with the support of the Ministry of Education and Science of Russia, the Carbon Supersite "Rosyanka" has been established. The aim of this project is to develop and test carbon balance management technologies. The primary productivity of phytoplankton plays a substantial role in reducing the concentration of carbon dioxide in the surface layer, and hence removing it from the atmosphere. Carbon is assimilated into organic matter during photosynthesis and is subsequently transferred from surface water to deeper layers through ingestion by vertically migrating animals or when submerged. Hence, our focus at this supersite was to assess the potential productive capacity of phytoplankton across different seasons using the active chlorophyll a fluorescence method. Active fluorescence parameters were measured by using a pulse fluorometer Water-PAM (Walz). Profile of underwater PAR and incident PAR illumination was performed by using Li-Cor complex. The maximum quantum efficiency of phytoplankton was considered in this work. It shows what fraction of absorbed light energy can be directed to photosynthesis under optimal conditions. The collected data revealed that phytoplankton consistently maintains a high level of photosynthetic activity throughout the annual cycle. Across all months, there is a natural decline in photosynthetic activity with increasing depth. The highest values of maximum quantum efficiency were observed in the subsurface layer. At all horizons there is a decrease of values in May, June and July, which is explained by the exhaustion of phytoplankton potential during active photosynthesis. July was the month with the lowest values of maximum quantum efficiency. In general, phytoplankton maintained high potential productive capacity throughout the study period.
BG13-A002
An Investigation of Inter-generic Gene Transfer in Bacteria Recovered from Hong Kong Coastal Waters
Jingxuan HU+, Kung Ming LEUNG, Grace LAI, Simon GRIFFIN#
The ISF Academy, Hong Kong SAR
Anthropogenic activities, such as sewage run-off, introduce antimicrobial-resistant microbes and their resistance genes into freshwater and marine environments (Adesiyan et al., 2022; Graves et al., 2021). However, the ease with which these genes may be transferred to aquatic species is unknown, as are any environmental factors, such as climate and other forms of pollution, that might facilitate the process. Escherichia coli strains 6n and 5a, isolated from heavy metal-contaminated coastal sediment in Hong Kong, contain a mobile element encoding tetracycline resistance genes tetR-tetA together with the mercury resistance operon. The homologous motif occurs extensively in Enterobacteriaceae so that, for Wong et al. (2023), its identification in the Vibrio cholerae plasmid pNDM-116-17 suggested inter-generic AMR transfer may be exacerbated by heavy metal pollution. Using E. coli 6n and 5a as donors and a selection of Vibrio spp. isolated from Hong Kong coastal waters, we have investigated inter-generic gene transfer and its possible modulating factors, such as metal ions, salinity and temperature. In these two E. coli strains, the location of the mobile element within the plasmid and chromosome respectively has also allowed some comparison between the efficiencies of conjugation vs. transformation. In early results, co-incubations in 3.5% w:v saline of either E. coli 6n or 5a with V. campbellii TDP6, V. harveyi TSW12 or V. parahaemolyticus DVW5 (non-resistant strains, which are easily distinguished from E. coli using CHROMagar™ Vibrio plates) produced marked increases in MIC of tetracycline in all three Vibrio spp., with transfer of the 6n plasmid producing the highest levels of resistance. However, when challenged with 10 µg/mL tetracycline in saline, the efficiency of transformation with E. coli 5a exceeded that of conjugation.
BG13-A003
Study on the Effects of Soil Microbiome on Arsenic Extraction by Iron Reducing Bacteria
Eui-Jeong HWANG1+, Yejin CHOI1, Hyeop-Jo HAN2, Jong-Un LEE1#
1Chonnam National University, Korea, South, 2Korea Institute of Geoscience and Mineral Resources, Korea, South
We investigated the impact of indigenous microbial communities on arsenic release by Shewanella putrefaciens in agricultural soil near abandoned metal mines. Out of 49 soil samples collected, eight exceeded arsenic contamination concern criteria of Korea. We selected three soils (F1, G7, G10) based on physicochemical properties and dominant species identified through next-generation sequencing. Arsenic concentrations were analyzed during a 28-week experiment under different conditions: sterilized soil + Shewanella, indigenous microbial soil, indigenous microbial soil + Shewanella, and sterilized soil. Elevated dissolved arsenic levels were observed in F1 soil of indigenous microbes + Shewanella at 10 weeks (4,571 μg/L), G7 soil of indigenous microbes at 28 weeks (2,021 μg/L), and G10 soil of indigenous microbes + Shewanella at 28 weeks (1,897 μg/L). Microbial community analysis revealed increased species diversity from 2 to 5 weeks when Shewanella was introduced into indigenous microbial soil. In F1 soil, the dominance of Shewanella (21.7%) at 2 weeks decreased to 0% at 10 weeks, while Clostridium increased from 5.8% to 42.7%. G7 soil showed an increase in Clostridium dominance (8.9% at 2 weeks to 44.8% at 28 weeks). In G10 soil, Shewanella dominance (22.4% at 2 weeks) decreased to 0% at 28 weeks, with Clostridium increasing from 8.0% to 41.7%. The changes in community distribution suggest that the coexistence of artificially injected Shewanella and indigenous microorganisms influences the species diversity and distribution of microbial communities. Long-term experimental results highlight the potential role of Clostridium, as the dominant species, in arsenic behavior, warranting further investigation. Overall, this study sheds light on the complex interactions within soil microbial communities and their impact on arsenic dynamics.
BG13-A004
Stabilization of Heavy Metals in Contaminated Agricultural Soil by Sulfate-reducing Bacteria
Yejin CHOI1+, Eui-Jeong HWANG1, Hui-Yeon KIM1, Hyeop-Jo HAN2, Jong-Un LEE1#
1Chonnam National University, Korea, South, 2Korea Institute of Geoscience and Mineral Resources, Korea, South
Crops cultivated in heavy metal-contaminated agricultural land can pose harmful effects on human health through consumption. Stabilization techniques have been widely applied in the field to remediate contaminated soils. Stabilization involves introducing various organic and inorganic stabilizing agents into the soil to reduce their mobility and bioavailability, thereby preventing their transfer to crops and the surrounding environment. If the soil below the stabilization depth is contaminated with heavy metals, there is a risk of upward mobilization of these metals over time due to capillary pressure. This study conducted experiments to investigate the stabilization of dissolved metals in deep soil by sulfate-reducing bacteria (SRB) through anaerobic respiration utilizing SO42- as an electron acceptor. Soil samples were collected from three agricultural sites near abandoned mines. Stabilization experiments were conducted over nine weeks, with soil supplied with only SO42- (SO4), only SRB (SRB), and both SRB and SO42- (SS). The efficiency of stabilization was evaluated by recovering soil at 1, 4, 7, and 9 weeks, followed by leaching with 0.1 N HCl and the Mehlich 3 single-extraction method for metals. For lead, 0.1 N HCl leaching showed stabilization efficiencies of 26-41% for SO4, 2-6% for SRB, and 26-37% for SS samples. Mehlich 3 leaching exhibited stabilization efficiencies for lead of 26-32%, 12-37%, 26-51% for SO4, SRB, and SS samples, respectively. For zinc and copper, SS samples showed relatively higher stabilization efficiencies, while arsenic did not exhibit clear stabilization effects. Time-dependent soil leachates were also analyzed, indicating a significant reduction in iron leaching in SO4 and SS samples compared to control samples. The results suggest that supplying SRB and appropriate SO42- to deep soil can effectively stabilize heavy metals, demonstrating potential applications for remediating contaminated subsurface soil.
BG13-A005
Assessing Groundwater Contaminations in Areas with High Densities of Private Sewage Treatment Facilities (PSTFs) in Jeju Island, Korea
Mijin KIM+, Man-Young JUNG#, Jinkeun KIM
Jeju National University, Korea, South
Since over 90% of drinking water originates from groundwater in Jeju Island, Korea, protecting the groundwater quality is vital for public health. However, Jeju Island continues to be developed, and even the mid-mountain areas where groundwater is mainly recharged are being developed indiscriminately. One of the issues caused by this overdevelopment is the private sewage treatment facilities (PSTFs) which are installed rapidly to recover the lack of public sewerage network systems in mid-mountain areas. Even though more than 10,000 PSTFs directly discharge effluents into the groundwater and cause groundwater quality to deteriorate, the efficiency of these PSTFs has not been accurately assessed. This study aimed to assess spatiotemporal variations in nitrate and human-origin microorganisms, the main components of contamination in the effluent of PSTF, in groundwater samples in areas with high densities of PSTF installations. According to these results, we intend to use them as a basis for establishing basic legal standards for the installation and management of PSTFs for groundwater conservation in Jeju Island. [This study was supported by Jeju Special Self-Governing Province and Jeju Groundwater Research Center].
BG13-A007
Demethylation of Methylmercury by Mackinawite Nanoparticles
Nida MANSOORA+, Seunghee HAN#, Sangwoo EOM, Eunji JUNG
Gwangju Institute of Science and Technology, Korea, South
Mackinawite nanoparticles (FeS) are commonly found in highly reducing estuarine sediments that are rich in organic matter and sulfides. FeS significantly impacts the availability of trace elements in these sediments. In oxic conditions, oxidation of Fe(II) in the sediment can produce hydroxyl radicals (·OH) at 84.7 μmol ·OH per g of FeS, comparatively higher than generated by zerovalent iron nanoparticles, siderite and pyrite in similar conditions. FeS oxidation is surface-mediated reaction, by which structural Fe(II) on FeS surface transform O2 to ·OH with the formation of H2O2 intermediate. This mechanism significantly contributes to the oxidation of various trace elements, such as Cd, As, Hg, Co, Pb, Cr, Cu, Mn, Mo, Ni, Zn, in sediments containing persistent and abundant FeS. Based on this literature review, we hypothesize that oxidative-reductive demethylation of methylmercury (MeHg) can occur by FeS nanoparticles through Fenton reaction mechanism. Our preliminary results show that even at low concentrations (3 g/L), FeS can demethylate MeHg and the results are being tested further by mass balance of different Hg species formed on the FeS surface, liquid, and gas phase. The demethylation rate constants and mechanism will be suggested by considering the effects of FeS and dissolved oxygen concentration, pH, and Fe(II)/Fe(III) complexation with diverse organic ligands. Considering redox conditions of estuarine sediment, our study suggest that the oxidation of FeS coupled to MeHg demethylation should be concerned due to ·OH production by Fenton or Fe(III) reduction.
BG13-A009
Currents of Contamination: Navigating the Microbial Seascape of Kuroshio's Microplastic Plastisphere
Priyanka MUTHU1+, Sakcham BAIROLIYA 2, Gowri Krishna GIRIJA1, Jiang SHIOU HWANG1, Ying NING HO1#
1National Taiwan Ocean University, Taiwan, 2Nanyang Technological University, Singapore
The surge in oceanic plastic waste is expanding the habitat for microorganisms, with taxonomically distinct microbial communities known as the 'Plastisphere' thriving on plastic materials. This study investigates the microbial populations associated with floating microplastics in the vulnerable Kuroshio circulation of the North-eastern Pacific Ocean, highlighting the intricate relationships between plastics and marine microorganisms. High-throughput sequencing (Oxford Nanopore sequencing) of 16S rRNA was employed to analyze microbiome profiles of microplastic assemblages sampled from the Kuroshio current. Distinct microbial communities exclusive to plastic surfaces were identified, emphasizing the unique nature of the plastisphere. Alpha diversity analysis revealed a significant difference in diversity between surface seawater and plastisphere communities across all stations. Notably, alpha diversity indices were consistently higher on microplastics compared to surface seawater communities (p < 0.05). Using the FAPROTAX database, prokaryotic metabolic functions based on 16S rRNA gene data were analysed. The results showed that chemoheterotrophy and aerobic chemoheterotrophy dominate in wood and seawater, while phototrophy-related functions prevail in plastics. STAMP analysis further uncovered distinct metabolic profiles between seawater, microplastics, and wood, underscoring the influence of substrate type on bacterial functions. This comprehensive study provides insights into the dynamic microbial communities across diverse environments, particularly in the context of plastic pollution. The findings contribute to our understanding of ecosystem dynamics and have implications for effective management strategies in marine ecosystems impacted by plastic waste.
BG15-A001
Three-globe Thermometer: A Novel Instrument for Field Observations in Biogeoscience
Atsushi MARUYAMA#+, Kensuke KIMURA
National Agriculture and Food Research Organization, Japan
A simple formula is proposed to calculate the air temperature from the temperatures of multiple spheres of different size and thus eliminate the effects of radiation on the measurement of air temperature. The formula is derived from energy balance and heat transfer theory for a spherical surface in external flow. Using this formula, we developed an instrument with which to obtain the air temperature from multiple thermocouples with spherical tips (multiple globes) without the need for a radiation shield and ventilation. Field experiments were conducted during summer and winter to determine the best combination of globe diameters from five different diameters (d = 0.25, 0.5, 1, 2, 4 mm). The best combination of globe diameters providing the highest accuracy was 0.25, 1, and 4 mm. The root-mean-square error (RMSE) of this combination for all data was 0.13 °C. The results demonstrate the sufficient accuracy of the proposed thermometer. The proposed thermometer can be used on various ecosystems where mains power is unavailable and expected to be widely used in the field of biogeoscience. The application of this thermometer to field observations in croplands for fine-scale mapping of air temperature on a regional scale will also be presented.
BG15-A003
How Geosciences Can Contribute to Conservation Efforts: A Case Study With Tsunamis and Coastal Species in New Zealand
Jean ROGER#+
GNS Science, New Zealand
Studies have shown that extreme natural events such as asteroid impacts, volcanic eruptions or climatic variations have the capacity to cause the extinction of many species on the surface of the globe in a relatively short period of time. On a smaller scale, it was underlined, through the analysis of past events, that natural hazards such as tsunamis could also have a lasting impact or even make certain species, particularly coastal ones, disappear by killing them directly and/or destroying their habitat. If hazard studies have made it possible to mitigate the impact of natural disasters on people and property in recent decades, this impact has not really been considered with regard to natural environments and the species they shelter, more particularly those which are considered endangered or on the brink of extinction with limited distribution areas and small population sizes. To date, only a handful of studies focusing on a particular species in a very specific region (e.g., impact of tsunamis on the critically endangered Javan rhinos in Indonesia, or the Juan Fernández Firecrowns hummingbirds in Chile, or impact of volcanic eruptions on the short-tailed albatross mostly breeding on Torishima Island active volcano, Japan) have been carried out without really proposing a globally applicable methodology. Numerous conservation projects are being implemented around the world to protect species, particularly in the context of the current collapse of global biodiversity. Unfortunately, protection areas are very often recognized as being unfavourable for human settlements, often precisely because of natural hazards, thus leaving little or no possibility for the species occupying them to recover after an event. With the example of the tsunami hazard and coastal species of New Zealand, we propose an action plan to integrate the consideration of natural hazards into conservation efforts and provide keys to conservation decision makers.
BG15-A004
Investigating the Growth Inhibition of Aspergillus Oryzae to Study Antifungal Activity in Environmental Isolates of Serratia spp.
Charlene NG+, Kung Ming LEUNG, Grace LAI, Simon GRIFFIN#
The ISF Academy, Hong Kong SAR
The steady rise in infections by fungal pathogens resistant to all current classes of antimicrobial drugs has highlighted an urgent need for new antifungal agents [1]. But just as fungal secondary metabolites provide many classes of antibacterial compounds, certain bacteria may offer a useful resource for novel antifungal agents. This project investigates antifungal activity in environmental strains of Serratia spp. isolated in Hong Kong. And, given that invasive aspergillosis is the most common fungal infection in Asia [2], we have used growth inhibition of Aspergillus oryzae (a non-clinical species) as part of a low-risk assay. DNA from 11 strains of Serratia, isolated from samples of soil and sediment, were sequenced using Illumina NovaSeq and Oxford Nanopore MinION platforms and their complete genomes generated by hybrid assembly where possible. Alongside this, a preliminary plate competition assay against A. oryzae, produced a range of growth inhibition, with S. marcescens 2AT2 and S. ureilytica E1 showing the strongest activity. Genomic analysis via BV-BRC suggests a number of candidates for antifungal activity of 2AT2 and E1, including multiple copies of chitinase (EC 3.2.1.14) and chitin binding proteins, a type VI secretion system (T6SS) and numerous genes for polyketide synthesis. Ongoing investigations to identify the genes responsible for this activity now focus on identifying elicitors of the antifungal response, together with RNA sequencing.
BG15-A008
Exploring Antimicrobial Resistance in Companion Avians in Homes and Pet Shops in Hong Kong
Sian BENNETT+, Kung Ming LEUNG, Grace LAI, Simon GRIFFIN#
The ISF Academy, Hong Kong SAR
Hong Kong is the biggest trading centre for CITES-listed species in the world. Between 2015 and 2019, over 4 million exotic animals from over 700 species were imported into – and mostly exported from – the territory (HKWTWG, 2022). While legal and illegal trafficking is clearly decimating for the animal species themselves, it also raises the risk of zoonotic infection from the viruses, microbes and parasites they undoubtedly carry. This study characterises antimicrobial-resistant bacteria present in faeces of companion avians in Hong Kong. Antimicrobial resistance (AMR) is identified as a major threat to public health and Hong Kong’s pet trade creates optimal conditions for transmission and dissemination. And since animals housed in pet shops might be expected to have more opportunity to exchange microbes than those in homes, we compare bacteria from both populations to test this hypothesis and to shed light on the carriage of AMR genes. Broad levels of resistance in faecal samples to ampicillin, augmentin, tetracycline and kanamycin were compared by colony counts on antibiotic-containing agar. Selected bacterial isolates showing multiple resistance patterns were streaked to purity before DNA extraction and sequencing via Illumina Novaseq and Oxford Nanopore MinION platforms. Draft and complete genomes were assembled using Unicycler v0.5.0, annotated by BV-BRC, and AMR genes were identified using CARD RGI v6.0.3. In early results, two Staphylococcus gallinarum isolates from faeces of Psittacus melanocephalus contained a chromosomally encoded extended-spectrum beta-lactamase giving resistance to cephalosporins and reduced susceptibility to ertapenem. A multi-drug resistance plasmid in SB4L showed homology with clinical strains of S. aureus identified in Taiwan and Shanxi and the AAC(6')-Ie-APH(2")-Ia gene it carries detected in multiple locations worldwide. Using the NCBI database, BLAST, MLST and geographical mapping elucidates relationships between isolates and genes, as well as likely routes of transmission.
BG15-A011
Crop Water Stress Monitoring Using Physiological Vegetation Index MTCI and CCI
Kyeong-Min KIM1#+, Hyun-Dong MOON1, Euni JO1, Bo-Kyeong KIM1, Subin CHOI1, Jae-Hyun RYU2, Hoyong AHN2, Jaeil CHO1
1Chonnam National University, Korea, South, 2Rural Development Administration, Korea, South
Crop stress monitoring could be applied to control agricultural environment, promoting efficient resource use, especially water. Destructive methods for detection of plant water status are reliable but not repeatable. Remote sensing method can indicate the physiological and growth states without destroying the plants. Pigments like chlorophyll and carotenoid absorb and reflect specific wavelength lights. Changes in pigment content result in altered reflection characteristics. In this study, a remote sensing technique using vegetation indices (i.e. MTCI and CCI) based on spectral reflectance was applied to crop water stress monitoring. MERIS terrestrial chlorophyll index (MTCI) decreases when chlorophyll content decline. Chlorophyll/carotenoid index (CCI) positively correlated with photosynthesis rate is proportional to ratio between chlorophylls and carotenoids. Soybeans were sown in pots at a greenhouse in Gwangju, Republic of Korea, and irrigation was controlled to induce water stress. The MTCI and CCI were calculated using reflectance on leaves observed with a portable spectrometer. The MTCI sensitively decreased on the non-irrigation conditions and such decline became larger with heat waves. The CCI showed less sensitivity to water deficit but had decreased significantly with heat waves. After re-irrigation, the MTCI increased more than before damage and CCI became more sensitive to heat stress. Analyzing MTCI and CCI together would be useful for crop monitoring to determine the conditions in which crops are exposed to drought and heat waves.
BG15-A013
Observation of Methane Emission Under Different Dissolved Oxygen Conditions in Rice Paddy in Naju, South Korea
Bo-Kyeong KIM1#+, Jong-Sung HA2, Seungtaek JEONG2, Jong-Min YEOM3, Hyunki KIM4,1, Hyun-Dong MOON1, Euni JO1, Jaeil CHO1
1Chonnam National University, Korea, South, 2Korea Aerospace Research Institute, Korea, South, 3Jeonbuk National University, Korea, South, 4National Institute of Crop Science, Korea, South
Methane (CH4) is a greenhouse gas that contributes 28 times than carbon dioxide (CO2). However, approximately a quarter of CH4 emissions of South Korea come from rice paddy. The flooded conditions in rice paddy significantly governs the water and carbon exchange. Further, the paddy water affects soil temperature and anaerobic conditions, closely tied to CH4 emission. We hypothesized that dissolved oxygen in paddy water would mitigate CH4 emissions by supplying oxygen to paddy soil. In this study, CO2 and CH4 fluxes were observed by using eddy covariance method in a rice paddy transplanted in June and harvested in October at the Agricultural Research and Extension Services in Naju, Jeollanam-do, South Korea (35º 01’ 36.93’’ N, 126º 49’ 18.92’’ E) to investigate the properties of CH4 emission under different dissolved oxygen conditions, considering soil temperature and vegetation growth. During the rice growing season, the CO2 flux decreased by photosynthesis of rice canopy, while the CH4 emissions increased with the development of rice tiller number because the aerenchyma in the stem provides the primary pathway for releasing CH4 gas from the soil to the atmosphere. In addition, the CH4 emission showed insensitivity to the dissolved oxygen of paddy water under its low conditions. However, the decrease in CH4 emissions was significant under high dissolved oxygen conditions. The relationship between methane emissions from rice paddy and dissolved oxygen in paddy water needs to be studied in conjunction with more diverse growing conditions.
BG16-A004
Greenhouse Gases Responses Between Different Flooding Conditions in the Fields
Siang-Heng WANG#+, Charles CHOU
Academia Sinica, Taiwan
The sink or source of greenhouse gases (GHG) is a critical issue for agricultural management since global GHG emissions and temperature have gradually increased in recent years. Because of fertilization, flooding, and cultivar selection by farmers, the biochemical reactions in the soil and plants are quite different. A laboratory study in the growth chamber and a field study in central Taiwan, a critical rice planting area, will be compared in this presentation. A chamber system will be set in a temperature–consistent plant growth chamber to quantify the gases released or absorbed from the different flowerpots with distinct rice cultivars. An eddy–covariance system will be set in the rice paddy field to measure the fluxes contributed by specific rice cultivars. This study compares the fluxes' responses between different cultivars and the fluxes' consistency between the growth chamber and the field to summarize the measurement methods well to establish more rice cultivation studies in the future.
BG16-A006
| Invited
Application of Machine Learning on Long-term Observations of Net Ecosystem Carbon Dioxide Exchange in Tropical Peatlands
Yazid IMRAN1#+, Yusri YUSUP2, Guan Xhuan WONG1, Lulie MELLING1,3
1Sarawak Tropical Peat Research Institute, Malaysia, 2Universiti Sains Malaysia, Malaysia, 3UN Sustainable Development Sustainable Solution (UN-SDSN Asia), Malaysia
Tropical peatlands are an important global carbon reservoir, storing about one-sixth of the world's peatlands' carbon pool. For this reason estimating and quantifying potential carbon dioxide (CO2) emissions from tropical peatlands are essential to address future climate change. The use of quantitative approaches such as machine learning (ML) techniques to model, predict and gap-fill carbon fluxes has been given much recent attention due to their ability to handle the apparent nonlinearity in ecosystem processes. To date, however, application of these algorithms on carbon fluxes from tropical peatlands have remained underexplored. This study aims to evaluate the ability of prevalent ML methods to model and predict CO2 net ecosystem exchange (NEE) measured using the eddy covariance technique in an undrained peat swamp forest in Sarawak, Malaysia using data collected over the period of a decade. The data were divided into daytime and nighttime data based on their photosynthetic photon flux density values. We evaluated ML algorithms that are widely-used in studies related to carbon fluxes, such as random forests and artificial neural networks. Current results show that these models performed rather poorly on tropical peatland NEE data, with all models observed to struggle to predict high and low NEE values leading to low R2 values (< 0.25) in spite of low errors. These models also showed particularly poor performance on nighttime data, and does not show improvement even after application of typical model-tuning methods such as regularization. The research will further discuss on possible paths to improve the prediction of NEE using ML methods such as better data processing and feature engineering, and using deep learning methods adapted for time series data such as the Long Short-Term Memory (LSTM) model.
BG16-A007
| Invited
Assessing the Impact of Land Use Change on Carbon Dioxide Exchange in Tropical Peatland Ecosystems
Frankie KIEW1#+, Takashi HIRANO2, Ryuichi HIRATA3, Guan Xhuan WONG1, Joseph WAILI1, Fellix SELI1, Lulie MELLING1,4
1Sarawak Tropical Peat Research Institute, Malaysia, 2Hokkaido University, Japan, 3National Institute for Environmental Studies, Japan, 4UN Sustainable Development Sustainable Solution (UN-SDSN Asia), Malaysia
Land use change has profound implications for ecosystems, particularly in tropical peatlands, where the intricate balance of the carbon dioxide (CO2) cycle can be significantly affected. Tropical peatlands play a crucial role in the global carbon cycle, serving as substantial carbon sinks. However, human activities, such as agricultural expansion, logging, and drainage for various land uses, have led to substantial land use changes in these ecosystems. These alterations have far-reaching effects on the peatland's CO2 balance, influencing both CO2 emissions and sequestration. This study explores the intricate relationship between land use change and the carbon dioxide balance in tropical peatland ecosystems, shedding light on the consequences for both local and global carbon dynamics. We began an Eddy Covariance (EC) measurement in 2011 to quantify the CO2 flux above a tropical peat swamp forest (PSF) in Sarawak, Malaysia. In 2017, the PSF was converted into an oil palm plantation (OPP), presenting us with an opportunity to evaluate the impact of peatland conversion on CO2 flux. The forest was a moderate CO2 sink (Net ecosystem exchange; NEE of -25 ± 179 g C m-2 yr-1) from 2011 to 2015. After the conversion (2017 to 2019), the ecosystem became a net CO2 source, with NEE of 2732 ± 655 g C m-2 yr-1. Despite a significant reduction in annual gross primary productivity (GPP; 3663 ± 189 vs. 721 ± 600 g C m-2 yr-1) following conversion, the annual ecosystem respiration (RE) is comparable between the two land uses (3638 ± 255 vs. 3454 ± 323 g C m-2 yr-1). Our analysis revealed a strong positive linear correlation between the annual NEE and groundwater level (GWL; R2 = 0.99, p < 0.05).
BG16-A009
Water-efficient Practices Reduce Methane Emissions from Paddy Rice: An Eddy Covariance Study in Taiwan
Yu-Ting SHIH#+, Charles CHOU, Yi-Ying CHEN
Academia Sinica, Taiwan
Paddy rice, a key food and economic crop in East Asia, has been under scrutiny due to methane (CH4) emissions during flooding, a concern highlighted at COP28. To address this, water-efficient methods like spike-watering are being promoted. This study, conducted from February to June 2023 in Taichung City, Taiwan, examined CO2 and CH4 emissions, filled missing data, and calculated the carbon budget using the eddy covariance method. The findings revealed that CH4 flux is more heat-dependent during flooding but remains relatively stable with wind variations. Wind, however, is a significant factor during spike irrigation. The carbon budget showed a CO2 sink of -17,634 kg-CO2 per hectare, comparable to the carbon sequestered after rice harvest (16.5 tons CO2 equivalent). The net CO2 sinks were -6,573 kg-CO2 per hectare, with a CH4 emission of 21.4 kg-CH4 per hectare (equivalent to 1,647.8 kg-CO2). Given these results, CH4 emissions cannot be overlooked when considering the carbon sink and its components. The study found that CH4 emissions peak (0.04 μmol/m2/s) during flooding and field drying, both of which are water management-related. However, in water-efficient operations, CH4 levels are low according to some paddy rice reports. Therefore, water-efficient practices not only conserve water but also reduce CH4 emissions.
BG17-A003
Coastal Ecological Time Series- Integrating Ecological Snapshots to Understand Coastal Carbon Cycling
Punyasloke BHADURY#+
Indian Institute of Science Education and Research Kolkata, India
The coastal Bay of Bengal is home to variety of biotopes with rich biodiversity, influences regional climatic patterns and supports the livelihood of millions of communities. There lacks dedicated ecosystem level monitoring and time series data that can aid towards understanding the effects of changing climate on marine bioresources of coastal ocean. In Sundarbans mangrove, using a series of combinatorial approaches including through the establishment of more than a decade old ecological time series- Sundarbans Biological Observatory Times (SBOTS) as well as seasonal time series- Sundarbans Seasonal Time Series (SuSTS), investigations are being undertaken to understand biocomplexity of microbiome and their role in coastal carbon dynamics. The temporal and spatial significance of members of Firmicutes and Bacteroides, in coastal water of Sundarbans in link with forms of carbon indicate their potential ecological significance. Using robust microcosm and mesocosm based experiments, the breakdown of complex forms of organic matter originating from mangrove litterfall by members of Firmicutes and Bacteroides have been intrinsically shown in Sundarbans. The ongoing studies show that unique microbial communities in the waterscapes of Sundarbans have adapted to prevailing environmental gradients and are key players in processes such as coastal carbon cycling.
Session Chair(s): Seunghee HAN, Gwangju Institute of Science and Technology
BG07-A006
Quantifying the Remineralization Rates of Sediment Organic Carbon of Jakarta Bay
Camellia TITO1,2#+, Dietriech Geoffrey BENGEN1, Tri PRARTONO1, Ario DAMAR1, Aan Johan WAHYUDI2
1IPB University, 2National Research and Innovation Agency
The remineralization process of organic carbon (OC) from nutrient riverine input (allochthonous) and photosynthesis (autochthonous) has significant implications for the chemical composition of seawater and the carbonate system within the coastal ecosystem. Therefore, it is important to study the remineralization rate of OC in coastal embayment. Jakarta Bay is an estuary that receives a considerable amount of organic materials from 13 river estuaries in the metropolitan area of Indonesia. Despite the existing knowledge of the environmental dynamics and ecological conditions, the rate of OC remineralization in this tropical coastal region remains poorly understood. This research aims to understand the degradability of OC and the potential impacts of its remineralization on coastal ecosystems. We analyze the remineralization rate of OC through closed-system incubation experiments by measuring surface sediment dissolved oxygen (DO) consumption rates. Finally, we discuss DO consumption rates as a proxy to estimate OC remineralization rates in Jakarta Bay. These observations highlight the rate of OC remineralization in estuaries that are highly susceptible to being affected by both human activities in the watershed (nutrient loading) and climate change.
BG07-A003
Impact Assessment of Nutrient Load Derived from Seepage Water Using Machine Learning
Takuma OIKAWA+, Katsuaki KOMAI#, Kanta ITO
Kitami Institute of Technology
Machine learning was used to assess the inflow of nutrient load to clarify the causes of suspended microalgae bloom, called blue-green algae, in an artificial lake. Field observations were carried out at Notsukeushi Park Pond in Kitami City, located in northern Japan, and phosphorus and nitrogen increase rates and hydrological parameters were measured approximately a hundred times. Since there is no source of surface water inflow to the study site, these data were utilized to construct a machine learning model based on a conceptual model that considers the inflow load due to seepage dynamics. Gaussian process regression, neural network, random forest, and k-nearest neighbor method were employed to estimate unknown parameters in seepage nutrient load compared to a simple linear regression model. Principal component analysis confirmed that the observed data contains a variety of conditions. It was confirmed that the significant reproducibility of phosphorus and nitrogen concentrations for the rainfall events improved by increasing the number of learning cycles. In contrast, the estimation accuracy over two hundred days was insufficient, suggesting that it is necessary to consider the influence of primary ecosystems.
BG07-A004
Microplastics Pollution in the Marine Ecosystem Australia
Pavitra C. MIRJANKAR1#+, Vikas Kumar MEENA2, Aaron SCHULTZ3, Tanveer ADYEL3, Asif QURESHI2
1Indian Institute of Technology Hyderabad And Deakin University, 2Indian Institute of Technology Hyderabad, 3Deakin University
Microplastics (MPs) are ubiquitous, persistent pollutants reported in abundance, and their pollution is an emerging threat to all terrestrial and aquatic ecosystems. They are widespread in all environments and can be found in Antarctica, deep-sea sediments, human blood, and breast milk. Hence, it is important to understand the physicochemical properties, as well as toxicological concerns, bioavailability, and environmental impact of the MPs. Environmental, social, and economic concerns regarding the impacts of microplastic pollution, with the limited understanding of the factors that affect their bioavailability, have attracted enormous interest in research. Recent studies indicate higher levels of microplastics in the marine aquatic ecosystem near industrial settlements and/or urban centres, with aquatic organisms in these areas showing substantial accumulation of microplastics in their bodies. Furthermore, various contaminants like heavy metals and other chemicals have been observed to readily adsorb on MPs, serving as carriers for various pollutants within the bodies of marine aquatic species. The present study aims to provide a comprehensive overview of MPs contamination in water around the coastal regions of Australia and their physical and chemical characteristics, shape, size, and their detrimental impacts on the ecosystem and marine biodiversity. We summarise the current study by identifying knowledge gaps and highlighting key research priorities in MPs, which is crucial for enhancing our understanding and addressing their environmental risks. Keywords: Microplastics (MPs), Marine Ecosystems, Interactions, Toxicity.
BG07-A007
Influence of Beaufort Gyre on the Spatiotemporal Variation of Total and Methylated Mercury in the Western Arctic Ocean
Sangwoo EOM1+, Hakwon JEONG1, Jihee KIM2, Tae Siek RHEE3, Jong Kuk HONG3, Seunghee HAN1#
1Gwangju Institute of Science and Technology, 2Korea Institute of Science and Technology, 3Korea Polar Research Institute
High mercury bioaccumulation in the Arctic Ocean is being observed despite the distance from anthropogenic sources. To understand basin-wide distributions of total mercury (THg) and methylmercury (MeHg) in seawater, we analyzed the vertical profiles of Hg and salinity obtained through three Arctic expeditions using the R/V icebreaker ARAON and GEOTRACES and performed comparisons between Arctic basin. When THg concentrations in surface (0 to 200 m) seawater were compared between the Canada Basin, Makarov Basin, Amundsen Basin, North Pole, and Nansen Basin, the highest THg concentration was observed in the Canada Basin, where Hg inputs from atmospheric deposition, coastal erosion, river runoff, and the Atlantic and Pacific Oceans are retained in the upper 200 m layer of the Beaufort Gyre. In contrast, the order of MeHg concentration in the upper 200 m layer was related to the degree of photodecomposition controlled by the sea ice extent, resulting in a decrease in the order of the North Pole > Nansen Basin > Amundsen Basin > Makarov Basin > Canada Basin. On the other hand, MeHg concentrations in the subsurface layer (50-100 m water depth) were highest in the Canada Basin, which can be explained by the highest in situ methylation and the lowest diffusion flux to the upper seawater layers, due to the strong stratification of seawater following the large supply of freshwater from the Pacific Ocean and Mackenzie River. Overall results suggest that future changes in the horizontal and vertical size of the Beaufort Gyre, sea ice extent, and freshwater discharge rate induced by climate change may affect the distribution of THg and MeHg in seawater, and may subsequently alter the impact of Hg on Arctic Ocean ecosystems.
BG07-A009
Characteristics of Sediment Mercury Methylation in the Beaufort Sea, Arctic Ocean
Hakwon JEONG1+, Jihee KIM2, Sangwoo EOM1, Seunghee HAN1#
1Gwangju Institute of Science and Technology, 2Korea Institute of Science and Technology
As river discharge, coastal erosion, and permafrost thawing caused by climate change are increased, the concentration and speciation of mercury (Hg) in sediment can be changed in the Arctic Ocean. In particular, the Beaufort Sea has strong Mackenzie River plume, and extensive area of submarine permafrost and mud volcanoes, which can provide diverse microbial communities contributable to Hg(II) methylation. This study analyzed total Hg (THg) and methylmercury (MeHg) concentrations in the surface (0-5cm) and subsurface (5-60cm) sediments, along with chemical and biological properties, in thirteen sites on the west and east transects in the Beaufort Sea. THg in surface sediment on the west line was higher in the slope (0.57nmol/g) than on the coastal shelf (0.41nmol/g), due to the hydrodynamic sorting of lithogenic particles. Conversely, MeHg was significantly higher in the inner shelf (0.18pmol/g) close to the Mackenzie delta, compared to the slope (0.003pmol/g). The east line showed irregular THg and MeHg trends, with slightly higher THg on the mid-shelf (0.45±0.04nmol/g) than the slope (0.37nmol/g) and inner shelf (0.36nmol/g). Elevated MeHg was also observed in the mid-shelf, which has a consensus with potential for in-situ Hg(II) methylation due to the presence of sulfuric carbon and Hg(II) methylating microbes. Regarding vertical distribution, THg in the west line showed no significant depth difference, while MeHg peaked at 50-60cm on the slope and 10-20cm on the shelf. Mud volcanoes maintained constant THg profiles but showed clear MeHg peaks in the surface layer. This contrasts with the vertical profiles observed in non-mud volcano sites where MeHg decreased until 10-20cm and then increased with depth, due to sulfate reduction coupled with anaerobic methane oxidation. Conclusively, cross-shelf transport of terrigenous organic matter and the presence of microbes influenced Hg distribution and speciation in the Beaufort Sea.
Session Chair(s): Bhoopesh MISHRA, Illinois Institute of Technology
BG13-A006
Comparison of Sb-bearing Minerals and Biogeochemical Features at Three Sites Subject to Antimony Contamination
Yidan ZHANG1#+, Maxim BOYANOV2, Edward O'LOUGHLIN2, Kenneth KEMNER2, Man Jae KWON1
1Korea University, 2Argonne National Laboratory
Antimony (Sb) is a toxic metalloid used in several anthropogenic activities. The presence of Sb in the environment, when at concentrations above guidelines, is considered as an environmental hazard due to its acute toxicity. Antimony can be released into natural environments as a biproduct or waste of industrial processes such as ore mining and metal refinery. Meanwhile, abandoned shooting ranges are also considered as contaminated legacy sites of Sb, because this metalloid is widely used in bullet as hardening agent. Upon releasing to the environments, the original form of Sb can then be subjected to multiple processes including weathering, oxidation, or reduction which alter its speciation. Among the two common oxidation states of Sb, Sb(III) is considered to be more toxic than Sb(V); however, in anoxic environment Sb(V) shows higher mobility. Therefore, exactly which Sb species is present in the environment essentially determines the impact this toxic metalloid exerts on the surrounding environments. Hence, for the better understanding of Sb as a contaminant it is necessary to conduct field survey at Sb-contaminated sites and to investigate the presence of Sb as well as its connection to surrounding biogeochemical features. In this field study, we visited three Sb-contaminated sites including a former shooting range, a Sb refinery, and a Sb mining site to collect biogeochemical samples and Sb-bearing minerals. We performed a series of geochemical and microbiological analysis to interpret the features of three sites. We also used XAFS to investigate the species of Sb-bearing minerals. This study provides detailed information in terms of how Sb contamination affects surrounding environments at Sb-contaminated sites.
BG13-A008
Effects of Phosphate on the Behavior of Sb(V) Associated with Ferrihydrite During Microbial Fe(III) and Sulfate Reduction
Yun Seo JANG1#+, Yidan ZHANG1, Maxim BOYANOV2, Edward O'LOUGHLIN2, Kenneth KEMNER2, Man Jae KWON1
1Korea University, 2Argonne National Laboratory
Antimony (Sb) is a toxic metalloid which commonly exist as Sb(III) and Sb(V), in which Sb(III) is more toxic. Sb(V) can adsorb onto host phase such as Fe(III) minerals and become immobilized. However, Sb(V) may be released anaerobic condition during Fe(III) reductive dissolution, and become mobilized. Upon releasing, aqueous Sb(V) can be reduced to Sb(III) by microorganisms in the presence of proper electron donors. Meanwhile, sulfate is another common substrate in subsurface environments, and the sulfide produced from microbial sulfate reduction can lead to abiotic Fe(III) reduction, as well as abiotic Sb(V) reduction. After Sb(V) reduction, the presence of Sb(III) in soils and water is considered as environmental hazard. The adsorption of Sb(V) onto Fe(III) minerals can be also affected by the presence of oxyanions such as phosphate, due to the competition of sorption sites on the Fe(III) mineral with. Therefore, the fate of Sb(V) when adsorbed on Fe(III) mineral is controlled by intricate factors including microbes, phosphate, and the redox cycle of Fe(III) and sulfate. This study uses anaerobic microcosms to investigate the change in mobility and speciation of Sb(V) when adsorb on ferrihydrite (Fe(III) oxide) in the presence of microbes, under sulfidogenic environment, and with different loadings of phosphate. The objectives here are understand if Sb(V) can be released from Fe(III) due to competition and phosphate, and upon releasing what speciation process would occur to Sb(V).
BG13-A012
Effect of Temperature and Irradiation on the Microbial Reactions by Bentonite Indigenous Microbes Under Fe(III) and Sulfate Reducing Conditions
Kanghyun PARK#+, Man Jae KWON
Korea University
Bentonite is a promising buffer material for deep geological repositories (DGRs) of spent nuclear fuel (SNF). However, bentonite can be a potential microbial source which can stimulate microbial interactions with surrounding materials and further affect the stability of the repository. Considering in long-term, bentonite and the indigenous microbes within the repository system can be exposed to both heat and irradiation resulting from the decay of radionuclides. Our previous study investigated activities of indigenous microbes in bentonite at 18 and 50 °C under Fe(III) and sulfate reducing conditions. Based upon this groundwork, we conducted two batch experiments with indigenous microbes in bentonite to 1) evaluate the temperature effect under more detailed conditions, and 2) assess the microbial activity and viability under irradiation. Microcosms were created with WRK bentonite and artificial groundwater amended with lactate as an electron donor, and Fe(III) (in ferrihydrite) and sulfate as electron acceptors. To determine the temperature effect, microcosms were incubated under six different temperature conditions ranging from 18 to 70 °C. To investigate irradiation effect, microcosms were irradiated with gamma-radiation at varying dose rates of 2 to 200 Gy/h for 11 days. Under different temperature conditions, microbial lactate utilization exhibited a transition near 40 °C, At lower temperatures, lactate was metabolized to acetate and propionate with higher Fe(III) reduction, whereas at higher temperatures, it transformed solely into acetate, followed by rapid sulfate reduction. In the irradiation experiment, abiotic changes of lactate decomposition and Fe reduction were observed during the irradiation period. After irradiation, microbial activity was observed up to a medium dose rate (10 Gy/h), albeit at slower rate, however there was no indication of microbial viability for higher dose rates. Microbial communities in both experiments will be analyzed using 16S rRNA gene sequencing and further will be correlated with the geochemical data.
BG13-A001
Histology, Enzymatic Activity, and Gene Expression Profiling of Hydrothermal Vent Crab Xenograpsus Testudinatus Exposed to Polyethylene Microplastic
Mark June CONSIGNA+, Li-Chun TSENG, Ching-Wen HUANG, Yi-Ta SHAO, Jiang-Shiou HWANG#
National Taiwan Ocean University
Hydrothermal vent (HV) crabs thrive in sulfur-rich shallow hydrothermal vents. This study investigates the effects of polyethylene microplastic (MPs) on the HV crab organs through histopathological examination, enzymatic activities, and gene expression. Previous research has not explored the ecotoxicological impact of MPs on HV crabs. Fluorescent green polyethylene microspheres (FGPE) were administered via feeding and immersion (0, 0.3, 0.6, and 1%) to the male (n=168), Xenograpsus testudinatus. Histopathology of organs (gills, hepatopancreas, midgut, and muscles), oxidative stress biomarkers (SOD, GPx, MDA, and CAT), and stress response genes (SOD, GPx, HSP, and CAT) were analyzed after a 7-day experiment. FTIR confirmed MPs in the HV crabs' fecal matter, indicating ingestion capability. Results revealed severe damage and atrophy in the hepatopancreas and gills of HV crabs at 1% FGPE in feeding and immersion. Moreso, the oxidative stress biomarkers (SOD, MDA, GPX, and CAT) significantly increased (p<0.05) at 1% of FGPE. Additionally, 1% FGPE significantly (p<0.05) affected the expression of SOD, GPx, HSP, and CAT genes. Ingesting MPs induced physiological changes in HV crabs, with hepatopancreas, serving as energy and toxin storage, exhibiting extreme alterations in histology, enzymatic activities, and stress response genes. This study provides insights into oxidative defense and gene expressions in response to MPs ingestion by a unique species inhabiting shallow hydrothermal vents.
BG13-A011
Evaluation of Heavy Metal Contents in Water, Sediments and Commonly Consumed Fish Species from the Lower Agno Watershed, Philippines
Manilyn CASA1#+, Loucel CUI1, Decibel FAUSTINO-ESLAVA1, Jenielyn PADRONES1, Juan Miguel GUOTANA1, Kennethjer ALEJO1, Kim Bryan CABRERA1, Ma Ericha AMANTE1, Francis GONZALVO1, Rosemarie Laila AREGLADO1, Maria Regina REGALADO1, Patrick BYRNE2, Emma BILES2, Richard WILLIAMS3
1University of the Philippines Los Baños, 2Liverpool John Moores University, 3University of Glasgow
The health of aquatic ecosystems affected by various stressors including industrial, urban and agricultural activities can be monitored and evaluated using fish assemblages as bioindicators. Environmental fluctuations can significantly impact heavy metals (HM) bioconversion from sediments and water which may cause harm to aquatic organisms and affect its biodiversity. One of the pollutants affecting freshwater ecosystems are HM that accumulate in fish which may pose risks to them and to higher trophic levels. Heavy metal concentrations in water, sediments and fish tissues of Oreochromis niloticus and Glossogobius sp. were assessed to determine water and ecological quality of the Agno River Basin (ARB). Fish, water and sediment samples were collected from representative sites within the Agno River including: (1) San Roque Dam in San Manuel, Pangasinan; (2) Viray River in Natividad, Pangasinan; (3) Tarlac River in Paniqui, Tarlac, and (4) Agno River in Brgy. Bocboc, San Carlos City, Pangasinan. Inductively Coupled Plasma – Optical Emission Spectrometry (ICP-OES) was used to analyze the HM concentrations present in the samples. The relative abundance of HM concentrations detected in fish tissues was found to be: Fe>Mn>Zn>Cu>Cr>Ni>Co>Cd while the average HM concentration in water and sediment samples was: Mn>Zn and Fe>Mn>Cd>Cr>Co>Zn>Cu>Ni>Pb>As. Results showed that, relative to WHO and USEPA SQC 2022 standard for sediments, Pb, Ni, Co, Cd, Zn, Cu, Cr, Fe and Mn exceeded the acceptable limits while most of the HM in water are below detection limit (DENR WQG, DAO 2016-08) and Ni, Co, Cr, Fe, Mn, and Cd in Oreochromis niloticus flesh and internal organs are significantly elevated (FAO/WHO 1989). The elevated concentrations of Cr, Cu, Zn, Ni, Mn and Fe in the sediments of Viray River is very likely geogenic in nature. Positive anomalies in samples from other sites will need to be further examined to determine contributors.
Session Chair(s): Si-Liang LI, Tianjin University
BG12-A009
| Invited
Substantial Contribution of Nocturnal Oxic Methane Production in Eutrophic Freshwaters
Zhe LI#+
Chongqing Institute of Green and Intelligent Technology, Chinese Academy of Sciences
Diel dynamics shape the large uncertainties in global freshwater methane emissions. During cyanobacterial blooms, we uncovered significant nocturnal methane emissions, about 73% of the daily total, in the eutrophic oxic surface layer. We explicitly showed that oxic methane production (OMP) on the water surface during the stratification period, which differs from the traditional pathway, is the primary source of CH4 emissions. Metagenomic and mass budget evidence supported the inference that OMP was mainly driven by methylphosphonates (MPn) degradation and related intensively to cyanobacteria-bacterial interactions in phosphorus-limited environments. Thermal stratification below the oxycline also performed as the stable “barrier” for the upwelling of inorganic P from the bottom to the surface layer, causing the intensification of P insufficiency. Surface methane oxidation might be inhibited due to the oversaturated oxygen caused by diurnal photosynthesis. We addressed that the nocturnal contribution of methane would substantially increase the global estimates of freshwater methane emissions.
BG12-A008
| Invited
Unraveling the Molecular Dynamics and Factors Influencing Recalcitrance of Dissolved Organic Matter: Insights from Laboratory Incubation and High-resolution Mass Spectrometry
Penghui LI1+, Chen HE2, Quan SHI2, Ding HE3#
1Sun Yat-sen University, 2China University of Petroleum, 3The Hong Kong University of Science and Technology
Dissolved organic matter (DOM) is crucial in aquatic ecosystems and global carbon cycling. DOM in the ocean is one of the largest carbon reservoirs on earth, and its recalcitrance, attributed to old radiocarbon age, remains unclear. To address this question, we utilize high resolution mass spectrometry (HRMS) to investigate the molecular dynamics of DOM from different sources during one-year bio-incubation. Our analysis, using Fourier transform ion cyclotron resonance mass spectrometry (FT-ICR MS), identified three types of formulas (Labile, Resistant and Product) based on their absence and presence in the initial and end samples. Our findings revealed different distributions of molecular properties (H/C, aromaticity, nominal oxidation state of carbon, etc.) for these those formulas, indicating that molecular properties could affect their lability and thus biogeochemical cycling. Additionally, we observed that the Product formulas in the short-time incubation could be degraded and regarded as Labile formulas in longer incubation, suggesting the significance of incubation time. By analyzing the dynamics of the relative abundance of identified formulas, we further developed the Change Ratio (CR) for identifying formulas with significantly increased or decreased intensity. Molecular properties of these Increase or Decrease formulas exhibited significant differences, further emphasizing their influence on lability. Interestingly, the relative intensities of Decrease formulas were found to be much lower than those of Increase formulas, contradicting with the dilution hypothesis and highlighting the dominance of molecular properties over concentration in determining DOM lability. Furthermore, the aromaticity distribution of these Increase and Decrease formulas mirrored that of surface-enriched and deep-enriched formulas in the open ocean, validating our laboratory incubation results against field investigations. Overall, our study demonstrates that the combination of laboratory incubation and HRMS facilitates a molecular-level understanding of DOM recalcitrance and thus global carbon cycling.
BG12-A002
Dynamics of Dissolved Organic Matter Composition and Characteristics During Extreme Flood Events in the Yangtze River Estuary
Zhao Liang CHEN1+, Haibo ZHANG2, Yuanbi YI3, Yuhe HE4, Penghui LI5, Yuntao WANG6, Kai WANG7, Zhenwei YAN3, Chen HE8, Quan SHI8, Ding HE3#
1The Chinese University of Hong Kong, 2National Marine Environment Monitoring Center, 3The Hong Kong University of Science and Technology, 4City University of Hong Kong, 5Sun Yat-sen University, 6Second Institute of Oceanography, Ministry of Natural Resources, 7Southern University of Science and Technology, 8China University of Petroleum
Understanding the molecular composition and fate of dissolved organic matter (DOM) during transport in estuaries is essential for gaining a comprehensive understanding of its role within the global biogeochemical cycle. In 2020, a catastrophic flood occurred in the Yangtze River basin. It is currently unknown whether differences in hydrologic conditions due to extreme flooding will significantly impact the estuarine to oceanic DOM cycle. We determined the DOM composition in the Yangtze River estuary (YRE) to the East China Sea by using Fourier transform ion cyclotron resonance mass spectrometry (FT-ICR MS) during the high discharge and the flood period (monthly average discharge was 1.2 times higher) on the same trajectory. Our study found that the composition of DOM is more diverse, and more DOM molecules were introduced to the YRE during the flood, especially in the freshwater end member. The result revealed that the DOM was significantly labile and unstable during the flood period. A total of 1840 unique molecular formulas were identified during the flood period, most of which were CHON, CHONS, and CHOS compounds, most likely resulting from anthropogenic inputs from upstream. Only 194 of these molecules were detected in the seawater end member after transporting to the sea, suggesting that the YRE served as a 'filter' of DOM. However, the flood enhances the transport of a group of terrigenous DOM, that is resistant to photodegradation and biodegradation. As a result, YRE experienced ~1.6 times higher terrigenous DOC flux than high discharge period. Considering the increased frequency of future floods, our study provides a preliminary basis for further research on how floods affect the composition and characteristics of estuarine DOM. With the help of the FT-ICR MS technique, we can now better understand the dynamic of DOM composition and characteristics in large river estuaries.
BG12-A006
Influences of Hydrodynamics and Lithological Backgrounds on Dissolved Inorganic Carbon in Subtropical Reservoirs
Wanfa WANG1, Wenhong SHI1#+, Jun ZHONG2, Yuanbi YI3, Si-Liang LI2
1Guizhou University, 2Tianjin University, 3The Hong Kong University of Science and Technology
Carbon migration, transformation, and emissions as CO2 in reservoir and lake systems have been extensively studied. However, uncertainties persist regarding carbon cycling variations in both hydrodynamics and lithological backgrounds within large thermal stratified river-reservoir systems. To bridge this knowledge gap, we combined measurements of water chemistry, isotopic compositions (d13C), partial pressure of CO2 (pCO2), and CO2 fluxes (FCO2) to elucidate the differences, control mechanisms, and environmental effects of various carbon biogeochemical processes in the Hongjiadu reservoir (HJD, karst reservoir) and Shangyoujiang reservoir (SYJ, non-karst reservoir), Yangtze River basin, China. Our results demonstrate that the stronger biological carbon pump (BCP) effect in the lentic area of the HJD reservoir limited CO2 emission (0.9 ± 5.0 mmol m−2 d−1) compared to the SYJ reservoir (50.9 ± 33.4 mmol m−2 d−1), leading to low dissolved inorganic carbon (DIC) and high saturation state of carbonate minerals in the lentic epilimnion. Although the released water from both reservoirs acted as hotspots for CO2 emissions, the results of higher Revelle factor (RF) in the HJD reservoir than SYJ reservoir suggest the greater buffer capacity and lower sensitivity of OC degradation changes in DIC. Moreover, we developed a two-dimensional hydrodynamic model for the HJD. Our calculations indicate that during weak hydrodynamics periods, the enhancement of the BCP effect resulted in substantial sequestration of DIC, reaching up to 379.6 t-DIC•d-1 in the water. Conversely, during periods of strong hydrodynamics, the DIC retention capacity decreased by 69.2 t•d-1, leading to reservoir CO2 emissions more than 7 times higher compared to weak hydrodynamic periods. Our findings emphasize the discernible impact of lithological backgrounds and hydrodynamic conditions on reservoir biogeochemical processes related to DIC. Therefore, the impact of varying geologic settings and hydrodynamic conditions should be considered to minimize errors in regional and global CO2 emission estimates.
BG12-A007
Dinoflagellates Show Greater Contribution Potential to Marine RDOC Relative to Diatoms as Revealed by Short-term Incubations
Futao FANG1#+, Zhuoyi ZHU1, Ding HE2, Yuanbi YI2
1Shanghai Jiao Tong University, 2The Hong Kong University of Science and Technology
Phytoplankton are major contributors of the marine dissolved organic matter (DOM). During phytoplankton death and decomposition, a substantial amount of intracellular organic matter is released into the water environment. These materials undergo microbial utilization and transformation, ultimately contributing to the refractory DOM pool. In this study, we conducted comparative experiments on the organic matter degradation and transformation processes of diatoms and dinoflagellates. We used amino acid and Fourier-transform ion cyclotron resonance mass spectrometry to investigate the differences in the released DOM between diatoms and dinoflagellates, as well as their distinct contributions to refractory DOM under microbial influence. Differences in the morphology of cell fragments after the death and lysis of diatom and dinoflagellate cells were observed. Dinoflagellate cell fragments exhibited greater dispersion, while diatom cell fragments tended to overlap. This disparity may result in dinoflagellate-derived particulate organic carbon (80.6%) being more readily decomposed and transformed than diatom-derived organic carbon (49.3%). Results analyzed using amino acids and FT-ICR MS of phase I indicated that diatoms contributed more labile DOM during the degradation of organic matter (THDAA-C%: 14.7% vs. 5.5%; MLBL: 12.0% vs. 2.2%). The DOC mineralization rate in the dinoflagellate incubation system (23.3%) was lower than in the diatom incubation system (29.6%). Additionally, the proportion of refractory carboxylic-rich alicyclic molecules was higher in the dinoflagellate incubation system (average: 56.7%) compared to the diatom incubation system (average: 50.6%). These findings suggest that the DOM released by dinoflagellates is more stable and contributes more significantly to refractory DOM under microbial influence. The presented results offer insights into the differential contributions of various phytoplankton to refractory DOM, thereby enhancing our understanding of marine carbon cycling at the molecular level.
BG12-A010
Terrigenous Organic Carbon Contributes to Reservoir Carbon Emissions: Potential Role of the Microbial Community Along a Trophic Gradient
Qiong TANG1+, Zhe LI2#
1Chinese Academy of Sciences, 2Chongqing Institute of Green and Intelligent Technology, Chinese Academy of Sciences
Freshwaters are important carbon sources to the atmosphere and are influenced by different sources of organic carbon (OC). Microbial community is a crucial trophic network driving carbon cycling in the aquatic ecosystems. Yet, whether and how their interactions affect carbon cycling and emissions in the reservoir remains unclear. Here, we explored the interactions between phytoplankton and bacteria in reservoirs along a trophic gradient. An increase in the trophic state intensified the interaction between phytoplankton and bacteria communities. Their diversity and niche breadth indexes both decreased. Such intensification was contributed not only by the input of nutrients triggering an increase in trophic state but also by the bulk input of terrigenous OC, shaping the concentrations of CO2 and CH4 in the water phase and their air-water fluxes along the trophic gradient. Upon this, a conceptual framework was proposed to explain the positive/negative feedback of phytoplankton-bacterial interactions to carbon emissions, projecting the dual regulation of aquatic ecosystems and carbon dynamics along a trophic gradient.
BG12-A015
Dissolved Oxygen Isotopes Reveal the Dynamics of Hypoxia in the Changjiang Estuary
Jun ZHOU#+, Huanting HU, Zhuoyi ZHU, Qianqian WANG
Shanghai Jiao Tong University
The expanding hypoxia zones in the Changjiang Estuary severely affects the stability of costal marine ecosystems. It is hard to quantify the different oxygen consumption processes during hypoxia, such as the water column respiration (WCR) and the sediment oxygen consumption (SOC), and distinguishing oxygen consumptions from physical mixing. The oxygen isotope composition of dissolved oxygen (DO δ18O) varies differently with oxygen concentration ([O2]) during WCR, SOC or physical mixing, making it a unique tracer for distinguishing and quantifying the oxygen cycling in the Changjiang Estuary during hypoxia. In this study, we evaluate the contributions of WCR and SOC to the total oxygen consumption budget using oxygen isotope fractionation factors of respiration. Our results suggest more than 3/4 of oxygen consumptions are through WCR. Based on the in-situ DO δ18O from the beginning till the end of hypoxia, we observe the oxygen depletion zone in the north (NODZ) starts in July, maximizes in August with lowest [O2] of 65 μM and a highest DO δ18O value of 14.250‰, and recovers in October. For the southern oxygen depletion zone (SODZ), the lowest [O2] and highest δ18O value for three months are all ∼ 90 μM and ∼ 10‰, indicating a more stable but long-lasting ODZ because of the influences from the low [O2] Taiwan warm current. We suggest that the dynamics of ODZs are associated with the primary productivity in the surface, as the production to respiration ratio calculated from oxygen isotopes are highly correlated to the apparent oxygen isotope fractionation factor of WCR. The NODZ is more sensitive to primary productions as the highly stratified water column intensifies WCR by preventing organic matter sinking to the bottom. Using an isotope-based diffusion-advection-respiration model, we obtain a lowest [O2] of ∼ 9 to 18 μM during hypoxia in this area.
BG12-A019
Hydrological and Microbial Influences on Carbon Dioxide and Methane Emissions in Tropical Headwater Streams of Madagascar
Vonihanitriniaina Diamondra Zoharilala ANDRIAMANANTENA RAMASIARISOA#+, Hojeong KANG
Yonsei University
Tropical headwater rivers serve as natural sources of greenhouse gases (GHGs), where stream hydrology and riverbed biogeochemistry exerting crucial in situ controls. Microbial decomposition of organic carbon in these environments can lead to the production of carbon dioxide (CO2) and methane (CH4), yet our understanding of the role of microbes in GHG production and emissions remains limited. This study integrates data on CO2 and CH4 concentrations and fluxes with biogeochemical information, sediment microbiota, and functional gene analysis to explore how water, land use cover, and sediment properties influence the dynamics of CO2 and CH4 across low-stream orders in Madagascar. Our findings reveal that soil respiration in the hyporheic zone is the primary source of CO2. The Ikopa headwater stream exhibits a substantial amount of dissolved CH4, closely linked to methanogenesis. This is supported by the prevalence of acetoclastic Methanosaeta spp. and hydrogenotrophs Methancocella spp., as well as the abundance of mcrA genes (methyl coenzyme A reductase gene). Moreover, our study highlights the headwater stream as a notable CH4 source in tropical settings, with an average total CH4 flux and CH4 ebullition rate 5 and 30 times higher than those of the global average, respectively. The ebullition pathway accounts for 40 to 90% of the total flux, with temperature emerging as a key driver for both CO2 and CH4 concentrations. Additionally, stream size and land cover control the emissions of CO2 and CH4.In summary, our study emphasizes the significant role of microbial community compositions within headwater streams in the emissions of CO2 and CH4 from tropical rivers. Through quantifying concentrations, fluxes, and identifying key drivers, we contribute valuable insights into the dynamics of greenhouse gas emissions in these critical ecosystems.
BG12-A004
Composition and Transformation Mechanisms of Dissolved Organic Matter at the Sediment-water Interface from Different Environments
Jinfeng GE+, Yulin QI#
Tianjin University
Dissolved organic matter (DOM) is an important component of the carbon cycle and serves as a crucial medium for the dynamic transformation of organic carbon. Investigating the sources, composition, and dynamic transformation mechanisms of DOM in different media is of great significance for understanding aquatic ecosystems and biogeochemical cycles in a given region. The sediment-water interface, which exhibits the largest physical, chemical, and biological gradients in natural water bodies, plays a key role in the exchange and processes of DOM, regulating the biogeochemical processes in watersheds. To better understand the compositional characteristics and transformation mechanisms of DOM at the sediment-water interface, this study employed Fourier-transform ion cyclotron resonance mass spectrometry with ultra-high mass resolution to analyze sediment columns under different salinity conditions. The results showed that organic matter molecules in low-salinity inland water bodies exhibited higher diversity and molecular weight, while organic matter molecules in high-salinity oceans displayed higher saturation. Sediment DOM molecules exhibited the highest specificity, mainly consisting of relatively unstable lipids and hydrocarbon compounds with high sulfur content. In contrast, pore water mainly contained low-molecular-weight nitrogen-containing compounds, with the lowest proportion of specific components. The composition characteristics of surface water and overlying water were more consistent, with slightly higher degrees of oxidation for the compounds and no apparent migration or transformation relationship. By calculating the H:C and O:C ratios of different compound types, it was found that methylation, hydrogenation, decarboxylation, and reduction processes occurred from overlying water to pore water to sediment. In summary, these findings provide new insights into the transformation processes of organic matter at the sediment-water interface in different environments and contribute to a theoretical reference for the source-sink mechanisms of sediments.
BG12-A011
Spatial Distribution and Photochemical Transformation of Dissolved Organic Matter in China’s Major Estuaries
Hui Ying MA#+, Si-Liang LI
Tianjin University
Estuarine coastal zones are rich in dissolved organic matter (DOM) due to the frequent migration and transformation of chemical elements, a process which is augmented by riverine input and marine disturbance. DOM in the oceans is a huge carbon sink that is closely related to both the global carbon cycle and climate change. A total of 255 surface water samples were collected primarily from China’s river estuaries and marginal seas to investigate DOM spatial distribution. The DOC concentration range in the coastal areas was 0.55~2.71 mg/L, with an average of 1.18 mg/L, including the Yellow and Bohai Seas (1.61 mg/L), East China Sea (1.20 mg/L) and the northern South China Sea (0.76 mg/L). In low latitude areas with higher radiation intensity, DOC concentrations were much lower compared with those in higher latitude, which was likely due to the photodegradation of DOM. Photochemical transformation are vital for the fate and ecological effect of oceanic DOM. However, the role of photochemistry in estuarial carbon cycle requires further investigation. Using water samples from two representative Chinese estuaries (the Yangtze River and Pearl River estuaries) as research windows, the changes in composition and bioavailability of DOM under sunlight irradiation were examined. The FT-ICR-MS results revealed that photodegradation led to the loss of moderately unsaturated structures and formulas with high O/C and low H/C ratios, and the preservation of aliphatic groups in oxygenated-sunlit water columns. With a specific focus on sulfur-containing DOM, one of the reactive components of DOM pool, we quantified the photo-transformation of organic sulfur to inorganic sulfur on the basis of precise measurements of dissolved organic sulfur (DOS) using ICP-MS. Our findings confirmed the significance of photodegradation to DOM/DOS fate in the surface waters of estuarine coastal zones. This research was funded by the National Natural Science Foundation of China (grant No.422210017).
Session Chair(s): Punyasloke BHADURY, Indian Institute of Science Education and Research Kolkata
BG17-A006
Are Coastal Phytoplankton Communities Better Equipped to Handle Ocean Acidification?
Anwesha GHOSH#+, Punyasloke BHADURY
Indian Institute of Science Education and Research Kolkata
Ocean acidification is an emerging problem wherein the high dissolution of atmospheric carbon dioxide into the oceans has induced chemical changes resulting in a lowering of oceanic pH. The global reduction of pH has significantly affected marine organisms including phytoplankton, corals, and shellfish. Coastal ocean acidification, however, is more variable and complex compared to open-ocean pH alterations, resulting in locally and regionally enhanced coastal ocean acidification. The Sundarbans, situated in the Ganga-Brahmaputra-Meghna Delta, witnessed rapid dial and seasonal alterations of pH, which far exceed the predicted global pH variabilities. A lab-scale mesocosm study was performed to understand the response of phytoplankton communities of the Mooriganga estuary, which flows through the Indian Sundarbans, to altered pH conditions. Subsequent changes in phytoplankton communities indicate the loss of some taxa leading to a shift toward large-sized taxons and the emergence of dinoflagellates, lowering functional diversity and chlorophyll-driven productivity. Such rapid alternations in primary producer community structure will have implications in nutrient transformations and ultimately on the productivity of fish and the fisheries industry.
BG17-A007
Seasonal Variability in the Carbonate System of the Sunda Shelf Sea: Implications for Coastal Ecosystems
Aan Johan WAHYUDI1#+, Patrick MARTIN2, Yuan CHEN2, Meilun ZHANG2, Su Ping HENG2, Oon Yee WOO2, Bernhard MAYER2, Jani TANZIL3
1National Research and Innovation Agency, 2Nanyang Technological University, 3National University of Singapore
The Sunda Shelf Sea, located in Southeast Asia, is a region of particular importance due to rapid urbanization, increasing anthropogenic pressures, and high marine biodiversity. In particular, corals are expected to be vulnerable to ocean acidification, but we have little knowledge of carbonate system dynamics in coastal regions of Southeast Asia. We will present six years of monthly carbonate system data from the Singapore Strait in the central Sunda Shelf, examining the seasonal and interannual variability of dissolved inorganic carbon (DIC), total alkalinity, CO2 partial pressure, and carbon stable isotopes of DIC in relation to salinity, temperature, and other environmental factors. Terrestrial inputs emerged as a major source of organic matter, the remineralization of which generates CO2 and acidifies coastal seawater. The carbonate system is therefore influenced by regional hydroclimate, which controls terrestrial inputs, and by physical oceanographic variability, which controls the advection of acidified coastal waters across the shelf sea. We will also discuss the complex interactions between the carbonate system and nutrient dynamics, shedding light on potential implications for the coastal ecosystem. This research not only contributes to a deeper understanding of the carbonate system in the Sunda Shelf Sea but also provides insights for managing future eutrophication and ocean acidification in this dynamic tropical marine environment.
BG17-A009
| Invited
South Asia Regional Hub on Ocean Acidification- Science of Ocean Acidification for Society
Punyasloke BHADURY#+
Indian Institute of Science Education and Research Kolkata
The coastal and marine ecosystems across South and South-east Asia have emerged as a key space today. More than 1.5 billion people co-exist along the coastlines with biotopes such as estuaries, mangroves, saltmarshes, lagoons and coral reefs. The rich local, indigenous and cultural knowledges of the people are influenced by ocean on a daily basis. With more than 25% of global population inhabiting the coastlines of South and South-east Asia, the rich marine bioresources serve as a source of livelihood, drive blue economy and contribute to regional GDPs. However, a number of stressors of anthropogenic origin are leading to ocean acidification which is adversely affecting sustainability of coastal and marine ecosystems across South Asia and wider Indo-Pacific. There are a number of challenges being faced in the region including limited data on changing ocean carbonate chemistry, lack of atlas of coastal ocean acidification such as in the Northern Indian Ocean and very limited blue financing initiatives that can support monitoring of regional seas and ocean. The establishment of South Asia Regional Hub on Ocean Acidification (SAROA), part of the Global Ocean Acidification Observing Network (GOA-ON) offers to bridge the gaps in knowledge linking ocean acidification with ocean sustainability. The existing regional and pan-regional frameworks such as South Asia Association for Regional Cooperation (SAARC), Bay of Bengal Initiative for Multi-Sectoral Technical and Economic Cooperation (BIMSTEC), ASEAN-India and QUAD offers opportunity to mainstream ocean acidification research within policy frameworks as well as from polycentric governance approaches. The synergy between the science of ocean acidification, integration of local knowledge and policies can form the basis for promotion of ocean-based enterprises through ocean financing to ultimately achieve sustainable ocean economy.
BG17-A005
Microbial Blue Carbon in Coastal Biotopes – A Meta Analysis from Global South
Arindam ROY#+, Punyasloke BHADURY
Indian Institute of Science Education and Research Kolkata
Microbial necromass, a persistent complex in soil become attraction magnet for researchers to quantify its contribution towards organic carbon stock to manage environmental change. Global South harbors a significant proportion of coastline. Despite that there’s a limited understanding on microbial residual carbon storage in coastal ecosystems across South. To address this research gap, we synthesized a dataset from 25 observations through literature survey. Microbial necromass carbon is the key component of soil organic carbon (24.92%) within first 20 cm of topsoil compared to 16.02 % in 0-10 cm, implies a rapid turnover. Fungal derived residual carbon is the major contributor to SOC in 0-10 cm. Highly abundant soil fungi and its large biomass attributed for major contribution as residual carbon in SOC than bacterial dead counterparts. The ratio of fungal necromass carbon/bacterial necromass carbon varies from 7.49 to 5.81 for 0-10 cm and 0-20 cm respectively. Fungi is the dominating driver to decompose complex substrates, elucidating microbial carbon pump in driving SOC stabilization. pH, total nitrogen stimulates the microbial blue carbon accumulation. These results also highlight the role of climatic factors in shifting ecosystem processes, microbial community structure for deducing the variability in its contribution to soil organic carbon pool of coastal ecosystems. Our study shed light on need to develop a core framework to find environmental attributes, regulating microbial necromass carbon to delineate C stock for addressing UN SDG 13 goals and beyond.
Session Chair(s): Xiujun WANG, Shanxi Agricultural University, Lishan RAN, The University of Hong Kong
BG09-A007
Substantially Enhanced Carbon Sink Capacity in the Chinese Loess Plateau Due to Reduced Aquatic Carbon Transport Through Effective Soil Conservation
Lishan RAN#+, Boyi LIU, Shuai CHEN
The University of Hong Kong
Aquatic export of terrestrial carbon plays a significant role in modulating the magnitude of terrestrial carbon sink capacity. Previous estimates of the terrestrial carbon sink may have been overestimated because not all carbon losses across heterogeneous landscapes are accurately determined and properly accounted for. This is particularly possible for catchments with high erosion and a strong terrestrial-aquatic carbon transfer potential. Meanwhile, soil erosion control is of global importance because accelerated soil erosion by human activity is a major threat to ecosystem viability. However, the significance and role of soil conservation in reshaping landscape carbon accounting has not been comprehensively integrated in the terrestrial carbon sink. In this work, we assessed the magnitude of terrestrial-aquatic carbon transfer in affecting the landscape-scale carbon balance in the semiarid Chinese Loess Plateau (CLP), the world’s most vulnerable region to soil erosion. The results show a surprisingly low terrestrial-aquatic carbon transfer that offset the terrestrial net ecosystem productivity by only 7.5%, which we attribute to the effective implementation of soil erosion control measures. Despite the highest soil erosion, the semiarid CLP acts as an effective carbon sink at 43.2 ± 22.6 g C m–2 year–1, which is comparable to temperate forest in absorbing atmospheric CO2. Moreover, carbon burial in reservoirs has created an additional anthropogenic carbon sink of 2.9 ± 1.1 g C m–2 year–1. Our findings indicate that effective implementation of soil conservation can significantly reduce terrestrial-aquatic carbon transport and enhance landscape carbon sequestration capacity. The co-benefits of soil conservation in erosion control and carbon sequestration have important implications for policy makers in other regions of the world undergoing increasing erosion intensity to pursue environmental sustainability and carbon neutrality.
BG09-A008
Dynamics and Drivers of Soil Carbonate in the Northern China: A Review and Perspective
Xiujun WANG1,2#+, Tongping LU3, Meiling MO4, Haolin ZHAO4, Jiaping WANG5
1Shanxi Agricultural University, 2University of Maryland, 3Peking University, 4Beijing Normal University, 5Shihezi University
Soil carbonate (SIC) is an important reservoir of carbon in arid, semi-arid and semi-humid regions, which exceeds soil organic carbon (SOC) greatly in drylands. However, there were not much done to evaluate the dynamics and drivers of SIC in the terrestrial ecosystems. While limited studies reported a reduction of SIC in topsoils due to acidification associated with nitrogen fertilization, there was also evidence of enhancement in SIC in subsoils under various fertilization measures. On the other hand, previous studies showed inconsistent findings on the relationship between SIC and SOC. While both negative and positive correlations between SOC and SIC may exist, water limitation and saline/alkaline conditions in the arid and semi-arid regions would be beneficial to carbonate formation. Thus, a positive relationship would be more common, in particular, when SOC and SIC stocks in deep soils are included, which implies that increasing SOC may lead to an increase of SIC in arid and semi-arid lands. Here, we present a summary of relevant studies conducted in the northern China, and provide a review on the SIC dynamics, drivers and its relationship with SOC. We explore the underlying mechanisms regulating the transformations of main soil carbon forms, and discuss the potential of carbon sequestration as SIC in arid and semi-arid lands.
BG09-A013
POC Composition and Its Impact on Bottom Water Hypoxia in the East China Sea
Hai-Yan JIN1#+, Jianfang CHEN2, Dewang LI1, Zhongqiang JI1, Ningxiao YU3,1, Ying LUO3, Bin WANG1, Zhi YANG2, Ling CHEN1
1Ministry of Natural Resources, 2State Oceanic Administration, 3Shanghai Jiao Tong University
Typical seasonal hypoxia systems was located off the Changjiang Estuary in summer. It is one of the largest coastal hypoxic systems in the world. The hypoxia formation is related to the diffusion of Yangtze River, water stability and strength of stratification, upwelling, water invasion of Taiwan warm current, nutrient supply and supply of a large amount of organic matter etc. In brief, suitable hydrological conditions(strong stratification), sufficient nutrient supply and large amount of organic matter input formed and maintained the summer hypoxia off Changjiang Estuary. POC and hypoxia process were monitored and investigated in the Changjiang estuary during summer season from 2020 to 2022. The result showed that terrestrial suspended particles transported by Changjiang are mainly trapped in Changjiang estuary turbidity zone and formed the turbidity front with high POC values. A patch of high POC concentrations in the surface water on the offshore was also found. And a significant positive correlation between Chl a and POC concentrations on the offshore surface indicates that high biomass contributes to the high POC concentrations. The δ13C values were higher than -23.02‰, and it confirms that the POC is mainly derived from marine sources. The correlation between POC and AOU indicates that the marine source POC decomposition consumes dissolved oxygen and leads to the generation of hypoxia off the Changjiang Estuary.
BG09-A001
Unexpected Reduction in Megacities’ Anthropogenic CO2 Emissions in Lower-middle Reaches of the Yangtze River During Extreme 2022 Heatwave
Jingye TAN1+, Jun WANG1#, Haikun WANG1, Zhu LIU2, Ning ZENG3, Ran YAN1, Xinyu DOU2, Xunmei WANG1, Meirong WANG4, Fei JIANG1, Hengmao WANG1, Weimin JU1, Jing CHEN5
1Nanjing University, 2Tsinghua University, 3University of Maryland, College Park, 4Nanjing University of Information Science & Technology, 5University of Toronto
An unprecedented heatwave hit the Yangtze River Basin (YRB) in August 2022. We analyzed changes of anthropogenic CO2 emissions in 8 megacities over lower-middle reaches of the YRB, using a near-real-time gridded daily CO2 emissions dataset. Compared to August 2021, emissions in 6 out of 8 megacities during the extreme 2022 heatwave decreased, especially in Shanghai with a decrease of 2.97 Mt CO2 (7.27%). Distinguishing by sectors, we find that power emissions in all megacities increased due to increased cooling demand, whereas industrial emissions decreased which was closely related to the China’s policy to ensure household power supply during heatwaves. Hence, reduction in industrial emissions counterbalanced increase in power emissions, leading to an overall decrease in CO2 emissions of 3.83 Mt across these 8 megacities. Consequently, extreme heatwaves may not invariably be linked to increased CO2 emissions due to policy interventions in the power distribution between industrial and residential demands. Our study offers valuable insights into the complexities of anthropogenic CO2 emissions in megacities amidst frequent summer heatwaves intensified by greenhouse warming.
BG09-A010
Biosphere-atmosphere Carbon Exchange and Global Warming Potential in a Restored Mangrove Ecosystem in Southern China
Zhe XU#+, Xianglan LI
Beijing Normal University
Mangroves serve as a highly efficient ecosystem for sequestering atmospheric CO2. However, whether restored mangroves act as carbon sinks or sources remained unclear. Recent studies have indicated that radiative forcing induced by methane (CH4) emissions and Albedo changes during mangrove restoration can lead to the warming effects on the climate. It is crucial to estimate the carbon exchange and global warming potential (GWP) of restored mangroves using quasi-continuous, high temporal resolution measurements. In this study, we measured the CO2, CH4, and Albedo fluxes using an open-path eddy covariance system in an 8-year-restored mangrove ecosystem located at the northern region of the mangrove distribution area in China. Results showed that the restore mangroves functioned as a CO2 sink, with the mean annual net ecosystem CO2 exchange (NEE) of –522 g C m−2 yr−1. The CO2 uptake of restored mangroves was stronger during the wet than dry seasons owing to a combined influence of higher photosynthetically active radiation and temperature. Our restored mangroves also acted a CH4 source, with the annual emission of 7.44 g C m–2 yr–1. The Albedo varied slightly with a range of 0.110–0.127. The integrated GWPs computed by joint CO2, CH4, and Albedo were –1329 and –1864 g CO2-eq m–2 yr–1 over the 20- and 100-year time horizons, respectively. The negative values revealed that a net cooling effect occurred in mangrove restoration, primarily driven by CO2 uptake. The warming effects caused by CH4 emissions and Albedo changes had the potential to partially offset the CO2 uptake by 12.9–37.6% and 0.084–0.419%, respectively. Even only restored for 8 years and located in the northern regions of mangrove distribution in China, our restored mangroves still had a positive effect on mitigating climate change, particularly due to a substantial cooling effect.
BG09-A011
How Sun-induced Chlorophyll Fluorescence Reveals the Carbon Sink Potential of Blue Carbon Ecosystems: A Mangrove Restoration Region Case Study
Yuting HUANG#+, Xianglan LI
Beijing Normal University
Accurately describing the dynamics of mangrove photosynthesis under the influence of climate change is crucial for quantifying the carbon sequestration potential of blue carbon ecosystems (BCEs). Sun-Induced Chlorophyll Fluorescence (SIF) can directly detect plant photosynthesis, but the relationship and mechanism between mangrove SIF and gross primary productivity (GPP), between the yield of SIF (SIFy) and light use efficiency (LUE) are still lacking consensus. In this study, we conducted long-term and high-frequency ground observations of SIF and GPP from 2021 to 2022, and investigated the relationship and mechanism between SIF and GPP in a mangrove restoration region. We used random forest algorithm to construct canopy photosynthesis estimation models based on SIF, and analyzed the driving factors affecting the canopy photosynthesis. The results showed that, from the diurnal scale to the seasonal scale, SIF-GPP had a strong positive correlation (R2>0.65, p0.001), and changed from nonlinear to linear. Light saturation caused nonlinear GPP-APAR response, which decreased with the increase of temporal scale but didn’t disappear. SIF and GPP still maintained nonlinear relationship with APAR on seasonal scales. In our study, SIFy and LUE were negatively correlated (r=-0.60, p0.001, seasonal scales), and the positive SIFy-APAR relationship was the main factor affecting the SIFy-LUE relationship. In addition, the GPP simulation had high accuracy (R2=0.90, MAE=0.63 μmol m-2 s-1, MSE and RMSE=0.81 μmol m-2 s-1), and the inclusion of environmental factors characterizing temperature and drought conditions contributed to GPP estimation. While the wind speed and vapor pressure deficit among the environmental factors contributed to the LUE simulation based on SIFy. Our study provided a theoretical basis for revealing the relationship and potential mechanism between SIF and mangrove canopy photosynthesis. New insights for quantifying the carbon sequestration potential of BCEs at large scales in the future were offered.
Session Chair(s): Bhoopesh MISHRA, Illinois Institute of Technology
BG15-A014
Soil Texture Governs the Temperature Sensitivity of Coastal Wetlands
Yeonsoo KWAK1+, Yerang YANG1, Jaehyun LEE2, Hojeong KANG1#
1Yonsei University, 2Korea Institue of Science and Technology
Coastal wetlands are significant reserves of organic carbon, primarily sequestered within the soil. However, these ecosystems are extremely vulnerable to climate change, notably sea level rise and rising global temperatures. Rising sea levels lead to tidal marsh migration and soil erosion, which significantly change soil properties including soil texture. These shifts in soil texture may interact with rising temperatures to reshape carbon decomposition patterns in coastal wetlands. Yet there is a lack of understanding of the temperature sensitivity (Q10) of coastal wetlands based on soil texture as well as its underlying mechanisms. This generates uncertainties in global-scale models for estimating coastal wetland carbon stock, as these models rely on fixed Q10 values. In this study, we investigated the Q10 of ten coastal wetlands along the coastline of South Korea. Soil samples were incubated for 40 days in four cycles spanning 10 to 30°C in 5-degree increments following a 14-day pre-incubation period. Samples were divided into aerobic and anaerobic treatments to simulate the characteristic low and high tides of the ecosystem. Q10 values exhibited a negative correlation with soil sand percentage in both aerobic and anaerobic samples. We attribute this correlation to the difference in soil carbon quality among the samples, following the ‘carbon quality-temperature hypothesis.’ The carbon quality-temperature hypothesis proposes that there is a positive correlation between Q10 and soil carbon recalcitrance. Soil redox data align with this hypothesis; sandy soils exhibited lower oxygen content, resulting in the slower depletion of labile carbon. This, in turn, reduced soil carbon recalcitrance. Our findings offer insight into the relationship between Q10 and soil texture, demonstrating the impacts of a changing soil landscape on the global carbon cycle, potentially escalating climate change.
BG15-A012
Origin and Regional Diversity of the Early Pliocene-Late Miocene Biogenic Bloom in the Atlantic Ocean
Emily LIU1#+, Anna Joy DRURY2, Bridget WADE3, Thomas WESTERHOLD4, David KING3
1Imperial College London, 2University of Leicester, 3University College London, 4University of Bremen
The Early Pliocene-Late Miocene Biogenic Bloom (LMBB) was a globally distributed event between ~8 – 4.5 Ma, coeval with major climatic and tectonic transitions. Utilising sediment records from Ocean Drilling Programme (ODP) Sites 982 (N Atlantic Ocean) and 1264 (SE Atlantic Ocean), this study generates a continuous record of carbonate content (% CaCO3) via calibration of X-ray fluorescence (XRF) ln(Ca/Fe) records spanning 8 to 3 Ma at orbital-scale resolution. Here, we present a comprehensive synthesis of CaCO3 content and mass accumulation rates (MARs), XRF elemental ratios of Ca/Fe, Ca/Si, K/Ti and Ba/Ti, spectral analysis, and micropalaeontological dissolution proxies, that provides an inter-site comparison between North and South Atlantic Ocean. We identify a time lag for the onset of the LMBB at the North Atlantic (~7.5 Ma) succeeding the South Atlantic (~7.9 Ma), attributed to the redistribution of nutrients induced by changes in intermediate-deep water formations that were potentially sourced from the Southern Ocean, rather than changes in the North Atlantic Deep Water formation. A general geographic pattern associated with the timing of the onset of the LMBB is identified across ocean basins with reference to timing proposed by previous studies, such that nutrient redistribution is likely to have contributed to the progression of the LMBB in addition to a global nutrient flux possibly initiated from the Pacific. The prevailing obliquity-precession pacing on % CaCO3 since 7.1 Ma at Site 1264 and since 6.5 Ma at Site 982 coincides with the onset of elevated CaCO3 MARs, which may be associated with enhanced glacial weathering contributing to spiked nutrient input at high latitudes. The termination of the LMBB is identified at 4.3 Ma and 3.3 Ma at Sites 982 and 1264 respectively, regardless of a long-term increase in carbonate preservation since the LMBB onset, reflecting a genuine presence of the LMBB at the Atlantic Ocean.
BG15-A006
Strategy of Spectral Imaging for Vegetation Using Micro-satellite and Drone
Yukihiro TAKAHASHI1#+, Garid ZORIGOO1, Nobuyasu NARUSE2
1Hokkaido University, 2Shiga University of Medical Science
Conventional analysis based on the limited number of bands with broadband optical filters installed at camera onboard most of satellites or drones are not sufficient. As many studies have reported, imaging at high spectral resolution provides practical information for them. Nevertheless, the hyperspectral or narrow-band imaging trials from space have not been regarded as practical. Since the vegetation spectrum is strongly affected by combinations of viewing and sun angles, in order to increase the opportunity of spectral imaging at any directions from satellites, construction of a big spectral library for all angles is essential. Using this spectral library we can observe the field with actual swath of 1,000-2,000 km from low earth orbit at several bands selected for individual purpose of vegetation investigation. To do this inexpensive spectrometer to be used on the ground, such as 1 K USD or less, was developed, which can record the relative angles between viewing and sun angles automatically. Also we have been developing 50-kg micro-satellites with camera that can chose limited number of bands among 400-600 bands from visible to NIR range, costing about 7 M USD including launch cost. Such 5 micro-satellites have been launched and operated successfully. If we work together internationally to build and operate 24 or 48 satellites and enough number of ground stations, we can image any area over the world immediately at cost of one large satellite at the highest accuracy.
BG15-A016
Uncertain Changes of Vegetation Greenness Interannual Variability on Half of the Global Vegetated Surface
Xiangzhong LUO1#+, Jiaqi TIAN2
1National University of Singapore, 2Nanjing University
Changes in the interannual variability (IAV) of vegetation greenness and carbon sequestration are key indicators of the stability and climate sensitivities of terrestrial ecosystems. Recent studies have examined the changes in the vegetation IAV using atmospheric CO2 observations and dynamic global vegetation models (DGVMs), however, reported different and even contradictory trends of IAV. Here, we investigate the changes in the IAV of vegetation greenness, quantified as coefficient of variability (CV), over the past few decades based on six long-term and three short-term satellite remote sensing products. Our results suggested that on half of the global vegetated surface, CV trends were uncertain (i.e., inconsistent CV trends when using different satellite remote sensing products). Meanwhile, we found that 22.20% and 28.20% of the global vegetated surface (i.e., mostly in the non-tropical land surface) show significant positive and negative CV trends (p ≤ 0.1), respectively. Regions with higher air temperature and greater aridity tend to have increasing CV trends, whereas greater vegetation greening trend and higher nitrogen deposition lead to smaller CV trends. Our study provides a remote sensing-based examination of the changes in the IAV of global vegetation greenness, and highlights the potential issues in studying the response of terrestrial ecosystems to climate change.
BG15-A007
Biological Oxygen Production Rate Enhanced by Sea Ice Melting in the Southern Ocean: Estimates from the O2/Ar and Triple Oxygen Isotope Approach
Jun ZHOU, Huanting HU#+
Shanghai Jiao Tong University
The Southern Ocean plays a critical role in regulating the global carbon cycle and the atmospheric CO2 level. The influx of CO2 into the deep ocean is enhanced by the biological pump through photosynthesis, which also produces organic matters sinking to the deep ocean for carbon storage on a longer time scale. The primary productivity or biological oxygen production of the Southern Ocean is mainly controlled by the availability of iron. Previous studies observed a decreasing trend of oxygen productions from low latitude to high latitude towards Antarctica. This is caused by the decreasing fluxes of iron from land to the Southern Ocean. In this study, we estimate the net and gross oxygen production rate of the Southern Ocean based on O2/Ar ratios and a triple oxygen isotope approach. We analyzed the O2/Ar ratios and triple oxygen isotope compositions of dissolved oxygen collected from the Cosmonaut sea in January, 2021. Averaged net and gross O2 production rate are 12.9 and 133 mmol O2 m-2 day-1, respectively. We do not observe latitudinal trend of O2 production rates in our samples because they are all close to the Antarctica (63° S to 67° S). We then compare the O2 production rate with the changes of sea ice concentration during the past 60 days prior to the sampling date. We observe some peaks of O2 productions correlate well with sea ice melting, indicating enhanced productivity induced by potential iron release from sea ice melting.
BG15-A018
League of Geophysical Research Exellences for Tropical Asia (LeXtra) Initiative
Masayuki KONDO#+
Hiroshima University
Tropical Asia is a complex geographical region, consisting of mainland and island components dominated by tropical rainforest, cropland, and savanna woodlands in drier areas. Forest-cover constitutes 236 million hectares (Mha), corresponding to approximately 15 % of the world’s tropical forests. A large part of tropical Asia is considered as a biodiversity hotspot, because it harbors a high number of endemic species, especially the most diverse mangrove species in the world. The region is also home to the most extensive tropical peatlands in the world, with an area of 25 Mha and an estimated carbon pool of 69 Pg C.In addition to the complexity and diversity of ecosystems, two major factors controlling the dynamics of carbon uptake and release make it challenging to assess the carbon budget (a net exchange of carbon in and out of the terrestrial boundaries of a certain region) in Southeast Asia: (1) the large interannual climate variability, due to the El Niño Southern Oscillation (ENSO) cycles, and (2) forest loss, due to land use, land-cover change, and forestry (LULUCF). Notably, synergies between ENSO-driven droughts and rapid LULUCF have resulted in several extreme episodes of carbon emissions into the atmosphere, particularly when forest fires occur. As a region characterized by key factors that exacerbate carbon emissions, the question has been raised whether carbon neutrality can be achieved in tropical AsiaTo better understand the state toward carbon neutrality in tropical Asia, here we established a research network named as “League of geophysical research eXellences for tropical asia (LeXtra)”. This presentation summarizes current issues in biogeochemical cycles and the current state of carbon neutrality in tropical Asia.
Session Chair(s): Jeehwan BAE, KyungHee Univ.
BG02-A010
Terrestrial Carbon Budget Estimation Over the Qinghai-Tibet Plateau from Eddy Covariance Flux Measurements Using Memory-based Deep Learning
Mengyao ZHAO1+, Wei HE2#, Peipei XU1, Ngoc Tu NGUYEN3, Hua YANG4, Chengcheng HUANG5
1Anhui Normal University, 2Zhejiang University of Technology, 3Hohai University, 4Beijing Normal University, 5China University of Geosciences
The terrestrial carbon sink of Qinghai-Tibet Plateau (QTP) is highly sensitive to global warming, and its size and distribution are quite uncertain. Using advanced deep learning methods with more in-situ flux data from recent extensive observation activities is expected to improve our understanding on the spatiotemporal regimes of net carbon exchange in this region. Here, we utilized in-situ flux data over 30 sites and multiple land surface data to construct long short-term memory networks for various ecosystem types in the QTP region and to estimate regional net ecosystem exchange from 2003 to 2018. For different ecosystems, the determination coefficient for the test set ranges from 0.74 to 0.96, and the root mean square error ranges from 0.16 to 0.64 gC m-2 mon-1. Our flux upscaling estimate points the entire region to a carbon sink, with an annual mean of 117.35 TgC year-1. Spatially, the Western and Northern alpine grasslands are sinks, gradually weakening from the North to the South; The alpine meadows in the East are sources, gradually weakening from the West to the East. During the study period, this regional sink increases at the rate of 0.015 TgC year-2. Alpine steppes dominate carbon sequestration and slightly decreases, ranging from 131.66 to 138.23 TgC year-1; Shrubs are small increasing sink, ranging from 1.96 to 3.68 TgC year-1; Alpine meadows are overall decreasing carbon sources, ranging from 15.16 to 24.21 TgC year-1; Wetlands are carbon sources in most years and keep increasing, with the largest emission of 6.31 TgC year-1 and the largest uptake of 2.17 TgC year-1. The increase in regional carbon sink is mainly contributed by shrubs, partially offset by the increased carbon emission in wetlands. Our study provides new insights into the terrestrial carbon budget over QTP.
BG02-A011
Spatio-temporal Variability and Environmental Controls of Temperature Sensitivity of Ecosystem Respiration Across the Tibetan Plateau
Danrui SHENG+, Xianhong MENG#, Shaoying WANG, Zhaoguo LI, Lunyu SHANG, Hanlin NIU
Chinese Academy of Sciences
Warming-induced carbon loss via ecosystem respiration (Re) is probably intensifying in the alpine grassland ecosystem of the Tibetan Plateau owing to more accelerated warming and the higher temperature sensitivity of Re (Q10). However, little is known about the patterns and controlling factors of Q10 on the plateau, impeding the comprehension of the intensity of terrestrial C-climate feedbacks for these sensitive and vulnerable ecosystems. Here, we synthesized and analyzed multiyear observations from 14 sites to systematically compare the spatio-temporal variations of Q10 values in diverse climate zones and ecosystems, and further explore the relationships between Q10 and environmental factors. Moreover, structural equation modeling (SEM) was utilized to identify the direct and indirect factors predicting Q10 values during the annual, growing, and non-growing seasons. The results indicated that the estimated Q10 values were strongly dependent on temperature, generally, with the average Q10 during different time periods increasing with air temperature and soil temperature measurement depth (5 cm, 10 cm, 20 cm). The Q10 values differentiated among ecosystems and climatic zones, with warming-induced Q10 declines being stronger in colder regions than elsewhere based on spatial patterns. NDVI was the most cardinal factor in predicting annual Q10 values, significantly and positively correlated with Q10. Soil temperature was identified as the other powerful predictor for Q10, and the negative Q10~Ts relationship demonstrates a larger terrestrial carbon loss potentiality in colder than in warmer regions in response to global warming. Note that the interpretations of the effect of soil moisture on Q10 were complicated, reflected in a significant positive relationship between Q10 and soil moisture during the growing season and a strong quadratic correlation between the two during the annual and non-growing season. These findings are conducive to improving our understanding of alpine grassland ecosystem carbon-climate feedbacks under warming climates.
BG02-A008
Creation of Methane Concentration Maps for the Paddy Rice Fields in Korea Using Meteorological Data and Machine Learning
Jiah JANG#+, Yangwon LEE
Pukyong National University
The recent rapid increase in greenhouse gas emissions has accelerated global warming. As a result, climate change is progressing in a more serious appearance. In particular, long-term greenhouse gases such as methane (CH4) have a warming effect about 15 to 34 times stronger than carbon dioxide (CO2), and thus the importance of calculating methane emissions generated in Korea is emerging. Agriculture is one of the major causes of methane emissions among human activities, accounting for about 43% of total methane emissions. Therefore, accurately predicting and identifying methane emissions from agricultural lands is an essential factor in responding to global warming and environmental problems. In this study, based on the GBM model, LDAPS meteorological data and FluxNet ground observation data in Cheorwon paddy areas were used, and a methane concentration map for methane emissions caused by paddy fields was generated for the Korean region. More detailed regional changes were identified with 1.5 km grid unit information to secure spatial detail. In addition, it was used as an important variable in predicting methane concentration by utilizing the relationship between various meteorological factors and methane emissions. Geothermal flux and latent heat flux affect the thermal properties and heat exchange process of the soil. Moisture, relative humidity, and soil moisture can affect methane production and emission in relation to the moisture state of farmland. By analyzing the daily data of the methane concentration in rice paddies on the Korean Peninsula, the predicted data was displayed on the map to visualize spatially and temporally. Through this, it is thought that the spatio-temporal characteristics of the methane concentration can be grasped and analyzed with better temporal detail.
BG02-A015
Enhancing Methane Uptake Through Afforestation of Steppe Grasslands
Ji Weon CHOI+, Hojeong KANG#, Yerang YANG
Yonsei University
Grassland ecosystems cover large areas of the Earth's surface and play a critical role in storing soil organic carbon and acting as methane (CH4) sinks, which is the second strongest greenhouse gas. However, the steppe grasslands are currently experiencing degradation due to various disturbances, including climate change, overgrazing, and land use change. Afforestation projects have been implemented to mitigate this degradation, but their effects on CH4 uptake remain unclear. This study aimed to evaluate the impact of afforestation on CH4 flux and the abundance of methanotrophs in grass lands. We observed CH4 flux and analyzed the soil physicochemical properties and abundance of methanotrophs in both natural grassland and afforested areas with Populus euramericana. The results revealed a higher CH4 uptake (+2.63 ± 0.23 mg CH4 m−2 day−1) in afforested areas compared to the natural grasslands (-0.17 ± 0.15 mg CH4 m−2 day−1). The abundance of methanotrophs was more abundant in afforested areas than in natural grasslands. A significant correlation was found between soil CH4 uptake and abundance of methanotrophs. In addition, our research identified a positive correlation between silt composition and abundance of methanotrophs, attributable to the enhanced water-holding capacity of silt, resulting in high organic matter for methanotrophs. Our findings suggest that afforestation of steppe grasslands has the potential for enhanced CH4 uptake by modifying soil physicochemical properties and microbial abundance, thus ultimately enhancing CH4 uptake.
BG02-A013
Quantifying the Impact of Urban Development on Changes in Forest Carbon Stocks
Jaewon SHIN#+, Sujong JEONG, Dong Yeong CHANG1,1
Seoul National University
Urban areas are responsible for a significant proportion of global carbon emissions. It is therefore crucial to manage carbon sources and sinks to mitigate global climate change. Urban forests act as primary sinks in urban areas, so accurate quantification of forest carbon stocks is essential for managing the carbon balance in these areas. In this study, we quantified changes in forest carbon stocks due to urbanization using high-resolution multisource remote sensing data, including Landsat images, and NASA Digital Elevation Model (NASADEM) data. The study areas include twenty South Korean cities that have undergone large-scale urban development between 2006 and 2023. We used Random Forest machine learning algorithms to calculate changes in forest carbon stocks due to urban development. To estimate total biomass and carbon stocks more accurately, the training dataset was optimized to represent the complex topography of the Korean Peninsula using integrated national forest inventory and topographic information at the regional level. Our results show that urban areas expanded by an average of 3.24 km2 per year, while forest areas decreased by an average of -1.93km2 per year over the 17-year period. This resulted in a reduction in forest carbon stocks of -10,118 tC per year. The estimated total loss of carbon stocks due to urban development was about -172,007 tC. Changes in urban forest carbon stocks were primarily due to differences in the size of the forest area preserved, and secondarily due to the composition of the forest. This study shows that high-resolution satellite remote sensing data can improve our understanding of carbon stock distribution and support carbon-neutral policies. This may be beneficial for countries facing the dual challenge of rapid urban development and carbon management commitments.
BG02-A009
Estimation of Fractional Urban Tree Canopy Cover Based on Machine Learning Algorithms and Optical Satellite Imagery
Bae SEJEONG+, Bokyung SON, Taejun SUNG, Yeonsu LEE, Jungho IM#, Yoojin KANG
Ulsan National Institute of Science and Technology
The spatial distribution of urban trees serves as an indicator for evaluating biomass, carbon storage, and absorption capacity of urban ecosystems. Although light detection and ranging (LiDAR) data has been extensively utilized in urban tree observation due to its high spatial resolution, it has limitations in accessibility and higher costs compared to satellite imagery. In this study, we estimated the fractional tree canopy cover (FTC) in urban areas using high-resolution optical satellite data from Sentinel-2. However, the relatively coarse resolution of satellite imagery makes it challenging to consider the heterogeneous landcover of urban areas. Therefore, Four machine learning (ML) methods (random forest, light gradient boosting machine, support vector regression, multi-layered perceptron) are compared, leveraging contextual information; average (mean) and standard deviation (std) values within a 30-meter grid derived from 10m resolution Sentinel-2. Additionally, to account for the heterogeneous landcover types in urban areas, fractional coverage maps for distinct landcover classes within 30m grids from the existing level 3 landcover map provided by the Ministry of Environment of South Korea were used. Then, four schemes with different combinations of input variables were compared. Notably, all ML methods show the best performance when all variables considering the heterogeneity of landcover (i.e., mean, std, and fractional cover) are used (Scheme 4, S4). Among ML models, the random forest (RF) model in S4 demonstrates superior performance, with an R2 of 0.8196, a mean absolute error (MAE) of 0.0749, and a root mean squared error (RMSE) of 0.1022. Subsequently, when the trained RF model is applied to entire city of Suwon, it also exhibits high accuracy (R2 of 0.8702, MAE of 0.0873, and RMSE of 0.1335). In this study, we present a method for estimating missed carbon sinks, taking into account the heterogeneity of urban landcover, utilizing Sentinel-2 satellite imagery.
BG02-A016
Toward High-resolution Carbon Uptake Monitoring: AI-driven GPP Estimation Using Satellite Imagery
Bokyung SON1+, Taejun SUNG1, Dongjin CHO1, Cheolhee YOO2, Jungho IM1#, Yeonsu LEE1, Jongho KIM3, Sujong JEONG3
1Ulsan National Institute of Science and Technology, 2The Hong Kong Polytechnic University, 3Seoul National University
Continuous and accurate monitoring of carbon fluxes is crucial for tracking climate change impacts and mitigating environmental degradation. Leveraging satellite data enables the assessment of carbon uptake in various vegetation types across different spatial and temporal resolutions. This study primarily focuses on estimating gross primary productivity (GPP) using high-resolution satellite imagery and employing machine learning techniques. Vegetation indices from the Moderate Resolution Imaging Spectroradiometer (MODIS) and Landsat satellites were used as independent variables, while daily GPP data from 126 stations in FLUXNET2015 was employed as a dependent variable for machine learning models. Through leave-one-station-out cross-validation, the study compares the performance of three machine learning techniques: Random Forest, Light Gradient Boosting Machine, and Artificial Neural Network (ANN). The ANN model demonstrated the highest performance, achieving a coefficient of determination of 0.734 and a root mean square error of 2.182 gC/m2/d. The high-resolution GPP estimated by the ANN model effectively captured urban carbon sinks in Seoul, South Korea, which were overlooked in lower-resolution datasets. Additionally, it exhibited discernible trends correlating with the proportion of urban vegetation spaces in Local Climate Zone classes. These research findings could provide a foundation for continuous and precise monitoring of carbon fluxes in urban areas through high-resolution GPP encompassing both natural and urban green spaces.
BG02-A002
Increased DOC Concentration of a Temperate Forest Stream in Korea During 2012–2022
Seung-Cheol LEE1+, Eun-Ju LEE1, Ji-Yeon CHA1, Kyuyeon LEE1, Seungwoo SON2, Sunghwan KIM2, Neung-Hwan OH1#
1Seoul National University, 2Kyungpook National University
Headwater streams deliver organic carbon from ~60% of land to large rivers. However, studies on temporal variation of DOC concentration ([DOC]) of forest headwater streams for more than a decade are rare in Korea. We have measured weekly stream [DOC] of a temperate forest from 2012 to 2022 in Korea. We have also analyzed radiocarbon isotope ratio (Δ14C) and molecular composition of the stream dissolved organic matter (DOM), using accelerated mass spectrometry and Fourier transform ion cyclotron resonance mass spectrometry (FT-ICR MS), respectively, for a subset of composite samples during winter months. Winter [DOC] was chosen as a baseline, as summer [DOC] is heavily influenced by precipitation. Stream [DOC] ranged from 0.2 to 3.2 (0.7±0.3, mean±s.d.) mg L-1, fluctuating seasonally, with the highest levels in summer (mean of 0.8 mg L-1) and the lowest in winter (mean of 0.4 mg L-1). Linear regression for the stream [DOC] showed an increase from 0.5 to 0.8 mg L-1 for the 11 years. The increase in stream [DOC] was observed in all four seasons. The stream DOM during winter was dominated by lignin-like compounds (70–80%), followed by tannin-like compounds (8–28%). Stream [DOC] in winter (2017–2020) was negatively correlated with the percentage of lignin-like compounds (O/C ≤ 0.67) while that was positively correlated with percentage of tannin-like compounds (O/C > 0.67). The composite stream Δ14C-DOC was the most depleted (-92‰) when the stream [DOC] was the highest, 0.7 mg L-1 among all February when mean [DOC] is the lowest in a year. The results suggest an increase in the release of microbially oxidized organic matter that could have been stored longer in the soil. The results also suggest that concentration and composition of DOM change over time, which can influence the degradation of DOM and CO2 evasion from large rivers downstream.
Session Chair(s): Lulie MELLING, Sarawak Tropical Peat Research Institute, George BURBA, University of Nebraska/LI-COR
BG16-A002
| Invited
Forecasting Crop Water Demands in Irrigated Potato Crops: Flux Science to Support Sustainable Agriculture
Ankur DESAI1#, Ammara TALIB2, Nikaan KOUPAEI ABYAZANI1+
1University of Wisconsin-Madison, 2Harvard University
Terrestrial water in the biosphere and atmosphere is linked through evapotranspiration (ET). In groundwater irrigated agricultural areas, some fraction of this water is lost to the atmosphere in the form of ET. Unsustainable groundwater extraction to meet the increasing demands of irrigated agriculture and climate change can result in prolonged periods of water depletion. One such region is the vegetable growing areas of the Wisconsin Central Sands (WCS) in the Midwestern region of the USA. To combat overexploitation of groundwater aquifers and support irrigation management, it is essential to quantify and compare crop and natural ecosystem (e.g., forest) water use demand based on ET to aid policymakers and water resources managers for water allocation. Our lab partnered with the Wisconsin Potato and Vegetable Growers Association (WPVGA) and the state of Wisconsin Department of Natural Resources (WiDNR) to quantify potato, natural ecosystem, and other crop ET in this region over a six year study period (2018-2023). In wet years, both irrigated potatoes and forests generally had similar rates of ET. Seasonal ET amounts were similar to total precipitation, implying that not all irrigated water was lost to the atmosphere, and some groundwater recharge is occurring, contrary to policy assumptions. In dry years, we found a stronger decrease in ET in the forests but limited change in potatoes, implying regional water supply stress occurring from high rates of irrigation, suggesting that precision irrigation and groundwater drought mitigation plans for potatoes may benefit regional water supplies. Eddy covariance flux towers played a pivotal role is providing a trusted baseline estimate of ET for both farmers and regulators. Considerations on tower placement, flux footprint, energy imbalance, and maintenance in center-pivot irrigated fields all required careful consideration and quality control.
BG16-A005
Tower-based Eddy Covariance Flux Measurements in Urban Beijing
Yibo HUANGFU1#+, Bin YUAN1, Xianjun HE1, Xiaoxiao ZHANG1, Ziyang LIU1, Thomas KARL2, Martin GRAUS2, Marcus STRIEDNIG2, Min SHAO1
1Jinan University, 2University of Innsbruck
Eddy covariance flux measurements were conducted for reactive gases, including non-methane volatile organic compounds (NMVOCs), ozone, NOx, and ClNO2, as well as greenhouse gases (GHGs) at 102-meter platform at a meteorological tower in Beijing from May to July 2021 and April to June 2023. The footprint climatology (90% contour lines) demonstrates that the measured flux can represent the summer emission characteristics of ~70 km2 of surrounding areas categorized as the typical urban landscape in the megacity of Beijing. Quality control and quality assurance procedure was conducted and the spectrum analysis shows high frequency loss can be neglected. The field campaign in urban Beijing shows that: (1) the different diurnal patterns and constituents between VOCs concentrations and fluxes in general indicates the role of atmospheric aging process; (2) the trends of typical tracer compounds represent the regular patterns and characteristics of sources at multiple timescale; (3) the importance of vehicle-related emissions for NMVOCs emissions was found to be declining, while the demand for eliminating volatile chemical product emissions was increasing; (4) NOx flux exhibited significant temporal and spatial characteristics; (5) natural gas leaks may be the main source of background methane emissions in urban Beijing.
BG16-A003
Enhancing Tropical Peatland Vulnerability Assessments Through Remote Sensing and Carbon Flux Measurements
Nikaan KOUPAEI ABYAZANI1#+, Iuliia BURDUN2, Ankur DESAI1, Kristell HERGOUALC'H3, Takashi HIRANO4, Lulie MELLING5,6, Erin SWAILS3, Angela Che Ing TANG7, Guan Xhuan WONG5
1University of Wisconsin-Madison, 2Aalto University, 3Center for International Forestry Research, 4Hokkaido University, 5Sarawak Tropical Peat Research Institute, 6UN Sustainable Development Sustainable Solution (UN-SDSN Asia), 7University of Toledo
Tropical peatlands are critical stores of carbon (C) and provide various ecosystem services, including C sequestration and flood prevention. However, anthropogenic activities such as drainage has compromised these essential services, turning these ecosystems into net C sources. Soil chamber flux measurements and flux towers have allowed for the monitoring of these C fluxes. Additionally, remote sensing has facilitated the monitoring of not only C fluxes, but also C-dependent variables such as water table level (WTL). In this study, we use in situ WTL measurements from tropical peatlands in Indonesia, Malaysia, and Peru to evaluate the effectiveness of the satellite-based Optical Trapezoid Model (OPTRAM). OPTRAM relies on analyzing the pixel distribution in the shortwave infrared transformed reflectance (STR) and normalized difference vegetation index (NDVI) space to calculate indices, which are then compared to in situ WTL data. We used 30-meter resolution Landsat 7 and Landsat 8 images for model parameterization. We found high and low OPTRAM indices to correspond to high and low WTL, respectively. Our findings also indicate that OPTRAM performs best in capturing tropical peatland temporal WTL dynamics in non-vegetated areas (0.75 < R < 1) using the “best pixel” approach, which selects the pixel with the highest Pearson correlation value. However, in densely vegetated areas, OPTRAM’s performance was notably weaker (~-0.5 < R < 0.5). The integration of OPTRAM and direct C flux measurements holds the potential to enhance peatland vulnerability assessments, including those related to peatland fire risk. In addition, this approach may help in prioritizing areas in need of restoration/management and may aid in mitigating the impact of hazardous haze events.
BG16-A001
Direct Flux Measurements for Immediate Societal Benefits: Simple Explanations, Data Cross-sharing & Weather Station-like Approach
George BURBA#+
University of Nebraska/LI-COR
Continental-scale research infrastructures and flux networks (e.g., AmeriFlux, AsiaFlux, ChinaFlux, ICOS, NEON, OzFlux), as well as numerous smaller GHG flux networks, and individual sites, measure CO2, CH4, and other GHG exchange, as well as water vapor fluxes (evapotranspiration, ET) between ecosystem and atmosphere. After four decades of academic use, the flux stations covered over 2100 stationary measurement locations, and numerous campaigns’ locations. Most measurements were used for process-level ecological and hydrological studies and long-term climate and ecosystem modeling. Such measurements use ultra-high-resolution methodology and state-of-the-art hardware vastly superior to typical monitoring-grade methods and equipment deployed outside academia for a wide range of non-academic decision-making applications. However, despite providing exceptional ways to measure GHG emissions and ET, these are very rarely utilized outside academia. The key reasons for such lack of utilization are: The perceived complexity of the method - can be resolved via simple-language explanations and a detailed guide described in the presentation The lack of data in the specific ecosystem or area and the associated expenses required to establish a new station - can be significantly reduced and often resolved by a peer-to-peer cross-sharing concept outlined in the presentation The absence of a robust overall approach to using flux measurements for immediate societal benefits - can be resolved by adopting an approach currently used by automated weather stations (AWS) feeding and tuning remotes sensing products and resulting in weather modeling and forecasting (see Figure below)The ultimate goal of this presentation is to ignite and provide a base for a discussion regarding the latest needs, ideas, and examples of the use of flux measurements for practical ‘everyday’ decision-making applications benefiting society.
Session Chair(s): Xiaobing ZHOU, Xinjiang Institute of Ecology and Geography, Chinese Academy of Sciences, China
BG03-A004
| Invited
Spatial Variations and Interspecific Differences in Xylem Anatomical Traits of Two Dominant Shrubs in the Desert Region of Northwest China
Yuanming ZHANG#+, Jing ZHANG, Hui SHEN
Chinese Academy of Sciences
Plant hydraulic traits are good predictors of the impact of global change on vegetation dynamics. The xylem anatomical structure is closely related to the efficiency and safety of water transport. In order to better clarify ecological adaptation strategies of desert shrubs, the interspecific and intraspecific variations of xylem anatomical structure were studied. Firstly, ten populations of the dominant shrub Reaumuria soongarica were selected along a west-east transect using an aridity index (AI) ranging from 0.02 to 0.09 in the desert region of northwest China. Based on AI, the sampling sites were divided into arid regions (0.05 ≤ AI < 0.2) and hyper-arid regions (AI < 0.05). Secondly, 5 sampling sites were selected from 10 sampling sites, in which R. soongarica and Calligonum mongolicum were co-distributed. Pearson correlation analysis, linear mixed models, and plant trait networks were used to analyze the spatial variation characteristics and climatic factors of 12 traits in three categories, including xylem anatomical traits, hydraulic functional traits, and mechanical strength. The main results of this study were: (1) high trait variations were observed in the anatomical structure of R. soongarica; (2) mean temperature of the driest quarter was one of the most important climatic factors driving the most trait variation; (3) the patterns of xylem structure traits in response to climate change differed between R. soongarica and C. mongolicum; (4) the trait network analysis results indicated that the central traits of both R. soongarica and C. mongolicum were mean vessel diameters, which was also the central trait in arid regions, but at the transect scale and hyper-arid regions, theoretical hydraulic conductivity was most closely related to other traits. Overall, this study will provide a scientific basis for evaluating the dynamics and stability of vegetation communities in northwest China under climate change.
BG03-A007
| Invited
Revegetation Promotes the Sequestration and Cycling of Soil Carbon and Nitrogen in the Desert Regions, Northern China
Xiaojun LI#+, Haoyu HE, Xinping WANG, Yanxia PAN
Chinese Academy of Sciences
As a key measure to curb desertification and to drive soil carbon (C) and nitrogen (N) cycling, revegetation has been increasingly implemented in drylands worldwide. However, the long-term effects of this restoration practice on the sequestration and cycling of soil C and N, especially the underlying processes remain poorly understood. In this study, soil organic carbon (SOC) and N stocks and their mineralization rates in revegetated sites along a chronosequence in the Tengger Desert were investigated to evaluate the impacts of revegetation. The results showed that revegetation significantly promoted SOC and N accumulation, with the increase rates of 14.25 g C m-2 yr-1 and 2.50 g N m-2 yr-1, respectively. A strong coupling relationship was found between SOC and N stocks. SOC and N sequestration primarily occurred in the upper 0-20 cm soil layer. It would take about 139 and 177 years for SOC and N stocks to reach the original level before degradation. Revegetation facilitates the transformations of SOC and N. Both SOC and N mineralization rates significantly increased with site age, with average mineralization rate of 16.61 mg C kg-1 d-1 and 22.28 mg N m-2 d-1, respectively. Attributional analyses indicated that the dynamic patterns in SOC and N were closely linked to revegetation-triggered changes in biotic and abiotic factors, including plant productivity, soil physico-chemical properties as well as microbial community composition. Our results suggested that the recovery of biogeochemical cycling of C and N is a long-term process, and therefore soil conservation is a key issue in water-limited ecosystems.
BG03-A005
Ecological Restoration in Degraded Land—using Microbial Organic Compound
Shaokun WANG#+, Xueyong ZHAO
Chinese Academy of Sciences
We are facing tremendous land degradation across the whole world, especially in the vulnerable dryland areas. There are about 42 million km2 of land under human-induced desertification. Numerous methods have been applied to combat desertification and many of them received a satisfactory restoration. However, some of the methods are time consuming, some are expensive and some may cause environmental problems. We developed a fast way to restore degraded land using microbial organic compound (MOC). Organic waste from straw and livestock dung were smashed into small pieces and mixed as raw organic compound. Effective cellulose decomposers were inoculated to accelerate the organic compound decomposition. The MOC could be used for degraded land restoration when the fermentation were done in two months. The optimized MOC was significantly efficient in rehabilitating bare sand dunes, accelerating biological soil crust formation, and cropland amendment. The MOC had a potential advantage for increasing water holding capacity, wind erosion resistibility and soil fertility. It is also a potential option to replace the use of chemical fertilizer in cropland. This technique provides an effective and ecological method that aims to accelerate successful restoration from degraded sandy land in the arid and semiarid areas.
BG03-A008
Climate and Human Impact Together Drive Changes in Ecosystem Multifunctionality in the Drylands of China
Xiaobing ZHOU+, Shihang ZHANG, Yongxing LU, Yuanming ZHANG#
Chinese Academy of Sciences
China's drylands encompass an area of approximately 6.60 × 106 km2 and are home to around 580 million people, providing crucial ecosystem services. The escalating impacts of global climate change are expected to exacerbate aridity, thereby adversely affecting ecosystem services and human well–being. Hence, there is a crucial need to prioritize the study of ecosystem multifunctionality (EMF) in drylands and investigate the underlying factors driving EMF changes. We collected field sampling and indoor analysis data, as well as raster level sampling data to obtain indices related to soil nutrients, vegetation, human footprint index (HFI), soil biodiversity index (SBI), and climate (mean annual temperature, MAT; mean annual precipitation, MAP; potential evapotranspiration, PET), and soil characteristics (soil sand content, Sand; soil moisture, SM; soil pH). EMF was calculated using the averaging approach, and the cluster–multi–threshold approach. The findings revealed significant correlations between EMF and all factors except pH and Sand. All factors collectively accounted for 52.7%~57.4% of the variation in mono– (the effect on each of the carbon, nitrogen and phosphorus functions separately) and multifunctionality. The combined effects of all factors had the greatest contribution (8.1%~16.3%) variation in EMF. HFI consistently emerged as the most important factor in controlling EMF variation and proved to be the most significant predictor of EMF changes. All factors examined were significant predictors of EMF change. Our study demonstrated that HFI played the most direct influence on EMF changes, surpassing the impact of any single variable. However, the overall contribution of climate (integrating MAP, MAT, and PET) to EMF change was also extremely important. Therefore, future assessments and predictions of ecological functions in drylands should consider not only the direct effects of climate change but also the integrated analysis of human impact.
BG03-A001
| Invited
The Ecological Significant of Non-rainfall in Revegetation Desert Area, Northwest China
Yanxia PAN#+, Xinping WANG
Chinese Academy of Sciences
Non-rainfall as an additional source of fresh water, may have a positive impact upon the ecosystems in arid and semi-arid zones. It is necessary to understand the formation characteristics and ecological contribution of non-rainfall when managing the shifting sand dune environments. Furthermore, the formation and utilization of non-rainfall water can modulate isotope variation characteristics of the atmosphere, plants and soil water reservoirs. This is especially significant for water resource management in arid desert areas where non-rainfall is an important supplemental water source. In this study, we measured the formation characteristics of non-rainfall in a revegetation stabilized semi-arid shrub desert which passing from a bare soil situation to a vegetated soil of Northwest China. We also analyzed the isotope variation and interaction characteristics of rainfall, non-rainfall, atmospheric water vapor, xylem water, leaf water and shallow soil water during non-rainfall events over two years. The results indicated that non-rainfall primarily formed at 0-3 cm soil layer, which increased surface soil water content, made up for the loss of water evaporation during the day. The presence of biological soil crusts (BSCs) helped to facilitate the formation of non-rainfall, moreover, non-rainfall amount was positively correlated with chlorophyll content in BSCs, which was beneficial to biomass accumulation of BSCs. The isotope analysis results indicated that the non-rainfall water line is close to local meteoric water line, with both having similar origins. Non-rainfall was mainly formed by radiative cooling of evaporated water produced shortly after rain and participated in the local water recycling. The atmospheric, plant and soil water all had high d values which indicated that evaporated water was a significant water source of different water reservoirs in this area. The leaf water of Artemisia ordosica was largely replenished by non-rainfall water compared to xylem water during non-rainfall events, so foliar water uptake was an important survival mechanism for Artemisia ordosica to adapt to drought environment during non-rainfall formation. Non-rainfall water contributed to 8-16% of the xylem water and the less rainfall, the higher the contribution rate. Our results are especially meaningful for arid desert regions where global climate change increases the importance of non-rainfall water.
BG03-A010
Vegetation Evolution and Restoration Characteristics at Inland River Basin in Northwestern Desert Land of China
Duoqing MAN1#, Jinnian TANG1, Yanxia PAN2+
1Gansu Desert Control Research Institute, 2Chinese Academy of Sciences
Through eco-measurement and research at Inland River basin in northwestern desert of China for 60a, it resulted: (1) desert vegetation flora has experienced four main stages from large area of wetland to underground water-table declined substantially; (2) the key populations of Phragmites communis, Tamarix ramosissima and Kalidium foliatum have been deteriorated systemically from meadow vegetation to the desert; Nitraria tangutorum has become into the largest natural population; Artemisia arenaria, Calligonum mongolicum, Zygophyllum xanthoxylum in the rain-fed desert are developing and degrading with precipitation fluctuation;Ephedra przewalskii and Reamuria soongorica which belong to the super-xerophyte have been developing in the deteriorated process; (3) with rain-fed area enlargement, desert herbal plants grow when precipitation was higher in the year, the plant diversity and coverage increased, and vice versa; some desert shrubs were relatively stable, its population improved when precipitation was over 140 mm, 100-140 mm for basic growth, and <100 mm degraded gradually; (4) most man-made plant species of windbreak and sand-fixation afforestation degraded under drought development, Haloxylon ammodendron had strong eco-adaptability as an introduced species, it has developed into the biggest windbreak and sand-fixation shrub forest, its big density and land drought were the main reasons for degradation, and sustainability could be improved under low density afforestation according to local plant carry capacity; (5) recent 20 years, with the integrated program implementation in the inland River basin, eco-water has been increased, underground water table has recovered in some desert surroundings, some micro-wetlands have formed, original desert meadow steppe and sandy land vegetation has restored again, and their ecosystems are developing positively; however, underground water table still reduces slowly in most areas, desertification has still developed.
BG03-A009
Plant Biomass Dynamics in a Desert Ecosystem, NW China: Present Condition and Climate Change Scenarios
Xinping WANG#+
Chinese Academy of Sciences
The temporal dynamics of vegetation biomass are of key importance for evaluating the sustainability of arid and semiarid ecosystems. In these ecosystems, biomass and soil moisture are coupled stochastic variables externally driven, mainly, by the rainfall dynamics. Based on long term field observations in northwestern (NW) China, we test a recently developed analytical scheme for the description of the leaf biomass dynamics undergoing seasonal cycles with different rainfall characteristics. The probabilistic characterization of such dynamics agrees remarkably well with the field measurements, providing a tool to forecast the changes to be expected in biomass for arid and semiarid ecosystems under climate change conditions. These changes will depend - for each season - on the forecasted rate of rainy days, mean depth of rain in a rainy day, and duration of the season. For the site in NW China, the current scenario of an increase of 10% in rate of rainy days, 10% in mean rain depth in a rainy day, and no change in the season duration leads to forecasted increases in mean leaf biomass near 25% in both seasons.
Session Chair(s): Yoori CHO, Climate Tech Center
BG04-A005
| Invited
Phenological Mismatch Between Bumble Bees and Alpine Plants
Gaku KUDO#+
Hokkaido University
Global warming affects seasonal events of various organisms and the phenological modifications may disturb the relationships among coexisting species. Symbiosis between plants and pollinators is the most important ecosystem service in the terrestrial ecosystems. In alpine ecosystems, bumble bees (Bombus spp.) are the most effective pollinators for many alpine plants. Thus, it is crucial to clarify how phenological modifications in bumble bees and alpine flowers affect the pollination symbiosis in the alpine ecosystems. The present study reports the mechanism of phenological mismatch between bee activity and flowering time of alpine plants in northern Japan. Observations of worker-bee abundance and flowering phenology over 12 years revealed that both of the flowering time and worker bee abundance highly varied from year to year. Flowering phenology of alpine-snowbed communities was strongly determined by the variation in snowmelt time, whereas the peak season of worker bees was relatively stable among years independent of weather and snowmelt conditions. As a result, phenological mismatch between worker bees and alpine flowers was intense in early-snowmelt years. Factors affecting the abundance of worker bees varied among bee species. Worker abundance of a typical alpine species was negatively influenced by the acceleration of snowmelt time and the phenological mismatch in the previous year. In contrast, worker abundance of subalpine species, i.e., overwintering and/or nesting at subalpine habitat and using alpine habitat for flower foraging, was independent or even positively influenced by the phenological mismatch. Hot summer was negatively related to the worker abundance in every species. These results suggest that global warming may decrease the foraging activity of bumblebees, especially for typical alpine bees, and may change the species composition of bumble bees in alpine ecosystems. Thus, the pollination symbiosis in the alpine ecosystems may be decayed by climate change.
BG04-A013
Estimation of the Flowering Period of Three Honey Tree Species Using Satellite Data
Minsu LEE1+, Sukyung KIM1, Kyu Rang KIM2, Hyun-Seok KIM1#
1Seoul National University, 2National Institute of Meteorological Sciences
In recent years, the global warming and climate change have resulted in shifts in flowering phenology. The flowering timing of honey tree species also has been changed, and it caused to decrease honey production and impact economic loss to beekeepers. Consequently, there is a need for updated phenological information on these honey tree. However, collecting field data on the flowering periods of various honey trees is a labor-intensive and costly endeavor. In this study, we utilized Harmonized Landsat Sentinel (HLS) satellite data from 2017 to 2022 to investigate flowering period of three species (Robinia pseudoacacia, Liriodendron tulipifera, Castanea crenata) recommended by Korea Forest Service as honey sources to assess the potential for utilization of satellite data to provide valuable phenological information on honey tree species. We calculated seasonal flowering index to observe the trend of the index and estimate the flowering periods. The results show that the trend that the index increased during the flowering period and then decreased afterward. As a result, we estimated the DOY 109-129 and DOY 129-159 for the flowering timing of R. pseudoacacia and L. tulipifera, respectively, which is similar to the generally known flowering periods for R. pseudoacacia (May to June) and L. tulipifera (June to July). And the case of C. crenata, we estimated DOY 168-191 for the flowering time which is similar to the generally known flowering periods of the chestnut tree (June to July). Therefore, we utilized the Harmonized Landsat and Sentinel satellite data to observe color and brightness changes during tree flowering stages. However, this method is needed to solve data loss issues and improve resolution.
BG04-A001
| Invited
STSMF - A Spatiotemporal Shape Model Fitting Method for Within-season Crop Phenology Detection
Ruyin CAO#+
University of Electronic Science and Technology of China
Crop phenological information must be reliably acquired earlier in the growing season to benefit agricultural management. Although the popular shape model fitting (SMF) method and its various improved versions (e.g., SMF by the Separate phenological stage, SMF-S) have been successfully applied to after-season crop phenology detection, these existing methods cannot be applied to within-season crop phenology detection. This discrepancy arises because the principle of optimizing curve matching in after-season phenology detection is inapplicable to the within-season scenario. To resolve this issue, a new method named spatiotemporal shape model fitting (STSMF) was developed. STSMF does not seek to optimize the local curve matching between the target pixel and the shape model; instead, it determines similar local VI trajectories in the neighboring pixels of previous years. The within-season phenology of the target pixel was thus estimated from the corresponding phenological stage of the determined local VI trajectories. When compared with ground phenology observations, STSMF outperformed the existing SMF and SMF-S which were modified for the within-season scenario (SMFws and SMFSws) with the smallest mean absolute error. The MAE values averaged over all phenological stages for STSMF, SMFSws, and SMFws were 9.8, 12.4, and 27.1 days at winter wheat stations; 8.4, 14.9, and 55.3 days at corn stations; and 7.9, 12.4, and 64.6 days at soybean stations, respectively. Intercomparisons between after-season and within-season regional phenology maps also demonstrated the superior performance of STSMF (e.g., correlation coefficients for STSMF and SMFSws are 0.89 and 0.80 at the maturity stage of winter wheat). Furthermore, the performance of STSMF was less affected by the detection time and the determination of shape models. In conclusion, the straightforward, effective, and stable nature of STSMF makes it suitable for within-season detection of agronomic phenological stages.
BG04-A017
The Phenological Eyes Network (PEN): A Journey Through Two Decades and the Future Vision of Long-term Phenology Monitoring
Taiga SASAGAWA1#+, Kenlo NASAHARA2
1Chiba University, 2University of Tsukuba
The Phenological Eyes Network (PEN) is an observation network for long-term vegetation dynamics, established in 2003 by a group of terrestrial remote sensing scientists. PEN has collected, archived, and published a large number of datasets about vegetation dynamics for more than twenty years. PEN provides informative datasets for the interpretation of optical satellite remote sensing data for ecosystem monitoring, including time-lapse photos of vegetation, spectral information of canopy, and atmospheric parameters, utilizing three main observation instruments: time-lapse cameras, spectroradiometers, and sky radiometers, respectively. In this presentation, we will review PEN’s achievements and contributions to the research community, mainly focusing on time-lapse photos and spectral information. Then, we will introduce a new observation system utilizing Raspberry Pi: a series of small, low-cost, and single-board computers. For instance, we will present a cost-effective yet high-quality time-lapse camera for Raspberry Pi as an alternative to our existing cameras with some examples. Moreover, we will also share a new observation scheme, like sound phenology using microphones and phenology of water content using microwave signals with GNSS receivers. Through this presentation, we hope for a new collaboration for the next twenty years of phenology observation.
BG04-A008
Application of KOPHEN Data for Phenology Research
Sangji LEE+, Sujong JEONG#, Jaewon SHIN, Jongho KIM
Seoul National University
The Korean Phenology Network (KOPHEN) has been established with the primary objective of comprehending adaptation mechanisms within biospheres, elucidating interactions, and forecasting prospective phenological changes under the influence of climate change. A fundamental aspect of realizing this overarching goal involves the integration of diverse scientific analyses derived from real observation data. Various methods are employed to monitor plant phenology; each approach has its own advantages and can complement others that may be overlooked. As an initial step towards this goal, we seek to proposes effective monitoring methods that combines two different scales of observation methods for the ongoing plants growing seasons: human field observations and satellite observations. We have been accumulating data over an extended period, involving continuous human field observations for 256 plant species in Korea since 2009. Additionally, we have calculated the start and end of the season using satellite data for the same duration. Specifically, the assessment of changes in the length of the growing season (LOS) comparing a decade (2014~2023) of human field observation data on deciduous broadleaf trees with MODIS NDVI.KOPHEN is planning further expansion of multi-scale initiatives, encompassing regional-scale monitoring through the utilization of pheno-cams and drones. By striving to integrate a broader spectrum of data sources, KOPHEN aims to enhance the confidence of status identification and prediction to plant phenological shifts. These efforts will help to utilize observational data more diversely to understand biosphere interactions and promote effective response to climate change.
BG04-A014
Comparison of Diverse Methods for Extracting Phenological Stages of Quercus Mongolica and Pinus Densiflora Using Digital Camera Images
Sukyung KIM1#+, Minki HONG2, Jeong-Soo PARK2, Hyun-Seok KIM1
1Seoul National University, 2National Institute of Ecology
Changes in plant phenology demonstrate profound impact of climate change on ecosystems. However, monitoring phenology requires time and effort. The monitoring system using digital cameras is widely utilized as an approach to complement the spatiotemporal limitations of direct observation or satellite-based remote sensing. Based on six years of digital image data, we quantified seasonal greenness changes (Green chromatic coordinate, Gcc) of two species (Quercus mongolica and Pinus densiflora) on Mt. Jeombong, and estimated phenological stages: the start (SOS) and end (EOS) of season. Comparison of phenophases estimated using five types of fitting functions (one cubic spline function and four different double logistic functions) and five extraction methods (two derivative-based methods, two threshold methods, and a curvature method) revealed that, for both species, the type of extraction method had a greater effect than the type of fitting function on SOS and EOS. On average, the curvature method estimated the earliest SOS and the latest EOS. As a result, the length of season (LOS) estimated by curvature method was at least 40 days longer for Q. mongolica, and 65 days longer for P. densiflora when compared to the 50th percentile threshold method and the first-derivative method. The variance between extraction methods was consistently larger than the interannual variance in phenophases, indicating that RGB image-based vegetation indices could overestimate or underestimate the physiological active period of vegetation by the extraction method. Therefore, it is essential to cross-validate phenophase extraction methods for different vegetation types utilizing multiple sources such as eddy covariance flux, leaf area index, and hyperspectral characteristics.
BG04-A015
| Invited
Climate Change Impacts on Grassland Phenology, Diversity and Pollen Exposure
Alfredo HUETE1#+, Ha NGUYEN2, Janet DAVIES3, Nikul KUMARI1, Paul BEGGS4
1University of Technology Sydney, 2Commonwealth Scientific and Industrial Research Organisation, 3Queensland University of Technology, 4Macquarie University
Climate warming and extreme weather events are altering the functioning and composition of terrestrial ecosystems with consequences for ecological processes, food security, and human health. Knowledge of phenology patterns over much of the Southern Hemisphere, including Australia, is sparse, and there is a lack of understanding of the key factors driving spatial and temporal shifts in phenology responses. In this project, we investigated how climate change is altering the phenology, plant diversity, and airborne pollen exposure in Australia's rainfed grasslands, currently experiencing both long-term climate warming and climate drying trends. We aimed to answer key questions on climate-driven shifts in grassland phenology and associated reproductive and pollen phenology. We also sought to determine how climate drying impacted on grass plant and grass pollen relationships. We combined satellite-derived grassland phenology timing and grass productivity (biomass) analyses with in situ aerobiome analyses of grass pollen concentrations and diversity, and in situ measures of greenness amount and timing from phenocams. Our study areas encompassed temperate C3 grasslands, tropical C4 grasslands, and transitional C3/C4 grassland sites. Preliminary results show that in temperate sites, there are clear advancing phenologies of both the grass growing and grass pollen seasons, coupled with declining grass biomass and grass pollen concentrations. By contrast, in mixed grassland and tropical sites, there were no clear advances in phenology and patterns were much more complex and dependent on grass diversity. In general, inter-annual trend relationships between grass and pollen phenologies were strong and became weaker at finer annual and seasonal scales. The expected outcomes of this ongoing project will be better management options to safeguard allergy sufferers and improved ecological and pollen forecasts under climate change. This will provide important public health benefits and disease mitigation strategies to Australia's urban and remote areas.
BG04-A016
Vegetation Canopy Structure Mediates the Response of Gross Primary Production to Environmental Drivers across Multiple Temporal Scales
Yaoyao ZHENG1+, Weiqing ZHAO1, Anping CHEN2, Yue CHEN1, Jiana CHEN1, Zaichun ZHU1#
1Peking University, 2Colorado State University
Gross primary production (GPP) is a critical component of the global carbon cycle and plays a significant role in the terrestrial carbon budget. The impact of environmental factors on GPP can occur through both direct (by influencing photosynthetic efficiency) and indirect (through the modulation of vegetation structure) pathways, but the extent to which these mechanisms contribute has been seldom quantified. In this study, we used structural equation modeling and observations from the FLUXNET network to investigate the direct and indirect effects of environmental factors on terrestrial ecosystem GPP at multiple temporal scales. We found that canopy structure, represented by leaf area index (LAI), is a crucial intermediate factor in the GPP response to environmental drivers. Environmental factors affect GPP indirectly by altering canopy structure, and the relative proportion of indirect effects decreased with increasing LAI. The study also identified different effects of environmental factors on GPP across time scales. At the half-hourly time scale, radiation is the primary driver of GPP. In contrast, the influences of temperature and vapor pressure deficit take on greater prominence at longer time scales. About half of the total effect of temperature on GPP is indirect through the regulation of canopy structure, and the indirect effect increases with increasing time scale (GPPNT-based models: 0.135 (half-hourly) vs. 0.171 (daily) vs. 0.189 (weekly) vs. 0.217 (monthly); GPPDT-based models: 0.139 vs. 0.170 vs. 0.187 vs. 0.215; values reported in gC m-2 d-1 °C-1, P<0.001); while the indirect effect of radiation on GPP is comparatively lower, accounting for less than a quarter of the total effect. Furthermore, we observed a direct, negative-to-positive impact of precipitation on GPP across timescales. These findings provide crucial information on the interplay between environmental factors and LAI on GPP and enable a deeper understanding of the driving mechanisms of GPP.
BG04-A002
Increasing Gross Primary Productivity Under Soil Warming and Wetting on the Tibetan Plateau
Qing PENG1+, Binghao JIA1#, Xin LAI2, Longhuan WANG1, Qifeng HUANG2
1Chinese Academy of Sciences, 2Chengdu University of Information Technology
The soil freeze-thaw process has undergone significant changes on the Tibetan Plateau (TP) in the context of global change, resulting in the changes of soil physical and chemical properties, thereby affecting the vegetation phenology and photosynthesis through affecting the utilization capacity of CO2 and light by vegetation. However, little is known about how soil temperature (ST) and soil moisture (SM) affect the gross primary productivity (GPP) on the TP at different seasons and elevations. In this study, the spatiotemporal variation patterns of GPP, ST, and SM were analyzed based on the Community Land Model version 5.0 (CLM5.0) simulations in order to illustrate the impacts of ST and SM in surface (0–10 cm) and root zone soil (0–100 cm) on GPP between 1979 and 2020. The results showed that the CLM5.0-based GPP and ST were in good agreement with in situ observations. ST, SM and GPP increased at the rates of 0.04 ℃ a−1, 2.4 × 10−4 mm3 mm−3 a−1, and 5.36 g C m−2 a−2, respectively. SM dominated the variations of GPP in winter (64.3%), while ST almost was the dominant factor in other periods, especially spring (99.9%) and autumn (94.7%). The explanatory power of ST and SM for GPP increased with elevation, especially for ST. The relative contributions of ST and SM to GPP at different time scales in root zone soil were similar to those in surface soil. This study provided a new understanding of how soil freeze-thaw affected GPP changes on the TP in the context of the intensification of warming and humidification.
BG04-A012
The Direct and Indirect Effects of the Environmental Factors on Global Terrestrial Gross Primary Productivity Over the Past Four Decades
Yue CHEN1+, Zaichun ZHU1#, Weiqing ZHAO1, Muyi LI1, Sen CAO1, Yaoyao ZHENG1, Feng TIAN1, Ranga MYNENI2
1Peking University, 2Boston University
Gross primary productivity (GPP) is jointly controlled by the structural and physiological properties of the vegetation canopy and the changing environment. Notable changes in global GPP in recent decades have been attributed to dramatic environmental changes. Environmental changes can affect GPP by altering not only the biogeochemical characteristics of the photosynthesis system (direct effects) but also the structure of the vegetation canopy (indirect effects). However, comprehensively quantifying the multi-pathway effects of environmental change on GPP is currently challenging. We proposed a framework to analyse the changes in global GPP by combining a nested machine-learning model and a theoretical photosynthesis model. We quantified the direct and indirect effects of changes in key environmental factors (atmospheric CO2 concentration, temperature, solar radiation, vapor pressure deficit (VPD), and soil moisture (SM)) on global GPP from 1982 to 2020. The results showed that direct and indirect absolute contributions of environmental changes on global GPP were 0.2819 Pg C yr-2 and 0.1078 Pg C yr-2. Direct and indirect effects for single environmental factors accounted for 1.36%−51.96% and 0.56%−18.37% of the total environmental effect. Among the direct effects, the positive contribution of elevated CO2 concentration on GPP was the highest; and warming-induced GPP increase counteracted the negative effects. There was also a notable indirect effect, mainly through the influence of the leaf area index (LAI). In particular, the rising VPD and declining SM negatively impacted GPP more through the indirect pathway rather than the direct pathway, but not sufficient to offset the boost of warming over the past four decades. We provide new insights for understanding the effects of environmental changes on vegetation photosynthesis, which could help modelling and projection of the global carbon cycle in the context of dramatic global environmental change.
Session Chair(s): Detchphol CHITWATKULSIRI, Kasetsart University, Channa RAJANAYAKA, Earth Sciences New Zealand, Kei NAKAGAWA, Nagasaki University, Kenichiro KOBAYASHI, Saitama University, Hitoshi MIYAMOTO, Shibaura Institute of Technology
HS16-A010
| Invited
Current Status of Disaster Emergency Wells in Japan and the Disaster Resilience Function of Groundwater
Takahiro ENDO#+
Osaka Metropolitan University
The objective of this study is to derive policy lessons based on the current status and practical examples of disaster emergency wells in Japan. Disaster emergency well is an institution where local wells are opened to nearby residents for drinking and domestic purposes in the event of disasters such as earthquakes or floods to cope with water outage. Some wells are registered in advance, while others are spontaneously opened after disasters. Among registered wells, some are installed by local governments, but many are privately owned by individuals, including residents, factories, and commercial facilities. The provision of groundwater is not mandatory and is left to the discretion of well owners. Therefore, disaster emergency well is characterized as an institution for mutual assistance. While the importance of groundwater during water outage after disasters has been frequently highlighted in newspapers, the adaptation status of disaster emergency well across Japan and how local wells were actually used in the event of disaster has remained unscrutinized. Consequently, this study utilizes Japan's statutory plan, the Municipal Disaster Prevention Plan, to reveal the nationwide distribution of municipalities that have already implemented a system of disaster emergency well. Furthermore, case studies are presented to elucidate the effectiveness of groundwater use during disasters and its limitations. Although underground water has traditionally been valued as an industrial, scenic, and environmental resource, this study adds its usefulness as a disaster prevention resource.
HS16-A016
Groundwater Trend Analysis for Enhanced Water Resource Resilience
Channa RAJANAYAKA1#+, Kei NAKAGAWA2, Jing YANG3, Eqin ZHAO2
1Earth Sciences New Zealand, 2Nagasaki University, 3National Institute of Water and Atmospheric Research
The intensifying water demands present unprecedented challenges for water resource management, underscoring the need for a comprehensive understanding of groundwater dynamics to ensure sustainable groundwater allocation. This imperative becomes even more crucial in regions anticipated to endure prolonged dry periods due to climate change, where groundwater is essential for sustaining baseflow and supporting instream ecosystems. Groundwater trend analysis plays a pivotal role in understanding and addressing the complexities of water resource sustainability. By systematically evaluating long-term groundwater level data, patterns, and fluctuations, along with associated systems such as climate, groundwater recharge, river flows, land use changes, sea level rise and water abstractions, decision-makers gain valuable insights into the aquifer's response to various stressors. Understanding the trends enables proactive planning and management strategies to mitigate the adverse effects of over-extraction, land-use changes, and climate-induced variations. Here we have developed a methodology based on statistical methods, conceptual modelling methods and spectral analysis, aiming to assess long-term groundwater trends and attribute any changes in long-term groundwater to climate and anthropogenic activities within the catchment. This method has been applied in two catchments with different climate and hydrogeological settings, one in New Zealand and the other in Japan. Through the application of the developed methodology under diverse climatic conditions, land use patterns, and water management regulatory systems, this presentation explores the critical importance of conducting groundwater trend analysis as a fundamental tool to support sustainable water allocation. The applications of this developed approach extend to supporting sustainable groundwater resource development and management, contributing to the resilience of social, economic, and ecological requirements for various water users.
HS16-A003
Urban Evapotranspiration and Its Effects on Water Budget and Energy Balance Under Global Warming: Review and Perspectives
Guo Yu QIU#+
Peking University
Urban evapotranspiration (ET) is one of the most important components of water and energy balance, and carbon cycle in urbans. It is also a natural process that is powerful enough to possibly mitigate the negative effects caused by urbanization and global warming. Increasing or regulating urban ET could possibly be a solution to overcome the negative impacts caused by urbanization and global warming. Since 2000, researches on urban ET have been increasing and significant progresses have been achieved. A review of these progresses will certainly further promote the related researches and social practices. Therefore, this study reviewed almost all the published papers on urban ET over the world, summarized its current progresses, scientific understandings, and forecasted the possible challenges in the future. Results achieved from this review would be helpful to use the power of ET to improve the livability of cities, guide the practices of sponge city construction and low impact development, mitigate the negative effect of urban heat island, and reduce urban carbon emission.
HS16-A012
Exploring the Crucial Role of Flow Naturalisation in Formulating Water Allocation Policies
Channa RAJANAYAKA1#+, Jing YANG2, Doug BOOKER2, Rachel SMITH2
1Earth Sciences New Zealand, 2National Institute of Water and Atmospheric Research
The hydrological cycle in numerous catchments worldwide has undergone significant modifications due to human activities. These alterations include the impoundment of rivers, creation of water diversions, and the discharge of irrigation, effluent, and treated wastewater into both land and water. Changes in land use and water extractions further contribute to this transformation. Measured flows in these catchments do not accurately represent natural flows due to anthropogenic influences. Consequently, directly measuring natural flows is unfeasible and necessitates estimation. Despite this challenge, estimating naturalised flows is crucial for various purposes, such as water allocation, resources management, ecological flow settings, impact assessments for consented activities, and evaluations of climate change impacts. Relying on altered measured flows for policy development may result in spatial and temporal unfairness in the treatment of the environment and water users. To address the challenge of altered surface and groundwater due to human activities, we have developed a framework for flow naturalisation. This framework comprises three components: data collection and analysis, flow alteration modelling from surface and groundwater abstraction/diversion, and flow naturalisation. The data collection and analysis involve gathering surface/groundwater abstraction and measured streamflow data, along with quality assurance/checking of data. Flow alteration modelling employs a streamflow depletion model and river routing model to estimate the spatial and temporal effects of surface/groundwater abstraction on streamflows. Finally, flow naturalisation combines measured streamflow and altered streamflow into a representative naturalised flow. This framework has been implemented in a user-friendly web-based tool. The presentation will demonstrate the significance of flow naturalisation as a pivotal component in developing river flow allocation policies, using a New Zealand case study as an illustrative example. We anticipate that this framework and tool will provide valuable support for water allocation management in catchments where natural flows have been modified by human activities.
HS16-A005
Characteristics of Inland Water Chemistry in New Zealand
Kei NAKAGAWA1#+, Hiroki AMANO2, Channa RAJANAYAKA3, Jing YANG4
1Nagasaki University, 2Tokai University, 3Earth Sciences New Zealand, 4National Institute of Water and Atmospheric Research
To address and adapt to the future climate change impacts on New Zealand’s primary sector, there is a growing need for increased irrigation. The intensification of livestock farming in recent years has led to water pollution issues, particularly from animal waste. In view of these concerns, it is crucial to study the status of inland water characteristics. In November 2023, water samples were collected from 33 sites of groundwater, and surface water from rivers, streams, lakes, pond, and dam in both the North and South islands of New Zealand to investigate the water chemistry characteristics. Water samples were stored in 50-100 ml plastic bottles and were analyzed for major dissolved ions in a laboratory. One sample showed a strongly acidic condition, posing challenges in achieving a charge balance error with measured ions only. This suggests potential pollution from heavy metal or other cations. The characteristics of water chemistry, excluding this particular sample, were assessed using a Piper trilinear diagram and Stiff patterns using major ions concentrations. According to the trilinear diagram, the majority of sites (62.5%) were classified as alkaline earth carbonate type, 8 sites (25.0%) as alkali non-carbonate type, two sites (6.25%) as alkaline carbonate type, and two sites (6.25%) alkaline earth non-carbonate type. The Stiff patterns show Ca-HCO3and Na-HCO3 types in most of the sites, and Na-Cl type was found in the specific location of the coastal area. One site, situated on the peninsula hill, appeared to be affected by flying salt from the sea. The pH levels of the samples ranged from 5.83 to 8.21, with a mean of 7.19, indicating that the inland water is slightly acidic to slightly alkaline. EC varied from 1.5 to 355.0 mS/m, with a mean of 24.1 mS/m. Self-organizing maps demonstrated diverse water quality characteristics across the sample sites.
HS16-A013
A Deep Learning Image Measurement System for Floating River Waste in Urban Canals of the Chao Phraya River Basin, Thailand
Maiyatat NUNKHAW1#+, Detchphol CHITWATKULSIRI2, Hitoshi MIYAMOTO1
1Shibaura Institute of Technology, 2Kasetsart University
River floating waste has become an emergent aquatic environmental issue since it could be a major source of ocean microplastic pollution problem. Currently, in many developing countries, e.g., Thailand in Southeast Asia, the river floating waste has not yet been fully managed due to the lack of an appropriate in-situ measurement system. Accurate field measurement of the waste outflows from rivers and streams to the coastal seas would be essential to tackle this issue. In this study, we assessed the applicability of a deep-learning image measurement system of river floating waste to urban canals in the Chao Phraya River basin. The image measurement system combined two deep-learning techniques, YOLOv5 and DeepSORT, to classify and track the river floating waste. The classes classified in this study were as follows: cans, cartons, plastic bottles, foams, glasses, papers, and plastics. The deep-learning parameters were fine-tuned using in-situ camera images obtained through the websites of administrative bodies in Bangkok, Thailand. The results of the waste classification showed that the mAP (mean Average Precision) of cans, cartons, plastic bottles, foams, glasses, papers, and plastics were 77, 73, 82, 69, 73, 72, and 71%, respectively. It would achieve an accuracy high enough to classify each waste class in the real river fields compared to the previous laboratory examination for the system development. Misclassifications also existed, e.g., in forms and plastics, due mainly to the waste degradation in the real river environment. Future research will focus on improving the current system, particularly reducing misclassifications of degraded waste.
HS16-A001
| Invited
Patch Size Effect of Submerged Aquatic Vegetation on Sedimentation
Keisuke NAKAYAMA1#+, Keita MATSUMURA1, Hiroki MATSUMOTO2, Tetsuya SHINTANI3
1Kobe University, 2Port and Airport Research Institute, 3Tokyo Metropolitan University
Submerged aquatic vegetation (SAV) provides critical ecosystem services in lakes and the coastal ocean, providing a nursery and habitat for various organisms. They can accumulate carbon and particulate organic matter and produce oxygen essential to ecosystem services, providing a nursery and habitat for various organisms. SAVs generally exist entirely in shallow water areas and grow in patches, meaning their interactions with waves and currents may induce complexity for mass transport. For instance, the more the SAV's blade bends, the more significantly the sediment accumulates. Therefore, this study uses the SAV model to investigate the effect of patch size on sedimentation by SAV meadows. Also, we conducted laboratory experiments to validate the SAV model. Particle image velocity (PIV) was used to measure velocities inside the SAV meadow in the laboratory. As a result, the SAV numerical model was successfully applied to simulate flows around a patched SAV meadow, and the results agreed with those of the laboratory experiments. The model showed that the SAV bent considerably, and the velocity adjacent to the bottom became slower when the elasticity was smaller. The patch occupancy of the channel width was revealed to be the most substantial factor in controlling sediment accumulation.
HS16-A015
Development of SPH-based Fluid-structure Interaction Model and Applications to Coastal Problems
Yoshiki TAKAMI+, Tetsuya SHINTANI#
Tokyo Metropolitan University
In this study, we developed a fluid-structure interaction numerical model based on the Smoothed Particle Hydrodynamics (SPH) method to analyze the complex waves and currents around deformable elastic obstacles such as wave dissipation blocks. We first focused on the method of neighboring search, wall representation and collision of particles to understand the differences appeared in in previous studies. We then proposed an improved solid-fluid interaction strategies which enables the stable calculation of a solitary wave generation and frictional force between solids to be applicable to realistic coastal problems. With these modifications, the present model was successfully developed that can account for floating, tipping, and sliding of solid bodies involving multiple structure interactions. Secondly, we carefully selected the effective radius, weight function and the equation of state to maintain stability and accuracy for calculations accompanying local high pressure and narrow particle spacing which will be required to analyze permeable breakwaters. To validate the accuracy of the present model, we simulated the two different types of phenomena which were tested in previous investigations using laboratory experiments: (1) dam-break wave problem (fluid only), and (2) interactions between an elastic plate and fluid. The results of the former test case demonstrated the accurate prediction of gravitational flow. For the latter verification, the present model also showed reasonable accuracy of less than 5% difference from the experimental data for the maximum displacement of the elastic plate and the temporal evolution of surface level. The present model is currently intended to be used for the design of coastal wave dissipating blocks, realizing the effective wave absorption, beautiful landscape and safety.
HS16-A018
Efficient Numerical Simulation by Lattice-Boltzmann Method with Adaptive Mesh Refinement
Tsuyoshi KASAHARA+, Tetsuya SHINTANI#
Tokyo Metropolitan University
Predicting and analyzing phenomenon such as tsunami and flooding are important for preventing our life from disaster. Numerical simulation is obviously effective approach for this purpose and recently the Lattice-Boltzmann Method (LBM) attracts attentions for its simplicity and high parallelization performance. LBM approximates the fluid as collections of virtual particles in computational cell and calculates velocity field from particle distribution varying through collision and propagation processes of the particles. Although LBM is computationally efficient, the efficiency still further needs to be improved for large-scale phenomenon. Therefore, in this study, we applied Adaptive Mesh Refinement (AMR), an efficient grid generation strategy, to LBM for efficient analysis. AMR changes grid resolution locally and temporally, increasing grid resolution where requires high accuracy, while decreasing resolution the other area to obtain high efficiency. In this study, to test the accuracy and efficiency of the AMR implementation for LBM, the three-dimensional dam-break problem with an obstacle was chosen. In this analysis, two different levels of grid resolution was used in the case of AMR, while the finest resolution of AMR was used for the uniform resolution case. As the validation, we compared the variation of water level at specific point and pressure at obstacle with the experimental result of a previous study. For the temporal variation of the water level, the uniform resolution case generally showed good results compared to the experimental value, while the case of the AMR showed a slight time delay compared to the experimental value and represented its feature. For the pressure, both cases of uniform and AMR well represented maximum experimental pressure. Lastly, we compared the computational cost between the uniform and AMR cases and found that the number of total grids and computational time in the AMR case was 1/4 of that in the uniform case.
HS16-A009
Deep Learning Model Refinement with Empirical Mode Decomposition for Groundwater Level Prediction in Kushiro Wetland, Hokkaido, Japan
Hitoshi MIYAMOTO1#+, Takumi YAMAGUCHI1, Yudai NEMOTO1, Tetsuya OISHI2,3
1Shibaura Institute of Technology, 2Public Works Research Institute, 3Civil Engineering Research Institute for Cold Region
Developing groundwater level prediction models is of fundamental importance in wetland restoration assessment. This study improved a deep learning model to predict groundwater level time series before and after river meander restoration for a nature restoration project in Kushiro Wetland in Hokkaido, Japan. This study introduced itEMD (iterative empirical mode decomposition) as a data preprocessing method in deep learning refinement. The data used for deep learning was the itEMD modes decomposed into three frequency bands with different fluctuation characteristics. Then, a CNN (convolutional neural network)-based deep learning model, itEMD-CNN, was constructed for each mode. The daily mean data for model training were groundwater level, precipitation, air temperature, sunshine hours, deepest snow cover depth, NDVI (normalized vegetation index), and river discharge for four field survey sites for six years before and after river meander restoration, respectively. Model refinement results showed that the itEMD-CNN model improved the prediction performance compared to the simple LSTM (long short-term memory) model in the previous study by an average of 15.6% and a maximum of 39.7% in R2 (coefficient of determination) and by an average of 2.2 cm and a maximum of 4.8 cm in RSME (root mean square error). These results strongly supported the effectiveness of the present itEMD-CNN model, which can accurately predict groundwater levels even with a limited amount of learning data.
Session Chair(s): Hung Soo KIM, Inha University
HS02-A003
Integrated Framework for Assessing Watershed Vulnerability Under Climate Changes and Human Impacts
Yu LI+, Xiang FU#, Zhipeng FAN
Wuhan University
The inescapable impacts of climate change on hydrologic flooding and droughts necessitate strategic interventions. Human activities, including water use, reservoir operations and inter-basin water transfers, have complex interactions with hydrologic conditions. However, existing methodologies lack an integrated framework that considers both future climate scenarios and human interventions. Utilizing the open-source Spatial Processes in Hydrology (SPHY) model, our research introduces an integrated framework for large basin-scale hydrologic modeling, focusing on four large adjacent basins in China. Our approach extends beyond conventional practices by incorporating future climate projections and human activities simulation. Specifically, we refine the water use and reservoir operation modules within the SPHY model. After calibration of historical conditions, based on Coupled Model Intercomparison Project Phase 6 (CMIP6) General Circulation Models (GCMs), this framework was utilized to assess the combined impacts of future climate conditions and reservoir operations on the hydrologic system at large basins scale. The developed framework aims to enhance our understanding of the complex interactions within large basins, enabling a holistic assessment of watershed exposure, vulnerability, and risk within large basins, and provide critical data references for inter-basin water transfer projects.
HS02-A006
Meteorological Drought Severity Classification Considering Emergency Water Supply Scale and Future Drought Projections Based on SSP Scenarios
Seungmin LEE+, Hyeonbin AHN, Kyunghun KIM, Soojun KIM, Hung Soo KIM#
Inha University
Various drought indices have been used to quantitatively define the severity of drought, which causes enormous damage worldwide. The Standardized Precipitation Index (SPI) has been used to quantify the severity of meteorological drought. However, since the SPI is calculated using precipitation only, there are limitations in quantifying and classifying drought severity. Therefore, this study proposed the Drought Severity Classification Index (DSCI) to overcome the limitations of SPI by using meteorological data such as precipitation, temperature, wind speed, humidity and so on and the drought damage scale from emergency water supply. We also analyzed the trend of future drought severity using the Social-Shared Pathway (SSP) scenarios. Historical data of emergency water supply and meteorological data were used as input data and weights calculated by the genetic algorithm were applied to estimate the DSCI. In addition, we used a cumulative distribution function of the estimated DSCI to classify drought severity. The comparison of drought severity classification of the DSCI and SPI showed that DSCI classifies the drought severity more accurately. Using three SSP scenarios (SSP1-2.6, SSP2-4.5, SSP5-8.5), we analyzed the future changes in drought severity based on the DSCI. These results could be used as a reference for establishing future strategies or directions for future drought management planning and policy.
HS02-A001
Is Holistic Bias Correction in Climate Model Simulations Feasible? – Insights from Time-frequency-based Bias Correction Approach
Cilcia KUSUMASTUTI1,2#+, Rajeshwar MEHROTRA1, Ashish SHARMA1
1UNSW Sydney, 2Petra Christian University
The latest generation of climate model simulations, while advanced, retain biases preventing their direct use. Consequently, employing bias correction (BC) procedures is essential. While various BC approaches exist, such as univariate BC approaches targeting specific statistical attributes like mean, standard deviation, or statistical distribution at a particular time scale – more complex multivariate BC approaches address broader statistical attributes, including interdependencies among variables. However, incorporating numerous variables in multivariate approaches increases complexity, resulting in higher uncertainty in the bias-corrected future climate simulations. In response to the demand for high-quality climate model simulations for their application in hydrologic and water resources studies, a holistic BC approach that minimizes biases without adding uncertainties is imperative. This paper presents a Wavelet-based Bias Correction (WBC) approach, a time-frequency-based BC. WBC rectifies systematic deviations in spectral attributes of raw climate model simulations, providing a higher degree of similarity of order one and two moments with observations and capturing temporal and spatial dependencies between climate variables. WBC employs wavelet analysis to extract trends, correcting climate signals in the current climate while ensuring continuity into future climate simulation. Its robustness is evident in adjusting two datasets exhibiting significant opposite trends – global mean sea level (GMSL) and the Arctic sea-ice extent, as well as bias-correcting sea surface temperature and precipitation in the Niño 3.4 region, matching temporal and spatial dependencies between simulations and observations. Due to its univariate nature, WBC provides greater stability compared to multivariate approaches in bias-correcting future climate simulations, making it a promising holistic BC approach. A user-friendly, standalone MATLAB-based application for WBC is developed, enabling easy utilization without the need for a MATLAB license, thereby ensuring open-access availability and simplifying practical implementation – an important advancement in improving the quality of climate model simulations for broader use.
HS02-A013
Hydrological Drought Assessment Based on a Multiscalar Standardized Terrestrial Water Storage Index
Jianfeng LI1#+, Aihong CUI2
1The Chinese University of Hong Kong, 2Hong Kong Baptist University
GRACE-based observations of terrestrial water storage (TWS) were used to develop a multiscalar standardized index to assess hydrological droughts. The index is called standardized terrestrial water storage index (STI). The proposed index reflects the surplus/deficit of the integration of all sub-surface and surface water components (e.g., groundwater and runoff) as measured by TWS. Compared to other drought indices, STI is good at capturing persistent drought events with less noise. Short-term STI (e.g., 3 and 6 months) have good correlations with long-term standardized meteorological drought indices such as SPI and SPEI (e.g., 18 and 24 months). The multiscalar STI is well correlated with variations of vegetation as measured by Normalized Difference Vegetation Index (NDVI) than uni-scalar drought indices.
HS02-A015
Prediction and Evaluation of Flood Inflow Based on Stress Scenarios
Taehyeong KIM#+, Boosik KANG, Jiyoung SUNG
Dankook University
Recently, flood damage due to concentrated and localized heavy rainfall due to abnormal climate is increasing. Because floods cause great social and economic losses, it is very important to predict the amount of runoff caused by heavy rainfall when it actually occurs. However, in Korea, there is limited reliable observational heavy rainfall event data among past observation data to evaluate the accuracy of runoff prediction. Therefore, in this study, we used the stress scenario approach and the HEC-HMS runoff model to investigate the effect of composite changes in rainfall and upstream flow in the Namgang Dam basin during the flood season on dam inflow Based on the observed heavy rain events, we created a stress scenario containing a variety of cases, used it as input data for the HEC-HMS model, and derived results to obtain forecast results according to various situations. Through these results, we not only analyzed various scenarios that could occur in the study area, but also evaluated whether the Namgang Dam inflow was more sensitive to rainfall or upstream boundary conditions. In follow-up research, we plan to use the data generated in this study to develop a machine learning-based AI-Surrogate model to predict flood inflow. This can serve as a tool to quickly obtain flood forecast data through simple input values without a physical model.
HS02-A010
Spatiotemporal Characteristics of Flood and Socio-economic Impacts: A Long-term (1988-2023) Satellite-based Monitoring and Analysis Over Global South
Ho Minh Tam NGUYEN1+, Young-Joo KWON1, Hyungjun KIM1,2#
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo
The increasing frequency and severity of floods, widely attributed to climate change, disproportionately impacts countries in the Global South. Despite their minimal contribution to global emissions, these regions are experiencing more frequent and devastating floods. This study aims to delineate the long-term flood patterns and their socio-economic impacts in these vulnerable regions; therefore, providing essential data for climate change adaptation strategy is crucial. We utilized the Normalized Difference Water index with the Otsu threshold method to extract monthly flood inundation extents over a long-term period from 1988 to 2023, using Landsat and Sentinel satellite imagery. These data were then combined with a Global human settlement dataset, including population and urban-rural layers, to operationally estimate the total affected population and MODIS Land cover dataset to estimate damaged agriculture due to floods. Our findings reveal a significant increase in the proportion of people exposed to floods between 1988-1997 and 2013-2022, a period that coincides with substantial urbanization. For instance, in Mozambique, the average percentage of the population exposed to floods rose from 1% to 1.9%; in Sudan, it increased from 0.2% to 1.7%; in the Democratic Republic of the Congo, it escalated from 0.03% to 1.4%; and in Honduras, it grew from 0.2% to 0.6%. This research contributes crucial quantitative estimations of flood exposure in the Global South, offering insights for a better understanding and development of targeted adaptation strategies in the context of rapid urban development.
HS02-A005
India’s Groundwater Depletion Challenge: Current Understanding, Future Projections, and Potential Adaptation Measures
Yadu POKHREL1#+, Amar Deep TIWARI1, Nishan BHATTARAI2
1Michigan State University, 2The University of Oklahoma
India’s groundwater crisis has been long discussed and widely debated. Yet, despite progress made in understanding the recent changes in groundwater systems in response to changing monsoonal patterns and accelerated irrigation pumping, many questions remain unanswered. In particular, critical gaps remain in the understanding of the fate of India’s groundwater systems under compounding pressures from rapidly growing demands and dwindling supplies. This presentation will discuss future projections of India’s groundwater depletion using results from coupled surface water-groundwater modelling and regression analyses considering a range of climate change and future water use scenarios. Further, it will illustrate future state of groundwater systems, along with spatio-temporal patterns, under varying warming levels and for different future time windows. Light will be also shed on various adaptation measures that may steer the region toward more sustainable pathways. Results presented will be based on two recent publications and ongoing modelling activities using fully process-based models that explicitly simulate coupled irrigation-groundwater systems.
Session Chair(s): Hung Soo KIM, Inha University
HS50-A009
Development and Application of Compound Flood Level Model Based on Machine Learning for Taehwa River, Korea
Kyunghun KIM+, Seongcheol SHIN, Minseok KIM, Soojun KIM, Hung Soo KIM#
Inha University
The world is experiencing an increase in both the frequency and intensity of flood disasters due to the effects of the climate change. In particular, the risk of coastal compound flood caused by the interaction of rainfall and storm surge has been increased due to the effect of sea level rise and the changes in rainfall intensity caused by the climate change. However, the concept of compound flood has not been used to estimate the design flood level in the coastal areas. Therefore, this study developed compound flood level model based on machine learning for the Taehwa river in coastal area. Before developing the model, we applied discrete wavelet transformation and rainfall-runoff model to identify the physical components of the compound flood level. We separated the astronomical tide component from the observed storm surge data by the wavelet transformation and simulated the rainfall-runoff component. The water level obtained from the sum of the two components was similar to the observed flood water level. A machine learning based Long Short Term Memory (LSTM) model was developed to estimate the compound flood level. The model’s performance was evaluated by evaluation indices. As the results, a NRMSE(Normalized Root Mean Square Error) of 5.27%, R-squared of 0.95, and PDIFF(Peak Difference) of 0.04m were obtained. We compared the design flood water level (5.79m) with the estimated compound flood level using the same criteria for the Taehwa river. The estimated compound flood level from the developed model was 6.15m, which was about 0.36m higher than the design level. Through the result, we confirmed that the flood prevention measures based on the design level are vulnerable to the compound flood. Acknowledgements: This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. 2022R1A2C2091773).
HS50-A001
Assessment of Jules Land Surface Model Coupled with CaMa-Flood for Seamless Streamflow Prediction Across Australia
Fitsum WOLDEMESKEL1#+, Christoph RUDIGER 1, Dai YAMAZAKI2, Hugh ZHANG3, Toby MARTHEWS4, Siyuan TIAN1, Jiawei HOU1, Wendy SHARPLES1, Chun-Hsu SU1
1Bureau of Meteorology, 2The University of Tokyo, 3Centre for Climate Research Singapore, 4UK Centre for Ecology & Hydrology
The Australian Bureau of Meteorology provides hydrological forecasts and projections at discrete spatio-temporal scales. As part of their ongoing research and development Program, the Bureau has set out to develop an improved implementation of the UK Met Office’s operational land surface model – Joint UK Land Environment Simulator (JULES) – in a whole-of-earth system modelling approach with a specific focus on Australia's unique hydrology and phenology. This approach will facilitate consistent and seamless hydrological reanalysis and prediction capabilities across a wide range of spatio-temporal scales. The aim of this study is twofold: (i) to implement a gridded hydrodynamic model, namely the Catchment-based Macro-scale Floodplain (CaMa-Flood), to simulate the hydrodynamics of rivers across Australia; (ii) to investigate how well JULES coupled together with CaMa-Flood (JULES-CaMaFlood) simulates streamflow across Australia. For the evaluation, JULES was run in an offline (forced with Australian Gridded Climate Data (AGCD) rainfall) and in two-way coupled atmosphere-land (BARRA-R2 reanalysis) systems. These are compared against the Bureau's operational landscape model (AWRA-L) across 460 catchments with diverse topographic and hydro-climatic conditions. In addition, comparison of the AGCD and BARRA-R2 rainfall forcing was carried out to examine the effects of differing rainfall on the runoff to streamflow generation within JULES-CaMaFlood. Preliminary results suggest that JULES-CaMaFlood performs reasonably well for perennial catchments while the metrics are generally lower for intermittent and ephemeral catchments. Assessment of simulated streamflow indicate that high model performance is achieved across northern Australia and along its east coast. However, the performance is relatively poor in the western and south-western parts of Australia, possibly due to the non-perennial nature of some of the catchments located in these regions. Future improvements will include incorporating surface-ground water interactions, impacts of reservoirs and regulations, data assimilation, as well as improvements in the JULES model physics.
HS50-A012
Hydrologic Modeling and Forecasting: Role of Complexity, Connectivity, and Nonlinearity
Bellie SIVAKUMAR#+
Indian Institute of Technology Bombay
Hydrologic systems are complex, nonlinear, and dynamically-evolving systems. They are made up of numerous interconnected components, each varying in both space and time. Over the past several decades, many theories have been developed for studying natural, physical, and socio-economic systems, especially under the umbrella of complex systems science. Applications of such theories and associated methods to numerous hydrologic systems around the world have yielded encouraging outcomes and advanced our understanding of hydrologic systems. In recent years, chaos theory and complex network theory have been gaining significant attention in hydrologic studies, including for identification of system complexity, prediction, catchment classification, and downscaling. These theories offer unique perspectives on the complexity, connectivity, and nonlinearity of hydrologic systems. The present study discusses the progress made in the applications of chaos theory and complex network theory in hydrology. In particular, it focuses on studies that have coupled the concepts of chaos theory and complex network theory (i.e. phase space reconstruction for network formation) for studying hydrologic systems. After reviewing several key aspects of these theories, specific applications of their coupling for studying complexity and connectivity in hydrologic systems are presented. The applications include temporal variability of rainfall (in India) and streamflow (in the United States), critical rainfall and streamflow monitoring stations (in India and Australia), and sediment transport dynamics (in the United States). The important role the coupling of chaos theory and complex network theory can play in advancing research on hydrologic systems is also discussed.
HS50-A003
Design of Optimal Hydrometric Networks in Poorly Gauged Basins
Jongho KEUM1#+, James LEACH2, Frezer AWOL3, Bouraïma KOUANDA4, Jafet ANDERSSON5, Paulin COULIBALY1
1McMaster University, 2Environment and Climate Change Canada, 3Ontario Power Generation, 4Mouhoun Water Agency, 5Swedish Meteorological and Hydrological Institute
Burkina Faso, located in West Africa, stands as one of the world’s least developed and the poorest nations. Due to financial limitations and a shortage of skilled personnel, the task of maintaining quality water resources information proves challenging. Given the current socioeconomic situation in Burkina Faso, it is crucial to establish an optimal hydrometric network to ensure high-quality hydrologic information at minimal monitoring cost. The country categorizes hydrometric stations into three classes: regional essential stations (Class 1), national essential stations (Class 2), and stations for specific needs (Class 3). The Baseline network encompasses Classes 1 and 2, while the National network extends to include Class 3 stations. Initiating the data-driven network design process involves collecting a robust time series. Burkina Faso, however, faces significant gaps in the observed time series data. Adopting the Worldwide HYPE and West-Africa HYPE models for flow data at existing and potential hydrometric stations, we employ an entropy-based multiobjective optimization. This method maximizes the joint entropy to ensure maximum information from the network while minimizing total correlation to eliminate redundancy. In addition, streamflow signatures and BGI aridity index were also embedded in the optimization in order to consider the catchment behavior and the climatic information. Unlike conventional network design approaches, where existing stations remain static, Burkina Faso’s hydrometric networks undergo redesign, allowing for the relocation of suboptimally situated and manually operated stations. This approach acknowledges that the observation period alone does not guarantee data quality. Through the optimization, hydrometric network and water resources managers are provided the ability to make informed decision, fostering improved water security and sustainable development.
HS50-A014
Dynamic Budyko Model: A Simple Calibration-free Runoff-generation Model
Basudev BISWAL#+, Prashant ISTALKAR
Indian Institute of Technology Bombay
In hydrology, process complexity increases both in temporal and spatial scale. Predicting streamflow at a large timescale (more than a year) is much easier than at a small (daily) timescale. One of the most commonly used frameworks for large timescale streamflow prediction is the Budyko framework. The Budyko framework provides precipitation partitioning into evapotranspiration and streamflow using dryness index, the ratio of potential evapotranspiration (PET) to precipitation (P). However, this framework cannot be applied at the daily timescale due to the assumption that small timescale hydrological partitioning is governed by both climate (P and PET) and catchment characteristics. Thus, the hydrological model predicting daily streamflow incorporates catchment characteristics in terms of free parameters in the model framework, which need to be estimated using calibration. However, large timescale hydrological partitioning is the result of small timescale hydrological partitioning. Thus, climate inputs should be sufficient to provide hydrological partitioning at the daily timescale. With this hypothesis, the Dynamic Budyko (DBv1) model was proposed, which predicts daily streamflow using climatic inputs and the concept of the instantaneous dryness index. Although the calibration-free DBv1 showed acceptable streamflow prediction performance in ungagged basins, its low performance compared to a fully calibrated hydrological model is not fully explored. In this study, we proposed a modified DBv1 (DBv2) model that shows a significant improvement in streamflow prediction performance. Also, we compared DBv2 with two well-known hydrological models, HBV and GR4J, in predicting daily streamflow for 416 MOPEX basins. The results show that the calibration-free DBv2 model performed as good as the calibrated HBV and GR4J in terms of runoff generation, with a median NSE of 0.66. Overall, this study challenges the long-term assumption that static catchment characteristics play a role in runoff generation at the small timescale.
HS50-A011
India Water Model: A Transboundary Water Modeling System Over South Asia and a 75-year Daily Streamflow Reanalysis
Manabendra SAHARIA#+, Ved PRAKASH
Indian Institute of Technology Delhi
Effective management of water resources requires reliable estimates of land surface states and fluxes, including water balance components. But most land surface models run in uncoupled mode and are often uncalibrated and hence suffer from large uncertainties at the local scale, hindering their adoption as a tool in real-time decision-making. Such integrated systems are also rare over India/South Asia where hydrometeorological extremes have wreaked havoc on the economy and people. The India Water model (IWM) is an integrated national hydrological-hydrodynamic water modeling system being built using the NASA Land Information System Framework (LISF). We simulated daily streamflow spanning the years 1949 to 2022 across South Asia's diverse river basins by calibrating using observed streamflow. Leveraging meteorological forcings from local and global sources, our model integrates NoahMP as the land surface model and the HyMAP river routing model to generate daily streamflow within the South Asian sub-continental river basins. We perform validation all major components of the terrestrial water cycle, including streamflow, in order to ensure the model's adaptability and relevance to the local nuances of basins, aligning the simulated daily streamflow patterns with observed data. This extensive reconstruction and evaluation of streamflow dynamics not only contribute significantly to filling the knowledge gap but also lay the foundation for more precise and informed water management strategies in the dynamic landscape of South Asia's river basins.
HS50-A010
Blue-Green-Grey Infrastructure Performance Evaluation for Flood Defence
Nakyung LEE+, Inkyung MIN, Yelim BANG, Juyeon JANG, Sanha KIM, Daeryong PARK#
Konkuk University
In urban drainage systems, the flood defense capacity of each infrastructure plays an important role in urban flooding and related disasters. Each infrastructure temporarily regulates flows to mitigate flood damage, and the ability to trap flows is highly relevant to flood mitigation. Therefore, It is important to quantify and predict the flood defense capacity of infrastructures. However there is a lack of research to quantify the capacity of these infrastructures. To solve this problem, A Flood defence index (FDI) that can quantify the defense capacity by utilizing the conveyance capacity (as available storage) is proposed on this study. SWMM, a storm water management model, was used to calculate the capacities of blue, green, and gray infrastructure facilities. Based on this, a flood defense index and defense performance curves were presented for the linked systems. These index and curve can be used in conjunction with real-time monitoring technologies to provide guidelines for the operating rules of infrastructure during extreme rainfall events, and can help decision makers establish facility-specific flood protection performance targets. Acknowledgement : This work was supported by Korea Environment Industry & Technology Institute(KEITI) through R&D Program for Innovative Flood Protection Technologies against Climate Crisis, funded by Korea Ministry of Environment(MOE)(RS-2023-00218973) and Water Management Program for Drought, funded by Korea Ministry of Environment(MOE)(2022003610003).
HS50-A007
Evaluation of the Securing Ecological Environmental Flow in the Naeseong River Basin Based on Reservoir Operation
Inkyung MIN+, Nakyung LEE, Yelim BANG, Juyeon JANG, Sanha KIM, Daeryong PARK#
Konkuk University
This study investigated an evaluation of the securing ecological environmental flow in the Naeseong river basin based on reservoir operation. A study was conducted on five reservoirs in the Naeseong river basin, a tributary of the Nakdong River. Hourly rainfall, maximum and minimum temperature, relative humidity, solar radiation time, and wind speed data from 1973 to 2020 of the Korea Meteorological Administration stations in South Korea were adopted. And hourly flow data from WAMIS were used. The SWAT model was used to produce monthly inflow data for the reservoirs. By applying the reservoir operation rate that adjusts the discharge amount according to the reservoir's remaining water volume, the linked operation of the multi-reservoir was simulated. The simulation was conducted for a total of 11 years, from 2010 to 2021, excluding 2015. The optimal demand distribution ratio that maximizes demand satisfaction within the basin and target environmental flow was selected according to the Downstream environmental flow. Furthermore, the amount of environmental flow secured at the downstream point of the basin when the optimal demand distribution ratio and target environmental flow were applied was evaluated. Through this study, it is expected that efficient multi-reservoir operation will be possible by establishing standards for linked operation of reservoirs. Moreover, it will be possible to effectively respond to drought by utilizing reservoirs as a means of alleviating water shortages in the basin. Acknowledgments: This research was supported by Korea Environment Industry & Technology Institute(KEITI) through Aquatic Ecosystem Conservation Research Program(or Project), funded by Korea Ministry of Environment(MOE)(RS-2022-KE002214) and Water Management Program for Drought, funded by Korea Ministry of Environment(MOE)(2022003610003).
Session Chair(s): Kenichiro KOBAYASHI, Saitama University, Kei NAKAGAWA, Nagasaki University, Hitoshi MIYAMOTO, Shibaura Institute of Technology, Channa RAJANAYAKA, Earth Sciences New Zealand
HS16-A008
| Invited
Climate Change Impact Assessment of the Precipitation Pattern and Flood Discharge in Kyushu, Japan
Yasuyuki MARUYA#+, Shinichiro YANO, Hiroki KIMURA, Satoshi WATANABE
Kyushu University
In previous studies, it has been demonstrated that precipitation patterns have been affected by climate change, leading to severe floods. Especially, in Kyushu, Japan, flood damage has been caused several times in recent years, such as the heavy rainfall in July 2020. Therefore, this study aims to assess the impact of climate change on the change of the precipitation pattern that has caused the flood discharge by targeting Kyushu, Japan. In this study, in order to compare the change of the precipitation pattern and flood discharge in the present and the future, we used d4PDF (Present climate: HPB, Future climate: +2K scenario and +4K scenario, we called them F2K and F4K, respectively) as the GCM simulation data. As a result, it was shown that the short-term precipitation such as the annual maximum 1 hourly and 2 hourly precipitation in the future (F2K and F4K) might be increased relative to the present (HPB). On the other hand, it was demonstrated that the precipitation duration times increase such as 24, 48, 72, and 168 hourly precipitation, the changing ratio with HPB of F2K might be decreased. Furthermore, it was found that the annual maximum 72 and 168 hourly precipitation in HPB and F4K will be the almost same. Moreover, the precipitation duration time and the maximum and accumulated precipitation in the precipitation duration time in the future (F2K and F4K) could be shortened and increased relative to the present (HPB). Therefore, it was suggested that the flood discharge in the future will be caused by the increase in short-term precipitation.
HS16-A017
| Invited
Hydrological Modeling and Assessment of Flood Discharge in a Future Climate: A Case Study of Bagmati River Basin, Nepal
Binaya Kumar MISHRA#+
Pokhara University
Recently, urban flood events are increasingly reported in many countries with enormous loss of life and livelihood; and property damage. The increase in urban flood events is largely attributed to haphazard infrastructural development, poor stormwater drainage system, land cover and climate change resulting more surface runoff and less groundwater recharge. Climate change is well known for alteration in future precipitation pattern with increased extreme precipitation and flood events. Simulation and assessment of future floods under climate change can help in policy formulation and mitigation of future flood risks. In every monsoon, several parts of Kathmandu valley get inundated causing disruption of traffic and various other activities; injury and deaths of human being and domestic animals; damage and displacement of private and public properties. HEC-HMS model was set-up for simulating flood discharge in Bagmati River Basin upstream of Khokana (Lalitpur) which cover Kathmandu valley of Nepal. Daily discharge data of three largest flood events during 1995-2015 were employed for calibration and validation of the HEC-HMS model. Performance of the flood simulation model was found to be quite satisfactory, judging from visual and statistical parameters. With present climate over 1980-2000 period and future climate over 2080-2100 period; very high-resolution (2km×2km) NHRCM climate model precipitation output for SSP5-8.5 emission scenario was applied for simulating and assessing future flood risks in the Kathmandu valley. Larger flood peaks were found for the future precipitation time-series data. Consequently, flood-frequency analysis using Gumbel distribution resulted significantly higher values of return-period floods and risks. Keywords: Climate Change, Bagmati River Basin, Food-frequency, HEC-HMS, NHRCM.
HS16-A020
Integrated Flood Mapping and Crowdsourcing Data with an Application of Data-driven Models in a Case Study of Bangban Bangsai Canal, Ayutthaya, Thailand
Detchphol CHITWATKULSIRI1#+, Hitoshi MIYAMOTO2
1Kasetsart University, 2Shibaura Institute of Technology
A flood map is one of the keys to predicting and mitigating the impact of flooding worldwide. The majority of flood map data is created using various applications, such as numerical modeling and geospatial data analysis. Data-driven techniques, such as deep learning models and generative artificial intelligence, now produce outputs that are substantially more reliable and faster. However, in order to improve the accuracy and precision of flood maps, the prediction model must be validated using primary field data. Crowdsourcing data, such as photos of flooding from the local communities in the area, can be improved and driven by the flood mapping model. This research used a data-driven model approach, such as Image-to-Image translation with conditional adversarial networks, to combine a deep learning model of flood maps generated from a hydraulic model with crowdsourcing data of flooding photos in the case study area to improve prediction. The trained model was developed using a generative adversarial network - GAN architecture. This research implemented a PIX2PIX module for flood depth recognition. It generated the flood map with the particular area and location from crowdsourcing flooding photos referring to the flood depth. This integration introduces an innovative technique for using crowdsourced flooding photo data to improve a flood prediction model using data-driven models. It was tested in a peri-urban with dense residential areas called Bangban Bangsai Canal in Ayutthaya, Thailand. Overall, the findings show that using crowdsourced data outperforms by 5.81% of RMSE and 0.91 of SSIM. The future direction of this research is currently localizing the coverage and quantity of crowdsourced input data in order to improve the effectiveness of flood map prediction.
HS16-A021
Archetypal Patterns of Urban Drainage Networks in an Asian Megacity
Hyeonju KIM#+, Soohyun YANG
Seoul National University
Urban drainage networks (UDNs) are one of essential infrastructures to protect urban residents from water-borne diseases and water-related hazards. The UDNs play a key role in collecting human-produced wastewater and pollutants and conveying them to a wastewater treatment plant, which in turn discharges the effluents into neighboring river bodies. It indicates that the layout and specification of UDNs are highly likely to be affected by the distribution and density of sources (e.g., households) and further influence the status of water quality (WQ) of urban streams. Nonetheless, there is little known about coupled relations among structural characteristics of UDNs, demographic and socio-economic characteristics for a given sewer-shed, and the resultant impacts on the WQ of urban streams. Therefore, we aim to uncover representative archetypes that illustrate the sewer-shed characteristics and the resultant WQ in their receiving streams, grouped by structural patterns of UDNs. This study addresses two hypotheses: (1) structure of UDNs exhibiting well-known scaling features of river networks indicates intensified urbanization of a given sewer-shed; (2) more urbanized sewer-sheds correlate with poorer WQ of receiving streams, which is distinguishable through UDNs' structural traits. The hypotheses are explored through the analysis for the megacity of Seoul, Korea (~16K persons/km2; ~605 km2). We focus on 40 sewer-sheds in Seoul, each having a discharge point into one of four major tributaries of the Han River (i.e., the Hongjae, the Jungnang, the Anyang, and the Tan streams), based on the presence of WQ measurement stations. We employ scaling features including Horton’s laws to assess the UDNs’ structural patterns. Urban attributes are described as core urbanization-indicative factors including population, land-use, educational infrastructure, and monitored WQ data. Our findings are expected to provide insights for the resilient design and management of UDNs and guide a deeper understanding of the WQ integrity of urban streams.
HS16-A022
Basic Study on Evaluating House Collapses Due to Flooding Using 1m Resolution Elevation Data
Nanako INOKAWA1#+, Kenichiro KOBAYASHI2
1Kobe University, 2Saitama University
The collapse of houses due to flooding is a critical issue so that many attempts have been carried out by many stakeholders to estimate the fluid force on the houses through inundation analysis using detailed elevation data, such as 5 meters. On the other hand more detailed elevation data, such as 1-meter resolution, has been published recently by Hyogo Prefecture, Japan. Therefore, the authors examined the accuracy of inundation analysis using the 1m resolution elevation data. As a result. It was revealed that it was possible to accurately reflect topography, especially between houses, using the 1m resolution. In this study, we also focused on the assessment of the risk of house collapses due to flooding by examining the fluid force and velocity between houses. Additionally, we considered the method of assessment of the risk of house collapses. The analysis utilized an inundation model based on the two-dimensional shallow water equation to simulate the flooding by a river bank breach in a densely residential area. As a result, it was found that considering the feature of individual houses is significant to evaluate the risk of house collapses.
HS16-A011
Evacuation Timeline and 3D Visualization of Urban Floods by Using Inundation Simulation and GIS Analysis
Naoya MAEDA#+, Haruka MATSUSHIMA, Hitoshi MIYAMOTO
Shibaura Institute of Technology
The ongoing phenomenon of global warming has precipitated unprecedented large-scale inundations within urban cities worldwide. Consequently, reliance solely on static information, such as hazard maps, for evacuation planning is deemed insufficient. This necessitates the consideration of vulnerable people, specifically women, children, and older people, in flood evacuation. This study conducted a flood simulation within Koshigaya City, situated in the Ayase River basin in Japan. Employing the iRIC software, a three-dimensional visualization of flood inundation dynamics and evacuation details pertinent to the disaster-vulnerable population was derived. The simulation incorporated flood flow rates anticipated under the influence of global warming. Evacuation patterns and temporal dynamics were scrutinized using the model results on inundation depth and flow velocity, with the resultant flood inundation visualized in three dimensions. Consequently, temporal variations in evacuation dynamics, walkable ranges for the disaster-vulnerable, and the lead time and route to evacuation shelters were delineated. Notably, disparities were unveiled, indicating that, compared to women, children exhibit variances in walkable water depth of up to 50 cm and evacuation time of up to 15 minutes. Future studies will incorporate individuals with physical disabilities and explore ways to enhance the information's comprehensibility.
HS16-A019
Estimation of the Wind Effect on Rainfall-runoff-inundation Simulation
Kenichiro KOBAYASHI#+
Saitama University
This presentation deals with an attempt to estimate the effect of the wind on the rainfall-runoff-inundation simulation. The shear stress term due to the wind with the bulk coefficient was added to the shallow water equation of the rainfall-runoff-inundation model. The rainfall-runoff-inundation model is composed of the 2D shallow water equation for the inland area, 1D dynamic wave equation for the river flow and depth averaged unsaturated flow model for mountainous area. The presentation shows how the wind effects both on the discharge of the river and inundation depth/distribution for the inland area.
Session Chair(s):
HS02-A009
An Approach to Set the Industrial Water Withdrawal Targets Based on Local Water-sector Needs Under the SBTN Context
Saritha PADIYEDATH GOPALAN1#+, Naota HANASAKI2, Taikan OKI1
1The University of Tokyo, 2National Institute for Environmental Studies
The industrial sector needs a clear way of minimizing its impact on water resources due to the increasing pressure on the water supply. Recently, Science-Based Targets for Nature (SBTN) issued detailed methodologies for companies to set initial targets on water use, enabling companies to align their efforts with global water-related sustainability efforts. Still, there needs to be a clear direction for the realization of this methodology in setting the targets for industrial water withdrawal. Here, we utilize the ‘Remaining Available Water’ (RAW) concept to set the water withdrawal target for the industrial sector based on local environmental needs. An industrial water withdrawal above the RAW indicates an unacceptable-level of withdrawal that will eventually affect the local water-sector needs. We applied this concept in the Chao Phraya River Basin, Thailand, using the H08 macro-scale model to evaluate the impact of (i) historic (1980-1999) and (ii) future (2080-2099) industrial water withdrawals because nearly 15 industrial estates (IEs) are located within the basin. Three simulations of (i) current industrial water withdrawal, (ii) a 50% increase in withdrawal, and (iii) a 100% increase in withdrawal were carried out. We found that the number of days during which the withdrawal exceeds the RAW values was (on average and ± standard deviation across IEs) 26±16.0, 31±15.7, and 33±16.1 days in a year under the current, 50% increase, and 100% increase in withdrawals, respectively, for the historic scenario. The same for the future scenario (under the extreme warming scenario of RCP 8.5) was 17±7.9, 20±8.0, and 23±9.3, which shows an increased water availability for the industrial sector in the future. Further adaptation measures have to be considered to reduce the unacceptable-level of water withdrawal below the RAW values at the IE locations. This simulation results by H08 model will help companies to develop their withdrawal targets.
HS02-A012
Impact of Water Spreading Weirs on Groundwater Recharge in Afar Region, Ethiopia
Hailemariam DOKO#+, Koji DAIRAKU
University of Tsukuba
The Afar Region in northeast Ethiopia is one of these lowland areas. The region’s variable and unreliable rainfall regularly lead to droughts and flooding, which frequently jeopardize agricultural production and the life of animal herds on which people’s livelihoods depend. Most people use traditional Agro-pastoral and pastoral farming systems that were previously sustainable but now lead to soil degradation and production shortfalls due to rising intensities of use. In Afar Region there are areas are influenced by floods stemming from the adjacent highland regions. To avoid these damages and to increase the available water resources in the implementation areas, a new technology Water Spreading Weirs (WSW) is introduced. Due to the design of the WSW, the water is forced to spread over a certain area where the surface water is retained for a certain time. The objective of this assignment was to develop a groundwater monitoring system to evaluate the influence of the Water Spreading Weir structures on groundwater recharge by installing groundwater data loggers in three groundwater wells. From the result groundwater levels in Shakayburo and in Duba are both decreasing in a very similar Trend, the groundwater level at the site in Duba started to increase while the groundwater level in Shakayburo further decreased. This increase in groundwater level in Duba may stem from local floods which may have occurred at that time around Duba. Thus, the increase is correlated with the infiltration of surface water. The groundwater levels recorded at the well in Regdan increased consequently to around 1.1 m above the initial hydraulic head. This indicates that the increase of groundwater levels in Regdan may stem from a local shallow aquifer that overlays the deep aquifer and is infiltrating through a semi-permeable layer into the main deeper aquifer.
HS02-A016
Nonlinear Effects of Global Temperature Rise on Major Breadbasket Failures Under Different Warming Levels
Somin PARK1#+, Yusuke SATOH1, Hyungjun KIM1,2
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo
The “nonlinearity” of climate change impacts on crop yield remains uncertain, while the impact of the rise in global mean temperature on crop growth is evident as demonstrated in previous studies. The extent of crop yield decline is not consistently proportional through the entire range of temperature rise; rather, it exhibits abrupt changes between certain warming levels, which varies significantly for different regions. Here, we determine the level of warming where a significant transition such as abrupt and/or irreversible change is identified. Our analysis presents such tipping points for major crop-producing, by employing multi-model ensemble simulations from the Global Gridded Crop Model Intercomparison (GGCMI). The nonlinear response of crop yield to global warming is captured by systematically perturbing temperatures from -1 to +6℃ in 1℃ increments, relative to the historical climatology of 1980-2010. The frequency of extreme heat and precipitation events is also incorporated, to discern the heat and water stress on crop growth. We evaluate crop yield changes at country level, considering both geographic regions and crop types. This study aims to deepen our understanding of temperature rise impacts on the food sector through defining the tipping points of the major breadbasket failures, which is crucial for the development of effective climate-resilient strategies to achieve UN SDG Goal 2 of ending hunger.
HS02-A023
Toward Holistic Perspective on Dam Efficacy in Transboundary Hydro-extremes Management
Abubaker OMER1#+, Hyungjun KIM1,2
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo
Research on assessing dams preparedness to mitigate hydrological extremes has grown under climate change and water conflicts. However, discerning the success or failure of these strategies remains challenging, especially in Transboundary Rivers. Here, we use a meta-analytic approach to examine 14 moderators of dam efficacy in flood and drought risk management. We synthesize impact assessment datasets from 287 articles for 12 transboundary basins across the globe. Findings show that forest cover and gross domestic product enhance dam efficacy in flood control. In flood hotspots, the synergy of dam management and institutional factors is the paramount determinant of dams performance. Conversely, the efficacy in the drought-prone basins is governed mainly by the interplay of institutional and socioeconomic factors. Climate aridity, precipitation anomalies, and hydropower dams lessens the dams effectiveness in mitigating both hydrological extremes. We argue that endorsing adaptive management through dams in transboundary basins requires a holistic approach. Thus, we emphasize accounting not only for the physical and engineering aspects, but also for the intertwined environmental, socioeconomic, and geopolitical implications.
HS02-A022
Assessing Watershed System Responses to Groundwater Sustainability
Tarekegn Dejen MENGISTU1,2#+, Il Moon CHUNG2
1University of Science and Technology, 2Korea Institute of Civil Engineering and Building Technology
Assessing the long-term availability of water resources under rapidly increasing population, urban expansions, and climate change anomalies is crucial to balance demand and supply. The continuous groundwater-surface water interactions (GSWI) are challenging due to a lack of viable information and process complexity. Addressing these challenges requires a holistic strategy, integrating sophisticated hydrological models and techniques to enhance our understanding of subsurface dynamics to assist water management strategies in accurately representing GSWI processes. This study aimed to assess the sustainability of groundwater reserves and hydrologic system responses under GSWI on a watershed scale. The application of the coupled SWAT-MODFLOW model was developed by linking SWAT with MODFLOW models. The coupled SWAT-MODFLOW was calibrated through a PEST-based approach by manually adjusting pre-calibrated SWAT and MODFLOW parameters simultaneously with stream flow and aquifer properties. The simulation performance of models was verified by comparing observation records and demonstrated satisfactory predictions of water balances and GSWI. The effects of GSWIs on assessing the exploitable amount of groundwater, groundwater recharge, and groundwater contributed to the environmental flow in a condition of sustaining ecosystems were determined. Applying calibrated parameters to quantify GSWI provides reasonable results minimizing uncertainty while considering the aquifer's physical nature. Then, the groundwater sustainability index was estimated from a coupled model. The area under investigation found in a moderate groundwater depletion conditions revealing a need of appropriate policy planning and management strategies to avoid long-term reduction. Therefore, the present study provides valuable insights that could serve as a reference to plan resilient water resources management strategies of achieving sustainable development goals. The study is carried out under the KICT research program, funded by the Ministry of Science and ICT, Project No. 20230426-001.
HS02-A021
Urban Infrastructure Design in the Climate Change Context: Modeling of Extreme Rainfall Processes Over a Wide Range of Time Scales
Van-Thanh-Van NGUYEN#+
McGill University
Extreme rainfalls of short time scales (from a few minutes to less than one day) are required for urban infrastructure design. These data are often limited or unavailable at the location of interest while those for the daily scale are widely available. Hence, it is important to develop a modeling method that could describe accurately the statistical properties of the extreme rainfall processes over a wide range of time scales so that rainfalls for sub-daily scales can be estimated from those for the daily scale. Furthermore, climate change has been recognized as having a profound impact on the rainfall process. Hence, climate models have been extensively used for the impact assessment. However, due to the limitations on detailed physical modelling and computational capability, outputs from these climate models are provided at too coarse resolutions and thus not suitable for these impact studies. Consequently, downscaling methods are needed for linking these coarse-scale climate simulations to the observed extreme rainfall records at a given location. Therefore, the main focus of this presentation is to introduce a scale-invariance (scaling) approach to the downscaling of extreme rainfall processes using the Generalized Extreme Value (GEV) distribution. This scaling GEV model was based on the scaling properties of the empirical statistical moments of the observed extreme rainfalls for different durations. The general mathematical framework and the scaling properties of this GEV model were described using both non-central moments (NCMs) and probability weighted moments (PWMs). The feasibility and accuracy of the proposed GEV/PWM mode were assessed using the long records of short-duration extreme rainfall data from a network of 74 raingauges located across Canada. Results of this numerical application have indicated that the extreme rainfall estimates given by the scaling GEV/PWM model are the most accurate as compared to those given by other existing scaling models.
Session Chair(s): Qingyun DUAN, Hohai University, Yang LANG, Yunnan University
HS50-A027
Hydrological Modeling in the Upper Lancang-Mekong River Basin Using Global and Regional Gridded Meteorological Re-analyses
Yang LANG1#+, Lifeng LUO2, Qingyun DUAN3
1Yunnan University, 2Michigan State University, 3Hohai University
Multisource meteorological re-analyses provide the most reliable forcing data for driving hydrological models to simulate streamflow. We aimed to assess different hydrological responses through hydrological modeling in the upper Lancang-Mekong River Basin (LMRB) using two gridded meteorological datasets, Climate Forecast System Re-analysis (CFSR) and the China Meteorological Assimilation Driving Datasets for the Soil and Water Assessment Tool (SWAT) model (CMADS). We selected the Pearson’s correlation coefficient (R), percent bias (PBIAS), and root mean square error (RMSE) indices to compare the six meteorological variables of the two datasets. The spatial distributions of the statistical indicators in CFSR and CMADS, namely, the R, PBIAS, and RMSE values, were different. Furthermore, the soil and water assessment tool plus (SWAT+) model was used to perform hydrological modeling based on CFSR and CMADS meteorological re-analyses in the upper LMRB. The different meteorological datasets resulted in significant differences in hydrological responses, reflected by variations in the sensitive parameters and their optimal values. The differences in the calibrated optimal values for the sensitive parameters led to differences in the simulated water balance components between the CFSR- and CMADS-based SWAT+ models. These findings could help improve the understanding of the strengths and weaknesses of different meteorological re-analysis datasets and their roles in hydrological modeling.
HS50-A006
Exploring the Spatial Interactivity Distribution of Hydrogeological Parameters
Zi Jun HSU#+, Jet-Chau WEN, Hong Ru LIN
National Yunlin University of Science and Technology
Past studies of hydrogeological parameters of aquifers have not using drawdown data from multiple sets of sequential pumping tests (SPT) at the same site to characterize the interaction of hydrogeological parameters (such as transmittance, T and storage coefficient, S) distribution field. Therefore, the purpose of this study was to use the same site (well site at the northeast corner of Yunlin University of Science and Technology, Douliu City, Yunlin County) collected for many years (20xx, 20xx..year, five groups in total) of SPT drawdown data. First, the interaction between the drawdown water levels from the same observation well and five sets of pumping tests was analyzed. Afterwards, this study used the numerical method of (hydraulic tomography, HT) to analyze the leakage data of five groups of SPTs., reverse calculation the distribution of T and S of five groups of SPT and a spatial comparison was performed, comparing the interaction between 5 sets of T and S distribution fields, discuss in different time and space background, interaction of distribution field of local hydrogeological parameters.
HS50-A022
Unravelling and Improving the Potential of Global Discharge Reanalysis Dataset in Streamflow Estimation in Ungauged Basins
Li ZHOU1#+, Lingxue LIU2
1Sichuan University, 2XIhua University
Mastery in forecasting the streamflow is of great importance in environmental and sustainability research. Although many global-scale reanalysis products provide a new way to overcome the lack of streamflow records in ungauged basins, streamflow estimation through hydrological models remains a great challenge mostly due to inevitable biases. In this study, we developed a novel bias-correction system equipped with the proposed Piecewise Random Forest (P-RF) model to improve the potential of GloFAS-ERA5 (GloFAS), a global-scale river discharge reanalysis product, as a calibration benchmark for building hydrological models in ungauged basins. Considering three ungauged scenarios, several cases of temporal, spatial, and spatiotemporal bias-corrections were implemented with a total of 13 river gauges located in the Min River Basin in China, and Fuji River Basin and Shinano River Basin in Japan. Then, the well-improved GloFAS discharge was applied for the calibration of the Block-wise use of the TOPMODEL (BTOP) model to evaluate its performance in substituting the discharge observations. The results show that: (1) the bias-correction system performs better on the temporal scale, which applies to ungauged basins lacking long-term continuous observations; (2) the integrity and adequacy of the samples used for training the P-RF model have a significant impact on the spatial and spatiotemporal bias-corrections, and they can be reliably estimated by the proposed metric, Ratio of the Valid samples' Proportion; and (3) the statistical metric differences between the simulated discharges obtained by the calibrated BTOP model using observations and GloFAS discharge, are reduced by 25% to 50% through the bias-correction.
HS50-A025
Intercomparison of Dam Operation Schemes in Global Hydrological Models
Shareena Azliani A AZIZ1#, Hyungjun KIM1,2+, Abubaker OMER1, Yusuke SATOH1
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo
Due to the need for better disaster prevention and water management, many dams are planned and being constructed in major river basins, particularly in the Global South. On top of global climate change, the presence of dams has significantly impacted the fluvial regime worldwide. Therefore, it is important to integrate dams in model-based impact assessment analysis of climate change using global hydrological models to avoid maladaptation. The currently available dam algorithms, applied globally, tend to be overly generalised to have shortcomings for representing actual conditions accurately. Many available schemes are oriented around water demands; with more recent studies focusing on flood control effects. There is still insufficient consideration of hydropower dams, despite increasing numbers of them within major river basins, e.g. the Mekong River. Furthermore, many studies focus on large reservoirs rather than small ones, even though cumulative impact of small reservoirs may still be significant. Such limited attention on a wider range of dam purposes and sizes in dam operation schemes may cause unoptimized hydropower generation and inappropriate water resource management, when formulating planning policies. Thus, a better and optimised dam operation scheme at a global scale is required. This study provides a dam algorithm intercomparison among four schemes. Two are inflow-and-demand based schemes which have better flexibility for coupling with global hydrological models, but have limitations in accounting for detailed reservoir operation. Meanwhile, the other two schemes are based on target-storage-and-release relationship, and, therefore, they allow better representation of seasonality and operation changes with further details in the information of dams. The intercomparison results will be assessed by investigating their behaviours and simulation sensitivity to different purposes, sizes, and output accuracy of over 100 dams globally distributed.
HS50-A016
Estimating the Daily Gridded Evapotranspiration Based on Maximum Entropy Production Principle
Kwanghun CHOI+, Kyungrock PAIK#
Korea University
Interpreting spatiotemporal variation of evapotranspiration over a region is one of the most challenging assignments in contemporary hydrology. Global evapotranspiration products have been generated through the complex computation algorithm and a considerable amount of input data. Contrary to these products, the methodology to estimate the evapotranspiration based on the Maximum Entropy Production (MEP) principle, meaning that the system tends to maximize the entropy production under physical constraints, employs relatively simple algorithm regardless of the surrounding setting. Also, the MEP-based evapotranspiration model requires only the traditional data which can be obtained from typical meteorological measurement devices or the remote sensing data. Considering the easy applicability and high temporal resolution, this model allows a researcher to generate the evapotranspiration data with any spatiotemporal resolution as they wish. On these backgrounds, we calculated the spatiotemporally distributed evapotranspiration over the Korean Peninsula based on the MEP principle on a daily scale. The input data for MEP-based evapotranspiration model were from the remote sensing data, and the spatial resolution of estimated evapotranspiration followed that of remote sensing data. Also, the forest map generated by the Korean Forest Service was utilized to provide information on botanic conditions in the Korean peninsula. Well-known global evapotranspiration products are utilized for evaluating simulation results.
Session Chair(s): Dong-Sin SHIH, National Yang Ming Chiao Tung University, Jian-Ping SUEN, National Cheng Kung University
HS12-A008
Surface Change Detection Using Planet Imagery with Google Earth Engine
Yu-Yun LIU#+, Yuan-Fong SU
National Taiwan Ocean University
Surface change detection is one of major application of remote sensing. Detect any changes on surface can be very useful in many ways. One of major example is using change detection for emergency response during catastrophic disaster such as the Noto-hantou earthquake occurred in 1st Jan. 2024 in Japan. Japan has similar disaster feature as Taiwan, we both have earthquake and typhoons. These disasters are the major triggers of landslide and even house collapse in urban area. In this study, we acquire Planet imagery before and after landslide and house collapse events in Taiwan and Japan and further upload to a cloud-based remote sensing platform (Google Earth Engine, GEE). In the GEE, we used Otsu-threshold method and percentile method to detect changes on surface. Preliminary results in the case in Taiwan show that the thresholds generated by the percentile method are nearly 300 higher than those of the Otsu threshold algorithm, with a higher accuracy in change detection.
HS12-A009
Applying Machine Learning Models to Predict Missing Weather Data Values for SWAT Model Building
Nhat Thanh TRAN#+, Yuan-Fong SU
National Taiwan Ocean University
Soil and Water Assessment Tool (SWAT) often requires a large amount of input data, of which weather data accounts for an important part. Inadequate weather data can affect the accuracy of SWAT model results. Currently, there are many different machine learning methods used to predict missing weather data by using available data to build a forecast model and using that model to infer missing data. In this study, two types of machine learning models, Linear Regression and Long Short-Term Memory (LSTM), will be used to reconstruct lost weather values of daily weather data sets including precipitation, temperature, wind, and relative humidity from 12 weather stations located in the Lanyang River watershed in northeast Taiwan. After being normalized, the weather datasets will be input into the same SWAT model to simulate surface runoff. For each simulated flow case obtained, the results are compared with the actual observed data. The effectiveness of each model is calculated and evaluated using two parameters Root Mean Square Error (RMSE) and Nash-Sutcliffe Efficiency (NSE). From there, find a prediction model with more appropriate results.
HS12-A007
Using SWAT Model to Assess Changes in Sediment Transportation in Wu River Basin Under Climate Change Scenarios
Yu-Cheng CHEN#+, Yuan-Fong SU
National Taiwan Ocean University
Global climate change has heightened the instability of Earth's climate system, amplifying the occurrence of extreme weather events. In Taiwan, this manifests as more frequent rainfall, notably characterized by short-duration heavy downpours. The rugged terrain of Taiwan has further compounded challenges, as the augmented upstream flow has precipitated substantial erosion and sedimentation infiltrating the rivers. The sediment deposition has substantial impacts on estuaries and coastal ecosystems. To cope with the challenge to realize the future changes of sediment transportation, we focus on the Wu River Basin in the central Taiwan. Using elevation and soil data from the Taiwan Ministry of the Interior, meteorological observations from the Taiwan Central Weather Bureau, and land use data from Google Earth Engine, the study integrates these datasets into the Soil & Water Assessment Tool (SWAT) to simulate sediment transportation in the Wu River Basin. Additionally, we will incorporate AR6 climate change datasets from the Climate Change Projection and Adaptation Knowledge Platform Project (TCCIP) to comprehensively assess the impact of climate change on sediment transportation in the Wu River Basin.
HS12-A011
Vibration Behavior Analysis of Bridge Piers Subjected to Erosion by Using Triaxial Accelerometers
Mao Chi WU#+, Dong-Sin SHIH
National Yang Ming Chiao Tung University
The climate in Taiwan is highly changeable, and heavy rainfall and flash floods frequently occur during the rainy season. With the increased discharges, the erosion around the bridge piers intensifies, threatening the stability of the bridge. This study explores the damage to bridge pier foundations caused by riverbed erosions. The riverbed and pier erosion flume experiments will be conducted in the National Yang-Ming Chiao Tung University laboratory. The study applies the novel vibration monitoring technology, a triaxial accelerometer, to detect the vibration caused by flow and scours. The study uses the Fast Fourier Transform to convert the signal from the acceleration domain to the frequency domain. As erosion depth increases, the load-carrying capacity of the bridge pier foundation is reduced, and the structure's stiffness and consequent vibrations are expected to decrease. This study designs four different discharges and two types of density of bridge piers to study this issue. The vibration frequency varies during the scouring process and tends to stabilize accordingly as the equilibrium scours. The study observed a significant vibration of vibration frequency before the pier collapsed. The oscillation between the stable frequency of equilibrium erosion and lower frequencies is apparent. The variations in the tilt angle of the bridge pier model are also observed during the erosion process. Finally, this study proposes a dimensionless empirical formula including pier diameter, the median particle size of the bed, Froude number of the flow, vibration frequency, pier density, and compressive strength of pier material to estimate the scouring.
HS12-A004
Optimal Deployment of Flood Control Facilities in Urban Areas Using SWMM-NSGA-II Approach
Ping-Hsuan HUANG, Jiun-Huei JANG#+
National Cheng Kung University
Under the influence of climate change and urbanization, flooding in cities has become severer due to the increase in rainfall intensity and decrease in space for flood control facilities. To reduce urban flooding, an algorithm was proposed in this study to optimize the deployment of flood control facilities through the combination of the SWMM (Storm Water Management Model, developed by the US Environmental Protection Agency) and the NSGA-II (Non-dominated Sorting Genetic Algorithm II). The algorithm performance was tested based on the SWMM simulation results under different rainfall return periods with multiple objectives including minimum cost, maximum flood reduction, and maximum carbon emission reduction. The sizes, numbers, and locations for detention ponds and seven types of LIDs (Low-impact development) were set as variables for optimization. Finally, the manhole surcharge discharges calculated by SWWM were input into the TELEMAC-2D to demonstrate the flood scenarios on the ground.
HS12-A012
Reservoir Level Measurement Via Satellite Altimetry: MoRLa - Innovative Filtering Approach
Kwanghee HAN1,2#+, Seokhyeon KIM3,1, Rajeshwar MEHROTRA1, Ashish SHARMA1
1UNSW Sydney, 2K-water, 3Kyung Hee University
As climate change and evolving water management policies increase the urgency for reliable hydrological monitoring, the task of accurately gauging reservoir levels becomes crucial. This is particularly true for areas lacking ground-based data. Our study introduces MoRLa: Measurement of Reservoir Level from Altimetry, a software innovation that refines satellite altimetry data to produce dependable water level estimates for such under-monitored regions. MoRLa uses dynamic water masks and three additional filters based on physical reasons to avoid the unreasonable removal of extreme values linked to natural disasters like floods and droughts. A significant discovery in our study is the effectiveness of the “dynamic water mask”, which is adopted differently based on actual water levels for each track, in reducing the compromise between data accuracy and conservation experienced in earlier water mask applications. We applied MoRLa in the Korean Peninsula, particularly focusing on the Hwang-Gang dam, where unannounced water discharges into downstream South Korea frequently cause substantial human and material damage. With the use of the software, we observed a considerable improvement in raw data accuracy in terms of ubRMSE, showing an increase from 3.25m, 1.16m, 0.87m, 0.35m to 1.49m, 0.08m, 0.24m, 0.26m for all type of satellites (Cryosat-2, ICESat-2, Sentinel-3A and B) covered in this study compared to using the maximum level water mask that possibly includes erroneous measurements, while keeping 73.2% to 91.5% of the total data amounts . This improvement represents a significant step forward in balancing data accuracy with data preservation, addressing a previous trade-off. The implications of our study are profound. It offers a method to significantly enhance the accuracy and reliability of water level data, which is crucial for effective transboundary water resource management in the face of the challenging dynamics of climate change and policy shifts.
Session Chair(s): Ashish SHARMA, UNSW Sydney, Ze JIANG, UNSW Sydney
HS13-A001
| Invited
Impact of Soil Texture on Agricultural Drought Evolution and Field Capacity Estimation in Humid Region
Meixiu YU#+
Hohai University
Soil moisture is an important indicator for monitoring agricultural drought, and is closely related to soil texture. However, the role that soil textures play in agricultural drought evolution in humid climates is not well understood. In the study, we systematically assessed the feasibility of the Soil Water Deficit Index (SWDI) for agricultural drought monitoring in humid regions, examined the impact of soil texture and groundwater depth on agricultural drought evolution, and estimated the field holding capacity for different soil textures in humid areas based on a large-scale regional soil moisture monitoring network. The results show that: (1) The SWDI has reasonably good performance in detecting severe and extreme agricultural drought, but it tends to overestimate the drought intensity during non-severe/extreme drought periods in humid regions, particularly for clay soils. (2) Sand soils are more prone to agricultural drought than clay soils, which are more resistant to severe and extreme agricultural drought with high air temperatures and low precipitation. (3) During drought aggravation, clay soil showed a delay of about 0-18 weeks from the lowest SWDI to the maximum groundwater depth, while the delay was only 0-5 weeks for non-clay soil textures. (4) The 95th percentile is proposed as the best estimator of field holding capacity for clay and loam, while Min(maxgs) is the best estimator for sand, loamy sand, and sandy loam. Overall, these findings provide insights into the role of soil texture and groundwater depth in agricultural drought evolution in humid regions, and offer practical guidance for field holding capacity estimation for different soil textures.
HS13-A011
A Global Impact Assessment Framework for Attributing Shifts in Hydrological Risks of Anthropogenic Climate Change
Jin PAK1#+, Suyeon MOON2, Yusuke SATOH1, Fraser LOTT 3, Seung-Ki MIN4, Hyungjun KIM1,2
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo, 3Met Office Hadley Centre, 4Pohang University of Science and Technology
Hydrological extremes have caused considerable damage compared to other disasters, and it is anticipated that climate change will further amplify these damages. This study aims to establish an assessment framework for estimating the shifts in hydrological risks induced by man-made climate change. We tested the framework with floods and droughts that occurred worldwide in 2022. Total runoff data from the HadGEM3-A-N216 large ensemble simulations fed a global hydrodynamic model (Catchment-based Micro-scale Floodplain; CaMa-Flood). To assess the human impacts, two sets of experiments, historicalExt and historicalNatExt (with and without anthropogenic forcing, respectively), have been compared. WeThe results show that, in general, RR and FAR increase as the river discharge get closer to extreme values, which indicates that human influence had a more significant impact on severer extreme events. For example, The Volga River showed maximum values for RR (44.76) and FAR (0.78) at the 99.9th percentile of river discharge. This suggests that the likelihood of flooding increased by 44.76 times, and 78% of the risk was attributed to human-induced climate change. Regarding socioeconomic impact assessment, we calculated changes in the exposed population and gross domestic product for both disasters. While an increase in physical risk generally led to an increase in socioeconomic damage in most regions, some areas exhibited a discrepancy between them due to the spatial mismatch. This indicates the necessity of impact assessment not only for physical risks but also from socioeconomic aspects. Our quantitative impact assessment framework can provide essential evidence for "Loss and Damage" agenda agreed upon in COP27, 2022 and also provides crucial insight into flood management strategies.
HS13-A008
| Invited
Identifying the Dominant Meteorological Factors Influencing Extreme Rainstorms Via a Novel Method Based on the Cumulative Distribution Function (CDF)
Xia WU#+
Taiyuan University of Technology
Extreme floods are often linked to intense rainstorm systems, but these systems can vary in their synoptic characteristics. Understanding the causative processes behind extreme rainstorms can aid in analyzing flood frequency and evaluating changes in flood occurrence and magnitudes. This study focuses on identifying the primary meteorological factors influencing extreme rainstorms using the ERA5 hourly reanalysis dataset in Henan, central China as a case study. Past 72-hour extreme precipitation events are examined, considering six potential factors: precipitable water (PW), average temperature (Tavg), temperature difference (Tdiff) between 850 hPa and 500 hPa, relative humidity (RH), convective available potential energy (CAPE), and vertical wind velocity (Wind). By employing metrics based on the cumulative distribution function (CDF), the drivers of each event and the dominant factor at a specific location are determined. In the central Chinese region of Henan, Wind and PW are found to be the primary factors during summer, while CAPE and Wind show a close relationship during winter. Specifically, for Zhengzhou city, Wind is identified as the main driver for extreme rainstorms in summer, whereas CAPE plays a crucial role in extreme precipitation events during winter. These findings emphasize the significance of considering strong water vapour transport during summer and atmospheric instability during winter for flood warning and mitigation. On the other hand, temperature-related factors have limited influence on the occurrence of extreme events in this study area. Analyzing the dominant factors provides valuable insights for future flood estimations and forecasts.
HS13-A007
Spatio-temporal Variability of Climatic and Hydrological Extremes in the Ajay River Basin, India
Sujata RAY#+, Shivanand MANDRAHA
Indian Institute of Science Education and Research Kolkata
Climatic and hydrological extremes are occurring with greater frequency and intensity because of human induced changes in climate. This may cause grave impacts on a nation's socio-economic condition. This study investigates multidecadal oscillations in extreme rainfall, temperature, and discharge of the Ajay River basin, in Eastern India. The quantile perturbation method and the Sen method were used to analyze the climatic variables. The second half of the century shows more intensified anomalies in the annual average of extreme rainfall. Both the annual average as well as the monsoon rainfall extremes show significant positive anomalies in the recent decade with a maximum value of 45%. The annual average of maximum temperature extremes shows a decreasing trend, which may be caused by increasing aerosol concentrations in the region. The extreme daily discharge of the upper basin lies within the natural variability, but the lower basin shows a 7 year long significant positive anomaly with a maximum value of 44%. The total monthly discharge in the lower basin is well correlated with the total monthly rainfall, which is consistent with the river being rain-fed. One-day lag correlation is higher in the upper basin, while two-day lag is prominent in the lower basin.
HS13-A002
Three-step Merging of Daily Multi-satellite Rainfall Products Using Probability Density Function Matching and Dynamic Bayesian Model Averaging
Yunyao CHEN1+, Binquan LI1#, Maihuan ZHAO2, Tuantuan ZHANG1, Zhijun WU1
1Hohai University, 2Yunhe (Henan) Information Technology Co., Ltd.
Fusing satellite precipitation data from different sources is an effective way for obtaining high-quality precipitation estimates. To enhance the accuracy of precipitation estimates, we presented a three-step strategy within a dynamic framework for merging satellite precipitation products. Firstly, the bilinear interpolation was adopted to downscale the spatial resolution of coarse products. Then, the systematic biases in the downscaled products were individually eliminated using the probability density function (PDF) matching method. Finally, the dynamic Bayesian model averaging (DBMA) method was utilized to merge the bias-corrected products, producing a final merged precipitation product with a daily 1-km scale. The three-step framework generated dynamic weights that varied spatiotemporally and was applied to merge three multi-satellite precipitation products, namely the Climate Prediction Center Morphing Technique (CMORPH), Integrated Multi-satellite Retrievals for GPM (IMERG), and Global Satellite Mapping of Precipitation (GSMaP), in the Kuye River Basin of China for the flood season (April to October) from 2008 to 2012. A total of 36 (80%) ground precipitation gauges were randomly selected for calibration and 8 (20%) for validation. The results revealed that the multi-satellite merged product significantly outperformed all original satellite products in terms of five statistical metrics (root mean square error (RMSE) = 6.47 mm and correlation coefficient (CC) = 0.65), and DBMA assigned higher weight (0.34) to corrected CMORPH. Moreover, the corrected CMORPH demonstrated higher skills in northern regions. It was found that the proposed three-step merging approach provided more detailed and significantly improved precipitation distribution information. In addition, we defined five different magnitudes of precipitation, namely light rain, moderate rain, heavy rain, rainstorm, and heavy rainstorm, to investigate the performance of the proposed method. The merged product had smaller variation ranges of the RMSEs and MAEs (mean absolute errors) over these five precipitation magnitudes, indicating more stable precision.
HS13-A009
Enhanced Daily Streamflow Simulation for Future Climates Using a Non-parametric Method with Variable Selection and Transformation
Ze JIANG1#+, Uwe HABERLANDT2, Ashish SHARMA1
1UNSW Sydney, 2Leibniz Universität Hannover
Simulating daily flows is challenging when considering non-stationarity. Non-parametric k-nearest neighbour (knn) resampling techniques have previously been applied successfully to generate stationary daily streamflow. This study aims to develop a knn bootstrap method for simulating daily streamflow in future climate, focusing on optimal predictor identification. The methodology involves resampling observed daily streamflow, utilizing both observed and simulated climatic variables from regional climate models, covering historical and projected future scenarios. Initially, resampling is executed individually for each month, commencing with January, where data from the preceding month serves as a conditional variable for the following one. Subsequently, the simulated monthly flows are disaggregated to daily values. We compare various strategies for identifying optimal predictors, including linear correlation, and partial mutual information with and without variable transformations. The approach is validated using general flow statistics considering current climate and a pseudo future. The method was tested across several catchments in the Harz mountains of Germany comprising five streamflow gauges with extensive daily records. Conditional climate variables were derived from both observations and the German Weather Service’s core ensemble of climate models. Results show that the performance of the approach can be improved with predictor selection and variable transformations. It can reasonably capture changes in the flow regime, especially when resampling is conditional on observed climate data under a pseudo future. This proposed approach and findings contribute valuable insights for enhancing daily streamflow simulation under changing climatic conditions.
Session Chair(s): Shuichi KURE, Toyama Prefectural University
HS19-A010
Quantitative Evaluations of Existing Infrastructure and Adaptation Measures Related to Green Infrastructure for Flood Damage Reduction in Toyama Prefecture, Japan
Ryuto FUJISHITA#+, Shuichi KURE
Toyama Prefectural University
In Japan, floods caused by typhoons and frontal rains are becoming more frequent and causing massive damage. Although multiple hazard assessments and various adaptation measures have been conducted for Japanese rivers, comparison of adaptation measures for different river basins and evaluation of rainfall storage functions using existing infrastructure are insufficient. Therefore, in this study, rainfall-runoff simulations and flood inundation simulations were conducted for five rivers in Toyama Prefecture, considering the effects of climate change, and several adaptation measures were quantitatively evaluated to propose optimal adaptation measures. In addition, the storage effects of reservoirs, paddy fields and others in Toyama Prefecture were evaluated on a sub-basin scale to understand the flood risk reduction effects of existing infrastructure. For adaptation measures, vegetation management in rivers, paddy field dams, a concrete dam reservoir, green infrastructure, and forest conservation management were evaluated in this study. The results of the analysis indicated that paddy field dams and vegetation management may have a significant effect on the Oyabe River. In addition, organizing storage functions will contribute to future studies of effective basin flood control.
HS19-A012
Research Dynamics in the Field of Water Resources on Climate Change in South Korea
Jaehwang LEE#+, Joohyung LEE, Young-Oh KIM
Seoul National University
While the IPCC (Intergovernmental Panel on Climate Change) regularly assesses the risks, impacts, and feasible response strategies to human-induced climate change on a global scale, this typically results in a generalized analysis. However South Korea is experiencing climate change at a rate faster than the global average, necessitating detailed research adapted to the specific circumstances and needs of this region. Ultimately, this study aims to create an IPCC report specifically tailored for the Korean region. For this purpose, the study was divided into three chapters for detailed analysis and organization: firstly, papers documenting observed impacts due to climate change, focusing on harmful factors; secondly, studies on various future climate change scenarios and models, including the uncertainties involved in forecasting; and thirdly, research on adaptation solutions and policies for climate change. Initially, a comparison with the research trend of climate change studies in the water resources sector of South Korea from 2014 to 2018 was conducted. After that, the results were categorized into three agreement levels: robust, moderate, and limited. The latest research indicates a slight increase in observed impacts, rising from 25% to 27% compared to the previous period, a decrease in impact forecasts and vulnerability collectively from 63% to 53%, while adaptation efforts have significantly increased, going from 12% to 20%. This increase in the adaptation sector suggests that the development of practical measures and strategic planning is becoming increasingly vital in South Korea’s response to climate change, signifying a shift towards more specific and effective adaptation strategies for affected regions and communities.
HS19-A015
Anticipating the Amplification of Flood Hazards in Java Island: A Climate Change Projection
Yeremia SIHOMBING1#, Mohammad FARID1+, Mohammad Bagus ADITYAWAN2, Arno Adi KUNTORO1, Idham Riyando MOE3, Rusmawan SUWARMAN1, Muhammad Rais ABDILLAH1
1Bandung Institute of Technology, 2Institut Teknologi Bandung, 3Ministry of Public Works and Housing
The escalating frequency of flood hazards in the past decade, driven primarily by anthropogenic climate change, poses a significant threat, particularly to Java Island's economic and social fabric. Recognizing the potential impact of floods, it is imperative for Java Island to understand the changing landscape of hazard emergence. This study employs simulations to create flood inundation maps based on historical return periods and climate change predictions. Utilizing data from various BMKG rain-gauge stations for historical context and extreme precipitation predictions from six IPCC models, coupled with the SSP2.45 and SSP4.85 schemes, we employ the RRI (Rainfall-runoff-inundation) model to simulate hydrological data for flood inundation mapping. Notably, the model has undergone calibration and validation in three major basins, demonstrating excellent agreement with observed data. Subsequently, a comprehensive analysis categorizes flood hazards in each sub-district, facilitating the calculation of hazard scores for each province. Consequently, the assessment of hazard score variations between the historical return period and climate change scenarios provides insight into the severity of climate change effects on established hydrology and hydraulic designs. This information is pivotal for both governmental and non-governmental entities in crafting effective policies and mitigation plans to proactively address future floods in vulnerable areas.
HS19-A005
Assessments on Surface Water Resources and Their Vulnerability and Adaptability in China Under the Background of Climate Change
Jia QIN1#+, Yongjian DING2,3, Tianding HAN2, Jinkui WU2, Zhang SHIQIANG4
1Northwest Institute of Eco-Environment and Resources, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3University of Chinese Academy of Sciences, 4Northwest University
A clear understanding of the changes of water resources under the background of environmental changes is of great significance for scientific management and utilization of water resources. This study systematically analyzed the spatial-temporal variations of surface water resources and and their vulnerability and adaptability in China since 2000. It is concluded that runoff of major rivers had been decreasing in eastern China and increasing in western China during 2000-2018. In the arid area of Northwest China, the alpine runoff has shown an overall upward trend since the late-1990s/early-2000s, with a 10%-25% increase caused by the increase of glacial meltwater and precipitation. The increases in precipitation and glacial meltwater with global warming caused a rapid expansion of lakes in the Qinghai-Tibet Plateau and Xinjiang, thus leading to an increase in total area and water quantity of lakes in China from 1995 to 2015. The mean contribution rates of climate change and human activity to runoff change in river basins of China were 53.5% and 46.5%, respectively, during the period of 2000-2010s. The driving factor of runoff change in many river basins has gradually changed from climate change (1950s‒2000) to human activity (2000-2018). During 2000-2018, the contributions of human activities to runoff change were 50%-80% in major rivers of eastern China. The precipitation increase, the application of water-saving technology, the establishment of flood control and drought relief engineering facilities, and the introduction of relevant policies and measures have helped to gradually reduce the vulnerability of water resources in most areas of North and Northwest China (except Xinjiang) from 2000 to 2010s. Based on the typical risk factors and vulnerability characteristics of water resources in different regions, it proposed some targeted adaptive measures correspondingly so as to scientifically deal with the problems of surface water resources in China.
HS19-A001
Hydrological Response to Climate Change and Urbanization of Bicol River Basin in the Philippines
Ernie BAÑARES1,2#+, Muhammad Shafqat MEHBOOB1, Jennifer CACAL1
1University of San Carlos, 2Sorsogon State University
Amidst the intricate challenges posed by climate change, rapid urbanization, and industrial expansion in the Philippines, the impact on the nation's water resources remains a neglected domain in scientific research. Addressing this gap, our study employs Water Evaluation and Planning (WEAP) software and climate forecasts from eight Global Circulation Models (GCMs) to assess the water balance in two vulnerable watersheds of the Bicol River Basin namely, Libmanan-Pulantuna Watershed (LPW) and Quinali Watershed (QW). These areas, sensitive to urbanization, serve as focal points for understanding the holistic implications of concurrent challenges. Through climate-urbanization scenarios, our study predicts future water availability in these watersheds, offering insights for environmental planning. Simulated streamflow aligns consistently with observed data, demonstrating a coefficient of determination (R2) from 0.66 to 0.85 and Nash-Sutcliffe Efficiency (NSE) from 0.57 to 0.67. Projections reveal a warming pattern and fluctuating precipitation in both catchments. Urbanization and industrialization emerge as more significant contributors to water stress than climate change, escalating water demand for domestic and industrial sectors. Quinali Watershed (QW) faces severe water deficiency due to urbanization and population growth, while Libmanan-Pulantuna (LPW) experiences lower unmet water demand. Agricultural scenarios show enduring water scarcity with Low Land Decline (LLD) and a diminishing trend with High Land Decline (HLD) toward 2100. Interestingly, due to declining agricultural land, both watersheds are projected to shift from water-insufficient to surplus regions by the end of the century. Despite the forecasted increase in water availability, urgent measures are needed to address unmet demands, especially in the Quinali Watershed. This study provides a blueprint for sustainable water management in the Philippines and underscores the imperative for timely interventions to mitigate water stress.
HS19-A011
Examination of Available Dataset for Flood Inundation Simulations in Ungauged River Basins, Japan
Hasune NUMAZAWA1#+, Shuichi KURE2
1Graduate School of Toyama Prefectural University, 2Toyama Prefectural University
In recent years, flood disasters have occurred frequently due to heavy rainfall, and the importance of evacuation of residents has been increasing and basin flood control is being promoted. Hence, hazard information needs to be improved. However, small and medium-sized rivers lack hazard information. Therefore, the purpose of this study is to propose a flood inundation analysis method suitable for small and medium-sized rivers with insufficient data by using topographic elevation data. Flood inundation analysis was conducted according to the guidelines for preparing flood inundation area maps for small rivers. The flow rate was calculated using the Assumed maximum rainfall in Hokuriku region. River cross section are created for each granularity of topographic elevation data by 5-meter mesh topographic elevation data, 1-meter mesh aerial laser survey data, and data provided by Toyama City. Calculation of breakwater locations using 1-meter mesh aerial laser survey data. Flood inundation calculations were performed using 5m mesh topographic elevation data for land side. From the results of the analysis, use of river cross-section data prepared by the most detailed data in the existing is recommended. In addition, the breakwater locations should be confirmed by aerial laser survey data and field survey data.
HS19-A003
Sensitivity Analysis of Meteorological Parameters to Understand Processes of Snowmelt Runoff Using Heat Budget Model
So KAZAMA#+
Tohoku University
In order to improve the accuracy of snowmelt estimation, we aimed to estimate vapor pressure distribution with high spatiotemporal resolution, and as a preliminary step, we investigated the correlation between vapor pressure and other meteorological data. The target area is the Yoneshiro River basin, 4,100 km2 and a main channel length of 136 km. One-hour data of vapor pressure data, relative humidity data, temperature data, wind direction data, and snow depth data from January 1 to December 31, 2015 at the Akita AMeDAS observation station. We calculated the coefficient that minimizes the sum of squared differences between the observed value and the regression equation with the objective variable as the relative humidity change and the explanatory variable as the temperature change. At this time, cases were classified into cases with snow and no snow, and cases with easterly winds and westerly winds. It was shown that when there is snow, the sensitivity of humidity is larger than when there is no snow. This is because snow-covered surfaces have low temperatures and low saturated vapor pressures, therefore the amount of water in the air is naturally small. When the temperature rises and the saturated vapor pressure increases, the ratio of humidity to the saturated vapor pressure becomes smaller, which is why the humidity decrease becomes larger. It was shown that when the wind blows from the east, the coefficient of determination is larger than when the wind blows from the west. This is thought to be due to the existence of the sea to the east. It was suggested that consideration of temperature, wind, and the presence or absence of snow cover is important for vapor pressure estimation that accurately estimates snowmelt water.
HS19-A020
Water and Sediment Load Changes and Their Response to Channel Erosion and Sedimentation in the Inner Mongolia Section of the Yellow River
Yin CHEN#+
China Institute of Water Resources and Hydropower Research
With the joint use of reservoirs in the upper reaches of the Yellow River and the implementation of soil and water conservation projects in the basin, the runoff and sediment load in the Inner Mongolia section of the river has changed, and the evolution of river channel has been dramatic. Based on the runoff & sediment load data and topographic information on typical hydrological station section, this paper analyzes the characteristics of runoff and sediment load variation, the evolutionary pattern of siltation by using the trend analysis methods, sediment load transport rate method, and water level-flow relationship in the Inner Mongolia river section. The results show that the annual runoff and sediment load of hydrological station decreased slightly from 1960 to 2020 in the Inner Mongolia river section. While the sediment siltation in the river section is generally on the rise, and the average annual siltation reaches 0.529 billion t. The joint utilization of Longyangxia and Liujiaxia reservoirs in 1987 is the main reason for the rapid growth of siltation, and the siltation is slightly reduced after 2005 in the Inner Mongolia River section. In addition, the critical sediment load coefficients of Bayan Gaole-Sanhu estuary and Sanhu estuary-Toudaoguai river sections were 0.0073 kg·s/m6 and 0.00496 kg·s/m6 from 1952 to1968, respectively, and which were 0.0053 kg·s/m6 and 0.0032 kg·s/m6 from1969 to 2020 respectively. This study can provide technical support for river flood control and reservoir water-sediment regulation in Inner Mongolia.
HS02-A011
Stream Flows Projection Under Changing Climate: A Case Study of Gilgit River in Upper Indus Basin of Pakistan
Arshad MAHMOOD+, Han Soo LEE#
Hiroshima University, Japan
Pro-active water resources management requires assessment of the possible impacts of climate change on the stream flows. Gilgit River Basin, a sub-basin of the Upper Indus Basin (UIB) in Pakistan, has a total drainage area of around 28000 km2, and consists of high elevation terrains with some of the steepest slopes and low elevation trenches. This study aims to project the stream flows in Gilgit River Basin at three different locations, Daniyar, Gilgit, and Alam bridge, under the IPCC climate change scenarios, through the applications of Soil and Water Assessment Tool (SWAT), by considering the physical aspects of the hydrological processes. The performance of the SWAT model for discharge simulations is calibrated in the study area with Modern-Era Retrospective analysis for Research and Applications, version 2 (MERRA-2) reanalysis data for meteorological parameters. In addition, land use land cover (LULC) and soil data were used in the SWAT model from Esri Sentinel-2 and Food and Agricultural Organization (FAO) respectively. During the calibration period, the results of the model in terms of discharge prediction are statistically significant with R2 values between 0.60 and 0.75 for all the three outlets. The model is first calibrated with historical data from 1990 to 2014, and then projected under Shared Socioeconomic Pathways (SSP2 4.5) scenario using Coupled Model Intercomparison Project Phase 6 (CMIP 6) GCM output for flows projection in the mountainous and data scarce regions. This study can be helpful to assist researchers and decision-makers in water resources management in the context of climate change and the resulting extreme flow conditions in the regions, most vulnerable to climate change.
HS02-A014
Assessing the Impact of Climate Change and COVID-19 on Residential Water Use in Seoul: A Study Using Bayesian Deep Learning and CMIP6 Models
Young-Ho SEO#+, Jang Hyun SUNG, Junehyeong PARK
Kangwon National University, Korea, South
The characteristics of residential water use (RWU) can be impacted by climate change and anthropogenic factors. Recently, Korea has experienced a socio-economic drought that has threatened the supply of residential water due to the scarcity of river water as well as COVID-19. Changes in human activity patterns that might be deeply related to climate changes and anthropogenic factors can lead to increased consumption of residential water. In this study, we explored the impact of the COVID-19 pandemic and the temperature rise on the RWU of Seoul, the capital city of Korea, which has a population of approximately 9.8 million. Firstly, it was revealed that there was a correlation of about 0.8 between temperature and RWU from 2015 to 2021. We found increases in estimated RWU due to the increase in temperature, similar to previous studies. However, RWU for 2020-2021 decreased, despite the increase in temperature in Seoul. The reason was found in the fact that the observed RWU decreased linearly as the number of new COVID-19 confirmed cases increased and was demonstrated through the modeling using the number of COVID-19 cases additionally. Secondly, considering the uncertainty in RWU data with short observation periods, we applied Bayesian-based deep learning techniques. We used temperature projection data from 18 climate models in CIMP6, based on the Shared Socioeconomic Pathways (SSP) scenario, to forecast changes in RWU. As a result, the Seoul area is expected to experience an increase in RWU by about 8% for summer and 1% for winter in the distant future (F3: 2071-2100) compared to the current period (H: 198-12010). With the natural recovery ability of precipitation likely to decrease and the instability of water sources increasing, it may become necessary to secure additional water sources in preparation for the increase in RWU.
HS02-A018
Evaluating the Snowmelt Dynamics and Runoff in the Himalayan Region
Suresh DEVARAJ#+, Kasiviswanathan K.S.
Indian Institute of Technology Roorkee, India
Global warming and abnormal human activities have accelerated natural variability of climate. Augmented seasonal changes has witnessed the depletion of snow and ice-covered regions in the Arctic, Antarctic, and the Himalayas (Third Pole) leading to increase in the frequency of disasters. Understanding the Snow cover (SC) extent and snow melt runoff including the impacts of climate change are crucial for the effectively managing water for agriculture, domestic water supply, industries and hydropower generation. This can be accomplished through mapping the snow dynamics for characterising the snow and to model the snow induced runoff. In the present study, an attempt was made to evaluate the snow dynamics and monitor the SC depletion with the aid of Sentinel 1 SAR and optical datasets at a high spatio-temporal resolution. With the temporal SC extent and climatic parameters as input, a robust snow melt runoff model was developed using machine learning approaches to simulate and forecast the stream flow. The study was carried out over Bhagirathi River Basin for simulating inflow to the Tehri reservoir at daily time scale. The developed methodology was also extended to forecast inflow for scheduling the reservoir operation with the aim to maximize the energy generation.
HS02-A019
Optimizing the Deployment of Lid Facilities on a Campus-scale and Assessing the Benefits of Comprehensive Control in Sponge City
Xianbao ZHA1#+, Pingping LUO2, Shuangtao WANG2, Tomoharu HORI1
1Kyoto University, Japan, 2Chang’an University, China
Rapid and intense urbanization has brought a wide range of serious issues like flooding and water pollution, which have become a great concern in a lot of cities. In response to these problems, Sponge City (SPC) has emerged as a potential solution. This study utilized the Stormwater Management Model (SWMM) to simulate urban runoff and determine an optimal combination of Low Impact Development (LID) strategies for reconstructing the study area. Upon analyzing the existing rainwater drainage system and revealed that it could only meet the design return period of 2-years, and identified the vulnerable flood-prone area and the maximum overflow node. After comprehensive consideration of various factors, the sponge reconstruction scenario selected four LID facilities combination: Porous pavement, Rain garden, Sunken green belt, and Green roof. Results indicated that when P=1-yr, 5-yr, 10-yr and 20-yr, the total runoff in the LID scenario decreased by 43.91%, 43.93%, 45.95% and 47.11%, respectively. LID facilities substantially mitigate stormwater runoff and peak flows during moderate to light rainfall events. These LID facilities prove effective in reducing pollutant concentrations (reduction rate is all over 42%), with notable reductions in Chemical Oxygen Demand (COD) and Suspended Solids (SS). This paper offers valuable insights that can serve as a reference for the construction or renovation of SPC, shedding light on effective strategies and considerations for managing stormwater and mitigating the impact of urbanization.
HS03-A008
Hydro-geographical Study on the Water Environment Focusing on River Water in the Islands of East Asia - Targeting Many Island Groups in Japan and Jeju Island -
Koji KODERA1,2#+, Yoshihiro IGARI1,3, Erina YAMAGATA4, Go YAMAKI5, Masaki HORIUCHI3, Masato ODA6, Yoichi MORIMOTO7, Masaki OPPATA1, Erika MIURA8
1Hosei University, Japan, 2Association for Regional and Environmental Sciences, Japan, 3Nippon Koei Co., Ltd., Japan, 4Fukushima University, Japan, 5Kyoshin Giken Co., Ltd., Japan, 6Chiba University, Japan, 7Japan Riverfront Reserch Center, Japan, 8Waseda University, Japan
There are many islands in East Asia, each with its own unique ecosystem and culture due to its maritime and isolated nature. Despite the issue of limited water resources on islands, water is used for agricultural purposes and as a water source for drinking water, and for sustainable use, it is important to understand water quality and the factors that form it. Therefore, in this presentation, we will clarify the relationship between the water quality of rivers and groundwater and the watershed environment in nine island groups in Japan and Jeju Island in South Korea, which the authors have been researching for many years. In most regions, surveys have been conducted several times a year, over several years. During the field survey, we measured basic items such as air temperature, water temperature, EC, pH, and flow rate, analyzed the TOC and major dissolved components of the samples we brought back, and analyzed the relationship with various watershed environmental information. The long-term survey results have clarified the characteristics of the water environment, mainly water quality, on each island, and the factors that form it, and have also clarified the relationship between the basin environment, such as topography and land use, and water quality. Even in the case of Jeju Island, it has become clear that the human influence is having an impact on rivers that flow around populated urban areas and farmland. Comparing water quality characteristics and water quality formation factors between islands, attempting to elucidate the anthropogenic and natural influences on the island water environment and their water quality formation processes, and based on the results, provide guidelines for water environment management on the islands.
HS03-A012
Hydrogeographical Comparison of River Basins in Japan -Focusing on the Mogami River and Abukuma River in the Tohoku Region-
Erina YAMAGATA1#+, Koji KODERA2,3, Yoshihiro IGARI2,4, Yoichi MORIMOTO5, Masaki HORIUCHI4
1Fukushima University, Japan, 2Hosei University, Japan, 3Association for Regional and Environmental Sciences, Japan, 4Nippon Koei Co., Ltd., Japan, 5Japan Riverfront Reserch Center, Japan
During the study, two major rivers in the Tohoku region of Japan, namely the Abukuma River and Mogami River, were selected to compare and examine the differences in their water environment. These two rivers are typical Japanese rivers that flow repeatedly through basins and valleys. However, the Ou Mountains, which extend from north to south in the middle of the Tohoku region, cause differences in snow cover and other factors in the two basins. Furthermore, the water environments, such as elevation, land use and geology, are also different. The study aimed to identify the characteristics of the two river basins and the differences that exist between them. Additionally, the study aimed to examine the factors that influence the formation of river water quality. The study conducted field surveys basically once a month for about a year. The survey and analysis items included water temperature, electrical conductivity, pH, RpH and major dissolved constituents. The results showed that there were differences in electrical conductivity and flow rate changes in both rivers during the snowmelt season from March to June. It was also found that there were differences in river water quality as well as basin characteristics such as land use. The volcanoes, agricultural lands and sewage treatment facilities in the basins were identified as factors that affect river water quality. The findings of this study were significant for future appropriate river basin management.
HS04-A003
Hybrid Deep Learning Models with Physical Process Description for Estimating Plant Transpiration
Xinguang HE1#+, Binrui LIU1, Na LIU2, Xinping ZHANG1, Huade GUAN3
1Hunan Normal University, China, 2Hengyang Normal University, China, 3Flinders University, Australia
Plant transpiration (Ec) estimation models can be broadly classified as physics-based and data-driven models. However, assuming the limitation of individual models, the integration of these two approaches has become a challenging task for Ec modeling under varying water conditions. To address this issue, we improved a simplified process-based model by including soil water potential to explicitly represent the dependence of Ec on root-zone moisture conditions. The improved Ec model (hereafter “BTA-Ψ”) was further coupled into the deep learning (DL) model, and subsequently, three hybrid DL model were developed by using three different integration ways. A Hybrid-Physics-Data (HPD) model is first formed by adding a complementary physical variable, which is generated by BTA-Ψ model, to a DL model along with driving variables to regress Ec. Then, a Physics-based Residual Learning (PRL) model is developed by using the residual learning method to integrate the BTA-Ψ and DL models. Finally, a Hybrid-Physics-Data-Residual Learning (HPDRL) model is constructed by mixing the HPD and PRL models. Three hybrid models are used to estimate daily Ec for the three species of trees and compared with two baseline models, the BTA-Ψ and pure DL models. The results show that the PRL and HPDRL models benefit from the integration of the BTA-Ψ and DL models via the residual learning method, and thus effectively improve daily Ec estimation. In contrast, the HPD model, limited by the flawed physics-based BTA-Ψ model, exhibits the weakest estimation skill among all three hybrid models. Especially, the HPDRL model further exhibits better generalization capability than the PRL and pure DL models.
HS04-A008
Drought Trigger Thresholds for Different Levels of Vegetation Loss in China and Their Dynamics
Wenwen GUO+, Shengzhi HUANG#, Qiang HUANG, Lin YE, Xudong ZHENG, Xiaoting WEI
Xi'an University of Technology, China
Frequent meteorological droughts can negatively impact terrestrial ecosystems by controlling the opening and closing of vegetation stomatal and altering vegetation structure to limit the ability of vegetation to sequester carbon. Due to the lagging and accumulation effects of drought on vegetation growth, drought trigger thresholds for different levels of vegetation loss are still unclear, which is very important for accurately assessing the future impacts of drought on terrestrial ecosystem. Therefore, this study proposed a framework to investigate drought trigger thresholds under various vegetation losses based on copula theory and conditional probabilities, and assessed the dynamics of drought trigger thresholds and possible causes, based on the random forest model. In addition, we used multiple GPP and soil water datasets for the analysis to ensure the robustness of relevant findings. The results show that: (1) there is a generally positive correlation between GPP and SPEI in China, and the response time of vegetation to drought is mostly on a short time scale (less than or equal to 4 months); (2) drought trigger thresholds are also higher in eastern China, with lower vegetation resistance and significantly higher risk of vegetation productivity loss than in other regions; (3) the trigger thresholds in northeastern China show a decreasing trend, with vegetation resistance gradually increasing. CO2 fertilization enhances vegetation drought resistance, but the magnitude of resistance increase is reduced due to the adverse effects of water stress and VPD on vegetation. The findings of this study may advance our comprehension of terrestrial ecosystem vulnerability and response to drought, and further provide scientific guidance for watershed water allocation, drought preparedness and risk management.
HS04-A009
A Convolutional Neural Network-based Ensemble Post-processing Model for Typhoon Precipitation Forecasts in Taiwan
Sing-Wen CHEN1#+, Jing-Shan HONG2, Hui-Ling CHANG3,4, Chuhsing Kate HSIAO1, Charlotte WANG1, Joyce JUANG3
1National Taiwan University, Taiwan, 2Central Weather Bureau, Taiwan, 3Central Weather Administration, Taiwan, 4National Central University, Taiwan
During the summer months from July to September, Taiwan is often affected by typhoons, which are accompanied by substantial rainfall and may lead to disasters such as floods and landslides. To predict precipitation levels, meteorologists frequently employ ensemble weather forecasts using Numerical Weather Prediction (NWP) models. However, the original predictions from NWP models may exhibit systematic errors. Consequently, researchers have explored statistical post-processing methods to eliminate systematic errors and enhance performance in probabilistic forecasting. In recent years, machine learning models such as Support Vector Machines (SVM) and Neural Networks (NN) have been utilized for statistical post-processing. Nevertheless, many existing methods do not consider spatial information, which plays a crucial role in prediction accuracy. In our study, the objective is to design a model based on Convolutional Neural Networks (CNN) to incorporate relationships between grid points. We use datasets related to Typhoon Sudelor and Typhoon Dujuan as examples for statistical post-processing to improve prediction outcomes. Additionally, we propose data augmentation methods and dynamic coordinates to address limitations in typhoon datasets. In our results, we compare the performance of CNN and Fully-Connected Neural Network (FCN) to assess the impact of spatial information. In summary, in most cases, both CNN and FCN outperform ensemble members, with CNN exhibiting superior performance compared to FCN. Furthermore, the results indicate that our proposed augmentation methods and dynamic coordinates are beneficial for prediction. Finally, through the comparison of FCN and CNN, we successfully leverage spatial information between neighboring grid points, aiding in the improvement of probability forecasting.
HS04-A010
A Novel Deep Learning Approach to Runoff Modeling in Dam-regulated Watersheds
Bin YU1+, Yi ZHENG1#, Shaokun HE2
1Southern University of Science and Technology, China, 2Wuhan University, China
While deep learning (DL) has achieved remarkable success in runoff modeling for natural watersheds, its efficacy in heavily regulated systems with large reservoirs hinges on the availability of reservoir operation data. This study introduces a novel framework for explicitly simulating reservoir operation within a DL-based runoff model, eliminating the reliance on inputting operation data. This approach involves constructing individual LSTM networks for the drainage area(s) and the reservoir(s), connected sequentially along the flow path. The reservoir LSTM component explicitly incorporates physical principles like water balance and storage capacity. The cascaded LSTM model was rigorously validated in the Upper Hanjiang River Basin (Hanjiang, the largest tributary of the Yangtze River), encompassing two heavily regulated reservoirs. The model exhibited superior performance in runoff modeling, exceeding 0.7 in Nash-Sutcliffe efficiency (NSE) scores for both reservoir inflow and outflow, and enabling reliable multi-year simulations of reservoir storage. Furthermore, the model successfully emulated the reservoir operation, with three distinct patterns identified for the two cascaded reservoirs. This novel approach paves the way for robustly assessing the impacts of climate change and human interventions (e.g., large water diversion projects) on the hydrology of dam-regulated watersheds.
HS04-A018
A Knowledge Guided LSTM and Its Application in Hydrological Simulations Affected by the Reservoir Operation
Runting CHEN#+, Dagang WANG
Sun Yat-sen University, China
Reservoir operations have caused significant disruptions on the hydrological processes of watersheds with intense human activities. To account for such effects in the monthly runoff simulation, we introduce a knowledge-guided deep learning model designed to emulate reservoir outflow. Prior knowledge, reflecting considerations for flood control, power generation, and water storage, is seamlessly integrated into the loss function of the Long Short-Term Memory (LSTM) network. The reservoir outflow model, coupled with a hydrological model, is employed to simulate streamflow at four hydrological stations in the Dongjiang River basin, where three large reservoirs are actively managing water resources. We assess the performance of three distinct methods: the priori knowledge-based LSTM, the original LSTM, and the conventional Level Pool Scheme (LPS), respectively, in simulating reservoir outflow. It is anticipated that the priori knowledge-based LSTM will outperform the other two schemes, consequently leading to a more accurate simulation of streamflow at hydrological stations. The proposed model serves as a robust tool for investigating hydrological processes under the influence of human activities, offering valuable insights into the complex dynamics of water management in the studied watershed.
HS04-A023
Improving Physically-based Hydrological Modeling with Machine-learning Reservoir Operation Modules
Yilan LI#+, Tongbi TU
Sun Yat-sen University, China
Dams and reservoirs have significantly altered river flow dynamics on a global scale. Accurately representing reservoir operations in hydrological models is crucial yet challenging. Detailed reservoir operation data is often inaccessible, necessitating the reliance on simplified reservoir operation modules in most hydrological models. To enhance the capability of hydrological models in capturing flow variability influenced by reservoirs, this study proposes a hybrid hydrological modeling framework. This framework combines a process-based hydrological model with a machine-learning-based reservoir operation module designed to simulate runoff under reservoir operations. The reservoir operation module utilizes an ensemble of three machine learning models: random forest, support vector machine, and AutoGluon. These models predict reservoir outflows using precipitation and temperature data as inputs. Subsequently, the Soil and Water Assessment Tool (SWAT) integrates these outflow predictions to simulate runoff. To assess the performance of this hybrid approach, the Xijiang Basin within the Pearl River Basin, China, is employed as a case study. The results underscore the superiority of the SWAT model coupled with machine learning-based reservoir operation models compared to alternative modeling approaches. This hybrid model effectively captures peak flows and runoff during dry periods. The Nash-Sutcliffe Efficiency (NSE) in daily runoff simulations demonstrates substantial improvement, ranging from 0.148 to 0.871. Correspondingly, enhancements in the coefficient of determination (R2) range from 0.084 to 0.424, surpassing the original reservoir operation modules in SWAT. In comparison to parameterization techniques lacking a dedicated reservoir module, NSE enhancements range from 0.074 to 0.553, and R2 improvements range from 0.001 to 0.175. The proposed hybrid modeling approach adeptly characterizes the impact of reservoir operations on river flow dynamics, resulting in enhanced accuracy in runoff simulation. These findings provide valuable insights for hydrological forecasting and water resources management in regions influenced by reservoir operations.
HS05-A004
A New GEWEX Regional Hydroclimate Activity in Central Asia
Petrus (Peter) VAN OEVELEN1#+, Sagynbek ORUNBAEV2,3, Maksim KULIKOV4, Michael BRODY1
1George Mason University, United States, 2American University of Central Asia, Kyrgyzstan, 3Kyrgyz Committee on Safety of Large Dams (KyrCOLD), Kyrgyzstan, 4University of Central Asia, Kyrgyzstan
In the early 1990s a newly formed GEWEX Program (Then called the Global Energy and Water cycle Experiment now: Global Energy and Water EXchanges project) launched a regional study to measure and model regional variations in the water and energy cycle. A continental scale experiment was needed to develop the ability to measure and model the components of the water and energy cycles over a macroscale land surfaces from smaller scale observations. These projects are now called Regional Hydroclimate Projects and are much broader than just the geophysical science and cover the entire earth system. In this presentation an overview of the evolution of these RHPs is shown along with a vision on the current and future relevance and importance of such projects along with the necessary additional activities such as cross cutting activities to link regional science to global efforts. In particular the development of a new RHP in Central Asia will be highlighted and how it links to regional activities such as AsiaPEX and Third Pole Environment – Water Sustainability (TPE-WS) RHPs as well as other large scale activities in the region focused on or related to high mountains, water sustainability and ecosystem health.
HS05-A005
Assessing Impact of Seasonal Warming on Permafrost Changes
Ruichao LI#+
Chinese Academy of Sciences, China
Permafrost is experiencing severe degradation in the context of global warming. And the climate warming is distinctly seasonal. The impact of seasonal warming on permafrost changes remains unknown. Here we conducted hypothetical control experiments and used the CLM5 to evaluate the impact of seasonal warming on permafrost change. The results reveal that permafrost changes are highly sensitive to changes winter temperatures. The active layer thickness increases by an average of 0.8 meters for each degree of warm season temperature increase. The active layer thickness increases by an average of 0.6 meters for each degree of cold season temperature increase. This study contributes to the enhancement of understanding the permafrost change to seasonal warming.
HS05-A006
Analysis of the Image of Global Glacier Tourism Destinations Based on Big Data on Tourist Reviews
Jianping YANG#+, Fan TANG
Chinese Academy of Sciences, China
Glaciers are attracting increasing attention in the context of climate change, and glacier tourism has also become a popular tourist product. However, few studies have been conducted concerning the image of glacier tourism destinations. To address this gap in the literature, in this study, we extracted destination images from 138,709 visitor reviews of 107 glacier tourism destinations on TripAdvisor using latent Dirichlet allocation (LDA) topic modeling, identified destination image characteristics using salience−valence analysis (SVA), and analyzed the differences in glacier tourism destination image characteristics across seasons and regions. According to the findings, the image of a glacier tourism destination consists of 14 dimensions and 53 attributes, with landscapes and specific activities representing the core image and viewing location and necessity representing the unique image. We identified significant seasonal and regional differences in the image of glacier tourism destinations. Finally, we discussed the unique image of glacier tourism destinations, the reasons for differences in the images, and the characteristics of different glacier tourism regions. This research could assist in the scientific management of their core images by glacier tourism destinations, as well as in the rational selection of destinations and travel timing by glacier tourists.
HS05-A010
Machine Learning-based Mapping of Fraction Snow Cover in High Mountain Asia by MODIS
Xiaohua HAO#+
Chinese Academy of Sciences, China
Fractional Snow Cover (FSC) is more suitable for reflecting the snow distribution in complex mountainous areas. In this study, the FSC algorithm of MODIS was developed based on the Multivariate Adaptive Regression Splines (MARS) model (LC-MARS) with different land types in the High Asian Mountains (HAM). Finally, the FSC from LC-MARS model is used to compared with the FSC of MOD10A1 and SnowCCI. The results show that: (1) The total Accuracy and Recall of the FSC inversion by the LC-MARS model are 93.4% and 97.1%, respectively, the overall RMSE is 0.148, and the MAE is 0.093, indicating high overall accuracy. (2) Under the same training samples, the inversion accuracy of LC-MARS model is higher than that of the linear regression model in forest areas, vegetation, and bare land, indicating that LC-MARS model is suitable for FSC inversion in the mountain forest area. (3) The overall RMSE of MOD10A1 is 0.178, and the MAE is 0.096; the overall RMSE of SnowCCI is 0.247, and the MAE is 0.131. The accuracy of the FSC product prepared by LC-MARS is higher than that of MOD10A1 and SnowCCI, indicating that the FSC inversion by LC-MARS has certain applications. value. In general, the LC-MARS model can fit high-dimensional nonlinear relationships, and can significantly improve the inversion accuracy of FSC in mountain forest areas. The LC-MARS model has high computational efficiency and is suitable for preparing large-scale long-time series FSC products. In this study, the daily MODIS FSC products in the Asian high mountains from 2000 to 2020 were prepared based on the LC-MARS model, which provided important data support for the research on climate change and hydrology, and water resources in the Asian high mountains.
HS05-A018
Hydrological Dynamics of Glacierized Himalayan Catchments: Insights from Multi-year Tracer-based Analysis on Snow and Glacier Melt Contributions to Streamflow
Tanveer DAR1#+, Nachiketa RAI1, Sudhir KUMAR2
1Indian Institute of Technology Roorkee, India, 2National Institute of Hydrology, Roorkee, India
In this research, we investigated the substantial role of snow and glacier melt as contributors to streamflow in Himalayan catchments, emphasizing their increasing influence as vital indicators of climate change. A comprehensive understanding of these streamflow components is crucial for effective water resource management. Our study focused on three catchments (Lidder, Sindh, and Vishow) in the western Himalayas, employing the spatio-temporal variability of isotopic signatures in various water sources (stream water, rainfall, winter fresh snow, snowpack, glaciers, springs, and wells), alongside hydrometeorological observations and Snow Cover Area (SCA) data. The key findings are as follows: (a) significant spatial and seasonal variability in endmember contributions to streamflow across the three catchments from 2018 to 2020; (b) dominance of snowmelt in streamflow, with varying average contributions in Lidder (spring: 59±9%, summer: 55±4%, autumn: 56±6%, winter: 55±9%), Sindh (spring: 43±6%, summer: 38±6%, autumn: 32±4%, winter: 33±5%), and Vishow (spring: 45±8%, summer: 40±6%, autumn: 39±6%, winter: 32±5%); (c) glacier melt contributions peaking at ~30% during the summer near the source regions; (d) primary uncertainties in streamflow components attributed to spatiotemporal variability of tracer signatures of winter fresh snow/snowpack (±1.9 to ±20%); (e) projections for future streamflow components suggesting up to a ~20% decrease in annual average streamflow in Lidder and Sindh if glacier contribution were to disappear entirely. The study underscores the environmental isotope analysis's significance, providing insights into water resources and a crucial indication of streamflow response to glacier loss amid a changing climate. Our results reveal a complex interplay between cryospheric depletion and its impact on runoff and streamflow, emphasizing the need for proactive environmental management strategies.
HS06-A002
Integrating Photo-sieving and Roughness Analysis to Investigate Grain Size Distribution in a Gravel River
Tung-Yang LAI#+, Chyan-Deng JAN, Kuan-Chung LAI, Hsiang-Wei CHEN, Yu-Chao HSU
National Cheng Kung University, Taiwan
The size and distribution of sediment in rivers affect flow resistance, sediment transport, and the distribution of benthic organisms. Traditional methods of manually sampling sediment are challenging for comprehensive investigations of grain size distribution on a large scale and with high frequency. However, recent advancements in UAV technology and SfM photogrammetric techniques enable researchers to obtain high-resolution orthoimages and accurate 3D point clouds at a reduced cost. These orthoimages can be used for photo-sieving analysis, while the 3D point clouds can establish the roughness distribution on the riverbed surface. This study was conducted in the upstream sections of Hershe River in central Taiwan, involving eight sets of manually sampled sediment particle size investigations and UAV aerial surveys to construct orthoimages and 3D point clouds. The Basegrain software was used for photo-sieving analysis, and the Cloudcompare software was utilized to calculate three roughness metrics, including roughness height, standard deviation, and detrended standard deviation. The study compared the bias between manual sampling and photo-sieving analysis, as well as the relationships between roughness and particle sizes obtained from both methods. The results showed that the bias between D50 obtained from photo-sieving and manual sampling varied from -27.7% to 43.1%, with an average deviation of 20.6%. The correlation coefficients between three roughness metrics and D50 from manual sampling ranged from 0.89 to 0.95, while those between three roughness metrics and D50 from photo-sieving analysis ranged from 0.8 to 0.91. The slope of the relationship between roughness and manual sampling was greater than that of photo-sieving. This study demonstrates the feasibility of integrating photo-sieving analysis with roughness for particle size interpretation, and it suggests that this approach can be applied to various study areas to explore the effects of different particle distributions or levels of material imbrication.
HS06-A007
Evolution of River Networks Towards Energy-efficient Network Patterns
Dnyanesh BORSE#+, Basudev BISWAL
Indian Institute of Technology Bombay, India
Channel networks across fluvial landscapes are believed to evolve towards minimizing energy expenditure, as evidenced by the resemblance between computer-generated optimal channel networks (OCNs) and actual river networks. However, the specific drivers behind these organizational patterns in river networks are not fully elucidated. Here we show using a probabilistic model that efficient organization of river networks is a consequence of basic natural processes and inherent landscape heterogeneity. We demonstrate this model using a planar matrix as a landscape where the flow directions of the network at all pixels are changed iteratively. We suggest that the higher-order channels with higher drainage areas would be relatively more stable than the lower-order channels. We use a power function to make these probabilistic changes in flow directions, where exponent (η) represents the extent of heterogeneity or stability corresponding to the drainage area. The higher η represents less heterogeneity or higher stability of drainage networks and vice versa. When we employ the starting point in the model as a random Eden-like network, we observe that a positive η value leads to a gradual reduction of ΔE over time. Interestingly, the most efficient networks are observed to emerge at η=0.5, suggesting that heterogeneity has an equally important role in minimizing energy expenditure. Striking the appropriate balance between forces trying to retain and modify the network leads to the network equally efficient as the optimal network obtained from the OCNet optimization model. Analysis of 10 islands, showing ΔE (%) between 5.6 and 29.1, supports the notion that natural landscapes rarely attain optimality, underscoring the challenges in predicting landscape evolutionary trajectories. The proposed framework holds promise for explaining the evolution of other tree-like networks in nature and for developing more efficient optimization methods for practical applications.
HS06-A012
Catchment-wise Evapotranspiration Based on the Maximum Entropy Production Principle
Kwanghun CHOI+, Kyungrock PAIK#
Korea University, Korea, South
Estimation of the catchment-wise evapotranspiration is pivotal for long-term rainfall-runoff analysis, but is challenging due to its complex nature and rarely available data. Recently, the Maximum Entropy Production (MEP) principle has shed new light in the evapotranspiration estimation. However, the MEP-based model has been tested only for a point (mostly flux tower sites) to date, and no applications attempted for the catchment scale. On this background, for the first time, we attempted to apply the MEP principle to obtain the catchment-wise evapotranspiration of the Daecheong and Chungju catchments in Korea. Model inputs of radiations, meteorological conditions, and botanic vigor were from the remote sensing data. Estimation results are evaluated through the water budget analysis with the measured precipitation and dam inflow data supplied by the Water Resources Management Information System. Our research suggests that the MEP-based evapotranspiration model is a powerful tool in hydrological utilization in the catchments scale.
HS06-A014
Experimental Study on Sediment and Flood Inundation Countermeasures by Sand Reservoir
Mikako ISHIKURA1+, Ichiro KIMURA1#, Norio HARADA2
1University of Toyama, Japan, 2Mitsui Consultans Co.Ltd., Japan
In recent years, sediment and flood inundation frequently occurs. To mitigate the disaster, we conducted a hydraulic experiment focusing on the effect of sand reservoir and the influence of the presence of driftwood on the sand capture ratio. In addition, we discuss on the possibility to establish the optimized design method for sand reservoir for disaster mitigation. The experimental apparatus was assumed to be about 1/100 of the actual scale, and three types of reservoirs with different widths are installed at the outlet of an inflow channel. Sand with average diameter 0.0665 cm and 7cm long driftwood model with specific gravity: 0.82 were used. The deposition shape of the sediment is measured with a 3D scanner. Remained sand in the reservoir is collected and dried in a furnace, and the capture ratio is determined. In the results, it is shown that sediment was temporarily stored in the sand reservoir, and the effect of suppressing the rapid sediment runoff was observed. The case with a larger width of the reservoir is more effective to decrease the total runoff of sand. In addition, the sand reservoir can delay the sand discharge and decrease the peak discharge of the sand. To check the influence of driftwood, wood models were supplied together with sand with different timing. It was found that the capture ration of the sand increases as the driftwood supply was made in more early time. Driftwood is generally considered to be one of the factors that aggravates disasters. However, the present result implies the possibility that driftwood contributes to disaster mitigation under certain conditions.
HS07-A014
Multidimensional Assessment of Global Dryland Changes Under Future Warming in Climate Projections
Cicheng ZHANG#+
Hunan Normal University, China
Drylands are the homes to over one-third of the world’s population, and are vulnerable to anthropogenic climate change. Based on climate projections, recent studies reported a substantial expansion of global drylands in the coming decades and attributed that expansion to future warming. However, the expansion of drylands contradicts a widespread vegetation greening and a slight runoff increase in dryland ecosystems in the same climate models. Here we re-examine changes in global drylands for the coming century and at two future warming targets (1.5 oC and 2 oC warming relative to the preindustrial level) based on outputs of climate models who participated in the CMIP5. In addition to aridity index (AI) that has been widely used to measure the atmospheric aridity, we also assess changes in drylands from the hydrologic and agro-ecological perspectives, using runoff (Q) and leaf area index (LAI) as indicators, respectively. Our results show that when the impact of elevated atmospheric CO2 concentration ([CO2]) on vegetation water consumption is considered in the estimation of potential evapotranspiration (EP) and AI, the expansion of atmospheric drylands is at a much slower rate (~0.16% per decade under RCP4.5 and ~0.30% per decade under RCP8.5) than previously reported. Moreover, the additional 0.5 oC does not lead to an evident further expansion of atmospheric drylands. In terms of hydrologic and agro-ecological drylands, both of them show significant shrinks over the coming decades, suggesting reduced hydrologic and agro-ecological aridity in the region. Finally, contrasting with previous perceptions, our results demonstrate that warming only plays a minor role in altering global drylands from all three perspectives. Increases in net radiation are primarily responsible for the expansion of atmospheric drylands, and increases in P and [CO2]-induced increases in vegetation water use efficiency are the key drivers of changes in hydrologic and agro-ecological drylands.
HS07-A018
Statistic Evaluation of Low-frequency Acoustic Wave Impact on Rainfall Stimulation
Mengyao WANG1#+, Ji CHEN1, Jiaye LI2, Jinzhao WANG3
1The University of Hong Kong, Hong Kong SAR, 2Dongguan University of Technology, China, 3Qinghai University, China
For securing more water resources, traditional solutions including seawater desalination are limited due to high cost and restricted operating conditions. Thus, acoustic stimulation of rainfall is a potential alternative method due to its low cost and convenient operation. Low-frequency acoustic field can be used to stimulate rainfall through evoking wavy motion of air particles in clouds which will significantly enhance the process of collision coalescence of cloud droplets and lead to their volume increase. Nevertheless, there is still a lack of rational methods to evaluate the effect of acoustic enhancement of rainfall in field experiments. To this end, in this study, nearly two-month field experiments of acoustic rainfall enhancement with 39 trials were carried out by our research team in the Tibetan Plateau. Statistical analysis was applied to evaluate the effect of acoustic wave on precipitation stimulation. The results of average rainfall intensity distribution using ordinary least square analysis disclose that acoustic interference has a considerable effect on rainfall enhancement.
HS08-A009
Unraveling the Nexus of Environmental Factors and Fish Interactions
Zhaofeng HAN1#+, Ji CHEN1, Yi LU2,1, Qian XU1
1The University of Hong Kong, Hong Kong SAR, 2Hong Kong Metropolitan University, Hong Kong SAR
As crucial sources of fresh water and food, rivers sustain diverse ecosystems and contribute to the overall well-being of communities. However, the rapid pace of economic development has introduced unprecedented challenges, exerting immense pressure on river systems. This escalating pressure, driven by urbanization, industrialization, and agricultural expansion, poses a significant threat to the delicate balance of environmental and ecological conditions in aquatic environments. In light of the escalating threats to riverine ecosystems, there is an urgent need to delve deeper into the various interactions among water movement, pollutant transport, and biological organisms. This research is motivated by the imperative to elucidate the underlying mechanisms driving the environmental and ecological changes in river systems. A comprehensive understanding of these interrelationships is essential for formulating effective strategies to protect and restore riverine ecologies in the face of rapid economic development. Results indicate that structural equation modeling provides a more nuanced comprehension of both direct and indirect effects of environmental factors on fish compared to conventional methods like linear fitting and principal component analysis.
HS08-A010
Study on the Origin of High Sulfate Groundwater and Its Influence on Carbon Cycle in Karst Groundwater in Shanxi Province
Xiaojuan QIAO1,2#+, Yu CHENG1, Xinyu CHAI1
1University of Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China
This paper analyzed the formation mechanism of high sulfate groundwater in the karst spring basin in the north. The sulfate (i.e., sulfur oxide end-members) proportion from sulphuric acid weathering carbonate rocks and was determined quantitatively. And then an improved method was established based on hydrochemical-runoff method. The main research conclusions o are as follows: The chemical type of groundwater in the study area is mainly changes from HCO3-CaMg and HCO3·SO4-Ca to HCO3·SO4-Ca·Mg along flow direction. The average concentration is 333.74 mg/L which exceeds the standard by 60% in karst water samples. The formation of chemical components in groundwater is mainly controlled by weathering of carbonate rocks and evaporative karst decomposition, but also interfered by human activities. Based on the δ34SSO4 and δ18OSO4 values of each source, IsoSource model results showed that the average contribution rate of gypsum end element, mine water end element, atmospheric precipitation end element and fertilizer end element were 54.50%, 29.37%, 7.75% and 8.38%, respectively, which indicate that the geochemical background of gypsum development is an important factor of groundwater pollution in the study area, and the total sulfate contribution of sulfuric acid from different sources (atmospheric acid deposition and sulfide oxidation in coal seam) is larger. According to the improved method, the net carbon sink in the rainy season (June to July) and the dry season (November to December) were 1.20 t and 1.07 t, respectively, and the potential carbon sources were 0.68 t and 0.94 t, respectively. Sulfuric acid weathering accounts for 36.0% and 46.6% of the total weathering of carbonate rocks in rainy season (June ~ July) and dry season (November ~ December). Sulfuric acid is involved in chemical weathering of carbonate rocks to a greater extent.
HS08-A011
Seasonal Changes in Nutrient Loads Along the Korean Peninsula (2012-2021): Contributions of Streamflow and Nutrient Concentration
Yena KIM+, Jonghun KAM#
Pohang University of Science and Technology, Korea, South
Under the hydrological cycle, atmospheric pollutants undergo wet deposition to the land surface and the nutrients on the land surface flow out to the coast through streamflow. Research on the total inland nutrient fluxes and the changes is essential to investigate changes in the aquatic ecosystem and water quality of coastal regions. However, assessment of the total nutrient fluxes discharging from land to the coast of the Korean Peninsula on a national scale remains limited. In this study, the total nutrients (TN, TP, Chl-a, and TOC) discharging from the inland to the coast of the Korean Peninsula were estimated over 2012-2021. The changes in the nutrient fluxes were investigated by season, coastal region, and the species of nutrients. A quantitative budget analysis was performed to find out how much the streamflow and the concentration of nutrients contribute to the change in total nutrient loads. Results showed that the seasonal and regional characteristics were various, depending on the nutrient species and season. During spring and winter, the contribution of the western coastal region of the Korean Peninsula to the total nutrient load was the largest. In summer and fall, the contribution of the Southern coastal region increased relatively. TN and TOC showed that the contribution of the change in streamflow was dominant (more than 84%) during four seasons. TP shows that the contribution of the concentration change was dominant and relatively larger than other species. Chl-a showed a more complex pattern in summer and fall. This study highlighted the hydrological linkage between inland and coastal regions via the hydrological and nutrient cycles over the Korean Peninsula.
HS08-A012
Investigating Parameters of Light-response Curves and Heat Flux Components from Fluxnet Sites
Jiyeong KIM+, Kyungrock PAIK#
Korea University, Korea, South
As global warming intensifies, better understanding natural carbon cycle has become important than ever. In this regard, the Gross Primary Production (GPP), which serves as a key quantity that represent the capability of ecosystem to hold carbon, needs to be well estimated. The GPP can be estimated from Light-Response Curves, which simply describe the GPP as a function of radiation with two parameters of the canopy light utilization efficiency (α) and maximum carbon uptake rate of the canopy at light saturation (β). We analyze how the latent heat flux (L) and energy storage (dS/dt) vary at daily time scale, with varying α and β. We investigated three Fluxnet sites of different vegetation in the United States. α and β exhibit a seasonal pattern, revealing differences among vegetation types. Especially the difference between C4 and C3 plants is noticeable. L and dS/dt also display a seasonality, like that of the GPP, showing differences among vegetation types. Overall positive correlation has been found between α, β, and energy balance components.
HS08-A014
The Impacts of Extreme Climate Change on Water-carbon Cycling Processes in Typical Subtropical Hilly Region of South China
Dandan REN+, Shuguang LIU#, Yiping WU
Central South University of Forestry and Technology, China
The rising extreme climate events, as one of the most typical features of climate change, have a great impact on the structure, composition and functioning of regional water-carbon ecosystems. Assessing the evolution of extreme climate events and their water-carbon effects can provide an important scientific basis for human society to mitigate and adapt to climate change. Previous studies focus on the influences of a single extreme climate on the water cycle or the carbon cycle, ignoring the comparison of the impacts of multiple extreme climate events on the coupled water-carbon cycle under long-term series in watershed scale. In this study, a framework combing observations and the SWAT-Daycent coupling model was used to characterize the spatial-temporal features of extreme climate events (i.e., drought, extreme precipitation, extreme heat, and extreme cold) and key components of the water cycle (i.e., ET, soil water) and carbon cycle (i.e., NPP, SOC) in the Xiangjiang River basin (XJRB) from 1970 to 2022. Then, the impacts of extreme climate events on the water-carbon cycle are quantified. The satisfactory performance of the coupled model demonstrates that the SWAT-DayCent model is capable of simulating water-carbon cycles processes at the watershed scale in the subtropics of China. Indicators of extreme precipitation and extreme temperature events in the XJRB in the past 53 years have shown an increasing trend. The correlation analysis between water and carbon cycle revealed that a tightly coupled relationship exists between soil water and NPP, while the synergy effect of ET and NPP towards decoupling gradually under the effects of extreme climate change. Our research highlights the importance of the interaction effects of multiple extreme climate events on the coupled water-carbon cycles. This study can contribute to formulating sustainable management strategies in humid subtropical regions and elsewhere in the world.
HS09-A001
Spatial Propagation Mechanisms of Lagged Compound Hydroclimatic Extremes Revealed by Complex Climate Networks
Hui-Min WANG+, Xiaogang HE#
National University of Singapore, Singapore
Extreme droughts and pluvials are recurrent natural hazards that often lead to disastrous socio-economic impacts. These hydroclimatic extremes are generally characterized by large-scale spatial-temporal patterns spanning thousands of kilometres with time-evolving features of expansion or shrinkage. The spatial-temporal dynamics of these hydroclimatic extremes can pose compound impacts across multiple locations. Understanding the propagation behaviour, including movement and propagation, is crucial for disaster response and mitigation. The spatial propagation dynamics of droughts/pluvials are inherently complex as they are often associated with and modulated by natural climate variability, such as El Niño-Southern Oscillation (ENSO), North Atlantic Oscillation (NAO), and atmospheric dynamics like Rossby waves. However, the specific influence of these drivers on the spatial propagation pathways of droughts and pluvials remains elusive. Here, we conduct a multi-layer complex network-based analysis to explore the interactions between drought/pluvial propagation pathways and potential modulating mechanisms with a focus on the conterminous United States. We first identify extreme drought and pluvial occurrences using self-calibrated Palmer Drought Severity Index (scPDSI) and Standardized Precipitation Index (SPI) during 1948–2016. We then apply event coincidence analysis (ECA) for all location pairs to construct fully-connected drought and pluvial complex networks, based on which we identify the spatial-temporal propagation pathways through community analysis. Subsequently, partial event coincidence analysis is carried out to elucidate the direct links from potential climate modulators (e.g., ENSO, NAO, and Rossby waves) to extreme event propagation. Our results provide insights into how climate variability and large-scale circulation patterns affect the spatial propagation of droughts and pluvials, offering valuable information for pre-emptive actions to mitigate remotely synchronized extreme events.
HS09-A007
Drought Dynamics in Southeast Asia: A Case Study of the 2014 Dry Spell Over Singapore and Malaysia
Shuping MA+, Xiao PENG, Xiaogang HE#
National University of Singapore, Singapore
In early 2014, regions within tropical Southeast Asia, including the Malay Peninsula and Singapore, are stricken by a severe drought. Remarkably, Singapore experiences its longest recorded drought since 1929, spanning 62 days from January 13 to March 15. We find that during the drought period, there is no El Niño phenomenon, which is generally considered most related to tropical droughts. Instead, the Atlantic sea surface temperatures show a tri-polar pattern, through which ocean-atmosphere interactions cause abnormal atmospheric circulation patterns. These further induce positive geopotential height anomalies over Southeast Asia that lead to the convergence of mid-level airflows and subsidence. Along the abnormal anticyclone, dry airflows from the west intensify the subsidence. We find that the seasonal averaged vertical motion (Omega) anomaly during 2014 Jan-Mar is unprecedented in the observational record from 1980 to 2020, with a return period of Omega likely (>66% probability) in the range of 40~92 years and the median is 137 years. However, this return period is likely underestimated if the compound impact of mid-level dry air and vertical motion is jointly considered with a bivariate return period likely exceeding 43~98 years. Climate projections based on the latest Coupled Model Intercomparison Project Phase 6 (CMIP6) models indicate that the frequency of the 2014 Singapore drought is likely to increase by twice in a business-as-usual carbon emission scenario. In addition, the dynamical process is identified as the primary factor that will heighten the drought frequency similar to the 2014 event in the future.
HS11-A010
Enhancing Urban Flood Predictions with Deep Learning-based Super-resolution
Hyuna WOO+, Hyeonjin CHOI, Minyoung KIM, Songhee LEE, Seong Jin NOH#
Kumoh National Institute of Technology, Korea, South
With the increasing frequency and scale of urban flood events caused by rapid climate change, it is important to provide rapid inundation prediction information for urban areas. High resolution urban inundation simulations using physically- and deep learning- based models require significant computational resources and costs. In this study, we develop and evaluate a method for producing high-resolution urban inundation information using a deep learning based super-resolution technique. The proposed super-resolution method can enhance low-resolution inundation information images to high resolution while maintaining as much of the physically based inundation information as possible. The implemented methods include CNN- and GAN-based deep learning methods. CNN-based super-resolution model directly maps low to high resolution using convolutional layers, while GAN-based super-resolution model leverages adversarial training to enhance the visual fidelity of low-resolution inundation information. The study area is the western region of Portland, OR, USA. The resolution enhancement performance is evaluated via quantitative indicators of the inundation image RGB spectrum. The proposed methods are expected to efficiently improve the computer resource and computation time compared to conventional physics-based models and support real-time flood predictions with high spatial resolution.
HS12-A001
Flooding Impact Assessment of Multi-hazard Under Climate Change Scenarios
Yi-Hua HSIAO1#+, Chun-Che CHEN1, Wei-Bo CHEN1, Ting-Yu LIANG1, Chia-Fa CHI1, Chih-Tsung HSU2, Dong-Sin SHIH3
1National Science and Technology Center for Disaster Reduction, Taiwan, 2Academia Sinica, Taiwan, 3National Yang Ming Chiao Tung University, Taiwan
In the past, the main focus was on assessing the hazard caused by a situation. For example, heavy rainfall events, drought, flood, landslide, storm surge, etc. A hazard analysis can discuss some of the risks and impact processes, but it is difficult to integrate and evaluate the multi-risks caused by different driving forces. According to the World Bank’s report, about 3.8 million km2 area and 790 million people in key natural hazard are highly exposed to two disasters at the same time; about 500,000 km2 area and 105 million people are exposed to 3 or more disasters. Therefore, it is necessary to assess multi-hazard risk. Multi-hazard mainly analyze the impact of different hazards on the same exposed target driven by the chain effects that occur "at the same time" or "sequentially". This study discusses the overview of flooding impacts caused by different hazards such as typhoon rainfall events and sea level rise. Flooding simulation of multi-hazard, taking the coast as the test area in Chiayi, Taiwan. The study considers typhoon rainfall events under climate change scenarios, astronomical tide, storm surge deviation, sea level rise estimates. The flooding simulation analysis was conducted based on extreme typhoon events in the base period and the 2°C warming scenario. Use this result to understand the impact of flooding caused by multi-hazard. This will facilitate future assessment of adaptation methods based on different gaps.
HS12-A002
Extreme Learning Machine for Real-time Flood Stage Forecasting
Shien-Tsung CHEN#+, Hung-Ying FU
National Cheng Kung University, Taiwan
This study employed the extreme learning machine (ELM) to create a real-time flood stage forecasting model for Lan-Yang River in Taiwan. It conducted a comparative analysis of forecasting outcomes against both the back propagation neural network (BPNN) and support vector machine (SVM). Gathering data from 41 flood occurrences spanning 1990 to 2021, 26 events were utilized for model calibration and 15 were for validation. The investigation delved into ELM's activation functions and hidden layer neuron quantities, determining an optimal model structure for forecasting flood stages 1 to 6 hours ahead. The findings revealed ELM's superiority over BPNN and SVM. Specifically, ELM's forecasting results showcased correlation coefficients exceeding 0.9 for lead times of 1 to 6 hours, alongside efficiency coefficients surpassing 0.8. Additionally, this study established an additional forecasting model by considering the forecasted rainfalls, and proved that adding forecasted rainfalls can effectively improve the performance of the flood stage forecasting.
HS12-A003
Analyzing Changes in River Channel Patterns Under the Climate Change Scenarios
Yi Hong LIN#+, Cheng-Hsin CHEN, Dong-Sin SHIH
National Yang Ming Chiao Tung University, Taiwan
With global climate change, disasters are occurring frequently worldwide. In Taiwan, extreme rainfall events influenced lead to substantial sediment transport in rivers. This transport process results in changes in river topography and flow paths. According to the 2021 adaptation report from the Water Resources Agency of the Ministry of Economic Affairs, the WuXi River basin faces challenges such as channel overflow, erosion and damage to the foundations of hydraulic structure due to channel oscillations, safety issues with aging embankment structures, land flooding risks, and changes in ecological environments. In the face of these challenges, effectively assessing the potential for river channel changes under extreme climate conditions becomes particularly important. This study focuses on the middle reach of the Wu River, selecting the study area from upstream cross-section 143000_080 to downstream cross-section 143000_037.This area encompasses issues related to hydraulic structures, ecological environments, and urban flooding within the Wu River basin. To address these concerns, the study integrates United Nations climate change scenarios (AR6), hydrological modeling (HEC-HMS), and river hydraulic bed modeling (SRH-2D) to simulate sediment transport in the river. The analysis explores different climate change scenarios, examining how changes in upstream inflow and sediment transport quantities correspond to variations in river channel evolution and sediment deposition. The climate change scenarios are based on the AR6 CMIP6 SSP1-2.6, SSP2-4.5, SSP3-7.0, and SSP5-8.5.Utilizing HEC-HMS to calculate boundary inflow and employing the SRH-2D model to simulate sediment movement in the river, with varying inflow rates and sediment transport amounts are simulated to analyze the changes in sediment transport. Based on the simulation results, the pathways of channel changes are analyzed, and the amount of sediment deposition in the river channel is quantified. The computed results are then provided as references for evaluating the safety of hydraulic structures, conducting ecological assessments, and simulating urban flooding, among other relevant fields.
HS12-A005
Fast Simulation of Compound Flooding Using Storm Water Management Model
Yen-Mo WU+, Jiun-Huei JANG#
National Cheng Kung University, Taiwan
Under the influence of global warming, “compound flooding” events caused by the simultaneous occurrence of storm surges and rainfall are widespread in coastal areas around the world. Taiwan is located on the main path of typhoons in the Pacific, which exacerbates the severity of compound flooding in coastal areas due to the combined influence of heavy rainfall and storm surges. Based on the Sustainable Development Goals proposed by the United Nations, it is necessary to produce compound flooding maps for coastal areas under different climate change scenarios as a reference for flood risk assessment. However, the high threshold for building two-dimensional numerical models and the expansive computation time required have increased the cost of compound flood maps. In this study, the one-dimensional SWMM (Storm Water Management Model) developed by the US Environmental Protection Agency was used to simulate the surface compound flooding in a quasi-two-dimensional manner. The fish farms, detention ponds, embankments, rivers, and other hydraulic features were set as individual components and the flow exchanges between these components were calculated using weir flow or pipe flow functions. After inputting rainfall and tidal boundary conditions, the compound flood scenarios for the past, present, and future under climate change can be simulated for compound flood risk analysis. The research results show that compared with the two-dimensional model, the proposed method greatly shortens the simulation time and reasonably displays the flooding depth on the ground in the research area under the combined impact of future rainfall and tidal conditions, which can be used as a reference to formulate compound flooding prevention and mitigation strategies in coastal areas.
HS12-A006
Soil Erosion Potential Map for Gaoping River Watershed
Ching-Nuo CHEN1#+, Chih-Heng TSAI2
1National Pingtung University of Science and Technology, Taiwan, 2Chia Nan University of Pharmacy and Science, Taiwan
Unsuitable development and utilization of land accelerates soil erosion, which has a significant impact on the eco-environment of terrestrial and aquatic ecosystems. The sediments generated from watershed erosion are transported to rivers via runoff, which are the main composition of river sediments and a major source of reservoir or river dam sediment deposition. The degree of soil erosion has a significant impact on the evolution of river channels, influencing river stability, flood prevention safety and river remediation planning. Hence, the control of sediment yield is crucial in catchment management. The object of investigation in this study is Gaoping River watershed. The Integrated Model for Flooding and Sediment-Laden Flow in Entire River Basin is used to simulate soil erosion, sediment yield, distribution of erosion caused by various rainfall events during long-term (from 1996 to 2020). Soil erosion potential maps were established according to the simulation results. The rainfall events of various rainfall patterns and characteristics during the long-term consisted 196 events, which were divided into eight groups of accumulated rainfall intervals. These were further simulated, and average depth of erosion analyzed. Subsequently, soil erosion potential maps were drawn. The results showed that the distribution of the erosion area increases as the cumulative rainfall increased. The accumulated rainfall of more than 200 mm can cause severe erosion in the upstream of Chishan, Laonong, Zhuokou, and the Ailiao Rivers in the upper slopes with steeper slopes and high elevations. Severe erosion increases with the increase in cumulative rainfall. The accumulated rainfall reaches more than 1000 mm, and the river basin is mostly moderately eroded including; the upper reaches of Chishan River with steep slope and high elevation, the upper reaches of Qiongxi River, Laonong River, Zhuokou River, and the Ailiao River. There is a large area of severe erosion in the upper reaches.
HS13-A003
Quantitative Assessment of Peak Flood Discharge: Unveiling Optimal Models for Hydraulic Infrastructure Planning in the Wainganga River Basin
Harshita Rani AHIRWAR1#+, Manish NEMA2, Anupam Kumar NEMA1
1Banaras Hindu University, India, 2SCIENTIST, India
In the realm of hydraulic infrastructure, encompassing structures such as barrages, dams, spillways, and bridges, the imperative lies in meticulous planning, intricate design, and adept management. The crux of this endeavour revolves around estimating the peak flood discharge, a parameter crucially contingent upon the desired return period. Flood frequency analysis is a pivotal method employed for unravelling the zenith discharge within a specified return period. This scholarly pursuit delves into the intricacies of frequency distribution research, specifically directed towards the annual maximum flood data gleaned from the Wainganga River Basin's Ashti, Ramakona, and Satrapur gauging stations spanning the temporal spectrum of 1987 to 2017. Discerning an optimal model for maximum flood analysis necessitates a reasonable examination of various probability distributions, notably the Lognormal, Log Pearson type-III, Gumbel extreme value type-I, and Weibull's technique. The discernment process relies on the meticulous application of goodness-of-fit (GOF) tests, including the discerning Kolmogorov–Smirnov, Anderson–Darling, and Chi-squared tests at a critical value 0.05 tailored to the proposed gauge stations. Noteworthy findings unfold as the Ashti station unequivocally favours the General Extreme Value distribution across all three tests, dictating its supremacy for ascertaining peak discharges at varying return periods. In contrast, the Ramakona and Satrapur gauging sites present a nuanced scenario. Chi-Square introduces a paradigm shift in the distribution hierarchy, diverging from the congruence observed in the Kolmogorov–Smirnov and Anderson–Darling tests. This intricate dissection precipitates the Log Pearson type-III selection for Ramakona and the General Extreme Value distribution for Satrapur. Ultimately, this comprehensive study culminates in the juxtaposition of diverse distributions across distinct gauging stations, offering invaluable insights to guide stakeholders and policymakers in crafting nuanced strategies aligned with the prophesied flood scenarios.
HS13-A005
| Invited
Recent Change of Rainfall Quantiles Based on Regional Frequency Analysis Across South Korea
Ju-Young SHIN1#+, Jun-Haeng HEO2, Jiyeon PARK1, Seoyoung KIM1
1Kookmin University, Korea, South, 2Yonsei University, Korea, South
The rising frequency of extreme rainfall events, intensified by climate change, has led to numerous floods in South Korea, resulting in escalating damage. This increase in variability challenges the dependability of current design standards for hydraulic structures. Consequently, it becomes imperative to revise these criteria to mitigate flood-related destruction. This research involved a regional frequency analysis of rainfall at 615 stations in South Korean, examining the effects of changing design criterion due to the heightened irregularity in extreme rainfall events. Unlike the common at-site frequency analysis, regional frequency analysis, which uses data from hydrologically homogeneous regions, provides more consistent design values: rainfall quantiles. This approach lessens the impact of abrupt changes in design criteria at individual locations from the results of at-site frequency analysis. The index flood method was adopted here as a technique for regional frequency analysis, covering durations from 1 to 72 hours. The study compared the rainfall values of quantiles calculated with data until 2017 against those computed with data up to 2022. Most areas showed no notable change in rainfall quantile, but regions experiencing exceptionally large extreme rainfall events saw a significant increase. These findings highlight the limitations of current design criteria, which are based on existing stationary, in accommodating future variability.
HS16-A002
Estimation of the Carbon Storage by Submerged Aquatic Vegetation
Momoka MARUYAMA1#+, Keisuke NAKAYAMA1, Katsuaki KOMAI2, Tomoyasu FUJII3, Kohji UNO4, Taketoshi SHIMIZU5, Jumpei OMORI6
1Kobe University, Japan, 2Kitami Institute of Technology, Japan, 3Nara University of Education, Japan, 4Kobe City College of Technology, Japan, 5Kobe City Construction Bureau, Japan, 6Kobe City Waterworks Bureau, Japan
As global warming has become an issue in recent years, blue carbon has attracted attention as a source of carbon dioxide absorption in coastal areas. Blue carbon is carbon sequestered or stored by marine organisms through photosynthesis and other processes. Various methods for estimating carbon sequestration in seagrass and seaweed meadows have been proposed. However, all methods require long-term observations and are difficult to apply to all aquatic plants, such as submerged aquatic vegetation with branches. In this study, we proposed a method to estimate carbon sequestration over a year using the dissolved inorganic carbon (DIC) equation. The DIC equation is an equation to determine net ecosystem production (NEP), which is the difference between the amount of carbon released through respiration and that absorbed through photosynthesis. The NEP was estimated with parameters obtained from laboratory experiments and data on hourly photon flux density and water temperature for one year. The growth and density changes of aquatic vegetations were also included in the DIC model. The estimated NEP agreed with other methods. The DIC model showed that the NEP varied widely with parameters and weather conditions.
HS16-A004
Internal Wave Mode in Lake Biwa
Hibiki YONEDA1#+, Keisuke NAKAYAMA1, Tatuya HIRAMI1, Tetsuya SHINTANI2, Kazuhide HAYAKAWA3, Chunmeng JIAO3
1Kobe University, Japan, 2Tokyo Metropolitan University, Japan, 3Lake Biwa Environmental Research Institute, Japan
In Lake Biwa, stratification is generated due to water temperature differences excluding well-mixed winter season. The change in water density induces the formation of internal waves when wind stress is applied to the lake surface. As internal waves affect the ecosystem and environment due to material transport in the lake, it is necessary to clarify the behaviours and characteristics of internal waves. The epilimnion thickness changes seasonally, and the Coriolis and topographical effects influence internal wave periods and amplitudes. Therefore, the study aims to elucidate the internal wave mode in Lake Biwa, theoretically and numerically, with the Coriolis, using the vertical water temperature profile obtained by field observations. Numerical simulation was conducted using a three-dimensional environmental model, Fantom, which revealed that the Kelvin and Poincaré internal waves were induced based on the topographical features under the Coriolis effect. Theoretical solutions also showed internal wave modes comparable to the numerical simulations. Estimated internal wave modes numerically and theoretically agreed with the field observations, suggesting the possibility of defining the internal wave periods in Lake Biwa using the theoretical solutions, enabling the quick estimation of internal wave mode.
HS16-A006
Combining Quantitative Microbiological Risk Assessment and Disability-adjusted Life Years to Assess Urbanization Effect on River-related Recreational Health Risks in the Bitan Scenic Area, Taiwan
Cheng-Shin JANG#+
Kainan University, Taiwan
The Bitan Scenic Area is the famous water-based recreational destination in northern Taiwan. To comprehensively analyze the damage of river microorganism on recreationist’s health, this study was to combine quantitative microbiological risk assessment (QMRA) and disability-adjusted life years (DALYs) to assess urbanization effect on health risks of river activities for recreationists in the Bitan Scenic Area. First, data on monthly river Escherichia coli (E. coli) concentrations were collected between 2014 and 2023 in the Bitan Scenic Area and upstream areas, which are located in the urban and rural regions, respectively. A questionnaire associated with exposure duration, frequency and ages for canoeists, swimmers, and fishers was performed in this area. Then, Monte Carlo simulation was used to characterize the probability distributions of QMRA and DALYs parameters for recreationists. After the uncertainty integration of the probability distributions of the aforementioned parameters, the β-Poisson dose-response function was adopted to quantify annual illness risks induced by river pathogenic E. coli. Finally, DALYs were used to analyze the sum of years of potential life lost and years lived with disability. The probability thresholds of 1×10-6 and 1×10-4 per person per year were regarded as acceptable regulation thresholds of recreational risks. This study results reveal that 90% confidence intervals of the annual disease burden (DB) range from 0.2-74.1×10−6 for canoeists, 0.01-94.0×10−6 for swimmers, and 0.3-128.9×10−6 for fishers in the Bitan Scenic Area. Because DB exceeds acceptable recreational regulation thresholds, recreationists in the Bitan Scenic Area pose a potential health risk. Owing to the urbanization, the DB increases by twice due to increasing river E. coli levels from upstream river sections to this scenic area. To protect recreationists’ health, effluent sewer systems, best management practices, and total maximum daily loads should be promptly implemented in this watershed.
HS16-A007
Demonstration and Effectiveness Evaluation of Low-impact Development Facilities in Wen Qing Water Recycling Center, Taoyuan City
Tung-Yu LU1, Chen-Wuing LIU2, Shi-Min LIU3, Yueh-Tan LEE4, Yu-Jia CHIU1#+, Hong-Yuan LEE3, Yu-Te LIN1, Gene Jiing-Yun YOU3, Shi-Min LIU3
1National Taiwan Ocean University, Taiwan, 2Department of Water Resources, Taiwan, 3National Taiwan University, Taiwan, 4Luzhu District Office, Taiwan
In recent years, Taiwan has promoted Low Impact Development (LID) in numerous development projects. However, due to the diverse rainfall patterns, soil compositions, and geographical variations across Taiwan, the efficacy of LID facilities can differ significantly. The various materials and designs on the runoff process further complicates achieving consistent stormwater management policies and effects across different regions. Therefore, continuous feedback based on the monitoring data of on-site facilities is crucial. This research focuses on the "Wenqing Water Garden, Water Resource Recycling Center" in Guishan District, Taoyuan City, Taiwan—an innovative sewage treatment center. The entire facility incorporates LID development features, such as green roofs, permeable pavements, ecological detention ponds, etc., while maintaining well-vegetated open spaces. The goal for water retention capacity is set at 80 mm/m². The study utilizes water level gauges to observe water level changes in different LID facilities during multiple rainfall events. These facilities include permeable pavements and detention ponds. The monitoring data reveals they can effectively collect rainwater, with storage capacities applicable to approximately 60 minutes duration within a 5 to 10-year repeated period. Drainage performance is a critical aspect of the study. For instance, a detention pond without a drainage system may take up to two weeks to dissipate water, especially on clay soil. However, with a drainage system, the water above the drainage pipe drains out within a few hours, and the remaining water below the drainage pipe takes about 1 to 2 days to dissipate. This highlights the importance of incorporating drainage systems for facilities like permeable pavements. Additionally, the study involves on-site soil sampling, laboratory water permeability tests, and Storm Water Management Model (SWMM) simulations. The SWMM model is calibrated with on-site data, providing engineers with parameters for design analysis, so they may predict the impact of future events.
HS16-A014
Hydroenergy Potential of Irrigation Reservoirs Across Japan According to Flow Regime Indicators
Atsuya IKEMOTO1#+, So KAZAMA1, Takeo YOSHIDA2, Ryosuke ARAI3
1Tohoku University, Japan, 2National Agriculture and Food Research Organization, Japan, 3Central Research Institute of Electric Power Industry, Japan
This study estimated flow indices for irrigation reservoirs across Japan using a neural network model constructed for unobserved catchments. The hydraulic energy content of each irrigation reservoir was then estimated using the flow indicators. The results indicate that irrigation reservoirs across Japan have a hydraulic energy content equivalent to approximately 4,129,000 MWh, which is the amount of electricity consumed by approximately 960,000 households per year. The carbon dioxide emissions equivalent to approximately 3.6 million t-CO2 were also calculated. The study's results can inform energy policy and agricultural village planning in Japan.
HS16-A023
Application of Complex Network Theory-based Time Series Forecasting Method for Urban Water Demand Forecasting
Jyotsna PANDEY#+, Venkata Vemavarapu SRINIVAS
Indian Institute of Science, Bangalore, India
Efficient management of water distribution systems relies on accurate water demand forecasting. This ensures the fulfillment of customer demand and pressure needs, while also aiding in formulating operational and strategic choices (e.g., pump scheduling and demand management). Various studies have proposed numerous stochastic (ARIMA, SARIMA) and machine learning (ANN, RF, LSTM) based methods and models for demand forecasting, as none is established to be universally superior. User requirements, seasonality, weather conditions, and population density are a few time-varying parameters that play a vital role in deciding water demand. A more comprehensive forecasting method must incorporate such factors to predict future demand efficiently. Recent literature reveals that the evolution of complex network theory (CNT) has revolutionized time series forecasting. By leveraging the power of network connections, researchers can now make more precise and reliable forecasts in fields like economics, pricing, and energy management. In this context, the present study aims to explore the potential of a CNT-based time series forecasting method for predicting urban water demand. The method is tailored to incorporate key parameters deciding customer demand. The performance of the CNT-based demand forecasting method is compared with existing methods through a case study. It highlights the potency of using this method and indicates its applicability for predicting water demand for different time horizons. Accurate demand forecasts will be key to gauging how water distribution network adapt to changing demands, ensuring their continued resilience and reliability, and informing effective operational and management strategies.
HS16-A024
Optimizing Spectral Analysis for Sewer Pipe Monitoring: A Study on Light Source and Intensity Variations in Dark Conditions
Hosoo LEE1+, Gwangmin OK1, Yeonghwa GWON2, Dongsu KIM2, Youngdo KIM1#
1Myongji University, Korea, South, 2Dankook University, Korea, South
In Korea, sewer pipe monitoring predominantly employs level measurement techniques. This method involves measuring distance using reflected waves off the water surface. However, this approach can lead to significant errors in flow measurement when the effective cross-sectional area of the sewer pipe is reduced due to sediment accumulation. In an effort to address this issue, continuous research has been conducted on level measurement using spectral information. Yet, there remains a lack of research in environments like sewer pipes, where no specific light source is present. Therefore, this study focused on identifying suitable light sources and intensities for accurate spectral information acquisition within sewer pipes. Under experimental conditions resembling those in sewer pipes, two types of light sources and two light intensities were used to create four different cases. For each case, the Optimal Band Ratio (OBR) was extracted for ten different water depths, and the R2 values corresponding to the depths based on the band ratio were compared and analyzed. This research is expected to offer a methodology for verifying changes in light sources and intensities when acquiring spectral information in environments similar to sewer pipes or darkroom conditions. Acknowledgement: This work was supported by Korea Environment Industry & Technology Institute(KEITI) grant, funded by Korea Ministry of Environment(MOE) (RE-2023-00218973).
HS16-A025
Spectral Information-based Technique for Estimating Sediment Height in Sewer Pipes
Hosoo LEE1+, Gwangmin OK1, Yeonghwa GWON2, Dongsu KIM2, Youngdo KIM1#
1Myongji University, Korea, South, 2Dankook University, Korea, South
In Korea, the incidence of urban flood has escalated notably in recent times. Urban flood distinct from flooding caused by external water sources, arises when internal water fails to be adequately expelled to external outlets. Predominantly manifesting under conditions of extreme precipitation, this form of flood is primarily attributed to the obstruction of sewer conduits, impeding the expulsion of internal waters. The occlusion of these conduits is often a consequence of sediment accumulation or the presence of foreign materials, challenges that are not readily identifiable using traditional sewer monitoring techniques focused on water level assessments. To address this gap, the present study employed spectral analysis for the quantification of sediment heights within sewer systems. Utilizing multispectral data, the study applied the Optimal Band Ratio Analysis (OBRA) methodology to ascertain the optimal band ratios correlating to sediment levels. This led to the formulation of an empirical relationship between sediment height and these optimal band ratios, enabling the calculation of sediment depths. This research is anticipated to contribute to the existing methods of monitoring sediment accumulation in sewer pipes. Acknowledgement: This work was supported by Korea Environment Industry & Technology Institute(KEITI) grant, funded by Korea Ministry of Environment(MOE) (RE-2023-00218973).
HS17-A006
Comprehensive Spatiotemporal Drought Assessment and Their Implications on Agricultural Sustainability: A Case Study of Afghanistan
Ahmad Tamim SAMIM+, Han Soo LEE#
Hiroshima University, Japan
Climate change and global warming have caused more frequent and severe extreme weather events, such as droughts. Drought, characterized by prolonged periods of low precipitation, significantly impacts communities and ecosystems. It's crucial to monitor and assess risks in regions prone to these events. This study aims to comprehensively evaluate drought severity, duration, and frequency and their implications for agricultural sustainability. It utilizes 40 years of MERRA-2 precipitation and temperature data and observed data from 60 stations between 2009 and 2020 to assess its suitability for each river basin. Additionally, crop yield data from 2016 to 2020 is examined to better understand the drought's impact on agriculture. The study utilizes the standardized precipitation evapotranspiration index (SPEI) to analyze drought occurrences. Initial findings highlight average frequency ratios for mild, moderate, severe, and extreme drought as 0.49, 0.13, 0.6, and 0.2, respectively. Mild drought lasts an average of 10 months per event, moderate for 6 months, severe for 8 months, and extreme for 2 months. Notably, the central and southwest regions of Afghanistan show prolonged durations, exceeding 15 months per event, indicating the highest average durations in this area. The south and central regions of the country, experiencing frequency ratios surpassing 0.5, exhibit the highest incidence of drought events. Specific years, notably 1985, 1987, 2000, 2001, 2002, 2003, and 2004, showed varying intensities of drought across all regions. The primary findings indicate that in 2001, Afghanistan experienced extreme drought conditions that significantly affected the entire country, particularly the crop yield. Similarly, a severe drought in 2018 had a substantial impact on two-thirds of Afghanistan's crop yield. This comprehensive study offers crucial insights into past drought events, aiding in anticipation of future occurrences, and facilitating the development of effective agricultural strategies.
HS17-A007
Global Dryness Could Intensify Vegetation Failure Even After Net-negative Emission is Achieved
Sanjit Kumar MONDAL1#+, Soon-Il AN1, Seung-Ki MIN2
1Yonsei University, Korea, South, 2Pohang University of Science and Technology, Korea, South
The response of global dryness and vegetation to CO2 removal experiments, especially for net-negative emission is immature. Here we conducted a thorough investigation to identify hysteresis and reversibility in global dryness, as well as the vegetation productivity’s response to dry and wet episodes, considering their asymmetrical nature. The asymmetry index (AI) includes two important aspects such as positive AI indicates a dominant increase of vegetation productivity during wet episodes compared to the decline in dry episodes and negative AI implies a larger reduction of productivity in dry years compared to an increase in wet years. Aggregate results from various drought indices and vegetation productivity reveal a dominant dryness in the CO2 decrease phase. Global dryness shows strong hysteresis and irreversible behavior over half of the global land with significant regional disparity. Irreversible changes in dryness are concentrated in specific areas, i.e., hotspots, covering over 14% of the global land, particularly pronounced in Northern Africa, Southwest Russia, and Central America. Moreover, a wider spread of negative asymmetry indicates a significant decrease in vegetation productivity caused by dryness. Importantly, the potential evapotranspiration is projected to be the primary driver of global dryness as well as vegetation asymmetry. Our findings suggest only CO2 alleviation is not enough to cope with drought rather implementing advanced water management strategies is a must to mitigate the impact of drought effectively.
HS17-A012
Comparative Analysis of the 2021-2022 Droughts in Kazakhstan, South Korea, and the USA Using Remote Sensing and Reanalsysis Data
Aigerim BOLATBEKKYZY+, Hyunglok KIM#
Gwangju Institute of Science and Technology, Korea, South
This study broadens the scope of traditional drought monitoring by conducting a comprehensive analysis of the most recent droughts during 2021-2022 in Kazakhstan, South Korea, and the USA. Utilizing data spanning from 1979 to 2023, we aim to analyze and compare the specific characteristics, impacts, and severity of these recent droughts across the three countries. Our focus includes understanding how these droughts differ from each other and from previous events in their respective regions. The increasing severity of droughts in recent years presents a global threat to agricultural productivity, water security, and socioeconomic stability. This research leverages traditional in-situ measurement-based indices such as the Standardized Precipitation Index (SPI), Palmer Drought Severity Index (PDSI), and Standardized Precipitation Evapotranspiration Index (SPEI), alongside advanced remote sensing technologies. These tools provide high spatial and temporal resolution images, essential for understanding the intricate dynamics of these drought conditions. The objectives of this study are threefold: 1) To identify and classify the drought trends and their distinct features in Kazakhstan, South Korea, and the USA during 2021-2022, 2) To compare the strengths and limitations of various drought indices in monitoring and assessing these events in different geographical and ecological settings, 3) To propose region-specific adaptations in the use of vegetation health (VH) indices like the Vegetation Condition Index (VCI) and the Temperature Condition Index (TCI) for more effective agricultural drought monitoring. Through this analysis, we aim to provide critical insights into the recent drought phenomena, enhancing the understanding and evaluation of drought indices. This will contribute to the development of more efficient and tailored drought monitoring and mitigation strategies suitable for each country's unique environmental and climatic conditions.
HS17-A015
Relative Contributions of Large-scale Atmospheric Circulation Dynamics and Anthropogenic Warming to the Unprecedented 2022 Yangtze River Basin Heatwave
Zeqin HUANG#+, Xuezhi TAN
Sun Yat-sen University, China
The unprecedented 2022 Yangtze River Basin (YRB) heatwave is a threat to human society and natural ecology, so the understanding of its underlying drivers is critical to regional climate adaptation and resilience. Here we conducted a multi-method attribution analysis on the contribution of atmospheric circulation change and anthropogenic impacts to the occurrence probability and intensity of this extreme heatwave. Based on the nonstationary statistical analysis, the 2022 YRB heatwave is a 1-in-900-year event and a 1-in-110-year event with and without considering the 2022 YRB heatwave in the fitting, respectively, which indicates that the surface air temperature (SAT) in the 2022 YRB heatwave is not possible without anthropogenic warming. The large-scale meteorological condition analysis shows that the 2022 YRB heatwave is featured with an anomalous high-pressure system that favors a hot and dry atmospheric column, overlaid by anomalous subsidence and clear skies which leads to warming and greater solar heating. The ensemble constructed circulation analogue analyses show that the circulation anomaly fails to explain the observed 2022 YRB SAT anomalies fully. Specifically, 46% (0.132±0.027 ºC decade-1) of the observed SAT trend during 1979-2022 (0.290±0.048 ºC decade-1) is caused by anthropogenic warming and the associated thermodynamic feedback, while the remaining 54% (0.157±0.038 ºC decade-1) of the trend is caused by changes in the large-scale atmospheric circulation. Our findings provide valuable information for climate adaptation and mitigation strategies in the context of a warming climate.
HS17-A016
Drought Risk Identification and Assessment Based on Disaster Causing Process and Climate Change
Yanqi WEI1#+, Haichao LI2, Yuliang ZHOU1
1Hefei University of Technology, China, 2Tsinghua University, China
Climate change can lead to and intensify drought disasters. Regional drought identification and assessment are significant for understanding the mechanisms that transform drought intensity into eventual loss. This study proposed a "meteorology and agricultural drought risk index" using precipitation, groundwater, land use, and crop growth model simulation. The CROPGRO-Soybean model was used to simulate crop growth and water deficit. The drought risk index was applied to quantify the spatiotemporal characteristics of regional drought risk in typical years. The results show that: (1) The sensitivity of leaf-related parameters exceeded that of other parameters during the vegetative growth stage, whereas the top weight and grain yield showed a higher sensitivity in the reproductive growth stage; (2) A semi-logarithmic law can describe the relationship between the drought sensitivity indicators and the loss risk during the four growth stages. The pod-filling phase is the most vulnerable stage for water deficit and with the highest loss risk; (3) Fuyang and Huainan sub-regions were more vulnerable to drought than other regions on the Huaibei Plain in 2001, while Huaibei and Suzhou Cities were the most susceptible areas in 2002. The results could provide effective decision support for the categorization of areas vulnerable to droughts.
HS19-A002
The Effect of Unsteady Discharge and Vegetation on the Development of Alternate Bar
Pawat WATTANACHAREEKUL1+, Takuya INOUE1#, Tomonori NAGATA2
1Hiroshima University, Japan, 2Hokkaido Regional Development Bureau, Japan
An alternate bar is a highly mobile bar that occurs due to the instability of the riverbed. The development of alternate bars under repeated unsteady discharge hydrographs over a long period is not well understood. Our study numerically investigated the development of alternate bars under repeated hydrographs, considering scenarios both with and without vegetation cover. We created four stages of hydrographs: first, the discharge rate increased to the peak discharge and remained constant, then decreased from the peak to the low discharge, followed by the low discharge constant. In the absence of vegetation cover, the alternate bar formed in the first period, and its development followed the hydrograph pattern. The height and morphology of the alternate bar changed during the increasing discharge period and then reached an equilibrium state where bar migrates to downstream area without morphological alteration during the peak discharge constant. Subsequently, the height and morphology of the alternate bar changed during the decreasing discharge period, showing a different alteration pattern with the increasing discharge period. However, there was no alteration during the low discharge constant. With vegetation cover, we found that vegetation reduced the migration rate of the alternate bar, which could lead to a stationary bar. The bar morphology with vegetation cover changed during the period of constant peak discharge, which differed from absence of vegetation cover case. Therefore, the bar morphology under the same peak hydrograph is significantly different between the two cases. Furthermore, we observed that the impact of each peak discharge varied during both the increasing and decreasing periods on the development of the alternate bar. Hence, the discharge value that generates the highest bar height under constant discharge conditions is not the same as under unsteady discharge conditions, which is the effect from the decreasing discharge period.
HS19-A004
The Changes in Erosion Depth Caused by Freezing and Thawing Due to Climate Change
Riho KIDO1#+, Takuya INOUE1, Shigeru MIZUGAKI2, Sumner TAMAKI1
1Hiroshima University, Japan, 2Civil Engineering Research Institute for Cold Region, Japan
In recent years, because the concentration of greenhouse gases has increased, the global average temperature has continued to rise. As a result, heavy rains and the number of tropical cyclones increase, and snow cover and permafrost decrease. One of the main factors contributing to sediment production in cold regions is freezing and thawing. This is the phenomenon that when the water existing in the weathered bedrock freeze and expand in volume, it destroys the rock structure and turns it into sediment. If temperatures rise, sediment production will decrease because water in the weathered bedrock no longer freezes, but if snow cover decreases, sediment production will increase because the insulation effect of snow cover will decrease and subsurface temperature fluctuations will increase. In this study, we predicted changes in erosion depth due to freezing and thawing on the slopes in Pekerebetsu River basin in Hokkaido before and after climate change. As a result, it was found that the erosion depth due to freezing and thawing will increase in Pekerebetsu River basin. There are two reasons for this. First, temperature in winter will rise and approach 0℃. The winter temperature in present climate of Pekerebetsu River basin is around -12℃, but that in future climate is around -7℃. Second, snow cover will decrease. The amount of snow will not decrease but as temperatures rise, snowfall will melt more easily. Thus, freezing and thawing will increase even during winter and erosion depth will increase due to climate change.
HS19-A007
Projected Changes in Average and Extreme Precipitation Under Global Warming in Vietnam
Thuy Chi TRAN1,2+, Qiuhong TANG3, Gang ZHAO1#, Nigel WRIGHT4
1Chinese Academy of Sciences, China, 2Hanoi University of Natural Resources and Environment, Viet Nam, 3Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, China, 4University of Birmingham, United Kingdom
The Clausius-Clapeyron relation suggests that the atmosphere will hold 6%-7% more vapor per degree warming. Due to regional differences in moisture availability, atmospheric convection, and other climatic factors, changes in average and extreme precipitation may depart from this theoretical value. This study focuses on Vietnam which, despite its high vulnerability to climate change, has had very few studies focused on the relationship between extreme precipitation and different global warming levels. Here, using downscaled climate data from Phase 6 of the Climate Model Intercomparison Project (CMIP6), we quantified projected changes in annual average and extreme daily precipitation in Vietnam for two future periods and four global warming levels. We found that the regional temperature rises approximately 0.5℃ more slowly than the increase of global temperature. While there are small changes in average precipitation, the extreme precipitation is projected to increase by 12.1% in 2030-2059 and 19.3% in 2070-2099 compared to present time. For every degree of global warming, extreme precipitation in Vietnam will increase by 5.5%, with the northern region increasing more than the southern region. Our results emphasize the significant effect of limiting warming at a global scale on local flooding risks and can also benefit developing mitigation and adaptation strategies in Vietnam.
HS19-A008
Investigation of Flood Control Effects According to Temporal Variations of Vegetation in River Channels
Hayato KAJITA+, Seiki KAWAGOE#
Fukushima University, Japan
Currently, there is a concern that flood inundation damage will increase due to the intensification of heavy rainfall in response to climate change. In order to mitigate the damage, basin flood control is being promoted, in which all stakeholders in a river basin cooperate with each other to take measures against water-related disasters. This study was undertaken to investigate a means of communicating information from river monitoring cameras that can be understood by residents, targeting small and medium-sized rivers where management equipment is in short supply. We focused our research on the Natsui River and its tributaries in Iwaki City, Fukushima Prefecture. This river was damaged by the East Japan Typhoon in 2019, including a levee failure. We sought the relationship between the river channel and social activities by developing basic information on the watershed, such as flow velocity and flow rate, and land use information. In addition, we processed three-dimensional information on the conditions inside and outside the river channel. In the past, in order to understand flow conditions such as abnormal runoff caused by heavy rainfall, river managers have been developing useful deciphering techniques such as water levels, flow rates, and velocities. These visualization information provides residents with the ability to intuitively understand the hazards. In order to obtain a more detailed understanding of the river characteristics, the spatial distribution characteristics of vegetation growth were obtained. The Normalized Difference Vegetation Index (NDVI) using satellite images was used as a data set to understand vegetation changes. Based on the information obtained, inundation analysis assuming abnormal runoff was conducted using the Rainfall-Runoff-Inundation Model (RRI Model), and the information will be reduced to information that can be linked to the camera.
HS19-A009
Research on Watershed Sediment Monitoring Takes Into Feeding Damage Effects Due to Climate Change
Tatsuki SAKUMA+, Seiki KAWAGOE#
Fukushima University, Japan
Observations of the effects of climate change have indicated an increased risk of slope failure in mountainous areas due to heavy rainfall. However, excessive recharge that induces slope failure is not the only effect of climate change. For example, in recent years, bare land has been observed in mountainous areas in southern Japan due to the feeding damage caused by the "Cervus nippon". In addition, there are indications of increased sediment production. Such a phenomenon is feared to spread to wider areas of Japan due to climate change and population decline. In order to detect such a situation before it occurs, it is necessary to develop a combined forecast of erosion and heavy rainfall, and to develop a technique to derive the state of degradation in the interior of mountainous areas. These developments will enable a rapid response to the increased risk of slope failure due to climate change. In this study, we collected basic data such as watershed information, average precipitation, and frequency of heavy rainfall in Fukushima Prefecture, where the habitat area of "Cervus nippon" as expanded and snow cover has decreased, with the aim of deriving the devastation status of the mountainous interior of Fukushima Prefecture based on stream water quality. In addition, sampling surveys were conducted mainly at points in surrounding streams where there were reports of "Cervus nippon", and these samples were analyzed using ICP-MS d ion chromatography to compare and verify their chemical composition.
HS19-A013
Numerical Simulation of Inland Urban Flooding for Evaluation of Several Adaptation Measures in Japan
Miyata HIDETOSHI#+, Shuichi KURE
Toyama Prefectural University, Japan
Toyama City has been experiencing frequent inland flooding due to climate change. There is requires to urgent measures to inland flooding. However, it is difficult to dealing with exacerbating disasters with gray infrastructure such as dams and levees. The concept of full river basin disaster management is being advocated. Therefore, the objective was to assess the risk of inland flooding in the target area, compare, and consider measures such as Paddy Field Dams, Residential Redirection, and Green Infrastructure. We conducted a modeling and analysis of inland flow using MIKEURBAN in the targeted area. Conducting surveys in areas lacking information and the results of the survey were integrated into the model. Reproducibility was verified by comparing the model analysis results with actual measured water depths and flooding records.
HS19-A014
Flood Inundation Simulations for Evaluation of Adaptation and Counter Measures in Japan and Indonesia
Akbar RIZALDI, Shuichi KURE#+
Toyama Prefectural University, Japan
Jakarta, Indonesia is a typical urbanized Asian city where flooding presents a challenge. Several factors contribute to floods in Jakarta, such as land-use change upstream and climate change. This study quantified the impacts of land-use and climate change using a flood inundation model to evaluate several structural and non-structural counter measures for mitigating the future flood damage. Also, these flood inundation simulations were applied to Japan to compare with Jakarta’s situations. The counter measures discussed in this study are 1) an increase of the flood flow capacity in the rivers in Jakarta, 2) recharge and retention ponds, 3) recharge wells and 4) green infrastructure including the paddy field dam. The counter measures were evaluated based on the Expected Annual Damage Cost and B/Cs. From the results of analysis, it was found that the structural counter measures will reduce the flood damage effectively but the implementation cost is too expensive, so that these counter measures are difficult to be implemented in Jakarta. So, non-structural measures should be considered to be implemented.
HS19-A016
Toward the Diffusion of Slow Sand Filtration in Rural Cambodia
Ai MUROYA#, Kazuki OKUYAMA+
Miyagi Prefectural Sendai Nika High School, Japan
Our field site, a village near the Angkor Complex in Cambodia, is designated as a protected area for archaeological sites, and to protect any buried ruins, digging is severely restricted in the area. Due to this circumstance, water supply is not available, and the majority of the villagers use wells as their water source. Sendai Nika High School has conducted field work in Cambodia since 2014, and our past and recent water testing suggest that some wells show high iron contain and detection of bacteria above reference values. From the surveys conducted during the fieldwork in August and December 2023, it has been shown that almost all villagers, especially those who are poor, use water purifiers to purify water for drinking water. Although using water purifiers costs less than consuming bottled water, companies sell water purifiers with high prices using loans taking advantage of the villagers' lack of knowledge, so it is still a financial burden to some. In addressing this problem, a proposed strategy involves the promotion of inexpensive water purifiers that villagers can make themselves, incorporating a mechanism based on slow sand filtration. This mechanism is a water purification method which uses sand and the power of a sticky mat of biological matter, called a “schmutzdecke” that forms on the sand surface. Fieldwork investigations in 2023 also indicate that the proposed type of water purifiers can be made with locally available materials and, the climate conditions of Cambodia, which the average annual temperature is around 30 degrees celsius, is an ideal temperature for the water purifier to function properly. Thus it has been shown that the idea of slow sand filtration water purificaters are optimal given the circumstances. We will report on the conditions under which we demonstrated this water purifier and how we devised it.
HS19-A017
Presentation of Hazard Information Considering the Characteristics of Flooding in Rapid-flowing Rivers, Japan
Shintaro MATSUMOTO#+, Shuichi KURE
Toyama Prefectural University, Japan
In Toyama Prefecture, there are steep rivers such as the Kurobe River, which is shown the fast downstream and characteristics of flooding are observed. Therefore, there is a need to make clear areas requiring in advance evacuation. In addition, the current hazard maps do not take into consideration the characteristics of flooding in steep rivers. Moreover, steep rivers are difficult to prediction and specifying of break points. and "breaking without overtopping," it is necessary to consider the effects of erosion and scouring on levees. Therefore, in this study, flood inundation analysis and the risk of the ground (just inundation, house inundation, horizontal evacuation is needed) is carried out with the purpose of providing clear hazard information for landside areas, considering the characteristics of flooding in steep rivers. Flood inundation analysis is conducted using MIKE 11 and MIKE 21. For the flood inundation analysis, the assumed maximum flow rate (once in 1,000 years) was used as the external force, and a spatial resolution of 30 m was used for the computational grid. In the calculation of the risk of the ground, sections are established. Weighting is applied to assess the susceptibility to breaching in each section. Evaluate the breaking. Additionally, to set the many breach points is done to consider embankment maintenance locations. And considerations are made for areas designated by the government as having the risk of erosion and scouring. Moreover, to consider about the countermeasures of the levee. As a result, the risk assessment of levees, considering erosion, scouring, and levee countermeasures in each section, was conducted, and the calculated the risk of the ground results clarified the danger in each region, taking into account the characteristics of steep river. Furthermore, considerations for countermeasures in the embankments resulted in changes in the risk of the ground.
HS21-A004
Application of Must Software to Simulate the Transport of Nitrogen Transformed Products
Jui-Sheng CHEN1#+, Zhong-Yi LAIO1, Ching-Ping LIANG2
1National Central University, Taiwan, 2Fooyin University, Taiwan
Over the past several decades, progress has been made towards developing multispecies transport analytical solutions. Most recently, we have developed a couple of advanced multispecies transport analytical models. MUSt in which FORTRAN executable files based on our developed multispecies transport analytical solutions are equipped with an interactive Graphical User Interface (GUI) has been developed. The GUI is designed to facilitate the users to perform a variety of real-world applications. In this study, we apply MUSt to simulate the transport of nitrogen transformed products: subject to only constant source. The results show that transport a distance near the injection point while the concentrations of and start to increase and then to decrease with the decrease in the concentration along the x direction, after a very short period of time.
HS21-A005
Application of MUSt Software Package for Assessing Health Risk Associated with Groundwater Chlorinated Solvent Contamination
Ching-Ping LIANG1#+, Jui-Sheng CHEN2, Zhong-Yi LAIO2
1Fooyin University, Taiwan, 2National Central University, Taiwan
MUSt (MUltiSpecies transport Analytical Models) is a software package in which a FORTRAN executable file based on a series of multispecies transport analytical solutions are equipped with a user-friendly Graphical User Interface (GUI). MUSt provides visual exploration in real time subsurface reactive chemical transport of multi-contaminants. The multispecies transport analytical model combined with health risk module can be used to more reasonably perform the health risk assessment. This study applies MUST to evaluate the health risk in a groundwater chlorinated solvent contaminated site located in southern Taiwan. The geographical distribution of non-carcinogenic and carcinogenic health risk is displayed for appropriate action for reducing groundwater pollution and protecting human health.
HS21-A010
Exploring the Potential of CAESAR-Lisflood Model to Understand Hydrological Processes in Mineralized Watersheds in the Philippines
Francis GONZALVO1#+, Decibel FAUSTINO-ESLAVA1, Juan Miguel GUOTANA1, Jenielyn PADRONES1, Loucel CUI1, Eduardo CALZETA1, Cristino Jr. TIBURAN1, Tomas Jr. REYES1, Grigorios VASILOPOULOS2, Thomas COULTHARD2, Richard WILLIAMS3
1University of the Philippines Los Baños, Philippines, 2University of Hull, United Kingdom, 3University of Glasgow, United Kingdom
Watershed numerical models are tools to predict a variety of processes that may occur at different spatial and temporal scales. In the past, a variety of landscape evolution models have been developed to simulate landscape change. However, such models have often been limited dimensionally and are constrained by short time scales. This limits the potential applicability of these models to other watersheds with different characteristics. In temperate countries, numerous models were developed and evolved to answer their predecessor’s limitations. One of these simulation tools is CAESAR-Lisflood, which is an open source two- (2) or three- (3) dimensional catchment morphodynamic model that operates over a wide range of spatial and temporal scales. This study assesses the model’s potential as a reliable simulation tool in explaining the changes in the fluvial landscape of mineralized watersheds in tropical countries such as the Philippines. The model was applied to the Itogon sub-catchment of the Agno River Basin on the island of Luzon, and the Buayan-Malungon River Basin in Mindanao. Both are watersheds in the Philippines. These sites were chosen to represent the broad differences in watershed characteristics, predominant land use, and extremes in weather conditions. Data gathered as inputs to the model include digital elevation model, rainfall, and sediment properties. Results showed notable patterns of erosion and deposition in both Luzon and Mindanao watersheds. The model generated values between sediment output and river discharge, increased exponentially during rainfall events. The results also show significant evidence that erosion and deposition patterns varied across watersheds as a function of predominant land use and rainfall variabilities. The data generated from the numerical model can be used as a starting point for determining the future landscape scenarios in these watersheds.
HS21-A011
An Iterative, Conceptual, and Distributed Streamflow Routing Model for Improved Flood Peak Estimations
Ekant SARKAR1#+, Kesav UNNITHAN2, Akshay KADU1, Basudev BISWAL1, Christopher RUDIGER3, Subashisa DUTTA4
1Indian Institute of Technology Bombay, India, 2Commonwealth Scientific and Industrial Research Organisation, Australia, 3Monash University, Australia, 4Indian Institute of Technology Guwahati, India
Accurate estimation of flood peaks holds utmost importance in enabling informed decision-making and effectively managing risks associated with catastrophic flood events. Flow velocity stands as an important factor influencing both the magnitude and timing of flood peaks. However, conventional conceptual routing models treat flow velocity spatially and temporally constant. In the present study, we introduce a conceptual, spatially-distributed, and iterative routing framework that considers the temporal variation of flow velocity. We used calibration-free Dynamic-Budyko model to estimate the runoff, which was then routed to the basin outlet using our proposed routing framework. The model performance was evaluated in multiple basins in India as well as in the United States. It was found that the dynamic velocity updation significantly helped in capturing the flood peaks, particularly the timing of flood peaks.
HS21-A012
Improving Streamflow Prediction Through a Model Combination Approach
Akshay KADU#+, Basudev BISWAL
Indian Institute of Technology Bombay, India
With the increased intensity and frequency of extreme climatic events, effective management of water resources becomes crucial for sustaining and maintaining various related services. Accurate prediction of streamflow during both wet and dry periods plays a vital role in formulating management policies and decision-making. Most rainfall-runoff (R-R) models developed so far focus on simulating high flow, resulting in poor prediction of recession or low flow driven mainly by the sub-surface groundwater storage. Moreover, these R-R models assume a unique relationship between storage and streamflow, which is untrue. To overcome the above issues, we developed a model combination framework that exploits the relative strengths of two structurally different models. We combined an R-R model with a recession flow model such that the former is used for predicting the high flows, and the latter is used for the recession or low flow prediction. The recession flow model we used in this study is based on the power-law relationship between groundwater storage and streamflow, which is updated dynamically depending on the antecedent storage conditions. The framework effectively considers the relevant past groundwater storage information while predicting the recession flow, thus improving the overall prediction accuracy. We found that the 25th, 50th, and 75th percentiles of mean absolute error (MAE) in mm/day decreased from 0.47, 0.62, and 0.77 to 0.38, 0.50, and 0.67, respectively, when the combination framework was employed instead of a standalone R-R model. Similarly, the logarithmic Nash-Suitcliff Efficiency (NSElog) during the recession period improved from (0.69, 0.77, and 0.82) to (0.88, 0.91, and 0.93). Our study, thus, suggests that a model combination framework can be used to improve the prediction during both wet and dry periods.
HS21-A014
A Framework for Selection of Optimal Calibration-validation Variables Using VIC-AMBHAS Model in Indian Tropical Basin
Shubham GOSWAMI1#+, Sekhar MUDDU2
1University of Nebraska-Lincoln, United States, 2Indian Institute of Science, Bangalore, India
Variable Infiltration Capacity model (VIC) is one of the most tested and used semi-distributed hydrological models since 1990s. It has been a usual practice to use gauged streamflow (Q) data for calibration-validation of VIC model since its development. Despite the ability of VIC to simulate soil moisture (SM) dynamics and evapotranspiration (ET), usage of SM/ET for calibration-validation was limited because of unavailability of long-term reliable observations. As computational capabilities improved and the need for more accurate and comprehensive water resource management grew, researchers and hydrologists started developing models that could represent the interactions between surface water and groundwater systems. The approach of integrated hydrological modelling was supported by rapid growth of global in-situ and remote sensing based hydrological datasets for land surface characterization, meteorological forcings and water budget fluxes/components including groundwater levels (GWL). These datasets are useful for improved parameterization, forcing and calibration-validation of integrated hydrological models. In this study, we propose a multivariate calibration-validation framework for one such integrated hydrological model VIC-AMBHAS. It involves detailed sensitivity analysis of model parameters and selection of optimal calibration-validation variable combinations. The novelty of proposed framework lies in its ability to calibrate and validate using alternative variables (such as SM, ET, GWL), particularly in regions where streamflow is regulated or semiarid tropical basins with excess water use/ water deficits - e.g. Cauvery basin in India wherein the streamflow component in recent decades in some sub-basins has become very low and nonexistent during several months. This framework is necessary in such regions to create data-driven plans for modifying agricultural practices, water use efficiency measures and improving watershed management strategies for reviving/ restoring the streamflow (Arakavathy and Noyyal sub-basins in Cauvery basin in southern India) by assessing water budget components (SM, ET, GWL, Q) for each model grid in such sub-basins.
HS21-A016
Development of a Vertical Quasi-two-dimensional Model for Hillslope Surface-subsurface Flow Applicable to Basin-scale Rainfall-runoff Simulation
Sora FUGAMI1#+, Yutaka ICHIKAWA1, Kazuaki YOROZU1, Hyunuk AN2, Yasuto TACHIKAWA1
1Kyoto University, Japan, 2Chungnam National University, Korea, South
Predicting runoff in response to rainfall is one of the critical issues in hydrology, and a number of rainfall-runoff models have been developed. The applicability of current practical models may be reduced without parameter calibration, but calibrated parameter values do not always reflect the actual characteristics of the catchment. With the recent increase in heavy rainfall disasters due to climate change, it is even more desirable to develop modeling methods that adequately represent the rainfall-runoff process to achieve reliable predictions. The Richards equation describes the flow of water in the soil, and physically-based models based on it can directly use field-observed values such as soil water retention and permeability as model parameters. However, their high computational cost makes it difficult to apply them to basin-scale rainfall-runoff simulation. In this study, we developed a vertical quasi-two-dimensional model for hillslope surface-subsurface flow (quasi-2D model), which is applicable to basin-scale rainfall-runoff simulation. The saturated-unsaturated subsurface flow is described by the vertical two-dimensional Richards equation, where the hydraulic gradient in the downward direction is approximated by the slope gradient. This simplification achieves low computational cost while maintaining the accuracy of the saturated-unsaturated flow computation, making it applicable to basin-scale rainfall-runoff simulation. A distributed rainfall-runoff model using the quasi-2D model was established and applied to the Kamo River basin (138 km2) in Kyoto, Japan. The rainfall-runoff simulation was performed for a flood event, and the model performance was evaluated by comparison with the observed river discharge. The simulated hydrograph generally reproduced the observed data without parameter calibration, although it tended to overestimate the peak discharge. For this catchment size, the quasi-2D model was able to complete the rainfall-runoff simulation in less than 1/10 of the actual time.
HS21-A017
Comprehensive Flood Risk Assessment for Mbabane, Eswatini, Using 3Di Modelling
Samkele TFWALA#+
University of Eswatini, Swaziland
In recent times, Eswatini, and particularly its capital city, Mbabane, has been grappling with the devastating impacts of severe floods. Despite the recurring nature of these inundations, a comprehensive flood risk assessment for Mbabane remains conspicuously absent from the research landscape. This study aims to address this critical gap by employing state-of-the-art modelling techniques, with a primary focus on the innovative 3Di model. The study recognizes the urgent need for a refined understanding of flood dynamics in Mbabane to develop effective mitigation and preparedness strategies. The 3Di model, known for its advanced capabilities in simulating complex urban flood scenarios, will be utilized to create a high-resolution, three-dimensional representation of the city's hydrological system. By integrating real-time rainfall data, land-use patterns, and topographical information, the model will simulate flood scenarios to assess vulnerability, exposure, and potential impacts on critical infrastructure. This study not only seeks to quantify the flood risk in Mbabane but also aims to provide actionable insights for urban planning and disaster management. The findings are anticipated to inform the development of resilient infrastructure, early warning systems, and community-based strategies to mitigate the adverse effects of floods in the capital city. Ultimately, this research aspires to contribute significantly to the discourse on flood risk assessment in Eswatini, fostering a sustainable and adaptive approach to urban development in the face of increasing climate-related challenges.
HS22-A006
Assessment of DWAT and SWAT Models Performance for Predicting Hydrologic Balances
Tarekegn Dejen MENGISTU1,2#+, Cheol Hee JANG2, Il Moon CHUNG2
1University of Science and Technology, Korea, South, 2Korea Institute of Civil Engineering and Building Technology, Korea, South
As the global climate undergoes continuous changes, the accurate assessment and prediction of hydrological processes become imperative for effective water resources management. Hydrological models support environmental decision-making by ensuring prediction reliability based on appropriate parametrization, evaluation, and application conditions. However, challenges persist in achieving a robust assessment of hydrological balance due to structural differences and model performance potentially misrepresenting crucial processes. This study presents a comparative analysis of the predictive capabilities of two distinct models, the Dynamic Water Assessment Tool (DWAT) and the Soil and Water Assessment Tool (SWAT), specifically focusing on their ability to simulate water balances. Both models underwent calibration and parameter optimization utilizing historical streamflow data. The simulation performance was evaluated by comparing predictions with observed data, employing various statistical metrics. Therefore, this study provides valuable insights into the predictive capabilities of both models, offering pertinent information for decision-makers involved in water resources management and climate adaptation planning.
HS22-A008
Predicting Streamflow Using Meteorological and Effluent Forecasts with the Dynamic Water Resources Assessment Tool Based on Machine Learning
Deokhwan KIM+, Cheol Hee JANG, Hyeonjun KIM, Jeonghyeon CHOI, Chul-gyum KIM, Jieun KIM#
Korea Institute of Civil Engineering and Building Technology, Korea, South
A complex system of water use, such as streamflow, groundwater, wastewater effluent and water reuse, significantly affects the availability of water resources in a basin during a drought. Especially as droughts and floods become more severe due to climate change, a comprehensive river water management system is needed to prepare for water shortages. The variation characteristics of streamflow are complex and diverse, not only because of meteorological factors such as precipitation and temperature, but also because of anthropogenic factors such as dams, reservoirs, groundwater and wastewater. In this study, we have predicted meteorological and wastewater effluents and applied them to the Dynamic Water Resources Assessment Tool (DWAT) to predict streamflow for the Geum River basin. DWAT is a water resources assessment tool that can be used free of charge worldwide and can be applied to small and medium-sized river basins for water resource planning and management that considers surface water as well as groundwater and water usage for various purposes (https://public.wmo.int/en/water/dynamic-water-resources-assessment-tool). In this study, predictors, which are climate indices with high correlation between global climate patterns and domestic meteorological characteristics, were applied to multiple regression models and artificial neural network models to generate ensemble meteorological forecasts. We selected hydrometeorological factors with high correlation with observed wastewater effluents, and applied the adjusted weights to the machine learning model to produce wastewater effluent forecasts. For the Geum River basin, we applied meteorological and wastewater effluent forecasts to the DWAT, a watershed hydrological model, to predict streamflow. Acknowledgments: This research was supported by Korea Environment Industry & Technology Institute (KEITI) through Water Management Program for Drought, funded by Korea Ministry of Environment (MOE)(2022003610002).
HS22-A009
Irrigation Water Return Flow Estimation Using Dynamic Water Resources Assessment Tool (DWAT)
Jeonghyeon CHOI#+, Cheol Hee JANG, Deokhwan KIM, Hyeonjun KIM, Jieun KIM
Korea Institute of Civil Engineering and Building Technology, Korea, South
Accurate consideration of irrigation water is necessary for precise assessment and prediction of streamflow in watersheds. In particular, the irrigation water supplied from major reservoirs in South Korea involves a complex structure of supply and return through irrigation canals, making it challenging to understand the status of water supply for stream maintenance. While the irrigation return flow rate is generally suggested to be around 35% in Korea, applying this rate uniformly leads to unreliable results. Rapid return rates analyzed in various studies range from 33.8% to 70.8%, showing a diverse distribution depending on irrigation practices and conditions. Therefore, it is necessary to estimate the return flow by considering the characteristics and conditions of each watershed or region for accurate assessment. Most studies for estimating return flows input the monitored irrigation water supply into a hydrological model and estimate the return flow at small paddy area. However, it is necessary to consider groundwater behavior at a basin scale. In this study, we monitored the streamflow from outside the target basin and the irrigation flow supplied to the paddy areas within the target basin located around Damyang Dam. The monitored data were used as input for the Dynamic Water resources Assessment Tool (DWAT) to estimate and analyze the return flow of the targeted paddy area. DWAT is a hydrological model equipped with a module capable of simulating hydrological processes in a paddy area. In the paddy module of DWAT, return flow was estimated based on the simulated surface and groundwater flows. The simulated total return flows showed a difference from the uniformly applied 35% return rate. It is expected that more accurate results can be obtained if monitoring data are secured. Acknowledgement: This research was supported by Environmental Fundamental Data Examination project of River Youngsan & River Seomjin Basin Management Committee.
HS30-A003
Long-term and Seasonal Changes in Lake Storage in the Arid Central Asia
Gang ZHAO1+, Suxia LIU1, Haoxin DENG1, Qiuhong TANG2#
1Chinese Academy of Sciences, China, 2Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, China
Knowing the storage variations in lakes and reservoirs are essential for water resources and environmental management, especially in the regions facing water scarcity. However, the quantification of the storage changes is limited by sparse in-situ observations and spatial coverage of space(air)-borne altimetric sensors. This hampers the attribution analysis of lake storage changes. Here, we combined long-term optical remote sensing and multi-source terrain elevation data to derive the monthly storage time series from 1985 to 2020 for 8544 lakes and reservoirs in Central Asia, where water scarcity has been hampering local socioeconomic sustainability. The regional total storage has been decreasing with a rate of -4.78 km3 year-1 mainly owing to the desiccation of the Aral Sea. For other lakes, there are 26% of them show decreasing while 22% show increasing trends. At a watershed-scale, the long-term changes in lakes are primarily caused by the changes in surface runoff, jointly affected by precipitation and temperature changes. We also found that 29% lakes in Central Asia experienced frequent seasonal dry out in the past decades. Such seasonal dry out is mainly caused by fast evaporation losses during the summer months. Our analysis highlights the co-regulation of surface runoff and lake evaporation in the storage losses in arid and semi-arid regions.
HS30-A013
A Deep Neural Network-based Improvement of SMAP Soil Moisture Data and Tau-Omega Model-based Interpretation
Jaese LEE#+, Jungho IM, Bokyung SON
Ulsan National Institute of Science and Technology, Korea, South
The brightness temperature (TB) at L-band (1.4 GHz) frequency is commonly analyzed using the zeroth-order radiative transfer equation, called the τ-ω model. The Soil Moisture Active Passive (SMAP) is a satellite mission that plays a key role in the global retrieval of soil moisture (SM) using the τ-ω model. The operational SMAP SM retrieval algorithms exhibit favorable agreement with various in-situ SM measurements. However, these algorithms exhibit diminished performance in densely vegetated areas or on rough surfaces, mainly due to limited information availability during the parametrization stage. This study introduces a deep neural network (DNN) model to replace the current τ-ω and roughness models. The theoretical dielectric constant was simulated using in-situ SM data with the dielectric model to directly train the DNN, establishing the relationship between measured TB and the retrieved dielectric constant. This involved correlating the measured V- and H-polarized TB with the τ-ω model parameters from one of the SMAP retrieval algorithms, SCA. The challenge of scale mismatch between point-based and SM data was mediated through triple collocation analysis. The proposed model was assessed using in-situ SM data that were not used in the DNN training process, and compared with existing SM retrieval models. The DNN exhibited improved agreement, characterized by higher correlation and lower random error, particularly in dense vegetation conditions. Additionally, by retrieving τ-ω model parameters using the developed DNN, a novel set of parameters of the τ-ω model was found.
HS30-A021
Estimation of Water Level Over River Stream and Artificial Lake Using C-band Synthetic Aperture Radar
Yangwan KIM+, Jongmin PARK#, Kijin PARK, Chanyoung KIM
Korea National University of Transportation, Korea, South
Widespread flooding leads to substantial fatalities and damages to hydrologic infrastructures such as dams and levees. Due to global climate change, the intensity and frequency of extreme precipitation tend to increase, leading to increased vulnerability to flood. For example, unprecedented summer rainfall during early July 2023 over the Goesan Dam in South Korea led to the overflow of the dam and the failure of the levee located at the downstream. Accordingly, the demand for establishing flood extent monitoring and flood prediction systems has risen by means of using remote sensing imagery. Remote sensing has advantages in acquiring information on the surface without physical contact with the material. Accordingly, various types of satellite imagery (e.g., optical, synthetic aperture radar [SAR], LiDAR) have been utilized for flood analysis. Among various types of imagery, Synthetic aperture radar (SAR) has been widely utilized as it sees through the cloud with high spatial resolution compared to other imagery. Therefore, this study utilized Sentinel-1 C-band backscatter to estimate the water level over inland water bodies (e.g., artificial reservoir and natural river stream) located in South Korea. Firstly, we developed the water body detection algorithm based on the automatic threshold decision methods and developed water-pixel versus water storage relationship. After quantifying the accuracy of water body detection algorithms, we implemented Random Forest to estimate the water storage using SAR. Finally, we estimated SAR based water level by utilizing stage-storage curve developed by the ground-based measurement. Acknowledgement: This work was supported by Korea Environment Industry & Technology Institute(KEITI) through R&D Program for Innovative Flood Protection Technologies against Climate Crisis Program(or Project), funded by Korea Ministry of Environment(MOE)(RS-2023-00218873).
HS32-A008
TyrainNow: An AI-based Model for Improving Typhoon Rainfall Nowcast
Hongyi YAO#+, Ji CHEN
The University of Hong Kong, Hong Kong SAR
Tropical cyclones (TCs) often trigger torrential rainstorms, resulting in huge damages to societies. Rational nowcasting TC rainstorms within even a lead-time of few hours plays a key role in mitigating potential socioeconomic losses. However, almost every year enormous losses due to TCs indicate our lower nowcasting capability. Being one of artificial intelligence (AI) applications, deep learning-based algorithms are a newly promising way for improving TC rainstorm nowcast, but most of them are subject to the trouble of blur, dissipation, and rainband location errors. Here we develop a generic and concise TC rainfall nowcasting model using radar observations, with a 2-hour lead time for every 6-min step. Crucially, the newly-developed model incorporates two components, a multi-task learning (MTL) neural network and posterior bias correction. Spatial and Temporal first-order Differences of radar observations are coupled with image structure similarity index through uncertainty weighting to balance the loss function on the U-Net backbone (STD U-Net hereafter), which is proved to enhance geographical continuity and nowcast accuracy. The improved nowcast is thereafter amended by quantile mapping to mitigate blurring. The model with only three more learnable parameters in MTL proves effective to mitigate the trouble and advances typhoon rainfall nowcasting accuracy compared to original U-Net and other methods without imposing notable computational overheads. The study affirms the explainability and generalizability of the newly-developed AI-based nowcasting model. We also publicize typhoon rainfall composite radar products for sustainable collaboration within the academic community. It is the first-ever open access typhoon rainfall dataset with high resolution (6 min, 1 km) in the region.
HS32-A015
Enhancing AI-based Precipitation Nowcasting Through the Integration of NWP Predictions
Hongxu ZHU#+, Ji CHEN
The University of Hong Kong, Hong Kong SAR
Precipitation nowcasting with high spatio-temporal accuracy has always been a challenging problem in meteorology, closely tied to people’s daily lives and governmental decision-making. Nowadays, widely adopted precipitation nowcasting methods rely on extrapolation techniques and deep learning approaches rather than numerical weather prediction (NWP) because of the drawback of NWP’s spinning-up stage. However, even the state-of-the-art AI models exhibit diminishing performance when forecasting under a two-hour lead time. This study aims to incorporate the initial field and boundary conditions and predictions in NWP as a priori information into the AI model in order to achieve better forecasts.
HS36-A011
Grace-based Dynamic Assessment of Hydrological Drought Trigger Thresholds Induced by Meteorological Drought and Possible Driving Mechanisms
Zhiming HAN#+
Northwest A&F University, China
Determining the threshold at which meteorological drought triggers hydrological drought is critical for early warning and proper mitigation of drought. However, drought trigger thresholds are difficult to determine owing to the nonlinearity between meteorological and hydrological drought, and their dynamics have not been explored. To this end, we introduce a precipitation-driven drought trigger threshold framework. This framework considers the multiscale characteristics of cumulative precipitation anomalies and incorporates the drought severity index of terrestrial water storage anomalies to characterize hydrological drought. The dynamics of trigger thresholds over time and the main drivers of these variations are further explored over China. The results show that hydrological drought is more sensitive to meteorological drought in south China, with some regions showing weak or negative correlations mainly determined by the differences between climate change and human activities. The risk of drought outbreak in the central, northeastern and southern regions of China is high, with trigger thresholds showing a dynamic decreasing trend over time (corresponding to lower cumulative precipitation anomalies), indicating weakened resistance to meteorological drought. Rising temperature is the main factor affecting dynamic changes in the trigger threshold. The drought trigger threshold framework proposed in this study is also applicable for assessments in other regions around the world. This study provides valuable insights and new approaches for understanding the mechanisms of hydrological drought formation. Furthermore, these results are expected to severe as a scientific basis for government departments to reduce water supply stress on human and natural systems and to develop adaptive management strategies.
HS36-A014
Exploring the Geospatial Patterns in Hydrochemical Parameters of Surface Waters in the Karst of Samcheok, South Korea
Regina Martha LUMONGSOD+, Heejung KIM#
Kangwon National University, Korea, South
Karst environments are unique because the high solubility of the underlying bedrock (e.g., carbonates) allows for the development of distinct landforms on the surface interconnected with a complex drainage system on the subsurface. This also emphasizes intricate surface-subsurface interactions in karst areas which can be greatly affected by changing environmental conditions. Samcheok, Gangwon Province is one such area that is underlain by limestone-bearing formations, giving way to the formation of karst landforms such as caves and sinkholes. In this study, the patterns in the hydrochemical characteristics of surface water were explored through geospatial analyses. Surface waters from four streams in Samcheok across two seasons (February 2020 – winter and April 2020 – spring) were analyzed: Osipcheon River, Yeosam Stream, Sohan Stream, and Gyogok River. Results show that the parameters in northeast Samcheok karst are mostly varied and appear to be dependent on the stream where the samples were taken from instead of the distance of the sampling point from the coast. Apparent patterns for pH and dissolved oxygen values do not adhere to common assumptions for the usual variation of parameters in terms of water salinity. Concentrations of cations and anions mostly varied in between the two seasons and showed different patterns in terms of linear correlation for concentration vs. distance to stream outlet graphs. High linear correlation was observed for April 2020 samples from Gyogok River for the following ions: Ca2+ (R2 = 0.976), Mg2+ (R2 = 0.9321), SO42- (R2 = 0.879), and HCO3- (R2 = 0.955). Research on geospatial patterns for hydrochemical parameters in environments susceptible to pollution such as karst areas is useful for land use planning and future research planning.
HS36-A017
Numerical Simulation Study of Radionuclide Migration in Fractured Porous Media in the Preselected Geological Disposal Area of High-level Radioactive Waste in Northern China
Litang HU#+, Lei TIAN, Shiqi HUANG
Beijing Normal University, China
Deep geological disposal is currently recognized worldwide as an economically and technically viable method for the disposal of high-level radioactive waste. Accurately understanding the mechanisms of groundwater flow and solute transport in fractured rocks is crucial for the design, construction, operation, and safety assessment of rock mass engineering. This paper constructs a numerical model of radioactive nuclide migration in fractured-porous media using the TOUGH2/EOS7R model, and predicts and assesses the migration of radioactive nuclides in groundwater around the new underground laboratory under various scenarios. The study finds that after 1,000 years of leakage, the mass fractions of nuclides 90Sr and 137Cs decrease to the 10-11 level, and the mass fractions of nuclides 239Pu and 238U decrease to the 10-6 level. Adsorption, radioactive decay, outflow to boundaries, and dissolution contribute 79.6%, 20.0%, 0.3%, and 0.1% respectively to the removal of nuclides from the media. The study also finds that fracture permeability is one of the key parameters affecting nuclide migration. The lower the fracture permeability, the more difficult it is for nuclides to diffuse along groundwater to the surroundings. When the fracture permeability is 1.0×10-14 m2, it is predicted that 239Pu will be successfully contained within a 40 m radius of the leakage point over 10,000 years. The approach proposed in this study, which uses a multiple-media continuum model to simulate nuclide migration, can provide references for similar regions and tools for nuclide safety protection.
HS40-A009
Downscaling GRACE(-FO) Data Resolution for Water Storage Anomalies: A Case Study of the Pearl River Basin and Adjacent Coastal Areas
Ange HU+, Shanshan DENG#, Yuxin LIU, Wenxi ZHANG
Guangxi University, China
The Gravity Recovery and Climate Experiment (GRACE) and its follow-on mission (GRACE-FO) provide data that enable the quantification of global water storage redistribution at the regional to global scale. However, the relatively low spatial and temporal resolution of the raw GRACE(-FO) data does not meet the requirements of accurately quantifying rapidly evolving water storage anomalies within the basin over time and space. Consequently, there is a necessity to downscale GRACE(-FO) data to enhance spatial resolution. In recent years, downscaling techniques based on data assimilation and statistical methods have been demonstrated to yield higher spatial resolution information while preserving the original trend of GRACE(-FO) data. Nevertheless, during extreme hydrological events, such as floods or droughts, the existing downscaling approaches struggle to effectively capture short-duration water mass anomalies, leading to significant errors in downscaling results during periods of water mass irregularities. Moreover, for regions with scarce or unevenly distributed observational data, the current downscaling methods are unable to fully utilize the observational data, which increases the uncertainty of the downscaled results. This study focuses on the Pearl River Basin in China and the adjacent coastal areas near its estuary, utilizing meteorological data (precipitation, evapotranspiration, runoff), geographical environmental data (elevation, topography), and anthropogenic data (population density) to improve the GRACE(-FO) resolution to 0.25°. The reliability of the downscaled results is validated through the hydrological extreme records and other evidences. Sensitivity analysis of parameters and models evolved in this downscaling method is conducted to evaluate the contributions of different parameters to regional terrestrial water storage, thereby verifying the robustness and reliability of the downscaling approach. The study also attempts to analyze the impact of different parameters on water mass anomalies and to investigate potential differences in downscaling terrestrial water storage and oceanic water storage using GRACE(-FO) data.
HS43-A006
Impact of Anthropogenic Disturbances and Climate Change on Riverine Nitrogen and Phosphorus Load
Ruixueer WU#+, Binghao JIA
Chinese Academy of Sciences, China
Nitrogen (N) and phosphorus (P) are priority nutrients controlling eutrophication of the aquatic ecosystems. Expanding anthropogenic activities (e.g. agricultural fertilization) have increased nutrient delivery from land to rivers, resulting in severe eutrophication in many major river basins in China. Additionally, atmospheric nitrogen deposition, primarily from combustion of biomass and fossil fuels, significantly impacts terrestrial ecosystem productivity and even stimulate N export from land to water. It indicates that climate change and anthropogenic disturbances have divergent impacts on the N and P delivery from soil to rivers. However, the spatial-temporal variations of riverine N and P remains a challenge to access in major river basins of China. Moreover, how riverine N and P loads respond to climate change and anthropogenic activities and quantitatively their relative contributions are still unclear. In this study, we firstly incorporated scheme for soil dissolved inorganic nitrogen (DIN) leaching and scheme for soil dissolved inorganic phosphorus (DIP) weathering into the Land Surface Model of the Chinese Academy of Sciences (CAS-LSM). Then, numerical simulations for the last four decades (1979-2018) were used to investigate the characteristics of annual riverine N and P export loads and the hotspots of N and P loss at the watershed scale. After that, we illustrated how anthropogenic disturbances and climate change affect riverine N and P export loads. This study is expected to provide a reference basis for nutrient and pollution management.
HS43-A012
A Soil Moisture Ensemble Prediction Framework Based on Non-stationary Vine Copula
Chenlu YU+, Dong WANG#, Along ZHANG
Nanjing University, China
Soil moisture plays a crucial role in the hydrological cycle (e.g., surface runoff and infiltration, groundwater recharge, solute transport and evapotranspiration), and accurate soil moisture prediction can provide much help for practical applications. In recent years, soil moisture displays evident nonlinear and variability, especially with global climate change and anthropogenic activities, adding the difficulty for predicting. In this paper, 4 variables including precipitation, temperature, evaporation, and antecedent soil moisture are used to predict soil moisture content of four layers (0~10 cm, 10~40 cm, 40~100 cm, and 100~200 cm) in Yunnan Province from 1951~2020. Taking time and five large-scale climate factors (including NINO3.4, NAO, AO, PDO and DMI) as covariates, the non-stationary of marginal distributions are detected and fitted with the best lag time. A vine copula predicting method cooperating Monte Carlo simulation technique is performed to realize both deterministic and probabilistic prediction of different vine structures. The Bayesian model average (BMA) method is applied to combine all predicted results, and the ensemble performance is compared with single vine structures. The effects of prediction are also verified by a traditional machine learning method (Random Forest, RF), and the possible influencing factors (number of simulations, copula structures and presence of non-stationarity) are also discussed. This paper offers a new approach for predicting soil moisture content under changing environment and has potential to be extended to other study areas.
HS43-A014
Prediction of Groundwater Solute Diffusion Coefficient and Migration Velocity Based on Parameter Inversion and Transformer Network
Yinquan MENG#+, Jianguo JIANG, Dong WANG
Nanjing University, China
Hydrodynamic dispersion in porous media is a critical, irreversible phenomenon delineating the transport and evolution of transition zones between two miscible solutions. This process has profound implications for environmental and industrial applications such as carbon dioxide storage, seawater intrusion into freshwater aquifers, and groundwater pollution management. Despite extensive research through experiments, theories, and simulations, understanding the microscopically heterogeneous yet macroscopically homogeneous nature of porous media remains challenging. The longitudinal dispersion coefficient, DL, is a pivotal parameter in this context, indicating the pollutants' dispersion capacity along the flow direction in porous media. Higher values of DL signify stronger dispersion capabilities, crucial for predicting pollutant migration rates and patterns. Another essential factor is the solute migration velocity, u, which reflects the fluid's motion state and significantly affects pollutant dispersion and migration. Current research leverages numerical computation and computer simulation, particularly the Lattice Boltzmann Method (LBM) combined with Random Walk Particle Tracking, to study these processes. However, the complexity and time-consuming nature of these methods necessitate more efficient alternatives. This study introduces an innovative approach integrating LBM, Random Walk Particle Tracking, and deep learning neural networks, specifically Convolutional Neural Networks (CNN) and Transformer networks. These networks, celebrated for their prowess in capturing complex patterns and long-range dependencies, have not yet been applied to estimate physical parameters in porous media. Our model represents a significant stride in efficiently and accurately computing critical hydrodynamic parameters. It holds immense potential for advancing environmental protection, soil contamination management, and water resource conservation, marking a new frontier in the predictive analysis of pollutant behavior in porous media.
HS43-A017
Evaluation of Peak and Flood Reduction Capacity of a Sponge City Under the Combined Action of River Flood and Urban Flood
Haichao LI1#+, Dawen YANG1, Ishidaira HIROSHI2, Yanqi WEI3
1Tsinghua University, China, 2University of Yamanashi, Japan, 3Hefei University of Technology, China
China is in the monsoon climate zone. Here the summer is hot and most of the annual rainfall occurs in this season. Short-term heavy rainfall is common, causing significant water flow into river basins, flooding, and the formation of river embankments; these embankments narrow river channels and flooding is accelerated, which presents a serious downstream safety threat. City drainage systems are often overcome by heavy rain and floods, and densely urbanized inland rivers often have limited space for safe expansion. Therefore, the systematic improvement of flood control capacity is a key challenge for urban stormwater management. In China, urban flood management models address urban and river floods independently, with limited collaboration between the responsible departments. As a result, the standard return periods of urban and river floods are different, the boundary conditions of both flood types are not fully considered, and their interplay is ignored. Urban and river floods will affect each other, and there are cases in which the flood risks are interdependent. The coordination of urban drainage and river flood systems should be a primary concern for effective urban flood control. As climate change and urbanization accelerate, the likelihood of floods and the impact on sponge cities has become a prominent issue. In this Chapter, the combined urban and river flood risks of Mianyang, and the efficiency of its sponge city construction, are explored from the perspective of river basins. A two-dimensional hydrodynamic rainfall-runoff-inundation (RRI) model is established for the middle- and upper-reaches of the Fujiang River, and validated using data from hydrological stations and satellites that were collected in the year 2020. Finally, the extreme flood events encountered in Mianyang City between 2015 and 2021 are evaluated.
HS43-A026
Analysis on Driving Factors and Prediction of Dynamic Change of Poyang Lake Area
Li REN#+, Yuxiang HE, Jiachen ZHU, Yutong LIU, Wenmei CAI, Wenjiao YANG, Jie ZHAO, Chenchen WU
Hohai University, China
Landsat8TM/OLI satellite FROM GLC remote sensing dataset is used to study the dynamic changes and driving factors of the area of Poyang Lake. The results show that: From 2001 to 2015, the area of Poyang’s area showed a downward trend, with a large intermediate fluctuation, but the overall trend was stable, and the dynamic variation degree was 0.07%. Using Person correlation and grey correlation analysis of the driving factors, it can be seen that in terms of natural factors, the precipitation factor has the greatest driving degree to the lake area. In the aspect of social factors, agricultural factors drive lake area obviously. Through the combination of the principal component analysis method and the analysis, it is concluded that the driving force of area is dominated by social factors. It is of great theoretical and practical significance to study water resources using remote sensing technology, which helps us grasp and study the dynamic change process of water resources in Poyang region timely and accurately. In addition, the driving factors influencing the area change of Poyang and the contribution of each driving factor to the area of Poyang are analyzed qualitatively and quantitatively, and used LSTM to predict the future changes of the area of Poyang. In order to improve the current problems such as the area shrinkage, ecological degradation and ecological single of Poyang , the paper provides a method guidance for the study on the influence of the dynamic change of shallow lake area in the future.
HS45-A002
| Invited
Exploring Drivers of Low Dissolved Oxygen in the Shenzhen River Estuary: A Data-driven Approach
Xiaoyu ZHANG1, Ye XIONG2, Jiping JIANG1#+
1Southern University of Science and Technology, China, 2Shenzhen Water (Group) Co., Ltd., China
Dissolved oxygen (DO) serves as a crucial indicator for surface water quality management. It directly reflects organismal growth conditions and the extent of water pollution. Recent years, many estuary areas in China observed low DO values, below 2 mg/L, which leads to organism mortality and affects biological resources and habitat carrying capacity. This study using field data to descript phenomenons of low DO observations and explore potential reasons in the estuary of Shenzhen River, China. It is a boundary river between Hong Kong and mainland China, originates from Wutong Mountain, eventually flowing into Shenzhen Bay and reaching the Lingdingyang. In recent years, concerns have arisen due to reported instances of low DO in the Shenzhen River estuary. According to the 2 years of the monitoring data in 2022 and 2023, mean DO was 4.57 mg/L and 5.58mg/L respectively. However, the estuary exhibits significant seasonal differences in DO in the research area, with higher levels at the beginning of the year followed by a decreasing trend. The lowest monthly mean drops to 3.93 mg/L, with lower nighttime mean 3.0 mg/L. These variations suggest either natural temperature cycle or regular anthropological impacts. Utilizing measured temperature data to estimate the theoretical saturation DO level, we delve into the impact of non-temperature factors. The findings reveal a distinct correlation between abrupt drops in DO and rapid surges in turbidity. Additionally, a significant negative correlation between nitrogen and DO is established. Through a comparative analysis of diurnal variations in ammonia nitrogen, total nitrogen, and dissolved oxygen, nitrogen emerges as a potential influential factor. Stream flow, pH values, and point source inputs are also integral considerations. Furthermore, Fourier analysis uncovers fundamental daily and monthly cycles. When coupled with continuous wavelet transformation (CWT), effective identification of abnormal fluctuations in DO becomes feasible.
HS45-A004
Characterizing Morphology of Landscapes to better Understand Their Evolution
Saba RAINA#+, Dnyanesh BORSE, Basudev BISWAL
Indian Institute of Technology Bombay, India
River networks reveal fascinating tree-like patterns that are the result of long-term evolution of the landscapes in response to climate change and various complex processes like hydrological and geological processes. Remarkably, river basins exhibit universal scaling relationships, despite their diverse geological, climatological, and topographical attributes. The origins of these scaling relationships are a subject of curiosity. Similar to raindrops that adopt spherical forms to minimize surface energy, river networks assume tree-like structures to minimize energy expenditure. The main objective of this study is to identify morphological indicators that gauge the river-basin energy efficiency. We introduced here the percentage of extra energy expenditure (ΔΕ) to represent the river-basin energy efficiency, which is the deviation between the energy expenditure of a river basin and the energy expenditure predicted by OCNet, an Optimal Channel Network model. Considering 25 islands from across the world, we found being positively correlated with Hack’s exponent. Hack’s exponent is defined here as the power-law exponent of main stream length vs. drainage area curve of independent basins, i.e., basins that drain directly to ocean. Two extreme cases, Hawaii (Hacks exponent: 0.58, : 29.14%) and Belle Île (Hacks exponent: 0.46, : 4.60%), exemplify this trend. To reinforce our finding, we investigated the Hawaiian Islands separately, which exhibit diverse geological ages and a variety of volcanic formations. Notably, positive correlation between ∆E and Hack’s exponent, respective to their geological ages, is distinctly evident across the Hawaiian Islands. This relationship becomes apparent when comparing the youngest island, Hawaii (Hack’s exponent: 0.58, ΔΕ: 29.14%, age: >0.43 million years), with the oldest island, Kauai (Hack’s exponent: 0.53, ΔΕ: 6.4%, age: 5.1 million years). Our study thus underscores the significance of the Hacks exponent as a valuable metric in understanding the evolution of a landscape, serving as a geomorphic signature of landscape evolution.
HS46-A003
Comprehensive Soil Erosion Prevention and Control Technology System in the Black Soil Region of Northeast China
Qingbin PAN#+
China Institute of Water Resources and Hydropower Research, China
Based on the statistics of soil erosion in the black soil region of Northeast China, soil and water conservation measures applicable to the region were systematically sorted out. On the basis of analyzing the soil conservation benefits of the main soil and water conservation measures, such as horizontal terrace field, pedunculated plant belt, contour farming and ecological restoration, and combining the soil erosion characteristics of different secondary sub-regions, the following system of measures is put forward: in the rolling hilly region, terrace field should be constructed to cut off the water channel within the long-slope, and horizontal terrace field and reservoirs should also be constructed to block and drain the confluence, thus realizing the management of the cultivated land with long and gentle slope. In the hilly and gully region, the development of erosion gullies should be stopped through comprehensive management of small watersheds by adopting ditch-head, valley and ponds protection, by the construction of high-standard farmland, and by the natural restoration; in the sandy and windy region, the key management areas should be concentrated in sandy land and agricultural and animal husbandry intertwined zones, and the main measures taken include planting of shrubs and grasses, enclosure grassland, natural restoration, the installation of sand barriers and the promotion of fodder feeding, and so on.
HS46-A004
Estimation of Carbon Emissions from Riverine Wetlands in Response to Water Levels Changes
Minseok KIM+, Hoyong LEE, Junhyeong LEE, Hung Soo KIM, Soojun KIM#
Inha University, Korea, South
Global warming and climate change caused by continued greenhouse gas emissions are having a negative impact on the world. In order to fundamentally solve these problems, it is necessary to solve the problem of carbon emissions, the source of greenhouse gas emissions. In this regard, the importance of wetlands is emerging as nature based solutions, which are carbon neutrality, ecosystem protection, and sustainable management and restoration techniques, are highlighted. Wetlands serve a variety of roles in addition to their traditional habitat functions as habitats for living organisms and carbon sinks. However, the carbon flux absorbed by wetlands has not yet been quantified so it is still unknown how much of a role wetlands play as carbon absorption. Therefore, this study aim to develop a methodology to calculate carbon flux according to the water levels by creating a wetland that reflects the hydrodynamic characteristics of a laboratory-scale river. Through the developed methodology for calculating carbon flux in wetlands, It is able to confirm the carbon flows of CO2 and CH4 in wetlands, which is expected to be used as basic data in calculating greenhouse gas inventories of wetlands in the future. This work was supported by Korea Environmental Industry&Technology Institute through Wetland Ecosystem Value Evaluation and Carbon Absorption Value Promotion Technology Development Project, funded by Korea Ministry of Environment(MOE)(2022003630001).
HS46-A008
Investigating the Spatial Distribution of Soil Moisture in the Reservoir by Using Fiber Optic Distributed Temperature Sensor
Bo-Cheng CHEN#+, Hong Ru LIN, Jet-Chau WEN
National Yunlin University of Science and Technology, Taiwan
The purpose of this study is to investigate the spatial distribution of water infiltration in a reservoir using the Fiber Optic Distributed Temperature Sensor (FO-DTS) to observe the temperature distribution in soil layers. The study site is located near the Douliu Irrigation in Gukeng Township, central Taiwan, and the reservoir covers an area of approximately 2 hectares, consisting of a precipitate pool and an infiltration pool. Fiber optic cables are deployed around both the precipitate and infiltration pools, intersecting at the center of each. FO-DTS is utilized to obtain comprehensive temperature information of the reservoir. The fiber optic cables are buried in three layers with a total depth of 60 cm; the first layer is buried 20 cm beneath the pool's shallow bottom, with the second and third layers each buried 20 cm apart, observing the stratified soil temperatures of the reservoir's bottom. Due to the phase delay in the cyclical temperature difference between the surface and subsurface, measuring temperatures at different depths can assess the rate of water infiltration into the subsurface and its replenishment effect on regional groundwater. Therefore, this study evaluates the infiltration capacity of the reservoir using temperature method. The results show that the temperature of the soil beneath the reservoir, after it is filled with water, is influenced by water infiltration and exhibits daily cyclical variability and the average soil temperature in different layers shows a negative correlation with depth. This demonstrates that the FO-DTS can capture the thermal front generated by water infiltration.
HS46-A009
Non-stationarity and Its Driving Forces of Annual Runoff and Sediment Load Under a Changing Environment in the Dongting Lake Basin, China
Dehua MAO#+, Ting WANG, Ruizhi GUO
Hunan Normal University, China
The processes of runoff and sediment inflow and outflow in Dongting Lake have undergone significant alterations in response to climate change and anthropogenic activities. we examined the temporal trends, periodicities, change points, and non-stationarity of annual runoff and sediment load series at eight hydrological stations in the Dongting Lake Basin from 1961 to 2021, and identified significant driving factors by employing a combination of the generalized additive models for location, scale, and shape framework and the random forest model. Results indicate a declining trend in annual sediment series at each station, a significant decrease at the Three Outlets and Chenglingji station and no significant trend in the annual runoff series at Four Rivers basin showed. Furthermore, the both exhibited variations during the 1980s to 1990s, with primary periodicities identified at 27-38 years for annual runoff series and strong oscillations at 11-39 years for annual sediment load series. Reservoir storage capacity contributed over 20% to the both at five stations. Moreover, the contribution of annual rainfall amount to changes in annual runoff series changes exceeded in annual sediment load series. Variations in annual mean temperature and wind speed also contributed by 6%~11% of annual runoff and sediment load series in Three Outlets, Taoyuan and Chenglingji station. Additionally, there was a shift in the lake area from sediment deposition to erosion between 2006 and 2021. Except for the annual runoff series at Guanjiapu station, the Hurst exponent revealed an unsustainable trend in the remaining seven stations. Considering future climate changes, reservoir expansion, and water allocation projects in the Four Rivers basin, the non-stationarity in the Dongting Lake Basin is expected to intensify. These results will serve as a reference for implementing improved measures to regulate runoff and sediment in the Dongting Lake Basin in the future.
HS50-A004
Numerical Simulation of Coupled Multiphase Fluid Flow and Elastic-viscous Mechanics for Gas Migration in Bentonite Considering Heterogeneous Distributions
Yu-Sheng LIN#+, Jui-Sheng CHEN
National Central University, Taiwan
The final disposal method for high-level waste is Deep Geological Disposal. This is where nuclear waste is buried in geological formations at depths greater than 300 meters, and canister and buffer materials are used to cover and secure it. By the principles of isolation and retardation, the waste decays harmlessly, isolating it from the biosphere and ensuring human health and environmental safety. However, after hundreds of years of disposal, gas may be generated due to the corrosion of metallic materials under anoxic conditions, radioactive decay of waste, or the radiolysis of water. With continuous gas pressure accumulation, the stress on buffer materials can no longer withstand it, leading to pathway dilation and fractures, allowing gas to escape. As gas degrades the barrier's capability, endangering the safety of the repository. Therefore, buffer materials play a crucial role in the repository, bentonite is commonly chosen as the buffer materials. In practical situations, bentonite exhibits different particle arrangements, porosity, and permeability, presenting heterogeneous distributions. This heterogeneity may lead to the formation of preferential pathways, particularly in regions with high porosity and loose particle arrangements, making gas flow more accessible and consequently influencing the gas migration behavior. Therefore, this study employs the THMC7.1 numerical model coupled multiphase fluid flow and elastic-viscous mechanics to simulate the homogeneous distributions of bentonite. The results successfully demonstrate variations in gas pressure accumulation and breakthrough. Subsequently, the study further considers heterogeneity by altering material parameters such as porosity and permeability. The analysis aims to investigate the impact of preferential pathways formed by heterogeneity on gas migration.
HS50-A005
Applying the Three-dimensional Variably Saturated Flow Model to Simulate Groundwater Flow in Pingtung Plain by Using THMC
Pham NHAN#+, Jui-Sheng CHEN
National Central University, Taiwan
Pingtung Plain is an agricultural area in southern Taiwan, that is recorded as having the lowest rate of tap water usage in all of Taiwan. Overexploitation of groundwater in this area has led to a drawdown in overall groundwater levels, seawater intrusion, and land subsidence. Additionally, this is an area with high rainfall, and the terrain is conducive to the creation of groundwater. However, constructed objects like roads and buildings have an impact on surface permeability, which is crucial for rainfall infiltration into groundwater. This study uses THMC (Thermal - Hydrology - Mechanics - Chemical) to simulate groundwater flow in the Pingtung plain using the variably saturated flow model. THMC model is water environment software developed by Prof. Gour-Tsyh Yeh and continuously expanded with a user-friendly interface platform by the CAMRDA team. With the aim of conducting regional groundwater flow modeling in Pingtung Plain, a 3-D finite element method flow model is established by using the interface of the THMC platform. The procedure includes determining the two-dimensional boundary of the study area combined with borehole and geological data under mesh generation. Then assign material properties and set hydrogeological parameters for simulation. The simulation first runs in a steady-state condition, then the result is input into the transient simulation as the first day of the simulation time period. Comparing and minimizing the differences in groundwater levels between observation data and simulation data is a calibration process for the developed model.
HS50-A013
What Mainly Controls Discharge-basin Area Scaling?: Channel Network Morphology-based Perspective
Akshay KADU#+, Basudev BISWAL
Indian Institute of Technology Bombay, India
The scaling of discharge with the basin area provides crucial insights into dominant hydrological processes. Previous studies primarily focussed on peak-discharge scaling and observed that the peak-flow scaling exponent can be lower than 1. This is typically interpreted in terms of the basin’s width function, representing the pure surface flow (PSF) condition. The present study extends the scaling analysis to the entire streamflow spectrum. We employ a Geomorphological Hydrologic Response Model (GHRM) that simulates the flow at the basin outlet as a combination of PSF and mixed surface subsurface flow (MSSF). The MSSF is modelled by considering a progressive desaturation of the active drainage network (ADN) downstream of the basin. The GHRM accounts for both ‘local’ and ‘regional’ sub-surface flow paths while simulating the streamflow, unlike conventional Dupit-Boussinesq’s aquifer-based low-flow models considering only the local sub-surface flow. Our results indicate that the scaling exponent gradually approaches 1 during the recession period, attributed to the increasing dominance of MSSF, directly proportional to the ADN length, which in turn is proportional to the basin area. Our model suggests that the exponent can exceed 1 during the late recession, as flow in smaller basins decreases at a higher rate in the absence of regional groundwater flow contributions. These findings imply that a basin cannot be viewed solely as a sum of its hillslopes, with implications for hydrological and ecological modelling. We also illustrate the complexity of discharge-area analysis due to factors such as spatio-temporal rainfall variation, flow generation mechanisms, and surface flow velocity.
HS50-A017
Quantifying the Impacts of Land Cover Change on Hydrological Responses Under SSP-RCP Scenario
Ermias Sisay BRHANE#+, Koji DAIRAKU
University of Tsukuba, Japan
Land use land cover (LULC) change induced by rapid anthropogenic activities is one of the major causes of change in hydrological and watershed processes. This study aims to assess the impacts of land cover change on the hydrological responses of the Upper Blue Nile (Abay) basin, the largest and most rich river basin in Ethiopia. Commonly, such assessments are accomplished by using distributed hydrological models in conjunction with different land use scenarios. To this end, we use the hydrological model, SWAT, and historical and future land cover scenarios from our previous study, produced by the FLUS model based on Land-Use Harmonization-2 (LUH-2). Three scenarios were considered for land use change projections: SSP1-1.9 as the low-emission scenario, SSP2-4.5 as the medium-emission scenario, and SSP5-8.5 as the representative high-emission scenario. Our land use dataset based on SSP_RCPs indicates a noticeable increase in the cropland (18 %) at the expense of forest (25.4 %) by the end of the year 2100 compared to the baseline year, 2015. As a response, simulation results indicate a median percent increase in the extreme flows and mean annual flows in the range of 1.8 % to 11.3 % across the sub-catchments. The direct conversion of forested areas to agriculture reduces the leaf area index, reducing evapotranspiration (ET) and increasing surface runoff. Further, the range of behavioral hydrological predictions indicated variation in the magnitudes of extreme flows simulated for the different land cover scenarios; for instance, uncertainty in the scenario labeled “Far Future” ranges from 15 to 180 m3 s−1 across sub-catchments. This study indicates that the recurrent flood events occurring in the upper Blue Nile River basin might be influenced by the changes in LULC at the catchment scale and suggests that model parameterization represents an uncertainty that should be accounted for in the land use change impact assessment.
HS50-A024
High-resolution Ensemble Hydrologic Modeling for Mid-range Streamflow Predictions Using GDAPS and WRF-Hydro
Yaewon LEE+, Bomi KIM, Garim LEE, Saehyeon OH, Seong Jin NOH#
Kumoh National Institute of Technology, Korea, South
Mid-range hydrologic forecasting is essential to understand the impact of hydrologic conditions on water quality and related aquatic ecosystem and to prepare for preemptive measures. In this study, we assess feasibility of high-resolution ensemble hydrologic modeling combined with numerical weather forecasting for mid-range streamflow predictions. The Global Data Assignment and Prediction System (GDAPS) is applied to the distributed hydrological model WRF-Hydro with a 100-meter resolution for streamflow predictions up to 10-day forecasting horizon in the Geumho River basin, a tributary of the Nakdong River, South Korea. Model-Independent Parameter Estimation and Uncertainty Analysis (PEST) model is utilized to reduce the parametric uncertainty of the high-resolution physical model. Then, to mitigate the uncertainty of mid-range weather forecasting information, multiple ensemble approaches are adopted and evaluated. In the presentation, we focus on a potential remedy to improve the performance of mid-range hydrologic predictions in the context of high-resolution.
HS51-A001
Climate Change-induced Thermodynamic Effects on the Localized Heavy Precipitation: The August 2022 Senjo-kousuitai Event in Tohoku, Japan
Ryotaro TAHARA#+, Yusuke HIRAGA
Tohoku University, Japan
In recent years, the frequency and magnitude of flood damage caused by localized heavy rainfall, known as “Senjo-kousuitai”, have been increasing in Japan. Therefore, understanding the response of localized heavy rainfall to climate change is critical for adaptation to flood damage. Here we take the August 2022 heavy rainfall event in the Tohoku and Hokuriku regions, we performed a pseudo global warming experiment based on SSP2-4.5. In the pseudo global warming experiment, the effects of each thermodynamic environmental field, such as air temperature and relative humidity were evaluated, and future changes in the “Senjo-kousuitai” and their mechanisms were analyzed. The results show that in two basins (the Arakawa River basin and the Nagasaki watershed), where precipitation was particularly heavy during observed heavy rainfall events, the basin-averaged 48-hour cumulative precipitation doubled when only the temperature warming effect was considered. On the other hand, when the warming effects of air and sea surface temperatures were considered, cumulative precipitation did not change significantly compared to the present climate, but rainfall became more intense and shorter in duration. The cumulative precipitation decreased when the warming effects of air temperature, sea surface temperature, and relative humidity were considered, indicating an increase in precipitation at sea compared to the present climate. These changes are explained by changes in the amount and duration of the water vapor flux and by the stabilization and destabilization of the atmosphere as indicated by the convective effective potential energy (CAPE).
HS51-A006
Hydrological Homogeneous Regions for Extreme Rainfall of South Korea Across Different Rainfall Durations
Ju-Young SHIN#+, Jiyeon PARK, Azamat BAIMAGANBETOV
Kookmin University, Korea, South
The intensity of rainfall is increasing, and rainfall events with high rainfall intensity cause flooding in urban areas. There is a need for realistic alternatives to the design criteria for urban flood defense facilities to prepare for urban flooding. It highlights the necessity for pragmatic design alternatives for urban flood defense mechanisms, especially against short-duration, high-intensity rainfall. For this reason, frequency analysis using sub-hourly rainfall observations is required to calculate design criteria. Due to the observation resolution of rain gauges, sub-hourly rainfall observations are subject to many uncertainties. To mitigate this uncertainty, it is necessary to apply a methodology such as regional frequency analysis instead of at-site frequency analysis. To date, regional frequency analysis of rainfall data has not considered the effect of duration when classifying hydrological homogeneous regions. Since the causes of rainfall events are different depending on the duration, the analysis method for rainfall data by duration should be different. In this study, we analyzed a hydrologically homogeneous region for various rainfall durations to investigate and compare the characteristics of short-duration and long-duration rainfall events. In this study, the Seoul area was selected as the target area, and the characteristics of extreme rainfall events were analyzed using data from AWS stations of the Korea Meteorological Administration in the Seoul area.
HS51-A008
Asymmetric Response of Terrestrial Hydrologic Cycles Up to Carbon Dioxide Removal
Jiwoo CHOI1+, Hyungjun KIM1,2#
1Korea Advanced Institute of Science and Technology, Korea, South, 2The University of Tokyo, Japan
Since the Industrial Revolution, the continuous increase in Earth's CO2 concentration due to human activities has led to serious climate change. Reducing CO2 emissions is important, but it is equally crucial to conduct Carbon Dioxide Removal (CDR) that has already been emitted into the atmosphere. Therefore, it is essential to analyze the changes in the climate system resulting from not only the increase but also the decrease in atmospheric carbon dioxide. In this study, a global river model, the Catchment-based Macro-scale Floodplain model (CaMa-Flood), was used to investigate the terrestrial hydrological responses to different levels of global warming. To force the model, total runoff data were collected from the piControl experiment (fixed CO2 at pre-industrial levels), the 1pctCO2 experiment (increasing CO2 by 1%/yr from pre-industrial), and the 1pctCO2-cdr (decreasing CO2 by 1%/yr after quadrupling) of five CMIP6 models (CNRM-ESM2-1, CanESM5, GFDL-ESM4, NorESM2-LM, and MIROC-ES2L). We investigated changes in hydrological variables such as river discharge and flooded area globally and for nine major river basins including the Amazon, Congo, and Mississippi. We further analyzed the asymmetricity and reversibility of the changes in hydrologic cycle.As a result, asymmetric responses in total discharge were observed in the Amur (-3.9%), Congo (4.2%), Lena (4.5%), Mississippi (-7.5%) between the earlier and latter half of the period, which implies that the discharge in Amur and Mississippi will overshoot after the peak of CO2 and recover with delay. Irreversible responses, which compare the first and last 20-year mean discharge, were shown in the Amur (7.8%), Lena (4.8%), Yenisei (3.3%). This suggests that even if the concentration of CO2 decreases sufficiently due to our successful efforts to reduce greenhouse gas emissions, the ramp-down pathway may differ significantly from the ramp-up in terms of hydrology, emphasizing the importance of taking swift action to tackle climate change before the overshooting.
HS52-A001
Precipitation Forcing-induced Uncertainties in Land Surface Model (LSM) Simulations
Seulchan LEE1+, Jongmin PARK2, Minha CHOI1#
1Sungkyunkwan University, Korea, South, 2Korea National University of Transportation, Korea, South
Land surface model (LSM) simulations have been one of the most effective ways to retrieve hydrological states and fluxes in ungauged regions. However, variables simulated from LSMs are prone to substantial uncertainties, mainly originating from precipitation forcings. The main reason of the uncertainty is the high level of spatio-temporal variability inherent in the precipitation data, which is particularly true over the Monsoon Asian (MA) region. When used as a forcing data of LSMs, the uncertainties are propagated through non-linear land surface processes, influencing fluxes of water and energy. Recent advances in remote sensing techniques have led to produce several multisource-based precipitation data, which has inherent uncertainty based on different algorithms. In this context, this study aims to evaluate precipitation estimates from Modern-Era Retrospective analysis for Research and Applications, version 2 (MERRA2), Global Data Assimilation System (GDAS), Integrated Multi-satellitE Retrievals for GPM (IMERG) and Climate Hazards Group InfraRed Precipitation with Station data (CHIRPS), and their capabilities as forcings in simulating hydrological processes over MA. We first analyze the accuracy of different precipitation estimates by comparing them against ground measurements-based Asian Precipitation - Highly-Resolved Observational Data Integration Towards Evaluation (APHRODITE) gridded data. Afterwards, soil moisture (SM) and evapotranspiration (ET) simulated from Noah-MP LSM along with different precipitation forcings are compared against the reference simulation to check the influence of different precipitation forcings. Finally, this study analyzes the propagation of spatio-temporal uncertainties in precipitation forcings towards simulated SM and ET.
HS52-A005
Evaluating ECOSTRESS Instantaneous Evapotranspiration Across the Korea
Kijin PARK1+, Chanyoung KIM1, Kiyoung KIM2, Jongmin PARK1#
1Korea National University of Transportation, Korea, South, 2Korea Institute of Hydrological Survey, Korea, South
Recently, in Korea, the effects of extreme weather due to global climate change have caused a localized energy imbalance, affecting the observation of evapotranspiration (ET). As 40-60% of the annual precipitation (about 1,200 mm) is lost to the atmosphere through ET, accurate quantification of ET is essential for water resource management. Traditionally, ET has been measured though ground-based observations (e.g., evaporation pan, lysimeter) while it has limitation in representing spatial behavior of ET. In order to overcome this, there is a recent trend to utilize hydrometeorological variables estimated from remote sensing imagery. In this study, we utilized Ecosystem Spaceborne Thermal Radiometer Experiment on Space Station (ECOSTRESS) imagery developed at National Aeronautics and Space Administration Jet Propulsion Laboratory and launched on the International Space Station in June 2018 to monitor the global vegetation water use and stress and ET globally. Among the various datasets, this study selected instantaneous ET calculated by the Priestley-Taylor Jet Propulsion Lab algorithm as the research data. ECOSTRESS instant ET estimates from June 2018 to December 2022 were compared and validated with the observed ET from 13 eddy covariance flux towers located in Korea. Overall results revealed that ECOSTRESS based ET showed capability to represent the detailed spatial distribution of ET. Acknowledgement: This work was supported by Korea National University of Transportation 2024.
HS52-A006
Improving Daily Precipitation Estimates by Merging Satellite and Reanalysis Data in Northeast China
Yuxi CAO+, Gaohong YIN#
Jilin University, China
Precipitation plays a crucial role in the water cycle, and accurate precipitation measurements are meaningful in hydrological studies. Conventional gauges directly measure precipitation but provide point measurements and demand expensive operational costs. Satellites and models yield spatially continuous precipitation estimates, while the errors and uncertainties remain unclear. Therefore, satellite and reanalysis data are often used with gauge measurements to characterize uncertainties and improve precipitation estimates. However, its application is hindered in regions with sparse gauging networks or where gauge data are inaccessible. Thus, the study proposed to improve daily precipitation estimates without relying on gauge measurements in Northeast China. The performance of satellite-based estimates (FY, IMERG, GSMaP) and reanalysis data (ERA5, CRA-40) are evaluated. A triple collocation-based method is used to quantify the uncertainty of different products and merge multi-source data sets. Afterward, we compare the merged high-resolution product against gauge measurements to validate its accuracy. Additionally, the Multi-Source Weighted-Ensemble Precipitation (MSWEP) is used as the reference data set and compared with the merged product. The outcome of the study will provide a comprehensive evaluation of various precipitation products in Northeast China. The high-accurate and high-resolution merged precipitation estimates will establish a solid data foundation for water cycle simulation in Northeast China.
HS52-A008
A Deep Learning Approach for the Prediction of Harmful Algal Blooms in the Nakdong River Basin in South Korea
Yookyung JEONG+, Kyuhyun BYUN#
Incheon National University, Korea, South
The heightened risk of harmful algal blooms (HABs) is intensified by extreme climatic and hydrologic events, along with the increased prevalence of non-point pollutant sources associated with agricultural and industrial activities. The deteriorating water quality due to HABs presents substantial challenges to water management and aquatic ecosystems. Specifically, the occurrence of HABs is influenced by intricate interactions among weather conditions and hydrologic and water quality factors. Predicting HAB occurrences and concentrations poses challenges for conventional physical models, primarily because they struggle to capture the sophisticated interactions of the occurrence factors and the characteristics of non-linear, non-stationary systems. To address this challenge, our objective is to develop a deep learning approach based on the wavelet transform, concentrating on key hydrologic and water quality factors for the Nakdong River in South Korea. Specifically, we extract the main factors that significantly impact HAB occurrence by analyzing the correlation of HAB occurrence and many factors. Through the application of the wavelet transform, we obtain denoised HAB data to improve the effectiveness of our predictive model. Subsequently, we utilize Long Short-Term Memory (LSTM) networks, incorporating the extracted key factors and denoised data as input data. Our preliminary results reveal a high Nash-Sutcliffe Efficiency (NSE) and a low Root Mean Squared Error (RMSE). These results demonstrate that the developed framework in this study makes it possible to predict HAB occurrence with high accuracy. Furthermore, we expect that the constructed model contributes to the establishment of the pre-emptive management for HAB occurrence. Acknowledgment: This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. NRF-2022R1A4A3032838).
HS52-A012
The Altitude Effect of δ18O in Precipitation and River Water in a Permafrost-Underlain Headwater Basin, Northeastern Tibetan Plateau, China
Xiong XIAO1+, Yang WANG2#
1Hunan Normal University, China, 2Inner Mongolia Normal University, China
The effect of altitude on stable isotopes in precipitation and river water is valuable for studying water cycle and paleo-elevation reconstruction. In this study, we collected precipitation and river water samples along an altitude transect in the Binggou Basin, Northeastern Tibetan Plateau. We also investigated the topographical and meteorological factors in the basin to understand the altitude effect and its influencing factors on the δ18O in precipitation and river water (δ18OP and δ18OR). Our results indicate that the δ18OP lapse rate was 0.25‰ per 100 meters, approximating the global average of 0.28‰ per 100 meters. The linearly fitting considering the average, lowest, and highest altitudes showed that the δ18OR lapse rates were 0.28‰ per 100 meters, 0.095‰ per 100 meters, and 0.07‰ per 100 meters, respectively. Notably, the linear relationship between the δ18OR values and average altitudes exhibited stronger correlations. Multiple linear regressions further confirmed that average altitude exerted the most significant influence on the δ18OR, affirming the feasibility of paleo-altitude reconstruction based on average altitude within this study region. We observed that the spring δ18OR lapse rates were higher than those in summer, with altitude playing a less prominent role in influencing the summer δ18OR. This can be attributed to the freeze-thaw cycle and the shift of runoff flowpaths from spring to summer. Our study underscores that the δ18OR lapse rates can exhibit strong seasonality with large variability when analyzed concerning different altitude parameters, associated with the seasonality of runoff generation processes influenced by the freeze-thaw cycle.
HS52-A013
A Comparative Study on Records of Stalagmite δ18O/δ13C and Trace Element Ratios from Zhenzhu Cave in Northern China Over the Past 130 ka
Zhiguo RAO#+
Hunan Normal University, China
On glacial-interglacial timescales, the records of stable oxygen isotopes (δ18O) from stalagmites in central China, and the records of East Asian summer monsoon (EASM) intensity/precipitation amount reconstructed from loess deposits in northern China, have been suggested to show different change patterns. Here, we report new records of trace element/Ca ratios (Mg/Ca, Sr/Ca, Ba/Ca, P/Ca) from stalagmite PS1 from Zhenzhu Cave in northern China over the past 130 ka. Combined with previously reported high-resolution stable carbon isotopes (δ13C) and δ18O records from the same stalagmite, and other EASM records, we discuss the regional hydroclimatic evolution. Based on two years’ monitoring results and the relationship between trace element/Ca ratios, the Mg/Ca of stalagmite PS1 is controlled by the percolating water on the dissolution intensity of bedrock and the leaching of soil-derived elements, and thus reflects the changes of local precipitation amount. Stalagmite growth rates and atmospheric dust activity may both affect the Sr/Ca of stalagmite PS1. The Mg/Ca and δ13C records exhibit highly in-phase co-variation on multi-millennial to orbital timescales and consistent long-term trends, which are also consistent with most loess based EASM precipitation amount records from northern China. These observations indicate that EASM precipitation amount in northern China shows a long-term decreasing trend from marine isotope stage (MIS) 5e-MIS5c-MIS5a-MIS3, followed by an increase towards MIS1. The phase consistency and the inconsistent changes in the long-term trends between the stalagmite PS1 δ18O and Mg/Ca (δ13C) records support that the stalagmite δ18O record reflects phase changes of the EASM rather than absolute changes in EASM intensity. We conclude that EASM precipitation amount (PS1 Mg/Ca and δ13C) and precipitation isotopes (PS1 δ18O) reflect different facets of the EASM circulation system over the past 130 ka.
HS52-A018
The Effect of Convective/Advective Precipitation Partitions on Precipitation Isotopes in the Monsoon Regions of China: A Case Study of Changsha
Xinping ZHANG1#+, Xiong XIAO1, Xinguang HE1, Zhuoyong XIAO1, Xin CHANG1, Huade GUAN2
1Hunan Normal University, China, 2Flinders University, Australia
Convective/advective precipitation partitions refer to the divisions of precipitation that are either convective or advective in nature, relative to the total precipitation amount. These distinct partitions can have a significant influence on stable isotope composition of precipitation. This study analyzed and compared the effect of precipitation partition on δ18O in precipitation (δ18Op) by using daily precipitation stable isotope data from Changsha station and monthly precipitation stable isotope data from the Global Network of Isotopes in Precipitation (GNIP), under different time scales, periods (i.e., annual, warm season and cold season), and precipitation intensities. The results showed that the correlation between the convective precipitation fraction (CPF) and total precipitation amount was influenced by the intensity of convection in different periods. On both daily and monthly scales, the CPF decreased as the precipitation amount increased during the warm season, while increased with increasing precipitation amount in the cold season. Regardless of the season, the δ18Op in Changsha consistently increased with increase in CPF on a daily scale. In the cold season, the effect of precipitation partition on δ18Op was stronger than that of the precipitation amount effect, as compared to the situation in the warm season. As a result, the regression line slope between the CPF and δ18Op increases with increasing precipitation intensity in the warm season, meaning that as the CPF increases, the δ18Op increases at a faster rate under higher precipitation intensity. Similarly, the slope increases with increasing precipitation intensity in the cold season. This suggests that precipitation intensity and convection intensity can affect the relationship between the CPF and δ18Op. Our findings shed light on how different precipitation partitions affect stable isotope composition of precipitation, thus enhancing our understanding of the variability of precipitation stable isotopes in the monsoon regions of China.
HS52-A019
External Forcing Mechanisms Controlling the Qiongdong Upwelling in the Northern South China Sea During the Holocene
Chao HUANG#+
Guangdong Ocean University, China
Coastal upwelling along the northern South China Sea controls regional marine productivity and thereby influences blue economies. However, centennial-scale upwelling variability and its associated forcing mechanisms are poorly understood, primarily due to the lack of high-resolution upwelling records beyond the instrumental and historical periods. Here we reconstruct monsoon-induced upwelling variations over the past 7000 years, based on a high-resolution (~30 yr) δ15N record from the upwelling zone off the east coast of Hainan Island. δ13C, δ15N, C/N, TOC and biogenic opal are determined to verify the dominant source of marine organic matter in the GH6 core, and δ15N values are used to indicate the variations in nitrate utilization by phytoplankton. The results show distinct centennial-scale variability, which is generally synchronous with solar activity, latitudinal shifts of the Intertropical Convergence Zone (ITCZ), and El Ni˜no-Southern Oscillation (ENSO) frequency. We conclude that the centennial-scale upwelling intensity was predominately induced by external solar forcing, with internal feedback such as latitudinal shifts of the ITCZ and ENSO variability as a mediator amplifying the solar variation signal. Our new findings indicate that external forcing mechanisms exerted a significant influence on upwelling variations before the Anthropocene and should be considered when producing future projections of upwelling changes at low latitudes.
HS52-A022
Transmission Characteristics and the Factors Influencing Stable Oxygen Isotopes in Precipitation, Soil Water, and Drip Water in Remi Cave, Western Hunan, China
Zhiguo RAO#+, Yunxia LI
Hunan Normal University, China
We conducted monthly in-situ monitoring of local precipitation, soil water at three different soil depths (SW-40, SW-50, SW-95), and five cave drip water sites (D1‒D5) in Remi cave, Central China, from January 2021 to July 2022. On an intra-annual timescale, local precipitation δ18O (δ18Op) showed a significant monthly variation, mainly controlled by changes in moisture sources, upstream convective activity, and rainout effects. With the increasing thickness of the soil layer above the cave, soil water δ18O (δ18Osoil) gradually became negative and leveled off, possibly because shallow soil water (SSW; SW-40, SW-50) responded sensitively to local year-round precipitation, accompanied by surface evaporation. In contrast, deep soil water (DSW; SW-95) was mainly replenished by heavy precipitation during the wet season, which had more negative δ18O. Due to the smoothing effect of water storage within the epikarst zone, the seasonal amplitude of drip water δ18O (δ18Od) variation at five drip sites was much smaller than those of δ18Op and SSW δ18Osoil. The mean δ18Od at sites D1 and D2 near the cave entrance was heavier than SSW δ18Osoil and the amount-weighted annual average δ18Op (δ18Op-aw), possibly due to evaporation from the thin overlying soil layer, together with the ventilation effect. However, the mean δ18Od at sites D3, D4 and D5, in the middle and inner parts of the cave, were lighter than δ18Op-aw and close to the value of DSW δ18Osoil and the amount-weighted average δ18Op in the wet season. This suggests that the thick soil layer overlying the cave raises the precipitation threshold, causing these sites to be mainly recharged by heavy rainfall in the wet season. Our observations indicate that the δ18O of stalagmites growing within the stable environment of RM cave, with a thick overlying soil layer, mainly inherit the wet-season δ18Op signal.
HS53-A002
Examining Ecological Drought-based Hydrological Flow Indicators for Integrated Water Management at the Watershed Scale
Jung-Hun SONG1#+, Hakkwan KIM2
1Chungnam National University, Korea, South, 2Seoul National University, Korea, South
Global warming has intensified unusual patterns in the water cycle, resulting in significant alterations and risks to ecosystems. Therefore, it is essential to develop a comprehensive management system that takes into account water flow, quality, and ecological aspects. This study focuses on developing flow indicators for hydrology that can assess the preservation of a natural and balanced flow. Our goal is to propose hydrological flow indicators based on ecological drought assessment at the watershed scale. First, we selected flow criteria such as Aquatic Base Flow to serve as thresholds for ecologically required flows. Second, we established grading criteria based on ecological drought assessments to evaluate the state of the water environment. Lastly, we proposed hydrological flow indicators that incorporate these flow criteria and ecological drought grades. We applied the proposed hydrological flow indicators to three watersheds: Gapyeonggyo, Yangyangdaegyo, and Seonsan, to assess their applicability. The evaluation results indicate that the selected flow criteria, which reflect monthly flow patterns, can serve as a robust quantitative index. These criteria are capable of assessing the extent to which the current flow deviates from historical averages. Furthermore, the grading criteria based on ecological drought classifications allowed us to evaluate whether the flow is consistent with natural conditions. The hydrological flow indicators proposed in this study may require further research and refinement, potentially through expert consultations. Nonetheless, they show promise as useful metrics for future integrated water management efforts. This work was supported by National Institute of Environmental Research (NIER). This work was also supported by Korea Environment Industry & Technology Institute(KEITI) through Water Management Program for Drought, funded by Korea Ministry of Environment(MOE)(RS-2023-0023194).
HS53-A004
Development of an Extreme Drought Response Protocol Through Reproduction of Past Drought Cases
Hyunjung KIM+, Gyumin LEE, Kyoungwon MIN, Doosun KANG#
Kyung Hee University, Korea, South
In South Korea, from the second half of 2022, the Yeongsan and Seomjin rivers experienced extreme drought that lasted until early 2023. Changes in precipitation patterns and an increase in the frequency of extreme hydrological events due to climate change are making it difficult to secure stable water resources. Furthermore, the basin with water distribution system which is vulnerable to drought due to increasing water demand depending on the characteristics of the water resources and the region. For this reason, a multifaceted water security strategy is needed to efficiently connect water supply chains such as dams and reservoirs across the country, including areas experiencing water shortages, and to eliminate vulnerable water supply areas in preparation for future water demand increases. Therefore, the goal of this study was to establish an emergency response protocol for each scale of water shortage based on the linked operation of water facilities. This study investigated various cases of response processes and systems to extreme drought events that have occurred in Korea in the past, and analyzed them to propose methods and protocols to appropriately respond to possible future extreme droughts and secure water supply stability. Therefore, the cases of extreme droughts that have occurred in the past at Youngsan and Sumjin river basins, their responses and alternative scenarios are quantitatively reproduced. Furthermore, this study proposes different response scenarios for more efficient response, and the appropriateness of water supply standards and emergency response methods by drought stage is evaluated. Ultimately, emergency response protocol and procedures that need to be improved in the future are derived through this process. Acknowledgement: This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Water Management Program for Drought, funded by Korea Ministry of Environment(MOE)(RS-2023-0023194).
HS53-A005
Sequential Adaptive Reallocation Algorithm for Drought Conditions Based on Hydropower Pinch Analysis and Long-term Forecasting
Doosun KANG#+, Amir Saman TAYERANI CHARMCHI, Fatemeh GHOBADI
Kyung Hee University, Korea, South
In the face of climate change, proactive water resources management is essential, particularly for drought mitigation. This study introduces the Sequential Adaptive Reallocation Algorithm (SARA), a novel framework using a 12-month ahead reservoir inflow prediction integrated with Hydropower Pinch Analysis (HyPoPA) for sustainable water management. SARA applies a rule-based, priority-driven approach to early-stage operational decision-making. By reconfiguring water allocations based on long-term predictive data and continuously aligning with HyPoPA's optimal conditions, SARA ensures efficient water resources distribution across multiple sectors. The algorithm's effectiveness is evaluated through a comparative analysis in a real-world drought scenario, assessing SARA's allocations against actual inflows and historical data. Preliminary results suggest that SARA's integration with HyPoPA enhances water allocation reliability and efficiency, outperforming conventional methods. This approach contrasts markedly with actual management strategies, which led to significant water losses, including over 25 gigawatt-hours of potential energy and approximately 3 billion cubic meters of water, as highlighted by HyPoPA. This approach signifies a substantial advancement in forecasting-based water management, promising enhanced sustainability and efficacy in countering drought impacts. Acknowledgement: This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Water Management Program for Drought, funded by Korea Ministry of Environment(MOE)(RS-2023-0023194).
HS53-A008
| Invited
Simple Direct Evapotranspiration Measurements with a New Cost-optimized ET Flux Sensor
George BURBA1#+, Sasha IVANS2
1University of Nebraska/LI-COR, United States, 2LI-COR, Inc., United States
With an estimated 2 billion people already affected by water scarcity and a projected 3 billion facing shortages by 2050, optimizing water management is crucial for sustainable water use. Evapotranspiration (ET) plays a vital role in the global water cycle, moving 500,000 km3 of water annually, with 70,000 km3 occurring over land. This amount surpasses the global water demand of approximately 4,600 km3 per year. By conserving just 5-10% of ET through retention in soil, groundwater, or freshwater bodies, a significant contribution can be made towards solving the global water scarcity issue. Accurate measurement of ET is essential for effective water management in specific areas. Conventional models such as potential, reference, max, equilibrium, and pan do not achieve the necessary level of accuracy, which is better than 5-10%. However, direct ET measurements using the eddy covariance method provide the required resolution. Historically, the high cost and complexity of this approach have limited its usage primarily to academic research. To address these challenges, a new cost-effective solution for direct, automated, and real-time ET measurements has been developed, to extend this technology beyond academia to broader research, regulatory, and commercial domains. The LI-710 sensor is a user-friendly device that measures ET, sensible heat, temperature, humidity, and air pressure every 30 minutes. It is significantly more affordable than typical flux stations, costing 5-10 times less, and consumes 3-15 times less power. Moreover, it can be easily installed and utilized by individuals with limited experience in the field. The preliminary field test results of this innovative technology will be compared with traditional higher-cost research-grade eddy covariance systems. By providing more accurate and affordable ET measurements, this new technology has the potential to optimize water management in various hydrological settings. Ultimately, it contributes to addressing the global water scarcity problem through sustainable water use.
HS53-A017
| Invited
An Inspection of the Sediment Control Works in Soil and Water Conservation Engineering, in Southern Taiwan
Yu-Wen SU#+, Yu-Chao HSU
National Cheng Kung University, Taiwan
ARDSWC, MOA., Taiwan (R.O.C.) to ensure that the sand control facilities can continue to function, achieve asset maintenance and management, and further achieve the purpose of extending the life of the project, this study was handled. Taking 14 watersheds in the work area of Tainan Branch, ARDSWC as the scope, we conducted inspections of 200 important sand control structures. The current functional evaluation level is A-level (the structure is in good condition and has sound functions) with 179 seats, B-level (slight wear and tear, but the original function can still be maintained) with 12 seats, C-level (partially damaged, affecting functionality) with 2 sests, and D-level (total damage or loss of function ) with 8 seats. Overall, 95% of the 200 structures in the target catchment area of this project are in good functional condition, and 5% are in a damaged or destroyed state, indicating that most sand control structures continue to exert functional benefits. Among the damage types of structures, the main damage is caused by water and sand impact damage (4 works) or soil and sand siltation (2 works). Significant changes in river soil and sand erosion are the main types that causes partial damage to structures (foundation erosion) and affects functionality. During the implementation of this study, four typhoons were encountered. After reviewing the record data of major typhoons and heavy rain events in the past 10 years, it is found that the number of impacts and disturbances caused by hillside slopes in southern Taiwan is smaller or milder. Based on the survey results, a life extension assessment of sand control facilities is conducted, and it is recommended to favor normal maintenance and management actions. If some foundation excavation affects the functional appearance of the structure, feedback can be provided as a reference for normal management design.
Session Chair(s): Doosun KANG, Kyung Hee University, Seokhyeon KIM, Kyung Hee University, Ashish SHARMA, UNSW Sydney, Dagang WANG, Sun Yat-sen University
HS53-A007
| Invited
Drought Propagation in the Yeongsan River Basin
Guhyup KANG#+, Jaehyeong LEE, Yeonjoo KIM
Yonsei University
Drought is a natural disaster with extensive economic, social, and environmental impacts. It affects the water cycle, the natural environment, and human society. Despite many studies, there still needs to be a comprehensive understanding of the characteristics, processes, and factors that drive drought propagation. We used remote sensing and a process-based modeling approach to better understand drought propagation in the Yeongsan River Basin. We used NASA Soil Moisture (SMAP) data and Vegetation Optical Depth to evaluate agricultural and ecological drought. We also implemented the Weather Research and Forecasting Model Hydrological modeling system (WRF-Hydro) to characterize drought propagation based on model outputs. By comparing the results from remote sensing and WRF-Hydro, we evaluated the performance of these two approaches in understanding drought propagation in the Yeongsan River Basin. Acknowledgment: This work was supported by the Basic Science Research Program through the National Research Foundation of Korea, which was funded by the Ministry of Science, ICT & Future Planning(No. 2020R1A2C2007670), and the Korea Environment Industry & Technology Institute (KEITI) through the Water Management Program for Drought, funded by the Ministry of Environment (MOE) of Korea (RS-2023-0023194).
HS53-A001
| Invited
Achieving Participatory Planning of Water Resources Using Shared Vision Model: Case Study on the Yeongsangang and Seomjingang Basins in South Korea
Joohyung LEE#+, Jaehwang LEE, Young-Oh KIM
Seoul National University
Korea's existing dams have been designed and operated to address droughts lasting 1 or 2 years, with a safety margin set to accommodate droughts occurring up to a return period of 20 years. However, recent multi-year droughts have severely impacted certain regions, reducing water supply while causing significant harm to actual water users. To prepare for droughts lasting over 2 years, a different approach from the current water allocation strategies is required. Developed countries like the United States have included both water suppliers and users in decision-making processes through shared vision planning, proving its effectiveness in devising water allocation plans. Therefore, this study aimed to design a shared vision model for the Jeonnam region in South Korea, which faced water supply difficulties due to severe drought from 2021 to early 2023. The model was intended to be used in actual water allocation planning, involving stakeholders from the model-building phase to reflect the water allocation mechanisms of two basins (Yeongsangang and Seonjingang) and consider the water supply adjustment standards of each dam. The constructed shared vision model was validated through structure and parameter verification tests, achieving over 90% and 85% correlation, respectively, using 2022 observational data. This model allows assessment of water storage of each dam and reservoir, flow rates of each basin, and the amount of supplied water under various inflow scenarios. By utilizing these variables, water suppliers and users can engage in conflict resolution based on scenarios discussed during meetings, achieving participatory planning for water resources. The model facilitates the formulation of sector-specific water allocation plans for extreme drought scenarios under normal circumstances and aids emergency response protocol establishment and real-time decision-making during severe drought occurrences.
HS53-A009
| Invited
Enhancing Water Distribution Decisions with an Emphasis on Fairness Under Drought Condition
Seung Beom SEO1#+, Hee Won JEE1, Yeonju KIM1, Jiheun KIM2
1University of Seoul, 2North Carolina State University
This study introduces a comprehensive, multi-lateral decision-making model specifically designed for managing drought conditions to address the complexities of water allocation across competing stakeholder interests. A polit study basin, the Yeongsan River basin in South Korea, supplies water for both domestic and agricultural water needs. However, it is vulnerable to persistent water scarcity, resulting in long-term drought and stakeholder conflict over water rights. The proposed framework has the dual goal of equitable and sustainable water allocation. The study employs a multi-objective optimization approach to identify solutions that balance the diverse interests of stakeholders while reducing potential conflicts. Two main objective functions are considered: i) maximization of the basin's net profit and ii) equitable water allocation based on quantitative reliability. Further, the study applies sequential game theory to evaluate different scenarios of cooperation and non-cooperation, particularly in the context of river water withdrawal restrictions in the upstream and midstream areas of the basin. Additionally, the framework suggests using Shapley values as a basis for determining compensation for collaborative efforts. This study underlines the importance of equity, efficiency, and sustainability in water resource management. It aims to offer valuable guidance to policymakers and stakeholders in making informed, fair decisions during drought conditions, considering multiple objectives and embracing the principles of fairness. Acknowledgement: This study was supported by the National Research Foundation of Korea (NRF), grant number NRF-2021R1C1C1004492.
HS53-A010
The Decision Support Framework for the Flood Early Warning
Tae Sung CHEONG#+
National Institute for Disaster Prevention
Small streams are known to be the most affected by climate change, and as flood damage has been on the rise in recent years, it is urgent to prepare measures to adapt to climate crisis. As the small stream is located at the top of the river network, the flood effect on the downstream river is large, so integrated flood management efforts using green infrastructure or natural-based solutions are required. Along with these structural measures, it is possible to reduce flood damage in small streams when non-structural efforts such as the development of a flood early warning system to reduce casualties are carried out. The research develops a decision support framework including measurement data-based flood prediction optimization model and criteria for issuing flood warning for the development of an early warning system and applies it to four small streams to verify the model. As a result of the verification, the flood prediction model is found to generate the flood event of small streams well, and it is expected that it can be used to develop a flood early warning system for small streams in the future.
HS53-A003
Sensitivity Analysis of Groundwater Levels to Surface Temperature Variations in South Korea Under Climate Change
Yaggesh Kumar SHARMA1#+, Dae Heon HAM1, Seokhyeon KIM1,2
1Kyung Hee University, 2UNSW Sydney
In South Korea, the region is heavily impacted by climate change, the goal of this study is to evaluate the effects of fluctuations in surface temperature on groundwater levels (WL). Rising air and surface temperatures can have a negative impact on groundwater which is an important resource in day to day life. We used information from about 500 monitoring wells that were placed thoughtfully all throughout South Korea and provided us with daily assessments of groundwater levels. The framework consists of quantile regression aimed at particular quantiles (e.g., q=0.5, 0.9, 0.95, 0.99) combined with a scaling analysis using the common logarithm for groundwater level (WL) data on the y-axis. This method makes it easier to find the slope of each regression, which helps determine the scaling factor, alpha. The metric known as alpha is used to assess how sensitive WL is to temperature. It represents the percentage change in groundwater level for every 1°C increase in air temperature. A primary focus of our research is the analysis of the alpha's spatial distribution with respect to particular quantiles. The study has important consequences since the sensitivity indicated by the scaling factor (alpha) at different quantiles helps to identify areas that are vulnerable to changes in groundwater levels caused by climate change. These kinds of findings are vital for formulating solutions and plans to mitigate the effects of groundwater resource changes brought on by climate change. This work highlights the significance of customized studies and interventions for particular places and adds to a more sophisticated understanding of groundwater dynamics within the context of global climate change. This work was supported by the Korea Institute of Energy Technology Evaluation and Planning (KETEP) and the Ministry of Trade, Industry & Energy (MOTIE) of the Republic of Korea (20224000000260).
HS53-A011
Projection of Extreme River Level in the Slums of San Salvador, El Salvador, Under Climate Change Conditions, Using the d4PDF Database
Mariana Beatriz AVALOS CABRERA#+, Masafumi YAMADA, Tomoharu HORI
Kyoto University
This study investigated the impact of climate change on extreme river levels in the metropolitan area of San Salvador, the capital of El Salvador, using a large ensemble climate simulation database for policy decision-making for future climate changes (d4PDF). Informal dwelling is a severe socio-economical issue in the city that emerged from rural-urban migration. The city has 792 slums in which 32% of its population settles. Many of these are located inside river channels. In 2020, two continuous tropical storms struck the country, the biggest in the last 22 years, and many of them were washed away or partially destroyed due to the rapidly increasing water level and their location inside the river. The studied basin has never been analyzed before. The extreme precipitation events were extracted from future climate simulations (over 5,000 years ranging from 2051 - 2111) in which global mean surface air temperatures are 4K higher relative to preindustrial levels. A two-dimensional, distributed hydraulic and hydrological model capable of simultaneously simulating rainfall-runoff and flood inundation (RRI Model) was used to simulate future extreme river flow levels. Over 100 actual river cross-sections were integrated into the model to improve reliability. Seven slum locations were selected to analyze how likely they are to be flooded, considering the altitude of their emplacement inside the river channel and the modeled river water levels, comparing it to the impact of the 2020 storms. Precipitation in the basin is expected to reduce by the end of the 21st century. However, extreme rainfall intensifies.
HS53-A012
Influence of Past River Level on Evacuation Decision with the Decision Criteria Acquisition Model
Genki KIRIMORI#+, Tomoharu HORI, Masafumi YAMADA
Kyoto University
In Japan, residents have recently been encouraged to make proactive evacuation decisions as a soft measure against flooding. The key to effective evacuation is how and which information residents use. Therefore, we focused on the evacuation decision criteria that residents obtain when using river water levels as a decision criteria. Specifically, using a reinforcement learning model that learns from a huge number of floods, we compared the learning results (1)when only the current river level was used and (2)when current and past river levels were used. As a result, (2)when past water levels were used, a more rapid rise in water levels could be recognized than when (1)past water levels were not used. On the other hand, an unnatural tendency was also observed in the learning results (decision criteria) due to the insufficient number of rainfall scenarios used as input.
HS53-A013
Evaluating the Underlying Potential of Buddhism Temples as Flood Evacuation Shelters
Ryo KOBAYASHI#+, Masafumi YAMADA, Tomoharu HORI
Kyoto University
Japan is facing a shortage of evacuation shelters, highlighting the need to designate new ones. Observing instances where temples, having escaped catastrophic damages during past disasters, were widely used as shelters nationwide, we hypothesized that temples might be well-suited as evacuation shelters. Grounded in this context, we conducted an analysis of temple geographical characteristics and examined their potential as emergency evacuation shelters during floods. We obtained the result that temples are often located on natural embankments, offering a relatively safe terrain against floods compared to their surroundings. The overlay analysis between temples, designated emergency evacuation shelters and flood-assumed areas did not show that temples is safer than designated emergency evacuation shelters for flood. However, their elevated location suggests that, depending on the surrounding conditions, temples could become relatively safe evacuation shelter. By the way, considering a maximum walking distance of 2 km for evacuation, designating temples as emergency shelters could enable up to 4.14 million people (3.3% of the population of Japan) to access evacuation by foot.
HS53-A014
One-hundred-and-fifty-year Impact Trend Assessment on Paddy Irrigation with Dam Reservoir Water Supply
Yuta INOUE, Tomoharu HORI#+, Masafumi YAMADA
Kyoto University
Climate change impact on paddy irrigation has been assessed including the relation between paddy crop growth and water supply by agricultural dam reservoir. Combined model of numerical paddy crop growth model based on AquaCrop and reservoir water supply operation has been developed. Then the model is applied to Chusei irrigation district in Mie Prefecture with the climate conditions simulated by a 150-year continuous experiment based on the RCP8.5 scenario. Combined simulation of crop growth and water supply operation has shown that the increasing trend in paddy yield stops around the 2070s, the timing of dam water storage becomes earlier as time goes on, and water stress becomes severer. The experiment s with different transplanting timing have shown that an earlier transplanting date than the current one is desirable from the viewpoint of average yield maximization, but a later transplanting date is desirable from the viewpoint of stable irrigation water supply.
HS53-A016
How Do the Backwater Prevention Watergates Actually Mitigates Inundations? Case-study in Japan
Masafumi YAMADA#+, Takahiro SAYAMA, Tomoharu HORI
Kyoto University
Dams, levees, and reservoirs - throughout human history we had developed various flood-control infrastructures and continuously built them on the river networks. These infrastructures are now almost omnipresent but spatially heterogeneous, and these in-situ infrastructures are necessarily to be included in the flood and inundation simulation models for that they may represent floods and inundations in a realistic way. However, the database of these in-situ infrastructures are not always available or not complete though available, and normally it takes lots of time and much effort for introducing them into the model. Therefore, the regional or nationwide (or sometimes global) quantification of the actual effect of these infrastructures on the flood and inundation disasters is not thoroughly undertaken. In this study, we focus on the specific infrastructure - backwater prevention watergate. We first made the nationwide database of the backwater prevention watergates from the official documents and maps: finally we revealed that in Japan there are more than 20000 watergates. Second, we projected these watergates onto the river networks of the 150 m resolution whole-Japan Rainfall-Runoff-Inundation model. Based on the comparison of the inundation characteristics of the simulation with and without these watergate models, we examined to quantify the actual effect of these watergates at mitigating and controlling inundation and inundation damages. In the presentation, we will show several examples from the latest large flood disasters.
Session Chair(s): Haiyun SHI, Southern University of Science and Technology, Yi ZHENG, Southern University of Science and Technology, Suning LIU, Southern University of Science and Technology
HS04-A012
| Invited
Deep Learning for Hydrological Sciences: Beyond the Water Cycle
Yi ZHENG#+, Siqi LI, Rui XIONG
Southern University of Science and Technology
The rapid increase of hydrological observation data has enabled deep learning (DL) to achieve great success in rainfall runoff modeling in recent years. However, the performance of deep learning in addressing less data-rich areas in hydrological sciences remains largely unexplored. This presentation introduces two recent study cases showcasing the application of DL for water quality and vegetation modeling. In the first study, we build long short-term memory models to simulate daily riverine nitrogen export in response to hydrometeorological and anthropogenic drivers. In a coastal watershed in southeastern China with a typical subtropical monsoon climate, the DL models exhibit excellent accuracy for both nitrogen concentration and flux. Furthermore, the flux model ensemble, without retraining, performs well in seven distinct watersheds in Asia, Europe, and North America. The study also shows that interbasin consistency of riverine nitrogen export exists across different continents, which stems from the similarities in rainfall-runoff relationships. In the second study, we develop a convolutional recurrent DL model to accurately predict fine-resolution spatiotemporal changes in grass coverage in arid regions. Applying the model to the Gobi Desert reveals that ecological flow regulation contributes to 61.8% of the total increase in grass cover (130.6 km2) in the study area (40,423 km2) over 2005-2015, nearly triple the contribution of local climate change (+23.0%). These studies unveil not only DL's accuracy in complex watershed processes beyond the water cycle but also crucial insights into relevant processes and management implications.
HS04-A001
Adaptive Machine Learning Based Multiobjective Optimization for Scavenging Residual Saltwater in Upstream Subsurface Dams
Jina YIN#+, Chunhui LU
Hohai University
Physically based groundwater flow and solute transport modeling has been limited for seawater intrusion remediation due to computationally intensive evolutionary algorithms. Data-driven machine learning approaches are promising to substitute groundwater numerical models within optimization due to high computing efficiency. However, machine learning surrogates can sometimes accumulate error of forecasting and result in infeasible optimal solutions. To improve fidelity level, this study proposes a novel adaptive machine learning surrogate-assisted multi-objective optimization method for aquifer desalinization. The methodology is demonstrated to seek optimal extraction and injection strategies for residual saltwater removal behind a subsurface dam located in a coastal aquifer. Objectives of minimizing the total extraction-injection rate and maximizing aquifer desalinization efficiency are considered. Three machine learning models including artificial neural network (ANN), gaussian process (GP) and response surface regression model (RSR) are developed to replace a high-fidelity seawater intrusion model for predicting chloride concentrations and salinity mass. Non-dominated Sorting Genetic Algorithm II (NSGA-II) is employed to solve the nonlinear optimization model and obtain Pareto-optimal schedules. Unlike most existing methods using the pre-determined surrogates, poorly-performed machine learning models are adaptively trained in the study to renew predictions during evolutionary search. The optimal solutions achieved by machine learning models are compared against those solutions obtained from one-shot original simulation model., and also verified using the original seawater intrusion model. Results indicate that the developed machine learning models do not only have strong predicting capability, but also maintain equivalent quality of Pareto-optimal solutions compared with those by original simulation models, while maintain the advantage of significantly reducing computational burden up to 95% of time-saving. Especially, the adaptively trained RSR model ensures desired accuracy so that it inhibits error accumulation of forecasting and correctly converges to true Pareto-optimal front. The study found that the proposed methodology had superior performance for multi-objective optimization of aquifer management in accurate convergence, widely-spread diversity, and computational efficiency than conventional methods.
HS04-A002
Assessment of the Evolution of Groundwater Quality Using Machine Learning and Deep Learning Models
Sayantan GANGULY#+, Anisha DAS, Dolon BANERJEE
Indian Institute of Technology Ropar
Groundwater has emerged as an extensively tapped natural resource across the globe to fulfill the demands of agriculture, domestic and industrial sectors. The susceptibility and vulnerability of groundwater quality to potential risks accentuates the imperative need for safeguarding and proficiently managing groundwater resources to ensure long-term sustainability. A prevalent approach employed for evaluating the quality of groundwater within a given region is the application of the Water Quality Index (WQI). The WQI serves as an evaluative metric for ascertaining the conformity of water quality to the established standards pertinent to a specific purpose or application. Historically, the computation of the WQI has entailed intricate calculations, protracted processes, and occasional inadvertent errors in subindex derivation. Consequently, there is a critical need to devise a befitting predictive model for WQI, enhancing the precision of groundwater quality assessments. The formulation of effective plans, policies, and management strategies for groundwater resources is contingent upon the capacity to anticipate pollution in groundwater resulting from various chemical constituents. This study utilises machine learning (ML) techniques and Artificial Neural Networks (ANN) algorithms to predict groundwater quality suitable for both agricultural and industrial purposes in California, US. The investigation involves the examination and forecasting of the Water Quality Index (WQI) employing ANN, Deep Neural Network (DNN), and the ML method of Extreme Gradient Boosting (XGBoost). The calculation of the WQI involved the utilisation of data spanning the temporal range from 1995 to 2023, encompassing ten parameters of utmost significance: total dissolved solids (TDS), sulphate, sodium, potassium, calcium, magnesium, nitrite, nitrate, chloride, and bicarbonate. Following a comprehensive assessment of model performance using metrics such as root mean square error (RMSE) and Nash-Sutcliffe Efficiency (NSE), the most optimal model was selected for predicting the Water Quality Index (WQI) in the region for the subsequent five years.
HS04-A005
Explaining the Mechanism of Multiscale Groundwater Drought Events: A New Perspective from Interpretable Deep Learning Model
Hejiang CAI1+, Haiyun SHI2#, Suning LIU2, Zhaoqiang ZHOU2, Vladan BABOVIC1
1National University of Singapore, 2Southern University of Science and Technology
This study presents a new approach to understand the causes of groundwater drought events with interpretable deep learning (DL) models. As prerequisites, accurate long short-term memory (LSTM) models for simulating groundwater are built for 16 regions representing three types of spatial scales in the southeastern United States, and standardized groundwater index (SGI) is applied to identify 539 groundwater drought events. Two interpretation methods, expected gradients (EG) and additive decomposition (AD), are adopted to decipher the machine-captured patterns and inner workings of LSTM networks. The EG results show that: 1) temperature-related features were the primary drivers of large-scale groundwater droughts, with their importance increasing as the drought event approached (54.2%~65.4%). Conversely, precipitation-related features were found to be the dominant factors in the formation of groundwater drought in small-scale catchments, with the overall importance of such features ranging from 55.9% to 58.6%; 2) the formation of small-scale groundwater droughts showed seasonal differences, with precipitation playing a dominant role as the drought event approached for winter groundwater droughts, while its importance decreased for summer groundwater droughts; and 3) both large-scale groundwater droughts and summer small-scale groundwater droughts exhibited a clear "trigger effect" from temperature-related factors. The AD method unveiled how the LSTM network behaved differently in retaining and discarding information when emulating different groundwater droughts. Overall, this study provides a new perspective for the causes of groundwater drought events and highlight the potential and prospect of interpretable DL in enhancing our understanding of hydrological processes.
HS04-A006
Learning Distributed Parameters of Land Surface Hydrologic Models Using a Generative Adversarial Network
Ruochen SUN#+, Qingyun DUAN
Hohai University
Calibrating distributed land surface hydrologic models presents a persistent challenge, often resulting in uneven spatial performance due to the oversimplification of complex spatiotemporal information contained in both observations and simulations. In this study, we propose a novel generative adversarial network-based Parameter Optimization (GAN-PO) method. By leveraging a deep neural network to discern model biases, we train a generative network to produce seamless parameter fields, minimizing distinctions between simulations and observations. Applied to the Variable Infiltration Capacity (VIC) model for simulating evapotranspiration (ET) over China's Huaihe river basin, GAN-PO demonstrates comparable performance to a state-of-the-art differentiable parameter learning (dPL) method in reducing model errors at the grid scale. GAN-PO and dPL both exhibit substantial enhancements in simulated ET compared to default parameters, surpassing the conventional calibration approach that integrates a global optimization algorithm and parameter regionalization technique. Notably, GAN-PO excels in preserving spatial consistency, outperforming alternative methods in spatial performance.
HS04-A013
Long-term Gridded Land Evapotranspiration Reconstruction Using Deep Forest with High Generalizability
Dashan WANG#+, Qiaomei FENG, Zhenzhong ZENG
Southern University of Science and Technology
Previous datasets have limitations in generalizing evapotranspiration (ET) across various land cover types due to the scarcity and spatial heterogeneity of observations, along with the incomplete understanding of underlying physical mechanisms as a deeper contributing factor. To fill in these gaps, here we developed a global Highly Generalized Land (HG-Land) ET dataset at 0.5° spatial resolution with monthly values covering the satellite era (1982–2018). Our approach leverages the power of a Deep Forest machine-learning algorithm, which ensures good generalizability and mitigates overfitting by minimizing hyper-parameterization. Model explanations are further provided to enhance model transparency and gain new insights into the ET process. Validation conducted at both the site and basin scales attests to the dataset’s satisfactory accuracy, with a pronounced emphasis on the Northern Hemisphere. Furthermore, we find that the primary driver of ET predictions varies across different climatic regions. Overall, the HG-Land ET, underpinned by the interpretability of the machine-learning model, emerges as a validated and generalized resource catering to scientific research and various applications.
HS04-A007
Integrating Five-stage Modeling and Machine Learning for Advanced Water Demand Forecasting: Towards Sustainable and Smart Water Resources Management
Yao WANG1+, Suning LIU1, Haiyun SHI1#, Ji CHEN2
1Southern University of Science and Technology, 2The University of Hong Kong
Facing the escalating global demand for water resources, efficient water demand forecasting has become increasingly vital. The progress in technology, especially in the realms of intelligent systems and data analytics, has revolutionized water resources management. By employing advanced predictive models such as machine learning and deep learning methods, researchers can better analyze and understand the complex patterns of water usage, thus enabling effective short-term and long-term planning. This study proposes an integration of the Five-Stage Water Demand Model with various machine learning models to predict water consumption, aiming to address the multifaceted complexities and dynamics of water demand patterns. According to the framework of the Five-Stage Water Demand Model, data is transformed into features the model can comprehend, such as economic indicators for each stage, population growth rates, and climate change indices. Appropriate machine learning algorithms are selected based on the characteristics of the data and the complexity of the problem, such as Random Forests and Convolutional Neural Networks. The models are trained using historical data and evaluated through cross-validation to assess their performance. A feedback mechanism is established to continuously monitor the discrepancy between the model's predictions and actual water demand. These models are designed to operate over various time scales, with a particular emphasis on medium and short-term forecasts at monthly and yearly intervals, to facilitate more flexible and efficient water management strategies. Additionally, the integration of machine learning models, incorporating socio-economic factors aids in a comprehensive understanding of water usage patterns. As the models are continuously optimized and trained on more refined data, the accuracy and reliability of the predictions are expected to improve further, pushing water resources management towards more intelligent, data-driven decision making. Facing the growing global challenges, this advances us towards a path of more adaptive, efficient, and sustainable water resources management practices.
HS04-A014
PSO-enhanced Graph Spiking Neural Networks Models for Universal Urban Flood Risk Assessment
Xuhong FANG+, Aifang CHEN, Jiaye LI#
Dongguan University of Technology
Urban flooding poses a growing severe threat to urban residents and their properties due to the acceleration of climate change and urbanization. Accurate and effective urban flood simulations are necessary to develop strategies for protecting communities and infrastructure. While physically based hydrodynamic models can accurately simulate urban floods, they are data and computational resources demanded. Meanwhile, artificial intelligent models driven by data are often not generalizable, as they are limited to specific urban areas. To address these limitations, we have pioneered the combination of Graph Convolutional and Spiking Neural Networks (Graph SNN) with Particle Swarm Optimization (PSO), to develop a novel urban flood risk assessment model. The model can efficiently analyze flood patterns with high inference speed and low energy consumption. The model employs a diverse dataset, which includes social media reports, global rainfall data, and Digital Elevation Models (DEM) from various cities. It represents urban areas as a fully interconnected graph, with edge weights determined by geographic proximity, elevation, and city affiliation. The model demonstrates strong performance and robustness optimized by PSO. When tested on a mixed-city dataset, the model achieved an 85% accuracy rate in predicting floods. This study demonstrates the potential of our PSO-enhanced Graph SNN model as a significant advancement in urban planning and disaster management. The results suggest that our PSO-enhanced Graph SNN model can be a sophisticated and applicable solution across diverse urban landscapes.
HS04-A016
Physical Mechanism-based Flood Routing Algorithm for Muskingum-recurrent Neural Networks
Zhaoxi LI+, Tiejian LI#, Jian SUN
Tsinghua University
River flood routing calculations are crucial for the effectiveness of flood forecasting and the scheduling of flood control measures. The Muskingum method, characterized by a robust physical mechanism, continues to undergo improvements and maintains widespread application in flood routing. In recent years, data-driven models such as machine learning and artificial intelligence have been widely used for flood forecasting. However, a notable limitation of these data-driven models is that their structures and parameters often lack an underlying physical basis, leading to challenges in interpretability. In this paper, we use Muskingum coefficient to define the internal weight parameters of the Recurrent Neural Network (RNN) and reconstruct the internal structure of RNN. This integration gives rise to the Muskingum-Recurrent Neural Network (MRNN) flood routing algorithm, which effectively combines the advantages of artificial intelligence with a physically-based mechanism for flood routing computation. Using hydrodynamic model, 8000 hydrographic data were generated in four channel with different characteristics, which were used for model training. The performance of MRNN with few parameters is comparable to that of traditional neural network model. In addition, MRNN is 3 orders of magnitude better than the traditional neural network model in mass conservation. The case study in Village Creek shows that the average pass rate of MRNN simulation results is 8.33% higher than that of other neural network models. With the training set reduced from 0.8 to 0.2, the NSE of MRNN only decreases by 3%, while that of ANN and LSTM decreases by 20% and 19% respectively. MRNN algorithm improves the efficiency of modeling, calibration and application, and can be directly applied to flood evolution prediction, providing model reference for constructing artificial intelligence water conservancy model. This study reveals that the neural network embedded with physical mechanism has great research potential in the field of hydrological research.
Session Chair(s): Ruochen SUN, Hohai University, Bellie SIVAKUMAR, Indian Institute of Technology Bombay
HS46-A005
A Method to Get Rainfall Intensity from Video
Zhixu BAI1#+, Nan YE2, Penghui CAI1
1Wenzhou University, 2Shanghai Institute of Technology
This research designs and validates a rainfall intensity video monitoring method (Video to Rainfall Intensity method, V2RI method) for monitoring urban rainfall in real-time and improving the use of video data collected by urban cameras at a low cost. The method extracts the rainfall velocity and drop diameters by analyzing the rainfall video. It uses the rainfall velocity-diameter relationship and the rainfall intensity-rainfall spectrum feature relationship for the inversion of rainfall intensity. The validation results based on Wenzhou city show that the method can be applied to daytime rainfall videos taken by civilian cameras, and can provide effective rainfall intensity monitoring for rainfall processes with moderate rainfall intensity and above, with an average error of ~10% in the accumulated rainfall for multiple rainfall events. The Monte-Carlo-based stability validation shows that the V2RI method has a certain degree of stability. The V2RI method is a potential data provider for the short-term forecast of mountain flash floods.
HS46-A006
Tropical Cyclone Risk Analysis Over Time Utilizing Multi-hazard Hurricane Index in the Southeastern United States
Jae Yeol SONG1+, Eun Sung CHUNG2#
1National Korea Maritime and Ocean University, 2Seoul National University of Science and Technology
The Southeast United States faces numerous threats from tropical cyclones due to the hazardous combination of strong wind-speed and heavy rainfall. These factors pose risks to coastal communities by causing storm surge and coastal flooding. In this study, we analyze the evolving tropical cyclone risks over the period of 1979-2022, taking into account the likelihood of coinciding wind and rainfall hazards with various combinations of social vulnerability factors associated tropical cyclones within the threatened area. NLDAS-2 and HURDAT2 are mainly used to obtain rainfall and wind-speed data from tropical cyclones and social vulnerability index are used to estimate the vulnerability of the impacted region. This study incorporates the increasing dataset and historical records over time, and evaluates the performance of the proposed approach between considering only wind-speed and both wind-speed and rainfall as the hazard component over time. Our findings show that the hazards from tropical cyclones based on the multi-hazard hurricane index were favorable until 2017 while wind based risks are becoming increasingly dominant in recent years. Our finding indicates that coastal communities are expected to be more vulnerable to tropical cyclone hazards related to wind, including heavy winds, storm surges, and coastal flooding, as opposed to risks associated with rainfall.
HS46-A002
Characteristics of Terrace Destruction in Typical Watersheds on the Loess Plateau Under Heavy Rainfall
Pengfei DU#+
China Institute of Water Resources and Hydropower Research
Compared with general rainfall, the damage to soil and water conservation measures in the Loess Plateau caused by heavy rainfall is more serious. Taking a rainstorm in July 2003 on the Loess Plateau as an example, the destruction of terraced fields in a typical watersheds caused by the heavy rain was investigated by a combination of field measurements and aerial photographs taken by an unmanned aerial vehicle (UAV). According to the morphology of the longitudinal section after the destruction of the terrace, the damaged terrace were summarized into five types: Ellipsoidal, Cylindrical, Conical, Stepped and Combined. Among the 95 terraces in the watershed, a total of 36 terraces were damaged, with a total of 126 erosion points, and the type of erosion was dominated by ellipsoidal type. The spatial location of the terraces where soil erosion disasters occurred was mainly concentrated in the middle slope and downslope position, and the gully-slope junction was the most prone to be eroded in the gully-slope system, with an average erosion intensity of about 8000 t/km2. The construction of drainage ditches can effectively reduce the damage of terraces by heavy rainfall, which is an important measure for the future management of sloping arable land in the Loess Plateau.
HS46-A007
Developing a Standardized Water Demand Indicator to Identify Water Stress and Prioritize Areas for Irrigation in India
Sneha KULKARNI1#+, Vinayak BHANAGE2
1The University of Tokyo, 2Hiroshima University
In various regions of India, crops often face the dual challenge of protecting against excessive water damage while requiring timely irrigation. As a result, many parts of India demand well-established irrigation systems to maximize crop cultivation and facilitate agricultural activities. To address this, we developed a novel Standardized Water Demand Indicator (SWDI) that evaluates spatial-temporal water-vegetation stress and pinpoints the sensitive regions needing a robust irrigation network. The association of Evapotranspiration (ET) and Potential ET (PET) provides a crop water demand. Hence, we used ET data from MODIS and correlated it with the Normalized Difference Vegetation Index (NDVI) to identify regions with irrigation requirements through the SWDI. Crop coefficient values for major crops in different areas and monthly precipitation data obtained from CHIRPS were also considered to prioritize regions based on irrigation needs. From 2001 to 2023, our study observed a significant correlation between ET and NDVI across most of India, highlighting regions such as northern Karnataka, eastern Maharashtra, and western Rajasthan with the highest demands for irrigation. The years 2002, 2008-2009, and 2014-2015 were identified as highly water-stressed periods across most parts of the country. The proven association between ET and NDVI through this study, coupled with the effectiveness of SWDI in identifying water stress areas, establishes a robust foundation for decision-makers or management practices to focus on areas requiring special attention.
HS46-A001
Analysis of Spatio-temporal Propagation Characteristics of Drought Based on Complex Network in South Korea
Hyeonbin AHN+, Kyunghun KIM, Seungmin LEE, Soojun KIM, Hung Soo KIM#
Inha University
Drought is caused by the interaction of water supply and demand, which is influenced by natural phenomena such as precipitation and human-induced factors, and has significant negative impacts on various aspects including the economy, environment, society and so on. Understanding the spatio-temporal characteristics of drought is a key element for water resource planning and management, disaster mitigation, and social resilience to climate variability. However, due to its complexity, quantifying the spatio-temporal characteristics of drought still remains a significant challenge. Complex network analysis has shown strong aspects in modeling complex interactions or patterns, and has been applied in hydrology to study spatial connections between hydrologic elements. Therefore, purpose of this study is to analyze the spatio-temporal characteristics of drought using the complex network analysis. We used the Standard Precipitation Index (SPI) to construct the drought network and applied the Event Synchronization (ES) method to estimate the links representing the drought connection between different areas. The results of the centrality and clustering analysis showed the main propagation areas and characteristics of the drought throughout South Korea. The results of the study can be used as a reference to develop an early warning detection system for droughts. Acknowledgements: This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Water Management Program for Drought Project, funded by Korea Ministry of Environment(MOE).(2022003610002).
HS46-A011
Hierarchical Bayes Approach: Transferring the Parameter Uncertainties from Multiple Stations to Regional Models and Ungauged Stations
Xia WU1#+, Qingyun DUAN2
1Taiyuan University of Technology, 2Hohai University
Total suspended solids (TSS) are commonly used as an indicator of water clarity to assess the degradation of water quality due to their harmful effects on aquatic ecosystems. However, measuring the concentration of TSS directly is a time-consuming lab analysis process. To address this issue, a turbidity-TSS model is widely used to approximate TSS levels. According to a study by the USGS, a linear regression model in log10 space is typically chosen as a surrogate model, which requires calibration of the slope and intercept using instantaneous TSS and turbidity data. The estimated parameters demonstrate instability when influenced by limited and fluctuating data. To enhance parameter stability during calibration, the integration of measurements collected from various sampling stations can offer more comprehensive insights. Consequently, a hierarchical Bayes approach has been introduced to pool information from multiple sampling stations for estimating and regionalizing parameters. The findings from both synthetic and real cases demonstrate that this methodology is capable of achieving the following benefits: 1) Effectively reducing parameter uncertainties for each individual station by identifying the regional distribution of parameters. 2) Reliably quantifying the uncertainties associated with regional parameters through integrating the posterior distributions from individual stations. 3) Transferring the parametric distribution to ungauged stations, thereby providing a solution for Predictions in Ungauged Basins (PUB).
Session Chair(s): Haiyun SHI, Southern University of Science and Technology, Suning LIU, Southern University of Science and Technology
HS04-A004
| Invited
On the Transferability of Regional LSTM Models: The Role of Training Data Homogeneity
Liguang JIANG1#+, Qiang YU2
1Southern University of Science and Technology, 2The Hong Kong Polytechnic University
The effectiveness of homogeneous versus heterogeneous training data for regional LSTM models has been a subject of debate. Some argue that regional LSTM models can benefit from heterogeneous training data, while others contend that training with homogeneous data is more effective. However, few studies have quantitatively evaluated the impact of training data homogeneity on the performance of regional LSTM models in the context of prediction in ungauged basins (PUB). This study hypothesizes that data homogeneity is a crucial factor in training regional LSTM models and leveraging such homogeneity can enhance model transferability. Here, the term "model transferability" is used to describe the model performance in PUB. To test this hypothesis, the transferability of regional LSTM models was evaluated through two different training strategies. The results show that the median NSE value of the C-LSTM model trained using the homogeneity-based strategy is 0.616 across 363 catchments, as opposed to 0.611 and 0.568 of the B-LSTM-NA and B-LSTM-WA models trained by the traditional strategy, i.e., using all available catchments with and without catchment attributes as additional model input. The enhancement in transferability of both C-LSTM and B-LSTM-WA models is primarily reflected in the simulation of low flows although C-LSTM is much better. However, the computational cost of the B-LSTM-WA model is higher. This study contributes to a better understanding of the role of training data homogeneity in model transferability and also provides an effective strategy for the practical training of the regional LSTM models.
HS04-A027
Gridded Runoff Projection Using Machine Learning Model in the Part Basins of Tibetan Plateau Under Climate Change
Haibo CHU#+, Zhuoqi WANG, Yulin JIANG
Beijing University of Technology
Gridded runoff projection can fully demonstrate the spatial variation of runoff and enable the capability of fine-scale forecasting. In this study, the runoff of the part basins of the Tibetan Plateau (TP) at a grid resolution of 0.25° was projected using a machine learning model coupling CMIP6 future climate scenarios. A typical machine learning model, long short-term memory (LSTM), was employed to reflect the response relationship of the hydrometeorological and underlying surface feature variables with runoff at each grid. Changes in the distribution of parameters in different LSTM models were analyzed to explore the mechanism of the runoff generation process for more accurate runoff projection. The source region of the Yellow River (YRSR) was selected as a case study, and future precipitation, temperature, and other hydrometeorological variables of four SSP climate scenarios are used as the inputs of well-calibrated LSTM models for the period from 2024–2099. The projected results showed that future runoff in the YRSR has an increasing trend, and the spatiotemporal changes are not significant. Through effective water resource management plans, these findings about the projected increase in runoff will assist in developing proactive adaptation strategies.
HS04-A019
An Approach of Using Social Media Data to Detect the Real Time Spatio-temporal Variations of Urban Waterlogging
Maochuan HU#+, Yilin CHEN, Xiaohong CHEN, Bingjun LIU
Sun Yat-sen University
Urban waterlogging has occurred frequently in recent years due to the impact of climate change and human activities. Real-time waterlogging information is crucial for disaster emergency management, but how to quickly obtain such information remains challenging. Social media data has been widely used to derive damage information because of its high real-time response, low acquisition cost, and high content integration. In this study, we propose an approach to extract real-time waterlogging points from social media data (Sina Weibo). First, social media data is obtained through web crawler technology; Then, de-duplication and de-noising methods are used to filter the data; Finally, a waterlogging point extraction method based on deep learning BERT-BiLSTMCRF model is proposed to extract waterlogging points. Taking the “7.20” rainstorm in Zhengzhou as an example, there was a rapid increase in the number of social media data during urban waterlogging. Social media data is highly sensitive to urban waterlogging disasters caused by extreme rainstorms. On the day with the heaviest rainfall (July 20), the number of Weibo waterlogging points (331) in the central city was 267 more than the official waterlogging points (64). There were many more Weibo-derived waterlogging points than the real-time official published waterlogging points. The waterlogging points obtained by this approach covered the official published real-time waterlogging points accounted for no less than 82% and they were mostly located around roads, especially in low-lying areas. In general, we demonstrate the feasibility and accuracy of social media data on rapid detection of real-time spatiotemporal variations of waterlogging caused by extreme rainstorms. Urban waterlogging disaster information extracted from social media data can rapidly reflect the real-time spatiotemporal variations of urban waterlogging disasters, can effectively cover and supplement data reported by government agencies, and can provide data support for urban waterlogging disaster prevention.
HS04-A020
Transferring Groundwater Knowledge Between the Contiguous US and Denmark
Yueling MA1#+, Julian KOCH2, Reed MAXWELL1
1Princeton University, 2Geological Survey of Denmark and Greenland
Groundwater is our largest freshwater reservoir, playing an important role in the global hydrologic cycle. Due to the scarcity of groundwater observations (e.g., water table depth, WTD), especially in developing countries, our knowledge of global groundwater systems is still limited. To address this challenge, many physically-based groundwater models have been developed to provide global WTD maps with spatial resolutions ranging from ~ 900 m to ~ 9 km. The simulated WTD maps were yet found to have large discrepancies from well observations. In addition, higher resolution WTD estimates are required at the city or individual farm level, where local decisions are often made. This is challenging for physically-based models, because of the dramatic increase in computational costs. Recently, we introduced a novel hyper-resolution (1 arcsec, ~ 30m) WTD product for the Contiguous US (CONUS) including groundwater pumping and uncertainty. The WTD product was produced by a random forest model trained on available WTD observations. Since the CONUS covers many different hydrogeological settings, the trained random forest model may be transferrable to other regions with a similar setting and limited observations. To test this hypothesis, we conduct a study on transferring groundwater knowledge between the CONUS and Denmark. We find that climate classification might be a missing input variable in the original random forest model, which significantly affects the model performance across regions. The joint model trained on data from the CONUS and Denmark outperforms the individual models trained separately on data from the CONUS and Denmark. This study provides additional insights into global groundwater hydrology and improves our confidence in producing a hyper-resolution global WTD map.
HS04-A025
Application of Deep Learning in Forecasting Water Quality Information in the Water System, A Case Study in Lai Chi Wo Catchment, Hong Kong
Yi LU1,2#+, Hongyi YAO2, Jieying MA3, Ji CHEN2, Zhaofeng HAN2, Hongxu ZHU2, Shi Jie WU3, Zherui XIAO3
1Hong Kong Metropolitan University, 2The University of Hong Kong, 3Hong Kong Chu Hai College
Rainfall in mountainous catchment areas often leads to a decline in river water quality due to an increase in suspended sediment from river banks and the river bed. This excess sediment can significantly impact drinking water usage and aquatic life. This study aims to enhance water quality management in the watershed by employing various deep learning (DL) algorithms to establish a predictive model for water quality, specifically focusing on turbidity and suspended solids concentration. The study utilizes a monitored dataset of water quality and hydrological parameters from the Lai Chi Wo (LCW) catchment in Hong Kong. As part of our exploration into the application of DL methods in hydrology, we will develop several types of artificial neural networks with varying structures, tailored to the characteristics of the data in this study. The predictive results will be analyzed and compared using different indices to inform the warning system. This study is committed to introducing innovative technologies and modern methodologies for the establishment of an intelligent water-safety-early-warning platform. Our goal is to mitigate the impact of human activities and natural disasters on environmental sustainability.
HS04-A017
Application of Distributed Runoff Model Vegetative Roughness Routine Using Remote Sensed Vegetation Data
Andre ARAUJO FORTES1#+, Masakazu HASHIMOTO2, Keiko UDO1
1Tohoku University, 2Kansai University
Riparian vegetation can impact the conveyance capacity of river channels, leading to an increased probability of floods and inundations. The common practice for considering vegetation in hydraulic models is the adoption of a higher static Manning coefficient when compared to unvegetated areas, but this does not accurately comprehend the vegetation and flow interactions. The adoption of a dynamic Manning setting that changes the coefficient value according to the flow conditions would bring more precise results. Vegetation parameters such as height and the leaf area index (LAI), a good descriptor of plant density, are key parameters for determining vegetative roughness, but such parameters are difficult to survey. With advances in remote sensing and machine learning techniques, surveying vegetation conditions in large areas has become possible. The research objective is to evaluate the applicability of satellite and machine learning derived vegetation parameters in a dynamic vegetative roughness routine in a distributed runoff model. The vegetation indices (VI) from satellite data with sparse resolution were related to the desired parameters and machine learning was used to obtain these relationships. With trained models, VIs from Sentinel-2 were used to map the parameters in the catchment scale. To consider the vegetation, the rainfall-runoff inundation (RRI) model was patched with a time-step roughness routine that worked under emergent and submerged vegetation scenarios. The combination of satellite imagery and machine learning could map the vegetation parameters. Mapping LAI with fine resolution was an easier task than the vegetation height. The lack of vertical data from optical imagery led to a confidence limitation in the height mapping. The application of the vegetation in the RRI model led to an increase in the water depth when compared to the adoption of a static value. In addition, a prolongation in the flood period resulted from considering the vegetation.
Session Chair(s): C.G. CUI, China Meteorological Administration
HS07-A003
The Research on Hydro-meteorology Coupling Method in Basin Flood Warning and Forecasting
C.G. CUI#+, Tao PENG, Zhiyuan YIN, Tieyuan SHEN
China Meteorological Administration
Flood disasters pose significant threats to life and property. The advancement of modern meteorological service technologies offers promising avenues for enhancing flood forecasting. This study emphasizes the integration of QPE/QPF to augment the accuracy of flood predictions through the Hydro-meteorology Coupling Method in Basin Flood Warning and Forecasting. Key findings include: Utilizing historical hydro-meteorological data and the Xin'AnJiang hydrological model for flood forecasting experiments revealed that both the qualification rate and efficiency coefficients meet hydrological forecasting standards. The calibrated parameters of this model are validated for hydrological predictions. Experiments with Radar Quantitative Precipitation Estimation (QPE) for flood forecasting indicated that uncalibrated radar QPE inputs into the hydrological model yielded suboptimal results. However, calibrated radar QPE inputs enhanced forecasting precision. Three evaluation metrics - the average certainty factor, flood forecast qualification rate, and peak occurrence time deviation (less than 3 hours) - all suggest superior flood simulation when utilizing calibrated radar rainfall data. Quantitative Precipitation Forecast (QPF) experiments highlighted that considering predicted rainfall improves flood forecasts, especially during heavy rainfall events. As rainfall concludes, its subsequent forecasts have diminished impact on flood predictions. Incorporating ensemble precipitation forecast products into flood predictions demonstrated that these products furnish more comprehensive rainfall input information for hydrological models. This not only provides a range for peak flow and its arrival time but also shifts from deterministic predictions to probabilistic forecasts, addressing the accuracy limitations of singular deterministic predictions.
HS07-A016
Spatio-temporal Characteristics of Precipitation Concentration and Their Linkage to Temperature Over China
Zequn LIN1+, Dagang WANG1#, Yi DU2, Yue MENG3
1Sun Yat-sen University, 2Anqing Normal University, 3Central University of Finance and Economics
Precipitation concentration represents the temporal unevenness of precipitation over a given period. A higher concentration increases the likelihood of concurrent flooding and drought. While most previous studies have focused on daily-scale precipitation concentration, investigations into its characteristics at sub-daily scales have been scarce. Furthermore, the influence of temperature on precipitation concentration across various temporal scales remains unclear. In this study, utilizing high-resolution precipitation products and the Gini index, we analyze the spatio-temporal characteristics of precipitation concentration across four different time scales (3-hour, 6-hour, 12-hour and 1-day) in China. The climatological analysis reveals a gradual increase in precipitation concentration from southeast to northwest China. The concentration at shorter temporal scales (3-hour and 6-hour) exhibit a notable increase across most parts of Southeastern China, while longer scales (12-hour and 1-day) show a significant decrease throughout most regions of Northwest China. These observed spatio-temporal patterns are closely linked to temperature variations. Higher temperatures intensify precipitation concentration at the 3-hour scale in Southeastern China by elevating the frequency of heavy precipitation events. Conversely, in Northwest China, the decline in concentration at the daily scale under warmer conditions is attributed to increased annual precipitation amounts driven by higher temperatures. This study holds great significance, as it indicates the future changes in the temporal distribution of precipitation over China under global warming.
HS07-A004
The Diabatic Feedback to Mei‑yu Fronts
Yang HU#+
China Meteorological Administration
Mei-yu fronts are often accompanied with evident diabatic heating due to the frontal cloud development. Here a new frontogenesis function is derived to isolate the effect of diabatic heating and reveal the dynamic and thermodynamic processes driving the evolutions of three typical Mei-yu fronts. It is found that the direct effect of latent heating (moisture depletion) is always frontogenetical (frontolytical) in the pre-frontal and frontal zone throughout the lifecycle of the front with latent heating (moisture depletion) in general dominates the front intensification (dissipation). Tilting is another critical process that turns the vertical gradient of equivalent potential temperature into horizontal gradient leading to frontogenesis during the front development stage, and, after the release of convective instability ahead of the front, flattens the front surface leading to frontolysis during the front decaying stage. In addition to this direct effect on Mei-yu fronts, diabatic heating also influences frontogenesis indirectly by changing local atmospheric circulation. To quantify such indirect effects, piecewise potential vorticity (PV) inversion is adopted to decompose the process of deformation frontogenesis into several parts associated with distinct PV anomalies. The balanced flow associated with the interior-level diabatic PV anomaly and the synoptic environment emerges as the most important contributor to the total deformation frontogenesis. However, the indirect effect of diabatic heating on Mei-yu frontogenesis is generally weaker in magnitude compared to the direct effect of temperature modification as well as the impact of moisture depletion. The results presented here add evidences about the importance of cloud feedback to the evolution of Mei-yu fronts and suggest the necessity of improved model representations of cloud processes in achieving a better simulation and prediction of Mei-yu rainfall.
HS07-A019
Evaluation of MODIS, ERA5 and MERRA2 Derived Integrated Precipitable Water Vapor Over India Using Ground-based GPS Data
Seema RANI#+, Jyotsna SINGH
Banaras Hindu University
Water vapor, a crucial yet variable element across time and space, holds significant importance in climate studies due to its fluctuating nature. However, in India, conventional methods like radiosonde for ground observations of water vapor are limited. With the advancement of technology, multi-sensor satellites and reanalysis datasets have come into play. Thus, this study presents a comparative analysis between daily estimates of total column water vapor derived from the Global Positioning System (GPS) and multi-sensor satellite (both infrared and near-infrared: MODIS IR and MODIS NIR)/reanalysis (ERA5 and MERRA2) data across nineteen stations for the period March 2013 to February 2014. The study also estimates seasonal and annual trends in water vapor over India during 2003-2022. The findings demonstrate a quantitative depiction of the daily variations in mean bias (b), root mean square error (RMSE), correlation coefficient (R), and Nash-Sutcliffe efficiency (NSE) among the different water vapor datasets. ERA5 shows a better agreement with GPS data across most of the stations (b = -4.83 to -2.13 mm, RMSE = 1.57 to 3.53 mm, R = 0.97 to 1, NSE = 0.88 to 0.99) as compared to other datasets. Among the MODIS water vapor products, the MODIS NIR clear column product exhibits a more robust correlation (R = 0.77 to 0.99) and a lower mean absolute bias (9.88 mm) with GPS data across the majority of stations when compared to the IR product (R = 0.85 to 0.97, absolute bias = 11.10 mm). Additionally, the trend result suggests increasing column water vapor in all the seasons. The highest increasing trend in water vapor is observed in post monsoon (2.23 mm/decade) followed by winter (1.84 mm/decade). The annual water vapor of the study area is increasing at the rate of 1.14 mm/decade. However, future studies may evaluate the dataset using long-term data horizontally and vertically.
HS07-A002
Post-processing Ensemble Precipitation Forecasts and Their Applications in Summer Streamflow Prediction Over a Mountain River Basin
Yiheng XIANG#+, Tao PENG
China Meteorological Administration
Ensemble precipitation forecasts (EPFs) can help to extend lead time and provide reliable probabilistic forecasts, which have been widely applied for streamflow predictions by driving hydrological models. Nonetheless, inherent biases and under-dispersion in EPFs require post-processing for accurate application. It's imperative to explore the skillful lead time of post-processed EPFs for summer streamflow predictions, particularly in mountainous regions. In this study, four popular EPFs, i.e. CMA, ECMWF, JMA, and NCEP were post-processed by two state of art methods, i.e. the Bayesian Model Averaging (BMA) and Generator-based Post-Processing (GPP) methods. These refined forecasts were subsequently integrated with the Xin’anjiang (XAJ) model for summer streamflow prediction. Performances of precipitation forecasts and streamflow predictions were comprehensively evaluated before and after post-processing. The results reveal that raw EPFs frequently deviate from ensemble mean forecasts, particularly underestimating torrential rain. There are also clear underestimations of uncertainty in their probabilistic forecasts. Among the four EPFs, ECMWF outperforms its peers, delivering skillful precipitation forecasts for 1-7 lead days and streamflow predictions for 1-4 lead days. The effectiveness of post-processing methods varies, yet both GPP and BMA address the under-dispersion of EPFs effectively. The GPP method, recommended as the superior method, can well improve both deterministic and probabilistic forecasting accuracy. Moreover, the ECMWF post-processed by GPP extends the effective lead time to 7 days and reduces the underestimation of peak flows. The findings of this study emphasizes the potential benefits of adeptly post-processed EPFs, providing a reference for the streamflow prediction over mountain river basins.
Session Chair(s): Salvatore GRIMALDI, University of Tuscia
HS40-A001
| Invited
Advancing Hydrological Design Simulation: Continuous Modeling for Small and Ungauged Basins
Salvatore GRIMALDI1#+, Francesco CAPPELLI1, Andrea PETROSELLI1, Ciro APOLLONIO1, Elena VOLPI2, Aldo FIORI2
1University of Tuscia, 2Roma Tre University
The potential advantages of continuous modeling in hydrological studies are widely acknowledged, particularly in the estimation of design hydrological input for practical applications. Continuous modeling offers the benefit of generating a diverse set of synthetic scenarios, serving as effective input for statistical analyses related to risk and hazard. Additionally, it enhances the accuracy of reproducing design flood volumes. Consequently, there is a discernible shift away from the conventional concept of designing hydrographs in favor of simulating design runoff. Recent emphasis has been placed on extending the application of continuous modeling to the complex context of small and ungauged basins. Utilizing a straightforward rainfall-runoff model structure that is inherently calibration-free, significant enhancements can be achieved in comparison to traditional techniques applied in such critical watersheds, such as the rational method. However, the broader adoption of this approach faces challenges, primarily due to the requirement of a simulated rainfall time series as input. Although generating simulated rainfall time series is considered feasible today, two main challenges persist: (i) the availability of numerous rainfall models without clear guidance on selecting the most appropriate one, and (ii) the non-user-friendly nature of many rainfall models, demanding a substantial theoretical background for successful application. This contribution delves into an investigation of these challenges.
HS40-A004
Strengthening East Asian Impact of HELPING Through Potential Collaborations with Local Community
Xudong ZHOU1#+, Luwen WAN2, Jingyu LIN3, Manqing SHAO4, Sifang FENG5, Beichen ZHANG6, Yuanhao XU7, Yuxin LI8, Yuan LIU9, Ming LIU10, Libo WANG5, Xinyan TAN11, Yajing CHEN5
1Ningbo University, 2Stanford University, 3Guangdong University of Technology, 4Texas A&M University, 5Beijing Normal University, 6University of Nebraska-Lincoln, 7Sun Yat-sen University, 8The University of Hong Kong, 9China Institute of Water Resources and Hydropower Research, 10South China University of Technology, 11Tsinghua University
The HELPING initiative faces challenges in achieving its initial goals, particularly in engaging a sufficient number of Asian early-career scientists and maintaining consistent media visibility through its ongoing activities. The lack of diverse participation from various relevant sectors hinders the initiative's ability to extend its impact beyond the confines of academic research. Inviting contributions from local communities could be a strategic solution to this problem. Hydro90 is a grassroots scientific community within the fields of hydrology and earth sciences. It actively disseminates the latest academic research, broadcasts news, and organizes a variety of educational events, such as lectures, webinars, and workshops. Its primary objective is to enhance communication among scholars and between scholars and the public, with a special focus on engaging younger audiences. With over 33,000 subscribers across multiple social media platforms, Hydro90 has established itself as an influential forum for sharing new knowledge and connecting individuals globally with similar interests. Hydro90 shares similar objectives with HELPING, but its reach is primarily limited to Chinese audiences. Collaboration and professional guidance from HELPING could enable Hydro90 to expand its scope and effectiveness. Organizing joint events could also bolster HELPING's recognition in East Asia and among Chinese-speaking communities.
HS40-A002
Climate Adaptation Strategies to Stabilize the Durum Wheat Productivity in Mediterranean Areas
Elena CRISTIANO1#, Malin GROSSE-HEILMANN1, Maria Cristina RULLI2, Roberto DEIDDA1, Francesco VIOLA1+
1University of Cagliari, 2Politecnico di Milano
Durum wheat is one of the most relevant crops, that ensures food security in Mediterranean areas. In these regions, durum wheat is a rainfed crop, that barely relies on additional irrigation to ensure high productivity. However, in a context of climate changes, the decrease of mean annual precipitation and of rainfall event frequency can negatively affect the durum wheat production. Moreover, the role of the CO2 and temperature increase on the durum wheat yield is still not clear and contrasting results have been found in the literature. To ensure a stable production, different adaptation strategies need to be investigated and implemented. Within the framework of the H2020 European Union project ARSINOE (“Climate-resilient regions through systemic solutions and innovations”), the potential climate change impacts on the durum wheat production in the Campidano region in Sardinia (Italy) have been evaluated, with the aim to identify local solutions that can be transferred and upscaled to the entire Mediterranean region. The analysis was developed using a calibrated Aquacrop model to simulate yield production under current and possible future climatic scenario and to estimate the additional irrigation required to ensure a stable productivity. In parallel, a series of Living Labs actively engaged multiple stakeholders (from farmers to producers, to public entities and decision makers) with the aim to identify problems and potential strategies to reach the common goals. Besides underlying the importance of stakeholder involvement, results show that emergency irrigation should be considered to maintain the actual durum wheat production in a context of climate changes and suggest that the use of unconventional water resources, such as rainwater harvesting, to ensure water availability and, at the same time, to reduce the pressure on the water supply system.
HS40-A006
Soil and Water Conservation Benefits Under General and Extreme Rainfall Conditions
Ying ZHAO1#+, Yin CHEN1, Qi YANG1, Duihu NING2
1China Institute of Water Resources and Hydropower Research, 2International Research and Training Center on Erosion and Sedimentation
The global climate change could lead to an intensified water cycle, and further increase the intensity and frequency of extreme rainfall events. Soil erosion induced by these extreme events could be several times than erosion induced by the general rainfall. Soil and water conservation practices are an effective way to prevent soil erosion. However, as extreme events become more frequent under global climate change, the runoff and sediment reduction effect might change since the extreme rainfall damages those practices. This research took Qiaozigou Watershed in the Loess Plateau in China as an example and analyzed the soil and water conservation benefits under general erosive rainfall and extreme rainfall. Daily rainfall data was collected from four rain gages inside the watershed from 1988-2021. Runoff and sediment yield were collected at the outlets of the two sub-watersheds from 1988-2004. It is found that the annual rainfall and annual erosive rainfall both showed a nonsignificant increase in the Qiaozigou watershed during the study period. The frequency of extreme rainfall increased from 1.23 station days in the last century to 1.82 station days in this century, with an increase of 48%. As for runoff and sediment reduction, the results indicated that after soil and water conservation practices, there is a delay in the timing of flow and sediment production under extreme rainfall. The east sub-watershed with both channel and slope treatments showed a better runoff and sediment reduction effect than the west sub-watershed with only slope treatments. For both watersheds, the runoff and sediment discharge reduction rates were greater than 70% under general erosive rainfall, but the reduction rates were less than 40% under extreme rainfall.
HS40-A005
Estimation of the Drawdown Time for the Design of Infiltration Basins
Aldo FIORI1#+, Marco FERRANTE2
1Roma Tre University, 2University of Perugia
Infiltration basins are often adopted for the managed aquifer recharge. The design, assessment and management of infiltration basins depends on the drawdown time, i.e. the time that is needed to completely empty the basin after it has been filled with water, for instance, after a flood event or by a managed discharge. The drawdown time depends on the hydraulic conductivity of the soil and its heterogeneous features. We propose a set of analytical solutions for the drawdown time in presence of heterogeneous soils, that can be helpful in the design and verification of such structures. The solutions are tested through Monte Carlo simulations in various realistic scenarios, using a modified Green Ampt model for layered soils and a model based on the integration of the Richards equation. Funding from Project “Ecosistema dell'innovazione—Rome Technopole” financed by EU-Next-GenerationEU, CUP:F83B22000040006 is acknowledged.
Session Chair(s): Jingyu WANG, Nanyang Technological University
HS07-A008
Asymmetric Seasonal Rainfall as a Sufficient Water Resource for a Reservoir Watershed in East Asia
Shih-Ming HUANG#+, Chuan-Yao LIN, Yi-Ying LIN
Academia Sinica
The East Asian monsoon rainfall is very important and serves as the sufficient water resource for reservoir watersheds in East Asia. Among them, the Feitsui Reservoir (FR) is the main source of water supply in northern Taiwan (NTW), especially for Taipei City. As a result of global-warming, Taiwan has experienced major droughts, resulting in insufficient water being stored in reservoirs, except in the FR. In this study, we discovered that precipitation from tropical cyclones (TCs; 29.97% of annual rainfall) wasn’t the dominant source of water in the Feitsui Reservoir Watershed (FRW); instead, the northeasterly monsoon (NEM) resulted in heavy rainfall in the eastern part of FRW in autumn–winter (33.65%). Our results indicated that the water resources of FRW were contributed by non-TC rainfall (70%). Therefore, the FR serves as a sufficient water resource, even during periods of severe drought. Because of the interaction between the northeasterly (southwesterly) monsoon and topography, the asymmetric rainfall boundary crossed the center of FRW, which concentrated the rain that fell in autumn–winter (mei-yu and summer) in the eastern (western) part of FRW and NTW regions. Our findings explain the seasonal rainfall characteristics and spatial-distributions in the FRW and establish a basis for investigating long-term rainfall variation in the FRW and improving hydrographic prediction under global-warming conditions, these can be extend to other reservoir watershed studies in East Asia.
HS07-A020
Sustainable Water Resources Management Using WRF-Hydro Hydrological Model Over the Amu River Basin, Afghanistan
Wahidullah HUSSAINZADA+, Han Soo LEE#
Hiroshima University
In the past century the water demand increased extensively due to rapid increase in the earth population. In response to the water scarcity issues a proper understanding of the water resources and its availability is crucial. Ground observation could reveal hydrological dynamics, but it is costly and time consuming. Hydrological models are good alternatives. In this study Weather Research and Forecast model hydrological enhancement (WRF-Hydro) was utilized to simulate the streamflow over mountainous basin in the northeast of Afghanistan with complex hydrology name Amu River Basin (ARB). Model was set up on daily time scale with spatial resolution of 3km and routing data of 250m. Global Land Data Assimilation System (GLDAS) were used as the forcing metrological input. The study period between 2010 to 2019 were divided into spin-up (2010-2013), calibration (2014-2016), and validation (2017-2019). The calibration process focused the three main processes (1) land surface model (LSM), (2) groundwater parameters, and (3) other hydrological parameters. Five station discharge observations were used to assess the model accuracy after careful quality controlling and elimination of the errors. Correlation coefficient (R), coefficient of determination (R2), Nash-Sutcliff efficiency (NSE), and Kling-Gupta efficiency (KGE) were adopted for the model accuracy assessment. Overall performance of the model over three rivers in the ARB are reasonably acceptable with R (0.85 to 0.42), R2 (0.73 to 0.17), NSE (0.52 to -8.64), and KGE (0.74 to -0.56). This study is the pioneer attempt on the simulation of the streamflow over ARB and could be useful source of data for the decision makers and scholars focusing on the environmental and water issue in the Central Asia as well as the water management authorities in Afghanistan.
HS07-A006
Analysis of the Characteristics of the Low-level Jets and Its Relationship Between Precipitation During the Mei-yu Season
Wen ZHOU#+, C.G. CUI
China Meteorological Administration
Here, we analyze the characteristics and the formation mechanisms of low-level jets (LLJs) in the middle reaches of the Yangtze River during the 2010 Mei-yu season using Wuhan station radiosonde data and the fifth generation of the European Centre for Medium-Range Weather Forecasts (ERA5) reanalysis dataset. Our results show that the vertical structure of LLJs is characterized by a predominance of boundary layer jets (BLJs) concentrated at heights of 900–1200 m. The BLJs occur most frequently at 2300 LST but are strongest at 0200 LST, with composite wind velocities >14 m s–1. Synoptic-system-related LLJs (SLLJs) occur most frequently at 0800 LST but are strongest at 1100 LST, with composite wind velocities >12 m s−1. Both BLJs and SLLJs are characterized by a southwesterly wind direction, although the wind direction of SLLJs is more westerly, and northeasterly SLLJs occur more frequently than northeasterly BLJs. When Wuhan is south of the Mei-yu front, the westward extension of the northwest Pacific subtropical high intensifies, and the low-pressure system in the eastern Tibetan Plateau strengthens, favoring the formation of LLJs, which are closely related to precipitation. The wind speeds on rainstorm days are greater than those on LLJ days. Our analysis of four typical heavy precipitation events shows the presence of LLJs at the center of the precipitation and on its southern side before the onset of heavy precipitation. BLJs were shown to develop earlier than SLLJs.
HS07-A017
Evaluation of the Community Land Model Versions 4.5 & 5 in Simulating Evapotranspiration and Its Three Components Over Globe
Wei HE#+, Dagang WANG
Sun Yat-sen University
The Community Land Model (CLM) is an effective tool for simulating biophysical processes, biogeochemical processes, and their interactions with the atmosphere. Compared with CLM4.5, CLM5 updated the parameterizations of three components of total evapotranspiration. The simulation performance over globe remains to be evaluated. In this study, CLM4.5 and CLM5 are used to simulate monthly global evapotranspiration and its components from 1981 to 2012. We assess their simulations against the products of GLEAM, PML and in situ datasets. Overall, CLM5 performed better in simulating total evapotranspiration and vegetation transpiration, but poorer for canopy interception. Model performance varies with vegetation type and density. When using GLEAM product as the benchmark, CLM5 performs better than CLM4.5 in simulating canopy interception, especially in areas with highly vegetated areas, achieving a KGE value of 0.68. However, CLM5 is inferior to CLM4.5 in simulating vegetation transpiration, especially in areas with moderate vegetation cover with KGE value smaller than 0.1. Taking PML data as the reference, CLM5 performs best in areas with LAI in the range from 0.5 to1.5, but there is a significant bias when LAI exceeds 5. In addition, in-situ measurements show that both models can simulate transpiration well, although some underestimation do exist. For canopy interception, the simulations of the two models are poor with substantial biases. In conclusion, this study explores the simulation capabilities of the CLM4.5 and 5 models for total evapotranspiration and its components. The evaluation results can provide important references for the future model development and application.
HS07-A009
The Impact of Precipitation with Different Temporal and Spatial Resolution on Flood Forecasting
Zhiyuan YIN+, Junchao WANG#, Haixia QI
China Meteorological Administration
Based on the spatial resolution 90m×90m DEM terrain data of Zhanghe reservoir in Jingmen city on Hubei province, the study coupled the three nested spatial resolution 3km×3km, 9km×9km and 27km×27km forecasting precipitation provided by the business model WRF of numerical forecast in Central China region with the lumped Xin'AnJiang model and the semi distributed hydrological model Topmodel respectively. In addition, based on the minutely precipitation combined with hydrological models, the simulation of runoff under different time resolution was analyzed. The following conclusions were obtained by comparing the experiments: (1) The results show that 3km and 9km flood forecasting were close to each other and were better than 27km in the deterministic coefficient and relative error of peak. In the prediction of peak current time difference, the flood forecasting results of 27km was in good agreement with the actual situation. (2) The efficiency coefficient of Xin'anjiang model was 10% - 20% higher than that of SCS model, and the relative error of flood peak was close to the peak and the time difference, but SCS model can be used for runoff simulation in areas without data. (3) The time resolution threshold existed in the efficiency coefficient of Xin'anjiang model and SCS model, and the resolution threshold of Xin'anjiang model was smaller than that of SCS model. When the resolution was about 15 min, the relative error of flood peak and the peak and the time difference of the two models can reached the minimum value. Acknowledgement: This work has been supported by the Open Project Fund of China Meteorological Administration Basin Heavy Rainfall Key Laboratory (2023BHR-Y26). The Meteorology Joint Science and Technology Innovation Fund of Wuhan Metropolitan Area (WHCSQY202305). Innovation and Development Special Project of China Meteorological Administration (CXFZ2022J019).
HS07-A007
The Weakening Relationship Between ENSO and the Following Summer Pacific Japan Teleconnection Since the Late 1990s
Po HU#+
China Meteorological Administration
The predictability and variability of extratropical climate are largely associated with tropical forcing through various teleconnections. The East Asia-Pacific/Pacific-Japan (EAP/PJ) teleconnection is one of the most important factors affecting the summer climate in East Asia. In this work, we confirm the weakening relationship between the El Niño-Southern Oscillation (ENSO) and the following summer PJ teleconnection after the late 1990s and diagnose the possible causes. The results show that compared with that of in 1981-1998, ENSO is less conducive to the formation of anomalous anticyclones in the following summer in the Northwest Pacific (NWP) and the northward propagating Rossby wave train from latitudes of NWP in 2000-2017, resulting in a weaker summer PJ teleconnection. Meanwhile, variation of ENSO feature since 2000 with a suppressed variability leads to a weakened response in the tropical Indian Ocean in the spring and summer. The reduced sea surface temperature response in the tropical Indian Ocean suppresses the excitation of eastward-propagating Kelvin waves and declines the capacitor effect of the Indian Ocean, which is unfavorable for generating anomalies in the NWP and motivating strong PJ teleconnection in meridional direction. Thus, the weakening relationship of ENSO-PJ after late 1990s is the result of the weakened ENSO’s impact on the formation of anticyclones in the following summer in NWP and the declined Indian Ocean capacitor effect on motivating meridionals wave train over East Asia and NWP region.
HS07-A013
An Improved Statistical Filter for Post Processing GRACE Gravity Field Models
Lin ZHANG+, Yunzhong SHEN#, Kunpu JI, Qiujie CHEN
Tongji University
The Gravity Recovery and Climate Experiment (GRACE) and its successor GRACE Follow on (GRACE-FO) have been providing monthly high-resolution gravity field model since April 2002, widely used in exploring global terrestrial water storage (TWS) changes and extreme climates. However, the original time-varying gravity field models are seriously contaminated by the south-north stripe noise, necessitating an efficient filtering method. The widespread empirical and constant DDK filtering methods are susceptible to insufficient or excessive filtering due to neglecting the actual precision information of time-varying gravity field models. In contrast, the statistical Parameter Filtering (PF) method incorporates the covariance matrices of monthly Spherical Harmonic Coefficients (SHCs) to estimate and denoise the signal parameters (i.e., linear trends, accelerations, annual and semi-annual periodic terms), while disregarding non-periodic and interannual signals. To address this issue, we improve the conventional PF method by incorporating those ignored signals based on their prior temporal correlations. The improved method is used to denoise the monthly SHCs of the Tongji-Grace2018 models from April 2002 to December 2016, comparing the results with the conventional PF method. The results show the improved PF solutions how higher signal-to-noise ratios and better agreement with CSR mascon solutions and NOAH hydrological models in global and basin analysis. Average Nash-Sutcliffe coefficients for the 22 largest basins worldwide using the improved PF solutions with CSR mascon and NOAH models are 0.90 and 0.19, significantly higher than 0.17 and -0.71 for the conventional PF solutions. Furthermore, the severities of drought and flood events in the 22 largest basins are accurately identified using the water storage deficit index (WSDI), constructed by the TWS anomalies from improved PF method, which best correlates with those of the Standardized Precipitation-Evapotranspiration Index (SPEI) drought index, with a mean correlation coefficient of 0.67, as compared to other conventional filtering solutions.
Session Chair(s): Ming-Che HU, National Taiwan University, Ke-Sheng CHENG, National Taiwan University
HS32-A001
Revision of Oceanic Niño Index Estimates
Che-Wei CHANG#+, Wen-Cheng HUANG
National Taiwan Ocean University
El Niño profoundly influences global climate and ecosystems, and NOAA relies on the Oceanic Niño Index (ONI) to monitor its occurrence alongside La Niña. Calculated from actual monthly sea surface temperatures within the Niño 3.4 region (5°S-5°N, 120°W-170°W), ONI derives by subtracting monthly sea surface temperatures there from a corresponding 30-year long-term average. The resulting three-month average represents the mid-month ONI value. Notable warming trends in the Niño-3.4 region since 1950 prompt NOAA to define ONI using multiple 30-year base periods. Currently, NOAA updates the 30-year baseline sea temperatures every five years. However, aligning the baseline with the ONI evaluation period causes temporal delays in ONI estimation. For example, ONI values from 2021 to 2025 will reference the 2006-2035 period, undergoing multiple revisions before confirming this base period. This study compares ONI using NOAA's "posterior" ONI and relies on the past 30 years of sea temperature data as an annually updated baseline, aiming to rectify ONI timeliness issues. Additionally, it uses the current month's sea temperature difference from the baseline average to depict temperature changes, deviating from a three-month moving average. ONI estimates reveal an 86.7% accuracy between NOAA’s "prior" and "posterior" ONI values. Conversely, this study's revised ONI values achieve an enhanced 89.7% accuracy against "posterior" ONI values and strongly correlate with NOAA's identification of El Niño and La Niña years. Furthermore, using the monthly temperature difference method effectively resolves ONI's timeliness issue compared to the three-month average temperature difference.
HS32-A002
Making Machine Learning More Transparent Using Explainable AI for Hydrological and Climatological Understanding
Wei SHANGGUAN#+, Feini HUANG
Sun Yat-sen University
With the rapid development of artificial intelligence (AI) in the field of hydrology and meteorology, the lack of interpretability in AI restricts its further commercialization in hydrology and meteorology. To address this issue, we conducted interpretability analysis for soil moisture prediction. We adopted the explainable artificial intelligence (XAI) method of global and local interpretability to interpret the model and developed a post-hoc interpretation system suitable for hydrological and meteorological forecasting. We found that at the station scale, the hysteresis of soil moisture itself and the cumulant of precipitation are more important for its prediction. At the same time, the Random Forest model can also find the impact of snow melting process on soil moisture. In addition, we also explored the prediction of global soil moisture drought. The prediction of grassland drought shows that soil temperature, atmospheric water deficit and latent heat flux are important variables, while the prediction of forest drought is more dependent on interannual time changes and time series. From the perspective of spatiotemporal prediction, we have established the Conv-LSTM model to predict soil moisture in China, using permutation importance and smooth gradient to explain the model globally and locally. The results showed that precipitation and soil properties have a significant impact on soil moisture, and the gradient spatiotemporal distribution of precipitation, net heat radiation, and temperature is consistent with basic physical cognition. This indicates that permutation importance and smooth gradient can better reflect the internal understanding of physical relationships within the model, enhancing its interpretability and trustworthiness. Overall, XAI has certain potential in hydrological and meteorological artificial intelligence forecasting, providing support for the development of AI in this field and improving the reliability of AI forecasting. We provided a XAI toolbox named ExplainAI, available at https://pypi.org/project/ExplainAI/. Papers at https://atmos.sysu.edu.cn/teacher/372.
HS32-A003
Bayesian Spatial Interpolation of High-resolution Rainfall Data: A Case Study in Singapore
Xiao PENG1#+, Biao LONG2, Xiaogang HE1
1National University of Singapore, 2Lanzhou University
Better management of urban water resources demands accurate, high-resolution rainfall data, particularly given the spatial complexity of urban landscapes. Deploying rainfall stations in every neighborhood is impractical, and direct downscaling using physics-based dynamic models from low-resolution global circulation model outputs can introduce substantial uncertainties without local evidence. In this study, we introduce a causality-based Bayesian spatial interpolation framework. First, we assume that real-world observations and their ‘poor’ simulation counterparts are different realizations stemming from the same stochastic process. Then, we extract key characteristics of the underlying process, such as spatial covariances, directly from simulations to interpolate rainfall from limited observations. The framework is tested in interpolating Singapore's monthly rainfall at a fine 500m resolution over 1981-2020 by integrating simulated spatial covariances with data from 14 National Environment Agency stations. Results demonstrate significantly improved model skill across all stations and calendar months in a leave-one-out cross-validation experiment. Additionally, the Bayesian foundation of the approach allows straightforward estimation of the associated uncertainties, offering valuable insights for future planning of the rainfall monitoring system. A counter-factual analysis explores the current station network's robustness under a changing climate, highlighting the need for supplementary measures during the drier months in a warming future. Overall, this framework presents a cost-effective solution for developing spatially continuous, high-resolution rainfall data, contributing to better management of locally relevant urban hydroclimate extremes.
HS32-A006
SoMo-Bench: A Benchmark Dataset for Machine Learning on Soil Moisture
Sungmin O1#+, Sujeong LIM2, Seon Ki PARK2
1Kangwon National University, 2Ewha Womans University
Benchmark datasets in the domain of machine learning (ML) aim to provide standardised data that represent real-world problems, allowing the quantitative evaluation and comparison of the performance of different ML algorithms. As ML becomes a powerful tool in Earth System Sciences, the community has started developing benchmark datasets for specific applications of interest, as seen in the examples of WeatherBench for meteorological data or Caravan for runoff data. In line with the recent efforts on building benchmark datasets, here we introduce a benchmark dataset for machine learning on soil moisture (‘SoMo-Bench’). In recent years, ML methods have been actively applied to simulate soil moisture dynamics; however, they are difficult to compare due to the inconsistency among the studies, including different data sources, preprocessing, and spatiotemporal scales. To overcome this issue, we aggregate and standardise existing global in-situ soil moisture data, with meteorological forcing data, at the daily scale and 0.25° spatial resolution. SoMo-Bench will support comparing the quality of competing ML algorithms and easy reproducibility by the community to facilitate the application of machine learning in soil moisture simulation.
HS32-A007
Spectrum Network Optimization for Connectivity of Water Resources System
You-Hong LIAO+, Ming-Che HU#
National Taiwan University
Extreme weather events and uneven water distribution cause challenges for water resources management in Taiwan. Accordingly, the Taiwanese Water Resources Agency conducts the "pearl chain" project to integrate the water resources systems through pipeline connections in Northern, Central, and Southern regions. This research focuses on reservoir connectivity and develops a water allocation model to determine optimal water transmission volumes through the pipeline system, meeting various water demands such as domestic, industrial, and agricultural needs. To best describe the periodic characteristics of hydrological phenomena, the model incorporates frequency spectrum analysis using Fourier series transformation to convert time domain data into frequency domain data, allowing analyzing on the frequency domain. Meanwhile, a minimum cost network flow optimization model is developed by replacing the flow variables to time-dependent flow functions in the network flow model with the objective function of minimizing spectrum discrepancies between water supply and demand. To validate the efficacy of the model, a spectrum network optimization case study of regional water resource allocation is presented. This research applies the model to the southern region of Taiwan, including Wushantou Reservoir, Tsengwen Reservoir, Nanhua Reservoir, and Gaoping River Weir, analyzing the water situation and evaluate potential enhancements resulting from different reservoir connectivity scenarios and aiming to determine the optimal outflow from reservoirs to effectively meet water requirements in the region. Results indicate that connecting Tsengwen Reservoir and Nanhua Reservoir effectively addresses severe water shortages in Tainan. Furthermore, with the existing pipeline connecting Nanhua Reservoir and Gaoping River Weir, the benefits of water allocation extend to Kaohsiung, particularly during the spring season.
HS32-A011
Divergence as an Indicator for Feature Selection for Land Cover Classification Using Machine Learning Method in a Cloud-based Remote Sensing Platform
Chun-Ju CHENG#+, Yuan-Fong SU
National Taiwan Ocean University
In recent years, monitoring and analyzing land cover changes have played a crucial role in disaster prevention and environmental management. Traditional methods of land cover classification have heavily relied on on-site surveys and aerial photograph analysis, which are time-consuming and high labor costs. In recent years, a cloud-based remote sensing platform called Google Earth Engine (GEE) has attracted extensive attention. With GEE it is much easier to access satellite imagery including optical and radar imageries. However, how to use these datasets efficiently is not widely documented. The goal of this study is to integrate optical and radar imagery in GEE for land cover classification by using divergence as an indicator for feature selection in order to enhance classification efficiency and accuracy. This research utilizes Sentinel-1 SAR and Sentinel-2 MSI imagery from the GEE, combining machine learning techniques, including Support Vector Machine (SVM) and Random Forests (RF), for land cover classification. We select six land cover categories including forest, grassland, cropland, built-up, bare soil, and water. Combining optical and radar imageries, we have 9 bands in total. Divergence is used as an indicator to identify which band is more important for land cover classification base on the over-all accuracy. The results shown that green band and descended vv polarization band could be dropped from the features for land cover classification.
HS32-A014
Long Lead Time Rainfall Nowcasting Using AI-based Deep Learning Algorithm
Xianqi JIANG#+, Ji CHEN
The University of Hong Kong
It is a critical need to provide timely and valuable alerts of rainstorms and floods to the public. However, it is still a world-class challenge to achieve rational nowcasting of rainstorms with a short lead time, normally within 6 hours, compared to the traditional weather forecast. Different deep learning algorithms have been adopted to improve its accuracy yet the lead time is still limited. This study focuses on nowcasting evolution of rainstorm clouds from radar echo mosaic images, which can be used to nowcast rainstorms, extending the lead time for emergency alerts and disaster mitigation. Using AI-based deep learning algorithm, the study proposes a new improved model for long lead time rainfall nowcasting. It is shown that it outperforms multiple state-of-the-art nowcasting methods for 2nd to 3rd hour nowcast. Three typical storm cases of different rainfall intensities from a radar dataset collected in China are evaluated and ways of future improvement are suggested.
HS32-A017
Image-based Automated Water Level Measurement in Channels Using Deep Learning Approach
Wei-Che HUANG#+, Xin-Yan YANG, Wu HONG-XIAN, Wen-Cheng LIU
National United University
Owing to its inherent capacity for self-learning, deep learning has found increasing applications across diverse domains, including the measurement of river water levels. Within the framework of this investigation, we leverage CCTV imagery, employing the YOLO network within the realm of deep learning to autonomously discern the precise position of the water gauge. Subsequently, we ascertain the water level by utilizing a virtual gauge and juxtapose it against the empirically measured water level. The research encompasses the utilization of a total of 28 hourly CCTV images collected over a span of 4 days for the purpose of YOLO network training. Following the training regimen, the YOLO network is deployed to automatically identify the position of the water gauge and compute the water level using real-time CCTV images obtained over the subsequent two days. The outcomes reveal a Root Mean Square Error (RMSE) of 0.10 meters, along with a Mean Absolute Percentage Error (MAPE) of 8.78%, signifying the differential between the water level computed by the deep learning YOLO network and the actual water level. These results underscore the efficiency of deep learning in swiftly and autonomously gauging river water levels.
HS32-A016
Estimation of Snow Depth and Snow Water Equivalent Using Machine Learning
Yasutaka WAKAZUKI#+, Hikaru ENDO
Ibaraki University
Climate changes in snowpack variables such as snow water equivalent and snow depth are essential in the impact assessment of water resources, social lifestyles, and snow tourism resources. However, high-resolution land snow data are not sufficiently provided to cover the uncertainty of climate change scenarios because the snowpack variables require high-resolution regional climate model simulations. In this study, we developed an empirical statistical model using machine learning (ML) to estimate daily snowpack variables from the output of high-resolution surface atmospheric variables. In developing the model, we used the dataset of NHRCM02, a high-resolution regional climate model simulation with a spatial grid size of 2 km, including land surface processes. The 20-year data have been provided for the present and future climate based on the RCP8.5 scenario in the NHRCM02. The snowpack variables of NHRCM02 are used as both the predictands in the learning of the model and reference data for the evaluation of the model. Multiple regression (MR), Multilayer Perceptron (MLP), XGBoost (XGB), and LightGBM (LGBM) have been applied as the statistical models, and the predicted results with these models are compared and evaluated. Predictands of the models are not actual snow variables but daily increments of the snowpack variables. The results showed good accuracy except for the MR. The predicted results of the models are corrected after the ML estimation with two schemes. The first scheme is the zero resetting at the end of August every year. The second scheme applies the correction ratio with the coordinates of the year day and quantile values of mean snowpack variables. The estimation showed promising results, which are shown in the presentation. Climate change signals of the snowpack variables were also estimated with higher accuracy. The S-18 project, related to Japan's climate change impact assessment and adaptation study, supported this study.
HS32-A010
Research on Method to Extreme Precipitation Nowcasting Based on Artificial Intelligence Model
Chao TAN+, Ji CHEN#, Hongxu ZHU
The University of Hong Kong
There is a great need to mitigate its socioeconomic effects through accurate nowcasting of extreme precipitation, and it’s important for improving modern urban governance, and alerting warning for flash floods and geological disasters. The rise of deep learning in recent years has brought significant changes in the field of nowcasting, with significant advantages in the integrated processing of meteorological data and the mining of physical features within the data. Current methods are subject to computing resources, computational capabilities and data limitation, with numerical weather predict methods struggling to capture turbulence dynamics and machine learning methods failing to obey intrinsic physical laws. Here we introduce an artificial-intelligence-based time-skip method for improving nowcasting of extreme precipitation prediction. On the basis trained on 10 years data of precipitation observations from the National Oceanic and Atmospheric Administration Climate Prediction Center MORPHing technique (NOAA-CMORPH) in the Guangdong-Hong Kong-Macao Great Bay Area, the model of ConvLSTM with time-skip produces plausible precipitation nowcasts and with lead times of up to 6h. The time-skip method obtains stronger deterministic forecast results when compared with precipitation assimilation NWP and general method of ConvLSTM. The method also works well with the root mean squared error (RMSE) and the correlation coefficient(R2), and its RMSE is less than 0.02 and R2 is not less than 0.6 compared to the observation results.
Session Chair(s): Jian-Ping SUEN, National Cheng Kung University, Kyungrock PAIK, Korea University
HS06-A003
Dune Resistance Dominates Low-flow Water-level in a Large Dammed Fluvial River
Yong HU1#+, Dongfeng LI2, Jinyun DENG3, Yitian LI3
1Chinese Academy of Sciences, 2Peking University, 3Wuhan University
Dunes are important for bedload transport in almost all large river systems and significantly contribute to flow resistance, which is fundamental for simulating discharge, sediment transport, and flood routing. However, dunes and flow resistance spatiotemporal dynamics in the Middle Yangtze River remain poorly studied. Here we used annual profiles of 450 cross-sections and in-situ data on river bathymetry, discharge, water levels, and sediment. We found that dunes developed and flow resistance increased (+10%) in the post-Three Gorges Dam period. We ascertain that the development of dunes plays the dominant role in augmenting flow resistance, as evidenced by roughness height change (+29%) using a modified Van Rijn method. Ultimately, dune development was incorporated into a hydrogeomorphic numerical model of the Yangtze River to improve flow resistance quantification, and thus, the water level simulation. Our findings provide insights into flow resistance in response to damming on large rivers and have important implications for riverine ecology and flood management.
HS06-A006
Rapid Emergence of Downstream Fining Captured from Numerical Modeling of Whole Landscape Evolution
Dongwoon KANG+, Kyungrock PAIK#
Korea University
Downstream fining, a spatial pattern found in typical stream bed material sorting along downstream, has widely been perceived in association with the concave-upward longitudinal profile in geomorphology community. In contrast, engineers have demonstrated the rapid emergence of downstream fining from flume experiments or 1d numerical modeling, without the evolution of longitudinal profile. To address the truth between these two hypotheses, we have implemented a long-term, sufficient enough to allow the formation of profile concavity, numerical simulations. We found that the downstream fining appears in a very short time span without the need of concave profile, which supports earlier flume or numerical experiments. However, as the landscape continues to evolve, the pattern in grain size sorting rather disappears, while the concavity of longitudinal profile becomes apparent.
HS06-A001
Infrastructure Impact and Riverbed Degradation at the Weir Downstream Reach
Fong-Zuo LEE1#+, Nhat Lam HUYNH NGUYEN2, Gwo-Fong LIN3
1National Chung Hsing University, 2Department of Civil Engineering of National Chung Hsing University , Taiwan, 3National Taiwan University
The primary risk of traffic disruption and potential loss of life stems from bridge failure caused by flood-induced scour around piers. Monitoring variations in scour in real-time is essential to prevent such bridge failures. A scour monitoring system has been created and implemented in the field. This system includes an array of vibration-based micro-electro-mechanical systems sensors, along with instruments to measure water level and flow velocity. During flood events, the scour monitoring system records changes in scour and deposition depths at the bridge piers over time. A numerical simulation module, combining one-dimensional and two-dimensional mobile-bed hydrodynamic models, is established to calculate scour and deposition depths based on field hydrological conditions. Field-measured data obtained from the real-time scour monitoring system are used for model validation. Various local scour formulas are evaluated to assess their applicability using field-measured data. Considering the complexity of hydraulic mechanisms related to sediment transport around the pier, a suitable local scour formula for Mingchu Bridge in Cho-Shui River at the Chi-Chi weir downstream reach is developed. The real-time scour monitoring system, in conjunction with the numerical simulation module developed in this study, offers precise information on scour and deposition processes at the bridge pier and downstream river reach. This information is valuable for decision-makers to assess the risk of bridge damage and understand river bed variations.
HS06-A004
Effect of Upstream Sediment Inflow Conditions on Sediment Transport Simulation by Grain Size
Shimon SUZUKI1+, Keiko UDO1#, Daisuke NAKAHARA1, Hiroshi TAKEBAYASHI2
1Tohoku University, 2Kyoto University
Decadal sediment supply from rivers to the coast is usually computed with a one-dimensional bed deformation model. The analysis needs to give various initial and boundary conditions, and the boundary conditions for sediment are especially significant. However, sufficient measured data on sediment have not yet been obtained, and appropriate conditions of sediment amount and grain size distribution from the upstream boundary should be given considering the effects of human activities such as dam construction and slope failure in mountainous areas. In this study, a one-dimensional riverbed deformation analysis was conducted for the period 2000-2019 in the basin of Abukuma River to evaluate the decadal effects of various upstream sediment inflow conditions on sediment transport to the coast. Increasing the sediment inflow from the upstream boundary increased the sediment supply to the coast and the amount of sediment deposited in the river channel, indicating that these trends differed with grain size. The sediment supplied to the coast consisted of silt and fine sand, while the medium and coarse sand from the upstream boundary of the river was deposited in the river channel. The simulation results show the mode of sediment transport during floods is mainly suspension, and the amount of the suspended load is affected by the sediment inflow from the upstream boundary. On the other hand, the supply of medium and coarse sand from the river to the coast was almost constant regardless of the inflow from the upstream boundary. This suggests that medium and coarse sand from the upstream boundary does not contribute to sediment supply to the coast on a 20-year scale. Sediment supply from the river to the coast was quantitatively demonstrated to be highly dependent on the inflow of silt and fine sand from the upstream edge of the river.
HS06-A011
A Simple Distributed Model for Direct Runoff Routing in a Catchment
Jisoo LEE+, Kyungrock PAIK#
Korea University
Direct runoff routing has been an important task in hydrological practices, and many distributed models have been developed to date. Hydrodynamic models such as dynamic, diffusive, and kinematic wave models provide sophisticated modeling results, but they demand a large number of high-resolution data. On the other end, step-by-step transition of waterbody has been conceptualized in simple models such as RRL (Road Research Lab.) method. Essentially the same idea has been adopted in most landscape evolution models. Whilst simple, the transition models lack in accommodating physics of flow: flow velocity is poorly estimated; the acceleration is ignored; and the dispersion is neglected. As a reasonable compromise between above two modeling directions, we propose a new model which basically partially transits water in each time step. This approach can simulate the nonlinear catchment response according to the spatial distribution of flow velocity, while preserving the computational efficiency of the simple model. The proposed model is compatible with data of typical resolutions, e.g., hourly rainfall and 30 m DEMs (Digital Elevation Models). The proposed model is calibrated and validated using observations in the Pyeongchanggang catchment in South Korea.
HS06-A010
Development of a Practical Surface Image Velocimeter Using Spatio-temporal Images for Small-sized Rivers
Kwonkyu YU1#+, Byungman YOON2, Seojun KIM2, Kang Min KOO3
1Dong-Eui University, 2Myongji University, 3HydroSEM Co., Ltd.
The purpose of this study is to present the most appropriate hardware and software configurations to produce a practical SIV(surface image velocimeter). The term 'practical' means that the system can measure the water level and flow velocity of the river at minute intervals, which is almost real-time in the actual river, and calculate the flow discharge from the measured data. In addition, it also means that this work is not done once, but continuously at all times. To make a practical SIV, we constructed the system with a CCTV, a water stage gauge, and an analysis software on an Android board. The camera continuously captures images for 30 seconds with 2 minute intervals. And the 11-parameter projection method was used in the software that analyzes the captured images to reconstruct the exact measurement points according to the changing water stage. In addition, a spatio-temporal image construction method was developed so that the directions of the images can be arranged in the main flow direction at each measurement point. The surface image velocimeter composed of the proposed method was produced and installed at small-sized rivers in Korea. And results of measurement of some heavy rainfall events showed that the proposed system can precisely measure flow discharge in a rapid and continuous manner.
HS06-A005
A Multiagent Modeling Framework for a Water Resource Allocation Problem in River System
Mengxiang ZHANG, Ting Fong May CHUI#+
The University of Hong Kong
Green infrastructures (GIs) for rainwater harvesting have gained widespread recognition in the sustainable management of numerous river systems. However, their implementation also presents new challenges for water resource allocation within these systems. This study aims to develop a multiagent modeling framework to address GI-driven water resource allocation problems in river systems shared by multiple urban areas, which simultaneously employ GIs for rainwater collection and utilization. The proposed framework encompasses all relevant stakeholders as agents, effectively combining watershed water resource allocation, urban water supply portfolio selection, and GI construction planning. It aims to: 1) determine the optimal water allocation scheme, 2) assess the hydrologic impacts of the scheme on the river system, and 3) evaluate the role of GIs in the allocation process. We apply the framework to the Colorado River Lower Basin, the United States. The study examines three water allocation schemes - water trading, quota, and tariff systems - and analyzes their design and performance in the context of water resource allocation within the river system. Additionally, the potential roles of GIs under these schemes are explored and discussed. Results indicate that all three allocation schemes effectively balance cost and equity considerations in water resource distribution while characterizing the respective impacts of each scheme on the river system. Moreover, our findings highlight the GI effect, demonstrating that the development of GIs for rainwater utilization can potentially reduce costs associated with the implementation of the three allocation policies. However, this may exacerbate existing inequities among water users in the allocation process. These insights offer valuable guidance for watershed and urban water managers understanding the complex interplay between GIs, water resource allocation, and hydrologic stability in shared river systems, and seeking to design and analyze sustainable water policies for arid river systems.
HS06-A015
Adaptability Assessment of Dapeng Bay and Coastal Reservoir Project to Sea Level Rise Scenarios - Analysis from the Perspective of Ecosystem Services
Hsueh Kuan CHEN+, Jian-Ping SUEN#
National Cheng Kung University
Along with the development of the economy, the extensive use of fossil fuels has exacerbated climate change, leading to global warming. Under the impact of warming, abnormal events such as droughts, floods, and sea level rise (SLR) are expected to occur more frequently. Taiwan has faced severe droughts in 2015 and recent years (from 2020 to 2023). Although the drought has been alleviated due to typhoons affecting Taiwan in 2023 summer, the task of developing new water resources remains imperative. As a potential new water resource development project, the lagoon in Dapeng Bay is considered a suitable site for the design of a coastal reservoir. However, to avoid repeating past mistakes, it is crucial to consider the balance between people and nature from the early stages of design and development. Ecosystem Services (ESs) provide a good concept for quantifying nature. This study combined physical models and Cost-Benefit Analysis (CBA) to calculate the ESs value of different categories and monetize the Ecosystem Services Value (ESV) in Dapeng Bay. Then, the synergy/trade-off of the coastal reservoir project on ESV in Dapeng Bay and the impact on organisms caused by changes in lagoon water quality will be evaluated. Finally, this study further discusses the threats that SLR will pose to coastal areas and the ability of coastal reservoirs to protect the Dapeng Bay area from seawater intrusion under SLR scenarios.
Session Chair(s): Dong WANG, Nanjing University, Xudong ZHOU, Ningbo University, Peng JIANG, Hohai University
HS43-A018
| Invited
Impacts of Rainstorm Characteristics on Flood Inundation Mitigation Performance of LID Measures Throughout an Urban Catchment
Qiongfang LI1#+, Zhengmo ZHOU1, Pengfei HE2
1Hohai University, 2Yellow River Institute of Hydraulic Research
The hydrological benefits of sponge city construction have sparked a variety of academic studies. However, the effectiveness of sponge city construction in mitigating flood inundation at the urban catchment scale remains rarely investigated. Therefore, the Jiaodong catchment in Zhenjiang City, which is a national sponge pilot city and has extensively implemented various LID measures, was selected as a study site. The SWMM-2DCA model was established, and then applied to evaluate the accumulative effectiveness of LID measures in flood mitigation under different 2-hour design rainstorms with different return periods and peak position coefficients. The results revealed that nearly 90% of the inundated area had an inundation depth of less than 0.15 m, and the impact of rainstorm characteristics on the maximum inundation depth was very limited. Both the maximum inundation volume and area were positively related to the return period and the peak position coefficient of rainstorms. The increase in the rainstorm return period could advance the start of inundation and retard the occurrence of peak inundation. After the implementation of LID measures, the maximum inundation volume and area could be significantly reduced by 63 ~ 98% and 41 ~ 96% respectively, but the average reduction rate for maximum inundation depth was only 3.7% for rainstorms with a return period longer than 10 years. This indicates that LID controls inundation better for volume and area than for depth. The absolute reductions in both maximum inundation area and depth almost reached their extreme values at the 10-year rainstorm return period. The effects of LID on the timing of peak inundation depended largely on the peak position of rainstorms. These findings could contribute to a better understanding of the flood inundation mitigation performance of sponge city construction.
HS43-A021
| Invited
Study on Dynamic Runoff Generation Mechanism and Modeling Based on Water-heat Multi-phase Coupling in Permafrost Area of the Source Region of the Yangtze River
Peng JIANG#+
Hohai University
The Qinghai-Tibet Plateau has experienced remarkable warming and wetting recently, which exacerbates the degradation of permafrost. It is still unclear for the feedback mechanism between water-heat-vapor transport with phase changes and the runoff generation during the freezing-thawing processes, posing new challenges on the assessment of runoff response and water conservation function of the alpine headwater area. This presentation will focus on the impact of changing energy and water phase state on the runoff generation processes in the permafrost active layer. Based on the in-situ observations, indoor single-factor control experiments and numerical simulations, this study strives to investigate the feedback mechanism of water-heat-vapor coupling and runoff generation processes during the freezing-thawing processes in the source region of the Yangtze River and identify the main controlling factors for the runoff evolution under climate change. Meanwhile, a dynamic runoff generation model will be built based on the conservation of water-heat-vapor coupling theory to realize the dynamic coupling of the energy and water phase changes and the runoff processes. The proposed model will be used to interpret future changes and uncertainties of runoff in the study region under climate change. It will contribute to illustrate the complex hydrological process and the spatiotemporal variations of water resources and accurately evaluate the eco-hydrological responses to future climate change in permafrost regions.
HS43-A005
Effects of Artificial Water Withdrawal on the Terrestrial Water Cycle in the Yangtze River Basin
Hejia WANG#+, Mingxiang YANG
China Institute of Water Resources and Hydropower Research
Clarifying the response of the terrestrial water cycle to the influence of climate change and human activities and accurately grasping the variations in the water cycle and water resources under the changing environment are the scientific basis for achieving the sustainable development of the Yangtze River Economic Belt. In this paper, a dataset of rasterized water consumption in the Yangtze River Basin was constructed, and an artificial water withdrawal module considering the process of water intake, water consumption and drainage was designed, which was coupled with the land surface model CLM4.5. The coupled model was calibrated by using the monthly observed discharge of several hydrological stations in the Yangtze River basin. The Nash efficiency coefficients (NSE) of the monthly discharge of the 15 hydrological stations ranged from 0.66 to 0.96, and the relative error (PBIAS) ranged from −13.5% to 16.5%. Two numerical simulation experiments were carried out to reveal the impact of artificial water withdrawal on the water cycle process in the Yangtze River Basin. The results indicate that artificial water withdrawal leads to an 0.1–0.3 m increase in groundwater table depth in most areas of the basin, and agricultural irrigation leads to a 0–0.03 mm3/mm3 increase in soil moisture in most areas. Climate change dominates the variation of discharge in the Yangtze River basin and leads to an increase in discharge at most stations.
HS43-A019
Assessing the Impacts of Climate Change on Urban Rainwater Harvesting Systems’ Hydrologic Performance Using an Analytical Probabilistic Approach
Jun WANG1#+, Jiachang WANG1, Shengle CAO1, Shouhong ZHANG2, Yiping GUO3
1Shandong University, 2Beijing Forestry University, 3McMaster University
As an effective climate change adaptation measure, rainwater harvesting (RWH) has been widely used in many cities to combat the urban water issues such as urban flooding and water scarcity under the threaten of extreme climate events increasing urbanization and rapid population growth. The conventional analytical probabilistic model has the advantage of computational efficiency and ease to use. This approach usually requires the exponential distribution of rainfall event characteristics including rainfall event depth, duration and inter-event time. It has been validated that the historical long-term hourly rainfall records in many countries and regions can well satisfy this exponential distribution assumption. However, the historical long-term hourly rainfall data are insufficient and difficult to obtain in many areas of China. Moreover, the observed long-term daily rainfall data usually has worse performance in rainfall event separation and fitting the exponential distribution of rainfall event characteristics than the hourly data. As a result, the conventional analytical probabilistic model (APM) for RWH systems based on daily rainfall data usually results in inaccuracy to some extent of hydrologic performance. To address the above limitations, this study proposes an approach to downscale the daily rainfall data to hourly data to promote the accuracy of the conventional APM. In addition, this study investigated the impacts of future climate change on runoff reduction and water supply performances of RWH systems using the APM for the first time. A few representative cities of China are tested as study areas. The General Circulation Models (GCMs) projected future (2025–2050) monthly rainfall at grid scale is downscaled to daily rainfall at a few stations in China. The responses of hydrologic performances of RWH systems to climate change are examined. The results of this study will provide scientific guidance for designing RWH systems with more climate change adaptability.
HS43-A020
Study on the Application of Different Optimization Algorithms in Watershed Hydrological Model of Shiquan Reservoir
Simin QU#+
Hohai University
Watershed hydrological model is the most important tool for real-time flood forecasting. Parameter optimization is an important study content of hydrological model. The application of simple and efficient parameter optimization method can improve the efficiency and promote the use of the model. Human-computer interaction parameter calibration method is time-consuming and laborious, and can be highly subjective. Automatic calibration methods are based on optimization algorithms to find the optimal value on the surface with the sum of error squares as the objective function and they are more objective, but there are still some problems in them. The paper takes the Shiquan Reservoir Watershed as the study area to construct Xinanjiang model. The system differential response parameter calibration method is used to optimize the sensitive parameters of the model and the optimized parameters and simulation results are compared with the human-computer interaction method and SCE-UA method to explore the applicability and efficiency of this method in watershed hydrological simulation. The results show that the system differential response parameter calibration method has better performance on efficiency and accuracy than human-computer interaction and SCE-UA methods. The calibrated parameters have shown good flood simulations results in Shiquan reservoir. The averaged deterministic coefficient reached 0.937. The system differential response parameter calibration method can be further expanded to be used in flood simulation of other watersheds and other models.
HS43-A016
Entropy and C-vine Copula Based Spatio-temporal Identification of Drought Considering Non-stationarity
Xiaopei JU1+, Dong WANG1#, Pengcheng XU2
1Nanjing University, 2Yangzhou University
Studies at both global and local levels suggest that droughts will become more frequent and severe as temperatures rise. Therefore, it is crucial to develop drought early warning methods that are adapted to environmental changes. This study proposes a stepwise dynamic coupling of the principle of maximum entropy (POME) with the C-vine Copula (DPC) conditional probability method to construct a prediction model. The model uses precipitation and high-temperature conditions to predict hydrological droughts (characterized by the runoff anomaly index (RAI)) for the Jinsha River Basin of China in two drought-prone seasons: summer (August) and autumn (October). The model comprises three main aspects. Firstly, the POME is used to fit the margins to reduce the uncertainty in fitting traditional parameter distributions. Secondly, temporal network theory is employed to model non-consistent joint distributions to address the lack of consideration for nonstationarity in probability prediction models. The conditional quantile function based on the C-vine Copula is carried out to generate simulated sequences. The study demonstrates that the optimal moments-based POME produces more accurate marginal probability distributions than those of parametric ones. Additionally, the results of the optimal time-window screening in the time network are generally consistent with the distribution of regional hydrological drought characteristics. In regions experiencing frequent and severe droughts, the model structure needs to be updated more frequently. The study tested the method by selecting two typical events in the basin: the summer drought in August 2009 and the autumn drought in October 2010. The predictions of RAI using the DPC model were consistent with the corresponding historical RAI observations over most of the basin. However, the autumn forecasts were less accurate than the summer ones, possibly due to the lower correlation of the autumn variables compared to those in summer. These findings can inform drought management strategies under climate change.
HS43-A010
Analyzing the Characteristics of 24 Solar Terms Precipitation Changes in China Based on SMMS Method
Along ZHANG#+, Dong WANG
Nanjing University
Under the joint influence of climate change and human activities, the spatiotemporal variability and trend of precipitation have changed. The traditional method of analyzing precipitation trends based on annual, monthly, and seasonal time scales has significant limitations. The research results cannot be well used to guide agricultural production and life, and the analysis of regional precipitation changes is not significant. The calculation workload is large, and there may be opposite trends in precipitation changes at adjacent stations. This contradiction may lead to errors in regional water resource planning and management decisions, and may cause safety hazards. In order to evaluate the spatiotemporal characteristics of regional precipitation and avoid the impact of the time scale of oil region precipitation, this study introduced the traditional 24 solar terms that guide agricultural production and life in China as the time scale, and used the system clustering maximum entropy multi window sliding trend co frequency trend (SMMS) method to achieve the analysis of regional precipitation trend changes. Redefine local microclimate zones and conduct detailed analysis of important solar terms such as the Spring Equinox, Summer Solstice, Autumn Equinox, and Winter Solstice, ensuring that the general patterns of precipitation changes do not differ significantly from the actual situation. Compared with traditional methods, the 24 solar term division time scale is more significant in studying changes in precipitation, and the SMMS method is more accurate and comprehensive in identifying regional precipitation trends. By combining the 24 solar terms with the SMMS method, not only can the research area be reasonably divided and the computational complexity be reduced, but the analysis can also be based on typical representative stations with the maximum regional information. In addition, it can effectively guide agricultural production and provide scientific reference basis for water resource allocation in different solar terms.
HS43-A027
Precipitation Updating Based on Rainfall-runoff System Differential Response for Flood Forecasting
Xiaoqin ZHANG#+, Rui QIN, Weimin BAO
Hohai University
Precipitation is one of the most important inputs of hydrologic models; the quality of precipitation data directly affects flood forecasting. In this study, an error correction method based on rainfall-runoff system differential response is established to improve flood forecasting by updating areal mean precipitation (AMP) and spatial distributed precipitation (SDP), respectively. The stepwise approximation approach and regularized least square algorithm are adopted to calculate the solutions. The performance of Xinanjiang model for flood forecasting by using updated AMP and SDP are compared in different scale basins in China. The case study results demonstrate that both the AMP and SDP updating can improve the accuracy of flood forecasting; and the SDP updating performs better due to the consideration of rainfall spatial distribution especially in basins with strongly uneven spatial distribution of rainfall. With higher accuracy and stronger stability, the proposed updating method based on rainfall-runoff system differential response is worthy of further applications for real-time flood forecasting.
HS43-A002
Coupling Coordination Analysis of the “Three Waters” System in the Yellow River Basin
Huanghao YU+, Binquan LI#
Hohai University
There is a complex relationship between resource-attributed water, ecological-attributed water and environmental-attributed water (three-waters) in the Yellow River Basin, such as competition, synergy and transformation. Exploring its intrinsic mechanism can provide guidance for water resources planning in the Yellow River Basin. In this study, 62 prefecture-level cities in the Yellow River Basin were selected as the research objects. Data of these cities were collected for the period from 2013 to 2022, including per capital water use, sewage treatment rate, NDVI, and economic losses from flooding. The key factors were obtained by screening using frequency statistics, expert consultation, correlation analysis and principal component analysis. Some methods, e.g., hierarchical analysis, entropy weighting, CRITIC weighting, projective tracing evaluation and combination assignment based on game theory, were used to obtain the weighting results of the “three waters” subsystems. The spatial and temporal distribution of the coupling coordination degree in the Yellow River Basin was calculated by using the coupling coordination degree model. The system dynamics model of the Yellow River Basin was constructed by determining the system boundary, causality analysis, and stock flow analysis. The future coupling and coordination of the “three waters” system under the scenarios of increase revenue and reduce expenditure, economic development, and environmental protection could be predicted. The results can provide the theoretical foundation for “three waters” integrated dispatch in the Yellow River Basin.
HS43-A003
Performance Enhancement of GRU Based Deep Learning Flood Forecasting Model with Attention Mechanism and FCN Model
Cheng CHEN+, Binquan LI#, Huihui LI
Hohai University
Accurate flood forecasting is the foundation of reservoir flood control optimization scheduling, and a long forecast leading time can provide sufficient time for optimizing decision-making. However, in semi-humid and semi-arid regions, the complex runoff generation mechanisms often result in low accuracy of hydrological models. In recent years, deep learning models have been widely applied to flood forecasting. This study developed a hydrological forecasting model based on the gated recurrent unit (GRU) network, and compared it with physically-based hydrological models (Xinanjiang model and vertically mixed runoff model) in the Yi River and Qin River basins in the middle reaches of the Yellow River. Furthermore, the GRU-FCN, Attention-GRU, and Attention-GRU-FCN hybrid models were developed by incorporating the fully convolutional network (FCN) and Attention mechanism. The FCN is capable of capturing the intricate temporal variations in time series data, while the Attention mechanism enhances the focus on crucial information within the input time series data. Each model utilizes hydro-meteorological characteristics (precipitation, evaporation, temperature, runoff, etc.) within the watershed for flood forecasting. The results indicated that the GRU model outperformed the Xinanjiang model and vertical mixed runoff model in terms of flood forecasting accuracy in the study area. However, the forecasting accuracy of the GRU model rapidly declines with the extension of forecast leading time. The Attention-GRU-FCN model exhibited higher forecasting accuracy than other models, and demonstrated more stable performance in longer forecast leading time scenarios. The Attention-GRU-FCN model may serve as a better approach for flood forecasting in semi-humid and semi-arid regions.
Session Chair(s): Xiaojun WANG, Nanjing Hydraulic Research Institute, Ministry of Water Resources
HS03-A007
| Invited
Character and Driving Factors for Agricultural Water Use in China
Xiaojun WANG1#+, Tao ZHANG2, Jianyun ZHANG2
1Nanjing Hydraulic Research Institute, Ministry of Water Resources, 2Ministry of Water Resources
Agricultural water use includes irrigation water use and water use for forestry, animal husbandry and fishery. In China, the agricultural water use, especially irrigation water use, constitutes a significant proportion and directly influences the country's water security strategy. This study analyzed the agricultural water use situation in 31 provincial-level administrative regions of China (excluding Hong Kong, Macau, and Taiwan) from 2001 to 2020. The results indicate that the average annual agricultural water use in China was 371.550 billion m3. Among geographical regions, Central-South and East China recorded the highest figures (94.021 and 93.868 billion m3, respectively). At the provincial level, Xinjiang, Jiangsu, and Heilongjiang had the highest agricultural water use (49.737, 28.314, and 25.166 billion m3, respectively). The trajectory of the center of gravity of agricultural water use, located at the intersection of Henan, Shaanxi, and Shanxi (110°E, 34°N), shows a trend of rapid northward movement (2001-2013) - slow northward movement (2013-2016) - rapid southward movement (2016-2020). This indicates that agricultural water use in some northern provinces has experienced a rapid increase followed by a more gradual trend. Based on trend analysis, agricultural water use shows a pattern of decrease (2001-2003) - increase (2003-2013) - decrease (2013-2020). During the increase phase, contributions were highest from provinces such as Xinjiang, Heilongjiang, and Jiangsu, with climate change and an expansion in irrigation area being the primary reasons for the increased agricultural water use in these provinces. In the decrease phase (2013-2020), multiple provinces made balanced contributions, with improved irrigation efficiency and the implementation of water-saving policies being the main reasons for the overall reduction in agricultural water use.
HS03-A015
Application of Satellite Imagery for Flood Management in Imjin River Within Border Area on the Korean Peninsula
Jin-gyeom KIM#+, Sungwha CHOI, Ki-mook KANG, Gibeom NAM, Eui-Ho HWANG
K-water Research Institute
The Imjin River, a representative transboundary river originating in North Korea and flowing into South Korea, is important for the regional hydrologic system in The Korean peninsula. With approximately 67% of its watershed located in North Korea, involved in the northern region significantly impacts Imjin River's water resources, affected by North Korea's water development initiatives. The operation of the Hwanggang Dam, positioned in the upper reaches of the Imjin River, introduces a risk of reducing water resources and flooding downstream. In the unique context of a divided nation where data sharing is unfeasible, the imperative for flood management through satellite technology becomes evident. This study used optical and radar satellite imagery to monitor the North Korean Hwanggang Dam and estimate water levels. Long-term water level data were required for calibrating hydrologic models and understanding the operational rules of the Hwanggang Dam. To estimate release from the Hwanggang Dam, a lumped rainfall-runoff model was designed and validated using observed data from the Gunnam Flood Control Reservoir, located downstream in South Korea. through this process, unauthorized discharges were proved in 2020 and during specific events, overextending simulation results. Additionally, in 2022, pre-release patterns preceding rainfall forecasts were observed, emphasizing the complexity of managing water resources in a divided geopolitical geography.
HS03-A011
Balancing Regional Freshwater Boundaries and Carbon Neutrality Goals in China’s Water-energy-environment Nexus
Jia Yi NG1#+, Xu ZHAO2, Hancheng DAI1
1Peking University, 2Shandong University
China faces challenging issues of water scarcity and climate change in this century. The Chinese government has committed to reaching carbon peak by 2030 and carbon neutrality by 2060 and has also deployed the Three Red Lines (TRLs) policy which aims to limit total annual water use to below 700km3 by 2030, with different targets for each province. Yet, these water guidelines fail to consider the local water endowment of each province and do not shed light on how current and future water use could put stress on our water resources. This gap could be filled by considering regional freshwater boundary (RFB) instead, which sets a limit for freshwater use based on monthly flow and corresponding environmental flow requirements. By comparing the TRLs targets with RFB, we could identify the gap between these policy-based goals and their practical implementation, and thus design specific regional economic strategies to achieve water targets in a carbon-neutral future. In this study, we first calculate RFBs for each Chinese province using a bottom-up approach by aggregating grid level (0.5°) RFB obtained from 15 different hydrological models to the provincial level. This is then used alongside the TRLs targets within a computable generable equilibrium (CGE) model. The CGE model evaluates the economic and environmental impacts of various scenarios considering carbon neutrality, water use targets, and solutions aimed at mitigating RFB exceedance, such as the South-to-North Water Diversion Project, water efficiency improvement and water reuse strategies. The holistic assessment of China’s climate and water policies reveals opportunities for coordinated policymaking among provinces and elucidates possible pathways for China to balance water, climate and economic goals.
HS03-A014
The Impact of Temporal Distribution of Rainfall on Peak Flood Discharge in the Rainfall-runoff Process
Byunghwa OH1+, Jongchun KIM2, Seok Hwan HWANG3#
1University of Science and Technology, 2Hajon Engineers & Consultants Co., Ltd., 3Korea Institute of Civil Engineering and Building Technology
Major factors influencing peak flood discharge in rainfall-runoff process typically include terrain characteristics, soil properties, watershed environments, and rainfall conditions. Among these, rainfall conditions are usually assessed using the concept of probability rainfall using frequent analysis based on return periods. Additionally, in practice, methods such as the Huff method, alternating blocking method, and Mononobe method are employed to synthesize the temporal distribution of rainfall. While there is considerable interest in the total amount of rainfall, studies on the impact of the temporal distribution of rainfall are relatively limited. In this context, we quantified how the temporal distribution of rainfall affects peak flood discharge in the rainfall-runoff process focusing on two variables: the relative temporal location of the rainfall peak and the concentration of rainfall amount. We repeatedly estimated the flood discharge using a rainfall-runoff model for 449 dimensionless time-rainfall distributions derived from both ground-observed rainfall and scenario-based reanalysis data. Our analysis reveals robust trends between peak flood discharge and the proposed two indicators for quantifying the temporal distribution of rainfall. The validity of our findings and the insights gained from this investigation will be presented. Acknowledgement: This research was supported by the National Research Foundation of Korea Grant funded by the Korean government (Ministry of Science and ICT), grant number NRF-2020R1A2C2014937.
HS03-A004
Study on Multiple Water Sources Joint Operation and Allocation Mode of the East Route of South-to-north Water Transfer Project in China Based on Simulation-optimization Model
Weifeng LIU#+
MWR General Institute of Water Conservancy Resources and Hydropower Planning and Design
The East Route of South-to-North Water Transfer Project is an important part of the national water network and a major strategic infrastructure to alleviate the severe shortage of water resources in the north of China. It has great theoretical and practical significance to choose a suitable scheduling mode for water supply to reduce the cost of water transfer in the East Route of South-to-North Water Transfer Project. A framework for water resources scheduling of the East Route of South-to-North Water Transfer Project is proposed in this study based on a simulation-optimization model, considering many factors such as the fairness of water use in the upstream and downstream of the water supply line and the left and right banks, and the efficiency of water resources utilization. Considering the current scheduling operation of the Eastern Route Project, we set up 3 different scenarios, one is to consider the current water source (Yangtze River, Hongze lake, Luoma lake and Xiaji lake) for the East Route of South-to-North Water Transfer Project, and optimize the water transfer route and water source to minimize the cost of water transfer; the second is to add the Shangji lake and Dongping lake to the current water source to optimize the optimal water transfer line and water source; the third is to further tap the water source of Hongze lake on the basis of the current water source, and optimize the optimal water transfer line and water source. The results show that, on the basis of guaranteeing the use of water resources by local users of the water source, the addition of the Shangji lake and Dongping lake and further tapping of the water source of Hongze lake can help to reduce the cost of water transfer of the East Route of South-to-North Water Transfer Project.
HS03-A010
Climate Change Impact Assessment on Water Resources Management in Eastern Asian Basins in South Korea
Bomi KIM1+, Garim LEE1, Dong Kook WOO2, Jihyeon JO2, Songhee LEE1, Seong Jin NOH1#
1Kumoh National Institute of Technology, 2Keimyung University
In this study, to analyze the impact of climate change on the water resource management of multipurpose dams, a combined rainfall-runoff and reservoir operation modeling was implemented under climate change scenarios. Then, the water supply reliability and flood risk indices were analyzed for two multipurpose dams in Korea, Hapcheon and Seomjingang Dam. By coupling the three concentrated rainfall-runoff models, GR4J, IHACRES, and TAU, and the reservoir operation models, the analysis considered projections under SSP2-4.5 and SSP5-8.5, projected by 12 global climate models. In comparison to SSP2-4.5, SSP5-8.5 showed greater variability among climate models, resulting in increased uncertainty in predictions for both drought and flood risk assessments. This variability was particularly pronounced in the far future (2081-2100). Dam-released flood volume was projected to increase by ~70% during 2081-2100 under SSP5-8.5 indicating a heightened flood risk due to climate change.
HS03-A009
Spatiotemporal Variability of Global Water Surface Extents Over the Past Three Decades
Young-Joo KWON1+, Ho Minh Tam NGUYEN1, Hyungjun KIM1,2#
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo
The water environment undergoes continual transformations over time, attributed to the combined influences of human activities on land and the effects of climate change. With the accumulation of satellite remote sensing data over an extended period, it has emerged as the optimal tool to monitor surface water, including rivers and lakes, discerning their spatial distributions and temporal changes. In particular, this study aims to estimate the variability of the water surface area of global reservoirs, leveraging products derived from satellite remote sensing. To assess changes in the global water surface extents over three decades, the Global Surface Water (GSW), a global Landsat-based product, was exploited. Here, we propose a methodology to generate a lake catalog by combining GSW's maximum water extent product with lake information from HydroLAKES, a global lake database. Subsequently, we estimated monthly time series of lake surface areas based on the monthly water extents from the GSW product. Our enhanced lake catalog boasts more than 20 % as many lakes as HydroLAKES by additionally incorporating smaller lakes. Simultaneously, we improved the catalog's accuracy by identifying and excluding misclassifications in HydroLAKES. This study will present validation results compared to the GRanD dataset and delineate long-term trends of global lake surface areas over 30 years. The product is anticipated to provide essential information for understanding long-term lake surface dynamics, which is crucial for water resource management, the global carbon cycle and freshwater aquatic ecosystems.
HS03-A002
Sand Mining in the Mekong Delta: Extent and Compounded Impacts
Edward PARK#+
Nanyang Technological University
Sand mining has accelerated in recent years primarily due to population increase and rapid urbanization. To meet demand, the rate of sand extraction often exceeds the rate of natural replenishment with serious environmental consequences. In this review paper, the Vietnamese Mekong Delta (VMD), a global hotspot for sand mining with a prolonged history of intensive riverbed extraction, is used as a representative case study to highlight the extent and compounded impacts of this activity. Sand mining budgets from literature present significant discrepancies, with estimates for the entire delta varying from around 8.5 to 42.2 Mm3/yr. These variances can be attributed to the challenges in the actual measurement of mining rates and the deployment of disparate methods across studies. Moreover, the widespread practice of illegal sand mining in the region further exacerbates the mismatch in budget calculations. Consequences of such mining activities manifest as deeply-incised riverbeds leading to riverbank and coastal erosion. Moreover, the massive sediment removal has resulted in river water level reductions, disrupted hydrological connectivity, and diminished floodplain inundation. The augmented backwater effect, a result of riverbed lowering, amplifies saltwater intrusion in dry seasons. While the physical and hydrological impacts have received attention, studies on the ecological and societal ramifications remain sparse. These impacts, further magnified by factors like upstream dams, irrigation infrastructures, excessive groundwater extraction, and sea-level rise (SLR), present a multifaceted challenge. This paper concludes by advocating for the adoption of remote sensing-based approaches for effective mapping of sand mining activities, and implementation of sustainable sand harvesting practices to balance developmental needs with environmental conservation.
Session Chair(s): Li-Pen WANG, National Taiwan University
HS11-A001
Basic Study on Three-dimensional Wind Field Estimation Using X-band Dual Polarized Phased Array Weather Radar
Shinya MABUCHI1#+, Kazuhiro YOSHIMI1, Syo YOSHIDA2
1Toyama Prefectural University, 2Meteorological Engineering Center
In recent years, water-related disasters caused by localized torrential rainfall have been increasing, especially in urban areas. However, predicting localized torrential rainfall is still difficult even with current technology. Phased array weather radar for high-speed, high-density observations may be able to prevent conventional disasters. Rainfall forecasting methods using phased-array weather has been proposed. But these methods have some problems. To solve these problems, we attempted to use the results of three-dimensional wind fields estimated from weather radar data for short-time rainfall prediction, such as localized torrential rainfall. As a basic study for this purpose, three-dimensional wind filed estimation were conducted using dual polarized phased array weather radar for high-density, high-speed observations. We confirmed the difference due to elevation angle density by performing the analysis at different elevation angle densities in this paper. And, we also confirmed the differences due to estimation method by performing the VVP method and the Dual Doppler analysis. The results showed that the higher elevation angle density resulted in less vertical wind. In the Dual Doppler analysis, it was found that the higher elevation angle density clearly showed the strength of the vertical wind. Comparing the results of the VVP method and the Dual Doppler analysis, it was found that the VVP method estimated downdraft, whereas the Dual Doppler analysis often estimated updraft. In addition, the estimated vertical wind by the Dual Doppler analysis showed less variation than estimated by the VVP method.
HS11-A002
Migration Activities Significantly Increase the Flood Exposure in Guangdong-Hong Kong-Macao Greater Bay Area: Identifying Sustainable Untapped Areas for Development and Migration
Kai FEI+, Haoxuan DU, Liang GAO#
University of Macau
The impact of migration activities on flood exposure remains unclear as the challenging in predicting migration patterns in urban development in economically vibrant coastal low-lying areas. Here, the flood-exposed migrants from 2000-2020 in Guangdong-Hongkong-Macao Greater Bay Area (GBA) are quantified, and the sustainable areas are assessed for development and migration. The migration activities increased the population by 33.95 million, yielding a ~75 – 84% increase in population exposure. The migrated population is more inclined to settle in non-floodplains than local residents. The proportion of flood exposure in GBA will still increase further by 2100. Finally, ~37 - 50% of non-built-up areas in GBA are assessed as the perfect fit for development and migration. Most areas are in the northern part of GBA, while the available spaces for some developed districts and cities are less than 20%.
HS11-A003
Incorporating Single-core Cell Lifecycle Evolution Into Object-based Convective Storm Nowcasting
Yun-Man HSU+, Li-Pen WANG#
National Taiwan University
Radar-based nowcasting plays a crucial role in meeting the urgent demand for short-term, high-intensity convective rainfall predictions. Given the dynamic and clustering nature of convective storms, object-based nowcasting has emerged as an effective approach, characterised by its ability to identify, track, and extrapolate their motion. These models excel in identifying rainfall objects in radar images and constructing their temporal associations. However, a critical limitation in many of existing methods lies in their lack of mechanism to incorporate the evolution of rain cell lifecycle into the nowcasting process. A recent study by Cheng et al. (2023) demonstrated the effectiveness of utilising convective core altitude – a property retrieved from three-dimensional radar data– to improve the prediction of the evolution of single-core convective cell lifecycle. Their results suggest that, compared to persistence nowcasts, the prediction errors in rainfall intensity can be reduced by 50% at 15-min forecast lead time. This research aims to enhance object-based nowcasting by developing methods to extend the cell evolution model proposed by Cheng et al. (2023) and to integrate it with an operational positional nowcasting model –a Kalman filter based object-based convective storm nowcasting model, recently co-developed by researchers from several international sectors and the UK Met Office (Wang et al., 2022). Based on the integration, probabilistic nowcasting will be undertaken to generate ensemble nowcasts that account for both positional and evolution variations. Ensemble members from each approach at each forecasting time step can constitute a convective storm ‘hazard’ map. We will indirectly evaluate the performance of two proposed approaches via assessing these hazard maps with radar observations.
HS11-A004
Examining the Temporal Scaling Characteristics of Extreme Rainfall: Analyzing Radar-derived Data for Probable Maximum Precipitation in South Korea
Soohyun KIM+, Dongkyun KIM#
Hongik University
This study examines the temporal scaling behavior of rainfall in South Korea using radar precipitation data. The radar data achieved a spatial resolution of 1km and a temporal resolution of 10 minutes from 2009 to 2018. The primary focus is on analyzing the correlation between maximum precipitation and duration, specifically the probable maximum precipitation(PMP). Employing the rolling sum method, 35 periods ranging from 10 minutes to 2 months were calculated. The study findings are summarized as follows:1) Radar-derived PMP values are notably higher than ground-based estimates, particularly in mountainous regions with sparse ground measurements;2) The relationship between PMP and duration deviates from the typical power-law distribution, driven by atypical short-term extreme rainfall events not adequately captured by ground-based networks;3) The power-law relationship is more pronounced for lower-quantile rainfall due to different rainfall generation mechanisms for lower-quantile rainfall;4) Analysis of extreme rainfall at random sampling locations reveals a strong dependence of the duration-maximum precipitation relationship on the density of the ground-gauge observation network;5) In shorter durations(10 minutes to 6 hours), the East Asian Rainy Season(EARS) exhibits more extreme rainfall than typhoons, while at longer durations, typhoons contribute more rainfall. This implies that the EARS and typhoons are linked to flooding in urban and riverine environments, respectively;6) the inclusion of Jeju Island in the analysis shows that typhoon events dominate PMPs for most durations. Given the anticipated increase in typhoon intensity and frequency near the Korean Peninsula due to climate change, along with a northward shift in their paths, the study underscores the necessity for effective flood defense measures and improvements in PMP assessments, particularly in the southern part of the peninsula.[This study was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT)(No.NRF-2021R1A2C2003471)].
HS11-A005
Evaluating and Validating Socio-economic Vulnerability in Seoul, South Korea
Chi VUONG TAI+, Dongkyun KIM#
Hongik University
The evaluation of vulnerability holds a pivotal role in mitigating disaster risks, attracting growing attention from researchers. Despite the common focus on spatial representation and analysis of vulnerability indices, there is a notable lack of efforts in vulnerability validation. In this study, the Principal Component Analysis (PCA) algorithm was applied to 38 socio-economic features, yielding 9 principal components to estimate the Socio-Economic Vulnerability Index (SEVI). Results revealed comparable vulnerability levels across various districts, validating well against the Subjective Expert-based Vulnerability Index. Internal validation, employing global uncertainty and sensitivity analyses through Monte Carlo simulations, scrutinized SEVI values and ranks. Findings exposed a correlation between higher vulnerability indices and increased bias in SEVI values, followed by an assessment of vulnerability uncertainty using SEVI ranks. A tornado diagram highlighted the significant explanation of the “number of families with only children and mother” feature, explaining 5% of SEVI variability. The proposed methodology is adaptable to regions with limited social and economic data. Based on results from the uncertainty test, we recommend that regions exhibiting minimal bias in SEVI values or ranks are reliable foundations for devising disaster risk mitigation strategies; conversely, other areas demand additional scrutiny. Furthermore, the outcomes of the sensitivity test offer valuable backing for prospective research endeavors in the selection of input features for socio-economic vulnerability assessments. Acknowledgements: This study was supported by: (1) The National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. NRF-2021R1A2C2003471) (50 % grant); (2) Korea Environment Industry & Technology Institute (KEITI) through R&D Program for Innovative Flood Protection Technologies against Climate Crisis Project, funded by Korea Ministry of Environment (MOE) (RS-2023-00218873) (50 % grant).
HS11-A006
High Temporal Resolution Distributed Rainfall-runoff Modeling with Hybrid CNN-LSTM in Ungauged Basins
Jeonghun LEE+, Dongkyun KIM#
Hongik University
This study proposes a new deep learning model to forecast 10-minute flow in ungauged watersheds using a spatially distributed CNN-LSTM network. The model effectively combines spatial and temporal information by integrating the strengths of convolutional neural networks (CNN), which excel at grasping spatial information, and long short-term memory (LSTM), which specializes in learning temporal relationships. The training dataset included 7 years (2012-2018) of 10-minute radar-gauge composite precipitation, temperature, elevation, and vegetation cover (NDVI) data with a 1-km resolution. To evaluate the performance of the model, it was applied to several ungauged watersheds located in diverse geographical areas within the Republic of Korea. The results showed that the proposed CNN-LSTM model surpassed the traditional LSTM model in terms of accuracy, highlighting the potential applications of this model in ungauged watershed hydrological modeling. Additionally, an analysis confirmed that the model accurately simulates the soil moisture-dependent runoff mechanism, which plays a crucial role in continuous hydrological modeling. * Acknowledgement: This study was supported by: (1) The National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. NRF-2021R1A2C2003471) (50 % grant); (2) Korea Environment Industry & Technology Institute (KEITI) through R&D Program for Innovative Flood Protection Technologies against Climate Crisis Project, funded by Korea Ministry of Environment (MOE) (RS-2023-00218873) (50 % grant).
HS11-A008
Enhancing Urban Flood Forecasting Accuracy: A Deep Learning-based Nowcasting Approach with Grid-specific Weighting
Hyojeong CHOI#+, Dongkyun KIM
Hongik University
Recent climate change has led to an increased risk of urban flooding due to extreme weather events, necessitating the development of high-resolution real-time precipitation forecasting models. However, existing data-based precipitation prediction models tend to underestimate the magnitude of extreme precipitation events. To address this issue, this study proposes the introduction of data-size-specific weights into the loss function of deep learning-based models. The study involves analyzing the probability density function (PDF) of precipitation events during the model's training period and applying various weighting functions (such as exponential, logarithmic, stair, sigmoid, cumulative distribution function - CDF) to compare and analyze the sectional performance of the model. The average Nash-Sutcliffe efficiency (NSE) and Root mean square error (RMSE) throughout the testing period were highest at 0.66 and 0.12, respectively, in the cumulative distribution weighting function. Moreover, the Critical success index (CSI) showed improved performance with the CDF weighting function at 0.62 for Threshold=0.1, while the logarithmic weighting function excelled at 0.27 for Threshold=5. These results demonstrate the impact of applying different types of weights to each section on the prediction performance. Acknowledgements: This study was supported by: (1) The National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. NRF-2021R1A2C2003471) (50 % grant); (2) Korea Environment Industry & Technology Institute (KEITI) through R&D Program for Innovative Flood Protection Technologies against Climate Crisis Project, funded by Korea Ministry of Environment (MOE) (RS-2023-00218873) (50 % grant).
HS11-A009
Outlier Correction for Enhancing Radar Rainfall Data: Iterative Localized Algorithm in Spatiotemporal Analysis
Yongchan KIM+, Dongkyun KIM#
Hongik University
Correcting outliers in radar rainfall data is essential in important applications such as analysis of extreme rainfall events, hydrological modeling, and prediction of flash floods. Despite its importance, existing methods for correcting outliers in radar data have limitations in effectively handling sporadic outliers due to the high-dimensionality and complex spatiotemporal characteristics of radar data. In response, this study developed a new approach that detects and corrects outliers based on local spatiotemporal scale radar rainfall statistics. In this approach, an outlier detection algorithm based on the simple 3-sigma rule in the spatiotemporal context and an algorithm that detects rapid changes between adjacent radar cells in a spatial context are repeated on a local scale to effectively improve the quality of radar rainfall data. The correction of outliers made the distribution of radar rainfall data similar to that of rain gauge data, and overall accuracy has been significantly improved. This proposed method not only utilizes 2D radar reflectivity data for outstanding practicality but also can contribute to improving the accuracy of analysis in various fields using radar rainfall data. Acknowledgements: This study was supported by: (1) The National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. NRF-2021R1A2C2003471) (50 % grant); (2) Korea Environment Industry & Technology Institute (KEITI) through R&D Program for Innovative Flood Protection Technologies against Climate Crisis Project, funded by Korea Ministry of Environment (MOE) (RS-2023-00218873) (50 % grant).
HS11-A011
Impact Assessment of Spatial Resolution on Urban Pluvial Flood Modeling
Hyeonjin CHOI1+, Jun Hak LEE2, Seungsoo LEE3, Bomi KIM1, Seong Jin NOH1#
1Kumoh National Institute of Technology, 2University of Oregon, 3Korea Environment Institute
Finding appropriate spatial resolution is crucial for accurate urban pluvial flood predictions and proper decision-making to mitigate damages from extreme events. Higher resolution modeling with more fidelity usually requires expensive computation resources, while lower resolution one may distort physical reality. The objective of this study is to assess the impact of spatial resolution on urban pluvial flood modeling. To achieve this, we use the physically-based urban flood model H12 to simulate various urban pluvial flood scenarios with spatial resolutions ranging from 1 to 50 meters in the western region of Portland, OR, USA. A comparative analysis is implemented to examine the sources of error in urban flood modeling by varying spatial resolutions and considering maximum variables and time variables, such as flood depth and volume. The uncertainties due to the spatial resolution of urban pluvial flood modeling are also evaluated from various perspectives, including multi-directional flow path analysis and the computational efficiency of hybrid parallel computing.
Session Chair(s): Jonghun KAM, Pohang University of Science and Technology, Wentao LI, Hohai University
HS10-A010
Contributions of Land Initialization and Subseasonal Rainfall Forecasts to River Water Availability Forecasts in Southeast Asia
Eunjee LEE1,2#+, Randal KOSTER2, Mauricio ARIAS3, Sophea Rom PHY3, Yuna LIM1,2, Jana KOLASSA4,2, Yujin ZENG1,2, Thanh DANG5, Miguel LAVERDE6, Fabio FARINOSI7
1University of Maryland, Baltimore County, 2NASA Goddard Space Flight Center, 3University of South Florida, 4Science Systems and Applications, Inc., 5National Institute of Water and Atmospheric Research, 6Asian Disaster Preparedness Center, 7European Union
Forecasts of water availability in river basins do not yet take full advantage of the information contained in subseasonal-to-seasonal (S2S) meteorological forecasts – information with the potential to improve water managers’ planning capability for periods extending beyond the timescale of the traditional weather forecast. This work examines the impact of subseasonal forecast meteorology on the prediction skill of subseasonal streamflow at fifteen gauges in the Mekong River basin and two other basins in Myanmar. We examined streamflow forecasts starting on January 1, April 1, July 1, and October 1 during each year of the 2001-2020 period; these retrospective forecasts utilized an offline land model driven with bias-corrected forecast meteorology from NASA’s GEOS S2S meteorological forecast system. Using gauge measurements for validation, we find reasonably high skill for the first forecast month (~30 days), particularly at the wet season and the dry season. We further examined the predictive skill by conducting two supplemental ensemble experiments: (1) applying the 20-year climatological forecast rainfall but utilizing our best model estimate of the land’s initial state (e.g., soil moisture) at each year, or (2) allowing the forecast rainfall to vary at each year but using a fixed initial condition of land at the start date. Our result indicates that the realistic land initialization explains most of the skill obtained with our offline system at the majority of the selected locations. Contribution from the subseasonal rainfall forecasts varies by season and region and can sometimes even offset the positive impact of the land initialization when the rainfall forecast skill is low, particularly during the transitional periods between dry and wet seasons. The subseasonal water forecasts for Southeast Asia can be further improved by considering river routing and reservoir operations, elements that are currently being integrated into our subseasonal water availability forecast system.
HS10-A003
Did Extreme Forcing Help or Hinder Extensive East Asia Spring Droughts?
Jonghun KAM#+, Byeong-Hee KIM
Pohang University of Science and Technology
In recent decades, pluvials and droughts have been more frequent and severe in East Asia (EA), especially in springtime. A skillful prediction skill of climate forecast models is warranted for EA pluvial and drought mitigation. In the last 30 years, EA experienced extreme spring pluvial and drought events in 1998 and 2011 when the ENSO signal was strong. In this study, we evaluate the predictability of three coupled general circulation models (CGCMs) and three atmospheric general circulation models (AGCMs) for the 1998 pluvial and 2011 drought. To ascertain the predictability source, three ensemble members of each model are grouped into high- and low-performance groups based on the predictive performance, and their composite anomalies are compared. Despite robust and similar prediction skills for the 1998 and 2011 ENSO events, CGCMs exhibit higher predictability for the 1998 pluvial compared to the 2011 drought. This asymmetry is attributed to the prediction skills of the upper-level atmospheric circulation pattern in the corresponding year. In AGCM experiments, this study found that the perfect prediction skill of SSTs is beneficial for the improvement of the predictability of EA springtime pluvials but still no improvement of EA springtime droughts. This study highlights a dominant role of random atmospheric noise, not extreme SST forcing, in the predictability of CGCMs for EA springtime precipitation extremes. However, the intercomparion results with AGCMs suggest that the improved predictability of the North Atlantic and Pacific Oceans can lead to a more skillful prediction of large-scale circulations and near-surface temperature over Eurasia and thus 1998-like pluvial in East Asia, but not 2011-like droughts. This study emphasizes the need to better understand potential predictability sources of EA springtime droughts to achieve the robust prediction of EA hydroclimatic extremes.
HS10-A005
Ensemble Hydrological Forecasting Using X-band Weather Radar for Pluvial Flood in Chinese Mega City
Dehua ZHU1#+, Yunqing XUAN2
1Nanjing University of Information Science & Technology, 2Swansea University Bay Campus
This two-year trial aims to bring together academics and industrial partners from UK and China to conduct a pilot study on the use of the active phased array radar to provide early urban flood warnings for Chinese mega cities, which facing challenging urban flood issues. This is the first in the world of cascade modelling using the cutting-edge active phase array radar (APRA) to provide rainfall monitoring and nowcasting information for a real-time two-dimension urban drainage model. The collaboration built up by this project and the first-hand experiment data will serve well to further catalyse the taking-up of state-of-the-art weather radars for urban flood risk management, and to tackle the innovation in tuning the radar technology to fit the complex urban environment as well as advanced modelling facilities that are designed to link the observations, providing decision making support to the city government. Recommendations for applying high spatial-temporal resolution precipitation data to real-time flood forecasting on an urban catchment are provided and suggestions for further investigation are discussed.
HS10-A001
Bias Correction of CMIP6 Ensemble Precipitation Predictions with Deep Learning Techniques
Zhu LIU#+, Bohan HUANG, Qingyun DUAN
Hohai University
Climate change is expected to alter the magnitude and spatiotemporal patterns of hydro-climate variables such as precipitation, which has significant impacts on the ecosystem, human societies and water security. Due to imperfect model structures, parameters and boundary conditions, direct model outputs are subject to large uncertainty, which needs serious evaluation and bias correction before usage. In this study, seasonal precipitation predictions from 30 Coupled Model Inter-comparison Project Phase 6 (CMIP6) models and Climate Research Unit (CRU) observations are used to evaluate historical precipitation climatology in global continents during 1901-2014. A grid based model heterogeneity oriented Convolutional Neural Network (CNN) is proposed to correct the ensemble mean precipitation bias ratio. Besides, regression based Linear Scaling (LS), distribution based Quantile Mapping (QM) and spatial correlation CNN bias correction approaches are employed for comparison. Results of model performance evaluation indicate that generally precipitation prediction is more reliable in JJA than DJF on the global scale. Most models tend to have larger bias ratio for extreme precipitation. Moreover, the proposed grid based model heterogeneity oriented CNN has better performance in ensemble mean bias correction than LS, QM and spatial correlation CNN, which could consider the relative model performance and capture the features similar to actual climate dynamics.
HS10-A011
Deep Learning-based Post-processing of Short-term Precipitation and Streamflow Forecasts
Wentao LI+, Qingyun DUAN#
Hohai University
Raw hydrometeorological forecasts from numerical weather prediction (NWP) or hydrological models may suffer from systematic bias and cannot be directly used. Statistical post-processing methods can be used to correct these biases and quantify forecast uncertainty, which is important for applications such as risk-based decision. Deep learning-based methods can make good use of multi-scale spatio-temporal information to improve forecast accuracy. In this research, we developed convolutional neural network-based post-processing methods to make full use of multiple spatial scale information in raw precipitation forecasts to improve forecast accuracy. Moreover, we apply long short-term memory (LSTM)-based methods to post-processing the streamflow forecasts and quantify the uncertainty. The preliminary results show that deep learning-based post-processing methods can improve raw hydrometeorological forecasts by utilization of multi-scale predictors and modeling the nonlinear relationship between predictors and predictands to improve the forecast accuracy. The post-processed forecasts are evaluated in both deterministic and probabilistic verification metrics such as continuous ranked probability skill score (CRPSS), probability integral transform (PIT) histogram and relative operating characteristic (ROC) curve. The benefits of using deep learning-based methods relative to traditional post-processing methods will also be discussed.
HS10-A012
Enhanced Tropical Cyclone Inflow Flood Forecasts by Using Deep Learning and Spatial‑temporal Information
Liu LI#+, Yue-Ping XU, Yuxue GUO
Zhejiang University
Reliable Tropical Cyclone (TC) precipitation and flood nowcasting play an important role in disaster prevention and mitigation. Especially for small-scale reservoirs, timely and accurate inflow forecasts are required to provide safe space for capturing high flows without having to resort to hazardous and damaging releases. Numerous studies have investigated the ability of deep learning in TC precipitation nowcasts. However, few of them focus on the skill of deep-learned TC precipitation forecasts in inflow flood forecasts. In this study, a novel framework is developed by introducing TC track information together with antecedent precipitation in the Convolution LSTM model (PTC-ConvLSTM). The ConvLSTM forecast precipitation is then input to an event-based Xinanjiang hydrological model for inflow flood forecasting, and the propagation of errors from TC track forecasts to inflow forecasts is further analyzed. The results show that TC track information enables a further 5% improvement compared to outputs from ConvLSTM with only precipitation information. PTC-ConvLSTM precipitation nowcasts present a probability of detection (POD) greater than 0.34 for a threshold of 5mm/h in a lead time of 6h. The nowcasts-driven flood forecasts have an NSE greater than 0 with a lead time of 5h at least. It is also indicated that the 100km error in TC track forecasts could generally result in 10% degradation in precipitation forecasts and a further 8% deterioration in the driven flood forecasts. The effectiveness of our model indicates that the precipitation nowcasts from deep learning have strong applicability in disaster mitigation.
HS10-A014
Understanding Nonlinear Dynamics and Chaos in Meteorological Parameters for Improved Rainfall Forecasts
Priya SHEJULE#+, Sreeja PEKKAT
Indian Institute of Technology Guwahati
A comprehensive analysis of the non-linear dynamics governing meteorological parameters is one of the primary requirements for making informed rainfall forecasts necessary for water resource sectors, and disaster preparedness. Earlier, hydrological processes have been regarded as stochastic phenomena. Nevertheless, recent findings have demonstrated that any time series might exhibit chaotic components along with the stochastic component. In the present study, attempt has been made to identify the non-linear trends within meteorological parameters such as rainfall, temperature, surface pressure, relative humidity, wind speed and mean sea level pressure, along with the identification and quantification of chaos present in these parameters. To extract nonlinear trends present in the meteorological time series, empirical mode decomposition (EMD) method was applied. We also applied Hurst exponent and the Lyapunov exponent as a chaos quantifier when trend and periodicity exists in the meteorological data. The hourly meteorological parameters were collected over a period of 2015–2019 for the Aizawl city in Mizoram, India. Our study shows that EMD successfully decompose and extracts trends in the meteorological series. The hourly meteorological parameters such as rainfall, wind speed, mean sea level pressure and surface pressure were found to be chaotic at 5% significance level. However, the negative Lyapunov exponent was found in case of temperature and relative humidity indicating the absence of chaos. The results obtained gives deeper understanding of meteorological parameters, providing necessary information for development of rainfall forecast model.
HS10-A013
Photosynthetic Response and Resilience in Pan-tropical Terrestrial Ecosystems: Insights from the Coupled Carbon-water-energy Cycle
Eun Han GOO1#+, Hyungjun KIM1,2
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo
Tropical terrestrial ecosystems play a critical role in global energy, water, and carbon cycles. However, the spatiotemporal variability of the coupling strength between photosynthetic activities and regional hydroclimate changes has not been comprehensively discussed. In this study, we use global satellite observations to investigate how tropical terrestrial ecosystems respond to water and radiation forcing anomalies. To monitor water availability, radiation intensity, and vegetation photosynthetic activity, Gravity Recovery And Climate Experiment (GRACE) terrestrial water storage, Clouds and the Earth’s Radiant Energy System (CERES) downward shortwave radiation at the surface, and long-term harmonized solar-induced chlorophyll fluorescence observations were used, respectively. The findings suggest that we can separate the vegetation photosynthetic response based on the coupling strength. Additionally, different vegetation types show distinct patterns under various water and energy driven conditions. Furthermore, we calculate the resilience of terrestrial ecosystems based on the relationship in inter-annual variability of photosynthesis and hydroclimate. Wet tropical forests located in the low latitudinal area including Amazon basin, Congo basin, and Indonesia exhibit positive correlation to radiation while negatively correlated to TWS. Photosynthesis negatively couples to water availability because of cloud cover, which follows TWS and precipitation increase suppress available radiation amount for ecosystems. These regions have mean annual precipitation over 2,000 mm, holding high productivity throughout the year. On the other hand, semi-arid grassland areas or savanna distributed in Eastern Amazon, Southern Africa, and Australia show different response pattern. Photosynthesis negatively couples to radiation availability because of surface temperature, which follows radiation increase, makes stomata close and suppress the ecosystems photosynthesis. The climate has a long dry season throughout the year in these regions. The suggested framework allows identifying the spatiotemporal change in recovery rate of the system against the external perturbations or the vulnerability of tropical forests to the extreme climate conditions such as droughts.
Session Chair(s): Yiping WU, Central South University of Forestry and Technology
HS08-A005
Large-scale Vegetation Response and Feedback to Terrestrial Water Storage Variation
Huade GUAN#+
Flinders University
Terrestrial vegetation requires water to survive and grow. Precipitation is often used as a proxy for assessing the influence of soil water availability on vegetation cover at the regional and continental scales, together with other climatic factors (temperature and solar radiation). Soil moisture of the top couple of meters, if available, would provide more direct information for investigating vegetation’s response and feedback to soil water variations. The terrestrial water storage (TWS) data derived from GRACE satellites provide opportunities for such investigation at large scales, as seen in several studies published recently. In this presentation, I will review these studies globally, with a focus on those about the TWS-vegetation interactions on the Australian continent.
HS08-A006
Response of Tropical Savannas to Variation in Soil Moisture in the North Australian Tropical Transect (NATT)
Shielo MUTA#+
University of Technology Sydney
Vegetative responses to low water availability had been investigated for long but the question on how different plant ecosystems adapt to varying levels of soil water is still not fully understood. Australia’s variable climate is contributing and shaping its unique landscapes and ecosystems. The Australian savanna landscapes are a region of mixed grasslands and scattered trees dominated by eucalyptus trees, acacias, and other drought resistant species. However, due to extremes in wetting and drying in the region, increasing water stress can threaten even the most drought tolerant species. Water stress is a limiting factor affecting the growth and productivity of plant ecosystems. We evaluated the sensitivity of the tropical vegetation growth dynamics across the water availability gradient in the North Australian Tropical Transect (NATT) using SMAP soil moisture, MODIS Enhanced Vegetation Index (EVI) and SMAP Gross Primary Productivity (GPP). Average soil moisture use efficiency shows strong relationship with EVI and GPP where increasing sensitivity to soil moisture availability was observed as the area becomes (more and more) water limited. Soil moisture and EVI show strong linear correlation (r=0.84) using the datasets from 16 sites along the transect from 2015-2022. Higher correlation with GPP and soil moisture are observed (r=0.92) among all sites. EVI and GPP are most sensitive to soil moisture in the driest sites. The strong linear correlation of GPP and EVI with soil moisture reflects how ecological systems can be impacted by water Our study also highlights how growth, and productivity are affected by extremes in soil moisture availability.
HS08-A004
Coupling Hydrological and Hydrodynamic Models for Dissolved Oxygen in a Dense Macrophyte Catchment
Thanh DANG#+, Sandy ELLIOTT, Linh HOANG
National Institute of Water and Atmospheric Research
Dissolved Oxygen (DO) plays a crucial role in sustaining aquatic life, particularly fish, and is a key indicator of water quality. Fluctuations in DO levels can significantly impact biological activities, potentially leading to a decline in aquatic populations, underscoring the importance of monitoring and modelling DO. This study focuses on the typical dairy farming (Toenepi) catchment (17 km2) in Waikato, New Zealand, employing two calibrated physics-based models: a SWAT hydrological model coupled with a one-dimensional hydrodynamic-ecological MIKE Ecolab model. River systems in this region often act as a sink for waste generated by agricultural, industrial, and residential activities, providing a nutrient-rich environment for the growth of macrophytes. The objective is to simulate variations in DO concentrations in this catchment, which has a high density of in-stream macrophytes. The findings of the study reveal several key insights. Firstly, within a dense macrophyte system, solar radiation and water temperature emerge as pivotal factors influencing DO levels. Solar radiation initiates production processes, resulting in an increase in DO, while elevated water temperatures contribute to a reduction in saturated DO within the water column. Secondly, the study highlights that, due to the dominance of oxygen production and reoxygenation over oxygen consumption (i.e., respiration and mineralization), DO concentrations exhibit an upward trend from upstream to downstream locations. Lastly, the research indicates that heightened nutrient levels, specifically nitrogen and phosphorus, may foster increased production, leading to higher DO concentrations during daytime hours and oxygen depletion overnight. This study provides valuable scientific support for stakeholders involved in the management of macrophytes within river systems.
Session Chair(s): Zhi LI, Northwest A&F University, Sung-Wook JEEN, Jeonbuk National University
HS36-A015
| Invited
Identifying Hydraulic Connectivity Among the Vadose Zone, Unconfined and Confined Aquifers in the Thick Loess Deposits Using Multiple Tracers
Wanzhou WANG, Zhi LI#+
Northwest A&F University
Low water flux and a thick vadose zone increase the likelihood that water bearing units are hydraulically disconnected in shallow groundwater systems. Particularly for the thick loess deposit of China, hydraulic connectivity among the vadose zone, unconfined and confined aquifers is still unclear since it is controversial whether the unconfined groundwater is recharged by precipitation or confined groundwater. Taking several loess tablelands as example, we collected precipitation, soil water, unconfined and confined groundwater to measure the contents of multiple tracers (e.g., hydrochemistry, δD, δ18Owater, δ17Owater, δ34S, δ18Osulfate, δ13C and 14C) to evaluate hydraulic connectivity among the vadose zone, unconfined and confined aquifers. Deep soil water can be recharged by precipitation with intensities ≥ 30−40 mm/day, and then vertically discharge to unconfined water primarily through matrix flow with an infiltration velocity of 0.15 m/year. Matrix flow dominates the water flux from the vadose zone to the unconfined aquifer with the rates of 85.4 ± 39.6 mm/year, reflecting the regional hydraulic equilibrium. The unconfined and confined aquifers exhibit negligible vertical hydraulic connectivity because of different recharge periods, flow patterns, water−rock interaction, water residence time and sulfate evolution behaviors. The identified connectivity supports local precipitation as the recharge source, which conflicts with the external source hypothesis. The utilization of multiple tracers in this study can complement each other to provide more comprehensive results, and the results greatly improve the conceptualization of vertical water exchange processes in the loess deposits.
HS36-A016
| Invited
The Role of Groundwater in Antarctic Lake Systems: A Perspective of Climate Change and Water Cycle
Sung-Wook JEEN#+, Soyeon LIM
Jeonbuk National University
In recent years, the role of groundwater has gained attention in the changes of the water cycle in the polar region, primarily driven by climate change. However, determining the recharge amount of groundwater in the active layer, which serves as a shallow aquifer in the polar region, is challenging. The variability in the depth of the active layer, storage amount of groundwater, and flow characteristics have rarely been studied compared to surface water and glaciers in the polar region. In this regard, this study evaluated the flow characteristics around two different lake systems near King George Island in Antarctica (named "Lake A" and "Lake B"), with a focus on groundwater. Groundwater flux was measured using seepage meters installed in lake bottoms, and hydraulic head differences were measured using piezometers installed within and around the lakes. The results indicated that Lake A was mostly a losing system, with dynamic groundwater-surface water interaction. However, the measured groundwater flux did not directly correlate with lake level changes, possibly due to the rapid response of the lake level to new precipitation and snow meltwater quickly contributing to the lake. This might also be related to changes in the thickness of the active layer. In contrast, Lake B showed consistent lake levels and size with corresponding groundwater influx, indicating a stable lake system. This aligns with the presence of a stable ecosystem with various lichens and moss species around Lake B, unlike Lake A. Therefore, it is suggested that groundwater, along with snow melting, plays a significant role in maintaining ecosystems in the Antarctic region. The approach used in this study can be valuable for evaluating the groundwater component's contribution in Antarctic lakes and understanding the role of groundwater in inland water ecosystems of Antarctica.
HS36-A018
| Invited
Efficient Utilization and Optimal Allocation of Agricultural Water Resources in the Yellow River Basin
Ying ZHAO#+
Ludong University
Water resources are basic natural resources and strategic economic resources. Under the joint influence of climate change and human activities, the efficient use and optimal allocation of water resources are of great significance to implementing the national primary strategy of "ecological protection and high-quality development in the Yellow River Basin". This paper focuses on the major scientific issues of limiting the efficient use and sustainable development of farmland water in the Yellow River Basin, adhering to the research idea of systematic hydrology in the whole basin (e.g., linkages from upper to downstream) and all-encompassing approach to food, focusing on the theory and technology of optimal allocation of water resources in the process of high-quality agricultural development. The improvement of water use efficiency, the optimal allocation of agricultural and ecological water distribution, the collaborative optimization of the water-food ecosystem, and the construction of farmland big data and information systems are discussed, and the challenges faced and countermeasures are pointed out. Our results will help to improve agricultural water saving in the whole basin, water resource allocation capabilities, and make suggestions for ecological protection and high-quality development in the Yellow River Basin.
HS36-A009
Gaining Insight Into the Reciprocal Relationship Between Climate Change-induced Effects on Plant Processes and Soil Water Dynamics
Sruthi SURENDRAN#+, Deepak JAISWAL
Indian Institute of Technology Palakkad
Plants, soil, and climate are intrinsically inter-related components of the ecosystem. Climate change affects not only plant physiology but also vadose zone soil processes. Stomatal conductance, photosynthesis, root growth, and other plant physiological activities are affected by climate conditions such increased temperatures, CO2 concentrations, and precipitation patterns. These changes affect soil-plant interactions such root water uptake, transpiration etc., which in turn affects soil water dynamics. Hence it is essential to evaluate implications of these climate-induced alterations on soil water dynamics and plant processes. We use a mechanistic plant growth model BioCro and a comprehensive model HYDRUS 1D to simulate plant growth and soil water transport respectively. BioCro simulates above-ground processes like light interception, photosynthesis, biomass partitioning, and transpiration at the leaf scale, scaling them up to field and canopy scales. However, soil water dynamics in BioCro is simulated using a simple approach and leaves much room for model improvement by integrating above and below-ground processes. On the other hand, HYDRUS 1D, a well-known model to simulate one-dimensional water transport in unsaturated porous media makes use of a simple statistical representation of roots, crop height, and Leaf Area Index (LAI) to simulate the effect of vegetation on soil water dynamics. Here, we investigate the effects of dynamic plant representation in HYDRUS 1D by incorporating BioCro results. We also incorporate HYDRUS 1D’s soil water simulation findings onto BioCro to determine how modifying soil water dynamics affects BioCro’s crop yield predictions. This approach exchanges input/output data between models. This paper also examines the future of coupling HYDRUS 1D and BioCro, demonstrating their usefulness and benefits. The combination of these models could help in improving climate change impact assessment on vegetation and water resources. By merging BioCro with HYDRUS 1D, researchers may better understand climatic, plant, and soil dynamics and make agricultural decisions.
HS36-A013
Multiple Isotopes Reveal the Impact of Land Use Change on Water-nitrate Coupling Processes in Deep Loess Deposits
Wangjia JI1#+, Yidi LIU1, Gurpal S. TOOR2, Zhi LI1
1Northwest A&F University, 2University of Maryland
Understanding the relationship between soil water and nitrate is critical to agricultural production and aquifer vulnerability assessments, especially in regions with intensive agricultural activities and thick unsaturated zones. As such, we sampled cultivated farmland and orchards with varying ages of apple and peach trees in the loess deposits to >15 m depth to measure the contents and isotopes of water and nitrate in soils. The water isotopes were used to analyze water movement, while the nitrate isotopes were further employed for nitrate source and transformation analysis. The conversion from farmland to orchards resulted in large water deficit because of root water uptake, but the high nitrate-nitrogen accumulation was mainly observed within 0–5 m under old apple orchards due to the overuse of chemical fertilizer. The water isotopes suggested that piston flow dominated water movement and nitrate transport in deep soils. Despite the recharge effect of precipitation and low surface evaporation, the strong transpiration effects resulted in no water fluxes in deep layers under old apple orchards. Further, the nitrate isotopes indicated that nitrate reservoirs were mainly contributed by soil organic nitrogen (44% ± 26%) and ammonium nitrogen fertilizer (36% ± 20%), but their transformation was dominated by nitrification under old apple orchards and by mineralization in deep layers. The nitrate fluxes suggested that the risks of nitrate bombs were temporarily weakened by lower dried soil layers under old apple orchards, but the limited denitrification potential make nitrate reach the aquifers in a few hundred years or more. This study provides new insights for hydrological and biogeochemical cycles in deep soils, and the dried soil layers and nitrate bombs under old apple orchards should be carefully considered for the sustainable development of terrestrial ecosystems and water resources in arid regions.
HS36-A003
Groundwater Recharge Prediction in Relation to Climate Change: Case of a Watershed in Korea
Sul-Min YUN1+, Il Moon CHUNG1, Sun Woo CHANG1, Se-Yeong HAMM2#
1Korea Institute of Civil Engineering and Building Technology, 2Pusan National University
Groundwater recharge rate is an important factor in groundwater assessment and development. Groundwater recharge rate in the Nakdong River basin in Korea until 2050s was predicted by using a multi-layer perceptron (MLP) and climate change scenarios. Input data consisted of changeable data (precipitation and landuse cover) and fixed data (drainage pattern by soil distribution, hydrogeology, river boundary, surface impervious rate, DEM, and land surface slope). The land use change until 2050s was predicted by using MOLUSCE plugin. An increasing tendency is anticipated in both urbanized area and forest area and a decreasing tendency in agricultural area, grassland, and bare field. Precipitation was used from the RCP 4.5 and RCP 8.5 climate change scenarios provided by the Korea Meteorological Administration. Spatially, the groundwater recharge rate in the study area showed high values in the eastern coastal area and relatively low values in the inland area. Because of its positive relationship with precipitation, the average groundwater recharge rate in the upper Nakdong River basin was lower than that in the lower Nakdong River basin. Learning using nine input data and one output (groundwater recharge rate) in the 2010s resulted in the correlation coefficient of 0.81 between water budget analysis and the MLP model. In the next step, the groundwater recharge rates were predicted in 2030s, 2040s, and 2050s, by inputting the land-use map in 2030s ̶ 2050s and the precipitation of 2030s ̶ 2050s based on the RCP 4.5 and RCP 8.5 scenarios into the MLP model. The groundwater recharge rates by using the RCP 4.5 scenario and RCP 8.5 scenario were 9.7-20.1% (an average of 14.7%) and 9.5-18.8% (an average of 13.9%) in 2025, respectively. Acknowledgement: This study was financially supported by the KICT Research Program (project no. 20230166-001, Development of Coastal Groundwater Management Solution) and the National Research Foundation of Korea (NRF) grants 2020R1A2B5B02002198 funded by the Ministry of Science and ICT.
HS36-A006
Analytical Assessment of Available Freshwater Resources in Coastal Aquifers with a General-head Inland Boundary Amidst Sea Level Rise
Wenyu XU1+, Bo FAN2, Jiazhi SUN1, Chunhui LU1#
1Hohai University, 2Ministry of Water Resources
Coastal Asian cities, featuring high population densities and social patterns of seaward migration due to abundant natural resources and convenient transportation, are facing the challenge of heightened seawater intrusion due to sea level rise (SLR) and increased freshwater demand. Traditional studies of seawater intrusion caused by SLR have been thoroughly examined for inland as constant-head (Dirichlet) and constant-flow (Neumann) boundaries, demonstrating the significant effect of inland boundaries on groundwater dynamics. However, these boundaries do not adequately account for the hydraulic connection between the modeling domain and the external region, nor the effects of freshwater extraction on the boundaries, potentially leading to inaccurate estimates of seawater intrusion and available groundwater. The general-head boundary (GHB), which frequently represents a natural inland boundary, may adequately characterize the hydraulic response of model boundaries while also minimizing model size and conserving head and flow accuracy at boundaries. This study introduces analytical solutions derived from Fourier transform and potential theory to examine seawater intrusion and determine the maximum sustainable pumping rate in both confined and unconfined aquifers with an inland GHB condition. A novel approach for analytically establishing the GHB boundary, characterizing a linear Robin boundary in confined aquifer and a nonlinear Type III boundary in unconfined aquifer, is provided. To validate the analytical method, three-dimensional SEAWAT numerical models were established, and an empirical coefficient correction approach was employed. This research evaluates how inland and seaside boundaries affect seawater intrusion processes. The proposed analytical model and its conclusions can be used to evaluate fresh groundwater resources efficiently in the context of SLR and complex boundary conditions.
Session Chair(s): Petrus (Peter) VAN OEVELEN, George Mason University, Yaoming MA, Chinese Academy of Sciences
HS05-A001
Comprehensive Study of the Land-atmosphere Interaction Over the Tibetan Plateau
Yaoming MA#, Weiqiang MA+
Chinese Academy of Sciences
The Tibetan Plateau (TP) has significant thermodynamic effects for regional climate change, where understanding land-atmosphere interaction process (LAIP) is an important prerequisite. However, estimation of the exact spatiotemporal variability of the LAIP over heterogeneous landscape of the TP remains a big challenge for scientific community. Focused on the above scientific question, a series of atmospheric scientific experiments and research programs have been conducted since the 1960s, quantitatively evaluating both the spatial distribution and the multi-timescale variation of LAIP via observation, remote sensing, and numerical simulation. Based on the three main approaches, the major advances on LAIP over the past 35 years are systematically summarized in this work. These progresses via observations further contributed to the improvement of remote sensing parameterization and numerical simulation of LAIP. Moreover, multisource (multispectral and thermal) satellite data have been successfully used to retrieve key land–atmosphere properties, which offers a feasible way to monitor LAIP at different spatiotemporal scales. Hourly data of land surface heat fluxes over the entire TP were first obtained too. The total annual evaporation is approximately 51.7 ± 2.1 km3 year-1 for high-elevation lakes with ice sublimation component accounting for around 10-25%. But the total annual evapotranspiration (ET) over the terrestrial surface of the TP are approximately 1238.3±57.6Gt yr-1 and 930.0±37.0 Gt yr-1 from the deferent remote sensing models. Future studies are recommended to focus on the optimization of the current three-dimensional comprehensive observation system, the development of advanced parameterization schemes and the investigation of LAIP on weather and climate changes over the TP and surrounding regions.
HS05-A002
Land Surface Evapotranspiration of Tibetan Plateau : Observation, Simulation and Multi-results Synthesis
Yinsheng ZHANG#+
Chinese Academy of Sciences
Land surface evapotranspiration (ET) is a key issue for land surface process and water resources. The ET in Tibetan Plateau (TP) is important for the "Asia Water Tower" due to it affect water resources by water loss. Thereby, precisely quantifying ET is necessary for an improved understanding of not only water storage in the "Asia Water Tower" but also the predictions of its future changes. However, existing products of ET have showed significant uncertainty in the TP, which has severely limited the knowledge of the multi-scale process and mechanism of terrestrial ET in the TP. This work intends to grasp the key process of ET on the alpine regions by the methods of enhanced observation of point-line-surface multi-scale water and heat exchange process; Completing the terrain correction, separating soil evaporation and vegetation transpiration in the land surface model and finally improving the simulation accuracy of the ET process in Alpine region. By making full use of existing observational data, the project will conduct multi-scale verification, evaluation, and fusion of multi-source data products to obtain high-reliability ET product in the TP. The product will reveal the spatial differentiation of ET restricted by hydrothermal coupling modes, clarify the response characteristics of ET to climate change at different scales, and analyze the multi-scale change process and mechanism of ET in the TP. The results can clearly grasp the water resources effects of ET changes, predict the changing trends of Asia water towers, and provide scientific support for the assessment of water resources environmental effects.
HS05-A003
The Slowdown of Increasing Groundwater Storage in Response to Climate Warming in the Tibetan Plateau
Longhuan WANG#+, Binghao JIA
Chinese Academy of Sciences
The change of groundwater storage (GWS) on the Tibetan Plateau (TP) is vital for water resources management and regional sustainability, but its estimation has large uncertainty due to insufficient hydrological measurements and diverse future climate scenarios. Here, we employ high-resolution land surface modeling, advanced satellite observations, global climate model data, and deep learning to estimate GWS changes in the past and future. We find a 3.51±2.40 Gt yr-1 increase in GWS from 2002–2018, especially in exorheic basins, attributed to glacier melting. The GWS will persistently increase in the future, but the growth rate is slowing down (0.14 Gt yr-1 for 2079–2100). Increasing GWS is projected over most endorheic basins, which is associated with increasing precipitation and decreasing shortwave radiation. In contrast, decreasing GWS is projected over the headwaters of Amu Darya, Yangtze, and Yellow river basins. These insights have implications for sustainable water resource management in a changing climate.
HS05-A016
Variation of Land Surface Water Flux to the Atmosphere Over the Tibetan Plateau: Perspectives from Earth Observation-based Evapotranspiration Datasets
Chaolei ZHENG#, Li JIA+, Guangcheng HU, Jing LU, Qiting CHEN, Min JIANG, Massimo MENENTI
Chinese Academy of Sciences
Evapotranspiration (ET) is an important process linking the land surface water and energy cycles. In the Tibetan Plateau (TP) region, the foreseeable increase in air temperature may have profound and complex effects on the local hydrological cycle, and is likely to increase the loss of water from the land surface to the atmosphere through ET. Quantifying ET and its regulatory mechanisms are major challenges for understanding the water cycle and land-atmosphere interactions in the TP region. We evaluated the performance of several Earth observation-based ET datasets in the TP region, and explored the spatiotemporal variation of ET in the same region. The accuracy of different global ET datasets was evaluated, and ETMonitor and PML-V2 provide the best accuracy with low overall high correlation, low bias, and low root mean square error. ETMonitor ET is also the only product with both high spatial (~1 km) and temporal (daily) resolution. ETMonitor ET may reflect the effect of mountain topography on ET better than other global products, i.e., ET values are higher in the humid valleys with denser vegetation cover and higher soil moisture, and ET values are lower on the mountain slopes at higher elevations with less vegetation cover and colder climate. Other ET products failed to capture the spatial patterns of ET in the mountainous regions, including the high-resolution datasets, and this suggests that the spatial resolution is not the only dominant factor leading to the poorer performance of these ET products in the mountain regions of the TP. The results show that multi-year average ET is 339 mm/yr in the TP region during 2000-2021, which accounts for about 51% of the total precipitation in the TP region. From 2000 to 2021, ET over the Tibetan Plateau shows an overall increasing trend with large spatial variability.
HS05-A017
Local Cooling and Drying Induced by Himalayan Glaciers Under Global Warming
Kun YANG1#, Franco SALERNO2+, Nicolas GUYENNON2
1Tsinghua University, 2National Research Council
Understanding the response of Himalayan glaciers to global warming is vital because of their role as a water source for the Asian subcontinent. However, great uncertainties still exist on the climate drivers of past and present glacier changes across scales. Here, we analyse continuous hourly climate station data from a glacierized elevation (Pyramid station, Mount Everest) since 1994 together with other ground observations and climate reanalysis. We show that a decrease in maximum air temperature and precipitation occurred during the last three decades at Pyramid in response to global warming. Reanalysis data suggest a broader occurrence of this effect in the glacierized areas of the Himalaya. We hypothesize that the counterintuitive cooling is caused by enhanced sensible heat exchange and the associated increase in glacier katabatic wind, which draws cool air downward from higher elevations. The stronger katabatic winds have also lowered the elevation of local wind convergence, thereby diminishing precipitation in glacial areas and negatively affecting glacier mass balance. This local cooling may have partially preserved glaciers from melting and could help protect the periglacial environment.
HS05-A019
Collaborative Observational and Modeling Initiative for Understanding of Asian Hydroclimatological System Under the Climate Change
Toru TERAO#+
Kagawa University
The Asian Precipitation Experiment (AsiaPEX) will call for an observational and modeling initiative, Asian Monsoon Year-II (AMY-II), to understand Asian hydroclimatological system under the climate change in the period between 2025 to 2028. The Tibetan Plateau, or the TPE regiion is a key of the Asian hydroclimatological system. The strategy of the AMY-II are the subregional observation platforms and integrated global analysis. For the subregional observation platforms, it would be important to define specific process that reach the interaction within the land-atmosphere coupling processes. In this talk, I would like to discuss different possible subregions surrounding the TPE region. For this discussion, I would like to focus on a process of the production of lower tropospheric high moist static energy airmass (HMSEA). The accumulation of HMSEA is oue of requirements for the establishment of Asian monsoon circulation. Due to differences of the surface process, the timing and amount of the HMSEA production are different in different regions. A discussion of this process will facilitate the definition of the process-oriented subregional platforms. The land-atmosphere coupling process controls the energy and water exchange and HMSEA production. In this paper, the local observation impact to the HMSEA production estimation will also be discussed.
HS05-A022
A Total Precipitable Water Product Based on Remote Sensing in Recent Decade in the Tibetan Plateau and Its Trend Analysis
Dabin JI#+, Jiancheng SHI, Qixiang SUN, Husi LETU
Chinese Academy of Sciences
Atmospheric water vapor is a key parameter in water cycle of the Tibetan Plateau. Lots of atmospheric water vapor products or datasets have been created using remote sensing or combination of remote sensing and ground observations, such as total precipitable water (TPW) product of SSM/I, NVAP, and AIRS/AMSU. However, most of these TPW products are limited in spatial or temporal coverage, especial the lack of the observation of TPW in recent decade. In this study, a daily TPW dataset from 2002 to 2017 with a spatial resolution of 0.05°×0.05° is produced in all-weather condition based on the combination of TPW from MODIS and TPW retrieved from AMSR-E and AMSR2 over land using our newly developed algorithm. In the creation of TPW dataset from 2002 to 2017, as a pre-process, all the three kinds of TPW data are re-projected into 0.25°×0.25° grid images for spatial consistency. And the TPW from MODIS water vapor product will be used as the reference TPW to calibrate the Microwave-TPW data derived from AMSR-E and AMSR2, because the TPW from MODIS water vapor product has the highest precision among all the TPW products in this study according to our validation. The calibration method is histogram matching. A matching histogram is built based on the overlapping area of the TPW from MODIS and AMSR-E or AMSR2 in clear sky condition, and then the matching histogram will be applied to the Microwave-TPW. Finally, the calibrated long term TPW product is further fused with MODIS TPW at a spatial resolution of 0.05° using a newly developed fusion algorithm. Besides the changing pattern will also be analyzed in both temporal and spatial scale based on the newly fused TPW product in the Tibetan Plateau.
Session Chair(s): Changhyun JUN, Korea University
HS45-A001
Research on the Integrated Water Resources Regulation Method of the Yangtze River and Yellow River Based on the Complex Network Analysis
Rui MA1#+, Zhipeng FAN2, Jiarui WAN3, Xuning GUO1, Weifeng LIU4, Jun HE1, Yunling LI1
1Ministry of Water Resources, 2Wuhan University, 3Changjiang River Scientific Research Institute, 4MWR General Institute of Water Conservancy Resources and Hydropower Planning and Design
The South-to-North Water Diversion and other large-scale cross-basin water transfer projects possess notable characteristics, including multiple sources of water supply, mutual aid from multiple lines, regulation through multiple projects, synergy with multiple objectives, and subjective game involving multiple parties. The key to enhancing the comprehensive benefits of the water network and ensuring a reliable water supply lies in achieving balanced and synergistic regulation and control of water resources. This paper utilizes complex network analysis modeling ideas and multi-objective optimization to examine the source-sink relationship within the natural river network as well as the sink-dissipation relationship within the artificial transmission and drainage system in both the Yellow River Basin and South-to-North Water Diversion Reception Area. Furthermore, it establishes an inter-basin network topology between the Yangtze River and Yellow River. By considering both network structure and connectivity, an objective function for assessing network resilience is constructed for the water resources system of these two rivers. Model constraints are listed based on basin characteristics and node settings to propose an integrated control model for cross-basin water resources management between the Yangtze River and Yellow River that optimizes indicators of network resilience. Additionally, principles, rules, and a joint application mode for integrated regulation of inter-basin water resources are proposed while considering synergy among water resources, economic society, and ecological environment.
HS45-A005
Deciphering the Self-organizing Nature of River Networks Through a Probabilistic Network Evolution Model
Dnyanesh BORSE#+, Basudev BISWAL
Indian Institute of Technology Bombay
River networks globally exhibit self-organizing tree-like patterns that adhere to statistical scaling laws, including Hack's law, and the distribution of contributing areas, upstream lengths and independent basin sizes etc. While simple statistical models have been employed to elucidate the evolution of these networks, they often fall short in accounting for the diversity in network structures. This study bridges this gap by integrating physically meaningful variables into a statistical modelling framework, enhancing our understanding of these complex landscape formations. Our model enables network growth in a headward direction through probabilistic decisions, driven by two free parameters. Simulations on a planar matrix generate tree-like networks that display power-law scaling relationships akin to real river networks. These parameters effectively capture variations in key network characteristics, such as the compactness coefficient and Hack's exponent, thereby offering insights into the diverse shapes and features of river networks. Further, we investigate the distribution of independent basin areas across 25 islands worldwide, uncovering a consistent power-law pattern. The research highlights that the power-law exponent is significantly influenced by landscape boundary characteristics, notably increasing with the compactness coefficient and fractal dimension. This underscores the crucial role of boundary conditions in shaping river networks. Incorporating a preferential headward growth mechanism, our probabilistic network growth model demonstrates the emergence of power-law behaviour in basin area distributions. This study not only sheds light on the self-organizing nature of river networks and their adherence to power laws in basin area distributions but also emphasizes the influence of boundary shapes on these patterns. The results contribute to a deeper understanding of the complex mechanisms driving the evolution of river networks, offering a more nuanced perspective on landscape dynamics.
HS45-A006
Optimizing Rainfall Data Integrity: A DTW-driven Graph Framework for Filling Missing Values in Automatic Weather Station Networks
Seoyeong KU1+, Jongyun BYUN2, Seunghyun HWANG1, Yookyung LEE1, Changhyun JUN2#
1Chung-Ang University, 2Korea University
Precise and real-time predictions of rainfall are crucial components of weather forecasting. Despite its importance, rainfall prediction remains a scientific challenge, mainly due to the complex geographic topology and spatio-temporal dependencies. To address these complexities and the relationships between multiple observations, we propose a novel methodology using Dynamic Time Warping (DTW) to construct a graph based on ground observations. DTW establishes connections between observations by determining optimal thresholds for each weather variable and analyzing the similarity of time series. Here, 27 points of Automatic Weather Station in Seoul, Korea, 4 types of data(e.g. precipitation, temperature, wind speed, wind direction, humidity), and two types of rainfall events (e.g. frontal precipitation, typhoon) are analyzed in this study. The data, recorded at 1-minute intervals, are transformed into various forms (e.g., average, cumulative, difference, etc.) for analysis. The study spans from January 2020 to December 2023 and evaluates the accuracy of imputing missing values using DTW. To evaluate the accuracy of filling missing values using DTW, we select a target rain-gauge and artificially create missing values by masking the observation data of the target rain-gauge for a specific rainfall event. Finally, we fill in the rainfall for the target rain gauge using observations from connected rain-gauges and edge weights. Accuracy is evaluated by comparing actual observed data with interpolated data using DTW-based graphs and traditional statistical methods. The results indicate higher accuracy compared to traditional approaches. In addition, this study holds potential for future multi-point rainfall forecasts using deep learning algorithms such as Graph Neural Networks. This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00243008 and was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. NRF-2022R1A4A3032838 & No. RS-2023-00250239).
HS45-A007
Assessing the Predictability Horizon for Streamflow and Water Quality from the Chaos Theory Point of View
Xiaoyu ZHANG1+, Jiping JIANG1#, Yi ZHENG1, Ashish SHARMA2
1Southern University of Science and Technology, 2UNSW Sydney
Streamflow prediction and water quality prediction are the major efforts for modelling and practitioners. Long-term prediction is challenged for many situations. How far can we predict forward in time with a valid accuracy? And how will the accuracy attenuate in space, with increasing distance? To solve these, the deterministic chaos theory may provide a new insight. Chaos theory suggests that inherent features reflecting the evolution structure of a system exist within the data collected from nature. By analyzing these intrinsic features in time series data, we can define the limit of forecast lead time, or the prediction horizon, for water quantity/quality of each monitoring site. In this research, the intrinsic chaotic characteristics (system invariants, such as Lyapunov exponent, correlation dimension, etc.) of river system time series data are identified. Then, we employ a data-driven nonlinear machine learning method called reservoir computing (RC) for iterative prediction. Analyzing the evolution of model prediction errors over time at different sites, we investigate the influence of data inherent properties on model-realized predictability. Finally, we manage to assess the predictability horizon given time series of river system data. The approach offers a novel analytical tool for understanding the characteristics of water quantity and quality data in river systems, as well as the complexity of nonlinear processes in watersheds. It holds significant implications for water environmental management and policy formulation.
HS45-A008
Uncertainty Analysis of Solute Transport in Discrete Fracture Networks - A Case Study for Taiwan's K-area Reference Case
Ting Wei HE#+, Tai-Sheng LIOU
National Chung Cheng University
Taiwan's final disposal of spent nuclear fuels (SNFs) aligns with the deep geological concept, burying them in low-permeability fractured rocks at a depth of 500 meters. For granitic host rocks, discrete fracture networks (DFNs) serve as primary radionuclide pathways, but their migration behavior is uncertain because DFN parameters are interpreted from limited data sampled from outcrops or finite-length boreholes. Therefore, uncertainty analysis is vital for evaluating transport characteristics in the near field and far field of the disposal facility. This study utilizes data from Taiwan’s K-area reference case and dfnWorks to model DFNs in a 100 cubic rock body. Transport characteristics are analyzed using particle tracking simulations, releasing 3000 particles in a small area centered on the upstream boundary. Variance-based Global Sensitivity Analysis (VGSA) is then used to identify parametric uncertainty. In contrast to the conventional Monte-Carlo (MC) method, sparse grid collocation (SGC) and polynomial chaos expansion (PCE) prove computationally efficient for a large sample of DFN parameters. An Ishigami function demonstrates SGC and PCE's computational efficiency over MC. Results show that SGC and PCE require 1500 or fewer computations to yield indices with relative errors of less than 1% compared to theoretical indices, while MC needed more than 6000 computations for similar accuracy. However, it is a challenging task to evaluate DFN parameter sensitivity using SGC and PCE. In a DFN case with four random fracture parameters, PCE sensitivity analysis to the 7th order yielded a poor fit with R 2 ≈ 0.14. Future research aims to elevate the performance of higher order PCE sensitivity analysis, and compare results against SGC and MC.
HS45-A003
Tipping Behaviors in Insurance-levee Interplays Under Climate Change
Woi Sok OH#+
Princeton University
Social dynamics is not isolated from hydrological dynamics; humans and water are interconnected via infrastructure in the form of coupled human-water systems (CHWSs). Here, infrastructure can be in either physical (e.g., levee, dam, reservoir) or intangible (e.g., social norm, institution, rule) form. Both forms of infrastructure protect CHWSs to sustain against uncertain shocks. In this study, I particularly focus on levees as physical infrastructure and index insurance and maintenance cooperation as soft infrastructure. Bangladesh will be the study area where levees are self-maintained by farmers due to the malfunctioning government. I develop an agent-based model to capture the strategic decisions of farmers in response to changing water levels and levee conditions. There are four possible strategies: (1) adopt insurance and cooperate in levee maintenance, (2) adopt insurance and free-ride in levee maintenance, (3) do not adopt insurance and cooperate in levee maintenance, and (4) do not adopt insurance and free-ride in levee maintenance. How do strategic decisions evolve in different combinations of levee and insurance index levels? I also check social inequity beyond economic profit to investigate interactions between the two outcomes (e.g., trade-off, synergy). In the next step, I check the effect of sea-level rise and water-level regime shifts on strategic decisions as climate-change scenarios. How will social tipping take place in different scenarios? This study offers valuable insights into understanding CHWS interplays and tipping behaviors against climate change, suggesting resilient strategies in the long term.
Session Chair(s): Ying ZHAO, Ludong University, Heejung KIM, Kangwon National University
HS36-A010
| Invited
Utilizing Reliability-based Methods for Hyporheic Zone Depth Delineation in Groundwater Remediation Strategies
Heejung KIM#+, Yang JAE E.
Kangwon National University
The behavior of natural phenomena such as hyporheic zone depths exhibits inherent statistical traits due to the significant variability of associated parameters. Previous studies have proposed a deterministic approach for delineating hyporheic zone depth using a simple field temperature measurement, as well as a probabilistic method to establish an appropriate statistical distribution model for hyporheic zone depth. Building upon this foundation, the current research endeavors to propose remediation strategies for contaminated groundwater systems in relation to hyporheic zone depth management. The primary focus involves predetermining the demand for hyporheic zone depth to achieve a required recovery ratio. Subsequently, the field hyporheic zone depth is adjusted in accordance with each strategy. The two probabilistic variables, demand and field values, are then modified to reduce the difference between them. The index utilized to evaluate each strategy in this paper is derived from the concept of reliability index, a common approach employed in various scientific and engineering disciplines, including the safety design of structures. The fundamental principle of safety design revolves around ensuring sufficient safety margins between a strength criterion and the requirements, which is precisely what the reliability index evaluates. The paper is structured to initially introduce the reliability-based approach in terms of the general concept and hyporheic zone depth management, followed by the development of the index. Finally, the paper concludes with a performance evaluation of the proposed strategies. This paper holds significant value as it combines previous research on the probabilistic property extraction of hyporheic zone depth with a novel approach to performance evaluation, offering potential as a valuable tool for the remediation of contaminated groundwater.
HS36-A005
Evolution Characteristics of Sediment Source in a Small Catchment in North China
Jingjing XU+, Pengfei DU#
China Institute of Water Resources and Hydropower Research
The composite fingerprint technique was introduced to make clear the characteristics of sediment sources contribution in typical catchment located in the transitional area from plateau to plain of North China under natural restoration. A catchment was selected named Dongshanwan catchment, where experience serious water erosion. In order to make clear the optimized composite fingerprints, 30 chemical properties and grain size composition were measured and statistically analyzed. Then, the multivariate linear mixed model was used to calculate the relative contribution rate of sediment sources. The time scale of the sediment process had been set up by the characteristics alluvium information. The corresponding deposition layer with rainfall can analyzed sediment yield intensity in check dam. The results indicated that the sedimentary period was divided into four stages from 2013 to 2019. The relative contribution rates of sediment sources in the three source areas of sandy grassland, forest and gully reached 30.16%, 38.88% and 30.93%, respectively. The relative contribution per unit area in the three source areas of sandy grassland, forest and gully reached 0.59, 0.86 and 13.70, respectively. The annual soil erosion modulus was 2917.39 t/(km2·yr) under natural restoration. Compared with the value of NDVI, the effect of total rainfall with daily rainfall greater than 25 mm on the contribution rate of sediment sources is more significant. There was a general trend for forest erosion modulus to decrease and for gully erosion modulus to increase over the period 2013-2019, the erosion modulus of sandy grassland tended to be stable over the period 2013-2019. This study clarified the sediment reduction benefits of source regions under natural restoration, but also provide a basis for the planning and construction of natural restoration projects in the transitional area from plateau to plain of North China in the future.
HS36-A001
Environmental Forensic Investigation of Groundwater Contaminated with BTEX and TPH in an Urban Area
Soonyoung YU1+, Jung-Woo HWANG2, Seong-Taek YUN2#
1Korea Institute of Geoscience and Mineral Resources, 2Korea University
The polluter-pays principle is the commonly accepted practice, whereas the principle is difficult to apply in groundwater contamination since it is challenging to trace contamination sources given the facts: (1) contamination slowly occurs in subsurface, (2) groundwater contamination is often detected a long time after it begins due to difficulty in awareness, (3) the location of sources can be different from where the contaminants are detected due to solute transport in groundwater flow, (4) fingerprints at receptors can be different from those at sources due to reactions during transport, (5) the accessibility to potential sources is limited owing to the challenges law enforcement faces in patrolling certain areas. In this study, several environmental forensic techniques were integrated to assess the sources and fates of BTEX and TPH in groundwater, including hydrochemistry, oil fingerprints, C and H isotopes of BTEX, and the concentrations of BTEX and TPH. Multivariate statistical and temporal trend analysis were conducted. The results suggested two different oil sources and spill incidents in the studied urban area. Biodegradation of benzene seemed recalcitrant in the highly contaminated anaerobic condition. Oil fingerprinting and mole fractions were effective to distinguish the contamination sources. The temporal data helped to estimate release times. The clustering and PCA results were effective to evaluate the hydrogeochemical processes with contamination. The compound specific isotope analysis supported the biodegradation of toluene, whereas sources could not be estimated based on isotopic data since the isotopic characteristics of potential sources were unknown. [Acknowledgement] This research was supported by the Korea Environment Industry & Technology Institute (KEITI) through two projects ‘Integrated environmental forensic approaches to trace source and pathways of subsurface contaminants (2021002440003)’ and ‘System development and field demonstration of in-situ chemical oxidation circulation designed based on numerical modelling (RS-2023-00220587)’, funded by Korea Ministry of Environment (MOE).
HS36-A008
The Effect of Rainfall Variability on N Dynamics in a Small Agricultural Catchment
Qiaoyu WANG1+, Jie YANG1, Bo FAN2, Chunhui LU1#
1Hohai University, 2Ministry of Water Resources
The rainfall variability has been testified to be unprecedentedly remarkable in the context of climate change. Extreme storms and droughts have occurred throughout the globe, causing serious impacts on society and ecosystems. The aim of this study is to explore the effect of rainfall variability on N dynamics, impacting water quality and aquatic ecosystems. A stochastic model of rainfall time series was used to simulate rainfall with the same parameter attributes as rainfall that arose during the past two decades in central Germany. The transport of flow and nitrate was simulated by the fully coupled surface-subsurface model HydroGeoSphere in a small agricultural catchment in central Germany. A sensitivity analysis was conducted. It was found that the amplitudes of the seasonal variations of storm duration and interstorm period are key parameters to alter the intensity and density of precipitation in different seasons. The intensive rainfall with short storm durations contributes to N retention; however, extreme rainfall with long interstorm periods facilitates N export in the summer. In order to identify the impact of the annual precipitation on N dynamics, three scenarios (with high, normal and low annual precipitations, respectively) were simulated. Based on the scenario of low annual precipitation, another scenario with lower plant uptake was considered to examine the importance of vegetation for aquatic ecosystems. The results suggest that higher precipitation can enhance the transformation and transport of nitrogen. The nitrogen retention capacity of catchments in the scenario of low annual precipitation is higher than in other scenarios. Nonetheless, when vegetation suffers from drought stress, the capacity will decline severely. Overall, our study reveals the response of N dynamics to rainfall variability, which provides theoretical support for us to protect aquatic ecosystems in the future.
HS36-A002
Enhanced Water Budget Analysis of Shallow Groundwater Dynamics and Their Impact on Subsurface Environments in Korean Cultivation Sites
Sun Woo CHANG#+, Il Moon CHUNG, Chul-gyum KIM, Min-Gyu KIM
Korea Institute of Civil Engineering and Building Technology
In the agricultural regions of South Korea, Water Curtain Cultivation (WCC) is widely implemented during the winter season, utilizing groundwater to maintain temperatures sufficiently for crop cultivation in greenhouses. This study aims to quantitatively analyze the impact of groundwater utilization in areas employing the WCC technique. The study area experiences groundwater depletion from November to March, followed by a recovery pattern in groundwater levels during the spring-summer period through recharge from precipitation and induced recharge from the river. Groundwater levels were observed at six monitoring wells, and stream levels were collected from two points spanning two years for use as modeling input and calibration data. Additionally, the morphology of two major weirs along the river was surveyed and utilized as input data for modeling. SWAT and MODFLOW were employed to simulate hydrological recharge and groundwater flow in the research area. The MODFLOW model was simulated and calibrated for the period from 2012 to 2014, in comparison with the observed groundwater levels. Precise analyses of groundwater disturbance and recovery revealed that groundwater depletion by WCC is mostly recovered due to induced recharge from the river and abundant summer rainfall contribution. Nevertheless, the aquifer did not fully recover during the entire cycle, and the average annual groundwater decrease in the study area was estimated at 2.5 cm/km². Simulation scenarios incorporating increased artificial recharges through groundwater reinjection indicated that a 20% artificial recharge of the aquifer allows the expected recovery of the aquifer. ACKNOWLEDGMENTS: This research was supported by a grant from the Development Program of Minimizing of Climate Change Impact Technology funded through the National Research Foundation of Korea (NRF) of the Korean government (Ministry of Science and ICT, Grant No.NRF-2020M3H5A1080735) and KICT Research Program (Project No. 20230166, Development of Coastal Groundwater Management Solution).
Session Chair(s): Xin LI, Chinese Academy of Sciences, Li JIA, Chinese Academy of Sciences
HS05-A007
Oceanic Repeaters Boost the Global Climatic Impact of the Tibetan Plateau
Yongkun XIE1#+, Jianping HUANG1, Guoxiong WU2, Yimin LIU2
1Lanzhou University, 2Chinese Academy of Sciences
The topography of the Tibetan Plateau (TP) has shaped the paleoclimatic evolution of the Asian monsoon. However, the influence of the TP on the global climate, beyond the domain of the Asian monsoon, remains unclear. Here we show that the Pacific, Atlantic, and Arctic Oceans act as efficient repeaters that boost the global climatic impact of the TP. The simulations demonstrate that oceanic repeaters enable TP heating to induce a wide-ranging climate response across the globe. A 1°C TP warming can result in a 0.73°C temperature increase over North America. Oceanic repeaters exert their influence by enhancing the air-sea interaction-mediated horizontal heat and moisture transport, as well as relevant atmospheric circulation pathways including westerlies, stationary waves, and zonal-vertical cells. Air-sea interactions were further tied to local feedbacks over the North Pacific, North Atlantic, and Arctic Oceans. Our findings highlight the crucial influence of TP heating variation on the current climate under a quasi-fixed topography, in contrast to topography change previously studied in paleoclimate evolution. Therefore, TP heating should be considered in research on global climate change.
HS05-A008
Changes in Glacier Area and Elevation in the Near-equatorial Region
Xin LI1#+, Shanshan REN2, Zheng DONGHAI1, Yushan ZHOU3
1Chinese Academy of Sciences, 2Lanzhou University, 3Central South University
In recent decades, the glacier area and elevation in the near-equatorial region have changed drastically, becoming an important indicator of global climate change. In this study, the glacier changes in 13 regions in the equatorial area were analyzed in detail based on the band ratio method and geodetic method using multi-temporal Landsat images, SRTM and Copernicus DEM data. The results indicate a consistent trend of glacier retreat and thinning across these regions. In terms of area, glaciers in the South America region witnessed a rapid decline from 1980 to 2000 and followed by a deceleration, shrinking by 12%-43% in six sub-regions. In contrast, glacier changes in Africa and Indonesia remained relatively stable throughout the study period. The glaciers of Mount Kenya and Kilimanjaro in Africa experienced reductions of around 78% and 31%, respectively, while Ngga Pulu in Indonesia decreased by 68%. For glacier thickness, the rate of glacier elevation change ranged from –0.14 ± 0.05 m a–1 to –1.8 ± 0.17 m a–1, with notable variations observed at Santa Isabel and Chimborazo in South America, with elevation change rates of –1.8 ± 0.17 m a–1 and –0.96 ± 0.07 m a–1, respectively. Finally, a comprehensive analysis of temperature and precipitation variations during the study period in the three regions revealed that the multifactorial changes in glaciers are closely related to the increase in temperature. Our study provides insights into glacier changes in the near-equatorial region and provides important insights into understanding the influence of climate on the regions.
HS05-A009
Airborne TomoSAR Campaign on Bayi Glacier
Jiali CHEN1, Xin LI2#+, Zheng DONGHAI2
1Lanzhou University, 2Chinese Academy of Sciences
As an important reservoir of solid water resources in the cryosphere, glacier is one of the most sensitive elements of climate change. Exploring the change of internal structural parameters such as glacier thickness is of great significance in water resource utilization, sea level rise and glacier disaster. Tomographic SAR (TomoSAR) has unique advantages in analyzing the internal structure of ground objects. The P-band and L-band glacier transparent and tomography remote sensing flight test was carried out on Bayi Glacier in the upper reaches of Heihe River in the Tibetan Plateau from March 28 to April 8, 2023. Meanwhile, airborne SAR ground calibration and ground observation of glacier thickness based on ground penetrating radar (GPR) were carried out simultaneously, and the data acquisition volume exceeded 3 TB. Preliminary results show that L-band tomographic SAR can detect subsurface bedrock at 50 m and grooving at 80 m, consistent with the subsurface features presented by the 100MHz GPR transects. It is obvious from the amplitude diagram that the P-band has better penetration ability, but there are more oversaturated signals in the P-band echo data, the image signal-to-noise ratio is relatively poor, and the interference phase of each trajectory has dense azimuthal fringes, which need to be further eliminated before tomography can be performed.
HS05-A011
Sedimentary Records of the Catastrophic Outburst Floods on the First Bend of the Yangtze River Since the Late Quaternary
Huiying WANG#+
China Earthquake Administration
Late Quaternary catastrophic drainage sourced from valley-blocking glacial debris flows on the First Bend of the Yangtze River cause anastomosing erosion and deposition that have strong potential to change the landscape morphology. It has been discovered that sedimentary deposits associated to such floods are widespread across continents, and share a few common traits of features and significance. Combined geomorphic features, sedimentologic interpretation and chronological results, we provide the comprehensive evidence of the flood landscapes and deposits developed in the Daju Basin downstream of the Tiger Leaping Gorge. The characteristics of spatial distribution are described based on the identification of typical erosional and depositional surface forms. Six stratigraphic sequences are divided into three main lithological units reflect at least two phases of progradation at ~20-18 ka and ~6.5-1.5 ka. The largest flood had a water depth of over 210 m, and the inferred flood magnitude had the order of 1 Sv. The stratigraphic successions are constructed to supply details for understanding the paleo-environmental relevance of the dynamics of flood events, and to provide a case for high magnitude outburst flood deposition models in the high mountainous area of the southeastern Tibetan Plateau.
HS05-A013
Research and Application of Zoning Methods for River Source Areas in the Qinghai-Tibet Plateau
Baodeng HOU1#+, Hongcai LIU2
1China Institute of Water Resources and Hydropower Research, 2North China Electric Power University
The Qinghai-Tibet Plateau, as the birthplace of many rivers in Asia, provides abundant water resources for many Asian countries and is known as the "Asian Water Tower". However, at present, the protection of the river source areas in the Qinghai-Tibet Plateau still needs to be strengthened, and there is relatively little research on the zoning of the source areas. On the basis of literature review and field investigation, this study constructed a zoning index system for the source areas of rivers that conforms to the characteristics of the Qinghai-Tibet Plateau (including 11 indicators such as slope gradient, landform type, glacier permafrost, annual precipitation, annual average temperature, annual evaporation, ecosystem type, water conservation, land use, population density, and GDP per unit area). A zoning method for the source areas of the Qinghai-Tibet Plateau was proposed, which comprehensively considers the first tributary method, single index method, and multi-index method (using analytic hierarchy cluster process for calculation). The source area of 33 major rivers of 8 major river systems, including the Yarlung Zangbo-Brahmaputra River, Yangtze River, Nu River, Lancang River, Irrawaddy River, Ganges River and Indus River, has been demarcated. The total area of the source areas of 33 major rivers is about 242,100 square kilometers, accounting for 9.68% of the total area of the Qinghai Tibet Plateau (about 2.5 million square kilometers). The area of each river source area accounts for 2% to 30% of the total basin area in the Qinghai Tibet Plateau, depending on the characteristics of each river basin.
HS05-A014
Extreme Precipitation Detection Ability of Four High-resolution Precipitation Products Datasets in Nepal
Sunil SUBBA1#+, Yaoming MA2, Weiqiang MA2, Cunbo HAN2
1University of Chinese Academy of Sciences, 2Chinese Academy of Sciences
Nepal's tendency for extreme precipitation (EP) makes it crucial to study its historical patterns. Topography of Nepal make it hard to get exact precipitation data for EP research from sparsely-gauged networks. This will hinder the dissemination of knowledge about Nepal's EP variability. The following considerations may explain the current research trend's shortcomings: (1) Few research employed recently published high-resolution precipitation products to assess EP detection capacity in Nepal, (2) Most studies focused on EP event characteristics rather than spatial and temporal variability. Four high-resolution precipitation product datasets (PPDs)—ERA5 Land reanalysis data, satellite-based precipitation data (PERSIANN_CCS_CDR), and merged datasets (CHIRPS_V2.0 and TPHiPr)—were evaluated for extreme precipitation detection across Nepal from 1985 to 2020 to address these issues. PPD performance was assessed using the Mann-Kendall test trend, Sen's slope estimator, and statistical and categorical indices. The TPHiPr combined dataset estimated monthly precipitation better than other PPDs. TPHiPr has the highest CSI, ACC, POD, and FAR. Thus, TPHiPr is the best PPD for predicting 0.1 mm of precipitation per day in Nepal. TPHiPr had the best temporal representation for most EP indices due to less representational mistakes. Some EP indices, such as frequency (R10mm, R20mm, and R25mm) and intensity (RX1 day, RX5 day, PRCPTOT, and R99p), correlated better between TPHiPr and the observed dataset. Based on these data, TPHiPr captured the spatial distribution of EP occurrences in Nepal from 1985 to 2020 better than other PPDs. This dataset can enhance Nepalese hydrometeorology and climate studies.
HS05-A015
Seasonal Catchment Memory for Rivers in High Mountain Asia
Haiting GU#+, Yue-Ping XU, Liu LI, Lu WANG
Zhejiang University
Rivers originating from the Tibetan Plateau (TP) play a vital role in providing a reliable water supply to nearly 2 billion people. Nevertheless, the balance of the Asian water tower has been impacted by climate change and human activities, leading to alterations in downstream water resources. Consequently, research focusing on seasonal hydrological forecasting bears significance for effective water resource management and ensures food security across a vast expanse of Asia. Seasonal catchment memory (SCM) suggests critical importance in improving runoff predictability and extending the forecastable time in seasonal hydrological forecasting. In pursuit of mechanism of SCM, the hysteresis loop is employed to investigate the transformation rule among precipitation, streamflow, and water storage on a seasonal scale. The proposed P2S model utilizes precipitation to estimate Terrestrial Water Storage Change (TWSC), and its estimations align with GRACE-derived TWSC. To comprehensively quantify the process and duration of SCM, the precipitation memory curve and influence/domination time are proposed based on the P2S model. The investigation of eight representative high mountain river basins reveals compelling findings. In precipitation-dominated basins, precipitation suggests a controlling role in SCM, with less than 10% of the precipitation retained in the catchment after four months. Moreover, during the monsoon season, the influence/domination time extends to six/four months, compared to three/one months during the winter season. Conversely, non-precipitation-dominated basins exhibit a long-term catchment memory. The findings of this study enable the identification of efficient lead times for seasonal streamflow forecasts. It indicates that precipitation during the winter season has little impact on the monsoon season's streamflow, while precipitation during the monsoon season may dominate the streamflow during the winter season.
Session Chair(s): Marcelo URIBURU QUIRNO, Comisión Nacional de Actividades Espaciales, Cheol Hee JANG, Korea Institute of Civil Engineering and Building Technology, Hwirin KIM, World Meteorological Organization
HS22-A005
HydroSOS: WMO Efforts for Supporting Member to Improve Water Resources Assessment and Management Capacity with Global Hydrological Status and Outlook System
Hwirin KIM1#+, Stefan UHLENBROOK1, Luis Roberto SILVA VARA1, Nakul PRASAD1, Sulagna MISHRA1, Katie FACER-CHILDS2, Harry DIXON2, Alan JENKINS2, Lucy BARKER2
1World Meteorological Organization, 2UK Centre for Ecology & Hydrology
World Meteorological Organization (WMO) identified significant gaps among several of its 193 Member states, including limited access to tools and systems, lack of information and reduced management capacity. This poses a challenge to an ever-growing number of people at risk from water-related hazards, alongside rapidly growing demands on water resources. Therefore, WMO decided to initiate a pilot WMO global Hydrological Status and Outlooks System (HydroSOS) in 2016 (Resolution 8, CHy-15). HydroSOS’s ambition is not limited to develop a simple tool, model or system for sub-seasonal and seasonal hydrological prediction. Rather, it is a holistic approach to provide a critical information including water availability to decision makers and stakeholders in the multiple sectors such as Agriculture, Disaster Risk Reduction, Water, Energy, Industry, Environment, among others. Under the HydroSOS initiatives, a demonstration portal was developed in 2021, the guidelines on Seasonal Hydrological Prediction (WMO-No.1274) were published in 2022, regional implementation plans for Africa, Asia, South America, Central America, South-West Pacific and Europe were approved in 2023 (Cg-19) and a Caribbean regional implementation plan is currently being drafted. The 1st state of global water resources was launched in 2022 and the 2nd report was published in 2023. Capacity building activities were also in place for developing countries through workshops, webinars, and training. The WMO Water Resources Assessment (WRA) webpage is designed to assist National Hydrological Services in implementing WRA by providing an evolving toolkit of appropriate and adaptable techniques. The Dynamic Water resources Assessment Tool (DWAT), freely available, was developed for providing more detailed information on regional, national or local water resources for planning and operation purpose and has been applied in 26 countries. WMO is supporting the implementation of HydroSOS based on the recently developed implementation plans that neatly reflected Members’ needs through the projects, funded by partners.
HS22-A004
Evaluation of the River Discharge in the Yeongsan-Seomjin River, and Geum River in the Republic of Korea Using DWAT (Dynamic Water Resources Assessment Tool, DWAT)
Cheol Hee JANG1#+, Hyeonjun KIM1, Deokhwan KIM1, Jeonghyeon CHOI1, Hyoungsub SHIN2
1Korea Institute of Civil Engineering and Building Technology, 2Environment Remotesensing Institute Inc.
Metropolitan areas around large rivers can use water stably even in the event of a drought, but the upstream areas with small and medium-sized rivers are vulnerable to water supply stability in drought season. Therefore, highly reliable evaluation and prediction of river discharge is necessary to prepare comprehensive solutions such as efficient operation of water supply facilities and optimal use of available water resources during drought season. In this study, river discharge was evaluated for 20-16, and 53 standard basins in the Yeongsan-Seomjin river, and Geum river basins, respectively, among major river basins in the republic of Korea. The Dynamic Water resources Assessment Tool (DWAT) was used as a assessment model. DWAT is a water resources assessment tool that can be used free of charge worldwide and can be applied to small and medium-sized river basins for water resource planning and management that considers surface water as well as groundwater and water usage for various purposes. The calibration period was set from 2012 to 2019, and the validation period was set from 2020 to 2021. In addition, simulation accuracy was calculated through a 1:1 comparison of observed and simulated discharge data based on the calibration point, and model efficiency (Nash Sutcliffe Efficiency, NSE) and coefficient of determination (R2) were applied as statistical values. As a result, NSE and R2 of more than 0.7 were secured for each calibration point.
HS22-A002
Comparison of Several Evapotranspiration Methods with DWAT Model for Streamflow Impact in Upper Nan Basin Thailand
Fatah MASHAWEE1#+, Pattara SUKTHAWEE1, Chaiwiwat VANSAROCHANA2, Nattapon MAHAVIK2
1Thai Meteorological Department, 2Naresuan University
The Dynamic Water Resources Assessment Tool (DWAT) is a hydrological model developed by KICT and supported by WMO to enable member countries used it in their missions. This model aims to manage water resources efficiently and sustainably. The results of applied DWAT model in the upper Nan River Basin from 2013-2020 was separated in two time period. Firstly, the calibrating of the model from 2013-2017 with measurement data from the American class-A pan for evapotranspiration shown the comparison of the model calibration data and discharge observation data at Station N.1 in Mueang District Nan Province has satisfaction statistics score from NSE, RSR, and R2 values as following 0.60, 0.63, and 0.72. In addition, the uncertainty of the model from RMSE and MAE values are 88.10 and 41.24. Secondly, The other model result with data set in 2018-2020, it was found that the efficiency of simulations comparation with the calibration results is an acceptable level, except for the RMSE value that was as high as 103.55, because of an outlier value that more than calibration data. However, the DWAT model utilized for forecasting, outlooks, or projections can be calculate with only the evapotranspiration from the equation for analysis. The DWAT model has two main evaporating equation name as the Penman-Monteith and Hargreaves (less complicated in calculation). The results of the analysis shown that the Hargreaves method) gave better results than Penman-Monteith for the upper Nan River basin area.
HS22-A007
Assessing the Impact of Climate Change on River Flow (Case Study: Ghara Sou River Basin, Iran)
Yashar FALAMARZI1#+, Cheol Hee JANG2
1Climatology Research Institute, 2Korea Institute of Civil Engineering and Building Technology
Water is essential for human beings and it is vital in various fields such as agriculture, navigation, energy production and manufacturing. Rapid urbanization, population growth and economic developments could potentially put stress on the water resources by increasing the water demand. In addition, climate change could also cause variations in quantity and quality of water resources. Therefore, assessing the impact od climate change on water availability is essential and requisite to adapt water resources management in rapid socio-economic development. I this study, impact of climate change on river flow in Ghara Sou River basin will be assessed. First, two hydrological models including DWAT and SWAT models is calibrated and validated for the period 1986-2018. Moreover, minimum and maximum temperature and rainfall outputs of MIROC GCM model under climate change scenarios SSP1-2.6, SSP2-4.5 and SPP5-8.5 is downscaled for the study area. Then, the downscaled data is fed into the calibrated hydrological to project monthly river flow in the period 2050-2075. The results will then be compared with the river flow in the baseline period (1991-2014) to assess the impacts of climate change on river flow.
HS22-A011
Results of DWAT Model Application on the Example of Oba River Basin, Kazakhstan
Tursyn TILLAKARIM#+, Serik SAIROV, Nurgalym SERIKBAY
National Hydrometeorological Center of the Republic of Kazakhstan
The Dynamic Water Assessment Tool (DWAT) aims to ensure sustainable and efficient management of water resources by adequately assessing their sources, volume, reliability and quality to inform long-term planning, assessment and policy development. The results of applying the DWAT model for the Oba River basin (Kazakhstan), which is the main lateral tributary of the Shulba reservoir, showed satisfactory results of model calibration. For model calibration, data from the observation network of the National Hydrometeorological Service of Kazakhstan in the period 2002-2018 were applied. The evaluation of the model performance, assessed by the criterion NSE, RSR, showed satisfactory results: NSE was 0.48, RSR was 0.72. Most of the water resources in the studied river basin are formed in the spring and summer season of the year, which is caused by melting of snow and ice cover. Mainly water resources are formed as a result of snow cover melting. Taking into account this peculiarity, it should be emphasized that the modelled water discharge reproduces well the spring season flow and shows well the hydrograph peak, also it should be noted that the model reproduces well the dates of spring flood onset. Thus, it should be noted that DWAT model well reproduces water discharge for the mountainous territory of Kazakhstan and can be used for forecasting the flow of the studied river basin.
HS22-A013
Application of the Dynamic Water Assessment Tool (DWAT) to Two Basins in Argentina
Marcelo URIBURU QUIRNO1#+, Suriano MICAELA2
1Comisión Nacional de Actividades Espaciales, 2University of Buenos Aires
DWAT was devised to analyse the portion of the water cycle occurring at catchment scale. With a distributed conceptual scheme, it simulates evapotranspiration, infiltration, catchment runoff, Paddy-field hydrology, snow melting, groundwater movement and channel routing. Examples of application include assessment of land-use changes over time, impacts on water availability under differing consumptive uses, and due to climate change. DWAT was applied to two very different basins in Argentina, both with rainfall regimes, but one in a semi-arid mountainous region, the Burrumayo basin, and the other in a more humid flatland region, the Santa-Lucía basin. The Burrumayo basin has an area of 351 km2 and an elevation range from 925 to 4775 masl. The potential evapotranspiration (Hargreaves) is 1100mm/y. A strong gradient is observed in the annual precipitation, increasing from 300mm to 1300mm, and a mean areal value of 926mm (concentrated mostly over the spring and the summer). The annual mean flow is about 9 m3/s, which are unevenly distributed over the year. The time of concentration is 10 hours. The Santa-Lucía basin has an area of 6200 km2 and an elevation range from 40 to 70 masl. The potential evapotranspiration is 1015mm/y, and the annual precipitation is 1200mm, evenly distributed over the year. The annual mean flow is 75 m3/s. The time of concentration is of about 3 days. Different modelling configurations were tested. The DWAT-parameter calibration performed better for one catchment component and one routing component for the Burrumayo, and one catchment component for the Santa-Lucía basin. The maximum Nash-Sutcliffe efficiency obtained for the calibration periods in both basins were 0.75 and 0.66, respectively, considered very good and good according to different authors. Volumetric fits were not as high, being above 0.50 in both cases. DWAT proved being a flexible tool, capable of simulating daily discharge time series satisfactorily.
HS22-A014
Application of DWAT in Operational Hydrological Forecasting Practice in Russia
Yuri SIMONOV#+, Andrey KHRISTOFOROV, Elena KUZNETSOVA
Hydrometcenter of Russia
Considering variety of natural conditions throughout the territory of Russian Federation, hydrological forecasting covers almost all types of forecasts: from short-term flood forecasting to sub-seasonal and seasonal predictions of streamflow characteristics, such as peak flow, spring runoff, inflow into reservoirs and many others. Variety of forecasting models and techniques are being used, based on watershed conceptual models, routing models, and statistical dependencies. The Dynamic Water Resources Assessment Tool (DWAT) was developed by the Republic of Korea as contribution to the WMO activities in hydrological forecasting and water resources assessment and management. DWAT was successfully tested in river basins in different countries. In 2017, the tool was tested under conditions of Russian Federation, for the tributaries of the Volga river basin, where snow dynamics and soil frost play significant part of hydrological regime formation. It was shown that output updating plays significant role in increasing the quality of DWAT simulations and forecasts for river basins in moderate climate with seasonal snowpack formation and its significant influence on the river flow. Application of DWAT together with output updating technique significantly improved simulation quality of daily, as well as monthly streamflow, generated from both rainfall and snowmelt. In 2022-2023, DWAT was applied to the Krasnodar reservoir watershed in order to simulate and forecast daily inflow for the reservoir's operation and management purposes. The river basin is of complex both mountainous and plain nature with flow formation in the Caucasus Mountains, the highest European mountainous range. Successful application of DWAT in different Russian watersheds showed good results and is promising towards implementation into operational forecasting practice of Russian Federation for different aspects of forecasting and water resources assessment.
HS22-A001
Evaluation of Multi-objective PSO and NSGA-II Optimization Algorithms for DWAT Modeling
Wonjin JANG+, Yonggwan LEE, Jeehun CHUNG, Jinuk KIM, Seong-Joon KIM#
Konkuk University
In our research, the objective is to design an automatic parameter calibration algorithm for the Dynamic Water Resources Assessment Tool (DWAT) utilizing Particle Swarm Optimization (PSO) and Non-Dominated Sorting Genetic Algorithm II (NSGA-II). We then evaluated the performance of these algorithms by applying them to the Seomjin, Geum, Youngsan river basin. PSO, a probabilistic optimization method, is inspired by the social behavior of biological swarms, whereas NSGA-II draws its inspiration from natural selection and Darwinian evolution as an optimization technique. DWAT contains multiple parameters that facilitate the simulation of runoff characteristics based on topographical factors, infiltration and evaporation, and groundwater. The parameter optimization algorithms developed are incorporated into Python for enhanced scalability and universality. To account for the spatial and temporal characteristics of each watershed, users have the option to select up to three from nine objective functions (coefficient of determination; R2, modified R2, Nash-Sutcliffe efficiency (NSE), modified NSE, Kling-Gupta efficiency, percent bias, root mean square error, ranked sum of squared error, Chi-squared). The application of PSO and NSGA-II in the automatic parameter calibration of the DWAT model for runoff analysis is anticipated to show higher modeling performance through multi-objective functions and dynamic parameter estimation specific to each standard watershed.
Session Chair(s): Ji CHEN, The University of Hong Kong
HS21-A001
Future Projections of Annual Rainfall from CMIP6 Models in Ho Chi Minh City, Vietnam
Dang NGUYEN DONG PHUONG1,2#+
1Seoul National University, 2Nong Lam University - Ho Chi Minh City
Climate risks have posed a major threat to many local communities settling in low-lying coastal megacities across the globe, including Ho Chi Minh City, Vietnam. Hence, this study aimed to contribute towards a comprehensive understanding of temporal trend patterns of annual rainfall and absolute extremes in Ho Chi Minh City over the last four decades (1980-2022) through multiple non-parametric statistical trend tests. Furthermore, this study employed the quantile delta mapping (QDM) method to develop daily bias-corrected rainfall data based on the outputs in the latest Coupled Model Intercomparison Project phase 6 (CMIP6) under eight shared socio-economic pathway (SSP) greenhouse gas emission scenarios. Evaluation of model performance was implemented by repeatedly leaving successive five years out in turn for estimating testing errors. The outcomes imply the high applicability of well-calibrated transfer functions, even for high quantiles, to the production of future rainfall scenarios. The projected changes in annual rainfall and absolute extremes were obtained by estimating multi-model medians from CMIP6 models for future periods of 2021-2040, 2041-2060, 2061-2080, and 2081-2100 with reference to the base period of 1995-2014. In general, the projections indicate a substantial increase in annual rainfall in Ho Chi Minh City, with Thu Duc Station consistently experiencing the highest increments. Under the high-end scenario (SSP5-8.5) by the end of the twenty-first century, the projected changes at Thu Duc Station are estimated to be approximately 30.9% (ranging from 8.3% to 77.8%). These findings provide a solid foundation for adapting and mitigating climate-related risks in Ho Chi Minh City.
HS21-A002
Similar Flood Dynamic Recognition Method Based on Data Mining
Yinghui LI#+
Seoul National University
The mismatch between flood forecasting lead time and reservoir dispatching period’s demand, and the contradiction between lead time’s length and forecasting accuracy are some of the key problems that restrict reservoir flood control dispatching based on hydrological forecasting. Hence, effectively improving the predictability during the flood generation period is significant for real-time flood control operations. Similar floods play a crucial role in flood control; however, the current static flood similarity identification makes it difficult to meet the dynamic demand of flood control decision-making. Given this, this study took Chitan Reservoir in Jinxi Basin, Fujian Province, China as the study target; extracted the similarity recognition features according to the runoff generation mechanisms, and constructed flood multi-factors time series sets. The study analyzed the essence of similar flood dynamic identification referring to data mining and multi-dimensional time series similarity mining theories and proposed a similar flood recognition method based on the Dynamic Time Warping algorithm (DTW). The method’s good performance in similar flood dynamic recognition has been confirmed. At the same time, we proposed a similar flood dynamic extension approach and blended it with the reservoir optimal operation model to construct a real-time flood control operation method. The research results indicated that a similar flood dynamic extension approach can serve real-time reservoir flood control decision-making at lower risk and guarantee flood control safety upstream and downstream. This research provides a new perspective for real-time reservoir flood control decision-making.
HS21-A003
Simple Physically-based Emulator of ILS (Integrated Land Simulator)
Roman OLSON#+, Kei YOSHIMURA, Tomoko NITTA
The University of Tokyo
ILS (Integrated Land Simulator) is a modelling framework for coupling models on a latitude/longitude grid. ILS is primarily designed for working with land surface models, but is general in its design. ILS currently consists of land surface model MATSIRO, which is coupled to the river routing and floodplain inundation dynamics model CaMa-Flood. In this configuration the coupled model is computationally heavy. This hinders the full uncertainty quantification of river flow to atmospheric forcing under different emissions scenarios. This also makes it more challenging to couple ILS to other Earth system model components, and to economic models. Recently, a fast physically-guided emulator of MATSIRO has been developed (Olson et al., in revision). It approximates daily-scale snow water equivalent, wetland water storage, top layer soil moisture, and runoff in MATSIRO using simplified equations. Here we present the ILS emulator that couples MATSIRO emulator with CaMa-Flood. As with the MATSIRO emulator, the input is daily atmospheric forcing: snowfall, rainfall, surface pressure, specific humidity, and atmospheric temperature. The output contains the original MATSIRO emulator output, as well as CaMa-Flood output, such as daily river stage, discharge, and flow velocity. We validate the ILS emulator discharge and stage vs. gauge and/or satellite observations and compare the emulator performance to the original ILS' performance. We discuss the transferability of MATSIRO emulator parameters to the ILS emulator. Furthermore, we compare the speed of the ILS emulator compared to the original ILS. We discuss the challenges of coupled soil and river routing simulation using the emulation technique. Finally, we discuss the areas where the ILS emulator can be applied and outline possible avenues for future research. Reference: Olson, K. Yoshimura and T. Nitta (in revision): A fast physically-guided emulator of MATSIRO land surface model. In revision at Journal of Hydrology.
HS21-A008
Spatiotemporal Projections of Precipitation in the Mekong River Basin Based on Regional Climate Model
Nam DO HOAI1#, Long TRINH-TUAN1+, Toan TRINH QUANG1, Van Thinh NGUYEN2, Hoa TRAN DINH1, Thao NGUYEN THI THU1, Anh TRAN PHUONG1, Tien NGUYEN THUY1
1Vietnam Academy for Water Resources, 2Seoul National University
In this study, future precipitation in Mekong River Basin (MRB) was projected using the Regional Climate Model (RegCM) driven by CNRM-ESM2-1, a Coupled Model Intercomparison Project Phase 6 (CMIP6) climate model. To address biases in the simulated precipitation over the MRB from the Regional Climate Model products, Quantile Mapping (QM) was employed for model bias correction. When compared to the original model outputs during the independent validation period, the QM technique resulted in a substantial reduction in bias and noteworthy improvements in representing precipitation indices. Across both future scenarios, there was an observable increasing trend in precipitation throughout the MRB. In particular, annual precipitation anomalies for 2070-2099 were 96 mm and 137 mm for the SSP245 and SSP585 scenarios, respectively. During spring and winter, precipitation exhibited a slight increase in the northern MRB but decreased in the southern MRB. Conversely, during summer and autumn, there was a significant and widespread increase in precipitation across almost the entire basin. Regarding daily rainfall, there is a significant increase of 5-10% in the number of days with precipitation exceeding 20 mm/day under the SSP585 scenario in the period from 2070 to 2099. It has been found significant alterations in the spatial distribution of future precipitation. Areas with annual precipitation exceeding 2400 mm and 1800 mm (westside of Annamite range) exhibited outward expansion in a circular pattern. Additionally, the central region with annual precipitation exceeding 1500 mm shifted westward, indicating an expansion of areas with annual precipitation exceeding 2400 mm and 1800 mm. In contrast, dry-season precipitation, as represented by the 400 mm isohyet, contracted primarily in a circular pattern toward the center. These changes suggest a contraction of areas with dry-season precipitation.
HS21-A009
Regionalization of Optimal Baseflow Separation Using Catchment-scale Characteristics
Yongen LIN#+, Dagang WANG, Yiwen MEI
Sun Yat-sen University
Baseflow, as an integral component of a river's flow, plays an indispensable role in replenishing water supplies and preserving the ecological balance of riverine environments. However, the process of determining baseflow is currently riddled with uncertainties, posing limitations to our thorough understanding of baseflow dynamics. In this study, we utilize daily streamflow records, specific electrical conductance records, and chemical mass balance theorem to calibrate the optimal parameters of the smooth minima baseflow separation method (SMM) in 857 watersheds over the Continental United States (CONUS), and then develop a regionalization model for the optimal SMM using random forest (RF) algorithm and 57 catchment-scale characteristics. In this way, we can extend the optimal baseflow separation to watersheds without tracer records. The results show that the RF prediction for the optimal parameters of SMM achieves an R2 of 0.76. Based on this, our regionalization model yields more reliable daily baseflow separation results compared to the traditional SMM, with the median Kling-Gupta Efficiency (KGE) increasing from 0.67 to 0.84 over 857 watersheds. The feature sensitivity analysis reveals that watershed area has the most significant impact on baseflow separation results, followed by hydro-meteorological characteristics of the watershed. The influence of soil properties on the outcomes is also found to be non-negligible. Based on our regionalization model, we further establish a baseflow dataset containing near 9000 watersheds over CONUS. This study can offer valuable insights for more accurate and reliable separation of baseflow from total flow, laying a solid foundation for understanding the dynamic processes in baseflow.
HS21-A015
Spatial-temporal Characteristics of Soil Erosion During Typhoon Events Over the Pearl River Basin
Xiao FENG#+, Ji CHEN
The University of Hong Kong
The Pearl River Basin (PRB) is confronted with the risks posed by tropical storms, particularly in the Guangdong-Hong Kong-Macao Greater Bay Area (GBA), which suffers significant economic losses due to typhoons. Between 2008 and 2018, an average of 5.5 tropical storms made landfall or passed through the PRB, resulting in around 34 typhoon days each year. These typhoons typically hit South China from Guangdong Province, leading to not only excessive precipitation but also increased soil erosion within the basin. Consequently, there is an urgent need to investigate the spatial and temporal patterns of soil erosion during typhoon events. To assess the impact of typhoons on soil erosion, the study employs the Soil and Water Assessment Tool (SWAT) to simulate hydrological processes across the PRB. The analysis focuses on the multi-year average rainfall and soil erosion data (2008-2018) from the PRB and its three major subbasins. It is observed that soil erosion exhibits spatial and seasonal variations in different subbasins, with steeper and longer slopes experiencing higher erosion rates, particularly at the start of the wet season when runoff increases. The study reveals that, on average, the GBA receives a greater proportion of annual rainfall during typhoons (17%) compared to the PRB as a whole (14%). Similarly, the ratios of soil loss are 17% in the GBA and 16% in the entire PRB. Furthermore, soil erosion displays interannual differences depending on the landing locations and the affected areas of different typhoons.
HS21-A021
An Improved Approach of Rainfall Runoff Modelling Using Fuzzy Logic
Ayushi PANCHAL#+, Sanjaykumar YADAV
Sardar Vallabhbhai National Institute of Technology
The runoff prediction in extreme climate change has become rigorous and the accurate estimate of surface runoff is required for water resources management. The most challenging aspect for the hydrologists as well as engineers is to generate the robust relationship between rainfall-runoff. There are various techniques including physically based model, conceptual hydrologic models along with the soft computing techniques used for developing relation between rainfall and runoff. A soft computing technique Fuzzy logic is the most flexible and simplest approach to implement for the river basins for predicting the flood. The present study evaluates performance of fuzzy logic approach using Mamdani Fuzzy Inference System. The model has been developed using fuzzy logic having inputs of rainfall data and evaporation data to determine the runoff at catchment outlet. The performance measures like MAPE, NRMSE, R-squared correlation, Pearson’s correlation co-efficient and Nash Sutcliffe coefficient of Efficiency (NSE) were determined to evaluate the performance of developed model. The outcomes show that, the developed fuzzy logic model performs well and gives supplementary accurate results according to the observed data. The performance and efficiency of the developed model implies the potential to establish a reliable runoff prediction system. The fuzzy logic-based rainfall runoff models without metrological or topographical parameters results in to reasonable accuracy. Fuzzy logic-based rainfall runoff models are flexible, easy to use and required less time to run.
HS21-A022
Heteroscedastic Extended Logistic Regression for Statistical Postprocessing of Ensemble Precipitation Forecasts
Rashmi YADAV#+, Sanjaykumar YADAV
Sardar Vallabhbhai National Institute of Technology
Prediction of the exact state of the atmosphere is physically not possible. The predicted parameters such as precipitation, temperature, wind, surface pressure, etc are generated by various ensemble prediction systems around the world. The statistical postprocessing of these quantitative predictions is carried out to improve the forecasts following the observed data. In the present study, the Heteroscedastic Extended Logistic Regression (HXLR) method of statistical postprocessing is applied to the 1-5 day lead time forecasts of the European Centre for Medium-Range Weather Forecast (ECMWF) for the Vishwamitri River basin. The ECMWF precipitation dataset from Aug 2008 is calibrated with the observed precipitation of the India Meteorological Department (IMD) gridded dataset at the resolution of 0.25*0.25. The data is divided into training (up to 24 Jul 2019) and testing datasets (25 Jul 2019 to 30 Sep 2021) for fitting HXLR. The probabilistic metrics Brier Score (BS) and area under the curve (AUC) of the receiver operating characteristics curve were used for the verification of the post-processed precipitation of ECMWF. After the postprocessing of the ensemble precipitation forecasts, the average BS of below 0.15 is observed for 1-5 days lead time. Similarly, the forecasts were improved showing a good AUC of above 0.85 for the lead time of up to 5 days forecasts by ECMWF. The statistically post-processed ensemble precipitation forecasts may serve as the input to drive a hydrological model for generating reliable flood forecasts at a lead time of up to 5 days.
Session Chair(s): Jonghun KAM, Pohang University of Science and Technology
HS09-A015
Attribution Study of Global Water Mass Transition Over the Past Two Decades Based on Multivariate Climate Indicators
Wenxi ZHANG+, Shanshan DENG#, Yuxin LIU, Ange HU
Guangxi University
Climate indices are widely recognized as significant influencing factors on water mass transition. Recent research indicates that the El Niño-Southern Oscillation (ENSO) is a primary driver of the decline in land freshwater availability. However, a single climate index is insufficient to explain the impact of climate variability on the hydrological cycle; multiple climate indices should be incorporated for analysis. We need a comprehensive analysis to clarify their spatio-temporal characteristics and physical mechanisms. The Gravity Recovery And Climate Experiment (GRACE) satellite data allows for the study of the relationship between climate variability and water storage. This study employs stepwise regression and random forest approaches to investigate the relationship between water mass transition and multivariate climate indices. We identified the climate indices which most significantly drive interannual-scale water mass migration from a global to a regional scale. Then we depicted the spatio-temporal patterns of land-sea water migration induced by key climate indices. We found that ENSO dominates the water mass change across most oceanic and mid-latitude inland regions. The Southern Hemisphere Annular Mode(SAM) exerts a triggering effect on water quality migration in high latitudinal regions of the Southern Hemisphere, while Arctic Oscillation significantly influences high-altitude regions globally. This study elucidates the driving mechanisms of climate indices on the hydrological cycle, contributing to the enhancement of global resource forecasting capabilities.
HS09-A003
Observational Evidence of the Gap Between the Risk and Awareness of Global Droughts
Murtaza Ahmad DAR+, Jonghun KAM#
Pohang University of Science and Technology
Drought is a pervasive natural hazard, causing devastating impacts on ecosystems and human societies around the world. A comprehensive study of global drought dynamics and corresponding public awareness is warranted for effective drought mitigation. This study examines a connection between drought events and public awareness using big social monitoring data. By integrating meteorological data, passive social monitoring via Google Trends, and advanced statistical analysis, this study addresses the multiple aspects of the drought from 2010 to 2021, including the characterization of past drought events (e.g., intensity and duration) as well as the dynamic evolution of public awareness. Our results show significant peaks in global drought events, particularly in 2015–2016 and 2019–2020, which correlate closely with an increase in public awareness from 2015 onwards. The result highlighted the pronounced gap between the frequency of drought events and the corresponding level of public awareness, mainly in developing countries. This study sheds light on the influential role of temporary recovery periods in shaping search behavior. This interdisciplinary study not only provides empirical evidence highlighting global differences in public interest in drought but also highlights its significant impact. As our climate continues to evolve, the insights gained from this study become paramount and urge policymakers worldwide to adopt proactive strategies and interventions to promote resilience and sustainability in the face of escalating environmental challenges. Conclusively, this study emphasizes the importance of a holistic understanding of the complex interplay between environmental change and societal awareness.
HS09-A014
Exploring Large-scale Flood Disaster Social Vulnerability in Taipei: A Self-organizing Map Approach
Tsung-Yi PAN1#+, Lo-Yi CHEN1, Jing-Ting WANG2, Hung-Chi KUO1
1National Taiwan University, 2Taipei City Fire Department
This study utilizes Self-Organizing Maps (SOM) to assess social vulnerability to flooding in Taipei City across 456 villages. Through the integration of large-scale flood potential simulations, the research provides detailed spatial insights into vulnerability patterns. These findings play a pivotal role in guiding targeted non-engineering disaster resilience initiatives, optimizing resource allocation for authorities and stakeholders. As climate change intensifies, the significance of these insights becomes more pronounced, contributing substantially to ongoing urban disaster risk reduction efforts. The research fosters the development of a more resilient urban environment capable of effectively navigating the challenges presented by a dynamically changing climate. In conclusion, the proactive and adaptive strategies informed by this research aim to build a city better prepared to confront and overcome the complexities of a shifting climate landscape. The study underscores the importance of continual efforts in enhancing Taipei City's preparedness and response strategies, ensuring sustainable and resilient urban development in the face of future flood-related challenges.
HS09-A016
Contrasting Changes in Extreme Snowmelt and Spring Flood Risk Across the United States
Eunsang CHO1#+, Jennifer JACOBS2, Carrie VUYOVICH3
1Texas State University, 2University of New Hampshire, 3NASA Goddard Space Flight Center
Snowmelt is a critical source of water but also a key driver of floods in regions with seasonal snow cover around worldwide. Recent spring floods, including snowmelt and rain-on-snow events along with the saturated soil moisture conditions, have had significant societal and economic impacts on communities across the U.S. However, the magnitude and direction of historical extreme snowmelt change are poorly known, especially in the north-central and northeastern U.S., where the relatively shallow snowpack is understudied by snow researchers. In this study, annual maximum snowmelt events are investigated from 1982 to 2022 across the continental U.S. These events are calculated from snowpack depletions using the observation-based 4-km gridded snow water equivalent product. We find contrasting changes in extreme snowmelt events between western mountainous regions and north-central regions. While there was a widespread reduction in extreme snowmelt over the western U.S., extreme snowmelt rates increased over the north-central U.S. Our findings provide strong evidence of enhanced snowmelt coinciding with the recent remarkable increases in streamflow and frequent spring flood events in the north-central U.S.
HS09-A004
Human Sensors of the Ongoing Drought from News and Social Media: A Case Study of the 2022/23 South Korea Drought
Seunghui CHOI+, Anqi LIU, Jonghun KAM#
Pohang University of Science and Technology
Exceptional droughts deteriorate socioeconomic losses and the mental health condition of the public, such as a spike in suicide rates or a surge in depression. Previous drought monitoring systems have focused on the physical condition of an emerging drought. Associated with physical measurements of drought, this study utilizes unstructured text data from news headlines and social media blogs as a sensor to detect the drought impacts. This study acquires over 15,000 local news articles in Naver and over 0.7 million X (formerly Twitter) posts from January 2020 to May 2023 using the keyword “Drought” in Korean. A Korean-based Natural Language Processing model trained by Korean Online That-gul Emotions (KOTE) is used to classify the textual data into 44 emotional states, including 25 negatives, 14 positives, four neutrals and one special emotion labeled as “No emotion”. The contributions of 16 regions to the national search activities volumes from Google Trends are used to disaggregate X data. The self-calibrating Effective Drought Index (scEDI) is calculated from the precipitation data, as an indicator of the drought. The emotions from both news and social media before and during drought are compared for comprehending social impact. Results show that both Naver news and X data witnessed a sharp increase during June 2022, according with the nadir of scEDI. Almost half Naver news are labeled as “No emotion” (42.8%), followed by positive (29.5%), and negative (21.5%). In contrast, X posts presents a higher percentage of negative emotions with 58.5%. Negative emotions of both Naver news and X posts experienced an expansion during drought, which mainly appear on populated and developed regions for X weighted by Google Trends regional contributions. This study emphasizes the importance of an interdisciplinary approach in improving drought response and mitigation plans, proposing the next generation drought monitoring system including emotion-focused coping.
HS09-A010
Monitoring the Impact of Climate Extremes and COVID-19 on the Public’s Sentiment Alteration in Water Pollution Complaints
Anqi LIU1+, Jonghun KAM1#, Sae Yun KWON1, Wanyun SHAO2
1Pohang University of Science and Technology, 2University of Alabama
Changing climate has increased the frequency of extreme events, such as floods and droughts, facing severe water scarcity and security challenges. The COVID-19 pandemic has restricted outdoor activities and reshaped public perceptions of environmental risks. Both climatic extremes and pandemic have been found to alter emotion and attitude of the public, resulting in degraded public physical and mental health. In contrast to traditional water monitoring systems, this research integrates public surveillance and focuses specifically on water pollution complaints to investigate the sentimental impact of climatic extremes and COVID-19 pandemic. This study leveraged over 9,900 water-related complaints from 2012 to 2020, which was available from the Alabama Department of Environmental Management. Utilizing the TextBlob package, the study computed polarity and subjectivity scores of these complaints and categorized them into different emotion and attitude types based on the scores. In addition, the bootstrapping was performed to assess the uncertainty of the corresponding sentiment alteration during specific events. The findings revealed that well-developed counties with substantial populations and high GDP level significantly contributed to half of the complaints. Socioeconomic development also played a role in sentiment alterations with opposite response in attitude during the flood event. Drought events increased negative complaints up to 35% with little alteration in attitude. During the COVID-19 pandemic, the complaints experienced increased positive and subjective complaints on a state level, emphasizing a broader impact of the pandemic on emotion and attitude toward water quality than that of extreme events. This study confirmed that the Alabama complaint platform is a valuable participatory surveillance system and applied Natural Language Processing to explore the potential of natural language process in advancing the current water monitoring and management system integrating emotion-focused coping. This research highlighted the value of citizen-participant in improving strategies of environmental governance and shaping effective water resource management.
HS09-A005
Hybrid Approach of Physics-informed Deep Learning Modelling to Assess the Record-breaking Hydroclimate Extreme Events Over Pakistan
Hassan RAZA+, Jonghun KAM#
Pohang University of Science and Technology
Record-breaking (RB) events are unprecedented values given the record dataset of field of interest such as temperature or streamflow. Climate change-driven surface warming has made these RB extreme events as usual events. Changes in precipitation patterns, varying temperature trends, and glacier-melt freshwater fluxes can change the frequency of record-breaking hydrological extremes (RBHE). Pakistan with many other countries around the globe is vulnerable to climatic changes and severely facing the consequences. The 2010 and 2022 floods displaced approximately 30 million individuals and caused staggering economic losses amounting to around 30 billion USD. On the contrary, the 2001 and 2017 droughts also had a profound impact on devastating irrigated agriculture. However, the timing and frequency of these RB hydrological extremes are yet not fully understood, particularly over the future. Timely prediction and understanding of these unprecedented hydrological extremes can lessen their impact. Early preparedness can leverage the secure and sustainable future of escalating 240 million lives. This study conducts a physics-guided deep learning approach to model the RBHE analysis to overcome the limitations of the conventional approaches including uncertainties in climate model projections. This study focuses on RBHEs defined from annual maximum and annual minimum streamflow and investigates the risk of wetting and drying RBHEs in the RCP 4.5 & RCP 8.5 radiative forcing scenarios from five regional climate models. Results showed that the Indus and Jehlum rivers exhibit relatively higher RBHE for annual max. flow as compared to annual min flow for wetting and vice versa for drying scenarios. However, Chenab and Kabul Rivers reflected an equal probability of RBHE for wetting and drying conditions. This study also found different emerging time of climate change attribution for RBHEs. This study suggests the potential of a hybrid approach in record-breaking extreme events detection and attribution.
Session Chair(s): Yusuke HIRAGA, Tohoku University
HS51-A011
Heavy Precipitation-high Temperature Events Under a Warming Climate: Characteristics, and Future Projections
Wenlu LI+, Haiyun SHI#
Southern University of Science and Technology
The spatial and temporal aggregation of high temperature and heavy precipitation can significantly amplify climate risks, surpassing the sum of their individual impacts on society and ecosystems. In this study, we identify and capture global heavy precipitation-high temperature events using GLDAS-CLSM daily-scale data through the relative threshold method and run path algorithm. We analyze the spatiotemporal evolution and seasonal characteristics of the long-term time series from 1948 to 2014. Our findings reveal spatial heterogeneity in response to global warming for heatwaves, heavy precipitation, and the compound events. From 1948 to 2014, approximately 83.8% of the global land mass witnessed an increasing trend in the occurrence frequency of heavy precipitation-high temperature events. During the period of 1948-2014, there was an increasing trend in the occurrence frequency of heavy precipitation-high temperature events on approximately 83.8% of the global land mass. High-risk areas with significant heavy precipitation-high temperature event occurrences exceeding 99% are concentrated in low latitudes near the equator, Western Europe, and western coastal areas of North America. Additionally, heavy precipitation-high temperature events exhibit higher occurrence frequencies in mountain ranges and plateau regions. Regarding seasonal characteristics, the compound events in June to August exhibit a more rapid fluctuation frequency for both heatwaves and heavy precipitation events. In December to January, on a global land scale, the proportion of risk hotspots affected by heavy precipitation-high temperature events is the highest. This study holds significant importance in effectively reducing the disaster chain impact of heavy precipitation-high temperature events and ensuring social and economic stability as well as sustainable development.
HS51-A004
Extreme Rainfall Estimation by Urban Surveillance Cameras
Xing WANG#+, Kun ZHAO
Nanjing University
Extreme rainfall often cause flooding, waterlogging, and landslides, exceptionally threatening urban development and human lives. Rainfall observations with high resolution are essential for disaster mitigation and prevention. However, the current rainfall observation systems have difficulty producing rainfall data with relatively high resolutions, specifically: As the most fundamental means, rain gauges provide ground-level, high-temporal-resolution rainfall observations. However, limited by excessive costs, high-density gauge networks are difficult to deploy, which leads to insufficient spatial representation of their observations; Remote sensing techniques, i.e., weather radar and satellites, can obtain relatively high spatial data widely used for weather observation tasks. Nevertheless, such measurements suffer from the intrinsic weakness of the principle and needs to be calibrated and validated by ground-level measurements. Therefore, a high-resolution, low-cost, ground-level rainfall observation network is not yet well-built. With the advantages of high spatial-temporal resolution, rainfall estimation by surveillance cameras is highly suitable for meteorological-related research and has bright prospects. In this study, from the viewpoint of surveillance sound space, a 3D printer was used to create a shelter for the surveillance camera to define the underlying surface of falling raindrops artificially. Combining the knowledge of meteorology, micro-physics, and acoustics of rainfall, the shelter structure was designed to standardize the acoustical behavior while enhancing the consistency and specificity of raindrop sound, especially in complex scenarios such as those disturbed by different levels of wind. After that, a CNN-based deep learning algorithms was used to classify extreme rainfall levels, and an audio-based extreme rainfall classification system was built. The experimental results show that the shelter facilitates audio-based rainfall representation; with the help of the shelter, our system achieved performance with 93.4% accuracy in extreme rainfall scenarios. Our study supports high-resolution rainfall data production on existing surveillance resources, developing a novel and reliable alternative for the perception of extreme rainfall.
HS51-A002
Response of Band-shaped Rainfall to Changes in Atmospheric Moisture in Tohoku, Japan
Yusuke HIRAGA#+, Ryotaro TAHARA, So KAZAMA
Tohoku University
This study aims to investigate the response of the band-shaped heavy rainfall to changes in atmospheric moisture using the Weather Research and Forecasting (WRF) model. The 2022 August heavy rainfall event in Tohoku, Japan was targeted for the analysis. We performed the simulation of the target event using various physical parameterizations and initial and boundary conditions to accurately simulate the rainfall. The use of the Goddard microphysics scheme with the Grenier–Bretherton–McCaa Scheme resulted in reasonable accuracy in the 48-hr basin-average precipitation depths. This study then perturbed the moisture supply in the initial and boundary conditions in the simulation to examine the effect of moisture changes on the rainfall pattern. The moisture amount and transport trajectory were modified to represent the different moisture supply conditions. Our analysis showed that the band-shaped rainfall pattern was significantly altered when the moisture supply changed, suggesting the importance of closely examining the moisture conditions for climate change and PMP studies. Additional studies performing similar analyses for different rainfall events are needed to generalize the responses.
HS51-A005
Evaluations of Different Precipitation Products' Performances and Their Effectiveness in Disaster Warning Across the Tibetan Plateau
Li ZHOU#+, Yibo DING
Sichuan University
The Tibetan Plateau, often refeered to as Asia’s water tower, is a focal point for studying spatiotemporal changes in water resources amidst global warming. Precipitation is an important supply of water resources to the Tibetan Plateau. Precipitation information is of great significance to support research on the Tibetan Plateau. In this study, we estimate the performance and applicability of Climate Prediction Center Merged Analysis of Precipitation (CMAP), Integrated Multi-Satellite Retrievals for Global Precipitation Measurement (IMERG), and Global Land Data Assimilation System (GLDAS) precipitation products in precipitation prediction and different disaster scenarios (including extreme precipitation, drought, and snow) over the Tibetan Plateau. Extreme precipitation and drought indexes are used to describe extreme precipitation and drought conditions. Statistical metrics are used to estimate and compare the performances of different precipitation products. The results show that (1) CMAP and GPCP precipitation products generally showed great and poor performance in predicting precipitation and disaster scenarios (including extreme precipitation and meteorological drought), respectively. IMERG also showed great performance and was slightly inferior to CMAP in the Tibetan Plateau. (2) R95p, R99p, Rx1day, and Rx5day could be better predicted by precipitation products. R10 and R20 could be badly predicted by precipitation products. (3) Different precipitation products showed that the bias of drought prediction increased as the time scale increased. (4) GLDAS series products showed that liquid precipitation could be better predicted than mixed and snow precipitation. (5) False alarms could have a greater bias of precipitation amount than correct alarms among different precipitation products. The findings of this study contribute to uncovering the performance variations among different precipitation products and identifying potential factors contributing to biases within these products. Additionally, the study sheds light on disaster characteristics and warning systems specific to the Tibetan Plateau.
HS51-A007
Development of Attention-based Multimodal Deep Learning Model for Water Level Prediction
Seongsim YOON1#+, Sangmin BAE2, Seyong KIM2
1Korea Institute of Civil Engineering and Building Technology, 2Hanyang AI Solution Center
This study presents the development of an innovative attention-based multimodal deep learning model for water level prediction, integrating 2D grid radar rainfall data and 1D time-series water level observation data. Traditional water level prediction models primarily rely on time-series data from water level stations, often overlooking the critical impact of rainfall information, particularly within a watershed. Our model addresses this gap by utilizing radar data to directly measure rainfall, enhancing prediction accuracy. The proposed model combines the strengths of Convolutional Long Short-Term Memory (ConvLSTM) networks for processing spatial-temporal radar data, standard LSTM networks for handling time-series water level data, and the Bahdanau attention mechanism for dynamic data integration. The ConvLSTM component captures precipitation dynamics crucial for understanding rainfall patterns, while a linear layer transforms water level data into a format suitable for the LSTM decoder. This decoder operates in both unidirectional and bidirectional modes, incorporating the Bahdanau attention mechanism to focus on relevant radar data segments, thereby refining prediction accuracy at each time step. This model was trained and validated using 10-minute interval data from May 2019 to October 2021, including water level data from three stations and radar rainfall data from the Ministry of Environment to apply the upper basin of the Hantan River. The proposed technique demonstrated more accurate water level predictions compared to the conventional single modal model. This study demonstrates the effectiveness of integrating heterogeneous data types, particularly for enhancing the accuracy and reliability of water level predictions. Acknowledgement : This paper was carried out under the KICT Research Program (project no. 20230155-001, Development of future-leading technologies solving water crisis against to water disasters affected by climate change) funded by the Ministry of Science and ICT.
HS51-A012
Compound Droughts and Floods at the Global Scale
Xiaogang HE#+, Hui-Min WANG
National University of Singapore
Spatial and temporal concomitant drought and flood events amplify the impact of individual episodes, but have not been systematically assessed, especially at the global scale. Harnessing the latest advances in complex network theory and event coincidence analysis, we identify the temporal trends and spatial hotspots of such compound extremes based on global climate forcing and land surface model simulations for the past seven decades (1950–2016). For temporally lagged extremes, we find that globally, about 5.9% and 7.6% of the land surface have experienced statistically significant (p<0.10) drought-pluvial seesaw behavior during the boreal spring-summer and fall-winter seasons, with an average of 11.1% and 11.4% of all droughts being followed by pluvials in the following season, respectively. For spatially synchronized extremes, we find that concomitant extremes with large spatial footprints can occur in many distant region pairs, not necessarily clustered in adjacent pixels, such as the simultaneous occurrence of extreme floods over southeastern Australia and southern Africa, and the simultaneous occurrence of extreme droughts over northern India and eastern Africa. Our novel data-driven approaches can help improve the understanding of the physical processes that drive the occurrence of these compound extremes. They can also inform policymakers and local stakeholders on the often overlooked but important risk of concomitant droughts and floods and therefore help design more effective water and agricultural management and adaptation plans.
HS51-A009
How Climate Change and Groundwater Extraction Will Shape the Future Global Terrestrial Water Cycle Pattern
Binghao JIA#+
Chinese Academy of Sciences
Human groundwater exploitation alters hydrological processes, subsequently influencing climate through land-atmosphere interactions. As socio-economic development progresses, the escalating water demand exacerbates conflicts with limited water resources. Nevertheless, the spatial-temporal changes in the global terrestrial water cycle under the combined impacts of climate change and groundwater extraction remain poorly understood. This study developed human water regulation projection schemes based on Shared Socio-economic Pathways (SSPs) and Representative Concentration Pathways (RCPs) scenarios, integrated into a global climate model (CAS-FGOALS-g3). Results show that irrigated area expansion predominantly governs changes in irrigation water use and industrial water demand is closely associated with manufacturing production and water use intensity. In addition, warmer temperatures lead to increasing evapotranspiration and reducing surface runoff and surface soil moisture, with more pronounced changes in medium and high scenarios. Groundwater extraction has a more pronounced impact on surface runoff in high-emission scenarios (SSP370 and SSP585), driven by increasing industrial and domestic water use due to population growth and industrial development. Major irrigated areas experience excessive groundwater extraction leading to declining groundwater storage. In northern India, the cooling effect of groundwater extraction weakens under medium emission scenarios (SSP245 and SSP460) in the mid-to-late 21st century, coinciding with stabilization in irrigation water usage and a reduction in irrigated area under these scenarios. This study underscores the complex interplay between human water use and hydroclimate within an evolving environment, emphasizing the critical need for effective water resource management to mitigate future water stress.
Session Chair(s): Jongmin PARK, Korea National University of Transportation
HS52-A021
| Invited
Variability of the Maritime Continent Intertropical Convergence Zone During the Past 30,000 Years
Xianfeng WANG#+, Shufang YUAN
Nanyang Technological University
The intertropical convergence zone (ITCZ) plays a key role in regulating tropical hydroclimate and global water cycle through changes in its convection strength, latitudinal position and width. The long-term variability of the ITCZ, along with the corresponding driving mechanisms, however, remains obscure, mainly because it is difficult to separate different ITCZ variables in paleoclimate proxy records. Here we compare speleothem oxygen isotope (δ18O) records from the Maritime Continent. Using the spatial gradient of speleothem δ18O along a transect across the ITCZ, we constrain ITCZ variabilities over the Maritime Continent during the past 30,000 years. We find that ITCZ convection strength overall intensified from the last glacial period to the Holocene, following changes in climate boundary conditions. The mean position of the regional ITCZ has moved latitudinally no more than 3o in the past 30,000 years, consistent with the deduction from the atmospheric energy framework. However, different from modern observations and model simulations for future warming, the ITCZ appeared narrower during both the late Holocene and most part of the last glacial period, and its expansion occurred during Heinrich stadials and the early-to-mid Holocene. We also find that during the last glacial and deglacial period, prominent millennial-scale ITCZ changes were closely tied to the variability of the Atlantic meridional overturning circulation, whereas during the Holocene, they were predominantly modulated by the long-term variability of the Walker circulation.
HS52-A020
Temporal and Spatial Patterns of Rain Isotopic Composition in a Coastal Hilly Region for Tracing Hydrological Processes
Huade GUAN1#+, Xiang XU2, Xinping ZHANG3, Erick BESTLAND1, Grzegorz SKRZYPEK4, Andrew LOVE1, Craig SIMMONS5
1Flinders University, 2Lanzhou University, 3Hunan Normal University, 4The University of Western Australia, 5The University of Newcastle
Hydrogen and oxygen isotopic composition of water, and their derived variables, work as ideal environmental tracers of hydrological processes in the environment. Knowledge of temporal and spatial patterns of rain isotopic composition is required for using these isotopic variables to trace water movement in a catchment. Some event isotopic composition extremes, if predictable, can provide opportunities to design specific sampling plans for investigating dynamic rainfall-runoff generation processes. This presentation is based on a few published studies on temporal and spatial patterns of isotopic composition of precipitation in the Mount Lofty Ranges of South Australia, together with the explanations of physical processes resulting in these patterns. Applications of using these patterns in investigating root zone moisture replenishment, rainfall-runoff generation, and groundwater recharge sources, will be demonstrated.
HS52-A016
| Invited
Holocene Typhoon History Recorded by Leaf Wax N-alkane Hydrogen Isotopes in a Subtropical Marr Lake
Guodong JIA#+, Jiantao CAO
Tongji University
The coastal region of South China is in the typical East Asian monsoon zone. Precipitation isotope records have been intensively used in the reconstruction of the East Asian summer monsoon history, but there is a lack of such a record in the coastal South China. A record of leaf wax n-alkane hydrogen isotope (δDwax) reflective of Holocene precipitation δD, from a marr lake in the coastal South China, was extracted in this study. The carbon isotope record of leaf wax n-alkanes from the same sediment core has been published and exhibits a humid climate from 9.2 to 1.8 ka, with a drying climate in the time periods before and after that. However, the δDwax record in this work does not agree with the above wet and dry variations, and even, contrary to what is commonly understood, exhibits higher values during 9.5-3.2 ka and lower values during other time periods. This is also distinct from the stalagmite isotope record that reflects the history of East Asian summer monsoon changes. We believe that the pattern of precipitation δD variations in the study area may have been strongly influenced by typhoon precipitation, which is a major feature of the coastal South China. Nowadays, δD values of typhoon precipitation (~57‰) are significantly lighter than those of monsoon precipitation (-39‰) and non-monsoon precipitation (-15‰) under normal conditions. Thus the δDwax records in this study should reflect the contribution of typhoon precipitation to the annual rainfall, i.e., typhoon precipitation decreased during the middle-late Holocene between 9.5-3.2 ka in the coastal South China, despite the humid climate, and increased during the early and late Holocene. This pattern of typhoon change in the Holocene may be related to the thermal state of the equatorial Pacific in some way.
HS52-A015
Tracer Applications with Highly Enriched and Depleted Deuterium Samples Using the Picarro CRDS Water Isotope Analyzer
Jinshu YAN#+, Thomas GOTTSCHALK, Joyeeta BHATTACHARYA, Magdalena E. G. HOFMANN, Jan WOŹNIAK
Picarro Incorporated
The precise measurement of highly-depleted and enriched deuterium samples has posed a persistent challenge in hydrological research. The 2H/1H ratio serves as tracer in highly enriched δH water isotope samples, enabling the tracking of hydrological pathways and biological activities. In contrast, the analysis of deuterium-depleted waters may be necessary for tracing the origin and movement of ground water or identifying Paleowater. Picarro water isotope analyzers (L21x0-i) have become a standard method for measuring the natural abundance of δO, δH, and O-excess in water isotopes. Memory effect and spectroscopic limits are two major challenges for measuring highly enriched and depleted water using Cavity Ring Down Spectroscopy. Here, we address both challenges by characterizing the memory effect for highly enriched/depleted δH samples with Picarro express mode, which provides a faster rate for efficient memory reduce/remove compared to the standard mode and by determining the spectroscopic limits of the analyzer. In this study, we tested the performance of the Picarro analyzers for a set of enriched samples with varying 2H/1H ratios of 0.1 to 2.0% (corresponding to δH values of about 6,000 to 130,000‰) and depleted samples 5 ppm and 10 ppm (corresponding to δH values of about -967‰ and -935‰). We found that (i) the analyzer shows an excellent linearity over a high and low δH range; (ii) the analyzer shows a negligible concentration dependence at high enrichment levels; (iii) the spectroscopic limits of the analyzer can be extended by reducing the injection volume (<1.8uL); (iv) the memory effect can be reduced significantly when using the express mode compared to the standard mode. Our results demonstrate the Picarro L21X0-i water isotope analyzer's excellent effectiveness in measuring both highly enriched and depleted δH water samples. In this presentation, we will cover optimal methodologies for these measurements.
HS52-A002
A Novel Transformer-based Architecture for Future Soil Moisture Prediction Using LDAS
Roberto CHANG-SILVA+, Byeongcheol KIM, Kyungil LEE, Seonyoung PARK#
Seoul National University of Science and Technology
Soil moisture prediction is crucial for understanding environmental issues and hydrological conditions. This study addresses a research gap by proposing a novel soil moisture prediction architecture based on the Transformer model, planning to use the North American Land Data Assimilation System (NLDAS) dataset. Motivated to enhance predictive accuracy, our approach leverages the Transformer's self-attention mechanism, dynamically weighing different positions in the input sequence. This is expected to capture temporal dynamics in soil moisture patterns. The use of multi-head attention mechanisms aims to improve the model's capacity to discern relationships within the data for better accuracy in soil moisture predictions, contributing to understanding environmental processes. The LDAS dataset, a rich repository of land surface observations, serves as the cornerstone, facilitating model training and validation across various geographical and climatic domains. As we design this forecasting architecture, our work represents a critical step towards proactive hydrological management. By refining future soil moisture predictions, we aim to lay the groundwork for a more anticipatory approach to environmental diagnosis, contributing to the discourse on advanced deep learning in hydrological forecasting and potential implications for sustainable water resource management practices.
HS52-A004
Toward Assimilation of Grace Terrestrial Water Storage Into a Land Surface Model for Hydrological Extreme Monitoring and Forecasting in the Texas-gulf Basin
Gaohong YIN1#+, Kei YOSHIMURA2
1Jilin University, 2The University of Tokyo
Floods and drought are global issues causing devastating damage to the ecosystem, human lives, and economics. Current flood and drought studies are heavily based on precipitation, whereas antecedent states of deep soil moisture and groundwater are less investigated. Terrestrial water storage (TWS) retrievals from the Gravity Recovery and Experiment (GRACE) and GRACE Follow-On (GRACE-FO) missions provide invaluable information on deep soil moisture and groundwater at a global scale. However, the coarse resolution limits its application to flood and drought studies. The study proposed to downscale GRACE TWS retrievals using hydrological estimates from land surface models for drought monitoring and flood prediction. GRACE-based TWS anomalies (TWSA) were spatially downscaled on a 0.5-degree grid using the long short-term memory (LSTM) approach. Afterward, the downscaled TWSA from GRACE will be assimilated into a land surface simulation to estimate vertically downscaled soil moisture, groundwater, and river discharge, which are subsequently used for drought and flood analysis. Preliminary results showed that GRACE captured the dynamic range of groundwater and soil moisture and could better detect droughts than LSMs at basin scale. However, GRACE performed inferiorly in representing the sub-basin and local flood and drought conditions. LSTM-based TWSA showed higher consistency with drought conditions at the sub-basin scale relative to GRACE TWSA. Additionally, the flood potential index calculated from LSTM-based TWSA showed improved capability to capture county-level floods, with a larger true positive rate.
HS52-A007
Study of Groundwater Storage Change in Inner Qinghai-Tibet Plateau Based on Joint Multi-source Data
Lan ZHANG1#+, Wenke SUN2, Zhan JINGANG3
1China Earthquake Administration, 2University of Chinese Academy of Sciences, 3Chinese Academy of Sciences
In the context of global warming, the Qinghai-Tibet Plateau is experiencing a warming and humidifying trend. Over the past two decades, most lakes in the central region have shown an expanding trend, while the changes in groundwater storage are complex. However, due to scarce ground-based observations, quantitative estimation and in-depth analysis of groundwater quantity changes in this region are still lacking. The Gravity Recovery and Climate Experiment (GRACE) satellite, widely utilized in studying global terrestrial water storage, particularly in regions lacking ground-based observations or where observations are sparse and unevenly distributed, provides constraints on groundwater storage changes. In recent years, improvements in datasets for the plateau, including glaciers and lakes, and refinements in models for soil moisture and snow water equivalent, offer conditions for further investigating changes in groundwater storage. We aims to estimate the changes in groundwater within the basins of the Qinghai-Tibet Plateau over the past two decades using GRACE observational data, lake water level-area data, glacier datasets, soil moisture, snow water equivalent, glacier catalogs, and glacial isostatic adjustment (GIA) models. The study employs an artificial neural network approach for data fusion, retaining high-resolution information on lakes and glaciers to enhance the spatial resolution of existing estimates of groundwater storage changes. This research contributes to a better understanding of the impact of climate change on the plateau's terrestrial water cycle system and associated environmental safety issues. Additionally, it provides scientific support for downstream water resource climate adaptation management.
HS52-A011
Reconstructing Long-term Global Water Mass Redistribution by Integrating Multisource Observations Using a Hybrid Model
Shanshan DENG1#, Yuxin LIU1, Wenxi ZHANG1, Ange HU1+, Yashan CHENG2
1Guangxi University, 2Officers College of PAP
The long-term changes in terrestrial water storage and their contribution to sea level are crucial for enhancing our understanding of climate change. However, the observation of terrestrial water storage and its components was scarce decades ago. This study introduces a novel framework for reconstructing a long-term dataset of global water mass redistribution with a relatively high level of accuracy. Firstly, terrestrial water storage is reconstructed by merging data from various sources, including land precipitation, land evapotranspiration, river runoff, glacial mass change, altimetric lake levels, hydrological extreme records, climate indicators, and more. This is achieved through the implementation of deep learning approaches. Secondly, the redistribution of ocean mass is reconstructed by simulating sea level fingerprints using the sea level equation and extracting dynamic variations in ocean mass through maximum covariance analysis. Finally, the accuracy of the long-term reconstruction of global water mass redistribution is assessed by closing sea-level budgets at both regional and global scales, as well as reproducing polar motion records. The findings from this study are expected to advance our understanding of how global water is redistributed and how different subsystems of the Earth interact with each other.
Session Chair(s): Jifu YIN, National Oceanic and Atmospheric Administration
HS30-A007
Spatially Downscaling SMAP Level 3 Soil Moisture Data Incorporating Higher Resolution Precipitation Information
Jhilam SINHA#+, Ashish SHARMA, Lucy MARSHALL
UNSW Sydney
Recent remote sensing techniques in measuring land surface interactions overcome the limitations of scarce point-scale soil moisture (SM) observations, providing quasi-global coverage at a functional temporal resolution. However, remotely sensed SM datasets are coarse (in tens of kilometers), making them unsuitable for application in regional studies. Therefore, spatial downscaling of coarse SM dataset using related covariates to local scale is imperative. In the present study, a spatial downscaling technique is presented that uses only high-resolution precipitation dataset obtained from Climate Hazards InfraRed Precipitation with Station (CHIRPS) to downscale coarser 36 km Soil Moisture Active Passive (SMAP) level 3 SM to the finer scale of precipitation dataset (i: e., 5 km). The algorithm incorporates a conditional relationship between antecedent precipitation and SM, defined as Antecedent Precipitation Index (API), at the coarser scale and translate it to the finer scale. The study is conducted over Continental US region (CONUS) using SM dataset from April 2015 to March 2020 (5 years). The proposed downscaling method effectively downscales SMAP SM, capturing the temporal and spatial dynamics of the original coarser dataset. The ensued finer SM dataset is also compared with the 9 km SMAP Level 3 dataset. Moreover, validation with 2 in-situ SM networks within the CONUS showed that the downscaled SM performed better than the original 36 km dataset and is in line with the 9 km dataset.
HS30-A015
Retrieving Forest Soil Moisture from SMAP Observations Considering Microwave Polarization Difference Index (MPDI) to Tau-Omega Model
Chang-Hwan PARK1#+, Thomas JAGDHUBER2, Andreas COLLIANDER3
1Ajou University, 2German Aerospace Center, 3California Institute of Technology
Estimation of soil moisture from microwave brightness temperature is extremely challenging in densely vegetated areas. Here, the retrieved soil moisture from SMAP tends to be consistently overestimated, sometimes exceeding the saturation of mineral soils. This means that based on current remotely sensed soil moisture, the phenomenon of climate extremes such as flood and drought cannot be properly detected or monitored over these regions which are important for forest and natural resources management and climate change research. We hypothesize that the main issue is that the scattering albedo (ω) and the optical depth (τ) is their parameterization solely with NDVI (Normalized Difference Vegetation Index), which neglect the polarization characteristics from vegetation structure. This study proposes a weighting factor between scattering and optical thickness, which is a function of MPDI (Microwave Polarization Difference Index), and applied it to both parameters simultaneously to increase scattering effect and decrease attenuation effect in high MPDI. The validation results performed in CRNS (Climate Reference Network) revealed that the consideration of MPDI is a critical factor in reducing the soil moisture overestimation errors and obtaining more accurate soil moisture over forested regions. This is evident in the increased correlation (from 0.41 to 0.50), reduced ubRMSE (from 0.03 to 0.02 cm3cm-3 ) and reduced bias (from 0.06 to 0.03 cm3cm-3) when compared to the SMAP.
HS30-A002
Study on the Differences of the Surface Heat Fluxes Between North and South Slopes of Mt. Qomolangma
Maoshan LI1#+, Yaoming MA2, Fanglin SUN2
1Chengdu University of Information Technology, 2Chinese Academy of Sciences
Mount Everest (Qomolangma) region has diversely unique natural conditions and complex surface landscapes, with significant differences in its north and south slopes. Its extremely high-elevation makes it closest to the free tropospheric atmosphere in the world, indicating that it is an ideal area for studying the water and heat exchange between the complex land surface and the atmosphere. The unique conditions of the north and south slopes of Mt.Qomolangma and the complex underlying surfaces lead to significant differences in the variation rules of surface energy flux in the north and south slopes of Mt.Qomolangma, thus the process of land-atmosphere interaction on the Tibetan Plateau is not fully understood. In this study, the variation of surface heat flux in the north and south slopes of Mt.Qomolangma was obtained by using TESEBS, remote sensing data of 8 cloud-free scenarios and observation data of 9 stations. MCD43A3 satellite data is used to improve the surface albedo, which makes the simulation results more accurate. The observed data were used to verify the model results. Results show that the mean bias of net radiation, ground heat, sensible heat, and latent heat flux are -15.27, 6.17, -11.32, 10.32 W·m-2. The net radiation flux is greater on the south slope than that on the north slope, and decreases rapidly from summer to autumn on the south slope. Under the influence of monsoon, the sensible heat flux of the north slope and latent heat flux of the south slope reach the maximum respectively in summer. The sensible heat flux of the north slope is dominant, while the latent heat flux of the south slope is dominant. The seasonal variation of soil heat flux in the south slope was more severe than that in the north slope.
HS30-A011
| Invited
The Methane, Carbon Dioxide and Water Vapor Fluxes Over a Large Lake and a Small Fishpond in Eastern China
Wei XIAO1+, Xuhui LEE2#, Mi ZHANG1
1Nanjing University of Information Science & Technology, 2Yale University
Global inland waterbodies are an important natural source of greenhouse gases to atmosphere. Based on long-term and continuous eddy-covariance observation at a large lake (Lake Taihu area 2400 km2; from 2011 to 2022) and at a small fishpond (area 0.03 km2; from 2017 to 2022) in eastern China, the temporal and spatial variability of CH4, CO2 and H2O fluxes over the inland waterbodies were investigated. Over Lake Taihu, the annual CH4 emission was 1.35 g C m−2 yr−1 in the eutrophic phytoplankton zone, 6.12 g C m−2 yr−1 in the submerged aquatic vegetation zone, and 36.0 g C m−2 yr−1 at the aquaculture farm. Negative CO2 flux was observed using open-path eddy covariance method, which is an artifact due to aerosol interference. We suggest that a closed-path eddy covariance system should be used for CO2 flux observation in high humidity and high pollution conditions. Over the freshwater aquaculture ponds, large annual CH4 emission was revealed, accounting for about three times the median flux reported by other researchers for similar freshwater aquaculture ponds. Ebullition was the main transport way accounting for 70% of the total CH4 flux. The pond was a weak CO2 sink, with annual mean value of −740 kg C m−2 yr−1. Annual lake evaporation was enhanced by increasing energy inputs including solar radiation and incoming longwave radiation and was weakened by surface feedback through outgoing longwave radiation.
HS30-A006
| Invited
Overcoming Challenges in Developing Soil Moisture and Vegetation Optical Depth Retrievals for Forested Areas Using L-band Radiometry
Andreas COLLIANDER1#+, Michael COSH2, Laura BOURGEAU-CHAVEZ3, Aaron BERG4, Xiaolan XU1, Vicky KELLY5, Paul SIQUEIRA6, Simon KRAATZ2, Leung TSANG7, Jongwoo JEONG7, Kyle MCDONALD8, Nick STEINER8, Mehmet KURUM9, Alexandre ROY10, Dara ENTEKHABI11, Simon YUEH1, Mario Julian CHAUBELL1
1California Institute of Technology, 2United States Department of Agriculture, 3Michigan Tech Research Institute, 4University of Guelph, 5Cary Institute of Ecosystem Studies, 6University of Massachusetts Amherst, 7University of Michigan, 8The City College of New York, 9University of Georgia, 10University of Quebec at Trois-Rivieres, 11Massachusetts Institute of Technology
Forests are one of the most essential components of the Earth system, accounting for a large part of the total global photosynthetic activity, storing a significant amount of the total carbon, and providing a habitat for countless species. They also offer critical resources to anthropogenic activities, such as timber, food, fiber, and firewood. Soil moisture (SM) plays a pivotal role in governing all these functions, and forests' biomass and water content are vital for understanding them and their evolution. Low-frequency remote sensing is the only way to acquire spatial distribution of forest SM because of its ability to carry the signal from the forest floor through the forest canopy. Moreover, the canopy has a unique signature that can be used to retrieve the vegetation optical depth (VOD) simultaneously with SM. VOD is related to the above-ground biomass (AGB) and water content of the forest. Accounting for the highly complex forest floor, understory, and canopy structures at the scale of the satellite footprint is the challenge in developing the SM, AGB, and vegetation water content (VWC) retrieval algorithms. NASA's Soil Moisture Active Passive (SMAP) mission and its partners organized field experiments in the temperate and boreal forest zones in the US and Canada, including detailed measurements of SM, forest floor characteristics, vegetation structural parameters, and VWC at the SMAP footprint scale (40 km) to understand these effects on its L-band (1.4 GHz) brightness temperature measurements. The collected data allow the accurate modeling of the ground emission and the forest canopy's attenuation, scattering, and emission. Additionally, the experiment areas were characterized by airborne and terrestrial lidar scans and ground-based VOD measurements using GNSS transmissiometry. These measurements will provide the first basis to establish quantified retrievals of forest SM, AGB, and VWC at the SMAP footprint scale.
HS30-A001
Reprocessed NOAA SMOPS Blended Satellite Soil Moisture Data Product
Jifu YIN#+, Xiwu ZHAN
National Oceanic and Atmospheric Administration
Soil Moisture (SM) is a vital state variable of land surface in hydrological, meteorological and climatological studies as it impacts energy, carbon and water interactions in the boundary layer. To make effective use of all available microwave-based datasets, we have developed a SM Operational Product System (SMOPS) at NOAA-NESDIS since 2012. What makes the SMOPS product unique is it provides the real time 6-hourly and daily global blended SM data products. However, the lack of long-term consistent SMOPS climate data record (SMOPScdr) means data quality varies significantly among the different versions, resulting in uncertainties of using multi-year SMOPS data for climatological studies and long-term data assimilations. To bridge this gap and meet the data requirements of our users, we developed the SMOPScdr by reprocessing and in turn combining all available microwave satellite SM observations since 2002. The SMOPScdr data product takes advantage of three advances: 1) refinement of AMSR-2 SM retrievals using an optimal machine learning model. The refined AMSR-2 SM retrievals show an overwhelming advantage in data accuracy over the currently operational AMSR2 product. As an important component of the SMOPS blended product, higher quality AMSR-2 SM retrievals enhance the SMOPScdr accuracy. 2) Calibration of AMSR-E brightness temperature (Tb) observations toward AMSR2 measurements through building the calibration models at pixel level using the Simultaneous Conical Overpass (SCO) method. 3). Bias-correction of the individual satellite SM data products toward the SMAP observations. The SMAP data product was used as a benchmark for the blending procedure, which makes the SMOPScdr depend solely on readily available satellite observations. With respect to the in-situ measurements, SMOPScdr shows better accuracy and higher spatiotemporal coverage in comparison with the individual satellite SM datasets.
HS30-A018
Global Drought Trends and Patterns Over the Past Two Decades from SMOPS Climate Data Records
Jicheng LIU1,2#+, Jifu YIN2, Xiwu ZHAN2, Li FANG2
1University of Maryland, 2National Oceanic and Atmospheric Administration
In the alarming context of global warming, higher frequency and severity in extreme weather conditions, such as droughts and floods, are expected by scientists. However, the detection of such events on a global scale poses a considerable challenge due to constraints related to data availability and consistency. Over the last decade, the Soil Moisture Operational Product System (SMOPS), developed at the National Environmental Satellite, Data, and Information Service (NESIDIS) of the National Oceanic and Atmospheric Administration (NOAA), has played a pivotal role by operationally providing a blended satellite soil moisture product from a number of individual satellite soil moisture products. Recently, a Climate Data Records (CDR) version of SMOPS has been developed, utilizing a machine learning approach to blend soil moisture products from individual satellite sensors, including AMSR-E, AMSR2, Soil Moisture and Ocean Salinity (SMOS), SMAP, ASCAT-A and ASCAT-B. This upgraded CDR version has exhibited superior quality when compared to previous version of SMOPS, and it now makes historical data available dating back to 2002. In this research, a global drought monitoring system was developed using the SMOPS CDR dataset and generated weekly global drought maps. These maps are then used to facilitate the analysis of statistics and temporal patterns of different drought levels over the past two decades at both the global and continental levels. The findings reveal consistent drought trends and patterns when compared to results from research conducted using alternative data and methodologies, highlighting the great potential of this newer version of SMOPS for drought monitoring applications in near real-time.
Session Chair(s):
HS17-A017
Resistance of Grassland to Drought and Heatwave Over the Temperate Semi-arid Climate Zone
Yangbin HUANG+, Huimin LEI#
Tsinghua University
Temperate semi-arid grassland is facing serious challenges in providing stable ecosystem productivity due to the increased frequency and severity of drought and heatwave. Previous studies have reported the widespread declining resistance of grassland, but the dominant factors determining resistance under different climate extremes (i.e., compound drought and heatwave, single drought and heatwave) are still remain poorly understood. In this study, we choose temperate semi-arid grassland of China as our study area. We use kernel normalized difference vegetation index (kNDVI) and near-infrared reflectance of vegetation (NIRV) as the proxies of vegetation productivity, and use the Standardized Precipitation and Evaporation Index (SPEI) and Standardized Temperature Index (STI) to identify drought and heatwave, respectively. We quantify grassland resistance to short-term and annual events using temporal scales of 8 days and yearly, respectively, by calculating the reciprocal of the difference in vegetation productivity anomalies before and during a climate extreme. Based on the results calculated above we will show the spatio-temporal variations of grassland resistance from 2000 to 2019 over typical steppe and sandy grassland. The dominated factors determining resistance under different climate extremes will be identified by the explainable machine learning. Particularly, responses of resistance to the dominated factors will be investigated by partial dependence plots while keeping other variables constant. Our analysis will provide critical insights into understanding and mitigating the impact of climate extremes on temperate semi-arid grasslands.
HS17-A005
El Niño-induced Drought Shifted Seedling Dynamics in a Seasonally Dry Tropical Forest in Northern Thailand
Prapawadee NUTIPRAPUN1#+, Sutheera HERMHUK2, Dokrak MAROD3, Mamoru KANZAKI4, Satoshi NANAMI5, Akira ITOH5
1The University of Tokyo, 2Maejo University, 3Kasetsart University, 4Kyoto University, 5Osaka Metropolitan University
El Niño promotes extreme drought by reducing rainfall and inducing severe drought periods in the tropics. Seedling dynamics in tropical forests are expected to be strongly affected by drought. However, there is a lack of studies about the impacts of El Niño-induced droughts on seedling dynamics in a seasonally dry tropical forest (SDTF), especially in Asia. In this study, we conducted a 7-year study to quantify the effects of drought on seedling recruitment and mortality in an SDTF in northern Thailand, encompassing a strong El Niño event. This SDTF includes two forest types: a deciduous dipterocarp forest (DDF), dominated by deciduous species, and a lower montane forest (LMF), dominated by evergreen species. During the El Niño event, rainfall decreased significantly from average years, and the dry period lasted three months longer than usual. This condition triggered massive seedling mortality in both forest types, with a more substantial effect on evergreen species in the LMF than on deciduous species in the DDF. Interestingly, the DDF also experienced a massive seedling recruitment during the El Niño period. This massive recruitment compensated for the mortality. Consequently, seedling density in the DDF increased while it declined in the LMF. Our findings provide the first long-term study for differential El Niño impacts on seedling dynamics across forest types and leaf habits in Southeast Asia. It suggests that future climate change, with more intense and frequent El Niño, could substantially alter seedlings' species composition and spatial distribution in Asian SDTFs, potentially impacting future forest structure and diversity.
HS17-A018
Spatio-temporal Analysis of Meteorological and Agricultural Drought in Mindanao Philippines: Hazard, SPI-VHI Correlation, Comparative Study, and El Nino Impact
Kenneth John DUHAYLUNGSOD#+, Rochelle CORONEL
Ateneo de Davao University
This study evaluates meteorological and agricultural drought in Mindanao, Philippines. Meteorological drought is evaluated using the Meteorological Drought Hazard Index (MDHI 1-12), derived from the Standardized Precipitation Index at timescales 1, 3, 6, and 12 months, based on Climate Hazards Group InfraRed Precipitation with Station. Agricultural drought assessment involves the Vegetation Health Index (VHI) from Land Surface Temperature data and Enhanced Vegetation Index obtained from Aqua Moderate Resolution Imaging Spectroradiometer. MDHI 1 indicates that 80% of Mindanao faces short-term meteorological drought and MDHI 12 shows 70% experience long-term meteorological drought. Compostella Valley (66% at MDHI 1), Surigao del Sur (97% at MDHI 3), Bukidnon (94% at MDHI 6), and Agusan del Sur (79% at MDHI 12) have the highest concentration of grids in the high-very high drought category. Areas susceptible to short-term and long-term drought differ. Southern Mindanao is highly susceptible to agricultural drought. However, while southern Mindanao is the most frequently impacted by drought, western Mindanao is the most vulnerable in intensity. The study also pinpoints areas at risk during El Niño, revealing how it changes drought patterns and its impact. Moreover, time series decomposition, correlation, and cross-correlations were done to SPI at different time points and VHI. No significant increase in the frequency but an increase of intensity of drought was seen over time. There is a spatial correlation at p-value < 0.05 and grids that significantly differ from the mean (95% confidence) were identified. Significant relationships between meteorological and agricultural drought indicators indicate that SPI can serve as an indicator of plant irrigation needs in the studied area. Ultimately, this research aims to provide crucial temporal and geospatial insights to vulnerable communities, water managers, and policymakers, assisting them in drought disaster risk reduction and management planning for Mindanao. Top of Form.
HS17-A013
Projection of Global Meteorological Drought Under Future Based on SSP Scenario
Young Hoon SONG#+, Eun Sung CHUNG
Seoul National University of Science and Technology
Because the severity and intensity of drought is difficult to project, the damage is more devastating than another natural hazard. Today, the high variability of climate variables due to climate change makes it more difficult to project hydrological disasters such as droughts. These phenomena have had a profound effect on countries strengthening their adaptation and mitigation strategies to respond to drought. Therefore, this study calculated meteorological drought indices to analyze the changes in future Extreme Drought Period (EDP), Extreme Drought maximum Duration (EDD), and Extreme Drought-fed Area (EDA) depending on SSP2-4.5 and SSP5-8.5 over the globe. As a result, the historical EDP, EDD, and EDA of GCMs were underestimated lower than CRU. The extreme droughts were projected to occur across all continents and timescales, and EDPs of SSP5-8.5 were higher than SSP2-4.5 as 76%. The extreme drought events in near (2031-2065) and far (2066-2100) futures were projected to increase for high emission scenarios, and EDPs for SSP5-8.5 were calculated as above 150 in far future. Furthermore, both EDD was not always proportional to levels of greenhouse gas (GHG) concentrations. On the contrary, and EDA in African continent was larger than different continents by 4% (South America), 18.3% (North America), 10.8% (Europe), 10.2% (Asia), and 8.4% (Oceania), respectively.
HS17-A022
Frequency Analysis and Comparison of Dam Inflow in the Han River Basin Using the Two-variable Copula Model: Based on Soyanggangdam and Chungju Dam
Jiyoung SUNG#+, Boosik KANG
Dankook University
Drought, one of the natural phenomena, is not easy to quantify because the beginning and end of the period of occurrence are not clear. For this reason, various criteria have been reviewed to clearly define the start and end of a drought based on rainfall and river runoff. In order to evaluate a meteorological drought, a univariate drought frequency analysis has been attempted based on precipitation. A study was conducted on multivariate frequency analysis using precipitation, and in particular, the case using the Copula model forms the main flow, but the drought frequency analysis using the Copula model is a meteorological model that mainly analyzes drought based on precipitation, and there is a limit to the hydrological drought analysis by judging the decrease in inflow of rivers and reservoirs, the decrease in dam storage rates, and the lack of water demand.
Therefore, this study intends to conduct a bivariate drought frequency analysis using the Copula model based on dam inflow for Soyanggang Dam and Chungju Dam, which are in charge of water supply and demand in the metropolitan area. First, the beginning and end of a drought are defined using the continuous theory proposed by Yevjevich (1967), and then the characteristic value of a drought is derived based on a threshold level that can be quantitatively interpreted. By analyzing the drought through bivariate analysis that can consider both characteristics using the Copula model and evaluating the drought through the calculation of the reproduction period, we will compare the two different dams in the same watershed.
Session Chair(s): Chengquan HUANG, University of Maryland
HS30-A008
Advancing Hydrologic Predictions Through Innovative Surrogate River Discharge
Hae Na YOON1#+, Lucy MARSHALL2, Ashish SHARMA2, Seokhyeon KIM3,2
1The University of Newcastle, 2UNSW Sydney, 3Kyung Hee University
Predicting hydrologic events is essential for reducing adverse impacts and supporting informed social decision-making. To address the challenges in hydrologic prediction associated with limited in-situ data, scientists increasingly employ remote sensing, notably the Surrogate River discharge (SR), which is derived to have strongly correlated data with streamflow and enhance predictions in ungauged basins (PUB). In particular, the satellite-derived measurement-calibration ratio (C/M ratio) has been regarded as effective as SR, primarily due to its noteworthy correlation with river discharge and widespread availability. However, its use as an SR has limitations, particularly in introducing variations in land features due to the integration of signals from two distinct pixels: the measurement and calibration pixels. Motivated by these challenges, this study presents a novel SR formula using an alternative referencing strategy to enhance the correlation between SR and streamflow. This innovative method assesses temporal signal variability by comparing it to the lowest reflectance value in the driest state of each pixel. The new SR is derived from L-band microwave data from the Soil Moisture and Ocean Salinity (SMOS). This novel SR methodology has been incorporated into the Surrogate River discharge Model (SRM) software as an R package, enabling open access and utilization by the wider public. The effectiveness of this new SR has been evaluated across 467 catchments associated with the Australian Hydrologic Reference Stations. The results demonstrate significant improvements in the Pearson linear correlation (R) between the proposed SR and streamflow. With the new approach, 44% of areas achieved an R value exceeding 0.4, greatly enhancing predictive accuracy, whereas the existing SR (C/M ratio from Ka-band microwave data) achieved this level of correlation in only 13% of areas. In summary, implementing this new SR method represents a substantial advancement in hydrologic predictions, especially in ungauged basins, and facilitates well-informed hydrology decisions.
HS30-A017
Examination of Surface Water Detection Using Multiple Microwave Radiometers
Kosuke YAMAMOTO1#+, Shinta SETO2, Dai YAMAZAKI3, Takuji KUBOTA1
1Japan Aerospace Exploration Agency, 2Nagasaki University, 3Tokyo University
Accurately capturing the spatiotemporal variations of surface water on Earth is crucial from the perspectives of land-atmosphere interaction and monitoring water-related disasters. Several global datasets with high spatial resolution have been developed mainly using satellite-borne optical sensors (e.g., Pekel et al., 2016). However, many of them provide only water probabilities or monthly average data, which are unsuitable for real-time monitoring. Rapid post-disaster assessments are facilitated through emergency observations using satellite-borne Synthetic Aperture Radar (SAR) (e.g., Ohki et al., 2020), while previous studies integrating such data into global datasets are limited. Spaceborne microwave radiometers are operated by many organizations in various countries and are not heavily affected by weather conditions, making it possible to monitor the global water surface at a certain frequency. In previous studies, Seto et al. (2018) calculated the Normalized Differential Frequency Index (NDFI; Takeuchi et al., 2009) from the observed brightness temperature and developed the Global Satellite Mapping of Wet Surface (GSMaWS) for the five-year period from 2013 to 2017 on a daily and 0.1° grid.In this study, surface water data by GPM-core/GMI, GCOM-W/AMSR2, and DMSP-F16, F17, and F18/SSMIS were generated through 2023 based upon Seto et al. (2018), by utilizing the gridding method of the Global Satellite Mapping of Precipitation (GSMaP). The surface water data estimated by each sensor were compared with the flooded fraction (fldfrc) estimated by Today's Earth, a global terrestrial hydrological simulation system developed and operated by JAXA and the University of Tokyo. The results showed that the water surface estimated by the microwave imagers is generally capturing seasonal variations well, especially in the lower reaches of continental rivers, with some challenges over high-latitude snowy regions due to the frequencies used to calculate the NDFI index.
HS30-A014
Machine Learning Enhanced Dielectric Mixing Model for Improved SMAP Soil Moisture Estimation
Chang-Hwan PARK1#+, Andreas COLLIANDER2
1Ajou University, 2California Institute of Technology
One of the primary sources of uncertainty in soil moisture estimation by using soil probes or satellites such as SMAP is a missing consideration of soil organic matter in the Dielectric Mixing Model (DMM). One solution for this issue can be integrating soil organic matter into the DMM through a data-driven approach, like Machine Learning Techniques. However, challenges arise, including the opaque nature of machine learning in understanding dielectric measurements' relationship with organic matter and the lack of global-scale direct dielectric measurements for machine learning training. To overcome these challenges, we propose a Machine Learning-Enhanced Dielectric Mixing Model including two key considerations. Firstly, we assume that feature engineering experiments can remove vegetation and roughness effects, facilitating the training of dielectric features from SMAP brightness temperature data. Secondly, we anticipate that this feature training will extract the actual wilting point and saturation point from the ML black box. These considerations aim to optimally derive crucial physical parameters connecting soil organic matter and dielectric constant in the DMM. Finally, preliminary results will be presented after exploring these possibilities with the new ML-enhanced DMM.
HS30-A004
The Fully Coupled Atmosphere-land-hydrology Process and Runoff Simulations Over the Source Region of the Yellow River
Jun WEN#+, Yaling CHEN
Chengdu University of Information Technology
The runoff of the Source Region of the Yellow RiverSRYR makes an important contribution to the water resources in the Yellow River basin. Based on the Weather Research and Forecasting Model Hydrological modeling system (WRF-Hydro) model, by using meteorological, hydrological observations and reanalysis data, the key variables of the coupled atmosphere-land-hydrological processes over the SRYR during the 2013 rainy season (May-August) are analyzed, and the simulation results of the fully coupled WRF-Hydro with those of the standalone WRF are compared, whose aim is to assess the impact of hydrological coupling on the regional atmospheric model settings. The results show that the WRF-Hydro model has ability to depict the characteristics of runoff over the SRYR with a Nash Efficiency Coefficient (NSE) of 0.44 during the calibration period and a NSE of 0.61 during the validation period. Compared with the standalone WRF model, the fully coupled model tends to show better performance with respect to temperature, downward long wave radiation, downward shortwave radiation, latent heat, sensible heat and soil temperature and moisture. Although the wet bias of the coupled simulated precipitation slightly increases (2.51 mm vs. 2.50 mm) due to the consideration of lateral flow of soil water, the simulation results of the land-atmosphere water-heat exchange fluxes and soil heat fluxes are comparably improved. Compared with the observations, the mean Root Mean Square Error (RMSE) of latent and sensible heat is reduced to 32.27 W∙m-2 and 24.91 W∙m-2, and of surface soil temperature and moisture is reduced to 4.22 K and 0.06 m3/m3. Besides, the fully coupled model is able to capture the variation characteristics of runoff with a NSE of 0.33, which indicates that the fully coupled WRF-Hydro model has great potential for characterizing coupled atmosphere-land-hydrological processes and runoff simulation in the cold climatical and complex topographic regions.
HS30-A012
Towards Monthly Data Product of H2O Cover of the Earth’s Surface for Global Surface Type Mapping
Chengquan HUANG1#+, Xiwu ZHAN2
1University of Maryland, 2National Oceanic and Atmospheric Administration
More than two thirds of the earth’s surface are covered by the liquid (water) or solid (snow/ice) phases of H2O. Not only does the H2O cover over land exhibit large seasonal changes, significant portions of the ocean water near the north and south poles also change phases during a year. Separate data products have been produced through efforts devoted to mapping different phases of H2O over land and ocean areas, including global surface water and flood products, snow cover data, and sea ice concentration data. The primary goal of this study is to integrate these products with the JPSS annual surface type product to achieve a monthly data product of surface H2O cover change across the globe. We will provide an overview of the JPSS annual surface type product and the H2O products used in this study, develop approaches to addressing the issues with each product, and produce a prototype global surface type product suite that captures the seasonal changes in H2O cover over the earth’s surface. This product suite will be validated using available high-resolution images, and will be analyzed to identify hotspots of H2O cover changes across the globe.
HS30-A010
Evapotranspiration and Drought Products from Coupled Microwave and Thermal Satellite Observations for Taiwan Weather Models and Agricultural Drought Monitoring
Li FANG1#+, Xiwu ZHAN1, Peng YU2, Christopher HAIN3, Martha ANDERSON4, Istvan LASZLO1
1National Oceanic and Atmospheric Administration, 2University of Maryland, 3NASA Marshall Space Flight Center, 4USDA-ARS Hydrology and Remote Sensing Laboratory
Evapotranspiration (ET) is a critical component of the water and energy balance of the land surface. As a water balance component, the actual ET amount indicates the soil moisture content status, and its negative anomaly may provide information on whether a drought may occur or is happening. As an energy balance component, the latent heat flux associated with ET is a significant energy source to the atmospheric dynamics and thus is an important variable of many numerical weather and climate prediction models. NOAA/NESDIS developed an operational GOES ET and Drought (GET-D) product system using GOES observations of downward solar radiation and land surface temperature to estimate daily ET and drought conditions. Adopting the GET-D science and software system and generating satellite-based ET and drought products is expected to enhance numerical weather and climate prediction and drought monitoring for the Taiwan region at the Taiwan Central Weather Administration (CWA). The GOES-based GET-D system has been reconfigured for observations from the Advanced Himawari Imager (AHI) for CWA by generating AHI-based daily ET and drought maps at 2km spatial resolution. ET estimates from the new system have been evaluated using in-situ observations over 20 stations in Taiwan region. This presentation will briefly introduce the product system for Taiwan, updates and improvements of the new system, and preliminary validation results.
HS30-A005
A Study on Interannual Characteristics and Driving Mechanism of Carbon Flux in the Alpine Wetland
Yixuan CHEN#+, Jun WEN
Chengdu University of Information Technology
In the context of global warming, the carbon process of alpine wetland ecosystems is complex and sensitive. However, the long-term dynamics and driving mechanisms of carbon balance in alpine wetland ecosystems are still unclear. This study used vorticity covariance (EC) technology to directly measure carbon dioxide (CO2) flux and analyzed the CO2 flux of the Ruoergai alpine wetland from 2017 to 2021, as well as the dynamics and driving mechanisms of CO2 flux. The results showed that during the growing season (June - October), the annual gross primary productivity (GPP) and ecosystem respiration (Re) of the ecosystem showed an unimodal pattern, while the annual net ecosystem CO2 exchange (NEE) of the ecosystem showed a V-shaped trend. The alpine wetland ecosystem is a carbon sink during the growing season, which is a reservoir of atmospheric carbon that absorbs more than releases. The daily average NEE, GPP, and Re over the years reached -3.10 ± 4.61, 4.78 ± 5.61, and 1.65 ± 1.56 umolm-2s-1, respectively. On the monthly scale, the effects of air temperature ( Ta ), soil temperature ( Ts ), photosynthetic photon flux density ( PPFD ), precipitation ( PPT ), air relative humidity ( RH ) and vapor pressure deficit ( VPD ) on NEE, GPP and Re were analyzed by the regression analysis. The results showed that Ta, Ts and PPT were the main determinants of monthly NEE changes, and NEE was negatively correlated with them. Ts and Ta largely determines the monthly variation of GPP, which is positively correlated with it. Ts and Ta are the main determinants of monthly Re variation, and Re is positively correlated with them.
Session Chair(s):
HS17-A002
Different Land-atmosphere Coupling Behaviors in the 2022 US Summer Drought-heatwave Events - Analysis and Model Forecast Study
Donghyuck YOON1#+, Jan-Huey CHEN2,3, Eunkyo SEO4
1Princeton University, 2University Corporation for Atmospheric Research, 3NOAA Geophysical Fluid Dynamics Laboratory, 4Pukyong National University
Compound drought-heatwave events were detected over three major regions of the Contiguous United States (CONUS), e.g., Northwest (NW), Great Plains (GP), and Northeast (NE), during July and August 2022. The developments of drought-heatwave events over these areas originate from different land-atmosphere (L-A) coupling behaviors during this period. The soil moisture (SM) and evapotranspiration (ET) were strongly coupled in the NW region and especially the GP region resulting in a heatwave induced by the decrease of ET and the SM deficit. In the NE region, where L-A coupling was weak, the heatwave governed ET through the increase of potential ET (PET), which played a crucial role in the development of drought. The impacts of these different coupling behaviors on the predictability of the 13-km Geophysical Fluid Dynamics Laboratory (GFDL) System for High-resolution prediction on Earth-to-Local Domains (SHiELD) during its 10-day forecasts were also investigated. The analysis was particularly focused on GP and NE, where significantly different L-A coupling behaviors were observed. The model’s warm bias in GP was closely associated with the overestimation of sensible heat flux, and the errors were further amplified through the L-A feedback. The predictability of SM variability in NE area was strongly linked to the heatwave forecast, which can be detected via the PET-related atmospheric variables Based on the results, we have found that the different L-A coupling behaviors can cause different impacts on the predictabilities of the model’s drought (land) and heatwave (atmosphere) forecasts.
HS17-A008
Anomalous Moisture Sources Contributed to the 2017-19 Southeast Australian Drought
Andréa S. TASCHETTO1#+, Milica STOJANOVIC2, Chiara HOLGATE3, Anita DRUMOND4, Jason EVANS1, Luis GIMENO2, Raquel NIETO2
1University of New South Wales, 2Universidade de Vigo, 3Australian National University, 4University of São Paulo
Southeast Australia experienced an unprecedented drought from 2017 to 2019 due to consistently below-average precipitation during these three cool seasons. Conditions worsened towards the end of the drought due to a positive Indian Ocean Dipole that preconditioned the region to the 2019-2020 Black Summer bushfires. Apart from the Indian Ocean Dipole event in 2019, there were no other obvious climate drivers that would explain the rainfall deficit at the start and development of the drought. In this study, we investigate the drought focusing on regional and local processes instead of remote climate modes of variability. Using a Lagrangian model to trace moisture sources back to the Murray Darling Basin, we have found that local processes played a crucial role in explaining the onset and development of the drought. We identify the sources of moisture to the cool season precipitation over southeast Australia and highlight a significant decline in moisture supply from the Tasman Sea in 2017 and 2018. We further show that anomalous atmospheric circulation diverted moisture to the northern areas of the drought region, depriving southeast Australia of its normal moisture quota. Our results provide an explanation for the moisture and rainfall deficit that caused the 2017-19 southeast Australian drought.
HS17-A014
Characteristics and Mechanism Analysis of Global Scale Drought Propagation from Surface Water to Groundwater
Lin LIU+, Haiyun SHI#
Southern University of Science and Technology
Traditional groundwater drought monitoring requires local observation data, which is difficult to investigate large-scale groundwater droughts. The Gravity Recovery and Climate Experiment Satellite (GRACE) provided a new perspective for groundwater drought estimation. The propagation relationship between groundwater drought and other types of droughts has not been fully explored. In this research, based on GRACE mass concentration solution, GGDI (GRACE Groundwater drought index) was utilized to assess groundwater drought globally. SPEI (Standardized precipitation evapotranspiration index) and SRI (Standardized runoff index) were used to characterize meteorological drought and surface hydrologic drought respectively. Drought events were captured by run theory method. The Pearson correlation coefficient and the spearman rank correlation coefficient were adopted to quantify the propagation time. The results indicated that (1) over 2003-2022, the worldwide groundwater drought events for a single grid range from 1 to 16. (2) Maximum accumulated duration of groundwater drought reaches 142 months; minimum accumulated duration of groundwater drought is 20 months. (3) The relationship between meteorological drought and groundwater drought derived by Pearson correlation is similar to that derived by the spearman rank correlation. The propagation time ranges from 2-47 months. However, the grids with propagation time 1 month accounted for 21.6%; the grids with propagation time 48 months accounted for 28.6%. (4) The Pearson correlation showed that the propagation time from surface hydrologic drought to groundwater drought ranges from 3 to 35 months. There is a lag effect in drought propagation especially groundwater drought. GGDI and run theory were reliable for identifying groundwater drought events. The results are of practical significance for global groundwater resources management. This study provides groundwater drought assessments from a global perspective and contributes to understanding drought development and migration mechanisms in hydrologic cycle.
HS17-A021
Comparative Analysis of Compound Drought and Hot Extreme Indices in Rajasthan, India
Nishant GAUR1#+, Sagar CHAVAN2, Amit SINGH2
1University of Edinburgh, 2Indian Institute of Technology Ropar
Due to significant climatic changes, the frequency and intensity of extreme weather events, such as floods, droughts, and heatwaves, are on the rise globally. There is need to account for the simultaneous occurrences of these extreme events due to the associated dire consequences to nature and mankind. The Compound extremes which are defined as concurrent or consecutive occurrences of extremes have the potential of greater impact on human life and the environment than individual extreme events. This work focuses primarily on understanding composite extremes, and examines the interaction between drought duration and extreme temperatures. For quantification of the compound extremes, several indices have been proposed that mainly include Compound drought and hot extreme index (CDHI), dry-hot magnitude index (DHMI), Standardized dry and hot index (SDHI) etc. These compound indices consider the collective impact of individual extremes, which are assessed through various individual extreme indices such as the standardized precipitation index (SPI), standardized temperature index (STI), drought indicator (DI), etc. In the present study, we have conducted a comparative analysis of the aforementioned compound indices to characterize the simultaneous occurrence of extreme precipitation and temperature events over the state of Rajasthan in India. We considered the temperature and precipitation data from the Indian Meteorological Department (IMD) for the period from 1951 to 2019. The result from the analyses reveals a complex interplay of weather extremes, specifically highlighting the connection between extended droughts and high temperatures within Rajasthan. The analysis highlighted a growing frequency and intensity of compound extremes, emphasizing the heightened vulnerability of the region to simultaneous occurrences of extreme climate activities. The spatial distribution of the compound indices are illustrated through maps for better understanding. This visual analysis facilitated a more straightforward assessment of the strengths and weaknesses of each index in explaining the combined aspects of climatic extremes.
HS17-A019
Assessing Socio-economic Impacts in Subnational Global Droughts: A Comparative Analysis of Combined Versus Single Drought Indicators
Sneha KULKARNI#+, Yohei SAWADA
The University of Tokyo
The accurate assessment of the propagation of drought hazards to socio-economic impacts poses a significant challenge and is still less explored. To address this, we analyzed a newly developed geocoded disaster dataset (GDIS) and checked how well commonly used drought indices pinpoint drought areas identified by GDIS. For the comparative analysis, a widely used Standardized Precipitation Index (SPI), Normalized Difference Vegetation Index (NDVI), Standardized Soil Moisture Index (SSI), and Temperature Condition Index (TCI) were globally computed at the subnational level. Between 2001 and 2021, out of 1641 drought events recorded by GDIS, NDVI identified the highest number at 1541, followed by SPI (1458), TCI (1439), and SSI (1376). NDVI excels at identifying droughts in highly vegetated areas compared to other indices, attributed to its sensitivity to precipitation, soil moisture, and inverse correlation with temperature. Existing single-input-based indices often provide limited insights into the complex nature of drought events and their propagation to socio-economic impacts. Therefore, we also introduced a novel Combined Drought Indicator (CDI) and assessed its performance against GDIS. In 1641 GDIS-documented drought events, CDI successfully identified 1550 occurrences, highlighting a notably strong association with GDIS in contrast to SPI, NDVI, SSI, and TCI. Based on CDI, the highest frequency of severe droughts (> 7) occurred in sub-Saharan Africa and South Asia. CDI observed persistent droughts in Argentina, Brazil, the Horn of Africa, western India, and north China, rendering these areas highly vulnerable to socio-economic droughts. CDI integrates meteorological, hydrological, and agricultural data using weighted methods to identify droughts and play a key role in minimizing inaccuracies in drought assessment. This emphasizes the importance of using CDI to evaluate socio-economic drought risks and prioritize areas of greater concern.
Session Chair(s): Jun-Hyeok SON, IBS Center for Climate Physics, Christian FRANZKE, Pusan National University
IG08-A009
Day Zero Drought: Time of First Emergence of Unprecedented Compound Extremes
Phynodocle Vecchia RAVINANDRASANA1,2#+, Christian FRANZKE2
1IBS Center for Climate Physics, 2Pusan National University
In a warmer world, it is increasingly pertinent to know the expected time of the emergence of unprecedented compound extreme events such as the “Day Zero Drought” (DZD), which will threaten local water supply. Especially unprecedented extreme events will constitute major challenges to societies. The time of first emergence (ToFE), measuring the emergence of unprecedented events, has rarely been employed in climate impact research. Here, we define the ToFE of anthropogenic DZD by using the fraction of attributable risk (FAR) of joint multi-year continuous threshold exceedance of the standardized Precipitation-Evapotranspiration Index and the River Flow Index, from data of a large ensemble climate projection simulation (CESM-LENS2). The results show a significant increase in multi-year water stress and drastic depletion in river flow towards the end of the 21st century under the SSP3-7.0 scenario. FAR is an effective approach for evaluating the anthropogenic signal behind the DZD. We found that 53% of ToFE of DZD would start by the decade of 2020 to 2040; in hotspot regions such as North America, the Mediterranean Regions, Southern Africa, China, Thailand, and Vietnam. In general, future projections show a shorter waiting time of DZD with long duration that will exacerbate the societal impact of water scarcity. Consistently, the DZD will affect more population in urban than in rural areas and more than a half of this population in a 2-degree rise in global temperature. Therefore, more proactive, and suitable local water strategies are relevant and urgently needed to avoid catastrophic societal impacts from water scarcity, as the majority of water-related problems are regional and idiosyncratic in nature; but international water management policies are essential for neighboring countries sharing stream rivers.
IG08-A016
Spatiotemporal Convolutional Approach for the Short-term Forecast of Hourly Heavy Rainfall Probability Integrating Numerical Weather Predictions and Surface Observations
Xi LIU#+
Nanjing Joint Institute for Atmospheric Sciences
The accurate prediction of short-term rainfall, and in particular the forecast of hourly heavy rainfall (HHR) probability, remains challenging for numerical weather prediction (NWP) models. Here, we present a deep learning (DL) model based on the convolutional recurrent neural network, PredRNNv2-AWS, for deterministic short-term rainfall prediction that integrates NWP-simulated atmospheric variables derived from the Precision Weather Analysis and Forecasting System (PWAFS) and surface rainfall observations. Our DL model produces realistic and spatiotemporally consistent hourly rainfall predictions for the next 13 hours. The quantitative evaluation shows that using surface rainfall observations as one of the predictors achieves higher performance (threat score) with 263% and 186% relative improvements over NWP simulations at the threshold of 5 mm/h for the first 3 hours and the entire forecast hours, respectively. While the optical flow method also performs well in the first three hours, its predictions quickly worsen in the final several hours compared to other experiments. The machine learning model, LightGBM, is then integrated to classify HHR from the predicted hourly rainfall of PredRNNv2-AWS. The results show that PredRNNv2-AWS can better reflect the actual HHR conditions than PredRNNv2 and PWAFS. A representative case demonstrates the superiority of PredRNNv2-AWS in predicting the evolution of the rainy system, which substantially improves the accuracy of the HHR prediction. The test experiment in the extreme flood of Zhengzhou exemplifies the generalizability of our proposed model. Our model offers a reliable framework for predicting target variables that can be obtained from numerical simulations and observations, e.g., visibility, wind power, solar energy, and air pollution.
IG08-A017
Enhancing AI's Capacity for Reliable Flood Forecasting with Prior Knowledge: A Step Towards Improved Flood Management and Social Welfare
Shaoxu ZHENG1#+, Zhan TIAN1, Qian KE2
1Southern University of Science and Technology, 2Erasmus University Rotterdam
Floods significantly challenge the progress towards Sustainable Development Goals, particularly in developing countries where the capacity for precise physical modeling and systematic monitoring is often constrained. Addressing this gap, our study pioneers an approach that synergizes the GR4H hydrological model with Google's innovative Time-series Dense Encoder (TiDE), along with other machine learning techniques, to enhance the prediction of extreme riverine events. Central to our methodology is the strategic incorporation of outcomes derived from hydrological models as foundational knowledge, which we rigorously assess for its potential to bolster predictive accuracy. Our analysis demonstrates the significant superiority of the TiDE_GR4H approach over the GR4H model in forecasting flood events with up to 7 days lead time. Particularly notable is its performance in 1-day advance predictions, where the Nash-Sutcliffe efficiency impressively increased from 0.68 to 0.82. This novel approach not only offers a more robust solution for flood warnings in regions with limited modeling capabilities but also marks a considerable advancement in flood risk management, especially for resource-limited settings. Our findings underscore the transformative potential of integrating established hydrological models with cutting-edge machine learning to inform critical flood mitigation strategies.
IG08-A004
| Invited
Extratropical Transition of the Tropical Cyclones in the Warmer World
Jung-Eun CHU#+, Hung Ming CHEUNG
City University of Hong Kong
Tropical cyclones (TCs) are high-impact weather systems that form over the warm tropical ocean and bring catastrophic damage to coastal areas. However, their impact extends beyond tropical regions. When a TC moves to the mid-latitudes, it undergoes a transformation known as an extratropical transition (ET), where it abruptly adapts to new environmental conditions and becomes an extratropical cyclone. Although extratropical cyclones generally have lower maximum wind speeds than TCs, they are larger in size, affecting larger areas and populations. As the climate warms, tropical cyclones are expected to intensify and last longer. However, accurately representing ET events in climate models and their future projections in a changing climate remains challenging. In our study, we used high-resolution Community Earth System Model (CESM) 1.2.2 (ATM~0.25°, OCN~0.1°) to examine the changes in global ET activities under increased concentrations (doubling and quadrupling) of carbon dioxide (CO2) in the atmosphere. We found that the global numbers of ET events under increased CO2 concentrations are similar to that in the climate with the current CO2 level. It is consistent with the lack of changes in the large-scale environment favorable to ET. However, we observe more intense storms upon the completion of the transition, with a more pronounced increase in near-surface wind speeds. We use a metric called “destructive potential”, which considers both wind speed and spatial extent of a storm, to assess the change in impacts by the storms after the transition is completed. Our findings indicate a decrease in the fraction of storms with lower destructive potential and an increase in storms with highly destructive potential when CO2 levels are quadrupled. Our study highlights the possibility of a heightened impact from the transitioned TCs in the mid-latitude region due to human-induced global warming.
IG08-A003
Climatic and Ecological Responses to Medium-sized Asteroid Collision
Lan DAI1#+, Axel TIMMERMANN2
1IBS Center for Climate Physics, 2Pusan National University
There is a chance of 1 in 2,700 that asteroid Bennu will hit Earth in 2182 CE. The collision of such medium-sized asteroids (~0.3-1 km in diameter) with our planet can inject massive amounts of dust into the atmosphere, with unknown consequences for terrestrial and marine ecosystems. Here, we use the coupled high-top Community Earth System Model Version 2 (CESM2) with interactive chemistry to investigate how medium-sized asteroid strikes would impact climate, vegetation, and marine productivity. Our idealized simulations show that globally dispersed dust layers of up to 400 Tg in mass block shortwave radiation to the surface for nearly two years, resulting in rapid global cooling and delayed weakening of the hydrological cycle for up to four years after the impact. The combined effects of reduced sunlight, cold temperature, and decreased precipitation significantly inhibit photosynthesis in the terrestrial ecosystem for almost nineteen months. Marine phytoplankton production decreases moderately within five months due to reduced sunlight. Subsequently, however, and depending on the iron amount of the asteroid, large diatom blooms occur over the eastern equatorial Pacific and Southern Ocean due to iron fertilization from strong upwelling and dust deposition, respectively.
Session Chair(s): Jui-Pin TSAI, National Taiwan University
IG06-A003
New Analytical Solution of Single-well-push-pull Test Considering Transient Flow
Heejun SUK1#+, Jui-Sheng CHEN2, Jize PIAO1, Soonyoung YU1, Seong-Kyun KIM1
1Korea Institute of Geoscience and Mineral Resources, 2National Central University
The single-well push–pull (SWPP) test has been extensively used in parameter estimation models. Numerous analytical solutions to the problem are available, all of which consider solute transport in a non-uniform flow field from steady radial flow created by the SWPP test. However, the non-uniform flow velocity is based on the Thiem equation and varies in a spatial manner, rather than a temporal manner. No analytical solution has been previously described for the solute transport equation of SWPP under fully transient flow. In this study, a new semi-analytical solution for solute
transport in the SWPP test was developed under fully transient flow. With the proposed solution, the differences between a transient flow SWPP model solution and a piecewise steady-state flow SWPP model solution were non-negligible; such differences increased with decreases in the dimensionless parameter related to aquifer flow properties, which is proportional to transmissivity, aquifer thickness, and porosity, but inversely proportional to the storage coefficient and pumping rate.
IG06-A018
From Boreholes to Models: Understanding the Influence of Spatial Borehole Density on the Construction of 3D Heterogeneously Hydrogeological Models
Duc-Huy TRAN#+, Shih-Jung WANG, Jia-Jyun DONG
National Central University
Hydrogeological material distribution has a substantial impact on fields including geotechnical engineering, groundwater dynamics, and geomechanics. This influence is predominantly derived from geological borehole data that reveal aquifer configurations. Spatial borehole density has been the key issue in the construction of hydrogeological models. This research utilized data from 437 lithological boreholes in the South Choushui River Alluvial Fan in Taiwan to examine how the spatial distribution of boreholes affects the development of 3D heterogeneous hydrogeological models (HHMs). It explores a true case and three scenarios of various borehole density. To reduce borehole density, a strategy of uniformly random selection of boreholes was proposed. The one-dimensional continuous-lag Markov chain was used to analyze the spatial characteristics of hydrogeological materials and generate realizations of the HHMs. The results of study demonstrate the influence of spatial borehole density on the configuration of HHMs, where increase in borehole density results in more complex and heterogeneous models, while a lower density exhibits a more continuous pattern. The coefficient of variation (CV) was used to measure the variability of model outcomes. Specifically, the 90th percentile (P90) CV value for clay thickness was determined to be 0.309 based on the outcomes of 40 HHMs. CV assessment shows that additional geological borehole data reduces the uncertainty of HHMs. This study illustrates the effect of spatial borehole density on the distribution of hydrogeological materials and the uncertainty associated with them. It provides important insights that contribute to improve the dependability of stochastic HHMs. The results can be used in a variety of fields, including engineering geology, environmental evaluations, land subsidence assessment, and groundwater management, etc.
IG06-A001
Nitrate Mediated Biostimulation of Petroleum-based NAPLs in Subsurface Environment with Dynamic pH Scenarios: A Hydrogeochemical Modelling Approach
Akanksha SRIVASTAVA#+, Renu V, Sheeja JAGADEVAN
Indian Institute of Technology (Indian School of Mines) Dhanbad
Aquifer contamination by organic matter is an essential ecological concern arising from their widespread application and persistence in the subsurface ecosystem. The biogeochemical interaction mechanism that exists in the subsurface contaminated with petroleum spills has a substantial influence on the biostimulation cleanup-process. This investigation uses a 2D-multicomponent biogeochemical reactive transport numerical model to simulate the biostimulation of petroleum-based NAPLs. The model is employed at a petroleum spill location adjacent to a hypothetical subsurface environment that contains naturally occurring reductants. In order to enhance the rate of biodegradation, nitrate is injected as a nutrient for bacterial growth. Additionally, when nitrate reacts with naturally occurring reductants, it lessens the amount of nitrate, makes the subsurface environment acidic, and hinders denitrifying bacteria from reproducing. Sequentially, five coupled models are used to assess the mechanisms involved. Biostimulation efficiently lowers the penetration depth of NAPLs and has resulted in a substantial drop in its concentration level, based on the current research. The results further indicate that aquifer pH adjustments somewhat inhibits the interference of natural reductants in the biostimulation mechanism. The biostimulation rate of petroleum-based NAPL appears to rise as the aquifer's pH level shifts from an acidic to a neutral pH. When the pH is neutral, the utilisation of nitrate is higher and bacterial growth is maximum. Thus, natural reductants significantly affect subsurface NAPL biostimulation and mobility. Thus, an in-depth analysis of such intervention required for real-life risk assessment and effective remediation.
IG06-A006
Exploring Hydrogeological Characteristics in the Yunlin Area of the Choshui River Alluvial Fan Using Transient Electromagnetic Methods
Ping-Yu CHANG#+
National Central University
In this study, we utilized the Transient Electromagnetic Method (TEM) to conduct measurements in the Yunlin region of the Choushui River alluvial fan. The aim was to develop a shallow resistivity model for the region, serving as a valuable correlation tool for future hydrogeological model establishment. Through a comparison of TEM resistivity inversion results with core records from nearby wells, we observed a noteworthy similarity in trends. Further insights were gained by spatially extrapolating resistivity data from 63 TEM measurement points across the study area to obtain resistivity distribution at various depths. The findings indicate that the area predominantly comprises sandy-muddy sediments with low resistivity (below 50 Ohm-m) at depths of 30-50 m. Beyond 50 m, there is a gradual expansion of sediments with resistivity higher than 60 Ohm-m. In Tuku Town, sediments with resistivity exceeding 100 Ohm-m were identified at depths ranging from 100 to 150 m, suggesting the presence of gravel or sand layers with more coarse-grained sediments in that locality. A comparison of cumulative strata subsidence centers in the Yunlin area from 1992 to 2020 reveals a potential correlation between certain spatial distributions and higher resistivity strata in the study area. This correlation merits further investigation and verification for a comprehensive understanding of the hydrogeological dynamics in the region.
IG06-A019
Long-term and Inter-annual Groundwater Storage Changes Over the Haihe River Basin from Satellite Gravimetry and In Situ Measurements
Jin LI1#+, Jing LI2, Jianli CHEN3, Xian SHI4
1Shanghai Astronomical Observatory, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3The Hong Kong Polytechnic University, 4Shanghai Astronomical Observatory
Locating at the North China plain, the Haihe River basin is one of the main basins in North China that have been experiencing dramatic variations in terrestrial water storage (TWS) in recent decades, due to both natural reasons and human activities. In this study we use GRACE (Gravity Recovery and Climate Experiment) and GRACE-FO (GRACE Follow-On) satellite gravimetry observations and land surface models to quantify the groundwater storage changes over the Haihe River basin. Results indicate that a decreasing trend and strong inter-annual variations are dominant in the groundwater changes over the basin. During the period 2002 to 2023, the groundwater loss rate is 8.3 ± 3.0 gigaton per year (Gt/yr). Dramatic decreases and increases in groundwater storage are found in the recent two decades, among which the acceleration of decrease during 2013-2019 and the abrupt increase during 2020-2023 are most prominent. These significant inter-annual variations are generally consistent with the basin-average changes revealed by water level measurements with more than 100 underground wells over the Haihe River basin. Comparison with the precipitation data as well as the global climate indexes suggests that the abrupt decreases or increases are mainly due to precipitation anomalies over the basin, which are likely correlated with the El Niño and La Nina events in recent years.
Session Chair(s): Pankaj KUMAR, Indian Institute of Science Education and Research Bhopal, Ramsankaran RAAJ, Indian Institute of Technology Bombay
IG16-A005
Are Deep Learning Methods Viable for Precipitation Downscaling Over the Highly Complex Terrain of the Western Himalayas?
Midhun MURUKESH#+, Pankaj KUMAR, Raj Pritam GUPTA
Indian Institute of Science Education and Research Bhopal
This study investigates the viability of deep learning methods for precipitation downscaling over the complex topography of the Western Himalayas. The Western Himalayas are distinguished by the presence of glaciers and snow cover, and their mass balance is influenced by the total precipitation occurring in this region. Recognizing the challenges posed by the region's highly complex terrain, we explore the application of deep learning techniques, specifically convolutional neural networks (CNN), for downscaling precipitation data. The broader objective is to demonstrate the potential of deep learning-based super-resolution techniques for extrapolating climate projections and generating a high-resolution dataset for the future period over this region. For demonstration, this study is confined to the historical period (1980–2020), leveraging two reanalysis products available over this region: the ECMWF reanalysis 5 (ERA5; 0.25ox0.25o horizontal resolution) and High Asia refined analysis version 2 (HARv2; 0.1ox0.1o horizontal resolution). Two CNN architectures of varying complexity, known as UNet and Nest-UNet, are deployed in this study. These networks follow an encoder-decoder type architecture, where high-resolution elevation data and other auxiliary variables like geopotential, temperature, surface pressure, and humidity can also be supplied as input parameters to enhance the physical consistency of downscaled precipitation data, which enables them to preserve complex hypsometric variation and extreme values of precipitation. Through rigorous evaluation, we assess the performance of these methods in capturing fine-scale precipitation patterns over the diverse and challenging landscape of the Western Himalayas. Our findings substantiate that deep learning is an effective tool for precipitation downscaling in geographically complex terrains, contributing valuable insights to hydro-climatologists. Detailed results will be presented at the conference.
IG16-A001
UAV Based Annual Geodetic Mass Balance Estimation – A Pilot Study in Panchinala-A Glacier, Western Himalayas, India
Navinkumar PERUMAL JAYARAMAN#+, Ajay GODARA, Sayantan MANDAL, Ramsankaran RAAJ
Indian Institute of Technology Bombay
Various studies reported that glaciers lying within the same climatic settings especially in Himalaya exhibit heterogenous melt behaviour. Studies have attributed this behaviour to presence of debris coverage, evolution of supraglacial features upon the glacier ablation zone. Changes in these supraglacial ponds and ice cliffs directly impact energy balance, melt rates, and mass balance of glaciers, providing insights into their response to changing environmental conditions. Satellite based images and elevation products are dominantly used to conduct such investigations. Unfortunately, their limited spatial resolution restricts in interpreting the complex relationships between various supraglacial features and glacier mass balance. To cater this, on-demand, low-cost Unmanned Aerial Vehicle (UAV) platform based high resolution observations are made nowadays. In this study, we estimated annual geodetic mass balance in whole ablation zone, assessed the changes in supraglacial ponds and ice cliffs using the orthoimages and Digital Surface Model (DSM) generated from UAV collected data. For this, multiple surveys were conducted on the ice ablation area of Pachinala-A glacier for two consecutive years (2021-2022). It is noteworthy to mention that this is the first study in the Indian Himalayas to conduct such multiple UAV surveys to estimate ablation wide annual mass balance of a glacier. Some of the interesting results obtained are as follows, a) ice ablation-wide mean elevation changes and annual geodetic mass balance is found to be -1.58 m and -1.34 m.w.e, and b) surface area surrounding the ice cliffs, taken at 50 m buffer, encompassing supraglacial ponds exhibits 21% higher mass loss than the remaining area, c) an increase of 86 % of total surface area of supraglacial ponds in year 2022 relative to 2021, and d) revealing prominent englacial channel flow due to the appearance of new supraglacial ponds. The knowledge gained through the obtained results demonstrate positive prospects of utilizing UAVs to monitor glacier 'health'.
IG16-A002
The Contemporary Pace of Climate Shift in the World’s “Third Pole”
Disha SACHAN#+, Jyoti SHARMA, Aaquib JAVED, Pankaj KUMAR
Indian Institute of Science Education and Research Bhopal
The Himalayas, known as the “third pole, " are a prominent cryospheric system accommodating the highest amount of freshwater apart from the poles. They feed nearly ten perennial river systems in and around the Indian subcontinent, supporting billions of lives downstream. However, the changing climate has hastened the melting of glaciers and receding snow cover in this region. Consequently, this has increased the risk of catastrophic events like glacial lake outburst floods, threatening human lives and infrastructure. Melting glaciers and decreased snow cover also alter the regional energy budget by influencing the albedo feedback and heat fluxes, changing the hydrological regimes of the glacier-fed rivers, and regulating the local temperature changes. The Himalayan ecosystem is highly vulnerable to climate change since it’s a biodiversity hotspot that hosts nearly 5000 species of flora and fauna. Thus, any change in the regional background climate is expected to cascade across the whole system. In the current study, we present the univariate and multivariate velocities of climate change derived from climatic variables like temperature, total precipitation, and snow cover obtained from the ERA5 reanalysis and MODIS satellite products for 2002-2022. The velocity of climate change is a comprehensive metric that indicates the local pace of the climate shift. We also present the climatic exposure and stress the organisms in this region have faced in the last two decades. The multivariate estimates of climate velocities were higher (2-4 km/yr) than the univariate estimates (-1 to 2 km/yr). The climatic stress, which indicates the movement of climatic isopleths in opposite directions, was also significantly high. These results point towards the higher exposure of cryospheric systems to climate change since they represent climatic cul-de-sacs. Our results highlight the urgent need to focus on mitigation and adaptation measures. Detailed results will be discussed further in the presentation.
IG16-A012
Decoding Hydrological Patterns in the Beas River Basin: Insights from SPHY Model on Snowmelt and Glacier Contributions
Ashutosh Laxman TARAL1+, Supratim GUHA2, Reet Kamal TIWARI1#, Iti SHRIVAS1, Eshrat FATIMA3,4
1Indian Institute of Technology Ropar, 2Korea Polar Research Institute, 3Helmholtz Centre for Environmental Research GmbH, 4University of Potsdam
Quantifying the impact of climate change on hydrologic features is essential for water resource management. The present study explores the hydrological processes of the Beas River basin, focusing on the upstream region of the Pandoh Dam in the Western Himalayas. The study evaluates the Spatial Processes in Hydrology (SPHY) model to comprehensively understand spatial and hydrological parameters such as precipitation, snow and glacier melt, and river discharge. The SPHY model is a valuable tool for assessing complex watershed behavior, especially in mountainous and glaciated regions like the Beas River basin. The upstream Beas River basin covers an area of about (≈ 5000 km2). During the winter season, approximately 45% of the basin is covered by snow, and about 15% remains covered by permanent snow and glaciers. This study aims to analyze the contributions of different sources such as snow and glacier melt, rain runoff, and baseflow runoff—to river discharge. Utilizing the SPHY model, we simulate the temporal patterns of runoff components at the outlet of Pandoh Dam, covering the period (1981 – 2010). The results showed that 43% of the total runoff in the basin was generated from snow about (21%) and glacier melting (22%). In contrast, rainfall-induced runoff was estimated to account for approximately 49%, while the simulated baseflow constituted 8% of the total flow. The average simulated runoff for the period 1981-2010 was 211.45 m3/s, while the observed average runoff for the years 2014-2020 increased to 225.68 m3/s. This rise in runoff in recent years is attributed to the influence of climate change. These findings emphasize the significance of snow and glacier-fed rivers in the Himalayan region and demonstrate the utility of the SPHY model for assessing water availability and understanding the impacts of climate change on hydrological processes in mountainous areas.
IG16-A008
Geospatial Observation for Glacier Area Changes Under the Influence of Climatic Variability in the Ravi Basin, Western Himalaya
Payal SHARMA#+, Rajesh KUMAR
Central University of Rajasthan
Significant deficiencies persist in our understanding of glacier area changes and the rate of glacier retreat, particularly concerning glaciers in the Ravi Basin, Western Himalayas. Therefore, the primary objective is to identify the changes in glacier areas over the decades and to estimate the rate of glacier retreat in the Ravi Basin. Multi-temporal satellite data, including ASTER DEM, Corona-KH 4, Landsat 4/5 Thematic Mapper (TM), Landsat 7 Enhanced Thematic Mapper (ETM+), Sentinel 2B, Landsat 8 OLI/TRS, Worldview and Google Earth Pro, have been used to analyze the spatial patterns of glacier area changes for a subset for 134 glaciers (>0.2 km2) lying between 4000-6100m elevation in the Ravi basin. This research evaluated the regional climatic trends (1958-2022) using gridded datasets from NASA Power Access Data viewer, and Terra climate. Statistical methods i.e., Mann-Kendall Test and Sen's Slope estimation have been applied showing an increasing trend of the minimum temperature by 0.14°C per year and no significant change in maximum temperature and precipitation over the glacierized basin. Also, the results validated with ground-based snout monitoring revealed that total glacier area in the Ravi basin decreased from 151.78km2 to 134.02km2 during 1971-2023 with an average retreat rate of 0.42km2 per year having overall retreat of 11.25%. The relative rate of glacier area changes in the Ravi River basin from 2009 to 2023 was three times that of 1980-2000. The glaciers situated between the altitudes of 4000m and 4800m have receded more than those at altitudes higher than 4800m. All glaciers, regardless of their orientation, have shrunk but South-facing glaciers retreated faster than those facing other directions. The smaller glaciers have retreated more than the larger glaciers. Our study suggests consistent monitoring of glacier dynamics in this area to precisely address the effect of regional warming on glaciers.
Session Chair(s): Kelvin NG, University of Birmingham, Zhan TIAN, Southern University of Science and Technology
IG08-A001
Unlocking the Dynamics of Extreme Wind Speeds in North Atlantic Storms
Jun-Hyeok SON1#+, Christian FRANZKE2, Seok-Woo SON3
1IBS Center for Climate Physics, 2Pusan National University, 3Seoul National University
North Atlantic extra-tropical storms are some of the most severe weather systems, causing enormous economic damages and threatening human lives. In general, these storms are characterized by strong cyclonic convergent surface winds, upward vertical flow, and precipitation. In specific confined areas inside the storm where downward flows occur with clear sky, extreme surface wind speeds are observed. Such a horizontal variation of vertical wind direction and surface wind speed can cause severe and damaging impacts; however, the underlying key dynamics are not understood. Here we show the dynamical and thermodynamical linkage between the horizontal wind impinging on the frontal surface at the lower troposphere, downward flow, and very intense surface wind speeds inside the storm. The anti-clockwise cyclonic wind into the cold frontal area is mainly responsible for generating the downward flow, which transports the high-altitude horizontal momentum to the surface layer causing intense surface wind speeds. About half of North Atlantic storms accompany the downward wind, and that downward flow is more frequently observed in the southern and western part of the storm center. Overall results illuminated in this paper have a far-reaching impact in multiple ways to enhance forecasting skills for devastating weather events associated with extra-tropical storms.
IG08-A007
Can We Forewarn Extreme Rainfall Events from Scaling Behaviors?
Lichao YANG#+
Capital Normal University
Climate variables, such as temperature, precipitation, relation humidity and river runoff are interconnected over long temporal and spatial distances. The correlations which averaged over temporal and spatial areas can be described by as simple relationship called ‘scaling’., also the long-term persistence (LTP). In this work, we study the LTP property of hourly precipitation and show how the LTP influences the occurrence of hourly extreme precipitation events. Specially, we model the hourly precipitation records by the generated artificial time series characterized by the same long-term persistent coefficient with the observed precipitation at each station, and compare them by investigating the statistics of return intervals and duration lengths of extreme precipitation events. To quantify how the previous extremes influence the occurrence of the future extremes, we apply a hazard function. Based on these findings, a statistical warning alert for extreme precipitation risk is suggested.
IG08-A002
Changing Temporal Volatility of Precipitation Extremes Due to Global Warming
Christian FRANZKE#+
Pusan National University
It is of utmost importance to understand how precipitation extremes change due to global warming. Here, we examine the volatility of precipitation extremes by analysing the waiting time distribution between events and the clustering of precipitation extremes. For this we use the ERA5 reanalysis data and high-resolution simulations with the Community Earth System Model (CESM). We find significant evidence for a power-law distribution of waiting times between precipitation extremes and of serial clustering of precipitation extremes. This suggests that precipitation extremes do not occur independently from each other. This is in contrast with previous studies which typically assume that precipitation extreme events occur independently from each other. CESM reproduces these properties well. The climate change simulations show that the waiting times between precipitation extremes become shorter and that at the same time the clustering of precipitation extremes increases. Hence, global warming affects the temporal characteristics of precipitation extremes and, thus, precipitation extremes will become more volatile.
IG08-A010
Increased Ocean-dependent Risk of Clustered and Single Storms Associated with Wind and Precipitation Extremes at Different Global Warming Levels
Alexia KARWAT#+, Christian FRANZKE, June-Yi LEE
Pusan National University
Strong extratropical cyclones associated with wind and precipitation extremes pose a serious risk that could be amplified by anthropogenic climate change. However, projections of clustered and single storms are often not statistically significant and sparse due to small ensemble sizes and a lack of high-resolution climate models. Using a new 50-member grand ensemble with 3-hourly model output for 5 different SSP scenarios, we systematically assess future cyclone risk and examine the waiting times of clustered and single storms in relation to wind and precipitation extremes. Cyclones cluster more efficiently in warmer and wetter regions, particularly under warming levels between 3°C and 4°C above historical average, while mean storm track activity will generally decline. In tandem with rising CO2 emissions, we find that cyclone clustering significantly increases by about 28% over northwest Europe by 2070-2100. Similarly, wind speeds above the 95th percentile occur more frequently over France and Germany at enhanced warming levels. Moreover, wind and precipitation extremes specifically linked to intense single storms dominate in the Northeast Pacific and South Pacific, affecting Australia, Tasmania, and New Zealand more severely under SSP3-7.0. The projected risks are driven by higher warming levels, accelerated sea-ice loss, and larger ocean feedback, increasing the likelihood of coastal flooding and more extreme periods of stormy weather worldwide.
IG08-A011
Responses of Tropical Cyclone Frequency Under CO2 Removal Scenarios
Mincheol MOON1+, Seung-Ki MIN1#, Jung-Eun CHU2, Soon-Il AN3
1Pohang University of Science and Technology, 2City University of Hong Kong, 3Yonsei University
Numerous prior studies have discussed the impact of global warming on tropical cyclones (TCs). However, there's a lack of understanding regarding TC activity post-global warming. In this study, through CO2 emission-driven experiments with CESM2 model, simulations of 400 years for scenarios involving Net-zero Emission CO2 (ZEC) and negative emission CO2 (IRCC) are conducted to analyze the responses of TC activity to CO2 removal forcing. Using the Okubo-Weiss-Zeta Parameter (OWZP) method for TC detection, which is independent of the model's resolution, we identified a hemispherically-asymmetric response with decreased TCs in the Northern Hemisphere and increased TCs in the Southern Hemisphere. Specifically, irreversible responses are prominent in the North Atlantic, the Eastern Pacific, and the West Pacific in the Northern Hemisphere, and the South Pacific in the Southern Hemisphere. Beyond TC frequency, we analyzed shifts in TC genesis location and track, linking them to environmental changes. These findings emphasize the necessity to regionally differentiate preparations for the TC activity based on CO2 reduction scenarios.
Session Chair(s): Sheng-Wei WANG, National Central University
IG06-A007
Optimizing In-situ Remediation: Integrating VASPPL Technique with Heterogeneity Characterization and Inverse Data Assimilation
Jize PIAO+, Heejun SUK#, Soonyoung YU, Seong-Kyun KIM
Korea Institute of Geoscience and Mineral Resources
In-situ remediation emerges as an effective and economical approach for mitigating subsurface oil contaminants. Our study introduces an innovative subsurface circulation technique named VAriable Strength/Period/Phase/Location (VASPPL), utilizing a pair of injection and extraction wells. Distinct from traditional continuous injection and extraction, VASPPL strategically varies these parameters such as pumping and injection rates, period of injection and extraction, phase difference between two periods, and location of injection and extraction well to circumvent preferential flow and enhance the contact efficiency between oxidants and oil contaminants. This research focused on the consideration of the subsurface's heterogeneous hydraulic properties in applying the VASPPL method and involves a stochastic evaluation of remediation efficiency under diverse operational conditions. To model the heterogeneity, we employ Sequential Gaussian Simulation (SGSIM), generating potential heterogeneity fields. Subsequently, we simulate various VASPPL scenarios using these realizations to estimate the impact of heterogeneity on the cumulative sweeping area. Further refining our approach, we integrate observation data from field tests with our simulation outcomes. This process involves inverse modeling to adjust the heterogeneity field. This method of data assimilation, combining both forward and inverse modeling, reduces the uncertainty inherent in remediation efficiency predictions due to site heterogeneity. This work was supported by Korea Environment Industry & Technology Institute (KEITI) through “System development and field demonstration of in-situ chemical oxidation circulation designed based on numerical modelling” funded by Korea Ministry of Environment (MOE) (RS-2023-00220587).
IG06-A002
The Numerical Simulation of Temperature Depth Profile in the Choshui Alluvial Fan, Central Taiwan
Wenfu CHEN#+
Chia Nan University
In this research, we use numerical simulation of groundwater temperature depth profile to determine the groundwater flow field in the Choshui alluvial fan, central Taiwan. The horizontal direction of groundwater flow and velocities are calculated by using Darcy’s equation, observed groundwater head and hydraulic conductivity. The vertical direction and velocity of groundwater in aquitard are determined by using a 2D heat transfer equation for the temperature depth profile. Our results show the directions of vertical groundwater flow are consistent with observed groundwater head data. The velocities of vertical flow in aquitards are 10-7 to 10-9 m/s. Velocity lower than 10-9 m/s in aquitard mean that heat transfer are dominated by thermal conduction than convection. The study area is divided into three subareas according to the recharge potential. (A) The upper fan with downward flow component is suitable for artificial recharge of groundwater. (B) The transition zone of upper fan to middle fan is not suitable for recharge because the upward flow in aquitard T1. (C) The middle fan is suitable for groundwater recharge, however, the flow velocity is lower.
IG06-A014
Experimental and Numerical Assessment of Fresh Water and Seawater Interactions in the Coastal Aquifer of the Taoyuan Tableland, Taiwan
Chuen-Fa NI1#+, Thanh Quynh DUONG2, Chia-Yu HSU1, Thai Vinh Truong NGUYEN1
1National Central University, 2Helmholtz Centre for Environmental Research - UFZ
Understanding the dynamics of water and mass interactions in the coastal area is essential to quantify the influences of near-shore land use on the coastal aquifers and water environment. The study aims to integrate innovative experiments and modeling techniques to assess the heat and water exchanges in the coastal aquifer of the Taoyuan Tableland in northwestern Taiwan. The site-specific hydraulic and heat tracer tests are conducted to obtain flow and heat transfer properties for the specific aquifer layers at the site. We then used the SEAWAT numerical model to quantify the freshwater and seawater interactions. The model calibration relies on the groundwater levels and quality obtained from monitoring wells installed perpendicular to the shoreline. The experimental results show that the active heat tracer tests could significantly improve the identification of aquifer layers along a well and allow for the estimations of high-resolution natural groundwater flux toward the sea. The estimated flow rate based on the heat tracer test is approximately 0.2 m/day per unit depth. The numerical model shows good agreement with the observed water levels in wells. In the study area, the location of the seawater/groundwater mixing interface is estimated at approximately 350m seaward from the shoreline, which suggests the submarine groundwater discharge zone for the site. The vertical profile model shows that the flow rate for the 100m depth aquifer varies from 51 to 60 m3/day per unit width, depending on the tidal variations and upstream groundwater levels. The results show a large flow rate discrepancy between experimental and numerical approaches, which the resolution scales of the approaches might induce in the calculations. The water levels obtained from the fully opened screen wells might mix the flow responses in different aquifer layers.
Session Chair(s): Chun-Hsiang KUO, National Central University, Seokhyeon KIM, Kyung Hee University
IG11-A003
Near-real Time Shakemap Estimation Using GMM with Consideration of Rupture Directivity Effect for an EEW System
Chun-Hsiang KUO1,2#+, Hsin-Hua HUANG3, Chin-Ting WENG1, Shu-Hsien CHAO2
1National Central University, 2National Center for Research on Earthquake Engineering, 3Academia Sinica
Ground Motion Model (GMM) is usually used in a regional earthquake early warning system to predict intensities of different area when preliminary earthquake parameters, e.g., magnitude and hypocenter location, are determined. However, in Taiwan, significant rupture directivity effects have been observed during several earthquakes and severe damages were caused in the areas near forward rupture direction. For example, the 2016 Meinong earthquake with MW of 6.5 left 117 fatalities and ~250 buildings damaged; the 2018 Hualien earthquake with MW 6.4 caused 17 fatalities and 14 buildings damaged. The most damaged area during both of the events were located in the forward rupture direction where relatively stronger intensity were also observed. Chao et al. (2019) utilized an advanced GMM (Chao et al. 2020) with consideration of a rupture directivity function (Convertito et al. 2012; Jan et al. 2018) to predict peak ground acceleration (PGA) and peak ground velocity (PGV) and found the result was better than that without considering a rupture directivity function. We therefore adopted the same technique and added approaches of determining rupture directivity parameters and constructing simplified fault model in near-real time for an earthquake early warning system (EEW). This new method allows the EEW system to generate a shakemap with consideration of rupture directivity effect. This study used recent earthquakes with magnitude larger than 5.5 to test the proposed method and it shows better predictions than traditional method especially for near-field area during an event with considerable directivity effect.
IG11-A005
| Invited
Customized Hybrid Early Warning Model for Predicting Earthquake-induced Peak Floor Acceleration of High-rise Building
Shu-Hsien CHAO1#+, Chiao-Chu HSU1, Yu-Tzu HUANG1, Che-Min LIN2, Chun-Hsiang KUO3,1
1National Center for Research on Earthquake Engineering, 2National Applied Research Laboratories, 3National Central University
Current earthquake early warning system (EEWS) in Taiwan broadcasts early warning messages for the locations with predicted intensity level at ground higher than Level 4 representing the predicted peak ground acceleration (PGA) higher than 25 gal. However, the earthquake-induced structural peak floor acceleration (PFA) in some structures may be significantly higher than 25 gal due to the structural resonance response which may induce damage and loss even PGA at ground is lower than 25 gal, especially for the high-rise buildings. The aim of this study is to develop a customized hybrid early warning model which can be used to predict the earthquake-induced peak floor acceleration of high-rise building by using the early arrival P-waves of detection spots and on-site P-wave. The proposed early warning model was developed based on the data collected from a high-rise building with well-instrumented structural monitoring system as well as the on- site and near-by strong motion instruments at ground. The ground motion intensity parameter which can well distinguish the level of structural resonance response was evaluated and selected first by using the data collected from the structural monitoring system of the high-rise building. Next, the on-site P-wave parameter which may be used to predict the pre-mentioned ground motion intensity parameter was evaluated by using the data collected from the on-site and near-by strong motion instruments at ground. Finally, a customized hybrid early warning model for predicting earthquake induced peak floor acceleration of high-rise building was proposed, and all collected data was used to validate the proposed model applicability and performance. The proposed model can be implemented in a new-build customized EEWS for a specific high-rise building to broad early warning message to people in the building with better accuracy to prevent damage and loss caused by earthquake-induced high PFA.
IG11-A009
| Invited
A Review of Early Hazard Warning Systems in Japan
Takashi OGUCHI#+
The University of Tokyo
Japan is subject to various natural hazards, including heavy rainfall, snowfall, earthquakes, tsunamis, and volcanic eruptions. Their consequences, such as rainfall-induced flooding and mass movements, often lead to disasters with human and economic losses. Therefore, the Japanese government has developed early warning systems for natural hazards. The Japan Meteorological Agency (JMA) is one of the fundamental units for this activity. For example, in 2008, they started using the Soil Water Index (SWI) to predict rainfall-induced mass movements using the latest rainfall observation record, and computational results are presented to the public in real time. Although the SWI is based on pedological and hydrological parameters obtained from areas underlain by granitic rocks, it shows broad applicability to geologically diverse regions, including most of Japan and Taiwan. The JMA also issues early warnings about heavy rainfall, heavy snow, strong wind, high waves, high tide, flood, lightning, fog, dry air, snow avalanches, icing, frost, snow melt, low temperature, tsunamis, and volcanic eruptions. Their earthquake early warning system uses seismometer observation data to warn of intense seismic shaking via smartphones, televisions, and radios immediately before it happens due to wave propagation. In 2007, the Fire and Disaster Management Agency (FDMA) also launched the J-Alert system to quickly inform the public of threats and emergencies via the wired and wireless systems of local governments concerning earthquakes, severe weather, and other dangers, such as launching a ballistic missile by a neighboring country. Overall, Japan’s early hazard warning systems are among the most developed in the world. However, the past use of the systems also indicated the necessity of further development and improvement. This presentation reviews Japan’s early hazard warning systems, states existing problems, and provides future perspectives.
IG11-A011
Optimal Stopping of Natural Hazard Cascades
Gabriel Lorenzo SANTOS1,2#+, Vena Pearl BONGOLAN3,4, Jesus Emmaneul SEVILLEJA5
1University of the Philippines Diliman, 2Ateneo de Manila University, 3De La Salle University Manila, 4AI4PEP Philippines, 5National Center for Mental Health
Decision makers are challenged with the uncertain nature of natural hazards, more so when these hazards interact and form a hazard cascade with varying spatial and temporal scales. Despite this, determining the optimal control decision to minimize the impact of hazard cascades based on multiple loss metrics remains the ultimate objective. In this research, we revisited our initial study presented during AOGS 2023, where we modeled the causal relationships of cascading natural hazards with emerging outbreaks as a Bayesian network, with each hazard and its states as nodes containing conditional probabilities and the causal relationship as the links. Here, we used the occurrence probabilities of each hazard in the network and ran multiple random walks to generate cascades and obtain conditional probabilities. We also assessed the impact of the cascades using exceedance probability curves on three loss metrics: persons requiring assistance, income loss, and infrastructure costs. To introduce something new for this conference, we extended our Bayesian network model into a causal influence diagram to incorporate control or decision nodes and utility nodes to identify the optimal level of control to stop a cascade. We applied the framework to the urbanized city of Marikina in the Philippines due to the city being frequented by floods during heavy rainfall, impacting several aspects of the city. We envision this framework to be used by urban planners and city decision makers for disaster preparation and risk mitigation.
IG11-A012
GNSS Data of High Time Rate: New Opportunities to Look Deeper Inside the Ionosphere
Vladislav DEMYANOV1,2#+, Ekaterina DANILCHUK3, Yury YASYUKEVICH4
1Institute of Solar and Terrestrial Physics, 2Irkutsk State Transport University, 3Irkutsk State University, 4Institute of solar-terrestrial physics SB RAS
The warning systems of natural hazards are based on the ground networks of GNSS receivers. However, a GNSS receiver is a “black box” which has never been tuned specially for the ionospheric explorations. GNSS receivers are the primary data source to compute scintillation indices (ROTI, S4, σφ). Reliability of the indices depends on the integration time, amplitude and carrier time rate, de-trending and filtering procedures. GNSS hardware and software play significant role, especially under multipath impact, too. All the issues degrade results of the ionosphere exploration. Besides, multi-scale complex nature of the ionospheruic disturbances, generated by the natural hazards, means that the sensitivity of the ionospheric indices depends on the time resolution of GNSS data. The earlier results based on the amplitude and phase measurements with the data time rate of 100 Hz demonstrated the new opportunity to look far beyond the limitations inside the ionosphere. We suppose that GNSS data registered with high time rate and involving a whole set of GNSS signal components, translated in several frequency bands, provide great novel opportunity to improve the sensitivity of the GNSS sounding methods to explore the ionosphere and enhance effectiveness of the ionospheric warning systems of natural hazards. We present and ready to discuss:1) Our results based on JAVAD, SEPTENTRIO, TRIMBLE, and LEICA receivers, demonstrating that the quality of the slant Total Electron Content (TEC) significantly depends on the GNSS receiver type/model;2) The performance of the ionospheric scintillation indices (ROTI, S4, σφ, d2fi) derived from the GNSS data registered with different time rate;3) Introducing the second-order derivative of the GNSS signal carrier phase (D2fi index) and the deviation frequency (fd - the boundary between the variable part of the phase variations spectrum and noises) as a novel promising scintillation indices to look much deeper inside the ionosphere. The work is financially supported by Russian Science Foundation (project No. 23-17-00157, https://rscf.ru/project/23-17-00157/).
Session Chair(s): Ying-Hsin WU, Kyoto University, Chih-Chung CHUNG, National Central University
IG07-A001
Assessing Long-term Changes in Landslide Restoration Using Landscape Metrics and Spatial Statistics
Uen-Hao WANG, Shyue-Cherng LIAW#+
National Taiwan Normal University
Landslides represent a predominant natural disturbance in forest ecosystems, often precipitating extensive landscape transformations. Despite their prevalence, natural restoration stands out as a noteworthy approach to rehabilitate disrupted ecosystems in Taiwan. This study focuses on the Liouguei experimental plantation, severely impacted by Typhoon Morakot, to delve into the dynamics of landslide mechanisms and long-term restoration. Leveraging multi-temporal landslide Geographical Information System (GIS) layers from the Forestry Bureau, we employ Landscape Metrics, Spatial Analysis, and Logistic Regression methods to scrutinize temporal and spatial alterations in forest restoration and identify pivotal factors steering landslide recovery. Our findings reveal that the initial four years’ post-landslides exhibit a higher percentage of natural restoration compared to the subsequent four years, with the former boasting a restoration rate 1.6 times greater than the latter. Landscape Metrics analysis underscores a surge in landslide patch numbers, increased complexity in patterns, and a fragmented and dispersed landscape structure immediately following Typhoon Morakot. However, both fragmentation and decentralization diminish over time. Logistic regression elucidates the significance of the Perimeter-Area Ratio (Para) Patch metric as the primary driver of natural restoration, accompanied by minor influences from factors such as distance from landslide edges, elevation, precipitation, and the Fractal Dimension Index (FRAC) Patch metric. Key insights gleaned suggest that the accessibility of seed sources is pivotal in landslide restoration, with areas featuring abundant seed reservoirs demonstrating a higher propensity for natural recovery. Habitat-wise, lower elevation coupled with higher precipitation emerges as conducive to natural restoration. These findings offer crucial insights for shaping future forest management strategies.
IG07-A010
How Rapidly Real Landscapes Evolve?
Jisoo LEE+, Kyungrock PAIK#
Korea University
Topography varies continuously due to various forcings. During the last decades, numerical models to simulate whole landscape evolution have been developed and significantly contributed to the discipline. However, it is rarely possible to prove simulation results because of lacking topography records. As an effort to address this basic problem, we investigated the topography change over the longest record available in Korea. We utilized historical topographic map made in the early 1900s when the modern surveying practices were introduced in the country. To deal with a finite domain, the Jeju island is chosen as the study area. We aimed to evaluate any topographic difference by comparing the historic topographic map and the modern Digital Elevation Model (DEM). For the comparison, the historic map given in the form of photographs should be converted into a digital format. We introduce a technique to convert the old map in the form of DEM. We quantitatively calculate the elevation differences between the old and present landscapes. Given that the historical map was made pre-industrial revolution in the island, we anticipate any elevation change attributed to rapid evolutionary processes such as anthropogenic processes and landslides.
IG07-A008
| Invited
Utilization of Big Data for Landslide Mapping in 2015 Gorkha Earthquake Affected Districts of Nepal - An Appraisal for Community Based Disaster Risk Reduction and Mitigation Approach
Suresh CHAUDHARY#+
National Society for Earthquake Technology - Nepal
Nepal, due to its location and diverse physical conditions, frequently suffering from both monsoonal and earthquake induced landslides. Every year the country is spending a significant number of resources for responding to landslides disasters. In this study, we extract distribution and intensity of landslides in 2015 Gorkha earthquake affected 14 districts of Nepal. We used openly available big data sources, and a heuristic, knowledge driven approach based on expert opinions from various descipline for landslide mapping. It was also combined with nine causative factors - geomorphology features, geology distribution, changing landuse/land cover (LULC), slope, aspect, drainage distance, relative relief and vegetation environment. The inventoried map was used to derive landslide susceptibility map of study area categorising into five hazard classes: very low, low, moderate, high, and very high. Our susceptibility maps are produced at different levels site-specific to national level in terms of scale Finally, susceptibility map is integrated with landslide risk reduction and management activities such as awareness raising, preparedness and response planning at local. Moreover, this study was also used for developing municipal risk sensitive land use planning in the study area.
IG07-A009
| Invited
Evaluation of Landslide Hazard in Response to Climate Change and Human Activities in North Sikkim District, Sikkim, India
Kapil GHOSH#+
Diamond Harbour Women's University
Landslide is one of the most hazardous geomorphic processes in the mountain area of Sikkim Himalaya. These processes are intensifying due to climate change and human activities (dam construction, land-use/ land-cover change). This proposed research will focus on getting a better understanding of the response of geomorphic processes of the slope to climate change. A landslide hazard zonation map was prepared to understand the spatial pattern of landslide hazards. Nine geo-environmental factors were considered and integrated with the GIS platform to produce a hazard zonation map. Simple statistics of this additive normalized incidence are computed and used to classify the entire study area into five meaningful landslide hazard zones. The highest incidence of landslide per km2 is recorded for very high-hazard zone (73.67%). The second highest frequency (8.43%) of landslide is found in the high-hazard zone. The status of landslide distribution in different watersheds in North Sikkim district shows that the number of new landslides (identified from satellite images) is comparatively larger than the old slides (identified from 1977 SoI toposheets of 1:50,000). Long-term climate variability has been analyzed from monthly precipitation and maximum and minimum monthly temperature data. Long-term (1950– 2002) rainfall and temperature irregularities are found through Mann-Kendall trend analysis and Sen’s slope analysis. The frequency of landslides in the last few years may be partially controlled by human interference along with the geo-environmental factors of the region. However, the climatic variability is controlling their frequency over different years.
IG07-A014
Integration of Geophysical, Geotechnical, and Rock Physics Diagnostic Techniques for Dynamic Elastic Moduli Determination of Construction on Landslide Prone: A Case Study at Ba Na Hill, Da Nang City, Viet Nam
Hop Phong LAI#+, Duy Thong KIEU, Pham HONG TRANG, Ngoc Dat PHAM
Vietnam Academy of Science and Technology
Vietnam has three-quarters of its territory in mountainous areas. Under the impact of climate change and extreme rain, landslides occur with increasing frequency. This caused great damage to both people and property. In particular, civil construction projects suffered the most damage. To minimize the damage that may occur during the construction design process, it is necessary to calculate ground conditions such as the thickness of the weathered crust and the elastic modulus of the soil layer to serve the design of resistant structures. slide, earthquake. This article presents some results using the integration of geophysical, geotechnical, and rock physics diagnostic techniques for dynamic elastic moduli determination. Dynamic elastic moduli are essential for civil engineering for many purposes since it has represented the load capacity of the soil before deformation to failure. To estimate the dynamic moduli such as Bulk moduli, Shear moduli, Young moduli, P-wave acoustic impedance, and Poisson's ratio for construction design at Ba Na, Da Nang city, both compressional (P) and shear (S) wave velocity are acquired and interpreted by integrating seismic refraction data and geotechnical data that has been validated by a useful technique called rock physics diagnostic (RPD). The subsurface profile is well divided into distinguished three weathering layers which characterized by compressional (P) wave velocity and shear (S) wave velocity ranging from 300-2900 m/s, 500-1500 m/s, respectively, and the unweathered granitic rock beneath the three weathering layers having P-wave velocity, S-wave velocity up to 3000 m/s and 1500-2500 m/s, respectively. The results found that the southeast part of the survey area has much higher weathered soil layers than those of the other parts, implying the lower moduli relation to higher landslide potential could be recognized in the southeast that is potentially suggested as more attention area for foundation design against landslide.
Session Chair(s): Cheolhee YOO, The Hong Kong Polytechnic University, Zhiwei LI, The Hong Kong Polytechnic University
IG33-A004
Long-term Satellite Observations Supports Urban Sustainable Development
Xuecao LI#+
China Agricultural University
Long-term global records of urban extent are helpful in evaluating the environmental impacts of anthropogenic activities. To facilitate cross-disciplinary application, we developed an advanced time-series based approach to extract long-term and fine spatiotemporal resolution urban extent maps, as well as other relevant ancillary datasets (e.g., Global Artificial Impervious Area data and Global Urban Boundary data). Using the derived urban extent time series data, we improved the traditional urban growth models to support diverse studies of urbanization under future shared socioeconomic pathways (SSPs) and the representative concentration pathways (RCPs). We also explored the response of carbon losses and vegetation phenology to urbanization, to mitigate possible risks caused by human activities and support decision-making on sustainable management in the future.
IG33-A009
Study on Spatial Heterogeneity of Heat Island in Local Climate Zone of Coastal City Based on Mobile Observation
Hongchi ZHANG#+, Jin BAI, Jialu GAO, Fei GUO
Dalian University of Technology
Under the influence of global warming and urbanization, urban heat island (UHI) has a huge impact on public health. Local climate zone (LCZ)-based schemes have been proven to assess urban climate. In this paper, taking the coastal city of Dalian as an example, a combined RS- and GIS-based method was used to obtain the LCZ map, and the mobile observation method was applied to analyze the air temperature distributions in each LCZ during daytime and nighttime in summer. The results show that (1) LCZ5 occupies the largest area (about 22%) in the built-up area, followed by LCZ3 and LCZ4. LCZD occupies the largest area in the land-cover area. (2) The UHI intensity (UHII) of LCZs in the central city of Dalian is LCZ1>LCZ3>LCZ7>LCZ10, LCZ9 having the lowest value of UHII. (3) The phenomenon of intra-LCZ variation occurs due to anthropogenic heat removal, mountains, water bodies, etc. (4) UHII showed significant diurnal variation, with nighttime UHII significantly higher than daytime.
IG33-A011
Analysis of Past and Future Urban Growth in Java Island (Indonesia) and Its Impacts on Surface Urban Heat Island and Thermal Comfort
Faiz Rohman FAJARY1#+, Han Soo LEE1, Tetsu KUBOTA1, Vinayak BHANAGE1, Radyan Putra PRADANA1,2, Hideyo NIMIYA3, I Dewa Gede ARYA PUTRA2
1Hiroshima University, 2Indonesian Agency for Meteorology, Climatology and Geophysics, 3Kagoshima University
Java is the most populated island in Indonesia with highly urbanized cities. This study aims to analyze urban growth and its effects on urban heat island (UHI) and thermal conditions using remote sensing in the western part of Java and the three focused urban areas: Jakarta metropolitan area (JMA), Bandung and Cimahi (BC), and Sukabumi (SKB) municipalities. This study also aims to predict urbanization based on the observed urban growth pattern by using a multilayer perceptron neural network-based Markov chain model. Landsat imageries with 30-m spatial resolution from three years were used: 2000, 2009, and 2019. The support vector machine method delivers good accuracy for land use and land cover classification. Surface UHI intensity (SUHII) is analyzed by considering land surface temperature (LST) differences between urban and rural areas. In the last two decades, urban areas have expanded significantly, and SUHII in JMA increased from 1.94 to 3.71 °C, similar in BC but with a lower magnitude. Meanwhile, SUHII in SKB fluctuated between 3.05 and 3.56 °C. LST of the unchanged urban pixels exhibited positive linear trends with magnitudes of 0.25, 0.16, and 0.14 °C/year in JMA, SKB, and BC, respectively. The urban thermal field variance index shows that the strongest UHI is most prevalent in urban pixels. Inside the three regions, the majority proportions are in the "very hot" and "hot" categories, based on the discomfort index. Apart from global warming, the projected increase in urbanization of 2030 and 2050 can have a local impact on worsening urban warming and thermal conditions in the future. The findings will be valuable to the government to develop action planning and policy implementation for sustainable cities.
IG33-A015
Analysis of River-groundwater Environmental Changes Due to Urban Expansion and Climate Change: A Case Study of Daejeon Area
Byeongju JUNG#+, Dong-Woo RYU
Korea Institute of Geoscience and Mineral Resources
Urbanization, along with the increase of impervious surfaces, is causing significant changes in the groundwater and river environments. This affects the natural recharge process of groundwater and can increase the risk of river drying and flooding. Additionally, climate change is frequently causing severe droughts and high temperatures in cities across Europe, and is also contributing to changes in the monsoon patterns and increased heavy rainfall in Asian regions. These changes lead to a decrease in biodiversity, deterioration in water quality, and changes in ecosystems. In this study, we aimed to predict the future changes in the groundwater and river environments affected by climate change and urbanization, using an urban water cycle model developed by integrating the urban expansion model and soil water balance model. Using the Daejeon area as a case study, we presented an urban expansion model based on historical data and applied shared socioeconomic pathways (SSP) to predict changes in groundwater recharge, evapotranspiration, and runoff. The results of simulating changes in the Daejeon area over 100 years, considering both urban expansion and land use changes along with SSP, showed an increase in urban density and a decrease in agricultural and forest lands. Both urbanization and climate change were predicted to decrease groundwater recharge while increasing surface runoff, although the decrease in groundwater recharge and the increase in runoff due to urban expansion and forest reduction were more significant than those caused by climate change. This suggests the critical importance of preventing indiscriminate urban expansion and conserving forests in response to climate change. This study is expected to contribute to understanding the impacts of urbanization and climate change on urban water cycles, predicting disaster possibilities, and establishing sustainable urban development strategies.
IG33-A012
Transforming Urban Greenspace Dynamics and Heat Stress Risks Amidst the Implementation of Hanoi's Master Plan 2030
Yuei-An LIOU1#+, Kim Anh NGUYEN2, Duy-Phien TRAN1
1National Central University, 2Institute of Earth Sciences Vietnam Academy of Science and Technology
Hanoi City has undergone significant transformation because of the implementation of Hanoi's Master Plan 2030, which introduced several challenges for the city, particularly concerning preserving urban green space (UGS). Our work aims to (1) analyze the UGS distribution changes, (2) identify heat stress-prone areas using anomalous land surface temperature (LST) patterns together with population susceptibility, and (3) propose solutions via an advanced UGS management platform. The Sentinel-2 satellite images were employed to analyze the changes in UGS, and LST was extracted from Landsat 8's thermal infrared band, which was employed in mapping heat stress risk. Our work focused on the inner area of Hanoi City and observed UGS changes from October 2016 to October 2018. The study's evaluation was implemented employing Google Earth images and on-site research information. The findings reveal a substantial decline in UGS, with woodland and shrubland decreasing by 1.3% and 4.4%, respectively, whereas grass cover grew by 2.4% over the past two years. The land cover classification had high accuracy (96% in 2018 and 88% in 2016). Moreover, our analysis revealed a greater risk concentrated in the core inner-city zones, characterized by highly populated residential areas and extensive built-up environments. Because air temperature (Ta) impacts human health more critically than LST, our future work will use a spatially continuous Ta dataset to study heat stress risks. The Ta dataset can be created from our recent Ta estimation framework using Machine Learning algorithms, showing an excellent performance. Identifying the distribution of heat stress risks is crucial, drawing the focus of city planners, governing bodies, and healthcare institutions.
IG33-A002
Production of High Resolution GPP Using Sentinel-2 Images
Hyebin PARK+, Yejin LEE, Seonyoung PARK#
Seoul National University of Science and Technology
In this study, high resolution Gross Primary Productivity (GPP) was produced by downscaling MODIS GPP to detect detailed GPP in urban area. This study used Sentinel-2 as high-resolution satellite images for downscaling and flux tower for model verification. Hong Kong, Washington D.C., and Suwon, which are megacities and have flux data, were the study areas. To compare the existing and proposed downscaling methods, four approaches were designed in this study. The first and second approaches consisted of Random Forest (RF) and Convolutional Neural Network (CNN), respectively, based on existing research methodologies. The third approach was designed using Super-Resolution Generative Adversarial Networks (SRGAN). The low-resolution GPP image obtained by upsampling MODIS GPP and the original MODIS GPP became the input of the model. The fourth approach proposed in this study combined SRGAN and existing research methodology. Vegetation indices that can correspond between MODIS and Sentinel-2 were used as SRGAN input. However, since the vegetation index pattern and the GPP pattern differ in downscaling, a loss that indicate the difference between GPP image predicted by existing research methodology and GPP image predicted by SRGAN was added. Then, the GPP spacetime pattern was analyzed from 2018 to 2023 in each urban area and the performance of each approach was evaluated.
Session Chair(s): I-Te LEE, Taiwan Space Agency
IG22-A005
Should We Teach the History of Hydrological Science to Our Students?
Basudev BISWAL#+
Indian Institute of Technology Bombay
Hydrological science has advanced considerably in the past few decades producing process-based dynamic models capable of providing reliable predictions of streamflow for various practical applications. However, the superior performance by current generation machine learning models have raised debates on the need to focus on understanding hydrological processes. I will highlight that any suggestion to ignore the importance of process understanding not only lacks relevance, but such suggestions are also not supported by evidence. A brief examination of the history of hydrological science reveals that data-based models have always played an important role in hydrological science. In fact, modern hydrological science emerged from classical fluid mechanics as a discipline, primarily based on observations but lacking rational explanations. With time those data-based models evolved into models incorporating considerable amount of process understanding. Overall, this presentation will emphasize the importance of critically examining the history of hydrological science.
IG22-A010
Development of a Low-cost Programmable Shaking Platform for Teaching the Basics of Earthquake Science and Engineering
Anthony Guiller URBANO1+, Eligio Jr. OBILLE1, Alfredo Mahar Francisco LAGMAY2, Hannah PEÑA3#
1University of the Philippines National Institute for Science and Mathematics Education Development, 2University of the Philippines Resilience Institute, 3National Chung Cheng University
In recognition of opportunities to integrate emerging technologies into the field of geoscience education, we are developing a microcontroller-based programmable earthquake ground motion simulator. The current prototype is pre-set to simulate horizontal ground motion based on seismometer data recorded during actual earthquake events, such as the July 2022 M7.0 Northwestern Luzon earthquake in the Philippines. The shaking platform is primarily being developed for classroom use to introduce to high school students certain concepts related to earthquake ground motion and the importance of designing earthquake-resilient structures. In earthquake-prone countries such as the Philippines, developing a low-cost and easily reproducible shaking platform could open up plenty of opportunities in advancing earth science education. Development of STEM resources such as the shaking platform seeks to promote research culture among high school students as they conduct investigations, gather and organize data, and identify patterns and trends.
IG22-A013
Developing Effective Earthquake Evacuation Drills at Schools
Satoko OKI#+, Kako OKURA, Akane YOSHIDA
Keio University
In Japan, all schools are required by law to conduct drills for disasters such as earthquakes, fires, and intruders. However, the effectiveness of these drills has not been verified. In earthquake drills at schools, it is common for students to get under their desks and then to be told to evacuate immediately to the school grounds. Principals measure how long it takes for school children to gather. In a real major earthquake, there must be many aftershocks, but these are not considered in drills. Furthermore, if it rains on the day of the drill, it is postponed until the next sunny day. In past major earthquakes, half of the school children were unable to move because they were too scared, some fell and broke bones on the way to the school grounds, and some became ill under the cold weather. On the other hand, in Japan, no school has collapsed in any earthquakes that have ever occurred, due to the earthquake-resistance policy of schools. In short, current evacuation drills do not reflect scientific facts from geosciences. This is partly responsible for the lack of efforts by academia to apply the knowledge and expertise of earth science to school safety. Therefore, we conducted practical training targeting schoolteachers, aiming to simulate the injuries and illnesses that could occur in a major earthquake, as well as the frequent aftershocks and power outages. As a result, it became evident for school teachers that classifying the severity of injuries and sharing information during power outages were challenging tasks. This presentation provides a detailed report on these analyses and proposes a more effective approach to evacuation drills. We also report the positive difference we observed in the school teachers and children after adopting the new drills.
IG22-A014
Effects of "Bosai Narrative" on the Uncertainty of Earthquake Occurrence
Kei USUI#+, Satoko OKI
Keio University
In this presentation, we will present "Bosai Narrative", an essay-based educational material for disaster prevention that approaches the uncertainty of earthquake occurrence. "Bosai Narrative" is an educational material that aims to help students realize the possibility of suffering from earthquake disasters (the word “Bosai” means disaster prevention in Japanese). In this material, the teacher assumes that a major earthquake occurs at a specific date and time in the near future, and students write stories in the first person about their own experience of the disaster. It is characterized by depicting disasters that have not "yet" occurred in the real world as if they had "already" occurred in the story world. This material was developed by Prof. Satoko Oki's laboratory in 2016 and is currently being worked on in schools around Japan. In Japan, one of the world's most earthquake-prone countries, in addition to hardware efforts such as constructing earthquake-resistant buildings and so on, various software efforts have been made to communicate the risks of earthquake disasters. However, current science cannot predict with a high degree of accuracy when, where, or how large an earthquake will strike. Therefore, damage prediction is also accompanied by uncertainty, making it difficult to take an approach. However, since “Bosai Narrative” is based on students’ own personal context, as many damage predictions are generated as the number of students. By practicing this in school, students can not only acquire damage predictions based on their personal situations, but they can further broaden their imaginations by being exposed to the various damage predictions created by their classmates. This is a partial but successful way of covering the uncertainty of damage prediction with variations of predictions. The effectiveness of this as a disaster prevention education is also evident in the data obtained from past practices.
IG22-A001
Using GenAI Tools in Teaching and Learning Earth Sciences
Su-Chin CHANG#+
The University of Hong Kong
Since 2023, a broad range of next-generation artificial intelligence tools have been offered to all HKU teachers and students for teaching and learning purposes. The new HKU policy embraces GenAI and motivates our teachers and students to explore the great potential of GenAI for the benefit of humanity. Regular training, online courses, and other resources are available on campus to ensure the best outcomes of using these non-traditional tools. In this presentation, I will share how GenAI tools are applied to design innovative teaching activities and provide examples of students’ learning achievements. Notably, student assignments from Earth Science courses “Earth Through Time” and “Earth System Science: Contemporary Issues” will be provided. I will also address the beauty and obstacles of engaging with GenAI in the classroom. This sharing aims to promote the development of a creative teaching and learning environment for Earth Sciences through interdisciplinary discussions.
IG22-A011
Sharing Data, Tools, and Knowledge: Resources and Initiatives
Feba FRANCIS1#+, Melissa HART2, Chris LENNARD3, Narelle VAN DER WEL4
1Université Catholique de Louvain, 2University of New South Wales, 3University of Cape Town, 4World Climate Research Programme
The WCRP Academy is the research training advisory and coordination arm of the World Climate Research Program. It is the flagship activity for WCRP´s mission: “to develop, share, and apply climate knowledge that contributes to societal well-being” and works to equip current and future climate scientists with the knowledge, skills and attributes required to tackle the world’s most pressing and challenging climate research questions. The Academy is a hub which connects training providers and users of training. Inclusion within the Academy implies that the training is of high quality and, as such, is a legitimate source of training and professional and capacity development platform that is targeted to climate scientists. In this presentation, we will introduce the Academy and our catalogue of climate science training, which collates in-house WCRP training activities and educational materials to the global science community. Further, the WCRP Academy encourages and invites all research and expert groups, academic and research institutions, government agencies and non-government organizations who provide climate science training and education to register as training providers and contribute to our online training catalogue. The WCRP Academy is building a global community of climate researchers at all career stages to provide global networking and development opportunities to facilitate lifelong learning, global equity, and skills matching for current and future research projects.
IG22-A004
Space Weather Education and Outreach Projects in Thailand
Suwicha WANNAWICHIAN1#+, Siramas KOMONJINDA1, Duangmanee WONGRATANAPHISAN1, Waraporn NUNTIYAKUL1, Achara SERIPIENLERT2, Thirasak PANYAPHIRAWAT1, Kotchanipa CHAINOI1
1Chiang Mai University, 2National Astronomical Research Institute of Thailand
Thailand's awareness about space weather has grown significantly in the past decade. It is now commonly accepted that space weather, the dynamics of particles, and radiation outside the Earth can significantly affect human activities on Earth. Our educational activities aim to exchange ideas, establish cooperation links, and develop a joint strategic working plan for fundamental problems and projects of particle detection, atmospheric physics, ionospheric physics, and aurora. Target Audiences are high school teachers, 3rd-4th year undergraduate students, and early-year graduate students who are either already working or interested in the related fields of particle physics, high-energy astrophysics, space physics, atmospheric physics, and computational techniques. The activities include scientific workshops, a space-weather war room, an Astronomy Olympiad camp, and research training. In particular, the workshop can lead to many research projects at the graduate and post-graduate level, for example, cosmic rays and neutron detectors, the study of the ionospheric disturbance and observations, and space-based observation of the auroral variability during substorm onset.
IG22-A006
Outreach Activities Related to the Sun and Coming Solar Maximum
I-Te LEE1,2#+, Huei-Wen SIAO3, Ping-Han CHENG4, Chao-Yen CHEN2
1Taiwan Space Agency, 2National Central University, 3Central Weather Administration, 4National Taipei University of Education
The sun is not only the source of light and heat for life on the Earth, but also affects the space environment due to its rapid and severe changes. In most mid and high school textbooks, they mainly focus on the movement of this giant star in the sky and its energy, but very few paragraphs talk about the solar activities, solar storms as well as what is space weather. Since the maximum of the solar cycle 25 is coming, therefore, we proposed an outreach education project named “Thousands of miles away, the origin of the space weather - the Sun". This project would conduct more experiments, activities, lectures, and demonstrations which are related to solar activities and solar storms. Through in-school and open activities, professional solar telescopes with light reduction equipment and special filters are used to observe the phenomena on the solar surface like sunspot, solar prominence and active region. Moreover, a hands-on paper model serves as a supplement to explain the solar structure. Meanwhile, this project will conduct training courses for teachers to provide more knowledge which is not shown in textbooks. The topics include how to set up a sunspot projection observation equipment, how to draw, count and classify sunspot, etc. After those courses, participants can have a further understanding of how to do solar observations. In the end, the project hopes all participants understand that the sun not only provides light and heat, but also further affects the space environment after joining this outreach activities.
IG01-A002
Divergent Response of Vegetation Photosynthesis to the Record-breaking Meiyu Event in 2020
Jiuyi CHEN#+, Bo QIU, Weidong GUO, Xin MIAO, Lingfeng LI
Nanjing University, China
Extreme precipitation events have posed a threat to global terrestrial ecosystems in recent decades. However, the response of terrestrial ecosystems to extreme precipitation in areas with various vegetation types and complex topography remains unclear. Here, we used satellite-based solar-induced chlorophyll fluorescence measurements, a direct proxy of photosynthetic activity, to assess the response of vegetation to the record-breaking extreme precipitation event during the East Asia monsoon season in eastern China in 2020. Our results demonstrate that vegetation was adaptable to moderate increases in precipitation, but photosynthetic activity was significantly inhibited by exposure to extreme precipitation because of insufficient photosynthetically active radiation and waterlogging. The responses of vegetation photosynthesis to extreme precipitation were regulated by both vegetation type and topography. Crops in the lowland areas in eastern China were severely damaged due to their higher vulnerability and exposure to extreme precipitation. The topography-induced redistribution of precipitation accounts for the modulation of vegetation response to extreme precipitation. Our research highlights the urgent need for effective management and adaptive measures of croplands under the elevated risk of extreme precipitation in the future.
IG01-A005
Mobile Network Data Analytical Modules of Population Movement Trend Around Points-of-interest Areas
Chia-Jung WU#+, Ming-Wey HUANG
National Science and Technology Center for Disaster Reduction, Taiwan
This study aims to improve the accuracy of risk assessment for the population affected by disasters, such as earthquakes, by cooperating with the government and using mobile-phone data provided by the telecommunication company. The mobile-phone data can reveal the temporal and spatial patterns of people’s movement and location in different areas. This can help estimate the number of affected people more precisely and identify abnormal crowd flow at specific locations. Based on this information, the competent authority can send real-time warning messages to those who are at risk. The mobile-phone data is presented in a grid unit of 500m×500m, and an analytic model is developed to compute the difference after an emergency event. We analyze the population changes after two natural events (one earthquake and one typhoon) and find that there are significant variations after the disasters. The comparison between the population of the background and those after the events can show the impact of the disasters. The change of mobile-phone data for the points of interest is consistent with the actual number of affected people reported by the government official at the time of the disaster. This confirms that the mobile-phone data can be a valuable tool to assist the commander in making decisions when responding to disasters.
IG01-A007
Dynamic Assessment of Spatiotemporal Population Distribution Based on Mobile Phone Data: A Case Study in Xining City, China
Benyong WEI#+, Guiwu SU, Wenhua QI
China Earthquake Administration, China
High-resolution, dynamic assessments of the spatiotemporal distributions of populations are critical for urban planning and disaster management. Mobile phone big data have real-time collection, wide coverage, and high resolution advantages and can thus be used to characterize human activities and population distributions at fine spatiotemporal scales. Based on six days of mobile phone user-location signal (MPLS) data, we assessed the dynamic spatiotemporal distribution of the population of Xining City, Qinghai Province, China. The results show that strong temporal regularity exists in the daily activities of local residents. The spatiotemporal distribution of the local population showed a significant downtown-suburban attenuation pattern. Factors such as land use types, holidays, and seasons significantly affect the spatiotemporal patterns of the local population. By combining other spatiotemporal trajectory data, high-resolution and dynamic real-time population distribution evaluations based on mobile phone location signals could be better developed and improved for use in urban management and disaster assessment research.
IG01-A014
Research on Seismic Risk Assessment Based on Residential Building Stock and Field Survey Results: A Case Study of 3 Cities, Shaanxi Province
Xia CHAOXU#+, Nie GAOZHONG, Wenhua QI, Li HUAYUE
China Earthquake Administration, China
The collapse and damage of buildings caused by earthquakes are the main reasons for casualties. High-precision building data is the key to improving the accuracy of earthquake disaster loss risk assessment. Although the field investigation method based on "township to township" can obtain more accurate building inventory data, considering the economy and timeliness, it is necessary to consider combining remote sensing and other diverse data to achieve the acquisition of building data. Based on the field survey data, combined with the Global Human Settlement Layer (GHSL) data, this paper obtains the proportion data of each type of building and its lethality level in each township based on the classification of building height, and realizes the calculation of the overall lethality level of the building level and township level on this basis. It is found that the fitting results between the calculated results and the field survey results are good, the error is within 0.15, and the fitting results R2 of Xian, Baoji and Ankang are 0.6552, 0.5788 and 0.5937 respectively. Based on this, this paper carries out the earthquake disaster loss risk assessment based on the building level, and finds that the risk of casualties caused by the same type of buildings in each city is different. Generally, the areas with high disaster loss risk in three cities are mainly distributed in urban areas, while the disaster loss risk in newly built areas of each city is relatively low, it can be found that Xi'an has the highest loss risk, while Baoji and Ankang are at the same level. Based on the method constructed in this paper, we can realize the quantitative assessment of earthquake disaster loss risk at the building level, so as to make the pre earthquake emergency preparation and post earthquake auxiliary decision-making more targeted and accurate.
IG01-A023
Urban Ground Deformation of the Greater Manila Area from 2014 to 2022 Using InSAR Time Series Analysis
Jolly Joyce SULAPAS1,2#+, Alfredo Mahar LAGMAY3, Audrei Anne YBAÑEZ1, Kayla Milcah MARASIGAN1, Julian Bernice GRAGEDA1
1University of the Philippines Resilience Institute, Philippines, 2University of the Philippines Nationwide Operational Assessment of Hazards (UP-NOAH), Philippines, 3University of the Philippines Diliman, Philippines
Land subsidence has become a significant global issue caused by either natural or anthropogenic factors, such as excessive groundwater extraction, rapid urbanization, and natural sediment compaction, and is exacerbated by climate change through rising sea levels. In the Philippines, it is recognized as a hazard that threatens Metro Manila and other urban areas. This paper presents updated vertical ground motion rates using Sentinel-1 interferometric synthetic aperture radar (InSAR) time series analysis from 2014 to 2022 through UK COMET’s LiCSAR products and the LiCSBAS package of Morishita et al. (2020). The results revealed a maximum subsidence rate of 10.8 cm/year in Bulacan Province coinciding with industrial and commercial complexes and evident as a contiguous distribution of large and expansive man-made structures. Such subsiding areas are observed as circular to elliptical deformation features in vertical motion maps co-located with zones of compressive motion in horizontal motion maps, most likely related to movements toward areas of peak subsidence. Additionally, these are usually centered on economic zones, tightly-packed residential areas, and technoparks. Towards the east and south of Metro Manila, elongated deformation is associated with the Valley Fault System where left-stepping en echelon faults and horst and graben occur. This is where damages to infrastructure (houses, buildings, road pavements, and walls) have been observed since the 1990s. There is a likely correlation between the splays and ground fissures of the fault and drawdown-induced subsidence. Monitoring this hazard is crucial as it increases the risk of floods, building and infrastructure damage, and economic loss, and exposes residents along the coast to worsening tidal incursions and storm surges due to climate change.
IG01-A026
Developing the Dynamic Crop Calendar of Paddy in Indonesia from 2001 - 2021
Amalia Nafisah Rahmani IRAWAN#+, Daisuke KOMORI
Tohoku University, Japan
According to the Food and Agriculture Organization (FAO), agricultural sectors absorb around 80% of drought’s direct impact. With the climate change impact indicated by the increase of temperature and the rainfall patterns that become more variable, could lead to more severe drought in some regions. This condition could increase the agricultural drought risk that might adversely affect food security. To improve the crop condition monitoring, crop management, and increase the crop production under changing climate, many researchers have developed the crop calendar dataset. The crop calendar contains information about when and where a specific crop is planted and harvested. However, there are two remaining gaps related to this crop calendar: 1) It was developed based on the specific period and then provided as a fixed calendar, thus cannot catch the diversity of cropping season under changing climates, and 2) It was provided on coarse spatial resolution, so it cannot capture the spatial variations, especially on the fragmented agricultural area. This study was conducted to develop the 1-km annual dry season crop calendar of paddy in Indonesia from 2001 – 2021.The crop calendar was developed using a model-based by utilizing the Normalized Difference Vegetation Index (NDVI) to monitor crop greenness that can identify crop growth. The NDVI dataset was obtained from Moderate Resolution Imaging Spectroradiometer (MODIS) through their MOD13A2 product with 16-days intervals from January 2001 – December 2021 with a total of 483 images. Then, the reconstruction of the NDVI timeseries was conducted using the ST-Tensor method, which is suitable for a cloudy and rainy region like Indonesia. After the agricultural area was isolated based on the land cover map from the Ministry of Forestry and Environment, the start of season (planting date), the peak of season, and the end of season (harvesting date) were determined.
IG04-A003
Interpretable Predictions of Chaotic Dynamical Systems Using Dynamical System Deep Learning
Mingyu WANG+, Jianping LI#
Ocean University of China, China
Making accurate predictions of chaotic dynamical systems is an essential but challenging task with many practical applications in various disciplines. However, the current dynamical methods can only provide short-term precise predictions, while prevailing deep learning techniques with better performances suffer from model complexity and interpretability. Here, we propose a new dynamic-based deep learning method, namely the dynamical system deep learning (DSDL), to achieve interpretable long-term precise predictions by the combination of nonlinear dynamics theory and deep learning method. As validated by three chaotic systems with different complexities, the DSDL significantly outperforms other dynamical and deep learning methods. Furthermore, the DSDL also reduces the model complexity and realizes the model transparency to make it more interpretable. We firmly believe that the DSDL is a promising and effective method for comprehending and predicting chaotic dynamical systems in the real world.
IG04-A005
Robust Prediction of Chaotic Systems with Random Errors Using Dynamical System Deep Learning
Zixiang WU+, Jianping LI#
Ocean University of China, China
To predict nonlinear dynamical systems, we recently proposed a novel method called Dynamical System Deep Learning (DSDL), which is based on the theory of dynamical system reconstruction and relies on data for model training. The robust prediction of real-world dynamical systems using observational data with errors is a practical issue. This study primarily investigates the robustness of DSDL in the presence of random errors in real training data. The performance of DSDL is tested on two example systems, namely the Lorenz system and the Kuramoto-Sivashinsky system. The results demonstrate that compared with different traditional deep learning methods and the fourth-order Runge-Kutta method (RK4), respectively, DSDL exhibits high accuracy and stability even in the presence of errors. In terms of accuracy, the DSDL results are comparable to the results of numerical solution method taking RK4 as an example and outperform the results of traditional deep learning. Notably, as the magnitude of errors decreases, the advantages of DSDL become more pronounced, indicating its ability to effectively utilize dynamic information within data sets. Moreover, unlike traditional methods, DSDL does not rely on original equations or hyperparameter optimization and is insensitive to random errors present in training sets. This dynamic-driven method provides greater potential for enhancing the predictive capabilities when analyzing Earth system observational data.
IG04-A007
Insights Into Indian Agriculture: A Deep Learning Approach to Understand the Climatic and Anthropogenic Influences on Rice Yield
Nairit SARKAR#+, Sujata RAY
Indian Institute of Science Education and Research Kolkata, India
Agricultural production, characterized by a prolonged cycle, is susceptible to various internal and external uncertainties. Variations in rainfall, extreme temperatures, fertilizer consumption, and irrigated areas can significantly impact crop yields. Rice serves as the predominant dietary staple for more than 60% of the world's population, playing a crucial role in ensuring food security. India, a significant contributor to world rice production with a 21.5% share, necessitates a comprehensive examination of the possible consequences of climate change and anthropogenic contributions to its rice yield. This study examines the agricultural dynamics of rice production in Indian districts, focusing on the trends of climatic factors and anthropogenic inputs. The non-parametric Mann-Kendall (MK) test, its modified version, and the Theil-Sen estimator were employed to identify and quantify significant trends. The study showed that despite declines in gross cropped area (GCA) across most districts, positive trends in production prevailed due to increased yield. Spearman's correlation test was employed to investigate one-to-one correlations between the factors and the rice yield to detect the most dominant contributor. The correlation test indicates that elevated fertilizer consumption and increased fraction of irrigated land in many districts significantly correlate to the rise in yields. Despite notable climatic changes over the past three decades, the correlation between rice yield and variations in annual and seasonal rainfall and extreme temperatures has proven mostly insignificant. The multivariate analysis using Artificial Neural Network (ANN) provided more insights than traditional correlation coefficients in finding the key contributing factors. The top three models, which exhibited the best fit, collectively established that anthropogenic inputs exerted the most substantial influence on the fluctuations in rice yield in India over the past three decades.
IG04-A009
Microearthquakes Detection Using a Machine Learning Analysis in Gangwon Province, South Korea
Byeongwoo KIM1#+, Minhwan KIM2, Tae-Kyung HONG1
1Yonsei University, Korea, South, 2Kyung Hee University, Korea, South
Gangwon province is located in the northeastern South Korea and characterized by mountainous terrains. The region experienced strong ground motions from a magnitude 4.8 earthquake in 2007, bringing concerns on potential seismic damage. Detection of scattered microearthquakes is challenging for conventional methods such as short-term to long-term average ratio analysis and matched filter analysis of which sensitivity is limited by ambient noise and station proximity. In this study, we detect offshore microearthquakes. We employ a machine learning-based approach for microearthquake identification to overcome the limitation. Utilizing the trained PhaseNet machine learning model, we successfully detect P and S phases in the seismic records and identify microearthquakes based on coherent phase arrivals across stations. We collect seismic data from 175 stations deployed in the northeastern area of South Korea since 2021. We select areas of relatively high seismic activity. We additionally collect seismic data from ~80 temporally-deployed geophones since April 2023. We observe around 70 microearthquakes every month. The microseismicity is high in the Hongcheon area and coastal regions of the East Sea (Sea of Japan). This study presents numerous microearthquakes in regions characterized by low seismicity, demonstrating the effectiveness of the method. Subsurface blind fault structures are illuminated by the microseismicity.
IG04-A012
Improved Statistical Downscaling for Short-term Forecasting of Summer Air Temperatures Based on Deep Learning Approach
Dongjin CHO#+, Jungho IM, Sihun JUNG
Ulsan National Institute of Science and Technology, Korea, South
Reliable early forecasting of extreme summer air temperatures is essential for effectively preparing and mitigating the socioeconomic damage caused by thermal disasters. Numerical weather prediction models have become valuable tools for operational forecasting air temperature. However, they incur high computational costs, resulting in coarse spatial resolution and systematic bias owing to imperfect parameterization. To address these problems, we attempted to develop a novel statistical downscaling and bias correction method (named DeU-Net) for the maximum and minimum air temperature (Tmax and Tmin, respectively) forecasts obtained from the Global Data Assimilation and Prediction System with a spatial resolution of 10 km to 1.5 km over South Korea through the fusion of deep learning (i.e., U-Net) and spatial interpolation. In this study, we used a methodology to decompose statistically downscaled Tmax and Tmin forecasts into temporal dynamics over South Korea and spatial fluctuations by pixels. When comparing the proposed DeU-Net with the dynamical downscaling model (i.e., Local Data Assimilation and Prediction System) and support vector regression (SVR)-based statistical downscaling model at the seen and unseen stations for forecasting the next-day Tmax and Tmin, respectively, DeU-Net showed the highest spatial correlation and the lowest root mean square error in all cases. In a qualitative evaluation, DeU-Net successfully produced a detailed spatial distribution most similar to the observations. A further comparison extending the forecast lead time to seven days indicated that the proposed DeU-Net is a better downscaling approach than SVR, regardless of the forecast lead time. These results demonstrate that bias-corrected high spatial resolution air temperature forecasts with relatively long forecast lead times in summer can be effectively produced using the proposed model for operational forecasting.
IG04-A016
Characteristics of Soil Geochemical Anomalies and Prospecting Prediction in Baixingtu Area, Alxa Right Banner, Inner Mongolia
Wen GAO+, Xianrong LUO#, Jiewei LI
Guilin University of Technology, China
In order to preferably select the prospecting prediction target area in Baixingtu area of Alxa Right Banner, 1:10,000 soil geochemical measurements were carried out on the basis of identifying the geological conditions of mineralization in the area. Elemental variation coefficients, ILR-Robust transform and ILR-PCA were used to analyze seven elements of Au, Ag, Co, Cu, Pb, Zn and As in the measuring area. The results show that: (1) ore-forming elements are mainly located at the intersection between the fracture and mineralized alteration zone. Au and Ag show very strong differentiation and enrichment characteristics with the highest mineralization potential, while Pb, Zn, As, Co and Cu show low differentiation and enrichment characteristics, and low mineralization potential. (2) ILR-Robust transformation eliminates the closure effect of the original data and makes the elements show standard normal distribution; the first principal component of ILR-PCA can extract the comprehensive information of the elements of the original data to the maximum extent, i.e., the positive end-load of PC1 (Au-Ag-As) is the mineralization indicator, and the intensity and morphology of elemental anomalies are controlled by the fracture and mineralization alteration zone, and the negative end-load (Co-Cu-Pb-Zn) is caused by the enrichment of elements in multi-phase magmatic hydrothermal activity. (3) Engineering verification of the mineralization target area No. Ⅰ has identified several gold (silver) ore (mineralization) bodies, and the gold and silver contents have reached the minimum industrial grade or above, indicating that the Baxingtu area has a large potential for gold and silver prospecting.
IG04-A018
Long-term PM2.5 Concentration Prediction Under Climate Changes Using Geo-AI Based Machine Learning Model
Wei Lun HSU1+, Yu Ju LIN1, Pei-Yi WONG1, Yu-Ting ZENG1, Shih-Chun Candice LUNG2, Chih-Da WU1#
1National Cheng Kung University, Taiwan, 2Academia Sinica, Taiwan
Air pollution is a pressing issue, threatening human health and societal development. The likely increase in air pollution due to climate change underscores the intricate interplay between air quality and environmental challenges in the 21st century. The objective of this study is to assess the changing trend of PM2.5 levels in response to climate change. In order to predict PM2.5 concentrations in Taiwan's mainland, where air quality stations are limited, this research combines the principles of land use regression and harnesses the capabilities of machine learning algorithms. The machine learning model incorporates various factors, including land use elements and other pertinent variables, enabling the capture of nonlinear relationships. Data comprising daily average PM2.5 observations and meteorological information spanning from 1994 to 2019 were gathered, with additional consideration given to related variables such as land use inventory and landmark data. Five machine learning algorithms, namely eXtreme Gradient Boosting (XGBoost), Gradient Boosting Machine (GBM), Light Gradient Boosting Machine (LGBM), Categorical Boosting (CatBoost), and random forest, were utilized to predict the PM2.5 concentration. The models' performance was evaluated through multiple validation processes. To project long-term PM2.5 levels based on the climate scenarios outlined in the IPCC Sixth Assessment Report (AR6), data on future projected temperature and precipitation will be obtained from the Taiwan Climate Change Projection Information and Adaptation Knowledge Platform (TCCIP). The projections for long-term PM2.5 concentration under climate scenarios SSP3-7.0 were conducted using climate data simulated by global climate models (GCMs), including MIROC6 and MPI-ESM1-2-LR. The analysis revealed that PM2.5 concentrations did not exhibit a definitive correlation with various climate scenarios.
IG04-A019
A Ship Speed Prediction Model Based on Meteorological Ocean Element Data
Jin ZHUYU#+
Chinese Academy of Meteorological Sciences, China
In order to more accurately predict the speed loss of ships under various sea conditions, a real-time vessel speed prediction model based on ensemble learning algorithm was proposed. Eighteen trans-Pacific vessel AIS speed data from China to North America were selected, and the wind speed, effective wave height, sea surface velocity, wave period and other elements of ERA5 and HYCOM data were selected as training features. The random forest method was used to calculate the relative importance of many input features. The selected features were trained into the ensemble learning model: LightGBM, which is a lightly and higher efficiency machine learning model compare with others, and the AIS speed data of one voyage was selected as the test set to verify the model effect. The results show that compared with the traditional stall equation based on the empirical formula, the ensemble learning model based on data-driven has better prediction performance. The RMSE of the predicted speed and the real vessel speed is 0.87, and the RMSE of the empirical equation is 2.02, the RMSE improvement rate is 56.9%. The running time of the model can reach the minute response, which meets the requirements of real-time ship speed prediction. The vessel speed prediction model with high accuracy and strong real-time performance can provide a theoretical basis for ships to take reasonable measures to avoid severe weather such as strong wind and waves in the future, which is of great significance to the improvement of ship navigation safety and the operation efficiency of vessels and related ports.
IG04-A028
Development of a High-resolution Dataset Based on the C-LSAT 2.0 Land Surface Air Temperature Dataset
Sihao WEI#+, Qingxiang LI
Sun Yat-sen University, China
Land surface air temperature is a crucial indicator of climate change and a significant focus of global and regional climate research. Scientists have long been committed to researching the homogenization of station data and the development of grid datasets. Several benchmark grid datasets of global land surface air temperature have been available since the instrumental era, including CRUTemp, GHCN, GISTEMP, BEST, and C-LSAT. These datasets have been crucial in supporting research related to global climate change. However, due to their rough resolution, many details of regional climate change are difficult to reflect. Based on the global land surface air temperature dataset C-LSAT 2.0 independently developed by our team, we develop a global long-time series (1901-2022) with high spatial resolution (0.5° × 0.5°) land surface air temperature grid dataset C-LSAT HR. The C-LSAT 2.0 station data undergoes quality control before being decomposed into a climatology field (1971-2000) and an anomaly field. The climatology and anomaly fields are then interpolated into 0.5° × 0.5° gridded data using partial thin-plate spline (TPS) and Adjusted Inverse Distance Weight (AIDW), respectively. Finally, the two fields are merged into C-LSAT HR. In the field of climatology, the global average mean absolute error (MAE) and root mean square error (RMSE) of C-LSAT HR are 0.263 °C and 0.439 °C, respectively. Regarding the anomaly field, the global average annual MAE and RMSE are approximately 0.4-0.6 ℃ and 0.6-0.9 ℃, respectively. The global land surface air temperature anomaly series based on C-LSAT HR and C-LSAT 2.0 exhibit a high level of consistency. The C-LSAT HR indicates that the average warming trend of each season in the Northern Hemisphere is higher than that in the Southern Hemisphere. Additionally, the average warming trend in winter and spring is higher than that in summer and autumn.
IG04-A030
Improving Deep Learning-based Ground Deformation Detection and Extraction from InSAR Images with Noisy Interferograms Synthesized by Generative Adversarial Networks
Xuekai LIN#+, Caijun XU
Wuhan University, China
With the ever-increasing volume and accessibility of InSAR images, the automatic detection and extraction of ground deformation signals from various tectonic or geological processes (e.g., earthquakes, volcanos, and landslides) have become a pressing and valuable task. Supervised deep learning approaches have shown great promise in this regard. However, these geological events occur infrequently, making it impossible to obtain a sufficient number of interferograms containing these ground deformation signals from the real world for deep learning model training. Consequently, most previous studies resort to using synthetic interferograms, which are a combination of synthetic deformation and simulated noise signals, to train the models. Unfortunately, the application of these models to real-world data is not yet satisfactory due to the gap between the distribution of synthetic and real data. While the number of real interferograms (positive samples) containing effective deformation signals is scarce, interferograms containing only noise (negative samples) are readily available. Generative Adversarial Networks (GAN), where a generator and a discriminator are included, are known for their ability to learn the distribution from real samples and produce realistic synthetic samples. In this work, we constructed a conditional GAN model with real-world noisy interferograms. In the GAN model, the generator produces synthetic noisy interferograms based on randomly generated vectors and topographic data to confuse the discriminator. In this way, more realistic noise signals that have the potential to bridge the distribution gap between the synthetic and real-world samples can be generated. Subsequently, we train deep learning models for ground deformation detection and extraction using these synthetic noisy interferograms as well as simulated deformation signals. Performance improvement could be observed when applying the model trained with interferograms synthesized by GAN to detect and extract deformation signals from real-world InSAR observations.
IG06-A004
Geochemical and Thermal Characteristics of Hot Spring Waters in the Japanese Island Arc
Risako KIMURA#+, Hitoshi TOMARU
Chiba University, Japan
A large number of hot springs are widely distributed in Japan, closely associated with the development of a geothermal regime in the island arc system. These areas are geologically important for understanding the fluid-rock reactions, material circulation processes, and the utilization of geothermal resources. In this study, we analyzed the chemical and isotopic composition of hot spring waters collected from various locations across the Japanese island arc to characterize the geochemical features and discuss the origin and geothermal history of these waters. We have employed hexadiagrams and trilinear diagrams in the classification of hot spring waters. Additionally, geothermometers with Na-K, Na-K-Ca, and SiO2 concentrations were used to estimate the subsurface temperatures. Hot spring waters exhibiting higher estimated temperatures are generally of meteoric water origin and enriched in Na-HCO3, Ca-SO4, Ca-HCO3, and Na-SO4. These waters are largely influenced by volcanic gases, volcanic fluids, and the thermal energy derived from recent volcanic activities. In contrast, hot spring waters with relatively lower temperatures, enriched in Na-Cl, are considered to have interacted with seawater and fossil seawater, often sourced from non-volcanic areas like sedimentary basins and coastal regions. The geochemistry of hot spring waters primarily reflects their interactions with rocks, especially in high-temperature environments, leading to active material circulation. It serves as a significant indicator of subsurface processes essentially linked to the development of the island arc system.
IG06-A005
Advancing Groundwater Level Prediction for Irrigation by Using the XGBoost-based Approach
Sheng-Wei WANG1#+, Yen-Yu CHEN2, Li-Chiu CHANG2
1National Central University, Taiwan, 2Tamkang University, Taiwan
Groundwater resources play a pivotal role in sustaining agriculture, and predicting groundwater levels is essential for effective water resource management. Agriculture faces significant impacts from climate change-induced alterations in rainfall patterns, especially during drought. The physical models and machine learning methods are the most popular approaches for groundwater level prediction, this study highlights the efficiency of the latter as an emerging technology, providing a viable alternative that demands less time and extensive hydrogeological data. Hence, this research employs the XGBoosting method to predict groundwater levels, incorporating pumping well electricity consumption, precipitation, and current groundwater levels as model features. The research zone around a groundwater observation well in central Taiwan encompasses 2,418 pumping wells and a rainfall observation station within a five-kilometer radius. In regions characterized by dense irrigation for agriculture, obtaining precise groundwater extraction data proves challenging. To address this, we utilize electricity consumption data from pumping motors as a quantifiable representation of pumping behavior. Monthly data from 2007 to 2019 and 2020 to 2021 were used for model training and testing, and predictions, respectively. R2 values of 0.99 and 0.60 are achieved for training and testing, with 0.72 for predictions, accompanied by an RMSE of 1.27. Notably, the model exhibits stability for up to 18 months. This study offers a valuable framework for proactive groundwater management, presenting a promising tool for sustainable agricultural water use. The findings underscore the importance of accurate groundwater predictions in fostering agricultural sustainability and resilience to climate change.
IG06-A008
Ground Subsidence and Hydrological Properties in Yangon, Myanmar
Saw MYAT MIN1#+, Yu WANG1,2, Yunung Nina LIN3, Win NAING4
1National Taiwan University, Taiwan, 2Nanyang Technological University, Singapore, 3Institute of Earth Sciences, Academia Sinica, Taiwan, 4University of Yangon, Myanmar
Yangon is the former capital city of Myanmar, hosting ~ 2.75 % of the total population (55 millions of people) in the country. The city is bounded by the Yangon River to the south and the Bago River to the east, with the Shwegondaing-Mingalardon anticline sandwiched in between. In the past century, the city of Yangon has gradually expanded from its core area above the anticlinal crest to the adjacent low-lying flood plain. Owing to the rapid population and economic growth in the past decade, the public water supply system failed to cover the whole metropolitan, leaving a large proportion of residents dependent on groundwater from private wells. The lack of proper groundwater regulations and the increased extraction of groundwater from the low-lying flood plain raise the risk of land subsidence and flood hazards in Yangon. This study aims to derive the long-term ground deformation of Yangon by using multi-temporal interferometric synthetic aperture radar (MTInSAR) techniques. We obtain displacement time series from the L-band ALOS data for the period of 2007-2009 and from the C-band Sentinel-1 data for the period of 2015 to 2022. Our result indicates higher subsidence rates (up to 2.8 cm/yr) in the eastern flood plain area of Yangon during 2007-2009, which further increased to more than 10 cm/yr during the period of 2015-2022. In the western flood plain area, the subsidence rate is a few millimeters per year during 2015-2022. For the downtown area, the ground subsidence rate is less prominent due to the Pleistocene formations exposed along the anticline. The subsidence record obtained in the western part of the city agrees with the long-term trend of the only groundwater head record in this area. Together with the aquifer system constructed from hydrological wells, we estimate the first geodesy-based hydrogeological properties for the Yangon area.
IG06-A009
Combining Convolutional Neural Network and Hydraulic Tomography for Hydraulic Heterogeneity Estimation
Zi-Yan CHOU+, Jui-Pin TSAI#
National Taiwan University, Taiwan
Characterizing the heterogeneity of hydraulic parameters (K or Ss) in the subsurface is crucial for contaminated site remediation. Hydraulic Tomography (HT) is a well-developed approach for estimating three-dimensional hydrogeological parameters fields by capturing variations of groundwater head stimulated by pumping/injection events. The head variations from HT are converted to three-dimensional parameter fields using successive linear estimation (SLE), a well-proven geostatistical inverse method in various scale problems. However, the computational efficiency decreases as the number of grids or head observations increases. To overcome this issue, we propose an HT-based convolutional neural network (HT-NN) to replace SLE for converting groundwater head variations into hydraulic heterogeneity. We generate 10000+ random fields and produce their corresponding head observations using a forward model as input and output data pairs for training HT-NN. The results show that HT-NN successfully converts the groundwater head variations into hydraulic parameters fields. The proposed HT-NN can be an efficient and alternative tool to depict the subsurface heterogeneity.
IG06-A010
An Impact Estimation of Irrigation and Groundwater Pumping on the Regional Hydro-climate Using an Earth System Model
Yusuke SATOH1#+, Yadu POKHREL2, Hyungjun KIM1,3, Tokuta YOKOHATA4
1Korea Advanced Institute of Science and Technology, Korea, South, 2Michigan State University, United States, 3The University of Tokyo, Japan, 4National Institute for Environmental Studies, Japan
Irrigation is an anthropogenic forcing to the Earth-system that alters the water and heat budgets at the land surface, leading to changes in regional hydro-climate conditions. It is imperative to better understand the nature, extent, and mechanisms through which irrigation affects the Earth's system. However, despite its increasing importance, irrigation remains a relatively nascent component in the Earth-system modeling community, necessitating advancements in modeling and a deepened understanding. Our research aims to improve the quantitative understanding of the impacts of irrigation and groundwater use as anthropogenic drivers on regional climate and environmental changes. To this end, we developed an improved Earth-system modeling framework that is based on MIROC-ES2L (Hajima et al 2020 GMD) coupled with hydrological human-activity modules (Yokohata et al. 2020 GMD), enabling the simulation of a coupled natural-human interaction. Employing this Earth-system model, we carried out a numerical experiment utilizing an AMIP set-up. Here, our ensemble simulation allows for statistical quantification of the irrigation impact differentiating them from the uncertainties arising due to natural variability. We have identified regions and seasons where irrigation exerts a discernible influence on regional hydro-climate. Notably, our results show substantial disparities—larger than or comparable to inter-annual variability—between simulations incorporating and excluding the irrigation process, particularly in heavily irrigated regions such as Pakistan and India. Our model demonstrates that the introduction of moisture into the soil through irrigation alters the hydrological balance of the land surface, consequently influencing the overlying atmosphere. Furthermore, our study delves into estimating regional variations in the contributions of groundwater and surface water use to these impacts. Emphasizing the importance of a more nuanced understanding of regional characteristics in irrigation impact assessments, our research underscores the significance of coupled earth system models in comprehending and predicting the intricate interplay between human activities and the Earth's climate system.
IG06-A012
Data-driven Investigations Into Land Subsidence Evolution and Its Impacts on Infrastructures in Choushui River Fluvial Plain
Thai Vinh Truong NGUYEN+, Chuen-Fa NI#, I-Hsien LEE, Gumilar Utamas NUGRAHA
National Central University, Taiwan
Severe land subsidence in Taiwan’s Choushui River Fluvial Plain (CRFP), primarily triggered by long-term groundwater extraction for agricultural irrigation, poses a major environmental threat. This study integrates data from an extensive range of monitoring systems, such as groundwater level monitoring wells, Global Positioning System (GPS) stations, survey leveling benchmarks, multi-level compaction monitoring wells, and Interferometry Synthetic Aperture Radar (InSAR), to investigate the complex patterns and causes of subsidence in this important agricultural region. The analysis demonstrates a significant correlation between the decline in groundwater levels and the rise in subsidence magnitudes. This relationship is particularly evident in areas with a high concentration of fine-grained sedimentary materials, where sediment compaction is most significant within the first 150 meters of depth. In addition, the study examines 292 Sentinel-1 SAR images using the SBAS-PSInSAR technique, revealing significant sinking in the southern part of CRFP, which is strongly associated with regions containing high percentages of fine-grained sediment. These findings emphasize the harmful impact of subsidence on essential infrastructures, particularly the high-speed railway, highlighting the necessity of ongoing monitoring and the integration of multiple monitoring approaches for efficient subsidence management. The study highlights the intricate nature of land subsidence in the CRFP and the ongoing need to expand and maintain land subsidence monitoring networks.
IG06-A013
Evaluation of Baseflow Dynamic Through Hydrological Signatures in Taiwan
Hsin-Yu CHEN#+, Hsin-Fu YEH
National Cheng Kung University, Taiwan
Baseflow comes from delayed sources associated with rainfall events and plays a critical role in sustaining streamflow and river ecosystems during non-rainy periods. Taiwan is facing increasingly severe water challenges, including droughts and floods due to extreme weather events. Evaluating baseflow is benefit for effective ecological and water resource management. However, baseflow cannot be directly observed and measured. To address this, this study employed baseflow separation methods combined with hydrological signatures to assess dynamic baseflow characteristics. This study utilized three separation streamflow approaches—UKIH, Lyne-Hollick, and Eckhardt algorithms—to quantify baseflow. Eleven baseflow dynamic signatures included baseflow index (BFI), frequency of high-baseflow and low-baseflow days, seasonality ratio (SR), representative baseflow percentiles (Qb5, Qb33, Qb50, Qb66 Qb95), concavity index (CI) and slope (SBDC) of baseflow duration curve, were used to characterize baseflow. This study investigated the spatial distribution of baseflow signatures and analyzed the factors influencing these signatures to get the following findings (1) a comparative analysis of different baseflow separation algorithms, (2) explanation of spatial regional patterns and upstream-downstream evolution of baseflow signatures, and (3) identification of significant influential factors on baseflow dynamics. These insights into baseflow processes and influencing factors are beneficial for enhancing environmental resilience and advancing water resource management in Taiwan catchments.
IG06-A015
Long-term Analysis of Hydrological Sensitivity and Memory Characteristics in Taiwan Catchments
Ting-Jui FANG#+, Hsin-Yu CHEN, Hsin-Fu YEH
National Cheng Kung University, Taiwan
In recent years, the world has been grappling with the impacts of abnormal and extreme weather events, and Taiwan is no exception. The unusual frequency of typhoons and droughts has resulted in uneven spatiotemporal distribution of precipitation, contributing to extreme climate disasters. The water resource in Taiwan is quite hard to store due to the rapid-changing river flow and the steep topography. Moreover, prevention of hydrological disasters such as floods and droughts become significant challenges. Notably, when considering the current climate factors, the inherent memory ability of the catchments itself is often neglected. The significance of streamflow within the catchment's memory reflects the importance of water storage and propagation in the hydrological system. Thus, understanding the degree of control over changes in streamflow becomes crucial. To better comprehend the behavior of Taiwan's catchments in response to external climate factors and internal memory characteristics, this study conducts an analysis across 67 catchments with data spanning over 30 years. In terms of the impact of climate factors, the study employs the relative streamflow elasticity coefficient to quantify the sensitivity of catchment streamflow to precipitation and potential evapotranspiration. This study understands how streamflow responds to external climate conditions. Regarding catchment memory, an analysis of climate parameters and streamflow is conducted to assess the significant influence of past hydrometeorological conditions on the streamflow in current year. The results indicate that the elasticity coefficient is effective in analyzing the sensitivity of catchments in Taiwan, revealing that certain catchments have memory capabilities. These findings contribute to the hydrological prediction and offer valuable insights for hydrological modeling, as well as water resource development and management.
IG06-A017
Optimization Strategies in Unstructured Mesh Generation for Micro-scale Porous Media
I-Hsien LEE#+, Chuen-Fa NI, Thai Vinh Truong NGUYEN
National Central University, Taiwan
To evaluate the chemical reactions, physical processes, and transport mechanisms of carbon dioxide in reservoir formations are essential. Particular emphasis should be placed on the changes in pore structure and rock properties. This study is to simulate the perfusion of carbon dioxide within the cores and explore fluid transport at the micro-scale. The main tasks of this project involve analyzing X-ray CT images, constructing pore networks based on image brightness, and comparing simulation results with image analysis using mesh generation module. The three-dimensional tetrahedral mesh of the pore network is generated using the unstructured mesh generation module, and a computable mesh file compatible with fluid mechanics software is created. Ultimately, the image analysis process will be integrated to provide the Institute of Nuclear Energy Research with a basis for subsequent refinement.
IG07-A002
Geotechnical Characterization and Shear Strength Analysis of Rain-induced Shallow Landslides in Mt. Diwata, Monkayo, Davao De Oro, Philippines
Kristine Mae CARNICER1,2#+, Joel MAQUILING1
1Ateneo de Manila University, Philippines, 2Ateneo de Davao University, Philippines
This study aims to identify the potential mechanism of the frequent rain-induced shallow landslides in Mount Diwata, Monkayo, Davao de Oro, Philippines. It will investigate how the shear strength parameters of the soil from various landslips relate to the moisture content and their physical and index properties. Analysis of the direct shear test results showed that the increase in the water content decreased the shear strength of the slopes in the landslide sites. This suggests that water saturation is the primary trigger of these slope failures since they occur after days of heavy rains. In addition, the study's findings also point to the significant influence of soil composition and grain size on the soil's shear strength behavior. While the friction angle generally decreases with increasing water content for both fine-grained and coarse-grained soils, a contrasting behavior for cohesion was observed for these two. The apparent cohesion rises with increasing water content for coarse-grained soils. However, for fine-grained soils, cohesion initially increases when the water content increases but decreases when a specific moisture content is attained. These findings suggest that the shear strength is primarily attributed to cohesion for fines and friction angle for the coarser particles. The data gathered in the study can provide valuable insights to identify the most appropriate engineering interventions and mitigating solutions for this recurring problem in Mount Diwata.
IG07-A004
Fundamental Study on Estimating the Location of Buried Objects Due to Landslides Using Particle Methods
Kodai MORI1#+, Satoru OISHI1,2
1Kobe University, Japan, 2RIKEN, Japan
Consider estimating the location of buried victims after the onset of a landslide involving people; it is necessary to detect the victims. This study uses the Smoothed Particle Hydrodynamics (SPH) method, a type of particle method for numerical analysis to estimate the burial position of an object assuming a victim. The Drucker-Prager model, a type of soil constitutive law, is used to analyze mudslides based on [Bui et al., 2008]. The Passively Moving Solid (PMS) model presented in [Koshizuka et al. 1998] has simplicity and high computational efficiency for the solid-liquid multiphase flow analysis method. In this method, a rigid body is modeled as a collection of particles. Like solid particles, object particles are calculated as particles with different densities. After that, the object particles are fixed as a rigid body. To ensure the validity of the analytical method, we refer to [Bui et al. 2020] and compare it with the soil self-weight collapse experiment in [Lube et al. 2014]. The PMS model was also validated by buoyant oscillations due to the density difference between the object and the fluid, as shown by [Wang et al., 2019]. Subsequently, as a fundamental stage of the research, a sensitivity analysis was conducted on the factors that could influence the final burial position under ideal conditions of only object particles, soil particles, and wall particles. Perturbations were applied to the slope angle, viscosity, and initial object particle distance as influencing factors, respectively, and the factors affecting the object burial position were considered.
IG07-A006
Development of Multi-spatial-temporal Fusion Technologies for Rock Slope Monitoring
Chih-Chung CHUNG#+, Bo-Chi CHEN, Chun-Cheng LIN, Yu-Zhi QIU, Te-Wei TSENG
National Central University, Taiwan
The rock slopes in Taiwan are hazardous due to the influence of climate and earthquakes. The rock slopes were analyzed for different trigger factors, simulating the impact range of rock slope sliding. However, in the early stage, the project is mainly based on laboratory experiments and numerical analysis. It still needs the application and verification of substantive monitoring technology. The main topic of this sub-project is the research and development of multi-spatio-temporal scale monitoring technologies integrated into the early warning of rock slopes. This task will be based on the survey results for different rock slope failure mechanisms and approach monitoring technologies at different time and space scales. First, the space scale to be monitored will be from long-range satellite or ground-based InSAR monitoring long-term LOS (Line of Sight) displacement, combined with developing a dual-band sacrificial GNSS displacement monitoring device in the local area for comparison and verification. Furthermore, the simultaneous development of long-term real-time photogrammetry of simple optical and thermal image modules will be applied to monitor a rock slope surface. In order to introduce and test distributed strain sensing by optical fiber, in conjunction with laboratory tests and evaluations to monitor slope deformation will be proceeded; extended to distributed vibration sensing (Distributed Acoustic Sensing, DAS) for vibration (earthquake or falling rocks) or even long-term seismic analysis, can further observe the change of the shear wave velocity in the rock slope with time; in addition, through the time domain reflection method (Time Domain Reflectometry, TDR ), which can be used to monitor rock nails or anchors. This Sub-project is the integrated base of the above-mentioned novel monitoring methods to feedback to calibrate and validate physical and numerical models.
IG07-A012
Rainfall Landslide Threshold Values for Shallow Landslides in Selected Areas of the Bicol Region, Philippines
Beth Zaida UGAT1#+, Decibel FAUSTINO-ESLAVA1, Jenielyn PADRONES1, Juan Miguel GUOTANA1, Yusuf SUCOL1, Jefferson RAPISURA1, Bianca Maria Laureanna PEDREZUELA1, Maria Regina REGALADO1, Rosemarie Laila AREGLADO1, Gabriel Angelo MAMARIL1, Loucel CUI1, Wei-Yu CHANG2
1University of the Philippines Los Baños, Philippines, 2National Central University, Taiwan
The Philippines is a gateway for extreme weather events in Asia. Every year, the country experiences several tropical cyclones and heavy rains that often result in disasters. One of the triggers for these disasters are shallow landslides that damage properties and cause great loss of lives. An emerging method to mitigate the effects of landslide disasters is the generation of rainfall landslide threshold values for susceptible areas. This study presents the results of an initiative to generate such thresholds for a volcanic region in the country. The work involved crafting a simplified data collection platform to build up a landslide database from which rainfall-landslide thresholds were generated using the empirical information. Correlation work to find associations between the thresholds and land cover types allows for exploring the use of threshold values to fortify ecosystems-based disaster risk reduction and management measures. For the study areas, Albay and Sorsogon, a total of 279 events from 1985 to 2022 were collected from various sources such as reports of mandated agencies, news articles, online reporting platforms, and even social media. Out of these, only 82 events qualified to be used for generating the threshold values. On average, 33mm/hr rainfall intensities trigger landslides within the study area. Depending on the land cover type, rainfall events can trigger landslides between 28 to 40mm/hr in agricultural areas, shrublands, and built-up areas. The threshold values per land cover type will be discussed, including implications on how the management of particular ecosystems can reduce risks associated with rainfall-induced landslides.
IG07-A013
Analyzing the Impact of Rainfall-induced Pore Pressure on Slope Stability: Perspectives from a Tank Model Using a 3-D Geological Model of a Dip Slope
Alvian R. YANUARDIAN#, Jia-Jyun DONG+, Chih-Hsiang YEH, Chia- Huei TU, Jia-Yi WU
National Central University, Taiwan
For any engineering project, a 3-D geological model is crucial for estimating geological conditions, especially those related to the hydrogeological and slope stability of the dip slope. This study proposes the tank model as a fast way to know the abnormal pore pressure changes caused by rainfall and geological conditions. Moreover, FLAC3D analysis is chosen to enhance our comprehension of the diverse factors influencing slope stability. We found that the bedding plane is not planar by LiDAR-based analysis, 16 borehole observations, and site observation. A fault in the West of the research area might cause it. Thus, polynomial surface analysis was carried out to identify the 3-D geological model in our research area. By analyzing the top of L2 from 6 boreholes, 38 corrected elevation points, and 8 LiDAR points, we successfully modeled the bedding plane controlled by fault where the structure contour at the West of the research area was relatively tilted to the Northwest. On the other hand, calibrating the tank model's parameters based on a hydraulic test was used to get the best fit simulated groundwater level’s result. Therefore, we adopted and re-calibrated the tank model’s parameters of the hydraulic test to ensure a fit for the rainfall case. Afterward, we made a prediction. As a result, the tank model's simulated groundwater level and the monitoring well's observed groundwater showed a good corresponding result with the RMSE close to zero. Moreover, our prediction of rainfall-pore pressure response also showed a good corresponding result. In conclusion, concerning different joint densities parallel to the slope surface, the findings indicate varying anisotropic distributions in pore water pressure and distinct shear strain areas corresponding to changes in joint density.
IG08-A005
The Link Between Atmospheric Persistence and European Heatwaves
Emma HOLMBERG1#+, Gabriele MESSORI1, Rodrigo CABALLERO2, Steffen TIETSCHE3, Davide FARANDA4
1Uppsala University, Sweden, 2Stockholm University, Sweden, 3European Centre for Medium-Range Weather Forecasts, Germany, 4University of Paris-Saclay, France
We investigate the link between European heatwaves and the persistence of large-scale atmospheric-circulation patterns. Leveraging concepts from dynamical systems theory, we assess atmospheric persistence, and reconcile this approach with the more conventional meteorological views of persistence. We find a weak yet significant link between the occurrence of heatwaves and anomalously persistent circulation patterns in the mid-troposphere, although few significant persistence anomalies when considering the surface circulation patterns. We thus argue that persistent atmospheric configurations are not a necessary requirement for heatwaves and that the results depend to a considerable extent on region and tropospheric level. Finally, we discuss the applicability of this metric to reforecast data, and the potential value of persistence as an additional forecast verification metric.
IG08-A008
Cluster Analysis of Tropical Cyclone Tracks Affecting South Korea Using a Self-organizing Map
Han-Kyoung KIM1+, Jong-Yeon PARK1#, Jun-Hyeok SON2
1Jeonbuk National University, Korea, South, 2IBS Center for Climate Physics, Korea, South
From 1982 to 2020, 144 tropical cyclones (TCs) that affect South Korea are classified into two clusters using a self-organizing map. TCs entering the emergency zone defined by the Korean Meteorological Administration (west of 132° E, north of 28° N) are considered as those affecting South Korea. These two clusters exhibit differences in the average genesis location, track length, and maximum wind speed of TCs. The first cluster has an average genesis location in the northwest part of the western North Pacific (WNP), with a relatively short track length and weaker maximum wind speed. From an interannual variability perspective, the frequency of TCs in the first cluster shows a high negative correlation with eastern Pacific sea surface temperature (SST) (corr = -0.43, P<0.01), interpreted as a result of variations in the Walker circulation caused by changes in eastern Pacific SST. In contrast, the second cluster has an average genesis location in the southeastern WNP, with a relatively long track length and stronger maximum wind speed. This cluster displays a strong positive correlation with central Pacific SST (corr = 0.54, P<0.01), and it is analyzed that the cause of the high correlation is related to the Gill-type response associated with central Pacific SST.
IG08-A014
Enhancing Climate Resilience Through Comprehensive Assessment of Slopeland Disaster Risk Under CMIP6 Scenarios
Yun-Ju CHEN#+, Yi-Hua HSIAO, Jun-Jih LIOU
National Science and Technology Center for Disaster Reduction, Taiwan
"The impacts of climate change are constantly increasing. It is crucial to understand disaster risks and implement climate risk assessments as outlined in Taiwan's "Climate Change Adaptation Act" (2023). This study aims to comprehensively assess climate change risks, specifically focusing on slopeland disaster risk under diverse CMIP6 warming scenarios. Utilizing climate model data after statistical downscaling, this study quantifies three critical indicators—hazard, vulnerability, and exposure—using the Quantile method. Additionally, geological disaster potential maps enhance the evaluation of terrain vulnerability. This study employs the aforementioned index-based approach to analyze slope disaster risk maps at different spatial scales, including 5km grids and township areas scales. Furthermore, for the convenience of users we have developed a Climate Change Disaster Risk Adaptation Platform (http://gg.gg/drancdr) , allowing online access to slopeland disaster risk maps. This interactive platform empowers users to query trends, assess risk levels for townships and cities, and explore climate indicators. The methodology employed in this research provides scientifically robust data, offering valuable insights for policymakers and stakeholders engaged in climate change adaptation and disaster risk management. This contribution aligns with ongoing efforts to fortify climate change resilience and foster sustainable development in the face of evolving climate challenges.
IG08-A015
Could “Hurricane” Pose Major Risk to Europe?
Kelvin NG#+, Gregor C. LECKEBUSCH
University of Birmingham, United Kingdom
Tropical cyclones (TCs) are recognized for their substantial socioeconomic impact on coastal cities. While some TCs remain confined to the tropics throughout their entire lifecycle, others migrate into the midlatitudes, retaining the physical characteristics of hurricanes. Some even undergo structural evolution, transforming into post-tropical cyclones (PTCs). We collectively refer to these phenomena as Cyclones of Tropical Origin (CTOs). CTOs can exhibit exceptional intensity, with hazards that distinguish them from typical extratropical cyclones. Recent occurrences of CTOs, such as remnants of Hurricane Ophelia (2017) and Hurricane Leslie (2018), have made landfall in Europe, resulting in significant damage. This prompts the question: are these isolated events? And will these events become more common in future climates? The current quantification of CTO risk is hindered by a lack of observations as well as lack of theoretical understanding of CTOs. In this presentation, we elucidate the fundamental principles of our methodology designed to address the challenge of insufficient observations, employing the UNSEEN approach. The UNSEEN approach enables the construction of a physically consistent event set, particularly suited for the study of extreme and rare events. Recently, this methodology has proven effective in typhoon hazard assessments in the Western North Pacific. Subsequently, we present preliminary results illustrating the genuine hazard posed by North Atlantic CTOs to Europe.
IG08-A018
Localizing Precipitation Parameters for Early Warning by Applying Machine Learning to Remotely Sensed Cloud Properties
Hwayon CHOI+, Yong-Sang CHOI#
Ewha Womans University, Korea, South
Early warning of precipitation is important globally to ensure people's safety and prevent economic losses from disasters related to rain. Since precipitation and cloud properties are closely related, we would like to try precipitation early warning using the properties of clouds. Additionally, these precipitation conditions are expected to vary depending on the region, so research is needed to determine independent conditions between regions. In this study, we aim to provide early warning individually for each region whether it will rain within the next 2 hours by using cloud brightness temperature, cloud optical thickness, and cloud effective radius among the cloud properties variables provided by geostationary satellites. Among the data used in this study, the cloud property variables were from the Korean geostationary satellite GEO-KOMPSAT-2A, and precipitation information was from Integrated Multi-Satellite Retrievals for Global Precipitation Measurement precipitation data. We used machine learning techniques to find precipitation conditions appropriate for each latitude and longitude, and measured the accuracy of the precipitation probability prediction algorithm using three indicators: Probability of Detection (POD), False Alarm Ratio (FAR), and Critical Success Index (CSI). As a result of this study, our method showed higher accuracy than previously known parameters, especially CSI. This result suggests that the missed alarm rate, the event of precipitation occurring despite not being forecast, has reduced. Additionally, precipitation conditions vary depending on the properties of clouds, and new regionalization is proposed by grouping areas with similar precipitation conditions. These results are expected to enable higher accuracy early warnings and improve understanding of precipitation conditions through localization using cloud properties information.
IG08-A019
Comparison of Different Downscaling Models for High-resolution Precipitation in Korea
Minjeong KONG+, Yong-Sang CHOI#
Ewha Womans University, Korea, South
Recently, extreme rainfall frequently occurring in South Korea has caused numerous casualties and property damage. To predict and manage such damage, high-resolution precipitation data is needed. However, there are limits to the data that can be obtained due to the lack of ground observatories. To overcome these limitations, we aim to produce and compare daily high-resolution (1 km) precipitation data using three models: linear regression, MK-PRISM (Modified Korea-Parameter elevation Relationships on Independent Slopes Model), and random forest model. In particular, the random forest model is a distance-based deep learning model newly proposed for producing high-resolution precipitation data. The daily precipitation data was based on ground observation station data from the Korea Meteorological Administration. The difference between estimated and observed values was calculated to measure the accuracy of the calculated high-resolution daily precipitation data. As a result, linear regression and random forest models tended to underestimate, while MK-PRISM tended to overestimate compared to observed values. Among the three models, the random forest showed the best performance. These findings could provide a universal daily precipitation estimation method based on deep learning that covers the entire South Korea. In addition, it will be helpful for estimating climate risk as basic data.
IG08-A020
Enhancing Quantitative Precipitation Estimation in the NWP Using Deep Learning Model
Haolin LIU#+, Zhenning LI, Jimmy Chi Hung FUNG, Alexis LAU
The Hong Kong University of Science and Technology, Hong Kong SAR
Precise precipitation quantification is vital for minimizing damage and safeguarding lives during extreme weather events, especially in a rapidly changing climate. Current quantitative precipitation forecasting (QPF) in numerical weather prediction (NWP) models heavily relies on parameterization schemes for microphysics, cumulus clouds, etc, introducing significant uncertainties due to our limited understanding of precipitation processes. To address this challenge, we propose a deep learning model based on the Vision-Transformer architecture. Our model directly utilizes fundamental meteorological variables computed by NWP models as inputs and quantitatively maps them to precipitation maps derived from satellite-merged data. We conducted Weather Research and Forecasting (WRF) model simulations with a 27km grid resolution over China and Southeast Asia from 2017 to 2021. We used simulation data from the wettest seasons of 2017-2019 for training and validated and tested the model on 2020 and 2021 data. The deep learning model aims to bypass uncertainties in physical parameterization schemes, driven by our incomplete understanding of physical processes, and reproduce high-resolution satellite rainfall observations (CMORPH data). Evaluation results on the test dataset demonstrate that our deep learning model effectively extracts meteorological features, leading to significant improvements in precipitation forecasting skill scores. Specifically, we achieved improvements of 21.7%, 60.5%, and 45.5% for light rain, moderate rain, and heavy rain, respectively, on an hourly basis. Two case studies under different synoptic conditions also exhibit promising results in estimating heavy precipitation during strong convective events. Overall, our proposed deep learning model offers vital insights into capturing precipitation-triggering mechanisms and enhancing precipitation forecasting accuracy. Additionally, we discuss the sensitivities of the fundamental meteorological variables used in our study, training strategies, and potential limitations. In conclusion, our approach addresses the limitations of current QPF methods, showing promise for more accurate precipitation forecasting, crucial for mitigating the impact of extreme weather events in a changing climate.
IG09-A003
Modern to Relict Sediment Continuum in the Taiwan Strait
Dominique VALDIVIA1#+, James LIU1, Rick YANG1, Aijun WANG2, Yonghang XU2, Yu-Min CHOU3, Chih-Chieh SU4, Yu-Shih LIN1
1National Sun Yat-sen University, Taiwan, 2Ministry of Natural Resources, China, 3Southern University of Science and Technology, China, 4National Taiwan University, Taiwan
The Taiwan Strait (TS) facilitates sediment exchange from Mainland China, encompassing large dispersal systems like the Zhujiang and Changjiang rivers, smaller rivers along the Zhejiang-Fujian coast, and those originating from Taiwan's mountainous rivers. A comprehensive multi-proxy investigation spanning the entire strait is essential to grasp the interplay between relict and modern sediments, enhancing comprehension of the modern-to-relict sedimentary continuum within the TS. Based on clay minerals, the primary fluvial source for sediments in the TS is sediments exported by the Changjiang River, which is enriched in Chlorite-Kaolinite. Another fluvial source, the Minjiang River, exported sediment enriched in Kaolinite. Sediments from Taiwanese rivers are enriched in Chlorite, which lacks Smectite. We identified two types of modern sediments: a) polymodal silt on the western side of the TS in the Zhe Min-Taiwan Strait mud belt, which is enriched with Kaolinite, b) polymodal silt on the eastern side of the TS is enriched with Chlorite-Smectite and exhibits a very low magnetic susceptibility. In the northeastern TS, in the Guanyin Depression, sediments exhibit a different type of bimodal silty sand enriched with Illite with very low magnetic susceptibility, which might correspond to a palimpsest type. In southern TS, TB is covered by well-sorted bioclastic coarse sand with high quartz content. Our findings suggest their sediments correspond to a transition from a relict type to a palimpsest type. At this preliminary stage, the information we collected shows the distribution and characteristics of relict and modern sediments in different parts of the TS. Our future work will be focused on understanding the interplay between modern and relict sediments and the hydrodynamic regime that might be responsible for the reworking, winnowing, and resuspension of particles.
IG09-A004
Mass-transport Complexes (MTCs) and Bathymetrical Control on Submarine Channels: A Case Study from the Taranaki Basin, NW New Zealand
Wenjing LI1#+, Nan WU2
1State Key Laboratory of Marine Geology, Tongji University, China, 2Tongji University, China
Mass-transport complexes (MTCs) are ubiquitous on continental margins worldwide. During emplacement, MTCs can evacuate tremendous volumes of sediment and dramatically modified seabed geomorphology. However, the role of MTCs, more specifically their top surfaces, in influencing subsequent sedimentation processes has been largely overlooked. Therefore, we adopt multibeam bathymetry and 3D seismic reflection data from Taranaki Basin, NW New Zealand, to investigate the interaction between buried MTCs and subsequent sedimentary processes. We interpret a shallow buried MTC that is c. 19km long and 16km wide, covering an area of c. 250km2, deposited near the upper slope of the study area. The existence of the headwall scarp and lateral margins has created a large ponding space on the top surface of the MTC. When subsequent channels debouch into the headwall scarp, their flow direction diverts from NNW to NNE, and the width and depth of the channel have increased from 640-1600m to 54-70m separately. The giant blocks (c.54-86m high, 370-600m wide) within MTC have created a set of local topography highs on the top surface, which have influenced the morphology of subsequent channels by regulating the direction of flow and defining the location of crevasses. Additionally, thrust-fault-like structures have been revealed on the western levee of the channel, indicating that lateral confining pressure generated by the flow energies are extremely high when the channel flows into these topographies. Thus, we suggest that the top surface of MTCs can cause huge accommodation spaces, forming a 'mini basin' like geometry that can divert the flow direction, enhance the erosional ability and flow energy, and control the distribution pattern of subsequent channelling processes. We indicate that this process can facilitate submarine sediment transportation and redistribution from shallow to deep marine settings, which is also essential for deciphering the pathways from sediment source to sink systems.
IG09-A013
A Hidden Submarine Giant: Observation, Interpretation and Implication
Nan WU#+
Tongji University, China
Submarine landslides (slides) are ubiquitous on continental margins worldwide, they can cause damaging tsunamis and destroy submarine infrastructures. In the Gippsland Basin and Bass Canyon regions, southeast offshore Australia, we observed a giant seabed slide (termed Bass Slide) extending more than 450 km and covering an area of c. 30,000 km2. We combine high-resolution multibeam bathymetry, 2D and 3D seismic reflection, and core data to investigate the kinematic indicators and preconditioning factors of the Bass Slide. We found at least five buried slides deposited below the headwall part of the Bass Slide. These buried slides exhibit a retrogressive pattern based on the spatial distribution of their basal shear surfaces. We demonstrate that the giant Bass Slide can be formed by repeated slope failure processes, and that landsliding is still active in shaping the system. This supports previous studies indicating that tsunamis have been a significant geomorphic process in the Gippsland Basin since the late Pleistocene. We therefore consider the study area to have a high tsunami risk, which requires modelling-based studies to determine if any coastal regions are at risk in the future.
IG09-A029
Various Amberground Marine Animals on Burmese Amber with Discussions on Its Age
Yingyan MAO+, Diying HUANG#
Chinese Academy of Sciences, China
Burmese amber represents the world’s most diverse biota in the Mesozoic. Previous studies have focused on the biodiversity of its inclusions, as well as pholadid borings. Here we report a variety of marine animals symbiotic with or adhere to Burmese amber or the amber deposits, including crinoid columns, corals and oysters. We propose that there is no distinct evidence indicating the secondary transportation of Burmese amber over long distances. The ancient sedimentary environment was likely located in the coastal area. The hardening time of the resin was not long after secretion. The resin has been mixed with fragments of marine organisms in the ancient sediments, and has been deposited for a longtime. The zircon age in the sediments surrounding amber approximately represents the age of Burmese amber, but due to limits of the method, the current zircon U-Pb SIMS age maybe younger. Therefore, as far as the situation is concerned, the age of Burmese amber may be close to the boundary between the Albian and Cenomanian, or even late Albian. We suggest that it is plausible to generally refer to the age of Burmese amber as mid-Cretaceous, and a precise age requires further biostratigraphic and chronological studies.
IG09-A030
The Spatiotemporal Evolution of the Early Cretaceous Jehol Biota in East Asia
Daran ZHENG1#+, Su-Chin CHANG2, Haichun ZHANG1
1Chinese Academy of Sciences, China, 2The University of Hong Kong, Hong Kong SAR
The modern terrestrial ecosystems greatly developed during the mid-Cretaceous, characterized by the dominance of angiosperms. The flourishment of the angiosperms drives elevated species richness by co-evolving with insects, vertebrates and fungi, strongly altering the Cretaceous climate and water cycles by increasing bedrock weathering. The Lower Cretaceous non-marine sediments in East Asia contain the famous Lagerstätte: the Jehol Biota. This Biota produced numerous exceptionally well-preserved fossils, including feathered dinosaurs, early birds, mammals, amphibians, pterosaurs, insects and early angiosperms, contributing to tracking the early evolution of modern terrestrial ecosystems. The Jehol Biota sensu stricto is a terrestrial fossil assemblage mainly distributed in northern Hebei Province, western Liaoning Province, and southeastern Inner Mongolia Region of the North China Craton, characterized by the 'Eosestheria-Ephemeropsis-Lycoptera' (EEL) assemblage. This assemblage has a very wide distribution in East Asia thus generating the view of the Jehol Biota sensu lato. The evolution of the Jehol Biota was generally divided into three evolving stages, i.e., Jehol Biota stages I to III (JBS I to III), represented by the fossil assemblages from the Dabeigou (~132–130 Ma), Yixian (~125–122 Ma) and Jiufotang (~122–115 Ma) formations, and their corresponding strata. The Jehol Biota begins with the appearance of elements like Ephemeropsis trisetalis (insect) and Peipiaosteus (fish) during the JBS I. It flourished during the JBS II, further developed during the JBS III, and finally transformed into the Fuxin Biota during the late Early Cretaceous. JBS Ⅱ was the evolutionary climax of the Jehol biota, and nearly all the typical vertebrates and angiosperms of this biota appeared. The biota’s survival of the middle Early Cretaceous breakup of Gondwana and the destruction of the North China Craton demonstrates an adaptive response to long-term environmental changes. This study widely investigated the Lower Cretaceous in East Asia, collecting abundant fossils to recover the Early Cretaceous terrestrial biodiversity and palaeogeography in East Asia. The spatiotemporal evolution of the Jehol Biota is evaluated after a comprehensive study from biostratigraphical, biogeographical, high-precision geochronological, and quantitative analyses.
IG09-A032
The Baiwan Biota from the Qinling Orogenic Belt Linked to the Early Cretaceous Biological Dispersal in Central China
Siyu SONG1#+, Daran ZHENG1, Xiao TENG1, Su-Chin CHANG2, Honghe XU3, Bo WANG3, Haichun ZHANG1
1Chinese Academy of Sciences, China, 2The University of Hong Kong, Hong Kong SAR, 3Nanjing Institute of Geology and Palaeontology, Chinese Academy of Sciences, China
The Qinling Orogenic Belt (QOB) was uplifted during the Jurassic, forming the boundary zone of the climate division in China. However, it remains unclear whether this Belt has developed as the palaeogeographic isolation barrier for the biological communications between the North China Craton (NCC) and South China Craton (SCC) during the Mesozoic. We here report the Baiwan Biota (ca. 123.9 Myr ago), a new Early Cretaceous terrestrial fossil assemblage from the Baiwan Formation of the Baiwan Basin, southwestern Henan Province in the QOB. This biota contains abundant invertebrate fossils, as well as an angiosperm fossil, mostly belonging to the typical elements of the Jehol Biota, which was widely distributed in East Asia. Biostratigraphical and detrital zircon analyses reveal the absence of drainage systems between the southern NCC and QOB. Further quantitative analyses support that the QOB prohibited the biological dispersal between the southern NCC and QOB during the Early Cretaceous, and the Jehol Biota (especially its aquatic components) was probably expanded along the Shangdan Fault within the QOB. This study reveals the unique palaeogeographical position of the QOB for exploring the development of Cretaceous terrestrial ecosystems.
IG10-A004
Numerical Investigation of Run-up and Sediment Transport of Tsunami-like Solitary Waves on Fine-sand Beaches
Shuo LI1,2+, Huabin SHI1#
1University of Macau, Macau, 2Zhuhai UM Science & Technology Research Institute, China
A two-phase Smoothed Particle Hydrodynamics (SPH) model is adopted in this study to numerically investigate the hydrodynamics and sediment transport by tsunami-like solitary waves in the swash zone of fine-sand beaches. The model is carefully calibrated and validated regarding the run-up height and the sediment transport rate under solitary waves in laboratory experiments. The calibrated model is then employed to investigate the influential factors of the run-up and the sediment transport. Dimensionless relationships between the factors and the run-up height and the sediment transport pattern are proposed based on a large number of numerical experiments. The quantitative results help to assess the impact of tsunami-like solitary waves on sandy beaches.
IG10-A005
A New Tsunami Earthquake Model for the 1771 Meiwa Event and Implication for the Bathymetric Effect on the Tsunami Boulder’s Distribution
Koki NAKATA1#+, Kazuhisa GOTO1, Hideaki YANAGISAWA2
1The University of Tokyo, Japan, 2Tohoku Gakuin University, Japan
In 1771, the large tsunami (Meiwa event) struck the Sakishima islands, Japan. By this event, tsunami run up ~ 30 m in elevation and 12000 people died. Previous studies proposed several tsunami source models for this event but it is still debated. In addition, more reliable and accurate historical record data was developed in recent years and these data was not used in the previous works. These studies also used coarser topographic and bathymetric data for the tsunami calculations and they may be insufficient for the accurate tsunami modeling. In order to update the source model of the Meiwa tsunami, we adopted high-resolution topographic and bathymetric data with the latest historical record as a constraint. The results show that a very large slip (30 m) is required in the shallow and narrow area along the Ryukyu Trench to reproduce the Meiwa tsunami run-up height distribution. Indeed, the model can be classified as a tsunami earthquake. As well as large fault rupture, inelastic deformation of unconsolidated sediments and/or submarine landslides may be involved in this large slip. Our high-resolution modeling allowed us to understand the detail propagation and run-up processes. For example, it was known that tsunami boulders are deposited along the coasts but their distributions were not uniform. Our modeling results suggested that these boulders were concentrated in the area where the tsunami was higher than the surroundings. The wave ray analysis further revealed that tsunami propagation was strongly controlled by bathymetry and hence boulders’ distribution as well. Since these boulders are fragments of corals or coral reefs, our results in turn suggest that the impacts of tsunamis on corals and coral reefs are also heterogeneous: their damage could have been controlled by bathymetry.
IG10-A008
Formation Processes of Erosional Landforms by the 2011 Tohoku-oki Tsunami
Haruki IMURA#+, Kazuhisa GOTO
The University of Tokyo, Japan
The 2011 Tohoku-oki tsunami caused extensive geomorphological changes along the Pacific coast of Tohoku, Japan. Although extensive surveys of tsunami deposits were conducted using various methods, tsunami erosional features have not been studied well due to the limited locations where erosion occurred and their transient natures. Nonetheless, residential and agricultural areas have been significantly damaged by the tsunami erosion. Understanding formation processes of erosional landforms by modern tsunamis are essential to better understand paleotsunami processes. In this research, we aimed to elucidate the formation processes of erosional landforms by the 2011 Tohoku-oki tsunami in various locations along the Pacific coast of Tohoku to clarify the factors that determine where erosion occurs through the field survey as well as analyses of satellite imageries and numerical calculations. Our results revealed that tsunami erosion is often caused by prolonged return flow rather than by the strong but short-lasting impact of run-up flow. In fact, while the run-up flow can cause some minor erosion at the coast, the return flow, which concentrates in low-lying coastal areas, generates a strong current with high Froude Number. This current toward the sea persists for tens of minutes and forms localized but significant erosional landforms. Our study also found that the tsunami erosional features are largely controlled not by the wave height but rather by the topography (slope inclination) in the inundation area. While, the localized erosional landforms are strongly influenced by the meter-scale microtopography. Our discovery underscores that coastal erosion by the tsunami is closely linked to both macro- and micro-topography. This in turn indicate that there is a predictability at the sites of future significant tsunami erosion based on the geomorphological analysis and tsunami sediment transport modeling.
IG10-A009
A Proposed Approach Towards Estimating Tsunami Drift to Aquaculture Rafts Through the Development of a Drift Simulation Model
Kento TANAKA1#+, Anawat SUPPASRI1, Yoshinori SHIGIHARA2, Fumihiko IMAMURA1
1Tohoku University, Japan, 2National Defense Academy, Japan
Coastal aquaculture is widely practiced in Japan. Aquaculture rafts, which consist of culture of shellfish and other macroalgal species, are generally placed in shallow marine regions – making them extremely susceptible to wave impacts. Tsunamis frequently cause damage to aquaculture rafts in Japan, even when tsunami generation source is distant. Despite a relatively small wave height, tsunami waves could result in drift motion of a freely floating object and hence, significant damage to the object. However, our knowledge of drift motion due to tsunami and the relationship between tsunami drift motion and aquaculture raft damage is still limited. Additionally, there are only few attempts in current literature that have developed methods in predicting tsunami drift damage to aquaculture rafts. Therefore, the objective of this study is to develop a model for drift simulation of aquaculture rafts during a tsunami, to predict and reduce the drift damage Tsunami drift, quantified by the object’s (in this case, raft’s) position and orientation, can be estimated by solving the equations of motion through numerical simulation of tsunami water level and current velocity. Since the aquaculture facilities have anchors for mooring, in this study, the equations of motion are solved including the frictional resistance due to the concrete anchors. However, due to the complex structure of aquaculture rafts, it is challenging to calculate drag coefficient just from numerical simulation. We have therefore also created models of aquaculture rafts and performed laboratory experiments to measure their drag coefficient. The improved model was applied to the 2022 Tonga volcanic tsunami scenario, with Yamada Bay, Japan as our case-study area. When validated with observation data, our results show that rafts that were damaged/not damaged during the 2022 event were similar to those simulated.
IG10-A010
Suggestion on Developing Indonesia Tsunami Observation Networks and Forecasting System Based on Deep Learning
Muhammad Rizki PURNAMA#+, Anawat SUPPASRI, Kwanchai PAKOKSUNG, Constance Ting CHUA, Fumihiko IMAMURA
Tohoku University, Japan
Past events of the catastrophic tsunami in Indonesia, such as Flores tsunami 1992, Banyuwangi tsunami 1994, The Great Indian Ocean tsunami 2004, Pangandaran tsunami 2006, Palu tsunami 2018, and Krakatau tsunami 2018, have caused significant damage and losses in the coastal area. Most of the events are triggered by a submarine earthquake. One of which is from the Java subduction zone. Three major earthquakes with tsunamis have been caused by deformation along this subduction zone. Thus, this zone covers most of the populated as well as critical areas spanning from Java to Nusa Tenggara. Therefore, Indonesia needs a decent Tsunami Early Warning System. There are only six existing OBPGs (Ocean Bottom Pressure Gauges) to inspect tsunami wave propagation in Indonesia's deep-sea area to issue an early warning. In this research, we assessed the optimal deployment of tsunami buoys along The Southern part of Java Island to Nusa Tenggara and made a simple deep-learning-based model to forecast the tsunami waveform in the nearshore area. First, we create a set of synthetic tsunami multi scenarios using a stochastic-slip earthquake model for the Java Megathrust fault. Next, we apply the empirical orthogonal functions (EOF) based on the tsunami scenarios to determine the initial location for the deployment of each tsunameter. We also assessed the reliability of the spacing and bathymetry for each suggested sensors. Finally, we apply a series of deep learning models to forecast tsunami waveforms and further inundation area in the nearshore area.
IG10-A024
A Decade After the Onslaught: Tracking Down Super Typhoon Haiyan Deposits and Other Potential Strong Wave Events in Leyte Island, Philippines Using eDNA
Wenshu YAP1#, Janneli Lea SORIA2+, Ronald ILOREN3, Mischa HAAS4, Adonis GALLENTES5, Jodivine NAVAROSA6, Mark Russel GUATNO7, Clyde PELESCO8, Nathalie DUBOIS 9, Fernando SIRINGAN5, Adam SWITZER1
1Nanyang Technological University, Singapore, 2Mindanao State University at Naawan, Philippines, 3ETH Zürich, Switzerland, 4Kanton Luzern, Dienststelle Umwelt und Energie, Switzerland, 5University of the Philippines, Philippines, 6Central Visayan Institute Foundation, Philippines, 7Guatno Surveying Services, Philippines, 8GeoPoint Land Surveying Services, Philippines, 9Eawag, Switzerland
Understanding the recurrence interval of extreme coastal events, such as super typhoons, is crucial for coastal zone management and resilient community development. While the sedimentary deposits of these extreme coastal events offer valuable records, their preservation potential beyond historical timescales presents a significant challenge. This study explores the viability of environmental DNA (eDNA) as a complementary tool for fingerprinting the overwash signatures of Super Typhoon Haiyan (ST Haiyan) in Leyte Island, Philippines, a decade after the event. In June 2023, we revisited and collected transect cores of the previous study conducted by Soria et al in 2017, which documented the thickness of the overwash deposits. The Nypa mangrove forest recorded a thickness of 5-7 cm, while inland, about 1.2 km from the coast, had a 1-3 cm thickness. The varying distances from the coast and deposit thicknesses allow us to capture potential spatial variations in deposit characteristics and eDNA preservation. Despite differences in deposit thickness, grain size, sorting, and composition between sites, eDNA analysis consistently differentiates ST Haiyan deposits from pre- and post-event soil samples. These findings demonstrate the remarkable persistence of eDNA within overwash deposits even under variable preservation conditions. This suggests the potential of eDNA as a valuable proxy for reconstructing past extreme events beyond traditional sedimentological approaches. This work presents a significant advancement in reconstructing historical coastal hazard events and their long-term impact on coastal communities. Leveraging eDNA’s resilience and discriminatory power opens a novel tool for enhancing the interpretability of sedimentary records of marine inundation events and extending typhoon history to centennial or millennial timescales, thereby informing coastal hazard mitigation strategies for a safer future.
IG11-A001
| Invited
Integration of Dynamical Downscaling and a Time-lagged Ensemble to Enhance Medium-range Forecasts for Agricultural Applications
Subin HA1, Eun-Soon IM1#+, Jina HUR2, Sera JO2, Kyo-Moon SHIM2
1The Hong Kong University of Science and Technology, Hong Kong SAR, 2National Institute of Agricultural Sciences, Korea, South
More accurate and reliable meteorological information in advance of up to a month is expected to have significant implications for impact sectors such as agricultural practices. With the increasing demand for subseasonal-to-seasonal weather forecasts, many organizations and institutions worldwide produce GCM-driven forecasts extending several months. However, the coarse resolution of these forecasts often hinders their applicability and usefulness for farmers and agricultural stakeholders, limiting their ability to make informed decisions based on accurate and localized meteorological information. In this regard, this study aims to produce fine-scale 1-month forecasts tailored in South Korea by dynamical downscaling of NCEP Climate Forecast System version 2 (CFSv2) operational forecasts initialized at different times. The optimal time-lagged ensemble technique, utilizing systematically selected members, is also employed to enhance predictability. By offering a range of potential meteorological conditions in advance, this approach is vital for facilitating the implementation of timely adaptation measures, thus assisting in mitigating the adverse impacts of natural hazards that are expected to worsen in a changing climate. Acknowledgments: This study was carried out with the support of “Research Program for Agricultural Science & Technology Development (Project No. PJ014882)”, National Institute of Agricultural Sciences, Rural Development Administration, Republic of Korea.
IG11-A002
Nowcasting of Landslides: A Geo-satellite Synthesis Approach for Real-time Hazard Mapping Across Asia and Oceania
Min-Jae KWON#+, Yong-Sang CHOI
Ewha Womans University, Korea, South
Landslides are one of the most widespread natural hazards on Earth, inflict huge losses of both life and property every year. In advance of landslide occurrences, people located in landslide hazard area need risk information to prepare for the disasters. According to landslide catalog, 75% of landslide cases are triggered by rainfalls which occurs in short time and needs near-real time monitoring. For continuous observation, geostationary satellite data are useful which cover global scale area and observe a short timescale. In this study, we use GEO-KOMPSAT-2A (GK2A), the latest geostationary satellite data (2 km and 10 minutes resolution). For a quick update of information on the landslide risk area, a hazard map is created based on the frequency ratio (FR). To evaluate the risk of landslides, five contributing factors for landslides are considered which are Enhanced Vegetation Index (EVI), land cover, soil moisture, elevation and slope gradient. They are respectively coupled with the NASA Global Landslide Catalog (GLC) data to calculate the FR, which includes landslide occurrence information from 1915 to 2022. The FR from each factor are combined to determine the final hazard area of landslides. Lastly, alarming area is defined as the high risky area where heavy rain is expected. In this study, the possibility of heavy rain is determined using GK2A L1B data to detect developing or mature clouds to give fast and near real-time information. In addition, it does not only analyze FR values uniformly, but furthermore, for areas where the correlation with factors are unusual, regional characteristics are identified through case analysis and reflected in the algorithm.
IG11-A004
Improvement of GK2A Forest Fire Detection Algorithm
Seoyoung CHAE#+, Yong-Sang CHOI
Ewha Womans University, Korea, South
Wildfire management is becoming more important around the world as disasters by wildfires increase due to climate change. Wildfires cause irreversible ecosystem destruction, loss of life, and property damage. It has been proven in many cases that early detection and rapid response to wildfires can reduce their impact. Detecting wildfires using satellite data has the advantage of being free from time and space constraints and can be cost-effective. Currently, GK2A is providing Level 2 wildfire detection data using its wildfire algorithm. The GK2A algorithm is based on the MODIS wildfire algorithm and contains temperature fluctuations due to the topographic lapse rate. The current algorithm uses the 3.8 µm and 10.5 µm channels for wildfire detection. The 3.8 µm channel is a combination of thermal and solar and has been known to detect high temperatures since the early days of satellite detection. However, the combination of the two sources inevitably leads to contamination from the larger energy source which is solar. If the other IR channels of GK2A can effectively observe surface temperature changes, it is reasonable to use other channels. In this study, we propose a more accurate algorithm for wildfire detection using channels other than the 3.8 µm channel. Using the Radiative Transfer Model to model brightness temperature changes caused by wildfires to found the reasons why 3.8 µm is difficult to use and the wildfire detection strengths of other channels. Based on the model results, improved the GK2A wildfire detection algorithm, and compared the GK2A algorithm and the renewal algorithm about the 2022 wildfire case.
IG11-A008
Independent Validation of Deep-learning-based Rainfall Induced Shallow Landslides Forecasting in Italy
Alessandro MONDINI1#, Massimo MELILLO1+, Fausto GUZZETTI1, Michele CALVELLO2, Gaetano PECORARO2
1National Research Council, Italy, 2University of Salerno, Italy
Geographical landslide early warning systems are difficult to evaluate. In this work, we assess the performance of a recently proposed deep-learning-based system for short-term forecasting of rainfall-induced shallow landslides in Italy. For our assessment, we use rainfall measurements from the same rain gauge network used to construct the forecasting system, and different and independent information on the timing and location of 163 rainfall-induced landslides that occurred in Italy in a period non covered by the data used to train the forecasting system. The new dataset is extracted from the FraneItalia catalogue (https://zenodo.org/records/7923683). Results confirm the good predictive performance of the forecasting system and reveal no geographical or temporal bias in the forecasts. The analysis shows that the forecasting system is effective at predicting multiple landslides in the same general area. Analysis of the false negatives shows that approximately one-third of the landslides were rockfalls, and for approximately another third there was uncertainty in the database about when or where landslides have occurred. We confirm that the deep-learning-based system analysed is well suited for short-term operational forecasting of rainfall-induced shallow landslides in Italy.
IG12-A007
Temporal and Spatial Studies Over a Scour Hole Downstream of a Grade‐control Structure
Tung Hsuan TSAI#+, Dong-Sin SHIH
National Yang Ming Chiao Tung University, Taiwan
In recent years, climate change has affected Taiwan, resulting in an increasing trend in rainfall intensity and frequency. The occurrence of intense rainfall events significantly impacts the erosion and accumulation of riverbeds. The erosion of these sediments can, in turn, cause damage to the foundations of in-river structures, thereby affecting the safety of these structures. Therefore, installing protective measures on the in-river structures is crucial to monitoring erosion. Common grade‐control structures are usually made of square or rectangular cement blocks. Hence, this study aims to utilize the different shapes of protection works to discuss their effects on downstream erosions. Laboratory flume experiments are conducted to study the impacts of scouring hold subjected to water flow. Moreover, the triaxial accelerometers are used to record vibration acceleration data of the protective structures. Vibration frequencies were obtained through the Fourier transformation of the acceleration data. Simultaneously, downstream erosion depth is recorded hourly using cameras, and Particle Image Velocimetry (PIV) was employed to calculate flow velocity and variations in the flow field within the scour hole. Theoretically, downstream erosion can decrease the foundation's bearing capacity, reducing structural stability and alterations in the overall structural vibration frequencies. This study explores the relationship between erosion depth and frequency under different flow rates and velocities as water flows over grade-control structures with different shapes.
IG12-A012
A Preliminary Study to Investigate the Relationship Between Urban Green Space and Mental Health
Jiyoon MOON#+, Kwangjae LEE
Korea Aerospace Research Institute, Korea, South
As the problem of urbanization intensifies around the world, the issue of human quality of life is also increasing. In particular, as part of improving the quality of life of urban residents, interest in urban green areas has steadily increased in the past, and there are studies showing that urban green areas provide various utility and functions to humans, thereby helping to improve physical and mental health. In this study, we tried to qualitatively investigate the relationship between urban green areas and human mental health, and the study area was targeted at Seoul, the capital of South Korea. NDVI acquired with Landsat 8 images was used to determine the distribution of urban green areas, and the number of depressive patients among mental diseases were used together to analyze the relationship between urban green space and mental health. As a result of the study, NDVI and depression were derived as Pearson correlation -0.084, and the probability of significance was 0.689. Kendall and Spearman's correlation coefficients were -0.040 and -0.064, and the probabilities of significance were 0.779 and 0.762, respectively. The results of this study did not show a high probability of significance of more than 95%, but recorded a correlation of about 70% or more, and it was confirmed that there was a negative correlation. Through this, it was confirmed that the higher the NDVI index, which means the more green spaces and the higher the vitality, the less patients with depression. In the future, it is necessary to continue to conduct related research to examine the relationship with depression as well as other mental diseases, and these findings are expected to be used as basic data for planning or expanding urban green areas in consideration of the number of patients with various diseases.
IG12-A015
Analysis of Urban Heat Island Through MODIS Land Surface Temperature Downscaling in Daegu Metropolitan City, Republic of Korea
Youngseok KIM#+, Siwoo LEE, Dongjin CHO, Jungho IM
Ulsan National Institute of Science and Technology, Korea, South
Investigating the spatiotemporal patterns of urban heat island (UHI) plays a crucial role in understanding urban thermal environments and in developing sustainable cities. Moderate Resolution Imaging Spectroradiometer (MODIS), offering land surface temperature (LST) with frequent revisits (i.e., four times a day) over global, has been widely used in urban climate studies. However, the coarse spatial resolution of MODIS LST (1 km) presents challenges in capturing detailed thermal distributions across heterogeneous urban areas. So, this study conducted the spatial downscaling of MODIS 1 km LST to 250 m and explored the spatiotemporal patterns of surface UHI (SUHI) by administrative district-level (dong) in Daegu, South Korea for the three years 2018, 2021, and 2023. For spatial downscaling, a kernel-driven method was used to combine the MODIS LST with several auxiliary variables related to the LST. Random forest (RF) and convolutional neural network (CNN) were utilized to build spatial downscaling models. To validate the downscaling performance, we aggregated the downscaled LSTs to 1 km and evaluated the aggregated 1 km LSTs with original 1 km MODIS LSTs. RF showed the superior performance than CNN showing a coefficient of determination of 0.86 with a root mean square error of 0.75 °C. As results of spatiotemporal patterns using SUHI intensity (SUHII) extracted from RF, Goseong-dong, Yucheon-dong, and Wondae-dong showed significant variations in SUHII over the study periods with -1.44 °C, -1.41 °C, and -1.38 °C, respectively. The SUHII was high in the order of summer, spring, autumn and winter all years. During spring, summer, and autumn, higher SUHII was observed during the daytime compared to nighttime, while the opposite pattern was evident during winter. These findings on spatiotemporal variation of SUHII can help understand patterns of UHI and formulate policies for UHI mitigation by administrative district-level in Daegu city.
IG12-A016
Hydrogeological Structure Identification Using the Transient Electromagnetic Method in the Northern Area of Choushui River Alluvial Fan, Central Taiwan
Agung Nugroho RAMADHAN+, Ping-Yu CHANG#, Jordi Mahardika PUNTU, Jun-Ru ZENG, Lingerew Nebere KASSIE
National Central University, Taiwan
This study aims to identify the hydrogeological structure in the northern area of the Choshui River Alluvial Fan, Changhua County, Central Taiwan, by using the Transient Electromagnetic (TEM) method. It is necessary to conduct this study since hydrogeological structure information is crucial for several reasons, such as groundwater exploration, groundwater management, land subsidence prevention, water supply planning, and environmental impact assessment. We deployed 54 TEM measurement sites to cover the Changhua area, using the FASTSNAP system with a 50 × 50 m transmitter loop configuration. Subsequently, the TEM data were analyzed based on available geological condition information and other geophysical measurements, such as existing borehole data and Vertical Electrical Sounding (VES) conducted previously. The results reveal that the eastern area near the Bagua Tableland mostly consists of a gravel layer, while the western area near the coast mostly consists of a clay layer. Overall, this study provides new insights into how to identify hydrogeological structure using the Transient Electromagnetic (TEM) approach.
IG12-A018
Investigation of Permafrost by Using Electrical Resistivity Imaging and Ground Penetrating Radar: A Case Study in Svalbard, Norway
Yin-Long CHEN+, Ping-Yu CHANG#, Jordi Mahardika PUNTU, Ding-Jiun LIN
National Central University, Taiwan
Over the years, climate change has significantly impacted the global ecological environment, with the polar regions being among the first to experience changes. Not only the environment above the surface has been affected, but also the subsurface. This study aims to characterize and find the interaction between the permafrost and active layer, by implementing Electrical Resistivity Imaging (ERI), and Ground Penetrating Radar (GPR). Along with the Nicolaus Copernicus University team, this study is eager to learn about this phenomenon in the Svalbard Archipelago, Norway. We collected the data by employing a Wenner array configuration using 40 electrodes with 1m spacing for the ERI, and a 100 MHz antenna frequency for the GPR. The profiling line is about 140 meters from the station and extends forward to the coast. The data were collected in 2022 and 2023, in order to observe the variation and behavior of the subsurface. Furthermore, the ERI and GPR results were integrated with groundwater level and temperature distribution data to enhance the result. Thus, a comprehensive understanding of the subsurface changes due to climate changes can be obtained. In summary, our geophysical approaches have proven to be a powerful tool for this purpose.
IG12-A022
Seismic Anisotropy of the Crust and Upper Mantle Beneath Rifts in Southern Tibet
Changhui JU#+
China Earthquake Administration, China
There are several large-scale N-S trending rift systems in southern Tibet, nearly perpendicular to the Indus-Yarlung Tsangpo Suture (IYS). Served as a focal point for Late Cenozoic magmatic activity, large to super-large metallic ore deposits have developed in southern Tibet and the formation of these deposits is closely related to the evolution of rift zones. We calculate the shear wave splitting parameters (Fast Polarization Direction and Delay Time, abbreviated as FPD and DT) by minimum energy method. North of the IYS, the predominant anisotropy is oriented from NNE to NE directions. South of the IYS, the distribution of anisotropy parameters is more complex, featuring various directions and intensity of anisotropy, and can be bounded in 87°E. In the west of NTR, subparallel to the seismic anisotropy to the north of IYS, NE oriented FPDs were observed, and can be interpreted as a coherent lithospheric deformation. Between NTR and XDR, subparallel to the strike of the orogen, E-W directed FPDs were calculated, with relatively small DTs. One possible explanation is the mantle convection caused by the sub-vertical subducting Indian lithosphere. In the east of NTR, orthogonal to the APM direction, NNW trending FPDs were obtained and can be attributed to the lithospheric deformation soured from the compressional deformation in the collisional front of the Himalayas.
IG12-A024
Monitoring Horizontal Mean Ocean Currents Under Typhoon Conditions Using Optical-fiber Distributed Acoustic Sensing
Sunke FANG+, Jianmin LIN#
Zhejiang University, China
The emerging distributed acoustic sensing (DAS) technology provides a potential way to monitor the sea state with pre-existing submarine optical-fiber (OF) cables, even in severe weather situations. Here, we present in situ observations of the microseismic noise during the passage of severe typhoon Muifa (2022), using a ~17 km DAS-instrumented OF cable located offshore from Daishan Island in the Zhoushan Archipelago, eastern China. The microseismic noise induced by ocean surface gravity waves (OSGWs) is mainly in the ~0.08 to 0.38 Hz frequency band. And the high-frequency (>0.3 Hz) component is tide-modulated and only observed during low-tide periods in areas of shallow water (<10 m). The noise component around 0.20 Hz at relatively deeper cable channels is observed strongly related to the sea-surface winds at the nearby ocean buoy (with a correlation coefficient of ~0.89), as well as the typhoon track. Furthermore, the OSGW propagation along the entire cable is estimated via frequency-wavenumber analysis and found to be significantly reversed during the typhoon passage, consistent with the observed sea-surface winds. Additionally, we propose a simple and effective method to estimate both the speeds and directions of horizontal mean ocean currents. It is based on the current-induced Doppler shifts of DAS-recorded OSGW dispersions. The measured currents are consistent with the tide-induced sea-level fluctuations and sea-surface winds. These observations demonstrate the potential feasibility of monitoring sea states under typhoon conditions using DAS-instrumented cables.
IG12-A025
Hydrous Mantle Transition Zone in the Western Himalayan Syntaxis
Guohui LI1#+, Yuanze ZHOU2, Yuan GAO1
1China Earthquake Administration, China, 2University of Chinese Academy of Sciences, China
Water in the Earth’s interior can significantly reduce mantle viscosity and melting temperature of rocks, which plays a very important role in the Earth's dynamic and chemical evolution, and habitability. Here, we image the P- and SH-wave velocities of the mantle transition zone by matching synthetic and observed triplicated seismic waveforms in the western Himalayan syntaxis. With respect to the IASP91 model, the depth of the 660 km discontinuity descends by 19~29 km. The P-wave velocity of mantle transition zone is normal, but the SH-wave velocity reduces a lot. These observations indicate that the mantle transition zone is rich in water. In addition, the existence of a partially melted low-velocity layer atop the mantle transition zone also suggests a water-rich mantle transition zone.
IG16-A003
Assessing Snowmelt and Forest Expansion in the Himalayan Region: Climate and Vegetation Dynamics
Jyoti SHARMA#+, Disha SACHAN, Aaquib JAVED, Pankaj KUMAR
Indian Institute of Science Education and Research Bhopal, India
Within the world's mountainous regions, Asia boasts the largest and most populous mountain system - the Himalayas. This distinctive terrain showcases a blend of glaciers and diverse vegetation, with the former crucially feeding perennial rivers in neighboring nations and the latter offering a spectrum of ecosystem services pivotal for supporting the livelihoods of local communities. It is endowed with an overwhelming richness of biodiversity, recognized among 36 global biodiversity hotspots. Since climate change is expected to bring alterations to all ecosystems, including those in the mountains, past studies have suggested higher vulnerability of the Himalayas to climate change, as warming in this region is greater than the global average rate. Consequently, most glaciers in the Himalayas are experiencing mass loss through melting and calving. This alteration in the availability of land surface water and the exposure of bare soil due to warming scenarios could potentially drive forest expansion. Such transformation from snow-covered areas to forests, including shifts in snowline altitude and treeline, might influence changes in surface energy fluxes by altering snow-albedo and triggering various vegetation feedback. However, the key factors steering vegetation change and the resulting impact on cooling or warming trends remain inadequately understood in the Himalayan region. The present study focuses on comprehending the patterns of snowmelt and forest expansion in the Himalayan region over the past two decades using satellite (MODIS) and re-analysis (ERA-5) datasets. Furthermore, the research aims to delve into the contribution of climatic and soil-related factors to the expansion of forests in the Himalayas. Preliminary results witnessed the greening trend in Sub-Tropical, Montane Temperate and Sub-Alpine Forests except Montane Wet Temperate Forest in the Himalayan region. Detailed findings will be discussed during the presentation.
IG16-A004
Characteristics of Western Disturbances Impacting Karakoram-Himalayan Region
Aaquib JAVED#, Pankaj KUMAR+
Indian Institute of Science Education and Research Bhopal, India
Extreme precipitation over the Himalayas is largely influenced by Western disturbances (WDs). In recent decades, there has been a notable strengthening of WD impact over the Karakoram (KR) region, playing a pivotal role in sustaining the “Karakoram Anomaly.” Utilizing the WD catalog derived from ERA5 and MERRA2 reanalysis datasets, our study reveals a statistically significant shift of approximately 9.7 degrees eastward in the core genesis zone for KR WDs. This shift indicates a migration towards more favorable conditions for cyclogenesis. We propose a novel parameter for identifying regions conducive to extratropical cyclogenesis. The observed shift in the core genesis is linked to increased genesis potential, convergence, and higher moisture availability along the WD path. Composite analysis further demonstrates a significant increase in moisture availability over the shifted zone. These findings underscore the crucial synoptic influence on the anomalous regional mass-balance phenomenon in the KR region.
IG16-A007
New Permafrost Maps in the Northern Hemisphere
Youhua RAN#+, Xin LI, Guodong CHENG
Chinese Academy of Sciences, China
Monitoring the thermal state of permafrost is important in many environmental science and engineering applications. However, such data are generally unavailable, mainly due to the lack of ground observations and the uncertainty of traditional physical models. This study produces novel permafrost datasets for the Northern Hemisphere (NH), including predictions of the mean annual ground temperature (MAGT) at the depth of zero annual amplitude (approximately 3 m to 25 m) and active layer thickness (ALT) with 1-km resolution for the period of 2000–2016, as well as estimates of the probability of permafrost occurrence and permafrost zonation based on hydrothermal conditions. These datasets integrate unprecedentedly large amounts of field data (1,002 boreholes for MAGT and 452 sites for ALT) and multisource geospatial data, especially remote sensing data, using statistical learning modelling with an ensemble strategy. Thus, the resulting data are more accurate than those of previous circumpolar maps. The datasets suggest that the areal extent of permafrost (MAGT≤0 °C) in the NH, excluding glaciers and lakes, is approximately 14.77 (13.60–18.97) millions km2 and that the areal extent of permafrost regions (permafrost probability>0) is approximately 19.82 millions km2. A biophysical permafrost zonation and hydrothermal condition-based permafrost zonation were also proposed. These new datasets based on the most comprehensive field data to date contribute to an updated understanding of the thermal state and zonation of permafrost in the NH. The datasets are potentially useful for various fields, such as climatology, hydrology, ecology, agriculture, public health, and engineering planning. All of the datasets are published through the National Tibetan Plateau Data Center, and the link is https://doi.org/10.11888/Geocry.tpdc.271190.
IG16-A014
Mapping the Temporal Evolution of Glaciers in Uttarakashi, Central Himalayas Using High Resolution Satellite Imagery
Iti SHRIVAS1+, Supratim GUHA2, Reet Kamal TIWARI1#, Ashutosh Laxman TARAL1
1Indian Institute of Technology Ropar, India, 2Korea Polar Research Institute, Korea, South
Glaciers are crucial indicators of climate change and hold immense importance in sustaining freshwater resources essential for various ecosystems and human societies. The present study focuses on identifying temporal changes in glaciers with respect to area from 2000 to 2023 for a sample of 19 glaciers in the Uttarkashi region of Uttarakhand in the Central Himalayas, India. The study utilizes data from Landsat 5 (TM), Landsat 7 (ETM+), and Landsat 8 (OLI) with 30 meters of spatial resolution and the PlanetScope satellite constellation with a high resolution of 3 meters to digitize glacier boundaries. The results underscore a reduction in glacier area by 2.89% throughout the study period. Significant variations in this trend are determined, with Glacier G1 exhibiting the highest reduction rate at 0.8831% y-1, while Glaciers G6 and G8 display negligible changes. Friedman test implies an identical rate of area change in different time intervals. The 95% confidence intervals, ranging from 0.0957% to 0.3233% % y-1 (2000-2011), 0.1757% to 0.5063 % y-1 (2011-2017), and 0.2060% to 0.6857% y-1 (2017-2023), further contribute to the understanding of the evolving dynamics of glacier response to changing climate conditions. Emphasizing the pivotal role of high-resolution satellite imagery in precise mapping and monitoring, this study provides valuable insights into the hydrological implications associated with the noticeable recession of glaciers in the Central Himalayas.
IG21-A004
Monitoring the Ionospheric Signatures of Very Low-frequency Transmitters with Micro-/nano-satellites
Jaeheung PARK1#+, Hosung CHOI2, Magnus IVARSEN3
1Korea Astronomy and Space Science Institute, Korea, South, 2Republic of Korea Army, Korea, South, 3University of Oslo, Norway
As the frequency of electromagnetic waves becomes lower, the signal can penetrate deeper into the sea, while the installation and operation costs get higher. That is why only some countries operate Very-Low-Frequency (VLF) transmitters that can be used to communicate with submersible vehicles. At the same time, during their normal operation, VLF transmitters produce a unintended signature in the ionosphere above. This presentation will give a brief introduction to the effects of VLF transmitter signals on ionospheric cold plasma and energetic particles originating in the magnetosphere. We also show examples of the signatures captured by Low-Earth Orbit (LEO) spacecraft, such as the Swarm constellation of the European Space Agency (ESA) and the Korean NextSat-1. Finally, we discuss the possible contribution to the topic of the recently launched Korean CubeSat fleet, SNIPE.
IG21-A007
Total Ionizing Dose and Displacement Damage Dose Effects on On-board Computer Candidate for a Super Low Earth Orbit Optical Satellite
Jongdae SOHN1#+, Junga HWANG1, Hojin LEE1, Jaeyoung KWAK1,2, Hyosang YOON3
1Korea Astronomy and Space Science Institute, Korea, South, 2Korea National University of Science and Technology, Korea, South, 3Korea Advanced Institute of Science and Technology, Korea, South
At this time, we present the effects of total ionizing dose and displacement damage on On-Board Computer (OBC) candidates for Super Low Earth Orbit (SLEO) optical satellite. The Optical Satellite aims to operate for more than two years with the mission of taking high-resolution images with a resolution of 50 cm at an altitude of 300 km or less and. This satellite is a small Earth observation satellite weighing about 100 kg, suitable for super low earth orbit. Modules tested include the Arduino modules such as MKR1010, YUN, UNO, PICO, DUE, and NANO, and the Raspberry Pi modules such as Zero W, 4B, 3+ compute Lite, 3+ compute, 3 compute, and 4 compute. The modules' displacement damage dose and total ionizing dose performance were studied using 100 MeV protons, 10 MeV electrons, and 60 Co irradiation. We performed Total Ionizing Dose (TID) and Displacement Damage (DD) experiments on Arduino modules and Raspberry Pi modules to select OBC candidates for ultra-low altitude optical satellites.
IG21-A015
Lessons Learned from PEARL-1H CubeSat Operation for Power Consumption and Management
Wei-Rong HUANG#+, Mei-Hua HSU, Chi-Kuang CHAO, Yun-Ru CHEN
National Central University, Taiwan
PEARL-1H (Propagation Experiment using kurz-Above-band radio in Low earth orbit) CubeSats integrated by National Central University (NCU) and Hon Hai Precision Industry Co., Ltd. (Foxconn) for educational training/scientific research was launched into a sun-synchronous orbit at 520 km altitude around 1030 local time sector by SpaceX Transporter-9 rideshare mission from Vandenberg Space Force Base on 11 November 2023. A Communication PayLoad (CPL) developed by Tron Future was installed on PEARL-1H for broadband communication experiment with beam-steering phase array antenna. PEARL-1H is a dual-EPS CubeSat designed to support CPL, requiring high-voltage power for its operation. There are two power distribution modules and two battery packs in PEARL-1H. Except for the battery raw power, all power sources providing the same voltage are shared and each BP is managed individually through each PDM. In this study, expected system operation under such a system is discussed along with a discussion of on-orbit data.
IG21-A016
Lessons Learned from PEARL-1C CubeSat Operation During ADCS Commissioning Phase
Mei-Hua HSU#+, Chi-Kuang CHAO, Wei-Rong HUANG, Yun-Ru CHEN
National Central University, Taiwan
PEARL-1C, a 6U XL CubeSat developed by National Central University (NCU) for educational training and scientific research, was successfully launched into a sun-synchronous orbit at an altitude of 520 km around 1030 local time sector by SpaceX Transporter-9 rideshare mission from Vandenberg Space Force Base on 11 November 2023. Onboard PEARL-1C, two payloads were included: a Ka-band communication payload (KCP) developed by Rapidtek Technologies and NCU for a broadband communication experiment, and a Compact Ionospheric Probe (CIP) developed by NCU for ionospheric plasma measurement. Prior to entering the normal operation phase, commissioning phases were conducted to assess the condition of each system. The Attitude Determination and Control System (ADCS) played a crucial role in controlling the satellite's attitude to achieve the required pointing for the payloads. During the ADCS commissioning phase, a sequential activation and checkout of sensors and actuators took place to ensure that the control operations would perform as expected. This poster aims to present the lessons learned from the PEARL-1C CubeSat operation during the ADCS commissioning phase.
IG21-A019
The 2nd-generation Compact Ionospheric Probe on CubeSat for Space Weather Mission
Yun-Ru CHEN#+, Chi-Kuang CHAO, Wei-Rong HUANG
National Central University, Taiwan
Compact ionospheric Probe (CIP) is a miniature version of Advanced Ionospheric Probe (AIP), a successful science payload on FORMOSAT-5 satellite to operate for more than 6 years for global ionospheric space weather and distributions of plasma density irregularities occurrence rates at low latitudes, developed by National Central University (NCU). It is an all-in-one in-situ ion sensor, which can measure ion concentrations, velocity, and temperature to monitor ionospheric space weather conditions to detect potential disruptions in space communication and navigation systems. The 2nd-generation CIP occupied 0.8U form vector, 776g of mass, and 3.5W of power consumption. Like its predecessor, the 1st-generation CIP, it has a capability to operate as a standalone payload or installed in a sensor package with multiple roles (a Retarding Potential Analyzer, an Ion Drift Meter, an Ion Trap, etc.), and sampling rates (128 Hz and 1,024 Hz). It is a slight increase in both weight and size to its predecessor, but improves its heat dissipation issues with its aluminum alloy shell, and adds an RS-485 communication interface to enhance compatibility with most commercial Cubesat. The 1st-generation CIP has been launched with IDEASSat (2021), INSPIRESat-1 (2022), and ARCADE (2023) missions. The 2nd-generation CIP had a maiden flight on Pearl-1C (2023) in a 520 km sun-synchronous orbit in the 1030 local time sector by SpaceX. In the future, NCU will deliver three 2nd-CIPs for ELITE (anticipating a very low earth equatorial orbit in 2025), PEAL-1A and 1B (500 km sun-synchronous orbit in 2025Q4), etc. It is welcome for space scientists to consider using CIPs for their upcoming space weather mission.
IG21-A021
Lessons Learned from SPATIUM-II Technology Demonstration Mission for Ionospheric TEC Measurements
Makiko KISHIMOTO1#, Necmi Cihan ORGER1+, Tharindu DAYARTHNA2, Meng CHO1, Hoda A. ELMEGHARBEL3, Chee Lap CHOW4, Li King Ho HOLDEN4, Man Siu TSE4
1Kyushu Institute of Technology, Japan, 2Arthur C Clarke Institute for Modern Technologies, Sri Lanka, 3Misr International University, Egypt, 4Nanyang Technological University, Singapore
KITSUNE/SPATIUM-II was developed as a dual satellite system in the same structure, and both systems were operated in low-Earth orbit for approximately a year between March 2022 and March 2023. SPATIUM-II is the second mission of SPATIUM program, and it was developed in collaboration between Kyushu Institute of Technology and Nanyang Technological University. SPATIUM program utilizes chip-scale atomic clock onboard while aiming to perform 3D ionosphere mapping, and there are several capabilities to demonstrate prior to scientific-level TEC measurements. SPATIUM-II payload received spread spectrum BPSK signal at 450 MHz transmitted from the ground station, and it was demodulated and processed onboard to detect propagation time delay between the ground station and the satellite. In addition, it used chip-scale atomic clock for the receiver software-defined radio clock source, and 1-PPS from onboard GPS receiver is used for time synchronization between the ground systems and the satellite receiver. In this study, lessons learned from TEC technology demonstration mission will be discussed based on on-orbit results together with how to improve the mission to measure ionospheric TEC with a small satellite.
IG22-A008
Process of High School Students' Data Interpretation in Earthquake Education Program
Chaeeun YOON#+
Ewha Womans University, Korea, South
In this study, we developed a scientific inquiry education program using earthquake big data for high school students, and understand the characteristics of each stage in the integrated inquiry process. Big data is one of the core information technologies of the future society, and the 2022 revised curriculum in Korea also emphasizes it as part of digital education. The activity of presenting data in the form of tables or graphs and interpreting their meaning is closely related to the data interpretation skill, which is the major inquiry in earth science education. The big data used in the program is landslide data caused by earthquakes around the world provided by the United States Geological Survey, and includes a total of 12 variables including region, date, size, fault type, and number of casualties. The educational program was conducted for 120 minutes for 37 first and second year high school students in Seoul, Korea. Using actual big data, students experienced a total of six stages of research: making research questions, developing hypotheses, selecting variables, transforming data, interpreting data, and drawing conclusions. In the ‘transforming data’ stage, the CODAP (Common Online Data Analysis Platform) program, a platform that allows students to easily process data, was used. The data used in the study were graphs and inquiry journals written by students. The characteristics of high school students' inquiry stages were analyzed focusing on the data interpretation process.
IG22-A012
Elementary and Middle School Students’ Learning Characteristics in Polar Education Program : Focusing on the Framework of the Polar-relatedness
Soyoung MUN#+
Ewha Womans University, Korea, South
The purpose of the study is to identify the characteristics of students by applying the polar-Relatedness analysis criteria developed to reduce students' psychological distancing toward the poles, and to provide implications for polar education in terms of science education. Polar, one of the unexplored areas on Earth, is an important object in the development of modern science and is a emerging research topic. They are highly valued for their research due to their geographical and climatic characteristics. However, it was noted that the general public still does not know about the poles and feels psychological distance. Accordingly, it is necessary to strategically develop a polar education program that eliminates obstacles that cause psychologically distant feeling, identify the characteristics that appear therein, and derive educational implications. In the analysis by subject, stage, and student, students showed different patterns. First, as a result of the subject analysis, it was the biology topic that increased interest in the poles. Next, results of the step-by-step analysis, it was found that the main class stage in narrowing the psychological distance to the pole was the ‘Local’ stage, which became a leap point to approach the personal range from the global range. Finally, results of each student's analysis, after the application of the polar education program, the cognitive aspect of ‘perspective’ was relatively poorly revealed, and it was found that it is a key factor to have a new perspective on the polar and various perspectives on the polar to narrow the psychological distance to the polar. This study is meaningful in that it drew attention to the subject of polar, which had not been noted in science education, and led to class contents. In addition, it is meaningful to develop teaching and learning methods that fit the characteristics of polar regions that are far away.
IG27-A023
Development of Maritime Issues Detection Technology and Service System Based on a Second Geostationary Ocean Color Imager (GOCI-II)
Hee-Jeong HAN1+, Kwang Seok KIM1, Ki-Beom AHN2, Suk YOON1, Hyun YANG3, Young-Je PARK1#
1Korea Institute of Ocean Science & Technology, Korea, South, 2Sirius K, Korea, South, 3Korea Maritime & Ocean University, Korea, South
The Korean geostationary ocean color satellite, GOCI-II, is a valuable tool for monitoring the waters surrounding the Korean Peninsula. With its ability to provide 12-band datasets at a spatial resolution of 250 meters, it is ideal for observing marine phenomena. The high temporal resolution of GOCI-II also ensures stable observational performance, making it an effective tool for detecting maritime issues such as red tide, brown tide (Sargassum horneri), sea ice, and chlorophyll bloom. By utilizing GOCI-II data, a maritime issue monitoring service system has been developed and compared with field or satellite data from 2022 to 2023. Through the customization of the system to meet the practical needs of the industry and the application of AI technology, a highly effective system can be established to respond to maritime issues.
IG27-A024
Accurate Estimation of Forest Phenology with Snow-free Vegetation Index Derived from Himawari/AHI: An Application of Third Generation Satellites for Ecosystem Monitoring
Taiga SASAGAWA1#+, Wei LI1, Yuhei YAMAMOTO1, Kazuhito ICHII1, Kenlo NASAHARA2
1Chiba University, Japan, 2University of Tsukuba, Japan
Vegetation phenology plays a vital role in terrestrial ecosystems, and many researchers have tried to estimate the start of the season (SOS) and end of the season (EOS) with vegetation indices, such as NDVI and EVI, derived from satellite data. However, these vegetation indices are strongly affected by the changes in the background, especially snow melting, and it causes significant noises for SOS and EOS estimation. Currently, a new snow-free vegetation index named NDGI has been developed, and it showed better performance for the estimation of SOS and EOS with MODIS data. Furthermore, some research showed that hypertemporal datasets derived from geostationary satellites enable more accurate estimation of vegetation phenology than polar orbit satellites, such as MODIS. Therefore, in this study, we aimed to combine the geostationary satellite dataset and NDGI for accurate SOS and EOS estimation of deciduous forests around East Asia. We calculated NDGI from our land surface reflectance dataset of Himawari/AHI and conducted curve-fitting against the time series of NDGI. Then, we estimate SOS and EOS and validate them with an in-situ observation dataset provided by the Phenological Eyes Network (PEN) in some sites. Our results show that the Himawari/AHI and NDGI combination more accurately estimated SOS and EOS than previous methods. It anticipates that the combination of geostationary satellite and NDGI can be an effective way for monitoring phenology, and we can apply this method to other geostationary satellites, such as GeoKompsat-2A/AMI, MTG-I/FCI.
IG27-A025
GeoNEXtool: A Tool of GeoNEX Geostationary Satellite Data for Carbon and Water Flux Modeling at Fluxnet Sites
Hirofumi HASHIMOTO1#+, Weile WANG2, Taejin PARK2, Andrew MICHAELIS2, Ian BROSNAN2
1California State University Monterey Bay, United States, 2NASA Ames Research Center, United States
We introduce GeoNEXtool to the science communities who uses the geostationary satellite data and Fluxnet data to analyze hourly vegetation response to the climate in the continental scale. The importance of the new generation geostationary satellite has been well recognized for the Fluxnet users because only the geostationary satellites can monitor the vegetation in such a high frequency (10 minutes frequency for full disk images). However, the number of research using the geostationary satellite data for ecosystem modeling is still small. One of the biggest reasons of this poor usage of the data is that the volume of the geostationary satellite data is too large for most of the scientists. We, NEX (NASA Earth Exchange) group, are generating the GeoNEX TOA (L1G dataset) and surface (L2 dataset) reflectance dataset in the geographic projection from the geostationary satellite data. To promote the data to the Fluxnet community, we created the GeoNEX subset datasets for each fixed network site, and developed the GeoNEXtool to make it easy to process the subset dataset in the same way the MODIStool can handle MODIS subset dataset. The selection of network sites and file formats of GeoNEX subset are same with MODIS subset dataset. The subset data includes the timeseries of 9x9 1-km pixel data around the sites. Using GeoNEXtool, we demonstrated simple usage of the GeoNEX subset data with Ameriflux subset data. The estimated GPP using GeoNEX subset data were compared with the GPP at Ameriflux sites. The GeoNEXtool and GeoNEX subset data can contribute to the research of the Fluxnet community by facilitating the use of the geostationary satellite data.
IG30-A002
Evaluation of the Potential of Using Machine Learning, the Moving Average and the Savitzky–Golay Filter to Simulate the Daily Soil Temperature in Gully Regions of the Chinese Loess Plateau
Dengfeng LIU1#+, Wei DENG1, Fengnian GUO1, Lan MA1, Qiang HUANG1, Qiang LI2, Guanghui MING3
1Xi'an University of Technology, China, 2Northwest A&F University, China, 3Yellow River Engineering Consulting Co., Ltd., China
Soil temperature is an important variable in earth science research. Machine learning provides a new approach to simulating soil temperatures to compare the land surface’s energy balance with traditional simulations of physical processes. The long short-term memory (LSTM) was used to explore its potential in simulations of soil temperature at five soil depths, and the simulated soil temperature was postprocessed by the moving average (MA) and the Savitzky–Golay filter (SG). The models were forced by various combinations of environmental factors, including daily air temperature (Tair), daily net radiation (Rn), daily shortwave radiation (Rs) and the soil temperature (Ts) of the upper layer, which were observed in the Hejiashan watershed on the Loess Plateau in China. The optimal combination of input was identified as Ts-last+Tair+Rn+Rs and this served as input to the model. The other three models, (i.e., multiple linear regression (MLR), multilayer perceptron (MLP) and bidirectional long short-term memory (Bi-LSTM)) were also applied to simulate the daily soil temperatures at the five depths to compare these with the results of LSTM and LSTM-MA-SG. The simulated results were evaluated by the coefficient of determination (R2), the mean absolute error (MAE), the root mean square error (RMSE) and the Kling–Gupta efficiency coefficient (KGE). The results showed that the performance of LSTM-MA-SG in simulating Ts was better than the other four models. The evaluation of the results of LSTM-MA-SG showed that the range of R2 at different depths was 0.993-0.999, the range of MAE was 0.104-0.387 °C, the range of RMSE was 0.132-0.498 °C, and the range of KGE was 0.982-0.991. In the simulation of all depths, the performance of LSTM-MA-SG improved compared with LSTM. The study provides a critical reference for simulations of soil temperature.
IG30-A003
Evaluation of Water Balance and Water Use Efficiency with the Development of Water-saving Irrigation in the Yanqi Basin Irrigation District of China
Huan CHENG1+, Dengfeng LIU1#, Guanghui MING2, Fiaz HUSSAIN3, Lan MA1, Qiang HUANG1, Mengxian MENG4
1Xi'an University of Technology, China, 2Yellow River Engineering Consulting Co., Ltd., China, 3PMAS-Arid Agriculture University Rawalpindi, Pakistan, 4China University of Geosciences, China
With the continuous expansion of cultivated areas, there is an increasing demand for irrigation water, resulting in an irrigation efficiency paradox. In this study, the water balance method and the improved IWMI water balance method were used with remote sensing and statistical data from 1980 to 2020 to analyze the changes in the irrigation water supply, consumption, and loss for improvement in irrigation water use efficiency in the Yanqi Basin. The arable land area in the irrigation district increased from 1672 km2 in 1980 to 2494 km2 in 2020. The traditional water use efficiency showed an increasing trend. The lowest value for the field water-use coefficient was exceeded to 0.81 from 2009 to 2020. The canal water-use coefficient was increased from 0.54 in 2009 to 0.82 in 2020. The irrigation water-use coefficient increased from 0.35 in 1998 to 0.68 in 2020, with a general upward trend. The water consumption ratio indicator DFg, determined using the improved water balance method, increased from 0.8390 in1980 to 0.8562 in 2020, and the average was 0.8436. Cultivated land’s actual irrigation water consumption per unit area reached the highest value of 8.41×106 m3/hm2/a in 2011 and the minimum value of 4.01×106 m3/hm2/a in 2020, while the total water diversion showed an increasing trend due to the continuous expansion of arable land. From 1980 to 2020, water diversion into the irrigation district changed from 1.214 km3 to 1.000 km3, and it reached a maximum of 1.593 km3 in 2000; water diversion into the irrigation district showed an overall upward trend. The findings showed an increase in IWUE in the Yanqi Basin irrigation district. These results provide a theoretical basis for breaking the paradox of irrigation efficiency, which can be used in the water resource management of irrigation districts.
IG30-A006
Spatial-temporal Adaptive Planning of Flood Managed Aquifer Recharge Guided by Deep Reinforcement Learning
Meilian LI+, Xiaogang HE#
National University of Singapore, Singapore
Flood-managed aquifer recharge (Flood-MAR) is a crucial yet untapped solution that can simultaneously mitigate flood and drought risks and boost groundwater supply. The key constraint for this multi-benefit adaptation is how much water and land are available for recharge, which requires effective planning from spatial and temporal aspects to repurpose existing agricultural landscapes. However, future evolution of such landscapes is subject to uncertainties in changing human-nature systems, which is further challenged by a warming climate that brings more floods and droughts. Traditional spatial planning approaches often assume perfect future predictions and rely on static policies, which cannot well adapt to dynamic and uncertain environments. While some studies have adopted artificial intelligence to facilitate urban planning and conservation planning, most of them do not consider the synergistic benefits of multi-sector planning across time and space. To address these limitations, we propose a multi-objective spatially explicit planning framework leveraging recent advances in deep reinforcement learning (DRL) to develop adaptive policies for joint agriculture and water management, with a focus on Flood-MAR. DRL Agents dynamically allocate lands for different Flood-MAR related actions (e.g., land retirement, on-farm-based, or wetland-based recharge) over time. The environment in DRL responds to these actions through changes in land use and groundwater storage. Rewards in DRL are designed based on agricultural revenues, action costs, and penalties for not meeting groundwater targets. To tackle the challenge of the vast solution space, we use the proximal policy optimization algorithm to train a policy network to estimate pixel-level action probabilities and a value network to evaluate the current policy. Through a case study in California’s San Joaquin Valley, this study underscores the potential of Flood-MAR to mitigate flood and drought risks in uncertain environments and the efficacy of DRL in guiding adaptive Flood-MAR policies.
IG30-A009
Assessment of Groundwater Contamination with PFAS and Possible Remedial Measures
Harish BHANDARY#+, Adnan AKBAR, Chidambaram SABARITHINAM, Yogeesha JAYARAMU
Kuwait Institute for Scientific Research, Kuwait
Per and Ployfluoroalkyl substances (PFAS) are class of chemicals belonging to a group of emerging contaminants (ECs), previously thought to be of little significance only to be discovered recently that they can adversely affect aquatic ecosystems and human health. Being the only source of natural freshwater, groundwater is of strategic importance for Kuwait. The new discoveries of different emerging contaminants have given rise to the notion that this resource has been contaminated by these pollutants, especially by the PFAS which are linked to oil field activities and firefighting foams that were used to combat the fire blazes in the immediate aftermath of the 1991 Gulf War. This study is aimed at evaluating the levels of contamination by PFAS of the fresh groundwater fields in Kuwait and recommending possible remediation measures. This paper presents the initial activities and results of the study to evaluate PFAS contamination of fresh groundwater. The study involved collection and analyses of groundwater samples from Al-Raudhatain and Umm Al-Aish fresh groundwater fields to determine the PFAS levels in them. The collected samples were analyzed for PFAS using standard USEPA method No. 8327 using liquid chromatography/tandem mass spectrometry (LC-MS/MS). Initial results indicate the contamination of groundwater with PFAS. Preliminary data of this ongoing study and future plans is discussed in this paper. This research will employ GIS and statistical tools to map pollutant distribution, identifying potential sources. Various treatment techniques, including granular activated carbon, ion exchange, and nanofiltration, will be explored for their efficacy in PFAS removal within a pump-and-treat system. The collected data and information will be assembled to evaluate the degree of contamination and effective remedial methods. The study is expected to provide the information necessary for the development of a comprehensive groundwater management and protection plan to address risks associated with such contaminants.
IG30-A010
Semi-analytical Rate-limited Sorption Model for Sequential Degradation Products in Two-dimensional Multispecies Transport Under Arbitrary Time-dependent Inlet Boundary Conditions
Thu-Uyen NGUYEN#+
National Central University, Taiwan
Many semi-analytical and analytical models for multispecies transport traditionally rely on solving coupled advection-dispersion equations (ADEs) in which sorption is commonly assumed to be equilibrium-controlled. Nevertheless, recent demonstrations indicate that more accurate predictions of contaminant transport in groundwater can be achieved by incorporating a rate-limited sorption process instead of relying on an equilibrium sorption assumption. This study is specifically designed to formulate semi-analytical models for the two-dimensional multispecies transport of a chemical mixture, including a parent compound and its degradation-daughter products. This transport is influenced by rate-limited sorption subject to arbitrary time-dependent inlet boundary conditions. The simulation results obtained from our newly developed semi-analytical model closely align with those generated using a numerical model based on the Laplace transform finite difference (LTFD) method, affirming the validity of the new approach. The impact of rate-limited sorption on contaminant plume migration is investigated under various time-dependent inlet boundary conditions. Sorption rate values vary from low to high, specifically 0.05, 0.5, 5, and 50 years⁻¹. The outcomes reveal that the predicted concentrations of all contaminants within the decay chain decrease as the sorption rate constant increases, irrespective of whether the boundary sources are constant or exponentially time-dependent. However, under pulse loading boundary conditions, concentrations of later degradation products tend to increase with the sorption rate constant. The semi-analytical models developed in this study accommodate different inlet boundary conditions, making them versatile tools for simulating the transport of sequentially degrading reaction products.
IG30-A011
The Presence, Ecotoxicological Implications, and Associated Risk Assessment of Organochlorine Pesticides (OCPs) in Rural and Semi-urban Areas of West Bengal, India
Suchitra MITRA#+, Sujata RAY
Indian Institute of Science Education and Research Kolkata, India
Despite the global prohibition of persistent organochlorine pesticides, recent evidence suggests continued usage in India for vector-borne disease eradication programs and agricultural practices. This study assesses the presence, ecotoxicological implications, and associated risks of 20 banned and restricted organochlorine pesticides (OCPs) in the surface water and groundwater of semi-urban (Nadia district) and rural areas (Birbhum district) across the winter, premonsoon, monsoon, and postmonsoon seasons. The OCP concentrations in the collected water samples were observed in the 1.53 to 106.90 ng/L range and were higher in the winter than in other seasons. The detection frequencies of OCPs ranged from 85% to 100% in all seasons, with a few exceptions. The highest mean concentrations were observed for ΣHCHs, ΣEndosulfans, and chlordane during the pre-monsoon and monsoon, except for the absence of chlordane in groundwater during the pre-monsoon season. In the winter season, ΣHCHs concentration in groundwater increased in agricultural areas. In semi-urban areas, OCPs like HCH, endosulfan sulfate, and heptachlor were in higher concentrations in the water. Concentrations of β-HCH, γ-HCH, p,p’-DDD, p,p’-DDT, and ΣEndosulfans in both groundwater and surface water did not significantly differ between pre-monsoon and monsoon seasons, except for elevated concentrations of aldrin and β-HCH in the monsoon season and ΣEndosulfans in the post-monsoon season in groundwater. OCPs like Aldrin, heptachlor, and trans-chlordane were in higher concentrations in the water of rural areas. The study highlights the poor and delayed implementation of the ban on OCPs in India, emphasizing the urgent need for stricter adherence to the National Implementation Plan (NIP) on pesticides to mitigate associated environmental risks.
IG30-A015
Biomonitoring of Heavy Metals in Blood, Urine and Hair of Children (5-18 Years) in Communities of Atoyac Basin, Mexico
Estefania MARTINEZ-TAVERA1#+, Carlos David YEVERINO-MARTINEZ1, S.B. SUJITHA2
1Universidad Popular Autónoma del Estado de Puebla, Mexico, 2Instituto Politécnico Nacional, Mexico
In central Mexico, the Atoyac basin encompasses an active volcano and the second most polluted basin. Henceforth, the study aims to determine the prevalence of heavy metals in the biological matrices of children aged between 5 to 18 whom reside in the Alto Atoyac watershed. Blood, urine, and hair samples were collected from 78 minors in two populations and the concentrations of six heavy metals (As, Cd, Cr, Pb, Hg, and Zn) in all three matrices were determines using a ICP MS. Clinical tests were also done on blood and urine samples to examine the health state of the study population. The findings revealed that nearly 96% of the individuals had at least one parameter in the clinical tests that was above the reference levels. The analysis of heavy metals in blood samples revealed that 100% of participants in both communities had levels that exceeded the reference values for arsenic, cadmium, chromium, and lead, indicating a potential health risk, except for mercury and zinc, where 88% and 98.6%, respectively, had levels that exceeded the reference. In terms of urine samples, HQ index values for arsenic showed no health risk, but chromium and lead values surpassed the reference for 100% of participants in both areas, while cadmium, mercury, and zinc showed a potential danger in 52%, 34%, and 52% of participants, respectively. Arsenic, cadmium, chromium, lead, and zinc levels in hair samples above were above the reference in 86%, 98%, 100%, 17%, and 21% of participants, respectively, whereas mercury posed no health risk in any of the samples. Correlations were found between different heavy metals in the study and their amounts and aberrant clinical indicators, revealing that these pollutants have a negative impact on participant’s; health and that many contaminants coexist in the region.
IG31-A003
Vulnerability to Extreme Heat Risks in Southeast Asia: The Role of Adaptation Finance
Rainbow Yi Hung LAM#+, Laurence DELINA
The Hong Kong University of Science and Technology, Hong Kong SAR
Extreme heat, often referred to as the “silent killer,” can have devastating impacts, particularly in regions like Southeast Asia, where urbanization and population density are on the rise. Vulnerable populations in this world region are at a higher risk of heat-related mortality and illness, as well as reduced efficiency of energy systems. Additionally, limited financial resources hinder cities' adaptation efforts, making finance a key determinant of vulnerability to extreme heat risks. While there is a growing awareness of the importance of financing climate adaptation and mitigation through the SENDAI framework for Disaster Risk Reduction (SFDRR) and the recent Conferences of Parties (COPs) to the United Nations Framework Convention on Climate Change, there is still a lack of holistic understanding of adaptation or disaster risk management efforts for urban extreme heat and a dearth of adaptation finance. This presentation reviews the literature on adaptation efforts addressing extreme heat in Southeast Asia and maps adaptation finance according to SENDAI priorities, particularly Priority 3. The review highlights the prominence of extreme heat adaptation projects, particularly green roofs or spaces, in Southeast Asia, which tend to emphasize the financing aspects more. However, we also demonstrate the need for more financial investment and research on extreme heat adaptation solutions for this region. Future research, thus, may explore extreme heat research projects in Southeast Asia and their corresponding funding organizations for further insight into adaptation finance for extreme heat.
IG31-A007
CMIP6 Dynamical Downscaling for Future Climate Projections: Enhancing Urban Resilience Against Heatwaves and Extreme Precipitation in the Pearl River Delta
Ziping ZUO#+, Zhenning LI, Mau Fung WONG, Jimmy Chi Hung FUNG, Alexis LAU
The Hong Kong University of Science and Technology, Hong Kong SAR
In the past year of 2023, recorded as Earth’s hottest year, various extreme weather events, including flash floods, record-shattering heatwaves, and wildfires, ravaged many regions. Increasing greenhouse gas emissions may pressurize the expanding cities, causing elevated morbidity and mortality, power and water resources shortages, infrastructure breakdowns, economic impact, and more. Urban areas need to adapt and enhance resilience to withstand the challenges posed by worsening future weather conditions, leveraging scientific insights. In this study, by applying a dynamical downscaling method on the multi-model ensemble from CMIP6, we present model projections of heatwaves and extreme precipitation in the Pearl River Delta (PRD), one of the most densely populated and urbanized regions in the world. We considered three Shared Socioeconomic Pathways (SSP1-2.6, SSP2-4.5, and SSP5-8.5) in the mid-21st century (2040-2049) and at the end of the century (2090-2099). Our results suggest heatwaves are expected to be more frequent, intense, extensive, and longer-lasting for SSP2-4.5 and SSP5-8.5 until the end of the 21st century. Under the worst-case scenario of SSP5-8.5, extreme heat events that occurred once every 10 years in the 2010s are expected to occur once each month from June to September. While heatwaves pose significant challenges, they can also contribute to altered atmospheric conditions, potentially amplifying the likelihood of extreme precipitation events. Extreme hourly precipitation shows intensification under SSP2-4.5 and SSP5-8.5 in the 2040s and 2090s. Specifically, in the 2040s, 55.6% of the land area experiences an increase in extreme hourly precipitation under SSP2-4.5, while 69.5% under SSP5-8.5. By the 2090s, these percentages will rise to 75.6% and 88.6%, respectively. Hong Kong as a key megacity within the PRD, will experience the highest hourly precipitation of 233 mm/h in the 2040s and 295.1 mm/h in the 2090s, a significant rise from 158.1 mm/h in the 2010s.
IG31-A010
Impacts of Concurrent Hot and Dry Extremes on Hydropower Demand and Supply in the Pearl River Delta Realized by Convection-permitting Projections
Zixuan ZHOU1+, Eun-Soon IM1#, Lin ZHANG2
1The Hong Kong University of Science and Technology, Hong Kong SAR, 2City University of Hong Kong, Hong Kong SAR
The Pearl River Delta (PRD) is a low-lying area surrounding the Pearl River estuary, comprising several most densely populated megacities in Southeast Asia. In the summer of 2022, PRD experienced a prolonged period of record-breaking high temperatures, straining the power grid due to increased air-cooling demand. Concurrently, droughts in major hydropower generating regions exacerbated the power supply-demand gap. Considering China's goal of achieving carbon neutrality by 2060, ensuring energy security becomes crucial in the context of worsening climate extremes and the growing reliance on hydropower. Therefore, it is essential to understand how concurrent hot and dry extremes (CHDE) will affect the hydropower sector to facilitate climate adaptation decisions. Most existing studies have focused on univariate analysis of single extremes using coarse-grid global climate models (GCMs), which may not fully capture the region-specific climate impacts of global warming. To address this issue, this study will integrate convection-permitting (CP) regional climate modeling to assess the impacts of CDHE on hydropower demand and supply. Specifically, the Weather Research and Forecasting (WRF) model will be employed to downscale the bias-corrected CMIP6 GCM projections under the SSP5-8.5 scenario over southeastern China. The downscaled high-resolution and high-quality regional dataset will provide an enhanced representation of regional hydroclimate conditions. Subsequently, the climate data which translates into cooling demand and water scarcity, will be combined with plant-level electricity generation data, installed capacity, and other non-climatic data at the provincial level, including investment and electricity price. By using regression models, this combined dataset will enable empirical estimation of the relationship between CDHE and hydropower demand and supply. Overall, the project would be a meaningful showcase of the synergy of interdisciplinary collaborations in climate change adaptation. [Acknowledgements] This research was supported by the Theme-based Research Scheme, T31-603/21-N, which was funded by the Research Grants Council (RGC) of Hong Kong.
IG31-A011
Evaluation of Spatial Extent of Urban Heat Island Over Major Cities in Punjab, India
Vinayak BHANAGE#+, Han Soo LEE
Hiroshima University, Japan
The Urban Heat Island (UHI) is the most evident example of microclimatic modification induced by the process of urbanization. In the past, many researchers have shown interest in studying the UHI phenomenon. However, these studies, especially over the Indian region, rarely examined the UHI effect in terms of its spatial extent. In this study, with the aid of land surface temperature data obtained from the MODIS satellite (2003-2018), the seasonal and diurnal variations in the spatial extent of UHI were analysed over the seven cities of Punjab, India. In this process, a single exponential decay model was adopted to determine the spatial extent of the UHI effect. Results show that the UHI effect's spatial extent varies substantially concerning the cities and time. During the daytime of the summer (winter) season, the spatial extent of the UHI effect ranges from 4.1 to 6.97 (4.63 to 5.95) times of the urban area, while in the night period of summer (winter) season, this extent spans between 3.92 to 9.83 (2.49 to 7.88) times of the urban area. The results of this study depict that UHI affects not only the urban areas but also the microclimate of the surrounding rural area.
IG32-A002
Evaluate the Effectiveness of Machine Learning in Training Urban Canopy Temperature in China
Yingchao GUO#+, Ning ZHANG
Nanjing University, China
Urban heat waves can intensify the urban heat island effect, which has profound implications for public health and the climate system. However, current numerical models of the Earth lack accurate representations of urban areas and involve intricate parametric physical processes, resulting in significant uncertainties in forecasting daily canopy temperature. Therefore, this study aims to assess the efficacy of machine learning methods in training canopy temperature. In this paper, we employ the xgboost method to establish a training emulator. The atmospheric forcing field data, encompassing downward long-wave radiation, downward short-wave radiation, temperature, humidity, wind speed, air pressure, and precipitation, that drives the Community Land Model (CLM) in the Community Earth System Model (CESM), is utilized as the training set. Through this training process, we derive the maximum daily canopy temperature. The results demonstrate the following:(1)he machine learning method yields a root mean square error (RMSE) for canopy temperature and a simulated canopy temperature from the CESM model, both below 1.4℃, with an R2 above 95%;(2)Significant overestimations are observed in most parts of the Beijing-Tianjin-Hebei region, southern region, and Fen-Wei Plains region, while noticeable underestimates occur in Tianjin and the Yangtze River Delta region;(3)Additionally, by substituting canopy temperature with ten land cover zone (LCZ) conditions, we observe that the RMSE of LCZ1 is the smallest, while LCZ5 exhibits the largest values. This indirectly indicates variations in machine learning methods across different LCZ cases;(4)Furthermore, by utilizing machine learning to expedite numerical model calculations and unveil underlying physical processes, we contribute to addressing the interpretability issue of machine learning to some extent.
IG32-A005
Optimizing Climate Data Analysis Workflows: Strategies and Lessons Learned from Two Case Studies
Alexander GOODMAN1#+, Colin RAYMOND2, Peter KALMUS1
1California Institute of Technology, United States, 2University of California Los Angeles, United States
Computational requirements for climate data analysis workflows have been dramatically increasing in recent years. This has occurred in proportion to increases in both spatial and temporal resolution and particularly in the context of climate models, the number of datasets being used in the analysis as well. Much emphasis on the tooling that has been developed to meet this need has been in the form of big data frameworks and parallel computing to perform analyses at scale. However, the use of such tools also has some important drawbacks such as creating additional complexity in the analysis codes (and therefore more prone to bugs) as well as potentially being very expensive. In practice, we have found that in many cases, climate data analysis codes are poorly optimized and so greater benefits can be gained simply from writing more performant code without immediately resorting to parallelism. Here we will describe examples of how to optimize publicly available codes for two algorithms that are highly relevant in recent climate modeling studies. These will include calculations for wet bulb temperature (Davies-Jones 2008) and extended heat index (Lu and Romps, 2022). We will demonstrate how our optimizations were able to improve the running times of both use-cases by two orders of magnitude.
IG32-A013
Evolving the Coupled Model Intercomparison Project (CMIP) to Better Support the Climate Community and Future Climate Assessments
Helene HEWITT1, John DUNNE2, Julie ARBLASTER3, Olivier BOUCHER4, Paul DURACK5, Tomoki MIYAKAWA6+, Matthew MIZIELINSKI1, Robert PINCUS7, Sasha AMES5, David HASSEL8, Birgit HASSEL9, Forrest HOFFMAN10,11, Martin JUCKES12, Guillaume LEVAVASSEUR4, Chloe MACKALLAH13, Vaishali NAIK2,14, Atef BEN NASSER4, Benjamin SANDERSON15, Isla SIMPSON16, Martina STOCKHAUSE17, Karl TAYLOR5, Beth DINGLEY18#, Daniel ELLIS18, Eleanor O'ROURKE18, Briony TURNER18
1Met Office, United Kingdom, 2NOAA Geophysical Fluid Dynamics Laboratory, United States, 3Monash University, Australia, 4Institut Pierre-Simon Laplace, Sorbonne Université / National Centre for Scientific Research, France, 5Lawrence Livermore National Laboratory, United States, 6The University of Tokyo, Japan, 7Columbia University, United States, 8National Centre for Atmospheric Science / University of Reading, United Kingdom, 9Deutsches Zentrum für Luft- und Raumfahrt, Germany, 10Oak Ridge National Laboratory, United States, 11University of Tennessee, Knoxville, United States, 12UK Research and Innovation, United Kingdom, 13Commonwealth Scientific and Industrial Research Organisation, Australia, 14NOAA Oceanic and Atmospheric Research, United States, 15Centre for International Climate and Environmental Research, Norway, 16National Center for Atmospheric Research, United States, 17German Climate Computing Center, Germany, 18CMIP International Project Office, United Kingdom
Over four decades, CMIP has driven massive improvements in the modelled representation of the Earth system, whilst also seeing huge growth in its scope and complexity. In its most recent phase, CMIP6, a broad spectrum of questions continues to be answered across twenty-four individual model intercomparison projects (MIPs). This science improves process understanding and assesses the climate’s response to forcing, systematic biases, variability, and predictability in line with WCRP Scientific Objectives. CMIP and its associated data infrastructure have become essential to the Intergovernmental Panel on Climate Change (IPCC) and other international and national climate assessments, increasingly including the downstream mitigation, impacts, and adaptation communities. However, despite the invaluable science produced from CMIP6 data, many challenges were still faced by the model data providers, the data delivery infrastructure, and users, which need to be addressed moving forwards. A specific challenge in CMIP6 was the burden placed on the modelling centres, in part due to the large number of requested experiments and delays in the preparation of the CMIP6 forcing datasets and climate data request. The CMIP structure is evolving into a continuous, community-based climate modelling programme to tackle key and timely climate science questions and facilitate delivery of relevant multi-model simulations. This activity will be supported by the design of experimental protocols, an infrastructure that supports data publication and access, and quasi-operational extension of historical forcings. A subset of experiments is proposed to be fast-tracked to deliver climate information for national and international climate assessments and informing policy and decision making. The CMIP governing panels are coordinating community activities to reduce the burden placed on modelling centres, continue to enhance novel and innovative scientific activities, and maximise computational efficiencies, whilst continuing to deliver impactful climate model data.
IG32-A014
Hydroclimate Changes in Sri Lanka Over the Past Millennium
Liangcheng TAN1#+, Xiqian WANG2, Jin ZHANG2, Mathara SAMANMALI3, Le MA2, Qiang LI2, Gang XUE4, Jingjie ZANG2, Hai CHENG5,1, Ashish SINHA6
1Institute of Earth Environment, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China, 3University of Colombo, Sri Lanka, 4Northwest University, China, 5Xi'an Jiaotong University, China, 6California State University Dominguez Hills, United States
Understanding the decadal variability of hydroclimate in Sri Lanka during historical time is of great significance for disaster prevention, water resource management, and agrarian economy in this area under a global warming scenario. However, the evolution patterns and driving mechanisms of decadal hydroclimate variability in Sri Lanka remain controversial due to lack of long-term and high-resolution records. Here we present the first temporally highly resolved stable isotope and trace element stalagmite records in Sri Lanka, covering the past millennium. Our records agree well with other hydroclimate records over Indian subcontinent and Southeast Asia, showing two notable humid intervals during the early medieval period and the late Little Ice Age, and prolonged droughts from 1200 to 1600 CE. By using this record, we further explore the driving mechanisms of hydroclimate variations in Sri Lanka on centennial to decadal scales and its possible impacts on societal changes.
IG32-A015
Temperature Variability Associated to Climate Feedback Using an Energy Balance Model
Hyoji KANG+, Minjeong CHO, Yong-Sang CHOI#
Ewha Womans University, Korea, South
Understanding the temperature variability is essential as the incidence of climate extremes changes potentially, even with a small shift of mean climate. However, the fundamental mechanism of temperature variability behind changes in mean climate remain largely unknown. Especially, the change in temperature variability might be subject to equilibrium climate sensitivity (ECS), as ECS implies the extent of Earth’s temperature response to increasing atmospheric greenhouse gases. In this facet, this study aims to explore the characteristic of temperature variability in response to the random forcing by different ECS. We assessed the change in temperature variability using the standard deviation of simulated temperatures for 100 years. For the sake of looking into this effect, we utilized the energy balance model, which enables to manipulate climate feedback and heat capacity for simulation of temperature in simple but conceptually physical framework. We obtained the relationship between the ECS and temperature variability, so that the future study can estimate the ECS by using temperature variability from observational data.
IG32-A020
Machine Learning-based Wildfire Detection Considering Environmental Context and Structural Similarity
Taejun SUNG#+, Yoojin KANG, Jungho IM
Ulsan National Institute of Science and Technology, Korea, South
The frequency and intensity of wildfires are increasing annually due to climate change, resulting in diverse and escalating damages. Geostationary satellites provide real-time acquisition of extensive wildfire information, facilitating efficient wildfire monitoring. Traditional satellite-based wildfire detection algorithms utilize the brightness temperature difference between the central pixel and its surrounding pixels to detect thermal anomalies. However, performance may decrease when environmental conditions vary between the central and surrounding areas. Additionally, traditional algorithms only employ vector-based statistics, neglecting the structural information inherent in satellite imagery. In this study, to address the limitations of traditional satellite-based wildfire detection algorithms, we developed a wildfire detection model based on light gradient boosting machine (LGBM) that incorporates environmental context correction and structural similarity comparison. The GK-2A (GEO-KOMPSAT-2A) satellite imagery was used as the main input variable, and the Korea Forest Service wildfire occurrence data was used as a reference. The detection performance of the LGBM model (precision: 98%, recall: 95.2%, F1 score: 96.6%) showed improvement after the application of environmental context correction and structural similarity comparison (precision: 98.5%, recall: 96.2%, F1 score: 97.3%). The LGBM model detected small wildfires that the GK-2A wildfire detection algorithm failed to identify and demonstrated higher detection rates. Environmental context correction and structural similarity comparison improved detection performance for extreme environmental conditions and low intensity wildfires, respectively. This study analysed error factors in traditional satellite-based wildfire detection algorithms and proposed a novel approach to improve them, suggesting the potential for a generalized wildfire detection model applicable in various environments.
IG33-A001
Spatial Characteristics of Daily Max/min Urban Surface Temperatures During Heat Waves: A Case Study of the Tokyo Metropolitan Area
Moena FUKATSU#+, Yuhei YAMAMOTO, Kazuhito ICHII
Chiba University, Japan
In response to climate change, Japan is facing an increasing frequency and intensity of heatwaves. The synergistic effect of urban heat island and extreme heat poses serious societal impacts, including heightened risk of heatstroke and increased energy consumption. This study investigates the relationship between land surface temperature (LST) and urban land use during heatwave conditions, under the assumption that the primary factor shaping the thermal environment during extreme heat lies in the urban surface structure. Focusing on the heatwave events of 2018 and 2023, we used Himawari-8/9 LST product to estimate the spatial distribution of daily maximum and minimum temperatures (Tmax and Tmin, respectively) in the urban areas surrounding Tokyo. The Himawari-8/9, Japan's geostationary satellite, LST product offers a spatial resolution of 0.02° and a temporal resolution of 10 minutes. The results showed that the Tmax during heatwaves exhibited a positive anomaly of 10–20°C in croplands and paddy fields and 5–10°C in urban areas compared to normal years (2015–2022). This suggests significant reflections of changes in surface water balance. On the other hand, the Tmin during heatwaves exhibited a higher positive anomaly in urban areas, indicating a strong influence of heat storage effects. Interestingly, in suburban inland areas, there were regions where high positive anomalies of both Tmax and Tmin overlapped, suggesting a compound effect of heat storage and local surface water balance.
IG33-A006
Optimization of Electric Scooter Placement Stations Based on Distance Tolerance
Yingqiu LONG1+, Jianwei YUE1#, Shaohua WANG2
1Beijing Normal University, China, 2Chinese Academy of Sciences, China
The proliferation of shared electric scooters(E-scooter) has facilitated urban mobility, yet it has also brought challenges such as disorderly parking and supply-demand imbalances. Given the current inadequacies in the quantity and spatial layout of shared E-scooter deployments, as well as the insufficient research on deployment stations, this study extensively analyzed the travel characteristics of E-scooters in Chicago. Employing a multi-criteria decision-making approach to assess factors influencing demand, the study aimed to maximize user coverage and minimize the total distance from users to deployment stations. To achieve this optimization goal, a distance tolerance-based maximum coverage placement model was developed, and a Deep Reinforcement Learning(Deep RL) was designed to solve the model. Case experiments confirmed the model's effectiveness in optimizing the layout of E-scooter deployment stations. The study also validated the feasibility and effectiveness of applying the Deep RL algorithm in facility placement by comparing its results with those obtained using the Gurobi solver and a genetic algorithm. This study provides valuable reference for the selection of facility sites for urban shared transportation, and the application of Deep RL offers a efficient perspective and approach to facility placement problems.
IG33-A007
Spatial Sensitivity Analysis of Evapotranspiration Over Korea Peninsula
Chanyoung KIM+, Kijin PARK, Jongmin PARK#
Korea National University of Transportation, Korea, South
Global climate change and extreme climate conditions intensifies the regional imbalance of water cycle components and water security, which leads to enhancing necessity of developing efficient and sustainable water management system. In Korea, Evapotranspiration (ET), a sum of soil evaporation and plant transpiration, accounts for 43% of annual precipitation, and thus, plays a critical role in understanding regional land-atmospheric components. ET is sensitive to various hydrometeorological variables such as relative humidity, air and surface temperature, vapor pressure, wind speed, and solar radiation. However, the sensitivity of each variable to ET may different based on the various conditions including land cover and land use, climate characteristics, and topographical aspects. Accordingly, this study explored spatial sensitivity of ET towards various hydrometeorological variables over Korea Peninsula. Specifically, this study implemented hydrometeorological variables from ECMWF Reanalysis version 5-land (ERA5-Land) from 2000 to 2022. In addition, various spatial sensitivity analysis tools (e.g., Regional Sensitivity Analysis [RSA], Variance-Based Sensitivity Analysis [VBSA], the Fourier Amplitude Sensitivity Test [FAST]) were employed to quantify the sensitivity of various hydrometeorological components to ET at grid scale. Acknowledgement: This work was supported by Korea National University of Transportation 2024.
IG33-A013
Consumption of Building Energy Under Global Warming
Soohyun AHN#+, Woosok MOON
Pukyong National University, Korea, South
Since the 1980s, an overabundance of urban land development projects has led to the proliferation of satellite cities around major metropolitan areas, resulting in heightened population density and increased energy demand. This surge in urbanization has amplified concerns regarding energy supply, highlighted by the widespread blackout incident on September 15, 2011, when reserve power dropped to 0 kW. A late-summer heatwave during this period was identified as a significant contributor to the escalating power demand, underscoring the necessity of accurate energy forecasting in the context of climate change. Consequently, precise prediction of building energy consumption has emerged as a critical issue. Among the tools gaining prominence for building energy simulation is EnergyPlus, developed by the U.S. Department of Energy (DOE). EnergyPlus simulates various aspects of building energy use, including heating, cooling, lighting, and ventilation. Operating fundamentally on weather data and building information, EnergyPlus underscores that weather is crucial for building energy simulation and energy-efficient retrofitting, given the strong dependency of building energy use on weather conditions. This model can serve as a significant indicator for power fluctuations due to climatic changes. The current study employs EnergyPlus to analyze trends in power variations in response to climatic shifts, aiming to enhance the predictability of electricity demand. This research supports the development of sustainable urban energy plans, taking into account the increasing variability and unpredictability associated with climate change. By focusing on building energy simulations, this study contributes to a deeper understanding of the relationship between urbanization, climate change, and energy demands, providing valuable insights for future urban planning and energy policy.
IG33-A014
Evolving Urban Heat Islands: A Comprehensive Study of Temporal and Developmental Impacts in South Korean Cities
Mijeong JEON#+, Woosok MOON
Pukyong National University, Korea, South
In the context of climate change induced by global warming, the urban heat island (UHI) effect has emerged as a significant concern in urban areas. As cities continue to expand, artificial structures such as buildings and roads increasingly absorb solar energy, leading to a rise in energy consumption. Recent research has predominantly focused on temperature differences between urban and rural regions, examining trends in urban temperature changes over time and daily temperature variations. However, it is worth noting that comprehensive studies on the UHI effect remain limited. Specifically, there has been a lack of research that simultaneously considers variables such as year, hour, and temperature in the context of daily cycle variations. Moreover, in the case of South Korea, there is still no research that utilizes data from all observation stations. With this backdrop, our study aims to investigate how the temperature daily cycle has evolved over time, from the past to the present, as a result of the UHI effect. We conduct an analysis using all data across South Korea and develop a simplified surface energy balance model for qualitative understanding. Additionally, we conduct a comparative analysis between major cities and newly developed urban areas to see the time-evolution of the UHI effect during the growth of a new city. The results of study align with previous research, indicating a more pronounced UHI effect during nighttime compared to daytime. Seasonally, this effect is most evident in autumn. We find that the UHI phenomenon is more noticeable in accordance with urban development. This distinction becomes particularly clear when comparing established major cities with newer urban regions. These findings suggest that the degree of urban development plays a significant role in the manifestation of the UHI effect, which has important implications for urban planning and sustainability in varying urban environments.
Session Chair(s): Yaohui LIU, Shandong Jianzhu University, Alessandro MONDINI, National Research Council
IG01-A003
Epidemic Modeling and the Cascade of Disasters: Applications to Indigenous Communities
Vena Pearl BONGOLAN1,2#+, Will Bryan JOSE3, Ray Gerard NUÑEZ3, Janinalaine PLATERO3, Julia Beatriz SABADO3
1De La Salle University Manila, 2AI4PEP Philippines, 3University of the Philippines
We continue our research on epidemiology: to monitor, via a telehealth backbone, remote and isolated communities of indigenous Ati peoples in the islands of Panay and Guimaras in the Philippines. The relatively small sizes of the communities, and their geographic spread is both boon and bane. We use statistical thresholds and apply epidemic models to give watches, warnings and emergency alerts for infections disease outbreaks in the communities. Predictive modeling comes in planning the emergency response, which will come from regional health offices and local government units. Our research on the cascade of disasters will be used to plan an optimal response to ensuing mental health issues from an infectious disease outbreaks. This latter is in the early stages, and currently concentrates on the recent Covid-19 epidemic and its toll on mental health.
IG01-A029
Empowering Healthcare of Indigenous Populations: A Digital Twin Approach for Preventing and Mitigating Risks and Outbreaks
Jose Marie Antonio MIÑOZA1,2#+, Jimuel Jr CELESTE2, Vena Pearl BONGOLAN3,4, Romulo DE CASTRO5
1Center for AI Research, 2University of the Philippines Diliman, 3De La Salle University Manila, 4AI4PEP Philippines, 5University of San Agustin
This research explores the strategic integration of Digital Twin technology within healthcare, particularly for indigenous communities, by employing advanced data fusion techniques to enhance precision and insight. Our study proposes a novel holistic framework for improving healthcare of marginalized communities. Through Digital twins, the health professionals and the community can monitor and identify potential health risks, predict disease progression to potential outbreaks, and enable proactive interventions by leveraging patient notes data, machine learning algorithms, and predictive modeling. In this study, information extraction using deep learning algorithms were leveraged to enhance patient care such as identification of treatment and symptoms, forecasting consultation demand, clustering of possible emergent diseases, with a distinct focus on addressing mental health issues. Our approach, since it is tailored for indigenous populations, represents a paradigm shift in healthcare management, promising increased resilience and responsiveness to the unique healthcare challenges that these communities face.
IG01-A008
Multi-dual Remote Sensing and Deep Learning Helps Disaster Risk Reduction
Yaohui LIU#+
Shandong Jianzhu University
Natural disasters are sudden and unpredictable, posing a serious threat to people’s lives, property, and economic and social stability. In recent years, the rapid development of multidisciplinary fields such as remote sensing technology, geographic information science, machine learning, and deep learning has provided rich data information and mature method models, providing sufficient support and scientific basis for urban disaster monitoring and risk management. The combination of multi-source data and multi-disciplinary methods is of great significance for minimizing natural disaster risks and disaster prevention and mitigation. To this end, this report mainly introduces the recent works of our research group on urban comprehensive disaster prevention and mitigation by integrating multi-source remote sensing data and deep learning. Firstly, based on high-resolution remote sensing data, a convolutional neural network model is constructed to achieve high-precision and automatic extraction of buildings. Secondly, using machine learning and data mining methods, combined with multi-source data such as street view images, road traffic, statistical data, and multi-temporal remote sensing images, the corresponding rules between building attribute information and building vulnerability are established. Finally, by applying the earthquake disaster loss model and combining statistical data such as population and economy, the damage to buildings, casualties, and economic losses in the study area under different earthquake intensities are quantitatively evaluated to provide auxiliary reference for daily earthquake damage defense and earthquake emergency management work.
IG01-A010
Disaster Management and Resource Development - Case Study of Developed and Developing Countries
Pratibha DEWANGAN1#+, Narayan Prasad DEWANGAN2,3, Pranay DEWANGAN4
1Government College of Teachers Education, 2Chhattisgarh Government, 3Chhattisgarh Swami Vivekanand Technical University, 4GAIL India Limited
The world can be understood socioeconomically as the developed and developing/undeveloped countries with respect to the geographical positioning and resources availability. The oceanic countries are particularly prone to frequent natural disasters. Often the underdeveloped countries suffer from the shortfall of local resources and mechanisms for which the global cooperation needs to be pulled in for rescue operations, rehabilitations and the management after the disaster is gone. This paper presents the global approach to quick deployment of the resources particularly in the developing countries for the better disaster management in the aftermath of the disaster.
IG01-A013
Characteristics of Seismic Disaster Awareness of China’s High School Students and Implications for Disaster Education Improvement: A Case Study in Weinan Area, China
Guiwu SU1#+, Tengfei ZHANG1, Wenhua QI1, Benyong WEI1, Minchao PEI2, Xinxin GUO1
1China Earthquake Administration, 2Academy of Plateau Science and Sustainability, People’s Government of Qinghai Province and Beijing Normal University
Raising people’s disaster awareness is a prerequisite to enhancing their disaster-coping capacities. For high school students, school education is a major pathway to cultivating their disaster awareness. However, existing exploration on disaster awareness of China’s high school students and associated education issues still remains far from sufficient so far. Based on UNISDR’s term of public awareness and our long-term similar prior work, this study thus firstly proposed an education objective-oriented construction of what earthquake disaster awareness (EDA) might be by fully incorporating UNESCO-UNEP’s classic understanding of what Environmental Education Objectives mean. With this novel concept construction that consists of 5 specific dimensions (i.e., risk perception and disaster sensitivity, earthquake disaster knowledge, earthquake disaster-coping skill and policies, attitude and values, and disaster reduction participation), several different sets of EDA-measurement questionnaires that deliberately target different public groups (i.e., students, teachers, students’ parents, and general public) were developed. Using these questionnaires, the current EDA status of Weinan people, China, and associated disaster education issues were carefully surveyed in 2019 through stratified sampling process. Data analysis of those of high school students shows that ①their overall EDA level is acceptable, but local risk perception and disaster sensitivity aspect is apparently unsatisfactory. ②Girls are better than boys in “attitude and values” and “participation” dimensions, while boys are better in “knowledge” and “skill and policies” aspects. ③As grades rise, students’ disaster reduction-focused attitude, values, and participation are more and more passive or indifferent. ④EDA impacting effects of different disaster education-focused extracurricular activities are clearly varied. With these findings, several education objective-specific policy recommendations for improving local school disaster education were finally provided. The central logic of this education objective-oriented construction of EDA has promising transferable implications for addressing similar issues of both other kinds of disasters and the disasters in other countries.
IG01-A019
Landslide Susceptibility Mapping Using Frequency Ratio and Analytical Hierarchy Process in the Mineralized Province of Benguet and the Volcanic Region of Southern Luzon, Philippines
Earvin Jon GUEVARRA1#+, Beth Zaida UGAT1, Decibel FAUSTINO-ESLAVA1, Bianca Maria Laureanna PEDREZUELA1, Jenielyn PADRONES1, Juan Miguel GUOTANA1, Jayson ARIZAPA1, Cristino Jr. TIBURAN1, Jefferson RAPISURA1, Gabriel Angelo MAMARIL1, Maria Regina REGALADO1, Loucel CUI1, Rosemarie Laila AREGLADO1, Carla DIMALANTA2
1University of the Philippines Los Baños, 2University of the Philippines Diliman
Landslides are one of the most destructive geohazards in the Philippines, claiming lives and destroying infrastructures. At the very least, they also interrupt traffic, especially in mountainous areas. To manage the adverse effects of landslides, Landslide Susceptibility Mapping is an important soft mitigation measure to reduce risks for communities in landslide-prone areas. This study generated Landslide Susceptibility Maps (LSM) for areas of different geological characteristics: the mineralized Benguet province and the volcanic region of Southern Luzon. There are eight (8) landslide causative factors considered for each of the geological areas, namely elevation, slope, soil, geology, land cover, faults and lineaments, and roads and rivers for both areas wherein alteration types are unique for mineralized areas while aspects were of importance for volcanic regions. The classes in factors were reclassified depending on their perceived influence on landslide susceptibility using the frequency ratio (FR) method. This is the correlation between the percentage of past landslides over the percentage of class size in a factor. The FR values were grouped into very low (0-0.25), low (0.25-0.50), moderate (0.50-0.75), high (0.75-1.00), and very high (>1) wherein very low is reclassified as one (1) while very high as five (5). The Analytical Hierarchy Process (AHP) developed by Saaty (1980) was used to generate the weights for the weighted overlay analysis of each geologic area. Eleven (11) experts rated the causative factors based on the effect of each factor on landslide susceptibility and were consolidated for final weights. LSM shows a high percentage of high to very high susceptibility in mineralized Benguet province due to its slopey terrains and widespread alteration while the volcanic region is generally high to very high susceptibility in mountainous areas. The results of this study contribute to the disaster risk reduction efforts of the local communities in the study areas.
IG01-A028
Deep Learning Forecast of Rainfall-induced Shallow Landslides in Italy
Alessandro MONDINI#+, Fausto GUZZETTI, Massimo MELILLO
National Research Council
Rainfall-induced landslides occur daily all around the world causing victims and damage to people, property, and the environment. The ability to anticipate their occurrence is crucial for effective landslide risk reduction and increased resilience. However, how much rain does it take to trigger a landslide? Empirical rainfall thresholds and coupled slope-stability and rainfall infiltration models are commonly used to anticipate the occurrence of rainfall-induced shallow landslides. However, evidence suggests that they may not be effective for operational forecasting over geographical scales. We propose a deep-learning-based modelling strategy to classify hourly rainfall measurements as able or not able to trigger landslides. We train a large ensemble of 2400 neural networks using hourly rainfall measurements taken by more than 2000 rain gauges and information on more than 2400 landslides that occurred in the period from February 2002 to December 2020 in Italy. Results show that (a) it is possible to anticipate the occurrence of rainfall-induced shallow landslides in Italy, and (b) the rainfall-induced shallow landslides occurrence is mainly controlled by the rainfall event characteristics. Our results open the possibility of improved operational rainfall-induced landslide forecasting in Italy.
IG01-A018
Soil Physical and Clay Mineralogical Characterization in Mineralized and Non-mineralized Landslide-prone Areas in Luzon, Philippines
Bianca Maria Laureanna PEDREZUELA1#+, Jenielyn PADRONES1, Isaac Qairo BURGOS2, Decibel FAUSTINO-ESLAVA1, Juan Miguel GUOTANA1, Beth Zaida UGAT1, Maria Regina REGALADO1, Jefferson RAPISURA1, Earvin Jon GUEVARRA1, Gabriel Angelo MAMARIL1, Loucel CUI1, Rosemarie Laila AREGLADO1, Rubenito LAMPAYAN1, Carla DIMALANTA3
1University of the Philippines Los Baños, 2Akita University, 3University of the Philippines Diliman
Soil properties are important in studying landslide mechanisms as water movement varies with different types of soil. However, this topic is still understudied in the Philippines. This study characterized the physical and mineralogical properties of soils from landslide areas of mineralized and non-mineralized zones in the Benguet Province and the Bicol region. Soil physical properties analyses such as soil texture, soil densities, Atterberg limit, hydraulic conductivity, and free swell test were carried out on selected representative samples taken from landslide scarps. X-ray Diffraction (XRD) analysis was done to determine the mineral composition of the soil samples. Results showed that the mineralized samples have higher sand percentage relative to the non-mineralized soils which exhibit relatively higher clay percentage. This, in turn, corresponds to the low to very high plasticity values of the mineralized samples in contrast to the intermediate to extremely high plasticity values of the non-mineralized samples. Soil texture-based rainfall-landslide thresholds show that slopes characterized by samples with low plasticities tend to have failures at lower thresholds, whereas samples with high plasticities fail at higher thresholds. Hydraulic conductivity tests also demonstrated low permeability of fine-grained soils, hence, a higher rainfall landslide threshold was generated for this soil type. Further, both mineralized and non-mineralized samples indicate negligible to low expansivity as denoted by their Free Swell Ratio values. XRD analysis of the non-mineralized samples revealed the presence of swelling clay minerals such as montmorillonite and non-swelling clay minerals such as illite and kaolinite. The cohesiveness of these clay minerals contributed to the overall slope stability in the non-mineralized zones. Contrastingly, mineralized samples contain intermediate (1-10%) amounts of quartz minerals due to silicic alteration which resulted in cohesionless sandy soils observed in the mineralized study sites. These pedological characteristics can be used to aid in generating site specific rainfall - landslide thresholds.
Session Chair(s): Dmitri KONDRASHOV, University of California, Los Angeles
IG04-A004
Dynamics-driven Predictions of Various Chaotic Systems Using Dynamical System Deep Learning Method
Hao LI+, Jianping LI#
Ocean University of China
In this paper, we proposed a novel method for predicting nonlinear chaotic dynamical systems—Dynamical System Deep Learning (DSDL). It fundamentally differs from machine learning methods based on mathematical statistics, as it can reconstruct the dynamical properties of a system using known time series information and make dynamics-driven predictions. When we applied Artificial Neural Network (ANN), Echo State Network (ESN), Long short-term Memory (LSTM), and DSDL to short-term forecasting of nonlinear chaotic dynamical systems which can represent the highly approximate atmospheric system, such as the Lorenz system and Lorenz 96 system, the results show that the DSDL method achieves the highest Effective Prediction Time (EPT) with the least time consumption, demonstrating the effectiveness and superiority of DSDL. For long-term predictions, we discover that the predictions from the DSDL method closely match the numerical solutions of various dynamical systems in statistical properties, indicating that DSDL is not only suitable for short-term weather forecasting but also for long-term climate prediction. Additionally, we employed Cross Validation Stepwise Regression (CVSR) algorithm to select key variables used by the DSDL during prediction, this endows the DSDL with interpretability, resolving the black-box issue present in traditional machine learning methods. Simultaneously, it improves prediction performance and reduces computational time.
IG04-A027
A General Method Based on Artificial Neural Networks for Estimating the Parameters of Partial Differential Equations Equations for Soil Thermodynamics and Hydrodynamics in Weather and Climate Models
Mikhail KRINITSKIY1,2#+, Victor STEPANENKO3
1Shirshov Institute of Oceanology, Russian Academy of Sciences, 2Moscow Institute of Physics and Technology, 3Lomonosov Moscow State University
Partial differential equations (PDEs) serve as a cornerstone in a multitude of scientific and engineering disciplines. Despite a rich history of numerical methodologies for tackling both direct and inverse PDE challenges, these traditional approaches often require extensive computational efforts, at times necessitating the power of supercomputing facilities. Additionally, conventional techniques for identifying PDEs presuppose specific functional forms for determining coefficients, thus restricting the spectrum of potential solutions. Such limitations have spurred a growing interest in leveraging artificial intelligence to both directly solve and identify PDEs. In this research, we introduce a novel approach employing artificial neural networks (ANNs) to identify PDEs without relying on stringent a priori suppositions about the function families that approximate PDE coefficients. This allows for the estimation of PDE coefficients by observing the progression of a PDE's direct solution. The effectiveness and precision of our ANNs-based strategy are verified through the study of the diffusion equation and the nonlinear diffusion-advection equation (Richards equation), which are applied to model heat and moisture dynamics in soil. Our results reveal that our new ANNs methodology surpasses the alternatives composed based on supposed forms of PDE parameters by at least an order of magnitude in both mean absolute percentage error (MAPE) and root mean square error (RMSE) of the estimated coefficients. Given the fundamental nature of the equations studied, it is envisioned that our ANNs-based approach will find successful application in a broader context, such as in the optimization of turbulence closures within hydrodynamic problems, where benchmark solutions of PDEs are often derived from high-fidelity direct Navier-Stokes simulations.
IG04-A006
Exploring Super-resolution Climate Downscaling to Facilitate Photovoltaic Power Assessments in Japan
Alessandro DAMIANI#+, Noriko ISHIZAKI, Hidetaka SASAKI
National Institute for Environmental Studies
We applied a perfect prognosis approach to downscale four meteorological variables over central Japan using four machine learning (ML) algorithms. In addition to commonly investigated variables, such as air temperature and precipitation, we also focused on wind speed and surface solar radiation, which are not frequently examined due to the scarcity of long-term, reliable high-resolution observational datasets. After training the ML models with perfect predictors, the downscaling performance of the four variables followed the order of: temperature > surface solar radiation > wind speed > precipitation. Having assessed the dependence of the downscaling accuracy on grid resolution, we focused on a super-resolution downscaling. We found that the convolutional neural network (CNN) generally outperformed the other linear and non-linear algorithms for all variables. The CNN was further able to reproduce extremes. With the rapid transition from coal to renewables, the need to evaluate low solar output conditions at a regional scale is expected to benefit from CNNs. Because weather affects photovoltaic (PV) power output in multiple ways, and future climate change will modify meteorological conditions, we focused on obtaining exemplary super-resolution application by evaluating future changes in PV power outputs using climate simulations. Our results confirmed the reliability of the CNN method for producing super-resolution climate scenarios and will enable energy planners to anticipate the effects of future weather variability.
IG04-A013
Evaluating Machine Learning Approaches for Bridging Atmospheric N2O Data Gaps from Antarctic Ice Cores
Nasrin SALEHNIA+, Jinho AHN#
Seoul National University
Ice cores play a crucial role as a repository, documenting atmospheric Greenhouse Gas (GHG) concentrations over the past 800 thousand years. However, the temporal resolution and gaps in these records limit our comprehensive understanding of greenhouse gases and climate dynamics. Among anthropogenic greenhouse gases in the contemporary atmosphere, N2O is the third most significant, with a lifespan of approximately 118-131 years, following CH4 and CO2. The global nitrogen cycle, regulated by intricate biological processes, governs atmospheric N2O levels. This study aims to simulate historical atmospheric N2O concentrations using Artificial Intelligence (AI) and Machine Learning (ML) techniques, integrating them with available paleo records. Antarctic ice cores provide CO2 and CH4 concentration data for N2O modeling over the last 800 thousand years (ka). The dataset is divided into training (70%), validation (15%), and test (15%) subsets based on temperature proxy data. N2O modeling involves Artificial Neural Networks (ANN), Wavelet Analysis (WL), and three distinct ML methods: Support Vector Machine, Tree, and Gaussian Process Regression (GPR). The results demonstrate that the GPR ML method produces a high-quality simulation with R2= 0.93, RMSE= 5.13 ppb, and MAE= 1.97 ppb. Consequently, this model is selected to address gaps in N2O data. These simulations aim to generate high-resolution N2O data, filling the gaps in existing ice core records. Future research will expand to modeling with alternative AI and ML methodologies, applying these techniques to diverse ice core records spanning various historical periods.
IG04-A024
Ice Model Calibration Using Semicontinuous Spatial Data
Won CHANG#+
University of Cincinnati
Rapid changes in Earth’s cryosphere caused by human activity can lead to significant environmental impacts. Computer models provide a useful tool for understanding the behavior and projecting the future of Arctic and Antarctic ice sheets. However, these models are typically subject to large parametric uncertainties, due to poorly constrained model input parameters that govern the behavior of simulated ice sheets. Computer model calibration provides a formal statistical framework to infer parameters, using observational data, and to quantify the uncertainty in projections due to the uncertainty in these parameters. Calibration of ice sheet models is often challenging because the relevant model output and observational data take the form of semicontinuous spatial data with a point mass at zero and a right-skewed continuous distribution for positive values. Current calibration approaches cannot handle such data. Here, we introduce a hierarchical latent variable model that handles binary spatial patterns and positive continuous spatial patterns as separate components. To overcome challenges due to high dimensionality, we use likelihood-based generalized principal component analysis to impose low-dimensional structures on the latent variables for spatial dependence. We apply our methodology to calibrate a physical model for the Antarctic ice sheet and demonstrate that we can overcome the aforementioned modeling and computational challenges. As a result of our calibration, we obtain improved future ice-volume change projections.
IG04-A025
A Bayesian Stochastic Lightning Scheme for Global Climate Models
Vincent VERJANS1#+, Christian FRANZKE2
1IBS Center for Climate Physics, 2Pusan National University
Lightning is a global cause of wildfires, and also influences tropospheric chemistry through the production of NOx compounds. Yet, lightning is represented in Global Climate Models only through crude parameterizations or is simply prescribed as a forcing input without inter-annual variability. Lightning is governed by micro-scale processes, which cannot be resolved at the scale of Global Climate Models. Because lightning depends on climate and weather conditions, we develop a data-driven stochastic lightning scheme, which enables internal consistency between modeled atmosphere and lightning events. Specifically, we use satellite-based observations of lightning flashes spanning close to three decades in order to relate lightning rates to climatic variables from reanalysis data. We design a stochastic lightning scheme, in which statistical distributions are calibrated to large-scale weather conditions, and account for realistic randomness. Our calibration uses Bayesian methods, allowing to derive posterior probability distributions for the parameters of the lighting scheme. We use a Bayesian Monte Carlo algorithm allowing efficient search through the parameter space and prioritizing accuracy in key quantitative targets. Sampling from the stochastic scheme allows to generate any number of stochastic lightning realizations from the calibrated statistical distributions. Furthermore, marginalizing over the Bayesian posterior distributions provides a straightforward manner to account for parametric uncertainty. As such, our novel stochastic scheme enables Global Climate Models to (1) produce lightning rates internally consistent with the modeled climate, (2) sample stochastic realizations of lightning events to represent internal variability, and (3) account for parametric uncertainty in the lightning scheme. We implement our lightning scheme within the Community Earth System Model 2.2. We perform global multi-decadal simulations demonstrating that vegetation and climate are sensitive to lightning variability, mostly through feedback processes associated with natural wildfire occurrence.
IG04-A015
Estimation of 3D Basement Relief from Gravity Data Using a Combined PSPU-Net Network
Xuegang LIU1#+, Meixia GENG2, Lin KAI1, Yusuf Ali MOHAMMED3
1China University of Geosciences, 2Technology Innovation Institute, 3Khalifa University of Science and Technology
Gravity survey plays an important role in the study of sedimentary basin systems, where hydrocarbons commonly occur. In this study, we developed PSPU-Net, a deep-learning method specifically designed to recover the basement interface from gravity data. The developed PSPU-Net is based on two effective deep-learning methods: the Pyramid Scene Parsing Network and U-Net. Basin modeling and forward calculation were conducted to generate the sediment-basement interface models and corresponding gravity datasets for the training and evaluation of PSPU-Net. The sediment-basement interface models were constructed by a series of randomly generated rectangles with filtering. Forward calculation of the gravity dataset was completed by the GPU-accelerated computing method and parabolic density contrast method to improve the modeling efficiency. The application on synthetic models demonstrates that the developed PSPU-Net can effectively recover the sediment-basement interface relief and provide generalization ability for different sediment-basement interface models. Finally, the proposed method was applied to the field data from eastern Somaliland, and normalization and transfer learning methods were used to enhance the accuracy of the proposed method in the case study. The application on synthetic models and field study substantiate the validity of the developed PSPU-Net as an effective tool for recovering basement relief from gravity data.
IG04-A014
RefinedBathyGAN: An Improved Deep Learning Based Super Resolution for Bathymetry - Evaluation and Sensitivity Analysis on Model Applications
Jose Marie Antonio MIÑOZA1,2#+, Vena Pearl BONGOLAN3,4, James GOFF5, Nigel WINSPEAR6, James TERRY7
1Center for AI Research, 2University of the Philippines Diliman, 3De La Salle University Manila, 4AI4PEP Philippines, 5University of New South Wales, 6CATRISX Services Ltd, 7Zayed University
Bathymetry is an essential factor when developing simulation models for geophysical phenomenon, given that the coarseness of how it is represented has significant effects on model accuracy. This study proposes an improved super resolution model to enhance bathymetry, by factor of two and four. These models outperformed the existing methods in terms of performance metrics such as Mean Squared Error (MSE), Peak Signal-to-Noise Ratio (PSNR), and Structural Similarity Index (SSIM). As the deep learning model able to preserve the bathymetric structure, this study also attempts to evaluate the effect of these newly introduce techniques when applied to actual numerical models through conducting sensitivity analysis on two case studies: Tohoku 2011 and Chile 2010 tsunami events. The findings could shed light on the effectiveness and potential applications of the proposed GAN model in refining bathymetric resolution for diverse scenarios, thus contributing valuable insights to the field of oceanographic research and modeling.
Session Chair(s): Taejin PARK, NASA Ames Research Center
IG01-A024
Downscaled 21st Century Global Fire Weather Projections
Taejin PARK1#+, Weile WANG1, Bridget THRASHER2, Hirofumi HASHIMOTO3, Andrew MICHAELIS1, Maria MADRAZO4, Hugo LEE5, Ju-Mee RYOO1,6, Sepideh KHAJEHEI1, Tsengdar LEE7, Ramakrishna NEMANI1, Ian BROSNAN1
1NASA Ames Research Center, 2Climate Analytics Group, 3California State University Monterey Bay, 4NASA Jet Propulsion Laboratory, 5Jet Propulsion Laboratory, California Institute of Technology, 6Bay Area Environmental Research Institute, 7National Aeronautics and Space Administration
Finer scale fire weather projections enable more effective planning, resource allocation, mitigation efforts, and public awareness to protect lives, property, and ecosystems in the face of increasing wildfire threats. In this presentation, we report on a new dataset that provides global fire weather projections derived from downscaled (0.25°) and bias-corrected daily Earth System Model (ESM) simulations. The dataset uses the Canadian Forest Fire Weather Index System framework to estimate fire danger by considering the effects of fuel moisture and wind on fire behavior and spread. It includes retrospective (1950-2014) and prospective (2015-2100) simulations from 33 ESMs. To make the dataset more accessible, the fire weather metrics are summarized at coarser temporal scales (monthly and annually), and source codes are provided for investigating daily fire weather. Multi-Model Ensemble data of monthly and annual fire weather metrics are also provided. This publicly available 5.1 TB dataset has the potential to be broadly used in not only for wildfire risk assessment but also for various future climate change impact assessments and preparedness.
IG01-A025
Post-wildfire Assessment: Temporal Analysis of Burned Area Spread and Withered Tree Estimation Using Harmonized Landsat and Sentinel-2
Seoyeong KU1+, Seunghyun HWANG1, Jongjin BAIK1, Hoyoung CHA2, Hyochan KIM1, Jeemi SUNG1, Changhyun JUN2#
1Chung-Ang University, 2Korea University
Wildfire-Affected Tree Withering is the process by which a tree withers over a long period of time after a wildfire, without being directly burned. Remote sensing is the most common method of indirect survey, as field surveys are difficult due to socioeconomic losses. As withered trees can be difficult to differentiate from seemingly live trees, relying solely on satellite data immediately after a wildfire may result in misclassification as unburned. Failure to manage withered trees could render the area susceptible to landslides and chain damage. Therefore, it is crucial to conduct continuous monitoring to detect and analyze changes in the burned area. This study examines the change in burned area over time following wildfire extinguishment and estimates the withered area using a high-resolution satellite dataset. For detecting burned area during 2017 to 2022 in South Korea, we utilized Normalized Burn Ratio, Normalized Difference Vegetation, Normalized Difference Soil Index, and Normalized Difference Water Index using Harmonized Landsat and Sentinel-2 for a total of one year at one-week intervals starting immediately after the wildfire. We considered the optimal model based on machine learning for estimating binary classification of the burned and unburned areas. Finally, we estimated the withered area of wildfire-affected trees by defining the expended burned area compared with the previous time, and also analyzed the changes in the burned area during the study period. Based on these result, it is clear which areas have withered and are vulnerable to chain damage from wildfires. This information can aid in rational decision-making for restoration planning. This research was supported by Korea Environment Industry & Technology Institute (KEITI) through Water Management Innovation Program for Drought (RS-2022-KE002032) funded by Korea Ministry of Environment and by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. RS-2023-00250239 & No. NRF-2022R1A4A3032838).
IG01-A004
Impact of Climate Factors on Vegetable Prices in China
Yun QIU1+, Jin-Soo KIM2#
1City University of Hong Kong, 2Korea Advanced Institute of Science and Technology
Climate extreme events have led to a global decline in vegetable production, often leading to elevated prices. Given that China accounts for half of the world's overall vegetable production, changes in its vegetable prices can substantially impact international food security. Here, we analyze the relationships between vegetable prices and climate factors across China. Our findings reveal a high correlation, particularly for temperature in the cold season, that low temperature increases vegetable prices, especially in southern China. However, seasonal precipitation anomalies do not significantly correlate with vegetable prices. Therefore, vegetable prices in winter and spring have strong variations as compared to summer and autumn due to cold extremes, which play as a key driver of the reduction in vegetable production, modulating vegetable prices. Such vegetable price fluctuations can further pose health concerns related to inadequate vegetable consumption. Therefore, these results highlight seasonal temperature prediction and long-term temperature projection to secure better vegetable production, essential for achieving food security and minimizing economic losses.
IG01-A009
Built-in Natural Defence Mechanisms in Tress : A Lesson from the Study of Tress
Narayan Prasad DEWANGAN1,2#+, Pratibha DEWANGAN3, Pranay DEWANGAN4
1Chhattisgarh Government, 2Chhattisgarh Swami Vivekanand Technical University, 3Government College of Teachers Education, 4GAIL India Limited
The defence system and mechanism are already built in the Trees as against the natural disasters and the human invasion. Trees are very intelligent in the survival struggle in the Darwinian sense and in this survival process it has learnt well & built in the natural defence mechanism. Trees communicate signals against environmental changes and threats to its community and they also feel like as if other living beings. Typical examples are shedding the leaves in winter to reduce the area exposed to cold atmosphere in winter and excreting bitter chemicals to repel to the insects attracted to it in search of the food and some species of tree have well developed fungal system in the root zones which are responsible for the transferring information of danger to tress in the community. That’s why they are said stationery life form on earth and have emerged as the most vital organ of the earth and supporting diverse form of life on earth. It has taught us not independency but the interdependency for mutual advantage and growth of ecological diversity on the planet Earth.
IG01-A027
| Invited
A Deep Learning Method for Peak Storm Surge Prediction
Zekai NI1#+, Wen ZHOU2
1City University of Hong Kong, 2Fudan University
Storm surges, typically referred to as the abnormal rising of seawater caused by tropical cyclones (TCs), pose significant threats to coastal regions, can result in severe damage to infrastructure, casualties and property losses in coastal region. While high-resolution hydrodynamic numerical models for storm surge prediction are well-developed, their computational expense and complexity render them infeasible for real-time, rapid forecasting and large-scale risk assessment. In this regard, neural network-based AI models offer a promising alternative, boasting unrivaled speed advantages intrinsic to data-driven prediction models. Our research introduces a novel deep learning model based on a hybrid Convolutional Neural Network (CNN) and Long Short-Term Memory (LSTM) algorithm for forecasting peak storm surges. The model utilizes a storm surge dataset created from SCHISM simulations of thousands of synthetic and historical TCs. Comprising three main components: a wind field encoder, a bathymetry encoder, and a Multilayer Perceptron (MLP), The model takes as input a time series of TC wind fields and multi-resolution bathymetric data around a coastal location, and outputs the peak storm surge of the location within a TC event. The model was trained on synthetic surge data and validated against historical TC events, demonstrating a RMSE of < 0.15m for peak surge predictions. Interpretability analysis of the model highlighted the potential of the bathymetry encoder in identifying locations prone to storm surge impacts. Beyond coastal stationary storm surge risk assessment, our model shows promise for rapid predictions of storm surge risk variations due to climate change. This work contributes to the existing body of knowledge by providing a efficient forecasting tool and opens avenues for enhancing real-time decision-making processes in the face of natural hazards.
Session Chair(s): Dmitri KONDRASHOV, University of California, Los Angeles
IG04-A001
AI in the Geosciences: Revisiting Geological Maps
Mark LINDSAY#+, Rebecca MONTSION, Lequn ZHANG, Yufu NIU, Sandra VILLACORTA
Commonwealth Scientific and Industrial Research Organisation
Geological maps are invaluable tools that provide essential information to understand and navigate the complexities of the Earth. Maps describe the distribution and relationships of rock types, structures, and other relevant features on or beneath the surface. These maps are often multi-purpose and instrumental in communicating complex interpretations in geology, environmental science, engineering, natural resource management, and land-use planning. Geological maps express the Earth as classes representing multivariate physical properties, providing a convenient summary to aid human understanding and thus simplifying the rich diversity of Earth's properties. However, the inherent uncertainty in maps regarding where and how observations are made is rarely quantified or qualitatively communicated. In addition, most map series are supplied in scale increments (e.g. 500 000, 250 000, 100 000, 50 000) with a commensurate increase in stratigraphic detail with smaller scales. As such, rock unit boundaries tend to change geometry and location with additional detail and smaller scales as an unintended artefact and source of error. This presentation will explore the concept of geological maps and propose AI-compatible, uncertainty-aware, multiscale property-based representations that have the potential to make the best of the underlying data and knowledge integral to map creation.
IG04-A029
Promote Scientific Data Sharing for the World’s Third Pole
Xin LI#+, Xiaoduo PAN, Ming FENG
Chinese Academy of Sciences
The Tibetan Plateau, also known as the world’s Third Pole, holds immense significance in the global context, influencing climate patterns, water resources, and biodiversity across Asia and even the globe. Scientific data related to the Tibetan Plateau is crucial for understanding of the complex interactions among its lithosphere, hydrosphere, cryosphere, biosphere, atmosphere, and anthroposphere. By promoting and sharing scientific data of the Third Pole, the international scientific community can contribute to the understand and preservation of this vital region and its far-reaching implications for the Earth system. The National Tibetan Plateau/Third Pole Environment Data Center (TPDC, https://data.tpdc.ac.cn) is one of the first 20 national data centers endorsed by the Ministry of Science and Technology of China in 2019. The TPDC is dedicated to consolidating and integrating extensive data resources of the Tibetan Plateau. The data center is featured by the most complete scientific data for the Tibetan Plateau and its surrounding regions, and is hosting more than 6,300 datasets collected from diverse disciplines, covering terrestrial surface, human-nature relationship, atmosphere, solid Earth, cryosphere, remote sensing, paleoenvironment, and others. The TPDC provides a cloud-based platform with integrated online data acquisition, quality control, analysis, and visualization capability to maximize the efficiency of data sharing. TPDC complies with the “findable, accessible, interoperable, and reusable (FAIR)” data sharing principles and strengthens its cooperation with international organizations, such as collaborating with WMO to promote the Global Cryosphere Watch project. It also collaborates with the ICIMOD on data exchanging, observation capability, capacity-building, and joint research. As a recommended data repository for international journals like Nature, AGU, ESSD, and Elsevier to encourage data authors to share their data along publications. Additionally, the TPDC provides data support for various international science programs, including TPE, GEWEX/GASS LS4P and WCRP-CORDEX CPTP.
IG04-A023
Retrieving Wind Wave Characteristics from X-band Navigation Radar Imagery Using Artificial Neural Networks
Mikhail KRINITSKIY1,2#+, Viktor GOLIKOV2, Vadim REZVOV2, Alexander GAVRIKOV3, Mikhail BORISOV2, Alexander SUSLOV3
1Shirshov Institute of Oceanology, Russian Academy of Sciences, 2Moscow Institute of Physics and Technology, 3Russian Academy of Sciences
Marine radars are vital for safe navigation at sea, detecting vessels and obstacles. Sea clutter, caused by Bragg scattering, is usually filtered out as noise. It becomes detectable in unfiltered radar images, acquired using SeaVision hardware package, when wind speed and wave height exceed certain thresholds. The characteristics of wind-induced ocean waves can be determined using these images. There are studies demonstrating this capability since 1964. However, traditional spectral methods for obtaining wave characteristics face limitations in improving accuracy. Deep learning techniques offer advantages in image processing tasks, being more robust and able to handle noisier data, yet delivering the results without Fourier transformations and not necessarily requiring long series of radar imagery. In our report, we present the method exploiting convolutional neural networks (CNNs) for estimating wind wave characteristics from shipborne radar imagery captured using SeaVision package. In particular, we train our CNN to infer significant wave height using estimates provided by the Spotter buoy as ground truth. Since the Spotter buoy measurements are costly and time consuming, we also demonstrate the capabilities of preliminary training of a CNN which improves generalization ability and overall quality of the acquisition of wind wave characteristics. Our CNN-based method has an advantage over the classical methods due to the low requirements for radar image data since we process just one SeaVision snapshot, whereas classical method requires more than 20 min of radar images.
IG04-A033
Using Machine Learning Approaches to Explore the Nonlinear Responses of Stomatal Conductance to Air Temperature
Hongmei LI#+, Gang ZHAO, Wenpeng XIE, Roman OLSON, Kei YOSHIMURA
The University of Tokyo
Stomata, the tiny cell-size pores on the leaf surfaces, serves as the key channel for global water and carbon flux in the land-atmosphere system. Specifically, when stomata open, atmospheric CO2 is absorbed by plants for photosynthesis, while inside water vapor escapes into the atmosphere through transpiration. Among the environmental factors, air temperature stands out as one of the most influential elements impacting various physiological processes in plants. However, the responses of stomatal conductance to air temperature have not been thoroughly explored. Most previous studies hold that stomatal conductance increases with temperature. This conclusion is only obtained under certain environmental conditions. There is still a lack of previous studies on stomatal response to air temperature under different environmental conditions. Here, we use machine learning methods to overcome this challenge. Specifically, three machine learning approaches (Deep Neural Network (DNN), Random Forest, and Support Vector Machine) and three physical models (Ball-Berry, Medlyn, and Eller model) are used to predict stomatal conductance and compared with observation. DNN shows a better performance than the other 5 models. Therefore, two post-interpretation techniques (Permutation Feature Importance (PFI) and Accumulated Local Effect (ALE)) are used inside DNN to explore how stomatal conductance responds to each environmental driver and how stomatal conductance responds to air temperature under different environmental conditions. PFI shows air temperature plays a most important role in stomatal conductance prediction. ALE represents that the stomatal aperture increases with rising air temperature under favorable environmental conditions. However, when plants experience water stress (high vapor pressure deficit and low soil water potential) and leaf temperature surpasses a threshold (20℃), stomatal conductance will decrease with rising air temperature. This research improves the understanding of the complex interplay between air temperature and other environmental drivers in regulating stomatal behavior and plant physiological responses.
IG04-A017
Spatiotemporally Consistent Global Dataset of the Fraction of Absorbed Photosynthetically Active Radiation (GIMMS FPAR4g) for 1982-2022
Weiqing ZHAO+, Zaichun ZHU#, Sen CAO
Peking University
The fraction of absorbed photosynthetically active radiation (FPAR) is an essential biophysical parameter that characterizes the structure and function of terrestrial ecosystems. Multiple long-term satellite-derived FPAR products, especially the 30-year+ GIMMS FPAR3g data, supported many in-depth insights into how terrestrial ecosystems interacted with global environmental changes. However, recent evaluation studies have pointed out notable discrepancies between the existing FPAR datasets and temporal inconsistencies within each product, there is a pressing need for satellite-derived FPAR datasets that offer consistent spatiotemporal insights and can be validated across their entire duration. Here, we used 4.6 million high-quality Landsat FPAR reference samples and the PKU GIMMS NDVI to develop a global FPAR dataset for half-month intervals at a spatial resolution of 1/12° from 1982 to 2022 using Back Propagation Neural Network (BPNN). Our dataset demonstrates a commendable Mean Absolute Percentage Error (MAPE) of 7.1% against Landsat benchmarks, comfortably meeting the 10% standard the Global Climate Observing System (GCOS) set. Comparisons of this dataset with ground-based measurements suggest root mean square error (RMSE) ranging from 0.11 to 0.14 with R-squared (R2) ranging from 0.79 to 0.84. Owing to its remarkable spatiotemporal coherence and continuity, the new generation of the GIMMS FPAR dataset promises to be a valuable asset for in-depth analyses of vegetation structures and functions spanning the last 40 years.
Session Chair(s): Fei CHEN, National Center for Atmospheric Research , Xiaoming SHI, The Hong Kong University of Science and Technology, Laurence DELINA, The Hong Kong University of Science and Technology
IG31-A008
Evaluating Social Resilience in the Guangdong-Hong Kong-Macau Greater Bay Area: A Case Study of Flood-prone Communities in Hong Kong and Zhuhai
Qingqing FENG+, Ji CHEN#
The University of Hong Kong
The Guangdong-Hong Kong-Macau Greater Bay Area (GBA) is no stranger to the challenges posed by heavy rainfall and severe floods, as witnessed on September 8, 2023, when a torrential downpour struck Hong Kong, resulting in a maximum hourly rainfall of 158.1 mm and direct economic losses exceeding HKD 2.8 billion. In this monsoon-dominated region, including Hong Kong and Zhuhai, flooding incidents are recurrent, emphasizing the need for a comprehensive evaluation of the social resilience of flood-prone communities. Focusing on Hong Kong and Zhuhai, two key cities within the GBA, this study aims to evaluate their ability to adapt, recover, and withstand disruptions caused by floods. To achieve this, a conceptual indicator-based framework will be proposed for assessing flood-prone community social resilience tailored to the unique characteristics of the GBA. To gather empirical data, the study will delve into the surrounding communities of 72 identified internal flooding risk points in Zhuhai (as identified by the city's Water Affairs Bureau in 2022) and 4 flooding blackspots in HK (newly reviewed in 2023 by the Hong Kong Drainage Services Department). By comprehensively evaluating the social resilience of flood-prone communities in both cities, the findings of this research may contribute valuable insights into the factors influencing community social resilience to flooding, ultimately assisting in the formulation of effective strategies for enhancing community preparedness and response in the face of recurrent flood events in the GBA.
IG31-A009
Generation of Future Typical Meteorological Year Datasets for Major Cities in Indonesia
Vinayak BHANAGE1#+, Han Soo LEE1, Tetsu KUBOTA1, Radyan Putra PRADANA1,2, Faiz Rohman FAJARY1, Hideyo NIMIYA3, I Dewa Gede ARYA PUTRA2
1Hiroshima University, 2Indonesian Agency for Meteorology, Climatology and Geophysics, 3Kagoshima University
Efficiently assessing the impact of climate on energy consumption in buildings is vital. Accurate information on the Typical Meteorological Year (TMY), representing typical hourly weather conditions throughout the year, is essential. This study focuses on generating future TMY datasets for major Indonesian cities, considering potential climate changes in four variables: surface air temperature, wind speed, relative humidity, and precipitation. The process involves identifying city-specific global climate models and calculating bias-corrected projections for monthly climate variations for the next four decades (2021-2060) under high-emission scenarios. Following this, the morphing technique has been employed to integrate the projected climatic changes into the existing TMY data (2011-2020), creating future TMY (FTMY) datasets. The resulting trends in FTMY exhibit a high correlation (>0.5) with the long-term averages of the respective climatic variables for all cities. Comparative analysis of current and FTMY data reveals a future increase of 1 to 3°C in surface air temperature for all selected cities. Significant perturbations are noted in precipitation and relative humidity, while minimal changes occur in wind speed. This investigation aims to guide the development of future weather datasets for building design, contributing to the advancement of sustainable cities.
IG31-A002
Intensified Landslide Risks in the Cities Over Complex Terrain Due to Global Warming
Xiaoming SHI1#+, Jianan CHEN2, Yang LIU1, Haoming CHEN1, Yueya WANG1, Jimmy Chi Hung FUNG1, Charles Wang Wai NG1, Zhongming LU1, Ruo-Qian WANG3
1The Hong Kong University of Science and Technology, 2The University of Hong Kong, 3Rutgers, The State University of New Jersey
Tropical cyclones (TCs) are expected to produce more intense precipitation under global warming. However, substantial uncertainties exist in coarse-resolution global climate models' predictions. Here, we use deep learning to aid targeted cloud-resolving regional simulations of extreme TC cases. Contrary to the Clausius-Clapeyron (CC) scaling, which indicates a 7% moisture increase per K warming, our simulations reveal more complex responses of TC rainfall. TCs will not intensify via stronger updrafts but through increased compactness and continuity in the organization of convective cores. Consequently, while localized hourly rainfall may adhere to the CC scaling, precipitation accumulation over city-sized areas could surge by 18%K-1. This super-CC intensification due to changing TC structure has profound implications for flood and landslide risks. Estimations using Hong Kong's slope data confirm this concern and suggest an up to 215% increase in landslide risks with 4-K warming, highlighting amplified threats from compound disasters under climate change.
IG31-A006
Adapting to More Severe Tropical Cyclone Hazards in the Pearl River Delta Region: An Air-wave-ocean Coupled Model Study
Zhenning LI#+, Jimmy Chi Hung FUNG, Mau Fung WONG, Alexis K.H. LAU
The Hong Kong University of Science and Technology
This study examines the impact of tropical cyclones (TCs) on the Pearl River Delta (PRD) coastal regions, which are highly vulnerable to TC-caused coastal hazards due to their long and meandering shoreline and well-developed economy. The study uses a sophisticated air-wave-ocean coupled model of high spatial resolution to reproduce 11 intense landfalling TCs since 2000 and compare their impact driven by present-day reanalysis data and a pseudo-global warming scenario projection for the 2090s. Results indicate that the 2090s thermodynamic status effectively increases the intensity of these TCs, leading to more severe coastal hazards including gale, rainstorm, and storm surges and waves. Except for the maximum surface wind speed and the accumulated rainfall increase, the most striking change that the community needs to adapt to is that a combination of mean sea level rise, storm surge, and wave height can reach more than a 300 cm increase in total water level at certain hot-spot coastlines, without considering the superposition of spring tides. Land reclamation, such as the artificial islands proposed by the "Lantau Tomorrow" vision in Hong Kong, is also investigated and found to effectively redistribute the storm surge water levels. This study provides valuable information for policymakers and stakeholders to guide climate adaptation and resilience usage in the PRD region and other related regions that are vulnerable to TC-caused coastal hazards.
IG31-A001
Study of Kidney Diseases in Relation to Extreme Heat for Atlanta Metropolitan Region
Tzu-Shun LIN1#+, Andrew NEWMAN1, Cenlin HE1, Fei CHEN2
1NSF National Center for Atmospheric Research, 2The Hong Kong University of Science and Technology
High temperature has been found to likely raise the risk of acute kidney injury, which is characterized by a precipitous decline in kidney function. Traditionally, kidney diseases in heat exposure have been investigated using ambient temperature data collected from individual monitoring stations or spatially gridded atmospheric reanalysis products. These datasets cannot capture heat exposures in urban areas characterized by heterogeneous fine-scale urban heat island with significantly higher temperature than surrounding rural areas, which can amplify extreme heat events in cities and disproportionately affect public health. Here, we first develop a 1-km spatial resolution regional climate dataset for 2013–2021 using a fully coupled atmosphere-land-urban modeling system, WRF-Urban, over the Atlanta metropolitan area with high-resolution maps of urban land-use types from the Local Climate Zone (LCZ). After evaluation, the bias in WRF-Urban simulated temperature fields is corrected using in-situ observations and machine learning models such as artificial neural networks and decision tree algorithms. The results demonstrated the ability of the WRF-Urban model in reproducing the observed extreme high and low surface-air 2-m temperature in urban areas by utilizing the LCZ maps, which seem to better specify various urban land-use types in the region of interests. Furthermore, temperature bias is effectively mitigated by employing machine learning approaches. The dataset will be used to quantify relationships between short-term heat exposure and hospitalizations for acute kidney injury in Atlanta area hospitals, as well as to offer inputs for quantitative risk assessment and economic evaluation of heat-health implications that can improve case management decisions.
IG31-A004
Extreme Heat Risk, Impacts, and Adaptation Strategies in Southeast Asia’s Megacities: A Bibliometric and Thematic Analysis
Sharon Feliza Ann MACAGBA#+, Laurence DELINA
The Hong Kong University of Science and Technology
This presentation examines the existing literature on extreme heat in Southeast Asia’s mega-urban areas, with a particular focus on the social and well-being risks and impacts on vulnerable populations, as well as the strategies to adapt and mitigate these risks, using bibliometric and thematic analysis. Our findings indicate that most literature on extreme heat in cities measures urban heat using different assessment tools, such as canopy urban heat island, land surface temperature, and using satellite images like MODIS. Some studies concentrate on the factors contributing to urban heat and its impacts, while others relate urban heat to spatial factors, such as land use changes, land use expansion, and urbanization. Population growth and increased energy consumption are also identified as factors exacerbating urban temperature. Although these studies concentrate on urban heat, research on its impacts to vulnerable populations usually relates to human systems and socio-economic conditions. Mental and social well-being are also mentioned in the literature discussing the impacts of extreme heat. Strategies to address the impacts of extreme heat on the mental and social well-being emphasize the need for green infrastructure and spaces, as well as well-designed and valued places. We found the need to enhance urban planning and design in cities, including the provision of amenities for urban heat adaptation approaches that simultaneously consider and include at-risk lower-income communities.
IG31-A012
Evaluation of Human Thermoregulatory Responses During Transitions Between Conditioned Indoor Spaces and Outdoor Environments
Devi S#+
Indian Institutes of Technology
This study investigates the impact of environmental temperature changes on thermal responses during the transition from conditioned indoor spaces to outdoor environments. The objectives of the study include the evaluation of the outdoor environments through field experiments; evaluation of the thermal responses through analytical studies and deducing the strategy for minimizing the thermal stress due to thermal perturbations. The paper is based on experimental field analysis of thermal sensation and comfort conducted in three metro stations in Delhi, India, representing a humid subtropical climate. Three metro stations are chosen based on factors such as commuter traffic, location, and area have their environmental characteristics measured. Four different days were selected based on Indian meteorological weather data (IMD) to represent four different weather conditions of the climatic region. Eight transient scenarios are considered on the selected days. Under these scenarios bioheat transfer model is used to analyse thermal stress and the sensory feedback during temperature shifts from +15°C to -15°C. We observed that the decrease of environmental temperature by -15°C prompts a 3-4°C reduction in regional skin temperatures. Cold receptor response decreases, and warm receptor response remains relatively stable. The neuronal discharge rates associated with cold impulses increase during this transition. Interestingly, variations in neuronal responses are observed, with decreasing rates as conditioned space temperature rises. Warm receptors vary from 0.5-2°C during the transition, indicating a subtle sensitivity to warm stimuli and heightened sensitivity to cold stimuli. The study provides a quantitative understanding of the neurophysiological mechanisms involved in thermal sensation, offering valuable insights into the dynamic nature of thermal perception, thermal perturbations and thermal stress during transitions.
IG31-A005
Integrated Policy and AI-assisted Technology Responses to Extreme Heat in Urban Southeast Asia
Laurence DELINA, Johanne CASTRO#+
The Hong Kong University of Science and Technology
Cities grapple with extreme heat as urban expansions exacerbate the urban heat island effect and extreme temperatures due to accelerating climate change. In response, cities implement policies to mitigate the impact of extreme heat, including increasing public awareness and strengthening adaptive capacities. Cities also employ artificial intelligence (AI)-assisted technologies to forecast heatwaves, develop evidence-based mitigation strategies, and optimize infrastructure construction to anticipate and address these impacts. While studies have quantified these impacts, identified vulnerabilities and risks, and evaluated and projected the outcomes of implementing adaptation and mitigation measures using AI-assisted technologies, these studies have primarily focused on cities in developed regions, such as the United States, Europe, and Australia. Research has also been sparsely conducted on the synergistic impacts of policy and AI-assisted technology responses to extreme heat. In order to address these gaps, this talk focuses on Southeast Asian cities, reviewing studies on integrated policy and AI-assisted technology responses to reveal strategic approaches and relevant actors to extreme heat impacts, adaptation, and mitigation. The review provides insights into future research needs to bridge the geographical gaps in urban overheating studies and policy-and-AI-assisted technology integration in cities.
Session Chair(s): Abang Mansyursyah Surya NUGRAHA, Nanyang Technological University, Amy GOUGH, Heriot-Watt University
IG09-A001
Cenozoic Multi-source-to-sink in the Barents Sea
Amando LASABUDA1,2#+
1The University of Sydney, 2University of Oslo
Multi-source-to-sink scenario would involve uncertain relative sediment input estimates from different source areas. This variation in sediment supply and discharge will have direct consequences on simulating basin filling over time and on reconstructing sedimentation pattern, which are useful to explore frontier basins. The Barents Sea is a unique multi-source-to-sink setting with complex tectonic and climatic history particularly in the Cenozoic (the last 66 Ma). The northwestern part of the Barents Sea area was subjected to major plate compression and subsequent rifting relative to the Greenland plate movement, while the southwestern part is more dominated by rifting episodes. To the north, the Barents Sea experienced transform plate movement with the Lomonosov Ridge and rifting. Both margins are characterized by seafloor spreading during the development of oceanic basins. The Barents Sea has also experienced episodic subsidence and uplift, and glacial erosion and isostatic rebound due to northern hemisphere glaciations. We applied numerical source-to-sink modelling to disentangle intricate relationship between tectonic and climatic forces, and their impact on the corresponding spatio-temporal sediment input and distribution in basin filling. We attempt to model plausible sediment routing based on paleogeographical reconstructions of the Barents Sea during the Cenozoic. Sedimentation pattern model will be calibrated with seismic and well data, and provenance analysis in terms of sediment thickness, seismic geomorphology and lithological control. This study will contribute to the enigmatic research question on the timing of opening of the Barents Seaway in the Cenozoic that connected the Atlantic and Arctic oceans.
IG09-A005
| Invited
How Do Climatic Changes Affect Sediment Density Flows? Insights from the Dead Sea Deep Drilling
Yin LU1#+, Edward POPE2, Jasper MOERNAUT3, Revital BOOKMAN4, Nicolas WALDMANN4, Amotz AGNON5, Shmuel MARCO6, Michael STRASSER3
1Tongji University, 2Durham University, 3University of Innsbruck, 4University of Haifa, 5Hebrew University of Jerusalem, 6Tel Aviv University
Sediment density flows (including flood plumes, turbidity currents, and debris flows) are major processes for transporting sediments and organic carbon from rivers, coasts or continental shelves into deep basins. These flows can also have serious socioeconomic consequences such as breaking seabed communications cables and pipelines. Given the potential impacts of climate change, it is important to quantify how sediment density flow processes are impacted by changing environmental conditions. However, it is unclear whether, and if so how, long-term climate changes affect the magnitude/frequency or type of sediment density flows within a specific water body. One approach to answering this question is to analyze a comprehensive geological record that comprises deposits that can be reliably linked to modern sediment flow processes. To address this question, we analyzed an unique ICDP deep core from the Dead Sea depocenter covering MIS 7-1. Based on an understanding of modern sediment density flow processes in the lake, we link homogeneous muds in the core to overflows (surface flood plumes), and link graded turbidites and debrites to underflows. Our dataset reveals (1) overflows are more prominent during interglacials, while underflows are more prominent during glacials; (2) orbital-scale climate changes affected the magnitude/frequency of the flows via changing salinity and density of lake brine and lake-level (Lu et al., 2022). The current research bridges the gap between our understanding of modern sediment density flow processes and deposits preserved in a long-term geological record in the Dead Sea, a tectonically active subaqueous environment (Lu et al., 2020). It has wider implications for turbidite paleoseismology and paleoclimate research in a tectonically active subaqueous environment.
IG09-A015
Unlocking Ancient Landscapes: How Extensive Source-to-sink Datasets Can Aid in Reconstructing Southeast Asia's Regional Palaeogeographies
Amy GOUGH#+, Max WEBB
Heriot-Watt University
Understanding past plate tectonic configurations, palaeoenvironments, and resultant lithofacies relies heavily on palaeogeographical reconstructions. In tectonically active and tropical regions, such as SE Asia, complexities arise, making these reconstructions challenging compared to more stable regions like North America. Challenges include the vast geographical extent, inaccessibility of large areas, poor exposure due to weathering, destruction of the geological record through subduction, and variability in the density of available literature. Despite these obstacles, the deep basins formed during the Cenozoic, coupled with high sedimentation rates, have remarkably preserved the sedimentary record of SE Asia and present-day exposure provides valuable data for comprehending basin evolution and palaeogeographic changes through time. A key method to overcome these obstacles is to use a data-heavy approach to these reconstructions, using source-to-sink provenance studies to investigate hidden clues in palaeo-terrane models, depositional routing pathways, and climate, all allowing for accurate reconstructions to be made. This work relies on databases of provenance data collected by the Southeast Asia Research Group (SEARG) over the last 40 years. These data include light mineral counts (851 samples), heavy mineral counts and ratios (408 samples), U-Pb zircon ages (581 samples), and foraminifera (1092 samples). The databases have been compiled into geological road maps, creating a spatial model that integrates field observations, structural measurements, lithological descriptions, and interpretations. The comprehensive dataset is reinforced by a repository of over 10,000 hand samples and 8,000 thin sections, alongside other published literature. This collective resource empowers us to adopt a data-driven approach, enabling a comprehensive evaluation of the onshore geology in Southeast Asia. Using this data, new palaeogeographic maps for the Cenozoic are presented to highlight how much information can be extracted from source-to sink-studies, and how this information can be used to reconstruct the regional past depositional environments of SE Asia.
IG09-A014
Sedimentary Provenance of the Cenozoic Deposits of Natuna Island, Indonesia: Implications for Onshore to Offshore Correlation and CCS in Sundaland
Max WEBB1#+, Amy GOUGH1, Ferdi ENDINANDA2
1Heriot-Watt University, 2Perenco
The benefits of onshore analogue studies for understanding the stratigraphy of offshore basins have long been known and used as a way of determining depositional pathways and environments. Onshore studies are of particular importance in SE Asia, where the links between onshore and offshore geology can be observed in present day systems as well as in the geological record. Few locations in SE Asia exemplify this intrinsic relationship more than the island of Natuna, off the northwest coast of Borneo. Natuna lies within the Indonesian Riau Archipelago, South China Sea and sits atop the Natuna Arch, a structural high that straddles the East and West Natuna basins, representing a type example of how we can use fieldwork campaigns to better understand subsurface geology. This research records a well preserved source-to-sink package, including an uplifted granitic basement that eroded into interbedded conglomerates and quartz-rich sandstones that were deposited in deltaic and paralic environments throughout the Cenozoic. U-Pb zircon geochronology, heavy minerals, and light minerals record dominantly local sourcing for Cenozoic sediments in the region with periodic influx of more diverse sources during the post-rift basin interlinkage phase (e.g., the Peninsular Malaysia and West Borneo). Uplift of the Natuna Arch during the two basin inversion events since the Oligocene has led to the erosion of the granitic basement into a series of sandstones and overlying siltstones that now form the lowlands of the island (the Raharjapura and Pengadah formations, respectively). These onshore sediments correlate directly in both age and sedimentology with Oligocene to Pliocene successions in the West and East Natuna basins that flank the island (e.g., the Grabus, Arang, and Muda formations). The exposure of these sediments onshore with direct access to their source material provides us with an unparalleled analogue for studying the potential for CCS projects in the subsurface.
IG09-A027
New Chronostratigraphic Constraints of Early-jurassic in the Northwestern Junggar Basin and Its Implications
Yangyang XIA1#+, Su-Chin CHANG1, Daran ZHENG2
1The University of Hong Kong, 2Chinese Academy of Sciences
The tectonic history of the northwest margin of the Junggar Basin is complex as multiple events occurred between the Carboniferous period and the early Jurassic. Despite many efforts, the tectonic evolution of this area remains controversial, mainly due to the need for reliable age determinations for critical formations. For example, the discovery of early Jurassic gray-green basalt and dark grey olivine basalt from the Wenzigou Formation in West Karamay provides evidence for understanding Mesozoic magmatic activity in northern Xinjiang. However, the previous age data for this formation obtained by different methods are inconsistent because of the significant uncertainties or poor sampling descriptions. Here, we present novel high-precision 40Ar/39Ar ages of 195.79 ± 0.48 Ma, 196.07 ± 0.50 Ma, and 197.40 ± 0.67 Ma for three basaltic samples from the Wenzigou Formation. Our study indicates that this formation is above the Triassic/Jurassic boundary. The new data will allow us to understand the geological background of this region further and provide reliable ages for correlating rocks from this critical formation and elsewhere.
IG09-A021
On Theoretical Longitudinal Profiles of Natural Rivers
Dongwoon KANG+, Kyungrock PAIK#
Korea University
Typical natural streams exhibit a concave-upward shape in their longitudinal profiles. Detailed shapes vary depending on factors such as flow discharge, sediment load, and the size of bed materials. Many studies have attempted to derive the profile as a functional form, on the theoretical basis. Here, we will first review existing analytical theories developed for detachment-limited and transport-limited streams. Importantly, the existing theory about the transport-limited stream is limited to a special case where bed materials are uniform in size. In fact, bed materials or grains with different sizes are mixed in nature, and their distribution varies dynamically over time together with the profile evolution. In this study, for the first time, we attempt to derive a functional form for the longitudinal profile of transport-limited stream with mixed grain sizes. We hypothesize that the threshold of motion which very differs between uniform vs. mixed size settings holds the key to determine the profile shape.
IG09-A006
Analysis and Prediction of Suspended Sediment Recession Curves
Laxmipriya MOHANTY1#, Basudev BISWAL2+
1Indian Institute of Technology Hyderabad, 2Indian Institute of Technology Bombay
River sediment load estimation has been increasingly important in recent days for several reasons, like predicting reservoir sedimentation, studying land erosion rates, and understanding sediment transport to oceans. To achieve this, sediment rating curve is the simplest technique to refer to instead of complex experimental procedures. The efficacy of rating curve estimation is based on the underlying physics behind the dynamic relationship between sediment and discharge. Current research is focused on understanding the dynamics across recession events followed by a decreasing trend of both concentration and discharge. Furthermore, we propose to express as a function of during the recession, where the exponent is assumed to vary with static catchment characteristics and the coefficient with dynamic factors. Hence, we propose that it is possible to predict a recession event considering past data, which can further predict for future days. The advantage of the proposed model is the prediction of future sediment concentration at a river cross section during a recession event. The performance of 35 US Geological Survey basins shows the 25th, 50th, and 75th values of NSE to be 0.55, 0.64, and 0.78, whereas the traditional Rating Curve method shows -0.05, 0.01, and 0.20, respectively. The results here signify the importance of recognizing the dynamic nature of relationships both along and across the recession.
Session Chair(s): Nan WU, Tongji University, Amando LASABUDA, The University of Sydney
IG09-A002
Assessment of Sediment Deposition and Shoreline Evolution at a Sandbar Port Breakwater: Two Case Studies in West Africa
Stephan LAWSON+, Keiko UDO#, Hitoshi TANAKA, Janaka BAMUNAWALA
Tohoku University
The sandbar breakwater is an innovative nature-based port solution, which addresses some aspects of the environmental, functional and financial constraints associated with conventional port breakwaters. Two newly constructed ports in West Africa are based on this concept due to the favorable unidirectional longshore sediment transport in this region. Hence, this study aimed to assess the impoundment of longshore sediment transport and shoreline evolution at the Port of Lomé, Togo and the Lekki Deep Sea Port (Dangote Sea Port), Nigeria. The shoreline positions were inferred from satellite images acquired before and after the construction of the ports. Upon calculating the rates of shoreline change, we estimated the volume of deposited sediment using the one-line coastline change model. Based on this approach, we found that the updrift shoreline at the study sites accreted between 10 – 23 m/year. Additionally, the estimated longshore sediment transport was in the magnitude of 1.0 – 7.0 ×105 m3/year. A comparative study at other locations along this coastline showed that the longshore sediment transport rate could further reach a magnitude of 106 m3/year. These rates are mainly influenced by the oblique waves approaching the coast coupled with sediment input from major rivers (in orders of 106 m3/year). These results also indicate that sediment availability within the West African coastal system is abundant and therefore, this innovative port solution could be adopted at other locations. However, coastal morphological changes could be enormous and detrimental to downdrift communities. As such, considerations for sustainable approaches to protect downdrift communities are vital for current and future developmental projects along the West African coastline.
IG09-A011
Contrasting Structural and Stratigraphic Aspects of the Western and Eastern Regions of the Singapore Strait – Results of Geophysical Data Interpretation
Abang Mansyursyah Surya NUGRAHA1#+, Stephen CHUA1, Andrew GREEN2, Uri SCHATTNER3, Yu Ting YAN1, Doug SLOGROVE2, Adam SWITZER1, Benjamin HORTON4,5
1Nanyang Technological University, 2University of KwaZulu-Natal, 3University of Haifa, 4City University of Hong Kong, 5Imperial
Previous studies have integrated field geology observations with borehole data to extrapolate basement stratigraphy and structures from onshore to offshore Singapore (Leslie et al., 2019; Dodd et al., 2019; Gillespie et al., 2019). However, the seabed and subsurface stratigraphy in the Singapore Strait are practically unexplored. Here, we present a detailed seabed relief and sub-bottom stratigraphic and structural record across most of Singapore's waters. A new interpretation of high-resolution seismic reflection and multibeam bathymetry data is proposed based on 567 line-km of geophysical data acquired across the Singapore Strait. Significant contrasts exist in the structure and stratigraphy of the western and eastern regions of the Singapore Strait, approximately partitioned at St. John Island. NE-SW and ENE-WSW-oriented faults and folds are observed from the seismic reflection profiles in the western region between St. John and Sudong Islands. The faults mainly intersect the Middle Triassic Jurong and Upper Triassic Sentosa groups. The preservation of the Quaternary sediments is limited in this region. In contrast, in the absence of the faults, the thick late Quaternary sequences are preserved in a network of buried channels in the eastern region. The Late Quaternary stratigraphic record includes five main stratigraphic units of fluvial-to-marine sequences. Major unconformities separate these units, probably associated with major sea-level lowstands. They are interpreted as being part of the Bedok Formation and Kallang Group. The younger deposits consist of unconsolidated sediment characterised by the amalgamation of climbing ripples and dunes to form sand ridges, as observed in sub-bottom profiles and bathymetry. These data provide evidence for long-lasting sea bottom currents in the area and are likely related to the drowning of the inner Sunda Shelf during the early Holocene. These new data underpin the importance of onshore-offshore geological models to our understanding of the evolution of both Singapore and the Singapore Strait.
IG09-A020
Anthropocene Environmental Change in the Singapore Strait: Insights from Offshore Sediments and Benthic Foraminifera
Yu Ting YAN1#+, Stephen CHUA2, Abang Mansyursyah Surya NUGRAHA2, Yuki SAWAI3, Yumi SHIMADA3, Toru TAMURA3, Benjamin HORTON4,5, Adam SWITZER2
1Earth Observatory of Singapore, 2Nanyang Technological University, 3National Institute of Advanced Industrial Science and Technology, 4City University of Hong Kong, 5Imperial
Rapid development in Singapore has led to substantial landscape changes over the past few decades, most notably in the southern coastal and offshore regions of the island in the Singapore Strait. Some major transformations in the area include land reclamation due to expansion of trade and commercial activities post-independence and the construction of the Marina Barrage and Marina Reservoir to safeguard Singapore water security in the 2000s. These landscape changes and their environmental impacts are likely to be documented in the sediment and fossil foraminiferal records. Foraminifera has been widely used for biomonitoring purposes and paleoenvironmental reconstruction due to their sensitivity to various environmental parameters and good preservation. To this end, sediment cores (~ 50 cm) have been collected from offshore Marina Bay where changes in foraminiferal communities were investigated downcore. Sedimentological and geochemical (e.g., XRF core scanning and bulk sediment δ13C) analyses were also conducted, and chronology is constrained by 210Pb dating. This work presents an examination on whether coastal development in southern Singapore over the last few decades has had any marked influence on nearshore marine sedimentation and aims to identify key foraminifera indicator species for understanding Anthropocene environmental change as well as biomonitoring purposes in Singapore.
IG09-A028
Jurassic Sedimentary Basin in Sri Lanka: Knowns and Unknowns
Su-Chin CHANG#+
The University of Hong Kong
Over 90% of Sri Lanka consists of high-grade metamorphic rocks, while a few sedimentary outcrops provide rare but significant information to reconstruct the paleoenvironments of this island nation. For example, the Jurassic strata from the Tabbowa Basin have allowed us to understand the Mesozoic world along the ancient margin of Gondwana. Since the early 20th century, abundant plants, including conifer, cycad, and fern, have been discovered in the Tabbowa beds. Additionally, diverse assemblages of insect trace fossils were found on the surface of these plant fossils, making it possible to discuss the plant-insect co-evolution further and the Jurassic ecosystems in general. However, the systematic study of these findings needs to be improved. Furthermore, the radiometric age determinations for these fossil-rich sedimentary rocks still need to be improved due to the limitations of suitable dating materials from this area. The long-term plan of this study is to conduct detailed geological, chronological, and paleontological investigations in the Tabbowa Basin. The result is expected to answer critical and fundamental questions, including the stratigraphic correlations among these Sri Lankan strata and other contemporaneous deposits in India and Australia and the post-Gondwana history of Sri Lanka.
IG09-A031
| Invited
Cretaceous Kachin Amber Biota from Northern Myanmar
Bo WANG1#+, Cihang LUO1, Han WANG2, Haichun ZHANG2
1Nanjing Institute of Geology and Palaeontology, Chinese Academy of Sciences, 2Chinese Academy of Sciences
Kachin amber (amber from northern Myanmar) contains the most diverse biota of all Cretaceous amber. During the last 100 years, Kachin amber has received worldwide scientific interest; more than 300 families of arthropods plus diverse plants and vertebrates have been reported. Kachin amber has been known for nearly 2000 years, and it has been traded with China since Han Dynasty times (202 B.C. to 220 A.D). The renaissance in Kachin amber research started at the very end of 20th century and the investigations on inclusions of Kachin amber are now in full bloom. We have re-investigated this biota based on new, abundant fossils and got some new and surprising discoveries. We found a number of arthropod groups that are rare or extremely rare in amber, e.g. crabs (Brachyura), camel spiders (Solifugae), whip-scorpions (Thelyphonida), and onychophorans (Onychophora). Insects are the most common group in Kachin amber and show a remarkable mixture of basal and derived forms. They document a particularly active time in the evolution of life on land, the Cretaceous terrestrial revolution. Flowering plants were flourishing and diversifying, the insects that fed on the flowers were also flourishing and diversifying, and the predators that fed on the insects (spiders, lizards, mammals, and birds) were flourishing and diversifying. The stories of plant, insect and other invertebrates, and predator interactions documented in Kachin amber offer an unprecedented view into the co-evolution of insects and plants, the evolution of pollination, adaptations to various types of food and habitats, and the formation of recent ecosystems and biotas. Although the list of exciting discoveries is long, only about 30% of the inclusions have been formally described from Kachin amber. Therefore the Kachin amber biota requires much more extensive and detailed taxonomic investigation.
IG09-A009
| Invited
Kinematics and Structure of Submarine Landslides: Insights from 3D Seismic Reflection Data
Harya Dwi NUGRAHA1,2#+, Christopher JACKSON3, Howard JOHNSON4, David HODGSON5
1University of Bergen, 2Universitas Pertamina, 3Jacobs, 4Imperial College London, 5University of Leeds
Mass-transport complexes (MTCs) are common features in deep-marine environments, and have been an efficient agent of sediment transport from their source to sink. Their emplacement can catastrophically displace sediment to continental slope and basin floor, and have a direct impact on society by generating tsunamis and destroying offshore infrastructure. The proliferation of high-resolution multibeam bathymetry and three-dimensional seismic reflection data have improved our understanding of their internal form and emplacement processes. However, uncertainties remain in terms of: (i) how the volume and flow behaviour of MTCs evolve during their translation, and what controls these changes; and (ii) how strain is distributed within MTCs, and its relationship to their internal architecture and geometry. To address these problems, three-dimensional seismic reflection, well, and bathymetry data from the Exmouth Plateau (the Gorgon Slide, offshore NW Australia) and the Makassar Strait (the Haya Slide, offshore Indonesia) are used. This study demonstrates that: (i) dynamic interaction between mass flows and substrate lead to the final volume is three times the initially evacuated volume on average, and the formation of intra-MTC flow cells that can translate with a different speed and runout distance; and (ii) strain distribution of an MTC is variable along strike, resulting in the variations of internal architecture and frontal geometry, partly controlled by the basal shear surface depth and morphology. This study shows that changes in MTCs volume and flow behaviour during transport from source to sink should be considered for geohazard and subsurface fluid system assessments.
IG09-A008
Headless Submarine Canyons and Their Feeding Fan Apron in the Lower Continental Slope to Abyssal Plain: A Case Study in the South China Sea
Biwen WANG1#+, Guangfa ZHONG1, Liaoliang WANG2, Min HE3, Benduo ZHU2, Huodai ZHANG2, Zhe WU3
1Tongji University, 2Guangzhou Marine Geological Survey, 3China National Offshore Oil Corporation
Headless submarine canyons represent the canyons confined in the continental slope with their heads detaching from the shore. Such canyons are understudied and generally considered to be dormant during high-stand sea levels, thus limited sediments can be transported into the deep sea. Herein, we report the Yitong submarine canyons – fan apron system (YCFS) in the northern South China Sea, which consists of a group of submarine canyons confined in the lower slope that are far away from terrigenous sediment sources, and a submarine fan apron in the abyssal plain. This system was studied by integrating multibeam bathymetric and two-dimensional multichannel seismic data, combined with International Ocean Discovery Program drilling data. The canyons exhibit erosion dominance, evident in their V-shaped cross-sections with incisions reaching depths of up to 708 meters. Canyon infillings consist of mass transport deposits and turbidites, while interfluves display characteristics like landslides, creep-typed sediment waves, and gullies, indicating the prevalence of mass transport and turbidity-current processes in both canyons and interfluves. The fan apron is predominantly depositional, featuring channels, channel-levee complexes, turbidite lobes, and mass transport deposits as the main depositional elements. In the canyon-to-fan transitions, supercritical turbidity current features and bedforms emerge, including plunge pools, connected sediment mounds, cyclic steps, and antidunes. These developments are associated with the deceleration and hydraulic-jump effects resulting from the shedding of high-velocity turbidity currents from the canyons. Late Miocene marked the initiation of YCFS, as uncovered by seismic stratigraphic analysis. The presence and persistence of YCFS are associated with the prolonged existence of an upslope margin-parallel basement high. This feature likely maintained a steep slope condition (up to 6.5◦), conducive to the formation of canyons and supercritical turbidity currents. The blocking influence of the basement high results in YCFS receiving a restricted supply of shallow-water sediments.
IG09-A022
The Interaction Process Among Channel Complexes, Mass-transport Complexes, and Turbidites: A Case Study from the Deepwater Taranaki Basin, NW New Zealand
Abi Dzikri ALGHIFARI#+, Nan WU
Tongji University
The Neogene and Quaternary sedimentary succession in the Taranaki Basin are marked by high sedimentation rates (30 to 45 cm/kyr), characterized by various depositional elements, including channel complexes, mass transport complexes (MTCs), and turbidites. Previous studies have investigated the distribution, triggers, and emplacement process of these depositional elements separately. However, the relationships between these elements, for instance, how older deposits impact subsequent sedimentation processes, has not been examined. In this study, we use high-resolution (c. 7 m) 3D seismic reflection datasets to investigate: i) how buried channel complexes influence the distribution of later MTCs and turbidites, ii) how deposited MTCs control the scale of subsequent turbidites and channels, iii) how deposited MTCs influence subsequent MTCs. Our results demonstrate that: i) the buried channels significantly affected the deposition pattern of MTCs and turbidites; ii) the buried MTCs can create a set of topography highs and lows, these local topography-highs could divert the flow direction of subsequent channels. Furthermore, the local topography lows may serve as a focal point for the later channel incision; iii) the buried MTCs can influence the distribution and thickness pattern of younger MTCs. Our findings indicate that these younger MTCs tend to deposit predominantly over areas with thicker older MTCs and in regions where turbidites are thinner. We indicate that MTCs, channel complexes, and turbidites can have a closed relationship. Understanding the interaction of these deposits could enhance our knowledge of sediment transportation and re-distribution in deep-water settings, offering new insights for sediment source-to-sink (S2S) studies.
Session Chair(s): Loren CHANG, National Central University, Erick LANSARD, Nanyang Technological University
IG21-A003
| Invited
Preliminary Results from Compact Ionospheric Probe Onboard PEARL-1C CubeSat
Chi-Kuang CHAO#+
National Central University
PEARL-1C (Propagation Experiment using kurz-Above-band radio in Low earth orbit) CubeSat developed by National Central University (NCU) for educational training/scientific research was launched into a sun-synchronous orbit at 520 km altitude around 1030 local time sector by SpaceX Transporter-9 rideshare mission from Vandenberg Space Force Base on 11 November 2023. A Compact Ionospheric Probe (CIP) especially customized for CubeSat dimension was installed onboard PEARL-1C to monitor global ionospheric space weather conditions resulting in space communication disruption and navigation outage for one year mission. The CIP is an all-in-one in-situ ion sensor also developed by NCU to measure ionospheric ion concentration, velocity, and temperature alternatively like its predecessor, Advanced Ionospheric Probe, onboard FORMOSAT-5 satellite. In this presentation, preliminary observations derived from the CIP measurements will be presented and some works on CubeSat operations will also be discussed after three months of early orbit phase.
IG21-A013
The Mission Design and Scientific Value of Kinetic Optical Yaw Observer (KOYO)
Yi Chung CHIU#+, Yu Shun WANG, Loren CHANG
National Central University
Kinetic Optical Yaw Observer (KOYO) is a 3U CubeSat project jointly developed by Hex20 Pty Ltd, AEGIVERSE Co Ltd and National Central University (NCU), Taiwan. The project starts in 2023/04 and is expected to be launched at 2024 Q4. The mission is mainly aimed at the space verification of fiber optic gyroscope (FOG). Comparing the data measured by the microelectromechanical systems (MEMS) gyroscope and the FOG in orbit ensures the accuracy of the FOG data, and also provides the FOG with the qualifications for space flight heritage. In terms of science object, NCU is responsible for designing the concept of operation (ConOps) for the air drag measurement. Although there is only single-axis (Yaw) measurement, it is possible to capture the dramatic changes in atmospheric density when passing through the terminator. Following the design experience of the International Satellite Program in Research and Education Constellation of Satellites (INSPIRESat) program, KOYO’s satellite uses HEX20’s 3U CubeSat box solution. In addition to the basic subsystems (power, data and communication), KOYO only uses passive magnets as an actuator for attitude stabilization in the attitude module because there is no pointing requirement. The mission architecture is very simple, but it still has great potential development. In addition to the goals of this mission, data from the payload can also be used to develop algorithms for retrieving air density, laying the foundation for future thermosphere observations. With the miniaturization of satellites and the increasing use of low-Earth orbit, the requirement for accurate orbit propagation will increase. The high-precision characteristics of FOG will become one of the solutions for the constellation system. The attitude and orbit data of the constellation can also be used as a data source of global thermosphere map.
IG21-A002
Autonomous Navigation for CubeSats Based on X-ray Pulsar Measurements
Sui CHEN#+, Francesco TOPPUTO
Politecnico di Milano
Recent technological advancement has led to a significant surge in the development of space exploration missions. Currently, space missions mainly rely on Earth ground-based Guidance, Navigation and Control (GNC) operations involving human-in-the-loop processes. Although reliable, the ground-based navigation approach is prone to prolonged periods of communication delay, lacking real-time capabilities and autonomy. In addition, the booming growth of users in space will inevitably lead to saturation of ground slots, hindering the progression of space exploration. Reducing the dependence on ground operation by developing on-board autonomous navigation methods represents a potential solution for future space missions. X-ray pulsar navigation represents an innovative concept for achieving autonomous spacecraft navigation. This technique, which utilises the pulsar’s signal time-of-arrival to determine a spacecraft’s position, has been shown to have superior accuracy. In this work, autonomous navigation based on X-ray pulsar timing measurements will be investigated for a CubeSat. Despite the size limitations imposed on CubeSats, which might restrict the use of X-ray detection instruments, recent missions such as CubeX have been proposed to employ miniaturised X-ray optics, allowing for these measurements on a small satellite. Three pulsars B0531+21, B1937+21 and B1821-24 are used as the signal sources to generate timing measurements. An extended Kalman filter is used for state estimation of the satellite. A dynamic model is derived considering the main perturbations including J2, J3, drag, solar radiation pressure and third-body effect. Simulation results show that the position estimation can be achieved with a 3-sigma accuracy below 1km. The promising results demonstrate the capability of estimating satellites’ states without relying on ground support. The significance of this study is anticipated to foster greater confidence in the implementation of X-ray pulsar based navigation, representing a foundational progression towards achieving fully autonomous navigation for CubeSat missions in the future.
IG21-A006
An Overview of the SNIPE Mission
Jaeheung PARK#+, Jaejin LEE, Jongdae SOHN, Tae-Yong YANG, Hosub SONG, Young-Joon JUNG, Youngbum SONG, Young-Sil KWAK, Junga HWANG
Korea Astronomy and Space Science Institute
The Small scale magNetospheric and Ionospheric Plasma Experiment (SNIPE) mission consists of four 6-U non-spinning CubeSats in constellation. Its primary science target is to resolve small-scale structures in the terrestrial ionospheric plasma and high-energy particles coming from the magnetosphere. Each satellite is equipped with 2 magnetometers, 2 Langmuir Probes (LPs) and 2 Solid-State Telescopes (SSTs), and the inter-satellite distance can be controlled by an onboard cold gas thruster. The 4 spacecraft were launched on 25 May 2023 from Naro Space Center in the Korean Peninsula to a dawn-dusk Sun-synchronous orbit at an altitude of 550 km. The Mission Operation Center (MOC) is located in Daejeon, Korea, and the science data have been downloaded to both the Daejeon MOC and the Kongsberg Satellite Services (KSAT) facility in Svalbard. In this presentation, we briefly overview the mission design, hardware specifications, ground-based test results, and on-orbit science data.
IG21-A008
| Invited
GBSAT: A CubeSat to Measure Proton Flux Aligned to the Geomagnetic Field
Hyosang YOON1#+, JaeHun JANG1, Junyoung YANG2, Sanghun LEE3, Jemin LEE1, Taegyun LEE4, Hyunmin KIM3, BeomJun CHUNG3, Woochan BANG5
1Korea Advanced Institute of Science and Technology, 2Korea Aerospace University, 3Daegu Gyeongbuk Institute of Science and Technology, 4Gwangju Institute of Science and Technology, 5Seoul National University
In this presentation, we introduce the GBSAT project, the 2022 winner of the CubeSat Contest hosted by the Korea Aerospace Research Institute (KARI). GBSAT, a 3U CubeSat, is designed to measure proton flux aligned with the geomagnetic field in low Earth orbit (LEO). In LEO, protons travel in a helical trajectory influenced by Earth's magnetic field. Protons with kinetic energies in the tens of MeV range exhibit a rotational radius of several tens of kilometers. Consequently, when observing protons in LEO, a notable difference in the trajectory altitude is observed depending on whether the detector faces westward or eastward. This results in variations in proton flux, a phenomenon known as the East-West effect of Cosmic-ray. To mitigate this, GBSAT's payload is aligned with the Earth's magnetic field, utilizing a magnetometer and magnetic torquers to ensure that the magnetic field does not influence the flux measurements. The satellite is equipped with an in-house developed Cosmic Ray Detection Module (CRDM) to detect protons. This presentation will delve into GBSAT's mission objectives, system design, development progress, and project team management. Notably, the project team comprises seven undergraduate students from five different universities, showcasing a collaborative and interdisciplinary effort.
IG21-A017
| Invited
PCUBE: A CubeSat Project for Probing, Controlling, and Understanding of Radiation Belt Environments
Yuto KATOH1#+, Yoshiharu OMURA2, Satoshi KASAHARA3, Iku SHINOHARA4, Mariko TERAMOTO5, Takefumi MITANI4
1Tohoku University, 2Kyoto University, 3The University of Tokyo, 4Japan Aerospace Exploration Agency, 5Kyushu Institute of Technology
PCUBE is a 5-year project (2023-2027) to investigate the rapid loss process of radiation belt electrons by plasma waves by (1) developing a radiation belt model fully incorporating rapid loss, (2) measuring the radiation belt loss process by originally developed instruments onboard a CubeSat, and (3) analyzing spacecraft data measured in terrestrial and Jovian magnetospheres. Recent studies clarified that the radiation belt varies more dynamically than conventionally expected due to the rapid loss process by electromagnetic plasma waves. Our project tries to confirm a hypothesis that the efficient loss of radiation belt electrons occurs along the plasma duct, which concentrates plasma waves along a specific field line where the plasma density is enhanced from those of the surroundings. To investigate the relationship between the plasma duct and the rapid loss process of radiation belt electrons, we need to observe the relativistic electron precipitation and the plasma density structure simultaneously in the Earth’s upper atmosphere. We develop a high-energy electron detector and a plasma density probe for a CubeSat. The electron detector uses the avalanche photo-diode, which we employed in the energetic electron detector onboard the Arase satellite. The developed detector covers a wide energy range from tens to millions of electron volts. By measuring the energy dependence of precipitating electrons into the Earth, we clarify the roles of electromagnetic waves in the radiation belt loss process. We also develop the plasma density probe by miniaturizing the 1-m length plasma probe used in conventional sounding rocket experiments. We will install the originally developed probes into a CubeSat to measure the loss of radiation belt electrons inside the plasma duct. Our project reveals the fundamental physics of the rapid loss of radiation belts, developing the theoretical basis to control the radiation belts.
IG21-A018
| Invited
Continuing Education Program for Undergraduate Students Using CubeSats at Kyushu Institute of Technology
Mariko TERAMOTO#+, Meng CHO, Kentaro KITAMURA, Koki KITAGAWA, Kohei MATSUI
Kyushu Institute of Technology
In 2012, the Kyushu Institute of Technology (Kyutech) developed, launched, and operated 27 nanosatellites. Among the satellite projects that Kyutech carried out, the BIRDS satellite project, which is an educational project, invited international students from countries with no experience in developing satellites to Kyutech and created 1U/2U CubeSats in cooperation with Japanese graduate students. The BIRDS project has developed CubeSats as a series of satellites spanning five generations, and has trained many graduate students. In recent years, satellites developed by the BIRDS project have been made open-source, and educational institutions outside Kyutech have begun to use them for satellite development and space education. Based on Kyutech's educational experience in space engineering, we designed a continuing education program using CubeSats for undergraduate students. In this program, second- and third-year undergraduate students design, develop, and operate CubeSats and model CubeSats during regular university undergraduate classes. Undergraduate students also develop a small rocket to reach an altitude of 1 km and release the model CubeSat. Issues that arise during the simultaneous development of a model CubeSat and a small rocket will be resolved through cooperation between the satellite and rocket teams. This educational program aims to develop human resources that can make decisions and judgments based on the wide range of knowledge and experience required in the aerospace field, and who can lead projects with a vision of what should be achieved. The satellite and rocket development under this program is scheduled to begin in the fall of 2024. In this presentation, we present an overview of this program and the status of its preparations.
IG21-A010
2U-size CubeSat Project for Space Weather Observation as a Human Resource Development of Undergraduate Students
Kentaro KITAMURA1#+, Hirokazu MASUI1, Teiji UOZUMI1, Mariko TERAMOTO1, Akiko FUJIMOTO1, Meng CHO1, Shuji ABE2, Akimasa YOSHIKAWA2
1Kyushu Institute of Technology, 2Kyushu University
Since the successful launch of the first CubeSat in 2003, CubeSat has been developed at many universities around the world over the past 20 year. As the number of development cases increased, there was a strong awareness of the application of CubeSat for space use. Especially since 2013, the commercial use of nano-satellites, including CubeSat, has also increased significantly, ratio of the satellites with weight of less than 10 kg reached 13% of all satellites launched in 2022. Although science missions using CubeSat have also been increasing, but most of them in Japan have been conducted by graduate schools of engineering, and there were very few cases that space science researchers involved to these CubeSat programs. Therefore, Kyushu Institute of Technology, in cooperation with Kyushu University, started the development of YOYSUBA-KULOVER, a 2U-sized CubeSat, in 2021FY with the main mission of space weather observation. The unique feature of this satellite project is that undergraduate students in science and engineering departments from different universities work together to develop the 2U CubeSat for science missions. This program is implemented as an early-stage practical education program to develop the human resources who will be responsible for future scientific satellite missions. The missions of the CubeSat are precise measurement of geomagnetic field with an accuracy of 0.1 nT to observe the magnetic perturbations related to the magnetic storms and/or aurora substorms and to capture the aurora in visible light during substorms. For these missions, the Use of COTS product for both the magnetometer and the camera enable us to reduce the cost and development time. YOTSUBA-KULOVER is currently in the final environmental testing phase of FM (Flight Model) and is scheduled to be released from the ISS into an orbit with altitude of 400km in September 2024.
Session Chair(s): Abang Mansyursyah Surya NUGRAHA, Nanyang Technological University, Masashi WATANABE, Nanyang Technological University
IG10-A002
Assessing Coastal Vulnerability Caused by Beach Erosion Under Future Climate Change and Coastal Population Dynamics: A Case Study of China
Shuai XIAO+, Keiko UDO#
Tohoku University
The loss of sandy beaches due to coastal erosion affects the entire coastal zone, as beaches serve as crucial barriers to coastlines, contribute to tourism revenue, and enrich coastal ecosystems. In the future, global climate change-induced sea level rise and wave height variations will further exacerbate the erosion processes. Coupled with the continuing trend of coastward population migration, coastal areas will inevitably face higher risks. Therefore, assessing coastal vulnerability caused by beach erosion is needed for better coastal management. This study selected fifteen vulnerability indicators related to beach erosion from the natural and socio-economic perspective, covering exposure (sandy beach area, beach slope, sea level rise, wave height, storm surge loss, land subsidence, and sediment supply), sensitivity (population density, tourism GDP ratio, marine fishery production, and land use type), and adaptive capacity (public budget, beach-protected rate, mangrove area, and coral reef area). Then the exposure index (EI), sensitivity index (SI), adaptive capacity index (AC), and beach vulnerability index (BVI) for each beach zone were calculated based on different multi-criteria decision-making approaches (e.g., simple average method, principal component analysis, entropy weight method). The spatial distribution of the coastal vulnerability status caused by beach erosion was mapped and the uncertainty caused by using different weightage methods was discussed. Lastly, future climate change and coastal population variations were involved in the calculations, and the resulting changes in vulnerability were discussed. The vulnerability hierarchy derived in this paper contributed to understanding the potential impact of erosion hazards on China’s coastal communities. Based on the contribution of each index, appropriate adaptation measures could be considered for each beach zone.
IG10-A012
An Assessment of Tropical Cyclone-induced Storm Surge Risk Incorporating Future Climate Change and Sea Level Rise Around the Coast of Singapore
Masashi WATANABE1#+, Constance Ting CHUA2, Jun Yu PUAH1, Elaine Hz TAN1, Adam SWITZER1
1Nanyang Technological University, 2Tohoku University
The location of Singapore along the equator means that the risk of tropical cyclones and, hence, storm surge in Singapore is likely to be negligible because tropical cyclones usually are not formed near the equator. However, on 27 December 2001, a tropical cyclone - Typhoon Vamei, classified as a category 1 typhoon - formed southeast of Singapore, demonstrating a potential localised risk of cyclone-induced storm surges in Singapore. Here, we examine how storm surge risk in Singapore may change because of sea level rise and increased typhoon intensity due to climate change. We conducted numerical simulations of storm surges around Singapore in multiple scenarios to understand this. For the simulation, we used Delft-3D/SWAN to calculate both potential storm surges and waves induced by tropical cyclones. We reproduced the storm surge caused by typhoon Vamei through numerical simulation and found that the storm surge in Singapore reached about 1.11 m. We then moved the path of Vamei southward while the size remained constant and calculated the maximum water level in the northern part of Singapore to be 1.87 m if the cyclone track runs through the Singapore Straits. We additionally ran the simulations by increasing water level by +0.5 m and +1.0 m due to future sea level rise induced by global warming. The simulations suggest a maximum water level of 1.65 m and 2.78 m for a Vamei style event at +0.5 m and +1.0 m respectively. This analysis provides policymakers and urban planners baseline insights to enhance coastal defence preparedness and formulate effective mitigation strategies.
IG10-A017
| Invited
Building Historically Oriented Storm Surge Awareness in the Philippines Since the 2013 Super Typhoon Haiyan Disaster
Janneli Lea SORIA#+
Mindanao State University at Naawan
Super Typhoon (ST) Haiyan in 2013 tragically attests to the vulnerability of the Philippine coasts to storm surge hazards. Concurrently, ST Haiyan also paved the way for raising storm surge awareness in the Philippines. While the Philippine archipelago is inherently prone to storm surges as it is located along the path of seasonal typhoons, little was known about the storm surge's devastating impacts on many local coastal communities until the 2013 Haiyan disaster. A decade after the devastating storm surge, actions focused on mainstreaming storm surge awareness are gaining traction. The growth in local awareness of storm surge hazards and impacts since the Haiyan disaster is demonstrated in multiple aspects including the operational monitoring and warning systems, Information, Education, and Communication (IEC) campaigns, and coastal hazards research. In June 2019, the state weather agency - Philippine Atmospheric, Geophysical and Astronomical Services Administration (PAGASA) launched a storm surge warning system. The new storm surge forecasting and warning system provides easy-to-understand visuals, including potential storm surge impacts, that are intentionally designed to bridge language gaps in warning communication that were magnified by the Haiyan disaster. Another institutional improvement in IEC is the inclusion of Disaster Risk Reduction as a subject in the basic education curriculum, in which storm surge is included as one of the topics covered in the hydrometeorological hazards. Government and private institutions are now incorporating historical typhoons in building multiple storm surge simulation and risk assessment scenarios. Sediment records of extreme wave events are validated against historical typhoon archives, which could eventually expand typhoon history into a millennial scale. While innovative approaches in disaster mitigation and preparedness are gaining momentum, the “no-build zone policy” for coastal protection persists as a contested issue in disaster risk governance.
IG10-A007
Effectiveness of Balloon as Tsunami Evacuation Signs on Evacuation Time and Evacuation Routes Through Evacuation Experiments in Virtual Reality
Shunnosuke NARITA#+, Shosuke SATO, Yudai MIKAMI, Fumihiko IMAMURA
Tohoku University
A tsunami evacuation building (TEB) is an emergency evacuation facility for evacuees who find it difficult to evacuate to higher ground before the tsunami reaches the coast. Currently, the number of TEBs around Japan's coasts is more than 15,000, approximately eight times more than before the 2011 Great East Japan Earthquake. Especially if the tsunami arrival time is short or the area is far from high ground, it is necessary to prepare that the evacuees can arrive TEBs as soon as possible. Kamakura City in Kanagawa, Japan, is one of the areas where the tsunami is expected to reach the area in a short time (8 minutes at the earliest), and the coastal areas are far from higher ground. Furthermore, many tourists who are not familiar with Kamakura City visit the coastal area. Therefore, TEB plays a necessary role not only for residents but also for tourists. However, although there are signs installed at TEB, it is difficult for tourists to tell which of the many buildings is TEB. Therefore, we propose to verify whether it is effective to install advertising Balloon-type Evacuation Signs (BES) on rooftops to visually inform evacuees of the TEB's location in a way that is easier to understand. Because on-site demonstration experiments are difficult, this study examined the differences in evacuation times and evacuation routes in the virtual reality of Kamakura City under four conditions with different BES and TEB maps. A total of 90 participants, divided into four groups, participated in this evacuation experiment. As a result, under conditions where the TEB map could not be accessed, BES shortened the route to the TEB and improved the evacuation completion rate by approximately 20% at the expected tsunami arrival time in this area.
IG10-A006
Relationship Between the Coral Reef System and the Tsunami Waves of the 2004 Indian Ocean Event in Malé Atoll
Elisa LAHCENE#+, Anawat SUPPASRI, Kwanchai PAKOKSUNG, Fumihiko IMAMURA
Tohoku University
Compared to renowned coral reef systems such as the Great Barrier in Australia or the one in American Samoa, the Maldivian reef system has been poorly studied. Therefore, the relationship between the 2004 Indian Ocean Tsunami (IOT) with the reef remains unclear. Following the tsunami event, some field-based studies suggest that specific reef areas offered protection against the tsunami waves. However, a quantitative study is lacking to assess the buffering role of the Maldivian reef. Considering its significance for fisheries and tourism, there is an urgent need to understand the Maldivian reef dynamics during the 2004 event. Here, we aim to address the scientific gaps related to the impact of the reef on the 2004 tsunami waves in Male Atoll. The central question is whether the Maldivian coral reef system acted as a buffer or not. If so, we quantify the extent of reduction or amplification of the tsunami characteristics along the shoreline. We hope to provide valuable insights into the specific mechanisms by which the Maldivian reef interacted with the 2004 tsunami, offering potential applications in coastal management and disaster preparedness. This research not only addresses a critical knowledge gap regarding the reef dynamic during a tsunami event, but also emphasizes the importance of considering coral reefs in the context of sustainable coastal management.
IG10-A019
Tsunamigenic Potentials of Two Volcanic Islands in the South China Sea: A Comparative Study of Didicas Volcano and Cendres Volcano
Kan ZHANG+, Linlin LI#
Sun Yat-sen University
South China Sea (SCS) and its surrounding regions are among the most active regions in terms of volcanic tsunamis. However, a significant research gap exists for such tsunamis in the SCS. Historical documents reveal that both Didicas Volcano in the Luzon Strait and Cendres Volcano in southeast offshore Vietnam have generated tsunamis in the past 100 years. To assess the tsunamigenic potentials of these two volcanos, we utilized NHWAVE and FUNWAVE for tsunami generation and simulation which take two generation mechanisms into account: underwater explosions and flank collapses. Through comparison, we provide a preliminary understanding of the potential tsunami impacts of these two volcanoes. Firstly, a volcano's ability to trigger tsunamis is largely influenced by its tectonic settings. Didicas Volcano is situated on the subduction zone of the Luzon Arc, with intense magma activity, increasing the potential for larger-scale volcanic events. This in turn could trigger substantial tsunamis reaching coastal areas as far as Southern coastlines of China. In contrast, Cendres Volcano, situated within the plate interior near the fracture zone at the western edge of the SCS, has weaker magma activity, suggesting a potentially smaller tsunami scale. The tsunami would primarily impact the coastal areas of Southeast Vietnam and nearby islands in the SCS. Secondly, the distribution of tsunami energy is largely controlled by bathymetry and topography along the propagation path. Due to the complex surrounding terrain, tsunami waves triggered by Didicas Volcano are influenced by the guiding effect of island arc. While being generated on the wide continental shelf, the tsunami propagation process triggered by Cendres Volcano exhibits very interesting behaviors. The comparative analysis of tsunamigenic potentials of these two volcanoes will enhance our understanding of volcanic tsunami hazards in the SCS, offering valuable insights for hazard preparation and tsunami early warning in this area.
IG10-A020
Potential Submarine Landslide-generated Tsunami Based on 3D Seismic Reflection Data: A Case Study from the Makassar Strait
Saaduddin SAADUDDIN1#+, Harya Dwi NUGRAHA2,3, Abang Mansyursyah Surya NUGRAHA4
1Hasanuddin University, 2University of Bergen, 3Universitas Pertamina, 4Nanyang Technological University
The connection between landslides and their potential to cause tsunamis remains underexplored in Indonesia's disaster management, particularly concerning submarine landslides. However, these events pose a significant danger to coastal communities and infrastructure. The 2018 Palu tsunami underscored the urgent need to address the risks associated with tsunamis triggered by submarine landslides. The Makassar Strait, situated between Kalimantan and Sulawesi islands, is influenced by currents from both the Pacific and Indian Oceans that carries sedimentary material. Analysis of reflection seismic data has identified numerous deposits that might serve as potential sources for submarine landslides. One such deposit, located west of Majene, has an estimated volume of 11 km3, although its tsunamigenic potential remains uncertain. Tsunami modeling indicates that such a volume could produce a tsunami approximately 3 meters high along Sulawesi Island's west coast, particularly considering its proximity to active tectonic zones, like the one that caused the 1969 Majene earthquake and subsequent tsunami. Our study shows that documented submarine landslides in seismic reflection data can be modelled to understand past events, which then can be used to assess potential impacts and design effective early warning systems to safeguard vulnerable coastal populations.
IG10-A014
A Proposed Approach Towards Developing Continuous Coastal Elevation Data for Tsunami-prone Areas in Indonesia
Constance Ting CHUA1#+, Anawat SUPPASRI1, Syamsidik SYAMSIDIK2,3, Fumihiko IMAMURA1
1Tohoku University, 2Universitas Syiah Kuala, 3Universitas Syiah Kuala
To support coastal monitoring, modelling of coastal floods and tsunami in Indonesia, a joint-research initiative – the SATREPS BRICC “Building Sustainable System for Resilience and Innovation in Coastal Community” was established between Indonesia and Japan. Continuous elevation model (DEM) from sea to shore is necessary to accurately monitor coastal and environmental changes, as well as model coastal hazards such as floods, storm floods and tsunami. However, the availability of high-resolution coastal elevation data is limited in many areas in Indonesia. Therefore, the aim of this study is to provide a systematic approach to developing high-resolution, continuous elevation data for flood and tsunami-prone areas in Indonesia. Currently, topography models (DEMNAS) and bathymetry models (BATNAS) provided by local agency, Badan Informasi Geospasial, are freely available for all of Indonesia, and a straight-forward solution would be to merge these two datasets through interpolation methods. However, such an approach is challenged by three key limitations: (i) differences in spatial resolution of the two datasets (8 m for DEMNAS and 108 m for BATNAS), (ii) differences in vertical reference systems (EGM2008 for DEMNAS and mean sea level for BATNAS), and (iii) data gaps in shallow water and subtidal areas. Collection of depth data in the shallow water region is constrained by manpower requirements, environmental conditions, changing tides, accessibility and navigational restrictions. In recent years, satellite-derived bathymetry has been recognised as a cost-efficient method to overcome data gaps in the shallow water areas. In this study, we capitalise on freely-available data by firstly using satellite imagery to derive shallow water topography and combining our models with DEMNAS and BATNAS models to develop continuous coastal elevation models for Indonesia at 10 m horizontal resolution and the final models are referenced at mean sea level.
Session Chair(s): Kentaro KITAMURA, Kyushu Institute of Technology, Hyosang YOON, Korea Advanced Institute of Science and Technology
IG21-A005
The Deep Space Radiation Probe: Development of a First Lunar Science Payload for Space Environment Studies and Capacity Building
Loren CHANG1#+, Wei-Yi LIN1, Yi-Hsuen CHOU1, Jen-Siang LIN1, Chieh LUNG1, Yi CHEN1, Yi Chung CHIU1, Chi-Kuang CHAO1, Jann-Yenq (Tiger) LIU1, Tungyuan HSIAO2
1National Central University, 2Hsing Wu University
Regions outside of Low Earth Orbit (LEO) are classified as “deep space”, including cislunar and lunar space. The deep space environment poses many challenges for human and robotic exploration, including stronger ionizing radiation fluxes, more extreme temperature variations, as well as limited data downlink volume. With the growth of the rideshare and hosted payload model aboard government and commercial lunar missions, developing the capacity to design and implement payloads and other space avionics for this environment is of increased importance this decade. Utilizing one of the growing number of rideshare opportunities offered by commercial lunar mission providers, National Central University (NCU) has been working on the rapid development of Taiwan’s first scientific payload for lunar lander use, with launch aboard the HAKUTO-R Mission 2 (M2) lander from ispace, inc. scheduled not earlier than Q4 2024. This Deep Space Radiation Probe (DSRP) will provide measurements of radiation dose, dose rate, and single event upset rate during the Earth-Moon transit, in lunar orbit, as well as on the lunar surface. DSRP utilizes elements of the on-board computer (OBC) developed and flight qualified aboard the NCU-developed IDEASSat 3U CubeSat mission in 2021, and was developed by a student team, in consultation with experienced engineers from the lunar lander team. In this paper, we will report on the objectives, concept of operation, design, and implementation of the DSRP project. We will also describe the steps taken to facilitate parallel development of the DSRP payload and the HAKUTO-R M2 lander, as well as lessons learned during the design, implementation, and qualification process. The radiation data provided by DSRP will be beneficial for the development of future deep space spacecraft avionics, as well as crewed missions, and will also serve to build the capacity for deep space spacecraft and payload development at NCU.
IG21-A001
Flight Model Development and Calibration of IAMMAP: Ionospheric Plasma and Current Observing Instrument for CAS500-3
Kwangsun RYU1#+, Seunguk LEE2, Suwhan PARK1, Jimin HONG1, Jinkyu KIM1, Wonho CHA1, Bon-ju KOO1, Seong-og PARK1, Du-young CHOI2, Chongrim CHOI2
1Korea Advanced Institute of Science and Technology, 2Chungbuk National University
The Ionospheric Anomaly Monitoring by Magnetometer And Plasma-probe (IAMMAP) is one of the scientific instruments for the Compact Advanced Satellite 500-3 (CAS 500-3) which is planned to be launched in 2025 by KSLV (Korean Space Launch Vehicle). The main scientific objective of IAMMAP is to understand the complicated correlation between the equatorial electro-jet (EEJ) and the equatorial ionization anomaly (EIA) which play important role in the dynamics of the ionospheric plasma behavior in the dayside equator region. IAMMAP is an instrument set of an impedance probe, a Langmuir probe for self-calibratable plasma measurement and magnetometers for EEJ current derivation. The designated sun-synchronous orbit along quasi-meridional plane makes the measurement suitable for studying EIA and EEJ. The impedance probe is expected to get electron density of the ionosphere with unprecedented precision by measuring upper-hybrid frequency of the ionospheric plasma that is not affected by the satellite geometry, the spacecraft potential, or contamination unlike the widely-used Langmuir probes for cubesat missions. A set of fluxgate magnetometers, which is named as AIMAG (Adaptive In-phase MAGnetometer), is expected to track the EEJ signature with the far-improved resolution and reduced noise by applying a newly devised circuit concept. The development status and calibration results for the flight model of IAMMAP are introduced with the expected scientific impacts and its implication for the future missions.
IG21-A009
Small Satellites Mission for Earthquake Prediction Among Asian Countries
Koichiro OYAMA1,2#+
1International Research Center for Space and Planetary environment Science, 2Asia Space Environment Research Consortium
We are studying abnormal behavior of ionosphere by expecting the prediction of the earthquake occurrence within 7-10 days in the near future Our past data analysis shows the followings; Dynamic explorer -2 data shows that O + density at the height of 300 km shows the minimum over the epicenter as well as geomagnetic equator. Two minima which is away from each other about 6-10 days before other merges around earthquake day. If you plot the place of two minimum in longitude and latitude, we can know the epicenter. If we plot the percent of the reduction normalized by the background O+ density, versus day, we know the date of earthquake. This method to predict earthquake might be applied within 30 degrees in geomagnetic latitude. Another fact observed by DEMETER and DMSP satellite is that plasma density over geomagnetic equator increases both day and night before the earthquake which occurred in mid latitude. In this case we cannot identify the epicenter in Japan. The abnormal behavior of Te at 600km can be used for the earthquake which occurs around Philippine. Accordingly, we might be able to predict the earthquake if we have a constellation of small satellite as below. 12 satellites to observe the same region need to fly over the epicenter. The altitude of the region to be studied is 300km -350 km, with the same local time every day (sun synchronous). To keep the orbiting height, thruster(s) is needed. Instruments which provide plasma density and electron temperature are enough. Since we need 12 satellite, we can share the cost among the earthquake suffering countries. The satellite accommodates common battery, telemeter, and data processing Unit. Soft wares which are needed for orbit calculation and scientific data analysis should be shared among the countries.
IG21-A012
Harnessing Small Satellites for Swift Equatorial Environmental Surveillance
Erick LANSARD#+, Noel PNG
Nanyang Technological University
There is a need for responsive and cost-effective satellite data acquisition in the equatorial region, emphasizing the confluence of low-cost satellite manufacturing and heightened ground pass opportunities. Recognizing the urgent need for new scientific data to enhance and refine existing climate models, this research underscores the pivotal role of equatorial-focused satellite missions in advancing our comprehension of climate change and urbanization-induced phenomena. The equatorial belt, with its unique environmental dynamics, demands a shift in observational capabilities. Traditional satellite systems face challenges in providing timely and comprehensive data due to cost constraints and limited ground pass opportunities. The emergence of low-cost satellite manufacturing technologies offers an unprecedented solution to these challenges. The need for new scientific data is evident in the context of climate models, where existing frameworks require constant refinement to accurately reflect the intricate interplay of environmental variables. Equatorial regions, often characterized by biodiversity hotspots and vulnerable ecosystems, serve as crucial indicators of global climate patterns. Rapid-response satellites enable more frequent and targeted observations, allowing scientists to garner crucial insights into the impacts of climate change and urbanization on these sensitive areas. Furthermore, the equatorial region's higher ground pass opportunities for satellites in low Earth orbit amplify the effectiveness of data collection. The increased revisits over equatorial zones enable the capture of information, facilitating a better understanding of climate phenomena. By bridging the gap between cost-effectiveness and enhanced observation capabilities, these satellites are playing a pivotal role in advancing climate models and the complex interactions between climate change and urbanization within the equatorial region.
IG21-A020
Space Science Using Satellite Constellations and Multiple Instruments
Hosub SONG#+, Jaeheung PARK, Jaejin LEE
Korea Astronomy and Space Science Institute
We introduce the ionosphere statistical studies by using satellite constellation and multiple instruments for the space environment on the Low Earth Orbit (LEO). In-situ observations using satellites provide important data for the space environment. Moreover, as satellites are manufactured in small with large numbers, observation methods using satellite constellations and multiple devices are increasing. Using satellite constellations such as SWARM satellites, the quasi-two-dimensional characteristics of Medium-Scale Traveling Ionospheric Disturbances (MSTIDs) occurring in the night mid-latitude ionosphere are analyzed through tandem observations made by two satellites flying side by side. Also, through multiple instruments on a single platform such as GRACE/GRACE-FO satellites, we study the relationship between Equatorial Plasma Bubble(EPB) and Neutral Density Disturbance (NDD) by simultaneously measuring electron density and neutral density. Therefore, in-situ observations using satellite constellations and multiple instruments contribute to advanced space environment research.
IG21-A014
| Invited
Lithosphere-atmosphere-ionosphere Coupling Phenomena Nowcasted by the MVP-LAI System
Yang-Yi SUN1#+, Chieh-Hung CHEN2, Kai LIN1
1China University of Geosciences, 2Chengdu University of Technology
At the end of 2021, a monitoring system, MVP-LAI (Monitoring Vibrations and Perturbations in Lithosphere, Atmosphere, and Ionosphere), was established in Leshan, Sichuan, China. The MVP-LAI system, with its instruments including the magnetometer, broadband seismometers, wind profile radar, barometers, field mill, Global Navigation Satellite System (GNSS) receivers, etc., is confined to an area of ~400 square meters. The purpose of establishing the system with all those collocated instruments is to nowcast vibrations and perturbations across various spheres, from the Earth's surface to space (http://geostation.top/). This presentation highlights the LAI coupling phenomenon observed several hours before the Mw 6.8 Luding earthquake (29.59◦ N, 102.08◦ E) on 5 September 2022, located about 175 km from the MVP-LAI system. On the other hand, we illustrate the system's capability to detect LAI coupling phenomena resulting from the distant Tonga volcano eruption (20.546°S 175.390°W) on 15 January 2022, over eleven thousand kilometers away. The MVP-LAI system effectively captured these phenomena, and we also incorporated the radio occultation observations from the low earth orbit satellite of the FORMOSAT-7/COSMIC2 mission.
Session Chair(s): Anawat SUPPASRI, Tohoku University, Constance Ting CHUA, Tohoku University
IG10-A016
| Invited
Sediments and eDNA from Tsunami Deposits of the 2018 Palu Earthquake Reflect Low Power and Short-term Tsunami Inundation
Adam SWITZER1#+, Jędrzej MAJEWSKI2, Wenshu YAP1, Rachel GUAN1, Winona WIJAYA1, Benazir BENAZIR3, Ella MEILIANDA4, Peter PARHAM1,5, Robert WEISS6, Jessica PILARCZYK7, Hermann FRITZ8, Federico LAURO1, Benjamin HORTON9,10
1Nanyang Technological University, 2Adam Mickiewicz University, 3Universitas Gadjah Mada, 4Syiah Kuala University, 5Universiti Kebangsaan Malaysia, 6Virginia Tech, 7Simon Fraser University, 8Georgia Institute of Technology, 9City University of Hong Kong, 10Imperial
On 28 September 2018, a magnitude 7.5 earthquake struck north of Palu, Central Sulawesi, Indonesia. The earthquake generated a tsunami with inundation depths above terrain of up to 6 m and run ups to 10 m above sea level. Inundation distances were topography dependent and exceeded 400 m in low-lying areas. A compound tsunami was likely generated by a combination of minor fault displacement and multiple submarine landslides. In places, co-seismic coastal subsidence >1 m likely exacerbated the inundation of tsunami waves. During a post tsunami survey in November 2018, we sampled three transects for sediment analysis and environmental DNA (eDNA); two in Palu City and one on the eastern coasts of Palu Bay at Pantoloan. The thin (<5 cm thick) tsunami deposits in Palu City are predominantly massive, fine- to medium-grained sand. The east coast samples at Pantoloan showed little reworking and are characterized by a continuous sand sheet that extends up to 250 m inland and fines and thin inland. Grain size ranges from coarse-grained sand to silty-fine-grained sand at the landward extent. This site also contained wave-transported blocks of sea wall found more than 130 m from the shoreline that suggest that velocities >5 m.s-1. We also analyze the environmental DNA in the tsunami-deposited sand and the underlying non-tsunami-derived sediments and soil. Multivariate analysis shows that microbial communities in the tsunami deposits of Palu City and Pantoloan are significantly different from those in the pre-tsunami layers. We find that the Palu tsunami deposits generally exhibit sedimentologic and stratigraphic characteristics that show a hybrid signature common to both storm and tsunami deposits. This observation likely reflects the short wavelength, relatively low power and short-term inundation of the compound tsunami and the limited availability and nearshore source of the sediments.
IG10-A001
Initial Results of Paleotsunami Research on Tongatapu Island, Tonga
Kazuhisa GOTO1#+, James GOFF2, Takashi ISHIZAWA3, Koki NAKATA1, Savelinga FAOLIU4, Penikolo VAILEA4, Katsumi KASAI1
1The University of Tokyo, 2University of New South Wales, 3Tohoku University, 4Tonga Geological Services
Tongatapu Island is vulnerable to large tsunamis because of its close proximity to the Tonga Trench. Furthermore, there are numerous tsunamigenic submarine volcanoes in the region. Indeed, the 2022 Hunga Tonga–Hunga Haʻapai (HT-HH) eruption generated a large tsunami that strongly impacted the island (e.g., Borrero et al., 2022). However, there has been limited research of prehistoric tsunamis on Tongatapu Island (Frohlich et al., 2009; Lavigne et al., 2021) and as such the paleotsunami history and paleosources of past event is uncertain. In this initial study, we carried out a field survey for both boulders and sandy deposits on Tongatapu Island finding evidence for both historical and paleotsunami events. For example, in the Kanokupolu area, the 2022 HT-HH tsunami deposits are still observable on the ground surface. Along a survey transect of the 2022 deposits we observed a large possible tsunami boulder on top of the coastal hill and trenches beneath it. Our trench survey revealed at least 6 event layers. Some or all of them could be tsunami deposits because they contain a number of shell and coral fragments. In addition, the fact that the boulder was at the highest point in the area means that any marine material could not have been washed in/reworked from sediments higher up but rather were transported at least 200 metres inland and 10 metres above sea level. Therefore, it seems reasonable to infer tsunami deposition at this site. Also, the bottom event layer is remarkable as this coral/shell deposit is directly covered by a thick tephra. Therefore, it seems reasonable to infer that this deposit may be linked with a volcanogenic tsunami. This research was supported by SATREPS, JST/JICA and JSPS.
IG10-A003
A New Framework for Tsunami Source Inversion Based on Tsunami Deposit Data
Hidetoshi MASUDA#+, Daisuke SUGAWARA
Tohoku University
Tsunami deposit is a crucial proxy for paleoseismology along the subduction zones. Numerical models of tsunamis have been utilized to reveal the seismological variables from tsunami deposit characteristics. The heterogeneity of coseismic slip is a key indicator of the fault kinematics and spatial pattern of earthquake occurrence and thus the heterogeneous fault model is needed for a better understanding of past earthquakes and tsunamis. However, the systematic inversion of tsunami sources based on tsunami deposits has not yet been established. Therefore, existing deposit-based tsunami source modeling employs simple, rather uniform fault models. Such simple models potentially hinder the in-depth understanding of paleoearthquakes. This study proposes a new framework for deposit-based tsunami source inversion. This method allows the estimation of a heterogeneous slip by utilizing a regional (hundreds of kilometers) distribution of a tsunami deposit and tsunami sediment transport modeling. A surrogate optimization technique was employed with deposit thickness-based evaluation criteria. The inversion framework was validated through a numerical experiment mimicking a giant (Mw 9.0) earthquake in the Japan Trench. We used an artificially synthesized fault model composed of 10 subfaults to generate an artificial dataset of tsunami deposit distribution in five selected lowlands along the coastline. A total of 440 thickness data were extracted and referred to constrain the tsunami source. We then iteratively conducted 500 simulations guided by the optimization algorithm. After all, although the general trend of the slip distribution was successfully reconstructed, the peak slip value was substantially underestimated. Since the peak slip was near the trench axis, the tsunami deposit in coastal lowlands may be insensitive to up-dip impulsive slip. Moreover, the local scarcity of the deposit data in the adjacent area of the peak slip also affected the estimation. Despite the uncertainties above, this new framework indicates a future direction of deposit-based subduction zone paleoseismology.
IG10-A013
The 2024 Noto Peninsula Earthquake: Tsunami Impact in Japan and the Sea of Japan
Anawat SUPPASRI1#+, Hidetoshi MASUDA1, Kwanchai PAKOKSUNG1, Daisuke SUGAWARA1, An-Chi CHENG2, Yoshinori SHIGIHARA3, Shuichi KURE4, Fumihiko IMAMURA1
1Tohoku University, 2Tohoku University, Japan, 3National Defense Academy, 4Toyama Prefectural University
An earthquake with magnitude of 7.6 occurred on the 1st January 2024 in the north of Noto Peninsula at 16 km depth with the maximum earthquake intensity observed as 7 in Japanese scale. Tsunami warning and major tsunami warning was issued and observed throughout the Japan Sea` coast as well as in the South Korea and Russia. In Japan, observed tsunamis were varying from 0.4 m to more than 1.2 m. There were some areas in Noto Peninsula inundated around few hundred of meters (few meters of inundation depth) by this tsunami causing building damage but no casualty was reported by the tsunami. Among the observed waveforms, the one recorded in Toyama is the only station that started from a negative wave. This suggests the possibility of another tsunami source in Toyama Bay similar to the previous Noto Peninsula earthquake occurred in 2007. This presentation provides summary of tsunami warning situation, tsunami trace heights and tsunami inundation area from field surveys and aerial images in Japan, an additional tsunami source (possible submarine landslide) that can explain also the observed waveforms in Toyama Bay and observed tsunami elsewhere in the Sea of Japan.
IG10-A011
A Proposal of Pre-simulated Tsunami Database for Tsunami Warning in Taiwan
An-Chi CHENG1#+, Anawat SUPPASRI2, Constance Ting CHUA2, Fumihiko IMAMURA2
1Tohoku University, Japan, 2Tohoku University
Taiwan is exposed to tsunami hazards generated from submarine earthquakes. Despite so, the risk of tsunamis is generally underestimated in Taiwan and therefore, tsunami warning systems are relatively under-prioritized. Effective warning systems rely on successful and timely issuance of tsunami warning. The threat of tsunami risk could be forecasted through the use of a pre-simulated tsunami database. A pre-simulated tsunami database provides an ensemble of tsunami events based on arbitrary earthquake scenarios, such that a rapid forecast can be made during an actual earthquake event. An example of a pre-simulated tsunami database systems is one operated by JMA, which allows the quick issuance of initial tsunami warning before its arrival. However, the system sometimes does not provide precise estimation due to several limitations, namely (1) the assumed fault strike parameters are not refined, (2) the resolution of bathymetry used is coarse, and (3) nearshore effects are mostly neglected. These effects should be considered when evaluating tsunami hazard in Taiwan due to its unique coastal topography and geomorphology. A pre-simulated tsunami database for Taiwan that address these limitations is proposed in this study. First, a sensitivity analysis on fault strike parameters was conducted. It is found that the range of change for every 30 degrees can give cost-valuable performance in estimating tsunami heights. Then, a sensitivity analysis on bathymetry data with 7 varying resolutions was performed. It is found that a minimum resolution of 50 m is needed to effectively reproduce both tsunami heights and arrival times. Lastly, the forecasting results from Green’s law (GL) approximation based on linear long wave simulation at offshore wave gauges with various depths were compared to results from nonlinear shallow water equations simulation. It is in our hopes that the outcomes of this research would be able to contribute to local tsunami warning operation in Taiwan.
IG10-A023
Tsunami Characteristics in Semi-enclosed Seas
Jiaying CUI+, Linlin LI#
Sun Yat-sen University
In the event of a large-scale tsunami occurring in a semi-enclosed seas, the tsunami energy is unable to dissipate into the open sea and can only be absorbed inside the ocean. This may result in significant basin oscillations, prolonged duration of sea surface fluctuation and other special hazard characteristics. Currently, our quantitative understanding of tsunami characteristics in semi-enclosed seas is limited. This study investigates the unique features of seismic tsunamis in three semi-enclosed sea basins with different scales, namely, the South China Sea with area of 3.5x106 km2, the Sulu Sea with area of 3.48x105 km2 and Celebes Seas with area of 2.8 x105 km2. In addition, this study incorporates actual earthquake cases from the Japan Sea for a comparative analysis, aiming to delve deeper into the differences in free oscillation patterns among different marine regions. By introducing a heterogeneous slip distribution model that takes into account rupture complexity, a more accurate assessment of the impact range of seismic tsunamis and potential tsunami hazards in semi-enclosed marine areas can be achieved. Additionally, incorporating spectral analysis methods allows for the analysis of tsunami energy and characteristic periods. Results showed that the oscillation period in different semi-enclosed marine areas is closely correlated with their respective areas and water depths. Furthermore, local topographic effects such as continental shelf oscillation and harbor oscillation exacerbate the impact of tsunami disasters. This study innovatively considers earthquake rupture complexity, numerical simulation accuracy, and regional vulnerabilities, providing valuable insights for tsunami hazard assessment in semi-enclosed seas. Our objective is to showcase the distinctive features of basin oscillations, offer scientific support for tsunami disaster response in this high-risk region and serve as a key reference for global earthquake and tsunami research in semi-enclosed seas.
Session Chair(s): Kazuhito ICHII, Chiba University, Alfredo HUETE, University of Technology Sydney, Taejin PARK, NASA Ames Research Center
IG27-A002
Development of the Geonex Cloud and Shadow Mask Product
Weile WANG1#+, Hirofumi HASHIMOTO2, Taejin PARK1, Ian BROSNAN1, Yujie WANG3
1NASA Ames Research Center, 2California State University Monterey Bay, 3NASA Goddard Space Flight Center
Cloud detection and filtering is a key component and a classical challenge in remote sensing data processing. Prolific algorithms have been developed to address this problem with information from spatial and spectral dimensions. Here we develop a new algorithm to answer the question by exploiting the hypertemporal information provided in observations of the latest geostationary satellites including GOES16/17/18, Himawari 8/9, and GK-2A. We treat the high-frequent time series of geostationary satellite images as a 4-D (2 spatial+1 temporal+1 spectral) data cube to detect, map, and track the development and movement of individual clouds (or cloud clusters) and shadows. Our algorithm synthesizes traditional remote sensing cloud tests, computer vision technology, as well as Machine Learning/Artificial Intelligence (ML/AI) tools. We have generated 10-minute daytime cloud masks for GOES and Himawari from 2019 to the current, and are extending our algorithm to nighttime clouds as well.
IG27-A018
Transfer-learning-based Approach to Retrieve the Cloud Properties Using Diverse Remote Sensing Datasets
Feng ZHANG1#+, Jingwei LI2, Wenwen LI1, Tong XUAN1, Baoxiang PAN3, Jun LI4, Han LIN5, Husi LETU6, Mustafa FARHAN7
1Fudan University, 2Shanghai Qi Zhi Institute, 3Lawrence Livermore National Laboratory, 4National Satellite Meteorological Center, 5Nanjing University of Information Science & Technology, 6Chinese Academy of Sciences, 7The Hong Kong University of Science and Technology
Clouds play an important role in the Earth-atmosphere system. However, various observational methods describe clouds differently, leading to cloud products being described with different characteristics, and affecting our understanding of clouds. To address this problem, we integrate different cloud products into the transfer-learning procedure of a deep learning model and determined cloud properties from Himawari-8 thermal infrared measurements. By doing this, we can obtain all-day cloud properties with high spatiotemporary resolution and high precision. We selected the Moderate Resolution Imaging Spectroradiometer (MODIS) science products to verify the accuracy of the Advanced Himawari Imager (AHI) operational products and model-based retrieval results during the daytime, and found that the accuracy of the cloud top height (CTH), cloud optical thickness (COT), and cloud effective radius (CER) retrieved by the model (CTH: 1.904 km, COT: 11.198, CER: 4.490 µm) is higher than that of AHI operational products (CTH: 2.860 km, COT: 14.755, CER: 11.172 µm). We also selected CALIPSO official cloud products to verify the accuracy of CTH and COT, and selected CloudSat official cloud products to evaluate the accuracy of CER. Results show that the accuracy of the model during the day (CTH: 1.99 km, COT: 15.60, CER: 9.62 µm) is higher than that of AHI operational products (CTH: 2.99 km, COT: 23.71, CER: 14.81 µm), and the difference of the accuracy of the model during day and night (CTH: 3.00 km, COT: 17.10, CER: 12.64 µm) is relatively small. These results indicate that the all-day cloud retrieval model maintains stable ability during day and night, and the accuracy of the model is higher than that of Himawari-8 AHI operational products. Overall, the model is capable of retrieving all-day cloud properties with high precision and high spatiotemporal resolution, helping people better understand the role of clouds in the Earth-atmosphere system.
IG27-A004
Enhancing Inter-calibration Consistency of Geostationary Imagers Through Comparative Analysis with NOAA-20 VIIRS
Taeyoung CHOI1#+, Changyong CAO2, Xi SHAO3,4, Sirish UPRETY3,4
1NOAA/GST, 2NOAA National Environmental Satellite, Data, and Information Service, 3National Oceanic and Atmospheric Administration, 4University of Maryland
Satellite-based remote sensing plays a pivotal role in weather, environmental, and climate studies, demanding high-quality and consistent level-1b radiance data products. This paper investigates the on-orbit calibration consistency among several geostationary imager platforms, launched by different countries, with a focus on their solar channels comparable to the Visible Infrared Imaging Radiometer Suite (VIIRS) onboard the National Oceanic and Atmospheric Administration's (NOAA) NOAA-20 satellite. Geostationary imagers such as Advanced Baseline Imager (ABI), Advanced Himawari Imager (AHI), and GEO-KOMPSAT-2A (GK2A) in the Geo-Ring initiative face challenges in consistent on-orbit calibration, owing to technological constraints such as moon-based calibration subject to lunar observations at various moon phase angles and uncertainties in lunar irradiance models, partial aperture of onboard solar diffusers, and large diurnal temperature variations. In contrast, the solar bands of NOAA-20 VIIRS have exhibited remarkable stability since launch, with fluctuations as low as 0.5% over a six-year period. NOAA-20 VIIRS has been selected by the GSICS (Global Space-based Inter-Calibration System) as the LEO imaging sensor reference. This study presents a demonstrative analysis of the frequent Simultaneous Nadir Overpass (SNO) observations between NOAA-20 VIIRS and selected geostationary imagers. The radiometric inter-consistencies between solar bands of LEO and GEO imagers are quantified after accounting for the spectral response function difference between geostationary imager bands and VIIRS. Furthermore, by using NOAA-20 VIIRS as the transfer reference, the inter-GEO sensor relative radiometric biases are also evaluated. This study underscores the importance of maintaining consistent GEO-LEO and GEO-GEO Level-1b products for downstream data quality. The findings presented here will help advancements in satellite instrumentation and calibration strategies, ensuring the continued accuracy and integrity of LEO and GEO imaging data essential for scientific research and applications in meteorology, environmental monitoring, and climate studies.
IG27-A009
Estimation of Land Surface Albedo Using Time-series Data from Himawari-8 AHI
Wei LI1#+, Kazuhito ICHII1, Beichen ZHANG1, Yuhei YAMAMOTO1, Wei YANG1, Taiga SASAGAWA1, Kenlo NASAHARA2
1Chiba University, 2University of Tsukuba
Himawari8 is a 3rd generation of Japanese geostationary orbit (GEO) meteorological satellites that carries one sensor, the Advanced Himawari-Imager (AHI). Since the Himawari-8 AHI continuously observes the Earth's hemisphere in multiple spectral bands every 10 minutes, its observation dataset is effective in reducing vacancies caused by clouds as well as detecting sudden changes on the ground. Land Surface albedo (LSA) plays a crucial role in the Earth's climate system, as it determines the fraction of incoming solar radiation that is reflected back into space, thereby understanding, and accurately measuring LSA is essential for climate modeling and predicting environmental changes. This study aims to estimate LSA using Himawari-8 AHI. We applied the kernel-driven Bidirectional Reflectance Distribution Function (BRDF) model as well as the 10-minute resolution AHI land surface reflectance dataset to estimate the BRDF parameters using different synthesized periods, and then calculated the black-sky and white-sky albedo, respectively. The validation of our results entailed comparisons with ground-based measurements from the Ground-Based Observations for Validation (GBOV) and the Moderate Resolution Imaging Spectroradiometer (MODIS) LSA product. The results show good agreement between our results and the ground-based observations and MODIS results. Moreover, the AHI's hyper-temporal resolution enables the acquisition of continuous LSA measurements than MODIS from data spanning 3-5 days in non-tropical regions and 16 days in tropical regions. The results show the potential of our results for continuous LSA observations in Himawari-8.
IG27-A026
Surface Solar Radiation Compositions Observed from New Geostationary Satellites Over the East Asia-pacific Region
Chong SHI1#+, Husi LETU2, Run MA2, Takashi NAKAJIMA3, Teruyuki NAKAJIMA4, Jun LI5, Peng ZHANG6, Jian XU7, Jiancheng SHI2, Liangfu CHEN2, Gegen TANA2, Anthony BARAN8,9, Huazhe SHANG2, Sude BILIGE10
1Aerospace Information Research Institute, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Tokai University, 4National Institute for Environmental Studies, 5China Meteorological Administration, 6National Satellite Meteorological Center, 7National Space Science Center, Chinese Academy of Sciences, 8Met Office, 9University of Hertfordshire, 10Inner Mongolia Normal University
Surface downward solar radiation compositions (SSRC), including photosynthetically active radiation (PAR), ultraviolet-A (UVA), ultraviolet-B (UVB), and shortwave radiation (SWR), with high spatial–temporal resolutions and precision are essential for applications including solar power, vegetation photosynthesis, and environmental health. The new-generation geostationary satellites, such as Himawari-8 and FY-4, provide an unprecedented opportunity to derive SSRC with high spatio-temporal resolution over the East Asia–Pacific (EAP) region. In this study, we develop a near-real time monitoring system and an advanced retrieval algorithm for the SSRC observation in the EAP region. Key features of the algorithm include combining the radiative transfer model with machine learning techniques, including full consideration of the effects of aerosol types, cloud phases, and gas components. Satellite SSRC products and the monitoring system are available in the CARE home page (http://www.slrss.cn/care_zh/).
IG27-A019
Improve the Geometric Accuracy of FY4/AGRI for Terrestrial Remote Sensing Applications
Xuanlong MA1#+, Zhenduo DENG1, Yuanyuan WANG2
1Lanzhou University, 2National Satellite Meteorological Centre
The FengYun-4 (FY4) is China's second-generation geostationary meteorological satellite series, operated by the National Satellite Meteorological Centre (NSMC). The Advanced Geostationary Radiation Imager (AGRI) aboard both the FY4A, launched in 2016, and the FY4B, deployed in 2021. The AGRI has a high spatial resolution, with 0.5 km for the red channel and 1 km for the near-infrared (NIR) channel. It performs full-disk scans every 15 minutes, providing a unique opportunity to monitor time-sensitive terrestrial phenomena, such as plant photosynthesis and transpiration. The geometric accuracy of the FY4/AGRI, initially corrected using the 4 km TIR channel by the NSMC, has not been extensively evaluated. Questions remain about whether more precise corrections are necessary to enhance its suitability for terrestrial remote sensing. Here we evaluated the spatial and temporal variations in geometric errors within the FY4/AGRI Level 1 data provided by NSMC. We found that the data exhibited variable geolocation offsets across the full disk, with significantly larger discrepancies at the image's periphery compared to its center. For example, an image captured on October 1, 2023, above the southern coast of Australia, exhibited a shift of 3-4 pixels eastward and 2-3 pixels southward. Furthermore, we observed that the geometric errors fluctuated over time, thereby reinforcing the need for refined geometric correction. To address this, we implemented a phase-only correction (POC) method, leveraging the high-resolution channel 2 data from AGRI (0.5 km resolution centered at 0.65 µm). The Global Self-consistent, Hierarchical, High-resolution Geography (GSHHG) database provided the shoreline polygons used as the reference for our corrections. The POC method demonstrated a robust capacity for improving geometric accuracy and proved to be sufficiently rapid for operational use. Overall, our approach refined the geometric accuracy of the original NSMC FY4/AGRI data, a critical step toward reliable quantitative terrestrial remote sensing applications.
Session Chair(s): Ping-Yu CHANG, National Central University
IG12-A002
Fluid Inclusion Evidence for Fracture-controlled Natural Gas Migration: A Case Study of Majiagou Formation in the Central Ordos Basin
Yanwei FENG#+, Yong CHEN
China University of Petroleum (East China)
The study of fluid inclusions can obtain the information of homogeneous temperature, freezing point temperature, salinity, pressure, which is an effective means to study oil and gas filling periods, reservoir formation times, and oil and gas transportation directions. By studying the methane-bearing fluid inclusions and contemporaneous aqueous inclusions, the formation period of natural gas can be determined, which is also important for studying the migration of natural gas and other issues. Taking the Member-5 of Ordovician Majiagou Formation in the central Ordos Basin as an example, the relationship between migration direction of natural gas and fault activities was investigated based on integrated observations of fluid inclusion petrology, laser-Raman spectroscopy, micro-thermometric measurements, and thermodynamic PVT simulation. The results indicate that the minerals in the veins of structural fractures are calcite, dolomite and magnesite. There are four types of fluid inclusions found in the veins, including methane-rich gas inclusions, CO2-bearing and methane-rich gas inclusions, methane-bearing aqueous inclusions and brine aqueous inclusions. The homogenization temperatures of the methane-bearing fluid inclusions ranged from 130.1℃ to 179.6℃, while the homogenization temperatures of the coexisting aqueous inclusions were in the ranges 112.3℃ to 173.3℃. Combined with the history of hydrocarbon generation and strata burial, the Early Cretaceous is the important period of natural gas accumulation for the Majiagou Formation in studied area. While, Early Cretaceous tectonic movement produced a large number of structural fractures by the Northeast-oriented faults. As the fluid inclusions in veins recorded the fluids of natural gas migration, experimental results prove that structural fractures had been channels for the migration of natural gas. The trapping pressures of fluid inclusions and pressure coefficients show a decreasing trend from SW to NE along the faults, which implies that the methane-bearing fluids migrated along the NE-trending faults.
IG12-A004
Stages of Hydrocarbon Accumulation and Reservoir Diagenetic Evolution of Qixia Reservoir in Shuangyushi Area, Northwest Sichuan Basin, China
Rui NI#+, Yong CHEN
China University of Petroleum (East China)
Based on drilling core observation, combined polarizing microscopic observation for thin section, cathodoluminescence and fluid inclusion analysis, this paper discusses hydrocarbon accumulation and diagenetic evolution of Qixia Formation in Shuangyushi in northwestern Sichuan. The results indicate that the upper reservoir of Qixia Formation of Shuangyushi in northwest Sichuan is sparry cloud limestone, and its fillings of diagenetic mineral can be divided into four stages, including early fine crystalline calcite, recrystallized calcite, quartz and albite filled in early limestone holes, and dolomite and calcite filled in pore cracks. Combined with the characteristics of fluid inclusions in different diagenetic stages and tectonic burial history analysis, it is found that study area experienced overall subsidence and deposition from Permian to Middle Triassic, recrystallized calcite was formed due to the increase of burial depth and hydrothermal action associated with Emei taphrogeny. The early-middle Triassic to middle Jurassic lower Cambrian source rocks reached the peak of oil generation, leading to the first stage of oil charged into Qixia Formation reservoir. Then the middle and lower Permian source rocks reached the peak of oil generation in the Early Jurassic and Early Cretaceous, representing the second stage of oil charging. Quartz and albite were formed due to the charging of silica-rich hydrothermal fluid. At the same time, due to the burial depth and the transformation of hydrothermal fluid, part of the crude oil cracked into bitumen, and the ancient gas reservoir began to form gradually. The Longmenshan area experienced continuous thrust deformation in the middle and late Mesozoic from late Yanshanian to Himalayan, structural fractures were filled with dolomite and calcite. Methane and asphalt inclusions were captured in the vein calcite, and the ancient gas reservoirs were adjusted accordingly, which indicated the characteristics of early accumulation and late adjustment. This paper is supported by fund 42173042.
IG12-A005
Hydrocarbon Accumulation Period of Sangonghe Formation in Central Junggar Basin
Hui ZHANG#+, Yong CHEN, Miao WANG
China University of Petroleum (East China)
The central region of the Junggar Basin has complex conditions for hydrocarbon accumulation, and the fluid inclusions and solid bitumens associated with oil and gas activities provide evidence for the deducing of the accumulation process. By using samples from the Triassic Sangonghe Formation reservoir, conclusions can be drawn through methods such as solid bitumen maturity (laser Raman spectroscopy, reflectance), oil source (biomarkers), and systematic analysis of fluid inclusion lithology, fluorescence spectra, and microthermometry. The following conclusions have been reached: The solid bitumens with low maturity (equivalent vitrinite reflectance ranging from 0.62% to 0.79%) originate from the source rocks of the Permian Fengcheng Formation and Lower Wuerhe Formation. Hydrocarbon inclusions are mainly found in two forms: early-stage inclusions within mineral particle fractures, showing yellow-green fluorescence (λmax=504~515, Q650/500=0.43~0.72); and late-stage inclusions within mineral fractures piercing through particles, showing blue-white fluorescence (λmax=462~469, Q650/500=0.21~0.32m). The homogenization temperature of the saline inclusions that coexisting with the first generation of hydrocarbon inclusions is 100~120°C, with a salinity range of 6.45~9.21 wt% (Eq.NaCl). The homogenization temperature of the saline inclusions that coexisting with second generation of hydrocarbon inclusions is 110~140°C, with a salinity range of 3.39~6.45 wt% (Eq.NaCl). Considering the tectonic evolution history, hydrocarbon generation and burial history, it is believed that there was the earliest oil and gas accumulation in the Early to Middle Jurassic in the study area. The tectonic uplift and erosion at the end of the Jurassic led to the destruction of the ancient oil reservoirs and the formation of solid bitumens. Subsequently, there were two periods of oil and gas accumulation in the Early Cretaceous and the Paleogene.
IG12-A006
An Identification Method of Fluid Inclusion for In-situ Cracking of Crude Oil
Yifan SONG#+, Yong CHEN, Miao WANG
China University of Petroleum (East China)
Natural gas formed by cracking of crude oil occurs in many basins globally. One of the key questions about such gas is whether it was produced by in-situ cracking of crude oil. Here, we propose a model for identifying in-situ cracking of crude oil based on fluid inclusion assemblages (FIAs). This model divides the crude oil cracking process into three main stages. Before cracking, only liquid oil and aqueous fluid are present in a reservoir, and two types of inclusions may be formed. During cracking, the reservoir may host up to four fluid phases (residual oil, aqueous fluid, natural gas, and solid bitumen), and in theory as many as fourteen types fluid inclusions can be trapped, which can be considered evidence for in-situ cracking. After complete cracking, liquid oil has been exhausted and only natural gas, solid bitumen and aqueous fluid remain in the reservoir; at this stage, up to six fluid inclusion types can be trapped, which can be indicative of cracking. We applied this model to study the genesis of natural gas in the Sinian Dengying Formation reservoir of the Anyue Gas Field in the Sichuan Basin. Six types of hydrocarbon-bearing primary inclusions were observed in fluorite. Notably, one type of inclusion showed consistent volumetric phase ratios of solid bitumen plus gas, suggesting that these inclusions originally captured crude oil, which subsequently underwent in-situ cracking in a closed system. These FIAs are consistent with our model and suggest that the fluid inclusions trapped in fluorite can record the in-situ cracking of crude oil, and can therefore be used as direct evidence for the genesis of natural gas. This study was supported by the Natural Science Foundation of China (42173042, 41873070; 42102152;), the fellowship of China Postdoctoral Science Foundation (BX20200385; 2021M703581), and Natural Science Foundation of Shandong Province (ZR2021QD012).
IG12-A017
Machine Learning-driven Analysis of 2D and 3D Resistivity Data
Jordi Mahardika PUNTU+, Ping-Yu CHANG#
National Central University
Resistivity methods have undergone significant evolution since the 1920s, with considerable advancements in equipment. Despite this progress, challenges persist in achieving effective and accurate data analysis, especially when dealing with the complexities of interpreting models and integrating multi-resistivity data. This study tackles these challenges by introducing advanced processing steps and data analysis techniques through the integration of Machine Learning (ML) with Python-based modeling and visualization. In the 2D case, Unsupervised Machine Learning (UML) was employed to analyze forward modeling and field data, aiming to precisely delineate structures observed within the 2D sections. This involved generating six synthetic models and collecting nine time-lapse electrical resistivity datasets from the field. The inverted resistivity sections obtained were then subjected to UML analysis and validated using the silhouette index method. Results demonstrated a significant enhancement in the accuracy of boundary delineation and interpretation, with the optimal number of clusters for the field data determined to be 5. In the 3D case, a model was constructed from multi-resistivity data, including Vertical Electrical Sounding (VES), Transient Electromagnetic (TEM), and Normal Borehole Resistivity (NBR). These data were assimilated to build a 3D Resistivity model, subsequently transformed into a 3D apparent geological model using Supervised Machine Learning (SML). Upon validation using classification accuracy and F1 metrics, the random forest algorithm outperformed other algorithms, providing resistivity ranges for clay, sand, and gravel as log 0-1.8 Ωm, log 1.81-2.20 Ωm, and log >2.20 Ωm, respectively. Overall, this study delivers a significant improvement in 2D and 3D resistivity analysis, transitioning from a qualitative approach, based on subjective visual judgment, to a quantitative approach employing cutting-edge ML methods.
Session Chair(s): Youngryel RYU, Seoul National University, Weile WANG, NASA Ames Research Center
IG27-A014
Current Development Status of Land Surface Datasets Using Third Generation Geostationary Satellites by CEReS, Chiba University
Kazuhito ICHII#+, Yuhei YAMAMOTO, Beichen ZHANG, Wei LI, Wei YANG
Chiba University
Third generation geostationary satellites such as Himawari-8, GOES-R, GK2A, FY-4A, provide high temporal frequency observation of land surfaces with multiple solar reflective and thermal infrared bands. Center for Environmental Remote Sensing (CEReS), Chiba University group is developing multiple land surface datasets and conducting application of these datasets. In this study, we will show our current status of dataset generation of Himawari-8 AHI data. Our data processing includes generation of cloud mask, land surface reflectance (including BRDF correction), land surface temperature, LAI/FPAR, evapotranspiration and gross primary productivity. Along with the development of these datasets, we would like to show some case studies of application of these datasets.
IG27-A020
Desert Vegetation Phenology Analysis with GOES-R Advanced Baseline Imager NDVI
Tomoaki MIURA1,2#+, Leiana BEYER1
1University of Hawaii at Manoa, 2Japan Agency for Marine-Earth Science and Technology
The Geostationary Operational Environmental Satellite – R Series (GOES-R) is one of new-generation geostationary satellites, acquiring a variety of data for weather monitoring, science, and forecasting. The Advanced Baseline Imager (ABI) onboard the GOES-R satellite series images over the conterminous US at 5 min intervals, having the potential to generate higher-temporal resolution vegetation index (VI) time series data than the conventional polar-orbiting satellite sensors in seasonally heavily clouded areas. Vegetation phenology of the Sonoran desert in the Southwest US is influenced by the seasonal rainfall pattern. In other words, the start and length of the vegetation growing season (SOS and LOS, respectively) is controlled mainly by the timing and amount of the rainfalls. In our previous analysis of vegetation phenology in this area, conventional polar-orbiting satellite sensor (i.e., Moderate Resolution Imaging Spectroradiometer) data had a large data gap around the summer monsoon season, resulting in large uncertainties in the satellite-derived SOS and LOS. In this study, we assessed how the hypertemporal data from ABI could improve the SOS and LOS estimation relative to a conventional satellite sensor, Visible Infrared Imaging Spectroradiometer (VIIRS), in Arizona, USA. The temporal signatures of the normalized difference vegetation index (NDVI) derived from ABI and VIIRS were comparable overall, and both datasets were subject to variations associated with varying sun-target-view geometries to the same extent. The ABI NDVI data were, however, less subject to data gaps than the VIIRS NDVI data. Likewise, the ABI NDVI temporal signatures showed much finer temporal variations than the VIIRS NDVI for the former having a much larger number of observations. These results indicate that the ABI hypertemporal data are advantageous even for characterizing desert vegetation phenology.
IG27-A003
Detection and Attribution of Seasonal Variation in Vegetation Activities Across Southeast Asia Using Himawari-8 AHI
Hase MISAKI1#+, Kazuhito ICHII1, Yuhei YAMAMOTO1, Wei LI1, Beichen ZHANG1, Kumagai TOMO'OMI2, Yoshiaki HATA2, Chandra Shekhar DESHMUKH3, Masahito UEYAMA4
1Chiba University, 2The University of Tokyo, 3APRIL, 4Osaka Prefecture University
Seasonal changes in vegetation activity over Southeast Asia and its driving environmental factors are still unknown. One of the reasons is the high cloud cover, which limits land surface observations from space. Conventional polar-orbiting satellites have difficulty in monitoring below the seasonal scale due to their low observation frequency. In contrast, Advanced Himawari Imager (AHI) onboard the Geostationary Earth Orbit satellite Himawari-8 has an observation frequency of 10 minutes and is expected to improve the acquisition frequency of clear-sky scenes. The purpose of this study is to capture the seasonal changes in vegetation by using Himawari-8, and furthermore, to evaluate the environmental factors that cause seasonal changes. To compare with AHI, MOD/MYD09GA products from Moderate Resolution Imaging Spectroradiometer (MODIS) were used. Normalized Difference Vegetation Index (NDVI) were calculated from each satellite atmospherically corrected reflectance datasets. To improve its accuracy, data with red band reflectance less than 0.01 or greater than 0.2 or Aerosol Optical Thickness greater than 0.6 were excluded. Each NDVI was composited for 16day maximum value. In site-based analysis, 16day composited NDVI was compared with Gross Primary Productivity (GPP) at sites from the target area. In spatial analysis, 16day composited AHI-NDVI was compared with climate variables such as precipitation, solar radiation, temperature, and soil moisture. The results in site-based analysis suggested that AHI has over 50 times higher acquisition of clear sky scene than MODIS. This greatly reduced the missing values in the MODIS-NDVI, and AHI-NDVI correlated much better with GPP than MODIS-NDVI at each site. This indicates that AHI can capture seasonal changes in more detail than MODIS. Also, in spatial analysis, the result of comparison between AHI-NDVI and climate variables showed that the environmental factors having impact on NDVI seasonal changes differed by landcover and the features of climate.
IG27-A008
Geostationary Satellite Reveals Dry Season Green-up of Southeast Asia Except Croplands
Jiaqi TIAN1#+, Xiangzhong LUO2
1Nanjing University, 2National University of Singapore
Southeast Asia is a global hotspot of natural carbon stock and biodiversity, however, the seasonality of its vegetation greenness remains unclear, which impedes our understanding of the vegetation-climate interaction in the region. Here, we utilized a new generation of geostationary satellite (i.e., Himawari-8) to examine the seasonal variations in vegetation greenness across Southeast Asia. We quantified the difference in NDVI between the dry and wet seasons (i.e., NDVId-w), and investigated the potential drivers for the seasonality in vegetation greenness. Across Southeast Asia, 63.4% of the regions (mainly rainforests and savannas) show positive (i.e., green-up in the dry season), while 36.6% of the regions (mainly croplands) show negative (i.e., green-up in the wet season). The positive anomaly in solar radiation is the main reason for the green-up of natural vegetation in the dry season, while a shift in climate sensitivity between the dry and wet seasons causes the green-up of croplands in the wet season. Our study provides an in-depth examination of vegetation greenness across Southeast Asia using geostationary satellite observations and uncovers potential factors underlying the seasonality.
IG27-A015
Monitoring Dynamic Vegetation Phenology with Combined Advanced Himawari Imager and MODIS Over Ozflux Sites
Alfredo HUETE1#+, Mahdi TAGHADOSI1, Ankur SRIVASTAVA1, Tomoaki MIURA2,3, Xuanlong MA4, Jamie CLEVERLY5
1University of Technology Sydney, 2University of Hawaii at Manoa, 3Japan Agency for Marine-Earth Science and Technology, 4Lanzhou University, 5James Cook University
Knowledge of climate change impacts on land surface phenology patterns for many regions in the Southern Hemisphere, including Australia, is sparse, resulting in a lack of understanding of the key factors driving spatial and temporal shifts in phenology responses. The Advanced Himawari Imager (AHI) onboard the Himawari-8/9 satellites provides high-temporal imagery to better understand how terrestrial ecosystems function by tracking important sub-daily and daily processes over multiple years. These sub-daily / daily processes include gross primary productivity (GPP), photosynthetic capacity, and phenological processes. The overall aim of this study was to gain deeper insights into the complex interplay between phenological dynamics and climate change across a diverse range of dryland to tropical biomes within Australia. The methodological approach included an evaluation of fusion and gap filling capabilities between MODIS and AHI observations and to explore and refine tower flux GPP and phenocam relationships with greenness and water stress indices through multiple compositing approaches. The combined AHI- MODIS data acquisition yielded higher quality, cloud-free data with increased landscape phenology fidelity, including better characterisation of vegetation index (VI) relationships with tower flux GPP measures. Adjustments in greenness compositing can better harmonise VI relationships with GPP fluxes. Overall, the improved biophysical understanding of ecosystem processes will enable better predictions of how ecosystems will respond to climate change (warming, drying, extreme events) and other disturbance regimes. The combined use of geostationary and polar orbiting satellite data will allow for a consistent comparison of a variety of ecosystem properties across all biomes and over long-term decadal time periods.
IG27-A006
High Spatiotemporal Resolution Satellite Data Reveal an Overestimation of Deforestation in Southeast Asian Tropical Forests
Seokjin HAHN1#+, Youngryel RYU1, Sungchan JEONG1, Juwon KONG2, Wonseok CHOI1
1Seoul National University, 2Yale University
Southeast Asian tropical forests, which is an important global carbon sink, has suffered deforestation from human activities and climate change. However, challenges in lacking spatiotemporal resolution of satellite sensors and data gap exacerbated from cloud cover, particularly across the wet tropical forest regions, limit the availability of reliable surface reflectance products. To address these limitations, we propose AGM-SNU (Analysis-ready data Generation Module developed in Seoul National University) that combines the polar orbiting satellites MODIS, Landsat-8 and Sentinel-2 with the geostationary satellite observations from GK-2A (GEO-KOMPSAT-2A). Our system consists of three processing steps: 1) preprocessing module including BRDF correction, histogram-based imagery harmonization and combination of GK-2A imagery into MODIS imagery, 2) image fusion algorithm (SFSDAF: enhanced Flexible Spatiotemporal Data Fusion) to combine coarse images and fine images and 3) gap-filling algorithm (NSPI: Neighborhood Similar Pixel Interpolator) to interpolate data gaps from cloud contamination. Our model generates daily gap-free images with 10 m spatial resolution. We comprehensively evaluated AGM-SNU surface reflectance using drone and tower-based hyperspectral in-situ ground truth data across different ecosystems in Republic of Korea. To estimate deforestation of Southeast Asian tropical forests, we generated high resolution daily gap-free AGM-SNU Surface Reflectance (AS-SR) from 2018 to 2022. We revealed overestimation of deforestation areas in MODIS compared to AS-SR using vegetation index thresholding method. Our findings support synergistic usage of polar orbiting satellites and geostationary satellites can improve estimation of deforestation areas and its trends over Southeast Asian tropical forests.
IG27-A005
GEOSIF: A Continental-scale Sub-daily Reconstructed Solar-induced Fluorescence Derived from OCO-3 and GK-2A Over Eastern Asia and Oceania
Sungchan JEONG#+
Seoul National University
The unique diurnal solar-induced chlorophyll fluorescence (SIF) sampling capability of OCO-3 can provide crucial insights into ecosystem dynamics at the sub-daily scale. However, potential applications of OCO-3 SIF have suffered from its inherent spatiotemporal discontinuity. In this study, we addressed the discontinuous observation coverage of OCO-3 SIF by utilizing information from continuous geostationary satellite observations from Geostationary Korea Multi-Purpose Satellite-2A (GK-2A). We generated continental-scale hourly reconstructed SIF over Eastern Asia and Oceania and comprehensively evaluated it. To do this, we trained an extreme gradient boosting model using OCO-3 SIF and GK-2A observations including four band Nadir BRDF Adjusted Reflectance (NBAR) (blue, green, red, and near-infrared), shortwave radiation, and vapor pressure deficit (VPD) using the data from August 2019 to July 2021. The reconstructed SIF showed robust agreement with OCO-3 SIF across diverse ecosystems, varying hours of the day, and different observation geometries (R2=0.68-79). We found the large relative importance of near-infrared reflectance, red reflectance, and shortwave radiation which explained 84.6% of SIF prediction. VPD played an increasing role under high-temperature conditions. The reconstructed SIF captured afternoon depression of photosynthesis across diverse ecosystems (63.9-88.9%), whose responses were consistent with the original OCO-3 SIF (65.5-90.2%). Our results showed a more pronounced afternoon depression in the physiological SIF yield than in a canopy structural proxy. In addition, diurnal changes in both canopy structural and physiological components of SIF showed a stronger relationship with VPD than that of temperature. These findings highlighted the benefits of the synergistic use of new-generation satellite observations to improve our understanding of large-scale diurnal ecosystem dynamics and its environmental drivers.
IG27-A017
Gross Primary Production and Transpiration Estimates at Eddy-covariance Flux Tower Sites by Data-driven Models, Geostationary Imagery, and Climate Data
Xiangming XIAO1#+, Li PAN1, Baihong PAN1, Cheng MENG1, Weile WANG2, Hirofumi HASHIMOTO2
1The University of Oklahoma, 2NASA Ames Research Center
Geostationary satellites provide observations of land surface at very high temporal resolution, which can be composited to generate daily data of land surface reflectance. Several publications have shown the potential of the surface reflectance from the geostationary satellites for characterization and monitoring of land surface dynamics. In this presentation, we will report a modeling work that uses daily composite data of land surface reflectance from the geostationary satellites, ERA5 climate data, and data-driven models to estimate daily gross primary production (GPP) and transpiration (T) at 10 sites equipped with eddy-covariance flux tower systems. This presentation is composed of three parts. First, we will introduce the Vegetation Photosynthesis Model (v3.0) and Vegetation Transpiration Model (v2.0). VPM estimates daily GPP (g C/m2/day) as a product of the amount of light absorbed by chlorophyll (APARchl) and light use efficiency. The major improvement of VPM v3.0 include (1) leaf traits (broadleaf vs needleleaf) for estimating light absorption, and (2) site-specific optimal air temperature for GPP (Topt-site). VTM estimates daily transpiration (mm H2O/day) as a product of daily GPP and transpiration ratio, which is estimated as an inverse of water use efficiency at the leaf level. Second, we will describe the data from the geostationary satellites in terms of the seasonal dynamics of surface reflectance and vegetation indices. Third, we will report the results of VPM (v3.0) and VTM (v2.0) simulations, driven by geostationary image data and ERA5 climate data; and the results of model accuracy and uncertainty, based on the carbon and water flux data as measured by the eddy-covariance flux tower systems. The results from this preliminary study at individual sites clearly lay out the foundation for us to further investigate the potential of geostationary satellites for modeling of GPP and T across the landscape and regional scales.
IG27-A001
Estimating Diurnal Gross Primary Production Considering Non-linearity with Absorbed Photosynthetically Active Radiation
Yuhei YAMAMOTO1#+, Kazuhito ICHII1, Wei YANG1, Youngryel RYU2, Minseok KANG3, Shohei MURAYAMA4, Su-Jin KIM5, Hideaki TAKENAKA1, Atsushi HIGUCHI1
1Chiba University, 2Seoul National University, 3National Center for Agro Meteorology, 4National Institute of Advanced Industrial Science and Technology, 5National Institute of Forest Science
The diurnal Gross Primary Production (GPP) of plants is crucial for detecting abrupt vegetation stress under hot/dry conditions and for comprehending the photosynthetic response during extreme events. Remote sensing based GPP estimation commonly employs Light Use Efficiency (LUE) models. The Japanese geostationary satellite Himawari-8/9 can estimate solar radiation, the main driver of photosynthetic activity, with a 10 min frequency. This enables regional estimation of diurnal GPP using an LUE model. In this study, we newly considered the direct/diffuse components of Absorbed photosynthetically active radiation (APAR) and the nonlinear relationship between APAR and GPP in the LUE model for more refined diurnal GPP estimation. The Eddy Covariance (EC)-LUE model was calibrated and validated using EC tower observations at four vegetation sites from June to August in 2016–2018. Estimation of direct/diffuse APAR requires direct and diffuse components of PAR and fraction of PAR (FPAR), respectively. PAR was estimated from the Himawari-8/9 solar radiation product. The diurnal FPAR was estimated from the solar zenith angle and canopy structure using the Forest Light Environment Simulator (FLiES). We compared the estimation accuracy of three models: conventional EC-LUE model, EC-LUE model considering the direct/diffuse APAR, and EC-LUE model incorporating the nonlinear relationship between APAR and GPP as a light response curve (LRC). The results showed that considering direct and diffuse APAR slightly suppressed the overestimation of daytime GPP under clear skies. In addition, the model incorporating LRC was found to improve underestimation under cloudy conditions as well as overestimation under clear skies.
IG27-A021
Hotspot Effect in Vegetation Canopy Reflectance: Observations and Modeling with Geostationary Himawari-8 Satellite Data
Wei YANG#+, Zhi QIAO
Chiba University
The hotspot effect refers to a special case of the bidirectional reflectance distribution function (BRDF) where backscattering reflectance increases rapidly. It happens when the solar and viewing directions coincide. The hotspot directional signatures can be used to remotely estimate canopy structure information for improving leaf biochemistry modeling, such as clumping index (CI), directional area scattering function (DASF), and spectral canopy scattering coefficients (CSC). The hotspot effect in vegetation canopy reflectance has been conventionally observed by field experiments or aerial remote sensing, which are limited in spatial and temporal coverages. As for satellite remote sensing, the Earth Polychromatic Imaging Camera (EPIC) launched to a sun-Earth Lagrange point orbit can observe the hotspot at a daily resolution, however, its spatial resolution is approximately 10 km. With the hyper-temporal (~10 minute) and improved radiometric resolutions, the third-generation geostationary meteorological satellites (e.g., Himawari-8) provide unprecedented opportunities to observe the hotpot effect at a moderate spatial resolution (0.5~1 km). In this study, we first extracted the hotspot directional signatures for different vegetation types using the Himawari-8 Advanced Himawari Imager (AHI) surface reflectance data. Then, a reflectance dataset composed of thousands of hotspot records was constructed to quantitatively evaluate the existing BRDF models. Finally, an enhanced version of Rahman-Pinty-Verstraete (ERPV) model was proposed to improve the simulation of hotspot signatures. The results indicated that the hotspot effects can be observed within approximately 14% days within one year for the full disk of Himawari data. Moreover, the proposed ERPV model noticeably outperformed exiting semi-empirical kernel-driven BRDF models and original RPV model in simulating the hotspot signatures for different vegetation types. The findings of this study are helpful for enhancing the applications of Geostationary satellite-based hotspot signatures in canopy reflectance.
Session Chair(s): Yunyue LI, Purdue University, Ping-Yu CHANG, National Central University
IG12-A020
Application of Vibroseis in Tunnel Geological Forward-prospecting
Jiansen WANG1#+, Bin LIU1, Xiangnan DING1, Xinji XU1, Gang FANG2
1Shandong University, 2National University of Singapore
Tunnel geological forward-prospecting technology can provide early detection of potential disasters, therefore ensuring the safe construction of the tunnel. This technology has now become a crucial aspect of the tunnel construction process. Currently, as the tunneling project progresses towards hazardous mountainous regions, the tunnel construction encounters intricate and fluctuating geological conditions, along with more severe safety hazards. The detection distance and accuracy of the existing tunnel seismic forward-prospecting method scarcely comply with the pressing disaster prevention requirements. Focusing on the need for long-distance and accurate detection of unfavorable geological structures, we have carried out research on the tunnel vibroseis method. In contrast to ground surface vibroseis exploration, the tunnel environment necessitates horizontal excitement, which poses a challenge for instrument development. We have developed a tunnel vibroseis instrument with an airbag topping component. After inflation, the airbag is capable of horizontally pushing the vibroseis, allowing it to couple with the surrounding rock and provide a substantial horizontal reaction force. Moreover, a time-frequency domain correlation method based on synchronized squeezed wavelet transform was presented to attenuate the wavelet sidelobe interference and obtain high quality similar pulse signals. Again in the time-frequency domain, a method of adaptive median filtering was suggested to sufficiently reduce the harmonic interference caused by horizontal excitation in tunnel environments. It is worth noting that the vibroseis wide-band seismic data can be perfectly matched with multi-scale waveform inversion to obtain the wave velocity distribution of the surrounding rock in front of the tunnel face. Several field case have proved that the self-developed vibroseis instrument and methods can effectively broaden the frequency band of tunnel seismic data, and improve the detection distance and accuracy. This abstract believe that vibroseis technology has a wide range of potential applications in tunnel geological forward-prospecting.
IG12-A021
Review of Mechanism of Intermediate-depth Earthquake
Dingding ZHANG1#+, Huiping ZHANG1, Heng ZHANG2, Yongsheng ZHOU1
1China Earthquake Administration, 2Chinese Academy of Sciences
It is generally believed that the mechanism of shallow earthquakes is producing brittle rupture and stick-slip friction along pre-existing faults, thereby releasing elastic strain energy to generate seismic waves. However, the mechanism of intermediate-depth earthquakes, whose focal depth is greater than 70km, is significantly different from shallow-depth earthquakes. The mechanism of intermediate-depth earthquakes has always been an important scientific question in the field of earth science, and it is also a long-term challenging problem. Geoscientists use different data and models to study this problem by different methods. For example, geophysicists use GPS, gravity field, electromagnetic wave field, seismic wave field, and seismic imaging technology. However, it is very complex for the geological structure where intermediate-depth earthquakes occur, and there are relatively weak constraints on pale-earthquakes. Structural geologists have conducted mineral chemistry of the pseudotachylyte produced by co-seismic slip, and studied structural deformation of related faults. However, the chronological data is still very lacking on pseudotachylyte. Tectonophysics use experiments to simulate earthquake process, such as frictional experiments. Based on these methods above, the main physical mechanisms of intermediate-depth earthquakes were proposed by several models, such as the dehydration fracture mechanism, phase change instability mechanism, shear melting instability mechanism, etc. However, these mechanisms are controversial. The occurrence of intermediate-depth earthquakes is accompanied by changes in temperature and pressure and the penetration of the melt and fluid as well as metamorphic reaction. Comprehensive research on metamorphism, chronology, experimental petrology and numerical simulation of the earthquake processes can provide a new window for exploring the mechanisms of intermediate-depth earthquakes.
IG12-A001
Multi-source and Multi-temporal Remote Sensing Images Analysis for the Ecological Assessment of the Futou Lake Watershed
Chang SUN#+, Xiaojun TAN
Huazhong University of Science and Technology
The study focuses on the analysis of remote sensing images to extract water bodies, classify land use, and compute and analyze ecological indices in the Futou Lake watershed from 1987 to 2022. The results reveal that: (1) During the periods 1985-2000, 2001-2010, and 2011-2020, the lake's average annual area was 176.72 km², 160.92 km², and 168.83 km², respectively. While there was a general decreasing trend in the area of water bodies, this trend has improved since 2010 due to ecological conservation programs. (2) Our system combines spatial control measures with cutting-edge neural network algorithms to effectively and timely monitor changes in water bodies. We use an upgraded U-Net++ convolutional neural network and the DeepLabV3+ network for water body extraction. (3) Since 1990, urban areas within watersheds have increased by an average of 2.75% annually. With the implementation of the "Grain-for-Green" policy, the vegetated area increased by 122.79 km² from 2010 to 2017. (4) During the "Grain-for-Green" project period, the Remote Sensing Ecological Index (RSEI) exhibited an upward trend along with an increase in vegetation area, indicating an improvement in the ecological environment. This study thoroughly investigated the impacts of urbanization on the watershed's environment and the positive role of ecological projects in promoting ecological restoration in the region. Additionally, the results demonstrate the potential of using advanced neural network techniques for efficient watershed monitoring, enabling quick and effective evaluation of the basin's ecological condition in the future.
IG12-A010
Automated National Shoreline Extraction and Spatio-temporal Change Analysis Using Remote Sensing Data
Ho Tin HUNG#+, Ya-Lun S. TSAI
National Taiwan University
National shoreline mapping is crucial for coastal management and tracking the dynamics of coastal geomorphology. However, traditional on-site surveys are labour-intensive and expensive due to the lengthy and rugged nature of shorelines. Advanced spaceborne remote sensing techniques have made high-quality open-source data more accessible, and multispectral-based shoreline extraction methods have been developed (Tsai and Tseng, 2023). In this research, we proposed an automated, cost-effective, and robust framework for global shoreline mapping using remote sensing data. The targeted national shoreline area is divided into sections with bounding boxes, and the remote sensing data for individual sections is selected based on data availability, data quality, and the tidal heights of the reference point of the bounding box. Subsequently, the remote sensing data for individual sections with tidal heights closest to zero is obtained. Principal component analysis (PCA) on multispectral data isolates the land and ocean surface and further extracts the shoreline. The United Kingdom shoreline area served as the pilot, including various types of shorelines and weather conditions, enabling the comparison of the model's robustness under different conditions. Preliminary results suggest that the proposed framework has high potential in automating shoreline mapping with adaptively selected remote sensing data. The proposed work holds great potential for shoreline extraction using remote sensing data for global application. Tsai, Ya-Lun & Tseng, Kuo-Hsin. (2023). Monitoring Multidecadal Coastline Change and Reconstructing Tidal Flat Topography. International Journal of Applied Earth Observation and Geoinformation. 118. 103260. 10.1016/j.jag.2023.103260.
IG12-A011
Early Holocene Paleoenvironment of Matsu Area Inferred from Stable Isotope Records of Archaeological Mollusk Shells
Horng-Sheng MII1#+, Kai-He LIN1, Meng-Yang LEE2, Kuang-Ti LI3, Shih-Wei WANG4
1National Taiwan Normal University, 2University of Taipei, 3Academia Sinica, 4National Museum of Natural Science
We have analyzed 531 stable isotope records of archaeological Mytilus shells collected from Liang Island archaeological sites (LDDWI; ~8300-7400 yrBP), Matsu area, 61 stable isotope records of modern Mytilus samples, and 36 hydrogen and oxygen isotope analyses of water samples collected from Matsu area to reconstruct the Holocene paleoenvironment of Matsu area. Mean hydrogen and oxygen isotope values of water samples are -4.2 ± 2.1‰ (N=18; V-SMOW) and -1.0 ± 0.3‰ for Nangan; and -3.7 ± 2.3‰ (N=18) and -1.0 ± 0.4‰ for Beigan, Matsu. Based on the isotope values and salinity observed, the water oxygen isotope values show the seasonal fluctuation and is related to the amount of freshwater mixed with the seawater. Mean carbon isotope values of 2 modern Mytilus shells are respectively -2.2 ± 0.6‰ (V-PDB; N=31; cooked) and -0.0 ± 0.4‰ (N=30; not cooked). Mean oxygen isotope values of 2 modern Mytilus shells are respectively -2.0 ± 0.7‰ (V-PDB) and -1.9 ± 0.6‰. Mean carbon and oxygen isotope values of 11 archaeological Mytilus shells are respectively 0.5 ± 0.5‰ and -1.2 ± 0.5‰ (N=531). There is no significant difference in mean carbon isotope values between modern not cooked and archaeological Mytilus shells. However, the mean oxygen isotope value of archaeological Mytilus shells is greater than that of modern. The ~8300-7400 yrBP water temperature was probably cooler than that of present. Seasonal fluctuation in oxygen isotope values are observed in both modern and archaeological samples. Based on the most well preserved six archaeological samples, the harvest seasons were Spring-Summer (N = 3), Summer-Autumn (N = 1), and Winter (N=2).
Session Chair(s): Zhonghua ZHENG, The University of Manchester, Ning ZHANG, Nanjing University, Jonathan JIANG, California Institute of Technology
IG32-A003
| Invited
Global Urban Canopy Parameters for the WRF Model
Weilin LIAO1#+, Yanman LI1, Ning ZHANG2, Xiaoping LIU1
1Sun Yat-sen University, 2Nanjing University
The intricacies of urban climate and environmental issues have become focal points of considerable attention in the 21st century. Numerical simulations serve as a vital tool for meteorological research and atmospheric science, offering higher spatiotemporal resolution meteorological data. Accurate representation of urban morphology parameters significantly enhances the precision of numerical simulation models in urban areas. However, despite available urban canopy parameters (UCP) data for 44 major cities in the US and 60 in China, a comprehensive global dataset representing urban morphology features is still lacking. This study aims to leverage existing global three-dimensional vector data of buildings (including building footprints and heights) to compile a comprehensive global UCP dataset. Using this dataset, the goal is to uncover regional characteristics of global urban morphology and enhance the performance of regional climate models (such as WRF) in simulating urban areas worldwide.
IG32-A006
Advancing Open Science in Atmospheric Research: Integrating Data Usability and Machine Learning
Jennifer WEI1#+, Irina GERASIMOV2, Thilanka MUNASINGHE3, Jihoon CHUNG3, Ethan CRUZ3, Neo KAZUKI3, Ying Tzu YU3, Zhi ZHENG3, Muhammad KHAN3
1NASA Goddard Space Flight Center, 2Adnet Systems, 3Rensselaer Polytechnic Institute
In the dynamic realm of atmospheric sciences, the convergence of data science methodologies and open data marks a transformative era, driving research advancements and nurturing aspiring scientists. This abstract highlights two pivotal projects that epitomize open science principles, aligning seamlessly with the session's objective of interdisciplinary synergy and the cultivation of emerging talent. As a NASA-certified data center, our foremost endeavor focuses on enhancing the visibility and traceability of NASA datasets within atmospheric science research. This initiative not only elevates these datasets' prominence but also establishes a robust framework ensuring their credibility in scholarly discourse. By bridging the gap between data sources and research publications, this project serves as an educational catalyst, nurturing a new generation of scholars in open collaboration and dataset authenticity. Concurrently, our second project pioneers an early warning system for flooding events, utilizing machine learning algorithms to predict flooded fractions. Through multi-source data fusion and predictive modeling, this initiative goes beyond forecasting; it embodies the core of open science by enabling proactive risk mitigation strategies. This project not only advances atmospheric sciences but also fosters an environment where young scholars engage in practical, data-driven solutions. These intertwined projects exemplify the fusion of data science with open data solutions, ensuring both the usability of quality datasets and the cultivation of scientific knowledge among emerging scholars. By spotlighting these impactful use cases, our aim is to foster discussions emphasizing the importance of open collaboration, data integrity, and the nurturing of scientific talent in atmospheric sciences.
IG32-A001
Carbon Data and Knowledge Service and Governance at CASA E-science Platform
Jing ZHAO1#+, Guoqing LI1, Tuo WANG1, Jian WANG2
1Chinese Academy of Sciences, 2National Earth Observation Data Center
With the increase of carbon satellites, sensors and data types over the world, the volume of carbon data has grown rapidly. The multi-source carbon data itself also has multi-dimensional spatiotemporal characteristics. This situation not only brings great challenges to the management, storage, and organization of carbon data but also exposes the inefficiencies in data acquisition, sharing, time-series data organization analysis and services, and deficiencies in quality assessment of existing data service platforms. Since initiated by the Chinese Academy of Sciences (CAS) and the National Earth Observation Data Center (NODA) of China in 2018, Cooperation on the reanalysis of Carbon SAtellite data (CASA) has been working on the carbon data and knowledge service and governance with E-science platform in line with FAIR and CARE principles. Based on multi-faceted credible needs of different interoperability processes on multi-star carbon products (GOSAT, GOSAT-2, OCO-2/3, TanSat, Sentinel-5P, FY-3D, GF-5, DQ-1, and the second generation carbon satellites), software and models, knowledge, and based on CASA's existing two levels of interoperability systems (centralized interoperability system and federated interoperability system), we builds "Carbon Data Portal" and "Carbon Knowledge Portal" and “Online Analysis Platform” in the field of global carbon observation. Then we built a CASA knowledge hub with redundant knowledge traceability and comparison capability and an online analytics cloud with the ability to evaluate target data inventory quality. CASA's e-science platform realizes the interoperability of multiple information sources, the ability to select redundant information sources, the ability to collect and analyze with the Quantitative Diagnostic Index (QDI), and the ability to express integrated service products. It will extend the carbon data information “Trust” service and provide better ways to utilize carbon data across domains where innovation and integration are now necessarily needed.
IG32-A019
Enhancing Wildfire Monitoring: AI Solution Using Geostationary Satellite
Yoojin KANG#+, Jungho IM
Ulsan National Institute of Science and Technology
Wildfire monitoring is crucial for ensuring a rapid and efficient response to mitigate their impact. Satellite remote sensing has proven its usefulness, leveraging extensive observational coverage. In this study, the Advanced Himawari Imager (AHI) has been employed to develop an artificial intelligence solution for wildfire monitoring, taking advantage of its frequent revisit cycle. The AHI facilitate the creation of deep learning-driven models for both fire detection and Fire Radiative Power (FRP) estimation using Convolutional Neural Network (CNN) and the Attentive Interpretable Tabular Learning Neural Network, respectively. The CNN-based fire detection model demonstrated noteworthy performance characteristics, particularly in terms of high recall (0.84) and precision (0.97). The use of CNN model surpassed the effectiveness of AHI's active fire products, showcasing robustness and a spatial distribution similar to that of MODIS active fire products. For FRP estimation, the developed model exhibited notable efficacy, with a correlation coefficient of 0.92, a mean bias error of -0.34, and a mean absolute percentage error of 27% when compared to traditional FRP retrieval techniques. The study also highlighted their synergistic impact. The enhanced fire detection and FRP estimation models collectively addressed underestimation issues related to AHI, showcasing significant improvements in accuracy. Moreover, the integration of fire detection and FRP retrieval offers the advantage of real-time tracking of emissions. This is particularly crucial for understanding the environmental impact of wildfires promptly. In summary, the developed artificial intelligence solution, leveraging AHI data and advanced neural network architectures, emerges as a comprehensive and effective tool for wildfire monitoring.
IG32-A022
Case Study on the Analysis of Large-scale Wildfire Damage and Estimation of Carbon Emissions Using Satellite Remote Sensing
Joongbin LIM#+, Sungeun CHA, Jongsu YIM, Keunchang JANG, MyoungSoo WON
National Institute of Forest Science
In March 2022, a large-scale wildfire occurred in the eastern coastal region of Korea, including Gangneung, Donghae, Uljin, and Samcheok. This wildfire caused significant damage, and the Korea Forest Service, through field investigations, announced that the fire-affected area in Uljin and Samcheok was approximately 20,923 hectares (ha), and in Gangneung and Donghae, it was about 4,000 hectares. The National Institute of Forest Science estimated the carbon emissions caused by the wildfire through the analysis of satellite images. For this study, Sentinel-2 satellite imagery and National Forest Inventory (NFI) data were utilized for the analysis. According to this analysis, the fire-affected area in Uljin and Samcheok was estimated to be about 18,329 hectares, and in Gangneung and Donghae, about 4,687 hectares. The carbon dioxide emissions from these wildfires were estimated to be approximately 1.05 million tons in Uljin and Samcheok, and about 260,000 tons in Gangneung and Donghae. Such analysis provides crucial baseline data for accurately assessing the impact of wildfires and for establishing future fire management and recovery plans.
IG32-A009
Two Crucial Issues in Impact Assessment Studies Using the CMIP6 Ensemble
Hideo SHIOGAMA#+
National Institute for Environmental Studies
Here we introduce two crucial issues in impact studies using the CMIP6 ensemble. The first issue is the ‘hot model’ problem. Because some climate models of CMIP6 (‘hot models’) were suggested to overestimate future global warming, the IPCC AR6 used the ‘assessed warming range’ instead of that in the raw ensemble. However, it is not clear how this advance in climate science can contribute to reducing climate-related uncertainties in impact assessments. Here, we show that the climate-related uncertainty of the economic impact of climate change in the world can be observationally constrained (31% of variance can be reduced under RCP4.5 or SSP2-4.5). Please see Shiogama et al. (2022, ERL, https://doi.org/10.1088/1748-9326/aca68d) for more details. The second issue is the ‘distinctiveness’ of SSP3-7.0. Because recent mitigation efforts have made high GHG emissions of SSP5-8.5 highly unlikely, SSP3-7.0 has received attention as an alternative high-end scenario for impact studies. However, the ‘distinctiveness’ of SSP3-7.0 may not be well-recognized by the impact community. Aerosol emissions increase or change little in SSP3-7.0 due to the assumption of a lenient air quality policy, while they decrease in the other SSP-RCPs of CMIP6 and all the RCPs of CMIP5. Here, we show that large aerosol emissions in SSP3-7.0 significantly suppress future increases in precipitation. We recommend impact researchers to compare impact simulations at the same warming level between SSP3-7.0 and SSP5-8.5 to examine the effects of aerosols in the case that such analyses are adequate. We also recommend ScenarioMIP for CMIP7 to exclude scenarios with extreme policies of aerosols (and land-use land-cover changes) from Tier 1 experiments and instead including them in Tier 2. Please see Shiogama et al. (2023, Nat. Clim. Chang. https://doi.org/10.1038/s41558-023-01883-2).
IG32-A010
Temperature and Precipitation Change Over South China in CMIP5 and CMIP6 Models: Historical Simulation and Future Projection
Dongdong PENG1#+, Tianjun ZHOU2
1China Meteorological Administration, 2Chinese Academy of Sciences
Revealing regional climate changes is vital for policymaking activities related to climate change adaptation and mitigation. South China is a well-developed region with dense population, but the climate projection uncertainty remains unevaluated. Here, we assess the historical simulations and future projection of climate change in South China based on the CMIP5/CMIP6 models. We show evidence that CMIP5/CMIP6 models can well reproduce the observed distributions of annual/seasonal mean temperature but show much lower skills for the precipitation. CMIP6 models outperform CMIP5 models in the historical simulations, as evidenced by more models with lower bias magnitude and higher skill scores. During 2021-2100, the annual mean temperature over South China is projected to increase significantly at a rate (℃ decade-1) of 0.53 (0.42~0.63)/0.59 (0.52~0.66), while the precipitation is projected to increase slightly at a rate (% decade-1) of 0.8 (0.14~1.65)/1.64 (0.96~2.44), under RCP8.5/SSP5-8.5 scenario, respectively. CMIP6 models project larger annual/seasonal mean temperature and precipitation trends than CMIP5 models under the equivalent scenarios. South China would robustly increase by more than 1.5 ℃ during 2041-2060 under RCP4.5/SSP2-4.5 and 4.5 ℃ during 2081-2100 under RCP8.5/SSP5-8.5 with respect to 1850-1900. The projection uncertainty of temperature is mainly dominated by model uncertainty (larger in near-to-middle-term) and scenario uncertainty (long term), while internal variability uncertainty contributes some to the near-term projection. The precipitation projection uncertainty is mainly dominated by internal variability (larger in near term) and model uncertainty (middle-to-long term), while the contribution of scenario uncertainty is much smaller than those two and can be neglected.
IG32-A008
How Well are Mei-yu Fronts Represented in CMIP6 Models?
Gregor C. LECKEBUSCH1#+, Kelvin NG1, Kevin HODGES2
1University of Birmingham, 2University of Reading
Due to the substantial socioeconomic impact of the East Asian Summer Monsoon (EASM), a crucial area of research involves understanding how the EASM and, consequently, the hydrological cycle over East Asia might evolve in future climates. Addressing this requires the utilization of reliable climate models. While studies on model evaluation commonly focus on the precipitation amounts generated during the EASM period, it is noteworthy that dynamical components like the Mei-yu front (MYF) have often been overlooked. Consequently, model outputs may be correct for the wrong reasons, as the dynamical components of the EASM could be misrepresented. In this study, we studied the representation of the MYF in 38 CMIP6 models during the period from May to August, comparing them to ERA5. Our findings uncover that several CMIP6 models face challenges in accurately reproducing the climatology of the MYF, and this performance variation is observed across different months. By categorizing models based on the meridional bias of MYF climatology in May, we discover distinct monthly evolutions within these clusters. Furthermore, our investigation investigates into the sources of these biases. Our study highlights a noteworthy association between the misrepresentation of MYF climatology in CMIP6 models and the portrayal of the North Pacific High, especially its western edge. The implications of these findings are also discussed.
IG32-A012
On the Global Warming Projections: A New Way from a Generalized Stochastic Climate Model and the Comparison with CMIP Models
Naiming YUAN1#+, Christian FRANZKE2, Feilin XIONG3, Zuntao FU4, Wenjie DONG1
1Sun Yat-sen University, 2Pusan National University, 3Beijing Municipal Climate Center, 4Peking University
Despite recent progress, the current Earth System Models (ESM) still project a large range of possible warming levels. Here we employ a generalized stochastic climate model to derive a response operator which computes the global mean surface temperature (GMST) given specific forcing scenarios to quantify the impact of past emissions on current warming. This approach enables us to systematically separate between the “forcing-induced direct” and the “memory-induced indirect” warming trends. Moreover, the natural induced GMST variability may be separated and is in good agreement with the ESM simulations. Compared to CMIP6 simulations, our data-driven approach projects lower global warming levels over the next few decades. The results suggest that CMIP6 models may have a stronger persistent property than warranted from the observational record, and this may contribute to the overestimated warming trend from CMIP models.
Session Chair(s): Alexander WINKLER, Max-Planck-Institute for Biogeochemistry, Jungho IM, Ulsan National Institute of Science and Technology, Zhonghua ZHENG, The University of Manchester
IG32-A007
Estimating Near-surface Marine Air Temperature Using High-resolution Infrared Radiation Sounder Data and In Situ Observations
Yuhan RAO1#+, Jessica MATTHEWS2, Lei SHI2
1North Carolina State University, 2National Oceanic and Atmospheric Administration
Near-surface air temperature is one of the essential climate variables that play a key role in climate monitoring and applications. Historically, sea surface temperature (SST) has been used to monitor temperature change over the ocean surface as a proxy due to the lack of reliable and consistent near-surface marine air temperature (MAT). Since the late 1970s, polar-orbiting environmental satellites carried High-resolution Infrared Radiation Sounder (HIRS) to collect information across different pressure levels of the atmosphere globally. HIRS data has been used to estimate the temperature and humidity values at standard pressure levels including near-surface air temperature. However, the estimated temperature and humidity data have limitations because it is only available during clear-sky conditions. Despite the clear-sky-only nature, HIRS-based temperature estimates still provide useful information for monitoring the change of near-surface MAT. In this research, we present our method to create a blended near-surface MAT data set using a gradient-boosting tree model to combine HIRS temperature retrievals with ship- and buoy-based measurements of MAT from the International Comprehensive Ocean and Atmospheric Data Set (ICOADS). The gradient-boosting tree model was first trained using match-up data pairs between HIRS temperature retrievals and height-adjusted MAT observations from ICOADS and other ancillary data. The trained model was then evaluated using independent observations of near-surface MAT from diverse data sources including NOAA research ships and international field campaigns. The overall evaluation shows that the gradient-boosting tree model-based MAT estimates are accurate when compared with the independent observations (bias: 0.08K; RMSE: 1.1K). This method will allow us to estimate near-surface MAT globally from 1979 and can be extended using the most recent infrared sounding instruments which can provide more than 40 years of long-term records for climate monitoring and applications.
IG32-A016
21st Century Surface Temperature Trends and Tipping Points
Jonathan JIANG1#+, Yong-Sang CHOI2, Yuan WANG3, Peter KALMUS1, Yuk YUNG1
1California Institute of Technology, 2Ewha Womans University, 3Stanford University
Emerging studies signal imminent "tipping points" due to climate change. This research examines global surface temperature trends using observational data and climate model simulations. Our analysis shows regional disparities in global warming rates, with the Arctic undergoing warming over three times the global mean. Using latitude-dependent temperature simulations from various Coupled Model Intercomparison Project Phase 6 (CMIP6) models, we evaluate their precision against observational data and identify models mirroring historical latitude-based values. Temperature forecasts are derived from ensemble simulations of the Shared Socioeconomic Pathway 2–4.5 (SSP2–4.5) by these vetted CMIP6 models. We identify the projected years when surface temperatures might elevate by 1.5, 2.0, and 2.5°C above preindustrial benchmarks, globally and for specific regions. Particularly in the Arctic, the predictions indicate a significant temperature escalation with potential worldwide implications. Additionally, using the NCAR CESM model, we probe the climate system's reversibility—integral to understanding tipping points. Following the CMIP benchmark experiment, we escalate CO2 concentration by 1% annually. At each decade's outset, we initiate a sensitivity run, retracting CO2 to its starting value for that period. The concluding climate conditions, including surface temperature, sea ice proportion, and sea level ascent, are juxtaposed against their initial states, assessing reversibility across the century. This approach provides a comprehensive assessment of climate system tipping points, highlighting the diverse repercussions of greenhouse gas-driven warming on various climate facets.
IG32-A018
Burned Area Mapping Using Deep Learning Approach Based on Cubesat Images
Byeongcheol KIM+, Seonyoung PARK#
Seoul National University of Science and Technology
Forest fire is one of the dangerous natural disasters. The estimation for burned area by forest fire is important to determine administration where make plans to deal with it. Remote sensing approach can help to estimate the burned area. If cubesat operated in a constellation is used in forest fire cases, high spatiotemporal resolution images can be acquired. In this study, the PlanetScope post-fire imagery was used to map the burned area in four study areas. To map the burned area, surface reflectance of visible and near infrared (NIR) band images and vegetation indices were used. Because of the absence of a short-wave infrared band (SWIR) in PlanetScope, new SWIR was added by downscaling of Landsat 8 and Sentinel-2 SWIR images. In this study, U-Net model based on convolutional neural network was used to estimate the burned area. Image patches were separated by 60%, 20%, and 20% ratio for training, testing, and validation datasets. Six metrics—intersection-over-union (IoU), mean IoU, precision, recall, F1-score, and Kappa coefficient from the prediction map—were used to assess the performance of the models. As the result, some vegetation indices can help to estimate the burned area perimeter with visible bands. But some snow and rocky areas caused false alarms when identifying the burned area. Using SWIR band in these areas can be improved the accuracy of prediction map.
IG32-A024
Advancing Wildfire Prediction Through Simplicial Graph Neural Networks for Partial Differential Equations
Jae Won CHOI1#+, Yuzhou CHEN2, Hugo LEE3, Hyun-Cheol KIM4, Yulia GEL1
1The University of Texas at Dallas, 2Temple University, 3Jet Propulsion Laboratory, California Institute of Technology, 4NOAA Air Resources Laboratory
Predicting the dynamics of complex systems, such as wildfires, often involves solving partial differential equations (PDEs) on irregularly spaced data. Traditional numerical methods struggle with such irregularity, prompting the exploration of physics-informed machine learning (PIML). While deep learning, particularly graph neural networks (GNNs), has shown promise, existing PIML methods face limitations in describing higher-dimensional structural properties, especially those existing on manifolds. This study introduces Simplicial Graph Neural Networks for Partial Differential Equations (SGNN-PDE), incorporating elements of Hodge theory and simplicial convolution defined on the Hodge Laplacian. In contrast to conventional methods, simplicial convolution enables a rigorous description of diffusion across higher-order structures, allowing for a more accurate approximation of complex underlying topology and geometry of the data. The focus of this research is on analyzing the performance of SGNN-PDE on wildfire datasets in the Eastern and Western U.S. By leveraging synthetic data and real-world wildfire processes, we demonstrate that SGNN-PDE outperforms state-of-the-art baselines in handling unstructured grids and irregular time intervals. The results showcase SGNN-PDE's competitive forecasting capabilities for weather and air quality, with the best outcomes highlighted in bold, while underlined text denotes the runner-ups' achievements. This approach provides a computationally efficient and effective solution for time-dependent PDEs in wildfire prediction, contributing to the advancement of physics-informed machine learning methods.
IG32-A004
Deep Learning-based Tide Level Prediction in Tidal River Reach
Zhixu BAI1#+, Di MA2, Yutai KE1
1Wenzhou University, 2NingboTech University
Tide levels in tidal reaches are affected by multiple factors such as astronomical tides, storm surges and upstream water inflows. The establishment of a physical process-based tide level prediction model requires in-depth knowledge and understanding of hydraulics and hydrological models. Even so, it is still impossible to avoid the problems of high cost of complex model construction and low computational efficiency. In this study, the effects of multiple deep learning models in tide level forecasting in tide-sensing river sections are compared using rainfall, celestial cycle and other data. The results show that through certain debugging, the deep learning models can meet the requirements of tide level forecasting.
Session Chair(s): Dengfeng LIU, Xi'an University of Technology, Fubo ZHAO, Xi'an Jiaotong University, Bo MING, Xi'an University of Technology
IG30-A005
| Invited
Embodiment of Consumption and Conservation of Energy-intensive Industrial Water Resources Under the Motivation of Carbon Peaking Policy
Chao MA#, Weiwen LIU+, Haixing GOU, Weiren HUANG, Ruixin ZHANG
Tianjin University
To support China's carbon peaking and carbon neutrality goals, improving water conservation and reducing carbon emissions in energy-intensive industries is critical. This paper presented a new quantitative methodology for the assessment of industrial water consumption and conservation pathways motivated by carbon peaking policy. Focused on the nine provinces in Yellow River Basin from 2015 to 2030, this study estimated the whole-process water consumption of the electric power industry, which is the primary component of both energy-intensive and water-intensive sectors. Subsequently, decomposition analysis was used to identify the factors that affect changes in water consumption. Furthermore, the study evaluated the water conservation potential through scenario analysis. The results indicate that the total water consumption for power generation in nine provinces is expected to reach 5.13 billion m3 by 2030, with an average water consumption factor of 0.97 m3/MWh. Spatially, there is a general trend of decreasing water consumption factor from the upper regions of the Yellow River to the lower provinces. The increase in water consumption can be decoupled through scale, structure, and intensity effects, which have positive, negative, and negative impacts, respectively. By 2030, the nine provinces have the potential to conserve up to 3.96 billion m3 of water through substitution of clean energy, improvement of traditional technology, and transmission of interregional power. And the water conservation is primarily attributed to the substitution of the operation and fossil energy utilization phase in conventional industries. These results will significantly contribute to the future coordinated management of energy and water resources.
IG30-A017
| Invited
Geochemical Study in an Area Affected by Gold Mining in Choco, Colombia
Andres Felipe ZUÑIGA CABEZAS1#+, Pedro Francicsco RODRIGUEZ ESPINOSA1, M.P. JONATHAN1, Jose Luis MARRUGO NEGRETE2, Sandra Soledad MORALES GARCIA1
1Instituto Politécnico Nacional, 2Universidad de Cordoba
The Choco biogeographic zone, in the Atrato River basin, is a tropical ecosystem in northwestern Colombia with immense biodiversity and highly impacted by alluvial gold mining (formal and informal); historically linked to the ancestral production systems of the black communities in the area. These mining activities altered the hydrodynamic characteristics, encouraged extensive deforestation, sedimentation, contamination of water and sediments, decrease in fish populations, among other impacts, which led to the Atrato River and its tributaries, being declared as subject of law to ensure its protection by the T-622-2016 sentence of the Colombian Constitutional Court. This study aims at the geochemical characterization of the sediments of the Quito River (tributary of the Atrato River) for the development of restoration criteria for areas affected by alluvial gold mining in the riverbed. A sampling season (rainy season) was carried out with 63 sampling points located in the main channel of the river and its main tributaries, for which 50 elements were analyzed among major elements, trace elements, rare earths, precious elements and platinum group elements by ICP-OES, ICP-MS, INAA, FA-MS (specific method for precious elements) and Cold Vapor (specific method for Hg) by partial and total digestions (AR and TD respectively). Amid the results obtained were average concentrations for Al of 2.01 % and 4.61% (AR-ICP-MS and TD-ICP-OES) and Fe of 2.17% and 2.77% (AR-ICP-MS / INAA), Pb of 7.56 ppm and 7.97 ppm (AR-MS and TD-ICP-OES/TD-ICP-MS) As of 2.25 ppm and 4.07 ppm (AR-MS / INAA) among others.
IG30-A004
Global At-risk Basins of Socio-ecological Impacts from Water Scarcity
Fubo ZHAO1#+, Yiping WU2
1Xi'an Jiaotong University, 2Central South University of Forestry and Technology
Water scarcity has been increasingly impacting social and ecological systems in the context of climate change. However, the actual and potential impacts of water scarcity on these systems are rarely assessed on a global scale. Herein, we developed a framework that integrates water scarcity and climate sensitivity to assess the socio-ecological vulnerability of global basins. We found that basins that already experience water scarcity exhibit a disproportionate magnitude of climate sensitivity, exacerbating the challenges associated with managing water resources. We identified the at-risk basins by integrating socio-ecological vulnerability and found that the most at-risk basins (n = 21), which collectively accommodate 500 hundred million inhabitants, are mainly located in developing countries, implying the urgent need of international cooperation for reducing these vulnerabilities. Current Integrated Water Resources Management (IWRM) and Climate Change Adaptation (CCA) may not be enough to alleviate the water crisis and to adapt to climate change in these at-risk basins. We urge policy makers in at-risk regions to integrate integrated water resources management and climate change adaptation measures to synergistically achieve related sustainable goals.
IG30-A001
Estimation of Daily Evapotranspiration in Gully Area Scrub Ecosystems on Loess Plateau of China Based on Multisource Observation Data
Fengnian GUO1+, Dengfeng LIU1#, Shuhong MO1, Qiang HUANG1, Lan MA1, Shimeng XIE1, Wei DENG1, Guanghui MING2, Jingjing FAN3
1Xi'an University of Technology, 2Yellow River Engineering Consulting Co., Ltd., 3Hebei University of Engineering
Evapotranspiration is an important process in the hydrologic cycle. In this study, different types of daily evapotranspiration were accurately estimated and comparatively analyzed for 2020–2021 in the gully area of Loess Plateau, China with multisource observation data. The daily actual evapotranspiration was directly observed by the eddy covariance system and then compared with the daily evapotranspiration simulated by HYDRUS-1D, and they showed reasonable agreement and similar variability characteristics it with a correlation coefficient of 0.71. The FAO-56 Penman-Monteith equation was used to calculate the reference evapotranspiration and compared with the pan evaporation in the study area. The reference evapotranspiration has a single-peak pattern and seasonal variation, similar to the actual evapotranspiration process during the annual period. The crop coefficient had seasonal-variation characteristics and remained 0.8 in the mid-growth period. The correlation analysis between evapotranspiration and environmental factors at different time scales suggested that energy was the dominant factor affecting evapotranspiration in the study area. The validation results of the complementary relationship of evaporation indicated a significant asymmetric complementary relationship in the study area. Both generalized nonlinear complementary relationship functions have good applicability, but the performance of the sigmoid function was slightly better than that of the polynomial function. The results provided a reference for local water resource management and agricultural production.
IG30-A008
A Global Framework for Evaluation of Recultivation Benefit Integrating Satellite Remote Sensing and Integrated Assessment Model
Hongtak LEE1+, Hyungjun KIM1,2#
1Korea Advanced Institute of Science and Technology, 2The University of Tokyo
Due to changes of climate, crop yield, population structure, market circumstances, the area of abandoned agricultural land continues to increase, while human and nature are competing for limited resources such as land. Recultivation of abandoned cropland can be a considerable solution to expand food production, while minimizing human land use expansion and associated impact on the emission cycle. However, regional environmental and socio-economic conditions, which cause the abandonment of cropland, would remain and act as cost burdens to recultivation; desertification of cropland, increase in irrigation/transportation cost, reduction of workforce, industrial policy, etc. For the integrated cost analysis of recultivation, we designed a brief framework to categorize the global scale cropland abandonment and suggest re-initiation costs. The proposed framework was integrated into an open source IAM (e.g. Global Change Analysis Model) as a testbed for comprehensive land-use scenario development. For the preliminary results, remotely sensed surface properties (e.g., land cover/use, NDVI, surface temperature, topography) data were employed for the detection and classification of abandoned cropland. FAO(Food and Agriculture Organization of the United Nations) and ILO(International Labour Organization) statistics were also merged to evaluate the possibility of recultivation and the expected revenue of recultivated cropland. The framework in this study enables us to seek potential future pathways on varying agricultural conditions due to various human-natural dimensions (e.g., regional hydroclimatology, crop yield, and cost/subsidy), and to make further optimal recultivation/afforestation policies based on global-scale cost evaluation.
IG30-A014
Oreochromis Niloticus as a Bioindicator of the Valsequillo Dam, Atoyac Basin, Mexico: Trace Element and Microplastics a Health Risk
Estefania MARTINEZ-TAVERA1#+, S.B. SUJITHA2, Genoveva ROSANO ORTEGA1
1Universidad Popular Autónoma del Estado de Puebla, 2Instituto Politécnico Nacional
Fifteen Oreochromis niloticus (Tilapia) fish were collected in the Manuel Ávila Camacho (Valsequillo) dam in the area after the macrophyte consortium to investigate the presence of microplastics in their digestive system and trace element in liver and muscle. The determination of microplastics was made through a difference in densities finding in all of them 2 to 24 fibers, which were characterized by a field emission scanning electron microscope (FSEM) finding a greater number of microplastics in fish obtained in the area near the macrophytes and traces of As, Pb, Zn, and Cu. Similarly, when performing muscle and liver analysis of the same fish, Zn> Cu> Mn> Cr> Ba> Ni> Pb> Hg> As> Co> Cd> Mo and Zn> Cu> Mn> Cr> Ni were found > Ba> Pb> Mo> Co> Hg> As> Cd respectively exceeding the international and national standards recommended for human consumption in both for Mn, Cr, Cu and Zn. Likewise, it was identified through Fourier transform infrared spectroscopy that 33.333% of the particles correspond to cotton, 31.111% polyamide, 22.222% polyester, and 13.333% synthetic cellulose, resulting in 66.666% of the total synthetic particles. This study provides information on the consequences of pollution levels in the basin, where the dam, as the last part of the basin, functions as a pollutant receptor and artificial wetland. However, it visualizes the need for public policies that address the complex problem and comprehensive sanitation for the benefit of those who inhabit it.
IG30-A013
An Analysis of Several Factors Related to the Formation of a Sinkhole in Puebla Mexico
José Jorge CARACHEO GONZÁLEZ1+, Pedro Francicsco RODRIGUEZ ESPINOSA1#, Estefanía MARTÍNEZ TAVERA2, Ángel Refugio TERÁN CUEVAS1
1Instituto Politécnico Nacional, 2Universidad Popular Autónoma del Estado de Puebla
The relationship between anthropogenic activity and the environment implies a delicate balance of both subjects of study, when that balance is disturbed harmful phenomena is likely to happen, an example of this is the formation of sinkholes, a geomorphological depression caused by the sinking of the overlying layers of soil, happening on a sudden way, sinkholes are phenomena involving the interaction of water and soil. From a general definition, sinkholes are divided into two main branches, those produced naturally and those produced by anthropogenic activity. Sinkholes' occurrence is accelerated by human activities tend to be frequent and are also associated with the lowering of the groundwater level, sinkholes associated with this formation mechanism usually occur on soils made up of unconsolidated sediment deposits where voids naturally exist and where a phenomenon known as piping takes place where the voids in the soil interconnect and due to the loss of sediments the natural support of the soil is lost, this naturally leads to the loss of the soil's capacity to support itself and as a consequence it collapses. Sinkholes represent a huge risk for the human population because they can engulf houses or entire buildings, in the actual case study of the Juan C. Bonilla sinkhole in Puebla, Mexico, which occurred in 2021; swallowed a house almost entirely, likewise, sinkholes are also associated with climate change, due to the intensity of rainy days caused by global warming. In the last few years, places all over the world have experienced the occurrence of sinkholes of anthropogenic origin, in non-karst environments, the most important actions to be taken for its prevention are, in the first instance, the identification of risks and geological and geotechnical characteristics of the soil, as well as the correct management of water resources and planning of the available land.
Session Chair(s): Xiaojing LI, Second Institute of Oceanography, Ministry of Natural Resources
OS16-A001
| Invited
ENSO Teleconnections and the Probabilistic Prediction of the Atmosphere at Seasonal-to-decadal Time Scales in the Extratropics
Stéphane VANNITSEM#+, Jonathan DEMAEYER
Royal Meteorological Institute of Belgium
The dynamics of the atmosphere (and of the climate system) is known to display the property of sensitivity to initial conditions. This property has considerable impact on our abilities to make predictions at all timescales, in particular in the seasonal-to-decadal range. Model teleconnections are also affected by these errors, limiting the potential of extracting signals at long time scales. The impact of both initial condition and boundary condition errors on ensemble forecasts is extensively explored in a reduced-order coupled extratropical ocean-atmosphere model -- that was developed over the years -- forced by a Tropical model (Vannitsem et al, 2021), with a particular emphasis on the impact of Tropical teleconnections on extratropical predictability. In this perfect model framework, the analysis reveals that the potential of teleconnections in improving the quality of climate predictions could only be realized provided that the Tropical dynamics is accurately predicted (Vannitsem, 2023). References: Vannitsem, S., Demaeyer, J., & Ghil, M. Extratropical low-frequency variability with ENSO forcing: A reduced-order coupled model study. Journal of Advances in Modeling Earth Systems, 13, e2021MS002530, https://doi.org/10.1029/2021MS002530, 2021. Vannitsem S., Impact of tropical teleconnections on the long-range predictability of the atmosphere at midlatitudes: A reduced-order multi-scale model perspective, J. Phys. Complex. 4 045006, https://doi.org/10.1088/2632-072X/ad04e8, 2023.
OS16-A018
| Invited
Improving Forecasts of El Niño Diversity: A Nonlinear Forcing Singular Vector Approach
Wansuo DUAN1#+, Lingjiang TAO2
1Institute of Atmospheric Physics, Chinese Academy of Sciences, 2Nanjing University of Information Science & Technology
Observations indicate that two types of El Niño events exist: one is the EP-El Niño with a warming center in the eastern tropical Pacific, and the other is the CP-El Niño with large positive SST anomalies in the central tropical Pacific. Most current numerical models are not able to accurately identify the different types of El Niño. The present study examines the dynamic properties of the ENSO forecast system NFSV-ICM which combines an intermediate-complexity ENSO model (ICM) with a nonlinear forcing singular vector (NFSV)-based tendency perturbation forecast model. This system is able to distinguish the different types of El Niño in predictions. Hindcasts show that the NFSV-ICM system is able to capture the horizontal distribution of the SST anomalies and their amplitudes in the mature phase of not only EP El Niño events but also CP-El Niño events. The NFSV-ICM is also able to describe the evolution of SST anomalies associated with the two types of El Niño up to at least two-season lead times, while the corresponding forecasts with the ICM are limited to, at most, one-season lead times. These improvements are associated with the modifications of the atmospheric and ocean processes described by the ICM through the NFSV-based tendency perturbations. In particular, the thermocline and zonal advection feedback are strongly modified, and the conditions of the emergence of both EP- and CP-El Niño events are improved. The NFSV-ICM therefore provides a useful platform for studying ENSO dynamics and predictability associated with El Niño diversities.
OS16-A003
Multidecadal Changes of the Seasonal Potential Predictability of Winter PNA and Associated Circulation Anomalies
Xiaoqin YAN1#+, Youmin TANG2,1
1Hohai University, 2University of Northern British Columbia
Based on the Community Earth System Model (CESM) ensemble hindcast data in period of 1900-2014, the multidecadal changes in the seasonal potential predictability of the winter Pacific-North American (PNA) teleconnection pattern and associated circulation anomalies have been investigated by using an information-based metric of relative entropy and the method of the most predictable component analysis. Results show that the seasonal potential predictability of winter PNA has significant multidecadal changes, with values much higher at the two ends of the 20th century and much lower in between particularly in 1930s and 1940s. The changes of the seasonal potential predictability of winter PNA are mostly reflected by the temporal evolutions of PNA rather than the location changes of active centers. Further, the changes are mostly contributed by the external forcing of El Niño-Southern Oscillation (ENSO) related sea surface temperature anomalies in tropical central and eastern Pacific. In particular, the combined effect of relatively lower amplitudes, shorter persistence and more eastward warming centers leads to the reduced seasonal potential predictability of PNA and associated circulation changes in the 1930s and 1940s.
OS16-A020
Seasonal Prediction of the Indian Ocean Dipole Mode Using Model Analogs
Yanling WU1+, Youmin TANG2,1#
1Hohai University, 2University of Northern British Columbia
A retrospective tropical Indian Ocean dipole mode (IOD) hindcast for 1958–2014 was conducted using 20 models from the sixth phase of the Coupled Model Intercomparison Project (CMIP6), with a model-based analog forecast (MAF) method. In the MAF approach, forecast ensembles are extracted from preexisting model simulations by finding the states that initially best match an observed anomaly and tracking their subsequent evolution, with no additional model integrations. By optimizing the key factors in the MAF method, we suggest that the optimal domain for the analog criteria should be concentrated in the tropical Indian Ocean region for IOD predictions. Including external forcing trends improves the skills of the east and west poles of the IOD, but not the IOD prediction itself. The MAF IOD prediction showed comparable skills to the assimilation-initialized hindcast, with skillful predictions corresponding to a 4- and 3-month lead, respectively. The IOD forecast skill had significant decadal variations during the 55-year period, with low skill after the early 2000s and before 1985 and high skill during 1985–2000. This work offers a computational efficient and practical approach for seasonal prediction of the tropical Indian Ocean sea surface temperature.
OS16-A016
A New Baseline Metrics for Evaluating ENSO Prediction Skill: Ocean Dynamic Persistence
Tong LEE#+, Ou WANG
Jet Propulsion Laboratory, California Institute of Technology
ENSO prediction skill from coupled models is contributed by the accuracy of the initial ocean state and the fidelity of coupled models in representing ocean-atmosphere interaction after initialization. Coupled-model initialization shock or drift can suppress the contribution of an accurate initial ocean to ENSO prediction skill. However, it is not clear how much predictability the initial ocean state alone can provide for El Niño/La Niña evolution without considering subsequent ocean-atmosphere coupling. Here, we address this question by performing a set of 12-month hindcasts of the 3-D ocean state using a global ocean model. The ocean model is initialized from the initial condition at every month and every year from 1992 to 2017 obtained from the ECCO ocean state estimation (https://ecco-group.org/). During each 12-month hindcast, the atmospheric forcings are set to their seasonal climatology. Therefore, any interannual ocean anomaly in the 12-month hindcasts is solely due to the evolution of the initial ocean state without subsequent ocean-atmosphere coupling. We refer to this as ocean dynamic persistence. It contrasts the statistical persistence (a baseline evaluation metrics for predictions) that damps the initial anomaly statistically as a function of prediction lead time. We show that ocean dynamic persistence has much better skill in predicting the Niño3.4 sea surface temperature anomaly (SSTA), an ENSO index, than statistical persistence. Therefore, ocean dynamic persistence raises the bar for the baseline metrics of evaluating ENSO prediction skill. Moreover, ocean dynamic persistence hindcasts outperform most dynamical and statistical models up to several months of lead time. Our result highlights the substantial predictability of El Niño/La Niña provided by ocean dynamic persistence alone. It also underscores the importance of reducing coupled model initialization shock and drift to maximize the positive contribution of ocean dynamic persistence to ENSO prediction skill.
OS16-A011
Evaluating Performance of the North Pacific Victoria Mode as an ENSO Predictor Based on Multi-model Ensemble Hindcasts
Zhengyi REN1#+, Ruiqiang DING2, Zongrong LI1, Jiangyu MAO1, Kai JI3
1Chinese Academy of Sciences, 2Beijing Normal University, 3China University of Geosciences
The Victoria mode (VM), similar to the Pacific meridional mode (PMM), is forced by North Pacific Oscillation atmospheric variability. Both the boreal spring VM and PMM can trigger the onset of El Niño–Southern Oscillation (ENSO) events in the following winter. Previous studies have examined the precursor relationship between the PMM and ENSO based on a subset of models drawn from the North American Multimodel Ensemble (NMME) system. They suggested that the PMM can act as a precursor to El Niño events, whereas it fails to predict La Niña events. Utilizing the hindcasts of these models from NMME, this study further investigates the role of the VM as an ENSO predictor to examine the real usefulness of the VM for ENSO prediction. Compared with the PMM, the VM can predict both El Niño and La Niña events with some skill, showing that the VM seems to be a more reliable predictor of ENSO. We found that the unique role of the VM in ENSO prediction originates from the symmetric impact of the VM on ENSO events. The VM, as a basin-scale sea surface temperature (SST) pattern, combines the role of the SST over the subtropical northeastern Pacific that is similar to the PMM in initializing El Niño events with that of the SST over the western North Pacific that is different from PMM in initializing La Niña events, resulting in the symmetric effect of the VM on ENSO prediction. Thus, it is useful to consider VM variability as a reference for ENSO prediction.
Session Chair(s): Tanghua LI, Nanyang Technological University, Nicole KHAN, The University of Hong Kong
OS08-A011
| Invited
Sea-level Science in Singapore and Southeast Asia
Benjamin HORTON1,2#+, Yudhishthra NATHAN3, Trina NG3, Christabel TAN3, Fangyi TAN3, Yun Fann TOH3, Jennifer WEEKS4
1City University of Hong Kong, 2Imperial, 3Nanyang Technological University, 4Met Office
Here’s a depressing fact: sea-level rise through to 2050 is fixed. No matter how quickly nations lower emissions now, the world is looking at about 15 to 30 centimetres of sea-level rise through the middle of the century, given the long-drawn impact of global warming on the oceans and ice sheets. Even under a stable climate, sea-level rise is expected to continue slowly for centuries. Beyond 2050, sea-level rise becomes increasingly susceptible to the world’s emission choices. If countries choose to continue their current paths, greenhouse gas emissions will likely result in ~3°C of warming by 2100, and a sea-level rise of up to 0.8 metres. Under the most extreme emissions scenario, rapid ice sheet loss from Greenland and Antarctica could lead to a sea-level rise approaching 2 metres by the end of this century and over 5 metres by 2150.Using case studies from Singapore and Southeast Asia, we illustrate the ways in which current methodologies and historical and geological data sources can constrain future projections, and how accurate projections can motivate the development of new sea-level research questions to mitigate and adapt to climate change. For example, we focus on the implications of rising sea levels to coastal ecosystems. With 3°C of warming, nearly all the mangrove forests and coral reef islands would be beyond their sea-level rise tipping point for survival.
OS08-A017
A Late-holocene Relative Sea-level Record from Pulau Tekukor, Singapore
Nurul Syafiqah TAN#+, Jennifer QUYE-SAWYER, Fangyi TAN, Jing Ying YEO, Wan Lin NEO, Lin Thu AUNG, Junki KOMORI, Yiran WANG, Gina SARKAWI, Zihan AW, Aron J. MELTZNER
Nanyang Technological University
Sea-level rise varies globally, but the amounts and rates differ significantly spatially and temporally. Coastal communities and low-lying islands such as Singapore are vulnerable to changes in relative sea level (RSL) that can occur due to changes in the sea-surface and/or land height at a particular location. Accurately projecting RSL at any location requires an understanding of the local to regional drivers of RSL change, revealed by past instrumental and/or geological records of known RSL variability. In Singapore, there are few long tide-gauge records, and the only five published late-Holocene data points are characterized by high temporal and vertical uncertainty. In this study, we present new Late Holocene sea-level index points (SLIPs) from coral microatolls at Pulau Tekukor in Singapore. Coral microatolls are fixed biological indicators of RSL that record past RSL changes with high (centimetre- to decimetre-scale) vertical precision. Their vertical upward growth is limited by lowest tides, and changes in surface elevation along their cross-sectional profiles reflect RSL trends as the coral was growing. By combining established techniques such as field surveys and U-Th dating with newer ones such as structure-from-motion photogrammetry and the latest iPhone LiDAR, we show that SLIPs from Pulau Tekukor indicate that RSL was near present between ca.400 and 100 cal. years BP. We also compare our data with other Late Holocene records from Singapore and against glacial isostatic adjustment (GIA) model predictions for the region. This comparison will help us understand the drivers of RSL change for Singapore, which can aid in future projections.
OS08-A009
Holocene Sea-level Evolution in Western Australia
Nicole KHAN1#+, Michael O'LEARY2, Abang Mansyursyah Surya NUGRAHA3, Roger CREEL4, Rahul KUMAR3, Tanghua LI3, Adam SWITZER3
1The University of Hong Kong, 2The University of Western Australia, 3Nanyang Technological University, 4Columbia University
Records of Holocene relative sea-level (RSL) change from Western Australia, a far-field location distal to former polar ice sheets, offer important constraints on ice melt contributions to global mean sea-level (GMSL) change. Despite this, recent efforts to reconstruct RSL have been limited, and the nature of Holocene RSL evolution in Western Australia remains debated in part due to biased comparisons of data. Here we review, re-evaluate, and aggregate RSL data from Western Australia following international standard protocol and explore the potential of sedimentary archives from beach ridge systems of southwestern Australia to produce accurate, high-resolution records of RSL change. We use these data to test several working hypotheses about ice sheet contributions to GMSL change during the Holocene and the influence of local (e.g., non-stationary tides) or higher-frequency (e.g., El Niño Southern Oscillation) drivers of sea-level variability. Improved constraints on the behaviour of relative sea level during the Holocene will provide necessary data for enhancing our understanding of earth rheology, ice sheet dynamics, and natural variability of sea-level changes under warm, interglacial climate states.
OS08-A001
Rates, Causes, and Implications of Island-scale Relative Sea-level Rise in the Equatorial Western Pacific Ocean During the Past ~5000 Years
Andrew KEMP1#+, Juliet SEFTON2, Simon ENGELHART3
1Tufts University, 2Monash University, 3Durham University
Stratigraphies of organic, intertidal sediment (e.g., mangroves) are archives of relative sea-level (RSL) change. At equatorial latitudes, RSL fall from a mid‑Holocene highstand caused by ongoing glacio- and hydro-isostatic adjustment inhibits accumulation of thick, undisturbed sediment sequences. In some locations however, island-scale subsidence occurs at a sufficiently fast (and linear) rate to cause net RSL rise during the past ~5000 years. On these unique islands it is possible to generate detailed RSL reconstructions to address the scarcity of equatorial data for evaluating the long‑term relationship of global and regional sea level to climate variability. We present new RSL reconstructions developed from thick sequences of mangrove sediment at two locations (Federated States of Micronesia and Samoa) with different geological histories. Presence of the taraxerol biomarker confirms the mangrove-origin of the sediment, while radiocarbon dates and age-depth models quantify accumulation histories with uncertainty. From these records we infer that island subsidence can reach ~1 mm/yr, which is an order of magnitude faster than subsidence estimated from crustal loading and thermal cooling in Micronesia. The cause of this subsidence is enigmatic, but RSL reconstructions provide empirical targets for hypothesis testing. In Samoa, subsidence is likely driven by recent volcanic loading. The new RSL reconstructions are added to a global-scale database that when analyzed by a spatio-temporal model estimates centennial-scale variability in global mean sea level that appears coeval with climate forcing, including the onset of historic and unprecedented rise in the late 19th and early 20th centuries. Recognition that islands in Micronesia experienced late Holocene RSL rise rather than fall provokes revaluation of migration routes in(to) remote Oceania. We propose that evidence of human arrival was submerged by RSL rise, resulting in an estimated settlement age that is too young. Archaeological evidence in Samoa supports RSL rise.
OS08-A010
Glacial Isostatic Adjustment of the Mid-holocene Sea-level Highstand Along China Coast
Tanghua LI1#+, Nicole KHAN2, Howard Kwok Yin YU2, Yonghui QIN2, Fengling YU3, Benjamin HORTON4,5
1Nanyang Technological University, 2The University of Hong Kong, 3Xiamen University, 4City University of Hong Kong, 5Imperial
The mid-Holocene highstand is a common characteristic of Holocene relative sea-level (RSL) reconstructions from regions distal from ice sheets. A highstand occurs when sea level was higher than present-day levels. The mid-Holocene highstand’s timing, magnitude and spatial pattern vary due to hydro-isostatic processes including ocean syphoning and continental levering. However, these highstand properties are poorly constrained along China coast because of a lack of accurate highstand RSL data. Here, we ran an ensemble of Glacial Isostatic Adjustment (GIA) models with varying lithospheric thickness, upper and lower mantle viscosities (both 1D and 3D). We computed the mean and standard deviation of the GIA models and derived the highstand distribution pattern and magnitude range along China coast. We produced the “treasure map” to identify the regions that have the highest probability of the preservation of a highstand record. We validated the highstand “treasure map” with published records showing evidence for the mid-Holocene highstand. The “treasure map” reveals that regions that are very likely (> 90% probability) to have the highstand preservation include west and northeast coasts of Bohai Sea, southwest coast of Yellow Sea, Yangtze River Delta, and Pearl River Delta. The “treasure map” can guide future RSL data collection efforts.
OS08-A007
Drivers of Holocene Relative Sea-level Change in the Bohai and Yellow Seas
Yonghui QIN1#+, Nicole KHAN1, Ryan MCKENZIE1, Tanghua LI2, Howard Kwok Yin YU1
1The University of Hong Kong, 2Nanyang Technological University
Changes in Holocene relative sea-level (RSL) are driven by a combination of eustatic, glacial- and hydro-isostatic adjustment (GIA), tectonic and local processes. Unravelling drivers of RSL change in the past allows for more accurate projection of their contribution to future sea-level change. The Bohai and Yellow Seas are located far-field from polar ice sheets and therefore are predicted to experience a RSL highstand during the mid-Holocene due to the influence of GIA. In contrast, reconstructions based on geological records raise doubts about the existence of a mid-Holocene highstand in the west and east coasts of the Bohai Sea and Yellow Sea, respectively, underlining the potential contribution of local processes. Therefore, the influence of regional (GIA) and local drivers to RSL change in the Bohai and Yellow Seas remains unknown. Here, we present a quality controlled, spatially comprehensive database of Holocene RSL amalgamated from extensive literature sources from all coasts surrounding these seas. We document detailed information on the location, age, sedimentary facies, elevation, and associated uncertainties in their measurement for each sample in the database. We also review lithological, biological, and/or chemical evidence to (re)interpret the indicative meaning of indicators relative to tidal levels to standardize RSL data from different indicators and coastlines and allow comparison with minimal bias. Finally, we develop criteria to assess the quality of constraint that each sample provides on the position and timing of past RSL. By comparing RSL records in the database with GIA models, we estimate contributions from local processes including sediment compaction, paleo-tidal range change and local land subsidence/uplift. Our results will help to reveal the contribution of local- and regional drivers of the observed sea-level change in the Bohai and Yellow Seas.
OS08-A004
| Invited
Quaternary Sea-level Change and Vertical Crustal Motion Along the Japanese Coastline
Jun'ichi OKUNO#+
National Institute of Polar Research
The analysis of vertical crustal motion, induced by various tectonic processes, has been helped by examining observed relative sea level (RSL) changes during the past 130,000 years. In this study, we endeavor to calculate the mean rate of crustal displacement along the coastal regions of Japan across three distinct temporal scales: 50 years, 7 thousand years, and 125 thousand years, utilizing data from tide gauges, Holocene RSL records, and the elevations of marine terraces formed during the last interglacial period approximately 125,000 years ago. Our calculations incorporate sea-level variations within the 50-year timeframe, which are derived from tide gauge observations, thermosteric sea-level changes, numerical modeling for glacial isostatic adjustment (GIA) induced by the last glacial cycle, as well as recent ice melt from mountain glaciers, Greenland, and Antarctica. This study also addresses uncertainties of the crustal motion rate inferred from temporal sea-level changes during the mid-to-late Holocene and the last interglacial period, respectively, based on the comparisons between RSL observations and GIA modeling. Furthermore, we discuss the input parameters of GIA modeling, focusing on the viscosity structure of the mantle and the melting history of ice sheets and their impacts on sea-level predictions along the Japanese coastline.
OS08-A003
Annual Amplitude and Phase of the Self-gravitating Sea Level Changes Including Pole Tide Effect After 2011
Taehwan JEON1#+, Ki-Weon SEO1, Shin-Chan HAN2
1Seoul National University, 2University of Newcastle
Polar motion records for more than a century have shown that the Earth’s rotation axis is not fixed at a point but constantly moving due to the various mass changes of the rotating Earth. When the rotation axis changes, so does the centrifugal (rotational) potential of the Earth, which affects the spatially broad-scale ocean mass distribution. Since the observed polar motion is dominated by the periodic wobbles, such as the Chandler wobble and the annual wobble, the corresponding regional sea level change also showed the complex temporal variations due to the superposition of those different pole tide periods (433 and 365 days, respectively). However, the amplitude of Chandler wobble was drastically reduced since about 2010, and thus the pole tide-induced sea level change would show relatively regular annual variations. Contrary to the period before the Chandler wobble weakening, the current polar motion is expected to add the predictable and consistent annual sea level variations to the changes due to climate-related surface mass changes of the Earth. Thus in this study, we analyzed the annual behavior of self-gravitating sea level changes considering both climate-related surface mass changes and the pole tide effect for 2011-2021. The result indicates the significant annual phase shift and the amplitude decrease over the mid-latitude region of Asia and Oceania due to the pole tide effect. For example, the annual phase advance by 2-4 weeks is predicted along the coast of East Asia, and the Eastern Australia and New Zealand show the phase delay of 2-3 weeks and the amplitude decrease by 20-30%.
Session Chair(s): Hidekatsu YAMAZAKI, Tokyo University of Marine Science and Technology, Sung Yong KIM, Korea Advanced Institute of Science and Technology
OS13-A006
| Invited
Observed Oceanic Responses to Typhoons Based on High-frequency Radar Measurements
Jun WEI#+
Sun Yat-sen University
Based on the HF radar measurements, the inertial and sub-inertial current patterns during the typhoon Koguma’s passage over the northern South China Sea are presented in this study. Although the typhoon-induced inertial motions are well known and were examined extensively in previous studies, using either pointwise ADCPs or single-station radar measurements, this study presents a larger domain of current velocities collected from 4 HF radar stations. In contrast to the previous studies focusing on typhoon-induced inertial oscillations, we analyzed wide-range current patterns that captured the complete evolution of the dipole structure during the typhoon Koguma’s passage. The dipole structure lasted for 3~4 days only and such a short-lived spatial evolution cannot be captured by ADCP and single-station radar measurements.
OS13-A003
| Invited
The Development of the Lake Michigan Modeling and Observational System
Meng XIA1#+, Miaohua MAO2, Nowrin MOW1, Ayumi FUJISAKI-MANOME3, Bishnupriya SAHOO1
1University of Maryland Eastern Shore, 2Chinese Academy of Sciences, 3University of Michigan
Accurate simulations of wind-waves are vital in evaluating their impacts on lake and coastal dynamics, especially when wave observations are sparse. In this study, wind-waves in Lake Michigan were simulated and calibrated using the unstructured version of SWAN (un-SWAN), and then we evaluated the FVCOM based wave-current-surge interactions (WCSI) coupled model by implementing various mesh resolution. Sensitivity experiments using different wind sources indicated that the simulated storm surge forced with CFSv2 winds had the best agreement with NOAA-NOS observations. For the effect of WCSI, it mostly modifies the storm surge and wave height in the shallow water along the coastline and around islands, wherein wave-induced setup and the depth-induced breaking are intense. In particular, the coastal surge in Lake Michigan is attributed to both the remote and local winds. And this coupled wave-current modeling system was also improved to investigate the seasonal circulation, and also the particle dynamics by comparing with the observed drifters which were released at 10- to 50-m depths with strong nearshore isobaths-following in July. From the simulated seasonal circulation. It was found that the effects of lake bathymetry on gyre circulation are greater than river inputs, strait exchanges, waves, and grid resolutions. Finally, this model system was coupled with atmospheric model and also drive by the climate change model to investigate the Lake Michigan dynamics, and model simulations found that decadal averaged surface current speed can rise at a relative rate of 6.5% until 2049 following the strength of wind. This model system is also coupling with ice model to simulate the sediment dynamics at Southern Lake Michigan.
OS13-A025
A Powerful Oceanic Observation System: Cabled Observatory Oceans
Hidekatsu YAMAZAKI1,2#+, Mamoru TANAKA3, Marika TAKEUCHI4, Eiji MASUNAGA5
1Tokyo University of Marine Science and Technology, 2Okinawa Institute of Science and Technology, 3Tokyo University of Science, 4National Oceanography Centre, 5Ibaraki University
Coastal ocean environment exhibits rapid change in time and space. Continuous long term measurements of environmental data are scarce. Environmental parameters, such as temperature and salinity, change due to multi-scale physical processes, such as the Kuroshio and internal waves. A different scale of physical process affects planktonic ecosystem differently. In order to investigate how planktonic ecosystem responds to multi-scale physical processes, we have deployed a cabled observatory system (Oshima Coastal Environmental data Acquisition Network System, OCEANS) in coastal area of Habu port (Oshima island, Tokyo). OCEANS consists of a shore station and an underwater node. The node carries various physical, chemical, and biological sensors; such as CT sensor, T-string, ADCP, ADV, PAR, wave gage, plankton camera (CPICS), Chlorophyl/Turbidity and Hydrophone. OCEANS provided long-term data sets for these parameters, particularly planktonic images obtained from CPICS are unprecedented planktonic ecosystem time series, that provided a long-term time series of planktonic diversity index. We present the characteristics of plankton diversity index with respect to the other observed parameters. We also investigated planktonic behavior against mixing conditions for a short time scale. The time series also provided to investigate how turbulence intensity changes seasonally. In addition to these biological aspect results, we observed resonated trapped internal tides and successfully modeled the observed processes.
OS13-A040
Estimation of Three-dimensional Current Fields Using Coastal Acoustic Tomography System in the Yeosu Bay, Korea
Yerin HWANG1+, Eun-Joo LEE1, Hajin SONG1, Byoung Nam KIM2, Ho Kyung HA1, Yo Han CHOI3, Jae-Il KWON2, Jae-Hun PARK1#
1Inha University, 2Korea Institute of Ocean Science & Technology, 3Underwater Survey Technology 21
Observation of current speeds in coastal seas is important because it can provide useful information for ship operations, fishing activities, and rapid responses to marine disasters. Coastal acoustic tomography (CAT) is a technology that can monitor current velocity or water temperature using reciprocal acoustic signals between CAT stations in coastal seas. Unlike traditional observations, CAT can produce time-varying two- or three-dimensional (3-D) current fields. The results of previous studies using CAT systems have been limited to reproducing depth-averaged two-dimensional current fields. Utilizing results from a high-resolution ocean model, we developed a novel method for estimating 3-D current fields by combining the inverse method with an artificial intelligence (AI) model. First, utilizing the ray tracing model ‘Bellhop,’ reciprocal travel times among five CAT stations using the ocean model outputs are computed. These five stations correspond to the locations where in-situ CAT systems were established for continuous monitoring of current changes in Yeosu Bay, Korea. Subsequently, the range-averaged currents at the five layers were estimated by incorporating this travel time difference data into AI model trained using the same ocean model outputs. Finally, inverse method is applied to each layer to estimate the 3-D current fields. The validation results revealed that this method performed well, reasonably producing time-varying two-layer-like current fields. They occasionally reveal an out-of-phase relationship between the upper and lower layers depending on the tidal phases. This method yielded average RMSEs of less than 4 cm/s on six simulation paths. Furthermore, when the same method was applied to in-situ CAT observations, average correlation coefficient of the along-channel current of each layer was 0.92 or higher. These results indicate that our method can be applied to the monitoring of 3-D current fields in coastal seas using a CAT system.
OS13-A009
Observed Wave-current Interactions in the Kuroshio Extension Region
Jingkai LI1#+, Zhaohui CHEN1,2, Xin MA1, Hongxuan WU1
1Ocean University of China, 2Qingdao National Laboratory for Marine Science and Technology
Ocean wave-current interactions are important physical processes at the sea surface, possibly causing extreme sea states in particular conditions. Usually, the interactions are more significant in regions with strong waves and background currents. In this paper, focusing on the Kuroshio Extension, we use buoy-measured and altimeter-derived wave data to show the variations in wave and current properties due to their interactions. Statistically, the wave height can be underestimated/ overestimated by approximate 4% when the current and wave are in the opposite/ same direction; in the regions with warm/ cold eddies, the wave height and wavelength are larger/ smaller inside the eddy than the outside by about 6% and 13%/ 4% and 10%, and the wave direction is deflected by -17°/ 13°; the wavenumber spectra of wave height and surface current speed are highly correlated with a power law k-2 at scales between 20 to 200 km. Besides, the convergence and divergence of wave energy resulted from the current-induced refraction of swell are captured. From another point of view, the wave-induced Stokes drift calculated with the directional spectrum could account for 59% of the reanalysis surface currents. And the accuracy of estimated surface current can be improved by up to 16% by considering the Stokes drift. The study provides quantitative analysis of observed wave-current interactions in the Kuroshio Extension regions from multi-perspective.
OS13-A012
Biogeochemical Responses to the Kuroshio Meandering in the Marginal Seas Around Japan
Xu ZHANG1#+, Yusuke UCHIYAMA2, Yonggang LIU1, Eiji MASUNAGA3
1Peking University, 2Kobe University, 3Ibaraki University
Biological processes affect the global carbon cycle on all time scales. The Kuroshio is accompanied by intense eddy activities that affect biogeochemical processes around its path. In general, localized upwelling due to mesoscale cyclonic eddies brings nutrient-rich subsurface water to the nutrient-depleted upper ocean to intensify near-surface primary production. In the present study, a synoptic, retrospective downscaling ocean modeling is developed for the marginal seas along the Kuroshio off Japan based on ROMS coupled with an NPZD biogeochemical model. The model domain encompasses both the Kuroshio and Kuroshio Extension regions with horizontal grid spacing of 3 km. The simulation is conducted for 8 years from 2008 to 2015 to account for spatiotemporal variability of the Kuroshio path. We focus on the changes in the primary productivity and the mechanisms behind it when the Kuroshio meander appears. The Kuroshio meander leads to the isopycnal layer elevation in the nearshore area and the isopycnal layer deepening in the offshore region, promoting and depressing the nitrate upwelling, respectively. Therefore, the mean vertical nitrate flux is an essential factor for the intense primary production. In addition, the effects of the eddy-induced nitrate flux become weaker, mainly produced by the shear instability, when the southward Kuroshio oscillation occurs.
OS13-A054
Exploring the Potential of N2 Fixation in the Subtropical Coastal Waters of South China
Run ZHANG#+, Juan TIAN
Xiamen University
N2 fixation represents an important source of new nitrogen for the marine ecosystem globally. To date almost all available studies were conducted in the tropical/subtropical oligotrophic oceanic regions. However, there is also accumulating evidence suggesting that N2 fixation may occur over a much broader spatial range. The coastal waters act as an interface between land and ocean, providing important services to human society. Such environments are under intensifying anthropogenic impacts, receiving large amount of inorganic and organic nutrient input. Does N2 fixation take place under the background of relatively high dissolved inorganic nitrogen concentration? If yes, what are the major controls on N2 fixation in coastal waters? Does there exist a water column-benthic coupling in the shallow waters? Above questions are in urgent need to be answered. In present study, we will try to combine multiple approaches, including the measurements of N2 fixation rate, nitrogenase (nifH) based diazotrophic composition, imaging, etc, to explore the potential of N2 fixation in the subtropical coastal waters in South China. The results obtained will add knowledge to marine nitrogen cycle and provide important insights into the biogeochemical responses in the coastal waters in the context of ongoing eutrophication.
OS13-A021
Seamount-induced Mixing Revealed Through Idealized Experiments and Its Parameterization in an Oceanic General Circulation Model
Qian CAO1+, Changming DONG1,2#
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory
Though hidden under hundreds if not thousands of meters of seawater, seamounts and the vertical mixing they induce are crucial components of mixing in the global ocean. To gain a deeper understanding of the influence of different seamount topographies on vertical mixing, and distributional characteristics and causes of seamount induced vertical mixing in different grid scales, this study builds a three-dimensional idealized seamounts in a regional ocean model. Results illustrate that, given a constant westward inflow, seamount-induced vertical mixing is mainly distributed on the north and south sides of the summit, the foot of the north and east sides, and downstream from the seamount. Mixing on the north and south sides of the seamount summit and at its foot, is caused by density fronts induced by friction between ambient currents and the seamount. By contrast, mixing downstream of the seamount is due to convective instability, lee waves, and seamount wake eddies. Vertical mixing enhancement at subgrid scales mainly occurs on the southern and eastern sides of the seamount summit, at its foot, and at the seabed. Furthermore, sensitivity experiments reveal that mixing intensity is affected by seamount topographic roughness. As the seamount height and slope increases, vertical mixing at the seamount summit is enhanced, and mixing on its slope gradually shifts to the seamount base. Due to limitations of global ocean model resolutions, seamount induced vertical mixing is often ignored. Consequently, based on the previous finding, a global background mixing coefficient (BMC) relationship is built from an Argo dataset-estimated BMC combined with seafloor topography roughness, and then applied to a global Oceanic General Circulation Model (OGCM). Results show that simulations of deep-sea water temperature and salinity improved after modifying the BMC in seamount-rich areas, with a simultaneous reduction of root-mean-square error by 17% and 12%, respectively.
Session Chair(s): Chunzai WANG, Chinese Academy of Sciences
OS01-A004
Poleward Migration as Global Warming’s Possible Self-regulator to Restrain Future Western North Pacific Tropical Cyclone’s Intensification
I-I LIN1#+, Suzana CAMARGO2, Chun-Chi LIEN1, Chun-An SHI1, Kossin JAMES P.3
1National Taiwan University, 2Columbia University, 3University of Wisconsin-Madison
Poleward migration is an interesting phenomenon regarding the shift of Tropical Cyclones (TCs) towards higher latitudes. As climate warms, TCs’ intensification is promoted, and yet over certain oceans, TCs may also migrate poleward into colder waters. To what extent this poleward shift can impact future TC’s intensification is unclear, and a quantitative understanding of these competing processes is lacking. Through investigating one of the most likely TC basins to experience poleward migration, the western North Pacific (WNP), here we explore the issue. Potential Intensity (PI, TC’s intensification upper bound) along TC’s intensification locations (from genesis to the lifetime maximum intensity location) are analysed. We find that poleward migration can partially cancel global warming’s positive impact on future WNP TC’s intensification. With poleward migration, the PI increasing trend slope is gentler. We estimate that poleward migration can reduce the increasing trend slope of the proportion of Category-5 PI by 42% (22%) under a strong (moderate) emission pathway; and 68% (30%) increasing trend slope reduction for the average PI. References: Lin, I-I*, Suzana J. Camargo, Chun-Chi Lien, Chun-An Shi, James P. Kossin, Poleward migration as global warming’s possible self-regulator to restrain future western North Pacific Tropical Cyclone’s intensification. npj Clim Atmos Sci 6, 34 (2023). https://doi.org/10.1038/s41612-023-00329-y.
OS01-A006
Impacts of PDO-induced Tropical Cyclone Heat Potential (TCHP) Changes on the Typhoon Intensification in the Philippine Sea
Kiduk KIM#+, Jae-Hun PARK, Jeong-Yeob CHAE, Hajin SONG
Inha University
Typhoon has significant impacts on ecosystems and human activities in the Northwestern Pacific and its marginal seas, which has led numerous studies about the dynamic and thermodynamic processes determining its fate. However, most of their focuses were on specific case studies. For better understanding of the effect of ocean to typhoon intensification for long-term aspect, we analyzed ~30 years of tropical cyclone heat potential (TCHP) using outputs from the global ocean reanalysis numerical model GLORYS12V1 and the best track data from the Joint Typhoon Warming Center. In the Philippine Sea, higher values of TCHP were identified during negative pacific decadal oscillation (PDO) phases compared to positive PDO phases. To estimate the relationship between TCHP and typhoon intensification, the gradient of the maximum sustained wind speed (Vmax) was calculated as a proxy for the intensification of tropical cyclone. The analysis reveals that the Vmax gradient of typhoons that were developed from tropical cyclones is more correlated with TCHP than that of tropical cyclones. Further analysis was conducted by categorizing strong PDO case, which was defined when the absolute value of PDO index is larger than the standard deviation of the long-term PDO index. The results reveal a higher correlation between the Vmax gradient and TCHP during the strong negative PDO periods. In addition, the average of Vmax shows a significantly higher value during the strong negative PDO periods. Background TCHP changes and air-sea heat exchange one-day before and after the passage of typhoons along the typhoon tracks show higher values during strong negative PDO periods, which implies that typhoons absorb more heat from the ocean to be intensified when the PDO is in the negative phase. Our results imply that the negative-PDO-induced warming of the Philippine Sea can significantly impact on the intensification of typhoon.
OS01-A001
Large-scale Anomalous Cyclone in the Western North Pacific
Haili WANG+, Chunzai WANG#
Chinese Academy of Sciences
The large-scale anomalous anticyclone in the western North Pacific (WNP) has been extensively studied, but the large-scale anomalous cyclone has not received much attention in the past years. In this study, we use observational data to find that the occurrence numbers of the anomalous cyclone and anticyclone in the WNP have been roughly the same from 1979 to 2020. Our analyses indicate that the WNP anomalous cyclone is an interannual circulation anomaly in the WNP, which can persist from boreal autumn to the subsequent spring during a La Niña year and from spring to summer during a developing El Niño year. To confirm the roles of the central equatorial Pacific, tropical Indian Ocean, and central WNP sea surface temperatures, we perform a suite of model experiments using an atmospheric general circulation model. The model experiments demonstrate that central equatorial Pacific warming contributes to the WNP anomalous cyclone during a developing El Niño year. Cooling in the central equatorial Pacific or the tropical Indian Ocean alone cannot induce the WNP anomalous cyclone, but the combination of central equatorial Pacific cooling, tropical Indian Ocean cooling, and central WNP warming can jointly induce the WNP anomalous cyclone during a La Niña year. Similar to the WNP anomalous anticyclone, the WNP anomalous cyclone and its climatic impacts deserve attention.
OS01-A017
Ocean Subsurface Has Significant Impacts on Tropical Cyclone Genesis
Cong GAO1#+, Lei ZHOU1, I-I LIN2, Chunzai WANG3
1Shanghai Jiao Tong University, 2National Taiwan University, 3Chinese Academy of Sciences
Genesis is a prerequisite for tropical cyclones (TCs) to manifest their destructiveness. The air-sea interaction when and where a TC occur is critical for its following development. Previous studies have shown negative feedback of TC-induced sea surface temperature (SST) cooling on TC intensity. Meanwhile, the magnitude of SST cooling is modulated by seawater temperature profiles. However, the ocean is generally assumed to be a passive receiver in terms of TC genesis. Recently, long-term observations have enabled documentation of the suppression of tropical cyclogenesis by ocean subsurface, but the physical mechanism is still unclear. Here, we apply microwave SST verified by Argo floats and drifters to explore SST cooling by pre-genesis TCs and the feedback on genesis. Our results reveal a significant and robust SST cooling under pre-genesis TCs, strongly influenced by ocean subsurface, plays a critical role in determining the fate of TCs.
OS01-A011
Redistribution of Tropical Cyclone-induced Ocean Subsurface Warming in the Northwestern Pacific Ocean
Qinya ZHANG+, Fanghua XU#, Xueyang ZHANG, Ruizi SHI
Tsinghua University
Tropical cyclones (TCs) -induced ocean mixing is an effective way to pump heat into subsurface ocean. About 42% of the TC-induced ocean subsurface warming (OSWTC) occurs in the Northwestern Pacific. Some studies indicated that the heat is primarily returned to the atmosphere locally in winter. While other studies indicated that the heat is primarily transported equatorward and thus influence the tropical Pacific ocean. To better understand the fate of OSWTC, based on two oceanic reanalysis data from 1994-2015, we conduct Lagrangian particle tracking analysis by releasing virtual particles representing OSWTC in a TC-hotspot in the Northwestern Pacific, and then track the movement of each virtual particle for one year to investigate OSWTC redistribution. It is found that about 25% of the particles returned to the mixed layer 30 days (~one month) after release. One year after release, only 25% of the particles in TC-hotspot still stay below local mixed layer. In the horizontal, about half of the heat remains in the generation area; about 30% of heat moves westward and enter the Kuroshio main axis, and then flows northward along the Kuroshio towards the Kuroshio extension; about 10% of the particles seeded in the TC-hotspot enter the Equatorial Undercurrent (EUC) along the Mindanao Current through southward advection; about 10% of OSWTC continue to enter the South China Sea through the Luzon Strait westward; only a small portion (2%) of the heat moves eastward along the Subtropical Countercurrent (STCC). In addition, the composite analysis of the sea surface height anomaly after TC passage shows that the subsurface warming signal moves westward at a speed of about 0.07 m/s, indicating the OSWTC movement is under the joint effect of the background current advection (0.04 m/s) and the 1st baroclinic Rossby wave propagation (0.08 m/s) in the local area.
OS01-A015
Estimating the Timing of Lifetime Maximum Intensity for Typhoons Approaching Korea
Ger Anne Marie DURAN#+, Il-Ju MOON
Jeju National University
In recent years, South Korea has seen a surge in typhoon-related costs of damages. This trend will likely continue as lifetime maximum intensity (LMI) migrates northward, bringing increasingly destructive typhoons closer to Korean shores. Thus, it is futile to know when and where LMI might occur to provide ample time for early warning preparations. In this study, we investigated the potential factors that can influence the timing of LMI. We found out that the time of LMI occurrence is highly correlated with the time of occurrence of maximum along-track maximum potential Intensity (MPI). Furthermore, the ocean coverage, latitude, and MPI itself play a role in attaining LMI. To highlight the effect of global warming, we employed a multivariate regression model to further apply the mentioned predictors to future synthetic tracks while using the CMIP6 scenarios as the future environment. Our result shows that there is a northward shift in the mean latitude of future LMI locations. Such findings are consistent with the ongoing poleward migration of LMI in the western North Pacific. Our study provides additional insight into tropical cyclone prediction which is crucial in mitigating the future impacts of typhoons in South Korea.
OS01-A014
Impact of the Winter Regional Hadley Circulation Over Western Pacific on the Frequency of Following Summer Tropical Cyclone Landfalling in China
Ruping HUANG1+, Shangfeng CHEN2#, Wen CHEN3, Renguang WU4
1China Meteorological Administration, 2Chinese Academy of Sciences, 3Yunnan University, 4Zhejiang University
The poleward migration of tropical cyclone (TC) activity in recent years has been linked to the expansion of the Hadley circulation (HC). Here, we investigate the impact of the winter regional HC over western Pacific (WPHC) on the frequency of following summer landfalling TC (LTC) in China. Results show that interannual variation of the LTC frequency has a very close connection with the northern WPHC edge (WPHCE). After removing the El Niño-Southern Oscillation signal, there still exists a significant correlation between them. When the winter WPHCE shifts poleward, the associated lower-level southwesterly (easterly) wind anomalies over the subtropical western Pacific (tropical central-eastern Pacific) induce sea surface temperature (SST) warming (cooling) anomalies therein via suppressing (enhancing) upward surface heat flux. In turn, the SST warming (cooling) excites an anomalous cyclonic (anticyclonic) circulation to its west via a Rossby wave response, thus maintaining the southwesterly (easterly) wind anomalies. In addition, the negative rainfall anomalies over the tropical central-eastern Pacific induced by negative SST anomalies can stimulate an anomalous intensive Walker circulation with anomalous upward motion around the tropical western Pacific. Through this positive air-sea interaction, the winter WPHCE signal would be preserved in the ocean and maintained to the succeeding summer, then favoring LTC genesis landward by decreasing the vertical wind shear and increasing the low-level vorticity and mid-level humidity. Meanwhile, anomalous mid-tropospheric easterly winds over the subtropics are favorable for steering more LTCs toward the China's coast. This study suggests that the winter WPHCE variation is a potential predictor for the prediction of the following summer LTC activity over China.
Session Chair(s): Dhrubajyoti SAMANTA, Nanyang Technological University, Tanghua LI, Nanyang Technological University
OS08-A012
Historical Sea Level Response to Volcanic Forcing Estimated from Large-ensemble Global Climate Model Simulations
Dhrubajyoti SAMANTA1#+, Kristin RICHTER2,3, Svetlana JEVREJEVA4, Benjamin GRANDEY1, Kristopher KARNAUSKAS5, Vedant VAIRAGI6, Elaine MCDONAGH2, Nathalie GOODKIN7, Susanna JENKINS1, Lock Yue CHEW1, Benjamin HORTON8,9
1Nanyang Technological University, 2Norwegian Research Centre, 3Bjerknes Centre for Climate Research, 4Centre for Climate Research Singapore, 5University of Colorado Boulder, 6University of Reading, 7Richard Gilder Graduate School, 8City University of Hong Kong, 9Imperial
Quantifying the impacts of volcanic eruptions is important to understanding low-frequency sea level variability. Previous studies have indicated a sudden fall in global mean sea level following large volcanic eruptions, attributed to a temporary reduction in ocean heat content, and a transient disturbance of the water cycle. Yet, our understanding of how sea level responds at a regional scale to such eruptions remains limited. Here, using a large ensemble of global climate model simulations from the Detection and Attribution Model Intercomparison Project (DAMIP), we study the regional sea level response to historical volcanic forcing (1850-2014). We specifically focus on the sterodynamic contribution to sea level change from volcano-only historical simulations. Our objectives are to 1) assess regional patterns of sea level response after the volcanic eruptions; and 2) investigate the underlying physical mechanisms responsible for the simulated regional sea level changes after major volcanic eruptions. Our analysis shows up to ~40 mm of regional sterodynamic (thermosteric plus dynamic) sea level fall within two years of major volcanic eruptions. Notably, Krakatau (1883), Mt. Agung (1963), El Chichon (1982), and Mt.Pinatubo (1991) induce the most pronounced sea level fall of up to ~ 40 mm in around Southeast Asia and the western Pacific. We also note the emergence of an El Niño-like state within one year of large eruptions, which is consistent with observations. We identified the predominant influence of volcanic forcing on interannual to decadal timescale sea level variability in historical simulations. Our findings provide new insights into regional sea level responses to historical volcanic eruptions, which may help reduce uncertainty in sea level simulation and sharpen the focus on proxy interpretations.
OS08-A006
Sea Level Variation in the Arctic Ocean Since 1979 Based on ORAS5 Data
Meixiang CHEN#+, Ying JIN
Hohai University
The Arctic is currently experiencing unprecedented changes across all components of the climate system, primarily driven by global warming. As an important indicator of climate change in the Arctic, sea level reflects variations in both the atmosphere and ocean. We analyze the sea level variation of the Arctic Ocean over the past four decades using ORAS5 data, which is the product of the latest reanalysis-analysis system produced by the European Centre for Medium-Range Weather Forecasts (ECMWF). ORAS5 accurately reproduces the main spatial features of the climatology and temporal evolution of sea surface height (SSH) in the Arctic Ocean, as observed by satellite altimeters, and reveals that seasonal variability is the most significant property of the sea level variation in this region. The seasonal cycle of SSH is closely linked to atmospheric circulation and sea ice formation. The first two dominant modes of the annual-mean SSH in the Arctic Ocean exhibit significant decadal variability. The first mode can be explained by the Ekman transport of wind related to the Arctic Oscillation (AO), which leads to antiphase changes in SSH on the continental shelves and in the deep basins. The second mode shows an antiphase oscillation of SSH between the Eurasian and Canadian Arctic Archipelago (CAA) sides and is driven by the wind anomaly associated with the Arctic dipole anomaly (DA). Due to the decadal variations associated with climate modes, particularly the AO, sea level in the Arctic Ocean has been continuously rising since the mid-1990s or early 2000s, with the most rapid sea level rise occurring in the Beaufort Sea.
OS08-A016
A Process-based Assessment of the Sea-level Rise in the Northwestern Pacific Marginal Seas
Hyeonsoo CHA1+, Jae-Hong MOON1#, Taekyun KIM1, Yuhe Tony SONG2
1Jeju National University, 2California Institute of Technology
Because regional sea-level rise can threaten coastal communities, understanding and quantifying the underlying process contributing to reginal sea-level budget are essential. Here, we assessed whether the regional sea-level rise on the northwestern Pacific marginal seas can be closed with a combination of observations and ocean reanalyses over 1993–2017, as well as with independent observations from in situ profiles including Argo floats and satellite gravity measurements since 2003. The assessment represents that the major contributions come from the land ice melt and sterodynamic components, while the spatial pattern and interannual variability are dominated by sterodynamic effect. The observation-based estimate further shows that along continental shelves, sterodynamic sea-level changes are substantially induced by ocean mass redistribution due to changes in ocean circulation. This result highlights the ocean mass change between the deep ocean and shallow marginal seas, which plays a role in driving regional sea-level rise and variability.
OS08-A015
Assessing Vulnerable Floodplains of Singapore to Sea-level Rise Over the Next 30 Years
Trina NG1,2#+, Huey Yew CHEONG3, Yanbin XU2, Wenjun ZHU2, Aurel MOISE1, Shinichi KAMIYA2, Benjamin HORTON4,5
1Centre for Climate Research Singapore, 2Nanyang Technological University, 3King's College London, 4City University of Hong Kong, 5Imperial
Sea-level rise in Singapore through to 2050 is fixed. No matter how quickly nations lower emissions now, Singapore is looking at 10 to 30 centimeters of mean sea-level rise through the middle of the century, given the long-drawn impact of global warming on the oceans and ice sheets. Here, we investigate the impact of sea-level rise on vulnerable floodplains in Singapore. Utilising updated sea-level projections, we employ a high-resolution (1-meter) Digital Elevation Model (DEM) to identify flood-prone areas situated below a predetermined elevation threshold. The analysis extends beyond mean sea level, incorporating the impact of extreme events such as high tides and surge levels that have the potential to reach up to 3 meters above mean sea level. Leveraging the Master Plan 2019 map, which delineates Singapore's land use planning for the next 15 years, we conduct a detailed analysis of specific floodplain areas. The study calculates the percentage of various land use categories exposed to sea level rise. Subsequently, we quantify and assess the economic impacts and risks associated with the exposed land use percentages.
OS08-A005
Indonesia Future Beach Loss Projections Due to Sea Level Rise
Daniel MARTUA1,2#+, Keiko UDO1, Shuai XIAO1
1Tohoku University, 2Universitas Indonesia
Indonesia has the world's second-longest coastline that makes Indonesia is highly vulnerable to sea level rise and shoreline retreat. Java Island is one of Indonesia's islands that has several sandy beaches along the coastline that faced the shoreline retreat problem by the losses of sandy beaches due to sea level rise. This study utilizes satellite imagery to generate a detailed map of sandy beaches locations, essential for analyzing the shoreline retreat. The prediction of beach loss and shoreline retreat, influenced by sea level rise, is assessed using the Bruun Rule. This assessment incorporates the Shared Socioeconomic Pathways (SSP) Scenarios for the year 2100. The map results indicate that increasing sea levels significantly affect shorelines, causing varying degrees of retreat depending on sandy beach characteristics. The impact ranges from minimal to complete retreat due to rising sea levels. Additionally, the northern coast of Java is projected to be more severely affected compared to the southern part, based on the rate of beach loss in that area. This situation needs a solid solution and comprehensive management to combat the beach loss.
Session Chair(s): Yusuke UCHIYAMA, Kobe University, Changming DONG, Nanjing University of Information Science & Technology
OS13-A056
How Does High Resolution Modelling of Shelf Seas Improve Our Understanding of Climate Risks on Vulnerable Regions in South East Asia?
Josh WIGGS1#+, Kate SALMON1, Sarah HOLMES1, Beatriz ARELLANO NAVA2, Paul HALLORAN2, Laura BURGIN1, Hamish STEPTOE1
1Met Office, 2University of Exeter
The Sunda Shelf, in Southeast Asia, forms a rich marine biodiversity hotspot, hosting 76% of global coral species, 75% of mangrove species, and 45% of sea grass species. These habitats play a pivotal role in supporting the region's fishing fleet, contributing to over 20% of the global catch, as well as sustaining aquaculture and providing coastal protection services, collectively valued in billions of dollars. The region is highly susceptible to the impacts of climate change, yet current Global Circulation and Earth System Models lack the requisite spatial resolution and physical processes to accurately project climate impacts in shelf sea environments. In this study, we employ a computationally efficient coastal shelf model, S2P3 v2.0, to simulate two distinct climate change adaptation scenarios—Shared Socioeconomic Pathway 2 (SSP245) representing a middle-of-the-road trajectory and SSP370 representing regional rivalry — until the year 2100. Utilising the latest climate model data from the Coupled Model Intercomparison Project Phase 6 (CMIP6), our model provides a spatial resolution of 10 km, enabling accurate representation of future sea surface temperatures and primary productivity in the Southeast Asia region. The outcomes of our simulations offer crucial data for estimating climate impacts on fisheries, identifying potential future hotspots, and establishing refugia for effective coral reef management. The model could be used to assess future climate impacts on other shelf seas worldwide, such as the Caribbean, which similarly provide essential ecosystem services. We will present a summary of our initial simulation results and analysis performed upon these, along with the results we have been able to obtain.
OS13-A004
The Capability and Limitation of a Hydrostatic Model in Simulating Frontogenesis
Yalin FAN#+
U.S. Naval Research Laboratory
Fronts and filaments are very common to the ocean, and can have a significant impact on the dynamics and structure of the upper ocean. With the increase of computational powers, regional models are now able to resolve these submesoscale features. Since they usually have a horizontal scale of O(1 km) or less, nonhydrostatic process start to kick in as the resolved horizontal scale of the motion becomes comparable with its vertical scale. However, due to computational limitations, hydrostatic models are still used for majority ocean simulations and predictions. Whether these models can correctly represent the frontogenesis at high resolution is not well understood. Furthermore, large eddy simulation studies have shown that Langmuir cells can significantly reduce the peak level of frontogenesis by fragmenting the filament into primary and secondary down-welling sites in a broad frontal zone. Whether the parameterized Langmuir turbulence in the hydrostatic models can produce similar effect is unclear. In this study, the Navy Coastal Ocean Model (NCOM) is used to simulate the life cycle of a sharp cold filament. The hydrostatic model is shown to be able to predict the correct characteristics of filament frontogenesis, but fail to capture the correct dynamics. The effect of horizontal mixing on frontogenesis is very small in the model, and the frontal arrest is controlled by the model’s subgrid-scale artificial regularization procedure instead of horizontal shear instability. Consequently, higher resolution is corresponding to stronger frontogenesis in the model. Thus, whether the hydrostatic model can produce realistic magnitude of frontogenesis is purely dependent on the characteristic of the front/filament simulated and model resolution. Furthermore, the parameterized effect of surface gravity wave forcing through vertical mixing is small on frontogenesis, and cannot represent the real physics of wave-front interaction.
OS13-A038
Spatiotemporal Variability of Eddies and Eddy Kinetic Energy in the Sulu Sea
Crizia ALCANTARA1#+, Charina Lyn REPOLLO2, Cesar VILLANOY1
1University of the Philippines, 2University of the Philippines Diliman
Eddies are rotating bodies of water that have physical, chemical, geological, and biological significance in the open ocean. Eddies are crucial to general water circulation since they mix water horizontally around the water column in open oceans and vertically within the eddy core. Eddy kinetic energy (EKE) is defined as the kinetic energy of the time-varying component of the velocity field. However, this definition contains all processes that vary in time, including coherent mesoscale eddies, jets, waves, and large-scale motions. This study aims to investigate the spatiotemporal variation of eddies in the Sulu Sea and describe the spatiotemporal variation of its EKE. This is achieved by analyzing the mesoscale eddy trajectory atlas produced by AVISO from 2003 to 2021 and then examining the EKE provided by AVISO and CMEMS. The seasonal cycle of eddies show that cyclonic eddies are abundant from November to February, while anticyclonic eddies are abundant from March to August. Empirical orthogonal function (EOF) analysis of the eddy kinetic energy of the Sulu Sea shows that the southern region of the Sulu Sea near the Sulu Islands has the highest eddy kinetic energy. Seasonal analysis of the EKE shows that during December, the Sulu Sea has the highest EKE, while it has the lowest during March. Analyzing the EOF of eddy kinetic energy, it was shown that the western boundary current of the Sulu Sea has a very strong signal despite the seasonality of the eddies.
OS13-A027
Cooperative Multi-agent Fast and Maneuverable Networked Observation Experiment at the Air-sea Interface of Mesoscale Eddy
Yi ZHANG, Dongxiao WANG#+
Sun Yat-sen University
It is difficult to characterize the fine structure of mesoscale eddy with traditional observations from research vessels, so there is an urgent need for mesoscale eddy air-sea interface observations with high temporal and spatial resolution. We use a variety of unmanned platforms such as unmanned surface vehicle (USV), wave glider, unmanned aerial vehicle (USV) to build a fast and maneuverable networked cooperative observation system for the air-sea interface, with the task-oriented observation of mesoscale eddy as the core. There are two 6-meter USVs equipped with ADCP, CTD and ultrasonic weather stations, as well as the ability to carry two expendable drifting air-sea interface buoys and deploy them automatically. The wave glider is also equipped with the same observation equipment as the USVs, except for drifting buoys. In addition, there are two USVs, one for network communications and the other for atmospheric boundary layer observations by using dropsonde. By constructing a cooperative control based on the multi-agent deep deterministic policy gradient algorithm, the observation paths of each unmanned platform are planned to accomplish the overall mission. After obtaining the simultaneous observation data, data assimilation is carried out through the ROMS, and the reanalysis data are generated for data mining to obtain a new target area with finer details. In order to obtain the fine structural features and their corresponding changes in the air-sea interface key variables, the mother ship immediately recovers and rapidly redeploys unmanned platforms to carry out enhanced observation in a new target area, and so on, to realize the cooperative tracking and observation of the target mesoscale eddy. We made a practical application to a mesoscale warm eddy in the east of the Xisha Islands in the South China Sea.
OS13-A007
Riverine Substance Transport Dynamics and Relative Dispersion Study in a Semi-enclosed Inland Sea
Xinyi KANG1#+, Meng XIA2
1Chinese Academy of Sciences, 2University of Maryland Eastern Shore
Given the considerable hydrodynamic and ecological implications associated with riverine substances in estuaries, a comprehensive investigation on their fates, pathways, and driving mechanisms is imperative. Consequently, observed drifters were deployed in the Bohai Sea (BS) in November 2019, revealing a close association between trajectories and wind patterns, particularly during periods of strong winds. To complement the observed trajectories, an unstructured‐grid‐based coupled particle‐tracking model was implemented for the BS to delineate the riverine particle transport dynamics during ice-free months (April to November) in 2019. The Lagrangian particle trajectories from riverine substances showed distinct spatial and temporal characteristics. Particles from the Yellow River travelled to the Central Basin in July 2019. Particles from the Hai and Liao Rivers were confined to local regions, whereas particles from the Luan River travel to the Central and Bohai Bay regions. In addition, relative dispersion of particles from each river in July 2019 was examined. Three different diffusion regimes including exponential, power, and linear growth were observed. Moreover, momentum analysis confirmed the important role of horizontal advection, Coriolis force, pressure gradient force, and vertical viscosity near the Yellow and Luan Rivers. Simultaneously, within the particles influencing areas from the Liao and Hai Rivers, the horizontal advection term is balanced by the pressure gradient and vertical eddy viscosity terms.
OS13-A014
Quantifying Connectivity Between Mesophotic and Shallow Coral Larvae in Okinawa Island, Japan, Based on a Quadruple Nested High-resolution Model
Yusuke UCHIYAMA1#+, Kimika TAKEYASU2, Satoshi MITARAI3
1Kobe University, 2Nippon Koei Co., Ltd., 3Okinawa Institute of Science and Technology Graduate University
Coral bleaching has recently been occurring extensively across the world’s oceans, primarily because of high water temperatures. Mesophotic corals that inhabit depths of approximately 30–150 m are expected to survive bleaching events and reseed shallow water corals afterward. In Okinawa, Japan, mesophotic coral ecosystems have been reported to serve as a refuge for preserving the genotypic diversity of bleaching-sensitive corals. The connectivity of larval populations among different habitats is a key element that determines the area to be conserved in desirable coral ecosystems. Because coral larvae are largely transported passively by ambient oceanic currents, particularly in the horizontal direction, numerical ocean circulation models greatly help to quantify connectivity with detailed spatiotemporal network structures. The present study aimed to quantify the short-distance connectivity of shallow and mesophotic coral larvae in reef areas on the northwest coast of Okinawa Island. To this end, a quadruple nested high-resolution synoptic ocean model at a lateral spatial grid resolution of 50 m was developed, which was capable of realizing detailed coastal currents influenced by complex nearshore topography, and coupled with an offline 3-D Lagrangian particle-tracking model. After validating the developed model, short-distance horizontal coral connectivity across reef areas on the northwest coast was successfully evaluated. The alongshore lateral connectivity had apparent asymmetry caused by depth-dependent horizontal currents, whereas the larvae spawned at shallow and mesophotic depths were reachable to each other. Such across-depth larval dispersal was attributable to the mixed-layer depth in the spawning period, viz., the boreal spring, which approximately coincides with the boundary between shallow and mesophotic coral, leading to the intensive vertical exchange of virtual larvae.
OS13-A022
The Impact of Waves Propagating from Outer Areas on the Wave Dynamics in the Pearl River Estuary Region
Shaotian LI1#+, Yineng LI2, Shiqiu PENG2
1South China Sea institute of Oceanology, Chinese Academy of Sciences, 2Chinese Academy of Sciences
The Pearl River Estuary (PRE) in the Northern South China Sea suffers from monsoons and typhoons, where surface waves are not only of distinct local characteristics but are also influenced by swells from the open ocean. In this study, we build a nested wave model with the proper wind input parameterization to analyze the impacts of waves from outer areas on the wave dynamics in the PRE region. In either summer or winter, waves from outside (swells) have a prominent impact on significant wave heights (SWHs) and wave periods (WPs), with the contribution to SWHs in summer increasing. The dominance of different wave compositions varies with seasons. The variability of wave ages confirms that swells dominate the PRE region in summer, while wind seas generated by the local wind control the wave dynamics in winter due to the intensified monsoon. Swells mainly come from the southern and eastern boundaries in summer and from the east in winter, respectively. Therefore, for an accurate wave simulation in the PRE region, it is necessary to consider swells from the outer region. Given the complex topography and coastline, the multi-nested model would be one of the most cost-effective and efficient ways.
OS13-A043
A Numerical Study of Plunging Breakers in the Nearshore Area Under the Influence of Wind
Nhat TRUONG1#+, Tso-Ren WU2, Chia-Ren CHU2, Chung-Yue WANG2
1Graduate Institute of Hydrological and Oceanic Sciences, 2National Central University
This study aims to understand the role of wind effects on developing plunging waves in the nearshore region. This study has three types of wind: onshore, offshore, and no wind. The Navier-Stokes Equation coupled with Large Eddy Simulation (LES) was used in this study to simulate and analyze the flow field. The Volume-of-Fluid method (VOF) has been adopted to track the air and water interface. Three numerical simulations involving solitary and regular waves are conducted and show good agreement with the laboratory experiments. After the validation, this study extensively explores the roles of wind speeds and directions on the temporal and spatial distribution, airflow structure, vertical velocity, and vorticity. Our results reveal that the onshore wind speed increases, breaking waves occur earlier, and their location shifts farther from the coastline. Besides that, higher offshore wind speed delays breaking waves and brings them closer to the coastline. In the absence of wind, waves push the airflow structure forward, accelerating vertical airflow velocity and generating airflow recirculation. Airflow separation and counterclockwise vortex patterns can be observed in onshore and offshore wind conditions. Wind speeds and directions play a crucial role in intensifying airflow vortices. The intensity of airflow vorticity in offshore wind scenarios is stronger than in onshore wind conditions. In addition, it was observed that airflow vortices weaken during breaking processes. Moreover, airflow vortices exhibit greater strength than water vortices during the breaking processes. Within the broader context, we present a comprehensive analysis and discussion of the intricate interactions between wind and breaking waves.
Session Chair(s): Yusuke UCHIYAMA, Kobe University, Zhiwei ZHANG, Ocean University of China
OS19-A041
| Invited
Role of Meso and Submesoscale Cyclonic Eddies Generated in the Island Wakes and the Regions Between the Kuroshio and the Southern Coast of Japan
Takeyoshi NAGAI#+, Gloria Silvana DURAN GOMEZ, Diego Alonso Dante PINGLO RODRIGUEZ, Gandy Maria ROSALES QUINTANA
Tokyo University of Marine Science and Technology
Although the Kuroshio carries a large amount of nutrients in subsurface layers, the question remains as to whether and how these nutrients in the subsurface layers are supplied to the sunlit layers before they reach the Kuroshio Extension. To address this question, the authors conducted the tow-yo microstructure surveys and revealed that the Kuroshio flowing over seamounts in the Tokara Strait, south of Kyushu Japan, forms an unprecedentedly large-scale turbulence hotspot spreading over 100-km with 100-1000-fold enhancement of turbulent dissipation rates. The tow-yo profiling with a nitrate sensor revealed that this turbulence hotspot is accompanied by a large nitrate diffusive flux with an average value of O(1 mmol m-2 day-1) at the base of euphotic zone in the Tokara Strait. Although these previous observations by the authors could successfully uncover the hotspot of turbulence and nutrient injection formed in the Tokara Strait, the roles of meso and submesoscale eddies formed behind the islands in the Kuroshio and in the regions between the Kuroshio and the coast still remain elusive. In this study, using the high-resolution observations and simulations, we show here that when the Kuroshio touches the Yaku Island south of Kyushu, it generates submesoscale cyclonic eddies that induce net nitrate upwelling at O(1 mmol m-2 day-1). When the Kuroshio shifted southward in the Tokara Strait, it generates submesoscale anticyclonic subsurface eddies in the island wakes, that are advected by the Kuroshio downstream. After the Kuroshio passes the Tokara Strait, these cyclonic eddies propagate downstream between the Kuroshio and off east coast of Kyushu. More importantly, the countercurrent along the coast associated with this cyclonic eddy generates negative potential vorticity. In the presentation, we will show how these cyclonic eddies affect mixing and nutrient injection along the southern coast of Japan.
OS19-A001
Observational Energy Transfers of a Spiral Cold Filament Within an Anticyclonic Eddy
Chunhua QIU1#+, Dongxiao WANG1, Ming FENG2, Jun YANG1
1Sun Yat-sen University, 2Commonwealth Scientific and Industrial Research Organisation
The ocean surface mixed layer represents a critical interface linking the ocean and atmosphere. The physical processes determining the surface mixed layer properties and mediate atmosphere-ocean exchange. Submesoscale processes play a key role in cross-scale oceanic energy transformation and the determination of surface mixed-layer properties, including the enhancement of vertical nutrient transport, leading to increased primary productivity. Herein, we presented observations of the spiral chlorophyll-a filament and its influence on turbulence within an anticyclonic eddy in the western South China Sea during August 2021. The filament had a negative Ertel potential vorticity associated with strong upwelled/downward currents (approximately 20-40 m/day). Across-filament sections of the in-situ profiles showed turbulent dissipation rates enhanced in the filament. We suggested this enhancement values can be attributed to submesoscale processes, which accounted for 25% of the total parameterized turbulent dissipation rates. The present parametrized submesoscale turbulent scheme overestimated the in-situ values. The filament transferred kinetic energy upward to anticyclonic eddy via barotropic instability and gained energy from the anticyclonic eddy via baroclinic instability. After kinetic energy budget diagnostic, we suggested besides symmetric instability, centrifugal instability and mixed layer baroclinic instability should also be included in the turbulence scheme to overcome the overestimation. The observed dual energy transfers between the anticyclonic eddy and filament, and the observed high turbulent energy dissipation within the filament, emphasized the need for these processes to be accurately parameterized regional and climate models.
OS19-A033
Asymmetry of Submesoscale Instabilities in Anticyclonic and Cyclonic Eddies
Hongyang LIN#+, Weian SHI, Qiang DENG, Jianyu HU
Xiamen University
The upper-ocean relative vorticity has been found to be cyclonically skewed, but altimetry observations indicate that long-lifespan mesoscale eddies tend to be anticyclonic. We are thus interested in whether cyclonic or anticyclonic eddies are more unstable under similar circumstances. Here we use submesoscale-resolving simulations of idealized mesoscale eddies, incorporating theoretical analyses, to investigate asymmetries of submesoscale instabilities within the anticyclones and cyclones. It is found that submesoscale filaments initiate at regions with the largest horizontal buoyancy gradients for both anticyclones and cyclones, but these filaments subsequently rotate outward in anticyclones while inward in cyclones. Hence submesoscales are more vigorous at anticyclone peripheries and the cyclone center. Such differing distributions and evolutions of submesoscale processes are primarily caused by changes in the background stratification associated with the decaying of mesoscale eddies. The active submesoscales near the cyclone center eventually distort its core structure radically, whereas the anticyclone remains largely unaffected.
OS19-A003
The Impact of Rough Topography on Behaviors of Mesoscale Eddies as Revealed by Submesoscale Resolving Simulations
Kaiwen ZHENG+, Zhiwei ZHANG#
Ocean University of China
Mesoscale eddies are ubiquitous in the world ocean and are a key factor in maintaining the global oceanic energy balance. Geophysical turbulence theory predicts that the eddy length scale should increase to Rhines scale as it inherits the inverse energy cascade from smaller scales that help to stabilize the ocean circulation system. However, satellite-observed mesoscale eddies are much smaller than predicted, which indicates that unclear forward energy cascades prevail in their life cycles. In this study, we explore the role of finite rough topography in modulating eddy kinetic energy and horizontal length scales by using a series of submesoscale resolving numerical simulations with parameters typical of the Drake Passage. Our results show that, when compared with those generated over a flat bottom, the presence of rough topography can substantially reduce the horizontal length scales of eddies by approximately 60%–70%, even in upper layers 2–3 km above the bottom. Rough topography also consumes significant amounts of eddy kinetic energy, as the volume-mean eddy kinetic energy over a rough bottom decreases by about 70%–80% when compared with that over a flat bottom. By using a dynamics- based decomposition method, we subtracted the submesoscale motions from total flow and found that, in addition to energetic internal lee waves, deep-ocean submesoscale processes (integrated over the bottommost 1 km) contributed roughly 22% of the total viscosity dissipation across the whole research domain over a rough bottom. Therefore, this study indicates that the role of deep-ocean submesoscale motions in the energy cascade and abyssal mixing should be considered in ocean model parameterizations in the future.
OS19-A011
Intrathermocline Eddy with Lens-shaped Low Potential Vorticity and Diabatic Forcing Mechanism in the South China Sea
Yuyi LIU+, Zhiyou JING#
Chinese Academy of Sciences
Intrathermocline eddies (ITEs), characterized by subsurface lens-shaped low potential vorticity (PV), are pervasive in the ocean. However, the abundance and generation mechanisms of these low-PV lenses are poorly understood owing to their weak surface signals and awkward sizes, which present an observational barrier. Using in-situ observations of the northern South China Sea (NSCS), a typical ITE with a lens-shaped low PV at a core depth of 30-150 m and a horizontal size of ~150 km was captured in May 2021. Combined with PV budget analysis, we investigate the underlying generation mechanism of low PVs within these ITEs using high-resolution reanalysis products. The results suggest that wintertime surface buoyancy loss driven by atmospheric diabatic forcing rather than frictional forcing is a crucial favorable condition for the ITE formation. These enhanced surface buoyancy losses produce a net upward PV flux and decrease PV in the weakly-stratified and deep winter mixed layer, which are preconditioned by anticyclonic eddies (AEs). While surface heating in the following spring tends to weaken the surface buoyancy loss and gradually causes a downward PV flux, the surface-injected high PV subsequently caps the low-PV water within the surface-intensified AEs and transforms them into ITEs. Approximately 22% of the 58 AEs detected by satellite altimetry in the NSCS are ITEs. More importantly, the lens-shaped low PVs within them are produced primarily by the enhanced surface buoyancy loss during wintertime. These findings provide a new dynamic explanation for the low-PV generation in ITEs, highlighting the crucial role of atmospheric diabatic forcing.
OS19-A023
Submesoscale Processes in the Kuroshio Loop Current: Roles in Energy Cascade and Salt/heat Transport
Tian TANG+, Zhiwei ZHANG#, Jinchao ZHANG
Ocean University of China
The Kuroshio Loop Current (KLC) is an important form of Kuroshio intrusion into the northeastern South China Sea (NESCS), which is significant to dynamical and biogeochemical processes in the NESCS. Recent studies suggested that the KLC is a hot spot of submesoscale processes (submesoscales) with spatiotemporal scales of O(1–10) km and O(1–10) days, but submesoscales’ roles in energy cascade and salt/heat transport remain obscure. Here, we investigate this issue through analyzing outputs from a submesoscale permitting simulation. We calculated the kinetic energy exchange rate between submesoscale and larger-scale processes (KER) using coarse-graining approach. It shows that KER is overall positive suggesting forward cascade in the KLC region, whose magnitude is comparable with the temporal change rate of larger-scale kinetic energy in the upper 200 m. Magnitude and direction of KER are closely associated with strain rate and horizontal divergence of background flows, respectively. In addition, submesoscales have elevated salinity and heat diffusivities in the KLC region, which are generally down-gradient at the KLC edge with magnitudes reaching O(102) m2s-1. During the KLC period, horizontal mixing by submesoscales can result in salt and heat transport of 0.88×1013g/kg·m3 and 0.71×1020 J westward into the NESCS interior, respectively. The magnitude of submesoscale salt/heat transport is an order of magnitude larger than that by the KLC eddy shedding. These results suggest that submesoscales play important roles in energy cascade and salt/heat transport in the KLC region, which therefore should be taken into account in the energy and salt/heat budgets.
Session Chair(s): Yusuke UCHIYAMA, Kobe University, Zhiwei ZHANG, Ocean University of China
OS19-A039
| Invited
On the Interactions and Energy Cascades of Multi-scale Oceanic Motions
Zhiyu LIU#+
Xiamen University
The Earth’s ocean is a forced-dissipative system being operated at a wide range of spatiotemporal scales. In order to achieve quasi-equilibrium, the kinetic energy in the ocean transfers from scales of forcing at the basin scale to viscous dissipation at the molecular scale. This energy transfer process, covering nearly ten orders of magnitude, is called energy cascade. Oceanic energy cascade is a fundamental issue of physical oceanography and also a classic puzzle due to challenges in observations as well as in numerical and theoretical modeling. Processes at all these scales occur in the western Pacific Ocean, for example from the strong western boundary currents, vigorous mesoscale eddies and internal waves down to small-scale overturns. Thus, it is an ideal experimental area for studies of oceanic energy cascade and multiscale interactions. Over the past four years, systematic studies on these topics were conducted via a combination of in-situ and remote sensing measurements, multiscale coupled numerical simulations, and theoretical analyses of ocean dynamics. Key findings/research outcomes include device of a dynamical decomposition of multi-scale oceanic motions, identification of the mechanism of tide-induced near-inertial waves (NIWs) and their interactions with wind-induced NIWs, and revealing mechanisms of the fission of shoaling internal solitary waves. With such research progress, we have gained a much better understanding of the interactions and energy cascades of multi-scale oceanic motions. Specifically, 1) by extending the dynamic theory of (un)balanced modes, we proposed a dynamical filter to decompose oceanic balanced and unbalanced motions, and obtained the decomposed physical fields and the corresponding governing equations for the two types of motions, thus establishing a new framework for quantifying the cross-scale interactions and associated energy transfers; 2) we identified a new mechanism of tide-induced NIWs, i.e., tidal forcing alone can generate a Garrett-Munk internal wave spectrum, and further elucidated the nonlinear interacting mechanisms controlling the mutual enhancement of wind- and tide-induced NIWs.
OS19-A025
| Invited
Review of Observational Submesoscale Processes in Coastal Regions
Sung Yong KIM#+
Korea Advanced Institute of Science and Technology
In this talk, we will review coastal submesoscale processes with high-frequency radars-derived surface currents, satellite-derived high-resolution surface chlorophyll concentrations, current and temperature profiles at a coastal mooring, and surface drifters to present physical and physio-biological interactions. For instance, this talk includes coastal chlorophyll blooms associated with on-shore and off-shore propagating vorticity, secondary circulation and vertical migration of thermocline led by horizontally migrating paired submesoscale eddies, and energy injection scales based on independent submesoscale surface observations.
OS19-A017
Lateral Buoyancy Gradients at Submesoscale and Their Dynamical Impacts in the Upper Ocean
Zhiyou JING1#+, Haijin CAO2
1Chinese Academy of Sciences, 2Hohai University
Active submesoscale lateral buoyancy gradients and their dynamical instabilities have been considered to catalyze the forward cascade of oceanic geostrophic energy and the vertical exchange of tracers (e.g., heat, nutrients, and carbon). Here, we preliminarily investigate the energy transformation and vertical fluxes associated with submesoscale turbulence of geostrophic eddy, using a nested realistic simulation and in-situ observations in the west Pacific. The atmospheric forced surface buoyancy loss is detected to directly produce a negative Ertel potential vorticity in conjunction with strain-induced frontogenesis that rapidly sharpens eddy fronts. The results show that up to ~30% of the mixed layer of eddies has negative PV. As a result, a variety of frontal instabilities are triggered and the forced symmetric instability is identified to be important for driving forward energy cascade and vertical communication in the upper ocean. Further analysis of energy budget indicates that ~75% of the submesoscale kinetic energy over the mixed layer is feed by the baroclinic instabilities. At the same time, submesoscale instabilities due to the presence of lateral buoyancy gradients are found to stimulate the vertical velocity up to ~100 m/day and facilitate an enhancement of vertical heat exchange between the surface and oceanic interior.
OS19-A024
Simulating the Global Ocean's Submesoscale with Kilometer-resolution Configurations in SW-HRESM
Shiming XU1#+, Xuantong WANG1, Shaoqing ZHANG2, Zhihao FAN1, Chenhui NING1
1Tsinghua University, 2Ocean University of China
The submesoscale is an essential part of the ocean's dynamics, which contains key processes for the energy cycle and the mass exchange of the ocean. In this talk we report recent activities for high-resolution ocean and sea ice model development, with the global average resolution at 2.4km. At this resolution, the model is capable to resolve a significant portion of the submesoscale. The model’s initial scientific and computational results are evaluated, including the kinetic energy and its cascading in the mesoscale-submesoscale range at global scale. We also introduce the porting of the model onto the Sunway supercomputer, which greatly improves its computational performance and enables long-term climate simulations. The model, both the ocean-sea ice coupled configuration and the fully coupled ones, serves as the backbone for the study of key processes and scientific questions of the physical oceanography and climate change. Ongoing works and future plan for the model improvements, as well as sub-kilometer-resolution flexible ocean models, are also discussed.
OS19-A034
Sub-deformation Scale Energy Spectrum Inferred from Relative Dispersion of Surface Drifters
Yu-Kun QIAN1#+, Joseph LACASCE2, Shiqiu PENG3
1South China Sea Instititue of Oceanology, 2University of Oslo, 3Chinese Academy of Sciences
The atmosphere exhibits a characteristic energy spectrum, with a K-3 spectrum at horizontal scales from 2000 to 200 km, and a K-5/3 spectrum below that. While a similar spectrum might be expected in the ocean, this has never been observed, due primarily to smaller eddy scales and the limited resolution of satellite data. However, energy spectra can be inferred from the dispersion of pairs of surface drifters, at scales down to tens of meters. We employ a suite of dispersion metrics to analyze drifter pairs in the Gulf of Mexico. The results suggest a K-3 spectrum from scales of 7-50 km and a K-5/3 slope at smaller scales. The results are thus qualitatively consistent with the atmospheric spectra, the first such identification in the ocean. The results are also consistent with several previous studies, which resolved portions of the spectra.
OS19-A027
Intensification of Submesoscale Frontogenesis and Forward Energy Cascade Driven by Upper-ocean Convergent Flows
Xiaolong YU#+
Sun Yat-sen University
Upper-ocean fronts are a key part of the climate system modulating both the energy cycles and material transports. The common paradigm is that oceanic frontogenesis at the mesoscales (10-200 km) is predominantly driven by horizontal confluent flows initiated by a background straining field. However, the mechanisms of frontogenesis down to the submesoscales (0.1-10 km) are still understudied, particularly through observations. In this study, we provide direct observational evidence that submesoscale frontogenesis is predominately driven by convergent flows based on a yearlong mooring array deployed in the northeast Atlantic. The mooring measurements provide rare insights into dynamical quantities including frontogenesis rate and horizontal divergence at spatial scales from 18 km down to 2 km. Both quantities exhibit strong seasonality and scale dependence, with larger magnitudes in winter and at smaller scales. Frontogenesis rate has a higher correlation with negative horizontal divergence (i.e., horizontal convergence) as the scale decreases, suggesting that convergent flows are the main factor in driving submesoscale frontogenesis. Crucially, rapid forward cascade of kinetic energy is found to preferentially take place during those periods of submesoscale frontogenesis. This work highlights a fundamental mechanism that may lead to significant forward energy cascade at the submesoscales, and calls for a more accurate submesoscale parameterization in climate-scale ocean models.
OS19-A015
Submesoscale Instabilities and Their Contributions to Phytoplankton Bloom in Frontal Region of the Taiwan Strait
Zhonghua ZHAO1#+, Yuwu JIANG1, Lie-Yauw OEY2, Bangqin HUANG1, Wenfang LU3
1Xiamen University, 2Princeton University, 3Sun Yat-sen University
Cruise, satellite, and model data consistently reveal that phytoplankton blooms always occur near the along-shore front during the down-front northeasterly monsoon relaxation period, while relatively low Chlorophyll-a concentration presents under persistent strong winds in the eutrophic winter and spring Taiwan Strait. Diagnoses of the high-resolution cruise observations and realistic model results demonstrate the existence of vigorous instabilities in the along-shore front region. The present study deciphers symmetric, submesoscale, and mesoscale baroclinic instabilities and their contributions to phytoplankton growth based on realistic model diagnoses as well as idealized model sensitivity experiments in terms of dimensionality and grid resolution. Despite the presence of restratifying baroclinic instability under persistent down-front wind, the destratification effect of the wind maintains steeply tilted isopycnals. Due to the limited restratification effect and enhancement of turbulent dissipation near the submesoscale front region, symmetric instability is unfavorable to phytoplankton growth. In contrast, with the relaxation of the destratifying down-front wind, submesoscale and mesoscale baroclinic instabilities play a dominant role in driving relatively strong and weak restratification near the submesoscale front and mesoscale eddy regions. This leads to significantly weaker turbulent dissipation and triggers relatively strong and weak near-surface phytoplankton blooms, respectively.
OS19-A002
Frontal Dynamics on the Norwegian Sea Slope and the Influences on the Phytoplankton Distributions
Yanlin WANG1+, Zhaoru ZHANG1#, Lixin QU1, Yisen ZHONG1, Meng ZHOU1, Sunnje BASEDOW2, Walker SMITH3
1Shanghai Jiao Tong University, 2University of Tromsø, 3Virginia Institute of Marine Science
The slope and shelf regions of the Norwegian Sea are characterized by high biological productivity that supports elevated biomasses of high-trophic-level predators and fisheries. The main currents in the Norwegian Sea Slope are the Norwegian Atlantic Slope Current carrying warm and saline water from the Atlantic, and the Norwegian Coastal Current carrying cold and fresh water. The Atlantic water and coastal water are topographically steered at the slope, forming a salinity-controlled density front corresponding to a strong slope current system. In spring 2019, a cruise was conducted in the Norwegian Sea slope and shelf regions for resolving mesoscale physical and biological processes by employing a Moving Vessel Profiler (MVP) equipped with coupled physical-biological sensors. This study integrates shipboard observational data, satellite data and numerical simulations from a high-resolution model to analyze the frontal dynamics and the influences on chlorophyll distributions. It was found that chlorophyll maxima occurred at the surface offshore of the front and at the subsurface inshore of the front, indicating a connection with the frontal subduction. Dynamic diagnosis based on the cruise data revealed strong relative vorticity and convergence at the surface front. The potential vorticity maxima aligned with the high-chlorophyll signals, implying the transport of phytoplankton by subducted water. A cross-front section was selected in the numerical simulations, which has similar density range and dynamic structure to the observed phenomenon. Subduction at the dense side of the front and the cross-front circulation are clearly evident on this section. By analyzing the horizontal flow field, it can be inferred that the shoreward branch of a mesoscale cyclonic eddy intensifies the front, and potentially triggered the cross-front circulation and vertical transport of phytoplankton.
Session Chair(s): Wansuo DUAN, Institute of Atmospheric Physics, Chinese Academy of Sciences
OS16-A013
| Invited
Impact of Intraseasonal Potential Vorticity Around the Eastern Tibetan Plateau on the Heavy Rainfall Events Over the Yangtze Basin in Summer 2016
Jiangyu MAO#+, Guanshun ZHANG
Chinese Academy of Sciences
Six persistent heavy rainfall events that occurred mostly over Hubei–Anhui–Jiangxi (HAJ) provinces within and south of the middle–lower Yangtze Basin during the summer of 2016 were regulated by the 10–20-day quasi-biweekly oscillation (QBWO). The characteristics and mechanisms of the QBWO associated with the HAJ rainfall events were examined using ERA-Interim reanalysis data. Composite analysis shows that during a QBWO cycle, the extreme wet (dry) phase of the HAJ rainfall was characterized by the strongest ascending (descending) motion associated with an anomalous upper-tropospheric saddle-shaped circulation field resulting from an eastward-propagating middle–high latitude wave train and westward-migrating tropical potential vorticity (PV) anomalies. The wet (dry) phase was preceded by the corridor establishment of significant anomalous poleward-directed (equatorward-directed) moisture transport over southern China on the northwestern side of the western North Pacific subtropical high in the lower troposphere. The corridor-related moisture convergence (divergence) over the HAJ tended to intensify as an anomalous anticyclone (cyclone) propagated northwestward to the northern South China Sea, in conjunction with the eastward-propagating mid-latitude wave train. The QBWO of the HAJ rainfall was closely linked with upstream PV anomalies generated over the eastern slope of the Tibetan Plateau (TP) due to topographic lateral friction. The PV budget analysis demonstrates that the horizontal PV advection and subsequent topographic friction with a four-day phase-lag between them dictated the QBWO of PV anomalies around the eastern TP. The TP-generated PV anomalies then migrate downstream to facilitate the development of the anomalous circulation over the HAJ.
OS16-A019
A Deep Neural Network-ensemble Adjustment Kalman Filter and Its Application on Strongly Coupled Data Assimilation
Zheqi SHEN#+, Renxi WANG
Hohai University
Due to the increasingly widespread application of coupled numerical models in weather and climate forecasting, coupled data assimilation has attracted broad attention. Among them, strongly coupled data assimilation (SCDA) can fully utilize observation information while updating all model components, which is the theoretically optimal coupled data assimilation method. However, it still faces some challenges at present. This study conducts SCDA experiments using the ensemble adjustment Kalman filters (EAKF). The conventional EAKF adopts linear and Gaussian assumptions, making it difficult to handle cross-component updates in strongly coupled data assimilation. The new approach employs nonlinear variable relationships established by a deep neural network (DNN) during the analysis stage of the EAKF, which nonlinearly projects observation increments into the state variable space. It can diminish errors in estimating cross-component error covariance arising from insufficient ensemble members, therefore improving the SCDA analysis. A conceptual coupled model is employed in this study to conduct twin experiments, validating the DNN–EAKF’s capability to outperform conventional EAKF in SCDA. The results reveal that the DNN–EAKF can make SCDA superior to WCDA with a limited ensemble size. This approach is anticipated to offer insights for future methodological integrations of machine learning and data assimilation and provide methods for SCDA applications in coupled general circulation models.
OS16-A007
Subseasonal Predictability of Early and Late Summer Rainfall Over East Asia
Xiaojing LI#+
Second Institute of Oceanography, Ministry of Natural Resources
Considering the significant differences in the rainfall characteristics over East Asia between the early [May–June (MJ)] and late [July–August (JA)] summer, this study investigates the subseasonal predictability of the rainfall over East Asia in early and late summer, respectively. Distinctions are obvious for both the spatial distribution of the prediction skill and the most predictable patterns, that is, the leading pattern of the average predictable time (APT1) between the MJ and JA rainfall. Further analysis found that the distinct APT1s of MJ and JA rainfall are attributable to their different predictability sources. The predictability of the MJ rainfall APT1 is mainly from the boreal intraseasonal oscillation signal, whereas that of the JA rainfall APT1 is provided by the Pacific–Japan teleconnection pattern. This study sheds light on the temporal variation of predictability sources of summer precipitation over East Asia, offering a possibility to improve the summer precipitation prediction skill over East Asia through separate predictions for early and late summer, respectively.
OS16-A009
Prediction of Summer Surface Air Temperature Over Northern Hemisphere Continents by a Physically Based Empirical Model
Wen XING1#+, Chunzai WANG2, Lei ZHANG2, Jiayu ZHENG2
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, 2Chinese Academy of Sciences
Summer surface air temperature (SAT) variability over Northern Hemisphere (NH) continents can profoundly impact human society, yet its seasonal prediction remains challenging, partly due to the limited prediction skill of dynamical models, especially over extratropical and high-latitude areas. Previous research has defined five indices associated with different atmospheric circulation patterns, which have important contributions to variations of summer SAT. This study further establishes a physically based empirical model (P-E model) using the Bayesian dynamic linear model method for the prediction of the indices, and uses the predicted indices to reconstruct the summer SAT anomaly field. Results show that the P-E model can reasonably well predict the five indices during 1950 to 2021. Combining this with the linear trend, the total summer SAT anomaly is also reconstructed. The high cross-validated hindcast skill for the period of 1950-2021 and independent forecast skill of 2022 indicate that the summer SAT over NH continents can be reasonably predicted by the P-E model.
OS16-A010
Understanding the Driving Forces of the North Pacific Victoria Mode
Zongrong LI1+, Ruiqiang DING2#, Jiangyu MAO1, Zhengyi REN1
1Chinese Academy of Sciences, 2Beijing Normal University
The Victoria Mode (VM) is defined as the second empirical orthogonal function (EOF) of sea surface temperature anomalies (SSTAs) in the North Pacific. It is independent of the Pacific decadal oscillation (PDO) and represents the second climate mode of North Pacific variability. Using a first-order autoregressive model and forcing indices that track the Aleutian low, the North Pacific Oscillation (NPO), anomalous ocean circulation in the Kuroshio–Oyashio Extension (KOE), and the cold tongue (CT) and warm pool (WP) El Niño–Southern Oscillation (ENSO), this study reconstructs the North Pacific SSTAs and examines the relative contributions of different forcing mechanisms to the VM variance. It is found that the NPO and ENSO, especially the WP ENSO, are the dominant sources of VM variability, whereas the contributions of the Aleutian low and zonal advection in the KOE region are relatively small. Further analysis shows that the forcing mechanisms acting on the VM are frequency dependent. At decadal and longer time scales, the VM variance comes mainly from the WP ENSO, whereas at interannual-time-scale contributions from the NPO and CT ENSO are important. This study suggests that the VM is an oceanic response to the NPO forcing and atmospheric teleconnections excited by ENSO events.
OS16-A017
Effectiveness of MPAS-A in Short and Extended Term Forecasting for Tropical Cyclones and Storm Surges
Tomoki SHIRAI#+, Taro ARIKAWA
Chuo University
Recent advancements in computer technology and the refinement of numerical weather models have facilitated the prediction of tropical cyclones (TCs) and the study of storm surge predictability at medium-term (~15 days) and sub-seasonal to seasonal (~2 months) scales (Vitart and Robertson 2018; Khalid et al. 2021). These advancements carry significant societal implications for disaster prevention by extending lead times and by bridging the gap between conventional short-term and long-term (climatological) forecasts at intermediate scales. Among the models developed for application across various time scales, MPAS (Model for Prediction Across Scales; Skamarock et al., 2012) has demonstrated robust TC forecasting performance, distinguishing itself among contemporary cloud-resolving models (Judt et al., 2021). In this study, as part of ongoing efforts to extend the storm surge forecast period to the intermediate scale mentioned above, we sought to validate the MPAS model against the Weather Research and Forecasting (WRF; Skamarock et al., 2008) model. WRF has been widely used for forecasting TCs and storm surges several days in advance with proven reliability. Several sensitivity analyses for several TCs in Japan revealed that MPAS offers similar accuracy to WRF in tracking TCs and generally surpasses WRF in forecasting TC intensity and the distribution of the 10-meter wind field. This is attributed to MPAS's more precise (sharp) reproduction of TC structure at comparable horizontal resolutions and its inherently higher nominal resolution than that of WRF. Consequently, MPAS shown to be as accurate as, or more accurate than, WRF in its storm surge forecast capabilities several days ahead. Further medium-term forecasting experiments with MPAS have confirmed the model's applicability. The findings of this study represent a solid advancement towards providing longer lead times in storm surge forecasts beyond the current capabilities of several-day-ahead predictions.
OS16-A006
Seasonal Variations of Air-sea Carbon Flux at the Cape Hatteras North Carolina Based on Vertical Profile of Carbon Dioxide in Lower Troposphere Obtained with a Gas Sensor Flying on an Unmanned Aerial Vehicle (UAV)
Jinchun YUAN#+
Elizabeth City State University
Although it was recognized as an important parameter in global carbon cycle, air-sea carbon flux was extremely hard to determine due to logistical difficulties in sea going operations. Since it is located at the intersection between two island chains, Cape Hatteras is surrounded by the ocean all around and it is well suited to determine air-sea carbon flux from and a land-based site. We conducted monthly studies of the vertical profiles of physical and chemical parameters including carbon dioxide of the marine air at Cape Hatteras using an unmanned aerial vehicle (UAV) from August of 2022 to present. A suite of physical and chemical sensors was flying on a UAV vertically from near surface to 120 m above ground approximately monthly. The chemical sensors included a carbon dioxide sensor that records concentrations of carbon dioxide twice per second. The physical sensors included a temperature sensor and a relative humidity sensor that record temperature and relative humidity twice per minute. The UAV was sent to a suite of elevations and stayed for a minute to record height as well as physical and chemical parameters. The variation of carbon dioxide near the surface will be used to estimate carbon fluxes and it’s seasonal variations.
Session Chair(s): Yusuke UCHIYAMA, Kobe University, Zhiwei ZHANG, Ocean University of China
OS19-A008
Multi-scale Dynamics Modulated Winter Bloom in the Oligotrophic Marginal Sea
Yuwu JIANG#+
Xiamen University
In the South China Sea, an oligotrophic marginal sea, winter phytoplankton bloom occurs seasonally to the west of the Luzon Strait. In situ observations from Bio-Argo float have revealed that the winter bloom from 2014 to 2015 was primarily attributed to the uplifted nutricline touching the deepened mixed layer, offering a channel for nutrient entrainment to the sunlit upper layer. Further, the Bio-Argo observations showed significant synoptical variability of the winter bloom. This study developed a process-oriented submesoscale-permitting physical–biological coupled model, which reasonably reproduced the seasonal and synoptical variabilities of the phytoplankton bloom observed by the Bio-Argo float. Model diagnoses and sensitivity experiments have revealed that mesoscale upwelling and submesoscale instability significantly contributed to the synoptical variabilities of winter bloom. Specifically, during winter, mesoscale vorticity advection-induced upwelling transported nutrient-rich water upward into the deepened mixed layer. Additionally, near-surface restratification induced by submesoscale baroclinic instability effectively retained phytoplankton cells within the sun-lit surface layer, advancing their growth and contributing to the synoptical enhancement of the phytoplankton biomass.
OS19-A004
A New Parameterization of Submesoscale Vertical Flux in the Ocean
Zhiwei ZHANG#+, Jinchao ZHANG
Ocean University of China
Oceanic submesoscale processes (submesoscales) with O(1–10) km horizontal scale can generate strong vertical buoyancy flux (VBF) that significantly modulate upper-ocean stratification. Because submesoscales cannot be resolved by the prevailing ocean models, their VBFs have to be properly parameterized in order to improve model performance. Here, based on theoretical scaling analysis, we propose a new parameterization of submesoscale VBF by simultaneously considering baroclinic instability and strain-induced frontogenesis, which are two leading generation mechanisms of submesoscales that typically co-occur in open ocean. Compared with the parameterization of Fox-Kemper et al. (2008; F08) that only considers the mixed-layer baroclinic instability, the new parameterization includes mesoscale strain rate and improves vertical structure function. Diagnostic validations based on submesoscale permitting simulation outputs suggest that the newly parameterized VBFs are more realistic than F08 in regard to three-dimension distributions. Through applying the Z23 parameterization into an eddy resolving OGCM (~9 km), we find that it can greatly reduce the deeper bias of the simulated mixed-layer depth.
OS19-A040
Influence of Submesoscale Eddies on Autumn Phytoplankton Blooms
Yeonju CHOI+, Yign NOH#, Hajoon SONG, Hyojun SEUNU
Yonsei University
Submesoscale eddies play a crucial role in regulating the vertical motions within the ocean’s surface boundary layer, affecting both stratification within the mixed layer and the entrainment at its base. These processes have mixed effects on phytoplankton growth: they enhance nutrient entrainment into the mixed layer while simultaneously inhibiting nutrient transport to the euphotic zone and restricting plankton dispersion out of this zone. In this study, we employ a Lagrangian plankton model alongside large-eddy simulations to investigate how submesoscale eddies affect autumn phytoplankton blooms. Specifically, we examine the influence of varying degrees of surface cooling on phytoplankton growth within the dynamics of the mixed layer shaped by these eddies, under nutrient-limited conditions. Our findings indicate that under strong cooling, the restratification effect of submesoscale eddies outweighs their entrainment effect, consequently limiting nutrient upflux to the euphotic zone and leading to only modest changes in phytoplankton growth. In contrast, under conditions of weak cooling, the presence of submesoscale eddies increases the turbulent kinetic energy within the mixed layer, surpassing the effects of convective turbulence, thus enhancing the efficiency of nutrient transport and promoting phytoplankton growth.
OS19-A036
Submesoscale Coherent Vortices Observed in the Aleutian Basin, Bering Sea
Kun ZHANG#+, Haibin SONG, Linghan MENG
Tongji University
Submesoscale coherent vortices (SCVs) are characterized by their smaller horizontal scales (below the Rossby deformation radius) and strong coherence, which are believed to play a special role in martials transport and energy cascade. Most of the SCVs were sporadically captured by a limited number of hydrographic profiles. Despite recent efforts employing high-resolution mooring arrays and glider hydrographic transects, the spatial structure and distribution of SCVs remain unclear. Utilizing concurrent marine seismic transects, current velocity, and temperature/salinity measurements from cruise MGL1111, this study distinctly elucidates the distribution and characteristics of SCVs in the Aleutian Basin, Bering Sea. The findings reveal the widespread presence of subsurface eddies throughout the Aleutian Basin, with 44 such eddies identified through marine seismic transects. These eddies are primarily submesoscale, boasting average diameters of approximately 20 km. Their thickness varies between 71.14 and 416.57 m. Notably, the core depth of SCVs is predominantly concentrated within the 100 to 200 m depth range, aligning with the depth range of the cold Bering Sea Intermediate Water. Only 5 SCVs exhibit core depths below 300 m, coinciding with the depth range of the Bering Sea Deep Water. Analysis of concurrent velocity data indicates that the majority of SCVs exhibit an anticyclonic property. Preliminary insights from the horizontal wavenumber spectrum suggest that these SCVs may contribute to an elevation in diapycnal mixing within the subsurface layers. These observations are believed to be benefit to the relevant parameterization of submesoscale currents and the influences of submesoscale currents on biogeochemical processes and energy cascade.
OS19-A010
Diurnal Variability of Overturning Instabilities in the Mixed Layer from Glider Array Observations
Ruixi ZHENG+, Zhiyou JING#
Chinese Academy of Sciences
The diurnal variability of mixed layer (ML) overturning instabilities remains poorly understood due to the challenge in capturing their rapid evolution across large spatiotemporal range. This study examines the ML overturning instabilities and their diurnal variabilities based on high-resolution data from 52 gliders in the South China Sea. The results of the field observation over two months show that negative potential vorticity occupies ~16% of the ML and facilitates several types of forced overturning instabilities, especially symmetric instability (SI). Surface diabatic atmospheric forcing is identified to primarily modulate the diurnal variability of these overturning cells, where nighttime surface cooling is found to energize SI with a ~2-hour phase lag. Consequently, over 60% of submesoscale restratification is observed to occur at night. These findings quantitatively highlight the important effects of diurnal variability of instabilities in enhancing ML restratification, which should be considered in the submesoscale parameterizations of ocean and climate models.
OS19-A026
Effects of Symmetric Instability on Potential Vorticity Budget in the Kuroshio Extension Region
Shu Yue MA1#+, Jihai DONG1, Changming DONG1,2
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory
As one kind of submesoscale instabilities, symmetric instability (SI) with spatiotemporal scales of O(100) m ~ O(1) km and O(1) hour exerts significant effects on vertical material transports and forward energy cascade in the ocean. The potential vorticity (PV) is an important conservative parameter controlling quasi-geostrophic flows, whose budget can be modulated by SI. However, due to the small spatial scale of SI which is hardly resolved by most current observations and regional models, how SI affects the PV budget and how big the effect is remain unclear. In this work, the effect of SI on the PV budget in the surface mixed layer of the Kuroshio Extension region is quantitatively analyzed based on high-resolution simulations by applying an existing SI parameterization scheme. Compared with the case without SI effects, negative PV is found to be eliminated in the surface mixed layer in the SI-parameterized case. The negative-PV likelihood in the SI-parameterized case is decreased by up to 12% due to SI. Analysis of the PV budget indicates that SI contributes to the PV budget mainly by modulating the friction term. The friction term tends to generate negative PV but its magnitude is decreased by 35% due to SI. Apart from the frictional term, both advection and non-adiabatic terms are also found to be modulated by SI. This work sheds light on the contribution of SI in the PV budget in the ocean mixed layer and suggests a significant role of SI in quasi-geostrophic PV dynamics.
Session Chair(s): I-I LIN, National Taiwan University
OS01-A002
Three Years of Hurricane Observations by Saildrones: Success and Lessons Learned
Chidong ZHANG1#+, Lev LOONEY2,3, Gregory FOLTZ3, Dongxiao ZHANG4,1, Andrew CHIODI4,1, Edward COKELET1, Jun ZHANG2, Edoardo MAZZA1, Nan-Hsun CHI1, Hauk SCHULZ4
1NOAA Pacific Marine Environmental Laboratory, 2University of Miami, 3NOAA Atlantic Oceanographic and Meteorological Laboratory, 4University of Washington
Studying air-sea interactions of tropical cyclones requires observations of surface energy fluxes near the centers of the storms, which are extremely difficult to take. Saildrones, uncrewed surface vehicles, have been deployed to take in situ observations that can be used to estimate air-sea energy fluxes of hurricanes since 2021. Through the three years of experimental deployments, it has been demonstrated that saildrones can be viable tools to take essential observations for hurricane studies and forecast that otherwise would not be possible. This study introduces the general practice of using saildrones to observe tropical cyclones, the successful steering of saildrones to intercept hurricanes and get into their eyewalls, and lessons learned that would guide the improvement of observing tropical cyclones using uncrewed systems.
OS01-A018
The State of the Air-sea Interface and Rapid Intensification of Tropical Cyclones: Multiphase Physics, Laboratory, and Open Ocean Observations
Alexander SOLOVIEV1#+, Breanna VANDERPLOW1, Roger LUKAS2, Brian HAUS3, David ORTIZ-SUSLOW4, Isaac GINIS5
1Nova Southeastern University, 2University of Hawaii, 3University of Miami, 4Naval Postgraduate School, 5University of Rhode Island
The state of the air-sea interface can be a factor in rapid intensification of tropical cyclones (Soloviev et al. 2017). The NOAA Saildrone observations in Hurricane Sam 2021 for the first time provided high-resolution imagery of the air-sea interface. This imagery is consistent with observations at University of Miami SUSTAIN. These laboratory and open ocean data indicate development of short waves resembling Kelvin-Helmholtz type interfacial waves (KH). Notably, KH at the air-sea interface starts at a wind speed above 33-35 m/s, coinciding with the transition to a tropical cyclone. KH waves at the air-sea interface develop and break within tens of milliseconds. It is an example of the process that is stable on average but unstable to fluctuations. KH at an interface with a very large density difference, like air and water, is strongly asymmetric with most action on the lower density side (Hoepffner et al., 2011). Breaking KH waves produce sea spray between whitecaps, while bubbles are mostly produced within whitecaps occupying only ~4% of the sea surface in tropical cyclones. Here we apply a VOF-to-DPM multiphase model with a mesh adaptation (Vanderplow et al. 2020). VOF-to-DPM can estimate the sea spray generation function directly at the air-sea interface. It discerns between near-spherical and non-spherical spray. For major tropical cyclones, non-spherical spray appears to dynamically dominate over near-spherical spray, which is an indication that the influence of surface tension is diminished and there is no clear separation between the air and water phases. The diminishing effect of surface tension indicates a transition to a different regime of the air-sea interaction that can be specific to major tropical cyclones. This is consistent with Lee et al. (2022) using different considerations. The consequences for the drag coefficient Cd, enthalpy exchange coefficient Ck, and Ck/Cd may include rapid intensification.
OS01-A008
Improvement of Global Forecast of Tropical Cyclone Intensity by Spray Heat Flux and Surface Roughness
Ruizi SHI1#+, Fanghua XU2
1Nanjing University of Information Science & Technology, 2Tsinghua University
In global forecasting systems, tropical cyclone (TC) intensity is usually underestimated, which is one of the major challenges for TC forecasting. One possible reason is the deficiency of physical parameterizations associated with ocean surface waves. To improve the TC intensity forecast, effects of two powerful wave-related processes, the spray-mediated heat flux and surface roughness, are considered in a global coupled ocean-atmosphere-wave system (CFSv2.0-WW3). A series of 24 h forecasting experiments for all TCs from May to October, 2019 are conducted, and comparisons are made against the International Best Track TC data. The results show that for strong TCs the underestimation of TC intensity in CFSv2.0-WW3 is significantly improved by the modified surface roughness parameterization and the accelerated spray heat flux parameterization based on gaussian quadrature. For strong TCs with initial wind speeds larger than 30 m/s, the error of TC maximum wind speed decreases by about 34.4%. To understand the associated dynamic and thermodynamic processes, a series of 120 h simulations for major hurricane Hagibis is conducted. It is found that the effect of spray-mediated heat flux contributes to 91.7% of the TC intensity improvement. The increased heat fluxes offset the negative contributions of vertical advection and ventilation, leading to enhanced entropy. The low-level pressure is then decreased, resulting in enhanced convergence of absolute vorticity, which overpowers the negative effects of frictional dissipation and vertical momentum advection. The study indicates that the application of these two wave-related parameterizations can potentially improve the global forecast and reanalysis of TC intensity.
OS01-A007
Near-inertial Response to a Typhoon on a Continental Slope in the Northern South China Sea
Han ZHANG#+
Second Institute of Oceanography, Ministry of Natural Resources
Typhoons have strong impacts on ocean. In 2018, Typhoon Mangkhut travelled over a moored station on continental slope in the northern South China Sea, the near-inertial oceanic responses are studied based on the Regional Ocean Modeling System (ROMS) model simulation combined with observation data. After Mangkhut, near-inertial currents can be divided into three layers: near-circular polarized in upper ocean, across-slope polarized in deep ocean and along-slope polarized near the bottom, thickness of the three layers depend on the slope steepness. According to across-slope and along-slope intensified currents, the near-bottom vertical velocities and near-inertial energy were intensified that reach ~0.002 m/s and ~20 J/m3 at the moored station. The analysis in across-slope section along with normal modes indicate that, the across-slope forth/back near-inertial flows bring cold/warm and salty/fresh water from deeper/shallower depth, increase vertical excursions of near-bottom isolines and near-inertial available potential energy. The near-inertial barotropic across-slope currents (reach ~0.08 m/s) were much greater than along-slope flow (reach ~0.02 m/s), with net uplift of water and net cooling of the whole water column ~0.5°C at the station. The core responses to Mangkhut were within the scope ~1° near the station. The near-inertial kinetic energy generated both at sea surface and bottom slope, then propagated vertically into ocean interior and horizontally into the South China Sea basin as well as some topography-trapped waves propagated along the slope. This work enriches the understanding of air–sea interactions in coastal regions and the effect of ocean topography, especially after a typhoon.
OS01-A013
Langmuir Turbulence Effects on Rapid Mixed Layer Deepening in Tropical Cyclone Environments
Bicheng CHEN1#+, Jiahao HUANG1, Dong WANG1, Qing LI2
1Xiamen University, 2The Hong Kong University of Science and Technology
The Tropical Cyclone generation and evolution hinge on sea surface temperature, which is controlled by the air-sea heat flux and the entrainment flux at the ocean mixed layer bottom. In the intense wind conditions of tropical cyclones, strong waves and current shears develop in the upper ocean, causing strong wave-current interaction and exceptionally robust Langmuir turbulence in the mixed layer. Such strong Langmuir turbulence facilitates vertical mixing, leading to a rapid mixed layer deepening event; thus, it significantly enhances entrainment from the thermocline to the mixed layer. This study employs a large-eddy simulation (LES) model to explore the rapid-deepening events under extreme wind conditions of tropical cyclones. Our primary objective is to establish a linkage from wind/wave forcing to the deepening rate and the entrainment flux, elucidating the mechanism of mixed-layer deepening attributable to Langmuir turbulence. Our findings reveal a distinct deepening rate caused by Langmuir turbulence, deviating from that induced by traditional shear turbulence. Furthermore, we identify multiple energetic modes in Langmuir turbulence, one of which predominantly contributes to the mixed-layer deepening event.
OS01-A012
Observations on the Interaction Between Typhoon Hinnamnor, Semidiurnal Internal Tides and Underlying Marine Heatwaves
Saranya J.S.+, Panini DASGUPTA, Sunghyun NAM#
Seoul National University
Typhoons, deriving their energy from warm sea surface waters, pose a significant concern as they increasingly interact with more frequent marine heatwaves (MHWs) in a changing climate. This study focuses on Typhoon Hinnamnor (2022), which, after an initial peak in intensity, exhibited a weakening and re-intensifying trend as it approached the Korean Strait, interacting with underlying MHW in the northern East China Sea (nECS). The interactions between typhoon Hinnamnor and MHWs before, during and after the typhoon passage, were examined using in-situ observational data collected from the Ieodo Ocean Research Station (IORS), the nearby Jeju Nambu Buoy in the nECS, and ship-based hydrographic observations, supplemented by reanalysis data products. Our study reveals a substantial increase in latent heat loss from the nECS (61-82 Wm-2) during the MHW condition, contributing to the re-intensification of the typhoon. Strong sea surface wind forcing associated with the re-intensified typhoon leads to enhanced vertical mixing and upwelling, resulting in a pronounced (0.90°C) sea surface cooling. The surface mixed layer deepens from 20 to 40 meters after the typhoon passage, facilitating the dissipation of the MHW and causing a significant reduction in thermal stratification. Additionally, our investigation identifies a robust semidiurnal internal temperature oscillation during the MHW period. The semidiurnal internal temperature oscillations become very weak after the typhoon passage due to substantial changes in background stratification, independent of the spring-neap tidal forcing. These findings underscore the importance of sustainable, long, and continuous time series observations to effectively monitor the interaction processes of extreme events within the context of a changing climate.
Session Chair(s): Yusuke UCHIYAMA, Kobe University, Jihai DONG, Nanjing University of Information Science & Technology, Zhiwei ZHANG, Ocean University of China
OS19-A029
| Invited
Subsurface Eddies Imaged by Seismic Oceanography Method
Haibin SONG#+, Kun ZHANG, Shun YANG, Linghan MENG, Mengli LIU
Tongji University
Subsurface eddies are an important mesoscale and submesoscale ocean phenomenon, which can be imaged with very high resolution, in particular laterally by the seismic oceanography method. Furthermore, high resolution images of physical properties such as temperature, salinity, density and sound velocity can also be derived through seismic inversion constrained by sparse CTDs/XBTs. Previous research results confirm that eddies usually show a lens-like geometry, like Meddies, or a bowl shape with no clear upper boundary. Some may also show spiral arms. These findings not only provide high resolution images of the vertical and lateral structure of eddies, but also image their associated fine structures (such as intrusions, layering, internal waves, etc.) related to mixing. The seismic oceanography method with a horizontal and vertical resolution of 10 m is appropriate for studying submesoscale currents (SMCs). In the immediate periphery of a Meddy, bands of water with numerous reflectors may be “spiral arms” of water, also called filaments. Similar patterns were found for an Arctic eddy. Seismic images and current velocity sections identify 23 mesoscale halocline eddies on the Chukchi Borderlands, Arctic Ocean. A mesoscale anticyclonic eddy was observed, this eddy had a core with a diameter of ∼26 km, a height of 250 m, and was surrounded by submesoscale spiral bands with large slopes. There were multi-arm structures at the boundaries of the eddy, forming submesoscale spiral bands. The steep spiral arms (dipangle can be up to ∼4°) may be caused by eddy stirring. Diapycnal diffusivities estimated from seismic data were enhanced. Enhanced diffusivities at the edges of eddies may be attributed to shear instabilities at the top and bottom edges and to submesoscale motions at the lateral edges of these eddies. We highlight the enhanced mixing at the edges of eddies in the halocline can increase the upward heat flux.
OS19-A037
Eddy Enhanced NIWs in the Northwestern South China Sea During Spring 2021
Hongzhou XU1#, Qi'an CHEN2+, Zheyang ZHANG2, Huichang JIANG2, Tong LONG2
1Instittue of Deep-sea Science and Engineering, Chinese Academy of Sciences, 2Chinese Academy of Sciences
A mooring array deployed in the northwestern South China Sea are utilized to study the impact of eddy on near-inertial waves (NIWs) during spring 2021. During the observation period, a relative weak cyclonic eddy passed through the mooring array and enhanced the Near-Inertial Kinetic Energy (NIKE). The enhanced NIKE mainly occurs above the mixed layer and shows a significant spatial asymmetry. The NIKE on the north side of the eddy is 3-4 times greater than the NIKE on the south side. Temporally, the enhanced NIKE mainly occurs shortly after the cyclone eddy center passes through the observation section, indicating that the enhanced NIKE mainly occurs on the east side of the eddy. In addition, the eddy also affects the energy distribution of different modes, resulting in the domination of the second and third modes. Moreover, given that the near-inertial wind work during this period is relatively small, we believe that the enhanced near-inertial energy mainly comes from the cyclonic eddy, and this has been proved by calculating the energy transfer rate between the eddy and NIWs.
OS19-A006
Submesoscales are a Significant Turbulence Source in Ocean Surface Boundary Layer
Jihai DONG1#+, Jacob WENEGRAT2, Abigail BODNER3, Xiaolong YU4, Changming DONG1,5, Jiwei TIAN6
1Nanjing University of Information Science & Technology, 2University of Maryland, 3New York University, 4Sun Yat-sen University, 5Southern Marine Science and Engineering Guangdong Laboratory, 6Ocean University of China
Submesoscale processes (eddies, fronts, filaments, etc.) are transitional scales linking meso-and small-scale processes in the ocean, with spatial scales ranging from 100 meters to 10 kilometers and temporal scales of O(1) day. With the development of observation methods and numerical models, submesoscale processes have been proven to widely exist in the ocean. Submesoscale processes have been considered an important pathway for the transfer of oceanic kinetic energy from large- and meso-scales to small-scale turbulence. However, due to the strong intermittency in both time and space, our current understanding of submesoscale contribution to the forward transfer of energy and quantification of oceanic turbulent dissipation remains insufficient. Based on observational data from the South China Sea and outputs from a global high-resolution model (MITgcm LLC4320, ~2km), this study analyzes the contribution of submesoscale processes in the oceanic surface boundary layer to turbulent dissipation from both regional and global perspectives. The results indicate that submesoscale processes are a significant pathway for energy dissipation in the regions with active fronts. On a global average, the relative contribution of submesoscale processes to upper ocean turbulent dissipation reaches 34% during winter. Considering that most regional ocean models and all climate models currently cannot resolve submesoscale processes and do not consider their parameterization, this study provides additional evidence that submesoscale processes are one of the reasons for the biases in simulating the upper mixed layer in present ocean models.
OS19-A042
Energy Budget of a Long-lasting Eddy in the Northern South China Sea
Bo HONG#+, Weikang ZHOU
South China University of Technology
The life cycle of an anticyclonic mesoscale eddy was examined in the northern South China Sea based on the in situ measurements, satellite and reanalyses data. The long-lasting eddy was tracked moving southwestward following the continental slope. Three stages could be defined according to its intensity and eddy energy budget. The results showed that the eddy obtained kinetic energy from the background through baroclinic instability during the growing period. The work from wind stress could be a dominant factor during the gust. Such fast response lead to a peak in the kinetic energy, which revealed an instant energy transfer from atmosphere to the ocean. The kinetic energy dissipate through shear instability during the eddy decay period. The energy budget provide an efficient way to evaluate the interaction of mesoscale eddy and background current.
OS19-A022
Submesoscale Coherent Vortices Generated by Kuroshio-islands Interaction in the Luzon Strait
Xincheng ZHANG1+, Zhiwei ZHANG1#, Yi WEI1, James C. MCWILLIAMS2, Wei ZHAO1, Jiwei TIAN1
1Ocean University of China, 2University of California, Los Angeles
Submesoscale coherent vortices (SCVs) are lens-shaped oceanic eddies that have the velocity core in the subsurface layer. Due to their conservative nature, SCVs can effectively trap water masses and thus play an important role in subsurface water transport. Based on the long-term observations from the South China Sea Mooring Array, we have observed many similar SCVs in the northeastern South China Sea (NESCS), which suggests that SCVs is really a common phenomenon in the NESCS. For these SCVs, the statistical results show that their shapes share a uniform Gaussian structure in vertical, and their horizontal, vertical, velocity scale are generally between 10 and 30 km, 100 and 300 m, and 0.10 and 0.35 m/s, respectively. By combing water mass tracing and high-resolution simulations, we founded that the SCVs with warmer and saltier water properties could be generated near the Luzon Strait through the elevated Kuroshio-Islands interaction. Further analysis shows that the total water transport of SCVs entering the SCS through Luzon Strait is estimated to be 0.20 Sv, accounting for 6.0% of that of Kuroshio (3.31 Sv calculated by the observations same mooring arrays) in 100-400 m. This result suggests that the SCVs originated near the Luzon Strait provide a novel and effective route for the water exchanges between the north western Pacific and the South China Sea, and then may play a potentially important role in the interaction between the western Pacific Ocean and the Indian Ocean.
OS19-A021
Effects of Balanced Motions and Unbalanced Internal Waves on Steric Height in the Mid-latitude Ocean
Xiujie ZHANG+, Xiaolong YU#
Sun Yat-sen University
The baroclinic component of the sea surface height, referred to as steric height, is governed by geostrophically balanced motions and unbalanced internal waves, and thus is an essential indicator of ocean interior dynamics. Using yearlong measurements from a mooring array, we assess the distribution of upper-ocean steric height across frequencies and spatial scales of O(1-20 km) in the northeast Atlantic. Temporal decomposition indicates that the two largest contributors to steric height variance are large-scale atmospheric forcing (32.8%) and mesoscale eddies (34.1%), followed by submesoscale motions (15.2%), semidiurnal internal tides (8%), super-tidal variability (6.1%) and near-inertial motions (3.8%). Structure function diagnostics further reveal the seasonality and scale dependence of steric height variance. In winter, steric height is dominated by balanced motions across all resolved scales, whereas in summer, unbalanced internal waves become the leading-order contributor to steric height at scales of a few kilometers.
Session Chair(s): Kewei LYU, Xiamen University, Hajoon SONG, Yonsei University
OS03-A009
| Invited
Observing Wave-affected Marginal Ice Zones in Southern Oceans by Satellite Radar Altimeter Synergy
Shiming XU1#+, Weixin ZHU1, Siqi LIU1, Lu ZHOU2, Alexander FRASER3, Clare EAYRS4
1Tsinghua University, 2Utrecht University, 3University of Tasmania, 4Korea Polar Research Institute
Marginal Ice Zone (MIZ) is an integral part of the Antarctic sea ice cover and usually associated with intensive air-ice-ocean interactions. Wave-affected MIZs form due to the wind wave/swell propagation into the ice pack, the ice breaking, the pronounced ocean mixing, as well as the potential positive feedback to the sea ice cover. However, great challenges exist for the satellite-based observations of the MIZ, mainly due to its small temporal and spatial scales. In this talk we introduce recent advances of observing MIZs with radar altimeters. Circumpolar remote sensing of Antarctic MIZs is carried out through the synergy of multiple satellite campaigns, with July of 2017 as the period of study. We show that, the wave-affected MIZ can be effectively retrieved with various radar altimeters, and the synergy of multiple campaigns greatly improves the temporal and spatial representation of the underlying MIZ. Hot-spots of MIZs are revealed around the Antarctic, especially around Ross/Amundsen Sea and Weddell/Riiser-Larsen Sea. Related topics, including the swell attenuation in the MIZ, are also discussed.
OS03-A013
The Responses of Antarctic Sea Ice and Overturning Cells to Meridional Wind Forcing
Hajoon SONG1#+, Yeonju CHOI1, Edward DODDRIDGE2, John MARSHALL3
1Yonsei University, 2University of Tasmania , 3Massachusetts Institute of Technology
Meridional winds over the seasonal ice zone (SIZ) of the Antarctic have undergone changes and likely contributed to sea ice extent variability in recent decades. In this study, using observations and an eddy-resolving channel model of the Antarctic SIZ, we investigate the influence of meridional wind changes on the sea ice distribution, and document how the underlying ocean might change. We find that southerly wind anomalies in austral winter lead to an increase in sea ice extent by encouraging equatorward sea ice drift. This results in more leads and polynyas, ice production and buoyancy loss near the coastal region and freshening out in the open ocean near the Antarctic Circumpolar Current. In contrast, southerly wind anomalies in austral summer reduce sea ice extent due to warming anomalies near the sea ice edge. This is a consequence of enhanced meridional overturning circulation (MOC) triggered by enhanced buoyancy loss through surface heat flux and brine rejection, which brings relatively warm water towards the summertime sea ice edge. A water-mass transformation analysis reveals the increased deep water formation caused by brine rejection and heat loss in leads and polynyas. Changes in sea ice extent and MOC behave in the opposite way when the sign of the wind anomaly is switched from southerly to northerly. Our study shows that meridional wind anomalies can modify not only the sea ice distribution, extent of polynyas and air-sea buoyancy fluxes, but also the ocean's MOC and bottom water properties.
OS03-A006
Quantifying the Role of the Eddy Transfer Coefficient in Simulating the Response of the Southern Ocean Meridional Overturning Circulation to Enhanced Westerlies in a Coarse-resolution Model
Yiwen LI#+
China University of Geosciences
The ability of a coarse-resolution ocean model to simulate the response of the Southern Ocean Meridional Overturning Circulation (MOC) to enhanced westerlies is evaluated as a function of the eddy transfer coefficient (κ), which is commonly used to parameterize the bolus velocities induced by unresolved eddies. The strongest eddy-induced MOC response, accounting for 82% of the reference eddy-resolving simulation, is achieved using a stratification-dependent κ with spatiotemporal variability. By decomposing the eddy-induced velocity into its vertical variation (VV) and spatial structure (SS) components, we find that the intensified eddy compensation response is primarily driven by the enhanced SS term, while the introduced VV term weakens the response. Additionally, the temporal variation of the stratification-dependent κ plays a key role in strengthening the eddy compensation response to intensified westerlies. The stronger eddy compensation response in the experiment with stratification-dependent κ than the constant κ can be attributed to the structure of κ and the vertical variation of the density slope. These findings highlight the significance of accurately representing κ for capturing the response of the Southern Ocean MOC and emphasize the role of the isopycnal slope in modulating the eddy compensation mechanism.
OS03-A005
Observation of Wind and Sea Ice Effects on Deep High-frequency Internal Waves in the Southern Drake Passage
Hajin SONG1#+, Kathleen A. DONOHUE2, Yong Hoon KIM3, Jae-Hun PARK1
1Inha University, 2University of Rhode Island, 3West Chester University
The high-frequency internal waves (HFIWs), represented by the internal wave continuum, contribute to the ocean mixing by providing energy for diapycnal mixing. It has been suggested that the sea ice shields the sea surface from the wind, enhances internal wave dissipation, and, in turn, suppresses the transmission of energy to the HFIW. However, supporting evidence is scarce partly due to the difficulty of long-term measurements under the sea ice. To investigate the impacts of wind and sea ice on the enhancement of HFIW, this study utilizes approximately 4-year-long near-bottom current records in the southern Drake Passage during 2007–2011. The observation reveals the internal wave continuum, the slope of which agrees well with the Garret-Munk empirical model. At the southernmost site, where sea ice extents in winter, the horizontal kinetic energy at periods shorter than 10.5 hours shows a significant cross-correlation with wind stress. In contrast to the ice-free season, the kinetic energy of HFIW shows interannual variation during the ice-covered season. The HFIW energy reaches its weakest level in 2011, when the wind stress was at its weakest and the sea ice concentration was at its highest. In 2008 and 2010, the HFIW energy is enhanced, coinciding with lower sea ice concentrations. In 2009, semi-diurnal internal tides, considered another prominent source for internal waves, caused a high-level HFIW event. At another site located south of the Southern Antarctic Circumpolar Current Front, near-inertial waves trapped by front crests appear to be related to HFIW’s variability at the near-bottom depth. Our results support the hypothesis that the sea ice extent can modulate the deep HFIW energy in the Southern Ocean, which would have a significant impact on polar ocean dynamics and potentially ecosystems.
OS03-A023
Wind-driven Variability of Sea Ice Extent in the Southern Ocean
Feba FRANCIS#+, Hugues GOOSSE
Université Catholique de Louvain
The Antarctic sea ice extent has high variability on various time scales, but the absence of a clear trend over the past few decades is one of the most intriguing features of recent climate change. Studies have shown that these trends are caused by both dynamic and thermodynamic processes. As for the interannual variability of the sea ice extent, the winds exert a key role. However, the role of winds varies over different sectors of the Southern Ocean. To analyze the potential role of the winds on sea ice extent in more detail, we conduct a few climate model simulations. Sensitivity experiments are performed with the NEMO ocean model and the EC-Earth Earth System Model, in which we force the model to follow observed (or reconstructed) winds through nudging. The initial set of experiments covers the satellite era 1979-2023, as we have the most precise estimates of wind changes in this period. The subsequent step is to nudge the models using the reconstructed winds based on instrumental and paleoclimate data.
OS03-A007
Two Different Trends of Antarctic Intermediate Water in the Southeast Pacific Ocean During the Argo Period: Using a Machine Learning Method
Wenlai SHA1, Jiuxin SHI1#+, Zhi LI2
1Ocean University of China, 2University of New South Wales
As one of the key components of the global ocean circulation, Antarctic Intermediate Water (AAIW) promotes the transfer of heat from the atmosphere to internal storage of the ocean through subduction and has an important impact on global climate change. Unsupervised machine learning method Gauss Mixture Model was applied to divide the southeast Pacific into nine subregions using temperature and salinity of Argo profiles from 2005 to 2021. In the model preprocessing, considerations were made to ensure the temporal distribution of the profiles is uniform, enabling a more in-depth analysis of water mass long-term variations. The temporal distribution of profiles quantity was also considered in the model preprocessing, allowing for further analysis of long-term water mass variations. This study distinguished the Peruvian Chilean Current System, Shallow Salinity Minima Water, Subantarctic Mode Water of different thickness, and potential AAIW formation zones between the Subtropical Front and the Subantarctic Front. The results indicated regional variations in the changes of AAIW within the subregions of the southeastern Pacific. The core of AAIW (at the minimum salinity) in the north of the southeast Pacific exhibited a warming trend (+0.016℃/year) and decreasing density (-1.45 g m-3/year), while no significant trend was observed in the southern AAIW. Analysis of the geostrophic flow field revealed that the northern warming AAIW primarily originated from the Southeastern Pacific Ridge north of the Subantarctic Front to the coastal of Chile, whereas the southern AAIW came from the western side of the Southeastern Pacific Ridge. It is evident that the application of Gauss Mixture Model in local areas can reflect more detailed features, particularly the internal differences within the water masses.
OS03-A016
Drivers and Mechanisms of the Record-high Sea Level in the Southeast Pacific During 2015-16 Observed by Satellite Altimetry
Jianjie FENG#+, Kewei LYU
Xiamen University
While the global sea level has been rising, the regional sea level exhibits substantial variations on various temporal and spatial scales modulated by natural climate variability. Based on satellite altimetry data, we find that the southeast Pacific (SEP) stands out from the leading mode of sea level variations in the Southern Ocean. Drivers and mechanisms of the unprecedentedly high sea level anomalies (>10 cm) in the SEP that occurred during 2015-16 are further examined based on atmospheric and ocean reanalysis products. A sea level budget analysis reveals the dominance of thermosteric effect throughout 2015-16 due to continues and deep-reaching ocean warming in the SEP. In response to the anticyclonic wind anomalies, the reduced latent heat loss into the atmosphere induced the warming anomalies in the upper layers of the central South Pacific, which were then advected eastward and accumulated in the SEP through increased downwelling. Meanwhile, the wind-driven barotropic mass convergence/divergence dominated the high-frequency sea level variations and determined the monthly extremes. We further identify a combination of two main factors that are responsible for the anomalous atmospheric circulation. The poleward-propagating Rossby wave response to the development of the 2015-16 strong El Niño gradually enhanced the stationary anticyclonic wind anomalies over the SEP. In contrast, the zonal wave number three (ZW3) not only had relatively large contribution during the developing phase of the El Niño but also dominated the spatial-time evolution of the extratropical wave-like patterns through its phase shift. Our study provides deep insight into this record-high sea level event in the SEP in terms of both atmospheric drivers and oceanic mechanisms, with important implications for understanding the ongoing and future sea level change.
Session Chair(s): Sooyoul KIM, Kumamoto University
OS11-A055
Compound Hazard Risk Assessment of Fluvial Floods and Storm Surges in the Pearl River Estuary
Jie YANG#+
Hohai University
Located in the lower reaches of a watershed, estuary may suffer frequently from flooding due to different drivers. Fluvial floods from heavy rain in upstream and storm surges from open sea environment are key drivers for coastal flooding, and their simultaneous occurrence may lead to higher severity of coastal hazards, especially city flooding. To assess compound hazard risk from fluvial floods and storms surges in the Pearl River Estuary, compound scenarios are designed based on data analysis and are numerically modeled to produce preliminary assessment results of extreme events of different return periods (RPs). In the present study, totally 56-year length data of river discharges and surge heights generated by tropical cyclones are analyzed and used to decide extreme events with RPs of 10, 50 and 100 years. The numerical results from tide-surge coupled modeling indicate that both the flood process and storm-surge process solely will elevate the water level in river networks and outside river mouths, resulting in flooding in low-lying areas, and further exacerbated flooding risk would occur when they exert influence together. However, flooding drivers differ depending on locations in the estuary. The lower part is mainly affected by astronomical tidal level superimposed with storm surges, which can not reach a long distance in upper estuary, while the upper part is dominantly influenced by flood peaks. At the same time, the competition of fluvial floods and coastal surge and tide would decide how far the saltwater would transport to upstream. Under different RPs of surge processes, the increase of fluvial flood peaks would noticeably weaken the saltwater intrusion length. When considering the same RP scenario of flood process, different surge processes would not alter the horizontal salinity distribution obviously, demonstrating more important role of river discharges than surges in determining the salinity pattern in the estuary.
OS11-A051
Dynamic Coastal Processes and Interactions Among Waves, Tides and River Discharge in Osaka Bay During Typhoon Jebi in 2018
Jae-Soon JEONG1#+, Han Soo LEE1, Nobuhito MORI2
1Hiroshima University, 2Kyoto University
Typhoon Jebi 2018 marked the most powerful typhoon to land in Osaka, Japan, within the past 25 years. This natural disaster, accompanied by a storm surge of approximately 2.0 meters and a significant wave height of 4.7 meters, entailed active investigation due to the severe damage inflicted on a bridge and the nearby coastal zones. In the northeastern part of Osaka Bay, where artificial islands and harbours are located, the combined impact of wind set-up and high waves led to a disastrous coastal inundation by storm surge and overtopping. However, accurately assessing the effects of various factors, such as river outflow, tide, and wind waves, on the magnitude of the inundation near a river mouth remains challenging. This study aims to explore the storm surge resulting from the interactions among river discharge, currents, and waves during the passage of Typhoon Jebi by establishing and applying a seamless river-ocean-wave coupled Seto Inland Sea (SIS) model based on the Semi-implicit Cross-scale Hydroscience Integrated System Model (SCHISM). The high-resolution unstructured-grid SIS model was validated for tides, waves, water temperature, and salinity. The results from diverse sensitivity tests show that tidal effects increased storm surge height by 0.12 m from 2.13 m to 2.24 m in front of the Yodo River mouth and amplified upstream reverse flow in the river. However, significant wave heights didn’t present meaningful differences depending on the tidal effect. As river discharge increased significantly from 700 m3/s to 2400 m3/s during the typhoon’s passage, the impact of river discharge on inundation and circulation combined with the restoration of baroclinic instability will be further investigated. Understanding the mechanisms behind the coastal zone inundation and the contribution of each factor in this study will be crucial for comprehensively predicting typhoon-induced sea level variations and formulating strategies to mitigate potential damage.
OS11-A031
Effect of Two-way Coupling Between Surface Flooding and Sewer Flow on Compound Flooding Due to Wave Overtopping and Sewer Reverse Flow
Junbeom JO1#+, Sooyoul KIM2, Jung Soo KIM3, Nobuhito MORI1
1Kyoto University, 2Kumamoto University, 3University of Bucheon
Compound flooding in many coastal areas occurs through the dynamic combination of multiple flooding factors. In many previous studies, the flooding risk is separately estimated along the coastlines (e.g., surge overflow and wave overtopping) and in the inland area (e.g., rainfall-runoff and sewer reverse flow). Developing a compound flooding calculation model should be required to overcome various challenges arising from independent flooding risk analysis. Therefore, research has been conducted using a fully coupled model to assess the risk of compound flooding due to surge overflow, wave overtopping, rainfall-runoff, and sewer reverse flow. The applicability of the developed model has been validated by reproducing Typhoon Jebi-induced compound flooding at Kansai Airport. For this, a bathymetry consisting of seven domains, including a high resolution of the innermost domain with a 10 m grid size, was constructed. The reproduced Typhoon Jebi is validated by comparing the calculated results with observed atmospheric (i.e., wind speed, wind direction, and pressure) and oceanographic (i.e., wave and storm tide) data from Kansai Airport and Osaka Bay. Furthermore, the calculated flooding depth from the compound flooding scenario agrees with the measured flooding depth rather than the independent flooding scenarios. However, the existing calculation is limited by employing a one-way coupling process in which the surface flow and sewer flow cannot affect each other. The calculation shows wave overtopping generated at 3:00 (UTC), while sewer reverse flow started at 4:30 (UTC). Consequently, a significant amount of flooding had already occurred on the surface when the sewer reverse flow was generated. It is implied that the surface flooding affected the reverse flow of seawater through the manholes. As a result, a two-way coupling between surface flooding and sewer flow calculations was implemented to evaluate the compound flooding scenarios more accurately.
OS11-A019
Joint Statistical and Numerical Modelling of Compound Flood Scenario Based on Historical Tropical Cyclone Events in Pearl River Delta
Haoxuan DU+, Kai FEI, Liang GAO#
University of Macau
In deltaic regions, compound flood events depend mainly on the interactions of storm tide and river flow. However, typhoon induced river flows are usually neglected and are not link to the compound events. This study presents a new framework for probabilistic assessment of compound floods, integrating physically based modeling and trivariate statistical analysis to capture the dynamic relationships between flood drivers and address time lags between peak values. Focused on the Pearl River Delta, the framework provides guidance for applying multiple inputs during compound flood events. Trivariate statistical relationships of river discharges are constructed based on the historical Typhoon events from 1957-2022. Results shows the potential extreme river-surge scenarios of designed 10-, 50-, and 100-year return period. Expect the mainstem of West River dominated by river flows and offshore areas dominated by surges, all other rivers, small streams, and adjacent floodplains are compounding zones (100-year return period). Overall, this study underscores the importance of a coupled modeling approach and provides insights for addressing compound flood risks in vulnerable coastal areas.
OS11-A035
Characterization of Storm Surge Along Liaoning Coast Under Typhoon Lekima
Bo GAO+, Yuxiang MA#
Dalian University of Technology
Under the backdrop of global climate change, the frequency and intensity of extreme weather events have significantly increased. Consequently, the risks associated with storm surges caused by typhoons in coastal areas have also escalated. This study focuses on Typhoon 'Lekima' and conducts numerical simulations to examine its direct impact on the sea area near Dalian, Liaoning Province. The simulations are based on the ADCIRC hydrodynamic model, utilizing the Holland model to provide the forced wind field and pressure field. Additionally, global tidal data are used as the open boundary tide level to simulate the process of storm surge generation. The accuracy of the model in simulating typhoon-induced storm surges is verified by comparing the results with measured data (including typhoons and tide levels). Subsequently, the study conducts a detailed analysis of the storm surge evolution process by combining the meteorological conditions during the impact of Typhoon 'Lekima' with historical storm surge conditions at various stations along the Dalian coast. The spatial distribution and spatiotemporal evolution of storm surges are investigated through a combination of comparing measured data and conducting ADCIRC numerical simulations. The findings demonstrate that the storm surge process along the coast of Dalian, Liaoning, is influenced by both the direct effects of typhoons and the indirect effects of external weather systems. Moreover, it is evident that the spatial and temporal distributions of storm surges caused by these factors differ significantly.
OS11-A052
Numerical Modeling of Effects of Flooding Mitigation Alternatives on Transient Wave Attenuation in Idealized Coastal Communities
Hai Van DANG1,2+, Sungwon SHIN1#, Suchan JOO1, Junhyeok LIM1, Jinhwan HUR1
1Hanyang University, 2Vietnam Maritime University
Coastal communities situated in low-lying regions face an increasing risk of severe flooding triggered by high surges and large waves. The sea level rise resulting from climate change induces shorelines to encroach onto coastal land, further exacerbating the detrimental impact of flooding events in coastal areas. To address this vulnerability, the implementation of coastal structures to mitigate the influence of extreme flooding events on coastal communities has become essential. Seawalls, submerged breakwaters, and mangrove forests have been widely deployed worldwide to mitigate wave overflows and their impact on near-coast regions. However, studies on the comprehensive intercomparison evaluating the protective efficacy of each measure against flooding events to provide guidelines in coastal design and planning have yet to be limited. Therefore, large-scale physical experiments were conducted to investigate the efficiency of natural (mangrove forests) and man-made (seawall and submerged breakwater) coastal structures against transient flows. The experiments involve varying wave amplitudes and surge levels to simulate long-wave dynamics. The experimental configurations, including submerged breakwater-only, seawall-only, combined seawall and submerged breakwater, idealized red mangrove forests (trunk-prop root system) constructed in 4 rows and 8 rows, are conducted. Additionally, a baseline configuration (absence of mitigation structures), are also included. Various instrumentations, including wave gauges, acoustic Doppler velocimeters, loadcells, and pressure sensors, are strategically installed to measure the water surface elevations, velocities, forces, and pressures, respectively. The performance of each mitigation configurations is examined by comparing their effects on inundation depth, velocity, and force reduction in the constructed environment. Furthermore, this study further investigated the hydrokinetic patterns in the idealized coastal communities under transient waves using the olaFlow-based model. The findings contribute valuable insights into hydrodynamic patterns of each configuration, providing helpful information for the design of effective coastal flooding mitigation strategies.
OS11-A058
Numerical Simulation of Storm Surge in Macau Based on a GPU-accelerated and LTS-based Shallow Water Model
He MA#+, Zhiguo HE, Peng HU
Zhejiang University
Storm surge can cause a major disaster in coastal areas, especially inundation. Reliable hydrodynamic modeling of storm surge process requires simulations with high resolution meshes, which leads to a great increase in the computational costs in traditional CPU hydrodynamic models. This article presented a fast numerical simulation model for inundation during storm surge using Graphics Processing Unit (GPU)-accelerated and the local time step (LTS) approach based on finite-volume shallow water model, and applied it to simulate storm surge in Macau, China, during storm surge caused by Typhoon Mangkhut accurately and rapidly. In this model, re-construction wind with Holland and ERA wind field was used to compute the typhoon parameters. The time step of each computational cell in the present model is set to close to the locally allowable maximum time step instead of setting time steps of a block as the locally minimum value. It is shown that numerical results of water level agree quite well with the available measured data in the observed stations of Macau, and the computational efficiency also has been greatly improved compared with classical shallow water model. The results proved that our model can simulate in minutes with GPU-acceleration, and it can improve seven fold in computational efficiency with LTS approach.
OS11-A017
| Invited
Wave Attenuation and Resistance Due to the Rhizophora Mangroves Considering the Prop Root Effect
Yu-Lin TSAI1#+, Che-Wei CHANG2, Nobuhito MORI3
1National Yang Ming Chiao Tung University, 2The University of Rhode Island, 3Kyoto University
Employing nature-based solutions to protect shorelines from extreme waves (i.e., tsunamis) and encounter climate change has been getting more attention in recent decades. However, some mechanisms behind it are still less explored—for example, the role of the plant shape in vegetation-induced resistance to water waves. This study investigated the Rhizophora mangrove-induced resistance to water waves and their attenuation using a fully nonlinear Boussinesq-type model. Adopting the perturbation method in expanding horizontal velocities, the vegetation module is developed, accomplishing the drag and inertia terms due to vegetation can be calculated with the vertical distribution of the Rhizophora mangrove tree and its prop roots. The relationship of the drag (Cd) and inertia (Cm) coefficients with Reynolds (Re) and Keulegan–Carpenter (KC) numbers proposed by Chang et al. (2022; doi: 10.1029/2022jc018653) was investigated. In addition, the numerical simulations were compared with the lab data in terms of wave attenuation to quantify the applicable ranges of the proposed Cd–Re/Cd–KC and Cm–KC relationships. Moreover, the spatial distributions of drag and inertia coefficients within the vegetated area were also discussed. This study hopes to pave the way for future wave-mangrove interaction research in providing accurate parameters for numerical modeling and further hazard mitigation using the Rhizophora mangroves. We will present the details of this study at the 2024 AOGS conference.
Session Chair(s): Gubash AZHIKODAN, Tokyo Metropolitan University
OS20-A001
How to Understand a Shallow Coastal Bays System’s Dynamics Using Coupled Modeling and Observational System
Meng XIA1#+, Miaohua MAO2, Xinyi KANG2, Nishat F. NIMNI1, Haoran LIU1, Lauren A. KITTELL-PORTER1, Anna WARGULA3, Bishnupriya SAHOO1, Katherine FITZENREITER4
1University of Maryland Eastern Shore, 2Chinese Academy of Sciences, 3United States Naval Academy, 4National Oceanic and Atmospheric Administration
The Maryland Coastal Bays (MCBs) system is a very shallow estuarine system with an average depth of 1m, and housed by two inlets, with Ocean City Inlet (OCI) and Chincoteague Inlet (CI). The circulation in this system is significant to material transports (e.g., debris, pollutants, and larvae) and was also impacted by the extreme weathers (e.g., hurricane, winter storm), so this study aims to develop a coupled modeling and observational system to this small scale, shallow bay system. To represent surface flows in the system, this study deployed 35 surface drifters at various tidal phases and wind conditions during 2017 and 2018 to investigate the drifter trajectory with the relationship of winds, tides. In additional, ADCP, CTD, wave instruments (e.g., signature) were deployed to measure the wave and circulation dynamics. These data analysis showed the impact of wind, wave and tide to this shallow bay dynamics. Then the wave-current based model was applied to simulate hydrodynamics, bay-ocean exchange, and wave and storm surge dynamics, blue crab recruitment and also coupled with the watershed model and Ground water information. Observed data derived from the National Data Buoy Center and United States Geological Surveys were used to compare with modeled results. Through this coupled modeling and observational system, it was found winds and extreme weathers impact the bay-ocean exchange and salinity gradient; wave can contribute to around 10% of water level and circulation during the passage of hurricane; severe mixing still exists during the extreme weather for this pretty shallow system; hurricane can favor some parts of the bay’s blue recruitment while some parts decrease. The finding from this study on the MCBs is hoped to provide insights into these shallow bays’ response to different dynamics in a holistic manner and to identify probabilities and consequences of what the future may hold.
OS20-A010
Saltwater Intrusion and Mixing in Two Different-sized Adjacent Macrotidal Estuaries
Ren NISHINO#+, Gubash AZHIKODAN, Katsuhide YOKOYAMA
Tokyo Metropolitan University
The present study focuses on saltwater intrusion and mixing dynamics in two different-sized adjacent macrotidal estuaries (tidal range <5m) located in Southwestern Japan. Intensive field surveys were conducted in both the Okinohata River estuary (8km long) and Chikugo River estuary (23km long) during a neap-spring tidal cycle from September 4 to 11, 2022. During the survey, vertical profiles of salinity were measured from downstream to upstream in both estuaries using a water quality sensor. The results showed that the changes in mixing conditions during a neap-spring transition were similar in both estuaries. The Salinity Interface Gradient (SIG), an indicator of saltwater mixing type, shows that the mixing conditions in both estuaries were stratified during neap tide, which changed to well-mixed during spring tide. However, when compared with the length of saltwater intrusion (SIL), the SIL increased nearly 2km from neap tide to spring tide in the Okinohata River estuary whereas it decreased nearly 3km in the Chikugo River estuary. The highest SIL was observed during spring tide for the Okinohata River estuary whereas during neap tide for the Chikugo River estuary. This may be due to the influence of riverbed topography and river discharge in both estuaries. The riverbed elevation was about -2m with a depth range of 3-5m in the Okinohata River estuary and -4 to -7m with a depth range of 5-7m in the Chikugo River estuary. The Okinohata River estuary has a higher riverbed elevation and shallower water depth, making it more difficult for a saltwater wedge to develop on the riverbed during neap tides. The study concluded that the changes in mixing patterns during a neap-spring transition will be similar for adjacent estuaries, but the distance of saltwater intrusion will be different and are influenced by different factors such as topography, river discharge, tides, etc.
OS20-A002
Salt Intrusion Dynamics in a Well-mixed Sub-estuary Connected to a Partially to Well-mixed Main Estuary
Wenping GONG#+
Sun Yat-sen University
Salt intrusion in estuaries has been exacerbated by climate change and human activities. Previous studies have primarily focused on salt intrusion in the mainstem of estuaries, whereas those in sub-estuaries (those branch off their main estuaries) have received less attention. During an extended La Niña event from 2021 to 2022, a sub-estuary (the East River estuary)alongside the Pearl River Estuary, China, experienced severe salt intrusion, posing a threat to the freshwater supply in the surrounding area. Observations revealed that maximum salinities in the main estuary typically preceded spring tides, exhibiting significant asymmetry in salinity rise and fall over a fortnightly timescale. In contrast, in the upstream region of the sub-estuary, the variation of salinity was in phase with that of the tidal range, and the rise and fall of the salinity were more symmetrical. Inspired by these observations, we employed idealized numerical models and analytical solutions to investigate the underlying physics behind these behaviors. It was discovered that under normal dry condition (with a river discharge of 1500 m3 s-1 at the head of the main estuary), the river-tide interaction and change in horizontal dispersion accounted for the in-phase relationship between the salinity and tidal range in the upstream region of the sub-estuary. Under extremely dry conditions (i.e., a river discharge of 500 m3 s-1 at the head of the main estuary), salinity variations were in-phase with those of the tidal range in the middle as well as the upstream region of the sub-estuary. The variation of salinity in the main estuary, along with those of salt dispersion and freshwater influx inside the sub-estuary collectively influenced salinity variation in the well-mixed sub-estuary. These findings have important implications for water resource management and salt intrusion prevention in the catchment area.
OS20-A003
Multi-decadal Morphological Evolution of a Radial-shaped Sand Ridges in the Southern Yellow Sea, China
Ya Ping WANG#+
Nanjing University
The tidal sand ridge in the southwestern Yellow Sea is globally unique due to its radial spread in morphology, elevation significantly exceeding the low-water level, and muddy deposits. In this study, we employ a numerical model to scrutinize the morphological evolution of the radial sand ridge system (RSR) spanning the period from 1979 to 2059. The model undergoes calibration and validation using hydrodynamic and sediment transport data, seabed topography, and grain size distributions obtained from sediment cores. Our findings reveal that the evolution of the RSR is predominantly controlled by tidal forces, and this expansion is projected to persist until 2059. This expansion is attributed to sediment contributions from both the abandoned Yellow River delta and the Yangtze delta, with the latter making a more substantial contribution. The ridges primarily consist of fine sand and mud, exhibiting diverse responses to regional hydrodynamics. The northern part of the RSR is characterized by the predominant distribution of silt and mud, whereas the southern part exhibits a higher percentage of coarse sediment. Sediment redistribution by wind and waves mitigates local morphological changes, resulting in improved sediment sorting. Consequently, top bed sediment layers feature a high volume of sand on ridges and an increased presence of fine sediment in channels. Elevated lands on sand ridges experience erosion, and deep channels undergo sediment accumulation, contributing to the spatial expansion of the RSR. Sea level rise amplifies regional erosion, particularly impacting areas with complex morphology, especially when sea level rise accelerates. This comprehensive analysis enhances our understanding of the long-term prediction of coastal morphology and the interpretation of seabed stratigraphy. The implications of this study extend to informing coastal management strategies.
OS20-A005
Fresh-seawater Mixing Intricately Regulate the Nitrogen Transformation Processes in the Peral River Estuary
Yunchao WU+, Xiaoping HUANG#, Jinlong LI, Zhijian JIANG, Songlin LIU
Chinese Academy of Sciences
The governing of nitrogen during its transport from terrestrial to estuary under the influence of diverse human activities and hydrodynamic environments, particularly in the fresh-seawater mixing zone, remains insufficient researched and lacks of basis. To address this gap, we employed multi-isotopes, including δ15N-NO3−, δ18O-NO3−, δ15N-NH4+, and δ15N-PN, as well as microbial function analysis, to investigate the nitrogen transformation processes in the Pearl River Estuary (PRE), a highly anthropogenic and terrestrial estuary. Principle component analysis (PCA) confirmed that the PRE could clearly partitioned into three zone, e.g., terrestrial area (T zone), mixing area (M zone) and seawater area (S zone), in terms of nitrogen transportation and transformation processes. The δ15N-NO3− (3.38±0.60‰) and δ18O-NO3− (6.35±2.45‰) results in the inner estuary (T area) indicate that NO3−attributed to the domestic sewage and groundwater discharge in the river outlets lead to a higher nitrification rate in the outlets of the Pearl River than in the reaching and seawater intrusion areas, although nitrate is rapidly diluted by seawater after entering the estuary. The transformation of nitrogen in the T zone was under significant nitrogen fixation (0.61±0.22 %) and nitrification processes (0.0043 ± 0.0032 %) (presumably driven by Exiguobacterium sp. (14.1 %) and Cyanobium_PCC-6307 (8.1 %)). In contrast, relatively low δ15N-NO3− (6.83±1.24‰) and high δ18O-NO3− (22.13±6.01‰) imply that atmospheric deposition has increased its contribution to seawater nitrate and denitrification (0.53±0.13 %) was enhanced by phytoplankton/bacterial (such as Psychrobacter sp. and Rhodococcus) in the S zone. The assimilation of NH4 results from the ammonification of NO3− reduces δ15N-NH4+ (5.36±1.49‰) and is then absorbed by particulate nitrogen (PN). The retention of nitrogen when fresh-seawater mixing enhances the elevation of δ15N-NH4+ (8.19 ± 2.19‰) and assimilation of NH4+, leading to an increase in PN and δ15N-PN (6.91 ± 1.52‰) from biological biomass (mainly Psychrobacter sp. and Rhodococcus).
OS20-A007
Development of Numerical Analysis Method Using MPM for Fluid-soil Interaction
Yota ENOMOTO#+, Taro ARIKAWA
Chuo University
In oceanic environments, complex phenomena such as landslide tsunamis and coastal erosion are driven by fluid-soil interactions. These phenomena have been studied using various approaches, leading to the proposal of numerous numerical analysis methods tailored to each specific case. Broadly, these methods can be categorized into the FDM-FEM coupling method and the particle method. FDM-FEM coupling approach, while beneficial in terms of computational efficiency, faces challenges in large-scale applications due to the complexity of mesh generation and limitations in representing interfaces. Conversely, the particle method, necessitating neighbor particle searches at each computational step, also incurs high computational costs, rendering it less feasible for large-scale computations. In this study, we adopt the Material Point Method (MPM) for modeling ground deformation. MPM represents soil deformation through the movement of Lagrangian particles and solves motion equations on a fixed Eulerian grid, thereby facilitating large-scale computation. Fluid discretization is achieved through the Finite Difference Method (FDM), chosen for its compatibility in data exchange at grid points. Our methodology involves a coupled calculation where pressure data from CADMAS-SURF/3D (Arikawa and Yamano, 2008) is transmitted to Anura3D (https://github.com/Anura3D/Anura3D_OpenSource/wiki), and porosity data from Anura3D is communicated back to CADMAS-SURF/3D. This bidirectional exchange facilitates progressive computation steps, linking the Anura3D node with the corresponding CADMAS-SURF/3D cell. Preliminary validation of our model indicates that the developed FDM-MPM coupling is capable of simulating various fluid-soil phenomena with promising accuracy. Future work will focus on large-scale calculations, optimizing grid partitioning and material point allocation to enhance computational efficiency.
OS20-A009
Environmental Drivers of Estuarine Fish Coilia Nasus Catch During Spawning Season in the Chikugo River Estuary, Japan
Vishal SINGH RAWAT#+, Gubash AZHIKODAN, Katsuhide YOKOYAMA
Tokyo Metropolitan University
The present study explains the relationship between the estuarine environment and fish catch in the macrotidal Chikugo River estuary, Japan. The catch data of representative fish, Coilia nasus was collected between 14.6 km and 16 km upstream from the river mouth. The fish catch data includes fish catch number, number of fishing trips, and the daily fishing hours, which were recorded by a fisherman from 2009 to 2020. Further, the total, standard, and fork lengths of fishes were measured from the pictures captured by the fisherman using an analysis and modelling software named Tracker. The environmental data was collected by instrumental monitoring for the same period at the 14.6 km station and the relationship between environmental parameters with corresponding CPUE (catch per unit effort) was investigated. The standard length (SL) distribution of fishes showed that most of the fishes caught by net ranged between 220 mm to 322 mm and belonged to a matured category of 2-3 years old. The linear relationship between CPUE and environmental parameters showed poor correlation, however, optimal ranges of environmental parameters exhibited favourable conditions for higher C. nasus catch. The optimal range of salinity and SSC was found to be 0.04-0.09 and 12.3-157 mg/L respectively. For discharge and temperature, the optimal range corresponding to high CPUE was 23-340 m3/sec and 16.57-32.47 °C respectively. Previous studies have reported that zooplankton copepods feed on suspended organic matter at the Estuarine Turbidity Maximum (ETM) zone with a salinity of 1. The C. nasus larvae and juveniles feed on these copepods for growth. Conversely, in the present study, high CPUE of C. nasus was found in front of saltwater intrusion and upstream of the ETM zone. The results show that mature C. nasus doesn’t feed and migrate to the regions of extremely low salinities for spawning.
OS20-A012
The Collapse Experiment of Partially Submerged Bidisperse Granular Columns
Ye ZHOU1#+, Huabin SHI2, Xiping YU3, Kang HE1
1Tsinghua University, 2University of Macau, 3Southern University of Science and Technology
Ocean geophysical events like landslides and tailing debris flows are usually induced by the arise of the interstitial water level within the granular mass, and typically affected by its particle composition. An experimental of partially submerged bidisperse granular column collapse on a flat bed is conducted to investigate its flow mobility and particle segregation by changing the particles, the finer-particle fraction, and the saturation level, i.e., the ratio of the initial height of the interstitial water level to the total height of the initial column. The final run-out of a partially submerged bidisperse column usually first decreases and then increases with an increasing initial water level, while also affected by particle composition. With respect to interstitial fluid, it is found to retard the collapse at the acceleration stage, while enhance the granular flow at the deceleration stage in an overall sense. With respect to particle composition, bigger particle-size difference and more finer-particle fraction correspond to a stronger flow mobility. It also observed that the particle segregation is affected majorly by particle composition and minorly by submerged level.
OS20-A013
Effect of Water Withdrawal Elevation on Mixing Dynamics in a Deep Freshwater Reservoir
Ghazaleh KHEIRI1+, Gubash AZHIKODAN1, Maurice DUKA2, Katsuhide YOKOYAMA1#
1Tokyo Metropolitan University, 2University of the Philippines Los Baños
This paper explores the effect of water withdrawal location on thermal stratification and mixing in a deep monomictic reservoir in Japan. The Ogouchi Reservoir has an effective storage capacity of 185Mm3 and a maximum depth of 105m. This reservoir experienced three periods based on operation schemes such as (i) Period-A (1957-1991): deep penstock withdrawal (DPW) located at 70m depth, (ii) Period-B (1992-2001): selective withdrawal (SW) located at 4m depth, and (iii) Period-C (2002-now): combination of SW (at 15m depth) and vertical curtain. The present study focuses on Periods A and C, and the years 1981 and 2017 were selected as their representative years. The water temperature and dissolved oxygen (DO) were measured weekly by the Tokyo Metropolitan Government at depths of 0, 2, 5, 10, and until 100m with 10m intervals. In 1981, the difference between surface and bottom water temperature was 15.7℃ in August, which gradually decreased to 2.1℃ in January and 0.1℃ in February. The difference between surface and bottom DO in January was around 4mg/l, and it became 0.41mg/l in February, which shows that complete mixing occurred. In 2017, the difference between surface and bottom water temperature was 20.1℃ in August, which decreased to 2.1℃ in January and 0.9℃ in February. The difference between surface and bottom DO in January and February was around 10mg/l, implying that complete mixing failed to occur. Thermal gradient (TG) was calculated as 0.0009℃/m in 1981 and 0.008℃/m in 2017. The DPW in 1981 drew surface water into the hypolimnion and caused a reduction in TG. The SW in 2017 caused strong summer stratification, and its effect continued until winter, causing higher TG. Finally, the study concluded that dam operation has an influence on mixing in the winter.
OS20-A014
Assessing Methods for Estimating Roughness Coefficient in a Vegetated Marsh Area Using Delft3D
Jennifer DUAN#+, Khalid AL ASADI
University of Arizona
A Delft3D-FLOW model was used to simulate tidal flow in Davis pond marsh in Louisianan, USA. The study area is a freshwater marsh consisting of one main channel and floodplain. Vegetation induced flow resistance greatly influences tidal flow dynamics in the marsh. This study evaluated eight approaches to estimate vegetation roughness, including two constant Manning’s n values, four empirical relations for calculating n, and two methods for calculating Chezy’s C values originally embedded in the Delft3D model. Simulated results of water surface elevation were compared with the corresponding field observation at eleven stream gauges in the study area. We concluded that the roughness coefficient for vegetated area varies with time as flow depth changes. Among the selected empirical relations for the vegetation roughness, the ones accounting for the effect of the vegetation frontal area and the degree of submergence have closely matched the measurements. To further verify the modeling results, we conducted a set of laboratory experiments to study the impact of vegetation on bed form resistance and bed load transport in mobile bed channel. Vegetation stems were simulated by using arrays of emergent polyvinyl chloride (PVC) rods in several staggered configurations. The total flow resistance was divided into bed, sidewall, and vegetation resistances. Bed resistance is further separated into grain and bed form resistances. This study found vegetation concentration has minor effects on bed load transport at low concentration (<3.3%). By analyzing experimental data using the Downhill Simplex Method (DSM), we formulated new empirical relations for calculating bed form resistance and bed load transport rate in vegetated channel. To quantify the importance of vegetation concentration, each relation was optimized with and without this parameter. The DSM results revealed that the incorporation of vegetation concentration significantly improved the prediction of bed form resistance, but slightly on the bed load transport rate.
Session Chair(s): Junde LI, Hohai University, Amandine SCHAEFFER, UNSW Sydney
OS17-A010
Inter-annual Variations of Upwellings in the South China Sea Associated with the Global Climate Change
Yineng LI#+, Shiqiu PENG
Chinese Academy of Sciences
In this study, the inter-annual variations of upwellings in the South China Sea (SCS) from 1958 to 2015 as well as their relationships with the climate variability are investigated using reanalysis data and numerical simulation. Results show that the impacts of ENSO and IOD on the upwellings in the three main regions, i.e., the East Coast of Vietnam (VE), Southwest of Hainan Island (HNW) and East of Hainan Island (HNE) were changed significantly after the 1990s under global warming. Specifically, the effects of El Niño on the upwellings in HNE (VE and HNW) were significantly weakened (enhanced) after the 1990s, while the effects of negative IOD on the upwellings in the three regions were significantly enhanced. These changes results in the increase of upwelling variance in VE and HNW and decrease of upwelling variance in HNE after the 1990s. Our study highlights the complexity of the mechanism driving the long term variations of upwellings in the SCS and the important of ENSO and IOD in the prediction of their long term changes.
OS17-A003
The East Australian Current as a Transport or Barrier of Passive Material. Impact on the Bluebottle (Physalia Physalis)
Amandine SCHAEFFER1#+, Natacha BOURG2, Anne MOLCARD2
1UNSW Sydney, 2Mediterranean Institute of Marine Science
The East Australian Current (EAC), as the western boundary current of the South Pacific Gyre, governs the flow along the East Coast of Australia, exhibiting meandering patterns and instabilities that generate fine-scale structures. Understanding the interplay between fine-scale processes and larger-scale EAC patterns is crucial as it impacts the passive transport of material, as well as chlorophyll-a distribution, an essential component of marine ecosystems. In this presentation, we consider both aspects. First, we investigate the relationship between fine-scale and large-scale variability in the EAC's separation dynamics. We focus on satellite and high-frequency radar data near the EAC's coherent jet and separation point. Our findings reveal that EAC separation enhances shelf-offshore exchange and offshore chlorophyll-a concentration, while fine-scale structures characterized by positive vorticity and strong strain, contribute to an elevation of chlorophyll-a levels in the region. Second, we model trajectories of the surface floating jellifish-like bluebottle. We investigate the influence of the EAC on its seasonal arrival to the coast, as opposed to weather patterns, and highlight the importance of ocean eddies. Considering the implications of our findings in the context of future climate conditions, it becomes evident that purely dynamical changes in the separation dynamics of the EAC may hold consequences for the distribution of many biological species along the east coast of Australia.
OS17-A002
Drivers of Ocean Warming in the Western Boundary Currents of the Southern Hemisphere
Junde LI1,2#+, Moninya ROUGHAN2, Colette KERRY2
1Hohai University, 2UNSW Sydney
Western boundary currents (WBCs) of the Southern Hemisphere transport heat poleward and are regions of rapid ocean warming. However, the mechanisms responsible for the enhanced warming over the Southern Hemisphere WBC extensions are still debated. Here we show that enhanced eddy generation in the WBC extensions through changes in barotropic and baroclinic instabilities results in enhanced ocean warming as the eddies propagate. This results from a poleward shift of the WBCs, associated with changes in the mid-latitude easterly winds. Consequently, the WBCs have penetrated poleward but not strengthened and are now transporting more heat into their extensions. Our study clearly elucidates the dynamic processes driving increased eddying and warming in the Southern Hemisphere WBC extensions and has implications for understanding and predicting ocean warming, marine heatwaves and the impact on the marine ecosystem in the WBC extensions under climate change.
OS17-A004
The Relative Importance of Eddy Trapping and Eddy Stirring
Tongya LIU#+
Second Institute of Oceanography, Ministry of Natural Resources
Previous studies generally suggest that oceanic mesoscale eddies can maintain a coherent structure throughout their lifecycle and transport the water mass within them. This has been widely regarded as a key characteristic of mesoscale eddies over the past decade. However, recent studies based on the Lagrangian framework indicate that coherent structures in the ocean may be quite limited. Surface drifters are used to examine the material transport capabilities of mesoscale eddies, and it is found that drifters initially enclosed by eddies tend to rapidly leak out from the eddy. Furthermore, a series of numerical experiments demonstrates that individual eddies can effectively carry initially enclosed water parcels, but in the presence of crowded eddies, significant water leakage occurs. Our results indicate that, compared to eddy trapping, eddy stirring may contribute more significantly to material transport.
OS17-A005
Variations of the Kuroshio Extension Axis Controlled by Local Wind Stress Curl
Mingshun FAN1#+, Xiaohui LIU2, Tongya LIU3, Dake CHEN2
1Zhejiang University, 2Ministry of Natural Resources, 3Second Institute of Oceanography, Ministry of Natural Resources
The Kuroshio Extension (KE) axis exhibits a typical interannual to decadal north-south shift. Previous studies have proposed that these variations are caused by the oceanic intrinsic variability or the eastern/central North Pacific wind stress curl. Here, we firstly obtain the KE axis index using EOF method based on the 200m subsurface temperature data, which is consistent with the index obtained based on the SSH data. The KE region shows the positive temperature anomalies and the clockwise circulation anomalies in the north phase of the KE axis. The reverse is true when the KE axis switches to the south phase. A lead correlation analysis indicates that the significant linear correlation appears in the local region when the wind stress curl anomalies lead the KE index 0-1 year and in the eastern/central North Pacific when the wind stress curl anomalies lead the KE index 2-4 years. It is worth noting that linear correlation does not necessarily imply causation. The results of our modeling sensitivity experiments further suggest that the local wind stress curl dominates the interannual to decadal variations of the KE, rather than other mechanism. When the wind stress curl anomalies are positive (negative) in the western North Pacific, negative (positive) local SSH anomalies and temperature anomalies are generated through Ekman divergence (convergence), causing the KE axis to shift southward (northward).
OS17-A008
Dipole Vertical Velocity of Mesoscale Eddies and the Mechanism
Ridong ZHANG1#+, Xiaohui LIU2, Tongya LIU3
1Ocean University of China, 2Ministry of Natural Resources, 3Second Institute of Oceanography, Ministry of Natural Resources
Mesoscale eddies accompanied by a highly variable vertical velocity that unable to be directly measured but show great importance in heat and biological material transportation, thus has been a difficulty under-explored. In this study, we analyze the vertical velocities of eddies in a high-resolution (1/32°) idealized domain based on the MITgcm model. A dipole structure of vertical velocity was found in cyclonic eddies, with downwelling occurring in the east and upwelling in the west, while anticyclonic eddies exhibit opposite characteristics. In addition, this opposite dipole pattern also appears in the composite results of eddies with the same polarity in subtropical and frontal regions, respectively. Using quasi-geostrophic omega equation, we have diagnosed and reproduce this dipole pattern and found that the beta-effect has a significant impact on it. Further numerical experiments were conducted to demonstrate the influence of sea level anomalies and background circulation. The study helps deepen the understanding of mesoscale vertical transport, and hopes to inspire further improvement.
Session Chair(s): Neil HOLBROOK, University of Tasmania
OS10-A010
| Invited
Roles of External Forcing and Internal Variability in Global Marine Heatwaves Change During 1982-2021
Lu DONG#+
Ocean University of China
As discrete prolonged extreme warm water events, marine heatwaves (MHWs) have become more frequent, stronger and longer-lasting during the past several decades. The relative contributions of external forcing and internal variability to these changes and their underlying drivers remain unclear. Here, analyses of 90 simulations in CESM2 reveal that external forcing dominates the increasing frequency by causing the mean warming of sea surface temperature (SST), accounting for 82% of the observed trends. Both the mean warming and increased variance of SST contribute to the longer-lasting MHWs during 1982-2021, with external forcing contributing 38% of the increase in the SST variance for global average. Internal variability, especially the Inter-decadal Pacific Oscillation (IPO), also plays an important role in regional MHW changes. The observed negative IPO trend during 1982-2021 favors increasing, strengthening and longer-lasting MHW over Kuroshio Extension, but decreasing and shorter-lasting MHW over the Northeast Pacific Coast.
OS10-A029
Vertical Structures of Surface Marine Heatwaves
Ying ZHANG1#+, Yan DU1, Ming FENG2, Alistair HOBDAY3
1Chinese Academy of Sciences, 2Commonwealth Scientific and Industrial Research Organisation, 3CSIRO Oceans and Atmosphere
A marine heatwave (MHW) is typically defined as an anomalous warm event in the surface ocean, with wide-ranging impacts on marine and socio-economic systems. The surface warming associated with MHWs can penetrate into the deep ocean; however, the vertical structure of MHWs is poorly known in the global ocean. Here, we identify four main types of MHWs with different vertical structures using Argo profiles: shallow, subsurface-reversed, subsurface-intensified, and deep MHWs. These MHW types are characterized by different spatial distributions with hotspots of subsurface-reversed and subsurface-intensified MHWs at low latitudes and shallow and deep MHWs at middle-high latitudes. These vertical structures are influenced by ocean dynamical processes, including oceanic planetary waves, boundary currents, eddies, and mixing. The area and depth of all types of MHWs exhibit significant increasing trends over the past two decades. These results contribute to a better understanding of the physical drivers and ecological impacts of MHWs in a warming climate.
OS10-A012
Understanding Global Subsurface Marine Heatwaves
Shujing ZHANG1#+, Neil HOLBROOK1, Alexander SEN GUPTA2, Annie FOPPERT1
1University of Tasmania, 2UNSW Sydney
Marine heatwaves (MHWs) are prolonged warm ocean temperature extremes that can have substantial impacts on marine organisms. MHWs have been typically identified at the ocean surface using daily satellite sea surface temperature data. However, MHWs not only occur at the ocean surface but also in the subsurface. Several regional MHW studies have detected subsurface MHWs in various locations such as the Tasman Sea, Northeast Pacific, North Atlantic Ocean, Indian Ocean, as well as the Mediterranean Sea. A limited number of studies have also characterized the subsurface MHWs on a global scale, providing their categories, spatial distributions as well as potential biological impacts. Although regional studies have explored possible drivers of subsurface MHWs, there has been a lack of a comprehensive framework to assess these drivers of subsurface MHWs on a global scale. In this study, we use monthly ocean temperature (T) and salinity (S) from gridded ARGO data since 2004 to detect subsurface MHWs in the upper 2000m of the global ocean. Our findings reveal that the most prolonged and intense subsurface MHWs within the 0-50m layer occurred in tropical oceans, whereas the subsurface MHWs in the layer extending from 50m to 2000m are more prominent in middle-to-high latitudes. During the past two decades, regions experiencing the highest biological exposure to subsurface MHWs are identified in the Northeast Pacific Ocean, Southeast Pacific, and South Atlantic Oceans. To examine the physical drivers of the global subsurface MHWs, we use “spice” and “heave” decomposition methods to separate the temporal temperature changes into those due to the water-mass property changes and those due to isopycnal displacements. This oceanic diagnosis on a global scale not only allows us to identify physical processes that caused MHWs but also helps to classify subsurface MHWs into different types that may have different impacts on pelagic marine species.
OS10-A027
Distinct Impacts of Anthropogenic Greenhouse Gas and Aerosol on Global Marine Heatwaves
Wei LIU1#+, Xianglin REN1, Robert ALLEN1, Se-Yong SONG2
1University of California, Riverside, 2Hanyang University
It is crucial to comprehend how humans affect marine heatwaves (MHWs) in the age of rapidly increasing climate change. Using historical and single forcing simulations of climate models, this study explores the distinct impacts of aerosols and anthropogenic greenhouse gases on global MHWs over the last several decades. The findings imply that variations in greenhouse gas concentrations cause more frequent, intense, and long-lasting MHWs. Anthropogenic aerosols, on the other hand, significantly reduce the intensity and growth of MHWs. Subsequent examination of the probability distribution of sea surface temperature (SST) indicates that aerosols and anthropogenic greenhouse gases have opposite effects on the SST probability distribution tails, causing the tails to contract and expand, respectively. Climate extremes, such as MHWs, are thus encouraged and reduced.
OS10-A005
Geographical Differences in Marine Heatwaves in Global Coral Reef Zones
Yulong YAO#+
South China Sea Institute of Oceanology, Chinese Academy of Sciences
Climate change has led to longer and more intense marine heatwaves (MHWs), which have severe impacts on marine ecosystems. Coral reefs are sensitive to intense MHWs, which often result in coral bleaching. However, the geographical difference in MHWs across the world's coral reefs has not been fully investigated. Here, we provide a comprehensive global assessment of the mean value, trend, and seasonal changes in MHWs across coral reef zones over 1982–2021, and further examine sea surface temperature (SST) variability between the 20th and 21st centuries, as well as projected changes in MHW metrics under 1.5°C global warming. We showed that the total days and mean intensity of MHWs increase from lower to higher latitudes, suggesting latitudinal differences. Globally averaged MHW total days and cumulative intensity increase in most coral reef zones, while the MHW mean intensity decreases. MHW total days are seasonally phase-locked, peaking in the boreal summer and winter in the Northern and Southern Hemispheres, respectively. The MHW category is dominated by moderate and strong, and both show increasing trends during 1982–2021. The empirical orthogonal function (EOF) analysis of the seasonal MHW total days revealed a clear El Niño-Southern Oscillation signal in EOF1. The increased SST variability in global coral reef zones shows higher model consensus under the two emission scenarios. High value areas of SST variability appear in the northern Red Sea, the Persian Gulf, Sumatra, and the Caribbean Sea. Longer and more intense MHWs may be triggered by future increases in upper ocean heat content and shallower mixed layer depths. Our results improve the understanding of geographical differences in coral reef responses to MHW and provide insights into their changes under 1.5°C global warming.
OS10-A014
Significant Reduction of Potential Exposure to Extreme Marine Heatwaves by Achieving Carbon Neutrality
Seokgeun OH+, Seok-Woo SON, Sujong JEONG, Yang Ki CHO#
Seoul National University
Marine heatwave (MHW), a prolonged period of anomalously warm seawater, has a catastrophic repercussion on marine ecosystems. With global warming, MHWs have become increasingly frequent, intense, and prolonged. To avoid irreversible damages from such extreme events, net-zero human-caused carbon emissions by 2050s, called carbon neutrality, were proposed. Here, we evaluate the impact of carbon neutrality on MHWs in the late 21st century using multi-model projections from the Coupled Model Intercomparison Project Phase 6 (CMIP6) Shared Socioeconomic Pathway (SSP)1-1.9 and SSP3-7.0 scenarios. It is found that if the current “regional rivalry” over carbon emissions policy continues into this century (i.e., SSP3-7.0), the MHWs in the late 21st century will become stronger over 1°C and longer lasting over 365 days than historical ones, especially in the western boundary current and equatorial current regions. Approximately 68% of the global ocean will be exposed to permanent MHWs, regionally 93% in the Indian Ocean, 76% in the Pacific Ocean, 68% in the Atlantic Ocean, 65% in the Coastal Ocean, and 48% in the Southern Ocean. Such extreme MHWs can be significantly reduced by achieving carbon neutrality (i.e., SSP1-1.9). In particular, the proportion of exposure to permanent MHWs can be reduced to as low as 0.02 to 0.07%, depending on the region. This result underscores the critical importance of ongoing efforts to achieve net-zero carbon emissions to reduce the potential ecological risks induced by extreme MHW exposure.
OS10-A020
Southern Hemisphere Eastern Boundary Upwelling Systems Emerging as Future Marine Heatwave Hotspots Under Greenhouse Warming
Shengpeng WANG1#+, Zhao JING2, Lixin WU2
1Laoshan Laboratory, 2Ocean University of China
Marine heatwaves (MHWs) exert devastating impacts on ecosystems and have been revealed to increase in their incidence, duration, and intensity in response to greenhouse warming. The biologically productive eastern boundary upwelling systems (EBUSs) are generally regarded as thermal refugia for marine species due to buffering effects of upwelling on ocean warming. However, using an ensemble of state-of-the-art high-resolution global climate simulations under a high carbon emission scenario, here we show that the MHW stress, measured as the annual cumulative intensity of MHWs, is projected to increase faster in the Southern Hemisphere EBUSs (Humboldt and Benguela current systems) than in their adjacent oceans. This is mainly because the additional warming caused by the weakened eastern boundary currents overwhelms the buffering effect of upwelling. Our findings suggest that the Southern Hemisphere EBUSs will emerge as local hotspots of MHWs in the future, potentially causing severe threats to the ecosystems.
OS10-A015
Accurate Detection of Marine Heatwaves Using Sea Surface Temperature from Geostationary Meteorological Satellite Himawari-8 Observations
Qi XIAO#+, Wei YANG
Chiba University
Marine heatwaves (MHWs) manifest when sea surface temperatures deviate significantly, surpassing 90% of seasonal fluctuations for more than five consecutive days, with notable impacts on marine ecosystems and commercial fisheries. To date, the detection of marine heatwaves has primarily relied on NOAA OISST. However, a notable issue arises here. NOAA can provide sea surface temperature data only twice a day, leading to a high likelihood of overlooking abnormal sea temperature changes. Additionally, due to frequent cloud cover over the sea, there is a tendency for data gaps. This comprehensive study leverages observational data collected by the Himawari-8 satellite to detect MHWs, meticulously comparing the results with NOAA data. The research delves into the spatial distribution characteristics of marine heatwaves and the discernible impact of the El Niño/La Niña phenomenon. Furthermore, the study conducts a thorough examination of the intricate mechanisms propelling marine heatwaves, exploring the influence of factors such as mixed-layer depth, ocean currents, and atmospheric temperature. The detailed analysis presented in this study not only showcases the valuable insights that Himawari-8 sea surface temperature (SST) data can offer in understanding MHWs but also underscores the significant variability in MHW characteristics when different daily SST data types from Himawari-8 are utilized. Moreover, the findings prominently highlight the substantial potential of Himawari-8 for MHW detection and ongoing monitoring. In conclusion, the utilization of Himawari-8 satellite data emerges as a powerful and indispensable tool for monitoring and comprehensively understanding these phenomena.
Session Chair(s): Nobuhito MORI, Kyoto University
OS11-A054
| Invited
Unexpected Early Arrived Tsunami at Toyama Bay Caused by the 2024 Noto Earthquake
Yuichiro TANIOKA#+, Yota ATOBE
Hokkaido University
A large earthquake (Mw7.6) occurred beneath the Noto Peninsula in Japan on 1st of January in 2024. The earthquake caused a devastating disaster in the Noto Peninsula in Japan by its strong shaking. Because a part of the fault was located offshore, the earthquake generated the tsunami. The tsunami also inundated the land and caused a disaster. The tsunami was observed at several tide gauges along the Japan Sea coast. The observed tsunami at Toyama City in Toyama Bay was particularly interesting. The first arrival tsunami goes down about several minutes after the earthquake. This tsunami cannot be explained by the tsunami generated by the co-seismic vertical deformation due to the earthquake. In this paper, we try to find a generation mechanism of this first arrival tsunami in Toyama Bay. Our tsunami simulation clearly shows that this first arrival tsunami was generated by the horizontal movement of the steep slope existing in the south of the Noto Peninsula by the earthquake. We found that the co-seismic westward movement of the steep slope dipping to the east caused the subsidence of the sea surface which generated the tsunami. The tsunami was propagated in Toyama Bay and observed at the tide gauge at Toyama City. This result shows that the steep slope in the sea is particularly important to generate a large tsunami.
OS11-A024
Interactions Between Subduction Zone Megathrust and Volcano Systems and Their Associated Hazard Chain: A Case Study from Tonga
Tingting ZHENG1+, Qiu ZHONG2, Qiang QIU3#, Jian LIN4, Zhen SUN1, Pengcheng ZHOU1
1Chinese Academy of Sciences, 2Guangdong Earthquake Agency, 3SCSIO, Chinese Academy of Scienc, 4South China Sea Institute of Oceanology, Chinese Academy of Sciences
Subduction zones are the most frequent locations of large earthquakes and super-volcanic activities, which can result in devastating disasters. Large volcanic eruptions have the ability to reshape landscapes, leading to submarine landslides and subsequent tsunamis. Additionally, the stress changes and fluid movements caused by these eruptions can activate faults, resulting in major earthquakes, landslides, and tsunamis within subduction zones. On the other hand, giant subduction zone earthquakes can also trigger volcano eruptions and tsunamis, forming a chain of marine geological hazards. Therefore, understanding the mechanisms of earthquake-volcano interactions and the associated hazard chain is crucial for disaster preparedness, comprehensive hazard assessments, and mitigation strategies. This study focuses on the interactions between megathrust earthquakes and the back-arc volcano system in the Tonga subduction zone. The investigation includes (1) analyzing seismic-volcano activities, (2) calculating both co-seismic and post-seismic stress and deformation changes caused by great earthquakes (Mw > 7.5) in the subduction zone, preceding volcanic eruptions and their impact on volcanic eruption, and (3) simulating potential tsunami impacts on surrounding areas and Pacific coastlines. Our investigation has yielded the following conclusions: (1) We have observed strong correlations between volcano eruptions and megathrust earthquakes; (2) The 2006 Mw 8.0 earthquake has exerted significant influence on the volcanos by loading and deforming them, resulting in positive effects on magma migration of the Hunga Tonga-Hunga Ha'apai (HTHH) volcano and triggering the eruption of the Home Reef volcano; (3) We propose that the shallow stressed megathrust and large-volume of rocks with steep slopes surrounding the volcano pose significant dangers and should be incorporated into following hazard chain assessments in this region. These new findings have enhanced our understanding of subduction zone volcanoes, earthquakes, and their triggering mechanisms. They also provide valuable insights into assessing potential marine-geohazard chains, not only in the Tonga region but also in subduction zones worldwide.
OS11-A025
A DEM-based Euler-lagrange Model for Surface Waves Generated by Granular Material Intruding Into a Water Body
Wenxin LI1#+, Huabin SHI2, Xiping YU1
1Southern University of Science and Technology, 2University of Macau
The effects of interstitial fluid on the behaviors of two approaching particles play an important role in the process of landslide generated waves. In this paper, an Euler-Lagrange model is developed to study the effects of interstitial fluid on the frictional behaviors of particle contacts which is resolved by the discrete element method (DEM). A formulation of the friction coefficient for immersed particle contacts, involving the effects of interstitial fluid viscosity and pressure, is proposed based on the results of a laboratory experiment. The enhancement effect of the porosity of granular materials on the inter-particle friction coefficient is taken into account. For the inter-particle normal contact force, an existing empirical formula of the coefficient of restitution for immersed particle collisions is adopted. The model is verified in the laboratory experiment of collisions between a single particle and a solid wall in both air and water. The model is further validated by simulating subaerial granular landslides into water down an inclined slope. Without the effects of interstitial fluid on the inter-particle friction coefficient, the propagation velocity of subaerial landslides intruding into the water and the generated tsunami wave are underestimated. Moreover, if the enhancement effect of the landslide porosity is excluded, the propagation velocity of the landslide and the generated wave are overestimated.
OS11-A030
Numerical Simulation of Tsunami-driven Debris Motion Using a 3D Immersed Boundary-cumulant Lattice Boltzmann Model
Guangwei LIU+, Jinfeng ZHANG, Qinghe ZHANG#
Tianjin University
Tsunamis can generate a large amount of debris that causes damage to buildings and infrastructure (Chock et al., 2013). The motion of tsunami debris poses great challenges to post-disaster rescue and reconstruction work, making it a research hotspot (Nistor et al., 2017). However, current numerical models (Ardianti et al., 2018; Hasanpour et al., 2021) have limitations in simulating high Reynolds number turbulent flow and have low computational efficiency. Recently, the lattice Boltzmann method (LBM), a new numerical method, has been developed that has high parallel scalability and computational efficiency (Krüger et al., 2017). By combining the LBM with the immersed boundary method, the LBM can simulate the motion of debris in complex flows. This study uses the cumulant lattice Boltzmann method (Geier et al., 2015) to develop a three-dimensional high Reynolds-number debris motion model that accurately simulates the movement process of debris driven by tsunami waves. The model provides a new research method for further studying the movement rules of tsunami debris, with high scalability and computational efficiency. Using the established numerical model, the settling process of underwater thrown rocks under dynamic water conditions was simulated, and the results were in good agreement with analytical solutions and experimental data (Xu et al., 2021). In summary, the three-dimensional lattice Boltzmann model developed in this study can overcomes the limitations of current numerical models and has high computational efficiency and scalability, making it a promising tool for studying tsunami debris movement. Key words:Lattice Boltzmann method; Immersed boundary method; Numerical simulation; Tsunami wave; Debris motion.
OS11-A032
Three Dimensional Simulations of Guishan Island Landslide Event
Yi-Xuan HUANG#+, Tso-Ren WU, Pichun HUNAG, Shu-Kun HSU
National Central University
In previous investigations, the estimation of tsunami characteristics induced by landslides often relied on approximating the total tsunami volume or employing empirical formulas. In this study, Guishan Island, located off the eastern coast of Taiwan, serves as the focal point. Leveraging the numerical model, specifically the Discontinuous Bi-viscous Model (DBM), we delve into the dynamic processes of landslides triggered by rockslides and the subsequent behavior of tsunamis generated by these landslides upon entering the ocean. The study was conducted with the effort of Huang (2018), which provided a detailed investigation of landslide features in the northern maritime region of Guishan Island. Through sub-bottom profiler, sides can sonar, multi-beam bathymetric data, remotely operated vehicle (ROV) dive data, and sparker seismic reflection data, Huang (2018) proposed that the landslide deposits can be divided into three MTD (Mass Transport Deposit) units (MTD1, MTD2, and MTD3). The main avalanche deposits are identified as MTD3, and a model was proposed to explain the lateral collapse and subsequent submarine landslide events. Drawing upon the measurements of MTD3 obtained from Huang's study (2018), the present study calibrated parameters in the DBM to reconstruct ancient tsunami events around Guishan Island. This not only enhances our understanding of the dynamic processes during landslide events but also provides a valuable foundation for disaster prevention references and the formulation of strategies for potential tsunami hazards in the future.
OS11-A041
The Impact of Building Collapse on Tsunami Evacuation Routes and Mortality Rates
Tatsuya AIKAWA+, Fukuto YOSHIDA, Tomoki SHIRAI, Taro ARIKAWA#
Chuo University
Lessons learned from the Great East Japan Earthquake of March 11, 2011 have led to an increased emphasis on preparedness for the largest tsunamis, with the expectation that evacuation guidance will reduce damage. Sakata et al. (2020) and Ishiyama et al. (2023) incorporated an algorithm for determining safer evacuation routes after avoiding tsunami inundation into the agent-based evacuation simulation of Arikawa and Oie (2015) and demonstrated its applicability to tsunami evacuation. However, earthquakes can cause buildings to collapse and block roads, creating the need to investigate their impact on evacuation. Therefore, this study uses a simulation model to investigate the impact of building collapse on mortality during evacuation and to demonstrate the importance of taking building collapse into account when evacuating. As a method, the locations where debris is likely to be generated were determined based on the age and structure of the building, and the height of the debris generated on the evacuation route was given as data for each cell based on the study by Oki et al. (2016) after assuming that the building collapsed. The walking speed of evacuees walking on the debris was uniformly set at 0.5 m/s based on the results of Okabayashi et al. (2007), and was differentiated from the walking speed of 1.0 m/s without considering building collapse. The results showed that the speed delay of evacuees caused by building collapse increased the time to complete evacuation, resulting in an increase in the number of fatalities. The results of this study indicate the importance of taking building collapse into account when guiding evacuation, and the development of an evacuation route search method that takes building collapse into account is an issue to be addressed in the future.
OS11-A042
Validation of an Evacuation Tower Location Determination Method Using Evacuation Simulation: A Case Study in Ambon
Jiahao TAN+, Taro ARIKAWA#
Chuo University
Choosing an appropriate site for setting up shelters is particularly important to devise a reasonable evacuation plan to enable as many evacuators as possible to evacuate smoothly. For example, in Japan, it is usually to calculate the length of an evacuation route or accessibility when the government finds appropriate locations for constructing evacuation buildings. Besides, Notsuda and Kishimoto (2005) have investigated a capacitated allocation model and new allocation model, successfully finding optimal locations. Van-Minh Le et al. (2015) have used liner programming approach to optimize sign placement for evacuation from tsunamis. However, such research is still not comprehensively considered in other parts of the world. In this study, we aim to apply the tsunami simulator Arikawa and Oie (2015) developed to conduct a case study using optimal evacuation tower location determination theory in Ambon. Ambon is a small island in Indonesia that has historically suffered from tsunamis. However, there are few evacuations plans that exist, with only a siren tower available to warn people the coming of tsunamis. Latief et al. (2016) found that the most recent tsunami event in Ambon was a landslide-induced tsunami in 1950, which indicates that landslide tsunamis could occur again in several minutes in the future. Therefore, it is quite necessary to establish an evacuation plan in Ambon that allows people to evacuate within a few minutes. Koyanagi and Arikawa (2016) demonstrate that tsunami evacuation building can effectively reduce evacuation distance as a method of software measures. The simulation results show a decrease in mortality rates attributed to the construction of tsunami evacuation buildings by been placed in appropriate places, which confirmed the optimal placing theory.
OS11-A039
Tsunami Simulation of the 1994 Taiwan Strait Mw7.3 Earthquake and Its Hazard Implication on the Northeast South China Sea
Ziyu ZHANG1#+, Linlin LI1, Peitao WANG2
1Sun Yat-sen University, 2Ministry of Natural Resources
On 16 September 1994, a Mw7.3 earthquake occurred in the Slope Fault Zone in the southwest part of the Taiwan Strait, the largest earthquake in the offshore region of south China since the 1918 Nan’ao Mw7.5 earthquake. Strong shaking was widely felt by coastal residents in southeast China, resulting in over 800 casualties. The earthquake also generated tsunami waves which were recorded by a tide gauge near Dongshan, Fujian. This event occurred in the Slope Fault Zone which is relatively less understood in comparison to the Littoral Fault Zone in the South China Sea. However, it holds an equal potential for generating submarine earthquakes larger than Mw7.0 and triggering destructive tsunamis. Therefore, it’s crucial to assess the potential seismic and tsunami hazards in the coastal regions of the northeast South China Sea. Due to the limited geophysical observations of the seismogenic structures of the Slope Fault Zone, the focal mechanism of this event remains controversial. To gain a better understanding of this event and its following tsunami, we reconstructed the seismic source parameters and conducted forward modeling of tsunami generation and propagation. We compared tsunami waveforms generated by both the uniform slip and a range of non-uniform slip fault models. Additionally, we conducted a comparison of these results with the tidal gauge record. Our findings revealed that the tsunami waves first arrived on the east coast of Fujian, China, and impacted a large area of South China and the west coast of Taiwan. Furthermore, we observed that slip distributions and the amount of displacement strongly influenced the characteristics of the tsunami. Submarine earthquakes and tsunamis pose a significant threat to the safety of coastal cities and infrastructure. Therefore, our research aims to provide some insights into understanding the potential tsunami hazards in the northeast South China Sea.
Session Chair(s): Linlin ZHANG, Institute of Oceanology, Chinese Academy of Sciences, Akira NAGANO, Japan Agency for Marine-Earth Science and Technology, 재학 이, GeoSystem Research Corporation
OS12-A015
| Invited
Pan-regional Characterization of the Variability in the Indonesian Seas
Huijie XUE#+, Yuan WANG
Xiamen University
The Indonesian Seas feature a wide-spectrum of variations in hydrography and circulation. This study applies a simple frequency-based time series decomposition method on the 20-year model outputs without data-assimilation, and demonstrates the spatial distribution of the variations in intra-seasonal, semi-annual, annual, and inter-annual bands, respectively. The modeled sea-level variations agree well with the AVISO in four bands, guaranteeing a robust performance. In general, the ITF variability is mainly influenced by the remotely generated inter-annual variability, regional annual forcings by monsoon, and local flow instability and fluctuations, with the semi-annual variation being minor but non-trivial. The four bands of variations are further used in K-mean clustering to investigate the inherent dynamical similarities/dissimilarities for a pan-regional characterization. The two sets of clusters based on the variations of the sea-level/thermocline and current speed emphasize the competing impacts of the annual and inter-annual variations in the Indonesian Seas, which lays on a "cross-road" of the inter-annual variation dominated NE-SW deep-ocean regime and the annual variation dominated NW-SE marginal sea regime. In complementary to the previously studied inter-annual variability, we conclude that the annual variation is primarily driven by the regional monsoon wind. Moreover, profiles of annual current variations show a significant difference between the main and east branch of the Indonesian Throughflow (ITF), where annual variations play a major role above (below) the thermocline in the main (east) branch.
OS12-A016
Kinetic Energy Cascade Induced by the Interaction of Mean Flow, Topography, and Mesoscale Eddies East of Taiwan: A Scale-to-scale Analysis
Dezhou YANG#+
Chinese Academy of Sciences
The scale-to-scale kinetic energy (KE) cascade induced by the nonlinear interaction among topography, Kuroshio Current, and mesoscale eddies is systematically investigated in the coarse-graining framework based on simulated data from the well-validated Regional Ocean Model System. The KE transfer exhibits inhomogeneous spatial and temporal distributions and varies with length scale. During current-topography interaction, the KE transfers downscale across larger scales and reversely across smaller scales with an inherent separation scale of 150 km northeast of Taiwan, resulting in a significant positive net KE flux for mesoscale motions. The transfer around Suao Ridge is consistently downscaled with significant seasonal variation that is stronger in summer and weaker in winter. South of Suao Ridge, the transfer is one order of magnitude weaker and changes greatly with time. The cyclonic (anticyclonic) eddy weakens (enhances) KE transfer in most study area. In particular, the cyclonic eddy reverses the transfer direction around Suao Ridge. The anticyclonic eddy triggers a significant bidirectional transfer south of Suao Ridge. Analyses show that the special arc-shaped topographic feature and northwestward Kuroshio intrusion current are responsible for the nature of bidirectional KE transfer northeast of Taiwan. The direction of mean current relative to the topography gradient determines the transfer direction. The large-scale circulation determines the transfer intensity by changing the horizontal shear and barotropic instabilities. The KE transfer caused by nonlinear dynamics contributes significantly to the total anticyclonic eddy-induced net KE flux changes. In particular, inverse KE cascade plays a key role in net KE flux changes in mesoscale motions east of Taiwan.
OS12-A012
New Perspectives on the Generation and Maintenance of the Kuroshio Large Meander
Yang YANG1#+, X. San LIANG2
1Xiamen University, 2Fudan University
The internal dynamical processes underlying the Kuroshio large meander are investigated using a recently developed analysis tool, multiscale window transform (MWT), and the MWT-based canonical transfer theory. Oceanic fields are reconstructed on a low-frequency mean flow window, a mesoscale eddy window and a high-frequency synoptic window with reference to the three typical path states south of Japan, i.e., the typical large meander (tLM), nearshore non-large meander (nNLM) and offshore non-large meander (oNLM) path states. The interactions between the scale windows are quantitatively evaluated in terms of canonical transfer, which bears a Lie bracket form and conserves energy in the space of scale. In general, baroclinic (barotropic) instability is strengthened (weakened) during the tLM state. For the first time we found a spatially coherent inverse cascade of KE from the synoptic eddies to the slowly varying mean flow; it occupies the whole large meander region but exists only in the tLM state. By the time-varying multiscale energetics, a typical large meander is preceded by a strong influx of mesoscale eddy energy from upstream with a cyclonic eddy, which subsequently triggers a strong inverse KE cascade from the mesoscale window to the mean flow window to build up the KE reservoir for the meander. Synoptic frontal eddies are episodically intensified due to the baroclinic instability of the meander, but they immediately feed back to the mean flow window through inverse KE cascade. These results highlight the important role played by inverse KE cascades in generating and maintaining the Kuroshio large meander.
OS12-A007
Spatiotemporal Features and Generation Mechanisms of Submesoscale Processes in the Western Tropical Pacific Ocean
Yuchao HUI1#, Linlin ZHANG2+
1Chinese Academy of Sciences, 2Institute of Oceanology, Chinese Academy of Sciences
The spatiotemporal characteristics and generation mechanism of submesoscale processes (SMPs) in the western tropical Pacific Ocean were investigated based on 1/30º Ocean General Circulation Model for Earth Simulator (OFES) outputs and mooring measurements. Elevated submesoscale activities are detected along the paths of Mindanao Current and Halmahera Eddy. Their spatial scales are short than 80 km and typical periods are in the band of 4-20 days. Mooring observations reveal that the SMPs not only exit the mixed layer, but also extend to 150m that is deeper than the mean thermocline. The SMPs exhibit obvious seasonal cycle, with high submesoscale kinetic energy (SMKE) appearing in summer and autumn and weak SMKE in winter and spring. Due to the shallow mixed layer depth, the pathway that SMPs extract available potential energy by mixed layer baroclinic instability is blocked. The barotropic instability associated the current-islands interactions is responsible for the generation and seasonal modulation of SMPs. Further energetic analysis indicates that the SMKE is mainly injected from the mean flow, with the kinetic energy conversion rate integrated in the upper 200 m of 17.1×10-7 m3/s3, which is almost as twice large as that of from mesoscale field (8.9×10-7 m3/s3). Furthermore, the SMKE budget results imply a forward dissipation process of SMPs, which reveals an important role of SMPs on the ocean energy cycle in the western tropical Pacific Ocean.
OS12-A013
| Invited
ENSO-related Temperature, Salinity, Current Variations in the Western Subarctic North Pacific Produced by CMIP6 GFDL-CM4 Climate Model
Akira NAGANO#+, Masahito SHIGEMITSU, Masahide WAKITA
Japan Agency for Marine-Earth Science and Technology
The ocean acidification at station K2 (47˚N, 160˚E) in the western subarctic North Pacific is affected by the El Niño-southern oscillation (ENSO) in the equatorial Pacific. In our previous studies based on the observations at K2, it was suggested that the ocean acidification in winter is accelerated by the change of physical conditions, especially by the enhanced entrainment of deep water rich in dissolved inorganic carbon into the mixed layer due to the El Niño-related intensification in the vertical eddy diffusivity. The variations in biogeochemical variables produced in the CMIP6 GFDL-CM4 climate model are consistent with the observation at K2. Therefore, we examined the variations in temperature, salinity, and current velocity in the western subarctic region from 1979 to 2014 derived from the climate model. The variation mode of current velocity, which has a phase reversal at depth layer of approximately 200–300 m, is excited by higher baroclinic Rossby wave modes than the first wave mode through the atmospheric ENSO teleconnection. Furthermore, in association with the deepening of the mixed layer in autumn to winter of El Niño years, cold and saline deep water is entrained into the mixed layer probably through the intensification in the vertical eddy diffusivity. These results support the mechanism of the winter ocean acidification suggested by our previous studies on the basis of the observations at K2.
OS12-A003
Seasonal Link Between Deepwater Overflow Through the Luzon Strait and Deep Western Boundary Current in the Philippine Sea
Qinbo XU#+
Chinese Academy of Sciences
The cold dense water from the Pacific sinks to the deep South China Sea (SCS) through the Luzon Strait, driving the abyssal and overturning circulations in the SCS, and affecting the Indonesia Throughflow and its associated heat and freshwater fluxes. Combining the ocean bottom pressure data and the hydrographic data, we reveal the seasonal link between Luzon Strait deepwater overflow (LSDO) and deep western boundary current (DWBC) in the Philippine Sea. The seasonal variation in the DWBC dominates the pressure difference between the Pacific and the SCS by adjusting the temperature field on the east side of the Luzon Strait, which in turn contributes to the seasonal variation in the LSDO. The enhanced DWBC in summer/autumn carries more relatively cold water from the high latitudes to the east of the Luzon Strait, increasing the local density and leading to the enhancement of the LSDO in autumn.
OS12-A010
Variability of Diurnal Internal Tides Observed in the Eastern Philippine Sea
Kang-Nyeong LEE1#+, Chanhyung JEON2, Xiao-Hua ZHU3, Hong Sik MIN4, Zhongxiang ZHAO5, Jae-Hun PARK1
1Inha University, 2Pusan National University, 3Second Institute of Oceanography, 4Korea Institute of Ocean Science & Technology, 5University of Washington
The internal tides generated from Luzon Strait (LS) have the highest energy globally and propagate both westward and eastward from the LS. Altimeter observations reveal that the low-mode diurnal internal tides (DITs) propagate eastward, extending into the Pacific Ocean. As they propagate, DITs refract equatorward due to the Coriolis effect, with their beam propagations potentially influenced by background currents including mesoscale eddies. In this study, we utilize in-situ round-trip acoustic echo time measurements between the seafloor and the sea surface from an array of 10 pressure-recording inverted echo sounders (PIES) to investigate the variabilities of DITs in the eastern Philippine Sea, approximately 2500 km away from the LS. The observation, conducted for about a year or 1.5 years during 2020–2021, revealed semi-annual variation in DITs with asymmetrical amplitudes during summer and winter periods. DITs extracted from the long-term multi-satellite altimeter measurements exhibit symmetrical semi-annual variation in the observation region, consistent with the barotropic diurnal tides in LS, which does not account for the observed asymmetrical variation with weakened amplitudes during summer periods. Utilizing a ray-tracing method based on the phase speed of DIT from the numerical simulation results (hybrid coordinate ocean model; HYCOM), we found that some portion of the DIT beams could reach to the PIES array in general. However, when warm eddies existed near the eastern side of the LS in summer months from July to September, the eddy-induced increased propagation speed of DITs could enhance their equatorward refraction, which appears to have resulted in the observed weakening of DIT amplitudes during summer periods. Freely-propagating DITs are one of the important sources for the diapycnal mixing in the northwestern Pacific, and our results imply that the significant time-varying features of DITs should be considered for a better parameterization of ocean mixing in the ocean and climate models.
Session Chair(s): Chan Joo JANG, Korea Institute of Ocean Science & Technology
OS21-A016
| Invited
Arctic Warming Contributes to Increase in Northeast Pacific Marine Heatwave Days Over the Past Decades
Sang-Wook YEH#+
Hanyang University
The frequency and duration of marine heatwaves have been increasing with ocean warming due to climate change. In particular, the Northeast Pacific has experienced intense and extensive marine heatwaves since the late 1990s – characteristically called “the Blob”. Here, an investigation of satellite-derived and reanalysis data supported by idealized coupled model experiments show that Arctic warming plays an important role in the increase in Northeast Pacific marine heatwave days during boreal summers. Strong Arctic warming has acted to change the atmospheric circulation pattern over the Northeast Pacific and reduce the low-level cloud fraction from late spring to early summer. We show that the enhancement of solar radiative heat fluxes and reduced latent heat loss over a relatively large area has favored an increase in sea surface temperatures and marine heatwave days. An idealized model experiment performed here, designed to isolate the impact of Arctic warming, supports this hypothesis. The projected changes of Arctic climate on the occurrence of marine heatwaves should be considered in climate change adaptation and mitigation plans.
OS21-A008
| Invited
Strong Subsurface Marine Heatwaves in the Tropical Western Pacific Ocean: Evolution, Drivers and Implication
Shijian HU1#+, Shihan LI2
1Hohai University, 2Chinese Academy of Sciences
Marine heatwaves (MHWs), which are discrete extreme oceanic warming events, have important impacts on the marine ecosystem, fishery resources, and social economy. Previous studies based on sea surface temperature suggest that MHWs in the tropical western Pacific Ocean are very weak. However, we find that the MHWs observed by the Tropical Atmosphere Ocean/Triangle Trans-Ocean Buoy Network buoys in the tropical western Pacific Ocean are unexpectedly strong in the subsurface layer (50–300 m depth). The ensemble mean intensity of subsurface MHWs shows a peak of about 5.2 ◦C at 150 m with an ensemble mean duration ranging from 13 to 22 days. It seems that the subsurface MHWs are strong and frequent in April–June but relatively weaker and less frequent in September and October than in other months. Anomalous sea surface convergence and Ekman down-welling play an important role in the evolution of subsurface MHWs in both onset and decay phases. Strong subsurface MHWs are likely to affect the fishery production of tropical western Pacific. Subsurface MHWs are widely observed across global oceans, extending beyond the tropical western Pacific region.
OS21-A010
Detecting Marine Heatwaves Below the Sea Surface Globally Using Physically Informed Statistical Learning
Xiang ZHANG1+, Furong LI1, Zhao JING1#, Bohai ZHANG2
1Ocean University of China, 2Beijing Normal University & Hong Kong Baptist University United International College
Extreme warm water events, known as marine heatwaves (MHWs), cause a variety of adverse impacts on the marine ecosystem. MHWs can occur everywhere in the oceanic epipelagic zone yet monitoring MHWs below the sea surface is still challenging due to sparse in-situ temperature observations. Here, we propose a statistical learning method guided by ocean dynamics, to capture the spatially and seasonally varying relationship between satellite-based sea surface observations (sea surface temperature and sea surface height) and subsurface MHWs in the oceanic epipelagic zone globally. This physically informed statistical learning method shows good skills in detecting subsurface MHWs over many parts of the global ocean. It outperforms both the classical ordinary least square regression and cutting-edge deep neural network models that do not utilize physical information. Our study provides a useful statistical learning method for near real-time monitoring of subsurface MHWs at a global scale and highlights the importance of incorporating physical information for enhancing the efficiency and interpretability of statistical learning.
OS21-A003
A Quantitative Analysis of Marine Heatwaves in Response to Rising Sea Surface Temperature
Min ZHANG#+
Ministry of Natural Resources
It has been proven that marine heatwaves (MHWs) have increased in frequency, duration, and intensity over the past few decades, and this trend will accelerate further under continued global warming. While more intense and frequent MHWs are an expected consequence of rising sea surface temperatures (SSTs) under continued global warming, it remains unclear to what degree per Celsius warming trend of SSTs contributes to the changes in the MHW metrics. Here, we focus on how the MHW metrics evolve with the SST warming trend by using an adaptive data analysis method based on observational datasets covering the past four decades. We find that the globally averaged increasing rates of the annual MHW frequency, duration, and maximum intensity are approximately 3.7 events, 7.5 days, and 2.2 degrees Celsius per degree Celsius of SST rise, respectively. The increasing rates for the annual MHW days and the fraction of the spatial extents to the global ocean affected by MHWs are approximately 58.8 days and 13.9% per degree Celsius of SST rise, respectively. Based on these observational-based increasing rates and the projected SST warming from the selected Coupled Model Intercomparison Project Phase 6 (CMIP6) models, the spatial distributions of changes in annual MHW days, frequency, and cumulative intensity are projected to exhibit 2-fold, 4-fold, and 6 to 8-fold increases under the three socioeconomic pathways (i.e., SSP126, SSP245, and SSP585), respectively. The globally averaged annual MHW days will increase to approximately 224.2 ± 26.9 days, and the largest changes are projected to occur in the northeast Pacific, the North Atlantic, the south Indian Oceans, and parts of the Southern Ocean, with approximately 14.8 ± 5.7% of the global ocean reaching a permanent MHW state by the end of the twenty-first century under SSP585.
OS21-A005
Arctic Marine Heatwave Projections Based on CMIP6 Models
Yan HE1+, Qi SHU1, Zhenya SONG1, Fangli QIAO2#
1Ministry of Natural Resources, 2State Oceanic Administration
Marine heatwaves (MHWs) and total heat exposures (THEs), the extreme warming events occurring in the oceans, seriously threaten the marine ecosystems and coastal communities in a warming climate. However, the future changes in MHWs and THEs in the Arctic Ocean are still unclear. Based on the latest CMIP6 climate simulations and projections under SSP5-8.5 scenario, we find that both MHWs and THEs in the Arctic Ocean are likely to become more intense and prolonged in a warming climate mainly due to the Arctic sea ice decline. The MMM indicates an increase of 0.78°C in MHW mean intensity when averaged over the Arctic Ocean. The projected Arctic Ocean MHW increase indicates that the marine ecosystems in the Arctic Ocean will face much greater threats from climate change than that in most of the global oceans.
OS21-A004
Representative Bias of Marine Heatwaves in the North Pacific Ocean Simulated by CMIP6 Models: A Clustering-based Approach
Wonkeun CHOI1+, Heeseok JUNG1, Zhenya SONG2, Chan Joo JANG1#
1Korea Institute of Ocean Science & Technology, 2Ministry of Natural Resources
Climate models are the primary tool for projecting marine heatwaves (MHWs). Assessing the simulation performance of the climate model is crucial before projecting future changes in MHW, as it helps comprehend how model bias can influence the interpretation of future changes. Previous research has mainly focused on assessing the common bias produced by multi-model ensembles of climate models. However, in the evaluation of individual models, certain groups exhibit comparable bias patterns, and clustering them can provide a variety of representative biases. In this study, we aimed to evaluate the MHW characteristics from 30 Coupled Model Project Intercomparison Phase 6 (CMIP6) models in the North Pacific Ocean compared to OISST reanalysis data for 33 years (1982–2014), and to cluster CMIP6 models with similar bias patterns in order to understand the representative bias. Based on similar patterns of MHW bias, hierarchical clustering was used to classify the 30 CMIP6 models into five groups. In terms of total MHW days, the first group showed a spatial distribution of overestimation similar to the Pacific decadal oscillation pattern. In addition, other groups showed a concentrated overestimation in the Kuroshio Extension, the southwestern North Pacific and the Bering Sea for their respective spatial distributions. Regarding the mean MHW intensity bias, more than 80% of the CMIP6 models showed a dipole pattern in the Kuroshio Extension. Thus, the performance of the ocean current simulation was assessed using the same model for each of the clusters. The clusters that show a dipole pattern in mean intensity indicate a simulation of the Kuroshio Current that extends further north than observed. By presenting representative biases that differ from the common biases but are shared by multiple models, this study suggests that it is necessary to identify representative biases to interpret the future MHWs simulated by specific climate models.
Session Chair(s): Linlin LI, Sun Yat-sen University, Yuichiro TANIOKA, Hokkaido University
OS11-A036
Tsunamigenic Potential of Intraplate Earthquakes in the Northern South China Sea
Linlin LI1#+, Philip Li-Fan LIU2, Qiang QIU3, Zhigang LI1, Peizhen ZHANG1
1Sun Yat-sen University, 2National University of Singapore, 3SCSIO, Chinese Academy of Scienc
The northern continental shelf in the South China Sea has developed two active fault zones. One parallels to the southern coastline of China which is known as the Littoral Fault Zone (LFZ); the other goes along the edge of continental shelf which is poorly known. The two sibling fault zones, both run ~1000 km-long and, have high seismic activity in the past, posing a great seismic and tsunami risk to the southern coast of China and the neighboring regions. Historically, the faults had generated many moderate to large earthquakes including 4 events with Mw >7 since 1600. The newly obtained geophysical data and geological records, clearly indicate strong earthquakes may have occurred in the segment that was previously assumed less seismogenic. Although the seismic hazard of both faults, especially LFZ has long been recognized, its associated tsunami hazard is ignored or underrated. Here, we carefully review historical documents of major earthquakes in the northern South China Sea (SCS). We find the majority of major historical earthquakes were accompanied by tsunami phenomena which were documented by local chronicles and genealogies, including the 1605 M 7.5 Qiongzhou, the 1604 M 8.0 Quanzhou events, 1918 M 7.5 Nanao, the 1992 Hainan event and the 1994 Taiwan Strait earthquake event. Based on the geological setting, available geophysical data and historical documents, we systematically reconstruct/recover the earthquake information of these tsunamigenic events and investigate the key features of tsunami hydrodynamics generated by such intraplate earthquakes located on shallow continental shelf. Our results suggest that the tsunami generated by earthquakes along these faults possesses unique features which may cause substantial damage in future.
OS11-A043
Tsunami Early Warning Using High-frequency Ocean Radar System in Kii Channel, Japan
Yuchen WANG#+, Kentaro IMAI
Japan Agency for Marine-Earth Science and Technology
The high-frequency (HF) ocean radar system is a shore-based remote sensing system that monitors sea surface currents, waves, and wind over large areas. It can measure tsunami-induced surface current velocity and provide information for tsunami early warning. An HF ocean radar system measured the tsunami velocity in Kii Channel, Japan, during the 2011 Tohoku earthquake. We adopted the tsunami data assimilation algorithm to predict coastal tsunami waveforms. It is a method that reconstructs the tsunami wavefield using offshore data. To process the HF radar data as the input, we initially converted the current velocity along the beam direction to into u, v directions (i.e., EW, NS directions). This process also involved the spatial interpolation of observational points from the beam of two HF radar land stations. The data assimilation started at 08:05 (UTC, hereafter) on March 11, 2011. We predicted coastal tsunami waveform at Kobe and compared it with real observations. The forecast at 08:10 underestimated the tsunami amplitude, achieving an accuracy of 50.1% with a mean squared prediction error (MSPE) of 0.0101. However, the forecast at 08:20 matched well with the real observation, boasting an accuracy of 82.9% and a reduced MSPE of 0.0098. At 08:30, it continued to perform similarly, maintaining consistency between the predicted and observed waveforms. The accuracy was 81.3% and the MSPE further decreased to 0.0093. Given that the tsunami arrived in Kobe at 09:10, our approach can make an accurate prediction at least 50 min before its arrival. To summarize, we demonstrated the effectiveness of the HF ocean radar system in tsunami early warning. The case study of the 2011 Tohoku tsunami yielded a remarkable accuracy of over 80%. In the future, we will investigate the relationship between the distribution of HF radar observational points and the forecast accuracy.
OS11-A046
Effects of Tide on Tsunami Induced Sediment Transportation
Fating LI1,2+, Linlin LI1#, Yu-Lin TSAI3
1Sun Yat-sen University, 2Kyoto University, 3National Yang Ming Chiao Tung University
Tsunami deposits can provide crucial insight when estimating the frequency, size, and possible source of historical tsunamis and paleo-tsunamis. However, previous studies usually ignore the interaction between tsunamis and tides in numerical modeling, leaving a research gap for evaluating tsunami-induced inundation and sediment transportation. Even though the field observations and numerical experiments have pointed out the tide effect on tsunami wave propagation, the tide-tsunami interaction with subsequent sediment transportation has not been quantitatively investigated. In this study, Hong Kong and Nan'ao Island, located in the northern South China Sea with tsunami deposit reported, are selected to showcase the tide effect on tsunami-induced sediment transportation in typical shallow marine environments and coastal plains respectively. By coupling a shallow water equation model with a non-hydrostatic wave/sediment module, COMCOT-SED (COrnell Multi-grid COupled Tsunami Model-SEDiment) is in charge of performing all the simulations in this study. Using a forward modeling approach, we will simulate the complete physical process of inundation and sediment transport induced by tsunamis. Tsunami scenarios are considered according to the earthquakes from the Littoral Fault Zone and the Manila Trench. In addition to sediment transport, this study will focus on analyzing the tide effect on tsunami wave propagation including the changes of tsunami wave heights and current velocities. Moreover, the interaction among tides, tsunamis, and sediment deposits will be also discussed. The findings of this study are expected to provide a quantitative understanding of the tide effect on the tsunami deposit process.
OS11-A053
Predicting Tsunami Impact in Asia-Oceania: Advanced Modelling of Wave Heights Using MOST
Nazeel SABAH#+, Daya SHANKER
Indian Institute of Technology Roorkee
In the tsunami-prone Asia-Oceania region, advanced forecasting of tsunami wave heights is critical for developing effective coastal defence strategies. This paper presents a novel approach to predict Level I tsunami heights (occurring once in 100 years) for six high-risk zones. Utilizing the Method of Splitting Tsunami (MOST), we model tsunamis in three phases: ocean floor deformation due to seismic events, deep ocean wave propagation, and coastal inundation. Our methodology uses Finite Difference Models to accurately simulate these phases. Significantly, we forecast the maximum wave height and inundation for realistic and worst-case scenarios, validated by an Artificial Neural Network algorithm. For instance, our study predicts a maximum wave height of 61.18 meters in Indonesia between 2051-2064, with an inundation area of 12 square kilometres and a maximum wave velocity of 20.1 knots. Similar forecasts are performed for other zones, providing crucial data for enhanced coastal defences and evacuation planning in the region. This comprehensive analysis is validated by an Artificial Neural Network algorithm, underscoring its accuracy and relevance for disaster preparedness strategies.
OS11-A048
Mechanism of Tsunami Wave Trapping on the Northern Continental Shelf of the South China Sea and Its Impacts
Xiwen LIU+, Linlin LI#
Sun Yat-sen University
The northern continental slope of the South China Sea (SCS) has significant impacts on the propagation of tsunamis generated from various tsunami sources in the SCS, including earthquakes originated from the Manila Subduction Zone, Littoral Fault Zone and Slope Fault Zone, and landslides on the continental slope (e.g., the Baiyun landslide, Qiongdongnan landslide, and Huaguang landslide). These impacts include reflection, shoaling, shelf oscillation and resonance induced by slope reflection. Therefore, understanding the role of the northern continental slope of the SCS is crucial for comprehending the generation and propagation mechanisms of tsunamis, as well as for assessing tsunami hazards along the southern coast. In this study: 1. Based on the water particle trajectories of tsunami progressive wave, a single-width mass is introduced to analyze the reflective and shoaling effects of the slope on tsunami waves. We aim to identity the determining factors that govern reflection and shoaling and present the corresponding reflective and shoaling coefficients during the wave-slope interaction process. 2.We analyzed the mechanism of tsunami wave trapping on the continental shelf, which is attribute to the reflection caused by continental slope. Then, continuous wavelet transforms of virtual tidal station data on the top of the slope and in the basin revealed the inherent frequencies of the slope and possible resonant frequencies. 3. Numerical simulations are performed to validate the slope's reflection and shoaling, as well as the resonance frequencies induced by slope reflection, quantifying the impacts of these slope processes on tsunami wave propagation in the South China Sea.
Session Chair(s): Emilia Kyung JIN, Korea Polar Research Institute, Jiuxin SHI, Ocean University of China
OS03-A010
| Invited
Dynamics for Cross-slope Water Exchange in the Ross Sea, Antarctica
Zhaoru ZHANG1#+, Yuanjie CHEN1, Michael DINNIMAN2, Zhiqiang LIU3, Lixin QU1, Chuning WANG1
1Shanghai Jiao Tong University, 2Old Dominion University, 3Southern University of Science and Technology
Water mass exchanges across the slope of the Ross Sea have critical impacts on not only the physical and biological environments of the Ross Sea shelf but also on the meridional overturning circulation. The central Ross Sea slope is a crucial region for the exchange of water masses. In this study, a high-resolution coupled ocean-sea ice-ice shelf model is used to investigate the controlling mechanisms for the cross-slope transports in the central Ross Sea. The vertical structure of cross-slope exchange is characterized by onshore transports of the Antarctic Surface Water (AASW) and Circumpolar Deep Water (CDW) and offshore transport of the Dense Shelf Water (DSW). Momentum balance analysis indicates that cross-slope transport exhibits high-frequency oscillations, with a periodicity of approximately 34 hours, which is associated with the Topographic Rossby Waves (TRWs), but its contribution to the net transport is small. The offshore transport of DSW is driven by the pressure gradient force associated with interfacial form stress at the CDW/DSW interface and bottom Ekman transport associated with the Antarctic Slope Current (ASC). The southeastward sea surface height gradient, induced by DSW displacing less dense water in the bottom layer, drives the onshore transport of CDW. This process is partially counteracted by the transport driven by baroclinic pressure gradient force and transport driven by advection resulting from spatial variations of the ASC.
OS03-A015
Responses of Dense Shelf Water in Ross Sea to Large-scale Atmospheric Variability
Sung-Ho CHOO1+, Taekyun KIM1#, Jae-Hong MOON1, Emilia Kyung JIN2
1Jeju National University, 2Korea Polar Research Institute
On the Antarctic continental shelf, Antarctic Bottom Water (AABW), a major component of the lower cell of the global overturning circulation, is formed through the mixing of various water masses. Seasonal changes in salinity flux in the Antarctic shelf waters are strongly affected by large-scale atmospheric variabilities. The Southern Annular Mode (SAM) and the Southern Oscillation (SO) are the most dominant large-scale atmospheric variabilities that affect the Southern Ocean. The main purpose of this study is to investigate the responses of ocean circulation, and subsequent changes in water masses to large-scale atmospheric variabilities. The Dense Shelf Water (DSW) generated in Ross Sea is a major source of AABW flows down to the abyssal Pacific Ocean. In this study, we introduced an ocean circulation model for the Ross and Amundsen Seas that considers physical interactions between ocean and ice-shelf. Sensitivity experiments are designed to examine the effects of SAM separate from the effects of SO. By comparing with the results of control experiments using the climate atmospheric forcing fields, DSW salinity anomaly in the Ross Sea continental shelf area were analyzed according to the variability of SAM or SO. The DSW salinity in Ross Sea is increased in positive SAM experiment, which was mainly attributed to more active sea ice formation under colder surface air temperature and stronger wind than control run. Also the evaporation minus precipitation (E-P flux) increase contributed to salinification of DSW in positive SAM experiment. The negative SAM experiment shows opposite results in Ross Sea shelf region. The response of DSW salinity to SO phase is less sensitive compared to SAM. However, the ocean currents in the eastern Ross Sea tend to sensitive to SO phase. The result of this study is expected to provide a perspective to predict the change in deep circulations in future climate scenarios.
OS03-A024
Effects of Ross Sea Circulations on Biological Transports and Aggregations
Heng HU+, Zhaoru ZHANG#, Huizi DONG
Shanghai Jiao Tong University
As one of the most productive areas in the Southern Ocean, the Ross Sea is an ideal region for studying of Antarctic marine biological resources and the controlling mechanisms for their distributions. In this study, we focused on the physical and biological control of aggregations and transports of three species (Antarctic krill, crystal krill and Antarctic silverfish) in the Ross Sea in summer. We analyzed the role of chlorophyll and sea ice distributions on the aggregation of these species. Lagrangian Coherent Structures (LCS) analysis was performed on the simulated flow fields from a coupled ocean-sea ice-ice shelf model in the Ross Sea, to investigate the effects of surface flows on mass transport which explains the mechanisms influencing the bio-aggregations. The results show that the aggregations of the three species are generally located in the area with low sea ice concentration as the open water can enhance the irradiance available to primary production. The aggregations are also affected by physical processes. Convergent flow structures in the northwestern Ross Sea and the coastal area off the Victoria Land allow the aggregation of Antarctic krill larvae, and the circular transport barrier near the Terra Nova Bay confines the larval movements of crystal krill and Antarctic silverfish within the Bay.
OS03-A014
Influence of Warming Climate Changes on the Future Evolution of Thwaites Glacier, West Antarctica
In-Woo PARK1,2+, Emilia Kyung JIN1#, Kang-Kun LEE2
1Korea Polar Research Institute, 2Seoul National University
Over a three-decade span of surveillance in Antarctica, it has contributed to sea level rise through the loss of ice mass. Ocean forcing stands out as a significant factor contributing to an acceleration in sea level rise from the Antarctic ice sheet. Despite attempts by various groups to couple ice-ocean interactions, projecting centuries into the future under climate change is constrained by the expensive computational cost in ocean modeling. An alternative approach is to parameterize sub-ice shelf melting using a physically based method. Thwaites Glacier in West Antarctica has experienced an intrusion of warm modified Circumpolar Deep Water (mCDW) leading to thinning ice shelves and continuous loss of ice mass. To investigate the future evolution of Thwaites Glacier under CMIP6 scenarios, we adopt two ocean parameterizations: 1) Potsdam Ice-shelf Cavity mOdel (PICO) and 2) PICOP. For surface mass balance (SMB), we employ a traditional SMB approach (NonSEB) and a surface energy balance (SEB) approach, accounting for an increase in ice surface melting under warming climate changes. In three-century projections, Thwaites Glacier consistently loses ice mass under both moderate and warming climate changes. Under warming climate changes, weak ocean forcings simulated by PICO displays that an increase in SMB driven by an increase in air temperature overcomes ice discharges, leading to a deceleration in sea level rise. In contrast, PICOP displays higher melting, leading to a dramatic increase in sea level rise. Moreover, in the SEB experiments, it is confirmed that sea level rise accelerates under the warming climate change as surface melting increases in both PICO and PICOP experiments starting objective of this study. Acknowledgements: This research was supported by Korea Institute of Marine Science & Technology Promotion(KIMST) funded by the Ministry of Oceans and Fisheries(RS-2023-00256677; PM24020).
OS03-A012
Spatiotemporal Characteristics of Antarctic Ice Sheet Mass Variations from 2003 to 2022 Revealed by Satellite Gravimetry
Wei WANG+, Yunzhong SHEN#, Qiujie CHEN, Fengwei WANG
Tongji University
The Antarctic Ice Sheet (AIS) holds enough water to raise the global sea level by 58 m and is vulnerable to global climate change. Given the current intensive global warming, we investigate the AIS mass changes from January 2003 to December 2022 using the newly released satellite gravimetry and atmospheric datasets. The results show that the continuous mass loss in the AIS between 2003 and 2020 was 141.8 ± 55.6 Gt/yr. During this period, the Amundsen Sea sector and the Antarctic Peninsula experienced apparent mass loss, while the geographical pattern of the Eastern Antarctic mass change is complex, with mass loss over the Coats Land and George V Land and gain over the Queen Mary Land, George V Land, and Coats Land. Between 2021 and 2022, the AIS showed a record-breaking mass gain of 129.7 ± 69.6 Gt/yr. Specifically, the mass gain over the East AIS and Antarctic Peninsula was unprecedented within the past two decades. Basin-scale analysis shows that the mass gain mainly occurred over Wilhelm II Land, Queen Mary Land, Wilkes Land, and the Antarctic Peninsula due to anomalously enhanced precipitation. Further investigation reveals that symmetrically distributed high-low pressure systems drive abnormal precipitation and mass accumulation from 2021 to 2022 at approximately 120°W and 60°E in the Southern Ocean.
OS03-A002
Potential Sources of Low-frequency Variability in Dronning Maud Land (Antarctica)
Stéphane VANNITSEM1#+, David DOCQUIER1, Sarah WAUTHY2, Jean-Louis TISON2
1Royal Meteorological Institute of Belgium, 2Université Libre de Bruxelles
The low-frequency variability of the d18O recorded in ice cores (FK17 and TIR18) drilled recently at two different locations in Dronning Maud Land (Antarctica), is investigated using multi-taper spectral method and singular spectrum analysis. Multiple dominant peaks emerge in these records with periods between 3 to 20 years. The two sites show distinct spectral signature, despite their relative proximity in space (about 100 km apart), suggesting that different processes are involved in generating the variability at these two sites. In order to clarify which processes are acting on d18O at these two locations, the impact of several climate indices as well as sea ice area is investigated using a directional dependence technique, known as the Liang-Kleeman rate of information transfer. This approach allows for isolating a common driver, the Indian Ocean Dipole, for both ice cores. For FK17, two additional drivers are isolated, the Pacific Decadal Oscillation and the sea ice area over 0-40°E, while for TIR18, the El-Niño/Southern Oscillation plays an important role. The implications of these findings are briefly discussed.
OS03-A004
Rapid Warming of the Southern Ocean Modulated by Inter-annual and Decadal Climate Variability
Kewei LYU#+, Yutong ZHENG
Xiamen University
As the emission of anthropogenic greenhouse gases increases, the Southern Ocean absorbs substantial heat from climate change and warms rapidly. In this study, we analyze updated ocean observational datasets and find that the warming of the Southern Ocean, especially within two warming hotspots in the South Pacific and the South Indian Ocean, presents significant interannual and decadal variations. Particularly, there was a rapid warming over 2003-2012, a warming slowdown or even cooling after 2013, and another surge of warming tendency over 2020-2022 under the influences of recent triple La Nina events. We further decompose the ocean temperature change into two processes: spiciness (temperature variation along neutral density surface) and heave (vertical heave of neutral density surface). Both the long-term trend and short-term variations of the Southern Ocean warming are dominated by the heave component. The drivers and mechanisms for the inter-annual and decadal variations of the Southern Ocean warming are currently under investigation.
Session Chair(s): Yukio MASUMOTO, The University of Tokyo, Sunghyun NAM, Seoul National University
OS06-A001
Can Coastal Upwelling Trigger a Climate Mode? A Study on Intraseasonal-scale Coastal Upwelling Off Java and the Indian Ocean Dipole
Takanori HORII1#+, Eko SISWANTO1, Iskhaq ISKANDAR2, Iwao UEKI1, Kentaro ANDO1
1Japan Agency for Marine-Earth Science and Technology, 2Sriwijaya University
Coastal upwelling along the southern coast of Java brings cold and nutrient-rich subsurface water to the surface. In this study, we explored whether the upwelling could trigger the onset of the Indian Ocean Dipole (IOD) by supplying cold water to the southeastern tropical Indian Ocean. We used satellite-based daily chlorophyll-a concentration (Chl-a) data during 2003-2020 as a proxy of the coastal upwelling. We focused on first Chl-a bloom that occurred in April–June, the onset phase of the positive IOD (pIOD). We found that the timing and strength of the upwelling signals were significantly correlated with the subsequent IOD peaks. Using observational datasets, we diagnosed processes associated with the upwelling affecting sea surface temperature (SST) in the southeastern Indian Ocean. Results indicate that after the cold-water upwelling south of Java, westward surface temperature advection plays a role in anomalously cooling the SST in the southeastern Indian Ocean and setting a favorable condition for the subsequent pIOD development. Accurate understanding of the upwelling and cold-water advection on an intraseasonal timescale during the pIOD onset phase will modify our seasonal prediction of Indian Ocean climate.
OS06-A004
Impacts of Sea Surface Temperature Gradient on Monsoon Intraseasonal Oscillation
Lei ZHOU1#+, Tao LIAN2, Baosheng LI3, Ting LIU4, Jianhuang QIN5, Yan DU6, Dake CHEN4
1Shanghai Jiao Tong University, 2Second Institute of Oceanography, Ministry of Natural Resources, 3Sun Yat-Sen University, 4Ministry of Natural Resources, 5Hohai University, 6Chinese Academy of Sciences
The northward-propagating monsoon intraseasonal oscillation (MISO) is the pronounced variability over the tropical Indian Ocean during the Indian summer monsoon. MISO is accompanied by significant air-sea interactions, however, the mechanism of the oceanic feedback to MISO is still a great scientific challenge. In this study, the role of the intraseasonal sea surface temperature (SST) gradient in MISO is diagnosed using reanalysis products and model experiments. It is well-known that an intraseasonal PBL convergence anticipates convection for approximately 3 days, which benefits the new convection buildup and enhances the MISO. This study finds that the positive meridional gradient of intraseasonal SST induces positive wind convergence in the planetary boundary layer (PBL) and leads convection by about 1-2 days. The meridional SST gradient at the intraseasonal timescale can effectively intensify the intraseasonal PBL convergence by the vertical momentum mixing. Before the deep convection center, the warm SST anomalies at intraseasonal timescale destabilizes the PBL and thus enhance downward transport of momentum from aloft. This accelerates the intraseasonal northerly wind in the PBL. Consequently, changes in the speed of intraseasonal northerly along the meridional direction strengthen the PBL wind convergence ahead of deep convection. In addition, historical runs from the CMIP6 models reveal that a strong (weak) SST meridional gradient at an intraseasonal timescale amplifies (lessens) the MISO intensity in the model simulation. Therefore, this study highlights the role of SST meridional gradient in the feedback to MISO, which differs from the weak contribution of the warm SST itself to the wind convergence mentioned in previous studies. Collectively, these findings indicate that consideration of oceanic feedback is necessary to improve the understanding and simulation of MISO.
OS06-A007
Seasonality of Relationship Between Tropical Cyclone Frequency Over the Southern Hemisphere and Tropical Climate Modes
Tomomichi OGATA#+
Japan Agency for Marine-Earth Science and Technology
In this study, the author examined the tropical cyclone (TC) activity over the southern hemisphere (SH) and its relationship with tropical climate modes, such as the El Niño–Southern Oscillation (ENSO), during the austral summer (December–January–February; DJF) and fall (March– April–May; MAM). The correlation analysis between the TC activity and the global sea surface temperature (SST) suggested that an increased TC activity over the southwestern and southeastern Indian Ocean (SWIO and SEIO) was associated with a La Niña-like SST pattern, while an increased TC activity over the southwestern Pacific (SWP) was associated with an El Niño-like SST pattern. The atmospheric conditions accompanying the TC increase over the SWIO/SEIO indicated that a La Niña induces tropospheric cooling over the tropics with cyclonic circulation anomalies over the TC genesis region. Both the SST anomalies and the cyclonic circulation anomalies were significantly correlated with TC genesis parameters, suggesting that they contributed to TC genesis. To investigate the SST precursors, a lead-lag correlation analysis was performed. For the TC variations over the SEIO, an SST pattern that resembled the Pacific Meridional Mode (PMM) was statistically significant at a two-season lead. However, such a TC-ENSO relationship is seasonally dependent, with different patterns during DJF and MAM. These results suggest that the Matsuno-Gill response to ENSO is an important factor in TC activity but that this influence is seasonally modulated over the SH.
OS06-A013
Preliminary Indices for Physical-biogeochemical Variability of Seychelles-Chagos Thermocline Ridge in the Tropical Indian Ocean
Hyoun-Woo KANG1#+, Ok Hee SEO1, Dong-Jin KANG2
1Korea Institute of Ocean Science and Technology, 2Korea Institute of Ocean Science & Technology
Characteristics of SCTR variability is well represented by the depth of 20oC (D20), where the open-ocean upwelling intensity is higher as the D20 is shallower. Since the thermocline depth variability is also well depicted by sea level anomaly in general, satellite derived sea level anomaly shows a very good correlation with D20 variability in seasonal to interannual timescales. On top of these physical indices, several biogeochemical indicators are proposed for the better understanding and seasonal prediction of biogeochemical variability of SCTR using physical-biogeochemical coupled ocean system model (KOSM). To validate KOSM performance, model derived D20 and sea surface height anomaly compared with observations or reanalysis data. It is encouraging that the seasonal cycle as well as interannual variability of SCTR intensity are comparatively well reproduced by the ocean system model. The subsurface chlorophyll-a maximum depth, a certain N:P ratio associated with nutricline depth and Alkalinity:DIC ratio are also highly interconnected with SCTR variability. The interannual variability of these SCTR indices is also discussed in connection with IOD and ENSO variability.
OS06-A006
Abrupt Dissolved Inorganic Carbon Anomaly in 2016 in Indian Ocean Using GFDL-MOM6-COBALT2 Simulation
Lin ZHANG#+, Enhui LIAO
Shanghai Jiao Tong University
Ocean carbon sink plays a crucial role in mitigating the anthropogenic carbon increase. Comprehending the driving mechanisms of ocean carbon sink variability is vital for grasping the ocean’s capacity to absorb carbon, particularly in light of escalating anthropogenic carbon emission. We found an abrupt carbon content increase in the Indian Ocean basin in 2016 based on a Dissolved Inorganic Carbon (DIC) reconstruction data product and an ocean-driven model simulation (GFDL-MOM6-COBALT2). This finding reveals a considerable interannual variability of the ocean basin’s carbon inventory, which might significantly affect the ocean’s carbon absorption ability. The carbon budget equation indicates the abrupt increase of ocean carbon is largely driven by the horizontal advection term which might be influenced by an anomalous circulation between the Indian Ocean and Pacific and Southern Oceans. Further analysis and discussion will elucidate the origins of this sudden increase in carbon content. Studying carbon fluctuations in the Indian Ocean is expected to enhance our understanding of ocean carbon sink variability.
OS06-A018
Understanding Biogeochemical Process Using Optically Measured High Frequency Nitrate Profiles in the Western Indian Ocean
Tae-Keun RHO#+, Dong-Jin KANG, Suyun NOH, Young Baek SON, Joonseong PARK
Korea Institute of Ocean Science & Technology
High frequency in situ observation of nitrate concentration is crucial to understand the episodic and transient events that lead to important temporal and spatial variations in nitrate concentration. In this study, we conducted vertically high frequency nitrate concentration using ISUS sensor connected to SBE 19 plus CTD with PAR, chlorophyll, and DO sensors. Vertically high-frequency nitrate concentration clearly showed depletion of nitrate within the surface mixed layer and sharp changes as the rapid increase or decrease of dissolved oxygen concentration, suggesting decomposition of organic material produced in the surface layer may be attributed to the vertical distribution of nitrate concentration within water column. However, the ratio was slightly different with depth at different station, which suggests that other processes such as physical mixing of different water mass also control the vertical nitrate distribution.
Session Chair(s): Zhenya SONG, Ministry of Natural Resources
OS21-A002
| Invited
Significant Impact of Ocean Current Variability on Marine Heatwaves Around Japan
Toru MIYAMA#+, Yasumasa MIYAZAWA, Hakase HAYASHIDA
Japan Agency for Marine-Earth Science and Technology
Marine heatwaves have been increasing in intensity and frequency around Japan in recent years, similar to other regions of the world. The Western Boundary Current System of the North Pacific, including the Kuroshio, Oyashio, and Tsushima Warm Currents, plays a significant role in the occurrence of marine heatwaves in this area. To gain a comprehensive understanding of ocean heatwaves in this region, we developed a dataset of marine heatwaves and cold spells around Japan using the JCOPE2M ocean reanalysis system, which was created by the Application Laboratory of the Japan Agency for Marine-Earth Science and Technology. Our dataset showed a substantial increase in the frequency and intensity of marine heatwaves, both at the surface and in the subsurface layer, particularly since 2015. The thermocline depth is affected by ocean currents, and marine heatwaves at the surface are significantly influenced by El Niño and tend to intensify towards the end of an El Niño event. Marine heatwaves have been on the rise in the Oyashio region since 2010, attributed to the warm-water eddy emanating from the Kuroshio Extension. Along the southern coast of Japan, marine heatwaves surged because of the Kuroshio large meander that began in 2017. Offshore, the Kuroshio meander has caused intense marine cold spells. Currently, an unprecedented marine heatwave, caused by the extreme northward shift of the Kuroshio Extension since 2022, is occurring. The Sea of Japan has experienced a warming trend in recent years, and the increase in the Tsushima Warm Current has significantly contributed to this warming. In addition to analyzing past marine heatwave variability, we are developing ensemble predictions of ocean heatwaves using the JCOPE2M ocean prediction system.
OS21-A001
| Invited
What Caused the 2022 Long-lasting Marine Heatwaves in the East China Sea?
Hyoeun OH1#+, Go-Un KIM2, Jung-Eun CHU3, Jin-Young JEONG2
1IBS Center for Climate Physcis, 2Korea Institute of Ocean Science & Technology, 3City University of Hong Kong
In 2022, the East China Sea experienced a record-breaking, long-lasting marine heatwave (MHW) that lasted for 62 days during the boreal summer, exceeding the average MHW duration in the East China Sea of 10 days by a factor of 6. Simultaneously, this year had numerous extreme events across Asia, including summer floods in China and Pakistan. This raises the question of whether these extremes are linked. In this study, we elucidate the key local and remote processes that led to the prolonged MHWs in the East China Sea in 2022. A diagnostic analysis using the mixed-layer heat budget equation was conducted to identify the drivers of changes in the frequency, duration, and intensity of the MHW. Our findings show that the combined effect of the ocean and atmosphere initiated the MHW through weakening of the vertical mixing in the ocean due to the large river discharge from the Yangtze River flood in China and intensified solar radiation, respectively. In addition, in the middle of the MHW period, an anomalous anticyclonic circulation, enhanced by the stationary Rossby wave, settled in the corresponding region and played a crucial role in prolonging the MHW until the arrival of Typhoon Hinnamnor in early September, which contributed to the dissipation of the event. This study provides valuable insights into the physical mechanisms of flood-related MHWs, which may have been increased by recent climate change.
OS21-A006
Wintertime Marine Extreme Temperature Events Modulate Phytoplankton Blooms in the North Pacific Through Subtropical Mode Water
Yong-Jin TAK1+, Hajoon SONG2#, Jong-Yeon PARK3
1Gangneung-Wonju National University, 2Yonsei University, 3Jeonbuk National University
Marine extreme temperature events (METs), including marine heatwaves (MHWs) and cold spells, have recently gained much attention owing to their vital influence on the marine ecosystem and social economy. Since METs can alter the upper ocean stratification and wintertime convective mixing in the northwestern North Pacific subtropical gyre (NPSG), their activities may modulate phytoplankton blooms by regulating entrainment of the subtropical mode water (STMW) with high NO3−. Furthermore, because STMW formed in the previous winter reemerges east of its formation site in the following winter, the METs activities imprinted in STMW affect phytoplankton blooms remote from its formation site. Here, we examined the relationship between the MET activities, STMW volume, and phytoplankton blooms using satellite observations and a data-assimilative coupled physical-biogeochemical model dataset. MET activities appearing in the STMW formation region during winter regulate the formation of STMW and the supply of NO3− from the subsurface, with the latter controlling the spring/autumn blooms in that region under NO3−-limited conditions. Subsequently, this water mass is transported eastward in the subsurface within the northern flank of the NPSG before reemerging east of the STMW formation site the following spring. This process results in a negative lag-correlation between MET activities and surface chlorophyll in the reemergence region; for example, MHWs in winter at the STMW formation site tend to lower the surface chlorophyll concentration one year later in the reemergence region. Our study suggests that the oceanic processes allow one year of predictability of the marine ecosystems by monitoring METs in the STMW formation site.
OS21-A012
Assessing the Impact of Climate Change on Sustainable Small-scale Fisheries in Coastal Regions of India and Taiwan
Louis George KOROWI1#+, Biraj Kanti MONDAL2, Mubarak MAMMEL1, Ming-Ann LEE1
1National Taiwan Ocean University, 2Netaji Subhas Open University
Climate change poses unprecedented challenges to coastal ecosystems, affecting the livelihoods of community’s dependent on small-scale fisheries. This study conducts a comprehensive assessment of the climate change impact on small-scale fisheries in the coastal areas of India and Taiwan. It also aims to develop standard operating procedures for an integrated social-ecological system (SES) for resilient management of the study areas to understand the complex interplay of environmental changes and their ramifications on local fisheries. Collected environmental and socio-economic data in two countries for analyzing the current situation of climate change in the study areas and identifying the long-term seasonal variations. Moreover, it is necessary to assess the relative vulnerability and mitigation or adaption strategies in physical, socio-economic perspectives by using the analytical hierarchy process (AHP). The research reveals discernible shifts in sea surface temperatures, ocean currents, and precipitation patterns, indicating the influence of climate change on the coastal environment. These alterations are explored in conjunction with documented changes in fishery productivity, species composition, and distribution. Through interviews with local fishers and community surveys, we delve into the socio-economic dimensions, assessing vulnerability, adaptation strategies, and resilience of coastal communities facing these climate-induced changes. Comparative analyses between the two regions highlight both commonalities and unique challenges. Indian coastal communities grapple with the intensification of monsoons and sea level rise, while Taiwanese fisheries face the impact of typhoons and warming waters. Despite differences, a shared concern emerges for the sustainability of small-scale fisheries in the face of climatic uncertainties. Our findings contribute to a nuanced understanding of the intricate relationships between climate change and small-scale fisheries, providing valuable insights for policy-makers, resource managers, and local communities. The study emphasizes the need for adaptive management strategies, community-based initiatives, and international collaboration to foster resilience and sustainability in the face of ongoing climate change impacts.
Session Chair(s): Yu-Lin TSAI, National Yang Ming Chiao Tung University
OS11-A011
Effects of Ocean Wave on the Coupled Atmosphere-ocean System for Tropical Cyclones
Nobuhito MORI1#+, Kouji GOTOU2, Keita MATSUMOTO2, Akihiro MUSA2, Koki IIDA1, Junichi NINOMIYA3, Tomoya SHIMURA1
1Kyoto University, 2NEC Corporation, 3Kanazawa University
Prediction and evaluation of typhoon intensity significantly impact the assessment of wind and flood damage, especially storm surge. This study used the coupled atmosphere-ocean-wave coupled model, COAWST model, to evaluate the impact of waves and oceans on typhoons. WRF was used for the atmosphere model, ROMS for the ocean model, and SWAN and WW3 for the wave model, and their effects on typhoon intensity were examined. Furthermore, the effects of grid resolution, waves, and oceans on typhoon intensity were evaluated using the Earth Simulator ES4, optimized on the vector supercomputer, and reproduced for Typhoon Haiyan in 2014 and Typhoon Jebi in 2018 with a minimum horizontal resolution of 2 km. It is found that higher resolution overestimates typhoon intensity, but ocean and wave coupling suppress development and are consistent with observations.
OS11-A045
Large-scale Climate Variability Behind the Wave Energy Extremes in the Yellow Sea During an Unusual Season
Dong Eun LEE1#+, Hye-Ji KIM1, Jeseon YOO2, Haedo BAEK1
1Chungnam National University, 2Korea Institute of Ocean Science & Technology
The Yellow Sea (YS) is exposed to various weather systems, which can pose a major threat to the adjacent coastal regions through the development of powerful oceanic surface waves. Unusually severe surface wave events in the YS occur with considerable frequency during the boreal spring (March-April-May), but have received less attention compared to winter and summer. This study focuses on the characteristics of spring extreme wave events in the YS, based on observational and long-term reanalysis datasets. Our analysis shows that the extreme waves, defined as waves with a daily maximum height in the upper 5% of all springs, start to build up about 12 hours before the peak waves and continue for a longer period after the peak have been reached. In the range of 6~24 hours following the peaks of the extreme wave events in the YS, swells propagating from the far western North Pacific arrive in the YS. These swells from the western North Pacific, possibly generated by the same mesoscale system that has caused the extreme wave heights in the YS a few days in advance and has travelled northeastward, contribute to maintaining higher wave energy levels in the YS for longer after the atmospheric source has been removed. The large-scale environmental conditions can provide the predictability of extreme waves in the basin developed by these findings. Our analysis further reveals that more intense events tend to occur with eastward shift of the Siberian High, while the events occur more frequently with El Niños. This study presents implications for assessing the risks associated with extreme waves in coastal regions and improving coastal management strategies in the YS.
OS11-A005
Improving the Accuracy of Data-driven Model for Predicting Wave Heights at an Offshore Construction Site
Kobayashi RYOTA1#+, Sooyoul KIM1, Watanabe KEN2, Mase HAJIME3
1Kumamoto University, 2Hydro Technology Institute Co., Ltd., 3Kyoto University
Judging the feasibility of offshore construction is complicated because it requires consideration of wave and weather conditions. However, the decision-making on whether or not construction is possible should be made early in the morning on site. Thus, to plan construction progress, accurate wave forecasts are critical. The reliability of wave prediction is still insufficient because 1.0 m in significant wave height is called the threshold for decision-making for offshore construction work in Japan. This study challenges to improve the accuracy of 24 hours ahead-forecasted significant wave heights below 2 m using a hybrid model of LSTM and ANN. Therefore, we conducted a series of experiments to develop an ANN-based model using the two ensemble training methods: 1) the inverse function method, and 2) the restoration extraction method. ANN models have a hidden layer with three layers and units ranging from 10 to 90 in 20 increments for training and testing. Each configuration with the unit and intermediate layer has 20 models for selecting the best performance model. The experimental results showed that both ANNs trained by the ensemble methods improved the prediction accuracy obtained from the LSTM wave prediction model: the averages of the correlation coefficient (CC), the root mean square error (RMSE), and the averaged normalized mean square error (NRMSE) by the inverse function method are 0.95, 0.15 m, and 5.5 %, while those by the restoration extraction method are 0.91, 0.21 m, and 7.6 %. The prediction accuracy was also improved compared to CC: 0.9, RMSE: 0.22 m, NRMSE: 7.9 % using the regular ANN and CC: 0.82, RMSE: 0.33 m, and NRMSE: 11.8 % by LSTM. These results show that ensemble ANN using the restoration-extraction method and the ANN using the inverse function method can be advantageous when small data are available.
OS11-A012
Historical and Future Climate Change Impact on Tropical Cyclone Characteristics
Yuting YAO#+, Tomoya SHIMURA, Takuya MIYASHITA, Nobuhito MORI
Kyoto University
Typhoon intensity, movement speed, and course significantly impact coastal hazards such as storm surges and storm waves. Furthermore, the impact of climate change on these typhoon characteristics is important for long-term coastal hazard assessment and planning. In this study, we evaluate the effects of global warming on typhoon intensity, movement speed, and courses for typhoons resulting from the non-warming experiment (Non-GW), the present climate experiment, and the future climate experiment (+4K) of the Large Climate Ensemble Projections d4PDF (Mizuta et al., 2017). The results show an increase in typhoon intensity, a decrease in the number of typhoons, and an eastward expansion of their paths.
OS11-A010
A Major Improvement of Atmospheric Wave Boundary Layer Model for Storm Surge Modeling by Including Effect of Wave Breaking on Air-sea Momentum Exchange
Anyifang ZHANG1+, Xiping YU2#
1Tsinghua University, 2Southern University of Science and Technology
Accurate estimation of the wind stress under extreme conditions is crucial for modeling storm surges and storm waves, which is important to the development of a warning system for coastal disaster prevention. The problem, however, is highly challenging owing to the presence of complex ocean surface processes under the action of unusually strong wind. Empirical formulas have been widely applied to estimate wind stress in storm surge mode although they fail to include the effect of sea surface conditions. In this study, the existing atmospheric wave boundary layer model is significantly enhanced by fully including various effects of wave breaking. Both the effect of wave breaking on the dissipation of energy and its effect on the transfer of momentum within the atmospheric boundary layer are carefully formulated. The wind stress coefficients obtained with the enhanced model are shown to be in good agreement with the measurements in not only deep but also shallow waters. The enhanced atmospheric wave boundary layer model is coupled with ocean wave as well as circulation models to simulate typhoon-induced storm surges and storm waves in the Pearl River Delta region. The computational results show that the coupled model with improved evaluation of the wind stress is substantially advantageous when compared with existing approaches.
OS11-A022
| Invited
Seasonal Advance of Intense Tropical Cyclones in a Warming Climate
Kaiyue SHAN1#+, Xiping YU2,1, Fengfei SONG3, Yanluan LIN1, Pao-Shin CHU4
1Tsinghua University, 2Southern University of Science and Technology, 3Ocean University of China, 4University of Hawaii
Intense tropical cyclones (TCs), which often peak in autumn, have destructive impacts on life and property, making it crucial to determine whether any changes in intense TCs are likely to occur. Here, we identify a significant seasonal advance of intense TCs since the 1980s in most tropical oceans, with earlier-shifting rates of 3.7 and 3.2 days per decade for the Northern and Southern Hemispheres, respectively. This seasonal advance of intense TCs is closely related to the seasonal advance of rapid intensification events, favoured by the observed earlier onset of favourable oceanic conditions. Using simulations from multiple global climate models, large ensembles and individual forcing experiments, the earlier onset of favourable oceanic conditions is detectable and primarily driven by greenhouse gas forcing. The seasonal advance of intense TCs will increase the likelihood of intersecting with other extreme rainfall events, which usually peak in summer, thereby leading to disproportionate impacts.
Session Chair(s): Robin ROBERTSON, Xiamen University Malaysia
OS02-A001
The Vertical Structure of Internal Lee Wave-driven Benthic Mixing Hotspots
Ying HE1#+, Toshiyuki HIBIYA2
1China Meteorological Administration, 2The University of Tokyo
In global ocean circulation and climate models, bottom-enhanced turbulent mixing is often parameterized such that the vertical decay scale of the energy dissipation rate ζ is universally constant at 500 m. In this study, using a non-hydrostatic two-dimensional numerical model in the horizontal-vertical plane that incorporates a monochromatic sinusoidal seafloor topography and the Garrett-Munk (GM) background internal wave field, we find that ζ of the internal lee wave-driven bottom-enhanced mixing is actually variable depending on the magnitude of the steady flow U0, the horizontal wavenumber kH and the height hT of the seafloor topography. When the steepness parameter (Sp=NhT/U0 where N is the buoyancy frequency near the seafloor) is less than 0.3, internal lee waves propagate upward from the seafloor while interacting with the GM internal wave field to create a turbulent mixing region with ζ that extends further upward from the seafloor as U0 increases, but is nearly independent of kH. In contrast, when Sp exceeds 0.3, inertial oscillation (IO) not far above the seafloor is enhanced by the intermittent supply of internal lee wave energy Doppler-shifted to the near-inertial frequency, which occurs depending on the sign and magnitude of the background IO shear. The composite flow, consisting of the superposition of U0 and the IOs, interacts with the seafloor topography to efficiently generate internal lee waves during the period centered on the time of the composite flow maximum, but their upward propagation is inhibited by the increased IO shear, creating a turbulent mixing region of small ζ.
OS02-A007
Generation of Superinertial Internal Tides Propagating Along the Coast: The Role of Topographic Modes in the Formation of Topographically Modified Internal Kelvin Waves
Yuki TANAKA#+
Tokyo University of Marine Science and Technology
Internal tides are an important energy source for diapycnal mixing in the ocean interior. It is known that the subinertial internal tides have a baroclinic vertical structure in deep areas but a more barotropic structure in shallower areas, making the conventional barotropic–baroclinic decomposition ineffective to separate internal tides from surface tides. To address this issue, Tanaka (2023) introduced a "topographic mode" which represents internal motions with a barotropic vertical structure, and proposed a new energy diagram enabling us to quantify the generation of subinertial internal tides. In this study, the applicability of this new energy diagram to superinertial internal tides is investigated by idealized numerical experiments incorporating a continental slope with a bump in the coastline at various inertial frequencies. The calculated results show that both the topographic and baroclinic modes are generated over the bump and propagate downstream along the coast, coupling to form a topographically modified internal Kelvin wave whose cross-sectional structure closely resembles that obtained by solving a two-dimensional eigenvalue problem for a superinertial frequency. The energy conversion rate from the surface to the topographic mode is about half of the energy conversion rate from the surface to the baroclinic mode when the tidal frequency is slightly superinertial, and maintains a non-negligible contribution even when the tidal frequency is substantially superinertial. The findings of this study indicate that the new energy diagram can be applied seamlessly across the critical latitudes and possibly provides a global distribution of the internal tide generation significantly larger than the previous estimates.
OS02-A003
Tidally-driven Turbulence in the Wake of Sharp Relief
Craig STEVENS1,2#+, Alain DE VERNEIL1, Cynthia BLUTEAU3, Pete RUSSELL4, Graham RICKARD1, Ata SUANDA5, Jasmin MCINERNEY1, Alice OVEREND1, Eleanor HAIGH1
1National Institute of Water and Atmospheric Research, 2University of Auckland, 3Fisheries and Oceans Canada, 4University of Otago, 5University of North Carolina Wilmington
Here we use observations and modelling to examine the tidally-forced wake region of a “mini-seamount”. We use a unique natural laboratory where a mini-seamount, combined with strong tides, generates a highly turbulent wake region. Project Turbulence EDDY BAthymetRy Experiments (TEddy-BarE) sampling focuses on the eddies created by the mini-seamount of Fishermans Rock in central Cook Strait (Aotearoa New Zealand). The seamount is in 300 m of water and its summit comes within 10 m of the ocean surface so it is effectively a steep-sided island but with no impact on the wind field. A strong tidal flow, coupled with the well-defined obstacle, spawns near-perfect eddies every six hours. While the tide partially returns eddies to the seamount, the residual flow is sufficient that the eddies will move away from their generation point. We combined ship-based sampling, drifting instrument packages and ocean glider mounted microstructure. We are able to connect the horizontal shear with the three-dimensional turbulence as the ship-based ADCP was able to provide highly resolved measurement of horizontal shear in wake zone and provide a useful comparison with numerical simulations. In high energy conditions the Lagrangian moorings were able to resolve dissipation rate from a wavenumber ADCP based approach. These provided a useful comparison with the very high turbulence levels in the rock wake although it was very difficult to remain on pre-determined station.
OS02-A002
Double Diffusion and Shear-driven Mixing in the Northwestern Sea of Japan
Dmitrii STEPANOV1#+, Alexander OSTROVSKII2
1V.I. Il'ichev Pacific Oceanological Institute, 2Shirshov Institute of Oceanology
Using fine structure measurements we analysis two processes (double diffusion and shear instability) responsible for vertical mixing in the zone of the westerly Primorye Current in the northwestern Sea of Japan. The Turner angle for the verification of double diffusion processes is estimated. The contributions of thermal convection and salt fingers to the buoyancy flux are studied. It is established that, due to differential diffusion, the layer from 80 to 170 m was involved in intense vertical mixing. In addition, we estimate the shear-driven vertical mixing below the mixed layer. Using the Thorpe sorting, the spatial scales of the turbulent areas are found as well as the turbulent dissipation rate and diapycnal diffusivity. Additionally, the vertical turbulent heat and salt fluxes are estimated. We show that enhanced vertical mixing is present below the mixed layer despite strong density stratification. In addition, the uplifted upward vertical heat flux and downward salt fluxes were observed. We compose a background diapycnal diffusivity profile over the continental slope in the northwestern Sea of Japan by associating the features of vertical mixing obtained by the Thorpe-scale method and finescale parameterization framework. This study was supported by the Russian Science Foundation N 23-27-00333 (https://rscf.ru/en/project/23-27-00333/).
OS02-A008
The Role of Surface and Bottom Forcings on the Genesis of Langmuir Supercells in the Coastal Ocean
Jiahao HUANG1+, Marcelo CHAMECKI2, Qing LI3, Bicheng CHEN1#
1Xiamen University, 2University of California, Los Angeles, 3The Hong Kong University of Science and Technology
In shallow-water coastal oceans, different types of turbulence originating from the surface boundary layer (SBL) and bottom boundary layer (BBL) may develop across the mid-layer of the water column and interact with each other. Langmuir turbulence (LT) is a crucial turbulent mixing process in the ocean SBL formed by the wave-current interaction. When LT extends to the BBL, a strong coherent structure called Langmuir Supercell (LSC) forms and occupies the whole water column. LSCs are crucial in modifying air-sea exchange, sediment resuspension, and mass transport in coastal oceans. Previous research suggests that the strength of LSCs may depend on the alignment of wind, wave, and background current. However, the mechanisms of their generation and attenuation are still unclear. To investigate this problem, we conduct numerical experiments for different idealized environments with coupled SBL-BBL using Large Eddy Simulations (LESs). Our results show that the wind/wave-current alignment strongly modulates the flow pattern. Strong coherent structures in the flow field are energized by the production term at the corresponding scale when the wind/wave and background current are aligned. When the wind/wave and current are oriented in opposite directions, the pattern of LSCs is completely eliminated; moreover, the turbulence within the different boundary layers is much weaker than that in a single boundary layer.
OS02-A012
High-frequency Internal Waves, High-mode Nonlinear Waves and K-H Billows on the South China Sea's Shelf Revealed by Marine Seismic Observation
Linghan MENG+, Haibin SONG#, Shun YANG, Kun ZHANG, Mengli LIU
Tongji University
From July to September 2009, a set of multi-channel seismic data was collected in the northern shelf area of the South China Sea. After the data was processed, we observed a series of shoaling events on one of the survey lines, including high-frequency internal waves, high-mode nonlinear internal waves, and shear instability. Using theoretical results from previous numerical simulations and field observations, coupled with local temperature and salinity data, we analyzed their depth distribution, waveform characteristics, and formation mechanisms, and discussed the influence of seafloor topography and stratification on the shoaling of solitary internal waves. We estimated the mixing parameters of seawater using a parameterization scheme based on hydrographic data and seismic data and found that the diapycnal mixing caused by these shoaling events in the shelf area were about 3.5 times greater than those on the slope. Consequently, the fission of internal solitary waves and the induced shear instability serve as significant mechanisms for the energy dissipation of internal solitary waves at the slope and shelf of the South China Sea. Additionally, the high-frequency internal waves generated during shoaling might also have a crucial role in this process.
Session Chair(s): Feba FRANCIS, Université Catholique de Louvain, Charan Teja TEJAVATH, National Center for Earth Science Studies
OS05-A001
| Invited
Uneven SST Warming Over the Indian Ocean and Its Impacts
Kyung-Ja HA1#+, Sahil SHARMA2,1, Ryohei YAMAGUCHI 3, Eui-Seok CHUNG1
1Pusan National University, 2IBS Center for Climate Physics, 3Japan Agency for Marine-Earth Science and Technology
The Indian Ocean sea surface temperature (SST) variability has influenced the mean climate and the variability of the global monsoons and climate. The previous studies had investigated the Indian Ocean basin-wide (IOBW) and dipole (IOD) modes, which may be related to the mean state and El Niño and Southern Oscillation (ENSO) relationship under anthropogenic global warming. Studies showed that the warming over the northern IO is associated with the significant warming in the equatorial eastern Pacific, the strengthened ENSO–EASM relationship has likely also contributed to the strengthened relationship between the northern IO and the EASM. In the present talk, a recent work on different SST warming over the Indian Ocean and its impacts will be emphasized. Most future projections conducted with coupled general circulation models simulate a non-uniform Indian Ocean warming, with warming hotspots occurring in the Arabian Sea (AS) and the southeastern Indian Ocean (SEIO). The study aimed to investigate the underlying physical drivers. For this, we employed ocean heat budget analysis using a suite of large ensemble simulations of the Community Earth System Model 2 to elucidate the causes of non-uniform Indian Ocean warming. The results demonstrated that enhanced future warming in the Arabian Sea will further reduce atmospheric surface pressure and generate more rainfall, also in the adjacent regions. In results, climate models show on average a 50% intensification of mean rainfall over the southern Arabian Peninsula and parts of western India by year 2100, if CO2 emissions are not cut drastically.
OS05-A010
| Invited
Role of Indian Ocean Precipitation Anomalies in Early Winter ENSO and IOD Teleconnection to the South Asian and North Atlantic Regions
Fred KUCHARSKI#+, Muhammad Adnan ABID, Alessandro RAGANATO, Franco MOLTENI
International Centre for Theoretical Physics
Interbasin teleconnections have become a hot topic in climate research because of their potential impacts on climate change patterns and seasonal forecasts. ENSO shows global teleconnections, also in the Indian and Atlantic Ocean and ENSO properties can be modified by teleconnections from the Indian and Atlantic Oceans. In this presentation, we will discuss how the ENSO teleconnection to the Indian Ocean can modify ENSO's further influences on climate in several regions, particularly the South Asian and North Atlantic regions. It is demonstrated that ENSO is associated with a strong rainfall/heating dipole in the Indian Ocean in early winter. This heating dipole shows substantial predictability and is partially forced by a direct ENSO teleconnection, and partially induced by a delayed impact from the Indian Ocean Dipole (IOD; which itself may be induced by ENSO in boreal autumn). This Indian Ocean rainfall/heating dipole also turns out to be the first EOF of winter rainfall and is crucial for mediating ENSO teleconnections to the South Asian winter monsoon and the North Atlantic regions. It is also demonstrated that the heating dipole induces substantial predictability in both regions (rainfall for South Asia and temperature in Europe). Finally, we investigate how the IOD independently of ENSO may influence North Atlantic climate and how this is represented in the SEAS5 seasonal forecasting system.
OS05-A003
The Changes of Precipitation Extremes in Peninsular Malaysia During Indian Ocean Dipole (IOD) and El Niño-Southern Oscillation (ENSO)
Muhammad Amirul Hakimi BIN ABDUL HALIM#+, Liew JUNENG, Abdul Azim AMIRUDIN, Afiqah Bahirah AYOUB, Muhamad Zuhairi MAT ZIN
Universiti Kebangsaan Malaysia
This study examines the individual and combined impacts of the positive Indian Ocean Dipole (IOD) and El Niño towards the changes of precipitation extremes in Peninsular Malaysia. This study used precipitation data from Climate Hazards centre InfraRed Precipitation with Stations (CHIRPS) of 5KM resolution. The extreme precipitation indices used in this study are from the Expert Team on Climate Change Detection and Indices (ETCCDI). The results show the impacts of the co-occurrence of IOD and El Niño events towards the precipitation extremes in Peninsular Malaysia are more amplified and significant compared to the individual impacts of the IOD and El Niño. During June-July-August (JJA), the impacts of IOD and El Niño individual events are less significant and almost similar but started showing differences during September-October-November (SON) in terms of rainfall anomalies. The rainfall anomaly showed slight increase in the eastern and western region during SON and during December-January-February (DJF) in the southern and eastern region during IOD positive but decreasing in the eastern region during El Niño. The co-occurrence of both events triggered significant decrease for rainfall anomaly over the eastern, northern, and southern region of Peninsular Malaysia during SON. The frequency of rainy days is significantly decreased during SON and subsequent March-April-May (MAM) throughout Peninsular Malaysia except in the northern region during SON. The consecutive dry days (CDD) showed significant anomalous increment throughout Peninsular Malaysia especially in the eastern, northern, and southern region during DJF during individual El Niño and the co-occurrence of IOD and El Niño. The same occurred to simple daily intensity index (SDII) where the intensity of rainfall is reduced significantly during the co-occurrence of IOD and El Niño during DJF especially in the eastern Peninsular Malaysia. Overall, the rainfall characteristics and anomalies showed remarkable spatio-temporal variations, modulated by IOD and ENSO, either combined or separately.
OS05-A008
Improving the Simulation of the South Asian Summer Monsoon Precipitation by Incorporating Sea Spray Effects Into a Climate Model
Yajuan SONG#+
Ministry of Natural Resources,First Institute of Oceanography
Sea spray plays an important role in heat and water exchange at the air-sea interface. A parameterization of the sea spray-induced latent and sensible heat fluxes was incorporated into a climate model, med the First Institute of Oceanography-Earth System Model version 2.0 (FIO-ESM v2.0). Our findings indicate that considering the effects of sea spray improve the simulated bias of summer monsoon precipitation over the South Asian monsoon region in the climate model. Sea spray contributes to enhanced ocean evaporation and heat transport firstly, leading to surface cooling in the northern Pacific and Indian Ocean. An anticyclone anomaly is intensified over the South China Sea, driven by anomalous easterly winds in the south and westerly winds in the north South Asian region. Changes in wind patterns and air humidity result in decreased water vapor transport in the south and increased transport in the north, leading to water vapor convergence over the Ghats mountains of western India and the northern India region, and divergence over the southeast side of the Tibet Plateau. As a result, precipitation increases over western India and northern India, while decreasing over the southeast side of the Plateau. Our study suggests that consideration of sea spray effects is a feasible way to mitigate the common biases of simulated summer monsoon precipitation in the climate models.
OS05-A009
Climate Precursors of Satellite Water Marker Index for Spring Cholera Outbreak in Northern Bay of Bengal Coastal Regions
Tomomichi OGATA1#+, Masami NONAKA1, Swadhin BEHERA1, Marie-Fanny RACAULT2
1Japan Agency for Marine-Earth Science and Technology, 2University of East Anglia
Cholera is a water-borne infectious disease that affects 1.3 to 4 million people, with 21,000 to 143,000 reported fatalities each year worldwide. Outbreaks are devastating to affected communities and their prospects for development. The key to support preparedness and public health response is the ability to forecast cholera outbreaks with sufficient lead time. How Vibrio cholerae survives in the environment outside a human host is an important route of disease transmission. Thus, identifying the environmental and climate drivers of these pathogens is highly desirable. Here, we elucidate for the first time a mechanistic link between climate variability and cholera (Satellite Water Marker; SWM) index in the Bengal Delta, which allows us to predict cholera outbreaks up to two seasons earlier. High values of the SWM index in fall were associated with above-normal summer monsoon rainfalls over northern India. In turn, these correlated with the La Niña climate pattern that was traced back to the summer monsoon and previous spring seasons. We present a new multi-linear regression model that can explain 50% of the SWM variability over the Bengal Delta based on the relationship with climatic indices of the El Niño Southern Oscillation, Indian Ocean Dipole, and summer monsoon rainfall during the decades 1997–2016. Interestingly, we further found that these relationships were non-stationary over the multi-decadal period 1948–2018. These results bear novel implications for developing outbreak-risk forecasts, demonstrating a crucial need to account for multi-decadal variations in climate interactions and underscoring to better understand how the south Asian summer monsoon responds to climate variability. If possible, we would like to mention about extended prediction using seasonal forecast system.
OS05-A013
Tackling Systematic Errors Over the Indian Ocean in Met Office and Partners Coupled Models
Charline MARZIN#+
Met Office
A working group was formed between the Met Office, The Bureau of Meteorology, ECMWF and other forecasting centres within the UM Partnership to understand and improve common systematic errors in the Indo-Pacific region and associated teleconnections. In particular, the significant cold SST biases in the Eastern Indian Ocean have a significant impact on the prediction skill of the seasonal forecasting systems for tropical rainfall, Australasian monsoon system and the representation of associated key teleconnections in climate models. The multi-disciplinary group aims to consolidate current diagnoses of model errors and how they evolve and develop a new set of diagnostics and metrics using a seamless modelling framework. This will help measure the impact of future improvements, as well as recommend potential model/DA developments and observation campaigns to mitigate these errors. The current strands of activities explore different hypotheses for the sources of errors in the region: the role of different initial conditions and coupled data assimilation, the bathymetry and potential role of the Indonesian throughflow, the sensitivity to various physics changes in the atmosphere and ocean models and the evolution of key biases and the air-sea interaction processes involved at different timescales using coupled NWP, sub-seasonal to climate modelling frameworks. Key results from the initial investigations coordinated across several modelling centres will be presented.
Session Chair(s): Kang XU, Chinese Academy of Sciences, Jian SHI, Ocean University of China
OS10-A016
| Invited
Multi-year North Pacific Marine Heatwave Dynamics: Roles of Atmospheric Wave Trains and Inter-basin Interactions
Jin-Yi YU#+, Yu ZHAO
University of California, Irvine
Consecutive marine heatwave (MHW) events unfolded over the past decade in the North Pacific, spanning extensive oceanic areas and exerting substantial impacts on regional ecosystems and human economic activities. While sharing similar intensities, basin-wide structures, and multi-year durations, the 2019-2022 event distinguishes itself from the preceding 2013-16 event in terms of heating center locations, associated atmospheric circulation patterns, and North Pacific-North Atlantic interactions. Through observational and modeling analyses, this study unravels the structures, evolutions of these two Pacific MHW events, and the driving mechanisms behind them. Emphasizing the indispensable roles of atmospheric wave trains and Pacific-Atlantic interactions, our research sheds light on their pivotal contributions to the formation and sustained multi-year durations of these North Pacific MHWs.
OS10-A013
Atmosphere Teleconnections from Abatement of China Aerosol Emissions Exacerbate Northeast Pacific Warm Blob Events
Hai WANG1#+, Xiao-Tong ZHENG1, Wenju CAI2,3, Zi-Wen HAN1, Shang-Ping XIE4, Sarah KANG5, Yu-Fan GENG1, Fukai LIU1, Chuan-Yang WANG1, Yue WU1, Baoqiang XIANG6,7, Lei ZHOU8
1Ocean University of China, 2Ocean University of China and Qingdao National Laboratory for Marine Science and Technology, 3Commonwealth Scientific and Industrial Research Organisation, 4University of California San Diego, 5Ulsan National Institute of Science and Technology, 6University Corporation for Atmospheric Research, 7NOAA Geophysical Fluid Dynamics Laboratory, 8Shanghai Jiao Tong University
During 2010-2020, Northeast Pacific (NEP) sea surface temperature (SST) experienced the warmest decade ever recorded, manifested in extreme marine heatwaves, referred to as “warm blob” events. Such events severely affect marine ecosystems and extreme weathers along the west coast of North America but causes of the dramatic NEP SST warming remain elusive. Here, we show that a rapid China aerosol abatement over the period likely made the warm blob events more frequent and intense through atmosphere teleconnections. Anomalous tropospheric warming induced by declining aerosols in China generated the atmospheric teleconnections from East Asia to the NEP, featuring an intensified and southward-shifted Aleutian Low. The associated atmospheric circulation anomaly weakens the climatological westerlies in the NEP and warms the SST there by suppressing the evaporative cooling. Thus, an increase in warm blob events, disproportionally large beyond the radiative effect, is likely as aerosols in China continue to decrease.
OS10-A006
Just Another Tasman Sea Marine Heatwave?
Neil HOLBROOK#+
University of Tasmania
Through late November and early December 2023, a severe category marine heatwave (MHW) was detected moving southwards off the east coast of Tasmania, Australia. The MHW was characterised by offshore sea surface temperature anomalies ~4oC above climatological values embedded within and around large anticyclonic eddies with warm anomalies to >1000m depth. Given the deleterious impacts from previous MHWs on marine ecosystems, fisheries, and aquaculture in the region, serious concerns were raised. To advise and prepare stakeholders, a series of online briefings was given by physical, biogeochemical, fisheries, and social scientists on the current and likely evolving environmental conditions associated with the MHW. So, how unusual was this event? Was it successfully forecast? Was it expected from our knowledge of large-scale modes of climate variability and their teleconnections? This presentation will discuss the characteristics, evolution – both forecast and projected – and emerging impacts of the November-December 2023 Tasman Sea MHW. It will be argued that the characteristics of this event mirror expectations from anthropogenic climate change, and that initialised seasonal SST forecasts were little different from expectations under climate change projections and trend persistence.
OS10-A004
Seasonal Stratification and Complex Local Dynamics Control the Sub-surface Structure of Marine Heatwaves in Eastern Australian Coastal Waters
Amandine SCHAEFFER#+, Alexander SEN GUPTA, Moninya ROUGHAN
UNSW Sydney
Marine heatwaves are extreme seawater temperature events that can have severe impacts on marine life. The extent of the ecological damage depends not only on the easily observed surface signature but on the marine heatwave structure at depth. However, due to a paucity of in situ sub-surface observations the vertical structure of marine heatwaves is poorly understood. Here we analyse the sub-surface coherence and controls of marine heatwaves using one of the world’s longest (28 years) records of daily sub-surface ocean temperature off Sydney, Australia. We show that seasonal stratification, large-scale circulation and local downwelling processes control the vertical coherence of coastal marine heatwaves. We define three classes of marine heatwaves which can extend through the water column, form in the shallow surface layer, or sub-surface independently, and are therefore not always evident in surface data. We conclude that sub-surface data need to be considered in monitoring marine heatwaves in coastal areas where maximum biological damage is reported.
OS10-A008
Intrinsic Short Marine Heatwaves from the Perspective of Sea Surface Temperature and Height
Yuwei HU1+, Xiao Hua WANG2#, Helen BEGGS3
1Chinese Academy of Sciences, 2Sino-Australian Research Centre for Coastal Management (SARCCM), School of Science, UNSW Canberra, 3Bureau of Meteorology
Marine heatwaves (MHWs) have recently been recognized as extreme climate events considering their devastating impacts on marine ecosystems. Identifying and quantifying both common and distinctive characteristics of historical events may contribute to future studies and predictions of regional MHWs. We analyzed the main spatiotemporal features of MHW metrics on a pixel-wise (~5km) scale over the Australian region using the gap-free Climate Change Initiative (CCI) and Copernicus Climate Change Service (C3S) Level 4 (L4) Sea Surface Temperature (SST) analyses from 1981 to 2020. Contributions of short events to MHWs show large regional dependence. Natural internal variability of the local climate system, such as the highly dynamic surface waters of boundary current regions, possibly contributes to most of these short events rather than the remote modulation of climate modes and/or ocean warming. The important role of ocean warming in MHWs is highlighted by the update from the 5-day to 10-day definition over the Great Barrier Reef (GBR) region. Sea Level Anomaly (SLA) metrics are applied to explore the relationship between SST metrics over the northwest and southeast coast of Australia. We found that longer MHWs tend to exhibit distinct patterns of SLA metrics reflecting different combinations of forcing factors. Therefore, SLA over the 90th percentile, as a recommended SLA metric, has the potential to identify MHWs or subsurface events, although limited by application area. Improving the understanding of these metrics is an efficient way to explore the physical characteristics of MHWs globally, which could greatly benefit future prediction and strategy making.
OS10-A018
Equatorial Western Pacific Easterly Wind Extremes Drive Marine Heatwaves Off Western Australia with La Niña as the Preconditioning Symptom
Yuxin WANG1#+, Neil HOLBROOK1, Jules KAJTAR2
1University of Tasmania, 2National Oceanography Centre
Western Australia (WA) marine heatwaves (MHWs) are warm water extremes off the WA coast, like the severe one in 2011, and have been known to cause significant ecological damage. Easterly wind stress anomalies in the western and central equatorial Pacific, termed "easterly wind extremes (EWEs)", play a role in both triggering WA MHWs and La Niña through oceanic wave dynamics. However, the exact role of La Niña in this process remains uncertain: is it only a preconditioning symptom in the chain of WA MHWs set off by EWEs, or it is the actual trigger of WA MHWs. Here, we investigate the relationships between WA MHWs, EWEs and La Niña by constructing a linear first baroclinic-mode reduced gravity model (RGM) and using pycnocline depth as the proxy for detecting WA MHWs and La Niña. Our findings reveal that the wind stress over the tropical western and central Pacific dominate WA pycnocline depth monthly variability compared with wind stress in other areas, accounting for over 60% of the variability. Additionally, by applying a large ensemble of idealized EWE RGM experiments, we found both EWEs and La Niña typically precede WA MHWs by approximately ~4 months (2-6 months) before WA MHWs. Notably, 25% of WA MHWs occur around 4 months after EWEs, without any preceding La Niña. This happens when EWEs are strong enough to trigger WA MHWs but not intense enough to induce a La Niña. Our results highlight that EWEs stand out as a more robust precursor to WA MHWs than La Niña, emphasizing their added value in enhancing the predictability of WA MHWs, especially when La Niña is absent.
OS10-A001
Interactions Between Cold Cyclonic Eddies and a Western Boundary Current Modulate Marine Heatwaves
Junde LI1,2#+, Moninya ROUGHAN2, Michael HEMMING 2
1Hohai University, 2UNSW Sydney
Marine heatwaves are known to cause severe ecosystem damage and therefore have received attention in recent years. However, the focus has tended to be on global (surface) studies, but not coastal waters. Cyclonic eddies are important and underappreciated components in the eddy-dominated western boundary current system, but their impacts on the path of the western boundary currents have largely been unexplored. Here we show that cold cyclonic eddies can modulate the most intense coastal marine heatwaves on record inshore of the East Australian Current. We show that the marine heatwave was driven and modulated by the lateral movement of the western boundary current jet and a cyclonic eddy. This study reveals that the interplay of cyclonic eddies and a western boundary current can drive coastal ocean warming, paving the way for future investigations into eddy interactions and the evolution of coastal marine heatwaves in other western boundary current regions.
OS10-A030
Compound Subsurface Marine Heatwaves in the Northwest Atlantic Coastal Ocean
Ke CHEN#+
Woods Hole Oceanographic Institution
The Northwest Atlantic coastal ocean is experiencing rapid warming along with frequent Marine Heatwaves. In comparison to surface-intensified Marine Heatwaves, subsurface heatwaves have more direct impacts on the marine ecosystem and fisheries but at the same time have been inadequately studied. In this work, observations and high-resolution numerical modeling are used to investigate the spatiotemporal occurrence and mechanisms of bottom-intensified, compound Marine Heatwaves on the southern New England shelf in the Northwest Atlantic coastal ocean. Realistic simulations reveal a hotspot of cross-isobath bottom intensified intrusions of warm and salty offshore water at a topographic trough. Examination of multiple events portraits a robust mechanism of locally enhanced bottom intrusion process leading to compound subsurface heatwaves. Persistent upwelling-favorable winds set up large-scale pressure gradient field, which is enhanced at the topographic trough and drives the large-distance onshore intrusion. Although highly anomalous waters on the shelf are connected with wind forcing, correlations between the wind stress anomaly and bottom salinity anomaly at the location of the enhanced intrusion is modest, implying the need to incorporate other factors to develop more deterministic prediction models for subsurface conditions on the shelf.
OS10-A007
Unraveling the Indian Monsoon's Role in Fueling the Unprecedented 2022 Marine Heatwave in the Western North Pacific
Qianghua SONG1+, Chunzai WANG1#, Yulong YAO2, Hanjie FAN3
1Chinese Academy of Sciences, 2South China Sea Institute of Oceanology, Chinese Academy of Sciences, 3Sun Yat-sen University
An unprecedented marine heatwave (MHW) event occurred in the middle-high latitude of the western North Pacific in the summer of 2022. We demonstrate that enhanced precipitation thousands of kilometers away fueled this extreme MHW event in July 2022. In the upper atmosphere of the MHW region, a persistent atmospheric blocking system is formed, which reduces convection and cloud cover and increases shortwave radiation at the ocean surface, leading to higher sea surface temperatures. Atmospheric perturbations induced by latent heat release from the extreme precipitation in the Indian summer monsoon region enhance this atmospheric blocking through the propagation of quasi-stationary Rossby waves. Our hypothesis is verified by using a numerical model that is forced with the observed atmospheric anomalous diabatic heating. This study sheds light on how a subtropical extreme event can fuel another middle-high latitude extreme event through an atmospheric bridge.
Session Chair(s): Yun-Ta WU, National Cheng Kung University, Huabin SHI, University of Macau
OS11-A056
| Invited
Long Term Analysis of Longshore Sediment Transport on Kulon Progo Coast in Yogyakarta, Indonesia
Mohammad FARID1#, Mohammad Bagus ADITYAWAN2+, Bagus Pramono YAKTI1, Arno Adi KUNTORO1, Widyaningtias WIDYANINGTIAS1, Joko NUGROHO1
1Bandung Institute of Technology, 2Institut Teknologi Bandung
The shoreline, defined as the boundary between land and sea, is one of the most dynamic landforms on Earth due to the constant battle between sediment deposition and erosion forces. Careful analysis of shoreline movement, also known as shoreline dynamics, provides critical insights for safe and sustainable coastal development. This study focuses on elucidating the short and long-term shoreline dynamics along the Kulon Progo coastline in Yogyakarta, Indonesia using both field surveys and remote sensing techniques. The particular coastal segment under investigation is bounded by two river mouths emptying into the sea at the western and eastern extremities. Historical shoreline positions were obtained through analysis of satellite imagery spanning multiple years. In-situ fieldwork activities further involved bathymetric profiling to map the nearshore seabed topography, tidal measurements, and sediment sampling to characterize the beach material. These primary measurements were integrated into numerical hydrodynamic models to simulate past and predict future shoreline changes under seasonal influences. Simulation outcomes were validated against observed satellite data showing sediment accretion dominance over an approximately 10 year period. However, seasonal fluctuations had major impacts. Erosion was most severe near the western jetty during dry months attributed to interrupted sediment flow. The coastline recovered rapidly in monsoon seasons due to heightened sediment deposition from full-capacity rivers discharging onto the beaches.
OS11-A028
Analyzing the Survival Mechanisms of Claviaster Libycus During Mass Extinction and the Impact of Hydraulic Structure Geometry on Local Scour Using Discontinuous Bi-viscous Model
Tso-Ren WU1#+, Pin-Jie LIN1, Jih-Pai LIN2, Mei-Hui CHUANG1, Yi-Xuan HUANG1, Jia-Jie CHU1
1National Central University, 2National Taiwan University
Previous research indicates that the survival rate of Claviaster libycus following mass extinction events surpasses that of regular echinoids. This investigation seeks to assess the flow dynamics and scour patterns resulting from the distinctive distorted morphology of Claviaster libycus using numerical modeling. Additionally, the study explores the potential application of this unique mechanism to mitigate local scouring associated with the foundations of hydraulic structures. The numerical model employed in this investigation, Splash3D, has been adapted from the open-source code Truchas, originally developed by the National Laboratory of the United States. Splash3D is designed for solving the three-dimensional, incompressible Navier-Stokes equations. The Volume of Fluid Method (VOF) is utilized to characterize the kinematics of the water and sand surfaces. As Claviaster libycus partially submerges in the sand, the rheological behavior of the bottom sand is characterized using the Discontinuous Bi-Viscous Model (DBM), derived from the conventional Bingham Model (BM). Unlike the BM model, the DBM model employs the yield strain rate instead of the yield stress to differentiate the plug from the liquefied zone. In the Plug zone, high viscosity signifies solid characteristics, with the plug-zone viscosity significantly surpassing that of the liquified zone. The liquified zones represent sand disturbed by local currents around irregular echinoids, while the plug zones depict undisturbed sand. The yield strain rate dictates the stiffness of the bottom sand, and the DBM model is employed to describe local scour around obstacles. According to numerical simulations and experimental results, when the gonopore of Claviaster libycus is directed downstream, it can reduce the generation of horseshoe vortices. Therefore, compared to the gonopore pointing upstream, having the gonopore directed downstream can decrease the local scour around the sea urchin. Detailed analysis results are presented in the conference.
OS11-A026
Investigation of Morphological Evolution of Singaraja Coast Using Topographic and Bathymetric Data
Adi PRASETYO1, Cahyo Nur Rahmat NUGROHO2+, Irham Adrie HAKIKI2#, Mohammad FARID3, Nobuhito MORI4
1Ministry of Public Works and Housing, 2Ministry of Public Works, 3Bandung Institute of Technology, 4Kyoto University
Singaraja Coast is located on the Buleleng Regency north coast of Bali Island. During the Dutch East Indies government, they built a port as a main gateway to the island and center of the economy. Today, even though the provincial government has been moved elsewhere, the main activities and development of Singaraja City is still centered around the coastal area. Because of that, potential hazards from the sea, will have a high risk impact on this zone. Several areas on Singaraja Coast are already protected by hard measures such as revetment, however some of these measures affect the buffer area so the beach is decreasing and the utilization potential is reduced. To better understand the coastal dynamics in this area so a more sustainable and adaptable approach can be used, frequent monitoring of morphological condition is performed in Singaraja Coast. Morphological change investigated by topographic and bathymetric measurement in selected coastline of 750 m in length which represent various utilizations in the hinterland and also provide access for using more advanced monitoring techniques. The monitoring program was initiated in 2023 and several measurements had been carried out in June, October, and November 2023 and will continue periodically for the next 5 years. From these initial measurements, several dynamics could be observed such as erosion that happened during east monsoon season in the coastline area while the moved sediment is deposited to the nearshore zone. The sand thickness in the coastline area is reduced in the range of 0.2 – 0.6m while the average thickness of sedimentation in the nearshore zone is ranging from 0.2 – 0.7m. These monitoring data will be used for analyzing the long-term dynamics and also validating the hazard model for the BRICC Project.
OS11-A003
Wave impact on beach erosion at Shirogahama Beach
Shinya KIYOTO#+, Sooyoul KIM, Gozo TSUJIMOTO
Kumamoto University
Sandy beaches have the role of attenuating waves and preventing them from entering land areas. However, recent studies predicted that 60% of beaches in Japan disappear completely. In addition, many artificial beaches in Japan have been created by artificially injecting gravel and sand, which are highly vulnerable. Therefore, it is essential for beach conservation to predict topographic changes in artificial beaches. In the present study, topographic observation and bottom sediment analysis were conducted at Shirougahama Beach, focusing on the foreshore topography and evaluating the amount of beach berm retreat due to rising sea levels and waves. First, we examined the beach characteristics using a polynomial approximation. As a result, it was found that Shirougahama Beach tends to erode. We also confirmed that a positive correlation between a foreshore gradient and grain sizes exists. Finally, the amount of shoreline recessions was evaluated using the Constructal Law. The sea level rise, S, was found to be 11.5 S when the wave height was 0.3 m, 12.5 S when the wave height was 0.5 m, and 13.7 S when the wave height was 0.5 m. As a result, it was found that waves largely influence beach erosion. As wave heights increase, the amount of shoreline recession increases.
OS11-A002
Parameterization of the Mangrove Shape (Rhizophora Stylosa) and Its Application to Wave Height Attenuation
Yusuke HASEGAWA1#+, Yu-Lin TSAI2, Che-Wei CHANG3, Nobuhito MORI3
1DPRI, Kyoto University, 2National Yang Ming Chiao Tung University, 3Kyoto University
Mangroves can attenuate tsunamis, storm surges, and waves. Their protective function against wave disasters is gaining increasing attention as a typical example of the green infrastructure/Eco-DRR (Ecosystem-based Disaster Risk Reduction) in coastal regions. Hydrodynamic models commonly employed additional friction or a drag-force term to represent mangrove-induced energy dissipation for simplicity. In this study, we conducted field surveys on the Iriomote Island of Okinawa, Japan, and Tarawa, Kiribati. By analyzing the series of field data, comprehensive parameterization of mangrove shapes, such as the trunk diameter at breast height, tree height, prop roots height, and the root system's projected areas, for hydrodynamic modeling was conducted. We also conducted the wave height attenuation based on the mangrove shape and age of the tree.
OS11-A023
Hydrodynamics and Morphological Data Monitoring System for Singaraja Coast as Implementation of Theme 1 of BRICC Project
Irham Adrie HAKIKI1#+, Adi PRASETYO2, Cahyo Nur Rahmat NUGROHO1, Mohammad FARID3, Nobuhito MORI4
1Ministry of Public Works, 2Ministry of Public Works and Housing, 3Bandung Institute of Technology, 4Kyoto University
Natural disasters are potential hazards that coastal communities frequently face such as coastal flooding, storm waves, and tsunami. The occurrence of some disasters too has changed due to climate changes which increases the challenges for mitigating the risk. For developing countries that have long coastlines, such as Indonesia, coastal areas are important regions that sustain the economics and livelihood of its people. Preserving the coastal area needs to factor the balance of security and sustainability because of many overlapping interests from the stakeholders if we want to adapt to the ever changing world. In Indonesia, data availability on a coastal area is one of the major problems for taking effective measures in handling such issues. The Building Sustainable System for Resilience and Innovation in Coastal Community (BRICC) project is made to improve the defense function of coastal areas in Indonesia based on the latest scientific evidence with one of main themes being real time and long-term monitoring for hydrodynamics and morphology data. Wave and current measurements are performed to analyze the hydrodynamics condition while topographic measurement and CCTV are used for morphological analysis. This paper aims to present the system we set in Singaraja Coast and the measured data that we have acquired. We intend to use the data to investigate the relation of wave action to the coast dynamics in Singaraja Coast. Afterwards, the data will be used for hazard model development and optimization in Indonesia.
Session Chair(s): Zhenhua XU, Chinese Academy of Sciences, Craig STEVENS, National Institute of Water and Atmospheric Research
OS02-A017
Internal Lee Wave Generation from Geostrophic Flow in the Northwestern Pacific Ocean
Zhenhua XU#+
Chinese Academy of Sciences
Among the global mapping of lee wave generation, a missing piece exists in the northwestern Pacific Ocean (NPO), which features complex topographies and energetic circulations. This study applies Bell’s theory to estimate and map internal lee waves generated by geostrophic flows in the NPO using Mercator Ocean reanalysis data and the full topographic spectra obtained from the latest synthetic bathymetry product. Unlike the dominant contributions from abyssal hills in the Southern Ocean, multiple topographies, including ridges, rises, and continental margins, result in an inhomogeneous lee wave generation with multiple hotspots in the NPO. Over ridges, the rough topography creates a high potential for triggering lee waves. Over rises and continental margins, the stronger currents at the shallow depths are favorable for lee wave generation. In the Kuroshio extension region, the rough topography and strong currents cause the strongest lee wave generation. The lee wave hotspots contributed by mean flow are concentrated in specific regions, while those by geostrophic eddies are widely distributed. Geostrophic eddies are the primary contributor to lee wave generation, which account for 74.6% of the total energy transferred from geostrophic flow to lee waves.
OS02-A004
The Effect of Tides on Eddy Viscosity Via K-Profile Parameterization in the South China Sea Near Luzon Strait
Zhitao YU#+, Yalin FAN
U.S. Naval Research Laboratory
The non-local K Profile Parameterization (KPP) is a one-dimensional parameterization of the vertical turbulence mixing in the water column. It is the main mixing scheme used in the HYbrid Coordinate Ocean Model (HYCOM). There are two distinct mixing regimes in KPP. In the ocean surface boundary layer (OSBL), the mixing is driven by surface forcing. In the ocean interior, vertical mixing is driven by resolved shear instability, internal wave breaking, and double diffusive mixing. In this research, two global HYCOM simulations conducted with and without tidal forcing are used to study how tides affect eddy viscosity in the South China Sea (SCS) near Luzon Strait in June 2018. Our analysis reveal that tides play a crucial role in modifying eddy viscosity. Specifically, tides enhance surface heat flux, and thus stabilize the OSBL and lead to a reduction of eddy viscosity in the OSBL at Luzon Strait. Moreover, internal tides generated at Luzon Strait propagate into the SCS under tidal forcing conditions. They increase the vertical shear of the velocity and consequently enhance eddy viscosity in the ocean interior. Notably, the HYCOM simulation with tides demonstrates substantial eddy viscosity, reaching the order of 10-3 m2/s at depth of ~2000 m at the Luzon Strait. The clear signature of spring-neap tidal cycle in the strong eddy viscosities attributed their generation to internal tides. Furthermore, due to the existence of the high-salinity North Pacific Tropical Water in the upper ocean of SCS (~125 m), double diffusive mixing generated by salt fingering is shown to be more important than the background internal wave contribution at these depths.
OS02-A019
Imprints of Shikoku Recirculation Gyre on the Spatial Patterns of Mixing Revealed by Argo Observations
Xing XU#+
Chinese Academy of Meteorological Sciences
Diapycnal mixing in the ocean plays a significant role in the kinetic energy budget as well as the regional marine system balance, however, their patterns are not well understood due to the limited and costly direct measurement on the dissipation scales. In this research, through fine-scale parameterizations using approximate 13,100 Argo profiles collected near the Shikoku Recirculation Gyre (SRG) during 2016-2018, we study the diapycnal mixing induced by internal waves in the presence of Kuroshio current, and find that the spatial patterns of diapycnal mixing are largely modulated by the Kuroshio current meandering. Observations shows that high values of dissipation rate ɛ are more frequently observed within the SRG, and the mean ɛ near the core of gyre reaching O(10-7) W·kg-1 is roughly 2 orders higher than the surrounding waters. By using an eddy-resolved climate model, we find that the SRG negative vorticity acts to attract the wind-generated near-inertial internal waves in the upper ocean, and promote the downward-propagation and breaking of waves that would lead to appreciable dissipations in ocean interiors.
OS02-A009
Satellite Observed Multisource Internal Tide Radiation and Interference in the Banda Sea
Peiwen ZHANG#+
Chinese Academy of Sciences
Both the semidiurnal and diurnal internal tides in the Banda Sea were investigated using multi-satellite altimeter data, through a combination of plane wave analysis technique and two-dimensional band-pass spatial filtering. The west and central Banda Sea are found to be dominated by semidiurnal internal tides, while the diurnal internal tides dominate the east. Multiple internal tidal sources were located at or nearby the Banda Arc, radiating significant internal tides inwards in complex interference patterns in the Banda Sea basin. The semidiurnal sources were situated on the northern and southern sides of the Banda Arc, emanating internal tides in opposite meridional directions. The semidiurnal tidal beams then experienced interference, shaping the heterogeneous energy fields in the west and central Banda Sea. The primary diurnal source was situated over the steep slope in the Aru Basin, with significant energy radiation westward and diffraction in the east Banda Sea. Based on the estimation of 27-year coherent satellite results, the total energy flux of mode-1 internal tides into the Banda Sea is about 4.82 GW, 58% contributed by semidiurnal tides and 42% by diurnal tides. This study represents the first observed mapping of the complex and inhomogeneous mode-1 semidiurnal and diurnal internal tidal energy fields over the entire Banda Sea. Furthermore, this study enables further characterization of tidal mixing properties and improvement of model mixing parameterizations in the Indonesian seas.
OS02-A015
Observed Near-inertial Waves Generated by Tropical and Extratropical Cyclones in the East China Sea
Jia YOU#+, Zhenhua XU
Chinese Academy of Sciences
Both tropical and extratropical cyclones can affect the East China Sea (ECS) shelf in summer. Based on a current mooring deployed in 2014, near-inertial waves (NIWs) triggered by both extratropical and tropical cyclones were examined. During the observation period, three tropical cyclones (i.e., NEOGURI, MATMO, and NAKRI) passed by the mooring site. MATMO and NAKRI led to obvious near-inertial responses. The weakest tropical cyclone (MATMO) caused the strongest NIWs due to its large translation speed and favorable position relative to the mooring site. Mode 1 dominates the vertical structure of the NIWs caused by tropical cyclones. Due to the modulation of the background vorticity, the NIWs show a significant blueshift. However, the NIWs caused by extratropical cyclones are mainly concentrated near the surface layer with a higher proportion of mode-2 NIWs. The highest value of the near-inertial kinetic energy generated by extratropical cyclones is about half of that generated by tropical cyclones. In addition, both two kinds of cyclones can lead to an enhancement of subinertial current in the ECS shelf. The nonlinear interactions between NIWs and semidiurnal internal tides (D2) are also evidenced, with the NIWs being a potential trigger for D2-f waves. This study highlights the important role of NIW on the nonlinear interactions and energy transfer within the internal wave spectral continuum in the continental shelf region.
OS02-A014
Vertical Mixing and Turbulence Characteristics Around Ieodo: Observations and Implications
Seung-Woo LEE#+, Suyun NOH, Jongmin JEONG, Su Chan LEE, Jaeik LEE, Yong-Chim MIN, Jin-Young JEONG
Korea Institute of Ocean Science & Technology
Vertical mixing and turbulence processes in the ocean play an important role in understanding the physical properties of seawater and their impact on biogeochemical systems. The Ieodo area in the northern East China Sea undergoes rapid bathymetric changes due to a submarine rock (sill), resulting in strong influences from internal waves and tides. However, our understanding of turbulence processes not only in the waters around Ieodo but also around the sill is still limited. In this study, we analyze ship-based observation data from September 2022 to investigate the characteristics of vertical mixing and turbulence around the Ieodo. From September 24 to 26, cross-sectional observations were made with shipboard instruments including CTD, VMP250 and ADCP to obtain profiles of temperature, salinity, density, dissolved oxygen, turbidity, fluorescence, and turbulence with an additional bottom mooring of a current meter 1.5 km southeast of Ieodo and a 30-hour continuous shipboard observing station 3 km away. The observations revealed a thermocline (pycnocline) in the 20-30 m depth range, yielding stability with a buoyancy frequency of O(10-3). Near the top of Ieodo, the pycnocline shallowed, and the upper layer ascended. Significant turbulence dissipation rates (O(>10-6 W/kg)) and large vertical diffusion coefficients (O(10-5-10-4 m2/s)) were observed at 30 m depth in the eastern and northern regions. The 30-hr continuous observation revealed strong turbulence with a 12-hour periodicity associated with semi-diurnal tidal currents. These strong turbulence processes were discussed in relation to biogeochemical factors such as dissolved oxygen, chlorophyll fluorescence, and turbidity. This study suggests that the waters around Ieodo, a submerged rock in the northern East China Sea, are crucial for understanding vertical mixing and turbulence processes and highlights the biogeochemical impacts of such turbulent processes.
OS02-A005
Irreversible Mixing Induced by Geostrophic Turbulence Over the Global Ocean
Tongya LIU1#+, Yu-Kun QIAN2, Xiaohui LIU3, Shiqiu PENG4, Dake CHEN3
1Second Institute of Oceanography, Ministry of Natural Resources, 2South China Sea Instititue of Oceanology, 3Ministry of Natural Resources, 4Chinese Academy of Sciences
Two recently proposed mixing diagnostics are employed to estimate the global surface irreversible mixing based on particle and tracer simulation driven by satellite-derived geostrophic velocities. These two novel diagnostics, similar to the traditional dispersion diffusivity and Nakamura’s effective diffusivity but defined in a localized and instantaneous sense, have the following advantages: 1) reconcile the theoretical discrepancies between Eulerian-, particle-, and contour-based diffusivities; 2) do not rely on the stationary and homogeneous assumptions of the turbulent ocean and are free from traditional average operators (e.g., Eulerian time-/space or along-contour mean). Our results show that evident discrepancies among these three types of diffusivities do emerge when employing traditional estimates. However, these discrepancies could be significantly mitigated with the adoption of new diagnostic methods, implying that the three types of diffusivities can be effectively reconciled within a global framework. Moreover, fine-scale mixing structures and transient elevated mixing events due to geostrophic stirring can be clearly identified by the two new diagnostics, in contrast to previous estimates that are spatially and/or temporally smoothed. In particular, it is interesting to note that large values of the new diagnostics usually occur along narrow filaments/fronts associated with mesoscale eddies, and elevated mixing is observed to be located at the periphery of eddies. Our study presents a novel revisit of the global surface mixing induced by geostrophic eddies with an emphasis on irreversibility, and provides new insights into previous questions regarding to different mixing diagnostics in the community.
OS02-A006
Critical Latitude Effects on Mixing and Energy Transfers with Additional Relative Vorticity
Robin ROBERTSON#+
Xiamen University Malaysia
Deep ocean mixing has been attributed to internal tides and waves. Mixing increases near the tidal critical latitudes as internal tides become resonant. The critical latitudes are defined as where the inertial frequency (based on the Coriolis parameter) equals the tidal frequency. Previous studies indicated that the critical latitude is shifted by local relative vorticity from currents or eddies, and the shifts can reach 5° of latitude. The effects of different vorticity fields associated with an eddy on critical latitude shifts and on mixing, internal waves, and energy shifts between frequencies through interactions of an eddy with a seamount were investigated. The critical latitude range, shifts in the critical latitude, and changes in mixing depended on the eddy strength and rotational direction. The direction and amplitude of critical latitude shift was related to the sign and intensity of the vorticity field, respectively. Psi occurred during a distinct phase of the simulations and was also dependent on the additional relative vorticity. PSI shifted energy within the first 180 days increasing the energy at low frequencies; however, by 360 days, the energy transfers changed and more energy appeared at the semidiurnal frequencies. A relation was developed to translate the critical latitude shift with the amount of additional relative vorticity. Most surprising was the response at high latitudes and the inflection point which occurred at 18oS, which were also dependent on the added relative vorticity.
Session Chair(s): Hongchun ZHANG, Nanjing University of Information Science & Technology
OS15-A008
| Invited
Advancing Sea Surface Temperature and Marine Heat Waves Predictions in the South China Sea: A 3D-Unet Deep Learning Model Integrating Multi-source Data
Jifeng QI#+
Institute of Oceanology Chinese Academy of Sciences
Accurate Sea Surface Temperature (SST) prediction is vital for disaster prevention, ocean circulation, and climate change. Traditional SST prediction methods, predominantly reliant on time-intensive numerical models, face challenges in terms of speed and efficiency. In this study, we develop a novel deep learning approach using a 3D-Unet structure with multi-source data to forecast SST in the South China Sea (SCS). SST, sea surface height anomaly (SSHA), and sea surface wind (SSW) are used as input variables. Compared to the Convolutional Long Short-Term Memory (ConvLSTM) model, the 3D-Unet model achieves more accurate predictions at all lead times (from 1 to 30 days) and performs better in different seasons. Spatially, the 3D-Unet model's SST predictions exhibit low errors (RMSE<0.5°C) and high correlation (R>0.9) across most of the SCS. The spatially averaged time series of SST, both predicted by the 3D-Unet and observed in 2021, show remarkable consistency. A noteworthy application of the 3D-Unet model in this research is the successful detection of marine heat wave (MHW) events in the SCS in 2021. The model accurately captured the occurrence frequency, total duration, average duration, and average intensity of MHW events, aligning closely with observed data. Sensitive experiments show that SSHA and SSW have significant impacts on the prediction of 3D-Unet model, which can improve the accuracy and play different roles in different forecast periods. The combination of 3D-Unet model with multi-source sea surface variables, not only rapidly predicts SST in the SCS but also presents a novel method for forecasting MHW events, highlighting its significant potential and advantages.
OS15-A001
Intelligent Recognition and Inversion of Internal Solitary Waves in the Northern South China Sea
Tongqing CHEN#, Zihan ZHANG+, Qinghe ZHANG
Tianjin University
The northern South China Sea is one of the areas where internal solitary waves are frequently observed, and the largest internal solitary wave is observed in this sea area. Internal solitary waves can exert significant influences on marine ecology, fishery resources, ship navigation and marine engineering. To assess the impact of internal solitary waves, it is important to obtain the position and geometric parameters of internal waves. Remote sensing is an important tool for obtaining internal wave parameters. MODIS remote sensing images of internal solitary waves in the northern part of the South China Sea were collected, and an intelligent recognition model of remote sensing images for internal solitary waves was established based on U-net neural network. This model was applied to extract the position of crest lines of internal solitary waves from remote sensing images in the South China Sea. Then, a fully connected deep learning neural network was used to build an intelligent inversion model of wave amplitude in the South China Sea, and the model was improved and optimized by various methods, including changing the network structure, replacing the activation function, regularization, etc. The model is applied to the data for intelligent inversion of internal solitary wave amplitude in the South China Sea. The results show that the model can reasonably obtain the wave amplitude of internal waves.
OS15-A003
An Accurate Spatial-temporal Typhoon Waves Prediction Model with Multi-output Neural Network and Parametric Cyclone Model
Wei-Ting CHAO#+
National Taiwan Ocean University
Typhoon waves induce devastating disasters in the coastal region. Therefore, accurate prediction of typhoon waves is crucial in reducing life and property losses for coastal protection research. In an earlier study, the neural network constructed a one-hour typhoon wave prediction with local station observation data in a specific area. However, sufficient prediction lead time and multiple gauge information are helpful for early warning and preparedness work. This study aims to develop an accurate spatial-temporal typhoon wave prediction model through a multi-output neural network and a parametric cyclone model. The meaningful typhoon parameters can be merged and transferred into more effective inputs (local pressure/wind from profile equations) through a parametric cyclone model. This method reduced the network structure's complexity and kept noteworthy information about the typhoon. Due to the error tolerance capability, ANN may alleviate the parametric model's evaluation error and sensitivity. Moreover, it can capture the nonlinear relationship between observed data and meteorological conditions to achieve accurate storm surge prediction. Overall, this hybrid model presented more efficiency and better accuracy. This model was applied to Taiwan's eastern, northeastern, and southwestern coastal regions, i.e., Hualien, Longdong, and Dongshi stations. A total of 15 historical typhoon events were chosen for model training and validation. It presented excellent capability for short lead-time typhoon-wave prediction and provided reasonable performance for longer lead time in each station.
OS15-A004
A Deep Learning Via 3D U-Net to Predict of Wave Height and Period
Yuqi DING1#+, Yuxiang MA1, Jie WANG2, Xiaokai LIU2
1Dalian University of Technology, 2Dalian Maritime University
Forecasting ocean wave parameters such as significant wave height and wave period is important in coastal and ocean engineering, especially for extreme sea states. In this study, a 3DU-Net based deep learning method including information of history waves and winds is proposed. A dataset constructed using 20 years’ the ERA5 reanalysis dataset and the CMA tropical cyclone tracks are used to train the models. a dataset suitable for normal and extreme sea state learning was constructed. Then a 3DU-Net based and a 3DCNN based forecasting models were trained separately. The results show the 3D-Unet model performed better than the 3DCNN model. In normal sea states, the prediction accuracy of the 3DU-net model increase about 10% in height and 15% in wave period. However, in extreme sea states, the 3DU-Net model also works better.
OS15-A007
Satellite-based Global Sea Surface Oxygen Mapping and Interpretation with Spatiotemporal Machine Learning
Jian SHAO#+
Zhejiang University
The assessment of dissolved oxygen (DO) concentration at the sea surface is essential for comprehending the global ocean oxygen cycle and associated environmental and biochemical processes, as it serves as the primary site for photosynthesis and sea-air exchange. However, limited comprehensive measurements and imprecise numerical simulations have impeded the study of global sea surface DO and its relationship with environmental challenges. This paper presents a novel spatiotemporal information embedding machine learning framework that provides explanatory insights into the underlying driving mechanisms. By integrating extensive in-situ data and high-resolution satellite data, the proposed framework successfully generated high-resolution (0.25°×0.25°) estimates of DO concentration with exceptional accuracy (R2=0.95, RMSE=11.95 μmol/kg, test number=2805) for near-global sea surface areas from 2010 to 2018, uncertainty estimated to be ±13.02 μmol/kg. The resulting sea surface DO dataset exhibits precise spatial distribution and reveals compelling correlations with prominent marine phenomena and environmental stressors. Leveraging its interpretability, our model further revealed the key influence of marine factors on surface DO and their implications for environmental issues. The presented machine learning framework offers an improved DO dataset with higher resolution, facilitating the exploration of oceanic DO variability, deoxygenation phenomena, and their potential consequences for environments.
OS15-A018
Integration of GNSS-R and SMOS for Sea Surface Salinity Retrieval Using Artificial Neural Network
Zheng LI+, Fei GUO#, Xiaohong ZHANG
Wuhan University
Sea surface salinity (SSS) is crucial to the marine ecosystem. Soil Moisture and Ocean Salinity (SMOS) has developed a geophysical model function (GMF) for sea surface brightness temperature and SSS, which incorporates sea surface wind speed and significant wave height (SWH) to retrieve the SSS. However, the relationship between sea surface brightness temperature and SSS is complex and influenced by various factors. The GMF that only includes sea surface wind speed and SWH cannot accurately characterize this relationship. Spaceborne Global Navigation Satellite System Reflectometry (GNSS-R) observations directly respond to sea surface roughness and offer low cost and high spatiotemporal resolution advantages. Therefore, in this study, spaceborne GNSS-R observations have been incorporated into the SMOS SSS retrieval. Additionally, an empirical model between SMOS brightness temperature and Argo SSS was developed using an artificial neural network (ANN). Compared to the conventional SMOS SSS retrieval method, the proposed method in this study significantly improves the SSS retrieval performance. Furthermore, comparisons were made with ground truth measurements from the National Data Buoy Center (NDBC) buoys, which indicated that the proposed method reduces the root mean square error (RMSE) of retrieving SSS by 27% and the absolute mean deviation by 24%. These provide references for the future application of spaceborne GNSS-R in SSS retrieval.
OS15-A020
Integrated UAV and DETR Study for Marine Debris Detection
Ye-Been DO+, Hong Joo YOON#
Pukyong National University
Marine debris, causing various issues such as the destruction of marine ecosystems, ship accidents, and a decline in the quality of tourism resources, is recognized as a common global marine environmental problem, as it moves across borders following wind and currents. Efforts to manage this issue includes the establishment of international agreements for marine pollution prevention and the provision of related regulations. In the case of The South Korea, the active coastal tourism industry and fishing activities contribute to a significant increase in the frequency and quantity of marine debris. Consequently, the nation is conducting comprehensive investigations into marine debris on a regional basis. However, the extensive costs and manpower required to survey entire maritime areas pose challenges. In particular, when urgent decision-making and pollution cleanup operations are required due to situations such as typhoons, there is a lack of immediate survey systems and tools. To address this gap, research is underway on the utilization of remote sensing methods for marine debris investigation. This study focuses on utilizing the UAV (Unmanned Aerial Vehicle) and the DETR (Detection with Transformer) model, a Transformer-based object detection model capable of flexible detection of marine debris of various sizes and quantities. The goal is to conduct efficient marine debris detection research, overcoming limitations of existing methods. This approach is anticipated to contribute to more effective national marine debris surveys and management in the future. This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE).
OS01-A003
Impact of Marine Heatwaves on Variations in Typhoon Intensity in the Western Pacific
Thi-Kieu-Diem NGUYEN#+, Po-Chun HSU
National Central University, Taiwan
Marine heatwaves (MHWs), characterized by extreme warm water events in the ocean, have become more frequent and intense due to climate change. To examine the impact of ocean warming and MHWs on the intensity of typhoons, we combined satellite and high-resolution ocean thermal reanalysis data from 1993 to 2023 in the western Pacific. Over these 30 years, there have been noticeable and consistent increases in sea surface temperatures (SST) and upper ocean heat content (OHC) near the typhoons’s core regions. The averaged MHW categories varied by about 0.2 to 2 during the summer, with a particularly significant upward trend observed between 2016 and 2023 (0.6 to 2). Years with intense MHW categories strongly correlated with elevated OHC prior to the typhoon seasons. We objectively obtained typhoon intensity by utilizing satellite remote sensing systems along established typhoon paths. The study period revealed significant year-to-year variations and regular oscillations in the highest intensities of typhoons. In the years following high MHW categories, there was a dramatic increase in average typhoon intensity, more significant than the average intensity observed between 1993 and 2023. This suggests that typhoons undergo rapid intensification by extracting energy from the abnormally warm water layers beneath MHWs. Our results emphasize the correlation between upper ocean warming caused by MHWs and the increasing likelihood of severe typhoons in this region if climate change continues unaddressed. Adopting measures to enhance resilience against anticipated rises in severe typhoons and progressively escalating ocean temperatures in the western Pacific is imperative. This study provides strong empirical evidence that increasingly severe MHW categories can significantly enhance typhoon intensities through the transfer of heat from the ocean. It also underscores the role of MHWs and ocean thermal structures in changing typhoon intensity, enhancing forecast accuracy, and understanding ocean responses during extreme events.
OS01-A005
Utilizing Himawari Satellite Data and Clustering Analysis to Investigate the Response of Ocean Chlorophyll Concentration and Sea Surface Temperature in the Northwest Pacific to Typhoons
Dimas Pradana PUTRA#+, Po-Chun HSU
National Central University, Taiwan
Typhoons intensely impact the upper ocean and have been shown to induce phytoplankton blooms through vertical mixing and upwelling of nutrients. However, the intricate and specific patterns of these blooms, are influenced by various environmental factors. This study addresses a critical knowledge gap by employing a province clustering analysis to investigate the spatiotemporal dynamics of chlorophyll-a and sea surface temperature induced by typhoons in the North West Pacific basin. Using Himawari-8 satellite data, chlorophyll-a concentrations, and sea surface temperature are monitored at various distances from typhoon eyes during the 7-day periods before and after each typhoon occurrence spanning from 2015 to 2022. The cluster analysis reveals distinct biogeochemical provinces, each demonstrating responses to typhoons. Furthermore, the research explores the relationships between physical drivers and bloom intensity by incorporating sea surface temperature data. The province-level clustering methodology provides an approach for mapping biophysical interactions and sampling extreme bloom events. This province-specific framework can guide the modeling and prediction of extreme typhoon-induced blooms and ecosystem impacts.
OS01-A010
High Blooming Caused by a Weak Typhoon Nalgae (2022) in the Northern South China Sea
Jia-En LIN#+, Yuchun LIN
National Taiwan Ocean University, Taiwan
Tropical Cycle (TC) is a strong atmospheric circulation over the tropical and subtropical ocean. The vigorous TC winds often cause intense interactions between the atmosphere and the ocean, leading to the upwelling of subsurface water, the asymmetric cooling and the chlorophyll blooming in the TC wakes, which are potentially linked to the TC intensity. This study focuses on the mechanism of a high chlorophyll blooming event caused by Typhoon Nalgae (2022), a tropical storm, in the South China Sea. After Typhoon Nalgae (2022) formed east of Philippines on October 27, 2022, it moved westward across Luzon Island and turned 90° northward into the North South China Sea. Typhoon Nalgae (2022) caused high phytoplankton blooming that reaches 3.86 mg m-3 in the wake (15°-20°N, 115°-118°E) 4-day after Typhoon Nalgae passed on November 4, 2022. According to the IBTrACs data, the average translation speed of Typhoon Nalgae is 4.54 m/s, which is moderate among the 406 TCs in the South China Sea from 1998 to 2022. After carefully examining the environmental data, we found that the such high blooming caused by a relative weak TC could be attributed to the combination of the shallowing of the Depth Chlorophyll-a Maximum (DCM) layer in the North South China Sea and the circling of TC path.
OS02-A011
Constructing Hydrological Waving Model and In Situ Sediments Observation Methods in the High School Scientific Activities
Ryo NAKAMURA1,2#+
1Miyagi Rifu High School, Japan, 2Japan Society of Ocean Education, Japan
I will introduce about the ocean wave effects for the sediments in the geoscience class and scientific activities in the high school. (1) Observe the ripple mark and wave effects for under ocean. One of science club students has observed ripple mark in underwater or along coast line in his surf activity everyday. He observed various wave length ripple mark in seabed surface and its depends on the ocean wave velocity and/or wave length. We constructed wave generator with frequency 4Hz and 8Hz in the 0.10m water depth. We found the factor of ripple mark width/length were depended on the wave frequency. (2) Leading students to construct oscillation mechanics and making constant velocity oscillating motion. In order to construct wave generation mechanics, it is necessary to oscillating by horizontal or vertical water compression. We adopted vertical one, therefore the repeated motion makes ascend and gravitational falling as “vertical oscillator”. It has led to repeatable hooked by finned two “Rotator” that connected by two motors. Motors has parallel bridging and facing each other and rotate opposite. We also need to suppresses micro horizontal miscellaneous vibrations. Top part of vertical oscillator has been loosely supported by paper strings. Finally we succeeded to construct constant wave generator in tens centi meter size for in situ wave observations. In this presentation, I would like to discuss about the possibility for constructing observation model with easy/not-expensive method.
OS02-A013
Spontaneous Near-inertial Wave Generation from Mesoscale Eddy
Ji LI#+, Zhenhua XU
Chinese Academy of Sciences, China
The timescale separation between slow balanced flows and fast internal gravity waves (IGWs) is crucial in mid-latitude atmosphere and ocean mesoscale dynamics. IGWs, linking large-scale climatological forcing to turbulent dissipation, play a vital role in multiscale energy transfer and turbulent mixing, particularly with mesoscale eddies dominating oceanic kinetic energy. Investigating the spontaneous generation of IGWs from balanced geostrophic vortices, both anticyclonic and cyclonic, reveals a universal spiral pattern occurring via an instability mechanism. In the vertical direction, mode 1 dominates, resulting in weak dissipation and long-distance propagation. The energy transfer to small-scale turbulence via IGWs is essential for mesoscale eddy energy dissipation. Comparing barotropic and baroclinic vortices suggests that nonzero horizontal strain and vorticity are crucial for the instability mechanism, with vortex baroclinicity intensifying IGWs. IGWs emitted from anticyclonic vortices are stronger than those from cyclonic ones. The near-balanced quasi-geostrophic state of the vortex post-IGW emission is accompanied by high-frequency inertial oscillations due to timescale separation. IGWs are generated by external linear forcing, forming a near-inertial wave (NIW) generation mechanism. The Doppler effect, influenced by mesoscale eddy propagation, results in a blue shift, causing resonance and strengthening NIWs intensity. The baroclinicity of mesoscale eddies is essential for this NIW generation mechanism. NIWs generated spontaneously share horizontal wavenumbers with the eddy but radiate energy toward the eddy center, remaining stationary relative to the propagating eddy. NIW intensity depends exponentially on Rossby number (0.04 to 0.1) and positively on Froude number. Anticyclonic mesoscale eddies emit stronger IGWs than cyclonic ones in both transient and forcing generation.
OS02-A016
Transient Response of Langmuir Turbulence in a Diurnal Cycle
Qing LI#+, Wentao PAN
The Hong Kong University of Science and Technology, China
Langmuir turbulence (LT) enhances turbulent mixing in the ocean surface boundary layer. Previous scalings of such LT enhanced turbulent mixing are mostly based on large eddy simulations (LESs) under constant forcing. The assumption when applying these scalings to parameterizations is that LT is in equilibrium with the forcing. Under transient forcing in a diurnal cycle, this assumption may break, especially in the morning when stabilizing solar radiation is increasing rapidly and turbulence is decaying. Here we study the transient response of LT in idealized diurnal cycles using LES. These LES experiments under smooth transient forcing are supplemented by similar experiments with abrupt changes in forcing. The goal is to better understand the timescale of the adjustment of LT to the changing forcing. Preliminary results of the transient response of LT to the changing solar radiation in idealized diurnal cycles, including its effects on momentum and tracer fluxes, will be presented. Implications for improving existing LT parameterizations will be discussed.
OS03-A003
No Recovery of Antarctic Sea Ice Under Net-zero Carbon Emissions
M. Inês CAJADA1#+, Seok-Woo SON1, Jinho YOON2, S. Y. Simon WANG3, Soon-Il AN4
1Seoul National University, Korea, South, 2Gwangju Institute of Science and Technology, Korea, South, 3Utah State University, United States, 4Yonsei University, Korea, South
The decline of sea ice area in recent years has raised questions about whether carbon reduction measures can mitigate sea ice loss. By integrating a climate model with net-zero and negative emission scenarios, the present study shows that the evolution of sea ice area in the Antarctic may differ from that in the Arctic. It is found that net-zero emissions lead to a slow recovery of Arctic sea ice area compared to its loss in a warming climate. However, they do not result in Antarctic sea ice recovery. The Antarctic sea ice area keeps decreasing especially in austral summer, remaining ice-free after 2050. Unless negative emissions are enhanced, Antarctic sea ice may not return to its initial state within one hundred years. This hemispherical-asymmetric sea ice change under net-zero scenario results from a slowdown of the Atlantic Meridional Overturning Circulation and the increase of ocean heat content in the Southern Ocean, which can explain the sea ice area response.
OS03-A008
Interannual Variations of Modified Circumpolar Deep Water and Glacier Meltwater in the Dotson-Getz Trough in Summer
Chunhu XIE1, Jiuxin SHI1#, Yongming SUN1+, Jindong JIANG2
1Ocean University of China, China, 2First Institute of Oceanography, China
The melting of the West Antarctic Ice Shelf has increased since the 1990s, driven by the relatively warm Circumpolar Deep Water (CDW) that penetrates into the West Antarctic Ice Shelf cavities through submarine glacial troughs across the continental shelf. In this study, temperature, salinity, and current velocity data obtained by the Chinese National Antarctic Research Expedition in the Dotson-Getz Trough (DGT) shows clear differences in distribution of modified Circumpolar Deep Water (mCDW) and Glacier Meltwater (GMW) in the summers of 2020, 2022 and 2023. Combined with contemporaneous wind data and additional temperature and salinity data from instrumented seals, the processes and mechanisms responsible for this variation are discussed. Compared with 2020, there is a significant increase in mCDW thickness in 2022 and 2023, with a doubling of total heat content as the mCDW inflow path across the DGT shifts towards the eastern bank. We propose that a southward shift in the westerly winds in the summer of 2022 moved the upper oceanic divergence zone southward towards the continental slope, promoting the upwelling of mCDW above 500 m. Concurrently, stronger westerly winds over the continental slope strengthened the eastward undercurrent, increasing the mCDW transport and the heat content to the DGT. As the input of mCDW increases, the content of GMW in the trough also increases significantly, and it is exported northward through multiple pathways on both sides of the trough. In addition, changes in the content of GMW can also affect the input of mCDW with further research needed. These observations show there is strong interannual variability in the strength, pathway and extent of mCDW and GMW inflows to the DGT and that care must be taken when planning observation programs for long-term monitoring of the oceanic heat input to the ice shelves of this globally significant region.
OS03-A011
Atmospheric CO2 Induced Changes in Antarctic Continental Shelf Water: Insights from a High-resolution Global Climate Model
Jaemin JU1+, Sunghyun NAM1, Taewook PARK2#
1Seoul National University, Korea, South, 2Korea Polar Research Institute, Korea, South
The Antarctic continental shelf water (ACSW) plays a crucial role as a buffer in the interaction of heat and materials between the Southern Ocean and Antarctica. Some Antarctic continental shelves generate high-salinity water, the source of Antarctic Bottom Water (AABW), a key component of global ocean circulation. However, the impacts of climate change in Antarctic shelf ocean environments remain uncertain and challenging. To examine the effects of atmospheric greenhouse gases in ACSW properties, we analyzed data from the Community Earth System Model version 1.2.2, a fully coupled high-resolution global climate model. Two climate scenarios were compared: Present-day Climate (PC) and the Future Climate (FC) runs. The PC experiment fixed atmospheric CO2 concentration at 367 ppm, while the FC experiment doubled it. Both model experiments were conducted by the Institute for Basic Science Center for Climate Physics in Busan, South Korea. Compared to PC experiments, the FC experiments showed an overall increase (0.243±0.169 °C) in ACSW bottom temperature, except in an area off the eastern Amundsen Sea and Bellingshausen Sea coasts. Salinity exhibited an overall freshening (0.203±0.146 g/kg), and the outflow of AABW from Antarctic continental shelf was entirely blocked in the FC experiment. In particular, contrasting ACSW property changes were found between the western and eastern Ross Sea: freshening on the west side (> 0.3 g/kg decrease in salinity) and warming on the east side (> 0.5 °C increase in temperature). To better understand these changes in Ross Sea water properties, we discussed the impacts of ocean circulation, ocean-atmosphere interaction, and sea ice melting/formation. This study provides significant insights into ACSW properties under doubled CO2 conditions and their implications for global ocean circulations through AABW formation in a changing climate.
OS03-A017
Four Different Mesoscale Eddies and Their Characteristics in the Southern Ocean
Hyojun SEUNU+, Hajoon SONG#, Junghee YUN, Kyungmin KWAK
Yonsei University, Korea, South
The mesoscale eddies are commonly classified into two categories based on anomalous sea surface height (SSH): anticyclones for positive SSH anomalies and cyclones for negative SSH anomalies. Recent studies have identified the existence of abnormal anticyclones and cyclones. In our study, we define abnormal mesoscale eddies based on sea surface density anomalies. These eddies, termed mode-water eddies and thinny, exhibit inverted isopycnal in the upper layer compared to normal mesoscale eddies. When applying detailed classification of mesoscale eddies to the satellite observations and a 1/20 degree resolution ocean model over the Southern Ocean, approximately 40% of the conventional eddies were actually classified as new types of eddies in the observations, and more were identified in the model data. Abnormal mesoscale eddies show distinct differences when compared with normal eddies. Particularly, a pronounced diffusivity was evident in mode-water eddies during the winter season. Mode-water eddies have a robust supply of iron due to enhanced vertical diffusion. The supplied iron, trapped in upper layer during stratified summer, led to vigorous biological activity when exposed to sunlight. These results suggest that the mesoscale eddy characteristics need to be re-evaluated after considering both normal and abnormal eddies separately.
OS03-A018
Effects of Antarctic Meltwater Inflow in Coupled Kim
Jin-Yun JEONG#+, Jun-Seong PARK, Myung-Seo KOO
Korea Institute of Atmospheric Prediction Systems, Korea, South
KIAPS is developing a spatio-temporal integrated coupled model system that can perform all predictions from a week to two months. At the first stage (2020-2022), the initial version of the coupled model was developed by coupling land (Noah with multiple parameterization; NoahMP), ocean (Nucleus for European Modelling of the Ocean; NEMO), and sea-ice (Sea Ice modelling Integrated Initiative; SI3) models based on the Korean Integrated Model (KIM). In the Second stage (2023-2026), not only the coupled model itself is improved, but also the wave model (Wave Watch III; WW3) is combined. In addition, coupling of the river-routing model (Catchment-based Macro-scale Floodplain; CMF) and land/ocean-sea-ice offline model are at a preliminary stage. During the spin-up process of ocean-sea ice offline model, we found that the coupled KIM underestimates Antarctic sea ice extent due to rapid sea ice loss in summer. To improve the predictive performance of Antarctica, we conduct experiments with meltwater inflow from the ice sheet or ice shelf into the ocean. Meltwater is known to affect the formation of sea ice by cooling the surface. Previous studies have shown that there are various ways to prescribe meltwater. It is sometimes distributed along its horizontal movement or injected directly in front of the ice shelf. Also, it is added to the surface or the ice shelf depth. Since the magnitude of the response varies depending on the methods, this study tries to follow several methods suggested in previous studies. The impact of the method difference of meltwater on the Antarctic and Southern Ocean on seasonal simulation in the coupled KIM will be shown. Acknowledgements: This work was carried out through the R&D project “Development of a Next-Generation Numerical Weather Prediction Model by the Korea Institute of Atmospheric Prediction Systems (KIAPS)”, funded by the Korea Meteorological Administration (KMA2020-02212).
OS03-A021
Intensification of the Antarctic Slope Current Due to Freshwater Forcing in a Warmer Climate
Myeong-Hyeon KIM1,2#+, Gyuseok YI1,2, June-Yi LEE2, Axel TIMMERMANN2, Wonsun PARK2, Sun-Seon LEE1
1IBS Center for Climate Physics, Korea, South, 2Pusan National University, Korea, South
The Antarctic slope current (ASC) flows westward along the Antarctic coastlines and influences heat exchange across the Antarctic continental shelf. Therefore, it could play an important role in regulating the Southern Ocean circulation by affecting processes such as ice melting and water mass formation. However, clarifying the mechanism and change of ASC in future climate using high-resolution climate model is still challenging. We show that ASC is projected to accelerate in response to CO2 increases by comparing present-day and CO2 increased simulations (2×CO2 and 4×CO2) conducted with the fully coupled ultra-high-resolution Community Earth System Model. The intensification of ASC was attributable to an increase in the gradient of sea surface height due to a decrease in salinity through geostrophic balance. This freshening was dominated by sea ice melting, while increases in runoff and precipitation minus evaporation played a minor role with regional and seasonal dependence. These results increased understanding about the future change of ASC using high-resolution simulations and have important implications for changes in mesoscale ocean circulation and the climate of Southern Ocean.
OS03-A022
Responses of the South Pacific Ocean to Record Low Sea Ice Extent in the Late 2010s
Seong-Hyun JO+, Jae-Hong MOON#, Taekyun KIM
Jeju National University, Korea, South
Under increasing greenhouse gas concentration, the surface of the Southern Ocean (SO) has warmed over recent decades with a cooling trend to the south, particularly in the southern Pacific sector. Thus, the SO has shown little warming in contrast to the rapid warming in the Arctic. The cooling of the South Pacific Ocean mainly occurs along the Antarctic polar front (APF) where surface cold water subducts to the ocean interior, forming the Antarctic Intermediate Water (AAIW). The surface cooling, poleward of the APF leads to increase in heat uptake and the heat taken up at the surface is transported northward, resulting in enhanced warming to the north. Since sea-ice melting is one of the important factors that affects the sea surface cooling, the amount of sea-ice extent (SIE) and sea-ice melting would directly link to changes of the heat uptake capacity and heat storage in the South Pacific Ocean. According to satellite National Snow and ice Data Center (NSIDC) datasets, the SIE of the Antarctic has decreased dramatically since 2015 and reached a record low in the late 2010s. In this presentation, we will show how the South Pacific Ocean responds to the record low SIE event in the aspect of heat uptake capacity and heat storage change.
OS04-A034
Trace Metal, Ionic, and Isotopic Concentrations in Hydrothermally-induced Submarine Groundwater Discharge Areas in Mabini, Batangas
Marmelou POPES1+, Chris Carl Agustin TOYADO2, M. Bayani CARDENAS3, Neil STURCHIO4, Raymond RODOLFO5, Mark LAPUS6, Caroline Marie JARAULA2#
1University of the Philippines Diliman, Philippines, 2University of the Philippines, Philippines, 3The University of Texas, United States, 4University of Delaware, United States, 5Ateneo de Manila University, Philippines, 6Agriculture Sustainability Initiatives for Nature, Inc., Philippines
Submarine groundwater discharge (SGD) is a significant pathway of terrestrial freshwater into coastal ecosystems, especially in areas where surface runoff and rivers are scarce, such as Mabini, Batangas. Underlain by limestone and fractured volcanic terrane complex with an active geothermal system, Mabini fringes the Macolod Corridor off Maricaban Strait. Thus, occurrences of hydrothermally-induced submarine groundwater discharges (HISGDs) are prevalent along its coasts. In Mabini, HISGDs manifest as spring- and curtain-type acidic hydrothermal water with- or without-gas emanations. HISGDs may be predominantly recirculated seawater or mixed with freshwater inputs. Due to the thermal and acidic nature of HISGDs and the possible injection of geothermal fluids, the discharges may be enriched with major and trace metals. Samples from spring-, curtain-type SGD, sediment porewater, groundwater, and even tap water were analyzed for their trace metal, ionic and isotopic compositions using ICP-MS, Ion Chromatograph, and EA-IRMS, respectively. Hierarchical clustering and non-metric multidimensional scaling plot of major and trace metals and physico-chemical parameters (i.e. pH, temperature, salinity) define two major clusters to which one is the terrestrial end-member and the other cluster is a gradient associated with increasing geothermal influence defined by elevated Li, B, Ni, Rb, Cs, Ba, Si, Mn, Fe, and As concentrations, low Br/Cl (~160), and low 𝛿2H/Cl. The elevated metal concentration is consistent with mineral leaching due to hot and acidic geothermal fluids, which cannot be attributed to groundwater as these were not elevated in groundwater samples. The low Br/Cl ratio signifies the influence of fresh groundwater since Br is depleted in such environments. The mixing of fresh groundwater, geothermal fluids, and ambient seawater forms a gradient that can be resolved by the 𝛿2H/Cl mixing line.
OS04-A039
Prospecting Seepage Sources of Submarine Groundwater Discharge and Nutrients Using Thoron (Radon-220)
Peter Paul BUCSIT1#+, Marmelou POPES2, Ann Elizabeth ENOVA1, Mishel Valery RANADA1, Caroline Marie JARAULA1
1University of the Philippines, Philippines, 2University of the Philippines Diliman, Philippines
Submarine groundwater discharge (SGD) is a conduit for water, nutrients, and other materials from land to the coastal environment that can influence water quality, biogeochemical cycling, and marine biodiversity. This study delves into Mabini and Tingloy in Batangas, a hydrothermally active region, located within the globally significant Verde Island Passage (VIP), renowned for its marine biodiversity and its marine protected areas. Utilizing the unique properties of the short-lived isotope thoron (Rn-220), and using RAD7 (Durridge, Inc.), a commercially available instrument, our primary objective is to pinpoint SGD seepage points and evaluate their impact on nutrient dynamics. Thoron, with its abundance in groundwater and short half-life of 56 seconds, emerges as a potential tracer, enabling the identification of specific point sources of SGD. By utilizing the RAD-AQUA accessory of RAD7, thoron concentrations of 110.06 to 160.60 Bq/m3 and 108.81 to 119.56 Bq/m3 were detected in the coastal areas of Brgy. Mainit, Mabini and Brgy. Gamao in Tingloy, Batangas, respectively. Both sites are known SGD sites that exhibit distinct bubble emanations from the seafloor which is indicative of hydrothermally-induced submarine groundwater discharge (HISGD). Concurrently, nutrient analyses of bottomwater samples from these sites show elevated silicate levels of 510.33 μM, hinting at a potential correlation between groundwater discharge and nutrient enrichment. Moreover, initial data from previously unexplored sites show significant thoron concentrations of 306.1 Bq/m3 and 112.7 Bq/m3 in coastal areas of Mabini and Tingloy, Batangas, signifying the possible occurrence of other point sources of SGD in these areas. The results of this study highlight the usefulness of thoron isotope as a prospecting tool for SGD, especially in ecologically important regions such as Verde Island Passage where it may stimulate collaborative and interdisciplinary research projects.
OS05-A004
Response of the Indian Ocean Meridional Overturning Circulation to the Subtropical Indian Ocean Dipole
Linfang ZHANG#+
Sun Yat-sen University, China
Using the GECCO3 reanalysis data, this work explores the Indian Ocean Meridional Overturning Circulation (IMOC) variability and mechanism during the mature phase of the subtropical Indian Ocean dipole (IOSD). The IMOC is decomposed into the Ekman component, geostrophic component, external mode and residue. The IMOC exhibits counterclockwise circulation anomaly in 0 - 30°S during the mature phase of the IOSD. While the Ekman component dominates in 10°S - 30°S, the geostrophic component prevails in 5°S - 20°S. During the mature phase of the positive IOSD events, while an anticyclonic wind anomaly over the southern Indian causes a convergence and sinking of the sea water near 30°S, a cyclonic wind field anomaly near 10°S induces a divergence and rising, causing a counterclockwise Ekman component anomaly in 10°S - 30°S. The geostrophic component anomaly in 5°S - 20°S is caused by the sea level anomaly (SLA) gradient around 10°S associated with the sea water temperature anomaly (STA). Low SLA in the west corresponds to cold STA, induced by upward vertical velocity anomaly from the cyclonic wind near 10°S. In the east, high SLA associates with warm STA due to downward velocity anomaly caused by westerly wind anomaly along the Java coast blocking the Indonesian Throughflow (ITF). Further Parallel Ocean Program (POP2) experiments confirmed that the Ekman component anomaly primarily responds to the wind field of the mature phase of the IOSD, and further revealed that the geostrophic component anomaly is affected by the wind field of both the developing and mature phases of the IOSD.
OS05-A007
The Role of Intra-seasonal Variability in the Summer Counter-wind Current Along South Sri Lanka Coast
Weiqiang WANG1#+, Qiang XIE1, Arulananthan K 2, Kang XU1, Hongyu XIN3, Weiqing HAN4
1Chinese Academy of Sciences, China, 2National Aquatic Resources Research and Development Agency, Sri Lanka, 3Chinese Academy of Sciences, Brazil, 4University of Colorado Boulder, United States
The spatiotemporal characteristics of the south Sri Lanka coastal current (SSLCC) during summer are examined in this study. Climatologically, the SSLCC flows eastward as a part of the southwest monsoon current (SMC) during summer. However, westward SSLCC occurred lasting more than 20 days in the summer of 2013, 2016, 2017, and 2018 based on the reanalysis data, implying significant interannual variability of the SSLCC. The analysis on the summer extreme westward SSLCC indicates that the intra-seasonal wind associated with atmospheric boreal summer intra-seasonal oscillation (BSISO) is the main factor leading to the westward SSLCC. Firstly, the northward propagation of the BSISO induces the westerly wind anomaly and positive wind stress curl anomaly along the south coast of Sri Lanka, which induces the westward SSLCC. Secondly, driven by equatorial Indian Ocean intra-seasonal wind, the low sea level anomaly associated with upwelling Rossby wave reflected from the west coast of Sumatra Island propagates westward. This propagation significantly influences the cyclonic circulation off the south coast of Sri Lanka, thus facilitating the occurrence of the westward SSLCC. The relative contributions of above two mechanisms are quantified using the reanalysis data and a simple linear, continuously stratified (LCS) ocean model. It reveals that the intra-seasonal wind forcing from southern Sri Lanka, equatorial Indian Ocean, and southern Bay of Bengal (BOB) are responsible for the westward SSLCC (on intra-seasonal timescale), contributing 53%, 30%, and 17% of the intra-seasonal westward SSLCC magnitude, respectively.
OS06-A002
Observations on Subantarctic Mode Water and Its Spatial and Temporal Variability in the Southwest Indian Ocean
Somang SONG+, Sunghyun NAM#
Seoul National University, Korea, South
The Southwest Indian Ocean (SIO) is an important region in terms of climatic dynamics due to its tight links to unique weather, climate patterns, biogeochemistry, fisheries, and ecosystems within and beyond the Indian Ocean. However, there are not many studies exploring the physical properties of water masses and their spatio- temporal variations, primarily due to lack of in-situ time-series observations. In this study, we present recent observational results obtained from six research cruises (2017, 2018, 2019, 2021, 2022, and 2023) across the SIO (5°N-27°S, 55-67°E) and from a subsurface mooring initially deployed in May 2019 and constantly operated at the center of the Seychelles-Chagos Thermocline Ridge (SCTR; 8°S, 61°E). One striking feature is a trace of Subantarctic Mode Water (SAMW) from the observed vertical oxygen maximum (~400m), existing between two oxygen minimum layers. SAMW is known to be formed along the Subantarctic Front from the western to the eastern Indian Ocean but not extending quite to the SCTR region until now. In addition to the finding, the study investigates spatial, interannual, and seasonal variability in properties of SAMW in the SIO, utilizing temperature, salinity, density, dissolved oxygen, potential vorticity, and isopycnal layer thickness using ship-based in-situ hydrographic and mooring data collected for six years (2017–2023). Preliminary findings on spatio-temporal variations of SAMW properties, among a few water masses, in the SIO contribute to our understanding of climate dynamics and offer insights into biogeochemical and ecological implications for marine ecosystems.
OS06-A008
Strong Suppression of the Upwelling at the Seychelles-Chagos Thermocline Ridge in December 2019 and Its Relationship to the Positive Indian Ocean Dipole
Eunsun LEE#+, Hanna NA, Sunghyun NAM
Seoul National University, Korea, South
The Seychelles-Chagos Thermocline Ridge (SCTR) is a prominent upwelling region in the southwestern tropical Indian Ocean, resulting from the southeast trade winds and the Indian monsoon winds. A Pressure-recording Inverted Echo Sounder (PIES) observed the acoustic travel time (tau) and bottom pressure at Station K (61˚E, 8˚S) in order to understand the SCTR upwelling variability from May 2019 to December 2021. The tau exhibited a minimum value in December 2019, and it was the lowest compared to those estimated from the historic hydrographic profiles for 16 years (2006–2021). The observed time series of tau was converted to the time series of vertical temperature profiles based on the relationship between tau and temperature. The converted vertical temperature profiles in December 2019 showed particularly warmer characteristics in the upper 300 m, which indicates strong suppression of the SCTR upwelling. Further analysis suggests that the suppression was linked to the westward propagation of the downwelling Rossby waves related to the prolonged and strong positive Indian Ocean Dipole (IOD). The positive IOD continued for seven months (May–November) with a relatively strong amplitude (maximum of 1.12 oC exceeding the three standard deviations), generating stronger positive wind-stress curl anomalies in the eastern Indian Ocean, which contributed to stronger downwelling Rossby waves. This study presents that the strong suppression of the SCTR upwelling in December 2019 was induced by the prolonged and strong positive IOD.
OS06-A014
Ecological Dynamics and Vertical Distribution of Mesozooplankton in the Upper 1,000m of the Seychelles-Chagos Thermocline Ridge During the 2018 Spring Intermonsoon
Minju KIM+, Suyun NOH, Dong-Jin KANG, Jung-Hoon KANG#
Korea Institute of Ocean Science & Technology, Korea, South
The vertical distribution of the mesozooplankton community in the upper 1,000 m was investigated in the open-ocean upwelling region known as Seychelles-Chagos Thermocline Ridge(SCTR) during the spring intermonsoon of 2018. The survey was conducted along two transects, 60°E and 67°E, from 3°S to 12°S, at 7 depth layers using the Multiple Opening/Closing Net and Environmental Sensing System. The total abundance of mesozooplankton decreased sharply with depth in all surveyed stations. The depth strata of surface to surface mixed layer(SML) at 8°S of 60°E–transect, and SML to pycnocline layer at 9°S of 67°–transect showed the highest abundance of mesozooplankton. Notable mismatches were observed between the peaks of mesozooplankton and chlorophyll-a(chl-a) concentrations, with chl-a showing relatively lower concentrations while the abundance of mesozooplankton was highest at 60°E, 8°S, and the opposite pattern was observed at 67°E, 12°S. The higher abundance of mesozooplankton in the 60°E–transect may be mainly attributed to surface convergence caused by a large anticyclonic eddy with relatively cooler temperatures in the surface mixed layer. Conversely, the strong westward south equatorial current may have led to a lower abundance of mesozooplankton at 67°E, 12°S. The differences observed between mesozooplankton abundance and chl-a concentrations highlight the intricate nature of trophic interactions and the significance of a nuanced understanding of the underlying mechanisms governing these relationships. Insights like these are essential for predicting and managing the effects of environmental changes on marine ecosystems. They provide valuable information for conservation and sustainable resource management efforts in the SCTR.
OS06-A015
Estimation of Spatio-temporal Variations of Particulate Organic Carbon in the Western Indian Ocean Based on In-situ Measurement and MODIS-Aqua
Sujin KANG+, Suyun NOH#, Yeseul KIM, Dong-Jin KANG
Korea Institute of Ocean Science & Technology, Korea, South
Understanding the distribution of particulate organic carbon (POC) in the marine environment is crucial for comprehending the ocean's role in storing and absorbing CO2. Phytoplankton in the surface ocean capture atmospheric carbon, fueling the biological carbon pump and influencing the dynamics of suspended marine POC. The Seychelles-Chagos Thermocline Ridge (SCTR) in the western Indian Ocean is an upwelling region that enhances biological productivity. Despite its significance, the spatial and temporal limitations of in-situ measurements of the POC in the western Indian Ocean are prompting the application of satellite-based POC estimation. To estimate surface POC concentrations, we analyzed POC concentrations during the Indian Ocean cruises in 2022 and 2023, and compiled the published POC data in the Indian Ocean, with average POC concentration values ranging from 34.0 to 71.0 mg m-3. Then, the surface POC concentrations were estimated using an empirical algorithm based on in-situ measured POC concentrations and reflectance of the MODIS-Aqua satellite data. Strong seasonal and interannual variability of the POC was found in the SCTR region (5°S-8°S, 50°E -60°E), except for coastal areas such as the Bay of Bengal and Arabian seas. This study presented here examines the spatio-temporal variations of the POC and aims to understand their association with the Indian Ocean Dipole (IOD).
OS06-A017
Latitudinal Characteristics of Mesozooplankton Communities in Neutral IOD Phase in the Western Indian Ocean Along 65°E
Hyeon KIM+, Minju KIM, Jung-Hoon KANG#
Korea Institute of Ocean Science & Technology, Korea, South
To understand the latitudinal characteristics of mesozooplankton communities along the meridian line (19︒S-2︒N, 65︒E), mesozooplankton samples were collected with a Multinet from surface to 1,000 m in five depth strata during daytime at four stations in the western Indian Ocean. The Indian Ocean Dipole index was almost in a near-neutral negative phase (-0.7 ~ -0.2) during this period. At 8︒S, the Seychelles-Chagos Thermocline Ridge (SCTR) was characterized by relatively lower temperatures and high chlorophyll-a concentrations at 50 m. Freshwater input was observed in the surface layer at 2︒N located in the Southwest Monsoon Current, with high chlorophyll-a at 50 m. A total of 110 mesozooplankton species were identified. The abundance of mesozooplankton in the 0-1,000 m water column ranged from 970 to 1,925 inds./m3 and was relatively higher at 8︒S and 2︒N. The majority of mesozooplankton was concentrated in the surface mixed layer and thermocline, and drastically declined below the thermocline. Copepods dominated the mesozooplankton community, accounting for 52~70% of total abundance. Paracalanus copepodites were the most common copepod across all stations. Other predominant groups included dinoflagellates, rhizarians, molluscs and ostracods. The mesozooplankton community structure exhibited significant latitudinal variations, in which, Canthocalanus pauper and Paracalanus parvus s.l were particularly abundant at 8︒S, while Pontellina plumata, Subeucalanus mucronatus and Temora discaudata were minority species that appeared only at 2︒N. A higher abundance of gastropod larvae occurred at 19︒S which coincided with the South Equatorial Current. The abundance of gastropods decreased, while Pyrocystis noctiluca increased northwards. Temperature, salinity, density and dissolved oxygen was found to explain 55.7% of the latitudinal variations in the mesozooplankton community. Latitudinal characteristics of mesozooplankton community were characterized by two controlling factors: currents (19︒S and 2︒N) and the SCTR (8︒S).
OS06-A019
The Potential Threat of Microplastics to Mesozooplankton in the Surface Mixed Layers of the Western Indian Ocean
Jung-Hoon KANG#+, Minju KIM, Dong-Jin KANG
Korea Institute of Ocean Science & Technology, Korea, South
The potential impact of microplastics to mesozooplankton and planktivores was assessed by measuring the ratio of microplastics to zooplankton by abundance in the western Indian Ocean. Microplastics and mesozooplankton (0.2 – 5 mm) were collected in the surface mixed layers (mean: 55 m) at 11 stations between 5°N and 16°S along 67°E using Multiple Opening and Closing Nets and Environmental Sampling System. Microplastics were detected at all of the 11 sampling stations, and classified into four types (fragment, paint particles, fiber, and film). The abundance of microplastics ranged from 0.05 to 0.53 particles m-3 (mean: 0.23±0.04 particles m-3). The dominant shape and polymer type of microplastics were fiber (mean: 70.5%), and mainly polyester (mean: 50.0%). The abundance of mesozooplankton ranged from 541 to 2,278 inds. m‑3 (mean: 1,252 inds. m‑3), in which the dominant taxa were copepods (adult and immature mean: 61.2%), Noctiluca scintillans (mean: 13.0%), and foraminiferans (mean: 8.4%). The mean ratios of microplastics to mesozooplankton were from 0.00005 (station 6°S) to 0.00043 (station 2°S) (mean: 0.00020), indicating that mesozooplankton may be more likely to encounter microplastics than natural preys in station 2°S. The dominant species in station 2°S was N. scintillans (mean 19%). N. scintillans are bioluminescent dinoflagellates that are phagotrophic and feeds on variety of organisms including diatoms, bacteria, detritus, protozoa, copepods, and eggs. The high ratio of microplastics to mesozooplankton implies that a relatively high number of microplastics may be mistaken to zooplanktivores for natural prey(food), indicating the increased level of potential contamination for consumers.
OS06-A020
Factors Controlling Nitrate Isotope Ratios of the Seychelles-Chagos Thermocline Ridge in the Southwestern Indian Ocean
Seonghee JEONG1+, Doshik HAHM1#, Dong-Jin KANG2, Tae-Keun RHO2, Sujin KANG2, Purena SON2, Tongsup LEE1
1Pusan National University, Korea, South, 2Korea Institute of Ocean Science & Technology, Korea, South
The Seychelles-Chagos Thermocline Ridge (SCTR) is a highly productive region in the Indian Ocean due to year-round upwelling. To understand the nitrogen cycle, we analyzed nitrate isotopes (δ15N, δ18O) in the Indian Ocean (60-68ºE, 4-12ºS), which includes the SCTR, using the Titanium reduction method. In the upper layer (≤150m), we observed discernible differences in nitrate isotopes between SCTR and non-SCTR. In the non-SCTR (south of 12ºS), characterized by oligotrophic conditions, the δ15N (δ18O) was 6 (3‰). SCTR had higher values, ranging from 7-15 ‰ for δ15N and 4-15 ‰ for δ18O. These elevated isotopic ratios are likely due to the preferential consumption of lighter isotopes during the assimilation of upwelled nitrate. In non-SCTR, where no significant upward nitrate input exists, there was no noticeable increase in the isotopic ratio. In the intermediate layer, nitrate concentration increased with depth, while δ15N remained almost constant at an average of 6.8±0.6‰. This similarity to organic matter δ15N (6.5‰) suggests that remineralization is important in determining the nitrate isotope ratio in the intermediate layer. Inflows of water masses appeared to impact certain isotopic ratios in the intermediate layer. In the northern area, at ~750 m, the highest intermediate δ15N (δ18O) was 8.2 (4.8‰). This is believed to be due to the inflow of Red Sea Water, which has high isotopic ratios due to denitrification occurring in an anoxic environment. In the southern area, 100-300 m, δ15N and δ18O were both over 7 and 4‰. The influence of Sub-Antarctic Mode Water, which has a high nitrate isotopic ratio due to fractionation by assimilation, was attributed to this. The δ15N (δ18O) in the bottom layer (>2500m) was 5(2.5‰), which was the lowest among the study region. This seemed to be due to the inflow of Circumpolar Deep Water, which has low isotopic ratios because of the remineralization.
OS07-A003
High-frequency Salinity Oscillations Observed from the Ieodo Ocean Research Station and Surface Drifters in the Northern East China Sea
Jungmin KIM+, Young-Gyu KIM, Sunghyun NAM#
Seoul National University, Korea, South
High-frequency (hours to one day) oscillations of salinity as well as sea surface temperature, surface current, subsurface temperature and mixed layer and thermocline depths, are crucial for better understanding vertical mixing and stratification, and ocean-atmosphere exchanges of heat, freshwater, and momentum. However, our comprehension of such high-frequency salinity oscillations in many seas remains challenging, primarily due to limitations in observational capabilities. In this presentation, we will provide recent observational results obtained from analyses of time series observed by moored and deployed sensors and deployed sensors at the Ieodo Ocean Research Station (I-ORS) and five satellite-tracked surface drifters deployed nearby the station in the northern East China Sea (in the vicinity of the diurnal critical latitude). We analyzed the I-ORS time series data of salinity and temperature observed at seven depths (3, 8, 11, 17, 21, 30 and 38 m) from May 10 to July 26, 2023, and sea surface salinity and temperature observed from the surface drifters deployed in July 10, 2023. Results reveal several processes, including clockwise-rotating diurnal-inertial resonant motions, semidiurnal internal tidal motions, and motions at higher tidal harmonics, underlying the high-frequency oscillations. Regular spring-neap cycles of diurnal and semidiurnal motions of tidal origin are found from vertical oscillations of isohaline, isotherm, isopycnal, mixed layer and thermocline depths, and horizontal (tidal) ellipses of surface motion, while intermittent amplifications of diurnal-inertial motions of wind origin are also observed. This study provides significant insights into high-frequency oscillations of salinity and other key physical parameters in the upper ocean and implications for turbulent mixing of both tide and wind origins, and ocean-atmosphere interaction processes.
OS07-A006
Zonal Structure of Tropical Pacific Surface Salinity Anomalies Affects the Eastern and Central Pacific El Niños Differently
Cong GUAN#+
Hohai University, China
Maximum sea surface salinity (SSS) anomalies are found in the central Pacific during the eastern Pacific El Niño (EPEN) and located further westward during the central Pacific El Niño (CPEN), but whether these affect the two events remains unclear. By performing ocean general circulation model experiments by modifying freshwater flux anomaly, we found salinity effects on surface warming during both types are highly sensitive to zonal locations of SSS anomalies, with the strongest warming induced by the SSS anomalies near the international dateline. Further analysis reveals that vertical mixing and entrainment dominate this temperature sensitivity, with the strongest response to SSS anomalies occurring in the central Pacific. The central-Pacific SSS anomalies increase the EPEN warming by 0.15℃ while the westward-located SSS anomalies make little contribution to the CPEN. Therefore, the distinctly zonal structures of SSS anomalies facilitate stronger EPEN than the CPEN, increasing their difference in intensity by about 10%.
OS07-A008
Impact of the Changjiang River Plume on Physical and Biogeochemical Responses in the East China Sea
So-Young KANG1+, Jae-Hong MOON1#, Taekyun KIM1, Chanhyung JEON2, Yuhe Tony SONG3
1Jeju National University, Korea, South, 2Pusan National University, Korea, South, 3California Institute of Technology, United States
This study investigated how freshwater discharged from Changjiang impacts the physical and biological responses and oceanic uptake of carbon dioxide (CO2) in the East China Sea by combining the sea surface salinity (SSS) product from the Soil Moisture Active Passive (SMAP) mission with other satellite measurements of sea surface temperature (SST) and chlorophyll-a (chl-a) concentration. The partial pressure of CO2 (pCO2) and its interannual variability were also estimated using an empirical regression with satellite-derived environmental variables. The bias-corrected SMAP SSS revealed that river discharge largely contributed to distinct interannual variations, with a seasonal evolution of sea-surface freshening. Compared to the SST and chl-a anomalies, we observed an enhancement of SST warming and primary production in the region where sea-surface freshening was robust. Simultaneously, the pCO2 was relatively low in the region where the SST and primary production were high. These results highlight that the heat and riverine nutrients trapped within the buoyant plume contributed to the sea-surface warming and chl-a enrichments, thereby leading to a drawdown of pCO2 by biological uptake. The estimates conducted here illustrate the synergistic utility of multiple satellite measurements for the evaluation of CO2 uptake capacity, complemented by in situ measurements of river-dominated marginal seas.
OS08-A002
Low-frequency Variability and Projected Changes of Dynamic Sea Level in the Maritime Continent
Peifeng MA1,2#, Nidheesh GANGADHARAN3, Pavel TKALICH2+
1Technology Centre for Offshore and Marine Singapore, Singapore, 2National University of Singapore, Singapore, 3Centre for Climate Research Singapore, Singapore
Coastal zones in the Maritime Continent are one of the most vulnerable regions in the world to sea-level rise and related hazards. Rate of regional sea-level rise often deviates from global-mean rate partly due to ocean circulation which redistributes water mass, salt, and heat non-uniformly within the ocean. Current global general circulation models (GCMs) are mostly not efficient to resolve regional ocean circulation and boundary currents due to their coarse resolution; therefore, dynamical downscaling of the global GCMs to regional scales using high-resolution ocean models is widely considered as an efficient solution to derive regional sea-level change projections. In this study, an eddy-resolving regional ocean model (NEMO) is used to dynamically downscale projected sea-level changes from a global climate model (EC-Earth) for SSP2-4.5 and SSP5-8.5 scenarios in the Maritime Continent region, covering the South China Sea (SCS) and other Southeast Asian Seas (SEAS). As a novel approach, we employ WRF-based downscaled atmospheric fields from the same parent model (EC-Earth) at the surface boundary for the ocean model projections. The low-frequency dynamic sea-level variability and relevant mass redistribution processes computed by prevailing climate modes in the region are discussed further. This Research is supported by Singapore’s National Research Foundation and National Environment Agency under the National Sea Level Programme Funding Initiative (Award No. USS-IF-2020-4).
OS08-A008
Comparative Review of Coastal Vulnerability for Climate Adaption in Korea
Dongseob SONG#+
Kangwon National University, Korea, South
Greenhouse gas emissions, which began to increase before the industrialization era, are continuously increasing, and future sea levels are expected to rise steeply compared to the past. The predicted sea level rise at the end of the 21st century based on the current sea level rise rate in Korea is higher than the world average, it will be difficult to guarantee the stability of Korea's sandy beaches. In order to preserve coastal areas damaged by continuous coastal development and use, sea level rise, typhoon invasion, and increased wave intensity, a coastal vulnerability assessment system is important to adapt to climate change. Approaches of coastal vulnerability assessment have been developed over the past several decades in the fields of coastal hazards such as typhoon, coastal erosion, swell, rip current and sea level rise, and it have been provided best methods for use in strategy of climate change vulnerability and adaptation. In Korea, the coastal disaster impact index is calculated and used to assess vulnerability to coastal disasters. The coastal disaster impact index consists of the coastal disaster exposure index and coastal sensitivity index. Based on the coastal disaster impact index, adaptation and response measures for each indicator, which is the lowest level, are being established in detail from level 1 to level 5 for each detailed administrative district. In this study, we reviewed the currently operating coastal disaster vulnerability assessment system and compared it with the cases of developed countries to examine areas that require supplementation in coastal disaster vulnerability assessment. Acknowledgement: This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2023-00280850).
OS08-A013
Investigating the Influence of IOD and ENSO on Sea Level Rise in Southeast Asia Using Satellite Altimetry
Eko HANDOKO1, Candida A. D. S. NUSANTARA1, Widodo Setiyo PRANOWO2,3, Joana FERNANDES4, Clara LÁZARO4, Tanghua LI5#+, Benjamin HORTON6,7
1Institut Teknologi Sepuluh Nopember, Indonesia, 2National Research, and Innovation Agency, Indonesia, 3Indonesia Naval Postgraduate Military Service School, Indonesia, 4Universidade do Porto, Portugal, 5Nanyang Technological University, Singapore, 6City University of Hong Kong, Hong Kong SAR, 7Imperial, United Kingdom
The Southeast region is an oceanic region characterized by considerable complexity due to the impact of the Pacific Ocean in the east and the Indian Ocean in the southwest. The El Niño-Southern Oscillation phenomena, occurring in the Pacific Ocean, affects the sea in the southeastern area. Furthermore, the Indian Ocean Dipole phenomenon in the western section of the southeast region also has a significant influence on the seas of the southeast region. This study proposes to investigate the impact of the Indian Ocean Dipole and El Niño-Southern Oscillation on the rise in the sea level in the Southeast Asia region. It will employ multi-satellite altimetry data spans over a period of 25 years to analyse the changes in sea levels and their associations.
OS08-A014
Coastal Evolution of Southern Singapore Since the Last Glacial Maximum: Evidence from High-resolution Geophysical Data
Stephen CHUA1#+, Abang Mansyursyah Surya NUGRAHA1, Andrew GREEN2, Uri SCHATTNER3, Doug SLOGROVE2, Yu Ting YAN1, Adam SWITZER1, Benjamin HORTON4,5
1Nanyang Technological University, Singapore, 2University of KwaZulu-Natal, South Africa, 3University of Haifa, Israel, 4City University of Hong Kong, Hong Kong SAR, 5Imperial, United Kingdom
Global mean sea level has fluctuated by > 100 m over glacial and interglacial cycles. The most recent sea level lowstand was during the Last Glacial Maximum (LGM) approximately 22,000-18,000 years ago when sea levels were 120 m below present levels. Such large sea-level changes have profound impacts upon the low relief Sunda Shelf, which was most recently inundated during the marine transgression 18,000-5,000 years ago. Previous studies have shed light on palaeogeography of the outer and middle shelf since the LGM, but little is known of the palaeogeographical evolution of the inner shelf. Singapore lies at the core of the tectonically-stable Sundaland and provides an excellent location to study coastline evolution since the LGM. We conducted a comprehensive geophysical survey of the Singapore Strait that included both multibeam bathymetry and high-resolution single-channel seismic (boomer) profiles. Here, we present a coastal evolution reconstruction of the eastern Singapore Strait since the LGM, constrained by seismic profiles where pre- and post-LGM sedimentary units have been identified and mapped. Chronology is inferred from the existing terrestrial borehole-derived stratigraphic model by matching chronohorizons offshore. Our stratigraphic record consists of five major strata that are bounded by two clear unconformities representing subaerially-exposed palaeosol formed during past marine lowstands (i.e., LGM (MIS2) and MIS 6). The coastline of Southern Singapore, prior to postglacial transgressions, extended up to 5 km beyond the modern coastline and was characterized by a low gradient coastal plain juxtaposed with large palaeochannels and a shallow foreshore. These incised palaeochannels were infilled rapidly as sea levels rose after the LGM, producing an embayment in the western sector and a broad estuarine environment in the central sector. Our results, derived from the first geoscientific survey in the inner Sunda Shelf, provide the first coastal evolution model of Southern Singapore from LGM to present.
OS08-A018
Foraminifera Environmental DNA as a Novel Proxy to Reconstruct Past Sea Level from Mangrove Environments in Peninsula Malaysia
Wenshu YAP1#+, Timothy SHAW1, Behara SATYANARAYANA2, Tanghua LI1, Jedrzej MAJEWSKI1, Jennifer WALKER3, Mohd Fadzil MOHD AKHIR2, Yun Fann TOH1, Abang Mansyursyah Surya NUGRAHA1, Adam SWITZER1, Benjamin HORTON4,5
1Nanyang Technological University, Singapore, 2Universiti Malaysia Terengganu, Malaysia, 3Rowan University, United States, 4City University of Hong Kong, Hong Kong SAR, 5Imperial, United Kingdom
Reconstructing past sea level in tropical mangrove environments often presents a challenge due to the poor preservation of microfossil tests including foraminifera. Here we explore the utility of foraminifera environmental DNA (eDNA) as a novel proxy for reconstructing sea level from sediments collected from the Matang Mangrove Forest Reserve, Peninsula Malaysia. Following an extensive field reconnaissance, we collected a 3 m core from the upper intertidal environment and modern surface samples across an intertidal-to-mangrove gradient with all sites surveyed relative to Malaysian national geodetic benchmark. We analyzed all samples for organic content, enumerated raw foraminiferal counts and also extracted foraminifera eDNA. By combining both eDNA metabarcoding with traditional microfossil count analyses, we gained insights into foraminifera communities in both modern and fossil environments to provide indicative meanings constraining the vertical uncertainty of mangrove sea level index points. We constrained core sample ages through Accelerator Mass Spectrometry radiocarbon dating of fine fraction sediments. We show core foraminiferal tests preserved throughout organic mangrove peats (~50%) and dominated by typical agglutinated taxa including Arenoparrella mexicana and Trochammina inflata. eDNA analyses yielded an average of 46,921 sequences representing 170 amplicon sequence variants (ASVs) and a diverse community dominated by monothalamous (single-chambered) taxa, such as Vellaria, Allogromia, and Hippocrepinella, that are often poorly preserved. Preliminary results from radiocarbon dating reveal in sequence ages approximately ~2000 years old. Multivariate analyses show distinct community composition between mangrove peats and intertidal marine muds that highlights the potential of eDNA’s to identify past environmental changes and constrain indicative meanings of mangrove peats where raw foraminiferal test might not be preserved. This Research/Project is supported by the National Research Foundation, Singapore, and National Environment Agency, Singapore under the National Sea Level Programme Funding Initiative (Award No. USS-IF-2020-1).
OS08-A020
The Sea Level Changes in South China Sea from Tide-gauge Records and Satellite Data
Fang ZOU1+, Chuang XU1, Guangyu JIAN1, Zhanhui HU1, Robert TENZER2#
1Guangdong University of Technology, China, 2The Hong Kong Polytechnic University, Hong Kong SAR
The importance of studding the sea level change (SLC) in South China Sea is emphasized by factors related to high population density, intensive urban and industrial development, particularly along the coast that involves a considerable land reclamation. To address this issue, we investigate spatiotemporal characteristics of the SLC in territories by analyzing tide-gauge records (TG) collected over the period between 1954 and 2019 and satellite-altimetry (SA) data from 1993 to 2019. The application of the ocean tide and inverted barometer corrections to TG data substantially decreased uncertainties in estimated rates of SLC by achieving a submillimeter accuracy. The SLC rates detected at six tide-gauge stations vary significantly even within this relatively small coastline. According to our estimates, the annual rates vary between 0.32±0.51 and 4.19±0.46 mm/yr from 1997 to 2019. These large differences are related to different pattern of ocean currents and the fresh water discharge in the Pearl River Estuary. The EOF analysis confirms the expected increasing rising in SLC, with two anomalous periods during 2002-2003 and 2015-2016 that are likely attributed to the El Niño-Southern Oscillation (ENSO). Our results indicate that SLCs is positively correlated with ENSO index and ENSO precedes several months (normally 5 months) the inter-annual SLC. The analysis of the GPS trends reveals a prevailing subsidence in territories, which aggravate the relative SLC estimates. Our results show that between 1997 and 2019 the absolute sea level raised at the annual rate of 3.17±1.56 mm/yr (when using the GPS+TG) and 2.88±0.59 mm/yr (when using SA observations).
OS08-A021
Heat and Momentum Effects on the Sea Level in the Yellow and East Seas from 1993 to 2021
MyeongHee HAN#+, Yeon S. CHANG, Jeseon YOO, Hak Soo LIM
Korea Institute of Ocean Science & Technology, Korea, South
The largest sea level difference between the Yellow Sea (YS) and the East Sea (ES; Sea of Japan) was observed in September (16.05 cm), whereas the smallest monthly average was found in December (1.84 cm) in the 29-year mean (1993-2021). In September, the sea level change (SLC) of absolute dynamic topography (ADT)was 1.93 cm in the YS and 2.49 cm in the ES. In December, the SLC of ADT was –4.88 cm in the YS and –3.65 cm in the ES. Using the ERA5 reanalysis data, the SLC by atmospheric sea surface net heat flux could be calculated as it was –0.54 cm in the YS and –0.32 in the ES in September, and –2.57 cm in the YS and –3.84 cm in the ES in December. Considering that the atmospheric and land effects by precipitation, evaporation, and runoff could be ignored, the rest of the SLC in each month might be contributed by the oceanic effect (i.e. ocean heat and mass transport divergences). The results indicated that the oceanic effect significantly raised the sea level in both YS (2.47 cm = 1.93 – (–0.54)) and ES (2.81 cm = 2.49 – (–0.32)) in September, whereas the atmospheric heat effect significantly lowered the sea level in the ES (–3.84 cm) because the oceanic effect was only 0.19 cm (= –3.65 – (–3.84)) in December. To analyze the oceanic effect that contributed to the SLC, the correlation between MSL and wind stress was investigated, indicating that the Ekman transport as an oceanic effect caused by wind stress could be one of the controlling factors contributing to the SLC in both September and December. The results require further quantitative analysis based on observations to investigate the oceanic and atmospheric effects on the SLC in the study regions as for future studies.
OS09-A001
Extreme Winter Events in the Subtropical Northern South China Sea
Pei-Yu FU#+, Yung-Yen SHIH, Yen-Tu LI, Yun-Zhen CHANG
Republic of China Naval Academy, Taiwan
The negative phase of Arctic Oscillation (AO) weakens Arctic westerly winds, allowing cold air to move to mid latitudes and even extend southward. However, the impact of cold air (negative AO) on marine biogeochemistry in low-latitude waters is still unclear. This study utilized marine biogeochemical data from cruises conducted during the winter from November to March between 2018 and 2023, to investigate the impact of extreme winter weather events on biogeochemical processes in low-latitude waters of northern South China Sea. It evokes higher phytoplankton biomass, carbon fixation rates, and particulate organic carbon export fluxes under pronounced negative AO level in winter. This is attributed to intense cold air causing the nutrients-rich subsurface water mixed well with surface water, stimulating phytoplankton growth, increasing marine biogeochemical cycling, and reducing carbon retention time (RT) within the euphotic zone, thus improving carbon removal from the upper to the deeper ocean.
OS09-A005
Differences in the Carbon Flux of Microbial Communities Between Seagrass and Unvegetated Incubations
Wei Yi Chen PATRICHKA+, An Yi TSAI#, Madeline OLIVIA
National Taiwan Ocean University, Taiwan
A seagrass meadow is one of the most important ecosystems in the world in terms of both its economic and ecological importance. Seagrass beds, which dominate primary production and contribute to secondary productivity, are another important characteristic of this ecosystem. There is no doubt that seagrass ecosystems are one of the most significant natural carbon sinks on earth, due to the fact that they are able to sequester significant amounts of carbon, store it as organic carbon for long periods, and are capable of occurring worldwide. The general conceptual framework emphasizes the importance of resource competition (nutrients) for the interaction between seagrasses and phytoplankton, yet direct interference also constitutes resource competition. In addition, the microbial loop (consuming bacterial biomass by grazers and using seagrass derived detritus by bacteria) may be an important mechanism for transferring seagrass-derived organic matter to aquatic food chains. Our study seeks to identify differences in carbon flux between seagrasses and unvegetated environments based on microbial communities. In unvegetated meadow and seagrass habitats, phytoplankton and bacterial growth and mortality were measured differently. According to this study, there was no significant difference in phytoplankton production between seagrass and unvegetated incubations at 28.2 and 27.4 mgC m-3d-1, respectively. Based on these, we estimated phytoplankton capturing carbon dioxide in the process at 90.7 and 91.3 mgC m-3d-1, respectively. Furthermore, the instantaneous growth rate of bacteria in seagrass habitats was 2.42 d-1, higher than that of unvegetated water. The carbon sources available for bacterial growth are mostly likely to come from two important sources in the seagrass meadow environment. During the photosynthesis process, DOC is released by seagrasses as the first step. Also during phytoplankton photosynthesis, another DOM is released extracellularly.
OS09-A007
Spatial Variations of Air-sea Gas Exchange of Carbon Dioxide in Tropical Western Pacific Surface Ocean During Typhoon Season
Veran WEERATHUNGA1+, Kai-Jung KAO1, Fei-Ling YUAN1, Wen-Chen CHOU2, Chin-Chang HUNG1, Wei-Jen HUANG1#
1National Sun Yat-sen University, Taiwan, 2National Taiwan Ocean University, Taiwan
The tropical western Pacific Ocean can play a crucial role in absorbing anthropogenic CO2, yet comprehensive studies on air-water CO2 gas exchange, particularly during the typhoon season (June to November) between 122 °E to 135 °E longitudes, are scarce. This study measured water surface pCO2 (at 5 m depth) and associated parameters such as water temperature and salinity from July 7th to 17th (Leg 1) and July 24th to August 3rd (Leg 2) in 2023. Leg 1 was conducted before the passage of two very strong typhoons over the western Pacific, namely Typhoon Doksuri (July 20th to 27th) and Typhoon Khanun (July 26th to August 1st), while Leg 2 took place following the passages of those typhoons. During Leg 2, significantly lower water temperatures (29.2 ± 0.4 °C) and higher wind speeds (14.2 ± 4.8 ms-1) were observed compared to those during Leg 1 (30.1 ± 0.2 °C and 9.2 ± 4.1 ms-1, respectively). Surface pCO2 was slightly lower during Leg 2 (382.6 ± 7.5 µatm) compared to Leg 1 (386.9 ± 5.9 µatm). Spatial pCO2 variation was mainly influenced by temperature changes, accounting for 44% and 72% during Leg 1 and Leg 2, respectively. The studied region of the tropical western Pacific Ocean acted as a strong sink of atmospheric CO2 (-7.2 ± 5.4 mmol m-2 d-1) after the passages of typhoons (Leg 2) and it was a weaker sink (-2.6 ± 2.5 mmol m-2 d-1) before the typhoons (Leg 1).
OS09-A008
What Small Phytoplankton Consume Bacteria? A Study Utilizing Acid Organelle Stains
Kuo-Ping CHIANG#+
National Taiwan Ocean University, Taiwan
Small phytoplankton have been reported not only as primary producers in the ocean but also as major grazers of bacteria. Global warming has led to an increase in surface seawater temperature, resulting in more stable ocean structures and significant seawater stratification. Therefore, surface phytoplankton are predicted to exhibit a more pronounced ability to capture energy through ingestion or to acquire the necessary nutrients for photosynthesis. Previously, observing phagocytosis in small pigmented eukaryotes under a microscope has been challenging. Furthermore, conducting prey addition experiments to study the composition of bacterivores is time-consuming. The purpose of this study is to use acid organelle stains to quickly determine the ingestion capabilities of small pigmented eukaryotes. Employing this method, the study examined the proportion of these eukaryotes with ingestion capabilities in the coastal waters of northeastern Taiwan. As a result, almost 55% of small pigmented eukaryotes exhibited positive responses to acid organelle stains, suggesting potential mixotrophy among groups such as chlorophytes, cryptophytes, stramenopiles and haptophytes. It should be noted that dinoflagellates and diatoms, which are known to produce nonlysosome fluorescence, were excluded from the analysis to avoid potential interference with the precision of this method. On the other hand, the heterotrophic eukaryotes identified here include MAST-1, 4, 7, 10, and Telonemia. This study provides information on bacterivores in the subtropical Pacific Ocean.
OS09-A013
Decoupling of High-resolution Surface PH and DO Reveals Biological Production Dynamic of the Changjiang Plume Waters
Dewang LI1#+, Bin WANG1, Hai-Yan JIN1, Yanyi MIAO1, Qianwen SUN1, Hongliang LI2, Feng ZHOU1, Jianfang CHEN2
1Ministry of Natural Resources, China, 2State Oceanic Administration, China
The stoichiometric ratio between seawater CO2 and dissolved oxygen (DO) during phytoplankton metabolism holds significant importance in assessing biogeochemical processes. We collected high-resolution underway data of temperature, salinity, DO, and pH in the inner shelf of the East China Sea during a cruise in May 2017. Our results showed high pH (8.4) and supersaturated DO (150%) in the outer Changjiang estuary. The DO and pH were significantly correlated, with a regression slope of 0.0029, which roughly followed the Redfield ratio. In contrast, a non-Redfield ratio manifested in a low-salinity patch on north of the Changjiang estuary, featuring a regression slope of 0.0088. The surface waters in the low-salinity patch displayed a pH of 8.5 and oxygen saturation of only 110%. The substantially faster air-sea equilibrium rate of O2 than CO2 probably caused such decoupling, which is used to assess the biological production dynamics. Theoretically, a greater regression slope implies an earlier onset of phytoplankton bloom. An end-member mixing model was constructed to estimate ΔDIC and ΔDO (sum of biological and air-sea exchange influences). Model results revealed that ΔDIC below −200 μmol kg−1 in the low-salinity patch, where ΔDO and Chl a were less than 50 μmol kg−1 and 2 μg L−1, respectively. We conducted a simulation to explore how air-sea exchanges modify the ΔDIC and ΔDO in surface plume waters. Results suggested that the biological signal of the decoupled waters likely preceded our observations by 7-10 days. Satellite results captured high-Chl a waters southwest of the low-salinity patch a week before our observation. Prevailing southwest winds were hypothesized to transport the high-Chl a waters to the north of the Changjiang estuary, during which Chl a decreased and oxygen diffused to the atmosphere.
OS09-A014
The Biological Responses Induced by the Dispersal of Changjiang Plume Waters and Upwelling Events Following Three Successive Typhoons
Yixuan TAO1+, Dewang LI1#, Xiaobo NI2, Bin WANG1, Hai-Yan JIN1, Feng ZHOU1, Jianfang CHEN2
1Ministry of Natural Resources, China, 2State Oceanic Administration, China
The dispersal of the Changjiang plume waters and upwelling/mixing of nutrient-replete bottom waters represent key processes influencing the biological production and blue carbon over the East China Sea. However, their impacts remain inadequately understood, particularly in the context of episodic events such as typhoon. In summer 2020, we deployed a buoy on the outer Changjiang Estuary to capture time-series data, including surface temperature, salinity, oxygen, Chl a, turbidity. During a series of successive typhoons—Bavi, Maysak, and Haishen—that traversed the East China Sea from 26 August to 6 September, substantial influences on hydrological and biogeochemical parameters were observed. Typhoon Bavi entered the middle East China Sea shelf on 25, resulting in a notable decrease in daily-average surface temperature from a maximum of 25.21 to 23.42°C between 24 and 26 August. Concurrently, salinity and turbidity increased from 28.00 to 29.47, and from 12.69 to 74.01 NTU, respectively, indicating strong disturbances and upward transport of cold and saline deep waters. Accordingly, the oxygen concentration dropped from 8.09 to 4.93 mg L−1. Four days later, daily-averaged Chl a and oxygen rebounded, increasing from 0.76 to 3.65 μg L−1, and from 4.93 to 6.34 mg L−1, respectively, suggesting a surge in biological production following typhoon-induced upwelling. The intense biological activities were interrupted by typhoon Maysak on 30 August, causing a spike in turbidity to 53-167 NTU. On 6 September, typhoon Haishen traversed the East China Sea through the Tokara Strait. Between 5 and 9 September, salinity decreased from 28.13 to 24.48, displaying significant diurnal fluctuations ranging from 19 to 28 within a day. Such low-salinity signal was probably induced by the advection of the Changjiang plume waters, propelled by typhoon wind. The low salinity waters also triggered substantial biological production, elevating Chl a to 6.05 μg L−1 on 10 September.
OS09-A020
Carbonate Dynamics in the Surface Philippine Sea, Summer 2023
Wei-Jen HUANG1#+, Kai-Jung KAO1, Veran WEERATHUNGA1, Fei-Ling YUAN1, Chin-Chang HUNG1, Wen-Chen CHOU2
1National Sun Yat-sen University, Taiwan, 2National Taiwan Ocean University, Taiwan
Despite of its large region, the role of the surface Philippine Sea at the western North Pacific Ocean was usually neglected in global carbon cycle. We conducted a research cruise on this study area when it encountered three Typhoons in summer 2023, which was the end of a strong La Niño. Discrete Total alkalinity (TA) and dissolved inorganic carbon (DIC) samples were taken in depths shallower than 500 m, and surface partial pressure of carbon dioxide (pCO2) was measured through an underway system in the surface layer (< 5 m). TA and DIC were normalized as nTA and nDIC to discuss the carbonate dynamics. The result shows that nTA were between 2290 – 2340 µmol kg-1 and nDIC was between 1963-2258 µmol kg-1. We calculated saturated DIC and compared it with the relationship between nTA and nDIC, suggesting that surface DIC and TA were affected by strong mixing and biological uptake in the surface layer while DIC release in the subsurface layer (<500 m). This result is consistent with underway pCO2 which was mostly undersaturated over the cruise. We suggest that this study area was affected by extreme weather and also climate changes and should be emphasized in the future.
OS09-A021
Carbon Fixation, Including Dissolved Organic Carbon, By Two Seaweeds, Sarcodia Suae and Agardhiella Subulata
Tzu-Chieh CHUNG#+
National Sun Yat-sen University, Taiwan
Marcoalgae (or called seaweed) are believed to play an important role to capture carbon and transfer CO2 to particulate organic carbon (POC) and dissolved organic carbon (DOC) when they grow in coastal environments. However, recent studies have shown that DOC release by seaweeds are variable accounting from 10% to 40% based on wild investigations, possibly due to DOC release method difference. In this study, we measured carbon fixation by two seaweeds, Sarcodia suae and Agardhiella subulata to quantify contribution of DOC release using large tank cultivation. The preliminary result showed that the carbon capture rate of S. suae and A. subulate ranged from (3.07 g -C m−2 d−1) and (5.56 g -C m−2 d−1), respectively. The release DOC rate of S. suae and A. subulata ranged from (0.224~0.629 g-C m−2 d−1) and (0.416~0.537 g-C m−2 d−1), respectively. The carbon fixation rate of S. suae is averagely 3.07 g-C m−2 d−1 and an average of 13.4% of this carbon is as DOC. The carbon fixation rate of A. subulate is averagely 5.56 g-C m−2 d−1) and an average of 6.6% of this carbon is as DOC. Our results suggest that DOC release by seaweeds are indeed variable and lower than previous studies. The result maybe species specifically and affected by cultured parameters such as temperature, light intensity, nutrient, DOC species and microbial activity. It is vital to survey contribution of DOC release by different seaweeds and measure these possible factors simultaneously in the future.
OS09-A025
Source, Distribution, and Ecological Effects of Particulate Organic Carbon (POC) in the Changjiang River (Yangtze) Estuary During an Extreme Drought Event
Ningxiao YU1,2+, Hai-Yan JIN2#, Dewang LI2, Bin WANG2, Ying LUO1, Qianwen SUN3, Jianfang CHEN4, Zhongqiang JI2, Zhi YANG4, Ling CHEN2
1Shanghai Jiao Tong University, China, 2Ministry of Natural Resources, China, 3Zhejiang University, China, 4State Oceanic Administration, China
As climate change intensifies, episodic and intensive drought events are increasing in frequency globally (IPCC, 2021). However, the impact of extreme drought on biogeochemical processes of POC in river-dominated shelf-marginal seas is still unknown. Here, samples from Yangtze River Estuary were collected under drought and non-drought (normal) conditions for a multiproxy geochemical study. We analyzed nutrients, DO, POC, δ13C-POC and C/N ratio to characterize the effects of drought event on POC sources, distribution, and ecological effects in the Changjiang River (Yangtze) Estuary. The results showed that the POC concentration in the Yangtze River estuary during the drought year ranged from 31.16 to 878.33 μg∙L⁻¹, significantly lower than the range of 28.46 to 5161.73 μg∙L⁻¹ in the normal year. In the drought year, Net Community Production (NCP) was estimated at 90.55-99.21 mg C∙m²∙d⁻¹ based on nutrients, accounting for only 22.4%-24.9% of the normal year. Our estimations also indicated a noteworthy reduction, approximately 72.8%, in the total POC within the euphotic layer of the study area during 2022 in comparison to the normal year (2021). Additionally, in terms of POC distribution, the impact of drought includes the contraction of the front and the strengthening of upwelling, resulting in two high-value areas of marine-derived POC in the surface water. One was located within the onshore freshwater front, while the other was situated in the offshore upwelling zone and contributing to the hypoxia in the bottom water.
OS09-A029
Coastal Acidification Under the Influence of Freshwater Input and Hypoxia: Status and Trends
Bin WANG1#+, Dewang LI1, Yanyi MIAO1, Qianwen SUN1, Xiao MA2, Hai-Yan JIN1, Jianfang CHEN2, Feng ZHOU1
1Ministry of Natural Resources, China, 2State Oceanic Administration, China
Coastal acidification, caused by both atmospheric CO2 and changes in coastal biogeochemical and hydrographic processes, is considered a manifestation of ocean acidification in coastal areas. In open oceans, the average rate of acidification caused by CO2 emissions is approximately -0.0016 pH yr-1. However, the coastal system is more vulnerable to ocean acidification. In the East China Sea, seasonal coastal acidification (with pH fluctuating by about 0.30 pH) frequently occurs along with seasonal hypoxia. In August 2018, survey data was collected to examine the combined effects of freshwater input and summer hypoxia events, focusing on differences in buffering capacity and biological effects. The lower buffering capacity of freshwater input from the Changjiang and Hangzhou Bay modifies the coverage area of low pH water in less saline water (S<30). Additionally, the remineralization processes of labile organic matter contribute to the acidification in bottom water. A combined data set was used to ascertain the influence of both river discharges and respiration processes. The correlation between pH and AOU (Apparent Oxygen Utilization) from eight years (2006, 2013, 2014, 2017, 2018, 2020, 2021, 2022) ranged from -0.0016 to -0.0026, generally following the Redfield Ratio. This indicates that organic matter respiration is the major contributor to coastal acidification in subsurface seawater (salinity>30). However, our results evidenced an accelerating rate of coastal acidification both in surface and hypoxic water. Due to the dynamic changes of coastal currents, the trend of coastal acidification is largely modulated by river discharges and seasonal hypoxia coherently.
OS09-A032
Deepening of the Thermocline Increases Primary Production in Winter vs Summer in the Northern South China Sea
Qinyu LIU#+
Donghai Laboratory, China
Coastal oceans make a disproportionate contribution to the global marine carbon sink, primarily due to their high primary production (PP). In this study, we conducted two cruises to investigate PP in large areas in the NSCS in summer and winter. In summer, integrated primary production (IPP) was about 349 mg C m-2 d-1, lower than the winter value of around 449 mg C m-2 d-1. IPP exhibited no significant seasonal difference on the shelf between summer and winter, while beyond the shelf, IPP was significantly (p<0.05) higher in winter compared to summer. Deepening of the thermocline increased the availability of nutrients in the upper euphotic layer and was responsible for the increased IPP in winter. Furthermore, the deepened thermocline induced changes in the photosynthetic efficiency and light adaptation of the phytoplankton community, which might be another important reason for the IPP increase in winter. Integrated new production (INP) and POC flux exported from the euphotic layer were also higher in winter than in summer. The increase in POC flux was more pronounced compared to INP because in addition to being affected like INP by the increase in nutrient supply and IPP in winter, the decrease of sea surface temperature would also lead to an increase in POC flux.
OS10-A002
Spatiotemporal Analysis of Marine Heatwave and Ocean Acidification Patterns Adjacent to the Philippines
Rose Angeli MACAGGA#+, Po-Chun HSU
National Central University, Taiwan
Continuous increase in the emission of anthropogenic carbon dioxide (CO2) into the atmosphere has caused adverse effects on oceans globally. Excess heat from the greenhouse effect in the atmosphere is absorbed by the ocean, causing extreme temperature water events known as marine heatwaves (MHWs). Increased concentration of CO2 is also being absorbed by ocean waters resulting to ocean acidification (OA). Intensification of these phenomena can cause detrimental effects on marine ecosystems. This study aims to analyze the spatiotemporal patterns of MHW and OA on ocean waters adjacent to the Philippines from 1985 to 2022. Satellite and numerical model data of sea surface temperature (SST), pH, and surface partial pressure of CO2 (spCO2) were used to determine the changes in the study area throughout the course of the study. Six MHW indices were used to define the frequency, duration, and intensity of MHW events. Empirical orthogonal function (EOF) analysis was performed to identify the spatiotemporal variability of the SST, pH, and spCO2 data. Variation in SST distribution is highly dependent on the ocean circulation governing the different regions, such as the Kuroshio Current, West Philippine Sea, and North Equatorial Current. Positive trend in monthly EOF of SST has been observed, while monthly EOF of pH and spCO2 showed inverse patterns. Negative trend with a rate of change of -0.1058/month and positive trend with a rate of change of 0.1003 μatm/month were observed for pH and spCO2, respectively. Anomalous years were identified to be 1988, 1998, 2010, and 2016 onwards. Climate variability due to El Niño Southern Oscillation (ENSO) and Pacific Decadal Oscillation (PDO) were also considered to be the physical drivers affecting the study area.
OS10-A009
Events of Marine Heatwaves and Marine Cold Spells in Penghu Islands and Taiwan Bank
Po-Chun HSU#+, Tzu-Ning CHEN
National Central University, Taiwan
This study employs satellite observations and reanalysis data to evaluate changes in sea surface temperature (SST) and ocean optical properties around Taiwan's Penghu Islands and the adjacent Taiwan Bank from 1985 to 2023. The Penghu Islands, crucial habitats for seagrass beds in Taiwan, experience intense summer upwelling in the nearby Taiwan Bank, propelled by a combination of Ekman transport and the centrifugal force of the South China Sea Warm Current. Our research focuses on Degree Heating Weeks (DHW), Marine Heatwave (MHW), and Marine Cold Spells (MCS) events. We also use ocean optical data to assess the spatiotemporal distribution of water quality, integrating this with surface downward carbon dioxide flux and pH value data to explore the multi-temporal and spatial impacts of ocean warming and acidification on seagrass bed ecosystems. Our findings reveal that the region around the Penghu Islands reached a Level 1 heat stress alert (DHW exceeding 4°C) in 12 out of the studied years, with most events occurring post-2015. SST analysis shows a marked annual increase in MHW events; the average incidence in the Penghu region climbed from once yearly between 1985 and 1994 to seven times annually between 2015 and 2023. The typical duration of each MHW event in the Penghu area ranges from 7 to 20 days. Between 2015 and 2023, the Penghu Islands underwent an average of around 120 days of MHW events annually, approximately fifteen times the figure from three decades prior. Moreover, we observed an increase not only in warmer SSTs during summer but also in MCS events during winter. These trends in extreme weather events are linked to the Pacific Decadal Oscillation, El Niño phenomena, and shifts in regional ocean currents.
OS10-A022
Evaluation and Projection of Marine Heatwaves in the South China Sea: Insights from CMIP6 Multi-model Ensemble
Kang XU1#+, Kai LIU2, Tongxin HAN1
1Chinese Academy of Sciences, China, 2National Marine Environmental Forecasting Center, China
This study evaluates the performance of 16 models sourced from the Coupled Model Intercomparison Project phase 6 (CMIP6) in simulating marine heatwaves (MHWs) in the South China Sea (SCS) during the historical period (1982−2014), and also investigates future changes in SCS MHWs based on simulations from three Shared Socioeconomic Pathway (SSP) scenarios (SSP126, SSP245, and SSP585) using CMIP6 models. Results demonstrate that the CMIP6 models perform well in simulating the spatial-temporal distribution and intensity of SCS MHWs, with their multi-model ensemble (MME) results showing the best performance. The reasonable agreement between the observations and CMIP6 MME reveals that the increasing trends of SCS MHWs are attributed to the warming sea surface temperature trend. Under various SSP scenarios, the year 2040 emerges as pivotal juncture for future shifts in SCS MHWs, marked by distinct variations in changing rate and amplitudes. This is characterized by an accelerated decrease in MHWs frequency and a notably heightened increase in mean intensity, duration, and total days after 2040. Furthermore, the projection results for SCS MHWs suggest that the spatial pattern of MHWs remains consistent across future periods. However, the intensity shows higher consistency only during the near-term period (2021−2050), while notable inconsistencies are observed during the medium-term (2041−2700) and long-term (2701−2100) periods under the three SSP scenarios. During the near-term period, the SCS MHWs are characterized by moderate and strong events with high frequencies and relatively shorter durations. In contrast, during the medium-term period, MHWs are also characterized by moderate and strong events, but with longer-lasting and more intense events under the SSP245 and SSP585 scenarios. However, in the long-term period, extreme MHWs become the dominant feature under the SSP585 scenario, indicating a substantial intensification of SCS MHWs, effectively establishing a near-permanent state.
OS10-A024
Observations on 2015-2016 Tasman Sea Marine Heatwaves Using Underwater Gliders: Physical and Biogeochemical Subsurface Characteristics
Saranya J.S.1#+, Amandine SCHAEFFER2, Julia ARAUJO3,4, Sunghyun NAM1, Romain LE GENDRE5, Daneeja MAWREN6, Kemgang Ghomsi FRANCK EITEL7,8
1Seoul National University, Korea, South, 2UNSW Sydney, Australia, 3University of Bologna, Brazil, 4National Center for Monitoring and Early Warning of Natural Disasters (CEMADEN), Brazil, 5French Research Institute for Exploitation of the Sea (Ifremer), New Caledonia, 6University of Cape Town, South Africa, 7The University of Yaoundé I, Cameroon, 8Institute of Geological and Mining Research, Cameroon
In 2015–2016, the Tasman Sea, located off the southeast coast of Australia, experienced its most prolonged and severe marine heatwave (MHW) on record. This event persisted for 251 days, reaching a peak intensity of 2.9 °C higher than the climatology. This abnormal sea surface warming was primarily driven by a typical convergence of heat associated with the southward flow changes of the southward flowing East Australian Current. This study, employing five event-based glider observations off the coast of Storm Bay along with the Maria Island mooring time series, comprehensively explores the cross-sectional structure and temporal evolution of physical and biogeochemical variables such as temperature, salinity, dissolved oxygen, and chlorophyll-a fluorescence in subsurface before, during, and after the Tasman Sea MHW in 2015–2016. Before the Tasman Sea MHW on June 16 to July 08, 2015, off the coast of Storm Bay showed a cross-sectional structure with a cold (10–13 °C), less saline (34–35), dissolved oxygen-rich (260–275 µmolkg-1), and chlorophyll-a fluorescence-rich (0.4–1.2 mgm-3) shelf. During the decay stage of the Tasman Sea MHW, when the MHW anomalies were transported towards the off coast of Storm Bay, the cross-shelf structure from glider observation (April 04 to May 06, 2016) significantly modified. The cross-sectional structure showed a warm (16–18 °C), saline (35–35.5), low oxygen (216–220 µmolkg-1), and chlorophyll-a fluorescence-rich (0.8–2.0 mgm-3) shelf. This study enlightens the implications of bio-physical parameters variability on the cross-sectional structure and temporal evolution of MHW anomalies off the coast of Storm Bay before, during and after the prolonged Tasman Sea MHW.
OS10-A025
Genesis, Trends, and Prospects of Marine Heatwaves in the Indian Ocean
Dushantha Sandaruwan Jayarathana WIJENDRA NAIDHELAGE 1,2#+, Wen ZHOU3, Matthew COLLINS2, Xuan WANG1, Erandani Lakshani WIDANA ARACHCHIGE4,5, Oluwafemi Ebenezer ADEYERI1
1City University of Hong Kong, Hong Kong SAR, 2University of Exeter, United Kingdom, 3Fudan University, China, 4Nanyang Technological University, Singapore, 5Imperial College London, United Kingdom
Marine heatwaves (MHWs) are prolonged periods of anomalous warm temperatures that can have significant effects on the marine environment. Unlike traditional SST variability studies, MHW research goes beyond the ocean-atmosphere interaction and focuses on how extreme warming affects marine ecosystems. This study specifically examines MHWs in the Indian Ocean, an area with limited research on the topic. The study covers the period from 1982 to 2022, analyzing MHWs in seasonal and interannual timescales to understand the effects of extreme warming on the region's marine ecosystems. Study found that major climate modes such as Indian Ocean Dipole (IOD) and El Niño significantly influence the occurrence of summertime MHWs by modulating the regional ocean-atmospheric interactions in the Indian Ocean. Subsurface warming played a major role in the genesis of MHWs in the Bay of Bengal and the Arabian Sea during the 2015 positive IOD event, which led to both severe MHW events and a reduction in surface nutrient levels. The frequency and duration of MHWs in the Indian Ocean have increased significantly since the mid-1990s, with a peak in 2019. El Niño events also strongly influence MHW occurrences, as evidenced by peaks in 1998 and 2015. Moreover, Global climate model datasets are used to analyze the variability of MHW characteristics over the region in future. Different emission scenarios show varying impacts on projected MHWs, with anthropogenic influence expected to accelerate the intensity and duration of these events. Further, we highlight the urgency of mitigating anthropogenic influence, enhancing marine conservation efforts, and building resilience to address the increasing threat of MHWs to ecosystems and economies worldwide in the near future.
OS10-A031
Shifting Responses of Phytoplankton to Atmospheric and Oceanic Forcing in a Prolonged Marine Heatwave
Weikang ZHAN#+, Ying ZHANG, Qingyou HE, Haigang ZHAN
Chinese Academy of Sciences, China
Marine heatwaves are becoming a severe challenge for marine ecosystems. However, current understanding of their impacts on phytoplankton, especially biomass and community structure, is still deficient or fragmentary. Here, we focus on the response of phytoplankton to a prolonged (372 days) marine heatwave in the southeastern tropical Indian Ocean in 2015-2016. Despite a similar surface warming throughout the marine heatwave, we found two distinctively different changes in chlorophyll-a (Chl) concentration, based on which the marine heatwave was divided into two phases of nearly equal duration. During Phase 1, the Chl concentration and phytoplankton biomass increased slightly, while during Phase 2 they decreased dramatically, with a marked shift in phytoplankton community towards smaller-size species. This difference mainly resulted from the change in dominant drivers of the marine heatwave, which shifted from atmospheric forcing (enhanced net air-sea heat flux) in Phase 1 to oceanic process (downwelling Kelvin waves) in Phase 2. The intensified near-surface stratification and upwelling Kelvin waves led to a slight surface nutrient increase in Phase 1, while the downwelling Kelvin waves suppressed the seasonal upwelling in Phase 2, resulting in a substantial decrease in nutrient supply from the subsurface ocean, and hence dramatic decreases in Chl concentration and biomass. Our results demonstrate the complex responses of phytoplankton to marine heatwaves and highlight the importance of distinguishing the driving mechanisms of marine heatwaves when evaluating their ecological impacts.
OS11-A001
Interfacial Tsunamis in a Two-fluid System
Chi-Min LIU#+
Chienkuo Technology University, Taiwan
This study presents a set of analytic solutions of interfacial tsunamis triggered by a sudden motion of sea bottom, and the corresponding applications in specific scenarios. Major mathematical techniques for deriving the solutions are Laplace and Fourier transforms in temporal and spatial dimensions. The Boussinesq approximation is applied to simulate the situations in oceans. Three fundamental types of seabed deformations, which include the rectangular, cosine and sine deformations, are considered and analyzed. Based on the derived solutions of these basic deformations, tsunamis induced by an arbitrary seabed deformation can be readily analyzed with the help of Fourier analysis.
OS11-A009
Probabilistic Tsunami Hazard Assessments by Using Different Tsunami Source Groups
Eishin WATANABE#+, Toshitaka BABA
Tokushima University, Japan
Large earthquakes and tsunamis are natural phenomena that include uncertainties. Therefore, it is preferable to use probabilistic tsunami hazard assessment to design coastal defense structures in resilient cities. However, assessment results are diverse due to different assumptions and models used. Because the record of past tsunamis is insufficient, we cannot say which assumption and model are superior to the others. Therefore, we need to quantitatively investigate the difference in the results derived from the different models. We performed tsunami calculations from a set of tsunami sources with heterogeneous slips on the fault in the Nankai Trough (group 1), defined occurrence probabilities based on the Gutenberg-Richter relationship, and evaluated the tsunami exceedance probability at arbitrary points as tsunami hazard curves. We also used the same method to evaluate the exceedance probability using a tsunami source group of homogeneous slip (group 2) and another heterogeneous tsunami source group (group 3) to investigate how the tsunami hazard curve changes depending on the tsunami source groups. The tsunami hazard curves constructed from the homogeneous fault slips (tsunami source group 2) were smaller than those constructed from the heterogeneous fault slip groups (groups 1 and 3). The small hazard assessment is because the homogeneous tsunami source group did not include large fault slip patches generating large tsunamis. The comparison of the tsunami sources with heterogeneous fault slips (groups 1 and 3) also showed significant differences. The results indicate that the tsunami hazard curves are sensitive to construction methods for tsunami sources.
OS11-A013
Surge in Macao Coastal Areas Under Easterly Winds
Zi YE1,2#+, Huabin SHI1
1University of Macau, Macau, 2Zhuhai UM Science & Technology Research Institute, China
Easterly winds may result in significant surge in coastal areas of Macao, west-side of the Pearl River Estuary. During Feb 19 to 23 of 2023, a sustained wind at even level 6 together with the high tide had caused flooding in the low-lying areas of Macao Inner Harbor. It was shown in the observations of tidal level in Macao that the wind-driven surge presented notable fluctuations with a period of about 6 hours, which was quite inconsistent with the insignificant variation in the wind field but aligns with half the duration of the tidal cycle. The tide-surge interactions under the sustained generally-strong winds (under normal meteorological condition other than tropical cyclones) are far from being clearly understood. Utilizing a high spatial-resolution three-dimensional FVCOM model covering the north shelf of South China Sea and focusing on Macao coastal area, in the present study we examine the wind-driven flow fields along the South China coast, in the Pearl River Estuary and within the narrow channels in Macao coastal areas. It is proposed that the 6-hour-periodic fluctuations in the wind-driven surge measured in Feb 2023 are due to the periodic change in the wind-driven current along the South China coast under the rotation of the tidal current. The surge in Macao Inner Harbor is highly correlated with the direction of the wind-driven current outside of the Pear River Estuary.
OS11-A029
Storm Surge Prediction by Machine Learning Models
Yujia WANG1,2#+, Huabin SHI1
1University of Macau, Macau, 2Zhuhai UM Science & Technology Research Institute, China
Storm surges induced by tropical cyclones seriously threaten the development of society and economy and the public safety of the Greater Bay Area. Developing storm surge prediction and forecasting techniques is of great significance to hazard prevention and mitigation. In this study, four machine learning models respectively based on the multilayer perceptron (MLP), recurrent neural network (RNN), long short-term memory neural network (LSTM), and bidirectional long short-term memory neural network (Bi-LSTM) are developed for the prediction of storm surge in Pearl River Estuary. A total of 257 historical tropical cyclone events affecting the Pearl River Estuary from 1968 to 2021 are adopted for model training and testing. It is shown that the MLP and the Bi-LSTM models have a good performances in predicting storm surge with the values of RMSE of both models are about 70 mm for the 1-h-leading prediction and below 190 mm for the 6-h-leading prediction. Among the four models, the LSTM model has a best performance in predicting the trend and the peak time of surge height, especially during severe and super typhoons.
OS11-A033
Evolution of Gravel Beach Profile Under Storm Condition: Laboratory Experiment and Numerical Modeling
Yun-Ta WU#+, Zi-Shen CHOU
National Cheng Kung University, Taiwan
Taiwan is vulnerable to the pathways of typhoons from the Western North Pacific. More than 50% of historical typhoons landed on the southeastern Taiwan, whose coastlines feature reflective and mostly covered by gravel and cobble. Although gravel beach can dissipate more wave energy compared to sandy beach, the coastlines face severe beach erosion due to storm waves and also narrow continental shelf in the southeastern Taiwan. In this study, we carried out physical model tests to investigate the possibility for beach nourishment using gravel. Experiments were conducted to mimic the situation of nourished gravel beach in front of coastal highway and to measure the beach profile changes during storm conditions using irregular waves. We measured free surface elevations and flow velocities near the gravel beach. The gravel beach profile changes were measured using an integrated laser and image processing tool to obtain 3D topographic maps. An open-source numerical model, XBeach-G, was used to reproduce the experiment. However, the determination of some parameters in the model is challenging. Here, we used the Generalized Likelihood Uncertainty Estimation (GLUE) method to calibrate five selected parameters so as to optimize the parameter sets used in the numerical model. The criterion to judge the quality of the calibration was based on the fit of the beach profile evolution from model-data comparison. Using the calibrated parameters, we have compared with different cases of experiments which has not been used for the calibration processes and also extend the parameter ranges which has not been conducted for experiments.
OS11-A047
Development of a Numerical Simulation Model to Evaluate the Inundation Duration by Storm Surge
Norihiko KONNO1#+, Toshinori OGASAWARA1, Tomokazu MURAKAMI2
1Iwate University, Japan, 2National Research Institute for Earth Science and Disaster Resilience, Japan
Countermeasures for storm surges are essential in disaster prevention due to the expected increase in typhoon intensity caused by global warming. Previous studies have focused on analyzing the maximum inundation depth as a standard for storm surge countermeasures. However, for effective evacuation planning, it is also crucial to predict the duration of inundation from the start of the storm surge to the end of drainage. However, in urban areas, the duration of inundation may be overestimated due to inadequate modeling of the sewerage system. In other words, the sewers significantly impact the drainage process of storm surges. Thus, this study aims to develop an inundation analysis model due to storm surge that considers the drainage action of sewage systems in urban areas and correctly evaluates the duration of inundation. The analysis focuses on the Port of Nagoya area to evaluate the potential inundation caused by the most significant possible storm surge. The initial values for the storm surge inundation calculations, including inundation depth and flow velocity, are given to the land area. An analytical model for inland water flooding is used to evaluate the inundation process, which can reproduce the drainage action of the sewerage system. The results indicate that the duration of inundation is shorter than the assumed time due to the drainage action of the sewage system. The topography and water level of the river may influence the duration of inundation. The analytical model used in this study provides valuable information on inundation duration, which can aid in determining evacuation measures and initial response to disasters.
OS11-A049
Numerical Simulation of the Generation and Propagation of Meteotsunami Waves in the Adjacent Seas of Taiwan
Yu-Chien CHENG+, Chih-Chieh YOUNG#
National Taiwan Ocean University, Taiwan
Unexpected meteotsunami-waves (MT-waves) induced by a tiny moving pressure disturbance and amplified by Proudman resonance have caused numerous accidents in the coastal oceans, harbors, or great lakes, e.g., 4.78 m in Nagasaki Bay (Japan), 4 m in Harbor Ciutadella (Spain), 3 m in Great Lakes (USA). In this study, our purpose was to investigate the temporal and spatial characteristics of MT-waves and how they would impact Taiwan’s coastal water. First, we collected the tidal and air pressure data at several stations. By Morlet Wavelet Transform, the disturbances of water heights with periods ranging from 0.5 h to 2 h were observed. Second, a hydrodynamic model was developed to simulate the generation and propagation processes of MT-wave. In the numerical experiments with constant water depth, different translation speeds (U) of air pressure disturbance were examined. Clearly, the amplification of MT-waves (due to Proudman resonance) depends on how the translation speed of air pressure disturbance approaches the celerity (C) of MT-wave. In comparison to the wave height induced by a static air pressure (Hs), the height of MT-waves over the simulated period would be greatly increased under the resonance condition (i.e., U = 1.0 C), e.g., up to 3.95 Hs at t = 3 h and 16.29 Hs at t = 10 h. Last, the real topography was adopted to investigate the influence of Proudman resonance and characteristics of MT-waves in the adjacent seas of Taiwan. The Proudman length was also calculated to effectively identify most dangerous areas for potential risk assessment.
OS11-A059
Estimation of Wave Forces on Building Structures During Tsunami Return Wave
Akio NAGAYAMA1#+, Ryoichi YANAGAWA2
1Kagoshima Unviersity, Japan, 2National Institute of Technology of Kagawa College, Japan
The 2011 Tohoku region Pacific Ocean earthquake triggered a devastating tsunami, impacting shore area buildings and structures. Against this background, we examine the estimated formula for tsunami wave force on the building. The formula currently used to predict wave force on buildings in Japan is calculated by tripling the static water depth pressure. Recent tsunami evacuation building conforms to government guidelines which use these formulas. However, the formula is only applied to swash waves due to the restricted scale of experimental equipment, requiring broader consideration for return wave conditions. Thus, our research has focused on adjusting the formula to account for return waves, using a large water tank in the laboratory. As a result, we identified the following points: 1) the tsunami force in the return wave equals that of the swash wave in water concentration zones, and 2) the adjusted formula might predict wave force based on building shape. In the paper, we revised the formula to include the drag force by velocity on side wall, and discuss the wave force during the return wave. Consequently, accuracy in estimating the force of the return wave has risen. Using the formula currently recommended in the guidelines results in an underestimation of wave force, since it only considers the impact of the wall hit by the return wave. By considering the effect on wave velocity of the impact on the side wall, the wave force can be more accurately predicted.
OS12-A001
Spatial Structure of Vertical Motions and Associated Heat Flux Induced by Mesoscale Eddies in the Upper Kuroshio-Oyashio Extension
Yushan QU1#+, Shengpeng WANG2, Zhao JING1, Hong WANG1
1Ocean University of China, China, 2Laoshan Laboratory, China
Vertical motions induced by mesoscale eddies in the upper ocean play a vital role in the heat transport over the global ocean. However, the spatial structure of vertical eddy velocity and associated heat flux remains unclear. This study addresses this issue in the Kuroshio-Oyashio Extension based on an eddy-rich Community Earth System Model simulation. Adopting a mesoscale eddy composite analysis, we show that the vertical eddy velocity is enhanced at edges of mesoscale eddies with a maximum magnitude of 0.8 m day−1 in the upper ocean for anticyclonic eddies (AEs) and 0.5 m day−1 for cyclonic eddies (CEs). The associated vertical heat flux is upward, reaching 52 and 32 W m−2 along AEs' and CEs' periphery, respectively. Diagnostic analysis suggests that the enhanced vertical eddy motions at eddy edges are primarily attributed to the ageostrophic secondary circulation (ASC) under the turbulent thermal wind balance that accounts for more than 70% of the vertical eddy velocity and 80% of vertical eddy heat flux in the upper ocean. This ASC is stronger in winter than summer due to the intense turbulent mixing induced by strong surface cooling and wind stirring in winter. Accordingly, the vertical eddy velocity and associated heat flux exhibit a distinct seasonal cycle.
OS12-A002
Parametric Subharmonic Instability of Diurnal Internal Tides in the Abyssal South China Sea
Qianwen HU#+
Chinese Academy of Sciences, China
Internal waves close to the seafloor of abyssal oceans are the key energy suppliers driving near-bottom mixing and the upwelling branches of meridional overturning circulation, but their spatiotemporal variability and intrinsic mechanisms remain largely unclear. In this study, measurements from 10 long-term moorings were used to investigate the internal wave activities in the abyssal South China Sea (SCS), which revealed diurnal parametric subharmonic instability (PSI) above rough topographies near its critical latitudes (CLs). The mooring locations are at comparable ocean depths of approximately 4000 m, which represents the average water depth of the SCS deep basin. Distinct bicoherence peak demonstrated horizontal phase coupling between three clockwise-rotated internal waves at frequencies of f, f, and 1 cpd, which was evidence of PSI occurring. Compared with flat topography, PSI near rough topography was significantly promoted by topographic-localized strong D1 with high-mode structures, creating abyssal NIW bursts. Bottom-reaching shipboard CTD profiles revealed that the bottom mixed layers became much thicker when approaching CLs, suggesting that abyssal PSI potentially accelerates the ventilation and upwelling of bottom water.
OS12-A004
Changes of Wave Characteristics Over Equatorial South China Seas
Low SHIEN YEE1#+, Liew JUNENG2, Nursalleh K. CHANG3, Jeong Yik DIONG3
1National University of Malaysia, Malaysia, 2Universiti Kebangsaan Malaysia, Malaysia, 3Malaysian Meteorological Department, Malaysia
The South China Sea's equatorial monsoon is influenced by the East Asian monsoon. Increasing of the global surface air temperature has potentially increased the surface wind speed, leading to changes in the wind wave characteristics. This has significant implications for coastal marine activities and socio-economy, underscoring the need to better understand regional ocean and low-level atmosphere conditions. Hence, this study aims to analyze the historical changes in significant wave height (SWH) over the equatorial SCS and their association with surface wind speeds (SWS). The analysis is based on the 38-year dataset of SWH and SWS at a 10m height from ERA5 produced European Center for Medium-Range Weather Forecasts (ECMWF) and also a wave hindcast product developed by the Malaysian Meteorological Department (MMD). While the ERA5 is made available at 25km grid resolution, MMD hindcast comes with a resolution of 25km and much higher 5km grids. The MMD wave hindcast is forced by the wind from ERA-Interim to simulate wave condition. Subsequent correlation analysis clarified the relationship between changes in SWS and SWH in Malaysia's coastal regions. Within the three SWH datasets (ERA5, MMD_5km, and MMD_25km), Spearman Rank Correlation and Pearson correlation coefficients indicated strong positive correlations for MMD_5km and ERA5 datasets (0.92 and 0.93, respectively) and moderate positive correlations for MMD_25km and ERA5 datasets (0.57 and 0.55, respectively). This suggests that MMD_5km aligns better with ERA5 in representing SWH. There is a decrease in the SWH and declining trends in SWS, annually from 1981 to 2018 where the reduction is particularly apparent along the Johor Straits and Sabah coastal area. This suggests a consistent decrease in both SWH and SWS whereas the SWH and SWS increased across the west coast of Peninsular Malaysia. The correlation analysis further revealed a positive correlation between SWS and SWH in this study.
OS12-A005
The Hadley Cell Expanding Poleward Weakened Winter Circulation in the Yellow Sea Over the Past Six Decades
Yucheng WANG1#+, Fangguo ZHAI2
1Laoshan Laboratory, China, 2Ocean University of China, China
Ocean circulation is of vital importance in modulating the physical and biogeochemical conditions of the Earth at regional and global scales. Using 59 years (1958‒2016) of high-resolution model outputs, we investigated the long-term changes of winter circulation in the Yellow Sea (YS), which is located between China and the Korean Peninsula as a midlatitude shelf sea of the western Pacific Ocean. The results indicated that the YS winter circulation was weakening over the past six decades. Volume transports of the northward warm current (YSWC) in the central area and southward coastal currents both largely decreased, which were most significant at approximately 35°N inside the YS. The largest volume transport trend magnitudes were 1.67×10‒3 Sv a‒1 for the YSWC and 1.47×10‒3 Sv a‒1 for coastal currents. Further analyses suggested that weakening of the YS winter circulation was caused by poleward expanding of the Hadley Cell (HC) over the eastern China seas. Anomalous northward movement of the descending branch of the winter HC led to anomalous descending air motions over the YS and adjacent areas, which shifted southward approaching the Earth’s surface and reached the southeastern North YS at the sea surface. The resultant anticyclonic surface wind anomalies generated a large-scale cyclonic gyre anomaly in the YS, which then caused weakening of the northward YSWC in the west and southward coastal currents in the east. The current study advances our understanding of how global shelf sea dynamics responds to past and future climate changes.
OS12-A008
Three Types of Typhoon-induced Upwellings Enhance Coastal Algal Blooms
Yuxuan LI#+
Chinese Academy of Sciences, China
Typhoons (hurricanes or tropical cyclones) developing in the Western North Pacific frequently reach the East China Sea (ECS) and cause various dynamic responses in the coastal area. The harmful algal blooms are increasingly reported off the coasts of Zhejiang Province, China, where has a complicated circulation pattern related to the Changjiang River Diluted Water (CDW), the Taiwan Warm Current (TWC), the Kuroshio Current (KC). Though the phosphate input from the intrusion of the Kuroshio Subsurface Water (KSSW) contributes a lot to the growth of the plankton, it remains unclear how do typhoons trigger algal bloom in the coastal seas. We used a fine-resolution coupled physical-biological model based on Regional Ocean Model System (ROMS) to reproduce oceanic responses during Super-Typhoon Chan-hom. The modeled surface Chl-a variations were highly consistent with satellite data, indicating a significant algal bloom phenomenon facilitated by the typhoon along the coast of Zhejiang Province. Through three-dimensional dynamic diagnostics, three types of typhoon-induced upwellings are revealed: the classical linear wind-Ekman pumping, nonlinear wave pumping (include low-frequency coastal shelf waves along the coasts and high-frequency near-inertial waves along the typhoon track), and eddy-induced pumping. These upwellings make the phosphate-rich bottom KSSW outcrop consecutively and then available to the subsequent phytoplankton blooms, suggesting the vital role of interaction between open sea and coastal ocean. This work proved the close connection between physical processes especially nonlinear effect and marine environment changes on the continental shelf under typhoon conditions. Furthermore, the developed diagnostic method and general upwelling mechanisms can apply to other shelf sea regions worldwide.
OS12-A009
Interannual Variations of Eddy Kinetic Energy in the Western Equatorial Pacific Ocean
Xueqi LIU, Hui ZHOU#+
Chinese Academy of Sciences, China
The interannual variation of eddy kinetic energy (EKE) in the western equatorial Pacific Ocean is investigated based on the satellite observations and model outputs in this study. Results reveal that the EKE exhibits vigorous interannual variations here, which is mainly attributed to the barotropic instability associated with the background currents, especially in the region of North Equatorial Countercurrent (NECC) and north of the New Guinea. The energetic NECC behaves northward shift and much stronger meander path, which favors the enhancement of EKE variation due to the enhanced barotropic instability. The strong interannual fluctuations in the strength of New Guinea Coastal Current/Undercurrent (NGCC/NGCUC) and the eastward current along equator contribute to the significant EKE interannual variations north of the New Guinea. Meanwhile, the interannual variations of EKE here also exhibit different characteristics in different flavors of El Niño. The EKE generally weakens in western equatorial Pacific during Eastern Pacific El Niño (EP-El Niño) events, but that north of the New Guinea is enhanced during the Central Pacific El Niño (CP-El Niño) events due to the occurrence of the much stronger eastward current along the equator in CP-El Niño events. These results will contribute to a better understanding the low-frequency eddy-mean flow interactions and also its role in local biological processes.
OS12-A011
An Intermediate Flow in Tropical Pacific Observed by Moored Current Meters
Xiaoluan YAN1#, Linlin ZHANG2+
1Chinese Academy of Sciences, China, 2Institute of Oceanology, Chinese Academy of Sciences, China
Six years of current meter observation from a subsurface mooring at 130°E ,8.5°N captured an eastward flow lower than North Equatorial Undercurrent (NEUC) between 1500-3000m. The mean velocity of this flow at 1500m and 2000m are 1.51± 0.08cm/s and 0.89 ± 0.07 cm/s. Its spatial distribution is studied using Argo absolute geostrophic velocity data and ocean reanalysis. In northwestern Pacific, this Lower-NEUC shifts poleward and is wider in Argo absolute geostrophic velocity data (300km) and narrower in reanalysis (150km). Vertically, the core of Lower-NEUC lies mostly on 27.5σ_θ, but it shifts from 1500m to 1300m between 130°E and 150°E. Reanalysis data shows L-NEUC’s generation is connected to deep eddies. After proving that L-NEUC is not a result of averaging west-propagating eddies, we showed that L-NEUC is eddy potential vorticity flux convergence. The zonal velocity derived from turbulent Sverdrup balance is close to observation and reanalysis velocity.
OS12-A018
On the Layered Structure and Seasonal Variation of the Water Exchanges in the Sulawesi Sea Areas as Well as the Associated Dynamics
Hua ZHANG#+
Chinese Academy of Sciences, China
The layered structure and seasonal variation of the water exchanges in the Sulawesi Sea areas, as well as the corresponding dynamics, are investigated using HYCOM data. A net inward water mass transport is identified in the upper and intermediate layers in the Sulawesi Sea and it is compensated by the net outward transport in the deep layer. As an important source of this net inward transport, the southward flow through the Sibutu Passage (denoted hereafter as Sibutu Flow) reaches 5.06Sv in winter, accounting for ~43% of the net inflow. However, it decreases substantially to 1.79Sv in summer, accounting for only 12% of the inflow. Further analysis reveals that this Sibutu Flow modulates the seasonal variation of the corresponding outward flow at the Makassar Strait, which is the only exit of the water mass in the Sulawesi Sea. In winter, the enhanced Sibutu Flow with a large amount of buoyant low-salinity water creates a strong eastward pressure gradient force and suppresses the surface intrusion via the eastern Mindanao-Sulawesi section. Conversely, this pressure gradient force weakens and shifts westward in summer, permitting a larger water intrusion from the eastern section. Given that the outward Makassar Flow is the main passage of the Indonesian Throughflow (ITF), our study highlights the essential role of the Sibutu Flow in modulating seasonal variabilities of the ITF via the Makassar Strait and, thus, the transfer of water masses and heat content between the Pacific and Indian Oceans.
OS13-A001
Upstream Extension of a Bottom-advected Plume and Its Mechanism: The Case of the Yellow River
Xiaojie YU#+
Ocean University of China, China
Hydrographic surveys have revealed that the Yellow River plume propagates in the direction opposite to that of a Kelvin wave (upstream) under a low river discharge condition, but turns downstream as the river discharge increases. A numerical model reproduced the upstream extension of the plume under the low river discharge condition and the transition to the downstream direction under the high river discharge condition, and confirmed that the summer wind is not the necessary condition for upstream extension of the plume. With the condition of low river discharge, the model also indicated the dependence of the upstream extension of the plume on the tidal range: extending upstream in spring tide but turning downstream in neap tide. The upstream movement of the plume results from the upstream transport of freshwater that depends on the upstream tide-induced residual current around the river mouth and the downstream density-driven current around the offshore plume front. With the condition of high river discharge, the upstream tide-induced residual current cannot compete with the downstream density-driven current and the plume turns downstream. Momentum analysis confirms the important roles of advection term and viscosity term in the condition of low river discharge and the shift to a Coriolis force-dominated system under high river discharge condition. An idealized model study suggests a dimensionless number for the river discharge changing the river plume extension from upstream to downstream under a specific upstream ambient current around the river mouth.
OS13-A002
Influence of Hydrothermal System on Oceanic Crustal Thickness During the Expansion Period of the South China Sea: Numerical Modeling
Huihui ZHANG#+, Lijuan HE
Chinese Academy of Sciences, China
Heat loss in the mid-ocean ridge hydrothermal system and heat supply in the deep mantle jointly affect the oceanic crust thickness. However, most predecessors pay attention to the deep lithosphere factors such as mantle temperature and mantle source composition, and little attention to the influence of the shallow hydrothermal cycle on the thickness of the ocean crust. The influence of the hydrothermal system on the oceanic crust thickness under two modes of single-path convective circulation and double-diffusion convective circulation during the expansion period is studied through finite element numerical simulation. The results show that: (1) In the single-path convective circulation model, the hydrothermal circulation has the effect of thinning the ocean crust before ocean crust accretion stabilizes; After the ocean crust accretion stabilized, the hydrothermal circulation makes the ocean crust thickness increase. (2) In the double diffusion convective circulation model, the magmatic fluid has a secondary thinning effect on the oceanic crust thickness and increases the temperature of the hydrothermal vent. (3) The expansion period of the South China Sea Basin is relatively short, and no abnormally thick ocean crust is found, so it is speculated that the ocean crust accretion has not reached a stable stage. Therefore, combined with the structural characteristics of the ocean crust in the South China Sea, hydrothermal circulation during the expansion period is considered an important factor leading to the abnormally thin ocean crust in the sea basin.
OS13-A005
A New Hybrid Coupled Model for ENSO Study. Part I: Model Description and Performance Evaluation
Yang YU1#+, Yinnan LI2, Rong-Hua ZHANG2, Shu-Hua CHEN1, Hongna WANG2
1University of California, Davis, United States, 2Chinese Academy of Sciences, China
The El Niño and Southern Oscillation (ENSO) constitute the most prominent interannual climate variation, originating from interactions between the tropical Pacific Ocean and the atmosphere. Effectively modeling ENSO’s onset and intensity has consistently posed a central challenge in related studies. In addressing this challenge, we present a novel Hybrid Coupled Model (HCM) built upon the Regional Ocean Modeling System (ROMS) framework. The ROMS model is coupled to a statistical atmospheric model, capturing interannual atmospheric anomalies such as wind stress and freshwater flux. These anomalies, pivotal in their interactions with interannual sea surface temperature anomalies, are vital in shaping the ENSO cycle. Our results demonstrate the HCM's capability to simulate the Eastern Pacific-type El Niño and La Niña events. Notably, the model exhibits stable simulations of ENSO's quasi-three-year oscillation characteristics with an air-sea coupling coefficient of 1.5. Furthermore, the HCM reproduces the three-dimensional evolution of ENSO, revealing that the most significant temperature anomalies occur beneath the surface at 200 meters rather than at the sea surface. To analyze temperature anomaly changes during the simulated ENSO cycle in the HCM, we introduce a post-processing budget scheme for the interannual temperature anomaly. The budget analysis highlights the dominance of the temperature advection process induced by interannual wind stress in the simulated ENSO. Conversely, vertical mixing negatively contributes to ENSO evolution, damping temperature anomalies from the ocean surface due to the surface heat flux feedback. The newly developed HCM is poised to serve as a potent simulation tool for ENSO investigations in the future.
OS13-A010
Investigating Wave Gradient and Its Impact to the Low Layer Atmosphere
Yuchun LIN1#+, Leo OEY2
1National Taiwan Ocean University, Taiwan, 2National Central University, Taiwan
Surface winds in the marine atmospheric boundary layer (MABL) are often modified by the surface status underneath. The small-scale features of sea surface temperature (SST) gradient are previously shown to positively couple with the wind stress divergence and curl by perturbing the turbulences of wind in the MABL throughout the world ocean. The influence of wave to wind is proposed by applying the similar but opposite mechanism to the gradients of significant wave height (Hs). This analysis is conducted using the satellite measured Hs over the North Pacific during the winter seasons from 1993 to 2016. The results show that waves over the western North Pacific are mostly wind driven: the wind stress divergence and curl are positive and linear correlated to the downwind and crosswind Hs gradients, respectively. The small-scale features of wave height gradient in the northeast regions of North Pacific signal a reversed energy transfer from wave to wind, where the wind stresses and Hs gradients are negatively correlated. Those regions are mostly dominated by swell, which transfers energy to the wind under certain circumstances.
OS13-A011
The New Operational of Indonesian Ocean Forecast System Based on High Resolution Couple Atmosphere-wave-ocean Model (InaCAWO)
Nelly Florida RIAMA+, Furqon ALFAHMI#
Indonesian Agency for Meteorology, Climatology and Geophysics, Indonesia
InaCAWO is a ocean-atmosphere modelling that recently addition to the Indonesian Ocean Forecast System (BMKG-OFS), which was jointly created by the Indonesian Agency for Meteorology, Climatology, and Geophysics, NC State University, and Baron Weather in 2023. The BMKG-OFS has been in operation since 2004, providing continuous and real-time marine weather forecasts and ocean modelling specifically for the Indonesian sea region. Previously, BMKG-OFS utilized wave modelling (Windwave-05, Wavewatch-III) and atmospheric modelling (WRF, GFS) as independent forces. The objective of couple modelling at these stages is to generate simulations that exhibit more accuracy and realism. The InaCAWO model is constructed based on the COAWST model. The components of the system consist of the regional oceanic model (ROMS), the atmospheric model (WRF), and the Simulating Wave Nearshore (SWAN) model. The system is connected to the Model Coupling Toolkit (MCT), which is a collection of processes for information modelling. The model InaCAWO has a geographical resolution of around 3 km and a temporal resolution of one hour. It consists of a grid with dimensions of 2036 x 1116 and includes 70 vertical layers. ECMWF is employed for providing beginning and boundary conditions in the field of atmospheric modelling, whilst MERCATOR is utilized for the purpose of ocean modelling. The atmospheric characteristics of InaCAWO have been assessed by analysing mean sea level, surface wind speed, and daily precipitation data obtained from synoptic observations spanning a year. However, the evaluation of oceanic properties relied on satellite and drifter measurements. The outcome suggests that the model achieves an accuracy of around 80% when employing contingency approaches for all parameters. InaCAWO can also record other distinctive Indonesian phenomena, including the amalgamation process in Indonesian throughflow using a T-S diagram, eddy circulations, intensified flows in tight straits, and freshwater discharge.
OS13-A013
Modeling Study on the Variability of Nutrient N/P Ratio and Nutrient Loading Effects on the Phytoplankton Dynamics in the Bohai Sea
Ruohan SUN1#+, Xinyi KANG1, Meng XIA2
1Chinese Academy of Sciences, China, 2University of Maryland Eastern Shore, United States
The Bohai Sea is a semi-enclosed inland sea, which is subject to serious eutrophication. Variations in phytoplankton distribution in the Bohai Sea are critical to the ecosystem health; thus, the Finite Volume Community Ocean Model (FVCOM) based integrated Compartment Model (FVCOM-ICM) was implemented to investigate the spatial and temporal variations on nutrient (N, P) and phytoplankton biomass in the Bohai Sea from 2010 to 2019. The simulated nutrient and phytoplankton biomass distribution were in good agreement with observation and real-time satellite imagery. Statistical analyses and numerical experiments revealed that phytoplankton biomass in the three sub-bays (Laizhou, Bohai, and Liaodong Bays) exhibited similar seasonal variations from 2010 to 2019. The phytoplankton biomass reached the spring bloom after May, decreased quickly after July, and increased again till the peak in October. Spatially, phytoplankton biomass in the Bohai Bay was highest among the three sub-bays. Moreover, phytoplankton biomass in the three sub-bays increased with dissolved inorganic phosphorus (DIP) loading. However, changing dissolved inorganic nitrogen (DIN) loading with fixed river discharge had a less extensive impact on phytoplankton variability, verifying the phosphorus limitation in the Bohai Sea. The DIN:DIP ratio from 2010 to 2019 in excess of the Redfield ratio also indicated phosphorus limitation in the Bohai Sea.
OS13-A017
Impacts of East Asian Monsoon on the Volume Transport in the Korea Strait and Its Reconstruction
Eun Young LEE1#+, Dong Eun LEE1, Young Gyu PARK2, Hye-Ji KIM1, Ju AH-HYUN1, Myeong Mo KANG1, Minsu SONG1
1Chungnam National University, Korea, South, 2Korea Institute of Ocean Science & Technology, Korea, South
Volume transport through the Korea Strait can be the key to understanding the thermohaline circulation of the East Sea under the different climate equilibrium, in the past or in the future. The numerical model can be a useful tool to investigate its specific role in the circulation of the East Sea. However, the regional models require high resolution data covering regional details, and there are limitations due to the lack of such data. Hear, we investigate the indicators that represent the volume transport of the Korea Strait (KS) at a larger spatial scale. We found that the volume transport of the KS is closely related to the East Asian monsoon dipole pattern. When the EASM is strong, the southerly wind, eastward Ekman transport and northward geostrophic currents across the KS are enhanced. The Kuroshio currents in the Tokara Strait exhibit a negative relationship with the volume transport of the KS. We construct a simple multilinear regression model using the East Asian monsoon and Kuroshio intensity as independent variables to reconstruct the volume transport of the KS. The resulting reconstruction shows a correlation coefficient of about 0.5 with observations, indicating a high level of predictive skill and providing confidence in the accuracy of our historical reconstruction. The mid-Holocene reconstruction suggests an increase of about 40% in the volume transport of the Korea Strait during summer, coinciding with a projected strengthening of the East Asian summer monsoon relative to the present.
OS13-A019
Influences of Physical Processes Induced by Seamounts on Vertical Mixing
He CHAOCHAO1#+, Changming DONG1,2
1Nanjing University of Information Science & Technology, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China
Seamounts are widely distributed in oceans, some in isolation and some in chains. Seamounts substantially influence the ocean’s flow field structures, enhancing mixing and playing an important role in material and energy exchange between surface and deep layers. In this study, to comprehensively understand the extent of seamounts' impact on oceanic mixing, we introduced the concept of vertical penetration rate (VPR) to quantify the vertical exchange within the oceanic environment, especially in seamount areas. High-resolution model data (LLC4320) were utilized to investigate the vertical mixing characteristics of the Emperor Seamount Chain region. Our results show that the seamount-induced VPR can reach 3-10 times that of non-mountainous areas. Four distinct physical processes, including Taylor caps, fronts, eddies, and internal waves, were investigated and these processes can significantly amplify the VPR within seamount-influenced zones. These findings aid in evaluating the implications of seamount-induced vertical mixing and provide valuable insights into its driving mechanisms for future studies.
OS13-A023
Effects of the Surface Geostrophic Currents Data in a Data Assimilative Regional Ocean Modeling System for the East Sea
Jae-Sung CHOI1+, Byoung-Ju CHOI1#, Kyungman KWON2, Gwang-Ho SEO3
1Chonnam National University, Korea, South, 2Korea Institute of Ocean Science & Technology, Korea, South, 3Korea Hydrographic and Oceanographic Agency, Korea, South
Ocean Data assimilation (DA) usually assimilates temperature and salinity data from the satellite and in-situ observation. In this study, the surface geostrophic currents calculated from gridded satellite altimeter data were assimilated using the Ensemble Kalman Filter (EnKF). To match the time scale of variability between the observed geostrophic current and model velocity, the current velocities from the model were low-pass filtered and the low-frequency component was assimilated. Optimal time window of low-pass filter was 31 days, which was obtained using the observed current from ocean buoys and the surface geostrophic current. To examine the effects of assimilation of geostrophic current, sensitivity experiments were conducted: Free run (Exp.FR), DA using only hydrographic data (Exp.TS), DA using hydrographic and surface geostrophic current data (Exp.GEO), shorter and longer moving average window (Exp.SW and Exp.LW), lower and higher observation error (Exp.LE and Exp.HE) relative to Exp.GEO, use of univariate covariance matrix in the EnKF (Exp.UC), and additional assimilation of the along-track SLA data (Exp.AT). The improvement was quantitatively evaluated in terms of correlation and normalized root mean square between the simulated variables from each experiment and observation data. Data assimilation in Exp.TS, Exp.HE, and Exp.UC improved prediction accuracy in temperature and salinity by 17.2%, 11.2%, and 15.3%, respectively, compared to the free run. Accuracy of surface current velocity was improved in Exp.SW, Exp.LE, and Exp.UC 70.4%, 85.4%, and 72.1% compared to the free run, respectively. Total performances of Exp.TS, Exp.HE, and Exp.UC were 16.8%, 13.0%, and 17.1% higher than the free run during the four summer months, respectively. Assimilation of the surface geostrophic current improved the surface current velocity while it slightly degraded hydrographic variables such as temperature and salinity. The use of univariate background error covariance for the hydrographic variables during the DA limited the degradation in the hydrographic variable performances.
OS13-A024
Application of the SWAN Model in Large-scale Wave Forecasting Simulations
Xinyuan ZHANG1#+, Ziyun WANG1, Changming DONG1,2
1Nanjing University of Information Science & Technology, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China
This study employs the third-generation numerical wave model, SWAN (Simulating WAves Nearshore), to predict the wave patterns along the North Pacific West Coast and the northern Indian Ocean from November 29, 2023, onwards (40°-150°E, 25°S-50°N). The model runs for over a month, with individual forecasts spanning 7 days. It operates at a spatial resolution of 1/25° and a temporal resolution of 3 hours. Elevation data from ETOPO (1/60° resolution) and wind data from GFS and ECMWF (0.25°×0.25° resolution) are utilized. The model also incorporates open boundaries with a horizontal accuracy of 0.5° using WaveWatch III data. The forecast accuracy is noteworthy, with minimal errors observed in the first two days and a strong correlation in the subsequent four days. This study demonstrates the model's precision in accurately forecasting wave hazards.
OS13-A028
Identifying Ship-wakes Using Machine Learning from Wave Observation Data
Yao LUO1#+, Dongxiao WANG2, Weiqiang WANG1, Gang PAN1
1Chinese Academy of Sciences, China, 2Sun Yat-sen University, China
Ship wakes generated in relatively shallow estuaries are subjected to complex dynamic processes such as nonlinear wave evolution and wave-wave interaction, Identifying ship-wakes in coastal waters are important for maritime and coastal management, including waterway planning, shoreline protection, and navigation-related problems in busy waters. In this study, a machine learning framework was developed to identify ship-wakes using supervised training algorithms. Wave data were measured at two stations in the Pear! River Estuary in South China, The two stations are 1,500 m apart, one is at near-field of the navigation channel, and the other is at far-field, Two machine learning techniques, namely, the multilayer perceptron (MLP) model and support vector machine (SVM) model, are employed, We used two data formats in the training and testing processes one is the digital data of wave time series, the other is the spectrogram derived from the time series. Tests suggested that spectrogram is a more appropriate format for both models versus the time-series format, The SVM model has higher cross-validation scores and higher computational costs compared to the MLP mode. The trained models using the near-field data can be used for predictions at the far-field location with high accuracy. Sensitivity tests revealed that long primary waves and primary wake chirps are the most critical components in the spectrogram among overall ship-wake characteristics for ship-wake recognition, The time and frequency resolutions in the spectrogram only have minor effects on model performance.
OS13-A029
Application of Machine Learning in Sea Surface Temperature Prediction: A Case Study in the Bay of Bengal
Udana WANIGASEKARA, Yao LUO, Zhang ZHENQIU, Weiqiang WANG, Gang PAN#+
Chinese Academy of Sciences, China
Sea Surface Temperature (SST) observation and forecasting is of significant importance in oceanography, meteorology, climatology, marine biology, and disaster management. Effective prediction of SST through physical-based numerical models or data-driven statistic models have been investigated in several studies. Artificial intelligence techniques have rapidly emerged as powerful tools for modelling and monitoring the oceans, several statistic models involving Machine and Deep learning (ML and DL) had been used for SST prediction. The current study was conducted to investigate the applicability of several ML and DL models supported by Empirical Mode Decomposition (EMD) methods. 8 different ML and DL models were used in this study. During pre-prepare stage, EMD, Ensemble EMD (EEMD), and Complete EEMD with Adaptive Noise (CEEMDAN) were employed to decomposition the data. Contrary to previous study results on EMD-based SST modeling, the results of this study indicate that EEMD method-based models perform better than other decomposition methods. Compared to EEMD method’s accuracy (0.89<R2<0.97, 0.18<RMSE<0.33), other decomposition methods were less accurate (0.80<R2<0.95, 0.24<RMSE<0.42). The noise added throughout the decomposition process in EEMD may have allowed the models to better adapt to the chaotic SST time series data, resulting in higher accuracy. Comparing the results of 8 ML and DL models, the Long Short-term Memory (LSTM) model (0.87<R2<0.98, 0.19<RMSE<0.35) performed the best, with a close second being the Ensemble voting regressor (0.88<R2<0.97, 0.19<RMSE<0.33). For longer prediction lengths, LSTM becomes less stable causing Ensemble prediction accuracy to increase over LSTM. For 4-week ahead predictions, Ensemble accuracy was 0.76<R2<0.93 and 0.31<RMSE<0.47, while LSTM accuracy was 0.69<R2<0.92, and 0.33<RMSE<0.49. Also, due to the complexity, the time consumption of the LSTM model seems higher than Ensemble. Therefore, it might be preferable to use a less resource-consuming Ensemble model in SST prediction as it yields a result with similar accuracy to LSTM in less time.
OS13-A041
Tidal Amplification and Distortion Under Sea Level Rise in Coastal Channels of Macao
Keke LI1,2#+, Huabin SHI1
1University of Macau, Macau, 2Zhuhai UM Science & Technology Research Institute, China
In this study, the effects of sea level rise (SLR) on the tide of the coastal channels in Macao, west of the Pearl River Estuary, are numerically investigated. Changes in the tidal range, amplitude and phase-lag of major tidal components, and tidal asymmetry under four SLR scenarios (i.e., 0.21 m, 0.56 m, 0.93 m and 1.99 m) are studied. It is shown that under SLR most of the major tidal components are amplified and the tidal range in the coastal channels on the west of Pearl River Estuary increases. The increase of the tidal range versus the rising height of the sea level is almost linear. Besides, the tide is also distorted by the SLR with a significant change in the tidal asymmetry. Under a 1.99m-SLR, the flood-dominant tide in the coastal channels around Macao reverses to be the ebb-dominant. The key contributors to the change in tidal asymmetry are the changes in M4 and MS4.
OS13-A046
Experiments on the Characteristics of the Spatial Distribution of Friction Velocity on Wind Waves
Natsuki FUJITA#+, Toshinori OGASAWARA
Iwate University, Japan
Climate change due to global warming is affecting the climate system worldwide, and its effects are becoming increasingly evident in the form of higher temperatures, extreme weather events, and rising sea levels. In particular, rising seawater temperatures will alter ocean circulation and wind conditions and may also affect wave generation and development processes. Because the process is a highly complex sea-surface boundary process between two different fluids, gas and liquid, it is generally treated as a bulk formula for the sea surface drag coefficient, focusing on momentum transport via sea surface resistance in the momentum and energy transport process. Therefore, improving the bulk equation to be adaptable to realistic phenomena in future global climate change system predictions is necessary. In this study, PIV (Particle Image Velocimetry) measurements are performed using a wind tunnel tank (17 m long, 1.2 m high, 0.5 m wide) that can generate various types of wind waves, from ripples to whitecaps with breaking waves, in order to obtain areal velocity fields on wind waves. Vertical wind velocity profiles are obtained based on the air velocity data obtained from the PIV analysis. The friction velocity is obtained using the logarithmic law method and compared with previous studies based on the vertical distribution. Furthermore, we calculate the areal friction velocity using the eddy correlation method and clarify its distribution characteristics on various wind waves in space and time. Using these friction velocities, we will propose a new bulk equation.
OS13-A047
Hydraulic Experiments on the Dynamic Characteristics of a Spar-type Offshore Floating Body
Reo YOKOYAMA#+, Toshinori OGASAWARA
Iwate University, Japan
The introduction of renewable energy is expected to expand from the perspective of realizing a low-carbon society. There are many examples of offshore wind power generation in Europe due to favorable wind conditions and less restrictive installation conditions for wind turbines than those on land. Most examples are monopile-type structures in which the tower is fixed to the seafloor. There are few examples of floating spar-type wind power generation facilities because of many issues, such as the need for more clarity regarding their dynamic characteristics. In this study, hydraulic experiments are conducted to study the characteristics of spar-type floating body motions in irregular waves. Two spar-type floating models were used: single cylindrical (SC) and double cylindrical (DC). The center of gravity is 28 cm and 26 cm, respectively. The models were photographed from the side and the top of the tank by a high-speed video camera, and their swaying characteristics were clarified by image analysis. The results confirmed that the vertical direction motion of the "sway" was small regardless of the shape of the floating structure. On the other hand, the direction motion of the "surge" tended to be more significant. However, the movement was more pronounced for SC than DC, presumably because the DC has a lower center of gravity than the SC. Furthermore, spectral analysis revealed relationships between the various wave quantities and dynamic characteristics.
OS13-A049
Reconstruction of the North Sea Water Inflows in the South-eastern Baltic Sea During the Middle-late Holocene Based on Studies of Contourite
Daria LASKINA#+
Russian Academy of Sciences, Russian Federation
The Baltic Sea is a semi-enclosed brackish sea. It has a limited water exchange with the North Sea since 8500 BP. Dense, salty and oxygen-saturated North Sea waters irregularly inflow the deep basins and cause stratification and recurring hypoxia. Anthropogenic impact enhances eutrophication and increases hypoxia. The time variability of hypoxia and the role of climate influence on it during the Middle to Late Holocene are still poorly understood. The North Sea waters flow as near-bottom contour currents in deep basins of the Baltic Sea where they form erosive and accumulative morphological features such as contourite moats and drifts. The study of contourites helps to reconstruct these inflows with high time resolution. Two sediment cores were studied for paleore construction of the North Sea water inflows during the Middle to Late Holocene. The cores were collected in the contourite channel in the Gdansk Basin and the contourite drift in the Eastern Gotland Deep. An Olympus Vanta-C X-ray fluorescence analyzer was used for geochemical analysis, grain-size analysis was performed on a SALD2300 laser particle analyzer, and organic matter (OM) content was determined as loss on ignition. In both sediments cores, a ln(Zr/Rb) proxy correlates well with the mean of sortable silt fraction (10-63 μm), which is commonly used to study the intensity of bottom paleocurrents. Elevated values of ln(Zr/Rb) and are revealed for the Middle Holocene and correspond to intense and frequent inflows. A low OM content in the sediments is found in this interval. A decrease in the intensity of the bottom currents is recorded around 500 BP to the present, coinciding with an increase of the OM in the core from the East Gotland Deep and its decrease in the core from the Gdansk Deep. The weakening of intensity of near-bottom currents is also registered at 3000-500 BP.
OS13-A051
Impact of Tides on Sea Water Variability in the Coastal Region of Gyeonggi Bay in the Yellow Sea
Suran KIM1+, Tae-Sung KIM2, Kyung-Ae PARK1#, Jae-Jin PARK2, Moonjin LEE2
1Seoul National University, Korea, South, 2Korea Research Institute of Ships and Ocean Engineering, Korea, South
Turbidity quantitatively represents the degree of water transparency caused by suspended materials or organisms. The Yellow Sea in the Korean Peninsula, influenced by its shallow depth, tidal currents, and sediment from rivers, exhibits significant optical spatiotemporal variability. This study aims to analyze this variability using turbidity data from Gyeonggi Bay in the Yellow Sea to understand the optical characteristics of seawater and the coastal marine environment. The analysis of turbidity data through tidal harmonic decomposition and FFT revealed that the periods associated with astronomical tides M2, S2, K1, O1, and shallow water tides M4, MS4 were most predominant. Wavelet analysis identified intermittent points with strong energy at various temporal scales. The analysis of turbidity variation factors showed tidal influence to be dominant under normal conditions, but the impact of wind speed and rainfall increased during typhoons or heavy rain. By applying a seawater turbidity calculation algorithm using Sentinel-2 data, the study observed changes in the spatiotemporal distribution of turbidity in Gyeonggi Bay following tidal cycles and heavy rain. The results are expected to be useful in interpreting and monitoring turbidity changes in coastal waters using optical satellite data.
OS13-A052
Significant Wave Height and Wave Direction Variability in the Yellow Sea and East China Sea
Hye-Jin WOO#+, Kyung-Ae PARK
Seoul National University, Korea, South
In this study, seasonal and interannual variability of significant wave height (SWH) and wave direction in the Yellow Sea and East China Sea were analyzed using European Center for Medium-Range Weather Forecasts (ECMWF) Reanalysis 5 (ERA5) data for the period from 1993 to 2018. The ERA5 SWH and wave direction were validated using the measurement from the Ieodo Ocean Research Station (IORS). Bias and root-mean-square error were 0.1 m and 0.4 m, respectively. In the analysis of spatial distribution, the mean SWH ranged from 0.3 to 1.6 m in the Yellow Sea and East China Sea. It was higher in the southern region than in the northern region and higher in the center of the Yellow Sea than in the coast. The standard deviation of the SWH also showed a pattern similar to the mean, with a range of 0.3 m to 0.9 m. In the Yellow Sea and East China Sea, SWH and wave direction showed clear seasonal variability. SWH was generally highest in winter and lowest in late spring or early summer. Due to the influence of the monsoon, the wave direction propagated mainly to the south in winter and to the north in summer. In the Yellow Sea and East China Sea, it seems that the SWH has a complex interannual variability due to the influence of typhoons in summer.
OS13-A057
Retrieval of Sea Water Turbidity in Gwangyang Bay Using Sentinel-2 Satellite Data
Suran KIM1+, Tae-Sung KIM2, Kyung-Ae PARK1#, Jae-Jin PARK2, Moonjin LEE2
1Seoul National University, Korea, South, 2Korea Research Institute of Ships and Ocean Engineering, Korea, South
Understanding the optical characteristics and variability of the coastal environment can be achieved through the turbidity of seawater. Gwangyang Bay, located on the southern coast of the Korean Peninsula, is greatly influenced by tidal effects, terrigenous sediments from land, dredging, and the fishing industry. Therefore, there is a need to develop a satellite reflectance-based turbidity calculation algorithm suitable for Gwangyang Bay, as algorithms developed for the ocean or other regions show low accuracy. In this study, a database of match-up points between Sentinel-2 satellite data and in-situ turbidity measurements was produced. We investigated existing turbidity formulas, compared their accuracies, and selected the optimal wavelength band for the Gwangyang Bay to develop a turbidity calculation algorithm. The turbidity formula derived from satellite optical data is expected to contribute to understanding the turbidity variability of the Korean Peninsula's coastal waters and to rapidly acquire extensive marine environmental information.
OS13-A058
Development of Low-cost GPS Buoy for Observing of Nearshore Currents
Dongseob SONG#+
Kangwon National University, Korea, South
Due to the effect of submerged breakwater installed to prevent coastal erosion, the flow of nearshore currents is influenced to direction and speed of currents. Quantitative data acquisition and analysis results for nearshore currents are needed to evaluate the effectiveness of submerged breakwater for stability of sediment transport aspect. In this paper, we employed the cost-effective GPS equipment to acquire Lagrangian data of nearshore currents, which plays a foundational role in the analysis of ocean circulation. The used GPS receiver is DGPS data logger which is supported by the Satellite Based Argumentation System, and it is installed to a floating platform. The DGPS data logger can be measured positioning data per 1 second with continuous NMEA-0183 protocol during 24 hours. In the initial experiment, the trajectory path of the GPS buoy was sensitive to the influence of the incident wave, and the trajectory of the GPS buoy showed a very irregular pattern as the submerged breakwaters were gradually constructed. Especially, the GPS buoy was more appropriate in understanding the flow of the rip current caused by the leakage of the wave energy between the submerged structures as the three submerged breakwaters were successively constructed. Acknowledgement: This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2023-00280850).
OS14-A014
Vertical Stratification as a Key Factor for the 2020 Spring Bloom in the Yellow Sea
Go-Un KIM1+, Jaeik LEE1, Yong Sun KIM1, Jae Hoon NOH1, Young Shin KWON2, Meehye LEE3, Jongmin JEONG1, Jin-Young JEONG1#
1Korea Institute of Ocean Science & Technology, Korea, South, 2Korea Polar Research Institute, Korea, South, 3Korea University, Korea, South
The Yellow Sea, critical for marine ecosystems supporting Korean and Chinese populations, significantly decreased phytoplankton bloom intensity in Spring 2020. While a previous study attributed this decline to COVID-19-related nutrient reduction, our previous research proposed an alternative explanation, highlighting weakened thermal stratification and a concurrent surface cooling anomaly as primary causative factors. However, the intricate relationship between the marine environment and the ecosystem remains incompletely understood. Through the analysis of observational and marine physical-biogeochemical model data, we identified weakened stratification as a key factor suppressing the 2020 spring bloom. Enhanced vertical mixing hindered nutrient and chlorophyll-a accumulation in the euphotic zone, resulting in a diminished phytoplankton bloom. In contrast, reduced nitrate and phosphate concentrations in 2020 were insignificant compared to 2017–2019 levels, despite a notable decline in March 2020 PM2.5 due to the COVID-19 pandemic. By April 2020, nutrient levels fell within the range of interannual variability based on long-term observations, indicating a negligible impact on the spring phytoplankton bloom. This study provides valuable insights into the influential role of marine physical factors in shaping phytoplankton biomass dynamics in the Yellow Sea.
OS14-A016
Subsurface Photosynthetically Active Radiation(PAR) Responses to Tropical Cyclones
Junwoo LEE+, Hajoon SONG#, Kyungmin KWAK, Donghyuk KIM
Yonsei University, Korea, South
Photosynthetically Active Radiation (PAR) represents the solar radiation available for photosynthesis and plays a pivotal role in the growth of phytoplankton. While PAR typically decreases exponentially with depth, it is also affected by the substance in the ocean such as phytoplankton and colored dissolved organic matter (CDOM). Hence, understanding its vertical distribution requires a comprehensive investigation of both physical and biogeochemical process. However, there are not enough studies on subsurface PAR in this regard. In this study, we use a regional ocean biogeochemical model in the Northwest Pacific to examine how subsurface PAR changes after the passage of Tropical Cyclones (TCs). Generally, PAR near 530nm at a depth of 100 m decreases after TCs pass. This reduction occurs due to an increase in CDOM and/or chlorophyll-a near the surface, hindering the penetration of PAR to deeper levels. The extent and distribution of these patterns vary across regions, signifying that the TCs’ impact on subsurface PAR is related to the ocean’s background nutrient conditions.
OS14-A017
Contrasting Effects of Langmuir Circulation on Winter and Summer pCO2 in the Bering Sea
Kyungmin KWAK1+, Hajoon SONG1#, Yong-Jin TAK2, Junwoo LEE1, Donghyuk KIM1
1Yonsei University, Korea, South, 2Gangneung-Wonju National University, Korea, South
Enhanced ocean mixing has a significant influence on ocean dynamics and biogeochemical processes. Particularly, the Langmuir circulation is important in deepening the mixed layer depth and affecting the nutrient supply in the highly productive Bering Sea. In this study, we used a global ocean biogeochemical model to investigate the impacts of the Langmuir circulation on the carbon cycle. Langmuir circulation increased wintertime oceanic partial pressure of CO2 (pCO2) due to enhanced carbon supply through intensified vertical mixing. In contrast, it decreased summertime pCO2 by elevating nutrient supply and enhancing the biological sink. Our findings suggest that Langmuir circulation modulates the seasonal pCO2 variability in the Bering Sea.
OS14-A021
Dynamics of Mineral Recrystallization and Early Diagenesis in Deep Marine Carbonate Sediments: Insights from Walvis Ridge Along the Tristan-Gough Hotspot (IODP 391)
Siddhant KUMAR+, Seunghee HAN#
Gwangju Institute of Science and Technology, Korea, South
This investigation examined interstitial water geochemistry and mineral-fluid interactions in four drilled cores extracted from Walvis Ridge, an extensive segment of the Tristan-Gough hotspot trail (IODP expedition 391). We focused on deep marine carbonate sediments, providing insights into mineral recrystallisation and early diagenesis at relatively lower temperatures (ranging from 2 to 40°C) across varying geological epochs. The major proxy elements under consideration were Ca, Mg, and Sr, comprising over 80% of the carbonate fraction in the sediment. By employing interstitial fluid profiles of Mg/Ca and Sr/Ca in conjunction with age and depth, we ascertained diagenesis from the dissolution and precipitation rates of calcite. XRD analyses of the sediment column revealed further evidence of early diagenesis of dolomite at only two specific sites (U1575 and U1576), which are situated farthest from the hotspot among the four cores (the other two are U1577, and U1578). The Sr/Ca fluid profile suggested that the recrystallization of the predominant calcite in deep marine sections was largely completed within the upper few hundred meters, while the mineral cementation process typically occurred at subsequent stages. Through the correlation between fluid and recrystallized carbonate, specifically in terms of Sr/Ca and Mg/Ca, we estimated reaction rates. Our findings lead to the hypothesis that these reaction rates are ultra-low, supported by the absence of evidence in proximal sites and the observation of only slight diagenesis in more distant sites.
OS15-A005
Identification of Chlorophyll Rings Using Deep Learning with Attention Mechanism
Guangjun XU1,2#+, Zhixia LIN1, Yucheng SHI1, Changming DONG3,4
1Guangdong Ocean University, China, 2Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), China, 3Nanjing University of Information Science & Technology, China, 4Southern Marine Science and Engineering Guangdong Laboratory, China
Chlorophyll, as a key indicator of marine phytoplankton and primary productivity, plays a crucial role in guiding marine fisheries. Chlorophyll rings (CRs), characterized by elevated chlorophyll and phytoplankton concentrations along the peripheries of oceanic eddies, have been occasionally observed. With the rapid advancements in artificial intelligence, an increasing number of deep learning networks are being deployed in the field of marine science. This study employs a deep learning algorithm with an attention mechanism to identify CRs from chlorophyll concentration data. This algorithm demonstrates outstanding performance in capturing the distinctive feature of CRs, resulting in higher identification accuracy compared to traditional methods. This research contributes to a more comprehensive understanding of the relationship between chlorophyll distribution and oceanic eddies, thus enhancing our knowledge of mesoscale physical and biological interactions.
OS15-A006
A Case Study of Hybrid Wave Prediction Model - Keelung WEC Test Site
Chung-Lun KUO1#+, Wei-Ting CHAO1, Da-Wei CHEN2, Zhi-Xiang ZHANG3, Sheng-Jie LIN3, Shiaw-Yih TZANG3
1National Taiwan Ocean University, Taiwan, 2Axesea Technology and Engineering Consulting Company, Taiwan, 3National Taiwan University, Taiwan
To achieve the goal of “Net-Zero Emissions by 2050”, the development of marine energy is currently an important issue. In order to assess the site selection for Wave Energy Converter (WEC) and meet the requirement for rapid analysis of on-site wave data, we propose a Hybrid Wave Prediction Model for wave energy estimation and validate the results at the Keelung WEC test site. This hybrid model combines observed wave data, numerical wave models, and AI models. The observed wave data comprises hourly wave heights from three existing stations at the Keelung test site. The Simulating WAves Nearshore (SWAN) model is used for the numerical wave simulation, and the three common AI models, including Back Propagation Neural Network (BPNN), AutoRegressive Integrated Moving Average (ARIMA), and Long Short-Term Memory (LSTM), are selected and their comparisons are given. The results indicate that BPNN and LSTM exhibit better performance under the limitation of observed data length, which provide reasonable predictions for wave heights. The correlation coefficient and the Root Mean Square Error (RMSE) are 0.893 and 0.314 m for BPNN model, respectively. While the correlation coefficient and the RMSE are 0.892 and 0.286 m for LSTM model, respectively. The prediction of the proposed hybrid model can provide a reference for assessing the potential of wave energy and site selection for WEC.
OS15-A009
Forecasting Marine Heatwaves in the South China Sea Using Machine Learning
Chaorong MI1#+, Haixia SHAN1, Changming DONG1,2
1Nanjing University of Information Science & Technology, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China
Marine Heatwaves (MHWs), as extreme oceanic meteorological events, exert significant impacts on ecosystems and socio-economic activities in the South China Sea. With the ongoing global climate change, the application of machine learning methods in ocean prediction and ecological research becomes increasingly crucial for better understanding and adapting to future marine environmental changes. This study aims to explore a machine learning-based approach for predicting the occurrence of summer MHWs in the South China Sea. We collect and integrate data from the National Oceanic and Atmospheric Administration (NOAA)'s Optimum Interpolation SST version 2.1 dataset, ECMWF's ERA5 dataset, ECMWF S2S reforecast dataset, and the Madden-Julian Oscillation (MJO) data from the Australian Bureau of Meteorology. These datasets serve as input data for the prediction model. Various machine learning algorithms, including random forests and ridge regression models, are employed for model development. The research results indicate that, for regression forecasting with a 1-week lead time, the ridge model performs the best among all models. However, for longer lead times, all models exhibit lower accuracy, leaning towards climatology forecasts. In terms of classification forecasting, the random forest model outperforms others, demonstrating superior capability in predicting extreme MHW events compared to regular MHW events. The outcomes of this study not only hold the potential to enhance the marine heatwave warning system in the South China Sea but also provide valuable information for marine ecological conservation and fisheries resource management in the region.
OS15-A011
Using a Machine Learning Approach to Reproduce Vortices Merging of Rotating Platform Experiment
Xiangyu SHEN1#+, Changming DONG1,2
1Nanjing University of Information Science & Technology, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China
The digital twin of the rotating tank serves as a virtual representation of the real physical experiments. In this report, the research progress is presented in using artificial intelligent technology to reproduce merging process of eddies in island wake in laboratory experiments conducted in a rotating tank. The study focuses on determining the minimum spatiotemporal resolution required for successfully reproducing eddies in island wakes. Our findings implies that it is feasible to design a digital twin of the rotating tank based on AI and laboratory data.
OS15-A015
Reconstruction of Satellite-derived Sea Surface Temperature Under Cloud and Cloud-free Areas Using Artificial Intelligence Approach: A Case Study for the Adjacent Seas of Taiwan
Jing Tian LIM+, Yu-Chien CHENG, Chih-Chieh YOUNG#, Ming-An LEE, Jun-Hong WU
National Taiwan Ocean University, Taiwan
Sea surface temperature (SST) that has a broad impact to global climate, regional weather, marine resources, and coastal disasters is an important parameter. Generally, SST data collection is one of the most essential tasks for these scientific or practical research. Nowadays, the advanced remote-sensing techniques would provide a much wider range of SST observation in space. However, the application of satellites might be interference by the atmospheric activities (i.e., cloud). Previous studies have utilized the concept of data interpolation and empirical orthogonal function (DINEOF) for the reconstruction of SST under cloud and cloud-free areas. Nevertheless, some small-scale patterns of SST haven’t been faithfully captured and reproduced. In this study, therefore, we developed an artificial intelligence approach, i.e., a temporal-spatial radial-based function neural network (TS-RBFNN) with an outlier filtering process (OTS-RBFNN), to effectively reconstruct daily-averaged SST around the adjacent seas of Taiwan during summer time. The characteristics of SST and cloud ratio were analyzed, followed by the SST reconstruction and the performance assessment (in terms of the RMSEs). By comparison to the DINEOF, SST reconstructions using TS-RBFNN and OTS-RBFNN were greatly improved. In particular, free of the impacts of outliers, the OTS-RBFNN would ensure reasonable pattern learning and thus reduce the errors in the reconstructed SST.
OS16-A004
Severe Reduction in Spawning Area and Larval Abundance of Walleye Pollock Under Future Warming in the Western East/Japan Sea
Yong-Yub KIM1#+, Seung-Tae LEE2, Bong-Gwan KIM3, Yang Ki CHO3, Chung il LEE4, Sangil KIM5, Yong-Jin TAK4
1IBS Center for Climate Physics, Korea, South, 2University of California, Santa Cruz, United States, 3Seoul National University, Korea, South, 4Gangneung-Wonju National University, Korea, South, 5Pusan National University, Korea, South
Despite extensive efforts to recover the walleye pollock stock in the Korean fishing region after its collapse in the late 1980s, the issue remains unresolved. To explore the future prospects of walleye pollock in the western East/Japan Sea (EJS) during the late 21st century, we employed a dynamical downscaling approach, developing high-resolution regional ocean climate models (1/20°) using selected Coupled Model Intercomparison Project 6 (CMIP6) global climate models. Our analysis focused on examining changes in the spawning area and larval distribution of walleye pollock in the western EJS. Under the SSP5-8.5 global warming scenario, the suitable spawning period ratio of walleye pollock saw a significant reduction of 76%. This decline in spawning grounds in the western EJS was primarily attributed to ocean warming resulting from decreased atmospheric surface cooling. Additionally, our particle tracking experiment revealed a substantial loss of eggs and larvae south of 38°N. The study projects a severe collapse of walleye pollock in the western EJS and suggests various collapse patterns based on local circulation under future warming conditions. These findings alert us to the need for adopting fishery management strategies to address the collapse of walleye pollock under global warming.
OS16-A008
Development of Biases in the Indian Ocean and IOD in the UK Met Office Coupled Seasonal Forecasting System
Marimel GLER1#+, Andrew TURNER2,1, Linda HIRONS2, Caroline WAINWRIGHT3, Charline MARZIN4
1University of Reading, United Kingdom, 2National Centre for Atmospheric Science, United Kingdom, 3Cardiff University, United Kingdom, 4Met Office, United Kingdom
The Indian Ocean (IO) is unique in its interaction with the Asian monsoon system and exhibits multiple modes of climate variability on intraseasonal-to-interannual timescales. For example, the Indian Ocean Dipole (IOD), an important coupled mode of interannual variability of sea surface temperature (SST) in the equatorial IO, has been shown to influence Indian monsoon rainfall and flooding in East Africa. A positive IOD event in 2019 was thought to have influenced the delayed monsoon withdrawal, widespread Australian bushfires, and extreme flooding in East Africa during that year. Despite the socio-economic importance of the IO, the region suffers large biases in weather and climate models used for seasonal forecasts and climate projections. In this study, the development of systematic biases in the IO mean state and IOD in the initialised UK Met Office Global Seasonal Forecasting System version 6 (GloSea6) is examined. The coupled GloSea6 hindcast ensemble is used to investigate biases in the atmosphere and ocean, including the thermocline, that develop from months to seasons ahead of boreal summer (JJA) and autumn (SON) as a function of lead time. Preliminary results show that the summer monsoon likely plays a role in driving coupled circulation biases in the eastern equatorial IO, and the development of positive IOD-like biases in the mean state that grow into the SON season via Bjerknes feedback. To investigate biases in the IOD, composite analysis of biases during positive and negative IOD years is performed. The lead-time dependence of the biases and their sensitivity to initialisation date are investigated by analysing multiple initialised runs from February to November. This work will contribute to our understanding of biases in the Indian Ocean and IOD in weather models, and their likely sources, and thus the wider implications for predictability of the IOD.
OS16-A014
Influence of Intraseasonal Variability of Sea Surface Temperature in the Arabian Sea on the Summer Monsoon Precipitation Over the Bay of Bengal
Jingyuan XI#+
Second Institute of Oceanography, MNR, China
Summer monsoon precipitation over the Bay of Bengal (BoB) has pronounced intraseasonal variability (ISV), which has a close relationship to the local intraseasonal sea surface temperature (SST). Before heavy precipitation, intraseasonal SST in the BoB often has a warm anomaly and propagates northward, which drives the atmosphere and tends to trigger the convection. Besides the local air-sea interaction, the ISV of SST in the Arabian Sea (AS) also has an effect on the precipitation over the BoB. Results show that a prominent heavy precipitation usually occurs when the warm intraseasonal SST anomaly appears early in the AS and moves northward prior to that emerges in the BoB. The warm SST anomaly in the AS affects the sea level pressure and then trigger a southwestly wind anomaly in the center of AS. This wind anomaly promotes the wind convergence moving northward from the southern tip of Indian peninsula to the north India and northern BoB, which directly influence the vertical moisture advection and finally the precipitation. Understanding this process will be helpful to improve the predictive skill of the ISVs during the Indian Summer Monsoon.
OS17-A006
Spatiotemporal Variation of Anticyclonic Eddies in the South China Sea During 1993–2019
Jianyu HU#+
Xiamen University, China
Based on the absolute dynamic topography data from the Copernicus Marine Environment Monitoring Service, this paper applies the Topographic Position Index to develop a new approach for mapping the anticyclonic eddies in the South China Sea (SCS). The results show that anticyclonic eddies are active in the deep basin of SCS, and the five selected parameters (number or frequency, lifetime, kinetic energy, amplitude, and area or radius) of anticyclonic eddies have a similar temporal variation and a similar spatial distribution pattern. (1) As for monthly variations, anticyclonic eddies are active in late spring and most active in summer. (2) The El Niño–Southern Oscillation had a stronger impact on the inter-annual variations of anticyclonic eddies in the SCS before 2013, resulting in a significant transition of inter-annual variations of these five parameters in around 2004. After 2013, most of these five parameters had a minimum in 2015 and a maximum in 2017. (3) Analyses show that the eddy activities in the SCS are significantly influenced by the monsoon wind and the western boundary current like Kuroshio. Therefore, the areas southwest of Taiwan Island and east of Vietnam are the two areas where the anticyclonic eddies are most active, with much larger eddy kinetic energy and much higher eddy amplitude.
OS17-A007
Unraveling the Eddy-driven Heat Transport in the Agulhas Leakage Region
Lansu WEI1+, Chunzai WANG2#
1South China Sea Institute of Oceanology, China, 2Chinese Academy of Sciences, China
The Agulhas leakage, which transports warm and salty Indian Ocean water into the Atlantic Ocean, plays a crucial role in global ocean circulation and climate. The mesoscale eddies from the leakage supply the primary source of heat and salt for the Atlantic meridional overturning circulation. This study combines eddy data with Argo profiles from 1993 to 2018 to investigate the three-dimensional structures of eddies, advancing our understanding of eddy-induced transport. Our analysis revealed that both the trapping and stirring processes of eddies influence eddy-induced transport. Anticyclonic eddies are found to transport heat in the meridional direction mainly through propagation (~60%). On the other hand, cyclonic eddies transport heat meridionally to the Atlantic Ocean primarily through the stirring of isotherms in the background field (~25%). These results further confirm that the stirring effect of cyclonic eddies is crucial for evaluating the impact of the Agulhas leakage on the Atlantic Ocean.
OS17-A009
The Changes in the States of Atmosphere and Ocean, and Their Exchanges by Surface Current Coupling
Ajin CHO1+, Hajoon SONG1#, Hyodae SEO2, Rui SUN3, Aneesh SUBRAMANIAN4, Bruce CORNUELLE3, Matthew MAZLOFF3, Art MILLER5
1Yonsei University, Korea, South, 2Woods Hole Oceanographic Institution, United States, 3University of California San Diego, United States, 4University of Colorado Boulder, United States, 5Scripps Institution of Oceanography, United States
Air-sea interaction near the western boundary currents is characterized by the mesoscale oceanic forcing, such as eddies and sea surface temperature (SST) fronts, influencing air-sea fluxes. These so-called frontal-scale air-sea interaction has been mainly discussed in the context of the atmospheric responses to the SST. The surface current also influences the atmospheric boundary layer by modifying air-sea momentum fluxes. However, it has been remained unresolved how surface currents alter air-sea turbulent heat fluxes and how the effect differs from the change of momentum flux. In this study, we use a new approach to investigate two different surface current feedbacks, namely, the current feedback through the momentum flux (CFB_TAU) and the current feedback through the turbulent heat flux (CFB_Q) modifying each bulk formula for the air-sea fluxes and the following seasonal changes in the boundary layers. The effect of surface current coupling is found to be active with the strong currents and the sign of response depends on whether the low-level wind-current angle is smaller or larger than a critical value. Both instant and seasonal responses show the increase/decrease of air-sea momentum and turbulent heat fluxes if the low-level wind and surface currents are opposite/aligned and the change of surface heat fluxes influences the local atmospheric humidity, temperature, and SST. Also, surface current coupling impacts the path of Kuroshio main stream and the energetics in the Kuroshio extension. Our results indicate the importance of mesoscale oceanic forcing near the western boundary currents, not only by the SST but also by the surface currents.
OS17-A011
Global Impacts of Mesoscale Eddies on Mixed Layer Depth: Typical and Atypical Eddies
Junghee YUN+, Hajoon SONG#, Hyojun SEUNU, Kyungmin KWAK
Yonsei University, Korea, South
Widely distributed across the global ocean, mesoscale eddies, which are coherent rotating water vortices, exhibit distinct physical and biogeochemical characteristics compared to their surroundings. Typically, anticyclonic eddies display negative surface density anomalies, while cyclonic eddies exhibit positive surface density anomalies. These eddies play a crucial role in shaping the spatiotemporal dynamics of mixed layer depth: anticyclonic eddies contribute to deepening the mixed layer, while cyclonic eddies contribute to the shallowing of the mixed layer. However, recent studies have identified the frequent occurrence of atypical anticyclonic eddies with positive density anomalies and cyclonic eddies with negative density anomalies. The classification of eddies based on polarity makes it challenging to comprehend the effects of atypical eddies on mixed layer depth. Therefore, this study is aimed at comprehending the global impacts of both typical and atypical eddies on mixed layer depth by employing a high-resolution Community Earth System Model version 1.2.2 (CESM1.2.2) climate simulation project, with about 25 km horizontal resolution and 30 vertical levels in the atmosphere, and about 10 km horizontal resolution and 62 levels in the ocean. Initially, the eddies were classified into four groups based on the polarity and sign of the surface density anomaly within the eddy: typical anticyclonic, atypical anticyclonic, typical cyclonic, and atypical cyclonic eddies. These categories accounted for 30.1%, 17.1%, 35.9%, and 16.9% of the total eddies in the global ocean, respectively. The composite analysis revealed that both typical and atypical anticyclonic eddies contribute to deepening the mixed layer, while both typical and atypical cyclonic eddies contribute to the shallowing of it. However, it should be noted that the magnitude of atypical eddy-induced mixed layer depth anomalies is much larger than that of typical eddy-induced anomalies, particularly along western boundary currents. The physical processes related to these findings will be further discussed during the presentation.
OS17-A012
Seasonal Variation of Mesoscale Horizontal Stirring in the North Pacific Ocean
Gyuseok YI1,2#+, Wonsun PARK2, June-Yi LEE2
1IBS Center for Climate Physics, Korea, South, 2Pusan National University, Korea, South
The mesoscale horizontal stirring (MHS) is closely linked to various mesoscale dynamical phenomena, encompassing not only eddies but also meanders, filaments, and fronts. A clear understanding of its seasonality holds the potential to enhance our understanding of horizontal mixing and material dispersion. Here, we analyze the seasonal variation of MHS in the North Pacific surface ocean using ocean reanalysis (GLORYS12) current velocity data with a horizontal resolution of 1/12° from 1993 to 2019. Based on the characteristic of stirring to separate adjacent fluid trajectories, MHS is quantified using the finite-size Lyapunov exponent (FSLE), one of the Lagrangian diagnostics. The FSLE in the North Pacific shows clear seasonality but the phases of its evolution differ regionally. We identify two major modes, which contribute to over 80% of the seasonality of FSLE in the North Pacific, through the application of empirical orthogonal function (EOF) analysis to the climatological monthly mean FSLE. The first mode (57%) exhibits a variation peaking in April within the Kuroshio Extension region and the Subtropical Countercurrent region, where baroclinic instability plays a significant role. The second mode (25%) peaks during the summer season over the Kuroshio area and coastal upwelling areas of western North America. It is found that the strong seasonality in the upwelling area is induced by the North Pacific High.
OS18-A006
Comparison Between Coupled Models with High and Low Resolution for North Equatorial Countercurrent (NECC) Simulation
Ying LI1+, Yongqiang YU1#, Xuhua CHENG2
1Chinese Academy of Sciences, China, 2Hohai University, China
The North Equatorial Countercurrent (NECC) has obvious interannual variation, which will have an important impact on the global climate. The simulation results of the high-low resolution Fgoals-f3-H and Fgoals-f3-L coupled models of the FGOALS climate system were compared, and these results were combined with data from SODA assimilation to analyze the climate mean state, inter-annual variation characteristics, and specific relationship between NECC and ENSO during the period of 1994-2014. This study compared and analyzed the simulated and observed NECC interannual changes. It also defined the wind stress zonal transport, flow axis position, and simulated and reanalyzed NECC transport volume in the range of 0°–10°N. The ocean model in the high-resolution version of FGOALS-f3-H, which has a horizontal resolution of roughly 10 km, is capable of simulating the NECC's strength, location, and link to the New Guinea Coastal Current (NGCC) and the Mindanao Current (MC), two low-latitude western boundary currents. On the other hand, the simulated NECC contains several simulation faults, such as weak intensity, wide flow width, weak inter-annual variation, and shallow depth. The low-resolution version FGOALS-f3-L has a horizontal resolution of roughly 100 km. The outcomes demonstrated that the two versions' simulations of the NECC's interannual variations differed. The transport volume weakens and the NECC, as simulated by FGOALS-f3-H, travels closer to the equator during El-Nino years. FGOALS-f3-L's simulation of the NECC relocated closer to the equator and increased traffic flow. Subsequent investigation revealed that the base of the high-low resolution version was primarily located north of 2°N, whereas the NECC simulated by the latter might extend south to the equator. This explained the discrepancy between the results of the high-low resolution version at the equator, which was between 0° and 3°N.
OS18-A009
Current Status and Future Direction of the NIMS/KMA Argo Program
Baek-Jo KIM#+
Korea Meteorological Administration, Korea, South
In order to improve the predictability of marine high-impacts weather such as typhoon and high waves, the marine observation network is an essential because it could be rapidly changed by strong air-sea interaction. In this regard, the National Institute of Meteorological Sciences, Korea Meteorological Administration (NIMS/KMA) has promoted the Argo float observation program since 2001 to participate in the International Argo program. In this study, current status and future direction of the NIMS/KMA Argo program are presented through the internal meeting and external expert forum. To date, a total of 264 Argo floats have been deployed into the offshore around the Korean Peninsula and the Northwestern Pacific Ocean. The real-time and delayed modes quality control QC system of Argo data was developed, and an official regional data assembling center (call-sign ‘KM’) was run. In 2002, the Argo homepage was established for the systematic management and dissemination of Argo data for domestic and international users. The future goal of the NIMS/KMA Argo program was to improve response to the marine high-impacts weather through a marine environment monitoring and observing system. The promotion strategy for this was divided into four areas: strengthening policy communication, developing observation strategies, promoting utilization research, and activating international cooperation.
OS18-A013
Application of Gravity Interface Inversion Based on Improved 3D Varying Density Model in South China Sea
Shuling LI#+
China University of Geosciences(Beijing), China
The gravity data are among the most important data sets for studying deep crustal structures and the tectonic evolution in South China Sea (SCS). The interface inversion by gravity anomalies can effectively estimate the depth of Moho interface and crustal thickness. However, the Moho interface inversion in SCS is facing challenges due to the density contract of crust-mantle drastic vary in three dimensions, which are associated with the complicated crustal styles. To meet the challenges of 3D variation of density in SCS, we present a strategy by joint use an improved variable density model which is composed of multiple polynomials to describe the differences of different crusts and seismic data to be constraints to estimate the Moho depth. We examine the approach with a synthetic example and then apply this strategy to invert the Moho interface in SCS. The inversion results of gravity data in SCS show that the variable density model cooperating with seismic data constraints can improve the reliability of Moho inversion. Moreover, we calculate crustal thickness and stretch factor from inversion results to recognize major tectonics in the SCS. Our inversion results, crustal thickness and tensile conditions provide us important clues for understanding crustal structure and geological units in SCS.
OS18-A015
Early Emergence of Ocean Temperature Changes Under Climate Change
Yutong ZHENG#+, Kewei LYU, Jianyu HU
Xiamen University, China
The world ocean is experienced rapid warming under global warming. Ocean temperature changes at certain regions and depths may even already exceed the range of natural variability and become evident. In this study, based on an updated ocean observational dataset (IAP) over 1960-2022, we estimate the Time of Emergence (ToE) for 3-D ocean temperature changes, both at depth levels and along density surfaces (i.e., spiciness), to show where and when long-term change can emerge from natural variability. The results show that there is a comparable early emergence for both temperature and spiciness changes in Atlantic, but with a broader region for temperature changes. For comparison, spiciness changes in Pacific and Indian Oceans generally emerge earlier than temperature changes, especially in southern hemisphere. From the spatial pattern of ToE in different neutral density surfaces, the spiciness changes mainly emerge in the density range of Subantarctic Mode Water and Antarctic Intermediate Water, especially in Pacific and Indian Oceans which correspond to its vertical distribution. The mechanisms for early emergence of ocean temperature changes are under investigation.
OS18-A016
Fuzzy Cluster Analysis of Water Mass in the Western Taiwan Strait in Spring 2019
Jia ZHU#+
Xiamen University, China
The classification of the springtime water mass has an important influence on the hydrography, regional climate change and fishery in the Taiwan Strait. Based on 58 stations of CTD profiling data collected in the western and southwestern Taiwan Strait during the spring cruise of 2019, we analyze the spatial distributions of temperature and salinity in the investigation area. Then by using the fuzzy cluster method combined with the T-S similarity number, we classify the investigation area into 5 water masses: the Minzhe Coastal Water (MZCW), the Taiwan Strait Mixed Water (TSMW), the South China Sea Surface Water (SCSSW), the South China Sea Subsurface Water (SCSUW) and the Kuroshio Branch Water (KBW). The MZCW appears in the near surface layer along the western coast of Taiwan Strait, showing low-salinity (<32.0) tongues near the Minjiang River estuary and the Xiamen Bay mouth. The TSMW covers most upper layer of the investigation area. The SCSSW is mainly distributed in the upper layer of the southwestern Taiwan Strait, beneath which is the SCSUW. The KBW is a high temperature (core value of 26.36oC) and high salinity (core value of 34.62) water mass located southeast of the Taiwan Bank and partially in the central Taiwan Strait.
OS18-A019
Potential Error Underestimation of Cross-validation in Missing Value Reconstruction in Ocean Satellite Data
Menghan YU#+, Haoyu JIANG
China University of Geosciences, China
Ocean remote sensing datasets often have the problem of missing values due to various reasons. However, many researches require spatiotemporal seamless data. Data reconstruction methods are commonly used to obtain such gap-free datasets. In reconstructing satellite remote sensing data, randomly masking original data for progressive cross-validation is a common method to indicate the performance of reconstruction. In this study, the accuracy of this validation method is analyzed. We artificially constructed two data missing patterns using the SST data in the East China Sea, one simulating natural cloud coverage and the other randomly masking the same percentage of original data. The results of reconstruction for the two types of masking were compared. The RMSE (root mean square error) of datasets that simulate real cloud coverage is more than 50% higher than that of the dataset randomly masking data, regardless of the data missing rate. This result implies that the error of satellite data gap-filling is underestimated when random masking of original data is applied for progressive cross-validation, which should be treated with care in applications.
OS18-A020
Estimation of Tropical West Pacific Ocean Acidification Rates Using Porites sp. Boron Isotopes
Timothy Glenn IRINGAN1#+, Charissa FERRERA1, Fernando SIRINGAN2, Christopher STANDISH3
1University of the Philippines Diliman, Philippines, 2University of the Philippines, Philippines, 3University of Southampton, United Kingdom
The process of decreasing seawater pH due to increasing atmospheric carbon dioxide known as ocean acidification is a global phenomenon with very strong regional effects. In the absence of an observational time series program, the relative abundance of carbonate boron isotopes (δ11B) is proven to be a viable indicator of seawater pH. Recent analytical developments that enable correction for an interference from scattered ions allow accurate and precise measurement of δ11B on carbonate by laser ablation multi collector inductively coupled plasma mass spectrometry (LA-MC-ICP-MS) irrespective of mass spectrometer model. Massive, long-lived corals are, in particular, prime candidates for time series reconstructions to a sub-monthly resolution using this method. In this study, cored samples of Porites sp. from two sites in the Philippines are subjected to elemental and boron isotope analysis at the University of Southampton. The first core from Ayuki Island, Surigao is fed by the North Equatorial Current and influenced by Pacific signals such as the El Niño Southern Oscillation. The second core in Mabini, Batangas is within a submarine groundwater discharge field with reported acidified conditions that are potentially comparable to future enhanced scenarios. This study aims to correlate different environmental drivers to variations in local pH using geochemical proxies. Palaeothermometry indicators will be calibrated against multi-scale ultra-high resolution satellite data, which will be used with coeval δ11B to derive the pH of the calcifying fluid. The remaining parameters will be calculated using the CO2sys program. Preliminary results show strong covariation among magnesium, strontium, uranium, and boron, which alludes to the former three elements’ shared sensitivity to temperature. Both the elemental and isotope data will be used to elucidate how the carbonate chemistry of Surigao and Mabini behaved for over 40 and 20 years, respectively.
OS18-A023
The Chinese Air-sea Heat Flux (CASFlux) Gridded Dataset: Description, Validation, and Application
Rongwang ZHANG#+
Chinese Academy of Sciences, China
As a new member of the global family of air-sea heat flux gridded datasets, this paper introduces the main production processes and and evaluates the performance of the first version of Chinese Air-Sea Heat Flux gridded dataset (CASFlux). CASFlux absorbed multi-source satellite remote sensing and reanalysis data and was trained by in situ observations from moored buoys, offshore platforms, flux towers, and so on. Machine learning and state-of-art parameterization algorithms were employed in the production of CASFlux. Compared to those extensively used flux products, CASFlux has significant regional advantages in the seas around China. In addition, CASFlux also performs well in some areas outside of the seas around China. Examples of the application of CASFlux in studies of long-term changes in air-sea heat flux, tropical cyclones, and marine heatwaves were provided. Next, more observations from areas outside of the seas around China will be used as validation and training data for the optimization and improvement of CASFlux, in order to continuously improve its performance in global oceans.
OS18-A032
Validation of NOAA-20/VIIRS Sea Surface Temperature and Error Characteristics in the Northwest Pacific
Hee-Young KIM+, Kyung-Ae PARK#
Seoul National University, Korea, South
In this study, data of infrared Sea Surface Temperature (SST) obtained from the next-generation high-resolution radiometer VIIRS on the NOAA-20 satellite were collected and collocated with in-situ measurements to verify accuracy in the Northwest Pacific. Data spanning from May 2020 to June 2023 were utilized, resulting in the generation of 75,700 match-up points. The NOAA-20/VIIRS SST showed a mean Root-Mean-Square-Error (RMSE) of approximately 0.52 K and a mean bias of -0.12 K when compared to SST observations from surface buoys. These values exceeded the accuracy of VIIRS SST reported in previous studies conducted in global oceans. Analysis of NOAA-20 SST error characteristics revealed seasonal variations, with negative biases observed in winter and spring, while positive biases were prominent during the summer. Additionally, diurnal variations were observed, with maximum RMSE and maximum positive biases occurring around 15-16 hours, and minimum RMSE and minimum biases around 22-24 hours. Furthermore, the errors in NOAA-20 SST were influenced by factors such as wind speed, satellite zenith angle, distance from the coast, and the gradient magnitude of SST. Generally, the mean bias of SST tended to increase positively with wind speeds above 14 m/s and increase positively or negatively with decreasing wind speeds below 5 m/s, depending on daytime or nighttime. Additionally, a larger satellite zenith angle led to a significant expansion of the SST error range. The proximity to the coastline (within 300 km) was associated with increased SST errors. Larger spatial gradients of SST amplified the average RMSE of satellite SST. Considering the distinct characteristics of SST accuracy and error patterns in regional seas, especially in the seas around the Korean Peninsula, this study emphasizes the need for a deeper understanding of the variations and distribution of SST errors.
OS18-A037
GNSS-R Multi-frequency Multi-system Loose/tight Combination Real-time Water Surface Altimetry Approach
Ziheng WU#+, Fei GUO
Wuhan University, China
GNSS-R technology is a new technology to study the height change of horizontal surface in recent years, which has the advantages of low cost and high time resolution. In this paper, a dual-antenna multi-system multi-frequency GNSS-R real-time water surface altimetry algorithm is investigated, which can solve the water surface altitude result by calendar element, and the real-time altimetry result on the calm water surface, such as lake surface, has an RMSE of 1.13cm; because of the small number of satellites received by the reflector antenna, the impact of loose/tight combination of double-difference model algorithms on the water surface altimetry accuracy is compared in this paper. The results show that in the case of fewer than about 15 valid satellites, the tight combination model can significantly improve the accuracy of the measurement; on the contrary, in the case of sufficient satellite data, the loose combination model has a faster convergence speed and higher accuracy.
OS18-A042
Progress in Attributing Mass Sea Level Change Over the Satellite Altimetry Period
Yuxin LIU1+, Shanshan DENG1#, Wenxi ZHANG1, Ange HU1, Yashan CHENG2
1Guangxi University, China, 2Officers College of PAP, China
In the context of climate change, water mass transpositions between the land and the ocean are dynamically balanced. The physical processes involved in terrestrial freshwater input driving mass sea level rise are complicated. It includes gravitational changes, Earth’s rotation changes, and solid Earth deformations in response to past and present-day global water mass redistributions, referenced as glacial isostatic adjustment and sea level fingerprints, respectively. In addition, the ocean dynamic processes driven by wind and thermal gradients are included. The Gravity Recovery and Climate Experiment (GRACE) mission has achieved innovative independent observations of the global gravitational field, which supports the exploration of the mechanisms of mass sea-level change over the last 20 years. However, mass sea level change over longer periods is poorly known due to limitations in the gravity field data. For this reason, this study provides a comprehensive investigation of the key factors driving ocean mass anomalies over the 1993–2018 period. The process utilizes the ERA5 reanalysis dataset's monthly averaged sea-surface wind products, the Center of Space Research's GRACE Release 06 Version 02 Mascon solutions, the Copernicus Climate Change Service's grided sea level anomaly products, the grided steric sea level anomaly products, and the terrestrial water storage reconstruction products. Also, sea level equations, maximum covariance analysis methods, and time series decomposition reconstruction methods are employed. The study aims to reproduce the physical processes of sea level mass change associated with land-to-ocean mass transposition. It is found that modeled sea level fingerprints are detectable but highly uncertain at inter-annual scales, and that an attribution study of low-frequency changes in global mass sea level during satellite altimetry periods is more plausible.
OS19-A007
Interannual Variation of Submesoscale Kinetic Energy in the Northeastern South China Sea Revealed by Numerical Simulations
Jinchao ZHANG+, Zhiwei ZHANG#
Ocean University of China, China
Although the seasonal variation of submesoscale processes has been well studied in the northeastern South China Sea (NE‐SCS), less attention has been devoted to the interannual variation. Based on the output from a submesoscale permitting hindcast simulation from 1991 to 2019 (with 1/30° horizontal grid spacing), interannual variation and modulation mechanisms of the submesoscale kinetic energy (KE) in the NE‐SCS are investigated in this study. The submesoscale KE is characterized by strong interannual variability, displaying larger magnitudes in 1993, 1998, 2004, 2015, and smaller magnitudes in 1997, 2001, 2009, and 2013. Further analysis suggested that interannual variability of submesoscale KE in the NE-SCS is primarily modulated by the mesoscale strain rate and mixed layer depth simultaneously. These variation are partially explained by the available potential energy (APE) release at submesoscale driven by frontogenesis-modulated mixed-transitional layer instability in winter.
OS19-A012
Steric Heights of Submesoscale Processes and Internal Gravity Waves in the Subtropical Northwestern Pacific and Northern South China Sea as Revealed by Moored Observations
Mingfang MIAO+, Zhiwei ZHANG#, Jinchao ZHANG, Yue WANG, Jiwei TIAN, Wei ZHAO
Ocean University of China, China
The Surface Water and Ocean Topography (SWOT) altimeter mission provides a good opportunity to globally detect submesoscale processes (submesoscales) from high-resolution sea surface height (SSH) measurements. However, in addition to the balanced mesoscale eddies and submesoscales, the measured SSH also contains signals of unbalanced internal gravity waves (IGWs) including internal tides (ITs) and supertidal IGWs (IGWs with frequencies of 3–8 cpd). Therefore, a quantitative understanding of the contributions of the above multiscale dynamic processes to the SSH is a prerequisite for exploring submesoscales from the SWOT-derived SSH data. Here, this issue was investigated through analyzing one-year moored observation-derived steric heights (SHs) in the subtropical northwestern Pacific (NWP) and northern South China Sea (SCS). In the sense of annual mean, the root-mean-squared (RMS) SHs of submesoscales and IGWs in the SCS are 1.30 and 5.54 cm, respectively, while they are only 0.70 and 3.19 cm in the NWP. Seasonally, the RMS SH of submesoscales is larger in winter than summer in both regions; with respect to the IGWs, their RMS SH is larger in summer than winter in the SCS but it is opposite in the NWP. Generally, the SHs of diurnal and semidiurnal ITs are dominated by the stationary component in both regions but the proportion of the nonstationary component is much larger in the NWP than the SCS. The sum of the SHs by nonstationary diurnal and semidiurnal ITs exceeds that of submesoscales except in winter in the SCS. Furthermore, we also found that the SHs of supertidal IGWs are always larger than those of submesoscales in both regions and both seasons. We also found that for all of the IGWs bands, the SHs are overwhelmingly attributed to the first mode. The results in this study will provide useful information for the application of SWOT data.
OS19-A013
Observations and Simulations of the Yellow River Plume Fronts
Zhixing CHEN+, Tao WANG#, Dan XU, Wensheng JIANG, Changwei BIAN
Ocean University of China, China
River plume fronts are with spatial scales of O(0.01-10) km and time scales of O(0.1-10) days, thus belonging to small- and submeso-scale structures. Although the estuarine and coastal communities rarely use the terminology “submesoscale currents (SMCs)” to describe plume fronts, they do have similar dynamical signals to SMCs in the open ocean, including strong horizontal buoyancy gradients, significant vertical velocities, horizontal convergence, and enhanced turbulent mixing. In this study, we conducted moored observations and numerical simulations to study the Yellow River plume fronts and their effects on biogeochemical processes. The river plume exhibits recurrent and sharp fronts under the effects of the geometry and strong tidal currents. A turbulent bore is observed to be generated at the front and transport the near-surface water with low turbidity and high dissolved oxygen into the water column. Under the effects of vertical mixing and cross-front currents, a three-layer structure of turbidity is formed behind the front. Through numerical simulations, we find that fronts play significant roles in salinity mixing of the plume region. Although frontal zones only occupy about 8% of the plume area, they are estimated to mix 28% of the buoyancy input.
OS19-A014
Submesoscale Processes in the Northern Red Sea: Insights from Underwater Glider Observations
Fushuo CHU1, Xiaolong YU2, Georgios KROKOS3, Ibrahim HOTEIT3, Khaled ASFAHANI3, Peng ZHAN1#+
1Southern University of Science and Technology, China, 2Sun Yat-sen University, China, 3King Abdullah University of Science and Technology, Saudi Arabia
The critical role of oceanic submesoscale currents in promoting energy cascade and modulating biogeochemical processes, as well as the heat budget in the upper ocean, has gained wide recognition. While high-resolution numerical simulations have enabled qualitative investigation of the spatiotemporal variability of submesoscale processes in the North Red Sea (NRS), observational evidence remains scarce. This study presents field observations by an underwater glider and provides insights into the mechanisms of submesoscales in the NRS. High-resolution glider and satellite observation data reveal submesoscale frontal features and deep mixed layer depths during winter. Diagnosis of potential vorticity and classifications of submesoscale instabilities demonstrate conducive conditions for the mixed-layer baroclinic, gravitational, and symmetric instability. Significant negative PV associated with robust fronts promotes the development of submesoscale processes. It is worth noting that submesoscale processes exhibit significant vertical motions, which could penetrate through the mixed layer. The findings demonstrate that robust fronts are capable of inciting non-trivial vertical heat transport in subtropical oceans, which are characterized by pronounced stratification. Biogeochemical observations suggest that coherent pathways via submesoscale processes lead to the vertical transport of biomass and oxygen patches, supp lying nutrients into the euphotic layer and ventilating hypoxic waters at depths. These results evidence the fundamental role played by submesoscale frontal dynamics in subtropical ocean basins.
OS19-A019
Spatio-temporal Variability of Submesoscale Suspended Sediment and Sea Surface Temperature Fronts in the Bohai Sea: Observations from Satellite Ocean Color Measurements
Tao WANG#, Weichen XIE+
Ocean University of China, China
Submesoscale fronts are ubiquitous in the ocean and play a significant role in energy transfer, mass transport, and biogeochemical processes. The spatio-temporal characteristics of submesoscale suspended sediment (SS) and sea surface temperature fronts (SST) in the Bohai Sea were investigated by the Moderate Resolution Imaging Spectroradiometer/Aqua (MODIS/A) products over the period 2003-2016. An improved gradient-based edge detection algorithm was implemented to extract submesoscale fronts with desirable results. Frontal probability (FP) was used to quantify the intensity of frontal activity. The results showed that submesoscale fronts in the Bohai Sea are limited by topography in spatial distribution, which were mainly located in the shallow coastal regions, the Bohai Strait, and the areas around islands and headlands. By performing empirical orthogonal function (EOF) decomposition analysis correlation analysis with several potential environmental factors, we found that the FP of the submesoscale SS and SST fronts both exhibited pronounced seasonality. However, their seasonal variations differ due to the different driving processes. These findings contributed to a clearer understanding of the submesoscale processes in the Bohai Sea and could inform ecological and environmental governance in this region. The novel algorithm for detecting submesoscale fronts can also be used to inform and validate the study of submesoscale fronts in other regions or even globally.
OS19-A028
Asymmetries Between Phases of Atlantic Multi-decadal Variability in the CMIP6 Multi Models
Haedo BAEK1#+, Dong Eun LEE1, Young Ho KIM2, Young Gyu PARK3, Hye-Ji KIM1, Eun Young LEE1, Ju AH-HYUN1, Myeong Mo KANG1, Minsu SONG1
1Chungnam National University, Korea, South, 2Pukyong National University, Korea, South, 3Korea Institute of Ocean Science & Technology, Korea, South
The Atlantic Multidecadal Variability (AMV) is a phenomenon in which North Atlantic Sea Surface Temperature Anomalies (SSTA) occur almost simultaneously in the subpolar and tropical regions, imprinting its impact not only in neighboring countries, but also in the global climate system. Due to its long lifespan, the natural variability associated with AMV seriously amplifies uncertainty of the future climate projections, as the exact mechanisms of the AMV remain unknown despite numerous previous studies. In this study, we investigate the asymmetry in two opposite AMV phases in different models using preindustrial control experiments from 46 different models participating in Coupled Model Intercomparison Project 6. When the model sensitivity between two opposite AMV phases in each model is investigated, it is found out that the strength and phase preference in terms of the tropical SSTA sensitivity to subpolar SSTA widely varies, resulting in AMV+ preferred groups, AMV+ preferred groups, or symmetric AMV groups. Among the three groups, it is most notable with the AMV+ preferred models that the net surface heat flux in the subpolar Atlantic adds heat from the atmosphere into the ocean during the positive AMV phase due to a robust hemispheric reduction of the Westerly and the Trades. In contrast, with the AMV+ preferred model during negative phases of AMV, or all other model groups during both AMV phases, the subpolar SSTAs associated with AMV originate from the ocean, rather than the atmosphere. The contrast can be the results of competition between subpolar and tropical SST influences, involving the surface ocean feedback in Tropical Atlantic. As the AMV+ positive group shows significantly larger weakening of the westerlies and trade winds during AMV+, Wind-upwelling-SST feedback associated with the equatorial convergence further intensifies the tropical positive feedback, in addition to the Wind-Evaporation-SST feedback. Asymmetry resides in the vertical stratification in Tropics.
OS19-A031
Understanding the Central North Atlantic Cold Bias in CMIP6 Models
Xia LIN1#+, Francois MASSONNET2, Pablo ORTEGA3, Helena Barbieri DE AZEVEDOB2, Xiaoming ZHAI4, Amanda FRIGOLA3
1Nanjing University of Information Science & Technology, China, 2Université Catholique de Louvain, Belgium, 3Barcelona Supercomputing Center, Spain, 4University of East Anglia, United Kingdom
The Central North Atlantic (CNA) sea surface temperature (SST) cold bias is a well-known issue in contemporary climate models, but the underlying causes are still not fully understood. In this study, we aim to characterize this CNA cold bias in the climate models that participated in the Coupled Model Intercomparison Project, phase 6 (CMIP6), investigate the possible causes of the CNA cold bias through an energy budget analysis, and discuss the possible ways to reduce the cold bias. Our findings reveal that the primary cause of the cold bias lies in an underestimation of the North Atlantic Current in the models, which results in an underestimation of the horizontal heat transport into the central CNA region. Furthermore, it is shown that the CMIP6 models tend to overestimate CNA air-sea turbulent heat fluxes, but we suggest that this overestimation is a consequence rather than a direct cause of the CNA cold bias. We further investigate the impact of spatial resolution on the accuracy of modeling surface currents and CNA SST. Two climate models show improvement in the strength of the North Atlantic Current and CNA SST when transitioning from coarse (~1o) to eddy-permitting (~0.25o) resolutions. However, this improvement is not universally observed across all climate models. Then, we discuss the importance of improving the mesoscale and sub-mesoscale parameterizations in climate models to well capture the strength and position of North Atlantic Current and related heat transport.
OS19-A035
Thermohaline Staircases Disrupted by Mesoscale Eddies in the Eastern Caribbean Sea Observed from Marine Seismic Data
Shun YANG1#+, Kun ZHANG1, Haibin SONG1, Barry RUDDICK2, Mengli LIU1, Linghan MENG1
1Tongji University, China, 2Dalhousie University, Canada
Thermohaline staircases and mesoscale eddies play crucial roles in the transport of heat, salt, and nutrients in the ocean, yet their complex relationship remains unclear due to the limitations in observational resolution. This study, utilizing high spatial resolution seismic images spanning 2518 km, reveals the widespread occurrence of thermohaline staircases and six subsurface mesoscale eddies in the eastern Caribbean Sea. The three-dimensional distribution of these features is demonstrated, with staircases spanning 70% of the seismic lines at depths ranging from approximately 400 to 600 m. Due to the shearing action of eddies, these staircases are disrupted and interrupted by six subsurface mesoscale eddies. The degree of disruption varies depending on the intensity of the shear. The high-resolution seismic images offer a clear and comprehensive illustration of how eddies disrupt staircases, enhancing our understanding of the intricate fate of these oceanographic phenomena.
OS20-A004
Transport Rate for Quantifying Local Physical Transport and Retention Conditions in Estuaries
Qubin QIN1#+, Jian SHEN2
1East Carolina University, United States, 2Virginia Institute of Marine Science, United States
The transport rate serves as a valuable metric alongside the commonly used transport timescales, aiding in the assessment of local transport dynamics within estuarine and coastal environments. In this presentation, we will emphasize a specific transport rate computed through tracer release, providing a means to quantify the local transport condition for long-standing autochthonous constituents originating from the system. The transport rate is computed in Chesapeake Bay, the largest estuary in the U.S.A., which clearly describes the temporal and spatial variations of local transport and retention conditions. In addition, we show that the transport rate can also be used to diagnose the relative importance of physical transport and retention compared to other environmental factors influencing the dynamics of reactive autochthonous constituents. As an example, the transport rate is used to evaluate the contribution of physical transport to variations in phytoplankton biomass in the James River, a tributary of Chesapeake Bay. Given the advantages, the transport rate provides an efficient tool for diagnosing local transport conditions modulating dynamics of autochthonous constituents and phytoplankton bloom in estuarine and coastal systems.
OS20-A006
Fate of Dissolved Organic Nitrogen in the Pearl River Estuary: Mixing or Biological Transformation
Xiaoping HUANG#, Yunchao WU+, Jinlong LI
Chinese Academy of Sciences, China
Estuaries are key areas for terrestrial material transport and marine biogeochemical processes, particularly those of dissolved inorganic nitrogen (DIN) and dissolved organic nitrogen (DON). However, the fate of DON in estuaries with a high runoff remains poorly understood. In this study, we explored the translocation and transformation of DON in the Pearl River Estuary (PRE) and adjacent coastal areas of southern China based on DON concentrations, optical and fluorescence characteristics, and environmental parameters. The results revealed that DIN and DON exhibited dissimilar distributions. The distribution of DIN was primarily influenced by freshwater-seawater mixing. In contrast, biological processes and freshwater-seawater mixing shaped the distribution of DON. High levels of DON in the terrestrial-dominated zone were predominantly anthropogenic sources through terrestrial inputs, whereas DON in the freshwater-seawater mixing zone and seawater-based zone were mainly influenced by biological activities, as high concentrations of Chla were observed in these two areas. DON exhibits fast dilution in low-salinity areas and retention in moderate-salinity areas (freshwater-seawater mixing area) in summer and winter, while undergoes a rapid decrease in open water areas during winter. Consequently, DON in the PRE and adjacent coastal areas exhibited nonconservative mixing despite seasonal variations. These findings provide novel insights into the role of DON in nitrogen biogeochemical processes in river-dominated estuaries and adjacent coastal areas.
OS20-A008
Modeling Estuarine Hydrodynamics and Dissolved Pharmaceutical Contaminant Transport Using DELFT3D-FLOW in Manila Bay, Philippines
Ann Elizabeth ENOVA1#+, Shyrill Mae MARIANO1, Randolph SINGH2, Diana AGA2, Cesar VILLANOY1, Caroline Marie JARAULA1
1University of the Philippines, Philippines, 2University at Buffalo, United States
Hydrodynamic modeling using simple open-source tools, such as DELFT3D-FLOW, coupled with quantification of the concentration of dissolved pharmaceutical and personal care products (PPCPs) in major rivers is valuable and useful for predicting transport of pollutants. PPCPs have become contaminants of emerging concern globally due to their increasing prevalence and effects on ecosystems and human health. This study used LC-MS to determine PPCP concentration in major rivers of Manila Bay, modeled pharmaceutical contaminants transport inside Manila Bay using an open-source software, DELFT3D-FLOW, and explored key factors affecting the pollutant transport model and its applicability to other urban coastal estuarine systems. Anhydro-erythromycin and caffeine were among the most frequently detected PPCPs in Pasig River and Pampanga River. The variation in land use (i.e urban, agricultural) and geographic concentration of hospitals affect the distribution of PPCPs. Through the model, it was determined that PPCP mostly comes from the Pasig River flowing south towards Parañaque and Cavite during the Southwest monsoon but moving northwest to Bulacan and Pampanga during the Northeast Monsoon. In a coastal estuary, river discharges significantly contribute to the resulting water circulation and pollutant transport trends. The predicted concentration of PPCPs are affected by non-point sources, which are challenging to account for in modeling. Seasonal factors, such as wind and tide, alter the concentration and direction of transport. Hydrodynamic modeling using DELFT3D-FLOW may be used to identify areas with high risk of exposure to other pollutants in other coastal estuarine systems. It is recommended to conduct targeted analysis of PPCPs in fish, corals, mussels, and sediments in Manila Bay. Additionally, management of the increasing occurrence of pharmaceutical contaminants in aquatic ecosystems need a multi-step and trans-disciplinary approach. This includes lowering usage and dosage of pharmaceuticals, better product design, and ensuring proper wastewater treatment systems.
OS20-A015
An Experimental Evaluation of Degradation of Cage Nets Under Different Environmental Conditions
Beema JIHAN1, Ashna ABBAS1, Firdhouz MOHAMED R1, Jithu RAVI1, Priya K. L.1, Gubash AZHIKODAN2#+, Katsuhide YOKOYAMA2
1TKM College of Engineering, India, 2Tokyo Metropolitan University, Japan
Cage farming is an emerging technique of raising aquatic organisms especially fishes, in a different aquatic environment. Nets play a crucial role in cage farming operations by containing and protecting the cultured organisms, allowing water to flow through them, for oxygenation, waste removal and preventing escape or predation. Different types of materials like nylon, polyester and HDPE are used for making nets. The choice of nets and their specifications can vary widely depending on the species being farmed, the specific goals of the aquaculture operation, and the environmental conditions of the farm site. It is very necessary to select a particular material to maintain the nets to ensure the success of cage farming operations, for the intended purpose and for the overall well-being of the cultured organisms. The materials of the net are susceptible to physical and chemical degradation due to environmental conditions such as salinity, pH, turbulence, sunlight etc. and can pose hazard to the farmed fishes and thereby enter the food chain. In order to study the pathway of degradation of the commonly used nets (namely HDPE, nylon and polyester), laboratory control experiments were carried out under exposure to salinity, natural sunlight and UV light, under dry and wet conditions. The weight loss experienced during different intervals of time as well as the microplastics generated during the experimental period were examined and the changes in polymeric characteristics were arrived at. A three-month study indicates the degradation of materials, especially those immersed in water. Among the materials, it was observed that Polyester shows a minimum change in the dry weights before and after immersion. However, the change visible for materials in the absence of water is negligible, which shows slow degradation of materials in dry conditions.
OS21-A009
Evaluation and Projection of Global Marine Heatwaves Based on CMIP6 Models
Zhenya SONG#+
Ministry of Natural Resources, China
Marine heatwaves (MHWs) are extreme climatic events that last for days to months and can extend up to thousands of kilometers and cause substantial ecological, social, and economic impacts. However, it continues to be challenging for climate models to accurately simulate MHWs. In this study, we evaluate 29 models from the Coupled Model Intercomparison Project Phase 6 (CMIP6) and 19 models from the CMIP5 in terms of their capabilities to simulate MHWs by examining the spatial patterns and temporal variations. Then, we estimate future changes until the end of the 21st century under SSP126, SSP245, and SSP585. The results show that the CMIP6 ensemble mean is more skillful in capturing the features of MHWs than that of the CMIP5. The biases of the CMIP6 models for the MHWs intensities are within ±0.5 ◦C over most of the oceans, except in the western boundary current regions and eastern tropical Pacific, where the modeled MHWs are up to 1.5 ◦C weaker than the observations. In comparison, the results from CMIP5 are greater than ±1.5 ◦C in most areas. Both the CMIP5 and CMIP6 models underestimate long-duration MHWs in the eastern tropical Pacific, where they are nearly 20 days shorter than the observations. In most areas, the CMIP5 models overestimate the MHWs durations (by over 25 days), while the biases of the CMIP6 models are within 10 days. The projected MHWs exhibit significant increases in the intensity and duration and reach maximum intensities of 4 ◦C. The largest changes are projected to occur in the tropics, North Pacific, and North Atlantic. When comparing the shared socioeconomic pathways for the increasing trend of MHWs, the most extreme MHWs occur under SSP585, with their intensities nearly doubling and a near-permanent MHWs state occurring by the 2070s.
OS21-A011
Marine Heatwaves/cold-spells Modulate Mixed Layer Depth Globally
Yindi WANG1#+, Changming DONG1,2, Wenjin SUN1
1Nanjing University of Information Science & Technology, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China
Marine Heatwaves (MHWs) and Marine Cold-Spells (MCSs) are extreme sea surface temperature (SST) events, yet their impact on mixed layer depth (MLD) remains uncertain. By merging OISST V2.1 reanalysis data with Argo profiles, this analysis uncovers that MHWs tend to result in a reduction of MLD. A significant correlation (-0.83) is observed between MHW intensity and the degree of MLD shallowing. Upper oceanic restratification emerges as a pivotal mechanism driving MLD shallowing during MHWs. In contrast, MCSs generally lead to an increase in MLD, with regional variations in correlation. Notably, in the Indian Ocean, stronger MCSs contribute to a shallower MLD. Mesoscale cyclonic eddies initiate MCSs and potentially contribute to MLD shallowing. Moreover, restratification within the mixed layer stands out as another mechanism influencing MLD shallowing during MCSs. This study elucidates the MLD response during MHWs and MCSs, enriching our comprehension of the oceanic modifications spurred by these phenomena.
OS21-A017
Marine Heat Waves in East Asia: Its Characteristics and Relation to Climate Variability
Hyung-Ju PARK+, Hanna NA#
Seoul National University, Korea, South
Marine Heat Waves (MHWs) denote anomalously warm surface seawater events, which can be prolonged for several months, adversely affecting marine ecosystems and biodiversity. This study examines the spatial distribution and temporal variations of MHWs in East Asia, utilizing 41 years of satellite-based sea surface temperature data. The results indicate that MHWs predominantly occur in the East Korea Bay (EKB), the East China Sea (ECS), and the Western North Pacific (WNP) for longer than 25 days annually. MHWs in the EKB and WNP exhibit relatively longer durations but are less frequent than those in the ECS. Despite the distinct statistical characteristics, the time series of MHW days across these regions have significant inter-correlations, suggesting a collective response to large-scale climate phenomena. Spectral analysis is used to divide the MHWs into interannual (shorter than six years) and decadal (longer than six years) components, with each component being influenced by distinct climate variabilities. Nearly half of the peaks from the interannual component align with the El-Niño to La-Niña transition. During this period, MHWs occur along with both intensified ocean currents and warm and moist air inflow induced by anomalous anticyclonic circulation near the surface. On the other hand, during the peaks without the El-Niño to La-Niña transition, MHWs are driven by enhanced downward shortwave radiation associated with a high-pressure system over the mid-to-upper troposphere, linked to a circum-global teleconnection pattern. The decadal component of the MHW days is aligned with East Asia’s surface warming, hiatus, and reacceleration. The non-stationary connectivity with Pacific Ocean decadal variability is also explored. Our study provides an integrated understanding of the relationships between the East Asian MHWs with distinct timescales and well-known climate modes, offering basic mechanistic insights: ocean advection-driven or heat flux-driven.
OS21-A018
Estimation of Marine Heatwaves in the East/Japan Sea: The Extreme Value Generalized Additive Model Approach
Seoncheol PARK1, Wonkeun CHOI2, Joonpyo KIM3+, Chan Joo JANG2#
1Hanyang University, Korea, South, 2Korea Institute of Ocean Science & Technology, Korea, South, 3Sejong University, Korea, South
As the global sea surface temperature increases, the frequency and intensity of marine heatwaves (MHWs) — phenomena in which the sea surface temperature extremely increases over thousands of kilometers for days to months — are expected to increase in the future. These intensifying MHW are damaging marine ecosystems and increasing the risk of significant socio-economic damage. To predict the damage to marine ecosystems caused by MHWs, a variety of statistical techniques have been used. Previous studies have shown that extreme value statistics can effectively represent an extreme value distribution of MHWs using central statistics. However, most previous analyses of extreme values assume that the characteristics of MHWs are linear and spatially independent. The generalized additive model (GAM), which is an extension of the standard linear model, provides a way to estimate a flexible and nonlinear variation among variables of interest. The extreme value generalized additive model (EVGAM) applies the idea of GAM to form a flexible parameter modeling of the generalized Pareto distribution (GPD), which is frequently used in extreme value analysis. The existing methods are based on pointwise estimation and do not reflect the MHW status of adjacent areas, meaning they do not consider spatial correlations. In this study, we introduce EVGAM and analyze the extreme MHW near the Korean peninsula with a generalized Pareto distribution to incorporate spatial correlations and capture nonlinear relationships. According to the real analysis results, we find that the proposed EVGAM catches the global behavior of MHWs across longitude, latitude, and time. Furthermore, we expect that we can predict nearby future changes in MHWs in the study area without the use of weather generator models.
OS21-A019
Analysis of Sea Surface Temperature Variations Off the South Coast of Korea During Summer Using Multiple Linear Regression Analysis
Sora AHN+, Byoung-Ju CHOI#, Jae-Sung CHOI
Chonnam National University, Korea, South
The summer water temperature along the south coast of Korea undergoes rapid variations, significantly impacting the coastal marine ecosystem. To investigate the factors influencing short-term variability of water temperature during summer, multiple linear regression analyses were performed using the sea surface temperature data during the summers from 2016 to 2021. The independent variables used for regression include alongshore and cross-shore Ekman heat transports in the Jeju Strait, as well as alongshore and cross-shore local heat transports. During the summers of the study period, excluding 2020, the standardized regression coefficients of the cross-shore Ekman heat transport were notably prominent. The analysis revealed that the primary factors affecting water temperature fluctuations off Cheongsando (CSD), at south coast of Korea, in summer are the cross-shore Ekman current and the cross-shore temperature gradient in the Jeju Strait. Especially, the cross-shore temperature gradient affects the coastal water temperature with a 3–4 days lag. These findings indicate the significance of wind data in developing a numerical model-based sea surface temperature prediction system to forecast summer ocean heatwaves along the south coast of Korea. Additionally, it emphasizes the importance of accurately simulating surface temperatures in the Jeju Strait and coastal currents along the southern coast. These results contribute to understanding marine heat waves events along the coast of Korea.
Session Chair(s): Yuanlong LI, Chinese Academy of Sciences
OS18-A038
| Invited
Numerical Models, Observing Systems, and Data Assimilation for Prediction of Mesoscale Eddies in the Ocean
Zhijin LI#+
Fudan University
Mesoscale eddies pervade the global ocean, characterized by a typical horizontal scale of approximately 100 km and a timescale on the order of a month. Forecasting these eddies is the primary objective in predicting the ocean's "weather" over periods ranging from days to a month. The success in forecasting mesoscale eddies arises from advances in eddy-resolving numerical models, observing systems, and, in particular, data assimilation algorithms. Mesoscale eddies arise from baroclinic flow instabilities, making their forecast highly sensitive to initial conditions. The forecasting model must be appropriately initialized to generate subsequent forecasts successfully. Data assimilation integrates various observations into the model forecast, producing optimal estimates of the ocean state to initialize numerical models. An effective combination of observations from the Argo float observing network and a constellation of altimetry satellites is crucial for accurate estimates of the ocean state at the mesoscale through data assimilation, ensuring success in forecasting mesoscale eddies. The ocean bottom can notoriously reach depths of 10,000 m, and temporal and spatial scales of the ocean state at different depths are disparately different. These ocean state characteristics pose multiple challenges in altimetry data assimilation. To tackle these challenges, multiscale data assimilation algorithms is suggested.
OS18-A003
| Invited
Numerically Efficient Normalization of Sea Surface Height Innovations for Wide-swath Altimeters
Max YAREMCHUK1#+, Christopher BEATTIE2, Gleb PANTELEEV1
1U.S. Naval Research Laboratory, 2Virginia Tech
The wide-swath altimetry enables sea surface height monitoring at several times better spatial resolution and accuracy than traditional nadir altimeters. This advancement comes at the expense of necessity to correctly process spatially correlated errors caused by the uncertainties in environmental conditions beneath the satellite and in the geometry and orientation of the on-board interferometer. Being highly correlated along and across the satellite swath, these errors present a certain challenge for accurate assessment of the SWOT precision matrix whose off-diagonal elements are too numerous for computationally efficient data processing in operations. Using the error covariance model of the Surface Water and Ocean Topography (SWOT) satellite as an example, we explore utility of the block-circulant approximation to its precision matrix for reconstructing SSH variability in the region of the East Greenland Current. An extensive set of 2d variational data assimilation experiments demonstrates that the proposed approximation of the precision matrix provides accurate and numerically efficient SSH retrievals in a wide range of the background-to-observation error ratios and realistic surface wave height distributions along the swath.
OS18-A008
Remote Sensing of Primary Productivity and Particulate Organic Carbon in Inland Waters Using Shipborne Polarimetric Lidar
Dapeng YUAN1+, Delu PAN2#
1Southern Marine Science and Engineering Guangdong Laboratory, 2Ministry of Natural Resources
The vertical profiles of the primary productivity (PP) and particulate organic carbon (POC) in inland waters observed during a shipborne polarimetric lidar experiment conducted from May 14 to May 20, 2022, were investigated. We developed a lidar carbon-based productivity model (LCbPM) to estimate the vertical profile distribution of water PP along the shipborne lidar tracks and established a model for retrieving POC applicable to inland waters based on a large number of in situ observations. The subsurface PP maximum (SPM) for a total of 400 km of tracks fluctuated in the range of 39.43 to 793.13 mg C m-3 d-1, which corresponds to a depth variation range of 0.23 to 8.80 m. The subsurface POC maximum (POCM) for a total of 400 km of tracks fluctuated in the range of 223.41 to 962.90 mg m-3, which corresponds to a depth variation range of 0.68 to 8.80 m. The optical properties and PP in Xinanjiang Reservoir retrieved from shipborne lidar observations are validated by in situ observations with determination coefficients of 0.7607 and 0.6875, respectively. The temperature has a higher positive correlation with chlorophyll-a concentration in the water compared to water PP, while the NH3–N concentration has a higher positive correlation and significant difference level for water PP compared to chlorophyll-a concentration in the water. The results of this study are significant for the future implementation of all-weather, large-scale, and high-precision evaluation of PP and POC in inland waters.
OS18-A012
The Reconstruction of Global Surface Temperature: The China-LSAT 2.0 Ensemble and the China-MST 2.0 Dataset
Zichen LI#+, Qingxiang LI
Sun Yat-sen University
The global surface temperature observational datasets are the foundation of global warming studies. The China-LSAT (China global Land Surface Air Temperature) 2.0 and China-MST (China global Merged Surface Temperature) -Interim, independently developed by the team from Sun Yat-sen University, have been adopted in the IPCC AR6 and regarded as the fifth benchmark global land air temperature dataset and global surface temperature dataset. Based on the integration of relevant new research results from several countries and regions over the past decade, China-LSAT 2.0 has facilitated numerous research results through innovative reconstruction methods and parameters, model uncertainty assessment, etc. China-LSAT 2.0 for the land component and ERSST v5 for the ocean component are merged into the global surface temperature dataset China-MST 2.0. According to the China-MST 2.0, we took the lead in pointing out that the so-called “Hiatus” since 1998 is only a statistical artifact. Furthermore, the Arctic has been the region with the fastest increase in surface temperature, warming more than twice as fast as the global average, which is known as ‘Arctic amplification’. The neglect of recent rapid warming in the Arctic generally leads to an underestimation of global warming trends. With the extrapolation of land surface air temperature, we developed two ensembles of reconstructed surface temperature datasets under different sea ice extent scenarios (Imax and Imin) to systematically evaluate the annual and seasonal warming trends and their uncertainties from 1900 to 2020 in the Arctic. Discussion of the extreme cases of two sea ice extent scenarios contributes to an understanding of the range of magnitude of Arctic warming rates.
OS18-A017
A Consistent Ocean Oxygen Profile Dataset with New Quality Control and Bias Assessment
Juan DU#+, Viktor GOURETSKI, Lijing CHENG
Chinese Academy of Sciences
The global ocean oxygen levels have declined in the past decades, posing threats to marine life and human society. High-quality and bias-free observations are crucial to understanding the ocean oxygen changes and assessing their impact. Here, we propose a new automated quality control procedure for ocean profile oxygen data. This procedure consists of a suite of nine quality checks, with outlier rejection thresholds being defined based on underlying statistics of the data. The procedure is applied to three main instrumentation types: bottle casts, CTD (Conductivity-Temperature-Depth) casts, and Argo profiling floats. Application of the quality control procedure to several manually quality-controlled datasets of good quality suggests the ability of the scheme to successfully identify outliers in the data. Collocated quality-controlled oxygen profiles obtained utilizing the Winkler titration method are used as unbiased references to estimate possible residual biases in the oxygen sensor data. The residual bias is negligible for electrochemical sensors typically used on CTD casts. We explain this as the consequence of adjusting to the concurrent sample Winkler data. However, our analysis finds a prevailing negative residual bias for the delay-mode Argo profiling floats varying from -4 to -1 µmol/kg among the data adjusted by different Argo data acquisition centers (DACs). The respective overall DAC-specific corrections are suggested. Applying the new QC procedure and bias adjustment resulted in a new global ocean oxygen dataset from 1920 to 2022 with homogeneous data quality across bottle samples, CTD casts, and Argo floats.
OS18-A022
A multi-level Parallel Approach to Increase the Computation Efficiency of a Global Ocean Temperature Dataset Reconstruction
Huifeng YUAN#+, Lijing CHENG, Zhong JIN, Jing LI
Chinese Academy of Sciences
A long-term ocean-gridded observational dataset with global coverage is crucial for ocean and climate research and operational oceanography. There is an increasing need to provide real-time datasets for climate monitoring and operational applications. However, the current data products from all international groups have at least a month delay for data release. One of the reasons for this delay is the long computation time of the global reconstruction algorithm. This report will introduce a multi-level parallel acceleration computing model to improve the efficiency of data construction through parallel computation, reduced code branch prediction, optimized data spatial locality, cache utilization, and other measures. This strategy has been applied to the EnOI-DE mapping approach proposed by the Institute of Atmospheric Physics (IAP), one of the world’s most widely used data products in the ocean and climate field. The proposed parallel computing model uses MPI, OpenMP, and SIMD technologies on the supercomputer "ORISE" in the Chinese Academy of Sciences. An evaluation indicates that the new construction strategy achieves an absolute error of 1x10-14, compared with the required accuracy of 1x10-4 in reconstruction. Compared with the traditional serial construction of MATLAB-based on a single node, the speed of the construction after parallel optimizations is speeded up by ~4.7 times. Furthermore, a large-scale parallel experiment of a long-term (>1000 months) gridded dataset based on over 16,000 processor cores proves the system's scalability, improving ~1200 times. This demonstrates the model's capability to reconstruct a new generation gridded dataset with higher spatial and temporal resolution, longer time series, and minimized analytical errors. This model represents another practice of the application of high-performance computing in oceanography and climatology, promoting the integration of the ocean and high-performance computing fields. This report will also introduce plans for heterogeneous computing systems such as CPU+GPU in the future.
OS18-A025
Enhancing Predictions of Air-sea Heat Fluxes from AMSR2 Microwave Observations Based on Deep Learning
Mengjiao WANG+, Haoyu WANG, Xiaofeng LI#
Chinese Academy of Sciences
Air–Sea heat fluxes play an important role in the global hydrological cycle and are therefore necessary to understand global climate variability. Using the bulk aerodynamic algorithm, heat fluxes are derived from the satellite surface wind and sea surface temperature (SST), as well as the air temperature (Ta) and specific humidity (qa). However, the latter two meteorological variables cannot be directly retrieved from remote sensing. Despite numerous attempts to develop algorithms using in situ measurements as training datasets, uncertainties persist in the retrieval of qa and Ta. Therefore, a new neural network technique is presented here that enhances the accuracy of qa and Ta compared to previous methods. The model utilizes data from five variables—wind, SST, column cloud liquid water, column water vapor, and rain rate—acquired from the Advanced Microwave Scanning Radiometer 2 (AMSR2) as input datasets. The model is trained and validated with the National Data Buoy Center (NDBC) buoy measurements. Based on the 116,576 global buoy collocations from 2012 to 2023, the root-mean-square errors (RMSE) of retrieved Ta and qa are 0.38 °C and 0.7 g/kg, respectively. Furthermore, for sensible and latent heat flux, the RMSE are 3.71 W/m2 and 19.59 W/m2, respectively.
OS18-A041
An New Real Time Quality Control Method for Argo Floats Based on Probability Distribution of the Historical Observations
Huizan WANG1#+, Senliang BAO1, Conghao LIN1, Yuzhu AN1, Zenghong LIU2
1National University of Defense Technology, 2Ministry of Natural Resources
Argo is a global ocean array of more than 3,500 free-drifting profiling floats that measure upper oceanic temperature and salinity from the surface to 2000 meters. There are two types of quality control (QC) for Argo data: delayed-mode quality control (DMQC) based on historical observations and simple real-time quality control (RTQC). There are still a lot of suspicious profiles following RTQC because there has been less comparison with historical observations, and automation needs to be increased, particularly to fulfill operational forecasting requirements. In this paper, An new RTQC method for Argo floats is proposed, which can identify abnormal profiles and data more accurately by comparing with historical observations and climatology data. The approximate probability distribution range of Argo temperature/salinity data in its region and time period is presented by combining the probability distribution of “optimal matching” historical profile observations and the distribution characteristics of World Ocean Atlas(WOA) climatology data. Furthermore, based on the discrimination of the probability distribution, the threshold of the corresponding probability distribution is set, and the concept of 3σ discrimination method of normal distribution is extended to 3σ discrimination under the full distribution condition, in order to achieve the purpose of automatically identifying abnormal profile data points. Based on the new Argo RTQC method proposed in this paper, quality control was conducted on the global Argo float profile provided by China Argo Real-Time Data Center website, which effectively identified abnormal profiles and salinity drifts. The identification results were consistent with visual judgment, indicating that the proposed method is reasonable and effective.
Session Chair(s): Yusuke UCHIYAMA, Kobe University
OS04-A040
The Origin of Selected Coastal Fishes Via Stable Isotope Analysis and Habitat Assessment
Nur Nabila Husna BAZLAN#+
Universiti Sains Malaysia
Fish landings and catch per unit effort of coastal fisheries were fluctuated from 2015 to 2021, based on the annual fisheries report from the Department of Fisheries. To conserve the sustainability of coastal fishes, several measures will be taken, such as stable isotope analysis. Telemetry and catch-and-release methods are widely employed in Malaysia for monitoring fish populations. However, there is a notable gap in research utilising stable isotope analysis in this region. Stable isotope analysis is particularly useful and an effective means of understanding the movement routes of fish. This study is therefore being carried out to determine the origin of selected coastal fish species in order to protect and conserve the area. Understanding the movement patterns and isotopic composition will help assess the relationship between movement behaviour and environmental factors and also to detect the original location. This will therefore help to conserve the rearing and breeding grounds. In addition, sampling sites for habitat assessment will determine fish affinities. Therefore, habitat assessment is a fundamental tool for fisheries management, serving as a basis for decisions on habitat restoration, the establishment of protected areas, and the sustainable use of resources.
OS04-A030
Arctic Rivers Make Global River Plumes Less Autotrophic
Chen-Tung Arthur CHEN#+, Ting-Hsuan HUANG
National Sun Yat-sen University
Estuaries are generally a source of CO2 to the atmosphere. Yet continental shelves are mostly a sink of CO2. It goes without saying that the system turns from heterotrophic to autotrophic somewhere outside of the river mouth. Small river plumes dissipate quickly, but large river plumes can extend hundreds of km on the continental shelf. It has recently been suggested that large river plumes are a large sink of CO2, but this conclusion was based on data from only six rivers and all those located in low latitude regions. More extensive investigations of the world's 18 largest rivers, including large Siberian rivers, in the study, make the global river plumes a smaller sink of CO2.
OS04-A031
Vertical Expansion of Global Oxygen Minimum Zones
Hongjing GONG+, Yuntao ZHOU#
Shanghai Jiao Tong University
The vertical changes of oxygen minimum zone (OMZ) are associated with alterations of biogeochemical cycle and mitigation of organisms to available habitats. However, the specific spatio-temporal changes and drivers affecting the vertical characteristics of global OMZ remain uncertain. Here, we examine the boundary depths and thickness of OMZ in the global ocean, using a combination of observed datasets from 1960 to 2022. Our results show widespread increasing trends in the thickness of both OMZ60 (i.e., dissolved oxygen, DO< 60 μmol kg-1) and OMZ20 (i.e., DO< 20 μmol kg-1) of the global ocean. The upper boundary of OMZ60 shows a shoaling trend in 91% of the areas, while the lower boundary exhibits a sinking trend in 79% of the areas. The most significant vertical expansion of OMZ has been observed in the North Pacific with shoaling upper boundary and sinking lower boundary. For main OMZ regions, temperature and wind are identified as the most crucial factors of physical processes influencing the spatial variability in vertical characteristics of OMZ60. Widespread vertical expansions of OMZ could intensify the vulnerability of mesopelagic fishes along with overfishing, leading to negative impacts on marine ecosystem and socioeconomic systems.
OS04-A037
Lagrangian Versus Eulerian Spectral Estimates of Surface Kinetic Energy Over the Global Ocean
Xinwen ZHANG1#+, Xiaolong YU1, Aurelien PONTE2
1Sun Yat-sen University, 2The French Research Institute for Exploitation of the Sea (Ifremer)
Geographical distributions and frequency content of ocean surface kinetic energy (KE) are estimated in a $1/48^\circ$ high-resolution global numerical model of the ocean circulation. Eulerian (fixed-point) KE estimates are considered as a reference which is compared to Lagrangian (along-flow) KE estimates in terms of rotary frequency spectrum and global maps of energy levels at low-frequency, tidal and near-inertial bands. Eulerian and Lagrangian KE exhibit similarities in the dominance of low-frequency motions and presence of distinct spectral peaks at semidiurnal, near-inertial, and diurnal frequencies. One notable difference is that Lagrangian spectra are smoother with wider and lower spectral peaks compared to Eulerian counterparts. Nevertheless, no significant differences are found between Lagrangian and Eulerian global KE levels provided adequate frequency bandwidths are chosen. Our findings demonstrate that Lagrangian observations of the Global Drifter Program have great potential to accurately map global KE variability at high frequencies (e.g., tidal and near-inertial).
OS04-A038
Paleo-sea Surface Temperature Reconstruction of Pujada Bay (Southern Philippines) from Archaea Lipids
Caroline Marie JARAULA1#+, Zenon Richard MATEO2, Kliti GRICE3, Martijn WOLTERING4, Ronald LLOREN5, Fernando SIRINGAN1
1University of the Philippines, 2Texas A&M University, 3Curtin University, 4Commonwealth Scientific and Industrial Research Organisation, 5ETH Zurich
Locus of the warmest sea surface temperatures (SST) is the Indo-Pacific Warm Pool which plays a significant role in the heat and hydrodynamic coupling between the ocean and the atmosphere. We study this dynamic interaction in an embayment in eastern Philippines with high sedimentation rates to capture centennial scale paleoclimate signals that are influenced by the El Nino Southern Oscillation, Pacific Decadal Oscillation, and East Asian Monsoon. Other groups reconstructed millennial-scale climate and oceanography of the southern Philippines. This paper aims to add slightly higher resolution reconstructed SST and, where data are suitable, reconstructed mean annual air temperature. This study employs isoprenoidal glycerol dialkyl glycerol tetraethers (isoGDGTs), biomarkers of archaea, to reconstruct sea surface temperatures and branched GDGTs (brGDGTs) to reconstruct mean annual air temperatures using recent calibration equations. This is one of a few stations in the Philippines that systematically collected SST as far back as 1970s and some sparse data to the mid-1940s to compare the paleo-temperature reconstruction. The range and fluctuations in the measured and reconstructed SST are similar. Temperature shifts at the heart of the warm pool for the Little Ice Age, Medieval Warm period, and during extreme El Niño Southern Oscillation perturbations are observed in the reconstructed data set. Sedimentological and multi-element analyses from an X-Ray Fluorescence core scan at 1 cm resolution distinctly indicate two stratigraphic units. Ti used as a proxy for precipitation, δ13C and C/N for organic matter source and preservation, Ba/Ti for paleoproductivity. Warming events are associated with increased productivity in the marine environment, whereas the terrestrial response is a decrease in productivity. The increase in productivity may also be related to enhanced marine phytoplankton bloom.
OS04-A032
Precession Modulation on Mid-latitude and Obliquity on High-latitude Arctic Sea Ice Coverage Over the Past 2.6 Million Years
Gagan MANDAL1+, Soon-Il AN1#, Axel TIMMERMANN2, Kyung-Sook YUN3, Jae-Heung PARK4
1Yonsei University, 2Pusan National University, 3IBS Center for Climate Physics, 4Seoul National University
Glacial-interglacial cycles characterize the Earth's climate during the Quaternary period, which spans from ∼0 to 2.6 Ma (million years before the present). These cycles are primarily caused by variations in external forcings, such as eccentricity (∼100 kyr), obliquity (∼41 kyr), and precession (∼23/19 kyr) orbital forcings, as well as variations in atmospheric CO2 concentration (GHG) and the corresponding climate feedbacks. Arctic sea ice is susceptible to temperature shifts over the glacial-interglacial cycles, yet little is known about how it reacts to external forcings. Here, we have used the Community Earth System Model version 1.2 (CESM1.2) in a quasi-continuous simulation to learn more about the response of the Arctic sea ice to variations in orbital, GHG, and continental ice sheet forcings on millennial timescales. Our research indicates that the dominating periodicity of Arctic sea ice shifted from ∼41 to ∼100 kyr across the Mid-Pleistocene transition (700–1200 ka) (MPT), similar to the climate state. The sea ice coverage was more pronounced during the post-MPT (0–700 ka) than the pre-MPT (1200–2600 ka) period. This is because, compared to the post-MPT period, enhanced GHG forcing during the pre-MPT period resulted in ∼38% stronger Arctic amplification and ∼21% higher global surface air temperatures, which led to warmer summers and less pronounced sea ice coverage. On the other hand, obliquity had a stronger effect at high latitudes and precession across the tropics and mid-latitudes. As a result, precession and obliquity controlled the amount of Arctic sea ice at the mid-and high-latitudes, respectively. Thus, our study demonstrated the critical role of orbital (GHG) forcing in regulating Arctic sea ice's latitudinal distribution (coverage) for the past 2.6 Ma.
OS04-A035
Global Emergence of Ocean Compound Climatic Impact-drivers
Lijing CHENG#+, Zhetao TAN
Chinese Academy of Sciences
The ocean is exposed to various climatic impact-drivers (CIDs) that affect society and marine ecosystems. However, a global view of the compound effect of different CIDs from the surface to the subsurface ocean is still lacking. Based on newly available ocean observations, we develop a global 3-D view of ocean exposure to long-term compound effects by applying a time-of-emergence approach to physical and biogeochemical CIDs such as temperature, salinity, dissolved oxygen, and pH. We find that individual and compound emergence of trends in different ocean CIDs has become increasingly pronounced globally over the past 60 years. Multiple CIDs emerge together in the subtropical and tropical Atlantic, the subtropical Pacific, the Arabian Sea, the Mediterranean Sea, and the Gulf of Mexico. Considering their intensity, duration, and magnitude, we find a higher and more widespread exposure of the epipelagic and mesopelagic zones to the emergence of compound CIDs compared to what is observed in the surface layer. Our results provide, for the first time, a global view from direct physical and biogeochemical observations of how the ocean is already subject to several pervasive and interconnected changes caused by climate change. They also underscore the urgent need to investigate how these changes affect marine ecosystems and populations.
OS04-A029
Relationship Between Seafloor Seismic Ground Motions and Its Corresponding Ambient Water Pressure Perturbation
Emmy Tsui-Yu CHANG#+
National Taiwan University
Significant seismic events produce discernible ground motions that are recorded by global seismic networks, influencing the ocean floors and disrupting water masses in the deep sea. This study analyzes ocean bottom pressure data acquired from two tsunami monitoring stations deployed by the Central Weather Administration (CWA, Taiwan) in Taiwan's eastern and southwestern offshore regions. The purpose is to unveil the correlation between seismic seafloor motions and ambient water perturbation. A comprehensive statistical analysis was conducted on the waveforms of the bottom-pressure time series spanning from 2018 to 2021. Given the negligible impact of water layer compressibility on low-frequency seafloor oscillations, the seafloor pressure induced by low-frequency seismic waves is directly proportional to seafloor acceleration. Notably, the minimal response of bottom pressure at a frequency of approximately 60 mHz (17s period), beyond the tsunami frequency band, prompted an investigation into the transition of water fluctuation in response to seismic Rayleigh waves. Power spectral analysis revealed that the proportionality coefficient of ground motions and water pressure perturbations equates to the mass of the water column at the observatory's installation or, approximately, the product of water density and ocean depth. However, the potential impact of sediment layer resonances introduces uncertainty in the pressure/acceleration transition in seafloor water pressures. This study addresses the practical concern of whether the threshold value in the PMEL tsunami monitoring system (Deep-Ocean Assessment and Reporting of Tsunami, DART) applies to regional earthquakes capable of generating hazardous trans-Pacific tsunamis. Additionally, it contributes to exploring the physical mechanisms involved in transforming energy from the solid earth to the ocean water layer.
Session Chair(s): Huizan WANG, National University of Defense Technology
OS18-A027
| Invited
Progress of Oceanic Observation During Tropical Cyclones
Han ZHANG#+
Second Institute of Oceanography, Ministry of Natural Resources
Tropical cyclones have strong impact on air-sea environment. The shortage of oceanic in-situ observation inhibits the understanding of the dynamics and processes during tropical cyclones. Because the advancement of technology, the observation methods during tropical cyclones are enriched, and the time comes for cooperative observation of moored and mobile instruments. This work briefly summarizes our moored observation in the past ten years as well as recent development and usage of unmanned instruments (e.g. glider, wave glider, unmanned ship, drifters) for the oceanic observation during tropical cyclones. These data uncover the sea surface wind and wave structures as well as air-sea heat fluxes during tropical cyclones, also thermal and dynamical response to tropical cyclones in upper ocean as well as the deep ocean. Cooperative observations are design and will be deployed in the coming years, aims to enrich the observation both on air-sea surface and in upper ocean, to uncover the detailed processes during tropical cyclones.
OS18-A002
Is the Indonesian Throughflow Strengthening in the Past Decades?
Yuanlong LI#+
Chinese Academy of Sciences
While the pivotal role of the Indonesian Throughflow (ITF) in the global ocean circulation and climate has been widely recognized, accurate estimation of its volume transport based on observational data remains challenging. This work provides an updated estimate of the monthly ITF geostrophic transport (ITFG) in the upper 700 m at the IX1 section between Indonesia and Australia. The ITFG estimate is better constrained by improved data correction and new salinity data products. The mean ITFG of 1993–2018 is 8.2 ± 0.2 Sv, in which contributions of the temperature and salinity components (ITFT and ITFS) are 5.5 ± 0.2 and 2.8 ± 0.1 Sv, respectively. The interannual variability (∼4.4 Sv in standard deviation) is dominated by ITFT, as the result of wind-driven thermocline dynamics, and slightly attenuated in amplitude by ITFS. The strengthening trend of 1.33 Sv decade−1 during 1993–2018 primarily arises from ITFS and secondarily from ITFT.
OS18-A010
Tsunami Data Assimilation Using the Tsunami Velocity Field Calculated from Tsunami Magnetic Field
Zhiheng LIN#+, Genta UENO, Shinya NAKANO
The Institute of Statistical Mathematics
The seawater driven by tsunami cuts the earth’s magnetic field, which generates an induced magnetic field. Magnetometers on land or seafloor can observe these magnetic fields, which can provide tsunami propagation information, including sea level change and tsunami propagation direction. Moreover, an analytical solution shows that tsunami-induced magnetic field can be calculated into tsunami velocity field in two horizontal directions, Vx and Vy. This velocity field can be applied to tsunami data assimilation for tsunami early warning. Compared to previous studies which mostly used tsunami sea level change data, tsunami velocity fields contain more information about tsunami, such as the change of tsunami propagation direction, which was expected to improve tsunami data assimilation. However, it has not been investigated. In this study, based on the seafloor tsunami magnetic field data of the 2009 Samoa and 2010 Chile tsunamis, we will show these two topics as follows:1. The horizontal tsunami velocities, Vx and Vy, calculated from the tsunami magnetic fields;2. Tsunami data assimilation based on the calculated tsunami velocity field, and comparison of the assimilated tsunami sea level change with the observation data from the DART stations. It will be the first time that far-field tsunami velocity field data will be used for tsunami data assimilation. In terms of tsunami early warning, tsunami data assimilation is promising because it does not rely on tsunami source models. As a result of our study, we will demonstrate the effectiveness of tsunami magnetic fields in early tsunami warning.
OS18-A021
A New Ocean Data Quality Control System Reveals a Stronger Ocean Warming Rate
Lijing CHENG#+, Zhetao TAN
Chinese Academy of Sciences
Over the past century, more than 20 million in-situ profiles with heterogeneous quality had been collected, leading to a high demand of a quality control (QC) procedure to identify outliers efficiently, accurately, and automatically. In this study, we present a new automatic QC system (namely CODC-QC) for ocean temperature and salinity observations. Unlike many existing QC procedures, no assumption is made of a Gaussian distribution law in CODC-QC as the statistical distribution of the variables are typically skewed. Instead, the 99% quantiles are used as thresholds to define the local climatological ranges. In addition, these thresholds are time-varying, which aims at reducing erroneously excluding good real-time data. The above strategies are used in the local climatological range check for temperature, salinity and vertical temperature gradient, in which the anisotropic feature of water properties and the topography barriers adjustment is accounted for. Additionally, the CODC-QC under the benchmark evaluation was applied to all temperature and salinity profiles in the World Ocean Database from 1940 to 2021. Result shows a significant dependency of the quality on instrumentation types. Finally, as ocean heat content (OHC) is a fundamental indicator of climate change, the impact of different QC systems on OHC estimation is examined. We found that applying CODC-QC will lead to a 15% stronger warming rate within 1991–2021 compared to the application of WOD-QC (NOAA/NCEI), implying a non-negligible source of error in OHC estimate. The new AutoQC system could support further improvement of the ocean sciences and other applications.
OS18-A029
High-resolution Sea Surface Salinity from the Fusion of GOCI and HYCOM Data Based on Machine Learning Over the East Asian Region
So-Hyun KIM1+, Taejun SUNG1, Seongmun SIM1, Daehyeon HAN1, Eunna JANG2, Jungho IM1#
1Ulsan National Institute of Science and Technology, 2Korea Institute of Ocean Science & Technology
Sea Surface Salinity (SSS) is a key variable that determines the density of seawater, affecting both surface and deep ocean circulation. A high spatiotemporal resolution of SSS is crucial for understanding oceanic phenomena in both open ocean and coastal areas. Satellite observations have been actively adopted for SSS estimation to overcome the limitations of in-situ measurements. To enhance the resolution of SSS, numerous studies have attempted to use high-resolution ocean color sensor data. However, due to the weak correlation between SSS and optically sensitive parameters in ocean, most studies have been constrained to coastal-focused areas. To broaden the research scope, we propose a machine learning-based approach for SSS estimation by combining the Geostationary Ocean Color Imager (GOCI) and the Hybrid Coordinate Ocean Model (HYCOM). We trained an artificial neural network (ANN) model with GOCI remote sensing reflectance (Rrs) and HYCOM SSS as inputs to simulate the SSS from the Soil Moisture Active Passive (SMAP) sensor. This approach enables application to both coastal and offshore areas across the East Asian region with a high spatial (1 km) and temporal (daily) resolution, allowing the observation of seasonal and spatial variation in SSS. When evaluated against SSS from SMAP and in-situ measurements, the proposed model showed comparable performance to those based on GOCI or HYCOM alone. Additionally, we conducted an analysis of the relationships between ocean color signals and SSS using Shapley Additive Explanations (SHAP) to show how the contributions of various input factors vary seasonally and spatially. Along with the novelties of this study, we will discuss some limitations such as cloud contamination and the uncertainty of GOCI Rrs over turbid waters.
OS18-A033
A Two-module Bias-correction Model for Sea Wave Hindcasting Based on the Long-short Term Memory Neural Network
Jiawen LIAO1+, Yineng LI2#, Junmin LI2, Shaotian LI3, Shiqiu PENG2
1学生, 2Chinese Academy of Sciences, 3South China Sea institute of Oceanology, Chinese Academy of Sciences
The lack of observations and biases of winds and terrain in the coastal region result in significant biases in the numerical modeling of sea waves. In this study, we establish a two-module bias correction model based on the Long-Short Term Memory neural network (denoted as TM-LSTM) which accounts for the data imbalance by separately training the neural network for low and high sea states. The in-situ observations in 2020 and 2021 are used to model training and testing, respectively. The test results show that TM-LSTM significantly reduces the Root Mean Square Error (RMSE) and Mean Absolute Error (MAE) of modeled sea waves by 52.9% and 65.5%, respectively. In addition, TM-LSTM outperforms the single-module model (denoted as SM-LSTM) that does not account for the imbalance of training data. Our results highlight the great value of deep learning in correcting biases for numerical models and the importance of accounting for data imbalance in training the neural network.
OS18-A036
Correction of Satellite Sea Surface Salinity Products Using Machine Learning
Senliang BAO1#+, Huizan WANG1, Hengqian YAN1, Juan DAI2, Jian CHEN3
1National University of Defense Technology, 2China University of Petroleum, 3Beijing Institute of Applied Meteorology
Although salinity satellites can provide high-resolution global sea surface salinity (SSS) data, the satellite data still display large errors close to the coast. In this paper, a nonlinear empirical method based on random forest is proposed to correct two Soil Moisture and Ocean Salinity (SMOS) L3 products in the tropical Indian Ocean, including SMOS BEC and SMOS CATDS data. The agreement between in-situ data and the corrected SMOS data is better than that between in-situ data and the original satellite data. The root-mean-square deviation (RMSD) of the satellite SSS data decreased from 0.366 to 0.275 and from 0.367 to 0.255 for SMOS BEC and SMOS CATDS, respectively. The effect of the correction model was better in the Arabian Sea than in the Bay of Bengal. The RMSD of corrected BEC (CATDS) SSS was reduced from 0.44 (0.48) to 0.276 (0.269), and the correlation coefficient was increased to 0.915 from 0.741(0.801) in the Arabian Sea while the correlation coefficient improved less than 0.02 in the Bay of Bengal. The cross-validation results highlight the robustness and effectiveness of the correction model. Additionally, the effects of different features on the correction model are discussed to demonstrate the vital role of geographical information in the correction of satellite SSS data. The proposed method outperformed other machine-learning methods with respect to the RMSD and correlation coefficient.
Session Chair(s): Yu UMEZAWA, Tokyo University of Agriculture and Technology, Wen-Chen CHOU, National Taiwan Ocean University
OS09-A011
| Invited
Changes in Surface Sediment Carbon Compositions in Response to Tropical Seagrass Meadow Restoration
Songlin LIU1+, Yuzheng REN2, Xiaoping HUANG1#, Peter MACREADIE3
1Chinese Academy of Sciences, 2University of Chinese Academy of Sciences, 3Deakin University
Seagrass meadows are declining at a global scale, threatening their capacity as blue carbon sinks. Restoration of seagrasses (via seagrass seeds or plant transplantation) may recover their carbon sequestration capacity. Previous studies have predominantly focused on sediment organic carbon (SOC), while variations in sediment carbon compositions remain poorly understood, limiting our comprehension of the influence of seagrass restoration on sediment carbon stability. Here, we researched the differences in surface (0~3 cm) sediment carbon compositions in response to tropical seagrass transplantation among species (Thalassia hemprichii and Enhalus acoroides); specifically, differences in labile, recalcitrant and refractory SOC, as well as sediment inorganic carbon (SIC) compositions variations under transplanted T. hemprichii and E. acoroides communities. It was found that seagrass transplantation enhanced suspended particle organic matter, and epiphyte and macroalgae input to surface sediment, which recovered the surface SOC concentration and stock rapidly to natural levels (increased ~1.6-fold) within two years following transplantation. The elevated contribution of epiphyte and macroalgae significantly increased the surface labile sediment organic matter (SOM), but not the recalcitrant and refractory SOM composition after short-term transplantation. Meanwhile, surface SIC was significantly elevated, which might be mainly ascribed to allochthonous carbonate particle trapped under transplanted area with implications for carbon sequestration. The higher canopy and longer leaf seagrass species, E. acoroides, had elevated SOC, SIC and was more labile composition, compared to T. hemprichii transplant. Overall, this research suggests that tropical seagrass transplantation can increase the surface SOC, SIC concentration by increasing the labile organic matter and allochthonous carbonate particle input, respectively, with varying significantly among seagrass species.
OS09-A012
Importance of Dissolved Organic Matter on Seagrass Meadows: A Coastal Blue Carbon Pathway Perspective
Jian-Jhih CHEN1#+, Wen-Chen CHOU2
1National Kaohsiung University of Science and Technology, 2National Taiwan Ocean University
Coastal blue carbon habitats play an important role in marine biogeochemical cycles. Previous studies suggest that these coastal ecosystems can make a significant contribution to carbon storage. Seagrass meadows have received attention for their ability to sequestrate inorganic carbon, which is considered a potential nature-based solution to reduce excessive carbon dioxide emissions. However, most studies focus on particulate organic carbon storage in the form living biomass. Less attention has been given to benthic dissolved organic matter (DOM) in seagrass meadows, which may represent an important fraction of carbon storage. In an effort to fill the research gap regarding the properties and quality of DOM dynamics in relation to seagrass meadows in Taiwan. Here, a pilot study was undertaken to broadly characterise of colored dissolved organic matter (CDOM) on seagrass meadows in Kenting Haikou. In this study, three-dimensional fluorescence excitation-emission matrix spectroscopy with parallel factor analysis and absorption spectroscopy were used to characterize the main sources of CDOM. The humification and fluorescence biological index were further used to examine the composition of CDOM. Our results show that three EEM-PARAFAC components were statistically identified from the PARAFACT model. These components were classified as Peak B (38%), Peak T (36%), Peak A (18%) and Peak D (8%). The high proportion of Peak B and Peak T suggest that the main composition of CDOM is protein-like. HIX values ranged from 0.6 – 2.57, with an average of 1.05 ± 0.41 while BIX values ranged from 0.29 – 3.9, with an average 1.18 ± 0.7. The low HIX and high BIX values indicate that the DOM is autochthonous and mainly produced by endogenous organisms. These results suggest seagrass meadows can generate DOM during their metabolism, which may be an overlooked carbon sequestration pathway.
OS09-A009
| Invited
Microbial Degradation of Phytoplankton-released Dissolved Organic Carbon: First Estimation of Microbial Carbon Pump (MCP)
Tzong-Yueh CHEN#+
National Taiwan Ocean University
The microbial carbon pump (MCP), the microbial formation and transformation of refractory dissolved organic carbon (RDOC), has been discussed for more than a decade. However, no field (real) estimation of MCP efficiency was reported. In this study, we examined the microbial degradation of freshly phytoplankton-produced dissolved organic carbon (DOC) fron coastal seawater for 2 months. The results showed that most photosynthetically fixed DOC was rapidly respired to CO2 with a very high degradation rate constant of 1.312±0.238 d-1. The non-linear Marquardt-Levenberg model indicated that the carbon sequestration from phytoplankton-released DOC through the MCP was 5.58±1.10%.
OS09-A004
A Comparative Study on Carbonate Chemistry in Seagrass Meadows: Unravelling Alkalinity Production Disparities in Reef and Terrestrial Sediments and Its Role on Carbon Sink Potential
Lan-Feng FAN1, Chi-Wei TONG1, Hui-Feng CHEN1, Jian-Jhih CHEN2, Ping-Chun CHEN1, En-Cheng Kong KONG1, Mariche NATIVIDAD1,3, Wen-Chen CHOU1#+
1National Taiwan Ocean University, 2National Kaohsiung University of Science and Technology, 3Ecosystems Research and Development Bureau
As one of the most productive ecosystems on Earth, seagrass meadows can sequester a large amount of carbon dioxide through photosynthesis, thereby serving as a nature-based solution for the mitigation and adaptation of climate change. In addition to conventional enhanced organic carbon storage, recent studies have shown that sedimentary total alkalinity (TA) production may represent an overlooked component of blue carbon. In this study, we conducted a comprehensive comparison of the carbonate chemistry of overlying water and pore water, sediment carbon content, mineral composition, and benthic TA fluxes between two contrasting seagrass meadows: one in organic carbon-rich reef sediments, namely Dongsha, and the other in organic carbon-poor terrestrial sediments, namely Haikou. The results show that the concentration of TA in pore water and sedimentary TA flux was higher, while the partial pressure of carbon dioxide (pCO2) was lower in the overlying water column for seagrass meadows growing in carbonate sediments (Dongsha) compared to those growing in silicate sediments (Haikou). This finding indicates that seagrass meadows in reef sediments with a high organic carbon content can act as hotspots for ocean alkalinity production. Consequently, targeting seagrass along reef sediments for restoration may further enhance the potential mitigation of climate change in seagrass restoration projects.
OS09-A010
Assessing the Community Metabolism of Restored Seagrass Meadows (Halodule Uninervis) in Taiwan: Implications for Carbon Sink Capacity
Mariche NATIVIDAD1,2+, Jian-Jhih CHEN3, Yi-Le SHEN4, Lan-Feng FAN1, Hsin-Yu CHOU1, Hsin-Chio CHANG1, Wen-Chen CHOU1#
1National Taiwan Ocean University, 2Ecosystems Research and Development Bureau, 3National Kaohsiung University of Science and Technology, 4Penghu Fisheries Biology Research Center
Seagrass meadows serve as major carbon sinks; however, their ability to fulfill this crucial ecological role diminishes rapidly with the decline of this ecosystem. The restoration of coastal habitats has garnered significant attention for enhancing recovery and as a nature-based approach to carbon dioxide removal. Yet, the metabolic system of restored meadows and their potential function as carbon sinks remains unexplored. In this study, we assess the community metabolic rates, including gross primary production (GPP), community respiration (CR), net community production (NCP), and the photosynthesis-to-respiration (P/R) ratio, for replanted seagrass (H. uninervis) and bare sediment through ex-situ core incubation. The mean GPP of seagrass beds and bare sediment was 5.2 ± 1.2 mmol O2 m-2 h-1 and 3.6 ± 0.9 mmol O2 m-2 h-1, respectively. The CR between seagrass beds and bare sediment was similar (-2.1 ± 0.4 vs. -2 ± 0.3 mmol O2 m-2 h-1). The mean NCP in seagrass beds was 9.2 ± 4.5 mmol O2 m-2 h-1, while it was -12.1 ± 7.1 mmol O2 m-2 h-1 in bare sediments. Both GPP and NCP were higher in seagrass beds compared to bare sediments. The P/R ratio for seagrass was 1.2 ± 0.1, higher than in bare sediment (0.8 ± 0.1). Our results indicate that restored seagrass meadows may shift the benthic ecosystem metabolism from a heterotrophic state in bare sediment to a net autotrophic system, thereby capable of acting as a carbon sink. The ecological viability of seagrass restoration emerges as a promising strategy for addressing climate change through carbon sequestration. This study represents the first attempt to quantify the metabolic performance of restored seagrass meadows in Taiwan.
OS09-A027
The Effect of Different Nitrogen Loading on the Chemical Composition and Decomposition Characteristics of Seagrass (Zostera Marina)
Toru MIYATA1, Yu UMEZAWA1#+, Yoshiki HORIKAWA1, Makoto WATANABE1, Shigeki WADA2, Masahiro NAKAOKA3, Tomohiro KUWAE4
1Tokyo University of Agriculture and Technology, 2University of Tsukuba, 3Hokkaido University, 4Port and Airport Research Institute
Nitrogen is one of the elements that can limit the primary production of plants, therefore nitrogen supply potentially affects coastal primary production. On the other hand, it is known that some secondary metabolites (e.g., phenolic compounds) that are not directly involved in growth and metabolic reactions, such as photosynthesis and respiration, act as protective compounds against predators and pathogens. Furthermore, in terrestrial higher plants, it has been reported that the abundance of these substances varies with the nitrogen supply. Thus, differences in nitrogen supply may contribute not only to the growth of seagrasses but also to the degradation characteristics of the seagrass-derived organic matter. In this study, we focused on the Zostera marina, widely distributed in the coastal area of Japan, and examined the potential effects of the nitrogen supply in the coastal area on the function of seagrass as “blue carbon,” focusing the following topics.1) “Estimation of nitrogen content in seagrass leaves by portable nitrogen meter.” The N contents estimated by the portable N meters for terrestrial grasses were compared with the chlorophyll content and actual nitrogen content of the Z. marina. Appropriate conditions that allow accurate assessment of N content of seagrass are investigated.2) “Evaluation of the effect of nitrogen content on the amount of structural and repellent substances in the seagrass leaves.” The amounts of structural substances and repellent substances of seagrass were evaluated using chemical treatments and Folin-ciocalteu method, respectively, and compared with the actual nitrogen content.3) “Evaluation of the decomposition characteristics of seagrass leaves in the different environmental conditions.” The effects of nitrogen loading on the decomposition characteristics of seagrass were evaluated through the incubation experiments in different environmental conditions.
OS09-A006
Spatiotemporal Variations of Partial Pressure of Carbon Dioxide in Chiku Lagoon During Summer
Fei-Ling YUAN1+, Kai-Jung KAO1, Veran WEERATHUNGA1, Wen-Chen CHOU2, Wei-Jen HUANG1#
1National Sun Yat-sen University, 2National Taiwan Ocean University
Coastal lagoons play a crucial role in the global carbon cycle with complex mechanisms. However, understanding the dynamics of these systems requires both partial pressure of CO2 (pCO2) variations and sufficient spatiotemporal pCO2 data collection. To address this issue, we deployed five lab-made Autonomous Buoys for inland Tidal Water (ABiTC) in Chiku Lagoon for over 36 hours between August 31st and September 2nd, 2020. Temperature, salinity, and pCO2 data were collected in a 1-minute interval. Diurnal temperature changes were consistent across all stations (30.7 ± 1.0 ℃), while salinity displayed semi-diurnal patterns with a spatial gradient increasing from the upper (7.2-16.0) to the lower lagoons (26.0-34.2). Notably, pCO2 and salinity showed an inverse relationship. The upper lagoon exhibited significantly higher pCO2 levels (2442 ± 902 μatm) and larger diurnal fluctuations (>1500 μatm) compared to the lower lagoon (448 ± 17 μatm and diurnal fluctuations ranged from 10 to 200 μatm). Low salinities acted as a strong source (7.5 ± 2.3 mmol m-2 hr-1) to atmospheric CO2 and high salinities acted as a weak source (0.7 ± 1.0 mmol m-2 hr-1). Our high time-resolution data revealed that during the wet season, Chiku Lagoon acts as a strong source of atmospheric CO2, with air-water CO2 gas exchange reaching 1.4 ± 0.7 mmol m-2 hr-1 (33.8 ± 16.3 mmol m-2 d-1).
OS09-A002
Assessing Blue Carbon Management Strategies in the Asia-pacific Region
Stefanny Rebeca ALVARADO#+
National Taiwan Ocean University
As global environmental concerns heighten, the effective management of blue carbon ecosystems emerges as a pivotal force in mitigating climate change and advancing sustainable development. The critical role of these ecosystems in carbon sequestration and biodiversity conservation underscores their significance. Amidst the escalating challenges of climate change, understanding how nations in the Asia-Pacific region, particularly Japan and Indonesia, address blue carbon management becomes imperative. This study employs UCINET 6 software to analyze and categorize blue carbon management strategies made by different stakeholders in Japan and Indonesia. The categorization includes key domains such as environmental education, research and technology, the economy, law and regulation, and regional and international cooperation. It considers a wide range of documentation such as published articles, data papers and public policies. The investigation serves as a crucial bridge between scientific knowledge and policy implementation. By systematically categorizing diverse approaches in the studied countries, the research aims to unveil patterns and variations in blue carbon management strategies. Simultaneously, it observes the interconnectivity of actors involved in these management strategies. The comparative analysis provides insights into the effectiveness of different pathways, offering valuable information for policymakers, environmentalists, and researchers. Additionally, as part of the research plan, recommendations specific to Taiwan's blue carbon management will be developed. In addressing the imperative for informed decision-making amidst a rapidly changing climate, this research anticipates contributing to the development of globally adoptable, robust policies, and strategies. As an integral part of the broader environmental sustainability discourse, the study seeks to empower stakeholders with transcendent knowledge, fostering collaborative and collective efforts towards a more resilient and sustainable future.
Session Chair(s): Liuqian YU, The Hong Kong University of Science and Technology (Guangzhou)
OS14-A008
Arctic Ocean Circulation in a Warming Climate
Estanislao GAVILAN PASCUAL-AHUIR#+, Yonggang LIU
Peking University
Arctic sea ice has been declining during the past decades, and climate models predict an ice-free summer Arctic by the end of the century. In the meantime, freshwater and heat storage increase, altering the surface stratification. Despite the CMIP efforts to predict the future, the large uncertainty among models cast doubts about how the Arctic Ocean surface circulation will respond to such buoyancy forces and how the freshwater output towards the Atlantic Ocean will change. This study investigates these aspects using the global ocean and sea ice model MITgcm-ECCO2 18km resolution. The MITgcm-ECCO2 model is forced with combined atmospheric data from ERA5 reanalysis data and the anomalies from coarse-resolution CMIP6 models. This combination enables us to solve the limitations of the Climate models in the Arctic basin. By the end of the integration, the wind-driven circulation has significantly changed. The Beaufort Gyre expands due to the change of the salinity in the mixing layer, and transpolar current is pushed towards the Barent Seas. The evolution of the surface circulation affects the net boundary transport at the straits of the Arctic basin. More specifically, the net transport across the Fram Strait decreases, enhancing the outflow across the Canadian Archipelago. Lastly, the redistribution of transport between the Fram and the Canadian Archipelago impacts the deep water formation in the marginal seas, affecting the strength of the AMOC circulation.
OS14-A015
Intraseasonal Response of Marine Planktonic Ecosystem to Summertime Madden-Julian Oscillation in the South China Sea: A Model Study
Wenfang LU1#+, Hengye REN1, Wupeng XIAO2, Zhigang LAI1, Qing ZHU2, Canbo XIAO1
1Sun Yat-sen University, 2Xiamen University
In summer, the Madden-Julian Oscillation (MJO) greatly influences the intraseasonal variability of the South China Sea (SCS). Previous studies have revealed MJO effects on surface chlorophyll concentration, but the impact of the MJO on the ecosystem's structure and functionality remains unexplored. Here, we investigated the marine ecosystem response to the MJO by analyzing phytoplankton pigment data collected in cruises during from 2010 to 2014. The results indicated the strong influence of the MJO on the structure of phytoplankton size classes (PSCs) in the upper 50 m of the SCS basin. To further explore the ecosystem's response to MJO, we utilized a well-calibrated physical-biogeochemical model (ROMS-CoSiNE) of the SCS to conduct numerical experiments with and without MJO forcings. Our model demonstrated that MJO-induced deep mixing and upwelling increased nutrients in the upper layer, increasing the Chl concentration with a higher proportion of nanophytoplankton (15%) and a lower proportion of picophytoplankton (−20%). Moreover, The MJO-forced model experiment exhibited a substantial enhancement in primary production (56%) and export production (23%), resulting in a notable decrease in the e-ratio. This reduction in the e-ratio cannot be attributed to changes in PSCs but can be explained by the time lag between primary and export production. This lag was prolonged by the physical processes of upwelling and mixing, which slows down the particle sinking. Our results emphasize the important role of MJO in regulating the ecosystem at intraseasonal scale, thus improving our comprehension of the nonsteady dynamics of ecosystems in the SCS.
OS14-A005
Temporal Variation of Summer Hypoxia off the Northern Changjiang (Yangtze River) Estuary During 1997-2014 and Its Association with ENSO
Feng ZHOU1#+, Xiao MA2, Anqi LIU3,1
1Ministry of Natural Resources, 2State Oceanic Administration, 3Hohai University
Hypoxia off the Changjiang Estuary has been the subject of much attention, yet systematic observations have been lacking, resulting in a lack of knowledge regarding its long-term change and drivers. By revisiting the repeated surveys of dissolved oxygen (DO) and other relevant hydrographic parameters along the section from the Changjiang Estuary to the Cheju Island in the summer from 1997 to 2014, rather different trends were revealed for the dual low-DO cores. The nearshore low-DO core, located close to the river mouth and relatively stable, shows that hypoxia has become more severe with the lowest DO descending at a rate of -0.07 mg/L/yr and the thickness of low-DO zone rising at a rate of 0.32m/yr. The offshore core, centered around 40-m isobath but moving back and forth between 123.5°E–125°E, shows large fluctuations in the minimum DO concentration, with the thickness of low-DO zone falling at a rate of -1.71m/yr. The probable factors affecting the minimum DO concentration in the two regions also varies. In the nearshore region, the decreasing minimum DO is driven by the increase in both stratification and primary productivity, with the enhanced extension of the Changjiang Diluted Water (CDW) strengthening stratification. In the offshore region, the fluctuating trend of the minimum DO concentration indicates that both DO loss and DO supplement are distinct. The DO loss is primarily attributed to bottom apparent oxygen utilization caused by the organic matter decay and is also relevant to the advection of low-DO water from the nearshore region. The DO supplement is primarily due to weakened stratification. Our analysis also shows that the minimum DO concentration in the nearshore region was extremely low in 1998, 2003, 2007 and 2010, related to El Niño signal in these summers.
OS14-A013
Modelling Sediment-water Fluxes: Impacts on Coastal Oxygen Dynamics and Hypoxia
Zheng CHEN1, Liuqian YU1#+, Jiying LI2, Jianping GAN2
1The Hong Kong University of Science and Technology (Guangzhou), 2The Hong Kong University of Science and Technology
Sediment-water exchanges are crucial for coastal oxygen dynamics, whereas their representation in ocean biogeochemical models is often too crude to characterize the nonlinear benthic-pelagic interactions. This work aims to quantify the effects of sediment-water fluxes on coastal water biogeochemistry and assess the sensitivity of model-simulated oxygen dynamics and hypoxia to the representation of sediment-water exchanges. To that aim, we implement a variety of sediment-water exchange schemes of different complexity levels to a coupled physical-biogeochemical model of the Pearl River Estuary (PRE), a large eutrophic system experiencing bottom-water hypoxia in summer. Model results show that the simulated oxygen dynamics and hypoxic extent are markedly sensitive to the representation of sediment-water nutrient and oxygen fluxes. In addition to directly contributing to hypoxia formation through sediment oxygen consumption, sediment-released nutrients, especially the more limiting nutrient phosphorus, significantly promote hypoxia development by fueling water column organic matter production. In the meantime, hypoxic conditions accelerate the legacy phosphorus release which further sustains water column productivity and maintains hypoxic conditions. These results highlight the critical role of sediment-water exchanges in regulating coastal ocean biogeochemistry and the importance of credibly representing sediment-water interactions to model ocean ecosystems.
OS14-A022
Modeling the Underlying Drivers of Spatiotemporal Evolution of CO2 Uptake in the Plume Discharged from the Changjiang River
So-Young KANG1+, Jae-Hong MOON1#, Daehyuk KIM1, Hyun-Chae JUNG2, Subin KIM3
1Jeju National University, 2Chonbuk National University, 3Korea Institute of Atmospheric Prediction System
The river-discharged freshwater from the Changjiang River in the East China Sea plays an important role in coastal systems in terms of their uptake of atmospheric carbon dioxide (CO2). In this study, Regional Ocean Modeling System (ROMS), a three-dimensional ocean circulation model combined biological-carbonate module (FENNEL) is used to investigate the underlying drivers of the spatiotemporal evolution of oceanic CO2 uptake within the Changjiang River Plume (CRP) in the summer of 2016.The simulated pCO2 exhibited distinct variations in the CRP, decreasing sharply from its maximum in the estuary to its minimum in the nearshore, and then moderately increasing to offshore. As a result, the CRP spatially transitioned from a source in the estuary to a strong sink of atmospheric CO2 in the nearshore, and to a weak oceanic CO2 uptake in offshore. Comparative experiments show that these evolution of seawater pCO2 were mainly driven by the combined effects of physical mixing and biological activity. Strong vertical mixing due to tides and upwelling inhibits biological production in the estuary despite being supplied with a high concentration of nutrients from the river, leading to high pCO2. In the nearshore region, the biological activity becomes stronger due to weakened vertical mixing, therefore triggering inorganic carbon consumption resulting in strong inorganic carbon consumption and consequent absorption of atmospheric CO2. Meanwhile, when the reduced pCO2 is transported from nearshore to offshore, oceanic CO2 uptake is mainly modulated by air-sea exchange as biological uptake is weakened in association with phosphate limitation. Additional experiment with increased concentrations of phosphate supplied from the river demonstrates the influence on the magnitude of CO2 uptake within the CRP. This study provides better insight into the understanding of the dynamical processes driving the spatiotemporal evolution of oceanic CO2 uptake within the river plume.
OS14-A006
A Particle Tracking Model for Margalefidinum Polykrikoides Bloom in Lower Chesapeake Bay: Integrating Biological Processes and Kinetic Parameter
Jian SHEN1#+, Xin YU2, Jilian XIONG3, Qubin QIN4, Jiabi DU5
1Virginia Institute of Marine Science, 2Oak Ridge Institute for Science and Education (ORISE), Supported by NCCOS, 3University of Washington, 4East Carolina University, 5Texas A&M University at Galveston
A particle tracking model has been developed to simulate harmful algal blooms (HABs) of Margalefidinium polykrikoides in Chesapeake Bay. The model takes advantage of both Lagrangian and Eulerian approaches, capable of simulating both particle trajectories and changes in algal biomass. The model integrates algal dynamics, including mixotrophic growth, respiration, and mortality, as well as diel vertical migration (DVM). It has demonstrated successfully simulations of M. polykrikoides bloom in lower Chesapeake Bay. Recently, the model has been upgraded by integrating Ocean Land Colour Imager (OLCI) satellite imagery for HAB forecasting. This involves using satellite imagery for weekly sequential correction of algal biomass and location, enabling a 7-10 day forecast of HABs. The results indicate that DVM, mixotrophic growth, respiration, and mortality significantly influence the accuracy of forecasting. To improve model accuracy, an autocalibration capability has been developed to determine sensitive biological parameters with high uncertainty using satellite imagery. Overall, we demonstrate that combining a particle tracking model, biological process, high-resolution satellite data, and autocalibration of biological parameters is an effective approach to track and predict HABs in coastal and estuarine waters. This methodology provides a novel framework for forecasting HAB locations and intensities, offering valuable insights for coastal managers.
OS14-A019
A Hybrid Ensemble Biogeochemical Data Assimilation System for the Red Sea: Implementation and Evaluation
Siva Reddy SANIKOMMU1#+, Yixin WANG1, Mohamad EL GHARAMTI2, Matthew MAZLOFF3, Ariane VERDY4, Georgios KROKOS1, Rui SUN3, Aneesh SUBRAMANIAN5, 6, Angela Kuhn CORDOVA4, Bruce CORNUELLE3, Ibrahim HOTEIT1
1King Abdullah University of Science and Technology, 2National Center for Atmospheric Research, 3University of California San Diego, 4Scripps Institution of Oceanography, 5University of Colorado Boulder, 6
A hybrid ensemble system is implemented for data assimilation (DA) into a coupled physical-biogeochemical ocean model of the Red Sea. The system consists of a Massachusetts Institute of Technology general circulation model (MITgcm) coupled with the Nitrogen-version of the Biogeochemistry, Light, Iron, Nutrients, and Gases (N-BLING) model, both configured at a 4 km resolution. The assimilation is based on the Data Assimilation Research Testbed (DART) and combines a time-varying ensemble generated using the Ensemble Adjustment Kalman filter (EAKF) with a pre-selected quasi-static (monthly varying) ensemble. The system is designed to assimilate observations of both physical (satellite sea surface temperature, altimeter sea surface height, and in-situ temperature and salinity) and biological (satellite chlorophyll) variables. The DA system accounts for uncertainties in the atmospheric forcing in MITgcm. Sensitivity experiments are conducted to delineate the impact of each physical and surface chlorophyll observation assimilation. The state estimates are evaluated against independent satellite and in-situ Glider observations of temperature, salinity, sea surface height, chlorophyll, and oxygen. The results indicate that the assimilation of physical fields significantly improves the physical state, both at the surface and subsurface, leading to slight improvements in surface chlorophyll. Enhanced subsurface temperatures and salinities contribute to an improvement in chlorophyll at deeper layers. Assimilation of surface chlorophyll significantly enhances surface chlorophyll forecasts and also improves the chlorophyll and oxygen features at the DCM and SOM, although their magnitudes are slightly overestimated overall. However, it reduces the assimilation improvements for physical variables, which is attributed to the lack of accounting for uncertainties in NBLING forcing. A new strategy, one-way coupled DA, in which physical and biological observations update the biological state while the physical state is updated only by physical observations, is developed and demonstrated to mitigate the negative impact of chlorophyll assimilation on the physical state.
Session Chair(s): Chin-Chang HUNG, National Sun Yat-sen University
OS09-A023
| Invited
Nickel for Tricho: The Implication on Blue Carbon Cycling
Tung-Yuan HO#+
Academia Sinica
Nitrogen (N2) fixation is a crucial process in the ocean that affects how carbon is cycled. The process provides fixed nitrogen to marine phytoplankton that absorb CO2 through photosynthesis. Trichodesmium (Tricho) is a major group of diazotrophic cyanobacteria responsible for large amount of N2 fixation in the tropical and subtropical oceans. N2 fixation is catalyzed by nitrogenase, an enzyme that is vulnerable to O2 and oxidative stress generated in photosynthesis. However, unlike other diazotroph, Trichodesmium can perform both N2 fixation and photosynthesis simultaneously, allowing it to thrive and bloom in the surface waters of the oligotrophic ocean. How Trichodesmium carry out N2 fixation and photosynthesis simultaneously under high light conditions is an important question. Our early research has shown that nickel (Ni) is vital for the growth of Trichodesmium and can increase its N2 fixation rates and superoxide dismutase (SOD) activities. We found that Trichodesmium needs high levels of Ni to maintain its N2 fixation rates under high light conditions. Our hypothesis is that the metal requirement for SOD synthesis would be elevated to reduce reactive oxygen species (ROS) stress while ROS production is elevated in photosystems under high light conditions. Our most recent study, Chen et al. (2022), has further uncovered how NiSOD protects N2 fixation in Trichodesmium from oxidative damage by reducing ROS stress under high light conditions. By producing and purifying the recombinant protein through E. coli, we custom-designed NiSOD antibody to validate and quantify its concentrations in Trichodesmium. We eventually demonstrated the critical role of NiSOD in Trichodesmium. The findings of the study explain why Trichodesmium can carry out N2 fixation and photosynthesis simultaneously and bloom in the high light environment of the tropical ocean. These results may also shed light on the mechanisms of photoinhibition for phytoplankton under high solar radiation conditions.
OS09-A026
Biological Carbon Pump in the East China Sea and the South China Sea
Chin-Chang HUNG#+
National Sun Yat-sen University
To mitigate the impacts of climate change, achieving carbon neutrality has become paramount. Previously, the estimation of negative carbon emissions was primarily focused on green carbon and yellow carbon. However, the oceans constitute one of the major global carbon pools, absorbing approximately 25-30% of the carbon dioxide from the atmosphere. Taiwan is committed to achieving net-zero carbon emissions by 2050, and the contribution of carbon absorption by the surrounding water cannot be overlooked. Therefore, this study aims to comprehensively review research on biological carbon pump (BCP or called particulate organic carbon (POC) flux) entering the bottom of the euphotic zone) sinks in the East China Sea, the South China Sea and the Kuroshio waters (i.e. the western North Pacific Ocean) near Taiwan. The results indicated that, the carbon sequestration in the East China Sea, the northern South China Sea, and the western North Pacific Ocean were 49.3±14.9, 19.9±4.5, and 26.4±7.8 Mt-CO2 yr−1, respectively. In other words, carbon sequestration by deep-sea blue carbon can account for about 33.5% of annual carbon emissions in Taiwan, suggesting that BCP cannot be ignored in order to achieve net-zero carbon emissions. Estimation uncertainty of BCP in seas around Taiwan can be affected by overlapping exclusive economic zone (EEZ), lateral carbon transport, typhoons, mesoscale eddies, and internal waves, but detailed spatiotemporal investigations in seas around Taiwan are urgent needed.
OS09-A022
Spatial Variation of POC Fluxes in Low Latitude Northwest Pacific Ocean
Hsueh-Han HSIEH#+, Chin-Chang HUNG
National Sun Yat-sen University
The oceanic carbon flux serves as a critical carbon sink on global scale. Over the past decades, the biological carbon pump (also called particulate organic carbon, POC, flux) has been acknowledged as a highly efficient mechanism for sequestering atmospheric carbon dioxide. To understand the oceanic carbon sink in warm oligotrophic waters, particularly in the low-latitude Northwest Pacific Ocean (NWP), we measured POC flux using floating sediment traps at depths of 150, 500, and 1000 m across latitudes 6°, 7.5°, 10°, and 13° with a longitudinal range of 134° to 135°. Our results revealed significant spatial variations in the particulate organic carbon (POC) fluxes at 150m in latitudes 6°, 7.5°, 10°, and 13°, measuring 31.7 ± 13.7, 42.0 ± 4.2, 35.4 ± 15.9, and 41.2 ± 2.3 mg-C m-2 d-1, respectively. The attenuation coefficient (b-value) of sinking particles exhibited variations across latitudes, with values of 0.23, 0.15, 0.18, and 0.26 for latitudes 6°, 7.5°, 10°, and 13°, respectively. Notably, the NWP area displayed a lower b-value compared to other low-latitude stations (SEATs). Our study further identified environmental factors affecting this variability, including high sea surface temperatures (SST), low productivity, and a thin mixed layer (33-40 m) within the study area. By assessing the variation in POC fluxes at different depths using a traditional particle degradation curve (i.e., Martine curve), we found that POC fluxes do not smoothly decrease with depth, suggesting that lateral particle transport may be the main reason for the increase in BCP at deep waters. Moreover, the BCP measured by sediment traps cannot be predicted by satellite remote sensing combined with biogeochemical models. Consequentially, it reveals that current satellite-biogeochemical models need to be revised, especially in oligotrophic warm waters in the future.
OS09-A031
Effect of Flood on Distribution and Characteristics of Particulate Organic Carbon in the Changjiang Estuary and Adjacent Seas
Ying LUO1+, Hai-Yan JIN2#, Dewang LI2, Ningxiao YU1,2, Bin WANG2, Jianfang CHEN3, Zhongqiang JI2, Ling CHEN2, Zhi YANG3
1Shanghai Jiao Tong University, 2Ministry of Natural Resources, 3State Oceanic Administration
The Changjiang River is the third largest river in the world, and its runoff carries a large amount of suspended particulate matter and nutrients into the East China Sea, which affects the biogeochemical processes of the Particulate Organic Carbon (POC). In the summer of 2020, there were continual flood events in the Changjiang River basin. Water samples were collected in the Changjiang Estuary and adjacent waters and total suspended particulate matter(TSM), POC, δ13C, nutrients, and chlorophyll a (Chl a) were analyzed in August 2020 to understand the impact of this flood on the distribution and characteristics of POC in the East China Sea. The results show that the distribution area of the Changjiang diluted water (CDW) in the East China Sea in 2020 is much wider than that in the normal year. Majority of the suspended particles transported by the Changjiang River are trapped in the turbidity front, and most of the terrigenous POC is difficult to transport across the turbidity front to the sea. The offshore area has higher POC concentrations than in previous years, with a wider area and further location. A significant positive correlation between surface Chl a and POC concentrations in the offshore indicates that high biomass contributes to the high POC concentrations. The δ13C values ranged from -23.02‰~-18.99‰ in the offshore high POC concentrations area and it confirms that the POC is mainly derived from marine sources. Offshore high POC concentrations area is under the influence of CDW and has high Chl a and nutrient concentrations, it indicates that the higher and wider POC concentrations offshore are due to the extension of the CDW. Furthermore, the δ13C value also indicates that the flood still carries part of the terrestrial organic matter signal to offshore.
OS09-A024
Sediment Trap and Empirical-derived Biological Carbon Pump in the South China Sea and Satellite-based Estimate
Syun-Han WU1+, Chin-Chang HUNG1#, Yung-Yen SHIH2, Hsueh-Han HSIEH1
1National Sun Yat-sen University, 2Republic of China Naval Academy
The transportation of carbon from the sea water surface to the deeper ocean involves two distinctive processes: physical and biological processes. The biological processes known as the biological carbon pump (BCP), plays a crucial role. The study builds upon previous research demonstrating that sinking flux of particulate organic carbon (POC) at the bottom of euphotic layer serves as a direct indicator of BCP efficiency. We compared BCP measured by sediment trap and satellite-derived algorithms in the South China Sea between May 2012 and December 2022. The BCP-measured by traps ranged from 25 to 110 mg C m-2 d-1. while satellite-derived BCP varied from 2 to ~132 mg C m-2 d-1. Both BCPs did not show remarkable correlation between sediment trap and satellite-derived algorithms. Our BCP measured by traps indicates that, satellite-derived values may underestimate by approximately 50-60% during winter, while satellite-derived values are closer to or slightly higher than trap-measured values by about 10-15% during summer. Overall, our research suggests current satellite-derived algorithms need to be improved including more seasonal sediment trap dataset in the future.
OS09-A019
| Invited
Differences of Primary Productivity Using Different Bio-tracers in Low-latitude Waters
Yung-Yen SHIH1#+, Yen-Tu LI1, Pei-Yu FU1, Chin-Chang HUNG2, Yun-Zhen CHANG 1
1Republic of China Naval Academy, 2National Sun Yat-sen University
Primary productivity (PP) is not only a fundamental entry point of blue carbon into the ocean but also a significant factor influencing climate change. However, the difference of PP between using stable and radioactive isotopic bio-tracers limit our understanding of marine carbon fixation rate by phytoplankton, i.e. PP. This study focuses on digging out the difference of PP estimated by using different bio-tracers, i.e. 13C and 14C, in the northern South China Sea, the waters around Taiwan, including 12 cruises from 2019 to 2023; in the northwest Pacific, the seas around Palau in 2023; and in the Indian Ocean, the lagoons and seas around Sri Lanka in 2023. The result showed a statistically significant positive linear relationship between 13C- and 14C-PP in different oceanic regions. It implicated that both 13C and 14C are proper bio-tracers for PP incubation among these low-latitude waters. It is however that the mean difference between 13C-PP and 14C-PP within the euphotic zone, i.e. 13C- and 14C-IPP, ~40% would cause a misestimate of large spatiotemporal-scale marine IPP since most of the satellite-based IPP was calibrated with the 14C-IPP database. It means that the potential difference between 13C- and 14C-IPP has to be minimized so that the satellite-based IPP can be validated by the compromised in situ 13C- and 14C-IPP data to further reach the true oceanic blue carbon.
OS09-A003
| Invited
Atmospheric CO2 Dynamics Under Oceanic Emission in the Equatorial Pacific
Shuangling CHEN#+
Second Institute of Oceanography, Ministry of Natural Resources
As the largest CO2 source (ocean releases CO2 into the atmosphere), the equatorial Pacific plays an important role in the global carbon cycle. It is known that, during El Nino (La Nina), the equatorial upwelling is suppressed (enhanced), which could reduce (increase) the supply of CO2 to the surface. Under climate change, how would these climate events affect atmospheric CO2 dynamics in the equatorial Pacific? In this study, we analyzed the seasonal and interannual dynamics of atmospheric CO2 concentrations observed from different satellite missions including NASA’s OCO-2, VIRS, and GOSAT-2, with a focus on the effect of climate events. It is the first time that a cross-sensor validation was conducted by comparing with in situ observations to provide some insights on the use of these CO2 satellite data in quantifying air-sea CO2 fluxes.
OS09-A016
Wet Nitrogen Deposition and Its Role in Biological Carbon Pump in the North Pacific Warm Pool
Vicente ABEDNEKO1#+, Chin-Chang HUNG1, Yung-Yen SHIH2, Hsueh-Han HSIEH1
1National Sun Yat-sen University, 2Republic of China Naval Academy
In the oligotrophic waters of the Pacific Ocean, wet deposition may play a crucial role in nutrient cycling and the growth of phytoplankton new production, the primary producers supporting marine ecosystems. This study investigates the significance of deposition-derived nitrogen (N) in driving new production of phytoplankton, particularly in the open ocean in the Pacific Warm Pool (PWP). We examined the influence of rainfall events in 10 sites within a 600,000 km2 Exclusive Economic Zone (EEZ) of the Republic of Palau territory on the deposition process and subsequent phytoplankton response in the summer of 2023. We found that long-term rainfall events can significantly enhance wet deposition of N to the surface ocean, promoting phytoplankton growth through the alleviation of surface N limitation. Our findings shows that NO3- concentration varied from 1 to 24 µM, whereas NO2 concentration ranged from 0.06 to 3 µM. Current estimates of deposition-derived nitrogen in open ocean systems are likely underestimated, due to movement of rainfall and time of precipitation collected. Using time and distance for calibrating wet deposition, estimates of wet deposition are more than twice the current collected value being deposited unto the oligotrophic water. The total nitrogen flux ranged from 0.20 to 0.71mg-N/m2/day-1 and it may contribute for about 5.7 to 20.4% of biological carbon pump (~20 mg-C/m2/day) in oligotrophic water in western North Pacific Ocean if a Redfield ratio is used. As a consequence, wet and dry nitrogen deposition may support important nutrient supply in the oligotrophic warm waters. Because future stratification may cause nutrient-rich water from the subsurface to be transported downward to the euphotic zone.
Session Chair(s): Yuki HARADA, Nagoya University, Yutian CAO, Sun Yat-sen University, Shaosui XU, University of California, Berkeley
PS03-A006
| Invited
Numerical Simulation of the Martian Diffuse Aurora
Yuki NAKAMURA1#+, Naoki TERADA2, Francois LEBLANC3, Ali RAHMATI4, Hiromu NAKAGAWA2, Shotaro SAKAI5, Kiyoka MURASE6, Ryuho KATAOKA7, Lauriane SORET8, Jean-Claude GERARD8, David A. BRAIN9, Kanako SEKI1,1
1The University of Tokyo, 2Tohoku University, 3National Centre for Scientific Research, 4University of California, Berkeley, 5Keio University, 6The Graduate University for Advanced Studies, 7National Institute of Polar Research, 8University of Liege, 9University of Colorado Boulder
Imaging UltraViolet Spectrograph (IUVS) instrument onboard the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft has discovered a new type of the Martian aurora, diffuse aurora, spanning across the nightside of Mars accompanied by the arrival of solar energetic particles (SEPs) at Mars. The origin of the Martian diffuse aurora has been believed to be SEP electrons since its discovery, however, previous numerical models failed to reproduce the altitude profiles of the Martian diffuse aurora when using the observed SEP electron energy spectrum. We have developed a Monte Carlo model to calculate the altitude profile of the CO2+ ultraviolet doublet (UVD) emission intensity due to precipitation of both solar energetic electrons and protons. Case studies for the December 2014 and September 2017 SEP events showed a significant contribution of SEP protons with energy greater than MeV at low altitude peaks, and the simulated altitude profiles were in good agreement with the IUVS observations. In this talk, we will also present preliminary results for the simulation of the Martian diffuse aurora including the effects of crustal magnetic fields.
PS03-A005
Photochemical Escape on Mars During the Global Dust Storm and the Solar Flare
Hao GU1#+, Xu HUANG1, Jun CUI1,2
1Sun Yat-sen University, 2Chinese Academy of Sciences
Atmospheric escape is crucial for driving the long-term climate evolution and habitability on Mars. Traditional studies usually focused on the long-term variations of atmospheric escape on Mars with solar radiation or Martian seasons. However, the variability of atmospheric escape with short-term drivers, such as the dust storm and solar flare, have not been thoroughly investigated. With the aid of multi-instrument measurements made by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft as well as a one-dimensional Monte Carlo model, we have evaluted the effects of the 2018 global dust storm (GDS) and the 2017 X8.2 solar flare on the photochemical escape of hot atomic C, N, and O on Mars. During the GDS, our calculations suggest that the C, N, and O escape rates are generally reduced by ~30-40% relative to the quiet, pre-GDS state, in direct contrast to the well-known result of GDS-induced strong enhancement of atomic H escape. During the solar flare, we find a modest decrease in the C escape rate of 8% about 1 h after the flare peak, followed by a recovery to the pre-flare level several hours later. However, an opposite trend is found for the N escape rate during the same period, which shows an increase of 20% followed by a recovery to the pre-flare level. We further propose that the above variations of photochemical escape essentially reflects the competition between two effects: the modification of hot atom production driven by the variation of the background atmosphere and the reduction of escape probability due to atmospheric expansion. During the GDS, the latter is usually more effective and responsible for the overall reduction of photochemical escape on Mars. During the solar flare, the former dominates the atomic N and O escape, while the latter dominates the atomic C escape.
PS03-A014
Joint Observations of the Response of Martian Induced Magnetosphere to the Upstream IMFs by of Tianwen1 and MAVEN
Lihui CHAI#+
Institute of Geology and Geophysics, Chinese Academy of Sciences
Since the orientation of the induced magnetospheres is controlled by the direction of the upstream IMFs, it has been long interested how induced magnetospheres response to the upstream IMF direction changes. However, to investigate, a two-points observation is needed with one spacecraft monitoring the upstream IMFs and the other observing the downstream induced magnetospheres’ response. Such kind of investigations is now possible for Martian induced magnetosphere since both the Mars Orbiter of Tianwen-1 mission and MAVEN mission carry magnetometers. In this study, we present a case study to show that when the direction of the IMF changes suddenly from a (-By, -Bz) to (+By, -Bz) in MSO coordinates system, a unipolar-like magnetic field (only +Bx) is presented in the downstream magnetic field time serious observations when the spacecraft travels from dusk side (+Y) to dawn side (-Y). It seems a simultaneous response is presented in the downstream draped field morphology. However, the geometry is way much complicated than we expected. More cases and detailed analyses will be discussed.
PS03-A008
Characteristic Timescales for the Dayside Martian Ionosphere: Chemistry, Diffusion, and Magnetization
Yutian CAO1#+, Jun CUI1,2
1Sun Yat-sen University, 2Chinese Academy of Sciences
Different boundaries could be defined in a planetary ionosphere where the dominant process in function switches from one to the other. Identifying these boundaries and understanding their variations are hence crucial for disentangling the complexity of the ionosphere. Focusing on Mars, we perform a data-driven analysis of various boundaries and the associated time constants based on the multi-instrument measurements made by the Mars Atmosphere and Volatile Evolution mission during six campaigns that sample broadly different internal and external conditions. The boundaries we investigate include the photochemical equilibrium (PCE) boundary, the magnetic frozen boundary, the ion collision boundary, and the ion gyration boundary. Our analysis reveals systematic solar cycle and diurnal variations in that all boundaries tend to be elevated at enhanced solar activity and on the dayside and dusk side of Mars. The variations with the magnetic environment are not observed for all boundaries except for the PCE boundary that exhibits an obvious elevation in strongly magnetized regions. Finally, our analysis suggests interesting species-dependent variations of different boundaries. In particularly, the PCE boundary shows the largest variability among all, with reduced boundary locations for all terminal species (NO+, HCO+, O2+, and H3O+) and one extra nonterminal species (CO+) owing to different chemical properties rendered 232by different ions.
PS03-A007
| Invited
Low-energy Electrons Observed by Mercury Plasma Particle Experiment Onboard Mio/BepiColombo During Its First Three Mercury Flybys
Sae AIZAWA1#+, Mathias ROJO2, Nicolas ANDRE3, Jean-André SAUVAUD4, Yoshifumi SAITO5, Alain BARTHE4, Emmanuel PENOU4, Shoichiro YOKOTA6, Andrey FEDOROV3, Quentin NENON4, Moa PERSSON7, Lina HADID8, Dominique FONTAINE8, Wataru MIYAKE9, Bruno KATRA8, Markus FRAENZ10, Norbert KRUPP10, Go MURAKAMI11
1Laboratoire de Physique des Plasmas, 2Institute for Research in Astrophysics and Planetology, 3University of Toulouse, 4Institute for Research in Astrophysics and Planetology (IRAP), National Center for Scientific Research (CNRS) - University of Toulouse (UPS) - National Center for Space Studies (CNES), 5Japan Aerospace Exploration Agency / Institute of Space and Astronautical Science, 6Osaka University, 7Swedish Institute of Space Physics, 8National Centre for Scientific Research/Sorbonne Université-Ecole Polytechnique, 9Tokai University, 10Max Planck Institute for Solar System Research, 11Japan Aerospace Exploration Agency
BepiColombo, launched in October 2018, is currently en route to Mercury. Although its planned orbit insertion is set for December 2025, BepiColombo continuously gathers new measurements during Mercury flybys. Throughout the cruise phase, the two spacecraft remain docked, with Mio protected behind the MOSIF sun shield, resulting in a limited field of view for Mio's instruments. Despite this constraint, the Mercury Plasma Particle Experiment (MPPE) on board Mio has already provided unique insights into the structure and dynamics of Mercury’s magnetosphere. Specifically, observations from the first Mercury flyby in October 2021 revealed time-dispersed injections of electrons of a few keV precipitating onto the surface and potentially causing X-ray fluorescence. Observations from the second Mercury flyby in June 2022 revealed on the nightside horn-crossing plasma sheet as well as inverted-V electron populations indicating the presence of Region 2 Field-Aligned-Current at Mercury previously unreported by MESSENGER. Finally, observations from the third Mercury flyby in June 2023 revealed fine-scale structures in plasma sheet electron populations. This presentation will summarize the characteristics of these low-energy electron populations observed during the first three Mercury flybys.
PS03-A013
Updated Status of BepiColombo and Initial Reports on Mercury Flyby Observations
Go MURAKAMI1#+, Johannes BENKHOFF2
1Japan Aerospace Exploration Agency, 2European Space Agency
The ESA-JAXA joint mission BepiColombo is now on the track to Mercury. After the successful launch of the two spacecraft for BepiColombo, Mio (Mercury Magnetospheric Orbiter: MMO) and Mercury Planetary Orbiter (MPO), commissioning operations of the spacecraft and their science payloads were completed. BepiColombo will arrive at Mercury in the end of 2025, and it has 7-years cruise with the heliocentric distance range of 0.3-1.2 AU. The long cruise phase also includes 9 planetary flybys: once at the Earth, twice at Venus, and 6 times at Mercury. Even before arrival, we already obtained fruitful science data from Mercury during three Mercury flybys completed on 1 October 2021, 23 June 2022, and 19 June 2023. We performed science observations with almost all the instruments onboard Mio and successfully obtained comprehensive data of Mercury’s magnetosphere such as magnetic fields, plasma particles, and waves. Here we present the updated status of BepiColombo/Mio, initial results of the science observations during the Mercury flybys, and the upcoming observation plans.
PS03-A012
Comparison of Electron Energy Spectra from a Numerical Model and Kaguya and ARTEMIS Observations Above the Lunar Surface
Masahisa KATO1#+, Yuki HARADA2, Masaki NISHINO3, Yoshifumi SAITO4, Shoichiro YOKOTA5, Futoshi TAKAHASHI6, Hisayoshi SHIMIZU7, Shaosui XU8, Andrew POPPE8, Jasper HALEKAS9
1Kyoto University, 2Nagoya University, 3Japan Aerospace Exploration Agency, 4Japan Aerospace Exploration Agency / Institute of Space and Astronautical Science, 5Osaka University, 6Kyushu University, 7The University of Tokyo, 8University of California, Berkeley, 9The University of Iowa
The lunar surface directly interacts with its ambient plasma because the Moon does not possess a dense atmosphere. The interactions cause lunar surface charging. Kato et al. (2023) developed a numerical model of photo-emitted electron energy spectra and compared the modeled and observed spectra, thereby discussing variations of the lunar surface potential based on a case study. The spatial distribution of the lunar surface potential is important for understanding of the near-surface dynamics of charged particles. However, the inhomogeneity of the lunar surface potential over a wide range of spatial scales is not fully characterized yet. In this study, we analyze electron observations by Kaguya and THEMIS-ARTEMIS probes in comparison with the numerical model of photo-emitted electron energy spectra to investigate the spatial distribution of the lunar surface potential. In particular, we discuss the surface potential variations associated with lunar magnetic anomalies.
PS03-A015
Statistical Study on L-O Mode Saturn Kilometric Radiation
Junhao PAN#+, Shengyi YE, Siyuan WU
Southern University of Science and Technology
The statistical characteristics of L-O (Lefthand-Ordinary) mode Saturn Kilometric Radiation (SKR) is studied using data from the Cassini spacecraft's RPWS instrument. We selected L-O mode events based on intensity, circular polarization and the DF (Direction Finding) results by using the electric field spectrogram data. A total of 488 L-O mode SKR events were selected from 2004 to 2017 by the L-O mode selection method. And their statistical characteristics are investigated. The frequency, intensity, and polarization properties of the L-O mode emissions are summarized. L-O events are mainly found in the frequency range of 20 - 400 kHz, with intensities ranging from 1e-15 to 1e-11 V2m2/Hz. They exhibit elliptical polarization in general. In the statistics of global distribution, we find the low-frequency emissions cannot enter the plasma. As the frequency gradually increasing, the L-O mode emissions can enter the torus. Saturn plasma torus may reflect low-frequency L-O mode emissions due to its high plasma density. We analyzed the global spatial distribution of polarization and found that high linear polarization emissions mainly occur at high latitude, while high circular polarization emissions mainly occur at low latitude.
Session Chair(s): Yufeng LIN, Southern University of Science and Technology, Tao CAI, Macau University of Science and Technology, Min DING, Southern University of Science and Technology
PS14-A003
| Invited
Divergence and Vorticity of Deep Rotating Convection in Jupiter’s Poles
Tao CAI#+
Macau University of Science and Technology
Jupiter’s polar vortices can be naturally generated in deep rotating convection model. Here we report the result on the divergence and vorticity of Jupiter’s polar vortices based on the deep convection model. We found a negative correlation between divergence and vorticity in Jupiter’s northern hemisphere, as predicted by theoretical models. However, this correlation weakens within the cyclones compared to their surroundings. We also found that the strength of correlation varies with the depth of the atmosphere, diminishing away from the interface between the convectively unstable and stable layers. The resolution of measurements used to calculate divergence and vorticity significantly affects this correlation. Furthermore, our findings suggest that the geostrophic approximation may not be suitable to Jovian atmosphere. We observed a transfer of vorticity from the deeper atmospheric layers to the upper ones. Additionally, kinetic energy appears to move from smaller to larger scales, aligning with observational data. This research enhances our understanding of Jupiter’s structure and dynamics. This work is supported by the National Natural Science Foundation of China (No. 12173105), and Guangdong Basic and Applied Basic Research Foundation (No. 2414050002575).
PS14-A001
Prospects for Jovian Seismology with the Lenghu Planetary Telescope
Yiqing ZOU1+, Fei HE2#, Dali KONG3, Yufeng LIN4, Zhaojin RONG2, Zhonghua YAO5, Yong WEI2
1The Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Shanghai Astronomical Observatory, Chinese Academy of Sciences, 4Southern University of Science and Technology, 5The University of Hong Kong
Jupiter is one of the top priorities for deep space exploration in China and other countries. A crucial and remaining unclear scientific topic in Jupiter exploration is depicting the structure of its interior. To gain insight into the internal structure of Jupiter, we propose to study Jupiter’s innards by planetary seismology. The ground-based observation, namely the Jupiter Seismologic Interferometer Polarization Imager (SIPI) in Lenghu, will be developed to obtain the Doppler velocity distribution on the surface of Jupiter and identify the oscillation signals. Lenghu has good observation conditions in China and even the world, providing a novel insight into studying the interior of Jupiter. This will also be the first study of the interior of Jupiter by using asteroseismology in China, which has significant implications for the exploration mission of Jupiter.
PS14-A005
Numerical Simulation of Double-diffusive Convection Driven Dynamos
Wei FAN+, Yufeng LIN#
Southern University of Science and Technology
The Earth's liquid outer core is mainly composed of iron and nickel, mixed with some lighter liquid elements such as silicon or oxygen. The crystallization of the inner core releases light elements and latent heat at the inner-core boundary (ICB), while the mantle extracts thermal energy from the outer core at the core-mantle boundary (CMB). This process leads to density anomalous that drive thermal and compositional convection in the liquid outer core. The diffusivity of thermal and compositional convection are different, leading to the- called top-heavy double diffusive convection when both thermal and compositional background gradients are destabilizing. However, most dynamo models actually assume that the diffusivity of thermal and compositional are equal, known as the co-density formalism, which can remove one degree of freedom and simplify the model. In our study, we conducted numerical simulations of 3-D dynamo using double diffusion formalism. We particularly force on the strong field regime in which the Lorentz force plays an important role. We analyze the flow structures, magnetic field morphonology and force balance of the double-diffusive convection driven dynamos and make some comparisons to the co-density dynamo. Implications for planetary dynamos will be discussed.
PS14-A002
| Invited
Formation and Evolution of the Isidis Basin on Mars Based on Numerical Simulations
Min DING1#+, Meng-Hua ZHU2, Mark WIECZOREK3, Ana-Catalina PLESA4, Kai WÜNNEMANN5
1Southern University of Science and Technology, 2Macau University of Science and Technology, 3Institut de Physique du Globe de Paris, 4German Aerospace Center, 5Museum für Naturkunde
The 1,800-km-diameter Isidis basin, located on Mars’ north-south dichotomy boundary, is the last impact basin formed in the ancient Noachian period, which may represent the end of early bombardment on Mars. The basin is ringed by a circumferential graben system, and shows the largest gravitational anomaly. The landing sites of the Perseverance, InSight, Curiosity, and Tianwen-1 missions are all close to the Isidis basin, whose data have the potential to provide further constraints on the regional composition and crustal structure. Albeit the prospected better understanding of this region with new observations, the long-term evolution of the regional crust and lithospheric structure is still unclear. In this study, we simulate the formation of the Isidis basin and investigate the evolution of the local crust and lithosphere by combining the shock physics code iSALE-2D and finite-element software Abaqus FEA. We propose a three-stage evolution: 1) An impactor with a diameter of ~220 km and velocity of ~8 km/s hits Mars ~3.9 Gyr ago. The geothermal gradient at that time is assumed to be ~ 20 K/km. In this scenario, a basin comparable with the size of Isidis forms. 2) The post-impact viscous relaxation, facilitated by the impact-induced melt pool, occurs on timescales of millions of years and relaxes the thickened crustal annulus but retains the basin structure. 3) The final stage considers the viscoelastic response of the regional thickened lithosphere to the surface basaltic deposits of several kms at ~3.5 Gyr ago, which induces lithospheric depression, positive gravity anomaly, and tensile stress that are comparable with observations. In summary, we explain the thermo-mechanical evolution of Isidis and provide self-consistent constraints on the regional thermal evolution. The viscoelastic relaxation of Isidis can help elucidate the origin of a super-isostatic mascon and exemplify the applicability of a thin-plate lithospheric flexure model to impact basins.
PS14-A004
Application of 3D Magnetic Inversion to Reveal the Depth Range and Magnetization of Magnetic Sources in the Lunar Crust
Hongyi WANG+, Shuo YAO#, Liang Hui GUO
China University of Geosciences
This work tries to apply a classic 3D magnetic amplitude inversion to reconstruct the magnetic sources in the lunar crust. We study the sources under a weak and a strong magnetic anomaly in Mare Tranquillitatis and in Oceanus Procellarum on the Moon respectively. Since there is no globally measured surface magnetic field for the Moon, a crustal magnetic anomaly model with grid resolution of 0.2° derived from in-orbit measurements is used. Firstly, we check the validity and robustness of the inversion technique for lunar condition with a synthetic model. Secondly, according to the test results of the model, the depth to the bottom of the magnetic source is fixed by the boundary identified by a relative criterion, which is 20% of the recovered maximum magnetization. Thirdly, the inversion is used to study the two lunar anomalies. The depth to the bottom of the magnetic carriers is about 30 km and 50 km under Oceanus Procellarum and Mare Tranquillitatis. The volumes of the two magnetic sources are at the scale of 10^4 and 10^5 km^3, respectively. Considering the different gravity anomalies in the two studied regions, the inversion results support that the magma intrusions containing different abundances of metallic iron are the most possible origins of the magnetic sources in the studied two regions. Besides, the thermal states of lunar crust under the two studied maria were probably different during the acquisition process of remanent magnetization. This work suggests that it is worthy to develop more complete 3D magnetic inversion technique for lunar magnetic anomalies in future.
PS14-A008
A Crustal Magnetic Field Model of Mars with Spherical Harmonic Degree Up to 140
Lin TIAN#+, Hao LUO, Aimin DU, Yasong GE, Ying ZHANG, Kuixiang ZHANG
Chinese Academy of Sciences
We develop a new crustal magnetic field model of Mars with spherical harmonic degree up to 140, which is based on orbiting measurements from Mars Global Surveyor (MGS), Mars Atmosphere and Volatile Evolution (MAVEN), and surface measurements from InSight and Zhurong. We follow the techniques from M14 model[Morschhauser et al., 2014] to inverse the spherical harmonic coefficients, including assigning different weights to the data of different sources, eliminating outliers with huber norm fitting, and employing the horizontal gradient of Bz component as L1 regularization term in the final model. It is found that our new model achieves the best spatial resolution ever before (~150 km). The unweighted misfits between our model and the MGS MPO, MGS AB/SPO and MAVEN are 8.0 nT, 9.9 nT, and 8.1 nT, respectively. Compared with the previous models, our model predictions are consistent with the surface measurements at InSight and Zhurong landing sites since the surface data are involved in the model inversion, which indicates the surface measurements are crucial to constrain the model downward continuation. The model characterizes the small-scale stratigraphic units on Mars, for example, the Lucus Planum, Apollinaris Patera, Hadriaca Patera, etc., contributing to the research of the structures of magnetic anomalies on Mars with different scales and the evolution of Martian dynamo.
PS14-A011
| Invited
Estimation of Geothermal Heat Flow Distribution in China and Adjacent Regions Using the Machine Learning Method
Ting YANG#+, Yijun LIU, Peng GUO
Southern University of Science and Technology
Geothermal heat flow (the heat lost by the Earth in unit time and unit area) is the most important observation to characterize the underground thermal state of the Earth in different regions. Due to the huge time and capital cost of direct measurement of geothermal heat flow, the spatial coverage of heat flow observations has been low and uneven. In order to solve this issue, researchers have implemented various geological and geophysical data proxies, such as seismic tomography, shallow geomagnetic anomalies, and tectonic thermal age, to estimate geothermal heat flow indirectly. Compared to other methods, machine learning methods can synthesize different types of data and give the best estimates of geothermal heat flow. However, the model score in the test set is usually much lower than that in the training set in previous heat flow machine learning models, casting doubt on the ability and reliability of using these machine learning models and proxies for heat flow prediction. We systematically investigate the influence of different factors on surface heat flow in mantle convection models and investigate the feasibility and accuracy of machine learning models in estimating geothermal heat flow. Using a global database, we carefully compared and screened data from different sources and incorporated high-quality geological and geophysical observation data obtained in China in recent years to train a new machine learning model for estimating geothermal heat flow in China. Compared with traditional interpolation methods, the new prediction of regional geothermal heat flow has much higher accuracy and is more closely related to tectonic structures. This newly predicted geothermal heat flow model may serve as a basis for further constraining the thermal and rheological structure of the lithosphere in China and for local geothermal resource exploration.
Session Chair(s): Tianran SUN, Chinese Academy of Sciences
PS17-A018
| Invited
Unique Global Viewing of Earth’s Dynamic Magnetosphere with the Solar Wind – Magnetosphere – Ionosphere Link Explorer (SMILE)
Colin FORSYTH1#+, Steve SEMBAY2, Chi WANG3, C. Philippe ESCOUBET4, Graziella BRANDUARDI-RAYMONT1, Lei DAI3, Lei LI3, Xiao-Xin ZHANG5, Li JING3, David AGNOLON4, Walfried RAAB4, Chris RUNCIMAN4, Benjamin VANOUTRYVE4, Sylvain VEY4, Arnaud MASSON4, Wen CHEN3, Xing SHI3, Javier SANCHEZ PALMA6, Sergio MORENO-AGUADO6, Andy READ2, Eric DONOVAN7, Emma SPANSWICK7, Jenny CARTER2, Hyunju CONNOR8, Tianran SUN3, Andrey SAMSONOV1, Jianhua ZHENG3, Syau-Yun HSIEH9, David SIBECK8, Georgios NICOLAOU1
1University College London, 2University of Leicester, 3Chinese Academy of Sciences, 4European Space Agency, 5China Meteorological Administration, 6Airbus, 7University of Calgary, 8NASA Goddard Space Flight Center, 9Johns Hopkins University Applied Physics Laboratory
The interaction between the plasma leaving the Sun and neutral particles in the exospheres of solar system bodies results in a soft X-ray emission which, if imaged, can help us to understand these interactions of the solar wind with these bodies on large scales. At magnetized bodies, the impact of the solar wind results in global deformations of planetary magnetic fields and physical processes at kinetic, fluid and global scales that capture and energise particles within magnetospheres which ultimately deposits energy into planetary ionospheres and atmospheres. While in-situ measurements have provided deep insights into small-scale processes in these regions, the global configuration of the system remains elusive, revealed only through simulation or climatological empirical models. A new joint mission between the European Space Agency (ESA) and Chinese Academy of Sciences (CAS) will provide a unique global view of our near-Earth space environment, enabling us understand the links between the Sun, magnetosphere and ionosphere. Due for launch in mid-2025, the SMILE (Solar wind Magnetosphere Ionosphere Link Explorer) mission is a novel endeavour to observe the coupling of the solar wind with the magnetosphere through to the ionosphere. To do this, SMILE will remotely sense the magnetosheath and cusps through X-ray emissions from solar wind charge exchange – a process by which neutral particles in Earth’s exosphere exchange charges with highly charged heavy solar wind ions. SMIILE will also measure the in-situ magnetic field and plasma properties and remotely sensing the northern hemisphere aurora in UV. In this talk, we will present the underlying science of the SMILE mission as well as the latest mission developments from ESA, CAS and the international instrument teams. We will also highlight possible synergies with existing missions and ground-based facilities, enabling global and local plasma processes to be studied in unprecedented detail and context.
PS17-A010
A Lunar-based Soft X-ray Imager (LSXI) for the Earth’s Magnetosphere
Fei WEI#+, Songwu PENG
Chinese Academy of Sciences
The Earth’s magnetosphere and that of the other planets such as the Jupiter plays a key role in the interaction between the solar wind and the planet’s upper atmosphere. Global perspective is crucial to understanding the overall interaction of the solar wind with magnetosphere. We propose to use the Moon as an ideal platform to obtain the global view of the Earth’s magnetosphere by a Lunar-based Soft X ray Imager (LSXI), which is to answer the call for the Chinese Lunar Exploration Program Phase IV. LSXI is a wide field-of-view Soft X-ray telescope, which can obtain X-ray image of the Earth’s magnetosphere based on the solar wind charge exchange (SWCX) X-ray emission, and it is capable of continuously monitoring the evolution of geospace conditions under the impact of the solar wind and simultaneously observe the bow shock, magnetosheath, magnetopause and cusps for the first time. In this report we represent the updated progress on the manufacture of the micro-pore optics and detectors for the LSXI, the performance of the prototype and its calibration results.
PS17-A017
Geospace X-ray Imager Mission (GEO-X)
Kumi ISHIKAWA1#+, Yuichiro EZOE1, Ryu FUNASE2,3, Harunori NAGATA4, Yoshizumi MIYOSHI5, Hiroshi NAKAJIMA6, Ikuyuki MITSUISHI5, Masaki NUMAZAWA1, Daiki ISHI2, Ralf C. BODEN2, Yuki SATOH6, Yosuke KAWABATA7, Ryota FUSE3, Shintaro NAKAJIMA2, Landon KAMPS4
1Tokyo Metropolitan University, 2Japan Aerospace Exploration Agency, 3The University of Tokyo, 4Hokkaido University, 5Nagoya University, 6Kanto Gakuin University, 7Tokyo University
GEO-X is a small satellite mission aimed at capturing X-ray images and visualizing the Earth’s magnetosphere (Ezoe et al., 2023, J. Astron. Telescope and Instrum.). The magnetospheric X-rays are generated by Solar Wind Charge eXchange (SWCX) reaction between a highly charged-state ion in the solar wind and a neutral atom in the exosphere. The SWCX emissions are expected to be strong at the magnetosheath and the cusps where high-density the solar wind ions exist, which mean that the X-ray emissions can reflect the magnetospheric structure and are expected as a remote imaging tool (Sibeck et al., 2018, Space Sci. Rev.). A payload for the GEO-X is required to reduce a size and a weight dramatically from conventional payloads onboard past X-ray astronomy missions. The GEO-X satellite will carry a light-weight X-ray imaging spectrometer consisting of an ultra light-weight telescope, a CMOS detector, and an optical blocking filter. The payload is designed to have a wide filed of view (5x5 deg) and a good spatial resolution (10 arcmin) in the 0.3-2 keV range. The GEO-X satellite is planned to be injected to a low-latitude orbit for visualization of the magnetosphere from outside the magnetosphere. Calculation of a number of detectable SWCX events were conducted with past solar wind data. The instrument background including a radiation noise was estimated using GOES proton fluxes and the GEANT4 simulation. Data points are counted in accordance with conditions which meet a signal-to-noise ration above 20 in each year between 1998 and 2011. The number of detectable data points is 43.7 per year with an average duration of 7 hours and has peak around the solar maximum. The GEO-X satellite is aimed to be launched around the solar maximum of solar cycle 25.
PS17-A003
Magnetopause Deformations Caused by Bow Shock Transients: 3-D Global Hybrid Simulations and Soft X-ray Imaging
Zhong-Wei YANG1+, Tianran SUN1#, Bin-Bin TANG1, Can HUANG1, Riku JARVINEN2, Parks K. GEORGE3, Dimitra KOUTROUMPA4, Xiaocheng GUO1, Chi WANG1
1Chinese Academy of Sciences, 2Finnish Meteorological Institute, 3University of California, Berkeley, 4Laboratoire Atmosphères, Milieux, Observations Spatiales
The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) is a joint mission of the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS). Primary goals are investigating the dynamic response of the Earth's magnetosphere to the solar wind (SW) impact via simultaneous in situ magnetosheath plasma and magnetic field measurements, X-Ray images of the magnetosheath and magnetic cusps, and UV images of global auroral distributions. Magnetopause deformations associated with magnetosheath high speed jets (HSJs) under a quasi-radial IMF condition are studied using a three dimensional (3-D) global hybrid simulation. Soft X-ray intensity calculated based on both physical quantities of solar wind proton and oxygen ions is compared. We obtain key findings concerning deformations at the magnetopause: Magnetopause deformations appear related to the foreshock transients; X-ray intensities estimated using solar wind H+ and self-consistent O7+ ions are consistent with each other. Visual spacecraft are employed to discuss the discrimination ability for capturing magnetopause deformations on Lunar and polar orbits, respectively. The magnetopause dynamics under other solar wind conditions will also be discussed. These preliminary results might contribute to the pre-studies for the SMILE and LEXI missions by providing qualitative and quantitative soft X-ray estimates of magnetospheric dynamic processes.
PS17-A014
A Three-dimensional Functional Cusp Model
Yuqi GONG#+, Tianran SUN
Chinese Academy of Sciences
The Earth's magnetopause and cusps are vital source regions for X-ray emissions in the geospace environment. Soft X-rays are generated through the solar wind charge exchange (SWCX) process, where high charge state solar wind ions (e.g., C6+, O7+, O8+, Fe12+) exchange charges with neutrals (e.g., H, H2O). From the soft X-ray imaging detection, it becomes possible to derive the large scale properties of the cusp. Despite advancements, reconstructing the three-dimensional (3D) cusp boundary from a two-dimensional (2D) X-ray image remains a challenging task, particularly in situations with rapid solar wind variations. In this context, we propose a 3D asymmetric model for cusp boundaries in functional form, based on MHD simulations. This model, characterized by six parameters, is based on an assumption that the cusp boundaries can be approximated as an ellipse on each spherical shell with a given altitude. This functional cusp model is expected to be used to reconstruct the cusp boundaries from X-ray images observed by future missions such as Solar wind Magnetosphere Ionosphere Link Explorer (SMILE), a joint space science mission proposed and supported by the European Space Agency and the Chinese Academy.
PS17-A012
Neural Network-based Method for Reconstructing the Earth's Three-dimensional Magnetospheric Structure from X-ray Images
Dalin LI#+, Rongcong WANG, Tianran SUN
Chinese Academy of Sciences
Soft X-ray imaging is a new method used to observe the structure of the Earth's magnetosphere. Reconstruction of the Earth's three-dimensional (3-D) magnetospheric structure from 2-D soft X-ray images is an important research topic in astronomical imaging and exploration. In this study, computed tomography (CT) is investigated for application to the planned Solar wind Magnetosphere Ionosphere Link Explorer (SMILE), where resulting images are collected at varying small angles. The restricted geometry of SMILE results in sparse projection data and reduced reconstruction quality. As such, a new algorithm is proposed, based on cone-beam computed tomography (CBCT) and utilizing 3-D generative adversarial networks (GAN) to supplement the 2-D soft X-ray images and increase the angular coverage of the projections. A complement optimization backpropagation network (COBN) is then used to reconstruct high-quality 3-D X-ray emissivity profiles in the magnetosphere. Meanwhile, the cumulative nature observation results may lead to the neglect of space environmental events at smaller time scales, introducing discontinuities in the study of space event variations. To address this issue, this paper proposes a neural network model driven by both OMNI observations and SXI observation X-ray images to dynamically estimate magnetospheric changes over an integrated time period. Experimental validation using MHD and Jorgensen models demonstrates that with the proposed methods exhibits a significant improvement in both peak signal-to-noise ratio (PSNR) and structural similarity index (SSIM) compared to the direct reconstructions. Consequently, the presented neural network-based approach appears to be feasible and aligns with the practical requirements of observational tasks, providing a novel avenue for dynamically estimating magnetospheric changes.
PS17-A009
Data Processing and Analysis for Lobster-eye-type Soft X-ray Imager
Songwu PENG#+, Fei WEI, Zhihui LV
Chinese Academy of Sciences
The wide field soft X-ray dynamic image of the Earth's magnetosphere can characterize its interaction process with the solar wind, such as the Soft X-ray Imager onboard SMILE satellite. The lobster-eye-type grazing incidence optical system is currently a powerful means to achieve large field of view soft X-ray imaging. Focusing is formed by multiple reflections of incident soft X-ray photons through an astonishing number of micrometer sized channel pores. The typical cross-shaped focal spot images that interact with each other cause complexity in image restoration. We have developed a simulation software for the lobster-eye-type soft X-ray imaging system based on geometric ray tracing, which can achieve fast imaging of complex soft X-ray sources. Based on this software, a machine learning algorithm is used to implement a functional relationship database between the optical source image and the image plane image. The orientation and intensity of soft X-ray sources can be quickly inverted from the X-ray images. The data processing method was validated based on the structural parameters of the SMILE satellite soft X-ray imager, which can be used for data processing and analysis of similar soft X-ray imagers.
PS17-A004
The Ultraviolet Imager on Smile
Yongmei WANG1#+, Xiaohong LIU1, Guojun DU2, Jinghua MAO1, Pengda LI1, Weipeng HUANG1, Jiu LIU1, Shui YU1, Xiao-Xin ZHANG3, Fei HE1, Sylvain VEY4
1Chinese Academy of Sciences, 2Beijing Institute of Space Mechanics & Electricity, 3China Meteorological Administration, 4European Space Agency
The UltraViolet Imager (UVI) is one of payloads aboard on the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) satellite. SMILE is a joint space science mission between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS). The main science object is to establish the solar wind properties simultaneously with the imaging instruments and in suit instruments. UVI is a compact FUV Camera with a 9.9degree circle field-of-view (FOV) to image the aurora oval of N2 Lyman-Birge-Hopfield (LBH) in 160-180nm spectral range on the SMILE orbit. The high stray light suppression level to ensure the aurora under fully sunlit conditions could be detected. The high sensitivity with sufficient spatial resolution will ensure the capability for tracking the aurora variation. UVI instrument is led by National Space Science Center (NSSC), CAS in China,collaborating with Europe Space Agency (ESA) and Centre Spatial de Liege (CSL) in Belgium. In this paper, the details including the optical design, detector system, structure & thermal control system, calibration on ground and initial performance will be reported.
PS17-A015
Enhancing Aurora Boundary Detection with Deep Convolutional Neural Networks: A Study for the SMILE Satellite Program
Ziyue WANG#+, Yongmei WANG
Chinese Academy of Sciences
SMILE (Solar Wind Magnetosphere Ionosphere Link Explorer) is the first-time joint science mission between European Space Agency (ESA) and National Space Science Center (NSSC) of the Chinese Academy of Sciences (CAS). Its core scientific objective is to investigate the dynamic response of the Earth’s magnetosphere to the solar wind. One of the payloads carried on it, UVI (Ultraviolet Imager), is a telescope designed with coaxial four-mirror optics, which continuously performs far-ultraviolet imaging of global auroras for nearly 50 hours. This study presents a novel approach for the preprocessing and segmentation of aurora images, utilizing the method CLACH (Contrast Limited Adaptive Histogram Equalization) followed by the U-net neural network for precise morphological and boundary extraction. In consideration of the in-orbit imaging for aurora often exhibits characteristics such as low contrast and high noise, the initial preprocessing stage employed CLACH to enhance the dynamic range and contrast of the raw aurora images, effectively highlighting faint auroral features against a variable background. Subsequently, the enhanced images were subjected to segmentation and classification by using the U-net neural network, renowned for its efficiency in segmenting complex images. The adaptation of U-net to aurora images proved highly effective, with the model achieving an impressive accuracy of 94% and a Jaccard index (IOU) of 0.81. These results demonstrate the robustness and applicability of our methodology to challenging aurora image analysis tasks. The integration of CLACH preprocessing with U-net segmentation represents a significant advancement in aurora research, offering a reliable tool for the detailed study of auroral structures and dynamics.
Session Chair(s): Zhonghua YAO, The University of Hong Kong
PS02-A009
Ancient Oceans on Mars: Hypotheses and New Evidence
Long XIAO#+, Jiannan ZHAO, Yutong SHI, Jun HUANG
China University of Geosciences
Martian surface has a great planetary dichotomy separating southern highlands from a huge area of northern plains. Informal hypothesizing by geologists considered the possibility of an Earth-like water body occupying the northern lowland. Considerable evidence was also accumulated for ancient water-related phenomena on the planet and the related implications for an Earth-like global hydrological cycle was recognized as closely tied to the ancient northern plains water body, named Oceanus Borealis. However, this hypothesis has been debated for several decades. The main piece of evidence against this hypothesis is that simulations from Mars climate models show that the atmosphere and temperature conditions of early Mars could not have supported the existence of oceans. Also, there is no evidence of Marine sedimentary rocks in the northern plains. Here we report the newly discovered evidence that support there was an ancient ocean in the northern lowland of Mars. China’s Tianwen-1/Zhurong rover encountered boulder-sized samples of the Vastitas Borealis Formation (VBF) that signifies the depositional processes that occurred in Oceanus Borealis. We report here on the first in situ analysis of the VBF that reveals sedimentary structures and features in surface rocks that suggest that the VBF was deposited in a marine environment, providing direct support for the existence of an ancient (Hesperian) ocean on Mars.
PS02-A006
| Invited
Microbiological and Geochemical Research in High-altitude Mars Analogs
Wei LIN1#+, Jianxun SHEN2, Yan CHEN2, Li LIU2
1Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Chinese Academy of Sciences
Recent years have witnessed an increasing number of international missions to search for signs of life on Mars. Mars analogs on Earth are invaluable sources for preliminary investigations. We select Earth’s near space and the Qaidam Basin as analogs for astrobiology research. Characterized by extreme coldness, desiccation, low atmospheric pressure, and intense ultraviolet (UV) and cosmic radiation, Earth’s near space at 20-40 km altitude serves as a natural analog to the Martian surface. After developing the Chinese Academy of Sciences Balloon-Borne Astrobiology Platform (CAS-BAP), we exposed selected microbial and desert soil samples to near space at 20-40 km altitude. We found magnetotactic bacteria with intracellular magnetite crystals illustrated enhanced survivability and produced more magnetosomes. Additionally, four bacterial strains isolated from exposed Qaidam desert soils displayed high resistance to a variety of environmental stressors, including high concentrations of aqueous perchlorate, indicating that some microorganisms may survive the shallow subsurface brines on Mars. The selection of landing sites and exploration targets is crucial for the success of life detection in Mars exploration. Within the Mars-like, hyperarid Qaidam Basin, we have identified more habitable niches for microbial colonization at depths of 5-25 cm in various landscapes, compared to both the surface and deep subsurface. Soils from the distal alluvial fan exhibit a higher propensity for concentrating pedogenic organic carbon compared to those from other landforms. Moreover, sedimentary organic matter can be preserved in aqueous deposits under hyperarid and highly radiative conditions. The observed increasing trends in organic carbon content along rivers suggest potentially slow degradation rates of organic matter relative to their exposure timescale. Our research provides new insights into the ongoing biosignature detection on Mars and highlights that the subsurface of distal fans or lake beds are promising candidate targets for life detection.
PS02-A001
Investigation of the Energetic and Radiative Transfer Properties of Exospheric Hydrogen with the Hydrogen Emission Line Interferometric Explorer (HELIX)
Walter HARRIS1+, Edwin MIERKIEWICZ2, Jason CORLISS1#, Dolon BHATTACHARYYA3, Gonzalo Augusto CUCHO PADIN4
1University of Arizona, 2Embry-Riddle Aeronautical University, 3University of Colorado, 4NASA Goddard Space Flight Center
The Hydrogen Emission Line Interferometric eXplorer (HELIX) is a mission concept to study the vertical distribution [H](z) and transport flux of p(H) in of neutral hydrogen in the transition region from Earth’s upper atmosphere into the exosphere. This transition, which is common to all terrestrial planets, plays a key role in the exchange of mass, momentum, and energy, between the atmosphere, local magnetic environment, and interplanetary space. It is also major factor in atmospheric evolution. HELIX builds on a legacy of space-based dayside measurement of the hydrogen emission that provides the basic parameters of neutral population and hint at the underlying escape kinetics. However, these data do not contain the detailed lineshape information necessary to obtain the thermal and non-thermal components of H energy distribution. HELIX simultaneously obtains the intensity and lineshape of emission from two transitions (Ly-alpha and Lyman-beta). The science instrument is a dual spectral channel, all-reflective spatial heterodyne spectrometer (SHS), a field-summing two-beam interferometer that combines high resolving power and etendue in a compact format. HELIX combines a spectral resolving power of R>200000 (dV > 1.5 km/s) with field of view (FOV) = 0.3 degrees and can be used to measure [H](z) and p(Z), characterize the thermal and non-thermal components of hydrogen, and resolve terrestrial hydrogen from background sources. HELIX is designed for study of terrestrial hydrogen but is scaled for use in interplanetary probes for similar explorations at Mars and Venus. It would launched on a high-heritage SmallSat into a polar LEO trajectory where it would obtain daily scans of the hydrogen intensity and lineshape from Earth’s limb into the middle exosphere. The resulting dataset would be used to constrain existing models of the evolution of hydrogen kinetics in the thermosphere.
PS02-A007
The Observation of Planetary Plasmas in the Extreme Ultraviolet from Ultra-small Platforms
Kazuo YOSHIOKA1#+, Masaki KUWABARA2, Go MURAKAMI3, Ichiro YOSHIKAWA1
1The University of Tokyo, 2Rikkyo University, 3Japan Aerospace Exploration Agency
The EQUULEUS CubeSat (6U) mission was successfully launched in November 2022 as a sub-payload of NASA's Space Launch System. EQUULEUS aims to demonstrate trajectory control techniques within the Sun-Earth-Moon region, with a pioneering mission to reach the Earth-Moon L2 point (EML2) as a nano-spacecraft. The mission carries a compact extreme ultraviolet (EUV) telescope called PHOENIX. Comprising a multilayer-coated mirror (6 cm diameter with Mo/Si coating), a metallic bandpass filter, and a 2-D photon counting device with microchannel plate and resistive anode, PHOENIX is optimized for observing the ionic helium emission line (wavelength of 30.4 nm), a significant component of Earth's plasmasphere. PHOENIX has obtained images of the plasmasphere in one flame by venturing far from Earth. This presentation will introduce the mission concept, telescope design, and results of Earth’s plasmasphere observation obtained during the cruising phase. The future applications of the PHEONIX for planetary exploration will also be discussed.
PS02-A010
The Characteristics of Sheared E× B Flow with the Varying Ion–neutral Collisions in Experimental Simulation
Xiao ZHANG1+, Yu LIU2, Jiuhou LEI2#
1Deep Space Exploration Laboratory, 2University of Science and Technology of China
Velocity shear flow is one of the main excitation mechanisms plasma instability, especially in partially ionized plasma occurred in astrophysical and space environments. However, most previous studies focused on fully ionized plasma. The emergence and development of plasma instabilities are significantly impacted by the inelastic collisions between the ions and neutrals in the partially ionized plasma, such as the charge exchange. The collision effect of neutral components and charged particles on velocity shear are still unclear. In this study, the effect of the ion–neutral collisions on the sheared E × B flow was experimentally investigated based on the ground experimental device, the response of velocity shear to neutral collisions was experimentally studied, and it was found that the development of velocity shear and instability will be significantly affected by neutral collisions. In the weak collision range, the shear-driven plasma instability, such as Kelvin–Helmholtz instability, was excited by the velocity-sheared flow. However, increasing ion–neutral collisions resulted in a decrease in the magnitude of the sheared E × B flow due to charge exchange–induced drag forces. Consequently, the Kelvin–Helmholtz instability is suppressed, and the Rayleigh–Taylor instability is triggered. The underlying mechanism was elucidated through experimental findings and numerical analysis. The result of this study proposes that a transition between the two modes occurred with increasing ion–neutral collision strength. This result is important for understanding the solar chromosphere and prominence and planetary ionospheres, where the plasma is partially ionized and the sheared E × B flow is often encountered.
PS02-A004
Planetary Exploration Outreach and Education Using NASA’s Solar System Treks
Emily LAW1#+, Brian DAY2
1NASA Jet Propulsion Laboratory, 2National Aeronautics and Space Administration
NASA's Solar System Treks Project (SSTP) online portals provide web-based suites of interactive visualization and analysis tools to enable mission planners, planetary scientists, students, and the general public to access mapped data products from past and current missions for a growing number of planetary bodies. The Solar System Treks portals (https://trek.nasa.gov) are being used for site selection and analysis by NASA and its international and commercial partners supporting upcoming missions. The portals offer great benefits for science, technology, engineering, art, and math (STEAM) education and public outreach, providing access to data from a wide range of instruments aboard a variety of past and current missions. As a component of NASA's Science Activation Infrastructure, they are available as resources for NASA STEAM programs, and to the greater STEAM community. As new missions are planned to a variety of planetary bodies, these tools facilitate public understanding of the missions and engage the public in the process of identifying and selecting where these missions will land. Today, 13 web portals in the program are available to the public. This list includes portals for the Moon; the planets Mercury, Venus, and Mars; the asteroids Bennu, Ryugu, Vesta, and Ceres; and the outer moons Titan, Europa, Ganymede and Phobos. The Icy Moons Trek portal features seven of Saturn’s smaller icy moons. All of the portals are unified under a project home site with supporting content. These web-based portals are free resources and publicly available.
This presentation for AOGS will detail and share examples of the how the portals can be applied to Planetary exploration outreach and education.
Session Chair(s): Young Jay RYU, The University of Chicago
PS18-A002
| Invited
A Hydrogen-enriched Layer in the Topmost Outer Core Sourced from Deeply Subducted Water
Yongjae LEE1#+, Taehyun KIM1, Joseph O’ROURKE2, Jeongmin LEE1, Stella CHARITON3, Vitali PRAKAPENKA3, Rachel HUSBAND4, Nico GIORDANO4, Hanns-Peter LIERMANN4, Sang-Heon SHIM2
1Yonsei University, 2Arizona State University, 3The University of Chicago, 4Deutsches Elektronen-Synchrotron
The Earth’s core–mantle boundary presents a dramatic change in materials, from silicate to metal. While little is known about chemical interactions between them, a thin layer with a lower velocity has been proposed at the topmost outer core (Eʹ layer) that is difficult to explain with a change in concentration of a single light element. Here we perform high-temperature and -pressure laser-heated diamond-anvil cell experiments and report the formation of SiO2 and FeHx from a reaction between water from hydrous minerals and Fe–Si alloys at the pressure–temperature conditions relevant to the Earth’s core–mantle boundary. We suggest that, if water has been delivered to the core–mantle boundary by subduction, this reaction could enable exchange of hydrogen and silicon between the mantle and the core. The resulting H-rich, Si-deficient layer formed at the topmost core would have a lower density, stabilizing chemical stratification at the top of the core, and a lower velocity. We suggest that such chemical exchange between the core and mantle over gigayears of deep transport of water may have contributed to the formation of the putative Eʹ layer.
PS18-A019
| Invited
Structure and Transport Properties of Chalcogen Hydrides at High Pressure
Jaeyong KIM#+, Zhongyan WU
Hanyang University
The structure and electronic transport properties of Se and Te elements under high hydrogen pressure were measured. For Se hydrides, the enhanced superconductivity values were obtained and on the verge of the β-Po–bcc phase transition, up to 9.4 K at 140 GPa. The superconducting transition is evidenced by a direct zero resistance drop and was further verified through its suppression under an external magnetic field with at 140 GPa. An abnormally high resistance peak preceding the drop to zero resistance exhibits granular superconductivity. Our studies demonstrate that selenium does not react with hydrogen at 182 GPa at room temperature or 102 GPa with laser heating to 3000 K, suggesting that the synthesis of selenium hydride requires higher energy conditions than the ones suggested in theoretical predictions. The results of the structural evolvements of Te, which shows similar trends, under hydrogen will be also presented.
PS18-A004
| Invited
Innovative High-pressure XRD Experiments with APS-U Sources and the Potential Applications for Geoscience
Changyong PARK1#+, Eric ROD1, Eduard ONECIC1, Curtis KENNEY-BENSON1, Richard FERRY1, Arun BOMMANNAVAR1, Maddury SOMAYAZULU1, Nenad VELISAVLJEVIC2
1Argonne National Laboratory, 2Lawrence Livermore National Laboratory
The APS-U source will deliver 500 times enhanced brightness, 20 times reduced horizontal source size, and 1000 times enhanced coherent fraction compared to the previous APS source, which improves all aspects of the performances of the existing techniques and enables new techniques. An experimental end station, 16-ID-E, at the High-pressure Collaborative Access Team (HPCAT), Sector 16 of the Advanced Photon Source, is planning to utilize all of these enhanced specifications and enable new capabilities for innovative high-pressure XRD experiments. To deliver highly coherent beam with maximum thermal and mechanical stabilities, a new horizontally deflecting double crystal monochromator (HDCM) and a horizontally deflecting double multilayer monochromator (HDMM) are introduced in the 16-ID-C optical hutch. The newly enabled XRD-based techniques include 2D scanning probe X-ray Diffraction Imaging (XDI) with a sub-micron resolution, grain Bragg Coherent Diffraction Imaging (g-BCDI) for polycrystalline materials, and time-resolved XRD (t-XRD) for fast pressure- and temperature-ramp experiments. The XDI technique will utilize 100 nm focused beam with pre-figured elliptical mirror optics; the g-BCDI will combine a priori established multi-grain crystallography approach to enable a registered, tracking probe of a targeted grain in polycrystalline sample while the sample’s texture evolves with pressure; and t-XRD will utilize the improved flux that is further boosted by HDMM’s 1-2 % bandwidth and a MHz frame-rate detector system, respectively. These XRD based techniques are compatible with each other in terms of the instrumental requirements so that they can be developed on an integrated experimental table. Each technique’s potential applicability to high-pressure planetary- and geo-sciences is discussed in this presentation. HPCAT operations are supported by DOE-NNSA’s Office of Experimental Sciences. The Advanced Photon Source is a U.S. Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357.
PS18-A017
Experimental Study on the Deformation Microstructures of Epidote Blueschists and Implications for Seismic Properties in Warm Subduction Zones
Yong PARK#+, Haemyeong JUNG
Seoul National University
To understand the deformation microstructures and seismic properties at the top of a subducting slab in warm subduction zones, deformation experiments of epidote blueschist were conducted in simple shear by using a modified Griggs-type (solid-medium high-pressure deformation) apparatus. Deformation experiments were performed under pressure of 0.9–1.5 GPa, temperature of 400–500 ℃, shear strain (γ) of 0.4–4.5, and shear strain rate of 1.5×10-5–1.8×10-4 s-1. After experiments, transmission electron microscopy (TEM) observations and electron backscattered diffraction (EBSD) mapping revealed that the lattice preferred orientation (LPO) of glaucophane was developed by dislocation creep, somewhat affected by the cataclastic flow at high shear strain. On the other hand, the LPO development of epidote was considered to have been affected by dislocation creep under a shear strain of 2<γ<4, but the LPO was highly affected by cataclastic flow with rigid body rotation under a high shear strain (γ>4). After calculating the seismic properties of deformed epidote blueschists, the average seismic velocities for P-wave (Vpaver) and S-wave (Vsaver) were determined to be in the range of 7.19–7.63 km/s and 4.22–4.47 km/s, respectively, and the seismic anisotropies for P-wave and S-wave were in the range of 4.5–11.0% and 3.91–6.40%, respectively. The Vpaver and Vsaver of experimentally deformed epidote blueschist were reduced about 8–13% and 6–11%, respectively, compared to the seismic velocities of lithospheric mantle surrounding the slab. Our experimental results indicate that the magnitude of shear strain and rheological contrast between component minerals plays an important role on the formation of LPOs of glaucophane and epidote. In addition, our seismic property calculations suggest that volume proportion and LPO types of constituent minerals are important factors in controlling the seismic velocity and anisotropy observed in warm subduction zones.
PS18-A011
Experimental Determination of the Interatomic Force Constant Under Extreme Environments
Dongzhou ZHANG1#+, Bin CHEN2
1The University of Chicago, 2University of Hawaii at Manoa
Interatomic force constant is an essential physical parameter in condensed matter that determines numerous physical phenomena such as phase transition, thermodynamics, elasticity and isotopic behavior. Although modern computational algorithms are capable of computing interatomic force constant under certain assumptions, an accurate experimental determination of interatomic force constant is imperative, especially under extreme pressure and temperature conditions. In this study, we present our recent experiments that aim to constrain the interatomic force constants in different solid systems (metallic Fe and mantle silicates) at high pressure-temperature conditions. Our study relies on different synchrotron X-ray based-techniques, such as Mossbauer spectroscopy and single crystal diffraction. We also discuss the application of our force constant measurement on the isotope fractionation behavior of earth and planetary materials.
Session Chair(s):
PS17-A011
| Invited
The LAPYUTA Mission: Life-environmentology, Astronomy, and Planetary Ultraviolet Telescope Assembly
Fuminori TSUCHIYA1#+, Go MURAKAMI2, Atsushi YAMAZAKI2, Shingo KAMEDA3, Akifumi NAKAYAMA 3, Masahiro IKOMA 4, Tomoki KIMURA5, Chihiro TAO6, Ryoichi KOGA7, Jun KIMURA8, Kei MASUNAGA2, Shotaro SAKAI9, Masami OUCHI10,4, Masaomi TANAKA1, Shin TORIUMI2, Kazuo YOSHIOKA10, Masato KAGITANI1
1Tohoku University, 2Japan Aerospace Exploration Agency, 3Rikkyo University, 4National Astronomical Observatory of Japan, 5Tokyo University of Science, 6National Institute of Information and Communications Technology, 7Nagoya University, 8The University of Osaka, 9Keio University, 10The University of Tokyo
Ultraviolet spectroscopy is one of the most powerful tools to cover a wide range of scientific fields, from planetary science to astronomy. Here, we propose a future UV space telescope, LAPYUTA (Life-environmentology, Astronomy, and PlanetarY Ultraviolet Telescope Assembly), selected as a candidate for JAXA’s 6th M-class mission in 2023. Launch is planned for the early 2030s. LAPYUTA will perform spectroscopic and imaging observations in the far ultraviolet spectral range (110-190 nm) with a large effective area (>300 cm2) and a high spatial resolution (0.1 arcsec). LAPYUTA's orbit is designed as an elliptical orbit with an apogee of about 2,000 km and a perigee of 1,000 km to avoid the influence of the geocorona when observing oxygen and hydrogen atoms and the Earth's radiation belt. LAPYUTA will accomplish the following four objectives, which are related to two scientific goals: understanding (1) the habitable environment and (2) the origin of structure and matter in the universe. Objective 1 focuses on the subsurface ocean environments of Jupiter's icy moons and the atmospheric evolution of the terrestrial planets. Objective 2 is to characterize the atmospheres and estimate the surface environment of exoplanets around the habitable zone by detecting their exospheric atmospheres. In cosmology and astronomy, Objective 3 will test whether the structures of present-day galaxies contain ubiquitous Lyα halos and reveal the physical origins of Lyα halos. Objective 4 elucidates the synthesis process of heavy elements from observations of ultraviolet radiation from hot gas immediately after neutron star mergers.
PS17-A006
| Invited
Recent Progress in Spaceborne Solar and Stellar Probing Technology at Extreme Ultraviolet Wavelength
Xianyong BAI1#+, Hui TIAN2, Yuanyong DENG3
1Chinese Academy of Sciences, 2Peking University, 3National Astronomical Observatories, Chinese Academay of Sciences
Extreme ultraviolet (EUV) wavelength provides an important tool to diagnose the solar and stellar activities and is one of the final windows to be opened up to astronomy. A joint team from the National Astronomical Observatories, Chinese Academy of Sciences, and the Peking University, starts to develop new spaceborne extreme ultraviolet probing technologies for solar and stellar observation since 2019. In the talk, we summarize recent progress. The Solar Upper Transition Region Imager Onboard the SATech-01 Satellite was successfully launched on July 27, 2022, aiming to test the on-orbit performance of the newly developed Sc/Si multi-layer reflecting mirror and the 2k×2k EUV CMOS imaging camera and to take full-disk solar images at 0.5 MK using the Ne VII 46.5 nm line with a filter width of ∼3 nm and a spatial resolution of 8 arcsecond. More than 700, 000 images have been taken so far. Recently, we developed a protype of the next generation full-disk integrated solar spectrograph and obtained the spectrum of He I 25.6 nm with a spectral resolution of 0.05 nm in the laboratory. Moreover, we are developing an EUV intensified CMOS detector, which has both integration mode for weak signal detection and photon counting mode for the observation of extremely weak stellar irradiance. A ground based EUV astronomical calibration facility, including the ability to test EUV cameras, solar and stellar EUV imagers and spectrographs, is also under construction.
PS17-A001
EUV Observations of the Coronal Activity on Exoplanet Host Stars
Hui TIAN#+
Peking University
In recent years, more and more researchers have realized that the space weather phenomenon (i.e., solar activity and its impact on the Earth space environment) should also exist in star-planet systems beyond the solar system. As the main sources of space weather, various types of magnetic activity in host stars’ coronae can produce strong electromagnetic and particle radiation that could damage biological tissues, change the chemical composition and lead to the erosion of the planetary atmospheres, thus affecting the origin and survival of life on exoplanets. However, our understanding of the stellar coronae is very limited, which greatly hampers our understanding of the impact of space weather on habitability. Thus, we suggest effectively probing the physical parameters of the coronae and monitoring various types of coronal activity of host stars as soon as possible. To achieve this, we need to build next-generation dedicated EUV (most importantly in the wavelength ranges of 170–285 Å and 90–140 Å) telescopes to perform long-term and continuous spectroscopic and photometric observations of nearby host stars (including but not limited to the host stars of some potentially habitable exoplanets). With these telescopes, we could systematically detect stellar coronal mass ejections and uncover coronal physical processes during stellar flares. By monitoring changes in the stellar EUV emission during exoplanet transits, we may also infer critical information about exoplanetary atmospheres, ionospheres and magnetospheres. Based on these observations, we can substantially improve our understanding of exoplanetary space weather and more accurately evaluate its role in forming a habitable world.
PS17-A005
Mapping Circumgalactic Mediums in the Nearby Universe
Li JI#+
Chinese Academy of Sciences
Mapping the circumgalactic medium (CGM) in emission is one of the important scientific goals for astronomers to either use the modern ground-based telescopes or the future space missions. CGMs are multi-phases, key to understand the galaxy ecosystem and its accretion and feedback. In this talk, I will briefly introduce a few scientific projects in our group for the efforts in the warm and hot diffuse emission in nearby universe with high spectral resolution data from UV and X-ray. In addition, I will introduce and summarize the developments of our proposed space missions for mapping CGMs in Lyman UV emission. In the end, I will highlight the prospects in CGM fields based on the existing and future facilities (such as SMILE, CSST, HUBS etc.) in China.
PS17-A002
Solar Wind Charge-exchange Contribution in Diffuse X-ray Background
Guiyun LIANG#+
Chinese Academy of Sciences
Since the1960s, Bowyer & Field (1969) found X-ray background radiation in different sky regions, and its flux is highly variable, and there are obvious excess in the soft X-ray. Energy spectrum from HEAO-1 satellite clearly revealed the soft X-ray excess, and a near-neighborhood low-temperature thermal radiation was proposed, e.g. the Local Hot Bubble (LHB) model. The ROSAT sky map in soft X-ray revealed a large number of irregular bands, also known as the Long Term Enhancement (LTE). However the LTE origin could not be explained by the LHB model. At the end of the last century, the model of solar wind charge-exchange was proposed to explain cometary X-ray observations, that completely changed the thinking of astrophysicists (Cravens 1997). Later, a perfect time match between ROSAT observations in specific sky regions and proton fluxes in the solar wind was found. Recently, Qu (2022) et al. reveal a strong correlation between the O VII flux in XMM-Newton observations and the periodic variations of the solar wind proton flux. During the same period, astrophysicists developed various models to simulate the contribution of solar wind charge exchange in the background X-ray radiation. Due to the low-resolution of the current observational energy spectrum, this contribution is calculated exclusively on the basis of theoretical simulations, which greatly limits the analysis of the spatial structure of the solar neighborhood. Because the clear distinction between the solar wind charge-exchange and thermal spectral features, it is the feasible to qualify the LHB and solar wind charge-exchange contributions by using the high-resolution spectroscopy. The Chinese Space Station Payload of diffuse X-ray explorer (DIXE) will provide the first observation constraint on qualifying the LHB and solar wind charge-exchange. In this talk, I also present our recent analysis of Martian X-rays by using an updated charge-exchange models (Liang et al. 2023).
Session Chair(s): Donghoon KIM, Korea University
PS18-A016
| Invited
Distribution of Mg and Si in Earth’s Mantle and Core Constrained by High-pressure Metal-silicate Partitioning and Elastic Properties
Zhicheng JING#+, Chang PU, Tao LIU
Southern University of Science and Technology
Comparison of Mg/Ca and Si/Ca ratios in the bulk silicate Earth with those of CI carbonaceous chondrites suggests the depletion of both Mg and Si in the Earth’s upper mantle compared to refractory lithophile elements. The missing Mg and Si can be explained by (1) the slight volatility of the two elements, (2) dissolution in the core during mantle-core differentiation, and (3) some hidden reservoirs enriched in these elements in the Earth’s mantle. High-pressure metal-silicate partitioning of Mg and Si and elastic properties of Mg- and Si-rich phases in the Earth’s deep mantle and core are required to evaluate the possibility of these scenarios. In this study, we performed new high pressure-temperature metal-silicate partitioning experiments of Mg and Si under conditions of 2–107 GPa and 2000–5300 K, using both a multi-anvil apparatus and laser-heated diamond anvil cells. Combining our data and those in the literature, we developed a self-consistent thermodynamic model that simultaneously incorporates all Mg-Si-O interactions in molten Fe-alloys, enabling the calculations of Mg, Si, and O distribution during the core formation and its subsequent cooling processes. Core accretion and exsolution models using our results suggest that a large quantity of Si and O can partition into the core during the core formation process and exsolve as Fe-rich SiO2 solids during its secular cooling. Significant dissolution of Mg in the core, however, requires high temperature equilibration during a giant impact. We also performed first-principles molecular dynamics simulations to calculate the density and elastic properties of the relevant Mg- and Si-rich phases in the Earth’s lower mantle and outer core to evaluate their seismic signatures. We will report our results on the Mg and Si distribution in the deep Earth employing both geochemical and geophysical constraints.
PS18-A018
| Invited
When Iron Meet Light Elements at Deep Earth's Conditions : A Computational Approach
Duck Young KIM#+
Center for High Pressure Science and Technology Advanced Research
Iron is the key element of human being’s industry and the main component of Earth. Thus, understanding of its interaction with environment at extremely high PT conditions is critical to model properly the structure and dynamics of the interior of Earth. In this talk, I will present series of our theoretical predictions on the nature of iron-rich compounds at lower mantle and inner core conditions. FeO2Hx and FeHx becomes superionic state at lower mantle and inner core conditions, respectively. Oxygen-inclusion in hcp-Fe enhances electron correlation comparable to bcc Fe, resulting in increase of resistivity. Last, I will present a possible mechanism of superionicity of iron-bearing compounds at high pressure, which may differentiate the condition of the interior of rocky planets.
PS18-A005
| Invited
High-pressure Ices Under Extreme Conditions
Bin CHEN#+, Meryem BERRADA
University of Hawaii at Manoa
Water (H2O) has a rich phase diagram and is present within various planetary environments in our Solar System. High-pressure ices, including Ice-VII, are present in large icy planets or moons and likely in Earth's interior as a result of progressive dehydration of water-bearing minerals in the subducting oceanic slabs. These high-pressure ice phases play a significant role in the dynamic evolution of the icy worlds at depth. To investigate the behaviors of high-pressure ices, we have developed an Externally-Heated Diamond Anvil Cell Experimentation (EH-DANCE) system, with the capability of fine-tuning high pressure-temperature conditions through an externally-heated diamond anvil cell (EHDAC), which is housed within a water-cooled enclosure providing a controlled environment (vacuum or inert gas atmosphere). Using the EH-DANCE system, we examined high-pressure ice phases to study their melting, structure, and thermoelastic properties under simultaneous high-pressure and high-temperature conditions. The melting of ice-VII was determined through the disappearance or reappearance of X-ray diffraction peaks from single or multigrain samples during multiple compression and decompression cycles at high temperatures. In particular, ice-VII was found to exhibit significantly higher melting temperatures at pressures exceeding 10 GPa compared to previous studies. Furthermore, X-ray diffraction measurements reveal the transition to a superionic body-centered cubic structure under extreme conditions when approaching the melting of the ice phase. Utilizing X-ray diffraction and Brillouin scattering, we also determined the thermal equation of state and single-crystal elasticity of ice-VII up to pressures of 80 GPa and temperatures of 1400 K. These findings suggest the existence of superionic ice within Earth's cold subducting slabs and the deep interiors of ice giants such as Uranus and Neptune. The presence of high-pressure ices, such as superionic ices, within subducting slabs challenges our current understanding of interactions between ice/water and rock in the silicate mantle under extreme conditions.
PS18-A003
IMPRESS: Integrated Mineral Physics Research and Education Software Suite
Meryem BERRADA1#+, Bin CHEN1, Siheng WANG2
1University of Hawaii at Manoa, 2University of Hawaii
The development of advanced software tools in mineral physics and extreme materials research has led to the creation of the "Integrated Mineral Physics Research and Education Software Suite" (IMPRESS). Within this comprehensive open-source suite, the recent focus has been on two pioneering tools: Raman Match and Brillouin View. Raman Match is specifically designed for the swift and accurate identification of Raman spectra, providing researchers with a powerful tool for mineral and material analysis. Conversely, Brillouin View serves a dual purpose, offering robust capabilities for the calibration of velocity data and the forward and reverse modeling of Cij parameters. The overarching goal of these innovative tools is to streamline data analysis while ensuring the reproducibility and reusability of results through collaborative code repositories. Raman Match facilitates the identification of mineral compositions via the RRUFF database, while Brillouin View ensures consistency in analytical methods, significantly elevating accuracy and efficiency in experimental practices across research groups. Accessibility and usability remain pivotal aspects, with a strong emphasis on providing comprehensive documentation, intuitive tutorials, and user support to cater to researchers at all proficiency levels. Continuous engagement with the scientific community through interactive workshops and seminars fosters collaboration, feedback, and ongoing enhancements, ensuring that the software remains at the forefront of cutting-edge research. Moreover, integration into national facilities such as the Advanced Photon Source at Argonne National Laboratory underscores the versatility and adaptability of these tools in swiftly analyzing data during time-sensitive experiments. The development of Raman Match and Brillouin View marks a significant milestone within the IMPRESS suite, offering refined analytical methods and paving the way for groundbreaking discoveries and expanded educational opportunities in mineral and rock physics and related disciplines.
Session Chair(s): Feng DING, Peking University
PS04-A001
| Invited
Modeling the Formation of Polar Cyclones of Giant Planets Driven by Moist Convection
Xianyu TAN#+
Shanghai Jiao Tong University
Polar cyclones of Jupiter and Saturn provide an intriguing laboratory to study giant-planet atmospheric dynamics in a rapidly rotating regime owning to abundant recent observations. Their stability, time evolution, and formation pathways in idealized model frameworks have been intensively studied, but simulations demonstrating the role of moist convection have not been carried out in more realistic model setups. This presentation will show general circulation modeling results in a box model concentrated in the polar regions in setups appropriate for giant planets. Investigations of cyclone formation driven by parameterized moist convection along with the radiative effects related to moisture and clouds will be presented, along with diagnoses of the energetics of the cyclonic systems.
PS04-A007
| Invited
Results from the Emirates Mars Mission: The Big Picture at the Red Planet
Siteng FAN1#+, Noora ALSAEED2, Hessa ALMATROUSHI3, Justin DEIGHAN4, Christopher EDWARDS5, Gregory HOLSCLAW4, Michael WOLFF6
1Southern University of Science and Technology, 2United Arab Emirates Space Agency, 3Mohammed Bin Rashid Space Centre, 4University of Colorado Boulder, 5Northern Arizona University, 6Space Science Institute
The Hope Probe of the Emirates Mars Mission (EMM) was launched in 2020, and began its science phase on May 23, 2021. Now in its extended mission phase, it continues to provide new insights into the dynamics of the Martian atmosphere on a planetary and sub-diurnal scale, with comprehensive geographic and local time coverage across multiple Martian years. From its novel high-altitude orbit with a period of 55 hours, the Hope Probe is using its infrared, visible, and ultraviolet remote sensing instruments to provide a unique set of measurements. The observations have been improving our understanding of the dynamics and physical processes in the lower and upper atmosphere of Mars, as well as their vertical coupling, especially the escape of light species to space. In this talk, I will summarize the discoveries and results from EMM, revealing atmospheric behavior and connections that challenge existing models and assumptions that we have of the Martian atmosphere, which leads to new global perspective of the Red Planet.
PS04-A009
Atmospheric Characteristics of Four Exoplanets Through High-resolution Near-infrared Transmission Spectra with IGRINS
Jinhee LEE1#+, Jae-Joon LEE1, Changwoo KYE2
1Korea Astronomy and Space Science Institute, 2Seoul National University
Over the past three decades, the discovery of exoplanets has surged, with confirmation of over 5,000 planets and a continuing upward trend. The majority of these exoplanets exhibit characteristics not found in our solar system, sparking debates about their origins. One avenue for investigating their origin involves observing their atmospheres. However, due to the challenges posed by their small size and faintness, atmospheric observation has proven exceptionally difficult, with only a limited number of planets having their atmospheres explored thus far. Transmission spectroscopy stands out as a popular and reliable method for delving into exoplanetary atmospheres. The use of high-resolution spectra is particularly advantageous, as it allows for clear detection of atmospheric molecules or atoms. Given the significance of C- and O-bearing molecules that are closely linked to planetary origins, the observation of CO and H2O in the near-infrared (NIR) range becomes crucial. IGRINS, developed by KASI and The University of Texas, stands out for its high throughput and spectral resolution (R~45,000). In this study, we observed two super Earths (55 Cancri e and Kepler-21 b) and two hot Jupiters (HD 189733 b and tau Boo A b) using IGRINS at the McDonald 2.7-m telescope. Despite being unable to directly detect specific molecules in our data, we successfully established upper limits for various molecules. This limits provide valuable insights into the atmospheric properties of the studied exoplanets and offer a basis for formulating hypotheses about their origins.
PS04-A002
Effects of Orbital Parameters on Surface Ice Sheet Distribution of Exoplanets Around M Dwarfs
Yueyun OUYANG#+, Feng DING
Peking University
The environment of terrestrial planets around M dwarfs depends highly on the orbital parameters, including the cold-trap region which directly impacts the global energy budget and long-term surface water evolution. Here we use an idealized land-atmosphere coupling model to calculate the maximum ice rate and distribution of habitable-zone terrestrial planet under different orbital parameters, assuming the planets to be arid, airless or with thin \ce{N2} atmosphere. We investigate seven orbital parameters and find that the most significant factors in deciding the cold-trap region are orbital ratio, obliquity and eccentricity. Stellar flux also plays an important role, but only when the planet has a thin \ce{N2} atmosphere. This result illustrates the possible surface ice sheet distribution on arid terrestrial planets and can aid predicting the climate of these exoplanets.
PS04-A006
Simulating Dust Processes Using a Variable-mesh High-resolution Martian Atmospheric Numerical Model (iAMAS-Mars)
Yongxuan ZHAO#+
University of Science and Technology of China
Mars dust has always been a key factor affecting Mars exploration and a focus of Mars science research, and simulation experiments using Mars numerical models are undoubtedly one of the most effective means. However, the resolution of traditional numerical models is coarse, and the boundaries of encrypted simulations are subject to abrupt changes and huge consumption of computational resources. We developed a irregular mesh numerical model of Mars (iAMAS-Mars), which can perform global simulations with smooth regional encrypted simulations, realize variable mesh resolution simulations, and allow multiscale weather phenomena to act in the encrypted region together. In addition, we have improved the parameterization scheme for dust, including multiple particle size distributions, dry deposition processes, and so on. Therefore, we have realized the variable grid resolution simulation of dust, and the experiment mainly focuses on the lifting process of dust, and the feedback effect of dust on the atmosphere. And We will show some results to reveal the effect of regional encryption on modeling Martian dust processes.
Session Chair(s): Takeshi IMAMURA, The University of Tokyo
PS12-A002
Venus Dayside Observation Campaign in 2023 with BepiColombo, Akatsuki, and Ground-based Telescopes
Yeon Joo LEE1#+, Antonio GARCÍA MUÑOZ2, Eric QUEMERAIS3, Atsushi YAMAZAKI4, Masateru ISHIGURO5, Stefano MOTTOLA6, Yeon-Ho CHOI7, Emmanuel MARCQ8, Thomas GRANZER 9, Stephan HELLMICH 10, Jooyeon GEEM5, Yoonsoo BACH7, Seiko TAKAGI11, Hiroaki SAITO 11, Hiroyuki NAITO12, Sunho JIN5, Hangbin JO5, Bumhoo LIM5, Léonard GEORGES THÉODORE LEBRUN 10, Minji JUNG13, Ekaterina CHORNAYA14, Jose SILVA1, Evgenij ZUBKO 1, Maxim ZHELTOBRYUKHOV14, Anton KOCHERGIN15, Joh Na YOON13, Hyun-il SUNG7, Hee-Jae LEE7, Myung-Jin KIM7, Shigeto WATANABE11, Manabu YAMADA16, Takehiko SATOH4
1Institute for Basic Science, 2French Alternative Energies and Atomic Energy Commission, 3Laboratoire Atmosphères, Milieux, Observations Spatiales, 4Japan Aerospace Exploration Agency, 5Seoul National University, 6German Aerospace Center, 7Korea Astronomy and Space Science Institute, 8National Center for Scientific Research (CNRS)/ Institut Pierre Simon Laplace (IPSL)/ Université de Versailles Saint-Quentin-en-Yvelines (UVSQ) / University Pierre et Marie Curie (UPMC), 9Leibniz-Institute for Astrophysics Potsdam, 10École Polytechnique Fédérale de Lausanne, 11Hokkaido University, 12Nayoro Observatory, 13Chungbuk National University, 14Russian Academy of Sciences, 15Far Eastern Federal University, 16Chiba Institute of Technology
Venus’s sulfuric acid clouds cover the globe entirely. These clouds reflect most incoming solar irradiance, resulting in a Bond albedo of ~0.8. The presence of an unknown absorber(s) and atmospheric gases that exist above and within the upper cloud layer reduces the reflectivity of Venus in the ultraviolet (UV) to visible wavelength range. Previous studies analyzed such reflected light to characterize the chemical composition, cloud structures, aerosols microphysical properties, and their variabilities in the mesosphere. In 2020, we conducted a 1st observation campaign with telescopes on the ground and in space. To further understand (1) the spectral properties of the unknown absorber(s) that likely exist in the clouds and (2) the SO2 gas abundance, we conducted the 2nd Venus dayside observation campaign in Sep-Oct 2023 together with ESA-JAXA’s BepiColombo UV spectrometer (PHEBUS), JAXA’s Akatsuki UV imager (UVI), and a total of eight ground-based observatories in Europe and East Asia. While space-based observations covered UV wavelength with the spectrometer and the imager, ground-based telescopes covered from the near-UV to near-infrared spectral range using spectrometers, band-pass filters, and polarizers. Our team acquired a rich data set providing a global view of Venus’s dayside over a broad wavelength range for analysis of spectra, or intensity and degree of polarization at specific filters, which a single instrument cannot achieve. Polarization measurement is an additional observed quantity that was missing in the 1st campaign.
PS12-A003
Temperature Retrievals from Akatsuki LIR Measurements and Comparisons with Radio Science: Implications for Venus’ Cloud Structure
Armin KLEINBOEHL1#+, Shigeru SUZUKI1, Makoto TAGUCHI2, Norihiko SUGIMOTO3, Takao SATO4, Takehiko SATOH5, Takeshi IMAMURA6
1California Institute of Technology, 2Rikkyo University, 3Keio University - Hiyoshi Campus: Keio Gijuku Daigaku - Hiyoshi Campus, 4Hokkaido Information University, 5Japan Aerospace Exploration Agency, 6The University of Tokyo
Thermal infrared measurements with the Longwave Infrared Camera (LIR) on Akatsuki have revolutionized our understanding of Venus with the discovery of stationary waves and the characterization of thermal tides in Venus’ middle atmosphere. A limitation of these measurements is that data only exist as brightness temperatures measured by the camera and any information pertaining to the altitude range to which the measurements are sensitive is not available to date. This limits our understanding of Venus’ weather and climate that can be gained from these thermal infrared measurements. The Venus sulfuric acid cloud layer is the predominant source of absorption in the 8-12 μm wavelength window covered by LIR. Hence, the derivation of atmospheric temperatures requires an understanding of the cloud cover and its vertical distribution. We use a cloud top height climatology based on measurements of the CO2 column density above the clouds by the Akatsuki IR2 camera at a wavelength of 2.02 μm as input to retrieve atmospheric temperatures from thermal infrared images and characterize their vertical sensitivity. We present retrievals of atmospheric temperatures from Venus images by LIR, together with their weighting functions that give the vertical sensitivity of the measurement. The retrieval algorithm is based on the one for the Mars Climate Sounder, which has been adapted for the Venus atmosphere. We provide comprehensive comparisons with temperatures retrieved from nearly-coincident measurements by the Akatsuki Radio Science investigation and evaluate the results in terms of temperature structure as well as structure of the cloud tops as seen at thermal infrared wavelengths.
PS12-A014
Venusian Ionosphere During Deep Solar Minima (2016-2022): Akatsuki Radio Science Observations
Keshav R. TRIPATHI1#+, Takeshi IMAMURA1, Raj CHOUDHARY2, Ambili K.M.2
1The University of Tokyo, 2Vikram Sarabhai Space Centre
During the deep solar minimum of solar cycle 24, the distinct characteristics of various layers within the Venusian ionosphere were investigated through a radio science experiment conducted aboard the Akatsuki spacecraft. Tracking of radio signals from the spacecraft took place at multiple locations: the Indian deep space network in Bangalore, the Usuda Deep Space Center in Japan, and the DLR Ground station in Weilheim, Germany [1]. The unique orbital geometry of the spacecraft presented rare opportunities for exploring the equatorial region of the Venusian ionosphere and atmosphere at low solar zenith angles (SZAs). Throughout the observation period spanning from 2016 to 2022, the peak of electron density consistently occurs at an altitude of approximately 141 km, maintaining stability for solar zenith angles ≤ 90°. The associated plasma density recorded during this period ranks among the lowest reported in existing literature. Furthermore, we emphasize that the Venusian ionosphere differs from the Chapman variation observed on Earth. Examining secondary ionospheric features, the V1 layer (~125 km altitudes) aligns well with the previous measurements. Akatsuki observations identified all three types of V1 layers and sporadic occurrences of the V0 layer (~110 km altitudes) in approximately 15% of cases. The presence of the V0 layer was observed independently of SZA and geographical constraints [2, 3]. Despite regular observations, nighttime occurrences of the ionosphere were limited. The significant findings from Akatsuki's observations of the Venusian ionosphere will be presented during the conference. References: [1] Tripathi, K. R., Choudhary, R. K., Ambili, K. M., & Imamura, T. (2023). JGR-Planets, 128, e2023JE007768. https://doi.org/10.1029/2023JE007768. [2] Ambili, K. M., Tripathi, K. R., Choudhary, R. K., & Imamura, T. (2022). MNRS, 516(4), 5555–5562. https://doi.org/10.1093/mnras/stac2624. [3] Tripathi, K. R., Choudhary, R. K., Ambili, K. M., Imamura, T., & Ando, H. (2022). Geophysical Research Letters, 49(7), e2022GL097824. https://doi.org/10.1029/2022gl097824.
PS12-A011
Vertical Structure of the Venusian Thermal Tide in Low-latitudes Clarified by the Akatsuki Radio Occultation Measurements
Hiroki ANDO1#+, Katsuyuki NOGUCHI2, Takeshi IMAMURA3, Masahiro TAKAGI1, Norihiko SUGIMOTO4, Yoshihisa MATSUDA5
1Kyoto Sangyo University, 2Nara Women's University, 3The University of Tokyo, 4Keio University, 5Tokyo Gakugei University
Downward propagation of the thermal tide has been detected by the Akatsuki radio occultation measurements for the first time. The angular momentum transport due to the thermal tide which propagates upward and downward directions from the cloud layer is one of the most likely mechanisms to generate and maintain the Venusian atmospheric superrotation. Though some optical measurements have shown the horizontal structure of the thermal tide at the cloud top level, it is difficult to investigate its vertical structure by these measurements. In this study, the vertical structure of the thermal tide in the Venusian low-latitudes (0˚-30˚ latitudes) were investigated by the Akatsuki radio occultation measurements. The result shows that the phase of the diurnal component little varies in the vertical direction, while that of the semidiurnal one tilts toward earlier local times above and below 60-65 km altitudes. This indicates that the semidiurnal one propagates upward and downward from the levels, and these structures are well consistent with theoretical and numerical studies. We also estimated angular momentum flux and acceleration rates of the superrotation induced by the semidiurnal tide in the equatorial region above 60 km altitude and found that the semidiurnal tide makes the atmosphere accelerated around the cloud top level (~65 km) and decelerated above the level. This is also well consistent with the theoretical studies, indicating that these studies have been validated observationally for the first time.
PS12-A015
Aerosol Properties in the ”Enormous Cloud Cover” of Venus as Inferred from Photometrically Improved IR2 Night-side Data
Takehiko SATOH1#+, Takao SATO2, Takeshi IMAMURA3, George HASHIMOTO4, Takeshi HORINOUCHI5
1Japan Aerospace Exploration Agency, 2Hokkaido Information University, 3The University of Tokyo, 4Okayama University, 5Hokkaido University
A very abrupt change of cloud opacity seen in the night-side disk of Venus, which we call Enormous Cloud Cover or ECC for short, was imaged by Akatsuki/IR2 and Venus Express/VIRTIS-M (Peralta et al., 2020). Similar phenomena were repeatedly recorded also by the ground-based instruments since the beginning of the night-side observations (Allen and Crawford, 1984), suggesting this phenomenon is not uncommon in the Venus atmosphere and may include essential dynamical implication. We perform radiative transfer (RT) analyses of ECC with comparison to Background Cloud (BC) to understand how aerosol properties change from BC to ECC. To improve the photometric accuracy, needed especially for the extremely-low radiance region (ECC), an alternative method to clean the IR2 1.735- and 2.26-um data has been developed (named RSS202). The new method uses an overexposed (12.97 s) 2.02-um image, recorded between the 2.26- and 2.32-um images, to cancel the contamination from the dayside. Acquisition of the 2.02-um image was introduced when the observing program suite was updated in June 2016 after which ECC was observed with IR2 in five occasions. The RSS202-processed data are validated against those processed with the original RSS method (Satoh et al., 2021). The correlation plot of the RSS radiance and the RSS202 radiance appears linear, indicating good consistency between two methods and the robustness of results with the data. We will present the results of RT analyses and discuss the variation of BC-to-ECC changes for different occasions. The variability will give us clues to understand the mechanism of this prominent phenomena in the Venus clouds.
PS12-A016
Role of a Kelvin Wave in the Formation of Venusian Clouds
Takeshi IMAMURA#+
The University of Tokyo
Venus is surrounded by sulfuric acid clouds that are essential to the planet's climate system. The upper part of the cloud is thought to be of photochemical origin, while the lower part of the cloud is highly variable and will be more affected by atmospheric dynamics causing condensation and evaporation of sulfuric acid. The specific dynamical processes responsible for the variability are poorly understood. Observations using near-infrared window wavelengths have revealed large opacity variations, which mostly occur in the lower part of the cloud layer. A significant feature is the planetary-scale dark cloud propagating with a period of 4.9-5.5 days, discovered through ground-based observations (Crisp et al. 1991). The IR2 camera aboard the Venus orbiter Akatsuki observed this phenomenon in more detail and found that the planetary-scale cloud discontinuity that spans in the north-south direction characterizes the propagating structure (Satoh et al. 2017; Peralta et al. 2020). The relatively large amplitude near the equator and the zonal propagation faster than the background atmosphere indicate that the cloud opacity variation is mainly induced by a Kelvin wave. A Venus GCM reproduced a 5.5-day periodicity in the thickness of the lower cloud driven by a Kelvin wave with a zonal wavenumber of unity (Ando et al. 2021). However, the observed sharp discontinuity was not reproduced in previous models. The present study proposes mechanisms for the cloud discontinuity from the viewpoint of atmospheric dynamics and cloud microphysics. A simplified dynamical model and a microphysical model are used to reproduce the phenomenon. This study aims to understand the role of the Kelvin wave in the formation of the cloud and the conditions necessary for the appearance of the observed sharp discontinuity.
PS12-A012
Constraining Size of Aerosol Particles Populating Uppermost Atmosphere of Venus by Means of the Glory Phenomenon
Evgenij ZUBKO#+, Yeon Joo LEE
Institute for Basic Science
Venus reveals phenomenon of the glory near opposition. This phenomenon manifests itself as surge in the phase function at small phase angles, less than 10 degree (see, e.g., Lee et al. 2017: Astron. J., 154, 44). It places important constraints on microphysics of the aerosol particles, in particular, their refractive index m and size distribution. We investigate interrelation between the shape of glory surge and parameters characterizing differential power-law size distribution of aerosol particles: the power index n, the bottom limit rmin, and the upper limit rmax. We model shape of an aerosol particle with a perfect sphere and compute its light-scattering response using our own implementation of the Mie theory. We assume predominantly sulfuric-acid composition of the aerosol particles, whose complex refractive index is m = 1.47 + 0i at wavelength 0.365 μm. We study light scattering at this wavelength over broad range of particle radius, r = 0.01 – 7.5 μm. The resulting light-scattering responses are averaged then with a power-law size distribution r–n and the index n spanning range from 1 to 4. Our modeling reveals that while the amplitude of glory surge appears to be dependent on all three parameters characterizing the power-law size distribution, positions of the local minimum and local maximum on the phase function is solely affected by the upper limit rmax. It is worth noting that the local minimum and maximum positions are known to be hardly affected by multiple-particle scattering in the upper haze layer (70–90 km) and, hence, it makes it possible immediate interpretation of the glory observations in terms of the largest size of aerosol particles populating the atmosphere of Venus.
PS12-A009
Characterization of the Unknown Absorbers in the Venusian Clouds
Ashimananda MODAK#+, Yeon Joo LEE
Institute for Basic Science
Venus’ clouds hold a several-decade-long mystery, unknown absorbers. These absorb a significant amount of solar energy, affecting energy budget and dynamics, but their observational properties are yet unclear. In this study, we investigate the absorption characteristics of the unknown absorbers using the Venus reflection spectra obtained using the Hubble space telescope’s STIS (Space Telescope Imaging Spectrograph) instrument. The observations cover a spectral range from 200 – 300 and 350 – 550 nm corresponding to two different grating systems G230LB and G430L respectively. In the spectral range of grating G230LB, the absorption in the reflected spectra is dominated by the SO2 and SO bands. Whilst in the second spectral range, primary absorber of the solar insolation is a chemical still known to the community as the unknown absorbers. Previous studies suggest maximum absorptions due to the unknown absorber is at 340 nm with a FWHM of 140 nm. Along the wavelengths, the absorption of SO, SO2, O3, and the unknown absorbers are entangled with each other to various degrees depending on their line strengths of absorptions. In order to separate the absorptions of SO and SO2 from that of the unknown absorber we analyze HST/STIS observations, using both the aforementioned gratings were made on January 27th, 2011. To construct the observed spectra, we use a state-of-the-art line-by-line radiative transfer model, KOPRA (Karlsruhe OPtimized Radiative transfer Algorithm) in conjunction with a retrieval control program which solves inverse problems iteratively based on multiparameter non-linear Levenberg-Marquardt method.
PS12-A013
Development of Planetary Lightning Detector (PLD) and Model Comparing with JEM-GLIMS Data for Venusian Lightning
Tatsuharu ONO1#+, Yukihiro TAKAHASHI1, Mitsuteru SATO1, Seiko TAKAGI1, Masataka IMAI2
1Hokkaido University, 2The University of Tokyo
Lightning is a phenomenon formed by electric discharge through the atmosphere that occurs not only on Earth. Some previous observations detected the possible signal originating from Venusian lightning. LAC onboard AKATSUKI recorded a potential signal on March 1, 2020 (Takahashi et al., 2020). If the lightning discharge generated its signal, the occurrence rate equals the estimated by the ground-based telescope observation (Hansell et al., 1995). Lightning could help reveal the Venusian atmospheric dynamics. Moist convection is a possible mechanism for generating lightning discharge in dense clouds. Lightning activity has correlated with the atmospheric activity. However, several issues, for example, its existence, mechanism, and distribution, prevent us from understanding Venusian lightning due to the monitoring time deficit. To enable us to achieve high-frequency monitoring observations, we have developed the Planetary Lightning Detector (PLD) for the 1.6-m Pirka telescope of Hokkaido University. PLD can distinguish between the lightning and the variation of the other light sources using two-band simultaneous photon counting. The first photomultiplier tube observes the wavelength of Venusian lightning(777 nm, FWHM = 1nm). The second photomultiplier tube simultaneously observes the background variation with the broadband filter, 700 nm (FWHM = 10 nm). If the PMT's signal of 777 nm has a considerable count value above the trigger level estimated by the noise amplitude, unlike the second PMT, the candidate waveform has been detected. From the data of observing Venus since 2021, we triggered several possible signals. We cannot rule out the possibility that all recorded light curves originate from noise or Cosmic rays. It might be disputable to conclude that we have detected lightning. We compare it with the model and Earth lightning light curve observed by JEM-GLIMS to test if the observed lightning is possible.
Session Chair(s): Emily LAW, NASA Jet Propulsion Laboratory
PS16-A016
| Invited
Challenges in Chandrayaan-3 Mission Operations of Lander and Rover – Post Landing
Srikanth MOTAMARRI#+
Indian Space Research Organisation
In any lunar landing mission, there comes an opportunity to demonstrate the safe and soft landing of lander on the lunar surface. The Lander module in turn carries the Rover which will touchdown the lunar surface for performing mobility and scientific operations using scientific payloads onboard. The prime mission objective of any Rover is to maximize the Rover movement over the lunar surface and operating the Rover payloads at every point and ensuring safe movement of the Rover. Chandrayaan-3. the prestigious lunar mission of India, wherein the Pragyaan Rover was launched onboard Vikram Lander which safely landed on the Lunar south pole region on 23rd August 2023 at 12:34 UT. After landing, the lander and rover initiated the targeted activities as per plan. The lander mission operations involve deploying the rover, operation of lander payloads, record and playback operations of lander and rover data. The rover mission operations include the pre-commissioning of the rover in full healthy condition, payload operations, rover mobility operations, imager operations to capture the lander and the terrain traversed by rover, data download from rover to lander, thermal, power management, final orientations for power generation of each mobility, and rover parked at an appropriate orientation conducive for power generation for next wake up etc. The first-time hand’s on experience of operating the rover from ground could be achieved only by appropriate mission planning and support from all the sub-system teams. All the multi-disciplinary activities were carried out semi-autonomously from ground flawlessly. This paper provides the detailed mission operations carried out at lander and rover end post successful landing.
PS16-A013
| Invited
Post-landing Operation of the Multi-band Camera on Board Slim
Kazuto SAIKI1#+, Makiko OHTAKE2, Yusuke NAKAUCHI3, Masaki NISHINO4, Hiroshi NAGAOKA3, Yoshiaki ISHIHARA4, Hiroyuki SATO4, Chikatoshi HONDA5, Risa MIYAZAKI4, Iori KAJITANI4, Ryusuke NISHITANI4, Takashi MIKOUCHI6, Shin-Ichiro SAKAI4, Shujiro SAWAI4, Seisuke FUKUDA4, Kenichi KUSHIKI4
1Ritsumekan University, 2Okayama University, 3Ritsumeikan University, 4Japan Aerospace Exploration Agency, 5The University of Aizu, 6The University of Tokyo
Smart Lander for Investigating Moon (SLIM) is a lunar lander that aims to be Japan's first successful soft landing on the moon. The scheduled landing date is January 19th. The Multi-Band Camera is the only scientific observation instrument on board SLIM, and we expect to be able to report on its operations at the AOGS venue. The main purpose of the SLIM project is to demonstrate various techniques for pinpoint landing within a hundred meters in radius on the moon. As a landing site, one of the small fresh craters just outside of the Theophilus crater is selected. There is olivine-rich lithology, which is probably mantle (or the lower part of the crustal) origin excavated by the Nectaris basin forming impact as suggested by the global distribution of the olivine-rich sites, well before the formation of the Theophlius. The purpose of MBC is to identify this unknown lithology and estimate its origin. MBC has a spatial resolution (1.3 mm/pixel at 10 m), which distinguishes plutonic rock texture and incorporates 10 bandpass filters for identifying mineral species. After a landing, a scanning operation will be carried out first. In that operation, images are captured by moving a mirror to scan the landscape, reconstructing approximately a 60° horizontal field of view from 333 captured images. Imaging is performed in a single band with 16x16 binning, resulting in a file size of approximately 850 Kbytes for the downlinked images. The next stage is 10-band observing operation. We use the scanned images to select rocks to observe, and observe them with 10 bands. To estimate the Mg# of olivine, we intend to use the wavelength of the absorption peak of olivine near 1 micron searched from the continuous spectrum data generated from discrete data of 10 bands using spline fitting.
PS16-A010
Chandrayaan-3: Accomplishments and Preliminary Science Results
Megala SENTHILKUMAR#+, Tirtha Pratim DAS
Indian Space Research Organisation Headquarters
Chandrayaan-3 mission was launched on 14th July 2023 by LVM3 M4 from Sriharikota. The integrated module carried out five Earth bound maneuvers, Trans lunar injection and then inserted in the lunar orbit on 5th August. After several lunar burns, the lander module was separated from the propulsion module on 17th August. Following two de-boost maneuvers, the Lander along with the 26kg Rover executed a flawless landing with an Autonomous Landing Sequencer, marking a significant milestone on 23rd August 2023. This accomplishment has placed India, the fourth country to master the soft-landing on the Moon and first country to land in the southern high latitudes on the Moon.Post landing, the Rover moved around the landing site and traversed a total of ~100m distance. Payloads on the Lander and Rover were deployed for in-situ investigations. The mission objectives were successfully accomplished and the payloads collected data pertaining to seismicity, thermo-physical properties, plasma environment and elemental composition of the landing region. The data analysis is in progress. The preliminary science findings from the payloads are as follows:o First-ever measurements of near-surface lunar plasma environment, indicating that the plasma near the surface is relatively sparse.
o First-ever probing of few cm of lunar regolith is done which shows strong vertical gradient of temperature.
o Seismometer recorded the movements of Rover, other payloads and few potential natural events.
o Detection of various elements major elements and several minor elements around the landing site by spectrometers on the Rover.The scientific data would be made available to public, in due course of time. Significant findings from Chandrayaan-3 payloads and their value addition to lunar scientific knowledge will be discussed in this paper.
PS16-A004
Project Status on Lunar Polar Exploration (LUPEX)
Hiroyasu MIZUNO1#+, Makiko OHTAKE2, Takeshi HOSHINO1, Dai ASOH1
1Japan Aerospace Exploration Agency, 2Okayama University
Lunar Polar Exploration (LUPEX) mission is a joint exploration for Japan Aerospace Exploration Agency (JAXA) and Indian Space Research Organisation (ISRO) in the south polar region on the Moon for exploring water resources and demonstrating mobility by a rover. LUPEX mainly aims to obtain data for the quantity and quality of lunar water to clarify whether it can be used for future sustainable activities and for understanding the principle of the water distribution and concentration to estimate the quantity and quality of water across the Moon. LUPEX spacecraft consists of a rover system developed by JAXA and a lander system developed by ISRO. The integrated spacecraft will be launched by the H3 rocket at the Tanegashima Space Center in Japan. Because of in-situ direct measurement of water is a key to achieve our mission objectives, seven kinds of instrument are on the rover; 1) Resource Investigation Water Analyzer (REIWA), 2) Advanced Lunar Imaging Spectrometer (ALIS), 3) Ground Penetrating Rader (GPR), 4) Mid-infrared Imaging Spectrometer (MIR), 5) Neutron Spectrometer (NS), 6) Exospheric mass Spectrometer for LUPEX (EMS-L), and 7) Permittivity and Thermophysical Investigation for Moon’s Aquatic Scout (PRATHIMA). The rover also has a drilling system to excavate the regolith as well as a sampling system to pick the regolith sample from a designated depth up to 1.5 meters. LUPEX rover has been developed under the basic design phase and keep testing in the subsystem level by using some bread board models. Development of REIWA and ALIS are under the detailed design phase, and we are manufacturing their engineering models. In this study, we will present the project status of LUPEX, especially on the basic design of the rover system and on development of REIWA and ALIS in the detailed design phase.
PS16-A024
Low Energy Micro-LIBS (LE-LIBS) Experiment Aboard the Chandrayaan-3 Pragyaan Rover
V. L. N. Sridhar RAJA#+, Adwaita GOSWAMI, Lohar K.A., Bijoy RAHA, Girish GOUDA, Pramod K.B., Umesh S.B., Karanth S.P., Sriram K. V.
Indian Space Research Organisation
Low-energy Laser Induced Breakdown Spectroscope (LE-LIBS) is one of the six Indian scientific instruments flown on board the Chandrayaan-3 mission, the 3rd ISRO (Indian Space Research Organization) mission to the Moon. The LE-LIBS, which is developed based on the LIBS technique employs 1.53-micron laser radiation as the excitation source and investigates the elemental composition of the lunar surface in-situ from the close-range distance of 200 mm ± 8 mm. Instrument’s optical resolution is < 1nm and the spectral acquisition range is from 220 nm to 800 nm. The payload housed inside the Warm Electronics Box (WEB) of the rover fires laser shots towards the lunar regolith/soil with a power density of ~ 6 GW/cm^2 per pulse. The LE-LIBS is operated for the first time on August 25, 2023, at 10:42:21 UTC for a duration of 35 seconds on a southeast site, while the last operation was performed on September 2, 2023, on a northeast site. During its nine-days of operation, nearly 700+ laser shots have interacted with the regolith in the lunar southern higher latitude region, providing valuable scientific data hitherto not available to the scientific community. The on-board data records are subjected to the data pre-processing sequence flow followed by the global-curve fitting, peak centroid estimation and elemental identification using the ground-generated GUI tools developed in the Python platform. Initial analysis of the first-ever recorded LIBS emission spectrum of the lunar regolith at a site, a few couple of meters away from the landing point, has indicated the presence of elements viz., O, Al, Si, Ca, Fe, Ti, Mn, and Cr. Later investigations are found to be even more promising regarding the detection of a few trace elements. This paper presents instrument configuration, onboard operational sequence and data products.
PS16-A001
Detailed Analysis of the Landing Site for ESA's Prospect Instrument
Sarah BOAZMAN1#+, David HEATHER1, Marius SCHWINNING1, Michelangelo FORMISANO2, Tristam WARREN3, Philipp REISS4, Christian GSCHEIDLE4, Csilla ORGEL1, Nicole SCHMITZ5, Alessandro FRIGERI2, Cristina DESANCTIS2, Matt HUTTON1, Sebastien BESSE1
1European Space Agency, 2Institute of Astrophysics and Planetary Science, 3University of Oxford, 4Technical University of Munich, 5German Aerospace Centre
ESA’s PROSPECT instrument is on board the NASA Commercial Lunar Payload Service (CLPS) 22 mission which is targeting the south polar region of the Moon. CLPS 22 is due to land within a 100 m landing ellipse centred at -84.496°S, 31.588°E, in the south polar region. PROSPECT is designed to sample volatiles from within the sub-surface to a depth of 1 m, therefore the landing ellipse should be located where thermal conditions support water ice to be stable if present. Detailed analysis of the landing ellipse was carried out to further understand the thermal conditions as well as the surface morphology, feature distribution and potential hazards such as slopes. Remote sensing was used with multiple datasets including NAC images, DIVINER data, a shape from shading digital elevation model, high resolution illumination and Earth visibility models and high-resolution thermal models to analyse the landing site. The high-resolution DEM showed slopes within the landing site to be maximum 6 ° and there are little changes in the elevation across the landing site, only small-scale topographic changes from craters. 83 craters were mapped in total within the landing ellipse and the craters varied in size, median area 15.5 m2, with smallest craters 2 m2 and the largest crater 2200 m2. The morphology of the landing ellipse and surrounding area was analysed, and 4 units were identified based on texture and crater distribution. The four units identified were smooth texture, undulating texture, rough but less textured and rough texture. Illumination and Earth visibility analysis showed mission windows on average 8-10 days for the period October 2026-October 2027, and longer mission windows when only illumination was considered of up to 13 days. The analysis will allow areas to be identified within the landing ellipse, which should be targeted or avoided.
PS16-A009
Magnetic Gradiometry and Noise Characterization Efforts for the Lunar Vertex Mission
Dany WALLER1#+, Sarah VINES2, Brian ANDERSON2, David BLEWETT2, Jasper HALEKAS3
1Johns Hopkins University, 2Johns Hopkins University Applied Physics Laboratory, 3The University of Iowa
The first Payloads and Research Investigations on the Surface of the Moon (PRISM1) delivery targets the Reiner Gamma (RG) swirl and magnetic anomaly. To characterize the magnetic anomaly source and study the potential connection of the associated “mini-magnetosphere” to albedo variations within the swirl, the Lunar Vertex (LVx) investigation will carry an array of vector magnetometers on the lander (VML) and an array of vector magnetometers on the rover (VMR). Both instruments were assembled and calibrated at the Johns Hopkins University Applied Physics Laboratory (APL). Measurements during descent recorded by VML and during surface operations by both VML and VMR will characterize the spatial and temporal variation of magnetic fields across the RG swirl. Using a novel approach in mitigating magnetic field contamination from the lander and rover, VML and VMR will place new bounds on the orientation, strength, and depth of the RG magnetic anomaly. Measuring local variations in the surface field is key for understanding the relationship between the magnetic anomaly and the optical swirl pattern. In preparation for the upcoming LVx mission, we use synthetic data and laboratory data incorporating magnetic sources to determine the accuracy and precision of the VML and VMR gradiometry technique for noise reduction. The algorithm developed using the novel LVx magnetic gradiometry technique is referred to as the tetrahedral correction algorithm and been validated for dipole-like sources using both synthetic data and experimental data. The tetrahedral correction algorithm is capable of identifying and removing noise from overlapping dipole sources with <10% residual errors. New work explores algorithm performance for noise removal of complex noise sources and initial results indicate that an iterative approach to removing overlapping noise sources is effective, with ongoing efforts to quantify algorithm performance using laboratory data.
Session Chair(s): Yoonyoung KIM, University of California, Los Angeles
PS05-A001
| Invited
Formation and Evolution of Cb-type Asteroid Ryugu Inferred from Return Sample Analysis
Tomoki NAKAMURA#+, Megumi MATSUMOTO
Tohoku University
We performed chemical and mineralogical analyses and physical property measurements of Ryugu samples. Numerical simulations incorporating these analysis results were also carried out in order to understand the formation, evolution, and impact destruction processes of parent asteroid Ryugu (Nakamura et al. 2022, Science). The interior of Ryugu used to contain a large amount of water, which was alkaline carbonate water containing salts and organic matter. The conditions were similar to those of the Earth's oceans. In this water, chemical reactions caused by water rock reactions progressed, and original Ryugu building brocks gradually transformed into hydrated and carbonate minerals. The parent asteroid Ryugu was formed in an extremely cold region (below -200°C) far from the sun about 2 million years after the formation of the solar system. Several million years later, the interior of the body was heated and filled with water, and aqueous alteration progressed. After that, the object cooled down, experienced a major impact, and was destroyed. The present Ryugu is an aggregate of some of the fragments produced by the destruction. In the presentation, I will introduce the evidence derived from return sample analysis that is required to develop the formation and alteration history of the parent asteroid Ryugu.
PS05-A004
| Invited
Updates on the Analysis of Bennu Samples Delivered to Earth by OSIRIS-REx
Shogo TACHIBANA1#+, Harold CONNOLLY, JR.2, Dante LAURETTA3, The OSIRIS-REx SAMPLE ANALYSIS TEAM3
1The University of Tokyo, 2Rowan University, 3The University of Arizona
NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, Security, and Regolith–Explorer) spacecraft explored B-type near-Earth asteroid (101955) Bennu from December 2018 to May 2021. The spacecraft data indicated that Bennu’s surface material contains hydrous silicates, carbonates, magnetite, and organic matter, which suggests that Bennu’s parent body once experienced aqueous alteration in its early stages of evolution. In October 2020, the spacecraft collected a sample of surface material inside the 20-m-diameter Hokioi crater. This sample was delivered to Earth via the Sample Return Capsule, landing in the Utah desert in the western United States on September 24, 2023. Through the curation work at NASA Johnson Space Center, more than 70 grams of Bennu material has already been extracted and containerized, which exceeds the mission goal (60 grams). The OSIRIS-REx Sample Analysis Team has started detailed analysis of the samples. To date, our results show that the Bennu samples are composed of phyllosilicates, magnetite, carbonates, and organic matter, as predicted by the spectroscopic observations of the asteroid’s surface, as well as iron sulfides. Results from the sample analysis will be presented at the meeting.
PS05-A017
| Invited
Disintegration of Comets
David JEWITT#+
University of California, Los Angeles
Many comets disintegrate. Often, the reasons are unknown, but a variety of mechanisms have been suggested. One leading process invokes anisotropic outgassing, which exerts a torque sufficient to rapidly change the angular momentum of the nucleus, potentially leading to rotational instability. In this talk I will describe empirical measures of spin changes in a sample and make comparisons with a simple model. Sub-kilometer nuclei have spin-up timescales comparable to their orbital periods, confirming that outgassing torques are quickly capable of driving small nuclei toward rotational disruption. Torque-induced rotational instability likely accounts for the paucity of sub-kilometer short-period cometary nuclei, and also for the pre-perihelion destruction of sungrazing comets (whose nuclei are very small). Torques from sustained outgassing on small active asteroids can rival YORP torques, even for mass-loss rates less than 1 g/s. [[• D. Jewitt, (2021). Systematics and Consequences of Comet Nucleus Outgassing Torques. Astronomical Journal, 161:262 (12pp)• D. Jewitt. (2022). Destruction of Long Period Comets. AJ, 164:158(9pp)]].
PS05-A019
Exploring Evolutions of Surface Depressions on Jupiter Family Comets
Bumhoo LIM+, Masateru ISHIGURO#
Seoul National University
The investigations into five Jupiter Family Comets (JFCs) —9P, 19P, 67P, 81P, and 103P— explored by a series of space missions have unveiled a remarkable diversity in their morphology and surface features. Cometary depressions discovered on their surfaces are common, yet their exact origins remain a subject of debate due to unique morphological traits and widely varying surface densities. Conventional explanations for their evolutions have been tied to near-sun orbital histories and subsequent mass-loss processes. This study delves into the evolutions of cometary depressions during two distinct orbital phases of JFC: the “active” phase in the inner solar system and the “reservoir” phase in the Kuiper Belt. Firstly, we demonstrate that the enlargement of the depressions during the active phase is insufficient to elucidate their formation, prompting consideration of depressions originating in earlier phases. Secondly, we explore the possibility that these depressions were produced by collisional events in the Kuiper Belt. Employing statistical analysis of collisional probabilities along with an established orbital model for the Kuiper Belt, we discern a broad spectrum of collisional probabilities among Kuiper Belt Objects (KBOs), depending on their orbital elements. Our analysis reveals that the size distribution of reproduced craters adequately accounts for existing variations in depression densities of four JFCs and one KBO (Arrokoth), except for an unusually high depression density of 81P. We conclude our discussion by addressing the possible causes of the high depression density in 81P and exploring its plausible origins.
PS05-A011
The Migrating Boulder in Khonsu Region of Comet 67P/Churyumov-Gerasimenko
Xiang TANG+, Xian SHI#
Shanghai Astronomical Observatory
European Space Agency’s Rosetta is by far the only space mission that performed long-term monitoring of comet at close distances. Its over two years’ rendezvous with comet 67P/Churyumov-Gerasimenko (hereafter 67P) revealed diverse evolutionary processes of this micro-gravity world. One of the intriguing findings by Rosetta is the ejection and recycling of dust particles via different activities, many of whose mechanism remain not entirely clear. The mobilisation of boulders several to tens of meters in size are even less understood, usually connected to geological changes. The most striking event of boulder migration is the ∼140 m-transport of a ∼30 m-diameter boulder, which is so far the largest boulder identified with displacement on 67P (El-Maarry et al. 2017). The event took place in the Khonsu region of the southern hemisphere of 67P, leaving no conspicuous trails or any prominent deformation in local areas. Several triggering mechanisms were proposed, including an outburst at the boulder site, seismic vibrations from nearby activities, or surface erosion beneath the boulder (El-Maarry et al. 2017, Hasselmann et al. 2019).In this work, we combine analysis of imaging data from Rosetta’s OSIRIS camera system with thermophysical modelling to further understand this unique event of boulder activity. We derived a detailed timeline of the boulder migration event and the evolution of local areas, narrowing the occurrence time of migration to within 36 hours in early October 2015, when the spacecraft was distanced from the nucleus. Combining actual and synthetic images for the geo-morphological analysis, we found relatively frequent dust activities around the boulder, some are potentially correlated with the migration event. Furthermore, we analyzed the thermal history of the boulder and its surrounding areas to find significant north-south dichotomy in the variation of temperature and ice concentration, that might lead to triggering activity for the boulder’s migration.
PS05-A016
Anatomy of a Comet Tail Transited by the Juno Spacecraft En Route to Jupiter
Peter JORGENSEN1, J. E. P. CONNERNEY2,3#+, John JORGENSEN1, Mathias BENN1, Anja ANDERSEN4, Troelz DENVER1, Scott BOLTON5
1Technical University of Denmark, 2Space Research Corporation, 3NASA Goddard Space Flight Center, 4University of Copenhagen, 5Southwest Research Institute
A star camera aboard the Juno spacecraft traveling from Earth to Jupiter serendipitously recorded the impact of interplanetary dust particles (IDPs) by imaging bits of the spacecraft ejected from the IDP impact sites. In essence, the Juno spacecraft, with its expansive ~60 m2 of solar arrays, served as a dust detector with orders of magnitude more aperture than dedicated dust detectors specifically designed and flown to detect dust impacts. Consequently, Juno recorded many impacts with the larger (few to tens of micro-meters) and less numerous IDPs that populate the inner solar system, establishing for the first time their distribution and source (Jorgensen et al., 2020). Six months prior to its arrival at Jupiter, the Juno spacecraft recorded a singular burst of interplanetary dust particle impacts attributed to passage through the extended tail of a comet. That comet has now been identified as the recently discovered Jupiter family comet P/2019 S3 Pan-STARRS (SPKID 1003641), affording a unique opportunity to characterize the dynamical motion of the comet’s dust tail. Dust impacting the spacecraft orbits under the influence of radiation pressure forces and gravity (ratio b = ~0.05), escaping the comet nucleus ~2 years prior to impact on the spacecraft and ~1 year post comet perihelion. Impacting dust, with an implied radius of ~10 mm, escaped the comet nucleus with a radial velocity of ~120 ms-1, appropriate to a comet with a radius of a few km.
PS05-A005
Time-series Photometric Surveys for Investigating Rotational Properties of Asteroids with KMTNet
Hee-Jae LEE1#+, Myung-Jin KIM1, Hong-Kyu MOON1, Young-Jun CHOI1,2
1Korea Astronomy and Space Science Institute, 2University of Science and Technology
The rotational properties of asteroids are essential for understanding their nature and can be revealed through time-series photometric measurements, commonly referred to as light curves. Although several studies on asteroid light curves have been published, only 3% of the identified asteroids possess confirmed rotation periods. Moreover, observational biases tend to favor asteroids exhibiting conspicuous amplitudes or abbreviated rotation periods, constraining our understanding of their physical properties. Hence, to achieve a broader understanding of the nature of asteroids, systematic photometric surveys of asteroids that can reduce such biases and increase the sample size are necessary. Consequently, we organized time-series photometric surveys using the Korea Microlensing Telescope Network (KMTNet), which comprises three 1.6-m telescopes equipped with 18 k ×18 k pixel CCD cameras distributed across the Cerro-Tololo Inter-American Observatory (CTIO), South African Astronomical Observatory (SAAO), and Siding Spring Observatory (SSO), enabling uninterrupted 24-h surveillance in the Southern Hemisphere. Commencing in the second half of 2019, our survey monitored the ecliptic plane within a 2° x 14° celestial region nightly at 25-min intervals. We observed observing approximately 40,000 asteroids annually and confirmed rotation periods for 10% of them. Notably, we successfully captured subtle variations in light curves of long-period asteroids. Intriguingly, approximately 55% of the observed asteroids were found to exhibit rotation periods exceeding 10 h; this proportion of asteroids was previously reported to be 35%. Our survey results endeavor to mitigate observational biases, expand sample size, and substantially contribute to identifying asteroids with extended rotation periods, thereby enriching our comprehension of asteroid dynamics.
PS05-A015
Thermal Imaging of C-type Asteroid 162173 Ryugu and Its Applications to Future Missions
Tatsuaki OKADA#+
Japan Aerospace Exploration Agency
Hayabusa2 has returned 5.4 grams of samples from the C-type asteroid 162173 Ryugu, and the initial descriptions and analyses show that the samples are most similar to CI chondrites regarding chemical, mineralogical, and isotopic composition. However, there are some reports that the physical properties of the samples are more like Tagish Late meteorites. This results may be caused by aqueous alteration and adsorption of CI chondrites by a long-time storage under atmospheric conditions after Earth entry. Even the returned samples have been destroyed by crash and fracture during the sampling at asteroid and during the reentry in the return capsule. Therefore, the original physical properties are important to be investigated. Thermal infrared imaging (thermography) is applicable to determine thermal inertia, resistance for temperature change, of the surface materials. In Hayabusa2, the first global thermal images of an asteroid have been taken for one asteroid rotation using TIR instrument, and the first global thermal inertia and roughness maps were constructed for Ryugu. We found that the surface boulders covering the entire asteroid have much lower thermal inertia (or higher porosity) compared with typical values for CI chondrites. We also discuss here the results for thermal inertia of boulders. This method will be applied to the asteroids 2001CC21 and 1998KY26 to be explored in the Hayabusa2 extended mission (Hayabusa2#). In addition, the updated thermal imager TIRI has been developed for the ESA Hera mission to asteroid Didymos and Dimorphos, and also for the RAMSES mission, which is under study, to asteroid Apophis.
PS05-A028
Planetary Science with the 0.7 – 5.0 µm SPHEREx Solar System Object All-sky Spectral Catalog
Carey M. LISSE1#+, James BAUER2, Yaeji KIM2
1Johns Hopkins University Applied Physics Laboratory, 2University of Maryland
SPHEREx, the Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer, is a cosmological mission in NASA's MIDEX astrophysics program that will launch in early 2025 and perform a 2-year all-sky near-infrared spectral survey at WISE sensitivity levels in 106 spectral bands between 0.75 - 5.0 µm with R = 41 to 135 while visiting every 6.2 x 6.2 arcsec pixel on the sky at least 4 times. More details concerning SPHEREx are available at http://spherex.caltech.edu. The upcoming SPHEREx spectral survey provides a fantastic opportunity to detect, spectrally categorize, and catalog hundreds of thousands of foreground solar system objects at WISE/NEOWISE sensitivities using a single stable, well-characterized and calibrated space-based remote sensing platform. The resulting spectra could be used for everything from discovering and characterizing families of asteroids, comets, Trojans, Centaurs, KBOs, interstellar objects, and potentially hazardous objects; to mapping the zodiacal light with higher spatial and spectral resolution than has ever been done previously; to augmenting the science return from other spacecraft missions like DAWN, PSYCHE,LUCY, and NEOSurveyor. However, great care will be required to properly convert the millions of individual SPHEREx LVF sky images into calibrated spectra with observational systematics removed. Providing the planetary science community with an accurate spectral data catalog will require the work of a dedicated team familiar with the SPHEREx mission and instrumentation, time domain astronomical observations, and big dataset archiving at the PDS and IRSA. In this paper we give an overview of the SPHEREx mission, and describe the promise and challenges of taking the SPHEREx sky-survey LVF imaging data obtained by a mission designed to study billions of fixed galaxies and produce a moving object catalog with scientific content even greater than of the previous NEOWISE NIR photometric all-sky catalog, for ~15 times less cost.
PS05-A020
Science Overview of the Emirates Mission to the Asteroid Belt
Noora ALSAEED1#+, Hoor ALMAZMI1, Paul HAYNE2, William BOTTKE3, Margaret LANDIS2
1United Arab Emirates Space Agency, 2University of Colorado Boulder, 3Southwest Research Institute
The Emirates Mission to the Asteroid Belt (EMA) is set to launch in 2028 to explore a diverse collection of main belt asteroids. Over a seven year period, EMA is planned to conduct flybys of six asteroids and rendezvous with the final seventh. The mission targets consist of asteroids representing five different asteroid families, with the ultimate goal of unraveling the origins and evolution of water-rich asteroids. Concurrently, the mission will be assessing potential space resources for future exploration endeavors. The three main questions EMA focuses on are: 1) What is the origin of volatile-rich asteroids? 2) Are these asteroids connected to specific meteorites? 3) What insights into main belt evolution can be gleaned from their chemical inventory and volatile abundances? To answer these questions, the following mission objectives were set: A) Determine the geologic history and volatile content of multiple main belt asteroids and investigate the interior structure of the rendezvous target. B) Determine temperatures and thermophysical properties on multiple asteroids to assess their surface evolution and volatile histories. The EMA remote sensing suite comprises: 1) a visible narrow-angle camera (NAC), 2) a mid-wave infrared spectrometer (MWIR), 3) a thermal IR spectrometer (TIR), and 4) a thermal IR camera (IR-cam). The MWIR instrument, MIST-A, is provided by the Agenzia Spaziale Italiana (ASI) in partnership with the Italian National Institute for Astrophysics (INAF) and Leonardo S.p.A., the NAC and IR-cam will be provided by Malin Space Science Systems, and the TIR will be provided by Northern Arizona University and Arizona State University.
Session Chair(s): Yeon Joo LEE, Institute for Basic Science
PS12-A001
Mesoscale Stationary Features on Venus at Visible Wavelengths
Jose SILVA1#+, Yeon Joo LEE1, Takeshi IMAMURA2
1Institute for Basic Science, 2The University of Tokyo
The recent observation of an enormous bow-shaped cloud structure that is stationary relative to the surface by the Japanese Akatsuki spacecraft has spurred new interest in Venus atmosphere dynamics and gravity wave studies. These features are of remarkable importance because they provide clues to the influence of surface topography on atmospheric circulation on the cloud tops, more than 60 km above. However, their ubiquitous appearance is enigmatic since previously modeled conditions near Venus’ surface would make the generation of such waves unlikely. Modern idealized simulations have been able to reproduce the observed large bow-shaped stationary structure, but mesoscale features have proven more elusive. These stationary features have been interpreted as gravity waves generated by surface topography. Gravity waves can significantly contribute to the angular momentum delivered to the cloud top, where superrotation is maintained. With large data bases from spacecraft observations including Akatsuki and past European space mission Venus Express, we are better poised than ever to track these features at a wide range of locations over Venus, mapping their distribution and properties to better constrain current circulation models. It is in this spirit that we present these findings of mesoscale stationary features on Venus using VIRTIS-M archived data at visible wavelengths, compared with previous observations from other facilities. Our results represent a sample of the currently available data set and show stationary structures with unexpected morphologies. With these early results, we aim to foster continued interest in these features and a deeper understanding on their role in the Venusian atmosphere.
PS12-A006
Enhanced Energization of Pickup Ions Around Mars from Interplanetary Shocks
Linxia HE1+, Jianpeng GUO1#, Fan ZHANG1, Haibo LIN1, Yan CHEN1, Dan ZHAO1, Weiduo MENG1, Yong WEI2, Libo LIU2, Ruoyu GUI1
1Beijing Normal University, 2Chinese Academy of Sciences
Ion pickup is one of the main loss mechanisms of the Martian neutral atmosphere, predominantly hydrogen (H) and oxygen (O). It has been reported that interplanetary (IP) shocks are good accelerators of pickup ions. However, the ion acceleration mechanisms associated with the shock arrival have not yet been fully elucidated. Using the lists of IP shocks detected by Mars Atmosphere and Volatile EvolutioN (MAVEN) (see Huang et al.[2021]), we find that 26 fast forward shock events (68.42% of the total) have continuously detected H+ pickup ions during shock passage, and these ions can possess higher energy after shocks. Heavy pickup ions (e.g. O+) escaping Mars along the solar wind electric field are often called an “ion plume”. Based on the MAVEN data from October 2014 to February 2023, we successfully identified one plume ion energization event associated with a transmitted IP shock propagating through the Martian magnetosheath on March 3, 2015. This event is unique in that the plume O+ ions that originated from similar source regions continuously entered the narrow field of view of STATIC during the IP shock passage. Our analysis suggests that the enhanced convection electric field due to IP shock compression is the primary factor contributing to the enhancement of energization of pickup ions. These findings provide a crucial clue to the understanding of how IP shocks facilitate ion escape through the pickup process.
PS12-A008
Climatology of Martian O2+ Perturbations as Observed In Situ by MAVEN/NGIMS from 2014 to 2023
Jaeheung PARK#+
Korea Astronomy and Space Science Institute
The Martian ionosphere is spatially inhomogeneous and filled with density perturbations spanning a wide range of scale sizes. This presentation reports climatology of ionospheric O2+ perturbations at Mars, as observed by the Neutral Gas and Ion Mass Spectrometer (NGIMS) onboard the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft between 2014 and 2023. O2+ density data at a 4-second cadence (~one data point every 16 km along the spacecraft orbit) is used, while ‘perturbation’ is defined as the ratio of residual O2+ density to the large-scale background. The residual and the background are separated by a Savitzky-Golay filter with a 140-second (~560 km along the spacecraft orbit) window. Generally, the Martian O2+ perturbations are stronger at night than at day, and clear contrast between the two emerges across the seasonally varying solar terminator. MAVEN encountered more intense perturbations in the local winter hemisphere than in summer, and above crustal magnetic anomalies than at non-magnetized regions. The climatology is not well predicted by solar wind electron density/temperature of thermospheric CO2 density.
PS12-A018
Climatology of the Residual Mean Circulation of the Martian Atmosphere and Contributions of Resolved and Unresolved Waves Based on EMARS
Anzu ASUMI1#+, Kaoru SATO1, Masashi KOHMA1, Yoshi-Yuki HAYASHI2
1The University of Tokyo, 2Kobe University
The objective of this study was to examine both the climatology of the residual mean circulation, and the roles of resolved wave (RW) and unresolved wave (UW) forcings over four Mars years, based on the transformed Eulerian mean equation system using the EMARS reanalysis dataset. While RW forcing was estimated directly as Eliassen–Palm flux divergence, the forcing by UWs, including subgrid-scale gravity waves, was estimated indirectly using the zonal momentum equation. This indirect method, devised originally for study of Earth’s middle atmosphere, is applicable to latitudinal regions having angular momentum isopleths connected from the surface to the top of the atmosphere, which are usually mid- and high-latitude regions. In low latitudes of the winter hemisphere, a strong residual mean poleward flow is observed at an altitude range of 40–80 km, where the latitudinal gradient of the absolute angular momentum is small. The strong poleward flow crosses the isopleths of angular momentum in the regions of its northern and southern ends, indicating the necessity of the wave forcing. Our results suggest that the structure of the residual mean circulation at mid- and high-latitude regions is largely determined by UW forcing, particularly above the altitude of 60 km, whereas the RW contribution is also large below the altitude of 60 km.
PS12-A007
Martian Polygonal Terrain and Its Hints of Hydrothermal Conditions on Ancient Mars
Jinhai ZHANG, Lei ZHANG#+, Chao LI
Chinese Academy of Sciences
Martian polygonal terrain, widely distributed on the surface, provides valuable geological insights into the environmental conditions during their formation, including aspects related to thermal conditions and the possibility of past aqueous activity of Mars. First, we provide an overview of the polygonal terrain on Mars, including their distribution, size, and possible formation mechanisms. Second, in order to quantitatively analyze the geometric features of polygonal terrain and their relationship with the ancient climate on Mars, we process images from the High-Resolution Imaging Science Experiment (HiRISE) of a polar region and recognize the boundaries of polygons. Subsequently, we calculate the polygonal terrain’s area, orientation, and wedge density to build up new constraints on the formation mechanism of the polygonal terrains. Finally, we report special frequency-variation patterns of Zhurong radar reflections and interpret them as buried polygonal terrain beneath the landing site. Sixteen polygonal wedges deeper than 35 m have been identified within ∼1.2 km traveling distance, indicating a potentially widespread distribution of such terrain under Utopia Planitia on Mars. Based on constraints of the geometric features of the polygons and the geological background of the landing site, the identified buried polygons are interpreted as having been generated by freeze-thaw cycles. The contrast above and below ∼35 m depth represents a notable transformation of aqueous activity or thermal conditions in the Late Hesperian–Early Amazonian. This finding is remarkable as it indicates that the mid-latitudinal region experienced a cold and wet environment near the freezing point of water around the Hesperian–Amazonian transition, possibly induced by Mars’s high obliquity. These studies on Martian polygonal terrain in terms of polygons’ geometric characteristics and the formation mechanism provide significant constraints for understanding the climate and environment of ancient Mars.
PS12-A005
MAVEN Observations of the Interloop Magnetic Reconnections at Mars
Guo CHEN1+, Can HUANG1#, Ying ZHANG1, Aimin DU1, Yasong GE1, Rongsheng WANG2, Lei WANG1, Lican SHAN1, Christian MAZELLE3, Hao LUO1
1Chinese Academy of Sciences, 2University of Science and Technology of China, 3Institute for Research in Astrophysics and Planetology (IRAP), National Center for Scientific Research (CNRS) - University of Toulouse (UPS) - National Center for Space Studies (CNES)
Magnetic reconnection between neighboring magnetic field loops, so-called inter-loop reconnection, is a common process to drive flares in the solar atmosphere. However, there is no direct evidence that a similar but less explosive process can take place on planets. The strong crustal fields on Mars generate plenty of magnetic loops in the near Mars regions, which provides a unique environment to research the inter-loop reconnection on a planet. Here, we report magnetic reconnection events between crustal field loops in the Martian ionosphere observed by MAVEN for the first time. During the current layer crossing, MAVEN recorded the characteristic signals of collisionless magnetic reconnection, including the Hall magnetic field, Alfvénic outflow, and electron energization. This finding implies that the inter-loop reconnection in the Martian ionosphere could contribute to the localized energy deposition and particle energization, which provides the seed source for aurora in the Martian atmosphere.
Session Chair(s): Durga Prasad KARANAM, Physical Research Laboratory, Wing-Huen IP, National Central University
PS16-A033
| Invited
Role of Ancient Impact Basins in Facilitating Late Stage Volcanism on the Moon: New Insights
Neeraj SRIVASTAVA#+, Neha PANWAR, Megha BHATT, Anil BHARDWAJ
Physical Research Laboratory
The early impact history of the Moon is not well understood. Several impact structures formed during the pre-Nectarian time have muted to no topographic signatures because of obliteration by subsequent impacts, unfavorable crustal conditions, volcanic resurfacing, and burial under the ejecta making them difficult to identify [1,2,3]. The gravity field acquired by the Gravity Recovery and Interior Laboratory (GRAIL) mission [4] aided in the identification and mapping of some of these large impact structures on the Moon [5]. The study presented here discusses in detail the geology of three pre-Nectarian impact basins viz. Grimaldi Basin, Crüger-Sirsalis Basin, and Australe North Basin [6,7,8] and their impact on the volcanism in the region. The Crüger-Sirsalis Basin and Australe North Basin are highly obscured basins and their presence was first confirmed using GRAIL [5]. The basins discussed above exhibit unique styles of magmatism with distinct volcanic units emplaced within each basin. They also act as hosts to late-stage volcanism on the Moon with Grimaldi Basin displaying evidence of volcanism as recent as 700 Ma [6]. We have used high-resolution topography, mineralogy, and panchromatic image data from various remote sensing missions to delineate the intimate relationship that the impact cratering processes share with volcanism on the Moon and its implications in understanding the lunar geological evolution. [1] Spudis P. D. et al. (1994) Sci. 266, 1848-1851 [2] Kamata S. et al. (2013) J. Geophys. Res. Planets, 118, 398–415 [3] Miljković K. et al. (2021) Nat Commun. 12, 5433 [4] Zuber M. T. et al. (2013) Sci. 339, 668-671 [5] Neumann G. A. et al. (2015) Sci Adv. 1(9), e1500852. [6] Singh, T., & Srivastava, N. (2020) Icarus 351, 113921 [7] Singh, T. et al. (2022) Icarus 376, 114875 [8] Panwar, N., & Srivastava, N. (2024) Icarus, 408, 115841.
PS16-A021
| Invited
Natural Ejection of Volatile Species from the Lunar Surface at the Polar Regions
Makiko OHTAKE1#+, Satoshi TANAKA2, Yusuke NAKAUCHI3, Keisuke ONODERA1, Hiroshi NAGAOKA3, Ryusuke NISHITANI2
1Okayama University, 2Japan Aerospace Exploration Agency, 3Ritsumeikan University
We identified water gas/ice absorptions in visible to near-infrared spectra obtained by Spectral Profiler onboard SELENE (Kaguya) in previous study. The absorptions were identified both in PSRs and non-PSRs during nighttime when no illumination reached the lunar surface, while nearly horizontal solar light at these regions could illuminated the sky. Detailed ray-trace, spectral shape, location, and observation timing analyses suggest that impact events cannot be their main origin. And we confirmed that the absorption signal we identified is not from the lunar surface and the volatile materials must be lofted (ejected) from the lunar surface and reached to a higher altitude in space, where illuminated by the Sun. Frequency, duration, and size of the identified water ejection events revealed that the lunar polar region is extremely active in terms of volatile migration. In this study, we investigated chemical composition of the identified volatile materials to see if any volatile species other than water were ejected from the lunar surface by conducting spectral fitting to the absorption identified spectra. Results suggest that methane and possibly ammonia were contained in the ejected material together with water and ratio of amount among these chemical species varied with time and location suggesting heterogeneous distribution of volatile species in the lunar surface layer (up to several tenth of centimeters). Although we are proposing that sublimation from the subsurface (~10 cm) is a most likely origin for the identified water, process to store and release methane and ammonia which have significantly lower sublimation temperature than water require future investigation.
PS16-A006
Geochemical Characteristics of the Lunar Apollo Basin Region
Yeming BAO#+, Dijun GUO, Yang LIU
Chinese Academy of Sciences
The Apollo basin is situated on the northeast of the most ancient and largest South Pole-Aitken (SPA) basin overlapping its inferred inner rim. It is selected as the candidate landing site for the Chang'e-6 sample return mission to be launched in 2024. In pursuit of the compositional characteristics and geologic implications of the Apollo basin region, we conducted a comprehensive analysis of the critical elements on the Moon, including FeO, TiO2 and Th. Data collected by the Multiband Imager (MI) onboard the Kaguya lunar orbiter satellite and Gamma‐Ray Spectrometer (GRS) onboard the Lunar Prospector were utilized to derive the concentrations of the three elements. Our analysis focused on the geochemical composition of specific geologic units and compared them to the geochemical characteristics of lunar samples brought back by previous missions. Results indicate that distinct impact basin units are subjected to varying degrees of mixing of lunar crustal materials, mantle materials, and impact ejecta. KREEP materials are absent in the mare basalts of the Apollo basin region. The ancient SPA mare is heavily contaminated with exotic materials due to postdated impacts and the younger Apollo mare exhibits compositional heterogeneity. Our investigations revealed complex material mixing processes and intricate magmatic evolution processes within the research region. The comparable TiO2 and Th abundances of the SPA ejecta (mixed with substantial upper mantle material) and Orientale ejecta (dominated by crustal material) suggest that the mantle overturn process occurred prior to the SPA impact event. Our results provide a systematic understanding of the evolution history of the Apollo basin region and offer valuable information for the analysis of samples returned from the Chang'e-6 mission.
PS16-A018
Understanding the Structural Variations Within the Shallow Subsurface of the Moon Using Meteorite Impacts as Tracers – A Model-based Study
Saurabh DATTA GUPTA#+
Indian Institute of Technology (Indian School of MInes), Dhanbad
The surface of the Moon is covered with fine layer of dust and debris formed due to a process called regolith gardening. Most of the roughness of the Moon’s surface is created due to regolith gardening which is primarily due to meteorite impacts. Different groups of meteors hit the Lunar surface, which generates a variable set of stress and strain on the surface. This study has been performed to capture the variation of the heterogeneities within the shallow lunar subsurface, due to the impacts of different sizes of meteors. The analysis can capture the heterogeneity of the Lunar surface up to a certain depth. The computation of acoustic impedance (AI) of the heterogenous area of the Lunar surface is the most significant hypothesis of this study. Different sizes of meteors fall at different velocities from variable distances. These variations affect the lunar surface differently by creating subsidence or cavities. These changes are observed in the different locations of the lunar surface, where based on the impact of meteor, density of the rock properties varies. We considered the projectile velocity of a meteoritic fall to be equivalent to the impact of velocity on the surface. Estimations of acoustic impedance (AI) based on assumed velocity and measured density of the rock property of the Lunar surface can characterize the geological heterogeneity of the surface in the current study. A proper characterization of AI of the Lunar surface and suitable information on acceleration will not only be useful to compute the distance of meteoric fall but also help in having an insight into the shallow subsurface structure or heterogeneities. Computation-based conceptual analytical study provides broad ideas about the heterogeneities within the Lunar surface, which is highly beneficial for planetary science studies. Details of this work and preliminary results will be presented.
PS16-A015
The Crustal Structure of the Moon: Constraints from the High-resolution Gravity Data
Shengxia GONG#+
Shanghai Astronomical Observatory
The lunar crust serves as a valuable repository of records accumulated since the Moon's inception, encapsulating its early history. This geological archive contains crucial information that could unravel significant aspects of lunar evolution. The unprecedented high-resolution gravitational data obtained by the lunar GRAIL mission provides a unique way to explore the internal structure of the Moon. In this study, we make use of the latest high-resolution lunar gravity data, expanded into spherical harmonic coefficients up to 1200 degrees (corresponding to a spatial resolution of 4.5 km), coupled with the lunar topography data obtained from the LOLA that onboard the LRO mission, expanded into spherical harmonic coefficients up to 2600 degree (corresponding to a spatial resolution of 2 km). By employing the effective density spectrum method along with the localized spectral analysis technique, we investigate the density structure of the lunar crust.
PS16-A014
Latitudinal and Longitudinal Asymmetries Caused by Space Weathering and Impact Gardening
Kilho BAEK1+, Sungsoo KIM1#, Chae Kyung SIM2,3
1Kyung Hee University, 2Korea Astronomy and Space Science Institute, 3Korea National University of Science and Technology
Space weathering is interactive processes of planetary surface and solar wind particles, micrometeorite bombardments, and cosmic rays. The lunar craters are good tools for analyzing asymmetries of space weathering caused by solar wind or micrometeorites. The wall quadrants of a lunar crater provide the advantages of being exposed to space weathering for the same amount of time since the crater was formed and being affected by different fluxes by slope of a crater wall. In the present work, we used about 30,000 craters covering latitudes within ±60° and the entire longitudes to measure latitudinal and longitudinal trends of flux variation. Through detailed analysis using a large number of craters, we discovered a latitudinal asymmetry and a distinct longitudinal offset between the northern and southern hemispheres. These results trace an evidence of impact gardening caused by meteoroids (probably several tens of meters in diameter) and suggest that meteoroids enter the Moon in an anisotropic or asymmetric way with preferences in direction, possibly along a certain line that intercepts a latitude in the northern hemisphere on average. We expect that these results help quantify the extent to which lunar regolith is mature by solar wind particles and is fresh by meteoroid impacts.
PS16-A012
NASA SSERVI: Bridging Science and Human Exploration
Emily LAW1#+, Gregory SCHMIDT2, Kristina GIBBS3, Brian DAY3
1NASA Jet Propulsion Laboratory, 2NASA Solar System Exploration Research Virtual Institute, 3National Aeronautics and Space Administration
The NASA Solar System Exploration Research Virtual Institute (SSERVI) is a virtual institute focused on research at the intersection of science and human exploration, training the next generation of exploration scientists, and developing the broad scientific and technical community. Part of SSERVI’s mission is to act as a hub for opportunities that engage the larger scientific and exploration communities to form new interdisciplinary, research-focused collaborations. SSERVI represents a close collaboration between science, technology and exploration, and was created to enable a deeper understanding of the Moon, Near Earth Asteroids (NEAs) and the moons of Mars. SSERVI is supported jointly by NASA’s Science Mission Directorate and Exploration Systems Development Mission Directorate. This talk will describe the research efforts of the SSERVI domestic teams that constitute the U.S. complement of the Institute and how the Institute engages the community through workshops, conferences, online seminars and classes, student exchange programs and internships. In addition, this talk will discuss SSERVI’s current international partnerships, a key part of its global mission. Currently, the research profile of the Institute integrates investigations of plasma physics, geology/ geochemistry, technology integration, solar system origins/evolution, regolith geotechnical properties, analogues, sample science, volatiles, PSRs, ISRU and human exploration potential of the target bodies as well as numerous other research areas. As the Institute’s teams build upon their proposed research, new opportunities for both domestic and international partnerships will be generated that will produce exciting new results and generate new ideas for scientific and exploration endeavors. SSERVI enhances the widening knowledgebase of planetary research by acting as a bridge between several different groups and bringing together researchers from: 1) scientific and exploration communities, 2) multiple disciplines across the full range of planetary sciences, and 3) domestic and international communities and partnerships.
Session Chair(s): Yoonyoung KIM, University of California, Los Angeles
PS05-A022
| Invited
Simulating Rubble-pile Asteroids as Granular Systems
Bin CHENG#+
Tsinghua University
Asteroids are minuscule in size compared to planets and might seem insignificant at first glance. However, they hold clues about how our solar system formed, and also hold promise and peril for humans as the source of both rich materials and Earth impact hazard. In contrast to large planets like Earth, Mars and the Moon, almost all asteroids are made up of gravitational aggregates, also called 'rubble piles'. Their surfaces are also covered by a layer of unconsolidated and loose materials, including from smooth dust to rough rocks to giant boulders, also called 'regolith'. These bodies are believed to be with no-or low-internal cohesion, and with large macro-porosity. Therefore, asteroids with rubble-pile structure show more complex dynamical properties in contrast to classical solid planets. Here, using a large-scale N-Body code DEMBody (now open-sourced at https://bin-cheng-thu.github.io/dembody-code/), we model the asteroids by a pile of loose granular particles. We consider the self-gravity, elastic force, friction, rolling resistance and cohesion between all constituent particles. We present how these granular systems behave under the exoteric forces in the solar system (e.g., YORP torque, tidal forces) or during the interaction with a spacecraft (e.g., touchdown, sampling).
PS05-A013
Quantitative Grain Size Estimation on Airless Bodies from the Negative Polarization Branch
Yoonsoo BACH1#+, Masateru ISHIGURO2, Jun TAKAHASHI3, Jooyeon GEEM2, Daisuke KURODA4, Hiroyuki NAITO5, Jungmi KWON6
1Korea Astronomy and Space Science Institute, 2Seoul National University, 3University of Hyogo, 4Japan Spaceguard Association, 5Nayoro Observatory, 6The University of Tokyo
The sunlight scattered in the backscattering direction by a rough surface is often polarized parallel to the scattering plane, opposite to the Fresnel reflection of a flat surface. This phenomenon is termed negative polarization (NP). Despite the emergence of numerous theoretical models attempting to elucidate these observations, each theory has its limitations. Thus, there persists a need for an effective empirical approach to identify a general trend. Our work focuses on an exhaustive review of various experimental studies, meticulously rectifying any typos or errors, identifying comparable samples, and unveiling two pivotal general trends in NP: its dependence on albedo and the size parameter (∝size/wavelength). Consequently, we suggest that multi-wavelength polarimetry into near-infrared (NIR) wavelengths possesses significant potential as an innovative method to quantify the grain size of airless celestial objects. Within this discussion, we discuss the cases of the Moon and Mars while presenting our new NIR polarimetry of the Dawn mission's targets, (1) Ceres and (4) Vesta. Our findings indicate that our method yields highly consistent grain size estimations for these objects when compared to other independent studies, notably recent thermal infrared modeling studies, underscoring the crucial significance of NIR polarimetry.
PS05-A014
Variation of Comet Water Production with Distance. Sensitivity to Macro- and Micro-model Parameters
Yingqi XIN1#+, Yuri SKOROV2,3, Yuhui ZHAO1, Ladislav REZAC2
1Chinese Academy of Sciences, 2Max Planck Institute for Solar System Research, 3Technische Universität Braunschweig
Understanding the observed gas activity concerning the parameters of the comet's nucleus poses a complex challenge. While solutions can be derived from specific thermal models, it is necessary to consistently rely on arbitrary values for model parameters that are inadequately known. In this work, we carry out a study of the dependence of gas activity on these parameters and assess the importance of each of them. We explore various structures of model porous dust layers, assessing solid-state and gas thermal conductivities to determine the possible range of effective thermal conductivity. The outcomes of the simulations are integrated into a thermal model that explicitly incorporates radiative thermal conductivity and the dust layer's resistance to gas flow. We conduct tests on the sublimation of water ice under three scenarios: the stationary crust model, the growing crust model, and the removing crust model, each evaluated at different heliocentric distances. The results reveal that when sublimation serves as the primary energy dissipation mechanism, uncertainties in the layer's structure have a negligible impact. However, as the relative significance of sublimation diminishes, the variability in solutions expands, reaching magnitudes of tens of percent. Anticipated significant uncertainties in effective thermal conductivity can also markedly influence gas production. Variations in the dust layer on the comet nucleus over an orbital period will lead to a significant asymmetry in the gas production rate curve between the inbound and outbound phases. The analysis performed shows that, although the parameter range has been constrained to some extent through insights from the Rosetta mission, the inherent uncertainty in certain model parameters (such as thermal conductivity) introduces ambiguity into theoretical simulation estimates. Therefore, exploring all potential solutions is preferable to providing a limited set of specific ones.
PS05-A009
A Numerical Study on Wind Erosion Threshold Velocity of Small Solar Bodies Using LBM-DEM
Qiujun WANG+, Cheng BIN#, Baoyin HEXI, Ying PIAO
Tsinghua University
Multiple aeolian-like surface features have been found on small solar bodies, such as sand ripples and wind-tails on comet 67P/Churyumov-Gerasimenko. The evolution process of these features driven by the gas-particle two-phase interaction needs to be studied to improve our understanding of cometary activity. Threshold velocity, which is the velocity at which the erosion process just occurs and it represents the ability to resist gas erosion, forms an intergral part of the understanding of the evolution process. By implementing the lattice Boltzmann method-discrete element method (LBM-DEM) approach with the partially saturated method (PSM) into our self-developed code, we developed a comprehensive framework (LBMCoupler) to simulate the gas-particle two-phase interaction on small solar bodies. Systematic simulations were conducted to investigate the relations between the threshold velocity and multiple physical parameters, including the friction coefficients and the cohesion strength. The fraction of particles at different states, which are determined according to their displacement, position, and velocity, is calculated to evaluate the threshold velocity under different conditions. Higher wind velocity is needed to initiate the grain motion process when the cohesion strength increases and the rolling friction coefficient has more influence on the process than the sliding friction coefficient. The proposed method is also applied to estimate the threshold velocity on comet 67P.
PS05-A018
Rotational Instability on Asteroid Phaethon: Past, Present and Its Implications
Hangbin JO1+, Masateru ISHIGURO1#, Derek RICHARDSON2, Sean MARSHALL3
1Seoul National University, 2University of Maryland, 3University of Central Florida
Selected as the target of the JAXA/ISAS DESTINY+ mission (Arai et al., 2018), asteroid 3200 Phaethon is a relatively large object of ~5 km (Hanuš et al. 2016) in diameter. It is orbiting in the inner Solar System with a highly eccentric and inclined orbit, making it a very unusual and prominent near-Earth and near-Sun object. Furthermore, it is famously regarded as the parent body of the Geminid meteor shower (Whipple, 1983; Gustafson, 1989). Another key feature of Phaethon is its fast rotation (3.6 hr, Hanuš et al. 2016) putting the asteroid in a near-critical state. Although the cohesion of ~50 Pa can keep the asteroid stable (Nakano & Hirabayashi, 2020), this is contrary to the findings of spacecraft observations on asteroids Ryugu and Bennu, which suggest that the regoliths of these asteroids are cohesionless (Arakawa et al., 2020; Walsh et al., 2022). Thus, when assuming a similar cohesionless surface state, it is reasonable to expect the surface of Phaethon to show hints of recent and/or frequent mass migration. Additionally, it has been hypothesized that the Geminids were formed by mass shedding by rotational instability in the past, caused by the Yarkovsky-O’Keefe-Radzievskii-Paddack (YORP) effect (Nakano & Hirabayashi, 2020). We present an overview of the implications by the past and present rotation of Phaethon. We first review our recent results of dynamical simulations supporting rotational instability as the ejection mechanism of the Geminids (Jo and Ishiguro, A&A accepted). We then provide our analysis on the current mass movement on Phaethon utilizing the combination of its latest shape model and the parallel n-body tree code PKDGRAV (Richardson et al., 2000; Stadel, 2001; Schwartz et al., 2012; Zhang et al., 2017), with the hope of contributing to the preparation for the DESTINY + mission.
PS05-A010
Regolith Resurfacing and Shedding on Spinning Spheroid Asteroids: Dependence on the Surface Mechanical Properties
Wenyue DAI1+, Yang YU2, Cheng BIN1, Baoyin HEXI1, Junfeng LI1#
1Tsinghua University, 2Beihang University
The YORP effect can effectively alter the rotational status of asteroids. The spin-up of the asteroid will lead to the surface instability and eventually trigger the regolith failure, followed by the landslide and mass shedding on the asteroid's surface. This work explores the dynamics of the rotation-induced resurfacing and shedding. Special attention is paid to the dependence of the post-shedding evolution on the regolith mechanical properties such as the cohesion. A qualitative semi-analytical model is proposed to explore the post-failure dynamics of a fast rotating asteroid, and the interaction between the surface mass rearrangement and the asteroid’s spin status is considered in this model. The surface region where the failure occurs, the total mass shed from the surface and the spin-down of the asteroid in this process are investigated. Based on our model, all the possible avalanche events following the regolith failure can be classified into 4 basic types, and their corresponding regions in the parameter space are given in a diagram. Results show that though the regolith cohesion is very small (> ~1-2 Pa), the cohesion plays an important role in the avalanche. Moreover, our model qualitatively constructs the links between the regolith’s properties and the dynamical fates of the shed material. The time scale of the YORP-induced shedding events is also discussed in this work.
PS05-A025
Influences of Substructures on Impact Processes of Small Celestial Bodies
Xiaoran YAN1#+, Patrick MICHEL2, Junfeng LI1
1Tsinghua University, 2CNRS, Observatoire de la Côte d'Azur
Hypervelocity impacts, ranging from local scale craters to global scale catastrophic disruptions, are one of the important reshaping and restructuring mechanisms on small celestial bodies. Various substructures, including monoliths, cracks, rubble piles, and regoliths, can affect the propagation of impact waves. To demonstrate this effect, we use the Material Point Method (MPM), which is an extension of the particle-in-cell method that is suitable for solving complex boundary conditions. We further develop an algorithm to calculate the contact force with nonpenetration constraint. The simulations reveal that internal damages can significantly alter the impact dynamics by weakening the body's fragmentation resistance. Additionally, the pebbles play a role in influencing ejecta trajectories at both high and low velocities. These insights are particularly relevant for space missions focused on asteroid exploration and defense strategies, such as the artificial impact on the asteroid (162173) Ryugu conducted by Hayabusa 2, and the DART impact. Ongoing efforts in this area further contribute to our comprehensive understanding of the dynamics and history of small celestial bodies, offering valuable insights into the formation and evolution of the solar system.
PS05-A006
Configuration of Single Giant Planet Systems Generating Oumuamua-like Interstellar Asteroids
Xiling ZHENG#+, Ji-Lin ZHOU
Nanjing University
The first discovered interstellar small object, 1I/Oumuamua, exhibits unique physical properties of extremely elongated geometric shape and characteristics of both asteroid and comet, which can be explained by its origin through tidal fragmentation. This mechanism suggests that Oumuamua was produced through extensive tidal fragmentation during a close encounter with a star or a white dwarf, resulting in its ejection from its original system. Based on this theory, a high initial orbit eccentricity and a small pericenter are necessary for the creation of Oumuamua-like objects, which inspires us to consider the possibility that Oumuamua's parent body underwent planetary perturbation and eccentricity excitation. We examine a giant planet's disturbance that affects planetesimals' orbital characteristics. Through long-term simulations, we observe the evolution of these planetesimals' orbital elements and their minimal pericenters, starting with the Sun-Jupiter system and considering different exoplanet systems, we have concluded that an eccentric Jupiter system is the configuration more likely to generate Oumuamua-like interstellar objects, while the ratio of extremely elongated interstellar objects to ordinary interstellar objects is about 4%.
Session Chair(s):
PS07-A005
On the Relation Between Jupiter's Aurora and the Dawnside Current Sheet
Yan XU1#+, Zhonghua YAO2, Binzheng ZHANG2, Peter DELAMERE3, Licia RAY4, William DUNN5, Sarah BADMAN4, Enhao FENG2, Zhiqi ZHENG2, Scott BOLTON6, Denis GRODENT7, Bertrand BONFOND7, Yong WEI8
1Southern University of Science and Technology, 2The University of Hong Kong, 3University of Alaska Fairbanks, 4Lancaster University, 5University College London, 6Southwest Research Institute, 7University of Liege, 8Chinese Academy of Sciences
Jupiter's auroral emission is a spectacular phenomenon that provides insight into energy release processes related to the coupling of its magnetosphere and ionosphere. This energy release is influenced by solar wind conditions. Using joint observations from Juno and the Hubble Space Telescope (HST), we statistically investigate the relationship between auroral power and current sheet variations under different solar wind conditions. In this study, we reveal that during global main auroral brightening events that are closely connected to solar wind compressions, the dawn side current sheet is substantially thinner than during times when a quiet auroral morphology is present. The global MHD simulation results also demonstrate the thinning of the dawn side current sheet under solar wind compression. Furthermore, the total current intensity in the current sheet is found to increase under solar wind compression conditions compared to the quiet period. These findings provide important observational evidence for how magnetospheric dynamics driven by solar wind behavior affect auroral activity, deepening our understanding of the coupling between Jupiter's magnetosphere and ionosphere.
PS07-A017
| Invited
ENA Detection from Low Earth Orbit and the Space Weather ENA Radiation Sensors (SWEATERS) Network
Alessandro MURA1#+, Elisabetta DE ANGELIS1, Stefano ORSINI1, Martina MORONI1, Christina PLAINAKI2, Rosanna RISPOLI1, Anna MILILLO1
1National Institute for Astrophysics, 2Italian Space Agency
The detection of Energetic Neutral Atoms (ENA) from Low Earth Orbit (LEO) is able to provide information on several ENA sources: ENA generated in the ring current region, those generated in magnetopause on the dayside equatorial region, and those generated by high latitudes, cusp precipitating ions. The relative importance of all these sources is strictly related to the instantaneous configuration of the Earth's magnetosphere, with obvious implications to space weather. In terms of diagnosis, ENA detection is an efficient way to globally view the ring current and shock-front population dynamics, while the measurement of magnetic field variations on ground, from which geomagnetic indices like Dst are derived, include the effects of all current systems, including the Chapman-Ferraro and the cross-tail ones. However, only occasional in-situ plasma data are available by orbiting spacecraft, and, so far, this technique has been used mainly from dedicated high altitude polar orbiting spacecraft, which do not allow a continuous and systematic monitoring, and a discrimination of the particle latitude distribution. Here we discuss the merits of a project of a Space WEATher Ena Radiation Sensors (SWEATERS). This is a proposed cluster of innovative ENA detectors, placed on low-altitude orbiting and three-axes stabilized spacecrafts. Such a cluster offers a multiple vantage point system for ENA imaging of the various magnetospheric regions. We introduce the scientific requirements for the ENA sensors, the results of the simulations of the ENA signal in different configurations, and we finally discuss the potential outcomes of such a network of ENA instruments.
PS07-A015
| Invited
Comparative Magnetospheric Environments: Testing Earth-based Concepts at Other Planets
Fran BAGENAL#+
Laboratory for Atmospheric & Space Physics, University of Colorado
Early exploration of the space environment started around Earth, naturally, but 65 years after Explorer 1 we have now measured the particles and fields of the space environments of planets throughout the solar system. Perhaps not surprisingly (at least to some people) very different environments are found at the various types of planets and in at different distances from the Sun. In this talk we will summarize what we have learned - from MESSENGER at Mercury; Parker Solar Probe at Venus; MAVEN at Mars; Juno at Jupiter; Cassini at Saturn; New Horizons at Pluto; and compare with the plethora of measurements around the Earth. Obviously missing from this list are recent missions to Uranus or Neptune that have been sadly neglected since the Voyager flybys in the 1980s. The processes driving these magnetospheres have important commonalities but also major differences. There are also important implications of these magnetospheric processes for planetary surfaces and atmospheres - as well as for instrumentation sent out to explore planetary systems. Looking to the future, we will consider the exciting new science that is on the horizon from Bebi Columbo at Mercury, JUICE and Clipper at Jupiter, and, with luck, a future mission to Uranus.
PS07-A013
Io Plasma Torus Impact on Jovian Magnetopause Variability
Enhao FENG1#+, Binzheng ZHANG1, Zhonghua YAO1, Peter DELAMERE2, Zhiqi ZHENG1, William DUNN3, Shengyi YE4
1The University of Hong Kong, 2University of Alaska Fairbanks, 3University College London, 4Southern University of Science and Technology
Recent research indicates that Jupiter's magnetosphere size and variability are not solely determined by upstream conditions but are also substantially influenced by the internal mechanisms within Jupiter's magnetosphere, specifically the rotating magnetodisc and interchange structures. Prior studies have demonstrated under nominal mass loading rates, i.e., 1,000 kg/s, the interchange structures within the magnetodisc may can exert a dynamic pressure substantially greater than the solar wind ram pressure, resulting in significant fluctuations in Jupiter's magnetopause. However, given the considerable range and uncertainties in the estimated rate of Io mass loading, it remains unclear whether scale and variability of Jupiter's magnetosphere is controlled by the extent of mass loading. In this study, we conducted a series of numerical experiments to explore the impact of mass loading rate on the variability of the Jovian magnetopause. Our results indicate that an enhanced rate of Io mass loading results in a larger magnetosphere with greater variability in the magnetopause location. This expansion of the magnetosphere during enhanced mass loading is contributed to the substantially higher radial dynamic pressure originated from the interchange structures. Our study emphasizes the significance of the Io mass loading rate in understanding the variations in Jupiter's magnetosphere. These insights are essential for elucidating the dynamic processes in internally mass-loaded and/or rapidly rotating systems.
PS07-A026
| Invited
Wave Phenomena as Diagnostic of Planetary Magnetospheric Responses to Solar Wind Impact
Shengyi YE#+
Southern University of Science and Technology
Rapid changes in solar wind conditions perturb the planetary magnetospheres, modifying the properties of the plasma within, providing energy for the generation of radio emissions and plasma waves. These waves reveal the dynamic processes in and around the planetary magnetospheres. The emissions often display periodicities caused by magnetic compressional waves induced by solar wind impact. Solar wind compressions increase the plasma density in the magnetosheath, keeping low-frequency radio emissions from escaping the planetary magnetosphere (e.g. continuum radiation at Jupiter and narrowband emissions at Saturn). We will discuss recent observations made by Juno and Cassini and their implications for the dynamics of planetary magnetospheres.
Session Chair(s): Makiko OHTAKE, Okayama University
PS16-A011
| Invited
Novel Moon Observational Methods Pioneered by Juno
Scott BOLTON1#+, Steven LEVIN2, John JORGENSEN3, John CONNERNEY4
1Southwest Research Institute, 2California Institute of Technology, 3Technical University of Denmark, 4NASA Goddard Space Flight Center
The Juno spacecraft arrived at Jupiter in 2016 and was inserted into a polar orbit with perijove near Jupiter’s equator. The mission was designed with a scientific payload of nine instruments, (Radio Science, Microwave Radiometer (MWR), Jovian Infrared Auroral Mapper (JIRAM), JunoCam, Magnetometer (MAG), Waves, Jovian Auroral Distribution (JADE), Jovian Energetic Detector (JEDI), Ultraviolet Spectrograph (UVS). Juno is also equipped with a visible light color camera, primarily to facilitate public engagement (JunoCam) but also used for science. Two additional instruments have been tapped for their science potential: a spacecraft subsystem, the Stellar Reference Unit (SRU), primarily serves the spacecraft attitude determination function, and the Advanced Stellar Compass (ASC) that serves the same function for the MAG investigation at the outer end of the magnetometer boom. An important part of Juno’s scientific return has come from the novel use of both the scientific payload and these engineering subsystems. This includes the use of Juno’s microwave radiometer to map the subsurface ice shells of the icy moons, Europa and Ganymede as well the rocky lava covered surface of Io. Additionally, the Juno SRU Team has repurposed the SRU as a low light imager to obtain high resolution images of Jupiter’s nightside atmosphere as well as that of the moons, illuminated in Jupiter-shine. Likewise, the ASC has been used to obtain images of Earth and moon and exploited to detect interplanetary dust particle (IDP) impacts on the Juno spacecraft, characteriing the interplanetary dust population between Earth and Jupiter. Examples of Juno’s novel observational methods will be presented and described.
PS16-A035
| Invited
A Time-dependent Model of the Lunar Sodium Exosphere
Wing-Huen IP#+, Ian-Lin LAI, Chen-Yen HSU, Hua-Shan SHI
National Central University
Solar wind interaction with the Moon has recently been recognized to be of importance in the production of the surface layer of water molecules. Long-term coronagraphic observations of the lunar sodium exosphere also indicated that solar wind sputtering could lead to significant variations in the corresponding brightness and column density. With a view to understand the related processes, the Taiwan University Lunar Investigation Project (TULIP) has embarked on the construction of a time-dependent lunar exospheric model including Na, H2O, He, Ne and other species. The major physical ingredients are the magnetospheric passage of the Moon, meteor stream crossing, surface composition inhomogeneity, and the shielding effect of the magnetic anomalies. The preliminary results of the spatial structure of the sodium exosphere and tail at different orbital phases will be presented.
PS16-A027
| Invited
Distinct Thermophysics at Lunar High Latitudes and Poles - Insights Through Recent Observations and Improved 3-D Modelling
Durga Prasad KARANAM#+, G. AMBILY, Anil BHARDWAJ
Physical Research Laboratory
Exploring and comprehending the thermophysical characteristics of the lunar surface is crucial for advancing resource prospecting and future exploration of the Moon. Existing studies have delved into factors like solar insolation, surface physical properties, and the influence of the uppermost porous layer. Most of the current understanding about the surface and subsurface thermophysics comes from the two Apollo missions and numerical modelling, but mostly limited to equatorial latitudes. These investigations demonstrated a good correlation between modelling outcomes and observational data. Further, Diviner radiometer onboard LRO has provided a global perspective, but only limited to surficial observations. However, recent studies through in-situ observations and modelling direct towards a distinct thermophysical behaviour at lunar high latitudes and poles, with a significant spatio-temporal variation, than previously thought. The possible reason for these dynamic variations could be local topography and illumination conditions at these locations that has not been addressed completely. Therefore, we are systematically investigating the thermophysical behaviour of lunar high latitudes and poles using recent observations and an improved three-dimensional thermophysical model. Initial findings reveal significant variations in the thermal environment at these sites, particularly at local scales, compared to that at other latitudes. This understanding holds substantial implications for future missions and in-situ studies. Details will be presented and discussed.
PS16-A034
Temporal Variations of Ar-40 and Rn-222 Density Distributions in the Lunar Exosphere from Transient Events
Ian-Lin LAI#+, Wing-Huen IP, Chen-Yen HSU, Yan-Ping CHEN
National Central University
Moonquakes play a pivotal role in the liberation of noble gases, notably 40A and Radon (222Rn) which is the decay product of 235U, from the moon's interior into its tenuous, surface-bound exosphere. The random-walk trajectories of these gas atoms are ballistic, characterized by much more frequent interactions with the lunar surface than with other gas particles. The details of the gas-surface interaction depend on the lunar surface temperature distribution and various photolytic and physico-chemical reactions, many of which are still under discussion. Following previous treatments guided by the measurement data from the Apollo/LACE experiment and the LADEE observations of the LDEX mission, we constructed time-dependent models of the 40Ar and 222Rn density distributions immediately after a transient outgassing event. Our theoretical work is to prepare for in-situ monitoring of these rare gases and moonquakes by Moon-based instruments in the near future.
PS16-A017
Detection of Secondary Craters on the Lunar Surface Based on Spectral Data and Deep Learning
Yiran WANG#+, Miao ZHUO
Southern University of Science and Technology
Craters are prominent geomorphological features on the moon's surface, categorized into primary and secondary craters. A primary crater forms directly from the impact of extraterrestrial meteorites, while a secondary crater emerges from the ejecta produced during the primary crater's formation. Secondary craters serve as evidence of significant impact events, while their presence can introduce uncertainties when estimating the age of the surface. Past studies on detecting secondary craters mainly focused on visually recognizing craters with irregular shapes or those arranged in chains or clusters. Nevertheless, manual methods prove inefficient for identifying secondary craters lacking distinct morphological characteristics. The formation of primary and secondary craters involves varying amounts of energy release, which can be discerned through remote-sensing spectral data. A spectral analysis of 6,000 primary and secondary craters reveals discernible differences between the two categories. This research introduces spectral data as a foundation for distinguishing between secondary and primary craters. The region around the Copernicus crater was chosen as the study area, where a deep learning model was trained and evaluated for automated secondary crater identification. Utilizing the well-trained model, the detection of secondary craters was conducted in the entire study area. A detailed database comprising primary and secondary craters adjacent to the Copernicus crater is established, encompassing over 0.7 million craters with diameters ≥140 m. The distribution characteristics and randomness analysis of impact craters highlight the effectiveness of the secondary detection method. Additional analysis of secondary craters in the Copernicus region has been undertaken, accompanied by a discussion of its scientific significance.
PS16-A020
Novel Design of Heat Flow Probe Electronics: Design, Development, Testing and Performance
Chandan KUMAR#+, Durga Prasad KARANAM, Sanjeev MISHRA, P. KALYAN REDDY, Janmejay KUMAR
Physical Research Laboratory
Thermal probes offer unique insight into the heat flow activity on the surface and subsurface of the Moon. The heat flow data over a long duration of time provides an excellent opportunity to gain insight into the thermophysical properties of the lunar surface and subsurface. It will also give us important clues about the thermal status of lunar crust, especially uppermost regolith which is crucial for solar insolation into the subsurface of the Moon. Spatially resolved highly accurate temperature measurements are required to derive the precise heat flow and thermal conductivity of the upper layers of the regolith. Temperature measurement accuracies better than 1 K are required and designing the Front-End Electronics for achieving this accuracy and resolution in Space environment is challenging. We have designed, developed and tested a new technique of temperature measurements for applications to Moon. The design is based on bridge circuit with near zero self-heating error. The Front-End that is designed can accommodate 10 RTD sensors mounted at different depths on a thermal probe that can be inserted into the Lunar surface. All the 10 channels are functionally independent in terms of acquisition of the analog signal from the RTDs. After that, the signals are multiplexed and digitized using an ADC and are processed further. We have designed the Front-End Electronics card, developed it for Space applications keeping in view all the qualification criterion and have carried out all the qualifications tests as well. Functional tests at various stages were carried out along with the performance test carried out at the end. The overall performance of the Electronics card is marked by a sensitivity level of better than 0.5 K and a resolution of ±0.5K. In this work, we will present the design concept, developmental stages, tests and performance of this novel technique in detail.
PS16-A003
In Search of the Carbonaceous Chondrite Impact Remnants on the Lunar Surface
Yazhou YANG1#+, Yang LIU2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences
The Moon has experienced an intense bombardment history since its formation. How the impact flux and the dominated impactor types evolve over time is crucial for many key scientific questions. For example, carbonaceous chondrites are relatively rich in water and volatiles, so did a large number of carbonaceous body collisions occur in a certain period, thus bringing water tot he Earth-Moon system? In addition, what was the spatial distribution of various small bodies in the solar system in the past, and how did it evolve to the current distribution pattern? Based on the returned lunar samples and a great deal of efforts on the statistics of impact craters on the lunar surface, several models on the evolution of impact flux have been established. However, information about the proportion of various types of impactors in different periods is lacking. To figure out how the dominated types of impactors on the lunar surface evolve over time, we need to find a large number of impactor remnants and identify their types and formation time. Generally, we may find impact remnants via sample analysis, in-situ detection, and orbital detection. With the in-situ spectral data obtained by the Chang’e-4 rover, which has a spatial resolution better than 1 mm/pixel, we have identified some impact remnants rich in carbonaceous chondrite. The formation age is estimated to be less than 1 Ma. We believe that if the spatial resolution of orbital hyper-spectral data can improve to a higher level, i.e. ~1 m/pixel in future lunar missions, we may have the chance to map out the distribution of carbonaceous impact remnants on the whole lunar surface. This will further provide some new insights to the delivery and migration of the lunar surface water, as well as the evolution of the impactor types over time.
Session Chair(s):
PS07-A002
Contemporaneous Appearances of Auroral Spirals and Transpolar Arc: Changes of Auroras and Field-aligned Current Profiles Before a Substorm and After its Recovery Phase
Motoharu NOWADA1#+, Yukinaga MIYASHITA2,3, Aoi NAKAMIZO4, Noora PARTAMIES5, Quanqi SHI1
1Shandong University, 2Korea Astronomy and Space Science Institute, 3Korea National University of Science and Technology, 4National Institute of Information and Communications Technology, 5The University Centre in Svalbard
Vortex-structured auroral spirals locally appeared and transpolar arc (TPA) with larger scale were contemporaneously observed by the Polar Ultraviolet imager (UVI), when a substorm almost recovered. These two different scale auroras were simultaneously seen following the appearances of the TPA that grew as aligned to the dawnside main auroral oval from the nightside to dayside (oval-aligned TPAs), and a chain of multiple auroral spirals located azimuthally around the poleward edge of the nightside auroral oval. To examine associated magnetotail structures before a substorm and after its recovery phase, we performed global magnetohydrodynamic (MHD) simulations, based on two different MHD codes: BAT-S-RUS (Block Adaptive Tree-Solar wind-Roe Upwind Scheme) and improved-REPPU (REProduce Plasma Universe), and examined how the profiles of field-aligned currents (FACs) varied in association with changes of the auroral form to TPA and/or auroral spirals. Prior to and after the auroral spirals and contemporaneous appearances of TPA and auroral spirals, Polar detected the oval-aligned TPA and dawnside TPA with the nightside end distorted toward the pre-midnight sector (“J”-shaped TPA). Global MHD simulations with the two different codes can reproduce them and associated FAC structures in the magnetotail. However, the auroral spirals and their nightside FAC profiles were not formed by both global MHD simulations, suggesting that their formation process cannot be treated within an MHD framework but are closely related with some kinetic process. When the “J”-shaped TPA and auroral spirals were contemporaneously observed, the two MHD simulations could not reproduce the TPA, auroral spirals and associated magnetotail FAC structures. Also, this result advocates that some kinetic effect might dominantly be exerted on auroral spirals.
PS07-A008
| Invited
Rolling-pin Distribution of Relativistic Electrons in Jupiter’s Magnetosphere
Huishan FU1#+, Chaoqi WANG1, Jinbin CAO1, Zhizhong GUO1, Wending FU1, Zhonghua YAO2, Yong WEI3, Binzheng ZHANG2
1Beihang University, 2The University of Hong Kong, 3Chinese Academy of Sciences
The electron rolling-pin distribution, showing electron pitch angles primarily at 0°, 90°, and 180°, has been widely reported in the Earth’s magnetosphere, but has never been reported in other planetary environment. Here, by utilizing the Jupiter Near-polar Orbiter (Juno) measurements, we report for the first time the electron rolling-pin distribution in Jupiter’s magnetosphere. We reveal the energy range of such distribution and find it appears only above 19.5 keV, falling well into the supra-thermal energy range, which reaches the relativistic energy level. Moreover, we quantitively reproduce the formation processes of such distribution by using an analytical model. Gratifyingly, the distribution derived from the analytical model agrees well with the Juno observations. These results, demonstrating that the electron rolling-pin distribution exists beyond the Earth, can improve our knowledge of electron dynamics in the planetary magnetosphere.
PS07-A007
Magnetosphere-ionosphere Coupling in the Terrestrial Planets: Model Development and Applications
Tong DANG1#+, Binzheng ZHANG2, Jiuhou LEI1, Zhonghua YAO2, Maodong YAN1, Sudong XIAO3, Tielong ZHANG4,1, John LYON5
1University of Science and Technology of China, 2The University of Hong Kong, 3Harbin Institute of Technology, 4Austrian Academy of Sciences, 5Dartmouth College
The magnetosphere-ionosphere coupled system exists widely in the space environment of planets in the solar system and is a key component of the space weather. As Earth-like planets, Venus and Mars are very similar to the Earth in terms of size and mass, but their magnetic fields are very different, leading to great differences in their magnetosphere-ionosphere coupling processes. In this study, we describe the development of high-resolution models for the magnetosphere-ionosphere system of different terrestrial planets. Combined with the observations, we also study the magnetosphere-ionosphere responses to the solar wind, and explore the physical mechanisms behind.
PS07-A003
Predicting the Location of the Jovian Polar Cusp Through MHD Diagnostics in Global Simulations
Junjie CHEN#+, Binzheng ZHANG, Zhonghua YAO
The University of Hong Kong
Accurate prediction of the location of the Jovian polar cusp is crucial for scientific research and future missions to Jupiter. The polar cusp is a spatially narrow region within a planetary magnetosphere, where plasma and energy from solar winds can directly access the low-altitude magnetosphere and ionosphere. In the terrestrial magnetosphere, when the dipole tilt angle is small, the large-scale magnetospheric structure typically displays dawn-dusk symmetry, resulting in the polar cusp being primarily located near the noon section. However, in Jupiter’s magnetosphere with the time scale of planetary rotation much shorter than the solar wind transition, this axial symmetry may not manifest, thereby impacting the polar cusp’s location. In this study, we simulated the high-latitude cusp of Jupiter using the Grid Agnostic MHD for Extended Research Applications (GAMERA) global magnetosphere simulation. We identified the cusp location using three different MHD diagnostics: magnetic depression, plasma density enhancement, and parallel ion number flux at high altitudes. The simulation results show significant dawn-dusk asymmetries and magnetic local time extensions of the cusp location, which are driven by the planetary fast rotation. Such configuration provides new insight into interpreting measurements from other rotationally-driven systems.
PS07-A011
Comparison of the Wave Poynting Flux Associated with Earth’s Auroral Streamer and Saturn’s Nightside Polar Arc
Ziyi YANG1+, Binzheng ZHANG2, Jiuhou LEI1#, Z. H. YAO3, William LOTKO4, Junjie CHEN1, Zhiqi ZHENG2
1University of Science and Technology of China, 2The University of Hong Kong, 3Chinese Academy of Sciences, 4Dartmouth College
Transient energy flux released from magnetotail during geomagnetic substorms can cause auroral streamer at ionospheric height, which evolves rapidly and takes on different shapes on slow-spinning Earth-like planets and faster-spinning giant planets. The cause of these rapid auroras is a hot research topic, and there have been some inferences from satellite observations. Based on high spatial and temporal resolution simulation, we tracked and analyzed the generation of these auroras on a global scale from magnetosphere to ionosphere on Earth and Saturn. Comparison simulations show that the auroras on Earth are mainly caused by the reconnection of open magnetic field lines in the magnetotail. In contrast, the generation of auroras on Saturn is more complicated due to the rotating magnetodisk. The equatorial Poynting fluxes are triggered by plasma velocity shears between corotation and sub-corotation regions, and then strengthened by closed magnetic field line reconnection and open magnetic field line reconnection.
Session Chair(s): Yuqi QIAN, The University of Hong Kong
PS11-A009
| Invited
Origin of Water on the Moon
Sen HU#+
Chinese Academy of Sciences
The growing remote sensing data sets and measurements of lunar return samples have confirmed that the Moon's surface has much higher water abundance than previously thought. Today, there are little doubts that most of the Moon’s surface harbour water in one form or another. However, the origin(s) of this lunar surface water, and its spatial distribution and evolution during regolith gardening remain largely unknown, despite key implications for future lunar surface exploration, and for better understanding the (sub)surface water reservoir and processing on Solar System airless bodies. Several potential sources and processes could have contributed to the water inventory at the surface of the Moon, such as (i) solar wind implantation, (ii) outgassing of volatiles during lunar volcanism, (iii) deposition of volatile-bearing pyroclastic deposits and minerals, and (iv) delivery by impacts of comets and asteroids. In this study, we investigated the water abundances and hydrogen isotopic compositions of impact glasses that were not highly homogenized during their formation on the Moon. The preliminary analytical results indicate that about 65% of water inventory on the Moon derives from solar wind implantation, about 20% of water originated from lunar materials, and about 15% of water is contributed from chondritic materials, based on the hydrogen isotopic compositions.
PS11-A003
High Content of Solar Wind-derived Water in Chang'e-5 Lunar Minerals
Chuanjiao ZHOU#+
Chinese Academy of Sciences
Remote sensing data revealed a widespread presence of solar wind-derived water (OH/H2O) on the lunar surface. Studies on Apollo samples provided strong evidence that solar wind proton implantation is an important source of water on the lunar surface. However, the distribution, occurrence, and influences on the formation of solar wind-derived water on the lunar surface have not yet been well investigated. The lunar samples collected by the Chang’e-5 (CE5) mission from middle latitude (43.06°N, 51.92°W) of the Moon are characterized by unique sampling location and age, different from Apollo samples, are expected to provide a reference for the formation and distribution of water on the lunar surface. Here, we show large amounts of solar wind-derived water in CE5 lunar minerals by infrared spectroscopy and nanoscale secondary ion mass spectrometry analyses. The water exists mainly in the form of OH. Considering the composition of CE5 lunar soils, we estimate the OH/H2O content in CE5 lunar soils to be ~170 ppm. In addition, combined with the results of microstructural and chemical composition analyses, the solar wind-derived water is affected by exposure time, crystal structure, and mineral composition. By comparing with remote sensing data and through lunar soil maturity analysis, the amount of water in CE5 provides a reference for the distribution of surficial water in middle latitude of the Moon. Our research reveals that lunar minerals are important reservoir of water, and formation and retention of water originating from solar wind occurs on airless bodies.
PS11-A001
First Magnetic and Spectroscopic Constraints on Attenuated Space Weathering at the Chang'e-5 Landing Site
Yuqi QIAN1#+, Long XIAO2, James HEAD3, Joseph MICHALSKI1
1The University of Hong Kong, 2China University of Geosciences, 3Brown University
Space weathering is a primary process altering the lunar surface, producing submicroscopic iron particles embedded in soil grains, which have diagnostic magnetic and spectroscopic effects. However, the space weathering of lunar soils from young geological units remains mysterious without solid constraints from returned samples. Chang'e-5 mission is the first lunar sample-return mission in decades. The Chang'e-5 landing and sampling unit (~2.0 Ga) is much younger than all Apollo and Luna units (>3.0 Ga). It has provided an unprecedented opportunity to reveal the recent space weathering characteristics with both returned soil samples and in situ investigation data. In this study, magnetic approaches (Vibrating Sample Magnetometer, Electron Paramagnetic Resonance Spectrometer, Mössbauer Spectrometer) were used to characterize the Chang'e-5 lunar soil for the first time after the return of the samples, strongly supporting it is among the most immature soils on the Moon with a metallic iron abundance of 0.42% and an Is/FeO value of 14+6/-10. Additional Landing Camera and Lunar Mineralogical Spectrometer (480–3200 nm) data obtained surrounding the sampling area were used to study the lateral effects of rocket exhaust. All data from soil samples and in situ observations have offered magnetic and spectroscopic constraints on the space weathering state of the Chang'e-5 site. The combined effects of rocket exhaust by removing the top highly weathered soil and the young age of the landing site with lesser degree of impact reworking may attenuate the maturity of Chang'e-5 lunar soils.
PS11-A011
Irradiation of Olivine by 20 keV Protons and Electrons: Simulation of Space Weathering by the Solar Wind
Zhenyu XU1+, Yazhou YANG2, Jianwei HAN1, Longlong ZHANG1, Yingqi MA1, Mengze TAO1, Hongwei LI1#
1Chinese Academy of Sciences, 2National Space Science Center, Chinese Academy of Sciences
Irradiation experiments have been carried out on olivine using 20 keV proton and electron beams, and changes in the near infrared (NIR) reflectance and chemical composition of the surface were measured. We found that, under certain conditions, the irradiation were shown to darken and redden the reflectance spectra of olivine samples. Dielectric breakdown is discussed as a mechanism for the change in reflectance spectra. Using scanning electron microscopy (SEM), LEMELLE (2003) observed that irradiation of the surface of iron-bearing olivines would cause structural damage. The destabilisation of olivine is probably due to electrostatic discharges leading to the breakdown of the dielectric lattice. The possibility that such processes could be responsible for significant space weathering of interplanetary dust particles and regoliths of planetary surfaces should be considered.
PS11-A012
What Shifts the CF of Lunar Surface Materials: Space Weathering or Impact?
Mengyuan ZHANG1+, Yazhou YANG2#, Zhiyong XIAO3, Yang LIU1
1Chinese Academy of Sciences, 2National Space Science Center, Chinese Academy of Sciences, 3Sun Yat-sen University
Spectroscopic remote sensing technique has been widely used in characterizing the surface mineralogical compositions of airless bodies, as most silicate rock-forming minerals, i.e. silicates, have diagnostic absorption features. However, space weathering processes including micrometeorite impacts, solar wind implantations, as well as possible inputs of ions from Earth wind, may cause significant spectral changes, and thus make the spectral interpretations difficult. The typical weathering product npFe0 can strongly darken and redden the visible and near-infrared (VNIR) reflectance spectral, and also weaken the diagnostic absorption bands. In contrast, the effects on the mid-infrared (MIR) are very limited. In our previous work (Yang et al., 2017 A&A), we have carried out pulsed laser irradiation simulations and spectral analysis. We found that the typical MIR spectral features of olivine, including the Christiansen feature (CF) which is an important index for mineralogical identification, remains even after heavily irradiation (stronger than the typical weathering process on the Moon). However, a study conducted by Lucey’s team (Lucey et al., 2016 Icarus) based on Diviner observations found that the CF position of more space-weathered lunar surface shifts to longer wavelength as compared to less weathered area. Therefore, the question arises as whether there are other processes that can cause shifts in CF? In this work, we focus on the impact process, where the instantaneous high pressure and high temperature generated during impact may induce changes in the mineral crystal structure, thereby resulting in shifts of the CF position. We conducted a thoroughly spectral analysis on samples subjected to varying degrees of impact and established a spectral index based on CF for qualitative characterization of impact degree. We will present detailed results, hopefully, it may help to better constrain the weathering process on the Moon surface.
PS11-A010
| Invited
Global Hall MHD Simulations of the Solar Wind Implantation Flux on the Lunar Surface
Lianghai XIE#+
Chinese Academy of Sciences
The solar wind can directly interact with the lunar surface and provide an important source for surface space weathering and water generation. Here we study the solar wind implantation flux on the lunar surface with global Hall MHD simulations. The shielding effects of both the Earth’s magnetosphere and lunar magnetic anomalies are considered. It is found that a large-scale lunar mini-magnetosphere can be caused by the solar wind interaction with the magnetic anomalies on the lunar far side, which causes a large shielding area on the surface. In addition, the Earth’s magnetosphere brings a longitudinal variation in the implantation flux, with minimum fluxes at 0°longitude. With the integrated flux over a lunation, we find that there are some local cavities on the implantation flux map, which are colocated with both the magnetic anomalies and the lunar swirls. Further studies show that there is a south-north asymmetry in the implantation flux, which can be used to explain the lower water content observed in the southern hemisphere. Our results provide a global map of the solar wind implantation flux on the lunar surface and are useful for evaluating the large-scale effect of solar wind implantation and sputtering on the space weathering and the water or gas generation of the surface.
PS11-A002
New Features of ENA Energy Revealed by the Chang’e-4 Mission on the Lunar Surface
Tianhua ZHONG1+, Lianghai XIE2#, Chi WANG2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences
Solar wind can directly interact with the lunar surface, and bring a space weathering effect. Some solar wind protons can be scattered as Energetic Neutral Atoms (ENAs), which include rich information of the solar wind-surface interaction. However, people still know little about the ENA truth on the lunar ground due to the lack of in situ measurements. Different from the previous in-orbit measurements, here we present the first ground-based ENA measurements by the Chang'E-4 rover, and find a good correlation between the mean ENA energy and the solar wind energy. Moreover, the loss rate of ENA energy can strongly depend on both the solar wind energy and the solar zenith angle, in which the energy loss rate can be enhanced by 73% when the solar wind energy increases from 400 eV to 1400 eV and can be reduced by 32% when the solar zenith angle increases from 57° to 71°. Combined with numerical simulations by SDTrimSP code, we propose that the solar wind protons can penetrate deeper into the lunar surface with a longer path length, when the solar wind energy is higher or the solar zenith angle is lower, which results in a larger energy loss rate for the scattered ENAs. Our results provide an important constraint for the solar wind-surface research, and have general implications in studying the surficial space weathering of the Moon and other airless bodies.
Session Chair(s):
PS09-A009
| Invited
1st, 2nd and 3rd Mercury Flyby Observations by MPPE (Mercury Plasma Particle Experiment) on BepiColombo/Mio
Yoshifumi SAITO1#+, Dominique DELCOURT2, Nicolas ANDRE3, Masafumi HIRAHARA4, Stas BARABASH5, Sae AIZAWA6, Yuki HARADA4, Lina HADID7, Kazushi ASAMURA8, Yoshifumi FUTAANA5, Takeshi TAKASHIMA8, Shoichiro YOKOTA9
1Japan Aerospace Exploration Agency / Institute of Space and Astronautical Science, 2National Centre for Scientific Research, 3University of Toulouse, 4Nagoya University, 5Swedish Institute of Space Physics, 6Laboratoire de Physique des Plasmas, 7National Centre for Scientific Research/Sorbonne Université-Ecole Polytechnique, 8Japan Aerospace Exploration Agency, 9Osaka University
Before arriving at Mercury in December 2025, BepiColombo experiences multiple Mercury flybys. The first, second, and third Mercury flybys were on 1 October 2021, 23 June 2022 and 19 June 2023, respectively. In the first, second and third flybys, the closest approach was at an altitude of about 200 km (240km for the third flyby) from Mercury's surface, and BepiColombo approached Mercury's magnetosphere from the dusk-side tail, crossed the low-altitude regions in the dawn-side southern (northern for the third flyby) hemisphere, and exited the magnetosphere in the dayside southern hemisphere. During the 1st Mercury flyby, MEA(Mercury Electron Analyzers), MIA(Mercury Ion Analyzer), HEP-ele(High Energy Particle instrument for electron) and ENA(Energetic Neutrals Analyzer) succeeded in observing energy spectra of low energy electrons and ions, high energy electrons and energetic neutrals in the Mercury magnetosphere. In particular, MEA discovered periodic precipitations of keV electrons with velocity dispersion in the midnight to dawn sectors. During the 2nd Mercury flyby, MEA, MIA, MSA(Mass Spectrum Analyzer), HEP-ele and ENA made observation of the Mercury's magnetosphere. In particular, ENA detected natural energetic neutrals from Mercury's magnetosphere for the first time. MEA discovered inverted-V like electron populations and MSA obtained mass identified ion energy spectra during part of the flyby passage in the magnetosphere. During the 3rd Mercury flyby, MSA succeeded in observing mass identified ion energy spectra during the whole period of the flyby. MIA and MSA energy spectra showed an existence of ions with energy higher than 10keV/q in the midnight to dawn sectors near closest approach. We are planning to turn on most of the MPPE analyzers during the future Mercury flybys scheduled in September 2024, December 2024 and January 2025. The observation with full performance of MPPE will start after Mio's arrival at Mercury in December 2025.
PS09-A007
Mercury’s Sodium-group Ion Escape Rates and Their Dependence on True Anomaly Angle
Weijie SUN1#+, Ryan DEWEY2, Xianzhe JIA2, Jim RAINES2, James SLAVIN2, Yuxia CHEN2, Tai PHAN3, Gangkai POH4,5, Shaosui XU3, Anna MILILLO6, Robert LILLIS3, Yoshifumi SAITO7, Stefano ORSINI6
1Space Sciences Laboratory, University of California, Berkeley, 2University of Michigan, 3University of California, Berkeley, 4NASA Goddard Space Flight Center, 5Catholic University of America, 6National Institute for Astrophysics, 7Japan Aerospace Exploration Agency / Institute of Space and Astronautical Science
Atmospheric escape, the process by which atmospheric particles, both neutral and ionized, are lost to outer space, is a fundamental scientific concept integral to the study of planetary atmospheric evolution and habitability. Despite extensive research on Venus, Earth, and Mars through in situ measurements and simulations, our understanding of atmospheric escape remains limited in the context of Mercury. This study focuses on the escape of the most abundant heavy ions at Mercury, specifically the sodium-group (Na+-group) ions. Our research reveals that the escape rates of these ions are influenced by Mercury’s orbital phase around the Sun, demonstrating a seasonal effect with rates ranging from 0.2 to 1 × 1025 atoms/s. Intriguingly, this rate is comparable to other inner planets, despite Mercury’s relatively tenuous exosphere. We hypothesize that this phenomenon can be attributed to several processes, including efficient photoionization, solar wind sputtering, and solar wind momentum exchange at Mercury. Furthermore, the Na+-group ions, as observed from MESSENGER’s in situ measurements, comprise several ion species such as sodium ion (Na+), aluminum ion (Al+), and magnesium ion (Mg+).
PS09-A003
Three-dimensional Hybrid-kinetic Simulations of the Magnetosheath Jets
Shahab FATEMI1#+, Maria HAMRIN1, Eva KRÄMER1, Herbert GUNELL1, Gabriella NORDIN1, Tomas KARLSSON2, Oleksandr GONCHAROV3
1Umeå University, 2KTH Royal Institute of Technology, 3Charles University in Prague
Magnetosheath jets are high-pressure regions that sporadically appear in Earth’s magnetosheath. These energetic entities, carrying excess energy and momentum, can significantly impact the magnetopause and disrupt the magnetosphere. Therefore, they play a crucial role in coupling the solar wind and Earth's magnetosphere. However, our understanding of the morphology and formation of these complex, transient events remains incomplete even two decades after their initial discovery. Based on oversimplified assumptions, earlier studies depicted magnetosheath jets as elongated cylinders with dimensions ranging from 0.1 RE to 5.0 RE (Earth radii). In this study, we utilize Amitis, a high-performance three-dimensional (3D in both configuration and velocity spaces) hybrid-kinetic plasma framework (particle ions and fluid electrons) running in parallel on Graphics Processing Units (GPUs). Presenting realistic scales, our study unveils the first global, 3D hybrid-kinetic simulations of the solar wind plasma interaction with Earth. These high-resolution simulations challenge the simplistic view of magnetosheath jets as cylinders. Instead, we show that the jets are intricate and interconnected structures with dynamic 3D characteristics. As these jets traverse the magnetosheath, they exhibit complex behaviors, including wrinkling, folding, merging, and splitting, before a subset reaches the magnetopause. Our findings are pivotal in advancing our understanding of magnetosheath jets and their significance in coupling between the solar wind and Earth's magnetosphere.
PS09-A012
| Invited
Recent Advancements in Understanding the Coupling Between the Solar Wind and the Magnetosphere in Near-earth Space
Kyoung-Joo HWANG#+, James BURCH, Kyunghwan DOKGO, Eunjin CHOI
Southwest Research Institute
The interaction between the solar wind and the magnetosphere drives various physical processes on the planet’s magnetopause that, in turn, are linked to the global magnetospheric and ionospheric dynamics. The primary physical processes governing the solar wind-magnetosphere coupling are magnetic reconnection and the Kelvin-Helmholtz instability (KHI). The former is triggered by large magnetic field shear, while the latter is powered by significant flow velocity shear. Both processes exhibit multi-scale features and can either compete or enhance each other. Near-Earth space serves as the most accessible laboratory for studying multi-scale physics of reconnection and KHI that is applicable to various heliospheric systems. This presentation focuses on a key advantage of geospace observations achieved by the high time-resolution dataset from MMS, with inter-spacecraft spacing down to electron scales. Recently highlighted aspects of the solar wind-magnetosphere coupling include reconnection-driven KHI and KHI-driven reconnection, leading to the development and evolution of multiple X-lines and associated solar wind mass, momentum, and energy transfer. We present our perspective on the unsolved problems, which can guide future studies on the solar wind-magnetosphere interaction in geospace, as well as throughout the heliosphere and the universe.
PS09-A010
| Invited
Mini-magnetospheric Interactions Between the Solar Wind and Mars' Crustal Magnetic Anomalies Using MAVEN Observations
Charles F. BOWERS1#+, Gina DI BRACCIO2, James SLAVIN3, Ben JOHNSTON4, Nick SCHNEIDER4, Shaosui XU5, David A. BRAIN4, Gangkai POH2,6, Abby AZARI7, Takuya HARA5
1Dublin Institute for Advanced Studies, 2NASA Goddard Space Flight Center, 3University of Michigan, 4University of Colorado Boulder, 5University of California, Berkeley, 6Catholic University of America, 7University of British Columbia
Mars possesses a unique magnetosphere in which the solar wind plasma interacts directly with both the ionospheric plasma and crustal magnetic anomalies that protrude from its surface. Due to the lack of a global, dipole magnetic field, the Martian magnetosphere largely behaves like an induced magnetosphere, whereby interplanetary magnetic field (IMF) flux tubes drape around the conducting ionosphere. However, there are regions on the surface in which the crustal magnetic fields are sufficiently strong so as to act as the primary obstacle to the solar wind flow. These crustal fields are sometimes aptly referred to as “mini-magnetospheres.” These mini-magnetospheres exhibit behavior locally that is more often associated with planets possessing intrinsic, dipole magnetic fields, such as magnetic reconnection between the draped IMF and the mini-magnetosphere connected to the surface of Mars. We present a summary of two local effects of mini-magnetospheric dynamics at Mars: magnetic flux rope formation and discrete aurora emissions. Using both electron pitch angle distributions and magnetic field data obtained from the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft, we demonstrate that magnetic flux ropes observed on the dayside of Mars possess varying magnetic topologies, suggesting they some were formed via mini-magnetospheric interactions, such as multiple X-line reconnection between the IMF and the underlying crustal anomalies. Furthermore, the ultraviolet spectrograph instrument onboard MAVEN has detailed the discrete aurora phenomenon, in which auroral emissions are detected primarily above regions of strong radial crustal magnetism. Our study shows that these auroral emissions over two mini-magnetospheres in Mars’ southern hemisphere are ultimately linked to magnetic reconnection between these crustal fields and the IMF, further demonstrating the fascinating mini-magnetospheric dynamics that take place at Mars. In summary, we present two examples of phenomena that highlight the complex interaction between the solar wind and Mars from the mini-magnetospheric point of view.
PS09-A013
Comparison of the Ionospheric Dynamo Current of Mars Above the Landing Sites of Insight and Zhurong: A Modelling Study
Hao LUO#+, Lin TIAN, Aimin DU, Yasong GE
Chinese Academy of Sciences
Previous observational studies suggest that the surface time-varying magnetic field of Mars originates in large part from the dynamo currents in the Martian ionosphere. However, whether there are significant differences in the strength, configuration, diurnal and seasonal variations of the dynamo currents above different regions need to be further studied. Here in this study, using the ionospheric parameters from Mars Data Base version 5.3 (MCD 5.3), six years of MAVEN magnetic field measurements, we model and compare the ionospheric dynamo currents above the landing sites of InSight (4.50° N, 135.62° E) and Zhurong (25.07° N, 109.90° E) and resulting surface magnetic variations at the two landing sites by conducting a modelling study. We find that the average dynamo current as well as its diurnal magnetic field amplitude on the Martian surface is slightly weaker at Zhurong than that at InSight due to the weaker magnetic field in the dynamo region. The current intensity difference between northern winter and summer is prominent at InSight than that at Zhurong. The Heliospheric distance effect-resulted plasma differences is the dominate reason for the difference at InSight while the both the Heliospheric distance and solar zenith angle (SZA) contribute the seasonal difference at Zhurong. The two factors cancelled out with each other and the current intensities is nearly the same at local summer and winter at Zhurong. This study provides a reference in an attempt to promote the understanding of the solar wind-Mars induced magnetosphere-ionosphere-Mars surface coupling process.
PS09-A011
| Invited
Global Simulations of Europa’s Plasma Interaction in Support of the Induction Experiment on the Europa Clipper Mission
Xianzhe JIA#+
University of Michigan
With a water ocean hidden underneath its icy surface, Jupiter’s moon Europa is a most intriguing target for the exploration of potentially habitable worlds. Scheduled to launch in October 2024 and arrive in the Jupiter system in 2030, NASA’s Europa Clipper mission will conduct multiple (~ 50) close flybys of Europa to investigate the moon’s habitability with its comprehensive suite of remote-sensing and in situ instruments. One of the investigations on the Clipper mission critical to characterizing the interior properties of Europa is the induction experiment, which utilizes the periodically varying magnetic fields imposed by Jupiter’s magnetosphere to perform magnetic sounding of the moon’s interior. By measuring Europa’s inductive responses at several natural frequencies, including those corresponding to the synodic and orbital periods, the Clipper induction experiment aims to determine key properties of Europa’s hydrosphere, in particular the thickness and conductivity of the subsurface ocean. However, the magnetic field in Europa’s vicinity contains not only the moon’s induced field, but also contributions from the interaction between Jupiter’s magnetospheric plasma and Europa’s atmosphere. Therefore, a crucial step in achieving the science goal of the induction experiment is to quantify and eventually separate out the plasma-produced magnetic perturbations from the measured field such that accurate measurements of the inductive response from Europa’s internal ocean can be obtained. Over the past decade, we have devoted extensive efforts to developing high-fidelity, multi-fluid magnetohydrodynamic (MHD) simulations of Europa’s plasma interaction. Our multi-fluid MHD model separately tracks different ion species originating from Jupiter’s magnetosphere and Europa’s ionosphere and incorporates key mass-loading and momentum-loading processes that arise from the interaction of Europa’s extended atmosphere with Jovian plasma. This presentation will provide an overview of the Europa Clipper mission and its planned induction experiment and describe our recent efforts on simulating Europa’s interaction with Jupiter’s magnetospheric plasma.
PS09-A002
Low Frequency Extensions of Saturn Kilometric Radiation: A Statistical View from the Entire Cassini Mission
Caitriona JACKMAN1#, Daragh HOLLMAN2, Elizabeth O'DWYER1, Alexandra FOGG1+
1Dublin Institute for Advanced Studies, 2University College Dublin
The Cassini mission spent 13 years in orbit around Saturn from mid-2004 to late-2017, and during that time was quasi-continuously measuring Saturn's radio emissions. One of the key elements of the radio spectrum at Saturn is the Saturn Kilometric Radiation (SKR), and in recent years several studies have been written on events called Low Frequency Extensions (LFEs) which represent strong, continuous extensions of the SKR down to lower frequencies. Thanks to recent work we now have a complete catalogue of LFEs observed throughout the Cassini mission. Here we explore their properties, from recurrence, to duration, to links with the ubiquitous Planetary Period Oscillations (PPOs). The results reveal LFEs as a highly useful remote diagnostic of magnetospheric dynamics at Saturn, with insights for analogous radio emissions at other planets including Earth and Jupiter.
PS01-A006
Unraveling Temporal Variabilities and Gas Dynamics in Io's Atmosphere Using the Submillimeter Array
Rong-Ting HSU1#+, Lin TING-YU2, Hui-Hui CHOU3, Yi-Shiang TZENG3, Wei-Ling TSENG1, Sheng-Yuan LIU4, Hau-Yu LIU5, Mark A. GURWELL6
1National Taiwan Normal University, Taiwan, 2National Tsing Hua University, Taiwan, 3National Central University, Taiwan, 4Academia Sinica, Taiwan, 5National Sun Yat-sen University, Taiwan, 6Center for Astrophysics | Harvard & Smithsonian, United States
The innermost Galilean satellite, Io, is known for its active volcanism as well as its essential role in shaping Jupiter’s magnetosphere. Io hosts a tenuous atmosphere, which is supported by sublimation of volcanic-origin surface SO2 deposits as well as gas species directly released from volcanic eruption (e.g., Moullet et al., 2010; Tsang et al., 2012; de Pater et al., 2020). In addition to SO2, the minor species of SO, NaCl, and KCl have been detected by SMA, IRAM NOEMA, and ALMA (e.g., Moullet et al., 2010; Roth et al., 2020; de Pater et al., 2020), though with limited temporal coverage. Here we used SMA to monitor Io’s atmosphere with a moderate observation cadence (~ weekly to bi-weekly; 9 nights in 2022-2023) to investigate the temporal variabilities and production mechanisms of its atmospheric gas species. With the advantage of SMA’s broad bandwidth, 23 SO2 lines have been detected simultaneously offering insights into gas excitation states through sophisticated atmospheric modeling and radiative transfer analysis. Investigation of the minor species is still in process.
PS01-A007
Jupiter's Post-dusk Magnetospheric Cusp
Yan XU1#+, Chris ARRIDGE2, Zhonghua YAO3, Binzheng ZHANG3, Licia RAY2, Sarah BADMAN2, William DUNN4, Robert EBERT5, Junjie CHEN3, Frederic ALLEGRINI5, William KURTH6, Tianshu QIN3, J. E. P. CONNERNEY7,8, David MCCOMAS9, Scott BOLTON5, Yong WEI10
1Southern University of Science and Technology, China, 2Lancaster University, United Kingdom, 3The University of Hong Kong, Hong Kong SAR, 4University College London, United Kingdom, 5Southwest Research Institute, United States, 6The University of Iowa, United States, 7Space Research Corporation, United States, 8NASA Goddard Space Flight Center, United States, 9Princeton University, United States, 10Chinese Academy of Sciences, China
The magnetospheric cusp connects the planetary magnetic field to interplanetary space, offering a unique opportunity for charged particles to precipitate to or escape from the planet. Terrestrial cusps are typically found near noon local time, but the characteristics of the Jovian cusp are unknown. Using datasets from multiple instruments onboard Juno, currently in a polar orbit around Jupiter, we present direct observational evidence of the Jovian cusp. Surprisingly, we discover the cusp in the post-evening sector, contradicting Earth-based predictions of a near-noon location. Nevertheless, the charged particle characteristics of the Jovian cusp are remarkably similar to those of the terrestrial and Saturnian cusp, implying similar cusp microphysics exist at different planets. These results demonstrate that while the basic physical processes may operate similar to those at Earth, the rapid rotation of Jupiter and its location in the heliosphere, can dramatically change the configuration of the cusp. This work provides significant insights towards a more complete understanding of the fundamental consequences of interactions between stars and planets.
PS01-A010
Unexpected Long-term Variations of Saturn's Ring Current Revealed by Energetic Neutral Atom Imaging
Yimeng LI1+, Chao YUE1#, Yixin SUN2, Xianzhe JIA3, Qiugang ZONG1, Xuzhi ZHOU1
1Peking University, China, 2Institute of Space Physics and Applied Technology, China, 3University of Michigan, United States
Monitoring the ring current is important for understanding the dynamical variability in planetary magnetospheres, such as acceleration and transport of the energetic charged particles. However, limited observational coverage by in-situ measurements at the outer planets makes it challenging to investigate the long-term dynamics of the global ring current. Taking advantage of the energetic neutral atom (ENA) imaging onboard the Cassini mission, we determine the long-term variations of hot plasma populations in Saturn’s global ring current. The suprathermal ring current population exhibits a clear local-time asymmetry with a nearly 11-year cycle with its peak oscillating between post-midnight and pre-midnight, while the intensity of the ring current energy content varies with a cycle of ~15 years. These results indicate that the dynamic characteristics of the suprathermal ring current population is closely related to the modulation of magnetic reconnections arising from the solar cycle and seasonal variations, among other variabilities in the inner magnetosphere. Moreover, the complex dynamics of Saturn’s ring current as revealed by our analysis offers a preview of what might be expected of the ring current at other giant planets, such as Jupiter, which will be imaged by ENA cameras onboard the JUICE mission.
PS01-A017
Numerical Simulations of Magnetic Effects on Zonal Flows in Giant Planets
Shanshan XUE, Yufeng LIN#+
Southern University of Science and Technology, China
Jupiter and Saturn exhibit alternating east-west jet streams as seen from surface. The origin of these zonal flows has been debated for decades. The high-precision gravity measurements by Juno mission and the grand finale of Cassini mission have revealed that the zonal flows observed at the surface may extend several thousand kilometres deep and stop around the transition region from molecular to metallic hydrogen, suggesting the magnetic braking effect on zonal flows. In this study, we perform a set of magnetohydrodynamic simulations in a spherical shell with radially variable electrical conductivity to investigate the interaction between magnetic fields and zonal flows. A key feature of our numerical models is that we impose a background dipole magnetic field on the anelastic rotating convection. By varying the strength of the imposed magnetic field and the vigor of convection, we investigate how the magnetic field interacts with the convective motions and the convection-driven zonal flows. Our simulations reveal that the magnetic field tends to destroy zonal flows in the metallic hydrogen and suppress zonal flows in the molecular envelope, while the magnetic field may enhance the poloidal convective motions. We extract a quantitative relation between the magnetic field strength and the amplitude of zonal flows at the surface from simulations, which roughly matches the observed magnetic field and zonal wind speed of Jupiter and Saturn. Our numerical simulations may support the scenario of deep convection-driven zonal winds which are confined to the molecular hydrogen layers in giant planets.
PS01-A018
Io Source of Heavy Ions in Jupiter’s Equatorial Ionosphere
Fran BAGENAL1#+, Vincent DOLS2, Phil VALEK3, Hunter WAITE3
1Laboratory for Atmospheric & Space Physics, University of Colorado, United States, 2University of Colorado Boulder, United States, 3Southwest Research Institute, United States
The JADE instrument on Juno has measured cold (<1 eV) heavy ions (sulfur and oxygen) in the equatorial ionosphere of Jupiter as the spacecraft made its closest approach to the planet (~3,500 km above 1 bar level), as reported by Valek et al. (2020) for 17 passes (between perijoves 6 and 23). The source of these heavy ions in Jupiter’s proton-dominated ionosphere remains unclear. The presence of sulfur and oxygen suggests they ultimately came from Io. Inward transport of plasma from the Io torus is slow and the total flux very small. Moreover, adiabatic heating would produce energetic particles reaching the equatorial ionosphere rather than cold populations. An alternative possible source could be neutral atoms that are ejected by the plasma interaction with Io’s atmosphere. We take estimates of the neutral fluxes from models of the Io plasma-atmosphere interaction and explore how the flux of neutrals reaching Jupiter depends on the ejection speed and direction. We then consider typical equatorial atmospheric conditions at Jupiter and evaluate how the incoming neutrals become cold heavy ions mixed into the ionosphere.
PS01-A020
Europa Clipper Mission Update and Preparations for Launch
Haje KORTH1#+, Robert PAPPALARDO2, Bonnie BURATTI2, Kate CRAFT1, Ingrid DAUBAR2, Samuel HOWELL2, Rachel KLIMA1, Erin LEONARD2, Alexandra MATIELLA NOVAK1, Cynthia PHILLIPS2
1Johns Hopkins University Applied Physics Laboratory, United States, 2California Institute of Technology, United States
Scheduled to launch in October 2024, NASA’s Europa Clipper will set out on a journey to explore the habitability of Jupiter’s moon Europa. At the beginning of the next decade, the spacecraft will orbit Jupiter, flying by Europa nearly 50 times over a four-year period to observe this moon’s ice shell and ocean, study its composition, investigate its geology, and search for and characterize any current activity. The mission’s science objectives will be accomplished using a highly capable suite of remote-sensing and in-situ instruments. The remote sensing payload consists of the Europa Ultraviolet Spectrograph (Europa-UVS), the Europa Imaging System (EIS), the Mapping Imaging Spectrometer for Europa (MISE), the Europa Thermal Imaging System (E-THEMIS), and the Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON). The in-situ instruments are the Europa Clipper Magnetometer (ECM), the Plasma Instrument for Magnetic Sounding (PIMS), the SUrface Dust Analyzer (SUDA), and the MAss Spectrometer for Planetary Exploration (MASPEX). Gravity and radio science will be achieved using the spacecraft's telecommunication system, and valuable scientific data will be acquired by the spacecraft’s radiation monitoring system. The assembly, testing, and launch operations (ATLO) are well underway, and the flight system integration and system-level testing has been completed at the Jet Propulsion Laboratory. The flight system and solar array have been delivered to Kennedy Space Center, where the system integration is in the process of being finalized. The launch period begins on 10 October 2024, and once lifted off, the Europa Clipper will be cruising to the Jupiter System with gravity assists by Mars followed by Earth on the way. The science team has completed the initial version of the mission’s Strategic Science Planning Guide and published a set of manuscripts describing the mission’s science and instruments.
PS01-A023
The Exospheres of the Five Main Uranian Satellites
Cesare GRAVA1#+, Ben TEOLIS1, Xianzhe JIA2, Jim RAINES2, Robert EBERT1
1Southwest Research Institute, United States, 2University of Michigan, United States
The Uranian system is one of the least explored environments in the Solar System. It was visited only once, by Voyager 2, in 1986, during a fast flyby that left us with many unanswered questions. As such, not one, but two NASA Decadal Surveys listed the Uranus Orbiter Probe (UOP) as a top-priority Flagship mission to be implemented in the upcoming decade. Its five major moons (Miranda, Ariel, Umbriel, Titania, and Oberon) are icy bodies of sizes comparable to the satellites of the gas giants (Jupiter and Saturn), and thus expected to have an exosphere (very tenuous, collisionless atmosphere) produced by sublimation (thermal desorption) and sputtering by magnetospheric ions. However, the Uranian moons are embedded in Uranus’ highly tilted magnetic field dipole. This configuration results in expected highly varying flux of precipitating magnetospheric plasma, and thus of sputtering efficiency, even during one rotation. Moreover, the large obliquity of the Uranian system means that these moons experience dramatic seasonal changes in the surface temperature, leading to transport of volatiles through the exosphere that depends upon the season. Recently, laboratory measurements of sputtering of ices, modeling of volatile transport and magnetosphere, and ground-based and space-based observations have provided valuable constraints on physical parameters, to the point that a study of the exospheres of these moons is timely and compelling. We presents results of a model that incorporates recent laboratory measurements of sputtering yields of protons on ices, ice composition measurements from telescopic observations, and novel simulations of exospheres and magnetosphere. The goal is to study how the exospheres of the five major Uranian moons change with insolation (season), orbit (plasma precipitation), and solar wind-magnetosphere interaction.
PS01-A025
Statistical Study on the Dayside Magnetic Reconnection in Jovian Magnetosphere
Jinyan ZHAO+, Ruilong GUO#
Shandong University, China
It is well-known that among the planets in the solar system, the planet with the strongest inherent magnetic field and largest-scale magnetosphere is Jupiter. Jupiter’s magnetosphere has more abundant plasma physical processes than other planets. Magnetic reconnection, an essential process in changing magnetic topology, plays a significant role in energizing charged particles. Therefore, exploring the magnetic reconnection in Jupiter’s magnetosphere is significant for understanding planetary magnetospheric dynamics. In the past, it was widely assumed that magnetic reconnection was difficult to occur in the dayside Jovian magnetosphere. Thus the related research has mainly focused on the night side of Jupiter’s magnetosphere, whether the traditional Vasyliūnas cycle or other observational or statistical studies. However, the recent discovery of dayside magnetodisk reconnection at Saturn suggests that the reconnection process might also exist in Jupiter’s dayside magnetodisk. In our study, we used data from Galileo and Voyager 2 spacecraft to identify 18 reconnection events in the range of 30-60 Jupiter radii (RJ). Due to the small amount of data, it is reasonable to infer that the occurrence rate of magnetic reconnection in the Jovian dayside magnetodisk should be significant. We analyzed the associated electron and ion fluxes, energy spectra, and characteristic energy and compared them to the nightside reconnection. The results show that the Jovian magnetodisk reconnection on the dayside appears to be equally effective in energizing particles as it is on the nightside. It means that the dayside magnetodisk reconnection might be one of the key processes for driving magnetospheric dynamics at Jupiter.
PS02-A002
TSUKUYOMI: To Realize a Low-frequency Radio Interferometer with the Maximum Baseline of Over 100 KM on the Moon
Takahiro IWATA1#+, Toru YAMADA1, Naoki ISOBE1, Yutaro SEKIMOTO1, Yasuyuki MIYAZAKI1, Naoto USAMI1, Satoru IGUCHI2, Keitaro TAKAHASHI3, Toshikazu OHNISHI4, Fuminori TSUCHIYA5, Daisuke YAMAUCHI6
1Japan Aerospace Exploration Agency, Japan, 2National Astronomical Observatory of Japan, Japan, 3Kumamoto University, Japan, 4Osaka Metropolitan University, Japan, 5Tohoku University, Japan, 6Okayama University of Science, Japan
The highly accurate observation in the lower frequency band below about 10 MHz is yet to be realized, so that this range is remarkable as one of the last frontiers for astronomy. This is mainly because that the terrestrial ionosphere prevents us from observing radio waves below the ionospheric cut-off frequency on the ground. It is, moreover, difficult to observe the faint radio waves from planets and astronomical objects even on the earth's orbit because of the interference caused by solar bursts, artificial noises and terrestrial aurora emissions. The lunar far-side is a suitable site for such the lower frequency astronomical observations because noises from the Earth can always be avoided and radio waves from the Sun can be shielded during the lunar night. One of the major targets of the astronomy on the lunar far-side is to realize the first detection of the 21-cm line of the neutral hydrogen from, so cold, the dark ages of the universe. This scientific goal can be realized by the radio interferometer with about 100 antennas of the maximum baseline of over 100 km which observe the radio frequency of 1-45 MHz. In the prototype phase, three extendable dipole antenna units will be installed. This interferometer will contribute not only to cosmology, but also to elucidation of planetary radio waves and understanding of the lunar ionosphere, dust, and subsurface structures.
PS02-A005
Outreach Activities on Planetary Sciences by the Hong Kong University and the Partners
Zhonghua YAO1#+, Jun CUI2,3, William DUNN4, Trill ZHANG5, Binzheng ZHANG1, Weiran LI1, Xiaoshu WU2, Dragon TAM5, Christopher HURLEY5
1The University of Hong Kong, Hong Kong SAR, 2Sun Yat-sen University, China, 3Chinese Academy of Sciences, China, 4University College London, United Kingdom, 5Yew Chung Yew Wah Education Network, China
Planetary sciences inherently captivate due to the enigmatic wonders they encompass. The study of planets, moons, asteroids, and other celestial bodies within our solar system and beyond prompts profound inquiries about the origins and nature of our universe. Consequently, outreach on planetary sciences is both naturally inspiring and of great importance. In collaboration with local schools and educational institutions, Hong Kong University and its partners are developing educational resources and programs to support teachers in integrating planetary sciences into their curricula. These initiatives aim to inspire the next generation of scientists, fostering a deeper understanding and appreciation of our place in the universe. Through these outreach activities, Hong Kong University and its partners are cultivating a dynamic, knowledgeable community of planetary science enthusiasts, advancing human knowledge and inspiring future generations to pursue careers in this exhilarating field.
PS03-A002
Statistical Mapping of Magnetic Topology at Venus
Shaosui XU1#+, Rudy FRAHM2, Yingjuan MA3, Janet LUHMANN1, David MITCHELL1, Moa PERSSON4
1University of California, Berkeley, United States, 2Southwest Research Institute, United States, 3University of California, Los Angeles, United States, 4Swedish Institute of Space Physics, Sweden
Despite Venus having insignificant intrinsic magnetic fields, the magnetic connectivity between the solar wind and the Venus ionosphere, or magnetic topology, is not as simple as expected and is also important for characterizing the Venus space environment. This study provides a technique combining superthermal electron energy and pitch angle distributions to infer up to 6 subtypes of magnetic topology at Venus. This enables us to determine magnetic topology with automated procedures using the Venus Express (VEx) observations from May 2006 to November 2014. We find that the draped topology (both ends of a field line not connected to the collisional ionosphere) is the dominant topology in the near-Venus space environment, >70%, except at low altitudes close to the ionosphere. The open (a field line connected to both the solar wind and the collisional ionosphere) and closed (a field line connected only to the collisional ionosphere) topologies make up 20%--30% on average of the magnetotail and up to 50% at low altitudes. This study provides the first characterization of the statistical distributions of different magnetic topologies at Venus.
PS03-A003
Whistler Mode Waves at the Moon and Mars: Implications for Terrestrial Chorus Waves
Yuki HARADA1#+, Satoshi KURITA2
1Nagoya University, Japan, 2Kyoto University, Japan
Whistler mode chorus waves have been observed for decades in the terrestrial magnetosphere. They are well known for their two distinct signatures in frequency-time spectrograms: discrete rising/falling tone elements and a power gap at half the electron cyclotron frequency. Multiple hypotheses have been proposed to explain these characteristics, and there exist ongoing debates as to what are the governing processes. Here we present whistler mode wave observations in completely different environments from the terrestrial inner magnetosphere: vicinities of the Moon and Mars. In both environments, whistler mode waves are driven by effective temperature anisotropy of electrons resulting from relatively large loss cone distributions. The loss cone distributions are caused by the reflection of perpendicular electrons from crustal magnetic fields and by the absorption of parallel electrons that impact the surface/atmosphere of the Moon/Mars. The generated whistler mode waves have been observed by THEMIS-ARTEMIS at the Moon and by MAVEN at Mars. The discrete rising tone elements have been identified for both the lunar and Martian whistler mode waves. Meanwhile, the two-band structure was observed at Mars, but an extensive search of banded waves at the Moon indicates the absence of gap formation in the lunar plasma environment surveyed by the ARTEMIS probes. We discuss these similarities and differences of whistler mode wave characteristics in a variety of plasma environments, particularly focusing on magnetic topology and associated categories of resulting wave-particle interactions. We propose that we could obtain useful and unique insights into the long-standing issues regarding the chorus wave characteristics by comparing the existing theories and terrestrial observations against new observations of whistler mode waves in these extreme plasma environments offered by the Moon and Mars.
PS03-A010
Nightside Ionospheric Structure and Composition on Mars Driven by Energetic Electron Precipitation
Shiqi WU1#+, Xiaoshu WU1, Jun CUI1,2, Yutian CAO1, Shu Xin LIAO1, Haoyu LYU3, Lei LI2
1Sun Yat-sen University, China, 2Chinese Academy of Sciences, China, 3Beihang University, China
Ionospheric chemistry plays an unexpectedly important role in the evolution of planetary habitability. This study is dedicated to a detailed modeling of the nightside Martian ionospheric structure and composition, a topic that has been poorly explored due to the absence of relevant measurements, but now becomes tractable owing to the unprecedented measurements made by the Mars Atmosphere and Volatile Evolution. Two-stream kinetic calculations and time-dependent fluid calculations are coupled to derive the nightside density profiles at 100–300 km for a large number of ion species, assuming solar wind electron precipitation as the only viable ionizing source in the ideal nonmagnetized atmosphere. Our calculations indicate the presence of a well-defined ionospheric peak at 146 km with a peak density of 8500 cm−3, as driven by the strong atmospheric “absorption” of precipitating electrons at low altitudes. The distribution of nonterminal species is roughly under chemical equilibrium below 170km, whereas for terminal species such as NO+ and HCO+, diffusion is effective at essentially all altitudes, in direct contrast to the dayside behavior. In the more realistic magnetized atmosphere, the ionospheric peak seldom exists due to the patchiness of electron precipitation. In particular, our model results agree fairly well with the MAVEN measurements, especially in view of the coincidence between electron depletion and thermal plasma void seen along many MAVEN orbits. Compared to the dayside, the nightside ionospheric composition has a much higher proportion of NO+ and lower proportion of CO2+ , likely indicative of nightside enhancement of atmospheric O and N.
PS03-A011
Asymmetric Distributions of the Low-frequency Whistler-mode Waves Within the Martian Induced Magnetosphere
Xiao MA+, Anmin TIAN#, Shichen BAI, Ruilong GUO, Mengmeng WANG, Quanqi SHI
Shandong University, China
Whistler-mode waves are a type of electromagnetic wave that widely exists in the magnetosphere of magnetized planets. However, recent studies have found that they can also be locally generated and observed in the magnetosphere of non-magnetized planets such as Mars. In the terrestrial magnetosphere, the global distribution pattern of whistler-mode waves is generally believed to be related to the magnetosphere topology. In this study, using data from MAVEN spacecraft, we find that the low-frequency whistler-mode waves in the Martian induced magnetosphere showed a special asymmetric distribution in the Mars-Solar-Electric (MSE) coordinate system. Wave instability analysis shows that the non-uniform background magnetic field and plasma density can modulate the global asymmetry of whistler-mode waves. This study reveals a new global asymmetric pattern of whistler waves within the Martian induced magnetosphere. Also, it provides new insights for the study of whistler-mode waves on non-magnetized planets.
PS04-A008
Advancing Martian Atmospheric Understanding: A 3D Global Circulation Model Based on FMS PCM
Zhixiang WAN#+, Feng DING, Yongyun HU
Peking University, China
This study presents a novel 3D Global Circulation Model (GCM) for Mars, developed using the Finite-Volume Cubed-Sphere (FMS PCM) model, to deepen our understanding of the Martian climate system. Addressing the gaps in existing models, especially in simulating CO2 ice caps, this research incorporates advanced physics modules, including CO2 phase transitions and dust-tracing capabilities. By simulating realistic Martian conditions and comparing results with observational data, significant insights into the evolution of Martian climate, polar ice cap dynamics, and atmospheric processes are provided. This model is a significant step forward in Martian climatology, offering essential groundwork for future explorations and a deeper understanding of Martian atmospheric phenomena, including dust cycles, temperature variations, and Martian paleoclimate.
PS04-A010
Characterising Exoplanet Atmospheres with Ground-based High-resolution Spectroscopy: Removal of Telluric Features Using Wavelet Analysis
Jae-Joon LEE#+
Korea Astronomy and Space Science Institute, Korea, South
The search for signs of life beyond solar system requires the detection of molecules in exoplanet atmosphere. Recent advance of high-resolution infrared spectrograph on large ground-based telescopes enabled detection of carbon monoxide and water in the atmospheres of hot giant exoplanets. The biggest obstacle in analysing high-resolution spectroscopic data from ground-based telescopes is removing the telluric features in the observed spectra, which is an imprint of Earth's own atmosphere. The often used approach is to apply Principle Component Analysis, which turned out to be working reasonably well. With very wide wavelength coverages of the recent state-of-the-art spectrographs, however, it has been common to divide the observed spectra into subsets of narrow wavelength coverage to make the problem more tractable. In this presentation, we investigate the impact of data sub setting using wavelet decomposition and discuss its effectiveness by applying the method to the observed spectra from IGRINS, infrared spectrograph onboard Gemini 8.1m telescope.
PS05-A007
Synthetic Tracking Technique for Enhanced Observation of Near-earth Objects
Chengxing ZHAI#+
The Hong Kong University of Science and Technology, Hong Kong SAR
Observing Near-Earth Objects (NEOs) plays a critical role in planetary defense efforts. The Chelyabinsk event highlighted the substantial damage caused by an about 20-meter-sized asteroid impact, emphasizing the importance of monitoring smaller asteroid threats. However, existing survey facilities, primarily focusing on asteroids larger than 100 meters, potentially allows asteroids in the 10-50 meter range to evade detection due to trailing loss caused by fast sky rates. To address this challenge, synthetic tracking (ST) emerges as a powerful technique for surveying small, fast-moving asteroids. By integrating multiple short exposure images in post-processing, ST mitigates trailing loss and enables the use of smaller telescopes for NEO observation over extended periods. In this presentation, we showcase the results of NEO observations using synthetic tracking, demonstrating the effectiveness of ST and the improved accuracy of astrometry it offers.
PS05-A008
Research of Secular Light Curves of Main-belt Comets
Jianchun SHI#+
Shanghai Astronomical Observatory, CAS, China
Main-belt comets are a new class of comets that originate in the main asteroid belt and have orbital characteristics similar to main-belt asteroids, but have coma or tails that resemble comet-like morphological characteristics. The discovery of main-belt comets means that there is still water ice in the main asteroid belt, which provides new clues for people to study the origin of water on Earth. The Secular Light Curves (SLCs) of main-belt comets reflects the brightness variation of a main-belt comet during its orbital period. The study of Secular light variation of main-belt comets is helpful for us to study the activity characteristics and activity evolution of main-belt comets. We plotted the SLCs of the nine main-belt comets discovered so far by collecting their Secular light variation data. The main conclusions include: The time and heliocentric distance corresponding to the beginning and end of the activity of comets in the main belt are asymmetrical compared with the time and heliocentric distance of perihelion. Comparing the activity changes of different regression cycles, it is found that the current activity of 238P/Read and 288P/(300163) is relatively stable; The activity of 433P increased compared to previous regression cycles; The activity of other main-belt comets decreased to different degrees compared with previous regression cycles. 133P/Elst-Pizarro and 176P/LINEAR had the aspect angle effect, which mean the nuclei of 133P/ElstPizarro and 176P/LINEAR have large obliquity and axis ratio. It can also be seen from SLC that 433P/(248370) had been active since 2010 perihelion passage, which was earlier than previously reported in 2016. 313P/Gibbs showed significant non-perihelion activity in the 2020 regression cycle.
PS05-A012
Radio Observation of Comets C/2022 E3 (ZTF) and 12P/Pons-Brooks
Juncen LI#+
Purple Mountain Observatory, China
We searched for rotational lines at 3.4mm wavelength in comet C/2022 E3 (hereafter E3), using the Purple Mountain Observatory 13.7 m radio telescope. The J = 1–0 lines of HCN were detected in E3 during the two periods of 2023 January 14–18 and February 1-3, with a beam resolution of 62.2'' and a velocity resolution of ∼0.21 km·s−1 per channel. The molecular production rates were computed. The mean HCN(1–0) production rate of 46P was (1.78 ± 0.43) × 1026 molec·s−1 and (3.78 ± 1.13) × 1025 in the above two periods, respectively. We found possible indications of time variation in the outgassing activity. The HCN line shapes gave primary information on the kinematics of the cometary atmosphere. The HCN linewidths provided a direct determination of the coma expansion velocity, which was about 0.6-1.2 km·s−1 at post-perihelion (1.1 au).Unfortunately, the J = 1–0 lines of HCO+ were not detected. Halley-type comet 12P/Pons-Brooks (hereafter 12P) has been drawing wide attention by exhibiting intriguing repetitive outbursts during every perihelion passage since its discovery. After almost 70 years, 12P is currently approaching the Sun again and has already experienced several intensive outbursts since July 2023. To investigate the mechanism of 12P’s activity, as well as the evolution of its gas and dust coma, we also observed 12P with Tianma 65m Radio telescope (TMRT).
PS05-A021
Radiogenic (87Sr/86Sr) and Stable (δ88Sr) Strontium Isotopic Composition of the HED Meteorites: Constraints on the Asteroidal Processes on Vesta
Harsh THAKUR1#+, Ramananda CHAKRABARTI1, Dwijesh RAY2
1Indian Institute of Science, India, 2Physical Research Laboratory, India
This study contributes to the understanding of the radiogenic and stable strontium isotopic compositions in HED meteorites, focusing on basaltic eucrites Lakangaon and Piplia Kalan, cumulate eucrite Vissannapeta, and howardite Lohawat. The 87Sr/86Sr ratios of Lakangaon and Piplia Kalan are reported as 0.703182 ± 2 ppm and 0.699935 ± 2 ppm, respectively, with Lakangaon exhibiting slightly higher radiogenic values, potentially influenced by its elevated silica content. Vissannapeta, a cumulate eucrite, shows an 87Sr/86Sr ratio of 0.699378 ± 3 ppm. Lohawat, a howardite, displays a more radiogenic 87Sr/86Sr ratio of 0.701617 ± 3 ppm, comparable to Vissannapeta, suggesting a need for further investigation into potential contributions from exogenous processes, fluid mobilization, or chemical complexity on Vesta's surface. The study employs Thermo Fisher Scientific Triton Plus for TIMS analysis, correcting for instrumental mass fractionation using internal normalization for 87Sr/86Sr measurements. Additionally, δ88/86Sr is determined using the Double Spike (87Sr – 84Sr) technique. The high Ni/Co ratios in Lakangaon, Piplia Kalan, and Vissannapeta suggest possible contamination by a chondritic impactor (CM/CR), highlighting the importance of analyzing these samples for insights into chondritic material mixing with achondrite parent bodies. The inclusion of Lohawat, a polymict breccia, provides an opportunity to explore mixing patterns among basaltic eucrites, cumulate eucrites, and diogenites. The preliminary data underscores the significance of silica content in influencing 87Sr/86Sr ratios, particularly in eucrites. The observed variations in δ88Sr values prompt further investigations into potential factors contributing to the radiogenic signatures, such as impacts, fluid mobilization, or surface chemical complexities on Vesta. This research enhances the database for radiogenic and stable strontium isotopic compositions, contributing valuable insights into the formation processes and history of the HED parent body (Vesta) and the broader understanding of early solar system dynamics.
PS05-A023
Impact Probability Computation of NEOs with Low Speed Encounters
Xiyun HOU1#+, Xin LIU1, Haowen CHENG2, Yao ZHANG2
1Nanjing University, China, 2National Astronomical Observatories, China
Currently, impact risk analysis of near-Earth objects (NEOs) is performed by projecting the ellipsoid of uncertainty onto the B-plane first and then calculating the impact probability based on the uncertainty ellipse projected on this plane. This way is based on the assumption of high-speed encounters between the NEO and the Earth. This assumption is valid for most NEOs, but not those with low speed encounters with the Earth or even temporarily captured by the Earth. In such a case, computing the cumulative impact probability by projecting the uncertainty ellipsoid onto a plane is no longer valid. Also, computing the instantaneous impact probability and integrating it along the close encounter trajectory may also be invalid, because the orbital dynamics of low-speed encounter is generally chaotic and assuming a linear mapping of the uncertainty ellipsoid is invalid. In this study, we will first analyze the uncertainty propagation of low speed encounters by Monte Carlo simulation to analyze how the uncertainty ellipsoid is twisted by the close-encounter. Then we will compute the impact risk of the NEOs based on the Monte Carlo simulation and compare the result with the one by assuming close-encounter as a high-speed one.
PS05-A026
WISE Observations of Outbursting Quasi-Hilda Comet P/2010 H2 (Vales)
Yoonyoung KIM#+
University of California, Los Angeles, United States
Outbursts in comets are not rare, but few have exhibited such a significant (a factor of 1000) increase as the quasi-Hilda comet P/2010 H2 (Vales). The Wide-field Infrared Survey Explorer (WISE) spacecraft imaged P/Vales, three months after its remarkable outburst on UT 2010 April 15. Dust ejecta from the outburst was detected in four infrared wavelength bands, revealing a noticeable difference in surface brightness gradient between the two thermal wavelengths (12 and 22 μm). We combined the infrared and optical data with a Monte Carlo model of dust dynamics to quantify the properties of the dust grains associated with the outburst. We found that (1) the grain albedo at solar phase angle 18.7 deg was 0.04; (2) the grain temperature was 160 K, consistent with the local isothermal blackbody temperature; (3) no strong indication of 4.6 μm band excess was present; (4) the maximum β value was determined to be 1.4; and (5) the total mass of dust ejecta was estimated to be ~10^9 kg. The outburst of P/Vales shares characteristics with similar-magnitude outbursts observed in other short-period comets, suggesting a potential similarity in their driving mechanisms.
PS05-A029
Jovian Trojan Colors: Crystalline Water Ice, Fairy Castles, and Impacts
Carey M. LISSE1#+, Audrey MARTIN2, Ian WONG3, Dina PRIALNIK4, Jordan STECKLOFF5, Yanga FERNANDEZ2
1Johns Hopkins University Applied Physics Laboratory, United States, 2University of Central Florida, United States, 3NASA Goddard Spaceflight Center, United States, 4Tel Aviv University, Israel, 5Planetary Science Institute, United States
We use the results of the New Horizons mission flyby of small KBO Arrokoth on 01 Jan 2019 (Stern+ 2019) to help interpret the nature of the Jovian Trojan asteroids (Lisse+ 2024), similar sized objects contained in two resonant orbital clouds at the L4 and L5 Lagrange points (Marzari+ 2002, Jewitt+ 2004). Specifically, we show how the information learned about the icy material making up Arrokoth and its fellow KBO and Centaur bodies (Lisse+ 2021, 2022; Steckloff+ 2021, Davidsson+ 2021), coupled with recent improved understanding of impact outcomes on small bodies (Richardson+ 2020), can help us explain why the Trojans have no water ice on their surface, two main reddish color groupings (Emery+ 2006, 2011; Brown 2016; Wong+ 2014; 2016; Jewitt 2018), and seem to have highly porous “fairy castles” on their surface (Sharkey+ 2019, Martin+ 2022, 2023). We argue from a timescale perspective that the Jovian Trojans are a large group of minor planetesimals that have evolved separately from the KBO-Centaur-Comet population. The mechanism creating the dominant two-color populations must be ongoing and recent, as the optical surfaces of the Jovian Trojans are re-worked on 100 Myr timescales via passing O/B stars, nearby supernovae, solar system passages through galactic Giant Molecular Clouds, and Galactic Cosmic Rays (Stern 2003). The most important processes acting on Kyr to Myr timescales are impacts and thermal sublimation of crystalline water ice. We show how thermophysical modeling of water ice behavior at 5.2 au in bodies of comet-like composition undergoing constant impact gardening can lead to the observed populations. We then use this thermophysical-impact modeling to make testable predictions for what the NASA LUCY mission (Levison+ 2021) should find in its upcoming flyby of six Trojans over the next decade.
PS05-A031
Surface Temperature Variations and Thermal Sublimation of (3200) Phaethon at Its Perihelion Crossing
Ian-Lin LAI#+, Wing-Huen IP, Chen-Yen HSU, Hua-Shan SHI
National Central University, Taiwan
The near-Earth asteroid (3200) Phaethon follows a highly eccentric elliptical orbit, reaching a heliocentric distance of just 0.14 AU at perihelion. During its closest approach to the Sun, Phaethon's surface temperature can exceed 1000 K which is hot enough to vaporize rock as a "rock comet." The Shape models by Hanuš et al. (2018) indicate an axis with a pole orientation at (318°, −47°) in ecliptic longitude and latitude. The significant asymmetry in surface temperature distribution on Phaethon is predominantly due to its distinctive shape combined with its axis orientation. This study aims to employ a thermal model integrated with the shape model to analyze surface temperature fluctuations and potential sublimation of surface material during perihelion to investigate the observed variations in brightness.
PS05-A032
Formation of Insoluble Organic Material from the Ultraviolet Irradiation of Laboratory Meteoritic Soluble Organic Material Analogs
Michel NUEVO1#+, Brian FERRARI2,3, David BOSWELL3, Scott A. SANDFORD1, Christopher J. BENNETT3, Yu-Jung CHEN4, Yu-Jong WU5
1NASA Ames Research Center, United States, 2Leiden Institute of Chemistry, Netherlands, 3University of Central Florida, United States, 4National Central University, Taiwan, 5National Synchrotron Radiation Research Center, Taiwan
We present results from the study of laboratory refractory organic residues which were exposed to ultraviolet (UV) photon radiation. These laboratory samples consist of mixtures of soluble organic compounds that have been detected in carbonaceous meteorites such as Murchison and Murray, and include amino acids,1,2 nucleobases,3,4 and sugar derivatives.5,6 Irradiation experiments were carried out on beamline TLS03 of the National Synchrotron Radiation Research Center (NSRRC) in Taiwan, which provides a broad-band photon beam in the 4–45-eV range with a ~1016 photons s-1 flux.7 In this study, mixtures of amino acids, nucleobases, and sugar derivatives were prepared, and exposed to UV radiation for 4, 8, 15, and 30 hours to study the evolution of their chemical and elemental compositions as a function of the radiation dose. Samples were analyzed using two independent techniques, namely, X-ray absorption spectroscopy (XAS) at the carbon, nitrogen, and oxygen edges on NSRRC’s beamline TLS20, and infrared microscopy at NASA Ames Research Center (California, USA). Results are compared with data from extraterrestrial materials,8 including meteoritic insoluble organic material (IOM), interplanetary dust particles (IDPs), and samples returned from asteroids Ryugu and Bennu by the Hayabusa2 and OSIRIS-REx missions, respectively, to understand the evolution of organic matter in environments such as the protosolar nebula.9 References: [1] Kvenvolden, K. et al., Nature, 228, 923 (1970). [2] Shock, E.L., Schulte, M.D., Cosmochim. Acta, 54, 3159 (1990). [3] Stoks, P.G., Schwartz, A., Nature, 282, 709 (1979). [4] Callahan, M.P., et al., Natl. Acad. Sci., 108, 13995 (2011). [5] Cooper, G., et al., Nature, 414, 879 (2001). [6] Furukawa, Y., et al., Natl. Acad. Sci., 116, 24440 (2019). [7] Nuevo, M., et al., Astrobiology, 14, 119 (2014). [8] Nuevo, M., et al., in preparation. [9] Ciesla, F.J., Sandford, S.A., Science, 336, 452 (2012).
PS06-A003
Development of a Terahertz Laboratory Measurement System for Future TUSKIMI Observations
Takayoshi YAMADA1#+, Hideto KANAMORI1, Makito KOBAYASHI2, Tomohiro TAKEMURA2, Hideaki MIYAMOTO2, Yasuko KASAI3,1
1National Institute of Information and Communications Technology, Japan, 2The University of Tokyo, Japan, 3NICT, Institute of Science Tokyo, Japan
The TSUKIMI (Lunar Terahertz SUrveyor for KIlometer-scale MappIng) mission aims to explore the energy resources on the global Lunar surface by passively measuring lunar radiation in the terahertz waveband (0.3 THz and 0.5 THz wavebands) from a lunar orbiting small satellite. It is essential to construct a database of terahertz wave properties of lunar soil constituents and resource materials such as water ice, in order to extract information on lunar surface soil composition from the dielectric constant estimated from the observed physical quantity, brightness temperature. In this study, we are developing a system to measure the complex permittivity and scattering coefficient of each of the above materials in the terahertz wave band, as well as the polarization and incident angle dependence. In this presentation, we will discuss the evaluation of the accuracy and precision of the obtained measurement results. Acknowledgment: This research and development includes the results achieved under "Exploration of water energy resources over a wide area on the moon using terahertz waves" (JPJ010777) within the "R & D of ICT priority technology" (JPMI00316) of the Ministry of Internal Affairs and Communications.
PS06-A005
Search for Water Vapor Signals from the Lower Thermosphere with Ground-based Observations
Paul HARTOGH#+, Borys DABROWSKI
Max Planck Institute for Solar System Research, Germany
Water vapor is photochemically rather stable in most of the middle atmosphere of the Earth and therefore frequently used as a tracer of air movements. Water vapor may be observed from satellite, airplanes & balloons as well as from ground. Ground-based observations may be performed with passive microwave spectroscopy either at 22.235 GHz or 183.310 GHz. While the 22 GHz line can be observed even from sea level at many latitudes, the observation of the 183 GHz line requires a very dry environment with low tropospheric absorption as available e.g. in very cold areas (Antarctica) or on high mountains. Vertical profiles of water vapor can be retrieved from the measured water vapor line shapes, containing altitude information through the pressure broadening of the lines. The altitude coverage of these measurements ranges from about 20 to 85 km. The upper vertical limit is given by the range where the Doppler broadening starts to exceed the pressure broadening. The amount of water vapor above 85 km altitude is usually rather low and ground-based detections of water in the lower thermosphere cannot be expected. Nevertheless, lower thermospheric water vapor was detected at 22 GHz along with Space Shuttle launches decades ago. Here we present the results of searching for lower thermosphere water vapor signals derived for three locations at 44, 55- and 72-degrees northern latitude.
PS06-A010
Experimental Analyses on Terahertz Wave Characterization of Bulk Density and Moisture Content for Lunar Simulants
Kazuma HIRAMATSU1#+, Suyun WANG1, Takayoshi YAMADA1, Yukio NAKANO2, Yasuko KASAI3,1
1National Institute of Information and Communications Technology, Japan, 2Tokyo Gakugei University, Japan, 3NICT, Institute of Science Tokyo, Japan
The Lunar Terahertz Surveyor for Kilometer-scale Mapping (TSUKIMI) mission aims to obtain global-scale observations of the brightness temperature of the Moon. In this study, we conducted preliminary Terahertz (THz) measurements on pure water, pure ice, and lunar simulant. To understand the THz characterization of the lunar regolith, we investigate probing specifications including frequency, polarization, and observation angle, as well as the effects of bulk density and soil moisture of the lunar simulants and compare them with the proposed model. The lunar simulants named FJS-1 are from the Shimizu Corporation in Japan, which refers to the Apollo lunar return samples. To prepare for the experiment, we design the different bulk densities of the lunar simulants with 1.576 g/cm3, 1.641 g/cm3, and 1.747 g/cm3, respectively, by pressing the weight of lunar simulant into a given container with a fixed volume. In addition, we prepare different water abundances of 10.03 %, 13.40 %, and 16.71 % by adding the respective water into the lunar simulants. The THz measurements of the lunar simulants with different bulk densities and water abundances were then conducted using two transceiver modules, two two-stage polarizers, and a scattering chamber ranging from 330 to 500 GHz. The initial investigations on THz characterization of the lunar simulants are readily applied to surface parameters inversion of lunar regolith with THz. Acknowledgement: This research and development includes the results achieved under "Exploration of water energy resources over a wide area on the moon using terahertz waves" (JPJ010777) within the "R & D of ICT priority technology" (JPMI00316) of the Ministry of Internal Affairs and Communications.
PS06-A013
Annual Variation of Middle Atmospheric Water Vapor from Three Latitudes
Borys DABROWSKI#+, Paul HARTOGH
Max Planck Institute for Solar System Research, Germany
MPS developed the first cooled autonomous water vapor spectrometer operating at 22 GHz in the early 1990s. This instrument was operated from 1994 to 2008 in Northern Norway. Based on the experience gained with this instrument, a new development started in 2005. This instrument is more sensitive, observes in two polarizations and included the calibration black bodies in the cryogenic dewar. A number of water vapor spectrometers based on the 2005 prototype were built from which MPS is operating three at three different locations. Recently these instruments were refurbished and a more modern operational software was created. In this presentation we show retrievals of middle atmospheric water vapor and compare the annual variations at the three locations.
PS06-A015
Microstructure-based Inversion for Regolith Physical and Structural Properties from Microwave Observations
Yuri SKOROV1,2#+, Johanna BUERGER2, Johannes MARKKANEN2, Juergen BLUM2, Paul HARTOGH1, Christian SCHUCKART2
1Max Planck Institute for Solar System Research, Germany, 2Technische Universität Braunschweig, Germany
Various studies have employed diverse computer models based on energy transport into a dense porous medium to extract information on pore size distribution and porosity as well as physical properties from microwave measurements. Thus, the estimation of dielectric properties of the material enables the inference of porous medium structure. As test samples, we consider measurements made for comet 67P with the MIRO instrument and measurements for the Moon made with the LRO/Diviner instrument. Multi-channel observations are analysed for media whose properties change with depth (e.g., ice content near the surface of a cometary nucleus).At the first stage we consider a direct problem where complex microscopic modelling is performed 1) to generate porous layers made of solid particles and porous aggregates, 2) to study the transfer of heat and radiation in such an environment, and 3) to generate synthetic brightness temperatures. The model layers have a very different structure, including cavities and cracks. Heat transfer is modelled taking into account radiative transfer in a dense porous medium, the effects of volumetric radiation absorption (the so-called solid-state greenhouse effect) and volumetric thermal emission. To estimate radiative heat transfer, we use both the geometric optics approximation and a much more complex description based on radiative transfer in a dense porous medium. The same methods are used to simulate the penetration of external optical radiation into the surface layer. To estimate radiation losses due to thermal emission, the Monte Carlo method of test particles is used for the opaque case. In the case of large aggregates with sizes larger than the thermal wavelength reflection at the interfaces between pebbles and void space between them are taken into account. Finally, we examine the sensitivity of the generated brightness temperature to changes in model parameters, intending to obtain restrictions on their values.
PS07-A004
Ion Cyclotron Waves Upstream from Mars
Jianpeng GUO#+
Beijing Normal University, China
The presence of ion cyclotron waves upstream from Mars indicates picked up ions originating from the Martian extended exosphere by the solar wind and loss of neutral atoms to interplanetary space. The occurrences and properties of proton cyclotron waves (PCWs) have been extensively investigated since their initial detection about 32 years ago, but little attention has been paid to heavy ion cyclotron wave (ICW) activity. Here we analyze whether or not ICWs can be generated near the Martian environment, and search the MAVEN date set for possible candidates for in situ signatures of ICWs upstream from Mars.
PS07-A006
Pitch-angle Scattering from Saturn's E-ring on Relativistic Electrons
Ze-Fan YIN1+, Xuzhi ZHOU1#, Yixin SUN2, Yixin HAO3
1Peking University, China, 2Institute of Space Physics and Applied Technology, China, 3Max Planck Institute for Solar System Research, Germany
The rings represent a crucial structure within the Saturnian system. Understanding the interaction between Saturn's rings and charged particles holds significant importance in comprehending Saturn's magnetospheric dynamics. The dense and larger dust within Saturn’s main rings is typically considered the absorbing source leading to particle loss, whereas the sparser and smaller dust in the outer rings is presumed to have a minor role in the dynamics of radiation belt particles. However, this understanding overlooks the angular scattering effect of Saturn's ring dust on the radiation belt particles. This study embarks on a quantitative investigation, utilizing numerical simulations and spacecraft observations, to comprehensively explore the pitch-angle scattering effect of Saturn's E-ring on radiation belt electrons. It also aims to delve into the manifestation of this angle scattering effect in spacecraft observations, thus providing a more holistic description of the role of Saturn's ring system in the dynamics of radiation belt electrons. These results would enhance our understanding and comprehension of Saturn's magnetospheric dynamics.
PS07-A009
What Controls the Dawn-dusk Asymmetry of Dayside Alfvénic Power: Interplanetary Magnetic Field or Conductance?
Shiqi FU1+, Binzheng ZHANG2, Jiuhou LEI1#, Ziyi YANG1, Tong DANG1, Xiaoli LUAN1
1University of Science and Technology of China, China, 2The University of Hong Kong, Hong Kong SAR
Alfvén waves are important carriers of solar wind energy into the Earth’s magnetosphere and ionosphere. Alfvénic energy, which has an important impact on the space environment, is observed to be more significant in the ionospheric postnoon than in the prenoon. The causes of this asymmetric Alfvénic energy distribution are explored by using global magnetohydrodynamic (MHD) simulations. We found that different-direction interplanetary magnetic field (IMF) By conditions cause the Earth's magnetic field at different locations to reconnect with the IMF and lead to different open magnetic field configurations, causing the dayside Alfvénic energy generated by magnetic reconnection to be injected into different sectors around noon along the magnetic field lines and the asymmetric dayside energy distribution. Specifically, positive IMF By conditions result in increased Alfvénic energy in the postnoon, which has been confirmed in satellite observations. The ionospheric conductance gradient was thought to cause the dayside asymmetric distribution of Alfvénic energy around noon. Controlled simulation experiments also revealed that this asymmetric distribution is not associated with conductance.
PS07-A012
The Impact Analysis of Solar Wind on the Outgassing of Cometary Material
Yong ZHAO1#+, Zhonghua YAO2
1Chinese Academy of Sciences, China, 2The University of Hong Kong, Hong Kong SAR
The stunning tails of comets are interesting astronomical phenomena to human beings and have been noticed for thousands of years. The bright tails also emit substantial materials into interplanetary space, including dusts and charged particles. The charged particles are picked up by solar wind magnetic fields, and thus could propagate together with solar wind to influence planetary space environments. In this presentation, we show the variation of cometary materials for successive days and potential influences by the solar wind during close visit.
PS07-A016
An Artificial Neural Network Proxy for the IMF at Mercury Derived from Messenger Magnetosheath Measurements
Charles F. BOWERS1#+, Caitriona JACKMAN1, Abby AZARI2, Matthew RUTALA1
1Dublin Institute for Advanced Studies, Ireland, 2University of British Columbia, Canada
This work uses machine learning techniques with an aim to address the challenge of exploring planetary solar wind-magnetosphere interactions in the absence of an upstream monitor. Mercury’s small magnetosphere is embedded in the dynamic and intense solar wind environment characteristic of the inner-heliosphere. Both the magnitude and orientation of the interplanetary magnetic field (IMF) traveling with the solar wind flow play a major role in the solar wind-magnetospheric interaction at Mercury, driving phenomena including the process of magnetic reconnection and the cycle of magnetic flux throughout the magnetosphere. The MErcury Surface, Space Environment, Geochemistry and Ranging (MESSENGER) spacecraft assessed Mercury’s plasma environment by providing in-situ magnetic field measurements of the solar wind, the magnetosheath, and the magnetosphere along each orbit. However, the nature of single-spacecraft observations makes it difficult to directly measure the impact of the IMF on the Mercury's magnetosphere due to the temporal separation between sampling of these regimes, which often exceed 3 hours. Changes in the IMF quickly reconfigure Mercury’s magnetosphere, but MESSENGER is blind to these changes downstream of the bowshock. Here, we present an artificial neural network (ANN) that estimates the strength and orientation of the IMF from the more than 250 days of magnetosheath observations obtained throughout the MESSENGER mission. The model was trained and tested on spacecraft position and magnetosheath magnetic field measurements to predict the magnitude and orientation of the IMF just upstream of the bowshock, thereby greatly increasing the temporal resolution of IMF measurements throughout the MESSENGER mission. Our results demonstrate the relational complexity between the magnetosheath and magnetosphere and are highly useful for future studies of IMF impact on Mercury’s magnetosphere using both MESSENGER data and future observations made by the BepiColombo mission.
PS07-A018
Characteristics of Compressional Waves in Jupiter's Plasmasheet Boundary Layers
Yuening CHEN1+, Shengyi YE1#, Zhonghua YAO2, Binzheng ZHANG2, Junjie CHEN2, Enhao FENG2
1Southern University of Science and Technology, China, 2The University of Hong Kong, Hong Kong SAR
Jupiter has the largest planetary magnetosphere in the solar system. Due to the angle between Jupiter's rotation axis and magnetic axis being about 10 degrees, Jupiter's high-speed rotation can lead to the formation of various complex magnetic field structures in its spatial environment, which often makes it difficult for single satellite exploration to distinguish spatiotemporal changes. The planetary aurora, as a visual optical radiation generated by magnetospheric activity, provides global images for us to understand the planetary magnetosphere, which can be used in conjunction with satellite observations to distinguish spatiotemporal changes. Previous studies have found that Jovian soft X-ray auroras exhibit periodic (~10 min) pulsations, with significant periodic differences in auroral intensity between the northern and southern hemispheres. Recent studies have revealed that the pulsations of Jovian soft X-ray arurorae are related to electromagnetic ion cyclotron waves modulated by compressional waves, but the correlation of the system has not yet been fully established. In order to investigate the reasons for the periodic changes in the intensity of Jovian aurora and to investigate whether there is a correlation between compressional waves near the current sheet region and the intensity of Jovian aurora in terms of the variation period, we try to analyze the characteristics of compressional waves in Jupiter's plasmasheet boundary layers. For this purpose, we use the magnetic field detected by Juno near the boundary of Jupiter's magnetotail plasmasheet to statistically analyze its characteristics, and preliminarily obtain some statistical results on the characteristics of compressional waves in Jupiter's plasmasheet boundary layers.
PS07-A019
Dependence of Axial Asymmetry in Jovian Magnetopause Reconnection Under Different IMF Conditions
Boding OUYANG1,2#+, Tong DANG1, Junjie CHEN3, Jiuhou LEI1, Binzheng ZHANG3
1University of Science and Technology of China, China, 2University of Leeds, United Kingdom, 3The University of Hong Kong, Hong Kong SAR
Unlike Earth, Jupiter has a peculiar and complex magnetosphere, which is unstable and has a different topology because of fast rotation. Utilizing a 3D magnetohydrodynamics(MHD) model the Grid Agnostic MHD for Extended Research Applications (GAMERA), we investigate the axial asymmetry in Jovian magnetopause reconnection under varying Interplanetary Magnetic Field (IMF) conditions. Findings reveal significant asymmetry in magnetospheric topology and separator line locations, particularly under eastward and westward IMF conditions. Northward IMF conditions present an axial symmetry about the dawn-dusk axis, while southward conditions present less evident magnetic reconnections. This has further the understanding of physical process of the magnetic reconnection between IMF and Jovian magnetosphere.
PS07-A020
Mapping of Jovian Magnetosphere-ionosphere System: Results from Three-dimensional Global Simulations
Hongyang LUO#+, Junjie CHEN, Zhonghua YAO, Binzheng ZHANG
The University of Hong Kong, Hong Kong SAR
The interaction between solar wind and planetary internal magnetic field (i.e., magnetosphere) of the earth is has been extensively studied in recent decades. By combining empirical geomagnetic field models with satellites data, such as the Tsyganenko model and THEMIS, a relatively accurate representation of the earth’s magnetosphere-ionosphere (M-I) connections can be achieved. However, for the Jovian system, the applicability of such terrestrial methodologies becomes questionable due to the limited availability of observational data, especially for the middle and outer Jovian magnetosphere. Recent numerical modeling suggests a Jovian magnetosphere with a largely closed polar cap and helical lobe magnetic field lines. This unusual magnetic topology is significantly different from earth and induces distinctive auroral morphology. This unique configuration is due to Jupiter’s fast rotation period and strong internal magnetic field, suggesting that that the mapping between ionospheric activity (e.g., aurora) and magnetospheric source region may not be as linear as our experience with earth indicates. In this study, we perform a series of three-dimensional global Magnetohydrodynamics (MHD) simulations of the Jovian magnetosphere to investigate the local time (LT) mapping between Jovian magnetosphere and ionosphere. The Jovian magnetospheric simulations use different interplanetary field orientations and both dipole and JRM33 Jupiter magnetic field model for the inner boundary M-I mapping. Results show that unlike the earth, the LT relation of the Jovian MI system is very nonlinear and north-south asymmetric. The difference between LT in the ionosphere and its magnetospheric origin increases as the magnetospheric distance from Jupiter increases (i.e., poleward of the main oval), due to rotational effect. Such feature is stronger in southern hemisphere for eastward IMF and in northern hemisphere for westward IMF. For region far away from the planet (>100Rj), the LT relation becomes unpredictable.
PS07-A022
Magnetospheric Origin of Jovian Aurora: Dawn Storms and Polar Emissions
Binzheng ZHANG#+
The University of Hong Kong, Hong Kong SAR
Jupiter has the most energetic and powerful auroral emissions in the solar system and exhibits complex morphologies that are distinct from the terrestrial aurora. The dynamic and unique features of the Jovian aurora are of particular interest, but their source and generation mechanisms are largely unknown. Combined with global-scale simulations of the Jovian magnetosphere, auroral imaging is an effective tool for remote sensing distant Jovian magnetospheric activities. In this study, we investigate the physical connection between magnetotail activities and the observed dynamic Jovian aurora signatures using global magnetosphere simulations, focusing on the magnetospheric origin of both dawn storms and polar emissions. The upward Field-aligned currents (FAC) and Alfvénic Poynting flux (S||) will be explored as proxies for monoenergetic and broadband precipitation, respectively. The morphologies of aurorae, FAC and S|| are key constraints for understanding the driving mechanisms of the observed auroral events. Preliminary simulation results have shown that FAC and S|| exhibit signatures that resemble UV auroral images of dawn storms and polar emissions, suggesting that global simulations are promising in investigating Jovian auroral activities under various upstream conditions. Synoptic diagnostics are developed to analyze the physical connections between the auroral power and magnetospheric activities. The simulation results are validated by auroral observations from both Juno and the Hubble Space Telescope and are potentially a significant contribution for the understanding of satellite measurements related to magnetospheric activities. The model results can also be used in future mission design, especially on the focus of science goals.
PS07-A023
Mirror Mode Waves in Saturn's Magnetosheath Under Dynamic Compression and Expansion Conditions
Xinya DUANMU1#+, Shengyi YE1, Zhonghua YAO2
1Southern University of Science and Technology, China, 2The University of Hong Kong, Hong Kong SAR
Mirror mode is a fundamental magnetic structure in planetary space environment, especially in the magnetosheath that is persistently compressed by solar wind. The boundary layers of Saturn's magnetosheath is in either expansion or compression state due to the interaction between the solar wind and Saturn's magnetosphere. Through the relative position change of the Cassini satellite and the magnetosheath boundary layers, the time intervals during which Saturn's magnetosheath is in dynamic compression and expansion states were clearly identified for the first time. Using magnetic field data collected by Cassini spacecraft, we classify the mirror mode waves(MMWs) as peak and dip types(Peaks and Dips) according to the magnetic morphology and discussed the distribution characteristics of mirror mode waves in Saturn's magnetosheath under dynamic compression and expansion conditions. We found that the occurrence rate of Peaks varies significantly near the magnetopause, while the occurrence rates of Dips vary little at various locations in the magnetosheath. At the same time, we also studied the impact of changes in solar wind conditions on the occurrence of MMWs. In this study, we also investigate the solar wind’s influences on wave occurrence. This study offers a new perspective on the fluctuations within Saturn's magnetosheath.
PS08-A002
Cloud Formation by Nucleation from Water Vapor Using Micrometeorites as Cloud Nuclei in the Mesosphere
Kyoko TANAKA1#+, Ingrid MANN2, Yuki KIMURA3
1Tohoku University, Japan, 2Arctic University of Norway, Norway, 3Hokkaido University, Japan
Observations of polar mesospheric clouds have revealed the presence of solid ice particles in the upper mesosphere. There are two possibilities for ice particle formation. The first is homogeneous nucleation, wherein new water nuclei are formed directly from the gaseous phase without substrate. The second is heterogeneous nucleation, which requires sufficient nuclei, such as dust grains, on which the water vapor deposits. Dust grains generated by meteor ablation are considered to serve as nuclei for heterogeneous nucleation since there is no aerosol in the mesosphere. Recently, we investigated the formation process of ice particles through nucleation from water vapor in the mesosphere (Tanaka, Mann, and Kimura, Atmos. Chem. Phys., 22,5639,2022). Previous studies used the classical nucleation theory have shown that the amorphous solid water particles can nucleate homogeneously. However, the rate predictions for water in the classical nucleation theory disagree with the experimental measurements by several orders of magnitude. We adopted a semi-phenomenological model for the nucleation process, which agrees with both experiments and molecular dynamics simulations. To calculate the nucleation process, we applied atmospheric conditions for the temperature, pressure, and cooling rate. The results indicate that homogeneous water nucleation is extremely difficult to occur in the mesosphere. If sufficient dust grains are present in the mesosphere region, most water molecules will deposit on the surfaces of the dust grains. However, if the number of dust grains is insufficient, new nuclei form; i.e., homogeneous nucleation occurs. We evaluated the competing process between homogeneous and heterogeneous nucleation and obtained the conditions required for the occurrence of heterogeneous nucleation. Our results suggest that the condensation process after meteor ablation is important.
PS08-A008
Simultaneous Meteor Plasma Observations by Radio Echoe and Optical Imaging
Shunsuke GOTO#+, Shoma ARAKI, Mari HASEGAWA, Yuji ONO, Shinsuke ABE
Nihon University, Japan
Meteor radio observations commonly rely on the "trail echo" method, capturing radio waves scattered by dense ionized columns formed along meteor paths and detected at receiving stations. The conditions for successful trail echo observations, where the positioning of transmitting and receiving stations concerning the meteor trail satisfies the angle of incidence equals angle of reflection, may not always align directly overhead for observers. Hence, establishing simultaneous observations of trail echoes and optical imaging requires a network of observations from multiple locations. This research aims to explore correlations between unexplored data obtained from meteor trail echo observations (radio echo intensity, echo duration, establishment conditions) and physical quantities related to meteors, such as atmospheric entry speed, entry angle, luminosity grade (size, mass), luminosity duration, luminosity composition, among others. The objective is to derive physical quantities solely from standalone trail echo data feasible for observations regardless of daytime, nighttime, or weather conditions. Meteor radio and optical observations were carried out using continuous radio transmission from Katsuura City, Chiba Prefecture (53.74580MHz, 50W), and receiving stations at Nihon University, and amateur stations around Tokyo area. The research focused on detecting meteors and investigating correlations through simultaneous radio and optical observations during the 2022 and 2023 Geminid, as well as the 2023 Perseids. The findings and correlations from these observations will be reported.
PS08-A011
Hypervelocity Impact Flash from H2O and Dirty Ices by Two-stage Light Gas Gan
Shotaro AKUTSU1#+, Kiyomasa KATO1, Kazuhide KOMAI1, Keita KIKUCHI1, Shinsuke ABE1, Masahisa YANAGISAWA2, Sunao HASEGAWA3
1Nihon University, Japan, 2University of Electro-Communications, Japan, 3Japan Aerospace Exploration Agency, Japan
It has been suggested that water ice may exist in craters in the permanent shadow of the Moon. The LCROSS mission impacted a part of the permanent shadow region and detected OH emissions, which is thought to be derived from water ice, from spectroscopic measurements of the impact flash. Results obtained by the LADEE spacecraft and the SOFIA infrared astronomical satellite further confirmed the presence of water on the Moon's surface. In order to compare emission and blackbody spectrum resulted from the pure water ice and dirty ice mixed with quartz glasses, spectroscopic measurements covering 300 - 800 nm wavelength region were carried out using JAXA/ISAS’s two-stage light gas gan. We will present the confirmed H2O ice related emissions such as OH and H from different ice targets.
PS11-A006
Influence of the Earthward and Tailward Flows in the Magnetotail on the Generation of the Lunar Surface Water
Huizi WANG1+, Quanqi SHI1#, Jiang ZHANG1, Chao YUE2, Lianghai XIE3, Jong-Sun PARK1, Timo PITKÄNEN1,4
1Shandong University, China, 2Peking University, China, 3Chinese Academy of Sciences, China, 4Umeå University, Sweden
Investigating the characteristics of the charged particles in the Earth’s magnetotail and the influence of them on the generation of lunar water by implantation of protons is critical for understanding the physical mechanisms for the transport of the plasma in the Earth-Moon system. When the Moon passes through the magnetotail, the tailward and earthward flows at radial distances earthward and tailward of the Moon, respectively, could be attributed to the generation of OH or H2O on the lunar surface. In this work, we estimate the proton differential energy fluxes for the earthward and tailward flow events and the time duration of these events per month observed by Acceleration, Reconnection, Turbulence, and Electrodynamics of the Moons Interaction with the Sun (ARTEMIS) satellites from January 2011 to January 2022, and use them as input parameters in the Monte Carlo model to calculate the amount of the water molecules for both flow cases. The modeling results show that the amount of water molecules produced by earthward flow events is higher than those produced by the tailward flow events. This indicates that the earthward flow-induced water molecules can stay at the lunar surface longer than the tailward flow-induced ones due to the low temperature at the lunar farside when the Moon is in the Earth’s magnetotail.
PS11-A007
Solar Wind Implantation Aids the Growth of Metallic Iron Particles in Lunar Soils: Spectral Evidence from Latitudinal Trend on the Moon
Xuejin LU+, Zongcheng LING#, Jian CHEN, Haijun CAO
Shandong University, China
Space weathering processes darken and redden the lunar reflectance spectra, suppressing the mineral absorption features. Previous researches have suggested that these spectral effects of lunar soils exhibit latitudinal and compositional variations. Nevertheless, how the spectral reddening effect varies with latitudes and composition, and the specific mechanisms are poorly understood. Multiple spectral parameters from the Kaguya Multiband Imager were derived to analyze the latitudinal spectral trend of lunar soils of various FeO contents. We analyzed the variational trend of 750- and 1550-nm reflectance with latitudes and composition. Spectroscopic evidence shows that as latitude decreases, the reflectance of lunar mature soils darkens and the spectral slope flattens. The observed spectral patterns in lunar swirls (magnetic anomalies) shares notable similarities with latitudinal spectral trends, indicating a common space weathering process controlled by the solar wind flux. We suggested that solar wind implantation may aid the coarsening process of metallic iron in mature soils and moderate the reddening effect of the spectral slope. Thus, a three-stage space weathering process was proposed: 1) rapidly weathering stage, spectral reflectance of fresh materials is reduced by space-weathering process dominated by solar wind irradiation; 2) fresh-to-mature stage, fresh materials become mature and spectra will be redder and darker with the accumulation of nanophase iron particles; 3) post-mature (or saturation) stage, some nanophase iron particles merge into larger “microphase” iron particles and moderate the spectral slopes. Such insights hold paramount importance in comprehending the spectral evolution exhibited by airless celestial bodies across the solar system.
PS11-A013
Distribution and Abundance of Solar Wind-derived Water in Lunar Soils from the Middle Latitude
Heng-Ci TIAN#+
Chinese Academy of Sciences, China
Near infrared spectral observations of the Moon show water-content increasing towards lunar poles and time-of-day variation up to 200 ppm. These features were thought to be related to solar wind implantation and (latitude-dependent) temperature-induced outgassing of H from soil surfaces. However, it is unknown whether or not the implanted solar wind-derived water can be preserved in the soils beneath the surface and the potential retention mechanisms. This question can also be raised by the large time-of-day variation of the surface water, which suggests a very fast outgassing rate. In order to explore the distributions and origins of water in the lunar regolith, it is important to analyze lunar soils from various latitudes. The lunar soils returned by Chang’e-5 mission from middle-latitude provide unique samples to probe water implantation and migration in lunar regolith and explore their correlation with latitude. We conducted a nanoSIMS-FIB-TEM combined analysis of the Chang’e-5 scooped and drill soil grains. The results shows that grain rims have high abundances of hydrogen and isotopic signatures consistent with a solar wind origin for lunar water in the soil. Hydrogen abundance varied with analysis depth in the soil grain rims, suggesting a dynamic equilibrium between the implanting of hydrogen in soil grains by the solar wind and diffusion outgassing of hydrogen at the soil grain rims. The hydrogen abundance in grain rims remained after heating, suggesting that the hydrogen could be preserved after grain burial. Comparisons with samples collected from Apollo missions showed that temperature and latitude play a key role in hydrogen implantation and preservation in lunar soil. In addition, the soil grains from drill core also have high water content on the grain surfaces, suggesting that solar wind-derived water could be preserved for hundreds of millions of years.
PS12-A004
Flux Ropes of Different Origins in the Martian Magnetotail
Lei WANG#+, Can HUANG
Chinese Academy of Sciences, China
Although current Mars has a very thin atmosphere, it is generally believed that ancient Mars had a thicker atmosphere. Ion escape plays a key role in the Martian atmosphere evolution. Based on observations in the Martian tail region by the Mars Atmosphere and Volatile EvolutioN mission, we report observations of helical magnetic structures of different origins during a single crossing of MAVEN's nightside. For the first time, we propose that tail reconnection acts as an accelerator for the ions which are brought from the dayside ionosphere. These ions can speed up in the wake region and get expelled away from Mars. Our research enhances the role of magnetic reconnection on the ion escape process of Mars, compared with the previous understanding.
PS12-A010
Analysis of Characteristic Nighttime Temperature of Potential Martian Cave Entrance Candidates
Jongil JUNG1#+, Nuri PARK2, Ik-Seon HONG3, Yu YI4, Young-Sil KWAK1, Jongdae SOHN1
1Korea Astronomy and Space Science Institute, Korea, South, 2Arizona State University, United States, 3Korea Institute of Geoscience and Mineral Resources, Korea, South, 4Chungnam National University, Korea, South
Martian caves may serve as human shelter in the future Mars explorations because they provide an environment impenetrable to cosmic rays, solar radiation and meteorites. More than 1,000 cave entrance candidates have been detected until now. however, their physical characteristics that can be exploited to detect more cave entrance candidates have not been explored in detail. Using previous research data, we explore the nighttime temperature of 100 cave entrance candidates and their surrounding areas to investigate 1) the nighttime temperature tendencies relative to their surrounding areas and 2) the extent of these temperature differences. We find that 79% of the cave entrance candidates exhibit higher temperatures than the surrounding areas, and 59% show a temperature difference over 20K, suggesting that the cave entrances may generally show higher temperatures than the surrounding areas during the nighttime. The results of these physical characteristics may contribute as parameters for detection of potential Martian caves.
PS14-A006
Modeling of the Martian Crustal Magnetic Field Using the Equivalent Source Dipole Method
Xiangfei TANG+, Yufeng LIN#
Southern University of Science and Technology, China
The contemporary magnetic field of Mars predominantly originates from the magnetized crust present on the Martian surface. The dynamo of Mars, which was responsible for the magnetization of the crust, existed in the distant past. Crustal magnetic fields record the history of the deep interior, specifically the longevity, morphology, and strength of the core dynamo. This, in turn, constrains core composition and dynamics, as well as the thermal evolution of the Martian core and mantle. Data sets collected by various spacecraft, including Mars Global Surveyor (MGS), Mars Atmosphere and Volatile Evolution (MAVEN), and Tianwen-1 missions, have sampled the Martian magnetic field within an altitude range of 90 km to 6,000 km. This has facilitated a more refined selection of data for modeling, thereby enhancing the resolution and enabling the use of modeling schemes that necessitate large volumes of data. These comprehensive models of the Martian magnetic field, which display small-scale and well-defined features, aid in establishing correlations with geological features. We present a novel model of the Martian crustal magnetic field, employing the equivalent source dipole method. The model is predicated on magnetic field data procured from the MGS and MAVEN, Tianwen-1. To mitigate the impact of the external field engendered by solar wind, data from the night side and orbits characterized by low solar wind activity were selected. The methodology employed involves the initial inversion of the radical magnetic moment, followed by the utilization of Huber weight to invert the three-direction magnetic moment. This process yields a model that exhibits convergence of the energy spectrum on the Martian surface within spherical harmonic degree 160. The spatial resolution of the new model on the surface is 133 km, corresponding to the spherical harmonic coefficient up to degree 160.
PS14-A007
Precession-driven Flows and Dynamos in Stably Stratified Planetary Cores
Rui CHENG+, Yufeng LIN#
Southern University of Science and Technology, China
Precession refers to the change of the orientation of a rotating object. Precession of celestial bodies is caused by the gravitational attraction of orbital companions. As a mechanical force, precession can destabilize the fluid motion inside fluid layers of planets, and this flow instability can provide power for the planetary dynamo. On the other hand, during the thermal evolution history of planets, due to the cooling of the planet’s core, the temperature gradient of the liquid core may be lower than the adiabatic temperature gradient. In this case, the fluid in the liquid core of the planet is in a stable stratified state, which inhibits the convection of the fluid core. This study investigates the fluid motion and the magnetic field changes inside the spherical shell under the combined action of precession and stable stratification using direct numerical simulations. By changing the strength of stable stratification, it is found that within a certain range, stable stratification can make the fluid inside the spherical shell more susceptible to instability. This instability is helpful for the generation and maintenance of magnetic fields, and helps us understand the reasons for the disappearance of magnetic fields on planets with weak core activity, such as Mars.
PS14-A010
Core-mantle Coupled Thermal Evolution of Mars
Tu ZHIYI#+, Yufeng LIN
Southern University of Science and Technology, China
The existence of a dynamo and the magnetic field strength are strongly dependent on the heat transfer rate through the mantle of the planet, which is calculated as a time-dependent function from the planetary thermal evolution model. Therefore, it is of great significance to study the thermal evolution of terrestrial planets to understand their magnetic field generation and evolution. Comparing the Earth with other terrestrial planets, the most striking difference is the state of the surface and the way heat is transported. The surfaces of other planets are not segmented but consist of a single plate, the so-called stagnant lid. Mars, at present, is a one-plate planet in which heat is generated by radioactive decay and transported to the surface by heat conduction through a single plate lying on top of a convecting mantle. Some evidence show that early Mars might had plate tectonics, so two kinds of thermal evolution models have been developed to study the effects of the two regimes. We constructed a 1-D parameterized convection model of the mantle consisting of a stagnant lid or plate tectonic regime, and then particularly emphasis on temperature differentials, variations in heat flow, and the evolution of stagnant lid thickness. Furthermore, an evaluation of the current state of the Martian core is conducted through a comparative assessment with the melting temperature curve specific to Mars. The model results show that a stagnant lid can indeed play a role of "insulation" for planets to a certain extent compared with plate tectonics.
PS15-A011
Searching Exoplanet Transits Through Machine Learning Techniques
Li-Chin YEH#+, Ing-Guey JIANG
National Tsing Hua University, Taiwan
Due to the availability of high-performance computers and the data release from big-scale sky survey projects, the machine learning has been employed in various fields in astronomy. We have developed a procedure of machine learning to search for exoplanet transits from several survey data. Our procedure employs the convolutional neural network (CNN) of deep learning techniques. Both 1D-CNN and 2D-CNN with different training processes are used and compared. The details of the procedure and the results will be presented.
PS15-A017
The Evolution of Ultra-short-period Planets
Peiwei TU#+, Ji-Wei XIE
Nanjing University, China
The recent discovery of exoplanets have revealed a special populations with orbital periods shorter than one day, also known as ultra-short-period (USP) planets, whose origin remains puzzling. Determining their age distribution and temporal evolution is vital for uncovering the secrets of their formation and evolution. With a sample of more than a thousand hot planets around Sun-like stars and kinematic methods from the Planets Across Space and Time (PAST) project, we present a detailed comparison of the characteristics of USP planets and their host stars with those of other hot planets (P < 10 days) and their host stars. The results of such comparison study can put important constraints on the formation mechanisms of USP planets.
PS15-A031
Current Status of Korea Microlensing Telescope Network
Chung-Uk LEE#+, Seung-Lee KIM, Dong-Joo LEE, Dong-Jin KIM, Sang-Mok CHA, Yongseok LEE, Sang-Min LEE, Hyun-Woo KANG, Chang Hee REE, Min-Su SHIN, Moo-Young CHUN, Jae-Woo KIM, Sungwook E HONG, Seung-Cheol BANG, Hong-Soo PARK
Korea Astronomy and Space Science Institute, Korea, South
Korea Astronomy and Space Science Institute has installed three identical 1.6-m telescopes and 340 M-pixel mosaic CCD cameras in Chile, South Africa, and Australia to search for exoplanets using the microlensing method. Korea Microlensing Telescope Network (KMTNet) officially started observation in October 2015. Based on the analysis of high-cadence photometric data obtained over eight years, a total of 186 exoplanets have been discovered so far. This accounts for 70% of 263 exoplanets found by the microlensing method over 20 years. 40% of the total observation time is used to observe the Galactic bulge. The remaining observation time is used for other research topics selected through panel reviews, such as supernovae, asteroids, external galaxies, etc. The observation system, the research achievements, and the future system upgrade plan are presented.
PS15-A032
Planets Across Space and Time (Introducing the PAST Project)
Ji-Wei XIE#+
Nanjing University, China
With over 5000 exoplanets discovered in the last decades, the map of known exoplanets has expanded significantly from the solar neighborhood (100-200 pc) to a much larger area (orders of 1000 pc) in the Galaxy thanks to the improvement of observational technology. We are therefore entering a new era of exoplanet census in the Milky Way Galaxy. In the Galactic context, one of fundamental questions in studying exoplanets is: what are the differences in the properties of planetary systems at different positions in the Galaxy with different ages? The answer to this question will provide insights on the formation and evolution of the ubiquitous and diverse exoplanets in different Galactic environments. To address this question, we conduct a research project, dubbed Planets Across Space and Time (PAST). In this presentation, we introduce recent progresses of the PAST project.
PS15-A033
Transmission Spectroscopy of Exoplanet Systems HD 189733 b and Qatar-8 b
Yeon-Ho CHOI1#+, Byeong-Cheol LEE1, Myeong-Gu PARK2, Tae-Yang BANG2, Jae-Rim KOO3, Kang-Min KIM1
1Korea Astronomy and Space Science Institute, Korea, South, 2Kyungpook National University, Korea, South, 3Kongju National University, Korea, South
SPECtrophotometer for TRansmission spectroscopy of exoplanets is a low-resolution optical spectrograph installed at Bohyunsan Optical Astronomy Observatory 1.8m telescope. Transmission spectroscopy provides insights into the atmospheric structure of exoplanets by observing their transits with a spectrograph. SPECTR is a highly efficient instrument that is designed to obtain the transmission spectra of transiting exoplanets in a wavelength range of 380 to 685 nm. SPECTR’s wide slit length of 10 arcmins makes it easy to find comparison stars that are close to the target within the same field of view. SPECTR will be used to survey exoplanets detected by Transiting Exoplanet Survey Satellite (TESS), providing useful insights into their radii across the wavelength range. Here, we will present a summary of the design and systemic performance of SPECTR.
PS16-A002
Lunarleaper – Unlocking a Subsurface World
Simon STAEHLER1#+, Anna MITTELHOLZ1, Hendrik KOLVENBACH1, Valentin T. BICKEL2, Joseph CHURCH1, Sven-Erik HAMRAN3, Ozgur KARATEKIN4, Birgit RITTER4, Jordan AARON1, Sofia COLOMA5, Matthias GROTT6, Larissa DE PALÉZIEUX DIT FALCONNET1, Johan ROBERTSSON1, Krzysztof WALAS7
1ETH Zurich, Switzerland, 2University of Bern, Switzerland, 3University of Oslo, Norway, 4Royal Observatory of Belgium, Belgium, 5University of Luxembourg, Luxembourg, 6German Aerospace Center, Germany, 7Poznan University of Technology, Poland
We present LunarLeaper, a robotic explorer concept in response to the ESA 2023 Small Missions call. Pits, volcanic collapse features with near-vertical walls, have been identified across the lunar and Martian surface. These pits are high priority exploration destinations because some, referred to as skylights, might provide access to subsurface lava tube systems. Lava tubes are of particular interest for future human exploration as they offer protection from harmful radiation, micrometeorites and provide temperate and more stable thermal environments compared to the lunar surface. We propose to use a small legged robot (ETH SpaceHopper, <10 kg, 12U), to access and investigate the pit edge, using its ability to access complex and steep terrain more safely than a wheeled rover. LunarLeaper will be deployed in Marius Hills near the pit and traverse across the lateral extent of the hypothesized subsurface lava tube. On its traverse it will take measurements with a ground penetrating radar and a gravimeter, measurements that will allow us to survey the subsurface structure and detect and map lava tube geometry if present. The robot will approach the pit edges and acquire high resolution images of the pit walls containing uniquely exposed layers of the lava flows and regolith layers. These images will allow not only scientific advances of lunar volcanism and regolith formation, but also enable assessment of the stability of the pit structure and its use as a possible lunar base. The mission is expected to last 1 lunar day. The robot could be delivered to the surface by a small lander, as they are currently developed and planned by various national and commercial agencies and hop off the landing platform without the need for a robotic arm. It is highly flexible in accommodation and can thus make full use of the new international lunar ecosystem.
PS16-A005
Cave Network Exploration Beneath Pit Cluster on the Moon by Using Grail
Ik-Seon HONG1#+, Kyeong Ja KIM1, Yu YI2
1Korea Institute of Geoscience and Mineral Resources, Korea, South, 2Chungnam National University, Korea, South
The lunar lava tubes are the perfect place to build a lunar base. It can protect humans from external factors such as cosmic rays, radiation, impact, temperature, and floating dust. Since the pit was first discovered in 2009, two hundred pits have been reported. Previous studies mainly focused on finding large-scale lava tubes. We propose a cave network as a new idea. Terrestrial lava tubes also form a network like an anthill, so they can be fully applied to the moon. Therefore, gravity exploration was performed for areas where impact melts pit clusters were considered to have a high possibility of a cave network. We analyze Bouguer gravity gradients from GRAIL data. We detect mass deficit signals in the pit cluster region on Copernicus, King, Stevinus, and Tycho. This result has limitations that can't strongly support the existence of a cave network underneath the pit cluster. Because the source of the mass deficit signal can be several, such as mantle subsidence or the presence of a low-density mass. Our results add one more to the existence of a cave network in these multiple elements. Therefore, the mass deficit signal in the pit cluster region suggests the possibility of a cave network.
PS16-A007
After Landing Calibration of SLIM’s Multi-band Camera (MBC) for Science Observation
Yusuke NAKAUCHI1#+, Kazuto SAIKI2, Makiko OHTAKE3, Masaki NISHINO4, Hiroshi NAGAOKA1, Yoshiaki ISHIHARA4, Hiroyuki SATO4, Chikatoshi HONDA5, Risa MIYAZAKI4, Iori KAJITANI4, Ryusuke NISHITANI4, Shin-Ichiro SAKAI4, Shujiro SAWAI4, Seisuke FUKUDA4, Kenichi KUSHIKI4
1Ritsumeikan University, Japan, 2Ritsumekan University, Japan, 3Okayama University, Japan, 4Japan Aerospace Exploration Agency, Japan, 5The University of Aizu, Japan
The Smart Lander for Investigating Moon (SLIM) spacecraft, launched by the Japan Aerospace Exploration Agency on September 7th, is scheduled for a "pin-point landing" on the Moon around the SHIOLI crater on January 20th. The landing site is chosen based on the likelihood of exposed mantle material observed by the "Kaguya" mission. The Multi-Band Camera (MBC) onboard SLIM is crucial for observing ejecta from the SHIOLI crater and estimating the Mg# (Mg / (Mg + Fe) atomic ratio) of lunar mantle materials. The MBC is a compact VIS-NIR camera with a Xenics VIS-IR sensor, 10 band-pass filters, a telephoto focusable optical system, and a movable mirror for panning and tilting. Preflight calibration involved using a barium sulfate integrating sphere in a clean and dark room at JAXA to obtain optical calibration data. The sensitivity, linearity, and stray light characteristics were investigated. The R2s of linearity line fitted against input light intensity, exposure time, and detector temperature were over 0.98, which is expected to obtain a calibration equation with 0.1 % accuracy. The stray light from outside of iFOV was less than 0.3 %. In-flight calibration included observing the Earth, the Moon, and deep space data from orbit. Lunar observations were conducted at different locations, with a spatial resolution of ~500 m/pixel and a phase angle of 65-90 degrees. The successful operation of the MBC's auto exposure (AE) function was confirmed during lunar observation. After pin-point landing, we will start scientific observations using MBC around the landing site. To improve the quality of scientific data, we are planning to observe InfraGold mounted on SLIM using MBC and obtain calibration data for all observable wavelength.
PS16-A019
Sample Return Mission Concepts of Purest Anorthosite (PAN) in the Primordial Lunar Crust and Impact-melt Rock from the Large Impact Basin on the Moon
Hiroshi NAGAOKA1#+, Tomokatsu MOROTA2, Makiko OHTAKE3, Yusuke NAKAUCHI1, Yuichiro CHO2, Seiji SUGITA2, Haruhisa TABATA2, Risa MIYAZAKI4, Mari AIDA4, Kasumi YOGATA4, Kazuto SAIKI5, Tetsuo YOSHIMITSU4, Osamu MORI4, Takanao SAIKI4
1Ritsumeikan University, Japan, 2The University of Tokyo, Japan, 3Okayama University, Japan, 4Japan Aerospace Exploration Agency, Japan, 5Ritsumekan University, Japan
The opportunity to advance key science of the Moon, promoted by the ARTEMIS program, will provide sample return mission. Our scientific objectives focus on the following two topics: 1) Constraints on lunar formation conditions leading the origin of Earth-Moon system, by verifying the lunar magma ocean (LMO) model [e.g., Warren 1985], and determining bulk silicate moon composition; 2) Reconstruction of impact history in the early solar system and verification of the late heavy bombardment hypothesis associated with giant planet migration model [e.g., Gomes et al. 2005]. We discuss these scientific importance, sampling sites of these sample, and the sample selection system using in-situ analysis instruments, in the case of robotic and/or human exploration. The purest anorthosite (PAN) consisting of more than 98% plagioclase, was widely observed on the lunar surface (Ohtake et al. 2009). The PAN outcrops observed at central peaks of large craters uplifted from a deep-seated layer, are very important sample to provide a key information of the primordial crust, which may be directly crystallized from LMO, because the surface crust has been brecciated by mixing and recrystallizing of numerous impact events (Nagaoka et al. 2023). We aim to access and return the fresh PAN rock recently fallen from the PAN outcrop of the central peak. Key information on the impact history in the solar system is provided by lunar cratering records. To understand the bombardment history before 3.8 billion years ago, formation ages of impact basins are important [Ryder 2022]. Their absolute ages are poorly determined yet, although the stratigraphic relationship, crater densities, and its topographic degradation states have derived their relative ages [Wilhelms, 1987]. Therefore, sample return of the impact melt rocks generated by the basin-forming impact is required to verify the late heavy bombardment hypothesis and reconstruct impact history in the early solar system.
PS16-A028
Updates on Mini-RF Operations, Data, and Applicability to Artemis Landing Zone Characterization
Angela STICKLE1#+, Wes PATTERSON1, Gareth MORGAN2
1Johns Hopkins University Applied Physics Laboratory, United States, 2Planetary Science Institute, United States
NASA’s Mini-RF instrument on the Lunar Reconnaissance Orbiter (LRO) is a hybrid-polarized, dual-frequency synthetic aperture radar (SAR) that operates at S- (12.6 cm) and X/C-band (4.2 cm). Mini-RF initially operated as a monostatic system, with the majority of data collected at S-band covering >95% of the poles. Controlled mosaics of derived Stokes products for both poles have been produced by the USGS and provide access to permanently shadowed regions (PSRs) at a resolution of 30 m. A transmitter anomaly led to Mini-RF transitioning to a bistatic architecture – i.e., transmitting from Arecibo Observatory (AO) or the Goldstone deep space communications complex antenna DSS-13 and receiving at the LRO spacecraft. Bistatic observations can target the Earth-facing portions of the south polar region. Although Mini-RF is not currently collecting S-band bistatic data, X-band acquisition is ongoing to address a variety of LRO science objectives. Bistatic data includes both S- and X-band observations and has a processed resolution of ~100 m in range and 2 m in azimuth. Mini-RF data provide unique and valuable insights for landing site characterization, the structure and properties of the lunar surface and shallow subsurface, and the potential presence of water ice in lunar regolith. Radar data characterize wavelength-scale scatterers (e.g., size-frequency distribution, morphology), provide insights into subsurface structure, and constrains bulk density and composition (i.e., dielectric permittivity); these are relevant for characterizing landing hazards, ensuring effective use of descent radar altimeter systems in the future, and providing insights for scientific exploration. The continued operation of Mini-RF in orbit around the Moon provides unique capabilities for measuring these properties and addressing science and engineering objectives of the Artemis and CLPS programs. We will present the rich array of radar coverage of the Artemis III zones and provide insights into landing safety and regions of scientific interest.
PS16-A030
Lunar Trailblazer: A Pioneering Smallsat for Lunar Water, Geology, and Landing Site Reconnaissance
Rachel KLIMA1#, Bethany EHLMANN2, Neil BOWLES3, Diana BLANEY2, Kerri DONALDSON HANNA4, Christopher EDWARDS5, Robert GREEN2, Carle PIETERS6, David THOMPSON2, Jasper MIURA2, Martha HOUSE7, James DICKSON2, Bea CHIKANI3+
1Johns Hopkins University Applied Physics Laboratory, United States, 2California Institute of Technology, United States, 3University of Oxford, United Kingdom, 4University of Central Florida, United States, 5Northern Arizona University, United States, 6Brown University, United States, 7Pasadena City College, United States
Lunar Trailblazer is a NASA SIMPLEx small satellite science mission for understanding the Moon’s water and water cycle. Selected in June 2019, Lunar Trailblazer is presently in assembly, on track to launch as a secondary payload on the Intuitive Machines IM-2 lander launch with SpaceX, scheduled for 2024. Identifying water, determining its form and abundance, and mapping the distribution of water ice and geologic units at <100m spatial scales relevant to robotic and human exploration provide critical knowledge for future lunar surface exploration. Trailblazer simultaneously measures composition, temperature, and thermophysical properties from a lunar polar orbit at high spatial and spectral resolution over select areas of the Moon. The objectives are to detect and map water on the Moon at key targets to (1) determine its form (OH, H2O or ice), abundance, and local distribution as a function of latitude, soil maturity, and lithology on the sunlit Moon; (2) assess possible time-variation in lunar water on sunlit surfaces; (3) use terrain-scattered light to determine the form, abundance, and distribution of exposed water in permanently shadowed regions; and (4) collect thermal data to understand how local albedo and surface temperature gradients affect ice and OH/H2O concentration, including the potential identification of new cold traps. Trailblazer will perform the highest-to-date spatial resolution compositional and thermophysical properties mapping at the Moon and conduct reconnaissance of potential future landing sites. Lunar Trailblazer’s international team is led by Caltech and managed by JPL. A Lockheed Martin-built and integrated ~200 kg smallsat carries two instruments: (1) JPL’s High-resolution Volatiles and Minerals Moon Mapper SWIR imaging spectrometer (<70 m/pixel, 0.6-3.6 μm, 10 nm spectral resolution) and (2) the UK-contributed, University of Oxford-built Lunar Thermal Mapper multispectral thermal imager (<50 m/pixel, 4 broadband thermal channels 6-100 μm, 11 compositional channels 7-10 μm).
PS16-A032
Volatile Composition of Volcanically Sourced Lunar Ice Deposits
Andrew WILCOSKI1#+, Catherine ELDER1, Margaret LANDIS2, Paul HAYNE2
1California Institute of Technology, United States, 2University of Colorado Boulder, United States
Water ice exists at the lunar poles, but the origins and compositions of ice deposits are not well understood (Lucey et al., 2022). Determining the source and composition of ice deposits is key to understanding the history of water in the solar system and the utility of these deposits as resources for lunar exploration. The composition of non-water volatiles within a deposit has been suggested as a useful metric in determining deposit origin (e.g., Mandt et al., 2022). However, volatile species may undergo several fractionating processes as they migrate from their sources to polar cold traps, resulting in ice compositions that differ significantly from source compositions. Before composition can be used as an indicator of ice origin, the amount of fractionation expected between sources and polar cold traps must be quantified. We investigate the expected composition of ice sourced from volcanic outgassing during the Moon’s most volcanically active period (4-2 Ga, Head et al., 2020). We build on previous work (Wilcoski et al., 2022) to model the atmospheric escape and temperature-dependent cold-trapping of volatile species released over 50,000 eruptions. Each eruption creates a transient collisional atmosphere primarily composed of CO but also containing H2O and several different sulfur species (e.g., SO2, H2S, S2, COS, CS2, and H2S2). We explore model behavior under several different assumptions of the composition and concentration of species outgassed. The model shows that many of these sulfur species condense as ice in cold traps. However, the composition and degree of fractionation within each deposit strongly depends on cold trap temperature. The warmest cold traps only sequester water ice, while sulfur species are concentrated in the coldest. Significant atmospheric escape of water decreases the accumulated water fraction relative to the source. These and other factors create ice deposits with compositions significantly different from those of their source.
PS17-A016
The Potential Drivers for Jupiter’s X-ray Auroral Pulsations
Zhonghua YAO1#+, William DUNN2
1The University of Hong Kong, Hong Kong SAR, 2University College London, United Kingdom
Jupiter’s rapidly rotating, strong magnetic field provides a natural laboratory that is key to understanding the dynamics of high-energy plasmas. Spectacular auroral x-ray flares are diagnostic of the most energetic processes governing magnetospheres but seemingly unique to Jupiter. The simultaneous in situ satellite and space-based telescope observations that reveal the processes that produce Jupiter’s x-ray flares, showing surprising similarities to terrestrial ion aurora. Electromagnetic waves are observed to modulate electromagnetic ion cyclotron waves, periodically causing heavy ions to precipitate and produce Jupiter’s x-ray pulses. The connection between X-ray pulsations with other types of waves (or pulsations) are crucial information to understand the whole physical story for X-ray auroral pulsations.
PS18-A009
Pressure Induced Structural Phase Transition in Quasi-two-dimensional Cu-based Organic-inorganic Hybrid Perovskite
Myeong Jun KANG1+, Min Jae KIM1, Young Jay RYU2, Soomin PARK3, Vitali PRAKAPENKA2, Yanbin WANG2, Jaeyong KIM3, Jong Mok OK1#
1Pusan National University, Korea, South, 2The University of Chicago, United States, 3Hanyang University, Korea, South
Organic-inorganic hybrid perovskites (OIHPs) are materials that can modulate the dimensionality of their inorganic octahedral based on the composition of organic molecular layer. These materials have garnered significant attention in recent years due to their positive environmental impact. In order to properly evaluate the progress made in this field, it is imperative to investigate the physical and chemical properties that emerge from the transition between three- and zero-dimensional states within OIHPs. As such, OIHPs represent an ideal platform to understand the fundamental physics underlying these intriguing materials. Practically, Phenylethylamine (C6H5CH2CH2NH3, PEA) based PEA2CuCl4 is a quasi-two-dimensional structure due to the length of the PEA molecule. It exhibits unique characteristics, including two-dimensional Heisenberg ferromagnetism, abnormal d-d transition absorption, and ferroelectricity. Our study aims to explore the pressure-dependent change in the properties of PEA2CuCl4. We conducted pressure-based Raman spectroscopy to examine the possible changes in physical properties due to structural phase transitions and/or microstructural changes. At 5~7 GPa, the structural phase transition induces a modification to the structure of the CuCl42- octahedron, transitioning from D4h to Oh symmetry, effectively inhibiting the Jahn-Teller distortion. The suppression of the d-d transition eliminates abnormal absorption, leading to a decrease in the bandgap. Furthermore, this suppression led to the loss of ordered hole orbital states, which could potentially lead to a decrease in the magnetic moment in PEA2CuCl4. After applying a pressure of 20 GPa, the organic layer is compressed, leading to another structural phase transition, where the octahedral layers phase into a repeating structure. Consequently, the material loses its two-dimensional nature and may observe changes or loss in various physical properties. In this presentation, we will highlight the effect of pressure on various physical properties which can offer a promising opportunity to develop next generation of eco-friendly spintronic and magnonic devices.
PS18-A010
Equation of State for Ti45Zr27Ni20Si8 Metallic Glass at High-pressure Using Brillouin Scattering
Soomin PARK1+, Jong Mok OK2, Young Jay RYU3, Min Jae KIM2, Myeong Jun KANG2, Vitali PRAKAPENKA3, Yanbin WANG3, Jaeyong KIM1#
1Hanyang University, Korea, South, 2Pusan National University, Korea, South, 3The University of Chicago, United States
Understanding of amorphous materials is important because of their superior physical properties such as high hardness, wear resistance, low thermal expansion coefficient, as well as excellent electrical and magnetic properties. Due to the lack of the periodic atomic arrangement in metallic glasses curtails the depth of structural and mechanical information. TiZrNiSi metallic glass is an examplar that shares structural similarity with amorphous, quasi-crystal, and crystalline materials formed with the same elements. To investigate the liquid state of the materials in the deep Earth’s core, Ti45Zr27Ni20Si8 metallic glasses were prepared by rapidly quenching the molten ingot in an Ar atmosphere. The absence of crystalline was confirmed by analyzing X-ray diffraction after which a small piece of the sample was loaded onto a 200 μm-sized diamond anvil cell. In this study, the physical and chemical properties of the Ti45Zr27Ni20Si8 metallic glass were investigated up to 50 GPa. Brillouin scattering technique was employed to derive the equation of state of the Ti45Zr27Ni20Si8 metallic glasses with increasing pressure to 50 GPa. The frequency variations of the transverse acoustic (TA) and longitudinal acoustic (LA) modes were estimated by measuring the Brillouin shift (GHz). Additionally, to complement the Brillouin scattering results, Raman spectroscopy was conducted to probe a diverse range of interactions among cation groups at THz frequencies. This additional spectroscopic technique provided valuable insights into the vibrational dynamics and structural changes induced by pressure, enhancing our understanding of the physical and chemical properties of the Ti45Zr27Ni20Si8 metallic glass. The study explored various mechanical properties, including isothermal bulk modulus, elastic coefficients, and the pressure-density relationship under ambient conditions. These results hold potential applications in diverse fields, such as materials science, manufacturing, and environmental engineering. And the results will be presented.
PS18-A012
Spectroscopic Evidence of Cation Medium-range Order in MgSiO3 and CaSiO3 Melts and Glasses
Young Jay RYU1#+, Yanbin WANG1, Tony YU1, Stella CHARITON1, Vitali PRAKAPENKA1, Nicolas GUIGNOT2, Andrew KING2, Laura HENRY2, Peter ENG1, Joanne STUBBS1, Mark RIVERS1
1The University of Chicago, United States, 2Synchrotron Soleil, France
Chemical and physical differentiation processes in the early history of Earth and other terrestrial planets were largely determined by the properties of silicate melts, such as density, elasticity, viscosity, elemental diffusivity, and partition coefficients between melts and solids. All of these properties are primarily controlled by the structure of the melts. Studies of evolution in the structural, elastic, and/or inelastic properties of silicate melts give critical constraints on the differentiation processes. Although there has been increasing number of theoretical and experimental studies, data corresponding to the actual conditions of the Earth’s deep interior are scarce, and quantitative determination of silicate coordination in melts and glasses remains a challenge. In this presentation, we first report the structural evolution of enstatite (MgSiO3) and wollastonite (CaSiO3) glasses up to 70 GPa using a combination of experimental techniques, including Raman and Brillouin spectroscopy as well as synchrotron X-ray diffraction. With increasing pressure, Raman vibrational modes of MgSiO3 and CaSiO3 reveal gradual modifications in the interconnectivity of the tetrahedral SiO4 network and change in coordination, resulting in several structural modifications at ~5, 20, and above 43 GPa. These changes are further corroborated by both Brillouin spectroscopy and X-ray diffraction results. Additionally, we report the structural evolution of MgSiO3 and CaSiO3 melts up to 12 GPa (~3000 K) measured in a Paris Edinburgh press. Structural evolution in silicate melts in the Earth’s deep interior will be discussed based on the combined glass and melt dataset.
PS18-A013
Large-volume High-pressure Research at GSECARS Beamlines, Advanced Photon Source
Tony YU#+, Young Jay RYU, Timothy OFFICER, Man XU, Vitali PRAKAPENKA, Stella CHARITON, Peter ENG, Joanne STUBBS, Mark RIVERS, Steve SUTTON, Yanbin WANG
The University of Chicago, United States
The development of synchrotron X-ray-based large-volume high-pressure techniques for studying earth, planetary, and other materials under extreme pressure and temperature (PT) conditions has been an ongoing effort at the GeoSoilEnviroCARS (GSECARS) beamlines of the Advanced Photon Source (APS) at the Argonne National Laboratory. Over nearly 30 years, these developments have provided users with state-of-the-art experimental setups and techniques to conduct coordinated research on materials in both the solid and liquid states. In this presentation we will demonstrate our latest techniques and their applications to tackle complex scientific questions: (1) 3D imaging of composite materials using the high-pressure X-ray tomographic microscope, (2) high PT ultrasonic velocity measurements on solids and liquids, (3) rheological properties of materials and acoustic emission monitoring at high PT, and (4) structure studies of non-crystalline materials using a Paris-Edinburgh Press combined with a multi-channel collimator. These techniques have provided the high-pressure community with a complete suite of tools for structure, density, elasticity, and viscosity measurements of various materials.
PS18-A014
Melting of Iron-bearing Bridgmanite: Implications for the Internal Structure of Super-earths
Donghoon KIM1#+, Sota TAKAGI2, Sally TRACY2, Yingwei FEI2, Chad MCCOY3, Sakun DUWAL3
1Korea University, Korea, South, 2Carnegie Institution for Science, United States, 3Sandia National Laboratories, United States
Melting is a key process in planetary interiors and strongly influences differentiation during the early history of a planet. The melting curve of (Mg,Fe)SiO3 may determine the temperature at the core-mantle boundary of the super-Earth planet, affecting heat flux and the generation of its internal magnetic field. Super-Earths are believed to complete their accretionary phase in a molten state. Hot super-Earths are likely molten at the surface, possessing magma oceans that may extend to the deep interior. The mantle evolution from a fully molten state to a solid will depend on the relationship between a planetary adiabat and the melt curve at ultrahigh pressures. Incorporating iron into the Mg-silicate end-member is expected to lower the melting temperature and influence the depth of a magma ocean. However, the extent of this effect has not been quantified experimentally. Bridgmanite, which is expected to contain 8-11% Fe in the pyrolite composition model of the lower mantle, has no experimental data for the melting of iron-bearing silicates at the extreme conditions relevant to the deep interiors of super-Earths, and extrapolated melting temperatures from experiments and the calculated melting curves are discrepant. In this study, we performed shock-compression experiments on iron-bearing bridgmanite (Mg0.92,Fe0.08)SiO3 in the range of ~450 GPa to constrain its melting point on the Hugoniot at the Z-facility. Our Hugoniot sound velocity measurements will allow for interpreting the melting point of Mg-rich silicates and offer insights into impact processes relevant to planetary formation and evolution.
PS18-A015
Investigation of High Pressure Raman Spectra in Quasi 2D Organic Inorganic Hybrid Perovskites
Min Jae KIM1+, Myeong Jun KANG1, Young Jay RYU2, Yanbin WANG2, Vitali PRAKAPENKA2, Soomin PARK3, Sungkyun PARK1, Jaeyong KIM3, Jong Mok OK1#
1Pusan National University, Korea, South, 2The University of Chicago, United States, 3Hanyang University, Korea, South
Organic-Inorganic Hybrid Perovskites (OIHPs) have been extensively studied recently for their potential applications in photovoltaics, optics, and magnonics devices [1]. These materials exhibit a diverse range of physical properties, such as multiferroic behavior, high absorption coefficient, long diffusion length, tunable band gaps, and canted spin arrangements.[2]. These properties are stem from various chemical compositions. Most of OIHPs consist of organic cations and metal halides, such as 2-methylbutane ((CH3(CH3)2NH3)+, MA), n-butylammonium ((CH3(CH2)3NH3)+, BA) and 2-phenylethylamine ((C6H5(CH2)2NH3)+, PEA) and MX4 (M = Cu, Mn, Ni, Co, X = Cl, Br, I, etc.). Furthermore, OIHPs can cover a wide range of dimensionality by adopting proper organic materials while inorganic perovskites only have 3D structure. [3] This tunable dimensionality makes OIHPs an intriguing material to exploring the dimension - dependent physical property of various chemical composition. Despite the various chemical compositions available, research on lead-based OIHP is dominant due to their excellent performance in photovoltaic devices. However, these materials have a negative impact on the environment and human health. Therefore, there is a need to develop lead-free and air-stable OIHPs to meet environmental requirements. In this work, we performed high pressure and temperature dependent Raman spectra measurement on PEA2MnCl4 single crystals, which can provide a way to directly modify the crystal structure and the local distortion of crystal structure. Raman spectra indicate that MnCl6 octahedra undergo distortion and PEA2 layers are fully collapsed under high pressure. Additionally, we found the phase transition in PEA2MnCl4 in various temperature. This suggests that exchange superexchange interaction in MnCl6 octahedra can be tuned by applying pressure. More study is on-going to clarify the spin texture, crystal structure and low temperature behavior, further research are needed, such as XRD measurement, low temperature MFM or STM, neutron scattering measurements.
PS19-A002
Constraints on Lateral Variations of Martian Crustal Thickness from Seismological, Gravity Field, and Radiotracking Measurements
Melanie DRILLEAU1#+, Henri SAMUEL2, Attilio RIVOLDINI3, Raphael GARCIA1, Clement PERRIN4, Mark WIECZOREK2, Doyeon KIM5, Philippe LOGNONNÉ6
1Institut Supérieur de l'Aéronautique et de l'Espace, France, 2Institut de Physique du Globe de Paris, France, 3Royal Observatory of Belgium, Belgium, 4Nantes Université/ Université d’Angers/ Le Mans Université/ Centre National de la Recherche Scientifique, France, 5Imperial College London, United Kingdom, 6Université Paris Cité, Institut de physique du globe de Paris, CNRS, France
Using body wave arrival times from about thirty seismic events recorded on Mars by the InSight mission and surface waves generated by the largest seismic event on Mars, combined with topography and gravity field modeling, we constrained lateral variations of crustal thickness through a Bayesian inversion approach, and the 1D structure in the mantle and core. The parameterization of the seismic structure relies on quantities that influence the thermochemical evolution of Mars, enabling the seismic velocities and densities in the different planetary envelopes to be consistently linked through common physical assumptions. We also investigated with further inversion sets the influence of deep mantle stratification on our findings, considering the recently discovered basal mantle layer above Mars' core (Samuel et al., 2023). Compared to a purely 1D structure, models with lateral variations of crustal thickness show different interpretations of the thermal evolution of Mars. We verified the compatibility of our results with InSight’s radiotracking data and the tidal Love number k2. Furthermore, we relocated the marsquakes and derived maps of seismicity recorded by InSight, which is mostly located along or North of the boundary between the Northern lowlands and the Southern highlands.
PS19-A004
Detecting Gravitational Wave with an Interferometric Seismometer Array on Lunar Nearside
Junlang LI1+, Fangfei LIU1, Yuan PAN1, Zijian WANG1, Mengdi CAO1, Mengyao WANG1#, Fan ZHANG1, Jinhai ZHANG2, Zonghong ZHU1
1Beijing Normal University, China, 2Chinese Academy of Sciences, China
Our Moon is by far the easiest natural, extraterrestrial celestial object for us to reach, and many space agencies, in particular the China National Space Administration, have publicized plans for manned missions there. Such high-profile projects must yield commensurate scientific outputs to justify their cost to the taxpayers. An important criterion for the selection of candidate experiments is the extent to which the Moon plays an integral and irreplaceable role, as opposed to offering only marginal advantages over Earth-orbit, space-based alternatives. In this study, we propose an experiment that excels in this regard, which considers the Moon as part of the experimental apparatus. Specifically, the Moon acts as a Weber bar-style resonant mass that responds to deci-Hertz gravitational waves (GWs). GW-excited lunar vibrations can be picked up by an array of (prefabricated on Earth and easy to transport to the Moon) small laser interferometric seismometers yielding GW detection. Such a setup would plug a gap in the GW frequency range already covered by the existing or underdevelopment detectors, and it can inform us on important astrophysics topics, such as the progenitors of Type Ia supernovae (SNe Ia) or intermediate mass black holes. We provide the instrument design as well as its deployment strategy, and we also summarize relevant science cases according to the estimated viable sensitivity.
PS19-A006
Description of Atmospheric Gravity Waves on Mars Based on InSight Seismic and Meteorological Observations
Keisuke ONODERA1#+, Kiwamu NISHIDA2, Rudolf WIDMER-SCHNIDRIG3, Taichi KAWAMURA4, Aymeric SPIGA5, Jorge HERNANDEZ-BERNAL5, Eleonore STUTZMANN6, Zongbo XU6, Anna HORLESTON7, Martin SCHIMMEL8, Naomi MURDOCH9
1Okayama University, Japan, 2The University of Tokyo, Japan, 3Black Forest Observatory, Germany, 4Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, France, 5Institut Pierre-Simon Laplace, France, 6Institut de Physique du Globe de Paris, France, 7University of Bristol, United Kingdom, 8Geociencias Barcelona, Spain, 9Institut Supérieur de l'Aéronautique et de l'Espace , France
Atmospheric gravity wave (AGW) is a common phenomenon on planets with atmosphere (e.g., Earth, Mars, Venus, and Jupiter). The restoring force driving AGWs is the buoyancy oscillation of air parcels, and their observation is useful for understanding the thermodynamic structure of the atmosphere. In this study, combining the InSight pressure and seismic data, we are trying to gain new insight into Martian AGWs and their interaction with the ground. Generally, information is limited to describe the AGWs using only meteorological data (e.g., pressure, wind speed), which poses limits for the determination of the propagation direction when a single station is available. However, measuring the tilt direction of a seismometer induced by AGWs allows us to estimate which direction AGWs travel. This provides us with essential information to investigate where and how AGWs are excited. In the presentation, following the description of AGWs recorded by the InSight pressure sensor, we will explain how they interact with the Martian surface by referring to the seismic data. Then, by retrieving the azimuth toward AGWs’ source, we will discuss variations in their excitation mechanism (e.g., caused by topography? or related to thermodynamical structure in the atmosphere?). Finally, we present an application of this phenomenon to assessing crustal rigidity.
PS19-A009
Digital Twin Mars: Marsquake Scenario Reconstruction Using a Game Engine
Chen GU#+
Tsinghua University, China
We present a game engine-based Digital Twin Mars system for reconstructing Marsquake scenarios. Utilizing seismic wave field simulation to catalog events from the Mars Quake service (MQS), we have reconstructed global ground motions on Mars. Taking into account the velocity model, Marsquake source mechanisms, and site effects, we also provide comprehensive insights into the uncertainties of ground motions arising from model misspecification. Furthermore, we have integrated virtual digital cities within the game engine. These cities function as models to demonstrate the potential impacts of Marsquakes on various infrastructure. This Digital Twin Mars system not only serves as an interactive platform to reconstruct and visualize Marsquake scenarios, but also acts as a playground for civil engineers to envision and plan for future human civilization on Mars.
PS19-A011
Assessing and Improving the Phasor Walkout Method for Identifying Low-frequency Spectral Peaks
Zhuowei XIAO1+, Juan LI1,2#, Zhongzheng MIAO1
1Chinese Academy of Sciences, China, 2University of Chinese Academy of Sciences, China
When searching for seismic normal modes and hums, we often observe spectral peaks emerging from the noisy background, which makes it challenging to determine if they are products of free oscillations or merely random noise. The phasor walkout method solves this issue by visualizing the Fourier spectrum construction at specific frequencies through vector summation in complex number space. The method assumes that the eigenfrequencies of free oscillation produce linear phasor walkout patterns, while spectral peaks of random noise produce irregular paths. Our study, however, reveals that random noise can contain spectral peaks with seemingly linear phasor walkout patterns with high R2 and Schuster significance values, highlighting the need to assess metrics used to interpret phasor walkout patterns. Through extensive synthetic signal and noise datasets, we evaluated previously used metrics like R2, Schuster significance, and our proposed complete/individual phasor sum ratio and deep learning techniques. The Kullback-Leibler divergence quantitatively assesses the effectiveness of these metrics in differentiating signal and noise spectral peaks. Using the 2011 Tohoku earthquake data, we validate these metrics' effectiveness on real-world data. Our results indicate that the complete/individual phasor sum ratio and deep learning classifiers more accurately distinguish low-frequency spectral peaks from noise compared to R2 and Schuster significance. While the deep learning model trained on synthetic data encounters the out-of-distribution issue with complex real-world data, the complete/individual phasor sum ratio remains a robust indicator for detecting seismic normal modes. This study assesses and enhances the phasor walkout method, thereby contributing to identifying seismic normal modes' eigenfrequencies on Earth and other planets.
PS19-A017
Lander Resonance and Super-high-frequency Marsquakes Recorded by the InSight
Lei ZHANG#+, Jinhai ZHANG
Chinese Academy of Sciences, China
The first high-performance seismograph on Mars, deployed by InSight, has been working for nearly two Martian years. The recorded seismic data has evident artificial characteristics in the high frequency band up to 10 Hz, probably caused by the resonance of the lander and near-field thermal events. However, their mechanisms remain unclear. Here we conduct a modal analysis of the InSight lander with a simplified finite-element model, and identify three natural frequencies from the InSight’s SEIS data of the first Martian year. The natural modes of the solar panels indicate an elastic modulus reduction of the solar panels (35% at most) and/or the property changes of the ground media beneath the lander due to a daily air temperature variation of approximately 100 K on Mars. These analyses help to avoid the potential interference of natural frequencies and improve the reliability of seismic data applications for interior structure of Mars. In addition, we model heat conduction under the InSight lander based on measured subsurface thermal parameters and air temperature records, which provide insights into heat flow in the shallow Martian subsurface. Diurnal and seasonal variations of subsurface temperature and their rates of temperature change are analyzed. Diurnal temperature variations >1 K only occur within 25 cm of the surface. The highest rate of temperature change appears around sol 440 (in summer), which coincides closely with the season of the dominant number of super-high-frequency marsquakes observed. Thermal-mechanical finite-element simulations indicate that heat-induced ground motion is evidently stronger in the daytime than at night. These results indicate that super-high-frequency marsquakes are most likely induced by thermal stress in shallow rocks that are on the surface or partially buried within 10 cm depth. Our study can quantitatively evaluate temperature-dependent natural modes of lander and the mechanism of near-field thermal quakes on extraterrestrial objects, which is significant for the seismic signal analysis and the inversion of planetary interior structures.
PS19-A024
Towards an International Infra-red and Visible Telescopic Monitoring Network for Lunar Impact Seismology Studies
Philippe LOGNONNÉ1#+, Marco DELBO2, Daniel SHEWARD3, Chrysa AVDELLIDOU4, Anthony COOK5, Sylvain CHATY3, Taichi KAWAMURA6, Rodrigo LEIVA7, Danielle MOSER8, Mark PANNING9, Jean-Pierre RIVET2
1Université Paris Cité, Institut de physique du globe de Paris, CNRS, France, 2Observatoire de la Côte d'Azur, France, 3Université Paris Cité, France, 4University of Leicester, United Kingdom, 5Aberystwyth University, United Kingdom, 6Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, France, 7Instituto de Astrofísica de Andalucía, Consejo Superior de Investigaciones Científicas, Spain, 8NASA Marshall Space Flight Center, United States, 9Jet Propulsion Laboratory, California Institute of Technology, United States
The NASA’s FarSide Seismic Suite (FSS) and China’s ChangE-7 Lunar missions will deploy seismometers on the Moon after 2026. However, joint operation is not planned, as they have different operational schedules and work independently. Locating new seismic sources, such as impacts, shallow moonquakes or deep moonquakes, will therefore remain a significant challenge. We present the potential of an Earth-based international Lunar Impact Flash monitoring network. This monitoring could provide the time of impacts on Moon’s near side and their epicentral distance with a location error, either small enough for seismic travel time inversion, or at least permit a search for a fresh crater by lunar orbiters (Sheward et al. 2022). Each located impact will provide the measurement of absolute travel time of seismic phase, which are crucial for structure inversion. Our estimates suggest about 23 impacts per year year on the near side to be above the detection threshold of FSS and 60 per year for a South pole located station with comparable sensitivity. Unlike existing visible light impact flash monitoring, which is confined to earthshine, during night time here on Earth, the first ever detection of short wave infra-red lunar impact flash (Sheward et al., 2023) has demonstrated that it is possible to extend significantly the number of observing hours into day light and potentially allowing the detection of impact flashes even on the dayside of the Moon. Monitoring and identifying these impacts is our goal, with already planned observing sites in France, England, Chile, USA and Japan. This could work alongside the citizen science observing network being set up for the LUMIO mission in 2027. We conclude by noting the importance for extending this network into other countries, in order to achieve constant time coverage and redundancy with respect to bad weather here on Earth.
PS19-A028
Lander Induced Thermo-elastic Noise at the FSS Location
Sreejaya KIZHAEKKE PAKKATHILLAM1#+, Philippe LOGNONNÉ2, Sébastien DE RAUCOURT1, Taichi KAWAMURA3
1Université Paris Cité, France, 2Université Paris Cité, Institut de physique du globe de Paris, CNRS, France, 3Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, France
Thermo-elastic noise on the Moon results from variations in solar radiation, causing elastic stress and strain within the lunar surface. This has been observed through experiments like SEIS on Mars, detecting noise generated during the eclipse of Phobos. While periodic temperature variations of the instrument are manageable, other, such as related to moving shadow on the ground or related to the solar radiation fluctuations, require numerical quantification due to difficulties in filtering them from the data. Hence, this study investigates first how the shadowing effect from the lander's structure and solar radiation variations impacts subsurface soil temperatures and consideration of this effect on the tilt recorded on the seismometers. We develop a 3D numerical model within Comsol Multiphysics 6.1 finite element package. The key element in adapting this model for use on Moon is accurately replicating the illumination conditions on the Lunar surface. Based on sub solar latitude and longitude derived using the JPL Horizons Ephemeris output, an illumination model is set at the instrument site for a desired duration. First, an analytical model is employed to find the transient solution of temperature at any given depth and time instances. The solution to the energy balance analysis determines the boundary conditions at the ground surface, which are then applied in the heat conduction equations governing subsurface temperature distribution. The numerical temperature distribution output at an unperturbed location, far away from the lander is then compared with the analytical solution. Once the 3D model is calibrated, the resulting temperature profiles can be utilized to assess the tilt of the seismometer feet and the sensitivity to additional solar radiation fluctuations. The findings suggest that the presence of a lander can exert substantial effects on the surrounding temperature environment under Lunar conditions, which introduces noise into the data collected by the seismometer.
PS19-A029
Japanese Activities to Establish a Seismic Observation Network on the Moon
Taichi KAWAMURA1#+, Satoshi TANAKA2, Takeshi TSUJI3, Akito ARAYA3, Keisuke ONODERA4
1Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, France, 2Japan Aerospace Exploration Agency, Japan, 3The University of Tokyo, Japan, 4Okayama University, Japan
Recently, lunar exploration has once again become a global trend and various space agencies are now planning a landing and manned mission to the Moon. In this context, Japan Aerospace Exploration Agency (JAXA) has identified 3 major scientific goals to be addressed in their future lunar missions and seismic observation network was listed as one of them. To achieve this, Japan has carried out a feasibility study (FS) for a lunar seismic observation system using an unmanned lander, as a step towards establishing a future seismic observation network. Key questions that were addressed during the FS was 1. challenge for night survival and long term observation and 2. development of high sensitivity seismometer. Continuous and long term observations are essential for a success of the seismic observation and this is very well demonstrated by success of Apollo and InSight. On the other hand, future lunar missions are likely to be closer to the pole which might have limitations in the power supply. We discuss our challenge and primary outcomes from the FS to realize our observation. From observations of Apollo, we know that many moonquakes are small in magnitude and requirements for our lunar seismometer is challenging. In addition to this, we also know that moonquake signals suffer from intense scattering and going to longer period is a key to obtain high quality seismic data. We will describe our activities to develop a seismometer and discuss the challenges we have for future developments.
PS19-A033
OH Airglow SWIR Observations: High Temporal Resolution Acquisition for Ionospheric Seismology Proof of Concept
Pierre-Yves FROISSART1,2#+, Philippe LOGNONNÉ3, Pierre SIMONEAU2, Kiwamu NISHIDA4
1Université Paris Cité, France, 2Office National d'Etudes et Recherches Aérospatiales, France, 3Université Paris Cité, Institut de physique du globe de Paris, CNRS, France, 4The University of Tokyo, Japan
Nightglow radiation is a very good marker of high-altitude dynamics. After a first detection of a tsunami signature by a camera in the O+ emission (red airglow at 250km) in 2011, only a few other tsunami detections have been recorded and none have been observed in OH SWIR emission, which is the brightest of all the nightglow emissions and the only compatible for shorter periods signals, such as seismic waves. On the other hand, these acoustic waves associated with earthquakes are systematically detected by other ionospheric instruments (GPS, radar), they have never been directly observed by an airglow camera. Can they be also detected by airglow? We present here our strategy for such proof of concept. If achieved, it will provide unique access to seismic waves propagation where ground instruments are not available: oceans, which cover more than 70% of the Earth's surface, but also to provide the harsh planetary environment of Venus, where airglow also exists and where it is not possible to send spacecraft to the ground. The recent development of SWIR cameras and the first detection of infrasound in OH radiation in 2020 opened the way for these detections. To better understand the continuous dynamics of the OH layer, we have deployed a first camera at La Réunion island in May 2023. Another one will be installed on the Japanese island of Oshima in February-March 2024 to try to detect the signature of a seismic event if one occurs during the course of this scientific study. The poster details our methodology for observing the airglow OH perturbations, from the instrument specifications to the first results of almost a year of observations on La Réunion and the expected events that we will observe from Japan.
Session Chair(s): Paul HARTOGH, Max Planck Institute for Solar System Research, Scott BOLTON, Southwest Research Institute
PS06-A001
Chemical Compositions and Formation Scenarios of Jupiter’s Polar Haze Inferred from 2-micron Juno/JIRAM Spectro-images
Jaekyun PARK1#+, Sang Joon KIM1, Mingyu JEON1, Chae Kyung SIM2,3, Henrik MELIN4, Regis COURTIN5, Jongho SEON1
1Kyung Hee University, 2Korea Astronomy and Space Science Institute, 3Korea National University of Science and Technology, 4University of Leicester, 5Paris Observatory
Recently, we have analyzed the 2-micron spectro-images of the polar haze of Jupiter utilizing JIRAM/Juno data archived at the Planetary Data System/JPL. From the analyses, we find that the 2-micron polar regions show fairly uniform and symmetrical distribution of the haze around the poles. We find no traces of recently discovered stratospheric polar jets (Cavalié et al., 2021) nor of the IR northern hot/bright spots on these images. The non-detections indicate that the major polar haze layers are under the jets and the IR bright spots; and the thermal radiation from the IR hot spots is negligible at 2-micron. From spectral analyses, we derive the haze optical depths and single scattering albedos between 2.0 and 2.5-micron. The derived spectral structure of the opacity is roughly similar to those of hydrocarbon and nitrile ices of Titan retrieved by Sim et al. (2013), who claim that the 2-micron features of the Titan’s haze mainly consist of alkane ices with the addition of a nitrile ice in the nitrogen-dominant atmosphere of Titan. This suggests similar chemical compositions and possibly similar formation mechanisms for the Jovian haze particles, but we may exclude the nitrile ice for the hydrogen-dominant Jupiter’s atmosphere.
PS06-A009
Observations of Io with the Juno Microwave Radiometer: First Results and Implications for Global Heat Flow
Shannon BROWN1#+, Scott BOLTON2, Steve LEVIN1, Zhimeng ZHANG1, Matt SIEGLER3, Jianqing FENG3
1California Institute of Technology, 2Southwest Research Institute, 3Planetary Science Institute
The NASA Juno mission performed two close fly-bys of Jupiter’s moon Io on December 30, 2023 and February 3, 2024. Juno carries a 6-channel microwave radiometer (MWR) operating between 0.6-22 GHz. The first fly-by observed Io’s north pole and the 2nd pass mapped latitudes within +/- 45o on the Jovian facing hemisphere. The broad frequency range of the MWR probes successively deeper into the Io sub-surface with the 0.6GHz channel probing the deepest. The sub-surface temperature, dielectric and surface roughness properties are encoded in the spectra obtained by the MWR. Here we report on the first spatially resolved observations of Io at frequencies below 22 GHz. We find the brightness temperatures decrease with increasing latitude and are coldest at the north pole, consistent with prior infrared observations of the surface skin temperature. We observe a strong spectral gradient in the lowest frequency channels (increasing with depth) reflecting the sub-surface temperature profile from which we can infer endogenic heat flow. We will give an overview of the MWR observations and initial inferences about the sub-surface thermal and compositional properties.
PS06-A011
Reproducing of Ganymede Brightness Temperature Observation from Microwave Radiometer/juno with a Scattering-inclusive Radiative Transfer Model
Hao-Yu YANG1,2#+, Yasuko KASAI3,2, Suyun WANG2, Ryusei MATSUNAGA4, Yu AOKI2,5
1Tokyo Institute of Technology, 2National Institute of Information and Communications Technology, 3NICT, Institute of Science Tokyo, 4Tokyo Gakugei University, 5Institute of Science Tokyo
JUNO had a close flyby of Ganymede from 1,038 kilometers above the surface on June 7 2021. We have been trying to reproduce Ganymede brightness temperature observation from Microwave Radiometer (MWR)/JUNO by using NICT scattering-inclusive radiative transfer model (RTM). NICT RTM including scattering for Ganymede underground. We model that as a random medium with rough top and bottom boundaries and a host medium situated beneath. The total scattering and emission consists of four sources: rough boundaries, the volume, and the boundaries and the volume interactions, and from atmospheric compositions. We focus the simulation of observation of brightness temperature for four frequency regions, 2.6 GHz, 5.2GHz, 10 GHz, 22 GHz. In the presentation, we will show the bias and difference between simulation and observation and possible results of the difference. Acknowledgment: This work encompasses outcomes from the project Exploration of water energy resources over a wide area on the moon using terahertz waves' (JPJ010777), part of the 'R&D of ICT priority technology' (JPMI00316) initiative, sponsored by the Ministry of Internal Affairs and Communications.
PS06-A004
The Submillimetre Wave Instrument (SWI) on JUICE: PCW1&2 and LEGA Preparations
Paul HARTOGH#+
Max Planck Institute for Solar System Research
The Submillimeter Wave Instrument (SWI) is part of the payload of ESA’s L1 mission JUICE (JUpiter ICy moons Explorer). It sounds the atmospheres of Jupiter and the Galilean moons in two Far Infrared bands covering the frequency ranges of 530 – 625 GHz and 1065 – 1280 GHz. Furthermore, it is designed to characterize the thermo-physical surface properties of Callisto, Ganymede and Europa during flyby and orbital phases. After the successful launch in April 2023 and the commissioning of the instrument, in 2024 two Payload Checkout Windows will take place followed by the Lunar Earth Gravity Assist (LEGA). The presentation will focus on the analysis of the commissioning data, PCW1/2 and the planned LEGA observations.
PS06-A012
Microwave Spectrometer Control Software: Managing Ground-based Microwave Spectrometers for SWI Calibration and Data Visualization
Borys DABROWSKI#+, Paul HARTOGH, Richard LARSSON
Max Planck Institute for Solar System Research
The Microwave Spectrometer Control is a pivotal software orchestrating ground based microwave spectrometers utilized as reference instruments for the Submillimeter Wave Instrument (SWI). They are placed next to the SWI Ground Reference Model (GRM). SWI and ground based receivers and spectrometers can be interconnected for calibration and analytical purposes. Microwave Spectrometer Control's comprehensive capabilities encompassing control, data storage, and visualization streamline the management of ground-based microwave spectrometers' operations and collected spectral data. The software seamlessly controls and supervises the ground-based microwave spectrometers, enabling efficient configuration of measurement parameters through its Graphical User Interface (GUI). This interface not only facilitates real-time monitoring but also presents a detailed display of measured spectra, showcasing both raw and calibrated data, crucial for precise radiometric observations. By facilitating the management and visualization of spectral data from ground-based microwave-spectrometers, the software emerges as a crucial tool in ensuring the accuracy and reliability of SWI calibration processes, enhancing the overall effectiveness and efficiency of microwave radiometry research. This presentation will illustrate the development progress and the structure and functionality of the software.
PS06-A008
Model-based Physical Parameter Retrieval for Passive Terahertz Wave Observations of the Moon
Suyun WANG1#+, Takayoshi YAMADA1, Yasuko KASAI2,1
1National Institute of Information and Communications Technology, 2NICT, Institute of Science Tokyo
The Lunar Terahertz SUrveyor for KIlometer-scale MappIng (TSUKIMI) mission employs a dual-frequency dual-polarization THz radiometer and seeks to monitor the THz wave brightness temperature of the Moon on a global scale. To fully utilize the THz wave brightness temperature data requires a comprehensive understanding of the coupling effects between dielectric and geometric features of lunar regolith, especially concerning observation angle, frequency, and polarization. Therefore, accounting for these effects becomes imperative for accurately extracting the physical parameters of the lunar regolith. In this study, we develop a THz radiative transfer model including scattering for lunar regolith. We model the lunar regolith as a random medium with rough top and bottom boundaries and a host medium situated beneath. The total scattering and emission consists of three sources: rough boundaries, the volume, and the boundaries and the volume interactions. To consider these sources, we model their respective phase matrices and apply the matrix doubling approach to couple these phase matrices to compute the total emission. Furthermore, we generate the simulated THz wave brightness temperature data for the region of interest of the Moon using the developed model, together with sensitivity analysis, to identify an optimized configuration for physical parameter inversion of lunar regolith from THz passive measurements by Kalman filter-based estimation method to resolve the nonlinear and complex boundary problems. Acknowledgement: This research and development includes the results achieved under "Exploration of water energy resources over a wide area on the moon using terahertz waves" (JPJ010777) within the "R & D of ICT priority technology" (JPMI00316) of the Ministry of Internal Affairs and Communications.
PS06-A016
TSUKIMI - lunar Terahertz SUrveyor for KIlometer-scale MappIng
Yasuko KASAI1,2#+, Hideaki MIYAMOTO3, Toshiyuki NISHIBORI4, Hiroyuki MAEZAWA5, Tetsuya HONDA6
1NICT, Institute of Science Tokyo, 2National Institute of Information and Communications Technology, 3The University of Tokyo, 4Japan Aerospace Exploration Agency, 5Osaka Metropolitan University, 6Space BD
We are developing a new era lunar mission, TSUKIMI: lunar Terahertz SUrveyor for KIlometer-scale MappIng, from November 2021. The purpose of TSUKIMI is to making a map the water vapor permittivity of the subsurface soil for future human activity on the Moon. We plan to measure the brightness temperature from subsurface of Moon using Terahertz (THz) remote sensor on-boarded minisatellite from Luner circular orbit from 100km above. Uniqueness of THz passive observation is 1) Subsurface observation, 2) Global wide range observation, and 3) Enables downsizing and weight reduction of sensor compared with microwave/active sensor. In this presentation, I will introduce the purpose and background, and overview.
PS06-A006
Morphology of the Excited Hydroxyl in the Martian Atmosphere and Ozon Photochemical Equilibrium
Dmitry S. SHAPOSHNIKOV1#, Mykhaylo GRYGALASHVYLY2, Alexander S. MEDVEDEV2+, Gerd SONNEMANN3, Paul HARTOGH2
1Moscow Institute of Physics and Technology, 2Max Planck Institute for Solar System Research, 3Leibniz-Institute of Atmospheric Physics
Monitoring excited hydroxyl (OH*) airglow is broadly used for characterizing the state and dynamics of the terrestrial atmosphere. Recently, the existence of excited hydroxyl was confirmed by satellite observations in the Martian atmosphere. The location and timing of its detection on Mars were restricted to a winter season at the north pole. We present three-dimensional global simulations of excited hydroxyl over a Martian year. The predicted spatio-temporal distribution of the OH* can provide guidance for future observations, namely by indicating where and when the airglow is likely to be detected. Moreover, atomic oxygen (O) and atomic hydrogen (H) in the Martian atmosphere are very important species, which play a role in chemistry, airglow, and energy budget. However, they cannot be directly measured by satellite remote sensing techniques. For the Earth atmosphere, retrievals based on OH* airglow observations and assumption about ozone photochemical equilibrium. This technique can be applied for the Martian atmosphere. Hence, additionally, we examine ozone photochemical equilibrium for the Martian atmosphere in more detail.
PS06-A002
The Modular Infrared Molecules and Ices Sensor (MIRMIS): An Instrument Visiting a Long-period Comet
Bea CHIKANI1#+, Neil BOWLES1, Keith NOWICKI1, Richard COLE2, Tomas KOHOUT3, Antti NÄSILÄ2, Geronimo VILLANUEVA4, Chris HOWE5, Geraint JONES6, Colin SNODGRASS7, Kerri DONALDSON HANNA8, Benjamin GREENHAGEN9, Patrick IRWIN10, Simon CALCUTT1, Rory EVANS1, Katherine SHIRLEY1, Tristram WARREN1, Tilak HEWAGAMA4,11, Shahid ASLAM4, Donald JENNINGS4, Altti AKUJÄRVI2, Antti PENTTILÄ3, Jon TEMPLE1, Henry ESBAUGH1, Aria VITKOVA1, Maisie RASHMAN1, Swati THIRUMANGALATH2, Sara FAGGI4, Leevi SALONEN2, Silvia PROTOPAPA12, Alexander KOKKA2, David KORDA3, Aurelie GUILBERT-LEPOUTRE13
1University of Oxford, 2VTT Technical Research Centre of Finland, 3University of Helsinki, 4NASA Goddard Space Flight Center, 5Rutherford Appleton Laboratory, 6University College London, 7University of Edinburgh, 8University of Central Florida, 9Johns Hopkins University Applied Physics Laboratory, 10Oxford University, 11University of Maryland, 12Southwest Research Institute, 13Laboratoire de Géologie
The Comet Interceptor mission, selected in 2019, is an ESA’s first F-class mission. It will be the first to visit a (yet-undiscovered) long-period comet or interstellar object. These objects are expected to be “pristine” having not been exposed to the Sun in the inner Solar System. A long-period comet may therefore preserve some of the most primitive material from the early solar system’s history. The mission will launch 3 spacecraft (main spacecraft A and 2 probes: B1 and B2) to the L2 Earth-Sun Lagrange point in which it will wait for a suitable target. The MIRMIS spectrometer is one of the instruments on board of Comet Interceptor mission. It is a collaboration between University of Oxford (UK) and VTT (Finland) as well as scientists from the University of Helsinki, NASA’s Goddard Space Flight Centre, University of Lyon and Southwest Research Institute. The instrument will map the ice and mineral composition of the target nucleus, it will provide characterisation of the gas coma, as well as the distribution of the surface temperatures of the comet nucleus. The spectrometer is composed of 3 moduels covering the spectral range of 0.9 to 25 µm. The Near and Mid Infrared modules (NIR/MIR) will measure spectra in the 0.9 to 5 µm, providing information on volatile species, such as water, CO, CO2 and organics. The Thermal Infrared Imager (TIRI), built at University of Oxford, will map the temperature and composition of the nucleus in the range of 6 to 25 µm, providing key information on the surface and near sub-surface thermal physical properties (e.g. cold traps, boulders/powdered regolith). The AOGS 2024 conference will be an opportunity to present the latest with the design and development of MIRMIS.
PS06-A014
Investigation of the Interrelationship Between the Properties of the Surface Layer, Internal Coma and Comet Activities
Yuri SKOROV1,2#+, Omar MOKHTARI3, Johannes MARKKANEN1, Ladislav REZAC1, Paul HARTOGH1, Nicolas THOMAS3
1Max Planck Institute for Solar System Research, 2Technische Universität Braunschweig, 3University of Bern
Investigating the properties of sublimation products emanating from the cometary nucleus is a crucial aspect of understanding the dusty-gas flow, particularly in light of the Rosetta mission. Today, we possess compelling evidence that the surface and internal coma are interconnected and exert mutual influence. Computer model simulations indicate that the microscopic characteristics of the dust crust profoundly impact the properties of the escaping gas. The hot, highly non-isothermal, porous dust layer significantly heats the evolved gas and reduces its density as water vapour traverses it. This observation aligns with the findings of the microwave MIRO instrument aboard Rosetta, which detected water vapour velocities that were visibly higher than those attributable to sublimation from bare irradiated ice. To elucidate the gas observations, we simulate gas flow through dense random porous dust layers and analyse the temperature and density of emitted molecules. Layers comprising monomers as well as layers constructed from porous aggregates are considered. Modelling is conducted for varying porosity values, distinct particle sizes, and dust layer thicknesses. The simulation results are integrated into two-layer thermal models encompassing effective thermal conductivity, volumetric light absorption, and the resistance of the dust layer to gas flow. Radiation transfer is calculated using geometric optics and the theory of radiative transfer in a dense medium. Finally, we examine the structure and properties of the non-equilibrium rarefied innermost coma. This analysis employs the DSMC kinetic model developed at the University of Bern and extensively utilized for cometary research. A comparison between theoretical outcomes and corresponding observations is conducted. Additionally, we explore the feasibility of resolving the inverse problem: what constraints on the properties of the dust crust can be obtained from observations?
Session Chair(s): Ji-Wei XIE, Nanjing University
PS15-A029
Korea Exoplanet Hunter: KMTNet
Sun-Ju CHUNG#+
Korea Astronomy and Space Science Institute
The Korea microlensing telescope network (KMTNet) is a system for finding exoplanets with the gravitational microlensing method and is composed of three identical 1.6 m telescopes at the Cerro Tololo Interamerican Observatory (CTIO) in Chile, the South Africa n Astronomical Observatory (SAAO), and the Siding Spring Observatory (SSO) in Australia. KMTNet can thus conduct 24 hr continuous high-cadence observations. Almost all planets detected by microlensing are located beyond the snow line, thus they are quite different from those detected by radial velocity and transit methods, which detected 94% of 5550 exoplanets discovered so far. Hence, microlensing planets play an important role to constrain planet formation theories. In this talk, I will present the excellent results so far of the KMTNet experiment, which has been officially initiated in 2016.
PS15-A014
Discovering Low-mass Free-floating Planets with Microlensing
Subo DONG#+
Peking University
Gravitational microlensing is the only known method to discover low-mass free-floating planets (FFPs). Ground-based surveys have found more than a dozen ultra-short microlensing events, with the intriguing implication that sub-Jovian FFPs are a few times more common than planets bound to stars. I will discuss the prospect of future space-based microlensing surveys to discover and characterize a large sample of low-mass FFPs.
PS15-A037
CHES: A Space-borne Astrometric Mission Searching for Habitable Planets Orbiting the Nearby Solar-type Stars
Jianghui JI1#+, Haitao LI1, Junbo ZHANG1, Su WANG1, Dong LI1, Guo CHEN1, Liang FANG1, Lei DENG1, Yao DONG2
1Chinese Academy of Sciences, 2Purple Mountain Observatory, Chinese Academy of Sciences
The Closeby Habitable Exoplanet Survey (CHES) mission is proposed to discover habitable-zone Earth-like planets of nearby solar-type stars (~ 10 pc away from our solar system) via microarcsecond relative astrometry (Ji et al. 2022), which is currently being considered by the Chinese Academy of Sciences as a possible space mission for future launch. The major scientific objectives of CHES are: to search for Earth Twins or terrestrial planets in habitable zones orbiting 100 FGK nearby stars; further to conduct a comprehensive survey and extensively characterize nearby planetary systems. The primary payload is a high-quality, low-distortion, high-stability telescope. The optical subsystem is a coaxial three-mirror an astigmat (TMA) with a 1.2 m-aperture, 0. 44 × 0. 44 field of view and 500 nm-900 nm working wave band. The camera focal plane is composed of a mosaic of 81 scientific CMOS detectors each with 4 k × 4 k pixels. The heterodyne laser interferometric calibration technology is employed to ensure microarcsecond level (1 μas) relative astrometry precision to meet the requirements for detection of Earth-like planets. The CHES satellite operates at the Sun–Earth L2 point and observes all target stars for 5 yr. CHES will offer the first direct measurements of true masses and inclinations of Earth Twins and super-Earths orbiting our neighbor stars based on microarcsecond astrometry from space. This will definitely enhance our understanding of the formation of diverse nearby planetary systems and the emergence of other worlds for solar-type stars, and finally provide insights to the evolution of our own solar system.
PS15-A007
Planetary, Substellar, and Stellar Population Synthesis Based on Astrometric Detection of Companions
Fabo FENG#+
Shanghai Jiao Tong University
Gaia, a survey of one billion stars, revolutionizes the detection of dark companions around bright stars, including planets, brown dwarfs, stars, compact objects, and black holes. Introducing the "Astrometric Bayes Factor Periodogram" (ABFP), I demonstrate its efficacy in utilizing multiple Gaia data releases (GDRs) for companion detection. Calibration and validation of ABFP with synthetic and real companions lead to the identification of millions of candidate companions across multiple GDRs. This sample facilitates the first-ever comprehensive population synthesis of various companion types. The upcoming Gaia DR4 is expected to confirm and enhance our understanding of these candidates, contributing to a more thorough exploration of diverse companions.
PS15-A003
The Progress of East Asian Planet Search Network
Huanyu TENG1#+, Bunei SATO2
1Korean Astronomy and Space Science Institute, 2Tokyo Institute of Technology
East Asian Planet Search Network (EAPS-Net) surveys late-G (including early-K) giant stars with precise radial velocities, aiming to search for planets around intermediate-mass stars in their evolved stages. The EAPS-Net began 20 years ago, with 48 exoplanetary systems discovered by telescopes in East Asia. In this presentation, we report the latest discoveries from the EAPS-Net and statistical information from planet surveys around evolved stars.
PS15-A015
Two Earth-sized Planets Characterized by the Keck Planet Finder
Fei DAI#+
University of Hawaii
We present the first precise mass measurements from the newly commissioned Keck Planet Finder (KPF). TOI-6255 (1.07 Re) and TOI-6324 (1.05 Re) are two Earth-sized planets on roughly 6-hour orbits around two nearby M dwarf host stars. KPF has precisely constrained the mass of both planets to more than 6 sigma precision. TOI-6255 and TOI-6324 are both top ranking targets for JWST/MIRI phase curve observations. We also discuss how these planets may be tidally distorted into football shapes.
PS15-A010
Characterizing Super-earths Through Transit Timing Variations
Ing-Guey JIANG1#+, Li-Chin YEH1, Ming YANG2, Billy EDWARDS3, Keivan STASSUN4, Napaporn A-THANO1
1National Tsing Hua University, 2Nanjing University, 3Netherlands Institute for Space Research, 4Vanderbilt University
The diversity of extra-solar planetary systems has impacted greatly on the researches of planetary science and planet formation. While the statistics of exoplanets could provide constraints on the scenarios of planet formation, characterizing the major population such as super-Earths would lead to cornerstones of late planet formation. We consider the measurement of physical parameters with higher precision for super-Earths as an important task. Through the technique of transit timing variations, we characterize two super-Earths in the most misaligned compact planetary system K2-266. The roles of new TESS and CHEOPS data will be presented.
PS15-A035
Transit Timing Variation Study of Hot Jupiters Using TESS
Bo MA#+
Sun Yat-sen University
Many hot Jupiters may experience orbital decays, which are manifested as long-term transit timing variations. We have analyzed 7068 transits from the Transiting Exoplanet Survey Satellite (TESS) for a sample of 326 hot Jupiters. These new mid-transit time data allow us to update ephemerides for these systems. By combining the new TESS transit timing data with archival data, we search for possible long-term orbital period variations in these hot Jupiters using a linear and a quadratic ephemeris model. We identified 26 candidates that exhibit possible long-term orbital period variations, including 18 candidates with decreasing orbital periods and 8 candidates with increasing orbital periods.
PS15-A025
Photodynamical Analysis of Circumbinary Planet System Toi-1338
Mutian WANG#+, Huigen LIU
Nanjing University
TOI-1338 is the first circumbinary planet system discovered by TESS. It has one transiting planet at P~95 d and an outer non-transiting planet at P~215 day, complemented by further RV observation. We present a global photo-dynamical modeling of TOI-1338 system that self-consistently accounts for the mutual gravitational interactions between all known bodies in the system. By comparing our model with additional data from the TESS Extended Mission and published radial velocity data from HARPS/ESPRESSO, we establish the three-dimensional architecture of the system. Our findings are summarized as follows: The findings are summarized as follows: (1) the inner transiting planet is extremely coplanar to the binary plane, making it a permanently transiting circumbinary planet at any nodal precession phases. We also updated the future transit ephemerides with improved precisions. (2) The outer planet, despite its untransiting nature, is also coplanar with the binary plane within ten degrees. (3) The inner planet's density is estimated to be extremely low, around 0.1 g/cm³. However, the mass constraint varies between the HARPS and ESPRESSO observations.
PS15-A027
Find Companions Around Transit Systems Via Light Travel Time Effect
Andong CHEN#+, Huigen LIU
Nanjing University
Unresolved companions influence the estimation of planetary radii, consequently impacting research on statistical properties. Additionally, close companions suppress the occurrence rate of planets. To gain a deeper understanding of planetary formation and evolution in binary systems, we suggest using the Light Travel Time Effect (LTTE) to detect companions through long-term transit observations. The LTTE arises from the Keplerian motion between a stellar companion (at distances of about 5-20 AU) and the host planet. Through forward numerical analysis, we ascertain that LTTE can induce more significant long-term Transit Timing Variations (TTV) than dynamic perturbations. By combining data from missions such as Kepler, TESS, PLATO, and ET2.0, the photometric observations will span a baseline of over 8000 days. We try to extract long-term TTV signals by employing the LTTE model and other alternative mechanisms to analyze both real and simulated data. We present a catalog of possible transiting S-type binary systems. Our retrieval results are consistent with the dominated region identified in forward analysis, demonstrating the capability of our retrieval code in accurately reproducing the properties of companions within this region. Finding companions via LTTE is an efficient and straightforward method to sculpt the architecture of planetary systems and conduct statistical research.
Session Chair(s): Philippe LOGNONNÉ, Université Paris Cité, Institut de physique du globe de Paris, CNRS, Sébastien DE RAUCOURT, Université Paris Cité
PS19-A013
| Invited
Seismology of the Giant Planets
Patrick GAULME#+
Thüringer Landessternwarte Tautenburg
Seismology applied to the giant planets of the solar system could drastically change our understanding of their deep interiors, as it has happened with the Earth, the Sun, Mars, the Moon, and many stars from the main-sequence to evolved phases. Studying the composition of giant planets is important for understanding both the mechanisms enabling their formation and the origins of planetary systems, in particular our own. Unfortunately, its determination is complicated by the fact that their interiors are thought not to be homogeneous, so that spectroscopic determinations of atmospheric abundances are probably not representative of the interiors. Instead, the determination of their compositions and structures rely on indirect measurements and interior models. Since they are mostly fluid and convective, seismology of the giant planets is actually much closer to that of the Sun and solar-like stars than that of terrestrial planets. In this colloquium, I will review the observational efforts that have been undertaken for the past two decades, especially the convincing results that have been obtained about Jupiter and Saturn, and discuss future developments of the field.
PS19-A007
| Invited
Development of Balloon-based Seismology for Venus Using Earth as an Analog
Siddharth KRISHNAMOORTHY1#+, Daniel BOWMAN2, James CUTTS1, Attila KOMJATHY3, Raphael GARCIA4, Léo MARTIRE1, David MIMOUN4,5, Jennifer JACKSON3, Quentin BRISSAUD6, Brian ELBING7, Jamey JACOB7, John WILDING3, Emalee HOUGH7, Zach YAP7, Solène GÉRIER4, Jacob IZRAELEVITZ1
1NASA Jet Propulsion Laboratory, 2Sandia National Laboratories, 3California Institute of Technology, 4Institut Supérieur de l'Aéronautique et de l'Espace, 5University of Toulouse, 6Norwegian Seismic Array, 7Oklahoma State University
Balloon-based seismology through the study of low-frequency seismo-acoustic signals (infrasound) has gained acceptance as a viable way to study seismic activity on Venus. Balloon-based barometers have the potential to detect and characterize atmospheric waves launched by venusquakes and volcanic eruptions while offering substantially longer instrument lifetimes in the Venus middle atmosphere, where temperature and pressure are significantly more benign (0-100°C, ~1 atm) as compared to the surface (> 460°C, ~90 atm). One of the major challenges in performing balloon-based seismology on Venus is the absence of ground-truth data for event identification and discrimination. To address this challenge, our activities are aimed at building a catalog of terrestrial balloon-recorded infrasound signals of geophysical provenance, using which signal predictions can be extended to Venus and the detectability of events can be analyzed. We will highlight our recently concluded Balloon-based Acoustic Seismology Study (BASS) campaign, which was a sequence of Earth-analog experiments for Venus balloon-based seismology. During the last three years, acoustic signals from epicentral and surface waves from earthquakes ranging from Magnitude 2.7 to Magnitude 7.5 were detected on high-altitude balloons. In addition, signals from volcanic eruptions and bolide-like signals were also recorded. Data collected were used to validate seismo-acoustic simulation tools, which are being expanded to include the Venus atmosphere. These tools will used to generate predictions of infrasound signals from geophysical events on Venus. We will also provide perspective on directions for future instrument development for Venus balloon flights.
PS19-A026
| Invited
Development Status of Seismometer Package for Dragonfly Relocatable Lander
Hiroaki SHIRAISHI1,2#+, Takefumi MITANI1, Taichi KAWAMURA3, Keisuke ONODERA4, Ryuhei YAMADA5, Satoshi TANAKA1, Hideki MURAKAMI6, Ralph LORENZ7
1Japan Aerospace Exploration Agency, 2宇宙航空研究開発機構, 3Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 4Okayama University, 5The University of Aizu, 6Kochi University, 7Johns Hopkins University Applied Physics Laboratory
Dragonfly is a relocatable lander that would use dual-quad rotors to perform soft-landings at multiple sites on the Saturn’s largest moon, Titan. The spacecraft will be launched in 2028 and explore Titan for ~3 years in the mid-2030s. The Geophysical and Meteorological package (“DraGMet”) onboard Dragonfly is a suite of sensors to monitor the Titan surface/subsurface environment. It includes a single-axis (vertical) sensitive seismometer, as well as two sets of small geophones, which are installed on the lander skids, together with temperature and pressure sensors, anemometer for wind speed/direction, measurement of thermal/electrical properties of surface material, and methane and hydrogen sensors. According to the current scenario, the seismometer will be lowered to sit on the ground by a winch at each landing site and protected from the wind loads using a pseudo-streamlined shield. During the seismic observation, the above-mentioned meteorological sensors should be simultaneously operated. Since the selection of Dragonfly mission on NASA New Frontiers Program, a series of laboratory/field tests have been conducting using qualified seismometer models with their proximity electronics, or preamplifier circuits. During these tests, a temperature dependence of sensor characteristic and its performance to measure natural ground motion (what is called ‘microseism’) were investigated at a tunnel of the domestic seismic observatory and/or inside a pressurized cryogenic chamber. The tolerance of Titan’s environment, where the surface would be extremely cold at 94 Kelvin, has been confirmed and several key parameters are clarified to design the flight model of seismometer package. The engineering models of seismometer package are fabricated and their environmental tests for space flight are currently conducted. In this paper, the outline of seismic experiment on Titan and development status of seismometer package will be described.
PS19-A008
| Invited
Strain Estimation Due to the Moon’s Spheroidal Motion Induced by a Gravitational Wave and Preliminary Estimation of the Signal to Noise Ratio Due to Deep Moonquakes Activity
Josipa MAJSTOROVIC1#+, Philippe LOGNONNÉ2
1Université Paris Cité, 2Université Paris Cité, Institut de physique du globe de Paris, CNRS
Gravitational waves (GWs) excite the vibration of all elastic bodies, including bodies such as Earth and Moon. Detecting GWs using the vibrations of the bars was first attempted by Weber in 1960, however without success. In this study we develop an analytical model of the interaction between GWs and the Moon with normal mode summation theory. We use a non-rotating spherical anelastic model of the Moon, constrained by seismic data, while for GWs we consider plane waves defined by three incident angles. We also consider a monochromatic GW source that only interacts with the vertical shear modulus gradient of the Moon. Several findings based on our analysis are made. First, we show that the only excited normal modes are the quadrupole modes of angular order two and that the relative amplitudes of their 5 singlets depend on the GW incident angles. Second, the lunar displacement highly depends on the GW frequencies and is the largest when GW frequency is the same as the frequency of one of the quadrupole modes. Third, the displacement response is highest at the lower frequencies of the Moon’s normal modes around mHz, and drops for high frequencies roughly as f-2. Fourth, we show that we can leverage the maximum of the analytical model by finding the best combination of incident GW angles and the latitude and longitude of the recording station. Next, we study the amplitude sensitivity to the regolith structure by modifying the initial lunar model with more realistic near surface structure. We conclude by providing estimates on the signal amplitude for seismic laser strain meter link with L-configuration which can be used as requirement for designing future Moon based detectors. Finally, we also compare this estimate with the continuous excitation of quadrupole modes by deep moonquakes activity.
PS19-A030
Seismic Observation with DraGMet SEIS
Taichi KAWAMURA1#+, Keisuke ONODERA2, Hiroaki SHIRAISHI3,4, Satoshi TANAKA3, Takefumi MITANI3, Hideki MURAKAMI5, Mark PANNING6, Ralph LORENZ7, Sebastien RODRIGUEZ8, Antoine LUCAS9
1Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 2Okayama University, 3Japan Aerospace Exploration Agency, 4宇宙航空研究開発機構, 5Kochi University, 6Jet Propulsion Laboratory, California Institute of Technology, 7Johns Hopkins University Applied Physics Laboratory, 8Université Paris-Diderot, 9Université Paris Cité
Dragonfly was selected as the 4th New Frontier Mission to explore the astrobiological feature of Titan. Among the suite of instruments on board, the Dragonfly Geophysics and Meteorology Package (DraGMet) is equipped with various geophysical and meteorological sensors to investigate the Titan’s surface and subsurface environment including a vertical short period seismometer. The instrument will be performing the first seismic observation in the icy world and there are huge uncertainties in its seismicity as well as the noise environment. To be well prepared for the observation, we describe here our approach to evaluate the seismic signal and the noise that we expect on Titan. We mainly focus here on atmospheric signals expected for Titan. we take a similar approach as that for InSight. InSight took numerical models of Mars such as Global Circulation Model (GCM) or Large Eddy Simulation (LES) as inputs and evaluated the ground response. This will enable us to evaluate the expected ambient noise as well as transient seismic events from atmosphere. While atmospheric activities act as a significant source of noise, some transient events such as pressure drops can be detected with seismometer and then be used to study subsurface structure and it would be important to have quantitative evaluation on their detectability. We would also discuss some other possible source that were pointed out in previous studies such as cryovolcanoes or geysers. We compare such signals with known instrumental noise and obtained environmental noise to discuss their detectability.
PS19-A016
Source Parameter Inversion Using Adjoint Simulation Based on Single-station Planetary Seismic Data
Lei ZHANG#+, Jinhai ZHANG
Chinese Academy of Sciences
Planet’s interior structure is important for unraveling the geological evolution history. Seismology is one of the most effective methods for the inversion of planetary interior structures. Accurate source information of the seismic events is a critical prerequisite for the inversion of interior structure. Typically, the more seismic stations used in the inversion, the more precise the inverted source parameters are. On Earth, seismic records from tens or even hundreds of stations are applied for earthquake source parameter inversion. In contrast, on extraterrestrial celestial bodies, each mission usually allows for the deployment of only one seismograph; therefore, we usually can only use single-station seismic records before the establishment of a seismic network. Thus, we have to conduct research using the seismic data observed by a single seismograph at the first step, since the traditional methods developed for multi-station records on Earth are no longer suitable. Green’s functions serve as the bridge between the seismic source and recorded data. Conventional seismic source parameter inversion involves multiple calculations of Green’s function from the source point to the station one by one, resulting in expensive computational costs, low inversion efficiency, and difficulties in extending to three-dimensional and/or globally accurate inversions. Here we take advantages of the reciprocity theorem and wavefield back-propagation, employing the spectral-element-method-based adjoint simulation to compute three-dimensional Green’s functions for the entire Mars. Subsequently, we established a seismic source parameter inversion framework based on single-station records. Synthetic benchmark results indicate that this method can exhibit both high computational efficiency and inversion accuracy. Our method benefits from the adjoint simulation and greatly improves the application potential of single-station seismic records on extraterrestrial celestial bodies. We apply this method to the parameter inversion of impact events on Mars recorded by the InSight and further validate its feasibility and reliability. This novel method provides valuable references for the source parameter and interior structure inversions based on single-station lunar seismic records in the near future, such as Chang’e-7 mission and Artemis III.
PS19-A038
A Microseismometer for Venus
William Thomas PIKE1#+, Tibor KREMIC2, Christina ADAMS2, Michael KRASOWSKI2
1Imperial College London, 2NASA Glenn Research Center
We describe here the development of a micromachined silicon seismometer, based on the instrument successfully deployed as part of InSight’s seismic payload, and the first tests under simulated Venus conditions in the Glenn Extreme Environments Rig. The extreme environment of Venus severely the limits the range of materials that can be used for both. However, the silicon sensor of InSight’s microseismometer offers the possibility of adapting a proven approach. The Mars design is based on a through-wafer-etched single-crystal-silicon suspension die incorporating gold sputtered electrodes, an insulating oxide, and electroplated coils. The capacitance between driven electrodes on the proof mass and receiver electrodes on a fixed glass support above the proof mass is used to transduce the seismic signal. These elements are potentially robust enough to operate in a Venus environment. We have adapted the InSight microseismometer design by adopting open-loop sensing and using thermocompressive bonding between the die frame and the glass. While we have demonstrated that open-loop operation does not compromise the noise floor of the device, it means that we no longer can utilize feedback to produce fine centering of the capacitance sensor. We have therefore modified the capacitance topology to allow operation over an enhanced tilt range, taking advantage of the extra die area freed up by the removal of the feedback coils. Initial testing has demonstrated the viability of the fabrication flow for a micromachined sensor adapted from the InSight microseismometer design that provides the potential for operation of seismic sensor on the surface of Venus. In parallel, we are undertaking the coupled development of electronics to drive the sensor’s capacitance transducer, with all operations based in the analog domain, and the packaging approach to allow integration of the sensor and its proximity electronics in a robust package.
Session Chair(s): Chung-Uk LEE, Korea Astronomy and Space Science Institute
PS15-A009
Disk Substructures and Planet Formation
Xuening BAI#+
Tsinghua University
The prevalence of substructures has been established as the new observational paradigm for protoplanetary disks (PPDs), but it remains largely elusive to what extent such substructures are related to planet formation. This talk will first provide a brief overview on recent progress in understanding PPD gas dynamics, followed by a discussion of the two major perspectives disk substructures: being potential causes and/or consequences of planet formation. It is shown that incorporating more realistic PPD gas dynamics, which is primarily governed by weakly-turbulent magnetized disk winds, is crucial to address these questions. Such studies point to efficient planet(esimal) formation in ring-like substructures, and that gap-opening from planet-disk interaction can be much easier than previously thought. The results also call for better understandings of the initial phase of disk formation.
PS15-A001
New Things Learned from Spatially Resolved Observations of Protoplanetary Disks Lately
Ruobing DONG#+
University of Victoria
Planets form in gaseous protoplanetary disks surrounding newborn stars. As such, the most direct way to learn how they form from observations, is to observe them forming in disks. In the past few years, many features in resolved images of protoplanetary disks, such as gaps and spiral arms, have been resolved. They may be associated with embedded (unseen) planets. By comparing observations with theoretical models of planet-disk interactions, the properties of still forming planets may be constrained. Such planets help us test planet formation models. I will introduce the current status of this field and highlight some of the latest developments.
PS15-A005
Streaming Instability: Born Again
Min-Kai LIN#+
Academia Sinica
The ‘streaming instability’ (SI) between dust and gas in protoplanetary disks is the leading mechanism to form planetesimals — the building blocks of planets. However, the simplicity of the SI can be challenged by the complex physics involved in a realistic protoplanetary disk. I describe how turbulence, vertical structure, and thermodynamics can hinder the SI; but also how accretion flows and magnetic fields can help to revive it, albeit in modified forms, which should be investigated in future simulations.
Session Chair(s): Taichi KAWAMURA, Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Doyeon KIM, Imperial College London
PS19-A035
| Invited
Preliminary Analysis of Data Recorded by Instrument for Lunar Seismic Activity Studies at the Landing Site of Chandrayaan 3
Jiju JOHN#+, Sriram K. V., Thamarai V., Teena CHOUDHARY, Srinivasa M. N., Madan Mohan MEHRA, Krishna K., Kalpana ARVIND
Indian Space Research Organisation
Chandrayaan 3 is the first ever mission to land at the south polar region of the Moon with the landing site at 69.37O S and 32.32O E. The lander payload, Instrument for Lunar Seismic Activity studies (ILSA) had the objective of studying the seismicity at the landing site. The seismicity of the lunar equatorial region has been well studied from the data provided by a set of instruments of the Apollo lunar seismic network. The studies by various authors have provided very good insights into planetary seismology of the Moon. After the Apollo era, there have been no major landing missions to Moon for a long time till the Chang’e 3 landed in 2013 and Chang’e 4 landed in 2019. Both these landers did not carry seismic instruments. It can be assumed that after a gap of around fifty years from the arrival of first seismic data from Moon, it is ILSA that has recorded seismic signals from the Moon. It is the first ever records from the lunar polar region. The instrument is first of its kind on the Moon as it employs sensing elements based on silicon micro machining technology, also called Micro Electro Mechanical Systems (MEMS) technology. ILSA has been designed for recording ground accelerations and was deployed on the lunar surface. It had three orthogonally arranged high sensitivity accelerometers in it. ILSA was operated during the lunar day spanning over 24 August 2023 to 02 September 2023. The instrument has recorded several distinct events of which the cause is known for many of them including the navigation of the rover and operation of science instruments involving mechanical activities. Some of the events are not correlated to any known activity. This paper presents the summary of events recorded by ILSA and a preliminary understanding of the data.
PS19-A014
| Invited
Introduction to the Calibration Experiments of the Chang'e 7 Lunar Seismometer
Shengquan ZHANG1+, Qingyu YOU1, Shuang YANG1, Huafeng LIU2, Xiaoqing WANG1, Qing XU1, Jinhai ZHANG1#
1Chinese Academy of Sciences, 2NGL, Huazhong University of Science and Technology
Chang’e-7 mission of China would deploy a seismograph at the landing site to measure the vibration state on the lunar surface, providing scientific basis for the study of the physical mechanism of moonquake formation and the internal structure of the Moon. This seismograph is onboard the bottom of the lander and would be released on the lunar ground after landed. We will present some recent progresses of testing and calibration, including the bandwidth, dynamic range, resolution and sensitivity, confirming that some key technical indicators of the instrument satisfy the requirements and that the calibration parameters meet the requirements of the subsequent scientific data inversion. We would also present some problems encountered in our experiments and our preliminary solutions.
PS19-A001
Newly Discovered Shallow Moonquakes: Temporal and Spatial Distribution
Keisuke ONODERA#+
Okayama University
The first seismic observation on an extraterrestrial body was conducted during the Apollo missions (11, 12, 14, 15, and 16), where two types of seismometers were deployed on the nearside of the Moon. One is a Long-Period (LP) seismometer, which has one vertical and two horizontal components and is sensitive at around 0.2 – 1.5 Hz. The other type is a Short-Period (SP) seismometer with only a vertical component having a high sensitivity at 1 – 10 Hz. In previous studies, the LP data were mainly used for the analysis, contributing to our understanding of the lunar seismicity and the internal structure. On the other hand, because of numerous unnatural signals and/or serious instrumental noises, most of the SP data have remained unexplored. Recently, I analyzed all the SP data and found 22,000 new seismic events, most of which are only identifiable by the SP sensor. The new events include thermal moonquakes, meteoroid impact events, and shallow moonquakes. Among them, I pay particular attention to shallow moonquakes because they are the largest quakes on the Moon and control the seismicity rate. Because of their small number of detections (28 events), shallow moonquakes remained one of the most mysterious quakes. However, identifying 46 new shallow moonquakes enabled me to gain new insight into the seismicity, regionality, and correlation with tidal force. In the presentation, focusing on the temporal and spatial distribution of the newly discovered shallow moonquakes, I would like to discuss their source mechanism and give some implications for future lunar seismic explorations.
PS19-A012
New Constraints on the Focal Mechanism of Deep Moonquakes
Biao YANG+, Jinhai ZHANG#
Chinese Academy of Sciences
Deep moonquakes are the most numerous events observed by Apollo seismographs, which are quite different from deep earthquakes in both waveforms and mechanisms. First, the sources of deep moonquakes are mainly located on the near side of the Moon, while deep earthquakes mainly occur in subduction zones; second, the source depth of deep moonquakes ranges from 700 to 1200 kilometers, which was previously believed to be non-seismic before the Apollo observation; third, the occurrence exhibits significant periodicity, with periods of 13.6 days and 27 days, related to the lunar tidal cycle. For the excitation of deep moonquakes, statistics of the frequency and polarity of moonquakes, and comparison with tidal stress had been conducted in previous studies, and concluded that tidal effects triggered deep moonquakes. But further evidence is lacking. Due to the highly heterogeneous lunar crust, traditional methods of inverting the source mechanism are not valid. The amplitude of seismic wave is affected by geometric diffusion, path attenuation, radiation patterns, and complicated scattering within lunar crust. Due to the deep depth of deep moonquakes, the direct SH wave and the ScSH wave have similar path above the mantle. Therefore, their amplitude ratio is less affected by shallow structures and the geometric diffusion and the path attenuation can be largely corrected. Besides, there is no P-SV wave conversion during the propagation of SH waves, so the amplitudes of the direct SH and ScSH waves are relatively large and easy to pick up. The revised ScSH/SH amplitude ratio can reflect the radiation pattern of focal mechanism thus better constrains the source mechanism of the moonquakes. We use the ScSH/SH amplitude ratio on transverse component, trying to constrain the focal mechanism, and further discuss the relationship between deep moonquakes and tides.
PS19-A021
Farside Seismic Suite (FSS): Lunar Seismology in the CLPS Era
Ceri NUNN1#+, Mark PANNING2, Sharon KEDAR1, Asad ABOOBAKER1, Glenn AVENI3, Kevin BIERNACKI4, Neil BOWLES5, Simon CALCUTT5, Gabrielle CHABAUD3, Melanie DRILLEAU6, Taoufik GABSI3, Raphael GARCIA6, Charlotte GIROUD7, Alain GIVAUDAN4, Anna HORLESTON8, Maurice KARAKAC4, Taichi KAWAMURA9, Thelma LESTAGE10, Philippe LOGNONNÉ11, Josipa MAJSTOROVIC3, Edward MILLER1, David MIMOUN6,12, Tanguy NEBUT3, Sébastien DE RAUCOURT3, Sreejaya KIZHAEKKE PAKKATHILLAM3, Constanza PARDO3, William Thomas PIKE13, Gabriel PONT14, Olivier ROBERT3, Daniel SHEWARD15, Sylvain TILLIER3, Renee WEBER 16, Arnaud WILHELM6
1California Institute of Technology, 2Jet Propulsion Laboratory, California Institute of Technology, 3Université Paris Cité, 4AstroParticule et Cosmologie, 5University of Oxford, 6Institut Supérieur de l'Aéronautique et de l'Espace, 7École Supérieure des Techniques Aéronautiques et de Construction Automobile (ESTACA), 8University of Bristol, 9Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 10Hensoldt Space Consulting, 11Université Paris Cité, Institut de physique du globe de Paris, CNRS, 12University of Toulouse, 13Imperial College London, 14National Centre for Space Studies, 15Observatoire de la Côte d'Azur, 16NASA Marshall Space Flight Center
The Farside Seismic Suite (FSS) will deploy two seismometers to Schrödinger Crater on the Moon’s farside. The seismometers will be deployed on the deck of a commercial lander provided by Draper Laboratory, with a launch scheduled for 2026. FSS was selected to fly under the PRISM (Payloads and Research Investigations on the Surface of the Moon) program, which NASA introduced to provide scientific payloads for the Commercial Lunar Payload Services (CLPS) program. Both of FSS’s seismometers are flight-proven on the Mars InSight mission: the vertical Very BroadBand (VBB) seismometer (the most sensitive seismometer ever built), and the Short Period (SP) sensor, the most mature compact triaxial sensor available for space applications. They are packaged together as a self-sufficient, lander-mounted payload that can survive independently, with power, communications and thermal control allowing continuous operation over multiple lunations. Thus, FSS will outlive the delivery lander, and provide a long-lived seismic experiment capable of: 1) Investigating deep lunar structure and the difference between near and farside seismic activity. 2) Understanding how the lunar crust is affected by the development of an impact melt basin. 3) Evaluating the current micrometeorite impact rate and local tectonic activity. The flight model of FSS is expected to be ready for delivery to the lander in early 2024, and the process is a model for long-lived lunar science in the CLPS and Artemis era, with independent power and communications. The development process tests the advantages of the different risk posture inherent in using commercial landers while still maximizing science return. With the potential for long-lived seismic stations based on the FSS model, this approach shows great promise for building a network of seismic stations that can achieve key science goals outlined in the planetary science decadal survey.
PS19-A027
Simulation of Seismic Ground Motion on the Far Side of the Moon
Sreejaya KIZHAEKKE PAKKATHILLAM1#+, Philippe LOGNONNÉ2, Taichi KAWAMURA3, Mark PANNING4
1Université Paris Cité, 2Université Paris Cité, Institut de physique du globe de Paris, CNRS, 3Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 4Jet Propulsion Laboratory, California Institute of Technology
The Moon's seismic exploration has historically focused on its near side since the deployment of Apollo seismometers in 1969, revealing unique characteristics like low attenuation and high scattering in recorded signals. However, the far side remains largely unexplored due to the absence of seismic data. To address this gap, NASA's Far Side Seismic (FSS) suite is set to launch in 2026 (Panning et al, 2022), targeting the Schrodinger Basin near the south pole. In the absence of actual far-side seismic data, this study relies on physics-based ground motion simulations to comprehend regional seismograms. The current study presents ground motions due to impacts and deep moon quakes on the FSS mission's landing site with a focus on scattering effects. For performing the numerical simulations, a 600km × 600km × 100km regional domain (spanning between latitude 650S - 750S, longitude 1100E - 1600E) is considered. The LROC topography data indicate that the tallest and deepest points in the domain are respectively 5.1km high and 8.1km deep. We have used SPECFEM3D, a spectral element based code for modeling and simulation as handling such significant topography is efficient by this method. The simulation domain is divided into 768 × 768 × 63 elements along the three directions. The mesh is designed such that its coarseness increases along the depth direction. The spatial resolution of the mesh provides a resolvable frequency of 1Hz and there are total of 4.62 billion degrees of freedom in the computational model. The simulations explore topography's impact on moon seismograms and analyze how features like 3D crust, random heterogeneity, faults in the crust, and basin geometry influence ground motion scattering. Through these simulations, the study aims to provide insights into the seismic characteristics of the Moon's far side, anticipating valuable data from the FSS suite in the near future.
PS19-A032
Lunar Optical Very Broad Band Seimometer
Sébastien DE RAUCOURT1#+, Gabrielle CHABAUD1, Raphael GARCIA2, Frédéric GUATTARI3, Frans IJPELAAN4, Taichi KAWAMURA5, Philippe LOGNONNÉ6, Tanguy NEBUT1, Gabriel PONT4, Olivier ROBERT1, Carla SANNA7, Sylvain TILLIER1
1Université Paris Cité, 2Institut Supérieur de l'Aéronautique et de l'Espace, 3MAÅGM, 4National Centre for Space Studies, 5Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 6Université Paris Cité, Institut de physique du globe de Paris, CNRS, 7Exail
The Apollo seismic experiment provided unique Moon seismology data, however understanding and knowledge on the Moon interior structure is limited its performances. 50 years later, the Mars seismometer Insight/SEIS demonstrated lower self-noise and better resolution. A spare model will be sent to the Moon in 2026 with the FSS (CLPS 12) mission. However, it is far from meeting the International Lunar Network (ILN) requirements. To meet those requirements, technological breakthrough is needed. By switching from electrostatic displacement sensors to interferometer, an improvement of several orders of magnitude is made on parasitic force (electrostatic noise to pressure radiation). The Lunar Optical Very Broad Band Seismometer is made of two subsystems: a mechanical oscillator and a displacement sensor. The mechanical oscillator is guided by a four blades hinge and equilibrate by a leaf-spring. It has a heavy proof mass (1Kg) and a low normal frequency (0.22Hz) to ensure low suspension noise. A locking device will hold the mobile part during launch and landing. The displacement sensor is based on a Michelson interferometer implemented on the sensors head and a laser source and optical readout electronic deported at the end of a single optical fiber. With this design, we have a very robust and simple sensor head that withstand high temperature range (-80°C to + 60°C) and a high performances electronic remaining in the warm enclosure of the lander. The tether in between is simple with only 2 copper wire and an optical fiber per axes. To minimize risk, the design benefits from high heritage. The mechanical oscillator uses the same technology – but different geometry for the pivot and spring. The optical readout technology is inherited from Fiber Optics Gyroscopes widely use in space. Prototype is under integration. This instrument will be candidate for all flight opportunities around 2030 (launch date).
Session Chair(s): Ing-Guey JIANG, National Tsing Hua University
PS15-A039
Origin of the GJ 1148 Planetary System by Planet-planet Scattering
Man Hoi LEE#+, Longhui YUAN
The University of Hong Kong
The GJ 1148 system has two Saturn-mass planets orbiting around an M dwarf star on eccentric orbits (e = 0.375 for both planets), with orbital periods of 41.4 and 532 days. The inner planet is in the regime of eccentric warm Jupiters. We have performed numerical experiments to study the planet-planet scattering scenario for the origin of this orbital architecture. We consider a third planet of 0.1 or 0.227 MJ (Jupiter’s mass) in the initial GJ 1148 system with initial orbital separations of 3.5, 4, and 4.5 mutual Hill radii. The majority of scattering results in planet-planet collisions, followed by planet ejections, and the removal of planets that come too close to the star. Among them, only the post-ejection two-planet systems have similar properties to the GJ 1148 system. Therefore, the simulation results suggest that the GJ 1148 system may have lost a giant planet. We have also performed simulations of the general problem of the origin of warm Jupiters by planet-planet scattering. As in the GJ 1148 simulations, a non-trivial number of stable two-planet systems are produced by ejection, which disagrees with the result from another study showing that two-planet systems arise exclusively through planet-planet collisions.
PS15-A008
Spin and Seasonal Variations for Planets in Compact Systems
Gongjie LI1#+, Howard CHEN2, Andre SUZANNE1
1Georgia Institute of Technology, 2Florida Institute of Technology
Spin variations of planets determine day-night cycles and seasonal variations, playing a crucial role in planetary habitability. In compact systems, particularly in proximity to the host star, strong tidal interactions with the host star and significant perturbations due to companion planets lead to chaotic variations in planetary spin-axis. This allows planets to escape tidal locking. In this study, we present the first detailed analysis of the 3D dynamics of planet spin-axis in compact systems with strong tidal interactions. We characterize the resulting statistical properties in both day-night cycles and long-term obliquity (seasonal) variations depending on different system parameters. Applying this analysis to TRAPPIST-1, we illustrate that obliquity variation due to secular spin-orbit resonances plays an important role for the habitable zone planets, and they can result in more significant day-night variations. In addition, we illustrate the dynamical effects on planet climate using 3-d global climate models.
PS15-A024
How Different Stellar Environments Shape the Planetary Systems
Huigen LIU#+
Nanjing University
Star forms in clusters and stellar environments vary a lot across the galaxy, which usually indicate different star formation rate, as well as the planetary formations. This talk focuses on both dynamical and radiative stellar environments, and discuss how the effects on planetary systems from the stage of protoplanetary disk in the first ~10 Myrs, and the dynamical evolution in the next ~Gyrs. Current sample of transiting planets in clusters provide some clues and constraints on different effects. E.g. the photoevaporation of external FUV and EUV can shorten the lifetime of gas disk, while the Lidov-Kozai effect makes the HJs form earlier and easier in dense stellar environments. More exoplanets detected in extreme environments are needed, for comparison. The China Space Station Telescope (CSST) would have the ability to detect the transiting HJs around the Galactic Halo, and will provide a good sample to compare with transiting planets detected via Kepler and TESS.
PS15-A022
Occurrence Rate as a Function of Stellar Age: Probing the Evolution of Exoplanetary Systems
Kento MASUDA1#+, Shota MIYAZAKI2
1Osaka University, 2Japan Aerospace Exploration Agency
Exoplanets orbiting close to their host stars may undergo various changes in their orbits and physical properties. For example, it has long been discussed that the shortest-period planets may have orbits unstable to tidal dissipation and spiral into their host stars. Recent transit observations of low-mass planets have also provided evidence for evaporation of their atmospheres, which provides clues to the internal composition of those planets. The stellar age dependence of the planet occurrence serves as a direct probe of such evolution. However, the accurate derivation of this dependence is fraught with challenges, including large uncertainties in estimating stellar ages and the difficulty of disentangling the age dependence from the dependence on other stellar parameters (e.g., mass and metallicity) that are correlated with age. We are therefore developing a statistical framework for estimating the planet occurrence as a function of various stellar parameters, fully taking these issues into account. In this talk, I will give an overview of the methodology, present the results of its application to a sample of gas giants from Doppler surveys, and discuss its potential applications for future surveys.
PS15-A013
An Easy Converging MCMC Code and Its Application to Exoplanet Science
Sheng JIN#+
Anhui Normal University
We introduce an automatic parallel tempering Markov Chain Monte Carlo (APT-MCMC) code that enables rapid convergence in the sampling of complex distributions. The code(Nii-C)has two advantages. First, an initial tuning stage is implemented to automatically adjust the proposal distributions for all model parameters across all parallel tempering chains as an MCMC sampler moves towards the global optimum. This can ensure that the real-time sampling acceptance rates are in the ideal range when the sampler explores different regions of a probability distribution. Second, Nii-C is a pure C language code and its parallel tempering algorithm is implemented using the Message-Passing Interface (MPI) protocol, which guarantees its fast execution speed. To facilitate the adaptation of the Nii-C code to different posterior distributions faced by various Bayesian analysis models, the user-defined prior and likelihood functions were designed to be as independent as possible and isolated into two separate source files. As examples, we provide two template applications in exoplanet science: one is a hierarchical radius relationship, and the other is a planetary orbital fitting model. The results of these models demonstrate the superiority of Nii-C in terms of speed and convergence capability.
PS15-A034
The Period-eccentricity Relation of Small Planets as a Probe Into the Initial Mass Distribution in the Protoplanetary Disk
Ke-Ting SHIN+, Ji-Wei XIE#
Nanjing University
From the 1990s to the early 21st century, the orbital eccentricities of spectroscopic binary stars and Doppler gas giant planets were found to decrease as their orbital periods shrink. This is apparently in line with people's expectation because gravitational tidal interactions damp eccentricities of close in bodies with short periods, and it places important constraints on tidal theories. In recent years, many smaller planets, e.g., super-Earths and sub-Neptunes, have been discovered, and it is wondered that whether they follow the similar pattern as their larger counterpart. Here, by compiling data from various exoplanet catalogs, we found that for small planets, in contrast to their larger counterpart, their eccentricities increase as their orbital periods decrease. Nevertheless, such a pattern is similar to that of our Solar system (Mercury, the small planet with the shortest orbital period has the largest eccentricity), and both can be explained by a common mechanism which transfers angular momentum deficit (AMD) inward and thus pumps up the eccentricities of inner small planets. Such similarity implies that some dynamical evolution processes have happened both inside and outside the Solar system. Furthermore, by fitting with the AMD model, the observed anti-correlation between orbital period and eccentricity of small planets actually places crucial constraints on the initial planetary disk condition (disk surface density profile) of planet formation.
PS15-A012
Inner Edges of Planetary Systems: Architectures and Stellar-mass-dependence
Mengfei SUN#+, Ji-Wei XIE
Nanjing University
The position of the innermost planet in a planetary system reflects the relationship of the entire system to the host star. This could provide more potentially important information about planetary formation and evolution processes. Here we use the $Kepler$ Data Release 25 (DR25) catalog, combined with LAMOST DR9, Gaia DR3, and California-Kepler Survey (CKS) catalog, to analyze and control the influence of stellar metallicity, stellar age, and observational bias to study the correlation between stellar mass and inner edge position. Previously, we analyzed these several stellar parameters using machine learning models and found that stellar mass dominates the relationship with the inner edge position. Finally, a consistent conclusion was obtained under the three data sets: as the stellar mass increases, the position of the inner edge will also increase significantly. The correlation between stellar mass and the inner edge is $0.765_{-0.042}^{+0.041}$. When analyzing single-planetary systems and multi-planetary systems respectively, the correlations between stellar mass and the inner edge are $0.696_{-0.044}^{+0.044}$ and $0.803_{-0.060}^{+0.061}$ respectively. Further comparing the observed statistical analysis results with the current analysis model, it was found that the most consistent theoretical models are pre-main-sequence (PMS) dust sublimation radius of a passive disk, an actively accreting disk with q = 1, and planet destruction by stellar tides. In addition, we found that the outer edge also shows a certain trend as the inner edge changes, so we will further discuss and analyze the theory of planetary system formation and evolution.
Session Chair(s): Doyeon KIM, Imperial College London, Philippe LOGNONNÉ, Université Paris Cité, Institut de physique du globe de Paris, CNRS
PS19-A019
| Invited
The Seismicity of Mars
Simon STAEHLER1#+, Savaş CEYLAN2, John CLINTON2, Nikolaj DAHMEN1, Cécilia DURAN1, Anna HORLESTON3, Taichi KAWAMURA4, Doyeon KIM5, Géraldine ZENHÄUSERN1, Domenico GIARDINI1, Philippe LOGNONNÉ6, Anna MITTELHOLZ1
1ETH Zurich, 2Swiss Seismological Service, 3University of Bristol, 4Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 5Imperial College London, 6Université Paris Cité, Institut de physique du globe de Paris, CNRS
Mars is the first planet on which earthquakes (“marsquakes”) were observed in situ and clearly connected to active tectonic units on the surface1-3. Mars shows no traces of plate tectonics, so pre-InSight the dominant tectonic process was assumed to be secular cooling and thus contraction of the lithosphere. Geological mapping of the surface had indicated many traces of recent volcanic activity and significant parts are covered by volcanic units4. The InSight seismic dataset localizes more than half of the observed seismic activity in Cerberus Fossae2, a young (<10 Ma5) graben structure in Elysium Planitia, previously interpreted as a result of dyke intrusion6 or large-scale tectonic stress5. Spectral analysis of marsquakes observed in this region show a warm, elastically weakened source region7, e.g. due to partial melting at lithospheric depths8 or deformation due to a mantle plume9. The significant contribution of this small region to Mars’ global seismic budget means that volcanism shapes the planet’s surface at a higher rate than contraction. We discuss the mechanisms of Martian seismicity as they are currently understood and their relation to orbitally observed tectonics. References: 1W. B. Banerdt et al., Nat. Geosci. 13, 183–189 (2020). 2D. Giardini et al., Nat. Geosci. 13, 205–212 (2020). 3P. Lognonné et al., Nat. Geosci. 13, 213–220 (2020). 4K. L. Tanaka et al., US Geol. Surv. Geol. Investig., 3292–3292 (2014). 5J. Vetterlein, G. P. Roberts, J. Struct. Geol. 32, 394–406 (2010). 6R. Ernst et al., Annu. Rev. Earth Planet. Sci. 29, 489–534 (2001). 7S. C. Stähler et al., Nat. Astron. 6, 1376–1386 (2022). 8A.-C. Plesa et al., in Advances in Geophysics, vol. 63, pp. 179–230 (2022). 9A. Broquet, J. C. Andrews-Hanna, Nat. Astron., 1–10 (2022).
PS19-A005
| Invited
Present Day Structure and Long-term Evolution of Mars Inferred from Insight Data
Henri SAMUEL1#+, Melanie DRILLEAU2, Attilio RIVOLDINI3, Raphael GARCIA2, Vedran LEKIC4, Jessica IRVING5, Zongbo XU1, James BADRO1, Philippe LOGNONNÉ6, James CONNOLLY7, Constantinos CHARALAMBOUS8, William Thomas PIKE8, Benjamin FERNANDO8, Quancheng HUANG4, Taichi KAWAMURA9, Tamara GUDKOVA10, William Bruce BANERDT11
1Institut de Physique du Globe de Paris, 2Institut Supérieur de l'Aéronautique et de l'Espace, 3Royal Observatory of Belgium, 4University of Maryland, 5Bristol University, 6Université Paris Cité, Institut de physique du globe de Paris, CNRS, 7ETH Zurich, 8Imperial College London, 9Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 10Russian Academy of Sciences, 11California Institute of Technology
During almost four years of operations between November 2018 and December 2022, the instruments from the InSight mission have collected various types of observations, such as atmospheric data, or magnetic and geodetic measurements, in addition to the first seismic data recorded at the surface of Mars. The analysis of this diverse geophysical dataset has not only allowed one to constrain the present-day structure of the Mars from the surface down to its core, but also to reconstruct its long-term thermal and chemical history. In particular, the inversion of seismic data collected by the SEIS instrument has revealed distinct present-day interior structures between the Red Planet and the Earth or the Moon, possibly resulting from early diverging evolutionary paths followed by these three terrestrial bodies. Despite its unique character, exploiting this singular set of observations - resulting for a large part from the fact that the InSight seismic network is constituted of a single station and a few dozens of exploitable events - has required developing original approaches specifically tailored for the context of the mission, using post-landing information. This has allowed to progressively refine the knowledge on Mars while gradually improving the techniques to interpret the growing dataset being collected. I will review several strategies we developed and applied to exploit this unique dataset along with major discoveries made during the course of the mission and after the cessation of the InSight lander activity at the end of 2022, along with future multi-disciplinary strategies to further extract the abundant and unexploited information still present in this geophysical record.
PS19-A003
Structure of the Martian Crust Below Insight from Surface Waves and Body Waves Generated by Nearby Meteoroid Impacts
Melanie DRILLEAU1#+, Eric BEUCLER2, Jing SHI3, Brigitte KNAPMEYER-ENDRUN4, Raphael GARCIA1, Veronique ANSAN2, Doyeon KIM5, Philippe LOGNONNÉ6, William Bruce BANERDT7
1Institut Supérieur de l'Aéronautique et de l'Espace, 2Nantes Université/ Université d’Angers/ Le Mans Université/ Centre National de la Recherche Scientifique, 3Université Paris Cité, 4German Aerospace Center, 5Imperial College London, 6Université Paris Cité, Institut de physique du globe de Paris, CNRS, 7California Institute of Technology
The knowledge of the crustal structure of Mars is essential for understanding the formation and evolution of the planet. Thanks to the very broadband seismometer of the InSight mission landed on the surface of Mars (now switched off after four terrestrial years of operation), seismic signals generated by meteorite impacts have been recorded. Five craters have been identified by orbital imaging to be located within a circle of 250 km radius around the lander. For two of these meteorite impacts, we successfully measured surface waves, which are mostly sensitive to the crustal structure in the first kilometers below the InSight lander. Using the two measured group velocity dispersion diagrams, in combination with body wave arrival times from five impact events, we obtained direct seismic constraints on the seismic velocity of the crust in the vicinity of the InSight landing site. Bayesian joint inversions of surface and body waves show a four-layer model for the Martian crust, compatible with high and low frequency P-wave receiver functions (PRFs) estimated in previous studies. We confirmed the existence of a uppermost low-velocity layer with a mean thickness of 1.2±0.2 km on average and Vs = 1.5±0.1 km/s, interpreted as cratered and tectonically deformed, layered volcanic (basaltic) materials, possibly interstratified with sedimentary and altered materials. A second layer of more cohesive material, possibly made of basaltic materials mixed with felsic rocks, is constrained with a bottom depth located at 11.5±3.1 km, and Vs = 2.4±0.2 km/s. Comparison with PRFs calculated in previous studies allows to select models compatible with all observations, and to define a seismic velocity model of the whole crust below InSight.
PS19-A010
Unraveling Marsquake Epicenters and Martian Tectonics Through Seismic Anisotropy Analyses
Jiaqi LI#+
Peking University
The NASA's InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander mission (2018-2022) recorded over 1,300 marsquakes during its four-year operation, demonstrating Mars as an active seismic environment. Though the successful detection of marsquakes stands as a noteworthy achievement of the mission, the crucial subsequent task of accurately locating these marsquakes remains substantially unfulfilled. For instance, less than 20 (only ~2%) of the detected marsquakes have been located using conventional locating algorithms, and their epicenters have large uncertainties and display a vague alignment with the distribution of known faults on Mars. Consequently, these limited and poorly located marsquakes hinder our understanding of marsquake mechanisms and their relation to Martian tectonics. To address this problem, we propose to develop an innovative marsquake locating algorithm for the InSight seismic station on Mars in this research proposal. This algorithm will enhance the accuracy of existing marsquake epicenter estimations, facilitate the placement of previously identified but unlocated marsquakes on the map, and constrain the properties of crustal seismic anisotropy on Mars. Our results will allow us to better comprehend the mechanisms underlying Martian seismic activity and illuminate the planet's current tectonics. Furthermore, understanding the nature of seismic anisotropy will provide insights into the composition and evolutionary history of the Martian crust. If anisotropy serves as an indicator of impact-induced porosity, it will reveal the crust's capacity of storing water and the potential for fluid migration, offering insights into the possible habitability on Mars. The new relocation algorithm also has the potential to be applied beyond Mars, facilitating event relocation in icy environments like Titan and Enceladus.
PS19-A015
Upper Mantle Low Velocity Zones of Mars Revealed by Receiver Functions and SS Precursors of InSight Seismic Data
Mingwei DAI+, Daoyuan SUN#, Zhu MAO, Huixing BI
University of Science and Technology of China
The detailed velocity structures of the Martian lithosphere provide crucial insights into the content of heat-producing elements, the thermal and compositional properties, and the differentiation process of Mars. In this study, we identify a robust negative Ps converted wave and related multiple phases in the receiver functions (RFs) of six high-quality marsquakes. These negative arrivals suggest the existence of a low-velocity zone (LVZ) in the upper mantle beneath the InSight landing site. Furthermore, for more distant events S1153a and S0976a, we observe strong negative SS precursors ~40–50 s before the SS waves, indicating a potentially widespread distribution of the LVZ. We perform the inversions to fit the waveforms of RFs and the SS precursors. The LVZ beneath the InSight landing site has a depth of 68 ± 5 km with a Vs reduction of 11% ± 4%. In contrast, the LVZs below the SS bounce points of S1153a and S0976a are more extreme, with LVZ depths and Vs reductions of ~90 km and ~40%, respectively. Taking into account the locations of these identified LVZs, we propose that these upper mantle LVZs are likely associated with partial melting induced by the mantle plume beneath Elysium Planitia.
PS19-A018
Investigating Subsurface Structure at the InSight Landing Site with Multiple Datasets
Wanbo XIAO1#+, Yanbin WANG1, Sebastián CARRASCO2, Zongbo XU3, Keisuke ONODERA4, Philippe LOGNONNÉ5, Taichi KAWAMURA6, Marouchka FROMENT7
1Peking University, 2University of Cologne, 3Institut de Physique du Globe de Paris, 4Okayama University, 5Université Paris Cité, Institut de physique du globe de Paris, CNRS, 6Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 7Université Paris Cité
The InSight mission is the most successful Mars mission that collected massive seismic data from Mars, which provides great opportunity for Martain seismology studies. The subsurface structure at the InSight landing site contains information of the recent evolution of Mars’ surface. However, different studies using different datasets presented different subsurface velocity profiles at the InSight landing site. In order to reduce the non-uniqueness of the subsurface structure inversion, we utilized multiple datasets as proposed in previous studies to jointly constrain the subsurface structure at the InSight landing site, including the H/V spectral ratio curve of marsquakes, compliance curve of convective vortex, and H/V compliance ratio of impact-generated infrasound. We first analyzed the sensitivity kernels of different datasets to help design the joint inversion. Then we included model prior information to make the model more physically reasonable. The inverted velocity profiles exhibit less S-wave velocity uniqueness than previous results, indicating a high-velocity layer underlain by a low-velocity in the shallow 100 m and a velocity transition layer in the Martian crustal top layer. These results are also well consistent with the current geological background of the study region.
PS19-A025
Solid/atmosphere Moment Partitioning in Hypervelocity Impacts on Mars from SEIS Recorded Seismic and Acoustic Signals and High Resolution Crater Imaging
Philippe LOGNONNÉ1#+, Carys BILL2, Gareth COLLINS2, Ingrid DAUBAR3, Doyeon KIM2, Benjamin FERNANDO2, Marouchka FROMENT4, Raphael GARCIA5, Taichi KAWAMURA6, Carène LARMAT7, Katarina MILJKOVIC8, Esteban ROUGIER7, Zhongbo XU4, Lei ZHOU7
1Université Paris Cité, Institut de physique du globe de Paris, CNRS, 2Imperial College London, 3Brown University, 4Université Paris Cité, 5Institut Supérieur de l'Aéronautique et de l'Espace, 6Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, 7Los Alamos National Laboratory, 8Curtin University
The SEIS VBB sensor detected 10 confirmed impacts on Mars, documented by both the seismic signal and the high-resolution imaging of the formed crater. For about half of them, a chirp in the seismic signal was also detected, which was generated by the ground shaking generated by infrasounds generated by the impact. At several detected impact sites, high resolution images show the imprint of the blast with a notable occurrence on Sol 1094, dated 12/24/2021, marking the largest impact detected by the InSight mission. The seismic source is constrained by the amplitude of seismic body waves, or surface waves for S1094b, and the imaged crater diameter. The acoustic source is constrained by the amplitude of indirect infrasounds and the imaged diameter of the blast zone. This allows two different estimations of these two sources: the first is the one acting on the ground, therefore associated with the seismic source while the second is acting just above the surface therefore associated with the acoustic source, each being expressed by seismic or acoustic moment, respectively. Comparing the seismic and acoustic moments for those confirmed impacts will provide the first estimation of the energy partitioning between ground and air for high velocity impacts on Mars, characterized by speeds and energies furthermore never recorded on Earth. We present here preliminary results of this analysis made with different seismic and hydrocode modeling and discuss the impact of seismic scattering, lateral variations, subsurface structure and atmospheric attenuation in our estimations of the seismic and acoustic moments and associated energy/moment partitioning.
PS19-A036
Are Insight 1-d Interior Models Good Enough: a Perspective Based on 3-d Crustal Models and Body Wave Travel Times
Doyeon KIM1#+, Melanie DRILLEAU2, Cécilia DURAN3, Domenico GIARDINI3, Jessica IRVING4, Brigitte KNAPMEYER-ENDRUN5, Vedran LEKIC6, Philippe LOGNONNÉ7, Mark PANNING8, Ana-Catalina PLESA5, Henri SAMUEL9, Mark WIECZOREK9
1Imperial College London, 2Institut Supérieur de l'Aéronautique et de l'Espace, 3ETH Zurich, 4Bristol University, 5German Aerospace Center, 6University of Maryland, 7Université Paris Cité, Institut de physique du globe de Paris, CNRS, 8Jet Propulsion Laboratory, California Institute of Technology, 9Institut de Physique du Globe de Paris
Travel time measurements of seismic waves on Mars have led to foundational discoveries about the spherically symmetric structure of the crust, mantle, and core. However, more than three quarters of these measurements are predominantly sensitive to the lithospheric structure between Elysium Planitia and Cerberus Fosse and inferences about global structure assume that the crustal structure directly beneath the InSight’s lander is representative of average Martian crust. This assumption can significantly bias our models of the global interior structure and dynamics of Mars. Here, we assess the goodness of our existing 1-D models of Mars by considering a 3-D seismic velocity model of the martian crust, in which global crustal thickness variations are determined by gravimetric modeling, using two seismic anchoring points: the crustal thickness estimates at the lander based on receiver function analyses and away from the lander from group velocity measurements of multiple orbit Rayleigh waves in S1222a. Using the fast marching algorithm, we perform 3-D ray tracing with our models and produce a series of global maps of crustal travel time correction for body wave measurements documented in the latest marsquake catalog by the Marsquake Service. Serendipitously, the source regions for most seismic events are ones for which 1-D models are sufficient for modelling travel times with direct P and S arrivals. However, care must be taken when incorporating travel time constraints from events located in other clusters outside the Cerberus Fosse and when utilizing PP, SS, PPP, and SSS data. Our work enables a refinement of our existing 1-D interior models and evolution of Mars, as well as marsquake locations and mechanisms.
PS19-A037
InSight Seismic Data Reveals the Signature of a New Intermediate-sized Impact Candidate
Constantinos CHARALAMBOUS1#+, Benjamin FERNANDO1, William Thomas PIKE1, Joe MCNEIL2, Valentin T. BICKEL3, Gareth COLLINS1, Ingrid DAUBAR4, Raphael GARCIA5, Anna HORLESTON6, Doyeon KIM1, Philippe LOGNONNÉ7, Aleksandra SOKOLOWSKA4, Simon STAEHLER8, Natalia WOJCICKA1, Savana WOODLEY9, Géraldine ZENHÄUSERN8, Bruce BANERDT10
1Imperial College London, 2Natural History Museum, 3University of Bern, 4Brown University, 5Institut Supérieur de l'Aéronautique et de l'Espace, 6University of Bristol, 7Université Paris Cité, Institut de physique du globe de Paris, CNRS, 8ETH Zurich, 9Open University, 10Jet Propulsion Laboratory
During its over four years of Mars surface operations, NASA's InSight mission has seismically detected eight meteoroid impact events associated with craters identified in orbital images, ranging from a few meters to 150 meters in diameter. However, these events were either at epicentral distances closer than 5 degrees (~300 km), localized through seismo-acoustic signals, or further than 60 degrees (~3500 km). It is unlikely that seismically detectable impacts have not occurred at intermediate distances, but until now it has not been possible to associate a seismic event with craters that have been observed to form during the mission. We can now report the identification of a seismic signature associated with an impact crater >10 m in diameter confirmed by orbital imaging. Using the event azimuth determined from the S-wave arrival, we associate a new crater with formation dates consistent with this event. The seismic signal also indicates the presence of candidate surface waves, as seen for two other confirmed teleseismic impact events and some nearby impacts. The intermediate size and distance of this event serves as a crucial anchor point, bridging the gap between recent nearby and distant impacts. This event re-calibrates earlier estimates of Very-High Frequency (VF) event locations, redefining the search area to identify other seismic events associated with impacts formed within InSight's lifetime. The event also presents a rare opportunity to study differences in seismic wave behavior between events with shallow and deeper sources, facilitating comparisons in source geometry and dynamics. The acquired data not only enhances understanding of the local geological context but also establishes a crucial reference point for exploring seismic wave propagation in intermediate epicentral distances, paving the way for comprehensive planetary seismology studies.
Session Chair(s): Fei DAI, University of Hawaii
PS15-A026
Eccentric Migration: A Unified Evolution Story for Hot Jupiters
Songhu WANG#+
Indiana University
The first discovered extrasolar worlds — giant, "hot Jupiter" planets orbiting perilously close to their parent stars — came as a surprise to solar-system-centric models of planet formation, prompting the development of numerous new theories in the past several decades. Among these, the high-eccentricity tidal migration theory has been particularly effective in explaining the dearth of nearby planetary companions to Hot Jupiters, as well as their observed spin-orbit misalignments. In this talk, I will delve into our new findings that challenge conventional wisdom and present complex dynamical characteristics for Hot Jupiters. Firstly, contrary to the notion of their "loneliness," we have demonstrated, through a careful analysis of the full four-year Kepler dataset, that at least 12% of hot Jupiters have additional nearby planetary companions. This observation implies that at least a fraction of hot Jupiters likely underwent a dynamically "cool" formation process, enabling them to retain nearby companions. Additionally, we have found that warm Jupiters exhibit spin-orbit alignment irrespective of their host stars' properties, indicating that the observed misalignment in hot Jupiter systems may be specific to their unique, dynamically hot migration paths rather than a universal phenomenon affecting other classes of giant planets. Current theories have been either too dynamically "cool" or "hot" to fully account for the observed properties of hot Jupiters. To reconcile these inconsistencies, we introduce a new, unified paradigm for hot Jupiter formation that aligns with all current lines of evidence.
PS15-A006
Evidence for Hidden Nearby Companions to Hot Jupiters and Its Implication on the Formation of Hot Jupiters
Donghong WU#+
Anhui Normal University
The formation of hot Jupiters has long been a subject of interest in the field of exoplanet science. The near absence of observed nearby planetary companions to hot Jupiters are widely quoted as evidence in support of high-eccentricity tidal migration, a framework in which hot Jupiters form further out in their natal protoplanetary disks before being thrown inward with extremely high eccentricities, stripping systems of any close-in planetary companions. We present new results from a search for transit timing variations across the full 4 yr Kepler data set, demonstrating that at least 12% ± 6% of hot Jupiters have a nearby planetary companion. This subset of hot Jupiters is expected to have a quiescent dynamical history such that the systems could retain their nearby companions. As a comparison, we find that about 70% ± 16% warm Jupiters possess nearby companions. We propose an “eccentric migration” framework for the formation of short-period giant planets through postdisk dynamical sculpting in compact multiplanet systems by combining our results with existing observational constraints. As a part of the framework, we conduct N-body simulations focusing on the formation of hot Jupiters via the disruption of resonant chains after the gas disk disappears. We find that the resonant chains are prone to instability following the dispersal of the gas disk, with more than 80% of instabilities occurring within 3 million years. Our simulations indicate that 33% ± 4% hot Jupiters and 70% ± 4% warm Jupiters could possess nearby companions. Furthermore, incorporating the effects of general relativity and tidal dissipation increases the isolation of hot Jupiters, resulting in nearby companion occurrence rates of 20% ± 4% for hot Jupiters and 69% ± 6% for warm Jupiters.
PS15-A004
The Formation of Hot Jupiter with Its Nearby Companions Subject to Atmospheric Mass Loss
Su WANG1#+, Chelsea, X. HUANG2, D.N.C. LIN3, Xiaochen ZHENG4
1Chinese Academy of Sciences, 2University of Southern Queensland, 3University of California, Santa Cruz, 4Beijing Planetarium
Gas giants in transiting multiple planetary systems are intrinsically much rarer compared to the transiting multiple planetary systems only host Super-Earth/Sub-Neptunes. Compared with the low-mass multiple planetary systems, the occurrence rate of multiple planetary systems with gas giants with longer periods increases and there is a pile-up near the 2:1 mean motion resonance. We investigate the configuration formation of short-period gas giant and its low-mass nearby planetary companions under the influence of the orbital migration of planets in the protoplanetary disk, the post orbital evolution influenced by the atmospheric mass loss and tidal effect induced by the central star. With higher mass loss fraction and shorter orbital period of gas giant, the mutual inclination can be excited to higher value which is a possible reason of more gas giant multiple planetary system with longer periods have been observed. The simulation results is consistent with the observed period ratio obtained from Kepler mission with a mass loss fraction less than 15% of its total mass. The planets in the observed giant multi-transiting systems may not lose too much atmosphere. And we predict 1-2 systems existed in TESS data with a single transiting super-earth within period of 10 days with TTV amplitude higher than three minutes due to a non-transiting gas giant.
PS15-A016
Atmospheric Circulation of Hot Jupiters: Roles of Clouds
Xianyu TAN#+
Shanghai Jiao Tong University
Clouds play a significant role in shaping planetary atmospheres. Observationally, clouds tend to mute spectral features, obscuring our inference of fundamental parameters of planetary atmospheres such as abundances and structure measurements. On the other hand, clouds in hot Jupiters' atmospheres, due to their strong radiative effects in high-temperature atmospheres and their coupling with atmospheric flows, facilitate a new window to probe climate dynamics in a regime that has never been encountered in our solar system planets. For both reasons, understanding clouds in a self-consistent dynamical framework is vital. This presentation will update our latest findings of cloud dynamics and their consequences on atmospheric heat transport and observational signatures of spectrum based on general circulation models of hot Jupiters.
PS15-A023
Understanding the Planetary Formation and Evolution in Star Clusters (UPiC). I. Evidence of Hot Giant Exoplanets Formation Timescales
Yuanzhe DAI+, Huigen LIU#, Jiayi YANG, Ji-Lin ZHOU
Nanjing University
Planets in young star clusters could shed light on planet formation and evolution since star clusters can provide accurate age estimation. However, the number of transiting planets detected in clusters was only $\sim 30$, too small for statistical analysis. Thanks to the unprecedented high-precision astrometric data provided by Gaia DR2 and Gaia DR3, many new Open Clusters(OCs) and comoving groups have been identified. The UPiC project aims to find observational evidence and interpret how planets form and evolve in cluster environments. In this work, we cross-match the stellar catalogs of new OCs and comoving groups with confirmed planets and candidates. We carefully remove false positives and obtain the biggest catalog of planets in star clusters up to now, which consists of 73 confirmed planets and 84 planet candidates. After age validation, we obtain the radius--age diagram of these planets/candidates. We find an increment of the fraction of Hot Jupiters(HJs) around 100 Myr and attribute the increment to the flyby-induced high-e migration in star clusters. An additional small bump of the fraction of HJs after 1 Gyr is detected, which indicates the formation timescale of HJ around field stars is much larger than that in star clusters. Thus, stellar environments play important roles in the formation of HJs. The Hot-Neptune desert occurs around 100 Myr in our sample. Combining photoevaporation and high-e migration may sculpt the Hot-Neptune desert in clusters.
PS15-A019
Early Accretion of Large Amount of Solids for Directly-imaged Exoplanets
Ji WANG#+
The Ohio State University
As the number of planetary mass objects (PMOs) at wider separation grows, there is emerging evidence that they form differently from their higher-mass brown-dwarf (BD) counterparts. Namely, PMOs' atmospheres are enriched by metals which is usually interpreted as a sign of solid accretion. However, there has been no quantitative analysis at population level to investigate the amount and timing of solid accretion. Here, we analyze a sample of directly-imaged exoplanets and show that these PMOs accrete large amount of solids. On average >100 Earth-mass solids (ranging from 72.3 to 885.7 Earth masses) are accreted to enrich planet atmospheres if forming via core accretion whereas the solid accretion needs to be 20 Earth masses if forming via gravitational instability. The result implies that the solid accretion process has to happen at an early stage (<1 Myr) when large amount of solids are available in young protoplanetary disks.
PS15-A002
Atmospheric Characterization and Formation of Super-jovian Exoplanets Under High Spectral Resolution
Yapeng ZHANG#+
California Institute of Technology
High-resolution spectroscopy (R>30000) provide great opportunities to carry out detailed atmospheric characterization of directly imaged exoplanets. Ongoing spectral surveys using state-of-the-art facilities including VLT/CRIRES+ and Keck/KPIC have been highlighting the power of this technique in measuring chemical and isotopic composition, radial velocity and spin of gas giant planets. I will present new spectral characterization on two super-Jupiter systems, YSES 1 b & c and HIP 99770 b, observed with CRIRES+ and KPIC respectively, as part of these surveys. The results on YSES 1 b & c, constraining chemical abundances and spins of two super-Jupiters within the same system, provide a uniform comparison of formation and evolution history of giant planets. HIP 99770 b with a reliable dynamical mass constraint is a great testbed for retrieval modeling. These results showcase the capability of characterizing faint (K_mag~18) or close (sma~17 au) super-Jupiters using ground-based facilities.
PS15-A021
Anomalous Light Element Abundances in Giant Planet Host Stars
Ruisheng ZHANG#+, Ji-Wei XIE
Nanjing University
Background: The formation of a planetary system is highly dependent on the chemical abundances of its host stars. Aims: In this paper, we want to evaluate the effect of chemical abundances other than [Fe/H] on the planetary architecture. Methods: We study the chemical abundances of the latest 765 confirmed planet hosts which host 1168 planets in SDSS, Keck and HARPS samples. Benefitting from the data given by high-resolution and high-quality spectra, we can precisely compare the chemical abundance difference between different stars which host different types of planets. Results: We find a statistically significant difference for light elements of the planetary host stars which host different kinds of planets. This kind of difference may suggest the different forming locations of the planets. Discussion: We also rule out the factors of boundary selection, stellar properties dependence, measurement uncertainty and statistical random which will lead to this result instead of planet factors.
PS15-A028
New Clues to Reveal Origins of Hot- and Warm-Jupiter from the RV Sample
Xiang Ning SU#+
Hainan University
Many studies have analyzed planetary occurrence rates and their dependence on the host’s properties to provide clues to planet formation, but few have focused on the mutual occurrence ratio of different kinds of planets. Such relations reveal whether and how one type of planet evolves into another, e.g. from a cold Jupiter to a warm or even hot Jupiter, and demonstrate how stellar properties impact the evolution history of planetary systems. We propose a new classification of giant planets, i.e. cold Jupiter(CJ), warm Jupiter(WJ), and hot Jupiter(HJ), according to their position relative to the snow line in the system. Then, we derive their occurrence rates(𝜂HJ, 𝜂WJ, 𝜂CJ) with the detection completeness of RV(Radial Velocity) surveys(HARPS& CORALIE) considered. Finally, we analyze the correlation between the mutual occurrence ratios, i.e. 𝜂CJ/𝜂WJ, 𝜂CJ/𝜂HJ or 𝜂WJ/𝜂HJ, and various stellar properties, e.g. effective temperature 𝑇eff . Our results show that the 𝜂HJ, 𝜂WJ and 𝜂CJ are increasing with the increasing 𝑇eff when 𝑇eff ∈ (4600, 6600]𝐾. Furthermore, the mutual occurrence ratio between CJ and WJ, i.e. 𝜂CJ/𝜂WJ, shows a decreasing trend with the increasing 𝑇eff . But, both 𝜂CJ/𝜂HJ and 𝜂WJ/𝜂HJ are increasing when the 𝑇eff increases. Further consistency tests reveal that the formation processes of WJ and HJ may be dominated by orbital change mechanisms rather than the in-situ model. However, unlike WJ, which favors gentle disk migration, HJ favors a more violent mechanism that requires further investigation.
Session Chair(s): John CONNERNEY, NASA Goddard Space Flight Center
PS01-A009
A Statistical Analysis of the Returning Flux Tubes in the Jovian Magnetosphere Based on Juno Observations
Dongwen HE#+, Chao YUE
Peking University
Returning flux tubes play a key role in the magnetic equilibrium in the magnetospheres of the gas giants. Using electron and proton flux as well as the magnetic field data during perijove passes of Juno spacecraft, we conducted a statistical research on returning flux tubes in the Jovian magnetosphere. A concentration of enhanced events with probable relationship to Europa was observed, and the magnetic variation of the events tended to be more dramatic near the equator, while there is an absence of relation between the enhanced/depressed pattern of the events and the magnetic latitude. These results may imply a different picture of returning flux tubes in the Jovian magnetosphere as that of Saturn and may support the interchange instability explanation for returning flux tubes.
PS01-A013
Europa Clipper’s Investigation of Europa’s Habitability
Steven VANCE1#+, Kate CRAFT2, Everett SHOCK3, Britney SCHMIDT4, Jonathan LUNINE4, Kevin HAND5, William MCKINNON6, Elizabeth SPIERS7, Chase CHIVERS8, Natalie WOLFENBARGER9, Erin LEONARD5, Kirtland ROBINSON3, Gregor STEINBRUEGGE5, Mikhail ZOLOTOV3, Lynnae C. QUICK10, Jennifer SCULLY5, Tracy BECKER11, Samuel HOWELL5, Roger CLARK12, Andrew DOMBARD13, Christopher GLEIN11, Olivier MOUSIS14, Mark SEPHTON15, Julie CASTILLO-ROGEZ5, Francis NIMMO16, Alfred MCEWEN17, Gudipati MURTHY5, Insoo JUN18, Xianzhe JIA19, Frank POSTBERG20, Krista SODERLUND21, Catherine ELDER5, Ishan MISHRA5, Kevin TRINH3, Ngoc TRUONG11, Fabian KLENNER22, Nozair KHAWAJA20
1Jet Propulsion Laboratory, California Institute of Technology, 2Johns Hopkins University Applied Physics Laboratory, 3Arizona State University, 4Cornell University, 5California Institute of Technology, 6Washington University in St. Louis, 7Jackson School of Geosciences, 8Woods Hole Institute of Oceanography, 9Stanford University, 10NASA Goddard Space Flight Center, 11Southwest Research Institute, 12Planetary Science Institute, 13The University of Illinois at Chicago, 14Laboratory of Astrophysics of Marseille, 15Imperial College London, 16University of California, Santa Cruz, 17University of Arizona, 18NASA Jet Propulsion Laboratory, 19University of Michigan, 20Freie Universität Berlin, 21The University of Texas, 22University of Washington
Introduction: The overarching goal of NASA’s Europa Clipper mission is to “explore Europa and investigate its habitability.” Performing this assessment is challenging because habitability entails many potential macroscopic states comprising many interdependent physical and chemical parameters among numerous processes, such that no single measurement or investigation can fully characterize it. Therefore, we must investigate Europa as an integrated system to understand the complete picture [Cockell et al. 2023, Vance et al. 2023].Science Structure: To investigate Europa’s habitability, Europa Clipper has three main mission objectives: (1) characterize the Ice Shell and Ocean: including their heterogeneity, properties, and the nature of surface–ice–ocean exchange; (2) characterize Europa’s Composition, identifying any non-ice materials on the surface and in the atmosphere, including any carbon-containing compounds; and (3) characterize Europa’s Geology: including surface features and high-science-interest localities. The mission will also address several cross-cutting science topics including looking for any current or recent activity by searching for evidence of thermal/color/albedo anomalies or changes and any plumes; performing geodesy and radiation measurements; and assessing high-resolution, co-located observations at sites to provide reconnaissance for a future potential landed mission. Synthesizing the mission’s science measurements across multiple instruments—and incorporating remote observations by Earth-based observatories, JWST, and other spacecraft such as Juno and JUICE—to constrain Europa’s habitability is a complex cross-disciplinary task. The mission’s Habitability Assessment Board (HAB) is charged with guiding the synthesis of Europa Clipper data. In this presentation, we will summarize the case for Europa’s habitability as presently understood and outline the myriad ways Europa Clipper will revolutionize our understanding of the habitability of this remarkable ocean world. References: Cockell, C. S. et al. (2023) Nat. Astro., 10.1038/s41550-023-02158-8.Vance, S. D. et al. (2023) Space Sci. Rev., 10.1007/s11214-023-01025-2.
PS01-A014
Interactions of the Galilean Satellites with Jupiter’s Plasma Environment: Recent Moon Flybys and Auroral Observations with Juno
Jamey SZALAY1#+, Frederic ALLEGRINI2, Fran BAGENAL3, Scott BOLTON2, Peter DAMIANO4, Robert EBERT2, Angele PONTONI2, Yash SARKANGO1, Joachim SAUR5, Ali SULAIMAN6, Phil VALEK2, Rob WILSON7
1Princeton University, 2Southwest Research Institute, 3Laboratory for Atmospheric & Space Physics, University of Colorado, 4University of Alaska Fairbanks, 5University of Koeln, 6University of Minnesota, 7University of Colorado Boulder
The study of moon-magnetosphere interactions at the outer planets has been reinvigorated with recent in-situ data. Specifically, Juno measurements at Jupiter have given critical insight into the nature of these interactions, providing simultaneous in-situ particles and fields measurements at the moons along with high-resolution imaging of Jovian auroral phenomena for the first time. Juno has recently performed close flybys of Io, Europa, and Ganymede, providing unprecedented plasma composition measurements with its plasma instrument JADE, the Jovian Auroral Distributions Experiment. We will summarize the plasma observations from Juno’s satellite flybys as well as new insights gained from observations connected to the satellites’ fluxtubes. We will also discuss how the various moons interact with their plasma environments, providing sources of pickup-ions to the Jovian magnetosphere and highlight how these interactions provide analogues for satellite-moon interactions applicable to other planetary systems.
PS01-A016
Local-time Variations in the Jovian Io-magnetodisk-magnetosphere System and Their Possible Connections to Magnetopause Compression and/or Solar-wind-driven Convection
Michel BLANC1#+, Marie DEVINAT1, Zhi-Yang LIU1, Yuki NAKAMURA2, Yuxian WANG3, Nicolas ANDRE4, Aneesah KAMRAN1, Quentin NENON1
1Institute for Research in Astrophysics and Planetology, 2The University of Tokyo, 3Chinese Academy of Sciences, 4University of Toulouse
The Jovian magnetosphere and its magnetodisk/plasmasheet are generally considered to be azimuthally symmetric at least over radial distances extending from the outer edge of the Io torus to about 50 Jovian radii. But there are also many pieces of evidence pointing to a local time asymmetry in this system and in the upper atmosphere to which it is coupled: at ionospheric altitudes, local time asymmetries have been observed in main aurora emissions and in neutral and ion winds; in the magnetosphere, similar asymmetries have been detected in magneto-disk thickness and in high-energy particle fluxes; finally, deep in the magnetosphere, local asymmetries apparently modulated by the solar wind pressure have also been observed in the Io plasma torus by JAXA’s Hisaki spacecraft. In this study, we will use a combination of analytical and numerical models of plasma convection and current flows in the Jovian magnetosphere in an attempt to place all these observations in the same theoretical framework. We will explore the possibility that they are all consistently related to a single current system driven by solar-wind-magnetosphere interactions extending deep inside the magnetosphere, as well as the alternative hypothesis that they are merely a consequence of local time asymmetries in the compression of the magnetospheric cavity by the solar wind. We will discuss the potential implications of either solution for our current understanding of the importance of the solar wind in MIT coupling at Jupiter.
PS01-A021
Characterization of the Surfaces and Near-surface Atmospheres of Ganymede, Europa and Callisto by JUICE
Federico TOSI1#+, Thomas ROATSCH2, Andre GALLI3, Ernst HAUBER2, Alice LUCCHETTI4, Philippa MOLYNEUX5, Katrin STEPHAN2, John CARTER6, Cecilia TUBIANA4, Claire VALLAT7, Olivier WITASSE8
1INAF - National Institute for Astrophysics, 2German Aerospace Center, 3University of Bern, 4National Institute for Astrophysics, 5Southwest Research Institute, 6Institut d’Astrophysique Spatiale (IAS), CNRS/Université Paris-Saclay, 7European Space Agency – European Space Astronomy Centre, 8European Space Research and Technology Centre
Starting from the state of the art about the surfaces and tenuous atmospheres of Jupiter’s icy Galilean moons Ganymede, Europa and Callisto, conducted both closely by means of several spacecraft and by telescopic observations, we show how the ESA JUICE mission, successfully launched in 2023, aims to expand knowledge in detail thanks to its scientific payload. The surface geology of the moons is the main evidence for their evolution and reflects internal heating induced by tidal interactions. Surface composition is the result of endogenous and exogenous processes, with the former providing valuable information on the potential composition of shallow subsurface liquid pockets, possibly connected to deeper oceans. Finally, the Galilean moons have tenuous atmospheres that result from the sputtering of charged particles hitting their surfaces. In the case of Europa, plumes of water vapor have also been reported, although their phenomenology is still poorly understood and will require in-depth future exploration.
Here we briefly summarize the main scientific objectives and investigations that JUICE will have to achieve about the surfaces and tenuous atmospheres of the icy Galilean moons. Based on the predicted trajectory, we show potential coverage maps and other examples of reference measurements. The scientific discussion and observational planning presented here is the result of years of work and discussion held within the JUICE Working Group 2 (WG2): “Surfaces and near-surface exospheres of satellites, dust and rings”. Acknowledgements: This work was partly supported by the Italian Space Agency (ASI), ASI-INAF grant n. 2023-6-HH.0.
PS01-A022
Galileo Observation of Electron Spectra Dawn-dusk Asymmetry in the Middle Jovian Magnetosphere: Evidence for Convection Electric Field
Chongjing YUAN1+, Elias ROUSSOS2#, Yong WEI3, Norbert KRUPP2, Zhi-Yang LIU4, Jianzhao WANG5
1INSTITUTE OF GEOLOGY AND GEOPHYSICS, CHINESE ACADEMY OF SCIENCES, 2Max Planck Institute for Solar System Research, 3Chinese Academy of Sciences, 4Institute for Research in Astrophysics and Planetology, 5University of Colorado Boulder
The electron radiation 5–20 Jovian radii (RJ) to Jupiter is critical as being the final baton in the relay of accelerating seed populations for the highest-energy electrons. Trapped at <5 RJ, such harsh electron environment is the one in all within our reach strengthful enough for synchrotron emissions as those remote astrophysical sources. One essential issue in understanding the nature of this intense electron environment is quantifying its seed population distribution to discern the controlling physics among a diversity of acceleration processes. We untangle the ball of thread by resolving the time variations to establish the longitudinal and radial distributions of 10–100s keV electron energy spectra measured by Galileo spacecraft. We show that the key parameters of spectra at 15–20 RJ exhibit a previously unexpected dawn-dusk asymmetry. This asymmetry is more prominent for 100s keV electrons, persistent but intensified from 1996 to 2001. We indicate that the featured dawn-dusk asymmetry is possibly the global manifestation of the convective transport driven by a dawn-dusk electric field with an origin distinct from the one discovered around 6 RJ. We suggest that this convective transport is engaged in the dynamics preconditioning the making of the innermost highest-energy electron radiation.
PS01-A008
Juno Microwave Radiometer Observations Into the Subsurface of the Ice Shells of Io, Europa and Ganymede
Anton ERMAKOV1#, Scott BOLTON2+, Zhimeng ZHANG3, Steven LEVIN3, Ryunosuke AKIBA4, Jonathan LUNINE5, Jianqing FENG6, James KEANE3, Kevin HAND3, Sidharth MISRA3, Paul HARTOGH7, David STEVENSON3, Matthew SIEGLER6, Lea BONNEFOY8
1Stanford University, 2Southwest Research Institute, 3California Institute of Technology, 4University of California, Santa Cruz, 5Cornell University, 6Planetary Science Institute, 7Max Planck Institute for Solar System Research, 8Observatoire de Paris
On June 7, 2021, and September 29, 2022, the NASA Juno spacecraft flew by Jupiter’s Galilean moons, Ganymede, and Europa, respectively. The closest approach distance was only ~1000 km above Ganymede, and only ~350 km above Europa. More recently, on December 30, 2023, Juno passed by Io at a distance of 1500 km and is planned do so a second Io flyby on February 3, 2024 at a similar distance. The close flybys were the first encounters with the moons in over two decades and provided the first opportunity to map the subsurface of their shells at multiple microwave frequencies using Juno’s Microwave Radiometer (MWR). The observations provided several swaths across the moons at six frequencies, ranging from 600 MHz to 22 GHz. The ice transparency at microwave frequencies is dependent on its purity; assuming pure ice, the observations probe depths ranging from meters to kilometers. The MWR observations represent the first resolved interrogation of Ganymede and Europa’s subsurface ice shell revealing new constraints on porosity, fracturing, differences in terrain type and possibly the thickness of the ice shell. These unprecedented measurements of Io, Europa and Ganymede will allow comparative studies of the surfaces and subsurface structures of the Jovian satellites. The Juno MWR measurements complement previous ground-based radar and microwave radiometry observations, which provided early characterization of these surfaces. A comparison of the microwave spectra for all three satellites will be presented, as well as a detailed analysis and interpretation of the Ganymede MWR data that provide new constraints on ice subsurface properties.
Session Chair(s): Federico TOSI, INAF - National Institute for Astrophysics
PS01-A015
| Invited
Infrared Observations of Io by Juno During Closest Approaches
Alessandro MURA1#+, Francesca ZAMBON1, Roberto SORDINI1, Rosaly LOPES-GAUTIER2, Candice HANSEN3, Alberto ADRIANI1, Heidi BECKER4, Pete MOUGINIS-MARK5, Christina PLAINAKI6, Giuseppe SINDONI6, Madeline PETTINE7, Giuseppe PICCIONI1
1National Institute for Astrophysics, 2California Institute of Technology, 3Planetary Science Institute, 4Jet Propulsion Laboratory, California Institute of Technology, 5University of Hawaii, 6Italian Space Agency, 7Cornell University
Since 2016, NASA's Juno mission has been actively observing Jupiter from a polar, highly elliptical orbit. Despite not being the primary scientific focus, Juno utilized its onboard cameras, including JIRAM, JunoCam, and SRU, to capture images and spectra of Jupiter's Galilean moons. JIRAM, the Jovian InfraRed Auroral Mapper, operates as a dual-band imager and spectrometer in the infrared range (2000-5000 nm). JunoCam serves as a visible color imager, while SRU, the Stellar Reference Unit, functions as a highly sensitive camera capturing visible wavelengths (450-1100 nm). JIRAM's imager channel consists of a single detector with 2D capability and two distinct filters (L band, ranging from 3.3 to 3.6 µm; M band, from 4.5 to 5 µm). The pixel angular resolution, equal to 0.01°, proves adequate for Juno's moon imaging. Initially, the spatial resolution at the moons' surfaces was approximately 100 km/pixel at the campaign's outset, but it has progressively improved to around 500 m. This discussion centers on the analysis of JIRAM's high-resolution images, enabling the characterization of volcanic thermal sources' location, morphology, and temperatures. Additionally, a comparison with visible range images is conducted. The latest data from Juno's orbit up to 62 is presented.
PS01-A011
Multi-wavelength Observations of Jupiter’s Northern Circumpolar Cyclones
Andrew INGERSOLL1+, Scott BOLTON2#, Candice HANSEN3, Glenn ORTON1, Steven LEVIN1, Davide GRASSI4, Leigh N FLETCHER5, Gerald EICHSTÄDT6, Michael H WONG7, Anton ERMAKOV8, Cheng LI9, John ROGERS10, Shawn BRUESHABER11, alessandro MURA4
1California Institute of Technology, 2Southwest Research Institute, 3Planetary Science Institute, 4Istituto Nazionale di Astrofica, 5University of Leicester, 6Independent Scholar, 7University of California, 8University of California, Berkeley, 9University of Michigan, 10British Astronomical Association, 11Michigan Technological University
Juno arrived at Jupiter in 2016 and was inserted into a polar orbit with its closest approach (“perijove”) near Jupiter’s equator. One of Juno’s first major discoveries was the existence of circumpolar cyclones covering both of Jupiter’s poles. Over the course of Juno’s prime and extended missions, the line of apsides of the orbit has experienced a constant northward migration due to Jupiter’s asymmetric gravity field. One result of this migration is the lowering the spacecraft’s altitude over Jupiter’s north pole. Recently, the altitude over the north pole has reduced sufficiently to allow Juno’s microwave radiometer (MWR) to resolve Jupiter’s circumpolar cyclones. The observations provide new insights into how the circumpolar cyclones evolve with depth. We will present results from multi-wavelength observations of Jupiter’s polar cyclones including visible light images (JunoCam), the infrared images (JIRAM) and microwave images (MWR). The combined data set reveals information on how the circumpolar cyclones compare and evolve with depth.
PS01-A012
Vertical Structures of Jupiter Circumpolar Cyclones as Retrieved from Juno/MWR Polar Observations
Jiheng HU1+, Cheng LI1#, Zhimeng ZHANG2, Fabiano OYAFUSO2, Shannon BROWN2, Glenn ORTON2, Leigh FLETCHER3, Shawn BRUESHABER4, Steven LEVIN2, Scott BOLTON5
1University of Michigan, 2California Institute of Technology, 3University of Leicester, 4Michigan Technological University, 5Southwest Research Institute
The periapsis of Juno’s orbit has been steadily approaching the Jovian North Pole due to the precession of its orbit. This change allows favorable observational opportunities for Juno’s Microwave Radiometer (MWR) to resolve each individual circumpolar cyclone (CPC). The MWR instrument, with its range of frequencies from 600 MHz to 22 GHz, has gathered unprecedented information on the thermal emission within these polar cyclones. We share early findings about the atmospheric structure inside the Jovian circumpolar cyclones retrieved from MWR’s multichannel observations, starting from the 50th flyby. We discuss multiple scenarios of the internal structures of the polar cyclones using a model that takes the differences in both temperature and composition from the surrounding regions into account.
PS01-A003
Dynamical Tides in Jupiter and the Role of Interior Structure
Yufeng LIN#+
Southern University of Science and Technology
The Juno spacecraft has obtained highly accurate tidal Love numbers, which provide important constraints on the tidal response and interior structure of Jupiter. In order to exploit these observations, it is necessary to develop an approach for accurately calculating the tidal response of Jupiter for a given interior model and to investigate the role of interior structure. We directly solve the linearized tidal equations of a compressible, self-gravitating, rotating and viscous fluid body using a pseudo-spectral method. The Coriolis force is fully taken into account but the centrifugal effect is neglected. We can simultaneously obtain the real and imaginary parts of the tidal Love numbers for a given planetary interior model. We calculate the tidal responses for three simple interior models of Jupiter which may contain a compact rigid core or an extended dilute core. All of models we consider can explain the fractional correction in k2 due to dynamical tides, but all have difficulties to reconcile the high-degree tidal Love number k4. We show that the Coriolis force significantly modifies gravity modes in an extended dilute core at the tidal frequency relevant to the Galilean satellites. We demonstrate that a thin stable layer in the outer region, if exists, would also influence the tidal responses of Jupiter.
Session Chair(s): Evgenij ZUBKO, Institute for Basic Science, Zhong Yi LIN, Institute of Astronomy
PS08-A004
| Invited
A Fast-developing All-sky Meteor Surveillance Network in China
Jian-Yang LI1#+, Xiaoshu WU1, Zhenye LI2, Wenjun LIANG1, Jun CUI1,2, Jifeng LIU2
1Sun Yat-sen University, 2Chinese Academy of Sciences
Ground-based meteor surveillance network is the most widely used technique to monitor meteors, which are meteoroids entering Earth’s atmosphere. We hereby report an all-sky meteor surveillance network that is currently under development in China. Our goal is to support a comprehensive study of the dynamic meteoroid environment in near-Earth space. The objectives include 1) Providing nearly continuous monitoring of meteors and precisely determining their 3D trajectories; 2) Discovering new meteor streams and identifying their parent bodies, especially those associated with asteroidal objects; 3) Detecting potential unknown long-period comet impactors to Earth; and 4) Studying the evolution of meteor streams and their contribution to the zodiacal cloud. Additionally, the network will support citizen science, public outreach, and education. The system is composed of a network of self-developed, all-sky cameras and an automated data center. With a limiting magnitude of 4.2 for stars, the cameras can take all-sky images at a frequency of up to 30 Hz, and automatically identify meteors and measure the astrometry using the onboard software. The data center combines the measurements and GPS-based time tags from multiple stations to reconstruct the 3D trajectories and velocities of meteors. The brightness of meteors is estimated with relative photometry utilizing star catalogs. The results are visualized in nearly real-time. A testing network was installed in Beijing in 2023 and has since been operated for one year and detected 7253 meteors, including both sporadic and 225 streams. A full-scale network that currently contains 14 stations was deployed in Guangdong Province and Hong Kong and Macau SARs in December 2023, covering an area of over 180,000 km2. It has successfully observed the Geminids and the Quadrantids meteor showers. In the long term, we plan to expand the network to cover whole China, increase the sensitivity, and add multiband imaging and eventually spectroscopic capability.
PS08-A001
Effect of the Perseids Meteor Shower on Aerosol Population in the Earth Stratosphere in 2022
Evgenij ZUBKO1#+, Maxim ZHELTOBRYUKHOV2, Ekaterina CHORNAYA2, Konstantin SHMIRKO3, Anton KOCHERGIN4, Gorden VIDEEN5, Yeon Joo LEE1
1Institute for Basic Science, 2Russian Academy of Sciences, 3Pacific Oceanological Institute, 4Far Eastern Federal University, 5Space Science Institute
Sporadic meteoroids and meteor-shower streams continually bombard the atmosphere of Earth, loading up to 60,000 metric tons of interplanetary-space materials on an annual basis. These meteoroids introduce a significant amount of refractory aerosol particles into the uppermost layers of the atmosphere, in excess of 10 km, where introduction of terrestrial dust particles is difficult. We measure the degree of linear polarization that initially unpolarized solar radiation acquires upon scattering in the atmosphere. We perform such observations using facilities of the Ussuriysk Astrophysical Observatory, a division of the Institute of Applied Astronomy of Russian Academy of Science (code C15). These measurements are conducted in the morning and evening twilight, when the underlying terrain remains in shadow, but the aerosol particles at high altitude are already illuminated by sunlight. The altitude of the shadow boundary in our measurements ranges from 1 km up to ~30 km. In twilight on August 10 and 12 of 2022, we performed polarimetric measurements of the Earth stratosphere around the maximum of the Perseids meteor shower. Our measurements reveal dramatic difference in the polarimetric response registered shortly before and after the Perseids maximum. Modeling suggests that prior to the Perseids maximum, the upper atmosphere was populated by aerosol particles consisting of materials with weak absorption. These materials are consistent with water ice and Mg-rich silicates; whereas, after the Perseids maximum we find aerosols that are of highly absorbing composition, consistent with predominantly carbonaceous composition of cometary nuclei, the parent bodies for most meteor showers.
PS08-A006
Simultaneous High-speed Three-color Imaging Observations of Lunar Surface Targeting Impact Flashes by the Quadrantids
Noriaki ARIMA1#+, Shinsuke ABE1, Miho KAWABATA2, Ko ARIMATSU2
1Nihon University, 2Kyoto University
Lunar impact flash (LIF) is a phenomenon that occurs when a cm-sized meteoroid impacts the Moon at several tens of kilometers per second, converting part of its kinetic energy into light. Typical naked-eye meteors observed on the ground have a diameter of about 1 mm. On the other hand, fireballs and large fireballs, which are brighter than Venus and the Moon, are meteoroids ranging in size from cm to several tens of cm, but their size (mass) distribution function is not known because they occur infrequently. Through LIFs, the impact frequency and size distribution of cm-sized meteoroids on the Earth-Moon system can be efficiently investigated, leading to a better understanding of the size range connecting meteoroids and asteroids. Single-band LIF photometry provides size and mass distributions of meteoroids impacting on the Moon, and simultaneous dual-band observations provide peak blackbody radiation temperature distributions from about 2000 to 6000 K during the flashes. Using a tricolor imager mounted on the Kyoto University 3.8 m Seimei telescope (TriCCS), we performed 98-fps simultaneous g, r, and i-band observations of the lunar surface on the nights of January 3 and 4, 2024, when the Quadrantids is at its maximum. This observation was made in preparation for the upcoming Perseids in this August. Simultaneous 3-band observations allow us not only to accurately determine the blackbody temperature of the LIFs, but also to follow the temperature evolution of the LIFs while capturing the onset phase of the emission with a high temporal resolution of 10 ms. In this talk, we will present the LIF detection method we are currently developing, the results of the analysis, and our strategy for the next observation.
PS08-A009
Annual Variation of Sodium in the Geminid Meteor Shower
Shinsuke ABE1#+, Keita KIKUCHI1, Koji MAEDA2, Tomoko ARAI3
1Nihon University, 2University of Miyazaki, 3Chiba Institute of Technology
An active asteroid (3200) Phaethon is the parent body of Geminid meteor shower. However, the age of the Geminid meteor stream is the subject that has been left unsolved. The mass or size distributions and atomic abundances of Na/Mg/Fe of the Geminids’ meteoroids provide important information to understand the origin and evolution of the Phaethon-Geminid stream Complex. Especially Sodium is perfect indicator to investigate the volatility within the meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using high sensitive large format 4K CMOS cameras. Sodium is perfect indicator to investigate the volatility within the meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high-sensitive large format CMOS cameras. More than 500 visible spectra of the Geminid meteors observed between 2017 and 2022 were analyzed. The variation of Na, Mg and Fe during meteor ablation in the atmosphere have been studied. Statistically significant variation of sodium in the Geminid meteors in the same years’ dust trail was found. It should be note that Na depletion in the Geminid meteors increased with decreasing the size of meteoroids. A clear yearly variation of Na in the Geminid meteor streams over 6-years were found. Different age of the Geminid meteoroids ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for sodium variation and yearly variation. Detailed discussion will be presented.
PS08-A010
Spectroscopic Identification of H2O Ice Related Emissions by Hypervelocity Impact Flash Experiments
Kiyomasa KATO1#+, Shotaro AKUTSU1, Kazuhide KOMAI1, Keita KIKUCHI1, Shinsuke ABE1, Masahisa YANAGISAWA2, Sunao HASEGAWA3
1Nihon University, 2University of Electro-Communications, 3Japan Aerospace Exploration Agency
It has been suggested that water ice may exist in craters in the permanent shadow of the Moon. The LCROSS mission impacted a part of the permanent shadow region and detected OH emissions, which is thought to be derived from water ice, from spectroscopic measurements of the impact flash. Results obtained by the LADEE spacecraft and the SOFIA infrared astronomical satellite further confirmed the presence of water on the Moon's surface. According to laboratory experiments of hypervelocity impact flashes on the H2O ice target, due to the high pressure, approximately 5000 Pa, of the chamber, the vapor cloud affected to the strong emission line, moreover the measurement wavelength could not cover the 656 nm region where the neutral hydrogen emission line appeared. In order to detect clear evidence of H2O ice-derived emissions such as OH and H, spectroscopic measurements over a wider wavelength range between 300-800 nm under a low pressure environment, ~3 Pa, were carried out using JAXA/ISAS’s two-stage light gas gun. We will present the confirmed H2O ice related emissions and discuss about the mechanism of these emissions.
PS08-A003
Analyses of Lunar Impact Flashes Detected by RoLIFE
Zhong Yi LIN1#+, Yan-Ping CHEN2, Wing-Huen IP2
1Institute of Astronomy, 2National Central University
In December 2017 and 2018, we participated for the first time in the monitoring campaign of lunar impact flashes by using two small telescopes at the Lulin observatory during the Geminid meteor storms. For the detection of lunar impact flashes in 2022, we reconstructed the observational system at Lulin Observatory and set up the Taiwan Astronomical Network of Ground-based Observations (TANGO) for lunar impact flash observations. In this work, the observational procedure and data processing/analysis methods will be introduced using the impact events detected in early and late 2023 and some physical properties of impact will be summarized and compared to the previous work.
PS08-A012
Performance Evaluation of the Lunar Impact Flash Observing Camera Onboard the 6U Spacecraft EQUULEUS
Shinsuke ABE1#+, Masahisa YANAGISAWA2, Ryota FUSE3, Satoshi IKARI4, Hirotaka KONDO3, Yuki HADANO1, Kazuhide KOMAI1, Kiyomasa KATO1, Shotaro AKUTSU1, Masaki TSUTSUI3, Shintaro NAKAJIMA5, Yosuke KAWABATA6, Kota MIYOSHI5, Akihiro ISHIKAWA3, Mariko AKIYAMA5, Hajime YANO7, Ryu FUNASE5,3
1Nihon University, 2University of Electro-Communications, 3The University of Tokyo, 4Meisei University, 5Japan Aerospace Exploration Agency, 6Tokyo University, 7Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
When a meteoroid with a diameter of several centimeters to several tens of centimeters impacts the lunar surface, a Lunar Impact Flash, here after "LIF", is produced in the visible to near-infrared wavelength range which can be observed by ground-based telescopes as a magnitude 5 to 11 with short duration, 0.01 to 0.1 seconds, flash. However, the long-term continuous LIF observation from the ground is difficult due to the limitation of the lunar phase, weather conditions, and Earth's rotation. Thus, LIF observation from a lunar orbit or near the Earth-Moon Lagrange Point L2 (EML2) can be strongly proposed. The lunar impact flash observing camera "DELPHINUS (DEtection camera for Lunar impact PHenomena IN 6U Spacecraft)." onboard the 6U spacecraft EQUULEUS (EQUilibriUm Lunar-Earth point 6U Spacecraft) flying to EML2, developed in collaboration with Nihon University, the University of Electro-Communications, the University of Tokyo, JAXA, and major manufacturers, has been launched on November 16, 2022, as a one of 10 piggyback 6U satellites onboard the NASA Artemis 1 SLS, and successfully detached from the SLS rocket. DELPHINUS has an image processing board to detect lunar impact phenomena with a duration of 10 s of milliseconds. This image processing board has an FPGA to realize real-time image processing as fast as 60 fps. DELPHINUS has two cameras with the same field- of-view, to avoid the false-detection due mainly to electrical noises and cosmic rays. After the checkout operation and first light imaging, the camera successfully took images of the far side of the moon during the lunar flyby, and comet ZTF (C/2022 E3) etc. This paper reports on the performance evaluation comparing the various images obtained pre-and-after flights.
Session Chair(s): Manu VARGHESE, National Space Science Centre, Jianjun LIU, Polar Research Institute of China
ST06-A003
| Invited
Precursor Signals Before Large Earthquakes- Summary from Our Study-
Koichiro OYAMA1,2#+, Chia-Hung CHEN3
1International Research Center for Space and Planetary environment Science, 2Asia Space Environment Research Consortium, 3National Cheng Kung University
Precursor signals have been reported by many people so far. This talk summarizes our study. Disappearance of afternoon over shoot of Te, measured HINOTORI satellite was reported as our fast EQ paper. Data analysis observed with Dynamics Explorer 2(DE- 2) shows that the minimum of O+ density occurs over the epicenter as well as geomagnetic equator. The study shows that the epicenter can be identified 5 days before the earthquake. A giant earthquake which occurs on 11 March 2011 in Tohoku area in Japan provides us useful information about the precursor, such as 1.the deepening of the midlatitude trough. 2. its equatorward movement, and 3. enhancement of O+ density over the geomagnetic equator. Regarding the Ionosphere observation from the ground, most of the papers discuss the deviation from the averaged value with respect to the days. However, very often the NmF2 precursor feature shows the gradual increase before earthquake, and shows the peak and then reduces again at one station, while another ionosonde station, the NmF2 shows a minimum on the day when NmF2 shows the peak. In order to confirm the precursor feature, data from many stations along the latitude are needed. As the ionosphere is strongly influenced by space weather effect, at least ,two geomagnetic disturbance index, Dst, Kp index and solar radio flux, F10.7 should be studied simultaneously. The neutral temperature profiles observed by TIMED satellite show the good relationship with NmF2. So far we speculate that dynamo electric field which is enhanced by the atmospheric waves modifies the ionosphere. But still detail physics is not clear. Recently we are studying the vertical ground motion by using Hi-Net data (slant gauge), as we believe that the atmospheric waves are triggered by the ground motion.
ST06-A002
Characteristics of Lyman Lines in Solar Cycles and Their Influences on the Earth's Ionosphere
Ryosuke OKUBO1#+, Kyoko WATANABE1, Shinnosuke KITAJIMA1, Satoshi MASUDA2, Akimasa IEDA2, Hidekatsu JIN3, Chihiro TAO3, Michi NISHIOKA3
1National Defense Academy of Japan, 2Nagoya University, 3National Institute of Information and Communications Technology
X-rays and extreme ultraviolet (EUV) emissions from the Sun contribute to the formation of the Earth's ionosphere. The Lyman-α line (121.6 nm; Lyα) is the strongest line emission of solar EUV emission, accounting for more than 50% of the EUV irradiance in the chromosphere and transition region (Fontenla et al., 1991), and thus are considered to contribute significantly to the Earth's ionosphere. However, other Lyman-series line emissions, including Lyman-β line (102.6 nm; Lyβ), have a smaller irradiance than Lyα, but because of their shorter wavelength, the energy of the line emission itself is higher than Lyα. Therefore, there is a possibility that these Lyman series emissions may have an impact on the Earth’s ionosphere than Lyα. Lemaire et al. (2012) investigated the relationship between Lyα and Lyβ emissions during the solar cycle 23 and found that the Lyα/β ratio varies between maximum and minimum periods. Then, in this study, we investigate the relationship between Lyα and Lyβ emissions observed by TIMED/EGS-SEE as in Lemaire et al. (2012) during the solar cycle 24, and their effects on the electron density variations in the Earth's ionosphere. We also calculated the altitude distribution of the ion production rate at each EUV wavelength using the GAIA model (Jin et al., 2011), which can simulate the effect of solar emission on the Earth's ionosphere. Using the results of these calculations, we discuss the effect of Lyman emission on the Earth's ionosphere.
ST06-A011
Ionospheric F-layer Scintillation Variabilities as Observed by COSMIC During Sudden Stratosphere Warming Events
Hailun YE+, Xianghui XUE#, Wen YI
University of Science and Technology of China
Sudden stratospheric warming (SSW) occurred in winter polar stratosphere play a significant effect on the global ionosphere and atmosphere. However, the SSW-induced effects on small-scale structure in the ionosphere are generally lack of understanding. Ionospheric F-layer irregularities is kind of small-scale structure, which can affect the trans-ionospheric radio wave, leading to so-called ionospheric scintillation phenomenon. Thus, the role of SSW on the small-scale structure in the ionosphere can be reflected by studying the characteristics of ionospheric scintillation during SSWs. In the present work, we investigate the variation of the equatorial premidnight F-layer scintillation over the American sector by using COSMIC/FORMOSAT-3 observation. It found that the occurrence frequency and altitude of ionospheric F-layer scintillation were obviously suppressed during SSWs. It suggested that SSWs have a significant effect on the small-scale structure in the Earth's ionosphere, having potential application for satellite navigation and communication.
ST06-A007
| Invited
Global Ionosphere Disturbed by Tropospheric and Thermospheric Lamb Waves of the 15 January 2022 Tonga Volcanic Eruption
Jann-Yenq (Tiger) LIU1#+, Tzu-Hsun KAO1, Bor-Shouh HUANG2, Yang-Yi SUN3, Chieh-Hung CHEN4, Katsumi HATTORI5, Tien-Chi LIU1, Po-Han LEE6
1National Central University, 2Academia Sinica, 3China University of Geosciences, 4Chengdu University of Technology, 5Chiba University, 6Central Weather Administration
At 04:05UT on 15 January 2022, intense Tonga volcanic eruptions induce prominent atmospheric disturbances and tsunami waves. Himawari-8 meteorological satellite images depict the induced upper-level tropospheric disturbances with horizontal speeds of about 315 m/s at 8.2 km altitude in the Lamb wave mode travel worldwide. Upon the traveling atmospheric disturbances (TADs) of the tropospheric Lamb wavefront arriving in Taiwan at 11:30UT, 98 ground-based barometers register increases and reach peaks at about 11:50UT in the atmospheric pressure; 28 tide gauges record enhancements and maximums of sea level fluctuations at about 14:30-17:30UT; and a local ionosonde observes that the ionosphere reaches the highest altitude at 14:30UT. The changes of the horizontal component of the Earth’s magnetic fields measured by 10 Taiwan magnetometers almost all point exactly toward the Tonga volcano upon the tropospheric Lamb wavefront arrival at 11:00-12:00UT, and away from the volcano at 22:00-23:00UT, which suggests a 487 m/s TID (traveling ionospheric disturbance or thermospheric Lamb wavefront) at about 130 km altitude also being activated. The horizontal components in magnetic field changes of 69 INTERMAGNET magnetometers show that both tropospheric and thermospheric Lamb waves triggered by Tonga volcanic eruptions are very powerful, and can induce intense dynamo currents and electric fields in the global ionosphere.
ST06-A015
GNSS Application for Space Weather Monitoring Over Taiwan
I-Te LEE1,2#+, Jyun-Ying HUANG3, Hsu-Hui HO3, Tungyuan HSIAO4
1Taiwan Space Agency, 2National Central University, 3Central Weather Bureau, 4Hsing Wu University
At the lower latitude region, the electron density distribution is significantly influence high-frequency and satellite communication as well as navigation and positioning services. Over Taiwan, there is high density of plasma during the day which associated with the equatorial ionization anomaly, and plasma bubbles/irregularities appear in the evening to midnight period. In order to monitor the variation of ionospheric electron density and the movement of ionospheric irregularities, the Space Weather Operational Office of Central Weather Administration (CWA/SWOO) has collaborated with Taiwan Space Agency and domestic scientific research teams from universities to establish various products which by applying the Global Navigation Satellite System (GNSS) signal. By using ground-based and space-based observations, CWA/SWOO provides real-time global and regional total electron content (TEC), scintillation index, rate of TEC index, as well as ionospheric radio occultation profile, etc. Meanwhile, a Global Ionospheric Specification and an ionosphere - thermosphere coupled assimilation system is operated by combining GNSS observations to reproduce three-dimensional electron density structure and short period forecast of ionosphere and thermosphere, respectively. In addition, in order to understand the relationship between positioning error and ionospheric feature, CWA/SWOO also conduct a system to monitor positioning of few reference stations around Taiwan in real-time. It would provide a good dataset to make comparisons of positioning error and irregularities.
Session Chair(s): Kyoko WATANABE, National Defense Academy of Japan
ST01-A006
| Invited
Recent Studies of Accelerated Electrons in Solar Flares Observed with Nobeyama Radioheliograph
Satoshi MASUDA1#+, Keitarou MATSUMOTO2
1Nagoya University, 2New Jersey Institute of Technology
Nobeyama Radioheliograph (NoRH) is a radio interferometer designed to observe the Sun, especially solar flares. After the operation by National Astronomical Observatory of Japan (NAOJ) from June 1992 to March 2015, NoRH was operated by Institute for Space-Earth Environmental Research (ISEE), Nagoya University as a representative of the International Consortium for the Continued Operation of Nobeyama Radioheliograph (ICCON) until March in 2020. During this operating period, a lot of solar flares were observed with NoRH. About 900 flares among them were recorded with a high time resolution of 0.1 second (event mode), instead of 1 second (normal mode). This high time-resolution is one of the unique and important characteristics of NoRH. The electron acceleration process during a solar flare takes place impulsively in a shorter time-scale compared with thermal processes. Thus, this high time-resolution imaging is quite useful to reveal the acceleration/transport/loss processes of high-energy electrons during a solar flare. Actually, we found observational features of bouncing motion of accelerated electrons along a magnetic loop in a solar flare (Matsumoto et al., 2023). Through accurate analyses of the microwave images, we obtained the information on pitch-angle of the high-energy electrons emitting microwaves. This is a quite useful approach for understanding the electron acceleration mechanism in solar flares. Another important characteristic of NoRH is its high sensitivity. It can detect a very weak (< one solar flux unit at 17 GHz) flare and can realize imaging observations w (Krucker et al., 2020). This characteristic somehow contributes to reveal the electron acceleration process in small solar flares. In this topic, collaboration with MUSER is very effective and some initial studies have been achieved. Moreover, the NoRH full-sun data for 28 years can be used to study various small activities even in quiet region which might be related with coronal heating.
ST01-A017
| Invited
New Findings of Energy Release and Particle Acceleration in Solar Flares Revealed by ASO-S/HXI Observations
Yang SU#+
Purple Mountain Observatory, Chinese Academy of Sciences
The Hard X-ray Imager (HXI) on board the Advanced Space-based Solar Observatory (ASO-S) observes spectra and images of solar X-ray bursts in the energy range of ~15-300 keV, with a spatial resolution as high as 3.1 arcsec and a time resolution as high as 0.125 s during burst mode. HXI has recorded more than 400 flares. The reconstructed images reveal interesting and fine structures of hard X-ray sources in flares. In this talk, a brief introduction on HXI and calibration work will be presented first., followed by a few new findings revealed by HXI data and other multi-wavelength observations, including (1) evidence of slipping reconnection as the cause of flare QPPs; (2) joint observations of HXI, Solar Orbiter/STIX, and WIND reveal the possible coronal origin of flare-related SEP electron event; (3) HXR fine structures in the looptop region reveal new details of acceleration process in flares. More related studies will also be briefly introduced.
ST01-A009
Solar Eruptive Phenomena Associated with Solar Energetic Electron Spectral Types
Linghua WANG1#+, Wen WANG2, Wenyan LI1, Sam KRUCKER3, Robert WIMMER-SCHWEINGRUBER4, Zheng SHENG2
1Peking University, 2National University of Defense Technology, 3University of Applied Sciences and Arts Northwestern Switzerland, 4Kiel University
The energy spectral shape of solar energetic electron events carries important information on the energetic electron source/acceleration at the Sun. We investigate the association of newly-identified six SEE spectral types with solar eruptive phenomena, including the downward double-power-law spectrum with break energy EBabove 20 keV (DDPLEB ≥20keV), downward double-power-law with EBbelow 20 keV (DDPLEB <20keV), upward double-power-law (UDPL), single-power-law (SPL), Ellision-Ramaty-like (ER) and logarithmic-parabola (LP). We find that the SPL type shows (the other five types show) a ~38% (~55%–82%) association with hard X-ray flares and a ~76% (~85%–93%) association with west-limb coronal mass ejections (CMEs). Among the other five types, DDPLEB <20keVand ER (LP and DDPLEB ≥20keV) types have a only ~7%–8% (~16%–20%) association with type II radio bursts and ~5%–9% (~11%–21%) association with halo CMEs; however, the UDPL type exhibits a significant (~47% and ~50%) association with type II bursts and halo CMEs, with a significantly faster median CME speed of 1000 km s-1. For DDPLEB ≥20keV (DDPLEB <20keV) with a positive (no) correlation between the spectral indexes and no (a positive) correlation between the spectral index and break energy, the spectrum appears to be flatter as the associated CME (flare) becomes faster (stronger). These results suggest that the SPL type can result from the initial acceleration process that likely occurs high in the corona, and then provide seed populations for further acceleration processes to form the other five types: DDPLEB <20keV and ER types via flare-related processes, LP and DDPLEB ≥20keV types via CME-related processes, and the UDPL type via CME-driven shocks.
ST01-A022
Solar Energetic Electron Events Observed by Solar Orbiter and Wind on 2022 March 6
Wenyan LI1#+, Linghua WANG1, Wen WANG2, Robert WIMMER-SCHWEINGRUBER3, Sam KRUCKER4
1Peking University, 2National University of Defense Technology, 3Kiel University, 4University of Applied Sciences and Arts Northwestern Switzerland
Here we present a comprehensive study of solar energetic electron (SEE) events with a fast-rise, fast-decay temporal profile on 2022 May 6, observed both by SolO/EPD at 0.5 AU and by Wind/3DP at 1 AU with a longitudinal separation of ~2° between the two spacecraft. SolO/EPD detect three SEE events at ~4-100 keV during 08:00 UT - 09:30 UT, while Wind/3DP only measures one SEE event at 0.6-40 keV between ~08:00 UT and 13:00 UT. According to the velocity dispersion analysis, the solar injection’s start-time (peak-time) of the first (third) EPD event agrees with the solar injection’s start-time (peak-time) of the Wind/3DP event within uncertainties. Three SEE events observed by EPD exhibit, respectively, a single-power-law (SPL) energy spectrum, an SPL spectrum, and a double-power-law spectrum with a downward-bending break near 9 keV. The 3DP SEE event shows an SPL energy spectrum with a spectral index similar to that of the first EPD event. On the hand, the three EPD events are likely accompanied by two HXR microflares measured by SolO/STIX, while the third event are associated with three EUV jets measured by SDO/AIA; the 3DP event is associated with the two HXR microflares and three jects. All these microflares/jets, as well as the magnetic field lines connecting to SolO and Wind, originate from the same active region (AR12957). Therefore, we can construct a formation scenario of these SEEs: the three events detected by SolO likely arise from different sources/processes at the Sun; as the electrons propagate from 0.5 AU to 1 AU, the three events merge into the one event detected by Wind.
ST01-A005
| Invited
Numerical Modeling of the Acceleration and Transport of Energetic Electrons in Solar Flares
Xiangliang KONG1#+, Fan GUO2, Bin CHEN3, Chengcai SHEN4, Xiaocan LI5, Jing YE6, Lulu ZHAO7, Feiyu YU1, Zelong JIANG1, Yao CHEN1, Joseph GIACALONE8
1Shandong University, 2Los Alamos National Laboratory, 3New Jersey Institute of Technology, 4Center for Astrophysics | Harvard & Smithsonian, 5Dartmouth College, 6Chinese Academy of Sciences, 7University of Michigan, 8The University of Arizona
Particle acceleration, transport, and subsequent emission processes are at the heart of the high-energy aspects of solar flares. Observations have suggested that an enormous number of particles are accelerated to high energies, and the nonthermal particles can carry a substantial portion of the released magnetic energy. These accelerated particles further propagate and precipitate, producing HXR footpoint sources in the dense chromosphere via thick-target bremsstrahlung and leading to chromosphere evaporation. Despite a long history of study, the whole process of energetic particles and their effects on flare dynamics is still an active field of research. Recently, we develop a macroscopic particle model that naturally incorporates electron acceleration and transport by combining the particle transport equation with large-scale MHD simulation of a solar flare. I will present our recent results on the numerical modeling of particle acceleration, transport, and emission in solar flares.
ST01-A003
Helium Pickup Ion Velocity Distributions to Probe and Evaluate Local Physical Processes
Keiichi OGASAWARA1#+, Harald KUCHAREK2, Berndt KLECKER3, Maher DAYEH1, Robert EBERT1
1Southwest Research Institute, 2University of New Hampshire, 3Max Planck Institute For Extraterrestrial Physics
Velocity distribution functions (VDFs) of He+ pickup ions (PUIs) were used to trace local physical processes within interplanetary coronal mass ejections (ICME) and corotating interaction regions (CIR). PUIs are measured by PLasma And SupraThermal Ion Compostion (PLASTIC) instrument onboard the Solar Terrestrial Relations Observatory (STEREO) in an unprecedented cadence and resolution. Overall, PUIs preserve the properties of the original ring distributions, and show consistent adiabatic cooling throughout two events. For shock associated events, the acceleration, heating, and pitch-angle scattering are characterized for both perpendicular and parallel shocks with notable differences. Compression related processes and diffusive shock acceleration are indicated by the perpendicular and the parallel shocks, respectively. Pitch angle scattering were correlated with magnetic field power spectral density at the Helium cyclotron, while the Alfven velocity determines the resonance condition. The 3D VDF observations of PUIs will be extremely useful for this type of analysis and this method can be applied to study shock injection processes and PUI transport processes even under the active conditions.
ST01-A016
| Invited
Observations of Energetic Particles with Solar Orbiter
Robert WIMMER-SCHWEINGRUBER1#+, Javier RODRIGUEZ-PACHECO2, George HO3
1Kiel University, 2University of Alcalá, 3Southwest Research Institute
Solar Orbiter has been observing the Sun and inner heliosphere since its launch in February 2020. Approaching the Sun as close as 0.28 au, just inside of Mercury’s orbit, it has recorded hundreds of energetic particle events. With its complement of ten scientific instruments, many of them with multiple sensors, and together with the fleet of other spacecraft in the heliosphere, it is uniquely well equipped to investigate how the solar eruptions produce energetic particle radiation that fills the heliosphere. In this presentation I will review some of the exciting observations by Solar Orbiter’s Energetic Particle Detector (EPD) and other instruments aboard Solar Orbiter.
ST01-A002
Dynamic Acceleration of Energetic Protons by an Interplanetary Collisionless Shock
Liu YANG1#+, Verena HEIDRICH-MEISNER2, Wen WANG3, Robert WIMMER-SCHWEINGRUBER4, Linghua WANG5, Javier RODRIGUEZ-PACHECO6, George HO7
1Macau University of Science and Technology, 2University of Kiel, 3National University of Defense Technology, 4Kiel University, 5Peking University, 6University of Alcalá, 7Southwest Research Institute
We investigate energetic protons accelerated by an interplanetary shock observed with unprecedented high-resolution measurements by the Electron-Proton Telescope sensor of the Energetic Particle Detector suite on board the Solar Orbiter spacecraft on 2021 November 3. We reconstruct the proton pitch-angle distributions (PADs) in the solar wind frame. We find that ∼1000-4000 keV protons exhibit a rapid-rise, rapid-decay temporal flux profile with a clear velocity dispersion ∼2 min before the shock, similar to impulsive solar energetic particle events. The velocity dispersion analysis (VDA) of this event gives a proton path length consistent with the length derived from the shock’s motion and magnetic field configuration. The peak spectrum in this event appears to be steeper than the spectrum at the shock. Furthermore, we find that ∼50-200 keV proton fluxes peak between ∼10 and ∼20 s before the shock with inverse velocity dispersion. Both the velocity dispersion event and the inverse velocity dispersion event are accompanied by magnetic kinks/switchbacks. In addition, we identify two distinct proton populations near the shock. One population at energies below ∼300 keV is characterized by a power-law spectrum with an index of ∼6-7 and a flux profile that increases before and decreases after the shock. The other population at energies above ∼300 keV shows a long-lasting, anti-sunward beamed PAD across the shock and a flux profile that remains relatively constant before and increases slightly after the shock. These results suggest that shock acceleration of energetic protons is highly dynamic due to temporal and/or spatial variations on the shock front. The observation of the velocity dispersion event further suggests that shock acceleration can be impulsive and efficient, possibly due to the interaction between the shock and magnetic kinks/switchbacks. Moreover, shock-drift acceleration likely plays an important role in accelerating energetic protons at interplanetary shocks.
ST01-A013
Archival Reanalyses for the Greatest Ground Level Enhancement on 23 Feb 1956
Hisashi HAYAKAWA1#+, Sergey KOLDOBSKIY2, Alexander MISHEV2, Stepan POLUIANOV2, Agnieszka GIL3, Inna USOSKINA2, Ilya USOSKIN2
1Nagoya University, 2University of Oulu, 3Polish Academy of Sciences
Intense solar eruptions occasionally accelerate charged particle to high energies. Such solar energetic particles (SEPs) can reach Earth, depending on the relative geometry between the Sun and the Earth. Occasionally, SEPs have sufficiently high energy and flux to be detected by ground-level detectors known as ground-level enhancements (GLEs) which are consequently numbered since 1942. Among such GLEs, GLE #5 on 23 Feb 1956 is associated with the hardest spectra and the greatest flux. As such, this GLE has been used as a benchmark reference for solar particle storms, radiation dose analyses, and as a bridge between the known GLEs and extreme solar particle events recorded in cosmogenic isotopes. However, we have found that the source datasets for GLE #5 were mostly based not on actual instrumental measurements but on their handdrawn spline curves. Here, we collect, review, and analyse available contemporaneous reports for the neutron monitor measurements of GLE #5 based on an archival investigation of original observational records and logbooks. The new datasets significantly revise the source datasets, improve the time-series accuracy, and leads to a slightly softer spectrum of SEPs than previously considered for this events.
Session Chair(s): Lulu ZHAO, University of Michigan
ST24-A007
| Invited
Forecast the ICME Magnetic Field in the Heliosphere Based on In-situ Observations at 1 Au
Chenglong SHEN1#+, Yutian CHI2, Dongwei MAO1
1University of Science and Technology of China, 2Deep Space Exploration Laboratory
Predicting the magnetic field configuration of the Interplanetary Coronal Mass Ejections (ICMEs) at the unique target location has long been a challenge. With more spacecraft launched recently, multipoint in situ measurements are becoming increasingly crucial in resolving this issue. Based on the in-situ observations at 1 AU, the Heliospheric ICME Magnetic Field model (HeIMF model) was developed to estimate the magnetic field configuration of ICME at the target point. The only inputs of this model are ICME magnetic field in-situ observations, and a flux rope fitting model is used to obtain magnetic and geometrical parameters. Based on self-similar expanding assumption, ICME parameters along the propagation path are calculated, and the magnetic profile is derived from parameters at the target point. An example ICME observed by Venus EXpress (VEX) at and STEREO-A (STA) is used to describe model details, and model uncertainties are also discussed by comparing observations and modeling results.
ST24-A014
Prediction of Next Solar Rotation Synoptic Maps Using an AI-based Photospheric Flux Transport Model
Hyun-Jin JEONG1#+, Mingyu JEON1, Daeil KIM1, Youngjae KIM1, Ji-Hye BAEK2, Yong-Jae MOON1, Sunghwan CHOI2
1Kyung Hee University, 2Korea Astronomy and Space Science Institute
In this study, we develop an AI-based photospheric flux transport model. We predict next solar rotation (27.3 days) synoptic maps by deep learning. We use synoptic maps for the last 3 solar rotations as the model input. The synoptic map is a global magnetic field map of the solar surface constructed by merging together solar frontside magnetograms, and has been widely used for initial boundary conditions of several space weather prediction models. Here we train and evaluate our deep learning model, which is based on the Pix2PixCC model, using data sets of SDO/HMI, SOHO/MDI, and NSO/GONG synoptic maps with a resolution of 360 by 180 (longitude and sin latitude) from 1996 to 2023. We show results from our deep learning model, and compare them with those from the persistence model and the conventional photospheric flux transport models, which include the effects of differential rotation, meridional flow, and diffusion on the solar surface. The averaged pixel-to-pixel correlation coefficient (CC) between the real and our generated data with a 10 degree in longitude is 0.51, and our results are higher than the persistence model results (0.36) and the flux transport model results (0.44). Our model can approximately generate magnetic features, e.g., diffusion of solar active regions and the motions of supergranules. We discuss the advantages and disadvantages of our model in view of overall magnetic field evolution. We present several positive prospects of our new methodology for the study of the sun and space weather forecast.
ST24-A008
Sunspot Light Bridges and Solar Active Region Evolution Processes
Fuyu LI1#+, Changhui RAO1, Xinhua ZHAO1, Yang GUO2, Xiaoying GONG1, Yuhao CHEN1, Nanbin XIANG1, Huaning WANG1
1Chinese Academy of Sciences, 2Nanjing University
Light bridges (LBs) are elongated bright lanes lying on the umbrae of sunspots. The formation mechanism of LBs is strongly related to the dynamic evolution of solar active regions (ARs). Flux system collisions and splits might exist during the full lifetime of ARs. In the developing phase of ARs, collisions are dominant, while splits in the decaying phase. To study the LBs and AR evolution processes, we employ observational data from the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory (HMI/SDO). According to our previous work, LBs have been categorized into: penumbral intrusion (type-A), sunspot/umbra merging (type-B) and umbral-dot emergence (type-C). Based on 109 LB samples from 69 ARs in 2014, we statistically investigate the relationship between LB types and AR evolution phases. Type-B LBs are more likely to be formed in the developing phase of sunspots/active regions. Type-A and type-C LBs mostly take shape in the decaying phase of flux systems. LBs are well matched with the weak field lanes (WFLs), except that aligned on the polarity inversion line of delta sunspots. For type-A and type-C LBs, the WFLs represent the splitting of magnetic flux systems. The sunspots tend to decay and split into several parts after type-A and type-C LBs formed. For type-B LBs, the WFLs declining are caused by collisions of flux systems. The sunspots merge and keep growing after type-B LBs formed. We conclude that type-B LBs are formed by collisions of flux systems, while type-A and type-C LBs are generated by splits.
ST24-A020
Statistical Models for Solar Flare Predictions
Yang CHEN#+
University of Michigan
We present novel statistical methods for early forecasting of solar flare events and compare them with machine learning approaches we adopted in our previous work. The results that will be presented include (1) strong and weak flare classification with spatial statistics features, together with physics and topological parameters; (2) active region-based solar flare intensity prediction with a mixed Long-Short Term Memory (LSTM) regression; and (3) Tensor Gaussian Process with Contraction model for solar flare forecasting combining data of various types and sources (PIL, HMI and AIA images). We will also compare the advantages and disadvantages of off-the-shelf and newly-developed machine learning methods and discuss future directions for research.
ST24-A003
Deep Learning Compression of Solar Polarization Spectra from Hinode SOT/SP
Jargalmaa BATMUNKH1#+, Yusuke IIDA1, Haruhisa IIJIMA2, Takayoshi OBA3
1Niigata University, 2Nagoya University, 3Max Planck Institute for Solar System Research
The complexities in space weather forecasting, particularly in predicting harmful effects triggered by solar flares, continue to persist. The extensive volume of observational solar spectral data accumulated by the Hinode satellite provides an opportunity for a comprehensive exploration of our sun’s behavior. However, the high-dimensional nature of the solar polarization spectra poses significant processing challenges, even with advanced computational methods. Our objective is to address this issue by developing a compression model specialized for solar spectra using deep learning methods. The attainment of such a model holds promise for enhancing various tasks, including solar flare prediction, automatic categorization of spectra, detection of anomalous spectra, and more. We constructed two distinct autoencoder models—deep (DAE) and 1D-convolutional (1D-CAE) autoencoders—to compress Stokes I and V polarization parameters. These models take polarimetric spectra as input, encode them into a smaller-sized representation, and then decode them back into output that should closely resemble the input. In addition to the general loss function, which is the sum of mean absolute errors (MAE) for Stokes I and V, we also explored a customized version of the loss function, where weighted MAE was applied specifically for Stokes V. The average standard deviation (std) of the DAE model resulted in 11.17% at the line centers and 5.32% at the continuums for Stokes I, and it was 11.09% at the line cores for Stokes V. In comparison, the 1D-CAE model exhibited an average std of 10.1% at the line centers and 3.56% at the continuums for Stokes I, with a value of 5.88% at the line cores for Stokes V. In summary, the 1D-CAE model demonstrated greater potential as a compression model for the polarimetric spectra. Additionally, incorporating a weighted loss function during model training had a positive impact on performance.
ST24-A005
Deep Learning Models for High-resolution Electron Flux Prediction at GEO: A Multi-channel Approach
Mengli TAN+, Xu SI, Xinming WU, Xin TAO#
University of Science and Technology of China
There are hundreds of satellites at the geosynchronous orbit (GEO) where is filled with energetic electrons. Electron flux at GEO can change sharply in a matter of hours or even an hour. This study employs advanced deep learning models, including Temporal Pattern Attention Long Short-Term Memory (TPA-LSTM) and Transformer, to predict high-resolution electron flux at GEO. Our models consider multiple input parameters, providing a unique approach compared to single-valued output models. Trained on a six-year dataset, the models exhibit notable prediction efficiencies (PE) for up to three days. Specifically, for 1-day predictions, PE values for 275 keV, 475 keV, >0.8 MeV, and >2 MeV electron flux are 0.799, 0.831, 0.849, and 0.881, respectively. The study contributes valuable insights for spacecraft safety and space research applications.
ST24-A023
Validation of Model Results in Response to the COSPAR ISWAT Challenge
Dedong WANG#+
GFZ Helmholtz Centre for Geosciences
The COSPAR International Space Weather Action Team (ISWAT) is a global hub for collaborations addressing challenges across the field of space weather. One of the objectives of the G3-04 team “Internal Charging Effects and the Relevant Space Environment” is model performance assessment and improvement. One of the expected outputs is a more systematic assessment of model performance under different conditions. The G3-04 team proposed performing benchmarking challenge runs. In this study, in response to the first benchmarking challenge (long-term simulation), we perform simulations for the year 2017 to validate the Versatile Electron Radiation Belt (VERB) code. The challenge requires not using any of the measurements from the NASA' s Van Allen Probes for setting up parameters of the code, such as boundary and initial conditions. In our simulations, we use data from the Geostationary Operational Environmental Satellites (GOES) to set up the outer boundary condition, which is the only data input for simulations. We validate our simulation results against measurements from Van Allen Probes. In particular, we ‘fly’ a virtual satellite through our simulation results and compare the simulated differential electron fluxes at 0.9 MeV and 57.27 degrees local pitch-angle with the fluxes measured by the Van Allen Probes. In general, our simulation results show good agreement with observations. We calculated several different matrices to validate our simulation results against satellite observations. Using the similar approach, we extend our simulations to several years long period and validate our simulation results against satellite observations in both long-term and specific geomagnetic storms. Several different validation matrices are calculated for both long-term and specific events.
Session Chair(s): Xin TAO, University of Science and Technology of China, Anton ARTEMYEV, University of California, Los Angeles
ST07-A008
| Invited
Quantifying Wave-particle Interactions in Plasma Instabilities
Jinsong ZHAO#+
Purple Mountain Observatory, Chinese Academy of Sciences
In collisionless plasmas such as the solar wind, the particle velocity distributions can be shaped by various wave-particle interactions, which lead to effective energy transfer between electromagnetic fields and particles. The commonly-observed quasi-monochromic waves by in-situ satellites are widely believed to be generated by plasma instabilities via wave-particle interactions. Thus, how to quantify the role(s) of wave-particle interactions in plasma instabilities is a fundamental problem in the space plasma community. Recently, we developed the theoretical method quantifying both resonant and nonresonant wave-particle interactions, and we performed the comprehensive analyses on the excitation mechanisms responsible for several typical plasma instabilities (e.g., electron heat flux instability, ion beam instability, and ion temperature anisotropy instability) in the solar wind. This report will introduce our new findings.
ST07-A015
Identification of Coupled Landau and Anomalous Resonances in Space Plasmas
Xuzhi ZHOU1#+, Jinghuan LI1, Zhi-Yang LIU2, Shan WANG1, Anton ARTEMYEV3, Yoshiharu OMURA4, Xiao-Jia ZHANG5, Li LI6, Chao YUE1, Qiugang ZONG1, Craig POLLOCK7, Guan LE8, James BURCH9
1Peking University, 2Institute for Research in Astrophysics and Planetology, 3University of California, Los Angeles, 4Kyoto University, 5The University of Texas at Dallas, 6China University of Geosciences, 7Denali Scientific, 8National Aeronautics and Space Administration, 9Southwest Research Institute
Wave-particle resonance is a ubiquitous interaction process between plasma waves and charged particles, during which the resonant particles experience a constant wave phase to enable an efficient wave-particle energy transfer. As the wave amplitude becomes large enough, the particles could be nonlinearly trapped in phase space to form resonance islands, which leads to a variety of observational signatures. Here, we present spacecraft observations of an oblique-propagating whistler wave event in the foreshock region, during which the Landau and anomalous resonances can be identified simultaneously. In this event, the ion parallel-speed distributions display a series of phase-space rings, which are direct evidence of Landau trapping for solar wind ions. The anomalous resonance, on the other hand, is characterized by the phase-bunched ion distributions in anti-phase with the wave magnetic field. This scenario is examined and validated by test-particle simulations, which reproduce the key observational signatures. Our results also indicate that the Landau and anomalous resonances are largely coupled due to the coexistence of the electric force and Lorentz force in the parallel direction.
ST07-A010
| Invited
Recent Results on Low-frequency Wave Generation and Related Energetic Particle Precipitation in the Earth Magnetosphere
Andrei DEMEKHOV1,2#+
1Polar Geophysical Institute, 2Russian Academy of Sciences
This report is devoted to a brief review of some recent results on the physics and manifestations of nonlinear wave-particle interactions in the Earth's magnetosphere. We will consider the frequency ranges of VLF chorus and electromagnetic ion-cyclotron (EMIC) waves. An attention will be paid to the relationship between wave generation and precipitation of energetic charged particles into the ionosphere. Effects of finite wave packet length on the energy range and efficiency of wave-related particle precipitation in the linear and nonlinear regimes will be considered. We discuss specific VLF chorus and EMIC wave events in which a combination of magnetospheric and low-altitude observations allow one to reveal a connection between the wave generation conditions and precipitation of energetic particles into the ionosphere. This work was supported by the Russian Science Foundation (grant No. 22-62-00048).
ST07-A009
Electron Heating by Magnetic Pumping and Whistler-mode Waves
Victor FRANTSUZOV1#+, Anton ARTEMYEV2, Xiaofei SHI2, Anatoli PETRUKOVICH3
1National Research University Higher School of Economics, 2University of California, Los Angeles, 3Space Research Institute
The investigation of mechanisms responsible for the heating of cold solar wind electrons around the Earth’s bow shock is an important problem of heliospheric plasma physics, because such heating is vitally required to run the drift-shock acceleration at the bow shock. The perspective mechanism for the electron heating is the magnetic pumping that considers electron adiabatic (compressional) heating by ultra-low-frequency waves and simultaneous scattering by high-frequency fluctuations. Existing models of the magnetic pumping have operated with external sources of such fluctuations. In this study, we generalize these models by introducing the self-consistent electron scattering by whistler-mode waves generated due to the anisotropic electron heating process. We consider an electron population captured within a magnetic trap created by ultra-low-frequency waves. Periodical adiabatic heating and cooling of this population drives the generation of whistler-mode waves scattering electrons in the pitch-angle space. The combination of adiabatic heating and whistler-driven scattering provides the electron acceleration and the formation of a suprathermal electron population that can further participate in the drift-shock acceleration.
ST07-A007
Simultaneous Occurrence of Unusually High-frequency EMIC and Magnetosonic Waves: PIC Simulations
Peng XIAO1+, Ameneh MOUSAVI2, Yifan WU1, Zeyin WU1, Zeyu AN1, Kaijun LIU3, Xin TAO1#
1University of Science and Technology of China, 2Space Science Institute, 3Southern University of Science and Technology
Electromagnetic Ion Cyclotron (EMIC) waves and magnetosonic (MS) waves are frequently observed phenomena in the Earth's magnetosphere, playing a critical role in the loss of ring current ions and relativistic electrons. Recent observations have highlighted an interplay between MS waves, anisotropic distributions of suprathermal protons, and high-frequency EMIC waves. A proposed hypothesis for this interaction suggests a coupling process where low energy protons (10–100 eV), heated perpendicularly by MS waves, can generate EMIC waves close to the local proton cyclotron frequency. In this work, we use 2D particle-in-cell (PIC) simulations to investigate the transfer of energy from MS waves to high-frequency EMIC waves. The results show that cold protons can be effectively heated by MS waves, leading to an anisotropic distribution that is unstable to the excitation of high-frequency EMIC waves. Our simulations offer novel insights into the generation of high-frequency EMIC waves, elucidating the energy transfer processes between MS waves and EMIC waves.
ST07-A017
Connection Between Chorus Wave Amplitude and Background Magnetic Field Inhomogeneity: A Parametric Study
Zeyin WU1+, Hua HUANG2, Yifan WU1, Xin TAO1#, Yuto KATOH3, Xiaogang WANG4
1University of Science and Technology of China, 2Research Center of Laser Fusion, 3Tohoku University, 4Harbin Institute of Technology
Whistler mode chorus waves frequently appear as discrete, repetitive, and quasi-monochromatic emissions with frequency chirping. With different wave amplitude and frequency chirping rate, chorus waves have been observed not only in the magnetosphere of the Earth but also in the magnetospheres of other planets, such as Saturn and Jupiter. Motivated by understanding different properties of chorus waves at these planets using the recently proposed “Trap-Release-Amplify” (TaRA) model, we perform a parametric study using Particle-In-Cell simulations by varying background magnetic field inhomogeneity and the corresponding threshold hot electron number density. We show the consistency between simulation results and theoretical predictions for threshold hot electron number density, chorus chirping rate, and wave amplitude. Our results suggest the significant role of the background magnetic field inhomogeneity in affecting chorus wave properties, including its amplitude at different planets as predicted by the TaRA model.
ST07-A021
Substorm Energetic Electron Precipitation: Electron Energy Range and Radial Location of the Precipitation Region
Ying ZOU1, Xiao-Jia ZHANG2#+, Anton ARTEMYEV3, Yangyang SHEN3, Xing MENG4, Vassilis ANGELOPOULOS3
1Johns Hopkins University Applied Physics Laboratory, 2The University of Texas at Dallas, 3University of California, Los Angeles, 4California Institute of Technology
Substorm energetic electron precipitation (EEP) from the equatorial magnetosphere to the atmosphere is the most powerful transient mesoscale driver for atmospheric chemistry dynamics and formation of the low-ionosphere (<100km) conductance layer. Two concurrent mechanisms are potentially responsible for EPP: resonant electron scattering by whistler-mode waves and electron scattering by magnetic field-line curvature in the magnetotail current sheet. The relative contribution of these mechanisms to EPP depends on latitudinal (radial) location of the precipitation regions, with higher importance of curvature scattering poleward from the inner magnetosphere region that is likely dominated by whistler-scattering. However, the low energy resolution of EEP measurements at low altitudes and large uncertainties of projection to the equator often refrains one to determine the precise energy range and radial localization of the substorm EEP. In this presentation, we will discuss one strong substrom EEP event (with electron precipiation up to ~1MeV) that lasts for three hours and covers the radial distance from the plasmapause to the near-Earth plasmasheet. Using ELFIN, Swarm, POES, and THEMIS observations, we show that 50-1000keV EEP within this large radial (latitudinal) domain is likely driven by curvature scattering, due to the earthward motion of the magnetotail current sheet. We also estimate the impact of such strong substrom EEP on the ionosphere ionization, in comparison with precipitation of plasma sheet (<30keV) electrons.
Session Chair(s): Hong-Jin YANG, Korea Astronomy and Space Science Institute
ST23-A003
Aurora Sightings Observed in Chinese History Caused by CIRs or Great-storm CMEs
Shuo YAO#+, Guowei WANG
China University of Geosciences
Auroras observed at middle and low geographic latitudes are related to external inputs and varying geomagnetic fields. This work aims to exclude corotating interaction region (CIR) storms and identify strong coronal mass ejection (CME) storms according to historical auroral records when the geomagnetic field varies substantially. An existing catalog of the aurora records in Chinese history reported by Zeng & Jin from 193 B.C. to 1911 A.D. is used. Archaeomagnetic field models are adopted to estimate the variation of the dipole field. According to the empirical relation between the equatorward boundary of the auroral oval, Dst index, and geomagnetic field intensity, the auroras caused by CIRs can be excluded, and those caused by strong CMEs are identified. After 1500 A.D., China’s magnetic latitude decreased substantially due to the pole shift. This shift provides a better opportunity to investigate the existence of great-level storms. These great-storm CMEs occurred in both solar maximum and minimum. The space weather modeling framework is used to calculate the cusp area and the downward ion flux through the cusp for varied geomagnetic field and solar wind. For the present solar wind condition and tilt angle <15°, stronger geomagnetic field tends to generate a larger cusp area and higher ion flux through the cusp. For the weaker solar wind in the Maunder minimum, the ion flux is lower, but the cusp area is similar to that at present.
ST23-A014
The Millennium Aurora Road — From China to Korean Peninsula, from East Asia to Europe
Yuqi WANG1#+, Yong WEI1, Fei HE1, Limei YAN1, Si CHEN2
1Chinese Academy of Sciences, 2Aerospace Information Research Institute, Chinese Academy of Sciences
Stargazing, a timeless practice connecting humanity to nature, has deeply influenced the historical records of civilizations worldwide. The aurora, a rare optical phenomenon, is documented in the historical records of East Asian and European civilizations. East Asian countries such as China, Korea, Japan, Vietnam, and the Ryukyu Islands have well-documented auroras in Chinese characters. European historical records of auroras below 55° N between 1000 and 1900 have been cataloged, with recent additions from North Africa, the Arabian Peninsula, and the Middle East. Building on Chinese scholars' astronomical surveys in the 1970s and 1980s, we've reorganized an unpublished Chinese aurora chronology from the 1980s. This research framework extends to the Korean Peninsula, where we systematically compile aurora records from ancient Korean history books, forming a comprehensive chronology from 1012 to 1843.Our study examines the colors used in ancient auroral records, classifying the chronology. A comparative investigation spanning China, North Korea, Japan, and Europe identifies solar outbursts and geomagnetic storm events over the past 2,000 years. Analyzing Korea's aurora evolution reveals a strong correlation with the long-term evolution of the regional geomagnetic field, showcasing its profound impact on Earth's atmosphere and space environment. The geographical distribution of aurora records in Asia and Europe aligns significantly with the Silk Road's scope. From the Korean dynasty to Japan, Vietnam, and the Ryukyu Islands, ancestors within the Han cultural sphere documented auroras using Chinese characters, providing insights into their civilizations. This practice extended along the Silk Road, where various cultures documented aurora phenomena in their languages. Today, these records contribute to interdisciplinary research in the history of science, space physics, and planetary science, coining the term "The Millennium Aurora Road" for this precious aurora database spanning the Eurasian continent for thousands of years.
ST23-A009
The Eight-year Solar Cycle During the Maunder Minimum Revealed by Historical Aurora Records
Limei YAN1+, Fei HE1, Xinan YUE1, Yong WEI1#, Yuqi WANG1, Si CHEN2, Kai FAN1, Hui TIAN3, Jiansen HE3, Qiugang ZONG3, Lidong XIA4
1Chinese Academy of Sciences, 2Aerospace Information Research Institute, Chinese Academy of Sciences, 3Peking University, 4Shandong University
The Maunder Minimum (1645–1715 AD) is a representative grand solar minimum with highly depressed activity and coincident with the “Little Ice Age.” The cyclic variation of solar activity, especially the cycle length during this period, is critical to understanding the solar dynamo but remains unknown. By analyzing the solar activity-related red equatorial aurora recorded in Korean historical books, we find a dominant eight-year cyclic variation of solar activity during the Maunder Minimum. This result provides a key constraint to theoretical models of the solar dynamo and the generation mechanism of grand solar minima.
ST23-A013
Relation of Sunspots and Red Auroras Recorded in Korean Chronicles
Rok-Soon KIM#+
Korea Astronomy and Space Science Institute
Records of sunspots and auroras in Korean chronicles have been used for scientific research, such as the solar activity cycle and its influence on the long-term Earth's climate. Using the information from these historical records from the 10th to the 18th century, we identified 38 sunspots and associated 25 red auroras, including sunspot size scaled from 1 to 6 and aurora intensity scaled from 1 to 5 according to the direction, length, and duration. We then examined the relationship between solar activity and Earth’s response in the last millennium. We assumed warm and cold periods before and after AD 1300, in which the warm period includes the Medieval Warming, and the cold period includes several grand minima. As a result, we found that the proportion of large sunspots with a scale of 3 and higher in the warm period (10/15, 66.7%) is three times higher than that in the cold period (5/23, 21.7%), even though the sunspot observation rates are similar in both periods. When we consider only the cold period, the geoeffectiveness of the large sunspots (4/5, 80%) was twice as strong as that of small sunspots of scale 1 or 2 (8/18, 44.4%). We also identified a recursive sunspot observed in 1185, and we speculate that this sunspot might result in similar geomagnetic activity to the Halloween event observed in 2003 due to its size. Based on our results, we suggest that the historical observation of the sunspot and aurora in Korean chronicles is valuable for studying not only long-term solar activity but also extreme solar activity and geomagnetic response. If the sunspot size is quantified through the relationship between the sunspot sketch and the modern sunspot number, the sunspot scale found in Korean chronicles can be a valuable indicator for understanding the Sun-Earth connection.
ST23-A010
Evolution and Disappearance of the Paleo-west Pacific Anomaly: Implications to the South Atlantic Anomaly
Yaochen YUE#+, Jiawei GAO, Yong WEI, Fei HE, Yuqi WANG
Chinese Academy of Sciences
Paleomagnetism and modern geomagnetic measurements indicate that SAA is undergoing rapid changes, with rapid expansion of area and rapid decreasing of intensity. Even in recent years SAA has expanded the minor minima seen in southern Africa. This has led to speculation that the expanding SAA may be an indicator of an upcoming geomagnetic reversal. However, how to know the future evolution direction of SAA is still debatable. Apparently, the study of the changes of other SAA-like structure anomaly regions in history has important implications for the study of SAA evolution. Here, we focus on the evolution and disappearance of the paleo West Pacific Anomaly (WPA). Utilizing the gufm1 model, it is found that WPA occurred between 1620 and 1810 CE. Over its duration, WPA underwent phases of rapid expansion, drift, and split, eventually the primary part vanished, while a new segment persisted and expanded. The striking similarity in evolutionary behavior between WPA and the rapid expansion, drift, and recent splitting in the SAA over the past century is noteworthy. This similarity can be attributed to the fact that WPA, like the SAA, is controlled by the reversal flux patch in the CMB on the northern hemisphere. Therefore, we posit WPA as a significant magnetic anomaly and propose that its evolutionary patterns can serve as predictive indicators for the future evolution of the SAA. Studying the evolution of WPA is an important means to understand the global magnetic field and the evolution of Southeast Asia magnetic field. It is of great significance for us to understand the nature of SAA and predict the evolution trend of SAA.
ST23-A005
Epidemics in Ancient China are Associated with Solar Activity
Si CHEN1#, Yong WEI2, Limei YAN2+, Kai FAN2, Yuqi WANG2
1Aerospace Information Research Institute, Chinese Academy of Sciences, 2Chinese Academy of Sciences
Epidemics perpetually pose a formidable threat to human society. Their causation is intricately linked to climate changes influenced by solar activity which is the Earth's primary energy source. However, the definite mechanisms through which solar activity and climate change synergistically impact the biosphere have remained contentious. Here, we present an extensive analysis utilizing the epidemic index sequences compiled from ancient Chinese historical books spanning over 2000 years. Quantitative statistical analysis establishes a positive association between epidemics and solar activity and uncovering a negative correlation with basic climate variables of temperature and precipitation. On a millennium time scale, solar activity exerts a direct influence on epidemic occurrences, while temperature and precipitation demonstrate indirect adverse effects. Notably, the climate variables contribute substantially more to the variance in epidemic patterns, underscoring the pronounced direct impact of climate factors. These findings suggest that the influence of the Sun on epidemics is more indirect and subject to modulation by additional factors.
Session Chair(s): Libo LIU, Chinese Academy of Sciences, Koichiro OYAMA, International Research Center for Space and Planetary environment Science
ST06-A005
| Invited
Transient Auroral Ionosphere Responses to Interplanetary Shock Prompt Impact
Jianjun LIU#+, Xiangcai CHEN, Zejun HU, Hongqiao HU, Xingxin ZHAO
Polar Research Institute of China
Interplanetary (IP) shock-driven sudden compression of the Earth’s magnetosphere produces electromagnetic disturbances in the polar ionosphere. Disturbed auroral ionosphere results in the intensification of auroral luminosity, plasma convection enhancement and sporadic E layer, which affects the radio wave propagation, degrade accuracy of radio navigation systems and so on. Several studies have examined the effects of IP shock on magnetosphere-ionosphere coupling systems using all-sky cameras and radars. In this study, we examine responses and drivers of the polar auroral ionosphere following an IP shock prompt compression on 16 June 2012. We observe the vertical drift and concurrent horizontal motion of the plasma. Observations from digisonde located at Antarctic Zhongshan station (ZHO) showed an ionospheric thick E region ionization and associated vertical downward plasma motion at F region. In addition, horizontal ionospheric convection reversals were observed on the Super Dual Auroral Radar Network (SuperDARN) ZHO and McMurdo (MCM) radar observations. Observational findings suggest that the transient convective reversal breaks the original shear equilibrium, it is expected that the IP shock-induced electric field triggers an enhanced velocity shear mapping to the E region. The horizontal motion of the plasma was attributed to the dusk-to-dawn electric field that existed during the preliminary phase of sudden impulse (SI) triggered by the IP shock. We also found that ionospheric convection reversals were driven by a downward field-aligned current. The results of these observations reveal the immediate and direct auroral ionosphere response to the IP shock, which is critical for understanding the global response of the magnetosphere following an abrupt change in IMF and solar wind conditions.
ST06-A004
Global Ionosphere Morphology Study with Coarse-grained Complex Network Models
Shihao WANG, Yang LIU#+, Kunlin YANG
Beihang University
Currently, the International GNSS Services uses nearly 500 observation stations globally on the ground to derive the global morphology for ionospheric total electron content. The resulting global ionospheric TEC map has become the main data source for studying the global ionosphere variabilities. Moreover, there are over 4000 ground GNSS observatories globally, constituting dense GNSS ionospheric observation network. With all those data sources, the global and regional ionospheric morphology can be investigated. The application and development of complex climate network sheds lights on related geoscience and space physics studies. By constructing a ionosphere complex network model, the spatiotemporal variation in ionosphere can be extracted more precisely. To address the problem, we apply complex network model to extract the spatiotemporal morphology and anomalies in ionosphere. The global ionosphere grids are established with global ionospheric map data, and the coarse-grained complex network is further constructed. The key nodes are well investigated, identified by degree, betweenness, cluster coefficients. Two coarse-grained methods are tried and discussed, the efficient information emergence method and reinforcement learning method. The constructed complex network model is tested with geomagnetic storms events in the recent two solar cycles. The spatial coupling mechanisms are revealed for different regions in different latitudes. The experimental results show that: 1) There is a strong negative correlation between the statistical features of the ionospheric network and the changes in geomagnetic index. The larger the intensity of the magnetic storm, the worse the global connectivity will be. 2) Solar activity significantly affects the general features of the ionospheric network, and intense solar activity enhances the connectivity of the network. 3) The ionospheric variations in low latitude regions demonstrate a greater impact on the global ionosphere compared to the rest regions, and the contributions of different regions to the ionosphere response vary to different geomagnetic storms.
ST06-A006
Reproduction of Electron Density in the Ionospheric D Region During Solar Flares Using PHITS and GAIA Models
Shinnosuke KITAJIMA1#+, Kyoko WATANABE1, Hidekatsu JIN2, Chihiro TAO2, Satoshi MASUDA3, Michi NISHIOKA2, Kiyoka MURASE4
1National Defense Academy of Japan, 2National Institute of Information and Communications Technology, 3Nagoya University, 4The Graduate University for Advanced Studies
Shortwave fadeout (SWF) occurs when the electron density in the ionospheric D region increases rapidly in a short period, mainly due to X-ray emission during solar flares. It is necessary to accurately understand the electron density variation in the ionosphere to estimate the occurrences of SWFs and their magnitudes. The GAIA (Jin et al., 2011) is one of the effective numerical simulation models for the whole global atmosphere, which can provide electron density variations throughout the ionosphere in solar flare emissions. However, it still does not account for photochemical reactions in the ionospheric D region. In this study, we used the PHITS code (Sato et al., 2023), a particle transport and collision simulation code using the Monte Carlo method, to reproduce electron density variations in the ionospheric D region due to flare X-ray emission. We input the GOES X-ray data into PHITS and simulated the altitude distribution of the ionization rate (q). We used the effective recombination coefficient (αeff) given by Gledhill (1986) and derived the electron density (ne) in the D region from ne2 =q/αeff . The variations of minimum frequency in the ionogram (fmin) during solar flares correspond to the electron density variations in the D region. We simulated fmin value using the electron density from the PHITS and GAIA. We compared their simulated fmin with observed fmin and validated the reproduction of electron density using PHITS. We also compared the electron density using PHITS with the observed electron density. The correlation coefficient between the simulated and observed fmin values indicated a good correlation of 0.87 by a linear function, and the true positive rate was ~70%. We found that PHITS might reproduce the electron density at the peak time of flare. In this presentation, we will discuss the reproduction of electron density variations using PHITS in detail.
ST06-A010
Occurrence of Red-green Low Latitude Aurora During Large Geomagnetic Disturbances: Case Studies
Manu VARGHESE1#+, Kazuo SHIOKAWA2, Balan NANAN3, Shreedevi P. R.2, Qing-He ZHANG4,3
1National Space Science Centre, 2Nagoya University, 3Shandong University, 4National Space Science Center, Chinese Academy of Sciences
Low latitude auroras are seen during large geomagnetic disturbances when precipitation of electrons from the inner magnetosphere occur. Stable Auroral Red (SAR) arcs formed from the overlap region between outer plasmasphere electrons and ring current ions contribute to 630 nm (red) emission in the equatorward edge of the auroral oval. Broadband flux of low energy electrons from the inner magnetosphere causes red-green auroras at low latitudes. However, the red emissions alone are usually seen because the green emissions are hidden below the horizon. Recent observations of the low latitude auroras at Rikubetsu (magnetic latitude, 34.70 N), in Japan in the rising phase of solar cycle 25 have shown comparable red-green intensity, which are unusual compared to previous observations. Two such events occurred during the geomagnetic storms on 28 February 2023 and 24 April 2023 (F10.7 = 157.9 and 135.5, SymHMin = -161 nT and -233 nT). Satellites overpasses over the location at the time of low latitude auroras have shown that the auroral oval expanded equatorward to ~480 N magnetic latitude. The study investigates the physical mechanisms responsible for these events using all sky images, solar wind and IMF parameters, magnetometer measurements and ionospheric (NOAA, SWARM and DMSP) satellites.
ST06-A017
Global Thermosphere Atmospheric Density Monitoring Using the Upcoming LEO Constellations
Yu GUO+, Xiaohong ZHANG, Fei GUO#
Wuhan University
Neutral atmospheric density is an important physical indicator in the study of the thermosphere. The upcoming Low-Earth-Orbit (LEO) satellite constellation will bring more opportunities for atmospheric density measurement and thermosphere monitoring. In this paper, we present a method to monitor global small-scale neutral atmospheric density using the upcoming LEO constellation. We conduct preliminary simulations and evaluations based on the atmospheric density generated by the Walker constellation and the NRLMSISE-00 model. The simulation results show that within the altitude range of 300 km to 600 km, reliable small-scale atmospheric density calculation can be achieved by using about 2,000 LEO satellites in a single layer. Furthermore, we develop a differentiated satellite usage strategy (HTLL) to address the sensitive phenomenon of atmospheric changes in high-latitude regions. The simulation results indicate that this differentiated satellite distribution approach can greatly reduce the number of satellites used while maintaining high-precision calculations. The methods presented in this paper have potential for future applications in the development of thermosphere-related scientific research and space security.
ST06-A014
The Electron Heat Fluxes Associated with Electron Precipitation in the Region of Diffuse Aurora
George KHAZANOV1#+, Suk-Bin KANG2
1NASA Goddard Space Flight Center, 2CUA IACS/ NASA GSFC
Electron heat flux that comes from the magnetosphere to the upper ionospheric altitudes controls the value of electron temperature in the core plasma, scale height, and, as a result, the total electron density content that is required for different kinds of space weather applications. Knowing the thermal electron heat flux at the upper ionospheric boundaries is the Achilles' heel of all ionospheric models. Such a thermal heat flux setting is especially difficult to justify in the region of the diffuse aurora that is connected to a large energy reservoir of electrons with energies of a few kiloelectron volts, the Earth's plasma sheet, where magnetosphere-ionosphere coupling processes are strongly interconnected. We use the simulated heat flux provided by SuperThermal Electron Transport (STET) code to estimate electron temperatures at the upper ionospheric altitudes and compare these results with corresponding observations from the Defense Meteorological Satellite Program satellite during Saint Patrick's Days 2013 and 2015 Geomagnetic Storms.
Session Chair(s): Linghua WANG, Peking University
ST01-A028
| Invited
Recent Observation and Modeling of the Sidereal Cosmic-ray Anisotropy at TeV Energies with the Tibet ASgamma Experiment
Kazumasa KAWATA#+
The University of Tokyo
Anisotropic features in the arrival directions of galactic cosmic rays at the sidereal time frame have been observed by various experiments including underground muon telescopes and ground-based air-shower arrays. The sidereal anisotropy at TeV energies observed at the Earth has two distinct large-scale structures: a deficit region ranging from ~150◦ to ~240◦ in Right Ascension (Loss-Cone) and an excess region from ~40◦ to ~90◦ (Tail-In), and recent high-statistics experiments have revealed that the amplitude and phase of the anisotropy dramatically change above ~100 TeV from those below ~100 TeV. In this presentation we study how the anisotropy at the heliospheric outer boundary can be modeled at TeV energies, by applying the idea of Liouville mapping to the experimental data of the Tibet ASgamma experiment.
ST01-A008
Numerical Modeling of Energetic Proton Precipitation to Explore the Origin of the Sustained Gamma-ray Solar Flare
Zelong JIANG1#+, Xiangliang KONG1, Fan GUO2, Meng JIN3, Xiaocan LI4, Feiyu YU1, Wenlong LIU1, Yao CHEN1
1Shandong University, 2Los Alamos National Laboratory, 3Lockheed Martin Advanced Technology Center, 4Dartmouth College
The powerful solar eruptions are often associated with sustained high-energy (>100 MeV) gamma rays. For example, during a powerful solar blast on 2012 March 7, the Fermi-LAT detected the longest sustained gamma-ray flare that lasted about 20 hours. More interestingly, the Fermi-LAT observed sustained gamma-ray emission from the solar eruption located on the back side of the sun, which should block direct light from the solar flare. A possible explanation is the coronal mass ejection (CME) shock-accelerated >300 MeV protons precipitate on the photosphere to produce the sustained gamma-ray via pions decay. However, a detailed simulation of the proton precipitation is still lacking. Here, we numerically model the precipitation of energetic protons by combining the data-driven magnetohydrodynamic (MHD) CME module with the particle transport model, then simulate the gamma-ray production process from the interaction of the precipitated protons with the solar atmosphere using the GEANT4 Monte Carlo package, which allows us to make direct comparison with the Fermi-LAT data. We use this model successfully to reproduce the sustained gamma-ray flare event on 2014 September 1. Our simulation results indicate that the sustained gamma rays were produced by shock-accelerated protons along the open field lines precipitating to the visible solar disk.
ST01-A012
| Invited
Solar Energetic Neutral Atoms – A New Window for Understanding the Physics of Solar Energetic Particles
Mihir DESAI1#+, Glenn MASON2, George HO1, Christina COHEN3
1Southwest Research Institute, 2Johns Hopkins University Applied Physics Laboratory, 3California Institute of Technology
Our Earth and the heliosphere are routinely impacted by solar disturbances e.g., flares, coronal mass ejections (CMEs), and solar energetic particles (SEPs). SEPs pose radiation threats to humans and technology. Despite recent progress, the origin and acceleration of SEPs is hotly debated. Flare-reconnection and CME-shock acceleration are two possibilities. Since in-situ SEP properties are altered during transit, knowledge of the unexplored region near the Sun is a fundamental missing piece. Recent observations show that energetic neutral atoms (ENAs) created by charge exchanging SEPs with the neutral coronal plasma can be detected at Earth. These ENAs travel unaffected by propagation effects, thus providing a sample of near-Sun SEP populations and bearing information about their sources and acceleration processes. Simultaneous measurements of SEPs and ENAs in individual events can help discriminate between the two solar sources. In this talk we discuss the tremendous potential that ENAs offer for advancing our understanding of SEP physics, and ultimately developing a reliable SEP monitoring and forecasting capability for safeguarding our home, technological assets and future deep space exploration.
ST01-A020
Forecasting Solar Energetic Particle Events Using the SEPcaster Model
Gang LI1#+, Meng JIN2, Sailee SAVANT3
1Macau University of Science and Technology, 2Lockheed Martin Advanced Technology Center, 3The University of Alabama in Huntsville
Solar energetic particles are the main safety concerns of astronaut and a major space weather hazard as they can damage ground- and space-based technological systems. A state-of-the-art forecasting model to accurately predict the time profile and spectra of these particles is becoming an urgent need in today's technology-advanced society. In this talk, I describe a physics-based operational SEP Forecast model, SEPCaster, for the energetic particle radiation environment in the inner solar system and Earth's magnetosphere. SEPCaster is based on two advanced research models: the Alfven Wave Solar Model (AWSoM) and the improved Particle Acceleration and Transport (iPATH) model. It operates in two distinct modes: an automated forecasting mode and a user-interactive mode. In the automated mode, SEPCaster runs with minimal human interaction, while in the interactive mode, users can modify the inputs and analyze specific events in greater detail. SEPcaster contains three modules: the first module automatically identifies and characterizes active regions (ARs). It then extracts eruption parameters including CME speeds and directions; these parameters are passed to the EEGGL/AWSoM module, which is the second module of SEPCaster, the physics process of CME eruption is followed in this module, producing the CME-driven shock profiles and the background solar wind profiles; these profiles are passed to the third module of SEPCaster, where the acceleration of SEPs at the shock front, the subsequent propagation of SEPs in the solar wind, are followed. The output of the SEPCaster model includes both time profiles of SEPs of given energy, and time-volving SEP spectra at locations of interest.
ST01-A029
Solar Flare Impulsivity and Its Relationship with White-light Flares and With CMEs
Kyoko WATANABE1#+, Seiji YASHIRO2,3, Satoshi MASUDA4, Nariaki NITTA5
1National Defense Academy of Japan, 2The Catholic University of America, 3NASA Goddard Space Flight Center, 4Nagoya University, 5Lockheed Martin Advanced Technology Center
The flare class (magnitude of solar flare) is one of the important parameters used in space weather forecasting. However, there are many examples where the flare class is not proportional to the magnitude of space weather phenomena. Also, even for solar flare emission only, thermal and non-thermal aspects of solar flare emission may not be proportional, and each shows different aspects. For example, hard X-ray emission is not so strong even in X-class flare, or hard X-ray is observed even in C-class flare. Also, most of large solar flares are accompanied by a CME, but it is not in some cases. Currently, there are no indicators for non-thermal aspects and/nor with or without CME. Therefore, in this study, based on the concept of Neupert effect (Neupert, 1968), we defined the non-thermal aspect as the impulsive parameter (IP), and investigated the relationship between the white light flare (WLF) which have non-thermal aspects and the occurrence of CME. We investigate how WLF depends on IP, then it is found that WLF tend to have large IP values. So the flare IP is one of the important factors if WL enhancement appears or not in a solar flare. Then, we investigated how CME itself and/or its physical parameters depend on IP index. It has been believed that most of CMEs are associated with long duration events (LDEs), but we found that there is only a weak correlation between the existence of CME and IP index, even small IP number is indicated LDEs. Finally, we also search for the relationship between WLF and CME as a function of IP and discuss the physical condition of WLF.
ST01-A023
Energy Spectra of Energetic Electrons in the Outermost Region of the Terrestrial Radiation Belt
Qianyi MA#+, Linghua WANG, Qiugang ZONG, Yongfu WANG, Zou HONG
Peking University
The energy spectrum of energetic particles can reflect the physical nature of their source/acceleration. In order to understand the not-well-known formation process of energetic electrons in the terrestrial outer radiation belt, here we present a comprehensive survey of the 50-600 keV electron energy spectra observed by the Beida Image Electron Spectrometer (BD-IES) onboard a Chinese Navigation BeiDou satellite in the outermost (L~6.5-10) radiation belt from October 2015 to February 2020. We utilize the pan-spectrum fitting method to self-consistently determine the energy spectral shape of omnidirectional electron fluxes, after considering the uncertainties both in electron flux J and energy E. During quiet times (substorm/storm periods), the selected 6707 (2369) samples are classified into three spectral groups: 6142 (1781) show a downward-bending (DB) spectrum, 429 (463) exhibit an upward-bending double-power-law (UDPL) spectrum, and 136 (125) have a single-power-law (SPL) spectrum. The DB group is further divided into three types: 63% (74%) with a downward-bending double-power-law (DDPL) spectrum, 21% (15%) with a logarithmic parabola (LP) spectrum, 15% (10%) with a generalized Ellison-Ramaty (ER) spectrum. We find that during quiet times, the SPL type shows the lowest electron fluxes and likely originates from the superhalo electrons observed by WIND in the interplanetary space via the adiabatic acceleration. The quiet times SPL type can serve as the seed population for the further acceleration processes in the magnetosphere to form the other spectral types during quiet times and substorm/storm periods.
Session Chair(s): Simon WING, The Johns Hopkins University
ST21-A003
Plasma Key Dynamics Understand by 3D Global MHD Simulations
Kyung Sun PARK#+
Chungbuk National University
One of the major challenges in magnetospheric physics is to understand the nature and processes that occur at the magnetopause and the magnetotail regions. For a long time, many observational and model studies have sought to determine the amount of energy and how it is transported process from the solar wind through the magnetosphere into the ionosphere. Global MHD simulations are a powerful tool for investigating the magnetic field topology and dynamics of the magnetosphere. Global simulation results show that magnetic reconnection is most efficient for southward interplanetary magnetic field (IMF), with the largest rates occurring where the magnetosheath magnetic field is nearly antiparallel to the geomagnetic field even including tilt effects. Viscous-like interaction at the magnetopause boundary can also be driven by the velocity shear with a rapid magnetosheath plasma even for southward IMF with By component. The simulation results suggested that magnetic reconnection at dayside magnetopause plays a significant role in the formation and periodic oscillation behavior of vortices. While significant progress has been made, questions remain unanswered. 1. How do magnetic reconnection and vortices occur in a highly asymmetric magnetosphere under weak and strong solar wind conditions? 2. What are the differences in the generation of vortices on the magnetopause and inside the magnetopause? 3. How do magnetic reconnection and vortex formation that occur on Earth's magnetosphere differ on other planets? This study aims to answer the questions from the simulation results of simulation of the magnetic 3D magnetic field configuration, dynamics, and plasma properties of the magnetosphere.
ST21-A001
| Invited
Kelvin-Helmholtz Instabilities Viewed by Global Hybrid Simulations of the Magnetosphere
Yu LIN1#+, Katariina NYKYRI2, Xuanye MA2, Jay JOHNSON3, Arthur HULL4, Peter DAMIANO5, Xueyi WANG1, Mark L. ADRIAN1
1Auburn University, 2Embry-Riddle Aeronautical University, 3Andrews University, 4University of California, Berkeley, 5University of Alaska Fairbanks
Surface waves due to Kelvin-Helmholtz instabilities (KHI) at the magnetopause boundary regions are believed to provide a major mechanism for the mass and energy transfer from the solar wind to the magnetosphere. Kinetic-scale physics has been shown to play key roles in the nonlinear KHI structures and in the associated particle transport. While the physics of KHI has been studied for decades, the solar wind control of its excitation and effects on global magnetospheric structure has only recently become available at required high-resolution using global simulations of the magnetosphere. In this talk, we take a close look at the generation and global-kinetic physics of KH waves in the magnetosphere with 3D global hybrid simulations using ANGIE3D. Our study will focus on a case under a northward IMF with finite By, in which KH waves are found at the high-latitude magnetopause, low-latitude boundary layer, around the cusp region, as well as in the plasma sheet turbulence. Our discussion will include the relationship between these KH waves and magnetic reconnection in the magnetosphere, as well as the roles of the kinetic-scale KHI in particle dynamics.
ST21-A008
PIC Simulation of Electron Only Kelvin-Helmholtz Instability at the Dayside Magnetopause
Eunjin CHOI1#+, Kyoung-Joo HWANG1, Kyunghwan DOKGO1, James BURCH1, David SIBECK2
1Southwest Research Institute, 2NASA Goddard Space Flight Center
The Kelvin-Helmholtz instability is one of the most important physical processes occurring on the dayside magnetopause. It has been widely studied within the MHD framework, often considering thicknesses of many ion gyroradii. However, several studies suggest the presence of a thin velocity shear layer at the subsolar region with a thickness less than an ion gyroradius. The significance of kinetics becomes more pronounced when the thickness of the velocity shear layer approaches the ion gyroradius. To account for the effects of particle kinetics, we conducted particle-in-cell (PIC) simulations, exploring how the Kelvin-Helmholtz instability is excited along such a thin dayside magnetopause. Our simulations reveal the evolution of an electron-only Kelvin-Helmholtz vortex preceding the occurrence of fluid-scale Kelvin-Helmholtz instability. As these vortices grow, the electron-only rolled-up flow generates current and magnetic field increase/decrease at the center of the vortex. We demonstrate the difference of electron-only vortices depending on the relative direction of shear velocity to the background magnetic field. Our simulation results are compared with the in-situ observation of the electron-only vortex observed by MMS, enabling the interpretation of detailed kinetics and evolution of the electron-only vortex.
ST21-A013
| Invited
Coupling of Kelvin-Helmholtz Vortices to the Ionosphere
Jay JOHNSON1#+, Alexander NAVARRO1, Simon WING2, Peter DELAMERE3, Shiva KAVOSI4, Steven PETRINEC5
1Andrews University, 2The Johns Hopkins University, 3University of Alaska Fairbanks, 4Embry-Riddle Aeronautical University, 5Lockheed-Martin
Shear in the flow at magnetopause boundaries leads to growth of Kelvin-Helmholtz waves, which develop nonlinearly into vortex structures. The twist in the field within these vortices generates field-aligned currents that contribute to magnetosphere-ionosphere coupling and power auroral emissions. Auroral bright spots have been observed at Earth, Jupiter, and Saturn in regions that map to the boundary layer, and it has been suggested that the bright spots are associated with Kelvin-Helmholtz vortices. We develop a quasi-static model to determine how the field aligned current structure depends on ionospheric and boundary layer parameters for vortex structures. A key finding is that there is an optimal vortex size that maximizes the strength of field-aligned currents and auroral precipitation. However, as the strength of the vortex increases beyond the linear regime, the current saturates, and the current broadens. For comparison with observations, we consider events where auroral bright spots are detected by DMSP SSUSI FUV when KH structures are observed by THEMIS/Cluster.
ST21-A011
KHIWI: Kelvin-Helmholtz Instability/Wave Investigation Mission Concept
Kyoung-Joo HWANG1#+, Katariina NYKYRI2, Chih-Ping WANG3, Hiroshi HASEGAWA4, James BURCH1, Stephen FUSELIER1, Andrei RUNOV3, Viacheslav MERKIN5, Mikhail SITNOV5, Takuma NAKAMURA6, Xuanye MA7, Kyunghwan DOKGO1, Eunjin CHOI1, Jerry GOLDSTEIN1,8, Yu LIN9, Xueyi WANG9
1Southwest Research Institute, 2NASA Goddard Space Flight Center, 3University of California, Los Angeles, 4Japan Aerospace Exploration Agency, 5Johns Hopkins University Applied Physics Laboratory, 6Austrian Academy of Sciences, 7Embry-Riddle Aeronautical University, 8The University of Texas, 9Auburn University
We present the conceptual framework of the Kelvin-Helmholtz Instability/Waves Investigation (KHIWI) mission. KHIWI aims to fill the gaps in our understanding of the magnetospheric system that have resulted from paying less attention to the flank magnetosphere and magnetopause dynamics associated with Kelvin-Helmholtz Instability (KHI). The roles and importance of this element in the solar wind-magnetosphere coupling (Q1), transport and escape of energetic particles (Q2), and the onset of the central magnetotail plasma sheet dynamics (Q3) have remained elusive. Answering Q1 enables us to ultimately resolve the long-standing Axford-Hines/Dungey dichotomy. Answering Q2, when combined with answering Q1, completes our understanding of roles and impact of flank dynamics as a channel for two-way transport. Answering Q3 impacts our understanding of the drivers of the unstable central current sheet and its self-consistent behavior via communications with flank dynamics. Coordinated measurements using two polar orbiters and three equatorial orbiters, for the first time, quantify the relative importance and effectiveness of KHI in the solar wind transport as well as plasma heating and acceleration in comparison to dayside subsolar and cusp reconnection. Three equator-orbiting satellites simultaneously probing the near-midnight plasma sheet and the dawn/dusk magnetopause, for the first time, explore a paradigm-shifting causality between unstable magnetotail current sheets and flank-side dynamics. This presenation focuses on these long-lasting and unexplored problems on Heliophysics research, offering a mission concept optimized for addressing these science questions.
Session Chair(s): Xuzhi ZHOU, Peking University, Xin TAO, University of Science and Technology of China
ST07-A014
| Invited
Effects of Nonlinear Interactions Between Electrons and Whistler-mode Chorus Waves on Precipitation of Different Timescales
Longzhi GAN1#+, Wen LI1, Qianli MA1,2, Jay ALBERT3, Kelly CANTWELL4, Robyn MILLAN4, Miroslav HANZELKA5
1Boston University, 2University of California, Los Angeles, 3Air Force Research Laboratory, 4Dartmouth College, 5GFZ German Research Centre for Geosciences
Nonlinear interactions between energetic electrons and whistler-mode chorus waves play a crucial role in driving electron precipitation. Phase bunching scatters electrons far from the loss cone into it, creating an additional source of precipitation. Meanwhile, anomalous scattering, which includes anomalous trapping and positive bunching, scatters electrons away from the loss cone, thereby reducing the source of precipitation that originates close to the loss cone. This source is the only one considered in quasilinear theory. This presentation studies the effects of nonlinear interactions between electrons and chorus waves on precipitation on two typical timescales. The shorter timescale ranges from 1 to 2 electron bounce periods, representing the typical timescale of microbursts. The other timescale exceeds tens of electron bounce periods, reaching a quasi-equilibrium state. Test particle simulations and theoretical analyses evaluate both timescales, indicating that nonlinear effects on precipitation are more significant at lower energies in the range of tens of keV. Furthermore, we demonstrate that realistic wave spectra and waveforms diminish the effects of nonlinear interactions close to the loss-cone, leading to simultaneous quasilinear and nonlinear precipitation. Additionally, we discuss the implications of these results on Low-Earth-Orbit (LEO) and stratospheric observations, such as the Balloon Array for Radiation Belt Relativistic Electron Losses (BARREL).
ST07-A003
Relativistic Electron Precipitation Driven by Mesoscale Transients in the Earth Magnetosphere
Anton ARTEMYEV1#+, Xiao-Jia ZHANG2, Andrei DEMEKHOV3,4, Xing MENG5, Vassilis ANGELOPOULOS1
1University of California, Los Angeles, 2The University of Texas at Dallas, 3Polar Geophysical Institute, 4Russian Academy of Sciences, 5California Institute of Technology
Precipitation of relativistic electrons into the Earth’s atmosphere regulates the outer radiation belt fluxes and contributes to magnetosphere-atmosphere coupling. One of the main drivers of such precipitation is electron scattering by whistler-mode waves. Such waves typically originate at the equator, where they can resonate with and scatter sub-relativistic (tens to a few hundred keV) electrons. However, they can occasionally propagate far away from the equator along field lines, reaching middle latitudes, where they can resonate with and scatter relativistic (>500 keV) electrons. Such a propagation is typical for the dayside, but statistically has not been found on the nightside where the waves are quickly damped along their propagation due to Landau damping. Here we explore two events of relativistic electron precipitation from low-altitude observations on the nightside. Combining measurements of whistler-mode waves from ground observatories, relativistic electron precipitation from low-altitude satellites, total electron content maps from GPS receivers, and magnetic field and electron flux from equatorial satellites, we show wave ducting by plasma density gradients is the possible channel that allows the waves to reach middle latitudes and scatter relativistic electrons. We suggest that both whistler-mode wave generation and ducting can be driven by equatorial mesoscale (with spatial scales of about one Earth radius) transient structures during nightside injections. We also compare these nightside events with observations of ducted waves and relativistic electron precipitation at the dayside, where wave generation and ducting are driven by ultra-low-frequency waves. This study demonstrates the potential importance of mesoscale transients (injections and ultra-low-frequency waves) in whistler-mode wave ducting and relativistic electron precipitation.
ST07-A005
Saturation Properties of Oblique Whistler Waves Generated by Low-beta Electrons
Yifan WU+, Xin TAO#
University of Science and Technology of China
Whistler mode waves are commonly observed in space plasma environments, including planetary magnetospheres and solar wind. While most whistler waves are driven by temperature anisotropy and propagate parallel to the background magnetic field, whistler waves tend to be excited in the oblique direction when electron plasma beta is very low (<0.025). Although the linear theory can explain the excitation processes of obliquely propagating whistler waves, the saturation properties and the parameter dependences remain undiscovered. In this work, we use the 2-dimensional PIC simulations to study the full-process wave-particle interactions of these waves. By scanning wide parameter ranges, we investigate the saturation properties of whistler waves and plasma parameters, including the wave intensity, the saturated temperature anisotropy, plasma beta, and linear instability threshold. The results should benefit the construction of numerical global plasma models by connecting wave and plasma parameters.
ST07-A006
Plasmaspause Surface Waves and Sawtooth Aurora
Jie REN#+
China University of Geosciences
Recent studies proposed that plasmapause surface waves (PSWs) might be the trigger of sawtooth auroras and showed the global distribution of sawtooth auroras in the upper atmosphere. However, it is unknown how PSWs are distributed in the magnetosphere and what triggers their generation. Six-year data from Van Allen Probes were used to investigate the spatial distributions and occurrence conditions of PSWs in the period of 5–30 min. My research revealed an obvious dawn-dusk asymmetry with highest occurrence rates at MLT = 15–21, which is consistent with sawtooth auroras, and found that the occurrence of PSWs is related to substorm activities. We also proposed that the preferential distribution of PSWs and sawtooth auroras in the duskside is probably due to the existence of plasmaspheric plume which can affect the excitation and propagation of eigenmode ULF waves due to the change of local Alfven speed. Besides, we found the existence of proton sawtooth aurora which should be related to the scattering caused by EMIC waves.
ST07-A004
Energetic Particle Precipitation in Sub-auroral Polarization Streams
Xiao-Jia ZHANG1#+, Anton ARTEMYEV2, Ying ZOU3, Xing MENG4, Vassilis ANGELOPOULOS2
1The University of Texas at Dallas, 2University of California, Los Angeles, 3Johns Hopkins University Applied Physics Laboratory, 4California Institute of Technology
Sub-auroral polarization streams (SAPS) are one of the most intense manifestations of magnetosphere-ionosphere coupling associated with the formation of intense field-aligned currents and strong polarization fields related to the ionospheric closure of those currents. Magnetospheric energy transport to the ionosphere within SAPS is associated with Poynting flux and the precipitation of thermal-energy (0.03-30 keV) plasma sheet particles. However, much less is known about the precipitation of high-energy (>50 keV) ions and electrons and their contribution to the low-altitude SAPS physics. This study examines precipitation within SAPS using the combination of equatorial THEMIS and low-altitude Swarm, DMSP, and ELFIN observations, which, jointly, cover the entire energy range of interest from a few eV up to a few MeV. We show that SAPS are usually embedded by the ion isotropy boundary, which includes strong 300-1000 keV ion precipitation. We also find that SAPS are commonly associated with intense precipitation of relativistic electrons (~3 MeV), well equatorward of the electron isotropy boundary. Such relativistic electron precipitation is likely due to electron scattering by electromagnetic ion cyclotron waves at the equator.
ST07-A011
Statistical Properties of Whistler Mode Waves Near the Lunar Surface by ARTEMIS
Abdul WAHEED1+, Xin TAO1#, Anton ARTEMYEV2
1University of Science and Technology of China, 2University of California, Los Angeles
During this study we investigate the statistical properties of whistler mode waves near the lunar surface. Whistler mode waves might play an important role in the loss and acceleration of energetical electrons near the lunar surface. These lower band whistler waves generated by anisotropy of upward electrons caused by surface absorption combined with magnetic reflection by crustal magnetic fields. In this study, we automatically detected lower band whistler waves from 10 years of ARTEMIS (Acceleration, Reconnection, Turbulence, and Electrodynamics of the Moon's Interaction with the Sun) mission. These lower band whistler waves have high occurrence rate at lower Altitude (RL(SSE) < 2), which indicate that lunar environment control the excitation of these waves. We performed the wave polarization analysis which shows these waves are quasi-parallel. We have further investigated the diffusion coefficient and main properties of lower band whistler wave near the lunar surface (RL(SSE) < 2). Our studies are beneficial to understanding the plasma environment near the lunar surface.
Session Chair(s): Yuqi WANG, Chinese Academy of Sciences
ST23-A015
Solar Activities and Climate Change During the Last Millennium Recorded in Korean and Chinese Chronicles
Hong-Jin YANG1#+, Chan-Gyung PARK2, Rok-Soon KIM1, Kyungsuk CHO1, Junhyeok JEON3
1Korea Astronomy and Space Science Institute, 2Jeonbuk National University, 3Chungbuk National University
Korean chronicles have a large amount of observational records of natural phenomena, including astronomical and meteorological events over two thousand years. Here we examine the correlation of solar activity and climate change from historical sunspot and frost records in the Korean chronicles. There are 42 sunspot records in Goryeo Dynasty (918–1392 CE) and 13 records in Joseon Dynasty (1392–1910 CE). The sunspot records in Goryeo Dynasty show a periodicity in good agreement with the well-known solar activity of 11 years. Korean sunspot records suggest that the solar activity in Joseon Dynasty decreased compared with that in the previous ∼500 years. In order to examine the long-period variation of solar activity, we include Chinese historical sunspot records in our analysis to supplement the lack of Korean records, and find a new ∼240-yr long-period solar activity from the power spectral analysis. Korean chronicles also have about 700 frost records during the last millennium. We investigate these frost records and find a sign of cooling down that can be interpreted as climate change during the last millennium. We also find ∼240-yr cooling period from the historical frost records, which is well in accord with that of solar activity. Therefore, we conclude that the solar activity has decreased during the last one thousand years and also has a long-term variation of ∼240 years.
ST23-A006
Long-term Evolution of the Thermosphere During the Holocene: Circulation and Solar Tides
Xu ZHOU1+, Y.H. CAI1, Zhipeng REN2, Yong WEI1, Yongxin PAN1, Xinan YUE1#
1Chinese Academy of Sciences, 2INSTITUTE OF GEOLOGY AND GEOPHYSICS, CHINESE ACADEMY OF SCIENCES
On timescales longer than the solar cycle, long-term changes in CO2 concentration and geomagnetic field have the potential to affect thermospheric dynamics. In this paper, we investigate the thermospheric dynamical response to these two factors during the Holocene, using two sets of ~12,000-yr control runs by the coupled thermosphere-ionosphere model, GCITEM-IGGCAS. The main results indicate that increased/decreased CO2 will enhance/weaken the thermospheric circulation throughout the Holocene, but this effect is nonlinear. The cooling effect of CO2 in the thermosphere further provides plausible conditions for atmospheric tidal propagation and increases the thermospheric tidal amplitude. Geomagnetic variations induce hemispheric asymmetrical responses in the thermospheric circulation. Large changes in the circulation occur at high latitudes in the hemisphere with distant magnetic poles drift, inferring a crucial role of geomagnetic non-dipole variations in circulation changes. A positive correlation between the diurnal migrating tide (DW1) and geomagnetic dipole moment is revealed for the first time. The amplitude of DW1 in temperature will increase by ~1–3 K for each 1×1022 Am2 increase in dipole moment.
ST23-A012
The Efficiency of Coronal Mass Ejection with Different IMF Preconditions on the Production of Megaelectronvolt Electron Content in the Outer Radiation Belt
Chongjing YUAN1+, Qiugang ZONG2#
1INSTITUTE OF GEOLOGY AND GEOPHYSICS, CHINESE ACADEMY OF SCIENCES, 2Peking University
Fifty-two coronal mass ejections (CMEs) from 2012 to 2017 are categorized into four types according to different interplanetary magnetic field (IMF) preconditions, and behaviors of 1.8-, 3.4-, 5.2- and 7.7 MeV electrons are quantitatively investigated using an Radiation Belt Content (RBC) index improved for nondipolar geomagnetic field configuration due to interaction with CMEs. Statistical analyses show that CMEs with continuous southward IMF from upstream of shock front to CME leading edge are the most efficient in the production of megaelectronvolt electron content, with RBC five times larger after shock arrival for 1.8-MeV channel, seven times larger for 3.4-MeV channel, and three times larger for 5.2-MeV channel; the 7.7-MeV channel also experiences less pronounced enhancements. For CMEs with continuous northward IMF from upstream of shock front to CME leading edge, clear dropouts of RBC are revealed. The depletion is the most significant for 1.8 MeV, and the magnitude of depletion gradually decreases when the electron energy goes higher. It is suggested that the location of magnetopause and plasmapause, and thus magnetopause shadowing and magnetopsheric waves like whistler mode chorus, contributes to the dynamics of megaelectronvolt electrons in the outer radiation belt, with energy dependence, in response to CMEs with different preconditions.
Session Chair(s): Wenda CAO, New Jersey Institute of Technology
ST28-A002
Supporting Space Weather Research with GST High-resolution Data at BBSO
Wenda CAO#+
New Jersey Institute of Technology
The 1.6-meter clear aperture, off-axis Goode Solar Telescope (GST), is the first facility-class solar telescope built in the U.S. in a generation. As one of the highest-resolution solar telescopes in the world, GST with its state-of-the-art instruments, routinely collects diffraction-limited spatial resolution photometric, spectroscopic and polarimetric data at Big Bear Solar Observatory (BBSO). Since its regular operation began in 2010, GST has been providing the community with open access to observations of the photosphere and chromosphere with unprecedented resolution, significantly advancing our understanding of the origin of solar activity and space weather, and the fundamental nature of the solar atmosphere. Current GST users are distributed over 62 universities, institutes, and observatories in 21 countries. GST has actively supported campaign observations with NASA space, rocket, and balloon missions (PSP, IRIS, Hinode, SO, NuStar, CLASP-2, BITSE, and SUNRISE-III), and other large ground-based facilities (ALMA, DKIST, GREGOR, NVST). BBSO now provides a permanent home to the SOLIS (Synoptic Optical Long-term Investigation of the Sun) facility built by the National Solar Observatory. This presentation gives an overview of the scientific and instrumental achievements accomplished with GST in the past few years.
ST28-A007
| Invited
The Relationship Between UV Bursts and Ellerman Bombs
Hui TIAN1#+, Yajie CHEN2
1Peking University, 2Max Planck Institute for Solar System Research
Ellerman bombs (EBs) are small-scale intense brightenings in Hα wing images, which are generally believed to be signatures of magnetic reconnection around the temperature minimum region of the solar atmosphere. In 2014, observations from the Interface Region Imaging Spectrograph (IRIS) reveal another type of small-scale reconnection event called ultraviolet (UV) bursts, in the lower solar atmosphere. Coordinated observations between IRIS and ground-based telescopes such as GST have shown a clear coincidence between the occurrence of some UV bursts and EBs. However, at the beginning it was unclear how the EBs are physically connected to UV bursts. In this talk, I will briefly review how high-resolution observations and state-of-the-art MHD simulations in the past ten years have been continuously improving our understanding of the relationship between these two phenomena.
ST28-A034
Evidence for the Universal Fast Magnetic Reconnection Mediated with Plasmoids
Zehao TANG#+
Chinese Academy of Sciences
Magnetic reconnection is a fundamental plasma process that converts magnetic energy into plasma thermal energy, bulk kinetic energy, and non-thermal energetic particles. It plays a critical role in triggering various plasma phenomena from small-scale laboratory experiments to large-scale astrophysical activities in the Universe. Magnetic reconnection in fully ionized plasmas has been intensively studied in the past few decades. Nevertheless, how neutral particles affect the magnetic reconnection process in a relatively much cooler partially ionized plasma environment is still less understood. The cool solar chromosphere offers a natural laboratory to study the magnetic reconnection process in partially ionized plasmas. However, convincing observational evidence for chromospheric magnetic reconnection has not been observed so far. Here, we report the direct observations of three chromospheric reconnection events in association with solar jets and Ellerman Bombs, which show clear magnetic reconnection characteristic signals such as cusp structures, current sheets, and plasmoids. These observations provide long-sought key evidence for the occurrence of fast magnetic reconnection. Combined with radiative magnetohydrodynamic simulation results, we propose that turbulent reconnection mediated with plasmoids is a universal reconnection mechanism regardless of partially or fully ionized plasma environments.
ST28-A038
Spectroscopic Analysis on a Spicule-like Jet Accompanying Transition Region Network Jets
Eun-Kyung LIM#+
Korea Astronomy and Space Science Institute
A rapid blueshifted excursion (RBE) or rapid redshifted excursion (RRE) appears as a ‘sudden widening of the line profile’ on the blue or red side of the line, following the definition given by Langangen. RBEs are often regarded as on-disk counterparts of Type II spicules based on their rapid upward Doppler speed (~40km/s) without following downward motion. On the other hand, there are some reports on the transition from RBEs to RREs indicating material falling back after ejections. We observe tiny spicular features that show a spectral shift from RBE to RRE in an enhanced network field of a quiet Sun region, using the fast imaging solar spectrograph built at the Goode Solar Telescope of Big Bear Solar Observatory. Two strong chromospheric lines, H$\alpha$ and Ca II 854.2 nm, are used for spectroscopy. The multi-layer spectral inversion technique is applied to both lines to obtain spectral parameters, including line-of-sight velocities and temperatures in time. Two events of our interest reveal spectral transitions from RBEs to RREs, with corresponding IRIS counterparts showing the parabolic up and down motion. We also detected intensity enhancements in AIA 193 and 304 channels at the early phase of RBEs, indicating possible heating during ejections. The temperature of the spicular structure shows a monotonic decrease during the RBE phase, suggesting continuous cooling after the energy deposit. We could not find any heating signatures after the RBE phase that is normally expected from type II spicules, and both RBE events we analyze show typical properties of small-scale jets.
ST28-A037
New Features Finding on Light Bridge Jets: Dark Hα Knots and Transparent Regions
Heesu YANG#+
Korea Astronomy and Space Science Institute
We report on dark Hα knots and the transparent region visible at the top of light bridge jets. The dark knots exhibit a distinctive structure with a flat alignment perpendicular to the jet thread with a thickness of 0.25 arcsecond, and a transparent region is located beneath them in \halpha~images. Their speeds are likely redshifted compared to the main body of the jets. Through a coordinated observation of the Goode Solar Telescope (GST) at Big Bear Solar Observatory (BBSO) and Interface Region Imaging Spectrograph (IRIS), we found that the dark knots and the transparent region in the Hα line are associated with Si IV emission of the light wall, oscillating EUV brightenings at the tip of the light bridge jets. The Si IV brightenings are blue-shifted and have large non -thermal speed. We will discuss the implications of these findings during the presentation.
ST28-A001
Meso-scale Photospheric Dynamical Processes During Chromospheric Fan-shaped Surges on Light Bridge
Yuzong ZHANG#+
Chinese Academy of Sciences
An intermittently and aperiodically occurring fan-shaped surge along light bridge has recently attained much attention for its enigmatic driving mechanism. With the aid of the high spatial and temporal resolution data from BBSO/GST, we attempt to explore the photospheric dynamic signals and magnetic features related to the fan-shaped surge process. On 25 June 2015, a series of fan-shaped surges intermittently with long smooth upper edges occurred and extended along an LB in the active region NOAA 12371. We measured the dynamic parameters of chromospheric surges with the Visible Imaging Spectrometer tuned at five spectral wavelengths around the Hα line, identified the photospheric dynamic behaviours with the TiO filter of Broadband Filter Imager, and acquired the distributions of the photospheric vector magnetic field by the inversion of Stokes polarisation parameters obtained from the Near InfraRed Imaging Spectro-polarimeter. In the photospheric granular LB, besides three kinds of proper motions of single grains, sometimes several adjacent grains were tightly packed to form a granular group (GG) moving together along the axis of the LB. We identified ten typical GGs with a mean area and lifetime of 0.34 arcsec2 and 439 s. They are strong enough to truncate the central dark lane and even occupy the entire cross-section of the LB, as well as their front is modulated to the arch-shaped morphology. Ahead of each surge, always one or more GGs appear. Additionally, the filamentary segment of LB is gradually invading the sunspot’s umbral core. The footpoint location of the surges is located at the flank of the LB with a stronger vertical current. This study unlocked a new fine dynamic structure GG occurring in the photosphere of LB, most likely the photospheric signals related to the intermittent eruptions of the fan-shaped surge with a long smooth upper edge.
Session Chair(s): Simon WING, The Johns Hopkins University
ST21-A006
| Invited
Multiscale Kelvin - Helmholtz Instability: Plasma Mixing and Energy Dissipation at the Earth’s Magnetopause
Adriana SETTINO1#+, Rumi NAKAMURA1, Yuri KHOTYAINTSEV2, Daniel GRAHAM2, Kevin BLASL1, Denise PERRONE3, Takuma NAKAMURA1
1Austrian Academy of Sciences, 2Swedish Institute of Space Physics, 3Agenzia Spaziale Italiana
The Kelvin-Helmholtz instability (KHI) is a shear-driven phenomenon frequently observed at the Earth's low-latitude magnetopause when the velocity shear is super Alfvénic. KHI represents a way for plasmas to give rise to a turbulent scenario and to convert the energy due to the large-scale motion of the shear flow into heat. Indeed, the evolution of the KHI is characterized by the nonlinear coupling of different modes, which tends to generate smaller and smaller vortices along the shear layer. Both kinetic simulations and in situ measurements, focusing on the kinetic effects during the nonlinear phase of the instability, have shown the generation of strong current sheets between well-developed vortices, and temperature anisotropy and agyrotropy at both ion and electron scales, in accordance with the multi-scale nature of the phenomenon. Moreover, KHI is thought to play a crucial role in the transport of solar wind plasma into the magnetosphere and to efficiently contribute to the formation of the low latitude boundary layer. Although the instability threshold is equally satisfied during both northward and southward interplanetary magnetic field (IMF) conditions, in-situ measurements show that KHI privileges the northward orientation. We investigate this different behavior by analyzing the kinetic features at both boundaries and inside the KH structures. Thus, we statistically investigate several KHI crossings observed by the Magnetospheric Multiscale mission for different IMF orientations. We observe that specific signatures connected to both local processes and global dynamics arise and affect the KHI evolution.
ST21-A009
Role of the Kelvin-Helmholtz Instability on the Plasma Transport, Heating and Acceleration
Katariina NYKYRI1#, Kyoung-Joo HWANG2+, Xuanye MA3
1NASA Goddard Space Flight Center, 2Southwest Research Institute, 3Embry-Riddle Aeronautical University
As space plasmas are highly collision less and involve several temporal and spatial scales, understanding the physical mechanisms responsible for energy and mass transport between these scales is a major challenge. In this talk we discuss the role of the velocity shear -driven Kelvin- Helmholtz (KH) Instability (KHI) on the plasma transport, heating and acceleration in the Earth’s magnetosphere. While KHI was traditionally considered as an ideal instability (and hence unable to directly transfer mass), observations and simulations during last 21 years have shown that secondary processes (such as magnetic reconnection, kinetic plasma wave modes, and turbulence) can develop inside KH vortices. These secondary processes can lead to rapid heating of the plasma and transport over magnetic boundaries. Furthermore, recent observations and simulations have shown that KHI can affect the transport, dynamics and escape of the high-energy particles. Magnetic reconnection can create large-scale diamagnetic cavities in the high-latitude magnetosphere where particles can be accelerated to 100s of keV in the reconnection quasi-potential. The acceleration mechanism creates strongly perpendicular pitch angle distributions for ions and electrons, likely contributing to the source for the ion temperature anisotropy in the high-latitude magnetosphere. The interaction of the high-latitude KHI and high-latitude reconnection may help explain the recent MMS spacecraft observations of 100s of keV trapped electrons detected within KHI vortices. Future multi-spacecraft missions are needed to study whether these particles are locally accelerated within KHI or whether they originate from diamagnetic cavities but are just captured by the KHI.
ST21-A002
| Invited
Magnetic Reconnection in the Kelvin-Helmholtz Instability at Earth
Frederick WILDER#+
The University of Texas at Arlington
The Kelvin-Helmholtz instability (KHI) manifests as surface waves along earth’s magnetospheric flanks. It is thought to be a major contributor to coupling mass, energy and momentum from the solar wind to the magnetosphere. One mechanism whereby this exchange can occur is through magnetic reconnection. In this talk, we will discuss magnetic reconnection that occurs on compressed current sheets during the KHI in the equatorial plane. We have compiled a list of 13 KHI events with prolonged observations by the NASA Magnetospheric Multiscale (MMS) mission. We investigate each current sheet for signatures of reconnection, and define an event ratio (ER). ER is the fraction of compressed current sheets during each KHI event that exhibit signatures of magnetic reconnection. We then investigate which parameters drive the ER for each event. This includes average solar wind conditions over the event, as well as the location of the satellite observations along the flanks. We find a strong correlation between the strength of northward interplanetary magnetic field (IMF) and ER, as well as higher prevalence of magnetic reconnection closer to earth.
ST21-A012
Waves Around a Crater-shaped Flux Rope in Nonlinear Kelvin-Helmholtz Vortex
Kyunghwan DOKGO1#+, Kyoung-Joo HWANG1, James BURCH1, Peter YOON2
1Southwest Research Institute, 2University of Maryland
The Earth's magnetopause is the boundary layer where the solar wind and the planetary magnetic field interact. Two important mechanisms that allow the exchange of energy, momentum, and particles across this layer are Kelvin-Helmholtz Instability (KHI) and magnetic reconnection. When KHI develops nonlinearly, it can trigger reconnection and generate flux ropes, and the evolution of these structures can enhance the transport of energy and mass from the solar wind to the Earth's magnetosphere. The MMS spacecraft observed a crater-shaped flux rope generated locally by Kelvin-Helmholtz vortex-induced reconnection on the dawnside tailward magnetopause. Two interlinked flux tubes were undergoing interaction, forming the magnetic depression of the flux rope. We investigate the properties and effects of high-frequency waves inside the crater-shaped flux rope. These waves are relevant for the acceleration and heating of charged particles through wave-particle interactions. The crater, the region of low magnetic field, is about 100 km wide, inside the flux rope that is about 650 km wide. We find two types of electrostatic waves inside the crater, depending on their frequencies and directions of propagation. The parallel waves are aligned with the magnetic field and have frequencies below the electron cyclotron frequency. The perpendicular waves are perpendicular to the magnetic field and have frequencies around the electron cyclotron frequency. We perform a linear analysis of the plasma instability that can produce the parallel waves, using a numerical solver. We find that the parallel waves can be excited by an electron beam with a speed of 5,000 km/s. These waves can effectively scatter and heat electrons with energies less than 100 eV. However, the origin of the perpendicular waves is still unknown and needs further investigation. We also present various waves that coexist in the flux rope.
ST21-A004
Spiral CT Scan: A State-of-art Technique for Analyzing Magnetic Reconnection in Space
Huishan FU#+, Zhe WANG, Jinbin CAO
Beihang University
For the first time, we reveal the distribution of plasma density, electron temperature, thermal pressure, and total pressure around a reconnection X-line, by using the spiral CT scan technique, which is a novel technique analogous to that in the hospital. This X-line was detected by the MMS spacecraft at the Earth’s magnetopause, and has been widely believed to host a non-guide-field reconnection in previous studies. With the help of such an advanced technique, we find that: (1) the plasma density is low on the magnetosphere side but high on the magnetosheath side; (2) the electron temperature is high on the magnetosphere side but low on the magnetosheath side; (3) the thermal pressure is high near the current sheet but low away from the current sheet; (4) the total pressure in the inflow region is higher than near the current sheet. Among these findings, the first three agree with classical theories, hence validate our novel scan technique; the last one implicates that anti-parallel magnetic field lines were being pushed together and the reconnection process was ongoing.
Session Chair(s): Xiao-Jia ZHANG, The University of Texas at Dallas, Anton ARTEMYEV, University of California, Los Angeles
ST07-A002
Test Models of Chorus Frequency Chirping
Xin TAO1#+, Fulvio ZONCA2, Liu CHEN3
1University of Science and Technology of China, 2Italian National Agency for New Technologies, Energy and Sustainable Economic Development, 3Zhejiang University
Chorus wave frequency chirping remains a challenging fundamental problem in space plasma physics. Various models, such as the sequential triggering model and the "Trap-Release-Amplify" (TaRA) model, have been proposed to understand why chirping occurs and how to estimate the chirping rate. In this work, we will present a simple numerical test to differentiate between the TaRA model and the sequential triggering model. Physical implications of our results will also be discussed.
ST07-A012
Velocity Space Signature of Resonant Energy Transfer Between Whistler Waves and Electrons in the Earth's Magnetosheath
Wence JIANG1#+, Daniel VERSCHAREN2, Hui LI1, Chi WANG1, Seongyeop JEONG3, Christopher OWEN2, Kristopher G. KLEIN4
1Chinese Academy of Sciences, 2University College London, 3Samsung Electronics Co. Ltd, 4The University of Arizona
Wave–particle interactions play a crucial role in transferring energy between electromagnetic fields and charged particles in space and astrophysical plasmas. Despite the prevalence of different electromagnetic waves in space, there is still a lack of understanding of fundamental aspects of wave–particle interactions, particularly in terms of energy flow and velocity-space characteristics. In this study, we combine a novel quasilinear model with observations from the Magnetospheric Multiscale mission to reveal the signatures of resonant interactions between electrons and whistler waves in magnetic holes, which are coherent structures often found in the Earth’s magnetosheath. We investigate the energy transfer rates and velocity-space characteristics associated with Landau and cyclotron resonances between electrons and slightly oblique propagating whistler waves. In the case of our observed magnetic hole, the loss of electron kinetic energy primarily contributes to the growth of whistler waves through the n = −1 cyclotron resonance, where n is the order of the resonance expansion in linear VlasovMaxwell theory. The excitation of whistler waves leads to a reduction of the temperature anisotropy and parallel heating of the electrons. Our study offers a new and self-consistent understanding of resonant energy transfer in turbulent plasmas.
ST07-A018
Parametric Study of Electron Interactions with Quasi-coherent Chorus and Their Convergence to a Diffusive Behavior
Miroslav HANZELKA1#, Yuri SHPRITS1, Dedong WANG2+, Bernhard HAAS1, Julia HIMMELSBACH1, Ondrej SANTOLIK3,4
1GFZ German Research Centre for Geosciences, 2GFZ Helmholtz Centre for Geosciences, 3Czech Academy of Sciences, 4Charles University
The quasilinear theory can quite successfully model the evolution of magnetospheric electron populations due to resonant interactions with plasma waves. Most numerical models implement a diffusive Fokker-Planck equation with bounce-averaged diffusion coefficients based on empirical models of averaged wave intensity. However, the quasilinear approach cannot capture nonlinear interactions driven by strong and coherent waves, for example by an element of the chorus emission, which cause rapid non-diffusive transport in pitch angle and energy on short time scales. We run the test-particle simulation with a realistic model of chorus elements to study the transition from coherent interactions to stochastic behavior. We prepare a set of rising-tone, lower band chorus elements with frequency bandwidth (related to the subpacket structure), wave normal angle distribution, chirp, and amplitudes based on spacecraft observations, complemented by a realistic spatial structure based on nonlinear growth theories. The backward-in-time particle tracing is used to retrieve the phase space density (PSD) evolution for each element. The density mappings are combined to obtain the perturbed PSD after interaction with a train of variable chorus elements. We then perform a parametric study of the convergence of discrete changes on short scales to stochastic, diffusive changes on longer time scales. Results from the test-particle simulations are compared with the Fokker-Planck description implemented in the VERB-2D (Versatile Electron Radiation Belt) code.
ST07-A022
Mms Observations of Upstream 3-seconds Waves In Earth’s Foreshock Region
Gangkai POH1,2#+, Guan LE1, Xochitl CANO-BLANCO3, Norberto ROMANELLI1, Weijie SUN4
1NASA Goddard Space Flight Center, 2Catholic University of America, 3National Autonomous University of Mexico, 4Space Sciences Laboratory, University of California, Berkeley
Ultra-low frequency (ULF) waves have been observed and studied extensively in the Earth’s ion foreshock region, with their basic wave properties determined. However, many questions regarding their plasma characteristics and generation mechanisms remain unanswered. One example of such ULF waves are the 3-seconds wave first observed in the ISEE magnetometer data and more recently by MMS. This class of ULF waves are always right-handed with periods near 3 seconds, near circularly polarized in the spacecraft frame, and typically occur in regions of high plasma β and are often associated with suprathermal ion populations. In this study, we presented magnetic field and plasma measurements of case study and statistical analysis of 3-seconds waves as observed by MMS upstream of the Earth’s ion foreshock region. We surveyed 3 months of MMS magnetic field and plasma data and identified ~35 intervals when MMS observed waves with period of ~3 seconds. Using FFT and minimum variance analysis, we confirmed that these waves have frequency of ~0.3 Hz (or 3.3s), and are near circularly right-handed polarized in the s/c frame, consistent with earlier studies. We have also utilized multi-spacecraft techniques to definitively determine the propagation direction of these waves in the plasma rest frame. We also analyzed the MMS FPI Burst mode data, when available, during observations of these 3-second waves to determine the ion distribution functions, which is then input into a dispersion solver to determine the instability that generated these 3-second waves. Interestingly, there is also a small subset (~5) of events where these 3-s waves were observed preceding lower frequency 30-s fast magnetosonic waves. Implications of these waves being observed near the edge of the foreshock will also be discussed.
ST07-A023
Energization of the Ions by EMIC Waves Using MMS Observation
Abid Ali ABID#+
University of Science and Technology of China
Electromagnetic ion cyclotron (EMIC) waves have been playing a significant role in inner magnetosphere and their proton band has been detected using the Magnetospheric-Multiscale (MMS) satellite observations in the inner magnetosphere. It has been examined that the intensity of EMIC waves gradually increases by decreasing the L shell. Thermal anisotropy of hot protons initiates the waves. The low-energy cold protons (ions) can be activated by the EMIC waves when the EMIC wave intensity is high. As a result, these formerly invisible protons are now visible. The EMIC waves whose frequency ranges from 0.001 Hz to 5 Hz in the inner magnetosphere and received considerable attention for energy transport across the magnetosphere. Since these waves act as mechanism for the loss of energetic electrons from the Van Allen radiation belt to the atmosphere, therefore, it is necessary to understand how and where they can be produced, as well as the direction of waves along the magnetic field lines. It is demonstrated that throughout the energy range of 1 eV to 100 eV, the number density and temperature anisotropy of the protons likewise rise as the intensity of the EMIC waves increases. A velocity distribution function has been also analyzed in the magnetosphere of Earth by using high-resolution MMS measurement.
Session Chair(s): Chi-Yen LIN, National Central University
ST19-A008
| Invited
2D and 3D Structures of Ionospheric Disturbances Related Typhoon and Tsunami
Katsumi HATTORI1#+, Rui SONG1, Jann-Yenq (Tiger) LIU2
1Chiba University, 2National Central University
Using the high-resolution GNSS observation, we studied the characteristics of 2-D and 3-D concentric traveling ionospheric disturbances (CTIDs) in the mid-latitude ionosphere before Typhoon Faxai landed in Bosō peninsula in Chiba, Japan, on 8 September 2019. The 2-D snapshots of TIDs with amplitudes of 0.05–0.10 TECU at 08:30–11:00 UT (17:30–20:00 LT) were extracted by the band-pass filter, which was ∼9–12 hours before the landfall. They exhibited a periodic feature of ∼24 min, a horizontal wavelength of ∼180 km, and a horizontal velocity of ∼190 m/s. Then, the 3-D structures were visualized for the first time and we found that the wavelike oscillations of Ne and oblique UW-DE alignments of dNe were recognized in the F2 layer. The 3-D geometry concerning dNe is identified as an inverted conic-like shape. Moreover, using the time-height plot method, the descending phase of dNe with increasing time was detected in 220–550 km, which indicated the presence of the upward AGWs continually propagating in the F2 layer. The limitation of the current study is that it cannot precisely reproduce the disturbed structures in the lower ionosphere below 200 km, probably owing to the deficiency of the prior condition and strict constraints in the vertical direction. Therefore, ionospheric parameters from multiple observation techniques, such as the middle and upper atmosphere radars and low-earth orbit satellites, would be introduced to improve the diagnosis precision. We also investigate 2D/3D structures of Ionospheric disturbances related to the 2011 Tohoku earthquake.
ST19-A009
| Invited
Gradients of the Total Electron Content in Asia Region
Libo LIU#+
Chinese Academy of Sciences
The ionosphere has fantastic and complicated spatial structures with various temporal/spatial scales. It is an important issue to monitor/investigate such complicated ionospheric structures and to understand their evolution. We conduct a study to explore the spatial structure of the ionosphere over Asia in terms of the total electron content (TEC) data. The TEC data are retrieved from the Beidou/Compass Geostationary Earth Orbit (GEO) satellite signals recorded by a network of Global Navigation Satellite System (GNSS) receivers built by our group (70+ receivers) and those in Asia. We will show the climatology features of the latitudinal gradients and case of the strong zonal gradients. Some typical cases are reported to reveal the interesting features of the spatial structures in TEC. In those cases, the zonal structures in TEC have shorter scales over wave-number 6 in longitude, much shorter than the global large scale longitudinal variations of scales within the wave-number 4. Our work indicates that the ionospheric phenomena should be understand with the extent of their spatial presence, although their physical drivers are still a puzzle question. Further, it calls for improving the spatial resolution to reliably reproduce the spatial structure of the ionosphere over such regions. It is validated that, when these structures we considered are present, both the current products of global ionospheric maps (GIM) of TEC and the empirical ionospheric model (IRI) fail to reproduce such gradients. It provides stronger challenge under geomagnetic active conditions.
ST19-A004
Observations of Secondary Gravity Wave in the Thermosphere Using Double Layer Airglow Network
Qinzeng LI1+, Jiyao XU1#, Hanli LIU2, Xiao LIU3, Wei YUAN1
1Chinese Academy of Sciences, 2National Center for Atmospheric Research, 3Henan Normal University
Gravity waves (GWs) strongly affect atmospheric dynamics and photochemistry and the coupling between the troposphere, stratosphere, mesosphere, and thermosphere. In addition, GWs generated by strong disturbances in the troposphere (e.g. thunderstorms and typhoons) can affect the atmosphere of Earth from the troposphere to the thermosphere. However, the fundamental process of GW propagation from the troposphere to the thermosphere is poorly understood because it is challenging to constrain this process using observations. Moreover, GWs tend to dissipate rapidly in the thermosphere because the molecular diffusion increases exponentially with height. In this study, a double-layer airglow network was used to capture concentric GWs (CGWs) over China that were excited by Typhoon Chaba (2016). We used ERA5 reanalysis data and Multi-functional Transport Satellite-1R observations to quantitatively describe the propagation processes of typhoon-generated CGWs from the troposphere, through the stratosphere and mesosphere, to the thermosphere. We found that the CGWs in the mesopause region were generated directly by the typhoon in the troposphere. However, the backward-ray-tracing analysis suggested that CGWs in the thermosphere originated from the secondary waves generated by the dissipation of the CGW and/or nonlinear processes in the mesopause region.
ST19-A002
D-region Ionospheric Resonance Induced by Pekeris Wave Associated with the 2022 Tonga Volcanic Eruption
Hiroyo OHYA1#+, Fuminori TSUCHIYA2, Tamio TAKAMURA1, Hiroyuki SHINAGAWA3, Yukihiro TAKAHASHI4, Alfred CHEN5
1Chiba University, 2Tohoku University, 3National Institute of Information and Communications Technology, 4Hokkaido University, 5National Cheng Kung University
The Hunga Tonga-Hunga Ha‘apai (HTHH) volcano explosively erupted on January 15, 2022, causing large pressure variations and triggering traveling ionospheric disturbances. Lamb and Pekeris waves were generated by the HTHH eruption. Both observed waves matched with theoretical characteristics, although the response of the D-region ionosphere has not been clear. In this study, we investigate the response by analyzing VLF/LF transmitter signals and atmospheric electric field. Three transmitters from JJI and JJY, Japan and BPC, China and one receiver in Tainan, Taiwan were used. Atmospheric electric field and pressure were observed in Chiba (CHB), Japan. The VLF/LF amplitudes for all paths and ground-based magnetic field at Kakioka showed variations with a period of 100-1000 s at both arrival time of Lamb and Pekeris waves. The phase velocities of Lamb and Pekeris waves were estimated to be ~307 m/s and ~235 m/s, respectively, which were in good agreement with previous studies (Watanabe et al., 2022). Amplitude of variation in the VLF/LF waves due to the Pekeris wave was larger than that due to Lamb wave. However, atmospheric pressure largely varied due to Lamb wave, although it slightly changed at arrival time of the Pekeris wave. Atmospheric electric field at CHB also showed similar variations with VLF/LF waves. In neutral wind simulations, similar variations in horizontal velocity for both waves were seen at 90 km altitudes, which would be caused by resonance between the stratopause and the lower thermosphere. The reason that the atmospheric electric field had the similar changes as the D-region altitude despite ground-based observations is probably because the change in the D-region altitude was reflected in the atmospheric electric field at the Earth’s surface via global electric circuit. In the presentation, we discuss the detailed mechanism of these phenomena.
ST19-A003
Analyzing Ionospheric Variations During the 21 August 2017 Total Solar Eclipse Using Global Ionospheric Specification
Chi-Yen LIN1#+, Jann-Yenq (Tiger) LIU1, Charles LIN2, Min-Yang CHOU3
1National Central University, 2National Cheng Kung University, 3NASA Goddard Space Flight Center
The Global Ionospheric Specification (GIS) utilizes the Gauss–Markov Kalman filter to assimilate the slant total electron content (TEC) observed from ground-based GPS receivers and space-based radio occultation instruments. This process reconstructs the three-dimensional (3D) ionospheric electron density structure and enables monitoring of space weather conditions. In this study, GIS with a high temporal resolution of five minutes is implemented to reconstruct the 3D electron density structure during the total solar eclipse on 21 August 2017 and to analyze the variations induced by the moon’s shadow. For a more comprehensive understanding of the ionosphere, data from an extended network of 2200 GPS stations across the continental United States are included for assimilation. The results indicate that the ionosphere's peak height (hmF2) experienced an uplift of 30–50 km in altitude at latitudes 25–40°N. Additionally, it was observed that the electron density depletion at higher altitudes (400 km) exhibited a more noticeable time delay compared to lower altitudes (200 km), particularly in low-latitude regions.
ST19-A006
Effects of the 21 June 2020 Solar Eclipse on Electromagnetic Fields on the Surface
Tianya LUO1, Yang-Yi SUN2#+, Pengyu ZHANG2
1Guangxi Transportation Science and Technology Group Co., Ltd., 2China University of Geosciences
This study highlights the effectiveness of the magnetotelluric (MT) method in detecting rapid changes in the ionospheric E region during the annular solar eclipse on 21 June 2020. The MT method successfully identified a significant decrease in the solar quiet current, lasting about 3.3 hours, during the eclipse, as well as observed, for the first time, short-period waves in the electric field with periods ranging from a few to dozens of minutes. These findings indicate non-stationary changes in the E-region current during the eclipse. The conventional understanding is that complex current systems in various geospheres are sources of electric and magnetic waves in the MT method, aligning with the theoretical plane wave assumption. The results of this study suggest that changes in the E-region structures due to reduced solar radiation can be a more straightforward source. These insights not only enhance our understanding of the source of electric and magnetic waves for MT but also demonstrate the potential of using observed electric and magnetic field variations to detect changes in the E region during space weather events.
Session Chair(s): Shiyong HUANG, Wuhan University, Luca SORRISO-VALVO, CNR - ISTP
ST10-A035
| Invited
Energy Transfer Analysis on Tridimensional Plasma Simulations
Christian VASCONEZ1#+, Raffaele MARINO2, ELizabeth MANOBANDA3
1Escuela Politecnica Nacional, 2École Centrale de Lyon, 3Universidad Tecnica de Ambato
We study the energy transfer rate in three-dimensional direct numerical simulations, using a Latice Boltzmann (LB) approach, of quasi collisionless space plasmas. The Yaglom-Politano-Pouquet law is analyzed in a turbulent-evolved scenario using a Hall magnetohydrodynamic model. Statistical properties of this kind of simulations are presented, and the so-called Local Energy Transfer (LET) proxy is also studied.
ST10-A030
Evolution of Turbulence Anisotropy in the Outer Heliosphere: Voyager 2 Observations
Xingyu ZHU#+
The University of Alabama in Huntsville
The solar wind plasma environment in the outer heliosphere is different from the inner heliosphere. An important factor influencing the turbulence evolution in the outer heliosphere is the pickup ions, primarily originated from neutral atoms from the interstellar medium. Pickup ions are not readily assimilated by the background solar wind plasma and thus provide extra free energies which can drive ion-scale instabilities. The unstable growing waves will end up taking part in the turbulent energy transport. However, how these pickup-ion-associated energies involve in turbulent cascade and influence turbulence evolution have yet to be studied. In this work, we study the solar wind turbulence evolution from 1 au to 33 au based on Voyager 2 magnetic field measurements. In all these time intervals, no ion-scale bumps are present in the turbulent spectra. We find that: (1) The perpendicular and trace power spectra (EB_perp and EB_trace) still follow a Kolmogorov-like spectrum until 33 au while the parallel power spectrum transits from -2 to -5/3 at heliocentric distance R~10 au; (2) At periods 10 s <τ< 500 s, quasi-parallel propagation dominates in 1 au<R<7 au, with quasi-perpendicular propagation gradually emerging at R>5au. For R > 7 au, oblique propagation becomes a primary component. (3) At larger periods of τ>100 s, increases with propagation angle in 1 au<R<5 au, and in contrast decreases with propagation angle at R>5 au due to the enhanced power level at propagation angles smaller than. We suggest that such enhancement may derive from the injection of the wave energy from the pickup ion source into the background tubulent cascade , and the injected wave energy is transferred across scales without leaving bumps in EB_perp and EB_trace.
ST10-A006
| Invited
Energy Transfer of Imbalanced Alfvénic Turbulence in the Heliosphere
Liping YANG1#+, Jiansen HE2, Daniel VERSCHAREN3, Hui LI4
1Chinese Academy of Sciences, 2Peking University, 3University College London, 4Los Alamos National Laboratory
Imbalanced Alfvénic turbulence is a universal process playing a crucial role in energy transfer in space, astrophysical, and laboratory plasmas. A fundamental and long-lasting question about the imbalanced Alfvénic turbulence is how and through which mechanism the energy transfers between scales. Here, we show that the energy transfer of imbalanced Alfvénic turbulence is completed by coherent interactions between Alfvén waves and co-propagating anomalous fluctuations. These anomalous fluctuations are generated by nonlinear couplings instead of linear reflection. We also reveal that the energy transfer of the waves and the anomalous fluctuations is carried out mainly through local-scale and large-scale nonlinear interactions, respectively, responsible for their bifurcated power-law spectra. This work unveils the energy transfer physics of imbalanced Alfvénic turbulence, and advances the understanding of imbalanced Alfvénic turbulence observed by Parker Solar Probe in the inner heliosphere.
ST10-A021
| Invited
Influence of Intermittency on the Energy Transfer Rate of Solar Wind Turbulence
Honghong WU1#+, Shiyong HUANG1, Xin WANG2, Li-Ping YANG3, Zhigang YUAN1
1Wuhan University, 2Peking University, 3Chinese Academy of Sciences
The intermittency in the solar wind turbulence influences the anisotropy of the spectral index and the scaling of multiorder structure functions. However, its influence on the energy transfer rate remains unclear. Here we identify the intermittency using the partial variance of increments method for the magnetic field data measured in the fast solar wind by the Ulysses spacecraft. We study the anisotropy by distinguishing the sampling direction using the angle θRB between the local magnetic field and radial direction. We analyze the multiorder structure function analyses and describe the role of intermittency in the framework of log-Poisson cascade model. We find the isotropic scaling with a complete removal of intermittency. We compare explicitly the anisotropy of the energy transfer rate before and after removing the intermittency for the first time. We find a distinct anisotropy with a cascade enhancement in the direction perpendicular to the local magnetic field. The removal of the intermittency greatly weakens the anisotropy by mainly reducing the perpendicular energy transfer rate. Our findings suggest that the intermittency effectively enhances the energy transfer rate, in particular in the perpendicular direction in the solar wind turbulence.
ST10-A028
| Invited
Electron-scale Electric Field Turbulence in the Solar Wind at 1AU: Clues to Understanding Energy Dissipation
Chadi SALEM1#+, John BONNELL1, Christopher CHASTON1, Kristopher G. KLEIN2, Luca FRANCI3, Vadim ROYTERSHTEYN4
1University of California, Berkeley, 2The University of Arizona, 3Queen Mary College, 4University of California, San Diego
Recent works on solar wind turbulence and dissipation suggest that kinetic-scale fluctuations are both heating and isotropizing the solar wind during transit to 1 AU. The nature of these fluctuations and associated heating processes are poorly understood. The Electric Field is key to understanding the nature of the dissipative processes (Landau damping, cyclotron damping, stochastic heating, or energization through coherent structures) that link fields and particles. The dissipation due to the fluctuations depends intimately upon the temporal/spatial variations of those fluctuations in the plasma frame. In order to derive that distribution in the plasma frame, one must also use magnetic field and density fluctuations, in addition to electric field fluctuations, as measured in the spacecraft frame (s/c) to help constrain the type of fluctuation and dissipation mechanisms that are at play. We present an analysis of electromagnetic fluctuations in the solar wind from MHD scales down to electron scales using data from the Artemis spacecraft at 1 AU. We focus on time intervals of pristine solar wind covering a range of plasma properties. We analyze magnetic and electric field, and density fluctuations from the 0.01 Hz up to 1 kHz. We compute electric to magnetic field ratio, magnetic compressibility, magnetic helicity, compressibility and other relevant quantities in order to diagnose the nature of the fluctuations at those scales, extracting information on the dominant modes composing the fluctuations. We also use the linear Vlasov-Maxwell solver PLUME to determine the various relevant modes of the plasma with parameters from the observed solar wind intervals. These results are supplemented by analysis of fully nonlinear kinetic simulations of decaying turbulence at small scales. We discuss the results and highlight the relevant modes as well as the major differences between our results in the solar wind and results in the magnetosheath.
ST10-A024
Observational and Statistical Analysis of the Solar Wind Fluctuation Lorentz Force Acceleration Spectra
Jingyu PENG1#+, Jiansen HE1, Xingyu ZHU2, Die DUAN3
1Peking University, 2The University of Alabama in Huntsville, 3National University of Defense Technology
Wave-particle interaction is considered to be an important mechanism for accelerating the solar wind. According to the second-order theory of wave-particle interaction, ions with fluctuating velocities experience the Lorentz force of a fluctuating magnetic field, which leads to the acceleration of solar wind ions. The Lorentz force acceleration spectra of protons and alpha particles are calculated and statistically analyzed using the magnetic field and ion velocities detected by the Parker Solar Probe. This analysis aims to provide observational evidence for the mechanisms of solar wind ion acceleration and contribute to our understanding of the preferential acceleration process of heavy ions in the solar wind.
ST10-A034
New Regime of Inertial Alfven Wave Turbulence from TRICE-2 Observations
Francesca DI MARE1,2#+, Gregory HOWES3
1The Catholic University of America/ NASA GSFC, 2NASA Goddard Space Flight Center, 3The University of Iowa
Turbulence represents one of the most important processes for coupling energy, mass, and momentum from the Solar wind into the Earth’s magnetosphere. The understanding of turbulence in the Auroral Cusp Ionosphere is an outstanding problem in space plasma physics due to disturbances in trans-ionosphere GPS signal propagation, and in most severe situation, abruption in GPS positioning services. A proper physical description of the turbulent mechanisms and their drivers is pre-requisite to overcome these limitations. We investigate the nature of turbulence detected in the cusp by TRICE-2 sounding rocket mission, using high-resolution measurements of the electric and magnetic field. Our analysis shows the first in-situ experimental evidence of the field fluctuation spectra over the inertial and dissipative wave number in an extremely low plasma beta conditions, as found in the auroral ionosphere and magnetosphere. We further characterize the wave dispersion of the dispersive/inertial Alfvén waves to study the onset of the dispersion regime and its dependence to the plasma parameter. The nature of these Alfvén waves play a key role in the Magnetosphere-Ionosphere coupling, which determines how the Earth is impacted by variable drivers of space weather.
ST10-A002
Effects of Alpha Particle Fraction on Kinetic Plasma Turbulence
Qiyang XIONG+, Shiyong HUANG#
Wuhan University
Solar activities have an extraordinary impact on interplanetary space, enriching the plasma dynamics including turbulent heating of various species. The small fraction of alpha particles is believed to play a significant role in the turbulent dynamics of the solar wind. Here we present fully kinetic particle-in-cell simulations to reveal the influences of the alpha particles in decaying plasma turbulence. Multiple run cases with different controlled variations of proton and alpha density are performed to compare and evaluate the energy conversion processes. It is found that the alpha particles can suppress the energy conversion rate with increasing density. Besides, the alpha particles show more heating preference than the proton species. These two positive charge species have more correlation in the temperature anisotropy as their densities are comparable. Our results provide a comprehensive understanding of the turbulence with different species compositions, especially with abundant heavy particles.
ST10-A009
Statistical Properties of Plateau-like Turbulence Spectra in the Martian Magnetosheath: Maven Observations
Wence JIANG1, Hui LI1#+, Xiaodong LIU1, Daniel VERSCHAREN2, Chi WANG1
1Chinese Academy of Sciences, 2University College London
The Martian magnetosheath provides us with a natural laboratory to study plasma turbulence in the presence of pickup ions and locally generated instabilities. Unlike the typical magnetic-field spectra with a single spectral scaling at magnetohydrodynamics (MHD) scales in Earth's magnetosheath, the magnetic-field spectra in the Martian magnetosheath during 4 years of Mars Atmosphere and Volatile EvolutioN observations frequently present an additional spectral break-point with a shallow slope at MHD scales which we define as a plateau-like spectral feature. The average occurrence rate of plateau-like magnetic-field spectra is 56.6% of our measurement intervals. At moderate pick-up angles, the occurrence rate increases to a maximum of ∼70.0%. Furthermore, we present a positive correlation with the local ion density and anti-correlations with the local βi and the solar Extreme Ultra Violet irradiance. A similar occurrence rate in the quasi-perpendicular and the quasi-parallel magnetosheath (60.1% vs. 52.9%) indicates that the plateau-like spectra are more likely formed locally than in the upstream solar wind. Our results suggest that energy injection from pickup ion driven micro-instabilities, for example, in the form of proton cyclotron waves, has insufficient time to evolve into a fully developed cascade in such a confined space like the Martian magnetosheath.
ST10-A010
Small-scale Magnetic Holes in the Solar Wind Observed by Parker Solar Probe
Lin YU+, Shiyong HUANG#, Zhigang YUAN, Kui JIANG, Yunyun WEI, Jian ZHANG, Sibo XU, Qiyang XIONG, Zhao WANG, Rentong LIN
Wuhan University
The small-scale magnetic hole (SSMH) is a common structure in the universe, characterized by magnetic field depression in a short time period, with the size in the order of proton gyro-radius. SSMHs near the Earth or other planets have been widely observed in recent years. However, SSMHs in the solar wind near the Sun are rarely investigated due to mission constraints. In our study, SSMHs in the pristine solar wind within a wide heliocentric distance range are analyzed based on the Parker Solar Probe (PSP) Mission measurements. A total of 2,416 SSMHs are successfully identified during the first six orbits of PSP. The occurrence rate of SSMHs decreases with the increasing heliocentric distance R. The spatial scale of these SSMHs obeys a bi-log-normal distribution, with the median scale L ∼ 137 km (∼6 ρp, proton gyro-radius). As interplanetary magnetic field Bave increases or R decreases, the upper limit of the spatial scale L corresponding to each bin extends to a larger value. The L corresponding to the maximum occurrence rate also increases when Bave increases and R decreases. Besides, the SSMHs tend to occur more frequently in a weak magnetic field with high thermal pressure in the solar wind. The results on the properties of SSMHs and their occurrence rate will shed light on the characteristics and the origin of SSMHs in the pristine solar wind.
Session Chair(s): Simon WING, The Johns Hopkins University, Jay JOHNSON, Andrews University
ST18-A001
Shock Ionospheric Waves Generated by the 18 November 2023 Starship Flight
Yury YASYUKEVICH1#+, Artem VESNIN2, Elvira ASTAFYEVA3, Valentin LEBEDEV2, Boris MALETCKII3, Artem PADOKHIN4
1Institute of solar-terrestrial physics SB RAS, 2Siberian Branch of the Russian Academy of Sciences, 3Institute of Earth Physics of Paris, 4Lomonosov Moscow State University
We used data from ground-based GNSS receivers and, for the first time, we recorded intensive 2000 km cone shock ionospheric waves after the Starship explosion. The waves had an amplitude of ~0.6–1.2 TECU. To the North, the waves propagated up to 2000 km (from first registration) with ~750 m/s velocity and azimuth 19°. Also, we recorded ~280 m/s waves in the northern direction. To the South, the region of wave propagation was less than 600 km. The cone angle was ~17.5° to the North and ~7° to the South against the flight track. The along-the-flight disturbance reached ~(24.5°N, −82.0°E), i.e. ~10° further than it was indicated in the available at current moment source. Our main findings are: 1) The shock wave had the form of the ionospheric planar wave along whole the flight track. 2) The flight generated up to 10 periods of wave disturbances. 3) Contradicting with previous studies the ionospheric waves propagated mainly to the North.
ST18-A002
| Invited
The Effect of Ionospheric Dynamics on the Evolution of Equatorial Plasma Bubbles
Hyosub KIL#+
Johns Hopkins University Applied Physics Laboratory
The most severe ionospheric turbulence and scintillation occur at night in the equatorial region in association with plasma bubbles. Plasma bubbles are nighttime phenomena, but some persist into the daytime, becoming the major sources of daytime electron density irregularities. However, the conditions for the persistence of bubbles during the daytime have not been clearly understood yet. This study investigates the evolution of bubbles throughout a day by analyzing satellite data from ROCSAT-1 and ICON data and conducting numerical simulations using the SAMI2 model. Bubbles generated just after sunset decay overnight and vanish before sunrise. However, bubbles generated after midnight can persist throughout the day. An essential condition for long lasting bubbles is the upward motion of the ionosphere during the daytime. Observations show a strong correlation between daytime irregularity distribution and vertical plasma motion, supporting this argument. Through numerical simulations, we demonstrate the role of ionospheric dynamics in the evolution of bubbles during the daytime.
ST18-A009
The Role of Soft Particles in Producing Radio Scintillations in the Cusp
Magnus IVARSEN1#+, Andres SPICHER2, Yaqi JIN1
1University of Oslo, 2University of Tromsø
The cusp, where the ionosphere can directly connect with the solar wind, see a constant ionization provided by soft particle precipitation. The F-region ionosphere is here particularly turbulent, as evident by the most prominent high-latitude scintillation hotspot. Soft precipitation has long been thought of as vital to the production of irregularities in the cusp, driving instabilities by producing density gradients. However, seasonal and geomagnetic activity-trends in irregularity occurrence are in fact opposite to those of precipitating particles. Scintillations maximize during winter and during geomagnetically active times, while the precipitating cusp particles maximize during summer and during quiet times. We show here a statistical study of the role of soft precipitation in producing density irregularities in the cusp, and present new reflections into the causal relationship between soft particle precipitation and scintillation occurrence. We show that there is no increase in the cusp-energy flux during disturbed conditions. We discuss other factors that drive irregularities, such as the convection of dense plasma from the dayside through the cusp. These results have implications for how the community should understand the cusp, indicating a much greater role for conductivity dynamics in the irregularity landscape than has thitherto been thought.
ST18-A006
| Invited
Geospace Storm Induced Medium Scale Traveling Ionospheric Disturbances at Midlatitudes
Shunrong ZHANG1#+, Yukitoshi NISHIMURA2, Philip ERICKSON1, Ercha AA1, Hyosub KIL3, Yue DENG4, Evan THOMAS5, Anthea COSTER1, Juha VIERINEN6
1Massachusetts Institute of Technology, 2Boston University, 3Johns Hopkins University Applied Physics Laboratory, 4The University of Texas at Arlington, 5Dartmouth College, 6University of Tromsø
Quiet-time medium-scale traveling ionospheric disturbances (MSTIDs) are often observed at midlatitudes during nighttime, especially, in summer. Their presence has been explained in terms of the Pekins Instability (PI), the associated ionospheric electromagnetics, and the Sporadic E-layer (Es) development. During geospace storms, however, enhanced storm-time electric fields exist in a variety of forms and intensities during different storm stages. They lead to some characteristic variations in electron density, including density gradients, at sub- and midlatitudes such as the midlatitude main trough and storm-enhanced density (SED). This research aims to characterize MSTIDs over continental US (CONUS) that are closely related to unique midlatitude processes and deviate significantly from known storm-time disturbances such as large-scale TIDs (LSTIDs) originating in auroral latitudes. This study provides first storm time observations of the westward-propagating medium-scale traveling ionospheric disturbances (MSTIDs), particularly, associated with SED, SAPS (subauroral polarization stream), and enhanced thermospheric westward winds over the continental US. In the four recent (2017–2019) geomagnetic storm cases examined in this study with minimum SYM-H indices ranging from approximately −200 to -50 nT, MSTIDs were observed in the evening with Bz being stably southward. The NW-SE elongated wavefronts with 2°–3° longitude separation propagated southwestward at 100-300 m/s zonal phase speeds. These TIDs were coincident with SED in its base region or concurrent small electron density patches adjacent to the SED. These disturbances were accompanying intense storm-time electric fields at subauroral latitudes (such as SAPS) as well as enhanced thermospheric westward winds. We propose that these electric fields reach intensities capable of triggering Perkins Instability, We propose that these electric fields reach intensities capable of triggering Perkins Instability with large growth rates, subsequently leading to the manifestation of MSTIDs.
ST18-A007
Unexpected Occurrence of Ionospheric Plasma Patch Structures and Irregularities from Low to High Latitudes
Yang-Yi SUN#+
China University of Geosciences
How ionospheric plasma density irregularities and scintillations develop at latitudes from low to high is a significant topic of interest in space science. Irregularities often appear unpredictably, indicating that the precise mechanisms and contributing factors behind the phenomena are not fully comprehended. This presentation will first focus on the unexpected emergence of nighttime F-region irregularities evolved from patch structures of plasma density enhancements due to the solar eclipse on 21 June 2020 in East Asia at low and middle latitudes. It is noteworthy that the summer solstice is an unfavorable season for the development of irregularities due to the weak pre-reversal enhancement in this longitudinal sector. Ground-based Global navigation satellite system (GNSS) networks and ionosondes recorded those patch structures and irregularities. The prolonged thermospheric convergence effect resulting from the moon obscuration has been identified as contributing to this phenomenon. Next, this presentation will introduce the unforeseen patch structures in the polar region originating from the plasma density enhancement at midlatitude in the nighttime, which contrasts with early knowledge that the patch structures stem from density enhancements in the noontime sector. The ion density and horizontal cross-track ion drifts of the Swarm satellite at ~460 km altitude reveal that the horizontal drifts can drive the plasma enhancement of the Midlatitude summer nighttime anomaly (MSNA) / Weddell sea anomaly (WSA) in the Southern Hemisphere. Both the eastward and westward drifts transport the nighttime plasma from midlatitude to the polar cap. The polar cap patches have been recognized as sources of irregularities at high latitudes.
ST18-A010
The Effect of Planetary Waves on the Day-to-day Variability of Equatorial Plasma Bubbles
Jeffrey KLENZING1#+, Jonathon SMITH2, Guiping LIU2, Sarah MCDONALD3, Preeti BHANEJA2, Alexa HALFORD2
1self, 2NASA Goddard Space Flight Center, 3U.S. Naval Research Laboratory
In the equatorial ionosphere, large persistent depletions in nighttime plasma density (sometimes referred to as “bubbles”) can arise when an unstable ionosphere is perturbed by wave activity. In this scenario, a seed perturbation (such as a gravity wave) on the bottom side of the ionosphere grows rapidly as a Rayleigh-Taylor Instability. Despite over 80 years of observations prediction of these plasma bubbles and the resulting ionospheric scintillation remains an outstanding challenge for the Space Weather community because the terrestrial IT system is driven through multiple energy paths. This talk will discuss the geophysical drivers that can enhance or suppress this instability in the ionosphere —such as geomagnetic storms and planetary waves —which can influence whether a seed wave will grow into a bubble on a given night at a given location. Previously, the day-to-day variability of the ionosphere due to lower atmospheric forcing was quantified by driving the SAMI3 model with the Whole Atmosphere Community Climate Model eXtended (WACCM-X) with the lower boundaries specified by the High Altitude Navy Global Environment Model (NAVGEM-HA) over an extended period of time. The variability levels of Total Electron Content from ground-based GPS measurements were found to be similar to those predicted by the model. Here we extend this analysis to investigate the day-to-day variability of the Rayleigh-Taylor Instability growth rate as calculated from SAMI3/WACCM-X/NAVGEM and its effect on the growth or suppression of plasma bubbles. We will compare with data to quantify the contribution of Planetary Waves and lower atmospheric forcing on bubbles and subsequent scintillation.
ST18-A008
| Invited
Simulation of Day-to-day Variability of Equatorial Plasma Bubbles Under Various Background Conditions
Tatsuhiro YOKOYAMA#+, Tatsuki YUTANI
Kyoto University
Equatorial plasma bubbles (EPBs) are a well-known phenomenon in the equatorial ionospheric F region. As it causes severe scintillation in the amplitude and phase of radio signals, it is important to understand and forecast the occurrence of EPB from a space weather point of view. In order to simulate the instability in the equatorial ionosphere, a 3D High-Resolution Bubble (HIRB) model has been developed. It provides a unique opportunity to characterize intermediate-scale EPB structure, which was not well resolved until very recently. In order to study the day-to-day variability of EPB occurrence, we have conducted a number of simulation runs under various conditions by changing background electric field and electron density. Suitable and unsuitable conditions for the generation of EPBs have been investigated by comparing with the linear growth rate of Rayleigh--Taylor instability.
ST18-A005
The Dependence of Scintillation Indices on the Ionospheric Parameters Over the Arctic Region
Yong WANG1+, P. T. JAYACHANDRAN2, Qing-He ZHANG3,1#, Zanyang XING1, Yu-Zhang MA1, J. RUOHONIEMI4, Simon SHEPHERD5
1Shandong University, 2University of New Brunswick, 3National Space Science Center, Chinese Academy of Sciences, 4Virginia Tech, 5Dartmouth College
In the last decade, the Rate of Change of Total Electron Content Index (ROTI) has been used for monitoring and quantifying ionospheric irregularities. It is considered a substitute for the standard scintillation indices. However, as far as we know, ROTI, as an index, still lacks validation studies to evaluate the general links between ROTI and scintillation indices. This study presents a statistical study on the dependence of ROTI on the standard scintillation indices estimated using Global Positioning System (GPS) receivers of the Canadian High Arctic Ionospheric Network (CHAIN). ROTI shows a linear dependence on the standard phase scintillation index (σφ), whereas no obvious dependence is on the standard amplitude scintillation index (S4). The linear dependence of ROTI on σφ is due to refractive effects that are manifested as TEC variations due to large-scale (greater than Fresnel-scale) structures. This implies that ROTI does not contain information on the scintillation-producing irregularities (Fresnel-scale). Therefore, using ROTI as a proxy for scintillation is not ideal for the polar region.
ST18-A003
Detection of Ionospheric Disturbances Caused by Powerful Underground Explosions by GNSS Radio Sounding
Artem PADOKHIN1#+, Sergei SHALIMOV2
1Lomonosov Moscow State University, 2Russian Academy of Sciences
Using dense networks of GNSS receivers located in California and Nevada, an analysis of the ionospheric responses to two underground explosions (January 21, 2022 M~3.3 mining explosion event 12 km NW of Carlin, Nevada and November 18, 2023 M~1.7 NNSA subsurface chemical test explosion at the Nevada National Security Site) with a magnitude less than the known threshold (M~6.5) for detecting the ionospheric response to earthquakes was carried out. It is shown that when registering these responses, it is necessary to take into account the possible anisotropy of the propagation of atmospheric disturbances at ionospheric altitudes due to both large-scale wind structures and the inclination of the geomagnetic field. Taking these factors into account makes it possible to reduce the magnitude threshold (compared to that established for earthquakes) of impulse lithospheric sources (explosions, volcanic explosions), the response to which can still be detected in the ionospheric total electron content variations.
ST18-A004
Information Theory Analysis of the Drivers of Scintillation
Noah KALIADKO1, Christopher INAE1, Jay JOHNSON1, Simon WING2#+, Yukitoshi NISHIMURA3, Sebastoijan MRAK4, Simon SHEPHERD5
1Andrews University, 2The Johns Hopkins University, 3Boston University, 4Johns Hopkins University Applied Physics Lab, 5Dartmouth College
Understanding the cause of atmospheric signal scintillation is important in improving the quality of satellite communications. A variety of information theory tests were performed between various ionospheric parameters (TEC and ionospheric velocity) and chain scintillation data (S4 and σφ) to analyze linear and non-linear correlations between the data from 2013 to 2021. The coordinates of the data were first converted to AACGM and magnetic local time and were then binned into quarter a degree by one hour bins. Both linear correlation and mutual information tests were used on data spanning a range of magnetic latitude and magnetic local time, with results from multiple days aggregated to form a collective set. Preliminary results indicate that there is correlation between the TEC rate and the σφ phase scintillation index around noon magnetic local time and ~70 degrees magnetic latitude with waiting times from zero up to 1 hour. When analyzing either storm or substorm intervals alone within the same timeframe, the correlation features previously observed were strengthened.
Session Chair(s): Jongchul CHAE, Seoul National University
ST28-A047
| Invited
Magnetic Reconnection as the Driver of the Solar Wind
Nour E. RAOUAFI1#+, Guillermo STENBORG1, Daniel B. SEATON2, Haimin WANG3, Jiasheng WANG4, Craig E. DEFOREST5, Bale STUART6, James DRAKE7, Vadim URITSKY8, Judith T. KARPEN9, Richard C. DEVORE9, Alphonse STERLING10, Tim HORBURY11, Louise HARRA12,13, Sofiane BOUROUAINE14, Justin C. KASPER15, Pankaj KUMAR16, Tai PHAN6, Marco VELLI17
1Johns Hopkins Applied Physics Laboratory, 2Southwest Research Institute, Boulder, CO 80302, USA, 3New Jersey Institute of Technology, 4New Jersey Institute of Technology , 5Southwest Research Institute, Boulder, CO, 6University of California, Berkeley, 7University of Maryland, 8Catholic University of America, 620 Michigan Avenue NE, Washington, DC, 9Heliophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD, 10NASA Marshall Space Flight Center, 11Imperial College London, 12World Radiation Center, 13ETH-Zurich, 14Florida Institute of Technology, 15BWX Technologies, Inc., Washington DC, 16Department of Physics, American University, Washington, DC, 17University of California, Los Angeles
We present EUV solar observations showing evidence for omnipresent jetting activity driven by small-scale magnetic reconnection at the base of the solar corona. We argue that the physical mechanism that heats and drives the solar wind at its source is ubiquitous magnetic reconnection in the form of small-scale jetting activity (a.k.a. jetlets). This jetting activity, like the solar wind and the heating of the coronal plasma, is ubiquitous regardless of the solar cycle phase. Each event arises from small-scale reconnection of opposite-polarity magnetic fields producing a short-lived jet of hot plasma and Alfvén waves into the corona. The discrete nature of these jetlet events leads to intermittent outflows from the corona, which homogenize as they propagate away from the Sun and form the solar wind. This discovery establishes the importance of small-scale magnetic reconnection in solar and stellar atmospheres in understanding ubiquitous phenomena such as coronal heating and solar wind acceleration. Based on previous analyses linking the switchbacks to the magnetic network, we also argue that these new observations might provide the link between the magnetic activity at the base of the corona and the switchback solar wind phenomenon. These new observations need to be put in the bigger picture of the role of magnetic reconnection and the diverse form of jetting in the solar atmosphere.
ST28-A043
| Invited
A Role of Small-scale Emerging Flux in the Solar Eruption
Satoshi INOUE#+, Huu Minh Triet NGUYEN, Ju JING, Haimin WANG
New Jersey Institute of Technology
Solar eruptions are widely believed to be energy release phenomena of free magnetic energy accumulated in the solar corona. However, how that energy is released is still an open problem. Recent high-resolution observations by Goode Solar Telescope (GST) found a small-scall emerging flux at a local area of the solar active region before the solar flares (Wang et al. 2017). However, it is not clear how exactly this emerging flux is involved in the onset of eruption. In this study, to clear this issue, we conduct a data-based magnetohydrodynamic (MHD) simulation. First, we construct a nonlinear force-free field (NLFFF) that is around an hour before the flare, and then a data-driven MHD simulation is performed to make a pre-eruption magnetic field where the NLFFF is used as the initial condition. Eventually, by giving ad hoc small-scale emerging flux in a pre-eruption magnetic field, we investigate the role of the emerging flux in solar eruption. As a result, first, a highly twisted flux rope is formed via tether-cutting reconnection, and it rises slowly. The evolution of the magnetic field at this stage is almost the same whether the emerging flux is given or not. However, during the subsequent fast eruption phase, a noticeable difference is found, which is a significantly faster eruption than when no emerging flux was given. These results suggest that the emerging flux affects the fast acceleration i.e., the torus instability. We will report the detailed physical process and discuss the comparison with observations, e.g., the evolution of the flare ribbons observed by GST.
ST28-A026
High-resolution Observations of Mass Motions Revealing Magnetic Structures of Solar Filaments
Rui LIU#+
University of Science and Technology of China
It is often envisaged that dense filament material lies in the dips of magnetic field lines belonging to either a sheared arcade or a magnetic flux rope. But it is also debated which configuration correctly depicts filaments’ magnetic structure, due to our incapacity to measure the coronal magnetic field. Here we address this issue by employing mass motions in filaments/prominences to diagnose its magnetic structure. For an active-region filament we found that the filament material predominately exhibits two kinds of motions, namely, rotation about the spine and longitudinal oscillation along the spine. The former is evidenced by antisymmetric Doppler shifts about the spine; the latter features a dynamic barb with mass extending away from the H-alpha spine until the transversal edge of the EUV filament channel. The composite motions of filament material suggest a double-decker host structure with mixed signs of helicity, comprising a flux rope atop a sheared-arcade system. For a prominence we investigated the dynamical properties of a bubble structure, which exhibit a disparate morphology in the H-alpha line-center compared to its line-wings’ images, indicating a complex pattern of mass motion along the line-of-sight. Combining Doppler maps with flow maps in the plane of sky derived from a Nonlinear Affine Velocity Estimator, we obtained a comprehensive picture of mass motions revealing a counter-clockwise rotation inside the bubble; with blue-shifted material flowing upward and red-shifted material flowing downward. This sequence of mass motions is interpreted to be either outlining a kinked flux rope configuration of the prominence bubble or providing observational evidence of the internal kink instability in the prominence plasma.
ST28-A012
Emerging Magnetic Flux Rope as an Energy Source for Coronal Heating
Yuandeng SHEN#+
Chinese Academy of Sciences
For decades, scientists have been puzzled by the origin of magnetic flux ropes in the solar atmosphere and how the corona maintains its extremely high temperature. While it is believed that magnetic flux ropes may emerge from the solar interior and transfer energy into the corona, there has been a lack of direct observational evidence to support this theory. Using high spatiotemporal observations from the Goode Solar Telescope and the Solar Dynamics Observatory, we report direct observational evidence of emerging magnetic flux ropes and their subsequent heating of the surrounding plasmas to the coronal temperature. These observations confidently confirm the emerging magnetic flux ropes theory, and they also suggest that emerging magnetic flux ropes are an important energy source for coronal heating.
ST28-A028
| Invited
M-class Solar Flares Observed by the New Vacuum Solar Telescope and Goode Solar Telescope
Xiaoli YAN#+
Chinese Academy of Sciences
Solar flare is one type of the powerful explosions in the solar atmosphere. However, the triggering mechanism and detailed process remain controversial. By using high resolution data observed by NVST of FSO and GST of BBSO, combined with SDO, Hinode and REHSSI observations, we study the initiation and the fine process of two M-class flares. Moreover, we also use static nonlinear force-free field extrapolation as well as data-driven magnetohydrodynamics modeling of the dynamic evolution of the coronal three-dimensional magnetic field to reveal the processes of the two M-class flares.
ST28-A015
| Invited
Moving White Light Flare Kernel in High Temporal Resolution Filimant Eruption Observation
Xu YANG#+, Wenda CAO, Vasyl YURCHYSHYN
New Jersey Institute of Technology
We carry out high-resolution observations of a filament-eruption-triggered X1.0 white-light flare that happened on October 2, 2022. The Visible Imaging Spectrograph (VIS) onboard the Goode Solar Telescope captured the full formation-eruption process of the Hα filament in its center field of view. Following the filament eruption, white-light emissions appear after the Ha ribbon brightens. According to the GST Broad-Band Imager data, the continuum intensity enhancement is ~10% in the photospheric TiO band around 7057 Å. The Helioseismic and Magnetic Imager onboard the Solar Dynameic Observatory reports ~20% of the data count increment for the continuum near Fe I 6173 Å. The Chinese Ha Solar Explorer presents ~40% boost at the continuum near Fe I 6569 Å. The dispersal motion of two white-light kernels is recorded by the high-cadence GST/TiO images, and it is also well accompanied by the motion of the VIS Hα flare ribbon front. One of these white light kernels presents a 55 km/s speed in the plane of the sky, while the other kernel is drifting much slower. We applied nonlinear force-free field extrapolation to confirm and explain the filament eruption and white-light flare kernel motion.
ST28-A029
High-resolution Observations of a C9.3 White-light Flare and Its Impact on the Solar Photosphere
Zhe XU#+
Yunnan Observatories, Chinese Academy of Sciences
We presented the detailed analysis of a C9.3 white-light (WL) flare using the high-resolution observations from the New Vacuum Solar Telescope (NVST). The WL flare occurred on the east solar limb (S04E55) on 2023 September 11 in NOAA AR 13431, and it produced only beam electrons with energies below 50 keV according to the ASO-S/HXI data. Two WL flare cores were clearly observed in the photospheric TiO band, and they were located at the two edges of a penumbra filament, which connected the positive and negative umbras of a delta-type sunspot. The WL flare cores also coincided with the two AIA 304 Å bright points in the bottom of the solar jet that followed the flare. Particularly, the WL flare significantly affected the plasma flow fields and the magnetic fields in the photosphere. We thus hypothesized that the WL flare and the photospheric variations are evidence that magnetic energy is being released in the lower atmosphere of the Sun.
ST28-A016
Energy-releasing Process for the 2013 May 13 X1.7 Limb Flare
Jinhua SHEN1#+, Haisheng JI2
1Xinjiang Astronimical observatory,Chinese Academy of Sciences, 2Chinese Academy of Sciences
In this paper, we reanalyze the X1.7 class limb flare that occurred on 2013 May 13 (SOL2013-05-13T01:56 UT), concentrating on the energy-releasing process using microwave observations mainly made by Nobeyama and X-ray observations made by RHESSI. The analysis was carried out in the context of EUV observations made by the Atmospheric Imaging Assembly on board Solar Dynamics Observatory. First, we complement the initiation process by showing that the initiation occurred together with material falling from a large-scale overlying prominence, a signature of drainage instability. The usual downward and upward motions of the microwave and X-ray sources are observed from their evolution. However, the microwave source’s height shows a recurrent decrease and increase during its overall upward motion; it shows a kind of recurrent contraction and expansion. The time period of the recurrent contraction and expansion corresponds to the period of post-contraction oscillation of EUV loops, and the oscillatory motions are closely correlated with four microwave/hard X-ray peaks that unusually increased nonthermal emission levels by several times. X-ray spectra get hardened during the oscillation. In addition, the rapid contraction of magnetic loops located on the outside of the erupting flux rope occurs 5 minutes after the onset of the flare, showing that the contraction of the peripheral magnetic loops is more likely due to the vortex and sink flows generated by an upward erupting magnetic flux rope rather than a coronal implosion. The results can provide more insight into the physics of dynamic coronal magnetic field and particle acceleration during solar flares.
ST28-A013
High-resolution Observation and Magnetic Modeling of a Solar Minifilament: The Formation, Eruption and Failing Mechanisms
Weilin TENG1#+, Yingna SU1, Rui LIU2, Jialin CHEN3, Yanjie LIU1, Jun DAI1, Wenda CAO4, Jinhua SHEN5, Haisheng JI1
1Chinese Academy of Sciences, 2University of Science and Technology of China, 3Hanjiang Normal University, 4New Jersey Institute of Technology, 5Xinjiang Astronimical observatory,Chinese Academy of Sciences
Minifilaments are widespread small-scale structures in the solar atmosphere. To better understand their formation and eruption mechanisms, we investigate the entire life of a sigmoidal minifilament located below a large quiescent filament observed by BBSO/GST on 2015 August 3. The Hα structure initially appears as a group of arched threads, then transforms into two J-shaped strips, and finally forms a sigmoidal shape. Unlike large scale filaments, the high-resolution observations by GST suggest that the evolution of this sigmoidal minifilament may be driven by flux feeding due to the footpoint rotation of one J-shaped branch. SDO/AIA observations in 171Å show that two coronal jets occur around the southern footpoint of the minifilament before the eruption. The eruption of the minifilament starts from the southern footpoint, then interacts with the overlying filament and fails. The aforementioned observational changes correspond to three episodes of flux cancellations observed by SDO/HMI. Unlike previous studies, however, the cancellation happens between the southern footpoint of the minifilament and an external polarity. We construct two magnetic field models before the eruption using the flux rope insertion method, and find an hyperbolic flux tube (HFT) above the cancellation site. The observation and modeling results suggest that the eruption is triggered by the external magnetic reconnection between the core field of the minifilament and the external fields due to flux cancellations. The minifilament eruption fails partly due to the interaction with the overlying filament, and partly because it hasn't reached the threshold height of the torus instability.
Session Chair(s): Shiyong HUANG, Wuhan University, Luca SORRISO-VALVO, CNR - ISTP
ST10-A023
A Detailed Examination of Energy Conversion from Reconnection Site to Reconnection Front
Yukang SHU+, San LU#, Quanming LU, Rongsheng WANG
University of Science and Technology of China
As a ubiquitous physical process in space plasmas and experimental plasmas, magnetic reconnection is responsible for converting magnetic energy to plasma kinetic energy and thermal energy, while also causing topological changes of magnetic fields. Former research has shown that energy conversion is not limited to the vicinity of the reconnection site. Dipolarization fronts (DF) play a significant role in energy conversion during magnetic reconnection. We examined the energy-converting process from the reconnection site to the reconnection front quantitatively via two-dimensional particle-in-cell (PIC) simulations. At the beginning of reconnection, energy conversion takes place in the diffusion region. As the DF is formed and propagates away from the X-line, it becomes the major energy-converting region. The DF primarily heats the plasma instead of accelerating them. Thus, the Poynting flux is mainly converted to enthalpy flux as the work done by the electric field is balanced by the work of the pressure gradient force. Intriguingly, the DF does not derive its energy source directly from the X-line but from the Poynting flux from the upper and lower boundaries of the DF. This suggests that energy conversion at the DF can persist even after the reconnection process ceases at the X-line. This way, a locally generated magnetic reconnection can affect more extended areas through the propagating reconnection front. Moreover, we studied how the guide field and background plasma density and temperature modify the reconnection rate and energy conversion process in detail. Our findings indicate that the guide field can decrease the growth rate of the electric field both near the reconnection site and at the DF, leading to reduced energy conversion at the DF. Additionally, the background plasma density and temperature can also influence the energy conversion during reconnection.
ST10-A014
Effects of Electron Vortices on the Magnetic Structures in the Terrestrial Magnetosheath
Zhao WANG1+, Shiyong HUANG1#, Zhigang YUAN1, Honghong WU1, Kui JIANG1, Sibo XU1, Yunyun WEI2, Jian ZHANG1, Qiyang XIONG1, Rentong LIN1
1Wuhan University, 2Hubei University of Arts and Science
Electron vortices are usually embedded within different magnetic structures in space plasmas. The effects, including the nonideal electric field, energy dissipation and magnetic field, of electron vortices on these magnetic structures are still unclear. Utilizing the unprecedented high-resolution data from the Magnetospheric Multiscale mission in the terrestrial magnetosheath, we statistically investigate these effects on magnetic structures. Strong correlations are found between the vorticities of electron vortices and nonideal electric fields, energy dissipation, respectively. However, they both have no obvious correlations with the scales of electron vortices. Most of electron vortices have positive contributions to magnetic fields of magnetic structures, such as strengthening the decrease (or increase) of Bt for current sheets and magnetic holes (or flux ropes and magnetic peaks). Our results reveal that the electron vortices play an important role in the evolution of magnetic structures.
ST10-A017
| Invited
Upstream Plasma Waves and Downstream Magnetic Reconnection at a Reforming Quasi-parallel Shock
Quanming LU1#+, Ao GUO1, Zhong-Wei YANG2
1University of Science and Technology of China, 2Chinese Academy of Sciences
With the help of a 2-D PIC simulation model, we investigate the long-time evolution of a quasi-parallel shock. Part of upstream ions are reflected by the shock front, and their interactions with the incident ions excite low-frequency magnetosonic waves in the upstream. Detailed analyses have shown that the dominant wave mode is caused by the resonant ion-ion beam instability, and the wavelength can reach tens of the ion inertial lengths. Although these plasma waves are directed toward the upstream in the upstream plasma frame, they are brought by the incident plasma flow toward the shock front, and their amplitude is enhanced during the approaching. The interaction of the upstream plasma waves with the shock leads to the cyclic reformation of the shock front. When crossing the shock front, these large-amplitude plasma waves are compressed and evolve into current sheets in the transition region of the shock. At last, magnetic reconnection occurs in these current sheets, accompanying with the generation of magnetic islands. Simultaneously, there still exist another kind of plasma waves with the wavelength of several ion inertial lengths in the ramp of the shock, which is excited by the nonresonant ion-ion beam instability. The current sheets in the transition region are distorted and broken into several segments when this kind of plasma waves are transmitted into the downstream, where magnetic reconnection and the generated islands have a much smaller size. No obvious ion flow can be observed around some X lines produced in magnetic reconnection, and it implies that electron-only reconnection may occur.
ST10-A015
Crater Structure Behind Reconnection Front
Shiyong HUANG#+, Qiyang XIONG, Zhigang YUAN, Kui JIANG, Lin YU, Sibo XU, Rentong LIN
Wuhan University
Magnetic reconnection is the physical process that converts the energy from the fields to the plasmas in space, astrophysical and laboratory plasmas. The reconnection front is the structure generated in the reconnection outflow region and participates in the energy release budget. Here, we first report a novel crater structure of magnetic field behind the reconnection front, which is well supported by both the in-situ observations from the Magnetospheric Multiscale mission and kinetic particle-in-cell simulations. The theoretical explanation from the simulations suggests that this crater structure is related to the electron deceleration motion in the outer electron diffusion region. From another perspective, the crater structure is the continuous impact of the high-speed outflow electron jets. Our results can establish a new understanding of the reconnection front and energy conversion during magnetic reconnection.
ST10-A007
| Invited
Interplay of Magnetic Reconnection and Current Sheet Kink Instability in the Earth's Magnetotail
Giulia COZZANI1#+, Markku ALHO2, Ivan ZAITSEV2, Hongyang ZHOU3, Sanni HOILIJOKI2, Lucile TURC2, Maxime GRANDIN2, Konstantinos HORAITES2, Yann PFAU-KEMPF2, Markus BATTARBEE2, Urs GANSE2, Konstantinos PAPADAKIS2, Minna PALMROTH2
1LPC2E, 2University of Helsinki, 3Boston University
We present results of a 3D global magnetospheric hybrid-Vlasov Vlasiator simulation where we investigate the interaction of magnetic reconnection and the kink instability developing in the magnetotail current sheet and propagating obliquely to the reconnection plane. We identify different phases of the instability (notably a growth phase and a saturation phase) and estimate the time evolution of the reconnection rate and of the energy conversion during the same time interval. Our findings indicate that the reconnection rate decreases during the instability growth phase, especially at the locations where the current sheet is perturbed the most by the kink mode. These results highlight the intricate three-dimensional relationship between reconnection and kink instabilities in the magnetotail, suggesting that the kink instability plays a significant role in modulating the reconnection energy conversion efficiency.
ST10-A001
Guide Field Dependence of Turbulent Outflow Associated with Magnetic Topologies and Energy Conversion in Magnetic Reconnection
Qiyang XIONG+, Shiyong HUANG#
Wuhan University
Energy conversion between fields and particles happens in various physical processes of space environment. Magnetic reconnection is one of those processes that can release energy rapidly and massively. The high-speed outflow jets generated by the reconnection can excite turbulence with intermittent structures. In this study, we reveal the effect of guide field on the energy conversion associated with topologies of those structures in the reconnection. Through the approaches of both particle-in-cell (PIC) simulations and Magnetospheric Multiscale (MMS) mission observations, it suggests that large guide field can promote the energy conversion as well as the O-type topology structures generation in the turbulent outflow. Our results provide significant evidences on the relationships between energy conversion of magnetic topologies in the reconnection outflow and the guide field conditions.
ST10-A019
Ion Modulations by Magnetosonic Whistler Waves in the Terrestrial Foreshock
Shan WANG1#+, Jinghuan LI1, Li LI2, Xuzhi ZHOU1, Zhi-Yang LIU3, Jiutong ZHAO4, Qiugang ZONG1
1Peking University, 2China University of Geosciences, 3Institute for Research in Astrophysics and Planetology, 4University of California, Berkeley
In the shock region, rich waves are excited and interact with particles to achieve the energy dissipation. Magnetosonic whistler waves commonly exist in the shock ramp or the upstream edge of ion-scale magnetic structures in the foreshock region. In the terrestrial foreshock, they are typically observed at around 1 Hz in the spacecraft frame. Using MMS observations, we investigate the interactions between such whistlers and ions. The cyclotron resonant velocity is often observed between incoming solar wind and reflecting ions, while sometimes it can approach to the reflecting population. Perpendicular to the background magnetic field, the population(s) far from the cyclotron resonant velocity exhibits 180-degree phase difference from the wave magnetic field (Bw), as can be explained by the anomalous resonance theory. In an event, the spatial inhomogeneity of the background magnetic field makes the near-cyclotron resonant reflecting ions have phases near 270 degrees from Bw, such that ions can gain energies from the electric fields. Along the wave propagation direction, for the events with sufficiently large longitudinal potentials, ions exhibit Landau trapping and form phase space holes. When the potential is not large enough, the longitudinal electric field can reflect part of the incoming ions, acting as an additional shock front, and the electric field may grow into large-amplitude spikes serving as the cross-shock potential field. The results demonstrate how magnetosonic whistler waves can significantly modulate ions compared to a smooth shock-like structure.
Session Chair(s): Charles LIN, National Cheng Kung University
ST26-A001
Properties of Gravity Waves Observed at Low and Mid-latitude by GOLD
Scott ENGLAND#+
Virginia Tech
Atmospheric gravity waves (GWs) are ubiquitous in the Earth’s upper atmosphere. It is believed that they originate from a variety of sources, including the lower atmosphere (as either primary or secondary waves that reach the thermosphere) and from the auroral region. It is believed that they are often closely related to traveling ionospheric disturbances (TIDs). Owing to the relative ease with which the charged particles can be observed, observations of TIDs from the ground are relatively commonplace. Direct observations of thermospheric GWs are comparatively less common, and many come from the upper regions of the thermosphere. Utilizing far UV airglow from space, GOLD is able to observe the neutral middle thermosphere. During dedicated campaigns, GOLD has been able to identify GWs in this region. Owing to its extended field of view, GOLD is also able to track the motion of these GWs over wide ranges of latitude. This allows properties of these waves such as their periods, propagation velocities and amplitudes to be deduced. A survey of the properties of the waves observed will be presented, along with a comparison to concurrent observations of TIDs.
ST26-A002
Penetrating Electric Field With/without Disturbed Electric Fields Simulated by MAGE and Observed by ICON MIGHTI
Qian WU#+, Dong LIN, Wenbin WANG, Liying QIAN, Haonan WU
National Center for Atmospheric Research
Penetrating and disturbed electric fields are the most notable effect of geomagnetic storms on nightside low latitude ionosphere. While the former arrives nearly instantaneously the latter takes more time as it requires the enhanced joule heating to work its way to generate thermospheric wind disturbance, which leads to dynamo variations. We use the MAGE model and ICON observation to investigate both during the July 7-8, 2022 geomagnetic storm event. The model was able to simulate the disturbed electric and penetrating electric fields. The simulations showed enhanced westward wind and the wind dynamo induce upward ion drift confirmed by the ICON zonal wind and ion drift observations. The simulated zonal wind variations are slightly late in arrival at the low latitudes. We also see the penetrating electric field suppresses the disturbed electric field.
ST26-A003
Lunar Tidal Geomagnetic Disturbance and Tidal Wind
Anmin TIAN#+
Shandong University
The geomagnetic field includes both solar diurnal variations (Sq) and lunar diurnal variations (L). Sq variations are attributed to equivalent currents in the ionosphere/ocean driven by thermally-excited solar tides. While L variations are believed to be generated by lunar tides that are gravitationally induced. Whether the ionospheric lunar tidal wind dynamo responsible for the L geomagnetic variations has only been a theoretical hypothesis and still needs to be confirmed through observation. We use TIMED satellite observations of E-region wind velocity data to construct global lunar variations and explain how they contribute to the variation in L geomagnetic variations. The semidiurnal lunar variation of wind velocity is dominant, similar to the geomagnetic field. The current pattern generated by the dynamo, driven by E-region tidal wind, is roughly consistent with the geomagnetic equivalent current. This work confirms and improves our understanding of the causal chain involving lunar gravity, atmospheric tides, E region dynamo, and geomagnetic disturbances.
ST26-A006
FORMOSAT-7/COSMIC-2 Observations of Ionosphere Responses to Forcing from Sun to Earth's Surface
Charles LIN1#+, P. K. RAJESH1, Chi-Yen LIN2, Jia-Ting LIN1, Shih-Ping CHEN1, Cheng-Yung HUANG3
1National Cheng Kung University, 2National Central University, 3Taiwan Space Agency
FORMOSAT7-COSMIC2 Mission is consist of six satellites equipped with GNSS radio occultation payload, in-situ ion density and velocity meters, and RF beacon transmitters. The constellation launched in June 2019 is situated at the low inclination orbit of 24 degree and the radio occultation observations could cover up to 40 degree latitudes. As the operational mission takes ~5000 observations of occultations, plus 100% duty cycle of ion measurements, it provides an unprecedented opportunity to observe the three-dimensional ionosphere hourly. Taking advantage of this special design of the mission, we have discovered several exciting new phenomena during the three year period. In this presentation, we will show how the minor magnetic storm could create severe ionosphere effects; how the Antartica stratospheric sudden warming oscillated and modify the ionosphere plasma; how the mission help identify the super plasma bubble created by the gigantic volcano eruption. All these findings are in the context of coupling the ionosphere to the external forcing sources from Sun to the terrestrial surface.
ST26-A010
Giant Ionospheric Density Hole Near the 2022 Hunga-Tonga Volcanic Eruption: Multi-point Satellite Observations
Jong-Min CHOI1#+, Charles LIN1, P. K. RAJESH1, Jia-Ting LIN1, Marty CHOU1, Young-Sil KWAK2, Shih-Ping CHEN1
1National Cheng Kung University, 2Korea Astronomy and Space Science Institute
A giant ionospheric hole was simultaneously detected in the in situ measurements of FORMOSAT‑7/COSMIC‑2 (F7/C2), Ionospheric Connection Explorer (ICON), Swarm missions, and ground‑based total electron content (TEC) by global navigation satellite system receivers, and F7/C2 Global Ionosphere Specification (GIS) data near Tonga, following the explosive volcano eruption on 15 January 2022. The TEC maps displayed the huge depletions that developed near Tonga after the eruption and gradually evolved. The ICON IVM, F7/C2 IVM and Swarm‑LP detected large depletions not only near Tonga, but also in the EIA trough region. The GIS observations clearly show the ionospheric hole that extends spatially near Tonga, especially strongly south/southward. The simultaneous observations showed that the ionosphere hole near Tonga combined with the EIA trough and finally evolved into a giant ionosphere hole around 07 UT. The ionospheric hole, which occurred at 05 UT near Tonga, extended over a wide area of 160°‑200°E and 25°S‑20°N and lasted for about 11 h. The F7/C2 and ICON satellites overpasses showed large ion density depletions by the hole at orbit altitudes, accompanied by enhancements in ion temperature and field‑aligned and perpendicular ion drift. Such a long‑lasting giant ionospheric hole by a seismic event has not been reported earlier, creating a unique ionospheric environment near Tonga after the eruption. The strong successive impulses by multiple volcano eruptions, together with O/N2 decrease in the summer hemisphere, interhemispheric wind, and water vapor injection into high altitudes apparently yielded such a giant ionospheric hole, 4–6 times larger than that observed during the Tohoku earthquake.
ST26-A008
Facilitating Worldwide Collaborations in the Geospace Dynamic Constellation (GDC) Era
Bea GALLARDO-LACOURT1,2#, Douglas ROWLAND1+, Larry KEPKO3, Katherine GARCIA-SAGE1
1NASA Goddard Space Flight Center, 2The Catholic University of America, 3National Aeronautics and Space Administration
The Geospace Dynamics Constellation (GDC) is NASA’s upcoming heliophysics mission. GDC is a community mission composed of six satellites. It aims to serve as a focal point for coordinated ionosphere-thermosphere-mesosphere (ITM) science on a global scale. This coordination will involve the collaboration of space-based and ground-based assets, simulations, and theory, all operating under the umbrella of the “ITM Great Observatory.” Recognizing the importance of synergy between GDC and the international community’s ground-based assets, the GDC science team has established a community group. This group serves as a nexus, offering ground-based observers valuable insights into the GDC mission and its scientific objectives. Furthermore, facilitates the coordination of ground-based efforts, ensuring that GDC measurements are leveraged to augment broader ITM science goals. GDC is currently seeking international scientific collaborations, particularly in ground-based observations that can leverage GDC measurements to address important science investigations. In essence, the GDC mission represents an exciting opportunity for global collaboration in the field of ITM science.
Session Chair(s): Eun-Kyung LIM, Korea Astronomy and Space Science Institute
ST28-A033
| Invited
Waves as a Heating Candidates in the Solar Atmosphere: An Emerging Perspective in the Framework of High Resolution Observations
Abhishek Kumar SRIVASTAVA#+
Indian Institute of Technology (BHU)
The existence of the hot solar atmosphere and origin of solar wind are two most outstanding problems in solar physics. Although the magnetohydrodynamic (MHD) waves and dissipation of magnetic energy are two viable physical processes for the heating and mass transport in the solar atmosphere, yet direct evidence of such processes often generates debate. The origin of the wave processes in the lower solar atmosphere play a vital role in energy transport and heating various layers of the solar atmosphere. The high-resolution observations from ground (e.g., GST/BBSO; SST etc) and space reveal the generation, propagation, and dissipation of these waves thereby providing stringent information on their heating capabilities. In this presentation, we discuss the novel high-resolution observations of wave processes in the lower solar atmosphere, and transport of the energy in overlying atmosphere. We discuss the current status in this area of research and delineate the future perspectives in the frame-work of ultra-high resolution observations vis-à-vis theoretical modelling.
ST28-A011
Upward Magneto-acoustic Oscillations in the Photosphere and Their Association with Coronal Heating
Haisheng JI#+
Chinese Academy of Sciences
We have an extensive study for the quasi-periodic perturbations on time profiles of the line of sight (LOS) magnetic field in 10x10 sub-areas in a solar plage region. The perturbations are found to be associated with the enhancement of He I 1083 nm absorption in a moss region, which usually signifies the brightening of EUV emission. The He I 1083 nm narrow band imaging was observed at BBSO with GST. FFT analysis of the perturbations gives a kind of spectra similar to that of Doppler velocity: a number of discrete periods around 5 minutes. The amplitudes of the magnetic perturbations are found to be proportional to magnetic field strength over these sub-areas. In addition, magnetic perturbations lag behind a quarter of the cycle in phase with respect to the p-mode Doppler velocity. We show that the relationships can be well explained with an MHD solution for the magneto-acoustic oscillations in high-beta plasma. The observational analysis also shows that, for the two regions with the stronger and weaker magnetic fields, the perturbations are always anti-phased. All findings show that the magnetic perturbations are actually magneto-acoustic oscillations on the solar surface, the photosphere, powered by p-mode oscillations. The findings may provide a new diagnostic tool for exploring the relationship between magneto-acoustic oscillations and the heating of the solar upper atmosphere, as well as their role in helioseismology. Both magnetic field and Doppler velocity are observed by HMI on board the SDO.
ST28-A020
Velocity Fluctuation and Temperature Fluctuation Observed in Umbral Oscillations with the Goode Solar Telescope
Jongchul CHAE#+
Seoul National University
f upward-propagating magnetoacoustic waves are adiabatic, the temperature fluctuates in phase with the pressure that is peaked during the phase of upward motion. We have inferred the temperature fluctuation in umbral oscillations from the Doppler widths of the H alpha line profiles taken with the Fast Imaging Solar Spectrograph of the Goode Solar Telescope at the Big Bear Solar Observatory. Surprisingly, the peak of temperature fluctuation occurred not during the phase of upward motion, but during the phase of downward motion. This behavior strongly suggests that the dynamics of umbral oscillations is not adiabatic, and the effect of radiative heating and cooling plays a significant role. We have adopted Newton’s law of radiative heating and cooling and solved the non-adiabatic energy equation. As a result, we find that the phase delay between velocity fluctuation and temperature fluctuation can be explained by the radiative heating/cooling with the relaxation time of a few tens of seconds.
ST28-A019
The Splitting of Peaks of Umbral Oscillation Power and the Height of the Transition Region
Soosang KANG#+, Jongchul CHAE
Seoul National University
The velocity power spectrum of umbral oscillations usually displays discrete peaks at frequencies above the acoustic cutoff frequency. When the frequency resolution and the SN ratio of the power spectrum is high enough, some peaks appear to be split. We attribute this splitting to the resonance of umbral oscillations trapped in the chromospheric cavity formed by the transition region and the temperature minimum. In order to understand how the height of the transition region affects the splitting, we have constructed a semi-analytical solution of acoustic waves in a non-isothermal, gravitationally-stratified medium. We assume that the waves are excited by the vertical motion observed in the photosphere, and there are no incoming waves from the upper boundary. As a result we have reproduced the peak splitting in the theoretical velocity power spectrum as expected. We find that the frequency difference in the splitting depends on the height of transition region and other atmospheric parameters such as sound speed. Specifically we analyzed a observed power spectrum obtained from a pore, and found that the splitting in this spectrum is best explained if the transition region is located 1500 km above the temperature minimum. Our results suggest that the splitting of peaks of umbral oscillation power may be exploited to infer the atmospheric structure including the height of the transition region.
ST28-A041
Solar Abundance Fractionation Linked to Chromospheric Alfvénic Waves in an Active Region Observed by FISS/GST and EIS/Hinode
Kyoung-Sun LEE1#+, Jongchul CHAE1, Hannah KWAK2, Kyeore LEE1
1Seoul National University, 2Korea Astronomy and Space Science Institute
The elemental composition across different areas of the solar corona differs from that in the photosphere. Typically, elements with a low first ionization potential (FIP) are more abundant compared to their photospheric levels, termed the "FIP effect." A recent prevailing model suggests "Abundance fractionation by the ponderomotive force," linked to magnetohydrodynamic waves, notably Alfvén waves. To explore the connection between abundance fractionation and Alfvén waves in the chromosphere, we analyzed Hα and Ca II data from the Fast Imaging Solar Spectrograph of the 1.6-meter Goode Solar Telescope for Alfvénic wave identification. Si X (low FIP element) and S X (high FIP element) spectra from the EUV Imaging Spectrometer onboard Hinode were examined to ascertain relative abundance in an active region. We found that FIP fractionation (coronal abundance) at the bright loop footpoint near the sunspot penumbra and superpenumbral fibrils, where predominantly propagating Alfvénic waves were detected. Further analysis of these waves (about 300 wave packets) revealed that 50% were downward propagating low-frequency Alfvénic waves. The spatial correlation between abundance fractionation and Alfvénic waves with observed wave characteristics supports the theoretical proposition of FIP fractionation induced by the ponderomotive force generated by Alfvénic waves in the chromosphere.
ST28-A039
Detection of Alfvénic Waves in Quiet-Sun Fibrils Using Spectroscopic Data Obtained by the FISS/GST
Hannah KWAK#+
Korea Astronomy and Space Science Institute
We report the spectroscopic detection of Alfvénic waves within the chromospheric fibrils of a solar quiet region. In contrast to previous studies that focused on transversal displacements in imaging data, our investigation concentrates on line-of-sight (LOS) velocity oscillations in spectral data. The observations were carried out with the Fast Imaging Solar Spectrograph of the 1.6 m Goode Solar Telescope of the Big Bear Solar Observatory. We applied a spectral inversion technique to the Hα and Ca II 8542 Å line profiles to determine various physical parameters, including LOS velocity in the chromosphere of quiet Sun. We detect a total of 385 Alfvénic wave packets in quiet-Sun fibrils. The mean values of the period, velocity amplitude, and propagation speed are 7.5 minutes, 1.33 km/s, and 123 km/s, respectively. We find that the detected waves are classified into three groups based on their periods, namely, 3, 5, and 10 minute bands. In addition, each group of waves exhibits distinct wave properties, indicating a possible connection to their generation mechanism. Indeed, the successful detection of additional 5 and 10 minute waves, characterized by small velocity amplitudes and previously undetected in earlier studies, can be attributed to our implementation of the spectroscopic method, which enables the measurement of waves with such small velocity amplitudes.
ST28-A018
Doppler Shift Oscillations of a Sunspot Detected by CYRA and IRIS
Dong LI#+
Chinese Academy of Sciences
The carbon monoxide (CO) molecular line at around 46655 Å in solar infrared spectra is often used to investigate the dynamic behavior of the cold heart of the solar atmosphere, i.e., sunspot oscillation, especially at the sunspot umbra. We investigated sunspot oscillation at Doppler velocities of the CO 7-6 R67 and 3-2 R14 lines that were measured by the Cryogenic Infrared Spectrograph (CYRA), as well as the line profile of Mg II k line that was detected by the Interface Region Imaging Spectrograph (IRIS). At the sunspot umbra, a periodicity of roughly 5 min is detected at the Doppler velocity range of the CO 7-6 R67 line that formed in the photosphere, while a periodicity of around 3 min is discovered at the Doppler velocities of CO 3-2 R14 and Mg II k lines that formed in the upper photosphere or the temperature minimum region and the chromosphere. Moreover, a time delay of about 2 min is measured between the strong CO 3-2 R14 line and the Mg II k line. The 3 min sunspot oscillation can be spatially resolved in the Doppler shifts, which might be regarded as a propagating slow magnetoacoustic wave. While the 5 min oscillation could be regarded as the solar p-mode wave.
Session Chair(s): Jiajia LIU, University of Science and Technology of China
ST05-A014
| Invited
Review of the Role of Small-scale Solar Activity in the Dynamics of the Coronal and Solar Wind Plasma
Nour E. RAOUAFI#+
Johns Hopkins Applied Physics Laboratory
Recent studies have revealed that small-scale solar activity, including bright points, jets, and spicules, plays a significant role in shaping the plasma dynamics within the solar atmosphere. Furthermore, this activity acts as both the source and driving force behind the solar wind while also accelerating energetic particles. This growing body of evidence is supported by high-quality observations of magnetic fields, extreme ultraviolet (EUV) emissions, and X-rays in the solar atmosphere. In situ measurements obtained near the Sun through instruments like Parker Solar Probe further contribute to our understanding. Modeling efforts have also emphasized the importance of small-scale activity in influencing plasma dynamics and energetics within the solar atmosphere and wind. Gaining a comprehensive understanding of these pervasive small-scale dynamics holds immense potential for providing critical insights into the nature and origin of the solar wind and shedding light on how this wind evolves from its source on the Sun to its journey through the near-Sun heliosphere. I will provide an overview of recent advances in understanding how small-scale solar activity impacts atmospheric dynamics and highlight promising prospects for future research in this area.
ST05-A013
A Roadmap to Decipher the Solar Wind: Transition from Local to Global Scale
Sahel DEY1#, Piyali CHATTERJEE2, Robertus ERDELYI3, Marianna KORSOS4+
1The University of Newcastle, 2Indian Institute of Astrophysics, 3The University of Sheffield, 4The University of Catania
Solar wind is a stream of highly energetic charged particles originating from the solar corona that escapes the solar gravity and fills the entire heliosphere. With a typical speed of 500 km/s, highly structured solar wind plasma dominates the space weather globally. Despite the paramount importance, several physical processes, such as the solar wind acceleration, variations in the solar wind speed, and their source regions, are yet to be understood. It is suggested that the magnetic topology at the photospheric height plays a pivotal role in characterizing the wind. At the smaller spatial scale (1-10 Mm), several features of the solar atmosphere contribute to its' highly dynamic and inhomogeneous nature. Solar spicules and swirls are significant among these building blocks of the global scale. Spicules are thin, elongated jet-like structures comprising cold and dense chromospheric plasma, making incursions often periodically into the much hotter solar transition region and coronal plasma. Along with these ubiquitous jets, spiraling hot plasma columns or swirls are also detected with the advent of recent high-resolution solar observations. We perform a series of three-dimensional radiative magnetohydrodynamics (rMHD) simulations that can self-consistently excite spicules and accompanying swirls in the background of open magnetic fields. With their enormous presence, spicules and swirls contribute significantly to the mass and momentum flux budget of the solar wind. Next, we study a global-scale solar atmospheric model of helmet streamers and pseudo-streamers to decipher the connection of magnetic complexity with the wind behavior. Finally, we present a roadmap to bridge the gap between two models of different scales by feeding the flux parameters of the local to the global one.
ST05-A006
Observations of Mini Coronal Dimmings Caused by Small-scale Eruptions in the Quiet Sun
Rui WANG#+
National Space Science Center of China
Small-scale eruptions could play an important role in coronal heating, generation of solar energetic particles (SEPs), and mass source of the solar wind. However, they are poorly observed, and their characteristics, distributions, and origins remain unclear. Here a mini coronal dimming was captured by the recently launched Solar Orbiter spacecraft. The observations indicate that a minifilament eruption results in the dimming and takes away approximately (1.65 ± 0.54) × 1013 g of mass, which also exhibits similar features as the sources of SEP events. The released magnetic free energy is of the order of ∼1027 erg. Our results suggest that weak constraining force makes the flux rope associated with the minifilament easily enter a torus-unstable domain. We discuss that weak magnetic constraints from low-altitude background fields may be a general condition for the quiet-Sun eruptions, which provide a possible mechanism for the transport of coronal material and energy from the lower to the middle or even higher corona.
ST05-A001
A Magnetic Reconnection Model for the Hot Explosion with Both Ultraviolet and Hα Wing Emissions
Guanchong CHENG#+
Chinese Academy of Sciences
Ellerman bombs (EBs) and ultraviolet bursts (UV bursts) are transient brightening events in the solar atmosphere, with statistical observations suggesting that about 20% of UV bursts are associated with EBs. This study aims to explore whether hot UV emissions and much colder Hα wing emissions can coexist in the same magnetic reconnection process and their positions within the reconnection region. We employed a 2.5D and 3D magnetohydrodynamic (MHD) simulation, enhancing it to include realistic radiative cooling and time-dependent ionization of hydrogen. Using the RH1.5D radiative transfer code, we synthesized the Si IV and Hα spectral line profiles based on MHD results. The simulation revealed a thin current sheet resulting from magnetic reconnection between emerged and background fields, leading to plasmoid instability and nonuniform density distributions. This results in a mix of hot tenuous and cooler dense plasmas at similar altitudes or even within the same plasmoid. The synthesized Si IV emissions show intensities above 106 erg s−1 sr−1 cm−2 Å−1 with line profiles wider than 100 km s−1. The Hα line profile exhibits typical EB characteristics. In conclusion, our simulations suggest that cold EBs and hot UV bursts can originate from the same reconnection process in the low chromosphere. EBs may appear minutes earlier or simultaneously with UV bursts at similar altitudes in a turbulent reconnection region below the middle chromosphere.
Session Chair(s): Nat GOPALSWAMY, NASA Goddard Space Flight Center
ST09-A014
| Invited
Halo Coronal Mass Ejection and Space Weather
Ryun Young KWON#+
Korea Astronomy and Space Science Institute
We highlight the significance of halo coronal mass ejections (CMEs) in space weather. Halo CMEs are characterized by their appearance as a bright halo surrounding the solar disk or occulting disk in coronagraphic images, with the angular width of 360 degrees. Prior to the 1970s, solar flares, which were easily observed and studied with ground-based observations, were believed to be the primary cause of short-term changes in space weather such as geomagnetic storms and solar radiation storms. However, with the discovery of CMEs and regular solar observations conducted by the SOHO mission, it has become widely accepted that CMEs, particularly halo CMEs, play a significant role in these space weather events and related phenomena. These phenomena encompass Morton/EUV waves, Type II radio bursts, solar energetic particle events, and interplanetary CMEs/shocks. In this talk, we begin by addressing the debate regarding whether halo CMEs constitute a distinct class of CMEs with differentiated physical properties from other CMEs or if they are simply a result of viewing perspective angles. Subsequently, we conduct a comprehensive review of case studies and statistical analyses aimed at establishing physical relationships between halo CMEs and space weather-related phenomena. Lastly, we delve into the physical properties of halo CMEs as inferred from the interpretations of various temporally correlated solar and space weather phenomena.
ST09-A017
NASA's Geospace Dynamics Constellation Mission -- A Strategic Hub for Space Weather Science in the Ionosphere/thermosphere
Douglas ROWLAND1#+, Katherine GARCIA-SAGE1, Larry KEPKO2
1NASA Goddard Space Flight Center, 2National Aeronautics and Space Administration
NASA's Geospace Dynamics Constellation (GDC), with an anticipated launch in the early 2030s, will serve as a strategic hub for ionosphere/thermosphere research activities and the science of space weather. On its own, GDC will fully characterize the ionospheric electrodynamics and thermospheric dynamics with multipoint in situ measurements at 350-400 km altitude that can assess longitudinal gradients on scales of 300+ km, and in-track/latitudinal scales of approximately 10 km, on timescales ranging from seconds to tens of minutes. In addition, GDC will fully characterize the thermosphere and ionosphere populations, including new capabilities like measurements of 3-d neutral wind, and detailed assessment of the neutral and ion composition and the plasma density profiles. GDC is particularly well suited as a 'strategic hub' that can be leveraged by other ground- and space-based observation campaigns to study a wide range of problems in I-T dynamics, M-I coupling, and space weather effects in Geospace. GDC will also carry a real-time space weather beacon, and will transmit critical space weather parameters within minutes of their observation. We will present the current status of GDC, its sampling scheme, measurement parameters, and a summary of instrumentation, in addition to showcasing its capability to address numerous problems in the study of space weather.
ST09-A002
| Invited
Extreme Space Weather in the Earth’s Space Environment
Alexandra FOGG1#+, D. HEALY2, Caitriona JACKMAN1, A. PARNELL2, S.C. MCENTEE1, Peter GALLAGHER1, John COXON3, Maria-Theresia WALACH4
1Dublin Institute for Advanced Studies, 2Maynooth University, 3Northumbria University, 4Lancaster University
Although not routinely used in space science, Extreme Value Theory (EVT) is used commonly to estimate return periods and return values of earthquakes or extreme weather. For example, the magnitudes of 1 in 100-year events for many natural phenomena are estimated to assist in societal preparedness. In this paper we present results from the application of bi- and multi-variate EVT to highly complex, multi-dimensional space weather datasets, and unravel the nature of extreme space weather observations. We estimate the return levels of system-scale observations of Earth’s ionosphere, and relate them to driving phenomena including storms, substorms, and sudden commencements.
ST09-A022
A Probabilistic Auroral Location Forecast Derived from Far-ultraviolet Auroral Boundaries and Geomagnetic Activity
Colin FORSYTH1#+, Michaela MOONEY2, Gareth CHISHAM3, Andy SMITH4, Christian LAO1, Larry PAXTON5
1University College London, 2University of Leicester, 3British Antarctic Survey, 4Northumbria University, 5Johns Hopkins University Applied Physics Laboratory
Using auroral boundaries determined from far ultraviolet images of the aurora (Chisham et al., 2022), we have examined auroral occurrence with respect to magnetic latitude, local time and the Kp index. Our results show that auroral occurrence is highly correlated (R2>90%) with observed Kp between values of 0o and 5o. We use linear fits between occurrence and Kp to build a probabilistic Auroral Location Forecast (ALF) which gives the likelihood of the aurora occuring at a given magnetic latitude and local time for any level of Kp. The model includes both correlated relationships between Kp and occurrence at low latitudes and anti-correlated relationships between Kp and occurrence at high latitudes, enabling the model to replicate behaviour expected within the expanding-contracting polar cap paradigm. The model also shows higher variability in the location of the auroral boundary close to the interface between the upward Region 2 currents and downward Region 1 currents. Validation of the model returns high Brier Skill Scores for both the range of Kp used in the model creation (Kp=0 – 5, Brier Skill Score = 0.569) and the range unseen by the model (Kp=6 – 9, Brier Skill Score = 0.532) indicating that the model is skillful in predicting the location of the aurora. The results of our analysis and outputs of ALF may be of interest to space weather professionals and ‘aurora chasers’ in determining the likelihood of aurora being present, particularly when coupled with forecasts of the Kp index.
Session Chair(s): Haisheng JI, Chinese Academy of Sciences
ST28-A021
| Invited
A Model of Umbral Oscillations Inherited from Subphotospheric Fast Body Modes
Juhyung KANG1+, Jongchul CHAE1#, Kyuhyoun CHO1, Soosang KANG1, Eun-Kyung LIM2
1Seoul National University, 2Korea Astronomy and Space Science Institute
Recent observational studies have paid attention to complex horizontal patterns of umbral oscillations that appear to move across the magnetic field, but their physical nature and origin are not fully understood theoretically. Previously, we observationally identified two-armed spiral-shaped wave patterns of umbral oscillations in the chromosphere of a pore using the Fast Imaging Solar Spectrograph on the Goode Solar Telescope. In this work, we propose a model of umbral oscillation inherited from subphotospheric fast body modes. Our model successfully reproduces the observed two-armed spiral-shaped wave patterns shown in the chromosphere with a superposition of several azimuthal and radial wave modes. Especially, our model can reproduce the horizontal patterns at three different frequency bands with a small number of radial modes only, as expected for the fast body modes. According to this model, the horizontal patterns of umbral oscillations are determined by the subsurface condition as well as the atmospheric condition inside the flux tube. Further numerical and observational studies are needed to verify this model of subphotospheric fast body modes.
ST28-A027
Intensity-velocity Correlation and Radiative Relaxation Time in Umbral Oscillations
Kyeore LEE#+, Jongchul CHAE
Seoul National University
Previous observations of umbral oscillations suggested that the Intensity-velocity correlation is hardly positive with the phase difference deviating significantly from zero. This result is against the expectation for adiabatic, upward-propagating waves, and was attributed to the effect of radiative heating and cooling on the acoustic waves. In this work, we further investigate the intensity-velocity correlation and the radiative relaxation time. We specifically examine how these factors depend on the atmospheric level and the location inside an umbra. We analyze a number of sunspots using not only H alpha line, but also Na I 5890 line taken by the Fast Imaging Solar Spectrograph of the Goode Solar Telescope at Big Bear. Additionally, we constructed the intensity and velocity fluctuation at every location. The correlation is calculated simply from the product mean of these fluctuations, and the phase difference is constructed as a function of frequency through the Fourier transform. We determine the radiative relaxation time by fitting this phase difference to a theoretical solution specified by the acoustic cutoff frequency. As a result, we find that the intensity-velocity correlation in the H alpha line is negative in all umbrae in agreement with our previous study. However, in the Na I line, positive correlations were found in two of seven umbrae near their centers, transitioning gradually to negative correlations toward the edges. These results regarding the intensity-velocity correlation directly reflect the radiative relaxation time, which spans 20-50 seconds in the Na I line, longer than the range of 10-20 seconds in the H alpha line. Larger values are observed closer to the umbral center, while smaller values are found near the umbral edge. Our results indicate that the effect of radiative heating and cooling is more important in the higher atmospheric level and near the umbral edge.
ST28-A040
| Invited
Sunspot Magnetic Relaxation Unveiled Through the Evolution Process of a Rapidly Evolving Light Bridge
Donguk SONG#+
Korea Astronomy and Space Science Institute
We present an process of the magnetic relaxation occurring within a sunspot, coinciding with the development of a transient light bridge (LB). By using high-resolution imaging and spectro-polarimetric data captured by the 1.6-meter Goode Solar Telescope installed at the Big Bear Solar Observatory, we observe the evolutionary process of a rapidly evolving LB. The LB is formed as a result of the strong intrusion of filamentary structures with relatively horizontal fields into the vertical umbral field region. An intense current density is detected along a specific region where the magnetic field topology undergoes rapid changes, particularly at the boundary between the LB and the umbra, and bright jets are observed intermittently and repeatedly in the chromosphere along this region through magnetic reconnection. In the latter part of our observation, the horizontal component of the magnetic field within the LB diminishes, leading to the restoration of the typical convection structure, manifested as umbral dots within the sunspot. Our findings provide a comprehensive perspective not only on the evolution of a LB itself, but also on its impacts in the neighboring regions, including the chromospheric activity and the change of magnetic energy of a sunspot.
ST28-A009
Death of Sunspots
Guiping RUAN1#+, Thierry ROUDIER2, Brigitte SCHMIEDER3, Jean-marie MALHERBE3, Yao CHEN1, Wenda CAO4, Chenxi ZHENG1
1Shandong University, 2Institut de Recherche en Astrophysique et Planétologie (IRAP), Université de Toulouse, National Center for Scientific Research, UPS, National Centre for Space Studies, 3Observatoire de Paris/ Université PSL/ National Centre for Scientific Research/ Sorbonne Université/ Université de Paris, 4New Jersey Institute of Technology
Working on the velocity scales at the solar surface it was proved the existence of the family of granules whose interaction with the magnetic field produces the formation of supergranules and network visible at the solar surface. We report the decay of a sunspot observed by the 1.6m Goode Solar Telescope (GST) with the TIO Broadband Filter Imager (BFI) and the Near-InfraRed Imaging Spectropolarimeter (NIRIS). The analysis was aided by the Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamic Observatory (SDO). In the first step we follow during 3 days the decay of the sunspot with HMI data by constructing its evolving area and total magnetic flux. In the second step the high spatial and temporal resolution of the GST instruments allows us to analyze the causes of the decay of the sunspot. For that we follow the emergence of granules in the moat region around the sunspot during 6 hours. The evolution of the Trees of Fragmenting Granules (TFGs) was derived from their relationship with the horizontal surface flows. We find that the area and total magnetic flux show an exponential decrease during the sunspot decay. We identify 22 moving magnetic features (MMFs) in the moats of pores, which is a signature of sunspot decay through diffusion. We note that the MMFs are constrained to follow the borders of TFGs during their journey away from the sunspot. TFGs and their development contribute to diffuse the magnetic field outside the sunspot. The conclusion of our analysis shows the important role of the TFGs in the decaying sunspots. Magnetic field is evacuated by the family of granules.
ST28-A046
The GST Observation of Small Loop Activities Above the Sunspot Light Bridge in NOAA AR 12673
Yeon-Han KIM1#+, Vasyl YURCHYSHYN2, Yan XU2, Su-Chan BONG1, Eun-Kyung LIM1
1Korea Astronomy and Space Science Institute, 2New Jersey Institute of Technology
The active region NOAA AR 12673 is the most flare productive active region in the solar cycle 24. On 2017 September 07, it produced an X1.3 flare, three M-class, and several C-class flares. We successfully observed several C-class flares from 16:50 UT to 22:00 UT using the 1.6m Goode Solar Telescope (GST; formerly NST) at Big Bear Solar Observatory (BBSO). Interestingly, we observed the active region in He I D3 and 10830 lines simultaneously. The data shows several interesting features: (1) small loop activities occurred above the sunspot light bridge (LB); (2) the loop looks bright in 10830 and dark in D3 respectively; (3) all SDO AIA images show the same bright loop as 10830 data (4) in 10830, loop activity starts from 21:05 UT and ends around 21:23 UT then is followed by flare brightening; (5) from the SDO HMI, the light bridge is located along the polarity inversion line of the sunspot. Based on the observed features, we suggest that the small loop activity above the sunspot light bridge is a miniature of large scale filament eruption associated with two-ribbon flares.
ST28-A003
The Length Scales of Photospheric Granules in Quiet Regions and Active Regions
Yanxiao LIU1+, Chaowei JIANG2#, Ding YUAN2, Pingbing ZUO2, Yi WANG2, Wenda CAO3
1Chinese Academy of Sciences, 2Harbin Institute of Technology, 3New Jersey Institute of Technology
By analyzing the NVST and GST data, we found that the sizes of granules display different types of distributions in different scale ranges. Those above 1420 km follow a Gaussian distribution, and demonstrate flat in flatness function, which reveals none intermittence and stable convection. And those with sizes between 265 and 1420 km are fitted by a combination of a power-law function and a Gauss function, and exhibit non-linearity in flatness function, which reveals that they are in the mixture of convection and turbulence. While the mini granules with sizes below 265 km follow a power-law distribution and demonstrate linearity in flatness function, indicating strong intermittence and turbulence. These results suggest a cascade process occurring in the photosphere fluid: large granules break down due to convective instability, which transports energy into small ones; then turbulence is induced and grows, which competes with convection and further causes the small granules to continuously split. Eventually, the motions in even smaller scales enter in a turbulence-dominated regime. However, the granules in active regions behave as stable convection in large size and full turbulence in small size with the lack of the mixture phase. This is different from those in quiet regions and is probably caused by the existence of strong magnetic fields in active regions that form wide granular lanes by magnetic pressure walls. Small granules dropping in such wide granular lanes are tearing and rotating by downflows due to momentum loss and behave fully turbulent. Similarly, the LP features show length spectra of the combination of a Gauss and a Power law function, demonstrate strong dynamics. While the magnetic fields are not fluids, turbulence theorems alone might not be sufficient to explain the dynamics. More investigations with high spatial and temporal resolutions of telescopes like GST are expected.
ST28-A045
Dynamic Evolution of a Fibril
Jie CHEN#+
Chinese Academy of Sciences
The GST observations were performed on NOAA active region 12132 (Sunspot 1). Based on the observations from GST, SDO and IRIS, we investigate the dynamic evolution of a fibril. The rotation and brightening of the fibril are analyzed.
Session Chair(s): Robertus ERDELYI, The University of Sheffield, Yajie CHEN, Max Planck Institute for Solar System Research
ST05-A004
| Invited
Loops in the Solar Transition Region
Zhenghua HUANG#+
Nanjing University
Loops are fundamental building blocks of the solar atmosphere. Their thermodynamics opens a window for understanding how the solar atmosphere is structured and heated. Transition region loops are extremely dynamic and less studied in the past. Thanks to the high resolution data achieved in the past ten years, we now know that the transition region is abundant of loops, which are associated with small-scale dynamic events occurred in this region. In this talk, we will focus on the dynamic evolution of transition region loops and its connection with energetic events. The basic physical parameters of transition region loops will also be presented and their difference than coronal loops will also be discussed. From this presentation, we will understand that transition region loops are a significantly different class of loops in the solar atmosphere than their coronal counterparts and they are important aspect of the complex solar atmosphere.
ST05-A007
Transient Hot Emissions Linked to the Changes in the Braiding Loop Pairs Observed in SDO/AIA
Yi BI#+
Chinese Academy of Sciences
Theoretically, both wave heating and reconnection-type heating could contribute to the heating of coronal loops, especially the warm loops at temperatures around 1-1.5 MK, which are ubiquitous, long-lived, and seemingly stable in the corona. However, there is still no observation showing the exchange of segments and footpoints of the braiding structures within coronal loops, which is expected to be the morphological evolution of the reconnected magnetic bundles, as implied by the picture of nanoflare. We developed a machine learning(ML) model to upscale and enhance the uninterrupted full-disk AIA images to match the simultaneous images taken by High-resolution Coronal Imager(Hi-C) during its brief flight. The AIA images enhanced by the ML model is successful for resolving some substructures braiding with each other in what appear to be a single AIA structure. In particular, the pairs of braiding loop strands were found to evolve to two parallel ones accompanying with impulsive heating in their footpoints, supporting that the interaction between the ML-resolved substructures producing a nanoflare.
ST05-A008
Solar Coronal Jets During Solar Cycle 24
Robertus ERDELYI1#+, Szabolcs SOÓS2,3, Jiajia LIU4, Marianna KORSOS5
1The University of Sheffield, 2Eötvös Loránd University, 3Hungarian Solar Physics Foundation, 4University of Science and Technology of China, 5The University of Catania
Here the spatial and temporal distributions of solar jets throughout Solar Cycle 24 is investigated. We report oscillatory properties of various physical parameters characterising solar jets throughout SC24. Further, systematic hemispherical differences in the oscillations are also identified. Finally, we report whether there is a pronounced solar cyclic variability of the associated power-law index of hot solar jets over Solar Cycle 24. Finally, we conducted a search for compelling signatures of the presence of an active longitude in the coronal jet database. However, we did not find any obvious evidence with a high probability of an active longitude, and therefore, this question remains to be addressed further.
ST05-A012
Study on the Fine Structure of Jets
Jie CHEN#+
Chinese Academy of Sciences
Jets often occur repeatedly from almost the same location. A complex solar jet was observed with two phases to the west of NOAA AR 11513. At high resolution we find that the two phases merge into one another and the accompanying footpoint brightenings occur at different locations. The phases originate from different magnetic patches rather than being one phase originating from the same patch. Photospheric line of sight (LOS) magnetograms show that the bases of the two phases lie in two different patches of magnetic flux that decrease in size during the occurrence of the two phases.
ST05-A010
| Invited
Magnetic Environment of the Plage Chromosphere with DKIST
David KURIDZE#+
National Solar Observatory
The strongly coupled hydrodynamic, magnetic and radiation properties in the solar chromosphere makes it a region of the Sun's atmosphere that is poorly understood. Despite a wealth of recent observations and numerical models, disentangling the processes that drive the chromospheric fine structure and dynamics remains one of the most compelling problems in solar physics. We use data obtained with the high-resolution Visible Broadband Imager (VBI) equipped with an Hβ filter and the Visible Spectro-Polarimeter (ViSP) at the Daniel K. Inouye Solar Telescope to investigate the fine-scale structure of the plage chromosphere. The large aperture and state-of-the-art instrumentation afforded by DKIST, allowed us to observe a large field-of-view at a spatial resolution of approximately 20 km in some instance. Spectropolarimetric inversions of the ViSP data in the Ca II 8542 ̊A and Fe i 6301/6302 ̊A lines are used to construct semiempirical models of the plage atmosphere. Inversion outputs indicate the existence of dense fibrils in the Ca II 8542 ̊A line. The analyses of the ViSP data show that the morphological characteristics, such as orientation, inclination and length of fibrils are defined by the topology of the magnetic field in the photosphere. Chromospheric maps reveal a prominent magnetic canopy in the area where fibrils are directed towards the observer.
ST05-A005
Of Spicules and Coronal Swirling Conduits
Piyali CHATTERJEE1#, Sahel DEY2, Jiajia LIU3, Robertus ERDELYI4+
1Indian Institute of Astrophysics, 2The University of Newcastle, 3University of Science and Technology of China, 4The University of Sheffield
At any given time, it is estimated that millions of spicules are present on the solar surface. We find an intriguing parallel between the simulated spicular forest in a solar-like atmosphere and the numerous jets of polymeric fluid in the laboratory when both are subjected to harmonic forcing. In our radiative (both 2D and 3D) MHD simulations with sub-surface convection, the solar surface oscillations are excited similarly to those harmonic vibrations. A forest of spicules are formed in our simulations with heights ranging between 6 and 20 Mm, bearing substantially closer resemblance to clusters of jets observed in the solar atmosphere. Taken together, the numerical simulations of the Sun and the laboratory fluid dynamics experiments provide insights into the mechanism underlying the ubiquity of jets. Our 3D numerical simulations further indicate an interesting relationship between spicules and what we refer to as "coronal swirling conduits" or CoSCos. In contrast to spicules that fall back to the solar chromosphere, the CoSCos form by drawing energy from the thermal and magnetic energy reservoir of the chromospheric plasma. These CoSCos have the potential to carry the rotational energy pulses further upward at Alfven speeds than the typical length of spicules seen in the Si IV emission lines even when spicules are falling sun-ward.
ST05-A002
Coronal Microjets in Quiet-sun Regions Observed with the Extreme Ultraviolet Imager Onboard Solar Orbiter
Zhenyong HOU1+, Hui TIAN1#, David BERGHMANS2, Hechao CHEN1, Luca TERIACA3, Udo SCHUEHLE3, Yuhang GAO1, Yajie CHEN3, Jiansen HE1, Linghua WANG1, Xianyong BAI4
1Peking University, 2Solar-Terrestrial Centre of Excellence, 3Max Planck Institute for Solar System Research, 4Chinese Academy of Sciences
We report the smallest coronal jets ever observed in the quiet Sun with recent high resolution observations from the High Resolution Telescopes (HRI-EUV and HRI-Lyα) of the Extreme Ultraviolet Imager (EUI) onboard Solar Orbiter. In the HRI-EUV (174 Å) images, these microjets usually appear as nearly collimated structures with brightenings at their footpoints. Their average lifetime, projected speed, width, and maximum length are 4.6 min, 62 km s^(-1), 1.0 Mm, and 7.7 Mm, respectively. Inverted-Y shaped structures and moving blobs can be identified in some events. A subset of these events also reveal signatures in the HRI-Lyα (H I Lyα at 1216 Å) images and the extreme ultraviolet images taken by the Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory. Our differential emission measure analysis suggests a multi-thermal nature and an average density of ~1.4x10^9 cm^(-3) for these microjets. Their thermal and kinetic energies were estimated to be ~3.9x10^24 erg and ~2.9x10^23 erg, respectively, which are of the same order of the released energy predicted by the nanoflare theory. Most events appear to be located at the edges of network lanes and magnetic flux concentrations, suggesting that these coronal microjets are likely generated by magnetic reconnection between small-scale magnetic loops and the adjacent network field.
ST05-A009
Small-scale Jets in Solar Orbiter/EUI Observations and Radiation MHD Models
Yajie CHEN#+
Max Planck Institute for Solar System Research
Extreme-Ultraviolet Imager (EUI) onboard Solar Orbiter provides an unprecedentedly high spatial resolution of ~200 km on the Sun, and it is able to resolve the smallest coronal jets ever observed in the quiet solar corona. Additionally, the cadence of EUI observations can reach 2-3 s, which allows for the capturing of the transient plasma flows and detailed evolution of the jets. These jets are generally believed to result from magnetic reconnection and may be important for mass and energy transfer in the corona. Furthermore, the tiny jets in the coronal holes may provide plasma to sustain the solar wind. In this talk, I will first present recent results of observations of small-scale jets taken by Solar Orbiter/EUI. Then I will show how the radiation MHD models reproduce the properties of the coronal jets and what we can learn about the generation mechanisms of the jets and their potential contribution to the solar wind from the models.
Session Chair(s): Qing-He ZHANG, National Space Science Center, Chinese Academy of Sciences, Manu VARGHESE, National Space Science Centre
ST09-A020
Relative Effects of Solar Wind Dynamic Pressure and IMF Bz on the Missed Early Part of the Main Phase of Geomagnetic Storms
Manu VARGHESE1#+, Balan NANAN2, Qing-He ZHANG3,2, Zanyang XING2
1National Space Science Centre, 2Shandong University, 3National Space Science Center, Chinese Academy of Sciences
We notice that an important early part of the main phase of the geomagnetic storms having positive main phase onset (MPO) is missed in the treatment of the main phase. The important early part between MPO and original 0-level of Dst (and SymH) seems missed on the belief that this part corresponds to the initial phase (IP) caused by eastward magnetopause current due to enhanced solar wind dynamic pressure. At the same time, it accepted in the literature that the main phase (MP) begins from MPO when Dst (and SymH) starts decreasing due to the increase (mainly) in the westward ring current due to IMF Bz southward. In this paper, we investigate the relative effects of the enhanced dynamic pressure and IMF Bz on the early part of MP and found that the early part is due to the dominance of the westward ring current over the eastward magnetopahse current. The missed part causes an inconsistency in the intensity DstMin (and SymHMin) and impulsive strength IpsDst (and IpsSymH) of the storms.
ST09-A016
| Invited
Ionospheric Space Weather from Global Navigation Satellite Systems
Yury YASYUKEVICH1#+, Alexander KISELEV2, Artem VESNIN2, Artem PADOKHIN3, Ilya EDEMSKIY2, Alexander IVANOV3, Alexei BYKOV2
1Institute of solar-terrestrial physics SB RAS, 2Siberian Branch of the Russian Academy of Sciences, 3Lomonosov Moscow State University
Global navigation satellite system (GNSS) provides huge data sets to study the Earth’s ionosphere and different aspects of space weather influence. The talk briefly reviews GNSS-based experimental studies of the ionospheric effects from solar flares, solar terminator, solar eclipses, magnetic storms, etc, mentioning recent events such as the ionospheric effects of the 2023 Turkey earthquake, the 31 December 2023 solar flare, the 18 November 2023 Starship explosion. Such researches are based on total electron content variations. Global electron content (GEC) is a tool to study the ionosphere as a global. Solar cycle 25 revealed its peculiarity in GEC (as well as in solar activity). Our team developed a free-to-use system to treat GNSS data – SIMuRG (https://simurg.space). The system could be useful for studying the ionospheric space weather. Talk partly is devoted to machine learning to study the Earth’s ionosphere. The work is financially supported by the Russian Science Foundation (project No. 23-17-00157).
ST09-A021
Global Simulation of the Solar Wind Validated with Ulysses Measurements
Chin-Chun WU1#+, Kan LIOU2, Brian WOOD1
1U.S. Naval Research Laboratory, 2Johns Hopkins University Applied Physics Laboratory
Accurate reconstruction of the solar wind plays an important role in the study of the heliosphere and space weather prediction. In this study, we perform a global simulation of the long-term solar wind evolution within 7 AU from 1995 to 2008 using G3DMHD, which is a data-driven, time-dependent, global three-dimensional (3-D) magnetohydrodynamic (MHD) numerical simulation model. The G3DMHD model starts at 18 solar radii and is driven by the solar synoptic maps, a refined version of the Wang-Sheeley model, and a set of conservation laws. To validate the model performance, the simulation result is compared with the hourly solar wind plasma and field data acquired by the Ulysses spacecraft in terms of several metrics: the yearly correlation coefficient (cc), mean squared prediction error (MSPE), mean absolute scaled error (MASE), and root mean squared error (RMSE). It is found that the strength of the solar wind magnetic field is normally underestimated during the solar minimum period, and overestimated during the solar maximum period. We will present a detailed comparison and discuss possible causes of the discrepancy.
ST09-A008
| Invited
Thermosphere UFKW Structures and Ionosphere Coupling as Observed by ICON
Jeffrey FORBES1#, Xiaoli ZHANG1+, Christoph ENGLERT2, Roderick HELLIS3, Michael STEVENS2, Brian HARDING4, John HARLANDER5, Kenneth MARR2, Jonathan MAKELA6, Thomas IMMEL4
1University of Colorado Boulder, 2U.S. Naval Research Laboratory, 3The University of Texas at Dallas, 4University of California, Berkeley, 5St. Cloud State University, 6University of Illinois at Urbana-Champaign
Atmospheric Ultra-Fast Kelvin waves (UFKWs) are eastward- and vertically-propagating oscillations with periods less than 1 week that are centered on the equator and confined to low latitudes. They are part of a whole spectrum of waves forced by the spatial-temporal variability of the heat of condensation ("latent heating'') that is released when rising moist air forms rain droplets, mainly in the tropics. At high altitudes UFKW reach large amplitudes due to the decrease in ambient density with height. Their growth is curtailed by the viscosity of the atmosphere near 102 km altitude where they reach maximum amplitudes. Here they interact with ionized particles (the ionosphere) and generate electric fields that ultimately drive ionospheric variability at higher altitudes (> 200 km), thus presenting an element of "space weather'' to navigation and communications systems. In this paper, UFKWs measured in connection with the ICON mission are used to reveal, for the first time, the height and latitudinal structures of temperatures and winds associated with UFKWs in this dissipative regime, and their corresponding effect on the ionosphere. These results can thus serve to assess the internal consistency of models that seek to simulate atmosphere-ionosphere coupling and related space weather effects induced by the wave spectrum excited in the lower atmosphere.
ST09-A009
Dependence of Solar Wind Parameters on the Transpolar Arc Occurrence Revealed by Novel Neural Network (Potential Learning)
Motoharu NOWADA1#+, Ryozo KITAJIMA2, Ryotaro KAMIMURA3, Quanqi SHI1
1Shandong University, 2Tokyo Polytechnic University, 3Tokai University
Transpolar arc (TPA) is a part of theta aurora and bar-shaped emissions growing from the poleward edge of the nightside main auroral oval to the dayside, frequently observed under northward and non-zero dawn-dusk interplanetary magnetic field (IMF) conditions. Based on a novel neural network (Potential Learning: PL), we extract the most influential and significant solar wind parameter(s) on the TPA occurrence and investigate the relationship between TPA occurrence and solar wind conditions. Using large databases of the OMNI solar wind, and auroral imagers obtained from the IMAGE and Polar missions from 1996 to 2005, we identified not only presence/absence of the TPAs but also the duration times of the TPA appearance. In this study, we selected the six parameters to characterize the solar wind conditions as the PL input parameters: the IMF-By and northward Bz components, solar wind velocity, number density, dynamic pressure, and reverse solar wind energy coupling function (anti-epsilon parameter) which is proposed by Kullen et al. (2002). The output parameter of PL is the TPA presence and absence, represented with 1 or 0. Under these input and output conditions, we investigate the most significant solar wind parameter(s) when the output shows “1”. We evaluated the PL performance and confirmed that the TPA occurrence can be predicted with about 70% accuracy from the six input solar wind parameters. The solar wind velocity was extracted as the most significant solar wind parameter for the TPA occurrence. We will interpret physically the most influential solar wind parameter(s) on the TPA occurrence which were extracted by PL, decreasing/increasing the numbers of the input solar wind parameters, and discuss what this result means physically at the point of view on solar wind control of the TPA occurrence.
Session Chair(s): Wenda CAO, New Jersey Institute of Technology
ST28-A010
| Invited
Astronomical Adaptive Optics Advances in IOE, CAS
Changhui RAO#+, Hao XIAN, Xuejun RAO, Hua BAO, Youming GUO, Shengqian WANG, Xinlong FAN, Jinlong HUANG
Chinese Academy of Sciences
There are more than 40 years history of adaptive optics (AO) in Institute of Optics and Electronics (IOE), Chinese Academy of Sciences since 1980. The research concern all the aspects including the theories study, devices manufacture, and system development. The recent advances on astronomical AO are reported in this presentation. The recent AO systems developments for 4-meter night-time optical telescope, 1.8-meter solar telescope CLST and the 1-m New Vacuum Solar Telescope at Fuxian Lake Solar Observatory are presented respectively. The deformable mirror (DM) advancement, such as Deformable Secondary Mirror and high density DM, are also introduced.
ST28-A008
The Wide Filed Adaptive Optics System of the New Vacuum Solar Telescope
Lanqiang ZHANG+, Xuejun RAO, Hua BAO, Youming GUO, Changhui RAO#
Chinese Academy of Sciences
The wide field adaptive optics system for solar observations had been developed and put in routine operation at the 1-meter New Vacuum Solar Telescope (NVST) in Fuxian Lake, Yunnan Observatory. This system adopts our proposed configuration based on the high order ground layer correction loop and the low order high altitude correction loop. Three correction modes, namely the conventional AO, ground layer adaptive optics (GLAO), and multi-conjugate adaptive optics (MCAO) with three layers correction, can be chosen with the sciences requirements. The DM for ground layer correction is inherited from the 151-element AO system, and two new DMs are added and conjugated to 2~5km and 7-10km, respectively. The opto-mechanical design allows for changing the conjugate height of the two DMs independently. Two multi-direction Shack-Hartmann wavefront sensors are employed for sensing the aberration from ground layer and high-altitudes turbulence. The control system is based on Multi-core CPUs platform, which is flexible for testing various control approaches. We summarize the design and report the observational results of different correction modes.
ST28-A044
Design of NVST Second-generation High-resolution Observation System
Zhenyu JIN#+, Hui LIU, Kaifan JI, Xiqun WANG
Chinese Academy of Sciences
NVST is a 1-meter vacuum solar telescope operated by China's Yunnan Observatory and installed on the bank of Fuxian Lake in Yunnan Province, China. Since the observation was put into operation in 2012, the high-resolution observation system has mainly carried out high-resolution conventional observations of the sun. NVST's high-resolution observation system consists of Tio channel (705.8nm) and Ha channel (656.28nm). The NVST team is planning a second-generation high-resolution observation system, adding two channels to the original one, namely the solar photospheric magnetic field measurement channel and the He I channel (1083nm). The high-resolution reconstruction algorithm is also improved to the NASIR algorithm.
ST28-A022
Progress on Mid-infrared Solar Observation at Huairou Solar Observing Station
Xianyong BAI#+
Chinese Academy of Sciences
In the past, ground-based solar observations mainly focused on the visible wavelength. The infrared wavelength, especially the mid-infrared band, is able to measure solar magnetic fields directly with the Zeeman splitting formula and to diagnose the coolest part of solar atmosphere as many molecular lines exists here. However, mid-infrared wavelength is a window that is not explored for solar physics. In this report, we discuss the properties of “cold bubbles” near the pore regions discovered with the CO lines around 4.66 microns by Cryogenic Infrared Spectrograph belonging to Goode Solar Telescope at Big Bear Solar Observatory. Moreover, we present the recent results from the Accurate Infrared Magnetic field Measurements of the Sun (AIMS), which has 1 meter aperture and is equipped with a fourier transform spectrometer (FTS) working at 10-13 microns and an imager working at 8-10 microns. AIMS has the ability to take solar spectrum with a 64x2 detector near Mg I 12.32 micrions with a spectral resolution of 0.004cm-1. Relative to the FTS with a single element detector from the McMath Pierce facility, the scanning time for a solar active region is reduced by two orders of magnitude.
ST28-A023
The Multi-slit Spectrometer of the Wide-field and High-resolution Solar Telescope of China
Zhi XU1#+, Yue ZHONG1, Zhen LI2, Mingde DING2, Cheng FANG2
1Chinese Academy of Sciences, 2Nanjing University
The spectrometer of the Wide-field and High-resolution Solar Telescope (WeHoST) is a multi-slit-scanning spectrograph with the ability to observe solar regions up to 5 arcmin * 5 arcmin. It is equipped with a polarimeter in dual-beam setup with a continuously rotating waveplate as the polarization modulator. The users are able to carry out full Stokes Spectro-polarimetric observations simultaneously in the MgI 517.3nm and Fe I 617.3nm lines to purse well-established spectro-polarimetric studies of the magnetic structures and plasma dynamic of the solar atmosphere. In this prestation, we describe the science requirements and defining features of this spectrometer.
ST28-A004
Frottage Method to Reveal Sub-arcsec Solar Magnetic Field in Ground-based Observation
Shangbin YANG#+
Chinese Academy of Sciences
Evolution of solar photospheric magnetic field in small scale plays an important role to understand the solar activity. However, the measurements of solar magnetic field with ground-based telescope are suffering from the atmosphere seeing (1 arcse) and the uncertainty taken by the weak polarization signal (∼0.1‰). Although speckle imaging technique has been successfully revealing high-resolution diffraction limit images from short-exposure intensity frames in the past, it is still difficult to realize the solar speckle polarimetry because of the noisy single short-exposure polarization image. In this paper, we proposed a new method to use the short exposure reconstructed images at multiple wavelength points to obtain the spatial amplified factor to multiply the short-exposure polarization signal, just like the uneven texture of frottage in art to reveal fine scales. We apply this method to the magnetic field measurements of Huairou Solar Observing Station (HSOS). After applying the speckle imaging technique to 128 frame amplified short-exposure polarization signals, we successfully reveal the sub-arcsec magnetic field structure, which is comparable with space SDO/HMI data at the closet time. This testing is confirming the feasibility of our method and the potential capability to be used in GST,DIKST, EST or future next generation larger aperture of ground solar telescopes.
ST28-A030
The Dynamics of Solar Prominences Revealed by New Vacuum Solar Telescope (NVST)
Jincheng WANG#+, Xiaoli YAN
Chinese Academy of Sciences
Solar prominences, intricate structures on the Sun's limb, have been a subject of fascination due to their thread-like features and dynamic behaviors. Utilizing data from the New Vacuum Solar Telescope (NVST) and other space telescopes, we investigate two types of dynamics in solar prominences: large upflow plumes and transverse swaying motions of vertical threads. On one hand, we observe two large plumes with high-resolution data, which are notably different from previously studied small-scale plumes. These large plumes originate at the top of a prominence bubble with a substantial projected area of 10−20 Mm². Before the occurrence of each large plume, the bubble expands and adopts a quasi-semicircular appearance. Simultaneously, the emission intensity of extreme-ultraviolet bands increases within the bubble. We conclude that these large plumes result from the breakup of the prominence bubble triggered by an enhancement of thermal pressure, separating from the bubble, likely through magnetic reconnection. On the other hand, transverse swaying motions are observed propagating upward, accompanied by upflowing materials inclined at 31 degrees relative to the plane of the sky. These motions display small-amplitude oscillations with corrected velocities of around 5 km/s and periods of 13-17 minutes. They can be interpreted as signatures of transverse magnetohydrodynamic (MHD) kink waves. Prominence seismology is employed to estimate the Alfven speed and magnetic field strength of the vertical threads, revealing values of approximately 21.5 km/s and 1.7 Gauss, respectively. The energy flux carried by these swaying motions is estimated to be about 1.1 × 104 erg/s/cm², which is insufficient for heating the corona. Our results also indicate that the observed vertical threads may not be true vertical magnetic structures but rather inclined magnetic structures. This study enhances our understanding of the dynamics and magnetic properties of solar prominences.
ST28-A014
Simultaneous Observations of a Breakout Current Sheet and a Flare Current Sheet in a Coronal Jet Event
Liheng YANG1#+, Xiaoli YAN2, Zhike XUE2, Zhe XU3, Qingmin ZHANG2, Yijun HOU2, Jincheng WANG2, Huadong CHEN2
1Yunnan observatories, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Yunnan Observatories, Chinese Academy of Sciences
Previous studies have revealed that solar coronal jets triggered by the eruption of mini-filaments (MFs) conform to the famous magnetic-breakout mechanism. In such scenario, a breakout current sheet (BCS) and a flare current sheet (FCS) should be observed during the jets. With high spatial and temporal resolution data from the SDO, the NVST, the RHESSI, the Wind, and the GOES, we present observational evidence of a BCS and a FCS formation during coronal jets driven by a MF eruption occurring in the active region NOAA 11726 on 2013 April 21. Magnetic field extrapolation show that the MF was enclosed by a fan-spine magnetic structure. The MF was activated by flux cancellation under it, and then slowly rose. A BCS formed when the magnetic fields wrapping the MF squeezed to antidirectional external open fields. Simultaneously, one thin bright jet and two bidirectional jet-like structures were observed. As the MF erupted as a blowout jet, a FCS was formed when the two distended legs inside the MF field came together. One end of the FCS connected the post-flare loops. The BCS’s peak temperature was calculated to be 2.5 MK. The FCS’s length, width and peak temperature was calculated to be 4.35-4.93 Mm, 1.31-1.45 Mm, and 2.5 MK, respectively. The magnetic reconnection rate associated with the FCS was estimated to be from 0.266 to 0.333. This event also related to a type III radio burst, indicating its influence on interplanetary space. These observations support the scenario of the breakout model as the trigger mechanism of coronal jets, and flux cancellation was the driver of this event.
Session Chair(s): Tatsuhiro YOKOYAMA, Kyoto University, Kyung Sun PARK, Chungbuk National University
ST27-A001
Introduction to the SOlar-Terrestrial Habitability Explorer (SOTHE)
Jiajia LIU#+, Yuming WANG
University of Science and Technology of China
Among more than 5000 exoplanets discovered up to now, around 60 are believed to be potentially habitable. The Sun-Earth system provides a unique example based on which detailed insights into the properties, formation, evolution, and thus habitability of exoplanets could be gained. However, simultaneously observing the Sun as a star and the Earth as an exoplanet has been rare. In this talk, I will briefly introduce the SOlar Terrestrial Habitability Explorer (SOTHE) to be deployed to the Sun-Earth L1 point. SOTHE will carry 5 payloads to obtain the spectra of the Sun and the Earth at the same time, together with images of the Earth at a number of unique passbands and the local plasma and magnetic field parameters at the L1 point. The core scientific goal of SOTHE is to conduct the first-ever simultaneous spectral observations of the Sun and Earth to explore key characteristics related to the habitability of the Sun-Earth system and provide a unique baseline for habitable exoplanets exploration.
ST27-A013
Introduction of Yokosuka Radio Polarimeter (YoRP) and Its Observation
Kyoko WATANABE1#+, Masumi SHIMOJO2, Kazumasa IWAI3
1National Defense Academy of Japan, 2National Astronomical Observatory of Japan, 3Nagoya University
EUV emission from the Sun, which has a significant impact on space weather conditions, is known to have a good correlation with the solar microwave emissions. In fact, we confirmed that there is a good correlation between solar EUV and microwave emissions, not only for variations of these emissions in solar cycle, but also for variations of these emissions due to solar flares. In our study, we mainly used EUV spectra observed by the TIMED/SEE and SDO/EVE, and microwave data obtained by the Nobeyama Radio Polarimeters (NoRP). For the solar cycle variations, it was found that among the microwave emissions, low-frequency microwave emissions such as 1 and 2 GHz contributed to the reproduction of the EUV emission spectrum. On the other hand, for solar flare emissions, microwave emissions with higher frequencies such as 17 and 35 GHz were found to correlate well with the EUV emission spectra. Microwave data with wide range of frequencies needed to understand space weather conditions in detail. In Japan, microwave emissions have been observed at Toyokawa and Nobeyama for more than 70 years (Shimojo and Iwai, 2023), but the observed frequencies are limited to seven: 1, 2, 3.75, 9.4, 17, 35, and 80 GHz. Not only to observe these microwave emissions continuously, but also to obtain dynamic spectra of microwave emissions including these frequencies, we installed a microwave observation system in our institute at Yokosuka. In this paper, we introduce the Yokosuka Radio Polarimeter (YoRP) and report the latest data acquisition status.
ST27-A004
Modelling the Magnetic Structure of a Large-scale Horse-shoe-like Filament
Kaifeng KANG1, Jun LIN1#+, Yang GUO2, Ilia ROUSSEV3, Rony KEPPENS4
1Chinese Academy of Sciences, 2Nanjing University, 3University of California Berkeley, 4Katholieke Universiteit Leuven
A horse-shoe-like filament appeared on the solar disc for the first time at 02:00 UT on 2015 November 7, and took 8 days to move to the central median on the solar disc. The active region AR 12452 around it was diffuse so that the magnetic field nearby was weak, the average field strength is 106 G. Therefore, the existing approaches to extrapolating the coronal magnetic field and to constructing the filament configuration in the region with strong background field do not work well here. On the basis of the regularized Biot–Savart laws method, we successfully constructed a data-constrained, non-linear force-free field configuration for this filament observed on 2015 November 14. The overall magnetic configuration obtained in this way matches well the morphology suggested by a 304 Å image taken by the Atmospheric Imaging Assembly on board Solar Dynamics Observatory. Magnetic dips in the configuration were coincident in space with the Hα features of the filament, which is lower in altitude than the features seen in 304 Å. This suggests that the cold plasma fills the lower part of the filament, and hot plasma is situated in the higher region. The calculation results of dips also indicate that the barbs of the filament are a natural consequence of the deformation of the magnetic flux rope, and are not anchored to the photosphere.
ST27-A008
Unusually Long Path Length for a Nearly Scatter-free Solar Particle Event Observed by Solar Orbiter at 0.43 Au
Robert WIMMER-SCHWEINGRUBER1#+, Liu YANG2, Raul GOMEZ-HERRERO3, Javier RODRIGUEZ-PACHECO3, George HO4, Glenn MASON5, Alexander WARMUTH6, Luciano RODRIGUEZ7, Daria SHUKHOBODSKAIA7, Francisco ESPINOSA LARA3, Ignacio CERNUDA3
1Kiel University, 2Macau University of Science and Technology, 3University of Alcalá, 4Southwest Research Institute, 5Johns Hopkins University Applied Physics Laboratory, 6Leibniz Institute for Astrophysics Potsdam, 7Royal Observatory of Belgium
Solar energetic particles (SEPs) are bound to the interplanetary magnetic field (IMF) by the Lorentz force. The expansion of the IMF close to the Sun focuses the particle pitch-angle distribution, and scattering counteracts this focusing. Solar Orbiter observed an unusual solar particle event on 9 April 2022 when it was at 0.43 astronomical units (au) from the Sun. The inferred IMF along which the SEPs traveled was about three times longer than the nominal length of the Parker spiral. Nevertheless, the pitch-angle distribution of the particles of this event is highly anisotropic, and the electrons and ions appear to be streaming along the same IMF structures. The angular width of the streaming population is estimated to be approximately 30 degrees. The highly anisotropic ion beam was observed for more than 12 h. This may be due to the low level of fluctuations in the IMF, which in turn is very probably due to this event being inside an interplanetary coronal mass ejection. The slow and small rotation in the IMF suggests a flux-rope structure. Small flux dropouts are associated with very small changes in pitch angle, which may be explained by different flux tubes connecting to different locations in the flare region. The unusually long path length along which the electrons and ions have propagated virtually scatter-free together with the short-term flux dropouts offer excellent opportunities to study the transport of SEPs within interplanetary structures. The 9 April 2022 solar particle event offers an especially rich number of unique observations that can be used to limit SEP transport models.
ST27-A003
A Novel Ion Composition and Three-dimensional Velocity Analyzer for the Topside Ionosphere
Keiichi OGASAWARA1#+, Heechan CHA2, Guy GRUBBS1, Dhirendra KATARIA1
1Southwest Research Institute, 2The University of Texas at San Antonio
A new ion composition and three-dimensional velocity analyzer, 3-Dimensional ion velocity and mass Imager (3DI), measures 3D velocity distribution functions (VDFs) for each major ion species in Earth’s topside ionosphere. The 3DI instrument is composed of a miniaturized electrostatic analyzer (ESA) and a deflector, backed by a static, magnet-based, mass spectrometer to separate molecular species. A micro-pixel read-out anode technique that significantly saves power in the particle detection system, and integrated it into an imaging microchannel plate (MCP). The prototype-sensor performances have been demonstrated for the ESA and deflector, magnet-based mass spectrometer, and anode in the laboratory. The miniaturization efforts are ongoing to fit within 2U size for the opportunities with space-limited platforms. The 3DI observations will be extremely useful in identifying ionosphere composition, mass-dependent ion transport such as upflows, and mass-dependent ion heating. Furthermore, the precise measurement of non-thermal plasma VDFs provides information to improve ionospheric environment modeling and ground-based radar observations. We will also discuss possible future applications.
ST27-A010
Sampling of the Probe for Radio Occultation of Ionospheric Layers (PROFILE) Instrument on the GDC Mission
Guiping LIU1#+, Douglas ROWLAND1, Olga VERKHOGLYADOVA2, Anthony MANNUCCI2, Panagiotis VERGADOS2, Thomas MEEHAN2
1NASA Goddard Space Flight Center, 2NASA Jet Propulsion Laboratory
The Probe for Radio Occultation oF Ionospheric LayErs (PROFILE) is a GNSS radio occultation receiver designed to operate on NASA’s Geospace Dynamics Constellation (GDC) mission. Combined with 5 in-situ sensors, PROFILE will make remote sensing measurements of electron density profiles, providing information on space weather effects in the ionosphere. Six satellites will be launched into a near polar orbit, and during ~2 years of time the satellites will be spread gradually, allowing for the first time to comprehensively observe the global response of the upper atmosphere across multiple temporal and spatial scales. For this study, we estimate the numbers of radio occultations that could be obtained by PROFILE during various phases of the mission. We also evaluate how the remote sensing observations would leverage with the in-situ measurements to maximize the science return from GDC.
ST27-A016
Links of the Terrestrial Temperature, Sea Levels with Solar Activity and Solar Orbital Motion
Valentina ZHARKOVA1#+, Irina VASILIEVA2
1Northumbria University, 2Main Astronomical Observatory
This paper explores the links between terrestrial temperature, sea levels and ice areas in both hemispheres with solar activity in- dices expressed through averaged sunspot numbers together with the summary curve of eigen vectors of the solar background magnetic field (SBMF) and with changes of Sun-Earth distances caused by solar inertial motion resulting from the gravitation of large planets in the solar system. Using the wavelet analysis of the GLB and HadCRUTS datasets two periods: 21.4 and 36 years in GLB, set and the period of about 19.6 years in the HadCRUTS are discovered. The wavelet analysis of ice and snow areas in the Southern hemisphere does not show any links to solar activity periods while in the Northern hemisphere the ice area reveals a period of 10.7 years equal to a usual solar activity cycle. The total solar irradiance (TSI) in March-August is found to grow with every year following closely the temperature curve, because the Sun moves closer to the Earth orbit owing to gravitation of large planets because of the solar inertial motion (SIM). We demonstrate that the additional TSI contribution caused by SIM is likely to secure the additional energy input to the Earth atmosphere and exchange between the ocean and atmosphere.
ST27-A011
The Impact of Solar – Terrestrial Plasma and Magnetic Field on the Detection of Gravitational Waves
Su WEI#+
Sun Yat-sen University
Space-borne gravitational waves (GWs) detection raises a new question for heliophysics: how does the solar-terrestrial space environment affect space-borne GWs detection? The space-borne GWs detection will use laser interferometry to measure the changes of displacement between two free test masses caused by GWs. the laser ranging accuracy is required to the order of picometer (10-12 m/Hz0.5), and the acceleration measurement accuracy, which describes whether the mass is "free", is required to the order of 10-15 m/s2/Hz0.5. We find that the space environment can cause two major effects on GWs detection: one is optical path difference (OPD) noise caused by laser propagation in space plasma; the other are magnetic moment force and Lorentz force generated by the interaction of space magnetic field with the test mass. Here, we evaluate the OPD noise due to space plasma, and the acceleration noise due to space magnetic field by magnetohydrodynamic (MHD) simulations and in-situ observations. We find that the acceleration noise due to the space magnetic field is of the order of 10% for the requirement of TianQin GWs detection at 1 mHz. In the range of 1 mHz to 1 Hz, the OPD noise due to laser propagation is maximum at 10 mHz, reaching 30% of the TianQin’s requirement. Moreover, we have found that time-delay interferometry can suppress the OPD noise, which can suppress the OPD noise to <10% of the TianQin’s requirement.
ST01-A004
Modeling Energetic Proton Transport in a Corotating Interaction Region: An Energetic Particle Event Observed by STEREO-A from 21 to 24 August 2016
Xinyi TAO1#+, Fang SHEN1, Wenwen WEI2, Yuji ZHU1, Xi LUO3, Xueshang FENG1
1Chinese Academy of Sciences, China, 2China Meteorological Adminstration, China, 3Shandong Institute of Advanced Technology, China
An energetic particle event related to a CIR structure was observed by STEREO-A from 21 to 24 August 2016. Based on an analysis of measurement data, we suggest instead of being accelerated by distant shocks, a local mechanism acting in the compression region could explain the flux enhancements of 1.8-10.0 MeV nucleon-1 protons. To verify our hypothesis, we developed a coupled model composed of a data-driven analytical background model providing solar wind configuration and a particle transport model represented by the focused transport equation (FTE) to simulate particle transport in the CIR region of interest in order to obtain the evolution of proton fluxes and derive the spectra. We find that the simulation is well correlated with the observation. The mechanism of particle scattering back and forth between the trap-like structure of interplanetary magnetic field in the compression region is the major factor responsible for the flux enhancements in this energetic particle event, and perpendicular diffusion plays an important role in the temporal evolution of proton fluxes.
ST01-A007
Formation of the Double-power-law Energy Spectra of Solar Energetic Particles
Feiyu YU1#+, Xiangliang KONG1, Fan GUO2, Yao CHEN1, Joseph GIACALONE3
1Shandong University, China, 2Los Alamos National Laboratory, United States, 3The University of Arizona, United States
The event-integrated energy spectra in large solar energetic particle (SEP) events often show a double-power-law feature. Although understanding particle acceleration and transport processes is a major theme in SEP studies, the underlying mechanism remains unclear. In this work, we first numerically simulate the acceleration of SEPs near the Sun at a CME-driven shock propagating through a streamer magnetic field. The energy spectra, both integrated over the whole simulation domain and in the streamer-nonstreamer transition region, can be described by a double power law. We suggest that the double-power-law distribution may emerge as a result of the superposition of energetic particles from various source regions with different acceleration rates. We also numerically simulate the propagation of SEPs from two source regions in the interplanetary space and calculated time-integrated spectra to mimic spacecraft observations. We assumed that two adjacent SEP populations are released near the Sun, and each is a power-law with exponential rollover. The time-integrated and instantaneous spectra resulting from the two-source case can display a double-power-law feature at different radial distances and longitudes. This further verifies that our proposed scenario of "mixing of SEPs from different source regions" can serve as a promising formation mechanism of the double-power-law feature in SEP energy spectra. Future multi-spacecraft observations of a single event at different locations in the interplanetary space may test the proposed formation mechanism of the double power-law spectrum.
ST01-A015
Field Line Curvature (FLC) Scattering in the Dayside Off-equatorial Minima Regions
Bin CAI+, Hui ZHU#
Shandong University, China
Magnetic field line curvature (FLC) scattering is an effective mechanism for collisionless particle scattering. Within terrestrial magnetosphere, the FLC scattering plays an essential role in shaping outer boundary of protons radiation belt, the rapid decay of ring current, and the formation of proton isotropic boundary (IB). However, previous studies have yet to adequately investigate the influence of FLC scattering on charged particles in the Earth's dayside magnetosphere, particularly in the off-equatorial magnetic minima regions. This study employs a magnetic field model to investigate the impacts of FLC scattering on ring current protons in the dayside magnetosphere, with a specific focus on the off-equatorial minimum regions in the northern and southern hemispheres. We analyze the spatial distribution of single and dual magnetic minima regions, adiabatic parameter, and pitch angle diffusion coefficients due to FLC scattering as functions of Kp. The effects of FLC scattering are significant not only on the dusk and dawn sides but also in the off-equatorial minima regions on the noon side, where it displays distinct hemispheric asymmetry. Additionally, we demonstrate the role of the dipole tilt angle in the hemispheric asymmetry of FLC scattering effects. During low to moderate geomagnetic activity periods, the incline of the magnetic axis with respect to the Sun influences the overall displacement of the dayside magnetosphere, consequently leading to hemispheric differences in FLC scattering effects. Our study holds significance for comprehending the FLC scattering effects in the off-equatorial region of Earth's dayside magnetosphere and for constructing more accurate dynamic model of particles.
ST01-A018
Betatron Acceleration or Cooling of Halo and Strahl Electrons in the Solar Wind
Weiduo MENG1#+, Jianpeng GUO1, Haibo LIN1, Huishan FU2, Meng ZHOU3, Dan ZHAO1, Yan CHEN1, Linxia HE1, Xianghan WANG1, Zelin WANG1
1Beijing Normal University, China, 2Beihang University, China, 3Nanchang University, China
Adiabatic acceleration or cooling of solar wind electrons has been studied extensively in observational, theoretical and simulation studies. However, direct identification of adiabatic betatron mechanism in the solar wind by in situ observations is still a rare opportunity. Here we show a distinct event of local betatron acceleration within a contracting small-scale flux rope (FR) in the solar wind, due to a local compression, and a localized betatron cooling event in the solar wind produced by a blob in a heliospheric plasma sheet due to its own expansion. We observed only the suprathermal halo electrons were effectively accelerated via the betatron acceleration mechanism, but then observed simultaneous energy dissipation of halo and strahl components attributed to the betatron cooling mechanism. In both events, the lower-energy suprathermal electrons (halo or strahl) were efficiently energizated/dissipated by the betatron mechanism, while the higher-energy suprathermal electrons dominated by the suprathermal halo component were hardly energizated/dissipated. Further studies of small-scale FRs and blobs in the vicinity of the heliospheric current sheet for the period 1995-2020 indicates that in situ signatures of the betatron acceleration/cooling process are essentially elusive.
ST01-A019
3D Velocity Distribution of Solar Wind Strahl and Halo Electrons Around ICMEs Observed by Multiple Spacecraft
Pinxu LIU#+, Linghua WANG, Qianyi MA, Wenyan LI
Peking University, China
The three-dimensional (3D) velocity distribution of solar wind strahl and halo electrons carry crucial information on the source, acceleration and transport of these suprathermal electrons. Here we present a study of the 3D velocity distribution of strahl and halo electrons around and within the interplanetary coronal mass injections (ICMEs) observed by PSP, SolO and/or Wind. First, we develop a new fitting method called anisotropic pan-spectrum fitting based on the pan-spectrum formula [Liu et al., 2020], to self-consistently obtain the features of suprathermal particle energy spectrum as a function of pitch angle. Secondly, we investigate the spatial and temporal evolution of the strahl and halo electron velocity distribution near and during ICMEs. Finally, we discuss the possible physical picture of the observed strahl and halo electrons.
ST01-A021
A Series of Solar Energetic Electron Events in May 2023
Tianhao LI#+, Linghua WANG, Wenyan LI
Peking University, China
Solar energetic electron (SEE) events are one of the most common solar particle acceleration phenomena observed in the interplanetary space. Here we present a study of nine SEE events observed by Wind/3DP at 1 AU within 68 hours around May 1st, 2023. All the nine events are accompanied by a SXR or HXR flare measured by SolO/STIX. Among these flares, two HXR flares are also detected by ASO-S/HXI. We compare the characteristics between outward-traveling SEEs and downward-traveling HXR-producing electrons including the timing, energy spectrum, electron number, etc. Furthermore, we investigate the solar source region of these SEE events.
ST01-A024
Suprathermal Electron Acceleration at the Earth's Bow Shock
Qianyi MA1#+, Linghua WANG1, Xinnian GUO1, Zixuan LIU1, Liu YANG1, Robert WIMMER-SCHWEINGRUBER2
1Peking University, China, 2Kiel University, Germany
The energy spectrum of energetic particles carries crucial information on their acceleration process. Here we present a comprehensive study of the in situ electron acceleration during 138 terrestrial bow-shock crossings measured by the Wind/3DP instrument with good suprathermal electron observations from 1994 to 2004. For each bow-shock crossing case, we utilize the nonlinear least-square shock fitting techniques to obtain the shock parameters and apply an extended pan-spectrum fitting method to self-consistently determine the energy spectral shape of omnidirectional suprathermal electron flux JA (JD) at ~0.1-200 keV in the upstream ambient solar wind (downstream). We find that the downstream suprathermal electrons generally show three spectral types: a single-power-law spectrum, double-power-law spectrum and triple-power-law spectrum. For the presence of significant shock electron acceleration with JD/JA > 1.5, the JD/JA ratio at ~0.4-10 keV is correlated with the magnetic compression ratio rB. We will also present the evolution of accelerated electron energy spectra at bow shocks.
ST01-A025
Electron and Ion Energy Spectra in 3He-rich Solar Energetic Particle Events
Junqi JIA1#+, Linghua WANG1, Glenn MASON2, Robert WIMMER-SCHWEINGRUBER3
1Peking University, China, 2Johns Hopkins University Applied Physics Laboratory, United States, 3Kiel University, Germany
Electron/3He-rich solar energetic particle (SEP) events are the most common solar particle acceleration phenomena detected in situ in the interplanetary medium. To investigate whether the acceleration/source of 3He is correlated with electron enhancement, we compare the energy spectra of both electrons and 3He-rich ions. We select 3He-rich SEPs with high sensitivity measurements on electrons and ions (including H, 3He, 4He, Fe, and O) observed by both solar orbiter and Wind. Utilizing a pan-spectrum fitting method, for the energy spectra of each species, we self-consistently determine the energy spectral shape of both electrons and ions, and examine their relationship. We will present the discussion of whether there is a potential correlation between 3He acceleration and electrons, which will help us better understand the generation of 3He-rich SEPs.
ST01-A027
The 2013 November 12 Solar Electron Event Associated with Solar Jets
Wen WANG1, Wenyan LI2#+, Andrea Francesco BATTAGLIA3, Sam KRUCKER3, Linghua WANG2
1National University of Defense Technology, China, 2Peking University, China, 3University of Applied Sciences and Arts Northwestern Switzerland, Switzerland
We investigate the hard X-ray (HXR) flare-associated “prompt” solar energetic electron (SEE) 2013 November 12 event with joint EUV jet observations from SDO/AIA and STEREO-A/EUVI. The SEE energy spectrum observed by Wind/3D Plasma and Energetic Particle shows a triple-power-law shape with a low-energy break of 10.0 ± 1.7 keV and a high-energy break of 56.6 ± 8.9 keV, which has never been reported before for jet-related SEE events. Associated HXR emissions observed by RHESSI and FGST/GBM show three distinctive peaks with different spectral indices βHPE of HXR-producing electrons (HPEs) derived by means of thick-target bremsstrahlung model. The high-energy spectral index β3 = 4.63 ± 0.65 of SEE is consistent with the HPE spectral index βHPE derived in HXR peak 1 but different from βHPE of HXR peak 2 and peak 3. The main stream of EUV jets reaches a speed of 370 ± 25 km s−1 after an acceleration of up to 2.9 ± 0.4 km s−2 in a timescale of ~2 minutes, and the acceleration time coincides with the decay phase of HXR peak 1. EUV observations from two different viewing directions help to reconstruct the jet magnetic configurations. After the investigation on HXR emissions and jet configurations, the interchange reconnection model triggered by the emerging flux could be a satisfactory explanation for this jet event.
ST01-A031
Shock Analysis of Energetic Proton Enhancements in October-November 2021
Ya-Hui YANG#+, Shao-Chun LU, You-Min CHEN
National Central University, Taiwan
In late October and early November 2021, two major explosions erupt from active regions (ARs) NOAA 12887 and 12891 individually leading to false alarm and miss cases separately in space weather forecasting. One produces the first ground-level enhancement (GLE) in solar cycle 25, and the other is relevant to intense geomagnetic disturbances. Two interplanetary shocks associated with two Earth-directed fast CMEs are observed on 2021 October 29-31 and November 3-4 by STEREO-A, WIND, Parker Solar Probe, and Solar Orbiter spacecraft. The longitudinal separations between two spacecraft can be up to about 54 degrees during this period. In this study, we aim to examine the effects of interplanetary shocks in accelerating energetic protons by implementing shock analysis with different approaches, including the estimations of shock parameters and propagation times. Based on the multi-spacecraft measurements of solar winds and energetic particles, the possible deformation of shocks or the interactions with ambient solar wind structures will also be discussed.
ST01-A032
Spectral Analysis of Solar Energetic Protons in Interplanetary Coronal Mass Ejections
You-Min CHEN#+, Chun-Wei HUANG, Shao-Chun LU, Ya-Hui YANG
National Central University, Taiwan
Interplanetary coronal mass ejections (ICMEs) is thought to be one of the potential sources of particle accelerations, especially the accompanied shock ahead of the ICME main body. However, due to the variety of plasma and magnetic field properties in ICMEs, the interactions between ICME and ICME or other transient structures, and the limitations of single-point in-situ measurements, not all the ICMEs can be found to have the correspondingly obvious enhancements in energetic proton fluxes. Moreover, the acceleration efficiency of energetic protons by ICMEs is still unclear. Accordingly, we attempt to characterize the spectral evolutions of solar energetic protons in this study based on the solar wind and particle observations by STEREO spacecraft together with its ICME catalogue to understand the role of ICMEs played in particle accelerations. The relationship of energetic proton enhancements with the ICME-driven shocks, sheath regions, or ambient solar wind structures will be discussed as well.
ST07-A016
| Invited
Evaluation of the Nonlinear Pitch Angle Scattering of Energetic Electrons by Coherent Whistler-mode Waves
Yuto KATOH#+, Genki ISHIZAWA, Masahiro KITAHARA
Tohoku University, Japan
Whistler-mode waves observed in the Earth's magnetosphere significantly contribute to both acceleration and loss processes of high-energy electrons through wave-particle interactions. The pitch angle scattering by whistler-mode waves results in the loss of energetic electrons from the magnetosphere. The precipitation of energetic electrons contributes to diffuse/pulsating aurora in the polar ionosphere. Recently, it has been clarified that low-pitch angle electrons are peculiarly trapped by coherent whistler-mode waves and are scattered away from the loss cone by anomalous trapping. This nonlinear process contradicts the conventional understanding that auroral electrons are diffusively scattered from the loss cone. We carry out a series of test-particle simulations to reveal how significant the nonlinear effects are in the evolution of the pitch angle distribution near the loss cone. We compute the motion of energetic electrons moving along a field line under a packet of monochromatic whistler-mode waves generated at the magnetic equator. Simulation results show the efficient pitch angle scattering into the loss cone of electrons near the loss cone and in a large pitch angle range. We analyze the phase space trajectories of all electrons in the simulation system. By considering a difference in the number of times the particle satisfies the resonance condition, we categorize 3 types of pitch angle scattering: resonant scattering, non-resonant scattering, and phase trapping. Results of the present study clarify that low pitch angle electrons move dynamically in the pitch angle-energy space due to the nonlinear effects in the resonant pitch angle scattering process.
ST09-A010
Beyond Prediction: Leveraging Interplanetary Environmental Information and Deep Learning to Reexamine and Understand Thermospheric Mass Density Variations
Wenbo LI+, Libo LIU#, Yiding CHEN, Yijia ZHOU, Huijun LE, Ruilong ZHANG
Chinese Academy of Sciences, China
This study examined the response of Thermospheric Mass Density (TMD) to various solar-terrestrial conditions during days 222 to 241 of 2014. This period is characterized by complex solar-terrestrial disturbances, such as geomagnetic storms, substorms, and space hurricanes. The various influencing factors involved in this period allow us to analyze the response of TMD to solar-terrestrial disturbances more comprehensively. The investigation involved analyzing TMD observations from the GRACE-A and Swarm-A satellites, along with model simulations. It was reported that during a typical space hurricane event (DOY 232, 2014), although there might be a substantial energy injection, there was no significant disturbance in global TMD. To delve deeper, Deep Learning (DL) models were developed, integrating Interplanetary Environment Information (IEI), solar activity, geomagnetic disturbances from the OMNI database, and TMD observations from the CHAMP satellite. These models were employed to evaluate the effects of key solar-terrestrial indices and parameters on TMD variations. The findings underscore the significant contribution of the By component of the interplanetary magnetic field in influencing TMD and highlight the importance of comprehensive IEI integration for a better understanding of TMD variations. The study further demonstrates that DL models, with strategically selected inputs, not only facilitate accurate predictions but also reveal diverse observational features, thus enriching our comprehension of the factors driving TMD variations.
ST09-A011
Statistical Study of Type III Solar Radio Bursts Using Parker Solar Probe
Tulsi THAPA1+, Yihua YAN1,2#
1Chinese Academy of Sciences, China, 2University of Chinese Academy of Sciences, China
Type III bursts are indirect indicators of energetic electrons travelling outward from the Sun along an open magnetic field line in the corona and interplanetary (IP) medium. A multitude of insights into plasma dynamics can thus be gleaned from the spatial and spectral evolution of type IIIs. We conducted a statistical assessment of only simple, intense, and isolated 43 IP type III bursts, as recorded by the FIELDS Instrument onboard the Parker Solar Probe (PSP) during Encounters 05 (E05) to 11 (E11). For the first time, we calculated the rise, peak and decay time, studying their spectral indices using a power-law approach. The spectral indices for rise, peak, decay, and total duration were determined as -0.48±0.02, -0.43±0.1, -0.68±0.02 and -0.65±0.02 respectively. These indices exhibit an inverse √f (frequency) nature with time profile. A mean drift rate of -29 MHz/s, typical of type III bursts, was obtained. The correlation analysis between drift rate and mean duration revealed a moderate value of 58%, indicating that radio bursts with faster drift rates tend to have shorter durations. Additionally, we determined the average electron beam velocities for the front, middle, and back of the exciter as 0.15c, 0.13c, and 0.08c, respectively, corresponding to electron energies ranging from tens of eV to hundreds of keV. Notably, faster electron beams were found to generate emissions with shorter durations. This ongoing work is being extended to include an analysis of the energy spectrum, density, temperature, and Pointing flux to comprehensively understand the dynamics of energetic electron behaviour in the low-frequency domain.
ST09-A018
Utilizing Jove Radio Telescopes for Enhanced Analysis of Thunderstorms, Jupiter, and Solar Activities
Tin Ngo KO#+, Skyler SIU, Charles LIU, Serena TSAI, Diana IBARRA
The ISF Academy, Hong Kong SAR
The NASA Radio JOVE Telescope Program was established in 1999. The program aims to provide an opportunity for radio enthusiasts to listen to and study natural, low-frequency (15~30 MHz) electromagnetic radiation emitted by Jupiter, the Sun, and the galaxy. Specialized Radio JOVE software can receive signals that can be analyzed. In 2023, the ISF Academy installed a Radio JOVE radio telescope in Hong Kong. Signals from the Sun and the galaxy were analyzed first. The signals from the Sun showed signs of high sunspot activity with solar flares, as shown by a spike in intensity of 20.5MHz (Wong, Zhou, Wong, 2023). These signals are emitted by radio landmarks and are multidirectional. These radio waves are generated by electrons and protons interacting with Jupiter’s magnetic field. The highly volcanic moon orbiting Jupiter, Io, also enhances the quality of the signals received. The JOVE received frequencies ranging from 15~30MHz, making it suitable for data collection of the radio signals from Jupiter, which are 10~40MHz in frequency. The results given could be used to analyze patterns and trends of Jupiter’s state during high sunspot activity and detect the thunderstorms on Jupiter.
ST09-A023
Design of Multilayer Shields for Low Earth Orbit Cosmic Radiation Environment Using Geant4, TOPAS, and MCNP6.2
Hojin LEE#+, Jongdae SOHN, Junga HWANG
Korea Astronomy and Space Science Institute, Korea, South
Space-grade electronic components are generally used for the operational stability of satellites, but recently, the trend to use commercial electronic components for LEO(Low Earth Orbit) satellites has become stronger. However, commercial electronic components require additional radiation shielding because the radiation resistance design is not at the level of space-grade components. When cosmic radiation passes through electronic components, TID(Total Ionizing Dose), SEE(Single Event Effect), and DD(Displacement Damage) appear. TID is absorbed dose, and its value increases in proportion to time. SEE and DD occur probabilistically due to electrical and physical phenomena. When electronic components are covered with a shield, the radiation flux reaching them is reduced, reducing the TID value and the probability of SEE and DD. This study designed a shield for the LEO environment using radiation simulation programs Geant4, TOPAS, and MCNP6.2, which were created based on Monte Carlo techniques. The cosmic radiation energy and flux at a 400 km altitude were calculated using the SPENVIS system. Using SPENVIS SHIELDOSE2, it was calculated that when electronic components are shielded with 1mm aluminum, about 7.3 krad of absorbed dose is generated per year. Using this result as a reference, we confirmed that Geant4, TOPAS, and MCNP showed the same results and further simulated multilayer shields. The 1-layer shield is composed of one of seven materials (Al, Fe, Cu, Ni, Ti, Pb, W), and the TID reduction efficiency was calculated for each thickness. The 2-layer shield adds 4mm aluminum in front of the 1-layer shield. 4mm aluminum refers to the outer wall of the satellite, assuming that electronic components are mounted inside the satellite. The 3-layer shield adds BPE (Borated Polyethylene) to the back of the 2-layer shield, taking neutron shielding into consideration.
ST10-A003
Characteristic Scales of MHD Turbulence in the Alfvénic Solar Wind
Luca SORRISO-VALVO1#+, Daniele TELLONI2, Raffaella D'AMICIS2, Emiliya YORDANOVA3
1CNR - ISTP, Italy, 2National Institute for Astrophysics, Italy, 3Swedish Institute of Space Physics, Sweden
We analyze the spectral and intermittency properties of the low-frequency fluctuations in Alfvénic intervals in the inner heliosphere. We consistently observe that the statistical properties of the fluctuations are not self-similar in a range of scales where shallow spectra (~1/f) are typically observed. These observations suggest that, at such scales, nonlinear interactions may be effectively generating a turbulent-like cascade, yet not fully developed. We thus explore the validity of the third-order moment scaling law and the associated energy transfer rate in the same range.
ST10-A005
Radial Evolution of Turbulence in the Inner Helisophere
Luca SORRISO-VALVO1#+, Daniele TELLONI2, Raffaella D'AMICIS3, Emiliya YORDANOVA4, Denise PERRONE5, Julia STAWARZ6
1CNR - ISTP, Italy, 2National Institute for Astrophysics, Italy, 3INAF - Institute for Space Astrophysics and Planetology, Italy, 4Swedish Institute of Space Physics, Sweden, 5Agenzia Spaziale Italiana, Italy, 6Northumbria University, United Kingdom
We present recent results on the radial evolution of turbulence in the inner heliosphere. Spectra, intermittency and third-order law are used to characterize the turbulence. We use measurements of the same plasma at different distances, obtained during occasional spacecraft alignments, measurements of plasma from the same solar source, and statistical ensembles, we determine the radial profiles of turbulence parameters. Results are discussed in the framework of current heliospheric models.
ST10-A008
Magnetic Reconnection Above Martian Crustal Field
Rentong LIN#+, Shiyong HUANG, Zhigang YUAN, Honghong WU, Kui JIANG
Wuhan University, China
Mars lacks a global intrinsic magnetic field but owns crustal magnetic anomalies mostly in the southern hemisphere. At subsolar, the crustal magnetic anomalies, i.e., crustal fields, directly interact with interplanetary magnetic field at the mini-magnetopause, the boundary between shocked solar wind and mini-magnetosphere. In the Martian magnetotail, the magnetic field topology is complex and flexible, especially over strong crustal field regions. However, the answer to how the magnetic field topology within crustal field regions transitions is elusive. Using the magnetic field and plasma measurements by Mars Atmosphere and Volatile Evolution, we report a case of magnetic reconnection at Martian mini-magnetopause and a case of interchange reconnection between the open and closed crustal fields in the near-Mars magnetotail. Protons and oxygen ions from Martian atmosphere were accelerated during reconnection and would probably escape along the L-direction. It suggests that magnetic reconnection can occur between interplanetary magnetic field and the crustal magnetic fields near subsolar, i.e., at Martian mini-magnetopause, and that interchange reconnection can occur between open and closed crustal fields in the Martian near-magnetotail. Reconnection at the magnetopause of mini-magnetosphere and interchange reconnection occurring on the nightside changes the magnetic field topology within the crustal field regions and contributes to heavy ion escape.
ST10-A011
Reconstruction of Electron Vortex in Space Plasmas
Lin YU+, Shiyong HUANG#
Wuhan University, China
Space plasmas are turbulent and maintain different types of critical points or flow nulls. Electron vortex, as one type of the flow null structures, is crucial in the energy cascade in turbulent plasmas. However, due to the limited time resolution of the spacecraft observations, one cannot analyze the three-dimensional properties of the electron vortex ever. In the present study, with the advancement of the FOTE-V method and the unprecedented high-resolution measurements from four MMS spacecraft, we successfully identify the electron vortex and then reconstruct its three-dimensional topology of the surrounding electron flow field. The reconstructed results show that the configuration of the electron vortex is elliptical. Comparison between the observation and reconstruction scales of the vortex indicates the reliable reconstruction of the flow velocity. Our study sheds light on the understanding of the topology and property of the electron vortex and its relationship with kinetic-scale magnetic holes.
ST10-A012
Statistical Characteristics of Electron Vortexes in the Terrestrial Magnetosheath
Zhao WANG+, Shiyong HUANG#, Zhigang YUAN, Yunyun WEI, Kui JIANG, Sibo XU, Jian ZHANG, Rentong LIN, Lin YU, Qiyang XIONG
Wuhan University, China
Utilizing the unprecedented high-resolution Magnetospheric Multiscale mission (MMS) data from September 2015 to December 2017, we perform a statistical study of electron vortexes in the turbulent terrestrial magnetosheath. On the whole, 506 electron vortex events are successfully selected. Electron vortexes can occur at four known types of magnetic structures, including 78, 42, 26, and 39 electron vortexes observed during the crossings of the current sheets (CS), magnetic holes (MH), magnetic peaks (MP), and flux ropes (FR) respectively. Except for the four types of structures, the rest of the electron vortexes are the 'Others' category, defined as unknown structures. The electron vortexes mainly occur in the subsolar region and only a few in the flank region. The total occurrence rate of all electron vortexes is 4.86 per hour, and on average, 3.65 events/hour in the X-Y plane and 3.26 events/hour in the X-Z plane. The durations of most of the electron vortexes concentrate within 0.5~1.5 seconds and are 1.09 seconds on average. The electron vortexes are ion-scale structures due to the average scale of 2.05 ion gyroradius. In addition, the means, medians and maxima of the energy dissipation J·E¢ in the electron vortexes are almost positive, implying that the electron vortex may be a potential coherent structure or channel for turbulent energy dissipation. All these results reveal the statistical characteristics of electron vortexes in the magnetosheath and improve our understanding of energy dissipation in astrophysical and space plasmas.
ST10-A016
Statistics of Intermittent Dissipation and Magnetic Field Topology at Kinetic Scales in the Magnetosheath Turbulence
Shiyong HUANG#+
Wuhan University, China
The dissipation of turbulence energy in kinetic-scale plasma has long been a challenging problem. As reported in previous simulation and observation studies, stronger energy conversion from bulk flow into the internal energy measured by the pressure-strain interaction term tend to occur within large flow stress and vorticity regions but not the structures with strong current. We wonder how the Ohmic dissipation which converts energy between electromagnetic fields and particles distribute within these regions, in addition, we also access the contributions to dissipation of different magnetic topologies. Our results indicate that intense Ohmic dissipation tends to occur in regions of strong current and PVI index. Furthermore, the dominant contribution of the "O-type" topologies to dissipation are also confirmed.
ST10-A018
Reconnection Rate and Transition from Ion-coupled to Electron-only Reconnection
Quanming LU#+, Yundan GUAN, San LU
University of Science and Technology of China, China
Standard collisionless magnetic reconnection couples with both electron and ion dynamics. Recently, a new type of magnetic reconnection, electron-only magnetic reconnection without ion outflow, has been observed, and its reconnection rate has been found to be much higher than that in ion-coupled reconnection. In this paper, using 2D particle-in-cell simulations, we find that when the ion gyroradius is much smaller than the size of the simulation domain, magnetic reconnection is standard with ion outflows. As the ion gyroradius increases, the ion response gradually weakens, and the reconnection rate becomes higher. Electron-only reconnection occurs when the ion gyroradius is comparable to the size of the simulation domain. This trend applies to both strong and weak guide field situations. Therefore, the key factor that controls the transition from ion-coupled reconnection to electron-only reconnection is the ratio between the ion gyroradius and the size of the simulation domain. We further show that, in electron-only reconnection, when the initial electron current sheet is thinner, the reconnection rate and the electron outflow speed are higher.
ST10-A020
Spontaneous Generation of Alfven Waves by Bursty Interchange Magnetic Reconnection in the Solar Corona
Liping YANG1#+, Jiansen HE2, Xueshang FENG1, Hui LI3, Fan GUO3, Hui TIAN2
1Chinese Academy of Sciences, China, 2Peking University, China, 3Los Alamos National Laboratory, United States
Alfven waves contribute significantly to the solar coronal heating, the solar wind acceleration, as well as Alfvenic turbulence formation. As a universal process, magnetic reconnection has long been credited as a potentially crucial source of Alfven waves, but how magnetic reconnection trigger Alfven waves remains elusive. Here, with simulations of three-dimensional bursty interchange magnetic reconnection in the solar corona, for the first time, we find that Alfven waves are spontaneously excited in the reconnection sheet and propagate bi-directionally even along the unreconnected magnetic fields. The enhanced total pressure inherently carried by flux ropes gives kicks to the magnetic fields, and the nearly same propagation speed of the flux ropes and the kicks makes the kicks growing into the observed Alfven waves, which have large amplitudes and high frequencies, carrying substantial energy for heating the quiet corona and accelerating the solar wind. Our findings demonstrate that Alfven waves are natural products of three-dimensional intermittent magnetic reconnection, bringing its fundamental significance for energy release, transport, and conversion occurring in the plasma system.
ST10-A025
Coupling Between Ion and Electron Motions in the Outer Electron Diffusion Region of Collisionless Magnetic Reconnection
Cong CHANG+, Quanming LU#, San LU, Kai HUANG, Rongsheng WANG, Yukang SHU
University of Science and Technology of China, China
Magnetic reconnection is a bursty dynamic process that involves the conversion from magnetic energy to plasma kinetic energy and thermal energy. In collisionless magnetic reconnection, ion and electron motions are decoupled and they become demagnetized at distinct scales known as the ion diffusion region (IDR) and the electron diffusion region (EDR), respectively. Based on previous satellite observations and simulations, the EDR can be further divided into inner and outer EDRs, where electrons exhibit different behaviors. To investigate the coupling between electron and ion motions in the EDR in detail, we conducted two-dimensional particle-in-cell simulations. The simulation results show that the speed of the electron outflow increases in the inner EDR. In the outer EDR, the electron outflow speed first increases and then decreases until reaching the boundary of the outer EDR. At the boundary of the outer EDR, the magnetic field is piled up and forms a dipolarization front. Furthermore, we revealed the electron and ion acceleration process by analyzing the contributions from the Lorentz force, the electric field force, and the pressure tensor term. The electrons are accelerated by the reconnection electric field in the out-of-plane direction and then diverted to the outflow direction by the Lorentz force when moving away from the X-line. Both electric field and electron pressure gradient force tend to drag the electron outflow. For ions, the Lorentz force and the ion pressure gradient force are almost balanced. It is also noted that the Hall electric field force does positive work on ions and is not negligible. The ions keep accelerating until they are coupled again with electrons at the dipolarization front. Our study of electron and ion motions in the EDR suggests the Hall nature of collisionless magnetic reconnection. This could help to understand the fast reconnection rate in Hall reconnection.
ST10-A026
Second Order Theory Calculations of Solar Wind Heating and Acceleration in the Inner Heliosphere
Jingyu PENG1#+, Xingyu ZHU2, Jiansen HE1, Die DUAN3
1Peking University, China, 2The University of Alabama in Huntsville, United States, 3National University of Defense Technology, China
The heating and acceleration of solar wind ions is a crucial issue in heliospheric physics. Wave-particle interaction may be a very important mechanism for the heating and acceleration of solar wind ions. The heating rates and accelerations contributed by Alfvén/ion cyclotron waves to protons and alpha particles at different radial positions of 0.1-0.4 au are theoretically calculated based on the second-order theory of wave-particle interactions using data from the 6-10 orbits of the Parker Solar Probe and a fluctuation power spectral model, and compared with observations. Theoretical calculations indicate that alpha particles experience higher acceleration and heating rates compared to protons. This is consistent with the faster and hotter alpha particles detected in-situ.
ST10-A027
Plasma Heating Associated with Vorticity: MMS Observations of Two Alfvén Vortices
Chenxi ZHAI+, Tieyan WANG#
Yunnan University, China
The intermittent fluctuations with localized current density or vorticity are believed to play a crucial role in the process of turbulence dissipation and plasma heating. Current theory and simulations of plasma turbulence have postulated a scenario where vorticity, depending on the sign of ω · B, are statistically better correlated with plasma heating than current density. However, whether this physical picture is compatible with in-situ observations remains unknown. Meanwhile, Alfvén vortices, which are key ingredients of coherent structures, serve as ideal candidate to test the theory. Indeed, plasma kinetic effects and energy conversion were found near Alfvén vortices through recent measurements. In this study, we present supporting evidence for this scenario by comparing plasma signatures occurring at two Alfvén vortices with opposite sign of ω · j. In these two vortices observed by Magnetospheric Multiscale, the ion temperature, as well as the temperature anisotropy are both positively correlated with parallel vorticity, whereas the correlations with parallel current densities are opposite. Combining these signatures suggests a better correlation associated with vorticity. Our result may further improve our understanding of intermittent energy transfer processes in collisionless plasmas.
ST10-A032
Electromagnetic Emission Due to the Interaction of Counter-streaming Plasma Flows in the Laboratory Magnetic Arch
Mikhail VIKTOROV#+, Artem KORZHIMANOV, Andrey SLADKOV, Andrey ELYASIN, Sergey KORYAGIN
Institute of Applied Physics of the Russian Academy of Sciences, Russian Federation
Laboratory study of the interaction of supersonic flows of highly ionized plasma with magnetic fields of the arched configuration is relevant for understanding the physical mechanisms of a number of space plasma phenomena observed in the inner regions of the coronal loops on the Sun, in the transition regions of planetary magnetospheres, such as, boundary layers of the Earth's magnetosphere and the planets of the solar system. In the present work we perform experiments on a compact laboratory setup, in which a collisionless plasma regime typical for space conditions is achieved. We study processes during the collision of two supersonic plasma flows injected along the magnetic field lines of the magnetic arch from its foots in opposite directions. Flows of fully ionized plasma are created by two independent plasma generators which evaporate the material of the aluminium cathode as a result of a vacuum arc discharge. During the interaction of plasma flows we detect non-thermal microwave plasma emission at frequency in the electron cyclotron range. The latter exactly corresponds to the magnetic field strength in the apex of the magnetic arch. We discuss possible kinetic mechanisms which could lead to the formation of a non-isotropic fraction of electrons during the collision of plasma flows in the magnetic arch which is responsible for excitation of plasma electromagnetic emission using theoretical estimates and numerical modelling. This work was supported by the Russian Science Foundation (Grant No. 23-12-00317).
ST11-A003
Fast Earthward Convection in the Magnetotail Plasma Sheet and Nonzero IMF By: MMS Statistics
Timo PITKÄNEN1,2#+, Ghai Siung CHONG2, Maria HAMRIN2, Anita KULLEN3, Heikki VANHAMAKI4, Jong-Sun PARK1, Motoharu NOWADA1, Audrey SCHILLINGS2, Eva KRÄMER2
1Shandong University, China, 2Umeå University, Sweden, 3KTH Royal Institute of Technology, Sweden, 4University of Oulu, Finland
We statistically investigate convective earthward fast flows using data measured by the Magnetospheric Multiscale (MMS) mission in the tail plasma sheet during 2017-2021. We focus on ‘frozen in’ fast flows and investigate the importance of different electric field components in the Sun-Earth (Vperpx) and dusk-dawn (Vperpy) velocity components perpendicular to the magnetic field. We find that a majority of the fast flow events (52% of 429) have the north-south electric field component (Ez) as the most relevant component (Ez category) and 26% have Ey and Ex as the relevant components (conventional category). The rest of the flow events, 22%, fall into the two ‘mixed’ categories, of which almost all these fast flows, 20% of 429, have Ey and Ez important for Vperpx and Vperpy, respectively. There is no Y-location preference for any type of the fast flows. The conventional fast flows typically have large magnetic field inclination angles (measured close to the neutral sheet) and Ez category small angles (measured both farther away from and close to the neutral sheet). Typical total speeds are highest in the mixed category. Typical perpendicular speeds are comparably high in the conventional and mixed categories. The slowest fast flows are measured in the Ez category. Favoured opposite Vperpy directions above and below the neutral sheet are statistically distinguishable under the influence of nonzero IMF By. The influence appears to be most efficient in the Ez category.
ST11-A007
Solar Wind Properties in Association with Non-parker Spiral Interplanetary Magnetic Field Structures at 1 AU
Jong-Sun PARK1#+, Quanqi SHI1, Jungjoon SEOUGH2, Hui ZHANG1
1Shandong University, China, 2Korea Astronomy and Space Science Institute, Korea, South
It is well-known that the rotation of the Sun leads the interplanetary magnetic field (IMF) lines embedded in the outward flowing solar wind to the Parker spiral configuration. For typical solar wind conditions (with a solar wind speed of about 400 km/s), the Parker spiral orientation (viewed from ecliptic zenith) has an angle of approximately 45° clockwise from the Sun-Earth line at Earth’s orbit distance. Occasionally, however, the orientation of the interplanetary field lines deviates significantly from the common Parker spiral configuration. Spacecraft observations revealed that the IMF can retain either nearly radial (outward or inward), tangential (dawnward or duskward), or even normal (northward or southward) direction on hourly time scales (hereinafter called the non-Parker spiral IMF structures). In this study, we statistically examine the distinctive features of these three types of non-Parker spiral IMF structures at 1 AU using upstream magnetic field and solar wind plasma/particle data measured by Wind spacecraft over the period from 1995 to 2022. By analyzing not only the annual and solar cycle variations of their occurrence probabilities but also the characteristics of the solar wind parameters for each type of non-Parker spiral IMF structures, we discuss the formation mechanisms of these unusual IMF structures that could play distinctive roles in controlling solar wind-magnetosphere interaction (that is, solar wind mass, momentum, and energy transfer to the magnetosphere) via the magnetic reconnection processes.
ST11-A008
On the Acceleration of Polar Cap Patches Entering the Nightside Auroral Oval: Multi-instrument Observations
Zanyang XING1#+, Jin YUYAN2, Qing-He ZHANG3,1, Larry LYONS4, Yongliang ZHANG5, Sheng LU1, Yu-Zhang MA1, Yong WANG1
1Shandong University, China, 2Chinese Academy of Sciences, China, 3National Space Science Center, Chinese Academy of Sciences, China, 4University of California, Los Angeles, United States, 5Johns Hopkins University Applied Physics Laboratory, United States
We report results from a study of nine polar cap patch events observed by multiple ground-based instruments in the nightside near the end of a sub-storm. The instruments include the all-sky imagers (ASI) at the Chinese Yellow River Station, EISCAT Svalbard and Tromso UHF radars, GPS receivers, and SuperDARN radars. The patches moved across the polar cap, intensified near the nightside poleward boundary of the auroral oval, and finally entered the auroral oval. The ASI images showed fine-scale structures and less steeper gradient at the trailing than leading edge of the patches, which seem caused by the plasma gradient-drift instability. The patches moved at a speed of ~350-520 m/s in the polar cap and accelerated when they entered the auroral oval. The poleward edge of the aurora suddenly brightened at around the patch-aurora contact region in association with flow enhancements and/or flow channels. Based on the observations, we suggest that the equatorward evolution of the polar cap patch is associated with enhanced ionospheric flows near the nightside oval, indicating increased tail reconnection rate and poleward boundary intensification of the auroral oval.
ST11-A010
Simultaneous Occurrence of Substorm and Pseudosubstorm
Yukinaga MIYASHITA1,2#+, Madeeha TALHA1,2
1Korea Astronomy and Space Science Institute, Korea, South, 2Korea National University of Science and Technology, Korea, South
Our previous studies showed that the auroral onset arc associated with a substorm develops in three steps. After initial auroral brightening, the onset arc extends azimuthally while its weak wavelike structure gradually grows. The onset arc then enhances further and its wavelike structure also grows more rapidly. Finally, poleward expansion begins. On the other hand, the pseudobreakup (pseudosubstorm) is similar to the early stage of the substorm onset arc development but subsides without proceeding to poleward expansion. Pseudobreakups often occur separately before a substorm, but the separate occurrence does not necessarily seem to be the case. Here, using Time History of Events and Macroscale Interactions during Substorms (THEMIS) data, we show substorm events in which a substorm auroral onset arc and a pseudobreakup arc appeared and developed simultaneously. While a substorm onset arc is developing, an auroral arc very similar to a pseudobreakup also appears and develops for some substorm events. We interpret this arc as a pseudobreakup arc. The pseudobreakup arc appeared either just equatorward or just poleward of the substorm onset arc. Such events are not rare, that is, they occurred for 20% of our selected substorm events. We will discuss the magnetotail processes associated with simultaneous substorm and pseudobreakup events.
ST11-A012
Dayside Magnetopause Energy Transfer Under Purely Southward IMF Condition: 3-D Global Hybrid Simulation
Yongyuan YI1#+, Meng ZHOU1, Yu LIN2, Ye PANG1, Xiaohua DENG3
1Nanchang University, China, 2Auburn University, United States, 3Wuhan University, China
In this paper, the dayside magnetopause energy transfer (energy transfer from the magnetopause boundary layer to the magnetosphere) and its dependence on the magnetopause dynamic evolution under purely southward IMF conditions are studied via 3-D global-scale hybrid simulation. We find that the energy input from the solar wind to the magnetopause boundary layer is mainly in the form of electromagnetic energy, while the energy input from the magnetopause boundary layer to the magnetosphere is mainly in the form of plasma energy. The energy transfer across the magnetopause surface exhibits temporal variability, driven by the dynamic evolution of reconnection and flux transfer events (FTEs). During the development of multiple X-line reconnection and FTEs, a substantial portion of solar wind energy does not directly penetrate the dayside magnetopause and enter the magnetosphere. Instead, it propagates poleward with the reconnection outflow and FTEs, and with the flow convection to the tail magnetopause within the magnetopause boundary layer. By including the ion kinetic physics, our results provide the details of the energy transport from the solar wind to the magnetosphere at the dayside magnetopause.
ST11-A018
Observation of Kinetic-scale Plasma Vortices in Earth's Magnetosheath
Shutao YAO#+
Shandong University, China
In space, collisionless plasmas often display vortex-like structures, which are frequently observed in turbulent plasma. The plasma downstream of the bow shock is highly turbulent and contains numerous vortices across a range of scales, from magnetohydrodynamic to particle-gyro scales. The presence of plasma vortices in the Earth's magnetosheath and their significant roles in space plasma were studied in previous studies. However, vortex generation on the ion-to-electron gyroscale has been lacking. Here, we present evidence of electron-scale vortices generated in Earth's bow shock by anisotropic electrons with a specific energy range. We also demonstrate the generation of ion-scale vortices by the ion diamagnetic drift in the magnetosheath and employ a kinetic equilibrium model to reconstruct the vortex features.
ST12-A006
A Statistical Study of the Response in Transition Region for Coronal EUV Waves
Xiaoqian WANG#+, Ruisheng ZHENG
Shandong University, China
Coronal extreme ultraviolent (EUV) waves are the globally propagating disturbances in the solar corona. Before the detection by the space-born EUV imagers, the existence of coronal EUV waves was predicted by the chromospheric propagating disturbances, Moreton waves. It is widely accepted that Moreton waves represent the chromospheric imprints of coronal EUV waves that compress downward during the lateral propagation. It is inevitable that coronal EUV waves will compress the interlayer between the corona and the chromosphere, the transition region (TR), before touching the chromosphere. However, the responses in TR of coronal EUV waves lack enough attention. Here, we focus on the wave signatures in He II 304 Å for a sample of 640 EUV waves from April 2010 to December 2021, in order to establish a “bridge” connecting coronal EUV waves and chromospheric Moreton waves. It has been observed that approximately 15% of all coronal wave events are characterized by responses in the transition region. Moreover, Moreton wave events account for about 4% of all coronal wave events, while constituting around 25% of the events with responses in TR. In addition, in events exhibiting responses in TR, there is a negative correlation between the brightness of wavefront in TR and the inclination angle of the eruption. These results indicate that the proportion of Moreton waves in events with responses in TR is much greater than the proportion in coronal wave events. Furthermore, whether coronal waves can compress into the lower atmosphere is jointly determined by the wavefront signal and the inclination angle of the eruption.
ST12-A009
| Invited
Taut Magnetic Structure May Steepen the Coronal Wave
Yihan LIU#+, Ruisheng ZHENG
Shandong University, China
Solar extreme ultraviolet (EUV) waves, recognized as propagating disturbances primarily observed in the Extreme Ultraviolet spectrum, are often attributed to fast magnetic-sonic waves or shocks. These phenomena commonly accompany various solar extreme events, ranging from flares and jets to solar eruptions. Existing literature extensively explores the mechanisms behind EUV wave generation, from eruption cores to coronal plasma disturbance induced by the waves. While previous studies acknowledge the role of coronal loops in EUV wave formation, their contribution is typically described in terms of visible oscillations or shock cores. Through a detailed observational case study, we propose that these coronal structures may play a direct role in steepening the wavefront. If confirmed, this insight challenges the prevalent physical descriptions of EUV waves, necessitating a reconsideration of the commonly accepted models.
ST12-A010
Restricted Jet Eruption Related EUV Wave
Jun LI#+, Ruisheng ZHENG
Shandong University, China
Coronal extreme ultraviolet (EUV) waves, large-scale disturbances accompanying solar eruptions, are observed in the extreme ultraviolet wavelengths. Using the joint observations from the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory and the Extreme Ultraviolet Imager on board the Solar Terrestrial Relations Observatory, we report an EUV wave event that occurred on April 12, 2017. Wave signals at 171 Å, 193 Å, and 195 Å are visible. These waves are driven by a jet, and the coronal loops related to the jet can be roughly divided into three groups: low loops, high loops, and open loops. When the jet erupts, a narrow wave signal is initially observed at the near end of the loops along the direction of the jet. Subsequently, a wider and weaker wave propagates outward and is seen at the far end of the loops in the 193 Å wavelength. The wave seen in the 195 Å is observed from the limb and is related to the opening of the high loops. We believe that this jet was a restricted eruption, as it is clear that the jet only moved to the middle of the coronal loops, above the low loops, and the low loops did not open. Afterwards, we can also see the jet falling. Among the three wave signals we observed, the waves at 193 Å and 195 Å likely formed due to the opening of external high loops, while the "wave" seen at 171 Å was merely the result of jet material moving along open loops, rather than a true wave.
ST12-A014
Research and Applications of Bidirectional Quasi-periodic Fast-propagating Magnetosonic Waves
Miao YUHU#+
Shenzhen Institute of Information Technology, China
Coronal quasi-periodic fast-propagating (QFP) magnetosonic waves in the solar coronaare a common wave phenomenon, which is often associated with solar activities such as flares and coronal mass ejections(CMEs). QFP waves provide a new detection tool for coronal seismology. Research has shown that these waves contain crucial physical information that can be used to diagnose characteristics of the flare core region, measure the coronal magnetic field, and investigate energy release and transport processes. Miao et al. (2021) reported that a bidirectional QFP (BQFP) wave event. The authors reported that the discovery of characteristics of BQFP waves is of significant importance for a deeper understanding of the nature of QFP waves and the establishment of relevant models. This study contributes to a more accurate diagnosis of the source location of QFP waves and the core region of solar flares. Despite significant improvements in observational data and numerical simulations over the past decade, the excitation mechanism of QFP waves remains incompletely understood. Ongoing advancements in observational technologies, particularly the gradual application of artificial intelligence in astronomical observations, are expected to deepen our understanding of solar oscillations in the future.
ST12-A022
Waves and Oscillations in Faint Coronal Hole Loops
Adel Sulaiman H. ALANEZY1#+, Istvan BALLAI1, Gary VERTH1, Viktor FEDUN1, Kartika SANGAL2, Abhishek SRIVASTAVA2
1The University of Sheffield, United Kingdom, 2Indian Institute of Technology (BHU) Varanasi, India
This study delves into the wave dynamics of small loops in a solar coronal hole using high-resolution EUV (e.g. 171 and 193 Å) data from the Atmospheric Imaging Assembly onboard Solar Dynamics Observatory (AIA/SDO). A number of active regions in the northern coronal hole have been isolated and the longitudinal and transversal oscillations of short and faint loops were studied. We measured the phase speeds of the propagating intensity disturbances by employing cross-correlation analysis, and by obtaining the slopes in time-distance plots. We obtained original and detrended light curves at different locations and characterised them by performing Fourier and wavelet analysis. The variation of the intensity has been collected after fitting the loops by linear longitudinal and transversal slits. All observed waves and oscillations undergo a spatial damping, therefore the signal was fitted with a decaying sinusoidal profile that allows us to diagnose the transport coefficients in these loops. The time-distance maps reveal clear propagation of intensity oscillations in all investigated EUV channels. We determined the nature of the intensity disturbances as slow magneto-acoustic waves by measuring their phase speeds. The time-distance maps, as well as the detrended light curves, show an increase and decrease in the amplitude of propagating 3 min oscillations over time. The Fourier power spectrum yields the presence of significant powers with several nearby frequencies in the range of 2–3 min (5–8 mHz), along with many other smaller peaks, so that these short loops support the propagation of multiple waves.
ST12-A023
Relationship Between Hα, Lyα and EUV Waves About an X2.1 Flare
Yue ZHOU1+, Li FENG1#, Yiwei NI2
1Chinese Academy of Sciences, China, 2Nanjing University, China
EUV waves have been widely studied, especially after the launch of AIA/SDO and are sometimes simultaneous observed with the Hα waves, only in highly inclined eruptions. The Hα waves serve as the manifestation of the fast-wave component of EUV waves but there are still many mysteries. SDI/ASO-S detects Lyα waveband (121.6±4.5 nm) and reflect the information of the transition region. A X2.1 class flare erupted on the northwestern solar limb, accompanied by Hα(GONG), Lyα(SDI) and EUV(AIA) waves and a type-II radio burst(RSTN). The wave propagates along the southwestern direction with the velocity of 560-622 km/s, advancing sequentially in the order of EUV, Lyα, and Hα waves. The harmonic lane of the type II radio burst split into 3 lanes, which may correspond to the split of EUV wave observed in AIA 193 ˚A bagan at At 17:56:40UT. Using the density model of Vrˇsnak, we obtain the height of the shock wave in the range of 1.35 to 1.6 solar radii, with a radial velocity of about 100 km/s, which is closely consistent of the radial velocity of EUV waves. The fast component of the split wave is about 650 km/s and the slow is about 370 km/s. The magnetic field of the faster is closed while that of the slow wave is open according to the analysis of PFSS.
ST14-A001
The Structure of Coronal Mass Ejections Recorded by the K-coronagraph at Mauna Loa Solar Observatory
Hongqiang SONG#+
Shandong University, China
Previous survey studies reported that coronal mass ejections (CMEs) can exhibit various structures in white-light coronagraphs, and ~30% of them have the typical three-part feature in the high corona (e.g., 2-6 R⊙), which has been taken as the prototypical structure of CMEs. It is widely accepted that CMEs result from eruption of magnetic flux ropes (MFRs), and the three-part structure can be understood easily by means of the MFR eruption. It is interesting and significant to answer why only ~30% of CMEs have the three-part feature in previous studies. Here we conduct a synthesis of the CME structure in the field of view (FOV) of K-Coronagraph (1.05-3 R⊙). In total, 369 CMEs are observed from 2013 September to 2022 November. After inspecting the CMEs one by one through joint observations of the Atmospheric Imaging Assembly, K-Coronagraph, and LASCO/C2, we find 71 events according to the criteria: (1) limb event; (2) normal CME, i.e., angular width ≥30°; (3) K-Coronagraph caught the early eruption stage. All (or more than 90% considering several ambiguous events) of the 71 CMEs exhibit the three-part feature in the FOV of K-Coronagraph, while only 30%-40% have the feature in the C2 FOV (2-6 R⊙). For the first time, our studies show that 90%-100% and 30%-40% of normal CMEs possess the three-part structure in the low and high corona, respectively, which demonstrates that many CMEs can lose the three-part feature during their early evolutions, and strongly supports that most (if not all) CMEs have the MFR structures.
ST14-A003
Effects of Coronal Magnetic Field Configuration on Particle Acceleration and Release During the Ground Level Enhancement Events in Solar Cycle 24
Xiangliang KONG1#+, Wenlong LIU1, Fan GUO2, Lulu ZHAO3, Feiyu YU1, Zelong JIANG1, Yao CHEN1, Joseph GIACALONE4
1Shandong University, China, 2Los Alamos National Laboratory, United States, 3University of Michigan, United States, 4The University of Arizona, United States
Ground level enhancements (GLEs) are extreme solar energetic particle events that are of particular importance in space weather. In solar cycle 24, two GLEs were recorded on 2012 May 17 (GLE 71) and 2017 September 10 (GLE 72), respectively, using a range of advanced modern instruments. Here we conduct a comparative analysis of the two events by focusing on the effects of large-scale magnetic field configuration near active regions on particle acceleration and release. Although the active regions are both located near the western limb, temporal variations of SEP intensities and energy spectra measured in situ display different behaviors at early stages. By combining a potential field model, we find the CME in GLE 71 originated below the streamer belt, while in GLE 72 it originated near the edge of the streamer belt. We reconstruct the CME shock fronts with an ellipsoid model based on nearly simultaneous coronagraph images from multiple viewpoints and further derive the 3D shock geometry at the GLE onset. The highest-energy particles are primarily accelerated in the shock–streamer interaction regions, i.e., likely at the nose of the shock in GLE 71 and the eastern flank in GLE 72, due to quasi-perpendicular shock geometry and confinement of closed fields. Subsequently, they are released to the field lines connecting to near-Earth spacecraft when the shocks move through the streamer cusp region. This suggests that magnetic structures in the corona, especially shock–streamer interactions, may have played an important role in the acceleration and release of the highest-energy particles in the two events.
ST14-A009
Comparison of I-ICME and M-ICME Fittings and In Situ Observation Parameters for Solar Cycles 23 and 24 and Their Influence on Geoeffectiveness
Zhiyong ZHANG1+, Chenglong SHEN1#, Yutian CHI2, Dongwei MAO1, Zhihui ZHONG1, Junyan LIU1, Can WANG3
1University of Science and Technology of China, China, 2Deep Space Exploration Laboratory, China, 3China Earthquake Administration, China
To understand the weaker geomagnetic activity in Solar Cycle 24, we present comparisons of interplanetary coronal mass ejections (ICMEs) fittings and in situ observation parameters in Solar Cycles 23 and 24. According to their in situ features, ICMEs are separated into two categories: isolated ICMEs (I-ICMEs) and multiple ICMEs (M-ICMEs). The number of I-ICMEs in Solar Cycles 23 and 24 does not show a strong difference, while the number of M-ICMEs, which have a high probability of causing intense geomagnetic storms, declines proportionally to the sunspot number in Solar Cycle 24. Despite no obvious variation in their distribution, the geoeffective ICMEs in Solar Cycle 23 have a larger average total magnetic field strength and a larger southern magnetic field than those of Solar Cycle 24. Since the average solar wind velocities of the two solar cycles differ, the geoeffective ICMEs in Solar Cycle 23 have a higher velocity and distinct speed distributions from those in Solar Cycle 24. The total magnetic flux and radius of I-ICMEs in Solar Cycle 23 are larger than those in Solar Cycle 24, while the axial magnetic field intensity is basically the same. We propose that geomagnetic activity in Solar Cycle 24 is lower than that of Solar Cycle 23, due to the smaller M-ICME number, the slower ICME speed, and absence of ICME events with significant southward magnetic field.
ST14-A013
Comparison of the Composition of ICMEs from Active Regions and Quiet-sun Regions
Jinrong LI1+, Hongqiang SONG1#, Hui FU1, Leping LI2, Ruisheng ZHENG1, Yao CHEN1
1Shandong University, China, 2National Astronomical Observatories of China, China
The composition of interplanetary coronal mass ejections (ICMEs), including the ionic charge states and elemental abundances of heavy elements, is tightly correlated with their source regions and eruption processes. This can help in analyzing the eruption mechanisms and plasma origins of CMEs, and deepen our understanding of energetic solar activities. The active regions and quiet-Sun regions have different physical properties; thus, from a statistical point of view, ICMEs originating from the two types of regions should exhibit different compositional characteristics. To demonstrate the differences comprehensively, we conduct survey studies on the ionic charge states of five elements (Mg, Fe, Si, C, and O) and the relative abundances of six elements (Mg/O, Fe/O, Si/O, C/O, Ne/O, and He/O) within ICMEs from 1998 February to 2011 August using data from the Advanced Composition Explorer. The results show that ICMEs from active regions have higher ionic charge states and relative abundances than those from quiet-Sun regions. For the active-region ICMEs, we further analyze the relations between their composition and flare class, and find a positive relationship between them, i.e., the higher the classes of the associated flares, the larger the means of the ionic charge states and relative abundances (except the C/O) within ICMEs. As more (less) fractions of ICMEs originate from active regions around the solar maximum (minimum), and active-region ICMEs usually are associated with higher-class flares, our studies might answer why the composition of ICMEs measured near 1 au exhibits a solar cycle dependence.
ST14-A026
The Impulsive Acceleration of a Solar Filament Eruption Associated with a B-class Flare
Xuechao ZHANG#+, Hongqiang SONG, Yao CHEN
Shandong University, China
The eruption of magnetic flux ropes (MFRs), often taking filaments together, leads to coronal mass ejections (CMEs). Theoretical studies propose that both the resistive magnetic reconnection and the ideal instability of an MFR system can release magnetic-free energy and accelerate CMEs (i.e., MFRs or filaments) during eruptions. Observations find that the full kinematic evolution of CMEs usually undergoes three phases: the initiation phase, impulsive acceleration phase, and propagation phase. The impulsive acceleration phase often starts and ceases simultaneously with the flare onset time and peak time, respectively. This synchronization can be explained by the positive feedback relationship between the acceleration of CMEs and flare magnetic reconnection, and suggests that the reconnection has the dominant contribution to the acceleration of CMEs. It is rare to see strong evidence that supports the dominant contribution of ideal instability to the acceleration. In this presentation, we report an intriguing filament eruption that occurred on 2011 May 11. Its complete acceleration is well recorded by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory. The kinematic analysis shows that the impulsive acceleration phase starts and ceases obviously earlier than the flare onset time and peak time, respectively, which means a complete asynchronization between the impulsive acceleration phase and flare rise phase, and strongly supports that the ideal instability plays a dominant role in this impulsive acceleration. Furthermore, the accompanied flare is a B-class one, also implying that the contribution of reconnection is negligible in the energy release process.
ST14-A027
Comparison of Helium Abundance Within ICMEs from Active Regions and Quiet-sun Regions in Two Solar Cycles
Jinrong LI1#+, Chengxiao ZHANG1, Hongqiang SONG1, Leping LI2, Xuechao ZHANG1, Rui WANG1, Yao CHEN1
1Shandong University, China, 2National Astronomical Observatories of China, China
Helium is the second most abundant element within solar wind and interplanetary coronal mass ejections (ICMEs). The helium abundance (AHe) of ICMEs is closely related to their source regions and the eruption process of CMEs. ICMEs can originate from both active regions and quiet-Sun regions. The number of active regions varies throughout the solar cycle, and their physical characteristics are different from those of quiet-Sun regions. Therefore, it is expected that ICMEs from different regions possess different characteristics. In this presentation, we conduct a statistical comparison on AHe within ICMEs from these two types of regions based on ACE observations from 1998 to 2011. The results show that AHe within active-region ICMEs exhibit a solar cycle dependence and the mean value is higher than that of quiet-region ICMEs. In the meantime, we compare the ICME AHe in two solar cycles and find that AHe within active-region (quiet-region) ICMEs in solar cycle 23 is lower (higher) than that in solar cycle 24. Further, we find that AHe within ICMEs associated with X-class flare is higher than those associated with C-class flare. Our study might explain why AHe within ICMEs exhibits the solar cycle dependence at 1 au.
ST14-A029
Toward a Unified Explanation for the Three-part Structure of Solar Coronal Mass Ejections
Bing WANG#+, Hongqiang SONG
Shandong University, China
Coronal mass ejections (CMEs) are associated with the eruption of magnetic flux ropes (MFRs), which usually appear as hot channels in active regions and coronal cavities in quiet-Sun regions. CMEs often exhibit a classical three-part structure in the lower corona when imaged with white-light coronagraphs, including a bright front, dark cavity, and bright core. For several decades, the bright core and dark cavity have been regarded as the erupted prominence and MFR, respectively. However, recent studies have clearly demonstrated that both the prominence and hot-channel MFR can be observed as the CME core. The current research presents a three-part CME resulting from the eruption of a coronal prominence cavity on 2010 October 7, with observations from two vantage perspectives, i.e., edge-on from the Earth and face-on from the Solar Terrestrial Relations Observatory (STEREO). Our observations illustrate two important results: (1) for the first time, the erupting coronal cavity is recorded as a channel-like structure in the extreme-ultraviolet passband, analogous to the hot-channel morphology, and is dubbed as the warm channel; and (2) both the prominence and warm-channel MFR (coronal cavity) in the extreme-ultraviolet passbands evolve into the CME core in the white-light coronagraphs of STEREO-A. The results suggest that we are working toward a unified explanation for the three-part structure of CMEs, in which both prominences and MFRs (hot or warm channels) are responsible for the bright core.
ST14-A030
The Differences in the Origination and Properties of the Near-earth Solar Wind Between Solar Cycles 23 and 24
Xinzheng SHI#+
Shandong University, China
The dependence of the origination and properties of the near-earth solar wind on the solar cycle activities is an important issue in solar and space physics. We use the improved two-step mapping procedure to trace the near-Earth solar winds back to their source regions from 1999 to 2020. The statistical results demonstrate that the improved procedure can trace the solar wind back to its source region more accurately. Then the solar wind is categorized into coronal hole (CH), active (AR), and quiet Sun (QS) solar wind based on the source region types. We find that the origination and properties of near-earth solar wind are both influenced by the solar cycle activities. The proportions of CH and AR (QS) wind in the solar cycle (SC) 23 is higher (lower) than those in the solar cycle 24. During the solar maximum and declining phases, the magnetic field strength, speed, helium abundance (AHe), charge states of three types of solar wind during the SC 23 are all higher compared to those during SC 24. During the solar minimum, although the SSNs of the two cycles are close, the above parameters of solar wind are higher during SC 24 compared to those of SC 23. This means that the SC 23 minimum is extremely weak. The properties of the solar wind during the solar minimum may help to predict the activity of the next solar cycle. The statistical results demonstrate that the origination and properties of the solar wind are significantly influenced by solar cycle activities.
ST14-A032
The Observation of a High-turnover Frequency Flare with a Microwave Spectrometer Working in 35–40 GHz
Zhao WU#+
Shandong University, China
The microwave spectrum contains valuable information about solar flares. Yet, the present spectral coverage is far from complete and broad data gaps exist above 20 GHz. Here we report the first flare (the X2.2 flare on 2022 April 20) observation of the newly built Chashan Broadband Solar millimeter spectrometer (CBS) working from 35 to 40 GHz. We use the CBS data of the new Moon to calibrate, and the simultaneous NoRP data at 35 GHz to crosscalibrate. The impulsive stage has three local peaks with the middle one being the strongest and the maximum flux density reaches ∼9300 solar flux unit at 35–40 GHz. The spectral index of the CBS data (αC) for the major peak is mostly positive, indicating the gyrosynchrotron turnover frequency (νt) goes beyond 35–40 GHz. The frequency νt is smaller yet still larger than 20 GHz for most of the other two peaks according to the spectral fittings with NoRPCBS data. The CBS index manifests the general rapid-hardening-then-softening trend for each peak and gradual hardening during the decay stage, agreeing with the fitted optically thin spectral index (αtn) for νt < 35 GHz. In addition, the obtained turnover frequency (νt) during the whole impulsive stage correlates well with the corresponding intensity (It) according to a power-law dependence (It∝nt4.8) with a correlation coefficient of 0.82. This agrees with earlier studies on flares with low turnover frequency (≤17 GHz), yet it is being reported for the first time for events with a high turnover frequency (≥20 GHz).
ST14-A035
Excitation of Multi-periodic Kink Motions in Solar Flare Loops: Possible Application to Quasi-periodic Pulsations
Mijie SHI#+, Bo LI, Shao-Xia CHEN, Mingzhe GUO
Shandong University, China
Magnetohydrodynamic (MHD) waves are often invoked to interpret quasiperiodic pulsations (QPPs) in solar flares. We study the response of a straight flare loop to a kink-like velocity perturbation using three-dimensional MHD simulations and forward model the microwave emissions using the fast gyrosynchrotron code. Kink motions with two periodicities are simultaneously generated, with the long-period component (PL = 57 s) being attributed to the radial fundamental kink mode and the short-period component (PS = 5.8 s) to the first leaky kink mode. Forward modeling results show that the two-periodic oscillations are detectable in the microwave intensities for some lines of sight. Increasing the beam size to (1′′)2 does not wipe out the microwave oscillations. We propose that the first leaky kink mode is a promising candidate mechanism to account for short-period QPPs. Radio telescopes with high spatial resolutions can help distinguish between this new mechanism and such customary interpretations as sausage modes.
ST14-A038
A Novel 3-D CME Catalog Based on the CME Automatic Detection with a Transformer Model
Jiahui SHAN1, Lei LU1, Yan ZHANG2, Li FENG1#+
1Chinese Academy of Sciences, China, 2Nanjing University, China
Coronal mass ejections are major drivers of geomagnetic storms which may cause severe space weather effects. Automating the detection, tracking, and three-dimensional (3-D) reconstruction of CMEs is important for operational predictions of CME arrivals. The COR1 coronagraphs aboard the Solar-Terrestrial Relations Observatory (STEREO) spacecraft have facilitated extensive polarization observations which are very suitable for the establishment of a 3-D CME system. We have developed such a 3-D system comprising four modules: classification, segmentation, tracking, and 3-D reconstructions. We generalize our previously pretrained classification model to classify COR1 coronagraph images. Subsequently, as there are no publicly available CME segmentation datasets, we manually annotate the structural regions of CMEs using LASCO C2 observations. Leveraging Transformer-based models, we achieve state-of-the-art results in CME segmentation. Furthermore, we enhance the tracking algorithm to generate the first automatic 2-D CME catalog based on the COR1 data. In the final stage, we apply filter operations to obtain CME masks automatically, eliminating the need for manual masking. By applying the polarization ratio technique, we are able to reconstruct the 3-D structure of CMEs. The present method exhibits higher precision, superior generalization ability, and provides reliable physical parameters of CMEs. The aforementioned 3-D CME system can be applied to any coronagraph data with the capability of polarization measurements.
ST14-A040
Analysis of a Failed Filament Eruption Using ASO-S and Solar Orbiter/STIX
Zhengyuan TIAN1+, Li FENG1#, Jun CHEN2, Hui LI1, Ying LI1, Yang SU3, Yu HUANG1, Weiqun GAN1, Weilin TENG1
1Chinese Academy of Sciences, China, 2Nanjing University, China, 3Purple Mountain Observatory, Chinese Academy of Sciences, China
The analysis of the activity and energy during the precursor phase plays an important role in understanding the mechanism of flare eruption. Here we investigate an M1.1 flare on March 29, 2023, which was accompanied by a failed filament erupt. Interestingly, combining imaging and spectral data from the HXI (on board ASO-S) and STIX (on board Solar Orbiter), we found that the precursor phase of the event showed higher energy radiation (25-50keV) than the main phase (15-25keV). The LST on board the ASO-S observed this non-thermal precursor brightening at the Lyα waveband firstly, and STEREO A WAVES captured a Type III radio burst during the precursor phase, indicating the generation of high-speed electron beams during this period. Using the STIX energy data, the dynamic evolution of the double-corona source was observed in the impulsive phase, and the magnetic null point position of NLFFF extrapolated corresponded to them, which was consistent with the breakout model, indicating that the magnetic reconnection process of breakout might occur in the impulsive phase. The current sheets were observed at the same time, which could correspond to different stages of breakout model. The external magnetic flux is much larger than the internal magnetic flux, which may be one of the reasons for the failed filament eruption. In this study, by integrating the above observations and energy analysis, we have explored the reasons behind the failed eruption of the flare event and the high-energy response during the precursor phase.
ST14-A042
Unraveling the Mystery for Rare Imprints of “Solar Tsunamis”
Ze ZHONG#+, Yao CHEN
Shandong University, China
Over the last few decades, lots of EUV waves driven by coronal mass ejections (CMEs) have been observed, but their counterparts in the chromosphere were rarely detected. The infrequent imprints have remained an unresolved mystery. Here, to shed light on this problem, we investigate photospheric magnetograms of all events that generated EUV waves associated with Moreton waves. We find that all Moreton waves predominantly erupt from the edge of the active region. Potential field extrapolation reveals that their magnetic configurations exhibit an inclination in the source region. We choose two representative events, one generated a Moreton wave and the other not, and conduct data-driven MHD simulations for their eruptions. Major simulation results, such as the eruption trajectory of the CME, macroscopic morphology, match well with the observations. We compare two event types, examining magnetic configurations and the evolution of shock waves. The events that generate Moreton waves are notably hindered by the magnetic field above the main polarity, resulting in an inclined eruption path, possibly due to their locations at the edge of the active region. In contrast, events unable to generate Moreton waves generally occur in the central region of a bipolar field, yielding a quasi-radial eruption that cannot compress the chromosphere effectively.
ST14-A043
Three-dimensional Numerical Modeling of Hard X-Ray Sources in Solar Flares
Feiyu YU1#+, Xiangliang KONG1, Fan GUO2, Yao CHEN1, Ze ZHONG1
1Shandong University, China, 2Los Alamos National Laboratory, United States
During solar flares, a large number of electrons are accelerated to high energies. These accelerated energetic electrons subsequently propagate and precipitate, producing footpoint hard X-ray (HXR) sources in the chromosphere through the thick-target bremsstrahlung. For the first time, HXR instruments onboard Solar Orbiter and ASO-S enable the imaging of a solar flare from two different viewpoints, which potentially can reveal the 3D features of flare dynamics. In this work, by combining the data-driven 3D MHD simulation of a solar flare with the particle transport equation, we build a macroscopic particle model that naturally incorporates the acceleration and propagation of energetic electrons. We will show our latest results on numerical modeling of electron acceleration, transport and emission in solar flares, and direct comparison between modeling results and the observations.
ST14-A045
First Multi-view Observations of an Erupting Prominence in the UV Lyman-alpha Line with SolO/Metis and ASO-S/LST
Shuting LI1#+, Alessandro BEMPORAD2, Li FENG1, Beili YING1
1Chinese Academy of Sciences, China, 2INAF- Astrophysical Observatory of Turin, Italy
A prominence eruption associated with a limb CME were observed on April 12, 2023 by the multi-channel Metis Coronagraph on-board the Solar Orbiter mission. The prominence, seen in the Metis UV Lyman-alpha images as a very bright and elongated arch propagating southward, is instead much weaker in Metis visible light (VL) images. The elongated arch splits into several blobs and becomes fainter with time as the prominence evolves. In our work, we studied the 3D position of the prominence to understand the reason for such a significant difference between these two channels. By considering the different processes responsible for the emissions, we obtained the time evolution of the electron density and the temperature of one blob of the prominence from VL and UV images, respectively. The derived thermodynamic evolution suggests the existence of unknown physical processes providing additional heating source during the plasma expansion, as also previously found with observations acquired by the UVCS spectrometer on-board SOHO. We also applied the same method to another branch of the prominence to further understand the physical process inside the entire prominence. The Lyman-alpha Solar Telescope (LST) on-board the Advanced Space-based Solar Observatory (ASO-S) mission also observed this eruption along the Earth-Sun view. The solar disk imager (SDI) on-board the LST – observed the prominence lifting from the south-west solar limb, with the south leg fixed onto the Sun as the prominence expand. Another purpose of this work is to combine observations acquired by Metis and SDI to study the prominence from the Lyman-alpha emission. In particular, Carrington maps of chromospheric Lyman-alpha emission measured by SDI will be employed to constrain the radiative component of the Lyman-alpha emitted by the prominence plasma expanding through corona.
ST15-A008
Interaction of Relativistic Electrons with Finite-length Packets of the Electromagnetic Ion Cyclotron Waves: The Role of Nonlinear Effects
Veronika GRACH1, Andrei DEMEKHOV2,1#+
1Russian Academy of Sciences, Russian Federation, 2Polar Geophysical Institute, Russian Federation
We consider relativistic electron interaction with finite-length packets of electromagnetic ion-cyclotron (EMIC) waves in the Earth radiation belts. We study the dependence of the interaction characteristics on the wave packet length and amplitude analytically (in the linear regime) and by test-particle numerical modeling (for nonlinear regime). We calculate the fluxes of particles precipitating into the ionosphere as a result of the studied interaction. We show that in both linear regime and force bunching regime related to the direct influence of the Lorentz force on the electron phase a decrease in the wave packet length broadens the interaction region to lower energies beyond the range of resonant values for the central wave packet wave number. As for the nonlinear trapping and phase bunching, the energy ranges for these regimes are not extended to lower energies, i.e., these regimes are possible only for the resonant energies for the central wave number. For the EMIC wave amplitudes corresponding to nonlinear interaction, there exists an energy range in which the precipitating electron flux is equal to or even slightly exceeds the limiting flux corresponding to the strong diffusion. The maximum (over energies) precipitating to trapped flux ratio is about unity and does not depend on the wave packet amplitude and length for sufficiently high wave amplitudes. The minimum energy for which significant precipitation occurs reaches about one half of the minimum resonant energy for the central wave number. These energies are about first hundreds of keV for the Earth magnetosphere. This work was supported by the Russian Science Foundation: projects no. 19-72-10111 (V.S. Grach, derivation of analytical expressions, numerical simulations, comparison of the analytical and numerical results) and 22-62-00048 (A.G. Demekhov, formulation of the problem, analysis of the results).
ST15-A010
High-frequency EMIC Waves: A Comprehensive Analysis of Instability Threshold and Nonlinear Evolution
Kyungguk MIN#+
Chungnam National University, Korea, South
Narrowband (∆f < 0.1 fcp), high-frequency (0.9 fcp < f < fcp) electromagnetic ion cyclotron (EMIC) waves, or HFEMIC waves for short, are a new type of EMIC waves. They are believed to be excited by low energy (< ~100 eV), very anisotropic protons which are quite prevalent during both quiet and active geomagnetic conditions. Here, we explore the instability threshold condition and nonlinear saturation of HFEMIC waves. Linear theory analysis at parallel propagation shows that the anisotropy-parallel beta relation at instability threshold approximately follows an inverse relation like the one for typical H-band EMIC waves. Unlike typical EMIC waves, however, the minimum temperature anisotropy required is very large (> 10), the convective growth rate at a fixed instability threshold is large because of small group velocity of HFEMIC waves, and heavy ions affect the instability only weakly, primarily through the introduction of stop bands. To investigate the nonlinear behavior, one-dimensional hybrid simulations are run assuming a dipole-like background magnetic field and with initial parameters constrained by observation. Despite a narrow source region (within about ±3◦ latitude due to a large anisotropy required for HFEMIC instability), HFEMIC waves in simulations can grow well above the thermal noise level, thanks to a small group velocity of HFEMIC waves at the equatorial source region. The saturation level is well within the range of observational amplitudes, and the wave evolution is primarily determined by the quasilinear process. We demonstrate that the present results compare favorably to the recent observational findings, thereby supporting anisotropic low-energy protons as free energy source for HFEMIC waves.
ST16-A013
What Can We Learn About the Strong Thermal Emission Velocity Enhancement (STEVE) as a Turbulent Phenomena?
Francesca DI MARE1,2#+, Elizabeth MACDONALD2, Michael HUNNEKUHL3, Laura BRANDT EDSON4,2
1The Catholic University of America/ NASA GSFC, United States, 2NASA Goddard Space Flight Center, United States, 3Independent Researcher, Germany, 4New Mexico Consortium, United States
The rapidly growing collaborations between scientists and participatory scientists, including the Aurorasaurus project, have unveiled the STEVE (Strong Thermal Emission Velocity Enhancement) phenomenon, an excellent candidate for a cutting-edge study of complex turbulent dynamics within the ionosphere. Unlike typical auroral precipitation, the STEVE phenomenon is associated with very high flows, structuring at multiple scales, and characteristic but understudied intermittency. Recent observations allow comparisons between the complex visible dynamics and microphysics of these differing regions. Plasma parameters and the evolution of Alfvén waves are studied through joint analysis of participatory science and spacecraft data. The nature of Alfvén waves plays a key role in the Magnetosphere-Ionosphere (M-I) interaction, in which kinetic energy is deposited through the precipitation of energetic particles and electromagnetic energy is dissipated. The focus of the research is the characterization of the evolution scales in which the main phenomenon STEVE and secondarily the associated green picket fence develops via the conjunction of the observations and the spacecraft passages of the SWARM and DMSP missions.
ST17-A001
Identification of Coronal Holes from Open Magnetic Field Regions Using Artificial Neural Network
Chia-Hsien LIN#+, Guan-Han HUANG
National Central University, Taiwan
Coronal holes are primary source regions of high-speed solar wind streams, which can have significant impact on Earth and the entire heliosphere. Therefore, accurate identification of coronal holes is important. They can be identified either as the darkest coronal regions with predominantly unipolar magnetic fields in observational images or as the regions with “open” magnetic field (OMF) lines, i.e., field lines extending to far away, in solar magnetic field models. In this study, the former definition is referred to as coronal holes (CHs) and the latter as OMF regions. While the two definitions are often considered as statistically related, studies have found non-negligible inconsistency between CHs and OMF regions, which can lead to ambiguity in the study of large-scale solar magnetic fields and inaccurate predictions of high-speed solar wind. The inconsistency can be due to OMF regions with high coronal emissions or CHs without open magnetic field lines. The objective of this work is to develop an Artificial Neural Network (ANN) model to identify the OMF regions that are consistent with CHs. The OMF regions and CHs are first determined from a realistic thermal magnetohydrodynamic model produced by Predictive Science, and the consistency level between the two is found to be 0.33. An Artificial Neural Network (ANN) model is then constructed and trained to predict the OMF regions consistent with CHs using eight quantities: magnetic field intensity, magnetic field expansion factor, thermal pressure, electron temperature, electron number density, mass density, and local coronal heating rate. The results show that the consistency level is improved by the model from 0.33 to 0.81.
ST17-A010
Phase Mixed Alfven Waves in Partially Ionised Solar Plasmas
Max MCMURDO#+, Istvan BALLAI, Gary VERTH, Viktor FEDUN
The University of Sheffield, United Kingdom
Phase mixing of Alfven waves is one of the most promising mechanisms for heating the solar atmosphere. The damping of waves in this case requires small transversal scales, relative to the magnetic field direction. Here this requirement is achieved by considering a transversal inhomogeneity in the equilibrium plasma density profile. Using a vertically stratified single fluid partially ionized plasma, we study the effectiveness of damping phase mixed shear Alfven waves and investigate the effect of varying the frequency of the driver and driver type. Our results show that the dissipation rate of shear Alfven waves strongly depends on the local ionization degree of the plasma. More importantly, in a partially ionized plasma, the damping rates of shear Alfven waves are several orders of magnitude larger than in the case of fully ionized plasma, providing evidence that phase mixing could be a large contributor to heating the lower solar atmosphere. The effectiveness of phase mixing is investigated for various drivers and we demonstrate that the damping of phase-mixed shear Alfven waves can provide sufficient heating to balance chromospheric radiative losses in the quiet Sun.
ST19-A001
Multi-instruments Observation of Ionospheric-thermospheric Dynamic Coupling Over Mohe (53.5°N, 122.3°E) During the April 2023 Geomagnetic Storm
Wenbo LI+, Libo LIU#, Yiding CHEN, Yuyan YANG, Tingwei HAN, Feng DING, Huijun LE, Ruilong ZHANG
Chinese Academy of Sciences, China
The variations of the Ionosphere-Thermosphere (I-T) system are strongly influenced by dynamical processes, with these effects being amplified during intense space environment disturbances such as geomagnetic storms, leading to multi-scale disturbance features in the I-T system. To comprehensively understand the influence of dynamic processes, it is necessary to have continuous and simultaneous observations of both the ionosphere and thermosphere. However, the scarcity of thermospheric observation presents a notable obstacle in advancing our understanding of dynamic processes. This work examines the responses of the I-T system during the April 2023 geomagnetic storm based on high-resolution continuous I-T system observations at Mohe observatory, a middle latitude station. Our observations identified both large-scale features and short-period oscillations within various key I-T parameters of the I-T system. Similar disturbed patterns in neutral winds occurred during the main and recovery phases of the geomagnetic storm. However, the oscillation features in many parameters of the I-T system are only observed during the main phase. The results of concurrent I-T system observations unveil the oscillation features of thermospheric winds, temperatures, the ionospheric F2 peak height, electron density, and total electron content, and provide a perspective for studying the influence of dynamic processes. These findings reveal the important influence of wind divergence on thermospheric temperature disturbances and its modulatory effect on ionospheric disturbances.
ST19-A005
A Unique Structure of the Ionospheric Current Over the Asian-Oceania Region Determined by the Combination of the Ground-based and Space-borne Magnetometers
Pengyu ZHANG+, Yang-Yi SUN#
China University of Geosciences, China
The ionosphere owns a complex electric current system mainly driven by the ionospheric electric field and thermospheric wind. Changes in current can generate geomagnetic signals that can be observed both on the ground and in space. In this study, we analyzed the ionospheric current in the Asia-Oceania region by utilizing geomagnetic data collected from magnetometers of ground-based observatories and SWARM satellites at ~450 km altitude. The results present the geomagnetic variations at the two distinct altitudes, encompassing longitudinal, latitudinal, and seasonal variations. Furthermore, the Ionosphere-Electrodynamics General Circulation Model (TIE-GCM) was employed to simulate the associated geomagnetic signals. This study is the first to combine dense geomagnetic data from multiple altitudes and simulations to understand the ionospheric current in the Asia-Oceania region. The differences between the observational geomagnetic signals at different altitudes, along with the simulations, reveal a unique current structure that has not been previously discovered. The findings provide a new understanding of the intricate evolution of the current systems, which contributes to our knowledge of the electric dynamics within Earth's ionosphere.
ST19-A007
Numerical Simulation of Acoustic-gravity Waves Generated by Lithospheric Activities
Ziniu XU#+, Yang-Yi SUN, Lin KAI
China University of Geosciences, China
Numerous studies reported widespread vibrations triggered by lithospheric activates can generate atmospheric acoustic-gravity waves and disturbances, leading to changes in the middle and upper layers of the atmosphere. In this study, we initiated an investigation by exploring the atmospheric dynamics equations in cylindrical symmetric coordinates. We derived analytical solutions for the wave equations, and investigating the evolution of atmospheric waves or disturbances through numerical simulations. Additionally, we introduce a novel theoretical coupling model, successfully showcasing the fundamental concept of Earth's sphere coupling.
ST21-A010
Multi-scale Wave Activities During the Magnetotail Flapping Associated with Electron-only and Ion Reconnections
Kyunghwan DOKGO#+, Kyoung-Joo HWANG, James BURCH, Eunjin CHOI
Southwest Research Institute, United States
Magnetotail flapping refers to the vertical up-and-down motion of the nightside current sheet. Due to its typical propagation along the dawn/dusk direction, the flapping can be a crucial ingredient in the communication between the central plasma sheet and the flank magnetopause. On July 17, 2017, the MMS spacecraft observed various wave activities during a flapping motion of the magnetotail. The initiation of the flapping was accompanied by electron-only reconnection, which evolved to regular ion reconnection with time. The flapping led MMS to repeatedly cross the northern and southern-side separatrix regions, where multiple wave activities were detected, including lower-hybrid waves (LHW), electron cyclotron waves (ECW), Langmuir waves (LW), and broadband electrostatic waves (ESW). High-time resolution MMS data enabled to resolve highly correlated LHW, ECW, and LW in the separatrix region, where lower frequency waves provide favorable conditions for the growth of higher frequency waves. Our findings indicate how these wave activities are associated with the temporal evolution of reconnection, providing new insights into the cross-scale processes from the global scale dynamics to the microscale kinetics and associated energy transfer via waves.
ST22-A007
Prediction of Solar Magnetic Synoptic Maps
Rui ZHUO1#+, Jiansen HE1, Die DUAN2, Ziqi WU1
1Peking University, China, 2National University of Defense Technology, China
The evolution of solar magnetic fields is significant for understanding and predicting solar activities. And our knowledge of solar magnetic fields largely depends on the photospheric magnetic field. Based on the spherical harmonic expansion of the photospheric magnetic field observed by Wilcox Solar Observatory, we analyze the time series of spherical harmonic coefficients and predict synoptic maps for Solar Cycle 25. We find that solar maximum year shave complex short-period disturbances, and the time series of coefficient g_0^7 is nearly in-phase with Sunspot Number, which may be related to solar meridional circulation. By incorporating Long Short-Term Memory networks (LSTM) with Empirical Mode Decomposition (EMD), we perform our forecast of synoptic maps truncated to Order 5, validating their relative reliability. This prediction not only addresses a gap in forecasting the global distribution of the solar magnetic field but also holds potential reference value for forthcoming solar observation plans.
ST22-A009
Origin and Evolution of Solar Wind from Solar Surface to 1 Au During the Solar Orbiter-earth Radial Alignment
Chuanpeng HOU1+, Jiansen HE1#, Alexis ROUILLARD2, Chuan LI3, Shihao RAO3, Xiangjing XU1, Ziqi WU1
1Peking University, China, 2Institute for Research in Astrophysics and Planetology/ Université Toulouse III—Paul Sabatier/ National Center for Scientific Research/ National Center for Space Studies, France, 3Nanjing University, China
The radial alignment between Solar Orbiter and Earth is utilized to investigate the origin and evolution of the solar wind. Employing a two-step backtracking method, we find that the solar wind detected by Solar Orbiter and Wind originated from the same solar source region during this period. Through multi-waveband imaging from the Solar Dynamics Observatory (SDO) and Chinese Hα Solar Explorer (CHASE) spacecraft, we obtained information about solar activities and chromospheric Doppler velocity distribution in the source region. The overall blue-shift velocity in the source region seems to be positively correlated with the interplanetary solar wind speed, with this correlation being particularly evident during the transition from interplanetary low-speed flow to high-speed flow. For the evolution of the solar wind, we compared the magnetic field, proton, and Alpha moments in the solar wind detected by Solar Orbiter and Wind. The results indicate that the solar wind measured by Solar Orbiter at a heliocentric distance of 0.4 Rs includes stronger velocity pulses compared to the solar wind measured by Wind, where the pulses are no longer pronounced. We compared the abundance of alpha particles inside and outside the pulses and speculated that, although both the pulses and the background solar wind originate from the same solar source region, the detailed physical processes leading to their formation could be different. Additionally, we compared differences in solar wind turbulence at multiple heliocentric distances.
ST22-A010
Inspecting Transient Processes in the Young Solar Wind Through Imaging and Probing Technique by Parker Solar Probe
Ziqi WU1#+, Jiansen HE1, Die DUAN2, Chuanpeng HOU1, Rui ZHUO1, Xingyu ZHU3, Zheng SUN1
1Peking University, China, 2National University of Defense Technology, China, 3The University of Alabama in Huntsville, United States
Parker Solar Probe revealed that the near-sun pristine solar wind is highly intermittent, full of structures from macro to microscales. The Wide-field Imager for Parker Solar Probe (WISPR) finds that the coronal rays are multi-layered and dynamic, with blob-like structures continuously flowing along. Flythroughs of near-sun heliospheric current sheets often record extended crossings of reconnection exhausts and encounter regions with high density and speed. To combine PSP's remote sensing and in-situ measurements, we develop a novel ``See and Touch" technique and apply it to PSP's 8th encounter. We identify these blobs and high-density jets as counterparts and investigate these structures from macro to microscales. We find that distant quasi-steady reconnections (at 3-4Rs) possibly generate the blobs/HDJs, while local intermittent reconnections generate minute-scale substructures such as magnetic flux ropes and smaller-scale jets. The local velocity profile indicates that the blobs undergo stretching during its radial evolution. In the kinetic scale, the proton VDF is more Maxwellian-like inside the HDJs, which suggests that the core components are possibly accelerated and merged with the beam components.
ST23-A008
Fifty-year Investigation of the Correlation Between the Geomagnetic Field and Climate
Yuqi WANG+, Yong WEI#
Chinese Academy of Sciences, China
After 50 years of research on the correlation between the geomagnetic field and climate, we have gained a deeper understanding that the regulation of climate by geomagnetic field changes is far more complex than previously imagined. In this paper, we comprehensively review the research connecting the geomagnetic field and climate over the past 50 years, examining different spatial and temporal scales. Our results demonstrate a significant correlation between geomagnetic field changes and climate at various scales, including millennial-scale geomagnetic reversals, thousand-year-scale geomagnetic shifts, centennial-scale geomagnetic abrupt, and even decadal-scale variations in geomagnetic activity. However, it's important to note that correlation does not imply causation, and the potential mechanisms by which the geomagnetic field influences climate change are still a subject of debate. The cosmic ray-cloud mechanism is the most promising avenue for understanding how the geomagnetic field regulates climate, operating effectively across different time scales, but its exact physical mechanisms and relative importance remain unresolved issues. We propose that understanding the correlation between the geomagnetic field and climate from the perspective of solar-terrestrial multisphere coupling is crucial, with a specific focus on the response of regional climate systems to changes in regional magnetic fields. By integrating knowledge from ancient times to the present, from regional to global perspectives, we aim to form a comprehensive understanding of the correlation between the geomagnetic field and climate change. The recent successful launch of Aoke-1, which can delicately characterize magnetic field changes in the South Atlantic anomaly (SAA), the first discovery of the centennial-scale Western Pacific Anomaly (WPA), and the rapid development of paleomagnetic/archaeomagnetic and paleoclimate data reconstruction have provided new historical opportunities for research on the geomagnetic field and climate. This progress indicates that the study of the impact of geomagnetic field changes on climate will be propelled to new heights.
ST23-A016
Investigation of Local Geomagnetic Variations in Taiwan from 1965 to 2023
Huei-Wen SIAO1#+, I-Te LEE2,3, Chih-Hsuan LI3, Jia-Sin KUO3
1Central Weather Administration, Taiwan, 2Taiwan Space Agency, Taiwan, 3National Central University, Taiwan
Earth’s magnetic field results from the superposition of signals originating from various sources. The most significant variations stem from geomagnetic storms, which are major disturbances in Earth's magnetosphere attributed to a very efficient exchange of energy from the solar wind into the space environment surrounding Earth. In addition to geomagnetic storms, the ground-based measurements occasionally exhibit smooth variations depending on local time, typically in the order of a few tens of nanoteslas (nT). This phenomenon is caused by Solar quiet (Sq) current, a type of electric current flowing in the sunlit side of the ionosphere. Although Sq current rise up a relatively small amplitude of geomagnetic field than storms and substorms, typically in the order of several hundreds of nT on the ground, studies on Sq current have been important for advancing our understanding the ionospheric electrodynamics and monitoring the local space weather conditions. This study undertook a comprehensive review of local geomagnetic field variations in Taiwan from 1965 to 2023, covering solar cycle 20 to 25 (1964-2023). The recorded data between July 1965 and December 2000 was measured by Lunping Observatory (LNP, 25.0N, 121.17E), located at approximately 14° north of the magnetic equator. Especially, this study involved the digitization of booklets containing the original geomagnetic field records from July 1965 to December 1993. The data for the past decade was obtained from the geomagnetic observatories of Taiwan Geophysical Networks for Seismology (TGNS), Central Weather Administration (CWA). These records provide a more extensive chronological coverage compared to the archived data available from the World Data Center (WDC) for Geomagnetism. This study aims to retrieve possible local geomagnetic influences in the past, and serves as a reference for evaluating the local impact of space weather in the future.
ST24-A002
Numerical Study of the Solar-Mars CME Event on December 4, 2021
Mengxuan MA1#+, Chenglong SHEN2, Fang SHEN1, Li-Ping YANG1
1Chinese Academy of Sciences, China, 2University of Science and Technology of China, China
Coronal Mass Ejection (CME) is one of the most severe phenomena in the solar atmosphere and a significant driving factor for various space weather disturbances. On December 4, 2021, a fast coronal mass ejection event occurred on the far side of the Sun, which was detected by the Bepi-Colombo probe when it reached 0.6 AU on December 6. On December 10, the CME arrived at the orbit of Mars, and both Tianwen-1 and MAVEN spacecraft observed this CME event. In this study, a three-dimensional MHD background solar wind model was combined with a spheromak CME model to simulate the three-dimensional morphology and propagation process of the above-mentioned CME event from the Sun to Mars. The shape of the CME observed by STEREO/SECCHI and SOHO/LASCO was reconstructed using the GCS method, and the initial position, velocity, and other parameters of the spheromak CME model were determined. By constraining the numerical simulation with magnetic maps observed by GONG, the morphology and position of the CME observed in white light were reproduced, and the structure and arrival time of the CME close to local detectors at 0.6 AU and 1.6 AU were obtained. In this study, by calculating the subnormal vector of the CME's magnetic field lines, the orientation of the magnetic flux ropeaxis of the CME was determined, revealing a significant rotation of the CME during its propagation. It is speculated that this rotation is caused by the asymmetric deceleration of the CME's western side compared to the eastern side due to the influence of the background solar wind, resulting in a rotational motion from east to west. In future research, we will further explore the factors that influence CME rotation and investigate additional possibilities for CME attitude changes.
ST24-A006
Coronal Hole Detection and Tracking with Machine Learning Methods
Junyan LIU1#+, Chenglong SHEN1, Yutian CHI2, Dongwei MAO1, Zhihui ZHONG1, Zhiyong ZHANG1, Luo JINGYU1, Can WANG3
1University of Science and Technology of China, China, 2Deep Space Exploration Laboratory, China, 3China Earthquake Administration, China
With the help of several different machine methods, we successfully detected and tracked the coronal hole region of extreme ultraviolet(EUV) 195-angstrom wavelength from the SDO satellite. Afterward, a catalog of the Coronal Holes(CHs) during the period from 2010 to 2022 was established. Our catalog tracks the detailed evolution characteristics of different coronal holes with a time accuracy of 12 hours. Based on this catalog, we found that the zonal coronal hole rotation rates are different from the differential rotation rates observed from the photosphere. The coronal hole rotation rates at different latitudes are almost the same. However, the meridional velocities of coronal holes are in good agreement with the solar meridional circulation. Besides, we also noticed a north-south asymmetry in the distribution, area, flux, and velocity of coronal holes. This asymmetry can be partly explained by some solar dynamo models and may help us to analyze the formation mechanism of coronal holes.
ST24-A009
Deploying a Deep Learning Model for Solar Flare Irradiance Translation
Sung-Hong PARK1#+, Junmu YOUN2, Seungwoo AHN2, Jeong-Heon KIM1, Kangwoo YI2
1Korea Astronomy and Space Science Institute, Korea, South, 2Kyung Hee University, Korea, South
Solar flares emit intense bursts of electromagnetic radiation in the solar atmosphere at all wavelengths, from radio waves to gamma rays. When large flares occur in the solar front disk as seen from the Earth, their earthward electromagnetic radiation, particularly ultraviolet (UV) and X-ray, can significantly impact the conditions of the Earth’s ionosphere and upper atmosphere. In this respect, it is crucial to better understand the characteristics of both UV and X-ray emissions from flares. We therefore developed a deep learning model that can generate irradiance in UV channels from X-ray, using a time series dataset of: (1) soft X-ray irradiance, as input, measured between 0.1 and 0.8 nm by the Geostationary Operational Environmental Satellites (GOES), and (2) UV irradiance, as output, for flare emission lines within a wavelength range of ~10 to 100 nm observed by the Extreme ultraviolet Variability Experiment (EVE) onboard the Solar Dynamics Observatory (SDO). Here we will present the details of the model development, performance and its science applications.
ST24-A012
CLEAR – All-clear Sep Forecast: A NASA Space Weather Center of Excellence
Lulu ZHAO#+, Tamas GOMBOSI
University of Michigan, United States
CLEAR will deliver capabilities for robust and quantifiable forecasts of the space radiation level of up to 24 hours, in support of aviation, satellites, and space exploration. Solar energetic particles (SEPs) can be accelerated over a wide range of energies extending up to GeVs. At relatively low energies (e.g., ~10 MeV), their flux intensity can exceed the background of galactic cosmic rays by several orders of magnitude. Protons of >100 MeV with elevated fluxes exceeding 1 proton flux unit are responsible for an increased astronaut exposure inside spacecraft shielding. Protons of >150MeV are very difficult to shield against as they can penetrate 20 gm cm (7.4 cm of Al, or 15.5 cm of water/human tissue). Furthermore, > 500 MeV protons can penetrate the atmosphere and pose radiation hazards to aviation. Besides protons, energetic heavy ions, e.g., Fe ions, can be of more severe radiation concerns. SEPs are hazardous not only to humans but also to electronics and other sensitive components in space, affecting satellite operations. The sparsity and high variability in terms of intensity, duration, composition, and energy spectra of SEP events make them difficult to predict. The CLEAR Center will develop, test and validate a self-contained, modular (“plug and play”) framework that includes all major elements impacting SEPs in the inner heliosphere: 4π maps of photospheric magnetic fields, corona (1 − 20Rs), inner and middle heliosphere (0.1 AU to Jupiter’s orbit) plasma environment, magnetic connectivity with respect to the solar source, flare/CME initiation, SEP seed population, flare and shock acceleration, and energetic particle transport. In addition, the framework will be able to accommodate radiation interaction models, which will be used to study the penetration of spacecraft walls, radiation effects on the terrestrial magnetosphere, and the radiation doses received by human tissues.
ST24-A013
An Attempt to Predict Sunspot Number Using Transformers
Gilbert PI1#+, Tsung-Che TSAI2, Jana SAFRANKOVA1, Zdenek NĚMEČEK1
1Charles University, Czech Republic, 2National Center for High-Performance Computing, Taiwan
Solar activity is a crucial factor in space weather. It follows an 11-year cycle, and previous studies have relied on historical records of sunspot numbers to predict the following cycle. Machine learning techniques such as Long Short-Term Memory (LSTM) have also been used to make these predictions and provide a reasonable result. Recently, the application of transformers has been rising and majorly replacing the LSTM in Natural Language Processing. However, the Transformers is not widely used in space weather prediction yet. In this study, we are introducing the transformers method to improve the sunspot number prediction. Numerous approaches are used to find the optimal prediction and compare it with previous results.
ST24-A015
Integrating Ionospheric Data Assimilation and Deep Learning for Three-dimensional Global Ionosphere Prediction
Chalachew Kindie MENGIST#+, Kyong-Hwan SEO
Pusan National University, Korea, South
Using the Ionospheric Data Assimilation Four-Dimensional (IDA4D) algorithm, a global three-dimensional electron density is reconstructed by assimilating ground-based GPS slant total electron content (STEC), radio occultation STEC, and radio occultation NmF2 data into the IRI model. The IDA4D outputs are fed into Convolutional Neural Networks (CNNs) to learn spatiotemporal patterns. Results are validated with ionosonde and CODE TEC data, demonstrating significant improvements. The approach reduces the root-mean-square error (RMSE) of Nmf2 and vertical TEC by 34% and 51%, respectively, compared to the IRI model. Furthermore, the IDA4D technique successfully reconstructs storm-time enhancement of the northern crest equatorial ionization anomaly during late evening hours, resulting from upward and northward plasma transport. The combination of IDA4D and CNNs predicts a three-dimensional electron density more accurately than the IRI model for up to two days.
ST24-A016
Fast Reconstruction of 3D Coronal Magnetic Fields in Various Solar Active Regions Using a Deep Learning Model
Jihye KANG#+, Hyun-Jin JEONG, Yong-Jae MOON
Kyung Hee University, Korea, South
The reconstruction of the 3D coronal magnetic field is essential for understanding magnetic structure that generate solar phenomena. However, numerical models to reconstruct the 3D coronal magnetic field are computationally time-consuming and they have also limitations in handling various solar active regions. Here, we use a deep learning model based on pix2pixHD algorithm to fast reconstruct the 3D coronal magnetic field in various solar active regions. We consider photospheric vector magnetic fields as input and 3D nonlinear force-free field (NLFFF) data from ISEE NLFFF database as output in 203 active regions. The training and evaluation of our model involve a total 2263 input and output data pairs, with 1584 pairs for training and 679 pairs for evaluation. The results show that the configurations of AI-generated magnetic polarities are similar to the original NLFFF ones. And we also discuss physical parameters and 3D magnetic structures calculated as model results in various active regions.
ST24-A021
Flare Forecasting Modeling Use Solar Full-disk Magnetic Field Event Streaming Dataset and Spiking Neural Network
Xinze ZHANG+, Zhongrui ZHAO, Long XU#, Xin HUANG
Chinese Academy of Sciences, China
Flare prediction is closely related to time, and currently, in the field of deep learning, spiking neural networks theoretically have advantages in handling time perspectives. However, they require a specific format of event stream dataset. Based on this, we constructed a full-disk magnetic field event stream dataset. We utilized this dataset for the temporal information prediction of solar flares. As spiking neural networks are still in the development stage, we look forward to more researchers conducting further studies based on our dataset and basic model.
ST24-A022
Flare Forecasting Modeling Use Three-dimensional Magnetic Fields
Zhongrui ZHAO+, Xinze ZHANG, Long XU, Xin HUANG#
Chinese Academy of Sciences, China
Due to limitations in observation techniques and theories, there are currently no mature three-dimensional observational data, solar flare forecasting mainly relies on one-dimensional (eg. soft X-ray flux) or two-dimensional data (eg. 2D magnetic field). Prior to this, we constructed a large-scale three-dimensional vector magnetic field dataset using nonlinear force-free magnetic field (NLFFF) extrapolation. In this work, we compared the similarities and differences between two-dimensional modeling and three-dimensional modeling using this dataset and explored the impact of vector magnetic fields on solar flare forecasting modeling.
ST26-A007
Impact of the Radio Occultation Retrieval on the Electron Density Profiles by the Equatorial Plasma Bubbles
Shih-Ping CHEN#+, Charles LIN, P. K. RAJESH
National Cheng Kung University, Taiwan
The rapid revisit period of the FORMOSAT-7/COSMIC-2 (F7C2) significantly enhances the temporal resolution of ionosphere monitoring in low latitudes. While having this advantage, the quality of electron density profiles (EDPs) is also crucial for applications such as data assimilation. On January 15th in 2023, more than 70% of the F7C2 EDPs from the Pacific to the Indian Ocean exhibited significant fluctuations following the major eruption of Hunga Tonga-Hunga Ha'apai. Similarly, these fluctuating EDPs are also commonly observed in daily RO observations, leading to a series of inaccuracies in data assimilations. This study presents, for the first time, a comprehensive investigation into the climatology of these fluctuating abnormal EDPs. The results suggest that these EDPs primarily occur during nighttime, and the fluctuation intensity depends on the alignment between RO links and the equatorial plasma bubbles (EPBs). The Bagged Trees (Random Forest) algorithm is utilized to classify normal and abnormal EDPs across varying times, days, locations, and solar activity levels. The developed algorithm detects EDPs affected by the EPBs as well as daytime irregularities. Climatology statistical results also illustrate monthly and longitudinal variations in the F7C2 EDP qualities that are independent of the EPB occurrences. The findings indicate that the machine learning algorithm is valuable for identifying or flagging poor-quality EDPs, enhancing the performance of data applications.
ST27-A005
Development of a GPU-accelerated Magnetohydrodynamic Code: OpenMHD-GPU
Seiji ZENITANI#+
Austrian Academy of Sciences, Austria
We have been developing an open-source magnetohydrodynamic code, OpenMHD [1]. It is a second-order multi-dimensional finite-volume code with the HLLD Riemann solver. Its CPU modules are parallelized with MPI-3 and OpenMP. The code was originally developed for our studies on magnetic reconnection, and then it has been made publicly available since 2010. As of 2024, more than ten papers were published by the users. In this contribution, we will present recent technical advances in OpenMHD. The code extensively takes advantage of NVIDIA’s graphics processing units (GPUs). The computing modules have been fully ported to GPUs with CUDA Fortran language. This made our simulations orders-of-magnitude faster than before. Thanks to OpenMHD-GPU, we can carry out medium-size simulations on public clouds such as Google Colaboratory. In addition, we have developed an advanced communication module, which uses MPI shared-memory (MPISHM) for intranode communication. This may be useful for multinode CPU/GPU systems. We also found GPUs useful for post-processing simulation data. As an example, we will show a simple shock finder, based on GPU-accelerated image-processing methods. [1] https://sci.nao.ac.jp/MEMBER/zenitani/openmhd-e.html.
ST27-A009
NASA's Geospace Dynamics Constellation Mission
Douglas ROWLAND1#+, Larry KEPKO2, Katherine GARCIA-SAGE1
1NASA Goddard Space Flight Center, United States, 2National Aeronautics and Space Administration, United States
The Geospace Dynamics Constellation (GDC) is NASA's next strategic Living With a Star mission. GDC's goals are: 1) Understand how the high-latitude ionosphere-thermosphere system responds to variable solar wind/magnetosphere forcing; and 2) Understand how internal processes in the global ionosphere-thermosphere system redistribute mass, momentum, and energy. Planned for launch in the early 2030s, GDC will use six identical observatories, each identically instrumented to fully characterize the magnetospheric drivers of the I-T system as well as the global response of the ionized and neutral gases. GDC will do this with a series of orbital configurations that will enable it to study the widest range of spatial and temporal scales to date, ranging from hundreds of kilometers and several seconds to tens of minutes, and extending through the regional to the global scale. This poster presents GDC's current status, measurement capabilities, sampling scheme, and model development efforts and show how GDC will et into the larger Heliophysics ecosystem, by 1) obtaining critically needed scientific observations; 2) providing a source for real-time space weather and situational awareness, as well as retrospective studies to further the science of space weather; 3) serving as a "strategic hub" for other space-based and ground- based efforts that want to leverage GDC to perform complementary science.
ST27-A012
A New Source of Global Electric Field in the Magnetosphere: Lunar Tide Electric Field
Quanqi SHI#+, Chao XIAO
Shandong University, China
The electric field plays important role in the Earth's magnetosphere dynamics. Traditionally recognized in global scale are the convection electric field and the corotation electric field. However, recent investigations utilizing electric field data from the Van Allen Probe satellite have revealed the existence of a previously unrecognized third global electric field, identified as the lunar tide electric field. This electric field can be described in an analytical model. Furthermore, the impact of the lunar tide electric field on the magnetosphere is examined through a comprehensive analysis of particle distribution. In essence, this discovery holds significant importance for our understanding of the Moon's impact on the Earth's magnetosphere.
ST27-A014
Solar Radio Burst Observation with KSRBL: Korean Solar Radio Burst Locator
Sujin KIM#+, Hongdal JUN, Su-Chan BONG
Korea Astronomy and Space Science Institute, Korea, South
The KSRBL is dedicated to observe the sun in the frequency range between 4.3 GHz to 18 GHz which is able to capture the gyrosynchrotron emission during solar flares. The continuous spectrum of the KSRBL has an advantage to find the turnover frequency of gyrosynchrotron emission which occurred mostly at the frequency less than 17 GHz. Recently, we have resumed normal operation of the KSRBL from 2020 September and available to capture radio bursts. In this poster, we present KSRBL operation status and data verification of observed radio burst. For the verification, we referred the data from the NoRP(Nobeyama Radio Polarimeters) which provides solar fluxes at seven fixed frequencies of 1, 2, 3.75, 9.4, 17, 35, and 80 GHz.
ST27-A015
Global Simulation of Corotating Interaction Regions and Their Driven Shocks in the Heliosphere (< 7 AU)
Kan LIOU1#+, Chin-Chun WU2
1Johns Hopkins University Applied Physics Laboratory, United States, 2U.S. Naval Research Laboratory, United States
Corotating interaction regions (CIRs) are an important dynamic solar wind structure in the heliosphere and are formed in the heliosphere when a slow and dense solar wind, originating from streamers, is compressed by a fast but tenuous solar wind, originating from coronal holes, from behind. It is well known that CIRs can drive shocks predominantly anti-sunward of 1 AU. Occasionally, CIR-driven shocks can be observed at 1 AU as demonstrated by previous studies. This study addresses the occurrence of CIR-driven shocks as a function of the radial distance from 18 solar radii to 7 AU using global magnetohydrodynamic simulation. We pay attention to the solar cycle variation of the CIR shock occurrence rate reported previously – there are more CIR shocks observed at 1 AU by the Wind spacecraft during the solar minimum year of cycle 23/24 than the minimum year of cycle 22/23. Our simulation suggests that such a difference is most likely due to a wider and more tilted slow wind regions in the cycle minimum 23/24. We will also present the CIR-shock occurrence rate at different radial distance and compare with the Ulysses observations.
ST28-A017
Locating Heating Channels of the Solar Corona in a Plage Region with the Aid of High-resolution 10830 Å Filtergrams
Parida HASHIM1#+, Haisheng JI2, Jinhua SHEN3
1Xinjiang Astronomical Observatory, CAS, China, 2Chinese Academy of Sciences, China, 3Xinjiang Astronimical observatory,Chinese Academy of Sciences, China
In this paper, we use a set of high-resolution He I 10830 Å filtergrams for a regional area in a plage, very likely an EUV moss area, as an interface layer to pin down the places of coronal heating on the photosphere. The filtergrams are obtained from the 1-meter aperture New Vacuum Solar Telescope (NVST). We divide the 10830 Å filtergrams into two kinds of regions: enhanced absorption patches (EAPs) and less absorption places (LAPs) that are viewed as darkened and translucent areas in the filtergrams. Using well-aligned, simultaneous data from multiple channels of the AIA and HMI on board SDO, we compare the EUV emissions, continuum intensity, emission measure, and temperature in the two kinds of regions. The results firstly confirm a previous result in that 10830 Å EAPs are located on intergranular lanes. Besides, the following progress has been made: 1) EUV emissions at 94, 131, 171, 193, 211, and 304 Å over the EAPs are stronger than the corresponding emissions over LAPs, except that emission at 335 Å. 2) The mission measure over the EAPs in the logarithmic temperature range of 5.5-6.3 is higher. 3) However, the temperature over the EAPs is lower. Based on the above results, we suggest that heating channels in the moss region can be traced down to some areas in intergranular lanes with enhanced density of both cool and hot material. The lower temperature over the EAPs is due to the mixing of both cool and hot material over the vent of the channels.
ST28-A024
High-precision Multichannel Solar Image Registration Using Image Intensity
Song FENG#+
Kunming University of Science and Technology, China
Solar images observed in different channels with different instruments are crucial to the study of solar activity. However, the images have different fields of view, causing them to be misaligned. It is essential to accurately register the images for studying solar activity from multiple perspectives. Image registration is described as an optimizing problem from an image to be registered to a reference image. In this paper, we proposed a novel coarseto-fine solar image registration method to register the multichannel solar images. In the coarse registration step, we used the regular step gradient descent algorithm as an optimizer to maximize the normalized cross correlation metric. The fine registration step uses the Powell–Brent algorithms as an optimizer and brings the Mattes mutual information similarity metric to the minimum. We selected five pairs of images with different resolutions, rotation angles, and shifts to compare and evaluate our results to those obtained by scale-invariant feature transform and phase correlation. The images are observed by the 1.6 m Goode Solar Telescope at Big Bear Solar Observatory and the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory. Furthermore, we used the mutual information and registration time criteria to quantify the registration results. The results prove that the proposed method not only reaches better registration precision but also has better robustness. Meanwhile, we want to highlight that the method can also work well for the time-series solar image registration.
ST28-A032
The Co-alignment Method for the Multi-wavelength Imaging Spectroscopic Data
Kaifan JI+, Yunfang CAI#, Yongyuan XIANG, Zhenyu JIN, Hui LIU
Chinese Academy of Sciences, China
The two-dimensional (2D) imaging spectroscopy observations always play an important role in solar physics studies, which can obtain not only the multi-wavelength spatial images but also the spectral information of the observation target. One of the observations based on the narrow-band filtergrams can deliver high spatial resolution monochromatic images with different wavelengths, and which can be used to synthesize the spectral profiles of target. However, the monochromatic images of off-band observed by the ground-based solar telescopes are recorded at different times, which induces additional image displacements resulting from the telescope vibrations and telluric atmospheric distortions. In this poster, we propose a new co-alignment method based on the optical flow to align the three-band Hα imaging spectroscopic data observed by the NVST, which is a very popular algorithm for motion image analysis. The method has higher accuracy and lower dependence on similar structures compared with cross-correlation alignment. To quantitatively evaluate the alignment results of two images with different similarities, we calculate the alignment accuracies between the images of different off-band and line center using raster images acquired by the Fast Imaging Solar Spectrograph (FISS) operating at GST, respectively. The result shows that our alignment algorithm could reach up to the accuracy of about 0.1’’ (within 1 pixel) under the similarity greater than 0.3, corresponding to the maximum offset wavelength of about 0.6Å. Otherwise, it is necessary to increase more intermediate off-band images for transition alignment. In addition, we package the well-aligned and scientifically ready data into a standard solar physics community format, which can provide convenience for the solar physicists to use high-resolution Hα imaging spectroscopic data of NVST.
ST28-A048
Polarization Crosstalk Calibration Methods for the Near-IR Imaging Spectropolarimeter at the GST
Taylor BAILDON#+
Big Bear Solar Observatory, United States
Big Bear Solar Observatory’s Near-IR Imaging Spectropolarimeter (NIRIS) is the second-generation near-IR polarimeter installed at the Goode Solar Telescope. NIRIS uses a dual Fabry-Perot system to perform high-resolution Solar imaging spectroscopy and polarimetry over a broad spectral range. While the dual-beam design of the polarimeter reduces seeing-induced polarization crosstalk, the relay optics between the telescope and the NIRIS detector introduce additional crosstalk which must be mitigated to obtain accurate Stokes profile measurements. We present and compare two methods for measuring the instrumental crosstalk Mueller matrix that is used in the calibration of NIRIS polarimetry data, and we compare the data from each method to simulated matrices produced from prior calibration data sets. We also discuss efforts made towards characterizing the cavity defects of the Fabry-Perot interferometers, as well as updates made to the NIRIS data processing pipeline.
ST30-A005
A Statistical Study of Space Hurricanes in the Southern Hemisphere
Sheng LU1#+, Zanyang XING1, Qing-He ZHANG2,1, Yongliang ZHANG3, Kjellmar OKSAVIK4, Larry LYONS5, Yu-Zhang MA1, Xiang-Yu WANG1, Yong WANG1, Balan NANAN1
1Shandong University, China, 2National Space Science Center, Chinese Academy of Sciences, China, 3Johns Hopkins University Applied Physics Laboratory, United States, 4University of Bergen, Norway, 5University of California, Los Angeles, United States
The space hurricane is a newly discovered large-scale three-dimensional magnetic vortex structure that spans the polar ionosphere and magnetosphere. At the height of the ionosphere, it has strong circular horizontal plasma flow with a nearly zero-flow center, and a coincident cyclone-shaped aurora caused by strong electron precipitation associated with intense upward magnetic field-aligned currents. By analyzing the long‐term optical observation onboard the Defense Meteorological Satellite Program (DMSP) F16-F19 satellite from 2005 to 2016, we found that the space hurricane in the Southern Hemisphere occurs in summer. In particular, the space hurricanes are more likely to occur in the dayside polar cap at magnetic latitude greater than 80°. We also found the space hurricane occurs mainly under dominant negative By and positive IMF Bz conditions. Those characteristics in Southern hemisphere are basically consistent with the characteristics of space hurricanes in the Northern hemisphere, and both of them support the high latitude lobe reconnection is the formation mechanism of space hurricane. In addition, based on plasma data detected by DMSP satellites, we found that the appearance of space hurricane greatly enhances the horizontal convective velocity, and the electron density increases on its dawn side. In space hurricane, electron temperatures typically increase significantly, accompanied by strong upward field currents and electron precipitation. The result will give a better understanding of the solar wind-magnetosphere-ionosphere coupling process under northward IMF conditions.
ST30-A007
Ionogram Predictions for Spread-F at Hainan with Two Different Neural Network
Zheng WANG1#+, Jinhui CAI2, Guojun WANG1, Pengdong GAO2, Jiankui SHI1
1Chinese Academy of Sciences, China, 2Communication University of China, China
Since the clear trace indicates the ionospheric electron density background and the Spread-F indicates disturbances/irregularities, the prediction of both ionograms with/without Spread-F is important to the research and application. There are currently no well-established neural networks specifically designed to predict the extensive information encompassed within ionograms, particularly the intricate characteristics of Spread-F. At Hainan Station (19.5oN, 109.1oE, magnetic 11oN) under Chinese Meridian Project, the ionosonde kept monitoring ionosphere and producing ionograms from 2002 to now, amassed hundreds of thousands of marked ionograms, classifying into frequency/range/mix/strong range/no Spread-F. In this paper, we approach the short-term prediction (next 30 minutes) of ionograms with/without Spread-F. To achieve this, we use two different Neural Network: (1) combining a spatio-temporal ConvGRU network and a super-resolution EDSR network; (2) a spatiotemporal information-preserving and perception-augmented model with incorporating a Local-Global discriminator. Through the two methods, they both achieve over 90% accuracy for the Spread-F forecast, and also a prediction of F trace corresponding to the plasma density profile.
ST30-A011
3-D Ionosphere Imaging at Middle-to-high Latitude in the Northern Hemisphere with a Data Assimilation System
Lingxin ZHAO#+
Shandong University, China
A ionospheric data assimilation system for the middle-to-high latitude in the northern hemisphere (>50°N) has been developed. The Empirical Canadian High Arctic Ionospheric Model (E-CHAIM) is used to calculate a more realistic and location-dependent background error covariance matrix, and using the three-dimensional variational (3DVAR) method for measurement updates, the ground and LEO-based total electron content (TEC) data are assimilated into the model to obtain the three-dimensional electron density distribution that is closer to the true state of the ionosphere. The spatial-temporal resolution of the reanalyzed 3-D electron density product is 2.5°in latitude, 5°in longitude, 25 km in altitude, and 5min in time. Using this system, we have reconstructed some structures and phenomena of the high-latitude ionosphere during magnetic storms, such as storm-enhanced density (SED) and polar cap patch, and obtained their three-dimensional spatial distribution characteristics and evolution over time.
ST30-A013
Directly Observation of Space Hurricane Disturbed Polar Thermosphere
Zhi-Feng XIU1+, Yu-Zhang MA1#, Qing-He ZHANG2,1, Zanyang XING1, Shunrong ZHANG3, Yongliang ZHANG4, Kjellmar OKSAVIK5, Larry LYONS6, Michael LOCKWOOD7, Yong WANG1
1Shandong University, China, 2National Space Science Center, Chinese Academy of Sciences, China, 3Massachusetts Institute of Technology, United States, 4Johns Hopkins University Applied Physics Laboratory, United States, 5University of Bergen, Norway, 6University of California, Los Angeles, United States, 7University of Reading, United Kingdom
The space hurricane is a three‐dimensional magnetic vortex structure with strong flow shears and electron precipitation in the polar cap. This study investigates for the first time how a space hurricane disturbs the polar thermosphere. During the formation and development of the space hurricane, the directional reversal of the horizontal neutral wind and the plasma convection will both be relocated from the poleward auroral oval boundary to the edge of the space hurricane, but the neutral wind responds slower compared to the plasma convection. Strong flow shears in the space hurricane causes enhanced Joule heating in the polar cap, which heats the thermosphere and triggers Atmospheric Gravity Waves (AGWs). Statistical results reveal that significant AGWs mainly are located on the dawnside of the space hurricane, suggesting that the space hurricane plays a significant role in ion‐neutral coupling and generation of polar cap AGWs.
ST32-A004
Numerical Experiments of Fast Magnetic Reconnection Driven by the Rapidly Expanding Plasma
Shanshan XU#+
Chinese Academy of Sciences, China
Three modes of magnetic reconnection, flux pile-up, Sonnerup, and hybrid, are examined in the context of driven magnetic reconnection via 2D and 2.5D magnetohydrodynamic (MHD) numerical simulations. They result from variances in gas pressure and magnetic field strength in the reconnection inflow region. The simulation demonstrates that the Spitzer diffusion region of magnetic reconnection is not just an X-point; instead, it appears as a slim and elongated current sheet that creates two pairs of the slow-mode shock on either end. These shocks contribute to forming four boundaries that separate the inflow from the outflow. In the regions far from the Spitzer diffusion region, two sets of intermediate waves stand inside the slow-mode shocks. The waves reverse the magnetic field inside the reconnection outflow region, and create a W-shape magnetic field in that region. The scenario that the slow-mode shock is located outside the intermediate wave is consistent with the inference of Priest (1972), and is contrary to that of Petschek & Thorne (1967) and Vasyliunas (1975). This is the most important result we acquired in this work.
ST32-A005
Firehose Instability in Electron-position Plasma
Chun-Sung JAO1#+, Reinaldo SANTOS DE LIMA2, Lin-Ni HAU3
1National Cheng Kung University, Taiwan, 2Universidade de São Paulo, Brazil, 3National Central University, Taiwan
Nonthermal velocity distributions naturally develop in weakly collisional plasmas, serving as sources for several known instabilities. The electromagnetic firehose instability arises from pressure anisotropy in magnetized plasmas, particularly when the pressure parallel to the background magnetic field significantly exceeds that in the perpendicular direction. In space environments, firehose instability is widely considered a crucial mechanism for regulating temperature anisotropies of electrons and protons, as observed in phenomena like the solar wind. In the electron-proton plasma, composed of particles with opposite charges and a significant mass ratio, the characteristics of proton and electron firehose instability differ. For instance, proton firehose instability can be defined in terms of propagating and non-propagating aperiodic modes. However, for electron firehose instability, there is no unique definition for the two branches. This study delves into the investigation of firehose instability in electron-positron plasmas, where particles carry opposite charges and possess equal mass. To scrutinize the characteristics of firehose instability in these plasmas, we will employ both linear theoretical models and nonlinear numerical simulations.
Session Chair(s): Qing-He ZHANG, National Space Science Center, Chinese Academy of Sciences, Michel BLANC, Institute for Research in Astrophysics and Planetology
ST30-A002
| Invited
Observation and Research on the Disturbances of the Upper Atmosphere and Ionosphere Caused by Severe Events in the Lower Atmosphere
Jiyao XU#+
Chinese Academy of Sciences
Severe events such as thunderstorms, typhoons, earthquakes, and volcanic eruptions that occur on the earth surface and lower atmosphere not only have serious impacts on human life, but also have significant impacts on the middle and upper atmosphere and ionosphere. The detection and research of phenomena and physical processes in the response of the upper atmosphere to these strong events are interesting topics. We have established a monitoring network of airglow over the Chinese Mainland. This network has conducted double-layer detection for OH airglow (with a radiation altitude of about 87 kilometers) and OI 630nm red line airglow (with a radiation altitude of approximately 250 kilometers) for about ten years. This report will present observations and research progresses on the physical processes of disturbances of the upper atmosphere and ionosphere caused by severe events such as thunderstorms, typhoons, and Tonga volcanoes using the airglow network and satellite detection.
ST30-A022
Satellite-based Climate and Tropical Weather Research at Nanyang Technological University, Singapore
Yee Hui LEE#, Erick LANSARD+
Nanyang Technological University
Climate change is a worldwide concern and is especially important for the tiny country such as Singapore. To tackle climate change, the understanding the different weather parameters and change is weather patterns locally, regionally and globally is critical. At Nanyang Technological University, satellites have been launched and will be launched for the gathering of such data for climate studies. Currently, teams of researchers have been working on the use of satellite-based technology such as GNSS as an all-weather operational robust methodology for the prediction of meteorological phenomena. GNSS signal is delayed by several atmospheric components such as water vapor, dry gasses, liquid water, hydrometeors while travelling from GNSS satellites to the earth station which is employed to retrieve different atmospheric parameters like precipitable water vapor (PWV), tropospheric gradient, atmospheric residual, wet delay which are necessary for weather forecast. Our researchers are also exploring the use of radio occultation as an essential technology for climate studies since it gives continuous and dependable data on atmospheric parameters with great vertical resolution and global coverage. Since radio occultation passes through the ionosphere, there has been active research on the use of radio occultation for climate parameters study. Our researchers aims to explore the capabilities of different correction factors by utilizing different ionospheric models to improve the radio occultation retrievals which can enhance the climate studies.
ST30-A019
Planetary-scale Waves in the Mesosphere and Low Thermosphere: Responses to Sudden Stratosphere Warming Events Via Multi-station Analysis
Maosheng HE1#+, Jeffrey FORBES2, Christoph JACOBI3, Guozhu LI4, Gunter STOBER5, Libo LIU4, Chi WANG4
1National Space Science Center, Chinese Academy of Sciences, 2University of Colorado Boulder, 3Leipzig University, 4Chinese Academy of Sciences, 5University of Bern
The mesosphere and low thermosphere (MLT) region serve as a crucial intermediary zone between the neutral atmosphere and the ionosphere. Within this transitional space, upward propagating atmospheric waves reach their peak amplitude before dissipating. As a result, the MLT not only functions as a natural laboratory for studying neutral atmospheric dynamics but also plays a pivotal role in ionospheric coupling. However, due to limitations in observational techniques, previous investigations into planetary-scale waves in the MLT have predominantly relied on single-station analyses, introducing certain uncertainties. To address these limitations, we combine wind observations from the meteor radars of the Chinese Meridian Circle Program and similar radars from other longitudinal sectors. Employing a Multi-Station method, our data enable the estimation of zonal wavenumbers and the exploration of planetary-scale waves, encompassing planetary waves and tides. Through case studies and multi-year statistical analyses, we unveil the response of these waves to Sudden Stratosphere Warming (SSW) events. Our statistical analysis reveals amplifications of multiple planetary wave normal modes during SSW events, while discerning the behavior of the first six migrating tides during SSW becomes challenging amid their seasonal variations. Furthermore, we observe a significant occurrence of secondary waves generated by wave-wave nonlinear interactions during SSW events.
ST30-A024
| Invited
Observations of the Ionospheric Plasma Irregularities Driven by Space Weather and Lithosphere Events
Charles LIN1#+, P. K. RAJESH1, Shih-Ping CHEN1, Jong-Min CHOI1, Tungyuan HSIAO2, Chi-Yen LIN3, Cheng-Yung HUANG4
1National Cheng Kung University, 2Hsing Wu University, 3National Central University, 4Taiwan Space Agency
FORMOSAT7-COSMIC2 Mission is consist of six satellites equipped with GNSS radio occultation (RO) payload, in-situ ion density and velocity meters (IVM), and RF beacon transmitters at low latitudes. Signal-to-noise ratio (SNR) of RO soundings provides observations of irregularity altitudes, and IVM measures in-situ density fluctuations at satellite altitude of 550 km. Combining RO, IVM, ground-based receivers of beacon and GNSS, it is like an observation suite of plasma irregularities that provides unprecedented number of observations that were not available previously. The observation suite provides opportunity to monitor the variations of plasma irregularity structure and possibly be able to see their growth and subsidence. As the solar activity elevated in 2023 and 2024, our observations show that seasonal irregularities occur more frequently with grater intensity. Meanwhile, as the magnetic storms also occur much more often with greater intensity, storm time variations of the irregularities become much more complex. In this presentation, we show that growth of strong low latitude plasma irregularities during storms and some of them last over the entire evening period. They are likely driven by the interplay of storm-time electric field and traveling ionospheric disturbances. Additionally, we also present the dynamic irregularities driven by other nature hazard events from the observation suite showing that the extreme event could lead to irregularity growth comparable to those driven by the magnetic storms.
ST30-A020
Precision Monitoring Telescope for L&S Band Solar Radio
Bingxian LUO#+, Wengeng HUANG, Mingliang ZHAO, Liqin SHI, Siqing LIU, Jing WANG
Chinese Academy of Sciences
The 10.7 cm solar radio flux (also known as F10.7 index) is highly sensitive to the state of the high chromosphere and low corona. It has a good correlation with extreme ultraviolet (EUV) radiation from solar and serves as an important parameter for characterizing solar activity levels. The F10.7 index has extensive applications not only in fundamental research but also in aerospace engineering, such as thermal atmospheric density models for orbit prediction and ionospheric models for radio wave propagation. It is a driving index required by many space environmental application models. Therefore, real-time monitoring of F10.7 has significant scientific significance and practical application value. Recently, the National Space Science Center of the Chinese Academy of Sciences has established a precise monitoring telescope for L&S band solar radio flux in Langfang, Hebei, China. This telescope is primarily designed for monitoring solar radio burst events in the L-band frequency points used by GNSS navigation systems and the 10.7 cm S-band frequency point. Its main purpose is to monitor solar radio burst events in the L-band and obtain F10.7 data in real time, providing alert services for GNSS solar radio interference events and real-time acquisition of F10.7 index. This report briefly introduces the composition, data acquisition, calibration methods, operational mode, and data quality evaluation results of this system. The results from nearly 2 years of operation show that the system works stably and autonomously, capable of automatic antenna opening, tracking, data retrieval, and inversion. Compared with Canadian data, the correlation coefficient is 95%, with an average error of 5.42 sfu, average absolute percentage error of 4.17%, and root mean square error of 7.06 sfu, meeting the requirements for daily operational needs.
ST30-A009
Observation, Monitoring, and Warning, of Space Hazards: CMU Space Weather War Room
Siramas KOMONJINDA1#+, Waraporn NUNTIYAKUL1, Suwicha WANNAWICHIAN1, Achara SERIPIENLERT2, Wirin SONSRETTEE3, Audcharaporn PAGWHAN4, Watchanon RUANGKUL5, Parkpoom SRITHIMAKUL6, Boonrucksar SOONTHORNTHUM2, Duangmanee WONGRATANAPHISAN1
1Chiang Mai University, 2National Astronomical Research Institute of Thailand, 3Panyapiwat Institute of Management, 4Mahidol University, 5Thailand Excellence Center in Physics, 6Pakgon Company Limited
Space Weather research was conducted in Thailand for more than 30 years in many dimensions. This includes the development of neutron monitors and the observation from Thailand where the cut-off rigidity is very high. Chiang Mai University’s ChangVan neutron monitor was ensemble under a collaboration between other Thai universities and a support from Shinshu University. Later, it was sent to Antarctica onboard the Xue Long icebreaker of PRIC in 2018-2019 and 2019-2020 expeditions and onboard the Araon icebreaker of KOPRI in 2023 – 2024. In 2023, Chiang Mai University introduced a new research facility, CMU Digital Innovation Center for Observation, Monitoring, and Warning, of Space Hazards or CMU space weather war room. This center aims to create a database of space weather data gathering from ground, space, and underground observatories with support from international collaborations. Public can access to this data from the monitors at Chiang Mai University or from the website of Thailand center of Excellent in Physics.
ST30-A001
| Invited
Importance, Perils, and Limitations of High Sampling of GNSS Signals for Space Weather Research
P. T. JAYACHANDRAN#+
University of New Brunswick
Global Navigation Satellite Systems (GNSS) are crucial in multi-disciplinary geospace research, including ionospheric research. High sampling data recently gained prominence in ionospheric research due to their importance in understanding a category of ionospheric irregularities called scintillation. The importance of high sampling rate GNSS data lies in its ability to capture the rapid fluctuations, which are essential for improving our understanding of the ionospheric behaviour and the modelling and forecasting/nowcasting. However, using high sampling rate GNSS data has inherent limitations and challenges. The higher sampling rates may lead to increased susceptibility to the receiver noise and multipath effects affecting data quality and precision. The higher sampling rate also brings the impact of code interference and receiver architecture into the picture. These can impact the measurement, leading to misinterpretation of the results as some fluctuations might not always be associated with genuine ionospheric variations. This talk will cover the importance of high sampling rate GNSS data in capturing intricate ionospheric dynamics while pointing out the factors that can contribute to the artificial signal/noise in the data.
ST30-A012
Recently Research Progress on the Polar Sporadic-E Layers
Yong WANG1+, David THEMENS2, Roger VARNEY3, Robert GILLIES4, Yu-Zhang MA1, Zanyang XING1, P. T. JAYACHANDRAN2, Qing-He ZHANG5,1#
1Shandong University, 2University of New Brunswick, 3SRI International, 4University of Calgary, 5National Space Science Center, Chinese Academy of Sciences
At high latitudes, the Sporadic-E layer (Es layer) is a common phenomenon but is still poorly understood due to sparse measurements and the difficulty of conventional mechanisms to operate. In this study, an interesting case of polar cap Es layer is first studied by using the twin incoherent scatter radars (northward looking face of Resolute Incoherent-Scatter Radar and Resolute Incoherent-Scatter Radar-Canada), a Canadian Advanced Digital Ionosonde, and a Magnetometer, all at Resolute, Canada. From several electron density profiles of the twin radars, the horizontal scale of the polar cap Es layer is found to be greater than 350 km. Moreover, the polar cap Es layer is determined to be drifting from the bottom F region (>150 km) to the lower E region. Furthermore, a unique appearance of double polar cap Es layers is observed. As a result, these peculiar signatures inspire a newly proposed process that involves the combination of localized electric fields and gravity waves.
Session Chair(s): Yuandeng SHEN, Chinese Academy of Sciences, Bo LI, Shandong University
ST12-A015
| Invited
Investigation the Coronal Loop Oscillations
Zongjun NING#+
Chinese Academy of Sciences
We study the loop oscillations after a solar flare on January 19, 2023, in the active region N11E40 3196, which is well observed by SDO/AIA. After tracing the loop position and fitting, we find that the loop oscillations have a period between 3 and 9 minutes at various loop locations, such as from leg to top or from the inner to outer. Their oscillating amplitudes decrease with time. After DEM analysis, we find that these loop position oscillations are resulted from the plasma density fluctuation. Meanwhile, it is interesting that the brightness at loop top display the oscillation with a typical period of 4-5 minutes. They are possible due to both the plasma density and temperature fluctuation there. Our findings provide the physical clues for studying and understanding the mechanism of the loop oscillation.
ST12-A001
| Invited
Characterising Atmospheric Oscillatory Behavior of Magnetic Helicity Flux in Eruptive and Non-eruptive Active Regions
Marianna KORSOS#+
The University of Catania
The magnetic helicity slowly and continuously accumulates in response to plasma flows tangential to the photosphere and magnetic flux emergence normal to it, feeding into the solar atmosphere. Analysing the evolution of magnetic helicity flux at different atmospheric heights is key to identifying its role in the dynamics evolution of eruptive flaring, confined flaring, and non-flaring active regions. For each studied active region, the emergence, shearing, and total magnetic helicity components are derived at different atmospheric heights. An oscillatory behaviour is searched for in these obtained magnetic helicity components. We found that the measured largest periodic oscillations of the three helicity flux components uniquely describe the three analysed categories of active regions.
ST12-A019
| Invited
Unveiling the Nature of EUV Waves with MHD Simulations
Jinhan GUO1#+, Peng-Fei CHEN1, Yiwei NI1, Yang GUO1, Stefaan POEDTS2, Brigitte SCHMIEDER3, Mingzhe GUO4
1Nanjing University, 2Katholieke Universiteit Leuven, 3Observatoire de Paris/ Université PSL/ National Centre for Scientific Research/ Sorbonne Université/ Université de Paris, 4Shandong University
Solar eruptions frequently produce global wavelike phenomena in the solar corona, carrying crucial information about magnetic fields and plasma along the travel path. Similar to seismic waves revealing Earth’s interior structure in geophysics, coronal magnetohydrodynamic (MHD) waves have become a pivotal probe for diagnosing coronal magnetic fields in solar physics. Despite extreme ultraviolet (EUV) waves being the most frequently observed wavelike phenomena that propagate in the global corona, a consensus about their nature remains elusive due to the lack of 3D physical data in remote-sensing observations. To address this issue, we aim to unveil the physical nature of EUV waves with the aid of MHD simulations. We conduct two types of simulations. The first type involves data-inspired modeling based on ideal magnetic configurations, used to investigate the relationships between wave characteristics and magnetic structures. The second type is a data-driven simulation where the initial magnetic fields are derived from observations, providing insights into wave properties in a more realistic magnetic configuration. Our simulations indicate that EUV waves can be explained very well by the field-line stretching model proposed by Chen et al. (2002), in which wave propagation is primarily dominated by the configuration of overlying magnetic field lines. This sheds light on inferring global coronal magnetic fields with EUV waves in future works, such as structures of large-scale coronal loops and separatrix layers.
ST12-A004
A New Model for the Driver of Decayless Kink Oscillation
Dong LI#+
Chinese Academy of Sciences
Decayless kink oscillations, which are nearly omnipresent in the solar corona, are believed to be driven by continuously operating energy supply. We investigate an external continuous excitation of an apparent decayless oscillation during an X1.1 flare on June 20, 2023 (SOL2023-06-20T16:42). The kink oscillation is detected as a transverse oscillation of the coronal loop, which reveals five apparent cycles with an average period of about 130±10 s. The oscillation amplitude does not show any significantly decay, suggesting a decayless oscillation. At the same time, the solar flare occurs in the vicinity of the oscillating loop and exhibits five main pulses in HXR, microwave, and UV emissions, which could be regarded as flare QPPs. They have similar periods of about 100-130 s, which may indicate successive and repetitive energy releases during the flare impulsive phase. The peak of each loop oscillation cycle appears to follow the pulse of the QPPs, suggesting that the transverse oscillation is closely associated with flare QPPs. Our observations support the scenario where the repetitive energy released following flare QPPs could be invoked as external, continuously operating drivers of the apparent decayless kink oscillation.
ST12-A005
Spatially Resolved Moving Radio Burst Associated with an EUV Wave
Lei LU#+
Chinese Academy of Sciences
Coronal mass ejections (CMEs) are large clouds of magnetized plasma ejected from the Sun and are often associated with the acceleration of electrons that can result in radio emission via various mechanisms. However, the underlying mechanism relating the CMEs and particle acceleration still remains a subject of heated debate. Here, we report multi-instrument radio and extreme ultraviolet (EUV) imaging of a solar eruption event on 2011 September 24. We determine the emission mechanism of a moving radio burst, identify its three-dimensional location with respect to a rapidly expanding EUV wave, and find evidence for CME shocks that produce quasiperiodic acceleration of electron beams.
ST12-A003
Simultaneous Horizontal and Vertical Oscillation of a Quiescent Filament Observed by CHASE and SDO
Jun DAI#+
Chinese Academy of Sciences
We present the imaging and spectroscopic observations of the simultaneous horizontal and vertical large-amplitude oscillation of a quiescent filament triggered by an extreme-ultraviolet (EUV) wave on 2022 October 2. Particularly, the filament oscillation involved winking phenomenon in Hα images and horizontal motions in EUV images. Originally, a filament and its overlying loops across AR 13110 and 13113 erupted with a highly inclined direction, resulting in an X1.0 flare and a non-radial coronal mass ejection. The fast lateral expansion of loops excited an EUV wave and the corresponding Moreton wave propagating northward. Once the EUV wave front arrived at the quiescent filament, the filament began to oscillate coherently along the horizontal direction, and the “winking filament” appeared concurrently in Hα images. The horizontal oscillation involved an initial amplitude of ∼10.2 Mm and a velocity amplitude of ∼46.5 km s−1, lasting for ∼3 cycles with a period of ∼18.2 minutes and a damping time of ∼31.1 minutes. The maximum Doppler velocities of the oscillating filament are 18 km s−1 (redshift) and −24 km s−1 (blueshift), which were derived from the spectroscopic data provided by the Chinese Hα Solar Explorer/Hα Imaging Spectrograph. The three-dimensional velocity of the oscillation is determined to be ∼50 km s−1 at an angle of ∼50° to the local photosphere plane. Based on the wave–filament interaction, the minimum energy of the EUV wave is estimated to be 2.7 × 1020 J. Furthermore, this event provides evidence that Moreton waves should be excited by the highly inclined eruptions.
ST12-A020
Data-constrained MHD Simulations on Global Corona Waves Generated by Inclined Eruptions
Yiwei NI1#+, Jinhan GUO1, Peng-Fei CHEN1, Li FENG2
1Nanjing University, 2Chinese Academy of Sciences
Solar Corona Waves are a large-scale global wave phenomenon generated by solar eruptions, manifested as Hα Moreton waves in Solar Chromosphere, Lyα waves in transition regions and EIT/EUV waves in the corona. Generally, the corona waves are isotropic and, can be dived into the piston-driven shock wave induced by Corona Mass Ejections and the non-wave component resulted by magnetic field lines stretching. However, the LST telescope onboard ASO-S observed an edge prominence eruption event and thereafter non-radial propagating EUV wave contains several wave fronts. We adopted the data-constrained MHD simulation and focused on the nature of various wave components. The simulation result shows that the inclined eruption intensifies the successive stretching of magnetic field lines toward the equator, leading to the mounting EIT wave front. The separatrix between the ambient corona loops and open magnetic field give birth to the board Quasi-periodic Fast-mode propagating (QFP) wave trains in the solar corona and the recurrent type II radio burst.
ST12-A007
Birth Places of Extreme Ultraviolet Waves Driven by Impingement of Solar Jets Upon Coronal Loops
Liang ZHANG1#+, Ruisheng ZHENG1, Huadong CHEN2, Yao CHEN1
1Shandong University, 2Chinese Academy of Sciences
Solar extreme ultraviolet (EUV) waves are large-scale propagating disturbances in the corona. It is generally believed that a vital key to the formation of EUV waves is the rapid expansion of the loops that overlie erupting cores in solar eruptions, such as coronal mass ejections (CMEs) and solar jets. However, the details of the interaction between the erupting cores and overlying loops are not clear because the overlying loops always instantly open after energetic eruptions. Here, we present three typical jet-driven EUV waves without CMEs to study the interaction between the jets and the overlying loops that remained closed during the events. All three jets emanated from magnetic flux cancellation sites in the source regions. Interestingly, after the interactions between the jets and overlying loops, three EUV waves respectively formed ahead of the top, the near end (close to the jet source), and the far (another) end of the overlying loops. According to the magnetic field distribution of the loops extrapolated through the potential field source surface method, it is confirmed that the birthplaces of three jet-driven EUV waves were around the parts of the overlying loops with the weakest magnetic field strengths. We suggest that the jet-driven EUV waves preferentially occur at the weakest part of the overlying loops, and the location can be subject to the magnetic field intensity around the ends of the loops.
Session Chair(s): Shunrong ZHANG, Massachusetts Institute of Technology, Bingxian LUO, Chinese Academy of Sciences
ST30-A014
| Invited
Coordinated Ground-based Ionosphere-thermosphere Observations During the Dec 1-2, 2023 Geospace Storm
Shunrong ZHANG1#+, Jiuhou LEI2, Jiyao XU3, Liwen REN3, Philip ERICKSON1, Ercha AA1, Anthea COSTER1
1Massachusetts Institute of Technology, 2University of Science and Technology of China, 3Chinese Academy of Sciences
After the burst of an M9.8 solar flare observed in AR3500 at around 2000 UT on November 28, 2023, a halo coronal mass ejection (CME) formed and rapidly approached Earth at a speed of approximately 910 km/s. This CME marked the culmination of a series of four Earth-bound CMEs, standing out as the final and largest event. Space weather agencies predicted appropriately its arrival time, estimating it around December 1, 2023, as well as the G3 (Kp 7) intense geomagnetic storm. Following these solar events, we closely monitored and decided to conduct internationally coordinated ground-based upper atmospheric observations to facilitate a detailed study of the CME's geoeffects. The coordination was achieved through a collaborative effort initiated among world incoherent scatter radars (ISRs) as well as observatories operated by the Chinese Meridian Project and instruments from other international partners, within the framework of the International Meridian Program (IMCP). This presentation will provide a preliminary analysis of the campaign, highlighting observations along the meridian circle at 120E/60W, where the simultaneous responses on both the dayside and nightside Magnetic Local Times (MLTs) during different storm phases are particularly interesting. These responses are related to ionosphere-thermosphere effects caused by penetration electric fields of solar wind-magnetosphere origin, traveling ionospheric/atmospheric disturbances excited in the auroral zone, subauroral magnetosphere-ionosphere-thermosphere coupling processes, and equatorial and low latitude plasma bubbles under the geomagnetic storm influence.
ST30-A008
Recent Progresses of Space Hurricane
Qing-He ZHANG1,2#+, Sheng LU2, Zhi-Feng XIU2, Yongliang ZHANG3, Kjellmar OKSAVIK4, Larry LYONS5, Liwen REN6, Zanyang XING2, Yu-Zhang MA2, Yong WANG2
1National Space Science Center, Chinese Academy of Sciences, 2Shandong University, 3Johns Hopkins University Applied Physics Laboratory, 4University of Bergen, 5University of California, Los Angeles, 6Chinese Academy of Sciences
This paper briefly summarize the recent progresses of research on space hurricane. The statistical results show that about 13 space hurricane events occur per year in average in the Northern and Southern Hemispheres. Space hurricane prefers to occur in higher solar activities and summer with large solar elevation angle and earth dipole tilt angle. It also prefers to occur strong positive By and Bz, and negative Bx in the Northern Hemisphere, and strong negative By and Bz, and positive Bx in the Southern Hemisphere. Space hurricane clearly heats the polar cap ionosphere through joule heating, and it can generate gravity waves and significantly heat the Thermosphere.
ST30-A010
Multi-instrument Analysis of the Segmentation of the Tongue of Ionization Into Two Dense Polar Cap Patches
Yu-Zhang MA1#+, Qing-He ZHANG2,1, Larry LYONS3, Kjellmar OKSAVIK4, Zanyang XING1, Yong WANG1, Marc HAIRSTON5, Jianjun LIU6, Balan NANAN1, Zhong-Xin DENG7, Qiang ZHANG8, Sihan ZHAO1
1Shandong University, 2National Space Science Center, Chinese Academy of Sciences, 3University of California, Los Angeles, 4University of Bergen, 5The University of Texas at Dallas, 6Polar Research Institute of China, 7China Research Institute of Radiowave Propagation, 8Tongji University
This paper investigates the evolution of two consecutive polar cap patches using multi-instrument observations from February 27, 2014. We provide insights into how the interplanetary magnetic field (IMF) variations influence the formation and segmentation of these patches. Our findings reveal that the entry of dayside dense plasma into the polar cap is predominantly driven by the modified convection near the cusp region, which is controlled by the transition of IMF By or the sudden drop of IMF Bz. Furthermore, we observe a rapid north-westward plasma flow within the patch segmentation region, accompanied by equatorward-expanded and enhanced convection near the cusp region. This fast-moving flow, approximately 1.5 km/s, is characterized by low density and high electron temperature during periods of intense auroral electrojets, shows a signature of a Subauroral Polarization Stream. This suggests that the fast-westward flow, in conjunction with the expansion and contraction of ionospheric convection, plays a crucial role in the segmentation of polar cap patches from the dayside plasma reservoir. This study provides a more comprehensive observation of the evolution of polar cap patches, thereby significantly advancing our understanding of the dynamic mechanisms governing patch formation and segmentation.
ST30-A006
| Invited
Equatorial Plasma Bubbles Observation Using 39.65 MHz VHF Radar at Chumphon, Thailand
Septi PERWITASARI1#+, Michi NISHIOKA1, Yuichi OTSUKA2, Susumu SAITO3, Supnithi PORNCHAI4, Jamjareegulgarn PUNYAWI 4
1National Institute of Information and Communications Technology, 2Nagoya University, 3National Institute of Maritime, Port and Aviation Technology, 4King Mongkut's Institute of Technology Ladkrabang
The equatorial plasma bubble (EPB) is one of the distinct phenomena in the equatorial ionosphere. This phenomenon affects radio waves propagating through it which may cause a fluctuation in amplitude and phase of the global navigation satellite system (GNSS) signals. Therefore, close monitoring and prediction of EPB events are crucial. The National Institute of Information and Communications Technologies (NICT) established cooperative research for ionospheric observation in Southeast Asia called SouthEast Asia Low-Latitude IOnospheric Network (SEALION) in 2002. Various ground-based ionospheric instruments have been in operation since. In January 2020, NICT in collaboration with King Mongkut's Institute of Technology Ladkrabang (KMITL) installed a 39.65 MHz VHF radar at Chumphon, Thailand to detect EPBs near the dip equator. This radar system consists of a linear array of 18 three-element Yagi antennas. Since the start of operation, the radar has observed EPBs caused by various events, not only geomagnetic activities but also extreme geologic events such as a volcano eruption. We will discuss the radar operation summary and a case study of an EPB event on December 3, 2023. The VHF radar observed Field-Aligned Irregularities (FAIs) associated with EPB after 12:00 UT. The geomagnetic condition on this day was in a recovery phase which EPBs do not likely occur. Another plausible cause was the Marapi volcano eruption at 7:45 UT which is located in Kototabang, Indonesia (0.38°S, 100.47°E). The FAI region reached ~600 km altitude, thus the EPB was expected to extend over Chiang Mai. Based on ionosonde observations, spread-F was also observed over Chumphon (~11:45 UT), Bac Lieu (~11:45 UT) and Chiang Mai (~12:45 UT). Detailed discussion on this event and a future collaboration prospect with the International Meridian Project will also be discussed in the presentation.
ST30-A021
Investigating the Complex Interplay and Longitude Heterogeneities of the Electrodynamic Response of the Low and Equatorial Latitude Ionosphere to Magnetic Storms with an IMCP-type Network
Michel BLANC1#+, Christine AMORY-MAZAUDIER2, Frederic PITOUT1
1Institute for Research in Astrophysics and Planetology, 2Laboratoire de Physique des Plasmas (LPP)/ National Centre for Scientific Research/ University Pierre and Marie Curie
While low-latitude ionospheric effects of magnetic storms have been studied in depth for decades with an increasing sophistication of instruments, many unknowns remain about: (1) the way the different storm-time disturbance mechanisms that take their roots at high latitudes overlay, interfere and propagate to low latitudes during the development of a storm; (2) how the observed large variability of magnetic storms translates into the equally large variability of their low latitude effects; (3) the systematic longitude variability of these effects, in addition to the local time variability, and the main parameters that best describe it. In this talk, we will first summarize the currently accepted understanding of the main mechanisms at work, with emphasis on the “Prompt Penetration” and “Disturbance Dynamo” electric field generation mechanisms. We will then make a first attempt at summarizing published observations of observational effects of these mechanisms in the different longitude sectors, based on ground-based instruments and networks. We will identify some general features of these observations and open questions for future studies. Finally, we will suggest ways by which a coordinated analysis of observations made by the IMCP network, which could take the form of an “IMCP Key Project”, will make it possible to address successfully and solve some of the open questions.
ST30-A015
Simulation of Nighttime Medium-scale Traveling Ionospheric Disturbances in the Midlatitude Ionosphere During Stormtime
Xiaochuan WANG1+, Jiuhou LEI1#, Shunrong ZHANG2, Zezhong LI1, Tong DANG1, Xiaoli LUAN1, Xiankang DOU1
1University of Science and Technology of China, 2Massachusetts Institute of Technology
Recent observations have revealed the occurrence of nighttime medium-scale traveling ionospheric disturbances (MSTIDs) over the continental US during storm conditions even without invoking the Es instability. While this phenomenon is considered to be electrified and likely associated with the Perkins instability, the influences of storm-enhanced density (SED), electric fields, and winds on the excitation of nighttime MSTIDs remain a complicated issue and require further quantitative analysis. In this study, we develop a two-dimensional numerical model of the nighttime ionospheric electrodynamics at midlatitudes using the ionospheric ion continuity equation and the electric field Poisson equation to investigate the characteristics of MSTIDs in the SED base region during storm conditions. We demonstrate that the magnetic inclination effect can explain the lower latitude preference of the MSTIDs during magnetic storms, while the development of MSTIDs is primarily influenced by intense storm electric fields under the background ionospheric condition of large density gradients associated with SED. However, the impact of neutral winds on the MSTID growth varies, depending on their specific direction determined by the strongly dynamic spatiotemporal variation of the thermosphere and ionosphere during storms. Therefore, the MSTID stormtime scenario results from a combination of multiple important factors.
ST30-A004
Multi-instrument Observations of the Evolution of Polar Cap Patches Associated with Flow Shears and Particle Precipitation
Duan ZHANG1+, Qing-He ZHANG2,3#, Kjellmar OKSAVIK4, Zanyang XING3, Larry LYONS5, Huigen YANG6, Guo-Jun LI7, Keisuke HOSOKAWA8, Kazuo SHIOKAWA9, Yu-Zhang MA3, Yong WANG3, Xiang-Yu WANG3
1National Space Science Center (NSSC), Chinese Academy of Sciences (CAS), 2National Space Science Center, Chinese Academy of Sciences, 3Shandong University, 4University of Bergen, 5University of California, Los Angeles, 6Polar Research Institute of China, 7Chongqing University of Posts and Telecommunications, 8University of Electro-Communications, 9Nagoya University
Simultaneous observations from Defense Meteorological Satellite Program, Swarm, Resolute Bay all-sky imagers, GPS Total Electron Content and Super Dual Auroral Radar Network, are used to investigate the evolution and key characteristics of the Tongue of Ionization (TOI) being restructured into a polar cap patch. Six satellites crossed the TOI of patch as it moved from the dayside to the nightside. It was initially hot, then a mix of both cold and hot, and finally it became a cold patch. This suggests that cold patch is not only a result of solar EUV radiation, but may also develop when a hot patch cools down. Soft-electron precipitation and flow shears both contribute to the TOI restructuring and the appearance of polar cap patch. The plasma density of patch at ~500 km was at least four times higher than at ~800 km. The plasma density enhancement gradually decreased as the patch evolved due to decreased production and transport of cold nightside low-density plasma. Moreover, the duskward motion of the patch was influenced by changes in the ionospheric convection pattern.
Session Chair(s):
ST12-A002
| Invited
The Magnetic Condition of Coronal Shocks Generate Type II Radio Bursts
Su WEI#+
Sun Yat-sen University
Type II radio bursts are thought to be produced by shock waves in the solar atmosphere. However, what magnetic conditions are needed for the generation of type II radio bursts is still a puzzling issue. Here, we quantify the magnetic structure of a coronal shock associated with a type II radio burst. Based on multiperspective extreme- ultraviolet observations, we reconstruct the three-dimensional (3D) shock surface. By using a magnetic field extrapolation model, we then derive the orientation of the magnetic field relative to the normal of the shock front (θBn) and the Alfvén Mach number (MA) on the shock front. Combining the radio observations from the Nancay Radio Heliograph, we obtain the source region of the type II radio burst on the shock front. It is found that the radio burst is generated by a shock with MA > 1.5 and a bimodal distribution of θBn. We also use the Rankine–Hugoniot relations to quantify the properties of the shock downstream. Our results provide a quantitative 3D magnetic structure condition of a coronal shock that produces a type II radio burst.
ST12-A011
| Invited
Resolved Magnetohydrodynamic Wave Lensing in the Solar Corona
Xinping ZHOU#+
Sichuan Normal University
Electromagnetic wave lensing, a common physical phenomenon recognized in visible light for centuries, finds extensive applications in manipulating light in optical systems such as telescopes and cameras. Magnetohydrodynamic wave is a common perturbation phenomenon in the corona. By using high spatio-temporal resolution observations from the Solar Dynamics Observatory, here, we report the observation of a magnetohydrodynamic wave lensing in the highly ionized and magnetized coronal plasma, where quasi-periodic wavefronts emanated from a flare converged at a specific point after traversing a coronal hole. The entire process resembles an electromagnetic wave lensing from the source to the focus. Meanwhile, the magnetohydrodynamic wave lensing is well reproduced through a magnetohydrodynamic numerical simulation with full spatio-temporal resolution. We further investigate potential applications for coronal seismology, as the lensing process encodes information on the Alfven´ speed, in conjunction with favorable geometric and density variations.
ST12-A016
Coordinated Transverse Motions in a System of Two Solar Coronal Loops with Elliptic Cross-sections
Bo LI#+, Mijie SHI, Shao-Xia CHEN, Mingzhe GUO
Shandong University
Imaging observations have demonstrated that cyclic transverse displacements of neighboring solar coronal loops may be coordinated. The cross-sections of individual loops, on the other hand, are suggested to be rarely circular. We adopt linear, ideal, pressureless magnetohydrodynamics (MHD) to examine axial fundamental transverse motions in a system of two identical, parallel, straight, coronal tubes, allowing for elliptic tube cross-sections and continuous transverse density variations from tube interior to the ambient corona. A finite-difference code is developed, and we focus on the period and damping time that best-fit the quasi-mode stage of the temporal evolution of internal motions. Our results for the case of circular cross-sections agree closely with those derived with the T-matrix formalism of scattering theory, thereby validating the two distinct approaches. For circular and elliptic cross-sections alike, the temporal attenuation of internal motions is accompanied by the development of small-scales around tube boundaries and the accumulation of perturbation energy densities around where the Alfven resonance is expected, suggesting the robustness of the notions of resonant absorption and phase mixing. Quantitatively, the periods and damping times depend both on the equilibrium configuration and on the symmetric and polarization properties of the internal flow patterns. When understood with kink mode theories of isolated tubes, the period (damping-time-to-period ratio) may return an axial Alfven time (inhomogeneity lengthscale) that deviates from the true value by some 20% (50%). We conclude that periods are more reliable a seismic parameter than damping times when standard seismological practice is applied to kink-like oscillations in multi-tube systems.
ST12-A008
Advances in the Study of Coronal Extreme Ultraviolet Waves
Yuandeng SHEN#+
Chinese Academy of Sciences
The hot and tenuous coronal plasma can support the propagation of various kinds of magnetohydrodynamic waves. In this talk, we mainly introduce two types of extreme ultraviolet (EUV) waves in the corona, namely, the large-scale EUV waves and the quasi-periodic fast-propagating (QFP) magnetosonic waves. Globally propagating EUV waves are intimately related to violent solar eruptions such as flares, coronal mass ejections, and the chromosphere Moreton waves. Due to the launch of space solar telescopes in the 1990s, large-scale EUV waves attracted a lot of attention from solar physicists due to two long-debating topics, i.e., it is unclear that large-scale EUV waves were driven by coronal mass ejections or flares, and whether they are true MHD waves or pseudo waves caused by coronal reconfigurations. Thanks to the high spatiotemporal resolution and multi-angle observations provided by advanced space and ground-based solar telescopes in recent years, we have achieved a deeper and complete understanding of the generation and physical properties of EUV waves. Besides, I will introduce the newly discovered QFP waves and their possible relationship to the large-scale EUV waves. In summary, we will present the main advances in the study of the two types of EUV waves in recent years, including observational and theoretical results.
ST12-A013
Excitation of Quasi-periodic Fast-propagating Waves in the Early Stage of the Solar Eruption
Jialiang HU#+
Chinese Academy of Sciences
We propose a mechanism for the excitation of large-scale quasi-periodic fast-propagating magnetoacoustic (QFP) waves observed on both sides of the coronal mass ejection (CME). Through a series of numerical experiments, we successfully simulated the quasi-static evolution of the equilibrium locations of the magnetic flux rope in response to the change of the background magnetic field, as well as the consequent loss of the equilibrium that eventually gives rise to the eruption. During the eruption, we identified QFP waves propagating radially outwards the flux rope, and tracing their origin reveals that they result from the disturbance within the flux rope. Acting as an imperfect waveguide, the flux rope allows the internal disturbance to escape to the outside successively via its surface, invoking the observed QFP waves. Furthermore, we synthesized the images of QFP waves on the basis of the data given by our simulations, and found the consistence with observations. This indicates that the leakage of the disturbance outside the flux rope could be a reasonable mechanism of QFP waves.
Session Chair(s): Honghong WU, Wuhan University
ST22-A005
Non-spherical Source Surface Potential Field Model for Coronal Magnetic Field Extrapolation
Ziqi WU#+, Jiansen HE, Rui ZHUO, Chuanpeng HOU, Tianhang CHEN
Peking University
The coronal magnetic field controls the genesis of the solar wind and initiates the solar eruption events. However, unlike the photospheric magnetic field, we cannot directly measure the coronal magnetic field but can only estimate it by extrapolation. A good extrapolation model is crucial to understanding the genesis of the solar wind, constructing heliospheric models, and forecasting space weather. The Potential Field Source Surface (PFSS) model is the most popular extrapolation model. It calculates the Poisson equations between the photosphere and the source surface based on the assumptions that (1) the coronal magnetic field is a potential field and (2) the magnetic potential is zero at the source surface. However, PFSS also presents many problems in practice, such as the arbitrary choice of source surface, underestimated open flux, and polarity mismatch with observations. As an optimization, our study presents a non-spheric source surface model with the Poisson equations calculated by the finite-element method in the irregular region between the photosphere and the source surface. This model performs better than PFSS, resulting in more sector boundaries on the source surface and more open flux. Hopefully, the non-spheric source surface model can give better results in magnetic field line tracing and solar wind model construction.
ST22-A002
| Invited
Solar Wind Velocity in the Outer Corona
Yuming WANG#+, Shaoyu LYU, Xiaolei LI, Jiajia LIU
University of Science and Technology of China
Based on the HI1 images of STEREO twin spacecraft, we established the CORrelation-Aided Reconstruction (CORAR) technique to locate and reconstruct the three dimensional (3D) structures of solar wind transients in the interplanetary space. Here, we extend the CORAR method to images of COR2 on board STEREO to study the evolution of small-scale transients in the outer corona from January to May 2010. We confirm that the transients can be located and reconstructed well by comparing the results with those of a self-similar expanding model. The speed distribution of the reconstructed transients generally shows the typical characteristic of slow solar wind. We further study the sources of the transients on the Sun, and find that most reconstructed transients are located near the top of streamer belts or the heliospheric current sheets and can be tracked back to the boundaries of closed-field and open-field regions along the field lines extrapolated by corona models. The formation mechanisms of these transients in the slow solar wind are also discussed.
ST22-A008
Spatial and Temporal Distribution of Velocities of Coronal Waves and Structures on Multiple Scales
Chuanpeng HOU1+, Jiansen HE1#, Alexis ROUILLARD2, Xiangjing XU1, Rui ZHUO1
1Peking University, 2Institute for Research in Astrophysics and Planetology/ Université Toulouse III—Paul Sabatier/ National Center for Scientific Research/ National Center for Space Studies
Waves and oscillations in the solar corona play a crucial role in various models related to the corona and solar wind environment, such as the formation of magnetic switchbacks through outward propagating waves and wave-wave interactions leading to turbulence, providing energy for heating the corona and solar wind. However, the coronal atmosphere is complex and dynamic, with a mixture of coronal plumes, waves, and eruptive activities at different scales. To better understand the wave environment and its subsequent impact on the corona and interplanetary solar wind, it is essential to quantitatively obtain the spatiotemporal distribution of coronal waves and structures at different scales and different propagation velocities under varying solar activity levels. SOHO/LASCO-C2 provides a means to study the corona at the nearest 1.4 solar radii (1.4Rs) from the solar surface, a region inaccessible to in situ probes. To achieve the above objectives, we develop a two-dimensional spatial + one-dimensional temporal wavelet transform procedure (wavelet-2D1T) and apply it to LASCO C2 images. We successfully obtain the spatiotemporal distribution of velocities for waves and structures under different solar activity levels. During the transit of Mars, the propagation velocities of disturbances in the corona can also be inferred through the disturbances of radio signals from Mars probes received by ground-based observatories. Hence, we could compare the velocities obtained through both methods. Additionally, we develop a graphical user interface (GUI) to facilitate the processing of LASCO-C2 images, the setting up of the wavelet-2D1T transform process, and the visualization of corresponding results.
ST22-A006
Flapping of Multifold Heliospheric Current Sheet
Rui ZHUO1#+, Jiansen HE1, Die DUAN2, Ziqi WU1, Chuanpeng HOU1
1Peking University, 2National University of Defense Technology
Observations of magnetotail current sheets on many planets, including Earth, Mercury, Venus, and Mars, show widely-existed flapping motion. As the most extensive current sheet in the heliosphere, however, there is no detailed conclusion about whether and how the heliospheric current sheet (HCS) flaps. Parker Solar Probe traversed HCS for five times serially near the perihelion of encounter 7. Based on MVA method and discontinuity type analysis, we find that HCS is multifold on a small scale, and at the same time, flapping upward and downward. The flapping speed is on the order of tens to hundreds km/s. Assuming that the velocity of solar wind is uniform over the same sphere, we construct a three-dimensional image of HCS, which illustrates what the flapping multifold HCS looks like. Our study shows that the heliospheric current sheet is neither flat nor static. Instead, multi-folding and flapping exist at the same time, and it's more complex than commonly thought. The dynamics at the source region of the multifold HCS in the solar atmosphere is also investigated, and its relation with the dynamics in the interplanetary space is discussed as well. This will lead us a deeper understanding of the 3D structure and motion of HCS.
ST22-A004
| Invited
Solar Close Observation and Proximity Experiments Mission Concept
Jun LIN#+
Chinese Academy of Sciences
The region close to the Sun is a totally unknown world to us, many important processes and phenomena occurring there are completely imperceptible on the Earth, and it is still an “uninhabited zone” for the deep space mission. This work is to introduce an unprecedented deep space mission that will enter the “uninhabited zone”, solving the puzzles that have challenged the solar physics society for around a century. These puzzles are related to the mechanisms for the solar eruption, detection of the coronal magnetic field, as well as the mechanism of the corona heating. The spacecraft will reach to the location closer to the Sun than the Parker Solar Probe would reach on an orbit of larger inclination to the ecliptic plane than the Solar Orbiter. The associated scientific goals include: 1. Entering the central structure of the energy release driving the solar eruption, performing in situ measurements of physical properties of the structure, and solving the problem of mechanisms of solar eruptions; 2. Acquiring the true thickness of the reconnecting current sheet connecting a coronal mass ejection to the associated solar flare, and renovating the classical theory and the physical scenario regarding the large-scale of magnetic reconnection; 3. Acquiring the coronal magnetic field via in situ measurement, obtaining unique evidence for identifying mechanisms of the corona heating, observing closely the polar magnetic field and plasma, revealing the role of the polar magnetic field and plasma in governing the global behavior of the solar activity.
Session Chair(s): Viktor FEDUN, The University of Sheffield, Chia-Hsien LIN, National Central University
ST17-A004
| Invited
Radiative Magnetohydrodynamic Simulations for Solar Surface Dynamics
Hideyuki HOTTA#+
Nagoya University
The solar surface is filled with turbulent thermal convection. The interaction between the turbulence and the magnetic fields leads to various phenomena, such as bright points, pores, and sunspots. There have been several efforts to understand these processes using numerical simulations. When the stratification, radiation energy transfer, partial ionization, and magnetohydrodynamic processes are appropriately treated, we can reproduce the solar surface well. In this talk, the efforts to understand the solar photosphere and current achievements are reviewed.
ST17-A005
Alfvén Pulse Driven Cool Jets in the Solar Chromosphere: Ideal MHD vs Two-fluid Regime
Abhishek Kumar SRIVASTAVA1#+, Balveer SINGH2, Kris MURAWSKI3, Bhola N. DWIVEDI4, Teimuraz ZAQARASHVILI5, Ding YUAN6, Eamon SCULLION7, Anshika SINGH1, Sudheer K MISHRA8
1Indian Institute of Technology (BHU), 2Aryabhatta Research Institute of Observational Sciences, 3Maria Curie-Skłodowska University, 4Rajiv Gandhi Institute of Petroleum Technology, 5University of Graz, 6Harbin Institute of Technology, 7Northumbria University, 8Kyoto University
The non-linear transverse velocity pulses akin of Alfvén pulses in 2.5-D numerical simulation of the realistic solar atmosphere, result in the evolution of field-aligned magnetoacoustic perturbations due to ponderomotive force. This further converts into the shocks while moving up into the stratified solar atmosphere. This process drives behind the cool spicule-like jets. In this presentation, we compare the entire physical process in ideal MHD and two-fluid regime. Comparative study demonstrates that in two fluid regime the spicule-like jets are reasonably formed when the thermal conduction and ion-neutral collisions are taken into account. These jets are able to transport substantial mass and energy flux into the solar atmosphere. They also exhibit the quasi-periodic rise and fall of the cooler plasma.
ST17-A003
System Level Babcock-Leighton Flux Transport Model-data Comparisons
Simon WING1#+, Jay JOHNSON2, Mausumi DIKPATI3
1The Johns Hopkins University, 2Andrews University, 3National Center for Atmospheric Research
System level Babcock-Leighton flux transport model-data comparisons were performed using information theory. The model was run with maximum meridional flow speed of 16.5 m/s with the flow speed is systematically varied by 20% (BLFT20) and 50% (BLFT50). Overall, the comparisons show that the model qualitatively captures the information flow among the toroidal field (proxied by the sun spot number), polar field (poloidal field), and meridional flow. BLFT20 generally compares better than BLFT50 suggesting that meridional flow variation of 20% generally may be more realistic than 50%. However, the information flow from the meridional flow to the polar field is captured better in BLFT50 than in BLFT20. This may suggest that perhaps the processes linking meridional flow to polar field has a stronger meridional variation. There is more information flow from the sunspot number to the polar field than the other way around in BLFT20. The information flow from the polar field to the sunspot number peaks at lag times (t) ~ 2 year and 7-9 years. The polar field from at least the last solar cycle carries information about the sunspot number in both BLFT20 and BLFT50, consistent with previous studies, which can shed light to the nature of the flux transport and its long term memory at the Sun. In particular, it can shed light on the nature of the diffusive/dissipative processes and advection in the turbulent flux transport. The larger the magnetic diffusivity, the shorter the memory and vice versa.
ST17-A002
Preliminary Investigations on the Relationship Between the Magnetic Pressure of Bipolar Pores with the Pore Movement and the Global Solar Magnetic Fields
Merlin MENDOZA#+, Chia-Hsien LIN
National Central University
Solar pores are small magnetic features whose locations at the photosphere represent the intersection, or foot points, of magnetic structures. Observations have shown that they are constantly in motion before either disappearing or evolving into a sunspot. Recent studies have shown that the direction of motion of pores, Φt, and the direction of maximum positive magnetic pressure difference, ΦdPo, are correlated with each other (Mendoza and Lin, 2023). In this work, we further examine the angle ΦdPo and the magnetic pressure difference between the front and back sides of the moving pores, ΔPmag, of 19 pairs of moving bipolar pores. We find that ΦdPo points towards greater or less than 180∘ and 0∘, depending on the magnetic field polarity of the pore and the polarity of the hemisphere where it is located, as defined by Hale’s Law. Specifically, ΦdPo is observed to be slightly pointing towards the north in the northern hemisphere and is slightly pointing towards the south in the southern hemisphere. Moreover, ΦdPo, for the leading and trailing pores of the bipolar pores are pointing in the same direction, either towards left or right, for both the northern and southern hemispheres. For the front – back difference of magnetic pressure, we find that the signs of ΔPmag averaged over the lifetime of the pores, ⟨ΔPmag⟩, for the leading and trailing pores of the bipolar moving pores are always opposite. That is, if one has +⟨ΔPmag⟩ the other one would have –⟨ΔPmag⟩.
ST17-A006
| Invited
What Kind of Problems in Solar Physics are Well Solved by Deep Learning?
Yong-Jae MOON#+
Kyung Hee University
In this talk, we introduce our recent applications of deep learning to solar and space weather data. We have successfully applied novel deep learning methods to the following applications: (1) image translations between solar images, (2) generation of UV/EUV images and magnetograms from Galileo sunspot drawings, (3) denoising solar magnetograms using supervised learning, (4) superresolution of solar magnetograms, (5) near real-time construction of solar coronal parameters based on MAS, (6) improvement of global IRI TEC maps using IGS TEC ones, (7) one-day forecasting of global TEC maps, (8) flare classification by CNN and visual explanation by attribution methods, (9) forecasting GOES solar X-ray profiles, and (10) three-day forecast of solar wind speed using solar images. We present major results and discuss what kinds of problems are well solved.
Session Chair(s): Kyungguk MIN, Chungnam National University
ST15-A001
On the Nonlinear Wave Growth Rate of Chorus Waves
Xin TAO1#+, Fulvio ZONCA2, Liu CHEN3
1University of Science and Technology of China, 2Italian National Agency for New Technologies, Energy and Sustainable Economic Development, 3Zhejiang University
Chorus waves, crucial for energetic electron dynamics in the Earth's radiation belts, are excited through nonlinear wave-particle interactions. However, the specific details of this amplification process remain debated. This talk presents a theoretical estimate of the nonlinear growth rate of chorus waves based on the recently proposed "Trap-Release-Amplify" (TaRA) model. We validate our results through comparison with computer simulations, revealing a remarkable similarity between chorus wave excitation and super-radiance in free electron lasers. Finally, we discuss the important physical implications of these findings.
ST15-A004
Characteristics of Wave-particle Power Transfer as a Function of Electron Pitch Angle in Nonlinear Chorus Excitation
Zeyin WU+, Xin TAO#
University of Science and Technology of China
Whistler mode chorus waves frequently appear as discrete, repetitive, and quasi-monochromatic emissions with frequency chirping. During the processes of wave generation and propagation, chorus waves can exchange energies with energetic electrons through nonlinear resonant interaction. Furthermore, the wave generation and electron distribution can be affected by the power transfer between electrons and chorus waves conversely. According to previous theoretical models of chorus wave, the pitch angle of the resonant electrons is one of the crucial parameters in the power transfer process. However, there are few researches specifically focusing on this parameter. Here we demonstrate several features of the resonant electrons’ pitch angle corresponding to the maximum power transfer through PIC simulations. The power transfer is shown to be concentrated around a specific pitch angle (about 60°) during the onset of the rising tone chorus wave. As the wave frequency increases, this pitch angle progressively increases, reaching 80° towards the end of the chorus element. Our results demonstrate that the resonant electrons with varying pitch angles contribute differently during nonlinear resonant interaction with chorus waves, and provide a good approximation of resonant pitch angle for the application of theoretical model of chorus wave.
ST15-A011
EMIC Wave Occurrence and Its Dependence on Geomagnetic Conditions: Results from 7 Years of Van Allen Probes Observations
Maria USANOVA#+
University of Colorado Boulder
Electromagnetic ion cyclotron (EMIC) waves are transverse plasma waves generated in the equatorial magnetosphere by ∼10–100 keV ion distributions with temperature anisotropy. EMIC waves can resonantly interact with multiple particle species, being an important loss process for both ring current ions and radiation belt electrons, as well as a cold plasma heating mechanism. They have been shown to act as an intermediary that couples energy and momentum between different energy magnetospheric plasma populations via various resonance mechanisms. In this talk, I will focus on the observations and statistical analysis of EMIC wave occurrence distribution from the NASA Van Allen Probes mission and discuss the importance of these results for modelling the dynamics of the inner magnetosphere.
ST15-A006
A Study of Energy Transfer by EMIC Propagation Using Arase Satellite and Ground-based Magnetometer Data
Jaeyoung KWAK1,2#+, Junga HWANG1, Yukinaga MIYASHITA1,2, Madeeha TALHA1,2, Yoshizumi MIYOSHI3, Kazuo SHIOKAWA3, Chae-Woo JUN4
1Korea Astronomy and Space Science Institute, 2Korea National University of Science and Technology, 3Nagoya University, 4University of California, Los Angeles
Pc1 waves detected by ground-based magnetometers are usually propagated from magnetospheric EMIC (electromagnetic ion cyclotron) waves. The EMIC waves are generated in several ways near plasmapause such as solar wind dynamic pressure or energetic particle injection from the magnetotail region. The EMIC waves undergo significant energy loss while they propagate along magnetic field lines and through the ionosphere. Although there have been many studies to investigate the characteristics of EMIC waves, only a few studies have focused on the entire life of the EMIC waves. In this study, we select and analyze magnetically conjugated EMIC wave events using MGF (Magnetic Field Experiment) on board Arase satellite and four different ground-based magnetometer data (MGD, MSR, STA, and BOH) which cover various L-value from L~1.22(STA) to L~2.89(MGD). The data period is from March 2017 to December 2023, which contains an entire available period of the Arase satellite data. We detect EMIC waves using both visual inspection and automatic wave detection algorithms. By observing the process from the creation to the extinction of the same waves, changes in the characteristics of EMIC waves and the degree of energy loss to the surrounding environment during the propagation process are revealed. This research was supported by the Young Scientist+ Research Program 2023 through the Korea National University of Science and Technology. (No. 2023YS19).
ST15-A012
Heavy Ion Effects on Filtered H-band EMIC Waves
Eun-Hwa KIM1#, Jay JOHNSON2+, Sung Jun NOH3, Mark ENGEBRETSON4, Khan-Hyuk KIM5, Wesley MARTIN2, Hyomin KIM6, Syun'ichi SHIRAIW1, Nicola BERTELLI1, Miles KIM2
1Princeton University, 2Andrews University, 3Los Alamos National Laboratory, 4Augsburg College, 5Kyung Hee University, 6New Jersey Institute of Technology
Left-handed polarized EMIC waves are generated by temperature anisotropy near the magnetic equator. These waves then propagate to the ground along the field line. H-band EMIC waves generated in frequency between H+ and He+ cyclotron frequencies often disappear during their propagation, which is termed "filtered H-band EMIC waves" [Noh et al., 2022]. In this presentation, we optimize heavy ion effects on H-mode EMIC wave propagation using the full-wave Petra-M code and reproduce wave spectra at lower and higher magnetic latitudes. We will also discuss the electron density effects on EMIC wave propagation. For the simulations, we utilize the global core plasma model (GCPM) in the Petra-M code. Since the GCPM's estimate of heavier ion density may not reflect realistic values, we assume a constant density profile for the heavier ions (He+ and O+) within the magnetosphere. Our findings reveal that a lower concentration of He+ and O+ ions above 3% can prevent wave propagation toward the Earth and cause filtering H-band EMIC waves.
ST15-A009
Prompt Appearance of Large-amplitude Emic Waves Induced by Solar Wind Dynamic Pressure Enhancement and the Subsequent Relativistic Electron Precipitation
Chao YUE#+, Yun YAN
Peking University
Electromagnetic ion cyclotron (EMIC) waves play an important role in relativistic electron dynamics. In this study, we find a large-amplitude EMIC wave event induced by the prompt enhancement of solar wind dynamic pressure on 6 November 2015. These large-amplitude EMIC waves are simultaneously observed by multiple satellites over 13 hr in magnetic local time (MLT) with a peak amplitude of ∼4 nT. Satellites at different locations observed different bands of EMIC waves, implying the importance of background plasma density in EMIC wave generation. Electron pitch angle distributions show obvious responses to EMIC wave activities. During EMIC wave appearance, the fluxes of relativistic electrons with pitch angles around 90° increase, while the fluxes of field-aligned relativistic electrons decrease, showing distinct “bite-out” signatures, indicating pitch angle scattering by EMIC waves, and the scattering efficiency depends on the amplitude and polarization of EMIC waves. Combined with phase space density profiles of electrons that are nearly constant at energies below the minimum resonant energy of electrons (Emin) but show dropout at energies above the Emin after EMIC wave activities, we conclude that large-amplitude EMIC waves can cause rapid electron loss down to several hundred keV. In addition, simultaneous observations of hundreds of keV electron precipitation and tens of keV proton precipitation by Polar Operational Environmental Satellites near the region where EMIC waves are observed, provide direct evidence of relativistic electron precipitation caused by the large-amplitude EMIC waves, ultimately driven by solar wind structures.
ST15-A003
Acceleration and Loss Processes of Radiation Belt Electrons Via Nonlinear Interactions with Whistler-mode Chorus Emissions
Yikai HSIEH#+, Yoshiharu OMURA
Kyoto University
Energetic electron accelerations and precipitations in the Earth’s outer radiation belt are highly associated with wave-particle interactions between whistler mode chorus waves and electrons. Two nonlinear processes, which change the energy and pitch angle of electrons effectively, take place in whistler mode wave-particle interactions. One is the nonlinear scattering, which makes electron energy slightly smaller. The other is the nonlinear trapping, which makes effective energy gain of the resonant electrons. We utilized the Green’s function method to reproduce the wave-particle interactions in the radiation belt and investigate the electron acceleration and precipitation interacting with both parallel and obliquely propagating chorus emissions. The formation processes and the loss processes of the outer radiation belt electron fluxes interacting with consecutive chorus emissions are traced by applying the convolution integrals for the Green’s functions. In the acceleration parts, MeV electrons are generated promptly due to the combination of cyclotron resonance and Landau resonance of oblique chorus waves. We compare the precipitation phenomena between parallel waves and oblique waves, and the results show that oblique chorus emissions lead to more electron precipitation than that led by parallel chorus emissions. Furthermore, we found that the acceleration process is stronger than the loss process, indicating that the radiation belt becomes stronger under the wave-particle interaction between chorus emissions and electrons comprehensively.
ST15-A007
Rapid Acceleration of Relativistic Protons by Electromagnetic Ion Cyclotron Waves in the Inner Jovian Magnetosphere
Yoshiharu OMURA1#+, Yikai HSIEH1, Danny SUMMERS2
1Kyoto University, 2Memorial University of Newfoundland
We present a physical mechanism for generating GeV protons in the Inner Jovian Magnetosphere [1], which may contribute to formation of the proton radiation belts. The mechanism consists of two nonlinear processes called anomalous trapping and relativistic turning acceleration (RTA) and involves a special form of nonlinear wave trapping by electromagnetic ion cyclotron (EMIC) waves. Necessary conditions for anomalous trapping and RTA include a near-equatorial source of EMIC waves, strong wave amplitudes (of the order of a few percent of the background magnetic field strength), and a source of protons of sufficiently high energy. The anomalous trapping occurs for energetic protons at low pitch angels, and it transports most of protons at low pitch angels to the energy and pitch angles satisfying the cyclotron resonance condition. Then the RTA occurs when the equator-ward moving protons encounter pole-ward moving EMIC waves, and they become entrapped and undergoes a turning motion due to increasing kinetic energy. The trapped ions then move poleward in the same direction as the waves and eventually become detrapped, but during the turning motion the ions undergo significant acceleration. We rigorously verify this process by providing the theory of nonlinear interactions between relativistic protons and coherent EMIC waves. The RTA process has been previously established for the analogous whistler mode wave-electron interaction. We confirm that a large portion of test protons experience RTA and that some protons of critical energy 240 MeV can be accelerated to 10GeV in a period of 5 seconds. References: [1] Sekine, T., Omura, Y., D. Summers, et al., Particle acceleration in Jupiter's ion radiation belts by nonlinear wave trapping, submitted to J. Geophys. Res. Space Phys., 2024.[2] Omura, Y., N. Furuya, and D. Summers (2007), J. Geophys. Res., 112, A06236, doi:10.1029/2006JA012243.
ST15-A002
Mapping Technique for Nonlinear Wave-particle Interactions
Anton ARTEMYEV#+
University of California, Los Angeles
The resonant interaction of energetic electrons and whistler-mode waves is an important mechanism of electron acceleration and scattering in the planetary radiation belts, solar wind, and at planetary bow shocks. For low amplitude waves, such an interaction is well described by the quasi-linear diffusion theory, whereas nonlinear resonant effects induced by high-amplitude waves are mostly investigated (analytically and numerically) using the test particle approach. This presentation overviews a mapping technique for the description of this nonlinear resonant interaction. We provide basic details of this technique and show multiple examples of it’s application.
Session Chair(s): Dedong WANG, GFZ Helmholtz Centre for Geosciences
ST16-A003
Statistical Analysis of Radiation Belt Electron Phase Space Density Profiles: From KeV Up to Multi-MeV
Alexander DROZDOV1#+, Anthony SAIKIN2, Quintin SCHILLER3, Allison JAYNES4, Dmitri KONDRASHOV2, Yuri SHPRITS5
1The Aerospace Corporation, 2University of California, Los Angeles, 3Space Sciences Innovations Inc, 4The University of Iowa, 5GFZ German Research Centre for Geosciences
Separating adiabatic and nonadiabatic changes can be achieved by analysis of phase space density (PSD) profiles revealing various mechanisms. Local acceleration results in growing PSD peaks, while localized rapid losses create deepening PSD minima. Radial diffusion typically shows a monotonic profile. Under unusually low plasma density conditions, local multi-MeV electron acceleration can occur through chorus wave-particle interactions, leading to the formation of growing PSD peaks signature. However, the role of radial diffusion and source population in the process of the multi-MeV electron enchantments remains unclear. The electron rapid loss can result from outward radial diffusion and wave-particle interaction, such as with electromagnetic ion cyclotron (EMIC) waves (with assistance of chorus, hiss and other waves), contributing to deepening PSD minima. However, the deepening PSD minima are observed at energies of ~10s-100s KeV, which are below the EMIC wave resonance energy. Those minima are likely resulting from hiss wave scattering and their corresponding L-shell-dependent lifetimes. In this study, we present a statistical analysis of PSD profiles using observations from Van Allen Probes and Geostationary Operational Environmental Satellite (GOES). Our analysis covers a wide energy range indicating a clear difference between KeV and multi-MeV electron populations. Furthermore, we investigate the controlling processes that shape the observed statistical distribution of PSD profiles performing a series of sensitivity tests, using the Versatile Electron Radiation Belts (VERB) code.
ST16-A002
| Invited
Why Chorus Waves are the Dominant Driver for Diffuse Auroral Precipitation
Xinliang GAO#+, Quanming LU
University of Science and Technology of China
Earth’s diffuse aurora, a widespread and featureless glow in the sky, is primarily caused by the atmospheric precipitation of 0.1-30 keV plasma sheet electrons. It significantly changes atmospheric chemical composition and ionospheric conductivity. Two distinct drivers, electrostatic electron cyclotron harmonic (ECH) waves and whistler-mode chorus waves, were proposed to explain diffuse aurora. Theories predicted that both waves should be equally important in scattering plasma sheet electrons, but observations showed that chorus waves are the dominant driver for diffuse auroral precipitation. How to resolve this contradiction remains a long-lasting challenge. Here, based on an analysis of multiple satellite data and computer simulations, we uncover the previously unseen fact that chorus and ECH waves are not independent. Surprisingly, chorus waves globally suppress ECH waves by rapidly reshaping the velocity distribution of electrons, leaving chorus waves as the primary contributor to diffuse auroral precipitation. The dominance of chorus waves is a natural consequence of the interplay between two waves. These findings represent an important step towards a more complete physical understanding of Earth’s and other magnetized planetary diffuse aurora.
ST16-A006
| Invited
Conjugate Observations of Magnetospheric and Ionospheric Phenomena During a Substorm Event
Shangchun TENG#+
The University of Hong Kong
This study investigates the comprehensive magnetospheric and ionospheric phenomena during a substorm event on December 14, 2013. The methodology involves analyzing data from satellites located within the plasmasphere at dusk-side of the Earth, as well as data from ionospheric satellites mapped in the subauroral region. Magnetospheric data were analyzed to identify key features during the substorm event. Proton injection into the ring current, presence of proton and helium band electromagnetic ion cyclotron (EMIC) waves with different polarization characteristics, and harmonic structures in these EMIC waves were identified. These harmonic structures coincided with the appearance of magnetosonic waves characterized by rising tone structures and heating of low-energy protons (<100 eV). Ionospheric satellites (DMSP F17 and POES 15) recorded enhanced proton precipitation contributing to the intensification of subauroral proton arcs. The analysis revealed that these enhanced proton fluxes were associated with variations in field-aligned currents (FACs) and drove dynamics within the Sub-Auroral Polarization Streams (SAPS). By combining and analyzing the magnetospheric and ionospheric datasets, this study provides a comprehensive understanding of magnetosphere-ionosphere coupling during substorms, particularly on the duskside. The complex interdependence and causal relationships among EMIC waves, proton precipitation, subauroral proton arcs, FAC variations, and SAPS dynamics were highlighted.
ST16-A014
Modeling of Ionospheric Conductivity Driven by Magnetospheric Electron Precipitation Using SPEAH-RIT and STET Codes
Suk-Bin KANG1#+, George KHAZANOV2, Alex GLOCER2, Qianli MA3,4
1CUA IACS/ NASA GSFC, 2NASA Goddard Space Flight Center, 3Boston University, 4University of California, Los Angeles
Magnetosphere-Ionosphere-Thermosphere are intimately coupled through particle transport, current system, and thermodynamics. Energetic (> 1 keV) electron precipitation from the magnetosphere deposit a significant amount of energy to the upper atmosphere during geomagnetically active times. Most of the energy deposited to the upper atmosphere is converted to impact ionization energy and increase ionospheric density and consequent conductivity. We simulate ionospheric conductivity and its variations due to electron precipitation using Superthermal Proton, Electron, Atomic Hydrogen tRansport in the Ionosphere and Thermosphere (SPEAH-RIT) and SuperThermal Electron Transport (STET) codes. We also calculate ionospheric conductance by integrating the altitudinal profile of the simulated conductivity and compare it to that estimated using a parameterized conductance, which is widely used in our community.
ST16-A005
| Invited
Generation of Traveling Ionospheric Disturbances and Equatorial Plasma Bubbles After the 2022 Tonga Volcanic Eruption
Atsuki SHINBORI1#+, Takuya SORI1, Nozomu NISHITANI1, Yoshizumi MIYOSHI1, Michi NISHIOKA2, Septi PERWITASARI2, Takuo TSUDA3, Nozomu NISHITANI1, Atsushi KUMAMOTO4, Fuminori TSUCHIYA4, Shoya MATSUDA5, Yoshiya KASAHARA5, Ayako MATSUOKA6, Iku SHINOHARA7, Yuichi OTSUKA1
1Nagoya University, 2National Institute of Information and Communications Technology, 3University of Electro-Communications, 4Tohoku University, 5Kanazawa University, 6Kyoto University, 7Japan Aerospace Exploration Agency
The Earth’s ionosphere is formed by a partial ionization of the upper atmosphere due to solar extreme ultraviolet radiation and particle precipitation from the magnetosphere. The electron density variation in the ionosphere is caused by both solar activities and lower atmospheric disturbances. Because this region influences the propagation of radio signals from global navigation satellite systems (GNSS) with its electrically charged particles, it is important to understand the generation mechanism of the electron density variation in the ionosphere associated with solar flares, geomagnetic storms, earthquakes, tsunamis, volcanic eruptions, and meteorological phenomena. The Tonga undersea volcanic eruption that occurred at 04:15 UT on 15 January 2022 is one of the most explosive events in the modern era, and a vertical plume reached approximately 55 km, corresponding to a height of the lower mesosphere. The intense explosion and subsequent plume generated acoustic and atmospheric gravity waves detected by ground-based instruments worldwide. Because a global-scale atmospheric and ionospheric response to such the large volcanic eruption has not yet been observed, it provides a unique opportunity to promote interdisciplinary studies of coupling processes in lithosphere-atmosphere-ionosphere-plasmasphere with ground-based and satellite observations (GNSS, SuperDARN, Arase, and Himawari-8). The Tonga volcanic eruption allows us to elucidate the propagation and occurrence features of traveling ionospheric disturbances, the generation of equatorial plasma bubbles, the cause of electron density holes around the volcano, and the magnetic conjugacy of magnetic field perturbations. In this talk, we will introduce an overview of ionospheric disturbances after the Tonga volcanic eruption and summarize what we know from this extreme event analysis.
Session Chair(s): Hongqiang SONG, Shandong University
ST14-A025
| Invited
Investigate Solar Eruptions with the Lyman-alpha Solar Telescope Aboard the ASO-S Mission
Li FENG#+
Chinese Academy of Sciences
The ASO-S mission has three payloads, a Full-disk vector MagnetoGraph (FMG) to measure photospheric magnetic Fields, a Hard X-ray Imager (HXI) to observe non-thermal signals from 30 to 200 keV, and Lyman-alpha Solar Telescope (LST) to take images of the Sun in Lyman-alpha and white light. In this presentation, we focus in the LST payload including the introduction to its three instruments, the current calibration progresses, and early observations. Particularly, we will discuss the properties of a failed eruption in the frame of the breakout model, the wave driven by a CME from the chromosphere to corona, and diagnostics of prominences by combining Lyman alpha and other wavelengths, etc.
ST14-A039
Parameter Effects on the Total Intensity of H I Lyman-alpha Line for a Modeled CME and Its Driven Shock
Beili YING#+, Li FENG
Chinese Academy of Sciences
The combination of the H I Lyman-alpha (121.6 nm) line formation mechanism with ultraviolet (UV) Lyman-alpha and white-light (WL) observations provides an effective method for determining the electron temperature of coronal mass ejections (CMEs). A key to ensuring the accuracy of this diagnostic technique is the precise calculation of theoretical Lyman-alpha intensities. This study performs a modelled CME and its driven shock via the three-dimensional numerical magneto-hydrodynamic simulation. Then, we generate synthetic UV and WL images of the CME and shock within a few solar radii to quantify the impact of different assumptions on the theoretical Lyman-alpha intensities, such as the incident intensity of the solar chromospheric Lyman-alpha line (Idisk), the geometric scattering function (p(theta)), and the kinetic temperature (Tn) assumed to be equal to either the proton (Tp) or electron (Te) temperatures. By comparing differences of the Lyman-alpha intensities of the CME and shock under these assumptions, we find that: (1) Using the uniform or Carrington maps of the disk Lyman-alpha emission Idisk as the incident emission underestimates the corona Lyman-alpha intensity (<10%) compared to the synchronic map, but the Carrington map yields better results than the uniform disk. (2) Neglecting the geometric scattering process leads to a relatively symmetric influence, with an error reversal interface at a latitude of approximately 40°. The Lyman-alpha intensity is overestimated above this latitude and underestimated below it. The relative errors increase with heliocentric distance, but do not exceed 10%. (3) Compared to the assumption Tn=Tp, using Tn=Te leads to more complex relative errors in CME Lyman-alpha intensity. The CME core and void are mostly overestimated, with maximum values exceeding 50%. In the CME front, both overestimates and underestimates exist( <35%). However, the electron temperature assumption has a smaller impact on the shock, with an underestimated relative error of less than 20%.
ST14-A044
| Invited
On Coronal Mass Ejection Initiation and Interplanetary Propagation
Nat GOPALSWAMY#+
NASA Goddard Space Flight Center
The current paradigm of coronal mass ejections is that magnetic reconnection in closed magnetic field regions results in the formation of a post eruption arcade at the Sun and a coronal mass ejection (CME) flux rope that propagates into the interplanetary medium. This flare reconnection usually follows when a seed flux rope becomes unstable. A recent finding is that the time evolution of the reconnected flux is similar to that of CME acceleration and the associated complex type III radio burst, confirming the simultaneous origin of the flare and CME in an eruption. One of the recently found effects on CME propagation is the back-reaction of the weak heliosphere on flux ropes that alters flux rope magnetic properties. This paper will summarize these results.
ST14-A002
Filament Eruption by Multiple Reconnections
Guiping RUAN1#+, Yang LIU1, Jinhan GUO2, Brigitte SCHMIEDER3, Yao CHEN1, Ruisheng ZHENG1, Jiangtao SU4, Bing WANG1
1Shandong University, 2Nanjing University, 3Observatoire de Paris/ Université PSL/ National Centre for Scientific Research/ Sorbonne Université/ Université de Paris, 4Chinese Academy of Sciences
We report on a filament eruption accompanied by a halo CME observed by the Global Oscillation Network Group (GONG), the Solar Terrestrial Relations Observatory (STEREO), the Solar Upper Transition Region Imager (SUTRI), the Atmospheric Imaging Assembly (AIA) and Helioseismic and Magnetic Imager (HMI) aboard the Solar Dynamic Observatory (SDO). We analyze the evolution of the fine structure in detail during the filament eruption. The filament changes its direction during the whole eruption process which contains multiple magnetic reconnections. We performed two models to explain this event. The first one is the NLFFF extrapolation, which is to construct the magnetic structures of the active region, particularly for the eruptive filament. The second one is a global model performed by COCONUT, which is obtained by the MHD relaxation process from the PFSS model coupling the polytropic solar wind. This model demonstrates the existence of open-field lines near the filament channel which explain coronal dimming and radio bursts very well. The result of extrapolation supports our speculation well.
ST14-A018
Interplanetary Magnetic Field Evolution of Coronal Mass Ejection from BepiColombo at 0.67 Au Up to Mars
Yutian CHI1#+, Chenglong SHEN2, Dongwei MAO2, Zhihui ZHONG2, Zhiyong ZHANG2, Yuming WANG2
1Deep Space Exploration Laboratory, 2University of Science and Technology of China
The goal of this study is to understand the magnetic field evolution of an ICME event detected by pairs of aligned spacecraft at different heliocentric distances. In this work, we report a CME event that was detected by the BepiColombo spacecraft (0.67 AU) and Tianwen-1 & MAVEN (1.66 AU) in-situ measurements, respectively. We found that the dependence of the maximum (mean) magnetic field strength of the ICME at the two points decreases with heliocentric distance as r−1.07 (r−1.29). The axial magnetic field strength (B0) derived from the force-free flux rope model decreases with heliocentric distance as r−1.78, suggesting that the in-situ observations may show the CME may not expand in a self-similar manner due to the spacecraft crossing the flux rope in a different region. Utilizing the deflection in interplanetary space, we reconstruct the trajectory of the CME spanning from 21.5 Rs to 342 Rs under the constraints of the CME initial velocity and the simulated solar wind velocity. We present solid evidence that the fast CME event was deflected toward the east in the interplanetary by approximately 16◦ at BepiColombo and 31◦ at Mars. The axis of the CME shows a clear clockwise rotation from 10.27◦ at BepiColombo to -12.45◦ at Mars. The 3D coronal rope ejection model (3DCORE) model, DIPS model, and the reconstructed CME magnetic field structure and orientation were found to be in good agreement with each other. The analysis of this event highlights the inherent innovative potential in Tianwen-1’s magnetometer data, presenting a novel avenue for investigating magnetic clouds encircling Mars. Observations capturing the same magnetic cloud at various heliocentric distances present an unprecedented opportunity to scrutinize the cloud’s magnetic properties and their evolution relative to distance.
ST14-A020
Three-dimensional Simulation of Thermodynamical Turbulence During a Coronal Mass Ejection
Jing YE1#+, John C. RAYMOOND2, Zhixing MEI1, Jun LIN1
1Chinese Academy of Sciences, 2Center for Astrophysics | Harvard & Smithsonian
Turbulence plays a key role in forming the complex geometry of the large-scale current sheet (CS) and fast energy release in a solar eruption. In this paper, we present full 3D high-resolution simulations for the process of a moderate coronal mass ejection (CME) and the thermodynamical evolution of the highly confined CS. Copious elongated blobs are generated owing to tearing and plasmoid instabilities, giving rise to a higher reconnection rate, and undergo the splitting, merging, and kinking processes in a more complex way in 3D. A detailed thermodynamical analysis shows that the CS is mainly heated by adiabatic and numerical viscous terms, and thermal conduction is the dominant factor that balances the energy inside the CS. Accordingly, the temperature of the CS reaches to a maximum of about 20 MK, and the range of temperatures is relatively narrow. From the faceon view in the synthetic Atmospheric Imaging Assembly 131 Å, the downflowing structures with similar morphology to supra-arcade downflows are mainly located between the post-flare loops and loop top, while moving blobs can extend spikes higher above the loop top. The downward-moving plasmoids can keep the twisted magnetic field configuration until the annihilation at the flare loop top, indicating that plasmoid reconnection dominates in the lower CS. Meanwhile, the upward-moving ones turn into turbulent structures before arriving at the bottom of the CME, implying that turbulent reconnection dominates in the upper CS. The spatial distributions of the turbulent energy and anisotropy are addressed, which show a significant variation in the spectra with height.
ST14-A008
On-disk Observation of Bidirectionally Propagating Plasma Blobs Near the Reconnection Site of a Solar Eruption
Zhenyong HOU1+, Hui TIAN1#, Maria MADJARSKA2, Hechao CHEN3, Tanmoy SAMANTA4, Xianyong BAI5, Zhentong LI5, Yang SU6, Wei CHEN5, Yuanyong DENG7, Hongqiang SONG8
1Peking University, 2Max Planck Institute for Solar System Research, 3Yunnan University, 4Indian Institute of Astrophysics, 5Chinese Academy of Sciences, 6Purple Mountain Observatory, Chinese Academy of Sciences, 7National Astronomical Observatories, Chinese Academay of Sciences, 8Shandong University
Current sheet is a commonly observed structure involved in solar eruptions. However, the physical properties of its fine structures during a solar eruption are rarely investigated. Here, we report an on-disk observation that displays 139 compact, circular or elliptic bright structures, presumably plasma blobs, propagating bidirectionally along a plasma sheet during a period of about 24 minutes around the peak time of an eruptive flare. From extreme ultraviolet images, we distinguish a plasma sheet connecting the flare loops and the erupting filament. The average width, duration, and projected velocities of these blobs are about 1.7$\pm$0.5 Mm, about 73$\pm$54 s, and about 190$\pm$81 km s$ ^{-1}$, respectively. The reconnection site rises with an average velocity of about 51 km s$ ^{-1}$. We have obtained the temporal variation of the blob number during the solar eruption, which is similar to that of the GOES X-ray flux. The observational results suggest that plasmoid instability plays an important role in the energy release process of solar eruptions.
ST14-A022
A Comparative Study Between the Eruptive and Confined Flares in a Newly Emerged Active Region
Hanzhao YANG#+
Sun Yat-sen University
Solar active regions (ARs) are the main sources of flares and coronal mass ejections (CMEs). However, the origin of CMEs is still uncertain. NOAA AR 12089, which appeared on 2014 June 10, produced 11 C-class and one M-class flares during its transit. Within four hours after the AR emerged, the first two C-class flares occurred and were accompanied with CMEs, while the subsequent flares were confined. To investigate why the AR produced eruptive flares so early, we compare the AR magnetic environment of the two eruptive flares to the largest confined flare (M1.1). We calculate the mean characteristic twist parameter (αFPIL) within the flaring polarity inversion line (FPIL) mask region versus the total unsigned magnetic flux of the AR (ΦAR) for the three flares, which considers the effects of both background magnetic field constraint and non-potentiality of the core region. We find that the αFPIL/ΦAR during the two eruptive flares is larger than the confined one. Furthermore, we compute the decay index along the polarity inversion line (PIL) before the onset of the three flares, revealing values of 1.77, 2.50, and 1.14, respectively. These results suggest that torus instability is the triggering mechanism of CMEs in this case. Finally, using the nonlinear force-free field extrapolation, the evolution of the corona magnetic field was investigated. The results indicate that a flux rope was formed through flux cancellation along the FPIL, which then ejected out and produced CMEs. Our research suggests that even for a newly emerged, small active region, if it has sufficiently weak background field constraint and strong non-potentiality, it can produce eruptive flares.
Session Chair(s): Alexandra FOGG, Dublin Institute for Advanced Studies, Chun-Sung JAO, National Cheng Kung University, Amar KAKAD, Indian Institute of Geomagnetism
ST32-A001
| Invited
Numerical Algorithms for Generating Loss-cone Distributions in Particle Simulation
Seiji ZENITANI1#+, Shinya NAKANO2
1Austrian Academy of Sciences, 2The Institute of Statistical Mathematics
Numerical algorithms to generate random variates that follow loss-cone velocity distributions in particle simulations are presented. We present loss-less Monte-Carlo methods for a subtracted Maxwellian, a Dory distribution, and a Kappa loss-cone distribution. For the subtracted Maxwellian, we propose a simple summation algorithm. For the Dory distribution, we utilize a gamma variate. For the kappa loss-cone distribution, we combine the gamma-variate method and an earlier method for the kappa distribution. We further discuss loss-cone distributions that are based on the pitch angle. We propose a novel algorithm that transforms an isotropic distribution into a pitch-angle-type loss-cone distribution, with help from a beta random variate.
ST32-A002
Solar Wind Interaction with Earth's Magnetosphere for a Time-varying Plasma and Magnetic Field: Global, Realistic, 3D Hybrid-kinetic Simulations
Shahab FATEMI#+
Umeå University
We present, for the first time, the global three-dimensional kinetic interaction between the solar wind and the entire magnetosphere of Earth using its true scales. Achieving this level of accuracy in kinetic modeling of the solar wind plasma interaction with Earth has been a long-standing challenge. We use Amitis, a high-performance hybrid-kinetic plasma model (particle ions, fluid electrons). Our model is three-dimensional (3D) in both configuration and velocity spaces and runs in parallel on Graphics Processing Units (GPUs). Our simulations incorporate typical solar wind plasma conditions near Earth, exploring a spectrum of time-varying Interplanetary Magnetic Field (IMF) orientations and solar wind dynamic pressure variations. The spatial and temporal scales of the magnetosphere are physically represented in our model, and no scaling has been applied in our simulations. We investigate the dynamic response of the foreshock, bow shock, and magnetopause to varying IMF orientations and solar wind variations, covering physical time scales exceeding an hour. Significantly, our study underscores substantial disparities between the outcomes derived from our hybrid-kinetic model and those obtained from Magnetohydrodynamics (MHD) simulations.
ST32-A003
| Invited
GCPIC Simulation of Whistler-mode Chorus Wave Generation and Associated Resonant Electron Signatures
Xueyi WANG1#+, Yoshiharu OMURA2, Huayue CHEN1, Yikai HSIEH2, Lunjin CHEN3, Yu LIN1, Xiao-Jia ZHANG3, Zhiyang XIA3
1Auburn University, 2Kyoto University, 3The University of Texas at Dallas
A 2-D GCPIC simulation in a dipole field system has been conducted to explore the excitation of oblique whistler mode chorus waves driven by energetic electrons with temperature anisotropy. It is found that the rising tone element of chorus waves with frequency chirping from low frequency to up to higher than the half electron gyro-frequency is generated at low latitudes. As the chorus wave propagates toward high latitudes, the wave becomes oblique and both the Landau and cyclotron resonance become significant. Two bands chorus waves are thus formed. In addition, we have found that electron holes in the wave phase space, which form due to nonlinear cyclotron resonance, oscillate in size with time during chorus wave subpacket formation. The associated inhomogeneity factor varies accordingly, giving rise to various frequency chirping in different phases of subpackets. Distinct nongyrotropic electron distributions are detected in both wave gyrophase and stationary gyrophase. The nonlinear physics associated with the wave growth and wave frequency chirping has been quantitatively evaluated in the process of chorus wave development.
ST32-A012
Externally Driven Field Line Resonance Polarization in a General Magnetospheric Geometry
Alex DEGELING1#+, Robert RANKIN2, Colin WATERS3, Andrew WRIGHT4
1Shandong University, 2University of Alberta, 3The University of Newcastle, 4University of St Andrews
The question of interest in this study is: Given the external driving of monochromatic MHD fast mode waves into the magnetosphere, what determines the location and polarization of (fundamental mode) field line resonances (FLRs), in the general case of a non-axisymmetric Alfvén speed and magnetic field topology? This is of particular interest for considering the role of FLRs, or Shear Alfvén Wave (SAW) eigenfunctions, in radiation belt and ring current particle energization, transport and loss by resonant wave-particle interactions. In particular, we seek to determine whether or not the SAW polarization direction remains constant as a function of position along a given field line with respect to neighbouring field lines, as has been assumed in previous studies. In addressing this question we seek to extend the works of: a) Wright et al., (Astrophys. J., 2016, J. Geophys. Res. 2021), which considered the case of a non-axisymmetric Alfvén speed in a dipole and compressed dipole magnetic fields (making the above assumption); and b) Rankin et al. (Adv. Space Res., 2006) and Kabin et al., (Ann. Geophys., 2007), which considered an arbitrary magnetic geometry, but made no constraints SAW polarization. A new formulation is proposed in which a constraint on polarization is imposed only in an average sense, which provides the degree of freedom necessary to define Resonance Zones similar to those of Wright et al, but also provides a means for the local magnetic field line properties (such as curvature and torsion) to affect the SAW polarization. The results of the new formulation are compared against the previous theories for the case of a dipole and more general compressed dipole field, and are compared against 3D MHD simulations of FLRs externally driven by fast mode waves in both magnetic field scenarios.
ST32-A011
Nonlinear Drift-bounce Resonance Between Charged Particles and Ultralow Frequency Waves
Li LI1#+, Xuzhi ZHOU2, Yoshiharu OMURA3, Qiugang ZONG2
1China University of Geosciences, 2Peking University, 3Kyoto University
Ultra-low frequency (ULF) waves contribute significantly to the dynamic evolution of Earth's magnetosphere by accelerating and transporting charged particles within a wide energy range. A substantial excitation mechanism of these waves is their drift-bounce resonant interactions with magnetospheric particles. Here, we extend the conventional drift-bounce resonance theory to formulate the nonlinear particle trapping in the ULF wave-carried potential well, which can be approximately described by a pendulum equation. We also predict the observable signatures of the nonlinear drift-bounce resonance, and compare them with spacecraft observations. We further discuss potential drivers of the pendulum including the convection electric field and the magnetospheric dayside compression, which lead to additional particle acceleration or deceleration depending on magnetic longitude. These drivers indicate preferred regions for nonlinear ULF wave growth, which are consistent with previous statistical studies.
ST32-A008
Multiple Auroras Induced by Interplanetary Shock: Plasma Wave Effects
Xingxin ZHAO1+, Qiugang ZONG2#, Jianjun LIU1, Zejun HU1
1Polar Research Institute of China, 2Peking University
Aurora, as a visualized space weather phenomena, often occurs with the increasing space weather activity like storms and substorms. These auroras, no matter structured or structureless, are related to the depositions of energy electrons or ions which may result from the wave-particle interactions. In this study, we present an event in which different auroras corresponding to different frequency waves are induced by interplanetary (IP) shock. At dawn side, the brightness of diffuse auroras observed by Yellow River station enhances after IP shock, while both Van Allen Probe A and THEMIS-D nearby observe the enhancements of whistler waves (with frequency range from 0.1fce to 0.5fce). At dusk side, periodic aurora arcs of 8min period are observed by Kaktovik station, with similar frequency ULF waves observed by nearby ground-based magnetometers. It suggests that IP shock excited ULF waves and whistler waves which results in the depositions of electrons via wave-particle interactions and finally result in auroras.
ST32-A006
Nighttime Geomagnetic Response to Solar Wind Dynamic Pressure Pulses
Tian ZHANG1#+, Yusuke EBIHARA1, Takashi TANAKA2
1Kyoto University, 2Kyushu University
By performing a global magnetohydrodynamic (MHD) simulation, we investigate the ground magnetic disturbances at high latitudes in response to solar wind dynamic pressure pulses, namely a sudden commencement (SC). The motion of the SC-associated field-aligned currents (FACs) in the ionosphere is shown during both preliminary impulse and main impulse (PI and MI). Large magnetic disturbances are found during MI on the nightside under large jumps of the solar wind pressure. The contributions from the FACs and the ionospheric currents to the magnetic response in high-latitude region are compared. In particular, the MI-associated Hall current flows sunward (anti-sunward) resulting in large northward (southward) ground magnetic disturbances at higher (lower) latitude in the post-midnight sector. The similar results are also found in the observations from North Europe and Canada. It is suggested that the blackout in Québec may be caused by the MI-associated Hall current during the SC passing over the Hydro-Québec power system on the nightside in March, 1989. The possible generation region and mechanism of the SC-associated FACs are under investigation.
ST32-A007
| Invited
Simulation Study of the Magnetosphere-ionosphere Response to the Solar Wind Impulse
Shigeru FUJITA#+
The Institute of Statistical Mathematics
A geomagnetic sudden onset (SC) is a magnetospheric response to sudden changes in the solar wind dynamic pressure, with distinctive plasma and magnetic field disturbances in the magnetosphere-ionosphere region. Because the SC is identified as a remarkable sudden change in the ground magnetic field, the SC has attracted the interest of many space scientists for a long time [Sano and Nagano, 2021]. Since then, SC has been extensively investigated based on observations made not only at the Earth's surface but also in the region up to the magnetosphere. A schematic model of SC was presented by Araki (1994) who summarized many observations and theories related to this phenomenon known up to that time. On the other hand, recent advances in supercomputing allow us to present new numerical results including three-dimensional global behaviors of the SC which cannot be obtained only by direct observations and theoretical analysis. The simulation study not only confirms the results of a previous model on the initial response of the magnetosphere-ionosphere system to solar wind changes (the preliminary impulse, PI) but also presents new findings on dynamical processes in the magnetosphere-ionosphere system in the period following the initial response (the main impulse, MI). Furthermore, the simulation also revealed a new physical process in the PI current system that had previously been observed but whose cause was unknown. Finally, the simulation study proposes the SC sequence in the context of the break and recovery of the steady magnetosphere-ionosphere convection system. The transient flow vortex in the flank magnetosphere in the main impulse phase plays an essential role in recovering the convection system. In the last, we would like to present newly discovered simulation results. References: Araki, in Solar Wind Sources of Magnetospheric Ultra-Low-Frequency Waves, AGU, 183, 1994.Sano and Nagano, Hist. Geo Space. Sci., https://doi.org/10.5194/hgss-12-131-2021, 2021.
Session Chair(s): Li FENG, Chinese Academy of Sciences
ST14-A021
| Invited
What Determines the Initiation of Solar Flares and Coronal Mass Ejections?
Kanya KUSANO#+
Nagoya University
Since solar flares and coronal mass ejections (CMEs) are the primary causes of space weather disturbances, predicting their occurrence and properties is an important research subject. However, since our predictive capability is not yet high enough, it is necessary to improve our understanding of what determines their initiation to improve predictability. We proposed the theoretical hypothesis that magnetic reconnection on the polarity inversion line may trigger the onset of an ideal magnetohydrodynamic (MHD) instability, which causes solar flares (Ishiguro & Kusano 2017 ApJ). We developed a new flare prediction scheme (kappa-scheme) based on this model and demonstrated that the kappa-scheme is able to predict large flares not only for the occurrence but also the onset location with a few exceptions (Kusano et al. 2020 Science). In addition, we conducted research to find parameters for determining eruptive flares accompanied by CMEs, using the non-linear force-free field extrapolated from vector magnetic field observation (Lin et al. 2020, and 2021 ApJ). In this lecture, first, I will review the results and challenges of those studies. Second, to clarify the problem in understanding the flare initiation mechanism, we will consider the characteristics of the flares that cannot be predicted by the kappa-scheme and present the issues necessary for more advanced flare prediction. Third, we discuss what determines the eruptivity of solar active regions by clarifying the characteristics of events in which the previous models failed to discriminate eruptive and non-eruptive flares.
ST14-A034
Magnetohydrodynamic Simulations of Explosive Solar Eruption Triggered by Small-scale Emerging Flux
Satoshi INOUE#+, Huu Minh Triet NGUYEN, Haimin WANG
New Jersey Institute of Technology
The initiation mechanism of the solar eruption is one of the key questions in solar physics. Recent high-resolution observation by Goode Solar Telescope found small-scale emerging flux at the local area of the solar active region just before the fare (Wang et al. 2017). Therefore the small-scale emerging flux is suggested to trigger or assist the eruption. In this study, we perform magnetohydrodynamic simulations of solar eruption using a coronal magnetic field based on the theoretical model to investigate the detailed eruption process triggered by small-scale emerging flux. First, we prepare the bipolar magnetic field assumed as the sunspots from which the potential field is extrapolated. Next, the twisting motion is imposed on the bottom surface to form highly sheared field lines. Finally, a small emerging flux, which has the opposite polarity to the pre-existing bipolar magnetic field, is given at the bottom surface. As a result, when the emerging flux with strong magnetic flux is given, the magnetic flux rope is formed immediately via reconnection between the emerging flux and pre-existing shared magnetic field, resulting in the ejective eruption. In contrast, when the emerging flux with weak magnetic flux is given, no magnetic flux ropes are formed, and the eruption does not occur immediately. However, the sheared magnetic field lines collapse suddenly under the continuous twisting motion that leads to an explosive eruption while such an eruption does not occur without the small emerging flux. According to our analysis, the former eruption is due to the torus instability and the latter is due to a loss of equilibrium. We will report on different mechanisms of eruptions triggered by small-scale emerging fluxes of different magnitudes.
ST14-A004
| Invited
Key Signatures of Prominence Materials and Category of Cold Materials Identified by Random Forest Classifier
Shuo YAO#+, Shuyi MENG, Zexin CHENG
China University of Geosciences
The origin of cold materials identified by different criteria is unclear. They are highly suspected to be erupted prominences. However, some cold materials defined by charge depletion exist in both quiet solar wind and interplanetary coronal mass ejections (ICMEs). Recently, solar observations show failed prominence eruption in coronal mass ejections (CMEs) that the prominence sometimes did not propagate into interplanetary space. This work uses Random Forest Classifier (RFC), which is an interpretable supervised machine-learning algorithm to study the distinct signatures of prominence cold materials (PCs) compared to quiet solar wind (QSW) and ICMEs excluding cold materials (ICMEEs). Twelve physical features measured by ACE at 1 au and the monthly averaged sunspot number are used in this study. The measurements from ACE are proton moments, magnetic field component Bz, He/H, He/O, Fe/O, mean charge of oxygen and carbon, C6+/C5, C6+/C4+, and O7+/O6+. According to the returned weights from RFC that are checked by support vector machine classifier, the most important in situ signatures of PCs are obtained. Next, the trained RFC is used to check the category of the cold materials not related to CME observations. The results show that most segments of the cold materials are from prominences, but four of them are possibly from ICMEEs; another one segment is possibly from QSW. The most distinct signatures of PCs are lower(C6+/C5+)/(O7+/O6+), proton temperature, and He/O. Considering the obvious overlaps on key physical features between QSW, ICMEEs, and PCs, the multifeature classifier shows an advantage in identifying them than solid criteria.
ST14-A011
Association Between a Failed Prominence Eruption and Mass Drainage of Another Prominence
Jianchao XUE#+, Li FENG, Hui LI
Chinese Academy of Sciences
Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here we present two prominence failed eruptions on 2022 October 26 and explore their connections. Using stereoscopic observations, the south prominence (PRO-S) erupts with untwisting motion, flare ribbons occur underneath, and new legs are formed during the eruption. The north prominence (PRO-N) rises up along with PRO-S, and the upper part disappears due to the catastrophic mass drainage along a flux tube after PRO-S failed eruption. We suspect that the eruption of PRO-S initiates by kink instability, further rises up with magnetic reconnection, and failed due to reconnection with surrounding fields. The flux tube connecting with the PRO-N horn structure overlies PRO-S, which causes the rising up of PRO-N during PRO-S eruption and mass drainage of PRO-N due to the evacuation after PRO-S eruption. This study suggests that a prominence may end its life through mass drainage along a long flux tube due to a failed eruption underneath.
ST14-A024
Can the Parker Solar Probe Detect a CME-flare Current Sheet?
Yuhao CHEN#, Jun LIN+
Chinese Academy of Sciences
A current sheet (CS) is the central structure in the disrupting magnetic configuration during solar eruptions. More than 90% of the free magnetic energy (the difference between the energy in the nonpotential magnetic field and that in the potential one) stored in the coronal magnetic field beforehand is converted into the heating and kinetic energy of the plasma, as well as accelerating charged particles, by magnetic reconnection occurring in the CS. However, the detailed physical properties and fine structures of the CS are still unknown, since there is no relevant information obtained via in situ detections. The Parker Solar Probe (PSP) may provide us with such information should it traverse a CS in an eruption. The perihelion of PSP’s final orbit is located at about 10 solar radii from the center of the Sun, so it can observe the CS at a very close distance, or even traverse the CS, which would provide us with a unique opportunity to look into the fine properties and structures of the CS, helping to reveal the detailed physics of large-scale reconnection that would have been impossible before. We evaluate the probability that PSP can traverse a CS, and examine the orbit of a PSP-like spacecraft that has the highest probability to traverse a CS.
ST14-A031
Physical Properties of Intermittent Reconnection During an M6.5 Flare with High-turnover-frequency
Zhao WU#+
Shandong University
Multipeak structures can usually be observed in the lightcurves of microwave emission and Hard X-Rays during flares. They have been interpreted to be induced by intermittent reconnections at the flaring region. Here we present the property study of multipeaks during the impulsive stage of an M6.5 solar flare with high-turnover frequencies of microwave spectra. Both lightcurves of microwave and HXRs denote six local peaks. The second one being the strongest with microwave flux density reaching ~3000 SFU at 35-40 GHz, and HXRs flux being ~2 orders of magnitude of the background. We find similar properties among all these peaks that (1) the microwave source locates at the looptop of flare loops, in between the dual HXRs footpoint sources; (2) spatial dispersion appears in microwave sources with lower energy source being closer to the footpoint; (3) the microwave spectra present high turnover frequencies of >15 GHz, and hard optically thin spectra with index of ~-0.8 - -0.4. The microwave imaging observations manifest systematic drift with the intermittent reconnection, and spectral fitting manifests an overall soft-hard-soft trend during the impulsive stage. The results provide solid evidence of the similar physical properties of the intermittent reconnections along the sequential coronal loops.
Session Chair(s): Yukinaga MIYASHITA, Korea Astronomy and Space Science Institute, Kyung Sun PARK, Chungbuk National University
ST11-A015
The Dayside Magnetosheath Pressure Profiles Under Radial IMF Conditions
Gilbert PI#+, Jana SAFRANKOVA, Zdenek NĚMEČEK
Charles University
The different pressure components, such as dynamic, magnetic, and thermal pressure, have varying ratios from the bow shock to the magnetopause. These ratios are significantly altered at the bow shock and vary in the sheath. Those pressures ultimately affect the location and shape of magnetopause. Based on simulations, the spatial profiles of pressures from the solar wind to the magnetopause are influenced by upstream IMF orientations. In this study, THEMIS observations were used to present the statistical results of the dayside magnetosheath and examine the variation of pressure profiles in the magnetosheath and their relation to upstream IMF conditions. The profiles near the Sun-Earth line and the global distribution in the dayside equatorial plane are discussed.
ST11-A001
Solar Cycle Variations in the Orientations of IMF Discontinuities
Sun LEE1,2#+
1Catholic University of America, 2NASA Goddard Space Flight Center
Transient events like hot flow anomalies and foreshock bubbles are common in the Earth's foreshock. These foreshock transients may play an important role in the solar wind-magnetosphere interaction. They typically occur when backstreaming ions accumulate at the intersection of interplanetary magnetic field (IMF) discontinuities with the bow shock. Discontinuity orientations play a key role in determining when and where transients form in the foreshock and strike the magnetopause. They also play a role in determining the amplitude, and significance, of individual transients. We investigate properties of the IMF discontinuity normals across a solar cycle. We compare ACE IMF discontinuity observations for 2001 and 2002 (solar maximum) and 2008 and 2009 (solar minimum). We employ both the Minimum variance analysis (MVA) and Cross-product methods to determine phase front normals. Most discontinuity normals point earthward and dawnward at longitudes ranging from 180º to 250º. A greater range of normal can be seen during solar minimum than during solar maximum. Normals lie further from the Sun-Earth line when solar wind densities are low and velocities are high. This provides a natural explanation for the observed tendency of transients to occur for low solar wind densities and high velocities in terms of longer discontinuity interaction times with the bow shock.
ST11-A017
Uncertainty in L1 Measurements Leads to an Appearance of Saturation of Geomagnetic Response
Nithin SIVADAS1#, David SIBECK1, Maria-Theresia WALACH2+
1NASA Goddard Space Flight Center, 2Lancaster University
Solar wind measurements at the L1 Lagrange point are an uncertain estimate of the actual electromagnetic and plasma parameters that drive the magnetosphere, as the measurements are far from the magnetopause reconnection site. This uncertainty leads to underestimating our planet's response to extreme space weather. Past research has concluded that with increasing solar wind strength, the response of the Earth appears to not increase proportionally and instead saturate during extreme space weather. In the last 40 years, theorists have proposed many explanations for this saturation effect. We explain how the saturation effect might be a misinterpretation created by ignoring uncertainty in the solar wind that impacts the magnetosphere. Therefore, we need to remove this misleading effect of uncertainties in the solar wind drivers before we can accurately estimate the geospace environment response. Furthermore, the work points to a surprisingly general result relevant to any correlation study: random measurement errors can cause a system's linear response to be perceived as non-linear.
ST11-A020
Dawn-dusk Asymmetry of Magnetopause Erosion at Geosynchronous Orbit Related to Reconnection
Hyangpyo KIM1,2#+, Rumi NAKAMURA1, Hyunju CONNOR3, Ying ZOU4, Ferdinand PLASCHKE5, Niklas GRIMMICH5, Brian WALSH6, Kathryn MCWILLIAMS7, J. RUOHONIEMI8
1Austrian Academy of Sciences, 2Austrian Academy of Sciences, 3NASA Goddard Space Flight Center, 4Johns Hopkins University Applied Physics Laboratory, 5Braunschweig University of Technology, 6Boston University, 7University of Saskatchewan, 8Virginia Tech
The dayside magnetopause moves in response to the upstream solar wind conditions, primarily the dynamic pressure and the vertical component of the interplanetary magnetic field (IMF). Notably, the magnetopause tends to be closer to Earth during periods of southward IMF, contrasting with its position during northward IMF. This phenomenon occurs because reconnection between the IMF and Earth’s magnetic field removes magnetic flux at the boundary layer, resulting in magnetopause erosion. Occasionally, the magnetopause approaches geosynchronous orbit when the magnetosphere is highly compressed and/or eroded, mainly during geomagnetic storms. Statistical studies have shown the magnetopause erosion often shows a dawn-dusk asymmetry at geosynchronous orbit. To delve into this, this study presents concurrent observations of magnetopause erosion and related dayside reconnection at geosynchronous orbit by utilizing data from THEMIS, GOES, and SuperDARN radar. The observations suggest that the presence of cold dense plasma in the duskside magnetosphere weakens reconnection rates and, consequently, causes the dawn-dusk asymmetry of magnetopause erosion.
ST11-A005
Changes in the Non-linear Statistical Dependence Between the Solar Wind and Geomagnetic Conditions During Solar Cycle 23
Sanni HOILIJOKI1#+, E. KILPUA1, Adnane OSMANE1, Lucile TURC1, Mikko SAVOLA1, Veera LIPSANEN1, Harriet GEORGE2, Milla KALLIOKOSKI3
1University of Helsinki, 2University of Colorado, 3Japan Aerospace Exploration Agency
The dynamics of the Earth’s magnetosphere are driven by the solar wind variations and transients. The largest variations in the near-Earth space are caused by interplanetary coronal mass ejections (ICME) but significant geomagnetic activity can also be driven by high-speed streams (HSSs) and stream interaction regions (SIRs). Solar wind – magnetosphere interactions generate fluctuations in the inner magnetosphere and modify electron population in the outer radiation belt. Ultra-low frequency (ULF) waves in the Pc5 range (2-7mHz) can accelerate electrons and cause changes in the electron flux up to several orders of magnitude. In this study we use mutual information from information theory to study the statistical dependency of the ULF waves and radiation belt electrons on the solar wind parameters and fluctuations over the Solar Cycle 23. Unlike Pearson correlation coefficient mutual information can also be used to investigate non-linear statistical dependencies between different parameters. We calculate correlation coefficients separately for each year and find that the non-linearity between the solar wind speed and some magnetospheric parameters is higher during solar maximum when most of the geomagnetic activity is driven by ICMEs, while the non-linearity decreases during the declining phase, as a larger portion of the geomagnetic activity is driven by HSSs and SIRs. On the other hand, for example, the southward component of the interplanetary magnetic field, Bz, has an opposite behavior during to solar cycle being more linear during solar maximum. To investigate further if the change of the ratio of ICMEs and HSSs is the possible cause of the changes in the non-linearity during the solar cycle, we calculate the correlation coefficients separately during ICMEs, HSSs/SIRs and quiet solar wind and compare it to the results from different years.
ST11-A019
| Invited
Global-scale Magnetosphere Convection Driven by Dayside Magnetic Reconnection
Lei DAI1#+, Minghui ZHU1, Ren YONG1, Walter GONZALEZ2, Chi WANG1, David SIBECK3, Andrey SAMSONOV4, C. Philippe ESCOUBET5, Binbin TANG1, Jiaojiao ZHANG1, Graziella BRANDUARDI-RAYMONT4
1Chinese Academy of Sciences, 2National Institute for Space Research (INPE), 3NASA Goddard Space Flight Center, 4University College London, 5European Space Agency
Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The Dungey cycle explains that steady-state convection within the closed part of the magnetosphere relies on magnetic reconnection in the nightside magnetospheric tail. Nevertheless, time-dependent models of the Dungey cycle suggest an alternative scenario where magnetospheric convection can be solely driven by dayside magnetic reconnection. In this study, we provide direct evidence supporting the scenario of dayside-driven magnetosphere convection. The driving process is closely connected to the evolution of Region 1 and Region 2 field-aligned currents. Our global simulations demonstrate that intensified magnetospheric convection and field-aligned currents progress from the dayside to the nightside within 10-20 minutes, following a southward turning of the interplanetary magnetic field. Observational data within this short timescale also reveal enhancements in both magnetosphere convection and the ionosphere's two-cell convection. These findings provide insights into the mechanisms driving planetary magnetosphere convection, with implications for the upcoming Solar-Wind-Magnetosphere-Ionosphere Link Explorer (SMILE) mission.
ST11-A002
Cross-polar Cap Potential Evolution During Different Geomagnetic Storms and Comparisons with Models
Igino COCO1#+, Federica MARCUCCI2, Stefano MASSETTI2, Fabio GIANNATTASIO1, Michael PEZZOPANE1, Alessio PIGNALBERI1
1Istituto Nazionale di Geofisica e Vulcanologia (INGV), 2National Institute for Astrophysics
The maximum electrostatic potential difference throughout the polar cap (Cross-Polar Cap Potential, CPCP) is commonly considered to be a measure of the degree of the solar wind - magnetosphere coupling as a consequence of reconnection processes. Several models try to reconstruct the CPCP on the basis of both measurements of external drivers only, such as the Interplanetary Magnetic Field intensity and orientation, the plasma pressure and velocity, and physical assumptions on Pedersen ionospheric conductivity. On the other hand, CPCP can be directly computed from the Super Dual Auroral Radar Network (SuperDARN) convection maps. However, the CPCP actually measured by SuperDARN is the result of a balance between dayside magnetic flux (and consequent plasma transport) opened by reconnection processes at the magnetopause and nightside magnetic flux closed by plasma coming back from the geomagnetic tail. Therefore, CPCP reconstructed by radars did not agree often with model predictions. In this study, we performed a comparison of the behaviour of CPCP obtained from SuperDARN, with the outputs of different CPCP models, during three major geomagnetic storms of the past solar cycle, pointing out possible physical explanations for the differences observed.
ST11-A021
Does the Heppner-Maynard Boundary Match the Locations of the Region 2 Field-aligned Currents?
Maria-Theresia WALACH1#+, Alexandra FOGG2, Adrian GROCOTT1, Mark LESTER3, John COXON4, Steve MILAN3, Harneet SANGHA3, Kathryn MCWILLIAMS5, Sarah VINES6, Brian ANDERSON6
1Lancaster University, 2Dublin Institute for Advanced Studies, 3University of Leicester, 4Northumbria University, 5University of Saskatchewan, 6Johns Hopkins University Applied Physics Laboratory
The high-latitude ionospheric convection is a useful tool in determining solar wind-magnetosphere interactions and nightside activity in the magnetotail. We can map the high-latitude convection pattern using the Super Dual Auroral Radar Network (SuperDARN), a distribution of ground-based radars which are capable of measuring line-of-sight ionospheric flows. As the SuperDARN coverage is not truly global, it is necessary to constrain the maps to be physical when the map fitting is performed. The lower latitude boundary of the convection, known as the Heppner-Maynard boundary (HMB), provides one such constraint. In the standard SuperDARN fitting, the HMB location is determined directly from the data, but data gaps can make this challenging. In this study we evaluate if the HMB placement can be improved using data from the Active Magnetosphere and Planetary Response Experiment (AMPERE), in particular for active time periods when the HMB moves to latitudes below 55 degrees of magnetic latitude. We find that the HMB as defined by SuperDARN and AMPERE are not always co-located. SuperDARN performs better when the AMPERE currents are very weak (i.e. during non-active times) and AMPERE can pick up fast expansions or contractions in the ionospheric current system associated with the convection. Using four events representative of a diverse range of geophysical conditions, we show that whilst overall there is agreement between the SuperDARN and AMPERE boundaries, there are also times when the two datasets disagree. This disagreement is non-systematic and an unexpected result. We find that disagreements primarily arise due to geometrical factors and a time-lag in expansions and contractions of the patterns.
Session Chair(s): Shuo YAO, China University of Geosciences
ST14-A023
| Invited
Expansion and Shrinkage of the Sheath and Magnetic Cloud Due to the Interaction of Two Interplanetary Coronal Mass Ejections
Rok-Soon KIM#+
Korea Astronomy and Space Science Institute
CME-CME interactions near the Sun (< 30 Rs) have been often studied, however, very few observations show the interaction and following structure deformation of CMEs during their propagation into the heliosphere. In this study, we investigated whether any specific signatures could be evidence for the interaction of two successive CMEs in near-Earth interplanetary space. For this, we selected six isolated CME-CME pairs that were expected to interact at 1 AU based on their ejecting times and propagating speeds. We then investigated in-situ solar wind and radio data to see if the signatures of the interaction could be detected. We note that the interaction phase can be inferred from the time difference in expected arrival at Earth for the two CMEs, denoted as ∆t, and categorized them as pre-, now, and post-interactions. As the results, we found that (1) there are reverse-drifting background emissions in the radio spectrum, indicating density increases due to the interaction, (2) during the pre- or now-phases, we identified abrupt decrease and subsequent recovery (hole-like) structures in density and magnetic field between the two interacting CMEs, and (3) the thicknesses of the sheath and magnetic cloud have solid linear relationships with the arrival time difference (∆t), representing a deformation of the CMEs due to the interaction. Based on these findings, we propose a CME-CME interaction scenario as follows: As the two CMEs approach each other, the interaction starts the density increases, and a magnetic hole is formed. Finally, the interaction ends with an elongated sheath and a shrunken magnetic cloud. Our results also demonstrate that the expected arrival time difference based on initial observations of CMEs helps in understanding the CME-CME interaction process near Earth.
ST14-A015
| Invited
Unveiling the Mechanism for the Rapid Acceleration Phase in a Solar Eruption
Ze ZHONG1#+, Yang GUO2, Yao CHEN1
1Shandong University, 2Nanjing University
Two major mechanisms have been proposed to drive the solar eruptions: the ideal magnetohydrodynamic instability and the resistive magnetic reconnection. Due to the close coupling and synchronicity of the two mechanisms, it is difficult to identify their respective contribution to solar eruptions, especially to the critical rapid acceleration phase. Here, to shed light on this problem, we conduct a data-driven numerical simulation for the flux rope eruption on 2011 August 4, and quantify the contributions of the upward exhaust of the magnetic reconnection along the flaring current sheet and the work done by the large-scale Lorentz force acting on the flux rope. Major simulation results of the eruption, such as the macroscopic morphology, early kinematics of the flux rope and flare ribbons, match well with the observations. We estimate the energy converted from the magnetic slingshot above the current sheet and the large-scale Lorentz force exerting on the flux rope during the rapid acceleration phase, and find that (1) the work done by the large-scale Lorentz force is about 4.6 times higher than the former, and (2) decreased strapping force generated by the overlying field facilitates the eruption. These results indicate that the large-scale Lorentz force plays a dominant role in the rapid acceleration phase for this eruption.
ST14-A016
Key Signatures and Possible Origins of Small Flux Ropes Compared to ICMEs and Quiet Solar Wind Studied by Multi-feature Classifier
Hongyi WANG+, Shuo YAO#, Shuyi MENG
China University of Geosciences
The in situ measured flux ropes ranged from 3 to 12 hours are classified as small-scale flux ropes (SFRs). The origins of the SFRs and how to identify different types of SFRs are still under debate. The SFRs are supposed to be mini-CMEs or jets from the solar corona, or to be formed by in situ magnetic reconnections. This work uses random forest classifier and 16 physical features to check the distinct and similar signatures among SFRs, magnetic clouds, erupted filaments, and quiet solar wind. It also considers two SFR subtypes based on proximity to Heliospheric Current Sheets (HCSs). The results highlight the most 5 distinct physical features of SFRs compared to magnetic clouds: O7+/O6+, plasma β, average charge state of Iron (avqFe), proton density (Np), and average charge state of Oxygen (avqO). Those are β, solar wind speed (Vp), Z-component of the magnetic field (Bz), total magnetic field strength (Btotal), and Np between SFRs and quiet solar wind. In the category of magnetic clouds, erupted filaments, and quiet solar wind, about 66% SFRs showing reconnection features are classified as MC. Almost 60% of SFRs far away from HCSs (SFR-Sun) are identified as MCs. Adding the two subtypes of SFRs in the training process, the most distinct signatures between SFR-Sun and MC are β, avqFe, O7+/O6+, Btotal and Bz. Those between SFR-SW and MC are O7+/O6+, β, avqO, avqFe and Vp. Initial results tend to support that there are different origins for SFRs. However, the current classification between SFR-Sun and SFR-SW does not achieve a high accuracy rate by machine learning, which may indicate that HCSs criteria for SFRs is not sufficient. Ongoing research is actively being pursued to develop a more accurate classification mechanism for the SFRs having different origins.
ST14-A010
The Contributions and Properties of Different Kinds of ICMEs and Solar Wind During Solar Cycles 23 and 24
Xinzheng SHI#+
Shandong University
The intensity difference between solar cycles 23 and 24 is evident. Statistical results indicate that the activity level has an impact on both ICMEs and solar wind. In the present study, the ICMEs are categorized into two types, flare CMEs (FCs) and nonflare CMEs (NFCs) by the QFe. The occurrence rates and proportions of FCs are both higher in solar cycle 23 than in solar cycle 24. In contrast, the occurrence rates of NFCs are almost the same during the two solar cycles. The speed, QFe, O7+/O6+, AHe, and first ionization potential bias are all higher for FCs than for NFCs. The above parameters inside NFCs and solar wind are almost the same. The solar cycle dependence of the parameters inside NFCs is more clear than that inside FCs. The intensity of the solar cycle also has a significant impact on the solar wind. In this study, the improved two-step mapping procedure is used to trace the solar wind back to its source region. The latitude distribution of the source regions of coronal holes (CHs) and quiet Sun (QS) solar wind varies greatly in the minimum phase of the two solar cycles. During the maximum and declining phases, parameters such as the footpoint magnetic field, B, speed, and AHe in the solar wind are higher during the solar cycle 23 compared to the solar cycle 24. However, during the minimum phase, these parameters are generally higher during the solar cycle 24 compared to the solar cycle 23. Both O7+/O6+ and QFe show a significant decrease during the minimum phase of solar cycle 23, indicating that the minimum phase of solar cycle 23 is characterized by an extremely weak solar activity.
ST14-A017
Initiation of Solar Wind from Small Coronal Hole Reflected by the Statistical Features of Heavy Ions
Shuyi MENG#+, Shuo YAO
China University of Geosciences
Recently, it has been reported that slow solar wind could be driven from open field region among closed-loop streamer region, which may be small scale coronal hole. It is still unclear how the slow wind be heated and accelerated from these small coronal holes (CH). This statistical work uses the measured abundance and charge of heavy ions by ACE from 1998 to 2011 to check the differences and similarities among Alfvenic slow wind, non-Alfvenic slow wind, fast wind, and Interplanetary Coronal Mass Ejections (ICMEs). The effect size is adopted in this work to quantitatively reveal the most distinct physical signatures. Both the speed criteria (slow vs. fast) and the CO charge criteria (“hot” vs. “cold”) are used to make classification. The results show that, despite the criteria, Alfvenic “slow” wind (ASW) always show similar He/O and Fe/O with non-Alfvenic “slow” wind (N-ASW). However, for the charge of Fe ions and the flux ratio between alpha particles and protons, the ASW is more alike the “fast” wind (FW). Similar FIP effects support that ASW and N-ASW have the same source of chromospheric materials. The charge of Fe ions support that more heating is possibly caused by reconnection above the freeze-in height of C and O in closed-field region than in open field region. It seems that ASW show similar signatures to FW which are related to magnetic field structures, including Alfvenic fluctuations, differential streaming, and ionization of Fe ions. They support the ASW being from small CH inside streamer region, and the initiation mechanism of ASW being a combination according to height.
ST14-A007
Comparison of Ion- Proton Differential Speed Between ICMEs and Solar Wind Near 1 Au
Xuechao ZHANG#+, Hongqiang SONG, Yao CHEN
Shandong University
Interplanetary coronal mass ejections (ICMEs) are the counterpart of coronal mass ejections in the interplanetary space. Solar wind is the continuous flow of charged particles from the Sun and can be divided into slow, intermediate, and fast winds. Both ICMEs and solar wind play significant roles in space weather and are important research topics in solar and space physics. One important issue is their kinetic property. In this presentation, we perform a statistical study on the ion-proton differential speed (Vip) for He2+, C5+, O6+, and Fe10+ in both ICMEs and solar wind based on measurements of Advanced Composition Explorer. The results show that the Vip is low within ICMEs and slow solar wind (< 400 km/s), while obvious in the intermediate (400 -- 600 km/s) and fast wind (> 600 km/s). In the meantime, we also perform a study on the ion-oxygen differential speed (Vio) within both ICMEs and solar wind. The results demonstrate that the Vio is almost zero for He2+, C5+, and Fe10+ within both ICMEs and solar wind, which confirms that all heavy ions might flow at the same bulk speed. The implications of the study are discussed.
Session Chair(s): Timo PITKÄNEN, Shandong University, Jong-Sun PARK, Shandong University
ST11-A023
Analysis of the Relationship Between Geomagnetic Disturbances and Ground Level Enhancement Events During Solar Cycles 24 and 25
Jinhye PARK1#+, Kyung Sun PARK2
1KASA, 2Chungbuk National University
Solar energetic particles (SEPs) are composed of protons, electrons, and heavy ions with energies ranging from hundreds of keV to MeV, and they are observed throughout the heliosphere. Large-scale SEP events are considered among the most critical phenomena regarding space weather. After accelerating in the solar corona region, SEPs propagate along solar magnetic fields into interplanetary space. SEP events are primarily observed through in-situ measurements in space, and a few large and fast SEPs, known as ground-level enhancements (GLEs), are detected on the ground. This study analyzed 19 GLE events during solar cycles 24 and 25. Most of these events originated from the western regions of the Sun, with two exceptions located at E9° and E8°. All but two events were associated with X-class flares; the remaining two were M-class. The speeds of the coronal mass ejections (CMEs) related to these GLE events ranged from 700 km/s to 3200 km/s. Four out of the 19 events were accompanied by significant geomagnetic disturbances, including a related magnetic substorm detected on the ground. However, only one event was associated with a strong magnetic storm. Even when the high speed and high density of solar wind associated with GLE events passes the Earth's magnetosphere, a geomagnetic disturbance does not necessarily occur. This is because it was accompanied mainly by the northward and weak southward interplanetary magnetic field (IMF). This study shows that GLE events accelerated by strong solar activities are observed under diverse solar wind and IMF conditions.
ST11-A013
Differences in Fast Flows Between Substorms and Pseudosubstorms in the Plasma Sheet
Kanpatom KASONSUWAN1#+, Yukinaga MIYASHITA2,3, Suwicha WANNAWICHIAN1
1Chiang Mai University, 2Korea Astronomy and Space Science Institute, 3Korea National University of Science and Technology
Substorms and pseudosubstorms (pseudobreakups) involve explosive auroral activities caused by magnetotail dynamics. Typically, auroral breakups are linked to magnetic reconnection or current disruption and are expected to exhibit fast flows in the magnetotail during the geomagnetic activity. This study primarily focuses on the differences in fast flows between substorms and pseudosubstorms based on superposed epoch analysis of data from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft. As the signature of fast flows, the variation of the northward magnetic field sharply develops, the earthward or tailward ion velocity increases, and the magnetic pressure grows exponentially. Statistical data show that the variations in these 3 parameters for pseudosubstorms are weaker than those for substorms after the flow front passes. The depletion trend in ion pressure variation following the flow front may serve as evidence indicating the underlying cause of the weakness for pseudosubstorms.
ST11-A014
Auroral Onset Locations and Maximum Extents of Multi-substorm Events from Polar VIS and UVI Observations
Suwicha WANNAWICHIAN1#+, Yukinaga MIYASHITA2,3
1Chiang Mai University, 2Korea Astronomy and Space Science Institute, 3Korea National University of Science and Technology
Multi-substorm events are investigated for the onset location variation of the visible and ultraviolet emissions. Auroral images, taken by the Visible Imaging System (VIS) and the Ultraviolet Imager (UVI) instruments onboard the Polar spacecraft, are analyzed to identify the latitudes of initial brightening and maximum poleward expansion for several substorms. For aurora associated with low-energy, "soft," precipitating electrons, the responsive auroral emissions were shown in Polar/VIS (557.7, 130.4, 391.4, and 630.0 nm) images. On the other hand, the FUV auroras are presented in Polar /UVI (LBH long, LBH short, 130.4, and 135.6 nm) images, representing the results of higher energy precipitating auroral particles (mostly electrons). We found that the visible auroras can have peak emission at either higher or lower latitudes, which are more and less expansive than the UV auroras. Depending on the magnetosphere dynamics, either low-energy or high-energy electrons could be in the near-Earth region, corresponding to lower latitudes of auroral expansion, than in the tailward region, corresponding to higher latitudes of auroral expansion. It must be noted that the spatial scale of substorm onset region in the magnetosphere should be very small. Thus, FUV and visible auroras should be initiated very close (less than), magnetically mapped to the magnetosphere. This similar location is seen from ground-based observation with higher resolution. At the same time, the limitation of the resolution of Polar/VIS and UVI should be considered. The differences of visible and FUV auroras in various substorm events are discussed and correlated with the solar wind conditions.
ST11-A009
Association of High-latitude Geomagnetic Perturbations and Pi1 and Pi2 Pulsations with the Three Steps of Auroral Onset Arc Development at Substorm Onset
Madeeha TALHA1,2#+, Yukinaga MIYASHITA1,2
1Korea Astronomy and Space Science Institute, 2Korea National University of Science and Technology
Using Time History of Events and Macroscale Interactions during Substorms (THEMIS) data, we studied the stepwise development in high-latitude geomagnetic perturbations and Pi1 and Pi2 pulsations at substorms onsets and their association with stepwise auroral onset arc development by analyzing four substorm events. We found that the geomagnetic perturbations and pulsations which are magnetic signatures of the substorm on the ground show stepwise changes and excitation similar to the development of the auroral onset arc which is a visual manifestation of the substorm. We observed minor to small changes in magnetic perturbations and excitation of Pi2 pulsations before initial brightening (IB) while excitation of Pi1 and second Pi2 at or around the further enhancement of onset arc (FE). Then, a steep fall in the magnetic northward component, and the largest amplitude and highest frequency Pi1 and Pi2 pulsations appeared at or after poleward expansion (PE). The appearance of FE in all four events and its association with magnetic perturbations and pulsations show that FE is an important step like IB and PE. The detailed analysis of the FE step using ground- and space-based data may provide information on the sequence of mechanisms behind the substorm as well as the mechanisms behind the excitation of Pi1 and Pi2 pulsations.
ST11-A024
| Invited
The Auroral Arc and Plasma Turbulence
Magnus IVARSEN1#+, Devin HUYGHEBAERT2, Jean-Pierre ST-MAURICE3, Glenn HUSSEY3
1University of Oslo, 2University of Tromsø, 3University of Saskatchewan
The radio aurora, the radar backscatter that invariably accompany displays of aurora, has been studied for decades, but key elements that make up its explanation are lacking. For example, it is thought that the plasma turbulence initiated by an auroral arc exists for the most part a distance away from the arc itself, thought to be a natural response of the ionosphere to the electrical connection of an auroral arc to the magnetosphere. We show how this response, the tendency for auroral turbulence to appear outside of auroral arcs, is clearly observed in an unprecedented view of the radar aurora, using the new ICEBEAR 3D radar. Capable of determining accurate 3D backscatter echo locations, we can treat auroral radar data as a 3D point cloud in geospace. We explore a few different explanations for why turbulence skirts the regions of most intense auroral particle precipitation, all of which touch upon the ionosphere-magnetosphere interaction in a major way.
ST11-A006
| Invited
Low-energy Ion Transport in Mercury’s Magnetosphere: BepiColombo Mio Observations and Test Particle Simulations
Yuki HARADA1#+, Yoshifumi SAITO2, Lina HADID3, Dominique DELCOURT4, Sae AIZAWA5, Nicolas ANDRE6, Moa PERSSON7, Markus FRAENZ8, Shoichiro YOKOTA9, Andrey FEDOROV6, Wataru MIYAKE10, Emmanuel PENOU7, Alain BARTHE7, Jean-André SAUVAUD7, Bruno KATRA3, Shoya MATSUDA11, Go MURAKAMI12
1Nagoya University, 2Japan Aerospace Exploration Agency / Institute of Space and Astronautical Science, 3National Centre for Scientific Research/Sorbonne Université-Ecole Polytechnique, 4National Centre for Scientific Research, 5Laboratoire de Physique des Plasmas, 6University of Toulouse, 7Institute for Research in Astrophysics and Planetology (IRAP), National Center for Scientific Research (CNRS) - University of Toulouse (UPS) - National Center for Space Studies (CNES), 8Max Planck Institute for Solar System Research, 9Osaka University, 10Tokai University, 11Kanazawa University, 12Japan Aerospace Exploration Agency
As opposed to the rotation-driven magnetospheres of Jupiter and Saturn, the circulation of Mercury's magnetosphere is expected to be completely dominated by solar wind-driven convection. In this sense, Mercury's magnetosphere offers a valuable end-member case of the most strongly solar wind-driven magnetosphere in our solar system. However, the global structure, variability, and consequences of magnetospheric convection at Mercury remain elusive partly owing to the lack of adequate observations of cold plasma in Mercury's magnetosphere. Here we present comparisons of low-energy ion observations by BepiColombo Mio during the Mercury flybys with test particle simulations, thereby exploring sources, transport, and surface precipitation of the observed low-energy ions. The new observations by Mio indicate the preferential transport of lower-energy ions of solar wind origin deep into the near-midnight, low-latitude magnetosphere. The test particle simulations suggest that magnetospheric convection plays a crucial role in transporting these low-energy ions and that the convection-driven ion transport results in the presence of relatively dense plasma within the deep magnetosphere and ion precipitation onto the near-equator nightside surface of Mercury. Future in-orbit observations by BepiColombo will provide unique data that enable a comprehensive investigation of solar wind coupling with Mercury's magnetosphere.
Session Chair(s): Sang-Mook LEE, Seoul National University
SE11-A001
Generation of Evolving Plate Boundaries and Toroidal Flow from Visco-plastic Damage-rheology Mantle Convection and Continents
Thorsten BECKER1#+, Lukas FUCHS2
1The University of Texas at Austin, 2Frankfurt University
Earth's style of planetary heat transport is characterized by plate tectonics which requires rock strength to be reduced plastically in order to break an otherwise stagnant lithospheric lid, and for rocks to have a memory of past deformation to account for strain localization and the hysteresis implied by geological sutures. Such dynamics lead to interesting mantle convection phenomena including those that Dave Yuen pursued through geodynamic modeling over the years. While we never worked directly with Dave, conversations with him and his encouragement helped sustain our efforts over the decades, starting from Dave critiquing our MSc thesis in the original German. Here, we explore ∼107 Rayleigh number, visco-plastic, 3-D global mantle convection with damage at a numerical resolution that approaches the finest levels that Dave would always push us toward. We show that oceanic lithosphere-only models generate strong toroidal-poloidal power ratios and features such as a mix of long-wavelength tectonic motions and smaller-scale, back-arc tectonics driven by downwellings. Undulating divergent plate boundaries can evolve to form overlapping spreading centers and microplates, promoted and perhaps stabilized by the effects of damage with long memory. The inclusion of continental rafts enhances heat flux variability and toroidal flow, including net rotation of the lithosphere, to a level seen in plate reconstructions for the Cenozoic. Both the super-continental cycle and local rheological descriptions affect heat transport and tectonic deformation across a range of scales, and we showcase both general tectonic dynamics and regionally applied continental breakup scenarios. Our work points toward avenues for renewed analysis of the typical, mean behavior as well as the evolution of fluctuations in geological and model plate boundary evolution scenarios.
SE11-A017
Constraining Subducting Slab Viscosity with Topography and Gravity Fields in Free-surface Mantle Convection Models
Ting YANG#+, Lijun DENG
Southern University of Science and Technology
Slab strength directly controls the allocation of the subducting slab’s gravity potential energy between the surrounding mantle convection and lithospheric plate motion. Constraining the subduction slab viscosity structure has been one of the main concerns in geodynamics over the past few decades. Surface topography and gravitational observations have provided unique constraints on the viscosity of subduction plates and suggest that slab viscosity is significantly lower than that suggested by mineral physics laboratory experiments. It is unclear whether the free-slip top boundary condition used in these studies affects the inverted slab viscosity. In this study, we develop 2-D free-surface subduction models that can generate accurate surface topography by a modified "sticky-air" method using Underworld2 software. We compare the computed topography and gravity in our free-surface subduction models with observations to constrain the subducting slab viscosity. Our model results support relatively weak slabs (20-120 times more viscous than the upper mantle) at the bending region, consistent with previous studies with a free-slip top boundary. The viscosity of the slab below the bending region barely affects the surface topography and gravity field, and both strong and weak slabs fit the observed topography and gravity field. Analysis of the slab stress and comparison with visco-plastic models suggest that depth-dependent plastic yielding is the main reason for the bending zone viscosity reduction. We also investigate the comprehensive relations between subduction interface viscosity, surface topography and gravity anomaly, and trench motion. Models with trench advance have abnormally low topography and gravity above the volcanic arc, contradicting subduction zone observations. Together with present trench motion observations and previous studies, we support the idea that the trench retreats under normal single-slab subduction conditions.
SE11-A013
Degree of Coupling in 3D Multilayer Lithospheric Buckling: Implications for Deformation and Pressure
Seok-Hyeon DO1#+, Byung-Dal SO1, Young Hong SHIN2
1Kangwon National University, 2Korea Institute of Geoscience and Mineral Resources
Buckling is a mechanical instability that occurs when the material with the strength contrast accommodates compressional stress. The lithosphere, influenced by various factors (i.e., composition, temperature, and pressure), exhibits a layered rheological structure with varying strength depending on the depth. The interplay between the strength contrast on the lithosphere and the tectonic compressional stress induced buckling instability. The lithosphere undergoes a complex stress regime by the relative plate motion and tectonic structures. To investigate the buckling geometry of various lithospheres that may occur under complex stress regimes, we performed 3D viscoelastic numerical modeling. Our multilayer models, with two layers of high strength sandwiched in a low strength matrix, mimicked simplified strength envelopes of the lithospheres. The various buckling geometries were compiled as a function of the internal (e.g., the strength contrast, the thickness of the layer) and the external (e.g., magnitude and orientation of the boundary conditions) factors. The thickness and strength of the weak layer between the two strong layers determined the degree of coupling. We found that boundary conditions dominate the overall geometry and symmetry. The boundary conditions with the extension produced a smaller cylindrical buckling structure than the uniaxial compression models. In biaxial compression models, the relative amount of shortening along both axes determines the axis of the symmetry. The findings contribute to understanding lithospheric scale buckling processes and their geological and tectonic implications in diverse regions.
SE11-A007
Some Speculations on the Cause of Low Subduction Angle of the Pacific Plate Beneath Northeast Asia and the Geodynamics Modeling to Address the Issue
Sang-Mook LEE#+, Ngoc Kien PHAM
Seoul National University
One of the big mysteries of plate tectonics is the low subduction angle of the Pacific Plate under Japan, the East Sea/Sea of Japan, and Northeast Asia, including Korea and China. It is the lowest angle in the globe, and by tracing the Benioff Zone, it is known that the slab of the Pacific Plate reaches depths of 700 km, more than 1000 km from the Japan Trench. Why Pacific slab subduction at a low angle remains speculative. There are at least three hypotheses. One is that the slab is supported by a three-dimensional buoyant flow trapped under it. Another one is that the slab remains floated in the upper mantle because of rapid trench rollback. In this study, we investigate the third possibility that a large plume head is stuck under the slab, providing the necessary buoyancy to keep the slab afloat. Using numerical methods, we examine how the density structure and the thickness of the slab affect the subduction angle. Our preliminary results serve as an essential step towards elucidating a significant issue of present-day plate tectonics understanding of the Western Pacific and beyond.
SE11-A003
The Effects of Coordinate System on Mantle Convection and the Cooling of Oceanic Lithosphere
Hang ZHANG#+, Manabu MORISHIGE, Hikaru IWAMORI
The University of Tokyo
Spreading of the lithosphere at the mid-ocean ridges is a fundamental geodynamical process, yet it is not fully understood. The half-space cooling (HSC) model assumes a purely conductive half-space with a cool surface, its prediction agrees well with the observed heat flow and subsidence data at young ages but deviates systematically at older ages. An alternative, the plate cooling model, fits the observed data well, but lacks a clear physical basis. Based on a series of numerical simulations, Huang and Zhong (2005) attributed this discrepancy to trapped heat and small-scale convection beneath older lithosphere, but their simulations were in the Cartesian coordinate system and yielded a mantle potential temperature higher than observation. Our study explores the effects of coordinate system on mantle convection, specifically in the 2D spherical annulus and the conventional Cartesian coordinates. In the spherical annulus, plumes form beneath intermediate-age regions and recurrently migrate towards the ridge until their heads hit the surface. Notably, under conditions of low internal heating and high viscosity, excess heat accumulates beneath the relatively older oceanic plate without small-scale convection. Increasing internal heating rate or decreasing viscosity, can intensify convection and initiate small-scale convection under old plates, while preserving the plume’s recurrent generation-migration patterns. With the identical conditions, the 2D Cartesian coordinate cases yield a higher average mantle temperature, closer to the spherical annulus cases with increased heating or decreased viscosity. These differences are inherent to the geometry. Overall, factors that elevate mantle potential temperature can intensify convection, make plumes migrate for shorter distances, and induce small-scale convection. Surface heat flow and subsidence calculated from the numerical simulation results indeed show a trend flatter than the HSC model, aligning with observation data.
SE11-A009
Machine Learning Approach to Decipher Important Statistics in the Earthquake Catalog for Large Earthquake Occurrence
Jinsu JANG#+, Byung-Dal SO
Kangwon National University
The spatiotemporal distribution and magnitude of seismicity documented over decades are important for understanding the pattern and mechanism of earthquake sequence. Here, machine learning (ML) explainers quantify the contributing factors to discriminate between Large Earthquake Occurrence (LEO) and non-LEO cases. Seventy-eight statistical values associated with the time, latitude, longitude, depth, and magnitude in the earthquake catalog are extracted from 202,706 spatiotemporal windows for training the ML classifiers. The ML explainers recognize the maximum magnitude of the window as the most important factor to improve the classification performance with the five most important statistics. Our approach provides a novel perspective to gain insight into the earthquake sequence.
SE11-A010
Ocean Bottom Electromagnetic Study of the Western Pacific Mantle: Observations and Geodynamic Interpretations
Hogyum KIM1#+, Sang-Mook LEE1, Kiyoshi BABA2, Hisashi UTADA2
1Seoul National University, 2The University of Tokyo
The recent proliferation of ocean bottom geophysical experiments has contributed to the accumulation of in-situ observations on the oceanic plates. However, some results showed inconsistencies that are challenging to solve using basic global models. One of the notable examples is from the Oldest-1 ocean bottom electro-magnetometer array experiment, conducted by Korean and Japanese scientists under the Pacific Array Program, on the oldest portion of the western Pacific. The result from the seafloor magnetotelluric survey showed that the low conductivity layer of the region, which is assumed to be an analog of the lithosphere, is almost ~170 km. The temperature structure derived from the classic half-space cooling model of the corresponding seafloor age (~175 Ma) could explain the derived electrical resistivity structure of the region. However, this explanation appears to be inconsistent with other observations on the region, such as the seafloor subsidence, heat flow observations, and abundance of Mesozoic volcanic activities in the region. Such inconsistency can be seen from other observations, such as the P-wave velocity structure and an electrical resistivity study conducted in the northwest Pacific basin. Several hypotheses, ranging from the global plate-cooling model with the sub-lithospheric convection to regional or local models, including the residuum of hotspot activities, have been considered to explain the in-situ observation from geodynamic perspectives. Multi-scaled, cross-disciplinary studies and the expansion of in-situ geophysical observation coverage may be necessary to understand the complexity.
Session Chair(s): Gabriele MORRA, University of Louisiana at Lafayette
SE11-A002
Testing Driving Mechanisms of Megathrust Seismicity with Explainable Artificial Intelligence
Fabio CAPITANIO#+
Monash University
Constraining the parameters controlling megathrust seismicity along major subduction zones has remained challenging. We use Explainable Artificial Intelligence (XAI) to assess the relevance of geophysical properties and motions along major subduction zones, as in previous analyses, paired with novel slab stress calculations, as proxies for the driving forces of subduction. These are the three dataset types of the input layer of a Fully Connected Network (FCN) trained to classify megathrust earthquake magnitudes. We, then, use a Layerwise Relevance Propagation (LRP) to estimate the input relevance, identifying features most relevant to the classification. XAI identifies the megathrusts curvature, sediment thickness and upper plate deformation relevance previously proposed, and reveals the relevance of slab stresses, showing the subduction dynamics controls on mega earthquakes. While the high relevance of slab pull reconciles with the paradigm of subduction, the highest values are found for trench-parallel stresses, suggesting the occurrence of large earthquakes on megathrust segments close to slab steps where trench-parallel forcing is maximised.
SE11-A008
Progress in Geodynamics Using Lattice Boltzmann Methods
Gabriele MORRA1#+, Peter MORA2, Leila HONARBAKHSH1, Mohammad BOROUMAND1
1University of Louisiana at Lafayette, 2 King Fahd University of Petroleum and Minerals
Lattice Boltzmann Method (LBM) uses a perturbative formulation of the Boltzmann equation to model mesoscale fluid-dynamics via reproducing distributions of particles moving and colliding on a lattice, which can be theoretically shown to scale to the macroscopic Navier-Stokes equation. We present many examples of geodynamics applications, across the entire range of planetary evolution, from the formation of a magma ocean and planetary cores to an heterogeneous solid state mantle and the emergence of plate tectonics. To demonstrate the validity of the approach in geodynamics, 18 tests of convection are shown for varying Prandtl and Rayleigh numbers as well as different boundary conditions. Further, we show how our highly optimized Thermal LBM implementation scales linearly on CPU clusters for 2D and 3D models. We test the model up to 2048 cores and demonstrate both high throughput and linear speedup to 290K cores on present clusters, and beyond with faster next generation interconnects. Finally, we show applications of two-phase flow to planetary core formation, synergy with machine learning to extract fundamental convection parameters and models of emergence of plate tectonics.
SE11-A014
Development of a Fluid Migration Model for the Geomechanical Sequestration System Using One Way Coupled DEM-LBM
Soojung AN1#+, Byung-Dal SO1, Gabriele MORRA2
1Kangwon National University, 2University of Louisiana at Lafayette
We present a novel approach in the field of geodynamics, focusing on the development of a 3-dimensional macroscale fluid flow model for geomechanical sequestration systems (e.g. enhanced geothermal and carbon capture storage systems). The proposed model integrates Discrete Element Method (DEM) and Lattice Boltzmann Method (LBM) through a one-way coupling mechanism, providing a comprehensive understanding of the fluid migration pathways through spontaneously generated fractures near subsurface reservoirs. We investigate the dynamic behaviour of fluid migration in geomechanically active anticline formations, taking into account the complex interplay between particle-scale mechanics and fluid flow phenomena. The results of this research have significant implications for the optimisation and monitoring of geomechanical sequestration processes, contributing to advances in sustainable energy and environmental management. This presentation aims to provide an insight into the DEM-LBM coupling strategy, the porosity derivation method and potential applications to geodynamics.
SE11-A006
Insights from 2-D Numerical Models of the Formation of a Weak Slab Interface on Volcano and Seismicity Distribution in the Southwest Japan Subduction Zone
Goeun HA1#+, Changyeol LEE2, Young-Hee KIM1
1Seoul National University, 2Yonsei University
Understanding the migration of the slab-derived fluids at subduction zones provides useful insights into the distribution of arc volcanoes and the generation of earthquakes. The fluids released from the sub-forearc slab hydrate the overlying mantle, and a weak hydrous layer decouples the subducting slab from the forearc mantle. This mechanical decoupling forms a cold nose by preventing the forearc mantle from participating in the corner flow. The weak hydrous layer along the sub-forearc slab interface provides a pathway for fluid transport toward the mantle wedge tip, which leads to non-volcanic seismic tremors in the forearc. The slab-derived fluids that migrate into the sub-arc dry peridotite in the mantle wedge generate melt through flux melting. In this study, we perform two-dimensional numerical simulations that consider both dehydration/hydration and fluid transport to explain unevenly distributed volcanoes and tremors in the Southwest Japan subduction zone. Our models tailored to the Kyushu and the Shikoku regions focus on how the weak hydrous layer develops and transports slab-derived fluids with different subduction settings and histories. In the Kyushu region, where an older plate subducts with a higher angle, slab dehydration occurs at deeper depths and the less slab-derived fluids reach the wedge corner along the weak hydrous layer. This corresponds to more frequent arc volcanic activities and a lack of tremors in the forearc. On the other hand, slab dehydration occurs at shallower depths at the Shikoku region, where a younger plate subducts with a lower angle, slab dehydration occurs at shallower depths and more slab-derived fluids reach the wedge corner along the weak hydrous layer. This explains the sparse distribution of arc volcanoes and frequent tremors in the forearc.
SE11-A004
Five Tectonic Modes of Mantle Convection and Its Implication for Earth’s Tectonic Evolution in History
Jinshui HUANG#+, Song XIANG
University of Science and Technology of China
Plate tectonics is the fundamental process that governs the solid Earth. However, when plate tectonics began and what the pre-plate tectonics looks like are still under debate. We did a large number of three-dimensional numerical simulations in a spherical shell domain and the results show that there are five tectonic modes of planetary mantle convection. The five modes are classified as: I) non-plate mobile lid mode, II) plate-like mobile lid mode, III) episodic plate-like lid mode, IV) episodic stagnant lid mode, and V) stagnant lid mode. These five modes are mainly controlled by the lithospheric strength (yield stress), tau, Rayleigh number, Ra, and internal heat rate, H. We performed a detailed analysis of the influences of tau, Ra and H on the convection modes, and found that the present Earth is now in Mode II, i.e., plate-like mobile lid mode. However, due to the higher internal heat rate and internal temperature, lower viscosity and larger Rayleigh number, the early Earth was in mode III, that is, episodic plate-like lid mode. This suggests that even if there was some kind of plate tectonics in the early Earth, the tectonic convective modes are different. Our results suggest that the pre-plate tectonics is in an episodic plate-like tectonics regime.
SE11-A005
Deep Dynamical Processes and Shallow Response of the Ri-Qing-Wei Basin
Sunyi LI#+, Yaoqi ZHOU
China University of Petroleum (East China)
In the process of lithospheric thinning of the North China Craton, the coupling relationship between deep mantle tectonics-magmatic activities and shallow crustal response has been a hotly debated topic in recent decades. Basic magmatic rocks from the late Mesozoic era (130-78 Ma) in the Ri-Qing-Wei Basin along the Shandong coast of Eastern China are divided into three groups based on geochemical and Sr-Nd isotopic data. Group I rocks have relatively higher SiO2 content and lower MgO and compatible trace element contents. They have higher initial 87Sr/86Sr ratios and lower εNd(t) values, indicating a magma source from the melting of an enriched lithospheric mantle. Group II has relatively low SiO2 content, high MgO and compatible trace element contents, lower initial 87Sr/86Sr ratios, and higher εNd(t) values. These characteristics indicate that the magma originated from decompression melting of the upwelling asthenospheric mantle. Group III rocks have elemental and isotopic compositions that are intermediate between the first two groups, indicating a source from a mixture of lithospheric and asthenospheric-derived melts. Considering the changes in the tectonic stress field and sedimentation rates during the late Mesozoic in the Ri-Qing-Wei Basin, it is evident that these geological activities are governed by a common geodynamic mechanism, rather than different independent tectonic events. In summary, the coupling of various shallow complex geological phenomena in the Ri-Qing-Wei Basin with a single deep geodynamic mechanism indicates that the continental arc rifting associated with the subduction of the ancient Pacific plate is identified as the deep geodynamic force driving this rapid lithospheric thinning.
SE11-A012
The Influence of Mascarene Basin Asthenosphere Reservoir on MORB Composition Along the Central Indian Ridge Between 8°S and 12°S: A Possible Link with the African Superplume
Clement Pierre Marc VINCENT1#+, Sidonie REVILLON2, Jung-Woo PARK3, Sang-Mook LEE1, Jonguk KIM4, Jihye OH4
1Seoul National University, 2SEDISOR/ Geo-Ocean University Brest-CNRS-IFREMER UMR 6538, Institut Universitaire Européen de la Mer, 3School of Earth and Environmental Sciences, Seoul National University, 4Korea Institute of Ocean Science & Technology
Along the Central Indian Ridge (CIR), the geochemical and isotopic signature of mid-ocean ridge basalts (MORB) from two segments between 8° and 12°S show a FOZO-like enrichment with high 3He/4He (R/RA) (> 10 RA), suggesting small auxiliary upwelling with a deep primordial mantle component. Based on complementary major and trace elements analysis as well as Sr, Nd and Pb radiogenic isotope compositions of MORB samples from the same location, we fine the presence of a FOZO/C-like enriched signature characterized by high Pb isotope ratios (206Pb/204Pb = 18.1134 – 19.1481; 207Pb/204Pb = 15.4710 – 15.6146 and 208Pb/204Pb = 37.8625 – 39.0332), relatively low 87Sr/86Sr (0.702767 – 0.702974) and high 143Nd/144Nd (0.512989 – 0.513118). According to a recent seismological study, an asthenospheric anomaly centered under the Mascarene Basin maybe flowing beneath the CIR. We propose that this plume-like anomaly named Mascarene Basin Asthenosphere Reservoir (MBAR) is the source of the enriched FOZO/C-like signature observed along these two segments of the CIR. Moreover, the close isotopic signature and location of the MBAR suggest that this plume-like anomaly may share a common deep origin with the different Indo-African plumes (e.g., Afar plume) inferred to be related to the African LLSVP. This argument implies that the CIR between 8° and 12°S is influenced by a branch of the African LLSVP.
Session Chair(s): Florian M. SCHWANDNER, NASA Ames Research Center
SE01-A030
Continental and Oceanic AAM Contributions to Chandler Wobble with the Amplitude Attenuation from 2012 to 2022
Xueqing XU#+
Chinese Academy of Sciences
We reconstructed the Chandler Wobble (CW) from 1962 to 2022 by combining the Eigen-oscillator excited by geophysical fluids of atmospheric and oceanic angular momentums (AAM and OAM). The mass and motion terms for the AAM are further divided with respect to the land and ocean domains. Particular attention is placed on the time span from 2012 to 2022 in relation to the observable reduction in the amplitude of the CW. Our research indicates that the main contributor to the CW induced by AAM is the mass term (i.e., the pressure variations over land). Moreover, the phase of the AAM-induced CW remains relatively stable during the interval of 1962–2022. In contrast, the phase of the OAM-induced CW exhibits a periodic variation with a cycle of approximately 20 years. This cyclic variation would modulate the overall amplitude of the CW. The noticeable amplitude deduction over the past ten years can be attributed to the evolution of the CW driven by AAM and OAM, towards a state of cancellation. These findings further reveal that the variation in the phase difference between the CW forced by AAM and OAM, may be indicative of changes in the interaction between the solid Earth, atmosphere, and ocean.
SE01-A037
High-quality Heat Flow Determination from Coastal Areas of Fujian Province, China
Yaqi WANG1#+, Guangzheng JIANG2
1Chinese Academy of Sciences, 2Chengdu University of Technology
Most heat flow data along the Fujian coast come from shallow boreholes of a few hundred metres with large uncertainties, and deep borehole measurements are needed to obtain high quality heat flow data. In this study, we obtained continuous temperature logs from seven boreholes located in the volcanic fault zone of eastern Fujian. The boreholes have experienced long shut-in times; thus, it can be expected that the temperature conditions have re-equilibrated after drilling and drill-mud circulation. Rock thermal conductivity and radiogenic heat generation were also measured on 79 core samples from these seven boreholes. The measured heat flow density was determined to be 44.2 ~ 89.9 mW/m2. This confirms the high heat flow values previously identified in the coastal area of Fujian. It is of great significance for the study of the distribution characteristics and exploitation of geothermal resources in the region.
SE01-A014
Sedimentary Composition and Significance of Lower Valley Cut and Deep-water Gravity Flow on Lingshan Island in the Riqingwei Basin of Eastern Shandong
Hongyu MU#+, Yaoqi ZHOU
China University of Petroleum (East China)
Using field section observation, logging and other data, a set of downcut valley sedimentation and a variety of gravity flow sedimentation combinations were identified in the Lingshan Island area of eastern Shandong through outcrop and core observation, thin section examination and particle size analysis. It is found that Lingshan Island is located on the steep slope of the Riqingwei Basin, and the main types of gravity flow sedimentation include landslide block, lower cut valley filling, turbid waterway filling, etc., and the whole constitutes a sedimentary sequence of water retreat, which has the characteristics of low-level system domain. The identification of the lower cut valley of Lingshan Island is of great significance for the division of sequence boundaries and stratigraphic comparison in the Riqingwei Basin.
SE01-A005
Güralp Smart Sensors - A Comparison of Next Generation Mid-band Seismometers and Traditional Sensor Technologies
Ella PRICE#+, Neil WATKISS
Guralp Systems Ltd
Mid-band seismometers usually have shorter period responses and higher noise floors when compared to broadband seismometer sensors. These seismometers have been hugely popular with permanent seismic networks and temporary experiments alike due to their cost-effectiveness, portability and ease of deployment allowing for network densification and rapid use. Güralp have historically led the way with such sensors with the 6T and 40T series which have been used globally in challenging environments over recent decades for local and regional seismic monitoring applications. Guralp have built on this tried and trusted platform to develop the next generation of mid-band sensor technology. The Güralp next-generation smart sensor module is designed to operate at any angle, without the use of a mechanical gimbal. This enables the entire sensor package to be rotated during installation and deployment without sacrificing data quality. All three components of the sensor are manufactured to the same design, eliminating inconsistencies in performance between horizontal and vertical components whilst maintaining an orthogonal orientation for redundancy. The new generation of sensor utilises novel materials and techniques to drastically improve the noise performance over traditional mid-band sensors. The sensor components include digital elements to the feedback loop, allowing for the sensor module to have an on-board serial server. This facilitates greater interoperability with Minimus based digitizer platforms, including automatic provision of sensor serial number, SOH channels and access to remotely adjust the long period corner between 1s and 120s. This makes the sensor module incredibly easy to deploy and mitigates against previous requirements for multiple instruments of varying responses. The sensor module has been successfully developed into a number of different packages for varying deployment scenarios including borehole (the Radian), offshore (Aquarius and Maris), vault (Certimus) and posthole (Certis) application. All packages use the latest digital technologies to reduce power consumption down to <300mW.
Session Chair(s): Sang-Mook LEE, Seoul National University
SE12-A021
| Invited
Future Deep: Future Drilling to Explore Earth’s Past
Sarah KACHOVICH#, Ron HACKNEY+
Australian National University
This presentation will provide an overview of existing proposals and new ideas for scientific drilling or Legacy Asset Projects in the regions that are a key focus for the Australian and New Zealand IODP Consortium (ANZIC), i.e. around Australia, New Zealand and Antarctica, and also in the southwest Pacific and Southern Ocean. Existing proposals and emerging ideas from the ANZIC community include, but are not limited to, constraining and understanding Antarctic ice-sheet stability, Southern Hemisphere paleoclimate, hazards linked to earthquakes and submarine slides, coral reefs and sea-level change, evolution of arcs and ocean plateaus, aquifers on continental shelves, value add through land-to-sea drilling and coring, microbiology, and human migration across now-submerged landscapes. Many of these initiatives align with the following science priorities that were identified during and after ANZIC’s planning workshop Future Drilling to Explore Earth’s Past (Future DEEP), held in April 2023:· Antarctica and the Southern Ocean coordination· Ground-truthing future climate change· Geohazards· Coastal zone· Kickstarting Australian ICDP membership· Legacy Assets Projects· Deep biosphere with funding now secured until mid-2027, ANZIC welcomes the opportunity to explore synergies between the above priorities and those with the rest of the Asia and Oceania region and to establish new collaborations that will further the goals of post-IODP scientific ocean drilling and enhance cooperation with the International Continental Scientific Drilling Program.
SE12-A016
Investigating the Necessity for Ocean Drilling of the Indian Ocean Seamounts
Jose JOHN SAVIO#, Bijesh CHERIYA MOOTHOOR, Nisha NAIR+, John Kurian PALAYIL
National Centre for Polar and Ocean Research
Seamounts provide critical information about the evolution of ocean basins and their interconnections with global tectonic processes. Morphometric parameters, geological and geophysical signatures, and distribution of seamounts across the ocean floor offer insights into past plate movements, dynamic interplay between mantle plumes, and hotspot volcanism. In addition, seamounts are repositories of paleomagnetic records and also serve as platforms for marine mineral formation. The rich diversity and largely unexplored nature of seamounts in the Indian Ocean present a unique opportunity to advance our understanding of tectonic and geodynamic processes, which lead to the formation of seamounts, paleoceanography, seamount mineralization, and the associated biodiversity. While various drilling experiments have targeted seamounts, however, the majority took place in the Pacific and Atlantic oceans, exploring sites like the Hawaiian-Emperor seamount chain, Mariana forearc seamounts, Louisville Seamount Trail, Rio Grande Rise, and others. The Indian Ocean hosts a number of seamounts, primarily formed by intraplate volcanism through hotspot activity. Drilling experiments specifically targeting seamounts of the Indian Ocean region are very limited. To address this knowledge gap, international partnerships among researchers and institutions are crucial, particularly in identifying key seamounts for targeted drilling, developing models of seamount evolution, conducting plate tectonic and paleoenvironmental reconstructions, identifying potential mineralization zones and understanding the implications of seamount ecosystems on biodiversity. Through the collaborative efforts of expertise and resources, this initiative aims to unravel the mysteries surrounding Indian Ocean seamounts, significantly contributing to our knowledge of Earth's dynamic processes and their implications for regional and global marine geology.
SE12-A008
Collaboration in Ocean Drilling on the Sunda Shelf
Zhifei LIU1#+, Thanawat JARUPONGSAKUL2, Noor Cahyo D. ARYANTO3, Edlic SATHIAMURTHY4
1Tongji University, 2Chulalongkorn University, 3National Research and Innovation Agency, 4University Malaysia Terengganu
The Sunda Shelf in SE Asia is the largest tropical shelf in the world and offers extraordinary conditions for comprehensive high-resolution studies to reconstruct major geomorphic changes in land-sea distribution and to assess associated interactions with global climate. We have proposed the collaboration through drilling the shelf on IODP Proposal #1007, entitled “Evolution of the Pliocene-Pleistocene Tropical Sunda Shelf (SE Asia): Reconstructing Sea Level Change, Drainage System Development, and Carbon Cycling”. The scientific objectives include: (1) to document the history of eustatic sea-level and coastline migration fluctuations, (2) to reconstruct the development of major river systems in the Sunda Shelf region, and (3) to evaluate the contribution of the glacial exposure of this major tropical shelf region as a massive sink for carbon over the past 5 Ma. Substantive collaboration needs to be carried out in neighboring countries to achieve the objectives of the drilling program, particularly among Thailand, Malaysia, Indonesia, and China. Collaboration with other participating countries is also highly encouraged, including Vietnam, Cambodia, Japan, Germany, France, United Kingdom, Switzerland, and United Sates. The recent 4th International Workshop on Drilling the Sunda Shelf (8-9 November 2023, Shanghai) further clarified the cooperation on a pre-study plan, including drilling/coring and analysis of testing cores, investing outcrop profiles formed during sea-level highstands, and interpreting seismic data for local drainage evolution. This presentation will also look forward to the promising prospects of collaboration in ocean drilling on the Sunda Shelf.
SE12-A019
Fostering Ecosystem for Marine Geoscientific Research in Indonesia Towards Global Engagement in Ocean Drilling Program
Nugroho D. HANANTO#+
National Research and Innovation Agency
Marine geoscientific research in Indonesia face the challenges of low critical mass of human resources, infrastructure and funding. These leads to a significantly low contribution to the development of science, technology and innovation of Indonesian scientists at national and global level. To overcome these challenges, in 2021, the Indonesian Government have decided to consolidate all research and innovation agency/institutions into single national agency (National Research and Innovation Agency, BRIN). The first role of the agency is to provide science/evidence-based policy at national (ministerial and agencies) and regional levels. Furthermore, the agency is to improve science and technology, research and innovation ecosystem trough roles as funding agency and executing agency. Focusing on marine geoscientific research, fostering a robust ecosystem requires a multifaceted approach. The first approach is to deploy large scale investment on infrastructures including research vessels and dedicated laboratories to provide sufficient means for researchers and their global partners to conduct marine geoscientific research in Indonesia. Opportunity to use facilities will be based on inclusivity to provide the nation with data and information according to national research priorities. The second approach is to provide funding scheme for research projects that can be accessed by the researcher trough a competitive open selection. This includes facilitates joint research projects with renowned marine geoscientists and institutions worldwide to leverage their expertise and resources including seek for partnership scheme with international organizations involved in ocean drilling programs. The third approach is to promote human resources development through Ph.D training, mentorship and internship for young and early career scientists and engineers. The agency also provide program to invite foreign researchers/professors to work with Indonesian scientists in their labs in Indonesia. By implementing these approaches, Indonesia can create a dynamic ecosystem for marine geoscientific research and actively participate in global ocean drilling programs.
SE12-A017
Orbital Scale Cyclicity of Sea Surface Temperature Over the Past 10 Million Years
Kyung-Eun LEE#+, Tae Wook KO
Korea Maritime and Ocean University
Various past temperature proxy records indicate long-term cooling of Earth’s climate during the past 10 million years. Yet, the existing records lack the temporal resolution needed to identify climate dynamics. Here, we present a new, extremely highly resolved (1 to 3 kyr), continuous alkenone temperature record spanning the past 10 million years, from the middle latitude northwestern Pacific margin to understand temperature response to climate forcing. Comparisons between changes in temperature, sea level (e.g., polar ice sheet volume) and astronomical cycles reveal that changes in periodicity of temperature ice sheet volume were generally modulated by those of eccentricity and obliquity over the past 10 Ma. However, the intensity of temperature and ice sheet volume changes varied over the entire time period. We compared our temperature record with those from the subarctic and western and eastern equatorial Pacific oceans, anticipating being able to reconstruct the evolution/variability of the subpolar front and North Pacific subtropical gyre during the northern hemisphere glaciation.
SE12-A015
Exploring the Role of Ocean Drilling Experiments in Advancing Present Understanding of Submarine Slope Failures in Indian Ocean Regions
Bijesh CHERIYA MOOTHOOR#+, Nisha NAIR, John Kurian PALAYIL
National Centre for Polar and Ocean Research
The submarine slope failure events, along passive and active continental margins, globally have been a key topic of interest to marine geoscientists for the past few decades. They play a pivotal role in transporting massive amounts of sediments to the deep offshore, thus shaping the continental margins. The events also control many socio-economic aspects including Tsunami threats, destruction to deep-offshore oil industry structures, offshore infrastructure, and submarine cable damages. Researchers face significant challenges in characterizing such events especially due to the scarcity of relevant marine geophysical/geological data sets, pertaining to sub-seafloor structural information. The ocean drilling experiments carried out in different continental margins over the globe have greatly contributed to the understanding of slope failure events (e.g. Gulf of Mexico, Norwegian Continental Margin). However, there is a noticeable gap in such investigations in the Indian Ocean region, which encompasses several low-gradient passive continental margins identified as large-scale slope failure-prone zones (e.g. Indian Continental Margin, Australian Continental Margin). The information derived from deep sea drilling experiments, provides critical data regarding sedimentation rates, pore pressure, fluid flow, tectonic/structural understanding, which can significantly enhance understanding of slope failure events along continental margins. This knowledge can directly contribute to predicting areas prone to failure, modelling probabilistic tsunamis, understanding the impact of fluid flow and gas seepage on slope stability, and also in assessing any possible threats to offshore industry and infrastructures. Given the substantial socio-economic impact of slope failure events, ocean drilling experiments focusing on this perspective are poised to exert a profound influence in the future.
SE12-A002
Repository Core Re-discovery Program (ReCoRD)
Minoru IKEHARA1#+, Junichiro KURODA2, Yusuke KUBO3
1Kochi University, 2The University of Tokyo, 3Japan Agency for Marine-Earth Science and Technology
In 2023, Japan Drilling Earth Science Consortium (J-DESC) and Kochi Core Center (KCC) launched a new program called "Repository Core Re-Discovery Program (ReCoRD)" that utilizes repository cores at KCC taken from the Indian Ocean and Western Pacific Ocean by DSDP, ODP, and IODP. Repository cores can be used for academic purposes by anyone who submits a sample request under the current IODP policy. ReCoRD aims to create new findings by reanalyzing core samples under this policy system, which is implemented by larger research teams composed of international and interdisciplinary researchers like science parties on an IODP expedition, rather than individuals or small groups. The drilling community members review ReCoRD Implementation Proposals submitted by researchers for their scientific significance, feasibility, and future expansiveness, and highly evaluated proposals will be forwarded to KCC. One or two proposals could be adopted by the KCC each year. According to the ReCoRD Data-Sample Request, non-destructive analyses of the targeted core samples will be conducted using analytical instruments at KCC (e.g., image scan, X-ray CT scan, and ITRAX). In parallel with the non-destructive analyses of core samples, individual IODP sample requests will be solicited from researchers who wish to participate. We believe that the ReCoRD program will contribute to promoting the Flagship Initiatives in the 2050 Science Framework. The first project in the Indian Ocean was conducted in 2023 summer (ReC23-01). The second (ReC23-02) and third projects (ReC23-03), focusing on the geological structure of the Japan Trench and the Miocene of the Japan Sea, will take place in 2024. In the near future, the project might be internationalized through collaboration/integration with Scientific Projects using Ocean Drilling ARChives (SPARCs) and Ocean Drilling Legacy Assets Projects (LEAPs).
SE12-A011
Multi-functional Research Vessel Tamhae3
Jinho KIM#+, Nam-Hyung KOO, Moo KANG, Kyong-O KIM, Gee-Soo KONG
Korea Institute of Geoscience and Mineral Resources
The construction of Tamhae No. 3 would be carried out from 2018 when the design began to 2024, when she will be delivered. She was built as a multi-functional 3D/4D geophysical research vessel that can explore submarine resources in waters around the world, including continental shelves, deep oceans, and the Arctic Ocean. The information and specifications of Tamhae3 are as follows. The length, width, and draft is 92 m, 21m, and 7.2 m, respectively. The gross tonnage is about 6,926 ton. The seismic exploration system includes 6 km x 8 streamers and 6 air gun arrays of 6,000 inch3. For the shallow and high resolution 2D/3D seismic survey, she has P-cable systems of 8 streamers. For the 3D/4D surveys of CCS, we installed 400 nodes of multi-component OBN system and could monitor a leakage in the underground before and after CO2 injection to the seabed. Tamhae3 can acquire potential field data through gravity meter and magnetometer as the conventional marine geophysical exploration. Also, single-beam and multi-beam echo-sounders were mounted on the blister of the bottom of Tamhae3, where SBP, ADCP, and wide-band echo-sounder were installed. In addition to, underwater precision positioning equipment and SVP were installed for precise position and depth survey, respectively. For the marine geology and geochemistry, we have multi corer, piston corer, and marine geochemical analytical equipment like micro gas chromatography which was contained in a movable container. The maximum range of the ship is about 20,000 NM for 60 days and she can acquire the data under sea state 5. She covers Ice-Class 1B and has DP2 as a dynamic positioning. Through exploration using Tamhae 3, we can present a vision for solving global issues related to the global climate change, geological disasters, and carbon dioxide reduction.
SE12-A001
The Significance of Well Logging Technology in Ocean Drilling Investigations
Weichao YAN#+, Ximei JIANG, Huilin XING
Ocean University of China
Well logging technology plays a crucial role in ocean drilling investigations. Most ocean drilling projects conduct well logging operations to obtain the rock physics characteristics of the marine geology, including geological features such as electrical properties, acoustic properties, elastic properties, and radioactive properties. They are essential for addressing geological questions such as stratigraphic interfaces, formation pressure, and the distribution pattern of structural fractures. In comparison to laboratory testing after core retrieval, well logging technology provides accurate rock physics characteristics under in-situ temperature and pressure conditions, with a small sampling interval that allows for the generation of continuous depth profiles of specific rock physics features. Despite the wealth of well logging data collected during ocean drilling expeditions, the limited number of well logging analysts for scientific drilling results in a lower utilization rate of well logging data. Therefore, there is a need to strengthen the analysis of logging data for future ocean drilling investigations. Taking the International Ocean Discovery Program (IODP) Expedition 372 (Hikurangi margin, New Zealand) as an example, various well logging tools such as geoVISION, SonicScope, NeoScope, proVISION Plus are introduced, emphasizing the role of well logging data in addressing questions related to marine geological sciences.
SE12-A020
Novel Autonomous and Cabled OBS Solutions for Offshore Seismic Research
Ella PRICE#+, Neil WATKISS
Guralp Systems Ltd
Seismologists have historically focused on land-based seismic research, due to the logistical and financial challenges presented by offshore installations. Güralp has developed technology which allows the seismology community to monitor offshore seismicity with greater ease, improving global seismic data resolution. Autonomous free-fall OBS units provide flexibility of deployment and redeployment in different locations. The Güralp Aquarius functions at any angle without using a gimbal system, and can wirelessly transmit SOH and seismic data to the surface via an integrated acoustic modem. This allows researchers to monitor and transmit data packets without offshore cabling, reducing logistical challenges whilst maintaining some degree of real-time data transmission. This has made the Aquarius well suited for instrument pools, such as the National Facility for Seismic Imaging in Canada. Alternatively, cabled solutions provide access to high-resolution data in real-time via a physical link to on-shore infrastructure. The Güralp Orcus provides a complete underwater seismic station with observatory grade seismometer and strong-motion accelerometer in a single package. The slimline Guralp Maris also provides a more versatile solution, making use of the same omnidirectional sensor as the Aquarius and can be installed either on the seabed or in a narrow-diameter subsea borehole. SMART cables show great potential for increasing the number of cabled ocean observatory deployments in the future with substantially reduced deployment costs to the research institute. Combining several applications into a single system, including seismic monitoring and telecommunications, large scale monitoring networks can be created cost effectively by combining efforts from several industries. Güralp is leading the way with a demonstration SMART Cable system to monitor volcanic and seismic activity in the Ionian Sea in collaboration with Instituto Nazionale Di Geofisica e Vulcanologia (INGV). This will be the first practical demonstration of this technology and there are plans for additional projects in the future.
Session Chair(s): Minoru IKEHARA, Kochi University
SE12-A005
Drilling Into the Caroline Plate in the Equatorial Western Pacific for Understanding the Formation and Rotational Evolution of Microplates and Back-arc Basins
Sang-Mook LEE#+
Seoul National University
The Caroline Plate is a mysterious microplate located in the equatorial Western Pacific. Several trenches surround it, the polarity of which remains debatable. However, extensional basins known as the Ayu Trough exist on the western side. The plate is primarily divided into two north-south spreading basins, the West and East Caroline Basins, with the Eauripik Rise in the middle. The location of the Eauripik Rise between two spreading centers suggests that it must be a leaky transform fault, but the exact nature of the rise remains unknown. Identifying the various tectonic elements of the Caroline Plate by drilling and analyzing the geochemistry of basement rocks is important for understanding the early tectonic evolution of the microplates and back-arc basins in the western Pacific. The Caroline Plate would likely have rotated if it evolved as a back-arc basin. By deploying a new borehole magnetometer, one may resolve the amount of rotation the basins have undergone over time. Such information would be critical in understanding other back-arc basins along the continental margin. In this presentation, I would like to elucidate how deep scientific drilling into the Caroline Plate and surrounding regions can lead to a better understanding of the nature of microplates and back-arc basins in general. I will also provide existing data and present-day knowledge of this region.
SE12-A003
Deep Drilling Into Ontong Java Plateau Basement Using a Combination of Riser and Non-riser Drilling System
Xixi ZHAO#+, Jian LIN, Qingsong LIU
Southern University of Science and Technology
Oceanic plateaus are the most important targets to elucidate the link between the dynamics in the Earth’s deep interior and their impact on the Earth’s surface through volcanic activity. Three enormous Pacific oceanic plateaus (Ontong Java, Manihiki and Hikurangi) formed at ~122 Ma and coincided with Oceanic Anoxic Event 1a. The Earth’s magnetic field also stopped reversing during this time interval (the Cretaceous Normal Superchron). Existing models for the origin of the Ontong Java Plateau cannot account for all of the observations made for the world’s largest igneous province (LIP). Drilling of the plateau basements during past DSDP and ODP cruises, using one drilling platform of JR-type non-riser ship, have significantly increased our knowledge of their structure, composition and age. However, the origin of oceanic plateaus is still controversial mainly due to the difficulty in drilling to depths of more than a few hundred meters into igneous basements. To develop models that satisfy existing data, new samples of Lower Cretaceous sediment and basement both on and off the Ontong Java Plateau are required. Future drilling into the igneous basements using a combination of riser and non-riser drilling systems over the next decade, would provide important information on the vertical and lateral variations in the lithospheric structure beneath the plateau, and may provide major breakthrough in understanding the enigmatic origin of the Ontong Java Plateau. Deep drilling should also provide unique and continuous archives and legacy data (such as the Earth's magnetic field intensity in Cretaceous) for understanding the physical and geological processes in the core and lithosphere and the formation of the large igneous provinces. A better understanding of LIP formation can help probe and evaluate how other terrestrial planetary bodies have evolved, where LIP magmatism rather than plate tectonics appears to be the norm (e.g., Mars, Moon, Venus, Mercury).
SE12-A007
Unravelling Thermal and Viscosity Structures of Mud Volcano 420 by Overpenetration of the Heat Probe in the Arctic Canadian Beaufort Sea
Young-Gyun KIM1#+, Jong Kuk HONG2, Young Keun JIN2, Byung-Dal SO1
1Kangwon National University, 2Korea Polar Research Institute
The physical properties of marine sediments far below the seafloor have only been explored via drilling by a well-equipped drill ship or a remotely operated drilling machine. Given equipment limitations, conventional gravity coring is not suitable except in regions of extremely soft lithology. Mud volcanos have been identified to act as one of the sources of methane emission from the marine sediments into the water column, and their quantitative flux assessment has received increasing attention. Due to the upward migration of fluid-rich sediments, the seafloor and mud volcano subsurface provide low strength, allowing the gravity corer to penetrate significantly deep into the seafloor. At Mud Volcano 420 in the Arctic Canadian Beaufort Sea, the gravity corer-based Ewing-type heat probe reached approximately 80 meters below the seafloor during IBRV Araon’s Arctic expeditions in 2017 and 2022. Pressure and temperature sensors (attached to the heat probe) and tension and velocity sensors (attached to the winch tethering the probe) allowed us to investigate the thermal and viscosity structures of Mud Volcano 420. Preliminary analysis indicated that thermal and viscosity were not linear with depth but had distinct depths of the local maximum. Despite the observed limitation of the vertical properties, we propose that these two structures enable us to assess eruption dynamics. If a perennial eruption supported by high buoyancy of fluid-rich sediments in the mud volcano occurs, we can calculate the first-order annual methane flux, based on the methane concentration in the pore waters. In this study, we present our preliminary results from overpenetration experiments of the heat probe at Mud Volcano 420.
SE12-A014
| Invited
Scientific Ocean Drilling in the Northern Indian Ocean for Unravelling the Tertiary-quarternary Records of Geological, Oceanographic and Tectonic Processes
Nisha NAIR#+, John Kurian PALAYIL
National Centre for Polar and Ocean Research
The northern Indian Ocean hosts large sedimentary deposits, which is a significant repository of paleoclimatic events in the region. Recent IODP (International Ocean Discovery Program) drilling in the northern Indian Ocean (353 Bay of Bengal/Andaman Sea; 354 Bengal Fan; 355 Indus Fan; 359 Maldives) opened a new phase of understanding the Indian Monsoon, however, there are still missing records. Recovering deep tectono-sedimentary archives from this region will help in closing the large gap in understanding the short- and long-term evolution of the Indian Monsoon, evolution of the Oxygen Minimum Zone (OMZ) in time and space within the Cenozoic, paleo-circulation, provenance and the timing of tectonic events etc. The Andaman-Nicobar subduction system along the northeastern Indian Ocean, is a unique margin due to being seismically active and strongly influenced by the monsoon system, which brings heavy rainfall and complex oceanographic conditions. The transition between convergence and transpressional tectonics leading to the subduction of thick pile of sediments thereby developing a broad forearc with a heavily faulted accretionary wedge, stress condition and their potential for tsunamigenic hazard, volcanic arcs and a heavily-sedimented backarc basin in a strike-slip dominated system makes Andaman a unique margin among the world oceans. Therefore, investigating the detailed geologic structures and rock properties in Andamans and nearby regions can address an array of high-priority objectives relevant to the IODP science. Thus, planned deep sea coring including wire line logging in this region can help to achieve insights into geological history of the northeastern Indian Ocean, the tectonic processes, and climate interactions.
SE12-A006
Preliminary Paleoceanographic Study for the Ocean Drilling at the Conrad Rise in the Indian Sector of the Southern Ocean
Juyeon YANG1, Minoru IKEHARA2, Hyuk CHOI1, Boo-Keun KHIM1#+
1Pusan National University, 2Kochi University
In this study, we conducted the preliminary study using the multi-proxy (biogenic opal, CaCO3, total organic carbon (TOC), total nitrogen (TN), C/N ratio, and carbon isotope (δ13C) of sediment organic matter) for a 10.47 m long COR-1bPC (54° 16’ S, 39° 46’ E; water depth 2828 m) that was collected at the Conrad Rise in the Indian sector of the Southern Ocean. The AMS 14C dating of planktonic foraminifera (N. pachyderma) refined the estimated age of COR-1bPC to be about 43 ka at the core bottom. Variation of multi-proxy was divided into the three interval, representing the hydrographic evolution of surface and bottom water properties. In terms of biogenic opal content, the diatom productivity in the surface water was low during the last glacial period, increased abruptly during the deglacial period, and remained high during the Holocene. In terms of CaCO3 content, the variation pattern of carbonate productivity was similar to that of biogenic opal content, but the dissolution effect was incredibly strong during the last glacial period. In contrast to the surface water productivity, TOC and TN contents, representing the marine organic matter, was high during the last glacial period and low during the Holocene with an abrupt decrease during the deglacial periods. Such variation implies that the preservation of TOC and TN contents was influenced more by the degradation rather than the production, which was supported by the relationship with C/N ratio and δ13C value. It indicates the change of dissolved oxygen concentration of the bottom water from the last glacial period to the Holocene. Core COR-1bPC records the paleohydrographic evolution of surface water and bottom water properties at the Conrad Rise in the Indian sector of the Southern Ocean since the Last Glacial Maximum.
SE12-A012
Melt-rock Reaction in the Lower Oceanic Crust and the Influence on the Evolution of Mid-ocean Ridge Basalts at the Central Indian Ridge (7°50’–8°30’s)
Sarang CHOI1#+, Jung-Woo PARK2, Jonguk KIM3, Jihye OH3, Changkun PARK4, Seung Hee HAN4
1Seoul National University, 2School of Earth and Environmental Sciences, Seoul National University, 3Korea Institute of Ocean Science & Technology, 4Korea Polar Research Institute
Various crustal processes shape both the lower oceanic crust and mid-ocean ridge basalts (MORBs). To better understand how these crustal processes influence MORB compositions, we conducted comprehensive petrographic and geochemical investigations on gabbroic rocks and erupted lavas dredged from a segment of the Central Indian Ridge (CIR) spanning from 7°50'S to 8°30'S.The petrographic and geochemical analyses of the gabbroic rocks revealed evidence of melt-rock reaction through reactive porous flow (RPF) in olivine-rich troctolite (Ol-rich troctolite), plagioclase-rich troctolite (Pl-rich troctolite), and gabbro. This process resulted in distinctive features in clinopyroxene, including disequilibrium textures with a troctolite/anorthosite matrix, complex variations in Mg#-Cr-Ti relationships, and considerable enrichment and fractionation of incompatible trace elements. A significant finding of our study is the close resemblance of trace element ratios in MORB and olivine-hosted melt inclusions to those of melts in equilibrium with clinopyroxene from Ol-rich troctolite, Pl-rich troctolite, and gabbro with Sr anomaly greater than ~0.7. This observation strongly indicates that the composition of MORB is influenced by the melt-rock reaction taking place in the lower oceanic crust. Furthermore, our findings suggest that evolved melts in equilibrium with clinopyroxene having Sr/Sr* values lower than ~0.7 are less likely to erupt onto the seafloor and are instead trapped within the lower oceanic crust. Finally, we present a comprehensive model for melt evolution in the lower oceanic crust at the 7°50'S-8°30'S CIR by integrating all petrological and geochemical data obtained from gabbroic rocks, MORB, and olivine-hosted melt inclusions. This holistic model contributes to a better understanding of the intricate processes governing MORB composition in the context of the lower oceanic crust dynamics at slow-spreading ridges.
SE12-A018
The Rodrigues Depth Anomaly, Another Result of the Reunion Hotspot - Central Indian Ridge Interaction
Jerome DYMENT1#+, Marcia MAIA2, Christophe HÉMOND2, M. Rezah BADAL3, Dass BISSESSUR3, Hemanaden RUNGHEN3, Beenseh Anand MOTAH3, Arshad RAWAT3
1Université Paris Cité / National Centre for Scientific Research, 2Geo-Ocean, UMR6538 CNRS-IFREMER-UBO-UBS, Institut Universitaire Européen de la Mer, 3Department for Continental Shelf, Maritime Zones Administration & Exploration (CSMZAE)
The Rodrigues Ridge and Rodrigues Island have long been recognized as reflecting the interaction of the Reunion hotspot with the Central Indian Ridge (CIR; Morgan, J. Geophys. Res., 1978). New and existing geophysical data allow us to define the Rodrigues Depth Anomaly (RDA), a vast oceanic area shallower by ~0.5 km and thicker by ~1 km with respect to the surrounding areas. The RDA includes Rodrigues Island and a large part of the Rodrigues Ridge on the CIR southwestern flank but, unlike the former, extends symmetrically on the CIR northeastern flank as well. Its western and eastern ends are characterized by ~1 km-high shoulders that mark the sudden onset of the ridge-hotspot interaction at ~20 Ma. The crust (as derived from the joint analysis of bathymetric and gravity data) progressively thins toward the CIR, although it remains thicker in two areas of the CIR centered around 18°15'S and 19°30'S. Noticeably, these areas display the most abundant volcanic activity in the last 2 Ma (with, in the second one, the Gasitao and Three Magi ridges) and are characterized by gaps of seismicity for the last 50 years, both observations being consistent with a stronger magmatism. Beyond the variety of bathymetric features known to reflect ridge-hotspot interactions including seamounts, ridges, and plateaus, depending on the hotspot strength, distance to and relative motion with the spreading center, and spreading rate (e.g., Dyment et al., Oceanography, 2007), we propose depth anomalies such as the RDA to be another less prominent but probably widespread type of bathymetric features formed as the result of more abundant magmatism at the spreading center resulting from the ridge-hotspot interaction.
Session Chair(s): Yasuyuki KANO, The University of Tokyo, Kenji SATAKE, National Central University
SE02-A005
| Invited
Potential Seismic Hazards and Strong Ground Motions in Seoul, South Korea
Byeongwoo KIM#+, Tae-Kyung HONG, Junhyung LEE, Seongjun PARK, Jeongin LEE
Yonsei University
Public concern regarding the potential occurrence of devastating earthquakes grows in Seoul, the capital city of South Korea where historical seismic damage was reported. The seismic activity in Seoul is predominantly characterized by strike-slip earthquakes, with fault planes aligned in the NNE–SSW direction, responding favorably to the ambient stress field. Seismicity rates are observed higher in the northwestern Seoul at depths of < 10 km. Micro-to-small earthquakes occur episodically in the central Seoul along the Chugaryeong fault system, traversing the city in a N-S direction. We examine historical seismic damages using numerical modeling of strong ground motions, confirming the occurrence of historical earthquakes. Seismicity distribution, focal mechanism solutions, geological features, and seismic and geophysical properties suggest the potential existence of earthquake-spawning blind faults in Seoul. We assess seismic hazard potentials for scenario earthquakes with magnitude Mw5.4 and focal depth of 7 km. Numerical modeling suggest upper bounds of peak ground accelerations to be ~11 m/s², presenting high seismic damage potentials, particularly in areas around river sides covered by alluvium. This information proves valuable for the prevention of seismic damages in the event of a plausible earthquake in Seoul.
SE02-A003
Re-examining the Dates of Japanese Historical Earthquakes at Midnight or Before Dawn
Kazuki KOKETSU1,2#+, Yuma KAMEI1, Satoko OKI1
1Keio University, 2The University of Tokyo
In pre-modern Japan, time was expressed using the 12-division system, which is based on that in China. This is an irregular time system, but each division can be approximately 2 hours. The divisions were called as times of animals and others. Among them, Time of Rat refers to midnight and 1 hour before and after that. This implies that Time of Rat on a certain day includes the period from around 23:00 to 24:00 on that day and the period from around 0:00 to 1:00 on the next day. In addition, in pre-modern Japan, the sense of date change was different from that in modern Japan. According to Hashimoto (1978), in the Heian period (784−1185), the date was changed between Times of Ox and Tiger, which is around 3:00. In the Edo period, there was a sense that the date changed at Time of Rabbit, which corresponded to the sunrise. When using historical earthquakes for scientific research, we need their dates in the modern sense. We thus reexamined the dates of historical earthquakes that were listed in Usami et al. (2013) with Times of Rat, Ox, and Tiger. The results were presented with O (left as is), ∆ (left as is in List, should be changed in DBs), X (should be changed), and ? (cannot be judged). Because of the circumstances mentioned above, it is often difficult for Time of Rat earthquakes to be judged based only on historical documents. Therefore, out of 10 of them, 5 were ?, 4 were O, and 1 was X. However, out of 25 Time of Ox earthquakes, only 4 were ?, 11 were O, 8 were ∆, and 2 were X. Out of 19 Time of Tiger earthquakes, 3 were ?, 13 were O, 2 were ∆, and 1 was X.
SE02-A007
Historical Tsunamis on the East Coast of Korea Originated from Japan
Kenji SATAKE1,2#+, Satoko MUROTANI3
1National Central University, 2University of Tokyo, 3National Museum of Nature and Science
The January 2024 Noto Peninsula earthquake (M 7.6) in Japan generated tsunami which was recorded on the east coast of Korea. The Korean coast has suffered from similar historical tsunamis from Japan. The most recent one was from the 1993 SW off Hokkaido earthquake (M 7.8), and the tsunami heights exceeded 2 m at Imwon. The previous 1983 Japan Sea earthquake (M 7.7), which occurred off Akita coast, caused the larger tsunami, about 5 m at Imwon, and caused significant damage including fatalities. Oshima-Ohshima, a small volcanic island located between the source regions of the 1993 and 1983 earthquakes, erupted in 1741 and caused the worst tsunami damage in Sea of Japan. The tsunami damage on the east coast of Korea was recorded in “Annals of Choson Dynasty,” and the tsunami heights were estimated as 3 to 4 m. To the north of the 1993 event, the 1940 Shakotan-oki earthquake (M 7.5) generated tsunami which was recorded at Najin in North Korea. To the south of the 1983 event, the 1833 Shonai-oki (M 7.5) and 1964 Niigata (M 7.5) earthquakes occurred but the tsunami was not recorded on the Korean coast. Ioki et al. (2017, Earth Planets Space) modeled an earthquake fault model (M 7.9) near Oshima-Ohshima, based on the distribution of tsunami deposits found in Okushiri Island and Hokkaido and dated in 12th century. Hattori (2023, J. Disaster Res.) reported sea surface disturbances along the Korean coast on May 13 and 14 in 1415, based on the record in “Chronology of the Li Dynasty,”, but their origin (tsunami or storm surge) is not known. The tsunami propagation in Sea of Japan is affected by the bathymetry, particularly the Yamato Rise located in the center. The tsunami heights on the Koran coast vary depending on the location of tsunami source.
SE02-A013
Damages and Aftershock Sequence of the August 1, 1729 Earthquake Occurred in the Noto Peninsula
Yasuyuki KANO1#+, Masaharu EBARA2, Kenji SATAKE3,4
1The University of Tokyo, 2Association for the Development of Earthquake Prediction, 3National Central University, 4University of Tokyo
Several historical earthquakes are known to have occurred in the vicinity of the epicenter of series of Noto Peninsula earthquakes, including those occured on May 5, 2023, and January 1, 2024. One notable earthquake occured on August 1, 1729, with an estimated magnitude ranging from M6.6 to 7.0. Historical records document damages to houses, landslides, and subsequent seismic activities. A document recorded in temples in Yanagida, Noto Town, and Wajima City indicate that the earthquakes occured around noon, with the third one in the evening being particularly significant. Additional historical documents also note that among the multiple earthquakes on August 1, there were two instances of larger earthquakes. The number of felt records in historical documents has been compiled. As pointed out in a previous study, it is evident that aftershocks persisted for two weeks after the August 1 earthquake. No noticeable earthquakes were reported in Wajima after August 15. The aftershock sequence of the August 1, 1729 earthquake is comparable to that of the May 5, 2023 earthquake.
SE02-A004
Classification of Tsunami Monuments to Preserve the Disaster Caused by the 1792 Volcanic Tsunami in Kyushu, Japan
Koshiro KIBATA#+, Toshitaka BABA
Tokushima University
Mt. Unzen in Kyushu, Japan, erupted in 1792 with active seismicity. This volcanic activity also triggered large collapses of the mountain, causing sediment to drop into the sea and a massive tsunami. This tsunami killed people more than 15,000 in the surrounding region. After the catastrophic disaster, residents constructed many tsunami monuments to preserve the disaster for the next generations. In this study, we investigated the tsunami monuments of the volcanic tsunami and compared them with those in other areas where repeatedly suffered from tsunamis caused by interplate earthquakes. We investigated the year of construction, inscription on the monument, monument type (stones, wood records, marks of tsunami height, etc.), and location from databases and previous studies. Based on this information, the monuments were classified into four types: damage records, learned lessons, tsunami height marks, and comforts of the spirit of the dead. The total number of tsunami monuments in this disaster was 41, of which 37 were stone monuments to comfort the spirit of the dead. We also conducted site surveys and found some areas around the tsunami monuments ruined due to overgrown grass. On the other hand, in other areas where interplate earthquakes repeatedly caused tsunamis, there were 7 monuments for learned lessons, 12 for damage records, 21 for tsunami height marks, and 2 for comforts of the spirit of the dead. The tsunami monuments and the surrounding areas were well-managed. We could observe efforts to raise residents' awareness of disaster prevention by using the tsunami monuments. The 1792 volcanic tsunami caused by mountain collapses was the only one record since the beginning of history, whereas tsunamis caused by interplate occurred multiple times. The difference in the tsunami monuments between the two regions would be related to the frequency of disasters.
Session Chair(s): Ignacio GONZALEZ-ALVAREZ, CSIRO
SE17-A003
Securing REE Sources for Sustainable Energy Transition in the Republic of Korea: A Strategic Approach
Sujeong LEE#+
Korea Institute of Geoscience and Mineral Resources
Rare Earth Elements (REEs) play a crucial role in the energy transition, contributing to clean energy technologies, permanent magnets, catalysts in clean energy production, energy storage, and efficient lighting. As a nation heavily reliant on energy and mineral resource imports, Korea recognizes the critical importance of REEs in advancing its economic and environmental objectives. The Republic of Korea's strategy focuses on diversifying sources and reducing dependence on limited suppliers for REEs. With a strong emphasis on international collaboration, the nation aims to fortify its REE supply chain in alignment with global sustainable energy goals. This is particularly crucial as Korea anticipates a significant import of REEs, acknowledging their pivotal role in clean energy technology production. The government has designated 33 critical minerals, including REEs, guiding efforts to ensure responsible mining practices, ethical sourcing, and community engagement. This strategic initiative extends beyond meeting domestic demand, aiming to contribute responsibly to the global REE supply chain. Investment in research and development is a key pillar of Korea's strategy, fostering innovation in recycling technologies and alternative sources for REEs. By promoting a circular economy, Korea aims to mitigate environmental impacts and enhance the sustainability of its REE resource utilization. As part of these efforts, we are conducting collaborative international research to recover REEs from the mine tailings discharged at the Mt Weld mine in Australia. Through this initiative, we aim to establish a more robust supply chain connecting Australia and Korea.
SE17-A002
Recent Advances on Rare Earth Elements Recovery Using Non-aqueous Medium
Rina KIM+, Seojin HEO, Ho-Sung YOON#, Chul-Joo KIM, Kyeong Woo CHUNG, Sujeong LEE
Korea Institute of Geoscience and Mineral Resources
The recent surge in demand for environmentally friendly practices in metal production has led to extensive research in the hydrometallurgy field, with a focus on replacing conventional mineral acid-based processes. Particularly, non-aqueous solvents like deep eutectic solvents (DES) have emerged as a promising alternative. In this study, several DES-based hydrometallurgy results, emphasizing the leaching of both primary and secondary rare earth element (REE) resources, expected to witness increased demand in the context of clean energy transition, were reviewed. As primary resources, bastnaesite and monazite are well-known REE minerals. It was reported that REEs with higher atomic number can be selectively leached from REE carbonate, similar with bastnaesite, in various DESs with choline chloride (ChCl) as a hydrogen bond acceptor (HBA); similar promising results were observed utilizing bastnaesite ore. For monazite, a pre-treatment involving NaOH roasting enabled rare earth hydroxide formation, allowing for efficient REE leaching using ChCl-PTSA (p-toluenesulfonic acid) DES. Secondary REE resources, such as coal fly ash and NdFeB magnet carbonylation slags, were also investigated. DES leaching from coal fly ash containing 0.22% REEs exhibited superior performance, with leaching efficiency ranging from 85 to 95%, surpassing mineral acid leaching. In the case of NdFeB magnet slags, it showed the possibility of selective leaching of Nd from Fe in EG (ethylene glycol)-MA (maleic acid) DES. While DESs show promise as effective REE leaching agents, challenges remain. The notable obstacle is the high viscosity of DES, posing issues that need resolution for the scalable implementation of these processes compared to traditional aqueous-based hydrometallurgical methods.
SE17-A001
The Australian REE Ecosystem
Ignacio GONZALEZ-ALVAREZ1,2#+
1CSIRO, 2The University of Western Australia
Over the past 50 years, population growth and technological advancements have escalated global demand for mineral resources by 400%. Amidst a dynamic geopolitical, energy, and technological landscape, Rare Earth Elements (REE) have emerged as strategically crucial resources for the foreseeable future. Global economic reserves of REE, estimated at 120,000 kt, are concentrated predominantly in China (37%), Vietnam (18%), Brazil (18%), Russia (10%), India (6%), and Australia (3%). However, actual production is dominated by China (63%), the USA (12%), Myanmar (10%), and Australia (9%). Demand for specific REEs such as Dy and Nd is projected to soar by >2600% and >700% over the next 25 years. Contrary to their name, Rare Earth Elements originating from supernova nucleosynthesis are not rare. The challenge lies in locating REE deposits and identifying them in geopolitically favourable areas with acceptable extraction costs, minimal environmental impact, and positive social engagement. These deposits are associated with high-temperature magmatic and hydrothermal events (High-T) or low-temperature weathering and sedimentary processes (Low-T). Carbonatites and ion-adsorption REE deposits, particularly promising, pose distinct exploration challenges, such as the small carbonatite footprints and limited regional datasets for effective data analytics. Efforts to advance REE exploration hinge on developing mappable proxies for mineralization, identifying favourable geological or landscape settings, and recognizing key signs and footprints. With its vast potential for Low- and High-T REE deposits, Australia could emerge as a significant global supplier. The country's expansive, deeply weathered cover blanket offers immense potential, contingent on cohesive efforts from Industry, Government Research Institutions, and Universities to support exploration, facilitate discoveries, and engage in key international collaborations, positioning Australia as a fundamental REE supplier for global technological domains.
Session Chair(s): Benoit TAISNE, Nanyang Technological University
SE16-A007
Relatively Stable Pressure Effects and Time-increasing Thermal Contraction Control Heber Geothermal Field Deformation
Guoyan JIANG#+
Wuhan University
Due to geological complexities and observational gaps, it is challenging to identify the governing physical processes of geothermal field deformation including ground subsidence and earthquakes. In the west and east regions of the Heber Geothermal Field (HGF), in southern California, USA, decade-long subsidence was occurring when injecting heat-depleted brines, along with transient reversals between uplift and subsidence. These observed phenomena contradict current knowledge that injection leads to surface uplift. Here we show that high-yield production wells at the HGF center siphon fluid from surrounding regions, causing wide-area subsidence, even at low-rate injection locations. Moreover, thermal contraction increases gradually with time and eventually overwhelms the pressure effects of pressure fluctuation and poroelastic response, which keep relatively stable during geothermal operations. The observed subsidence anomalies result from the siphonic effect and thermal contraction. We further demonstrate that thermal contraction dominates long-term trends of surface displacement and seismicity growth, while the pressure effects drive near-instantaneous changes.
SE16-A012
| Invited
Deformation, Mixing, and Decoupling of Nd Hf Chemical Heterogeneities at Mid-ocean Ridges
Boda LIU1#+, Yan LIANG2
1Chinese Academy of Sciences, 2Brown University
Mantle rocks representing the residue of melting are petrological probes of the interior of the Earth. A common assumption in the interpretation of Nd-Hf isotope ratios of residue samples is that the residue retains the isotope ratios in the source. However, this assumption is debated because melt and solid of different isotopic composition could undergo chemical exchange, altering the isotopic signature of the source. By modeling the transport of chemical heterogeneities in the melting region beneath mid-ocean ridges, we show that the chemical heterogeneity marked by Nd or Hf isotope ratio is deformed and its isotopic signals could be damped and decoupled. At fast-spreading ridge, a maximum melt fraction of 1% has been observed. Our model shows that original circle-shaped heterogeneity is dispersed in between the solid flow and the effective transport velocity assuming chemical equilibrium. The Nd isotope ratio in the center of the chemical heterogeneity tends to decay to the value of background mantle. The amount of decay depends on the strength of dispersion, which itself is strongly dependent on the melt fraction. The melting region beneath a slow or ultraslow-spreading ridge have smaller or even zero melt fraction, which resulted in much weaker or no dispersion. Therefore, chemical heterogeneities beneath ultraslow and slow ridges can preserve larger isotopic variability in the source compared to fast ridges, which is consistent with observed Nd isotopic variability in residues of ultraslow and slow ridges compared to fast ridges. Current simulations also demonstrate that 2D mantle flow and melt migration at fast-spreading ridge produce chromatography fractionation of Nd with respect to Hf, causing their isotope ratios to decouple. Nd-Hf isotope ratios in the residue at ultraslow-spreading ridge stay coupled Spatial sampling of Nd and Hf isotope ratios is required to validate the effect of chromatography fractionation on Nd-Hf isotope ratios.
SE16-A016
Chemical Compositional Variation of Basalts of the Fuji Volcano, Central Japan, Decoded by Unsupervised Machine Learning
Yusuke KATSUKI1,2#+, Shuhei SAKATA1, Tatsuji NISHIZAWA3, Masaki TAKAHASHI4, Shun-Ichi NAKAI1, Hitomi NAKAMURA2, Satoru HARAGUCHI1, Hikaru IWAMORI1
1The University of Tokyo, 2Geological Survey of Japan, 3Mount Fuji Research Institute, 4Nihon University
Mt. Fuji has erupted voluminous basaltic to basaltic-andesitic lava flows for more than one hundred thousand years. The limited range in composition makes it difficult to elucidate magma processes beneath the Fuji volcano. To resolve the characteristics of such limited compositional variation and to extract statistically independent features hidden in the dataset, we applied an unsupervised machine learning technique, Independent Component Analysis, to the major element compositional dataset of whole rock samples. We identify four independent components (IC1-4) as the compositional vectors. Crystal fractionation simulation by MELTS with a variable H2O content and pressure of crystallization was also performed to deduce the geological processes/sources corresponding to the individual ICs. As a result, IC2 represents a vector with increasing Ti, Fe, K, P and decreasing Si, Al, Mg, Ca, which broadly reflects the compositional variability associated with different H2O contents at a similar temperature-pressure condition along the crystallization paths. IC2 is especially sensitive to the H2O content less than ca. 2 wt%. IC3 represents a vector with increasing Al and decreasing Mg, which broadly reflects the compositional variability with different pressures at a similar H2O-temperature condition along the crystallization paths. Both IC2 and IC3 likely represent the crystallization processes in the upper to mid crust where plagioclase and pyroxene are the major crystallization phases. The remaining two components, IC1 and IC4, have not been successfully explained by the crustal crystallization processes described above. IC1 represents a vector with increasing Si and decreasing Ti, Fe, Mg, K, P. IC4 represents a vector with increasing Si, Ti, and decreasing Fe, Mg. Plausible geological processes/sources that correspond to IC1 and IC4 will be estimated by performing more forward model calculations, including not only crystallization processes but also melting processes in the crust and upper mantle.
SE16-A015
Genetic Relationship Between High-silica Rhyolites and Dacites: A Case Study of the Early Cretaceous Felsic Volcanic Rocks in the Central Lhasa Subterrane
Yu HUANG1#+, Zhidan ZHAO2, Di-Cheng ZHU2
1Chang'an University, 2China University of Geosciences
High-silica rhyolites (SiO2 content>75%) represent the ultimate product of felsic magma evolution and provide crucial insights into crustal growth and differentiation. However, the effectiveness of crystallization differentiation, storage conditions, and ascent mechanisms in felsic magma remains a subject of debate due to its high viscosity and poor fluidity. The widespread occurrence of Early Cretaceous felsic volcanic rocks in the central Lhasa subterrane offers an exceptional opportunity to investigate magma generation, evolution, transportation, as well as crustal differentiation. In this study, we focus on the Early Cretaceous high-silica rhyolites and dacites from the Sailipu and Coqen areas in the central Lhasa subterrane by integrating zircon morphological studies, zircon U-Pb ages and Hf-isotope data analysis, bulk-rock major and trace element compositions characterization along with bulk-rock Sr-Nd-Pb isotope analysis. The high-silica rhyolites and dacites investigated in this study frequently occur together, exhibiting comparable ages and isotopic signatures, suggesting a plausible genetic association between them. The varying zircon εHf(t) values (−12.2 to +5.2) as well as the εNd(t) values (−9.5 to −1.1), imply an open-system processes involving both mantle-derived magmas and ancient crustal materials. The high-silica rhyolites are characterized by high SiO2 content (77.6-80.3 wt%, anhydrous basis), ratios of (FeO*/MgO) (4.1-6.9), and a differentiation index (DI = 84.6–91.3). However, they exhibit lower levels of MgO, TiO2, P2O5, and values for (10,000×Ga/Al) (1.66-1.79), suggesting significant magmatic differentiation has occurred in the formation of these samples. Zircon morphological studies, Hf isotopes analysis, and zircon thermometers indicate the occurrence of magma recharge and reactivation of crystal mush due to the input of hot mantle-derived magmas. We propose a two-stage model to explain the formation process of these high-silica rhyolites: polybaric crystallization during the ascent of dacitic magmas followed by subsequent crystallization at shallow depths prior to eruption.
SE16-A011
| Invited
Prolonged Near-solidus and Steady-state Magma Storage Leading to Thermal Maturation of the Toba Magma Reservoir
Ping-Ping LIU1#+, Dian-Bing WANG1, Luca CARICCHI2, Sun-Lin CHUNG3
1Peking University, 2University of Geneva, 3Institute of Earth Sciences, Academia Sinica
The Toba volcanic system in Indonesia has produced two of the largest eruptions (>2,000 km3 dense-rock equivalent [DRE] each) on Earth since the Quaternary. U–Pb crystallization ages of zircon span a period of ∼600 ky before each eruptive event, and in the run-up to each eruption, the mean and variance of the zircons’ U content decrease. Thermal and geochemical modeling of zircon U-Pb ages and U contents show that caldera-forming eruptions at Toba are the result of progressive thermal maturation of the upper crustal magma reservoir, which grows and chemically homogenizes, by sustained magma influx at average volumetric rates between 0.008 and 0.01 km3/y over the past 2.2 My. Greyscale intensity and Ti-in-quartz diffusion modeling also indicate that the residence time of quartz crystals within the crustal magma reservoir was estimated to vary from ∼100 to 400 kyrs, which is of similar orders of magnitude with those obtained by zircon U-Pb and allanite U-Th ages. Moreover, the majority of quartz crystals were crystallized at relatively low and constant temperatures during the repose period prior to the super-eruptions. We argue that sustained and stable magma influx, instead of pre-eruptive magma reheating, is essential to maintain the thermally steady-state Toba crustal magma reservoir and leads to thermal maturation with rapid aggregation of different magma batches prior to the super-eruptions.
SE16-A003
Probabilistic Analysis of Influence of Volcanic Ash from Volcanoes in Northeast Asia
Sungsu LEE1#+, Hee Jung HAM2, Yoo Jung KIM3, Seulgi LEE1
1Chungbuk National University, 2Kangwon National University, 3National Disaster Management Research Institute
The volcanoes that could potentially impact or cause damage in the Northeast Asian region consist of several active volcanoes located in the Korean Peninsula, Japan, and the northeastern region of China, including the well-known Mt. Baekdu (also known as Mt. Changbaishan). Furthermore, more than tens of active volcanoes situated in Russia's Kamchatka Peninsula pose a threat to the region, despite being over 3,000 km away. They can significantly affect air travel around the Korean Peninsula in the event of eruptions. In this study, we conducted a probabilistic analysis of the potential influence of volcanic ash on the northeast region of Asia using numerical simulations of volcanic ash dispersion. The simulations were based on meteorological data from 2005 to 2014, and hypothetical eruption scenarios for major volcanoes were considered. The results indicate that in the case of Baekdu and Aso volcanoes erupting with a volcanic explosivity index of 7, the highest probability of affecting the entire Korean Peninsula occurs when the eruption takes place between July and September. Meanwhile, ash predominantly affects Japan when eruptions occur during the spring and winter seasons. There is also a probability that ash can travel far enough to reach Okinawa and Taiwan. Additionally, if Ulreungdo experiences a similar eruption during the same period, there is a potential impact on the region. Most of these impacts are attributed to the pressure distribution of seasonal large air masses in the East Asian region. This research was conducted with the support of the National Disaster Management Research Institute under the Ministry of Public Administration and Security, as part of the project titled 'Development of Volcanic Ash Vulnerability Assessment Technology and Utilization Research on Risk Assessment Technology (1/2),' identified by the project code 'NDMI-JUYO-2023-08-03-02’
Session Chair(s): Yu WANG, National Taiwan University
SE15-A022
Active Faults and Earthquake Geology in South Korea
Jin-Hyuck CHOI#+
Korea Institute of Geoscience and Mineral Resources
The Korean peninsula has been considered a tectonically stable region due to no destructive earthquakes in modern society. Note that there is no historical records of any earthquake involving surface ruptures. After the 2016 Mw 5.5 Gyeongju earthquake, however, large-earthquakes has highlighted as an important issue to the public people. Also, multidisciplinary research projects were conducted for active fault mapping and paleoseismological investigations. Here I introduce the results of recent investigations associated with the pre-historical large-earthquakes. Particularly, I will focus on spatio-temporal history of earthquake surface ruptures along the Yangsan Fault in SE Korea. Also, I will present the geologic records of earthquake surface rupture on the Gongju Fault System in the central part of the S Korea. The smaller offsets indicate either moderate-sized earthquakes on minor faults or distributed deformation associated with the large earthquakes. I will discuss the characteristics of the crustal deformation of the Korean Peninsula and fault behaviors in very slow-deforming regions.
SE15-A007
Paleoearthquakes with Longer Recurrence Intervals on the Eastern Serteng Shan Fault Over the Past 90ka, North China
Xin SUN1+, Yanxiu SHAO2#, Wenjun ZHENG1, Xingwang LIU3, Yunsheng YAO3, Peng HUI1
1Sun Yat-sen University, 2China Earthquake Administration, 3Lanzhou Institute of Seismology
The purpose of paleoearthquake research is to reveal prehistoric strong earthquake events as much as possible through various methods, prolong the catalog of destructive strong earthquakes, and enable scientists to better understand the laws of strong earthquakes occurring on fault zones. The Ordos block with a stable interior in northern China has many active normal faults in its surrounding area. Many big earthquakes occurred on these normal faults in history. Several M7 historical earthquakes ruptured its north boundary, including the Lang Shan fault, the Serteng Shan fault, the Wula Shan, and the Daqing Shan fault. In this study, we conducted a paleoearthquake investigation along the eastern section of the Serteng Shan fault by large trenches. Seven events are identified by clear markers of colluvial wedges. The dozens of optically stimulated luminance dating brackets the events. The dating results show that the seven events occurred after ~90 ka B.P., and the recent five occurred after 50 ka B.P. The OxCal modeling indicates the most recent event likely occurred in 7.0 ± 1.1 ka B.P. The penultimate event was around 25.0 ± 2.2 ka B.P.; the other three events occurred in 35.6 ± 1.5 ka B.P., 41.3 ± 1.9 ka B.P., and 46.2 ± 2.4 ka B.P. from young to old. The recurrence intervals present greatly vary and long (>5 ka). Combining displacements of two high terraces and the corresponding ages and geometry of the main fault, we determine the uniform vertical slip rate of 0.12 ± 0.02 mm/yr during the last 90 ka.
SE15-A019
Rising the Namcha Barwa: Crustal Structure Beneath the East Himalayan Syntaxis and the Relation to Its Rapid Uplift and Exhumation
Hao DONG#, Jialin QI, Sheng JIN+, Gaofeng YE, Wenbo WEI
China University of Geosciences
The East Himalayan Syntaxis (EHS) is featured with an abrupt U-turn of all geological boundaries, geomorphic features and river systems at the east end of the Himalayan orogenic belt. The core part of EHS, also known as Namcha Barwa (NB), is believed to be the region with strongest Cenozoic uplift and exhumation in Tibetan Plateau. Different tectonic models have been proposed to explain the rapid uplift, which results in a series of high-angle faults and the exhumation of NB, despite the lack of high-resolution geophysical data to distinguish between them. To better understand the mechanism beneath the rapid growth of regional elevation, magnetotelluric array data were collected in 2020-2022 to constrain the 3D electrical structure beneath the EHS. The resistivity model reveals highly conductive anomalies around the NB region, which is interpreted to be the decompression melts caused by the rapid uplift of the region. On the other hand, the crustal structure directly beneath NB is imaged as highly resistive NNE directed wedge-shaped anomaly. Consistent with previous larger scale resistivity and velocity structures, the resistive “wedge” may reflect the northward intrusion of deep materials into the crust of the Lhasa block, which further induces the uplift of regional structure. With the gradual intrusion of the wedge, the uplift may gradually expand to the northeast, forming the long and narrow surface compound anticline responses and related fault systems.
SE15-A016
New Marine Heat Flow Observations in the Ulleung Basin, East Sea (Sea of Japan)
Young-Gyun KIM1#+, Yoon-Mi KIM2, Yunseok CHOI2, Seondong KIM3, Byung-Dal SO1
1Kangwon National University, 2Korea Institute of Geoscience and Mineral Resources, 3Oceanic C&T
Marine heat flow observations play an important role in enhancing our understanding various oceanographic and geological phenomena, such as ocean warming, focused flow in sediments, natural resources, and tectonics. These observations provide information on the geothermal gradient and thermal properties of sediments. Since the 1960s, when marine heat flow observations were first used as evidence for plate tectonics, observations have been conducted in the oceans for various disciplines and objectives. However, the known distribution of marine heat flow remains regionally skewed, given the limitations in the shipboard equipment, accessibility of study areas, and research objectives. In the Ulleung Basin of the East Sea (Sea of Japan), only the findings of foreign researchers prior to 1994 were accessible, until Korean researchers conducted their investigations in 2007 as a part of their gas hydrate development efforts. Despite the inclusion of the 2007 observations, the number and distribution of marine heat flow in the Ulleung basin were still insufficient in representing the entire region. Furthermore, observations made by the Korean researchers in 2007 highlighted the necessity of verifying the reliability of marine geothermal observations predating 1994. In 2022 and 2023, new marine heat flow observations were recorded in the deep Ulleung Basin using the R/V Tamhae 2. These observations can potentially expand the coverage of our observations and provide evidence for the reliability of pre-1994 data. In this presentation, we present the preliminary findings of the newly-acquired geothermal gradients and outline our plans for future research.
SE15-A009
Late Quaternary Slip Rate Along the North Longshou Shan Fault in the Southern Alashan Block
Shiqi WEI#+, Wenjun ZHENG, Fuer YANG, Jinquan MO
Sun Yat-sen University
The collision of the Indian and Eurasian plates during the Cenozoic resulted in the formation and uplift of the Tibetan Plateau in stages. Along the northeastern margin of the Tibetan Plateau, forming a northwest-southeast-trending basin-mountain tectonic geomorphic pattern consists of the Qilian Shan, the Hexi Corridor, and the low mountainous areas on the southern margin of the Alashan block. The North Longshou Shan fault, located on the southern margin of the Alashan block, is the boundary fault separating Longshou Shan from Chaoshui Basin. It strikes northwest-southeast with a length of ~110 km and dips to the southwest at angles of 50-70°. A detailed study was conducted in Yindunzigou and Er’daogou to constrain the late Quaternary slip rate of the fault, as well-preserved terraces were clearly offset in both sites. Topographic data were measured using an unmanned aerial vehicle photogrammetry system, while cosmogenic nuclide dating samples were collected to determine the time of terrace formation. Six terraces (T0-T5) were identified in Yindunzigou based on their height above the present riverbed. The fault scarp heights of T1, T2, T3, T4, and T5 are 2.32±0.40 m, 3.15±0.73 m, 7.50±0.85 m, 12.53±1.64 m, and 16.62±2.52 m, respectively. A sample collected from T3 yielded an age of 38.87±0.55 ka. Therefore, an average vertical slip rate of 0.19±0.03 mm/yr was obtained for T3. In Er’daogou site, terraces T1, T2, T3, and T4 were vertically offset by 0.24±0.11 m, 1.59±0.38 m, 6.47±1.37 m, and 12.59±2.12m, respectively. Two samples collected from T3 and T4 constrained their formation ages at 26.02±0.56 ka and 37.18±0.79 ka, and the average vertical slip rate was calculated at 0.29±0.05 mm/yr. The results show that the average vertical slip rate of the North Longshou Shan fault ranges between 0.19 mm/yr and 0.29 mm/yr since the late Quaternary.
SE15-A001
Present-day Crust Movement on Borderland Between China and Myanmar: Insight from GNSS Observations
Guojie MENG#+
Institute of Earthquake Forecasting, China Earthquake Administration
The borderland between China and Myanmar lies in the junction zone among the eastern edge of the Myanmar arc, the southeast edge of the Qinghai Tibet Plateau and the Sunda plate. To investigate the crustal deformation and its tectonics of the borderland, we have processed the data of regional GNSS networks from 1998 to 2020 around the region. The multi-scale spherical wavelet algorithm is employed to estimate regional strain rate field for investigating the crust deformation and earthquake risk. The results show that the strong compression and subduction of the Indian plate towards the east side of the Myanmar block resulted in the GPS station on the Myanmar arc moving towards the Qinghai Tibet Plateau in NNE direction with the Indian plate at a speed of about 30mm/a. The shear strain accumulation in the Myanmar arc area is obvious. The main compressive stress of the Myanmar arc is nearly east-west compression with a vertical tectonic trend at the outer side of the arc, and nearly south-north compression with a parallel structure at the inner side of the arc and the Irrawaddy River basin. The Sagaing fault is located in the high value area of the principal strain rate and shear strain rate, and there is subsection activity. The velocity of the two sides of the northern segment is obviously different, and the shear strain accumulates significantly, showing dextral shear movement and shortening. The middle segment of the Sagaing fault moves towards NNW at a speed of about 20mm/a, which is characterized by dextral strike slip and extension. The joint action of Eurasian plate and Indian plate makes the Sichuan Yunnan block revolve clockwise around the eastern Himalayan tectonic belt, the GPS speed deflects from west to east and from north to south to southeast and south, the speed gradually decreases to southeast, and it is distributed in the southwest of Yunnan in a dispersive manner. The Xiaojiang fault zone is generally sinistral strike slip. The middle segment of the Red River fault has a low strike slip rate, while the north and south segments have a high shear rate. The Dayingjiang fault in southwestern Yunnan shows the characteristics of east-west extension and obvious sinistral strike slip trend. The Longling-Ruili fault is characterized by dextral strike slip and extension. The NE trending Nantinghe fault, Menglian fault and Jinghong-Daluo fault are in a low shear state, dominated by left lateral strike slip. The northwest southeast trending Lancang fault and Wuliangshan fault are characterized by dextral strike slip, while the northwest trending Longling-Lancang fault zone is characterized by dextral strike slip and tension. The magnitude of strain rate accumulation is related to seismic activity. The future seismic risk of Shijun fault, Wanding fault, Nantinghe fault and the middle part of Wuliangshan fault in the high strain rate area deserves attention. The results of this study are of great significance for earthquake disaster assessment and understanding of the tectonic dynamic characteristics of the borderland between China and Myanmar.
SE15-A014
Hydro-mechanical Modeling on the Deformation of Mobile Shales: Insights Into Shear Dilation Effects on the Anomalous Uplift at Zhong Liao Tunnel, Taiwan
Eh TAN1#+, Jia-Xun LIN2, Wei-Hau WANG3
1Academia Sinica, 2National Central University, 3National Chung Cheng University
Mobile shales can deform ductilly or brittlely under a wide range of conditions. Mobile shales are dynamic and potentially hazardous geological features, but understanding their behavior can lead to safer environments, improved natural resource exploration, and a deeper understanding of Earth's geological processes. The northern exit of Zhong Liao Tunnel on Highway 3 has experienced anomalous uplift since its construction. Between 2000 and 2016, this region had risen by 130 cm while undergoing shortening by 90 cm, a rate that cannot be solely attributed to pure tectonic movement. Drilling records within this area have revealed the presence of high excess fluid pressure layers in the Gutingkeng mudstone formation. This region provides a good test ground to understand the deformation behavior of mobile shales. To model the deformation of mobile shales containing over-pressured fluids, we employed a 2D hydro-visco-elasto-plastic numerical geodynamic model. Furthermore, we incorporated strain-rate- and fracture-dependent porosity into the model, introducing shear dilation and drastically weakening at high strain rate areas. This effect produces a larger uplift velocity and reduces the spacing between the two faults, bringing the model results closer to observed field data.
SE15-A018
Cross-fault Deformation During and Following the 2022 Guanshan-Chihshang Earthquakes in the Central Longitudinal Valley Area, Eastern Taiwan
Yu WANG1,2#+, Sheng-Han WU1, Hoi Ling Birde CHOU1, Yi-Yu LI1, Wai San CHENG1, Andrew HO1, Jian-Ming CHEN1, Sze-Chieh LIU3, Chia-Yun HSIEH1, Siang DUAN1, Saw MYAT MIN1, Ei Mhone Nathar MYO1, Yuan-Lu TSAI4, Nai-Wun LIANG1, Jhih-Hao LIAO1, Tsz Yau Amundsen LAM1, En-Wei CHANG1, J. Bruce H. SHYU1
1National Taiwan University, 2Nanyang Technological University, 3Academia Sinica, 4CPC Corporation
We documented the co-seismic surface rupture and its cross-fault deformation associated with the Mw 6.4 and 6.8 Guanshan-Chihshang earthquakes on 17 and 18 September 2022 along the Yuli fault within the central part of the Longitudinal Valley in eastern Taiwan. Our result suggests the co-seismic rupture of 2022 roughly matches the locations of surface ruptures of 1951 around the Yuli town area, with a similar amount of cross-fault left-lateral displacement between the 1951 and the 2022 earthquakes. South of the Yuli, the maximum left-lateral displacement recorded across the rupture can reach 1.4 meters, with the fault scarp resembling a high-angle west-dipping fault geometry. The co-seismic surface ruptures were accompanied by significant post-seismic shallow after-slip at least during the first 3 months after the earthquake. The amount of cross-fault after-slip is close to, or even higher than the co-seismic cross-fault displacement, consistent with local witness accounts and post-event field photos which showed continuous damage and displacement of building floors and roads after the earthquake. Such shallow post-seismic slips were also observed along the main fault trace in the 2014 South Napa earthquake, and likely represent the shallow elastoplastic behavior of the sub-vertical fault in the young alluvial sediments.
Session Chair(s): Bo WANG, Nanjing University, Shengsi SUN, Northwest University
SE06-A008
| Invited
Central China Orogenic Belt and Amalgamation of East Asian Continents
Yunpeng DONG1,2#+
1Northwest University, 2Western University
The Central China Orogenic Belt (CCOB) comprises, from the east to the west, the Tongbai-Dabie, Qinling, Qilian and Kunlun Orogens, and preserves abundant and important amalgamation records of the North China, South China, Qaidam, Tarim and Qiangtang Blocks. The CCOB offers an excellent window to the tectonic evolution from Proto-Tethys to Paleo-Tethys domains and the formation of East Asian continent. In this Centennial Review of Gondwana Research, we assemble comprehensive and multidisciplinary information of geological, geochemical, geophysical and high-precision geochronological data set from individual orogens of the CCOB, together with a synthesis of Paleomagnetic data, to gain insights on the tectonic framework and evolutionary history of CCOB. The detailed and highly-integrated analysis leads to the following major conclusions. (1) Prior to ca. 550 Ma, break-up of the Rodinia supercontinent led to the formation of Proto-Tethys Ocean, wherein the above crustal blocks were isolated discrete units. (2) During ca. 541–485 Ma, spreading of all the embranchments of the Proto-Tethys Ocean at the early stage and the onset of subduction at the late stage. (3) Up to ca. 485–444 Ma, continued subduction of the Proto-Tethys Oceans resulted in opening and closing of the back-arc basin in the Qinling area. (4) During ca. 444–420 Ma, the Proto-Tethys Oceans along the Qilian and Shangdan were closing. (5) During ca. 420–300 Ma, the Paleo-Tethys Ocean in the Kunlun area inherited the Proto-Tethys Ocean, while the Paleo-Tethyan Mianlue Ocean experienced spreading. (6) At ca. 300–250 Ma, subduction retreat of the Kunlun Ocean occurred from the Aqikekulehu-Kunzhong suture to the Muztagh-Buqingshan-Anemaqen suture. (7) The Paleo-Tethys Ocean underwent eastward diachronous closing processes throughout the Kunlun to Qinling and Dabie areas during ca. 250–200 Ma; (8) The entire CCOB range has evolved into intracontinental deformation since 200 Ma.
SE06-A012
Sedimentary and Provenance Constraints on Carboniferous Multiple-stage Paleogeographic and Tectonic Transitions in the East Kunlun-Qaidam
Yukun QI+, Jiaopeng SUN#
Northwest University
The Carboniferous tectonic processes of the East Kunlun-Qaidam region located at the present-day northern Tibetan Plateau are of a great significance for understanding the geologic evolution of the Paleo-Tethyan Ocean. There is a debate concerning Carboniferous source-to-sink relation and topographic background of the East Kunlun-Qaidam. Some previous studies proposed that the East Kunlun-Qaidam was in a passive continental margin that tilted southward to the South Kunlun Ocean related to the oceanic crust spreading. In contrast, others indicate that, the East Kunlun-Qaidam was positioned in the north-dipping back-arc region inboard the East Kunlun magmatic arc. To resolve this debate, we investigated the well-exposed Carboniferous sedimentary successions in the Qimantagh, Dulan, and the northern Qaidam. A set of new provenance data were obtained, including paleocurrents, sandstone composition, and zircon U-Pb geochronology. These results show that the main peaks of detrital zircon ages are concentrated at ca. 350–250 Ma. The existence of Carboniferous-age detrital zircons, in combination with northward-directed paleocurrents, constrains magmatic activity of the East Kunlun magmatic arc during this period and further implies the subduction of the South Kunlun Ocean lithosphere, and suggest that East Kunlun-Qaidam was a northward-tilting back-arc extension basin during the Carboniferous. The sources mainly came from the south, and the Paleo-Tethys South Kunlun Ocean was in the subduction stage at that period. The obvious spatial differences in the provenance of the Carboniferous reflect complicated source-sink systems that existed in this paleogeographic pattern. Furthermore, percentage of zircons with Precambrian ages significantly varies through time, indicating changing in provenances along with a rapid uplift and exhumation of the basement. The dominance of detrital zircons with ages of ca. 2500–1700 Ma suggests additional sediment dispersal from the basement of East Kunlun and Qaidam, as well as the remnants of the Northern Qaidam Orogenic Belt during the early stage.
SE06-A009
Detrital Zircon Dataset from the Qilian-Qaidam-Kunlun Collage, Northern Tibet and It’s Tectonic Implications
Weidong HE#+
Northwest University
In the past decades, detrital zircon geochronology has been most widely used in sediment provenance research and basin analysis. In our research, we present a brief introduction to the procedure, methods, and results of the collection and summarization of an updated detrital zircon U-Pb geochronology database for the Qilian-Qaidam-Kunlun collage in northern Tibet. A total of 620 samples with 59830 lines of raw data were compiled, including 70 samples with in-situ detrital zircon Lu-Hf isotopes. Samples from 7 different geologic sub-units are briefly categorized and primarily discussed to highlight characteristic age spans, probability density distributions, major peaks, and εHf(t) values for sediments with different depositional ages. Its detailed raw data will be periodically accessible in the Deep-Time Digital Earth repository. Traditional data processing and visualization techniques might readily ignore internal variations in possible source regions with the accumulation of detrital zircon age data. This study further synthesizes these metadata collections using the Kolmogorov-Smirnov (K-S) test and multidimensional scaling (MDS) statistical analysis. Combined with the detrital zircon age facies for discriminating and comparing multiple samples, we hope to provide new constraints on the provenance analyses, crustal evolution, tectonic history, and supercontinent reconstructions of the Qilian-Qaidam-Kunlun collage, the northern part of the Qinghai-Tibet Plateau.
SE06-A017
Research on Detrital Zircons Chronology from the Ordovician to Devonian Strata of the South Qinling: Implication for Shangdan Ocean Closure
Fenhong LUO+, Hujun GONG#
Northwest University
The Shangdan Ocean represents an important part of the collision and convergence of the North China and Yangtze plates, and there is great controversy about the age of the two blocks' convergence. Through detailed CL images, trace elements, and U-Pb dating of the detrital zircons of the Ordovician-Devonian clastic rock strata in the South Qinling belt, this study aims to clarify the provenance areas of different ages and the changes of the tectonic environment, hoping to provide valuable information for the early Paleozoic tectonic evolution process of the Qinling Orogenic Belt. According to the U-Pb chronology of detrital zircons, the detrital zircons of the Devonian and Silurian samples show two main age ranges of 430-450 Ma and 710-840 Ma, and the Ordovician samples take 710-850 Ma as the primary age range, lacking the age of ~440 Ma. Compared with the zircon age spectrum in the surrounding terranes, 430-450 Ma is mainly the provenance of the North Qinling Belt, and 710-840 Ma is the provenance of the Yangtze Block and the South Qinling Belt. By zircon trace elements and age spectrum comparison combined with DZmix simulation, the provenance of the Devonian and Silurian samples has the characteristics of bidirectional source provenance from the North Qinling, the South Qinling, and the Yangtze Block. In contrast, the provenance of the Ordovician samples has the characteristics of unidirectional source provenance from the South Qinling and the Yangtze Block in the south, obviously lacking the origin of the north. It indicates that the provenance of the South Qinling has changed significantly during the Ordovician-Silurian. Based on the regional geology and previous research results, we believe that the Shangdan Ocean has closed, and the collision between the North Qinling Belt and Yangtze Blocks during the Ordovician-Silurian.
SE06-A001
Tectonic Attributes and Continental Affinities of the Precambrian Blocks in the Southwestern Central Asian Orogenic Belt
Bo WANG#+
Nanjing University
Numerous ribbon-like micro-plates develop in the southwestern part of the Central Asian Orogenic Belt (CAOB), they are important constituents of the Kazakhstan microcontinent, understanding of their tectonic attributes, continental affinities and crustal evolution is essential for the reconstruction of the accretionary history and geodynamic processes of the CAOB. The controversies remain for a long time about the basement compositions, tectonic settings and affinities of the micro-plates. This paper compiles recently published geological and isotopic chronological data, and summarizes rock assemblages, ages and tectonic settings of the Precambrian basement, and further analyzes the tectonic attributes of the micro-plates and their possible affinities with the surrounding continental plates. The available data indicate that the Meso- and Paleoproterozoic crystalline basement only develop in a few micro-plates (such as Chinese Central Tianshan, Kyrgyz Middle Tianshan, Issyk-Kul, Zheltau and Kokchetav), but are not recorded in the other micro-plates (such as South Yili, North Yili-Aktau, Chu-Ili, Karatau, Baikonur, Erementau and Ulutau) in the SW CAOB. However, similar Neoproterozoic metamorphic and magmatic rocks were documented in all these micro-plates and form the comparable metamorphic and crystalline basement. A comprehensive comparison and analysis allow us to conclude that these micro-plates may have different origins, but they experienced similar tectonic and magmatic evolution since Neoproterozoic, and underwent comparable paleogeographic environment, suggesting Early Neoproterozoic convergent orogenesis, Late Neoproterozoic continental rifting and formation of passive continental margins during the opening of the Paleo-Asian Ocean.
SE06-A010
The Lithosphere Structure of the Junggar Basin, NW China: Evidence for Its Origin of a Fossil Oceanic Lithosphere
Yingjie YANG1#+, Shucheng WU2, Yixian XU3, Juan Carlos AFONSO4, Anqi ZHANG1
1Southern University of Science and Technology, 2China University of Geosciences (Wuhan), 3Zhejiang University, 4University of Twente
The recycling of oceanic lithosphere into the deep mantle at subduction zones is one of the most fundamental geodynamic processes on Earth. During the closure of an ocean, ancient oceanic slabs are thought to be consumed entirely in subduction zones due to their negative buoyancy. Yet, it is recently suggested that small pieces of oceanic slabs could be trapped along paleo-subduction zones. What remains far more enigmatic is whether significant portions of paleo-oceanic lithosphere could eventually avoid the fate of subduction and be accreted to continental lithosphere, thus contributing to continental growth through time. We present seismic evidence for a preserved paleo-oceanic lithosphere beneath the Junggar region in northwestern China. We show that un-subducted oceanic lithosphere in the West Junggar has been preserved beneath the Junggar Basin, becoming a piece of the Eurasian continent. This scenario is likely to have occurred in other continents throughout Earth’s history, providing an additional and commonly underestimated contribution to the growth of continental lithosphere.
Session Chair(s): Bo HUI, Northwest University
SE06-A015
| Invited
Assessing Models for Neoproterozoic—Early Paleozoic Paleogeographic Configurations of Gondwana
Ryan MCKENZIE1#+, Cody COLLEPS2, Adam NORDSVAN1, Paul MYROW3, Nigel HUGHES4
1The University of Hong Kong, 2University of Potsdam, 3Colorado College, 4University of California, Riverside
Numerous disparate models exist for the pre-Pangean amalgamation and configuration of Gondwana, particularly for the various continental blocks that make up modern Asia. In this contribution we critically evaluate new and published provenance and paleobiogeographic data that span the late Neoproterozoic—Early Paleozoic geologic record. Specifically, we statistically assess extensive stratigraphically resolved detrital zircon age data in conjunction with geologic and paleontological records from the major constituents of northcentral-to-northeastern Gondwana to test existing models for paleogeographic configurations. Our time-series comparisons provide insights into the amalgamation history of various Asian terranes at the geologic period level and help to resolve the marginal relationships between these terranes in East Gondwana.
SE06-A005
Early Neoproterozoic Subduction-related Tectonics Along the Northwestern Margin of the Yangtze Block, South China
Bo HUI#+
Northwest University
The early Neoproterozoic granitoids exposed in the Bikou Terrane preserve vital information for understanding the Tonian tectonic evolution along the northwestern margin of the Yangtze Block, South China. However, their accurate forming age, petrogenesis, and tectonic attributes remain ambiguous. This study reports new results on zircon U–Pb geochronology, zircon Hf isotopes, whole-rock geochemistry, and Sr–Nd isotopes of the four granitoid plutons from the Bikou Terrane. Detailed zircon U–Pb dating results reveal that the quartz monzonite and monzogranite were formed at ca. 860 Ma, whereas the granodiorite was emplaced at ca. 825 Ma. The quartz monzonite and monzogranite samples exhibit consistent isotopic compositions, indicating that they shared the same magma source, whereas the monzogranite was formed by differentiation crystallization of primitive quartz monzonite melt. The quartz monzonite samples are calc-alkaline in composition and have high ratios of Sr/Y and (La/Yb)N, coinciding well with the adakitic rocks. The positive values of εHf(t) (+4.8–+6.7) and εNd(t) (+1.7–+2.1) indicate that they were formed by the interaction between slab-derived melt and mantle wedge. This mechanism may be triggered by a slab roll- back process in an arc-related setting. The Maliupu granodiorite samples are classified as calc-alkaline I-type granitoids. They are featured by highly evolved εHf(t) values from −15.0 to −10.9 and εNd(t) values from −11.8 to −11.9, with Hf and Nd model ages ranging between 2.63 and 2.20 Ga, implying they were derived from partial melting of the ancient lower mafic crust and were formed in a subduction-related setting. Therefore, the new data, combined with previous studies, provide an essential link in the evidence chain for the hypothesis that the northwestern periphery of the Yangtze Block was in a persistent subduction-related tectonic regime in the early Neoproterozoic.
SE06-A014
Late Carboniferous to Permian Paleoclimatic and Tectono-sedimentary Evolution of the Central Ordos Basin, Western North China Craton
Hua TAO#+
Northwest University
The paleogeographic and tectonic environments of the North China Craton experienced dramatic transitions throughout the end-Carboniferous to Permian during the protracted subduction-collision orogenesis along the southern Paleo-Asian Ocean. The resultant topographic growth within the Andean-Type continental arc significantly triggered climatic shift. To depict relations between topographic variation of the continental arc and depositional environment changes of the sink, we conducted a synthesized work incorporating petrology, geochemistry, and geochronology on Carboniferous and Permian strata in the central Ordos Basin, western North China Craton. The geochemical data of 36 mudstones show that the paleosalinity gradually decreased, reflecting the environmental transition from marine to continental environments. The U-Pb dating results of 563 detrital zircon yield three distinct age ranges: 260–470 Ma (29%), 1700–2100 Ma (40%), and 2200–2600 Ma (25%). The ca. 260–470 Ma are the age characteristics of Cambrian to Triassic subduction-related magmatic rocks in the Andean-type continental margin. The ca. 1700–2100 Ma and ca. 2200–2600 Ma aged detrital zircons compare well with age distributions for basement rocks of North China Craton. Further correlations imply that the Carboniferous-Permian sediments in the central Ordos were sourced from the Andean-type continental arc stretching across the northern North China Craton, which is directly related to the southward subduction of the Solonker Ocean as the southern branch of the Paleo-Asian Ocean. In addition, there is an obvious crustal thickening event that led to provenance uplift in continental arc at the end of the Permian, indicated by increasing number of zircons with ages close to the deposition age of the host sediments in the Shiqianfeng Formation. This tectonic event was coeval with climatic transition from humid to arid since accumulation of the Shiqianfeng Formation, expressed by evolving depositional environment from coal-bearing tidal flat via deltaic, to red-color seasonal lake.
SE06-A007
Foreland Basin Development in Response to Proto-Tethyan Ocean Closure, Western North China Block
Jiaopeng SUN1#+, Yunpeng DONG1,2
1Northwest University, 2Western University
Closure timing of the northeastern Proto-Tethys between the Qilian/Qinling terranes and the North China Block remains unsolved, with assumptions ranging from end-Ordovician to the Devonian. To address this issue, integrated studies of stratigraphy and geochronology were conducted on Late Ordovician strata in the southwestern Ordos, which recorded earliest tectonic transition from passive margin to foreland basin in the westernmost North China Block. Stratigraphic and paleontologic syntheses demonstrate that pre-Katian strata are shallow-marine deposits dominated by benthonic faunas. While, Katian successions above a paraconformity are characterized by deep-water debrites and turbidites containing abundant planktonic graptolites. Provenance analysis reveals an evolving source from the North China Block basement to the Qilian/Qinling arc terranes at the beginning of Katian (ca. 450 Ma). Detrital zircons from pre-Katian quartz arenites yield ages of ca. 1600–2800 Ma, significantly older than their depositional timing. In contrast, Katian turbidites in the southwestern Ordos and the North Qilian Orogen display similar age patterns dominated by ca. 450–900 Ma ages. These clues imply a basin-filling shift from passive margin to underfilled foreland, separated by forebulge unconformity formation at Sandbian/Katian boundary. Stratigraphic correlation further suggests that sequence of foreland basin-infill transitions was broadly simultaneous along-strike over ~1200 km across the southwestern North China Block, including forebulge flexural uplift, followed by rapid shallow shelf drowning to abyssal plain, until arrival and superimposition of arc-derived turbidites. Along-strike synchronicity of orogenic activities implies that closure of the northeastern Proto-Tethys was nearly synchronous. The L-shaped orogen-parallel foreland encompassing the southwestern North China Block unveils oroclinal bending of the Qilian/Qinling collision belt, which still dominates geology of the present northeastern Tibet. Our new insights provide a stratigraphic constraint for the timing and mode of the initial elimination of northeastern Proto-Tethys.
SE06-A013
Early Cretaceous Volcanic Rocks in the Central Lhasa Suberrane, South Tibet: Insights Into Crustal Evolution and Crust-mantle Interaction
Yu HUANG1#+, Zhidan ZHAO2, Di-Cheng ZHU2
1Chang'an University, 2China University of Geosciences
The Lhasa Terrane in southern Tibet is widely recognized as having separated from the northern margin of Gondwana and undergoing a protracted and intricate evolution. Abundant Early Cretaceous volcanic rocks are present in the central Lhasa subterrane, Tibet, playing an essential role in models aimed at comprehending the tectonic-magmatic evolution and mantle-crust interaction of this terrane. In this study, we present a well-preserved section of Zenong Group volcano-sedimentary sequence in Eyang, Xainza area within the central Lhasa subterrane. Our new data combined with existing literature data indicate that there was an extensive period of magmatism (approximately 140 Ma to 102 Ma) throughout the Early Cretaceous in the central Lhasa subterrane, reaching its peak around 113 Ma with remarkable compositional diversity. The composition of Early Cretaceous volcanic rocks in the central Lhasa subterrane underwent a temporal transition from high-silica rhyolites to dacites and andesites, exhibiting a reverse cyclicity. Moreover, the intermediate rocks from the upper section display elevated whole rock εNd(t) and zircon εHf(t) values, as well as decreased 87Sr/86Sr ratios compared to the high-silica rocks from the lower section. These observations collectively suggest: (a) involvement of open-system processes encompassing mantle-derived magmas and ancient crustal-derived materials; (b) an increasing contribution of mantle sources in the magma genesis; (c) variable magma origins with distinct petrogenetic histories rather than a uniform source involving assimilation-fractional crystallization processes. We propose that the high-silica rhyolites in the lower section of the Xainza area (≥ ca. 120 Ma) are associated with slab roll-back, while the dacites and andesites in the upper section (≤ ca. 120 Ma) are linked to slab break-off during southward subduction of Bangong-Nujiang Ocean lithosphere. Furthermore, it is evident that the ancient basement of the central Lhasa subterrane underwent localized reworking by mantle-derived melts.
SE06-A011
Thermal Evolution of the Metamorphism in the Eastern Taiwan: Implications for Blueschist Exhumation
Yiqiong ZHANG1#+, Kamil USTASZEWSKI2
1China National Petroleum Corporation, China (CNPC), 2Friedrich-Schiller-Universität Jena
Taiwan is located along an active plate boundary between the Eurasian and Philippine Sea Plates, with convergence rates amounting to about 80 mm/yr. The island has since long served as a cradle for many tectonic concepts. The Yuli Belt in Taiwan’s eastern Central Range encloses high pressure (HP) mafic–ultramafic blocks in intensely deformed greenschist-facies metasediments. It is still debated how its structures relate to those of the westerly and easterly adjacent units. We integrated new and published Raman-spectroscopic measurements on carbonaceous matter from metasedimentary successions across the Tailuko and Yuli Belts and combined these results with new cross sections. Our results suggest temperature variations of up to 150°C within the Yuli Belt itself, with lower temperatures between 400 and c. 460°C within the metasediments and up to 550° in spotted schists directly underlying the HP metamafic assemblages. No temperature gradient can be found across the Shoufeng Fault separating the Yuli and Tailuko belts in the west. The most pronounced temperature gradient exists across a fault contact between the Yuli Belt and the easterly adjacent Chulai Fm. Both Chulai Fm. and Backbone Slates to the west of the Tailuko Belt exhibit T<400°C. In combination with lithological similarities, we consider the Chulai Fm. an easternmost extension of the Backbone Slates. We suggest that the Yuli Belt was initially emplaced on top of lower-grade Paleogene successions. Later, the nappe succession was overprinted by E-vergent backfolding of the Central Range and contemporaneous backthrusting along the Shoufeng Fault, leading to the presently observed synformal structure of the Yuli Belt.
Session Chair(s): Po-Fei CHEN, National Central University
SE09-A001
Anisotropic Structure of the Upper Mantle in the South China Sea and Its Implications
Mei XUE1#+, Lin LI1, Ting YANG2, Chenguang LIU3
1Tongji University, 2Southern University of Science and Technology, 3Ministry of Natural Resources
The South China Sea (SCS) is located at the intersection of the Eurasian, Pacific, and India-Australia plates. Many models have been proposed for the opening of the SCS. This study aims to constrain these models through the anisotropic structure of the central basin of the SCS and its surroundings. Based on the seismic data recorded by ten ocean bottom seismometers recovered from two passive seismic experiments conducted by Tongji University in the central basin of the SCS in 2012 and 2014, three different shear wave splitting methods are used to obtain the XKS splitting results of the central basin for two global earthquakes and the S phase splitting results provided by 20 regional earthquakes surrounding the SCS. The SKS splitting results demonstrate the presence of strong anisotropy with the NE fast direction in the central basin of the SCS, which may be related to mantle flow along the ocean ridge during seafloor expansion and the mantle flow dragged by the subduction of the proto SCS plate. Strong anisotropy is also observed in the upper mantle surrounding SCS and the obtained fast directions vary with azimuths and are consistent with previous SKS-splitting results, GPS, and plate motions, and importantly correspond well to the regional tectonics or mantle convection models. The anisotropic results are consistent with the expected results of the extrusion model driven by the collision of the Indian Eurasian plate and the slab pull of proto-SCS. The anisotropy results are inconsistent with the ideal upwelling driving model of the mantle plume. Unfortunately, due to the limited splitting observations in the central basin, the anisotropic results cannot confirm or falsify the "Atlantic-type" seafloor spreading model, the backarc spreading model, and the plate-edge rifting model.
SE09-A003
Estimating Crustal Thickness in the Northern Philippines Through Ambient Noise Autocorrelation
Emi ULFIANA1,2+, Po-Fei CHEN2#, Bor-Shouh HUANG1, Nghia Cong NGUYEN1,2, Teresito BACOLCOL3
1Academia Sinica, 2National Central University, 3Philippine Institute of Volcanology and Seismology
The Philippine Mobile Belt comprises accreted terranes composed of ophiolites, island arcs, and continental fragments. It absorbs the approximately 9 cm/year convergence between the Sundaland Plate to the west and the Philippine Sea Plate to the east. Understanding the crustal thickness variations across the Philippines is crucial for distinguishing collision boundaries and comprehending the complexities of tectonic evolutions. In this study, we conducted ambient noise autocorrelation to extract coherent signals of PmP using five stations in northern Luzon (A) and five stations in NW Mindoro (B). Prior to autocorrelation, temporal normalization and spectral whitening were applied, followed by phase-weighted stacking. The resulting two-way travel times range between 7.7 and 10.3 seconds for (A) and 8.7 and 13.1 seconds for (B). These times correspond to crustal thicknesses of 27.4 to 39.7 kilometers and 31.9 to 52.9 kilometers, respectively, as derived from the 3D local P-wave velocity model. Our main findings and preliminary interpretations indicate that the crust beneath Luzon is thicker in the western regions compared to the eastern parts. This suggests a limited influence of magmatic processes in the latter. Moreover, our observations reveal that the crust beneath Mindoro becomes thicker in proximity to the Palawan Continental Block and thinner toward the extension of the Pleistocene Macolod Corridor rifting. Overall, our results align comparably with findings derived from gravity data.
SE09-A007
3D Shear Wave Velocity Structures Beneath Marapi Volcano, Western Sumatra by Ambient Noise Tomography
Fanda FITRIANDITHA1+, Po-Fei CHEN1#, Abraham ARIMUKO2, Daryono DARYONO2
1National Central University, 2Indonesian Agency for Meteorology, Climatology and Geophysics
Indonesia The approximately 60 mm/yr oblique convergence of the Indo-Australian and Sundaland plates along the Sunda Trench has been divided into trench-normal and trench-parallel components. The Sumatra Arc exhibits magmatic activity in the subduction zone driven by the former, while the Great Sumatra Fault (GSF), both located in western Sumatra, is a sinistral strike-slip fault accommodating those of the latter. Among these features, Marapi Volcano is the most active, having recently erupted on December 3rd, 2023. Understanding the potential interaction of the magma chamber beneath Marapi with the GSF is intriguing and crucial for hazard mitigation. This study employs ambient noise tomography (ANT) to investigate the 3D shear wave velocity structures beneath Marapi Volcano. The ANT process involves cross-correlation of continuous recordings between pairs of stations, followed by stacking to extract the Empirical Green’s Function (EGF) representing the inter-station media. Data from 26 mini-broadband stations, managed by BMKG (Indonesian Agency for Meteorology, Climatology, and Geophysics) and centered around the Marapi volcano, were employed for analysis. The Phase Weighted Stack (PWS) technique was adopted to enhance signals with coherent phases. The derived EGF was then analyzed for dispersion curve using Frequency Time Analysis (FTAN). Subsequently, a tomographic scheme was employed to perform the inversion for the 3D shear wave velocity structures that best fit the observed dispersion data. Given the dense distribution of stations, we expect the results to offer high resolution, allowing for a better understanding of the crust and upper mantle beneath the Marapi Volcano.
SE09-A005
Ground Motion Prediction Equation in the Lombok Region Using Machine Learning
Edy SANTOSO#+
Indonesian Agency for Meteorology, Climatology and Geophysics
The paper examines the strengths and weaknesses of various machine learning methods in forecasting ground-motion intensity measures based on source characteristics, source-to-site distance, and local site conditions. Traditionally, linear regression models with preset equations and coefficients are utilized for this purpose, but their limitations in capturing intricate nonlinear patterns in data can be restrictive. Hence, this study comparatively explores the potential advantages of alternative machine learning techniques such as Linear Regression, Random Forest, and XGBoost as statistical methods for ground motion prediction. The research assesses the variability of ground motions from event to event and site to site by incorporating them as random effect terms to minimize uncertainty. These algorithms are trained using a specific database containing 588 ground motions, recorded from 242 seismic events ranging from magnitude 1.5 to 6.9, within distances of 0–50 km from Lombok Island and its surrounding areas between 2007 and 2023.The findings demonstrate that both Random Forest and XGBoost consistently outperform Linear Regression across three evaluation metrics Mean Squared Error (MSE), Root Mean Squared Error (RMSE), and R-squared (R2). Moreover, the evaluation results indicate that these algorithms exhibit desirable characteristics such as magnitude scaling and distance dependency without relying on pre-established equations or coefficients.
SE09-A002
Seismotectonics of Sulawesi, Indonesia
Yopi SERHALAWAN1,2+, Po-Fei CHEN1#
1National Central University, 2Indonesian Agency for Meteorology, Climatology and Geophysics
Sulawesi Island, located in eastern Indonesia, lies at the triple junction of the Australian, Sunda, and Philippine Sea plates. It exhibits a distinctive K-shape, with each arm having undergone independent geological evolution. Driven by the latest Miocene collision (~5 Ma) between the Banggai-Sula microcontinent and the East Arm, the deformation is accommodated by the corresponding motion of individual blocks at various locations, resulting in specific patterns of seismic moment release. In this study, we investigate the distributions of shallow earthquakes (< 60 km) based on the ISC-EHB and BMKG catalogs, as well as the focal mechanisms based on the GCMT catalog, to study the seismotectonics of Sulawesi. The results are grouped into five regions with characteristic seismic patterns well corresponding to tectonic signatures and geodetic observations. The main findings can be summarized in two parts. First, thrust earthquakes release seismic energy due to oceanic plate subduction, including, in order of moment release, those along the North Sulawesi Trench to the north, the Makassar Strait Thrust to the west, and the Tolo and Buton Thrust to the southeast. Notably, there is a seismic gap near the center of the North Arm that may indicate potential risk for damaging earthquakes, while those of the Batui Thrust are only minor. The second part involves left-lateral strike-slip motions along the Central Sulawesi Fault System. The occurrence of the 2018 Mw 7.6 Palu earthquake not only filled the gap of seismic deficiency on the Palu-Koro fault but also activated overall seismic activity in Sulawesi. Additionally, note the low seismicity on the segment offshore northwest Sulawesi, which may be beyond the high relative motion between the Makassar and North Sula Block.
SE09-A009
The Disparities in Thickness Between the Thermal and Seismic Lithosphere Beneath the Global Precambrian Cratons and Its Geodynamic Implications
Chaoqiang CHEN#+, Lijuan HE
Chinese Academy of Sciences
Cratons play an important role in the evolution of Earth and usually exhibit extremely thick and strong lithosphere roots and low surface heat flow. Most cratons remain in a stable state throughout their long evolutionary process. However, the stability of a few cratons was lost, the thickness of the lithosphere was greatly reduced, and surface heat flow greatly increased. Significant thinning of the lithosphere is one of the most obvious features of craton destruction. However, even within the same area, the lithospheric thickness values estimated from different methods can vary a lot. The thickness disparities between the thermal and seismic lithosphere remain unclear. On the basis of the latest global heat flow data and crustal stratification information, we calculated the thickness of the thermal lithosphere of cratons globally and conducted a detailed comparison to that of the seismic lithosphere. We found that 1) the thickness of the thermal lithosphere of most cratons is more than 150 km, while that of the Bundelkhand, Singhbhum, and upper Yangtze craton ranges from approximately 120-150 km. The thickness of the eastern North China craton, lower Yangtze craton and Wyoming craton ranges from only approximately 80-100 km. 2) For most cratons, the thickness of the seismic lithosphere is tens of kilometers (30-141 km) larger than that of the thermal lithosphere, except for the Wyoming craton, eastern North China craton, upper Yangtze craton, and Dahawar craton. 3) The part between the bottom boundaries of the seismic and thermal lithosphere can be considered as the rheological boundary layer (RBL), which is related to the craton stability. The thicker the RBL is, the higher the craton stability. 4) Due to plate subduction, the water content in the upper mantle is high, the viscosity is low, and the thickness of the RBL of cratons is small.
SE09-A008
Utilizing 2-D Waveform Modeling for Analyzing Dual First P Arrivals Beneath Northeastern Taiwan
Hung-Yu YEN1+, Po-Fei CHEN2#
1Academia Sinica, 2National Central University
The Formosa Array, a dense seismic array with around 140 stations, has been deployed in Northern Taiwan since 2017. With the high-density seismic network, previous studies have identified intriguing observations featuring distinct dual first P arrivals from deep earthquakes beneath NE Taiwan. In their research, the suggested mechanism for the delayed P arrival has been attributed to the energy scattered from the magma diapirs. However, validating their model solely through fitting arrival times with the ray-tracing method is not comprehensive. To explain the significant later P phase, we re-examine data from several deep earthquakes beneath NE Taiwan as recorded by the Formosa Array and validate our idea through 2-D waveform modeling. We set up a velocity structure with (A) a high Vp anomaly in the mantle wedge above Ryukyu subduction, and (B) a slightly high Vp Eurasian lithosphere to the west with a sub-vertical boundary – based on results of tomographic studies. In light of the simulations, we conclude that (1) the small-amplitude first P phase is attributed to the energies radiated near the nodal point of the focal mechanism and propagated through (A); (2) those of the significant later P phase are analogous to a strong head wave propagating along (B) to the surface. Accordingly, stations of zero delay time between the first and second P provide a first-ever portrayal of the Eurasian lithosphere boundary by waveform constraints.
Session Chair(s): Chung-Han CHAN, National Central University, Kazuyoshi NANJO, University of Shizuoka
SE04-A023
Slip Rate and Earthquake Potential of the Maidan Fault in Southwestern Tianshan Inferred from GPS and InSAR Observations
Xiaohang WANG+, Caijun XU#, Yangmao WEN, Guoyan JIANG
Wuhan University
The Maidan Fault (MDF), as an important piedmont fault of the Tianshan Mountains, plays an important role in regulating the strain due to the oblique subduction of the Tarim Basin beneath the Tianshan Mountains. However, due to lack of near-field geodetic data of surface deformation, current knowledges on the slip rate and seismic hazard of the MDF are limited. Here we used InSAR and GPS to monitor interseismic deformation of the MDF. Through integrating high-resolution InSAR velocity observations and published GPS velocities, we obtained high precision interseismic surface displacement rate maps. And it reveals that the MDF is a boundary fault dividing the Tarim Basin and the Tianshan Mountains. We further conducted geodetic inversions to infer the slip rates and interseismic coupling of the MDF based on the elastic block model. Our inversion results show that there are three asperities on the MDF. The western segment of the MDF is strongly locked, while the eastern segment is partially coupled. However, there are very few historical earthquakes occurred along the MDF, especially in the western segment. Therefore, the western segment of the MDF is possibly characterized with high seismic hazard.
SE04-A022
Reconstructing the Rupture Characteristics and the Associated Tsunami Dynamics for the Littoral Fault in the Northern South China Sea
Qiang QIU1#+, Linlin LI2, Zhigang LI2, Weitao WANG2
1SCSIO, Chinese Academy of Scienc, 2Sun Yat-sen University
Understanding earthquake rupture characteristics of a particular fault from previous events are crucial for future seismic and tsunami hazard assessments. However, due to lack of detailed information of geological structure and long-term geophysical and geodetical observation, these factors are poorly known. The Littoral Fault of the northern South China Sea runs parallelly along the southern coast of China, starting at Niushan Island to the east and, ending at Northern Bay area in Hainan Island to the west, ~1200 km in length. This fault is comparable in length with the Sumatran Fault in Indonesia and the San Andreas Fault in US, but the seismogenic behaviors of the fault is much less studied than those of the other two faults. Importantly, previous ruptures in the east and west segment of the fault remain a seismic gap which seats right in front of the populous cities i.e., Hong Kong, Macao in the Greater Bay Area. The gap has not ruptured by earthquakes with Mw>5 based on both the historical and modern seismological records. However, the high-resolution seismic data retrieved within the gap indicate that at least 7 events occurred previously with an averaging time interval of 5000 years. Here, we integrate this seismic structure data and earthquake-cycle modeling to reconstruct the rupture nucleation, propagation and healing process of the Greater Bay Area segment of the Littoral Fault. The constrained earthquake-cycle model will in turn provide earthquake rupture source models for tsunami modeling. Our results will provide new insights about future plausible rupture scenarios and tsunami dynamics for the seismic and tsunami hazard assessments and hazard mitigation strategies, and eventually contribute to the sustainable economic development of the Greater Bay Area.
SE04-A009
Seismicity Analysis in the Weiyuan-Rongxian Area, Sichuan Basin, China
Yanzhen LI+, Hongyi LI#
China University of Geosciences
The Weiyuan-Rongxian shale gas field in the Sichuan basin, China, has experienced numerous earthquakes in recent years, causing significant casualties and property loss. To investigate the spatial-temporal evolution of seismicity and seismic fault structures, in this study, we first utilize a deep-learning-based picking algorithm –(PhaseNet) to identify seismic phases from raw seismic data between March 2019 and October 2020, and then employ a Rapid Earthquake Association and Location technique (REAL) to associate these seismic picks. Finally, the VELEST and GrowClust methods are performed to build a high-precision earthquake catalog containing 18912 earthquakes. Our results reveal that the spatial-temporal distribution of earthquake swarms indicates a complex fault system. In the northern part of Weidong block (R1), the earthquakes illuminate a shovel-shaped structure that the dip angle of the fault plane gradually decreases with depth. In the south of Weidong block (R2), the natural fractures with dip angles of about 80° control the distribution pattern of earthquakes. In the Weixi block (R3), the Molin fault and basement fault form a typical structural wedge that bounds a triangular or wedge-shaped fault block. The majority of earthquakes located below the buried depth of the shale gas and spatio-temporal correlations between seismicity and industry operations both suggest that they are probably induced by hydraulic fracturing. The migration front of the earthquakes can be modeled by fluid diffusion with the diffusivity D between 0.2 m2/s and 3.5 m2/s. The Ms 5.2 earthquake occurring on 18 December 2019 is located in a positive ~10 kpa Coulomb failure stress area generated by the 8 September, 2019, Ms 5.4 earthquake, reaching the typical static triggering threshold. Therefore, in addition to fluid diffusion, the stress perturbation caused by previous seismic ruptures may be considered as another factor of earthquakes occurring in the Weiyuan-Rongxian.
SE04-A010
Investigation of the 2011 Yingjiang, Yunnan, China Ms 5.8 Earthquake Sequence: Seismic Migration, Seismogenic Mechanism, and Hazard Implication
Ke DU+, Hongyi LI#
China University of Geosciences
On March 10, 2011, an Ms 5.8 earthquake struck Yingjiang City, western Yunnan, China, causing significant damage and attracting widespread attention. Due to the sparse distribution of seismic stations and the complexity of the geological structure around the hypocenter, its seismogenic structure and mechanism remain controversial. In this study, with the aid of machine-learning-based detection and location workflow and template matching technique, we build a high-precision earthquake catalog containing 1791 earthquakes ranging from December 1, 2010, to April 30, 2011. Our result shows that the foreshocks initiated in an extensional stepover (stepover 1), and then bilaterally extended northeast and southwest, with migration fronts that can be simulated by fluid diffusion model with diffusivities of 0.8 m2/s and 0.19 m2/s, respectively. The mainshock occurred at the southwest end of the foreshocks, around the other stepover (stepover 2) connected the northeast and middle segments of the Dayingjiang fault and activated the northwest-trending fault near stepover 2, jointly forming a conjugate fault system with the northeast-trending faults. Additionally, we determine the full moment tensor solutions for eight earthquakes with relatively large magnitudes, among which the mainshock characterizes a significant volume compaction component and a shallow centroid depth of about 5 km. Furthermore, Coulomb failure stresses caused by five foreshocks on the mainshock fault plane is ~24 kPa, reaching the typical static triggering threshold. Therefore, we suggest that both the fluid diffusion and stress perturbation constitute an important factor in triggering the mainshock and the severe seismic damage during the moderate Yingjiang earthquake may be due to the combined effects of the sedimentary basin effect and shallow centroid depth. This study provides new insights into further understanding the spatiotemporal evolution, seismogenic mechanism, and hazard implication for the Yingjiang Ms 5.8 earthquake.
SE04-A013
The Seismic Activity of the Beijing Area Based on an Enhanced Long-term Earthquake Catalog
Huiying GE1+, Hongyi LI1#, Tongli WANG2
1China University of Geosciences, 2Beijing Earthquake Agency
The Beijing area is located in the northwestern edge of the North China Plain, bordered by the Taihang Mountains to the west and the Yanshan Mountain range to the north. The area is surrounded by several active faults, posing a certain seismic risk.In this study, we combined the graphics processing unit-based match and locate (GPU-M&L) and machine learning technique to study the seismicity in the Beijing area. Continuous waveform data recorded by 29 seismic stations from the China Earthquake Networks Center (CENC) from 2010 to 2020 were collected. Out of 3,405 earthquakes, 1,884 were selected as templates for GPU-M&L processing for earthquake detection. These were further refined by noise reduction using DeepDenoiser to select events with clear seismic phases, followed by phase picking with Phasenet and relocation using hypoDD. Repeating earthquakes were identified by segmented cross-correlation in time and frequency domains, and similar earthquake groups were clustered using GrowClust with cross-correlation values over 0.9.As result, we identified 7,516 seismic events, approximately 2.2 times the number listed in the CENC earthquake catalog. Of these, about 5000 events are relocated using the hypoDD. In Jiudaohe, earthquakes delineate a fault with an SW-NE-orientation on the surface, most activity at depths of 5-10km, becoming shallower and denser northwest. In Gaoliying, the distribution of earthquakes aligns along the Huangzhuang-Gaoliying fault strike at depths of 5-15 km, inclined towards the SE direction with a dip angle of 75-90◦. We obtained a slip rate of approximately 4.4 mm/yr at the seismogenic depths of Hangzhuang-Gaoliying Fault, and a slip rate of 0.4-1.5 mm/yr at a depth of 10.8 km in Jiudaohe. Our results offer a reliable and rich data foundation for the assessment of earthquake risks, contributing to the disaster prevention and mitigation efforts in the Beijing region.
SE04-A014
Rebuilding a High-precision Catalogue for the China Yangbi Earthquake Foreshock Sequence with GPU-M&L 2.0
Zeyu MA1+, Hongyi LI1#, Min LIU2
1China University of Geosciences, 2The Chinese University of Hong Kong
An MS 6.4 earthquake occurred on 21 May 2021 in Yangbi County, Yunnan Province, China, on the southeastern edge of the Tibetan Plateau. Several foreshocks larger than magnitude 4.0 occurred before the mainshock and it was followed by a rich aftershock sequence, making it a typical pre-main-post type earthquake sequence. The construction of a high-precision catalogue of foreshock sequences can help to understand the nucleation mechanism of earthquakes. Due to the controversies in the previous studies on the nucleation mechanism of the Yangbi earthquake, we reconstruct a high-precision seismic catalogue of the foreshock sequence using the newly developed GPU-based Match and Locate (GPU-M&L 2.0) technique, in combination with the LOC-FLOW seismic identification and location workflow. This catalogue provides a more accurate depiction of the distribution of the seismogenic faults and the spatio-temporal migration characteristics of the foreshocks. Our findings indicate that most sections of the faults in the region were activated during the foreshock stage, rather than through a gradual activation process with aftershocks. We divide the foreshock sequence into two stages based on the two major foreshocks. In the first stage, the foreshocks migrated mainly in a northwest direction, and in the second stage, the foreshocks migrated in a northwest and southeast bi-directional direction. The spatial development characteristics of the activation of the foreshock and the mainshock suggest that the Yangbi earthquake sequence is more consistent with a cascade model. We fit the spatio-temporal migration process of the early foreshock catalogue with an empirical formula for fluid transport. Several large foreshocks might have broken the seal of fluid reservoirs, then fluids interacted with the pre-existing fault zones which activated a fluid-driven earthquake sequence. Aided by fluid diffusion, the previously segmented fault zones were connected to form a longer fault zone, resulting in the 6.4 magnitude Yangbi earthquake.
SE04-A029
Subcriticality, Criticality, or Supercriticality: How Many "Daughters" Does Each Earthquake Have?
Jiawei LI#+
Southern University of Science and Technology
Seismicity can be conceptualized as branching processes, wherein background earthquakes (immigrants), assumed to be driven by the forces of plate tectonics, have the potential to trigger cohorts of earthquakes, referred to as first-generation “daughters.” These first-generation events, in turn, can act as “mothers” to trigger second-generation “daughters,” creating a cascading effect. In this dynamic process, a critical parameter known as the branching ratio n, the mean number of “daughters” triggered per “mother,” plays a pivotal role in reflecting the transition state of the crustal system. The transition point occurs at n = nc = 1, demarcating the subcritical regime (n < 1) from the supercritical regime (n > 1). However, all methods for estimating n based on a catalog generally neglect or incorrectly address two critical factors: 1) the finite-size effect (FSE) resulting from the selection of earthquake catalogs of limited duration and spatial extent, and 2) censorship resulting from the assumption of a minimum magnitude m0 above which earthquakes can trigger “daughters,” which has no reason to be equal to the catalog cutoff magnitude Mco. In this study, we propose a novel framework to correct the FSE and censorship from the apparent branching ratio napp to the true branching ratio ntrue, based on the ETAS model with a spatially varying background rate. The framework embeds a model to characterize napp as a function of Mco and stresses that scanning this function is also a way to identify or constrain the value of m0. By applying the earthquake catalog observed in California, New Zealand, and China to our analysis framework, we demonstrate that seismicity operates close to the critical point nc. The criticality of seismicity has significant implications on our understanding of seismicity patterns, on the forecastability of aftershocks and for earthquake hazard mitigation and risk management.
SE04-A024
Identifying the a-value and b-value in the Matano Fault by Using the Least Square and Likelihood Methods
Madona 1#+, Mohammad Syamsu ROSID1, Nelly Florida RIAMA2
1University of Indonesia, 2Indonesian Agency for Meteorology, Climatology and Geophysics
The Matano Fault is one of the active faults in the Sulawesi mainland, extending in a northwest-to-southeast direction. The defect exhibits a sinistral slip mechanism, with a displacement rate of 5 millimeters per annum. The rocks located north of the fault line have undergone a displacement of around 20 km, suggesting that this fault has resulted in a cumulative northwestward shift of rocks totaling around 20 km since its formation. Examining the seismic vulnerability of a region is a crucial measure in mitigating the impact and minimizing the harm caused by earthquakes. The seismic intensity, referred to as the a-value, and the susceptibility of the rock, known as the b-value, are two earthquake parameters that can function as risk indicators. The objective of this research is to determine the a-value and b-value in the Matano fault by employing the Least Square and Likelihood methods. According to the USGS and BMKG databases, 1,287 earthquakes were reported at the Matano fault between 1923 and 2023 in total. The a-values for the Least Square and Likelihood techniques are 4.7069 and 4.7471, respectively. The b-values are 0.5547 and 0.5544, respectively. Identifying the a-value and b-value of earthquake magnitude can serve as a precursor and enable the prediction of future earthquakes in the Matano fault.
SE04-A001
Earthquake Forecasting in Sumatra: Application of the Area Source Model and the Seismicity Smoothing Model
Rizki WULANDARI1#+, Chung-Han CHAN2
1Sumatera Institute of Technology, 2National Central University
We introduce an earthquake forecasting approach tailored for Sumatra, Indonesia. Our methodology integrates an area source model and a seismicity smoothing technique. The initial step in building the earthquake catalog involves declustering, designed to remove foreshocks and aftershocks within specified distance and time parameters linked to the mainshocks. Considering catalog completeness, we include events with a magnitude of Mw ≥ 4.8 recorded between 1964 and 2006 for model training. The area source is divided into five subregions, taking into account the tectonic framework, neotectonic architecture, and geological conditions. The seismicity rate within each subregion is determined using the Gutenberg-Richter relation, expressed as log10(N) = a - bM. To apply the smoothing model, we conducted tests with various bandwidths (i.e., 25, 50, 75, and 100 km), assuming a b-value of 1.0. Smaller bandwidths reveal detailed spatial heterogeneity, with a 50 km bandwidth proving optimal for forecasting performance in our study area. Both forecasting models heightened seismic activity along the Sumatran fault and the Sunda trench. To validate our models, we employ Molchan diagrams for quantitative assessment, demonstrating that both models outperform the 1% null hypothesis, underscoring their effectiveness in earthquake forecasting. Moreover, the smoothing model provides a superior forecast for future events with Mw ≥ 5.5. The findings from this study offer valuable insights for refining seismicity analysis methodologies, particularly in earthquake-prone regions like Sumatra, enabling a more precise understanding of earthquake patterns and their implications for seismic hazard assessment.
SE04-A011
Study for Characterizing Potentiality Earthquake and Tsunami Hazard: Probabilistic Seismic Hazard Analysis and Potential Tsunami Height Simulation in the Coastal Area of Sumatra
Wahyu TRIYOSO1#+, Widjo KONGKO2, Gegar PRASETYA3
1Bandung Institute of Technology, 2Badan Riset dan Inovasi Nasional, 3Ikatan Ahli Tsunami Indonesia
This study utilizes integrated geological, geodetic, and seismological data to evaluate the potential for tsunamis and seismic hazards in the coastal area of Sumatra. The focus is estimating the potential level of ground shaking generated from seismic activity within the Sumatra Fault Zone (SFZ) and subduction zone, using Peak Ground Acceleration (PGA) as a measure. This study combines models developed by various researchers and earthquake catalogs from various periods. This study compiled a complete catalog of shallow earthquakes between 1963-1999 and 1963-2006. δAIC was used to assess the reliability of the models. One model emerged as the most reliable in this study in all tests. This model was constructed by combining a smooth seismicity model from relatively small to moderate earthquake catalog data with a relatively uniform background model. The model is then weighted by the normalized seismic moment rate derived from the surface strain rate. Longer observation periods and using a complete catalog of earthquakes, even if they are relatively small to moderate, can produce more reliable and accurate models. The Seismic Hazard Function (SHF) is calculated by considering magnitudes of 6.5 to 9.2 for subduction sources and 6.5 to 7.8 for SFZ sources. In addition, tsunami heights were simulated to estimate the potential hazard risk. The tsunami source model in this study considers the potential for giant earthquakes and tsunamis in the subduction zone off the south coast of Sumatra Island in the long term. The potential source zone is characterized using correlation dimension (DC) cross-correlation based on a catalog of shallow earthquakes from 2010 to 2022 and SHmax values of surface strain rate or seismic moment rate. The findings provide valuable insights into seismic and tsunami hazards, which can benefit future mitigation strategies. The results of this study have implications for the implementation of seismic mitigation measures.
Session Chair(s): Ping TONG, Nanyang Technological University
SE08-A001
3-D High-resolution Velocity Structure of the Indo-Eurasian Continental Collision Zone
Jiawei LI1,2+, Shunping PEI3,1#, Quan SUN4, Hanlin LIU5, Wei LIU1,2, Qian HUA1,6, Lei LI1,2
1Chinese Academy of Sciences, 2University of Chinese Academy of Sciences, 3Yunnan University, 4Yangtze University, 5Institute of Tibetan Plateau Research, Chinese Academy of Sciences, 6Shaanxi Earthquake Agency
As the front edge of the continental collision zone, the Indo-Eurasian continental collision belt has great significance for studying the plate collision process, plateau uplifting mechanism and orogenic activities within the plateau. Several models have been proposed to explain north-south compression collision and east-west extension based on geological and geophysical observations. Among them, the distance and shape of subducted India's lower crust and its geometry under the southern Tibet rift are still controversial. To address these issues, we analyze arrival times of P- and S-wave from 35,193 local and regional earthquakes recorded by 575 permanent and temporary stations, and apply an improved double-difference tomography method to obtain high-resolution 3-D P- and S-wave velocity structures of the crust and upper mantle and the locations of the relocated events in the Indo-Eurasian continental collision zone. The east-west velocity profiles reveal that there exists a discrete high-velocity layer dipping eastward at depths of 40-60 km beneath the Longgar rift (LGR), Tingri-Nyima rift (TNR), Xianza-Dinggye rift (XDR), and Yadong-Gulu rift (YGR), which suggests that the subducted Indian lower crust had experienced tearing. On the basis of comprehensive analysis about seismicity, source mechanism of large earthquake in the mantle, and tomographic images, we propose a new dynamic model to present India-Eurasia collision and North-South rifts formation. The significant character of this model is that, the rifts do not cut through the crust vertically but obliquely.
SE08-A010
3D Crustal Structures Beneath the Southern Korean Peninsula and Coastal Areas Using Seismic Full Waveform Inversion
Jung-Hun SONG1#+, Junkee RHIE1, Seongryong KIM2
1Seoul National University, 2Korea University
Constraining detailed three-dimensional (3-D) crustal structures is crucial for understanding tectonic history and assessing the impact of multi-scale crustal heterogeneities on seismic wave propagation. Precise measurement of velocity gradients is necessary, relying on accurate numerical simulations for seismic waveforms, for construction of an accurate 3-D crustal velocity model. We applied seismic full waveform inversion for developing 3-D crustal structures in the southern Korean Peninsula (SKP), using seismic waveforms from regional earthquakes. Despite the SKP region being recognized as a tectonically stable intraplate area, earthquakes with small-to-moderate magnitudes (Mw 3~5) have consistently occurred within the peninsula and adjacent coastal areas. This calls for a high-resolution seismic velocity model for estimating ground motions from potential earthquakes, facilitating seismic hazard analyses, and understanding the fundamental mechanisms behind distinct earthquakes. We used the spectral-element method for waveform simulations and adjoint methods for calculating finite frequency sensitivity kernels. We iteratively updated the initial seismic velocity model by applying multiple schemes (i.e., conjugate gradient, l-bfgs) to calculate velocity gradients at different iterations, thereby enhancing the accuracy of the gradient for an optimized model. Isotropic velocities were initially updated, followed by the incorporation of radially anisotropic parameters as the model improved. The improvement of an updated model was indicated by a total reduction of phase and amplitude misfits. We observed enhancements in the amplitudes of multiscale structures at different depths, contributing to improved waveform fitting. Notable features include prominent low-velocity anomalies in sedimentary basins and NE-SW trending low-velocity anomalies aligning with granite intrusions extending from the peninsula to coastal areas. New features were depicted, such as linear trends in radially anisotropic structures along major fold-and-thrust belts and near the boundaries of massifs. The observed structures suggest a tectonic inheritance in old continental remnants derived from multiple deformation events controls regional seismic activity.
SE08-A011
Imaging Intrinsic Attenuation Tomography from Array-based Measurements of Teleseismic Surface Waves
Xueyang BAO#+
Southern University of Science and Technology
Intrinsic attenuation describes the dissipation of seismic wave energy in anelastic media. It provides essential constraints to the thermal and rheological structures and the associated deformation mechanisms in the Earth’s deep interior. However, imaging intrinsic attenuation is more difficult than wave-speed tomography due to the complex effects of elastic heterogeneities on seismic wave amplitude. Here we derive an array-based theory of surface-wave propagation that well accounts for intrinsic attenuation and other factors of elastic heterogeneities such as scattering and present a novel method for isolating intrinsic attenuation properly. We carry out synthetic inversions to validate the effectiveness of our method, with synthetic seismograms computed from a newly developed algorithm that counts in physical dispersion and dissipation in anelastic media and maintains accuracy and stability even if intrinsic attenuation is strong. Compared to the traditional method that does not behave well in the synthetic inversion, our method well recovers the input intrinsic attenuation anomalies. Our results suggest that this new method can successfully resolve intrinsic attenuation from the complicated effects of elastic heterogeneities. Our method is promising in accurately imaging high-resolution attenuation structures with low computational cost given the rapidly developed seismic-array data acquisition.
SE08-A012
P and S Wave Velocity Structures of the Eastern Sino-Korean Craton
Yanbing LIU#+, Tae-Kyung HONG, Junhyung LEE, Seongjun PARK, Jeongin LEE, Byeongwoo KIM
Yonsei University
This study investigates the eastern North China Craton (ENC), Korean Peninsula, and Bohai and Yellow Seas. These areas are located in the convergence region of ancient Asian Ocean, Tethys Ocean, and Pacific Ocean, collectively constituting the eastern Sino-Korean Craton (SKC). The areas currently undergo a significant craton destruction process. However, the precise boundaries of major geological units and their stress conditions are still inadequately understood. A velocity tomography of the entire eastern Sino-Korean Craton (SKC) demands refinement, particularly at the China-South Korea border, where the resolution is relatively poor due to the absence of collaborative works based on seismic data from both Chinese and South Korean stations. The study integrates a comprehensive dataset, combining 87,260 earthquakes recorded at 680 Chinese seismic stations since 2008 and 5,400 earthquakes recorded at 483 South Korean seismic stations since 2017. A joint inversion method, VELEST, is employed to determine velocity models and hypocenters, which are refined using a double difference method, HYPODD. All the seismic events are relocated, and 1D minimum velocity models are improved. Different regions with diverse geological backgrounds undergo separate relocation procedures. The P and S arrival times for the Korean dataset are obtained using both a machine learning method PHASENET and manual picking. The machine learning model is trained to be adapted to the Korean data set. Subsequently, the TOMODD tomography method is applied to image the P-wave and S-wave velocity structures. The inverted models reveal the P and S wave velocity structures of the eastern SKC, featuring pronounced anomalies and low-velocity layers intricately connected to the ongoing craton destruction process. This research contributes new insights into the tectonic evolution and seismic activity of this dynamic region.
SE08-A029
Adjoint-state Traveltime Tomography (TomoATT)
Ping TONG#+, Jing CHEN, Masaru NAGASO, Mijian XU, Shijie HAO
Nanyang Technological University
Adjoint-state traveltime tomography is an efficient approach for determining subsurface seismic structures (Vp, Vs, anisotropy) and earthquake locations using body wave traveltime data. One remarkable feature of this approach is its independence from ray tracing. Instead, the traveltime field is obtained by numerically solving the Eikonal equation. When imaging subsurface structures, any traveltime discrepancies observed at seismic stations are transported back to the media to identify the causes, achieved by solving the adjoint equation of the Eikonal equation. When locating earthquakes, the adjoint method initially switches the roles of sources and seismic stations, and subsequently, it accurately determines earthquake locations by relocating (virtual) receivers. Absolute arrival times, common-source differential arrival times, common-receiver differential arrival times, and second-order differential arrival times, with various sensitivities, can effectively constrain subsurface structures and earthquake locations. Notably, adjoint-state traveltime tomography has also been extended to invert surface wave traveltime data for seismic velocity and anisotropy. The usage of the associated software package, TomoATT, can be found at www.tomoatt.com.
SE08-A013
Investigation of Crust-to-upper-mantle Structure in Gangwon Province Using a Combined Analysis of Ambient Noise Tomography and Earthquake-based Eikonal Tomography
Seongjun PARK#+, Tae-Kyung HONG
Yonsei University
Gangwon Province in South Korea, located near the eastern margin of the Eurasian plate, has experienced complex tectonic evolution including continental collisions and rifting. The region presents relatively low seismicity in the Korean Peninsula. However, moderate-size earthquakes and clustered earthquakes around potential Quaternary faults raise concerns on potential seismic risks that are supported by historical seismic damage records. The medium properties may provide essential information on seismic and tectonic natures, which is crucial for mitigating seismic risks. We investigate crust-to-upper-mantle seismic velocity structures in the region using the ambient noise tomography and earthquake-based Eikonal tomography based on dense seismic networks with 265 stations. Inter-station Green’s functions are retrieved by cross correlating one-year-long noise records in 2022. The fundamental-mode Rayleigh-wave group velocities are measured at periods of 1-15 s from the Green’s functions for 31,532 station pairs, followed by the tomographic inversion. We additionally analyze Rayleigh waves from 337 global MW5.5-8.1 earthquakes in 2018-2022. We measure Rayleigh-wave travel times at stations using a cross-correlation technique, determining phase velocities at periods of 20-80 s over the region. Finally, 3-D shear-wave velocity structures at depths up to ~200 km are inverted from the Rayleigh-wave velocities by the linearized inversion combined with the Markov-chain-Monte-Carlo technique. The velocities generally increase with depth, exhibiting significant lateral variations. At depths of < ~2 km, we find low velocities along the east coast and basin areas and high velocities in mountain areas. At depths of 3-20 km, strong velocity contrasts are observed around notable earthquakes. At depths of ~30-40 km, high velocities appear along the east coast, suggesting shallow Moho depths. At deeper depths, we observe low velocities in the eastern margin, which may be associated with the absence of lithospheric root. The observations may contribute to comprehension of seismic and tectonic processes in the region.
SE08-A016
Constraints on the Crustal Seismic Properties of the Southern Korean Peninsula Using Virtual Deep Seismic Sounding
Young Oh SON1#+, Young-Hee KIM1, Chunquan YU2
1Seoul National University, 2Southern University of Science and Technology
The southern Korean Peninsula (SKP) represents an important link between continental blocks of North and South China and the island arcs of Japan. It is dominated by several NE-SW to NNE-SSW trending tectonic units that include Yeongnam Massif and Gyeongsang Basin in SE of SKP, Gyeonggi Massif in NW, and Okcheon Belt in between. Knowledge of the average P-wave velocity (VP), thickness (H) and P-to-S velocity ratio (κ) of the SKP crust can provide key information on its crustal composition, isostasy, and thermal state. In this study, we constrain VP, H, and κ of the continental crust of the SKP via a joint analysis of Virtual Deep Seismic Sounding (VDSS) and P-wave receiver function (PRF). For VDSS, we inverted for H and VP by fitting traveltimes and phases of direct S and SsPmp recorded by 188 stations (106 broadband seismometers and 150 accelerometers) in SKP. Our preliminary results of VP and H range within ~6.0 – 6.7 km/s and ~23 – 34 km, respectively. Differential arrivals of converted phases in the PRF were combined with VP and H from VDSS to compute κ, mostly within ~1.66 – 1.82. Crustal constituents inferred from obtained VP and κ lie within typical range of metamorphic rocks and granites, with intermediate to felsic composition. High VP over 6.4 km/s in southern part of Yeongnam Massif and Gyeongsang Basin might reflect magmatic underplating induced by the subduction of Izanagi Plate in the Cretaceous. Similar value in the southwestern part of Okcheon Belt seems to be related with rifting between Precambrian massifs in the Paleozoic. Shallow Moho (~23 – 25 km) along the eastern coast shows evidence for the opening of the East Sea of Korea (Sea of Japan). Generally lower κ in the Gyeonggi Massif might infer different tectonic origin compared to other units.
SE08-A022
Multiscale Seismic Imaging of Noise Tomography and Receiver Function in the Xing'an-Mongolia Orogenic Belt and Northern of the North China Craton Based on Short Period Dense Array
Jian XU#+
Sun Yat-sen University
The research area is in the eastern part of Inner Mongolia, which is also the junction of the North China Craton and the Xing'an-Mongolia Orogenic Belt. The southern of the research area, which belongs to the North China Craton, is rich in gold deposits, while the northern part is characterized by a large amount of non-ferrous and rare metal minerals in the Xing'an-Mongolia Orogenic Belt. In order to explore the deep faults, rock masses, and their respective crustal characteristics that control these two areas, from June to September 2023, we have invested 379 short period seismometers and carried out three tasks: dense array, short profile, and long profile, with a spacing of 50-1500 meters between stations. We set up a dense array of 379 instruments in the Yinxiangou gold mine area of the North China Craton. A short profile, formed by 109 instruments, passed through the Karaqin metamorphic core complex and the Nenjiang -Balihan deep fault, which reveal the process of the North China Craton's destructive structure. In order to reveal the interaction between the North China Craton and the Xing'an-Mongolia Orogenic Belt, a long profile was formed by 211 instruments. The observation periods were 7-35 days. A background noise imaging study was conducted in the Yinxiangou ore, and we collected 18000 Rayleigh wave phase velocity curves. The shallow velocity structure of 3.5km in the Yinxiangou mining area was obtained through inversion. We conducted receiver function research on short and long profile, more than 7000 receiver functions were obtained, revealing the complex structures of deep faults, complex rock masses, and the characteristic of crustal of the two regions.
SE08-A025
| Invited
Seismic Imaging of Crustal Structures Beneath Sedimentary Basins: Case Studies in the Ordos Basin and the Gulf of California
Chunquan YU#+, Weiliang YIN, Chengxin SHUAI, Tao YANG
Southern University of Science and Technology
Seismic imaging of crustal structures beneath sedimentary basins is challenging, as low-velocity sediments often generate strong reverberations that mask desired signals or cause significant delays. Recently, a new method has been developed to image the Moho by taking advantage of the presence of sediments. The method relies on Pn and its first crustal multiples PnPn from regional earthquakes. The difference between PnPn and Pn is essentially a critical PmP reflection from the bottom of the crust. Both synthetic tests and field examples demonstrate the usefulness of this method. In this study, we apply this method to two case studies in the Ordos basin and the Gulf of California. In the Ordos basin, joint analyses of Pn multiples and conventional receiver functions provide constraints on the shallow sedimentary structure and the thickness, Vp and Vp/Vs ratio of the crystalline crust. The absolute crustal Vp ranges from 6.45 to 6.57 km/s and the Vp/Vs ratio ranges from 1.73 to 1.78, suggesting an overall intermediate crustal composition beneath the northern Ordos basin. Crustal thickness beneath the interior of the northern Ordos basin is about 40 km, consistent with predictions from Airy isostasy. In the Gulf of California, conventional passive source methods are unable to image the crustal structure because of no station coverage. We take advantage of the high seismic activity in this region and apply waveform modeling of near-source Pn multiples to determine its crustal structure. The crustal thickness beneath the northern part of the Gulf of California ranges from 10~20 km, generally consistent with thin crust estimated by active source studies. We expect that the method can be applied to other regions covered by sedimentary basins.
SE08-A028
| Invited
P-wave Azimuthal Anisotropy of New Zealand Revealed by Adjoint-state Traveltime Tomography
Shucheng WU1+, Jing CHEN2, Ping TONG2#
1China University of Geosciences (Wuhan), 2Nanyang Technological University
The omission of seismic anisotropy in current reference models covering the entire New Zealand has been an obstacle to achieving a comprehensive understanding of deformation and dynamics along the complex Pacific-Australian plate boundary segment. Here we present a 3D azimuthally anisotropic model that encompasses both the North and South Islands of New Zealand to a depth of 40 km, using over 1 million local P-wave arrival times and a newly developed adjoint-state travel time tomography technique. This model is built upon the New Zealand-wide 3D isotropic velocity model, serving as an essential and incremental update to the existing model. Our new model highlights significant variations in anisotropy across the plate boundary region, indicating distinct deformation states between tectonic blocks. In the North Island, pronounced along-strike changes in anisotropy are evident beneath the Hikurangi forearc, which could be attributed to variations in stress regime associated with the oblique plate convergence and changes in interseismic coupling of the subduction megathrust. The oblique plate motion further induces pure shear deformation in the middle to lower crust of the southern backarc, resulting in strong anisotropy with fast axes perpendicular to the principal axes of maximum horizontal compression. In contrast, seismic anisotropy in the central South Island primarily stems from the preferential alignment of minerals, notably within the Haast schist in the Otago block. However, anisotropy in the middle to lower crust of the northern South Island may represent inherited structures that originated during past southward subductions along the Gondwana margins at ~100 Ma. Our new model offers valuable insights into the intricate geological processes occurring within the plate boundary region.
SE01-A011
High-resolution Enviromagnetic Records of the Last Deglaciation from Haojiatai, North China
Ping LIU#+
University of Chinese Academy of Sciences, China
Nihewan Basin is one of a series of well-developed East Asian Cenozoic basins in Hebei Province, North China, which has abundant Nihewan Beds of fluvio-lacustrine origin underlain by the Pliocene eolian Red Clay and overlain by the late Pleistocene loess and paleosol. The fluvio-lacustrine sequence is rich sources of mammalian faunas and Paleolithic sites, which is famous in the world, thus providing unique insights into our understanding of land mammal biochronology and early human settlements in East Asia. After the demise of the Nihewan paleo-lake, the loess and paleosol during the last deglaciation was covered in the Nihewan Basin, same as in the Chinese Loess Plateau. Detailed paleoclimate records during the last deglaciation are highly valuable for understanding rapid climatic changes and mechanisms. High resolution paleoclimate records in the Nihewan Basin is essential due to its sensitivity to climate variability and importance for human inhabitance. A high resolution environmental magnetic investigation has been performed on a sedimentary sequence from Haojiatai in the central of Nihewan Basin, which covers the period of 13 ka. Detailed magnetic minerals are identified from the top loess and paleosol the same as the Chinese Loess Plateau, which are magnetite as the main magnetic carriers, corresponding to rapid climate fluctuations after the Last Glacial Maximum. Our findings reflect the rapid climate fluctuations during cold and warm periods in the lake sediments, which were ultimately controlled by climate changes during the last deglaciation.
SE01-A017
Revising Magnetic Anomaly Lineations in the Northwestern Pacific Ocean Using the Latest Data
Juri UDA1#+, Masao NAKANISHI1, William W. SAGER2
1Chiba University, Japan, 2University of Houston, United States
We revised magnetic anomaly lineations from Late Jurassic to Early Cretaceous in the northwestern Pacific. Ocean using the latest geomagnetic data. Five magnetic anomaly lineation sets exist in the northwestern Pacific Ocean (e.g., Nakanishi et al., 1992). Nakanishi et al. (1989, 1992) identified magnetic anomaly lineations in the western Pacific Ocean. After then, Some works revised them in the limited areas; in the Central Pacific Basin (Nakanishi et al., 1998), around Shatsky Rise (Nakanishi et al., 1999; 2015), and around Japan Trench (Nakanishi, 2011). There are still places where magnetic anomaly lineations are identified. The geomagnetic data for this study are obtained from the databases of several domestic and overseas organizations (e.g., Japan Agency for Marine-Earth Science and Technology and National Oceanic and Atmospheric Administration/National Geophysical Data Center). The data are composed of total geomagnetic field data obtained by a surface-towed magnetometer and vector geomagnetic data obtained by a shipboard vector magnetometer. We calculated magnetic anomalies using Comprehensive Model 4 (CM4, Sabaka et al., 2004) and the latest International Geomagnetic Reference Field (IGRF, Alken et al., 2021). For the areas where useful data are insufficient, we determined the strikes of magnetic anomaly lineations using vector geomagnetic data. We revised the magnetic anomaly lineations are revised in the vicinity of the Shatsky Rise and Japan Trench, and Kuril trenches. We revised the strike of magnetic anomaly lineations west of Shatsky Rise. The new strike, N38°W is parallel to abyssal hill fabric.
SE01-A020
Implications of Goethite and Its Polymorphs in the Lower Mantle: A First Principles Approach
Sparsh SHARMA#+, Gaurav SHUKLA
Indian Institute of Science Education and Research Kolkata, India
Goethite (α-FeOOH) is one of the most common iron oxyhydroxides found on the surface of the Earth and inside the crust. It is an essential component of rust and bog-iron ores and a primary hydrous mineral. The study of hydrous minerals is of paramount relevance as they are crucial in transporting water into the Earth’s interior and affect the geophysical and geochemical processes. Recent studies have proposed that Goethite and its polymorphs might have the capability to transport water to the lowermost part of the mantle up until the core-mantle boundary and might contribute to the formation of seismic heterogeneities like the ULVZs. Thus, a study of Goethite and its polymorphs might play a pivotal role in understanding the water, hydrogen, and oxygen cycles inside the Earth and the role of iron in the deep Earth processes. Using the first principles studies, we tried to understand the structural changes associated with α-FeOOH, ε -FeOOH, and Py-Phase (FeOOHx) as they undergo the lower mantle pressures. The first principles calculations were performed using Density-functional Theory (DFT) as implemented in the Quantum Espresso package, and the thermodynamics, electronic, and thermoelastic properties of different phases of Goethite and their stability in the pressure-temperature conditions of the deep Earth have been studied.
SE01-A026
High Resolution Crustal Property Maps for the Southern Korean Peninsula Via Teleseismic P-wave Coda Autocorrelation
Hyejeong CHO1+, Sang-Jun LEE2#, Seongryong KIM1, Junkee RHIE1
1Seoul National University, Korea, South, 2Korea National University of Education, Korea, South
The crustal thickness (H) and P-wave velocity over S-wave velocity ratio (κ), are basic information for seismology to analyze earthquake location, wave propagation, hazard assessment, and so on. Although several crustal models for the southern Korean peninsula have been constructed by various methods, including receiver function analysis, and tomography, their resolution is limited due to the limited number of stations in KP before 2016. Thus, in this study, 290 accelerometers operated during 2018-2020 are used to measure H and κ beneath each station, extracting reflection responses via autocorrelation. The recent technique adopting spectral whitening to autocorrelation enhances high frequency energy in teleseismic records and suppresses zero-lag signals in autocorrelation functions, which makes Moho reverberations extracted stably. The preliminary results show more detailed features than the previous models, such as a shallow H along the Honam shear zone, or a low κ in the middle of Yeongnam massif, in addition to a consistent pattern to the previous models. Our results can be improved by combining additional information, such as receiver function, and ambient noise autocorrelation.
SE01-A036
Crustal Anisotropy and Deformation Implication in the East Margin of Tibetan Plateau
Yuan GAO#+, Xinyi LI, Ying LI, Shuyu LI, Jianhui TIAN, Peng WU
China Earthquake Administration, China
Strong complicated tectonic movements with high seismicity are in the east margin of Tibetan Plateau. The S wave splitting (SWS) of local earthquake records indicates seismic anisotropy in the upper crust, which is related to the crustal stress and deformation. Therefore, SWS could be available to study the crustal deformation. In order to investigate the crustal deformation, this study shows the seismic anisotropy of SWS in the upper crust in the east margin of Tibetan Plateau. Firstly, the polarizations of fast S waves (PFS) in the study area show the dominant orientations nearly parallel to the compressive stress directions or the strikes of faults, although always scattered at some of stations. With the observed PFS characteristics, it is effective to extract the compressive stress directions. In addition, the PFS data could also be adopted to analyze the tectonic information, such as the strike of fault or the important tectonic boundary. Secondly, the time-delays of slow S waves (TDSS) always relate to the crustal deformation, as well as the local seismicity. It means that TDSS could reveal the local temporal tectonic information, too. Last, SWS could also show the pattern of spatial differential PFS distribution, which indicates the different anisotropic subzones in the upper crust in the east margin of Tibetan Plateau. Further it suggests that SWS is effective to detect the crustal seismic anisotropy and tectonic implications [supported by NSFC Projects 42330311 & 41730212, National Key R&D Project of China 2017YFC1500304].
SE02-A014
AI-based Framework as a Tool for Comprehensive Earthquake Catalog
Jongwon HAN1#+, Keun Joo SEO2, Ah-Hyun BYUN3, Seongryong KIM1, Dong-Hoon SHEEN4, Donghun LEE1
1Korea University, Korea, South, 2Korea Meteorological Administration, Korea, South, 3KEPCO Engineering & Construction Company, Inc., Korea, South, 4Chonnam National University, Korea, South
This study introduces an advanced framework that merges deep learning (DL) with conventional techniques for processing seismic data from the southern Korean Peninsula (SKP). The framework effectively expands the catalog to include micro-earthquakes (<ML 2.0), going beyond the limits of physics-based methods. This reduces manual human efforts significantly and facilitates near-automated analysis. Covering data from over 300 stations in the SKP from 2012 to 2021, this approach greatly decreases processing time by integrating Graphics Processing Units and parallel computing. A retrained DL phase picker in our framework accurately identifies P and S seismic phases, associating them with 66,858 seismic events. Using DL-based methods, we precisely assessed the seismic properties of natural earthquakes in the SKP, providing a more comprehensive catalog with a lower magnitude of completeness compared to the previous catalog. Furthermore, our framework effectively identified micro-earthquakes not only in a temporary seismic network of the SKP but also in other regions (i.e., Yukon, Canada, and Khovsgol, Mongolia), outperforming conventional methods. After identifying the polarities of P-waves with a DL model, we automatically determined their focal mechanisms and precisely estimated the stress fields in the study areas. These compiled earthquake catalogs are invaluable for future seismological studies, such as seismic tomography and hazard assessment, and underscore the potential of DL in revealing seismotectonic features in areas with low seismic activity.
SE02-A015
Semi-analytical Calculation of Nearfield Tsunami and Seismic Waves in a Stratified Half-space by the Discrete Wavenumber Method
Hiroshi TAKENAKA1#+, Tomotsugu WATANABE1, Takeshi NAKAMURA2
1Okayama University, Japan, 2Central Research Institute of Electric Power Industry, Japan
We develop a quasi-analytical method for calculating of nearfield tsunami and seismic waves for a flat multi-layered ocean-solid earth model. The surface layers are sea water, where each layer is assumed to be a uniform layer of a compressible and inviscid fluid with a constant acoustic velocity and a density stratification (density gradient). A gravity field with constant acceleration g acts in the downward direction in the fluid, and is ignored in the solid. The response at any position in ocean-solid earth model, including the sea surface and sea bottom, due to a buried dislocation source in the solid earth is calculated with the propagator matrices and the discrete wavenumber summation. These operations produce the complete nearfield synthetics of the displacement, particle velocity, strain, pressure, and stress for sub-oceanic earthquake sources, which include all acoustic, body and surface wave phases as well as tsunami waves and static deformation. Around near-fault area under the sea the seawater motion associated with tsunami generation immediately follows the sea-bottom seismic motion, permanent sea-bottom deformation and ocean acoustic waves. The present method could be a useful tool to interpret the dynamic and quasi-static motion above and on the sea floor which may be extracted from the pressure, seismic, acoustic and/or strain (optical) sensor records at the sea floor.
SE04-A002
Healing Process of the Longmenshan Fault After the 2008 Wenchuan Earthquake Reflected in GNSS Time-series
Jing ZHAO1#+, Zhengyi YUAN1, Xiaoxia LIU2
1China Earthquake Networks Center, China, 2China Earthquake Administration, China
We collected and calculated the GNSS continuous observation data. Using the time-series results of GNSS continuous stations after the Wenchuan earthquake, the dynamic evolution of fault locking and slip deficit rate in the middle and southern sections of the Longmenshan fault zone was inverted using the TDEFNODE (McCaffrey et al., 2013) and analyzed, and the healing process after the Wenchuan earthquake was discussed based on the inversion results. The results show: (1) The locking fraction of the ruptured area around the Wenchuan earthquake epicenter gradually increased, which was basically in creeping state in 2010, and then in state of strongly locked in 2013. The locking area also gradually increased from the southwest of the Wenchuan earthquake epicenter to the epicenter, which indicates that this part of the fault has been healing rapidly. Most of the ruptured zone in the northeast of the epicenter is still in creeping state and the fault has not yet begun healing. (2) The area near the Lushan earthquake epicenter and its SW direction of the fault has been in a strong state of locking, and the slip deficit rate of the completely locked area has been decreasing year by year, probably indicating that the healed region shares part of the compression effect of the Bayan Har block on the Sichuan Basin (Zhao et al., 2021).The above results indicate that the healing process and activity characteristics of different segments of the Longmenshan ruptured fault are significantly different after earthquake. The southwest segment of the Longmenshan fault zone is in state of strongly locked and the background for a major earthquake has strengthened in the case of rapid accumulation of compressive elastic strain. This work was supported by Science for earthquake resilience (XH23047A).
SE04-A003
Early Forecast of Aftershock Shaking: A New Scheme Based on Extreme Value Statistics and Bayesian Estimation
Kaoru SAWAZAKI#+
National Research Institute for Earth Science and Disaster Resilience, Japan
The aftershocks that follow a major earthquake often bring additional severe damage to society. Although minor tremors do not directly cause significant damage, the repetition of many small shakings can lead to anxiety among the victims, raising concerns about deteriorating health conditions and other related issues. Therefore, providing an outlook on aftershock activity as soon as possible after the mainshock is strongly desired. Typically, the overlap of seismic waveforms in seismic records during seismically active periods causes the failure of P and S phase picking, leading to deterioration of earthquake catalog. To address this issue, in this study, I propose a new scheme to forecast ground shaking due to aftershocks using the extreme value statistics and Bayesian estimation, without relying on earthquake catalog. The maximum amplitude of seismic records within certain time intervals follows a non-stationary Frechet distribution (Sawazaki, 2021). By using Bayesian estimation of the parameters governing this distribution, it is possible to calculate the exceedance probability of the maximum amplitude of future seismic motion, as well as the exceedance probability of the occurrence number of shakings exceeding any threshold value. I applied this method to aftershock sequences that followed major crustal earthquakes in Japan. As a result, using seismic records within one hour of the mainshock, it was possible to reasonably provide the forecast for up to approximately one week afterward. The forecasted values for the maximum amplitude tended to be consistently overestimated overall, due to the saturation of amplitude with respect to magnitude of earthquakes. On the other hand, the number of felt earthquakes fell within the expected range of forecast.
SE04-A004
Feasibility of Real-time Seismic Intensity Prediction by Combining Deep Learning and Simulated Data
Ahyi KIM1#+, Anju OHTA1, Yukino YAZAKI1, Masami YAMASAKI1, Hisahiko KUBO2
1Yokohama City University, Japan, 2National Research Institute for Earth Science and Disaster Resilience, Japan
When an earthquake occurs, prompt identification of the seismic intensity and arrival time of a large shake is important in terms of ensuring the safety of the population, timing of evacuation, rescue operations, etc. Yet, predicting seismic intensity with high spatial resolution accurately typically requires increasing seismic station density, a solution often impeded by cost constraints. Consequently, current methods supplement this with geological information, which unfortunately leads to variable accuracy dependent on the quality and amount of such data. In this study, we tried alternative approach: a deep learning-based method for predicting seismic intensity that does not rely on existing geological information. Utilizing the Long-Short Time Memory (LSTM) deep learning model, a real-time seismic intensity prediction model was developed specifically for the area around Yokohama City, characterized by its relatively insufficient training data. The model predicts real-time seismic intensity at a specific point based on data from four surrounding observation points, utilizing the K-NET strong-motion seismograph network. The study employed three training approaches: (1) using only real observation data, (2) combining real and simulated data, and (3) exclusively using simulated data. Predictions were evaluated using immediate (0-second lead time) and short-term (8-second lead time) prediction. Assessment metrics included Mean Absolute Error (MAE) and Root Mean Square Error (RMSE), compared against weighted averages and maximum values from input points. Results showed that immediate predictions were more accurate than comparative methods, and short-term predictions were equally or more precise. Furthermore, the study explored prediction potential in areas without historical data by creating 2000 simulated data points for scenario earthquakes. These scenarios were based on randomly determined earthquake parameters within existing data ranges. When the model was applied to the real observed data used in (1)-(3) above, the predictions performance was nearly as good as previous models, indicating effectiveness in unmonitored areas.
SE04-A005
Probabilistic Seismic Hazard Assessment for Continental Southeast Asia
Chung-Han CHAN#+
National Central University, Taiwan
We conducted a comprehensive assessment of seismic hazard in continental Southeast Asia by creating an extensive earthquake and fault database, developing seismic models for each seismogenic source, and generating regional seismic hazard maps. Our earthquake database comprises earthquake parameters sourced from various catalogs, such as the ISC, ISC-GEM, the global ANSS Comprehensive Catalogs, Seismological Bureau, and the Thai Meteorological Department in Thailand. To ensure consistency, we meticulously curated the earthquake data by eliminating duplicate events and standardizing magnitudes onto a moment magnitude scale. In order to account for epistemic uncertainty in seismic activity, we employed several seismic models, including the Gutenberg-Richter relationship, the pure characteristic earthquake model, and SHERIFS (Seismic Hazard and Earthquake Rate In Fault Systems), to forecast rupture probabilities along multiple fault segments. Incorporating the Vs30 map, which represents the average shear velocity down to a depth of 30 meters and was derived from an analysis of topographic slope, we considered site-specific effects and conducted a thorough assessment of probabilistic seismic hazards across continental Southeast Asia. The highest levels of seismic hazard were identified in the vicinity of the Sagaing Fault, which traverses several major cities in central Myanmar. The Sunda megathrust, with the potential for a magnitude 8.9 earthquake resulting from multiple-segment rupture, posed significant seismic hazards along the Western Coast of Myanmar and eastern Bangladesh. Additionally, our study revealed notable seismic hazard levels in northern Vietnam and along the boundary between Myanmar, Thailand, and Laos, primarily due to a series of strike-slip faults that have the potential to generate moderate to large earthquakes. The findings of this study hold great significance for various stakeholders, including regional governments such as The Association of Southeast Asian Nations (ASEAN), non-governmental organizations (NGOs), and insurance/reinsurance companies.
SE04-A006
Fluctuations of B-value Related to a Magnitude 6.9 Earthquake and a Seismic Swarm in the Noto Peninsula, Japan
Sota MAEGAWA#+, Toshitaka BABA
Tokushima University, Japan
Fluctuations of the b-value may indicate changes in the surrounding stress field and are possibly beneficial for earthquake prediction. Previous studies showed that the b-value decreased in the source region before the 2004 Sumatra earthquake and 2011 off the Pacific coast of the Tohoku earthquake. However, the timing and pattern of the b-value fluctuation differ in regions and earthquakes, and earthquake prediction based on b-values is a long way from a practical level. In this study, we analyzed fluctuations of b-value in the Noto Peninsula, Japan, where a M6.9 earthquake occurred in 2007, and a seismic swarm has been occurring since December 2020, to discuss the relationship between earthquake occurrence and spatial-temporal variation of b-values. We used the earthquake catalog of Japan Meteorological Agency from 1919. Although an extended period of the data provides an accurate analysis, we used data in a period after 1990 when there was enough data on earthquakes of M2 and greater. We therefore assumed Mc of 2.0 in the analyses. The b-value analyses focused on the southwestern part of the Noto Peninsula (region 1), where the M6.9 earthquake occurred, and the northeastern part (region 2), where the seismic swarm activity has been active. The b-value decreased preceding the M6.9 earthquake in the region 1, while no specific change was observed before a M6.5 earthquake in the region 2. There was an inverse correlation between the temporal changes of the b-values of the two regions. This inverse correlation may suggest an unclarified relationship between the M6.9 earthquake and the seismic swarm activity.
SE04-A015
Regional Crustal Stress Field in the Eastern Margin of the Eurasian Plate Around the Korean Peninsula
Junhyung LEE#, Dong Geon KIM+, Tae-Kyung HONG
Yonsei University, Korea, South
Regional crustal stress field is mainly influenced by regional tectonics. The regional stress field composition is crucial information for assessment of seismic hazard potentials. The Korean Peninsula is located in the eastern margin of the Eurasian plate. The region is surrounded by the Okhotsk, Pacific, and Philippine Sea plates. We investigate the regional crustal stress field in the Korean Peninsula using a stress inversion technique based on the focal mechanism solutions of earthquakes in the region. We collect the focal mechanism solutions of 473 earthquakes in the Korean Peninsula from previous studies. Also, we newly determine the focal mechanism solutions of 92 earthquakes using a long-period waveform inversion and P phase polarity analysis. The strike-slip earthquakes are dominant in the region around the Korean Peninsula. Reverse faulting and strike-slip faulting earthquakes occur in the western East sea. Normal faulting earthquakes are observed in the central Yellow Sea. We observe that the dominant compression directions are ENE-WSW, which may be associated with a combination of lateral compression from the Pacific and Philippine Sea plates. The observation may be useful for understanding the local stress field perturbation in the region.
SE04-A016
Chain of Paleoseismic and Paleolandslide Damming Events in the Namche Barwa Syntaxis--Sedimentary Records from River Valley
Ping WANG#+
China Earthquake Administration, China
Geological process of Eastern Himalaya Syntaxis (SE Tibetan Plateau) affected by tectonic and climate activities since the late Quaternary are extremely intense, which facilitates seismic activity and subsequent geological disaster. However, research into the traces of paleoearthquakes are scarce due to the complex geologic environment, facing huge challenges of seismic hazards assessment for railway and water conservancy engineering projects. In this study, thick fluvial-lacustrine sediments in the upper strath valley of the Tsangpo Gorge in the EHS show records of seismic activity in the form of soft-sediment deformation structures. Two earthquakes could be recognized from plenty of soft and brittle deformations structures of eight sections in the lower and upper terraces. They were dated by OSL and 14C as ~21 ka and ~7920±20 cal yr BP. Modern analogs and the association with surface ruptures suggest that the magnitude (Ms) of the Holocene earthquake was 7-7.5, suggesting that it may be attributed to the thrust activity of the Lulang Fault on the western Eastern Himalaya Syntaxis. The intensity and magnitude (Ms) of the Pleistocene earthquake are estimated as at least VII and 7, if this earthquake was also probably due to activity of the Lulang Fault.
SE04-A017
Prediction Efficiency Test of GPS Strain Parameters Based on Molchan-diagram and R-value
Zhengyi YUAN#+, Jing ZHAO, Huaizhong YU
China Earthquake Networks Center, China
The preparation and occurrence of moderate-strong earthquakes are always accompanied by the accumulation and release of crustal strain. Therefore, it is of great significance to study the spatial distribution features of GPS strain parameters for the earthquake prediction. In this paper, multi-period Global Positioning System (GPS) velocity fields of Chinese mainland (west of 107°E) are collected, and a variety of crustal strain parameters and corresponding gradient values are calculated using spherical least-squares collocation method. Combined with the earthquakes over MS5.0 (including aftershocks) occurring in the following 1-3 years, the prediction efficiency of each parameter is quantitatively evaluated by Molchan-diagram method. The results show that (1) the maximum shear strain rate and the second strain rate invariant have better prediction effect than the area strain rate; (2) the gradient values of the above two parameters have better prediction effect than their original values. Besides, the prediction efficiency test using the second strain in-variant gradient based on dynamic R-value scanning is further carried out, and the result mani-fests that R-values of the above parameter converge between 200 and 400 days, which indicates that it has a good prediction effect on the annual earthquakes greater than MS5.0.
SE04-A019
The Influence of Boundary Zone Structure of Active Tectonic Block on the Propagation of Strong Ground Motion Caused by Fault Activity
Dongli ZHANG#+, Xin SUN, Zijian FENG, Peng HUI, Shiqi WEI
Sun Yat-sen University, China
The boundary zone of active blocks not only serves as the main area for large earthquake preparation but also influences the propagation of strong ground motion due to its unique structure and geomorphic features, ultimately controls the distribution of earthquake disasters. The Yuncheng Basin, located in the east of the Ordos block is a part of the southwestern Shanxi graben system. In this study, a three-dimensional stratigraphic and velocity structural model of the Yuncheng Basin and its surrounding areas has been established for strong ground motion simulation. As an essential input, the finite fault source model of the Xiezhou segment, which characterized with strongest activity in the middle section of the northern Zhongtiaoshan fault, is set up with the potential magnitude Mw7.5 according to the seismic hazard evaluation. The corresponding seismic moment (Mo) is about 2.238e+27 dyne∙cm. The fault model reveals that the Xiezhou segment extends downward to a depth of 24km, and the dip angle (θ) decreases gradually from ground surface (θ=65°) to deep (θ=40°). The fault rupture surface on the source model is characterized by 74km in length along the strike direction and 32km in width extending the inclination. Three asperities are presumed on the rupture surface to simulate the inhomogeneity distribution of seismic energy and dislocations. The average slip(D)on the rupture is 369cm computing based on the formula Mo=uAD. The presume source depth is -15km. The simulation results presents that the distribution of seismic ground motion is affected significantly by the active block boundary zones and geomorphologic patterns. The peak of ground accelerations (PGA) in the computing area are concentrated in trips along the fault strike and restricted within northern region of the Yuncheng basin by the Zhongtiao Shan in the south direction and the uplift terrain of the Emei terrace.
SE04-A020
Influences of Active Tectonics on the Changes of Hydrological Precursors—Example of the Earthquakes in Qinghai, China in Recent Years
Huaizhong YU#+, Zhengyi YUAN
China Earthquake Networks Center, China
During the periods of 2021-2022, the 22 May 2021 Ms7.4 Maduo, 8 January 2022 Ms6.9 Menyuan, and 26 March 2022 Ms6.0 Delingha earthquakes occurred consecutively in Qinghai province, China. The hydrological observation instruments set up by the China Earthquake Administration allow us to study the dynamic processes in the well-aquifer systems during the establishment of criticality. Particularly, the observations played an important role in the prediction of the 8 January 2022 Ms6.9 Menyuan earthquake that was approved by the People’s Government of Qinghai province. To explore the performance of the hydrological observations in detecting earthquakes that occurred on different active tectonic blocks, we calculate the relative amplitudes of the pre-seismic changes. Results indicate that markedly pre-seismic change is found if the observation station and the detection earthquake are on the same block, and moderate change is found if they are on the adjacent blocks, while the precursor is hard to be identified if they are on the separated blocks. The variations in the hydrological responses may be caused by the strength weakening (or dilatancy) of source media. And the increased volumes in the crust can be evidenced by the changes in the geodetic time series in the same neighborhoods and during the same period, augmenting stress loading between the blocks.
SE04-A021
Spatiotemporal Changes in Stress State Off the Coast of Hokkaido and Tohoku Districts, Japan
Kazuyoshi NANJO#+
University of Shizuoka, Japan
Monitoring the Earth’s stress state plays a role in our understanding of an earthquake’s mechanism and in the distribution of hazards (Nanjo, 2020). Crustal deformation due to the occurrence of the 2003 Tokachi earthquake of magnitude (M) 8 and the 2011 M9 Tohoku earthquake caused stress perturbation in nearby regions. However, implications of future seismicity are still uncertain. Here, we evaluated changes in the b-value, a measure of the relative abundance of small and large earthquakes, as a function of space and time in northern Japan. Assuming that the b-value is negatively correlated with differential stress, we conducted an analysis based on b-values of seismicity off the coast of Tohoku district (Nanjo et al., 2012; Nanjo, 2023) to infer that the stress relieved by the 2011 Tohoku earthquake has not yet recovered to levels found before the earthquake. Contrary to the previous study on b-values (Tormann et al., 2015), we argued that the hazard of a great tsunami-producing earthquake off the coast of Tohoku district is unlikely to already be almost as high as it was just before the 2011 event. Many centuries of stress accumulation are required to rebuild stress and produce another great event (Bürgmann et al., 2016). Near the high-slip zone of the 2003 Tokachi rupture, we showed a pronounced decade-scale decrease in b, suggesting that the stress is accumulating. Comparison with previous studies on coupling between the Pacific plate and the continental plate (Iinuma, 2018; Matsu’ura, 2019; Nishikawa et al., 2019) showed that the zone of a decrease in b fell into an area of stronger coupling. The result is remarkably similar to the Tohoku case. It would be worthwhile to carefully monitor the spatiotemporal distribution of b-values off the coast of Hokkaido district.
SE04-A025
Evaluations of Long-period Ground Motions and Response Characteristics of Base-isolation Building by the Large Earthquakes Along the Nankai Trough
Sora TORIUMI1+, Atsuko SHIRAYAMA1#, Tadamichi YAMASHITA2, Shinji ITO3
1Tokushima University, Japan, 2Dynamic Control Design Office, Japan, 3Daiwa House Industry Co., Ltd., Japan
Recently, long-period seismic motions such as the Nankai Trough earthquakes have been predicted to occur. In the case of base-isolated buildings, the temperature of the seismic isolation devices rises due to the increased amount of energy absorbed during earthquakes, and their horizontal characteristics change under longer time and multiple cycles than normally assumed. The methods used to calculate the multi-cyclic characteristics of seismic isolation devices are the refined method and the simplified method. In this paper, time history response analysis considering multi-cyclic characteristics under long-period ground motions assuming the Nankai Trough Earthquakes and the Showa-Nankai Earthquakes is performed using the simplified method and exact method. The study targets base-isolated buildings with lead plug type laminated rubber bearings (LRB) or high damping rubber type laminated Rubber bearings (HDR). The purpose of this study is to clarify the response of the superstructure and isolation devices by comparing the analysis results and the cumulative absorbed energy under different long-period ground motions. In addition, long-period ground motions that cause changes in the multi-cyclic characteristics of isolation devices are identified using the acceleration, velocity, and displacement response spectra and energy spectra. As a result, base-isolated buildings with HDR, the effect of the difference in evaluation method between the quasi-simple method and the simplified method on the response is extremely small, regardless of the input earthquake motion, so the simplified method is sufficient to evaluate the response. In a base-isolated building with LRBs, the maximum response acceleration and the maximum response shear coefficient are evaluated to be larger with the quasi-simplified method than with the simplified method. Furthermore, as the change in characteristics increases, the difference in response between the simplified method and the quasi-simplified method increases, and the accuracy of the analysis using the simplified method deteriorates.
SE04-A026
Characteristics of Long-period Ground Motions and Building Behavior Based on the Strong Motion Records Observed at the 2011 Off the Pacific Coast of Tohoku Earthquake
Shunei MORI+, Atsuko SHIRAYAMA#, Sora TORIUMI, Keito SASAKI
Tokushima University, Japan
The characteristics of long-period ground motion of several area were studied using the strong motion records of the 2011off the Pacific coast of Tohoku earthquake. In this earthquake, seismic tremors with intensity levels of 6 or higher were observed over a wide area in the Tohoku and Kanto regions. The long-period pulse with period about 20 seconds is significant in velocity seismograms and displacement seismograms of main shock. The velocity response spectrum of the main shock showed no significant peaks between 5 and 10 seconds. In the Kanto Plain, Osaka Plain, and Nobi Plain, long-period seismic tremors with long-period components were observed, causing high-rise buildings to sway with large amplitude for a long time. In the Tokyo area, the pseudo-velocity response spectrum showed a slightly predominant component with a period of 6 to 8 seconds. However, the spectral level was found to be about 80 kine at the highest point, which is not at a level where this input would cause excessive building response. The bay area of Osaka is known as a location where long-period seismic motions are greatly amplified. In the 2011off the Pacific coast of Tohoku earthquake, although the Osaka bay area was more than 750 km from the epicenter, large shaking was observed on the upper floors of one of the largest skyscrapers in western Japan, which was constructed in this area, causing damage to non-structural components, such as trapped elevators, damaged fire doors, and sprinklers. This was attributed to the resonance between the building and the long duration, specific period of predominant seismic motion caused by the amplification of the deep ground structure.
SE04-A027
Focal Mechanism Solution of Earthquakes Above M4.0 in the Chinese Mainland in 2021-2023
Zhigao YANG#+
China Earthquake Networks Center, China
The focal mechanism can provide information about the seismogenic structure, which is urgently needed after an earthquake. The rapid production of focal mechanism solutions for strong earthquakes has become a routine task for major seismological agencies around the world. With the construction of more high-rise buildings in the Chinese mainland, small and medium-sized earthquakes may also cause significant shaking of high-rise buildings and social panic. The rapid release of focal mechanism solutions for small and medium earthquakes has attracted increasing attention from society and scholars. Based on real-time waveform data from more than 1,000 broadband seismic stations in the Chinese mainland, we developed an automatic inversion system for focal mechanism solutions based on the regional seismic waveform fitting method. It can give the focal mechanism, moment magnitude, and centroid depth of the M4.0-6.5 earthquake in the Chinese mainland within 5-15 minutes after an earthquake occurrence. We provide a catalog of the focal mechanism solutions, moment magnitude, and centroid depth of nearly 300 earthquakes inverted from 2021 to 2023. Compared with the GCMT catalog, the Kagan angle of most earthquake focal mechanisms does not exceed 30°. The advantages of our catalog are that the lower limit of magnitude is reduced from around 5.0 to 4.0, and the centroid depth is better correlated with structural boundaries and crustal thickness. The automatic processing results of the latest earthquake's focal mechanism, moment magnitude, and centroid depth are usually released in about 15 minutes, and the manually reviewed results are usually published within a few days.
SE04-A028
Deep Learning-based Epicentral Distance Estimation for Earthquake Location
Bosung SUH+, Jongwon HAN, Seongryong KIM#
Korea University, Korea, South
The conventional method of earthquake source location requires a phase picking process for large amounts of observed waveform data. In this study, we designed a Convolutional Neural Network (CNN) architecture that estimates the epicentral distance from 3 component waveform data of a single station. Our dataset for training and testing consists of local earthquake waveform data from permanent stations operated in the southern Korean Peninsula (SKP). The seismic records of stations within 100 km from the epicenter from 2016 to 2022 were used as the original dataset. For the training dataset, data augmentation process was performed by producing randomly shifted waveforms of each waveform within 10 seconds in order to increase the number of waveform data from 101,437 to 1,014,370 and to prevent overfitting of the model. Combining predicted epicentral distances from multiple stations, epicenters of events were determined by multilateration, which is a method of geographic localization based on the distance from reference points. In addition, we applied bootstrap calculation of the multilateration process with distances of randomly selected stations to estimate uncertainties of the location procedure and to stabilize it. Without the phase picking process, the model successfully estimated epicentral distances with an average error of 5 km. As an application of the method, we found the epicenter of the 2019 Ml 3.9 Sangju earthquake in the SKP with an error of 1.5 km.
SE04-A030
The 2022 Mw 7.3 Southwest Sumatra Tsunami Earthquake: Rupture Up-dip of the 2007 Mw 8.4 Bengkulu Event
Tao XIA1+, Lingling YE1#, Yefei BAI2, Thorne LAY3, Hiroo KANAMORI4, Luis RIVERA5, Sesar Prabu Dwi SRIYANTO6
1Southern University of Science and Technology, China, 2Zhejiang University, China, 3University of California Santa Cruz, United States, 4California Institute of Technology, United States, 5Université de Strasbourg/ National Centre for Scientific Research, France, 6Badan Meteorologi, Klimatologi, dan Geofisika, Indonesia
On 18 November 2022, a moderate earthquake struck offshore southern Sumatra, generating a tsunami with 25 cm peak amplitude recorded at tide gauge station SBLT. Our W-phase solution indicates a shallow dip of 6.2°, compatible with long-period surface wave radiation patterns. Inversion of teleseismic body waves indicates a shallow slip distribution extending to the trench with maximum slip of ~4.1 m and seismic moment of 1.05x1020 Nm (MW 7.3). Joint tsunami modeling indicates a shallow rigidity of ~23 GPa to simultaneously fit seismic and tsunami data. We find a low moment-scaled radiated energy of 4.4x10-6, similar to the 2010 MW 7.8 Mentawai event (3.1x10-6) and other tsunami earthquakes. The 2022 event ruptured up-dip of the 2007 Bengkulu event, demonstrating shallow seismogenic capability of a megathrust that had experienced a deeper megathrust event. We consider seismogenic behavior of the shallow megathrust and concern for future tsunami earthquakes in subduction zones globally.
SE06-A018
Crustal Imaging of the Global Archean Cratons
Alolika CHAKRABORTY#+, Kajaljyoti BORAH
Indian Institute of Science Education and Research Kolkata, India
A craton is the old and stable part of the continental crust which has remained intact throughout a lot of cycles of crustal formation and depletion, thus studying them and their structure helps us in understanding the evolution of the earth’s crust. The evolution of the Precambrian crust and its formation is still a matter of debate. To understand this better we need better geophysical imaging of the earth’s crust. We need to understand what correlation the geometry and the depth of the Moho has with its composition and age. In this study we have mainly focused on the global Archean Cratons, how the thickness of the crust varies in them and what we can infer from them. We have used a total of 436 stations and found out the variation in the crustal depth using two methods. First, we have used the H-K stacking method to get the average crustal thickness and the average Vp/Vs ratio for the stations. Then we have used this Vp/Vs value in the initial model for Jointly inverting the Receiver function data with the Rayleigh Wave group velocity dispersion data. We have also checked the trends shown by the results obtained from our study with the ages of the cratons.
SE06-A019
Aseismic Zone in the Intensely Orogenic Belt of Taiwan
Yutsung LO1#+, Horng-Yuan YEN1, Hsin-Hua HUANG2, Chung-Pai CHANG1
1National Central University, Taiwan, 2Academia Sinica, Taiwan
Taiwan, located at the convergence of the Eurasian Plate and the Philippine Sea Plate, experiences frequent seismic activity, particularly in the collision zone of the Longitudinal Valley. However, in the most intensely colliding regions, there exists a rare phenomenon known as an aseismic zone, where seismic activities are notably absent. This study aims to deeply investigate the seismic activity patterns in Taiwan and the underlying causes of the aseismic zone. Through the establishment of a temporary seismic observation network in the mountainous region of the Central Range and the integration of seismic, gravity observations, and geological data, we seek a comprehensive understanding of subsurface structures. Utilizing earthquake data from the Taiwan region between 2011 and 2018, P-wave and S-wave arrival time determinations were conducted, analyzing a total of 20,967 seismic events covering depths ranging from 0 to 60 kilometers. Employing the double-difference tomography method, a three-dimensional velocity model was constructed. Through a joint inversion process with gravity data using the velocity-density conversion method, the model resolution was optimized to minimize differences between travel times and gravity values in the calculation of subsurface structures. The inversion process and residual distribution are presented in Figure 2. The results indicate that the region primarily resolved by seismic waves is between 4 and 20 kilometers, with particularly good resolution observed from below 20 kilometers to 40 kilometers beneath the Longitudinal Valley. The velocity model reveals that the aseismic zone exhibits a relatively low-velocity region, and deep-seated high-velocity material is identified, speculated to be the iron-magnesium layer in the lower crust, serving as evidence of subduction in the Eurasian Plate. The genesis of the aseismic zone is likely related to volcanic activity, resulting in a low-velocity zone and the subsequent absence of seismicity. Observational results from other studies further support this theory.
SE06-A020
Joint Inversion of Seismic and Gravity Data to Explore the Structure of the Aseismic Zone in the Hsuehshan Range of Taiwan
Jun Wei XU#+
National Central University, Taiwan
Taiwan is located in the collision zone between the Eurasian plate and the Philippine Sea plate, leading to a significant number of earthquakes. These seismic activities serve as valuable materials for studying the orogeny. However, research on the Hsuehshan region is relatively scarce, prompting the utilization of available data to investigate the structure of Hsuehshan. This study employs long-term observational data from the Central Weather Administration and data obtained from the National Central University's temporary seismic station to explore the structure below the Hsuehshan region. Due to the limited resolution of seismic waves in shallow layers (<2 km ), gravity data, known for its good control in shallow layers, is integrated. By combining gravity and velocity structure inversion, models of velocity and density for the research area are obtained. The seismic distribution within 15 kilometers offers good resolution only in shallow layers. Shallow Vp velocity maps show relative velocities that can be compared with Paleogene and Miocene strata on geological maps. The central Vp values in the research area exhibit relatively low values before a depth of 10 km, followed by a contrasting pattern with high-speed regions beyond 10 km depth.
SE07-A003
Heat Flow and Thermal Structure Study in the South-central Section of the Tan Lu Fault Zone: Constraint on Focal Depth
Yibo WANG1#+, Lijuan HE2, Sven FUCHS2, Shengbiao HU2
1Institute of Geology and Geophysics, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China
Whether active fractures are thermal anomalies is a cutting-edge scientific issue in geothermics. Geothermal measurements of the San Andreas Fault reveal no heat flow anomaly, and then the "heat flow paradox" was proposed. The Tan Lu Fault Zone (TLFZ) is the most important fault in eastern Asia and is still active currently. We have carried out extensive geothermal measurements in the south-central TLFZ: the heat flow in the southern TLFZ is concentrated in the range 55-65 mW/m2; the highest heat flow site LZSD (93 mW/m2) is determined by the high heat production rocks, so the southern TLFZ is not a thermal anomaly. In contrast, the heat flow value in the central section of the TLFZ is over 80 mW/m2, which is likely to be a thermal anomaly zone. Simulations and calculations show that the heat generated by the fault activity is not significant (1-6 mW/m2). Temperature field study in the southern TLFZ confirms the correlation between the bottom boundary of focal depth and the 350 °C isotherm, which is not the case in the middle section. The differences in the present-day thermal state of the TLFZ are the result of differences in the influence of tectono-thermal events in different regions, with the "Craton destruction" event at the late Early Cretaceous having altered the property of lithosphere in East China (Lower Yangtze Craton and the north part of the eastern North China Craton), while the south part of the eastern has only undergone the lithospheric thinning process. Difference in paleo-lithospheric thickness is likely to be the main reason for the different present-day thermal state and the decoupling of focal depth from the 350 °C isotherm.
SE07-A006
Dynamic Stress Waves of Turkey Mw7.8 Earthquake Recorded in Shanxi, China
Yongqian CHEN1,2+, Huai ZHANG1#, Yaolin SHI1
1University of Chinese Academy of Sciences, China, 2Shanxi Earthquake Agency, China
Four-component borehole strain gauges, as an important means of ultra-wideband crustal stress monitoring, can directly record the dynamic horizontal strains caused by incoming seismic waves. The Mw7.8 earthquake occurred in Turkey on February 6, 2023, at 1:17:37 UTC, and waveform data from this earthquake were recorded at the Yingxian four-component borehole strain station located in north-central Shanxi prefecture. In this study, different seismic phases, such as P-wave, S-wave, and surface wave, were identified in the strain seismic waves recorded by a four-component borehole strain gauge with a sampling rate of 10 Hz at the Yingxian station in Shanxi prefecture. The characteristics of the dynamic stress changes in the far-field were analyzed by using the stress petal diagram. The results show that the surface wave oscillation period is about 20 seconds, the amplitude of body stress is 0.6 kPa, and the value of shear stress amplitude is 1.1 kPa. The Coulomb stress change on the Liuleng Mountain Fault near the station (striking 300°, dipping NE 65°, positive fault) is close to 1.27 kPa. Although the magnitude of the Coulomb stress change of the present earthquake is low, far from reaching the threshold value of dynamic stress triggering (0.01-0.1 MPa), the actual region did not observe any earthquake being triggered. Indeed, no earthquake was observed to be triggered in the region. However, the research method provides the possibility of quantitatively analyzing the dynamic stress wave characteristics for the observation of high-precision borehole strains.
SE07-A007
Estimating Effective Normal Stress During SSE In Bungo Channel from Slip Velocities and Shear Stress Variations
Yojiro SASAGAWA#+, Toshinori SATO
Chiba University, Japan
Slow slip events (SSEs) are quasistatic phenomena which slip very slowly along the plate surface and which do not radiate seismic energy. They have been reported since Global Network Satellite System (GNSS) observations began in the 1990s. It is important to investigate stress state when SSEs occur because they are newly tectonic mechanism along plate boundary. Theoretical analysis using Rate- and state-dependent friction law have shown quasistatic slip behaviors following velocity weakening (e.g. Rice and Tse, JGR, 1986). Kobayashi and Sato (GRL, 2021, https://doi.org/10.1029/2021GL095690) estimated spatiotemporal slip distributions of the BOSO SSEs using GNSS data and plotted their shear stress change vs. slip velocity. Most trajectories are similar to theoretical stable trajectories whose gradients are equal to the product of the friction coefficients of the slipping plate (a-b) and the effective normal stress (σ'n). In this study, we estimated effective normal stress from SSEs in Bungo Channel, Japan. This region was detected four SSEs until now. We used daily F5 data by the Geospatial Information Authority of Japan (GSI). First, GNSS data was removed liner trends and seasonal variations. Next, we smoothed the detrended data and divided displacements into every-month. From every-month displacements, we estimated the spatiotemporal slip distributions for the SSE. To calculate shear stress change, we used the Coulomb 3.3 program by the U. S. Geological Survey (USGS). We plotted shear stress change vs. slip velocity and estimated effective normal stress from gradient of the trajectories during slip acceleration. As a result, the value of σ'n was 20-30 MPa for 2018 event. We analyze other three events now and will compare properties of each events. Acknowledgment. We used daily F5 data by GSI, and the Coulomb 3.3 program by the USGS. This work was supported by JSPS (23K03541).
SE07-A009
The 2023 Kahramanmaraş, Türkiye Earthquake Doublet: Cascading-like Triggered Ruptures on Bifurcating Faults
Ao ZHENG#+
University of Chinese Academy of Sciences, China
On 6 February 2023, an earthquake doublet consisting of Mw 7.8 and Mw 7.6 events struck southeastern Türkiye near the East Anatolian fault, which accommodates the collision between the Eurasian and Arabian plates. Here we reconstruct the kinematic rupture processes for the two earthquakes by combining the backprojection analysis of teleseismic P waves and the joint finite-fault inversion of an integrated dataset, including synthetic aperture radar displacements, static global navigation satellite system offsets, and teleseismic and strong-motion waveforms. Our preferred models show that both events are attributed to the sinistral strike-slip mechanism within bifurcating faults. The Mw 7.8 earthquake originates on a splay fault branching from the East Anatolian fault, and then the rupture bilaterally extends along the main strand of the East Anatolian fault for about 320 km. The rupture of the subsequent Mw 7.6 earthquake initiates on the middle section of the northern strand of the East Anatolian fault, and also extends bilaterally for about 155 km. The entire rupture of the Mw 7.8 earthquake propagates at a subshear velocity, whereas the westward rupture of the Mw 7.6 earthquake follows a supershear velocity, which is also confirmed by the observations of far-field Mach waves. Our analysis based on the Coulomb failure stress changes highlights the cascading-like triggering between the two events, also indicates the probably increased seismic hazard on the Sürgü fault and the Pütürge segment of the East Anatolian fault.
SE07-A010
Simple Relationship Between Thermal Conductivities and Elastic Wave Velocities of Rocks
Sheqiang MIAO#+, Yongsheng ZHOU
China Earthquake Administration, China
The thermal conductivity of rocks is the most basic parameter used to understand the internal thermophysical processes, thermal structure, and thermal evolution history of the Earth. However, thermal conductivity measurements are time consuming and complicated. Seismic wave velocities are much easier to obtain, even for underground geological units that cannot be directly measured. Therefore, if a relationship exists between these two physical parameters, it would undoubtedly provide a simple and fast method to obtain the thermal conductivity of underground rocks. Considering this, we measured the thermal diffusivities of samples recovered from ultrasonic velocity experiments to 1000 °C using the Laser Flash Apparatus LFA 457 from NETZSCH. We then obtained thermal conductivity through the sample specific heat capacity and density. The chemical composition of the samples (SiO2 content) and the content and distribution pattern of the main minerals were characterized, and then the correlations between the thermal conductivity and the wave velocity at room and high temperatures were analyzed. The results indicate that the thermal conductivity of the rocks is a segmented function of the wave velocity, bounded by a SiO2 content of 65%, and that the thermal conductivity and the wave velocity are roughly linear in silica content subdomains from 65% to 100% and from 30% to 65%. One application of these findings is that, when calculating the lithospheric thermal structure, instead of the previous method of first layering the crust, then assigning a lithology to each layer, and finally assigning a thermal conductivity value to the layers based on the lithology, it is only necessary to know the field wave velocity structure of the region in order to assign a thermal conductivity value to the corresponding rock layer. This greatly facilitates accurate and convenient acquisitions of the thermal structure of the lithosphere.
SE07-A012
R2AU-Net and Transfer Learning for Improved Seismic Phase Detection in Volcanic Regions
Yuji NAKAMURA1+, Yukino YAZAKI1, Yohei YUKUTAKE2, Yuki ABE3, Ahyi KIM1#
1Yokohama City University, Japan, 2The University of Tokyo, Japan, 3Hot Springs Research Institute of Kanagawa Prefecture, Japan
In volcanic regions, earthquakes swarm related to volcanic activity frequently occur, and their rapid detection and measurement are crucial for volcanic disaster mitigation. However, currently, these processes ultimately rely on human judgment, requiring a vast amount of time and cost, making real-time detailed verification impossible. To solve this problem, in this study we construct a model that can more accurately detect earthquakes occurring in the Hakone volcano, using the R2AU-Net, which adds both recurrent residual units and attention mechanisms to the U-Net architecture. Performance evaluation and parameter tuning were conducted on seismic waveforms of about 30,000 events that occurred in the Hakone volcano from 1999 to 2020. As a result, the precision and recall of P-wave detection of the model trained with Hakone’s earthquake data were 95.7% and 87.6%, respectively, significantly improving compared to the existing model using the same Hakone data in this study. Next, recognizing the challenge of limited data in many volcanic areas, we further explored transfer learning for broader applicability. The model, initially trained with Hakone’s data (model HKN), was adapted for Kirishima Volcano, which has about 2,300 recorded events, 13 times fewer than Hakone. This adaptation involved fixing the encoder weights of model HKN and initializing the decoder weights for Kirishima’s data (model KSM), enabling effective transfer learning. The results of applying this model to the observation data of Kirishima, which was not used for training, showed that the performance of the model KSM significantly improved the performance of seismic phase detection compared to the case where the model HKN was applied as is, indicating that it is possible to construct a phase pick model by transfer learning even for volcanoes where training data is insufficient.
SE07-A013
Co- and Post-seismic Stress Transfer on the Main Himalayan Thrust Fault Induced by the 2015 Gorkha Mw7.8 Earthquake
Chong YUE1#+, Xiaofan LI1, Chunyan QU2, Yali WANG1
1China Earthquake Networks Center, China, 2China Earthquake Administration, China
As the most prominent boundary between the Indian plate and the Eurasian plate, the Himalayan orogeny has experienced strong earthquakes. The 2015 Gorkha Mw7.8 earthquake is the most well–observed and well–recorded seismic event in the Himalayan orogen in the modern era, and it provides a rare case to study the stress transfer on the main Himalayan thrust fault (MHT). Based on the Burgers rheological model, we further calculated the co-seismic △CFS, the post-seismic V–△CFS and the C–△CFS induced by the event in the flat-ramp slip model. There is an obvious stress release in the main rupture but an obvious stress loading in the up-dip and down-dip directions of the main rupture zone. Six Mw≥6.0 aftershocks are located in the co-seismic △CFS loading zone or the junction zone between the loading and unloading areas. Post-seismic viscoelastic relaxation of the lithosphere and afterslip present opposite patterns compared to those of the co-seismic △CFS, and the loading stress in the main rupture zone will promote the stress accumulation in the flat-ramp structure and the shear movement between the hanging wall and footwall, which is conducive to the recovery of fault strength. In the down-dip direction of the rupture zone, the post-seismic viscoelastic relaxation and afterslip will release the co-seismic Coulomb stress loading in these regions. The un-ruptured area on the west side of the main shock and the shallow MFT still has the regional seismic risks in the future.
SE07-A018
Laohushan Creep Behavior of the Haiyuan Fault: Insight from the Mineralogical and Frictional Properties of Fault Rocks
Xi MA#+, Yongsheng ZHOU, Lei ZHANG, Changrong HE
China Earthquake Administration, China
Shallow creep has been observed in the Laohushan segment which lies within a seismic gap between the co-seismic ruptures of the 1920 Haiyuan M8.5 earthquake and the 1927 Gulang M8.0 earthquake. However, there has been a lack of geological and mechanical evidence to explain the mechanism behind this shallow creep. In this study, we carried out detailed fieldwork along the entire Laohushan fault, analyzed the mineralogy and microstructures of the fault rocks, and then performed frictional experiments on two fault gouges at various temperature and pressure conditions and observed the microstructural evolution of the experimental samples. The mineralogical analyses show that fault rocks are rich in clay minerals along the Laohushan creep segment, especially in the fault gouge up to a content of 53 wt%, and there is a positive association between clay mineral content in fault gouges and the creep rates along the Laohushan fault. Microstructural observations show that fault gouges exhibit extensive well-developed clay foliation with kinking, folding, and shape preferred orientation, and the fault rocks exhibit networks of carbonate veins healing cracks and fluid-assisted dissolution and precipitation processes of hard minerals. The frictional experiments show that clay-rich gouges have a low frictional coefficient of 0.46-0.58, with positive a-b values of 0.0035-0.0052, reducing to 0-0.0015 at 200 ℃. The experimental samples exhibit microstructural evolution of pervasive well-developed clay foliation and fewer clast fractures, resulting in velocity-strengthening stable sliding behavior. We developed a geological and frictional model of shallow creep on the Laohushan fault, suggesting that weak clay minerals with well-foliated microfabric in fault gouges, which, as demonstrated by frictional experiments, control the Laohushan shallow creep along the Haiyuan fault at a depth of less than 8 km. This finding is consistent with the shallow creep estimated from geodetic data and repeating earthquakes.
SE07-A019
Mechanism of Aseismic Creep of Fault: Evidence from Geological Observation and Frictional Experiments Along Haiyuan Fault and Xianshuihe Fault
Yongsheng ZHOU#
China Earthquake Administration, China
Aseismic creep has been observed in the Haiyuan fault and Xianshuihe fault in the eastern Tibetan Plateau. To study the mechanism of creep slip, we carried out detailed fieldwork along the creep segments of fault, analyzed the mineral compositions and microstructures of the fault rocks, and performed frictional experiments on fault gouges under various temperature and pressure conditions in the laboratory. The results revealed that content of weak minerals, such as, clay minerals are very high in the fault rocks along the creep segment, especially in the fault gouge at the fault core. Microstructural observations showed that minerals dissolution and precipitation, as well as ductile deformation were developed to form foliation in weak minerals from the fault gouges. The frictional experiments indicated that the clay-rich gouges showed low frictional coefficients, and velocity-strengthening sliding behavior of fault with positive a-b values at 20 to 250 ◦C and 100MPa effective normal pressure with 30MPa pore pressure conditions. The microstructures of experimental deformed samples exhibited pervasive well-developed clay foliation and fewer clast fractures, which is very similar with natural fault gouge. Our results suggest that the enrichment of weak clay minerals in the fault zone generates a well-foliated microfabric controls the shallow aseismic creep along the fault. This work is supported by the National Natural Science Foundation of China (Grant No. U2139202, U1939201), the National Nonprofit Fundamental Research Grant of China, Institute of Geology, China Earthquake Administration (Grant No. IGCEA1813).
SE07-A021
Study on Small Earthquakes Picking and Seismic Frequency Analysis Based on EQT
Xiaofan LI#+, Yanlu MA, Chong YUE
China Earthquake Networks Center, China
EQTransformer is a multi-task deep neural network for simultaneous earthquake detection and phase picking with a hierarchical attentive model. In order to compare the EQT and manual picking, we select 245,051 seismic phases from 895 stations in China in 2016 and detect 11913 earthquakes using EQT. The results show that the Pg arrival-time difference which is less than 0.1s is accounted for 57%, and the Sg arrival-time difference which is less than 0.2s is accounted for 39%, which indicate EQT can perform a good detection and arrival time picking in China. We choose 5 stations in China, namely YUT, XKR, JZG, DOH and SGT, and collect the daily seismic data from 2016 to 2019. Based on EQT, the seismic frequency analysis is studied about the Yutian 7.3 earthquake in Xinjiang, Jiashi 6.4 earthquake in Xinjiang, Jiuzhaigou 7.0 earthquake in Sichuan, Tangshan 4.8 earthquake in Hebei, and Qianguo 4.3 earthquake in Jilin. The results show that for those < 5.0 earthquakes, such as Qianguo 4.3 earthquake, the number of small earthquakes does not increase significantly before the earthquake; in Tangshan area, the frequency of small earthquakes is relatively high; there are some small earthquake intensification phenomena before Yutian earthquake and Jiashi earthquake.
SE07-A022
Improving Focal Mechanism Solutions with 3-D S-wave Ground Motion: Toward Routine Determination of the Focal Mechanisms and Detailed Earthquake Source Characterization with Gyeongju Hi-density Broadband Seismic Network (GHBSN) Data
Sangwoo HAN#+, Young-Hee KIM
Seoul National University, Korea, South
Accurate earthquake focal mechanisms are crucial for uncovering the fault orientations and the sense of fault slip. The focal mechanisms are typically obtained by the analysis of P-wave first-motion polarities or by the moment tensor inversion. However, in the region with sparse station coverage, retrieving reliable solutions for small earthquakes (M<3) can be quite challenging. To increase the quality of focal mechanism solutions, we developed a method that utilizes S-wave polarizations that can be applied in a routine and systematic way. We conducted quantitative assessments using a high-density broadband seismic network comprising 200 stations (GHBSN) that cover a 50 km by 50 km zone of the 2016 Mw 5.5 Gyeongju earthquake sequence in southeastern Korea. Through rigorous synthetic tests, we assessed focal mechanisms using three different datasets: P-wave first-motion polarities, S/P amplitude ratios, and S-wave polarization directions, which were obtained from subsets of the GHBSN with varying noise levels. Results indicate that utilizing the S-wave polarization directions effectively reduces the minimum required number of stations. In noise-free condition, the solution could be derived with only two stations, while three are needed considering realistic noise levels for a ML 2.6 event that occurred within the GHBSN. For the observed waveforms of the ML 2.6 earthquake, we only required three stations with the constraints of S-wave polarization directions with S-wave splitting correction. Lastly, we applied our method to determine focal mechanisms of 159 small earthquakes (0.6≤ML≤2.6) that occurred within the network since 2019. We obtained ~90% strike-slip and ~10% reverse faulting mechanisms having spatially different distributions depending on their focal depths. We found that reverse faulting mechanisms are mostly concentrated at shallower depths. The variation of focal mechanisms appears to be spatially related to the fault geometry as well as shear stress variation after the 2016 Gyeongju earthquake.
SE07-A030
Research on New Methods and Equipment for Seismological Monitoring of Glaciers on the Qinghai-Tibet Plateau
Dan WANG#+, Lei ZOU, Bo ZHOU, Jiangshan SHEN
SmartSolo Inc., China
Glacier seismology combines the advantages of glaciology and seismology to form a young interdisciplinary subject. Icequakes are vibrations produced during the movement and breakup of glaciers, ranging from small squeaks to sudden ruptures or slides equivalent to earthquakes (MW7). According to the location and mechanism of icequake occurrence, icequakes can be divided into five types: surface fissures, stick-slip movement, iceberg calving, subglacial flow, and hydraulic fracturing. In addition to traditional seismological methods, icequake research can also be conducted using multidisciplinary methods such as GPS, numerical simulation, and glacier physical properties. Icequake research can further explore the occurrence process and risk assessment of ice avalanches. We review advances in glacier seismology. Our users use SmartSolo scientific instruments to successfully analyze ice avalanche events through vibration signals by observing multi-parameter glacier environment and climate changes, combined with seismological observation instruments. Provide a new and effective monitoring method for glacier seismic monitoring. It enriches the process observation and risk assessment methods of ice avalanche occurrence, and the combination of multiple parameters further improves the accuracy and effectiveness of ice avalanche event monitoring.
SE07-A031
Exploring dML Correction and Correlation with VS30 for Improved Local Magnitude Calculations in Taiwan
Hsin-Yu CHEN1#+, Chun-Hsiang KUO1,2, Horng-Yuan YEN1
1National Central University, Taiwan, 2National Center for Research on Earthquake Engineering, Taiwan
Taiwan is located at the boundary of the Philippine Sea Plate and the Eurasia Plate, resulting in numerous active faults and frequent seismic activity. The calculation of local magnitudes is influenced by diverse geological characteristics at each seismic station, leading to variations in computed values. To represent local magnitude of an earthquake event, average magnitude value obtained from many stations are utilized. VS30, which denotes the time average S-wave velocity of the top 30-meter layers, is commonly used for site classification. The term " dML " signifies the difference between the earthquake event magnitude and the magnitudes obtained from individual stations. The application of dML correction is particularly crucial for smaller earthquakes, which may only be recorded by stations located close to the epicenter. In such cases, all stations may be situated on either hard rock or soft soil, potentially causing underestimation or overestimation of local magnitude. Moreover, seismic instruments placed downhole substantially minimize interference from surface noise, enabling the acquisition of high-quality ground motion signals. This improvement enhances the precision of earthquake localization and monitoring capabilities, especially for regional small earthquakes. The difference in seismic wave velocities between the layers at the surface and downhole seismometers leads to divergence in the calculated local magnitude results. When employing downhole recordings for local magnitude determination, an underestimation occurs due to their smaller amplitudes compared to surface recordings. The objective of this study is to explore the correlation between dML and VS30 and assess the impact of dML correction on local magnitude results. Additionally, we aim to evaluate differences in local magnitude calculations resulting from ground and downhole recordings due to site amplification effects. By implementing dML correction, we anticipate contributing to greater consistency in earthquake catalogs, thereby enhancing the accuracy of seismicity rates for seismic hazard analysis.
SE07-A033
Large Area Crustal Deformation Monitoring by Using Interferometric Analysis of Setentinel-1 SAR Images
Jicang WU#+, Weiwei BIAN, Hongyu LIANG, Lei ZHANG, Lizhi LOU
Tongji University, China
Sentinel-1 SAR satellite is designed with quick revisit time interval, short space baseline and global coverage, this benefits for deformation monitoring of earth surface. However, LOS rate obtained by general MT-InSAR method, such as PS-InSAR, or SBAS, is frame based and relative to the geometry of SAR image. It is difficult to merge adjacent frames to get the whole picture of large area crustal deformation. In this paper, a uniform datum for crustal movement is defined and LOS rates of individual frames obtained by MT-InSAR method are all reduced to the same uniform datum. Then results of different frame/track can be combined together to obtain crustal deformation of the whole plate and even the global continent, so as to offer a global viewing angle to better understand mechanism of earthquakes and plate motion.
SE07-A035
Pore Pressure and Stress Changes in Fault Systems: A Case Study of the Changning Salt Mines
Meng FU1#+, Kai DENG1, Ke JIA2
1Chengdu University of Technology, China, 2Northwestern Polytechnical University, China
The vicinity of Changning salt mines has witnessed a surge in minor to moderate seismic events, closely correlating in time and space with the fluid injection and extraction operations at the mines since 2006. To investigate the impact of these mining activities on fault stability, we calculate stress disturbances caused by fluid injection/extraction and compare the results to those estimated by local seismicity rate variations. The calculation reveals that within 2 km of the wellheads, the Coulomb stress change caused by injection activities reaches ~0.1 MPa. In contrast, at distances of 2-6 km away from the wellheads, the stress change is only on the order of 0.01 MPa or less. On the other hand, the Coulomb stress change within 2 km of the wellheads is estimated to be on the order of 0.1 MPa based on local seismicity variations and the seismicity rate model, which is consistent with our calculations. However, beyond this 2 km range, the estimated stress changes exceeds our computational results, implying additional perturbations from smaller earthquakes and hydraulic fracturing activities south to the swarm. To validate the reliability of our equivalent model's outcomes, we discussed the spatiotemporal distribution of Coulomb stress under varying scenarios, including different receiver faults, hydraulic diffusion coefficients, and non-co-located equivalent wells. These discussions confirmed the soundness and reliability of our findings. Furthermore, we observed a parallel increase in the cumulative seismic moment in the Changning area with the continuation of injection activities. Our study concludes that fluid injection at the Changning salt mines significantly alters the stress environment within 2 km of the wellheads. Additionally, seismic events in more distant areas are likely triggered by interactions between earthquakes and hydraulic fracturing activities in the southern region. These insights provide valuable guidance for seismic risk management in similar geological settings.
SE07-A036
Trend Analysis of High-rate GNSS Data Prior to the 2011 Tohoku-Oki Earthquake Focusing on Spatial Distribution
Yuta MITSUI#+, Riko ARAI
Shizuoka University, Japan
A recent study claimed to have discovered a tendency for an exponential acceleration of surface displacement to occur several hours before major earthquakes exceeding magnitude 7, including the 2011 Tohoku-Oki earthquake (magnitude 9). This discovery was made by analyzing stacked high-rate GNSS data from 5-minute sampling precise point positioning solutions. The findings suggested the existence of accelerating slow slip (pre-slip) events just before large earthquakes. However, high-rate GNSS data contain noise from various sources, including satellite orbit and clock errors, atmospheric delays, multipath effects, and receiver internals. Therefore, such discoveries require careful verification. In our study, we performed a trend analysis of the high-rate GNSS data, focusing on the spatial distribution of trends related to the 2011 Tohoku-Oki earthquake. Our analysis concentrated on the several hours preceding the mainshock. The data revealed a predominance of positive trend values across Eastern Japan. Notably, in the coastal areas near Miyagi Prefecture, close to the mainshock's epicenter, these positive trend values did not show any systematic increase. This observation raises questions about the mechanical causal relationship between the observed trends and the mainshock. Furthermore, the positive values observed across Eastern Japan could be effectively characterized as the first principal component.
SE07-A038
Tourmaline Fault Mirrors Records the Paleoearthquake in the Himalayan Orogen
Yongsheng ZHOU, Lining CHENG#+
China Earthquake Administration, China
Fault mirrors, a highly reflective smooth fault surface, have been observed in the different types of fault (silicate, carbonate, and hematite) and are considered as a recorder of fault slip. A particular type of fault mirror, tourmaline fault mirror (TFM), has been found in several N-S trending normal faults (Yadong-Gulu fault, Xainza-Dinggye fault, Kung Co fault, and Lhazag fault) from the Himalayan orogen, detailed study on the TFM is helpful for revealing the deformation process and past seismic activity of these normal faults. Here, we reported the TFM in the Himalayan orogen for the first time and performed microstructural and geochemical studies on a typical TFM from the Everest area. Based on SEM and TEM observations, the TFM comprises three layers, the dynamic recrystallization layer (DR layer), the partial melting layer (PM layer), and the amorphous material layer (AM layer). TEM analysis and EBSD “no solution” output confirm the pervasive and homogeneous occurrence of interstitial amorphous materials in the PM layer and AM layer, these amorphous materials are expected to be produced by the solidification of partial melts, combining to the Ti-in-Qtz thermometry result of >900 ℃ at the position close to the TFM surface, we propose that the TFM formed by the high-temperature frictional melting at seismic slip. Combining with field, microstructural, and geochemical evidence, we propose a conceptual model for the evolution of the TFM from tourmaline precipitation, coseismic deformation, to post-seismic healing. The widespread occurrence of the TFM within the fault zone and slip surface suggests that tourmaline may control the strength and slip behavior of the N-S trending normal faults in the Himalayan orogen.
SE07-A039
Attempting to Detect Intermediate-term Slow Slip Events in the Shallow Region of the Suruga Trough (Eastern End of the Nankai Trough)
Kikuchi YUJI1#+, Yuta MITSUI1, Masayuki KANO2
1Shizuoka University, Japan, 2Tohoku University, Japan
Many short-term slow slip events (S-SSEs) have been detected in the Nankai Trough subduction zone, Japan, using the Global Navigation Satellite System (GNSS), strainmeters, and tiltmeters. Recently, SSEs with durations significantly longer than those of typical S-SSEs have been observed near the trench, especially off the Kii Peninsula and Cape Muroto. In our study, we estimated the time periods when intermediate-term SSEs may have occurred in the shallow part of the Suruga Trough (eastern end of the Nankai Trough) by observing changes in the GNSS baseline lengths between the upper and lower plates of the trough. By calculating the correlation coefficients between the GNSS baseline length data and a template that simulates surface displacement associated with SSEs, and by converting the moving average data of the baseline length into velocity, we detected three possible SSE signals within the analysis period. Among the detected SSEs, one was synchronous with repeating earthquakes around the Suruga Trough. For further analysis, we used elastic Green’s function to make a preliminary fault model, utilizing the observed displacements during the possible SSE periods. This model suggested that the observed displacements could be explained by a fault located slightly deeper than directly beneath Suruga Bay. Additionally, we analyzed volume strainmeter data and multi-component strainmeter data from the Japan Meteorological Agency to confirm whether strain changes corresponded with the strainmeter data during the potential SSE periods.
SE07-A041
A Trial of Automated Detection Based on Inflection Point Analysis of High-rate GNSS Data: Case Study of Slow Slip Events off the Boso Peninsula
Riko ARAI#+, Yuta MITSUI
Shizuoka University, Japan
Slow slip events (SSEs) exhibit a wide range of time scales, but those lasting from about 100 seconds to one day are less frequently detected. Often, these detections are indirect, inferred from clusters of tremors and low-frequency earthquakes. Direct geodetic detection of SSEs is crucial for an in-depth understanding of these phenomena. Our study aims to improve detection of such events using high-rate GNSS data with sub-daily sampling intervals, specifically a dataset of 5-minute precise point positioning solutions from the Nevada Geodetic Laboratory. Our initial research demonstrated that the noise in high-rate GNSS data hinders signal detection through template matching. We have thus developed a method for automated detection of inflection points in time series data at event onset and conclusion. We predefine numerous potential inflection points and apply broken-line regression, assuming a Laplace distribution and using maximum likelihood estimation, to identify significant inflection points. This presentation focuses on re-detecting signals from slow slip events previously identified in studies using low-noise, daily-sampled GNSS data, serving as a performance test for our method. We concentrate on events off the Boso Peninsula, along the Sagami Trough and Japan Trench subduction zones in East Japan, specifically from 2011, 2016, and 2018. Our detection tests successfully re-identified the 2011 and 2018 events at various observation points, where displacements were around 1 to 2 cm. The detected displacement directions, start times, and end times closely matched those reported in earlier studies. However, the 2016 event, with less than 1 cm displacement, eluded clear detection, likely due to its signal being too weak against the noise. This highlights the potential and limitations of our method in detecting subtle geodetic signals in high-rate GNSS data.
SE07-A045
Detection of Modes of Earth's Free Oscillation Excited by the Philippines Mw7.6 Earthquake Using Fiber Borehole Strainmeters
Wentao ZHANG#+, Wenzhu HUANG, Guoheng QI
Chinese Academy of Sciences, China
With the development of fiber optic sensing, fiber borehole strainmeters are popular because of the advantages of strong adaptability to the extreme environment and special sensitivity to some low-frequency geophysical signals especially. Previous studies have reported many examples of observing solid earth tides using fiber borehole strainmeters. In this study, we reported the observations of low-frequency Earth’s free oscillations excited by Philippines Mw7.6 earthquake using fiber borehole 4-component strainmeters. Using Bartlett’s method (also known as the method of averaged periodograms), almost all of zero-order spherical oscillation modes (0S2 to 0S38) and toroidal oscillations (0T3 to 0T35) between 0.2 and 4.5 mHz were detected in this paper. In addition, pattern of interaction between the modes with close frequencies (cross-coupling effect) was also detected. Our results showed that fiber borehole strainmeters have a benefit for observations of Earth’s long period ground motions and provide an interesting complement to classical seismological instrumentation.
SE08-A014
Relationship Between Groundwater Level Changes and Seismic Velocity Variations in Jeju Volcanic Island, South Korea
Sujin LEE+, Seongryong KIM#
Korea University, Korea, South
In volcanic islands, heterogeneities of aquifers have been reported as problems in analyzing the perturbation of groundwater. The Jeju volcanic island in the south of the Korean Peninsula is a typical area, where horizontally and vertically disconnected multiple aquifers have been formed due to the long history of overlapping eruptions. In this study, seismic velocity variations were measured to investigate their relationship with groundwater level between 23 seismometers installed from 2013 to 2015 in the island. As an initial result, we identify a strong negative correlation between the average variations of seismic velocity and the groundwater level in time for the frequency range of 0.5-0.7 Hz. In addition, the pattern of the velocity change are similar with monthly accumulated precipitation especially during summer season. These observations suggest a previously reported poro-elastic system potentially connecting surface-ground water interactions and elastic property changes in the surrounding medium.
SE08-A015
Eikonal Tomography and Azimuthal Anisotropy of Rayleigh Wave Phase Velocity Using a Dense Accelerometer Network in the Southern Korean Peninsula
Jaeyeon KIM+, Seongryong KIM#
Korea University, Korea, South
Eikonal Tomography was conducted using 325 densely deployed accelerometers across the southern Korean Peninsula. Using ambient seismic noise, the phase velocities of Rayleigh waves were determined for tomography corresponding to frequencies from 0.2 to 1.0 Hz, in less commonly used frequency bands over array scales of several hundred kilometers. This might be attributed to the densely deployed array, or the effect that even if the retrieved velocity maps are piecewise or incomplete, aggregating them all could yield a comprehensive velocity map. The tomographic results revealed a pronounced low velocity trend in the Gyeongsang Basin at frequencies above approximately 0.4 Hz, with weaker low velocity tendencies appearing in Taebaeksan Basin and other smaller basins along the Okcheon Belt as the frequency increased. Additionally, low velocity trends were observed in the southwestern part of the Gyeonggi Massif and in basaltic regions like Jeju Island, also. These tendencies seem to reflect the geology of the Korean Peninsula. In higher frequencies, spatial distribution of high velocity anomalies was similar to the topography of the peninsula. The azimuthal anisotropy results generally indicate a northeast-southwest direction for the fast axis, with tendencies following fault and tectonic lines around the Gyeongsang Basin. This study is expected to give more comprehensive understanding in the structure of the uppermost crust of southern Korean Peninsula and able to applicable to other arrays of similar scale worldwide.
SE08-A017
Teleseismic Constraints on the Crustal Structure Beneath Gyeongju, S. Korea from High-density Seismic Array Data
Minkyung KIM1#+, Hobin LIM2, Young-Hee KIM1, Junkee RHIE1, Tae-Seob KANG3, Kwang-Hee KIM4, Jin-Han REE5
1Seoul National University, Korea, South, 2Korea Institute of Geoscience and Mineral Resources, Korea, South, 3Pukyong National University, Korea, South, 4Pusan National University, Korea, South, 5Korea University, Korea, South
Teleseismic radial and tangential receiver functions (R-RFs and T-RFs, respectively) are computed to reveal crustal seismic structure and anisotropy, using data from the Gyeongju Hi-density Broadband Seismic Network (GHBSN) in southeastern Korea. The GHBSN consists of 200 stations that densely cover the epicenter of 2016 Mw 5.5 Gyeongju earthquake in an area of 50 km by 50 km and also traverses several strike-slip faults, notably Yangsan, and Ulsan faults from west to east. Common conversion point stacking and H-κ stacking (Zhu and Kanamori, 2000) of the R-RFs with a regional 3D velocity model (Rhie et al., 2016) show that the Moho depth beneath the GHBSN varies from 34 km in the west to 25 km in the east. Stacked RF images further show two step-like changes in Moho depth; its abrupt change from 34 km to 28 km is found near the Yangsan fault and another change from 28 km to 25 km near the Ulsan fault. The H-κ stacking estimates an average P-to-S velocity ratio of 1.78, slightly higher than 1.80 at the eastern coast, indicating mafic composition linked to Gyeongsang Basin magmatism in the Cretaceous to early Paleogene. Joint analysis of the R-RFs and T-RFs shows complex azimuthal anisotropy, reflecting contributions from major fault systems. Although the degree of anisotropy is variable, the NNW-SSE trending fast symmetric axes (FSA) are mostly dominant. However, we observe that the degree of deviation from the dominant FSA direction increases toward east. In particular, the FSAs obtained from the stations in close proximity to the NNE-SSW striking Yangsan fault generally align parallel to the fault strike. Also, the NE-SW trending fast symmetric axes are observed in the east of the Ulsan fault. Lastly, the average delay time is 0.32 s, which corresponds to the degree of anisotropy of ~4%.
SE08-A018
The Crustal Structure in the Northern of the Tibet Plateau Revealed by P-wave Receiver Function
Jiawei TAN+, Xuzhang SHEN#
Sun Yat-sen University, China
The uplift of the Tibetan Plateau is a result of the collision between the Indian and Eurasian tectonic plates. The growth and evolution of the plateau, particularly the mechanisms driving its outward expansion, remain subjects of debate. The Qilian Mountains, situated at the forefront of the plateau's northeastward expansion, hold significant implications for understanding the plateau's northward growth due to their unique crustal structure and anisotropy. This study utilized seismic data recorded by 600 short-period dense seismic arrays that span the entire western Qilian Mountains, Qaidam Basin, and Kunlun Mountains. A total of 6735 P-wave receiver functions (PRFs) were computed and selected to generate migration images. The results reveal noticeable dislocations in the Moho beneath the North Qilian suture zone, where the crust rapidly thickens. This could potentially represent the crustal differences prior to the amalgamation of the Central and North Qilian. Conversely, the crust beneath the South Qilian is thinning, and a weak Moho is widespread. These observations provide valuable insights into the geophysical processes shaping the Tibetan Plateau.
SE08-A020
Sedimentary Structure of the Tarim Basin, China, Revealed by Ambient Noise Analysis
Tongtong XIE1+, Yingjie YANG1#, Tao XU2, Xiaobo TIAN2, Jiyan LIN3, Chenglong WU2, Zhanwu LU4
1Southern University of Science and Technology, China, 2Chinese Academy of Sciences, China, 3China Earthquake Administration, China, 4Chinese Academy of Geological Sciences, China
Imaging the fine structure of sedimentary basins is important for natural resource exploration. The Tarim basin, situated in the northwest of China, is the largest inland basin in China and rich in oil and natural gas resources. Previous studies on the sedimentary structure in the Tarim basin are mostly obtained by high-resolution active-source seismic surveys, which are highly costly and environmentally unfriendly. In this study, we use ambient noise tomography, a more efficient and economical method, to construct the sedimentary velocity structure at the southeast margin of the Tarim basin. Based on ambient noise data recorded by a linear short-period dense array, we calculate multi-component (RR, TT and ZZ) cross-correlation functions (CCFs). We observe and analyze the first higher mode Rayleigh waves from CCFs between individual station pairs at a short period band of 0.2 -2 s. After the verification of the credibility of the first higher mode surface waves, we demonstrate that the inclusion of the first higher mode dispersion curves helps image deeper structures with an increase of average depths from ∼ 0.73 to ∼ 1.24 km. We measure Love wave dispersion curves at a period band of ~0.3-11.5 s from T-T component CCFs and obtain a fine sedimentary velocity structure with a depth reaching 10 km based on ambient noise tomography, which reveals clear layered sedimentary structure, the paleo Tadong uplift, and the thrust Cherchen fault. Our study demonstrates that the ambient noise tomography method based on data from dense arrays has great potential for deep resource exploration in sedimentary basins.
SE08-A021
The Velocity Structure of the Divergence Area in Sichuan, China and the Luding Ms6.8 Earthquake
Wen YANG#+, Xuemei ZHANG, Jie LIU
China Earthquake Networks Center, China
The intersection area of the Xianshuihe Fault, the Anninghe Fault and the Longmenshan Fault in Sichuan, China, known as the divergence area, is the transition area of Songpan-ganzi block, Sichuan-Yunnan block and Yangzi block, and their tectonic activities reflect the extrusion tectonic characteristics of Songpan-ganzi block and Sichuan-Yunnan block towards Yangzi block. Historically, strong earthquakes occurred frequently in this region. The 2013 Lushan MS 7.0 earthquake, the 2015 Kangding MS 6.3 earthquake swarm, the 2022 Lushan MS 6.1 earthquake, and the Luding MS 6.8 earthquake occurred in this region sequently after the Wenchuan MS8.0 earthquake in 2008. The study of velocity structure in this area is of great scientific significance to the study of seismic environments and dynamic processes. In this study, we applied the travel time tomography method to invert the velocity structure in the divergence area. We selected the earthquakes and stations within the range of 100.8-104, 28.2-31.2 from March 2019 to June 2023. The results show that there is obvious lateral heterogeneity in the velocity structure of the mid-upper crust in the divergence area, which may correlate with the geological structure. The intersection area between the Xianshuihe fault zone and the Longmenshan fault zone exhibited a significant high-velocity anomaly, which may be related to the rigid lithology of the basement. In contrast, it shows a significant low-velocity anomaly on the west side in the Luding-Shimian section of the Xianshuihe fault zone, which may reflect the structure of gas-bearing rocks. The 2022 Luding MS 6.8 earthquake is located in the conjunctional areas of high and low P-wave velocity anomalies, which were more prone to the accumulation of strain energy.
SE08-A023
Detection of Shallow Sedimentary Layers by Autocorrelation Analysis
Tomotsugu WATANABE#+, Hiroshi TAKENAKA
Okayama University, Japan
We propose how to treat the signals of autocorrelation for detecting shallow sedimentary layers. Seismic interferometry is one of the most useful tools for extracting information of subsurface structures. Application of autocorrelation to ground motion records has been studied to detect the boundary between the bedrock and sedimentary layers. The trace of autocorrelation function may be equivalent to the zero-offset velocity profile in seismic exploration, so its signals represent reflected waves from the interface of subsurface velocity structures, and the time delay of them corresponds to the two-way travel time between surface and the layer boundaries. We can compute autocorrelation function easily by inverse-Fourier-transforming power spectrum. To make its signals clearer, both the spectral whitening and filtering methods are employed. The former removes the source effect from power spectra, and the latter extracts the components over the frequency range of interested. The parameters for these operations are selected empirically by trial and error to emphasize the signals. In particular, the signals reflected from shallow sedimentary layers appear around zero seconds, but these are hidden by the filtering effect because the autocorrelation function then has the large and broad peak at zero seconds. In this study, we develop a new method for removing this effect to detect shallow sedimentary layers clearer. We exploit the logarithmic power spectra and its inverse Fourier transform which is called cepstrum. First, we vanish the lower order term of the cepstrum instead of applying spectral whitening. We then apply the filtering method to the logarithmic power spectra. Finally, we can derive the power spectra which keeps the amplitude approximately flat around one, so its autocorrelation function has the peak like a delta function at zero seconds. We can then identify the signals reflected from shallow sedimentary layers with high resolution than ones from the conventional method.
SE08-A024
Seismic Activity Characteristics and Fine Crustal Feature Beneath the Weiyuan, Sichuan and Its Adjacent Areas
Guangbao DU+, Qingju WU#, Xuemei ZHANG, Ruiqing ZHANG
China Earthquake Administration, China
In this paper, we collected the seismic travel-time data both form a local dense array in Rongxian-Weiyuan area since 2019 and from the seismic networks. Double-difference seismic tomography method was used to invert the high-resolution three-dimensional velocity structure and accurate hypocentral locations. The results show that earthquakes occurred in clusters, showing N-S direction, which are not associated with slip faults; the focal depth in the area is generally in the range of 2-5km. Secondly, the earthquakes are associated with velocity anomalies. It is visible that the earthquakes occurred at the high Vs anomalies in the shallow; on the other hand earthquakes mostly occur in the high-to-low anomaly transition zones of Vp and Vs in the depth of 7-10km. Synthesis of the relocation and velocity profile, we speculate that the thickness of sedimentary cap is about 4-6km, and some moderate earthquakes mostly occur in crystalline basement. Significant higher P wave velocity anomalies are observed underlying the north of Huangjuepo fault earthquake area in depth 7-10km compared with the Rongxian earthquake area, which makes it more difficult for north of Huangjuepo fault earthquake area to rupture, leading to the earthquake occurrence later in this region.
SE08-A026
Unified Shallow Crust for the Chuncheon Basin, South Korea, Using Trans-dimensional Bayesian Joint Inversion of Surface-wave-dispersion and Horizontal-to-vertical Spectral-ratio Data
Cheng SONG1+, Jan DETTMER2, Min Hyug KOH1, Junkee RHIE1, Sang-Jun LEE3, Seongryong KIM4#
1Seoul National University, Korea, South, 2University of Calgary, Canada, 3Korea National University of Education, Korea, South, 4Korea University, Korea, South
We image a unified 3-D shallow crustal structure by combining horizontal-to-vertical spectral ratio (HVSR) analysis with ambient noise tomography (ANT). Shallow crustal structure is of engineering and public safety interest, particularly in basin areas. Ground motion amplification and duration of ground motion by basin resonance are influenced by the shallow structure. Therefore, reliable seismic hazard assessment and precise ground-response prediction of earthquake scenarios rely on accurate 3-D shear-wave velocity structure. Surface wave dispersion (SWD) curves obtained by ANT are sensitive to average velocities and carry travel time information while HVSR curves are sensitive to the shape of the subsurface structure and hold relative amplitude information. Trans-dimensional Bayesian joint inversion where the number of layers is treated as an unknown parameter allows us to leverage the complementary sensitivities of SWD and HVSR curves. The hierarchical framework permits uncertainty estimation with parsimonious models that favor simple shallow structure. We validated our method through synthetic tests. Subsequently, our method is applied to field data collected in the Chuncheon Basin, where we calculate SWD curves by ambient noise tomography and HVSR curves by the single-station method utilizing ambient noise. Results display a soil layer at ~10 m and bedrock at ~200 m depth inside the basin and at ~100 m depth in the surrounding areas. Results show lateral slow shear-wave velocity inside the basin at the same depth, which is consistent with geological information.
SE08-A027
Virtual Head Waves in Ocean Ambient Noise
Jie LI1#+, Peter GERSTOFT2, Martin SIDERIUS3, Jun FAN1
1Shanghai Jiao Tong University, China, 2University of California, San Diego, United States, 3Portland State University, United States
The Green’s function retrieval in media with horizontal boundaries usually only considers the extraction of direct and reflected waves but ignores the virtual head waves, which have been observed experimentally from ocean ambient noise and used to invert for geometric and environmental parameters. This paper derives the extraction of virtual head waves from ocean ambient noise using a vertically spaced sensor pair in a Pekeris waveguide. Ocean ambient noise in the water column is a superposition of direct, reflected, and head waves. The virtual head waves are produced by the cross-correlations between head waves and either reflected waves or other head waves. The locations of sources that contribute to the virtual head waves are derived based on the method of stationary phase. It is the integration over time of contributions from these sources that makes the virtual head waves observable. The estimation of seabed sound speed with virtual head waves using a vertical line array is also demonstrated. The slope of the virtual head waves is different from that of direct and reflected waves in the virtual source gather; it is therefore possible to constructively stack the virtual head waves. The predictions are verified with simulations.
SE08-A030
Seismic Activity Analysis at the Central Indian Ocean Ridge Near the Rodriguez Triple Junction Using the Matched Filter Method
Shiho YAMADA1#+, Toshinori SATO1, Tomoaki YAMADA2, Masanao SHINOHARA2
1Chiba University, Japan, 2The University of Tokyo, Japan
At the first segment of the Central Indian Ocean Ridge, which extends north of the Rodriguez Triple Junction, there is a hydrothermal vent field named as Kaireihydrothermal vent field (KHF). To reveal the crustal structure and seismicity, we conducted a seismic survey using ocean bottom seismometers (Sato et al. Tectonophysics, 2023, https://doi.org/10.1016/j.tecto.2023.230113). We showed that Vp exceeded 6.0 km/s at ~2 km depth below the seafloor beneath Yokoniwa Rise, which is a non-transform offset massif. We detected a seismic cluster in a normal fault zone 3–5 km northwest of the KHF. Manty events occurred in a high Vp/Vs ratio area. This suggests that seawater seeping downward has serpentinized peridotite at depth. At the first segment of the ridge, we detected distinct shallow and deep seismic clusters. In the study, natural earthquakes were detected manually by visual inspection. However, this method limits the number of earthquakes that can be detected, and many earthquakes may still exist. In this presentation, in order to detect more earthquakes, a matched filter method was used. The matched filter method takes advantage of the similarity in waveforms of seismic events that are close. The waveforms of seismic events that have already been found are used as templates, and cross-correlations between them and continuous waveform data are calculated. The method then detects waveforms with high correlation as seismic events. We attempted to detect more earthquakes at the survey region. Acknowledgments. This work was supported by a Grant-in-Aid for Scientific Research on Innovative Areas from the Ministry of Education, Culture, Sports, Science and Technology (Grant Number 20109002, TAIGA project).
SE09-A006
Geometries and Stress Regimes of the Two Convergent Slabs Beneath the Northern Sulawesi, Indonesia
Po-Fei CHEN1#+, Yopi SERHALAWAN1,2
1National Central University, Taiwan, 2Indonesian Agency for Meteorology, Climatology and Geophysics, Indonesia
The subducting slab beneath Northern Sulawesi, Indonesia, exhibits a double convergent subduction, as revealed by Wadati-Benioff seismicity. The south-dipping slab along the North Sulawesi Trench is attributed to the subduction of the Celebes Sea plate, triggered by the late-Miocene collision between the Banggai-Sula microcontinent and the East Arm of Sulawesi. However, the origin of the north-dipping slab is obscured, as seismicity cannot be traced to the trench on the surface. Some propose it as the west extension of the west-dipping Sangihe slab to the east, with nearly a 90° rotation. Others refer to it as the Sula slab, a remnant of the Indian Oceanic slab initiated by the early Miocene collision between the northern part of the Australian plate and the North-Arm of Sulawesi. In this study, we initially utilized data from the ISC-EHB catalogue and applied a clustering scheme to group seismicity, depicting the geometries of the two convergent slabs. Subsequently, we projected P- and T-axes of intermediate-depth earthquakes from the GCMT catalogue, using both geographic and slab coordinates, to assess stress regimes of the slabs. The main findings revealed that the Celebes Sea slab exhibited an average strike of 92° and a dip of 71°. The overall configuration appeared non-linear, with an increasing dip at greater depths, potentially linked to slab rollback. In contrast, the Sula slab displayed steeper subduction, dipping at 73° to the north-northwest, with a strike angle of 253°. Notably, the absence of earthquakes in the western part of the Sula slab at depths of 60-230 km was interpreted as the upper slab detaching during the initial stage of collision in the early Miocene.
SE12-A004
Paleoceanography of Ulleung Basin, East Sea (Japan Sea) for the Last 600 ka
Jeongwon KANG, Sangmin HYUN, Yunji KIM#+, Jin Hyung CHO
Korea Institute of Ocean Science & Technology, Korea, South
Paleoceanographic evolution of Ulleung Basin, East Sea (Japan Sea) during the last 600 ka was reconstructed using geochemical parameters of the Giant Piston Core, GPC-2B. Alkenone concentrations, sediment lightness (L*), and two tephra layers (Aso-4 and Aso-3; 88 ka BP and 133 ka BP) indicated that GPC-2B sediment core spans the last 600 ka (MIS 16). Similar to previous studies, well developed foliation and bioturbation were observed in the sediment core, suggesting that the geochemical characteristics related with paleoenvironment and paleoproductivity would have been well preserved. This study aims to reconstruct the history of terrestrial organic matter input and its related paleoclimate changes using various sediment organic compounds, such as alkenone and alkene. In addition to organic geochemical proxies, the inorganic geochemical parameters are planned to be used to reconstruct paleoclimate and paleoenvironment of Ulleung Basin. Because GPC-2B holds the history spanning 600 ka in the mid-latitude ocean, through comparisons with sediment cores obtained in low-latitude Pacific Ocean and/or Indian Ocean, the relevance of climate changes between latitudes over the past hundreds of thousand years are planned to be studied.
SE12-A013
Some Preliminary Results of Applying Convolutional Neural Network Methods to Classify Minerals Under Polarized-light Microscope Images
Gilbert HONG#+, Sang-Mook LEE
Seoul National University, Korea, South
Identifying the type and state of minerals within thin sections using microscopic observation is one of the crucial procedures in petrological and mineralogical studies that is widely done manually. To enhance the efficiency of this process, we attempt to develop an application that automatically allocates mineral grains within a microscope image based on its microstructure and chemical attributes using machine learning techniques. As an initial step, a convolutional neural network (CNN) model was applied for classifying images of individual mineral grains under polarized-light microscopy. We used PyTorch, and compared with existing pre-trained classification models such as ResNet to assess performance and effectiveness. Training and test datasets were established based on previously analyzed photomicrographs taken under both plane and cross-polarized light. Images mainly were obtained from public data generated during past projects (e.g., post-moratorium IODP expeditions). These datasets mostly contain photos of fresher mineral grains from lithology such as granites and oceanic basalts. Highly altered grains are more difficult to distinguish and lower precision is expected when identifying them. Therefore, future studies will aim to enhance the precision of heavily altered mineral classification by integrating information from other mineral analysis methods, such as Raman and energy dispersive spectroscopy (EDS).
SE15-A004
Synthesis on the Metamorphism Along Chingshui River Deciphering the Geologic History of Yuli Belt, Taiwan
Yuan Hsi LEE1, Geraldine GUNTANG2#+, Yuan-Hsi LEE2, Lucas MESALLES2, Wan-Ling TSAI2, Karl JABAGAT2
1National Chengchi University, Taiwan, 2National Chung Cheng University, Taiwan
Taiwan is known to be the site of the arc-continent collision between two (2) plates: The South China Sea oceanic crust (Eurasian Plate) and the Philippine Sea plate which resulted in the formation of the Yuli Metamorphic Belt. Within this belt, the tectonic blocks and metapelites have undergone a profound transformation through high-pressure and high-temperature conditions, creating an intriguing puzzle for geologists to unravel. Zircon is a resilient silicate mineral that emerges as a valuable tool for investigating multiple geological processes because of its abundance and resistance. Moreover, discerning the differences between an igneous and a metamorphic zircon in terms of the textures, U-Pb ages, and low Th/U ratios in the rock samples such as metaplagiogranites and metapelites ; and identifying the temperatures of carbonaceous materials in the metamorphic rocks along Chingshui River, will help to establish a vital link to the pressure-temperature conditions, ultimately deepening our understanding of the possible mechanisms that underlie the metamorphic transformation of both the ultramafic-mafic tectonic blocks and the surrounding metasedimentary matrix of Yuli Belt from the subduction to exhumation. The ages of ~8 Ma and ~16 Ma for metamorphic and igneous zircons, respectively, are similar from the recorded age dates, as well as the relatively high metamorphic temperatures of ~500° C.
SE15-A008
Early-middle Holocene Strong Earthquake Quiescence Is Association with Incompleted Stratiogralic Records Along the Helishan Southern Fault, on the Latest Activity Boundary of the NE Tibetan Plateau
Wenjun ZHENG1#+, Shiqi WEI1, Xulong WANG2, Xin SUN1, Yanxiu SHAO3, Qiyun LEI4
1Sun Yat-sen University, China, 2Chinese Academy of Sciences, China, 3Tianjin University, China, 4China Earthquake Administration, China
The formation of the Tibetan Plateau began with India-Asian collision ~60 million years ago (Ma), continental basin uplift was delayed in northern Tibetan until ~25-20 Ma. Strong deformation could be clearly visualized through those growth strata within the Cenozoic basins and the uplifting of the neighboring mountain at the northeastern plateau, and its latest boundary of expansion is in the north of Hexi corridor 2 Ma ago. In the north side of the Hexi corridor, these faults formed 4-2 Ma ago represents the latest northeast boundary, and among them the Helishan fault are the most important and representative during the Quaternary and especially in the Holocene. Their Holocene activities are characteristic of strong earthquakes through the geomorphic offsets, and the most confident event is the historic earthquakes (~M8) that is well-documented at 180 AD. These paleoearthquake events are potentially recorded in the sediments that could be revealed by the trenches perpendicular to the fault scarp. The combination of several trenches enables us to make a continuous sequence of earthquake events to investigate millennial activities of the Helishan fault during the late Quaternary. We extracted 8 trenches along the Helishan southern fault, and observed frequent earthquakes during the late Holocene, but apparent quiescence occurs during the early-middle Holocene. The late Holocene activities are recorded within continuous aeolian sediments when the Westlies are prevalent in the past 5 ka. The early-middle quiescence is due to mostly incomplete deposition records, when Asian monsoon invades into the Hexi corridor during the early-middle Holocene. Apparent quiescence results in misunderstanding of the latest activities of the Helishan southern fault. Therefore, the Holocene activities recovered from the Helishan southern faults make clear that the TP expansion is persistent on the millennial scale during the Holocene, and the northeast outward is continuous during the whole Quaternary.
SE15-A015
Advanced Earthquake Analysis: Utilizing Deep Learning and Satellite Imagery for Precise Mapping of Surface Ruptures
Yire CHOI1+, Jin-Hyuck CHOI1, Yeonju CHOI2#
1Korea Institute of Geoscience and Mineral Resources, Korea, South, 2Korea Aerospace Research Institute, Korea, South
Surface ruptures from earthquakes provide crucial evidence, and their precise mapping offers insights into the connection between seismic activities and faults. An innovative approach in this field is the employment of remote sensing techniques, including satellite imagery, for the meticulous mapping of these ruptures. Utilizing satellite imagery, specifically high-resolution Pléiades-1B data, this model excels in identifying and analyzing the geometric aspects of surface ruptures from a Mongolian earthquake. The model's precision in detecting ruptures and characterizing crack features was validated by aligning its results with previous research, achieving over 90% accuracy in rupture detection and less than 5% error in characteristic information. The model's adaptability was further affirmed through its successful application to various rupture types, accurately measuring key features like orientation and length. This automated approach, leveraging satellite technology, offers significant potential for field studies and fundamental data collection on seismic events and their resultant surface deformations.
SE15-A017
Landform Reconstruction and Provenance Analysis for Estimating Fault Slip Rates in Slowly Deforming Regions
Taehyung KIM#+, Dong-Eun KIM, Jin-Hyuck CHOI, Yire CHOI, Hoil LEE, Min HAN
Korea Institute of Geoscience and Mineral Resources, Korea, South
Understanding slip rates is crucial for predicting earthquakes and estimating how frequently they occur. However, in slow-deforming areas, the long seismic intervals challenge the full understanding of long-term seismic patterns. This study specifically focused on the Yangsan Fault (YF) which is one of the active strike-slip faults situated within the Korean Peninsula. Through geomorphological analyses and trench surveys along the YF, we found evidence of prehistorical surface ruptures and verified stratigraphic indicators of past earthquakes. Our landform restoration analyses revealed a lateral displacement of roughly 320 meters, a finding further supported by changes observed in the origin of gravel within streams cross to the YF. By utilizing a burial age of 830,000 years for a gravel deposit uncovered in a trench wall, we computed the slip rate for this lateral displacement to be around 0.32‒0.48 millimeters per year. These findings highlight the importance of using diverse research methodologies to diminish uncertainties when measuring offsets and timings, especially in comprehending the long-term slip rate in intraplate regions.
SE15-A021
Case Studies on Kinematics of Paleoearthquakes Estimated by Drone-derived DEM Analysis
Chaehyeon CHOI+, Jin-Hyuck CHOI#, Eun-Seok BANG, Hoil LEE
Korea Institute of Geoscience and Mineral Resources, Korea, South
We introduce two case studies; the Yangsan Fault in South Korea and the Mogod Fault in Mongolia, on geomorphic offsets along the paleo-earthquake surface ruptures. We use high-resolution drone-derived Digital Elevation Model (DEM) to detect and measure the geomorphic offset. In the Gyeongju Samreung site lying on the Yangsan Fault, we use drone LiDAR-derived Digital Terrain Model (DTM) to conduct topographic profiles parallel and perpendicular to earthquake surface ruptures. The most notable result is the along-fault variations in vertical separations, and this enables us to infer that the Yangsan Fault underwent mostly strike-slip earthquakes. On the Mogod Fault, utilizing photogrammetry-based Digital Surface Model (DSM), we estimate approximately 33 meters of horizontal offset and 2 meters of vertical offset. This estimation is based on the reconstruction of the offset channel using MATLAB-based GUI LaDiCaoz. Senses of vertical separation are in discord between the topographic profile (2D) analysis and the 3D geomorphic reconstruction, and we attribute this difference to the dominant horizontal offset of the inclined geomorphic feature. Our study highlights that the drones offer significant advantages for analyzing earthquake surface ruptures.
SE16-A001
Towards an Interpretable Volcanic Earthquake Classification Method Using Transformer Encoders
Yugo SUZUKI1+, Yohei YUKUTAKE2, Masami YAMASAKI1, Ahyi KIM1#
1Yokohama City University, Japan, 2The University of Tokyo, Japan
In volcanic areas, active earthquake swarms frequently occur in association with volcanic activity. The number of these earthquakes increases as eruptions approach, and there are reported cases in which the number of low-frequency earthquakes in particular tends to increase, but the detailed mechanisms remain unknown. Accurate classification of volcanic earthquake types is very important to clarify the relationship between these earthquakes and eruptions, but at present these processes are ultimately left to human judgement, which requires a great deal of time and human cost, and the classification criteria are also subjective. Therefore, to perform the above process more objectively and accurately, we developed a model to classify the earthquake types using the encoder part of Transformer, a type of deep learning. To verify the performance of the constructed model, earthquakes occurring at the Mount Asama, where various types have been observed, were selected for analysis. We classified A-Type (tectonic earthquakes), B-Type (low-frequency earthquakes) and noise and the F1 scores are 0.876, 0.964 and 0.995 respectively, which are equivalent or better than other machine learning models. Furthermore, visualization of the attention weights to clarify the classification criteria of the model showed that in correctly classified earthquakes, they were focused on the onset of P and S waves for A-Type, and on the middle part of the event signal from the P wave onset for B-Type, indicating similar classification criteria of those used by human hands. However, despite the good classification accuracy, there were some cases where the weights were distributed, and further examination suggested that one of the main causes was the uncertainty in the labelling of the training data. In order to construct a more accurate model in the future, it is important to examine the data that have already been classified by human with unified standard for labelling.
SE16-A002
Development and Social Implementation of Unmanned Autonomous Measurement Technology for Inaccessible Locations - On the Subject of Volcanic Eruptions
Hiromichi KANAI1#+, Keiji NAGATANI2, Yasushi HADA3, Takashi KOI4, Katsushige SHIRAKI5, Toru SHIMADA1
1Kokusai Kogyo Co., Ltd., Japan, 2The University of Tokyo, Japan, 3Kogakuin University, Japan, 4Hokkaido University, Japan, 5Tokyo University of Agriculture and Technology, Japan
Policies such as “i-Construction” by the Ministry of Land, Infrastructure, Transport and Tourism are being promoted to solve the problem of labor shortages due to the aging and declining population for the construction industry in Japan. However, development and social implementation of unmanned autonomous measurement and construction technologies that especially using in the area where dangerous for human are still insufficient. To address these issues, Cross-ministerial Strategic Innovation Promotion Program Phase 3(SIP Phase 3) has been launched since November 2023 to with the objectives that accelerating research and development of remote and automated technologies for reducing manpower and industrial accidents at construction sites by the establishing innovative construction production processes. During volcanic eruptions, pyroclastic flows, volcanic ash and other phenomena cause catastrophic damage to various aspects including human health, infrastructure and wide variety industries. Even worse, it has been reported that the accumulation of fine-grained pyroclastic debris can lead to situations that debris flow which caused by tiny rainfall occurs frequently for a long time. Therefore it is very important for volcanic disaster prevention to observe ash fall conditions and rainfall around the volcano. But the area near the erupted crater is highly dangerous and be designated as a restricted area. Our research team has been involved in the development of unmanned survey technology in volcanic areas using unmanned aerial vehicles (UAVs), and based on these technologies in the SIP Phase 3, we aim to development and social implementation of unmanned survey technology in inaccessible areas during volcanic eruptions. In this presentation, we introduce the technologies developed to date and the prospects for future research.
SE16-A004
Spatial Distribution of Potential Threats of Volcanic Ash in Northeast Asia
Sungsu LEE1#+, Hee Jung HAM2, Yoo Jung KIM3, Seulgi LEE1
1Chungbuk National University, Korea, South, 2Kangwon National University, Korea, South, 3National Disaster Management Research Institute, Korea, South
Among the hundreds of active volcanoes in the Northeast Asian region, Mt. Baekdu (also known as Mt. Changbaishan) and several volcanoes located in Kyushu, Japan, have documented or investigated histories of eruptions with explosions significant enough to propel ashes hundreds and thousands of kilometers away. Since the eruption of any volcano is highly unpredictable, both in timing and scale, it is nearly impossible to adequately prepare for the potential disasters it might cause in the future. In this study, we identified Mt. Baekdu and Mt. Aso as two representative potential threats to Northeast Asia concerning volcanic ash. We conducted numerical simulations involving thousands of hypothetical volcanic ash dispersion based on meteorological data from 2005 to 2014. The results are presented as spatial distributions of ash concentration in terms of PM10, both near the ground and at flight levels. The projected deposition of ash on the ground was also analyzed to illustrate the spatial distribution around Northeast Asia, primarily in Korea and Japan. This research received support from the National Disaster Management Research Institute under the Ministry of Public Administration and Security, as part of the project titled 'Development of Volcanic Ash Vulnerability Assessment Technology and Utilization Research on Risk Assessment Technology (1/2),' identified by the project code 'NDMI-JUYO-2023-08-03-02.
SE16-A006
Detecting Low-level Earthquake Tremblors in Hong Kong’s Super Volcano
Tristan HUI#+, Andrew LIN, Aidan HONG, Chi Ho HO, Diana IBARRA
The ISF Academy, Hong Kong SAR
It is known that Hong Kong rests on top of an ancient supervolcano, last active approximately 140 million years ago and classified as extinct. However, volcanic activity still continues; the magma movement in the volcano's magma chamber causes tremblors (weak earthquakes) across Hong Kong. Through detection and analysis of tremblors, the data can be used to monitor volcanic activity in Hong Kong, looking for potential signs of future volatility. The possible volcanic action from Hong Kong will pose a significant threat to Hong Kong and surrounding areas, hence the significance of this project. Previous observations from the Hong Kong Observatory have found that there have been at least two felt tremblors in Hong Kong per year from 1979 to 2021, some of which are ≤2 on the Mercalli scale, and Lau, 2021 further finds that there are frequent continuous tremblors ≤2 on the Mercalli scale ranging from a few hours to a few days in length. While the Hong Kong Observatory records tremblors and earthquakes ≥3 on the Richter scale, it does not usually report smaller tremblors. This is due to the sensor’s central location in the city, where artificial activity (e.g., construction) affects results. As such, this project will place five sensitive seismographs in five locations spread across Hong Kong (Cyberport, Chai Wan, Mai Po, Mui Wo, and Hoi Ha Wan) to detect tremblors as low as one on the Richter scale. Through the analysis of the collected data, the project aims to build on existing baselines of volcanic activity through more accurate detection in more locations.
SE16-A008
Imaging Shallow Volcanic Structures of Mt. Halla, Jeju Island Using Ambient Noise Double Beamforming Tomography
Min Hyug KOH1#+, Cheng SONG1, Sang-Jun LEE1, Junkee RHIE1, Seongryong KIM2
1Seoul National University, Korea, South, 2Korea University, Korea, South
47 of 3C nodal 5 Hz geophones were installed in a NW-SE line with a length of approximately 5. 1 km along the hiking trail on Mt. Halla at central Jeju island. The shallow crustal depths of Mt. Halla, Jeju Island was imaged using ambient noise tomography. Approximately 40 days of continuous streams of data were used to calculate cross-correlation functions (CCFs) between all station pairs. Double beamforming (DBF) was used to directly measure both Rayleigh and Love waves from vertical-vertical (ZZ) and transverse-transverse (TT) components of CCFs from 0.7 s to 2 s periods. Shear wave velocity profiles (Vsv, Vsh) were obtained by inverting Rayleigh and Love wave phase velocity using 1D Markov Chain Monte Carlo (MCMC) trans-dimensional Bayesian inversion. Isotropic Vs and radial anisotropy ξ profile was obtained. High-velocity structure at the southeast portion of the array coincided with the region between Bangae-oreum, Witbangae-oreum, and trachyte dome, which may indicate magmatic intrusions, whereas low-velocity body was observed at the center of the array. These zones of strong velocity contrasts act as points of reflections and lead to complex propagation of surface waves at shallow depths. The upper layer shows significant positive anisotropy (Vsv < Vsh), indicating a system of shallow sills layers and/or lava flows. Predominantly strong negative anisotropy (Vsv > Vsh) is observed at the bottom layer, which reflects a vertically aligned magmatic plumbing system consisting of dyke swarms.
SE16-A009
Electrical Conductivity of Epidote at High Temperature and High Pressure
Duojun WANG#+, Zhiqing ZHANG
University of Chinese Academy of Sciences, China
Electromagnetic studies have revealed high-conductivity anomalies in subduction zones, however, the causes for these anomalies are unclear. We report new results on the electrical conductivity of Epidote, which were measured at 0.5-3.0 GPa and 573-1273 K using impedance spectroscopy. Our results show the electrical conductivity of the Epidote increases with the increase in temperature, after dehydration of the Epidote, there is a slight increase in conductivity. By combining with geophysical observations, we found epidote could provide a clue for high conductivity anomaly in the hot subduction zone.
SE16-A010
Geodynamic Reconstruction of West Pacific Subduction Beneath the Changbaishan Volcanic Province, Northeast Asia
Tao ZHU1#+, Diandian PENG2, Lijun LIU3
1China Earthquake Administration, China, 2University of Illinois at Urbana-Champaign, United States, 3Institute of Geology and Geophysics, Chinese Academy of Sciences, United States
Changbaishan (also known as Baitoushan in Korea) volcano is located in the border area between China and North Korea. As a typical example of active and hazardous intraplate stratovolcano, the mechanism of this volcano is not well understood. Although Changbaishan volcano is about 1200 km west of the western Pacific subduction zone, it has been always attributed to dynamic processes associated with Pacific subduction, including hot upwelling in the big mantle wedge, deep slab dehydration, continuous piling up and upward thickening of stagnant Pacific slab and the upward escape of entrained oceanic asthenosphere material. Therefore, the westward subduction of the Pacific plate is the key to explore the mechanism of Changbaishan volcano. In this study, we use 4-D geodynamic models based on sequential data assimilation to reproduce past subduction along the west Pacific margin. These geodynamic models, which are carried out with the spherical finite element code CitcomS, assimilate plate motion, lithospheric thermal structure and chemical composition. The predicted present-day Pacific slab geometry matches observation inferred from seismic tomography, indicating the feasibility of our model results within the region of Changbaishan volcano. This work is supported by National Natural Science Foundation of China (NSFC, Grant 41974103) and a part of the Self-initiated project, modeling on the geodynamic subduction of the Pacific plate beneath the Changbaishan volcano since the Cenozoic, supported by the Institute of Geophysics, China Earthquake Administration.
SE16-A017
The Sources and Magmatic Processes of Lavas from the Benham Rise in the West Philippine Basin
Long YUAN1+, Quanshu YAN2#, Xuefa SHI2
1Ministry of Natural Resources, China, 2State Oceanic Administration, China
Since the early Cenozoic, the Philippine Sea Plate has undergone complex tectonic-magmatic evolution, and the West Philippine Basin (WPB) in this plate experienced the overlapping effects of back-arc processes and intraplate processes (forming a series of positive topographies such as Benham Rise and Urdaneta Plateau) (Hickey-Vargas, 1998; Ishizuka et al., 2013; Barretto et al., 2020; Yan et al., 2022). However, the origin and magmatic process of these plateaus and their adjacent seamounts in the WPB is still in debate. In this study, we analyzed the in situ major- and trace element compositions of the plagioclases and clinopyroxenes and the in situ Sr isotopic compositions of plagioclase in basalts collected from the Benham Rise (Site DSDP-292) during DSDP (Deep Sea Drilling Program) Expedition 31. The results showed that both of clinopyroxenes and plagioclase phenocrysts exhibited a variety of disequilibrium characteristics, and the zoned textures of the clinopyroxenes and plagioclases were produced by the addition of multiple phase magma replenishment into magma chamber. The lavas from the Benham Rise could be formed by 10–20% partial melting of garnet pyroxenite. The light rare earth element contents and some incompatible element ratios (e.g., Ba/Sr and Sr/La) of cores of the plagioclase and clinopyroxene phenocrysts are different from those of their rims, and yet the Sr isotopic compositions of cores of the plagioclase phenocrysts are similar to those of rims of them, suggesting that their parental magma could be originated from a same mantle source but undergo obvious fractional crystallization processes. In addition, compared to whole rock compositions, the plagioclase phenocrysts from site 292 record Sr isotopic variations, reflecting their mantle sources is heterogeneity. We suggested that the Benham plume is chemically heterogeneity, and the complex magmatic processes produced variations in the elemental compositions of mineral and lavas.
SE16-A018
PGE Geochemistry of Macquarie Island Basaltic Glasses and Picrites
Gyuchan PARK1#+, Jung-Woo PARK2, Vadim KAMENETSKY3
1Seoul National University, Korea, South, 2School of Earth and Environmental Sciences, Seoul National University, Korea, South, 3Chinese Academy of Sciences, China
Investigating mid-ocean ridge basalt (MORB) glasses and picrites from Macquarie Island, this study aims to shed light on the behavior of sulfide and platinum-group elements (PGE) in the evolution of primitive MORB magmas. They show a wide range of compositional variations due to various degrees of partial melting and magma differentiation. The decreasing PGE contents in MORB glasses with decreasing MgO highlight the compatibility of PGE during magma differentiation. Positive correlations between PGE concentrations in MORB glasses and picrites suggest liquid sulfide as the predominant host for PGE. Sulfides captured in high Fo# (= 88 – 90) olivine crystals in picrites indicate early sulfide saturation. The structure of sulfides mainly composed of central pyrrhotite surrounded by chalcopyrite and pentlandite at their mineral boundaries suggests subsolidus re-equilibration at lower temperatures (650 – 350 °C) compared to monosulfide-solid solution and intermediate solid solution assemblages found in other MORBs. Multiple analyses on individual sulfide grains reveal PGE distribution during the crystallization of liquid sulfide; Ir-group PGE and Re partition into MSS; Pd into pentlandite; Pt and Au into alloys rather than sulfides. However, significant differences in PGE contents between replicate analyses of some picrites imply the presence of micro-sized platinum-group minerals such as Ru-Ir-Os alloys, Pt alloys, or Ir-Ru sulfarsenides. Although they are variably PGE-depleted due to early sulfide segregation, PGE ratios of Macquarie Island MORB glasses and picrites should be similar to those of primary magmas if all PGE partition similarly to sulfide liquid. Despite elevated and varying La/Sm ratios, they exhibit a Ru/Pd range akin to global MORBs, indicating a limited influence of mantle fertility and partial melting degree on PGE fractionation. Global MORBs display lower Ru/Pd ratios than the primitive mantle, suggesting a higher bulk partition coefficient of Ru than Pd during mid-ocean ridge melting.
SE16-A019
Mantle Heterogeneity and Crustal Processes Preserved in Olivine-hosted Melt Inclusions from the Ridge-transform Intersection of the Central Indian Ridge at 16.5°S
Sunghwan IM1#+, Jung-Woo PARK2, Sarang CHOI1, Jonguk KIM3, Andrey A. GURENKO4, Seongjun CHOI1
1Seoul National University, Korea, South, 2School of Earth and Environmental Sciences, Seoul National University, Korea, South, 3Korea Institute of Ocean Science & Technology, Korea, South, 4Centre de Recherches Pétrographiques et Géochimiques, France
We present geochemical characteristics of 37 olivine-hosted melt inclusions in an olivine-phyric mid-ocean ridge basalt (MORB) located at a fracture zone in the Central Indian Ridge (CIR) at 16.5°S, to unravel detailed magma evolution processes and mantle heterogeneity in this region. The post-entrapment modification-corrected melt inclusions generally exhibit higher MgO and Mg# than the carrier basalt. They also display a diverse range of enrichment ([La/Sm]N=0.29-3.85, K2O/TiO2=0.05-0.70), exceeding the intra- and inter-segment variations in the nearest CIR axis ([La/Sm]N=0.38-3.20, K2O/TiO2=0.02-0.61). Some of the melt inclusions have extremely positive Sr anomalies, indicating interaction with gabbroic rocks. However, this reaction was limited in other melt inclusions with Sr anomalies consistent with those in the CIR basalts. Fractional crystallization modelling confirms the Sr anomaly in the latter inclusions was controlled by primary magma composition and plagioclase fractionation, rather than lower crust contamination. The melt inclusions were further divided into Enriched-MORB (E-MORB) and Normal-MORB (N-MORB) types. E-MORB inclusions share geochemical similarities with basalts from Réunion Island and MORBs in the CIR influenced by Réunion plume, suggesting a significant contribution from the fossil Réunion hotspot to the mantle source of the E-MORB melts. The N-MORB inclusions exhibit a wide variation of Pb isotopic ratios (207Pb/206Pb=0.806-0.857, 208Pb/206Pb=1.99-2.11), inconsistent with a binary mixing of depleted mantle and fossil Réunion hotspot components, suggesting the involvement of a third component with low 208Pb/206Pb and 207Pb/206Pb ratios and depletion in incompatible trace elements. The CO2-H2O saturation depth of the melt inclusions was calculated to be 5-13 km, deeper than that of the average slow-spreading ridge. This is likely due to the cooler geotherm near the fracture zone. The variability in melt inclusion compositions indicates ineffective magma mixing and homogenization during differentiation.
SE16-A020
Characteristics of Magma in Ijen Caldera Pumice Products Based on Geochemical Analysis
Putri AMALIA#+, Mirzam ABDURRACHMAN, Idham ANDRI KURNIAWA, Firman SAUQI
Bandung Institute of Technology, Indonesia
On the northern part of the Ijen Caldera wall, there are many eruptive caldera deposits which are dominated by the presence of pumice. Generally, when viewed physically, caldera product deposits in Indonesia look homogeneous, marked by the same color. However, in the deposition of the Ijen Caldera product, it actually has quite a contrasting layer, which is characterized by the existence of a boundary between the dark pumice product and the light pumice product. Rock geochemical research was carried out using XRF and ICP-MS analysis methods consisting of 8 samples. Based on geochemical analysis, it shows that the composition of the dark pumice product contains 50-58 wt% SiO2 while the light pumice product contains 60-62 wt% SiO2. This Ijen Caldera pumice product is classified as magma with High-K Calc-Alkaline affinity. Based on the main element and trace element data plotted on the Harker diagram, it is known that the differentiation process includes magma mixing and then dominant fractional crystallization occurs. There are differences in color layers in the Ijen Caldera pumice product because it is influenced by magma which is rich in silica (SiO2 60-62 wt%) so that it becomes a bright pumice product. Furthermore, the crystals grow as the magma cools and shows that the magma solution is decreasing so that the silica content also decreases (SiO2 50-58 wt%) and this is what becomes the dark pumice product.
SE17-A004
Search for Hidden Pegmatitic Lithium Deposits by Audio Magnetotelluric (AMT) and Geo-electrochemical (GET) Measurements: A Case Study of Murong Lithium Deposit in Western Sichuan, China
Panfeng LIU#+
Guilin University of Technology, China
The Murong lithium deposit in western Sichuan Province is located in the northeastern part of the Yajiang dome group and the western periphery of the Jiajika rare metal ore field. The newly discovered Jiajika lithium deposit nearby is currently the largest pegmatitic spodumene deposit in Asia. It is considered that this region possesses good metallogenic prospecting potential for rare metals. However, due to the intense landform incision and thick Quaternary coverage in the plateau area, the conventional geophysical and geochemical exploration methods (soil and high-power electrical measurement) have poor prospecting effect. Based on the comprehensive study of the GET and AMT in the Murong lithium mining area of Yajiang, this paper discusses a set of new technical combinations suitable for deep prospecting, so as to provide a new technical method for prospecting the same type of deposits in this area. The results show the geoelectrochemical combination anomaly of Li and associated elements (Be, Rb, Cs) within 500 m has a good indication effect on deep lithium ore bodies. The gradient zone of the resistivity curves of the AMT measurement can reflect the occurrence position and approximate burial depth of veined mineralized bodies and pegmatite. Drilling verification suggests that the anomalies agree well with the location of ore bodies (mineralization), which indicates that the comprehensive method has practical significance for deep prospecting and can reduce prospecting risk. It is necessary to conduct prospecting predictions and delineate prospecting target areas around the mining area, which points out the direction for future prospecting work.
SE17-A005
Characterization of Phayaung Taung Deposit: Geological Characteristics, Formation Processes, CO2 Fluid Inclusions, and Gold Deposit Type
Naing Aung KHANT1+, Heejung KIM1#, Chungwan LIM2, Khin ZAW3, Yang JAE E.1
1Kangwon National University, Korea, South, 2Kongju National University, Korea, South, 3Seoul National University, Korea, South
Myanmar possesses a wide range of mineral resources, which consist of several small-scale enterprises as well as a few globally significant mines. One notable gold deposit is the Phayaung Taung mine, located in the northeastern area of Mandalay in central Myanmar. The gold deposit is found among the alternating layers of quartzite and phyllite units of the Late Proterozoic Chaung Magyi Group in the Mergui Belt. The Phayaung Taung deposit contains mostly secondary gold, which originated from the main gold generated during the sulfide ore stage. The gold is often found inside tourmaline-quartz and sulfide-bearing quartz veins. While the subject region has been investigated in terms of occurrence, geological context, and ore mineralogy, there has been a lack of comprehensive research on fluid inclusions using Raman analysis. In this study, we provide the findings of the Raman analysis conducted on fluid inclusions containing CO2. Additionally, we introduce a novel approach for determining the pressure-depth correlations by considering the density and temperature range of the CO2 fluid inclusions. Raman examination reveals the absence of water within the bubbles seen in CO2-containing fluid inclusions, with densities ranging from 288.82 kg/m³ to 969.68 kg/m³. The presence of N2 in the CO2 fluid inclusions is very little. The entrapment pressure of the CO2 fluid inclusions was determined to be 169 MPa, while the most recent recorded recrystallization pressure was 16 MPa. The estimated depth of the CO2 fluid inclusions was around 5.63 km, whereas late recrystallization happened at a depth of roughly 0.53 km. This recrystallization is likely associated with the uplifting and deformation event in the Mergui Belt. This study categorizes the Phayaung Taung deposit in the Mergui Belt as a mesozonal, structurally emplaced orogenic gold deposit, offering valuable information on its geological features and formation mechanisms.
Session Chair(s): Caibo HU, University of Chinese Academy of Sciences
SE07-A001
Finite Element Numerical Simulation of the Coseismic and Postseismic Deformation of the 2015 Gorkha (Nepal) Earthquake
Yuhang CHEN+, Mingqian SHI, Caibo HU#
University of Chinese Academy of Sciences
On April 25, 2015, a Mw 7.8 earthquake (84.71E, 28.15N) occurred in the portion of the Main Himalayan Thrust (MHT), near the city of Gorkha, about 80 km northwest of Kathmandu in central Nepal. The largest magnitude 7.3 aftershock occurred 12 days after the main shock. The earthquake is characterized by low dip, unruptured to the surface, complex fault geometry, complex media structure and strong surface relief. In this paper, GPS and InSAR data, seismic tomography data, and rheological structural data of the region are extensively collected, and 3D finite element models of the coseismic and postseismic deformations of the 2015 Nepal earthquake is established by using a self-developed 3D viscoelastic finite element program. The models can take into account factors such as complex fault geometry, complex media structure and strong surface relief, etc. The numerical simulation results of coseismic and postseismic deformation obtained from the optimal reference model are consistent with the actual GPS and InSAR data. This paper also discusses the effects of different dip angles, whether or not the surface is ruptured, and the inhomogeneity of the medium on both sides of the fault on the simulation results, and also discusses the differences between the coseismic and postseismic deformation characteristics of the 2015 Nepal earthquake and the 2008 Wenchuan earthquake. The self-developed 3D viscoelastic finite element program can be widely used for numerical simulation of coseismic and postseismic deformation of large earthquakes.
SE07-A002
The Inversion Based on Finite Element Models of Coseismic Rupture Dislocation Distribution for Large Earthquakes
Caibo HU#+, Yuhang CHEN, Yaolin SHI
University of Chinese Academy of Sciences
The inversion of coseismic rupture dislocation distributions for large earthquakes is a scientific problem of great interest to seismology and geodesy. Currently, this inversion work is mainly based on seismic dislocation theory and utilizes analytical and semi-analytical models such as uniform elastic semi-infinite space, layered uniform semi-infinite space, and spherical layered uniform model for inversion. It is difficult for these models to take into account the effects of practical factors such as surface relief and lateral inhomogeneity of the medium. In this paper, through the self-developed three-dimensional parallel elastic finite element program, we can study the effects of complex fault geometry, complex media structure and strong surface relief on the coseismic deformation of large earthquakes, and flexibly partition the geometry of seismic faults, obtain the Green's function numerical solution of the coseismic deformation of the unit dislocation on the surface of different subfaults in the directions of strike-slip and inclination, so as to invert the distribution of dislocations of coseismic rupture in large earthquakes based on the joint GPS and InSAR data of coseismic surface deformation of the actual large earthquakes. In this paper, the effects of different subfault divisions, number of GPS observation points and number of freedom degrees on the inversion accuracy are firstly investigated through theoretical modeling to verify the correctness and feasibility of the inversion method based on the finite element models. Finally, the coseismic rupture dislocation distribution of the 2008 Mw 7.9 Wenchuan earthquake is jointly inverted by GPS and InSAR data using this inversion method, and the inversion results are in good agreement with the previous results.
SE07-A024
| Invited
Lithospheric Rheology and Stresses Gleaned from Intraplate and Megathrust Alaska Earthquakes
Yan HU1#+, Jian ZHANG2, Kejing HUANG2, Jeffrey T. FREYMUELLER3
1Deep Space Exploration Laboratory, 2University of Science and Technology of China, 3Michigan State University
Study on the postseismic deformation of large earthquakes may help constrain the lithospheric rheological property and lithospheric stress redistribution due to the earthquake. We have developed a three dimensional viscoelastic finite element model to study deformation processes of the 2018 Mw7.9 oceanic crustal and 1964 Mw9.2 megathrust earthquakes. The model includes a 40-km elastic upper plate, a 90-km elastic subduction slab overlying an 80-km viscoelastic asthenosphere, viscoelastic continental and oceanic upper mantle. The biviscous Burgers rheology is used to represent the viscoelastic relaxation of earthquake-induced stresses in the upper mantle. The time-dependent, stress-driven afterslip is simulated through a 2-km weak shear zone attached to the fault. We applied the grid-search approach to constrain the rheological properties of the model space. The viscosities of the asthenosphere and mantle wedge are determined to be 2×1018 Pa s with an acceptable range of 1-4×1018 Pa s and to be 2×1019 Pa s with a range of 0.5-5×1019 Pa s, respectively. Model results indicate that a localized weak mantle wedge of ~1018 Pa s beneath Lower Cook Inlet is required to better reproduce GPS observations in this region. The weakened mantle wedge may be due to the fluids dehydrated from the underlying slab. The 2018 Alaska earthquake promoted coseismic and postseismic stress loading of up to 0.9 and 0.1 bar, respectively, on the shallow subduction interface near the Kodiak Island, but there is no obvious triggered seismicity, probably due to the low stress status already released by the 1964 Mw 9.2 Alaska earthquake.
SE07-A037
Coseismic Coulomb Stress Changes Induced by the 2020-2021 Alaska Earthquake Sequence in and Around the Shumagin Gap and Their Influence on the Alaska-Aleutian Subduction Interface
Jianjun WANG#+, Caijun XU, Lei YANG
Wuhan University
Three Mw>7.0 earthquakes occurred in the Shumagin seismic gap and its adjacent area in the Alaska-Aleutian subduction zone during 2020 - 2021, including the Mw7.8 Simeonof thrust earthquake on July 22, 2020, the Mw 7.6 Sand Point strike-slip earthquake on October 19, 2020, and the Mw 8.2 Chignik thrust earthquake on July 29, 2021. The spatial and temporal proximity of these three earthquakes prompts us to probe stress triggering effects among them. Here we examine the coseismic Coulomb stress change imparted by the three earthquakes and their influence on the subduction interface. Our results show that: (1) The Simeonof earthquake has strong loading effects on the subsequent Sand Point earthquake and the Chignik earthquake, with the Coulomb stress changes of 3.95 bars and 2.89 bars respectively. The Coulomb stress change caused by the Sand Point earthquake at the epicenter of the Chignik earthquake is merely around 0.01 bars, suggesting the negligible triggering effect on the latter earthquake; (2) The triggering effects of the Simeonof earthquake, the Sand Point earthquake and the Chignik earthquake on aftershocks within three months for each mainshock are not well pronounced with the statistical triggering rates of 38%, 14% and 43% respectively. Other factors might have played a dominant role in promoting the occurrence of those aftershocks, for instance, the roughness of the subduction interface, the complicated velocity structure of the lithosphere and the heterogeneous prestress therein; (3) The three earthquakes caused remarkable coseismic Coulomb stress changes on the subduction interface nearby these mainshocks, with an average Coulomb stress change of 1.49 bars in the shallow region directly inboard of the trench.
SE07-A011
Geochemical and Hydrogeological Tools for Seismic Hazard Assessment
Giovanni MARTINELLI1#+, Lisa PIEROTTI2, Gianluca FACCA2, Fabrizio GHERARDI2
1National Institute of Geophysics and Volcanology, 2National Research Council of Italy
Recognition of Earthquake-Prone Areas (REPA) is a series of phenomenological methods that have been developed in recent decades to identify locations with a high likelihood of experiencing strong earthquakes. The information on potential earthquake sources provided by the REPA method is a key aspect of the seismic hazard assessment. We integrated worldwide data on the geographical distribution of geofluids with global data on earthquake incidence, heat flow distribution, and S-wave dispersion. This allowed us to acquire a deeper understanding of the development of local stress-strain fields. We concentrated on regions distinguished by the presence of thermal waters and/or the emission of deep-seated gases, as indicated by the isotope composition of related helium. The spatial arrangement of these fluids may function as an indirect signal of anomalous permeability in the Earth's crust caused by processes of crustal deformation. The mapping of thermal springs has highlighted areas that have experienced extensive tectonic activity. Essentially, places with both tectonic activity and thermal springs will likely continue to experience earthquakes until major global geodynamic events change the current state of tectonic activity. Geofluid locations generating large components from the Earth's mantle have been discovered in areas that are not typically associated with seismic activity. These areas are characterised by abnormal heat flow and probably abnormal dispersion of S wave values. The approaches outlined could assist in accurately identifying places where deep faults, capable of reaching the upper mantle layers, are consistently influenced by higher values of crustal permeability. This is likely owing to unreported or unexplained small crustal strain occurrences. We have established a protocol to initially identify regions with a high likelihood of experiencing earthquakes in unforeseen locations around the globe. The current study incorporated geofluids into the existing catalogue of geological factors that are valuable for Seismic Hazard Assessment.
SE07-A014
Deformation Monitoring by Employing Dual Frequency, Android-based Smartphones and Low-cost Multi-GNSS Receivers – A Simulation Test
Chien Zheng YONG#+, Robert ODOLINSKI, Paul DENYS
University of Otago
Multi-constellations and multi-frequencies (two or more) Global Navigation Satellite Systems (GNSS) allow Android-based smartphones and low-cost receivers to achieve precise positioning (at the millimetre to centimetre level) for any baseline length. This opens up the possibility of using much more cost-effective sensors that cost hundreds of dollars instead of more than ten times the cost for the geodetic grade GNSS receivers and antennas that are commonly used in deformation monitoring. In this study, we explore the practicability of using Android-based smartphones and low-cost multi-constellation, dual-frequency GNSS receivers to augment the existing cGNSS network in New Zealand. New Zealand plate boundary zone consists of diverse active tectonic processes from the Hikurangi subduction setting in the North Island to the Marlborough strike-slip fault zone. Followed by the Alpine transpressional fault and Puysegur subduction trench in Fiordland of the South Island. The current continuous GNSS (cGNSS) sites in the North Island of New Zealand are reasonably well-distributed along the Hikurangi trench with station spacing of approximately 25 km, whereas the spatial spacing is about 100 km in the South Island. The smartphone and low-cost cGNSS options with a temporal resolution of 1 Hz data sampling allow for the possibility of detecting short wavelength variations in ground movements and localised deformation effects by cGNSS network densification. We benchmarked all our results against expensive geodetic-grade Trimble NetR9 receivers and antennas. We conducted positioning performance tests in a simulated setting by introducing lateral movements on a sliding platform for all the analysed GNSS antennas and receivers. Our study will demonstrate that the economically viable counterparts provide a comparable capability to the geodetic-grade GNSS receivers in detecting such movements. This infers the cost-effective GNSS receivers can augment the existing geodetic network to exploit an economically viable possibility of monitoring deformation motion in higher spatial and temporal resolutions.
SE07-A017
Correct Sensor-orientation Determination Based on Integrated Analyses of Earthquake and Microseism Records
Seongjun PARK#+, Tae-Kyung HONG
Yonsei University
Seismometers are often installed with incorrect azimuthal orientations. It is required to verify the sensor orientations for the proper seismological analysis. Conventional methods to determine the sensor orientations typically utilize the polarization of earthquake-origin P or Rayleigh waves to estimate sensor orientations. The conventional approaches require long recording times to collect earthquake records. Recently, a microseism-based method has been proposed, enabling instant sensor-orientation determination based on only short records. However, the method requires local reference seismometers with correct orientation information. Each method has its limitations and uncertainties. We propose a novel method that combines the individual analyses based on earthquake-origin P waves, earthquake-origin Rayleigh waves, and microseisms. First, we apply the earthquake-phase analyses to seismometers with sufficient earthquake records, determining the sensor orientations based on differences between apparent polarization directions and great-circle directions. We then determine the orientations of all seismometers using the Rayleigh-waves in microseisms, by comparing the apparent polarization directions between the seismometers and local reference seismometers. Seismometers with pre-determined orientations are used as reference seismometers. Finally, we determine the representative seismometer orientations by weighted-averaging the seismometer-orientation estimates from the three analyses. We apply the method to dense seismic network with 377 seismometers in South Korea. We analyze 448 global earthquakes from 2018 to 2022 and 13-day-long microseism records in June 2022. The orientations of all seismometers are determined stably with standard errors of < ~1°, supporting the effectiveness of the method for prompt and accurate determination of seismometer orientations. Approximately 38 % of seismometers exhibit misorientation angles of > 10°, emphasizing the importance of considering sensor orientation in seismic record analyses.
SE07-A020
Shear-enhanced Electrical Conductivity of Synthetic Graphite-bearing Gouges: Implications for Electromagnetic Observations in Carbonaceous Shear Zones
Jinyu CHEN#+, Lu YAO
China Earthquake Administration
Crystalline graphite (Gr) can be enriched within fault zones due to mechanical or chemical processes and is considered a material that promotes fault weakening and electrical conductivity (σ) enhancement at fault zones. Geophysical observations suggest highly conductive anomalies in the carbonaceous shear zones and low apparent resistivity anomalies prior to an earthquake. However, to date, there are insufficient systematic real-time observations of the mechanical and electrical characteristics of shearing carbon-bearing gouges. Given this, we designed a novel experimental assembly in a rotary shear apparatus. Thus, electrical conductivity measurements on synthetic Gr-bearing gouges along a fault-parallel direction were conducted during a progressive fault slip. Long-displacement friction experiments were performed at fixed velocity (∼1 mm/s), normal stress (2 or 5 MPa), and under ambient temperature, N2 atmosphere conditions. Our results showed that an initial very limited shear displacement caused an abrupt enhancement of the σ. Quartz gouges maintained high steady-state electrical conductivity and frictional coefficient in the Gr content of 3.4–13.6 vol.%. It is associated with an ad-hoc fabric (graphite–cortex clasts) present in the principal slip zone. For high Gr content, excess Gr flakes fill the pores and help develop mechanically lubricated surfaces. In contrast, even with low-Gr content (< 2.4 vol.%), calcite gouges could develop smooth slip surfaces. We propose that Gr content as low as 3.4 vol.% can cause high conductivity anomalies in natural shear zones. The initiation of slips within carbonaceous shear zones can be detected by identifying unusual temporal signals using electromagnetic stations. However, the level of electrical conductivity of a fault zone cannot be used to infer its frictional strength, which is related to the crystal properties (e.g., hardness and crystal structure) of the rock-forming minerals.
SE07-A034
Comparison of Grace Mascon and Spherical Harmonic Products: a Case Study on Seismic Change Signals
Jing LI1#+, Jin LI2, Xian SHI3, Jianli CHEN4
1Chinese Academy of Sciences, 2Shanghai Astronomical Observatory, Chinese Academy of Sciences, 3Shanghai Astronomical Observatory, 4The Hong Kong Polytechnic University
The gravimetry observations from the GRACE (Gravity Recovery and Climate Experiment) twin satellites have been widely used in global change research since their launch in 2002. GRACE gravimetry serves as a powerful tool for studying seismic changes of large earthquakes. At present, the commonly used GRACE data products mainly consist of two types: one is the spherical harmonics (SH) coefficient products, which require the users to perform post-processing; the other is the mass concentration (Mascon) products, which are released in more recent years and dedicated to easier utilization of the data. Even though Mascon products are generally believed to provide higher spatial resolution (than SH products), they are mostly applied in hydrological investigations. Whether Mascon products prevail over SH products or not in seismic applications remains a question. In this study, we conduct comprehensive comparisons between the Mascon products and SH products in extracting seismic gravity-change signals of large earthquakes. During the comparisons, we take the three gigantic seismic events as case studies, including the 2004 Mw9.3 Sumatra earthquake, the 2010 Mw8.8 Chile earthquake, and the 2011 Mw9.0 Japan earthquake. We analyze the detection capabilities of two types of products for seismic signals in land-ocean boundary regions. Results show that both Mascon and SH products are able to detect the seismic-change effects of the three large earthquakes. However, the Mascon products exhibit some limitations in capturing the details of seismic change signals compared to the SH products, especially for the seismic signals in oceanic areas, where the SH products can reveal larger signal amplitudes and more detailed information. Therefore, when using GRACE and GRACE-FO data to study seismic change signals of large earthquakes, especially for those occurring in land-ocean boundary regions, the SH products might be a better choice.
SE07-A027
Study on Dynamic Response of Well Water Level Induced by Earthquake and Its Mechanism
Baiyang CHEN1+, Fuqiong HUANG2,1#
1Institute of Disaster Prevention, 2China Earthquake Administration
The widespread groundwater in the earth's crust is highly sensitive to crustal stress and solid deformation. Therefore, an in-depth study of the response of groundwater to earthquakes is of great significance for a comprehensive understanding of the evolution of hydrogeological processes and tectonic activities in the shallow crust of the earth on a spatiotemporal scale. When an earthquake occurs, the coseismic variation of water level has a certain correlation with the magnitude of the earthquake and the distance from the wellhead to the epicenter. Although the coseismic variation of water level is closely related to seismic magnitude and well seismic distance, it is still affected by the hydrogeological conditions where the observed well is located. Well water level shows obvious directivity and difference to seismic response, which proves the existence of fault shielding. Moreover, the change of tectonic stress state will affect the change of coseismic water level of observation Wells, which has certain guiding significance for earthquake prediction.
Session Chair(s): Junle JIANG, The University of Oklahoma
SE07-A004
S-wave Velocity Structure and b-value Distribution Before the Luding Ms6.8 Earthquake Reveal the Seismogenic Mechanism
Qian HUA1,2+, Shunping PEI3,1#, Yihai YANG2, Lei LI1,4, Xiaotian XUE1, Jiawei LI1,4, Hanlin LIU5, Wei LIU1,4
1Chinese Academy of Sciences, 2Shaanxi Earthquake Agency, 3Yunnan University, 4University of Chinese Academy of Sciences, 5Institute of Tibetan Plateau Research, Chinese Academy of Sciences
On September 5, 2022, an Ms6.8 earthquake shocked the Luding County, southwest China, which broke the quiescence of large earthquake in the Moxi section of the Xianshuihe fault. In this study, we collected seismic waveforms from a dense seismic array deployed from May 2019 to May 2020 in the Moxi section to investigate the fine shallow crustal S-wave velocities by ambient noise tomography. Meanwhile, based on the double-difference relocation method, we relocated the earthquakes in the Luding area, which were further used to spatially map the b-value distribution through an improved least-squares b-value imaging technique. Combined these results, we discussed the seismogenic structure and mechanism of the Luding earthquake. High-resolution images show that the Luding mainshock located in an area of high velocity and high stress, where is considered as an asperity on the Moxi section. To the southeast of the mainshock, we recognized another high velocity asperity where a lot of aftershocks occurred. The earthquake distribution reveals a hidden normal fault on the west side of the mainshock, charactered as an associated structure of the Xianshuihe fault system, on which the largest M5.0 aftershock occurred. Our results indicate that the high velocity asperity on the Moxi section acted as a "rivet" structure and controlled the overall spatial distribution of Luding earthquake sequence. Identifying this special "rivet" structures through high-resolution imaging of crustal velocities and spatial b-values can effectively evaluate seismogenic capacity of active faults, which is of great significance to seismic hazard assessments.
SE07-A005
| Invited
Fault Structure Responsible for the 2016 Gyeongju Earthquake Sequence in South Korea, Inferred from a Stress Field Constraint
Chandong CHANG1#+, Tae-Seob KANG2
1Chungnam National University, 2Pukyong National University
The 2016 ML 5.8 Gyeongju earthquake, the largest instrumentally recorded event in the Korean Peninsula, has been accompanied by thousands of discernible aftershocks for years. The earthquake epicenters scatter quite widely over an area of ~6 km by 6 km, with the focal depths ranging 10-18 km, which indicates that the earthquakes might have occurred by reactivating a somewhat complicated fault network. The knowledge of fault geometry and kinematics is essential to understanding the physical process of earthquakes. To unveil fault structures responsible for earthquakes, we develop a new technique to extract fault planes from individual focal mechanisms based on a stress constraint. In this method, we first estimate the prevailing state of stress by stress inversion of the focal mechanisms. A parameter called fault instability, a function of the stress and fault orientation, is calculated for each of the two nodal planes. The nodal planes, whose instabilities are more than ~30% higher than those of their counterpart nodal planes, are shown to represent true fault planes, which is confirmed by a series of tests using synthetic focal mechanisms with known fault planes. We apply this technique to the well-constrained focal mechanism dataset compiled from the Gyeongju earthquake catalog. We determine fault plane orientations with their respective hypocentral locations, which can provide better constraints for modeling the fault network than using hypocentral locations only. The determined fault network consists of several fault structures with four distinct orientations constituting several conjugate systems.
SE07-A008
Seismogenic Structures in the Western Foothills of the Yunlin-Chiayi Area, Taiwan: Insights from a Short-period Seismic Network
Yu-Chih HUANG1#+, Strong WEN2, Dayi CHEN3, Che-Min LIN4
1National Center for Research on Earthquake Engineering, NIAR, 2National Chung Cheng University, 3Central Weather Bureau, 4National Applied Research Laboratories
The Western Foothills are situated along the deformation front of the Taiwan orogen, characterized by highly active faults and a complex seismogenic structure that has historically caused significant damage. In the Yunlin-Chiayi area, a complex fault system exists, comprising thrust faults, strike-slip faults, and potentially blind faults beneath the alluvial plain. It is important to note that different fault types exhibit distinct rupture patterns and damage distribution. Therefore, evaluating the activity level of each fault and understanding their interrelationships is crucial. The compact, lightweight, and easy-to-use short-period (nodal) seismometer can be rapidly deployed in the field with a larger number of units to facilitate intensive observations. In recent years, dense short-period seismic networks have provided valuable insights into the spatiotemporal distribution of seismic activity and crucial parameters related to fault activity. To enhance our understanding of seismic activity in the Western Foothills of the Yunlin-Chiayi area, we established a temporary seismic network with regular maintenance and data retrieval processes. This network comprised 18 short-period seismometers with a station spacing of 5-10 km, allowing for more comprehensive observations. During the operation of the seismic network, Event 112065 (ML=5.5, max. Intensity=5-), which occurred on September 5, 2023, was the most significant, preceded by foreshocks and followed by numerous aftershocks. The focal mechanism indicates right lateral strike-slip faulting, aligning with the orientation of the Meishan Fault. Additionally, we detected numerous events with magnitudes ranging from 1 to 3 and focal depths less than 20 km. Most events occurred on the hanging wall of the Dajianshan and Chukou Faults, with some seismicity beneath the Western Coastal Plain. Examining the correlation between seismic activity and seismogenic structures enhances our understanding of potential seismic hazards in the region.
SE07-A023
Detection of the Buried Miryang Fault with Active and Passive Seismic Techniques
Lanbo LIU1#+, Su Young KANG2, Kwang-Hee KIM2
1University of Connecticut, 2Pusan National University
Miryang Fault (MF) is one of the most important branches of the Yangsan Fault system that dominates neo-tectonics in southeast Korean Peninsula. The most significant earthquake events in modern history, i.e., the 2016 ML5.8 Gyeongju earthquake occurred on the Yangsan Fault; and the 2017 ML 5.4 Pohang Earthquake also occurred in the vicinity. Using the national and regional earthquake monitoring network Heo et al (2023) identified five earthquake clusters via microearthquake distribution. Miryang Fault is one of the five clusters that can be arguably defined as an active branch of the Yangsan Fault system. However, as they also pointed out, it is difficult to relate the micro-seismicity on the Miryang Fault directly to the surface fault expressions, despite the strike of the clustered Miryang Fault seismicity closely sub-parallel to the surface fault expression. Furthermore, all the detected micro-seismic events occurred along a lineament following the strike of MF, but the seismicity cannot clearly define the north terminating point of the fault. To solve this puzzle, we conducted passive and active seismic surveys along five cross-section profiles in the GeonCheon-Ri valley with the attempt to locate the Miryang fault. All the five profiles are designed roughly perpendicular to the inferred strike of the Miryang Fault. The longest profile is about 9 kilometers with a station spacing of 75 meters and the shortest profile is about 300 m with station spacing of 2 m. We employed several seismic interferometry techniques including time domain cross-correlation and cross-coherence in frequency domain by surface wave dispersion inversion for getting the shear wave velocity structure near the fault zone. The analysis results suggest that the Miryang fault appears to have several sub-branches in the GeonCheon-Ri valley; with a bit extended speculation, we can argue that Miryang fault may just terminate in the vicinity of the GeonCheon-Ri valley.
SE07-A025
Rupture Characteristics and Seismogenic Mechanisms of the Kunlun Pass-Jiangcuo Fault in the Northeastern Tibetan Plateau: Insights from the 2021 Mw 7.4 Maduo Earthquake
Kuilin XIAO1+, Qiang QIU2#
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, 2SCSIO, Chinese Academy of Scienc
The Tibetan Plateau is divided into several rigid tectonic blocks that are connected by large-scale active faults. Over the past three decades, earthquakes with magnitude Mw>7 in China have occurred along the boundaries of the Bayan Har block, indicating the block is seismically very active. One exception to this seismic pattern is the Maduo earthquake on May 22, 2021, which occurred on a strike-slip subfault in the block interior along the Kunlun Pass-Jiangcuo fault and registered a magnitude Mw 7.4 even larger than these boundary seismicity. There are many subfaults interior of the Bayan Har block, which could potentially rupture similarly to the Maduo earthquake. Additionally, the Maduo earthquake has disturbed the stress field, potentially expediting failure of these off-boundary faults. Therefore, it is crucial to clarify the rupture characteristics and seismogenic mechanisms of these off-boundary faults, exemplified by the Maduo earthquake, for a comprehensive assessment of seismic hazard in the region. In this study, we assemble InSAR and GNSS geodetic data as constraints in the kinematic slip inversion and seismic cycle model to study the slip characteristics and rupture behaviors of the Maduo earthquake. We use an optimization method that automatically discretizes fault dislocation elements to balance slip resolution and spatial details. Our results show the Maduo earthquake ruptured in segmentation, with high slip focus on the eastern portion at depths ~2-6 km and slip deficits shallower than ~2 km. Our seismic cycle models show the shallow slip deficits are likely due to a transition in frictional properties, changing from weakly rate-weakening in the eastern segment to rate-strengthening in the western segment. Our findings offer new insights into the seismogenic mechanisms for Kunlun Pass-Jiangcuo fault and the evolution of strain and stress during seismic cycles, which are crucial for future seismic hazard assessment in this region.
SE07-A015
Characteristics and Models of Tectonic Deformation in Shanxi Rift Region
Ruichun LIU#+
Shanxi Earthquake Administration
The present tectonic deformation characteristics of Shanxi Rift Valley is of great significance for us to fully understand the evolution law of rift structure and deeply understand the dynamic genetic mechanism of rift earthquake. Under the constraint of GPS crustal motion velocity field, the current horizontal deformation characteristics of Shanxi Rift are quantitatively studied by comprehensive use of block rigid motion and elastic deformation models. The results show that the current horizontal deformation of Shanxi Rift has the characteristics of zoning and segmentation, and the deformation modes of each basin are obviously different. The Xinding, Taiyuan and Linfen basins in the middle of the rift are dominated by shear deformation along the main fault strike, while the tensile/compressive deformation along the vertical main fault strike is weak; In the north and south sections of the rift, Datong and Yuncheng basins are dominated by tensile deformation along the strike of the main vertical fault, and the shear along the strike of the main fault is less than the tensile deformation. The present tectonic deformation model of the Shanxi Rift is influenced by the differential movement of the Ordos block, the North China Plain block, the Qinling tectonic belt and the Yinshan-Yanshan tectonic belt, and its tectonic deformation parameters can be explained by the tectonic extension model of the tensile zone at the tail of the shear zone. The dextral shear deformation is significant in the middle of the rift, but there is no obvious tensile deformation, which is related to the difference of counterclockwise rotation rate between the Ordos block and the North China Plain block. While the Yinshan-Yanshan tectonic belt and Qinling tectonic belt block the right shear in the middle of the rift, resulting in expansion at the south and north ends of the rift.
SE07-A016
Crustal Rheological Layering Revealed in Multiscale Signals of Natural and Anthropogenic Processes at Pawnee, Oklahoma
Junle JIANG#+, Segun BODUNDE, Jacob WALTER, Brett CARPENTER, Jose VITERI
The University of Oklahoma
Oklahoma has experienced a significant increase and decrease in human-induced earthquakes in the past decade. The Mw5.8 Pawnee earthquake in 2016 is the largest recorded event linked to wastewater injection, rupturing a previously unmapped Sooner Lake Fault (SLF). Two months after the event, eight continuous Global Navigation Satellite Systems (GNSS) stations were deployed around the SLF, adding to the growing monitoring networks in the state. Here, we use multi-year geophysical observations from the Pawnee region to estimate the spatiotemporal evolution of seismicity and strain and probe the rheological properties of intraplate faults and crustal layers. We process the GNSS position time series to reveal transient signals due to crustal processes from late 2016 to 2022. The largest rapid deformation signals coincide with an M3.9 event within earthquake swarms in 2019. Interestingly, the GNSS stations farthest from the faults primarily exhibit subsidence, attributable to poroelastic deformation due to changes in injection activities into shallower rock formations. In contrast, near-fault stations show larger horizontal movements and uplift, suggesting an origin of faulting processes. Over the recorded post-seismic period, seasonal signals predominate the vertical GNSS components, whereas the horizontal components show similar steady trends, with intrastation differences in average rates below ~1 mm/yr. The lack of spatially localized, transient geodetic strain suggests that postseismic fault slip is either persistently weak over years or short-lived within two months of the Pawnee event. We further estimate decadal GNSS secular rates over a larger region and find differential movements of ~1 mm/yr between the Pawnee array and nearby stations, which may be explained by the viscoelastic flow of the lower crust. We derive updated source models of the Pawnee mainshock and swarm events to estimate stress changes and assess the contributions of aseismic slip and poroelastic and viscoelastic deformation.
Session Chair(s): Hongfeng YANG, The Chinese University of Hong Kong
SE07-A032
| Invited
Cascading Foreshocks and Preslip Phase of the 2019 Weiyuan Mw 5.0 Earthquake
Hongfeng YANG1#+, Jinping ZI2
1The Chinese University of Hong Kong, 2Shenzhen Research Institute, The Chinese University of Hong Kong
It has long been in debate whether earthquakes start by preslip or cascade triggering of small magnitude events. By far both models are supported by observations in different regions, but it remains unclear whether the two mechanisms may concurrently exist in nature. Here we report the first case of dual mechanisms that were both observed during the 2019 Weiyuan Mw 5.0 earthquake. The earthquake struck the Weiyuan shale gas field in September 2019, leading to fatality and infrastructure damage. Nearby hydraulic fracturing activities were absent at least three months before the mainshock. By running template matching detection from 4 near-field stations, we find an intense foreshock sequence that occurred 6 minutes before the mainshock, exhibiting a cascade triggering manner. Furthermore, we observe a robust nucleation phase during the mainshock, shortly before the impulsive P waves. Our observation provides the first evidence of dual mechanisms are concurrent, advancing our understanding of earthquake nucleation.
SE07-A042
Precise Relocation and Source Characterization of Two Earthquake Sequences in Yellow Sea Using Regional Lg-wave Observations
Jun Yong PARK1#+, Young-Hee KIM1, Won-Young KIM2, Xuzhang SHEN3
1Seoul National University, 2Columbia University, 3Sun Yat-sen University
We investigated two earthquake sequences that occurred in the Gunsan Basin in the middle of Yellow Sea. The first sequence started with the 4.7 Mw event on 18 January 2021 followed by five aftershocks. The second, the 4.2 Mw event on 3 December 2021 was followed by two earthquakes. The focal mechanisms of two mainshocks are strike-slip faulting along steeply dipping nodal planes striking NW (~305º) and SW (~215º) at a depth of ~10 km. Two earthquake sequences occurred in the region with relatively low seismicity in the Yellow Sea. An investigation into the seismogenic faults and rupture processes associated with these earthquakes can provide valuable information about their properties. The seismographic stations, 160–550 km from the source area, lacked close-in stations. Hence, we used Lg-wave, which has strong amplitudes and propagates well around Yellow Sea region with continental crust. We conducted epicentral relocation by measuring differential travel times of the Lg-wave centered at a group velocity of 3.3 km/s from closely located event pairs by the cross-correlation technique. We achieved root-mean-squared residual time and bootstrap uncertainties of the epicenters of 0.0153 s and 0.12 km, which is much less than a factor of 37 and 11 compared to the initial location uncertainty, respectively. Both earthquake sequences exhibit a NW-SE trend, which aligns well along one of the nodal planes. We further performed an empirical Green's function analysis to investigate rupture properties using corner frequency estimation. We found that the Mw 4.7 event has weak or no directivity, which indicates symmetrical circular or bi-lateral rupture with radius of ~0.4 km based on Brune (1970) model. In contrast, we found that the corner frequencies at stations around the Mw 4.2 event exhibits strong azimuthal variation and directivity to SE direction, which indicates a uni-lateral rupture.
SE07-A043
Rupture Properties of Small Earthquakes in Southern Korean Peninsula
Min-Seong SEO1#+, Sangwoo HAN1, Won-Young KIM2, Young-Hee KIM1
1Seoul National University, 2Columbia University
The Southern Korean Peninsula (SKP) hosts a dense network of seismic stations, providing an opportunity to study the rupture properties for small earthquakes with good azimuthal coverage. Hence, the SKP may serve as an exemplary location for investigating the rupture characteristics of earthquakes in stable continental region (SCR). We aim to resolve rupture properties of earthquakes with magnitude exceeding 2 by employing the empirical Green’s function method to compute relative source time functions. This method allows us to probe apparent rupture durations in various directions, and these durations are inverted for rupture parameters (rupture direction, length, velocity, and degree of asymmetry) under the assumption of a line source model. We adopt Bayesian inference to quantify the uncertainties of parameters robustly accounting for the data error and trade-offs. Our analysis for 28 earthquakes with M ≥ 2 in SKP since 2019 reveals that the majority of events (~70%) can be effectively modeled using the line source model, thus showing a clear fault rupture plane, which can be primarily attributed to significant rupture directivity effects. About 15% of the events show no obvious directivity in rupture propagation, suggesting a bilateral or symmetrical circular crack model for their sources, and the rest were unresolved. Our finding thus implies that the simple estimation of stress drops based on the symmetrical circular rupture models may lead to potential for the directional ruptures. The estimates of rupture length and velocity have relatively large uncertainties due to a trade-off. The rupture length tends to increase with magnitude, showing general accordance with the previously suggested scaling relationship for SCR earthquakes. Besides, the well-resolved rupture velocities are between 0.56 and 0.94 times the shear wave velocity (VS), which is comparable to the range reported for large crustal earthquakes (0.7 – 0.9 VS).
SE07-A044
| Invited
The Role of Fluid in Earthquake Nucleation and Precursory Processes
Shengji WEI#+
Nanyang Technological University
The precursors of a large earthquake are critical to understand its nucleation and rupture evolution, however, robust observations are rare due to lack of near field observations and hence there are active debates on the modes of earthquake nucleation. Here we take advantage of near fault seismic observations for two representative earthquakes, the 2018 Mw6.0 shallow thrust earthquake in central Myanmar low land and the 2024 Mw7.5 western Japan shallow thrust event, to investigate their seismic precursors. We found that the Mw6.0 event was preceded by ~6s of seismic precursor that is located at the same place of mainshock hypocenter and has a magnitude of 4.1. The amplitude of the precursor does not increase with time and its spectrum does not show deficient in high frequency energy. It is more like a regular earthquake that was not associated with a slow nucleation process. In contrast, the 2024 Mw7.5 western Japan earthquake was preceded by several years of precursory seismicity near the mainshock hypocenter, associated with opening or volume increase at the depth of ~15 km, as documented by the near fault GPS observations. Together with low velocity structure and very slow initial rupture of the mainshock, we suggest the fluid concentration at the upper and lower crust boundary may have migrated into the upper crust, triggering the background seismicity as well as the initial mainshock rupture, and responsible for the slow rupture propagation. The contrast between the precursors of the two cases suggest that the richness and concentration of crustal pore fluid is diverse between faults, which plays a critical in governing the preparation and initiation of the rupture of large earthquakes. Dense near fault seismic observations and detailed waveform analysis are critical to further understand the generalization of such processes.
SE07-A046
| Invited
Earthquake Nucleation and Foreshock Mechanisms: Cascade Triggering, Aseismic Slip, Fluid Flows, or a Combination of Them?
Zhigang PENG#+
Georgia Institute of Technology
Understanding the nucleation process of large earthquakes is crucial for accurate earthquake prediction and seismic hazard mitigation. While earthquake nucleation process has been widely observed in the laboratory and numerical simulation, it is difficult to observe them directly in the field. Some studies have considered foreshocks as the by-product of such nucleation process. While many large earthquakes also have foreshocks, it is currently impossible to effectively distinguish foreshocks from ordinary earthquake sequences. In addition, the physical mechanism of foreshock generation is still in debate. In this talk I first summarize foreshock observations in the last decades, and present several foreshock mechanisms: cascade-triggering, aseismic slip, fluid diffusions, or a combination of them. Next, I present several case studies of foreshocks in East Asia, including the 2010 M6.7 Yushu and 2021 M6.1 Yangbi earthquakes in China and the 2024 M7.5 Noto earthquake in Japan. I focus primarily on how different results/conclusions can be made by different dataset/methods. Finally, I offer some suggestions on how to move forward on the research topic of earthquake nucleation and foreshock mechanisms.